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Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


1

Chicago  

Office of Environmental Management (EM)

Laboratory - Lee Zachos * lzachos@anl.gov * Brookhaven National Lab - Jill Clough-Johnson * clough@bnl.gov Chicago * Fermi National Accelerator Lab - Sandra Efstathiou *...

2

Chicago  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DeWillican Middleton Small Business Program Manager July 29, 2013 Chicago * The majority of supplies and services acquired by the Chicago Office is provided by our Management and Operating (M&O) contractors. Site and Facility Management Contractors (FMCs) Chicago * Contact each of the laboratories' and develop a relationship with the small business liaison officers. The liaisons will have information on the upcoming acquisitions for the future and other outreach activities that are planned. Chicago * M&O Contractor Liaisons * Ames Laboratory - Andrea Spiker spiker@ameslab.gov * Argonne National Laboratory - Lee Zachos * lzachos@anl.gov * Brookhaven National Lab - Jill Clough-Johnson * clough@bnl.gov Chicago * Fermi National Accelerator Lab - Sandra

3

Flash Center for Computational Science The University of Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

Flash Center for Computational Science Flash Center for Computational Science The University of Chicago Flash Center for Computational Science Mira Early Science Project Conference Argonne National Laboratory 15 May 2013 Carlo Graziani Flash Center University of Chicago New Insights Into Buoyancy-Driven Turbulent Nuclear Combustion from Large-Scale 3D FLASH Simulations Flash Center for Computational Science The University of Chicago What are Type Ia supernovae? Supernova Cosmology Project Flash Center for Computational Science The University of Chicago What are Type Ia supernovae? Supernova Cosmology Project Peak luminosities of most Type Ia SNe are similar - making them excellent "cosmic yardsticks" Flash Center for Computational Science The University of Chicago

4

University of Chicago, Chicago, Illinois,  

Office of Legacy Management (LM)

University of Chicago, Chicago, Illinois, University of Chicago, Chicago, Illinois, from December 1982 to October 1987 Department of Ener Technical Services B y ivision Oak Ridge Operations Office December 1989 -1 _--_ _ ~~~ ---- m.. *-*...___, .a. dez4em. A I LEGAL NoT1CE This report was prepared as an account of work sponsored by the United States Government. Neither the United States nor the United States Department of Energy, nor any of their employees, nor any of their contractors, subcontractors, or their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness or usefulness of any information, apparatus, product or process disclosed, or represents that its use would not infringe privately owned rights. '

5

IA Blog Archive  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

71 IA Blog Archive en IA News Archive http:energy.goviaia-news-archive IA News Archive

6

Residence Inn Chicago Midway Airport Residence Inn Chicago Midway Airport  

E-Print Network (OSTI)

Residence Inn Chicago � Midway Airport Residence Inn Chicago � Midway Airport 6638 S. Cicero Avenue by Marriott Chicago Midway Airport is located ten miles from downtown Chicago. The hotel offers free shuttle-suite, extended-stay hotel - 5 blocks from Midway Airport � 5 floors, 132 suites � AAA 3 Diamonds � Complimentary

Pritchard, Jonathan

7

Holiday Inn Chicago Midway Airport Holiday Inn Chicago Midway Airport  

E-Print Network (OSTI)

Holiday Inn Chicago ­ Midway Airport Holiday Inn Chicago ­ Midway Airport 6624 S. Cicero Avenue of arrival. Holiday Inn Chicago Midway Airport is located just ten miles from downtown Chicago and offers complimentary 24 hour airport shuttle service to and from Midway Airport. The hotel offers amenities

Pritchard, Jonathan

8

Wildlife in Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

386-A September 12, 1970 386-A September 12, 1970 Forest Preserve District of Cook County George W. Dunne, President Roland F. Eisenbeis, Supt. of Conservation WILDLIFE IN CHICAGO In August of 1803, when a detachment of soldiers came here from Detroit to build Fort Dearborn, they found only four crude cabins, situated on the north bank of the Chicago River. Three were occupied by French fur traders -- LeMaie, Ouilmette and Pettle -- and one was vacant. In 1833, when Chicago was incorporated as a village, there were only 200 people here. Wolves were still a problem, especially in winter. On October 6, 1834, a black bear -- the last wild one seen in Chicago was killed near the intersection of LaSalle and Adams Streets. Game was so plentiful that the region was a hunter's paradise .

9

THE UNIVERSITY' OF CHICAGO  

Office of Legacy Management (LM)

.G: THE UNIVERSITY' OF CHICAGO DATE December 28, 194s I TO C. F. Hiskey DLP*Rr"LNT MUCtft+-3I DEPARTMENT This document ConhtS Of...2, IN RE: Bloaaningtcn' Experiments pages and...

10

The University of Chicago, Chicago, I  

NLE Websites -- All DOE Office Websites (Extended Search)

.** .** # [Contribution from the George Herbert Jones Laboratory, The University of Chicago, Chicago, I l l i n o i s ] ffjl j t18 The Isotopic Discrimination of Some Solutes in Liquid Ammonia YQHJCLY ItHbEASABLS Arlen Viste and Henry Taube (1) ( a ) Department of Chemistry, Augustana College, Sioux F a l l s , South Dakota; (b) Department of Chemistry, Stanford University, Stanford, California. Abstract The nitrogen isotopic discrimination of some s a l t s and metals, studied in liquid ammonia solution at -50°C, decreases in magnitude in the order Pb , Ca , Li , Ag , Na , Li, K , Na, K. The i s o t o p i c discrimination appears t o provide q u a l i t a t i v e information about the strength of the cation-solvent i n t e r a c t i o n in liquid ammonia. Introduction Dissolving an anhydrous s

11

The University of Chicago Chicago, Illinois  

Office of Legacy Management (LM)

r \ ffs- sd %+/2-Z ; -- -37 d ~~;sT;,LLURGICAL PROJECT FOR11 i!P-73 The University of Chicago Chicago, Illinois 3 t-&LA% tf-s-6G-7 I CL LA- EL+ I;'OTICE OF Tl;;RklINkTICN CF SUF-',CCNTF&CT Contract No. 7401-37- 122 To: 3% Tool and Snpineering Conpahy 4555 !:' . Addison Street Chiwo, Ilu , Subcontractor Attention: Mr. Ralph Daleiden Office Manager Gentlerllen: You are hereby notified that by mason ofnormal. expiration certain subcontract between you and The University of Chicago dated February 20, 1944 and bearing descriptive nurrber above indicated, is terminate; as of the30th day of Juqe , 1944. i,ccording to our records, unpaid invoices: we have on hand the following #4912 ?1,136.50 4913 429.62 4911 69.00 4914 749.13 4987 390.75 !7e believe these to be the full extent of our liability to you.

12

MMSNF 2013 Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

Argonne National Laboratory Argonne National Laboratory University of Chicago Chicago Photography courtesy Thomas F Ewing Program: Last Modified: Oct. 14, 2013 Summary Discussion at MMSNF 2013 workshop For a wrap-up of the last workshop, see MMSNF 2013 Chicago Workshop Summary. MMSNF Workshops Learn more about the series at MMSNF Workshops. Privacy and Security Notice Program The Materials Modeling and Simulation of Nuclear Fuels (MMSNF) workshop series aims at stimulating research and discussions on models and simulations of nuclear fuels and coupling the results into fuel performance codes, with the hope that this leads to improved fuel designs. Although centered on multi-scale model development and computer simulations, close connections to theory, experiment and technology are encouraged.

13

Category:Chicago, IL | Open Energy Information  

Open Energy Info (EERE)

IL IL Jump to: navigation, search Go Back to PV Economics By Location Media in category "Chicago, IL" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Chicago IL Commonwealth Edison Co.png SVFullServiceRestauran... 74 KB SVHospital Chicago IL Commonwealth Edison Co.png SVHospital Chicago IL ... 68 KB SVLargeHotel Chicago IL Commonwealth Edison Co.png SVLargeHotel Chicago I... 75 KB SVLargeOffice Chicago IL Commonwealth Edison Co.png SVLargeOffice Chicago ... 76 KB SVMediumOffice Chicago IL Commonwealth Edison Co.png SVMediumOffice Chicago... 73 KB SVMidriseApartment Chicago IL Commonwealth Edison Co.png SVMidriseApartment Chi... 77 KB SVOutPatient Chicago IL Commonwealth Edison Co.png SVOutPatient Chicago I... 74 KB SVPrimarySchool Chicago IL Commonwealth Edison Co.png

14

Wildlife in Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

650 October 7, 1961 650 October 7, 1961 Forest Preserve District of Cook County John J. Duffy, President Roberts Mann, Conservation Editor David H. Thompson, Senior Naturalist WILDLIFE IN CHICAGO Few people realize that there is enough native wildlife worth mentioning in roaring, jam-packed Chicago, nor that very much of it is left in its fringe of adjoining suburbs. Surprisingly, this is not the case. Just as rural people become accustomed to urban life, some wild birds and mammals have adjusted to city life and are holding their own. A few kinds seem to be more numerous in parts of metropolitan Chicago than they were in those same areas a hundred years ago. The white-tailed deer, long extinct in this part of Illinois, is on the increase in the Chicago region. In recent winters two of them, perhaps chased by dogs, were rescued from the ice on the lake front -- one at Jackson Park and the other in the Calumet region.

15

The Chicago Academy of Sciences  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago Academy of Sciences Chicago Academy of Sciences Nature Bulletin No. 547-A De3cember 7, 1974 Forest Preserve District of Cook County George W. Dunne, President Roland F. Eisenbeis, Supt. of Conservation THE CHICAGO ACADEMY OF SCIENCES The Chicago Academy of Sciences is 117 years old this year. Chicago itself is not much older. It is significant of the rapid growth of our country, that only 100 years ago Chicago was a sprawling pioneer community. In fact, when the Academy was founded in 1857, it was the first scientific institution on the scene and one of the first museums in the West. The Smithsonian Institution in Washington had been founded only eleven years earlier and Robert Kennicott, first director of the Chicago Academy, was a young protégé of Smithsonian's director, the great Spencer Fullerton Baird.

16

The University of Chicago,  

Office of Legacy Management (LM)

a?-&= a?-&= d -j-his document consists Of............--- -,...figures pages an_d...~.....~~.....--.-----~--~~es k --ye.. No ,.... &...ot /u cople:s, 3' . . . . . . . . . . . . SERVICE & supply SUBCONTRACT # 740~37-m 115 This subcontract entered into this 1st day of.Agril 1944 by and between The University of Chicago, a corporation not for pecuniary profit organized under the laws of the State of Illinois, of Chica,o, Yontractorfl and R. Krasberg & Sons ALif Illinois (hereinafter called the g. co. a corpration organized under the laws of the State 6f. llllnols , of Chicago, llllnols (hereinafter called the ltSubcorltractorlt. VW?REAS, the Contractor has heretofore entered into a contract with the United States of America (represented by its duly designated contracting officer) under

17

Chicago Area Alternative Fuels Deployment Project (CAAFDP) |...  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

Meeting arravt061tibingham2012o.pdf More Documents & Publications Chicago Area Alternative Fuels Deployment Project (CAAFDP) Chicago Area Alternative Fuels Deployment Project...

18

American Chemical Society Award Winners, Chicago, III.  

Science Journals Connector (OSTI)

American Chemical Society Award Winners, Chicago, III. ... Copyright 1970 American Chemical Society ...

1970-10-01T23:59:59.000Z

19

After the Blast: Building and Unbuilding Memories of Port Chicago  

E-Print Network (OSTI)

Personnel Who Served at Port Chicago After Explosion Monday3f.htm. Comments Page: Port Chicago Historians SeekCommittee on Natural Resources. Port Chicago Naval Magazine

Arbona, Javier

2013-01-01T23:59:59.000Z

20

Urban Nature Centers and House Prices in Chicago  

E-Print Network (OSTI)

Transit Line: Chicagos Midway Line, 1983-1999, Real Estateimpact of Chicagos new Midway rapid transit line provides afor the new Orange Line to Midway Airport, which opened in

McGrath, Daniel T PhD; MCMILLEN, DANIEL P

2007-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Chicago Climate Action Plan | Open Energy Information  

Open Energy Info (EERE)

Action Plan Action Plan Jump to: navigation, search Name Chicago Climate Action Plan Agency/Company /Organization City of Chicago Focus Area Buildings, Energy Efficiency - Central Plant, Greenhouse Gas, Other, Non-renewable Energy, Transportation, Renewable Energy Phase Prepare a Plan Topics Low emission development planning Resource Type Case studies/examples Availability Free Website http://www.chicagoclimateactio Locality Chicago, IL References Chicago Climate Action Plan[1] Overview Chicago's Climate Action Plan addresses both mitigation of and adaptation to climate change and encompasses the entire city (rather than only City operations). The plan contains a high-level overview of Chicago's climate action initiatives, including 26 mitigation strategies and nine adaptation

22

FTCP Site Specific Information - Chicago Office | Department...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

- Chicago Office FTCP Agent Organization Name Phone E-Mail Chicago Office Patrick N. Smith (OR) (Interim FTCP Agent) 865574-0960 smithpn@oro.doe.gov Annual Workforce Analysis...

23

Chicago Metropolitan Agency for Planning Data Dashboard  

Energy.gov (U.S. Department of Energy (DOE))

The data dashboard for Chicago Metropolitan Agency for Planning, a partner in the Better Buildings Neighborhood Program.

24

Category:Mason, IA | Open Energy Information  

Open Energy Info (EERE)

IA IA Jump to: navigation, search Go Back to PV Economics By Location Media in category "Mason, IA" The following 16 files are in this category, out of 16 total. SVQuickServiceRestaurant Mason IA MidAmerican Energy Co (Iowa).png SVQuickServiceRestaura... 64 KB SVFullServiceRestaurant Mason IA MidAmerican Energy Co (Iowa).png SVFullServiceRestauran... 64 KB SVHospital Mason IA MidAmerican Energy Co (Iowa).png SVHospital Mason IA Mi... 73 KB SVLargeHotel Mason IA MidAmerican Energy Co (Iowa).png SVLargeHotel Mason IA ... 72 KB SVLargeOffice Mason IA MidAmerican Energy Co (Iowa).png SVLargeOffice Mason IA... 73 KB SVMediumOffice Mason IA MidAmerican Energy Co (Iowa).png SVMediumOffice Mason I... 69 KB SVMidriseApartment Mason IA MidAmerican Energy Co (Iowa).png

25

New approaches for modeling type Ia supernovae  

E-Print Network (OSTI)

ich and J. Stein. On the thermonuclear runaway in Type IaSmall-Scale Stability of Thermonuclear Flames o in Type IaS. E. Woosley. The thermonuclear explosion of chandrasekhar

Zingale, Michael; Almgren, Ann S.; Bell, John B.; Day, Marcus S.; Rendleman, Charles A.; Woosley, Stan

2007-01-01T23:59:59.000Z

26

Clean Cities: Chicago Area Clean Cities coalition  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

Chicago Area Clean Cities Coalition Chicago Area Clean Cities Coalition The Chicago Area Clean Cities coalition works with vehicle fleets, fuel providers, community leaders, and other stakeholders to reduce petroleum use in transportation. Chicago Area Clean Cities coalition Contact Information Samantha Bingham 312-744-8096 samantha.bingham@cityofchicago.org Coalition Website Clean Cities Coordinator Samantha Bingham Photo of Samantha Bingham Samantha Bingham is an Environmental Policy Analysis for the City of Chicago and has served as the coordinator for the Chicago Clean Cities coalition since 2006. Samantha manages several of the city's air quality improvement programs, coordinates responses to grant solicitations, and through analytical support and subject-matter knowledge assists in developing city policies and ordinances. In her role as a Clean Cities

27

Chicago Area Alternative Fuels Deployment Project (CAAFDP)  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

risks - Unforeseen permitting issues - Construction delays - Availability of equipment * Gas Technology Institute (GTI) * Chicago Area Clean Cities Coalition * State of Illinois,...

28

UNIVERSITY OF ILLINOIS AT CHICAGO MUPP DEGREE  

E-Print Network (OSTI)

UNIVERSITY OF ILLINOIS AT CHICAGO MUPP DEGREE Student Handbook AY20102011 Department......................................................................................... 4 3. Scope of the Handbook............................................... 12 6.3.4. Physical Planning (PP) Concentration

Illinois at Chicago, University of

29

Chicago Area Alternative Fuels Deployment Project (CAAFDP)  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Partners Patson-Exel-Diageo City of Chicago Richard M. Daley Mayor Vehicles -12 CNG conversions Infrastructure -1 new public CNG station Project Partners Peoples Gas ...

30

Chicago Metropolitan Agency for Planning Data Dashboard | Department...  

Energy Savers (EERE)

Data Dashboard Chicago Metropolitan Agency for Planning Data Dashboard The data dashboard for Chicago Metropolitan Agency for Planning, a partner in the Better Buildings...

31

Chicago Metropolitan Agency for Planning Summary of Reported...  

Energy Savers (EERE)

Summary of Reported Data Chicago Metropolitan Agency for Planning Summary of Reported Data Summary of data reported by Better Buildings Neighborhood Program partner Chicago...

32

January 11, 2007 Chicago ATLAS Group  

E-Print Network (OSTI)

for sLHC US ATLAS Tier 2 / 3 computing facility Joint with Indiana University Remote monitoringJ. Pilcher January 11, 2007 Chicago ATLAS Group #12;January 11, 2008 J. Pilcher2 Introduction Very exciting time for the LHC program and ATLAS First collisions later this year ATLAS will be ready Chicago

33

Abstract IA37: Clinical genomics  

Science Journals Connector (OSTI)

...Research. 15 October 2014 meeting-abstract Clinical Genomics Clinical Genomics: Oral Presentations - Invited Abstracts Abstracts...2013; San Diego, CA Abstract IA37: Clinical genomics Katherine A. Janeway Dana-Farber Cancer Institute...

Katherine A. Janeway

2014-10-15T23:59:59.000Z

34

Chicago Metropolitan Agency for Planning Summary of Reported Data  

Energy.gov (U.S. Department of Energy (DOE))

Summary of data reported by Better Buildings Neighborhood Program partner Chicago Metropolitan Agency for Planning.

35

Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

9 AC Level 2 9 AC Level 2 Philadelphia Atlanta 10 AC Level 2 Washington D.C. 31 AC Level 2 Washington State 263 AC Level 2 3 DC Fast Charge Oregon 419 AC Level 2 14 DC Fast Charge San Francisco 56 AC Level 2 9 DC Fast Charge Los Angeles 250 AC Level 2 2 DC Fast Charge San Diego 324 AC Level 2 1 DC Fast Charge Phoenix 400 AC Level 2 13 DC Fast Charge Tucson 99 AC Level 2 Dallas/FW 200 AC Level 2 Houston 84 AC Level 2 Nashville 225 AC Level 2 4 DC Fast Charge Knoxville 150 AC Level 2 3 DC Fast Charge Memphis 22 AC Level 2 Chattanooga 56 AC Level 2 6 DC Fast Charge Copyright:© 2009 ESRI Public Blink Charging Units Reporting Data in The EV Project 0 120 240 360 480 60 Miles ² Idaho National Laboratory 2/11/2013 INL/MIS-12-26073 Project to Date through December 2012 Legend Project Regions

36

Chicago Operations Office: Technology summary  

SciTech Connect

This document has been prepared by the Department of Energy`s (DOE) Environmental Management (EM) Office of Technology Development (OTD) to highlight its research, development, demonstration, testing, and evaluation (RDDT and E) activities funded through the Chicago Operations Office. Technologies and processes described have the potential to enhance DOE`s cleanup and waste management efforts, as well as improve US Industry`s competitiveness in global environmental markets. The information has been assembled from recently produced OTD documents which highlight technology development activities within each of the OTD program elements. OTD technologies addresses three specific problem areas: (1) groundwater and soils cleanup; (2) waste retrieval and processing; and (3) pollution prevention. These problems are not unique to DOE, but are associated with other Federal agency and industry sites as well. Thus, technical solutions developed within OTD programs will benefit DOE, and should have direct applications in outside markets.

Not Available

1994-12-01T23:59:59.000Z

37

String Landscape and Supernovae Ia  

E-Print Network (OSTI)

We present a model for the triggering of Supernovae Ia (SN Ia) by a phase transition to exact supersymmetry (susy) in the core of a white dwarf star. The model, which accomodates the data on SN Ia and avoids the problems of the standard astrophysical accretion based picture, is based on string landscape ideas and assumes that the decay of the false broken susy vacuum is enhanced at high density. In a slowly expanding susy bubble, the conversion of pairs of fermions to pairs of degenerate scalars releases a significant amount of energy which induces fusion in the surrounding normal matter shell. After cooling, the absence of degeneracy pressure causes the susy bubble to collapse to a black hole of about 0.1 solar mass or to some other stable susy object.

L. Clavelli

2011-10-09T23:59:59.000Z

38

UNIVERSITY OF ILLINOIS AT CHICAGO MUPP DEGREE  

E-Print Network (OSTI)

UNIVERSITY OF ILLINOIS AT CHICAGO MUPP DEGREE Student Handbook AY2012-2013 Department of Urban......................................................................................... 4 3. Scope of the Handbook............................................... 13 6.3.4. Physical Planning (PP) Concentration

Illinois at Chicago, University of

39

Evaluating Sites for Industrial Cogeneration in Chicago  

E-Print Network (OSTI)

and hospital complexes; and new, densely populated residential developments that have large thermal and electric demands. Potential sites have been evaluated as part of a project to encourage industrial cogeneration applications in Chicago. Energy...

Fowler, G. L.; Baugher, A. H.

1982-01-01T23:59:59.000Z

40

Lessons Learned: Creating the Chicago Climate Action Plan | Open Energy  

Open Energy Info (EERE)

Lessons Learned: Creating the Chicago Climate Action Plan Lessons Learned: Creating the Chicago Climate Action Plan Jump to: navigation, search Name Lessons Learned: Creating the Chicago Climate Action Plan Agency/Company /Organization City of Chicago Partner Global Philanthropy Partnership, ICLEI Focus Area Buildings, Energy Efficiency - Central Plant, Greenhouse Gas, Other, Non-renewable Energy, Transportation, Renewable Energy Phase Create a Vision, Determine Baseline, Develop Goals, Prepare a Plan, Get Feedback, Create Early Successes Topics Low emission development planning Resource Type Lessons learned/best practices Availability Free Publication Date 6/1/2008 Website http://www.chicagoclimateactio Locality Chicago, IL References Lessons Learned: Creating the Chicago Climate Action Plan[1] Overview

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

ChiCago MediCine University of  

E-Print Network (OSTI)

ChiCago MediCine University of on the midway SPRING2008 Biological Sciences Division medical the health of millions. Spring 2008University of Chicago Medicine on the Midway A Hutterite boy has blood

Ober, Carole

42

Chicago Office 9800 South Cass Avenue  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Office of Science Office of Science Chicago Office 9800 South Cass Avenue Argonne, Illinois 60439 ·tf= N= R= OMNP= MEMORANDUM FOR GREGORY H. WOODS GENERAL COUNSEL GC-1/FORS FROM: SUBJECT: ROXANNE E. PURUCfEf= j-r�= MANAGER �rl-1?= CHICAGO OFFICE {CH) 2013 ANNUAL NATIONAL ENVIRONMENTAL POLICY ACT {NEPA) PLANNING SUMMARY Section 5{a){7) of Department of Energy Order 451.1B, Change 3, NEPA Compliance Program, requires each Secretarial Officer and Head of Field Organization to submit an

43

Alliance of Chicago Community Health Services, L3C 215 W. Ohio, 4th floor Chicago, IL 60654  

E-Print Network (OSTI)

Alliance of Chicago Community Health Services, L3C 215 W. Ohio, 4th floor Chicago, IL 60654 Phone at the Alliance of Chicago Community Health Services (Alliance). He/She is responsible for programming design life cycle for the Alliance EHR, which includes the following primary tasks: o Programming

Liblit, Ben

44

Chicago Solar Express Reduces Costs, Wait Times  

Office of Energy Efficiency and Renewable Energy (EERE)

The Solar Express program in Chicago, Illinoisfunded through a SunShot Initiative Rooftop Solar Challenge (RSC) I award of $750,000is making it faster, easier, and cheaper for residents to go solar by cutting long wait times and fees for solar permits.

45

Chemists react to new compounds in Chicago  

Science Journals Connector (OSTI)

...areas such as analytical chemistry and agrochemicals, researchers showcased new environmentally...only the active twin, drugmakers and agrochemical companies are increasingly relying...for a prod-uct with just the right composition. At the Chicago meeting a group of...

RF Service

1995-09-08T23:59:59.000Z

46

2009 National Electric Transmission Congestion Study - Chicago Workshop |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Chicago Workshop 2009 National Electric Transmission Congestion Study - Chicago Workshop On September 17, 2008, DOE hosted a regional pre-study workshop in Chicago, IL to receive input and suggestions concerning the 2009 National Electric Transmission Congestion Study. The agenda, full transcript, and documents submitted for consideration for the 2009 study are available below. 9-17-08 Congestion Workshop Agenda - Chicago, IL.pdf Transcript - 2009 National Electric Transmission Congestion Study Chicago Workshop.pdf Statement of Michael J. Kormos, PJM Interconnection, submitted at 2009 Congestion Study Chicago workshop.pdf More Documents & Publications 2009 National Electric Transmission Congestion Study - San Francisco Workshop 2009 National Electric Transmission Congestion Study - Las Vegas Workshop

47

2009 National Electric Transmission Congestion Study - Chicago Workshop |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Chicago Workshop 2009 National Electric Transmission Congestion Study - Chicago Workshop On September 17, 2008, DOE hosted a regional pre-study workshop in Chicago, IL to receive input and suggestions concerning the 2009 National Electric Transmission Congestion Study. The agenda, full transcript, and documents submitted for consideration for the 2009 study are available below. 9-17-08 Congestion Workshop Agenda - Chicago, IL.pdf Transcript - 2009 National Electric Transmission Congestion Study Chicago Workshop.pdf Statement of Michael J. Kormos, PJM Interconnection, submitted at 2009 Congestion Study Chicago workshop.pdf More Documents & Publications Blackout 2003: Electric System Working Group Technical Conference - Comments and Recommendations 2009 National Electric Transmission Congestion Study - San Francisco

48

Steamboat IA Geothermal Facility | Open Energy Information  

Open Energy Info (EERE)

IA Geothermal Facility IA Geothermal Facility Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Steamboat IA Geothermal Facility General Information Name Steamboat IA Geothermal Facility Facility Steamboat IA Sector Geothermal energy Location Information Location Washoe, Nevada Coordinates 40.5608387°, -119.6035495° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":40.5608387,"lon":-119.6035495,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

49

Chicago Clean Energy Alliance | Open Energy Information  

Open Energy Info (EERE)

Alliance Alliance Jump to: navigation, search Name Chicago Clean Energy Alliance Place Chicago, Illinois Year founded 2009 Website http://www.theccea.org Coordinates 41.850033°, -87.6500523° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.850033,"lon":-87.6500523,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

50

Archive Reference Buildings by Climate Zone: 5A Chicago, Illinois |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

A Chicago, Illinois A Chicago, Illinois Archive Reference Buildings by Climate Zone: 5A Chicago, Illinois Here you will find past versions of the reference buildings for new construction commercial buildings, organized by building type and location. A summary of building types and climate zones is available for reference. Current versions are also available. You can download ZIP files that contain the following: An EnergyPlus software input file (.idf) An html file showing the results from the EnergyPlus simulation (.html) A spreadsheet that summarizes the inputs and results for each location (.xls) The EnergyPlus TMY2 weather file (.epw). benchmark-v1.0_3.0-5a_il_chicago.zip benchmark-v1.1_3.1-5a_usa_il_chicago-ohare.zip benchmark-new-v1.2_4.0-5a_usa_il_chicago-ohare.zip More Documents & Publications

51

Categorical Exclusion Determinations: Chicago Office | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Office Chicago Office Categorical Exclusion Determinations: Chicago Office Categorical Exclusion Determinations issued by Chicago Office. DOCUMENTS AVAILABLE FOR DOWNLOAD July 17, 2013 CX-010689: Categorical Exclusion Determination Generic CX Determination for Financial Assistance Awards CX(s) Applied: Unknown Date: 07/17/2013 Location(s): Illinois Offices(s): Chicago Office June 5, 2013 CX-010531: Categorical Exclusion Determination Renovation of the LSU Nuclear Science Building and Development of LSU's Nuclear Workforce Development Program CX(s) Applied: B3.14 Date: 06/05/2013 Location(s): Illinois Offices(s): Chicago Office February 9, 2012 CX-008000: Categorical Exclusion Determination Crystal Chemistry of Toxic Metal Sequestration CX(s) Applied: B3.6 Date: 02/09/2012

52

Chicago Joins President Obama's Better Buildings Challenge to...  

Office of Environmental Management (EM)

Joins President Obama's Better Buildings Challenge to Reduce Energy Use and Save Money Chicago Joins President Obama's Better Buildings Challenge to Reduce Energy Use and...

53

Video: Argonne + Chicago Scholars program - LaVaun Bowling |...  

NLE Websites -- All DOE Office Websites (Extended Search)

Video: Argonne + Chicago Scholars program - LaVaun Bowling Share Topic Community Education High school Undergraduate students Internships Environment Environmental science &...

54

2011 Annual Planning Summary for Chicago Operations Office (CH)  

Energy.gov (U.S. Department of Energy (DOE))

The ongoing and projected Environmental Assessments and Environmental Impact Statements for 2011 and 2012 within the Chicago Operations Office (CH) (See Science APS).

55

Quadrennial Energy Review August 8, 2014 Chicago , Il.  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

August 8, 2014 Chicago, Il. Panel 1: Highway Infrastructure and Energy Transportation Infrastructure from the MAFC Perspective. Ernie Perry, PhD. ebperry@wisc.edu University Of...

56

Quadrennial Energy Review Stakeholder Meeting #9: Chicago, IL  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

At the Quadrennial Energy Review Stakeholder Meeting 9: Chicago, IL Rail, Barge, Truck Transportation Issues August 8, 2014 Opening Remarks The Honorable Rahm Emanuel, Mayor of...

57

THE LOCAL HOSTS OF TYPE Ia SUPERNOVAE  

SciTech Connect

We use multi-wavelength, matched aperture, integrated photometry from the Galaxy Evolution Explorer (GALEX), the Sloan Digital Sky Survey, and the RC3 to estimate the physical properties of 166 nearby galaxies hosting 168 well-observed Type Ia supernovae (SNe Ia). The ultraviolet (UV) imaging of local SN Ia hosts from GALEX allows a direct comparison with higher-redshift hosts measured at optical wavelengths that correspond to the rest-frame UV. Our data corroborate well-known features that have been seen in other SN Ia samples. Specifically, hosts with active star formation produce brighter and slower SNe Ia on average, and hosts with luminosity-weighted ages older than 1 Gyr produce on average more faint, fast, and fewer bright, slow SNe Ia than younger hosts. New results include that in our sample, the faintest and fastest SNe Ia occur only in galaxies exceeding a stellar mass threshold of approx10{sup 10} M{sub sun}, leading us to conclude that their progenitors must arise in populations that are older and/or more metal rich than the general SN Ia population. A low host extinction subsample hints at a residual trend in peak luminosity with host age, after correcting for light-curve shape, giving the appearance that older hosts produce less-extincted SNe Ia on average. This has implications for cosmological fitting of SNe Ia, and suggests that host age could be useful as a parameter in the fitting. Converting host mass to metallicity and computing {sup 56}Ni mass from the supernova light curves, we find that our local sample is consistent with a model that predicts a shallow trend between stellar metallicity and the {sup 56}Ni mass that powers the explosion, but we cannot rule out the absence of a trend. We measure a correlation between {sup 56}Ni mass and host age in the local universe that is shallower and not as significant as that seen at higher redshifts. The details of the age-{sup 56}Ni mass correlations at low and higher redshift imply a luminosity-weighted age threshold of approx3 Gyr for SN Ia hosts, above which they are less likely to produce SNe Ia with {sup 56}Ni masses above approx0.5 M{sub sun}.

Neill, James D.; Martin, D. Christopher; Barlow, Tom A.; Foster, Karl; Friedman, Peter G.; Morrissey, Patrick; Wyder, Ted K. [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Sullivan, Mark [University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH (United Kingdom); Howell, D. Andrew [Las Cumbres Observatory Global Telescope Network, 6740 Cortona Dr., Suite 102, Goleta, CA 93117 (United States); Conley, Alex [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ONM5S3H8 (Canada); Seibert, Mark; Madore, Barry F. [The Observatories of the Carnegie Institute of Washington, 813 Santa Barbara Street, Pasadena, CA, 91101 (United States); Neff, Susan G. [Laboratory for Astronomy and Solar Physics, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Schiminovich, David [Department of Astronomy, Columbia University, New York, NY 10027 (United States); Bianchi, Luciana [Center for Astrophysical Sciences, Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218 (United States); Donas, Jose; Milliard, Bruno [Laboratoire d'Astrophysique de Marseille, BP 8, Traverse du Siphon, 13376 Marseille Cedex 12 (France); Heckman, Timothy M. [Department of Physics and Astronomy, Johns Hopkins University, Homewood Campus, Baltimore, MD 21218 (United States); Lee, Young-Wook [Center for Space Astrophysics, Yonsei University, Seoul 120-749 (Korea, Republic of); Rich, R. Michael [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States)

2009-12-20T23:59:59.000Z

58

Secretary Chu and Chicago Mayor Rahm Emanuel to Make Energy Efficiency...  

Energy Savers (EERE)

Secretary Chu and Chicago Mayor Rahm Emanuel to Make Energy Efficiency Announcement Secretary Chu and Chicago Mayor Rahm Emanuel to Make Energy Efficiency Announcement June 5, 2012...

59

Supersoft Sources as SN Ia Progenitors  

E-Print Network (OSTI)

of the existence of supersoft X­ray sources. It is argued that SNe Ia are thermonuclear explosions of accreting C is that they represent thermonuclear disruptions of mass accreting white dwarfs (WDs). Thus, the basic ingredient

Greiner, Jochen

60

ETODOS NUM ERICOS EN INGENIER IA  

E-Print Network (OSTI)

CONSERVATIVOS ENERG #19; IA-MOMENTO Jos#19;e M. Goicolea Ruig#19;omez y Juan Carlos Garc#19;#16;a Orden EscuelaM #19; ETODOS NUM #19; ERICOS EN INGENIER #19; IA R. Abascal, J. Dom#19;#16;nguez y G. Bugeda (Eds.upm.es Palabras clave: Din#19;amica no lineal, mecanismos, sistemas multicuerpo exibles, energ#19;#16;a- momento

Romero, Ignacio

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Focus Series- Chicago-Energy Impact Illinois (EI2)  

Energy.gov (U.S. Department of Energy (DOE))

Focus Series - Chicago-energy Impact Illinois (EI2) - A community-based, boots-on-the-ground outreach campaign. Through a house party initiative, EI2 brought Chicago homeowners, neighbors, and friends together to learn about energy efficiency opportunities, while increasing demand for home energy assessments and upgrades.

62

Engineering May 11, 2013 UIC University of Illinois at Chicago  

E-Print Network (OSTI)

Engineering May 11, 2013 UIC University of Illinois at Chicago Dear Engineering Graduates Nelson Dean and Professor #12;Engineering May 11, 2013 UIC University of Illinois at Chicago Class . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . PhD, Master of Science, Master of Energy Engineering, and Master of Engineering SINGING OF "THE STAR

Illinois at Chicago, University of

63

Why do we power our cars with gas? NBC Chicago  

ScienceCinema (OSTI)

Why can we only power our cars with gas? NBC-Chicago tackles this question with a trip to Argonne National Lab, where work on the Omnivorous Engine (runs on any blend of ethanol, butanol, and gasoline) and electric vehicles continues. A segment from NBC-Chicago's "Good Question" series.

None

2013-04-19T23:59:59.000Z

64

DOE Office of Science - Chicago Office  

NLE Websites -- All DOE Office Websites

spacer spacer spacer spacer About DOE Organization News Contact Us Search Go Button spacer U.S. Department of Energy Science & Technology Energy Sources Energy Efficiency The Environment Prices & Trends National Security Safety & Health spacer Office of Science Chicago Office - Integrated Support Center spacer spacer CURRENT SOLICITATIONS Open Solicitations Unsolicited Proposals spacer spacer BUSINESS OPPORTUNITIES Office of Acquisition and Assistance Energy Related Inventions Doing Business with DOE spacer spacer HOW DO I FIND OUT ABOUT? Educational Materials Frequently Asked Questions Links Human Resources Services Office of Chief Counsel spacer spacer COMMUNITY Special Events Laboratory Community Involvement Programs Public Participation Policy Speakers Bureau

65

Independent Oversight Inspection, Chicago Office and Argonne National  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Office and Argonne Chicago Office and Argonne National Laboratory - September 2006 Independent Oversight Inspection, Chicago Office and Argonne National Laboratory - September 2006 September 2006 Independent Oversight Inspection of Classification and Information Control Programs at the Chicago Office and Argonne National Laboratory This report presents the results of inspection activities by the Office of Independent Oversight's Office of Security Evaluations in the area of classification and information control (CIC) at the Office of Science (SC) Chicago Office (CH), the Argonne Site Office, and the Argonne National Laboratory (ANL). To ensure a thorough evaluation, the subtopic areas of program administration, authorities, guidance, training, document reviews, and program evaluation were assessed. The data collection activities were

66

Business Opportunity Session Materials - December 14, 2011, Chicago |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Business Opportunity Session Materials - December 14, 2011, Chicago Business Opportunity Session Materials - December 14, 2011, Chicago Business Opportunity Session Materials - December 14, 2011, Chicago Our Business Opportunity Sessions bring small business owners and Departmental small business advocates together to talk about the best ways we can be partnering with the small business community. Download the presentation material below from our December 14, 2011, Business Opportunity Session held in Chicago, IL. For more information about Business Opportunity Sessions, visit our website. Sign up for our email list to get invites to upcoming events. How To Do Business with DOE Chicago BOS Dec 14 2011.pdf How To Do Business with DOE Charleston WV Nov 14 2011 BOS.pdf More Documents & Publications Regional Small Business Summit Material

67

Chicago Joins Better Buildings Initiative | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Better Buildings Initiative Better Buildings Initiative Chicago Joins Better Buildings Initiative June 5, 2012 - 2:34pm Addthis Secretary Chu joined Chicago Mayor Rahm Emanuel to announce the city’s participation in the Better Buildings Challenge. | Photo by Brooke Collins. Secretary Chu joined Chicago Mayor Rahm Emanuel to announce the city's participation in the Better Buildings Challenge. | Photo by Brooke Collins. April Saylor April Saylor Former Digital Outreach Strategist, Office of Public Affairs What does this project do? Chicago is committing to reduce building energy use by 20 percent in 24 million square feet within the next five years. 14 Chicago buildings (totaling almost 14 million sq. ft.) already signed on to join the program, which will save more than $5 million a year

68

Independent Oversight Inspection, Chicago Office and Argonne National  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Office and Argonne Chicago Office and Argonne National Laboratory - September 2006 Independent Oversight Inspection, Chicago Office and Argonne National Laboratory - September 2006 September 2006 Independent Oversight Inspection of Classification and Information Control Programs at the Chicago Office and Argonne National Laboratory This report presents the results of inspection activities by the Office of Independent Oversight's Office of Security Evaluations in the area of classification and information control (CIC) at the Office of Science (SC) Chicago Office (CH), the Argonne Site Office, and the Argonne National Laboratory (ANL). To ensure a thorough evaluation, the subtopic areas of program administration, authorities, guidance, training, document reviews, and program evaluation were assessed. The data collection activities were

69

City of Chicago - Building Energy Code | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago - Building Energy Code Chicago - Building Energy Code City of Chicago - Building Energy Code < Back Eligibility Residential Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Insulation Program Info State Illinois Program Type Building Energy Code Provider City of Chicago The Chicago Energy Conservation Code (CECC) requires residential buildings applying for building permits to comply with energy efficient measures which go beyond those required by the [http://www.dsireusa.org/library/includes/incentive2.cfm?Incentive_Code=I... Illinois Building Energy Code]. The applicability of the CECC to commercial construction was superseded when the state of Illinois adopted the more stringent IECC 2009 model code. Illinois state law in 2009 also mandated

70

154th National American Chemical Society Meeting Chicago, III. Sept. 10 to 15, 1967  

Science Journals Connector (OSTI)

154th National American Chemical Society Meeting Chicago, III. ... Copyright 1967 American Chemical Society ...

1967-08-01T23:59:59.000Z

71

University of Illinois at ChicagoUniversity of Illinois at ChicagoUniversity of Illinois at ChicagoUniversity of Illinois at Chicago ----BioE Seminar SeriesBioE Seminar SeriesBioE Seminar SeriesBioE Seminar Series FridayFridayFridayFriday,,,, SeptemberSep  

E-Print Network (OSTI)

University of Illinois at ChicagoUniversity of Illinois at ChicagoUniversity of Illinois at ChicagoUniversity of Illinois at Chicago ---- BioE Seminar SeriesBioE Seminar SeriesBioE Seminar SeriesBioE Seminar Series 60607606076060760607 The Second Law of Energy Degradation Including Biological and Intelligent Processes The Second Law

Kostic, Milivoje M.

72

Rolling Hills (IA) | Open Energy Information  

Open Energy Info (EERE)

Rolling Hills (IA) Rolling Hills (IA) Jump to: navigation, search Name Rolling Hills (IA) Facility Rolling Hills (IA) Sector Wind energy Facility Type Commercial Scale Wind Facility Status In Service Owner MidAmerican Energy Company Developer MidAmerican Energy Company Energy Purchaser MidAmerican Energy Company Location Massena IA Coordinates 41.230443°, -94.75459° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.230443,"lon":-94.75459,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

73

Chicago Operations Office 9800 South Cass Avenue  

Office of Legacy Management (LM)

y,: y; , i y,: y; , i 4- 1 .' f?Qj /J < b !. i-. .* ;+ ,.- Department of Energy Chicago Operations Office 9800 South Cass Avenue Argonne, Illinois 60439 : / *- I (jr-. _ __-rCILC-. .-WI __ James L. Liverman, Acting Assistant Secretary for Environment, HQ UNIVERSITY OF ARIZONA On January 17, 1978, Edward J. Jascewsky, Department of Energy (DOE), and Walter H. Smith, Argonne National Laboratory (AX), visited the University of Arizona. The purpose of the visit teas to discuss the past operations of c$rtain facilities that were previcusly used by the Bureau of Mines for the Atomic Energy Coxission xork. Enclosed are three drawings showing the location of these facilities. The Bureau of Mines activities have been closed down for abour fifteen years, and the property of concern is now owned by the L'niversiry of

74

Opportunities with Laboratories under the Chicago Office  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Opportunities with Opportunities with Laboratories under the Chicago Office 1 Princeton Plasma Physics Laboratory 1. Mechanical Engineering Services; Larry Dudek; $188,000 2. Phone system; William Bryan; $300,000 3. Engineering Support Services; Charles Neumyer; $1,417,116 4. Conceptual design of New PS&T Building; Shawn Connolly; $500,000 Lawrence Berkeley National Laboratory (LBL) 1. Software Maintenance and support for ALS software; 9/30/2011; $556,000 (Biointuition) 2. Consulting services to conduct a hazard survey; 9/30/11; $549,000 (Alphatrac, Inc.) 3. Analytical Laboratory services; 7/31/11; $465,000 (BC Laboratories, Inc.) LBL Continued.... 4. Blanket Order to provide photo artwork; 9/30/2011; $460,000 (CMP) 5. Pick-up and delivery courier servicces for as- needed services; 5/31/2011; $250,000 (IDS

75

Chicago Joins President Obama's Better Buildings Challenge to Reduce  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

President Obama's Better Buildings Challenge to President Obama's Better Buildings Challenge to Reduce Energy Use and Save Money Chicago Joins President Obama's Better Buildings Challenge to Reduce Energy Use and Save Money June 5, 2012 - 2:26pm Addthis NEWS MEDIA CONTACT (202) 586-4940 CHICAGO - U.S. Energy Secretary Steven Chu joined Mayor Rahm Emanuel at an event in Chicago today to announce that the city is joining the Obama Administration's Better Buildings Challenge, part of the initiative launched last year by President Obama to catalyze investment in commercial and industrial building energy upgrades and support new jobs across the country. As a partner in this national initiative, Chicago is committing to reduce energy use by 20 percent across nearly 24 million square feet of public and private building space within the next five years. The Better

76

Chicago Business Features Argonne Woman in Nuclear Physics | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Business Features Argonne Woman in Nuclear Physics Chicago Business Features Argonne Woman in Nuclear Physics Chicago Business Features Argonne Woman in Nuclear Physics January 9, 2012 - 4:08pm Addthis Kawtar Hafidi is an experimental nuclear physicist, working in the medium energy physics group at Argonne. Image courtesy of Argonne National Laboratory. Kawtar Hafidi is an experimental nuclear physicist, working in the medium energy physics group at Argonne. Image courtesy of Argonne National Laboratory. Chicago Business has the scoop about Kawtar Hafidi, an Argonne National Laboratory nuclear physicist who just snagged the Association for Women in Science's 2011 Innovator Award for her research in the field of the color of quarks. Hafidi is one of many women in science who's changing the equation to accomplish the Department's mission. At Argonne, she leads

77

Metallurgical Laboratory at the University of Chicago | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Operational Management » History » Manhattan Project » Signature Operational Management » History » Manhattan Project » Signature Facilities » Metallurgical Laboratory at the University of Chicago Metallurgical Laboratory at the University of Chicago Photo of the Met Lab and the Stagg Field Bleachers Photo of the Met Lab and the Stagg Field Bleachers One of the most important branches of the Manhattan Project was the Metallurgical Laboratory (Met Lab) in Chicago. Using the name "Metallurgical Laboratory" as cover at the University of Chicago, scientists from the east and west coasts were brought together to this central location to develop chain-reacting "piles" for plutonium production, to devise methods for extracting plutonium from the irradiated uranium, and to design a weapon. In all, four methods of plutonium

78

Nuclear Energy Panel Discussion at University of Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

Nuclear Energy Panel Discussion at University of Chicago Nuclear Energy Panel Discussion at University of Chicago Director's Welcome Organization Achievements Highlights Fact Sheets, Brochures & Other Documents Multimedia Library About Nuclear Energy Nuclear Reactors Designed by Argonne Argonne's Nuclear Science and Technology Legacy Opportunities within NE Division Visit Argonne Work with Argonne Contact us For Employees Site Map Help Join us on Facebook Follow us on Twitter NE on Flickr Celebrating the 70th Anniversary of Chicago Pile 1 (CP-1) Argonne OutLoud on Nuclear Energy Argonne Energy Showcase 2012 Highlights Bookmark and Share Nuclear Energy Panel Discussion at University of Chicago Did you miss this event? Watch recording of "Lessons from Fukushima" The event's webcast is over, but you can still watch and/or download the

79

Preliminary Notice of Violation, University of Chicago - EA-2006...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Issued to the University of Chicago related to Nuclear Safety Program Deficiencies at Argonne National Laboratory On March 7, 2006, the U.S. Department of Energy issued a...

80

Weapons in the City: Weapon Use in Chicago Homicide Cases.  

E-Print Network (OSTI)

??This study used data from the homicides in Chicago 1965-1995 dataset (N=9,340) to examine the relationship between the use of certain types of weapons in (more)

Johnson, Natalie Jo

2007-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

Focus Series - Chicago-Energy Impact Illinois (EI2) | Department...  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

Illinois (EI2) Focus Series - Chicago-energy Impact Illinois (EI2) - A community-based, boots-on-the-ground outreach campaign. Through a "house party" initiative, EI2 brought...

82

THE UNIVERSITY OF CHICAGO CHARACTERIZATION OF PROTEIN FOLDING INTERMEDIATES  

E-Print Network (OSTI)

THE UNIVERSITY OF CHICAGO CHARACTERIZATION OF PROTEIN FOLDING INTERMEDIATES FOR DELINEATION ............................................................................................................ 1 1.1 Why study protein folding .............................................................................. 3 1.2.1 How fast should a protein fold ........................................................... 3

Sosnick, Tobin R.

83

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

in the Fermilab Art Gallery are a collection of about ten years of painting the urban landscape in and around Chicago. I chose to exhibit a decade of work to demonstrate the...

84

DOE Cites University of Chicago for Nuclear Safety Violations | Department  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

University of Chicago for Nuclear Safety Violations University of Chicago for Nuclear Safety Violations DOE Cites University of Chicago for Nuclear Safety Violations March 7, 2006 - 11:42am Addthis WASHINGTON , DC - The Department of Energy (DOE) today issued a Preliminary Notice of Violation (PNOV) to the University of Chicago (University), the Management and Operating contractor for DOE's Argonne National Laboratory (ANL), for nuclear safety violations identified through several safety reviews and inspections conducted by DOE. A series of reviews and inspections, the most recent of which occurred in 2005, identified breakdowns in the contractor's quality improvement, radiation protection, work process, and independent and management assessment programs. Prior to 2005, senior contractor management at ANL

85

A threat-based definition of IA and IA-enabled products.  

SciTech Connect

This paper proposes a definition of 'IA and IA-enabled products' based on threat, as opposed to 'security services' (i.e., 'confidentiality, authentication, integrity, access control or non-repudiation of data'), as provided by Department of Defense (DoD) Instruction 8500.2, 'Information Assurance (IA) Implementation.' The DoDI 8500.2 definition is too broad, making it difficult to distinguish products that need higher protection from those that do not. As a consequence the products that need higher protection do not receive it, increasing risk. The threat-based definition proposed in this paper solves those problems by focusing attention on threats, thereby moving beyond compliance to risk management. (DoDI 8500.2 provides the definitions and controls that form the basis for IA across the DoD.) Familiarity with 8500.2 is assumed.

Shakamuri, Mayuri; Schaefer, Mark A.; Campbell, Philip LaRoche

2010-09-01T23:59:59.000Z

86

A threat-based definition of IA- and IA-enabled products.  

SciTech Connect

This paper proposes a definition of 'IA and IA-enabled products' based on threat, as opposed to 'security services' (i.e., 'confidentiality, authentication, integrity, access control or non-repudiation of data'), as provided by Department of Defense (DoD) Instruction 8500.2, 'Information Assurance (IA) Implementation.' The DoDI 8500.2 definition is too broad, making it difficult to distinguish products that need higher protection from those that do not. As a consequence the products that need higher protection do not receive it, increasing risk. The threat-based definition proposed in this paper solves those problems by focusing attention on threats, thereby moving beyond compliance to risk management. (DoDI 8500.2 provides the definitions and controls that form the basis for IA across the DoD.) Familiarity with 8500.2 is assumed.

Shakamuri, Mayuri; Schaefer, Mark A.; Campbell, Philip LaRoche

2010-07-01T23:59:59.000Z

87

Comparison of Recent SnIa datasets  

E-Print Network (OSTI)

We rank the six latest Type Ia supernova (SnIa) datasets (Constitution (C), Union (U), ESSENCE (Davis) (E), Gold06 (G), SNLS 1yr (S) and SDSS-II (D)) in the context of the Chevalier-Polarski-Linder (CPL) parametrization $w(a)=w_0+w_1 (1-a)$, according to their Figure of Merit (FoM), their consistency with the cosmological constant ($\\Lambda$CDM), their consistency with standard rulers (Cosmic Microwave Background (CMB) and Baryon Acoustic Oscillations (BAO)) and their mutual consistency. We find a significant improvement of the FoM (defined as the inverse area of the 95.4% parameter contour) with the number of SnIa of these datasets ((C) highest FoM, (U), (G), (D), (E), (S) lowest FoM). Standard rulers (CMB+BAO) have a better FoM by about a factor of 3, compared to the highest FoM SnIa dataset (C). We also find that the ranking sequence based on consistency with $\\Lambda$CDM is identical with the corresponding ranking based on consistency with standard rulers ((S) most consistent, (D), (C), (E), (U), (G) least consistent). The ranking sequence of the datasets however changes when we consider the consistency with an expansion history corresponding to evolving dark energy $(w_0,w_1)=(-1.4,2)$ crossing the phantom divide line $w=-1$ (it is practically reversed to (G), (U), (E), (S), (D), (C)). The SALT2 and MLCS2k2 fitters are also compared and some peculiar features of the SDSS-II dataset when standardized with the MLCS2k2 fitter are pointed out. Finally, we construct a statistic to estimate the internal consistency of a collection of SnIa datasets. We find that even though there is good consistency among most samples taken from the above datasets, this consistency decreases significantly when the Gold06 (G) dataset is included in the sample.

J. C. Bueno Sanchez; S. Nesseris; L. Perivolaropoulos

2009-10-01T23:59:59.000Z

88

Secretary Chu and Chicago Mayor Rahm Emanuel to Make Energy Efficiency  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago Mayor Rahm Emanuel to Make Energy Chicago Mayor Rahm Emanuel to Make Energy Efficiency Announcement Secretary Chu and Chicago Mayor Rahm Emanuel to Make Energy Efficiency Announcement June 5, 2012 - 9:02am Addthis CHICAGO - U.S. Energy Secretary Steven Chu will join Chicago Mayor Rahm Emanuel to make a major announcement about the City of Chicago's commitment to energy efficiency as part of the Obama Administration's all-of-the-above approach to American energy. Energy use in buildings accounts for more than 40 percent of U.S. energy use. By improving the energy efficiency of America's buildings, we can help families and businesses save money by saving energy. WHAT: Major announcement on energy efficiency by the Department of Energy and the City of Chicago WHO: U.S. Secretary of Energy Steven Chu and City of Chicago Mayor Rahm

89

City of Chicago won't sweat the flu with Argonne's help | Argonne...  

NLE Websites -- All DOE Office Websites (Extended Search)

City of Chicago won't sweat the flu with Argonne's help By Louise Lerner * September 7, 2011 Tweet EmailPrint This spring, officials at Chicago's Department of Public Health (CPDH)...

90

Category:Des Moines, IA | Open Energy Information  

Open Energy Info (EERE)

IA IA Jump to: navigation, search Go Back to PV Economics By Location Media in category "Des Moines, IA" The following 16 files are in this category, out of 16 total. SVFullServiceRestaurant Des Moines IA MidAmerican Energy Co (Iowa).png SVFullServiceRestauran... 64 KB SVQuickServiceRestaurant Des Moines IA MidAmerican Energy Co (Iowa).png SVQuickServiceRestaura... 64 KB SVHospital Des Moines IA MidAmerican Energy Co (Iowa).png SVHospital Des Moines ... 73 KB SVLargeHotel Des Moines IA MidAmerican Energy Co (Iowa).png SVLargeHotel Des Moine... 72 KB SVLargeOffice Des Moines IA MidAmerican Energy Co (Iowa).png SVLargeOffice Des Moin... 73 KB SVMediumOffice Des Moines IA MidAmerican Energy Co (Iowa).png SVMediumOffice Des Moi... 69 KB SVMidriseApartment Des Moines IA MidAmerican Energy Co (Iowa).png

91

Chicago-area SIAM student chapters visit Argonne | Argonne National  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago-area SIAM student chapters visit Argonne Chicago-area SIAM student chapters visit Argonne May 10, 2013 Tweet EmailPrint Forty undergraduate students, graduate students, and postdocs from Chicago-area SIAM chapters visited Argonne's Mathematics and Computer Science (MCS) Division on April 12 for a look into some of the exciting applied mathematics research being performed at the laboratory. The morning included ten "research vignettes" presented by MCS staff. Scalable power grid dynamics simulation (Shrirang Abhyankar) Data science for scientific computing: Learning and intelligent optimization (Prasanna Balaprakash) Parallel multigrid solvers (Jed Brown) Large-scale Gaussian process calculation without matrix factorizations (Jie Chen) Scaling computational fluid dynamics beyond a million cores (Paul

92

Technical Qualification Program Description - Integrated Support Center, Chicago Office  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

DEPART ENT of Office of DEPART ENT of Office of ENERGY I Science Integrated Support Center Chicago Office Technical Qualification Program Description ~~~~~~'?£H(.k:1/Zi.':"r'fl. ; ;!. / ; h tJ/ tl oxa nn e E. Purucker, M anager ~ Office of Science - Chicago Office Technical Qualification Program Description Revision 2, November 2010 CONCURRENCE The Office of Science-Chicago Office (SC-CH) is the sponsor for this Technical Qualification Program (TQP) Description. This is applicable to SC-CH, New Brunswick Laboratory (NBLL Ames Site Office (AMSO) and Argonne Site Office (ASO). These offices are in joint participation and endorsement of the SC-CH Technical Qualification Program process and have also provided concurrence below. The SC-CH Manager is the approval authority for this program description.

93

Focus Series - Chicago-Energy Impact Illinois (EI2)  

NLE Websites -- All DOE Office Websites (Extended Search)

Focus Series CHICAGO-ENERGY IMPACT ILLINOIS (EI2) Energy Impact Illinois Learns That Parties Sell Upgrades When Better Buildings Neighborhood Program partner Energy Impact Illinois (EI2) didn't achieve the response expected from a mass media advertising campaign, program administrators saw an opportunity to try a different strategy-one that relied more on a community-based, boots-on-the-ground outreach campaign. Through a "house party" initiative, EI2 brought Chicago homeowners, neighbors, and friends together to learn about energy efficiency opportunities, while increasing demand for home energy assessments and upgrades. Following is an abridged transcript of an interview with Dan Olson, senior energy efficiency planner, and Emily Plagman, senior energy planner for the Chicago Metropolitan

94

Obama Administration Hosts Great Lakes Offshore Wind Workshop in Chicago  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Hosts Great Lakes Offshore Wind Workshop in Hosts Great Lakes Offshore Wind Workshop in Chicago with Great Lakes Wind Collaborative Obama Administration Hosts Great Lakes Offshore Wind Workshop in Chicago with Great Lakes Wind Collaborative October 28, 2010 - 12:00am Addthis WASHINGTON - The White House Council on Environmental Quality and the U.S. Department of Energy hosted a workshop with the Great Lakes Wind Collaborative in Chicago on October 26 - 27, 2010, focused on the siting of offshore wind power in the Great Lakes. The two day workshop brought together wind developers, Federal and state regulators, environmental advocates, and other regional stakeholders to discuss methods for ensuring greater clarity, certainty and coordination of Federal and state decision-making for offshore wind development in the Great Lakes.

95

City of Chicago - Small Business Improvement Fund | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

City of Chicago - Small Business Improvement Fund City of Chicago - Small Business Improvement Fund City of Chicago - Small Business Improvement Fund < Back Eligibility Commercial Industrial Savings Category Heating & Cooling Commercial Heating & Cooling Heating Cooling Construction Commercial Weatherization Manufacturing Heat Pumps Appliances & Electronics Commercial Lighting Lighting Home Weatherization Insulation Design & Remodeling Windows, Doors, & Skylights Solar Buying & Making Electricity Water Heating Maximum Rebate Industrial property: $150,000 Single owner/tenant commercial property or landlord: $100,000 Multi-tenant building: $250,000 per property, $50,000 per tenant/landlord Program Info State Illinois Program Type Local Grant Program Rebate Amount 25%, 50%, or 75% of the costs, depending on size of the applicant

96

Argonne-University of Chicago Shuttle | Argonne National Laboratory  

NLE Websites -- All DOE Office Websites (Extended Search)

Visiting Argonne Visiting Argonne Site Access Policy Map Argonne-University of Chicago Shuttle Map of Argonne Download a map of the Argonne site. Access to the site Site Access Policy All visitors to Argonne require appropriate authorization before they are allowed on the Argonne site. Argonne-University of Chicago Shuttle The schedule below is effective August 25, 2010. A free shuttle bus makes round trips between Argonne National Laboratory and The University of Chicago. Shuttle service will be provided on Mondays, Wednesdays and Fridays only from September through April. From May through August, the shuttle will operate every weekday to accommodate the increase in student riders. The shuttle does not run on laboratory holidays. For more information, please contact Tracy Lozano (tlozano@anl.gov or 630/252-9625) at Argonne.

97

MOVIE "CHICAGO CITY COUNCIL: READY FOR REFORM?" (27 minutes/color)  

E-Print Network (OSTI)

, transportation, and health care. 8. Investigate how many of the reform proposals were in place twenty years afterMOVIE ­ "CHICAGO CITY COUNCIL: READY FOR REFORM?" (27 minutes/color) SYNOPSIS Following the death of Mayor Harold Washington, residents and reformers of Chicago still hoped for continued reform in Chicago

Illinois at Chicago, University of

98

Chicago Office NEPA Tracking Number U. S. DEPARTMENT OF ENERGY  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

SFCH F 560-ACQ SFCH F 560-ACQ (11/05) Previous editions are obsolete. ~1,6~.. --1 b Chicago Office NEPA Tracking Number U. S. DEPARTMENT OF ENERGY OFFICE OF SCIENCE -- CHICAGO OFFICE NATIONAL ENVIRONMENTAL POLICY ACT (NEPA) ENVIRONMENTAL EVALUATION NOTIFICATION FORM To be completed by "financial assistance award" organization receiving Federal funding. For assistance (including a point of contact), see "Instructions for Preparing SC-CH F-560, Environmental Evaluation Notification Form ". Solicitation/Award No. (if applicable): N/A Organization Name: New Brunswick Laboratory (NBL) Title of Proposed Project/Research: GENERIC CATEGORICAL EXCLUSION (CX) FOR THE NBL: Renovations and maintenance activities for buildings, structures, infrastructures and equipment

99

DOE - Office of Legacy Management -- Bendix Aviation Corp Pioneer Div - IA  

Office of Legacy Management (LM)

Bendix Aviation Corp Pioneer Div - Bendix Aviation Corp Pioneer Div - IA 05 FUSRAP Considered Sites Site: BENDIX AVIATION CORP., PIONEER DIV. (IA.05 ) Eliminated from consideration under FUSRAP Designated Name: Not Designated Alternate Name: Pioneer Division, Bendix Aviation Corporation Bendix Aviation Corporation Bendix Pioneer Division IA.05-1 IA.05-2 IA.05-3 Location: Davenport , Iowa IA.05-1 Evaluation Year: 1990 IA.05-2 IA.05-4 Site Operations: Conducted studies to investigate the feasibility of using sonic cleaning equipment to decontaminate uranium contaminated drums. IA.05-1 Site Disposition: Eliminated - Potential for contamination considered remote based on limited operations at the site IA.05-2 IA.05-4 IA.05-5 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium IA.05-1

100

DOE - Office of Legacy Management -- Titus Metals - IA 04  

Office of Legacy Management (LM)

from consideration under FUSRAP Also see Documents Related to TITUS METALS IA.04-1 - Argonne National Laboratory Memorandum; Lonergan to Novak; Subject: Extrusion of Billets,...

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

City of Chicago - Green Permit and Green Homes Programs | Department of  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

City of Chicago - Green Permit and Green Homes Programs City of Chicago - Green Permit and Green Homes Programs City of Chicago - Green Permit and Green Homes Programs < Back Eligibility Commercial Industrial Institutional Residential Schools Savings Category Heating & Cooling Home Weatherization Construction Commercial Weatherization Commercial Heating & Cooling Design & Remodeling Bioenergy Solar Lighting Windows, Doors, & Skylights Heating Buying & Making Electricity Water Water Heating Wind Program Info State Illinois Program Type Green Building Incentive Provider City of Chicago The City of Chicago encourages building design, construction and renovation in a manner that provides healthier environments, reduces operating costs and conserves energy and resources through their Green Permit Program. The

102

Conformal cosmological model and SNe Ia data  

SciTech Connect

Now there is a huge scientific activity in astrophysical studies and cosmological ones in particular. Cosmology transforms from a pure theoretical branch of science into an observational one. All the cosmological models have to pass observational tests. The supernovae type Ia (SNe Ia) test is among the most important ones. If one applies the test to determine parameters of the standard Friedmann-Robertson-Walker cosmological model one can conclude that observations lead to the discovery of the dominance of the {Lambda} term and as a result to an acceleration of the Universe. However, there are big mysteries connected with an origin and an essence of dark matter (DM) and the {Lambda} term or dark energy (DE). Alternative theories of gravitation are treated as a possible solution of DM and DE puzzles. The conformal cosmological approach is one of possible alternatives to the standard {Lambda}CDM model. As it was noted several years ago, in the framework of the conformal cosmological approach an introduction of a rigid matter can explain observational data without {Lambda} term (or dark energy). We confirm the claim with much larger set of observational data.

Zakharov, A. F., E-mail: zakharov@itep.ru [National Astronomical Observatories of Chinese Academy of Sciences (China); Pervushin, V. N. [Joint Institute for Nuclear Research, Bogoliubov Laboratory for Theoretical Physics (Russian Federation)

2012-11-15T23:59:59.000Z

103

Type Ia Supernova Explosion: Gravitationally Confined Detonation  

Science Journals Connector (OSTI)

We present a new mechanism for Type Ia supernova explosions in massive white dwarfs. The scenario follows from relaxing assumptions of symmetry and involves a detonation born near the stellar surface. The explosion begins with an essentially central ignition of a deflagration that results in the formation of a buoyancy-driven bubble of hot material that reaches the stellar surface at supersonic speeds. The bubble breakout laterally accelerates fuel-rich outer stellar layers. This material, confined by gravity to the white dwarf, races along the stellar surface and is focused at the location opposite to the point of the bubble breakout. These streams of nuclear fuel carry enough mass and energy to trigger a detonation just above the stellar surface that will incinerate the white dwarf and result in an energetic explosion. The stellar expansion following the deflagration redistributes mass in a way that ensures production of intermediate-mass and iron group elements with ejecta having a strongly layered structure and a mild amount of asymmetry following from the early deflagration phase. This asymmetry, combined with the amount of stellar expansion determined by details of the evolution (principally the energetics of deflagration, timing of detonation, and structure of the progenitor), can be expected to create a family of mildly diverse Type Ia supernova explosions.

T. Plewa; A. C. Calder; D. Q. Lamb

2004-01-01T23:59:59.000Z

104

The distant type Ia supernova rate  

SciTech Connect

We present a measurement of the rate of distant Type Ia supernovae derived using 4 large subsets of data from the Supernova Cosmology Project. Within this fiducial sample,which surveyed about 12 square degrees, thirty-eight supernovae were detected at redshifts 0.25--0.85. In a spatially flat cosmological model consistent with the results obtained by the Supernova Cosmology Project, we derive a rest-frame Type Ia supernova rate at a mean red shift z {approx_equal} 0.55 of 1.53 {sub -0.25}{sub -0.31}{sup 0.28}{sup 0.32} x 10{sup -4} h{sup 3} Mpc{sup -3} yr{sup -1} or 0.58{sub -0.09}{sub -0.09}{sup +0.10}{sup +0.10} h{sup 2} SNu(1 SNu = 1 supernova per century per 10{sup 10} L{sub B}sun), where the first uncertainty is statistical and the second includes systematic effects. The dependence of the rate on the assumed cosmological parameters is studied and the redshift dependence of the rate per unit comoving volume is contrasted with local estimates in the context of possible cosmic star formation histories and progenitor models.

Pain, R.; Fabbro, S.; Sullivan, M.; Ellis, R.S.; Aldering, G.; Astier, P.; Deustua, S.E.; Fruchter, A.S.; Goldhaber, G.; Goobar, A.; Groom, D.E.; Hardin, D.; Hook, I.M.; Howell, D.A.; Irwin, M.J.; Kim, A.G.; Kim, M.Y.; Knop, R.A.; Lee, J.C.; Perlmutter, S.; Ruiz-Lapuente, P.; Schahmaneche, K.; Schaefer, B.; Walton, N.A.

2002-05-20T23:59:59.000Z

105

The Distant Type Ia Supernova Rate  

DOE R&D Accomplishments (OSTI)

We present a measurement of the rate of distant Type Ia supernovae derived using 4 large subsets of data from the Supernova Cosmology Project. Within this fiducial sample, which surveyed about 12 square degrees, thirty-eight supernovae were detected at redshifts 0.25--0.85. In a spatially flat cosmological model consistent with the results obtained by the Supernova Cosmology Project, we derive a rest-frame Type Ia supernova rate at a mean red shift z {approx_equal} 0.55 of 1.53 {sub -0.25}{sub -0.31}{sup 0.28}{sup 0.32} x 10{sup -4} h{sup 3} Mpc{sup -3} yr{sup -1} or 0.58{sub -0.09}{sub -0.09}{sup +0.10}{sup +0.10} h{sup 2} SNu(1 SNu = 1 supernova per century per 10{sup 10} L{sub B}sun), where the first uncertainty is statistical and the second includes systematic effects. The dependence of the rate on the assumed cosmological parameters is studied and the redshift dependence of the rate per unit comoving volume is contrasted with local estimates in the context of possible cosmic star formation histories and progenitor models.

Pain, R.; Fabbro, S.; Sullivan, M.; Ellis, R. S.; Aldering, G.; Astier, P.; Deustua, S. E.; Fruchter, A. S.; Goldhaber, G.; Goobar, A.; Groom, D. E.; Hardin, D.; Hook, I. M.; Howell, D. A.; Irwin, M. J.; Kim, A. G.; Kim, M. Y.; Knop, R. A.; Lee, J. C.; Perlmutter, S.; Ruiz-Lapuente, P.; Schahmaneche, K.; Schaefer, B.; Walton, N. A.

2002-05-28T23:59:59.000Z

106

REGIONAL ECONOMICS APPLICATIONS LABORATORY CHICAGO BUSINESS ACTIVITY INDEX  

E-Print Network (OSTI)

Statistics reported total nonfarm payroll employment increased marginally by 54,000 in May. Job gains activity and the decrease of non-manufacturing employment. In May, the national and regional economy) increased 0.48 percent in May. In the Chicago region in May, manufacturing employment increased 0.34 percent

Shim, Moonsub

107

THE UNIVERSITY of CHICAGO THE IRVING B. HARRIS GRADUATE SCHOOL  

E-Print Network (OSTI)

THE UNIVERSITY of CHICAGO THE IRVING B. HARRIS GRADUATE SCHOOL of PUBLIC POLICY STUDIES ANNOUNCEMENTS Fall 2001 #12;More information regarding The Irving B. Harris Graduate School of Public Policy or doctoral program can be found on the World Wide Web, URL www.HarrisSchool.uchicago.edu/. Or you may contact

He, Chuan

108

iiSHAREDAMBITION The Universityof Illinois at Chicago  

E-Print Network (OSTI)

iiSHAREDAMBITION The Universityof Illinois at Chicago and NorthLawndalearehonoredto presentTheBarackObama Foundation withourproposal tohost the Barack Obama Presidential Library #12;3 2 The University of Illinois. This is not its destination but rather the origination of something greater: energy emanating outward in shallow

Illinois at Chicago, University of

109

Affordable Housing Fact Book Chicago Rehab Network 4. Converting  

E-Print Network (OSTI)

Vacant Owner Renter White Hispanic Other African American Affordable Housing Fact Book Chicago/Ethnicity: Largely White, racial mix Household Income: $39,599, increased 10.4% Cluster Characteristics Converting a substantial number of households in Converting commu- nities continue to be rent burdened as rents increased

Illinois at Chicago, University of

110

Affordable Housing Fact Book Chicago Rehab Network 1. Homeowning  

E-Print Network (OSTI)

White Black Hispanic Other Vacant Owner Renter Affordable Housing Fact Book Chicago Rehab Network 1 multifamily Racial/Ethnicity : Racially segregated in individual communities Household Income: $48, households in Homeowning communities tend to have long-term tenures, lower vacancy rates, and higher incomes

Illinois at Chicago, University of

111

Affordable Housing Fact Book Chicago Rehab Network 2. Thinning  

E-Print Network (OSTI)

Vacant Ow ner Renter Hispanic Other White African American Affordable Housing Fact Book Chicago multifamily and single-family Racial/Ethnicity : Primarily African American Household Income: $28 Household Size 3.2 % of Residents in Poverty 29.6% % Change in Poverty -12.7% % Children with Lead Poisoning

Illinois at Chicago, University of

112

Intermediate-band Photometry of Type Ia Supernovae  

E-Print Network (OSTI)

We present optical light curves of five Type Ia supernovae (2002er, 2002fk, 2003cg, 2003du, 2003fk). The photometric observations were performed in a set of intermediate-band filters. SNe 2002er, 2003du appear to be normal SN Ia events with similar light curve shapes, while SN 2003kf shows the behavior of a brighter SN Ia with slower decline rate after maximum. The light curves of SN 2003cg is unusual; they show a fast rise and dramatic decline near maximum and do not display secondary peak at longer wavelengths during 15-30 days after maximum light. This suggests that SN 2003cg is likely to be an intrinsically subluminous, 91bg-like SN Ia. Exploration of SN Ia feature lines through intermediate-band photometry is briefly discussed.

Wang, X; Zhang, T; Li, Z; Wang, Xiaofeng; Zhou, Xu; Zhang, Tianmeng; Li, Zongwei

2004-01-01T23:59:59.000Z

113

Visualizing Type Ia Supernova Explosions at NERSC  

NLE Websites -- All DOE Office Websites (Extended Search)

Supernova Explosions Supernova Explosions Visualizing Type Ia Supernova Explosions Childs1a-Supernovasm.png Deep inside a dying star in a galaxy far, far away, a carbon fusion flame ignites. Ignition may happen in the middle or displaced slightly to one side, but this simulation explores the consequences of central ignition. In a localized hot spot, represented here by a deformed sphere with an average radius of 100 km, carbon is assumed to have already fused to iron, producing hot ash (~10 billion K) with a density about 20% less than its surroundings. As the burning progresses, this hot buoyant ash rises up and interacts with cold fuel. Rayleigh-Taylor fingers give rise to shear and turbulence, which interacts with the flame, causing it to move faster. In about 2 seconds, the energy released blows the entire white dwarf star up,

114

DOE - Office of Legacy Management -- Iowa Army Ammunition Plant - IA 02  

Office of Legacy Management (LM)

Army Ammunition Plant - IA 02 Army Ammunition Plant - IA 02 FUSRAP Considered Sites Iowa Army Ammunition Plant, IA Alternate Name(s): Burlington Ordnance Plant Iowa Ordnance Plant Silas Mason Company IA.02-3 Location: Located in Township 70 North, Range 3 West, Section 32, 5th Principal Meridian, Des Moines County, Burlington, Iowa IA.02-1 IA.02-5 Historical Operations: Assembled nuclear weapons, primarily high explosive components and conducted explosives testing using the high explosive components and depleted uranium. AEC and ERDA operations conducted under permit from the Department of the Army. IA.02-3 IA.02-4 Eligibility Determination: Eligible IA.02-5 Radiological Survey(s): Assessment Survey IA.02-2 Site Status: Cleanup pending by U.S. Army Corps of Engineers. IA.02-6

115

University of Illinois Chicago UIC | Open Energy Information  

Open Energy Info (EERE)

UIC UIC Jump to: navigation, search Name University of Illinois - Chicago (UIC) Place Chicago, Illinois Zip 60607-7113 Product Public research university with a research budget of more than USD 250m. Coordinates 41.88415°, -87.632409° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.88415,"lon":-87.632409,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

116

Chicago Pile reactors create enduring research legacy - Argonne's  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago Pile reactors create enduring research Chicago Pile reactors create enduring research legacy About Director's Welcome Organization Achievements Highlights Fact Sheets, Brochures & Other Documents Multimedia Library Visit Argonne Work with Argonne Contact us Nuclear Energy Why Nuclear Energy? Why are some people afraid of Nuclear Energy? How do nuclear reactors work? Cheaper & Safer Nuclear Energy Helping to Solve the Nuclear Waste Problem Nuclear Reactors Nuclear Reactors Early Exploration Training Reactors Basic and Applied Science Research LWR Technology Development BORAX-III lighting Arco, Idaho (Press Release) Heavy Water and Graphite Reactors Fast Reactor Technology Integral Fast Reactor Argonne Reactor Tree CP-1 70th Anniversary CP-1 70th Anniversary Argonne's Nuclear Science and Technology Legacy

117

Microsoft Word - Chicago Transcript 10 07 08 FINAL.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

7/2008 7/2008 Chicago, Illinois Page 1 U.S. Department of Energy Pre-Congestion Study Regional Workshops for the 2009 National Electric Congestion Study Chicago, IL September 17, 2008 8:30 a.m.-12:00 p.m. Transcript David Meyer: Well, good morning, ladies and gentlemen. I'm David Meyer from the Department of Energy. And I welcome you to our workshop on our 2009 congestion study. Before I get started in a brief presentation, I want to introduce some of my colleagues here. Lot Cooke, who's not at this table presently, but he'll be here shortly. He's from our general counsel's office. Peggy Welsh is from Energetics and has helped us organize the workshops. We have Elliott Nethercutt, also from my office. He's helping us with some of the arrangements here. We have Joe Eto from Lawrence Berkeley Laboratory. And

118

STATEMENT OF CONSIDERATIONS REQUEST BY THE UNIVERSITY OF CHICAGO  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

UNIVERSITY OF CHICAGO UNIVERSITY OF CHICAGO AS OPERATOR OF ARGONNE NATIONAL LABORATORY UNDER U.S. DEPARTMENT OF ENERGY CONTRACT NO. W-31-109-ENG-38 FOR A BLANKET ADVANCE WAIVER OF DOMESTIC AND FOREIGN RIGHTS OF THE ENGELHARDT INSTITUTE OF MOLECULAR BIOLOGY, MOSCOW, RUSSIA UNDER SUBCONTRACT NO. ANL-943352403 W(A)-95-012, CH-0860 The proposed Argonne National Laboratory (ANL) subcontract to Engelhardt Institute (Engelhardt) is directed to developing methods to assist in the determination of genome structure. Specifically, it will be directed toward a collaboration between ANL, which has developed an approach for economical, rapid, high volume DNA sequencing, referred to as Sequencing by Hybridization, and Engelhardt, which has developed a technique called Sequencing by Hybridization on Microchip (SHOM). The proposed project is multiyear and is

119

Chicago Office NEPA Tracking Number U. S. DEPARTMENT OF ENERGY  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

SGCH F 560-ACQ SGCH F 560-ACQ (11/05) Previous editions are obsolete. Chicago Office NEPA Tracking Number U. S. DEPARTMENT OF ENERGY OFFICE OF SCIENCE -- CHICAGO OFFICE NATIONAL ENVIRONMENTAL POLICY ACT (NEPA) ENVIRONMENTAL EVALUATION NOTIFICATION FORM To be completed by "financial assistance award" organization receiving Federal funding. For assistance (including a point of contact), see "Instructions for Preparing SC-CH F-560, Environmental Evaluation Notification Form ". Solicitation/Award No. (if applicable): N/A Organization Name: New Brunswick Laboratory (NBL) Title of Proposed Project/Research: GENERIC CATEGORICAL EXCLUSION (CX) FOR THE NBL: Indoor Bench Scale Research Projects and Conventional Laboratory Operations Total DOE Funding/Total Project Funding:

120

THE UNIVERSITY OF CHICAGO Operator of Argonne National Laboratory  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

UNIVERSITY OF CHICAGO UNIVERSITY OF CHICAGO Operator of Argonne National Laboratory Comments on the Department of Energy Notice of Inquiry Concerning Preparation of Report to Congress on the Price-Anderson Act January 30, 1998 Following are responses to the questions in the Notice of Inquiry published in the Federal Register on December 31, 1997: 1. Should the DOE Price-Anderson indemnification be continued without modification? The extension of Price-Anderson indemnification is critically important to the continuation of the DOE program respecting nuclear materials and facilities. We recommend several changes in the Act in answer to succeeding questions, but a continuation of the indemnity as is would be preferable to any changes that might endanger the Act's basic scheme of protection of the

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


121

Chicago Green Office Challenge | ENERGY STAR Buildings & Plants  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago Green Office Challenge Chicago Green Office Challenge Secondary menu About us Press room Contact Us Portfolio Manager Login Facility owners and managers Existing buildings Commercial new construction Industrial energy management Small business Service providers Service and product providers Verify applications for ENERGY STAR certification Design commercial buildings Energy efficiency program administrators Commercial and industrial program sponsors Associations State and local governments Federal agencies Tools and resources Training In this section How can we help you? Build an energy program Improve building and plant performance Earn the ENERGY STAR and other recognition Benchmark energy use ENERGY STAR in action Communicate and educate ENERGY STAR communications toolkit Bring Your Green to Work with ENERGY STAR

122

Chicago Pile 1 (CP-1) 70th Anniversary  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago Pile 1 (CP-1) 70th Anniversary Chicago Pile 1 (CP-1) 70th Anniversary About Director's Welcome Organization Achievements Highlights Fact Sheets, Brochures & Other Documents Multimedia Library Visit Argonne Work with Argonne Contact us Nuclear Energy Why Nuclear Energy? Why are some people afraid of Nuclear Energy? How do nuclear reactors work? Cheaper & Safer Nuclear Energy Helping to Solve the Nuclear Waste Problem Nuclear Reactors Nuclear Reactors Early Exploration Training Reactors Basic and Applied Science Research LWR Technology Development BORAX-III lighting Arco, Idaho (Press Release) Heavy Water and Graphite Reactors Fast Reactor Technology Integral Fast Reactor Argonne Reactor Tree CP-1 70th Anniversary CP-1 70th Anniversary Argonne's Nuclear Science and Technology Legacy Argonne's Nuclear Science and Technology Legacy

123

Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction  

NLE Websites -- All DOE Office Websites (Extended Search)

Information Information Resources Printable Version Share this resource Send a link to Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction Workshop Materials to someone by E-mail Share Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction Workshop Materials on Facebook Tweet about Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction Workshop Materials on Twitter Bookmark Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction Workshop Materials on Google Bookmark Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction Workshop Materials on Delicious Rank Solid-State Lighting: 2009 Solid-State Lighting Chicago Market Introduction Workshop Materials on Digg Find More places to share Solid-State Lighting: 2009 Solid-State

124

The Chicago Tribune sees the "wonder" in APS  

NLE Websites -- All DOE Office Websites (Extended Search)

The Chicago Tribune sees the "wonder" in APS The Chicago Tribune sees the "wonder" in APS Clipping of Chicago Tribune Ever wonder what the editors of the Chicago Tribune think of the Advanced Photon Source (APS)? Wonder no more. True, the APS didn't make the cut as one of the "official" "7 Wonders of Chicago" in a reader-survey contest recently staged by the newspaper. (All seven finalists happen to be located within Chicago city limits.) But the APS and its technologies were deemed worthy of singling out as a wonder nonetheless in the closing two paragraphs of the September 15, 2005, story on the contest in the paper's Tempo section. "You told us about things we had never thought of," wrote Tribune senior correspondent Charles Leroux. "For instance, the Advanced Photon Source at

125

DOE-funded Silicon-Graphene Research Leads to Chicago-based Technology...  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE-funded Silicon-Graphene Research Leads to Chicago-based Technology Startup Graduate students at Northwestern University are commercializing a silicon (Si)-graphene technology...

126

UMore Ph IA CR Report 7-8-10.pdf  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

PHASE IA ARCHAEOLOGICAL AND PHASE IA ARCHAEOLOGICAL AND ARCHITECTURAL HISTORY SURVEY FOR THE UMORE PARK RESEARCH WIND TURBINE PROJECT, DAKOTA COUNTY, MINNESOTA SHPO File No. Pending Client No. Pending The 106 Group Project No. 10-18 Submitted to: Barr Engineering Company 4700 West 77th Street Minneapolis, MN 55435-4803 Submitted by: The 106 Group Ltd. The Dacotah Building 370 Selby Avenue St. Paul, MN 55102 Principal Investigators: AnneKetz, M.A., RPA Greg Mathis, M.C.R.P. Report Authors: Mark Doperalski, B.S. Miranda Van Vleet, M.H.P July 2010 UMore Park Wind Turbine Project Phase IA Archaeological and Architectural History Survey Page i MANAGEMENT SUMMARY During May of 2010, The 106 Group Ltd. (106 Group) conducted a Phase IA archaeological and architectural history survey for the University of Minnesota Outreach, Research, and

127

CIRCUMSTELLAR ABSORPTION IN DOUBLE DETONATION TYPE Ia SUPERNOVAE  

SciTech Connect

Upon formation, degenerate He core white dwarfs are surrounded by a radiative H-rich layer primarily supported by ideal gas pressure. In this Letter, we examine the effect of this H-rich layer on mass transfer in He+C/O double white dwarf binaries that will eventually merge and possibly yield a Type Ia supernova (SN Ia) in the double detonation scenario. Because its thermal profile and equation of state differ from the underlying He core, the H-rich layer is transferred stably onto the C/O white dwarf prior to the He core's tidal disruption. We find that this material is ejected from the binary system and sweeps up the surrounding interstellar medium hundreds to thousands of years before the SN Ia. The close match between the resulting circumstellar medium profiles and values inferred from recent observations of circumstellar absorption in SNe Ia gives further credence to the resurgent double detonation scenario.

Shen, Ken J. [Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Guillochon, James [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Foley, Ryan J., E-mail: kenshen@astro.berkeley.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2013-06-20T23:59:59.000Z

128

Abstract IA14: Functional genomics and cancer vulnerabilities  

Science Journals Connector (OSTI)

...Cancer Research. November 2014 meeting-abstract Genomics Genomics: Oral Presentations - Invited Abstracts Abstracts...2013; San Diego, CA Abstract IA14: Functional genomics and cancer vulnerabilities William C. Hahn Dana-Farber...

William C. Hahn

2014-11-01T23:59:59.000Z

129

EARLY EMISSION FROM TYPE Ia SUPERNOVAE  

SciTech Connect

A unique feature of deflagration-to-detonation (DDT) white dwarf explosion models of supernovae of type Ia is the presence of a strong shock wave propagating through the outer envelope. We consider the early emission expected in such models, which is produced by the expanding shock-heated outer part of the ejecta and precedes the emission driven by radioactive decay. We expand on earlier analyses by considering the modification of the pre-detonation density profile by the weak shocks generated during the deflagration phase, the time evolution of the opacity, and the deviation of the post-shock equation of state from that obtained for radiation pressure domination. A simple analytic model is presented and shown to provide an acceptable approximation to the results of one-dimensional numerical DDT simulations. Our analysis predicts a {approx}10{sup 3} s long UV/optical flash with a luminosity of {approx}1 to {approx}3 Multiplication-Sign 10{sup 39} erg s{sup -1}. Lower luminosity corresponds to faster (turbulent) deflagration velocity. The luminosity of the UV flash is predicted to be strongly suppressed at t > t{sub drop} {approx} 1 hr due to the deviation from pure radiation domination.

Rabinak, Itay; Waxman, Eli [Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 76100 (Israel); Livne, Eli, E-mail: itay.rabinak@weizmann.ac.il [Racah Institute of Physics, Hebrew University, Jerusalem (Israel)

2012-09-20T23:59:59.000Z

130

The 1.05-?m feature in the spectrum of the Type Ia supernova 1994D: He in SNe Ia?  

Science Journals Connector (OSTI)

......SNe Ia). Although the agreed basic scenario is thermonuclear fusion within a white dwarf (WD), the process leading...a pressure wave into the WD which then triggers thermonuclear fusion in the core. In this scenario, explosion can......

P. A. Mazzali; L. B. Lucy

1998-04-01T23:59:59.000Z

131

lColon Cancer Patterns of Care in Chicagoof Care in Chicago  

E-Print Network (OSTI)

lColon Cancer Patterns of Care in Chicagoof Care in Chicago Progress, preliminary results Disparities in Stage-Specific Colorectal Cancer Mortality: 1960-2005. Am J Public Health. 2010 October 1, 2010;100(10):1912-6. 2 #12;Colon Cancer Patterns of Care in Chicago · XXXXX · Goals 1. Examine how prior screening

Illinois at Chicago, University of

132

General Merchandise 2009 TSD Chicago Low Plug Load Baseline | Open Energy  

Open Energy Info (EERE)

General Merchandise 2009 TSD Chicago Low Plug Load Baseline General Merchandise 2009 TSD Chicago Low Plug Load Baseline Jump to: navigation, search Model Name General Merchandise 2009 TSD Chicago Low Plug Load Baseline Building Type Mercantile (Retail Other Than Mall) Model Type Baseline Model Target Type ASHRAE 90.1 2004 Model Year 2009 IDF file http://apps1.eere.energy.gov/buildings/energyplus/models/Miami/2009_TSD_GeneralMerch_LPL_Baseline.idf XML file http://apps1.eere.energy.gov/buildings/energyplus/models/Miami/2009_TSD_GeneralMerch_LPL_Baseline.xml City, State Chicago, IL Climate Zone Climate Zone 5A Retrieved from "http://en.openei.org/w/index.php?title=General_Merchandise_2009_TSD_Chicago_Low_Plug_Load_Baseline&oldid=270182" Category: Building Models What links here Related changes Special pages

133

DOE - Office of Legacy Management -- Chicago South IL Site - IL 06  

NLE Websites -- All DOE Office Websites (Extended Search)

South IL Site - IL 06 South IL Site - IL 06 FUSRAP Considered Sites Chicago South, IL Alternate Name(s): University of Chicago Charles Herbert Jones Chemical Laboratory Ryerson Physical Laboratory Eckhart Hall Kent Chemical Laboratory Ricketts Laboratory IL.06-3 Location: University of Chicago, Ellis Avenue and East 58th Street, Chicago, Illinois IL.06-3 Historical Operations: Performed activities associated with (1) production and purification of plutonium, which involved the handling and processing of uranium compounds; (2) demonstrating the self-sustaining nature of the fission process and the production of Pu-239 from U-238 (nuclear fission and Chicago Pile-1); and (3) health effects (metal toxicology and radiation effects). IL.06-5 IL.06-6 IL.06-7 Eligibility Determination: Eligible IL.06-1

134

DOE - Office of Legacy Management -- Chicago South IL Site - IL 06  

Office of Legacy Management (LM)

South IL Site - IL 06 South IL Site - IL 06 FUSRAP Considered Sites Chicago South, IL Alternate Name(s): University of Chicago Charles Herbert Jones Chemical Laboratory Ryerson Physical Laboratory Eckhart Hall Kent Chemical Laboratory Ricketts Laboratory IL.06-3 Location: University of Chicago, Ellis Avenue and East 58th Street, Chicago, Illinois IL.06-3 Historical Operations: Performed activities associated with (1) production and purification of plutonium, which involved the handling and processing of uranium compounds; (2) demonstrating the self-sustaining nature of the fission process and the production of Pu-239 from U-238 (nuclear fission and Chicago Pile-1); and (3) health effects (metal toxicology and radiation effects). IL.06-5 IL.06-6 IL.06-7 Eligibility Determination: Eligible IL.06-1

135

Shanghai and Chicago Take Their Clean Energy Relationship to the Next Level  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Shanghai and Chicago Take Their Clean Energy Relationship to the Shanghai and Chicago Take Their Clean Energy Relationship to the Next Level Shanghai and Chicago Take Their Clean Energy Relationship to the Next Level November 8, 2010 - 4:29pm Addthis Chicago Mayor Richard M. Daley with his Shanghai counterpart Han Zheng at signing of the Eco-City Partnership agreement in Shanghai on September 20, 2010, attended by Mark Ginsberg of DOE-EERE | Photo Courtesy of www.chicagosistercities.com Chicago Mayor Richard M. Daley with his Shanghai counterpart Han Zheng at signing of the Eco-City Partnership agreement in Shanghai on September 20, 2010, attended by Mark Ginsberg of DOE-EERE | Photo Courtesy of www.chicagosistercities.com Andy Oare Andy Oare Former New Media Strategist, Office of Public Affairs With support from the U.S. Department of Energy's Office of Energy

136

Simulations of Turbulent Thermonuclear Burning in Type Ia Supernovae  

E-Print Network (OSTI)

Type Ia supernovae have recently received considerable attention because it appears that they can be used as "standard candles" to measure cosmic distances out to billions of light years away from us. Observations of type Ia supernovae seem to indicate that we are living in a universe that started to accelerate its expansion when it was about half its present age. These conclusions rest primarily on phenomenological models which, however, lack proper theoretical understanding, mainly because the explosion process, initiated by thermonuclear fusion of carbon and oxygen into heavier elements, is difficult to simulate even on supercomputers. Here, we investigate a new way of modeling turbulent thermonuclear deflagration fronts in white dwarfs undergoing a type Ia supernova explosion. Our approach is based on a level set method which treats the front as a mathematical discontinuity and allows for full coupling between the front geometry and the flow field. New results of the method applied to the problem of type Ia supernovae are obtained. It is shown that in 2-D with high spatial resolution and a physically motivated subgrid scale model for the nuclear flames numerically "converged" results can be obtained, but for most initial conditions the stars do not explode. In contrast, simulations in 3-D, do give the desired explosions and many of their properties, such as the explosion energies, lightcurves and nucleosynthesis products, are in very good agreement with observed type Ia supernovae.

W. Hillebrandt; M. Reinecke; W. Schmidt; F. K. Roepke; C. Travaglio; J. C. Niemeyer

2004-05-11T23:59:59.000Z

137

Type Ia Supernovae Yielding Distances with 3-4% Precision  

E-Print Network (OSTI)

The luminosities of Type Ia supernovae (SN), the thermonuclear explosions of white dwarf stars, vary systematically with their intrinsic color and light-curve decline rate. These relationships have been used to calibrate their luminosities to within ~0.14-0.20 mag from broadband optical light curves, yielding individual distances accurate to ~7-10%. Here we identify a subset of SN Ia that erupt in environments having high ultraviolet surface brightness and star-formation surface density. When we apply a steep model extinction law, these SN can be calibrated to within ~0.065-0.075 mag, corresponding to ~3-4% in distance -- the best yet with SN Ia by a substantial margin. The small scatter suggests that variations in only one or two progenitor properties account for their light-curve-width/color/luminosity relation.

Kelly, Patrick L; Burke, David L; Hicken, Malcolm; Ganeshalingam, Mohan; Zheng, Weikang

2014-01-01T23:59:59.000Z

138

Signatures of A Companion Star in Type Ia Supernovae  

E-Print Network (OSTI)

While type Ia Supernovae (SNe Ia) have been used as precise cosmological distance indicators, their progenitor systems remain unresolved. One of the key questions is if there is a non-degenerate companion star at the time of a thermonuclear explosion of a white dwarf (WD). In this paper, we investigate if an interaction between the SN ejecta and the companion star may result in observable footprints around the maximum brightness and thereafter, by performing multi-dimensional radiation transfer simulations based on hydrodynamic simulations of the interaction. We find that such systems result in variations in various observational characteristics due to different viewing directions, while the predicted behaviors (redder and fainter for the companion direction) are opposite to what were suggested by the previous study. The variations are generally modest and within observed scatters. However, the model predicts trends between some observables different from observationally derived, thus a large sample of SNe Ia...

Maeda, Keiichi; Shigeyama, Toshikazu

2014-01-01T23:59:59.000Z

139

Double degenerates and progenitors of supernovae type Ia  

E-Print Network (OSTI)

We report on systematic radial velocity surveys for white dwarf - white dwarf binaries (double degenerates - DDs) including SPY (ESO Supernovae Ia progenitor survey) recently carried out at the VLT. A large sample of DD will allow us to put strong constrains on the phases of close binary evolution of the progenitor systems and to perform an observational test of the DD scenario for supernovae of type Ia. We explain how parameters of the binaries can be derived from various methods. Results for a sample of DDs are presented and discussed.

R. Napiwotzki; L. Yungelson; G. Nelemans; T. R. Marsh; B. Leibundgut; A. Renzini; D. Homaier; D. Koester; S. Moehler; N. Christlieb; D. Reimers; H. Drechsel; U. Heber; C. Karl; E. -M. Pauli

2004-03-25T23:59:59.000Z

140

Search for double degenerate progenitors of supernovae type Ia with SPY  

E-Print Network (OSTI)

We report on a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY).

R. Napiwotzki; H. Drechsel; U. Heber; C. Karl; E. -M. Pauli; N. Christlieb; H. -J. Hagen; D. Reimers; D. Koester; S. Moehler; D. Homeier; B. Leibundgut; A. Renzini; T. R. Marsh; G. Nelemans; L. Yungelson

2002-10-07T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

Spectral Observations and Analyses of Low-Redshift Type Ia Supernovae  

E-Print Network (OSTI)

1.3.2 Thermonuclear Supernovae . . . . . . . . 1.4 Why WriteIa are the result of thermonuclear explosions of C/O whiteIa are the result of thermonuclear explosions of C/O white

Silverman, Jeffrey Michael

2011-01-01T23:59:59.000Z

142

INDECOMPOSABLE RACKS OF ORDER p 2 MAT IAS GRA  

E-Print Network (OSTI)

INDECOMPOSABLE RACKS OF ORDER p 2 MAT ?? IAS GRA ? NA Abstract. We classify indecomposable racks order is trivial. 1. Introduction Racks and quandles have been considered by G. Wraith and J. Conway categories, one is immediately led to the notion of a rack. On the other hand, in [ESS, EGS, S] and [LYZ1

Graña, Matías

143

INCOMPLETE CARBON-OXYGEN DETONATION IN TYPE Ia SUPERNOVAE  

SciTech Connect

Incomplete carbon-oxygen detonation with reactions terminating after burning of C{sup 12} in the leading C{sup 12} + C{sup 12} reaction (C-detonation) may occur in the low-density outer layers of white dwarfs exploding as Type Ia supernovae (SNe Ia). Previous studies of carbon-oxygen detonation structure and stability at low densities were performed under the assumption that the velocity of a detonation wave is derived from complete burning of carbon and oxygen to iron. In fact, at densities {rho} {<=} 10{sup 6} g cm{sup -3} the detonation in SNe Ia may release less than a half of the available nuclear energy. In this paper, we study basic properties of such detonations. We find that the length of an unsupported steady-state C-detonation is {approx_equal}30-100 times greater than previously estimated and that the decreased energy has a drastic effect on the detonation stability. In contrast to complete detonations which are one-dimensionally stable, C-detonations may be one-dimensionally unstable and propagate by periodically re-igniting themselves via spontaneous burning. The re-ignition period at {rho} {<=} 10{sup 6} g cm{sup -3} is estimated to be greater than the timescale of an SN Ia explosion. This suggests that propagation and quenching of C-detonations at these densities could be affected by the instability. Potential observational implications of this effect are discussed.

Dominguez, Inma [Departamento de Fisica Teorica y del Cosmos, University of Granada, 18071 Granada (Spain); Khokhlov, Alexei [Department of Astronomy and Astrophysics and the Enrico Fermi Institute, University of Chicago, Chicago, IL 60637 (United States)

2011-04-01T23:59:59.000Z

144

The EqIA Publishing Template Impact Assessment Summary  

E-Print Network (OSTI)

The EqIA Publishing Template Impact Assessment Summary 1. Name of policy, function or service. Bedgebury 5 year strategy and development plan. This is a partial assessment. 2. Purpose and aims with ETWF: Sustainable Resource, Climate Change, Natural Environment, Quality of Life, Business and Markets

145

HOSPITALITY AND TOURISM MANAGEMENT MAJOR Virgu1iaTech  

E-Print Network (OSTI)

Hospitality Facilities Planning and Methods I (3) Management (3) #HTM 3484 Socio-Cultural Impacts of Tourism 4414 Food and Beverage Management (Pre: HTM 3414) * #HTM 4464 Human Resources Management in HospHOSPITALITY AND TOURISM MANAGEMENT MAJOR Virgu1iaTech Panplil College of BusIness Department

Virginia Tech

146

Circumstellar interaction of the type Ia supernova 2002ic  

Science Journals Connector (OSTI)

......with arguments in favour of a high-energy SN Ia event in this case, raises...WD explosion with a high kinetic energy of ejecta. The SN 1.5 origin of...2002ic-like events requires an accurate energy audit, for which the direct detection......

N. N. Chugai; R. A. Chevalier; P. Lundqvist

2004-12-01T23:59:59.000Z

147

Thermonuclear supernova models, and observations of Type Ia supernovae  

E-Print Network (OSTI)

In this paper, we review the present state of theoretical models of thermonuclear supernovae, and compare their predicitions with the constraints derived from observations of Type Ia supernovae. The diversity of explosion mechanisms usually found in one-dimensional simulations is a direct consequence of the impossibility to resolve the flame structure under the assumption of spherical symmetry. Spherically symmetric models have been successful in explaining many of the observational features of Type Ia supernovae, but they rely on two kinds of empirical models: one that describes the behaviour of the flame on the scales unresolved by the code, and another that takes account of the evolution of the flame shape. In contrast, three-dimensional simulations are able to compute the flame shape in a self-consistent way, but they still need a model for the propagation of the flame in the scales unresolved by the code. Furthermore, in three dimensions the number of degrees of freedom of the initial configuration of the white dwarf at runaway is much larger than in one dimension. Recent simulations have shown that the sensitivity of the explosion output to the initial conditions can be extremely large. New paradigms of thermonuclear supernovae have emerged from this situation, as the Pulsating Reverse Detonation. The resolution of all these issues must rely on the predictions of observational properties of the models, and their comparison with current Type Ia supernova data, including X-ray spectra of Type Ia supernova remnants.

E. Bravo; C. Badenes; D. Garcia-Senz

2004-12-07T23:59:59.000Z

148

UNITED STATES ATOMIC ENERGY COMMISSION CHICAGO OPERATIONS OFFICE  

Office of Legacy Management (LM)

$$ ,_, . $$ ,_, . UNITED STATES ATOMIC ENERGY COMMISSION CHICAGO OPERATIONS OFFICE TELEPHONE 9600 SOUTH CASS AVENUE (312) 739-7711 ARCONNE. ILLINOIS 60439 ^,/" _. i ' > ;.:a c. JAN 17 1975 Martin B. Biles, Director Division of Operational Safety, HQ _ DISPOSAL OF SCRAP COPPER, CYCLOTRON DISMANTLING PROJECT, NUCLEAR RESEARCH CENTER, CARNEGIE-MELLON UNIVERSITY (CMU) Enclosed for your information is a copy of the October 28, 1974, letter from T. Morris (CMD) to J. Krupa (CH) with pages 1-4 and 8-16 of its attachment (the October 23, 1974, F. Bomba to T. Morris, memo- randum; pages 5-7 are economically omitted as they were not relevant to the subject of this letter) regarding disposal of 4 to 6 tons of copper. The enclosure contains a summary of data obtained from

149

Introduction to the Intellectual Property Law Division (IPL) Chicago Office  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Patent Law Reform- Patent Law Reform- America Invents Act DOE Patent Attorney Conference September 13, 2011 Mark Dvorscak Deputy Chief Counsel Chicago Office 2 H.R. 1249 Significant Changes to U.S. Patent System Short Title: Leahy-Smith America Invents Act Passed by the House June 23, 2011 Senate Adopts House Version (Sept. 6) Approved September 8 Heads to President for Signature Effective Date - 1 Year After Enactment unless otherwise specified First Inventor to File * Transitions the U.S. to a first-inventor-to file patent system from a first-to-invent while maintaining a 1-year grace period for disclosures. - Each application receives an "effective filing date" - Patentability Judged on Availability of Prior Art Available Prior to that date. - Invention Must Still be New, Useful, and

150

UNITED STATES ENERGY RESEARCH AND DEVELOPMENT CHICAGO OPERATIONS OFFICE  

Office of Legacy Management (LM)

CHICAGO OPERATIONS OFFICE 9800 SOUTH CASS AVENUE ARGONNE, ILLINOIS 80439 TELEPHONE (312) 739-7711 ADMINISTRATION JUL 11977 Hal Hollister, Acting Director Division of Operational and Environmental Safety, HQ RESURVEY PROGRAM - BRUSH BERYLLIUM COMPANY A visit to the Brush Beryllium Company (presently called Brush Wellman), Cleveland, Ohio was made by Edward J. Jascewsky and members of the Argonne National Laboratory survey team on May 17, 1977. The group met with Martin Powers and Nate Bass, Vice Presidents of Brush Wellman. The purpose of the visit was to determine if any radiological survey was needed as a result of past Atomic Energy Commission (AEC) contract work. The work performed by Brush Beryllium involving radioactive materials was done at two locations in the Cleveland area. One site was located

151

Preliminary Notice of Violation,University of Chicago - EA-2006-02 |  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Chicago - EA-2006-02 Chicago - EA-2006-02 Preliminary Notice of Violation,University of Chicago - EA-2006-02 March 7, 2006 Preliminary Notice of Violation issued to the University of Chicago related to Nuclear Safety Program Deficiencies at Argonne National Laboratory This letter refers to the Department of Energy's (DOE) Office of Price-Anderson Enforcement's (OE) investigation of the nuclear safety program deficiencies that were identified in 2005 by several DOE organizations who performed routine assessments of Argonne National Laboratory's (ANL) Price-Anderson Amendments Act (PAAA) and environment, safety, and health programs. An investigation summary report was issued to you on December 21, 2005. An enforcement conference was held on January 25, 2006, in Germantown, Maryland, with you, members of your staff, and senior

152

Reference Buildings by Climate Zone and Representative City: 5A Chicago,  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Reference Buildings by Climate Zone and Representative City: 5A Reference Buildings by Climate Zone and Representative City: 5A Chicago, Illinois Reference Buildings by Climate Zone and Representative City: 5A Chicago, Illinois In addition to the ZIP file for each building type, you can directly view the "scorecard" spreadsheet that summarizes the inputs and results for each location. This Microsoft Excel spreadsheet is also included in the ZIP file. For version 1.4, only the IDF file is included. refbldg_5a_usa_il_chicago-ohare_post1980_v1.3_5.0.zip refbldg_5a_usa_il_chicago-ohare_post1980_v1-4_7-2.zip More Documents & Publications Reference Buildings by Climate Zone and Representative City: 5B Boulder, Colorado Reference Buildings by Climate Zone and Representative City: 6A Minneapolis, Minnesota Reference Buildings by Climate Zone and Representative City: 6B Helena,

153

Thinking American, Working American, Playing American Folk Dance in Chicago, 1890-1940  

E-Print Network (OSTI)

Examination of folk dance in the Chicago area from 1890 to 1940 reveals the centrality of the body to ideas about education in the early twentieth century. The dissertation illuminates the circulation of folk dance practices in higher education...

Herzogenrath, Jessica

2014-07-23T23:59:59.000Z

154

Building America Technology Solutions for New and Existing Homes: Advanced Boiler Load Monitoring Controllers, Chicago, Illinois  

Energy.gov (U.S. Department of Energy (DOE))

In this project, the Building America team Partnership for Advanced Residential Retrofit (PARR) installed and monitored an ALM aftermarket controller, the M2G from Greffen Systems, at two Chicago area multifamily buildings with existing OTR control.

155

On-Road Remote Sensing of Automobile Emissions in the Chicago Area: Year 2  

E-Print Network (OSTI)

On-Road Remote Sensing of Automobile Emissions in the Chicago Area: Year 2 Peter J. Popp, Gary A from automobiles are at a maximum when the air/fuel ratio is rich of stoichiometric, and are caused

Denver, University of

156

On-Road Remote Sensing of Automobile Emissions in the Chicago Area: Year 1  

E-Print Network (OSTI)

On-Road Remote Sensing of Automobile Emissions in the Chicago Area: Year 1 Peter J. Popp, Gary A.1 Carbon monoxide emissions from automobiles are at a maximum when the air/fuel ratio is rich

Denver, University of

157

Where have all the brownfields gone? : lessons for Chicago 15 years in  

E-Print Network (OSTI)

The Chicago Brownfields Initiative was born of a high profile and well-respected public planning process to change the "brownfields" project from one that relied on liability to one that relied on private investment to ...

Ekerdt, Molly H. (Molly Heinzmann)

2009-01-01T23:59:59.000Z

158

Lessons in sustainable design : case study of a school in Chicago  

E-Print Network (OSTI)

This thesis develops an approach to environmentally sustainable design through the hypothetical redesign of the South Loop School in Chicago. Sustainable architecture seeks to reinforce ecological relationships to the ...

Hootman, Heather

1994-01-01T23:59:59.000Z

159

Site A/Plot M Disposal Site, Chicago, Illinois, Fact Sheet  

Office of Legacy Management (LM)

District to return the sites to the District. The first reactor to achieve a self-sustaining and controlled chain reaction, CP-1, was moved from the University of Chicago to...

160

The new food-tech city : adapting Chicago's post-stockyard urbanism  

E-Print Network (OSTI)

This thesis examines the latent potential of Chicago's former Union Stock Yard, which consequentially draws attention to the polarities of industrial food production. The Union Stock Yard was once symbolic of an era where ...

Burnham, Justin (Justin Paul)

2012-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

Statistical analysis of aerosol species, trace gasses, and meteorology in Chicago  

E-Print Network (OSTI)

possible pollutant sources. Keywords Atmospheric aerosols . Canonical correlation analysis . Chicago air pollution studies involve collection and anal- ysis of atmospheric aerosols and concurrent meteorol- ogy) and principal component analysis (PCA) were applied to atmospheric aerosol and trace gas concentrations

O'Brien, Timothy E.

162

from the President hen Mark Twain wrote of "that astonishing Chicago" in Life on the Mississippi,  

E-Print Network (OSTI)

Whitney describes how we are beginning a third Industrial Revolution [see page 18]; institutions of this revolution. IIT has a long history of noteworthy contributions to Chicago's greatness, and we are poised

163

The relation between Brazilian and Chicago Board of Trade soybean prices: a time series test  

E-Print Network (OSTI)

THE RELATION BETWEEN BRAZILIAN AND CHICAGO BOARD OF TRADE SOYBEAN PRICES ? A TIME SERIES TEST A Thesis BRUNO MELCHER Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements... for the degree of MASTER OF SCIENCE May 1991 Major Subject: Agricultural Economics THE RELATION BETWEEN BRAZILIAN AND CHICAGO BOARD OF TRADE SOYBEAN PRICES ? A TIME SERIES TEST A Thesis by BRUNO MELCHER Approved as to style and content by: ' f J David...

Melcher, Bruno

1991-01-01T23:59:59.000Z

164

An Analysis of Department of Defense Instruction 8500.2 'Information Assurance (IA) Implementation.'  

SciTech Connect

The Department of Defense (DoD) provides its standard for information assurance in its Instruction 8500.2, dated February 6, 2003. This Instruction lists 157 'IA Controls' for nine 'baseline IA levels.' Aside from distinguishing IA Controls that call for elevated levels of 'robustness' and grouping the IA Controls into eight 'subject areas' 8500.2 does not examine the nature of this set of controls, determining, for example, which controls do not vary in robustness, how this set of controls compares with other such sets, or even which controls are required for all nine baseline IA levels. This report analyzes (1) the IA Controls, (2) the subject areas, and (3) the Baseline IA levels. For example, this report notes that there are only 109 core IA Controls (which this report refers to as 'ICGs'), that 43 of these core IA Controls apply without variation to all nine baseline IA levels and that an additional 31 apply with variations. This report maps the IA Controls of 8500.2 to the controls in NIST 800-53 and ITGI's CoBIT. The result of this analysis and mapping, as shown in this report, serves as a companion to 8500.2. (An electronic spreadsheet accompanies this report.)

Campbell, Philip LaRoche

2012-01-01T23:59:59.000Z

165

Learning from the scatter in type Ia supernovae  

SciTech Connect

Type Ia Supernovae are standard candles so their mean apparent magnitude has been exploited to learn about the redshift-distance relationship. Besides intrinsic scatter in this standard candle, additional scatter is caused by gravitational magnification by large scale structure. Here we probe the dependence of this dispersion on cosmological parameters and show that information about the amplitude of clustering, {sigma}{sub 8}, is contained in the scatter. In principle, it will be possible to constrain {sigma}{sub 8} to within 5% with observations of 2000 Type Ia Supernovae. We identify three sources of systematic error - evolution of intrinsic scatter, baryon contributions to lensing, and non-Gaussianity of lensing - which will make this measurement difficult.

Dodelson, Scott [Particle Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500 (United States); Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637-1433 (United States); Vallinotto, Alberto [Particle Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500 (United States); Department of Physics, The University of Chicago, Chicago, Illinois 60637-1433 (United States)

2006-09-15T23:59:59.000Z

166

RADIOACTIVELY POWERED RISING LIGHT CURVES OF TYPE Ia SUPERNOVAE  

SciTech Connect

The rising luminosity of the recent, nearby supernova 2011fe shows a quadratic dependence with time during the first Almost-Equal-To 0.5-4 days. In addition, studies of the composite light curves formed from stacking together many Type Ia supernovae (SNe Ia) have found similar power-law indices for the rise, but may also show some dispersion that may indicate diversity. I explore what range of power-law rises are possible due to the presence of radioactive material near the surface of the exploding white dwarf (WD). I summarize what constraints such a model places on the structure of the progenitor and the distribution and velocity of ejecta. My main conclusion is that for the inferred explosion time for SN 2011fe, its rise requires an increasing mass fraction X {sub 56} Almost-Equal-To (4-6) Multiplication-Sign 10{sup -2} of {sup 56}Ni distributed between a depth of Almost-Equal-To 10{sup -2} and 0.3 M {sub Sun} below the WD's surface. Radioactive elements this shallow are not found in simulations of a single C/O detonation. Scenarios that may produce this material include helium-shell burning during a double-detonation ignition, a gravitationally confined detonation, and a subset of deflagration to detonation transition models. In general, the power-law rise can differ from quadratic depending on the details of the velocity, density, and radioactive deposition gradients in a given event. Therefore, comparisons of this work with observed bolometric rises of SNe Ia would place strong constraints on the properties of the shallow outer layers, providing important clues for identifying the elusive progenitors of SNe Ia.

Piro, Anthony L., E-mail: piro@caltech.edu [Theoretical Astrophysics, California Institute of Technology, 1200 East California Boulevard, M/C 350-17, Pasadena, CA 91125 (United States)

2012-11-10T23:59:59.000Z

167

The Diversity of Variations in the Spectra of Type Ia Supernovae  

E-Print Network (OSTI)

for the degree of DOCTOR OF PHILOSOPHY Approved by: Chair of Committee, Lifan Wang Committee Members, Nicholas Suntze George Kattawar Sean McDeavitt Head of Department, George R. Welch August 2012 Major Subject: Physics iii ABSTRACT The Diversity... of Variations in the Spectra of Type Ia Supernovae. (August 2012) Andrew James Wagers, B.A., Berea College; M.S., Stephen F. Austin State University Chair of Advisory Committee: Dr. Lifan Wang Type Ia supernovae (SNe Ia) are currently the best probe...

Wagers, Andrew James

2012-10-19T23:59:59.000Z

168

Experto Universitario Java Enterprise 2012-2013 Depto. Ciencia de la Computacin e IA  

E-Print Network (OSTI)

Experto Universitario Java Enterprise © 2012-2013 Depto. Ciencia de la Computación e IA Lenguaje Lenguaje Java Avanzado © 2012-2013 Depto. Ciencia de la Computación e IA Lenguaje Java 2 Índice. Ciencia de la Computación e IA Lenguaje Java 3 Java · Java es un lenguaje OO creado por Sun Microsystems

Escolano, Francisco

169

Experto Universitario Java Enterprise 2012-2013 Depto. Ciencia de la Computacin e IA  

E-Print Network (OSTI)

Experto Universitario Java Enterprise © 2012-2013 Depto. Ciencia de la Computación e IA Lenguaje Avanzado © 2012-2013 Depto. Ciencia de la Computación e IA Depuración y logs - 2 · El depurador de Eclipse Enterprise Lenguaje Java Avanzado © 2012-2013 Depto. Ciencia de la Computación e IA Depuración y logs - 3 El

Escolano, Francisco

170

Teor'ia de Grupos y Mec'anica Qu'antica Luis A. Seco  

E-Print Network (OSTI)

determinado por el Hamiltoniano de la energ'ia, un operador que, actuando sobre una funci'on /(x 1 ; : : : ; xTeor'ia de Grupos y Mec'anica Qu'antica Luis A. Seco Universidad de Toronto. Notas del curso; Teor'ia de Grupos y Mec'anica Cu'antica, L. Seco. U.I.M.P. La Coru~na, 27 Junio -- 1 Julio, 1994

Seco, Luis A.

171

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

The large range of time and length scales involved in type Ia supernovae (SN Ia) requires the use of flame models. As a prelude to exploring various options for flame models, we consider, in this paper, high-resolution three-dimensional simulations of the small-scale dynamics of nuclear flames in the supernova environment in which the details of the flame structure are fully resolved. The range of densities examined, 1 to $8 \\times 10^7$ g cm$^{-3}$, spans the transition from the laminar flamelet regime to the distributed burning regime where small scale turbulence disrupts the flame. The use of a low Mach number algorithm facilitates the accurate resolution of the thermal structure of the flame and the inviscid turbulent kinetic energy cascade, while implicitly incorporating kinetic energy dissipation at the grid-scale cutoff. For an assumed background of isotropic Kolmogorov turbulence with an energy characteristic of SN Ia, we find a transition density between 1 and $3 \\times 10^7$ g cm$^{-3}$ where the nature of the burning changes qualitatively. By $1 \\times 10^7$ g cm$^{-3}$, energy diffusion by conduction and radiation is exceeded, on the flame scale, by turbulent advection. As a result, the effective Lewis Number approaches unity. That is, the flame resembles a laminar flame, but is turbulently broadened with an effective diffusion coefficient, $D_T \\sim u' l$, where $u'$ is the turbulent intensity and $l$ is the integral scale. For the larger integral scales characteristic of a real supernova, the flame structure is predicted to become complex and unsteady. Implications for a possible transition to detonation are discussed.

A. J. Aspden; J. B. Bell; M. S. Day; S. E. Woosley; M. Zingale

2008-11-17T23:59:59.000Z

172

General Merchandise 2009 TSD Chicago Low Plug Load 50% Energy Savings |  

Open Energy Info (EERE)

Low Plug Load 50% Energy Savings Low Plug Load 50% Energy Savings Jump to: navigation, search Model Name General Merchandise 2009 TSD Chicago Low Plug Load 50% Energy Savings Building Type Mercantile (Retail Other Than Mall) Model Type 50% Energy Savings Model Target Type ASHRAE 90.1 2004 Model Year 2009 IDF file http://apps1.eere.energy.gov/buildings/energyplus/models/Miami/2009_TSD_GeneralMerch_LPL_50percent.idf XML file http://apps1.eere.energy.gov/buildings/energyplus/models/Miami/2009_TSD_GeneralMerch_LPL_50percent.xml City, State Chicago, IL Climate Zone Climate Zone 5A Retrieved from "http://en.openei.org/w/index.php?title=General_Merchandise_2009_TSD_Chicago_Low_Plug_Load_50%25_Energy_Savings&oldid=270181" Category: Building Models What links here Related changes

173

DOE - Office of Legacy Management -- Chicago North IL Site - IL 05  

Office of Legacy Management (LM)

North IL Site - IL 05 North IL Site - IL 05 FUSRAP Considered Sites Chicago North, IL Alternate Name(s): National Guard Armory 124th Field Artillery Armory Illinois National Guard Armory Site IL.05-4 IL.05-5 Location: 5200 Cottage Grove Avenue, Chicago, Illinois IL.05-4 Historical Operations: Processed and stored uranium metal, resulting in uranium metal and dry uranium oxide contamination. Metallurgical operations were conducted by the University of Chicago, an MED contractor. IL.05-5 IL.05-7 IL.05-8 Eligibility Determination: Eligible IL.05-1 IL.05-2 IL.05-3 Radiological Survey(s): Assessment Surveys, Verification Surveys IL.05-6 IL.05-7 Site Status: Certified-Certification Basis, Federal Register Notice Included IL.05-7 Long-term Care Requirements: Long-Term Surveillance and Maintenance Requirements for Remediated FUSRAP Sites S07566_FUSRAP

174

TIlE UNIVERSITY OF CHICAGO OFFICE OF FACILITIES PLANNING & MANAGEMENT  

Office of Legacy Management (LM)

TIlE UNIVERSITY OF CHICAGO TIlE UNIVERSITY OF CHICAGO OFFICE OF FACILITIES PLANNING & MANAGEMENT * 5555 SOUTIi EU..IS AVENUE CHICAGO, D..LINOIS 60637 (312) 702-1700 April 20, 1989 Mr. David Adler c/o FUSRAP Bechtel National P.O. Box 350 Oak Ridge, Tennessee 37831·350 RE: KE1\7 HALL - Re.r.pQvat of basement drainlines Dear Mr. AdJer: Per our phone conversation on April 12, 1989 I am writing this letter to confirm the fact that the contaminated drainlines and surrounding soil, in the basement of Kent Hall, wer excavated and legaUy disposed of in 1983. This work was carried out in conjunction with the total gutting and renovation of the building. If you need additional infonnation please conta<:t me. incerely, * ~l('~~d~ I !:ynn C. Bender Director LCB:bg

175

Chicago Office CX Determinations | U.S. DOE Office of Science (SC)  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago Office CX Determinations Chicago Office CX Determinations Safety, Security and Infrastructure (SSI) SSI Home Facilities and Infrastructure Safeguards & Security Environment, Safety and Health (ES&H) Organization Chart .pdf file (82KB) Phone Listing .pdf file (129KB) SC HQ Continuity of Operations (COOP) Implementation Plan .pdf file (307KB) Categorical Exclusion Determinations SLI & SS Budget Contact Information Safety, Security and Infrastructure U.S. Department of Energy SC-31/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-4097 F: (301) 903-7047 Categorical Exclusion (CX) Determinations Chicago Office CX Determinations Print Text Size: A A A RSS Feeds FeedbackShare Page Categorical Exclusion Determination Documents (CX Determinations): * Determination Date Name of Action: Description Categorical Exclusion Number External link

176

Chicago Office CX Determinations | U.S. DOE Office of Science (SC)  

NLE Websites -- All DOE Office Websites (Extended Search)

Chicago Office CX Determinations Chicago Office CX Determinations Integrated Support Center (ISC) ISC Home About Services Freedom of Information Act (FOIA) Privacy Act Categorical Exclusion Determinations Contact Information Integrated Support Center Roxanne Purucker U.S. Department of Energy 9800 S. Cass Avenue Argonne, IL 60439 P: (630) 252-2110 Larry Kelly U.S. Department of Energy 200 Administration Road Oak Ridge, TN 37830 P: (865) 576-0885 Categorical Exclusion (CX) Determinations Chicago Office CX Determinations Print Text Size: A A A RSS Feeds FeedbackShare Page Categorical Exclusion Determination Documents (CX Determinations): * Determination Date Name of Action: Description Categorical Exclusion Number External link 07/17/2013 Generic Categorical Exclusion Determination for Financial Assistance Awards .pdf file (905KB) Various

177

The Recurrent Nova U Scorpii - A Type Ia Supernova Progenitor  

E-Print Network (OSTI)

We derive the mass of the white dwarf in the eclipsing recurrent nova U Sco from the radial velocity semi-amplitudes of the primary and secondary stars. Our results give a high white dwarf mass of M_1 = 1.55 \\pm 0.24M_\\odot, consistent with the thermonuclear runaway model of recurrent nova outbursts. We confirm that U Sco is the best Type Ia supernova progenitor known, and predict that the time to explosion is within ~700,000 years.

T. D. Thoroughgood; V. S. Dhillon; S. P. Littlefair; T. R. Marsh; D. A. Smith

2001-09-28T23:59:59.000Z

178

Tension in the Recent Type Ia Supernovae Datasets  

E-Print Network (OSTI)

In the present work, we investigate the tension in the recent Type Ia supernovae (SNIa) datasets Constitution and Union. We show that they are in tension not only with the observations of the cosmic microwave background (CMB) anisotropy and the baryon acoustic oscillations (BAO), but also with other SNIa datasets such as Davis and SNLS. Then, we find the main sources responsible for the tension. Further, we make this more robust by employing the method of random truncation. Based on the results of this work, we suggest two truncated versions of the Union and Constitution datasets, namely the UnionT and ConstitutionT SNIa samples, whose behaviors are more regular.

Hao Wei

2010-04-07T23:59:59.000Z

179

KPD1930+2752 - a candidate Type Ia supernova progenitor  

E-Print Network (OSTI)

We present spectra of the pulsating sdB star KPD1930+2752 which confirm that this star is a binary. The radial velocities measured from the H-alpha and HeI6678 spectral lines vary sinusoidally with the same period (2h 17m) as the ellipsoidal variability seen by Billeres et al. (2000). The amplitude of the orbital motion (349.3+-2.7 km/s) combined with the canonical mass for sdB stars (0.5 solar masses) implies a total mass for the binary of 1.47+-0.01 solar masses The unseen companion star is almost certainly a white dwarf star. The binary will merge within about 200 million years due to gravitational wave radiation. The accretion of helium and other elements heavier than hydrogen onto the white dwarf which then exceeds the Chandrasekhar mass (1.4 solar masses) is a viable model for the cause of Type Ia supernovae. KPD1930+2752 is the first star to be discovered which is a good candidate for the progenitor of a Type Ia supernova of this type which will merge on an astrophysically interesting timescale.

P. F. L. Maxted; T. R. Marsh; R. C. North

2000-07-18T23:59:59.000Z

180

Search for progenitors of supnernovae type Ia with SPY  

E-Print Network (OSTI)

We have started a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor surveY - SPY). About 400 white dwarfs were checked for radial velocity variations during the first 15 months of this project, twice the number of white dwarfs investigated during the last 20 years. We give an overview of the SPY project and present first results Fifty four new DDs have been discovered, seven of them double lined (only 18 and 6 objects of these groups were known before, respectively). The final sample is expected to contain 150 to 200 DDs. Eight new pre-cataclysmic binaries were also detected. SPY is the first DD survey which encompasses also non-DA white dwarfs. SPY produces an immense, unique sample of very high resolution white dwarf spectra, which provides a lot of spin-off opportunities. We describe our projects to exploit the SPY sample for the determination of basic parameters, kinematics, and rotational velocities of white dwarfs. A catalogue with a first subset of our white dwarf data has already been published by Koester et al. 2001.

R. Napiwotzki; N. Christlieb; H. Drechsel; H. -J. Hagen; U. Heber; D. Homeier; C. Karl; D. Koester; B. Leibundgut; T. R. Marsh; S. Moehler; G. Nelemans; E. -M. Pauli; D. Reimers; A. Renzini; L. Yungelson

2002-03-09T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
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We encourage you to perform a real-time search of NLEBeta
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181

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA  

Gasoline and Diesel Fuel Update (EIA)

0.00-1.99 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA ME MI MA MD MN MS MT MO NE ND OH NV NM NY NH NC OK OR PA RI SC SD TN TX UT VT WA WV WI AZ VA DC 0.00-1.99 2.00-2.99 3.00-3.99 4.00-4.99 5.00-5.99 6.00-6.99 7.00+ 18. Average Price of Natural Gas Delivered to U.S. Onsystem Industrial Consumers, 1996 (Dollars per Thousand Cubic Feet) Figure 19. Average Price of Natural Gas Delivered to U.S. Electric Utilities, 1996 (Dollars per Thousand Cubic Feet) Figure Sources: Federal Energy Regulatory Commission (FERC), Form FERC-423, "Monthly Report of Cost and Quality of Fuels for Electric Plants," and Energy Information Administration (EIA), Form EIA-176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." Note: In 1996, consumption of natural gas for agricultural use

182

Search for double degenerate progenitors of supernovae type Ia with SPY  

E-Print Network (OSTI)

We report on a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (SN Ia Progenitor surveY - SPY). About 560 white dwarfs were checked for radial velocity variations until now. Ninety new DDs have been discovered, including short period systems with masses close to the Chandrasekhar mass.

R. Napiwotzki; N. Christlieb; H. Drechsel; H. -J. Hagen; U. Heber; D. Homeier; C. Karl; D. Koester; B. Leibundgut; T. R. Marsh; S. Moehler; G. Nelemans; E. -M. Pauli; D. Reimers; A. Renzini; L. Yungelson

2002-10-29T23:59:59.000Z

183

Jordan Cove Energy Project Fort Chicago Energy Partners L.P.  

E-Print Network (OSTI)

Jordan Cove Energy Project Fort Chicago Energy Partners L.P. 1.0 Bcfd Coos Bay, Oregon Oregon LNG Funding Partners 1.0-1.5 Bcfd Astoria, Oregon Portwestward LNG Facility Portwestward LNG, LLC 0.7-1.25 Bcfd Clatskanie, Oregon Kitimat LNG Facility Apache Corp 0.64 -1.0 Bcfd Kitimat, British Columbia

184

2013 NIAC Spring Symposium Chicago, IL -March 12-14, 2013  

E-Print Network (OSTI)

Research 10:30 Poster Overview NIAC Phase II Fellows will briefly introduce their studies. Posters Address Bryan Wunar, Director, Center for the Advancement of Science Education, Chicago Museum of Science & Industry Education and Public Outreach: Inspiring the Next Generation 2:00 Geoffrey Landis, NASA GRC Venus

185

GCI Monthly A publication of the Great Cities Institute at the University of Illinois at Chicago  

E-Print Network (OSTI)

1 GCI Monthly A publication of the Great Cities Institute at the University of Illinois. I hope the summer treated you well, and that you can join us at Great Cities with renewed energy at the University of Illinois at Chicago. She holds a PhD degree in Computer Science from the University of Toronto

Illinois at Chicago, University of

186

REPORT ABSTRACT The Chicago Health, Environmental Exposure, and Recreation Study (CHEERS)  

E-Print Network (OSTI)

the health risks of limited contact water recreation activities - motor boating, canoeing, fishing, kayaking-disinfected, wastewater from water reclamation plants of the Metropolitan Water Reclamation District of Greater Chicago, the funder of CHEERS. CHEERS was designed using the methods of USEPA studies of water recreation and health

Illinois at Chicago, University of

187

The 474rd Convocation at the University of Chicago Address: "Value in an Uncertain Economy"  

E-Print Network (OSTI)

The 474rd Convocation at the University of Chicago Address: "Value in an Uncertain Economy" By Lars. Expanding your knowledge and refining your analytical skill are investments in your own human capital. This uncertainty, however, alters the decisions we make and alters value as determined by a market economy. I

Hansen, Lars Peter

188

UNIVERSITY OF CHICAGO TOPOLOGY AND HETEROGENEITY AT THE RATE-LIMITING STEP  

E-Print Network (OSTI)

UNIVERSITY OF CHICAGO TOPOLOGY AND HETEROGENEITY AT THE RATE-LIMITING STEP OF THE PROTEIN FOLDING .......................................................................... 2 1.3 Physical processes in protein folding...................................................... 5 of the rate-limiting step in protein folding ...................... 11 1.4.1 Two-state mechanisms and TS

Sosnick, Tobin R.

189

Analytical Expressions For Light-Curves Of Ordinary And Superluminous Supernovae Type Ia  

E-Print Network (OSTI)

Ordinary supernovae of type Ia (SNeIa) may be produced by the thermonuclear explosion of white dwarfs (WDs), which after their nascence in proto-planetary nebulae accrete fall-back matter and approach the Chandrasekhar mass limit. If the detonation continues into the fall-back layer and/or if the SNIa debris collide with it, they may produce a super Chandrasekhar SNIa. A few underlying physical assumptions of such model yield a very simple master formula that reproduces quite well the bolometric light-curves of both ordinary and supeluminous SNeIa. Other main properties of SNeIa, including the empirical 'brighter-slower' Philipps' relation that was used to standardize ordinary SNeIa as distance indicators and led to the discovery of the accelerating expansion of the universe are also reproduced.

Shlomo Dado; Arnon Dar

2014-02-06T23:59:59.000Z

190

Type Ia supernova rate studies from the SDSS-II Supernova Study  

SciTech Connect

The author presents new measurements of the type Ia SN rate from the SDSS-II Supernova Survey. The SDSS-II Supernova Survey was carried out during the Fall months (Sept.-Nov.) of 2005-2007 and discovered {approx} 500 spectroscopically confirmed SNe Ia with densely sampled (once every {approx} 4 days), multi-color light curves. Additionally, the SDSS-II Supernova Survey has discovered several hundred SNe Ia candidates with well-measured light curves, but without spectroscopic confirmation of type. This total, achieved in 9 months of observing, represents {approx} 15-20% of the total SNe Ia discovered worldwide since 1885. The author describes some technical details of the SN Survey observations and SN search algorithms that contributed to the extremely high-yield of discovered SNe and that are important as context for the SDSS-II Supernova Survey SN Ia rate measurements.

Dilday, Benjamin; /Chicago U.

2008-08-01T23:59:59.000Z

191

Type Ia supernovae selection and forecast of cosmology constraints for the Dark Energy Survey  

Science Journals Connector (OSTI)

We present the results of a study of selection criteria to identify Type Ia supernovae photometrically in a simulated mixed sample of Type Ia supernovae and core collapse supernovae. The simulated sample is a mockup of the expected results of the Dark Energy Survey. Fits to the \\{MLCS2k2\\} and SALT2 Type Ia supernova models are compared and used to help separate the Type Ia supernovae from the core collapse sample. The Dark Energy Task Force Figure of Merit (modified to include core collapse supernovae systematics) is used to discriminate among the various selection criteria. This study of varying selection cuts for Type Ia supernova candidates is the first to evaluate core collapse contamination using the Figure of Merit. Different factors that contribute to the Figure of Merit are detailed. With our analysis methods, both SALT2 and \\{MLCS2k2\\} Figures of Merit improve with tighter selection cuts and higher purities, peaking at 98% purity.

Eda Gjergo; Jefferson Duggan; John D. Cunningham; Steve Kuhlmann; Rahul Biswas; Eve Kovacs; Joseph P. Bernstein; Harold Spinka

2013-01-01T23:59:59.000Z

192

Microsoft PowerPoint - IEEE IAS PES 102313.pptx  

NLE Websites -- All DOE Office Websites (Extended Search)

DOE's ARRA DOE's ARRA Smart Grid Program Steve Bossart, Senior Energy Analyst IEEE IAS/PES Pittsburgh Section October 23, 2013 ‹#› Topics * OE ARRA Smart Grid Program * OE ARRA Smart Grid Progress * Results and Case Studies * Life After ARRA Smart Grid ‹#› DOE OE ARRA Smart Grid Program ‹#› American Recovery and Reinvestment Act ($4.5B) * Smart Grid Investment Grants (99 projects) - $3.4 billion Federal; $4.7 billion private sector - > 800 PMUs covering almost 100% of transmission - ~ 8000 distribution automation circuits - > 15 million smart meters * Smart Grid Demonstration Projects (32 projects) - $685 million Federal; $1 billion private sector - 16 storage projects - 16 regional demonstrations Smart Grid ARRA Activities ‹#› Smart Grid investment from ARRA field projects

193

Type Ia Supernova: Burning and Detonation in the Distributed Regime  

E-Print Network (OSTI)

A simple, semi-analytic representation is developed for nuclear burning in Type Ia supernovae in the special case where turbulent eddies completely disrupt the flame. The speed and width of the ``distributed'' flame front are derived. For the conditions considered, the burning front can be considered as a turbulent flame brush composed of corrugated sheets of well-mixed flames. These flames are assumed to have a quasi-steady-state structure similar to the laminar flame structure, but controlled by turbulent diffusion. Detonations cannot appear in the system as long as distributed flames are still quasi-steady-state, but this condition is violated when the distributed flame width becomes comparable to the size of largest turbulent eddies. When this happens, a transition to detonation may occur. For current best estimates of the turbulent energy, the most likely density for the transition to detonation is in the range 0.5 - 1.5 x 10^7 g cm^{-3}.

S. E. Woosley

2007-09-26T23:59:59.000Z

194

Type Ia Supernova Hubble Residuals and Host-Galaxy Properties  

SciTech Connect

Kim et al. (2013) [K13] introduced a new methodology for determining peak- brightness absolute magnitudes of type Ia supernovae from multi-band light curves. We examine the relation between their parameterization of light curves and Hubble residuals, based on photometry synthesized from the Nearby Supernova Factory spec- trophotometric time series, with global host-galaxy properties. The K13 Hubble residual step with host mass is 0.013 ? 0.031 mag for a supernova subsample with data coverage corresponding to the K13 training; at ? 1?, the step is not significant and lower than previous measurements. Relaxing the data coverage requirement the Hubble residual step with host mass is 0.045 ? 0.026 mag for the larger sample; a calculation using the modes of the distributions, less sensitive to outliers, yields a step of 0.019 mag. The analysis of this article uses K13 inferred luminosities, as distinguished from previous works that use magnitude corrections as a function of SALT2 color and stretch param- eters: Steps at> 2? significance are found in SALT2 Hubble residuals in samples split by the values of their K13 x(1) and x(2) light-curve parameters. x(1) affects the light- curve width and color around peak (similar to the?m15 and stretch parameters), and x(2) affects colors, the near-UV light-curve width, and the light-curve decline 20 to 30 days after peak brightness. The novel light-curve analysis, increased parameter set, and magnitude corrections of K13 may be capturing features of SN Ia diversity arising from progenitor stellar evolution.

Nearby Supernova Factory; Kim, A. G.; Aldering, G.; Antilogus, P.; Aragon, C.; Bailey, S.; Baltay, C.; Bongard, S.; Buton, C.; Canto, A.; Cellier-Holzem, F.; Childress, M.; Chotard, N.; Copin, Y.; Fakhouri, H. K.; Feindt, U.; Fleury, M.; Gangler, E.; Greskovic, P.; Guy, J.; Kowalski, M.; Lombardo, S.; Nordin, J.; Nugent, P.; Pain, R.; Pecontal, E.; Pereira, R.; Perlmutter, S.; Rabinowitz, D.; Rigault, M.; Runge, K.; Saunders, C.; Scalzo, R.; Smadja, G.; Tao, C.; Thomas, R. C.; Weaver, B. A.

2014-01-17T23:59:59.000Z

195

A mutant of Escherichia coli defective in penicillin-binding protein 5 and lacking D-alanine carboxypeptidase IA.  

Science Journals Connector (OSTI)

...preparation of D-alanrne car- boxypeptidase IA of...IA, because a mutant defective in D-alanine carbox...both activities were defective or both were normal...residual D-alanine car- boxypeptidase IA activity...and to obtain a mutant defective in PBP-6 are in progress...

Y Nishimura; H Suzuki; Y Hirota; J T Park

1980-07-01T23:59:59.000Z

196

Stellar Populations and the White Dwarf Mass Function: Connections To Supernova Ia Luminosities  

E-Print Network (OSTI)

We discuss the luminosity function of SNe Ia under the assumption that recent evidence for dispersion in this standard candle is related to variations in the white dwarf mass function (WDMF) in the host galaxies. We develop a simple parameterization of the WDMF as a function of age of a stellar population and apply this to galaxies of different morphological types. We show that this simplified model is consistent with the observed WDMF of Bergeron et al. (1992) for the solar neighborhood. Our simple models predict that WDMF variations can produce a range of more than 1.8 mag in M$_B$(SN Ia), which is comparable to the observed value using the data of Phillips (1993) and van den Bergh (1996). We also predict a galaxy type dependence of M$_B$(SN Ia) under standard assumptions of the star formation history in these galaxies and show that M$_B$(SN Ia) can evolve with redshift. In principle both evolutionary and galaxy type corrections should be applied to recover the intrinsic range of M$_B$(SN Ia) from the observed values. Our current inadequate knowledge of the star formation history of galaxies coupled with poor physical understanding of the SN Ia mechanism makes the reliable estimation of these corrections both difficult and controversial. The predictions of our models combined with the observed galaxy and redshift correlations may have the power to discriminate between the Chandrasekhar and the sub-Chandrasekhar progenitor scenarios for SNe Ia.

Ted von Hippel; G. D. Bothun; R. A. Schommer

1997-06-11T23:59:59.000Z

197

Tension and Systematics in the Gold06 SnIa Dataset  

E-Print Network (OSTI)

The Gold06 SnIa dataset recently released in astro-ph/0611572 consists of five distinct subsets defined by the group or instrument that discovered and analyzed the corresponding data. These subsets are: the SNLS subset (47 SnIa), the HST subset (30 SnIa), the HZSST subset (41 SnIa), the SCP subset (26 SnIa) and the Low Redshift (LR) subset (38 SnIa). These subsets sum up to the 182 SnIa of the Gold06 dataset. We use Monte-Carlo simulations to study the statistical consistency of each one of the above subsets with the full Gold06 dataset. In particular, we compare the best fit $w(z)$ parameters (w_0,w_1) obtained by subtracting each one of the above subsets from the Gold06 dataset (subset truncation), with the corresponding best fit parameters (w^r_0,w^r_1) obtained by subtracting the same number of randomly selected SnIa from the same redshift range of the Gold06 dataset (random truncation). We find that the probability for (w^r_0,w^r_1)=(w_0,w_1) is large for the Gold06 minus SCP (Gold06-SCP) truncation but is less than 5% for the Gold06-SNLS, Gold06-HZSST and Gold06-HST truncations. This result implies that the Gold06 dataset is not statistically homogeneous. By comparing the values of the best fit (w_0,w_1) for each subset truncation we find that the tension among subsets is such that the SNLS and HST subsets are statistically consistent with each other and `pull' towards LCDM (w_0=-1,w_1=0) while the HZSST subset is statistically distinct and strongly `pulls' towards a varying w(z) crossing the line $w=-1$ from below (w_00). We also isolate six SnIa that are mostly responsible for this behavior of the HZSST subset.

S. Nesseris; L. Perivolaropoulos

2007-01-09T23:59:59.000Z

198

Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors  

E-Print Network (OSTI)

Context: Manganese is predominantly synthesised in Type Ia supernova (SN Ia) explosions. Owing to the entropy dependence of the Mn yield in explosive thermonuclear burning, SNe Ia involving near Chandrasekhar-mass white dwarfs (WDs) are predicted to produce Mn to Fe ratios significantly exceeding those of SN Ia explosions involving sub-Chandrasekhar mass primary WDs. Of all current supernova explosion models, only SN Ia models involving near-Chandrasekhar mass WDs produce [Mn/Fe] > 0.0. Aims: Using the specific yields for competing SN Ia scenarios, we aim to constrain the relative fractions of exploding near-Chandrasekhar mass to sub-Chandrasekhar mass primary WDs in the Galaxy. Methods: We extract the Mn yields from three-dimensional thermonuclear supernova simulations referring to different initial setups and progenitor channels. We then compute the chemical evolution of Mn in the Solar neighborhood, assuming SNe Ia are made up of different relative fractions of the considered explosion models. Results: We ...

Seitenzahl, Ivo R; Roepke, Friedrich K; Ruiter, Ashley J

2013-01-01T23:59:59.000Z

199

RADIOLOGICAL SURVEY AT 5823/5849 NORTH RAVENSWOOD AVEXJE CHICAGO, ILLINOIS  

Office of Legacy Management (LM)

RADIOLOGICAL SURVEY RADIOLOGICAL SURVEY AT 5823/5849 NORTH RAVENSWOOD AVEXJE CHICAGO, ILLINOIS Prepared by M.R. LANDIS Environmental Survey and Site Assessment Program Energy/Environment Systems Division Oak Ridge Associated Universities Oak Ridge, TN 37831-0117 Project Staff J.D. Berger R.C. Gosslee E.A. Powell G.R. Foltz M.J. Laudeman A. Wallo* C.F. Weaver Prepared for U.S. Department of Energy as part of the Formerly Utilized Sites - Remedial Action Program FINAL REPORT OCTOBER 1989 This report is based on work performed under contract number DE-AC05-760RC0033 with the U.S. Department of Energy. *with the U.S. Department of Energy, Division of Facility and Site Decommissioning -- LIST OF FIGURES Page FIGURE 1: Map of Chicago, Illinois Indicating the Location of the Facility at

200

Overview of sSupply of Chicago/Milwaukee Gasoline This Spring:  

Gasoline and Diesel Fuel Update (EIA)

Supply of Chicago/Milwaukee Gasoline Spring 20001 Supply of Chicago/Milwaukee Gasoline Spring 20001 Joanne Shore, Petroleum Division Tight Supply at the Beginning of Summer Gasoline Season This summer's run-up in Midwest gasoline prices, like other recent price spikes, stemmed from a number of factors. The stage was set for gasoline volatility as a result of tight crude oil supplies, which led to low crude oil and low product stocks and relatively high crude oil prices. With little stock cushion to absorb unexpected events, Midwest gasoline prices surged when a number of supply problems developed, including pipeline and refinery supply problems, and an unexpectedly difficult transition to summer-grade Phase II reformulated gasoline (RFG). Prior to the current summer driving season, gasoline stocks were low

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

Microsoft Word - DOE-ID-13-052 Chicago EC B3-6.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 SECTION A. Project Title: Development of Novel Porous Sorbents for Extraction of Uranium from Seawater - The University of Chicago SECTION B. Project Description The University of Chicago proposes to develop highly porous sorbents for the extraction of uranium from seawater. This will be accomplished through design and investigation of new multifunctional uranyl chelators and engineering on nanoporous supports that facilitate cooperative sorbent interactions. Once candidate materials have been synthesized, they will be evaluated for uranium binding capacities, selectivity, uptake and elution kinetics, durability, and reusability. SECTION C. Environmental Aspects / Potential Sources of Impact Radioactive Material Use - It is expected that 2 grams of depleted uranium will be used each year. The depleted uranium is

202

Current Research at the University of Chicago Enrico Fermi Institute and James Franck Institute  

ScienceCinema (OSTI)

These talks will give an overview of physics research at the University of Chicago centered in two research institutes. The Enrico Fermi Institute pursues research in some core areas of the physical sciences. These include cosmology, particle physics, theoretical physics, particle astrophysics, and cosmochemistry. The EFI talk will focus on some examples of these activities which together will provide a broad overview of EFI science. Research at the James Franck Institute centers on the intersection between physics, chemistry and materials science, with the aim to unravel the complex connections between structure and dynamics in condensed matter systems. The JFI is also home to the Chicago Materials Research Science and Engineering Center. The JFI talk will provide highlights of current projects by JFI members.

Simon Swordy

2010-01-08T23:59:59.000Z

203

INDECOMPOSABLE RACKS OF ORDER p2 MAT'IAS GRA"NA  

E-Print Network (OSTI)

INDECOMPOSABLE RACKS OF ORDER p2 MAT'IAS GRA"NA Abstract.We classify indecomposable racks of order p2(p a prime). There a of prime order is trivial. 1.Introduction Racks and quandles have

Graña, Matías

204

Structural studies of allosteric regulation in the class Ia Ribonucleotide reductase from Escherichia coli  

E-Print Network (OSTI)

Ribonucleotide reductase (RNR) converts ribonucleotides to deoxyribonucleotides, the building blocks for DNA replication and repair. The E. coli class Ia enzyme requires two subunits to catalyze the radical-based reduction ...

Zimanyi, Christina Marie

2013-01-01T23:59:59.000Z

205

Type Ia supernova rate at a redshift of ~;0.1  

SciTech Connect

We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement of the detection efficiency, using a Monte Carlo simulation, provides the type Ia supernova explosion rate at a redshift {approx} 0.13. The result is 0.125{sub -0.034-0.028}{sup +0.044+0.028} h{sub 70}{sup 2} SNu where 1 SNu = 1 SN/10{sup 10} L{sub {circle_dot}}{sup B}/century. This value is compatible with the previous EROS measurement (Hardin et al. 2000), done with a much smaller sample, at a similar redshift. Comparison with other values at different redshifts suggests an evolution of the type Ia supernova rate.

Blanc, G.; Afonso, C.; Alard, C.; Albert, J.N.; Aldering, G.; Amadon, A.; Andersen, J.; Ansari, R.; Aubourg, E.; Balland, C.; Bareyre,P.; Beaulieu, J.P.; Charlot, X.; Conley, A.; Coutures, C.; Dahlen, T.; Derue, F.; Fan, X.; Ferlet, R.; Folatelli, G.; Fouque, P.; Garavini, G.; Glicenstein, J.F.; Goldman, B.; Goobar, A.; Gould, A.; Graff, D.; Gros,M.; Haissinski, J.; Hamadache, C.; Hardin, D.; Hook, I.M.; deKat, J.; Kent, S.; Kim, A.; Lasserre, T.; LeGuillou, L.; Lesquoy, E.; Loup, C.; Magneville, C.; Marquette, J.B.; Maurice, E.; Maury, A.; Milsztajn, A.; Moniez, M.; Mouchet, M.; Newberg, H.; Nobili, S.; Palanque-Delabrouille,N.; Perdereau, O.; Prevot, L.; Rahal, Y.R.; Regnault, N.; Rich, J.; Ruiz-Lapuente, P.; Spiro, M.; Tisserand, P.; Vidal-Madjar, A.; Vigroux,L.; Walton, N.A.; Zylberajch, S.

2004-05-11T23:59:59.000Z

206

~ VII -ATTiVIT EDILIZIE .. Servizio di Ateneo per lEnergIa  

E-Print Network (OSTI)

~ VII - ATTiVIT? EDILIZIE n'p. .' .. Servizio di Ateneo per lEnergIa - N AlJZ43 ········ - .·:tri

Di Pillo, Gianni

207

Infrastructure Assessment Mission: USACE Infrastructure Assessment (IA) Planning and Response Teams (PRTs) have two main  

E-Print Network (OSTI)

, and structural engineering applications; urban search & rescue (US&R) support; and water/wastewater) include pre- and post-declaration support for deploying an IA management cell, water/wastewater assessment

US Army Corps of Engineers

208

Gamma-rays from Type Ia supernova SN2014J  

E-Print Network (OSTI)

The whole set of INTEGRAL observations of type Ia supernova SN2014J, covering the period 16-162 days after the explosion has being analyzed. For spectral fitting the data are split into early and late periods covering days 16-35 and 50-162, respectively, optimized for Ni-56 and Co-56 lines. As expected for the early period much of the gamma-ray signal is confined to energies below $\\sim$200 keV, while for the late period it is most strong above 400 keV. In particular, in the late period Co-56 lines at 847 and 1248 keV are detected at 4.7 and 4.3 sigma respectively. The lightcurves in several representative energy bands are calculated for the entire period. The resulting spectra and lightcurves are compared with a subset of models. We confirm our previous finding that the gamma-ray data are broadly consistent with the expectations for canonical 1D models, such as delayed detonation or deflagration models for a near-Chandrasekhar mass WD. Late optical spectra (day 136 after the explosion) show rather symmetric ...

Churazov, E; Isern, J; Bikmaev, I; Bravo, E; Chugai, N; Grebenev, S; Jean, P; Kndlseder, J; Lebrun, F; Kuulkers, E

2015-01-01T23:59:59.000Z

209

2010-2011 Depto. Ciencia de la Computacin e IA Especialista Universitario Java Enterprise  

E-Print Network (OSTI)

© 2010-2011 Depto. Ciencia de la Computación e IA Especialista Universitario Java Enterprise Struts Sesión 4: Introducción a Struts 2 #12;© 2010-2011 Depto. Ciencia de la Computación e IA Especialista · Taglibs · Internacionalización · Validación · Conceptos nuevos en Struts 2 #12;© 2010-2011 Depto. Ciencia

Escolano, Francisco

210

Experto Universitario Java Enterprise 2012-2013 Depto. Ciencia de la Computacin e IA  

E-Print Network (OSTI)

Experto Universitario Java Enterprise © 2012-2013 Depto. Ciencia de la Computación e IA Lenguaje Java Avanzado Sesión 3: Tratamiento de errores #12;Lenguaje Java Avanzado © 2012-2013 Depto. Ciencia de · Tipos genéricos #12;Lenguaje Java Avanzado © 2012-2013 Depto. Ciencia de la Computación e IA Errores - 3

Escolano, Francisco

211

Constraining the double-degenerate scenario for Type Ia supernovae from merger ejected matter  

E-Print Network (OSTI)

We follow the mass blown during the WD-WD merger process in the Double-Degenerate (DD) scenario for type Ia supernovae (SN Ia), and find that the interaction of the SN ejecta with this wind affects the early (thermal energy and then to additional radiation. The radiation could be interpreted as an explosion originating from a progenitor having a radius of one solar radius or more, contradicting observations of SN 2011fe.

Levanon, Naveh; Garca-Berro, Enrique

2014-01-01T23:59:59.000Z

212

THE DISCOVERY OF THE MOST DISTANT KNOWN TYPE Ia SUPERNOVA AT REDSHIFT 1.914  

SciTech Connect

We present the discovery of a Type Ia supernova (SN) at redshift z = 1.914 from the CANDELS multi-cycle treasury program on the Hubble Space Telescope (HST). This SN was discovered in the infrared using the Wide-Field Camera 3, and it is the highest-redshift Type Ia SN yet observed. We classify this object as a SN Ia by comparing its light curve and spectrum with those of a large sample of Type Ia and core-collapse SNe. Its apparent magnitude is consistent with that expected from the {Lambda}CDM concordance cosmology. We discuss the use of spectral evidence for classification of z > 1.5 SNe Ia using HST grism simulations, finding that spectral data alone can frequently rule out SNe II, but distinguishing between SNe Ia and SNe Ib/c can require prohibitively long exposures. In such cases, a quantitative analysis of the light curve may be necessary for classification. Our photometric and spectroscopic classification methods can aid the determination of SN rates and cosmological parameters from the full high-redshift CANDELS SN sample.

Jones, David O.; Rodney, Steven A.; Riess, Adam G. [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Mobasher, Bahram [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Dahlen, Tomas; Casertano, Stefano; Koekemoer, Anton [Space Telescope Science Institute, Baltimore, MD 21218 (United States); McCully, Curtis; Keeton, Charles R.; Patel, Brandon [Department of Physics and Astronomy, Rutgers, State University of New Jersey, Piscataway, NJ 08854 (United States); Frederiksen, Teddy F.; Hjorth, Jens [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen (Denmark); Strolger, Louis-Gregory [Department of Physics, Western Kentucky University, Bowling Green, KY 42101 (United States); Wiklind, Tommy G. [Joint ALMA Observatory, ESO, Santiago (Chile); Challis, Peter [Harvard/Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Graur, Or [School of Physics and Astronomy, Tel-Aviv University, Tel-Aviv 69978 (Israel); Hayden, Brian; Garnavich, Peter [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Weiner, Benjamin J. [Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States); Filippenko, Alexei V. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); and others

2013-05-10T23:59:59.000Z

213

CIMAT, VIII Escuela de verano, 30 de julio -12 de agos* Introducci'on a la Geometr'ia de la Mec'anic*  

E-Print Network (OSTI)

* *fluencia de una fuerza F(x) se define su energ'ia (como funci'on de su posici'on y velocidad) por E = T +* * V donde la energ'ia cin'etica T = m(x`)2=2 y la energ'ia potencial V (x) es una funci'on que(x) entonces su energ* *'ia E se mantiene constante en el tiempo (la Ley de Conservaci'on de Energ'ia

Bor, Gil

214

Verifying the Cosmological Utility of Type Ia Supernovae: Implications of a Dispersion in the Ultraviolet Spectra  

SciTech Connect

We analyze the mean rest-frame ultraviolet (UV) spectrum of Type Ia Supernovae (SNe) and its dispersion using high signal-to-noise ratio Keck-I/LRIS-B spectroscopy for a sample of 36 events at intermediate redshift (z=0.5) discovered by the Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS). We introduce a new method for removing host galaxy contamination in our spectra, exploiting the comprehensive photometric coverage of the SNLS SNe and their host galaxies, thereby providing the first quantitative view of the UV spectral properties of a large sample of distant SNe Ia. Although the mean SN Ia spectrum has not evolved significantly over the past 40percent of cosmic history, precise evolutionary constraints are limited by the absence of a comparable sample of high-quality local spectra. The mean UV spectrum of our z~;;=0.5 SNe Ia and its dispersion is tabulated for use in future applications. Within the high-redshift sample, we discover significant UV spectral variations and exclude dust extinction as the primary cause by examining trends with the optical SN color. Although progenitor metallicity may drive some of these trends, the variations we see are much larger than predicted in recent models and do not follow expected patterns. An interesting new result is a variation seen in the wavelength of selected UV features with phase. We also demonstrate systematic differences in the SN Ia spectral features with SN light curve width in both the UV and the optical. We show that these intrinsic variations could represent a statistical limitation in the future use of high-redshift SNe Ia for precision cosmology. We conclude that further detailed studies are needed, both locally and at moderate redshift where the rest-frame UV can be studied precisely, in order that future missions can confidently be planned to fully exploit SNe Ia as cosmological probes.

Nugent, Peter E; Ellis, R.S.; Sullivan, M.; Nugent, P.E.; Howell, D.A.; Gal-Yam, A.; Astier, P.; Balam, D.; Balland, C.; Basa, S.; Carlberg, R.; Conley, A.; Fouchez, D.; Guy, J.; Hardin, D.; Hook, I.; Pain, R.; Perrett, K.; Pritchet, C.J.; Regnault, N.

2008-02-28T23:59:59.000Z

215

Utilizing Type Ia Supernovae in a Large, Fast, Imaging Survey to Constrain Dark Energy  

E-Print Network (OSTI)

We study the utility of a large sample of type Ia supernovae that might be observed in an imaging survey that rapidly scans a large fraction of the sky for constraining dark energy. We consider information from the traditional luminosity distance test as well as the spread in SNeIa fluxes at fixed redshift induced by gravitational lensing. We include a treatment of photometric redshift uncertainties in our analysis. Our primary result is that the information contained in the mean distance moduli of SNeIa and the dispersion among SNeIa distance moduli complement each other, breaking a degeneracy between the present dark energy equation of state and its time variation without the need for a high-redshift supernova sample. To address photometric redshift uncertainties, we present dark energy constraints as a function of the size of an external set of spectroscopically-observed SNeIa that may be used for redshift calibration, nspec. We find that an imaging survey can constrain the dark energy equation of state at the epoch where it is best constrained with a 1-sigma error of sigma(wpiv)~0.03-0.09$, depending upon various assumptions. In addition, the marginal improvement in the error sigma(wpiv) from an increase in the spectroscopic calibration sample drops once nspec ~ 10^3. This result is important because it is of the order of the size of calibration samples likely to be compiled in the coming decade and because, for samples of this size, the spectroscopic and imaging surveys individually place comparable constraints on the dark energy equation of state. In all cases, it is best to calibrate photometric redshifts with a set of spectroscopically-observed SNeIa with relatively more objects at high redshift than the parent sample of imaging SNeIa.

Andrew R. Zentner; Suman Bhattacharya

2008-12-01T23:59:59.000Z

216

Discovering the Nature of Dark Energy: Towards Better Distances from Type Ia Supernovae -- Final Technical Report  

SciTech Connect

Type Ia supernovae (SNe Ia; exploding white-dwarf stars) were the key to the Nobel-worthy 1998 discovery and subsequent verification that the expansion of the Universe is accelerating, driven by the effects of dark energy. Understanding the nature of this mysterious, yet dominant, component of the Universe is at the forefront of research in cosmology and fundamental physics. SNe Ia will continue to play a leading role in this enterprise, providing precise cosmological distances that improve constraints on the nature of dark energy. However, for this effort to succeed, we need to more thoroughly understand relatively nearby SNe Ia, because our conclusions come only from comparisons between them and distant (high-redshift) SNe Ia. Thus, detailed studies of relatively nearby SNe Ia are the focus of this research program. Many interesting results were obtained during the course of this project; these were published in 32 refereed research papers that acknowledged the grant. A major accomplishment was the publication of supernova (SN) rates derived from about a decade of operation of the Lick Observatory Supernova Search (LOSS) with the 0.76-meter Katzman Automatic Imaging Telescope (KAIT). We have determined the most accurate rates for SNe of different types in large, nearby galaxies in the present-day Universe, and these can be compared with SN rates far away (and hence long ago in the past) to set constraints on the types of stars that explode. Another major accomplishment was the publication of the light curves (brightness vs. time) of 165 SNe Ia, along with optical spectroscopy of many of these SNe as well as other SNe Ia, providing an extensive, homogeneous database for detailed studies. We have conducted intensive investigations of a number of individual SNe Ia, including quite unusual examples that allow us to probe the entire range of SN explosions and provide unique insights into these objects and the stars before they explode. My team's studies have also led to the identification of subsamples of SNe Ia that can be used to provide the most reliable cosmological distances, and we developed ways to deal with the dust that makes SNe Ia appear fainter than they really are. Using the KAIT/LOSS sample, we produced an excellent Hubble diagram (galaxy recession speed vs. distance), accurately showing the expansion of the Universe. Even smaller scatter was achieved when spectroscopic characteristics were taken into account. Another high-quality Hubble diagram was constructed with SNe Ia from the Sloan Digital Sky Survey (SDSS). These Hubble diagrams provide useful new constraints on the nature of the dark energy that is accelerating the expansion of the Universe. As an added bonus of our research, we also studied core-collapse SNe, which differ fundamentally from SNe Ia.

Filippenko, Alexei Vladimir [Univ. California, Berkeley

2014-05-09T23:59:59.000Z

217

Ed Jascevsky Safety Division ChIcago Operations Office MIT CONTFACT INFCE"ATION  

Office of Legacy Management (LM)

;/:4,4 (; . 1.; ;/:4,4 (; . 1.; e octo: ' J : 18, 1976 Ed Jascevsky Safety Division ChIcago Operations Office MIT CONTFACT INFCE"ATION During the discussions on October 8, 1976, you iquired about information relative to work done by MIT as background infomation for survey planning. The enclosed information is parephrased frorc an unpublished history of program work carried out by the Process Eevclopncnt Group of the Dl.ti,si.on of Raw Katerids, I believe this work was done under contract nuder AT(30-1)956. Robert IE. Allen Process Facilities Safety Branch Division of Safety, Standards, and Compliance Fnclosure: As stated I I . ..--@q$?.. .... ............................................ ........ ..- .......................... . ... ... .- ................... .._ ................ .... ..__ ..............

218

Microsoft PowerPoint - How To Do Business with DOE Chicago BOS Dec 14 2011.pptx  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Business Opportunities Session Business Opportunities Session Chicago, Illinois December 14, 2011 Office of Small and Disadvantaged Business Utilization (OSDBU) Office of Small and Disadvantaged Business Utilization (OSDBU) Office of Small and Disadvantaged Business Utilization (OSDBU) Office of Small and Disadvantaged Business Utilization (OSDBU) Presenter: Nickolas A. Demer Acquisition Team Leader December 14, 2011 EVOLUTION OF DOE EVOLUTION OF DOE EVOLUTION OF DOE EVOLUTION OF DOE Manhattan Project - August 1941 - Development of nuclear energy warheads Atomic Energy Act of 1946 - Established the Atomic Energy Commission (AEC) - Established the Atomic Energy Commission (AEC) - Civilian control of atomic energy weapons Atomic Energy Act of 1954 - Empowered AEC to also regulate commercial nuclear power industry

219

CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE  

SciTech Connect

We present multi-band optical photometry of 94 spectroscopically confirmed Type Ia supernovae (SNe Ia) in the redshift range 0.0055-0.073, obtained between 2006 and 2011. There are a total of 5522 light-curve points. We show that our natural-system SN photometry has a precision of {approx}< 0.03 mag in BVr'i', {approx}< 0.06 mag in u', and {approx}< 0.07 mag in U for points brighter than 17.5 mag and estimate that it has a systematic uncertainty of 0.014, 0.010, 0.012, 0.014, 0.046, and 0.073 mag in BVr'i'u'U, respectively. Comparisons of our standard-system photometry with published SN Ia light curves and comparison stars reveal mean agreement across samples in the range of {approx}0.00-0.03 mag. We discuss the recent measurements of our telescope-plus-detector throughput by direct monochromatic illumination by Cramer et al. This technique measures the whole optical path through the telescope, auxiliary optics, filters, and detector under the same conditions used to make SN measurements. Extremely well characterized natural-system passbands (both in wavelength and over time) are crucial for the next generation of SN Ia photometry to reach the 0.01 mag accuracy level. The current sample of low-z SNe Ia is now sufficiently large to remove most of the statistical sampling error from the dark-energy error budget. But pursuing the dark-energy systematic errors by determining highly accurate detector passbands, combining optical and near-infrared (NIR) photometry and spectra, using the nearby sample to illuminate the population properties of SNe Ia, and measuring the local departures from the Hubble flow will benefit from larger, carefully measured nearby samples.

Hicken, Malcolm; Challis, Peter; Kirshner, Robert P.; Bakos, Gaspar; Berlind, Perry; Brown, Warren R.; Caldwell, Nelson; Calkins, Mike; Falco, Emilio; Fernandez, Jose; Friedman, Andrew S.; Groner, Ted; Hartman, Joel [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Rest, Armin [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Cramer, Claire E. [NIST (National Institute of Standards and Technology), Gaithersburg, MD 20899 (United States); Wood-Vasey, W. Michael [Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States); Currie, Thayne [NASA, Goddard Space Flight Center, Greenbelt, MD 20771 (United States); De Kleer, Kathy [Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States); Esquerdo, Gil; Everett, Mark, E-mail: mhicken@cfa.harvard.edu [Planetary Science Institute, 1700 East Fort Lowell Road, Tucson, AZ 85719 (United States); and others

2012-06-01T23:59:59.000Z

220

IAS15: a fast, adaptive, high-order integrator for gravitational dynamics, accurate to machine precision over a billion orbits  

Science Journals Connector (OSTI)

......error behaves like a random walk. Our tests show that ias15 is superior to a mixed-variable...that ias15 follows Brouwer's law. We test our integrator in a wide variety of cases...focus on the two-body problem, a simple test case where we know the correct answer......

Hanno Rein; David S. Spiegel

2015-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

A U.S. Department of Energy laboratory managed by The University of Chicago ATLAS Call for Proposals  

E-Print Network (OSTI)

-energy and reaccelerated CARIBU beams available on target for the November 2013 PAC (posted at http://www.phy.anl.gov/atlas/facility and the instrumentation can be accommodated properly. Guy Savard Scientific Director of the ATLAS Facility PhysicsA U.S. Department of Energy laboratory managed by The University of Chicago ATLAS Call

Kemner, Ken

222

FROM RACKS TO POINTED HOPF ALGEBRAS AS ANDRUSKIEWITSCH AND MAT IAS GRA ~  

E-Print Network (OSTI)

FROM RACKS TO POINTED HOPF ALGEBRAS NICOL #19; AS ANDRUSKIEWITSCH AND MAT #19; IAS GRA ~ NA (C X; c q ), where X is a rack and q is a 2-cocycle on X with values in C #2; . Racks and cohomology of racks appeared also in the work of topologists. This leads us to the study of the structure of racks

Graña, Matías

223

Flames in Type Ia Supernova: Deflagration-Detonation Transition in the Oxygen Burning Flame  

E-Print Network (OSTI)

Flames in Type Ia Supernova: Deflagration-Detonation Transition in the Oxygen Burning Flame S. E of these regions can be supersonic and could initiate a detonation. Subject headings: supernovae: general a late time transition of the thermonuclear burning to a detonation wave (e.g., Hoflich et al. 1995

224

Section I. Summary of Project Activities Section I-A. 2008-2009 Project Summary  

E-Print Network (OSTI)

Section I. Summary of Project Activities Section I-A. 2008-2009 Project Summary University year, we accomplished the following: · Established a dual career opportunity procedure vetted to address, communicate procedures for the new daycare facility, and to explore the potential

Farritor, Shane

225

SEASONAL V A R IA TIONS IN STRUCTURE AND CIRCULATION IN THE RED SEA  

E-Print Network (OSTI)

SEASONAL V A R IA TIONS IN STRUCTURE AND CIRCULATION IN THE RED SEA A DISSERTATION SUBMITTE D and surface circulation in the Red Sea, occur r ing along the north-south axis of the Sea and extending fr om on in the northern Red Sea is frorn the nor th-northwest throughout the year' during the winter ( fr om October

Luther, Douglas S.

226

Seminar Ia, cetrti letnik, stari program LONGITUDINAL DYNAMICS OF PARTICLES IN ACCELERATORS  

E-Print Network (OSTI)

Seminar Ia, cetrti letnik, stari program LONGITUDINAL DYNAMICS OF PARTICLES IN ACCELERATORS Author motion of charged particles in particle accelerators. The technique of acceleration by electromagnetic waves is explored and the stability of motion under such acceleration is inspected. The seminar

?umer, Slobodan

227

Final Technical Report: Discovering the Nature of Dark Energy: Towards Better Distances from Type Ia Supernovae  

SciTech Connect

The final technical report from the project "Discovering the Nature of Dark Energy: Towards Better Distances from Type Ia Supernovae" led at Rutgers the State University of New Jersey by Prof. Saurabh W. Jha is presented, including all publications resulting from this award.

Saurabh W. Jha

2012-10-03T23:59:59.000Z

228

SponSored by http://www.ntu.edu.sg/ias/oCpA8  

E-Print Network (OSTI)

SponSored by http://www.ntu.edu.sg/ias/oCpA8 International Conference on physics education · Statistical and Nonlinear physics · Science Education · Women in Physics Sir Michael PEPPER Univ. College or poster presentations. All posters at the conference will be considered for the 2014 OCPA-APS Outstanding

Faraon, Andrei

229

THE CARNEGIE SUPERNOVA PROJECT: SECOND PHOTOMETRY DATA RELEASE OF LOW-REDSHIFT TYPE Ia SUPERNOVAE  

SciTech Connect

The Carnegie Supernova Project (CSP) was a five-year observational survey conducted at Las Campanas Observatory that obtained, among other things, high-quality light curves of {approx}100 low-redshift Type Ia supernovae (SNe Ia). Presented here is the second data release of nearby SN Ia photometry consisting of 50 objects, with a subset of 45 having near-infrared follow-up observations. Thirty-three objects have optical pre-maximum coverage with a subset of 15 beginning at least five days before maximum light. In the near-infrared, 27 objects have coverage beginning before the epoch of B-band maximum, with a subset of 13 beginning at least five days before maximum. In addition, we present results of a photometric calibration program to measure the CSP optical (uBgVri) bandpasses with an accuracy of {approx}1%. Finally, we report the discovery of a second SN Ia, SN 2006ot, similar in its characteristics to the peculiar SN 2006bt.

Stritzinger, Maximilian D. [The Oskar Klein Centre, Department of Astronomy, Stockholm University, AlbaNova, 10691 Stockholm (Sweden); Phillips, M. M.; Campillay, Abdo; Morrell, Nidia; Krzeminski, Wojtek; Roth, Miguel [Carnegie Observatories, Las Campanas Observatory, La Serena (Chile); Boldt, Luis N. [Argelander Institut fuer Astronomie, Universitaet Bonn, D-53111 Bonn (Germany); Burns, Chris; Freedman, Wendy L.; Madore, Barry F.; Persson, Sven E. [Observatories of the Carnegie Institution for Science, Pasadena, CA 91101 (United States); Contreras, Carlos [Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Victoria 3122 (Australia); Gonzalez, Sergio [Atacama Large Millimeter/Submillimeter Array, European Southern Observatory (Chile); Folatelli, Gaston [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Salgado, Francisco [Leiden Observatory, Leiden University, NL-2300 RA Leiden (Netherlands); DePoy, D. L.; Marshall, J. L.; Rheault, Jean-Philippe; Suntzeff, Nicholas B. [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843 (United States); Hamuy, Mario, E-mail: max.stritzinger@astro.su.se, E-mail: max@dark-cosmology.dk, E-mail: mstritzinger@lco.cl [Departamento de Astronomia, Universidad de Chile, Santiago (Chile)

2011-11-15T23:59:59.000Z

230

Abstract IA08: PTEN and PI3K signaling in brain development and disease  

Science Journals Connector (OSTI)

...Abstract IA08: PTEN and PI3K signaling in brain development and disease Suzanne J. Baker...an increased genetic susceptibility to brain tumors. However, inherited mutation of...and tumor suppression in the mammalian brain. Recently, germline or somatic mutations...

Suzanne J. Baker

2014-12-01T23:59:59.000Z

231

Turbulent Oxygen Flames in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

Turbulent Oxygen Flames in Type Ia Supernovae A. J. Aspden1 , J. B. Bell1 , and S. E. Woosley2 oxygen flames. The two aims of the paper are to examine the response of the inductive oxygen flame to intense levels of turbulence, and to explore the possibility of transition to detonation in the oxygen

232

The superconducting spin valve and triplet superconductivity I.A. Garifullin a,n  

E-Print Network (OSTI)

The superconducting spin valve and triplet superconductivity I.A. Garifullin a,n , P.V. Leksin s t r a c t A review of our recent results on the spin valve effect is presented. We have used coefficient DF and the exchange splitting I of the conduction band in the F layer [1]. For pure Fe the value

Fominov, Yakov

233

CIMAT, VIII Escuela de verano, 30 de julio -12 de ago* Introducci'on a la Geometr'ia de la Mec'ani*  

E-Print Network (OSTI)

con un valor fijo de la energ* *'ia corresponden a secciones del cono del inciso (a) por * *energ'ia tienen el mismo semi-eje mayor. 11.Demuestra la tercera ley de Kepler: toda soluci'on peri Introducci'on a la Geometr'ia de la Mec'ani* *ca Cl'asica Problemas 7 - 12

Bor, Gil

234

Steam System Balancing and Tuning for Multifamily Residential Buildings, Chicago, Illinois (Fact Sheet), Building America Case Study: Technology Solutions for New and Existing Homes, Building Technologies Office (BTO)  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Steam System Balancing Steam System Balancing and Tuning for Multifamily Residential Buildings Chicago, Illinois PROJECT INFORMATION Project Name: Steam System Balancing and Tuning for Multifamily Residential Buildings Location: Chicago, IL Partners: Partnership for Advanced Residential Retrofit www.gastechnology.org Building Component: Steam heating distribution system and controls Application: Retrofit; Multifamily Year Tested: 2011-2012 Applicable Climate Zone(s): Cold humid continental PERFORMANCE DATA Cost of Energy Efficiency Measure (including labor): $9,000 on average Projected Energy Savings: 10.2% heating savings Chicago's older multifamily housing stock is primarily heated by centrally metered steam or hydronic systems. Often, significant temperature differentials

235

ENERGY RESEARCH AND DEVELOPMENT ADMlNlSTRATldN CHICAGO OPERATIONS OFFICE  

Office of Legacy Management (LM)

RESEARCH AND DEVELOPMENT ADMlNlSTRATldN RESEARCH AND DEVELOPMENT ADMlNlSTRATldN CHICAGO OPERATIONS OFFICE 9999 SOUTH CASS AVENUE - .~-- ARGONNE, ILL!&+ bt.499 _ In Reply Refer TO: SEP. 1 61975 Martin B. Biles, Director Division of Operational Safety, HQ CARNEGIE-MELLON UNIVERSITY (CMU) CYCLOTRON DISMANTLING PROJECT The purpose of this memorandum is to summarize the dismantling activities which have been performed or are planned at the CMU, Nuclear Research Center, Saxonburg, Pennsylvania, site for purposes of preparing the site for unrestricted release from a radiological standpoint. Facility Description and Background Attachment 1 shows a schematic of the main building (which housed the synchrocyclotron, laboratories, machine shop, and offices) and adjacent ancillary facilities. Not shown (direction of location shown by arrows)

236

IA REP0 SAND85-2809 Unlimited Release UC-92A  

Office of Scientific and Technical Information (OSTI)

IA REP0 SAND85-2809 Unlimited Release UC-92A IA REP0 SAND85-2809 Unlimited Release UC-92A Printed July 1986 High Energy Gas Fracture Experiments in Fluid-Filled Boreholes-Potential Geothermal Application J. F. Cuderman, T. Y. Chu, J. Jung, R. D. Jacobson Prepared by Sandia National Laboratories Albuquerque, New Mexico 87 185 and Livermore, California 94550 for the United States Department of Energy under Contract DE-AC04-76DP00789 DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency Thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process

237

File:USDA-CE-Production-GIFmaps-IA.pdf | Open Energy Information  

Open Energy Info (EERE)

IA.pdf IA.pdf Jump to: navigation, search File File history File usage Iowa Ethanol Plant Locations Size of this preview: 776 × 600 pixels. Full resolution ‎(1,650 × 1,275 pixels, file size: 303 KB, MIME type: application/pdf) Description Iowa Ethanol Plant Locations Sources United States Department of Agriculture Related Technologies Biomass, Biofuels, Ethanol Creation Date 2010-01-19 Extent State Countries United States UN Region Northern America States Iowa External links http://www.nass.usda.gov/Charts_and_Maps/Ethanol_Plants/ File history Click on a date/time to view the file as it appeared at that time. Date/Time Thumbnail Dimensions User Comment current 16:13, 27 December 2010 Thumbnail for version as of 16:13, 27 December 2010 1,650 × 1,275 (303 KB) MapBot (Talk | contribs) Automated bot upload

238

Mechanistic studies of proton-coupled electron transfer in aminotyrosine- and fluorotyrosine- substituted class Ia Ribonucleotide reductase  

E-Print Network (OSTI)

Ribonucleotide reductase (RNR) catalyzes the conversion of nucleotides to 2'- deoxynucleotides in all organisms. The class Ia RNR from Escherichia coli is active as an a2p2 complex and utilizes an unprecedented mechanism ...

Minnihan, Ellen Catherine

2012-01-01T23:59:59.000Z

239

Generation of a stable, aminotyrosyl radical-induced ?2?2 complex of Escherichia coli class Ia ribonucleotide reductase  

E-Print Network (OSTI)

Ribonucleotide reductase (RNR) catalyzes the conversion of nucleoside diphosphates to deoxynucleoside diphosphates (dNDPs). The Escherichia coli class Ia RNR uses a mechanism of radical propagation by which a cysteine in ...

Minnihan, Ellen Catherine

240

IA --"-IScience Service Featuse 'I WHY T i E IJEAYIiER ?  

E-Print Network (OSTI)

No. 591 April 3 IA --"-IScience Service Featuse 'I WHY T i E IJEAYIiER ? II city located oa the Ice.pp';g a% Bidialo, The ice c h i l l s a t h i n laye:. of a i r aver the Sake aridto laewwd. NOW$ vhen r may be srrfficionl t o produce a sheet cloud and g i ~ eBuffalo a day not oalg dwnt arid chilly Lu

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

Especialista Universitario Java Enterprise 2010-2011 Depto. Ciencia de la Computacin e IA  

E-Print Network (OSTI)

Especialista Universitario Java Enterprise © 2010-2011 Depto. Ciencia de la Computación e IA Sesión 1: Introducción a JMS #12;Servicios de Mensajes con JMS © 2010-2011 Depto. Ciencia de la Computación · Una Aplicación JMS · PTP · Pub/Sub #12;Servicios de Mensajes con JMS © 2010-2011 Depto. Ciencia de la

Escolano, Francisco

242

On the Thermonuclear Runaway in Type Ia Supernovae: How to Run Away?  

Science Journals Connector (OSTI)

Type Ia supernovae (SNe Ia) are thought to be thermonuclear explosions of massive white dwarfs (WDs). We present the first study of multidimensional effects during the final hours prior to the thermonuclear runaway that leads to the explosion. The calculations utilize an implicit, two-dimensional hydrodynamic code. Mixing and the ignition process are studied in detail. We find that the initial chemical structure of the WD is changed, but the material is not fully homogenized. In particular, the exploding WD sustains a central region with a low C/O ratio. This implies that the explosive nuclear burning will begin in a partially carbon-depleted environment. The thermonuclear runaway happens in a well-defined region close to the center. It is induced by compressional heat when matter is brought inward by convective flows. We find no evidence for multiple spot or strong off-center ignition. Convective velocities in the WD are on the order of 100 km s-1, which is well above the effective burning speeds in SNe Ia previously expected right after the runaway. In our calculations, the ignition occurs near the center. Then, for ? 0.5-1 s, the speed of the burning front will neither be determined by the laminar speed nor the Rayleigh-Taylor instabilities but by convective flows produced prior to the runaway. The consequences are discussed for our understanding of the detailed physics of the flame propagation, the deflagration to detonation transition, and the nucleosynthesis in the central layers. Our results strongly suggest the preconditioning of the progenitor as a key factor for our understanding of the diversity in SNe Ia.

P. Hflich; J. Stein

2002-01-01T23:59:59.000Z

243

Testing the DistanceDuality Relation with Galaxy Clusters and Type Ia Supernovae  

Science Journals Connector (OSTI)

In this Letter, we propose a new and model-independent cosmological test for the distance-duality (DD) relation, ? = DL (z)(1 + z)2/DA (z) = 1, where DL and DA are, respectively, the luminosity and angular diameter distances. For DL we consider two sub-samples of Type Ia supernovae (SNe Ia) taken from Constitution data whereas DA distances are provided by two samples of galaxy clusters compiled by De Filippis etal. and Bonamente etal. by combining Sunyaev-Zeldovich effect and X-ray surface brightness. The SNe Ia redshifts of each sub-sample were carefully chosen to coincide with the ones of the associated galaxy cluster sample (?z DA (z) ? DL (z), we have tested the DD relation by assuming that ? is a function of the redshift parameterized by two different expressions: ?(z) = 1 + ?0 z and ?(z) = 1 + ?0 z/(1 + z), where ?0 is a constant parameter quantifying a possible departure from the strict validity of the reciprocity relation (?0 = 0). In the best scenario (linear parameterization), we obtain ?0 = 0.28+0.44 0.44 (2?, statistical + systematic errors) for the De Filippis etal. sample (elliptical geometry), a result only marginally compatible with the DD relation. However, for the Bonamente etal. sample (spherical geometry) the constraint is ?0 = 0.42+0.34 0.34 (3?, statistical + systematic errors), which is clearly incompatible with the duality-distance relation.

R. F. L. Holanda; J. A. S. Lima; M. B. Ribeiro

2010-01-01T23:59:59.000Z

244

Evaluation of copper for divider subassembly in MCO Mark IA and Mark IV scrap fuel baskets  

SciTech Connect

The K Basin Spent Nuclear Fuel (SNF) Project Multi-Canister Overpack (MCO) subprojection eludes the design and fabrication of a canister that will be used to confine, contain, and maintain fuel in a critically safe array to enable its removal from the K Basins, vacuum drying, transport, staging, hot conditioning, and interim storage (Goldinann 1997). Each MCO consists of a shell, shield plug, fuel baskets (Mark IA or Mark IV), and other incidental equipment. The Mark IA intact and scrap fuel baskets are a safety class item for criticality control and components necessary for criticality control will be constructed from 304L stainless steel. It is proposed that a copper divider subassembly be used in both Mark IA and Mark IV scrap baskets to increase the safety basis margin during cold vacuum drying. The use of copper would increase the heat conducted away from hot areas in the baskets out to the wall of the MCO by both radiative and conductive heat transfer means. Thus copper subassembly will likely be a safety significant component of the scrap fuel baskets. This report examines the structural, cost and corrosion consequences associated with using a copper subassembly in the stainless steel MCO scrap fuel baskets.

Graves, C.E.

1997-09-29T23:59:59.000Z

245

Observational constraints from SNe Ia and Gamma-Ray Bursts on a clumpy universe  

E-Print Network (OSTI)

The luminosity distance describing the effect of local inhomogeneities in the propagation of light proposed by Zeldovich-Kantowski-Dyer-Roeder (ZKDR) is tested with two probes for two distinct ranges of redshifts: supernovae Ia (SNe Ia) in 0.015 gamma-ray bursts (GRBs) in 1.547 < z < 3.57. Our analysis is performed by a Markov Chain Monte Carlo (MCMC) code that allows us to constrain the matter density parameter \\Omega_m as well as the smoothness parameter $\\alpha$ that measures the inhomogeneous-homogeneous rate of the cosmic fluid in a flat \\LambdaCDM model. The obtained best fits are (\\Omega_m=0.285^{+0.019}_{-0.018}, \\alpha= 0.856^{+0.106}_{-0.176}) from SNe Ia and (\\Omega_m=0.259^{+0.028}_{-0.028}, \\alpha=0.587^{+0.201}_{-0.202}) from GRBs, while from the joint analysis the best fits are (\\Omega_m=0.284^{+0.021}_{-0.020}, \\alpha= 0.685^{+0.164}_{-0.171}) with a \\chi^2_{\\rm red}=0.975. The value of the smoothness parameter $\\alpha$ indicates a clumped universe however it does not have an impact on the amount of dark energy (cosmological constant) needed to fit observations. This result may be an indication that the Dyer-Roeder approximation does not describe in a precise form the effects of clumpiness in the expansion of the universe.

Nora Bretn; Ariadna Montiel

2013-03-06T23:59:59.000Z

246

MRR 23 '94 B:44 FROM DOE-IPLD-CHICAGO TO RGCP-HQ OAGE.O00  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

23 '94 B:44 FROM DOE-IPLD-CHICAGO TO RGCP-HQ OAGE.O00 23 '94 B:44 FROM DOE-IPLD-CHICAGO TO RGCP-HQ OAGE.O00 * * STATEMENT OF CONSIDERATIONS REQUEST BY THE CARBORUNDUM COMPANY (CARBORUNDUM) FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN PATENT RIGHTS UNDER ITS SUBCONTRACT WITH SOLAR TURBINES INCORPORATED (SOLAR) UNDER DOE CONTRACT NUMBER DE-AC02-92CE40960; W(A)-93-027; CH-0784 The Carborundum Company (Carborundum), has requested a waiver of domestic and foreign patent rights for all subject inventions of its employees under a subcontract it expects to enter under DOE's prime contract with Solar Turbines Incorporated (Solar) for the development of a ceramic stationary gas turbine under contract No. DE-AC02-92CE40960. Carborundum is a wholly owned subsidiary of British Petroleum whose manufacturing and research and development facilities are located primarily in the

247

Especialista Universitario Java Enterprise Componentes de presentacin 2012-2013 Depto. Ciencia de la Computacin e IA Sesin 4  

E-Print Network (OSTI)

Especialista Universitario Java Enterprise Componentes de presentación © 2012-2013 Depto. Ciencia presentación © 2012-2013 Depto. Ciencia de la Computación e IA Sesión 4 Experto Universitario Java Enterprise Componentes de presentación © 2012-2013 Depto. Ciencia de la Computación e IA Sesión 4 Experto Universitario

Escolano, Francisco

248

Experto Universitario Java Enterprise Componentes de presentacin 2012-2013 Depto. Ciencia de la Computacin e IA Sesin 1  

E-Print Network (OSTI)

Experto Universitario Java Enterprise Componentes de presentación © 2012-2013 Depto. Ciencia de la Universitario Java Enterprise Componentes de presentación © 2012-2013 Depto. Ciencia de la Computación e IA Componentes de presentación © 2012-2013 Depto. Ciencia de la Computación e IA Sesión 1 Experto Universitario

Escolano, Francisco

249

Utilizing Type Ia Supernovae in a Large, Fast, Imaging Survey to Constrain Dark Energy  

Science Journals Connector (OSTI)

We study the utility of a large sample of Type Ia supernovae (SNe Ia) that might be observed in an imaging survey that rapidly scans a large fraction of the sky for constraining dark energy. We consider both the information contained in the traditional luminosity distance test as well as the spread in Ia SN fluxes at fixed redshift induced by gravitational lensing. As would be required from an imaging survey, we include a treatment of photometric redshift uncertainties in our analysis. Our primary result is that the information contained in the mean distance moduli of SNe Ia and the dispersion of SN Ia distance moduli complement each other, breaking a degeneracy between the present dark energy equation of state and its time variation without the need for a high-redshift (z 0.8) SN sample. Including lensing information also allows for some internal calibration of photometric redshifts. To address photometric redshift uncertainties, we present dark energy constraints as a function of the size of an external set of spectroscopically observed SNe that may be used for redshift calibration, N spec. Depending upon the details of potentially available, external SN data sets, we find that an imaging survey can constrain the dark energy equation of state at the epoch where it is best constrained w p, with a 1? error of ?(w p) ? 0.03-0.09. In addition, the marginal improvement in the error ?(w p) from an increase in the spectroscopic calibration sample drops once N spec ~ a few ? 103. This result is important because it is of the order of the size of calibration samples likely to be compiled in the coming decade and because, for samples of this size, the spectroscopic and imaging surveys individually place comparable constraints on the dark energy equation of state. In all cases, it is best to calibrate photometric redshifts with a set of spectroscopically observed SNe with relatively more objects at high redshift (z 0.5) than the parent sample of imaging SNe.

Andrew R. Zentner; Suman Bhattacharya

2009-01-01T23:59:59.000Z

250

Building America Case Study: Balancing Hydronic Systems in Multifamily Buildings, Chicago, Illinois (Fact Sheet)  

SciTech Connect

In multifamily hydronic systems, temperature imbalance may be caused by undersized piping, improperly adjusted balancing valves, inefficient water temperature and flow levels, and owner/occupant interaction with the boilers, distribution and controls. The effects of imbalance include tenant discomfort, higher energy use intensity and inefficient building operation. This paper explores cost-effective distribution upgrades and balancing measures in multifamily hydronic systems, providing a resource to contractors, auditors, and building owners on best practices to improve tenant comfort and lower operating costs. The research was conducted by The Partnership for Advanced Residential Retrofit (PARR) in conjunction with Elevate Energy. The team surveyed existing knowledge on cost-effective retrofits for optimizing distribution in typical multifamily hydronic systems, with the aim of identifying common situations and solutions, and then conducted case studies on two Chicago area buildings with known balancing issues in order to quantify the extent of temperature imbalance. At one of these buildings a booster pump was installed on a loop to an underheated wing of the building. This study found that unit temperature in a multifamily hydronic building can vary as much as 61 degrees F, particularly if windows are opened or tenants use intermittent supplemental heating sources like oven ranges. Average temperature spread at the building as a result of this retrofit decreased from 22.1 degrees F to 15.5 degrees F.

Not Available

2014-09-01T23:59:59.000Z

251

Health-hazard evaluation report HETA 82-309-1630, Inland Steel, East Chicago, Indiana  

SciTech Connect

Environmental and breathing-zone samples were analyzed for polynuclear aromatic hydrocarbons (PAHs) and coal-tar-pitch volatiles at the Inland Steel Company, East Chicago, Indiana in November, 1982 and September, 1984. The evaluation was requested because of concern about employee exposures during maintenance of the coke battery precipitator at the number 2 facility. Four former employees were interviewed. The cyclohexane soluble fraction of coal-tar-pitch volatiles ranged from 0.232 to 0.668 mg/m/sup 3/. The OSHA standard is 0.15mg/m/sup 3/. Naphthalene concentrations up to 0.107mg/m/sup 3/ were detected. The OSHA standard for naphthalene is 50mg/m/sup 3/. Other PAHs detected included phenanthrene, fluorene and acenaphthene. The employees reported experiencing local skin, eye, ear, nose, and throat irritation while working on the coke battery precipitator in the past. Personal protective measures such as wearing safety boots, barrier creams on exposed skin surfaces, and showering and changing clothes before leaving the facility were implemented. The authors conclude that a potential health hazard from PAHs and coal-tar-pitch volatiles is being adequately addressed by the facility. Recommendations include continuing the present personal protective measures and providing emergency rescue training.

Almaguer, D.; Orris, P.

1985-10-01T23:59:59.000Z

252

Building America Case Study: Advanced Boiler Load Monitoring Controllers, Chicago, Illinois (Fact Sheet)  

SciTech Connect

Beyond these initial system efficiency upgrades are an emerging class of Advanced Load Monitoring (ALM) aftermarket controllers that dynamically respond to the boiler load, with claims of 10% to 30% of fuel savings over a heating season. For hydronic boilers specifically, these devices perform load monitoring, with continuous measurement of supply and in some cases return water temperatures. Energy savings from these ALM controllers are derived from dynamic management of the boiler differential, where a microprocessor with memory of past boiler cycles prevents the boiler from firing for a period of time, to limit cycling losses and inefficient operation during perceived low load conditions. These differ from OTR controllers, which vary boiler setpoint temperatures with ambient conditions while maintaining a fixed differential. PARR installed and monitored the performance of one type of ALM controller, the M2G from Greffen Systems, at multifamily sites in the city of Chicago and its suburb Cary, IL, both with existing OTR control. Results show that energy savings depend on the degree to which boilers are over-sized for their load, represented by cycling rates. Also savings vary over the heating season with cycling rates, with greater savings observed in shoulder months. Over the monitoring period, over-sized boilers at one site showed reductions in cycling and energy consumption in line with prior laboratory studies, while less over-sized boilers at another site showed muted savings.

PARR

2014-09-01T23:59:59.000Z

253

The Chicago Center for Green Technology: life-cycle assessment of a brownfield redevelopment project  

Science Journals Connector (OSTI)

The sustainable development of brownfields reflects a fundamental, yet logical, shift in thinking and policymaking regarding pollution prevention. Life-cycle assessment (LCA) is a tool that can be used to assist in determining the conformity of brownfield development projects to the sustainability paradigm. LCA was applied to the process of a real brownfield redevelopment project, now known as the Chicago Center for Green Technology, to determine the cumulative energy required to complete the following redevelopment stages: (1)brownfield assessment and remediation, (2)building rehabilitation and site development and (3)ten years of operation. The results of the LCA have shown that operational energy is the dominant life-cycle stage after ten years of operation. The preservation and rehabilitation of the existing building, the installation of renewable energy systems (geothermal and photovoltaic) on-site and the use of more sustainable building products resulted in 72 terajoules (TJ) of avoided energy impacts, which would provide 14 years of operational energy for the site.

Thomas Brecheisen; Thomas Theis

2013-01-01T23:59:59.000Z

254

CIMAT, VI Escuela de verano, 25 de julio 7 de agosto 1999 Introducci'on a la Geometr'ia de la Mec'anica Cl'asica  

E-Print Network (OSTI)

parametrizada por (x(t); ?? x(t)): (d) Dibujar las gr'aficas de su energ'ia cin'etica T = ( ?? x) 2 =2 y potencial­ vaci'on de energ'ia, E = T + V = constante: (e) Repetir los 4 incisos anteriores con x(1) = 2; ?? x(0CIMAT, VI Escuela de verano, 25 de julio ­ 7 de agosto 1999 Introducci'on a la Geometr'ia de la Mec

Bor, Gil

255

CIMAT, VI Escuela de verano, 25 de julio -7 de agosto 1999 Introducci'on a la Geometr'ia de la Mec'anica Cl'asica  

E-Print Network (OSTI)

(t), `x(t)). (d)Dibujar las gr'aficas de su energ'ia cin'etica T = (x`)2=2 y potencial* * V = x2- vaci'on de energ'ia, E = T + V = constante. (e)Repetir los 4 incisos anteriores con x(1) = 2, `x CIMAT, VI Escuela de verano, 25 de julio - 7 de agosto 1999 Introducci'on a la Geometr'ia de la

Bor, Gil

256

Study of the Detonation Phase in the Gravitationally Confined Detonation Model of Type Ia Supernovae  

Science Journals Connector (OSTI)

We study the gravitationally confined detonation (GCD) model of Type Ia supernovae (SNe Ia) through the detonation phase and into homologous expansion. In the GCD model, a detonation is triggered by the surface flow due to single-point, off-center flame ignition in carbon-oxygen white dwarfs (WDs). The simulations are unique in terms of the degree to which nonidealized physics is used to treat the reactive flow, including weak reaction rates and a time-dependent treatment of material in nuclear statistical equilibrium (NSE). Careful attention is paid to accurately calculating the final composition of material which is burned to NSE and frozen out in the rapid expansion following the passage of a detonation wave over the high-density core of the WD; and an efficient method for nucleosynthesis postprocessing is developed which obviates the need for costly network calculations along tracer particle thermodynamic trajectories. Observational diagnostics are presented for the explosion models, including abundance stratifications and integrated yields. We find that for all of the ignition conditions studied here a self-regulating process comprised of neutronization and stellar expansion results in final 56Ni masses of ~1.1M ?. But, more energetic models result in larger total NSE and stable Fe-peak yields. The total yield of intermediate mass elements is ~0.1M ? and the explosion energies are all around 1.5 ? 1051 erg. The explosion models are briefly compared to the inferred properties of recent SN Ia observations. The potential for surface detonation models to produce lower-luminosity (lower 56Ni mass) SNe is discussed.

Casey A. Meakin; Ivo Seitenzahl; Dean Townsley; George C. Jordan IV; James Truran; Don Lamb

2009-01-01T23:59:59.000Z

257

IS WX CEN A POSSIBLE TYPE Ia SUPERNOVA PROGENITOR WITH WIND-DRIVEN MASS TRANSFER?  

SciTech Connect

WX Cen is one of a few compact binary supersoft X-ray sources (CBSS) in the Galaxy that is a possible Type Ia supernova (SN Ia) progenitor. The supersoft X-ray radiation is explained as hydrostatic nuclear burning on the surface of the white dwarf component that is accreting hydrogen from a stellar companion at a high rate. If the mass donor in this system has a low mass, as has been suggested in the literature, one would expect a high wind-driven mass transfer rate. In that case, the orbital period of the system should increase. To test this theoretical prediction, we have monitored the system photometrically since 2010. By using four newly determined eclipse timings together with those collected from the literature, we discovered that the orbital period is decreasing at a rate of dP/dt = -5.15 Multiplication-Sign 10{sup -7} days yr{sup -1}. The long-term decrease in the orbital period is contrary to the prediction that the system is powered by wind-driven accretion. It therefore seems plausible that the mass donor could be more massive than the white dwarf, and that the mass transfer is driven by the thermal instability of the donor star. This finding suggests that WX Cen is a key object to check the physical mechanisms of mass accretion in CBSS. The corresponding timescale of the period change is about P/P-dot {approx} 0.81 x 10{sup 6} yr, indicating that WX Cen may evolve into an SNe Ia within one million years in the Galaxy.

Qian, S.-B.; Shi, G.; Zhu, L.-Y.; Liu, L.; Zhao, E.-G.; Li, L.-J. [Yunnan Observatories, Chinese Academy of Sciences (CAS), P.O. Box 110, 650011 Kunming (China); Fernandez Lajus, E.; Di Sisto, R. P., E-mail: qsb@ynao.ac.cn [Facultad de Ciencias Astronomicas y Geofisicas, Universidad Nacional de La Plata, 1900 La Plata, Buenos Aires (Argentina)

2013-08-01T23:59:59.000Z

258

On the Thermonuclear Runaway in Type Ia Supernovae: How to run away?  

E-Print Network (OSTI)

Type Ia Supernovae are thought to be thermonuclear explosions of massive white dwarfs (WD). We present the first study of multi-dimensional effects during the final hours prior to the thermonuclear runaway which leads to the explosion. The calculations utilize an implicit, 2-D hydro code.Mixing and the ignition process are studied in detail. We find that the initial chemical structure of the WD is changed but the material is not fully homogenized. The exploding WD sustains a central region with a low C/O ratio. This implies that the explosive nuclear burning will begin in a partially C-depleted environment. The thermonuclear runaway happens in a well defined region close to the center. It is induced by compressional heat when matter is brought inwards by convective flows. We find no evidence for multiple spot or strong off-center ignition. Convective velocities are of the order of 100 km/sec which is well above the effective burning speeds in SNe Ia previously expected right after the runaway. For about 0.5 to 1 sec, the speed of the burning front will neither be determined by the laminar speed nor the Rayleigh-Taylor instabilities but by convective flows produced prior to the runaway. The consequences are discussed for our under- standing of the detailed physics of the flame propagation, the deflagration detonation transition, and the nucleosynthesis in the central layers. Our results strongly suggest the pre-conditioning of the progenitor as a key-factor for our understanding of the diversity in SNeIa.

P. Hoeflich; J. Stein

2001-12-07T23:59:59.000Z

259

Reconstruction of Hessence Dark Energy and the Latest Type Ia Supernovae Gold Dataset  

E-Print Network (OSTI)

Recently, many efforts have been made to build dark energy models whose equation-of-state parameter can cross the so-called phantom divide $w_{de}=-1$. One of them is the so-called hessence dark energy model in which the role of dark energy is played by a non-canonical complex scalar field. In this work, we develop a simple method based on Hubble parameter $H(z)$ to reconstruct the hessence dark energy. As examples, we use two familiar parameterizations for $H(z)$ and fit them to the latest 182 type Ia supernovae Gold dataset. In the reconstruction, measurement errors are fully considered.

Hao Wei; Ningning Tang; Shuang Nan Zhang

2007-02-28T23:59:59.000Z

260

Reconstruction of a Deceleration Parameter from the Latest Type Ia Supernovae Gold Dataset  

E-Print Network (OSTI)

In this paper, a parameterized deceleration parameter $q(z)= 1/2 - a/(1 + z)^b$ is reconstructed from the latest type Ia supernovae gold dataset. It is found out that the transition redshift from decelerated expansion to accelerated expansion is at $z_T=0.35^{+0.14}_{-0.07}$ with $1\\sigma$ confidence level in this parameterized deceleration parameter. And, the best fit values of parameters in $1\\sigma$ errors are $a=1.56^{+0.99}_{-0.55}$ and $b=3.82^{+3.70}_{-2.27}$.

Lixin Xu; Chengwu Zhang; Baorong Chang; Hongya Liu

2007-01-17T23:59:59.000Z

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

On the Stability of Thermonuclear Burning Fronts in Type Ia Supernovae  

E-Print Network (OSTI)

The propagation of cellularly stabilized thermonuclear flames is investigated by means of numerical simulations. In Type Ia supernova explosions the corresponding burning regime establishes at scales below the Gibson length. The cellular flame stabilization - which is a result of an interplay between the Landau-Darrieus instability and a nonlinear stabilization mechanism - is studied for the case of propagation into quiescent fuel as well as interaction with vortical fuel flows. Our simulations indicate that in thermonuclear supernova explosions stable cellular flames develop around the Gibson scale and that deflagration-to-detonation transition is unlikely to be triggered from flame evolution effects here.

F. K. Roepke; W. Hillebrandt

2004-04-26T23:59:59.000Z

262

Unbiased Estimate of Dark Energy Density from Type Ia Supernova Data  

Science Journals Connector (OSTI)

Type Ia supernovae (SNe Ia) are currently the best probes of the dark energy in the universe. To constrain the nature of dark energy, we assume a flat universe and that the weak energy condition is satisfied, and we allow the density of dark energy, ?X(z), to be an arbitrary function of redshift. Using simulated data from a space-based SN pencil-beam survey, we find that by optimizing the number of parameters used to parameterize the dimensionless dark energy density, f(z) = ?X(z)/?X(z = 0), we can obtain an unbiased estimate of both f(z) and the fractional matter density of the universe, ?m. A plausible SN pencil-beam survey (with a square degree field of view and for an observational duration of 1 yr) can yield about 2000 SNe Ia with 0 ? z ? 2. Such a survey in space would yield SN peak luminosities with a combined intrinsic and observational dispersion of ?(mint) = 0.16 mag. We find that for such an idealized survey, ?m can be measured to 10% accuracy, and the dark energy density can be estimated to ~20% to z ~ 1.5, and ~20%-40% to z ~ 2, depending on the time dependence of the true dark energy density. Dark energy densities that vary more slowly can be more accurately measured. For the anticipated Supernova/Acceleration Probe (SNAP) mission, ?m can be measured to 14% accuracy, and the dark energy density can be estimated to ~20% to z ~ 1.2. Our results suggest that SNAP may gain much sensitivity to the time dependence of the dark energy density and ?m by devoting more observational time to the central pencil-beam fields to obtain more SNe Ia at z > 1.2. We use both a maximum likelihood analysis and a Monte Carlo analysis (when appropriate) to determine the errors of estimated parameters. We find that the Monte Carlo analysis gives a more accurate estimate of the dark energy density than the maximum likelihood analysis.

Yun Wang; Geoffrey Lovelace

2001-01-01T23:59:59.000Z

263

One-dimensional delayed-detonation models of Type Ia supernovae: Confrontation to observations at bolometric maximum  

E-Print Network (OSTI)

The delayed-detonation explosion mechanism applied to a Chandrasekhar-mass white dwarf offers a very attractive model to explain the inferred characteristics of Type Ia supernovae (SNe Ia). The resulting ejecta are chemically stratified, have the same mass and roughly the same asymptotic kinetic energy, but exhibit a range in 56Ni mass. We investigate the contemporaneous photometric and spectroscopic properties of a sequence of delayed-detonation models, characterized by 56Ni masses between 0.18 and 0.81 Msun. Starting at 1d after explosion, we perform the full non-LTE, time-dependent radiative transfer with the code CMFGEN, with an accurate treatment of line blanketing, and compare our results to SNe Ia at bolometric maximum. Despite the 1D treatment, our approach delivers an excellent agreement to observations. We recover the range of SN Ia luminosities, colours, and spectral characteristics from the near-UV to 1 micron, for standard as well as low-luminosity 91bg-like SNe Ia. Our models predict an increase...

Blondin, Stphane; Hillier, D John; Khokhlov, Alexei M

2012-01-01T23:59:59.000Z

264

The p-Process in the Carbon Deflagration Model for Type Ia Supernovae and Chronology of the Solar System Formation  

SciTech Connect

We study nucleosynthesis of p-nuclei in the carbon deflagration model for Type Ia supernovae (SNe Ia) by assuming that seed nuclei are produced by the s-process in accreting layers on a carbon-oxygen white dwarf during mass accretion from a binary companion. We find that about 50 % of the p-nuclides are synthesized in proportion to the solar abundance and that p-isotopes of Mo and Ru which are significantly underproduced in Type II supernovae (SNe II) are produced up to a level close to other p-nuclei. Comparing the yields of iron and p-nuclei in SNe Ia we find that SNe Ia can contribute to the galactic evolution of the p-nuclei. Next, we consider nucleochronology of the solar system formation by using four radioactive nuclides and apply the result of the p-process nucleosynthesis to simple galactic chemical evolution models. We find that when assumed three phases of interstellar medium are mixed by the interdiffusion with the timescale of about 40 Myr 53Mn/55Mn value in the early solar system is consistent with a meteoritic value. In addition, we put constraints to a scenario that SNe Ia induce the core collapse of the molecular cloud, which leads to the formation of the solar system.

Kusakabe, Motohiko [Department of Astronomy, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan); Iwamoto, Nobuyuki [Japan Atomic Energy Agency, Tokai, Ibaraki 319-1195 (Japan); Nomoto, Ken'ichi [Department of Astronomy, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)

2006-07-12T23:59:59.000Z

265

Stable isotope-assisted NMR characterization of interaction between lipid A and sarcotoxin IA, a cecropin-type antibacterial peptide  

SciTech Connect

Highlights: ? Recombinant sarcotoxin IA was successfully produced with {sup 13}C- and {sup 15}N-labeling. ? Sarcotoxin IA adopts an N-terminal ?-helix upon binding to lipid A-embedding micelles. ? Two lysine residues are involved in lipid A-mediated antibacterial activities. -- Abstract: Sarcotoxin IA is a 39-residue cecropin-type peptide from Sarcophaga peregrina. This peptide exhibits antibacterial activity against Gram-negative bacteria through its interaction with lipid A, a core component of lipopolysaccharides. To acquire detailed structural information on this specific interaction, we performed NMR analysis using bacterially expressed sarcotoxin IA analogs with {sup 13}C- and {sup 15}N-labeling along with lipid A-embedding micelles composed of dodecylphosphocholine. By inspecting the stable isotope-assisted NMR data, we revealed that the N-terminal segment (Leu3Arg18) of sarcotoxin IA formed an amphiphilic ?-helix upon its interaction with the aqueous micelles. Furthermore, chemical shift perturbation data indicated that the amino acid residues displayed on this ?-helix were involved in the specific interaction with lipid A. On the basis of these data, we successfully identified Lys4 and Lys5 as key residues in the interaction with lipid A and the consequent antibacterial activity. Therefore, these results provide unique information for designing chemotherapeutics based on antibacterial peptide structures.

Yagi-Utsumi, Maho [Institute for Molecular Science and Okazaki Institute for Integrative Bioscience, National Institutes of Natural Sciences, Okazaki 444-8787 (Japan) [Institute for Molecular Science and Okazaki Institute for Integrative Bioscience, National Institutes of Natural Sciences, Okazaki 444-8787 (Japan); Graduate School of Pharmaceutical Sciences, Nagoya City University, Nagoya 467-8603 (Japan); Yamaguchi, Yoshiki [Graduate School of Pharmaceutical Sciences, Nagoya City University, Nagoya 467-8603 (Japan) [Graduate School of Pharmaceutical Sciences, Nagoya City University, Nagoya 467-8603 (Japan); Advanced Science Institute, RIKEN, Wako 351-0198 (Japan); Boonsri, Pornthip [Institute for Molecular Science and Okazaki Institute for Integrative Bioscience, National Institutes of Natural Sciences, Okazaki 444-8787 (Japan) [Institute for Molecular Science and Okazaki Institute for Integrative Bioscience, National Institutes of Natural Sciences, Okazaki 444-8787 (Japan); Department of Chemistry, Faculty of Science, Kasetsart University, Bangkok 10900 (Thailand); Iguchi, Takeshi [Bioscience Research Laboratory, Fujiya Co., Ltd., Hadano, Kanagawa 257-0031 (Japan)] [Bioscience Research Laboratory, Fujiya Co., Ltd., Hadano, Kanagawa 257-0031 (Japan); Okemoto, Kazuo [Department of Biochemistry and Cell Biology, National Institute of Infectious Disease, Tokyo 162-8640 (Japan)] [Department of Biochemistry and Cell Biology, National Institute of Infectious Disease, Tokyo 162-8640 (Japan); Natori, Shunji [National Institute of Agrobiological Sciences, Tsukuba 305-8602 (Japan)] [National Institute of Agrobiological Sciences, Tsukuba 305-8602 (Japan); Kato, Koichi, E-mail: kkatonmr@ims.ac.jp [Institute for Molecular Science and Okazaki Institute for Integrative Bioscience, National Institutes of Natural Sciences, Okazaki 444-8787 (Japan) [Institute for Molecular Science and Okazaki Institute for Integrative Bioscience, National Institutes of Natural Sciences, Okazaki 444-8787 (Japan); Graduate School of Pharmaceutical Sciences, Nagoya City University, Nagoya 467-8603 (Japan); The Glycoscience Institute, Ochanomizu University, Tokyo 135-0064 (Japan); GLYENCE Co., Ltd., Nagoya 474-0858 (Japan)

2013-02-08T23:59:59.000Z

266

The influence of coyotes on an urban Canada goose population in the Chicago metropolitan area  

SciTech Connect

Canada geese (Branta canadensis) have become common in many urban areas, often creating nuisance problems for human residents. The presence of urban geese has raised concerns about the spread of disease, increased erosion, excessive noise, eutrophication of waterways, and general nuisance problems. Goose populations have grown due to an increase in urbanization resulting in an abundance of high quality food (urban grass) and suitable nesting sites, as well as a decrease in some predators. I monitored nest predation in the Chicago suburbs during the 2004 and 2005 nesting seasons using 3 nest monitoring techniques to identify predators: video cameras, plasticine eggs, and sign from nest using a classification tree analysis. Of 58 nests monitored in 2004 and 286 in 2005, only raccoons (Procyon lotor) and coyotes (Canis latrans) were identified as nest predators. Raccoons were responsible for 22-25% of depredated nests, but were rarely capable of depredating nests that were actively defended by a goose. Coyotes were responsible for 75-78% of all Canada goose nest depredation and were documented killing one adult goose and feeding on several others. The coyote is a top-level predator that had increased in many metropolitan areas in recent years. To determine if coyotes were actively hunting geese or eggs during the nesting season, I analyzed coyote habitat selection between nesting and pre-nesting or post-nesting seasons. Coyote home ranges (95% Minimum Convex Polygon) were calculated for 19 coyotes to examine third order habitat selection related to goose nest abundance. A 100 m buffer (buffer habitat) was created and centered on each waterway edge and contained 90% of all nests. Coyotes showed selection for habitats during all seasons. Buffer habitat was the top ranked habitat in both pre-nesting and nesting seasons, but dropped to third ranked in post-nesting season. Habitat selection across seasons was compared using a repeated measures MANOVA. Habitat selection between pre-nesting and nesting seasons (P=0.72) were similar, while between post-nesting and nesting seasons there was a nearly significant difference (P=0.07). The insignificant change in habitat use across seasons suggests that coyotes did not switch habitat use to take advantage of goose nests. Alternatively, the change in ranking of buffer habitat across seasons suggests that coyotes may have switched habitat use to take advantage of goose nests. The results are not clear as large individual variation between coyotes due to differences in habitat availability, and social status interfere with the results of the analysis. Even though I failed to find strong support for coyotes actively hunting goose nests, they nevertheless were the primary nest predator in the area and may influence Canada goose populations. To determine the potential influence of coyotes on the Canada goose population, I created a Canada goose matrix population model that included variables such as coyote predation on adults and nests as well as coyote influence on nest desertion. Using the base population model I calculated the Canada goose population to be increasing with {lambda} = 1.055. The removal of all coyote influence on the goose population would allow {lambda} to increase to 1.214. Nest predation was the most important factor related to coyotes: the removal of coyote nest predation from the model resulted in a population growth rate {lambda} = 1.157. Modeling results suggest coyotes are serving as a limiting factor for the Canada goose population within the Chicago metropolitan area.

Brown, Justin L.; /Ohio State U.

2007-01-01T23:59:59.000Z

267

Inference for the dark energy equation of state using Type IA supernova data  

E-Print Network (OSTI)

The surprising discovery of an accelerating universe led cosmologists to posit the existence of "dark energy"--a mysterious energy field that permeates the universe. Understanding dark energy has become the central problem of modern cosmology. After describing the scientific background in depth, we formulate the task as a nonlinear inverse problem that expresses the comoving distance function in terms of the dark-energy equation of state. We present two classes of methods for making sharp statistical inferences about the equation of state from observations of Type Ia Supernovae (SNe). First, we derive a technique for testing hypotheses about the equation of state that requires no assumptions about its form and can distinguish among competing theories. Second, we present a framework for computing parametric and nonparametric estimators of the equation of state, with an associated assessment of uncertainty. Using our approach, we evaluate the strength of statistical evidence for various competing models of dark energy. Consistent with current studies, we find that with the available Type Ia SNe data, it is not possible to distinguish statistically among popular dark-energy models, and that, in particular, there is no support in the data for rejecting a cosmological constant. With much more supernova data likely to be available in coming years (e.g., from the DOE/NASA Joint Dark Energy Mission), we address the more interesting question of whether future data sets will have sufficient resolution to distinguish among competing theories.

Christopher Genovese; Peter Freeman; Larry Wasserman; Robert Nichol; Christopher Miller

2008-05-27T23:59:59.000Z

268

Flame-driven deflagration-to-detonation transitions in Type Ia supernovae?  

E-Print Network (OSTI)

Although delayed detonation models of thermonuclear explosions of white dwarfs seem promising for reproducing Type Ia supernovae, the transition of the flame propagation mode from subsonic deflagration to supersonic detonation remains hypothetical. A potential instant for this transition to occur is the onset of the distributed burning regime, i.e. the moment when turbulence first affects the internal flame structure. Some studies of the burning microphysics indicate that a deflagration-to-detonation transition may be possible here, provided the turbulent intensities are strong enough. Consequently, the magnitude of turbulent velocity fluctuations generated by the deflagration flame is analyzed at the onset of the distributed burning regime in several three-dimensional simulations of deflagrations in thermonuclear supernovae. It is shown that the corresponding probability density functions fall off towards high turbulent velocity fluctuations much more slowly than a Gaussian distribution. Thus, values claimed to be necessary for triggering a detonation are likely to be found in sufficiently large patches of the flame. Although the microphysical evolution of the burning is not followed and a successful deflagration-to-detonation transition cannot be guaranteed from simulations presented here, the results still indicate that such events may be possible in Type Ia supernova explosions.

F. K. Roepke

2007-09-26T23:59:59.000Z

269

Flame Evolution During Type Ia Supernovae and the Deflagration Phase in the Gravitationally Confined Detonation Scenario  

E-Print Network (OSTI)

We develop an improved method for tracking the nuclear flame during the deflagration phase of a Type Ia supernova, and apply it to study the variation in outcomes expected from the gravitationally confined detonation (GCD) paradigm. A simplified 3-stage burning model and a non-static ash state are integrated with an artificially thickened advection-diffusion-reaction (ADR) flame front in order to provide an accurate but highly efficient representation of the energy release and electron capture in and after the unresolvable flame. We demonstrate that both our ADR and energy release methods do not generate significant acoustic noise, as has been a problem with previous ADR-based schemes. We proceed to model aspects of the deflagration, particularly the role of buoyancy of the hot ash, and find that our methods are reasonably well-behaved with respect to numerical resolution. We show that if a detonation occurs in material swept up by the material ejected by the first rising bubble but gravitationally confined to the white dwarf (WD) surface (the GCD paradigm), the density structure of the WD at detonation is systematically correlated with the distance of the deflagration ignition point from the center of the star. Coupled to a suitably stochastic ignition process, this correlation may provide a plausible explanation for the variety of nickel masses seen in Type Ia Supernovae.

D. M. Townsley; A. C. Calder; S. M. Asida; I. R. Seitenzahl; F. Peng; N. Vladimirova; D. Q. Lamb; J. W. Truran

2007-06-07T23:59:59.000Z

270

Constraining a bulk viscous matter-dominated cosmological model using SNe Ia, CMB and LSS  

E-Print Network (OSTI)

We present and constrain a cosmological model which component is a pressureless fluid with bulk viscosity as an explanation for the present accelerated expansion of the universe. We study the particular model of a constant bulk viscosity coefficient \\zeta_m. The possible values of \\zeta_m are constrained using the cosmological tests of SNe Ia Gold 2006 sample, the CMB shift parameter R from the three-year WMAP observations, the Baryon Acoustic Oscillation (BAO) peak A from the Sloan Digital Sky Survey (SDSS) and the Second Law of Thermodynamics (SLT). It was found that this model is in agreement with the SLT using only the SNe Ia test. However when the model is submitted to the three cosmological tests together (SNe+CMB+BAO) the results are: 1.- the model violates the SLT, 2.- predicts a value of H_0 \\approx 53 km sec^{-1} Mpc^{-1} for the Hubble constant, and 3.- we obtain a bad fit to data with a \\chi^2_{min} \\approx 400 (\\chi^2_{d.o.f.} \\approx 2.2). These results indicate that this model is ruled out by the observations.

Arturo Avelino; U. Nucamendi; F. S. Guzmn

2008-01-10T23:59:59.000Z

271

Parametrizing the transition to the phantom epoch with Supernovae Ia and Standard Rulers  

E-Print Network (OSTI)

The properties of some particular parametrizations of the dark energy Equation of State (EoS) are studied by using Supernovae Ia data (HST Cluster Supernova Survey) combined with Standard Ruler datasets (Cosmic Microwave Background (CMB) and Baryon Acoustic Oscillations (BAO)). In this sense, we propose some parametrizations that may present a (fast) transition to a phantom dark energy EoS (where $w_{DE}<-1$) and compare the results with the $\\Lambda$CDM model. The best fit of the models is obtained by using Sne Ia and Standard Ruler datasets, which provides some information about whether the phantom transition may be supported by the observations. In this regard, the crossing of the phantom barrier is allowed statistically but the occurrence of a future singularity seems unlikely. Furthermore, the reconstruction of a (non-)canonical scalar field Lagrangian from the EoS parameter is studied, where shown that EoS parametrizations can be well reconstructed in terms of scalar fields.

Leanizbarrutia, Iker

2014-01-01T23:59:59.000Z

272

Verifying the Cosmological Utility of Type Ia Supernovae:Implications of a Dispersion in the Ultraviolet Spectra  

SciTech Connect

We analyze the mean rest-frame ultraviolet (UV) spectrum ofType Ia Supernovae(SNe) and its dispersion using high signal-to-noiseKeck-I/LRIS-B spectroscopyfor a sample of 36 events at intermediateredshift (z=0.5) discoveredby the Canada-France-Hawaii TelescopeSupernova Legacy Survey (SNLS). Weintroduce a new method for removinghost galaxy contamination in our spectra,exploiting the comprehensivephotometric coverage of the SNLS SNe and theirhost galaxies, therebyproviding the first quantitative view of the UV spectralproperties of alarge sample of distant SNe Ia. Although the mean SN Ia spectrumhas notevolved significantly over the past 40 percent of cosmic history,preciseevolutionary constraints are limited by the absence of acomparable sample ofhigh quality local spectra. The mean UV spectrum ofour z 0.5 SNe Ia and itsdispersion is tabulated for use in futureapplications. Within the high-redshiftsample, we discover significant UVspectral variations and exclude dust extinctionas the primary cause byexamining trends with the optical SN color. Although progenitormetallicity may drive some of these trends, the variations we see aremuchlarger than predicted in recent models and do not follow expectedpatterns.An interesting new result is a variation seen in the wavelengthof selected UVfeatures with phase. We also demonstrate systematicdifferences in the SN Iaspectral features with SN lightcurve width inboth the UV and the optical. Weshow that these intrinsic variations couldrepresent a statistical limitation in thefuture use of high-redshift SNeIa for precision cosmology. We conclude thatfurther detailed studies areneeded, both locally and at moderate redshift wherethe rest-frame UV canbe studied precisely, in order that future missions canconfidently beplanned to fully exploit SNe Ia as cosmological probes.

Ellis, R.S.; Sullivan, M.; Nugent, P.E.; Howell, D.A.; Gal-Yam,A.; Astier, P.; Balam, D.; Balland, C.; Basa, S.; Carlberg, R.G.; Conley,A.; Fouchez, D.; Guy, J.; Hardin, D.; Hook, I.; Pain, R.; Perrett, K.; Pritchet, C.J.; Regnault, N.

2007-11-02T23:59:59.000Z

273

CIMAT, VIII Escuela de verano, 30 de julio -10 de ago* Introducci'on a la Geometr'ia de la Mec'ani*  

E-Print Network (OSTI)

conservativo. 18.Sea A(E) el 'area dentro de una curva de fase cerrada que corresponde a nive* *l de energ'ia Introducci'on a la Geometr'ia de la Mec'ani* *ca Cl'asica Problemas 13 - 19

Bor, Gil

274

LATE-TIME SPECTRAL OBSERVATIONS OF THE STRONGLY INTERACTING TYPE Ia SUPERNOVA PTF11kx  

SciTech Connect

PTF11kx was a Type Ia supernova (SN Ia) that showed time-variable absorption features, including saturated Ca II H and K lines that weakened and eventually went into emission. The strength of the emission component of H{alpha} gradually increased, implying that the SN was undergoing significant interaction with its circumstellar medium (CSM). These features, and many others, were blueshifted slightly and showed a P-Cygni profile, likely indicating that the CSM was directly related to, and probably previously ejected by, the progenitor system itself. These and other observations led Dilday et al. to conclude that PTF11kx came from a symbiotic nova progenitor like RS Oph. In this work we extend the spectral coverage of PTF11kx to 124-680 rest-frame days past maximum brightness. The late-time spectra of PTF11kx are dominated by H{alpha} emission (with widths of full width at half-maximum intensity Almost-Equal-To 2000 km s{sup -1}), strong Ca II emission features ({approx}10,000 km s{sup -1} wide), and a blue 'quasi-continuum' due to many overlapping narrow lines of Fe II. Emission from oxygen, He I, and Balmer lines higher than H{alpha} is weak or completely absent at all epochs, leading to large observed H{alpha}/H{beta} intensity ratios. The H{alpha} emission appears to increase in strength with time for {approx}1 yr, but it subsequently decreases significantly along with the Ca II emission. Our latest spectrum also indicates the possibility of newly formed dust in the system as evidenced by a slight decrease in the red wing of H{alpha}. During the same epochs, multiple narrow emission features from the CSM temporally vary in strength. The weakening of the H{alpha} and Ca II emission at late times is possible evidence that the SN ejecta have overtaken the majority of the CSM and agrees with models of other strongly interacting SNe Ia. The varying narrow emission features, on the other hand, may indicate that the CSM is clumpy or consists of multiple thin shells.

Silverman, Jeffrey M. [Department of Astronomy, University of Texas, Austin, TX 78712-0259 (United States); Nugent, Peter E.; Filippenko, Alexei V.; Cenko, S. Bradley [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Gal-Yam, Avishay [Benoziyo Center for Astrophysics, The Weizmann Institute of Science, Rehovot 76100 (Israel); Sullivan, Mark [School of Physics and Astronomy, University of Southampton, Southampton SO17 1BJ (United Kingdom); Howell, D. Andrew [Las Cumbres Observatory Global Telescope Network, Goleta, CA 93117 (United States); Pan, Yen-Chen; Hook, Isobel M., E-mail: jsilverman@astro.as.utexas.edu [Department of Physics (Astrophysics), University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom)

2013-08-01T23:59:59.000Z

275

Type Ia supernova diversity: white dwarf central density as a secondary parameter in three-dimensional delayed detonation models  

Science Journals Connector (OSTI)

......function of redshift. The standard model of SNe Ia relies on the nuclear fusion of the initial composition (predominantly 12C and 16O) of...generated from a Monte Carlo based algorithm. The primary input parameters are the number of the ignition kernels and the......

I. R. Seitenzahl; F. Ciaraldi-Schoolmann; F. K. Rpke

2011-07-01T23:59:59.000Z

276

EARLY RADIO AND X-RAY OBSERVATIONS OF THE YOUNGEST NEARBY TYPE Ia SUPERNOVA PTF 11kly (SN 2011fe)  

SciTech Connect

On 2011 August 24 (UT) the Palomar Transient Factory (PTF) discovered PTF11kly (SN 2011fe), the youngest and most nearby Type Ia supernova (SN Ia) in decades. We followed this event up in the radio (centimeter and millimeter bands) and X-ray bands, starting about a day after the estimated explosion time. We present our analysis of the radio and X-ray observations, yielding the tightest constraints yet placed on the pre-explosion mass-loss rate from the progenitor system of this supernova. We find a robust limit of M-dot {approx}<10{sup -8}(w/100 km s{sup -1}) M{sub sun} yr{sup -1} from sensitive X-ray non-detections, as well as a similar limit from radio data, which depends, however, on assumptions about microphysical parameters. We discuss our results in the context of single-degenerate models for SNe Ia and find that our observations modestly disfavor symbiotic progenitor models involving a red giant donor, but cannot constrain systems accreting from main-sequence or sub-giant stars, including the popular supersoft channel. In view of the proximity of PTF11kly and the sensitivity of our prompt observations, we would have to wait for a long time (a decade or longer) in order to more meaningfully probe the circumstellar matter of SNe Ia.

Horesh, Assaf; Kulkarni, S. R.; Carpenter, John; Kasliwal, Mansi M.; Ofek, Eran O. [Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Fox, Derek B. [Astronomy and Astrophysics, Eberly College of Science, Pennsylvania State University, University Park, PA 16802 (United States); Quimby, Robert [IPMU, University of Tokyo, Kashiwanoha 5-1-5, Kashiwa-shi, Chiba (Japan); Gal-Yam, Avishay [Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100 (Israel); Cenko, S. Bradley [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); De Bruyn, A. G. [Netherlands Institute for Radio Astronomy (ASTRON), Postbus 2, NL-7990 AA Dwingeloo (Netherlands); Kamble, Atish; Wijers, Ralph A. M. J. [Center for Gravitation and Cosmology, University of Wisconsin, Milwaukee, WI 53211 (United States); Van der Horst, Alexander J. [Universities Space Research Association, NSSTC, Huntsville, AL 35805 (United States); Kouveliotou, Chryssa [Space Science Office, VP-62, NASA-Marshall Space Flight Center, Huntsville, AL 35805 (United States); Podsiadlowski, Philipp; Sullivan, Mark; Maguire, Kate [Department of Physics (Astrophysics), University of Oxford, Keble Road, Oxford OX1 3RH (United Kingdom); Howell, D. Andrew [Las Cumbres Observatory Global Telescope Network, Santa Barbara, CA 93117 (United States); Nugent, Peter E. [Computational Cosmology Center, Lawrence Berkeley National Laboratory, 1 Cyclotron Road, Berkeley, CA 94720 (United States); Gehrels, Neil [NASA-Goddard Space Flight Center, Greenbelt, MD 20771 (United States); and others

2012-02-10T23:59:59.000Z

277

Experto Universitario Java Enterprise Validacin e internacionalizacin 2012-2013 Depto. Ciencia de la Computacin e IA Spring  

E-Print Network (OSTI)

Experto Universitario Java Enterprise Validación e internacionalización © 2012-2013 Depto. Ciencia #12;Experto Universitario Java Enterprise Validación e internacionalización © 2012-2013 Depto. Ciencia Java Enterprise Validación e internacionalización © 2012-2013 Depto. Ciencia de la Computación e IA

Escolano, Francisco

278

TheThe ScienceScience ForumForum (as I(as I picturepicture itit)) Scholarly work  

E-Print Network (OSTI)

#12;Robotics TheThe ScienceScience ForumForum (as I(as I picturepicture itit)) Humanities Scholarly of photonics, robotics, telematics, dynamic physical rendering and intelligent sensors served as the basis to inspire four bestselling authors. The results are four short stories which paint amusing, thought

Torras, Carme

279

EXCELLENTIA CoLumbIA ENgINEErINg66 echanical engineers think about the design, construction, material proper-  

E-Print Network (OSTI)

responsibility for understanding how engines work, how buildings can be more efficiently built, and howHEALTH EXCELLENTIA CoLumbIA ENgINEErINg66 M echanical engineers think about the design the environment affects bridge architecture. They also apply their knowledge to the workings of the human body

Hone, James

280

ANALYSIS OF LIMIT CYCLE STABILITY IN A TAP-CHANGING TRANSFORMER V. Donde I.A. Hiskens  

E-Print Network (OSTI)

ANALYSIS OF LIMIT CYCLE STABILITY IN A TAP-CHANGING TRANSFORMER V. Donde I.A. Hiskens Department of transformer tap changing and load dynamics. Lin- earization of a Poincar´e map is used to prove local of the region of attraction can then be obtained. 1. INTRODUCTION Interactions between tap-changing transformers

Hiskens, Ian A.

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281

A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data  

E-Print Network (OSTI)

Consistency between Carnegie Supernova Project (CSP) and SDSS-II supernova (SN) survey ugri measurements has been evaluated by comparing SDSS and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 magnitude level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 magnitudes in ugri, with rms scatter ranging from 0.043 to 0.077 magnitudes. The u band agreement is promising, with the caveat that only four of the nine supernovae are well-observed in u and these four exhibit an 0.038 magnitude supernova-to-supernova scatter in this filter.

Mosher, J; Corlies, L; Folatelli, G; Frieman, J; Holtzman, J; Jha, S W; Kessler, R; Marriner, J; Phillips, M M; Stritzinger, M; Morrell, N; Schneider, D P

2012-01-01T23:59:59.000Z

282

Beyond the bubble catastrophe of Type Ia supernovae: Pulsating Reverse Detonation models  

E-Print Network (OSTI)

We describe a mechanism by which a failed deflagration of a Chandrasekhar-mass carbon-oxygen white dwarf can turn into a successful thermonuclear supernova explosion, without invoking an ad hoc high-density deflagration-detonation transition. Following a pulsating phase, an accretion shock develops above a core of 1 M_sun composed of carbon and oxygen, inducing a converging detonation. A three-dimensional simulation of the explosion produced a kinetic energy of 1.05E51 ergs and 0.70 M_sun of 56Ni, ejecting scarcely 0.01 M_sun of C-O moving at low velocities. The mechanism works under quite general conditions and is flexible enough to account for the diversity of normal Type Ia supernovae. In given conditions the detonation might not occur, which would reflect in peculiar signatures in the gamma and UV-wavelengths

Eduardo Bravo; Domingo Garcia-Senz

2006-04-03T23:59:59.000Z

283

Sensitivity study of explosive nucleosynthesis in type Ia supernovae: Modification of individual thermonuclear reaction rates  

Science Journals Connector (OSTI)

Background: Type Ia supernovae contribute significantly to the nucleosynthesis of many Fe-group and intermediate-mass elements. However, the robustness of nucleosynthesis obtained via models of this class of explosions has not been studied in depth until now.Purpose: We explore the sensitivity of the nucleosynthesis resulting from thermonuclear explosions of massive white dwarfs with respect to uncertainties in nuclear reaction rates. We put particular emphasis on indentifying the individual reactions rates that most strongly affect the isotopic products of these supernovae.Method: We have adopted a standard one-dimensional delayed detonation model of the explosion of a Chandrasekhar-mass white dwarf and have postprocessed the thermodynamic trajectories of every mass shell with a nucleosynthetic code to obtain the chemical composition of the ejected matter. We have considered increases (decreases) by a factor of 10 on the rates of 1196 nuclear reactions (simultaneously with their inverse reactions), repeating the nucleosynthesis calculations after modification of each reaction rate pair. We have computed as well hydrodynamic models for different rates of the fusion reactions of 12C and of 16O. From the calculations we have selected the reactions that have the largest impact on the supernova yields, and we have computed again the nucleosynthesis using two or three alternative prescriptions for their rates, taken from the JINA REACLIB database. For the three reactions with the largest sensitivity we have analyzed as well the temperature ranges where a modification of their rates has the strongest effect on nucleosynthesis.Results: The nucleosynthesis resulting from the type Ia supernova models is quite robust with respect to variations of nuclear reaction rates, with the exception of the reaction of fusion of two 12C nuclei. The energy of the explosion changes by less than ?4% when the rates of the reactions 12C+12C or 16O+16O are multiplied by a factor of 10 or 0.1. The changes in the nucleosynthesis owing to the modification of the rates of these fusion reactions are also quite modest; for instance, no species with a mass fraction larger than 0.02 experiences a variation of its yield larger than a factor of 2. We provide the sensitivity of the yields of the most abundant species with respect to the rates of the most intense reactions with protons, neutrons, and ?. In general, the yields of Fe-group nuclei are more robust than the yields of intermediate-mass elements. Among the species with yields larger than 10?8M?, 35S has the largest sensitivity to the nuclear reaction rates. It is remarkable that the reactions involving elements with Z>22 have a tiny influence on the supernova nucleosynthesis. Among the charged-particle reactions, the most influential on supernova nucleosynthesis are 30Si+p?31P+?, 20Ne+??24Mg+?, and 24Mg+??27Al+p. The temperatures at which a modification of their rate has a larger impact are in the range 2?T?4 GK.Conclusions: The explosion model (i.e., the assumed conditions and propagation of the flame) chiefly determines the element production of type Ia supernovae and derived quantities such as their luminosity, while the nuclear reaction rates used in the simulations have a small influence on the kinetic energy and final chemical composition of the ejecta. Our results show that the uncertainty in individual thermonuclear reaction rates cannot account for discrepancies of a factor of 2 between isotopic ratios in type Ia supernovae and those in the solar system, especially within the Fe group.

Eduardo Bravo and Gabriel Martnez-Pinedo

2012-05-18T23:59:59.000Z

284

A PRECISION PHOTOMETRIC COMPARISON BETWEEN SDSS-II AND CSP TYPE Ia SUPERNOVA DATA  

SciTech Connect

Consistency between Carnegie Supernova Project (CSP) and SDSS-II Supernova Survey ugri measurements has been evaluated by comparing Sloan Digital Sky Survey (SDSS) and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 mag level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 mag in ugri, with rms scatter ranging from 0.043 to 0.077 mag. The u-band agreement is promising, with the caveat that only four of the nine supernovae are well observed in u and these four exhibit an 0.038 mag supernova-to-supernova scatter in this filter.

Mosher, J.; Sako, M.; Corlies, L. [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Folatelli, G. [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Frieman, J.; Kessler, R. [Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Holtzman, J. [Department of Astronomy, MSC 4500, New Mexico State University, P.O. Box 30001, Las Cruces, NM 88003 (United States); Jha, S. W. [Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, J. [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Phillips, M. M.; Morrell, N. [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Stritzinger, M. [Oskar Klein Centre for Cosmo Particle Physics, AlbaNova University Center, 106 91 Stockholm (Sweden); Schneider, D. P., E-mail: jmosher@sas.upenn.edu [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States)

2012-07-15T23:59:59.000Z

285

A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data  

SciTech Connect

Consistency between Carnegie Supernova Project (CSP) and SDSS-II Supernova Survey ugri measurements has been evaluated by comparing Sloan Digital Sky Survey (SDSS) and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 mag level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 mag in ugri, with rms scatter ranging from 0.043 to 0.077 mag. The u-band agreement is promising, with the caveat that only four of the nine supernovae are well observed in u and these four exhibit an 0.038 mag supernova-to-supernova scatter in this filter.

Mosher, J.; /Pennsylvania U.; Sako, M.; /Pennsylvania U.; Corlies, L.; /Pennsylvania U. /Columbia U.; Folatelli, G.; /Tokyo U. /Carnegie Inst. Observ.; Frieman, J.; /Chicago U., KICP /Chicago U., Astron. Astrophys. Ctr.; Holtzman, J.; /New Mexico State U.; Jha, S.W.; /Rutgers U., Piscataway; Kessler, R.; /Chicago U., Astron. Astrophys. Ctr. /Chicago U., KICP; Marriner, J.; /Fermilab; Phillips, M.M.; /Carnegie Inst. Observ.; Stritzinger, M.; /Aarhus U. /Stockholm U., OKC /Bohr Inst. /Carnegie Inst. Observ.

2012-06-01T23:59:59.000Z

286

{chi}{sup 2} versus median statistics in supernova type Ia data analysis  

SciTech Connect

In this paper we compare the performances of the {chi}{sup 2} and median likelihood analysis in the determination of cosmological constraints using type Ia supernovae data. We perform a statistical analysis using the 307 supernovae of the Union 2 compilation of the Supernova Cosmology Project and find that the {chi}{sup 2} statistical analysis yields tighter cosmological constraints than the median statistic if only supernovae data is taken into account. We also show that when additional measurements from the cosmic microwave background and baryonic acoustic oscillations are considered, the combined cosmological constraints are not strongly dependent on whether one applies the {chi}{sup 2} statistic or the median statistic to the supernovae data. This indicates that, when complementary information from other cosmological probes is taken into account, the performances of the {chi}{sup 2} and median statistics are very similar, demonstrating the robustness of the statistical analysis.

Barreira, A. [Centro de Fisica do Porto, Rua do Campo Alegre 687, 4169-007 Porto (Portugal); Departamento de Fisica da Faculdade de Ciencias da Universidade do Porto, Rua do Campo Alegre 687, 4169-007 Porto (Portugal); Avelino, P. P. [Departamento de Fisica da Faculdade de Ciencias da Universidade do Porto, Rua do Campo Alegre 687, 4169-007 Porto (Portugal); Centro de Astrofisica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto (Portugal)

2011-10-15T23:59:59.000Z

287

Small-scale Interaction of Turbulence with Thermonuclear Flames in Type Ia Supernovae  

E-Print Network (OSTI)

Microscopic turbulence-flame interactions of thermonuclear fusion flames occuring in Type Ia Supernovae were studied by means of incompressible direct numerical simulations with a highly simplified flame description. The flame is treated as a single diffusive scalar field with a nonlinear source term. It is characterized by its Prandtl number, Pr << 1, and laminar flame speed, S_L. We find that if S_L ~ u', where u' is the rms amplitude of turbulent velocity fluctuations, the local flame propagation speed does not significantly deviate from S_L even in the presence of velocity fluctuations on scales below the laminar flame thickness. This result is interpreted in the context of subgrid-scale modeling of supernova explosions and the mechanism for deflagration-detonation-transitions.

J. C. Niemeyer; W. K. Bushe; G. R. Ruetsch

1999-05-07T23:59:59.000Z

288

Initiation of the Detonation in the Gravitationally Confined Detonation Model of Type Ia Supernovae  

Science Journals Connector (OSTI)

We study the initiation of the detonation in the gravitationally confined detonation (GCD) model of Type Ia supernovae (SNe Ia). In this model, ignition occurs at one or several off-center points, resulting in a burning bubble of hot ash that rises rapidly, breaks through the surface of the star, and collides at a point on the stellar surface opposite the breakout, producing a high-velocity inwardly directed flow. Initiation of the detonation occurs spontaneously in a region where the length scale of the temperature gradient extending from the flow (in which carbon burning is already occurring) into unburned fuel is commensurate to the range of critical length scales which have been derived from one-dimensional simulations that resolve the initiation of a detonation. By increasing the maximum resolution in a truncated cone that encompasses this region, beginning somewhat before initiation of the detonation occurs, we successfully simulate in situ the first gradient-initiated detonation in a whole-star simulation. The detonation emerges when a compression wave overruns a pocket of fuel situated in a Kelvin-Helmholtz cusp at the leading edge of the inwardly directed jet of burning carbon. The compression wave preconditions the temperature in the fuel in such a way that the Zel'dovich gradient mechanism can operate and a detonation ensues. We explore the dependence of the length scale of the temperature gradient on spatial resolution and discuss the implications for the robustness of this detonation mechanism. We find that the time and the location at which initiation of the detonation occurs varies with resolution. In particular, initiation of a detonation had not yet occurred in our highest resolution simulation by the time we ended the simulation because of the computational demand it required. However, it may detonate later. We suggest that the turbulent shear layer surrounding the inwardly directed jet provides the most favorable physical conditions, and therefore the most likely location, for initiation of a detonation in the GCD model.

Ivo R. Seitenzahl; Casey A. Meakin; Don Q. Lamb; James W. Truran

2009-01-01T23:59:59.000Z

289

Study of the Detonation Phase in the Gravitationally Confined Detonation Model of Type Ia Supernovae  

E-Print Network (OSTI)

We study the gravitationally confined detonation (GCD) model of Type Ia supernovae through the detonation phase and into homologous expansion. In the GCD model, a detonation is triggered by the surface flow due to single point, off-center flame ignition in carbon-oxygen white dwarfs. The simulations are unique in terms of the degree to which non-idealized physics is used to treat the reactive flow, including weak reaction rates and a time dependent treatment of material in nuclear statistical equilibrium (NSE). Careful attention is paid to accurately calculating the final composition of material which is burned to NSE and frozen out in the rapid expansion following the passage of a detonation wave over the high density core of the white dwarf; and an efficient method for nucleosynthesis post-processing is developed which obviates the need for costly network calculations along tracer particle thermodynamic trajectories. Observational diagnostics are presented for the explosion models, including abundance stratifications and integrated yields. We find that for all of the ignition conditions studied here, a self regulating process comprised of neutronization and stellar expansion results in final \\iso{Ni}{56} masses of $\\sim$1.1\\msun. But, more energetic models result in larger total NSE and stable Fe peak yields. The total yield of intermediate mass elements is $\\sim0.1$\\msun and the explosion energies are all around 1.5$\\times10^{51}$ ergs. The explosion models are briefly compared to the inferred properties of recent Type Ia supernova observations. The potential for surface detonation models to produce lower luminosity (lower \\iso{Ni}{56} mass) supernovae is discussed.

Casey A. Meakin; Ivo Seitenzahl; Dean Townsley; George C. Jordan IV; James Truran; Don Lamb

2008-06-30T23:59:59.000Z

290

Initiation of the detonation in the gravitationally confined detonation model of type Ia supernovae.  

SciTech Connect

We study the initiation of the detonation in the gravitationally confined detonation (GCD) model of Type Ia supernovae (SNe Ia). In this model, ignition occurs at one or several off-center points, resulting in a burning bubble of hot ash that rises rapidly, breaks through the surface of the star, and collides at a point on the stellar surface opposite the breakout, producing a high-velocity inwardly directed flow. Initiation of the detonation occurs spontaneously in a region where the length scale of the temperature gradient extending from the flow (in which carbon burning is already occurring) into unburned fuel is commensurate to the range of critical length scales which have been derived from one-dimensional simulations that resolve the initiation of a detonation. By increasing the maximum resolution in a truncated cone that encompasses this region, beginning somewhat before initiation of the detonation occurs, we successfully simulate in situ the first gradient-initiated detonation in a whole-star simulation. The detonation emerges when a compression wave overruns a pocket of fuel situated in a Kelvin-Helmholtz cusp at the leading edge of the inwardly directed jet of burning carbon. The compression wave preconditions the temperature in the fuel in such a way that the Zel'dovich gradient mechanism can operate and a detonation ensues. We explore the dependence of the length scale of the temperature gradient on spatial resolution and discuss the implications for the robustness of this detonation mechanism. We find that the time and the location at which initiation of the detonation occurs varies with resolution. In particular, initiation of a detonation had not yet occurred in our highest resolution simulation by the time we ended the simulation because of the computational demand it required. However, it may detonate later. We suggest that the turbulent shear layer surrounding the inwardly directed jet provides the most favorable physical conditions, and therefore the most likely location, for initiation of a detonation in the GCD model.

Seitenzahl, I. R.; Meakin, C. A.; Lamb, D. Q.; Truran, J. W. (Physics); (Univ. of Chicago); (Max-Planck-Inst. for Astrophysics); (Univ. of Arizona)

2009-07-20T23:59:59.000Z

291

Study of the detonation phase in the gravitationally confined detonation model of type Ia supernovae.  

SciTech Connect

We study the initiation of the detonation in the gravitationally confined detonation (GCD) model of Type Ia supernovae (SNe Ia). In this model, ignition occurs at one or several off-center points, resulting in a burning bubble of hot ash that rises rapidly, breaks through the surface of the star, and collides at a point on the stellar surface opposite the breakout, producing a high-velocity inwardly directed flow. Initiation of the detonation occurs spontaneously in a region where the length scale of the temperature gradient extending from the flow (in which carbon burning is already occurring) into unburned fuel is commensurate to the range of critical length scales which have been derived from one-dimensional simulations that resolve the initiation of a detonation. By increasing the maximum resolution in a truncated cone that encompasses this region, beginning somewhat before initiation of the detonation occurs, we successfully simulate in situ the first gradient-initiated detonation in a whole-star simulation. The detonation emerges when a compression wave overruns a pocket of fuel situated in a Kelvin-Helmholtz cusp at the leading edge of the inwardly directed jet of burning carbon. The compression wave preconditions the temperature in the fuel in such a way that the Zeldovich gradient mechanism can operate and a detonation ensues. We explore the dependence of the length scale of the temperature gradient on spatial resolution and discuss the implications for the robustness of this detonation mechanism. We find that the time and the location at which initiation of the detonation occurs varies with resolution. In particular, initiation of a detonation had not yet occurred in our highest resolution simulation by the time we ended the simulation because of the computational demand it required. However, it may detonate later. We suggest that the turbulent shear layer surrounding the inwardly directed jet provides the most favorable physical conditions, and therefore the most likely location, for initiation of a detonation in the GCD model.

Meakin, C. A.; Seitenzahl, I.; Jordan, G. C.; Truran,, J.; Lamb, D.; Physics; Univ. of Chicago; Univ. of Arizona

2009-07-20T23:59:59.000Z

292

NUCLEOSYNTHESIS IN TWO-DIMENSIONAL DELAYED DETONATION MODELS OF TYPE Ia SUPERNOVA EXPLOSIONS  

SciTech Connect

For the explosion mechanism of Type Ia supernovae (SNe Ia), different scenarios have been suggested. In these, the propagation of the burning front through the exploding white dwarf (WD) star proceeds in different modes, and consequently imprints of the explosion model on the nucleosynthetic yields can be expected. The nucleosynthetic characteristics of various explosion mechanisms are explored based on three two-dimensional explosion simulations representing extreme cases: a pure turbulent deflagration, a delayed detonation following an approximately spherical ignition of the initial deflagration, and a delayed detonation arising from a highly asymmetric deflagration ignition. Apart from this initial condition, the deflagration stage is treated in a parameter-free approach. The detonation is initiated when the turbulent burning enters the distributed burning regime. This occurs at densities around 10{sup 7} g cm{sup -3}-relatively low as compared to existing nucleosynthesis studies for one-dimensional spherically symmetric models. The burning in these multidimensional models is different from that in one-dimensional simulations as the detonation wave propagates both into unburned material in the high-density region near the center of a WD and into the low-density region near the surface. Thus, the resulting yield is a mixture of different explosive burning products, from carbon-burning products at low densities to complete silicon-burning products at the highest densities, as well as electron-capture products synthesized at the deflagration stage. Detailed calculations of the nucleosynthesis in all three models are presented. In contrast to the deflagration model, the delayed detonations produce a characteristic layered structure and the yields largely satisfy constraints from Galactic chemical evolution. In the asymmetric delayed detonation model, the region filled with electron capture species (e.g., {sup 58}Ni, {sup 54}Fe) is within a shell, showing a large off-set, above the bulk of {sup 56}Ni distribution, while species produced by the detonation are distributed more spherically.

Maeda, K. [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Roepke, F.K.; Fink, M.; Hillebrandt, W.; Travaglio, C. [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching (Germany); Thielemann, F.-K., E-mail: keiichi.maeda@ipmu.j [Department Physik, Universitaet Basel, CH-4056 Basel (Switzerland)

2010-03-20T23:59:59.000Z

293

INITIATION OF THE DETONATION IN THE GRAVITATIONALLY CONFINED DETONATION MODEL OF TYPE Ia SUPERNOVAE  

SciTech Connect

We study the initiation of the detonation in the gravitationally confined detonation (GCD) model of Type Ia supernovae (SNe Ia). In this model, ignition occurs at one or several off-center points, resulting in a burning bubble of hot ash that rises rapidly, breaks through the surface of the star, and collides at a point on the stellar surface opposite the breakout, producing a high-velocity inwardly directed flow. Initiation of the detonation occurs spontaneously in a region where the length scale of the temperature gradient extending from the flow (in which carbon burning is already occurring) into unburned fuel is commensurate to the range of critical length scales which have been derived from one-dimensional simulations that resolve the initiation of a detonation. By increasing the maximum resolution in a truncated cone that encompasses this region, beginning somewhat before initiation of the detonation occurs, we successfully simulate in situ the first gradient-initiated detonation in a whole-star simulation. The detonation emerges when a compression wave overruns a pocket of fuel situated in a Kelvin-Helmholtz cusp at the leading edge of the inwardly directed jet of burning carbon. The compression wave preconditions the temperature in the fuel in such a way that the Zel'dovich gradient mechanism can operate and a detonation ensues. We explore the dependence of the length scale of the temperature gradient on spatial resolution and discuss the implications for the robustness of this detonation mechanism. We find that the time and the location at which initiation of the detonation occurs varies with resolution. In particular, initiation of a detonation had not yet occurred in our highest resolution simulation by the time we ended the simulation because of the computational demand it required. However, it may detonate later. We suggest that the turbulent shear layer surrounding the inwardly directed jet provides the most favorable physical conditions, and therefore the most likely location, for initiation of a detonation in the GCD model.

Seitenzahl, Ivo R. [Department of Physics, University of Chicago, Chicago, IL 60637 (United States); Meakin, Casey A.; Truran, James W. [Joint Institute for Nuclear Astrophysics, University of Chicago, Chicago, IL 60637 (United States); Lamb, Don Q. [Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637 (United States)

2009-07-20T23:59:59.000Z

294

SN 2003du: Signatures of the Circumstellar Environment in a Normal Type Ia Supernova?  

E-Print Network (OSTI)

We present observations of the Type Ia supernova 2003du and report the detectionof an unusual, high-velocity component in the Ca II infrared triplet, similar tofeatures previously observed in SN 2000cx and SN 2001el. This feature exhibits a large expansion velocity (~18,000 km/s) which is nearly constant between -7 and +2 days relative to maximum light, and disappears shortly thereafter. Otherthan this feature, the spectral evolution and light curve resemble those of a normal SN Ia. We find that the Ca II feature can plausibly be caused by a dense shell formed when circumstellar material of solar abundance is overrun by the rapidly expanding outermost layers of the SN ejecta. Model calculations show that the optical and infrared spectra are remarkably unaffected by the circumstellar interaction. In particular, no hydrogen lines are detectable in either absorption or emission. The only qualitatively different features are the strong, high-velocity feature in the Ca II IR-triplet, and a somewhat weaker O I feature near 7,300 AA. The morphology and time evolution of these features provide an estimate for the amount of accumulated matter and an indication of the mixing in the dense shell. We apply these diagnostic tools to SN 2003du and infer that about 2 x 10^{-2} M_sun of solar abundance material may have accumulated in a circumstellar shell prior to the observations. Furthermore, the early light curve data imply that the circumstellar material was originally very close to the progenitor system, perhaps from an accretion disk, Roche lobe or common envelope.

C. L. Gerardy; P. Hoeflich; R. A. Fesen; G. H. Marion; K. Nomoto; R. Quimby; B. E. Schaefer; L. Wang; J. C. Wheeler

2003-09-23T23:59:59.000Z

295

Sensitivity study of explosive nucleosynthesis in Type Ia supernovae: I. Modification of individual thermonuclear reaction rates  

E-Print Network (OSTI)

We explore the sensitivity of the nucleosynthesis due to type Ia supernovae with respect to uncertainties in nuclear reaction rates. We have adopted a standard one-dimensional delayed detonation model of the explosion of a Chandrasekhar-mass white dwarf, and have post-processed the thermodynamic trajectories of every mass-shell with a nucleosynthetic code, with increases (decreases) by a factor of ten on the rates of 1196 nuclear reactions. We have computed as well hydrodynamic models for different rates of the fusion reactions of 12C and of 16O. For selected reactions, we have recomputed the nucleosynthesis with alternative prescriptions for their rates taken from the JINA REACLIB database, and have analyzed the temperature ranges where modifications of their rates have the strongest effect on nucleosynthesis. The nucleosynthesis resulting from the Type Ia supernova models is quite robust with respect to variations of nuclear reaction rates, with the exception of the reaction of fusion of 12C nuclei. The energy of the explosion changes by less than \\sim4%. The changes in the nucleosynthesis due to the modification of the rates of fusion reactions are as well quite modest, for instance no species with a mass fraction larger than 0.02 experiences a variation of its yield larger than a factor of two. We provide the sensitivity of the yields of the most abundant species with respect to the rates of the most intense reactions with protons, neutrons, and alphas. In general, the yields of Fe-group nuclei are more robust than the yields of intermediate-mass elements. Among the charged particle reactions, the most influential on supernova nucleosynthesis are 30Si + p \\rightleftarrows 31P + {\\gamma}, 20Ne + {\\alpha} \\rightleftarrows 24Mg + {\\gamma}, and 24Mg + {\\alpha} \\rightleftarrows 27Al + p. The temperatures at which a modification of their rate has a larger impact are in the range 2 < T < 4 GK. (abridged)

Eduardo Bravo; Gabriel Martnez-Pinedo

2012-04-09T23:59:59.000Z

296

Incompatibility of a comoving Ly-alpha forest with supernova-Ia luminosity distances  

E-Print Network (OSTI)

Recently Perlmutter et al. suggested a positive value of Einstein's cosmological constant Lambda on the basis of luminosity distances from type-Ia supernovae. However, Lambda world models had earlier been proposed by Hoell & Priester and Liebscher et al. on the basis of quasar absorption-line data. Employing more general repulsive fluids ("dark energy") encompassing the Lambda component we quantitatively compare both approaches with each other. Fitting the SN-data by a minimum-component model consisting of dark energy + dust yields a closed universe with a large amount of dust exceeding the baryonic content constrained by big-bang nucleosynthesis. The nature of the dark energy is hardly constrained. Only when enforcing a flat universe there is a clear tendency to a dark-energy Lambda fluid and the `canonical' value Omega_M = 0.3 for dust. Conversely, fitting the quasar-data by a minimum-component model yields a sharply defined, slightly closed model with a low dust density ruling out significant pressureless dark matter. The dark-energy component obtains an equation-of-state P = -0.96 epsilon close to that of a Lambda-fluid. Omega_M = 0.3 or a precisely flat spatial geometry are inconsistent with minimum-component models. It is found that quasar and supernova data sets cannot be reconciled with each other via (repulsive ideal fluid+dust+radiation)-world models. Compatibility could be reached by drastic expansion of the parameter space with at least two exotic fluids added to dust and radiation as world constituents. If considering such solutions as far-fetched one has to conclude that the quasar absorption line and the SN-Ia constraints are incompatible.

Jens Thomas; Hartmut Schulz

2001-03-18T23:59:59.000Z

297

Top photo by Steve Rodie. A naturalized drainage swale in this resi-dential development near Chicago drastically reduces both mowing and  

E-Print Network (OSTI)

Top photo by Steve Rodie. A naturalized drainage swale in this resi- dential development near Chicago drastically reduces both mowing and stormwater runoff. Photo far left: Grouping trees and shrubs makes them easier to manage and is ultimately healthier for them. Photo opposite: Closely spaced grasses

Farritor, Shane

298

HELIUM-IGNITED VIOLENT MERGERS AS A UNIFIED MODEL FOR NORMAL AND RAPIDLY DECLINING TYPE Ia SUPERNOVAE  

SciTech Connect

The progenitors of Type Ia supernovae (SNe Ia) are still unknown, despite significant progress during the past several years in theory and observations. Violent mergers of two carbon-oxygen (CO) white dwarfs (WDs) are a candidate scenario suggested to be responsible for at least a significant fraction of normal SNe Ia. Here, we simulate the merger of two CO WDs using a moving-mesh code that allows for the inclusion of thin helium (He) shells (0.01 M{sub Sun }) on top of the WDs at an unprecedented numerical resolution. The accretion of He onto the primary WD leads to the formation of a detonation in its He shell. This detonation propagates around the CO WD and sends a converging shock wave into its core, known to robustly trigger a second detonation, as in the well-known double-detonation scenario for He-accreting CO WDs. However, in contrast to that scenario where a massive He shell is required to form a detonation through thermal instability, here the He detonation is ignited dynamically. Accordingly the required He-shell mass is significantly smaller, and hence its burning products are unlikely to affect the optical display of the explosion. We show that this scenario, which works for CO primary WDs with CO- as well as He-WD companions, has the potential to explain the different brightness distributions, delay times, and relative rates of normal and fast declining SNe Ia. Finally, we discuss extensions to our unified merger model needed to obtain a comprehensive picture of the full observed diversity of SNe Ia.

Pakmor, R.; Springel, V. [Heidelberger Institut fuer Theoretische Studien, Schloss-Wolfsbrunnenweg 35, D-69118 Heidelberg (Germany); Kromer, M. [Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa, Chiba 277-8583 (Japan); Taubenberger, S. [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Str. 1, D-85748 Garching (Germany)

2013-06-10T23:59:59.000Z

299

New Hubble Space Telescope Discoveries of Type Ia Supernovae at z > 1: Narrowing Constraints on the Early Behavior of Dark Energy  

E-Print Network (OSTI)

We have discovered 21 new Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to trace the history of cosmic expansion over the last 10 billion years. These objects, which include 13 spectroscopically confirmed SNe Ia at z > 1, were discovered during 14 epochs of reimaging of the GOODS fields North and South over two years with the Advanced Camera for Surveys on HST. Together with a recalibration of our previous HST-discovered SNe Ia, the full sample of 23 SNe Ia at z > 1 provides the highest-redshift sample known. Combined with previous SN Ia datasets, we measured H(z) at discrete, uncorrelated epochs, reducing the uncertainty of H(z>1) from 50% to under 20%, strengthening the evidence for a cosmic jerk--the transition from deceleration in the past to acceleration in the present. The unique leverage of the HST high-redshift SNe Ia provides the first meaningful constraint on the dark energy equation-of-state parameter at z >1. The result remains consistent with a cosmological constant (w(z)=-1), and rules out rapidly evolving dark energy (dw/dz >>1). The defining property of dark energy, its negative pressure, appears to be present at z>1, in the epoch preceding acceleration, with ~98% confidence in our primary fit. Moreover, the z>1 sample-averaged spectral energy distribution is consistent with that of the typical SN Ia over the last 10 Gyr, indicating that any spectral evolution of the properties of SNe Ia with redshift is still below our detection threshold.

Adam G. Riess; Louis-Gregory Strolger; Stefano Casertano; Henry C. Ferguson; Bahram Mobasher; Ben Gold; Peter J. Challis; Alexei V. Filippenko; Saurabh Jha; Weidong Li; John Tonry; Ryan Foley; Robert P. Kirshner; Mark Dickinson; Emily MacDonald; Daniel Eisenstein; Mario Livio; Josh Younger; Chun Xu; Tomas Dahlen; Daniel Stern

2006-11-17T23:59:59.000Z

300

CHASING THE IDENTIFICATION OF ASCA GALACTIC OBJECTS (ChIcAGO): AN X-RAY SURVEY OF UNIDENTIFIED SOURCES IN THE GALACTIC PLANE. I. SOURCE SAMPLE AND INITIAL RESULTS  

E-Print Network (OSTI)

We present the Chasing the Identification of ASCA Galactic Objects (ChIcAGO) survey, which is designed to identify the unknown X-ray sources discovered during the ASCA Galactic Plane Survey (AGPS). Little is known about ...

Anderson, Gemma E.

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301

CP Tech Center I Iowa State University I 2711 S. Loop Dr. Suite 4700,Ames, IA 50010-8664 I 515-294-5798 FOR MORE INFORMATION  

E-Print Network (OSTI)

CP Tech Center I Iowa State University I 2711 S. Loop Dr. Suite 4700,Ames, IA 50010-8664 I 515 calcium sulfate in the form of hemihydrate (plaster) in the cement (false set) or the uncontrolled early

302

??eia e e et ??? oa0 to 3i5ontinBoB5 PieeFi5e Hinea tiTiUation ...  

E-Print Network (OSTI)

PieeFi5e Hinea tiTiUation. I.R. de Farias JR., M. ?hao, and H. ?hao. State University of New York at jumalo. {defariasy m|haoy |hon??ia}@??ffalo.ed?.

303

LAX XXlCfl jX?iK, Idd+?KYLViG?IA  

Office of Legacy Management (LM)

f f , : I~&l, samtier cipwati8Aa CffUm - . Jiux.lCJ d,# 1754 - - _- - .- t :; . Jesse e. ahizmn*~*ter -2.' -------- - _ &tV' hi@A l f izau Bkteriala ;' . . 1 -7 I _' i' . Fpr&G& r&Q Q,&& fu &fI& L;&& -l&d 2;,i' iI,;/Qi' rIGN CQ&GgJy p;E& p;~p>gyf LAX XXlCfl jX?iK, Idd+?KYLViG?IA i-icfer~~o is &o ta yaw rwarandu3;: l P iimwmbec L?, 1953, reque&in~ a d&q.&ti of khority tA A&sister prog= for th+zz developmrrrl, Ii-&k& & acyui8itti ef c;uYletit*type and reswitlitc-type urtim bi:aPing eres and far t3-u jx*uctim and acquisitian 6f W ;aniU CCm- csa:ratc~ fhzi awes wit2n Lhe Six&e of Pemlsyzvania. 1 da not b&i- the projscrt fmr the pkcch2670 +S eroa from i&d.&

304

Direct numerical simulations of type Ia supernovae flames I: The landau-darrieus instability  

SciTech Connect

Planar flames are intrinsically unstable in open domains due to the thermal expansion across the burning front--the Landau-Darrieus instability. This instability leads to wrinkling and growth of the flame surface, and corresponding acceleration of the flame, until it is stabilized by cusp formation. We look at the Landau-Darrieus in stability for C/O thermonuclear flames at conditions relevant to the late stages of a Type Ia supernova explosion. Two-dimensional direct numerical simulations of both single-mode and multi-mode perturbations using a low Mach number hydrodynamics code are presented. We show the effect of the instability on the flame speed as a function of both the density and domain size, demonstrate the existence of the small scale cutoff to the growth of the instability, and look for the proposed breakdown of the non-linear stabilization at low densities. The effects of curvature on the flame as quantified through measurements of the growth rate and computation of the corresponding Markstein number. While accelerations of a few percent are observed, they are too small to have any direct outcome on the supernova explosion.

Bell, J.B.; Day, M.S.; Rendleman, C.A.; Woosley, S.E.; Zingale, M.

2003-11-24T23:59:59.000Z

305

Thermonuclear .Ia Supernovae from Helium Shell Detonations: Explosion Models and Observables  

Science Journals Connector (OSTI)

During the early evolution of an AM Canum Venaticorum system, helium is accreted onto the surface of a white dwarf under conditions suitable for unstable thermonuclear ignition. The turbulent motions induced by the convective burning phase in the He envelope become strong enough to influence the propagation of burning fronts and may result in the onset of a detonation. Such an outcome would yield radioactive isotopes and a faint rapidly rising thermonuclear ".Ia" supernova. In this paper, we present hydrodynamic explosion models and observable outcomes of these He shell detonations for a range of initial core and envelope masses. The peak UVOIR bolometric luminosities range by a factor of 10 (from 5 ? 1041 to 5 ? 1042 erg s1), and the R-band peak varies from M R,peak = 15 to 18. The rise times in all bands are very rapid (40Ca through 56Ni) and unburnt He. Thus, the spectra around peak light lack signs of intermediate-mass elements and are dominated by CaII and TiII features, with the caveat that our radiative transfer code does not include the nonthermal effects necessary to produce He features.

Ken J. Shen; Dan Kasen; Nevin N. Weinberg; Lars Bildsten; Evan Scannapieco

2010-01-01T23:59:59.000Z

306

Comparison of the Legacy and Gold SnIa Dataset Constraints on Dark Energy Models  

E-Print Network (OSTI)

We have performed a comparative analysis of three recent and reliable SnIa datasets available in the literature: the Full Gold (FG) dataset (157 data points $0dataset (140 data points $0dataset (115 data points $0datasets are consistent with each other at the 95% confidence level, the latest (SNLS) dataset shows distinct trends which are not shared by the Gold datasets. We find that the best fit dynamical $w(z)$ obtained from the SNLS dataset does not cross the PDL $w=-1$ and remains above and close to the $w=-1$ line for the whole redshift range $0datasets (FG and TG) clearly crosses the PDL and departs significantly from the PDL $w=-1$ line while the LCDM parameter values are about $2\\sigma$ away from the best fit $w(z)$. In addition, the $(\\Omega_{0m},\\Omega_\\Lambda)$ parameters in a LCDM parametrization without a flat prior, fit by the SNLS dataset, favor the minimal flat LCDM concordance model. The corresponding fit with the Gold datasets mildly favors a closed universe and the flat LCDM parameter values are $1\\sigma - 2\\sigma$ away from the best fit $(\\Omega_{0m},\\Omega_\\Lambda)$.

S. Nesseris; L. Perivolaropoulos

2005-12-02T23:59:59.000Z

307

Phenomenology for Supernova Ia Data Based on a New Cosmic Time  

E-Print Network (OSTI)

A new phenomenological theory for the expansion of our universe is presented. Because fundamental supporting theory is still in development, its discussion is not presented in this paper. The theory is based on a new algebraic expression for cosmic time G Rho t^2=3/32Pi, which correctly predicts the WMAP measured cosmological constants and the fundamental Hubble parameter H(t) for the expansion of the universe. A replacement for dark matter, called here "dark mass", is proposed which scales as with the expansion and incorporated. It does not react with ordinary matter, except gravitationally, and produces flat rotational curves for spiral galaxies. Also a new expression for the approaching velocity of radiation in a closed 3-sphere expanding universe is given that accounts for the early degrading negative approach of radiation for z > 1.7. The expression is v = Hr-c. Combining these three elements produces a luminosity distance dL that successfully predicts the apparent magnitude of exploding supernova Ia stars and even the new gamma ray bursts with no need for dark energy or acceleration of the expansion of the universe.

Charles B. Leffert

2007-07-26T23:59:59.000Z

308

Evaluating Systematic Dependencies of Type Ia Supernovae: The Influence of Deflagration to Detonation Density  

E-Print Network (OSTI)

We explore the effects of the deflagration to detonation transition (DDT) density on the production of Ni-56 in thermonuclear supernova explosions (type Ia supernovae). Within the DDT paradigm, the transition density sets the amount of expansion during the deflagration phase of the explosion and therefore the amount of nuclear statistical equilibrium (NSE) material produced. We employ a theoretical framework for a well-controlled statistical study of two-dimensional simulations of thermonuclear supernovae with randomized initial conditions that can, with a particular choice of transition density, produce a similar average and range of Ni-56 masses to those inferred from observations. Within this framework, we utilize a more realistic "simmered" white dwarf progenitor model with a flame model and energetics scheme to calculate the amount of Ni-56 and NSE material synthesized for a suite of simulated explosions in which the transition density is varied in the range 1-3x10^7 g/cc. We find a quadratic dependence ...

Jackson, Aaron P; Townsley, Dean M; Chamulak, David A; Brown, Edward F; Timmes, F X

2010-01-01T23:59:59.000Z

309

A Test of Tully-Fisher Distance Estimates Using Cepheids and Type Ia Supernovae  

E-Print Network (OSTI)

We update and extend the results of Shanks (1997, MNRAS, 290, L77) by making a direct test of Tully-Fisher distance estimates to thirteen spiral galaxies with HST Cepheid distances and to ten spiral galaxies with Type Ia supernova (SNIa) distances. The results show that the Tully-Fisher distance moduli are too short with respect to the Cepheid distances by 0.46+-0.11mag and too short with respect to the SNIa distances by 0.49+-0.18mag. Combining the HST Cepheid and the best SNIa data suggests that, overall, previous Tully-Fisher distances at v~1000 kms-1 were too short by 0.43+-0.09mag, a result which is significant at the 4.6 sigma level. These data therefore indicate that previous Tully-Fisher distances should be revised upwards by 22+-5% implying, for example, a Virgo distance of 19.0+-1.8Mpc. The value of Ho from Tully-Fisher estimates is correspondingly revised downwards from Ho=84+-10kms-1Mpc-1 to Ho=69+-8kms-1Mpc-1. There is evidence that the Tully-Fisher relation at large distances is affected by Malmquist bias. In this case, we argue that Ho<50kms-1Mpc-1 cannot be ruled out by Tully-Fisher considerations.

T. Shanks

1999-01-24T23:59:59.000Z

310

Parametrizing the transition to the phantom epoch with Supernovae Ia and Standard Rulers  

E-Print Network (OSTI)

The reconstruction of a (non)canonical scalar field Lagrangian from the dark energy Equation of State (EoS) parameter is studied, where it is shown that any EoS parametrization can be well reconstructed in terms of scalar fields. Several examples of EoS parameters are studied and the particular scalar field Lagrangian is reconstructed. Then, we propose some new parametrizations that may present a (fast) transition to a phantom dark energy EoS (where $w_{DE}dark energy EoS are studied by using supernovae Ia data (HST Cluster Supernova Survey) combined with Standard Ruler datasets [Cosmic Microwave Background (CMB) and Baryon Acoustic Oscillations (BAO)] and its comparison with the $\\Lambda$CDM model is analyzed. Then, the best fit of the models is obtained, which provides some information about whether a phantom transition may be supported by the observations. In this regard, the crossing of the phantom barrier is allowed statistically but the occurrence of a future singularity seems unlikely.

Iker Leanizbarrutia; Diego Sez-Gmez

2014-04-14T23:59:59.000Z

311

A POSSIBLE EVOLUTIONARY SCENARIO OF HIGHLY MAGNETIZED SUPER-CHANDRASEKHAR WHITE DWARFS: PROGENITORS OF PECULIAR TYPE Ia SUPERNOVAE  

SciTech Connect

Several recently discovered peculiar Type Ia supernovae seem to demand an altogether new formation theory that might help explain the puzzling dissimilarities between them and the standard Type Ia supernovae. The most striking aspect of the observational analysis is the necessity of invoking super-Chandrasekhar white dwarfs having masses {approx}2.1-2.8 M{sub Sun }, M{sub Sun} being the mass of Sun, as their most probable progenitors. Strongly magnetized white dwarfs having super-Chandrasekhar masses have already been established as potential candidates for the progenitors of peculiar Type Ia supernovae. Owing to the Landau quantization of the underlying electron degenerate gas, theoretical results yielded the observationally inferred mass range. Here, we sketch a possible evolutionary scenario by which super-Chandrasekhar white dwarfs could be formed by accretion on to a commonly observed magnetized white dwarf, invoking the phenomenon of flux freezing. This opens multiple possible evolution scenarios ending in supernova explosions of super-Chandrasekhar white dwarfs having masses within the range stated above. We point out that our proposal has observational support, such as the recent discovery of a large number of magnetized white dwarfs by the Sloan Digital Sky Survey.

Das, Upasana; Mukhopadhyay, Banibrata [Department of Physics, Indian Institute of Science, Bangalore 560012 (India); Rao, A. R., E-mail: upasana@physics.iisc.ernet.in, E-mail: bm@physics.iisc.ernet.in, E-mail: arrao@tifr.res.in [Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Mumbai 400005 (India)

2013-04-10T23:59:59.000Z

312

Type Ia Supernovae with Bi-Modal Explosions Are Common -- Possible Smoking Gun for Direct Collisions of White-Dwarfs  

E-Print Network (OSTI)

We discover clear doubly-peaked line profiles in 3 out of ~20 type Ia supernovae (SNe Ia) with high-quality nebular-phase spectra. The profiles are consistently present in three well-separated Co/Fe emission features. The two peaks are respectively blue-shifted and red-shifted relative to the host galaxies and are separated by ~5000 km/s. The doubly-peaked profiles directly reflect a bi-modal velocity distribution of the radioactive Ni56 in the ejecta that powers the emission of these SNe. Due to their random orientations, only a fraction of SNe with intrinsically bi-modal velocity distributions will appear as doubly-peaked spectra. Therefore SNe with intrinsic bi-modality are likely common, especially among the SNe in the low-luminosity (~40% of all SNe Ia) part on the Philips relation \\Delta m15(B) >~ 1.3. Bi-modality is naturally expected from direct collisions of white dwarfs (WDs) due to the detonation of both WDs and is demonstrated in a 3D 0.64 M_Sun-0.64 M_Sun WD collision simulation.

Dong, Subo; Kushnir, Doron; Prieto, Jose L

2014-01-01T23:59:59.000Z

313

Three-Dimensional Simulations of the Deflagration Phase of the Gravitationally Confined Detonation Model of Type Ia Supernovae  

E-Print Network (OSTI)

We report the results of a series of three-dimensional (3-D) simulations of the deflagration phase of the gravitationally confined detonation mechanism for Type Ia supernovae. In this mechanism, ignition occurs at one or several off-center points, resulting in a burning bubble of hot ash that rises rapidly, breaks through the surface of the star, and collides at a point opposite breakout on the stellar surface. We find that detonation conditions are robustly reached in our 3-D simulations for a range of initial conditions and resolutions. Detonation conditions are achieved as the result of an inwardly-directed jet that is produced by the compression of unburnt surface material when the surface flow collides with itself. A high-velocity outwardly-directed jet is also produced. The initial conditions explored in this paper lead to conditions at detonation that can be expected to produce large amounts of $^{56}$Ni and small amounts of intermediate mass elements. These particular simulations are therefore relevant only to high luminosity Type Ia supernovae. Recent observations of Type Ia supernovae imply a compositional structure that is qualitatively consistent with that expected from these simulations.

G C Jordan IV; R T Fisher; D M Townsley; A C Calder; C Graziani; S Asida; D Q Lamb; J W Truran

2007-03-21T23:59:59.000Z

314

The Joint Efficient Dark-energy Investigation (JEDI): Measuring the cosmic expansion history from type Ia supernovae  

E-Print Network (OSTI)

JEDI (Joint Efficient Dark-energy Investigation) is a candidate implementation of the NASA-DOE Joint Dark Energy Mission (JDEM). JEDI will probe dark energy in three independent methods: (1) type Ia supernovae, (2) baryon acoustic oscillations, and (3) weak gravitational lensing. In an accompanying paper, an overall summary of the JEDI mission is given. In this paper, we present further details of the supernova component of JEDI. To derive model-independent constraints on dark energy, it is important to precisely measure the cosmic expansion history, H(z), in continuous redshift bins from z \\~ 0-2 (the redshift range in which dark energy is important). SNe Ia at z > 1 are not readily accessible from the ground because the bulk of their light has shifted into the near-infrared where the sky background is overwhelming; hence a space mission is required to probe dark energy using SNe. Because of its unique near-infrared wavelength coverage (0.8-4.2 microns), JEDI has the advantage of observing SNe Ia in the rest frame J band for the entire redshift range of 0 energy are discussed, with special emphasis on the improved precision afforded by the rest frame near-infrared data.

M. M. Phillips; Peter Garnavich; Yun Wang; David Branch; Edward Baron; Arlin Crotts; J. Craig Wheeler; Edward Cheng; Mario Hamuy; for the JEDI Team

2006-06-28T23:59:59.000Z

315

Constraining the dark energy and smoothness parameter with typeIa supernovae and gamma-ray bursts  

Science Journals Connector (OSTI)

The existence of inhomogeneities in the observed Universe modifies the distance-redshift relations thereby affecting the results of cosmological tests in comparison to the ones derived assuming spatially uniform models. By modeling the inhomogeneities through a Zeldovich-Kantowski-Dyer-Roeder approach which is phenomenologically characterized by a smoothness parameter ?, we rediscuss the constraints on the cosmic parameters based on typeIa supernovae (SNeIa) and gamma-ray bursts (GRBs) data. The present analysis is restricted to a flat ?CDM model with the reasonable assumption that ? does not clump. A ?2 analysis using 557 SNeIa data from the Union2 compilation data (R. Amanullah et al., Astrophys. J. 716, 712 (2010).) constrains the pair of parameters (?m, ?) to ?m=0.27-0.03+0.08 (2?) and ??0.25. A similar analysis based only on 59 Hymnium GRBs (H. Wei, J. Cosmol. Astropart. Phys. 08 (2010) 020.) constrains the matter density parameter to be ?m=0.35-0.24+0.62 (2?) while all values for the smoothness parameter are allowed. By performing a joint analysis, it is found that ?m=0.27-0.03+0.06 and ??0.52. As a general result, although considering that current GRB data alone cannot constrain the smoothness ? parameter, our analysis provides an interesting cosmological probe for dark energy even in the presence of inhomogeneities.

V. C. Busti; R. C. Santos; J. A. S. Lima

2012-05-07T23:59:59.000Z

316

Improving the Field Performance of Natural Gas Furnaces, Chicago, Illinois (Fact Sheet), Building America Case Study: Technology Solutions for New and Existing Homes, Building Technologies Office (BTO)  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

the Field Performance the Field Performance of Natural Gas Furnaces Chicago, Illinois PROJECT INFORMATION Project Name: Improving Gas Furnace Performance-A Field and Lab Study at End of Life Location: Chicago, IL Partnership for Advanced Residential Retrofit www.gastechnology.org Building Component: Natural Gas Furnaces Application: New and/or retrofit; Single and/or multifamily Year Tested: 2012/2013 Applicable Climate Zone(s): All or specify which ones PERFORMANCE DATA Cost of Energy Efficiency Measure (including labor): $250 for adjustments Projected Energy Savings: 6.4% heating savings Projected Energy Cost Savings: $100/year climate-dependent Gas furnaces can successfully operate in the field for 20 years or longer with

317

THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. III. CORRELATED PROPERTIES OF TYPE Ia SUPERNOVAE AND THEIR HOSTS AT 0.9 < z < 1.46  

SciTech Connect

Using the sample of Type Ia supernovae (SNe Ia) discovered by the Hubble Space Telescope (HST) Cluster Supernova Survey and augmented with HST-observed SNe Ia in the Great Observatories Origins Deep Survey (GOODS) fields, we search for correlations between the properties of SNe and their host galaxies at high redshift. We use galaxy color and quantitative morphology to determine the red sequence in 25 clusters and develop a model to distinguish passively evolving early-type galaxies from star-forming galaxies in both clusters and the field. With this approach, we identify 6 SN Ia hosts that are early-type cluster members and 11 SN Ia hosts that are early-type field galaxies. We confirm for the first time at z > 0.9 that SNe Ia hosted by early-type galaxies brighten and fade more quickly than SNe Ia hosted by late-type galaxies. We also show that the two samples of hosts produce SNe Ia with similar color distributions. The relatively simple spectral energy distributions expected for passive galaxies enable us to measure stellar masses of early-type SN hosts. In combination with stellar mass estimates of late-type GOODS SN hosts from Thomson and Chary, we investigate the correlation of host mass with Hubble residual observed at lower redshifts. Although the sample is small and the uncertainties are large, a hint of this relation is found at z > 0.9. By simultaneously fitting the average cluster galaxy formation history and dust content to the red-sequence scatters, we show that the reddening of early-type cluster SN hosts is likely E(B - V) {approx}< 0.06. The similarity of the field and cluster early-type host samples suggests that field early-type galaxies that lie on the red sequence may also be minimally affected by dust. Hence, the early-type-hosted SNe Ia studied here occupy a more favorable environment to use as well-characterized high-redshift standard candles than other SNe Ia.

Meyers, J.; Barbary, K.; Fakhouri, H. K.; Goldhaber, G. [Department of Physics, University of California Berkeley, Berkeley, CA 94720 (United States); Aldering, G.; Faccioli, L.; Hsiao, E. [E.O. Lawrence Berkeley National Lab, 1 Cyclotron Rd., Berkeley, CA 94720 (United States); Barrientos, L. F. [Departmento de Astronomia, Pontificia Universidad Catolica de Chile, Santiago (Chile); Brodwin, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Dawson, K. S. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Deustua, S.; Fruchter, A. S. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Doi, M.; Ihara, Y. [Institute of Astronomy, Graduate School of Science, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Eisenhardt, P. [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States); Gilbank, D. G. [Department of Physics and Astronomy, University Of Waterloo, Waterloo, Ontario, N2L 3G1 (Canada); Gladders, M. D. [Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637 (United States); Gonzalez, A. H. [Department of Astronomy, University of Florida, Gainesville, FL 32611 (United States); Hattori, T. [Subaru Telescope, National Astronomical Observatory of Japan, 650 North Aohaku Place, Hilo, HI 96720 (United States); Kashikawa, N., E-mail: jmeyers314@berkeley.edu [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Collaboration: Supernova Cosmology Project; and others

2012-05-01T23:59:59.000Z

318

PULSATING REVERSE DETONATION MODELS OF TYPE Ia SUPERNOVAE. I. DETONATION IGNITION  

SciTech Connect

Observational evidences point to a common explosion mechanism of Type Ia supernovae based on a delayed detonation of a white dwarf (WD). Although several scenarios have been proposed and explored by means of one, two, and three-dimensional simulations, the key point still is the understanding of the conditions under which a stable detonation can form in a destabilized WD. One of the possibilities that have been invoked is that an inefficient deflagration leads to the pulsation of a Chandrasekhar-mass WD, followed by formation of an accretion shock around a carbon-oxygen rich core. The accretion shock confines the core and transforms kinetic energy from the collapsing halo into thermal energy of the core, until an inward moving detonation is formed. This chain of events has been termed Pulsating Reverse Detonation (PRD). In this work we explore the robustness of the detonation ignition for different PRD models characterized by the amount of mass burned during the deflagration phase, M {sub defl}. The evolution of the WD up to the formation of the accretion shock has been followed with a three-dimensional hydrodynamical code with nuclear reactions turned off. We found that detonation conditions are achieved for a wide range of M {sub defl}. However, if the nuclear energy released during the deflagration phase is close to the WD binding energy ({approx}0.46 x 10{sup 51} erg {yields} M {sub defl} {approx} 0.30 M {sub sun}) the accretion shock cannot heat and confine the core efficiently and detonation conditions are not robustly achieved.

Bravo, Eduardo; GarcIa-Senz, Domingo [Department de FIsica i Enginyeria Nuclear, Universitat Politecnica de Catalunya, Diagonal 647, 08028 Barcelona (Spain)], E-mail: eduardo.bravo@upc.edu, E-mail: domingo.garcia@upc.edu

2009-04-20T23:59:59.000Z

319

The effect of turbulent intermittency on the deflagration to detonation transition in SN Ia explosions  

E-Print Network (OSTI)

We examine the effects of turbulent intermittency on the deflagration to detonation transition (DDT) in Type Ia supernovae. The Zel'dovich mechanism for DDT requires the formation of a nearly isothermal region of mixed ash and fuel that is larger than a critical size. We primarily consider the hypothesis by Khokhlov et al. and Niemeyer and Woosley that the nearly isothermal, mixed region is produced when the flame makes the transition to the distributed regime. We use two models for the distribution of the turbulent velocity fluctuations to estimate the probability as a function of the density in the exploding white dwarf that a given region of critical size is in the distributed regime due to strong local turbulent stretching of the flame structure. We also estimate lower limits on the number of such regions as a function of density. We find that the distributed regime, and hence perhaps DDT, occurs in a local region of critical size at a density at least a factor of 2-3 larger than predicted for mean conditions that neglect intermittency. This factor brings the transition density to be much larger than the empirical value from observations in most situations. We also consider the intermittency effect on the more stringent conditions for DDT by Lisewski et al. and Woosley. We find that a turbulent velocity of $10^8$ cm/s in a region of size $10^6$ cm, required by Lisewski et al., is rare. We expect that intermittency gives a weaker effect on the Woosley model with stronger criterion. The predicted transition density from this criterion remains below $10^7$ g/cm$^3$ after accounting for intermittency using our intermittency models.

Liubin Pan; J. Craig Wheeler; John Scalo

2008-03-12T23:59:59.000Z

320

THE DETONATION MECHANISM OF THE PULSATIONALLY ASSISTED GRAVITATIONALLY CONFINED DETONATION MODEL OF Type Ia SUPERNOVAE  

SciTech Connect

We describe the detonation mechanism composing the 'pulsationally assisted' gravitationally confined detonation (GCD) model of Type Ia supernovae. This model is analogous to the previous GCD model reported in Jordan et al.; however, the chosen initial conditions produce a substantively different detonation mechanism, resulting from a larger energy release during the deflagration phase. The resulting final kinetic energy and {sup 56}Ni yields conform better to observational values than is the case for the 'classical' GCD models. In the present class of models, the ignition of a deflagration phase leads to a rising, burning plume of ash. The ash breaks out of the surface of the white dwarf, flows laterally around the star, and converges on the collision region at the antipodal point from where it broke out. The amount of energy released during the deflagration phase is enough to cause the star to rapidly expand, so that when the ash reaches the antipodal point, the surface density is too low to initiate a detonation. Instead, as the ash flows into the collision region (while mixing with surface fuel), the star reaches its maximally expanded state and then contracts. The stellar contraction acts to increase the density of the star, including the density in the collision region. This both raises the temperature and density of the fuel-ash mixture in the collision region and ultimately leads to thermodynamic conditions that are necessary for the Zel'dovich gradient mechanism to produce a detonation. We demonstrate feasibility of this scenario with three three-dimensional (3D), full star simulations of this model using the FLASH code. We characterized the simulations by the energy released during the deflagration phase, which ranged from 38% to 78% of the white dwarf's binding energy. We show that the necessary conditions for detonation are achieved in all three of the models.

Jordan, G. C. IV; Graziani, C.; Weide, K.; Norris, J.; Hudson, R.; Lamb, D. Q. [Flash Center for Computational Science, University of Chicago, Chicago, IL 60637 (United States); Fisher, R. T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States); Townsley, D. M. [Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487 (United States); Meakin, C. [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Reid, L. B. [NTEC Environmental Technology, Subiaco WA 6008 (Australia)

2012-11-01T23:59:59.000Z

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321

Off-center ignition in type Ia supernova: I. Initial evolution and implications for delayed detonation  

E-Print Network (OSTI)

The explosion of a carbon-oxygen white dwarf as a Type Ia supernova is known to be sensitive to the manner in which the burning is ignited. Studies of the pre-supernova evolution suggest asymmetric, off-center ignition, and here we explore its consequences in two- and three-dimensional simulations. Compared with centrally ignited models, one-sided ignitions initially burn less and release less energy. For the distributions of ignition points studied, ignition within two hemispheres typically leads to the unbinding of the white dwarf, while ignition within a small fraction of one hemisphere does not. We also examine the spreading of the blast over the surface of the white dwarf that occurs as the first plumes of burning erupt from the star. In particular, our studies test whether the collision of strong compressional waves can trigger a detonation on the far side of the star as has been suggested by Plewa et al. (2004). The maximum temperature reached in these collisions is sensitive to how much burning and expansion has already gone on, and to the dimensionality of the calculation. Though detonations are sometimes observed in 2D models, none ever happens in the corresponding 3D calculations. Collisions between the expansion fronts of multiple bubbles also seem, in the usual case, unable to ignite a detonation. "Gravitationally confined detonation" is therefore not a robust mechanism for the explosion. Detonation may still be possible in these models however, either following a pulsation or by spontaneous detonation if the turbulent energy is high enough.

F. K. Roepke; S. E. Woosley; W. Hillebrandt

2006-09-04T23:59:59.000Z

322

A Three-Dimensional Picture of the Delayed-Detonation Model of Type Ia Supernovae  

E-Print Network (OSTI)

Deflagration models poorly explain the observed diversity of SNIa. Current multidimensional simulations of SNIa predict a significant amount of, so far unobserved, carbon and oxygen moving at low velocities. It has been proposed that these drawbacks can be resolved if there is a sudden jump to a detonation (delayed detonation), but this kind of models has been explored mainly in one dimension. Here we present new three-dimensional delayed detonation models in which the deflagraton-to-detonation transition (DDT) takes place in conditions like those favored by one-dimensional models. We have used a SPH code adapted to SNIa with algorithms devised to handle subsonic as well as supersonic combustion fronts. The starting point was a C-O white dwarf of 1.38 solar masses. When the average density on the flame surface reached 2-3x10^7 g/cm^3 a detonation was launched. The detonation wave processed more than 0.3 solar masses of carbon and oxygen, emptying the central regions of the ejecta of unburned fuel and raising its kinetic energy close to the fiducial 10^51 ergs expected from a healthy Type Ia supernova. The final amount of 56Ni synthesized also was in the correct range. However, the mass of carbon and oxygen ejected is still too high. The three-dimensional delayed detonation models explored here show an improvement over pure deflagration models, but they still fail to coincide with basic observational constraints. However, there are many aspects of the model that are still poorly known (geometry of flame ignition, mechanism of DDT, properties of detonation waves traversing a mixture of fuel and ashes). Therefore, it will be worth pursuing its exploration to see if a good SNIa model based on the three-dimensional delayed detonation scenario can be obtained.

Eduardo Bravo; Domingo Garcia-Senz

2007-12-04T23:59:59.000Z

323

Timescale stretch parameterization of Type Ia supernova B-band light curves  

SciTech Connect

R-band intensity measurements along the light curve of Type Ia supernovae discovered by the Cosmology Project (SCP) are fitted in brightness to templates allowing a free parameter the time-axis width factor w identically equal to s times (1+z). The data points are then individually aligned in the time-axis, normalized and K-corrected back to the rest frame, after which the nearly 1300 normalized intensity measurements are found to lie on a well-determined common rest-frame B-band curve which we call the ''composite curve.'' The same procedure is applied to 18 low-redshift Calan/Tololo SNe with Z < 0.11; these nearly 300 B-band photometry points are found to lie on the composite curve equally well. The SCP search technique produces several measurements before maximum light for each supernova. We demonstrate that the linear stretch factor, s, which parameterizes the light-curve timescale appears independent of z, and applies equally well to the declining and rising parts of the light curve. In fact, the B band template that best fits this composite curve fits the individual supernova photometry data when stretched by a factor s with chi 2/DoF {approx} 1, thus as well as any parameterization can, given the current data sets. The measurement of the data of explosion, however, is model dependent and not tightly constrained by the current data. We also demonstrate the 1 + z light-cure time-axis broadening expected from cosmological expansion. This argues strongly against alternative explanations, such as tired light, for the redshift of distant objects.

Goldhaber, G.; Groom, D.E.; Kim, A.; Aldering, G.; Astier, P.; Conley, A.; Deustua, S.E.; Ellis, R.; Fabbro, S.; Fruchter, A.S.; Goobar, A.; Hook, I.; Irwin, M.; Kim, M.; Knop, R.A.; Lidman, C.; McMahon, R.; Nugent, P.E.; Pain, R.; Panagia, N.; Pennypacker, C.R.; Perlmutter, S.; Ruiz-Lapuente, P.; Schaefer, B.; Walton, N.A.; York, T.

2001-04-01T23:59:59.000Z

324

Exploring Cosmological Expansion Parametrizations with the Gold SnIa Dataset  

E-Print Network (OSTI)

We use the SnIa Gold dataset to compare LCDM with 10 representative parametrizations of the recent Hubble expansion history $H(z)$. For the comparison we use two statistical tests; the usual $\\chi_{min}^2$ which is insensitive to the parametrization number of parameters, and a statistic we call the p-test which depends on both the value of $\\chi_{min}^2$ and the number $n$ of the parametrization parameters. The p-test measures the confidence level to which the parameter values corresponding to LCDM are excluded from the viewpoint of the parametrization tested. For example, for a linear equation of state parametrization $w(z)=w_0 + w_1 z$ the LCDM parameter values ($w_0=-1$, $w_1=0$) are excluded at 75% confidence level. We use a flat prior and $\\Omega_{0m}=0.3$. All parametrizations tested are consistent with the Gold dataset at their best fit. According to both statistical tests, the worst fits among the 10 parametrizations, correspond to the Chaplygin gas, the brane world and the Cardassian parametrizations. The best fit is achieved by oscillating parametrizations which can exclude the parameter values corresponding to LCDM at 85% confidence level. Even though this level of significance does not provide a statistically significant exclusion of LCDM (it is less than $2\\sigma$) and does not by itself constitute conclusive evidence for oscillations in the cosmological expansion, when combined with similar independent recent evidence for oscillations coming from the CMB and matter power spectra it becomes an issue worth of further investigation.

R. Lazkoz; S. Nesseris; L. Perivolaropoulos

2005-11-10T23:59:59.000Z

325

Table 2 -Lime use and practices on Corn, major producing states, 2001 CO GA IL IN IA KS KY MI MN MO NE NY NC ND OH PA SD TX WI Area  

E-Print Network (OSTI)

Table 2 - Lime use and practices on Corn, major producing states, 2001 CO GA IL IN IA KS KY MI MN.7 Table 2 - Lime use and practices on Corn, major producing states, 2000 CO IL IN IA KS KY MI MN MO NE NY use and practices on Corn, major producing states, 1999 CO IL IN IA KS KY MI MN MO NE NC OH SD TX WI

Kammen, Daniel M.

326

The Peninsula Chicago The Peninsula Chicago  

E-Print Network (OSTI)

is located at the top of the hotel. All guestrooms and suites feature marble bathrooms with separate shower

Pritchard, Jonathan

327

Fisica Geral IA (2010/1) Nome 1 2 3 R1 R2 R3 Media Conc  

E-Print Network (OSTI)

Fisica Geral IA (2010/1) Nome 1 2 3 R1 R2 R3 M´edia Conc 1 ANDERSON SILVEIRA SALDANHA 0.5 5.2 4.7 0.7 3.5 4.5 1.5 - - 3.57 D M´edia 2.60 4.64 5.93 5.54 6.08 8.37 4.60 #12;20 40 60 80 100 A B C D FF 23

Stariolo, Daniel Adrián

328

First detection of $^{56}$Co gamma-ray lines from type Ia supernova (SN2014J) with INTEGRAL  

E-Print Network (OSTI)

We report the first ever detection of $^{56}$Co lines at 847 and 1237 keV and a continuum in the 200-400 keV band from the Type Ia supernova SN2014J in M82 with INTEGRAL observatory. The data were taken between 50th and 100th day since the SN2014J outburst. The line fluxes suggest that $0.62\\pm0.13~M\\odot$ of radioactive $^{56}$Ni were synthesized during the explosion. Line broadening gives a characteristic ejecta expansion velocity $V_e\\sim 2100\\pm 500~{\\rm km~s^{-1}}$. The flux at lower energies (200-400 keV) flux is consistent with the three-photon positronium annihilation, Compton downscattering and absorption in the $\\sim~1.4~M\\odot$ ejecta composed from equal fractions of iron-group and intermediate-mass elements and a kinetic energy $E_k\\sim 1.4~10^{51}~{\\rm erg}$. All these parameters are in broad agreement with a "canonical" model of an explosion of a Chandrasekhar-mass White Dwarf (WD), providing an unambiguous proof of the nature of Type Ia supernovae as a thermonuclear explosion of a solar mass co...

Churazov, E; Isern, J; Kndlseder, J; Jean, P; Lebrun, F; Chugai, N; Grebenev, S; Bravo, E; Sazonov, S; Renaud, M

2014-01-01T23:59:59.000Z

329

Chasing the phantom: A closer look at type Ia supernovae and the dark energy equation of state  

Science Journals Connector (OSTI)

Some recent observations provide >2? evidence for phantom dark energya value of the dark energy equation of state less than the cosmological-constant value of ?1. We focus on constraining the equation of state by combining current data from the most mature geometrical probes of dark energy: type Ia supernovae (SNe Ia) from the Supernova Legacy Survey (SNLS3), the Supernova Cosmology Project (Union2.1), and the Pan-STARRS1 survey (PS1); cosmic microwave background measurements from Planck and WMAP9; and a combination of measurements of baryon acoustic oscillations. The combined data are consistent with w=?1 for the Union2.1 sample, though they present moderate (?1.9?) evidence for a phantom value when either the SNLS3 or PS1 sample is used instead. We study the dependence of the constraints on the redshift, stretch, color, and host galaxy stellar mass of SNe, but we find no unusual trends. In contrast, the constraints strongly depend on any external H0 prior: a higher adopted value for the direct measurement of the Hubble constant (H0?71??km/s/Mpc) leads to ?2? evidence for phantom dark energy. Given Planck data, we can therefore make the following statement at 2? confidence: either the SNLS3 and PS1 data have systematics that remain unaccounted for or the Hubble constant is below 71??km/s/Mpc; else the dark energy equation of state is indeed phantom.

Daniel L. Shafer and Dragan Huterer

2014-03-06T23:59:59.000Z

330

Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution  

E-Print Network (OSTI)

We have discovered 16 Type Ia supernovae (SNe Ia) with the Hubble Space Telescope (HST) and have used them to provide the first conclusive evidence for cosmic deceleration that preceded the current epoch of cosmic acceleration. These objects, discovered during the course of the GOODS ACS Treasury program, include 6 of the 7 highest-redshift SNe Ia known, all at z>1.25, and populate the Hubble diagram in unexplored territory. The luminosity distances to these and 170 previous SNe Ia are provided. A purely kinematic interpretation of the SN Ia sample provides evidence at the > 99% confidence level for a transition from deceleration to acceleration or similarly, strong evidence for a cosmic jerk. Using a simple model of the expansion history, the transition between the two epochs is constrained to be at z=0.46 +/- 0.13. The data are consistent with the cosmic concordance model of Omega_M ~ 0.3, Omega_Lambda~0.7 (chi^2_dof=1.06), and are inconsistent with a simple model of evolution or dust as an alternative to dark energy. For a flat Universe with a cosmological constant. When combined with external flat-Universe constraints we find w=-1.02 + 0.13 - 0.19 (and $dark energy, P = w\\rho c^2. Joint constraints on both the recent equation of state of dark energy, $w_0$, and its time evolution, dw/dz, are a factor of ~8 more precise than its first estimate and twice as precise as those without the SNe Ia discovered with HST. Our constraints are consistent with the static nature of and value of w expected for a cosmological constant (i.e., w_0 = -1.0, dw/dz = 0), and are inconsistent with very rapid evolution of dark energy. We address consequences of evolving dark energy for the fate of the Universe.

Adam G. Riess; Louis-Gregory Strolger; John Tonry; Stefano Casertano; Henry C. Ferguson; Bahram Mobasher; Peter Challis; Alexei V. Filippenko; Saurabh Jha; Weidong Li; Ryan Chornock; Robert P. Kirshner; Bruno Leibundgut; Mark Dickinson; Mario Livio; Mauro Giavalisco; Charles C. Steidel; Narciso Benitez; Zlatan Tsvetanov

2004-02-23T23:59:59.000Z

331

Failed-detonation Supernovae: Subluminous Low-velocity Ia Supernovae and their Kicked Remnant White Dwarfs with Iron-rich Cores  

Science Journals Connector (OSTI)

Type Ia supernovae (SNe Ia) originate from the thermonuclear explosions of carbon-oxygen (C-O) white dwarfs (WDs). The single-degenerate scenario is a well-explored model of SNe Ia where unstable thermonuclear burning initiates in an accreting, Chandrasekhar-mass WD and forms an advancing flame. By several proposed physical processes, the rising, burning material triggers a detonation, which subsequently consumes and unbinds the WD. However, if a detonation is not triggered and the deflagration is too weak to unbind the star, a completely different scenario unfolds. We explore the failure of the gravitationally confined detonation mechanism of SNe Ia, and demonstrate through two-dimensional and three-dimensional simulations the properties of failed-detonation SNe. We show that failed-detonation SNe expel a few 0.1 M ? of burned and partially burned material and that a fraction of the material falls back onto the WD, polluting the remnant WD with intermediate-mass and iron-group elements that likely segregate to the core forming a WD whose core is iron rich. The remaining material is asymmetrically ejected at velocities comparable to the escape velocity from the WD, and in response, the WD is kicked to velocities of a few hundred km s1. These kicks may unbind the binary and eject a runaway/hypervelocity WD. Although the energy and ejected mass of the failed-detonation SN are a fraction of typical thermonuclear SNe, they are likely to appear as subluminous low-velocity SNe Ia. Such failed detonations might therefore explain or are related to the observed branch of peculiar SNe Ia, such as the family of low-velocity subluminous SNe (SN 2002cx/SN 2008ha-like SNe).

George C. Jordan, IV; Hagai B. Perets; Robert T. Fisher; Daniel R. van Rossum

2012-01-01T23:59:59.000Z

332

FAILED-DETONATION SUPERNOVAE: SUBLUMINOUS LOW-VELOCITY Ia SUPERNOVAE AND THEIR KICKED REMNANT WHITE DWARFS WITH IRON-RICH CORES  

SciTech Connect

Type Ia supernovae (SNe Ia) originate from the thermonuclear explosions of carbon-oxygen (C-O) white dwarfs (WDs). The single-degenerate scenario is a well-explored model of SNe Ia where unstable thermonuclear burning initiates in an accreting, Chandrasekhar-mass WD and forms an advancing flame. By several proposed physical processes, the rising, burning material triggers a detonation, which subsequently consumes and unbinds the WD. However, if a detonation is not triggered and the deflagration is too weak to unbind the star, a completely different scenario unfolds. We explore the failure of the gravitationally confined detonation mechanism of SNe Ia, and demonstrate through two-dimensional and three-dimensional simulations the properties of failed-detonation SNe. We show that failed-detonation SNe expel a few 0.1 M{sub Sun} of burned and partially burned material and that a fraction of the material falls back onto the WD, polluting the remnant WD with intermediate-mass and iron-group elements that likely segregate to the core forming a WD whose core is iron rich. The remaining material is asymmetrically ejected at velocities comparable to the escape velocity from the WD, and in response, the WD is kicked to velocities of a few hundred km s{sup -1}. These kicks may unbind the binary and eject a runaway/hypervelocity WD. Although the energy and ejected mass of the failed-detonation SN are a fraction of typical thermonuclear SNe, they are likely to appear as subluminous low-velocity SNe Ia. Such failed detonations might therefore explain or are related to the observed branch of peculiar SNe Ia, such as the family of low-velocity subluminous SNe (SN 2002cx/SN 2008ha-like SNe).

Jordan, George C. IV; Van Rossum, Daniel R. [Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637 (United States); Perets, Hagai B. [Physics Department, Technion, Israel Institute of Technology, Haifa 32000 (Israel); Fisher, Robert T. [Department of Physics, University of Massachusetts Dartmouth, 285 Old Westport Road, North Dartmouth, MA 02740 (United States)

2012-12-20T23:59:59.000Z

333

He H`ike no ka Ho`opihapiha `ia o ka Pepa Noi Komo no ka Papahana Ho`omkaukau Kumu `iwi `o Kahuawaiola  

E-Print Network (OSTI)

45 a `oi ma ka pae 300 a ma luna a`e paha a e k ana n koina `lelo a mo`omeheu Hawai`i e helu `ia nei`omeheu Hawai`i. 7. ka puka `ana ma ho`okahi o n papa penei: HWST 205, 471, 472, 473, 474; a i `ole ka `ae a ka `ekolu kau kona l`ihi i kkulu `ia no ka ho`omkaukau `ana i n kumu Mauli Ola Hawai`i no ka ho`ona`auao ma

Wiegner, Tracy N.

334

Summary of the Geographic Information System workshop, held in Chicago, Illinois, May 29--30, 1991. Final report, December 1989--December 1991  

SciTech Connect

The Gas Research Institute, in conjunction with Argonne National Laboratory, sponsored a workshop on May 29--30, 1991, in Chicago, Illinois, to give gas utilities the opportunity to learn about the availability, applications, and benefits of Geographic Information Systems (GISs). This report is a synopsis of that workshop and contains brief discussions, followed by copies of the viewgraphs shown at the workshop, for the following GIS topics: (1) introduction to GIS, (2) data development, (3) analytical functions, (4) use for gas pipeline right-of-way applications, and (5)video imaging and simulation.

Thompson, P J; Sullivan, R G; Sundell, R C; Messersmith, J [Argonne National Lab., IL (United States)] [Argonne National Lab., IL (United States)

1991-12-01T23:59:59.000Z

335

Foreword to Special Issue: Papers from the 52nd Annual Meeting of the APS Division of Plasma Physics, Chicago, Illinois, USA, 2010  

SciTech Connect

We present in this Special Issue of Physics of Plasmas the review, tutorial, and invited papers of the 2010 Annual Meeting of the American Physical Society's (APS) Division of Plasma Physics. This was the 52nd year of this meeting, and it was held in Chicago, Illinois on 8-12 November 2010. The meeting program was made up of over 100 review, tutorial, and invited oral presentations, and a significant fraction of these speakers prepared manuscripts which were peer-reviewed and are contained in this Special Issue.

Allen, Steve L. [Lawrence Livermore National Laboratory, Livermore, California 94550 (United States); Davidson, Ronald C. [Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543 (United States)

2011-05-15T23:59:59.000Z

336

[The Journal of Geology, 2014, volume 122, p. 381396] 2014 by The University of Chicago. All rights reserved. 0022-1376/2014/12204-0003$15.00. DOI: 10.1086/675908  

E-Print Network (OSTI)

[The Journal of Geology, 2014, volume 122, p. 381­396] 2014 by The University of Chicago. All, University of Brighton, Brighton BN2 4GJ, United Kingdom; 2. Department of Geological Sciences, University provided a reference for (U-Th)/He dating on relatively young uranium-poor apatites. The combined data

Min, Kyoungwon

337

3/26/13 Section of brain does more than expected, Universityof Chicago scientists find -chicagotribune.com www.chicagotribune.com/health/ct-x-monkeys-processing-visual-information-0320-20130320,0,298755.story 1/3  

E-Print Network (OSTI)

- chicagotribune.com www.chicagotribune.com/health/ct-x-monkeys-processing-visual-information-0320 of brain does more than expected, Universityof Chicago scientists find - chicagotribune.com www.chicagotribune.com/health/ct-x-monkeys-processing and troubleshooting HOME PROTECTION PLANS From foundation to fixtures FESTIVAL OF HOMES Five financial things every

Freedman, David J.

338

Enforcement Letter - Chicago  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

16, 2002 16, 2002 Dr. Peter Paul, [ ] Brookhaven Science Associates Brookhaven National Laboratory Building 460 P.O. Box 5000 Upton, NY 11973-5000 Subject: Enforcement Letter Dear Dr. Paul: This letter refers to an evaluation by the Department of Energy (DOE) of three reports of noncompliances with quality assurance and/or occupational radiation protection provisions of DOE's nuclear safety requirements occurring at Brookhaven National Laboratory (BNL). These issues, described below, were reported into the Noncompliance Tracking System (NTS) by your staff and involved procurement and/or control of radioactive sources. 1. On January 19, 2001, BNL reported that an [radioactive] neutron source in an unlabeled package had been moved from a posted High Radiation Area to radiologically controlled

339

Presentations | MMSNF 2013 Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

Privacy and Security Notice Presentations Available Presentations from the Materials Modeling and Simulation of Nuclear Fuels (MMSNF) 2013 workshop. Presented on Presentation Title Authors Session Oct. 14, 2013 Welcome and announcements Ewing, Tom (ANL, USA) and Rosner, Robert (UC, USA) Opening Oct. 14, 2013 First-principles DFT+U modeling of paramagnetic UO2 and (U,Pu) mixed oxides [366KB, posted: Oct. 13, 2013 ] Dorado, Boris (CEA, DAM, DIF, France), Garcia, Philippe (CEA, DEN, DEC, France) Atomistic Models and Simulations Oct. 14, 2013 Computational study of energetics and defect-ordering tendencies for rare earth elements in uranium dioxide [1.5MB, posted: Oct. 28, 2013 ] Solomon, Jonathan M. (UC Berkeley, USA), Alexandrov, Vitaly (UC Berkeley, UC Davis, USA), Sadigh, Babak (LLNL, USA), Navrotsky, Alexandra (UC Davis, USA), Asta, Mark (UC Berkeley, UC Davis, USA) Atomistic Models and Simulations

340

MMSNF 2013 Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

Program: Program: Last Modified: Oct. 14, 2013 Privacy and Security Notice Program The Materials Modeling and Simulation of Nuclear Fuels (MMSNF) workshop series aims at stimulating research and discussions on models and simulations of nuclear fuels and coupling the results into fuel performance codes, with the hope that this leads to improved fuel designs. Although centered on multi-scale model development and computer simulations, close connections to theory, experiment and technology are encouraged. In addition to research focused on existing or improved types of LWR reactors, efforts also exist internationally to develop innovative nuclear fuels and materials for future generations of nuclear reactors. A key rationale behind this workshop is to contribute toward improving the

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341

Posters | MMSNF 2013 Chicago  

NLE Websites -- All DOE Office Websites (Extended Search)

Privacy and Security Notice Privacy and Security Notice Posters Available Posters from the Materials Modeling and Simulation of Nuclear Fuels (MMSNF) 2013 workshop. Presented on Poster Title Author(s) ID Session Oct. 14, 2013 Atomistic simulation of radiation damage of metallic and oxide fuels by swift heavy ion irradiation Starikov, Sergey (JIHT RAS, Russia), Pisarev, Vasily (JIHT RAS, Russia), Kuksin, Alexey (JIHT RAS, Russia), Stegailov, Vladimir (JIHT RAS, Russia) PA4 A Oct. 14, 2013 Density functional theory for fission products transport in UO2 [2.5MB, posted: Oct. 28, 2013 ] Ducher, Roland (IRSN, France), Dubourg, Roland (IRSN, France) PA5 A Oct. 14, 2013 Kinetic Monte Carlo study of oxygen defect migration in urania fuel Hoffman III, Richard T. (GA Tech, USA), Bahera, Rakesh (GA Tech, USA), Deo, Chaitanya S. (GA Tech, USA) PA7 A

342

Enforcement Letter - Chicago  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Shirley Strum-Kenny Shirley Strum-Kenny [ ] Stony Brook University Hospital Administration Building, Room 310 Stony Brook, NY 11794-0701 Subject: Enforcement Letter (NTS-CH-BH-BNL-BNL-1998-0004) EA-1999-02 Dear Dr. Strum-Kenny: This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances concerning an event at the Radiation Therapy Facility (RTF) occurring in March 1998. In November 1998, DOE conducted an investigation to determine whether violations of DOE's nuclear safety rules associated with the event had occurred. The resulting Investigation Summary Report was transmitted to you on February 19, 1999. On March 11, 1999, you participated in an Enforcement Conference, along with Brookhaven Science Associates (BSA) management, to discuss the occurrence, its

343

AAAS Chicago Meeting  

Science Journals Connector (OSTI)

...toward automation. Shown in operation will be the Szent-Gyorgyi...facil-ities the company now has in operation in Baton Rouge, La., and...method of converting ordinary boiler steam into pyrogen-free...beam parametric amplifier in operation. This is a vacuum tube which...

Raymond L. Taylor

1959-12-04T23:59:59.000Z

344

Chicago Radiocarbon Dates V  

Science Journals Connector (OSTI)

...the early pottery making groups that has been estimated...18. This site, which falls in the Late Horizon, is...Indian House Pit in Oregon (Klamath House): Indian house...indication of wheni the main group of these paiait-ings...

W. F. Libby

1954-11-05T23:59:59.000Z

345

Anniversary in Chicago  

Science Journals Connector (OSTI)

... And the contract has just been signed for southern California's combined nuclear power and desalination plant, expected to be not only the world's biggest, but one of the ...

1967-12-02T23:59:59.000Z

346

University of Chicago Description  

E-Print Network (OSTI)

? The first self-sustaining, synthetic nuclear reaction occurred in an underground racket ball court or in International House (a private entity affiliated with the University) and housing is guaranteed for students who submit their application on time. Details are available on the Housing Office website. Courses

Bristol, University of

347

AAAS Chicago Meeting  

Science Journals Connector (OSTI)

...in their own fields. Other featured...Congeners (fusel oil, alde-hydes...radiography of production parts, and...the entire cumulative case-history...television production. We will also...products and production tech-niques...rotor and a field-align-ing...Association, Illinois Chapter Booth...

Raymond L. Taylor

1959-12-04T23:59:59.000Z

348

AAAS Chicago Meeting  

Science Journals Connector (OSTI)

...special needs; conducts fundamental research in measurement...stellite and standard engine exhaust valves after...principle prod-ucts-diesel electric locomotives...for utili-ties, and diesel-electric power for...standard sterilization cycle. "Time" scope labels...

Raymond L. Taylor

1959-12-04T23:59:59.000Z

349

Discover Northwestern: Chicago Campus  

E-Print Network (OSTI)

, visit www.fueleconomy.gov to find your vehicle's fuel economy. Annual fuel consumption x Price per the true cost of your commute? COMPARE YOUR ANNUAL COMMUTING COSTS: DRIVING ALONE PUBLIC TRANSIT 1. FUEL $ $ Determine your fuel costs through the following calculations: One-way distance (miles) to work or transit

Shahriar, Selim

350

Testing Models of Intrinsic Brightness Variations in Type Ia Supernovae, and their Impact on Measuring Cosmological Parameters  

E-Print Network (OSTI)

For spectroscopically confirmed type Ia supernovae we evaluate models of intrinsic brightness variations with detailed data/Monte-Carlo comparisons of the dispersion in the following quantities: Hubble-diagram scatter, color difference (B-V-c) between the true B-V color and the fitted color (c) from the SALT-II light curve model, and photometric redshift residual. The data sample includes 251 ugriz light curves from the 3-season Sloan Digital Sky Survey-II, and 191 griz light curves from the Supernova Legacy Survey 3-year data release. We find that the simplest model of a wavelength independent (coherent) scatter is not adequate, and that to describe the data the intrinsic scatter model must have wavelength-dependent variations. We use Monte Carlo simulations to examine the standard approach of adding a coherent scatter term in quadrature to the distance-modulus uncertainty in order to bring the reduced chi2 to unity when fitting a Hubble diagram. If the light curve fits include model uncertainties with the c...

Kessler, Richard; Marriner, John; Betoule, Marc; Brinkmann, Jon; Cinabro, David; El-Hage, Patrick; Frieman, Joshua; Jha, Saurabh; Mosher, Jennifer; Schneider, Donald P

2012-01-01T23:59:59.000Z

351

THE EFFECT OF THE PRE-DETONATION STELLAR INTERNAL VELOCITY PROFILE ON THE NUCLEOSYNTHETIC YIELDS IN TYPE Ia SUPERNOVA  

SciTech Connect

A common model of the explosion mechanism of Type Ia supernovae is based on a delayed detonation of a white dwarf. A variety of models differ primarily in the method by which the deflagration leads to a detonation. A common feature of the models, however, is that all of them involve the propagation of the detonation through a white dwarf that is either expanding or contracting, where the stellar internal velocity profile depends on both time and space. In this work, we investigate the effects of the pre-detonation stellar internal velocity profile and the post-detonation velocity of expansion on the production of {alpha}-particle nuclei, including {sup 56}Ni, which are the primary nuclei produced by the detonation wave. We perform one-dimensional hydrodynamic simulations of the explosion phase of the white dwarf for center and off-center detonations with five different stellar velocity profiles at the onset of the detonation. In order to follow the complex flows and to calculate the nucleosynthetic yields, approximately 10,000 tracer particles were added to every simulation. We observe two distinct post-detonation expansion phases: rarefaction and bulk expansion. Almost all the burning to {sup 56}Ni occurs only in the rarefaction phase, and its expansion timescale is influenced by pre-existing flow structure in the star, in particular by the pre-detonation stellar velocity profile. We find that the mass fractions of the {alpha}-particle nuclei, including {sup 56}Ni, are tight functions of the empirical physical parameter {rho}{sub up}/v{sub down}, where {rho}{sub up} is the mass density immediately upstream of the detonation wave front and v{sub down} is the velocity of the flow immediately downstream of the detonation wave front. We also find that v{sub down} depends on the pre-detonation flow velocity. We conclude that the properties of the pre-existing flow, in particular the internal stellar velocity profile, influence the final isotopic composition of burned matter produced by the detonation.

Kim, Yeunjin; Jordan, G. C. IV; Graziani, Carlo; Lamb, D. Q.; Truran, J. W. [Astronomy Department, University of Chicago, Chicago, IL 60637 (United States); Meyer, B. S. [Physics and Astronomy Department, Clemson University, Clemson, SC 29634 (United States)

2013-07-01T23:59:59.000Z

352

Neutron Diffraction Residual Strain Tensor Measurements Within The Phase IA Weld Mock-up Plate P-5  

SciTech Connect

Oak Ridge National Laboratory (ORNL) has worked with NRC and EPRI to apply neutron and X-ray diffraction methods to characterize the residual stresses in a number of dissimilar metal weld mockups and samples. The design of the Phase IA specimens aimed to enable stress measurements by several methods and computational modeling of the weld residual stresses. The partial groove in the 304L stainless steel plate was filled with weld beads of Alloy 82. A summary of the weld conditions for each plate is provided in Table 1. The plates were constrained along the long edges during and after welding by bolts with spring-loaded washers attached to the 1-inch thick Al backing plate. The purpose was to avoid stress relief due to bending of the welded stainless steel plate. The neutron diffraction method was one of the methods selected by EPRI for non-destructive through thickness strain and stress measurement. Four different plates (P-3 to P-6) were studied by neutron diffraction strain mapping, representing four different welding conditions. Through thickness neutron diffraction strain mappings at NRSF2 for the four plates and associated strain-free d-zero specimens involved measurement along seven lines across the weld and at six to seven depths. The mountings of each plate for neutron diffraction measurements were such that the diffraction vector was parallel to each of the three primary orthogonal directions of the plate: two in-plane directions, longitudinal and transverse, and the direction normal to the plate (shown in left figure within Table 1). From the three orthogonal strains for each location, the residual stresses along the three plate directions were calculated. The principal axes of the strain and stress tensors, however, need not necessarily align with the plate coordinate system. To explore this, plate P-5 was selected for examination of the possibility that the principal axes of strain are not along the sample coordinate system axes. If adequate data could be collected the goal would be to determine the strain tensor's orientation and magnitude of strain along each principle axis direction.

Hubbard, Camden R [ORNL

2011-09-01T23:59:59.000Z

353

TESTING MODELS OF INTRINSIC BRIGHTNESS VARIATIONS IN TYPE Ia SUPERNOVAE AND THEIR IMPACT ON MEASURING COSMOLOGICAL PARAMETERS  

SciTech Connect

For spectroscopically confirmed Type Ia supernovae we evaluate models of intrinsic brightness variations with detailed data/Monte Carlo comparisons of the dispersion in the following quantities: Hubble-diagram scatter, color difference (B - V - c) between the true B - V color and the fitted color (c) from the SALT-II light curve model, and photometric redshift residual. The data sample includes 251 ugriz light curves from the three-season Sloan Digital Sky Survey-II and 191 griz light curves from the Supernova Legacy Survey 3 year data release. We find that the simplest model of a wavelength-independent (coherent) scatter is not adequate, and that to describe the data the intrinsic-scatter model must have wavelength-dependent variations resulting in a {approx}0.02 mag scatter in B - V - c. Relatively weak constraints are obtained on the nature of intrinsic scatter because a variety of different models can reasonably describe this photometric data sample. We use Monte Carlo simulations to examine the standard approach of adding a coherent-scatter term in quadrature to the distance-modulus uncertainty in order to bring the reduced {chi}{sup 2} to unity when fitting a Hubble diagram. If the light curve fits include model uncertainties with the correct wavelength dependence of the scatter, we find that this approach is valid and that the bias on the dark energy equation-of-state parameter w is much smaller ({approx}0.001) than current systematic uncertainties. However, incorrect model uncertainties can lead to a significant bias on the distance moduli, with up to {approx}0.05 mag redshift-dependent variation. This bias is roughly reduced in half after applying a Malmquist bias correction. For the recent SNLS3 cosmology results, we estimate that this effect introduces an additional systematic uncertainty on w of {approx}0.02, well below the total uncertainty. This uncertainty depends on the choice of viable scatter models and the choice of supernova (SN) samples, and thus this small w-uncertainty is not guaranteed in future cosmology results. For example, the w-uncertainty for SDSS+SNLS (dropping the nearby SNe) increases to {approx}0.04.

Kessler, Richard; Frieman, Joshua A. [Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States)] [Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Guy, Julien; Betoule, Marc; El-Hage, Patrick [Laboratoire de Physique Nucleaire et des Hautes Energies, UPMC Univ. Paris 6, UPD Univ. Paris 7, CNRS IN2P3, 4 place Jussieu, F-75005 Paris (France)] [Laboratoire de Physique Nucleaire et des Hautes Energies, UPMC Univ. Paris 6, UPD Univ. Paris 7, CNRS IN2P3, 4 place Jussieu, F-75005 Paris (France); Marriner, John [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States)] [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Brinkmann, Jon [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States)] [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); Cinabro, David [Department of Physics, Wayne State University, Detroit, MI 48202 (United States)] [Department of Physics, Wayne State University, Detroit, MI 48202 (United States); Jha, Saurabh [Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States)] [Department of Physics and Astronomy, Rutgers University, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Mosher, Jennifer [Department of Physics and Astronomy, University of Pennsylvania, 203 South 33rd Street, Philadelphia, PA 19104 (United States)] [Department of Physics and Astronomy, University of Pennsylvania, 203 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P., E-mail: kessler@kicp.uchicago.edu [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States)

2013-02-10T23:59:59.000Z

354

Planning for the Transition to Long-Term Stewardship at Three U.S. Department of Energy-Chicago Operations Office Facilities  

SciTech Connect

This paper describes a pilot study that resulted in the generation of draft planning documents for the upcoming transition from remediation construction to long-term stewardship at three national laboratories managed by the U.S. Department of Energy (DOE)-Chicago Operations Office (CH). The remediation construction work at these facilities is being completed under the DOE's Office of Environmental Management (EM) Program. Once the remediation is complete, the responsibility for long-term stewardship (LTS) of the closed waste sites is expected to be transferred to the DOE organization responsible for managing each of the three facilities (i.e., the site landlord). To prepare for this transfer, an extensive planning effort is required. This pilot study utilized the DOE guidance in effect at the time to (1) develop a series of documents identifying applicable requirements that the LTS Programs will need to satisfy, issues that need to be resolved before the transfer can proceed, and criteria to be used to determine when active remediation is complete and a given site is ready for transfer to the LTS Program; (2) examine alternate structures for possible LTS Programs; and (3) develop draft LTS Implementation Plans. This advanced planning effort yielded a number of observations and lessons learned that are applicable to any facility approaching the end of its remediation construction phase.

Moos, L. P.; Ditmars, J. D.; Heston, S. L.; Granzen, G. A.; Holzemer, M. J.; Bennett, D. B.

2003-02-26T23:59:59.000Z

355

Gorchakova-IA  

NLE Websites -- All DOE Office Websites (Extended Search)

Mokhov Oboukhov Institute of Atmospheric Physics Russian Academy of Sciences Moscow, Russia T. B. Zhuravleva Institute of Atmospheric Optics Tomsk, Russia Introduction Study of...

356

Variations ia Variscan Granites  

Science Journals Connector (OSTI)

... the compositional variations within the Caledonian belt, may both be attributed to variations in the geothermal gradient. In Nature Physical Science this week (April 2), he takes these studies ... studies a stage further by showing that the correlation within the belt between composition and geothermal gradient also applies to the Variscan granites.

1973-04-06T23:59:59.000Z

357

IA News Archive  

Office of Environmental Management (EM)

field-type-text-with-summary field-label-hidden">

U.S. Secretary of Energy Ernest Moniz traveled...

358

Competition between $\\beta$-delayed proton and $\\beta$-delayed $\\gamma$ decay of the exotic $T_z$ = -2 nucleus $^{56}$Zn and fragmentation of the IAS  

E-Print Network (OSTI)

A very exotic decay mode at the proton drip-line, $\\beta$-delayed $\\gamma$-proton decay, has been observed in the $\\beta$ decay of the $T_z$ = -2 nucleus $^{56}$Zn. Three $\\gamma$-proton sequences have been observed following the $\\beta$ decay. The fragmentation of the IAS in $^{56}$Cu has also been observed for the first time. The results were reported in a recent publication. At the time of publication the authors were puzzled by the competition between proton and $\\gamma$ decays from the main component of the IAS. Here we outline a possible explanation based on the nuclear structure properties of the three nuclei involved, namely $^{56}$Zn, $^{56}$Cu and $^{55}$Ni, close to the doubly magic nucleus $^{56}$Ni. From the fragmentation of the Fermi strength and the excitation energy of the two populated 0$^{+}$ states we could deduce the off-diagonal matrix element of the charge-dependent part of the Hamiltonian responsible for the mixing. These results are compared with the decay of $^{55}$Cu with one proton ...

Rubio, B; Fujita, Y; Blank, B; Gelletly, W; Agramunt, J; Algora, A; Ascher, P; Bilgier, B; Cceres, L; Cakirli, R B; Fujita, H; Ganioglu, E; Gerbaux, M; Giovinazzo, J; Grvy, S; Kamalou, O; Kozer, H C; Kucuk, L; Kurtukian-Nieto, T; Molina, F; Popescu, L; Rogers, A M; Susoy, G; Stodel, C; Suzuki, T; Tamii, A; Thomas, J C

2015-01-01T23:59:59.000Z

359

Expectations for the Hard X-ray Continuum and Gamma-ray Line Fluxes from the Type Ia supernova SN 2014J in M82  

E-Print Network (OSTI)

The hard X-ray continuum and gamma-ray lines from a Type Ia supernova dominate its integrated photon emissions and can provide unique diagnostics of the mass of the ejecta, the $^{56}$Ni yield and spatial distribution, its kinetic energy and expansion speed, and the mechanism of explosion. Such signatures and their time behavior "X-ray" the bulk debris field in direct fashion, and do not depend upon the oftimes problematic and elaborate UV, optical, and near-infrared spectroscopy and radiative transfer that have informed the study of these events for decades. However, to date no hard photons have ever been detected from a Type Ia supernova in explosion. With the advent of the supernova SN 2014J in M82, at a distance of $\\sim$3.5 Mpc, this situation may soon change. Both NuSTAR and INTEGRAL have the potential to detect SN 2014J, and, if spectra and light curves can be measured, would usefully constrain the various explosion models published during the last $\\sim$thirty years. In support of these observational ...

The, Lih-Sin

2014-01-01T23:59:59.000Z

360

DOE - Office of Legacy Management -- Iowa State University Ames Laboratory  

Office of Legacy Management (LM)

Iowa State University Ames Iowa State University Ames Laboratory - IA 01 FUSRAP Considered Sites Site: Iowa State University Ames Laboratory (IA.01 ) Eliminated from further consideration under FUSRAP Designated Name: Not Designated Alternate Name: None Location: Wallace Road , Ames , Iowa IA.01-1 IA.01-2 Evaluation Year: Circa 1985 IA.01-3 Site Operations: Produced uranium and thorium metal, recovered uranium scrap, and conducted studies and experimental investigations in connection with chemistry and metallurgy of natural uranium and its allied forms. IA.01-1 IA.01-4 IA.01-5 IA.01-6 IA.01-7 Site Disposition: Eliminated - Referred to Chicago Operations Office for appropriate action IA.01-6 Radioactive Materials Handled: Yes Primary Radioactive Materials Handled: Uranium, Thorium IA.01-1

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While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

RELATIVISTIC SHOCK BREAKOUTS-A VARIETY OF GAMMA-RAY FLARES: FROM LOW-LUMINOSITY GAMMA-RAY BURSTS TO TYPE Ia SUPERNOVAE  

SciTech Connect

The light from a shock breakout of stellar explosions, which carries a wealth of information, strongly depends on the shock velocity at the time of the breakout. The emission from Newtonian breakouts, typical in regular core-collapse supernovae (SNe), has been explored extensively. However, a large variety of explosions result in mildly or ultrarelativistic breakouts, where the observed signature is unknown. Here we calculate the luminosity and spectrum produced by relativistic breakouts. In order to do so, we improve the analytic description of relativistic radiation-mediated shocks and follow the system from the breakout itself, through the planar phase and into the spherical phase. We limit our calculation to cases where the post-breakout acceleration of the gas ends during the planar phase (i.e., the final gas Lorentz factor {approx}< 30). We find that spherical relativistic breakouts produce a flash of gamma rays with energy, E{sub bo}, temperature, T{sub bo}, and duration, t{sup obs} b{sub o}, that provide the breakout radius ( Almost-Equal-To 5 R{sub Sun }(t{sup obs}{sub bo}/10 s)(T{sub bo}/50 keV){sup 2}) and the Lorentz factor ( Almost-Equal-To T{sub bo}/50 keV). They also always satisfy a relativistic breakout relation (t{sup obs}{sub bo}/20 s) {approx} (E{sub bo}/10{sup 46} erg){sup 1/2}(T{sub bo}/50 keV){sup -2.68}. The breakout flare is typically followed, on longer timescales, by X-rays that carry a comparable energy. We apply our model to a variety of explosions, including Type Ia and .Ia SNe, accretion-induced collapse, energetic SNe, and gamma-ray bursts (GRBs). We find that all these events produce detectable gamma-ray signals, some of which may have already been seen. Some particular examples are: (1) relativistic shock breakouts provide a natural explanation to the energy, temperature, and timescales of low-luminosity GRBs. Indeed, all observed low-luminosity GRBs satisfy the relativistic breakout relation. (2) Nearby broad-line Type Ib/c (like SN 2002ap) may produce a detectable {gamma}-ray signal. (3) Galactic Type Ia SNe may produce detectable {gamma}-ray flares. We conclude that relativistic shock breakouts provide a generic process for the production of gamma-ray flares.

Nakar, Ehud [Raymond and Beverly Sackler School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978 (Israel); Sari, Re'em [Racah Institute for Physics, Hebrew University, Jerusalem 91904 (Israel)

2012-03-10T23:59:59.000Z

362

Solar Wind: Manifestations of Solar Activity E N CYC LO PE D IA O F AS T R O N O MY AN D AS T R O PHYS I C S Solar Wind: Manifestations of Solar  

E-Print Network (OSTI)

Solar Wind: Manifestations of Solar Activity E N CYC LO PE D IA O F AS T R O N O MY AN D AS T R O PHYS I C S Solar Wind: Manifestations of Solar Activity The Sun's outer atmosphere, the corona, is continually heated and expands to create the solar wind. Solar activity waxes and wanes with the 11 yr cycle

Webb, David F.

363

Projected rotational velocities of WD1614+136 and WD1353+409 - implications for the rate of galactic Type Ia supernovae  

E-Print Network (OSTI)

The white dwarf stars WD1614+136 and WD1353+409 are not sufficiently massive to have formed through single star evolution. However, observations to date have not yet found any evidence for binarity. It has therefore been suggested that these stars are the result of a merger. In this paper we place an upper limit of approximately 50kms on the projected rotational velocities of both stars. This suggests that, if these stars are the results of a merger, efficient angular momentum loss with accompanying mass loss must have occurred. If the same process occurs following the merging of more massive white dwarf stars, the predicted rate of Type Ia supernovae due to merging white dwarfs may have been greatly over-estimated. Further observations to determine binarity in WD1614+136 and WD1353+409 are therefore encouraged.

P. F. L. Maxted; T. R. Marsh

1998-03-17T23:59:59.000Z

364

Chandra Observation of the Cluster of Galaxies MS 0839.9+2938 at z=0.194: the Central Excess Iron and SN Ia Enrichment  

E-Print Network (OSTI)

We present the Chandra study of the intermediately distant cluster of galaxies MS 0839.9+2938. By performing both the projected and deprojected spectral analyses, we find that the gas temperature is approximately constant at about 4 keV in 130-444h_70^-1 kpc. In the inner regions, the gas temperature descends towards the center, reaching sun yr^-1 and 96-126 M_sun yr^-1, respectively within 74h_70^-1 kpc where the gas is significantly colder. Along with the temperature drop, we detect a significant inward iron abundance increase from about 0.4 solar in the outer regions to about 1 solar within the central 37h_70^-1 kpc. Thus MS 0839.9+2938 is the cluster showing the most significant central iron excess at z>~ 0.2. We argue that most of the excess iron should have been contributed by SNe Ia. By utilizing the observed SN Ia rate and stellar mass loss rate, we estimate that the time needed to enrich the central region with excess iron is 6.4-7.9 Gyr, which is similar to those found for the nearby clusters. Coinciding with the optical extension of the cD galaxy (up to about 30h_70^-1 kpc), the observed X-ray surface brightness profile exhibits an excess beyond the distribution expected by either the beta model or the NFW model, and can be well fitted with an empirical two-beta model that leads to a relatively flatter mass profile in the innermost region.

Yu Wang; Haiguang Xu; Zhongli Zhang; Yueheng Xu; Xiang-Ping Wu; Sui-Jian Xue; Zongwei Li

2005-06-12T23:59:59.000Z

365

Trump International Hotel & Tower Chicago Trump International Hotel & Tower Chicago  

E-Print Network (OSTI)

and detail-oriented amenities, including personal attaché service. 339 graciously appointed guestrooms

Pritchard, Jonathan

366

ChicagoCOLVIN2008.ppt  

NLE Websites -- All DOE Office Websites (Extended Search)

Safe Nanotechnology Safe Nanotechnology Safe Nanotechnology Setting the Stage for Safe Handling Setting the Stage for Safe Handling Dr. Vicki Colvin colvin@rice.edu The World Needs New Innovations! Water purification that is cheaper, better and easier Detecting and curing disease with practical medicine Nanomaterials Can Help Solve Problems BiMetallic Catalysts Removing TCE in water Nanogold on silica Tumor capillary Carcinoma cells Shrinking Tumors 50 nm Magnetite particles Water purification Defining Nanotechnology From E56 ASTM terminology standard - free on www.astm.org nanotechnology, n-A term referring to a wide range of technologies that measure, manipulate, or incorporate materials and/or features with at least one dimension between approximately 1 and 100 nanometers (nm). Such applications exploit those properties, distinct from bulk or molecular systems, of

367

Emily Conover University of Chicago  

E-Print Network (OSTI)

Meeting 4 / 19 #12;12 B selection Look for time correlation between muons and a single event: · energy: 4 >600MeV muon, veto 500 ms · Possible improvement by utilizing additional variables: · Improved muon energy (FIDO) · track length through target or GC · dE/dx (Energy above minimum ionizing) · number

368

Multi-Megawatt Organic Rankine Engine power plant (MORE). Phase IA final report: system design of MORE power plant for industrial energy conservation emphasizing the cement industry  

SciTech Connect

The Multi-Megawatt Organic Rankine Engine (MORE) program is directed towards the development of a large, organic Rankine power plant for energy conservation from moderate temperature industrial heat streams. Organic Rankine power plants are ideally suited for use with heat sources in the temperature range below 1100/sup 0/F. Cement manufacture was selected as the prototype industry for the MORE system because of the range of parameters which can be tested in a cement application. This includes process exit temperatures of 650/sup 0/F to 1110/sup 0/F for suspension preheater and long dry kilns, severe dust loading, multi-megawatt power generation potential, and boiler exhaust gas acid dew point variations. The work performed during the Phase IA System Design contract period is described. The System Design task defines the complete MORE system and its installation to the level necessary to obtain detailed performance maps, equipment specifications, planning of supporting experiments, and credible construction and hardware cost estimates. The MORE power plant design is based upon installation in the Black Mountain Quarry Cement Plant near Victorville, California.

Bair, E.K.; Breindel, B.; Collamore, F.N.; Hodgson, J.N.; Olson, G.K.

1980-01-31T23:59:59.000Z

369

The University of Iowa College of Engineering Engineering Professional Development  

E-Print Network (OSTI)

Naperville, IL City of Rock Island Rock Island, IL City of St. Charles St. Charles, IL City of W. Des Moines Great Lakes Dredge and Dock Chicago, IL Habitat for Humanity Iowa City, IA Hall and Hall EngineersAmericanEnergy Sioux City, IA MNTAP: Valley Craft Lake City, MN Moffat and Nichol Long Beach, CA NextERA Energy (FPL

Jacob, Mathews

370

Consolidative Involved-Node Proton Therapy for Stage IA-IIIB Mediastinal Hodgkin Lymphoma: Preliminary Dosimetric Outcomes From a Phase II Study  

SciTech Connect

Purpose: To compare the dose reduction to organs at risk (OARs) with proton therapy (PT) versus three-dimensional conformal radiotherapy (3D-CRT) and intensity-modulated radiotherapy (IMRT) in patients with mediastinal Hodgkin lymphoma (HL) enrolled on a Phase II study of involved-node radiotherapy (INRT). Methods and Materials: Between June 2009 and October 2010, 10 patients were enrolled on a University of Florida institutional review board-approved protocol for de novo 'classical' Stage IA-IIIB HL with mediastinal (bulky or nonbulky) involvement after chemotherapy. INRT was planned per European Organization for Research and Treatment of Cancer guidelines. Three separate optimized plans were developed for each patient: 3D-CRT, IMRT, and PT. The primary end point was a 50% reduction in the body V4 with PT compared with 3D-CRT or IMRT. Results: The median relative reduction with PT in the primary end point, body V4, was 51% compared with 3D-CRT (p = 0.0098) and 59% compared with IMRT (p = 0.0020), thus all patients were offered treatment with PT. PT provided the lowest mean dose to the heart, lungs, and breasts for all 10 patients compared with either 3D-CRT or IMRT. The median difference in the OAR mean dose reduction with PT compared with 3D-CRT were 10.4 Gy/CGE for heart; 5.5 Gy/CGE for lung; 0.9 Gy/CGE for breast; 8.3 Gy/CGE for esophagus; and 4.1 Gy/CGE for thyroid. The median differences for mean OAR dose reduction for PT compared with IMRT were 4.3 Gy/CGE for heart, 3.1 Gy/CGE for lung, 1.4 Gy/CGE for breast, 2.8 Gy/CGE for esophagus, and 2.7 Gy/CGE for thyroid. Conclusions: All 10 patients benefitted from dose reductions to OARs with PT compared with either 3D-CRT or IMRT. It is anticipated that these reductions in dose to OAR will translate into lower rates of late complications, but long-term follow-up on this Phase II INRT study is needed.

Hoppe, Bradford S., E-mail: bhoppe@floridaproton.org [University of Florida Proton Therapy Institute, Jacksonville, FL (United States); Flampouri, Stella; Su Zhong; Morris, Christopher G. [University of Florida Proton Therapy Institute, Jacksonville, FL (United States); Latif, Naeem [University of Florida Hematology/Oncology, Jacksonville, FL (United States); Dang, Nam H.; Lynch, James [University of Florida Hematology/Oncology, Gainesville, FL (United States); Li Zuofeng; Mendenhall, Nancy P. [University of Florida Proton Therapy Institute, Jacksonville, FL (United States)

2012-05-01T23:59:59.000Z

371

IA_50m_Wind  

NLE Websites -- All DOE Office Websites (Extended Search)

Metadata also available as Metadata: IdentificationInformation DataQualityInformation SpatialDataOrganizationInformation SpatialReferenceInformation EntityandAttributeI...

372

+ . -. . -. . .__ .. .. -..---. ---.. . --. --. -. L IA Science Service Feature  

E-Print Network (OSTI)

, "the bent'' - i.e.9 ''Also it is P l * t l Y the A l l The thermometer reading alone merely tella us with heat vhen the thermometer the temperature of the air to be far below freezing. In Arizona people mny

373

"Report Date","U.S.",,,"PADD I",,,"PADD IA",,,"PADD IB",,,"PADD IC",,,"PADD II"  

U.S. Energy Information Administration (EIA) Indexed Site

Residential Heating Oil Prices (Before and After Change in Aggregation Methodology)" Residential Heating Oil Prices (Before and After Change in Aggregation Methodology)" "Report Date","U.S.",,,"PADD I",,,"PADD IA",,,"PADD IB",,,"PADD IC",,,"PADD II" ,"Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference","Old Reported Value ($ per Gallon)","New Revised Value ($ per Gallon)","Difference"

374

Enforcement Letter -Chicago-02/24/2000  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4, 2000 4, 2000 Yoon I. Chang, PhD [ ] Argonne National Laboratory-East 9700 South Cass Avenue Argonne, IL 60439-4832 Subject: Enforcement Letter (NTS-CH-AA-ANLE-ANLE-1999-0009) Dear Dr. Chang: This letter refers to the Department of Energy's (DOE) evaluation of the facts and circumstances concerning the above referenced Noncompliance Tracking System (NTS) report describing bioassay program deficiencies at Argonne National Laboratory- East (ANL-E). This report was submitted to DOE on December 23, 1999. Approximately thirteen months previous to this NTS report's submittal, DOE's Office of Enforcement and Investigation (EH-Enforcement) issued to all DOE and contractor Price-Anderson Amendments Act coordinators a memorandum explaining EH-Enforcement's experience with and concern regarding contractor bioassay program

375

DOE Office of Science - Chicago Office  

NLE Websites -- All DOE Office Websites (Extended Search)

DEPARTMENT OF ENERGY (DOE) DEPARTMENT OF ENERGY (DOE) In 1977 the Administration and Congress acted to further consolidate federal energy policy, R&D, and nuclear energy defense functions. ERDA was integrated with the Federal Energy Administration and other federal energy functions to create a Cabinet-level U.S. Department of Energy. The governmental elements brought together to form DOE included the Federal Energy Regulatory Commission; the Economic Regulatory Administration; the automotive research and development sections of the Environmental Protection Agency; Solar Research and Development from the National Science Foundation; and Fossil Energy and Development from the Department of the Interior's Office of Coal Research, as well as several Power Administrations.

376

Chicago Operations Office 9800 South Cass Avenue  

Office of Legacy Management (LM)

Office Office 9800 South Cass Avenue Argonne,, Illinois 60439 James L. Liver-man, Acting Assistant Secretary for Environment, HQ THE DOW CHEMICAL COMPANY On December 8, 1977, Edward J. Jascewsky, Department of Energy (DOE), and Walter Smith, Argonne National Laboratory (ANL), visited The Dow Chemical Company, Walnut'Creek, California. The purpose of the visit was to discuss the past operations at these facilities under Atomic Energy Commission (AEC), Contract AT (40-l)-GEN 236, which involved process studies on different uranium ores. Discussions were held with Dr. Charles Levine, Radiation Safety Officer. He identified four rooms (j/l, 2, 18, and 25) in the Research Building that were used during the period of the contract. A survey of the facility was performed by Messrs. Jascewsky and Smith.

377

The University of Chicago Department of Statistics  

E-Print Network (OSTI)

in a parallel fashion by using distributed computing methods such as Folding@Home. The analysis of these large

Stephens, Matthew

378

The University of Chicago Department of Statistics  

E-Print Network (OSTI)

movements of WTI crude oil prices can be observed during the period from 1986 to 2008. Spectral analysis

Stephens, Matthew

379

Public Meeting In Chicago - Rail Infrastructure Presentation  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

average. The railroad cycle time is the time it takes a railroad to move a loaded coal train from the mine to the power plant plus the time it takes to move the train back to the...

380

Great Cities Institute Real-Time Chicago  

E-Print Network (OSTI)

on turnpikes and toll roads. Her book, Paying the Toll: Local Power, Regional Politics, and the Golden Gate Bridge won the Abel Wolman Award of the Public Works Historical Society in 2009. Dyble earned a Ph

Illinois at Chicago, University of

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

Redefining the edge : housing on Chicago's waterfront  

E-Print Network (OSTI)

This thesis proposes an approach to the design of urban housing which uses the public realm to reconcile the various desires of the city for continuous, accessible fabric, the developer for property value raising enhancements, ...

Montalto, Anthony Olindo

1995-01-01T23:59:59.000Z

382

Manufacturing serendipity: Chicago Innovation Exchange enhancing...  

NLE Websites -- All DOE Office Websites (Extended Search)

Releases Feature Stories Science Highlights In the News Experts Guide Media Contacts Social Media Photos Videos Fact Sheets, Brochures and Reports Summer Science Writing...

383

Chicago, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Aerotecture International Inc American Bar Association Section on Environment American Science and Technology Corporation AST Boeing Co Carbon Green BioEnergy LLC Carbon...

384

The University of Chicago Department of Statistics  

E-Print Network (OSTI)

is a Tukey neologism for the term scatterplot diagnostics. Scagnostics are characterizations of the 2D. These characterizations include such measures as density, shape, outliers, and texture. Tukey never published the idea. Paul Tukey discussed it briefly at an IMA workshop on visualization in 1989. We introduce a set

Stephens, Matthew

385

Chicago Area Alternative Fuels Deployment Project (CAAFDP)  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Project Partners in April 2010 * NEPAs Submitted - 100% of OEM Vehicles - 100% of Vehicle Conversions - 100% of Infrastructure * Detailed Project Plan Established for each Project...

386

Chicago Operations Office 9800 South Cass Avenue  

Office of Legacy Management (LM)

On January 17, 1978, Edward J. Jascewsky, Department of Energy (DOE), and Walter H. Smith, Argonne National Laboratory (AX), visited the University of Arizona. The purpose of...

387

Chicago South, Illinois, Site Fact Sheet  

Office of Legacy Management (LM)

Laboratory, and Eckart Hall. Other buildings associated with this site-the New Chemistry Laboratory and Annex, west stands of Stagg Field, and Ricketts Laboratory- have been...

388

The University of Chicago Department of Statistics  

E-Print Network (OSTI)

can be used to test the trends of extremes and variability of climate variables, an important problem cyclone winds. It was found that an inhomogeneous upward trend for cyclone wind speeds is pronounced at high quantile values. However, there is no trend in the mean lifetime-maximum wind speed. This example

Stephens, Matthew

389

IA Blog Archive | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

materials used in four clean energy technologies: wind turbines, electric vehicles, solar cells and energy-efficient lighting. October 1, 2010 Secretary Chu and John Berry...

390

Surface detonation in type Ia supernova explosions?  

E-Print Network (OSTI)

We explore the evolution of thermonuclear supernova explosions when the progenitor white dwarf star ignites asymmetrically off-center. Several numerical simulations are carried out in two and three dimensions to test the consequences of different initial flame configurations such as spherical bubbles displaced from the center, more complex deformed configurations, and teardrop-shaped ignitions. The burning bubbles float towards the surface while releasing energy due to the nuclear reactions. If the energy release is too small to gravitationally unbind the star, the ash sweeps around it, once the burning bubble approaches the surface. Collisions in the fuel on the opposite side increase its temperature and density and may -- in some cases -- initiate a detonation wave which will then propagate inward burning the core of the star and leading to a strong explosion. However, for initial setups in two dimensions that seem realistic from pre-ignition evolution, as well as for all three-dimensional simulations the collimation of the surface material is found to be too weak to trigger a detonation.

F. K. Roepke; S. E. Woosley

2006-09-25T23:59:59.000Z

391

IA News Archive | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

a report on the proposed Keystone XL pipeline project. December 10, 2010 United States-Russia Joint Statement on the Results of the Nuclear Energy and Nuclear Security Working...

392

IA CRYPTOGRAPHIC SERIES THE INDEX OF COINCIDENCE  

E-Print Network (OSTI)

to make assumptions of plain-text equivalents for the cipher letters constituting a message assumptions whatever of plain-text values Jor the cipher letters. It is true that cipher systems admitting employing as many as 125 random mixed secondary alpha- bets can be solved without assuming a plain

Babinkostova, Liljana

393

Type Ia Supernovae Project at NERSC  

NLE Websites -- All DOE Office Websites (Extended Search)

principles is difficult because simulation results are quite sensitive to how the thermonuclear runaway is ignited (e.g., at the center or slightly off center on one side); to...

394

IA Blog Archive | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

between the two countries. June 16, 2014 Ministers Meet in Addis Ababa for U.S.-Africa Energy Ministerial Learn more about the U.S.-Africa Energy Ministerial, held June 3-4,...

395

The University of Iowa College of Engineering Engineering Professional Development  

E-Print Network (OSTI)

Naperville, IL City of Rock Island Rock Island, IL City of St. Charles St. Charles, IL City of W. Des Moines and Marshall Grapevine, TX Great Lakes Dredge and Dock Chicago, IL Habitat for Humanity Iowa City, IA Hall MidAmerican Energy Sioux Falls, SD MNTAP: Valley Craft Lake City, MN Moffat and Nichol Long Beach, CA

Casavant, Tom

396

DEPARTMENT OF ENGLISH & LINGUISTICS  

E-Print Network (OSTI)

. Louis, MO Actress, Stage Left, Chicago, IL Assistant to Artistic Director, Immediacy Theatre Project Case Manager, Liberty Mutual Group; Kansas City, MO Editorial Assistant in Health Professions; Elsevier, AmeriCorps; Hawley, MA Iowa Attorney General; Des Moines, IA Librarian; Liberty, MO Missouri State

Gering, Jon C.

397

Forthcoming Events  

Science Journals Connector (OSTI)

...Dental Assoc., Los Angeles, Calif. (H. Hillenbrand, ADA, 2'' E. SLipCrior St.. Chicago. Ill.) 17-21. NeuLtron Pilc Research, svmp., Vienna. Austl-ia. (Internlational Atomic Iner(gs Agency. 11 Kirntner Ring. Vi-enna I) 17-22...

1960-09-23T23:59:59.000Z

398

Oak Ridge Associated Universities  

Office of Legacy Management (LM)

Facility and Site Decommissioning U.S. Department of Energy ORAU 89lA-42 VERIFICATION OF REMEDIAL ACTION ON VENTILATION SYSTEMS JONES CHEMICAL LABORATORY UNIVERSITY OF CHICAGO CHICAGO, ILLINOIS M. R. LANDIS Radiological Site Assessment Program Manpower Education, Research, and Training Division FINAL REPORT JANUARY 1989 ORAU 89IA-42 3 VERIFICATION OF REMEDIAL ACTION ON VENTILATION SYSTEMS JONES CHEMICAL LABORATORY UNIVERSITY OF CHICAGO CHICAGO, ILLINOIS Prepared by M.R. Landis Radiological Site Assessment Program Manpower Education, Research, and Training Division Oak Ridge Associated Universities Oak Ridge, TN 37831-0117 Project Staff J.D. Berger R.D. Condra J.F. Lisco C.F. Weaver Prepared for U.S. Department of Energy as part of the Formerly Utilized Sites -

399

Berkeley Supernova Ia Program V. Late-time spectra of Type Ia Supernovae  

Science Journals Connector (OSTI)

......normal-velocity objects, the red points HV objects and the black...A. Diamond-Stanic, E. Gates, K. Hiner, M. Kandrashoff...2004) 128:387. Hicken M. , Wood-Vasey W. M., Blondin S...al. ApJ (2009) 699:L139. Wood-Vasey W. M. , et al. ApJ......

Jeffrey M. Silverman; Mohan Ganeshalingam; Alexei V. Filippenko

2013-01-01T23:59:59.000Z

400

1 | EqIA Summary| Diversity Team| 08/12/08 EqIA Summary  

E-Print Network (OSTI)

, in particular benefits relating to age as there will be a strong focus on bio energy, which will support fuel economy and fuel security issues. Monitoring/Evaluation The Action Plan will be monitored primarily

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

Art Gallery Header Public Access current show schedule contact us cultural events archive General Information Art Gallery Header Public Access current show schedule contact us cultural events archive General Information "I have always felt that science, technology, and art are importantly connected, indeed science and technology seem to many scholars to have grown out of art." -Robert Rathbun Wilson This convergence of art and science occurs daily in the Fermilab Art Gallery. It is a space for art exhibitions, chamber music concerts and where the top quark and big bang are debated over coffee. It is also a quiet space for contemplation and beauty. Current Status of Access to Fermilab Fermilab Examined – a Juried Exhibition by members of the Fermilab Photography Club 11/18/13-1/26/14 Artist Reception 11/20/13 Current Exhibition Upcoming Exhibition

402

South Chicago Heights, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Heights, Illinois: Energy Resources Heights, Illinois: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.4808681°, -87.6378211° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.4808681,"lon":-87.6378211,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

403

Chicago Operations Off ice 9800 South Cass Avenue  

Office of Legacy Management (LM)

3 1977 3 1977 James L. Liverman, Acting Assistant Secretary for Environment, HQ BUREAU OF MINES - UTAH On November 28, 1977, Edward J. Jascewsky, Department of Energy (DOE), and Walter H. Smith, Argonne National Laboratory (ANL), visited the U. S. Bureau of Mines Metallurgy Research Center in Salt Lake City, Utah. The purpose of the visit was to discuss the past operations at the facility that involved work under an Atomic Energy Commission (AEC) contract during the early 1950's. The work performed involved the development of processes for uranium recovery from various types of ore. In addition, a small pilot plant was operated at this site. Discussions were held with William A. McKinney, Research Director, Don Seidel, Research Supervisor, John Baur, Radiation Protection Officer,

404

Chicago Ridge, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

217°, -87.7792196° 217°, -87.7792196° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.7014217,"lon":-87.7792196,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

405

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

General Information General Information Fermilab Arts & Lecture Series Kirk Road & Pine Street, P.O. Box 500, MS 111, Batavia, IL 60510 - 0500 Phone: Voice - 630.840.ARTS(2787), Fax - 630.840.5501 E-Mail: audweb@fnal.gov Tickets are sold on a first-come, first-served basis. Tickets may be charged on MasterCard, Visa, or Discover or paid for by check. Mail Order. Send a check (payable to Fermilab) or charge authorization with a self-addressed, stamped envelope to Fermilab Arts Series, P.O. Box 500, MS111, Batavia, IL 60510-0500. Telephone. For information and tickets call 630/840.ARTS (2787). An answering machine will take your confidential message during times that the box office manager is not available. Box Office Hours. At present our box office is being staffed on a part-time

406

West Chicago, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Illinois: Energy Resources Illinois: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 41.8847507°, -88.2039607° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.8847507,"lon":-88.2039607,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

407

Chicago Heights, Illinois: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

46°, -87.6355995° 46°, -87.6355995° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.506146,"lon":-87.6355995,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

408

From the Chicago Pile 1 to next-generation reactors  

Science Journals Connector (OSTI)

The aim of this contribution is that of presenting a simple, elementary description of the nuclear reactor physics, a science which had its beginning more than half a century ago with the Enrico Fermi and his ...

Augusto Gandini

2004-01-01T23:59:59.000Z

409

Chicago Office NEPA Tracking Number U. S. DEPARTMENT OF ENERGY  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

Important Farmland Non-Attainment Areas for Ambient Air Quality Standards Class I Air Quality Control Region Special Sources of Groundwater (e.g. Sole Source Aquifer)...

410

Chicago Office (SC-CH) Integrated Support Center Qualifying Official...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

issue the trainee, you are ready to issue certification. You should sign or initial the ESS record or qualification card, as applicable. The certification is issued by a letter...

411

Appropriate-Technology Small-Grants Program, Chicago Operations Office  

SciTech Connect

Grants totaling $1,290,837 were awarded during FY 1979 to 60 program participants in Illinois, Indiana, Michigan, Minnesota, Ohio and Wisconsin. Review showed that some grantees misused grant monies and did not comply with grant provisions primarily due to insufficient on-site monitoring of the grantees' progress and expenditures. Recommendations to achieve the objectives of the program were: more timely and systematic monitoring; curtail or stop funds for grant projects with unsatisfactory progress or of questionable merit; substantiate expenditures by grantees before disbursing grant funds; and consider increasing program management capability by staffing alternatives. Corrective action taken or planned by the Manager/Regional Representative is identified in an appendix. (PSB)

Not Available

1981-05-29T23:59:59.000Z

412

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

you will find no entrance. The building is encapsulated; it is a space-trap, a great cavern with all its potential for expressing apartness, mystery and entombment. It serves as...

413

CHICAGO HOUSE PARTIES SHOW WAYS TO UPGRADE | Department of Energy  

Energy Savers (EERE)

created Energy Impact Illinois (EI2) to promote home energy upgrades in single-family homes, multifamily housing units, and commercial buildings to help the region meet its 2008...

414

Proceedingsof the American Control Conference Chicago, Illinois June 2000  

E-Print Network (OSTI)

, engine clutch, CVT, electric motor, lead-acid battery, vehicle driveline, hydraulic brakes powertrain [3]. Parallel Hybrid Electric Vehicles (PHEV) are HEVs configured such that the electric motor of the vehicle's power ultimately comes from fuel. The battery is recharged by using the electric motor

Peng, Huei

415

Proceedingsof the American Control Conference Chicago, Illinois June 2000  

E-Print Network (OSTI)

Hangzhou, 310027, P. R. China jwu@iipc .zju.edu.cn Gang Li The school of EEE Singapore egli@ntu are presented to illustrate the effectiveness of the pro- posed strategy. Index Terms-Finite word length-point arith- metic. The FWL effects have been well studied in digital sig- nal processing, especially

Chen, Sheng

416

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

quantities in the Electroweak sector of particle physics, including measurements of Higgs boson couplings, and searches for new physics, specifically supersymmetry. Hildreth has...

417

Dylan Hatt, Sean Johnson The University of Chicago  

E-Print Network (OSTI)

summary: Relationship between wind speed and energy? #12; Particles collide with turbine Transfer of these 6000 sq. mi? Go to Google maps and look at the Rail Splitter Wind Farm in IL See 16 turbines in 4 sq. mi. So estimate (6000 sq. mi.)*(16 turbines)/(4 sq. mi.) ~ 20,000 turbines in Illinois #12;Illinois

Collar, Juan I.

418

DavidB. Malament Chicago and La Salle,lllinois  

E-Print Network (OSTI)

J/Roment angular momentum ("ZAM criterion"). The other is castin terms of the "compassof inertia" on the axis("CIA and CIA criteria. Third, I'll abstracttwo (seemingly)modestconditions of adequacythat one might expect

Barrett, Jeffrey A.

419

QER Public Meeting in Chicago, IL: Rail, Barge, Truck Transportation...  

Energy Savers (EERE)

- Statement Henri Boulet, Executive Director, LA-1 Coalition - Presenation Chris Smith, Senior Program Manager for Freight, the American Association of State Highway and...

420

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

success of the scientific progress and applications they enable. Katsouleas will review progress toward a new accelerator paradigm based on plasmas capable of dramatically...

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Archived Reference Climate Zone: 5A Chicago, Illinois  

Energy.gov (U.S. Department of Energy (DOE))

Here you will find past versions of the commercial reference building models for existing buildings constructed before 1980, organized by building type and location. A summary ofbuilding types and climate zonesis available for reference.Current versionsare also available.

422

Archived Reference Climate Zone: 5A Chicago, Illinois  

Energy.gov (U.S. Department of Energy (DOE))

Here you will find past versions of the commercial reference building models for existing buildings constructed in or after 1980, organized by building type and location. A summary of building types and climate zones is available for reference. Current versions are also available.

423

Focus Series - Chicago-Energy Impact Illinois (EI2)  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

an opportunity to try a different strategy-one that relied more on a community-based, boots-on-the-ground outreach campaign. Through a "house party" initiative, EI2 brought...

424

Alternative Fuels Data Center: City of Chicago Program Encourages...  

Alternative Fuels and Advanced Vehicles Data Center (EERE)

to more than 1,500 vehicles. To maximize petroleum displacement, the city developed a "lockout" policy for its FFVs: Using the existing fuel management system, the fleet requires...

425

Benefits of Prospective Commissioning for Condominiums in Chicago  

E-Print Network (OSTI)

, and maintainability of the CC were questioned by management staff and the residents. The management staff of the building had no ?as-built? drawing to consult as they addressed resident complaints, which limited their effectiveness. Design issues that surfaced... in the building. Perhaps the most egregious design issue was the failure of the domestic water boilers due to tube fouling. The fouling was caused principally by back-drafting within the boilers themselves; not only a mechanical equipment maintenance issue...

Chimack, M.; Walker, C.

2004-01-01T23:59:59.000Z

426

UNITED STATES ATOMIC ENERGY COMMISSION CHICAGO OPERATIONS OFFICE  

Office of Legacy Management (LM)

or related information regarding: ;: 39th Street Warehouse East Pavilion - Museum of Science and Industry 2: Ryerson Physical Laboratory Drexel House (this has not been...

427

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

in Holography, Photography and Mixed Media by Lori Napoleon, Ed Wesly, and Todd Johnson On Display: 92208 - 111008 92608 - Lecture 12-1pm Curia II - Wilson Hall Artist...

428

Computation Institute Argonne National Lab & University of Chicago  

E-Print Network (OSTI)

;5 #12;6 #12;7 #12;8 "Computation may someday be organized as a public utility ... The computing utility countries, 25 models 8,000 registered users 1,900 registered users Downloads to date · 49 TB · 176,000 files Grid Computing #12;27 #12;28 US$3 #12;29Credit: Werner Vogels #12;30Credit: Werner Vogels #12

Heiser, Gernot

429

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

global scape, rapid retreat of mountain glaciers is not only contributing to global sea level rise, but threatening fresh water supplies in many of the world's most populous...

430

October 34, 2013 | Chicago www.law.northwestern.edu/professionaled  

E-Print Network (OSTI)

and Chief Executive Officer, CDW Corporation, Vernon Hills, Illinois Crane Kenney, President, Business and Corporate Secretary, CDW Corporation, Vernon Hills, Illinois 12:30­1:30 p.m. | Lunch ­ provided 1:30­2:30 p-Employment and Compliance, Brunswick Corporation, Lake Forest, Illinois 2:30­3:30 p.m. | Cross-border Activity: A Focus

Shahriar, Selim

431

Argonne microbial ecologist named to Crain's Chicago Business...  

NLE Websites -- All DOE Office Websites (Extended Search)

Your Health", to be held at the Advanced Photon Source Auditorium on the Argonne campus. Gilbert holds a Ph.D. in Marine Microbiology from the University of Nottingham, UK. To...

432

Community Career Resources CAREER TRANSTIONS CENTER OF CHICAGO  

E-Print Network (OSTI)

Assessments, MTBI and SVII: $50 each - including required interpretation session (membership required) EVANSTON PUBLIC LIBRARY 1703 Orrington Ave. 60201 847-448-8600 www.epl.org Career Counselling on the second-NET CENTER, EVANSTON 1615 Oak Street Evanston, IL 60201 IDES: 1-888-367-4382. http://www.ides.state.il.us/general

Shull, Kenneth R.

433

Chicago Metropolitan Agency for Planning Summary of Reported...  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

could enter their address to find out their MyHomeEQ score, which shows the total energy consumption of their home per square foot. MyHomeEQ also compares their home to...

434

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

Extreme Beams for Mysterious Particles Dr. Regina Rameika April 23, 2010 @ 8 p.m.- Tickets 7 Neutrinos are among the most abundant particles in the universe. The sun is a neutrino...

435

TQP Qualifying Official Training Approaches- Office of Science, Chicago  

Energy.gov (U.S. Department of Energy (DOE))

A QO is an individual who has the technical experience and/or education in a particular technical area and who, with the necessary training, is authorized to sign qualification cards for designated competencies.

436

Argonne Chicago Scholars: Kevin Banks | Argonne National Laboratory  

NLE Websites -- All DOE Office Websites (Extended Search)

--Workplace pipeline Search Show All All Videos Argonne OutLoud: "Computation, Big Data, and the Future of Cities" David Danielson - Assistant Secretary for Energy...

437

Argonne National Laboratory is managed by The University of Chicago  

E-Print Network (OSTI)

medium Metal foam support In-tank HX and manifolds Al liner Carbon fiber Multi-layer vacuum insulation Al-Hydride Hydrogen Storage System Analysis Tool Carbon Fiber LinerGlass Fiber Sintered SS Filter 4% Al Foam H2 HTFWh/L). #12;7 AC H2 Storage System Thermally insulated, filament wound carbon fiber/epoxy PV Super AC powder

438

Chicago Operations Off ice 9800 South Cass Avenue  

Office of Legacy Management (LM)

On December 7, 1977, Edward J. Jascewsky, Department of Energy (DOE), and Walter H. Smith, Argonne National Laboratory (ANL), visited the Colorado School of Mines Research...

439

Chicago Operations Off ice 9800 South Cass Avenue  

Office of Legacy Management (LM)

On November 29, 1977, Edward J. Jascewsky, Department of Energy (DOE), and Walter H. Smith, Argonne National Laboratory (ANL), visited the University of Utah's Medical Research...

440

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

Imagined Landscape - Melanie P. Brown, Suzanne K. Loechl, Julian E. Williams On Display: December 4, 2014 -January 29, 2015 Artist Reception - December 12 5-7pm Fermilab Art...

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

Light and the Landscape William Worcester On Display: December 8, 2010 - February 4, 2011 Artist Reception -December 10, 2010 5-7pm Fermilab Art Gallery, Wilson Hall Painting...

442

Proceedings of the American Control Conference Chicago, Illinois June 2000  

E-Print Network (OSTI)

coefficient of the valve. The approximation error of the nonlinear flow map- ping is deal with via certain Robust Control of Hydraulic Actuators Regulated by Proportional Directional Control Valves with Deadband-rod hydraulic actuators regulated by proportional directional control(PDC) valves with deadband and nonlinear

Yao, Bin

443

Fermilab Cultural Events in Chicago's Far West Side  

NLE Websites -- All DOE Office Websites (Extended Search)

was so evocatively revisited by Nellie McKay on her recent recording Normal as Blueberry Pie. Songs by the great Billy Strayhorn complete a night of intoxicating revelry. "The...

444

Residents, Alien Policies, and Resistances: Experiences of Undocumented Latina/o Students in Chicagos Colleges and Universities  

E-Print Network (OSTI)

not naturalized U.S. citizens, such as Gabriel, aliens. are four categories that aliens or foreign nationals canare considered illegal aliens or undocumented (Yale-

Diaz-Strong, Daysi; Meiners, Erica

2007-01-01T23:59:59.000Z

445

UNIVERSITY OF ILLINOIS AT CHICAGO 412 SOUTH PEORIA STREET, M/C 348, CHICAGO, IL 60607-7064  

E-Print Network (OSTI)

): 13. (In Chinese). CONFERENCE PRESENTATIONS AND REPORTS Ning Ai. "Challenges of Sustainable Urban. "Integrated Approaches to Promoting Sustainable Urbanization: Experiences at the World Bank." The 9th Energy and Infrastructure Unit Massachusetts Bay Commuter Railroad Company, Cambridge, MA, 10/03 ­ 7

Illinois at Chicago, University of

446

Ij,  

Office of Legacy Management (LM)

nts yocument consists of.. _____ .P __.______ nts yocument consists of.. _____ .P __.______ ' , z 3 *I . . ? c -TV b q ' ? J ,=i Ij, ia .) L pages and ._______ a _________ _ ____._._._.______ figures No...s ____ of ______ d?copies, Series-.-B ____, SERVICE & SUPPLY SUBCOKTRACT #7401-37-146 This subcontract entered into this 28th d;iy of February between The TJniversity of Chicago, ICJ@ by ati a corporation not for-$%&r;? profit organized under the laws of the State of Illir,ois, of Chicago, Illinois (hereinafter called the "ContractorI' and Quality Hardware & Machine-Corp.a organized under the la\js of the State of Illinois corporation (hereinafter called the %ubcontractor.") -.-* of Chicago, Illinois- liJIBR.EAS , the Contractor has heretofore entered into a contract with the

447

K-corrections and spectral templates of Type Ia supernovae  

E-Print Network (OSTI)

discovery that the cosmic expansion is now accelerating; this acceleration is believed to be driven by dark energy,

Hsiao, E. Y.

2008-01-01T23:59:59.000Z

448

Type Ia Supernova Spectral Line Ratios as Luminosity Indicators  

E-Print Network (OSTI)

crucial role in the discovery of the dark energy, v i a theled to the discovery of the "dark energy" (Riess et al.

Bongard, Sebastien; Baron, E.; Smadja, G.; Branch, David; Hauschildt, Peter H.

2005-01-01T23:59:59.000Z

449

Closest Type Ia Supernova in Decades Solves a Cosmic Mystery  

NLE Websites -- All DOE Office Websites (Extended Search)

use to measure cosmic growth, a technique that in 1998 led to the discovery of dark energy - and 13 years later to a Nobel Prize, "for the discovery of the accelerating...

450

The Photometric Properties of Nearby Type Ia Supernovae  

E-Print Network (OSTI)

discovery and subsequent study of the accelerating expansion of the Universe and dark energy (discovery that the Universe is expanding at an accelerating rate, probably due to an unexplained, unidentified dark energy.

Ganeshalingam, Mohan

2012-01-01T23:59:59.000Z

451

Rates, progenitors and cosmic mix of Type Ia supernovae  

Science Journals Connector (OSTI)

......2004) from the supernova survey spin-off of the GOODS project (Giavalisco et al. 2004). The mentioned Gaussian DDT is...fig. 13 in Greggio (2005). For this reason, we take the liberty of re-discussing here the Della Valle et al. interpretation......

Laura Greggio; Alvio Renzini; Emanuele Daddi

2008-08-01T23:59:59.000Z

452

IA Scieaoe Service Foature 1 WHY THE ITEATHER ' 1  

E-Print Network (OSTI)

high, 6 feet wide and 3 feet through can lift a man off his feet in n strong vind, It 0811 raise a mile the leader to go higher. Tsvo miles high is not an uncommon attainment f o r the first kite, nhile four miles increases suddenly, the strain on the wire may reach the breaking point and anay will go the kites and wire

453

Nicolas Turenne @ INRA 2006 1 Sujets Projets IA  

E-Print Network (OSTI)

.62 computer,internet,7.58 plane,car,5.77 LISTING abuse accommodation activity admission airport alcohol

Turenne, Nicolas

454

Math PUrview - Summer 1998 - IAS/Park City Mathematics Institute ...  

E-Print Network (OSTI)

The selected teachers are individuals who are interested in the dual role of initiating reform within their own classrooms and assuming a leadership role in local...

455

2012 Professional Development Meeting; Ames, IA Research update: Bee health  

E-Print Network (OSTI)

, pumpkins · Cantaloupes, watermelons · Carrots, canola, alfalfa · Almonds, macadamia and other nut crops #12+ million ac), most wheat (24 million ac), canola, cotton, etc. · Rates range from 0.25-1.25 mg

Jurenka, Russell A.

456

Burning Thermals in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

. It is generally agreed that they result from the thermonuclear explosion of a white dwarf accreting matter from that a thermonuclear explosion is involved means that a realistic model requires an understanding of both the ignition

457

The Photometric Properties of Nearby Type Ia Supernovae  

E-Print Network (OSTI)

1.1.1 Thermonuclear SNe . . . . . . 1.1.2 Core-Collapseby which they explode: thermonuclear and core collapse.thesis is focused on thermonuclear SNe, I describe the two

Ganeshalingam, Mohan

2012-01-01T23:59:59.000Z

458

SN Ia host galaxy properties and the dust extinction distribution  

Science Journals Connector (OSTI)

......due to the destruction or dispersion of the dusty interstellar medium by stellar winds prior to the ignition of the supernova. In...the possibility that the geometry of the dusty interstellar medium (ISM) (and hence the extinction distribution) may change......

B. W. Holwerda; A. Reynolds; M. Smith; R. C. Kraan-Korteweg

2015-02-01T23:59:59.000Z

459

Microsoft PowerPoint - IEEE IAS PES 102313.pptx  

NLE Websites -- All DOE Office Websites (Extended Search)

Devices in SGIG Projects Results and Case Studies Recent DOE SGIG Reports 15 * Economic Impact of Smart Grid Investments April 2013 * 2012 Progress Report July...

460

Dynamic Optimization of IA-32 Applications Under DynamoRIO  

E-Print Network (OSTI)

programs statically is diminishing. The advent and increased use of shared libraries, dynamic class loading, and runtime binding means that the compiler has, even with difficult to accurately obtain profiling data, less is known and very accurate profiling data can be obtained. This thesis presents two uses of the Dynamo

Amarasinghe, Saman

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

Oddelek za fiziko Seminar Ia -1. letnik, II. stopnja  

E-Print Network (OSTI)

the whole history, the mankind has been facing problems of energy sufficiency and efficiency. Nowadays, when is solar power. The energy of solar photons has already been implemented in solar cells generating electrical energy. But solar energy can be used directly to produce heat and drive a generator as well

?umer, Slobodan

462

Tracked Flame Simulation for Type Ia Yongmin Zhang1  

E-Print Network (OSTI)

tracking of the ame front which is critically important to the accurate modeling of turbulent thermonuclear, and the strength and brightness of the burning are all determined by the speed of thermonuclear burning 12, 13 needs to model the propagation of thermonuclear burning inside the exploding star. The mech- anism

New York at Stoney Brook, State University of

463

LES Simulations of Turbulent Combustion in a Type Ia Supernovae  

E-Print Network (OSTI)

to be thermonuclear explosions of white dwarfs. SNIa are important sources of energy and chemical elements deposited of the burning are all determined by the speed of thermonuclear burning [27]. The problem of turbulent combustion. The mechanism and the speed of thermonuclear burning in SNIa remain an unsolved theoretical problem. A recent

New York at Stoney Brook, State University of

464

Visualizing Buoyant Burning Bubbles in Type Ia Supernovae at...  

NLE Websites -- All DOE Office Websites (Extended Search)

simulation was conducted using a specialized low Mach number hydrodynamics code for thermonuclear flames. Adaptive mesh refinement was used to focus resolution on the bubble,...

465

Cosmology with Type Ia The Sloan Digital Sky Survey  

E-Print Network (OSTI)

- Present) - Cosmic Microwave Background - Supernovae and Dark Energy - Galaxy Clustering SDSS Supernova% of recollapse density · Favors Dark Energy #12;M51: June 2005 M51: July 2005 #12;#12;· Easy to identify · Geometry is flat · ~70% Dark Energy · ~30% Matter · There was a Big Bang · There will be a Big Chill #12

Cinabro, David

466

NJ WY AK AL CA AR CO CT DE FL GA HI ID KS IL IN IA IA KY LA  

Gasoline and Diesel Fuel Update (EIA)

accomplishments accomplishments are impressive in themselves, and associ- ated with each milestone is the expansion of future produc- tion opportunities as another technical barrier is overcome. The extension of recovery opportunities into deep water has established the deep offshore as an area of considerable national significance. A second source of increased supply is gas from coalbed formations. Natural gas production from coalbed methane fields continued to grow in 1996 as projects initiated mainly in the early to mid 1990's matured through the dewatering phase into higher rates of gas production. Coalbed forma- tions contribute almost 1 trillion cubic feet, roughly 5 per- cent, to total U.S. production. Continued production growth from coalbeds is not likely in light of the precipitous drop in new wells completed in coalbed formations since the termination of the production tax

467

Berkeley Supernova Ia Program I. Observations, data reduction and spectroscopic sample of 582 low-redshift Type Ia supernovae  

Science Journals Connector (OSTI)

......Astier et al. ; Riess et al. ; Wood-Vasey et al. ; Hicken et al...with one CCD in each of the red and blue arms of the spectrograph...AJ 112 2408. 45 Hicken M. , Wood-Vasey W. M., Blondin S...A. 1994 AJ 108 2233. 118 Wood-Vasey W. M. 2007 ApJ 666......

Jeffrey M. Silverman; Ryan J. Foley; Alexei V. Filippenko; Mohan Ganeshalingam; Aaron J. Barth; Ryan Chornock; Christopher V. Griffith; Jason J. Kong; Nicholas Lee; Douglas C. Leonard; Thomas Matheson; Emily G. Miller; Thea N. Steele; Brian J. Barris; Joshua S. Bloom; Bethany E. Cobb; Alison L. Coil; Louis-Benoit Desroches; Elinor L. Gates; Luis C. Ho; Saurabh W. Jha; Michael T. Kandrashoff; Weidong Li; Kaisey S. Mandel; Maryam Modjaz; Matthew R. Moore; Robin E. Mostardi; Marina S. Papenkova; Sung Park; Daniel A. Perley; Dovi Poznanski; Cassie A. Reuter; James Scala; Franklin J. D. Serduke; Joseph C. Shields; Brandon J. Swift; John L. Tonry; Schuyler D. Van Dyk; Xiaofeng Wang; Diane S. Wong

2012-09-21T23:59:59.000Z

468

The University of Iowa College of Engineering Engineering Professional  

E-Print Network (OSTI)

Clipper Windpower Cedar Rapids, IA CNH Burlington, IA Crystal Group Hiawatha, IA DENSO International

Casavant, Tom

469

Real-time x-ray absorption spectroscopy of uranium, iron, and manganese in contaminated sediments during bioreduction  

E-Print Network (OSTI)

National Laboratory, Berkeley, California 94720 University of Chicago, Chicago, Illinois 60637 Savannah River

Tokunaga, T.K.

2008-01-01T23:59:59.000Z

470

Long-term stability of organic carbon-stimulated chromate reduction in contaminated soils, and its relation to manganese redox status  

E-Print Network (OSTI)

National Laboratory, Berkeley, California 94720 e 'university of Chicago, Chicago, Illinois 60637 Savannah River

Tokunaga, Tetsu K.; Wan, Jiamin; Lanzirotti, Antonio; Sutton, Steve R.; Newville, Matthew; Rao, William

2007-01-01T23:59:59.000Z

471

U. of I. study casts doubt on bubble fusion report Chicago Tribune; Chicago, Ill.; Jul 25, 2002; Jeremy Manier, Tribune staff reporter;  

E-Print Network (OSTI)

using "cold fusion." Nuclear fusion, the potent energy source that powers the sun and hydrogen bombs on a tabletop, possibly providing a cheap and clean source of energy. In contrast to the cold fusion debacle, Suslick said, "The concept of getting fusion this way is not in any way crackpot--as opposed to cold

Suslick, Kenneth S.

472

Category:Utility Rate Impacts on PV Economics By Location | Open Energy  

Open Energy Info (EERE)

Utility Rate Impacts on PV Economics By Location Utility Rate Impacts on PV Economics By Location Jump to: navigation, search Impact of Utility Rates on PV Economics Montgomery, AL Little Rock, AR Flagstaff, AZ Phoenix, AZ Tucson, AZ Arcata, CA LA, CA San Francisco, CA Boulder, CO Eagle County, CO Pueblo, CO Bridgeport, CT Wilmington, DE Miami, FL Tampa, FL Atlanta, GA Savannah, GA Des Moines, IA Mason, IA Boise, ID Chicago, IL Springfield, IL Indianapolis, IN Goodland, KS Wichita, KS Lexington, KY New Orleans, LA Shreveport, LA Boston, MA Baltimore, MD Caribou, ME Portland, ME Detroit, MI Houghton-Lake, MI Traverse City, MI International Falls, MN Minneapolis, MN Kansas City, MO Jackson, MS Billings, MT Greensboro, NC Wilmington, NC Bismarck, ND Minot, ND Omaha, NE Concord, NH Atlantic City, NJ Albuquerque, NM Las Vegas, NV Reno, NV New York, NY

473

Fermilab Today  

NLE Websites -- All DOE Office Websites (Extended Search)

3, 2004 3, 2004 Calendar Monday, September 13 11:00 a.m. Special Astrophysics Seminar - Curia II Speaker: P. Hoeflich, University of Texas Title: Physics of Type Ia Supernovae for Cosmology: I 2:30 p.m. Theoretical Astrophysics Seminar - Curia II Speaker: C. Wagner, Argonne National Laboratory/University of Chicago Title: Supersymmetry, Dark Matter and Electroweak Baryogenesis 3:30 p.m. DIRECTOR'S COFFEE BREAK - 2nd Flr X-Over 4:00 p.m. All Experimenters' Meeting - Curia II Special Topic: NuMI/MINOS Tuesday, September 14 3:00 p.m. Special Astrophysics Seminar - Curia II Speaker: P. Hoeflich, University of Texas Title: Physics of Type Ia Supernovae for Cosmology: II 3:30 p.m. DIRECTOR'S COFFEE BREAK - 2nd Flr X-Over 4:00 p.m. Accelerator Physics and Technology Seminar - 1 West

474

2013 Annual Workforce Analysis and Staffing Plan Report- Office of Science Chicago Office  

Energy.gov (U.S. Department of Energy (DOE))

Managers perform an annual workforce analysis of their organization and develop staffing plans that identify technical capabilities and positions they need to ensure safe operation of defense nuclear facilities.

475

THE UNIVERSITY OF CHICAGO BAYESIAN ANALYSIS OF GENETIC ASSOCIATION DATA, ACCOUNTING  

E-Print Network (OSTI)

. Finally and most importantly, I thank my wife Mingming Zhang, for her love, trust, support and sacrifice;To Mingming and In Memoriam of My Mom, Zezhi #12;ABSTRACT In this dissertation research, we tackle

Stephens, Matthew

476

Reference Buildings by Climate Zone and Representative City: 5A Chicago, Illinois  

Office of Energy Efficiency and Renewable Energy (EERE)

In addition to the ZIP file for each building type, you can directly view the "scorecard" spreadsheet that summarizes the inputs and results for each location. This Microsoft Excel spreadsheet is also included in the ZIP file. For version 1.4, only the IDF file is included.

477

A U.S. Department of Energy Laboratory Operated by The University of Chicago  

E-Print Network (OSTI)

integration of the hydrogen storage subsystem with the fuel cell (or ICE) power plant #12;6 Pioneering Science virtual center Special Facilities (ANL) (APS, IPNS) Materials & Processes (Others+ANL) Life Cycle Analyses

478

Improving the Field Performance of Natural Gas Furnaces, Chicago, Illinois (Fact Sheet)  

SciTech Connect

The objective of this project is to examine the impact that common installation practices and age-induced equipment degradation may have on the installed performance of natural gas furnaces, as measured by steady-state efficiency and AFUE. PARR identified twelve furnaces of various ages and efficiencies that were operating in residential homes in the Des Moines Iowa metropolitan area and worked with a local HVAC contractor to retrieve them and test them for steady-state efficiency and AFUE in the lab. Prior to removal, system airflow, static pressure, equipment temperature rise, and flue loss measurements were recorded for each furnace. After removal from the field the furnaces were transported to the Gas Technology Institute (GTI) laboratory, where PARR conducted steady-state efficiency and AFUE testing. The test results show that steady-state efficiency in the field was 6.4% lower than that measured for the same furnaces under standard conditions in the lab, which included tuning the furnace input and air flow rate. Comparing AFUE measured under ASHRAE standard conditions with the label value shows no reduction in efficiency for the furnaces in this study over their 15 to 24 years of operation when tuned to standard conditions. Further analysis of the data showed no significant correlation between efficiency change and the age or the rated efficiency of the furnace.

Rothgeb, S.; Brand, L.

2013-11-01T23:59:59.000Z

479

Chicago Office CX Determinations | U.S. DOE Office of Science...  

Office of Science (SC) Website

Monitoring of C02 Sequestration .pdf file (412KB) B3.1, B3.7 09172014 MIT Solid State Solar-Thermal Energy Conversion Center (S3TEC) .pdf file (135KB) B3.6 08012014 DIII-D...

480

E-Print Network 3.0 - airspace chicago il Sample Search Results  

NLE Websites -- All DOE Office Websites (Extended Search)

conditions, this paper assessed Flexible Airspace Management that reconfigures Source: NASA - Center-TRACTION Automation System (CTAS) Collection: Energy Storage, Conversion and...

Note: This page contains sample records for the topic "ia 1970-1981 chicago" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

Evaluating the costs and benefits of increased funding for public transportation in Chicago  

E-Print Network (OSTI)

(cont.) off-peak ridership, is at or slightly below break-even with respect to net benefits if the CTA cost structure and tax source of subsidy remains unchanged. In order to justify any significant additional long-term ...

Schofield, Mark L., 1973-

2004-01-01T23:59:59.000Z

482

PLEASE SCROLL DOWN FOR ARTICLE This article was downloaded by: [UIC University of Illinois at Chicago  

E-Print Network (OSTI)

Occupational and Environmental Hygiene Volume 15(1): 114­119, 2000 Copyright c° 2000 Applied Industrial Hygiene and Personal Sampling in Exposure Estimation Nurtan A. Esmen and Thomas A. Hall Health Sciences Center sampling in exposure assessment, the theory shown also suggests areas of further applied and the- oretical

Illinois at Chicago, University of

483

PLEASE SCROLL DOWN FOR ARTICLE This article was downloaded by: [UIC University of Illinois at Chicago  

E-Print Network (OSTI)

Industrial Hygiene 1047-322X/00 $12.00 + .00 Multicomponent Error Model for Mass Measurement Based Size Fractionating Aerosol Samplers Nurtan A. Esmen Health Sciences Center, University of Oklahoma, Oklahoma City that can be used in occupational and environmental exposure assessment. It took roughly 70 years from

Illinois at Chicago, University of

484

Celebrating Sightings --2008 A Publication of the University of Chicago Divinity School  

E-Print Network (OSTI)

. FRANKLIN 24 Collisions and Doubts MARTIN E. MARTY 25 Billy Graham's Final Crusade JAMES L. EVANS 26 Black MARTIN E. MARTY 29 Buddhists on the Brain DAN ARNOLD 30 The Future of New Orleans JAMES B. BENNETT 32 or Spectacle? CYNTHIA GANO LINDNER 36 Allah's Trailblazer R. JONATHAN MOORE 38 Watch Your Language MARTIN E

He, Chuan

485

Microsoft PowerPoint - How To Do Business with DOE Chicago BOS...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Affairs 541990 - All Other Professional Scientific and Technical Services 541330 - Engineering Services 541611 - Administrative Management and General Management Consulting...

486

THE UNIVERSITY OF CHICAGO UNIFYING FRAMEWORK FOR THE PREDICTION OF PROTEIN FOLDING  

E-Print Network (OSTI)

. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37 2.3.7 Biasing Energies used for sequential stabilization . . . . . . . . . . . 41 2.3.8 Software-native contacts. . . . . . . 51 2.5 Comparison to all atom molecular dynamics simulations . . . . . . . . . . . 61 Simulated Annealing (MCSA) Minimization . . . . . . . 32 2.3.2 Sampling using Ramachandran Maps

Sosnick, Tobin R.

487

A U.S. Department of Energy Laboratory Operated by The University of Chicago  

E-Print Network (OSTI)

Cells, and Infrastructure Technologies Program Systems Analysis Workshop July 28-29, 2004 Washington, D of Hydrogen, Fuel Cells, and Infrastructure Office of FreedomCAR and Vehicle Technologies Office of Budget: HTGR Central Distributed: Nuclear Power Utilization: Fuel Cell + H2 ICE Vehicles Hybrid Electric

488

Title of Project: Ramp High Occupancy Vehicle (HOV) Sponsors: Chicago Metropolitan Agency for Planning  

E-Print Network (OSTI)

: reduced travel delay, value of travel time saved, fuel volume savings, fuel cost savings, reduced vehicle the scope of work: 1. Determine appropriate set of parallel streets to be modeled as alternative routes using planning agency data 7. Input traffic data to the FREQ traffic simulation model for the 2030

Illinois at Chicago, University of

489

ORISE: Chicago No-Notice takes training to a higher standard  

NLE Websites -- All DOE Office Websites (Extended Search)

One day was spent entirely on classroom and hands-on training, including reviewing conduct of operations within the Incident Command System construct-deemed the gold...

490

Chicago 54, Ill. United Stat.s Department of the Interior  

E-Print Network (OSTI)

sandwiched between two !lerkle insulating pads. By placing the dry ice between the packages of f ish fillets, a flexible l4-ply Merkle insulation pad ,was used below the dry ice, and a 6-ply flexible pad over it when. In later experiments, the insulation under the dry ice was changed to a rigid 6- ply Merkle pad, It inches

491

FACILITIES ENGINEER WEST CHICAGO Execute capital projects for manufacturing facilities and utilities systems: scope development, cost  

E-Print Network (OSTI)

facilities and utilities systems: scope development, cost estimation, system design, equipment sizing ENGINEERING: Lead capital project design, development and execution for facility and utility capital Utilities systems (Vacuum, Hydraulics, Waste Water treatment, etc.) o Buildings and grounds, including

Heller, Barbara

492

Microsoft Word - DOE-ID-13-052 Chicago EC B3-6.doc  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

- It is expected that about 1 liter of waste stream containing 2 grams of depleted uranium will be generated each year. The waste will be stored in the lab inside a vented hood...

493

Secretary Moniz Announces Travel to Chicago, North Dakota, New Mexico for Quadrennial Energy Review  

Energy.gov (U.S. Department of Energy (DOE))

Energy Secretary Ernest Moniz will host several meetings on the Quadrennial Energy Review (QER) and visit the Waste Isolation Pilot Plant in early August.

494

Mapping out the "hotspots": Examining the spatial patterns of heat morbidity in Chicago, Illinois  

E-Print Network (OSTI)

.242 % HH alone 0.233 % no vehicle 0.183 % 1 room 0.182 % Hispanic -0.178 % Black 0.159 % institutionalized · % HH alone & over 65 yrs old · % over 65 years old · % Hispanic (-) · % no vehicle r2 = 0 65 yrs old · % householder alone · % separated · % widowed · % divorced · % naturalized

Hall, Sharon J.

495

A Question of Priority: Small at Chicago or Blackmar at Kansas?  

E-Print Network (OSTI)

" and the history of social thought. This is the conclusion Jones and Kronus (1976, p. 8) drew from their survey of 792 ASA members (Full, Associate, and Foreign) in 1974 (with 445 usable returns). And since specialists within those four subfields of...- the ... discipline amount to only a minority of ASA membership, it is fair to assume that most American sociologists care a 'good deal about sociology's past. For example, fully 96.2% (428) of the respondents believe Durkheim is. "still worthwhile reading," with 424...

Sica, Alan

1990-01-01T23:59:59.000Z

496

ENERGY RESEARCH AND DEVELOPMENT ADMlNlSTRATldN CHICAGO OPERATIONS...  

Office of Legacy Management (LM)

within ERDA or burial as active waste with J' the exceptions of a hydraulic tank and pumps which will be shipped to a licensed radioactive waste burial ground for disposal. 2....

497

THE UNIVERSITY OF CHICAGO AN UPPER BOUND ON THE FREE ENERGY OF THE TRANSITION STATE  

E-Print Network (OSTI)

.........................................................................................vii Chapter 1 Introduction to Protein Folding ................................................................................ 1 1.1 Why study protein folding ...................................................................................4 1.2 Transition States of Protein Folding Pathways

Sosnick, Tobin R.

498

2008 WIND TECHNOLOGIES MARKET REPORT  

E-Print Network (OSTI)

J. 2009. Presentation at WINDPOWER 2009, Chicago, Illinois,and EPC Price Trends. WINDPOWER 2009, Chicago, Illinois,in the Downturn." WINDPOWER 2009, Chicago, Illinois, May 5,

Bolinger, Mark

2010-01-01T23:59:59.000Z

499

Mitigation, Adaptation, Uncertainty -- Growing Water  

E-Print Network (OSTI)

Water project was inspired by three historic Chicago engineering feats: the reversal of the Chicago River, the Deep

Felsen, Martin; Dunn, Sarah

2008-01-01T23:59:59.000Z

500

1861 The Meteoritical Society, 2008. Printed in USA. Meteoritics & Planetary Science 43, Nr 11, 18611877 (2008)  

E-Print Network (OSTI)

of Chicago, 5640 S. Ellis Ave., Chicago, Illinois 60637, USA 6Glenn T. Seaborg Institute, Lawrence Livermore

Grossman, Lawrence