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1

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

2

Tom Lograsso, Ames Laboratory (Iowa State University), Future...  

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

Tom Lograsso, Ames Laboratory (Iowa State University), Future Directions in Rare Earth Research: Critical Materials for 21st Century Industry Tom Lograsso, Ames Laboratory (Iowa...

3

DOE - Office of Legacy Management -- Ames Laboratory Research...  

Office of Legacy Management (LM)

Ames Laboratory Research Reactor Facility - IA 03 FUSRAP Considered Sites Site: Ames Laboratory Research Reactor Facility (IA.03) Designated Name: Alternate Name: Location:...

4

Making Stuff Outreach at the Ames Laboratory and Iowa State University  

SciTech Connect

The U. S. Department of Energy's Ames Laboratory in Ames, Iowa was a coalition partner for outreach activities connected with NOVA's Making Stuff television series on PBS. Volunteers affiliated with the Ames Laboratory and Iowa State University, with backgrounds in materials science, took part in activities including a science-themed Family Night at a local mall, Science Cafes at the Science Center of Iowa, teacher workshops, demonstrations at science nights in elementary and middle schools, and various other events. We describe a selection of the activities and present a summary of their outcomes and extent of their impact on Ames, Des Moines and the surrounding communities in Iowa. In Part 2, results of a volunteer attitude survey are presented, which shed some light on the volunteer experience and show how the volunteers participation in outreach activities has affected their views of materials education.

Ament, Katherine; Karsjen, Steven; Leshem-Ackerman, Adah; King, Alexander

2011-04-01T23:59:59.000Z

5

Phenotypic Data Collection and Sample Preparation for Genomics of Wood Formation and Cellulosic Biomass Traits in Sunflower: Ames, IA location.  

Science Conference Proceedings (OSTI)

Three fields were planted in Ames in 2010, two association mapping fields, N3 and A, and a recombinant inbred line field, N13. Phenotype data and images were transferred to UGA to support genetic and genomic analyses of woody biomass-related traits.

Marek, Laura F.

2011-06-17T23:59:59.000Z

6

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

7

2011 Annual Planning Summary for Ames Site Office (Ames) | Department...  

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

Ames Site Office (Ames) 2011 Annual Planning Summary for Ames Site Office (Ames) The ongoing and projected Environmental Assessments and Environmental Impact Statements for 2011...

8

Ames Laboratory Research Reactor Facility Ames, Iowa  

Office of Legacy Management (LM)

,, *' ; . Final Radiological Condition of the Ames Laboratory Research Reactor Facility Ames, Iowa _, . AGENCY: Office of Operational Safety, Department of Energy ' ACTION: Notice of Availability of Archival Information Package SUMMARY: The'Office of Operational Safety of the Department O i Energy (DOE) has reviewed documentation relating to the decontamination and decommissioning operations conducted at the Ames Laboratory Research Reactor Facility, Ames, Iowa and has prepared an archival informati0.n package to permanently document the results of the action and the site conditions and use restriction placed on the . site at the tim e of release. This review is based on post-decontamination survey data and other pertinent documentation referenced in and included in the archival package. The material and

9

AMEE | Open Energy Information  

Open Energy Info (EERE)

AMEE AMEE Jump to: navigation, search Name AMEE Place London, United Kingdom Sector Carbon Product AMEE aims to build the largest engine to calculate carbon footprints for organisations, companies and individuals. Clients include Morgan Stanley, Google, UK Department of Energy and Climate Change Coordinates 51.506325°, -0.127144° 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":51.506325,"lon":-0.127144,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

10

Home | Ames Laboratory  

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

ABOUT | NEED A MATERIAL | NEWS CENTER | RESEARCH | TECH ABOUT | NEED A MATERIAL | NEWS CENTER | RESEARCH | TECH TRANSFER | CONTACT search LOG IN | RARE EARTH METALS | CRITICAL MATERIALS INSTITUTE | STAFF/ASSOCIATES | VISITORS | BE A PART OF AMES LAB | STUDENTS | EDUCATORS | FUNDING AGENCIES | INDUSTRY | RESEARCHERS | COMMUNITY RARE EARTH METALS Current Market Prices About Rare Earth Metals Materials Preparation STAFF/ASSOCIATES Operations Forms & Documents Find People VISITORS How To Get Here Tours of Ames Laboratory Local Events Calendar BE A PART OF AMES LAB Job News Human Resources Ames Lab At A Glance STUDENTS K-12 Resources Undergraduates Graduates and Others EDUCATORS Science Bowl SULI Program VFP Program FUNDING AGENCIES DOE/Contractor Research Highlights Contract INDUSTRY Technology Transfer Unique Capabilities

11

Ames Laboratory Technologies Available for Licensing - Energy ...  

Bookmark Ames Laboratory Technologies Available for Licensing - Energy Innovation Portal on Google; Bookmark Ames Laboratory Technologies Available ...

12

Routine environmental audit of Ames Laboratory, Ames, Iowa  

SciTech Connect

This document contains the findings identified during the routine environmental audit of Ames Laboratory, Ames, Iowa, conducted September 12--23, 1994. The audit included a review of all Ames Laboratory operations and facilities supporting DOE-sponsored activities. The audit`s objective is to advise the Secretary of Energy, through the Assistant Secretary for Environment, Safety and Health, as to the adequacy of the environmental protection programs established at Ames Laboratory to ensure the protection of the environment, and compliance with Federal, state, and DOE requirements.

1994-09-01T23:59:59.000Z

13

Pb-Free Sn-Ag-Cu-Mn Solder - Energy Innovation Portal  

Anderson, Iver E. (Ames, IA), Harringa, Joel (Ames, IA), Walleser, Jason K. (Idaho Falls, IA) Assignee: Iowa State University Research Foundation, ...

14

About Rare Earth Metals | Ames Laboratory  

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

About Rare Earth Metals About Rare Earth Metals What Are Rare Earths? Ames Laboratory's Materials Preparation Center The Ames Process for Purification of Rare...

15

Ames Laboratory | Open Energy Information  

Open Energy Info (EERE)

Ames Laboratory Ames Laboratory Jump to: navigation, search Name Ames Laboratory Place Ames, Iowa Zip 50011-3020 Product Research facility focused on solutions to energy-related problems. Coordinates 30.053389°, -94.742269° 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":30.053389,"lon":-94.742269,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

16

Ames Laboratory, Former Production Workers Screening Projects...  

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

Laboratory, Former Production Workers Screening Projects Ames Laboratory, Former Production Workers...

17

An aerial radiological survey of the Ames Laboratory and surrounding area, Ames, Iowa. Date of survey: July 1991  

Science Conference Proceedings (OSTI)

An aerial radiological survey of the Ames Laboratory and surrounding area in Ames, Iowa, was conducted during the period July 15--25, 1991. The purpose of the survey was to measure and document the terrestrial radiological environment at the Ames Laboratory and the surrounding area for use in effective environmental management and emergency response planning. The aerial survey was flown at an altitude of 200 feet (61 meters) along a series of parallel lines 350 feet (107 meters) apart. The survey encompassed an area of 36 square miles (93 square kilometers) and included the city of Ames, Iowa, and the Iowa State University. The results are reported as exposure rates at 1 meter above ground level (inferred from the aerial data) in the form of a gamma radiation contour map. Typical background exposure rates were found to vary from 7 to 9 microroentgens per hour ({mu}R/h). No anomalous radiation levels were detected at the Ames Laboratory. However, one anomalous radiation source was detected at an industrial storage yard in the city of Ames. In support of the aerial survey, ground-based exposure rate and soil sample measurements were obtained at several sites within the survey perimeter. The results of the aerial and ground-based measurements were found to agree within the expected uncertainty of {+-}15%.

Maurer, R.J.

1993-04-01T23:59:59.000Z

18

2013 Annual Planning Summary for the Ames Site Office | Department...  

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

Ames Site Office 2013 Annual Planning Summary for the Ames Site Office 2013 Annual Planning Summary for the Ames Site Office The ongoing and projected Environmental Assessments and...

19

Environmental Survey preliminary report, Ames Laboratory, Ames, Iowa  

Science Conference Proceedings (OSTI)

This report presents the preliminary findings of the first phase of the environmental Survey of the United States Department of Energy's (DOE) Ames Laboratory, conducted April 18 through 22, 1988. The Survey is being conducted by an interdisciplinary team of environmental specialists, led and managed by the Office of Environment, Safety and Health's Office of Environmental Audit. Individual team members are being supplied by private contractors. The objective of the Survey is to identify environmental problems and areas of environmental risk associated with the Ames Laboratory. The Survey covers all environmental media and all areas of environmental regulation. It is being performed in accordance with the DOE Environmental Survey Manual. This phase of the Survey involves the review of existing site environmental data, observations of the operations carried on at the Ames Laboratory, and interviews with site personnel. The Survey team developed a Sampling and Analysis (S A) Plan to assist in further assessing certain of the environmental problems identified during its on-site activities. The S A plan is being developed by the Idaho National Engineering Laboratory. When S A is completed, the results will be incorporated into the Ames Laboratory Environmental Survey findings for inclusion in the Environmental Survey Summary Report. 60 refs., 13 figs., 20 tabs.

Not Available

1989-03-01T23:59:59.000Z

20

New approaches for modeling type Ia supernovae  

SciTech Connect

Type Ia supernovae (SNe Ia) are the largest thermonuclearexplosions in the Universe. Their light output can be seen across greatstances and has led to the discovery that the expansion rate of theUniverse is accelerating. Despite the significance of SNe Ia, there arestill a large number of uncertainties in current theoretical models.Computational modeling offers the promise to help answer the outstandingquestions. However, even with today's supercomputers, such calculationsare extremely challenging because of the wide range of length and timescales. In this paper, we discuss several new algorithms for simulationsof SNe Ia and demonstrate some of their successes.

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

2007-06-25T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" 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

Materials Preparation Center | Ames Laboratory  

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

Materials Preparation Center Materials Preparation Center Materials Preparation Center The Materials Preparation Center (MPC) is a U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences, Division of Materials Sciences & Engineering specialized research center located at the Ames Laboratory. MPC operations are primarily funded by the Materials Discovery, Design, & Synthesis team's Synthesis & Processing Science core research activity. MPC is recognized throughout the worldwide research community for its unique capabilities in purification, preparation, and characterization of: Rare earth metals [learn about rare earths] Single crystal growth Metal Powders/Atomization Alkaline-earth metals [learn more, wikipedia] External Link Icon Refractory metal [learn more, wikipedia] External Link Icon

22

Ames Site Ofice 9800 South Cass Avenue  

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

of Energy of Energy Ames Site Ofice 9800 South Cass Avenue Argonne, Illinois 60439 January 15, 2013 MEMORANDUM FOR GREGORY H. WOODS, GENERAL COUNSEL OFFICE OF THE GENERAL COUNSEL FROM: SUBJECT: CYNTHIA BAEBLER, MANAGER iLJ�= AMES SITE OFFICE AMES SITE OFFICE (AMSO) 2013 ANNUAL NATIONAL ENVIRONMENTAL POLICY ACT (NEPA) PLANNING SUMMARY Section 5(a)(7) of DOE Order 451.1B Change 3, NEPA Compliance Program, requires

23

Image Library of Ames Lab on Flickr  

DOE Data Explorer (OSTI)

Ames has made their photos available on Flickr since 2009. The photos are organized into six sets, with the "Rare Earths' set being the largest.

24

UESC Project Overview: NASA Ames Research Center  

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

NASA Ames Research Center NASA Ames Research Center Utility Energy Services Contract Project Overview Federal Utilities Partnership Working Group Philadelphia, PA October 2011 NASA Ames Research Center Utility Energy Services Contract 2 Today's Discussion * NASA Ames Research Center (ARC) Energy Challenges * UESC Project Goals * Energy and Water Conservation Projects * Project Benefits and Results * Q&A NASA Ames Research Center Utility Energy Services Contract 3 NASA's Energy Challenges * Compliance with federal mandates - EISA, EPAct, Executive Orders (prior to UESC ARC was behind all of its goals) * Very low electric cost (<$0.05/kWh) * Not eligible for electric incentives through local utility (ARC purchases power from WAPA) * Aging mechanical and electrical infrastructure requiring significant

25

Former Worker Medical Screening Program - Ames Laboratory Former...  

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

Ames Laboratory Former Workers Former Worker Medical Screening Program (FWP) Project Name: Medical Monitoring of Former Workers at the Ames National Laboratory Covered DOE Site:...

26

On the Brightness of Supernova Ia  

E-Print Network (OSTI)

Before 1998 the universe expansion was thought to be slowing down. After 1998 the universe expansion is thought to be accelerating up. The key evidence came from the observed brightness of high redshift supernovae Ia in 1998. Astronomers found that the observed brightness of high redshift supernovae Ia is fainter than expected. Astronomers believe this means that the universe expansion is accelerating up. In this paper it is argued that if the ionized gas in the universe space is taken into account, then the brightness of the high redshift supernova Ia should be fainter than expected. The universe expansion does not need to be accelerating up. The exotic form of energy (dark energy) does not need to be introduce

Yijia Zheng

2013-10-01T23:59:59.000Z

27

Conference on Physics with Large Gamma-Ray Detector Arrays, Volume II Proceedings  

E-Print Network (OSTI)

Laboratory, Berkeley, CA 94720 University of California, Davis, CA 95616 Iowa State University, Ames, IA 50010 Rutgers University, New Brunswick,

Lawler editor, G.

2010-01-01T23:59:59.000Z

28

Analysis of Hexanitrostilbene (HNS) and Dipicryethane (DPE) for Mutagenicity by the Ames/Salmonella Assay  

Science Conference Proceedings (OSTI)

The Ames/Salmonella assay, developed by Professor Bruce Ames at the University of California, Berkeley, is a rapid and sensitive assay for detecting mutagenicity of various chemical compounds (Maron and Ames, 1983). It is a widely accepted short-term assay for detecting chemicals that induce mutations in the histidine (his) gene of Salmonella typhimurium. This is a reverse mutation assay that detects the mutational reversion of his-dependent Salmonella to the his-independent counterpart. Thereby, mutagenic compounds will increase the frequency of occurrence of his-independent bacterial colonies. The assay utilizes the specific genetically constructed strains of bacteria either with or without mammalian metabolic activation enzymes (S9), Aroclor induced rat liver homogenate to assess the mutagenicity of different compounds. In this study, we will use the Ames/Salmonella assay to investigate the mutagenicity of Hexanitrostilbene (HNS) from both Bofors and Pantex, and Dipicryethane (DPE).

Wu, R; Felton, J

2007-10-12T23:59:59.000Z

29

Ames Site Office 9800 South Cass Avenue  

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

Ames Site Office Ames Site Office 9800 South Cass Avenue Argonne, Illinois 60439 January 9, 2012 MEMORANDUM FOR TIMOTHY G. LYNCH FROM : DEPUTY GENERAL COUSNEL FOR LITIGATION CYNTHIA K. BAEBLER MANAGER SUBJECT: AMES SITE OFFICE (AMSO) 2012 ANNUAL NATIONAL ENVIRONMENTAL POLICY ACT (NEPA) PLANNING SUMMARY Section 5(a)(7) of DOE Order 451.1B Change 2, NEPA Compliance Program, requires each Secretarial Officer and Head of Field Organization to submit an annual NEPA Annual Planning Summary to the Office of General Counsel. We have reviewed your associated December 5, 2011, memorandum and in consultation with Ames Laboratory staff determined that we have no Environmental Impacts Statements or Environmental Assessments either ongoing or forecast for the next 12 to 24 months.

30

Voluntary cleanup of the Ames chemical disposal site.  

SciTech Connect

The U.S. Department of Energy completed a voluntary removal action at the Ames chemical disposal site, a site associated with the early days of the Manhattan Project. It contained chemical and low-level radioactive wastes from development of the technology to extract uranium from uranium oxide. The process included the preparation of a Remedial Investigation, Feasibility Study, Baseline Risk Assessment, and, ultimately, issuance of a Record of Decision. Various stakeholder groups were involved, including members of the regulatory community, the general public, and the landowner, Iowa State University. The site was restored and returned to the landowner for unrestricted use.

Taboas, A. L.; Freeman, R.; Peterson, J.; Environmental Assessment; USDOE

2003-01-01T23:59:59.000Z

31

Video Supplements for Papers from the Superconducting and Magnetism Low-temperature Laboratory at AMES Laboratory  

DOE Data Explorer (OSTI)

The Superconductivity and Magnetism Low-temperature Laboratory is part of the Condensed Matter Physics group in the Department of Physics and Astronomy at Iowa State University and Ames Laboratory. Some of the publications from this lab have data and figures on video. These videos have been posted online with their "parent" publications.

32

2012 Annual Planning Summary for Ames Site Office  

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

The ongoing and projected Environmental Assessments and Environmental Impact Statements for 2012 and 2013 within Ames Site Office.

33

Baldrige Award Recipients--Ames Rubber Corporation (1993)  

Science Conference Proceedings (OSTI)

... soundly. Its approach to environmental management is now part and parcel of Ames Rubber's quality management process. ...

2013-09-11T23:59:59.000Z

34

INTERNATIONAL SYMPOSIUM ON PROCESSING AND HANDLING ...  

Science Conference Proceedings (OSTI)

... MS 106-5, Cleveland, OH 44135; Iver Anderson, Ames Laboratory, Iowa State University, 122 Metals Development Bldg, Ames, IA 50011-3020; John Pusateri, ...

35

Rates and progenitors of type Ia supernovae  

SciTech Connect

The remarkable uniformity of Type Ia supernovae has allowed astronomers to use them as distance indicators to measure the properties and expansion history of the Universe. However, Type Ia supernovae exhibit intrinsic variation in both their spectra and observed brightness. The brightness variations have been approximately corrected by various methods, but there remain intrinsic variations that limit the statistical power of current and future observations of distant supernovae for cosmological purposes. There may be systematic effects in this residual variation that evolve with redshift and thus limit the cosmological power of SN Ia luminosity-distance experiments. To reduce these systematic uncertainties, we need a deeper understanding of the observed variations in Type Ia supernovae. Toward this end, the Nearby Supernova Factory has been designed to discover hundreds of Type Ia supernovae in a systematic and automated fashion and study them in detail. This project will observe these supernovae spectrophotometrically to provide the homogeneous high-quality data set necessary to improve the understanding and calibration of these vital cosmological yardsticks. From 1998 to 2003, in collaboration with the Near-Earth Asteroid Tracking group at the Jet Propulsion Laboratory, a systematic and automated searching program was conceived and executed using the computing facilities at Lawrence Berkeley National Laboratory and the National Energy Research Supercomputing Center. An automated search had never been attempted on this scale. A number of planned future large supernovae projects are predicated on the ability to find supernovae quickly, reliably, and efficiently in large datasets. A prototype run of the SNfactory search pipeline conducted from 2002 to 2003 discovered 83 SNe at a final rate of 12 SNe/month. A large, homogeneous search of this scale offers an excellent opportunity to measure the rate of Type Ia supernovae. This thesis presents a new method for analyzing the true sensitivity of a multi-epoch supernova search and finds a Type Ia supernova rate from z {approx} 0.01-0.1 of r{sub V} = 4.26{sub -1.93 -0.10}{sup +1.39 +0.10} h{sup 3} x 10{sup -4} SNe Ia/yr/Mpc{sup 3} from a preliminary analysis of a subsample of the SNfactory prototype search. Several unusual supernovae were found in the course of the SNfactory prototype search. One in particular, SN 2002ic, was the first SN Ia to exhibit convincing evidence for a circumstellar medium and offers valuable insight into the progenitors of Type Ia supernovae.

Wood-Vasey, William Michael

2004-08-16T23:59:59.000Z

36

Ames, Iowa: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Ames, Iowa: Energy Resources Ames, Iowa: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.02335°, -93.625622° 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":42.02335,"lon":-93.625622,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

37

Type Ia Supernovae Project at NERSC  

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

Type Ia Supernovae Type Ia Supernovae Supernova-1.jpg Update: Recent Berkeley Lab Computing Sciences News about supernovae: read more... Key Challenges: Understanding Type Ia...

38

Nanomaterials Safety Implementation Plan, Ames Laboratory | Department of  

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

Nanomaterials Safety Implementation Plan, Ames Laboratory Nanomaterials Safety Implementation Plan, Ames Laboratory Nanomaterials Safety Implementation Plan, Ames Laboratory Ames Laboratory has limited activities involving nanomaterials. Potential hazards associated with nanomaterials work are addressed through the Laboratory's Integrated Safety Management System (ISMS) and specifically the Readiness Review process. Readiness Review provides the identification and evaluation of potential hazards and establishes effective control mechanisms to ensure protection of the employee and the environment. To date, hazards associated with projects involving nanomaterials have been determined to be amenable to conventional controls such as ventilation and use of personal protective equipment. The Laboratory recognizes that nanotechnology is an emerging field and that

39

Ames Electric Department- Residential Energy Efficiency Rebate Programs  

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

The City of Ames Electric Services offers a variety of services and rebates for residential customers interested in purchasing energy efficient appliances or making energy efficiency improvements...

40

M. Meyyappan and Cattien V. Nguyen NASA Ames Research ...  

Science Conference Proceedings (OSTI)

Page 1. M. Meyyappan and Cattien V. Nguyen NASA Ames Research Center ... Si3N4 on Silicon substrate Nguyen et al., Nanotechnology, 2001, Vol. ...

Note: This page contains sample records for the topic "university ames ia" 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

Videos from AMES Laboratory on YouTube  

DOE Data Explorer (OSTI)

Ames Lab created a channel on YouTube near the end of 2009. This collection of clips provides quick looks at some of the outreach activities, educational explanations of various research projects (presented by the researcher involved), and the 2010 State of the Lab Address by Ames Lab Director Alex King. Approximately 50 videos are currently available.

42

Rare Earth Metals and Alloys | Ames Laboratory  

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

Mpc » Rare Earth Metals and Alloys Mpc » Rare Earth Metals and Alloys Rare Earth Metals and Alloys Terbium (Tb) and Cerium (Ce) phosphors in your computer screen allow you to see GREEN. Europium (Eu) is the source of the RED light and BLUE emitted by our display. The Ames Laboratory has been actively involved in the preparation of very pure rare earth metals since the early 1940's when Dr. Frank H. Spedding and his group of pioneers developed the ion-exchange process, a technique that separates the "fraternal fifteen" plus yttrium and scandium. As a result of this and subsequent work, high-purity oxides are available from which high-purity rare earth metals can be prepared. In most cases, the rare earth oxides are first converted to their respective fluorides and are then reduced metallothermicaly on a kilogram

43

Radiological survey support activities for the decommissioning of the Ames Laboratory Research Reactor Facility, Ames, Iowa  

SciTech Connect

At the request of the Engineering Support Division of the US Department of Energy-Chicago Operations Office and in accordance with the programmatic overview/certification responsibilities of the Department of Energy Environmental and Safety Engineering Division, the Argonne National Laboratory Radiological Survey Group conducted a series of radiological measurements and tests at the Ames Laboratory Research Reactor located in Ames, Iowa. These measurements and tests were conducted during 1980 and 1981 while the reactor building was being decontaminated and decommissioned for the purpose of returning the building to general use. The results of these evaluations are included in this report. Although the surface contamination within the reactor building could presumably be reduced to negligible levels, the potential for airborne contamination from tritiated water vapor remains. This vapor emmanates from contamination within the concrete of the building and should be monitored until such time as it is reduced to background levels. 2 references, 8 figures, 6 tables.

Wynveen, R.A.; Smith, W.H.; Sholeen, C.M.; Justus, A.L.; Flynn, K.F.

1984-09-01T23:59:59.000Z

44

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

45

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

46

Ames Electric Department - Residential Energy Efficiency Rebate Programs |  

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

Ames Electric Department - Residential Energy Efficiency Rebate Ames Electric Department - Residential Energy Efficiency Rebate Programs Ames Electric Department - Residential Energy Efficiency Rebate Programs < Back Eligibility Multi-Family Residential Residential Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Appliances & Electronics Home Weatherization Construction Commercial Weatherization Design & Remodeling Heat Pumps Commercial Lighting Lighting Maximum Rebate Appliances: 50% of the equipment cost Programmable Thermostats: 3 per household Room AC: 2 per household Program Info State Iowa Program Type Utility Rebate Program Rebate Amount Energy Star New Home: $500 Energy Audit: FREE Lighting: $2 - $16 per fixture Lighting Sensors: $10 per unit Refrigerators: $25 - $100 Freezers: $50 Dishwashers: $50

47

Rapporteurs Report: Tom Lograsso, Ames Laboratory and Nick Morley...  

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

in Rare Earth Research: Critical Materials for 21st Century Industry Inspection Report: IG-0615 Audit of Acquisition of Scientific Research at Ames Laboratory, ER-B-95-05...

48

Environmental monitoring at Ames Laboratory: Calendar year 1975  

SciTech Connect

This is an annual report summarizing the effluent and environmental monitoring program at the Ames Laboratory of the United States Energy Research and Development Administration. An inventory of the radioactive materials and certain chemicals released to the environment is included. A summary of the radioactivity found in the environment is presented. An estimate of the radiation dose to the public resulting from the operations of the Ames Laboratory is stated. (auth)

Voss, M.D.

1976-04-01T23:59:59.000Z

49

Ames Laboratory integrated safety management self-assessment report  

SciTech Connect

The implementation of Integrated Safety Management (ISM) at Ames Laboratory began with the signing of the ISM Implementation Charter on February 24, 1997 (see Appendix A). The first step toward implementation of ISM at Ames Laboratory is the performance of a Self-Assessment (SA). In preparation for the SA, a workshop on ISM was provided to the Laboratory`s Environment, Safety, and Health (ES&H) Coordinators, Safety Review Committee members, and the Environment, Safety, Health and Assurance (ESH&A) staff. In addition, a briefing was given to the Laboratory`s Executive Council and Program Directors. Next, an SA Team was organized. The Team was composed of four Ames Laboratory and four Department of Energy-Chicago Operations Office (DOE-CH) staff members. The purpose of this SA was to determine the current status of ES&H management within Ames Laboratory, as well as to identify areas which need to be improved during ISM implementation. The SA was conducted by reviewing documents, interviewing Ames Laboratory management and staff, and performing walkthroughs of Laboratory areas. At the conclusion of this SA, Ames Laboratory management was briefed on the strengths, weaknesses, and the areas of improvement which will assist in the implementation of ISM.

NONE

1997-10-01T23:59:59.000Z

50

Labs at-a-Glance: Ames Laboratory | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames Laboratory Ames Laboratory Laboratories Ames Laboratory Argonne National Laboratory Brookhaven National Laboratory Fermi National Accelerator Laboratory Lawrence Berkeley National Laboratory Oak Ridge National Laboratory Pacific Northwest National Laboratory Princeton Plasma Physics Laboratory SLAC National Accelerator Laboratory Thomas Jefferson National Accelerator Facility Laboratory Policy and Evaluation Safety, Security and Infrastructure Laboratory Science Highlights Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 Labs at-a-Glance: Ames Laboratory Print Text Size: A A A RSS Feeds FeedbackShare Page Ames Laboratory Logo Visit the Ames Laboratory website External link Ames Laboratory Quick Facts

51

Toward Exascale Computing of Type Ia and Ib,c Supernovae: V&V...  

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

Toward Exascale Computing of Type Ia and Ib,c Supernovae: V&V of Current Models PI Name: Don Lamb PI Email: lamb@oddjob.uchicago.edu Institution: University Of Chicago Allocation...

52

Ames Site Office Homepage | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Home Home Ames Site Office (AMSO) AMSO Home About Current Projects Contract Management Environment, Safety and Health (ES&H) Resources Contact Information Ames Site Office U.S. Department of Energy 9800 S. Cass Avenue Argonne, IL 60439 P: (630) 252-6167 F: (630) 252-2855 Ames Site Office Pictured Right: Ames Laboratory Ames Laboratory 1 of 2 Print Text Size: A A A RSS Feeds FeedbackShare Page The Ames Site Office (AMSO) is an organization within the U.S. Department of Energy's Office of Science with responsibility to oversee and manage the Management and Operating (M&O) contract for the Ames Laboratory in Ames, Iowa. Ames Laboratory is one of ten Office of Science Laboratories and is a single program laboratory with a primary mission on delivering breakthrough science and technology in the area of Basic Energy Sciences. The AMSO is

53

Ames Electric Department - Commercial Energy Efficiency Rebate Programs |  

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

Ames Electric Department - Commercial Energy Efficiency Rebate Ames Electric Department - Commercial Energy Efficiency Rebate Programs Ames Electric Department - Commercial Energy Efficiency Rebate Programs < Back Eligibility Commercial Industrial Savings Category Heating & Cooling Commercial Heating & Cooling Cooling Appliances & Electronics Other Heat Pumps Commercial Lighting Lighting Maximum Rebate Appliances: 50% of equipment cost per unit Lighting: Will not exceed equipment cost per unit, (contact AED about incentives expected to exceed $10,000) Power Factor Correction Equipment: Incentives over $15,000 will be examined on case by case basis Custom Rebate: Incentives over $15,000 willexamined on case by case basis Program Info State Iowa Program Type Utility Rebate Program Rebate Amount Refrigerators: $25 - $100

54

Prospective Type Ia supernova surveys from Dome A  

E-Print Network (OSTI)

Prospective Type Ia Supernova Surveys From Dome A A. Kim a ,are conducive toward Type Ia supernova surveys forheterogeneities within the Type Ia supernova class, reducing

Kim, A.

2010-01-01T23:59:59.000Z

55

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

56

Comparison Between Field Data and NASA Ames Wind Tunnel Data  

DOE Green Energy (OSTI)

The objective of this analysis is to compare the measured data from the NASA Ames wind tunnel experiment to those collected in the field at the National Wind Technology Center (NWTC) with the same turbine configuration. The results of this analysis provide insight into what measurements can be made in the field as opposed to wind tunnel testing.

Corbus, D.

2005-11-01T23:59:59.000Z

57

Renewable Energy Microgrid Testbed at NASA Ames Research  

E-Print Network (OSTI)

Renewable Energy Microgrid Testbed at NASA Ames Research Center Joel Kubby, Dan O'Leary, Zachary #12;Goals · Set-up a unique microgrid test-bed for renewable energy generation, monitoring and storage · Use the facility for testing systems integration, optimization and control of new renewable energy

Lee, Herbie

58

DC Optimal Power Flow Formulation in AMES Leigh Tesfatsion  

E-Print Network (OSTI)

23 of a user-specified maximum day. AMES includes an Independent System Operator (ISO a demand bid to the ISO for the day-ahead market for day D+1. Each demand bid consists of two parts: fixed demand (i.e., a 24-hour load profile) to be sold downstream at a regulated price r to its retail

Tesfatsion, Leigh

59

Iowa State University | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Beardshear Hall Beardshear Hall Research Research & Economic Development Research Units ISU Technology Search Students & Research at ISU DOE ARPA-E Biofuel Project DOE Office of Science Funding ISU & Ames Lab Tech Marketing Summaries ISU research in Energy Citations Database ISU research in E-print Network Ames Laboratory is a DOE National Laboratory operated under contract by Iowa State University Physicist developing, improving designer optical materials Chemists discover proton mechanism used by flu virus to infect cells ISU, Ames Lab's Bryden & McCorkle win 2010 R&D 100 Award New tool for cell research may help unravel secrets of disease Search this site: Search ISU's vision is to lead the world in advancing the land-grant ideas of putting science, technology, and human creativity to work.

60

Nucleosynthesis in type Ia supernovae driven by asymmetric thermonuclear ignition  

Science Conference Proceedings (OSTI)

Type Ia Supernovae (SNe Ia) are believed to be thermonuclear explosions of a white dwarf. They can be used as mature cosmological standardized candles, leading to the discovery of the accelerating expansion of the Universe. However, the explosion mechanism has not yet been fully clarified. In this paper, we first present nucleosynthetic features of a leading explosion scenario, namely a delayed-detonation scenario. Based on this, we propose a new and strong observational constraint on the explosion mechanism through emission lines from neutron-rich Fe-peaks. Especially, we show that an asymmetry in the explosion is likely a generic feature. We further argue that the diversity arising from various viewing angles can be an origin of observational diversities of SNe Ia seen in their spectral features (suspected possible biases in cosmology) and colors (related to the extinction estimate in cosmology). Using these new insights could open up a possibility of using SNe Ia as more precise distance indicators than currently employed.

Maeda, Keiichi [Institute for the Physics and Mathematics of the Universe (IPMU), Todai Institutes for Advanced Study (TODIAS), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan)

2012-11-12T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" 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

Critical Materials and Rare Futures: Ames Laboratory Signs a New Agreement  

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

Critical Materials and Rare Futures: Ames Laboratory Signs a New Critical Materials and Rare Futures: Ames Laboratory Signs a New Agreement on Rare-Earth Research Critical Materials and Rare Futures: Ames Laboratory Signs a New Agreement on Rare-Earth Research June 15, 2011 - 7:07pm Addthis The plasma torch in the Retech plasma furnace is one tool used in Materials Preparation Center to create ultra-high purity metal alloy samples, particularly rare-earth metals, located at the Ames Lab. | Photo Courtesy of the Ames Lab Flickr The plasma torch in the Retech plasma furnace is one tool used in Materials Preparation Center to create ultra-high purity metal alloy samples, particularly rare-earth metals, located at the Ames Lab. | Photo Courtesy of the Ames Lab Flickr Charles Rousseaux Charles Rousseaux Senior Writer, Office of Science

62

Ames Laboratory scientists discover new family of quasicrystals | Argonne  

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

Science Science Computing, Environment & Life Sciences Energy Engineering & Systems Analysis Photon Sciences Physical Sciences & Engineering Energy Frontier Research Centers Science Highlights Postdoctoral Researchers Ames Laboratory scientists discover new family of quasicrystals July 16, 2013 Tweet EmailPrint Scientists at the U.S. Department of Energy's (DOE) Ames Laboratory have discovered a new family of rare-earth quasicrystals using an algorithm they developed to help pinpoint them. Quasicrystalline materials may be found close to crystalline phases that contain similar atomic motifs, called crystalline approximants. And just like fishing experts know that casting a line in the right habitat hooks the big catch, the scientists used their knowledge to hone in on just the right spot for new quasicrystal materials

63

The Universe Adventure - Today's Universe  

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

4: Today's Accelerating Universe 4: Today's Accelerating Universe The Universe Today Dark matter has aided in forming the universe we see today; however, many questions regarding the cosmos remain. What is the status of the Universe today? We know the Universe is expanding... But what do we know about the expansion? Supernova survey. Surveys of supernova provide scientists with information about the history of the Universe. Classroom Cosmology Classroom Cosmology: Toilet Paper Cosmology In 1997 advances in telescope technology allowed astronomers to conduct redshift surveys of very distant type Ia supernovae. This enabled them to look further back into the Universe's history than previously possible. Their stunning results rivaled Hubble's original discovery and turned cosmology on its head. While most theoretical models predicted that the

64

Environmental monitoring at Ames Laboratory: calendar year 1980  

SciTech Connect

The results and conclusions from the Ames Laboratory environmental monitoring programs for the Ames Laboratory Research Reactor (ALRR) and other Laboratory facilities are presented. The major areas of radiological monitoring were ALRR effluent air, environmental air, effluent water and environmental water. A summary of the radioactivity found in the environment is presented. The ALRR ceased operation on December 1, 1977. Decommissioning activities began January 3, 1978, and are scheduled for completion October 1, 1981. Analysis of air samples collected at the ALRR on-site station showed no radioactivity that could be attributed to ALRR operations. The radiosotope of significance in the ALRR stack effluent was tritium (H-3). The yearly individual dose from H-3 at the exclusion fence was estimated to be 0.016 mRem and the estimated dose to the entire population within an 80 Km (50 mile) radius of the ALRR was 26.6 man-Rem. These values are 0.0032% and 0.026%, respectively, of the doses derived from the concentration guides. On September 1, 1978, the ALRR site was connected to the City of Ames sanitary sewage system. All liquids (except building foundation and roof water) from the ALRR complex are now discharged to the sewage system negating the requirement for monitoring chemical constituents of effluent and environmental waters. In the radioactive liquid waste released to the City of Ames sewage system from the ALRR complex, H-3 was the predominant isotope. After dilution with other waste water from the ALRR complex, the potential dose was not more than 0.68% of the dose derived from the concentration guide. Building foundation and roof water are discharged to a drainage gulch on site.

Voss, M.D.

1981-04-01T23:59:59.000Z

65

Turbulent Combustion in Type Ia Supernova Models  

E-Print Network (OSTI)

We review the astrophysical modeling of type Ia supernova explosions and describe numerical methods to implement numerical simulations of these events. Some results of such simulations are discussed.

F. K. Roepke; W. Hillebrandt

2006-09-15T23:59:59.000Z

66

Progenitors of type Ia supernovae in elliptical galaxies  

Science Conference Proceedings (OSTI)

Although there is a nearly universal agreement that type Ia supernovae are associated with the thermonuclear disruption of a CO white dwarf, the exact nature of their progenitors is still unknown. The single degenerate scenario envisages a white dwarf accreting matter from a non-degenerate companion in a binary system. Nuclear energy of the accreted matter is released in the form of electromagnetic radiation or gives rise to numerous classical nova explosions prior to the supernova event. We show that combined X-ray output of supernova progenitors and statistics of classical novae predicted in the single degenerate scenario are inconsistent with X-ray and optical observations of nearby early type galaxies and galaxy bulges. White dwarfs accreting from a donor star in a binary system and detonating at the Chandrasekhar mass limit can account for no more than {approx}5% of type Ia supernovae observed in old stellar populations.

Gilfanov, M.; Bogdan, A.

2011-09-21T23:59:59.000Z

67

Kenneth W. Pratt  

Science Conference Proceedings (OSTI)

... Clinical and Laboratory Standards Institute, CLSI (formerly NCCLS), Area Committee on ... Chemistry, Ph.D., Iowa State University, Ames, IA, 1981. ...

2012-11-15T23:59:59.000Z

68

NASA/Ames Global Emissions Data Set (GLEMIS) | Open Energy Information  

Open Energy Info (EERE)

NASA/Ames Global Emissions Data Set (GLEMIS) NASA/Ames Global Emissions Data Set (GLEMIS) Jump to: navigation, search Tool Summary LAUNCH TOOL Name: NASA/Ames Global Emissions Data Set (GLEMIS) Agency/Company /Organization: National Aeronautics and Space Administration Sector: Land Focus Area: Forestry, Agriculture Topics: GHG inventory Resource Type: Dataset, Maps Website: gcmd.nasa.gov/records/GCMD_NASA_AMES_GLEMIS.html NASA/Ames Global Emissions Data Set (GLEMIS) Screenshot References: NASA/Ames Global Emissions Data Set (GLEMIS)[1] "NASA-CASA data sets include global maps for predicted fluxes of soil nitrogen gases (N2O and NO), methane (CH4), and carbon monoxide (CO), plus predictions of net primary production (NPP) and carbon storage in leaf, wood, root, litter, and surface soil pools. Others data sets will follow.

69

SBOT IOWA AMES LAB POC Lisa Rodgers Telephone  

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

IOWA IOWA AMES LAB POC Lisa Rodgers Telephone (515) 294-4191 Email rodgers@ameslab.gov GOODS Photographic Equipment and Supplies Merchant Wholesalers 423410 Computer and Computer Peripheral Equipment and Software Merchant Wholesalers 423430 Other Commercial Equipment Merchant Wholesalers 423440 Other Professional Equipment and Supplies Merchant Wholesalers 423490 Electrical Apparatus and Equipment, Wiring Supplies, and Related Equipment Merchant Wholesalers 423610 Electrical and Electronic Appliance, Television, and Radio Set Merchant Wholesalers 423620 Other Electronic Parts and Equipment Merchant Wholesalers 423690 Industrial Machinery and Equipment Merchant Wholesalers 423830 Industrial Supplies Merchant Wholesalers 423840 Other Miscellaneous Durable Goods Merchant Wholesalers

70

Theoretical cosmic Type Ia supernova rates  

E-Print Network (OSTI)

The aim of this work is the computation of the cosmic Type Ia supernova rates at very high redshifts (z>2). We adopt various progenitor models in order to predict the number of explosions in different scenarios for galaxy formation and to check whether it is possible to select the best delay time distribution model, on the basis of the available observations of Type Ia supernovae. We also computed the Type Ia supernova rate in typical elliptical galaxies of different initial luminous masses and the total amount of iron produced by Type Ia supernovae in each case. It emerges that: it is not easy to select the best delay time distribution scenario from the observational data and this is because the cosmic star formation rate dominates over the distribution function of the delay times; the monolithic collapse scenario predicts an increasing trend of the SN Ia rate at high redshifts whereas the predicted rate in the hierarchical scheme drops dramatically at high redshift; for the elliptical galaxies we note that the predicted maximum of the Type Ia supernova rate depends on the initial galactic mass. The maximum occurs earlier (at about 0.3 Gyr) in the most massive ellipticals, as a consequence of downsizing in star formation. We find that different delay time distributions predict different relations between the Type Ia supernova rate per unit mass at the present time and the color of the parent galaxies and that bluer ellipticals present higher supernova Type Ia rates at the present time.

R. Valiante; F. Matteucci; S. Recchi; F. Calura

2008-07-15T23:59:59.000Z

71

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":""}]}

72

AME:NDMENT OF SOLICITATION/MODIFICATION OF CONTRACT  

National Nuclear Security Administration (NNSA)

AME:NDMENT OF SOLICITATION/MODIFICATION OF CONTRACT AME:NDMENT OF SOLICITATION/MODIFICATION OF CONTRACT 1. CONTRACT 10 CODE PAGE 1 OF 224 PAGES 2. AMENDMENT/MODIFICATION NO. M202 3. EFFECTIVE DATE October 1, 2003 4. REQUISITION/PURCHASE REQ. NO. 5. PROJECT NO. (If applicable) 6. ISSUED BY CODE 7. ADMINISTERED BY (If other than Item 6) CODE U.s. Department of Energy N.itional Nuclear Security Administration Sandia Site Office Mail Stop 0184 P.O. Box 5400 AlbuauerQue, NM 87185-5400 8. NAME AND ADDRESS OF CONTRACTOR (No., street, county, state, ZIP Code) 9A. AMENDMENT OF SOLICITATION NO. Sandia Corporation P. O. Box 5800 Albuquerque, NM 87185 98. DATED (SEE ITEM 11) 10A. MODIFICATION OF CONTRACT/ORDER NO. DE-ACO4-94AL85000 108. DATED (SEE ITEM 13) October 1, 1993 CODE II-ACIL~ CODE 11. THIS ITEM ONLY APPLIES TO AMENDMENTS OF SOLICITATIONS

73

The progenitors of subluminous type Ia supernovae  

DOE Green Energy (OSTI)

We find that spectroscopically peculiar subluminous SNe Ia come from an old population. Of the thirteen subluminous SNe Ia known, nine are found in E/S0 galaxies, and the remainder are found in early-type spirals. The probability that this is a chance occurrence is only 0.1%. The finding that subluminous SNe Ia are associated with an older stellar population indicates that for a sufficiently large lookback time (already accessible in current high redshift searches) they will not be found. Due to a scarcity in old populations, hydrogen and helium main sequence stars and He red giant stars that undergo Roche lobe overflow are unlikely to be the progenitors of subluminous SNe Ia. Earlier findings that overluminous SNe Ia (DELTA m{sub 15} (B) < 0.94) come from a young progenitor population are confirmed. The fact that subluminous SNe Ia and overluminous SNe Ia come from different progenitor populations and also have different properties is a prediction of the CO white dwarf merger progenitor scenario.

Howell, D. Andrew

2001-02-01T23:59:59.000Z

74

Iowa Start-up Taps Ames Laboratory Technology in Challenge | Department of  

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

Taps Ames Laboratory Technology in Challenge Taps Ames Laboratory Technology in Challenge Iowa Start-up Taps Ames Laboratory Technology in Challenge August 10, 2011 - 2:21pm Addthis Using gas atomization technology developed at the Ames Lab (click through the photo to see a video), IPAT will be able to make titanium powder 10 times more efficiently than traditional powder-making methods. Above right, 1.8 grams of gas atomized titanium powder makes a finished 1.8 gram titanium bolt. | Image Courtesy of IPAT Using gas atomization technology developed at the Ames Lab (click through the photo to see a video), IPAT will be able to make titanium powder 10 times more efficiently than traditional powder-making methods. Above right, 1.8 grams of gas atomized titanium powder makes a finished 1.8 gram titanium bolt. | Image Courtesy of IPAT

75

City of Ames, Iowa (Utility Company) | Open Energy Information  

Open Energy Info (EERE)

Iowa (Utility Company) Iowa (Utility Company) Jump to: navigation, search Name Ames City of Place Iowa Utility Id 554 Utility Location Yes Ownership M NERC Location MRO NERC MRO Yes ISO MISO Yes Operates Generating Plant Yes Activity Generation Yes Activity Transmission Yes Activity Buying Transmission Yes Activity Distribution Yes Activity Wholesale Marketing Yes Alt Fuel Vehicle Yes Alt Fuel Vehicle2 Yes References EIA Form EIA-861 Final Data File for 2010 - File1_a[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Utility Rate Schedules Grid-background.png Industrial Rates Industrial Large Commercial Rates Commercial Residential Residential Small Commercial Rates Commercial Average Rates

76

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

Science Conference Proceedings (OSTI)

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

77

National Laboratories - Energy Innovation Portal  

Name Address City, State; Ames Laboratory: Ames Laboratory: Ames, IA: Argonne National Laboratory: 9700 S. Cass Avenue: Argonne, IL: Brookhaven ...

78

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":""}]}

79

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

80

Spectral diversity of Type Ia Supernovae  

E-Print Network (OSTI)

We use published spectroscopic and photometric data for 8 Type Ia supernovae to construct a dispersion spectrum for this class of object, showing their diversity over the wavelength range 3700A to 7100A. We find that the B and V bands are the spectral regions with the least dispersion, while the U band below 4100A is more diverse. Some spectral features such as the Si line at 6150A are also highly diverse. We then construct two objective measures of 'peculiarity' by (i) using the deviation of individual objects from the average SN Ia spectrum compared to the typical dispersion and (ii) applying principle component analysis. We demonstrate these methods on several SNe Ia that have previously been classified as peculiar.

J. Berian James; Tamara M. Davis; Brian P. Schmidt; Alex G. Kim

2006-05-05T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" 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

After 15 Years, A New Top Earning Patent At Ames Lab | Department of Energy  

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

After 15 Years, A New Top Earning Patent At Ames Lab After 15 Years, A New Top Earning Patent At Ames Lab After 15 Years, A New Top Earning Patent At Ames Lab January 20, 2012 - 11:32am Addthis Ames Laboratory senior metallurgist Iver Anderson explains the importance of lead-free solder in taking hazardous lead out of the environment by eliminating it from discarded computers and electronics that wind up in landfills. Anderson led a team that developed a tin-silver-copper replacement for traditional lead solder that has been adopted by more than 50 companies worldwide and has generated more than $39 million in licensing income. Michael Hess Michael Hess Former Digital Communications Specialist, Office of Public Affairs What are the key facts? As of the end of June 2011, lead-free solder generated $38.9 million

82

Low Dose Radiation Research Program: Bruce N. Ames  

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

University of California, Berkeley Technical Abstracts 2002 Workshop: Comparison of Low-Dose Radiation, Endogenous Oxidants, and Micronutrient Deficiencies through Analyses of DNA...

83

Visualizing Buoyant Burning Bubbles in Type Ia Supernovae at...  

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

Burning in Supernovae Buoyant Burning Bubbles in Type Ia Supernovae bubble-s.jpeg Flame ignition in type Ia supernovae leads to isolated bubbles of burning buoyant fluid. As a...

84

Changing scene highlights III. [Iowa State University  

DOE Green Energy (OSTI)

The research programs in progress at Ames Laboratory, Iowa State University, are reviewed: hydrogen (storage), materials, catalysts, TRISTAN (their laboratory isotope separator), coal preparation, coal classification, land reclamation (after surface mining, nitinol, neutron radiography, grain dust explosions, biomass conversion, etc). (LTC)

Not Available

85

LINKING TYPE Ia SUPERNOVA PROGENITORS AND THEIR RESULTING EXPLOSIONS  

Science Conference Proceedings (OSTI)

Comparing the ejecta velocities at maximum brightness and narrow circumstellar/interstellar Na D absorption line profiles of a sample of 23 Type Ia supernovae (SNe Ia), we determine that the properties of SN Ia progenitor systems and explosions are intimately connected. As demonstrated by Sternberg et al., half of all SNe Ia with detectable Na D absorption at the host-galaxy redshift in high-resolution spectroscopy have Na D line profiles with significant blueshifted absorption relative to the strongest absorption component, which indicates that a large fraction of SN Ia progenitor systems have strong outflows. In this study, we find that SNe Ia with blueshifted circumstellar/interstellar absorption systematically have higher ejecta velocities and redder colors at maximum brightness relative to the rest of the SN Ia population. This result is robust at a 98.9%-99.8% confidence level, providing the first link between the progenitor systems and properties of the explosion. This finding is further evidence that the outflow scenario is the correct interpretation of the blueshifted Na D absorption, adding additional confirmation that some SNe Ia are produced from a single-degenerate progenitor channel. An additional implication is that either SN Ia progenitor systems have highly asymmetric outflows that are also aligned with the SN explosion or SNe Ia come from a variety of progenitor systems where SNe Ia from systems with strong outflows tend to have more kinetic energy per unit mass than those from systems with weak or no outflows.

Foley, Ryan J.; Kirshner, Robert P. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Simon, Joshua D.; Burns, Christopher R. [Observatories of the Carnegie Institution for Science, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Gal-Yam, Avishay [Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100 (Israel); Hamuy, Mario [Departamento de Astronomia, Universidad de Chile, Casilla 36-D, Santiago (Chile); Morrell, Nidia I.; Phillips, Mark M. [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Shields, Gregory A. [Department of Astronomy, University of Texas, Austin, TX 78712 (United States); Sternberg, Assaf, E-mail: rfoley@cfa.harvard.edu [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, 85741 Garching (Germany)

2012-06-20T23:59:59.000Z

86

Ames Laboratory to Lead New Research Effort to Address Shortages in Rare  

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

Laboratory to Lead New Research Effort to Address Shortages in Laboratory to Lead New Research Effort to Address Shortages in Rare Earth and Other Critical Materials Ames Laboratory to Lead New Research Effort to Address Shortages in Rare Earth and Other Critical Materials January 9, 2013 - 12:13pm Addthis NEWS MEDIA CONTACT (202) 586-4940 WASHINGTON - The U.S. Department of Energy announced today that a team led by Ames Laboratory in Ames, Iowa, has been selected for an award of up to $120 million over five years to establish an Energy Innovation Hub that will develop solutions to the domestic shortages of rare earth metals and other materials critical for U.S. energy security. The new research center, which will be named the Critical Materials Institute (CMI), will bring together leading researchers from academia, four Department of Energy

87

NASA Ames Saves Energy and Reduces Project Costs with Non-Invasive Retrofit Technologies  

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

NASA Ames Saves Energy and Reduces Project Costs NASA Ames Saves Energy and Reduces Project Costs with Non-Invasive Retrofit Technologies The Wireless Pneumatic Thermostat Enables Energy Efficiency Strategies, Ongoing Commissioning and Improved Operational Control Harry Sim CEO Cypress Envirosystems harry.sim@cypressenvirosystems.com www.cypressenvirosystems.com NASA Ames Reduced Project Cost by Over 80% with Non-Invasive Retrofit Technologies * Legacy Pneumatic Thermostats  Waste energy  High maintenance costs  Uncomfortable occupants  No visibility * Project Scope  14 buildings  1,370 pneumatic thermostats  Integration with campus BAS  Diagnostics for ongoing commissioning * Traditional DDC Retrofit  Cost over $4.1 million  Asbestos exposure/abatement  Occupants significantly disrupted

88

Ames: Oct 1, 2010 - Sept 30, 2011 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2010 - Sept 30, 2011 Ames: Oct 1, 2010 - Sept 30, 2011 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards Ames: Oct 1, 2010 - Sept 30, 2011 Argonne: Oct 1, 2010 - Sept 30, 2011 BNL: Oct 1, 2010 - Sept 30, 2011 Fermilab: Oct 1, 2010 - Sept 30, 2011 LBNL: Oct 1, 2010 - Sept 30, 2011 ORNL: Oct 1, 2010 - Sept 30, 2011 PNNL: Oct 1, 2010 - Sept 30, 2011 PPPL: October 1, 2010 - September 30, 2011 SLAC: Oct 1, 2010 - Sept 30, 2011 JLab: Oct 1, 2010 - Sept 30, 2011 FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards

89

Ames: Oct 1, 2012 - Sept 30, 2013| U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2012 - Sept 30, 2013 Ames: Oct 1, 2012 - Sept 30, 2013 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards Ames: Oct 1, 2012 - Sept 30, 2013 Argonne: Oct 1, 2012 - Sept 30, 2013 BNL: Oct 1, 2012 - Sept 30, 2013 Fermilab: Oct 1, 2012 - Sept 30, 2013 LBNL: Oct 1, 2012 - Sept 30, 2013 ORNL: Oct 1, 2012 - Sept 30, 2013 PNNL: Oct 1, 2012 - Sept 30, 2013 PPPL: Oct 1, 2012 - Sept 30, 2013 SLAC: Oct 1, 2012 - Sept 30, 2013 JLab: Oct 1, 2012 - Sept 30, 2013 FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards FY 2007 SC Laboratory Performance Report Cards

90

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

Office of Science (SC) Website

Ames Site Office CX Determinations Ames Site 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 Ames Site 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 07/10/2013 Sensitive Instrument Facility .pdf file (792KB) B3.6

91

Ames: Jan 1, 2007 - Sept 30, 2007 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Jan 1, 2007 - Sept 30, 2007 Ames: Jan 1, 2007 - Sept 30, 2007 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards FY 2007 SC Laboratory Performance Report Cards Ames: Jan 1, 2007 - Sept 30, 2007 Argonne: Oct 1, 2006 - Sept 30, 2007 BNL: Oct 1, 2006 - Sept 30, 2007 Fermilab: Jan 1, 2007 - Sept 30, 2007 LBNL: Oct 1, 2006 - Sept 30, 2007 ORNL: Oct 1, 2006 - Sept 30, 2007 PNNL: Oct 1, 2006 - Sept 30, 2007 PPPL: Oct 1, 2006 - Sept 30, 2007 SLAC: Oct 1, 2006 - Sept 30, 2007

92

Ames: Oct 1, 2005 - Sept 30, 2006 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2005 - Sept 30, 2006 Ames: Oct 1, 2005 - Sept 30, 2006 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards FY 2007 SC Laboratory Performance Report Cards FY 2006 SC Laboratory Performance Report Cards Ames: Oct 1, 2005 - Sept 30, 2006 Argonne: Oct 1, 2005 - Sept 30, 2006 BNL: Oct 1, 2005 - Sept 30, 2006 Fermilab: Oct 1, 2005 - Sept 30, 2006 LBNL: Oct 1, 2005 - Sept 30, 2006 ORNL: Oct 1, 2005 - Sept 30, 2006 PNNL: Oct 1, 2005 - Sept 30, 2006 PPPL: Oct 1, 2005 - Sept 30, 2006

93

Ames: Oct 1, 2009 - Sept 30, 2010 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2009 - Sept 30, 2010 Ames: Oct 1, 2009 - Sept 30, 2010 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards Ames: Oct 1, 2009 - Sept 30, 2010 Argonne: Oct 1, 2009 - Sept 30, 2010 BNL: Oct 1, 2009 - Sept 30, 2010 Fermilab: Oct 1, 2009 - Sept 30, 2010 LBNL: Oct 1, 2009 - Sept 30, 2010 ORNL: Oct 1, 2009 - Sept 30, 2010 PNNL: Oct 1, 2009 - Sept 30, 2010 PPPL: October 1, 2009 - September 30, 2010 SLAC: Oct 1, 2009 - Sept 30, 2010 JLab: Oct 1, 2009 - Sept 30, 2010 FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards

94

Ames: Oct 1, 2007 - Sept 30, 2008 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2007 - Sept 30, 2008 Ames: Oct 1, 2007 - Sept 30, 2008 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards Ames: Oct 1, 2007 - Sept 30, 2008 Argonne: Oct 1, 2007 - Sept 30, 2008 BNL: Oct 1, 2007 - Sept 30, 2008 Fermilab: Oct 1, 2007 - Sept 30, 2008 JLab: Oct 1, 2007 - Sept 30, 2008 LBNL: Oct 1, 2007 - Sept 30, 2008 ORNL: Oct 1, 2007 - Sept 30, 2008 PNNL: Oct 1, 2007 - Sept 30, 2008 PPPL: Oct 1, 2007 - Sept 30, 2008 SLAC: Oct 1, 2007 - Sept 30, 2008 FY 2007 SC Laboratory Performance Report Cards

95

Ames: Oct 1, 2008 - Sept 30, 2009 | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2008 - Sept 30, 2009 Ames: Oct 1, 2008 - Sept 30, 2009 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards Ames: Oct 1, 2008 - Sept 30, 2009 Argonne: Oct 1, 2008 - Sept 30, 2009 BNL: Oct 1, 2008 - Sept 30, 2009 Fermilab: Oct 1, 2008 - Sept 30, 2009 LBNL: Oct 1, 2008 - Sept 30, 2009 ORNL: Oct 1, 2008 - Sept 30, 2009 PNNL: Oct 1, 2008 - Sept 30, 2009 PPPL: Apr 1, 2009 - Sept 30, 2009 SLAC: Oct 1, 2008 - Sept 30, 2009 JLab: Oct 1, 2008 - Sept 30, 2009 FY 2008 SC Laboratory Performance Report Cards FY 2007 SC Laboratory Performance Report Cards

96

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

Office of Science (SC) Website

Ames Site Office CX Determinations Ames Site 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 Ames Site Office CX Determinations Print Text Size: A A A RSS Feeds FeedbackShare Page Categorical Exclusion Determination Documents (CX Determinations): *

97

Ames: Oct 1, 2011 - Sept 30, 2012| U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ames: Oct 1, 2011 - Sept 30, 2012 Ames: Oct 1, 2011 - Sept 30, 2012 Laboratory Policy and Evaluation (LPE) LPE Home Staff M&O Contracts SC Laboratory Appraisal Process FY 2013 SC Laboratory Performance Report Cards FY 2012 SC Laboratory Performance Report Cards Ames: Oct 1, 2011 - Sept 30, 2012 Argonne: Oct 1, 2011 - Sept 30, 2012 BNL: Oct 1, 2011 - Sept 30, 2012 Fermilab: Oct 1, 2011 - Sept 30, 2012 LBNL: Oct 1, 2011 - Sept 30, 2012 ORNL: Oct 1, 2011 - Sept 30, 2012 PNNL: Oct 1, 2011 - Sept 30, 2012 PPPL: Oct 1, 2011 - Sept 30, 2012 SLAC: Oct 1, 2011 - Sept 30, 2012 JLab: Oct 1, 2011 - Sept 30, 2012 FY 2011 SC Laboratory Performance Report Cards FY 2010 SC Laboratory Performance Report Cards FY 2009 SC Laboratory Performance Report Cards FY 2008 SC Laboratory Performance Report Cards FY 2007 SC Laboratory Performance Report Cards

98

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

99

Notes on the compatibility of type Ia supernovae data and varying--$G$ cosmology  

E-Print Network (OSTI)

Observational data for type Ia supernovae, shows that the expansion of the universe is accelerated. This accelerated expansion can be described by a cosmological constant or by dark energy models like quintessence. An interesting question may be raised here. Is it possible to describe the accelerated expansion of universe using varying--$G$ cosmological models? Here we shall show that the price for having accelerated expansion in slow--varying--$G$ models (in which the dynamical terms of $G$ are ignored) is to have highly non--conserved matter and also that it is in contradiction with other data.

Shojai, F

2013-01-01T23:59:59.000Z

100

Restframe I-band Hubble diagram for type Ia supernovae up toredshift z ~; 0.5  

SciTech Connect

We present a novel technique for fitting rest frame I-bandlight curves on a data set of 42 type Ia supernovae (SNe Ia). Using the result of the fit, we construct a Hubble diagram with 26 SNe from the subset at 0.01 < z < 0.1. Adding two SNe at z {approx} 0.5 yields results consistent with a flat Lambda-dominated ''concordance universe'' (OmegaM,Omega Lambda) = (0.25, 0.75). For one of these, SN 2000fr, new near infrared data are presented. The high redshift supernova NIR data are also used to test for systematic effects in the use of SNe Ia as distance estimators. A flat, Lambda = 0, universe where the faintness of supernovae at z {approx} 0.5 is due to grey dust homogeneously distributed in the intergalactic medium is disfavored based on the high-z Hubble diagram using this small data-set. However, the uncertainties are large and no firm conclusion may be drawn. We explore the possibility of setting limits on intergalactic dust based on B - I and B - V color measurements, and conclude that about 20 well measured SNe are needed to give statistically significant results. We also show that the high redshift restframe I-band data points are better fit by light curve templates that show a prominent second peak, suggesting that they are not intrinsically underluminous.

Nobili, S.; Amanullah, R.; Garavini, G.; Goobar, A.; Lidman, C.; Stanishev, V.; Aldering, G.; Antilogus, P.; Astier, P.; Burns, M.S.; Conley, A.; Deustua, S.E.; Ellis, R.; Fabbro, S.; Fadeyev, V.; Folatelli,G.; Gibbons, R.; Goldhaber, G.; Groom, D.E.; Hook, I.; Howell, D.A.; Kim,A.G.; Knop, R.A.; Nugent, P.E.; Pain, R.; Perlmutter, S.; Quimby, R.; Raux, J.; Regnault, N.; Ruiz-Lapuente, P.; Sainton, G.; Schahmaneche, K.; Smith, E.; Spadafora, A.L.; Thomas, R.C.; Wang, L.

2005-04-01T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
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to obtain the most current and comprehensive results.


101

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,...

102

Turbulence-Flame Interactions in Type Ia Supernovae  

E-Print Network (OSTI)

Turbulence-Flame Interactions in Type Ia Supernovae A. J.Normalised time (e) Normalised flame speed Normalised time (length scale (cm) Laminar flame width Gibson scale Cell

Aspden, Andrew J; Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50A-1148, Berkeley, CA 94720 (Authors 1, 2 & 3); Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (Author 4); Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (Author 5)

2008-01-01T23:59:59.000Z

103

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

104

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

105

Burning Thermals in Type Ia Supernovae A. J. Aspden1  

E-Print Network (OSTI)

Burning Thermals in Type Ia Supernovae A. J. Aspden1 , J. B. Bell1 , S. Dong2 , and S. E. Woosley2 ABSTRACT We develop a one-dimensional theoretical model for thermals burning in Type Ia supernovae based for the burning and for the expansion of the thermal due to changes in the background stratification found

Bell, John B.

106

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,

107

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)

176, "Annual Report of Natural and Supplemental Gas Supply and Disposition." 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...

108

Fitting Type Ia supernovae with coupled dark energy  

E-Print Network (OSTI)

We discuss the possible consistency of the recently discovered Type Ia supernovae at z>1 with models in which dark energy is strongly coupled to a significant fraction of dark matter, and in which an (asymptotic) accelerated phase exists where dark matter and dark energy scale in the same way. Such a coupling has been suggested for a possible solution of the coincidence problem, and is also motivated by string cosmology models of "late time" dilaton interactions. Our analysis shows that, for coupled dark energy models, the recent data are still consistent with acceleration starting as early as at $z=3$ (to within 90% c.l.), although at the price of a large "non-universality" of the dark energy coupling to different matter fields. Also, as opposed to uncoupled models which seem to prefer a ``phantom'' dark energy, we find that a large amount of coupled dark matter is compatible with present data only if the dark energy field has a conventional equation of state w>-1.

Amendola, L; Piazza, F; Amendola, Luca; Gasperini, Maurizio; Piazza, Federico

2004-01-01T23:59:59.000Z

109

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

110

Late Light Curves of Normally-Luminous Type Ia Supernovae  

E-Print Network (OSTI)

The use of Type Ia supernovae as cosmological tools has reinforced the need to better understand these objects and their light curves. The light curves of Type Ia supernovae are powered by the nuclear decay of $^{56}Ni \\to ^{56}Co \\to ^{56}Fe$. The late time light curves can provide insight into the behavior of the decay products and their effect of the shape of the curves. We present the optical light curves of six "normal" Type Ia supernovae, obtained at late times with template image subtraction, and the fits of these light curves to supernova energy deposition models.

J. C. Lair; M. D. Leising; P. A. Milne; G. G. Williams

2006-01-05T23:59:59.000Z

111

TYPE Ia SUPERNOVAE STRONGLY INTERACTING WITH THEIR CIRCUMSTELLAR MEDIUM  

SciTech Connect

Owing to their utility for measurements of cosmic acceleration, Type Ia supernovae (SNe Ia) are perhaps the best-studied class of SNe, yet the progenitor systems of these explosions largely remain a mystery. A rare subclass of SNe Ia shows evidence of strong interaction with their circumstellar medium (CSM), and in particular, a hydrogen-rich CSM; we refer to them as SNe Ia-CSM. In the first systematic search for such systems, we have identified 16 SNe Ia-CSM, and here we present new spectra of 13 of them. Six SNe Ia-CSM have been well studied previously, three were previously known but are analyzed in depth for the first time here, and seven are new discoveries from the Palomar Transient Factory. The spectra of all SNe Ia-CSM are dominated by H{alpha} emission (with widths of {approx}2000 km s{sup -1}) and exhibit large H{alpha}/H{beta} intensity ratios (perhaps due to collisional excitation of hydrogen via the SN ejecta overtaking slower-moving CSM shells); moreover, they have an almost complete lack of He I emission. They also show possible evidence of dust formation through a decrease in the red wing of H{alpha} 75-100 days past maximum brightness, and nearly all SNe Ia-CSM exhibit strong Na I D absorption from the host galaxy. The absolute magnitudes (uncorrected for host-galaxy extinction) of SNe Ia-CSM are found to be -21.3 mag {<=} M{sub R} {<=} -19 mag, and they also seem to show ultraviolet emission at early times and strong infrared emission at late times (but no detected radio or X-ray emission). Finally, the host galaxies of SNe Ia-CSM are all late-type spirals similar to the Milky Way, or dwarf irregulars like the Large Magellanic Cloud, which implies that these objects come from a relatively young stellar population. This work represents the most detailed analysis of the SN Ia-CSM class to date.

Silverman, Jeffrey M. [Department of Astronomy, University of Texas, Austin, TX 78712-0259 (United States); Nugent, Peter E. [Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States); Gal-Yam, Avishay; Arcavi, Iair; Ben-Ami, Sagi [Benoziyo Center for Astrophysics, 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; Graham, Melissa L. [Las Cumbres Observatory Global Telescope Network, Goleta, CA 93117 (United States); Filippenko, Alexei V.; Bloom, Joshua S.; Cenko, S. Bradley; Clubb, Kelsey I. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Cao, Yi; Horesh, Assaf; Kulkarni, Shrinivas R. [Cahill Center for Astrophysics, California Institute of Technology, Pasadena, CA 91125 (United States); Chornock, Ryan; Foley, Ryan J. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Coil, Alison L. [Department of Physics, University of California, San Diego, La Jolla, CA 92093 (United States); Griffith, Christopher V. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Kasliwal, Mansi M., E-mail: jsilverman@astro.as.utexas.edu [Observatories of the Carnegie Institution of Science, Pasadena, CA 91101 (United States); and others

2013-07-01T23:59:59.000Z

112

VELOCITY EVOLUTION AND THE INTRINSIC COLOR OF TYPE Ia SUPERNOVAE  

SciTech Connect

To understand how best to use observations of Type Ia supernovae (SNe Ia) to obtain precise and accurate distances, we investigate the relations between spectra of SNe Ia and their intrinsic colors. Using a sample of 1630 optical spectra of 255 SNe, based primarily on data from the CfA Supernova Program, we examine how the velocity evolution and line strengths of Si II {lambda}6355 and Ca II H and K are related to the B - V color at peak brightness. We find that the maximum-light velocity of Si II {lambda}6355 and Ca II H and K and the maximum-light pseudo-equivalent width of Si II {lambda}6355 are correlated with intrinsic color, with intrinsic color having a linear relation with the Si II {lambda}6355 measurements. Ca II H and K does not have a linear relation with intrinsic color, but lower-velocity SNe tend to be intrinsically bluer. Combining the spectroscopic measurements does not improve intrinsic color inference. The intrinsic color scatter is larger for higher-velocity SNe Ia-even after removing a linear trend with velocity-indicating that lower-velocity SNe Ia are more 'standard crayons'. Employing information derived from SN Ia spectra has the potential to improve the measurements of extragalactic distances and the cosmological properties inferred from them.

Foley, Ryan J.; Sanders, Nathan E.; Kirshner, Robert P., E-mail: rfoley@cfa.harvard.edu [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2011-12-01T23:59:59.000Z

113

The Rate of Type Ia Supernovae at High Redshift  

E-Print Network (OSTI)

We derive the rates of Type Ia supernovae (SNIa) over a wide range of redshifts using a complete sample from the IfA Deep Survey. This sample of more than 100 SNIa is the largest set ever collected from a single survey, and therefore uniquely powerful for a detailed supernova rate (SNR) calculation. Measurements of the SNR as a function of cosmological time offer a glimpse into the relationship between the star formation rate (SFR) and Type Ia SNR, and may provide evidence for the progenitor pathway. We observe a progressively increasing Type Ia SNR between redshifts z~0.3-0.8. The Type Ia SNR measurements are consistent with a short time delay (t~1 Gyr) with respect to the SFR, indicating a fairly prompt evolution of SNIa progenitor systems. We derive a best-fit value of SFR/SNR 580 h_70^(-2) M_solar/SNIa for the conversion factor between star formation and SNIa rates, as determined for a delay time of t~1 Gyr between the SFR and the Type Ia SNR. More complete measurements of the Type Ia SNR at z>1 are necessary to conclusively determine the SFR--SNR relationship and constrain SNIa evolutionary pathways.

Brian J. Barris; John L. Tonry

2005-09-22T23:59:59.000Z

114

The diversity of Type Ia Supernovae: evidence for systematics?  

E-Print Network (OSTI)

The photometric and spectroscopic properties of 26 well observed Type Ia Supernovae (SNeIa) were analyzed with the aim to explore SNIa diversity. The sample includes (Branch-)normal SNe as well as extreme events like SNe 1991T and 1991bg, while the truly peculiar SNIa, SN2000cx and SN2002cx are not included in our sample . A statistical treatment reveals the existence of three different groups. The first group (FAINT) consists of faint SNeIa similar to SN1991bg, with low expansion velocities and rapid evolution of SiII velocity. A second group consists of ``normal'' SNeIa, also with high temporal velocity gradient (HVG), but with brighter mean absolute magnitude =-19.3 and higher expansion velocities than the FAINT SNe. The third group includes both ``normal'' and SN1991T-like SNeIa: these SNe populate a narrow strip in the SiII velocity evolution plot, with a small velocity gradient (SVG), but have absolute magnitudes similar to HVGs. While the FAINT and HVG SNeIa together seem to define a relation between RSi(II) and Dm15(B), the SVG ones either do not conform with that relation or define a new, looser one. The RSi(II) pre-maximum evolution of HVGs is strikingly different from that of SVGs. The impact of this evidence on the understanding of SNIa diversity, in terms of explosion mechanisms, degree of ejecta mixing, and ejecta-CSM interaction, is discussed.

S. Benetti; E. Cappellaro; P. A. Mazzali; M. Turatto; G. Altavilla; F. Bufano; N. Elias-Rosa; R. Kotak; G. Pignata; M. Salvo; V. Stanishev

2004-11-02T23:59:59.000Z

115

Carbonate clumped isotope compositions of modern marine mollusk and brachiopod shells  

E-Print Network (OSTI)

, leaving the oxygen isotope paleother- mometer underdetermined in most geologic applicationsCarbonate clumped isotope compositions of modern marine mollusk and brachiopod shells Gregory A, Baltimore, MD 21218, USA b Department of Geological & Atmospheric Sciences, Iowa State University, Ames, IA

Grossman, Ethan L.

116

William Ames  

Science Conference Proceedings (OSTI)

... Physics Graduation Date: 5/2009 Hometown: Fairfax, Virginia Project: I worked measuring contact resistances and electron mobility in graphene ...

2010-10-05T23:59:59.000Z

117

Audit of Acquisition of Scientific Research at Ames Laboratory, ER-B-95-05  

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

S. DEPARTMENT OF ENERGY S. DEPARTMENT OF ENERGY OFFICE OF INSPECTOR GENERAL REPORT ON AUDIT OF ACQUISITION OF SCIENTIFIC RESEARCH AT AMES LABORATORY The Office of Inspector General wants to make the distribution of its reports as customer friendly and cost effective as possible. Therefore, this report will be available electronically through the Internet five to seven days after publication at the following alternative addresses: Department of Energy Headquarters Gopher gopher.hr.doe.gov Department of Energy Headquarters Anonymous FTP vm1.hqadmin.doe.gov U.S. Department of Energy Human Resources and Administration

118

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 -

119

DISTRIBUTED FLAMES IN TYPE Ia SUPERNOVAE  

Science Conference Proceedings (OSTI)

At a density near a few x10{sup 7} g cm{sup -3}, the subsonic burning in a Type Ia supernova (SN) enters the distributed regime (high Karlovitz number). In this regime, turbulence disrupts the internal structure of the flame, and so the idea of laminar burning propagated by conduction is no longer valid. The nature of the burning in this distributed regime depends on the turbulent Damkoehler number (Da{sub T}), which steadily declines from much greater than one to less than one as the density decreases to a few x10{sup 6} g cm{sup -3}. Classical scaling arguments predict that the turbulent flame speed s{sub T} , normalized by the turbulent intensity u-check, follows s{sub T}/u-check = Da{sub T}{sup 1/2} for Da{sub T} {approx}burns as a turbulently broadened effective unity Lewis number flame. This flame burns locally with speed s{sub l}ambda and width l{sub l}ambda, and we refer to this kind of flame as a lambda-flame. The burning becomes a collection of lambda-flames spread over a region approximately the size of the {integral} scale. While the total burning rate continues to have a well-defined average, s{sub T}{approx}u-check, the burning is unsteady. We present a theoretical framework, supported by both one-dimensional and three-dimensional numerical simulations, for the burning in these two regimes. Our results indicate that the average value of s{sub T} can actually be roughly twice u-check for Da{sub T} {approx}> 1, and that localized excursions to as much as 5 times u-check can occur. We also explore the properties of the individual flames, which could be sites for a transition to detonation when Da{sub T} {approx} 1. The lambda-flame speed and width can be predicted based on the turbulence in the star (specifically the energy dissipation rate epsilon*) and the turbulent nuclear burning timescale of the fuel tau {sup T}{sub nuc}. We propose a practical method for measuring s{sub l}ambda and l{sub l}ambda based on the scaling relations and small-scale computationally inexpensive simulations. This suggests that a simple turbulent flame model can be easily constructed suitable for large-scale distributed SNe flames. These results will be useful both for characterizing the deflagration speed in larger full-star simulations, where the flame cannot be resolved, and for predicting when detonation occurs.

Aspden, A. J.; Bell, J. B. [Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50A-1148, Berkeley, CA 94720 (United States); Woosley, S. E. [Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (United States)

2010-02-20T23:59:59.000Z

120

Redshift-Independent Distances to Type Ia Supernovae  

E-Print Network (OSTI)

We describe a procedure for accurately determining luminosity distances to Type Ia supernovae (SNe Ia) without knowledge of redshift. This procedure, which may be used as an extension of any of the various distance determination methods currently in use, is based on marginalizing over redshift, removing the requirement of knowing $z$ a priori. We demonstrate that the Hubble diagram scatter of distances measured with this technique is approximately equal to that of distances derived from conventional redshift-specific methods for a set of 60 nearby SNe Ia. This indicates that accurate distances for cosmological SNe Ia may be determined without the requirement of spectroscopic redshifts, which are typically the limiting factor for the number of SNe that modern surveys can collect. Removing this limitation would greatly increase the number of SNe for which current and future SN surveys will be able to accurately measure distance. The method may also be able to be used for high-$z$ SNe Ia to determine cosmological density parameters without redshift information.

Brian J. Barris; John L. Tonry

2004-08-04T23:59:59.000Z

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121

National Laboratories - Energy Innovation Portal  

Name Address City, State; Ames Laboratory: Ames Laboratory: Ames, IA: Argonne National Laboratory: 9700 S. Cass Avenue: Argonne, IL: Brookhaven National Laboratory

122

Ames Lab Plays Elemental Role in New PBS Special | Department of Energy  

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

Lab Plays Elemental Role in New PBS Special Lab Plays Elemental Role in New PBS Special Ames Lab Plays Elemental Role in New PBS Special April 4, 2012 - 2:34pm Addthis New York Times technology correspondent David Pogue -- host of NOVA’s popular “Making Stuff” series -- takes viewers on a quest to understand chemistry and all of the materials of life: the 118 unique elements that make up the amazing periodic table, including the 90 naturally-occurring elements and those created by scientists. | Photo courtesy of PBS. New York Times technology correspondent David Pogue -- host of NOVA's popular "Making Stuff" series -- takes viewers on a quest to understand chemistry and all of the materials of life: the 118 unique elements that make up the amazing periodic table, including the 90 naturally-occurring

123

The type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf star  

E-Print Network (OSTI)

The absolute magnitudes of Type IA supernovae. Astrophys. J.in a Sublu- o minous Type Ia Supernova: SpectropolarimetryL. Could There Be a Hole in Type Ia Super- novae? Astrophys.

2008-01-01T23:59:59.000Z

124

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

125

CALIFORNIA INSTITUTE OF TECHNOLOGYDISTINGUISHED ALUMNI AWARDS Dr. Mihran S. Agbabian MS 1948 CE Fred Champion Professor Emeritus of Civil Engineering, University  

E-Print Network (OSTI)

CALIFORNIA INSTITUTE OF TECHNOLOGYDISTINGUISHED ALUMNI AWARDS Dr. Mihran S. Agbabian MS 1948 CE Fred Champion Professor Emeritus of Civil Engineering, University of Southern California 2000 Dr. Bruce N. Ames PhD 1953 BI Professor/Biochemistry, University of California, Berkeley 1977 Dr. John P

Greer, Julia R.

126

Microsoft PowerPoint - Joel Riekin.pptx  

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

University University Iowa State University of Science and Technology Simplified Powder Processing and Microstructural Control of Fe-based ODS Alloys Support from the Department of Energy-Office of Fossil Energy is gratefully acknowledged through Ames Laboratory contract no. DE-AC02-07CH11358 J. R. Rieken 1 , I.E. Anderson 2 , and M.J. Kramer 2 1 Materials Science and Engineering, Iowa State University, Ames, IA 2 Division of Materials Sciences and Engineering, Ames Laboratory (USDOE), Ames, IA "Fe-Based ODS Alloys: Role and Future Applications" Fabrication, Microstructure Preservation & Mechanical Properties University of California-San Diego: November 18th, 2010, San Diego, CA Iowa State University Iowa State University of Science and Technology Future Generation Power Reactors

127

Optical Spectra of Type Ia Supernovae at z=0.46 and z=1.2  

E-Print Network (OSTI)

We present optical spectra, obtained with the Keck 10-m telescope, of two high-redshift type Ia supernovae (SNe Ia) discovered by the High-z Supernova Search Team: SN 1999ff at z=0.455 and SN 1999fv at z~1.2, the highest-redshift published SN Ia spectrum. Both SNe were at maximum light when the spectra were taken. We compare our high-z spectra with low-z normal and peculiar SNe Ia as well as with SNe Ic, Ib, and II. There are no significant differences between SN 1999ff and normal SNe Ia at low redshift. SN 1999fv appears to be a SN Ia and does not resemble the most peculiar nearby SNe Ia.

Coil, A L; Filippenko, A V; Leonard, D C; Tonry, J; Riess, A G; Challis, P M; Clocchiatti, A; Garnavich, P M; Hogan, C J; Jha, S; Kirshner, R P; Leibundgut, B; Phillips, M M; Schmidt, B P; Schommer, R A; Smith, R C; Soderberg, A M; Spyromilio, J; Stubbs, C; Suntzeff, N B; Woudt, P A; Coil, Alison L.; Matheson, Thomas; Filippenko, Alexei V.; Leonard, Douglas C.; Tonry, John; Riess, Adam G.; Challis, Peter; Clocchiatti, Alejandro; Garnavich, Peter M.; Hogan, Craig J.; Jha, Saurabh; Kirshner, Robert P.; Schmidt, Brian P.; Schommer, Robert A.; Soderberg, Alicia M.; Stubbs, Christopher; Suntzeff, Nicholas B.; Woudt, Patrick

2000-01-01T23:59:59.000Z

128

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 they probe the dependence of this dispersion on cosmological parameters and show that information about the amplitude of clustering, {sigma}{sub s}, is contained in the scatter. In principle, it will be possible to constrain {sigma}{sub s} to within 5% with observations of 2000 Type Ia Supernovae. They 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; /Fermilab /Chicago U., Astron. Astrophys. Ctr.; Vallinotto, Alberto; /Fermilab /Chicago U.

2005-11-01T23:59:59.000Z

129

Type Ia Supernova Spectral Line Ratios as LuminosityIndicators  

SciTech Connect

Type Ia supernovae have played a crucial role in thediscovery of the dark energy, via the measurement of their light curvesand the determination of the peak brightness via fitting templates to theobserved lightcurve shape. Two spectroscopic indicators are also known tobe well correlated with peak luminosity. Since the spectroscopicluminosity indicators are obtained directly from observed spectra, theywill have different systematic errors than do measurements usingphotometry. Additionally, these spectroscopic indicators may be usefulfor studies of effects of evolution or age of the SNe~;Ia progenitorpopulation. We present several new variants of such spectroscopicindicators which are easy to automate and which minimize the effects ofnoise. We show that these spectroscopic indicators can be measured byproposed JDEM missions such as snap and JEDI.

Bongard, Sebastien; Baron, E.; Smadja, G.; Branch, David; Hauschildt, Peter H.

2005-12-07T23:59:59.000Z

130

Investigating the Flame Microstructure in Type Ia Supernovae  

E-Print Network (OSTI)

We present a numerical model to study the behavior of thermonuclear flames in the discontinuity approximation. This model is applied to investigate the Landau-Darrieus instability under conditions found in Type Ia supernova explosions of Chandrasekhar mass white dwarfs. This is a first step to explore the flame microstructure in these events. The model reproduces Landau's linearized stability analysis in early stages of the flame evolution and the stabilization in a cellular flame structure in the nonlinear stage.

F. K. Roepke; W. Hillebrandt; J. C. Niemeyer

2002-04-02T23:59:59.000Z

131

Reflections on Reflexions: I. Light Echoes in Type Ia Supernovae  

E-Print Network (OSTI)

In the last ten years, observational evidences about a possible connection between Type Ia Supernovae (SNe) properties and the environment where they explode have been steadily growing. In this paper I discuss, from a theoretical point of view but with an observer's perspective, the usage of light echoes (LEs) to probe the CSM around SNe of Type Ia since, in principle, they give us a unique opportunity of getting a three-dimensional description of the SN environment. In turn, this can be used to check the often suggested association of some Ia's with dusty/star forming regions, which would point to a young population for the progenitors. After giving a brief introduction to the LE phenomenon in single scattering approximation, I derive analytical and numerical solutions for the optical light and colour curves for a few simple dust geometries. A fully 3D multiple scattering treatment has also been implemented in a Monte Carlo code, which I have used to investigate the effects of multiple scattering. In particu...

Patat, F

2004-01-01T23:59:59.000Z

132

Could There Be A Hole In Type Ia Supernovae?  

E-Print Network (OSTI)

In the favored progenitor scenario, Type Ia supernovae arise from a white dwarf accreting material from a non-degenerate companion star. Soon after the white dwarf explodes, the ejected supernova material engulfs the companion star; two-dimensional hydrodynamical simulations by Marietta et. al. show that, in the interaction, the companion star carves out a conical hole of opening angle 30-40 degrees in the supernova ejecta. In this paper we use multi-dimensional Monte Carlo radiative transfer calculations to explore the observable consequences of an ejecta-hole asymmetry. We calculate the variation of the spectrum, luminosity, and polarization with viewing angle for the aspherical supernova near maximum light. We find that the supernova looks normal from almost all viewing angles except when one looks almost directly down the hole. In the latter case, one sees into the deeper, hotter layers of ejecta. The supernova is relatively brighter and has a peculiar spectrum characterized by more highly ionized species, weaker absorption features, and lower absorption velocities. The spectrum viewed down the hole is comparable to the class of SN 1991T-like supernovae. We consider how the ejecta-hole asymmetry may explain the current spectropolarimetric observations of SNe Ia, and suggest a few observational signatures of the geometry. Finally, we discuss the variety currently seen in observed SNe Ia and how an ejecta-hole asymmetry may fit in as one of several possible sources of diversity.

Daniel Kasen; Peter Nugent; R. C. Thomas; Lifan Wang

2003-11-01T23:59:59.000Z

133

THE SDSS-II SUPERNOVA SURVEY: PARAMETERIZING THE TYPE Ia SUPERNOVA RATE AS A FUNCTION OF HOST GALAXY PROPERTIES  

Science Conference Proceedings (OSTI)

Using data from the Sloan Digital Sky Supernova Survey-II (SDSS-II SN Survey), we measure the rate of Type Ia supernovae (SNe Ia) as a function of galaxy properties at intermediate redshift. A sample of 342 SNe Ia with 0.05 0.15) SNe Ia in highly star-forming galaxies. We consider that the high levels of dust in these systems may be obscuring the reddest and faintest SNe Ia.

Smith, Mathew [Department of Physics, University of Western Cape, Bellville 7530, Cape Town (South Africa); Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX (United Kingdom); Dilday, Benjamin [Las Cumbres Observatory Global Telescope Network, 6740 Cortona Dr., Suite 102, Goleta, CA 93117 (United States); Marriner, John; Frieman, Joshua [Center for Particle Astrophysics, Fermilab, P.O. Box 500, Batavia, IL 60510 (United States); Kessler, Richard [Department of Astronomy and Astrophysics, University of Chicago, 5640 S. Ellis Ave, Chicago, IL 60637 (United States); Bassett, Bruce [African Institute for Mathematical Sciences, 6-8 Melrose Road, Muizenberg 7945 (South Africa); Cinabro, David [Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States); Garnavich, Peter [Department of Physics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556 (United States); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers, State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Lampeitl, Hubert [Astrophysics, Cosmology and Gravity Centre (ACGC), Department of Mathematics and Applied Mathematics, University of Cape Town, Rondebosch 7701 (South Africa); Sako, Masao [Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Sollerman, Jesper, E-mail: matsmith2@gmail.com [Oskar Klein Centre, Department of Astronomy, AlbaNova, Stockholm University, SE-106 91 Stockholm (Sweden)

2012-08-10T23:59:59.000Z

134

Status report on the collection and preparation of coal samples for the Ames Laboratory Coal Library  

SciTech Connect

In comparing and evaluating experimental results on coal generated in different laboratories, or even within the same laboratory, it is necessary to begin the work on samples which are reproducibly equivalent. Also, there must be a sufficient store of the material for ongoing investigations. Thus, the problem is difficult because of the heterogeneity of coal, both at the large bulk level and at the microscopic sample level. This affects the capability to assess the significance of discrepancies in experimental results among laboratories, even if the experimental conditions are carefully controlled. In collecting coal samples from a mine or a preparation plant, considerations must be made to assure a representative bulk sampling and to reduce the material into suitable working samples which accurately and reproducibly reflect the composition of the bulk sample. At the collection site, changes in the coal occur immediately upon exposure to air, resulting in marked deterioration of caking properties, solubility, tar yield, heating value, and other properties. This necessitates that measures be followed to preserve the samples in ''inert'' environments as much as possible. Thus, at each point the collection, transportation, preparation, storage, and preservation of the samples must be rigorously controlled and reproducibly implemented. Such precautions are emphasized in descriptions of the Penn State and the Exxon coal collections. This interim report provides information on an approach to establish a coal library at the Ames Laboratory. The coals serve as a collection of well-characterized materials for both the laboratory's own staff and, eventually, for other interested investigators. This report documents our efforts to date and includes the criteria for coal selection, the procedure for coal sampling, and the techniques utilized in the prevention of changes in the coals throughout the period prior to utilization. 8 refs., 2 figs., 6 tabs.

Biggs, D.L.; Birlingmair, D.H.; Fisher, R.W.; Greer, R.T.; Kaelin, R.A.; Markuszewski, R.; Smith, B.F.; Squires, T.G.; Venier, C.G.; Wheelock, T.D.

1985-01-01T23:59:59.000Z

135

THE DIFFUSE GAMMA-RAY BACKGROUND FROM TYPE Ia SUPERNOVAE  

SciTech Connect

The origin of the diffuse extragalactic gamma-ray background (EGB) has been intensively studied but remains unsettled. Current popular source candidates include unresolved star-forming galaxies, starburst galaxies, and blazars. In this paper, we calculate the EGB contribution from the interactions of cosmic rays accelerated by Type Ia supernovae (SNe), extending earlier work that only included core-collapse SNe. We consider Type Ia events not only in star-forming galaxies, but also in quiescent galaxies that lack star formation. In the case of star-forming galaxies, consistently including Type Ia events makes little change to the star-forming EGB prediction, so long as both SN types have the same cosmic-ray acceleration efficiencies in star-forming galaxies. Thus, our updated EGB estimate continues to show that star-forming galaxies can represent a substantial portion of the signal measured by Fermi. In the case of quiescent galaxies, conversely, we find a wide range of possibilities for the EGB contribution. The dominant uncertainty we investigated comes from the mass in hot gas in these objects, which provides targets for cosmic rays; total gas masses are as yet poorly known, particularly at larger radii. Additionally, the EGB estimation is very sensitive to the cosmic-ray acceleration efficiency and confinement, especially in quiescent galaxies. In the most optimistic allowed scenarios, quiescent galaxies can be an important source of the EGB. In this case, star-forming galaxies and quiescent galaxies together will dominate the EGB and leave little room for other contributions. If other sources, such as blazars, are found to have important contributions to the EGB, then either the gas mass or cosmic-ray content of quiescent galaxies must be significantly lower than in their star-forming counterparts. In any case, improved Fermi EGB measurements will provide important constraints on hot gas and cosmic rays in quiescent galaxies.

Lien, Amy; Fields, Brian D. [Department of Physics, University of Illinois, Urbana, IL 61801 (United States)

2012-03-10T23:59:59.000Z

136

Reflections on Reflexions: I. Light Echoes in Type Ia Supernovae  

E-Print Network (OSTI)

In the last ten years, observational evidences about a possible connection between Type Ia Supernovae (SNe) properties and the environment where they explode have been steadily growing. In this paper I discuss, from a theoretical point of view but with an observer's perspective, the usage of light echoes (LEs) to probe the CSM around SNe of Type Ia since, in principle, they give us a unique opportunity of getting a three-dimensional description of the SN environment. In turn, this can be used to check the often suggested association of some Ia's with dusty/star forming regions, which would point to a young population for the progenitors. After giving a brief introduction to the LE phenomenon in single scattering approximation, I derive analytical and numerical solutions for the optical light and colour curves for a few simple dust geometries. A fully 3D multiple scattering treatment has also been implemented in a Monte Carlo code, which I have used to investigate the effects of multiple scattering. In particular, I have explored in detail the LE colour dependency from time and dust distribution, since this is a promising tool to determine the dust density and derive the effective presence of multiple scattering from the observed properties. Finally, again by means of Monte Carlo simulations, I have studied the effects of multiple scattering on the LE linear polarization, analyzing the dependencies from the dust parameters and geometry. Both the analytical formalism and MC codes described in this paper can be used for any LE for which the light curve of the central source is known.

F. Patat

2004-09-28T23:59:59.000Z

137

Turbulence-Flame Interactions in Type Ia Supernovae  

SciTech Connect

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 x 107 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 x 107 g cm-3 where the nature of the burning changes ualitatively. By 1 x 107 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.

Lawrence Berkeley National Laboratory, 1 Cyclotron Road, MS 50A-1148, Berkeley, CA 94720 (Authors 1, 2& 3); Department of Astronomy and Astrophysics, University of California at Santa Cruz, Santa Cruz, CA 95064 (Author 4); Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794 (Author 5); Aspden, Andrew J; Aspden, Andrew J.; Bell, John B.; Day, Marc S.; Woosley, Stan E.; Zingale, Mike

2008-05-27T23:59:59.000Z

138

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

139

2901 South Loop Drive, Suite 3100 ~ Ames, Iowa 50010-8634 IowaStateUniversity~Universityof Missouri-Columbia~LincolnUniversity  

E-Print Network (OSTI)

in selecting maintenance strategies. Typically, a roadway management system includes a set of analysis tools-Swailmi (1994) introduces the framework for municipal maintenance management systems. It is focused for use for a maintenance management system (MMS). Then, it is combined with city's subsystem to eliminate conflicts between

Beresnev, Igor

140

REPORT OF THE PRESIDENT,~ -01 OF THE UNIVERSITY OF BRITISH COLm~IA~ -  

E-Print Network (OSTI)

38 R~port of the Instructor in Physical Education for Women 39 g~portof the Office!: Co Second Yearoo.....eoQ....oo........... Third Year.....OOO..OO..O.............Fourth Ye~.O..O.O.OIO; Engineer 134; Farmer 75; Inspector 21; Insurance 34; Lawyer 39; Lumberman 33; Manager 54; Merchant 97

Pulfrey, David L.

Note: This page contains sample records for the topic "university ames ia" 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

Ames/Salmonella mutagenicity assay of natural and synthetic crude oils including a Fischer-Retorted Estonian shale oil  

DOE Green Energy (OSTI)

DMSO extracts of a variety of natural and synthetic crude oils were tested for genotoxic activity in the Ames/Salmonella bioassay. Both mutagenic and cytotoxic potentials are cited. Natural crude oils and their refined products and upgraded synfuels are less mutagenic than parent crude shale oils which in turn are less mutagenic than the coal derived distillate blend sample, SRC II. However, this order is not true for cytotoxicity induced by these oil samples; therefore, caution must be exercised in the assessment of their mutagenic potential without consideration of other influential factors including cytotoxicity.

Strniste, G.F.; Nickols, J.W.

1981-01-01T23:59:59.000Z

142

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

143

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

144

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

145

Princeton University  

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

WHG 72711 PRINCETON UNIVERSITY INSTRUCTIONS FOR INVENTION DISCLOSURE FORM This Invention Disclosure Form is for use by University Faculty, Staff, and Students to report the...

146

*Corresponding author. E-mail address: #ame@zen.phys.columbia.edu (J. Hong).  

E-Print Network (OSTI)

Nuclear Instruments and Methods in Physics Research A 540 (2005) 464­469 Fusion neutron detector calibration using a table-top laser generated plasma neutron source R. Hartkea , D.R. Symesa,?, F. Buersgensa, Department of Physics, The University of Texas at Austin, Austin, TX 78712, USA b Sandia National

147

Next-Generation Petascale Simulations of Type Ia Supernovae ...  

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

deflagration to detonation transition model Deflagration to detonation transition model. Min lOng, Dan van Rossum, Sean Couch, George Jordan, Brad Gallagher, Don Lamb, University...

148

Type Ia Supernovae Rates and Galaxy Clustering from the CFHT Supernova Legacy Survey  

E-Print Network (OSTI)

The Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS) has created a large homogeneous database of intermediate redshift (0.2 rates, properties, and host galaxy star formation rates. The SNLS SN Ia database has now been combined with a photometric redshift galaxy catalog and an optical galaxy cluster catalog to investigate the possible influence of galaxy clustering on the SN Ia rate, over and above the expected effect due to the dependence of SFR on clustering through the morphology-density relation. We identify three cluster SNe Ia, plus three additional possible cluster SNe Ia, and find the SN Ia rate per unit mass in clusters at intermediate redshifts is consistent with the rate per unit mass in field early-type galaxies and the SN Ia cluster rate from low redshift cluster targeted surveys. We also find the number of SNe Ia in cluster environments to be within a factor of two of expectations from the two component SNIa rate model.

M. L. Graham; C. J. Pritchet; M. Sullivan; S. D. J. Gwyn; J. D. Neill; E. Y. Hsiao; P. Astier; D. Balam; C. Balland; S. Basa; R. G. Carlberg; A. Conley; D. Fouchez; J. Guy; D. Hardin; I. M. Hook; D. A. Howell; R. Pain; K. Perrett; N. Regnault; S. Baumont; J. Le Du; C. Lidman; S. Perlmutter; P. Ripoche; N. Suzuki; E. S. Walker; T. Zhang

2008-01-31T23:59:59.000Z

149

Mtrologie des supernovae de type Ia pour la cosmologie : instrumentation et analyse calorimtrique.  

E-Print Network (OSTI)

??L'utilisation des supernovae de type Ia comme indicateurs de distance est un pilier du modle de concordance actuel en cosmologie. Le travail d'instrumentation prsent dans (more)

Juramy, Claire

2006-01-01T23:59:59.000Z

150

Diversity of supernovae Ia determined using equivalent widths of Si II 4000  

E-Print Network (OSTI)

Spectroscopic and photometric properties of low and high-z supernovae Ia (SNe Ia) have been analyzed in order to achieve a better understanding of their diversity and to identify possible SN Ia sub-types. We use wavelet transformed spectra in which one can easily measure spectral features. We investigate the \\ion{Si}{II} 4000 equivalent width ($EW_w\\lbrace\\ion{Si}{II}\\rbrace$). The ability and, especially, the ease in extending the method to SNe at high-$z$ is demonstrated. We applied the method to 110 SNe Ia and found correlations between $EW_w\\lbrace\\ion{Si}{II}\\rbrace$ and parameters related to the light-curve shape for 88 supernovae with available photometry. No evidence for evolution of $EW_w\\lbrace\\ion{Si}{II}\\rbrace$ with redshift is seen. Three sub-classes of SNe Ia were confirmed using an independent cluster analysis with only light-curve shape, colour, and $EW_w\\lbrace\\ion{Si}{II}\\rbrace$. SNe from high-$z$ samples seem to follow a similar grouping to nearby objects. The $EW_w\\lbrace\\ion{Si}{II}\\rbrace$ value measured on a single spectrum may point towards SN Ia sub-classification, avoiding the need for expansion velocity gradient calculations.

V. Arsenijevic; S. Fabbro; A. M. Mourao; A. J. Rica da Silva

2008-09-18T23:59:59.000Z

151

Office of Acquisition and Assistance - Information for Small...  

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

or support service activities, please contact me directly. M&O Contractors Location Ames Laboratory Ames, IA Argonne National Laboratory Argonne, IL Brookhaven National...

152

ATP Project Brief - 00-00-5561  

Science Conference Proceedings (OSTI)

... City, UT) will be subcontracted to develop fabrication methods for constructing AMRs from brittle materials, and Ames Laboratory (Ames, IA) will be ...

153

Latin American Section List  

Science Conference Proceedings (OSTI)

Name AffiliationCity, State, CountryLatin American Section2013 Members208 Members as of October 1, 2013Abril, RubenDSM Nutritional ProductsBoulder, CO, USAAcevedo, NuriaUniversity of GuelphAmes, IA, USAAcosta, EdgarUniversity of TorontoToronto, ON, CanadaA

154

Development of Enhanced Electric Arc Furnace Models for Transient Analysis Gilsoo Jang  

E-Print Network (OSTI)

University Seoul, Korea Weiguo Wang ESCA-Alstom Tacoma, WA USA G. T. Heydt Ari- zona State Univer- sity Tempe, AZ USA S. S. Venkata Iowa State Uni- versity Ames, IA USA Byongjun Lee Korea University Korea to the interaction of the high demand currents of the loads with the supply system impedance. In order to adequately

155

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

156

A preliminary analysis of the energy transfer between the dark sectors of the Universe  

E-Print Network (OSTI)

We study the mutual interaction between the dark sectors (dark matter and dark energy) of the Universe by resorting to the extended thermodynamics of irreversible processes and constrain the former with supernova type Ia data. As a byproduct, the present dark matter temperature results in good agreement with independent estimates of the temperature of the gas of sterile neutrinos.

Jia Zhou; Bin Wang; Diego Pavon; Elcio Abdalla

2008-07-20T23:59:59.000Z

157

NREL Unsteady Aerodynamics Experiment in the NASA-Ames Wind Tunnel: A Comparison of Predictions to Measurements  

SciTech Connect

Currently, wind turbine designers rely on safety factors to compensate for the effects of unknown loads acting on the turbine structure. This results in components that are overdesigned because precise load levels and load paths are unknown. To advance wind turbine technology, the forces acting on the turbine structure must be accurately characterized because these forces translate directly into loads imparted to the wind turbine structure and resulting power production. Once these forces are more accurately characterized, we will better understand load paths and can therefore optimize turbine structures. To address this problem, the National Renewable Energy Laboratory (NREL) conducted the Unsteady Aerodynamics Experiment (UAE), which was a test of an extensively instrumented wind turbine in the giant NASA-Ames 24.4-m (80 feet) by 36.6-m (120 feet) wind tunnel. To maximize the benefits from testing, NREL formed a Science Panel of advisers comprised of wind turbine aerodynamics and modeling experts throughout the world. NREL used the Science Panel's guidance to specify the conditions and configurations under which the turbine was operated in the wind tunnel. The panel also helped define test priorities and objectives that would be effective for wind turbine modeling tool development and validation.

Simms, D.; Schreck, S.; Hand, M.; Fingersh, L.J.

2001-06-22T23:59:59.000Z

158

Gamow-Teller strengths in 24Na using the 24Mg(t,3He) reaction at 115 AMeV  

E-Print Network (OSTI)

Gamow-Teller transitions from 24Mg to 24Na were studied via the (t,3He) reaction at 115 AMeV using a secondary triton beam produced via fast fragmentation of 150 AMeV 16O ions. Compared to previous (t,3He) experiments at this energy that employed a primary alpha beam, the secondary beam intensity is improved by about a factor of five. Despite the large emittance of the secondary beam, an excitation-energy resolution of ~200 keV is achieved. A good correspondence is found between the extracted Gamow-Teller strength distribution and those available from other charge-exchange probes. Theoretical calculations using the newly developed USDA and USDB sd-shell model interactions reproduce the data well.

M. E. Howard; R. G. T. Zegers; Sam M. Austin; D. Bazin; B. A. Brown; A. L. Cole; B. Davids; M. Famiano; Y. Fujita; A. Gade; D. Galaviz; G. W. Hitt; M. Matos; S. D. Reitzner; C. Samanta; L. J. Schradin; Y. Shimbara; E. E. Smith; C. Simenel

2008-07-15T23:59:59.000Z

159

THE FIRST MAXIMUM-LIGHT ULTRAVIOLET THROUGH NEAR-INFRARED SPECTRUM OF A TYPE Ia SUPERNOVA  

Science Conference Proceedings (OSTI)

We present the first maximum-light ultraviolet (UV) through near-infrared (NIR) Type Ia supernova (SN Ia) spectrum. This spectrum of SN 2011iv was obtained nearly simultaneously by the Hubble Space Telescope at UV/optical wavelengths and the Magellan Baade telescope at NIR wavelengths. These data provide the opportunity to examine the entire maximum-light SN Ia spectral energy distribution. Since the UV region of an SN Ia spectrum is extremely sensitive to the composition of the outer layers of the explosion, which are transparent at longer wavelengths, this unprecedented spectrum can provide strong constraints on the composition of the SN ejecta, and similarly the SN explosion and progenitor system. SN 2011iv is spectroscopically normal, but has a relatively fast decline ({Delta}m{sub 15}(B) = 1.69 {+-} 0.05 mag). We compare SN 2011iv to other SNe Ia with UV spectra near maximum light and examine trends between UV spectral properties, light-curve shape, and ejecta velocity. We tentatively find that SNe with similar light-curve shapes but different ejecta velocities have similar UV spectra, while those with similar ejecta velocities but different light-curve shapes have very different UV spectra. Through a comparison with explosion models, we find that both a solar-metallicity W7 and a zero-metallicity delayed-detonation model provide a reasonable fit to the spectrum of SN 2011iv from the UV to the NIR.

Foley, Ryan J.; Marion, G. Howie; Challis, Peter; Kirshner, Robert P.; Berta, Zachory K. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Kromer, Markus; Taubenberger, Stefan; Hillebrandt, Wolfgang; Roepke, Friedrich K.; Ciaraldi-Schoolmann, Franco; Seitenzahl, Ivo R. [Max-Planck-Institut fuer Astrophysik, Karl-Schwarzschild-Strasse 1, D-85748 Garching bei Muenchen (Germany); Pignata, Giuliano [Departamento de Ciencias Fisicas, Universidad Andres Bello, Avda. Republica 252, Santiago (Chile); Stritzinger, Maximilian D. [Department of Physics and Astronomy, Aarhus University, Ny Munkegade, DK-8000 Aarhus C (Denmark); Filippenko, Alexei V.; Li Weidong; Silverman, Jeffrey M. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Folatelli, Gaston [Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), Todai Institutes for Advanced Study, University of Tokyo, Kashiwa 277-8583 (Japan); Hsiao, Eric Y.; Morrell, Nidia I. [Carnegie Observatories, Las Campanas Observatory, La Serena (Chile); Simcoe, Robert A., E-mail: rfoley@cfa.harvard.edu [MIT-Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, 37-664D Cambridge, MA 02139 (United States); and others

2012-07-01T23:59:59.000Z

160

Spectral Modeling of SNe Ia Near Maximum Light: Probing the Characteristics of Hydro Models  

E-Print Network (OSTI)

We have performed detailed NLTE spectral synthesis modeling of 2 types of 1-D hydro models: the very highly parameterized deflagration model W7, and two delayed detonation models. We find that overall both models do about equally well at fitting well observed SNe Ia near to maximum light. However, the Si II 6150 feature of W7 is systematically too fast, whereas for the delayed detonation models it is also somewhat too fast, but significantly better than that of W7. We find that a parameterized mixed model does the best job of reproducing the Si II 6150 line near maximum light and we study the differences in the models that lead to better fits to normal SNe Ia. We discuss what is required of a hydro model to fit the spectra of observed SNe Ia near maximum light.

E. Baron; S. Bongard; David Branch; Peter H. Hauschildt

2006-03-03T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" 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

THE LOW-VELOCITY, RAPIDLY FADING TYPE Ia SUPERNOVA 2002es  

SciTech Connect

SN 2002es is a peculiar subluminous Type Ia supernova (SN Ia) with a combination of observed characteristics never before seen in an SN Ia. At maximum light, SN 2002es shares spectroscopic properties with the underluminous SN 1991bg subclass of SNe Ia, but with substantially lower expansion velocities ({approx}6000 km s{sup -1}) more typical of the peculiar SN 2002cx subclass. Photometrically, SN 2002es differs from both SN 1991bg-like and SN 2002cx-like supernovae. Although at maximum light it is subluminous (M{sub B} = -17.78 mag), SN 2002es has a relatively broad light curve ({Delta}m{sub 15}(B) = 1.28 {+-} 0.04 mag), making it a significant outlier in the light-curve width versus luminosity relationship. We estimate a {sup 56}Ni mass of 0.17 {+-} 0.05 M{sub Sun} synthesized in the explosion, relatively low for an SN Ia. One month after maximum light, we find an unexpected plummet in the bolometric luminosity. The late-time decay of the light curves is inconsistent with our estimated {sup 56}Ni mass, indicating that either the light curve was not completely powered by {sup 56}Ni decay or the ejecta became optically thin to {gamma}-rays within a month after maximum light. The host galaxy is classified as an S0 galaxy with little to no star formation, indicating that the progenitor of SN 2002es is likely from an old stellar population. We also present a less extensive data set for SN 1999bh, an object which shares similar photometric and spectroscopic properties. Both objects were found as part of the Lick Observatory Supernova Search, allowing us to estimate that these objects should account for 2.5% of SNe Ia within a fixed volume. Current theoretical models are unable to explain the observed characteristics of SN 2002es.

Ganeshalingam, Mohan; Li Weidong; Filippenko, Alexei V.; Silverman, Jeffrey M.; Shen, Ken J. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Chornock, Ryan; Foley, Ryan J.; Kirshner, Robert P.; Calkins, Mike [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Matheson, Thomas [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Milne, Peter, E-mail: mganesh@astro.berkeley.edu [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States)

2012-06-01T23:59:59.000Z

162

EARLY PHASE OBSERVATIONS OF EXTREMELY LUMINOUS TYPE Ia SUPERNOVA 2009dc  

Science Conference Proceedings (OSTI)

We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is DELTAm{sub 15}(B) = 0.65 +- 0.03, which is one of the slowest among SNe Ia. The peak V-band absolute magnitude is estimated to be M{sub V} = -19.90 +- 0.15 mag if no host extinction is assumed. It reaches M{sub V} = -20.19 +- 0.19 mag if we assume the host extinction of A{sub V} = 0.29 mag. SN 2009dc belongs to the most luminous class of SNe Ia, like SNe 2003fg and 2006gz. Our JHK{sub s} -band photometry shows that this SN is also one of the most luminous SNe Ia in near-infrared wavelengths. We estimate the ejected {sup 56}Ni mass of 1.2 +- 0.3 M{sub sun} for the no host extinction case (and of 1.6 +- 0.4 M{sub sun} for the host extinction of A{sub V} = 0.29 mag). The C II lambda6580 absorption line remains visible until a week after the maximum brightness, in contrast to its early disappearance in SN 2006gz. The line velocity of Si II lambda6355 is about 8000 km s{sup -1} around the maximum, being considerably slower than that of SN 2006gz. The velocity of the C II line is similar to or slightly less than that of the Si II line around the maximum. The presence of the carbon line suggests that the thick unburned C+O layer remains after the explosion. Spectropolarimetric observations by Tanaka et al. indicate that the explosion is nearly spherical. These observational facts suggest that SN 2009dc is a super-Chandrasekhar mass SN Ia.

Yamanaka, M.; Arai, A.; Chiyonobu, S.; Fukazawa, Y.; Ikejiri, Y.; Itoh, R.; Komatsu, T.; Miyamoto, H. [Department of Physical Science, Hiroshima University, Kagamiyama 1-3-1, Higashi-Hiroshima 739-8526 (Japan); Kawabata, K. S. [Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Kinugasa, K.; Hashimoto, O.; Honda, S. [Gunma Astronomical Observatory, Takayama, Gunma 377-0702 (Japan); Tanaka, M. [Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033 (Japan); Imada, A.; Kuroda, D. [Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Kamogata, Asakuchi-shi, Okayama 719-0232 (Japan); Maeda, K.; Nomoto, K. [Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa (Japan); Kamata, Y. [National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588 (Japan); Kawai, N. [Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan); Konishi, K., E-mail: myamanaka@hiroshima-u.ac.j [Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa, Chiba, 277-8582 (Japan)

2009-12-20T23:59:59.000Z

163

Millersville University  

E-Print Network (OSTI)

Violence Weapons Theft Use of University Equipment Section VII COMMUNICATIONS Guidelines for placing VIII EMPLOYEE SAFETY AND HEALTH Campus Emergency Procedures Threat Assessment Team Suspicious Leave Annual Leave #12; Section IX ATTENDANCE AND LEAVE continued Personal Leave Sick Leave Sick

Hardy, Christopher R.

164

Symbiotic stars as possible progenitors of SNe Ia: binary parameters and overall outlook  

E-Print Network (OSTI)

Symbiotic stars are interacting binaries in which the first-formed white dwarf accretes and burns material from a red giant companion. This paper aims at presenting physical characteristics of these objects and discussing their possible link with progenitors of type Ia supernovae.

Miko?ajewska, J

2011-01-01T23:59:59.000Z

165

g-MODE EXCITATION DURING THE PRE-EXPLOSIVE SIMMERING OF TYPE Ia SUPERNOVAE  

SciTech Connect

Prior to the explosive burning of a white dwarf (WD) that makes a Type Ia supernova (SN Ia), the star 'simmers' for {approx}10{sup 3} yr in a convecting, carbon-burning region. I estimate the excitation of g-modes by convection during this phase and explore their possible effect on the WD. As these modes propagate from the core of the WD toward its surface, their amplitudes grow with decreasing density. Once the modes reach nonlinear amplitudes, they break and deposit their energy into a shell of mass {approx}10{sup -4} M{sub sun}. This raises the surface temperature by {approx}4 x 10{sup 8} K, which is sufficient to ignite a layer of helium, as is expected to exist for some SN Ia scenarios. This predominantly synthesizes {sup 40}Ca, but some amount of {sup 28}Si, {sup 32}S, and {sup 44}Ti may also be present. These ashes are expanded out with the subsequent explosion up to velocities of {approx}20, 000 km s{sup -1}, which may explain the high velocity features (HVFs) seen in many SNe Ia. The appearance of HVFs would therefore be a useful discriminant for determining between progenitors, since a flammable helium-rich layer will not be present for accretion from a C/O WD as in a merger scenario. I also discuss the implications of {sup 44}Ti production.

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

2011-09-01T23:59:59.000Z

166

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 structure which, de- pending on density, may involve separate regions of carbon, oxygen and silicon burning, all propagating in a self-similar, subsonic front. The separation between these three burning regions

167

A Test for the Nature of the Type Ia Supernova Explosion Mechanism  

E-Print Network (OSTI)

Currently popular models for Type Ia supernovae (SNe Ia) fall into two general classes. The first comprises explosions of nearly pure carbon/oxygen (C/O) white dwarfs at the Chandrasekhar limit which ignite near their centers. The second consists of lower-mass C/O cores which are ignited by the detonation of an accreted surface helium layer. Explosions of the latter type produce copious Fe, Co and Ni K-alpha emission from 56Ni and 56Co decay in the detonated surface layers, emission which is much weaker from Chandrasekhar-mass models. The presence of this emission provides a simple and unambiguous discriminant between these two models for SNe Ia. Both mechanisms may produce 0.1-0.6 solar masses of 56Ni, making them bright gamma-ray line emitters. The time to maximum brightness of 56Ni decay lines is distinctly shorter in the sub-Chandrasekhar mass class of model (approximately 15 days) than in the Chandrasekhar mass model (approximately 30 days), making gamma-ray line evolution another direct test of the explosion mechanism. It should just be possible to detect K-shell emission from a sub-Chandrasekhar explosion from SNe Ia as far away as the Virgo cluster with the XMM Observatory. A 1 to 2 square meter X-ray telescope such as the proposed Con-X Observatory could observe K-alpha emission from sub-Chandrasekhar mass SNe Ia in the Virgo cluster, providing not just a detection, but high-accuracy flux and kinematic information.

Philip A. Pinto; Ronald G. Eastman; Tamara Rogers

2000-08-21T23:59:59.000Z

168

WHITE DWARF/M DWARF BINARIES AS SINGLE DEGENERATE PROGENITORS OF TYPE Ia SUPERNOVAE  

SciTech Connect

Limits on the companions of white dwarfs in the single-degenerate scenario for the origin of Type Ia supernovae (SNe Ia) have gotten increasingly tight, yet igniting a nearly Chandrasekhar mass C/O white dwarf from a condition of near hydrostatic equilibrium provides compelling agreement with observed spectral evolution. The only type of non-degenerate stars that survive the tight limits, M{sub V} {approx}> 8.4 on the SN Ia in SNR 0509-67.5 and M{sub V} {approx}> 9.5 in the remnant of SN 1572, are M dwarfs. While M dwarfs are observed in cataclysmic variables, they have special properties that have not been considered in most work on the progenitors of SNe Ia: they have small but finite magnetic fields and they flare frequently. These properties are explored in the context of SN Ia progenitors. White dwarf/M dwarf pairs may be sufficiently plentiful to provide, in principle, an adequate rate of explosions even with slow orbital evolution due to magnetic braking or gravitational radiation. Even modest magnetic fields on the white dwarf and M dwarf will yield adequate torques to lock the two stars together, resulting in a slowly rotating white dwarf, with the magnetic poles pointing at one another in the orbital plane. The mass loss will be channeled by a 'magnetic bottle' connecting the two stars, landing on a concentrated polar area on the white dwarf. This enhances the effective rate of accretion compared to spherical accretion. Luminosity from accretion and hydrogen burning on the surface of the white dwarf may induce self-excited mass transfer. The combined effects of self-excited mass loss, polar accretion, and magnetic inhibition of mixing of accretion layers give possible means to beat the 'nova limit' and grow the white dwarf to the Chandrasekhar mass even at rather moderate mass accretion rates.

Wheeler, J. Craig, E-mail: wheel@astro.as.utexas.edu [Department of Astronomy, University of Texas at Austin, Austin, TX 78712 (United States)

2012-10-20T23:59:59.000Z

169

Noname manuscript No. (will be inserted by the editor)  

E-Print Network (OSTI)

-mail:akshayd@iastate.edu S. Tirthapura Department of Electrical and Computer Engineering, Iowa State University, Ames, IA diseases [74], political science [20], and historical linguistics [34]. Here we consider the problem.g., horizontal gene transfer, gene duplication, convergent evolution, and varying evolutionary rates) [67]. Here

Sanderson, Michael J.

170

Edible Applications Technology Division List  

Science Conference Proceedings (OSTI)

Name AffiliationCity, State, CountryEdible Applications Technology Division2013 Members362 Members as of October 1, 2013Acevedo, NuriaUniversity of GuelphAmes, IA, USAAdam, RoyOilseeds International LtdSan Francisco, CA, USAAdriaenssens, MarkBarry Callebau

171

Food Safety & Functionality Forum Division List  

Science Conference Proceedings (OSTI)

Name AffiliationCity, State, CountryFood Structure & Functionality Forum Division2013 Members116 Members as of July 1, 2013Acevedo, NuriaUniversity of GuelphAmes, IA, USAAdriaenssens, MarkBarry CallebautPennsauken, NJ, USAAimutis, WilliamCargill IncWayzata

172

Complex Hydrides - A New Frontier for Future Energy Applications - DOE Hydrogen and Fuel Cells Program FY 2012 Annual Progress Report  

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

5 5 FY 2012 Annual Progress Report DOE Hydrogen and Fuel Cells Program Vitalij K. Pecharsky, 1 Marek Pruski, 2 L. Scott Chumbley, 3 Duane D. Johnson, 4 Takeshi Kobayashi 5 1 FWP Leader: Ames Laboratory, 253 Spedding Hall, Ames, IA 50011, Email: vitkp@ameslab.gov, Phone: (515) 294-8220 2 PI: Ames Laboratory, 230 Spedding Hall, Ames, IA 50011, Email: mpruski@iastate.edu, Phone: (515) 294-2017 3 PI: Ames Laboratory, 214 Wilhelm Hall, Ames, IA 50011, Email: chumbley@iastate.edu, Tel.: 515-2947903; 4 PI: Ames Laboratory, 311 TASF, Ames, IA 50011, Email: ddj@ameslab.gov, Phone: (515) 2949649 5 Ames Laboratory, 229 Spedding Hall, Ames, IA 50011, Email: takeshi@iastate.edu, Phone: (515)-294-6823 DOE Program Officer: Dr. Refik Kortan

173

UNIVERSITY OF MINNESOTA University Services  

E-Print Network (OSTI)

Church Street SE Minneapolis, MN 55455-0110 Office: 612-624-3557 Fax: 612-626-6278 www.uservices.umn.edu MEMORANDUM January 29, 2010 TO: Executive Team, Twin Cities Deans, Faculty Researchers FROM: Kathleen O'Brien, Vice President Subject: Status Report on the University of Minnesota and the Central Corridor Light

Amin, S. Massoud

174

NC STATE UNIVERSITY UNIVERSITY HOUSING  

E-Print Network (OSTI)

name to enter it on your application. Only current and accepted students will appear in the search box of the application process 1 #12;NC STATE UNIVERSITY SELECT THE FALL 2012 TERM 2 Once accepted by NC State, students accepting the terms and conditions associated with the Agreement. ELECTRONIC SIGNATURE #12;NC STATE

175

On October 15, 2010, the University of Memphis Center for Information Assurance (CfIA) hosted the 3rd  

E-Print Network (OSTI)

digital devices, and we encourage you to read the excellent summary from the National Counter-Intelligence for an unspecified period of time. This policy applies to anyone entering the country, including US citizens

Memphis, University of

176

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

177

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

178

Constraining the spin-down timescale of the white-dwarf progenitors of Type Ia supernovae  

E-Print Network (OSTI)

Justham (2011) and DiStefano et al.\\ (2011) proposed that the white-dwarf progenitor of a Type Ia supernova (SN Ia) may have to spin down before it can explode. As the white dwarf spin-down timescale is not well known theoretically, we here try to constrain it empirically (within the framework of this spin-down model) for progenitor systems that contain a giant donor and for which circumbinary material has been detected after the explosion: we obtain an upper limit of a few $10^{\\rm 7} {\\rm yr}$. Based on the study of Di Stefano & Kilic (2012) this means that it is too early to rule out the existence of a surviving companion in SNR 0509-67.5.

Meng, Xiangcun

2013-01-01T23:59:59.000Z

179

THE FLORIDA STATE UNIVERSITY UNIVERSITY HEALTH SERVICES  

E-Print Network (OSTI)

THE FLORIDA STATE UNIVERSITY UNIVERSITY HEALTH SERVICES HEALTH & WELLNESS CENTER University Health-8958 Healthcare Compliance Information Florida State University's University Health Services (UHS) is staffed service laboratory; pickup service is available for students whose insurance requires the use of Lab Corps

Weston, Ken

180

Integral Airframe Structures (IAS)---Validated Feasibility Study of Integrally Stiffened Metallic Fuselage Panels for Reducing Manufacturing Costs  

Science Conference Proceedings (OSTI)

The Integral Airframe Structures (IAS) program investigated the feasibility of using "integrally stiffened" construction for commercial transport fuselage structure. The objective of the program was to demonstrate structural performance and weight equal ...

Munroe J.; Wilkins K.; Gruber M.

2000-05-01T23:59:59.000Z

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181

In vivo cofactor biosynthesis and maintenance in the class Ia ribonucleotide reductase small subunit of Escherichia coli  

E-Print Network (OSTI)

The small subunit ([beta]2) of Escherichia coli class Ia ribonucleotide reductases (RNRs) contains a diferric tyrosyl radical (Y*) cofactor essential for the conversion of nucleotides to deoxynucleotides that are needed ...

Wu, Chia-Hung, Ph. D. Massachusetts Institute of Technology

2009-01-01T23:59:59.000Z

182

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

183

SELF-SHIELDING OF SOFT X-RAYS IN TYPE Ia SUPERNOVA PROGENITORS  

SciTech Connect

There are insufficient super-soft ({approx}0.1 keV) X-ray sources in either spiral or elliptical galaxies to account for the rate of explosion of Type Ia supernovae (SNe Ia) in either the single-degenerate or the double-degenerate scenarios. We quantify the amount of circumstellar matter that would be required to suppress the soft X-ray flux by yielding a column density in excess of 10{sup 23} cm{sup -2}. We summarize evidence that appropriate quantities of matter are extant in SNe Ia and in recurrent novae that may be supernova precursors. The obscuring matter is likely to have a large, but not complete, covering factor and to be substantially non-spherically symmetric. Assuming that much of the absorbed X-ray flux is re-radiated as blackbody radiation in the UV, we estimate that {approx}<100 sources might be detectable in the Galaxy Evolution Explorer All-sky Survey.

Wheeler, J. Craig [Department of Astronomy, University of Texas at Austin, Austin, TX (United States)] [Department of Astronomy, University of Texas at Austin, Austin, TX (United States); Pooley, D., E-mail: wheel@astro.as.utexas.edu [Department of Physics, Sam Houston State University, Huntsville, TX (United States)

2013-01-10T23:59:59.000Z

184

The Cellular Burning Regime in Type Ia Supernova Explosions - I. Flame Propagation into Quiescent Fuel  

E-Print Network (OSTI)

We present a numerical investigation of the cellular burning regime in Type Ia supernova explosions. This regime holds at small scales (i.e. below the Gibson scale), which are unresolved in large-scale Type Ia supernova simulations. The fundamental effects that dominate the flame evolution here are the Landau-Darrieus instability and its nonlinear stabilization, leading to a stabilization of the flame in a cellular shape. The flame propagation into quiescent fuel is investigated addressing the dependence of the simulation results on the specific parameters of the numerical setup. Furthermore, we investigate the flame stability at a range of fuel densities. This is directly connected to the questions of active turbulent combustion (a mechanism of flame destabilization and subsequent self-turbulization) and a deflagration-to-detonation transition of the flame. In our simulations we find no substantial destabilization of the flame when propagating into quiescent fuels of densities down to ~10^7 g/cm^3, corroborating fundamental assumptions of large-scale SN Ia explosion models. For these models, however, we suggest an increased lower cutoff for the flame propagation velocity to take the cellular burning regime into account.

F. K. Roepke; W. Hillebrandt; J. C. Niemeyer

2003-12-03T23:59:59.000Z

185

DLMF: Chapter 19 Elliptic Integrals  

Science Conference Proceedings (OSTI)

... B. C. Carlson. Mathematics Department and Ames Laboratory (US Department of Energy), Iowa State University, Ames, Iowa. ...

2013-05-03T23:59:59.000Z

186

Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z \\lesssim 0.3, of which 270 (52%) are spectroscopically identified as SNe Ia. The remaining 246 SNe Ia were identified through their light curves; 113 of these objects have spectroscopic redshifts from spectra of their host galaxy, and 133 have photometric redshifts estimated from the SN light curves. Based on consideration of 87 spectroscopically confirmed non-Ia SNe discovered by the SDSS-II SN Survey, we estimate that 2.04+1.61-0.95 % of the photometric SNe Ia may be misidentified. The sample of SNe Ia used in this measurement represents an order of magnitude increase in the statistics for SN Ia rate measurements in the redshift range covered by the SDSS-II Supernova Survey. If we assume a SN Ia rate that is constant at low redshift (z < 0.15), then the SN observations can be used t...

Dilday, Benjamin; Bassett, Bruce; Becker, Andrew; Bender, Ralf; Castander, Francisco; Cinabro, David; Filippenko, Alexei V; Frieman, Joshua A; Galbany, Lluis; Garnavich, Peter M; Goobar, Ariel; Hopp, Ulrich; Ihara, Yutaka; Jha, Saurabh W; Kessler, Richard; Lampeitl, Hubert; Marriner, John; Miquel, Ramon; Molla, Mercedes; Nichol, Robert C; Nordin, Jakob; Riess, Adam G; Sako, Masao; Schneider, Donald P; Sollerman, Jesper; Wheeler, J Craig; Ostman, Linda; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Pan, Kaike; Simmons, Audrey; Snedden, Stephanie

2010-01-01T23:59:59.000Z

187

AME 514 -Applications of Combustion -Spring 2013 Homework #3 Due Friday 4/5/13, 4:30 pm in the drop box in OHE 430N (Xerox room). If you're off  

E-Print Network (OSTI)

AME 514 - Applications of Combustion - Spring 2013 ­ Homework #3 Due Friday 4/5/13, 4:30 pm · Joulin, G., Sivashinsky, G. I. (1994). Combust. Sci. Technol. 98, 11-23. Theoretical description of flames in Hele-Shaw cells. · Yoshida, A. (1988). Proc. Combust. Inst. 22, 1471-1478. Very good

188

On the hydrogen emission from the type Ia supernova 2002ic  

DOE Green Energy (OSTI)

The discovery of SN 2002ic by the Supernova Factory and the subsequent spectroscopic studies have led to the surprising finding that SN 2002ic is a type Ia supernova with strong ejecta-circumstellar interaction. Here we show that nearly 1 year after the explosion the supernova has become fainter overall, but the H-alpha emission has brightened and broadened dramatically compared to earlier observations. We have obtained spectropolarimetry data which show that the hydrogen-rich matter is highly aspherically distributed. These observations suggest that the supernova exploded inside a dense, clumpy, disk-like circumstellar environment.

Wang, Lifan; Baade, Dietrich; Hoflich, Peter; Wheeler, J. Craig; Kawabata, Koji; Nomoto, Ken'ichi

2003-12-10T23:59:59.000Z

189

Uncertainty Quantification Tools for Multiphase Flow Simulations using MFIX  

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

Uncertainty Uncertainty Quantification Tools for Multiphase Flow Simulations using MFIX X. Hu 1 , A. Passalacqua 2 , R. O. Fox 1 1 Iowa State University, Department of Chemical and Biological Engineering, Ames, IA 2 Iowa State University, Department of Mechanical Engineering, Ames, IA Project Manager: Steve Seachman University Coal Research and Historically Black Colleges and Universities and Other Minority Institutions Contractors Review Conference Pittsburgh, June 11 th - 13 th 2013 X. Hu, A. Passalacqua, R. O. Fox (ISU) Uncertainty quantification DOE-UCR Review Meeting 2013 1 / 44 Outline 1 Introduction and background 2 Project objectives and milestones 3 Technical progress Univariate case Multivariate case Code structure 4 Future work X. Hu, A. Passalacqua, R. O. Fox (ISU) Uncertainty quantification DOE-UCR Review Meeting 2013 2 / 44 Introduction and background Outline 1 Introduction

190

Agricultural Mitigation of Greenhouse Gases: Science and Policy Options  

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

Agricultural Mitigation of Greenhouse Gases: Science and Policy Options Agricultural Mitigation of Greenhouse Gases: Science and Policy Options Keith Paustian (keithp@nrel.colostate.edu; 970-491-1547) Natural Resource Ecology Laboratory Colorado State University Ft. Collins, CO 80523 Bruce Babcock (babcock@iastate.edu; 515-294-6785) Cathy Kling (ckling@iastate.edu; 515-294-5767) Center for Agriculture and Rural Development Iowa State University Ames, IA 50011-1070 Jerry Hatfield (hatfield@nstl.gov; 515-294-5723) USDA - National Soil Tilth Laboratory Ames, IA 50011 Rattan Lal (lal.1@osu.edu; 614-292-9069) School of Natural Resources The Ohio State University Columbus, OH 43210-1085 Bruce McCarl (mccarl@tamu.edu; 979-845-1706) Department of Agricultural Economics Texas A&M University College Station, TX 77843-2124 Sandy McLaughlin (un4@ornl.gov; 865-574-7358)

191

Finsler geometric perspective on the bulk flow in the universe  

E-Print Network (OSTI)

Astronomical observations showed that there may exist a bulk flow with peculiar velocities in the universe, which contradicts with the (\\Lambda)CDM model. The bulk flow reveals that the observational universe is anisotropic at large scales. In fact, a more reliable observation on the anisotropy of spacetime comes from the CMB power spectra. The WMAP and Planck satellites both show that there is a hemispherical power asymmetry at large-angular scales. In this paper, we propose a "wind" scenario to the bulk flow (or the anisotropy of spacetime). Under the influence of the "wind", the spacetime metric could become a Finsler structure. By resolving the null geodesic equation, we obtain the modified luminosity distance, which has a dipolar form at the leading order. Thus, the "wind" describes well the bulk flow. In addition, we perform a least-(\\chi^2) fit to the data of type Ia supernovae (SNe Ia) in the Union2.1 compilation. The peculiar velocity of the bulk flow has an upper limit (v_{bulk}\\lesssim 4000 \\rm{km/s}), which is compatible with all the existing observational values.

Zhe Chang; Ming-Hua Li; Sai Wang

2013-03-07T23:59:59.000Z

192

Photometric Observations of the Type Ia SN 2002er in UGC 10743  

E-Print Network (OSTI)

Extensive light and colour curves for the Type Ia supernova SN 2002er are presented as part of the European Supernova Collaboration. We have collected UBVRI photometry from ten different telescopes covering the phases from 7 days before until 619 days after maximum light. Corrections for the different instrumental systems and the non-thermal spectrum of the supernova (S-corrections) have been applied. With the densely sampled light curves we can make detailed comparisons to other well-observed objects. SN 2002er most closely resembles SN 1996X after maximum, but clearly shows a different colour evolution before peak light and a stronger shoulder in V and R bands compared to other well-observed SNe Ia. In particular, the rise time appears to be longer than what is expected from rise-time vs.decline-rate relation. We use several methods to determine the reddening towards SN 2002er based on the colour evolution at near peak and at late phases. The uvoir (bolometric) light curve shows great similarity with SN 199...

Pignata, G; Benetti, S; Blinnikov, S; Hillebrandt, W; Kotak, R; Leibundgut, B; Mazzali, P A; Meikle, P; Qiu, Y; Ruiz-Lapuente, P; Smartt, S; Sorokina, E; Stritzinger, M; Stehle, M; Turatto, M; Marsh, T; Martin-Luis, F; McBride, N; Mndez, J; Morales-Rueda, L; Narbutis, D; Street, R

2004-01-01T23:59:59.000Z

193

The Cellular Burning Regime in Type Ia Supernova Explosions - II. Flame Propagation into Vortical Fuel  

E-Print Network (OSTI)

We investigate the interaction of thermonuclear flames in Type Ia supernova explosions with vortical flows by means of numerical simulations. In our study, we focus on small scales, where the flame propagation is no longer dominated by the turbulent cascade originating from large-scale effects. Here, the flame propagation proceeds in the cellular burning regime, resulting from a balance between the Landau-Darrieus instability and its nonlinear stabilization. The interaction of a cellularly stabilized flame front with a vortical fuel flow is explored applying a variety of fuel densities and strengths of the velocity fluctuations. We find that the vortical flow can break up the cellular flame structure if it is sufficiently strong. In this case the flame structure adapts to the imprinted flow field. The transition from the cellularly stabilized front to the flame structure dominated by vortices of the flow proceeds in a smooth way. The implications of the results of our simulations for Type Ia Supernova explosion models are discussed.

F. K. Roepke; W. Hillebrandt; J. C. Niemeyer

2003-12-08T23:59:59.000Z

194

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

195

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

196

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

197

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

198

Math in Architecture - CECM - Simon Fraser University  

E-Print Network (OSTI)

The Parthenon, Athens, Greece. 4. Page 5. Santa Maria Novella, Florence, Italy. 5. Page 6. A Church, Ia, Santorini Island, Greece. 6...

199

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

Science Conference Proceedings (OSTI)

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

200

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

Note: This page contains sample records for the topic "university ames ia" from the National Library of EnergyBeta (NLEBeta).
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to obtain the most current and comprehensive results.


201

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

202

Analysis of Reaction-Diffusion Systems for Flame Capturing in Type Ia Supernova Simulations  

E-Print Network (OSTI)

We present a study of numerical behavior of a thickened flame used in Flame Capturing (FC, Khokhlov (1995)) for tracking thin unresolved physical flames in deflagration simulations. We develop a steady-state procedure for calibrating the flame model used, and test it against analytical results. We observe numerical noises generated by original realization of the technique. Alternative artificial burning rates are discussed, which produce acceptably quiet flames. Two new quiet models are calibrated to yield required "flame" speed and width, and further studied in 2D and 3D setting. Landau-Darrieus type instabilities of the flames are observed. One model also shows significantly anisotropic propagation speed on the grid, both effects increasingly pronounced at larger matter expansion as a result of burning; this makes the model unacceptable for use in type Ia supernova simulations. Another model looks promising for use in flame capturing at fuel to ash density ratio of order 3 and below. That "Model B" yields f...

Zhiglo, Andrey V

2009-01-01T23:59:59.000Z

203

ASD(NII)/DoD CIO SUBJECT: Defense Industrial Base (DIB) Cyber Security/Information Assurance (CS/IA) Activities  

E-Print Network (OSTI)

directing the conduct of DIB CS/IA activities to protect unclassified DoD information, as defined in the Glossary, that transits or resides on unclassified DIB information systems and networks. 2. APPLICABILITY. This Instruction applies to OSD, the Military Departments, the Office of

unknown authors

2010-01-01T23:59:59.000Z

204

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

205

Photometric Observations of the Type Ia SN 2002er in UGC 10743  

E-Print Network (OSTI)

Extensive light and colour curves for the Type Ia supernova SN 2002er are presented as part of the European Supernova Collaboration. We have collected UBVRI photometry from ten different telescopes covering the phases from 7 days before until 619 days after maximum light. Corrections for the different instrumental systems and the non-thermal spectrum of the supernova (S-corrections) have been applied. With the densely sampled light curves we can make detailed comparisons to other well-observed objects. SN 2002er most closely resembles SN 1996X after maximum, but clearly shows a different colour evolution before peak light and a stronger shoulder in V and R bands compared to other well-observed SNe Ia. In particular, the rise time appears to be longer than what is expected from rise-time vs.decline-rate relation. We use several methods to determine the reddening towards SN 2002er based on the colour evolution at near peak and at late phases. The uvoir (bolometric) light curve shows great similarity with SN 1996X, but also indications of a higher luminosity, longer rise time and a more pronounced shoulder 25 days past maximum. The interpretation of the light curves was done with two independent light curve codes. Both find that given the luminosity of SN 2002er the 56Ni mass exceeds 0.6 Msun with prefered values near 0.7 Msun. Uncertainties in the exact distance to SN 2002er are the most serious limitation of this measurement. The light curve modelling also indicates a high level of mixing of the nickel in the explosion of SN 2002er.

G. Pignata; F. Patat; S. Benetti; S. Blinnikov; W. Hillebrandt; R. Kotak; B. Leibundgut; P. A. Mazzali; P. Meikle; Y. Qiu; P. Ruiz-Lapuente; S. Smartt; E. Sorokina; M. Stritzinger; M. Stehle; M. Turatto; T. Marsh; F. Martin-Luis; N. McBride; J. Mendez; L. Morales-Rueda; D. Narbutis; R. Street

2004-08-12T23:59:59.000Z

206

Direct Analysis of Spectra of the Peculiar Type Ia Supernova 2000cx  

E-Print Network (OSTI)

The Type Ia SN 2000cx exhibited multiple peculiarities, including a lopsided B-band light-curve peak that does not conform to current methods for using shapes of light curves to standardize SN Ia luminosities. We use the parameterized supernova synthetic-spectrum code SYNOW to study line identifications in the photospheric-phase spectra of SN 2000cx. Previous work established the presence of Ca II infrared-triplet features forming above velocity about 20,000 km/s, much higher than the photospheric velocity of about 10,000 km/s. We find Ti II features forming at the same high velocity. High-velocity line formation is partly responsible for the photometric peculiarities of SN 2000cx: for example, B-band flux blocking by Ti II absorption features that decreases with time causes the B light curve to rise more rapidly and decline more slowly than it otherwise would. SN 2000cx contains an absorption feature near 4530 A that may be H-beta, forming at the same high velocity. The lack of conspicuous H-alpha and P-alpha signatures does not necessarily invalidate the H-beta identification if the high-velocity line formation is confined to a clump that partly covers the photosphere and the H-alpha and P-alpha source functions are elevated relative to that of resonance scattering. The H-beta identification is tentative. If it is correct, the high-velocity matter must have come from a nondegenerate companion star.

D. Branch; R. C. Thomas; E. Baron; D. Kasen; K. Hatano; K. Nomoto; A. V. Filippenko; W. Li; R. J. Rudy

2004-01-15T23:59:59.000Z

207

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

208

The Universe Adventure - The Modern Universe  

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

Modern Universe Modern Universe Like astronomers throughout history, modern cosmologists are interested in making an accurate model of the Universe. Starting with the laws of physics which explain how fundamental particles and forces interact, physicists derive general equations describing the evolution of the Universe's structure. Cosmologists use experimental evidence to select a set of initial conditions enabling them to solve the general equations, and calculate the state of the Universe at times in the past, present, or future. This generates a possible model, which can be tested by comparing the phenomena it predicts with observational data. In this manner, following the rigorous scientific method, cosmologists work to build a successful Universal model. In the next section we will examine evidence for the current Big Bang

209

New Eyes on the Expanding Universe: The SuperNova/Acceleration Probe (SNAP)  

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

New Eyes on the Expanding Universe: The SuperNova/Acceleration Probe (SNAP) New Eyes on the Expanding Universe: The SuperNova/Acceleration Probe (SNAP) The Equation of the Universe PowerPoint Presentation The Cosmological Constant Slide 5 Hubble's Great Discovery - and Einstein's "biggest blunder" Slide 7 Slide 8 Slide 9 Slide 10 Slide 11 Slide 12 Slide 13 Slide 14 A Revolution in Cosmology Slide 16 Who Ordered That?! What we don't know Slide 19 Slide 20 Slide 21 Dark Energy Task Force Slide 23 Slide 24 Slide 25 Slide 26 Slide 27 "Standard-izable" Candles Slide 29 Slide 30 Slide 31 Slide 32 Slide 33 Slide 34 Slide 35 Slide 36 Slide 37 Slide 38 Slide 39 What is the Physical Mechanism for Type Ia SNe? Discovering Supernovae Slide 42 The Expansion History of the Universe Discovering Supernovae from Space Gravitational Weak Lensing Slide 46 Slide 47

210

Measurements of the Rate of Type Ia Supernovae at Redshift z < ~0.3 from the SDSS-II Supernova Survey  

Science Conference Proceedings (OSTI)

We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z {approx}< 0.3, of which 270 (52%) are spectroscopically identified as SNe Ia. The remaining 246 SNe Ia were identified through their light curves; 113 of these objects have spectroscopic redshifts from spectra of their host galaxy, and 133 have photometric redshifts estimated from the SN light curves. Based on consideration of 87 spectroscopically confirmed non-Ia SNe discovered by the SDSS-II SN Survey, we estimate that 2.04{sub -0.95}{sup +1.61}% of the photometric SNe Ia may be misidentified. The sample of SNe Ia used in this measurement represents an order of magnitude increase in the statistics for SN Ia rate measurements in the redshift range covered by the SDSS-II Supernova Survey. If we assume a SN Ia rate that is constant at low redshift (z < 0.15), then the SN observations can be used to infer a value of the SN rate of r{sub V} = (2.69{sub -0.30-0.01}{sup +0.34+0.21}) x 10{sup -5} SNe yr{sup -1} Mpc{sup -3} (H{sub 0}/(70 km s{sup -1} Mpc{sup -1})){sup 3} at a mean redshift of {approx} 0.12, based on 79 SNe Ia of which 72 are spectroscopically confirmed. However, the large sample of SNe Ia included in this study allows us to place constraints on the redshift dependence of the SN Ia rate based on the SDSS-II Supernova Survey data alone. Fitting a power-law model of the SN rate evolution, r{sub V} (z) = A{sub p} x ((1+z)/(1+z{sub 0})){sup {nu}}, over the redshift range 0.0 < z < 0.3 with z{sub 0} = 0.21, results in A{sub p} = (3.43{sub -0.15}{sup +0.15}) x 10{sup -5} SNe yr{sup -1} Mpc{sup -3} (H{sub 0}/(70 km s{sup -1} Mpc{sup -1})){sup 3} and {nu} = 2.04{sub -0.89}{sup +0.90}.

Dilday, Benjamin; /Rutgers U., Piscataway /Chicago U. /KICP, Chicago; Smith, Mathew; /Cape Town U., Dept. Math. /Portsmouth U.; Bassett, Bruce; /Cape Town U., Dept. Math. /South African Astron. Observ.; Becker, Andrew; /Washington U., Seattle, Astron. Dept.; Bender, Ralf; /Munich, Tech. U. /Munich U. Observ.; Castander, Francisco; /Barcelona, IEEC; Cinabro, David; /Wayne State U.; Filippenko, Alexei V.; /UC, Berkeley; Frieman, Joshua A.; /Chicago U. /Fermilab; Galbany, Lluis; /Barcelona, IFAE; Garnavich, Peter M.; /Notre Dame U. /Stockholm U., OKC /Stockholm U.

2010-01-01T23:59:59.000Z

211

Fudan University HSK level 6  

E-Print Network (OSTI)

of King Mongkut's University of Technology Thonburi 0 Australian National University Plasma Research

Takada, Shoji

212

The Universe Adventure - Expansion  

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

Expansion: Chunk-by-Chunk Expansion: Chunk-by-Chunk A sample of the Universe. A very small portion of the Universe. In order to better understand the significance of expansion, let's look at a cubic sample of space. By considering a finite volume we can follow changes in the size of the Universe as we move forwards and backwards in time. Remember, only the size of the cube will change. The galaxies inside the cube stay the same size. This animation illustrates how our cubic piece of the Universe changes with time. If the Universe followed the simplest expansionary models, its size would increase linearly with time. The Universe would continue to expand at a constant rate forever. If you look at only a narrow time-slice of the Universe's history, it does, in fact, appear that this is how the Universe

213

The Universe Adventure - Credits  

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

School) GraphicWeb Design Melissa McClure (student, University of Rochester) Jonathan Thai (student, UC Irvine) 2005 Summer (Universe Adventure rev 2.0) Lead Content guided by...

214

Joint Outreach Task Group (JOTG) Calendar: September  

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

FWP Event K-25 Oak Ridge, TN 6 7 8 9 10 11 12 Local Event X-10 Oak Ridge, TN 13 FWP Event Ames Laboratory Ames, IA 14 15 16 17 JOTG Event, Livermore, CA JOTG Event, Emeryville, CA...

215

Nevada University Transportation  

E-Print Network (OSTI)

illnesses and disabilities · Development of professionals and future leaders in the area of transportationNUTC Nevada University Transportation Center University of Nevada, Las Vegas Sustainable Transporation in Arid Regions 2007-2009 Biennial Report 5 #12;2007-2009 Nevada University Transportation Center

Ahmad, Sajjad

216

Distant Supernovae and the Accelerating Universe  

E-Print Network (OSTI)

The observation of SN 1997ff at redshift 1.7 has been claimed to refute alternative models such as grey dust or evolution for the faintness of distant supernovae, leaving only an accelerating Universe as a viable model. However, a very simple one parameter evolution model, with the peak luminosity varying as an exponential function of cosmic time, converts the flux vs. distance law of the critical density matter-dominated model into that of the concordance Omega_matter = 0.3 flat vacuum-dominated model with an error no larger than 0.03 mag over the range 0-2 in redshift. A grey dust model that matches this accuracy can easily be contrived but it still fails by overproducing the far-IR background or distorting the CMB. Models that involve oscillation between photons and axions could emulate an exponential function of cosmic time without violating these background constraints. Clearly a better and well-tested understanding of the Type Ia supernova explosion mechanism and the origin of the correlation between the decay rate and luminosity is needed before any effort to reduce statistical errors in the supernova Hubble diagram to very small levels.

E. L. Wright

2002-01-12T23:59:59.000Z

217

Constraints on SN Ia progenitor time delays from high-z SNe and the star formation history  

E-Print Network (OSTI)

We re-assess the question of a systematic time delay between the formation of the progenitor and its explosion in a type Ia supernova (SN Ia) using the Hubble Higher-z Supernova Search sample (Strolger et al. 2004). While the previous analysis indicated a significant time delay, with a most likely value of 3.4 Gyr, effectively ruling out all previously proposed progenitor models, our analysis shows that the time-delay estimate is dominated by systematic errors, in particular due to uncertainties in the star-formation history. We find that none of the popular progenitor models under consideration can be ruled out with any significant degree of confidence. The inferred time delay is mainly determined by the peak in the assumed star-formation history. We show that, even with a much larger Supernova sample, the time delay distribution cannot be reliably reconstructed without better constraints on the star-formation history.

F. Frster; C. Wolf; Ph. Podsiadlowski; Z. Han

2006-01-19T23:59:59.000Z

218

A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey  

Science Conference Proceedings (OSTI)

We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at z {le} 0.17 and 27 SN events in 492 maxBCG clusters at 0.1 {le} z {le} 0.3. We find values for the cluster SN Ia rate of (0.37{sub -0.12-0.01}{sup +0.17+0.01}) SNur h{sup 2} and (0.55{sub -0.11-0.01}{sup +0.13+0.02}) SNur h{sup 2} (SNux = 10{sup -12}L{sub x{circle_dot}}{sup -1} yr{sup -1}) in C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be (0.31{sub -0.12-0.01}{sup +0.18+0.01}) SNur h{sup 2} and (0.49{sub -0.11-0.01}{sup +0.15+0.02}) SNur h{sup 2} in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be (2.04{sub -1.11-0.04}{sup +1.99+0.07}) SNur h{sup 2} and (0.36{sub -0.30-0.01}{sup +0.84+0.01}) SNur h{sup 2} in C4 and maxBCG clusters, respectively. The ratio of the SN Ia rate in cluster early-type galaxies to that of the SN Ia rate in field early-type galaxies is 1.94{sub -0.91-0.015}{sup +1.31+0.043} and 3.02{sub -1.03-0.048}{sup +1.31+0.062}, for C4 and maxBCG clusters, respectively. The SN rate in galaxy clusters as a function of redshift, which probes the late time SN Ia delay distribution, shows only weak dependence on redshift. Combining our current measurements with previous measurements, we fit the cluster SN Ia rate data to a linear function of redshift, and find r{sub L} = [(0.49{sub -0.14}{sup +0.15}) + (0.91{sub -0.81}{sup +0.85}) x z] SNuB h{sup 2}. A comparison of the radial distribution of SNe in cluster to field early-type galaxies shows possible evidence for an enhancement of the SN rate in the cores of cluster early-type galaxies. With an observation of at most 3 hostless, intra-cluster SNe Ia, we estimate the fraction of cluster SNe that are hostless to be (9.4{sub -5.1}{sup +8.3})%.

Dilday, Benjamin; /Rutgers U., Piscataway /Chicago U. /KICP, Chicago; Bassett, Bruce; /Cape Town U., Dept. Math. /South African Astron. Observ.; Becker, Andrew; /Washington U., Seattle, Astron. Dept.; Bender, Ralf; /Munich, Tech. U. /Munich U. Observ.; Castander, Francisco; /Barcelona, IEEC; Cinabro, David; /Wayne State U.; Frieman, Joshua A.; /Chicago U. /Fermilab; Galbany, Lluis; /Barcelona, IFAE; Garnavich, Peter; /Notre Dame U.; Goobar, Ariel; /Stockholm U., OKC /Stockholm U.; Hopp, Ulrich; /Munich, Tech. U. /Munich U. Observ. /Tokyo U.

2010-03-01T23:59:59.000Z

219

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.&

220

Prospects for Type Ia Supernova explosion mechanism identification with gamma rays  

E-Print Network (OSTI)

The explosion mechanism associated with thermonuclear supernovae (SNIa) is still a matter of debate. There is a wide agreement that high amounts of of radioactive nuclei are produced during these events and they are expected to be strong gamma-ray emitters. In the past, several authors have investigated the use of this gamma-ray emission as a diagnostic tool. In this paper we have done a complete study of the gamma-ray spectra associated with all the different scenarios currently proposed. This includes detonation, delayed detonation, deflagration and the off-center detonation. We have performed accurate simulations for this complete set of models in order to determine the most promising spectral features that could be used to discriminate among the different models. Our study is not limited to qualitative arguments. Instead, we have quantified the differences among the spectra and established distance limits for their detection. The calculations have been performed considering the best current response estimations of the SPI and IBIS instruments aboard INTEGRAL in such a way that our results can be used as a guideline to evaluate the capabilities of INTEGRAL in the study of type Ia supernovae. For the purpose of completeness we have also investigated the nuclear excitation and spallation reactions as a possible secondary source of gamma-rays present in some supernova scenarios. We conclude that this mechanism can be neglected due to its small contribution.

Jordi Gomez-Gomar; Jordi Isern; Pierre Jean

1997-09-05T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" 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

EVALUATING SYSTEMATIC DEPENDENCIES OF TYPE Ia SUPERNOVAE: THE INFLUENCE OF CENTRAL DENSITY  

SciTech Connect

We present a study exploring a systematic effect on the brightness of Type Ia supernovae using numerical models that assume the single-degenerate paradigm. Our investigation varied the central density of the progenitor white dwarf at flame ignition, and considered its impact on the explosion yield, particularly the production and distribution of radioactive {sup 56}Ni, which powers the light curve. We performed a suite of two-dimensional simulations with randomized initial conditions, allowing us to characterize the statistical trends that we present. The simulations indicate that the production of Fe-group material is statistically independent of progenitor central density, but the mass of stable Fe-group isotopes is tightly correlated with central density, with a decrease in the production of {sup 56}Ni at higher central densities. These results imply that progenitors with higher central densities produce dimmer events. We provide details of the post-explosion distribution of {sup 56}Ni in the models, including the lack of a consistent centrally located deficit of {sup 56}Ni, which may be compared to observed remnants. By performing a self-consistent extrapolation of our model yields and considering the main-sequence lifetime of the progenitor star and the elapsed time between the formation of the white dwarf and the onset of accretion, we develop a brightness-age relation that improves our prediction of the expected trend for single degenerates and we compare this relation with observations.

Krueger, Brendan K.; Jackson, Aaron P.; Calder, Alan C. [Department of Physics and Astronomy, State University of New York-Stony Brook, Stony Brook, NY (United States); Townsley, Dean M. [Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL (United States); Brown, Edward F. [Department of Physics and Astronomy, Michigan State University, East Lansing, MI (United States); Timmes, Francis X., E-mail: brendan.krueger@stonybrook.edu [Joint Institute for Nuclear Astrophysics, Notre Dame, IN (United States)

2012-10-01T23:59:59.000Z

222

HIGH-RESOLUTION SIMULATIONS OF CONVECTION PRECEDING IGNITION IN TYPE Ia SUPERNOVAE USING ADAPTIVE MESH REFINEMENT  

E-Print Network (OSTI)

We extend our previous three-dimensional, full-star simulations of the final hours of convection preceding ignition in Type Ia supernovae to higher resolution using the adaptive mesh refinement capability of our low Mach number code, MAESTRO. We report the statistics of the ignition of the first flame at an effective 4.34 km resolution and general flow field properties at an effective 2.17 km resolution. We find that off-center ignition is likely, with radius of 50 km most favored and a likely range of 4075 km. This is consistent with our previous coarser (8.68 km resolution) simulations, implying that we have achieved sufficient resolution in our determination of likely ignition radii. The dynamics of the last few hot spots preceding ignition suggest that a multiple ignition scenario is not likely. With improved resolution, we can more clearly see the general flow pattern in the convective region, characterized by a strong outward plume with a lower speed recirculation. We show that the convective core is turbulent with a Kolmogorov spectrum and has a lower turbulent intensity and larger integral length scale than previously thought (on the order of 16 km s?1 and 200 km, respectively), and we discuss the potential consequences for the first flames. Key words: convection hydrodynamics methods: numerical nuclear reactions, nucleosynthesis, abundances supernovae: general white dwarfs Online-only material: color figures 1.

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

2012-01-01T23:59:59.000Z

223

Direct numerical simulations of type Ia supernovae flames II: The Rayleigh-Taylor instability  

Science Conference Proceedings (OSTI)

A Type Ia supernova explosion likely begins as a nuclear runaway near the center of a carbon-oxygen white dwarf. The outward propagating flame is unstable to the Landau-Darrieus, Rayleigh-Taylor, and Kelvin-Helmholtz instabilities, which serve to accelerate it to a large fraction of the speed of sound. We investigate the Rayleigh-Taylor unstable flame at the transition from the flamelet regime to the distributed-burning regime, around densities of 10e7 gm/cc, through detailed, fully resolved simulations. A low Mach number, adaptive mesh hydrodynamics code is used to achieve the necessary resolution and long time scales. As the density is varied, we see a fundamental change in the character of the burning--at the low end of the density range the Rayleigh-Taylor instability dominates the burning, whereas at the high end the burning suppresses the instability. In all cases, significant acceleration of the flame is observed, limited only by the size of the domain we are able to study. We discuss the implications of these results on the potential for a deflagration to detonation transition.

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

2004-01-12T23:59:59.000Z

224

Constraining deflagration models of Type Ia supernovae through intermediate-mass elements  

E-Print Network (OSTI)

The physical structure of a nuclear flame is a basic ingredient of the theory of Type Ia supernovae (SNIa). Assuming an exponential density reduction with several characteristic times we have followed the evolution of a planar nuclear flame in an expanding background from an initial density 6.6 10^7 g/cm3 down to 2 10^6 g/cm3. The total amount of synthesized intermediate-mass elements (IME), from silicon to calcium, was monitored during the calculation. We have made use of the computed mass fractions, X_IME, of these elements to give an estimation of the total amount of IME synthesized during the deflagration of a massive white dwarf. Using X_IME and adopting the usual hypothesis that turbulence decouples the effective burning velocity from the laminar flame speed, so that the relevant flame speed is actually the turbulent speed on the integral length-scale, we have built a simple geometrical approach to model the region where IME are thought to be produced. It turns out that a healthy production of IME invol...

Garca-Senz, D; Cabezon, R M; Woosley, S E

2006-01-01T23:59:59.000Z

225

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

226

FLAMES IN TYPE Ia SUPERNOVA: DEFLAGRATION-DETONATION TRANSITION IN THE OXYGEN-BURNING FLAME  

Science Conference Proceedings (OSTI)

The flame in a Type Ia supernova is a conglomerate structure that, depending on density, may involve separate regions of carbon, oxygen, and silicon burning, all propagating in a self-similar, subsonic front. The separation between these three burning regions increases as the density declines until eventually, below about 2 x 10{sup 7} g cm{sup -3}, only carbon burning remains active, the other two burning phases having 'frozen out' on stellar scales. Between 2 and 3 x 10{sup 7} g cm{sup -3}, however, there remains an energetic oxygen-burning region that trails the carbon burning by an amount that is sensitive to the turbulence intensity. As the carbon flame makes a transition to the distributed regime (Karlovitz number {approx}> 10), the characteristic separation between the carbon- and oxygen-burning regions increases dramatically, from a fraction of a meter to many kilometers. The oxygen-rich mixture between the two flames is created at a nearly constant temperature, and turbulence helps to maintain islands of well-mixed isothermal fuel as the temperature increases. The delayed burning of these regions can be supersonic and could initiate a detonation.

Woosley, S. E. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Kerstein, A. R. [Combustion Research Facility, Sandia National Laboratories, Livermore, CA 94551 (United States); Aspden, A. J., E-mail: woosley@ucolick.org, E-mail: arkerst@sandia.gov, E-mail: ajaspden@lbl.gov [Center for Computational Sciences and Engineering, Lawrence Berkeley National Laboratory, CA 94720 (United States)

2011-06-10T23:59:59.000Z

227

TYPE Ia SUPERNOVAE: CALCULATIONS OF TURBULENT FLAMES USING THE LINEAR EDDY MODEL  

SciTech Connect

The nature of carbon burning flames in Type Ia supernovae is explored as they interact with Kolmogorov turbulence. One-dimensional calculations using the Linear Eddy Model of Kerstein elucidate three regimes of turbulent burning. In the simplest case, large-scale turbulence folds and deforms thin laminar flamelets to produce a flame brush with a total burning rate given approximately by the speed of turbulent fluctuations on the integral scale, U{sub L} , This is the regime where the supernova explosion begins and where most of its pre-detonation burning occurs. As the density declines, turbulence starts to tear the individual flamelets, making broader structures that move faster. For a brief time, these turbulent flamelets are still narrow compared to their spacing and the concept of a flame brush moving with an overall speed of U{sub L} remains valid. However, the typical width of the individual flamelets, which is given by the condition that their turnover time equals their burning time, continues to increase as the density declines. Eventually, mixed regions almost as large as the integral scale itself are transiently formed. At that point, a transition to detonation can occur. The conditions for such a transition are explored numerically and it is estimated that the transition will occur for densities near 1 x 10{sup 7} g cm{sup -3}, provided the turbulent speed on the integral scale exceeds about 20% sonic. An example calculation shows the details of a detonation actually developing.

Woosley, S. E. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Kerstein, A. R.; Sankaran, V. [Combustion Research Facility, Sandia National Laboratory, Livermore, CA 94551 (United States); Aspden, A. J. [Center for Computational Science and Engineering, Lawrence Berkeley National Laboratory, Berkeley, CA 94720 (United States); Roepke, F. K., E-mail: woosley@ucolick.or, E-mail: arkerst@sandia.go, E-mail: AJAspden@lbl.go, E-mail: fritz@mpa-Garching.mpg.d [Max Planck Institut fuer Astrophysik, Garching (Germany)

2009-10-10T23:59:59.000Z

228

ON THE NATURE OF THE PROGENITOR OF THE Type Ia SN2011fe IN M101  

SciTech Connect

The explosion of a Type Ia supernova, SN2011fe, in the nearby Pinwheel galaxy (M101 at 6.4 Mpc) provides an opportunity to study pre-explosion images and search for the progenitor, which should consist of a white dwarf (WD), possibly surrounded by an accretion disk, in orbit with another star. We report on our use of deep Chandra observations and Hubble Space Telescope observations to limit the luminosity and temperature of the pre-explosion WD. It is found that if the spectrum was a blackbody, then pre-SN WDs with steady nuclear burning of the highest possible temperatures and luminosities are excluded assuming moderate n{sub H} values, but values of kT between roughly 10 eV and 60 eV are permitted even if the WD was emitting at the Eddington luminosity. This allows the progenitor to be an accreting nuclear-burning WD with an expanded photosphere 4-100 times the WD itself, or a super-critically accreting WD blowing off an optically thick strong wind, or possibly a recurrent nova with luminosities an order of magnitude lower than Eddington. The observations are also consistent with a double degenerate scenario, or a spinning down WD that has been spun up by accretion from the donor.

Liu Jifeng [National Astronomical Observatory of China, Beijing 100012 (China); Di Stefano, Rosanne; Wang Tao; Moe, Maxwell [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-04-20T23:59:59.000Z

229

Capturing the Fire: Flame Energetics and Neutronizaton for Type Ia Supernova Simulations  

E-Print Network (OSTI)

We develop and calibrate a realistic model flame for hydrodynamical simulations of deflagrations in white dwarf (Type Ia) supernovae. Our flame model builds on the advection-diffusion-reaction model of Khokhlov and includes electron screening and Coulomb corrections to the equation of state in a self-consistent way. We calibrate this model flame--its energetics and timescales for energy release and neutronization--with self-heating reaction network calculations that include both these Coulomb effects and up-to-date weak interactions. The burned material evolves post-flame due to both weak interactions and hydrodynamic changes in density and temperature. We develop a scheme to follow the evolution, including neutronization, of the NSE state subsequent to the passage of the flame front. As a result, our model flame is suitable for deflagration simulations over a wide range of initial central densities and can track the temperature and electron fraction of the burned material through the explosion and into the expansion of the ejecta.

A. C. Calder; D. M. Townsley; I. R. Seitenzahl; F. Peng; O. E. B. Messer; N. Vladimirova; E. F. Brown; J. W. Truran; D. Q. Lamb

2006-11-01T23:59:59.000Z

230

DOE Solar Decathlon: Team Ontario: Queen's University, Carleton University,  

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

Team Ontario: Queen's University, Carleton University, and Algonquin Team Ontario: Queen's University, Carleton University, and Algonquin College Team website: ontariosd.ca Photo of members of the Queen's University, Carleton University, and Algonquin College Solar Decathlon 2013 team on the deck of their partially constructed house. Several members are laughing and throwing snowballs. Enlarge image The Queen's University, Carleton University, and Algonquin College Solar Decathlon 2013 team (Courtesy of the Queen's University, Carleton University, and Algonquin College Solar Decathlon 2013 team) he Queen's University, Carleton University, and Algonquin College audiovisual presentation Jury Feedback Architecture Contest Market Appeal Contest Engineering Contest Communications Contest Team Deliverables Project Manual Construction Drawings

231

University of Nebraska-Lincoln and University of Florida (Building...  

Open Energy Info (EERE)

Nebraska-Lincoln and University of Florida (Building Energy Efficient Homes for America) Jump to: navigation, search Name University of Nebraska-Lincoln and University of Florida...

232

Norwich University, Stanford University and Kentucky/Indiana...  

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

of Energy, (202) 779-3295 Jason.Lutterman@ee.doe.gov Norwich University, Stanford University and Team KentuckyIndiana Take the Affordability Contest and University of...

233

RECIPIENT:Bowling Green State University STATE: OH PROJECT TITLE:  

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

', ', , , 1'.1 'Pagf;: 1 of 2 RECIPIENT:Bowling Green State University STATE: OH PROJECT TITLE: Coastal Ohio Wind Project for Reduced Barriers to Deployment of Offshore Wind Energy Funding Opportunity Announcement Number Procurement Instrument Number NEPA Control Number CID Number COP DE-EE0003871 GFO-0003871-001 EE3871 Based on my review oftlle information concerning the proposed action, as NEPA Compliance Officer (authorized under DOE Order 45I.IA), I have made the following determination: CX, EA, EIS APPENDIX AND NUMBER: Description: A9 Information gathering (including, but not limited to, literature surveys, inventories, audits), data analysis (including computer modeling), document preparation (such as conceptual design or feasibility studies, analytical energy supply

234

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

235

A Measurement of the Rate of Type Ia Supernovae in Galaxy Clusters from the SDSS-II Supernova Survey  

E-Print Network (OSTI)

ABRIDGED We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at z <0.17 and 27 SN events in 492 maxBCG clusters at 0.1 < z < 0.3$. We find values for the cluster SN Ia rate of $({0.37}^{+0.17+0.01}_{-0.12-0.01}) \\mathrm{SNu}r h^{2}$ and $({0.55}^{+0.13+0.02}_{-0.11-0.01}) \\mathrm{SNu}r h^{2}$ ($\\mathrm{SNu}x = 10^{-12} L_{x\\sun}^{-1} \\mathrm{yr}^{-1}$) in C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be $({0.31}^{+0.18+0.01}_{-0.12-0.01}) \\mathrm{SNu}r h^{2}$ and $({0.49}^{+0.15+0.02}_{-0.11-0.01})$ $\\mathrm{SNu}r h^{2}$ in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be $({2.04}^{+1.99+0.07}_{-1.11-0.04}) \\mathrm{SNu}r h^{2}$ and $({0.36}^{+0.84+0.01}_...

Dilday, Benjamin; Becker, Andrew; Bender, Ralf; Castander, Francisco; Cinabro, David; Frieman, Joshua A; Galbany, Llus; Garnavich, Peter; Goobar, Ariel; Hopp, Ulrich; Ihara, Yutaka; Jha, Saurabh W; Kessler, Richard; Lampeitl, Hubert; Marriner, John; Miquel, Ramon; Moll, Mercedes; Nichol, Robert C; Nordin, Jakob; Riess, Adam G; Sako, Masao; Schneider, Donald P; Smith, Mathew; Sollerman, Jesper; Wheeler, J Craig; stman, Linda; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Pan, Kaike; Simmons, Audrey; Snedden, Stephanie

2010-01-01T23:59:59.000Z

236

Rare Earth Metals | Ames Laboratory  

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

are critical components in modern electronic technologies, ranging from TVs, fluorescent light bulbs, cell phones and computers to "green" magnets in electric motors that power...

237

Productive commercialization of university technology.  

E-Print Network (OSTI)

??Productive commercialization of university technology is a concern for the many stakeholders of the commercialization system. Do more total university research expenditures and more university (more)

Winder, Charles

2012-01-01T23:59:59.000Z

238

The Rise and Fall of Type Ia Supernova Light Curves in the SDSS-II Supernova Survey  

Science Conference Proceedings (OSTI)

We analyze the rise and fall times of Type Ia supernova (SN Ia) light curves discovered by the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. From a set of 391 light curves k-corrected to the rest-frame B and V bands, we find a smaller dispersion in the rising portion of the light curve compared to the decline. This is in qualitative agreement with computer models which predict that variations in radioactive nickel yield have less impact on the rise than on the spread of the decline rates. The differences we find in the rise and fall properties suggest that a single 'stretch' correction to the light curve phase does not properly model the range of SN Ia light curve shapes. We select a subset of 105 light curves well observed in both rise and fall portions of the light curves and develop a '2-stretch' fit algorithm which estimates the rise and fall times independently. We find the average time from explosion to B-band peak brightness is 17.38 {+-} 0.17 days, but with a spread of rise times which range from 13 days to 23 days. Our average rise time is shorter than the 19.5 days found in previous studies; this reflects both the different light curve template used and the application of the 2-stretch algorithm. The SDSS-II supernova set and the local SNe Ia with well-observed early light curves show no significant differences in their average rise-time properties. We find that slow-declining events tend to have fast rise times, but that the distribution of rise minus fall time is broad and single peaked. This distribution is in contrast to the bimodality in this parameter that was first suggested by Strovink (2007) from an analysis of a small set of local SNe Ia. We divide the SDSS-II sample in half based on the rise minus fall value, t{sub r} - t{sub f} {approx} 2 days, to search for differences in their host galaxy properties and Hubble residuals; we find no difference in host galaxy properties or Hubble residuals in our sample.

Hayden, Brian T.; /Notre Dame U.; Garnavich, Peter M.; /Notre Dame U.; Kessler, Richard; /KICP, Chicago /Chicago U., EFI; Frieman, Joshua A.; /KICP, Chicago /Chicago U. /Fermilab; Jha, Saurabh W.; /Stanford U., Phys. Dept. /Rutgers U., Piscataway; Bassett, Bruce; /Cape Town U., Dept. Math. /South African Astron. Observ.; Cinabro, David; /Wayne State U.; Dilday, Benjamin; /Rutgers U., Piscataway; Kasen, Daniel; /UC, Santa Cruz; Marriner, John; /Fermilab; Nichol, Robert C.; /Portsmouth U., ICG /Baltimore, Space Telescope Sci. /Johns Hopkins U.

2010-01-01T23:59:59.000Z

239

UNIVERSITY OF CALIFORNIA, SANTA CRUZ UNIVERSITY OF CALIFORNIA OBSERVATORIES  

E-Print Network (OSTI)

UNIVERSITY OF CALIFORNIA, SANTA CRUZ UNIVERSITY OF CALIFORNIA OBSERVATORIES Postdoctoral Scholar - Employee The University of California Observatories invites applications for one Postdoctoral Scholar of funding. For appointments within the University of California, the total duration of an individual

California at Santa Cruz, University of

240

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

Science Conference Proceedings (OSTI)

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

Note: This page contains sample records for the topic "university ames ia" 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.


241

Three-dimensional numerical simulations of Rayleigh-Taylorunstable flames in type Ia supernovae  

SciTech Connect

Flame instabilities play a dominant role in accelerating the burning front to a large fraction of the speed of sound in a Type Ia supernova. We present a three-dimensional numerical simulation of a Rayleigh-Taylor unstable carbon flame, following its evolution through the transition to turbulence. A low Mach number hydrodynamics method is used, freeing us from the harsh time step restrictions imposed by sound waves. We fully resolve the thermal structure of the flame and its reaction zone, eliminating the need for a flame model. A single density is considered, 1.5x107 gm/cc, and half carbon/half oxygen fuel--conditions under which the flame propagated in the flamelet regime in our related two-dimensional study. We compare to a corresponding two-dimensional simulation, and show that while fire-polishing keeps the small features suppressed in two dimensions, turbulence wrinkles the flame on far smaller scales in the three-dimensional case, suggesting that the transition to the distributed burning regime occurs at higher densities in three dimensions. Detailed turbulence diagnostics are provided. We show that the turbulence follows a Kolmogorov spectrum and is highly anisotropic on the large scales, with a much larger integral scale in the direction of gravity. Furthermore, we demonstrate that it becomes more isotropic as it cascades down to small scales. Based on the turbulent statistics and the flame properties of our simulation, we compute the Gibson scale. We show the progress of the turbulent flame through a classic combustion regime diagram, indicating that the flame just enters the distributed burning regime near the end of our simulation.

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

2005-01-28T23:59:59.000Z

242

Constraining deflagration models of Type Ia supernovae through intermediate-mass elements  

E-Print Network (OSTI)

The physical structure of a nuclear flame is a basic ingredient of the theory of Type Ia supernovae (SNIa). Assuming an exponential density reduction with several characteristic times we have followed the evolution of a planar nuclear flame in an expanding background from an initial density 6.6 10^7 g/cm3 down to 2 10^6 g/cm3. The total amount of synthesized intermediate-mass elements (IME), from silicon to calcium, was monitored during the calculation. We have made use of the computed mass fractions, X_IME, of these elements to give an estimation of the total amount of IME synthesized during the deflagration of a massive white dwarf. Using X_IME and adopting the usual hypothesis that turbulence decouples the effective burning velocity from the laminar flame speed, so that the relevant flame speed is actually the turbulent speed on the integral length-scale, we have built a simple geometrical approach to model the region where IME are thought to be produced. It turns out that a healthy production of IME involves the combination of not too short expansion times, t_c > 0.2 s, and high turbulent intensities. According to our results it could be difficult to produce much more than 0.2 solar masses of intermediate-mass elements within the deflagrative paradigma. The calculations also suggest that the mass of IME scales with the mass of Fe-peak elements, making it difficult to conciliate energetic explosions with low ejected nickel masses, as in the well observed SN1991bg or in SN1998de. Thus a large production of Si-peak elements, especially in combination with a low or a moderate production of iron, could be better addressed by either the delayed detonation route in standard Chandrasekhar-mass models or, perhaps, by the off-center helium detonation in the sub Chandrasekhar-mass scenario.

D. Garcia-Senz; E. Bravo; R. M. Cabezon; S. E. Woosley

2006-09-15T23:59:59.000Z

243

Revealing Type Ia supernova physics with cosmic rates and nuclear gamma rays  

E-Print Network (OSTI)

Type Ia supernovae (SNIa) remain mysterious despite their central importance in cosmology and their rapidly increasing discovery rate. The progenitors of SNIa can be probed by the delay time between progenitor birth and explosion as SNIa. The explosions and progenitors of SNIa can be probed by MeV nuclear gamma rays emitted in the decays of radioactive nickel and cobalt into iron. We compare the cosmic star formation and SNIa rates, finding that their different redshift evolution requires a large fraction of SNIa to have large delay times. A delay time distribution of the form t^{-1.0 +/- 0.3} provides a good fit, implying 50% of SNIa explode more than ~ 1 Gyr after progenitor birth. The extrapolation of the cosmic SNIa rate to z = 0 agrees with the rate we deduce from catalogs of local SNIa. We investigate prospects for gamma-ray telescopes to exploit the facts that escaping gamma rays directly reveal the power source of SNIa and uniquely provide tomography of the expanding ejecta. We find large improvements relative to earlier studies by Gehrels et al. in 1987 and Timmes & Woosley in 1997 due to larger and more certain SNIa rates and advances in gamma-ray detectors. The proposed Advanced Compton Telescope, with a narrow-line sensitivity ~ 60 times better than that of current satellites, would, on an annual basis, detect up to ~ 100 SNIa (3 sigma) and provide revolutionary model discrimination for SNIa within 20 Mpc, with gamma-ray light curves measured with ~ 10 sigma significance daily for ~ 100 days. Even more modest improvements in detector sensitivity would open a new and invaluable astronomy with frequent SNIa gamma-ray detections.

Shunsaku Horiuchi; John F. Beacom

2010-06-30T23:59:59.000Z

244

University Connections | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Research on the "Go" with OSTI mobile Research on the "Go" with OSTI mobile Research on the "Go" with OSTI mobile Get the EDUconnections widget and many other great free widgets at Widgetbox! University Spotlight Program The U.S. Department of Energy (DOE) Office of Scientific and Technical Information (OSTI) connects with university research departments and libraries across the nation to increase awareness of DOE's valuable scientific and technical information. OSTI "spotlights" individual universities with connections to DOE scientific research programs. Visit our spotlight below to see examples of universities that are supporting and advancing scientific research and discovery! University Spotlight Visit our Spotlight Archive to learn about great colleges and universities

245

University and College Contacts  

Science Conference Proceedings (OSTI)

... University of Kentucky Office of External Scholarships Dr. Lisa Broome-Price Lisa.broome-price@uky.edu (859) 257-1537 OR Experiences in ...

2013-09-24T23:59:59.000Z

246

Stanford University | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Prof. Wendy Mao create amorphous diamond Stanford University Dept. of Sustainability and Energy Management Stanford School of Engineering San Francisco, bordered by the Bay and...

247

PULSE at Stanford University  

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

Photon Science @ SLAC - LCLS - LUSI - SSRL - PULSE - Stanford University Go Search Home Publications Atomic & Molecular Physics Condensed Matter Physics Single Molecule Imaging...

248

DOE Virtual University  

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

The Department of Energy Virtual University (DVU) is a central venue for executing, managing, partnering and sharing corporate learning activities and programs. The DVU provides employees cost...

249

NETL F 451.1-1/1 Categorical Exclusion (CX) Designation Form  

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

PMCPVT 2011 Ron Harp 1012011 - 9302014 Ames, IA Unique Lanthanide-Free Motor Construction Develop, construct, and test new bench-scale motor prototypes that do not...

250

GEORGIA SOUTHERN UNIVERSITY University System of Georgia  

E-Print Network (OSTI)

specialties in accounting information systems, business intelligence, electronic commerce, enterprise resource selective student body representing 49 U.S. states and more than 100 nations. The University continues the State of Georgia and the region through the benefits of higher education, offering both campus

Hutcheon, James M.

251

Universal software safety standard  

Science Conference Proceedings (OSTI)

This paper identifies the minimum subset required for a truly universal safety-critical software standard. This universal software standard could be used in but is not limited to the following application domains: commercial, military and space ... Keywords: software safety, system safety, validation, verification

P. V. Bhansali

2005-09-01T23:59:59.000Z

252

CORNELL UNIVERSITY POLICY LIBRARY  

E-Print Network (OSTI)

________________________________________________________________________________________________________________________________________________ ________________________________________________________________________________________________________________________________________________ 1 Cornell University prohibits the smoking or carrying of lighted cigars, cigarettes or pipes in all Brochure Cornell University Dining Brochure Faculty Handbook Human Resource Policy 6.11.4, Staff Complaint and Grievance Procedure Student Handbook City of Ithaca Municipal Code Respiratory Effects of Passive Smoking

Manning, Sturt

253

UNIVERSITIES IN TEXAS, PRIVATE  

E-Print Network (OSTI)

Caption FOR PUBLIC UNIVERSITIES IN TEXAS, PRIVATE SUPPORT IS THE ENGINE OF QUALITY. Indeed, state support (general revenues) today provides just one-third of Texas A&M University's total budget per student as Texas A&M. COLLEGE OF SCIENCE http://www.science.tamu.edu 3257 TAMU College Station

254

UNIVERSITY POLICE ANNUAL SECURITY  

E-Print Network (OSTI)

UNIVERSITY POLICE 2013 ANNUAL SECURITY AND FIRE SAFETY GUIDE In compliance with the Jeanne Clery Disclosure of Campus Security Policy and Campus Crime Statistics Act The University of New Orleans. Please take a moment to read the following information. #12;ANNUAL SECURITY AND FIRE SAFETY GUIDE 2013

Kulp, Mark

255

MAY 2 7 1927 \\_ UNIVERSITY OF IDAHO  

E-Print Network (OSTI)

CONWAI', !I.A. Boise IIi,~h Srhool RALt·ll DolGLA~ CoRDON, ll.S.( Pre-Med.) Ashton lftr,h S£1tool Ri£1ts

O'Laughlin, Jay

256

Pacific Northwest National Laboratory: INstItute for INterfacIaL cataLysIs  

E-Print Network (OSTI)

of Chemistry University of Calgary,Alberta, Canada T2N 1N4 New Orleans National Meeting Modeling the Fischer-Tropsch study Fischer-Tropsch synthesis: An Introduction First discovered by Sabatier and Sanderens in 1902: CO + H2 CH4 Ni,Fe,Co Fischer and Tropsch reported in 1923 the synthesis of liquid hydrocarbons with high

257

INFORMATION EXCELLENTIA CoLumbIA ENgINEErINg238  

E-Print Network (OSTI)

that bends and twists. "Computers, geometry, and physics are my ingredients. I mix them up in a bowl and what science as well. B.A.Sc., University of Toronto (Canada), 1997; M.S., California Institute of TechnologySPUn Associate Professor of Computer Science #12;

Hone, James

258

Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations  

E-Print Network (OSTI)

The light curve of a type Ia supernova decays at a rate set by the beta-decay lifetimes of the Ni-56 and Co-56 produced in the explosion. This makes such a light curve sensitive to the value of the Fermi constant G_F at the time of the supernova. Using data from the CfA Supernova Archive, we measure the dependence of the light curve decay rate on redshift and place a bound on the time variation of G_F of |(dG_F/dt)/G_F| < 10^(-9) / y.

Ferrero, Alejandro

2010-01-01T23:59:59.000Z

259

Type Ia Supernova Properties as a Function of the Distance to the Host Galaxy in the SDSS-II SN Survey  

E-Print Network (OSTI)

We use type-Ia supernovae (SNe Ia) discovered by the SDSS-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host galaxy center, using the distance as a proxy for local galaxy properties (local star-formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light-curves using both MLCS2k2 and SALT2, and determine color (AV, c) and light-curve shape (delta, x1) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4-sigma level) finding is that the average fitted AV from MLCS2k2 and c from SALT2 decrease with the proj...

Galbany, Lluis; Ostman, Linda; Brown, Peter J; Cinabro, David; D'Andrea, Chris B; Frieman, Joshua; Jha, Saurabh W; Marriner, John; Nichol, Robert C; Nordin, Jakob; Olmstead, Matthew D; Sako, Masao; Schneider, Donald P; Smith, Mathew; Sollerman, Jesper; Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Elena; Malanushenko, Viktor; Oravetz, Dan; Simmons, Audrey; Shelden, Alaina

2012-01-01T23:59:59.000Z

260

University of Missouri | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Missouri Missouri Research Research at Mizzou Vice Chancellor for Research Core Facilities Research Centers Undergraduate Research Research News & Multimedia DOE Research Reports UM Researchers in E-print Network Illumination Magazine Harnessing Radioactivity for Cancer Therapy Scientists from the University of Missouri, Oak Ridge National Lab and the University of Tennessee Graduate School of Medicine harness alpha particles for radiation cancer therapy. Gold Coated Lanthanide Phosphate Nanoparticles for Targeted Alpha Generator Radiotherapy, PLOS ONE Alpha Particle Therapy, Credit: Nathan Hurst Search this site: Search UM Columbia has a reputation of excellence in teaching and research and is the flagship campus of the four-campus University of Missouri System. Resources

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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

UNIVERSITY OF CALIFORNIA, SANTA CRUZ UNIVERSITY OF CALIFORNIA OBSERVATORIES  

E-Print Network (OSTI)

UNIVERSITY OF CALIFORNIA, SANTA CRUZ UNIVERSITY OF CALIFORNIA OBSERVATORIES POSTDOCTORAL SCHOLAR ­ EMPLOYEE The University of California Observatories invites applications for one Postdoctoral Scholar of California, the total duration of an individual's postdoctoral service may not exceed five years, including

California at Santa Cruz, University of

262

Measurement of Omega_m, Omega_Lambda from a blind analysis of Type Ia supernovae with CMAGIC: Using color information to verify the acceleration of the Universe  

E-Print Network (OSTI)

Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space

2006-01-01T23:59:59.000Z

263

Gene F. Parkin, P.E. B.S.C.E. University of Iowa, Iowa City, IA; 1970 (with High Distinction)  

E-Print Network (OSTI)

Stimulation of Anaerobic Digestion," Water Research, 17, 677 (1983). 11. Hergenroeder, R. and Parkin, G of Anaerobic Toxicity by Batch and Semi-Continuous Assays," Jour. Water Pollution Control Fed., 52, 720 (1980 Anaerobic Reactors: Response to Toxic Substances," Water Science and Tech., 15, 261 (1983). #12;2 13.

Stanier, Charlie

264

Delaware State University | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Delaware State University Delaware State University Research Office of the Associate Provost for Research General Research Capability Center for Integrated Biological & Environmental Research Experimental Program to Stimulate Competitive Research Delaware IDeA Network of Biomedical Research Excellence Faculty Research DSU Leads the Way in Better Buildings DSU is one of the first university partners in the US to join the Department of Energy's Better Buildings inititative to reduce its carbon footprint by 25% by 2015. Secretary of Energy Chu participated in the DSU kick-off program to commemorate the school's efforts in July 2012. Read more about this showcase project. Search this site: Search Prestigious research projects underway by Delaware State University (DSU) serve to enhance DSU's land-grant mission and its contributions to the

265

University | OpenEI  

Open Energy Info (EERE)

University University Dataset Summary Description Provides annual energy usage for years 1989 through 2010 for UT at Austin; specifically, electricity usage (kWh), natural gas usage (Mcf), associated costs. Also provides water consumption for 2005 through 2010. Source University of Texas (UT) at Austin, Utilities & Energy Management Date Released Unknown Date Updated Unknown Keywords Electricity Consumption Natural Gas Texas Unit Cost Electricity Unit Cost Natural Gas University Water Data application/vnd.ms-excel icon Energy and Water Use Data for UT-Austin (xls, 32.8 KiB) Quality Metrics Level of Review Some Review Comment Assume data was reviewed by someone at UT-Austin prior to adding to website. Temporal and Spatial Coverage Frequency Annually Time Period 1989 - 2010

266

Ideal Gas Stephani Universes  

E-Print Network (OSTI)

The Stephani Universes that can be interpreted as an ideal gas evolving in local thermal equilibrium are determined, and the method to obtain the associated thermodynamic schemes is given

Bartolom Coll; Joan Josep Ferrando

2003-12-04T23:59:59.000Z

267

Quantum mechanical Universal constructor  

E-Print Network (OSTI)

Arbitrary quantum states cannot be copied. In fact, to make a copy we must provide complete information about the system. However, can a quantum system self-replicate? This is not answered by the no-cloning theorem. In the classical context, Von Neumann showed that a `universal constructor' can exist which can self-replicate an arbitrary system, provided that it had access to instructions for making copy of the system. We question the existence of a universal constructor that may allow for the self-replication of an arbitrary quantum system. We prove that there is no deterministic universal quantum constructor which can operate with finite resources. Further, we delineate conditions under which such a universal constructor can be designed to operate dterministically and probabilistically.

Pati, A K; Pati, Arun K.; Braunstein, Samuel L.

2003-01-01T23:59:59.000Z

268

Quantum mechanical Universal constructor  

E-Print Network (OSTI)

Arbitrary quantum states cannot be copied. In fact, to make a copy we must provide complete information about the system. However, can a quantum system self-replicate? This is not answered by the no-cloning theorem. In the classical context, Von Neumann showed that a `universal constructor' can exist which can self-replicate an arbitrary system, provided that it had access to instructions for making copy of the system. We question the existence of a universal constructor that may allow for the self-replication of an arbitrary quantum system. We prove that there is no deterministic universal quantum constructor which can operate with finite resources. Further, we delineate conditions under which such a universal constructor can be designed to operate dterministically and probabilistically.

Arun K. Pati; Samuel L. Braunstein

2003-03-19T23:59:59.000Z

269

Texas Tech University  

E-Print Network (OSTI)

Texas Tech University :: TechAnnounce http Academic Departmental Citing scheduling conflicts with the Texas Oklahoma-Texas Tech football game and international environmental reporters, experts and industry and government leaders to the Hub City. Texas Tech

Rock, Chris

270

NCAR and the Universities  

Science Conference Proceedings (OSTI)

The National Center for Atmospheric Research (NCAR) has a responsibility for enhancing and assisting the national university-based atmospheric research effort. This responsibility is met partly by programs of research at NCAR that involve ...

Wilmot N. Hess

1985-05-01T23:59:59.000Z

271

EPCglobal : a universal standard  

E-Print Network (OSTI)

This thesis evaluates the likelihood of EPCglobal becoming the universal RFID standard by presenting a framework of ten factors used to analyze and determine if EPCglobal is moving in the right direction. The ten factors ...

Aguirre, Juan Ignacio

2007-01-01T23:59:59.000Z

272

Universal desktop fabrication  

Science Conference Proceedings (OSTI)

Advances in digital design and fabrication technologies are leading toward single fabrication systems capable of producing almost any complete functional object. We are proposing a new paradigm for manufacturing, which we call Universal Desktop Fabrication ...

T. Vilbrandt; E. Malone; H. Lipson; A. Pasko

2008-01-01T23:59:59.000Z

273

Thermodynamics of Fractal Universe  

E-Print Network (OSTI)

We investigate the thermodynamical properties of the apparent horizon in a fractal universe. We find that one can always rewrite the Friedmann equation of the fractal universe in the form of the entropy balance relation $ \\delta Q=T_h d{S_h}$, where $ \\delta Q $ and $ T_{h} $ are the energy flux and Unruh temperature seen by an accelerated observer just inside the apparent horizon. We find that the entropy $S_h$ consists two terms, the first one which obeys the usual area law and the second part which is the entropy production term due to nonequilibrium thermodynamics of fractal universe. This shows that in a fractal universe, a treatment with nonequilibrium thermodynamics of spacetime may be needed. We also study the generalized second law of thermodynamics in the framework of fractal universe. When the temperature of the apparent horizon and the matter fields inside the horizon are equal, i.e. $T=T_h$, the generalized second law of thermodynamics can be fulfilled provided the deceleration and the equation of state parameters ranges either as $-1 \\leq q thermodynamics can be secured in a fractal universe by suitably choosing the fractal parameter $\\beta$.

Ahmad Sheykhi; Zeinab Teimoori; Bin Wang

2012-10-29T23:59:59.000Z

274

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

275

TYPE Ia SUPERNOVA PROPERTIES AS A FUNCTION OF THE DISTANCE TO THE HOST GALAXY IN THE SDSS-II SN SURVEY  

Science Conference Proceedings (OSTI)

We use Type Ia supernovae (SNe Ia) discovered by the Sloan Digital Sky Survey-II SN Survey to search for dependencies between SN Ia properties and the projected distance to the host-galaxy center, using the distance as a proxy for local galaxy properties (local star formation rate, local metallicity, etc.). The sample consists of almost 200 spectroscopically or photometrically confirmed SNe Ia at redshifts below 0.25. The sample is split into two groups depending on the morphology of the host galaxy. We fit light curves using both MLCS2K2 and SALT2, and determine color (A{sub V} , c) and light-curve shape ({Delta}, x{sub 1}) parameters for each SN Ia, as well as its residual in the Hubble diagram. We then correlate these parameters with both the physical and the normalized distances to the center of the host galaxy and look for trends in the mean values and scatters of these parameters with increasing distance. The most significant (at the 4{sigma} level) finding is that the average fitted A{sub V} from MLCS2K2 and c from SALT2 decrease with the projected distance for SNe Ia in spiral galaxies. We also find indications that supernovae (SNe) in elliptical galaxies tend to have narrower light curves if they explode at larger distances, although this may be due to selection effects in our sample. We do not find strong correlations between the residuals of the distance moduli with respect to the Hubble flow and the galactocentric distances, which indicates a limited correlation between SN magnitudes after standardization and local host metallicity.

Galbany, Lluis; Miquel, Ramon; Oestman, Linda [Institut de Fisica d'Altes Energies, Universitat Autonoma de Barcelona, E-08193 Bellaterra (Barcelona) (Spain); Brown, Peter J.; Olmstead, Matthew D. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States); Cinabro, David [Department of Physics and Astronomy, Wayne State University, Detroit, MI 48201 (United States); D'Andrea, Chris B.; Nichol, Robert C. [Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX (United Kingdom); Frieman, Joshua [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellise Avenue, Chicago, IL 60637 (United States); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, John [Center for Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Nordin, Jakob [E.O. Lawrence Berkeley National Lab, 1 Cyclotron Rd., Berkeley, CA 94720 (United States); Sako, Masao [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Schneider, Donald P. [Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802 (United States); Smith, Mathew [Department of Physics, University of Western Cape, Bellville 7535, Cape Town (South Africa); Sollerman, Jesper [Oskar Klein Centre, Department of Astronomy, AlbaNova, SE-106 91 Stockholm (Sweden); Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard, E-mail: lluis.galbany@ist.utl.pt [Apache Point Observatory, P.O. Box 59, Sunspot, NM 88349 (United States); and others

2012-08-20T23:59:59.000Z

276

The Universe Adventure - Early Models  

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

Early Models of the Universe Ready for Blast-off Space exploration missions contribute greatly to our understanding of the Universe. With our new understanding of the fundamental...

277

J Apostolov Zlatomir D University  

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

of Tennessee-Knoxville Group C Group I Saparov Bayrammurad University of Delaware Nguyen Lam T. Florida State University Kanitpanyacharoen K itpanyach Waruntorn Warunt...

278

Auburn University | Open Energy Information  

Open Energy Info (EERE)

University Place Auburn, Alabama Zip 36849 Product Largest university in Alabama, enrolling approximately 23,000 students in 230 undergraduate, graduate, and professional programs....

279

Split University | Open Energy Information  

Open Energy Info (EERE)

Jump to: navigation, search Name Split University Place Zagreb, Croatia Sector Hydro, Solar Product Croatia-based electrical engineering faculty of Split University....

280

California Stanford University of University Institute of University California of Southern  

E-Print Network (OSTI)

California Stanford University of University Institute of University California of Southern Technology California ____________________________________________________________ February 15, 2011 Dear Representative, As Congress considers funding options for the remainder of fiscal year (FY) 2011, California

Narayanan, Shrikanth S.

Note: This page contains sample records for the topic "university ames ia" 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.


281

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\\le0.12$. Assuming a flat cosmology with $\\Omega_m = 0.3=1-\\Omega_\\Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({\\rm systematic})^{+0.90}_{-0.71}({\\rm statistical})] \\times 10^{-5} {\\rm SNe} {\\rm Mpc}^{-3} h_{70}^3 {\\rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rat...

Dilday, Benjamin; Frieman, J A; Holtzman, J; Marriner, J; Miknaitis, G; Nichol, R C; Romani, R; Sako, M; Bassett, B; Becker, A; Cinabro, D; De Jongh, F; Depoy, D L; Doi, M; Garnavich, P M; Hogan, C J; Jha, S; Konishi, K; Lampeitl, H; Marshall, J L; McGinnis, D; Prieto, J L; Riess, A G; Richmond, M W; Schneider, D P; Smith, M; Takanashi, N; Tokita, K; van der Heyden, K; Zheng, N Yasuda C; Barentine, J; Brewington, H; Choi, C; Crotts, A; Dembicky, J; Harvanek, M; Im, M; Ketzeback, W; Kleinman, S J; Krzesi?ski, J; Long, D C; Malanushenko, E; Malanushenko, V; McMillan, R J; Nitta, A; Pan, K; Saurage, G; Snedden, S A; Watters, S; Wheeler, J C; York, D

2008-01-01T23:59:59.000Z

282

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

283

Universe Adventure Web Standards  

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

Universe Universe Adventure Web Standards for the Smart Physics Student Author: Patrick Lii - plii@ugastro.berkeley.edu Date: August 3, 2007 ABSTRACT You may be wondering: why are the Universe Adventure web standards so impor- tant? And why do I have to read this stupid document about them? The old versions of our site were plagued with messy (and faulty) coding: the pages were littered with broken links, missing images, broken flash files, and all sorts of other problems which made the site highly inaccessible. When we tried to fix these errors, we found that the coding was so incredibly messy that a simple edit like changing some of the words in a paragraph or adding an image took hours rather than minutes. In fact, the coding was so horrific that we simply constructed an entirely new site rather than making the laborious attempt to fix the old one. In order to make sure that future students working

284

University Location Project Description  

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

Location Project Description Location Project Description Boise State University Boise, Idaho Boise State University has undertaken a study of the structural setting and geothermal potential at Neal Hot Springs that will integrate geology, geochemistry, and geophysics to analyze the site on the western Snake River plain. Boise State will determine if Neal Hot Springs sustains the necessary rock dilation and conduit pathways for hydrothermal fluid flow and successful geothermal development. The result will be new data acquisition, including a deep geophysical survey and fault surface data. Colorado School of Mines Golden, Colorado Colorado School of Mines will conduct an investigation near Homedale, Idaho, an area that straddles volcanic rock and unconsolidated sediments.

285

Making the Standard Candle: A study of how the progenitor white dwarf modulates the peak luminosity of type Ia supernovae  

SciTech Connect

The goals of the proposed research as stated in the proposal were to: Build a suite of one-dimensional initial models of different metallicities and central densities. Using the improved flame capturing scheme, simulate the explosion of a white dwarf with embedded Lagrangian tracer particles, and post-process the thermal histories of the tracers to reconstruct the nucleosynthesis of the explosion. Survey the effects of a changing progenitor metallicity on the isotopic yields. Of particular interest is 1) whether the linear relation between the mass of 56Ni synthesized and the pro- genitor metallicity is moderated by the effect of electron captures in the core; and 2) how a varying central density alters the relation between metallicity and 56Ni mass. Using these results, examine how the observed metallicity distribution would affect the brightness distribution of SNe Ia and the isotopic ratios about the Fe-peak.

Brown, Edward F [Michigan State University

2010-01-21T23:59:59.000Z

286

Determining the motion of the solar system relative to the cosmic microwave background using type Ia supernovae  

E-Print Network (OSTI)

We estimate the solar system motion relative to the cosmic microwave background using type Ia supernovae (SNe) measurements. We take into account the correlations in the error bars of the SNe measurements arising from correlated peculiar velocities. Without accounting for correlations in the peculiar velocities, the SNe data we use appear to detect the peculiar velocity of the solar system at about the 3.5 sigma level. However, when the correlations are correctly accounted for, the SNe data only detects the solar system peculiar velocity at about the 2.5 sigma level. We forecast that the solar system peculiar velocity will be detected at the 9 sigma level by GAIA and the 11 sigma level by the LSST. For these surveys we find the correlations are much less important as most of the signal comes from higher redshifts where the number density of SNe is insufficient for the correlations to be important.

Christopher Gordon; Kate Land; Anze Slosar

2007-11-27T23:59:59.000Z

287

Quantum Universe Hitoshi Murayama (Berkeley)  

E-Print Network (OSTI)

Quantum Universe Hitoshi Murayama (Berkeley) University of Tennessee, Jan 22, 2007 #12;COBE showed quantum origin of the universe #12;400Kyr 13.7Byr 1min 10 -10sec #12;To understand physics at the largest made of? · How did it come to be? · Why do we exist? Moving from philosophy to physics Quantum Universe

Murayama, Hitoshi

288

201107861 1..6  

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

Kinetically Kinetically inhibited order in a diamond-lattice antiferromagnet Gregory J. MacDougall a,1 , Delphine Gout a,b,c , Jerel L. Zarestky d , Georg Ehlers a , Andrey Podlesnyak a , Michael A. McGuire b , David Mandrus b,e , and Stephen E. Nagler a a Neutron Scattering Science Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831; b Materials Science and Technology Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831; c Jülich Centre for Neutron Science-Spallation Neutron Source, Forschungszentrum Jülich, 52425 Jülich, Germany; d Ames Laboratory and Department of Physics and Astronomy, Iowa State University, Ames, IA 50011; and e Department of Materials Science and Engineering, University of Tennessee, Knoxville, TN 37996 Edited* by M. Brian Maple, University of California, San Diego, La Jolla, CA, and approved August 2, 2011 (received for review May 17, 2011) Frustrated

289

Graduate Handbook Clemson University  

E-Print Network (OSTI)

Graduate Handbook Clemson University #12;2 Table of Contents Introduction to fundamental knowledge in a student's chosen area of concentration (i.e., applied fluid mechanics, construction to fundamental knowledge in a student's chosen area of concentration (i.e., applied fluid mechanics, construction

Bolding, M. Chad

290

Cornell University Facilities Services  

E-Print Network (OSTI)

- substation design engineers, protective relay engineers, dispatchers in the control centers etc. AnotherRequirements Specification for and Evaluation of an Automated Substation Monitoring System Mladen for the Automated Analysis Substation System (AASS) implemented at Texas A&M University, aimed at monitoring

Manning, Sturt

291

Texas Tech University System  

E-Print Network (OSTI)

Texas Tech University System :: Huffaker Named as Texas Tech System General Counsel http://www.texastech.edu/stories/12-03-TTUS-Washington-DC-Trip.php[4/2/2012 8:13:27 AM] Chancellor Hance and leadership from the Texas visited with Texas Tech students and Congressional interns while in Washington, D.C. March 27, 2012 Texas

Rock, Chris

292

UNIVERSITY OF FINANCIAL MANAGEMENT  

E-Print Network (OSTI)

UNIVERSITY OF HAWAI`I FINANCIAL MANAGEMENT INFORMATION SYSTEMS (FMIS) ON-LINE QUICK REFERENCE GUIDE Reference Guide FIXED ASSETS SYSTEM (FFX) Scrn Num Screen Name 502 Asset Maintenance Use this screen-2093 Fixed Assets System (FFX), Inventory Maintenance - transfer, disposal of equipment, decal, equipment

293

Models for universal usability  

Science Conference Proceedings (OSTI)

This paper discusses how model-based approaches can support designers and developers to address a number of challenges raised by universal usability, such as the possibility of obtaining user interfaces able to adapt to any device and usability evaluation ... Keywords: abstract user interfaces, authoring environments, heterogeneous clients, multi-platform user interfaces, remote evaluation, task Models

Fabio Patern

2003-11-01T23:59:59.000Z

294

Universal nonlinear entanglement witnesses  

Science Conference Proceedings (OSTI)

We give a universal recipe for constructing nonlinear entanglement witnesses able to detect nonclassical correlations in arbitrary systems of distinguishable and/or identical particles for an arbitrary number of constituents. The constructed witnesses are expressed in terms of expectation values of observables. As such, they are, at least in principle, measurable in experiments.

Kotowski, Marcin; Kotowski, Michal [College of Inter-Faculty Individual Studies in Mathematics and Natural Sciences, Warsaw University, PL-Warszawa (Poland); Center for Theoretical Physics, Polish Academy of Sciences, Aleja Lotnikow 32/44, PL-02-668 Warszawa (Poland); Kus, Marek [Center for Theoretical Physics, Polish Academy of Sciences, Aleja Lotnikow 32/44, PL-02-668 Warszawa (Poland)

2010-06-15T23:59:59.000Z

295

Northwestern University Transportation Center  

E-Print Network (OSTI)

Northwestern University Transportation Center 2011 Business Advisory Committee NUTC #12;#12;I have the pleasure of presenting our Business Advisory Committee members--a distinguished group of transportation industry lead- ers who have partnered with the Transportation Center in advancing the state of knowledge

Bustamante, Fabián E.

296

Broadband and universal service  

Science Conference Proceedings (OSTI)

Section 254(b)(3) of the 1996 Telecommunications Act established the objective that residents of rural areas should have access to advanced telecommunications and information services comparable to services in urban areas. Pursuant to the passage of ... Keywords: Broadband policy, Empirical analysis, Rural, Telecommunications policy, Universal service

David Gabel

2007-07-01T23:59:59.000Z

297

University of Waste Procedures  

E-Print Network (OSTI)

University of Maryland Hazardous And Regulated Waste Procedures Manual Revised July 2001 #12;Review II. HAZARDOUS WASTE MANAGEMENT III. BIOLOGICAL, PATHOLOGICAL AND MEDICAL WASTE (BPMW) MANAGEMENT IV. LOW-LEVEL RADIOACTIVE WASTE (LLRW) MANAGEMENT V. EMERGENCY PROCEDURES VI. WASTE MINIMIZATION VII

Rubloff, Gary W.

298

California Stanford University of University of Institute of University California Southern  

E-Print Network (OSTI)

California Stanford University of University of Institute of University California Southern Technology California March 13, 2012 The Honorable Dianne Feinstein 331 Hart Senate Office Building Washington, DC 20510-0504 Dear Senator Feinstein: On behalf of California's research universities, we write

Southern California, University of

299

The Universe Adventure - Redshift  

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

Expansion of the Universe Expansion of the Universe Redshift Expansion of Space Redshifts Light The expansion of space redshifts light. As space expands, light waves get stretched and their wavelengths shift. The more that light is stretched, the longer its wavelengths become, and the color of each wave shifts toward the red end of the light spectrum. We say that this light is redshifted. The Doppler Effect in action. A moving fire truck's siren changes pitch as it moves past you. This is known as the Doppler Effect. To get a better idea of how this actually works, we'll look at a common phenomenon: the Doppler Effect. Imagine you hear a fire truck coming right toward you. As the truck approaches, the pitch of the siren gets higher and higher. As soon as the truck passes you however, the pitch drops lower as

300

Nuclear Energy University Programs  

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

NEUP FY2011 Process Presentation to NEAC December 9, 2010 Marsha Lambregts, NEUP-IO Manager FUNDED R&D PROPOSALS BY STATE 2010 * Awards/Full Submissions - 42/128 * Awards to PIs for first time - 29 * Awards to junior faculty - 20 * Awards that are experimental - 30 * Awards in materials and waste - 30 * Awards to Nuclear Engineering Faculty - 18 * Number of universities receiving awards - 26 * Number of awards with lab partners - 20 * Number of universities receiving awards for first time - 8 2 2010 INFRASTRUCTURE * Major Reactor: 4 awards for a total of $3.75 M * Minor Reactor: 12 awards for $1.95 M * General Scientific Infrastructure: 33 award for $7.47 M * Since 2009, $ 19.438 M has been awarded in General Scientific Infrastructure (did not issue Major or Minor Reactor calls in 2009).

Note: This page contains sample records for the topic "university ames ia" 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.


301

Regional University Alliance  

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

Alliance Alliance Developed by the National Energy Technology Laboratory in collaboration with NETL-Regional University Alliance WVU National Research Center for Coal and Energy Fossil Consulting Services, Inc. The AVESTAR(tm) Center provides a state-of- the-art, highly realistic, dynamic simulator for a coal-fired power plant using Integrated Gasification Combined Cycle (IGCC) technology with CO 2 capture. The system is based on Invensys' DYNSIM ® software

302

WESTERN UNIVERSITY Disaster Plan  

E-Print Network (OSTI)

.7 Assumptions 1.7.1 Emergency 1.7.2 Disaster 1.8 Concept of Operations 1.8.1 Background 1.8.2 Emergency Response/Administrative Unit Responsibilities 1.8.8 Situation Reports 2. UTILIZING THE DISASTER PLAN 2.1 Emergency Process Members ­ Individual Responsibilities #12;WESTERN UNIVERSITY Disaster Plan January, 2013 2.7.1 VP

Sinnamon, Gordon J.

303

Universal battery terminal connector  

SciTech Connect

This patent describes a universal battery terminal connector for connecting either a top post battery terminal or a side post battery terminal to a battery cable. The connector comprises an elongated electrically conductive body having: (a) first means for connection to a top post battery terminal; (b) second means for connection to a side post battery terminal, and (c) third means for receiving one end of a battery cable and providing an electrical connection therewith.

Norris, R.W.

1987-01-13T23:59:59.000Z

304

The Universe Adventure - The Homogenous and Isotropic Universe  

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

Our View of the Universe Our View of the Universe All observations that have been made using the most powerful telescopes show that the universe looks the same in all directions. The average density of galaxies is the same throughout the universe and does not change with distance or direction. This is called the Cosmological Principle. Distribution of Galaxies On average and at large scales, the distribution of galaxies is the same throughout the universe. Since the expansion of space occurs evenly at every point in the universe, galaxies are separating from each other at about the same pace, giving the universe a nearly uniform density and structure. As a result, the universe appears smooth at large distance scales. In scientific terms, it is said to be homogeneous and isotropic.

305

College/University: University of Indonesia; Jakarta, Indonesia  

E-Print Network (OSTI)

Education College/University: University of Indonesia; Jakarta, Indonesia Highest degree: B, under revision First name: Meta Last name: Djojosubroto Date of birth: 21.11.1975 Country: Indonesia E

Manstein, Dietmar J.

306

University Science Highlights  

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

universities/highlights/ The Office of Science is universities/highlights/ The Office of Science is the single largest supporter of basic research in the physical sciences in the United States, providing more than 40 percent of total funding for this vital area of national importance. It oversees - and is the principal federal funding agency of - the Nation's research programs in high-energy physics, nuclear physics, and fusion energy sciences. en {B0DFBA1D-D6A0-4920-8E73-4779F8F5ACEA}http://science.energy.gov/np/highlights/2013/np-2013-12-a/ Modeling Cosmic Nucleosynthesis First measurements of isotopes produced by Argonne's new CARIBU facility provide insight into the creation of the elements in the universe. Thu, 09

307

NEVADA UNIVERSITY TRANSPORTATION CENTER UNIVERSITY OF NEVADA, LAS VEGAS  

E-Print Network (OSTI)

of professionals and future leaders in the area of transportation systems. · Support of career growthNEVADA UNIVERSITY TRANSPORTATION CENTER UNIVERSITY OF NEVADA, LAS VEGAS 2011-2012 ANNUAL REPORT #12 University Transportation Center (NUTC) Vision: The NUTC will strive to become a nationally recognized center

Ahmad, Sajjad

308

Nanoscale Vise Puts the Squeeze on Ferroelectric Materials  

Science Conference Proceedings (OSTI)

May 26, 2009... State University, Northwestern University, Motorola, Ames Laboratory, Intel Corporation, and Tricorn Tech contributed to this development.

309

Fermilab Today | University of Arizona  

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

A&M University Dec. 12, 2012 NAME: Texas A&M University HOME TOWN: College Station, Texas MASCOT: Reveille COLORS: Maroon and white COLLABORATING AT FERMILAB SINCE: Early 1980s....

310

2009 University Coal Research Program  

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

2009 University Coal Research Program 2009 University Coal Research Program Description The University Coal Research (UCR) Program provides grants to U.S. colleges and universities to support fundamental research and to develop efficient and environmentally responsible fossil energy technologies. Funded by the U.S. Department of Energy (DOE) Office of Fossil Energy (FE), the program is carried out by DOE's National Energy Technology Laboratory (NETL).

311

1993 - CECM - Simon Fraser University  

E-Print Network (OSTI)

Feb 2, 2001... differentiability of convex functions on various Banach spaces,'' Regional Functional Analysis Conference, Miami University , Oxford, Ohio. 8.

312

Postscript - CECM - Simon Fraser University  

E-Print Network (OSTI)

NERSC/MSRI Workshop. on. Parallel Symbolic Computation. CECM. Centre for Experimental &. Constructive Mathematics. Simon Fraser University. Berkeley...

313

DOE Solar Decathlon: Gallery of Kentucky/Indiana: University...  

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

KentuckyIndiana: University of Louisville, Ball State University and University of Kentucky Photos of University of Louisville, Ball State University and University of Kentucky's...

314

CURRICULUM VITAE University of Idaho  

E-Print Network (OSTI)

CURRICULUM VITAE University of Idaho NAME: Scarnecchia, Dennis L. DATE: July 26, 2004 RANK OR TITLE of Idaho 1990-June 1998, Associate Professor, Department of Fish and Wildlife Resources, University of Idaho 1985-90, Assistant Professor, Department of Animal Ecology, Iowa State University 1986

315

University of Toronto Governing Council  

E-Print Network (OSTI)

In policies approved by the Governing Council, the University community has held that the essential purpose on any issue without reference to prescribed doctrine, as well as the right to criticize the University use of University facilities, in accordance with its policies as they are defined from time to time

Sun, Yu

316

The Future of University Nuclear Engineering Programs and University  

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

The Future of University Nuclear Engineering Programs and The Future of University Nuclear Engineering Programs and University Research and Training Reactors The Future of University Nuclear Engineering Programs and University Research and Training Reactors Nuclear engineering programs and departments with an initial emphasis in fission were formed in the late 1950's and 1960's from interdisciplinary efforts in many of the top research universities, providing the manpower for this technical discipline. In the same time period, for many of these programs, university nuclear reactors were constructed and began their operation, providing some of the facilities needed for research and training of students engaged in this profession. However, over the last decade, the U.S. nuclear science and engineering educational structure has not only stagnated but has reached a state of

317

The Future of University Nuclear Engineering Programs and University  

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

The Future of University Nuclear Engineering Programs and The Future of University Nuclear Engineering Programs and University Research and Training Reactors The Future of University Nuclear Engineering Programs and University Research and Training Reactors Nuclear engineering programs and departments with an initial emphasis in fission were formed in the late 1950's and 1960's from interdisciplinary efforts in many of the top research universities, providing the manpower for this technical discipline. In the same time period, for many of these programs, university nuclear reactors were constructed and began their operation, providing some of the facilities needed for research and training of students engaged in this profession. However, over the last decade, the U.S. nuclear science and engineering educational structure has not only stagnated but has reached a state of

318

Collaborative University Research Education | ORNL  

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

Collaborative University Research Collaborative University Research SHARE Collaborative University Research ORNL scientist Jonathan Mielenz works in an anaerobic chamber used to handle biomass-degrading microbes at the Joint Institute for Biological Sciences.Source: ORNL Flickr site With a strong commitment to education, ORNL maintains relationships with many educational institutions and organizations. Many student and faculty programs are administered through Oak Ridge Associated Universities (ORAU) and include opportunities for undergraduates, graduates, postgraduates, faculty, and some pre-college students. The lab also partners with the University of Tennessee in several joint research efforts and though programs aimed at training the next generation of interdisciplinary scientists. These collaborations include:

319

Jong-Woo Kim  

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

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Jong-Woo Kim Argonne National Laboratory 9700 S. Cass Ave 432/B008 Argonne, Il 60439 Phone: 252-0248 Fax: 252-7392 E-Mail: jwkim@aps.anl.gov Education/Experience: 2007 - present: Assistant Physicist, Advanced Photon Source, Argonne National Lab. 2005-2007: Postdoctoral Research Associate, APS/μ-CAT, Ames Laboratory, Argonne, IL. Ph. D. Condensed Matter Physics; Iowa State University, Ames, IA; 2005 M.S. Physics; Yongsei University, Seoul, Korea; 2000

320

Doug Robinson  

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

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Doug Robinson Argonne National Laboratory 9700 S. Cass Ave 432/B007 Argonne, Il 60439 Phone: 252-0247 Fax: 252-7392 E-Mail: drobinsn@aps.anl.gov Education/Experience: 2009 - present: Physicist, Argonne National Lab. 1997 -2009: Beamline Scientist, APS/μ-CAT, Ames Laboratory, Argonne, IL. 1988-1997: Staff Scientist, Microelectronics Research Center, Iowa State University, Ames, IA Ph.D. Condensed Matter Physics, University of Illinois, Urbana,

Note: This page contains sample records for the topic "university ames ia" 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.


321

A localised subgrid scale model for fluid dynamical simulations in astrophysics II: Application to type Ia supernovae  

E-Print Network (OSTI)

The dynamics of the explosive burning process is highly sensitive to the flame speed model in numerical simulations of type Ia supernovae. Based upon the hypothesis that the effective flame speed is determined by the unresolved turbulent velocity fluctuations, we employ a new subgrid scale model which includes a localised treatment of the energy transfer through the turbulence cascade in combination with semi-statistical closures for the dissipation and non-local transport of turbulence energy. In addition, subgrid scale buoyancy effects are included. In the limit of negligible energy transfer and transport, the dynamical model reduces to the Sharp-Wheeler relation. According to our findings, the Sharp-Wheeler relation is insuffcient to account for the complicated turbulent dynamics of flames in thermonuclear supernovae. The application of a co-moving grid technique enables us to achieve very high spatial resolution in the burning region. Turbulence is produced mostly at the flame surface and in the interior ash regions. Consequently, there is a pronounced anisotropy in the vicinity of the flame fronts. The localised subgrid scale model predicts significantly enhanced energy generation and less unburnt carbon and oxygen at low velocities compared to earlier simulations.

W. Schmidt; J. C. Niemeyer; W. Hillebrandt; F. K. Roepke

2006-01-23T23:59:59.000Z

322

Early and late time VLT spectroscopy of SN 2001el - progenitor constraints for a type Ia supernova  

E-Print Network (OSTI)

We present early time high-resolution (VLT/UVES) and late time low-resolution (VLT/FORS) optical spectra of the normal type Ia supernova, SN 2001el. The high-resolution spectra were obtained 9 and 2 days before (B-band) maximum light in order to detect narrow hydrogen and/or helium emission lines from the SN CSM. No such lines were detected in our data. We therefore use photoionisation models to derive upper limits of 1x10^-5 and 6x10^-5 Msol/yr, assuming wind velocities of 10 and 50 km/s, respectively, for the mass loss rate from the progenitor system of SN 2001el. This excludes a symbiotic star in the upper mass loss rate regime from being the progenitor of SN 2001el. The low-resolution spectrum was obtained in the nebular phase of the supernova, \\~400 days after the maximum light, to search for any hydrogen rich gas originating from the SN progenitor system. However, we see no signs of Balmer lines in our spectrum. Therefore, we model the late time spectra to derive an upper limit of ~0.03 Msol for solar a...

Mattila, S; Sollerman, J; Kozma, C; Baron, E; Fransson, C; Leibundgut, B; Nomoto, K

2005-01-01T23:59:59.000Z

323

The Universe Adventure - Current Research  

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

Current Research Current Research When launched, the Supernova Acceleration Probe (SNAP) will study the effects of dark energy by surveying distant type Ia supernovae and making detailed measurements of weak gravitational lensing. With the new Large Hadron Collider (LHC) at CERN nearing full completion, experimentalists will soon be able to test certain elements of String Theory. While not definitive, these tests will cast some light upon the theory's parameters and may even provide clues into the identity of dark matter. Meanwhile, theorists continue to investigate the implications of String Theory for Big Bang cosmology, particularly the effects of strings on cosmic inflation. As particle physicists eagerly await the results from the new LHC, observational cosmologists are busy developing astronomical experiments,

324

Gcb0511 800..812  

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

Interannual Interannual variability in global soil respiration, 1980±94 J A M E S W . R A I C H * , C H R I S T O P H E R S . P O T T E R { and D W I P E N B H A G A W A T I {,1 *Department of Botany, Iowa State University, Ames, IA, 50011, USA; {Ecosystem Science and Technology Branch, NASA-Ames Research Center, Moffett Field, CA 94035, USA; {Department of Civil and Construction Engineering, Iowa State University, Ames, IA, 50011 USA Abstract We used a climate-driven regression model to develop spatially resolved estimates of soil-CO 2 emissions from the terrestrial land surface for each month from January 1980 to December 1994, to evaluate the effects of interannual variations in climate on global soil- to-atmosphere CO 2 fluxes. The mean annual global soil-CO 2 flux over this 15-y period was estimated to be 80.4 (range 79.3±81.8) Pg C. Monthly variations in global soil-CO 2 emissions followed closely the mean temperature

325

University Coal Research | Department of Energy  

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

University Coal Research University Coal Research Universities frequently win Fossil Energy research competitions or join with private companies to submit successful research...

326

Clean Cities: Clean Cities University Online Learning  

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

University Online Learning to someone by E-mail Share Clean Cities: Clean Cities University Online Learning on Facebook Tweet about Clean Cities: Clean Cities University Online...

327

Florida International University | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Spotlight Archive Spotlight Archive Contact Florida International University Professors and Faculty of Interest Prof. Osama Mohammed receives IEEE Energy Conversion Award Prof. Osama Mohammed receives IEEE Energy Conversion Award Prof. Madhavan Nair's groundbreading research may lead to new hope in the battle Prof. Madhavan Nair's groundbreading research may lead to new hope in the battle against Neuro-AIDS Asst. Prof. Vagelis Hristidis awarded Google Research Award Asst. Prof. Vagelis Hristidis awarded Google Research Award Exceptional Students and Alumnus DOE Fellow Duriem Calderin on his way to DOE's Hanford Site DOE Fellow Duriem Calderin on his way to DOE's Hanford Site DOE Fellow, Rosa Ramirez hired by DOE's Environmental Management Professional De DOE Fellow, Rosa Ramirez hired by DOE's Environmental Management Professional Development Corps

328

The Universe Adventure - Links  

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

Links Links Cosmology and Space Cosmic Journey A site chronicling the history of scientific cosmology, presented by the American Institute of Physics. Hubble Ultra-Deep Field Skywalker Lets you explore the famous Hubble Deep Field photo, which is the deepest view (in the visible spectrum) into the sky to date. QuietBay Constellation Tutorial A fun and easy tutorial to familiarize yourself with the night sky. Astronomy Picture of the Day Astronomy Picture of the Day features a new image from the universe every day, with short explanations written by professional astronomers. The Solar System NASA site that includes images and profiles of the planets (plus Pluto). Earth Guide An Earth planetary science site created by the Japan Science and Technology Agency describing many of the features of Earth and its place in the

329

NANYANG TECHNOLOGICAL UNIVERSITY  

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

Naing Naing Aung, Xingbo Liu Naing Naing Aung, Xingbo Liu 03-12-2012 Development of Self-Powered Wireless-Ready High Temperature Electrochemical Sensors for In-Situ Corrosion Monitoring of Boiler Tubes WestVirginiaUniversity College of Engineering and Mineral Resources DoE Award No. DE- FE0005717 Project Objectives  To develop in-situ corrosion monitoring sensors for corrosion of USC boiler tubes in next generation coal-based power systems  To develop thermal-electric based energy harvesting and telecommunication devices for the self-powered wireless ready sensor system Current Milestones July to September 2011 Initiate preliminary high-temperature electrochemical corrosion rate (ECR) probe design October to December 2011 To complete the design and construction of (ECR)

330

The Universe Adventure - Atoms  

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

Matter and Atoms Matter and Atoms Richard Feynman "If, in some cataclysm, all of scientific knowledge were to be destroyed, and only one sentence passed on to the next generations of creatures, what statement would contain the most information in the fewest words? I believe it is that...all things are made of atoms." -Richard P. Feynman, winner of the 1965 Nobel Prize in Physics All is atoms Matter is made of atoms, and atoms are comprised of protons, neutrons, and electrons. Everything in the Universe is made of matter. Though matter exists in many different forms, each form is made out of the same basic constituents: small particles called atoms. Atoms themselves are made of smaller particles: protons, neutrons, and electrons. Protons and neutrons are composed of even smaller particles called quarks.

331

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

332

Universal RFP 11202k  

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

AND OBJECTIVES AND OBJECTIVES UNIVERSAL MUSIC GROUP (UMG) is seeking proposals from qualified energy service providers (ESP) and generators interested in assisting us in an effort to protect the environment through the consumption of renewable electricity and to reliably meet the electrical needs of our facilities. We hope to reduce emissions and alleviate other negative environmental impacts of our energy consumption. Therefore UMG is seeking to purchase 100% green power for our facility in Santa Monica, CA. Our preference is to purchase a product with the greatest amount of new renewable generation. UMG is looking to spend the same amount it currently spends on electricity or as close to that as possible. UMG wants a fixed rate product that is not tied to the PX price. UMG will only switch electricity providers if

333

Nuclear Energy University Programs  

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

1 Status 1 Status Presentation to Nuclear Energy Advisory Committee (NEAC) June 15, 2011 Michael Worley, NEUP Program Manager NEUP Funding is Program Driven Program Directed Funding Program Supported Funding Mission Supported Funding Natl. Labs Universities DOE-NE HQ Peer Review DOE NE Program Drivers 2 3 Summary of Improvements and New Programs for FY 2011 * Expand "Blue Sky" Research and Development (R&D) * Initiate Integrated Research Projects (IRP) * Expand and improve peer review data base * Evaluate adoption of NRC and NNSA Metrics as appropriate to NEUP * Conduct peer review at pre-application stage for R&D 2011 Proposed NEUP Budget - $61.8M * Program Directed Integrated Research Projects (IRP) - $12.0M (NEW)

334

Pennsylvania State University | .EDUconnections  

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

Old Main, Credit: George Chriss Old Main, Credit: George Chriss Research Research at Penn State Capabilities and Projects Institutes of Energy and the Environment Huck Institutes of Life Sciences Materials Research Institute Eberly College of Science Alternative Energy Research Research Publications Faculty Expertise Database Research News DOE Research Results Penn State Commencement 2012 United States Secretary of Energy Dr. Steven Chu was the commencement speaker at Penn State's Eberly College of Science 2012 spring graduation ceremony held May 5 at the Bryce Jordan Center on the University Park campus. Read more. Search this site: Search Over the past ten years, more than 28,000 graduate degrees were conferred by Penn State, including over 6,300 doctoral degrees. Resources About Penn State

335

The Universe Adventure - Composition  

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

Elemental Abundances Elemental Abundances Understanding Our History A Star is Born An accretion disk forms during the birth of a star. There are precise physical and chemical processes that govern the evolution of planets, stars, and galaxies. By analyzing the structure and chemical content of astronomical objects, scientists can garner valuable information about what the universe's conditions must have been like long ago in order to account for currently observed elemental ratios. Formation of a Galaxy A forming galaxy. The Composition of the Earth We can begin in our own backyard. Geologists have determined that the Earth is composed primarily of heavy elements (those containing many protons and neutrons). The crust and mantle are made up of compounds containing large traces of oxygen, nickel, aluminum, magnesium, iron, silicon, and sulfur.

336

The Universe Adventure - Feedback  

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

Contact Us Contact Us First Name (optional): Simpson Last Name (optional): Homer E-Mail Address (if you would like to hear back from us): How can we contact you? Occupation (high school student, physics teacher, cosmologist, et cetera): What is your occupation? Type: Type of Feedback Organization/Format Content Fundamentals of Cosmology Evidence for the Big Bang Eras of the Cosmos The Final Frontier Glossary Other Comments and Feedback: We appreciate your comments! - The Universe Adventure Team submit reset [ top ] Site Content National Science Foundation Department of Energy S.D. Bechtel, Jr. Foundation [ Site Map ] optimized for Firefox [ UC Berkeley ] [ UC Berkeley Physics ] [ Particle Adventure! ] [ Contact Us ] Copyright © 2005 Lawrence Berkeley National Laboratory Physics Division |

337

Oak Ridge Associated Universities  

Office of Legacy Management (LM)

the the Office of Environmental Restoration U.S. Department of Energy RADIOLOGICAL SURVEY OF THE FORMER BLISS AND LAUGHLIN STEEL COMPANY FACILITY BUFFALO, NEW YORK J. D. BERGER Environmental Survey and Site Assessment Program Energy/Environment Systems Division DRAFT REPORT APRIL 1992 c -. ..". FlLS\COPY x_.. --. RADIOLOGICAL SURVEY OF THE FORMER BLISS AND LAUGHLIN STEEL COMPANY FACILITY 110 HOPKINS STREET BUFFALO, NEW YORK Prepared by J. D. Berger Environmental Survey and Site Assessment Program Energy/Environmental Systems Division Oak Ridge Associated Universities/Oak Ridge Institute for Science and Education Oak Ridge, Tennessee 37831-0117 Project Staff R. D. Condra D. A. Gibson M. J. Laudernan R. B. Slaten Prepared for Department of Energy

338

Efficient universal blind computation  

E-Print Network (OSTI)

We give a cheat sensitive protocol for blind universal quantum computation that is efficient in terms of computational and communication resources: it allows one party to perform an arbitrary computation on a second party's quantum computer without revealing either which computation is performed, or its input and output. The first party's computational capabilities can be extremely limited: she must only be able to create and measure single-qubit superposition states. The second party is not required to use measurement-based quantum computation. The protocol requires the (optimal) exchange of O(J log(N)) single-qubit states, where J is the computational depth and N is the number of qubits needed for the computation.

Vittorio Giovannetti; Lorenzo Maccone; Tomoyuki Morimae; Terry G. Rudolph

2013-06-12T23:59:59.000Z

339

DOE Solar Decathlon: Norwich University  

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

Norwich University Norwich University Team website: www.nusd2013.org Photo of members of the Norwich University Solar Decathlon 2013 team standing in front of a building on campus. Enlarge image The Norwich University Solar Decathlon 2013 team (Courtesy of the Norwich University Solar Decathlon 2013 team) he Norwich University audiovisual presentation Jury Feedback Architecture Contest Market Appeal Contest Engineering Contest Communications Contest Team Deliverables Project Manual Construction Drawings Menu and Recipes Neither the United States, nor the Department of Energy, nor the Alliance for Sustainable Energy LLC, nor any of their contractors, subcontractors, or their employees make any warranty, express or implied, or assume any legal liability or responsibility for the accuracy, completeness, or

340

REGULATIONS OF THE UNIVERSITY OF FLORIDA  

E-Print Network (OSTI)

, the University Police, the University's armored car vendor, and the staff of the Florida Museum of Natural

Roy, Subrata

Note: This page contains sample records for the topic "university ames ia" from the National Library of EnergyBeta (NLEBeta).
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341

UNIVERSITY STUDENT TITLE OF TALK OU  

Science Conference Proceedings (OSTI)

... EL University of Puerto Rico Rivera-Cotty, Norman Instrumentation of Geothermal Heat Pump Test System EL Loyola University ...

2012-12-17T23:59:59.000Z

342

Universal Lighting Technologies | Open Energy Information  

Open Energy Info (EERE)

Product Universal Lighting Technologies develops, manufactures and markets energy efficient lighting technologies including HID, CFLs and ballasts. References Universal...

343

University Partnerships / Academic Alliances | National Nuclear...  

National Nuclear Security Administration (NNSA)

Home > About Us > Our Programs > Defense Programs > Office of Research, Development, Test Capabilities and Evaluation > University Partnerships Academic Alliances University...

344

EVOLUTION OF POST-IMPACT COMPANION STARS IN SN Ia REMNANTS WITHIN THE SINGLE-DEGENERATE SCENARIO  

Science Conference Proceedings (OSTI)

The nature of the progenitor systems of Type Ia supernovae is still uncertain. One way to distinguish between the single-degenerate scenario and double-degenerate scenario is to search for the post-impact remnant star. To examine the characteristics of the post-impact remnant star, we have carried out three-dimensional hydrodynamic simulations of supernova impacts on main-sequence-like stars. We explore the evolution of the post-impact remnants using the stellar evolution code MESA. We find that the luminosity and radius of the remnant star dramatically increase just after the impact. After the explosion, post-impact companions continue to expand on a progenitor-dependent timescale of {approx}10{sup 2.5}-10{sup 3} years before contracting. It is found that the time evolution of the remnant star is dependent not only on the amount of energy absorbed but also on the depth of the energy deposition. We examine the viability of the candidate star Tycho G as the possible remnant companion in Tycho's supernova by comparing it to the evolved post-impact remnant stars in our simulations. The closest model in our simulations has a similar effective temperature, but the luminosity and radius are twice as large. By examining the angular momentum distribution in our simulations, we find that the surface rotational speed could drop to {approx}10 km s{sup -1} if the specific angular momentum is conserved during the post-impact evolution, implying that Tycho G cannot be completely ruled out because of its low surface rotation speed.

Pan, Kuo-Chuan; Ricker, Paul M. [Department of Astronomy, University of Illinois at Urbana-Champaign, 1002 West Green Street, Urbana, IL 61801 (United States); Taam, Ronald E., E-mail: kpan2@illinois.edu, E-mail: pmricker@illinois.edu, E-mail: taam@northwestern.edu [Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208 (United States)

2012-11-20T23:59:59.000Z

345

BNL | Physics of the Universe  

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

Core Capabilities Facilities Physics of the Universe image Exploring the Frontiers of Energy, Intensity and the Cosmos Brookhaven leads high-energyparticle physics experiments...

346

1999 - CECM - Simon Fraser University  

E-Print Network (OSTI)

Jan 16, 2001 ... October 14th ``Doing Math in the Presence of Technology,'' Colloquium, Department of Mathematics and Statistics, Miami University of Ohio...

347

Fermilab Today | Baylor University Profile  

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

the Run 2B Level 1 Tracking Trigger (XFT) PARTICLE PHYSICS RESEARCH FOCUS: Higgs boson, QCD, searches for new phenomena WHAT SETS PARTICLE PHYSICS AT BAYLOR UNIVERSITY...

348

Fermilab Today | University of Oklahoma  

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

to emerge from the Large Hadron Collider. Our theory group also works on nonperturbative quantum field theory. WHAT SETS PARTICLE PHYSICS AT THE UNIVERSITY OF OKLAHOMA APART? OU...

349

Fermilab Today | Boston University Profile  

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

simulations of quantum chromodynamics, cosmology, and the application of mathematics to quantum field theory. WHAT SETS PARTICLE PHYSICS AT BOSTON UNIVERSITY APART? We have a...

350

Universe creation on a computer  

E-Print Network (OSTI)

The purpose of this paper is to provide an account of the epistemology and metaphysics of universe creation on a computer.

Gordon McCabe

2005-11-13T23:59:59.000Z

351

NETL: Onsite Research - University Projects  

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

Onsite Research University Projects The National Energy Technology Laboratory (NETL) is helping to overcome a growing national problem of a diminishing number of new energy...

352

University Turbine Systems Research Program  

SciTech Connect

The primary areas of university research were combustion, aerodynamics/heat transfer, and materials, with a few projects in the area of instrumentation, sensors and life (ISL).

Leitner, Robert; Wenglarz, Richard

2010-12-31T23:59:59.000Z

353

Thesis - CECM - Simon Fraser University  

E-Print Network (OSTI)

Midwest Symposium on Circuit Theory, Colorado State University, pp. 13.0-13.10 . 1965. [31] R. McConnell. A Certifying Algorithm for the Consecutive Ones...

354

University Graduate School Academic Bulletin  

E-Print Network (OSTI)

Scholar of Psychological and Brain Sciences William Estes Oscar R. Ewing Professor of Philosophy J), Elliot R. Smith* (Psychological and Brain Sciences), Olaf Sporns* (Psychological and Brain Sciences144 University Graduate School 2009-2010 Academic Bulletin Cognitive Science University Graduate

Indiana University

355

CALIFORNIA STATE UNIVERSITY, RISK MANAGEMENT  

E-Print Network (OSTI)

performance within the CSU System. #12;2004 ­ 2005 Risk Management Annual Report Page 3 · Chaired the CSU-04 2004-05 Fullerton System-Wide #12;2004 ­ 2005 Risk Management Annual Report Page 10 University · International travel · Facilities use · Deferred maintenance Working with the University's Risk Management

de Lijser, Peter

356

CURRICULUM VITAE University of Idaho  

E-Print Network (OSTI)

CURRICULUM VITAE University of Idaho NAME: Wall, Richard Wayne DATE: August 25, 2006 RANK OR TITLE of Idaho, Moscow, Idaho, 1989, EE M.Engr., Electrical Engineering, University of Idaho, Moscow, Idaho, 1989, EE Certificates and Licenses: Professional Registration: State of Idaho Professional Engineer

Kyte, Michael

357

CURRICULUM VITAE University of Idaho  

E-Print Network (OSTI)

CURRICULUM VITAE University of Idaho NAME: Abdel-Rahim, Ahmed DATE: December 15, 2005 RANK OR TITLE) Certificates and Licenses: Professional Engineer (PE), State of Idaho EXPERIENCE: Teaching, Extension and Research Appointments: Assistant Professor, Civil Engineering Department, University of Idaho, Moscow

Kyte, Michael

358

Council of University Transportation Centers  

E-Print Network (OSTI)

Council of University Transportation Centers 13th Anniversary CUTC Awards Banquet January 9, 2010 Omni Shoreham Hotel Washington, D.C. #12;Council of University Transportation Centers 13th Anniversary Awards Banquet Saturday, January 9, 2010 Welcome Stephen Albert, CUTCVice-President WesternTransportation

Nagurney, Anna

359

Universal: Order (2013-SE-26004)  

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

DOE ordered Universal Lighting Technologies, Inc. to pay a $7,264 civil penalty after finding Universal had manufactured and distributed in commerce in the U.S. 454 units of model B140R277HP, a noncompliant fluorescent lamp ballast.

360

University IPv4 Deployment Status  

Science Conference Proceedings (OSTI)

... edu.usd. University of South Dakota, [3] 3/3/3 [I], [1] 2/2/2 [I], [1] 1/1/1 [I]. edu.sdstate. South Dakota State University, [3] 3/0/2 [I], [2] 2/2/2 [O], [1] 1/0/ ...

Note: This page contains sample records for the topic "university ames ia" 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.


361

Universal service: A new definition?  

Science Conference Proceedings (OSTI)

The concept of ''universal service obligation'' (USO) has been around for decades; however, its definition continues to change. The notion that the last mile of fixed-line access should be subsidized has spread around the world, despite well reasoned ... Keywords: Auctions, Pricing policy, Subsidy, Universal service/access/connectivity

James Alleman; Paul Rappoport; Aniruddha Banerjee

2010-02-01T23:59:59.000Z

362

NEUP Approved Universities | Department of Energy  

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

NEUP Approved Universities NEUP Approved Universities NEUP Approved Universities U.S. universities and colleges must apply to the U.S. Department of Energy to administer NEUP scholarships and fellowships. That is done through a separate solicitation operated by the Department of Energy's Idaho field office. If your university is not listed below, contact NEUP@inl.gov. Approved Universities Auburn University Boise State University Clemson University College of Southern Maryland Colorado School of Mines Duke University Francis Marion University Georgia Institute of Technology Idaho State University Illinois Institute of Technology Kansas State University Lakeshore Community College Linn State Technical College Massachusetts Institute of Technology Miami Dade College Missouri University of Science & Technology

363

Gorchakova-IA  

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

(3D) Radiation Codes (Cahalan 2000). In the present work, the broadband fluxes of solar radiation are calculated using two different approaches. The purpose is * to compare...

364

Oak Ridge Universities  

Office of Legacy Management (LM)

Oak Ridge Oak Ridge Universities Prepared for Division of Remedial Action Projects U.S. Department of Energy C O M P R E H E N S I V E R A D I O L O G I C A L S U R V E Y O F F - S I T E P R O P E R T Y X N I A G A R A F A L L S S T O R A G E S I T E L E W l s T o N , N E W Y O R K J . D . B E R G E R R a d i o l o g i c a l M a n p o w e r E d u c a t i o n ' Site Assessment Program Research, and Training Division FINA], May REPORT 1 9 8 4 COMPREHENSIVE MDIOLOGICAI SURVEY OFF-SITE PROPERTY X NIAGARA FAI-LS STORAGE SITE LEWISTON' NEI'I YORK u. s. F o r m e r l y U t i l i z e d P r e p a r e d f o r Department of EnergY a s p a r t o f t h e S i t e s - - R e u e d i a l A c t i o n P r o g r a m R a d i o l o g i c a l M a n p o w e r E d u c a t i o n , O a k R i d g e O a k R i d g e , J . D . B e r g e r P r o j e c t J . B u r d e n * R . D . C o n d r a D . L . D a v i s J . S . E p l e r * P . W . F r a m e W . 0 . H e l t o n R . C . G o s s l e e S t a f f J . A . P e r r y I { . L . S n i t h T . J . S o w e l l G . M . S t e p h e n s L . B . T a u s * C . F . W e a v e r B . S . Z a c h a r e k Prepared by S i t e A s s e

365

Closed Sessions Program The closed session program plan is given in detail in Appendix I-A. The program started  

E-Print Network (OSTI)

for enhancing renewable energy usage · Assist in education and research in renewable energy · Changing behavior on "Energy for Sustainable Development: Perspectives from the Arab Region", followed by 20-minute presentations by participating Middle East Universities on their country specific energy profiles, with emphasis

366

Ab initio formation energies of FeCr alloys P. Olsson a,*, I.A. Abrikosov b  

E-Print Network (OSTI)

University, Box 534, SE-75121 Uppsala, Sweden c Department of Nuclear and Reactor Physics, Royal Institute Uppsala, Sweden b Condensed Matter Theory Group, Physics Department, AAngstroom Laboratory, Uppsala reactors, face centered cubic (fcc) and hexagonal close packed (hcp) phases were considered in order

367

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

368

Early and late time VLT spectroscopy of SN 2001el - progenitor constraints for a type Ia supernova  

E-Print Network (OSTI)

We present early time high-resolution (VLT/UVES) and late time low-resolution (VLT/FORS) optical spectra of the normal type Ia supernova, SN 2001el. The high-resolution spectra were obtained at -9 and -2 days to allow the detection of narrow hydrogen and/or helium emission lines from the circumstellar medium of the SN. No such lines were detected, and we therefore use photoionisation models to derive upper limits of 9x10^-6 Msun/yr and 5x10^-5 Msun/yr for the mass loss rate from the progenitor system assuming velocities of 10 km/s and 50 km/s, respectively, for a wind extending to outside at least a few x 10^15 cm away from the SN explosion site. These limits exclude a symbiotic star in the upper mass loss rate regime from being the progenitor of SN 2001el. The low resolution spectrum was obtained in the nebular phase of the SN, 400 days after the maximum light, to search for any hydrogen rich gas originating from the SN progenitor system. However, we see no signs of Balmer lines in our spectrum. Therefore, we model the late time spectra to derive an upper limit of ~0.03 Msun for solar abundance material present at velocities lower than 1000 km/s within the SN explosion site. According to simulations of Marietta et al. (2000) this is less than the expected mass lost by a subgiant, red giant or main sequence secondary star at a small binary separation as a result of the SN explosion. Finally, we discuss the origin of high velocity Ca II lines. We see both the CaII IR triplet and the H&K lines in the -9 days spectrum at a very high velocity of up to 34000 km/s. The spectrum also shows a flat-bottomed Si II `6150 A' feature similar to the one previously observed in SN 1990N at -14 days. We compare these spectral features to those observed in SNe 1984A and 1990N at even higher velocities.

S. Mattila; P. Lundqvist; J. Sollerman; C. Kozma; E. Baron; C. Fransson; B. Leibundgut; K. Nomoto

2005-01-20T23:59:59.000Z

369

Ontario Universities: Going Greener The University of Western Ontario  

E-Print Network (OSTI)

biological wastewater treatment and gasification of municipal wastes. o Reducing the effects of mining an estimated energy savings of 5500 gigajoules/year As part of its yearly capital renewal plan, the University

Ma, Bin

370

The Universe Adventure - Formation and Structure of the Universe  

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

The Geometry of the Universe and Structure Formation BOOMERanG and the CMB CMB data collected by the balloon-based BOOMERanG and MAXIMA experiments provided crucial evidence in...

371

A Measurement of the Rate of type-Ia Supernovae at Redshift $z\\approx$ 0.1 from the First Season of the SDSS-II Supernova Survey  

E-Print Network (OSTI)

We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $z\\le0.12$. Assuming a flat cosmology with $\\Omega_m = 0.3=1-\\Omega_\\Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({\\rm systematic})^{+0.90}_{-0.71}({\\rm statistical})] \\times 10^{-5} {\\rm SNe} {\\rm Mpc}^{-3} h_{70}^3 {\\rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rate, $r_V \\propto (1+z)^{\\beta}$, we obtain a value of $\\beta = 1.5 \\pm 0.6$, i.e. the SN Ia rate is determined to be an increasing function of redshift at the $\\sim 2.5 \\sigma$ level. Fitting the results to a model in which the volumetric SN rate, $r_V=A\\rho(t)+B\\dot \\rho(t)$, where $\\rho(t)$ is the stellar mass density and $\\dot \\rho(t)$ is the star formation rate, we find $A = (2.8 \\pm 1.2) \\times 10^{-14} \\mathrm{SNe} \\mathrm{M}_{\\sun}^{-1} \\mathrm{year}^{-1}$, $B = (9.3^{+3.4}_{-3.1})\\times 10^{-4} \\mathrm{SNe} \\mathrm{M}_{\\sun}^{-1}$.

Benjamin Dilday; R. Kessler; J. A. Frieman; J. Holtzman; J. Marriner; G. Miknaitis; R. C. Nichol; R. Romani; M. Sako; B. Bassett; A. Becker; D. Cinabro; F. DeJongh; D. L. Depoy; M. Doi; P. M. Garnavich; C. J. Hogan; S. Jha; K. Konishi; H. Lampeitl; J. L. Marshall; D. McGinnis; J. L. Prieto; A. G. Riess; M. W. Richmond; D. P. Schneider; M. Smith; N. Takanashi; K. Tokita; K. van der Heyden; N. Yasuda; C. Zheng; J. Barentine; H. Brewington; C. Choi; A. Crotts; J. Dembicky; M. Harvanek; M. Im; W. Ketzeback; S. J. Kleinman; J. Krzesi?ski; D. C. Long; E. Malanushenko; V. Malanushenko; R. J. McMillan; A. Nitta; K. Pan; G. Saurage; S. A. Snedden; S. Watters; J. C. Wheeler; D. York

2008-01-22T23:59:59.000Z

372

AMES Success Stories - Energy Innovation Portal  

1 Success Stories; Category Title and Abstract Company / Laboratories Date; Industrial Technologies Lead Free Solder. A lead free solder, developed at ...

373

Division of Chemical & Biological Sciences | Ames Laboratory  

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

Division of Chemical & Biological Sciences Division of Chemical & Biological Sciences Image Welcome Research teams in this Division conduct fundamental and applied studies of how...

374

Ames Laboratory Technology Marketing Summaries - Energy ...  

Innovative microstructures that can direct light in a manner similar to the way semiconductors can ... the efficiency of conventional incandescent ...

375

AME 327: Thermodynamics I CATALOG DATA  

E-Print Network (OSTI)

. Gas power cycles. Refrigeration and heat pump cycles. Tests. Practice and Assessment Methods: In order the course description: Engineering Science: 3.0 credits or 100% Engineering Design: 0 credits Prepared by

376

What are the Rare Earths? | Ames Laboratory  

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

made from neodymium-iron--boron have been used in a variety of products, including electric motors and hybrid cars components. The Elements Scandium Sc symbol Scandium...

377

Ames Laboratory Technology Marketing Summaries - Energy ...  

Innovative microstructures that can direct light in a manner similar to the way semiconductors can ... the efficiency of conventional incandescent light bulbs.

378

UNIVERSITY OF THE DISTRICT OF  

E-Print Network (OSTI)

UNIVERSITY OF THE DISTRICT OF COLUMBIA 1 Removal of Eutrophic Nutrients from Wastewater-Supplemented Digester Elutriate in the Fermentor 2. The Effect of Differential- Heating of Digester Elutriate on its

District of Columbia, University of the

379

International Programs Oregon State University,  

E-Print Network (OSTI)

Philippines Vietnam Azerbaijan Ghana* Malawi Slovakia Cambodia Guatemala Mexico South Korea AVAILABILITY, AZERBAIJAN Major: Industrial Engineering, minor: Business, Senior Education: Crescent Valley High School (FLEX exchange program); Qafqaz University (Azerbaijan), 2005-07 Experience: Future Leaders Exchange

Escher, Christine

380

Hamdard University | Open Energy Information  

Open Energy Info (EERE)

Hamdard University Hamdard University Jump to: navigation, search Name Hamdard University Place Karachi, Pakistan Zip 74600 Sector Solar Product University setting up Pakistan's first solar lab. Coordinates 24.88978°, 67.028511° 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":24.88978,"lon":67.028511,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

Note: This page contains sample records for the topic "university ames ia" 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

Purdue University | Open Energy Information  

Open Energy Info (EERE)

Purdue University Purdue University Jump to: navigation, search Logo: Purdue University Name Purdue University Address West Lafayette, IN Zip 47907 Phone number (765) 494-4600 Website http://www.purdue.edu/ Coordinates 40.42747955036°, -86.920051574707° 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":40.42747955036,"lon":-86.920051574707,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

382

EAST CAROLINA UNIVERSITY BENEFITS INFORMATION  

E-Print Network (OSTI)

that the transaction has transpired. Optional Retirement Plan (ORP) It takes 5 years of membership to be vested in this program. When you depart from the University, you need to complete an ORP-3 form to indicate your plans

383

Fermilab Today | Oklahoma State University  

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

University group is involved in top quark studies, searches for a non-Standard Model Higgs boson, heavy flavor tagging and upgrade of the pixel detector in the ATLAS experiment....

384

Is the Universe really expanding?  

E-Print Network (OSTI)

The Hubble law, determined from the distance modulii and redshifts of galaxies, for the past 80 years, has been used as strong evidence for an expanding universe. This claim is reviewed in light of the claimed lack of necessary evidence for time dilation in quasar and gamma-ray burst luminosity variations and other lines of evidence. It is concluded that the observations could be used to describe either a static universe (where the Hubble law results from some as-yet-unknown mechanism) or an expanding universe described by the standard Lambda cold dark matter model. In the latter case, size evolution of galaxies is necessary for agreement with observations. Yet the simple non-expanding Euclidean universe fits most data with the least number of assumptions. From this review it is apparent that there are still many unanswered questions in cosmology and the title question of this paper is still far from being answered.

John G. Hartnett

2011-07-13T23:59:59.000Z

385

PNNL: About PNNL - University Partnerships  

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

students In 2011 PNNL and Washington State University partnered to pilot a program in which graduate students in selected areas would do part of their dissertation work at PNNL....

386

The University Intercampus Program in  

E-Print Network (OSTI)

.........................................................................................6 E. Balancing Program Load and Outside Work....................................................7 FThe University of KANSAS Intercampus Program in Communicative Disorders AUDIOLOGY Au.D. HANDBOOK ......................................................... 5 II. Au.D. Program

Peterson, Blake R.

387

Visualizing the protein sequence universe  

Science Conference Proceedings (OSTI)

Modern biology is experiencing a rapid increase in data volumes that challenges our analytical skills and existing cyberinfrastructure. Exponential expansion of the Protein Sequence Universe (PSU), the protein sequence space, together with the costs ... Keywords: azure, blast, cog, computational bioinformatics, data visualization, data-enabled life sciences, delsa, em, hadoop, hive, mapreduce, mpi, multidimensional scaling, needleman-wunsch, protein annotation, protein sequence universe, psu, sammon, sequence similarity, twister, uniprot, uniref

Larissa Stanberry, Roger Higdon, Winston Haynes, Natali Kolker, William Broomall, Saliya Ekanayake, Adam Hughes, Yang Ruan, Judy Qiu, Eugene Kolker, Geoffrey Fox

2012-06-01T23:59:59.000Z

388

University Advanced Coal Generation Research  

Science Conference Proceedings (OSTI)

In 2012, the Electric Power Research Institute (EPRI) was a sponsor of projects conducted under the auspices of two consortia that support university research for coal-based power generation: the Biomass and Fossil Fuel Research Alliance (BF2RA) in the United Kingdom and the University Turbine System Research (UTSR) program of the United States Department of Energy (DOE). This technical update report describes the progress made in both of those ...

2012-12-12T23:59:59.000Z

389

Low Dose Radiation Research Program: Universities  

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

Universities Universities | Duke University | Loma Linda University | Northwestern University | University of Chicago | University of California Davis | Northwestern University University of Chicago University of California Davis Effects of Low Dose Irradiation on NF-κB Signaling Networks and Mitochondria Principal Investigator: Dr. Gayle Woloschak DOE Low Dose Research Program Projects Low dose-low dose rate irradiation leads to long term changes in numbers of mitochondria and mitochondrial genomes - Principal Investigator: Gayle Woloschak, Professor, Department of Radiation Oncology, Northwestern University, Chicago, IL, USA NF-κB-mediated pro-survival network in low dose radiation-induced adaptive protection - Principal Investigator: Jian Jian Li, Professor, Department of Radiation Oncology, University of California Davis, Davis,

390

Observational Study of Higher Dimensional Magnetic Universe in Non-linear Electrodynamics  

E-Print Network (OSTI)

In this work, we have considered the flat FRW model of the universe in $(n+2)$-dimensions filled with the dark matter and the magnetic field. We present the Hubble parameter in terms of the observable parameters $\\Omega_{m0}$ and $H_{0}$ with the redshift $z$ and the other parameters like $B_{0},\\omega, \\mu_{0},\\delta,n,w_{m}$. The natures of magnetic field $B$, deceleration parameter $q$ and $Om$ diagnostic have also been analyzed for accelerating expansion of the universe. From Stern data set (12 points), we have obtained the bounds of the arbitrary parameters by minimizing the $\\chi^{2}$ test. The best-fit values of the parameters are obtained by 66%, 90% and 99% confidence levels. Now to find the bounds of the parameters ($B_{0},\\omega$) and to draw the statistical confidence contour, we fixed four parameters $\\mu_{0},\\delta,n,w_{m}$. Here the parameter $n$ determines the higher dimensions and we perform comparative study between three cases : 4D $(n=2)$, 5D $(n=3)$ and 6D $(n=4)$ respectively. Next due to joint analysis with BAO observation, we have also obtained the bounds of the parameters ($B_{0},\\omega$) by fixing other parameters $\\mu_{0},\\delta,n,w_{m}$ for 4D, 5D and 6D. The best fit of distance modulus for our theoretical model and the Supernova Type Ia Union2 sample are drawn for different dimensions.

Chayan Ranjit; Shuvendu Chakraborty; Ujjal Debnath

2013-04-04T23:59:59.000Z

391

ISW effect as probe of features in the expansion history of the Universe  

E-Print Network (OSTI)

In this paper, using and implementing a new line of sight CMB code, called CMBAns [1], that allow us to modify H(z) for any given feature at any redshift we study the effect of changes in the expansion history of the Universe on the CMB power spectrum. Motivated by the detailed analytical calculations of the effects of the changes in H(z) on ISW plateau and CMB low multipoles, we study two phenomenological parametric form of the expansion history using WMAP data and through MCMC analysis. Our MCMC analysis shows that the standard LCDM cosmological model is consistent with the CMB data allowing the expansion history of the Universe vary around this model at different redshifts. However, our analysis also show that a decaying dark energy model proposed in [2] has in fact a marginally better fit than the standard cosmological constant model to CMB data. Concordance of our studies here with the previous analysis showing that Baryon Acoustic Oscillation (BAO) and supernovae data (SN Ia) also prefer mildly this dec...

Das, Santanu; Souradeep, Tarun

2013-01-01T23:59:59.000Z

392

Building a Universal Nuclear Energy Density Functional  

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

Building a Universal Nuclear Energy Density Functional Building a Universal Nuclear Energy Density Functional VaryMatrix.png Collaboration with mathematicians and computational...

393

Robert Gordon University | Open Energy Information  

Open Energy Info (EERE)

search Name Robert Gordon University Address Centre for Research in Energy and the Environment The Robert Gordon University Schoolhill Place Aberdeen Zip AB10 1FR Sector Marine...

394

University Coal Research | Department of Energy  

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

University Coal Research University Coal Research University Coal Research Universities frequently win Fossil Energy research competitions or join with private companies to submit successful research proposals. Today approximately 16 percent of the Office of Fossil Energy's annual R&D funding goes to academic institutions. The University Coal Research Program Universities have traditionally fared well in the Energy Department's open competitions for federal research grants and contracts. In 1979, however, the Department took an additional step to encourage greater university participation in its fossil energy program. The agency set aside funding for a special university-only competition that required professors to conduct cutting-edge research alongside students who were pursuing advanced

395

California State University CSU | Open Energy Information  

Open Energy Info (EERE)

State University CSU Jump to: navigation, search Name California State University (CSU) Place Los Angeles, California Zip 90802-4210 Sector Solar Product One of the largest higher...

396

DOE Solar Decathlon: 2009 Rice University  

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

the Rice University team on a deck extending from their unfinished Solar Decathlon house. The house is sided in corrugated metal. Rice University students display team spirit while...

397

NETL Regional University Alliance (NETL-RUA)  

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

PDF-539KB NETL-RUAs five universities are regionally recognized and share a long history of supporting NETLs energy research. Additionally, the member universities have...

398

Colorado State University | Open Energy Information  

Open Energy Info (EERE)

Colorado State University Jump to: navigation, search Name Colorado State University Place Colorado Utility Id 56493 References EIA Form EIA-861 Final Data File for 2010 -...

399

University of Colorado Technologies Available for Licensing ...  

Wind Energy; Partners (27) Visual Patent Search; Success Stories; News; Events; University of Colorado Technologies Available for Licensing The University of Colorado ...

400

CECM: Summer Meeting 2007 - Simon Fraser University  

E-Print Network (OSTI)

Lunch at the Himalayan Peak restaurant. Shrum Science Building P8495 ? Simon Fraser University ? 8888 University Drive ? Burnaby ? BC ? V5A 1S6 ? Canada ? p...

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to obtain the most current and comprehensive results.


401

University of Michigan | Open Energy Information  

Open Energy Info (EERE)

University of Michigan Jump to: navigation, search Name University of Michigan Place Ann Arbor, Michigan Zip 48109 Product Offers research across all disciplines. References...

402

University Coal Research | Department of Energy  

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

Science & Innovation Clean Coal Crosscutting Research University Coal Research University Coal Research Clean Coal Turbines Gasification Fuel Cells Hydrogen from Coal Coal...

403

HancherAuditorium University Creative Services  

E-Print Network (OSTI)

Government Iowa Memorial Union Iowa House Hotel University Bookstore University Box Office Center for Student Planning, Design and Construction Office of Sustainability Utilities and Energy Management Human Resources

Stanier, Charlie

404

University of Colorado Technology Marketing Summaries - Energy ...  

University of Colorado Technology Marketing Summaries. Here youll find marketing summaries for technologies available for licensing from the University of Colorado ...

405

NETL Regional University Alliance (NETL-RUA)  

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

Integrated Program Team NETL Regional University Alliance (NETL-RUA) About NETL-RUA - Integrated Program Team Integrated Program Team Member Universities History Mission Team...

406

NETL Regional University Alliance (NETL-RUA)  

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

State University Institutes of Energy and the Environment, 2008-present Director, Biomass Energy Center, Pennsylvania State University, 2006-present Associate Professor,...

407

Fermilab Today | Northern Illinois University Profile  

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

Nothern Illinois University June 4, 2009 NAME: Northern Illinois University HOME TOWN: DeKalb, Illinois MASCOT: Huskie SCHOOL COLORS: Cardinal red and black PARTICLE PHYSICS...

408

Oak Rigde Associated Universities (ORAU) Radiation Emergency...  

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

Oak Rigde Associated Universities (ORAU) Radiation Emergency Assistance CenterTraining Site (REACTS), ORAU Director Oak Rigde Associated Universities (ORAU) Radiation Emergency...

409

CECM: Summer Meeting 2007 - Simon Fraser University  

E-Print Network (OSTI)

Sandy Rutherford being introduced by Michael Monagan. Shrum Science Building P8495 ? Simon Fraser University ? 8888 University Drive ? Burnaby ? BC ? V5A...

410

CECM: Summer Meeting 2007 - Simon Fraser University  

E-Print Network (OSTI)

Sandy Rutherford talking about applications of queuing theory in the public sector. Shrum Science Building P8495 ? Simon Fraser University ? 8888 University...

411

CECM: Summer Meeting 2007 - Simon Fraser University  

E-Print Network (OSTI)

Sandy Rutherford with Nikolas Karalis during the poster session. Shrum Science Building P8495 ? Simon Fraser University ? 8888 University Drive ? Burnaby ? BC...

412

UNIVERSITY OF CALIFORNIA, SAN DIEGO Experiments on Vortex Symmetrization in Magnetized Electron Plasma Columns  

E-Print Network (OSTI)

. Soloshenko IA et al (2000) Plasma Phys Reports 26:792 22. Laroussi M, Mendis DA, Rosenberg M (2003) New J

California at San Diego, University of

413

DOE Solar Decathlon: Norwich University  

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

Norwich University Norwich University Delta T-90 House www.nusd2013.org Norwich University's mission at the U.S. Department of Energy Solar Decathlon 2013 is to show that high-performance, solar-powered dwellings can be affordable and beautiful. The Delta T-90 House accommodates New England's unique seasons and is designed to be affordable for those earning 20% less than the Vermont median income. Design Philosophy The house explores the hidden values and richness within a conservation-based lifestyle and respects the interdependency between the economy and the built environment. The Delta T-90 House is guided by the beliefs that high-performance, solar-powered dwellings should be available to all and that good design is not a function of cost. By maximizing the building envelope first and then using simplified mechanical systems as a

414

Tuning universality far from equilibrium  

E-Print Network (OSTI)

Possible universal dynamics of a many-body system far from thermal equilibrium are explored. A focus is set on meta-stable non-thermal states exhibiting critical properties such as self-similarity and independence of the details of how the respective state has been reached. It is proposed that universal dynamics far from equilibrium can be tuned to exhibit a dynamical phase transition where these critical properties change qualitatively. This is demonstrated for the case of a superfluid two-component Bose gas exhibiting different types of long-lived but non-thermal critical order. Scaling exponents controlled by the ratio of experimentally tuneable coupling parameters offer themselves as natural smoking guns. The results shed light on the wealth of universal phenomena expected to exist in the far-from-equilibrium realm.

Markus Karl; Boris Nowak; Thomas Gasenzer

2013-02-05T23:59:59.000Z

415

Universal Energy | Open Energy Information  

Open Energy Info (EERE)

Energy Energy Jump to: navigation, search Name Universal Energy Place Nanjing, Jiangsu Province, China Sector Solar Product Universal Energy is a PV module and solar hot water systems manufacturer. Universal Energy has a manufacturing base in Nanjing, China. Coordinates 32.0485°, 118.778969° 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":32.0485,"lon":118.778969,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

416

The University of Rochester | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Rochester River Campus Rochester River Campus Research Research at Rochester Synergy Centers & Institutes Medical Center Hajim School of Engineering and Applied Sciences Big Data at the University of Rochester Student Contributions to Research Nobel Laureates associated with UR & DOE DOE Research Reports Featured Research: High Energy Density Plasma Science DOE's Office of Fusion Energy Sciences supports basic research at the University of Rochester Fusion Science Center to explore and control the properties of magnetic fields in high energy density plasmas. Read more. Omega Laser Facility * Laboratory for Laser Energetics DOE National Nuclear Security Administration Search this site: Search The University is a vibrant center for discovery and innovation, with researchers engaged in cutting-edge work across the humanities,

417

DOE Solar Decathlon: Purdue University  

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

Purdue University Purdue University Purdue University's INhome-short for Indiana home-earned an overall second-place finish at the U.S. Department of Energy Solar Decathlon 2011. After the competition, the house was relocated to Chatham Square, a new housing development in Lafayette, Indiana, that is part of a broader neighborhood revitalization effort. The house is unchanged from its Solar Decathlon configuration except that the garage was moved to the opposite side of the house to accommodate the shape of the lot. The house was on display throughout 2012 and is currently offered for sale. The INhome provides a realistic and balanced vision for ultra-efficient housing. It is fully functional yet practical and features efficient systems and sustainable design without sacrificing modern comforts and

418

DOE Solar Decathlon: Stanford University  

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

Stanford University Stanford University Start.Home solardecathlon.stanford.edu For the U.S. Department of Energy Solar Decathlon 2013, Stanford University designed the Start.Home to provide energy efficiency at the push of a button to a new generation of environmentally conscious occupants. With modular architecture and advanced controls to optimize each component, the house aims to spark a revolution by lowering the entry barrier for an ultra-efficient house and making sustainability trendy, social, and affordable. Design Philosophy The Start.Home is built on a simple, three-by-three modular grid and integrates core, public, and private modules as well as multiple technologies to optimize value and energy efficiency. These spaces can be added or subtracted to allow the house to grow with the family by filling

419

Bucknell University | Open Energy Information  

Open Energy Info (EERE)

University University Jump to: navigation, search Hydro | Hydrodynamic Testing Facilities Name Bucknell University Address Civil & Mechanical Engineering Departments, Hydraulic Flume, 701 Moore Avenue, Dana Engineering Building Place Lewisburg, PA Zip 17837 Sector Hydro Phone number (570) 577-3193 Website http://www.bucknell.edu/x16287 Coordinates 40.955691952072°, -76.88521027565° 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":40.955691952072,"lon":-76.88521027565,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

420

The Age of the Universe  

E-Print Network (OSTI)

A minimum age of the universe can be estimated directly by determining the age of the oldest objects in the our Galaxy. These objects are the metal-poor stars in the halo of the Milky Way. Recent work on nucleochronology finds that the oldest stars are 15.2+/-3.7 Gyr old. White dwarf cooling curves have found a minimum age for the oldest stars of 8 Gyr. Currently, the best estimate for the age of the oldest stars is based upon the absolute magnitude of the main sequence turn-off in globular clusters. The oldest globular clusters are 11.5+/-1.3 Gyr old, implying a minimum age of the universe of t_universe > 9.5 Gyr (95% confidence level).

Brian Chaboyer

1998-08-19T23:59:59.000Z

Note: This page contains sample records for the topic "university ames ia" 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

Fabrication of Emissible Metallic Layer-by-Layer Photonic ...  

Iowa State University and Ames Laboratory researchers have developed a method for increasing the efficiency of conventional incandescent light bulbs.

422

Mechanochemical Preparation of Phosphonium Salts and ...  

Researchers at Iowa State University and Ames Laboratory have developed a unique, solvent-free mechanochemical preparation method to prepare ...

423

Significance Test in Speaker Recognition Data Analysis with ...  

Science Conference Proceedings (OSTI)

... and Computational Mathematics Division, Information Technology Laboratory, National Institute ... fourth ed., Iowa State University Press, Ames, (1988 ...

2012-10-16T23:59:59.000Z

424

General Phase Transformations - Non-Ferrous: Part III  

Science Conference Proceedings (OSTI)

Mar 5, 2013 ... Location: Henry B. Gonzalez Convention Center Session Chair: Matthew Kramer, Ames Laboratory; Greg Thompson, University of Alabama...

425

The University of WisconsinMadison 9 The University  

E-Print Network (OSTI)

. PHYSICS LIBRARY 4220 Chamberlin Hall 1150 University Avenue, 608­262­9500 physics.library.wisc.edu WENDT LIBRARY 215 N. Randall Avenue, 608­262­3493 wendt.library.wisc.edu This is the primary library for engi

Wisconsin at Madison, University of

426

University Coal Research/Historically Black Colleges and Universities &  

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

University Coal Research/Historically Black Colleges and Universities & Other Minority Institutions Contractor Review Mtg. University Coal Research/Historically Black Colleges and Universities & Other Minority Institutions Contractor Review Mtg. June 3, 2003 Table of Contents Disclaimer Papers and Presentations Day 1 - Session A Day 1 - Session B Day 2 - Session A Day 2 - Session B Posters - Project Accomplishments 2000 Awards Abstracts of 2002 Awards Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government or 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 disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof.

427

University Coal Research / Historically Black Colleges and Universities &  

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

University Coal Research / Historically Black Colleges and Universities & Other Minority Institutions Contractors University Coal Research / Historically Black Colleges and Universities & Other Minority Institutions Contractors Review Meeting June 9-10, 2004 Table of Contents Disclaimer Papers and Presentations Opening Session Session A Session B Abstract Only Abstract & Poster Presentation of Project Accomplishments Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government or 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 disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof.

428

University of New Orleans/1 University Calendar/2  

E-Print Network (OSTI)

& Anthropology, Louisiana State University, Baton Rouge, LA 70803, USA, 11 Potsdam Institute for Climate Impact, and ethanol for 1 hour to remove fat, oil, waxes and resins. This was followed by a series of Acid. of Arch. Sci. 36, 1342­1353 (2009). 30. Luzzadder-Beach, S., Beach, T. P. & Dunning, N. P. Wetland fields

Kulp, Mark

429

24 Universities Receiving Funding to Train Next Generation of...  

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

Bradley University Peoria, IL 999,981 Indiana University Indianapolis, IN 1,323,532 University of Kentucky Research Foundation Lexington, KY 1,500,000 University of...

430

The Universe Adventure - Site Map  

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

Index Pages Index Pages Help Teachers Credits Developers Feedback Links Glossary: A-E | F-J | K-O | P-T | U-Z Fundamentals of Cosmology Cosmology The Beginnings of Cosmology The Ancient Universe The Modern Universe -> Cosmic Conundrums: Cosmology Light The Electromagnetic Spectrum -> Movie: Travelling Photons -> Down the Rabbit Hole: At the Speed of Light -> Classroom Cosmology: The Speed of Light Apparent Magnitude -> Sidequest: Absolute and Apparent Magnitude -> Down the Rabbit Hole: Luminosity versus Observed Brightness -> Down the Rabbit Hole: Standard Candles -> Cosmic Conundrums: Light Matter Blackbody Radiation -> Movie: Temperature Matter and Atoms -> Down the Rabbit Hole: Electric Charge -> Down the Rabbit Hole: Quantum Mechanics -> Cosmic Conundrums: Matter

431

The Age of the Universe  

E-Print Network (OSTI)

Globular clusters are the oldest objects in the Galaxy whose age may be accurately determined. As such globular cluster ages provide the best estimate for the age of the universe. The age of a globular cluster is determined by a comparison between theoretical stellar evolution models and observational data. Current uncertainties in the stellar models and age dating process are discussed in detail. The best estimate for the absolute age of the globular clusters is $14.6\\pm 1.7\\,$Gyr. The one-sided, 95\\% confidence limit on the lower age of the universe is $12.2\\,$Gyr.

Brian Chaboyer

1996-05-16T23:59:59.000Z

432

SOFT MATTER INTERFACES (SMI) Group Leader: Elaine DiMasi  

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

Brook University, 3 NIST, 4 Argonne National Laboratory, 5 University of Illinois, 6 Ames Laboratory, 7 University of California, Berkeley TECHNIQUES AND CAPABILITIES...

433

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

434

Universal Parsing Agent - Available Technologies - PNNL  

Search PNNL. PNNL Home; About; Research; Publications; Jobs; News; Contacts; Universal Parsing Agent ...

435

Universal Ownership: Why Environmental Externalities Matter to  

Open Energy Info (EERE)

Universal Ownership: Why Environmental Externalities Matter to Universal Ownership: Why Environmental Externalities Matter to Institutional Investors Jump to: navigation, search Tool Summary Name: Universal Ownership: Why Environmental Externalities Matter to Institutional Investors Agency/Company /Organization: UNEP-Financing Initiative Focus Area: Industry Topics: Co-benefits assessment Resource Type: Lessons learned/best practices Website: www.unepfi.org/fileadmin/documents/universal_ownership.pdf Universal Ownership: Why Environmental Externalities Matter to Institutional Investors Screenshot References: Universal Ownership: Why Environmental Externalities Matter to Institutional Investors[1] Logo: Universal Ownership: Why Environmental Externalities Matter to Institutional Investors Summary "This study assesses the financial implications of unsustainable natural

436

Des Moines Area Community College | .EDUconnections  

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

Ames Laboratory Ames Laboratory is one of DOE's 10 Office of Science world-class research laboratories, located on the Iowa State University campus just 35 miles from the Des Moines Area Community College. Ames Lab is operated by Iowa State University. Ames Laboratory Ames Laboratory is one of DOE's 10 Office of Science world-class research laboratories, located on the Iowa State University campus just 35 miles from the Des Moines Area Community College. Ames Lab is operated by Iowa State University. Scientific Programs Science Undergraduate Laboratory Internships at Ames Lab Pre-Service Teacher Program DOE Ames Lab Faculty and Student Program (FaST) DOE Ames Lab Community College Institute Program Des Moines Area Community College Des Moines Area Community College Des Moines, Iowa DOE Applauds DMACC's Science and Technical Programs Agri/Natural Resources Biology Biomass Operations Biotechnology Environmental Science Information Technology Manufacturing Technology Microcomputers Civil Engineering Pre-Medical Telecommunications

437

Action Plan UNIVERSITY OF MISSOURI  

E-Print Network (OSTI)

, financially and philosophically, to a carbon-neutral future. Since the signing, he and the university have sustainability. Additional Strategies and Projects Transportation Currently, transportation accounts for less, transportation will play a larger role in its greenhouse gas profile. The Climate Action Plan recommends

Taylor, Jerry

438

Universal service and disabled people  

Science Conference Proceedings (OSTI)

The EU regulatory framework enacted 25 May 2011 has the objective to provide functionally equal access to telecommunication services for disabled persons. What are the rules, who are the target groups, and what obstacles do they face when using various ... Keywords: Disabled people, European regulation, Relay services, Universal service

Nico van Eijk; Joost Poort

2012-03-01T23:59:59.000Z

439

FLORIDA STATE UNIVERSITY Procedures for  

E-Print Network (OSTI)

will be required that describes the purpose for the costs and the direct benefit to the proposed project's scopeFLORIDA STATE UNIVERSITY Procedures for Participant Support Costs Effective: May 15, 2006 Budgeting for Participant Costs Whenever Participant Support Costs are proposed in a budget, a detailed justification

Weston, Ken

440

UNIVERSITY OF CALIFORNIA Los Angeles  

E-Print Network (OSTI)

: Results of parity checker training tion builds a small network up instead of whittling a huge network down. Antsaklis Department of Electrical Engineering University of Notre Dame Notre Dame, IN 46556 Abstract An algorithm for constructing and training multilayer neural networks, dependence identification,is presented

Rennels, David A.

Note: This page contains sample records for the topic "university ames ia" 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

What's informatics at Indiana University?  

Science Conference Proceedings (OSTI)

This Indiana University School of Informatics was the first of its kind in the United States (2000). It includes programs in Bloomington and at IUPUI in Indianapolis. The School has developed a unique undergraduate curriculum that allows students to ... Keywords: bioinformatics, chemical informatics, computing, human-computer interaction/design, informatics, media arts and science, security

James Shea

2009-10-01T23:59:59.000Z

442

Graduate Seminar University of Regina  

E-Print Network (OSTI)

University of Regina Title: On the energy of graphs Date: Tuesday December 1, 2009 Time: 1:00 p.m. Place: Math & Stats Lounge (CW 307.20) Abstract The concept of the energy of a graph was defined by Ivan Gutman in 1978 and originates from theoretical chemistry. To determine the energy of a graph, we

Argerami, Martin

443

GEORGETOWN UNIVERSITY FINANCIAL AFFAIRS MANUAL  

E-Print Network (OSTI)

: A. Employees are encouraged to utilize the preferred University partnership with Anthony Travel when destination and the specific travel dates, noting that the boarding pass was lost; and b) there is a hotel or other third party receipt supporting the person's trip. The traveler must provide the hotel bill

Riesenhuber, Maximilian

444

WASTE DISPOSAL SECTION CORNELL UNIVERSITY  

E-Print Network (OSTI)

2/07 WASTE DISPOSAL SECTION CORNELL UNIVERSITY PROCEDURE for DISPOSAL of RADIOACTIVE MATERIALS This procedure has been developed to ensure the safety of those individuals who handle radioactive waste identified hazardous waste, or other unusual issues require special consideration. Contact the Department

Manning, Sturt

445

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.

446

Per Capita Consumption The NMFS calculation of per capita consumption is  

E-Print Network (OSTI)

351 Bessey Hall, Ames, IA 50011, USA 2 Azerbaijan National Academy of Sciences Patamdar 40, Baku AZ1073, Azerbaijan 3 Southern Research Station, USDA Forest Service Athens, GA 30602, USA Abstract

447

Biology, History, Status and Conservation of Sacramento Perch, Archoplites interruptus  

E-Print Network (OSTI)

of freshwater fishery biology. Vol. II. Ames (IA): IowaWassmann Journal of Biology 24:141–160. Cook SJ, Philippmacrochirus. Invasion Biology 1:55-65. Mathews SB. 1962. The

Crain, Patrick K; Moyle, Peter B

2011-01-01T23:59:59.000Z

448

The Universe Adventure - Galaxial Motion  

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

Bulk Motions of Galaxies Bulk Motions of Galaxies Galaxy Diagram The Structure of a typical Spiral Galaxy. Galaxies are most often found in clusters and are thus subject to gravitational forces from their neighbors. The relative motion that results from these interactions causes deviations from the cosmological principle called bulk flow. Measuring the peculiar velocities enables cosmologists to calculate the masses of interacting galaxies. Using this technique scientists can estimate the total density of matter in the Universe. During the recombination epoch, the Universe had cooled sufficiently for nucleosynthesis to occur. However, this process produces only a few elements, and looking at the abundance of these elements today is indicative of the rate of nucleosynthesis and the amount of baryonic mass

449

The Universe Adventure - Dark Energy  

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

Energy Energy Dark Energy An artist's conception of Dark Energy. Imagine you toss an apple straight up into the air. Due to gravity, one would expect the apple to come right back down to earth. But what if it doesn't? What if, due to some unseen force your apple continues going up, at an accelerated rate, no matter how much gravity pleads and begs for the apple to come back down. Could this really happen? Could there really be "anti-gravity?" On the scale of the Universe, there is; say "hello" to Dark Energy. In the most basic sense, Dark Energy is akin to negative gravity. Where gravity is attractive, Dark Energy is repulsive. Dark Energy causes the Universe to expand at an increasing rate. For example, to a viewer on earth, gravity would attract a distant galaxy towards Earth, but Dark

450

Oak Ridge Associated Universities II  

Office of Legacy Management (LM)

Prepared by Prepared by Oak Ridge Associated Universities II Prepared for Division of Fuel - Cycle and Material Safety II U.S. Nuclear Regulatory Commission L RADIOLOGICAL SURVEY OF THE W. R. GRACE PROPERTY WAYNE, NEW JERSEY P. W. FRAME Radiological Site Assessment Program Manpower Education, Research, and Training Division FINAL REPORT January 1983 RADIOLOGICAL SURVEY OF THE W.R. GRACE PROPERTY WAYNE, NEW JERSEY Prepared for Division of Fuel Cycle and Material Safety U.S. Nuclear Regulatory Commission P. W. Frame Project Staff J. D. Berger A. J. Liu R. D. Condra A. M. Pitt G. R. Foltz T. J. Sowell J. R. Frazier C. F. Weaver R. C. Gentry T. S. Yoo Prepared by Radiological Site Assessment Program Manpower Education, Research, and Training Division Oak Ridge Associated Universities

451

The Universe Adventure - Fundamental Particles  

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

Fundamental Particles Fundamental Particles Chart of Fundamental Particles All matter in the universe is comprised of fundamental particles. So what exactly makes up this matter? All matter is made of fundamental particles that came into being at the birth of the Universe. Quarks experience the strong force which is carried by massless particles called gluons. They bond together in specific combinations to form protons, neutrons, and other hadrons. Leptons do not experience the strong force but may interact via the electromagnetic force, the weak force, or both. Anti-quarks and anti-leptons are exactly the same as their quark and lepton counterparts, but have an opposite charge. All massive particles are influenced by the force of gravity. Quark-Gluon Plasma: 10-12 Seconds After the Big Bang

452

The University of Maryland | .EDUconnections  

Office of Scientific and Technical Information (OSTI)

Maryland Maryland Research Division of Research Centers and Institutes Energy Research Climate Adaption Research National Security Research Faces of Research Nobel Laureates associated with UMD & DOE DOE Research Results Nanostructures for Electrical Energy Storage (NEES) The University of Maryland's NEES is a multi-institutional research center, one of 46 Energy Frontier Research Centers (EFRC) established by the U.S. Department of Energy. The group's focus is developing highly ordered nanostructures that offer a unique testbed for investigating the underpinnings of storing electrical energy. Search this site: Search Founded in 1856, the University of Maryland is Maryland's flagship institution and plays a leadership role as one of the country's premier centers for academic scholarship and research.

453

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. '

454

The age of the universe  

Science Conference Proceedings (OSTI)

An overview of the current controversy on the age of the universe is presented. It is shown that the age of the oldest star, globular clusters, yields an age estimate of approximately 14 {+-} 2 {+-} 2 Gyr (where the first {+-} is statistical and the second systematic, and the two should {ital not} be added in quadrature), with a firm lower bound of {ge} 10 Gyr. It is shown how radioactive dating, nucleocosmochronology, also yields a firm lower bound of {approx_gt} 10 Gyr. The currently favored values for the Hubble constant, when converted to ages using a cosmological model with zero cosmological constant, are shown {ital not} to be in conflict with statistical and systematic uncertainties at the present time when one takes both into account, even for critical density universes. 25 refs. , 3 figs., 1 tab.

Schramm, D.N.

1996-10-01T23:59:59.000Z

455

A map of the universe  

SciTech Connect

We have produced a new conformal map of the universe illustrating recent discoveries, ranging from Kuiper belt objects in the Solar system, to the galaxies and quasars from the Sloan Digital Sky Survey. This map projection, based on the logarithm map of the complex plane, preserves shapes locally, and yet is able to display the entire range of astronomical scales from the Earth s neighborhood to the cosmic microwave background. The conformal nature of the projection, preserving shapes locally, may be of particular use for analyzing large scale structure. Prominent in the map is a Sloan Great Wall of galaxies 1.37 billion light years long, 80 percent longer than the Great Wall discovered by Geller and Huchra and therefore the largest observed structure in the universe.

Gott III, J. Richard; Juric, Mario; Schlegel, David; Hoyle, Fiona; Vogeley, Michael; Tegmark, Max; Bahcall, Neta; Brinkmann, Jon

2003-10-20T23:59:59.000Z

456

Millersville University Health Services Health Form Instructions Millersville University Health Services is dedicated  

E-Print Network (OSTI)

laboratories as ordered by a medical provider. Health Services works cooperatively with Quest, ACM, and CDDMillersville University Health Services Health Form Instructions Millersville University Health, and health education. Health Services Information Millersville University Health Services is centrally

Hardy, Christopher R.

457

University Reciprocating Engine Program Review  

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

University Reciprocating Engine Program Review University Reciprocating Engine Program Review April 9-10, 2003 Table of Contents Disclaimer Papers and Presentations Meeting Overview & Outcomes [PDF-192KB] Agenda [PDF-143KB] DOE/EERE/DER Natural Gas Reciprocating Engines Program The Advanced University Reciprocating Engine Research Program (AUREP) is a Distributed Energy Resources (DER) Program managed within DOE's Office of Energy Efficiency and Renewable Energy (EERE). Click on the link above to find abundant information on the natural gas reciprocating engine program (Technology Primer, Related Programs, Documents & Resources, News & Events, Solicitations and the DER Site Map). Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government or 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 disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof.

458

Page 430 The California State University Sonoma State University 2012-2013 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY  

E-Print Network (OSTI)

Page 430 The California State University Sonoma State University 2012-2013 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY EX OFFICIO TRUSTEES The Honorable Edmund G. Brown, Jr. Governor of California The Honorable Gavin Newsom Lieutenant Governor of California The Honorable John Pérez Speaker of the Assembly

Ravikumar, B.

459

Page 430 The California State University Sonoma State University 2011-2012 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY  

E-Print Network (OSTI)

Page 430 The California State University Sonoma State University 2011-2012 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY EX OFFICIO TRUSTEES The Honorable Edmund G. Brown, Jr. State Capitol Governor of California Sacramento 95814 The Honorable Gavin Newsom State Capitol Lieutenant Governor of California

Ravikumar, B.

460

The California State University Page 429Sonoma State University 2008-2010 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY  

E-Print Network (OSTI)

The California State University Page 429Sonoma State University 2008-2010 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY EX OFFICIO TRUSTEES The Honorable Arnold Schwarzenegger State Capitol Governor of California Sacramento 95814 The Honorable John Garamendi State Capitol Lieutenant Governor of California

Ravikumar, B.

Note: This page contains sample records for the topic "university ames ia" 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

Page 426 The California State University Sonoma State University 2010-2011 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY  

E-Print Network (OSTI)

Page 426 The California State University Sonoma State University 2010-2011 Catalog TRUSTEES OF THE CALIFORNIA STATE UNIVERSITY EX OFFICIO TRUSTEES The Honorable Arnold Schwarzenegger State Capitol Governor of California Sacramento 95814 The Honorable John Garamendi State Capitol Lieutenant Governor of California

Ravikumar, B.

462

University students' satisfaction of studying in e-university: Hamdan Bin Mohammed e-University case study  

Science Conference Proceedings (OSTI)

E-learning is a new trend in vibrant educational environment. The study method is unique as it allows learners to get education interactively through extensive use of information technology and web based technology. Many universities such as University ... Keywords: Hamdan Bin Mohammad e-University, e-learning, evaluation, satisfaction, satisfaction level

Abdullah AlSagheer Hamdan Bin

2011-04-01T23:59:59.000Z

463

DOE Announces $375,000 Grant to Lincoln University and the University...  

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

engineering program. The partnership between Lincoln University, a minority-serving higher education institution in Jefferson City, and the University of Missouri-Rolla...

464

The Catholic University of America, George Washington University, and American University Solar Decathlon 2011 Project Manual  

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

U.S. DEPARTMENT OF ENERGY SOLAR DECATHLON 2013 U.S. DEPARTMENT OF ENERGY SOLAR DECATHLON 2013 PRIMARY FACULTY CONTACT Bill Jelen School of Architecture and Planning The Catholic University of America 620 Michigan Ave., NE Washington, D.C. 20064 jelen@cua.edu (202) 344-5513 PRIMARY STUDENT CONTACT Kyle Noell School of Architecture and Planning The Catholic University of America 620 Michigan Ave., NE Washington, D.C. 20064 91noell@cardinalmail.cua.edu (301) 648-0506 As Built Project Manual 22 August 2013 Harvest Team Capitol dc www.teamcapitoldc.org Construction Documents Project Manual Published 8/22/2013 U.S. D.O.E. Solar Decathlon 2013 Page - 2 TABLE OF CONTENTS Table of Contents .................................................................................................................................................................. 2

465

Nuclear Energy University Program | Department of Energy  

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

Energy University Program Energy University Program Nuclear Energy University Program NEUP Award Recipients FY2009 to FY2013 Click on the icons to find out the values of the awards given to each school. The darker the icon, the more recent the award. Drag and zoom map to see more recipients. Investing in the next generation of nuclear energy leaders and advancing university-led nuclear innovation is vital to fulfilling the Office of Nuclear Energy's (NE) mission. This is accomplished primarily through NE's Nuclear Energy University Programs (NEUP), which was created in 2009 to consolidate university support under one initiative and better integrate university research within NE' technical programs. NEUP engages U.S. colleges and universities to conduct research and development (R&D), enhance infrastructure and support student education

466

California State University, Fullerton EMERGENCY OPERATIONS PLAN  

E-Print Network (OSTI)

California State University, Fullerton EMERGENCY OPERATIONS PLAN Revised March 2012 #12;Foreward The California State University's Emergency Operations Plan (EOP) defines the scope of preparedness and incident Presidential Directive (HSPS5), the National Incident Management System (NIMS), the California Standardized

de Lijser, Peter

467

University of Southern California 2010 -2011  

E-Print Network (OSTI)

University of Southern California 2010 - 2011 Distinguished Lecturer Series Viterbi Keynote Thursday, March 3, 2011 Dr. Elwyn Berlekamp Professor Emeritus University of California, Berkeley of California, Berkeley Wednesday, April 6, 2011 "Markov, Wiener and Shannon: a Progression" Dr. Andrew Viterbi

Safonov, Michael G.

468

1 Introduction - CECM - Simon Fraser University  

E-Print Network (OSTI)

Proof: Let us write r 1; :::; rs for the rows of M. For each row rk of M and each ...... the construction of universal Gr obner bases and universal standard forms. A.

469

Nuclear Energy University Program | Department of Energy  

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

Energy University Program Nuclear Energy University Program NEUP Award Recipients FY2009 to FY2013 Click on the icons to find out the values of the awards given to each school. The...

470

University Programs Listing-Professional Educators  

Science Conference Proceedings (OSTI)

University programs listing in lipids, fats, oils, surfactants and related materials. University Programs Listing-Professional Educators Professional Educators Common Interest Group aocs awards Educators fats global inform job listings member mem

471

Quantum Mechanics and Representation Theory Columbia University  

E-Print Network (OSTI)

Quantum Mechanics and Representation Theory Peter Woit Columbia University Texas Tech, November 21 2013 Peter Woit (Columbia University) Quantum Mechanics and Representation Theory November 2013 1 / 30 #12;Does Anyone Understand Quantum Mechanics? "No One Understands Quantum Mechanics" "I think

Woit, Peter

472

Tel Aviv University | Open Energy Information  

Open Energy Info (EERE)

search Name Tel Aviv University Place Tel Aviv, Israel Zip 69978 Sector Solar Product R&D of solar energy, fuel cells and new materials References Tel Aviv University1...

473

External Program Review University of Idaho  

E-Print Network (OSTI)

7/20/2012 External Program Review University of Idaho Overview 1 Program review, as it is widely that the University of Idaho "exercise the leadership and coordination necessary for periodic program review

Kyte, Michael

474

University Admissions: ValeriePickett,Director  

E-Print Network (OSTI)

University Admissions: ValeriePickett,Director UniversityAdmissions,MSC3A New, Appointed Regent from Clovis for term expiring January 1, 2011. Chris Anaya, Appointed Regent from Moriarty

Castillo, Steven P.

475

NETL Regional University Alliance (NETL-RUA)  

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

About NETL Regional University Alliance (NETL-RUA) About NETL-RUA Integrated Program Team Member Universities History Mission Team Posters PDF-9MB Factsheet PDF-539KB NETL-RUA...

476

University of Ljubljana Faculty of Electrical Engineering  

E-Print Network (OSTI)

calculation for different criteria. Ancillary service management: load forecast, power system reserve forecast#12;2 3 University of Ljubljana Faculty of Electrical Engineering University of Ljubljana Faculty of Electrical Engineering Doctoral Programme Electrical Engineering Doctoral Programme Electrical Engineering

?umer, Slobodan

477

J. Fluid Mech. (2007), vol. 592, pp. 447469. c 2007 Cambridge University Press doi:10.1017/S0022112007008701 Printed in the United Kingdom  

E-Print Network (OSTI)

address: Departamento de Ingenier´ia Aeroespacial y Mec´anica de Fluidos, Universidad de Sevilla, Camino

Gelfond, Michael

478

Steffen Staab University of Koblenz-Landau  

E-Print Network (OSTI)

theory: analysis of conflict. Harvard University Press, Cambridge Nowak A, Szamrej J, Latané B (1990

Golbeck, Jennifer

479

The University of Maryland Energy Research Center  

E-Print Network (OSTI)

.S. ranking in the 2007 DOE Solar Decathlon. The university's campus is a living laboratory of "smartgrid

Gruner, Daniel S.

480

NETL Regional University Alliance (NETL-RUA)  

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

Center for Multiscale Modeling for Engineering Materials Carnegie Mellon University Electricity Industry Center Center for Sustainable Engineering Center for Nanoenabled...

Note: This page contains sample records for the topic "university ames ia" 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

Universal quantum computation with shutter logic  

Science Conference Proceedings (OSTI)

We show that universal quantum logic can be achieved using only linear optics and a quantum shutter device. With these elements, we design a quantum memory for any number of qubits and a CNOT gate which are the basis of a universal quantum computer. ... Keywords: interaction-free measurement, optical CNOT gate, optical quantum computation, quantum interrogation, quantum memory, quantum shutter, universal quantum computer

Juan Carlos Garca-Escartn; Pedro Chamorro-Posada

2006-09-01T23:59:59.000Z

482

CALIFORNIA IGETC EQUIVALENCIES TO BINGHAMTON UNIVERSITY  

E-Print Network (OSTI)

CALIFORNIA IGETC EQUIVALENCIES TO BINGHAMTON UNIVERSITY OF THE STATE UNIVERSITY OF NEW YORK GENERAL of courses that prospective transfer students attending California Community Colleges may complete to satisfy the lower-division breadth and general education requirements at both the University of California

Suzuki, Masatsugu

483

Energy Research at the University of Regina  

E-Print Network (OSTI)

Energy Research at the University of Regina The University of Regina has long understood, there was recognition that the availability of energy is fundamental to that growth. For these reasons, the University made energy (as a part of energy and environment) one of its thematic research areas in 2000

Argerami, Martin

484

Texas Tech University Department of Chemical Engineering  

E-Print Network (OSTI)

Texas Tech University Department of Chemical Engineering Lubbock, TX 79409-3121 Application degree at Texas Tech University ____________________________________ Che E specialties and skills to which I am applying at Texas Tech University as a part of the application. If my application

Zhang, Yuanlin

485

HOCHSCHULE ESSLINGEN: University of Applied Sciences  

E-Print Network (OSTI)

and Electrical Engineering Social work, health and nursing Building services, energy and environmental and Electrical Engineering Automation Systems / Software, Field Busses and Networks #12;Automation Systems in university rankings. For more information about the university, visit http://www.hs-esslingen.de/en/the-university/profile

Duchowski, Andrew T.

486

Table of Contents University Calendar . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .1  

E-Print Network (OSTI)

research uni- versity of the State of Louisiana, was established by the Louisiana Legislature in 1956 of 1958. In September 1958, Louisiana State University in New Orleans, which was renamed the University at http://upcom.uno. edu/docs/StrategicPlan2007-2010.pdf. As a member of the Louisiana State University

Kulp, Mark

487

China Initiatives at Michigan State University  

E-Print Network (OSTI)

China Initiatives at Michigan State University Office of China Programs The Office of International Studies and Programs at Michigan State University established the Office of China Programs in July 2005 to help implement President Lou Anna K. Simon's "China Initiative," part of the university's long

Liu, Taosheng

488

Vertical Contracts and Mandatory Universal Distribution  

E-Print Network (OSTI)

Vertical Contracts and Mandatory Universal Distribution Larry S. Karp Jeffrey M. Perloff July 2012 vendor. If a monopoly uses a single vendor, the government may impose a mandatory universal distribution consumer welfare. Keywords: vertical restrictions, mandatory universal distribution, new product oligopoly

Kammen, Daniel M.

489

Universality in Pure Gravity Mediation  

E-Print Network (OSTI)

If low energy supersymmetry is realized in nature, the apparent discovery of a Higgs boson with mass around 125 GeV points to a supersymmetric mass spectrum in the TeV or multi-TeV range. Multi-TeV scalar masses are a necessary component of supersymmetric models with pure gravity mediation or in any model with strong moduli stabilization. Here, we show that full scalar mass universality remains viable as long as the ratio of Higgs vevs, tan beta is relatively small (\\lesssim 2.5). We discuss in detail the low energy (observable) consequences of these models.

Jason L. Evans; Masahiro Ibe; Keith A. Olive; Tsutomu T. Yanagida

2013-02-21T23:59:59.000Z

490

Research universities for the 21st century  

SciTech Connect

The `public outcomes` from research universities are educated students and research that extends the frontiers of knowledge. Measures of these `public outcomes` are inadequate to permit either research or education consumers to select research universities based on quantitative performance data. Research universities annually spend over $20 billion on research; 60% of these funds are provided by Federal sources. Federal funding for university research has recently grown at an annual rate near 6% during a time period when other performers of Federal research have experienced real funding cuts. Ten universities receive about 25% of the Federal funds spent on university research. Numerous studies of US research universities are reporting storm clouds. Concerns include balancing research and teaching, the narrow focus of engineering education, college costs, continuing education, and public funding of foreign student education. The absence of research on the `public outcomes` from university research results in opinion, politics, and mythology forming the basis of too many decisions. Therefore, the authors recommend studies of other nations` research universities, studies of various economic models of university research, analysis of the peer review process and how well it identifies the most capable research practitioners and at what cost, and studies of research university ownership of intellectual property that can lead to increased `public outcomes` from publicly-funded research performed by research universities. They advocate two practices that could increase the `public outcomes` from university research. These are the development of science roadmaps that link science research to `public outcomes` and `public outcome` metrics. Changes in the university research culture and expanded use of the Internet could also lead to increased `public outcomes`. They recommend the use of tax incentives to encourage companies to develop research partnerships with research universities.

Gover, J. [Sandia National Labs., Albuquerque, NM (United States)] [Sandia National Labs., Albuquerque, NM (United States); Huray, P.G. [Univ. of South Carolina, Columbia, SC (United States)] [Univ. of South Carolina, Columbia, SC (United States)

1998-05-01T23:59:59.000Z

491

BIG IDEAS FOR JOB CREATIOn A PROJECT OF ThE UnIvERSITy OF CALIFORnIA, BERKELEy AnD ThE AnnIE E. CASEy FOUnDATIOn  

E-Print Network (OSTI)

businesses generate more jobs. · Developing new jobs in emerging or resurgent sectors, such as clean energy-skilled workers. We sought to avoid gimmicks (such as one-time budget transfers), as well as wasteful incentive

California at Berkeley, University of

492

Oak Ridge Associated Universities Procurement Questionnaire Application  

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

Associated Universities Procurement Questionnaire Associated Universities Procurement Questionnaire Application System Supplier Profile PIA, Oak ridge Operations Office Oak Ridge Associated Universities Procurement Questionnaire Application System Supplier Profile PIA, Oak ridge Operations Office Oak Ridge Associated Universities Procurement Questionnaire Application System Supplier Profile PIA, Oak ridge Operations Office Oak Ridge Associated Universities Procurement Questionnaire Application System Supplier Profile PIA, Oak ridge Operations Office More Documents & Publications Occupational Medical Surveillance System (OMSS) PIA, Idaho National Laboratory Occupational Medicine - Assistant PIA, Idaho National Laboratory ORO Verification of Employment Tracking System(VETS) PIA, Oak ridge Operations Office