Sample records for astrophysics division nsd

  1. NASA/TM-2013-217509 Goddard's Astrophysics Science Division Annual Report 2012

    E-Print Network [OSTI]

    Christian, Eric

    : NASAAccess Help Desk NASA Center for AeroSpace Information 7115 Standard Drive Hanover, MD 21076 #12;NASA Royal Road Hanover, MD 21076-1320 Springfield, VA 22161 #12;Astrophysics Science Division Annual Report

  2. astrophysics science division: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Robert Fefferman, Dean Chemistry Websites Summary: & Astrophysics, Chemistry, Computer Science, Geophysical Sciences, Mathematics, Physics, and Statistics. It also Astronomyand...

  3. NSD Methodology Report | Department of Energy

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagement ofConverDyn NOPR ConverDyn NOPR ConverDyn2DepartmentNSD

  4. Nuclear Science Division, 1995--1996 annual report

    SciTech Connect (OSTI)

    Poskanzer, A.M. [ed.

    1997-02-01T23:59:59.000Z

    This report describes the activities of the Nuclear Science Division (NSD) for the two-year period, January 1, 1995 to January 1, 1997. This was a time of major accomplishments for all research programs in the Division-many of which are highlighted in the reports of this document.

  5. Nuclear Systems Design and Analysis (NSD&A) Division | Department of Energy

    Office of Environmental Management (EM)

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  6. The Status and future of ground-based TeV gamma-ray astronomy. A White Paper prepared for the Division of Astrophysics of the American Physical Society

    E-Print Network [OSTI]

    Buckley, J; Dingus, B; Falcone, A; Kaaret, Philip; Krawzcynski, H; Pohl, M; Vasilev, V; Williams, D A

    2008-01-01T23:59:59.000Z

    In recent years, ground-based TeV gamma-ray observatories have made spectacular discoveries including imaging spectroscopy observations of galactic sources of different classes, and the discovery of rapid gamma-ray flares from radio galaxies and active galactic nuclei containing supermassive black holes. These discoveries, and the fact that gamma-ray astronomy has the potential to map the radiation from dark matter annihilation in our Galaxy and in extragalactic systems, have attracted the attention of the wider scientific community. The Division of Astrophysics of the American Physical Society requested the preparation of a white paper on the status and future of ground-based gamma-ray astronomy to define the science goals of a future observatory, to determine the performance specifications, to identify the areas of necessary technology development, and to lay out a clear path for proceeding beyond the near term. The white paper was written with broad community input, including discussions on several dedicat...

  7. Birth of Neutrino Astrophysics

    ScienceCinema (OSTI)

    None

    2011-10-06T23:59:59.000Z

    Based mainly on the results of two experiments, KamiokaNDE and Super-KamiokaNDE, the birth of neutrino astrophysics will be described. At the end, the result of the third generation Kamioka experiment, KamLAND, will be discussed together with the future possibilities.Organiser(s): Daniel Treille / EP DivisionNote: * Tea & coffee will be served at 16:00 hrs. Please note unusual day.

  8. The Status and future of ground-based TeV gamma-ray astronomy. A White Paper prepared for the Division of Astrophysics of the American Physical Society

    E-Print Network [OSTI]

    J. Buckley; K. Byrum; B. Dingus; A. Falcone; P. Kaaret; H. Krawzcynski; M. Pohl; V. Vassiliev; D. A. Williams

    2008-10-02T23:59:59.000Z

    In recent years, ground-based TeV gamma-ray observatories have made spectacular discoveries including imaging spectroscopy observations of galactic sources of different classes, and the discovery of rapid gamma-ray flares from radio galaxies and active galactic nuclei containing supermassive black holes. These discoveries, and the fact that gamma-ray astronomy has the potential to map the radiation from dark matter annihilation in our Galaxy and in extragalactic systems, have attracted the attention of the wider scientific community. The Division of Astrophysics of the American Physical Society requested the preparation of a white paper on the status and future of ground-based gamma-ray astronomy to define the science goals of a future observatory, to determine the performance specifications, to identify the areas of necessary technology development, and to lay out a clear path for proceeding beyond the near term. The white paper was written with broad community input, including discussions on several dedicated open meetings, and a number of APS or other conferences. It contains an executive summary, detailed reports from the science working groups, and appendices with supplementary material including the full author lists for the different sections of the white paper and a glossary.

  9. Physics division annual report 2006.

    SciTech Connect (OSTI)

    Glover, J.; Physics

    2008-02-28T23:59:59.000Z

    This report highlights the activities of the Physics Division of Argonne National Laboratory in 2006. The Division's programs include the operation as a national user facility of ATLAS, the Argonne Tandem Linear Accelerator System, research in nuclear structure and reactions, nuclear astrophysics, nuclear theory, investigations in medium-energy nuclear physics as well as research and development in accelerator technology. The mission of nuclear physics is to understand the origin, evolution and structure of baryonic matter in the universe--the core of matter, the fuel of stars, and the basic constituent of life itself. The Division's research focuses on innovative new ways to address this mission.

  10. Particle Astrophysics

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

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  11. Nuclear Astrophysics

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItemResearch > TheNuclear Astrophysics One of the great scientific challenges is

  12. Physics Division activities report, 1986--1987

    SciTech Connect (OSTI)

    Not Available

    1987-01-01T23:59:59.000Z

    This report summarizes the research activities of the Physics Division for the years 1986 and 1987. Areas of research discussed in this paper are: research on e/sup +/e/sup /minus// interactions; research on p/bar p/ interactions; experiment at TRIUMF; double beta decay; high energy astrophysics; interdisciplinary research; and advanced technology development and the SSC.

  13. NSD Methodology Report

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn'tOrigin of Contamination in Many Devils Wash,Energy NREL Job TaskWelcome RemarksNational

  14. Division of Finance Division of Finance Alignment

    E-Print Network [OSTI]

    Hayden, Nancy J.

    Division of Finance Division of Finance Alignment September 11, 2014 1 #12;Division of Finance of Finance Goal of the DF Alignment Project The internal and external alignment of the Division of Finance of Finance The Process We Followed 17 Meetings17 Meetings 120+ Pages of Data 103 Themes 12 Meta Themes Goals

  15. High energy astrophysical processes

    E-Print Network [OSTI]

    Todor Stanev

    2005-04-18T23:59:59.000Z

    We briefly review the high energy astrophysical processes that are related to the production of high energy $\\gamma$-ray and neutrino signals and are likely to be important for the energy loss of high and ultrahigh energy cosmic rays. We also give examples for neutrino fluxes generated by different astrophysical objects and describe the cosmological link provided by cosmogenic neutrinos.

  16. Superconducting Magnet Division

    E-Print Network [OSTI]

    Superconducting Magnet Division DOE NP Program Review - July 06 1 Brookhaven Magnet Division - Nuclear Physics Program Support Activities Superconducting Magnet Program RHIC Operations Support Spin Summary Peter Wanderer, DOE review, July 25, 2006 Acting Head, Superconducting Magnet Division #12

  17. Finance Division Employee Status Form Finance Division

    E-Print Network [OSTI]

    Crews, Stephen

    Finance Division Employee Status Form Finance Division CB 1225, 104 Airport Drive Chapel Hill, NC Phone: 919-962-7242 finance.unc.edu Failure to Follow Instructions Below Will Delay Processing Today information in five areas: 1. Division-wide emergency call tree 2. Finance Web site contacts 3. Departmental

  18. Astrophysical Models, and

    E-Print Network [OSTI]

    Wargelin, Bradford J.

    correspondientes, faltantes los modelos. Nuestras medidas tambiâ??en permiten determinar la exactitud c astrophysically relevant L­shell x­ray spectra because these emanate from colder regions the plasma

  19. RESEARCH UPDATE Ecology Division

    E-Print Network [OSTI]

    1 RESEARCH UPDATE Ecology Division Biotype has changed its name to Ecotype! Following the re-organisation of Forest Research into five science Divisions and three Support Divisions, the former Woodland Ecology Branches to form the new Ecology Division. We decided to give the divisional newsletter a new name (and

  20. Nuclear & Particle Physics, Astrophysics, Cosmology

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Nuclear & Particle Physics science-innovationassetsimagesicon-science.jpg Nuclear & Particle Physics, Astrophysics, Cosmology National security depends on science and...

  1. Physics division annual report 2005.

    SciTech Connect (OSTI)

    Glover, J.; Physics

    2007-03-12T23:59:59.000Z

    This report highlights the research performed in 2005 in the Physics Division of Argonne National Laboratory. The Division's programs include operation of ATLAS as a national user facility, nuclear structure and reaction research, nuclear theory, medium energy nuclear research and accelerator research and development. The mission of Nuclear Physics is to understand the origin, evolution and structure of baryonic matter in the universe--the matter that makes up stars, planets and human life itself. The Division's research focuses on innovative new ways to address this mission and 2005 was a year of great progress. One of the most exciting developments is the initiation of the Californium Rare Ion Breeder Upgrade, CARIBU. By combining a Cf-252 fission source, the gas catcher technology developed for rare isotope beams, a high-resolution isobar separator, and charge breeding ECR technology, CARIBU will make hundreds of new neutron-rich isotope beams available for research. The cover illustration shows the anticipated intensities of low-energy beams that become available for low-energy experiments and for injection into ATLAS for reacceleration. CARIBU will be completed in early 2009 and provide us with considerable experience in many of the technologies developed for a future high intensity exotic beam facility. Notable results in research at ATLAS include a measurement of the isomeric states in {sup 252}No that helps pin down the single particle structure expected for superheavy elements, and a new low-background measurement of {sup 16}N beta-decay to determine the {sup 12}C({alpha},{gamma}){sup 16}O reaction rate that is so important in astrophysical environments. Precise mass measurements shed new light on the unitarity of the quark weak-mixing matrix in the search for physics beyond the standard model. ATLAS operated for 4686 hours of research in FY2005 while achieving 95% efficiency of beam delivery for experiments. In Medium-Energy Physics, radium isotopes were trapped in an atom trap for the first time, a major milestone in an innovative search for the violation of time-reversal symmetry. New results from HERMES establish that strange quarks carry little of the spin of the proton and precise results have been obtained at JLAB on the changes in quark distributions in light nuclei. New theoretical results reveal that the nature of the surfaces of strange quark stars. Green's function Monte Carlo techniques have been extended to scattering problems and show great promise for the accurate calculation, from first principles, of important astrophysical reactions. Flame propagation in type 1A supernova has been simulated, a numerical process that requires considering length scales that vary by factors of eight to twelve orders of magnitude. Argonne continues to lead in the development and exploitation of the new technical concepts that will truly make an advanced exotic beam facility, in the words of NSAC, 'the world-leading facility for research in nuclear structure and nuclear astrophysics'. Our science and our technology continue to point the way to this major advance. It is a tremendously exciting time in science for these new capabilities hold the keys to unlocking important secrets of nature. The great progress that has been made in meeting the exciting intellectual challenges of modern nuclear physics reflects the talents and dedication of the Physics Division staff and the visitors, guests and students who bring so much to the research.

  2. Division of Agriculture,

    E-Print Network [OSTI]

    Ray, David

    DAFVM Division of Agriculture, Forestry, and Veterinary M e d i c i n e Visit us online at www to the Mississippi State University Division of Agriculture, Forestry, and Veterinary Medicine. Discrimination based-3-14) Mississippi State University's Division of Agriculture, Forestry, and Veterinary Medicine, or DAFVM

  3. DIVISION OF GRADUATE STUDIES

    E-Print Network [OSTI]

    Palffy-Muhoray, Peter

    recipients at the time of their graduation to monitor and project the scientific workforce. Between 1961DIVISION OF GRADUATE STUDIES 2012-2013 ACADEMIC YEAR REpORT Excellence in Action Division of Graduate Studies #12;Division of Graduate Studies Kent State University 2012 - 2013 Academic Year Report

  4. Physics Division: Annual report, 1 January-31 December 1985

    SciTech Connect (OSTI)

    Not Available

    1987-05-01T23:59:59.000Z

    This report summarizes the research programs of the Physics Division of the Lawrence Berkeley Laboratory during calendar 1985. The Division's principal activities are research in theoretical and experimental high energy physics, and the development of tools such as sophisticated detectors to carry out that research. The physics activity also includes a program in astrophysics, and the efforts of the Particle Data Group whose compilations serve the worldwide high energy physics community. Finally, in addition to the physics program, there is a smaller but highly significant research effort in applied mathematics. Some specific topics included in this report are: Research on e/sup +/e/sup -/ annihilation, superconducting super collider, double beta decay, high energy astrophysics and interdisciplinary experiments, detector research and development, electroweak interactions, strong interaction, quantum field theory, superstrings and quantum gravity, vortex methods and turbulence and computational mathematics.

  5. Strangeness in Relativistic Astrophysics

    E-Print Network [OSTI]

    Jurgen Schaffner-Bielich; Stefan Schramm; Horst Stocker

    2007-11-16T23:59:59.000Z

    In these lecture notes, the role of strangeness in relativistic astrophysics of compact stars is addressed. The appearance of strange particles, as hyperons, kaons, and strange quarks, in the core of compact stars is examined and common features as well as differences are presented. Impacts on the global properties of compact stars and signals of the presence of exotic matter are outlined for the various strange phases which can appear in the interior at high densities.

  6. Astrophysics Visual Analytics at NERSC

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Our current understanding of dark energy comes primarily from the study of supernovae. The Nearby Supernova Factory (SNfactory) is an international astrophysics...

  7. What physics and astronomy courses Astrophysics

    E-Print Network [OSTI]

    Sussex, University of

    Essentials What physics and astronomy courses are there? MPhys Astrophysics Physics Physics (research placement) Physics with Astrophysics Theoretical Physics BSc Physics Physics with Astrophysics Theoretical Physics Foundation year for UK and EU students Physics and Astronomy degrees (with a foundation

  8. Argonne Physics Division - ATLAS

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    ATLAS Operations personnel, and to various experimental instrument specialists in the Physics Division. The PAC members will review each proposal for scientific merit and...

  9. astrophysics: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    neutrino cooling and associated limits on neutrino properties; and high-energy astrophysical neutrinos. W. C. Haxton 2012-09-17 3 Nuclear astrophysics CiteSeer...

  10. Nuclear and particle physics, astrophysics and cosmology (NPAC) capability review

    SciTech Connect (OSTI)

    Redondo, Antonio [Los Alamos National Laboratory

    2010-01-01T23:59:59.000Z

    The present document represents a summary self-assessment of the status of the Nuclear and Particle Physics, Astrophysics and Cosmology (NPAC) capability across Los Alamos National Laboratory (LANL). For the purpose of this review, we have divided the capability into four theme areas: Nuclear Physics, Particle Physics, Astrophysics and Cosmology, and Applied Physics. For each theme area we have given a general but brief description of the activities under the area, a list of the Laboratory divisions involved in the work, connections to the goals and mission of the Laboratory, a brief description of progress over the last three years, our opinion of the overall status of the theme area, and challenges and issues.

  11. Nuclear Masses in Astrophysics

    E-Print Network [OSTI]

    Christine Weber; Klaus Blaum; Hendrik Schatz

    2008-12-09T23:59:59.000Z

    Among all nuclear ground-state properties, atomic masses are highly specific for each particular combination of N and Z and the data obtained apply to a variety of physics topics. One of the most crucial questions to be addressed in mass spectrometry of unstable radionuclides is the one of understanding the processes of element formation in the Universe. To this end, accurate atomic mass values of a large number of exotic nuclei participating in nucleosynthesis are among the key input data in large-scale reaction network calculations. In this paper, a review on the latest achievements in mass spectrometry for nuclear astrophysics is given.

  12. Astrophysics at NERSC

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItem NotEnergy,ARMForms About BecomeTechnologiesVehicle PartsAnnualAstrophysics

  13. Nuclear Science Division annual report, October 1, 1984-September 30, 1985

    SciTech Connect (OSTI)

    Mahoney, J. (ed.)

    1986-09-01T23:59:59.000Z

    This report summarizes the activities of the Nuclear Science Division during the period October 1, 1984 to September 30, 1985. As in previous years, experimental research has for the most part been carried out using three local accelerators, the Bevalac, the SuperHILAC and the 88-Inch Cyclotron. However, during this time, preparations began for a new generation of relativistic heavy-ion experiments at CERN. The Nuclear Science Division is involved in three major experiments at CERN and several smaller ones. The report is divided into 5 sections. Part I describes the research programs and operations, and Part II contains condensations of experimental papers arranged roughly according to program and in order of increasing energy, without any further subdivisions. Part III contains condensations of theoretical papers, again ordered according to program but in order of decreasing energy. Improvements and innovations in instrumentation and in experimental or analytical techniques are presented in Part IV. Part V consists of appendices, the first listing publications by author for this period, in which the LBL report number only is given for papers that have not yet appeared in journals; the second contains abstracts of PhD theses awarded during this period; and the third gives the titles and speakers of the NSD Monday seminars, the Bevatron Research Meetings and the theory seminars that were given during the report period. The last appendix is an author index for this report.

  14. Superconducting Magnet Division

    E-Print Network [OSTI]

    Gupta, Ramesh

    Superconducting Magnet Division Permanent Magnet Designs with Large Variations in Field Strength the residual field of the magnetized bricks by concentrating flux lines at the iron pole. Low Field Design Medium Field Design Superconducting Magnet Division Dipole and Quadrupole Magnets for RHIC e

  15. Hypertension Research Division

    E-Print Network [OSTI]

    Berdichevsky, Victor

    Hypertension & Vascular Research Division Department of Internal Medicine Jeffrey L. Garvin, Ph.D. ­ Division Head #12;Prevalence of Hypertension in U.S. Men by Age and Ethnicity 18 ­ 29 30 ­ 39 40 ­ 49 50 Prevalence of High BP Adapted from Burt et al. Hypertension 1995;25:305. 25 50 75 #12;Introduction

  16. Superconducting Magnet Division

    E-Print Network [OSTI]

    McDonald, Kirk

    Superconducting Magnet Division Ramesh Gupta 20T Target Solenoid with HTS Insert Solenoid Capture Laboratory New York, USA http://www.bnl.gov/magnets/staff/gupta #12;Superconducting Magnet Division Ramesh of HTS may significantly reduce the amount of Tungsten shielding · Summary #12;Superconducting Magnet

  17. Physics Division annual report 2004.

    SciTech Connect (OSTI)

    Glover, J.

    2006-04-06T23:59:59.000Z

    This report highlights the research performed in 2004 in the Physics Division of Argonne National Laboratory. The Division's programs include operation of ATLAS as a national user facility, nuclear structure and reaction research, nuclear theory, medium energy nuclear research and accelerator research and development. The intellectual challenges of this research represent some of the most fundamental challenges in modern science, shaping our understanding of both tiny objects at the center of the atom and some of the largest structures in the universe. A great strength of these efforts is the critical interplay of theory and experiment. Notable results in research at ATLAS include a measurement of the charge radius of He-6 in an atom trap and its explanation in ab-initio calculations of nuclear structure. Precise mass measurements on critical waiting point nuclei in the rapid-proton-capture process set the time scale for this important path in nucleosynthesis. An abrupt fall-off was identified in the subbarrier fusion of several heavy-ion systems. ATLAS operated for 5559 hours of research in FY2004 while achieving 96% efficiency of beam delivery for experiments. In Medium Energy Physics, substantial progress was made on a long-term experiment to search for the violation of time-reversal invariance using trapped Ra atoms. New results from HERMES reveal the influence of quark angular momentum. Experiments at JLAB search for evidence of color transparency in rho-meson production and study the EMC effect in helium isotopes. New theoretical results include a Poincare covariant description of baryons as composites of confined quarks and non-point-like diquarks. Green's function Monte Carlo techniques give accurate descriptions of the excited states of light nuclei and these techniques been extended to scattering states for astrophysics studies. A theoretical description of the phenomena of proton radioactivity has been extended to triaxial nuclei. Argonne continues to lead in the development and exploitation of the new technical concepts that will truly make RIA, in the words of NSAC, ''the world-leading facility for research in nuclear structure and nuclear astrophysics''. The performance standards for new classes of superconducting cavities continue to increase. Driver linac transients and faults have been analyzed to understand reliability issues and failure modes. Liquid-lithium targets were shown to successfully survive the full-power deposition of a RIA beam. Our science and our technology continue to point the way to this major advance. It is a tremendously exciting time in science for RIA holds the keys to unlocking important secrets of nature. The work described here shows how far we have come and makes it clear we know the path to meet these intellectual challenges. The great progress that has been made in meeting the exciting intellectual challenges of modern nuclear physics reflects the talents and dedication of the Physics Division staff and the visitors, guests and students who bring so much to the research.

  18. PHYSICS DIVISION CHEMICAL HYGIENE PLAN

    E-Print Network [OSTI]

    Kemner, Ken

    PHYSICS DIVISION CHEMICAL HYGIENE PLAN 2008 Prepared by _________________________________________________ T. Mullen Physics Division Chemical Hygiene Officer Reviewed by ___________________________________________________ J. Woodring Site Chemical Hygiene Officer Approved

  19. High Energy Astrophysics: Overview 1/47 High Energy Astrophysics in Context

    E-Print Network [OSTI]

    Bicknell, Geoff

    High Energy Astrophysics: Overview 1/47 High Energy Astrophysics in Context 1 Some references The following set of volumes is an outstanding summary of the field of High Energy Astrophysics and its relation to the rest of Astrophysics High Energy Astrophysics, Vols. 1,2 and 3. M.S. Longair, Cam- bridge University

  20. SMITHSONIAN ASTROPHYSICAL OBSERVATORY VISITING COMMITTEE REPORT

    E-Print Network [OSTI]

    's greatest strengths is its high-energy astrophysics group. While the Chandra satellite will likely continue of astrophysics research and prioritize SAO's major new initiatives (e.g., playing a major role in GMT). The VC. Scientific Research Program High Energy Astrophysics The high-energy astrophysics group at CfA is arguably

  1. Theoretical Particle Astrophysics

    SciTech Connect (OSTI)

    Kamionkowski, Marc

    2013-08-07T23:59:59.000Z

    Abstract: Theoretical Particle Astrophysics The research carried out under this grant encompassed work on the early Universe, dark matter, and dark energy. We developed CMB probes for primordial baryon inhomogeneities, primordial non-Gaussianity, cosmic birefringence, gravitational lensing by density perturbations and gravitational waves, and departures from statistical isotropy. We studied the detectability of wiggles in the inflation potential in string-inspired inflation models. We studied novel dark-matter candidates and their phenomenology. This work helped advance the DoE's Cosmic Frontier (and also Energy and Intensity Frontiers) by finding synergies between a variety of different experimental efforts, by developing new searches, science targets, and analyses for existing/forthcoming experiments, and by generating ideas for new next-generation experiments.

  2. Photoneutron reactions in astrophysics

    SciTech Connect (OSTI)

    Varlamov, V. V., E-mail: Varlamov@depni.sinp.msu.ru; Ishkhanov, B. S.; Orlin, V. N.; Peskov, N. N.; Stopani, K. A. [Moscow State University, Skobeltsyn Institute of Nuclear Physics (Russian Federation)

    2014-12-15T23:59:59.000Z

    Among key problems in nuclear astrophysics, that of obtaining deeper insight into the mechanism of synthesis of chemical elements is of paramount importance. The majority of heavy elements existing in nature are produced in stars via radiative neutron capture in so-called s- and r processes, which are, respectively, slow and fast, in relation to competing ?{sup ?}-decay processes. At the same time, we know 35 neutron-deficient so-called bypassed p-nuclei that lie between {sup 74}Se and {sup 196}Hg and which cannot originate from the aforementioned s- and r-processes. Their production is possible in (?, n), (?, p), or (?, ?) photonuclear reactions. In view of this, data on photoneutron reactions play an important role in predicting and describing processes leading to the production of p-nuclei. Interest in determining cross sections for photoneutron reactions in the threshold energy region, which is of particular importance for astrophysics, has grown substantially in recent years. The use of modern sources of quasimonoenergetic photons obtained in processes of inverse Compton laser-radiation scattering on relativistic electronsmakes it possible to reveal rather interesting special features of respective cross sections, manifestations of pygmy E1 and M1 resonances, or the production of nuclei in isomeric states, on one hand, and to revisit the problem of systematic discrepancies between data on reaction cross sections from experiments of different types, on the other hand. Data obtained on the basis of our new experimental-theoretical approach to evaluating cross sections for partial photoneutron reactions are invoked in considering these problems.

  3. Argonne Physics Division - ATLAS

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    call 911 on the internal phones (or 252-1911 on cell phones) Safety Tom Mullen, Physics Division Safety Engineer. Please Note: If you have any comments or concerns regarding...

  4. Director, Division of Investigations

    Broader source: Energy.gov [DOE]

    The Federal Energy Regulatory Commission is looking for an experienced, highly skilled executive to serve as Director of the Division of Investigations (DOI) in the Office of Enforcement (OE). The...

  5. Division Student Liaisons

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    None Fire Protection (FP-DO) Robert J. Farris (Rob) 667-9045 sirraf@lanl.gov K493 Nuclear Criticality Safety None Operations Support Division (OS-DO) None Radiological...

  6. Guidance Systems Division ,

    Office of Legacy Management (LM)

    Oockec No. 10-0772 22 OCT 1981 Bcndlx CorporaLion ' Guidance Systems Division , ATTN: Mr. Wf 11 la,,, Hnrr,,or Manngar, PlanL Englne0rtny Teterboro, New Jersey 07608 uwm STATES...

  7. Astrophysical thermonuclear functions

    E-Print Network [OSTI]

    William J. Anderson; Hans J. Haubold; Arak Mathai Mathai

    1993-08-23T23:59:59.000Z

    Stars are gravitationally stabilized fusion reactors changing their chemical composition while transforming light atomic nuclei into heavy ones. The atomic nuclei are supposed to be in thermal equilibrium with the ambient plasma. The majority of reactions among nuclei leading to a nuclear transformation are inhibited by the necessity for the charged participants to tunnel through their mutual Coulomb barrier. As theoretical knowledge and experimental verification of nuclear cross sections increases it becomes possible to refine analytic representations for nuclear reaction rates. Over the years various approaches have been made to derive closed-form representations of thermonuclear reaction rates (Critchfield 1972, Haubold and John 1978, Haubold, Mathai and Anderson 1987). They show that the reaction rate contains the astrophysical cross section factor and its derivatives which has to be determined experimentally, and an integral part of the thermonuclear reaction rate independent from experimental results which can be treated by closed-form representation techniques in terms of generalized hypergeometric functions. In this paper mathematical/statistical techniques for deriving closed-form representations of thermonuclear functions will be summarized and numerical results for them will be given. The separation of thermonuclear functions from thermonuclear reaction rates is our preferred result. The purpose of the paper is also to compare numerical results for approximate and closed-form representations of thermonuclear functions. This paper completes the work of Haubold, Mathai, and Anderson (1987).

  8. Frontiers of Astrophysics - Workshop Summary

    E-Print Network [OSTI]

    Heino Falcke; Peter L. Biermann

    1997-11-07T23:59:59.000Z

    We summarize recent results presented in the astrophysics session during a conference on ``Frontiers of Contemporary Physics''. We will discuss three main fields (High-Energy Astrophysics, Relativistic Astrophysics, and Cosmology), where Astrophysicists are pushing the limits of our knowledge of the physics of the universe to new frontiers. Since the highlights of early 1997 were the first detection of a redshift and the optical and X-ray afterglows of gamma-ray bursts, as well as the first well-documented flares of TeV-Blazars across a large fraction of the electromagnetic spectrum, we will concentrate on these topics. Other topics covered are black holes and relativistic jets, high-energy cosmic rays, Neutrino-Astronomy, extragalactic magnetic fields, and cosmological models.

  9. Physics & Astrophysics press.princeton.edu

    E-Print Network [OSTI]

    Landweber, Laura

    Physics & Astrophysics 2013 press.princeton.edu #12;in a nutshell 1 in a nutshell 2 princeton frontiers in physics 3 textbooks 7 astronomy & astrophysics 10 princeton series in astrophysics 12 physics 15 princeton series in physics 16 quantum physics 17 condensed matter 18 mathematics, mathematical

  10. nuclear data for astrophysics resources, challenges, strategies,

    E-Print Network [OSTI]

    nuclear data for astrophysics resources, challenges, strategies, michael smith, eric lingerfelt tytler univ. california san diego san diego, california, usa #12;·nuclear astrophysics is an exciting Observation [RXTE GS1826-24] ·understanding of many fascinating astrophysical phenomena rely on input nuclear

  11. Nuclear astrophysics and electron beams

    SciTech Connect (OSTI)

    Schwenk, A. [Institut für Kernphysik, Technische Universität Darmstadt, 64289 Darmstadt, Germany and ExtreMe Matter Institute EMMI, GSI Helmholtzzentrum für Schwerionenforschung GmbH, 64291 Darmstadt (Germany)

    2013-11-07T23:59:59.000Z

    Electron beams provide important probes and constraints for nuclear astrophysics. This is especially exciting at energies within the regime of chiral effective field theory (EFT), which provides a systematic expansion for nuclear forces and electroweak operators based on quantum chromodynamics. This talk discusses some recent highlights and future directions based on chiral EFT, including nuclear structure and reactions for astrophysics, the neutron skin and constraints for the properties of neutron-rich matter in neutron stars and core-collapse supernovae, and the dark matter response of nuclei.

  12. Warp propagation in astrophysical discs

    E-Print Network [OSTI]

    Nixon, Chris

    2015-01-01T23:59:59.000Z

    Astrophysical discs are often warped, that is, their orbital planes change with radius. This occurs whenever there is a non-axisymmetric force acting on the disc, for example the Lense-Thirring precession induced by a misaligned spinning black hole, or the gravitational pull of a misaligned companion. Such misalignments appear to be generic in astrophysics. The wide range of systems that can harbour warped discs - protostars, X-ray binaries, tidal disruption events, quasars and others - allows for a rich variety in the disc's response. Here we review the basic physics of warped discs and its implications.

  13. Chemistry Division Department of Biological

    E-Print Network [OSTI]

    Heller, Barbara

    1 Chemistry Division Department of Biological and Chemical Sciences, Illinois Institute-13 Chemistry Division invites nominations for Kilpatrick Fellowship for the academic year 2012's Chemistry Department from 1947­1960. Mary Kilpatrick was a chemistry faculty member from 1947

  14. Superconducting Magnet Division

    E-Print Network [OSTI]

    Ohta, Shigemi

    Superconducting Magnet Division MAGNETIC DESIGN OF E-LENS SOLENOID AND CORRECTOR SYSTEM FOR RHIC* R.6 A gun collectors gun Combined Horizontal and Vertical Corrector Design Both types of dipole correctors. Gupta, M. Anerella, W. Fischer, G. Ganetis, X. Gu, A. Ghosh, A. Jain, P. Kovach, A. Marone, S. Plate, A

  15. Solid State Division

    SciTech Connect (OSTI)

    Green, P.H.; Watson, D.M. (eds.)

    1989-08-01T23:59:59.000Z

    This report contains brief discussions on work done in the Solid State Division of Oak Ridge National Laboratory. The topics covered are: Theoretical Solid State Physics; Neutron scattering; Physical properties of materials; The synthesis and characterization of materials; Ion beam and laser processing; and Structure of solids and surfaces. (LSP)

  16. integration division Human Systems

    E-Print Network [OSTI]

    integration division Human Systems Eye-Movement Metrics: Non-Intrusive Quantitative Tools for Monitoring Human Visual Performance Objective Approach Impact A reliable quantitative yet non-intrusive methodologies that provide quantitative yet non-intrusive measures of human visual performance for use

  17. Security Division 2007 Annual Report

    E-Print Network [OSTI]

    Computer Security Division 2007 Annual Report #12;TAble of ConTenTS Welcome Division Organization The Computer Security Division Responds to the Federal Information Security Management Act of 2002 Security Information Technology 15 Security Testing and Metrics 17 Validation Programs and Laboratory Accreditation 17

  18. Computer, Computational, and Statistical Sciences Division

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Computing CCS Division Computer, Computational, and Statistical Sciences Division Computational physics, computer science, applied mathematics, statistics and the integration of...

  19. Physics division annual report 1999

    SciTech Connect (OSTI)

    Thayer, K., ed.; Physics

    2000-12-06T23:59:59.000Z

    This report summarizes the research performed in the past year in the Argonne Physics Division. The Division's programs include operation of ATLAS as a national heavy-ion user facility, nuclear structure and reaction research with beams of heavy ions, accelerator research and development especially in superconducting radio frequency technology, nuclear theory and medium energy nuclear physics. The Division took significant strides forward in its science and its initiatives for the future in the past year. Major progress was made in developing the concept and the technology for the future advanced facility of beams of short-lived nuclei, the Rare Isotope Accelerator. The scientific program capitalized on important instrumentation initiatives with key advances in nuclear science. In 1999, the nuclear science community adopted the Argonne concept for a multi-beam superconducting linear accelerator driver as the design of choice for the next major facility in the field a Rare Isotope Accelerator (WA) as recommended by the Nuclear Science Advisory Committee's 1996 Long Range Plan. Argonne has made significant R&D progress on almost all aspects of the design concept including the fast gas catcher (to allow fast fragmentation beams to be stopped and reaccelerated) that in large part defined the RIA concept the superconducting rf technology for the driver accelerator, the multiple-charge-state concept (to permit the facility to meet the design intensity goals with existing ion-source technology), and designs and tests of high-power target concepts to effectively deal with the full beam power of the driver linac. An NSAC subcommittee recommended the Argonne concept and set as tie design goal Uranium beams of 100-kwatt power at 400 MeV/u. Argonne demonstrated that this goal can be met with an innovative, but technically in-hand, design. The heavy-ion research program focused on GammaSphere, the premier facility for nuclear structure gamma-ray studies. One example of the ground-breaking research with Garnmasphere was the first study of the limits of stability with angular momentum in the shell stabilized nobelium isotopes. It was found that these heaviest nuclei could be formed at surprisingly high angular momentum, providing important new insight into the production mechanisms for super-heavy elements. Another focus continues to be experiments with short-lived beams for critical nuclear astrophysics applications. Measurements revealed that {sup 44}Ti is more readily destroyed in supernovae than was expected. Major progress was made in collecting and storing unstable ions in the Canadian Penning Trap. The technique of stopping and rapidly extracting ions from a helium gas cell led directly to the new paradigm in the production of rare isotope beams that became RIA. ATLAS provided a record 6046 hours of beam use for experiments in FY99. The facility pressed hard to support the heavy demands of the GammaSphere Research program but maintained an operational reliability of 93%. Of the 29 different isotopes provided as beams in FY99, radioactive beams of {sup 44}Ti and {sup 17}F comprised 6% of the beam time. The theoretical efforts in the Division made dramatic new strides in such topics as quantum Monte Carlo calculations of light nuclei to understand microscopic many-body forces in nuclei; QCD calculations based on the Dyson-Schwinger approach which were extended to baryon systems and finite temperatures and densities; the structure of heavy nuclei; and proton decay modes of nuclei far from stability. The medium-energy program continues to focus on new techniques to understand how the quark-gluon structure of matter impacts the structure of nuclei. The HERMES experiment began making measurements of the fraction of the spin of the nucleon carried by the glue. Drell-Yan experiments study the flavor composition of the sea of the proton. Experiments at Jefferson lab search for clues of QCD dynamics at the hadronic level. A major advance in trace isotope analysis was realized with pioneering work on Atom Trap Trace Analysis, exploitin

  20. Particle Acceleration in Astrophysical Sources

    E-Print Network [OSTI]

    Amato, Elena

    2015-01-01T23:59:59.000Z

    Astrophysical sources are extremely efficient accelerators. Some sources emit photons up to multi-TeV energies, a signature of the presence, within them, of particles with energies much higher than those achievable with the largest accelerators on Earth. Even more compelling evidence comes from the study of Cosmic Rays, charged relativistic particles that reach the Earth with incredibly high energies: at the highest energy end of their spectrum, these subatomic particles are carrying a macroscopic energy, up to a few Joules. Here I will address the best candidate sources and mechanisms as cosmic particle accelerators. I will mainly focus on Galactic sources such as Supernova Remnants and Pulsar Wind Nebulae, which being close and bright, are the best studied among astrophysical accelerators. These sources are held responsible for most of the energy that is put in relativistic particles in the Universe, but they are not thought to accelerate particles up to the highest individual energies, $\\approx 10^{20}$ eV...

  1. Mission | APS Engineering Support Division

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    APS Engineering Support Division (AES) Search Button About Welcome Overview Visiting the APS Mission & Goals Find People Organization Charts Committees Job Openings User...

  2. Laser-Compton backscattering for nuclear astrophysics

    SciTech Connect (OSTI)

    Utsunomiya, Hiroaki [Department of Physics, Konan University, 8-9-1, Okamoto, Higashinada, Kobe 658-85-1, Japan and The Center for Nuclear Study, University of Tokyo, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)

    2014-05-09T23:59:59.000Z

    Using ?-ray beams for experimental nucleosynthesis study forms a new branch of nuclear astrophysics. I introduce typical experimental investigations and give a future prospect of this branch.

  3. Microsoft Word - Nuclear_Astrophysics_Summary

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    work and other H. Y. Lee (LANL): Improving neutron capture rate predictions using Apollo + HELIOS N. Scielzo (LBNL): Neutron spectroscopy with ion traps for astrophysics...

  4. Calibration in High-Energy Astrophysics Statistical Methods

    E-Print Network [OSTI]

    van Dyk, David

    Calibration in High-Energy Astrophysics Statistical Methods Statistical Computation Empirical Illustrations Accounting for Calibration Uncertainty: High Energy Astrophysics and the PCG Sampler David A. van Dyk Accounting for Calibration Uncertainty #12;Calibration in High-Energy Astrophysics Statistical

  5. astrophysical thermonuclear reactions: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    well as experimental investigations are motivated. T. Rauscher 1998-10-15 4 Astrophysical thermonuclear functions Astrophysics (arXiv) Summary: Stars are gravitationally stabilized...

  6. astrophysics magnet facility: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    there are magnetic helicity fluxes. A Brandenburg; P J Kpyl 2007-05-24 19 High energy astrophysics with the next generation of radio astronomy facilities Astrophysics...

  7. Workshop on Thermonuclear Reaction Rates for Astrophysics Applications

    E-Print Network [OSTI]

    Workshop on Thermonuclear Reaction Rates for Astrophysics Applications 24-25 November 2011, Athensrd and final circular for the Workshop on Thermonuclear Reaction Rates for Astrophysics Applications

  8. Systems Division NO. REV. NO.

    E-Print Network [OSTI]

    Rathbun, Julie A.

    Conditioning Unit (PCU) is compatible with a solar panel array. The Solar Panel Simulator and the PCU Test SetAerospace Systems Division NO. REV. NO. EATM-17 PCU - SOLAR PANEL SIMULATOR TEST REPORT:' Courtois ~ll~K. Hsi #12;MO. REV. MO. EATM-17 ~ Systems Division PCU - Solar Panel Simulator Test Report

  9. $?$-cluster ANCs for nuclear astrophysics

    E-Print Network [OSTI]

    M. L Avila; G. V. Roachev; E. Koshchiy; L. T. Baby; J. Belarge; K. W. Kemper; A. N. Kuchera; D. Santiago-Gonzalez

    2014-06-23T23:59:59.000Z

    Background. Many important $\\alpha$-particle induced reactions for nuclear astrophysics may only be measured using indirect techniques due to small cross sections at the energy of interest. One of such indirect technique, is to determine the Asymptotic Normalization Coefficients (ANC) for near threshold resonances extracted from sub-Coulomb $\\alpha$-transfer reactions. This approach provides a very valuable tool for studies of astrophysically important reaction rates since the results are practically model independent. However, the validity of the method has not been directly verified. Purpose. The aim of this letter is to verify the technique using the $^{16}$O($^6$Li,$d$)$^{20}$Ne reaction as a benchmark. The $^{20}$Ne nucleus has a well known $1^-$ state at excitation energy of 5.79 MeV with a width of 28 eV. Reproducing the known value with this technique is an ideal opportunity to verify the method. Method. The 1$^-$ state at 5.79 MeV is studied using the $\\alpha$-transfer reaction $^{16}$O($^6$Li,$d$)$^{20}$Ne at sub-Coulomb energies. Results. The partial $\\alpha$ width for the $1^-$ state at excitation energy of 5.79 MeV is extracted and compared with the known value, allowing the accuracy of the method to be evaluated. Conclusions. This study demonstrates that extracting the Asymptotic Normalization Coefficients using sub-Coulomb $\\alpha$-transfer reactions is a powerful tool that can be used to determine the partial $\\alpha$ width of near threshold states that may dominate astrophysically important nuclear reaction rates. \\end{description}

  10. Canadian Nuclear Astrophysics Institute Letter of Intent

    E-Print Network [OSTI]

    Herwig, Falk

    nuclear physics data as well as astronomical observations, both of which are critically needed in order 1 Canadian Nuclear Astrophysics Institute Letter of Intent Final version April 29, 2011), astrophysics and nuclear physics theory and computational simulation (TC) as well as nuclear physics

  11. Physics & Astrophysics press.princeton.edu

    E-Print Network [OSTI]

    Landweber, Laura

    Physics & Astrophysics 2010 press.princeton.edu #12;1 Textbooks 4 Astronomy & Astrophysics 10 at Princeton University Press. In these difficult times, we are delighted to be seeing record-breaking sales avoid) fraud wherever it may arise. Bracing reading, this short book is a perfect fit for courses

  12. ENERGY & ENVIRONMENT DIVISION ANNUAL REPORT 1979

    E-Print Network [OSTI]

    Cairns, E.J.

    2010-01-01T23:59:59.000Z

    Population Impacts of Geothermal Energy Development in thethe DOE Division of Geothermal Energy. S. L. Phillips and E.to DOE Division of Geothermal Energy, January 30, 1980.

  13. EARTH SCIENCES DIVISION ANNUAL REPORT 1978

    E-Print Network [OSTI]

    Authors, Various

    2012-01-01T23:59:59.000Z

    of Energy's Division of Geothermal Energy has undertaken aand Ghormley, E. L. , 1976. Geothermal energy conversion andof the Division of Geothermal Energy, and is compatible with

  14. Physics Division computer facilities

    SciTech Connect (OSTI)

    Cyborski, D.R.; Teh, K.M.

    1995-08-01T23:59:59.000Z

    The Physics Division maintains several computer systems for data analysis, general-purpose computing, and word processing. While the VMS VAX clusters are still used, this past year saw a greater shift to the Unix Cluster with the addition of more RISC-based Unix workstations. The main Divisional VAX cluster which consists of two VAX 3300s configured as a dual-host system serves as boot nodes and disk servers to seven other satellite nodes consisting of two VAXstation 3200s, three VAXstation 3100 machines, a VAX-11/750, and a MicroVAX II. There are three 6250/1600 bpi 9-track tape drives, six 8-mm tapes and about 9.1 GB of disk storage served to the cluster by the various satellites. Also, two of the satellites (the MicroVAX and VAX-11/750) have DAPHNE front-end interfaces for data acquisition. Since the tape drives are accessible cluster-wide via a software package, they are, in addition to replay, used for tape-to-tape copies. There is however, a satellite node outfitted with two 8 mm drives available for this purpose. Although not part of the main cluster, a DEC 3000 Alpha machine obtained for data acquisition is also available for data replay. In one case, users reported a performance increase by a factor of 10 when using this machine.

  15. DIVISION 16 -ELECTRICAL 16000 GENERAL

    E-Print Network [OSTI]

    DIVISION 16 - ELECTRICAL _____________________________________________________________ 16000 GENERAL A. Design Considerations 1. All drawing, specifications and construction shall conform to the following: National Electrical Code National Electrical Safety Code National Fire Protection Association

  16. Division 1137 property control system

    SciTech Connect (OSTI)

    Pastor, D.J.

    1982-01-01T23:59:59.000Z

    An automated data processing property control system was developed by Mobile and Remote Range Division 1137. This report describes the operation of the system and examines ways of using it in operational planning and control.

  17. Lawrence Berkeley National Laboratory Engineering Division Office

    E-Print Network [OSTI]

    /4867399 DMAttia@lbl.gov Administrative Staff Glenda Fish Division Office Administrator 510/4867123 GJFish

  18. Reconciling Nuclear and Astrophysical Constraints

    E-Print Network [OSTI]

    Dexheimer, V; Schramm, S

    2015-01-01T23:59:59.000Z

    In view of new constraints put forth by recent observations and measurements in the realm of astrophysics and nuclear physics, we update the non-linear realization of the sigma model as to reflect such constraints. By doing this, we obtain new equations of state that may be used to describe neutron stars. Such equations of state are obtained by investigating different ways by which the vector mesons self-interact. Furthermore, we also investigate the role played by the delta mesons in the model. As a result, we are able to develop equations of state that are in better agreement with data, such as nuclear compressibility and slope of the symmetry energy at saturation, star masses, radii, and cooling profiles.

  19. Indian Institute of Astrophysics Bangalore 560034

    E-Print Network [OSTI]

    Udgaonkar, Jayant B.

    of galaxies, active-galactic nuclei, quasars, gamma-ray bursts. Theoretical Astrophysics and related Physics satellite link. A recent addition is the High Altitude GAmma Ray (HAGAR) array comprising of seven

  20. SKA Organisation Jodrell Bank Centre for Astrophysics

    E-Print Network [OSTI]

    Tian, Weidong

    SKA Organisation Jodrell Bank Centre for Astrophysics Room 3.116 Alan Turing Building. The SKA Organisation is based in the Alan Turing Building, The University of Manchester and will move

  1. Computer Sciences and Mathematics Division | ornl.gov

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Computer Sciences and Mathematics Division SHARE Computer Sciences and Mathematics Division The Computer Science and Mathematics Division (CSMD) is ORNL's premier source of basic...

  2. Computational Sciences and Engineering Division | ornl.gov

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Computational Sciences and Engineering Division SHARE Computational Sciences and Engineering Division The Computational Sciences and Engineering Division is a major research...

  3. Neutrinos in Physics and Astrophysics

    E-Print Network [OSTI]

    G. G. Raffelt

    2003-03-05T23:59:59.000Z

    The observed flavor oscillations of solar and atmospheric neutrinos determine several elements of the leptonic mixing matrix, but leave open the small mixing angle Theta_13, a possible CP-violating phase, the mass ordering, the absolute mass scale m_nu, and the Dirac vs. Majorana property. Progress will be made by long-baseline, tritium endpoint, and 2-beta decay experiments. The best constraint on m_nu obtains from cosmological precision observables, implying that neutrinos contribute very little to the dark matter. However, massive Majorana neutrinos may well be responsible for ordinary matter by virtue of the leptogenesis mechanism for creating the baryon asymmetry of the universe. In future, neutrinos could play an important role as astrophysical messengers if point sources are discovered in high-energy neutrino telescopes. In the low-energy range, a high-statistics observation of a galactic supernova would allow one to observe directly the dynamics of stellar collapse and perhaps to discriminate between certain mixing scenarios. An observation of the relic neutrinos from all past supernovae has come within reach.

  4. The Sun Asphericities: Astrophysical Relevance

    E-Print Network [OSTI]

    J-P. Rozelot; S. Pireaux; S. Lefebvre; T. Corbard

    2004-04-01T23:59:59.000Z

    Of all the fundamental parameters of the Sun (diameter, mass, temperature...), the gravitational multipole moments (of degree l and order m) that determine the solar moments of inertia, are still poorly known. However, at the first order (l=2), the quadrupole moment is relevant to many astrophysical applications. It indeed contributes to the relativistic perihelion advance of planets, together with the post-Newtonian (PN) parameters; or to the precession of the orbital plane about the Sun polar axis, the latter being unaffected by the purely relativistic PN contribution. Hence, a precise knowledge of the quadrupole moment is necessary for accurate orbit determination, and alternatively, to obtain constraints on the PN parameters. Moreover, the successive gravitational multipole moments have a physical meaning: they describe deviations from a purely spherical mass distribution. Thus, their precise determination gives indications on the solar internal structure. Here, we explain why it is difficult to compute these parameters, how to derive the best values, and how they will be determined in a near future by means of space experiments.

  5. Firewall Phenomenology with Astrophysical Neutrinos

    E-Print Network [OSTI]

    Afshordi, Niayesh

    2015-01-01T23:59:59.000Z

    One of the most fundamental features of a black hole in general relativity is its event horizon: a boundary from which nothing can escape. There has been a recent surge of interest in the nature of these event horizons and their local neighbourhoods. In an attempt to resolve black hole information paradox(es), and more generally, to better understand the path towards quantum gravity, firewalls have been proposed as an alternative to black hole event horizons. In this letter, we explore the phenomenological implications of black holes possessing a surface or firewall. We predict a potentially detectable signature of these firewalls in the form of a high energy astrophysical neutrino flux. We compute the spectrum of this neutrino flux in different models and show that it is a possible candidate for the source of the PeV neutrinos recently detected by IceCube. We further show that, independent of the generation mechanism, IceCube data can be explained (at $1\\sigma$ confidence level) by conversion of accretion on...

  6. Physics, Computer Science and Mathematics Division. Annual report, January 1-December 31, 1980

    SciTech Connect (OSTI)

    Birge, R.W.

    1981-12-01T23:59:59.000Z

    Research in the physics, computer science, and mathematics division is described for the year 1980. While the division's major effort remains in high energy particle physics, there is a continually growing program in computer science and applied mathematics. Experimental programs are reported in e/sup +/e/sup -/ annihilation, muon and neutrino reactions at FNAL, search for effects of a right-handed gauge boson, limits on neutrino oscillations from muon-decay neutrinos, strong interaction experiments at FNAL, strong interaction experiments at BNL, particle data center, Barrelet moment analysis of ..pi..N scattering data, astrophysics and astronomy, earth sciences, and instrument development and engineering for high energy physics. In theoretical physics research, studies included particle physics and accelerator physics. Computer science and mathematics research included analytical and numerical methods, information analysis techniques, advanced computer concepts, and environmental and epidemiological studies. (GHT)

  7. NASA/TM-2014-217523 Goddard's Astrophysics Science Division Annual Report 2013

    E-Print Network [OSTI]

    Christian, Eric

    ..................................................................................................................................................1 2013 Year in Review ..............................................................................................

  8. NASA/TM2009214182 The Astrophysics Science Division Annual Report 2008

    E-Print Network [OSTI]

    Christian, Eric

    ....................................................................................................................................1 I. 2008: Year in Review

  9. DIVISION 6 -WOOD AND PLASTICS 06000 GENERAL

    E-Print Network [OSTI]

    DIVISION 6 - WOOD AND PLASTICS ________________________________________________________________________ 06000 GENERAL 1. For both woods and plastics, special attention is called to matters of flame spread-dried. 3. For exterior wood or plastic framed structures, see Division 4 for dimensions of Sample Panel

  10. Education Strategy Team Policy Division

    E-Print Network [OSTI]

    Rambaut, Andrew

    Education Strategy Team Policy Division DFID 1 Palace Street London SW1E 5HE 30 October 2009 TEL fellowships in India under the Wellcome Trust/DBT India Alliance2 . We believe that such investment is vital/Global-health-research/WTX055734.htm 2 Wellcome Trust/DBT India Alliance: http://www.wellcomedbt.org/index.htm #12;to support

  11. Publishing Division The Edinburgh Building

    E-Print Network [OSTI]

    Rosenberger, Alfred H.

    Publishing Division The Edinburgh Building Shaftesbury Road Cambridge CB2 2RU, UK TELEPHONE 01223 Building, Cambridge CB2 2RU, UK 40 West 20th Street, New York NY 10011-4211, USA 477 Williamstown Road Record [1] walter carl hartwig 2 The origin of primates [5] david tab rasmussen The earliest primates

  12. astrophysical scenarios pushing: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    for an Astrophysical Scenario Astrophysics (arXiv) Summary: In some models of gamma-ray bursts super-strong electric fields (Esim 1014 rm statvolt cm-1) have...

  13. Biosciences Division Media Mentions | Clean Energy | ORNL

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Biosciences Division Publications Newsletters Organizational Charts Research Highlights Media Mentions Clean Energy Home | Science & Discovery | Clean Energy | Supporting...

  14. Westinghouse Advanced Reactors Division Plutonium Fuel Laboratories

    Office of Legacy Management (LM)

    Radiological Condition of the Westinghouse Advanced Reactors Division Plutonium Fuel Laboratories Cheswick, Pennsylvania -. -, -- AGENCY: Office of Operational Safety, Department...

  15. Finance Division EXTRA MILE AWARD PROGRAM

    E-Print Network [OSTI]

    Crews, Stephen

    Finance Division EXTRA MILE AWARD PROGRAM Nomination Form Instructions Any fulltime or parttime permanent or temporary SPA employee within the Finance Division who works 20 or more provided. The seven major departments within the Finance Division to choose from are described below

  16. Analytical Chemistry Division's sample transaction system

    SciTech Connect (OSTI)

    Stanton, J.S.; Tilson, P.A.

    1980-10-01T23:59:59.000Z

    The Analytical Chemistry Division uses the DECsystem-10 computer for a wide range of tasks: sample management, timekeeping, quality assurance, and data calculation. This document describes the features and operating characteristics of many of the computer programs used by the Division. The descriptions are divided into chapters which cover all of the information about one aspect of the Analytical Chemistry Division's computer processing.

  17. EARTH SCIENCES Lower-Division Requirements

    E-Print Network [OSTI]

    Constable, Steve

    2012-2013 EARTH SCIENCES Lower-Division Requirements Math 20A_____ 20B_____ 20C_____ 20D (BILD 3) _____ SIO 50* _____ Group A: Earth Science Upper-Division Core Requirements (all courses _____ Introduction to Geophysics SIO 104 _____ Paleobiology and History of Life* Group B: Upper-Division Earth

  18. Computer Security Division 2008 Annual Report

    E-Print Network [OSTI]

    Computer Security Division 2008 Annual Report #12;TAble of ConTenTS Welcome 1 Division Organization 2 The Computer Security Division Responds to the Federal Information Security Management Act of 2002 3 Security Management and Assistance Group (SMA) 4 FISMA Implementation Project 4 Publications

  19. The Cosmic Battery in Astrophysical Accretion Disks

    E-Print Network [OSTI]

    Contopoulos, Ioannis; Katsanikas, Matthaios

    2015-01-01T23:59:59.000Z

    The aberrated radiation pressure at the inner edge of the accretion disk around an astrophysical black hole imparts a relative azimuthal velocity on the electrons with respect to the ions which gives rise to a ring electric current that generates large scale poloidal magnetic field loops. This is the Cosmic Battery established by Contopoulos and Kazanas in 1998. In the present work we perform realistic numerical simulations of this important astrophysical mechanism in advection-dominated accretion flows-ADAF. We confirm the original prediction that the inner parts of the loops are continuously advected toward the central black hole and contribute to the growth of the large scale magnetic field, whereas the outer parts of the loops are continuously diffusing outward through the turbulent accretion flow. This process of inward advection of the axial field and outward diffusion of the return field proceeds all the way to equipartition, thus generating astrophysically significant magnetic fields on astrophysicall...

  20. ASTROPHYSICAL FLUID DYNAMICS VIA DIRECT STATISTICAL SIMULATION

    SciTech Connect (OSTI)

    Tobias, S. M. [Department of Applied Mathematics, University of Leeds, Leeds LS2 9JT (United Kingdom); Dagon, K.; Marston, J. B., E-mail: smt@maths.leeds.ac.uk [Department of Physics, Brown University, Providence, RI 02912-1843 (United States)

    2011-02-01T23:59:59.000Z

    In this paper, we introduce the concept of direct statistical simulation for astrophysical flows. This technique may be appropriate for problems in astrophysical fluids where the instantaneous dynamics of the flows are of secondary importance to their statistical properties. We give examples of such problems including mixing and transport in planets, stars, and disks. The method is described for a general set of evolution equations, before we consider the specific case of a spectral method optimized for problems on a spherical surface. The method is illustrated for the simplest non-trivial example of hydrodynamics and magnetohydrodynamics on a rotating spherical surface. We then discuss possible extensions of the method both in terms of computational methods and the range of astrophysical problems that are of interest.

  1. MATERIALS AND MOLECULAR RESEARCH DIVISION. ANNUAL REPORT 1980

    E-Print Network [OSTI]

    Searcy, Alan W.

    2010-01-01T23:59:59.000Z

    of trans­ uranium organometallic chemistry, particularlyfor Uranium Isotope Separation," Chemistry Division, IsotopeOlander, "Uranium Enrichment by Laser," Chemistry Division,

  2. analytical sciences division: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Division Environmental Management and Restoration Websites Summary: Chemical Sciences and Engineering Division Director Assoc Director Ops Assoc Director Science Yates...

  3. MATERIALS AND MOLECULAR RESEARCH DIVISION. ANNUAL REPORT 1980

    E-Print Network [OSTI]

    Searcy, Alan W.

    2010-01-01T23:59:59.000Z

    for Uranium Isotope Separation," Chemistry Division, Isotopeof trans­ uranium organometallic chemistry, particularlyOlander, "Uranium Enrichment by Laser," Chemistry Division,

  4. MPhys (Hons) in Astrophysics MPhys (Hons) in Physics

    E-Print Network [OSTI]

    Sussex, University of

    Essentials Courses MPhys (Hons) in Astrophysics MPhys (Hons) in Physics BSc (Hons) in Physics MPhys (Hons) in Physics (research placement) MPhys (Hons) in Physics with Astrophysics BSc (Hons) in Physics with Astrophysics MPhys (Hons) in Theoretical Physics BSc (Hons) in Theoretical Physics Foundation year for UK

  5. Calibration in High-Energy Astrophysics Statistical Methods

    E-Print Network [OSTI]

    van Dyk, David

    Calibration in High-Energy Astrophysics Statistical Methods Empirical Illustrations Accounting for Calibration Uncertainty in High Energy Astrophysics David A. van Dyk1 Vinay Kashyap2 Taeyoung Park3 Jin Xu4 David A. van Dyk Accounting for Calibration Uncertainty #12;Calibration in High-Energy Astrophysics

  6. Probing New Physics with Astrophysical Neutrinos

    E-Print Network [OSTI]

    Nicole F. Bell

    2008-11-06T23:59:59.000Z

    We review the prospects for probing new physics with neutrino astrophysics. High energy neutrinos provide an important means of accessing physics beyond the electroweak scale. Neutrinos have a number of advantages over conventional astronomy and, in particular, carry information encoded in their flavor degree of freedom which could reveal a variety of exotic neutrino properties. We also outline ways in which neutrino astrophysics can be used to constrain dark matter properties, and explain how neutrino-based limits lead to a strong general bound on the dark matter total annihilation cross-section.

  7. Computational aspects of astrophysical MHD and turbulence

    E-Print Network [OSTI]

    Axel Brandenburg

    2001-09-27T23:59:59.000Z

    The advantages of high-order finite difference scheme for astrophysical MHD and turbulence simulations are highlighted. A number of one-dimensional test cases are presented ranging from various shock tests to Parker-type wind solutions. Applications to magnetized accretion discs and their associated outflows are discussed. Particular emphasis is placed on the possibility of dynamo action in three-dimensional turbulent convection and shear flows, which is relevant to stars and astrophysical discs. The generation of large scale fields is discussed in terms of an inverse magnetic cascade and the consequences imposed by magnetic helicity conservation are reviewed with particular emphasis on the issue of alpha-quenching.

  8. High-Energy Astrophysics and Cosmology

    E-Print Network [OSTI]

    John Ellis

    2002-10-26T23:59:59.000Z

    Interfaces between high-energy physics, astrophysics and cosmology are reviewed, with particular emphasis on the important roles played by high-energy cosmic-ray physics. These include the understanding of atmospheric neutrinos, the search for massive cold dark matter particles and possible tests of models of quantum gravity. In return, experiments at the LHC may be useful for refining models of ultra-high-energy cosmic rays, and thereby contributing indirectly to understanding their origin. Only future experiments will be able to tell whether these are due to some bottom-up astrophysical mechanism or some top-down cosmological mechanism.

  9. Astrophysics experiments with radioactive beams at ATLAS

    SciTech Connect (OSTI)

    Back, B. B.; Clark, J. A.; Pardo, R. C.; Rehm, K. E., E-mail: rehm@anl.gov; Savard, G. [Physics Division, Argonne National Laboratory, Argonne, IL 60439 (United States)] [Physics Division, Argonne National Laboratory, Argonne, IL 60439 (United States)

    2014-04-15T23:59:59.000Z

    Reactions involving short-lived nuclei play an important role in nuclear astrophysics, especially in explosive scenarios which occur in novae, supernovae or X-ray bursts. This article describes the nuclear astrophysics program with radioactive ion beams at the ATLAS accelerator at Argonne National Laboratory. The CARIBU facility as well as recent improvements for the in-flight technique are discussed. New detectors which are important for studies of the rapid proton or the rapid neutron-capture processes are described. At the end we briefly mention plans for future upgrades to enhance the intensity, purity and the range of in-flight and CARIBU beams.

  10. Summary of nuclear and particle astrophysics sessions

    SciTech Connect (OSTI)

    Wilkes, R.J. [Department of Physics, FM-15, University of Washington, Seattle, Washington 98195 (United States)

    1995-07-10T23:59:59.000Z

    Astrophysics is gaining increased attention from the particle and nuclear physics communities, as budget cuts, delays, and cancellations limit opportunities for breakthrough research at accelerator laboratories. Observations of cosmic rays (protons and nuclei), gamma rays and neutrinos present a variety of puzzles whose eventual solution will shed light on many issues ranging from the nature of fundamental interactions at extreme energies to the mechanisms of astrophysical sources. Several important detectors are just beginning full-scale operation and others are beginning construction. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

  11. Health, Safety, and Environment Division

    SciTech Connect (OSTI)

    Wade, C [comp.] [comp.

    1992-01-01T23:59:59.000Z

    The primary responsibility of the Health, Safety, and Environmental (HSE) Division at the Los Alamos National Laboratory is to provide comprehensive occupational health and safety programs, waste processing, and environmental protection. These activities are designed to protect the worker, the public, and the environment. Meeting these responsibilities requires expertise in many disciplines, including radiation protection, industrial hygiene, safety, occupational medicine, environmental science and engineering, analytical chemistry, epidemiology, and waste management. New and challenging health, safety, and environmental problems occasionally arise from the diverse research and development work of the Laboratory, and research programs in HSE Division often stem from these applied needs. These programs continue but are also extended, as needed, to study specific problems for the Department of Energy. The results of these programs help develop better practices in occupational health and safety, radiation protection, and environmental science.

  12. Neutrinos in physics, astrophysics, and cosmology

    E-Print Network [OSTI]

    A. D. Dolgov

    2000-06-12T23:59:59.000Z

    A brief review of neutrino anomalies in particle physics and of the role played by neutrinos in cosmology and astrophysics is presented. The main part of the talk is dedicated to the impact of neutrinos and in particular of neutrino oscillations on BBN and to a possible spatial variation of primordial abundances.

  13. Neutrino Mixing and Oscillations in Astrophysical Environments

    E-Print Network [OSTI]

    A. B. Balantekin

    2014-01-22T23:59:59.000Z

    A brief review of the current status of neutrino mixing and oscillations in astrophysical environments, with particular emphasis on the Sun and core-collapse supernovae, is given. Implications of the existence of sterile states which mix with the active neutrinos are discussed.

  14. Neutrino astrophysics : recent advances and open issues

    E-Print Network [OSTI]

    Volpe, Cristina

    2015-01-01T23:59:59.000Z

    We highlight recent advances in neutrino astrophysics, the open issues and the interplay with neutrino properties. We emphasize the important progress in our understanding of neutrino flavor conversion in media. We discuss the case of solar neutrinos, of core-collapse supernova neutrinos and of SN1987A, and of the recently discovered ultra-high energy neutrinos whose origin is to be determined.

  15. Neutrino mixing and oscillations in astrophysical environments

    SciTech Connect (OSTI)

    Balantekin, A. B. [Physics Department, University of Wisconsin, Madison WI 53706 (United States)

    2014-05-02T23:59:59.000Z

    A brief review of the current status of neutrino mixing and oscillations in astrophysical environments, with particular emphasis on the Sun and core-collapse supernovae, is given. Implications of the existence of sterile states which mix with the active neutrinos are discussed.

  16. Chemical Technology Division annual technical report 1997

    SciTech Connect (OSTI)

    NONE

    1998-06-01T23:59:59.000Z

    The Chemical Technology (CMT) Division is a diverse technical organization with principal emphases in environmental management and development of advanced energy sources. The Division conducts research and development in three general areas: (1) development of advanced power sources for stationary and transportation applications and for consumer electronics, (2) management of high-level and low-level nuclear wastes and hazardous wastes, and (3) electrometallurgical treatment of spent nuclear fuel. The Division also performs basic research in catalytic chemistry involving molecular energy resources, mechanisms of ion transport in lithium battery electrolytes, and the chemistry of technology-relevant materials and electrified interfaces. In addition, the Division operates the Analytical Chemistry Laboratory, which conducts research in analytical chemistry and provides analytical services for programs at Argonne National Laboratory (ANL) and other organizations. Technical highlights of the Division`s activities during 1997 are presented.

  17. On Making Relational Division Comprehensible

    E-Print Network [OSTI]

    McCann, Lester I.

    pno jno qty S1 P1 J1 200 ... ... ... ... S5 P6 J4 500 FIE 2003 ­ p.8/33 #12;A More Practical Example,pno(SPJ) and pno(weight=17(P)) sno pno pno S1 P1 P2 S2 P3 P3 S2 P5 S3 P3 S3 P4 S4 P6 S5 P1 S5 P2 S5 P3 S5 P4 S5 P5 S5 P6 FIE 2003 ­ p.10/33 #12;Division in Relational Algebra Idea: Find the values that do

  18. Colorado Air Pollution Control Division - Construction Permits...

    Open Energy Info (EERE)

    search OpenEI Reference LibraryAdd to library Web Site: Colorado Air Pollution Control Division - Construction Permits Forms and Air Pollutant Emission Notices (APENs)...

  19. EARTH SCIENCES DIVISION. ANNUAL REPORT 1977.

    E-Print Network [OSTI]

    Witherspoon, P.A.

    2011-01-01T23:59:59.000Z

    8erkeley Laboratory (LBL), the Earth Sciences Division, wasactivation analysis: rare earth element distribution (D)can be used to generate earth- quake records for use in

  20. Enforcement Letter, Westinghouse Waste Isolation Division - October...

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

    to Westinghouse Waste Isolation Division related to Quality Assurance and Occupational Radiation Protection Noncompliances at the Waste Isolation Pilot Plant On October 3, 2000,...

  1. Sandia National Laboratories: Internal Combustion Engine Division...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Internal Combustion Engine Division conference CRF Researchers Received "Best Paper" Award for Paper Presented at American Society of Mechanical Engineers' (ASME) 2012 Internal...

  2. Chemical Sciences Division | Advanced Materials |ORNL

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    reduce costs, and minimize the environmental impact in the production of rare-earth metals and alloys. The division's Nuclear Analytical Chemistry and Isotopics...

  3. Nuclear Data for Astrophysics: Collections at NucAstroData.org

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    In May of 2003, Dr. Michael Smith, Physics Division, ORNL, published a paper announcing the launch of the new website NucAstroData.org and the rationale behind it. An excerpt from the abstract of that paper, found in volume 718, pages 339-346, of ScienceDirect - Nuclear Physics A, explains: "In order to address important astrophysics problems such as the origin of the chemical elements, the inner workings of our Sun, and the evolution of stars, crucial nuclear datasets are needed. Recent evaluation and dissemination efforts have produced a number of such datasets, many of which are online and readily available to the research community. Current international efforts in this field are, unfortunately, insufficient to keep pace with the latest nuclear physics measurements and model calculations. A dedicated effort is required to update and expand existing datasets. I discuss several strategies and new initiatives that would ensure a more effective utilization of nuclear data in astrophysics. These include launching a new web site, www.nucastrodata.org, to aid in locating available nuclear data sets, and an interactive online plotting program with an easy-to-use graphical user interface to over 8000 reaction rates." This website continues to be resource for the nuclear astrophysics community. NucAstroData provides both links to datasets around the world and a repository where researchers can upload their own data. Tools for generating and manipulating reaction rates, merging libraries of data, plotting data and performing other tasks are provided under the website's Infrastructure section and the menu selection for software leads to useful codes.

  4. Particle acceleration in astrophysical shear flows

    E-Print Network [OSTI]

    Frank M. Rieger; Peter Duffy

    2005-01-10T23:59:59.000Z

    We consider the acceleration of particles due to a velocity shear in relativistic astrophysical flows. The basic physical picture and the formation of power law momentum spectra is discussed for a non-relativistic velocity field using a microscopic approach. We identify possible sites for shear acceleration in relativistic astrophysical jets and analyze their associated acceleration timescales. It is shown in particular that for a mean scattering time $\\tau$ scaling with the gyro-radius, the acceleration timescale for gradual shear scales in the same manner as the synchrotron cooling timescale, so that losses may no longer be able to stop the acceleration once it has started to work efficiently. Finally, the possible role of shear acceleration is discussed with reference to the relativistic jet in the quasar 3C~273.

  5. Particle acceleration efficiencies in astrophysical shear flows

    E-Print Network [OSTI]

    F. M. Rieger; P. Duffy

    2005-02-04T23:59:59.000Z

    The acceleration of energetic particles in astrophysical shear flows is analyzed. We show that in the presence of a non-relativistic gradual velocity shear, power law particle momentum distributions $f(p) \\propto p^{-(3+\\alpha)}$ may be generated, assuming a momentum-dependent scattering time $\\tau \\propto p^{\\alpha}$, with $\\alpha > 0$. We consider possible acceleration sites in astrophysical jets and study the conditions for efficient acceleration. It is shown, for example, that in the presence of a gradual shear flow and a gyro-dependent particle mean free path, synchrotron radiation losses no longer stop the acceleration once it has started to work efficiently. This suggests that shear acceleration may naturally account for a second, non-thermal population of energetic particles in addition to a shock-accelerated one. The possible relevance of shear acceleration is briefly discussed with reference to the relativistic jet in the quasar 3C 273.

  6. Data Mining in Gamma Astrophysics Experiments

    E-Print Network [OSTI]

    M. Frailis; A. De Angelis; V. Roberto

    2005-03-24T23:59:59.000Z

    Data mining techniques, including clustering and classification tasks, for the automatic information extraction from large datasets are increasingly demanded in several scientific fields. In particular, in the astrophysical field, large archives and digital sky surveys with dimensions of 10E12 bytes currently exist, while in the near future they will reach sizes of the order of 10E15. In this work we propose a multidimensional indexing method to efficiently query and mine large astrophysical datasets. A novelty detection algorithm, based on the Support Vector Clustering and using density and neighborhood information stored in the index structure, is proposed to find regions of interest in data characterized by isotropic noise. We show an application of this method for the detection of point sources from a gamma-ray photon list.

  7. An Astrophysical Explanation for the Great Silence

    E-Print Network [OSTI]

    James Annis

    1999-01-22T23:59:59.000Z

    An astrophysical model is proposed to answer Fermi's question. Gamma-ray bursts have the correct rates of occurrence and plausibly the correct energetics to have consequences for the evolution of life on a galactic scale. If one assumes that they are in fact lethal to land based life throughout the galaxy, one has a mechanism that prevents the rise of intelligence until the mean time between bursts is comparable to the timescale for the evolution of intelligence. Astrophysically plausible models suggest the present mean time between bursts to be $\\sim 10^8$ years, and evolutionarily plausible models suggest the rise of intelligence takes $\\sim 10^8$. Hence, this model suggests that the Galaxy is currently undergoing a phase transition between an equilibrium state devoid of intelligent life to a different equilibrium state where it is full of intelligent life.

  8. Megaton Water Cerenkov Detectors and Astrophysical Neutrinos

    E-Print Network [OSTI]

    Maury Goodman

    2005-01-21T23:59:59.000Z

    Although formal proposals have not yet been made, the UNO and Hyper-Kamiokande projects are being developed to follow-up the tremendously successful program at Super-Kamiokande using a detector that is 20-50 times larger. The potential of such a detector to continue the study of astrophysical neutrinos is considered and contrasted with the program for cubic kilometer neutrino observatories.

  9. Compact binary mergers: an astrophysical perspective

    E-Print Network [OSTI]

    S. Rosswog

    2010-12-22T23:59:59.000Z

    This paper reviews the current understanding of double neutron star and neutron star black hole binaries. It addresses mainly (nuclear) astrophysics aspects of compact binary mergers and thus complements recent reviews that have emphasized the numerical relativity viewpoint. In particular, the paper discusses different channels to release neutron-rich matter into the host galaxy, connections between compact binary mergers and short Gamma-ray bursts and accompanying electromagnetic signals.

  10. Physics Division ESH Bulletin 02-7 New Physics Division Procedure

    E-Print Network [OSTI]

    Physics Division ESH Bulletin 02-7 New Physics Division Procedure Applies to disablement of Physics-Interlock Disablement form is completed and given to the ESH Officer for filing 6/10/02 INTERLOCKS, TEMPORARY DISABLEMENT FILE maintained by Physics Division ESH Officer) #12;

  11. Astrophysical Gyrokinetics: Basic Equations and Linear Theory

    E-Print Network [OSTI]

    Gregory G. Howes; Steven C. Cowley; William Dorland; Gregory W. Hammett; Eliot Quataert; Alexander A. Schekochihin

    2006-05-04T23:59:59.000Z

    Magnetohydrodynamic (MHD) turbulence is encountered in a wide variety of astrophysical plasmas, including accretion disks, the solar wind, and the interstellar and intracluster medium. On small scales, this turbulence is often expected to consist of highly anisotropic fluctuations with frequencies small compared to the ion cyclotron frequency. For a number of applications, the small scales are also collisionless, so a kinetic treatment of the turbulence is necessary. We show that this anisotropic turbulence is well described by a low frequency expansion of the kinetic theory called gyrokinetics. This paper is the first in a series to examine turbulent astrophysical plasmas in the gyrokinetic limit. We derive and explain the nonlinear gyrokinetic equations and explore the linear properties of gyrokinetics as a prelude to nonlinear simulations. The linear dispersion relation for gyrokinetics is obtained and its solutions are compared to those of hot-plasma kinetic theory. These results are used to validate the performance of the gyrokinetic simulation code {\\tt GS2} in the parameter regimes relevant for astrophysical plasmas. New results on global energy conservation in gyrokinetics are also derived. We briefly outline several of the problems to be addressed by future nonlinear simulations, including particle heating by turbulence in hot accretion flows and in the solar wind, the magnetic and electric field power spectra in the solar wind, and the origin of small-scale density fluctuations in the interstellar medium.

  12. astrophysical mhd code: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    astrophysical plasmas motivates the implementation of almost conservative MHD computer codes. They should efficiently calculate, use highly parallelized schemes scaling well with...

  13. astrophysics international workshop: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    and cosmological models. Heino Falcke; Peter L. Biermann 1997-11-07 5 Workshop on Thermonuclear Reaction Rates for Astrophysics Applications Computer Technologies and Information...

  14. West Virginia University Division of Human Resources

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    on the WVU Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted version and this printed copy, the posted version on the Web page is controlling. Page 1 of 2 of this administrative procedure has been posted on the WVU Division of Human Resources Web page hr.wvu.edu. In the event

  15. West Virginia University Division of Human Resources

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    on the WVU Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted version and this printed copy, the posted version on the Web page is controlling. Page 1 of 3 Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted

  16. West Virginia University Division of Human Resources

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    on the WVU Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted version and this printed copy, the posted version on the Web page is controlling. Page 1 of 2 been posted on the WVU Division of Human Resources Web page hr.wvu.edu. In the event of a conflict

  17. West Virginia University Division of Human Resources

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted version and this printed copy, the posted version on the Web page is controlling. Page 1 of 2 Employment been posted on the WVU Division of Human Resources Web page hr.wvu.edu. In the event of a conflict

  18. West Virginia University Division of Human Resources

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted version and this printed copy, the posted version on the Web page is controlling. Page 1 of 2 Access been posted on the WVU Division of Human Resources Web page hr.wvu.edu. In the event of a conflict

  19. Satellite Meteorology and Climatology Division Roadmap

    E-Print Network [OSTI]

    Kuligowski, Bob

    Satellite Meteorology and Climatology Division Roadmap NOAA NESDIS Center for Satellite Applications and Research #12;SMCD Roadmap 2 NOAA/NESDIS/STAR Satellite Meteorology and Climatology Division Roadmap September 2005 NOAA Science Center, 5200 Auth Road, Room 712, Camp Springs, MD 20746 #12;SMCD

  20. Nuclear Engineering Division Think, explore, discover, innovate

    E-Print Network [OSTI]

    Kemner, Ken

    : "Application of an Annular Metallic Fuel with Lower Gas Plenum for Sodium- cooled Fast Reactor") ANS N. Stauff Award ANS K. Laurin-Kovitz 2013 Best Paper Award in Reactor Physics Division (RPD) (Paper Title Nuclear Society E. Merzari, H. Ninokata(***) 2010 Best Paper in Reactor Physics Division (RPD) American

  1. Progress Report on Power Division Work Plan

    E-Print Network [OSTI]

    RPS & impacts on PNW · Analysis of negative wholesale power prices · Wind Integration Forum · Maintain balancing" DR pilot programs · Tracking Smart Grid Demo Project ­ ­ Will include "conventional" and "load/windProgress Report on Power Division Work Plan Power Committee Meeting October 2010 1 #12;The Division

  2. EMS Division Potential Benefits of Selected

    E-Print Network [OSTI]

    driven by a high speed gas turbine supplied power to a 400 HP superconductive homopolar motor during at Overcome by New Technology: Cryocoolers & Cu Fiber brushes2 #12;EMS Division Baseline with Multi-turn Field Coil Multi-turn Armature Cryostat Steel Flux Return #12;EMS Division Homopolar Motor Technology

  3. LEADERSHIP TRAINING DIVISION Undergraduate Program Application

    E-Print Network [OSTI]

    Emmons, Scott

    LEADERSHIP TRAINING DIVISION Undergraduate Program Application 1 For more information: Questions in school: College: School in Israel: (if applicable): Major/Minor: High School: #12;LEADERSHIP TRAINING DIVISION Undergraduate Program Application 2 QUEST LEADERSHIP FELLOWSHIP The mission of Quest is to inspire

  4. Materials Sciences Division 1990 annual report

    SciTech Connect (OSTI)

    Not Available

    1990-12-31T23:59:59.000Z

    This report is the Materials Sciences Division`s annual report. It contains abstracts describing materials research at the National Center for Electron Microscopy, and for research groups in metallurgy, solid-state physics, materials chemistry, electrochemical energy storage, electronic materials, surface science and catalysis, ceramic science, high tc superconductivity, polymers, composites, and high performance metals.

  5. PHYSICS DIVISION ESH BULLETIN 07-02

    E-Print Network [OSTI]

    , and sealed or open celled lead-acid. No batteries should be disposed of in the trash. HOW TO MANAGE USED the Division Waste Generator to dispose lead-acid (car) batteries or if you have any questions. ReferencePHYSICS DIVISION ESH BULLETIN 07-02 BATTERY RECYCLING May 21, 2007 ORNL recycles all types

  6. Aviation Human Factors Division Institute of Aviation

    E-Print Network [OSTI]

    AHFD Aviation Human Factors Division Institute of Aviation University of Illinois at Urbana Systems Monitoring and Control Gavin R. Essenberg, Douglas A. Wiegmann, Aviation Human Factors Division experiments with more difficult path selection tasks might reveal if there are advantages for motion. Overall

  7. School of Art Division of Graphic Design

    E-Print Network [OSTI]

    Moore, Paul A.

    .372.7763 419.372.6955 fax lyoung@bgsu.edu www.bgsu.edu/art BOWLING GREEN STATE UNIVERSITY Division of Graphic.bgsu.edu/art BOWLING GREEN STATE UNIVERSITY 1) Be of Junior (60+ hours) or Senior (90+ hours) standing withinSchool of Art Division of Graphic Design 1020 Fine Arts Center Bowling Green, Ohio 43403-0204 419

  8. Fixed Income Division Nomura International plc

    E-Print Network [OSTI]

    Macrina, Andrea

    Fixed Income Division © Nomura International plc Symmetry methods for quadratic Gaussian models International plc Outline Motivation The quadratic Gaussian distribution The quadratic Gaussian process The quadratic Gaussian model #12;Fixed Income Division 3© Nomura International plc Part 1 Motivation #12;Fixed

  9. 1998 Chemical Technology Division Annual Technical Report.

    SciTech Connect (OSTI)

    Ackerman, J.P.; Einziger, R.E.; Gay, E.C.; Green, D.W.; Miller, J.F.

    1999-08-06T23:59:59.000Z

    The Chemical Technology (CMT) Division is a diverse technical organization with principal emphases in environmental management and development of advanced energy sources. The Division conducts research and development in three general areas: (1) development of advanced power sources for stationary and transportation applications and for consumer electronics, (2) management of high-level and low-level nuclear wastes and hazardous wastes, and (3) electrometallurgical treatment of spent nuclear fuel. The Division also performs basic research in catalytic chemistry involving molecular energy resources, mechanisms of ion transport in lithium battery electrolytes, and the chemistry of technology-relevant materials. In addition, the Division operates the Analytical Chemistry Laboratory, which conducts research in analytical chemistry and provides analytical services for programs at Argonne National Laboratory (ANL) and other organizations. Technical highlights of the Division's activities during 1998 are presented.

  10. Earth Sciences Division Research Summaries 2006-2007

    E-Print Network [OSTI]

    DePaolo, Donald

    2008-01-01T23:59:59.000Z

    the commencement of the Earth Sciences Division 30 yearstelling. Happy Anniversary! Earth Sciences Division ears YTritium in Engineered and Earth Materials Stefan Finsterle,

  11. APS Engineering Support Division (AES) | Advanced Photon Source

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    APS Engineering Support Division (AES) The APS Engineering Support Division provides reliable operations and technical support to the Advanced Photon Source user community. AES...

  12. astrophysical 8lid t7li: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    neutrino cooling and associated limits on neutrino properties; and high-energy astrophysical neutrinos. W. C. Haxton 2012-09-17 3 Nuclear astrophysics CiteSeer...

  13. E-Print Network 3.0 - astrophysical black holes Sample Search...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    PDF DIR ASTROPHYSICS Summary: dwarfs, neutron stars, black holes - supernovae - gamma-ray bursts stellar evolution versus galaxy... TALK DIR PDF DIR MASTER ASTROPHYSICS ...

  14. Alpha resonant scattering for astrophysical reaction studies

    SciTech Connect (OSTI)

    Yamaguchi, H.; Kahl, D.; Nakao, T. [Center for Nuclear Study (CNS), University of Tokyo, RIKEN campus, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan); Wakabayashi, Y.; Kubano, S. [The Institute of Physical and Chemical Research (RIKEN), 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan); Hashimoto, T. [Research Center for Nuclear Physics (RCNP), Osaka University, 10-1 Mihogaoka, Ibaraki, Osaka 567-0047 (Japan); Hayakawa, S. [Istituto Nazionale Fisica Nucleare - Laboratori Nazionali del Sud (INFN-LNS), Via S. Sofia 62, 95125 Catania (Italy); Kawabata, T. [Department of Physics, Kyoto University, Kita-Shirakawa, Kyoto 606-8502 (Japan); Iwasa, N. [Department of Physics, Tohoku University, Aoba, Sendai, Miyagi 980-8578 (Japan); Teranishi, T. [Department of Physics, Kyushu University, 6-10-1 Hakozaki, Fukuoka 812-8581 (Japan); Kwon, Y. K. [Institute for Basic Science, 70, Yuseong-daero 1689-gil, Yuseong-gu, Daejeon 305-811 (Korea, Republic of); Binh, D. N. [30 MeV Cyclotron Center, Tran Hung Dao Hospital, Hoan Kiem District, Hanoi (Viet Nam); Khiem, L. H.; Duy, N. G. [Institute of Physics, Vietnam Academy of Science and Technology, 18 Hong Quoc Viet, Nghia do, Hanoi (Viet Nam)

    2014-05-02T23:59:59.000Z

    Several alpha-induced astrophysical reactions have been studied at CRIB (CNS Radioactive Ion Beam separator), which is a low-energy RI beam separator at Center for Nuclear Study (CNS) of the University of Tokyo. One of the methods to study them is the ? resonant scattering using the thick-target method in inverse kinematics. Among the recent studies at CRIB, the measurement of {sup 7}Be+? resonant scattering is discussed. Based on the result of the experiment, we evaluated the contributions of high-lying resonances for the {sup 7}Be(?,?) reaction, and proposed a new cluster band in {sup 11}C.

  15. Astronomy, Astrophysics, and Space Physics in Greece

    E-Print Network [OSTI]

    V. Charmandaris

    2006-04-18T23:59:59.000Z

    In the present document I review the current organizational structure of Astronomy, Astrophysics and Space Physics in Greece. I briefly present the institutions where professional astronomers are pursuing research, along with some notes of their history, as well as the major astronomical facilities currently available within Greece. I touch upon topics related to graduate studies in Greece and present some statistics on the distribution of Greek astronomers. Even though every attempt is made to substantiate all issues mentioned, some of the views presented have inevitably a personal touch and thus should be treated as such.

  16. Plasma Astrophysics | Princeton Plasma Physics Lab

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOnItemResearch > TheNuclear AstrophysicsPayroll,Physics Physics An errorPlantPlasma

  17. astrophysical nuclear reactions: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    astrophysical nuclear reactions First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 Nuclear astrophysics...

  18. Computer Generation of Process Explanations in Nuclear Astrophysics

    E-Print Network [OSTI]

    Langley, Pat

    Computer Generation of Process Explanations in Nuclear Astrophysics Sakir Kocabas (uckoca describe Astra, a computational aid for generating process explanations in nuclear astrophysics. The system capture, as well as novel fusion reactions that produce neutrons and deuterium. The system has also

  19. Computer Generation of Process Explanations in Nuclear Astrophysics

    E-Print Network [OSTI]

    Langley, Pat

    Computer Generation of Process Explanations in Nuclear Astrophysics Sakir Kocabas (uckoca In this paper we describe Astra, a computational aid for generating process explanations in nuclear astrophysics and neutron capture, as well as novel fusion reactions that produce neutrons and deuterium. The system has

  20. astrophysical gamma ray: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    astrophysical gamma ray First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 Astrophysical Gamma Ray...

  1. TeV Particle Astrophysics II: Summary comments

    E-Print Network [OSTI]

    Thomas K. Gaisser

    2006-12-11T23:59:59.000Z

    A unifying theme of this conference was the use of different approaches to understand astrophysical sources of energetic particles in the TeV range and above. In this summary I review how gamma-ray astronomy, neutrino astronomy and (to some extent) gravitational wave astronomy provide complementary avenues to understanding the origin and role of high-energy particles in energetic astrophysical sources.

  2. Workshop on Thermonuclear Reaction Rates for Astrophysics Applications

    E-Print Network [OSTI]

    Workshop on Thermonuclear Reaction Rates for Astrophysics Applications 24-25 November 2011, Athens circular for the Workshop on Thermonuclear Reaction Rates for Astrophysics Applications, to be held of thermonuclear reaction rates. The topics of the workshop, in relation with thermonuclear reaction rates

  3. Biology and Medicine Division: Annual report 1986

    SciTech Connect (OSTI)

    Not Available

    1987-04-01T23:59:59.000Z

    The Biology and Medicine Division continues to make important contributions in scientific areas in which it has a long-established leadership role. For 50 years the Division has pioneered in the application of radioisotopes and charged particles to biology and medicine. There is a growing emphasis on cellular and molecular applications in the work of all the Division's research groups. The powerful tools of genetic engineering, the use of recombinant products, the analytical application of DNA probes, and the use of restriction fragment length polymorphic DNA are described and proposed for increasing use in the future.

  4. Chemical Sciences Division annual report 1994

    SciTech Connect (OSTI)

    NONE

    1995-06-01T23:59:59.000Z

    The division is one of ten LBL research divisions. It is composed of individual research groups organized into 5 scientific areas: chemical physics, inorganic/organometallic chemistry, actinide chemistry, atomic physics, and chemical engineering. Studies include structure and reactivity of critical reaction intermediates, transients and dynamics of elementary chemical reactions, and heterogeneous and homogeneous catalysis. Work for others included studies of superconducting properties of high-{Tc} oxides. In FY 1994, the division neared completion of two end-stations and a beamline for the Advanced Light Source, which will be used for combustion and other studies. This document presents summaries of the studies.

  5. Earth Sciences Division collected abstracts: 1979

    SciTech Connect (OSTI)

    Henry, A.L.; Schwartz, L.L.

    1980-04-30T23:59:59.000Z

    This report is a compilation of abstracts of papers, internal reports, and talks presented during 1979 at national and international meetings by members of the Earth Sciences Division, Lawrence Livermore Laboratory. The arrangement is alphabetical (by author). For a given report, a bibliographic reference appears under the name of each coauthor, but the abstract iself is given only under the name of the first author or the first Earth Sciences Division author. A topical index at the end of the report provides useful cross references, while indicating major areas of research interest in the Earth Sciences Division.

  6. Nuclear and High-Energy Astrophysics

    E-Print Network [OSTI]

    Fridolin Weber

    2002-07-01T23:59:59.000Z

    There has never been a more exciting time in the overlapping areas of nuclear physics, particle physics and relativistic astrophysics than today. Orbiting observatories such as the Hubble Space Telescope, Rossi X-ray Timing Explorer (RXTE), Chandra X-ray satellite, and the X-ray Multi Mirror Mission (XMM) have extended our vision tremendously, allowing us to see vistas with an unprecedented clarity and angular resolution that previously were only imagined, enabling astrophysicists for the first time ever to perform detailed studies of large samples of galactic and extragalactic objects. On the Earth, radio telescopes (e.g., Arecibo, Green Bank, Parkes, VLA) and instruments using adaptive optics and other revolutionary techniques have exceeded previous expectations of what can be accomplished from the ground. The gravitational wave detectors LIGO, LISA VIRGO, and Geo-600 are opening up a window for the detection of gravitational waves emitted from compact stellar objects such as neutron stars and black holes. Together with new experimental forefront facilities like ISAC, ORLaND and RIA, these detectors provide direct, quantitative physical insight into nucleosynthesis, supernova dynamics, accreting compact objects, cosmic-ray acceleration, and pair-production in high energy sources which reinforce the urgent need for a strong and continuous feedback from nuclear and particle theory and theoretical astrophysics. In my lectures, I shall concentrate on three selected topics, which range from the behavior of superdense stellar matter, to general relativistic stellar models, to strange quark stars and possible signals of quark matter in neutron stars.

  7. Extragalactic database. VII Reduction of astrophysical parameters

    E-Print Network [OSTI]

    G. Paturel; H. Andernach; L. Bottinelli; H. Di Nella; N. Durand; R. Garnier; L. Gouguenheim; P. Lanoix; M. C. Marthinet; C. Petit; J. Rousseau; G. Theureau; I. Vauglin

    1998-06-10T23:59:59.000Z

    The Lyon-Meudon Extragalactic database (LEDA) gives a free access to the main astrophysical parameters for more than 100,000 galaxies. The most common names are compiled allowing users to recover quickly any galaxy. All these measured astrophysical parameters are first reduced to a common system according to well defined reduction formulae leading to mean homogeneized parameters. Further, these parameters are also transformed into corrected parameters from widely accepted models. For instance, raw 21-cm line widths are transformed into mean standard widths after correction for instrumental effect and then into maximum velocity rotation properly corrected for inclination and non-circular velocity. This paper presents the reduction formulae for each parameter: coordinates, morphological type and luminosity class, diameter and axis ratio, apparent magnitude (UBV, IR, HI) and colors, maximum velocity rotation and central velocity dispersion, radial velocity, mean surface brightness, distance modulus and absolute magnitude, and group membership. For each of these parameters intermediate quantities are given: galactic extinction, inclination, K-correction etc.. All these parameters are available from direct connexion to LEDA (telnet lmc.univ-lyon1.fr, login: leda, no passwd OR http://www-obs.univ-lyon1.fr/leda ) and distributed on a standard CD-ROM (PGC-ROM 1996) by the Observatoire de Lyon via the CNRS (mail to petit@obs.univ-lyon1.fr).

  8. Financial Services Division of Administration & Finance

    E-Print Network [OSTI]

    de Lijser, Peter

    Financial Services Division of Administration & Finance (657) 278-2512 / Fax (714) 278: May Wong / Financial Services (CP-300). Instructions are at Questions? Email Directive11@fullerton.eduwww.finance

  9. Export Controls Compliance Division of Research

    E-Print Network [OSTI]

    Suzuki, Masatsugu

    Export Controls Compliance Division of Research of this document is to provide overall guidance on export control regulations and internal procedures information contained in their Export Control Compliance programs in the development of this document. #12

  10. EARTH SCIENCES DIVISION ANNUAL REPORT 1978

    E-Print Network [OSTI]

    Authors, Various

    2012-01-01T23:59:59.000Z

    of electrolytes: IX, rare earth chlorides, nitrates, andU E OF AQUIFER RESPONSE TO EARTH TIDES AS A MEANS O F SLawrence Berkeley Laboratory, Earth Sciences Division, 1977.

  11. EARTH SCIENCES DIVISION ANNUAL REPORT 1978

    E-Print Network [OSTI]

    Authors, Various

    2012-01-01T23:59:59.000Z

    of Energy's Division of Geothermal Energy has undertaken aand Ghormley, E. L. , 1976. Geothermal energy conversion andi a , Mexico, i n Geothermal energy: a n o v e l t y becomes

  12. Community Development Department Building & Safety Division

    E-Print Network [OSTI]

    BUILDING, RESIDENTIAL AND GREEN BUILDING CODES, AMENDING FREMONT MUNICIPAL CODE TITLE vn (BUILDING TO ENERGY REGULATIONS THE 2010 CALIFORNIA,GREEN BUILDING CODE The City of Fremont proposed to adopt local................ Community Development Department Building & Safety Division 39550 Liberty Street

  13. Energy Research and Development Division STAFF REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division STAFF REPORT NATURAL GAS RESEARCH AND DEVELOPMENT 2013 Annual Report CALIFORNIA ENERGY COMMISSION Edmund G. Brown Jr., Governor OCTOBER 2013 CEC5002013111 #12; CALIFORNIA ENERGY COMMISSION Linda Schrupp Primary Authors Prepared for: California

  14. Argonne National Decision and Information Sciences Division

    E-Print Network [OSTI]

    Argonne National Laboratory Decision and Information Sciences Division Introducing EMTools conforms to expecta- tions. Argonne National Laboratory, developer of the successful Synchronization Matrix and exercise tool: EMTools. EMTools integrates the func- tionality of Argonne's previous-generation emergency

  15. Acquisition Notice Posting Headquarters Acquisition Division

    E-Print Network [OSTI]

    Christian, Eric

    the technology readiness of the selected systems, provide tangible, innovative technology products, are cost CROSSCUTTING CAPABILITY DEMONSTRATIONS DIVISION TECHNOLOGY DEMONSTRATION MISSIONS PROGRAM General Information, NASA plans to begin the Technology Demonstrations Missions Program. One of the greatest challenges

  16. Materials Sciences Division Integrated Safety Management Plan

    E-Print Network [OSTI]

    Materials Sciences Division Integrated Safety Management Plan Revised: February 9, 2012 Prepared by: signed Feb. 9, 2012 Rick Kelly, Facility/EH&S Manager Submitted by: signed Feb. 9, 2012 Miquel Salmeron.1 RESPONSIBILITY AND AUTHORITY THROUGH LINE MANAGEMENT............................................................5

  17. Argonne National Laboratory Physics Division annual report, January--December 1996

    SciTech Connect (OSTI)

    Thayer, K.J. [ed.

    1997-08-01T23:59:59.000Z

    The past year has seen several of the Physics Division`s new research projects reach major milestones with first successful experiments and results: the atomic physics station in the Basic Energy Sciences Research Center at the Argonne Advanced Photon Source was used in first high-energy, high-brilliance x-ray studies in atomic and molecular physics; the Short Orbit Spectrometer in Hall C at the Thomas Jefferson National Accelerator (TJNAF) Facility that the Argonne medium energy nuclear physics group was responsible for, was used extensively in the first round of experiments at TJNAF; at ATLAS, several new beams of radioactive isotopes were developed and used in studies of nuclear physics and nuclear astrophysics; the new ECR ion source at ATLAS was completed and first commissioning tests indicate excellent performance characteristics; Quantum Monte Carlo calculations of mass-8 nuclei were performed for the first time with realistic nucleon-nucleon interactions using state-of-the-art computers, including Argonne`s massively parallel IBM SP. At the same time other future projects are well under way: preparations for the move of Gammasphere to ATLAS in September 1997 have progressed as planned. These new efforts are imbedded in, or flowing from, the vibrant ongoing research program described in some detail in this report: nuclear structure and reactions with heavy ions; measurements of reactions of astrophysical interest; studies of nucleon and sub-nucleon structures using leptonic probes at intermediate and high energies; atomic and molecular structure with high-energy x-rays. The experimental efforts are being complemented with efforts in theory, from QCD to nucleon-meson systems to structure and reactions of nuclei. Finally, the operation of ATLAS as a national users facility has achieved a new milestone, with 5,800 hours beam on target for experiments during the past fiscal year.

  18. UNIVERSITY OF CALIFORNIA, SANTA CRUZ DIVISION OF GRADUATE STUDIES

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    and Graduate Division coordination of efforts to increase graduate support and postdoctoral placement through

  19. Organization of ISI by Divisions and Constituent Units Information Sciences Division

    E-Print Network [OSTI]

    Bandyopadhyay, Antar

    Biological Sciences Division Agricultural and Ecological Research Unit Human Genetics Unit Biological Unit Canteen Security Unit Medical Welfare Unit Telephone Unit Transport Unit Guest House Audio Visual

  20. NO. REV. NO. Systems Division DATE

    E-Print Network [OSTI]

    Rathbun, Julie A.

    -~ NO. REV. NO. EATM-15 PAGE OF ~ Systems Division DATE EASEP /PSEP Solar Panel Development Design+"'--.:L'_;;;J....;::::::..··-=·~::!!:!!!e::...._ K. Hsi #12;NO. REV. NO. EATM-15 EASEP/PSEP Solar Panel Development ~ Systems Division Design of the EASE-PSEP Solar Panel Array~PA::G:,:E:..::=l=~o:F~=2=7= DATE 20 Nov. 1968 1. 0 SUMMARY Electrical power

  1. Earth Sciences Division annual report 1989

    SciTech Connect (OSTI)

    Not Available

    1990-06-01T23:59:59.000Z

    This Annual Report presents summaries of selected representative research activities from Lawrence Berkeley Laboratory grouped according to the principal disciplines of the Earth Sciences Division: Reservoir Engineering and Hydrology, Geology and Geochemistry, and Geophysics and Geomechanics. We are proud to be able to bring you this report, which we hope will convey not only a description of the Division's scientific activities but also a sense of the enthusiasm and excitement present today in the Earth Sciences.

  2. Weapons Experiments Division Explosives Operations Overview

    SciTech Connect (OSTI)

    Laintz, Kenneth E. [Los Alamos National Laboratory

    2012-06-19T23:59:59.000Z

    Presentation covers WX Division programmatic operations with a focus on JOWOG-9 interests. A brief look at DARHT is followed by a high level overview of explosives research activities currently being conducted within in the experimental groups of WX-Division. Presentation covers more emphasis of activities and facilities at TA-9 as these efforts have been more traditionally aligned with ongoing collaborative explosive exchanges covered under JOWOG-9.

  3. Earth Sciences Division collected abstracts: 1980

    SciTech Connect (OSTI)

    Henry, A.L.; Hornady, B.F. (eds.)

    1981-10-15T23:59:59.000Z

    This report is a compilation of abstracts of papers, reports, and talks presented during 1980 at national and international meetings by members of the Earth Sciences Division, Lawrence Livermore National Laboratory. The arrangement is alphabetical (by author). For a given report, a bibliographic reference appears under the name of each coauthor, but the abstract itself is given only under the name of the first author (indicated in capital letters) or the first Earth Sciences Division author.

  4. Biology Division progress report, October 1, 1991--September 30, 1993

    SciTech Connect (OSTI)

    Hartman, F.C.; Cook, J.S.

    1993-10-01T23:59:59.000Z

    This Progress Report summarizes the research endeavors of the Biology Division of the Oak Ridge National Laboratory during the period October 1, 1991, through September 30, 1993. The report is structured to provide descriptions of current activities and accomplishments in each of the Division`s major organizational units. Lists of information to convey the entire scope of the Division`s activities are compiled at the end of the report.

  5. A laser application to nuclear astrophysics

    SciTech Connect (OSTI)

    Barbui, M.; Hagel, K.; Schmidt, K.; Zheng, H.; Burch, R.; Barbarino, M.; Natowitz, J. B. [Cyclotron Institute, Texas A and M University, 3366 TAMU, College Station, TX (United States); Bang, W.; Dyer, G.; Quevedo, H. J.; Gaul, E.; Bernstein, A. C.; Donovan, M. [Center for High Energy Density Science, C1510, University of Texas at Austin, Austin, TX 78712 (United States); Bonasera, A. [Cyclotron Institute, Texas A and M University, 3366 TAMU, College Station, TX, U.S.A. and INFN- Laboratori Nazionali del Sud, via S.Sofia 62, 95125 Catania (Italy); Kimura, S. [Department of Physics, Università degli Studi di Milano, Via Celoria 16, 20133 Milano (Italy); Mazzocco, M. [Dipartimento di Fisica e Astronomia Università degli Studi di Padova and INFN Sezione di Padova, Via Marzolo 8, I-35131 Padova (Italy); Consoli, F.; De Angelis, R.; Andreoli, P. [Associazione Euratom-ENEA Sulla Fusione, Via Enrico Fermi 45, CP 65-00044 Frascati, Rome (Italy); Ditmire, T. [Center for High Energy Density Science, C1510, University of Texas at Austin, Austin, TX, 78712 (United States)

    2014-05-09T23:59:59.000Z

    In the last decade, the availability in high-intensity laser beams capable of producing plasmas with ion energies large enough to induce nuclear reactions has opened new research paths in nuclear physics. We studied the reactions {sup 3}He(d,p){sup 4}He and d(d,n){sup 3}He at temperatures of few keV in a plasma, generated by the interaction of intense ultrafast laser pulses with molecular deuterium or deuterated-methane clusters mixed with {sup 3}He atoms. The yield of 14.7 MeV protons from the {sup 3}He(d,p){sup 4}He reaction was used to extract the astrophysical S factor. Results of the experiment performed at the Center for High Energy Density Science at The University of Texas at Austin will be presented.

  6. Guidelines for axion identification in astrophysical observations

    E-Print Network [OSTI]

    K. Zioutas; Y. Semertzidis; Th. Papaevangelou

    2005-12-21T23:59:59.000Z

    The origin of various celestial phenomena have remained mysterious for conventional astrophysics. Therefore, alternative solutions should be considered, taking into account the involvement of unstable dark-matter particle candidates, such as the celebrated axions or other as yet unforeseen axion-like particles. Their spontaneous and induced decay by the ubiquitous solar magnetic fields can be at the origin of persisting enigmatic X-ray emission, giving rise to a steady and a transient/local solar activity, respectively. The (coherent) conversion of photons into axion(-like) particles in intrinsic magnetic fields may modify the solar axion spectrum. The reversed process can be behind transient (solar) luminosity deficits in the visible. Then, the Sun might be also a strong source of ~eV-axions. Thus, enigmatic observations might be the as yet missing direct signature for axion(-like) particles in earth-bound detectors.

  7. PLUTO: a Numerical Code for Computational Astrophysics

    E-Print Network [OSTI]

    A. Mignone; G. Bodo; S. Massaglia; T. Matsakos; O. Tesileanu; C. Zanni; A. Ferrari

    2007-03-12T23:59:59.000Z

    We present a new numerical code, PLUTO, for the solution of hypersonic flows in 1, 2 and 3 spatial dimensions and different systems of coordinates. The code provides a multi-physics, multi-algorithm modular environment particularly oriented towards the treatment of astrophysical flows in presence of discontinuities. Different hydrodynamic modules and algorithms may be independently selected to properly describe Newtonian, relativistic, MHD or relativistic MHD fluids. The modular structure exploits a general framework for integrating a system of conservation laws, built on modern Godunov-type shock-capturing schemes. Although a plethora of numerical methods has been successfully developed over the past two decades, the vast majority shares a common discretization recipe, involving three general steps: a piecewise polynomial reconstruction followed by the solution of Riemann problems at zone interfaces and a final evolution stage. We have checked and validated the code against several benchmarks available in literature. Test problems in 1, 2 and 3 dimensions are discussed.

  8. Few-body models for nuclear astrophysics

    SciTech Connect (OSTI)

    Descouvemont, P., E-mail: pdesc@ulb.ac.be [Physique Nucléaire Théorique et Physique Mathématique, C.P. 229, Université Libre de Bruxelles (ULB), B 1050 Brussels (Belgium); Baye, D., E-mail: dbaye@ulb.ac.be [Physique Nucléaire Théorique et Physique Mathématique, C.P. 229, Université Libre de Bruxelles (ULB), B 1050 Brussels (Belgium); Physique Quantique, C.P. 165/82, Université Libre de Bruxelles (ULB), B 1050 Brussels (Belgium); Suzuki, Y., E-mail: suzuki@nt.sc.niigata-u.ac.jp [Department of Physics, Niigata University, Niigata 950-2181 (Japan); RIKEN Nishina Center, Wako 351-0198 (Japan); Aoyama, S., E-mail: aoyama@cc.niigata-u.ac.jp [Center for Academic Information Service, Niigata University, Niigata 950-2181 (Japan); Arai, K., E-mail: arai@nagaoka-ct.ac.jp [Division of General Education, Nagaoka National College of Technology, 888 Nishikatakai, Nagaoka, Niigata 940-8532 (Japan)

    2014-04-15T23:59:59.000Z

    We present applications of microscopic models to nuclear reactions of astrophysical interest, and we essentially focus on few-body systems. The calculation of radiative-capture and transfer cross sections is outlined, and we discuss the corresponding reaction rates. Microscopic theories are briefly presented, and we emphasize on the matrix elements of four-body systems. The microscopic extension of the R-matrix theory to nuclear reactions is described. Applications to the {sup 2}H(d, ?){sup 4}He, {sup 2}H(d, p){sup 3}H and {sup 2}H(d, n){sup 3}He reactions are presented. We show the importance of the tensor force to reproduce the low-energy behaviour of the cross sections.

  9. Studies of High Energy Particle Astrophysics

    SciTech Connect (OSTI)

    Nitz, David F [Michigan Technological University; Fick, Brian E [Michigan Technological University

    2014-07-30T23:59:59.000Z

    This report covers the progress of the Michigan Technological University particle astrophysics group during the period April 15th, 2011 through April 30th, 2014. The principal investigator is Professor David Nitz. Professor Brian Fick is the Co-PI. The focus of the group is the study of the highest energy cosmic rays using the Pierre Auger Observatory. The major goals of the Pierre Auger Observatory are to discover and understand the source or sources of cosmic rays with energies exceeding 10**19 eV, to identify the particle type(s), and to investigate the interactions of those cosmic particles both in space and in the Earth's atmosphere. The Pierre Auger Observatory in Argentina was completed in June 2008 with 1660 surface detector stations and 24 fluorescence telescopes arranged in 4 stations. It has a collecting area of 3,000 square km, yielding an aperture of 7,000 km**2 sr.

  10. New Prospects in High Energy Astrophysics

    SciTech Connect (OSTI)

    Blandford, Roger; /KIPAC, Menlo Park

    2011-11-15T23:59:59.000Z

    Recent discoveries using TeV, X-ray and radio telescopes as well as Ultra High Energy Cosmic Ray arrays are leading to new insights into longstanding puzzles in high energy astrophysics. Many of these insights come from combining observations throughout the electromagnetic and other spectra as well as evidence assembled from different types of source to propose general principles. Issues discussed in this general overview include methods of accelerating relativistic particles, and amplifying magnetic field, the dynamics of relativistic outflows and the nature of the prime movers that power them. Observational approaches to distinguishing hadronic, leptonic and electromagnetic outflows and emission mechanisms are discussed along with probes of the velocity field and the confinement mechanisms. Observations with GLAST promise to be very prescriptive for addressing these problems.

  11. A high energy photon polarimeter for astrophysics

    E-Print Network [OSTI]

    Eingorn, Maxim; Vlahovic, Branislav; Wojtsekhowski, Bogdan; Urciuoli, Guido Maria; De Persio, Fulvio; Meddi, Franco

    2015-01-01T23:59:59.000Z

    A high-energy photon polarimeter for astrophysics studies in the energy range from 20 MeV to 1000 MeV is considered. The proposed concept uses a stack of silicon micro-strip detectors where they play the roles of both a converter and a tracker. The purpose of this paper is to outline the parameters of such a polarimeter and to estimate the productivity of measurements. Our study supported by a Monte Carlo simulation shows that with a one-year observation period the polarimeter will provide 5.5 % accuracy of the polarization degree for a photon energy of 100 MeV, which would be a significant advance relative to the currently explored energy range of a few MeV. The proposed polarimeter design could easily be adjusted to the specific photon energy range to maximize efficiency if needed.

  12. Prospects of High Energy Laboratory Astrophysics

    SciTech Connect (OSTI)

    Ng, J.S.T.; Chen, P.; /SLAC

    2006-09-21T23:59:59.000Z

    Ultra high energy cosmic rays (UHECR) have been observed but their sources and production mechanisms are yet to be understood. We envision a laboratory astrophysics program that will contribute to the understanding of cosmic accelerators with efforts to: (1) test and calibrate UHECR observational techniques, and (2) elucidate the underlying physics of cosmic acceleration through laboratory experiments and computer simulations. Innovative experiments belonging to the first category have already been done at the SLAC FFTB. Results on air fluorescence yields from the FLASH experiment are reviewed. Proposed future accelerator facilities can provided unprecedented high-energy-densities in a regime relevant to cosmic acceleration studies and accessible in a terrestrial environment for the first time. We review recent simulation studies of nonlinear plasma dynamics that could give rise to cosmic acceleration, and discuss prospects for experimental investigation of the underlying mechanisms.

  13. Investigating High Field Gravity using Astrophysical Techniques

    SciTech Connect (OSTI)

    Bloom, Elliott D.; /SLAC

    2008-02-01T23:59:59.000Z

    The purpose of these lectures is to introduce particle physicists to astrophysical techniques. These techniques can help us understand certain phenomena important to particle physics that are currently impossible to address using standard particle physics experimental techniques. As the subject matter is vast, compromises are necessary in order to convey the central ideas to the reader. Many general references are included for those who want to learn more. The paragraphs below elaborate on the structure of these lectures. I hope this discussion will clarify my motivation and make the lectures easier to follow. The lectures begin with a brief review of more theoretical ideas. First, elements of general relativity are reviewed, concentrating on those aspects that are needed to understand compact stellar objects (white dwarf stars, neutron stars, and black holes). I then review the equations of state of these objects, concentrating on the simplest standard models from astrophysics. After these mathematical preliminaries, Sec. 2(c) discusses 'The End State of Stars'. Most of this section also uses the simplest standard models. However, as these lectures are for particle physicists, I also discuss some of the more recent approaches to the equation of state of very dense compact objects. These particle-physics-motivated equations of state can dramatically change how we view the formation of black holes. Section 3 focuses on the properties of the objects that we want to characterize and measure. X-ray binary systems and Active Galactic Nuclei (AGN) are stressed because the lectures center on understanding very dense stellar objects, black hole candidates (BHCs), and their accompanying high gravitational fields. The use of x-ray timing and gamma-ray experiments is also introduced in this section. Sections 4 and 5 review information from x-ray and gamma-ray experiments. These sections also discuss the current state of the art in x-ray and gamma-ray satellite experiments and plans for future experiments.

  14. Energy Technology Division research summary - 1999.

    SciTech Connect (OSTI)

    NONE

    1999-03-31T23:59:59.000Z

    The Energy Technology Division provides materials and engineering technology support to a wide range of programs important to the US Department of Energy. As shown on the preceding page, the Division is organized into ten sections, five with concentrations in the materials area and five in engineering technology. Materials expertise includes fabrication, mechanical properties, corrosion, friction and lubrication, and irradiation effects. Our major engineering strengths are in heat and mass flow, sensors and instrumentation, nondestructive testing, transportation, and electromechanics and superconductivity applications. The Division Safety Coordinator, Environmental Compliance Officers, Quality Assurance Representative, Financial Administrator, and Communication Coordinator report directly to the Division Director. The Division Director is personally responsible for cultural diversity and is a member of the Laboratory-wide Cultural Diversity Advisory Committee. The Division's capabilities are generally applied to issues associated with energy production, transportation, utilization, or conservation, or with environmental issues linked to energy. As shown in the organization chart on the next page, the Division reports administratively to the Associate Laboratory Director (ALD) for Energy and Environmental Science and Technology (EEST) through the General Manager for Environmental and Industrial Technologies. While most of our programs are under the purview of the EEST ALD, we also have had programs funded under every one of the ALDs. Some of our research in superconductivity is funded through the Physical Research Program ALD. We also continue to work on a number of nuclear-energy-related programs under the ALD for Engineering Research. Detailed descriptions of our programs on a section-by-section basis are provided in the remainder of this book.

  15. The History of Metals and Ceramics Division

    SciTech Connect (OSTI)

    Craig, D.F.

    1999-01-01T23:59:59.000Z

    The division was formed in 1946 at the suggestion of Dr. Eugene P. Wigner to attack the problem of the distortion of graphite in the early reactors due to exposure to reactor neutrons, and the consequent radiation damage. It was called the Metallurgy Division and assembled the metallurgical and solid state physics activities of the time which were not directly related to nuclear weapons production. William A. Johnson, a Westinghouse employee, was named Division Director in 1946. In 1949 he was replaced by John H Frye Jr. when the Division consisted of 45 people. He was director during most of what is called the Reactor Project Years until 1973 and his retirement. During this period the Division evolved into three organizational areas: basic research, applied research in nuclear reactor materials, and reactor programs directly related to a specific reactor(s) being designed or built. The Division (Metals and Ceramics) consisted of 204 staff members in 1973 when James R. Weir, Jr., became Director. This was the period of the oil embargo, the formation of the Energy Research and Development Administration (ERDA) by combining the Atomic Energy Commission (AEC) with the Office of Coal Research, and subsequent formation of the Department of Energy (DOE). The diversification process continued when James O. Stiegler became Director in 1984, partially as a result of the pressure of legislation encouraging the national laboratories to work with U.S. industries on their problems. During that time the Division staff grew from 265 to 330. Douglas F. Craig became Director in 1992.

  16. North Atlantic DivisionNorth Atlantic Division SuperstormSuperstorm SandySandy

    E-Print Network [OSTI]

    US Army Corps of Engineers

    North Atlantic DivisionNorth Atlantic Division SuperstormSuperstorm SandySandy Dredging Industry BriefDredging Industry BriefDredging Industry BriefDredging Industry Brief 3 April 20133 April 2013 #12;NAD Sandy Dredging BriefNAD Sandy Dredging Brief · Purposep · Goals · Sandy Program Overview

  17. SHR Service Team: Academic Divisions -Contact Matrix Primary Contact by Unit/Division

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    SHR Service Team: Academic Divisions - Contact Matrix Primary Contact by Unit/Division Astronomy Consultation Dawn Harker Teresa Roffe Barbara Lorimer Last Revised: 07/07/2010 Mail Stop: SHR-Service Teams Fax: 831-459-2661 1 of 2 #12;SHR Operations Services Team One SHR Partner Services Senior Manager, SHR

  18. Transportation Energy Technology DivisionEnergy Technology Division --TribologyTribology

    E-Print Network [OSTI]

    -frictionless carbon coatings to the components when appropriate · Develop and evaluate polymer composite materials to their prototype using Hitco C/C composite and anodized aluminum material combination. · Fabricated and evaluatedTransportation Materials Energy Technology DivisionEnergy Technology Division -- Tribology

  19. Division of Student Life 20122013 ANNUAL REPORT Division of Student Life

    E-Print Network [OSTI]

    1 Division of Student Life 2012­2013 ANNUAL REPORT Division of Student Life #12;2 The Power to Transform: Expectations of Our Students At UW­Madison, we know that the Wisconsin Experience has learning inside and outside the classroom to make the world a better place?" In the eight departments

  20. Energy Technology Division research summary -- 1994

    SciTech Connect (OSTI)

    Not Available

    1994-09-01T23:59:59.000Z

    Research funded primarily by the NRC is directed toward assessing the roles of cyclic fatigue, intergranular stress corrosion cracking, and irradiation-assisted stress corrosion cracking on failures in light water reactor (LWR) piping systems, pressure vessels, and various core components. In support of the fast reactor program, the Division has responsibility for fuel-performance modeling and irradiation testing. The Division has major responsibilities in several design areas of the proposed International Thermonuclear Experimental Reactor (ITER). The Division supports the DOE in ensuring safe shipment of nuclear materials by providing extensive review of the Safety Analysis Reports for Packaging (SARPs). Finally, in the nuclear area they are investigating the safe disposal of spent fuel and waste. In work funded by DOE`s Energy Efficiency and Renewable Energy, the high-temperature superconductivity program continues to be a major focal point for industrial interactions. Coatings and lubricants developed in the division`s Tribology Section are intended for use in transportation systems of the future. Continuous fiber ceramic composites are being developed for high-performance heat engines. Nondestructive testing techniques are being developed to evaluate fiber distribution and to detect flaws. A wide variety of coatings for corrosion protection of metal alloys are being studied. These can increase lifetimes significant in a wide variety of coal combustion and gasification environments.

  1. Nuclear Chemistry Division annual report FY83

    SciTech Connect (OSTI)

    Struble, G. (ed.)

    1983-01-01T23:59:59.000Z

    The purpose of the annual reports of the Nuclear Chemistry Division is to provide a timely summary of research activities pursued by members of the Division during the preceding year. Throughout, details are kept to a minimum; readers desiring additional information are encouraged to read the referenced documents or contact the authors. The Introduction presents an overview of the Division's scientific and technical programs. Next is a section of short articles describing recent upgrades of the Division's major facilities, followed by sections highlighting scientific and technical advances. These are grouped under the following sections: nuclear explosives diagnostics; geochemistry and environmental sciences; safeguards technology and radiation effect; and supporting fundamental science. A brief overview introduces each section. Reports on research supported by a particular program are generally grouped together in the same section. The last section lists the scientific, administrative, and technical staff in the Division, along with visitors, consultants, and postdoctoral fellows. It also contains a list of recent publications and presentations. Some contributions to the annual report are classified and only their abstracts are included in this unclassified portion of the report (UCAR-10062-83/1); the full article appears in the classified portion (UCAR-10062-83/2).

  2. astrophysical reaction rate: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 Workshop on Thermonuclear Reaction Rates for Astrophysics Applications Computer Technologies and Information...

  3. astrophysical reaction rates: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 Workshop on Thermonuclear Reaction Rates for Astrophysics Applications Computer Technologies and Information...

  4. astrophysical applications spectroscopie: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    OVII OVIII NeXII SiXIV FeXVII NeXI Topic1:HotStarX-rays Cohen, David 2 Workshop on Thermonuclear Reaction Rates for Astrophysics Applications Computer Technologies and Information...

  5. astrophysical systems kinetic: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 Thermonuclear Kinetics in Astrophysics CERN Preprints Summary: Over the billions of years since...

  6. Technology development for a neutrino astrophysical observatory. Letter of intent

    SciTech Connect (OSTI)

    Chaloupka, V.; Cole, T.; Crawford, H.J. [and others

    1996-02-01T23:59:59.000Z

    The authors propose a set of technology developments relevant to the design of an optimized Cerenkov detector for the study of neutrino interactions of astrophysical interest. Emphasis is placed on signal processing innovations that enhance significantly the quality of primary data. These technical advances, combined with field experience from a follow-on test deployment, are intended to provide a basis for the engineering design for a kilometer-scale Neutrino Astrophysical Observatory.

  7. Technology Development for a Neutrino AstrophysicalObservatory

    SciTech Connect (OSTI)

    Chaloupka, V.; Cole, T.; Crawford, H.J.; He, Y.D.; Jackson, S.; Kleinfelder, S.; Lai, K.W.; Learned, J.; Ling, J.; Liu, D.; Lowder, D.; Moorhead, M.; Morookian, J.M.; Nygren, D.R.; Price, P.B.; Richards, A.; Shapiro, G.; Shen, B.; Smoot, George F.; Stokstad, R.G.; VanDalen, G.; Wilkes, J.; Wright, F.; Young, K.

    1996-02-01T23:59:59.000Z

    We propose a set of technology developments relevant to the design of an optimized Cerenkov detector for the study of neutrino interactions of astrophysical interest. Emphasis is placed on signal processing innovations that enhance significantly the quality of primary data. These technical advances, combined with field experience from a follow-on test deployment, are intended to provide a basis for the engineering design for a kilometer-scale Neutrino Astrophysical Observatory.

  8. Chemical Technology Division annual technical report, 1996

    SciTech Connect (OSTI)

    NONE

    1997-06-01T23:59:59.000Z

    CMT is a diverse technical organization with principal emphases in environmental management and development of advanced energy sources. It conducts R&D in 3 general areas: development of advanced power sources for stationary and transportation applications and for consumer electronics, management of high-level and low-level nuclear wastes and hazardous wastes, and electrometallurgical treatment of spent nuclear fuel. The Division also performs basic research in catalytic chemistry involving molecular energy resources, mechanisms of ion transport in lithium battery electrolytes, materials chemistry of electrified interfaces and molecular sieves, and the theory of materials properties. It also operates the Analytical Chemistry Laboratory, which conducts research in analytical chemistry and provides analytical services for programs at ANL and other organizations. Technical highlights of the Division`s activities during 1996 are presented.

  9. March 30, 2009 16:44 Geophysical and Astrophysical Fluid Dynamics gafdbo09 Geophysical and Astrophysical Fluid Dynamics

    E-Print Network [OSTI]

    Al Hanbali, Ahmad

    March 30, 2009 16:44 Geophysical and Astrophysical Fluid Dynamics gafdbo09 Geophysical (geophysical) fluid models: two-dimensional vortical systems in a generalized streamfunction-vorticity rep

  10. Life Sciences Division annual report, 1988

    SciTech Connect (OSTI)

    Marrone, B.L.; Cram, L.S. (comps.)

    1989-04-01T23:59:59.000Z

    This report summarizes the research and development activities of Los Alamos National Laboratory's Life Sciences Division for the calendar year 1988. Technical reports related to the current status of projects are presented in sufficient detail to permit the informed reader to assess their scope and significance. Summaries useful to the casual reader desiring general information have been prepared by the Group Leaders and appear in each group overview. Investigators on the staff of the Life Sciences Division will be pleased to provide further information.

  11. Nuclear Astrophysics Animations from the Nuclear Astrophysics Group at Clemson University

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Meyer, Bradley; The, Lih-Sin

    The animations are organized into three sections. The r-Process Movies demonstrate r-Process network calculations from the paper "Neutrino Capture and the R-Process" Meyer, McLaughlin, and Fuller, Phys. Rev. C, 58, 3696-3710 (1998). The Alpha-Rich Freezeout Movies are related to the reference: Standard alpha-rich freezeout calculation from The, Clayton, Jin, and Meyer 1998, Astrophysical Journal, "Reaction Rates Governing the Synthesis of 44Ti" At the current writing, the category for Low Metallicity s-Process Movies has only one item called n, p, 13C, 14N, 54Fe, and 88Sr Time evolution in convective zone.

  12. The NASA Astrophysics Data System: Overview

    E-Print Network [OSTI]

    M. J. Kurtz; G. Eichhorn; A. Accomazzi; C. Grant; S. S. Murray; J. M. Watson

    2000-02-04T23:59:59.000Z

    The NASA Astrophysics Data System Abstract Service has become a key component of astronomical research. It provides bibliographic information daily, or near daily, to a majority of astronomical researchers worldwide. We describe the history of the development of the system and its current status. We show several examples of how to use the ADS, and we show how ADS use has increased as a function of time. Currently it is still increasing exponentially, with a doubling time for number of queries of 17 months. Using the ADS logs we make the first detailed model of how scientific journals are read as a function of time since publication. The impact of the ADS on astronomy can be calculated after making some simple assumptions. We find that the ADS increases the efficiency of astronomical research by 333 Full Time Equivalent (2000 hour) research years per year, and that the value of the early development of the ADS for astronomy, compared with waiting for mature technologies to be adopted, is 2332 FTE research years. The ADS is available at http://adswww.harvard.edu/.

  13. The NASA Astrophysics Data System: Data Holdings

    E-Print Network [OSTI]

    C. Grant; A. Accomazzi; G. Eichhorn; M. J. Kurtz; S. S. Murray

    2000-02-04T23:59:59.000Z

    Since its inception in 1993, the ADS Abstract Service has become an indispensable research tool for astronomers and astrophysicists worldwide. In those seven years, much effort has been directed toward improving both the quantity and the quality of references in the database. From the original database of approximately 160,000 astronomy abstracts, our dataset has grown almost tenfold to approximately 1.5 million references covering astronomy, astrophysics, planetary sciences, physics, optics, and engineering. We collect and standardize data from approximately 200 journals and present the resulting information in a uniform, coherent manner. With the cooperation of journal publishers worldwide, we have been able to place scans of full journal articles on-line back to the first volumes of many astronomical journals, and we are able to link to current version of articles, abstracts, and datasets for essentially all of the current astronomy literature. The trend toward electronic publishing in the field, the use of electronic submission of abstracts for journal articles and conference proceedings, and the increasingly prominent use of the World Wide Web to disseminate information have enabled the ADS to build a database unparalleled in other disciplines. The ADS can be accessed at http://adswww.harvard.edu

  14. Astrophysics of Dust in Cold Clouds

    E-Print Network [OSTI]

    B. T. Draine

    2003-04-28T23:59:59.000Z

    Nine lectures reviewing the astrophysics of dust in interstellar clouds. Topics include: (1) Summary of observational evidence concerning interstellar dust: broadband extinction, scattering of starlight, polarization of starlight, spectroscopy of dust, IR and FIR emission, and depletions of grain-forming elements. (2) Optics of interstellar dust grains: dielectric functions of nonconducting and conducting materials, calculational techniques, formulae valid in the Rayleigh limit, Kramers-Kronig relations, microwave emission mechanisms, and X-ray scattering. (3) IR and FIR emission: heating of interstellar dust, including single-photon heating, and resulting IR emission spectrum. (4) Charging of dust grains: collisional charging, photoelectric emission, and resulting charge distribution functions. (5) Dynamics: gas drag, Lorentz force, forces due to anisotropic radiation, and resulting drift velocities. (6) Rotational dynamics: brownian rotation, suprathermal rotation, and effects of starlight torques. (7) Alignment of interstellar dust: observations and theories. (8) Evolution of the grain population: dust formation in outflows, grain growth in the ISM, photodesorption, and grain destruction in shock waves. (9) Effects of dust grains: photoelectric heating, H2 formation, ion recombination, coupling of gas to magnetic fields, and dust grains as indicators of magnetic field direction.

  15. Department of Natural Resources and Water Divisions (Nebraska)

    Broader source: Energy.gov [DOE]

    This chapter describes the duties of the Department of Natural Resources and divides the state into two water divisions for administrative purposes. Water Division 1 consists of all the lands of...

  16. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT SMART GRID ROADMAP and Development Division funding efforts are focused on the following RD&D program areas: · Buildings EndUse Energy Efficiency · Renewable Energy Technologies · Transportation The Smart Grid Roadmap

  17. Nuclear Science Division Annual Report 1995-1996

    E-Print Network [OSTI]

    Authors, Various

    2010-01-01T23:59:59.000Z

    Saladin5, and C.H. Yu6 Nuclear Science Division, LawrenceMoretto, G.J. Wozniak, Nuclear Science Division, LawrenceComment on “Probing the Nuclear Liquid-Gas Phase Transition”

  18. Engineering Research Division publication report, calendar year 1980

    SciTech Connect (OSTI)

    Miller, E.K.; Livingston, P.L.; Rae, D.C. (eds.)

    1980-06-01T23:59:59.000Z

    Each year the Engineering Research Division of the Electronics Engineering Department at Lawrence Livermore Laboratory has issued an internal report listing all formal publications produced by the Division during the calendar year. Abstracts of 1980 reports are presented.

  19. Linking Sulfur Metabolism to the Cell Division Machinery in Yeast

    E-Print Network [OSTI]

    Blank, Heidi M.

    2010-07-14T23:59:59.000Z

    The longstanding view has been that metabolism allows for cell division to take place, but that metabolic processes do not actively promote cell division. I have recently challenged this notion by identifying a unique gain-of-function metabolic...

  20. Mesoscale & Microscale Meteorological Division / NCAR WRF Nature Run

    E-Print Network [OSTI]

    Michalakes, John

    Mesoscale & Microscale Meteorological Division / NCAR WRF Nature Run John Michalakes Josh Hacker overview and petascale issues Nature run methodology Results and conclusion #12;Mesoscale & Microscale's atmosphere #12;Mesoscale & Microscale Meteorological Division / NCAR Description of Science · Kinetic energy

  1. The mechanism of chloroplast division in higher plants

    E-Print Network [OSTI]

    Proctor, John Michael

    2013-02-22T23:59:59.000Z

    of chloroplasts found in a normal mesophyll cell. The process of chloroplast biogenesis has been well characterized at the cellular level, but the molecular basis of chloroplast division and the role of nuclear genes in the control of plastid division...

  2. ENVIRONMENT, SAFETY & HEALTH DIVISION Chapter 24: Training

    E-Print Network [OSTI]

    Wechsler, Risa H.

    ENVIRONMENT, SAFETY & HEALTH DIVISION Chapter 24: Training Quick Start Summary Product ID: 520-group.slac.stanford.edu/esh/eshmanual/references/trainingQuickstart.pdf 1 Who needs to know about these requirements The requirements of Training apply to all persons on-site, employees and non-employees, their SLAC

  3. West Virginia University Division of Human Resources

    E-Print Network [OSTI]

    Mohaghegh, Shahab

    Resources Web page hr.wvu.edu. In the event of a conflict between the current posted version and this printed copy, the posted version on the Web page is controlling. Page 1 of 9 Family Medical Leave Act Division of Human Resources Web page hr.wvu.edu. In the event of a conflict between the current posted

  4. Building an R package Division of Biostatistics

    E-Print Network [OSTI]

    Carlin, Bradley P.

    Building an R package Yen-Yi Ho Division of Biostatistics School of Public Health, University of Minnesota Yen-Yi Ho Building an R package #12;Steps Prepare your functions, example data sets Build package in man subdirectory) Write a package vignette Build and install the R package (R CMD build) Check the R

  5. Mentor Program Information Division of Biology

    E-Print Network [OSTI]

    Kaufman, Glennis A.

    Mentor Program Information Division of Biology 116 Ackert Hall Manhattan, KS 66506 Kansas State will never be released for public information unless requested by the mentor. It is used only if a current K-State student requests to speak with a specific mentor and is kept private until that time. However, it may

  6. University of Massachusetts Physical Plant Division

    E-Print Network [OSTI]

    Mountziaris, T. J.

    with all applicable rules and regulations. As of the date of this policy, the University of Massachusetts1 University of Massachusetts Amherst Physical Plant Division March 26, 2007 From: Pat Daly. To this end, the Property Office of the University of Massachusetts Amherst shall provide the Physical Plant

  7. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    (Chairman) F. Willeke, DESY 1. Follow up of previous Meeting The first report by the DANE Machine AdvisoryK K DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, May 11, 2000 Note: G-55 Report by DANE Machine Advisory Panel on 2nd Meeting held on 4-5 May 2000 J. M. Jowett, CERN S. Myers, CERN

  8. Materials Sciences Division 1990 annual report

    SciTech Connect (OSTI)

    Not Available

    1990-01-01T23:59:59.000Z

    This report is the Materials Sciences Division's annual report. It contains abstracts describing materials research at the National Center for Electron Microscopy, and for research groups in metallurgy, solid-state physics, materials chemistry, electrochemical energy storage, electronic materials, surface science and catalysis, ceramic science, high tc superconductivity, polymers, composites, and high performance metals.

  9. Lectures on Linear Algebra over Division Ring

    E-Print Network [OSTI]

    Aleks Kleyn

    2014-10-11T23:59:59.000Z

    In this book i treat linear algebra over division ring. A system of linear equations over a division ring has properties similar to properties of a system of linear equations over a field. However, noncommutativity of a product creates a new picture. Matrices allow two products linked by transpose. Biring is algebra which defines on the set two correlated structures of the ring. As in the commutative case, solutions of a system of linear equations build up right or left vector space depending on type of system. We study vector spaces together with the system of linear equations because their properties have a close relationship. As in a commutative case, the group of automorphisms of a vector space has a single transitive representation on a frame manifold. This gives us an opportunity to introduce passive and active representations. Studying a vector space over a division ring uncovers new details in the relationship between passive and active transformations, makes this picture clearer. Considering of twin representations of division ring in Abelian group leads to the concept of D vector space and their linear map. Based on polyadditive map I considered definition of tensor product of rings and tensor product of D vector spaces.

  10. Student Regulations and Procedures Academic Division

    E-Print Network [OSTI]

    Student Regulations and Procedures Academic Division 2007/2008 11 Students Union Code information regarding their course, tuition fees, award ceremonies and other matters www.mmu.ac.uk/academic's Articles of Government (Article 1.1). As prescribed in the Articles of Government (Article 12

  11. Student Regulations and Procedures Academic Division

    E-Print Network [OSTI]

    Student Regulations and Procedures Academic Division 2007/2008 3 RULES FOR STUDENT CONDUCT fees, award ceremonies and other matters www.mmu.ac.uk/academic/student_regulations.php #12;RULES of Governors in accordance with the following Articles of Government: 7.1.6 Subject to the responsibilities

  12. Division of Human Resources Termination Of

    E-Print Network [OSTI]

    Meyers, Steven D.

    Division of Human Resources Termination Of Domestic Partnership Health Stipend Questions (813) 974 Insurance Stipend will terminate as of the Effective Date on this Termination of Domestic Partnership Health. ______ The Domestic Partnership Declaration attested to and filed by me with USF shall be and is terminated

  13. Division of Student Affairs 107 Conklin North

    E-Print Network [OSTI]

    Moore, Paul A.

    A. Herman graduated from Bowling Green State University's College Student Personnel program in 1990, August 31st to the Office of the Division of Student Affairs, Bowling Green State University, Attn: Beth Bowling Green State University Shelli A. Herman graduated from Bowling Green State University's College

  14. DIVISION S-6--SOIL & WATER MANAGEMENT & CONSERVATION

    E-Print Network [OSTI]

    DIVISION S-6--SOIL & WATER MANAGEMENT & CONSERVATION Soil Organic Carbon Sequestration Rates soil column within 20 yr following culti- Carbon sequestration rates, with a change from CT to NT, can in approximately 40 to and returning to the original land cover or other peren- 60 yr. Carbon sequestration rates

  15. Earth Sciences Division annual report 1990

    SciTech Connect (OSTI)

    NONE

    1991-06-01T23:59:59.000Z

    This Annual Report presents summaries of selected representative research activities grouped according to the principal disciplines of the Earth Sciences Division: Reservoir Engineering and Hydrogeology, Geology and Geochemistry, and Geophysics and Geomechanics. Much of the Division`s research deals with the physical and chemical properties and processes in the earth`s crust, from the partially saturated, low-temperature near-surface environment to the high-temperature environments characteristic of regions where magmatic-hydrothermal processes are active. Strengths in laboratory and field instrumentation, numerical modeling, and in situ measurement allow study of the transport of mass and heat through geologic media -- studies that now include the appropriate chemical reactions and the hydraulic-mechanical complexities of fractured rock systems. Of particular note are three major Division efforts addressing problems in the discovery and recovery of petroleum, the application of isotope geochemistry to the study of geodynamic processes and earth history, and the development of borehole methods for high-resolution imaging of the subsurface using seismic and electromagnetic waves. In 1989 a major DOE-wide effort was launched in the areas of Environmental Restoration and Waste Management. Many of the methods previously developed for and applied to deeper regions of the earth will in the coming years be turned toward process definition and characterization of the very shallow subsurface, where man-induced contaminants now intrude and where remedial action is required.

  16. Ruiying Wu PhD Biosciences Division

    E-Print Network [OSTI]

    Kemner, Ken

    1 Ruiying Wu PhD Biosciences Division BIO-202 Argonne National Laboratory E-mail: rwu@anl.gov 9700 to millimeter wave National Natural Science Foundation of PR China (NSFC) #12;2 Grant # - 39970189 1998 ­ 2000 National Natural Science Foundation of PR China (NSFC) Grant # - 39770633 SELECTIVE HONORS AND AWARDS 1

  17. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    K K DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, 28 November, 2002 IR-12 together with the total losses around the rings. Results seem encouraging, as calculated loss rates at IR2 in details and compared to calculated losses for the KLOE and the DEAR cases. 1 Introduction Background rates

  18. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    K K DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, March 10, 1997 Note: BM-1 BUNCH current. This measurement allows to calculate energy losses due to parasitic beam-vacuum chamber losses. In this Note we present results of the measurements and their analysis, comparing the results

  19. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    KKKK KKKK DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, January 13, 1993 Note: IR to see how much heat has to be removed. The two main sources of heat are: 1) Resistive losses due. Technol. 5(6) 3446 (1987). #12;IR-1 pg. 6 APPENDIX IA Losses in the I.R. 1) Resistive losses in Be: dp dz

  20. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    KKKK KKKK DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, October 26, 1994 Note: RF enough (i.e. if the parasitic losses are low with respect to the energy left by each passing bunch-zero longitudinal electric field on the cavity axis. Being azimuthally symmetric, it is possible to calculate them

  1. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    K K DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, July 16, 1996 Note: RF-19 losses and prevents to reach the operating voltage range. The RF cavity of the DANE -Factory Accumulator and electrical conductivities. Multipactoring (MP) is a phenomenon of resonant electron discharge which can occur

  2. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    K K DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, December 14, 1995 Note: CD-5, are also needed in order to minimise the losses. In order to use this device as a transverse kicker, two) excitation. #12;CD-5 pg. 3 The combined magnetic and electric field gives a net deflecting Lorentz force

  3. DANE TECHNICAL NOTE INFN -LNF, Accelerator Division

    E-Print Network [OSTI]

    Istituto Nazionale di Fisica Nucleare (INFN)

    KKKK KKKK DANE TECHNICAL NOTE INFN - LNF, Accelerator Division Frascati, Sept. 26, 1991 Note: RF-4 and vacuum simpler and less expensive. The cavity will be made of copper which has better electrical and thermal conductivity to reduce the RF losses and keep the cooling easier. #12;RF-4 pg. 2 Multipacting (MP

  4. Division of Human Resources Payroll Certification Process

    E-Print Network [OSTI]

    Meyers, Steven D.

    Division of Human Resources Payroll Certification Process Questions (813) 974-7955 Payroll/Payroll Processing Rev. 04/2010 Payroll Certification is the process by which departments submit to Payroll the hours to be paid for each employee within each department. This process utilizes the online Certification System

  5. Tempe Transportation Division: LNG Turbine Hybrid Electric Buses

    SciTech Connect (OSTI)

    Not Available

    2002-02-01T23:59:59.000Z

    Fact sheet describes the performance of liquefied natural gas (LNG) turbine hybrid electric buses used in Tempe's Transportation Division.

  6. Energy Technology Division research summary 1997.

    SciTech Connect (OSTI)

    NONE

    1997-10-21T23:59:59.000Z

    The Energy Technology Division provides materials and engineering technology support to a wide range of programs important to the US Department of Energy. As shown on the preceding page, the Division is organized into ten sections, five with concentrations in the materials area and five in engineering technology. Materials expertise includes fabrication, mechanical properties, corrosion, friction and lubrication, and irradiation effects. Our major engineering strengths are in heat and mass flow, sensors and instrumentation, nondestructive testing, transportation, and electromechanics and superconductivity applications. The Division Safety Coordinator, Environmental Compliance Officers, Quality Assurance Representative, Financial Administrator, and Communication Coordinator report directly to the Division Director. The Division Director is personally responsible for cultural diversity and is a member of the Laboratory-wide Cultural Diversity Advisory Committee. The Division's capabilities are generally applied to issues associated with energy production, transportation, utilization or conservation, or with environmental issues linked to energy. As shown in the organization chart on the next page, the Division reports administratively to the Associate Laboratory Director (ALD) for Energy and Environmental Science and Technology (EEST) through the General Manager for Environmental and Industrial Technologies. While most of our programs are under the purview of the EEST ALD, we also have had programs funded under every one of the ALDs. Some of our research in superconductivity is funded through the Physical Research Program ALD. We also continue to work on a number of nuclear-energy-related programs under the ALD for Engineering Research. Detailed descriptions of our programs on a section-by-section basis are provided in the remainder of this book. This Overview highlights some major trends. Research related to the operational safety of commercial light water nuclear reactors (LWRS) is funded by the US Nuclear Regulatory Commission (NRC). In addition to our ongoing work on environmentally assisted cracking and steam generator integrity, a major new multiyear program has been initiated to assess the performance of high-burnup fuel during loss-of-coolant accidents. The bulk of the NRC research work is carried out in four ET sections: Corrosion: Mechanics of Materials; Irradiation Performance: and Sensors, Instrumentation, and Nondestructive Evaluation. The Transportation of Hazardous Materials Section is the other main contributor; staff from that Section have worked closely with NRC staff to draft a new version of the NRC Standard Review Plan that will be used to provide guidance to NRC reviewers of applications for the renewal of nuclear plant licenses.

  7. PORTFOLIO ALLOCATION REVIEW NSF DIVISION OF ASTRONOMICAL SCIENCES

    E-Print Network [OSTI]

    Ong, Rene A.

    . INTRODUCTION A. The State of Astronomy in the United States We are entering a golden age in the history been a convergence of, e.g., high-energy (particle) physics and astrophysics in particle- astrophysics with no clear rationale as to why that balance had been maintained. 3. Based upon findings (1) and (2

  8. INTRAMURAL GOLF TOURAMENT ALL DIVISIONS Fall 2011 Division Sunday Sept. 18

    E-Print Network [OSTI]

    Omiecinski, Curtis

    INTRAMURAL GOLF TOURAMENT ALL DIVISIONS Fall 2011 Division Sunday Sept. 18 GOLF M W Team Member ?? EMAIL Tee-Time FIRST NAME LAST NAME or F TEAM NAME @psu.edu 9:00 AM Matt McTague M last round mim5187 Frankie Kehs M last round fjk5012 Chase Roman M Tiger Wood cer197 Dustin Hartzel M Tiger Wood dnh124 9

  9. TO: HR and Business Contacts FROM: Division of Human Resources

    E-Print Network [OSTI]

    Almor, Amit

    MEMORANDUM TO: HR and Business Contacts FROM: Division of Human Resources DATE: October 25, 2013 RE: Human Resources Fall 2013 Forum The Division of Human Resources will sponsor an HR Forum from 1 to the Division of Human Resources' Organizational and Professional Development Office at hrtrain

  10. TO: HR and Business Contacts FROM: Division of Human Resources

    E-Print Network [OSTI]

    Almor, Amit

    TO: HR and Business Contacts FROM: Division of Human Resources DATE: September 6, 2012 RE: Human Resources Fall 2012 Forum The Division of Human Resources will sponsor an HR Forum from 1-4 p in person or by webinar. Any questions about the forum may be e-mailed to the Division of Human Resources

  11. MIT Plasma Science and Fusion Center Fusion Technology & Engineering Division

    E-Print Network [OSTI]

    Fusion Technology & Engineering Division 1. Costing of 4 "Reference" Options 2. Equalization of TF;MIT Plasma Science and Fusion Center Fusion Technology & Engineering Division Total Cost (M$) vs. A; MMIT Plasma Science and Fusion Center Fusion Technology & Engineering Division J.H. Schultz M

  12. DIVISION OF DRUG ABUSE CONTROL A Project Evaluation

    E-Print Network [OSTI]

    Touretzky, David S.

    L,: . -'" -- . : NARCONON 1/1 DIVISION OF DRUG ABUSE CONTROL FA-48-72 74-007 75-009 A Project. In Relation to the Stated Objectives of the Division of Drug Abuse Control's Application .......... II ........·..··.· Appendix C - NARCONON - Division of Drug Abuse Control Contract ..·.............·..... Appendix D - Job

  13. Charge exchange reactions and applications to astrophysics

    SciTech Connect (OSTI)

    Cheoun, Myung-Ki; Ha, Eunja; Kajino, T. [Department of Physics, Soongsil University, Seoul, 156-743 (Korea, Republic of); National Astronomical Observatory, Mitaka, Tokyo 181-8589 (Japan) and Department of Astronomy, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Tokyo 113-0033 (Japan)

    2012-11-12T23:59:59.000Z

    Neutrino-induced reactions have been known to play important roles as the neutrino process on the nucleosynthesis in core collapsing supernovae (SNe) explosions because expected neutrino flux and energy are sufficiently high enough to excite many relevant nuclei in spite of small cross sections of the weak interaction. However, we do not have enough data for the neutrino reaction to be exploited in the network calculation. Only a sparse data in the relevant energy range is known, in specific, for {sup 12}C. Therefore we have to rely on theoretical estimation of the reaction, which has two different modes, charge current (CC) and neutral current (NC). In particular, CC reactions are closely related to charge exchange reactions (CEXRs) which are feasible in the experiment, such as, (p,n) or (n,p) reactions. These CEXRs are usually dominated by the Gamow-Teller (GT) transition in the lower energy region. In this respect, any theoretical approaches for the neutrino reaction should be investigated for the CEXR because we have and expect more useful experimental data. After confirming our models to the GT strength deduced from the CEXR, we calculated neutrino-induced reactions in the energy range below the quasielastic region for nuclei of astrophysical importance. Our calculations are carried out with the Quasi-particle Random Phase Approximation (QRPA), which successfully described the nuclear beta decays of relevant nuclei. To describe neutrino-nucleus reactions, general multipole transitions by the weak interaction are considered for CC and NC reactions. Both reactions are described in a theoretical framework. Our results are shown to well reproduce the data from CEXRs and the sparse experimental data related to the neutrino-induced reaction, and further extended for neutrino reactions on various nuclear targets. Parts of the results are reported in this talk.

  14. The Planck Surveyor mission: astrophysical prospects

    E-Print Network [OSTI]

    G. De Zotti; L. Toffolatti; F. Argüeso; R. D. Davies; P. Mazzotta; R. B. Partridge; G. F. Smoot; N. Vittorio

    1999-03-27T23:59:59.000Z

    Although the Planck Surveyor mission is optimized to map the cosmic microwave background anisotropies, it will also provide extremely valuable information on astrophysical phenomena. We review our present understanding of Galactic and extragalactic foregrounds relevant to the mission and discuss on one side, Planck's impact on the study of their properties and, on the other side, to what extent foreground contamination may affect Planck's ability to accurately determine cosmological parameters. Planck's multifrequency surveys will be unique in their coverage of large areas of the sky (actually, of the full sky); this will extend by two or more orders of magnitude the flux density interval over which mm/sub-mm counts of extragalactic sources can be determined by instruments already available (like SCUBA) or planned for the next decade (like the LSA-MMA or the space mission FIRST), which go much deeper but over very limited areas. Planck will thus provide essential complementary information on the epoch-dependent luminosity functions. Bright radio sources will be studied over a poorly explored frequency range where spectral signatures, essential to understand the physical processes that are going on, show up. The Sunyaev-Zeldovich effect, with its extremely rich information content, will be observed in the direction of a large number of rich clusters of Galaxies. Thanks again to its all sky coverage, Planck will provide unique information on the structure and on the emission properties of the interstellar medium in the Galaxy. At the same time, the foregrounds are unlikely to substantially limit Planck's ability to measure the cosmological signals. Even measurements of polarization of the primordial Cosmic Microwave background fluctuations appear to be feasible.

  15. Environmental Effects for Gravitational-wave Astrophysics

    E-Print Network [OSTI]

    Enrico Barausse; Vitor Cardoso; Paolo Pani

    2015-01-07T23:59:59.000Z

    The upcoming detection of gravitational waves by terrestrial interferometers will usher in the era of gravitational-wave astronomy. This will be particularly true when space-based detectors will come of age and measure the mass and spin of massive black holes with exquisite precision and up to very high redshifts, thus allowing for better understanding of the symbiotic evolution of black holes with galaxies, and for high-precision tests of General Relativity in strong-field, highly dynamical regimes. Such ambitious goals require that astrophysical environmental pollution of gravitational-wave signals be constrained to negligible levels, so that neither detection nor estimation of the source parameters are significantly affected. Here, we consider the main sources for space-based detectors -- the inspiral, merger and ringdown of massive black-hole binaries and extreme mass-ratio inspirals -- and account for various effects on their gravitational waveforms, including electromagnetic fields, cosmological evolution, accretion disks, dark matter, "firewalls" and possible deviations from General Relativity. We discover that the black-hole quasinormal modes are sharply different in the presence of matter, but the ringdown signal observed by interferometers is typically unaffected. The effect of accretion disks and dark matter depends critically on their geometry and density profile, but is negligible for most sources, except for few special extreme mass-ratio inspirals. Electromagnetic fields and cosmological effects are always negligible. We finally explore the implications of our findings for proposed tests of General Relativity with gravitational waves, and conclude that environmental effects will not prevent the development of precision gravitational-wave astronomy.

  16. Fitting Narrow Spectral Lines in High Energy Astrophysics Using Incompatible Gibbs Samplers

    E-Print Network [OSTI]

    van Dyk, David

    for the data degradation processes (van Dyk et al., 2001). Efficient X-ray Spectral Fitting Hierarchical' & $ % Fitting Narrow Spectral Lines in High Energy Astrophysics Using Incompatible Gibbs Samplers Siemiginowska (Harvard-Smithsonian Center for Astrophysics, USA, aneta

  17. Biology Division progress report, October 1, 1993--September 30, 1995

    SciTech Connect (OSTI)

    NONE

    1995-10-01T23:59:59.000Z

    This Progress Report summarizes the research endeavors of the Biology Division of the Oak Ridge National Laboratory during the period October 1, 1993, through September 30, 1995. The report is structured to provide descriptions of current activities and accomplishments in each of the Division`s major organizational units. Lists of information to convey the entire scope of the Division`s activities are compiled at the end of the report. Attention is focused on the following research activities: molecular, cellular, and cancer biology; mammalian genetics and development; genome mapping program; and educational activities.

  18. Electromagnetically-Induced Frame-Dragging around Astrophysical Objects

    E-Print Network [OSTI]

    Ruiz, Andrés F Gutiérrez

    2015-01-01T23:59:59.000Z

    Frame dragging (Lense-Thirring effect) is generally associated with rotating astrophysical objects. However, it can also be generated by electromagnetic fields if electric and magnetic fields are simultaneously present. In most models of astrophysical objects, macroscopic charge neutrality is assumed and the entire electromagnetic field is characterized in terms of a magnetic dipole component. Hence, the purely electromagnetic contribution to the frame dragging vanishes. However, strange stars may posses independent electric dipole and neutron stars independent electric quadrupole moments that may lead to the presence of purely electromagnetic contributions to the frame dragging. Moreover, recent observations have shown that in stars with strong electromagnetic fields, the magnetic quadrupole may have a significant contribution to the dynamics of stellar processes. As an attempt to characterized and quantify the effect of electromagnetic frame-dragging in this kind of astrophysical objects, an analytic soluti...

  19. Experimental astrophysics with high power lasers and Z pinches

    SciTech Connect (OSTI)

    Remington, B A; Drake, R P; Ryutov, D D

    2004-12-10T23:59:59.000Z

    With the advent of high energy density (HED) experimental facilities, such as high-energy lasers and fast Z-pinch, pulsed-power facilities, mm-scale quantities of matter can be placed in extreme states of density, temperature, and/or velocity. This has enabled the emergence of a new class of experimental science, HED laboratory astrophysics, wherein the properties of matter and the processes that occur under extreme astrophysical conditions can be examined in the laboratory. Areas particularly suitable to this class of experimental astrophysics include the study of opacities relevant to stellar interiors; equations of state relevant to planetary interiors; strong shock driven nonlinear hydrodynamics and radiative dynamics, relevant to supernova explosions and subsequent evolution; protostellar jets and high Mach-number flows; radiatively driven molecular clouds and nonlinear photoevaporation front dynamics; and photoionized plasmas relevant to accretion disks around compact objects, such as black holes and neutron stars.

  20. Satio Hayakawa and dawn of high-energy astrophysics in Japan

    E-Print Network [OSTI]

    Nishimura, J

    2015-01-01T23:59:59.000Z

    Pioneering works and stimulation by S. Hayakawa for the development of high-energy astrophysics in Japan.

  1. Section III, Division 5 - Development and Future Directions

    SciTech Connect (OSTI)

    D. K. Morton; R I Jetter; James E Nestell; T. D. Burchell; T L (Sam) Sham

    2012-07-01T23:59:59.000Z

    This paper provides commentary on a new division under Section III of the ASME Boiler and Pressure Vessel (BPV) Code. This new Division 5 has an issuance date of November 1, 2011 and is part of the 2011 Addenda to the 2010 Edition of the BPV Code. The new Division covers the rules for the design, fabrication, inspection and testing of components for high temperature nuclear reactors. Information is provided on the scope and need for Division 5, the structure of Division 5, where the rules originated, the various changes made in finalizing Division 5, and the future near-term and long-term expectations for Division 5 development. Portions of this paper were based on Chapter 17 of the Companion Guide to the ASME Boiler & Pressure Vessel Code, Fourth Edition, © ASME, 2012, Reference.

  2. Physics division. Progress report, January 1, 1995--December 31, 1996

    SciTech Connect (OSTI)

    Stewart, M.; Bacon, D.S.; Aine, C.J.; Bartsch, R.R. [eds.] [comps.] [and others

    1997-10-01T23:59:59.000Z

    This issue of the Physics Division Progress Report describes progress and achievements in Physics Division research during the period January 1, 1995-December 31, 1996. The report covers the five main areas of experimental research and development in which Physics Division serves the needs of Los Alamos National Laboratory and the nation in applied and basic sciences: (1) biophysics, (2) hydrodynamic physics, (3) neutron science and technology, (4) plasma physics, and (5) subatomic physics. Included in this report are a message from the Division Director, the Physics Division mission statement, an organizational chart, descriptions of the research areas of the five groups in the Division, selected research highlights, project descriptions, the Division staffing and funding levels for FY95-FY97, and a list of publications and presentations.

  3. SUMMER Research Opportunity in Solar Astrophysics Important information meeting 11:00 Monday 9 March 2009

    E-Print Network [OSTI]

    Zita, E.J.

    Martin Solar and Astrophysics Laboratory (LMSAL) in Palo Alto, CA, is just down the road from StanfordSUMMER Research Opportunity in Solar Astrophysics Important information meeting 11:00 Monday 9 March 2009 Solar astrophysics is becoming even more exciting with the advent of new solar observing

  4. Chemical Technology Division. Annual technical report, 1995

    SciTech Connect (OSTI)

    Laidler, J.J.; Myles, K.M.; Green, D.W.; McPheeters, C.C.

    1996-06-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division`s activities during 1995 are presented. In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including advanced batteries and fuel cells; (2) methods for treatment of hazardous waste and mixed hazardous/radioactive waste; (3) the reaction of nuclear waste glass and spent fuel under conditions expected for an unsaturated repository; (4) processes for separating and recovering selected elements from waste streams, concentrating low-level radioactive waste streams with advanced evaporator technology, and producing {sup 99}Mo from low-enriched uranium; (5) electrometallurgical treatment of different types of spent nuclear fuel in storage at Department of Energy sites; and (6) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems.

  5. Earth Sciences Division annual report 1980

    SciTech Connect (OSTI)

    Not Available

    1981-07-01T23:59:59.000Z

    Summaries of the highlights of programs in the Earth Sciences Division are presented under four headings; Geosciences, Geothermal Energy Development, Nuclear Waste Isolation, and Marine Sciences. Utilizing both basic and applied research in a wide spectrum of topics, these programs are providing results that will be of value in helping to secure the nation's energy future. Separate abstracts have been prepared for each project for inclusion in the Energy Data Base. (DMC)

  6. Chemical Technology Division annual technical report, 1994

    SciTech Connect (OSTI)

    NONE

    1995-06-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division`s activities during 1994 are presented. In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including advanced batteries and fuel cells; (2) technology for fluidized-bed combustion; (3) methods for treatment of hazardous waste and mixed hazardous/radioactive waste; (4) the reaction of nuclear waste glass and spent fuel under conditions expected for an unsaturated repository; (5) processes for separating and recovering transuranic elements from waste streams, concentrating radioactive waste streams with advanced evaporator technology, and producing {sup 99}Mo from low-enriched uranium for medical applications; (6) electrometallurgical treatment of the many different types of spent nuclear fuel in storage at Department of Energy sites; and (8) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also conducts basic research in catalytic chemistry associated with molecular energy resources and novel ceramic precursors; materials chemistry of superconducting oxides, electrified metal/solution interfaces, molecular sieve structures, and impurities in scrap copper and steel; and the geochemical processes involved in mineral/fluid interfaces and water-rock interactions occurring in active hydrothermal systems. In addition, the Analytical Chemistry Laboratory in CMT provides a broad range of analytical chemistry support services to the technical programs at Argonne National Laboratory (ANL).

  7. Chemical Technology Division, Annual technical report, 1991

    SciTech Connect (OSTI)

    Not Available

    1992-03-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division`s activities during 1991 are presented. In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including advanced batteries and fuel cells; (2) technology for fluidized-bed combustion and coal-fired magnetohydrodynamics; (3) methods for treatment of hazardous and mixed hazardous/radioactive waste; (4) the reaction of nuclear waste glass and spent fuel under conditions expected for an unsaturated repository; (5) processes for separating and recovering transuranic elements from nuclear waste streams; (6) recovery processes for discharged fuel and the uranium blanket in the Integral Fast Reactor (IFR); (7) processes for removal of actinides in spent fuel from commercial water-cooled nuclear reactors and burnup in IFRs; and (8) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also conducts basic research in catalytic chemistry associated with molecular energy resources; chemistry of superconducting oxides and other materials of interest with technological application; interfacial processes of importance to corrosion science, catalysis, and high-temperature superconductivity; and the geochemical processes involved in water-rock interactions occurring in active hydrothermal systems. In addition, the Analytical Chemistry Laboratory in CMT provides a broad range of analytical chemistry support services to the technical programs at Argonne National Laboratory (ANL).

  8. Searches for Astrophysical and Cosmological Axions

    SciTech Connect (OSTI)

    Asztalos, S J; Rosenberg, L J; van Bibber, K; Sikivie, P; Zioutas, K

    2006-05-03T23:59:59.000Z

    The axion remains, after nearly 30 years, the most compelling and elegant solution to the strong-CP problem, i.e. why this symmetry is protected in QCD in spite of CP violation elsewhere. The axion is expected to be extremely light, and possess extraordinarily feeble couplings to matter and radiation. Because of its small couplings, the axion has defied experimental confirmation and is unlikely to be discovered in conventional laboratory experiments (i.e. production-detection). Nevertheless, a sufficiently light axion would have been produced abundantly in the Big Bang and is an excellent candidate for the dark matter of the Universe. Through the axion's two-photon coupling, implying axion-photon mixing in an external electromagnetic field, galactic halo axions may be feasibly detected by their resonant conversion to RF photons in a microwave cavity permeated by magnetic field with current technology. Over the past decade experiments have already set interesting limits in mass and coupling; upgrades in progress to photon detection schemes at or below the standard quantum limit will soon enable definitive searches. Similarly, axions produced in the solar burning core might be detectable by their conversion to x-rays in a magnetic helioscope. Indeed current published limits already equal the best bounds on axion-photon coupling inferred from the concordance of stellar evolution models and observations, from horizontal branch stars. Significant improvements in both the mass range and sensitivity of the axion helioscope technique will be forthcoming in the next few years. This report will first summarize the theoretical background of the axion, and laboratory, astrophysical and cosmological limits on its mass and couplings. Cavity microwave searches for cosmic axions will then be reviewed, focusing on the current large-scale experiments (ADMX in the US; CARRACK in Japan), and their enabling technologies (HFET and SQUID amplifiers; Rydberg-atom single-quantum detection). Last, the searches for solar axions will be discussed, with particular attention to the CAST experiment at CERN. The conclusion provides a basis for cautious optimism that a definitive verdict on the axion, or at least its role as a dark matter component, could be expected within a decade.

  9. [1] P.T. de Zeeuw and C. Hunter. Astrophysical Journal, 356:365, 1990. [2] C. Hunter and P.T. de Zeeuw. Astrophysical Journal, 389:79, 1992.

    E-Print Network [OSTI]

    Terzi, Bal?a

    REFERENCES [1] P.T. de Zeeuw and C. Hunter. Astrophysical Journal, 356:365, 1990. [2] C. Hunter and P.T. de Zeeuw. Astrophysical Journal, 389:79, 1992. [3] F. Bertola and M. Capacciolli. Astrophysical Journal, 200:439, 1975. [4] J. Binney. Comments Astrophysics, 8:27, 1978. [5] M. Schwarzschild

  10. Neutrinos, Rare Isotopes of Exotic Nuclei and Nuclear Astrophysics

    E-Print Network [OSTI]

    A. B. Balantekin

    2014-10-21T23:59:59.000Z

    The connection between neutrino physics, nucleosynthesis of elements in astrophysical sites, laboratory measurements with rare exotic nuclei and astronomical observations is discussed. The key role played by neutrinos is emphasized and the close connection between neutrino physics and nucleosynthesis is highlighted.

  11. AIAA20005175 THE SUN AS AN ASTROPHYSICAL LABORATORY

    E-Print Network [OSTI]

    Schrijver, Karel

    AIAA­2000­5175 THE SUN AS AN ASTROPHYSICAL LABORATORY Carolus J. Schrijver, Alan M. Title Stanford spacecraft to the effects of mass ejections. The variability of the Sun pro­ vides a unique opportunity. Time and again, the Sun has served as the foundation for our thinking about stars and other

  12. GLAST and Very High Energy astrophysics Berrie Giebels

    E-Print Network [OSTI]

    Boyer, Edmond

    Polytechnique - CNRS/IN2P3 F-91128 Palaiseau Cedex, France The pioneering age of high energy gamma-ray assembled and is scheduled for launch in 2007. At that point, gamma-ray astrophysics will enter again the status of the major Cerenkov telescopes has been pre- sented. By the time the Gamma ray Large Area

  13. Calibration in High-Energy Astrophysics Statistical Computation

    E-Print Network [OSTI]

    van Dyk, David

    : Effective area records sensitivity as a function of energy Energy redistribution matrix can vary with energy/location Point Spread Functions can vary with energy and location Exposure Map shows how effective area variesCalibration in High-Energy Astrophysics Statistical Computation Back to Calibration Uncertainty

  14. astrophysically interesting nuclear: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    astrophysically interesting nuclear First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 CALCULATIONS OF...

  15. The Astrophysical Journal, in press The XRay Sun in Time.

    E-Print Network [OSTI]

    Guedel, Manuel

    that are achieved on the Sun during short flaring episodes. In 2­temperature fits to ROSAT data, the higher distribution in temperature, with the hotter plasma at 12--30 MK and the cooler plasma below 10 MK. We inferThe Astrophysical Journal, in press The X­Ray Sun in Time. A Study of the Long­Term Evolution

  16. UNIVERSITY OF CALIFORNIA, SANTA CRUZ DEPARTMENT OF ASTRONOMY AND ASTROPHYSICS

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    , the solar system, stellar structure and evolution, planets, high energy astrophysics, extragalactic, Santa Cruz (UCSC) invites applications for an on-going pool of qualified part-time temporary lecturer contingent upon availability of funding. TO APPLY: Applications are accepted via the UCSC Academic Recruit

  17. (DOI: will be inserted by hand later) Astrophysics

    E-Print Network [OSTI]

    Boyer, Edmond

    1 (DOI: will be inserted by hand later) c ESO 2011 Astronomy & Astrophysics First stars XIV. Sulfur of the Galaxy. In particular the site of the formation remains uncertain because, at low metallicity, the trend of this -element versus [Fe/H] remains unclear. Moreover, although sulfur is not bound significantly in dust grains

  18. Astronomy & Astrophysics manuscript no. (will be inserted by hand later)

    E-Print Network [OSTI]

    Brun, Allan Sacha

    Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Seismic tests for solar, Homi Bhabha road, Mumbai 400005, India (antia@tifr.res.in) 4 Department of Physics, University computed accurate 1-D solar models including both a macro- scopic mixing process in the solar tachocline

  19. Trojan horse particle invariance: The impact on nuclear astrophysics

    SciTech Connect (OSTI)

    Pizzone, R. G.; La Cognata, M. [Laboratori Nazionali del Sud - INFN, Catania (Italy); Spitaleri, C. [Universitá di Catania and Laboratori Nazionali del Sud - INFN (Italy); Bertulani, C. A. [Texas A and M University, Commerce (United States); Mukhamedzhanov, A. M. [Texas A and M University, College Station, Texas (United States); Blokhintsev, L. D. [Moscow State University, Moscow (Russian Federation); Lamia, L.; Spartá, R. [Universitá di Catania and Laboratori Nazionali del Sud - INFN, Catania (Italy); Tumino, A. [Universitá Kore, Enna (Italy)

    2014-05-02T23:59:59.000Z

    In the current picture of nuclear astrophysics indirect methods and, in particular, the Trojan Horse Method cover a crucial role for the measurement of charged particle induced reactions cross sections of astrophysical interest, in the energy range required by the astrophysical scenarios. To better understand its cornerstones and its applications to physical cases many tests were performed to verify all its properties and the possible future perspectives. The key to the method is the quasi-free break-up and some of its properties will be investigated in the present work. In particular, the Trojan Horse nucleus invariance will be studied and previous studies will be extended to the cases of the binary d(d, p)t and {sup 6}Li(d,?){sup 4}He reactions, which were tested using different quasi-free break-up's, namely {sup 6}Li and {sup 3}He. The astrophysical S(E)-factor were then extracted with the Trojan Horse formalism applied to the two different break-up schemes and compared with direct data as well as with previous indirect investigations. The very good agreement confirms the independence of binary indirect cross section on the chosen spectator particle also for these reactions.

  20. Atmospheric and Geophysical Sciences Division: Program report, FY 1987

    SciTech Connect (OSTI)

    Not Available

    1988-05-01T23:59:59.000Z

    In 1988 the Atmospheric and Geophysical Sciences Division began its 15th year as a division. As the Division has grown over the years, its modeling capabilities have expanded to include a broad range of time and space scales ranging from hours to years, and from kilometers to global, respectively. For this report, we have chosen to show a subset of results from several projects to illustrate the breadth, depth, and diversity of the modeling activities that are a major part of the Division's research, development, and application efforts. In addition, the recent reorganization of the Division, including the merger of another group with the Division, is described, and the budget, personnel, models, and publications are reviewed. 95 refs., 26 figs., 2 tabs.

  1. New Stream-reach Development (NSD) Final Report | Department...

    Broader source: Energy.gov (indexed) [DOE]

    to help individuals and organizations evaluate the feasibility of developing new hydropower sources in the United States. New Stream-reach Development Report More Documents &...

  2. Chemical Technology Division annual technical report, 1986

    SciTech Connect (OSTI)

    Not Available

    1987-06-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division's activities during 1986 are presented. In this period, CMT conducted research and development in areas that include the following: (1) high-performance batteries - mainly lithium-alloy/metal sulfide and sodium/sulfur; (2) aqueous batteries (lead-acid, nickel/iron, etc.); (3) advanced fuel cells with molten carbonate or solid oxide electrolytes; (4) coal utilization, including the heat and seed recovery technology for coal-fired magnetohydrodynamics plants, the technology for fluidized-bed combustion, and a novel concept for CO/sub 2/ recovery from fossil fuel combustion; (5) methods for recovery of energy from municipal waste; (6) methods for the electromagnetic continuous casting of steel sheet; (7) techniques for treatment of hazardous waste such as reactive metals and trichloroethylenes; (8) nuclear technology related to waste management, a process for separating and recovering transuranic elements from nuclear waste, and the recovery processes for discharged fuel and the uranium blanket in a sodium-cooled fast reactor; and (9) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also has a program in basic chemistry research in the areas of catalytic hydrogenation and catalytic oxidation; materials chemistry for associated and ordered solutions at high temperatures; interfacial processes of importance to corrosion science, surface science, and catalysis; the thermochemistry of zeolites and related silicates; and the geochemical processes responsible for trace-element migration within the earth's crust. The Division continued to be the major user of the technical support provided by the Analytical Chemistry Laboratory at ANL. 127 refs., 71 figs., 8 tabs.

  3. Chemical technology division: Annual technical report 1987

    SciTech Connect (OSTI)

    Not Available

    1988-05-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division's activities during 1987 are presented. In this period, CMT conducted research and development in the following areas: (1) high-performance batteries--mainly lithium-alloy/metal sulfide and sodium/sulfur; (2) aqueous batteries (lead-acid, nickel/iron, etc.); (3) advanced fuel cells with molten carbonate or solid oxide electrolytes; (4) coal utilization, including the heat and seed recovery technology for coal-fired magnetohydrodynamics plants and the technology for fluidized-bed combustion; (5) methods for the electromagnetic continuous casting of steel sheet and for the purification of ferrous scrap; (6) methods for recovery of energy from municipal waste and techniques for treatment of hazardous organic waste; (7) nuclear technology related to a process for separating and recovering transuranic elements from nuclear waste, the recovery processes for discharged fuel and the uranium blanket in a sodium-cooled fast reactor, and waste management; and (8) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also has a program in basic chemistry research in the areas of fluid catalysis for converting small molecules to desired products; materials chemistry for liquids and vapors at high temperatures; interfacial processes of importance to corrosion science, high-temperature superconductivity, and catalysis; the thermochemistry of various minerals; and the geochemical processes responsible for trace-element migration within the earth's crust. The Division continued to be the major user of the technical support provided by the Analytical Chemistry Laboratory at ANL. 54 figs., 9 tabs.

  4. Chemical Technology Division annual technical report 1989

    SciTech Connect (OSTI)

    Not Available

    1990-03-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division's activities during 1989 are presented. In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including high-performance batteries (mainly lithium/iron sulfide and sodium/metal chloride), aqueous batteries (lead-acid and nickel/iron), and advanced fuel cells with molten carbonate and solid oxide electrolytes: (2) coal utilization, including the heat and seed recovery technology for coal-fired magnetohydrodynamics plants and the technology for fluidized-bed combustion; (3) methods for recovery of energy from municipal waste and techniques for treatment of hazardous organic waste; (4) nuclear technology related to a process for separating and recovering transuranic elements from nuclear waste and for producing {sup 99}Mo from low-enriched uranium targets, the recovery processes for discharged fuel and the uranium blanket in a sodium-cooled fast reactor (the Integral Fast Reactor), and waste management; and (5) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also has a program in basic chemistry research in the areas of fluid catalysis for converting small molecules to desired products; materials chemistry for superconducting oxides and associated and ordered solutions at high temperatures; interfacial processes of importance to corrosion science, high-temperature superconductivity, and catalysis; and the geochemical processes responsible for trace-element migration within the earth's crust. The Division continued to be administratively responsible for and the major user of the Analytical Chemistry Laboratory at Argonne National Laboratory (ANL).

  5. Physics division annual report - October 2000.

    SciTech Connect (OSTI)

    Thayer, K. [ed.

    2000-10-16T23:59:59.000Z

    This report summarizes the research performed in the past year in the Argonne Physics Division. The Division's programs include operation of ATLAS as a national heavy-ion user facility, nuclear structure and reaction research with beams of heavy ions, accelerator research and development especially in superconducting radio frequency technology, nuclear theory and medium energy nuclear physics. The Division took significant strides forward in its science and its initiatives for the future in the past year. Major progress was made in developing the concept and the technology for the future advanced facility of beams of short-lived nuclei, the Rare Isotope Accelerator. The scientific program capitalized on important instrumentation initiatives with key advances in nuclear science. In 1999, the nuclear science community adopted the Argonne concept for a multi-beam superconducting linear accelerator driver as the design of choice for the next major facility in the field a Rare Isotope Accelerator (RIA) as recommended by the Nuclear Science Advisory Committee's 1996 Long Range Plan. Argonne has made significant R&D progress on almost all aspects of the design concept including the fast gas catcher (to allow fast fragmentation beams to be stopped and reaccelerated) that in large part, defined the RIA concept the superconducting rf technology for the driver accelerator, the multiple-charge-state concept (to permit the facility to meet the design intensity goals with existing ion-source technology), and designs and tests of high-power target concepts to effectively deal with the full beam power of the driver linac. An NSAC subcommittee recommended the Argonne concept and set as tie design goal Uranium beams of 100-kwatt power at 400 MeV/u. Argonne demonstrated that this goal can be met with an innovative, but technically in-hand, design.

  6. Nuclear Science Division 1994 annual report

    SciTech Connect (OSTI)

    Myers, W.D. [ed.

    1995-06-01T23:59:59.000Z

    This report describes the activities of the Nuclear Science Division for the period of January 1, 1994, to December 31, 1994. This was a time of significant accomplishment for all of the programs in the Division. Assembly of the solar neutrino detector at the Sudbury Neutrino Observatory is well under way. All of the components fabricated by LBL were shipped to Sudbury early in the year and our efforts are now divided between assisting the assembly of the detector and preparing software for data analysis once the detector is operational in 1996. Much of the activity at the 88-Inch Cyclotron centered on Gammasphere. The {open_quotes}early implementation{close_quotes} phase of the detector ended in September. This phase was extremely successful, involving over 60 experiments with nearly 200 users from 37 institutions worldwide. The mechanical structure was installed and the final electronic system is expected to operate in March 1995. The Division concurrently hosted a conference on physics for large {gamma}-ray detector arrays at the Clark Kerr Campus at UC Berkeley in August. This was a very successful meeting, reflecting the enthusiasm for this field worldwide. Also at the Cyclotron, the progress toward weak interaction experiments using ultra-thin sources passed a major milestone with the trapping of radioactive {sup 21}Na atoms. We are now engaged in a major upgrade of the experimental area and the outlook is very promising for these novel experiments. Another highlight of research at the Cyclotron was the confirmation of element 106. This development allowed the original LLNL/LBL discovery team to move forward with their proposal to name this element seaborgium.

  7. Environmental Chemistry Division annual report, 1989

    SciTech Connect (OSTI)

    Newman, L.

    1990-01-01T23:59:59.000Z

    The research activities making up the programs in the Environmental Chemistry Division of the Department of Applied Science are presented. Some of the more significant accomplishments during 1989 are described and plans for 1990 are discussed briefly. Publications for the period are listed and abstracts are provided. Research objectives and principal investigators are given for each of the active programs. A list of personnel and collaborators during the past year is presented. The support distribution of FY 1989 is approximately 85% from the Department of Energy (65% Office of Health and Environmental Research), and 15% other agencies (principally from the Electric Power Research Institute).

  8. Oregon Public Health Division | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, searchOfRoseConcernsCompany Oil andOpenEITODOOregon Public Health Division Jump

  9. UGI Utilities Electric Division | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTri Global Energy LLC Place: Dallas,UGI Utilities Electric Division Jump

  10. Hawaii Department of Land and Natural Resources Division of Forestry...

    Open Energy Info (EERE)

    Name: Hawaii Department of Land and Natural Resources Division of Forestry and Wildlife Address: Kalanimoku Building 1151 Punchbowl St., Room 325 Place: Honolulu, Hawaii Zip:...

  11. California Public Resources Code Division 3, Chapter 4 - Geothermal...

    Open Energy Info (EERE)

    California Public Resources Code Division 3, Chapter 4 - Geothermal Resources Jump to: navigation, search OpenEI Reference LibraryAdd to library Legal Document- StatuteStatute:...

  12. UC ACADEMIC SENATE SANTA CRUZ DIVISION Committee on Educational Policy

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    UC ACADEMIC SENATE SANTA CRUZ DIVISION Committee on Educational Policy Policy on the Appointment. However, CEP believes that good educational policy requires that Senate faculty regularly teach

  13. Utah Division of Environmental Response and Remediation Underground...

    Open Energy Info (EERE)

    Environmental Response and Remediation Underground Storage Tank Branch Webpage Jump to: navigation, search OpenEI Reference LibraryAdd to library Web Site: Utah Division of...

  14. Vermont Agency of Natural Resources Wastewater Management Division...

    Open Energy Info (EERE)

    Vermont Agency of Natural Resources Wastewater Management Division Water Pollution Control Permit Regulations Jump to: navigation, search OpenEI Reference LibraryAdd to library...

  15. affairs division llnl: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Division of Student Affairs Biology and Medicine Websites Summary: of Disability Services Texas A&M University ATTN: Documentation Coordinator Mailstop 1224 College Station, Texas:...

  16. DIVISION OF ACADEMIC AFFAIRS OFFICE OF THE REGISTRAR

    E-Print Network [OSTI]

    AARH ARCH Facility Management FCMG COSC Global Art, Design, and Construction GADC ARCH Sustainable PETE PETE Radiological Health Engineering RHEN NUEN #12;DIVISION OF ACADEMIC AFFAIRS OFFICE

  17. applied science division: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Remediation & Water Resources Kenneth Hurst Williams 6 PAUL O. WENNBERG Division of Engineering and Applied Science Geosciences Websites Summary: Fellowship. LARGE PROJECTS:...

  18. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    supplies, dry cooling systi Energy Research and Development Division FINAL PROJECT REPORT INLET AIR SPRAY COOLINGUse Energy Efficiency · Renewable Energy Technologies · Transportation Inlet Air Spray Cooling

  19. Chapter 50 Division for Air Quality: General Administrative Procedures (Kentucky)

    Broader source: Energy.gov [DOE]

    Chapter 50 of the Division of Air Quality section within Energy and Environment Cabinet Department For Environmental Protection outlines the general administrative procedures for maintaining air...

  20. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT INTEGRATING BIOENERGETICS, SPACIAL · Transportation Integrating Bioenergetics, Spatial Scales, and Population Dynamics for Environmental Flow

  1. applied chemistry division: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    their independent research identity and become a chemistry research leader of the future. Funding for the most Oxford, University of 6 DIVISION OF MARINE AND ATMOSPHERIC CHEMISTRY...

  2. Occupational Hygiene & Chemical Safety Division Department of Environmental Health & Safety

    E-Print Network [OSTI]

    Machel, Hans

    Occupational Hygiene & Chemical Safety Division Department of Environmental Health & Safety Risk (most common ­ personal hygiene very important); d) storage ­ leaks; and e) waste ­ storage and disposal

  3. The Division of Student Affairs An Organizational Overview

    E-Print Network [OSTI]

    Howitt, Ivan

    The Division of Student Affairs An Organizational Overview FY14 #12;2 #12;3 An Organizational . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4 Organizational Profile

  4. Key Facts about the Biosciences Division | Argonne National Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    to understand biological mechanisms relevant to bioremediation, climate change, energy production, and the protection of human health. BiosciencesDivisionKeyFactsOct20...

  5. 64 _____________________________________Math & Computational Sciences Division High Performance Computing and Visualization

    E-Print Network [OSTI]

    Perkins, Richard A.

    64 _____________________________________Math & Computational Sciences Division High Performance Computing and Visualization Research and Development in Visual Analysis Judith Devaney Terrence Griffin John

  6. MATERIALS AND MOLECULAR RESEARCH DIVISION. ANNUAL REPORT 1980

    E-Print Network [OSTI]

    Searcy, Alan W.

    2010-01-01T23:59:59.000Z

    Staff Seminars in Metallurgy and Materials Science,University, Department of Metallurgy, Cleveland, OH, JuneMaterials Research," Metallurgy Division, Department of

  7. California Department of Conservation, Division of Oil, Gas,...

    Open Energy Info (EERE)

    Jump to: navigation, search Name: California Department of Conservation, Division of Oil, Gas, and Geothermal Resources Place: Sacramento, California Coordinates: 38.5815719,...

  8. LUCERNE FOODS LTD. (A Division of Canada Safeway Limited)

    E-Print Network [OSTI]

    Farrell, Anthony P.

    LUCERNE FOODS LTD. (A Division of Canada Safeway Limited) Processing Plant: 31122 South Fraser Way and Vegetable Processing Plant Location: Abbotsford, BC Job Description: Lucerne Foods, Clearbrook processing

  9. PART III DIVISION 13 PAGE 1 RUTGERS DESIGN STANDARDS MANUAL NOV 2008 DIVISION 13 SPECIAL CONSTRUCTION

    E-Print Network [OSTI]

    operating condition. The system #12;PART III DIVISION 13 PAGE 2 RUTGERS DESIGN STANDARDS MANUAL NOV 2008 detail battery calculations per NFPA 72. 4. Indicate all A/C, fans, Dampers to be monitored by fire alarm detailed battery calculations per the

  10. Chemical Technology Division annual technical report, 1993

    SciTech Connect (OSTI)

    Battles, J.E.; Myles, K.M.; Laidler, J.J.; Green, D.W.

    1994-04-01T23:59:59.000Z

    Chemical Technology (CMT) Division this period, conducted research and development in the following areas: advanced batteries and fuel cells; fluidized-bed combustion and coal-fired magnetohydrodynamics; treatment of hazardous waste and mixed hazardous/radioactive waste; reaction of nuclear waste glass and spent fuel under conditions expected for an unsaturated repository; separating and recovering transuranic elements, concentrating radioactive waste streams with advanced evaporators, and producing {sup 99}Mo from low-enriched uranium; recovering actinide from IFR core and blanket fuel in removing fission products from recycled fuel, and disposing removal of actinides in spent fuel from commercial water-cooled nuclear reactors; and physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also conducts basic research in catalytic chemistry associated with molecular energy resources and novel ceramic precursors; materials chemistry of superconducting oxides, electrified metal/solution interfaces, molecular sieve structures, thin-film diamond surfaces, effluents from wood combustion, and molten silicates; and the geochemical processes involved in water-rock interactions. The Analytical Chemistry Laboratory in CMT also provides a broad range of analytical chemistry support.

  11. Chemical Technology Division, Annual technical report, 1991

    SciTech Connect (OSTI)

    Not Available

    1992-03-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division's activities during 1991 are presented. In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including advanced batteries and fuel cells; (2) technology for fluidized-bed combustion and coal-fired magnetohydrodynamics; (3) methods for treatment of hazardous and mixed hazardous/radioactive waste; (4) the reaction of nuclear waste glass and spent fuel under conditions expected for an unsaturated repository; (5) processes for separating and recovering transuranic elements from nuclear waste streams; (6) recovery processes for discharged fuel and the uranium blanket in the Integral Fast Reactor (IFR); (7) processes for removal of actinides in spent fuel from commercial water-cooled nuclear reactors and burnup in IFRs; and (8) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also conducts basic research in catalytic chemistry associated with molecular energy resources; chemistry of superconducting oxides and other materials of interest with technological application; interfacial processes of importance to corrosion science, catalysis, and high-temperature superconductivity; and the geochemical processes involved in water-rock interactions occurring in active hydrothermal systems. In addition, the Analytical Chemistry Laboratory in CMT provides a broad range of analytical chemistry support services to the technical programs at Argonne National Laboratory (ANL).

  12. TO: HR and Business Contacts FROM: Division of Human Resources

    E-Print Network [OSTI]

    Almor, Amit

    TO: HR and Business Contacts FROM: Division of Human Resources DATE: September 24, 2012 RE: Reminder: Human Resources Fall 2012 Forum This is a reminder that you will need to register online by the Division of Human Resources, this forum will include information about benefits updates to annual

  13. NUCLEAR SCIENCE AND TECHNOLOGY DIVISION OAK RIDGE NATIONAL LABORATORY

    E-Print Network [OSTI]

    McDonald, Kirk

    NUCLEAR SCIENCE AND TECHNOLOGY DIVISION OAK RIDGE NATIONAL LABORATORY U.S. DEPARTMENT OF ENERGY Rennich, Phil Spampinato (spampinatop@ornl.gov, 865-576-5267) Equipment Decommissioning and Disposition September 1, 2004 Oak Ridge National Laboratory #12;2 NUCLEAR SCIENCE AND TECHNOLOGY DIVISION OAK RIDGE

  14. BUSINESS AND ACCOUNTANCY DIVISION 2003-2005 CATALOG UPDATE

    E-Print Network [OSTI]

    Gering, Jon C.

    BUSINESS AND ACCOUNTANCY DIVISION 2003-2005 CATALOG UPDATE Changes effective 2004-2005 Accounting the following admission requirements before enrolling in upper division business and/or accounting courses: 1 and Debate COMM 381 Business and Professional Communication STAT 190 Basic Statistics OR STAT 290 Statistics

  15. Division of Human Resources Retirement Renewed Membership & Reemployment Restrictions

    E-Print Network [OSTI]

    Meyers, Steven D.

    Division of Human Resources Retirement Renewed Membership & Reemployment Restrictions Questions employer after you have been retired for 12 calendar months. #12;Division of Human Resources Retirement Renewed Membership & Reemployment Restrictions Questions (813) 974-2970 Rev. 02/2012 If you are reemployed

  16. LIBRARY COMMITTEE BERKELEY DIVISION of the ACADEMIC SENATE

    E-Print Network [OSTI]

    California at Berkeley, University of

    LIBRARY COMMITTEE BERKELEY DIVISION of the ACADEMIC SENATE Annual Report 1996-97 The Library administration of the Library and perform[ing] such other duties relative to the Library as may be committed to the Division." · In accordance with this charge, the Library Committee took action on the following topics

  17. CONDENSED MATTER THEORIST, MATERIALS SCIENCE DIVISION ARGONNE NATIONAL LABORATORY

    E-Print Network [OSTI]

    6/29/11 CONDENSED MATTER THEORIST, MATERIALS SCIENCE DIVISION ARGONNE NATIONAL LABORATORY Argonne Division, preferably by e-mail (norman@anl.gov), otherwise by regular mail (MSD-223, Argonne National Lab, Argonne, IL 60439). Please use the subject line "CMT Search" in any e-mail correspondence. Argonne

  18. JSME TED Newsletter, No.40, 2003 JSME Thermal Engineering Division

    E-Print Network [OSTI]

    Kandlikar, Satish

    JSME TED Newsletter, No.40, 2003 JSME Thermal Engineering Division THERMAL ENGINEERING TED Newsletter on the WEB Thermal Engineering Division Newsletter No.40 July 2003 Contents [Japanese versionth ASME-JSME Thermal Engineering Joint Conference (AJTEC-2003) Prof. Shigefumi NISHIO (University

  19. Southwest Research Institute Signal Exploitation and Geolocation Division

    E-Print Network [OSTI]

    Chapman, Clark R.

    Southwest Research Institute ® Signal Exploitation and Geolocation Division CERTIFIED TO ISO 9001:2008 BY LLOYD'S REGISTER QUALITY ASSURANCE APRIL 1, 2012 CERTIFICATE NUMBER: UQA 0111601 ISO 9001:2008 Quality to have the division quality management system certified to the stringent quality standards of ISO 9001

  20. ADVANCED LIGHT SOURCE DIVISION FY2008 SELF-ASSESSMENT REPORT

    E-Print Network [OSTI]

    Knowles, David William

    ....................................................................3 E4. Division participates in pollution prevention, energy conservation, recycling, and wasteADVANCED LIGHT SOURCE DIVISION FY2008 SELF-ASSESSMENT REPORT November 7, 2008 Prepared by to confined space, energized electrical work); waste management criteria (SAAs, waste sampling, NCARs

  1. Software & Services Group Developer Products Division Copyright 2011, Intel Corporation. All rights reserved.

    E-Print Network [OSTI]

    California at Berkeley, University of

    Software & Services Group Developer Products Division Copyright© 2011, Intel Corporation. All & Services Group Developer Products Division Copyright© 2011, Intel Corporation. All rights reserved. *Other Division Copyright© 2011, Intel Corporation. All rights reserved. *Other brands and names are the property

  2. Boston University College of Engineering Division of Materials Science and Engineering

    E-Print Network [OSTI]

    Lin, Xi

    Boston University College of Engineering Division of Materials Science and Engineering Annual | Division of Materials Science and Engineering | Highlights | 1 Message from the Division Head Boston University has many interdisciplinary research activities in materials science and engineering, spanning

  3. STATUS OF GEOTHERMAL RESERVOIR ENGINEERING RESEARCH PROJECTS SUPPORTED BY USDOE/DIVISION OF GEOTHERMAL ENERGY

    E-Print Network [OSTI]

    Howard, J.H.

    2011-01-01T23:59:59.000Z

    BY USDOE/DIVISION OF GEOTHERMAL ENERGY J J. H. Howard and W.BY USWE/DIVISION O GEOTHERMAL ENERGY F Berkeley, CaliforniaWE), Division of Geothermal Energy (mS) proposed that

  4. High-energy Astrophysics and the Virtual Observatory

    E-Print Network [OSTI]

    P. Padovani

    2005-07-26T23:59:59.000Z

    The Virtual Observatory (VO) will revolutionise the way we do Astronomy by allowing easy access to all astronomical data and by making the handling and analysis of datasets at various locations across the globe much simpler and faster. I report here on the need for the VO and its status in Europe, concentrating on the recently started EURO-VO project, and then give two specific applications of VO tools to high-energy astrophysics.

  5. Magnetohydrodynamic Particle Acceleration Processes: SSX Experiments, Theory, and Astrophysical Applications

    SciTech Connect (OSTI)

    Brown, Michael R.

    2006-11-16T23:59:59.000Z

    Project Title: Magnetohydrodynamic Particle Acceleration Processes: SSX Experiments, Theory, and Astrophysical Applications PI: Michael R. Brown, Swarthmore College The purpose of the project was to provide theoretical and modeling support to the Swarthmore Spheromak Experiment (SSX). Accordingly, the theoretical effort was tightly integrated into the SSX experimental effort. During the grant period, Michael Brown and his experimental collaborators at Swarthmore, with assistance from W. Matthaeus as appropriate, made substantial progress in understanding the physics SSX plasmas.

  6. Statistical Issues in Astrophysical Searches for Particle Dark Matter

    E-Print Network [OSTI]

    Jan Conrad

    2014-10-14T23:59:59.000Z

    In this review statistical issues appearing in astrophysical searches for particle dark matter, i.e. indirect detection (dark matter annihilating into standard model particles) or direct detection (dark matter particles scattering in deep underground detectors) are discussed. One particular aspect of these searches is the presence of very large uncertainties in nuisance parameters (astrophysical factors) that are degenerate with parameters of interest (mass and annihilation/decay cross sections for the particles). The likelihood approach has become the most powerful tool, offering at least one well motivated method for incorporation of nuisance parameters and increasing the sensitivity of experiments by allowing a combination of targets superior to the more traditional data stacking. Other statistical challenges appearing in astrophysical searches are to large extent similar to any new physics search, for example at colliders, a prime example being the calculation of trial factors. Frequentist methods prevail for hypothesis testing and interval estimation, Bayesian methods are used for assessment of nuisance parameters and parameter estimation in complex parameter spaces. The basic statistical concepts will be exposed, illustrated with concrete examples from experimental searches and caveats will be pointed out.

  7. Biology and Medicine Division annual report, 1985

    SciTech Connect (OSTI)

    Not Available

    1986-04-01T23:59:59.000Z

    This book briefly describes the activities of the Biology and Medicine Division of the Lawrence Berkeley Laboratory. During the past year the Donner Pavilion program on the treatment of arteriovenous malformations in the brain has chalked up very significant successes. The disease control rate has been high and objective measures of success using cerebral angiography have been established. The new high resolution positron emitting tomographic imager has been demonstrated to operate successfully. In the Radiation Biophysics program, the availability of higher mass ions up to uranium has allowed us cell and tissue studies in a radiation domain that is entirely new. Using uranium beams, investigators have already made new and exciting findings that are described in the body of the report.

  8. Integrated switch for simultaneous mode-division multiplexing (MDM) and wavelength-division multiplexing (WDM)

    E-Print Network [OSTI]

    Stern, Brian; Chen, Christine P; Tzuang, Lawrence D; Cardenas, Jaime; Bergman, Keren; Lipson, Michal

    2015-01-01T23:59:59.000Z

    Leveraging the spatial modes of multimode waveguides using mode-division multiplexing (MDM) on an integrated photonic chip allows unprecedented scaling of bandwidth density for on-chip communication. Switching channels between waveguides is critical for future scalable optical networks, but its implementation in multimode waveguides must address how to simultaneously control modes with vastly different optical properties. Here we present a platform for switching signals between multimode waveguides based on individually processing the spatial mode channels using single-mode elements. Using this wavelength-division multiplexing (WDM) compatible platform, we demonstrate a 1x2 multimode switch for a silicon chip which routes four data channels with low (power penalties below 1.4 dB on all channels while routing 10 Gbps data when each channel is input and routed separately. The switch exhibits an additional power penalty of less than 2.4 dB when all f...

  9. Chemical Technology Division annual technical report, 1990

    SciTech Connect (OSTI)

    Not Available

    1991-05-01T23:59:59.000Z

    Highlights of the Chemical Technology (CMT) Division's activities during 1990 are presented. In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including advanced batteries and fuel cells; (2) technology for coal- fired magnetohydrodynamics and fluidized-bed combustion; (3) methods for recovery of energy from municipal waste and techniques for treatment of hazardous organic waste; (4) the reaction of nuclear waste glass and spent fuel under conditions expected for a high-level waste repository; (5) processes for separating and recovering transuranic elements from nuclear waste streams, concentrating plutonium solids in pyrochemical residues by aqueous biphase extraction, and treating natural and process waters contaminated by volatile organic compounds; (6) recovery processes for discharged fuel and the uranium blanket in the Integral Fast Reactor (IFR); (7) processes for removal of actinides in spent fuel from commercial water-cooled nuclear reactors and burnup in IFRs; and (8) physical chemistry of selected materials in environments simulating those of fission and fusion energy systems. The Division also has a program in basic chemistry research in the areas of fluid catalysis for converting small molecules to desired products; materials chemistry for superconducting oxides and associated and ordered solutions at high temperatures; interfacial processes of importance to corrosion science, high-temperature superconductivity, and catalysis; and the geochemical processes responsible for trace-element migration within the earth's crust. The Analytical Chemistry Laboratory in CMT provides a broad range of analytical chemistry support services to the scientific and engineering programs at Argonne National Laboratory (ANL). 66 refs., 69 figs., 6 tabs.

  10. Physics Division annual review, 1 April 1979-31 March 1980

    SciTech Connect (OSTI)

    Not Available

    1980-01-01T23:59:59.000Z

    The Physics Division Annual Review presents a broad but necessarily incomplete view of the research activity within the Division for the year ending March 1980.

  11. EFFECTS OF POLLUTANTS ON BIOLOGICAL SYSTEMS. CHAPTER FROM THE ENERGY AND ENVIRONMENT DIVISION ANNUAL REPORT 1979

    E-Print Network [OSTI]

    Authors, Various

    2010-01-01T23:59:59.000Z

    to DOE Division of Geothermal Energy, January 30, 1980.in utilization of geothermal energy that adequate andthe DOE Division of Geothermal Energy. S. L. Phillips and E.

  12. E-Print Network 3.0 - astrophysics gravitational waves Sample...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    position in astrophysics 3D supercomputer simulation of the formation Summary: , Gamma-ray bursts, nucleosynthesis, sources of gravitational waves and computational methods....

  13. The Madison plasma dynamo experiment: A facility for studying laboratory plasma astrophysics

    E-Print Network [OSTI]

    Cooper, C. M.

    The Madison plasma dynamo experiment (MPDX) is a novel, versatile, basic plasma research device designed to investigate flow driven magnetohydrodynamic instabilities and other high-? phenomena with astrophysically relevant ...

  14. Particle Physics & Astrophysics David MacFarlane, Director

    E-Print Network [OSTI]

    Wechsler, Risa H.

    Division Head CDMS Richard Partridge Dept Head KIPAC Computing Stuart Marshall Dept Head DES David Burke Services Mgr. Debbie Tryforos Assistant to the Director Sensors & Detectors Chris Kenney Dept Head Redwood Conference Rooms SLUO Debbie Tryforos Assistant to the Director HEP Faculty Coordiantor Assistant

  15. Energy Division progress report, fiscal years 1994--1995

    SciTech Connect (OSTI)

    Moser, C.I. [ed.

    1996-06-01T23:59:59.000Z

    At ORNL, the Energy Division`s mission is to provide innovative solutions to energy and related issues of national and global importance through interdisciplinary research and development. Its goals and accomplishments are described in this progress report for FY 1994 and FY 1995. The Division`s expenditures in FY 1995 totaled 44.9 million. Sixty percent of the divisions work was supported by the US DOE. Other significant sponsors include the US DOT, the US DOD, other federal agencies, and some private organizations. The Division`s programmatic activities cover three main areas: (1) analysis and assessment, (2) transportation systems, and (3) energy use and delivery technologies. Analysis and assessment activities involve energy and resource analysis, preparation of environmental assessments and impact statements, and impact statements, research on emergency preparedness, analysis of energy and environmental needs in developing countries, and transportation analysis. Transportation systems research seeks to improve the quality of both civilian and military transportation efforts. Energy use and delivery technologies focus on building equipment, building envelopes, (walls, roofs, attics, and materials), improvement of energy efficiency in buildings, and electric power systems.

  16. Environmental Research Division technical progress report: January 1986--October 1987

    SciTech Connect (OSTI)

    Not Available

    1988-07-01T23:59:59.000Z

    Technical process in the various research activities of Argonne National Laboratory's Environmental Research Division is reported for the period 1986-1987. Textual, graphic, and tabular information is used to briefly summarize (in separate chapters) the work of the Division's Atmospheric Physics, Environmental Effects Research, Fundamental Molecular Physics and Chemistry, and Organic Geochemistry and Environmental Instrumentation Programs. Information on professional qualifications, awards, and outstanding professional activities of staff members, as well as lists of publications, oral presentations, special events organized, and participants in educational programs, are provided in appendices at the end of each chapter. Individual projects under each division are processed separately for the data bases.

  17. December 6

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    new hardware is in production including pdsfdtn2. Next procurement will probably be in early 2012. Shares: Shares have been calculated and sent to NSD and Physics Division for...

  18. Nuclear Engineer

    Broader source: Energy.gov [DOE]

    This position is located in the Nuclear Safety Division (NSD) which has specific responsibility for managing the development, analysis, review, and approval of non-reactor nuclear facility safety...

  19. Oblique propagation of nonlinear electrostatic waves in dense astrophysical magnetoplasmas

    SciTech Connect (OSTI)

    Masood, W.; Siddiq, M. [Theoretical Plasma Physics Division, PINSTECH, P. O. Nilore, Islamabad 54000 (Pakistan); National Centre for Physics (NCP), Shahdara Valley Road, 44000, Islamabad (Pakistan); Rizvi, H. [Theoretical Plasma Physics Division, PINSTECH, P. O. Nilore, Islamabad 54000 (Pakistan)

    2011-10-15T23:59:59.000Z

    Nonlinear quantum ion-acoustic waves in dense dissipative as well as non-dissipative magnetized plasmas are investigated employing the quantum hydrodynamic model. In this regard, Zakharov Kuznetsov Burgers equation is derived in quantum plasmas, for the first time, using the small amplitude perturbation expansion method. The unique features of nonlinear electrostatic structures in pure electron-ion quantum magnetoplasma are highlighted and the parametric domain of the applicability of the model is unequivocally expressed. The present study may be useful to understand the nonlinear propagation characteristics of electrostatic shock and solitary structures in dense astrophysical systems where the quantum effects are expected to dominate.

  20. Direct reactions for nuclear structure and nuclear astrophysics

    SciTech Connect (OSTI)

    Jones, Katherine Louise [University of Tennessee

    2014-12-18T23:59:59.000Z

    Direct reactions are powerful probes for studying the atomic nucleus. Modern direct reaction studies are illuminating both the fundamental nature of the nucleus and its role in nucleosynthetic processes occurring in the cosmos. This report covers experiments using knockout reactions on neutron-deficient fragmentation beams, transfer reactions on fission fragment beams, and theoretical sensitivity studies relating to the astrophysical r-process. Results from experiments on 108,106Sn at the NSCL, and on 131Sn at HRIBF are presented as well as the results from the nucleosynthesis study.

  1. Tomorrow optical interferometry: astrophysical prospects and instrumental issues

    E-Print Network [OSTI]

    F. Malbet

    2006-09-14T23:59:59.000Z

    Interferometry has brought many new constraints in optical astronomy in the recent years. A major leap in this field is the opening of large interferometric facilities like the Very Large Telescope Interferometer and the Keck Interferometer to the astronomical community. Planning for the future is both easy --most specialists know in which directions to develop interferometry-- and difficult because of the increasing complexity of the technique. I present a short status of interferometry today. Then I detail the possible astrophysical prospects. Finally I address some important instrumental issues that are decisive for the future of interferometry.

  2. The Astrophysical Virtual Observatory to EURO-VO Transition

    E-Print Network [OSTI]

    P. Padovani

    2005-11-09T23:59:59.000Z

    The Astrophysical Virtual Observatory (AVO) initiative, jointly funded by the European Commission and six European organisations, had the task of creating the foundations of a regional scale infrastructure by conducting a research and demonstration programme on the VO scientific requirements and necessary technologies. The AVO project is now formally concluded. I highlight AVO's main achievements and then describe its successor, the EURO-VO project. With its three new interlinked structures, the Data Centre Alliance, the Facility Centre, and the Technology Centre, the EURO-VO is the logical next step for the deployment of an operational VO in Europe.

  3. Atomic data for astrophysics. Calculations, benchmarking and distribution

    SciTech Connect (OSTI)

    Del Zanna, G. [Department of Applied Mathematics and Theoretical Physics University of Cambridge Wilberforce Road, Cambridge, CB3 0WA (United Kingdom)

    2012-05-25T23:59:59.000Z

    Some recent R-matrix and distorted-wave calculations, done as part of the UK APAPNetwork, are presented. They are focused on some ions important for the EUV and the X-rays, in particular for the solar corona. A long-term and novel project to benchmark atomic data against laboratory and astrophysical data is summarised, highlighting new plasma diagnostics. The various ways in which the atomic data are made available to the various communities through e.g. the CHIANTI and the VAMDC EU framework are also presented.

  4. Astrophysical search strategies for accelerator blind dark matter

    E-Print Network [OSTI]

    James D. Wells

    1998-08-06T23:59:59.000Z

    A weakly interacting dark-matter particle may be difficult to discover at an accelerator because it either (1) is too massive, (2) has no standard-model gauge interactions, or (3) is almost degenerate with other states. In each of these cases, searches for annihilation products in the Galactic halo are useful probes of dark-matter properties. Using the example of supersymmetric dark matter, I discuss how astrophysical searches for dark matter may provide discovery and mass information inaccessible to collider physics programs such as the Tevatron and LHC.

  5. Chemical Technology Division annual technical report, 1992

    SciTech Connect (OSTI)

    Battles, J.E.; Myles, K.M.; Laidler, J.J.; Green, D.W.

    1993-06-01T23:59:59.000Z

    In this period, CMT conducted research and development in the following areas: (1) electrochemical technology, including advanced batteries and fuel cells; (2) technology for fluidized-bed combustion and coal-fired magnetohydrodynamics; (3) methods for treatment of hazardous waste, mixed hazardous/radioactive waste, and municipal solid waste; (4) the reaction of nuclear waste glass and spent fuel under conditions expected for an unsaturated repository; (5) processes for separating and recovering transuranic elements from nuclear waste streams, treating water contaminated with volatile organics, and concentrating radioactive waste streams; (6) recovery processes for discharged fuel and the uranium blanket in the Integral Fast Reactor (EFR); (7) processes for removal of actinides in spent fuel from commercial water-cooled nuclear reactors and burnup in IFRs; and (8) physical chemistry of selected materials (corium; Fe-U-Zr, tritium in LiAlO{sub 2} in environments simulating those of fission and fusion energy systems. The Division also conducts basic research in catalytic chemistry associated with molecular energy resources and novel` ceramic precursors; materials chemistry of superconducting oxides, electrified metal/solution interfaces, and molecular sieve structures; and the geochemical processes involved in water-rock interactions occurring in active hydrothermal systems. In addition, the Analytical Chemistry Laboratory in CMT provides a broad range of analytical chemistry support services to the technical programs at Argonne National Laboratory (ANL).

  6. EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CERN PS DIVISION

    E-Print Network [OSTI]

    Boyer, Edmond

    EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH CERN ­ PS DIVISION CERN/PS 2002-016 (AE) CLIC Note 514 practically conserved. However EGUN simulations have been performed to ensure electron laminar flow

  7. Updated November 1, 2013 Division of Agriculture, Forestry,

    E-Print Network [OSTI]

    Ray, David

    Updated November 1, 2013 Division of Agriculture, Forestry, and Veterinary Medicine Administrative, & Aquaculture Dr. Eric Dibble (Interim) Forest Products Dr. Rubin Shmulsky Forestry Dr. Andrew Ezell Associate Turner Assistant Dean Vacant Director, Agricultural & Forestry Experiment Station Dr. George Hopper

  8. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Modeling, Landscape Genetics, and Habitat Connectivity for the Mohave Ground Squirrel to Guide Renewable Energy Research and Development Division FINAL PROJECT REPORT Habitat Energy Development JANUARY 2013 CEC5002014003 Prepared for: California Energy Commission Prepared

  9. Earth Sciences Division annual report 1981. [Lead abstract

    SciTech Connect (OSTI)

    Not Available

    1982-09-01T23:59:59.000Z

    Separate abstracts were prepared for the 59 papers of the 1981 annual report of the Earth Sciences Division at Lawrence Berkeley Laboratory. The general topics covered included nuclear waste isolation, geophysics and reservoir engineering, and geosciences. (KRM)

  10. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT SAIC SOLAR DISHUse Energy Efficiency · Energy Innovations Small Grants · EnergyRelated Environmental Research · EnergyUse Energy Efficiency · Renewable Energy Technologies · Transportation Solar Dish Concentrator

  11. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT HYBRID SOLAR LIGHTINGUse Energy Efficiency · Energy Innovations Small Grants · EnergyRelated Environmental Research · EnergyUse Energy Efficiency · Renewable Energy Technologies · Transportation Hybrid Solar Lighting

  12. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Commission Marla Mueller Contract Manager Guido Franco Program Area Lead Energy-Related Environmental Energy Research and Development Division FINAL PROJECT REPORT A SEASONAL DECEMBER 2011 CEC5002013035 Prepared for: California Energy Commission Prepared by: Lawrence Berkeley

  13. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    CEC5002013042 Prepared for: California Energy Commission Prepared by: Lawrence Berkeley National · EnergyRelated Environmental Research · Energy Systems Integration · Environmentally Preferred Advanced. The information from this project contributes to Energy Research and Development Division's Buildings End

  14. Title 14 CCR, Division 2, Chapter 4 - Development, Regulation...

    Open Energy Info (EERE)

    4 CCR, Division 2, Chapter 4 - Development, Regulation, and Conservation of Oil and Gas Resources Jump to: navigation, search OpenEI Reference LibraryAdd to library Legal Document-...

  15. Agricultural Engineering and Socio-Economics Division Field Contents Member

    E-Print Network [OSTI]

    Banbara, Mutsunori

    Agricultural Engineering and Socio-Economics Division Field Contents Member Environmental, H. Professor TADA,A.Associate Professor Geotechnical and Environmental Engineering for Agricultural for agricultural land and rural areas including bountiful beautiful nature; Geotechnical and environmental

  16. Sustainability attheUniversityofPittsburgh Facilities Management Division

    E-Print Network [OSTI]

    Jiang, Huiqiang

    Sustainability attheUniversityofPittsburgh Facilities Management Division Updated January 2014 #12;SustainabilityattheUniversityofPittsburgh · Sustainable Design and Construction · Energy Conservation · Pollution/Emissions Reduction · Greening of the Campus · Recycling #12;SustainableDesignand Construction Design Standards · FM

  17. Page 1 of 3 Acquisition Services Management (ASM) Division

    E-Print Network [OSTI]

    Page 1 of 3 Acquisition Services Management (ASM) Division Subcontracts, ASM-SUB P.O. Box 1663 within the benchmark codes require numbers of MPI ranks which are not practical on a single node

  18. IT Division's Julie Petersen Attends Networking Conference with...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    1 800-333-7638 (Inside the US) 1 510-486-7600 (Globally) 1 510-486-7607 (Globally) Report Network Problems: trouble@es.net Provide Web Site Feedback: info@es.net IT Division's...

  19. R. S. Driof, Process Demlopnant Dranch, Production Division

    Office of Legacy Management (LM)

    S. Driof, Process Demlopnant Dranch, Production Division 7 i 7; I; " k>JSTI'IC AT TIE CifiICAL CCNSTXICTIOS COXi'O+TIO:? PIX)T PIGIT-JUL'I 31, 19% Chemico ban fouzd tw...

  20. Biology Division progress report, October 1, 1984-September 30, 1985

    SciTech Connect (OSTI)

    Not Available

    1986-01-01T23:59:59.000Z

    The body of this report provides summaries of the aims, scope and progress of the research by groups of investigators in the Division during the period of October 1, 1984, through September 30, 1985. At the end of each summary is a list of publications covering the same period. For convenience, the summaries are assembled under Sections in accordance with the current organizational structure of the Biology Division; each Section begins with an overview. It will be apparent, however, tha crosscurrents run throughout the Division and that the various programs support and interact with each other. In addition, this report includes information on the Division's educational activities, Advisory Committee, seminar program, and international interactions, as well as extramural activities of staff members, abstracts for technical meetings, and funding and personnel levels.

  1. Occupational Hygiene & Chemical Safety Division Department of Environmental Health & Safety

    E-Print Network [OSTI]

    Machel, Hans

    Occupational Hygiene & Chemical Safety Division Department of Environmental Health & Safety Risk all connections and fittings prior to start of anesthesia. Carefully pour Isoflurane from Environmental Health & Safety before re-entering the laboratory. REFERENCES 1. Procedure

  2. 58 University of Minnesota Morris 200911 Catalog Academic Division Structure

    E-Print Network [OSTI]

    Amin, S. Massoud

    (page 157) Spanish (page 173) Theatre Arts (page 178) The Division of the Humanities is composed of 10, and Spanish student clubs with a variety of projects; opportunities for language students to travel and study

  3. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT SMUD OFFPEAK OVERCOOLING PROJECT DECEMBER 2007 CEC5002013066 Prepared for: California Energy Commission Prepared by: Davis Energy Group #12; PREPARED BY: Primary Author(s): David Springer Davis Energy Group Davis, CA

  4. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT Developing5002013109 Prepared for: California Energy Commission Prepared by: Growpro Inc #12; Prepared by Waimauku, New Zealand Contract Number: PIR-07-001 Prepared for: California Energy Commission Abolghasem

  5. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT EMISSIONS REDUCTIONS FROM RENEWABLE ENERGY AND ENERGY EFFICIENCY IN CALIFORNIA AIR QUALITY MANAGEMENT DISTRICTS DECEMBER 2011 CEC5002013047 Prepared for: California Energy Commission Prepared by: Synapse Energy

  6. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT PLANNING ALTERNATIVE5002013021 Prepared for: California Energy Commission Prepared by: Facet Decision Systems, Inc. #12-08-030 Prepared for: California Energy Commission Linda Spiegel Contract Manager Linda Spiegel Office Manager

  7. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT ASSESSMENT OF PIEZOELECTRIC MATERIALS FOR ROADWAY ENERGY HARVESTING Cost of Energy and Demonstration Roadmap Prepared for: California Energy Commission Prepared by: DNV KEMA Energy & Sustainability JANUARY 2014 CEC5002013007

  8. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT PRELIMINARY ESTIMATES5002013051 Prepared for: California Energy Commission Prepared by: Lawrence Berkeley National Laboratory: 500-99-013 Prepared for: California Energy Commission Steve Ghadiri Contract Manager Fernando Piña

  9. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT ENERGY for: California Energy Commission Prepared by: San Diego State Research Foundation #12: California Energy Commission Raquel Kravitz Program Manager Fernando Pina Office Manager Energy Systems

  10. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT Demonstration: California Energy Commission Prepared by: Electric Power Research Institute #12; Prepared by: Primary: California Energy Commission Jamie Patterson Contract Manager Fernando Pina Office Manager Energy Efficiency

  11. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT GREENGUIDE FOR SUSTAINABLE ENERGY EFFICIENT REFRIGERATED STORAGE FACILITIES MARCH 2013 CEC-500-2013-145 Prepared for: California Energy for: California Energy Commission Anish Gautam Contract Manager Virginia Lew Office Manager Energy

  12. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT DEVELOPMENT Energy Commission Prepared by: Lawrence Berkeley National Laboratory #12; PREPARED BY: Primary-09-010 Prepared for: California Energy Commission Matthew Fung Contract Manager Virginia Lew Office Manager Energy

  13. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT ENERGY for: California Energy Commission Prepared by: San Diego State Research Foundation #12 Energy Commission Raquel E. Kravitz Program Manager Fernando Pina Office Manager Energy Systems Research

  14. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT LIGHTING CALIFORNIA'S FUTURE RetrofitIntegrated Classroom Lighting System (RICLS) Prepared for: California Energy Commission Managed by: Architectural Energy Corporation Prepared by: Finelite Inc. FEBRUARY 2013 CEC

  15. Unit Leadership Development Program and Evaluation for P Division

    E-Print Network [OSTI]

    Raybon, Felicia K.

    2006-12-15T23:59:59.000Z

    Division P undertook the Unit Leadership Development Program in March 2005. This Program was designed to facilitate leadership development in the workplace and develop those men and women who work everyday to accomplish the mission of Organization...

  16. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    or pricing event. The California Energy Commission is considering standards that would include a requirement Energy Research and Development Division FINAL PROJECT REPORT Technology MARCH 2013 CEC5002012077 Prepared for: California Energy Commission Prepared by: Heschong Mahone

  17. Lisa C. Tracy Acting Director Division of Natural Gas Regulatory...

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

    November 17, 2014 Lisa C. Tracy Acting Director Division of Natural Gas Regulatory Activities U.S. Department of Energy (FE-34) Office of Oil and Gas Global Security Office of...

  18. OFFICE OF FOSSIL ENERGY NATURAL GAS DIVISION SERVICE LIST

    Energy Savers [EERE]

    appfergasIntraAuthReport.do?queryNameserviceListPrint&docketNumber14-96-LNG 13 OFFICE OF FOSSIL ENERGY NATURAL GAS DIVISION SERVICE LIST FE DOCKET NO: 14-96-LNG ...

  19. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    ENERGY BALANCE UPDATE AND DECOMPOSITION ANALYSIS FOR THE INDUSTRY AND BUILDING SECTORS APRIL 2013 · Transportation California Energy Balance Update and Decomposition Analysis for the Industry and Building Energy Research and Development Division FINAL PROJECT REPORT CALIFORNIA

  20. RIKEN Center for Emergent Matter Science Strong Correlation Physics Division

    E-Print Network [OSTI]

    Fukai, Tomoki

    Device Research Team Emergent Soft Matter Structure Reserch Team Emergent Functional Polymers Research Information Electronics Division Quantum Functional System Research Group Quantum Optics Research Group Quantum Electronics Research Team Emergent Phenomena Observation Technology Research Team Quantum Nano

  1. Library and Information Services Division Current References 2009-1

    E-Print Network [OSTI]

    Library and Information Services Division Current References 2009-1 The Year of Darwin 2009 Discovering Darwin at NOAA Central Library: Resources on Charles Darwin, Evolution, and the Galapagos Islands National Oceanographic Data Center NOAA Central Library October 2009 http

  2. Biology Division. Progress report, August 1, 1982-September 30, 1983

    SciTech Connect (OSTI)

    Not Available

    1984-01-01T23:59:59.000Z

    The Biology Division is the component of the Oak Ridge National Laboratory that investigates the potential adverse health effects of energy-related substances. The body of this report provides summaries of the aims, scope and progress of the research of groups of investigators in the Division during the period of August 1, 1982, through September 30, 1983. At the end of each summary is a list of publications covering the same period (published or accepted for publication). For convenience, the summaries are assembled under Sections in accordance with the current organizational structure of the Biology Division; each Section begins with an overview. It will be apparent, however, that currents run throughout the Division and that the various programs support and interact with each other.

  3. Oklahoma Cooperative Extension Service Division of Agricultural Sciences

    E-Print Network [OSTI]

    Balasundaram, Balabhaskar "Baski"

    E-1010 Oklahoma Cooperative Extension Service Division of Agricultural Sciences and Natural Resources Oklahoma State University Oklahoma Prescribed Burning Handbook Oklahoma Prescribed Burning Research Associate, Natural Resource Ecology and Management Oklahoma Prescribed Burning Handbook Oklahoma

  4. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT ASSESSMENT OF LARVAL Coastal Boundary Layer Flow SEPTEMBER 2007 CEC5002013049 Prepared for: California Energy Commission Energy Commission Joe O'Hagan Contract Manager Linda Spiegel Office Manager Energy Generation Research

  5. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT ENERGYEFFICIENT Energy Commission Prepared by: Lawrence Berkeley National Laboratory #12; PREPARED BY: Primary.lbl.gov Contract Number: 500-06-053 Prepared for: California Energy Commission Paul Roggensack Contract Manager

  6. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT ENERGYEFFICIENT HIGHTECH BUILDINGS DECEMBER 2008 CEC5002013062 Prepared for: California Energy Commission Prepared by-06-053 Prepared for: California Energy Commission Paul Roggensack Contract Manager Virginia Lew Office Manager

  7. analysis division microbiology: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    EMCAS are stored in HDF format and can be quickly retrieved or exported in text and spreadsheet formats Kemner, Ken 36 18th Engineering Mechanics Division Conference (EMD2007)...

  8. Energy Research and Development Division DRAFT PROJECT REPORT

    E-Print Network [OSTI]

    Use Energy Efficiency · Renewable Energy Technologies · Transportation Natural Gas Energy Efficiency Energy Research and Development Division DRAFT PROJECT REPORT NATURAL GAS ENERGY EFFICIENCY in Buildings ­ Roadmap for Future Research is the final report for the Buildings Natural Gas Roadmap

  9. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    efforts are focused on securing stable and economical storage, transportation, and delivery of natural gas-Use Energy Efficiency · Renewable Energy Technologies · Transportation California Natural Gas StorageEnergy Research and Development Division FINAL PROJECT REPORT CALIFORNIA NATURAL GAS STORAGE

  10. COLLABORATION INNOVATION INTEROPERABILITY DISCOVERY PARTNERSHIP External Research Division

    E-Print Network [OSTI]

    Narasayya, Vivek

    and excitement for how computing technologies can help address major scientific and educational challenges. Tony Hey Corporate Vice President, External Research Division, Microsoft Research 1 Advancing a New Era

  11. Engineering Research Division report on reports: calendar year 1979. [LLL

    SciTech Connect (OSTI)

    Gardner, C.L.; Johnston, S.J. (eds.)

    1980-03-01T23:59:59.000Z

    A bibliography of publications of members of the Engineering Research Division of the Electronics Engineering Department is presented for 1979. Abstracts for 148 publications are included, along with author and keywork indexes. (RWR)

  12. 2013 Huayu Enrichment Scholarship 1 Educational Division, TECO in Canada

    E-Print Network [OSTI]

    Shoubridge, Eric

    2013 Huayu Enrichment Scholarship 1 Educational Division, TECO in Canada 2013 Huayu Enrichment Scholarship PURPOSE Huayu Enrichment Scholarship is executed in accordance with "Ministry of Education Huayu Enrichment Scholarship (HES) International Student Directions" (see Appendix 1

  13. Simulating Astrophysical Jets in Laboratory Experiments Paul M. Bellan, Setthivoine You, and Scott C. Hsu

    E-Print Network [OSTI]

    Bellan, Paul M.

    C. Hsu Caltech 128-95, Pasadena, CA 91125, USA April 23, 1993 Abstract. Pulsed power technology and increases the pinch force, thereby collimating the jet. Keywords: astrophysical jet, collimation, kink, MHD, pinch, stagnation 1. Experiment motivation and design A magnetically driven astrophysical jet

  14. astrophysically significant gamma-ray: Topics by E-print Network

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    astrophysically significant gamma-ray First Page Previous Page 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 Next Page Last Page Topic Index 1 Astrophysical...

  15. A Search for Astrophysical Neutrino Point Sources with Super-Kamiokande

    E-Print Network [OSTI]

    Tokyo, University of

    A Search for Astrophysical Neutrino Point Sources with Super-Kamiokande Eric Thrane A dissertation Abstract A Search for Astrophysical Neutrino Point Sources with Super-Kamiokande Eric Thrane Chair to the upward-going muon dataset at Super-Kamiokande. We find interesting signals from two sources: RX J1713

  16. Astrophysical Thermonuclear Functions for Boltzmann-Gibbs Statistics and Tsallis Statistics

    E-Print Network [OSTI]

    R. K. Saxena; A. M. Mathai; H. J. Haubold

    2004-06-22T23:59:59.000Z

    We present an analytic proof of the integrals for astrophysical thermonuclear functions which are derived on the basis of Boltzmann-Gibbs statistical mechanics. Among the four different cases of astrophysical thermonuclear functions, those with a depleted high-energy tail and a cut-off at high energies find a natural interpretation in q-statistics.

  17. 41 Current projects Climate Variability Research Research within this Division focuses on large-scale

    E-Print Network [OSTI]

    Haak, Hein

    Research Division participates in the informal network for Earth System Models of Intermediate Complexity

  18. Lawrence Berkeley National Laboratory Facilities Division- Optimizing Activity-level Work Planning and Control Lessons Learned

    Broader source: Energy.gov [DOE]

    Presenter: Ken Fletcher, Deputy Division Director for Facilities, Lawrence Berkeley National Laboratory

  19. Harrison Radiator Division's Energy Management, Reporting and Accounting System

    E-Print Network [OSTI]

    Goubeaux, R. J.

    HARRISON RADIATOR DIVISION'S ENERGY MANAGEMENT, REPORTING and ACCOUNTING SYSTEM Ronald J. Goubeaux Harrison Radiator Division Lockport, New York ABSTRACT Energy management is essential for obtaining the lowest possible product..., farm equipment, small aircraft and other types of vehicles. The energy management, reporting and accounting system that is covered in this paper is operating in Harrison's West Complex of the New York Operations located in Lockport, Western...

  20. MORDECAI-MARK MAC LOW CHAIR, DIVISION OF PHYSICAL SCIENCES

    E-Print Network [OSTI]

    Glover), $149,912, August 1, 2003 ­ July 31, 2006 National Science Foundation, "CAREER: Structure, and K. Keil (editors), Protostars and Planets V: 63-80. Tucson: University of Arizona Press. Glover, S by gravitational collapse from static initial conditions. Astrophysical Journal Supplement 169: 239-268. Glover, S

  1. Annual Report: Hydrodynamics and Radiative Hydrodynamics with Astrophysical Applications

    SciTech Connect (OSTI)

    R. Paul Drake

    2005-12-01T23:59:59.000Z

    We report the ongoing work of our group in hydrodynamics and radiative hydrodynamics with astrophysical applications. During the period of the existing grant, we have carried out two types of experiments at the Omega laser. One set of experiments has studied radiatively collapsing shocks, obtaining high-quality scaling data using a backlit pinhole and obtaining the first (ever, anywhere) Thomson-scattering data from a radiative shock. Other experiments have studied the deeply nonlinear development of the Rayleigh-Taylor (RT) instability from complex initial conditions, obtaining the first (ever, anywhere) dual-axis radiographic data using backlit pinholes and ungated detectors. All these experiments have applications to astrophysics, discussed in the corresponding papers either in print or in preparation. We also have obtained preliminary radiographs of experimental targets using our x-ray source. The targets for the experiments have been assembled at Michigan, where we also prepare many of the simple components. The above activities, in addition to a variety of data analysis and design projects, provide good experience for graduate and undergraduates students. In the process of doing this research we have built a research group that uses such work to train junior scientists.

  2. A new method to generate dust with astrophysical properties

    SciTech Connect (OSTI)

    Hansen, J F; van Breugel, W; Bringa, E M; Graham, G A; Remington, B A; Taylor, E A; Tielens, A G

    2010-04-21T23:59:59.000Z

    In interstellar and interplanetary space, the size distribution and composition of dust grains play an important role. For example, dust grains determine optical and ultraviolet extinction levels in astronomical observations, dominate the cooling rate of our Galaxy, and sets the thermal balance and radiative cooling rates in molecular clouds, which are the birth place of stars. Dust grains are also a source of damage and failure to space hardware and thus present a hazard to space flight. To model the size distribution and composition of dust grains, and their effect in the above scenarios, it is vital to understand the mechanism of dust-shock interaction. We demonstrate a new experiment which employs a laser to subject dust grains to pressure spikes similar to those of colliding astrophysical dust, and which accelerates the grains to astrophysical velocities. The new method generates much larger data sets than earlier methods; we show how large quantities (thousands) of grains are accelerated at once, rather than accelerating individual grains, as is the case of earlier methods using electric fields.

  3. LOW-TEMPERATURE CRYSTALLIZATION OF AMORPHOUS SILICATE IN ASTROPHYSICAL ENVIRONMENTS

    SciTech Connect (OSTI)

    Tanaka, Kyoko K.; Yamamoto, Tetsuo [Institute of Low Temperature Science, Hokkaido University, Sapporo 060-0819 (Japan); Kimura, Hiroshi [Center for Planetary Science, Kobe 657-8501 (Japan)

    2010-07-01T23:59:59.000Z

    We construct a theoretical model for low-temperature crystallization of amorphous silicate grains induced by exothermic chemical reactions. As a first step, the model is applied to the annealing experiments, in which the samples are (1) amorphous silicate grains and (2) amorphous silicate grains covered with an amorphous carbon layer. We derive the activation energies of crystallization for amorphous silicate and amorphous carbon from the analysis of the experiments. Furthermore, we apply the model to the experiment of low-temperature crystallization of an amorphous silicate core covered with an amorphous carbon layer containing reactive molecules. We clarify the conditions of low-temperature crystallization due to exothermic chemical reactions. Next, we formulate the crystallization conditions so as to be applicable to astrophysical environments. We show that the present crystallization mechanism is characterized by two quantities: the stored energy density Q in a grain and the duration of the chemical reactions {tau}. The crystallization conditions are given by Q>Q{sub min} and {tau} < {tau}{sub cool} regardless of details of the reactions and grain structure, where {tau}{sub cool} is the cooling timescale of the grains heated by exothermic reactions, and Q{sub min} is minimum stored energy density determined by the activation energy of crystallization. Our results suggest that silicate crystallization occurs in wider astrophysical conditions than hitherto considered.

  4. Screened Coulomb potentials for astrophysical nuclear fusion reactions

    E-Print Network [OSTI]

    Theodore E. Liolios

    2000-09-04T23:59:59.000Z

    The electron-screening acceleration of laboratory fusion reactions at astrophysical energies is an unsolved problem of great importance to astrophysics. That effect is modeled here by considering the fusion of hydrogen-like atoms whose electron probability density is used in Poisson's equation in order to derive the corresponding screened Coulomb potential energy. That way atomic excitations and deformations of the fusing atoms can be taken into account. Those potentials are then treated semiclassically in order to obtain the screening (accelerating) factor of the reaction. By means of the proposed model the effect of a superstrong magnetic field on laboratory Hydrogen fusion reactions is investigated here for the first time showing that, despite the considerable increase in the cross section of the $% dd$ reaction, the $pp$ reaction is still too slow to justify experimentation. The proposed model is finally applied on the $H^{2}(d,p) H^{3}$ fusion reaction describing satisfactorily the experimental data although some ambiguity remains regarding the molecular nature of the deuteron target. Notably, the present method gives a sufficiently high screening energy for Hydrogen fusion reactions so that the take-away energy of the spectator nucleus can also be taken into account.

  5. Liquid xenon detectors for particle physics and astrophysics

    SciTech Connect (OSTI)

    Aprile, E.; Doke, T. [Department of Physics, Columbia University, New York, New York 10027 (United States); Advanced Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555 (Japan)

    2010-07-15T23:59:59.000Z

    This article reviews the progress made over the last 20 years in the development and applications of liquid xenon detectors in particle physics, astrophysics, and medical imaging experiments. A summary of the fundamental properties of liquid xenon as radiation detection medium, in light of the most current theoretical and experimental information is first provided. After an introduction of the different type of liquid xenon detectors, a review of past, current, and future experiments using liquid xenon to search for rare processes and to image radiation in space and in medicine is given. Each application is introduced with a survey of the underlying scientific motivation and experimental requirements before reviewing the basic characteristics and expected performance of each experiment. Within this decade it appears likely that large volume liquid xenon detectors operated in different modes will contribute to answering some of the most fundamental questions in particle physics, astrophysics, and cosmology, fulfilling the most demanding detection challenges. From detectors based solely on liquid xenon (LXe) scintillation, such as in the MEG experiment for the search of the rare ''{mu}{yields}e{gamma}'' decay, currently the largest liquid xenon detector in operation, and in the XMASS experiment for dark matter detection, to the class of time projection chambers which exploit both scintillation and ionization of LXe, such as in the XENON dark matter search experiment and in the Enriched Xenon Observatory for neutrinoless double beta decay, unrivaled performance and important contributions to physics in the next few years are anticipated.

  6. No-hair theorem for Black Holes in Astrophysical Environments

    E-Print Network [OSTI]

    Gürlebeck, Norman

    2015-01-01T23:59:59.000Z

    According to the no-hair theorem, static black holes are described by a Schwarzschild spacetime provided there are no other sources of the gravitational field. This requirement, however, is in astrophysical realistic scenarios often violated, e.g., if the black hole is part of a binary system or if it is surrounded by an accretion disk. In these cases, the black hole is distorted due to tidal forces. Nonetheless, the subsequent formulation of the no-hair theorem holds: The contribution of the distorted black hole to the multipole moments that describe the gravitational field close to infinity and, thus, all sources is that of a Schwarzschild black hole. It still has no hair. This implies that there is no multipole moment induced in the black hole and that its second Love numbers, which measure some aspects of the distortion, vanish as was already shown in approximations to general relativity. But here we prove this property for astrophysical relevant black holes in full general relativity.

  7. Formation of super-heavy elements in astrophysical nucleosynthesis

    SciTech Connect (OSTI)

    Zagrebaev, V. I.; Karpov, A. V.; Mishustin, I. N.; Greiner, Walter [Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Moscow Region (Russian Federation); Frankfurt Institute for Advanced Studies, J.W. Goethe-Universitaet, Frankfurt (Germany)

    2012-10-20T23:59:59.000Z

    The unexplored area of heavy neutron-rich nuclides is extremely important for the understanding of the r process of astrophysical nucleogenesis. For elements with Z>100 only neutron deficient isotopes (located to the left of the stability line) have been synthesized so far. The 'north-east' area of the nuclear map can be reached neither in fusion reactions nor in fragmentation processes. Low energy multi-nucleon transfer reactions are quite promising for the production and study of neutron-rich heavy nuclei including those located at the superheavy (SH) island of stability [1]. The neutron capture process is considered here as an alternative method for the production of SH nuclei. Requirements for the pulsed reactors of the next generation that could be used for the synthesis of long-living neutron rich SH nuclei are formulated. Formation of SH nuclei in supernova explosions is also discussed and the abundance of SH elements in nature is estimated.

  8. TA-DA: A TOOL FOR ASTROPHYSICAL DATA ANALYSIS

    SciTech Connect (OSTI)

    Da Rio, Nicola [European Space Agency, Keplerlaan 1, 2200-AG Noordwijk (Netherlands); Robberto, Massimo, E-mail: ndario@rssd.esa.int [Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 (United States)

    2012-12-01T23:59:59.000Z

    We present the Tool for Astrophysical Data Analysis (TA-DA), a new software aimed to greatly simplify and improve the analysis of stellar photometric data in comparison with theoretical models, and allow the derivation of stellar parameters from multi-band photometry. Its flexibility allows one to address a number of such problems: from the interpolation of stellar models, or sets of stellar physical parameters in general, to the computation of synthetic photometry in arbitrary filters or units; from the analysis of observed color-magnitude diagrams to a Bayesian derivation of stellar parameters (and extinction) based on multi-band data. TA-DA is available as a pre-compiled Interactive Data Language widget-based application; its graphical user interface makes it considerably user-friendly. In this paper, we describe the software and its functionalities.

  9. The Theoretical Astrophysical Observatory: Cloud-Based Mock Galaxy Catalogues

    E-Print Network [OSTI]

    Bernyk, Maksym; Tonini, Chiara; Hodkinson, Luke; Hassan, Amr H; Garel, Thibault; Duffy, Alan R; Mutch, Simon J; Poole, Gregory B

    2014-01-01T23:59:59.000Z

    We introduce the Theoretical Astrophysical Observatory (TAO), an online virtual laboratory that houses mock observations of galaxy survey data. Such mocks have become an integral part of the modern analysis pipeline. However, building them requires an expert knowledge of galaxy modelling and simulation techniques, significant investment in software development, and access to high performance computing. These requirements make it difficult for a small research team or individual to quickly build a mock catalogue suited to their needs. To address this TAO offers access to multiple cosmological simulations and semi-analytic galaxy formation models from an intuitive and clean web interface. Results can be funnelled through science modules and sent to a dedicated supercomputer for further processing and manipulation. These modules include the ability to (1) construct custom observer light-cones from the simulation data cubes; (2) generate the stellar emission from star formation histories, apply dust extinction, a...

  10. On numerical considerations for modeling reactive astrophysical shocks

    SciTech Connect (OSTI)

    Papatheodore, Thomas L.; Messer, O. E. Bronson, E-mail: tpapathe@utk.edu, E-mail: bronson@ornl.gov [Department of Physics and Astronomy, University of Tennessee, Knoxville, TN 37996 (United States)

    2014-02-10T23:59:59.000Z

    Simulating detonations in astrophysical environments is often complicated by numerical approximations to shock structure. A common prescription to ensure correct detonation speeds and associated quantities is to prohibit burning inside the numerically broadened shock. We have performed a series of simulations to verify the efficacy of this approximation and to understand how resolution and dimensionality might affect its use. Our results show that in one dimension, prohibiting burning in the shock is important wherever the carbon burning length is not resolved, in keeping with the results of Fryxell et al. In two dimensions, we find that the prohibition of shock burning effectively inhibits the development of cellular structure for all but the most highly resolved cases. We discuss the possible impacts this outcome may have on sub-grid models and detonation propagation in models of Type Ia supernovae, including potential impacts on observables.

  11. Laboratory Tests of Low Density Astrophysical Equations of State

    E-Print Network [OSTI]

    L. Qin; K. Hagel; R. Wada; J. B. Natowitz; S. Shlomo; A. Bonasera; G. Roepke; S. Typel; Z. Chen; M. Huang; J. Wang; H. Zheng; S. Kowalski; M. Barbui; M. R. D. Rodrigues; K. Schmidt; D. Fabris; M. Lunardon; S. Moretto; G. Nebbia; S. Pesente; V. Rizzi; G. Viesti; M. Cinausero; G. Prete; T. Keutgen; Y. El Masri; Z. Majka

    2012-03-20T23:59:59.000Z

    Clustering in low density nuclear matter has been investigated using the NIMROD multi-detector at Texas A&M University. Thermal coalescence modes were employed to extract densities, $\\rho$, and temperatures, $T$, for evolving systems formed in collisions of 47 $A$ MeV $^{40}$Ar + $^{112}$Sn,$^{124}$Sn and $^{64}$Zn + $^{112}$Sn, $^{124}$Sn. The yields of $d$, $t$, $^{3}$He, and $^{4}$He have been determined at $\\rho$ = 0.002 to 0.032 nucleons/fm$^{3}$ and $T$= 5 to 10 MeV. The experimentally derived equilibrium constants for $\\alpha$ particle production are compared with those predicted by a number of astrophysical equations of state. The data provide important new constraints on the model calculations.

  12. Extracting cosmic microwave background polarisation from satellite astrophysical maps

    E-Print Network [OSTI]

    Baccigalupi, C; De Zotti, G; Smoot, G F; Burigana, C; Maino, D; Bedini, L; Salerno, E

    2002-01-01T23:59:59.000Z

    We present the application of the Fast Independent Component Analysis technique for blind component separation to polarised astrophysical emission. We study how the Cosmic Microwave Background (CMB) polarised signal, consisting of $E$ and $B$ modes, can be extracted from maps affected by substantial contamination from diffuse Galactic foregrounds and instrumental noise. We perform the analysis of all sky maps simulated accordingly to the nominal performances of the Low Frequency Instrument (LFI) aboard the Planck satellite; the sky signal is modeled as a superposition of CMB, generated by a Gaussian, nearly scale invariant cosmological perturbation spectrum, and the existing simulated polarisation templates of Galactic synchrotron. Our results indicate that the angular power spectrum of CMB $E$ modes can be recovered on all scales up to $\\ell\\simeq 1000$, corresponding to the fourth acoustic oscillation, while $B$ modes can be detected, up to their turnover at $\\ell\\simeq 100$ if cosmological tensor amplitude...

  13. ENZO: AN ADAPTIVE MESH REFINEMENT CODE FOR ASTROPHYSICS

    SciTech Connect (OSTI)

    Bryan, Greg L.; Turk, Matthew J. [Columbia University, Department of Astronomy, New York, NY 10025 (United States); Norman, Michael L.; Bordner, James; Xu, Hao; Kritsuk, Alexei G. [CASS, University of California, San Diego, 9500 Gilman Drive La Jolla, CA 92093-0424 (United States); O'Shea, Brian W.; Smith, Britton [Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824 (United States); Abel, Tom; Wang, Peng; Skillman, Samuel W. [Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Menlo Park, CA 94025 (United States); Wise, John H. [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, 837 State Street, Atlanta, GA (United States); Reynolds, Daniel R. [Department of Mathematics, Southern Methodist University, Box 750156, Dallas, TX 75205-0156 (United States); Collins, David C. [Department of Physics, Florida State University, Tallahassee, FL 32306 (United States); Harkness, Robert P. [NICS, Oak Ridge National Laboratory, 1 Bethel Valley Rd, Oak Ridge, TN 37831 (United States); Kim, Ji-hoon [Department of Astronomy and Astrophysics, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States); Kuhlen, Michael [Theoretical Astrophysics Center, University of California Berkeley, Hearst Field Annex, Berkeley, CA 94720 (United States); Goldbaum, Nathan [Institute for Astronomy, University of Edinburgh, Edinburgh EH9 3HJ (United Kingdom); Hummels, Cameron [Department of Astronomy/Steward Observatory, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721 (United States); Tasker, Elizabeth [Physics Department, Faculty of Science, Hokkaido University, Kita-10 Nishi 8, Kita-ku, Sapporo 060-0810 (Japan); Collaboration: Enzo Collaboration; and others

    2014-04-01T23:59:59.000Z

    This paper describes the open-source code Enzo, which uses block-structured adaptive mesh refinement to provide high spatial and temporal resolution for modeling astrophysical fluid flows. The code is Cartesian, can be run in one, two, and three dimensions, and supports a wide variety of physics including hydrodynamics, ideal and non-ideal magnetohydrodynamics, N-body dynamics (and, more broadly, self-gravity of fluids and particles), primordial gas chemistry, optically thin radiative cooling of primordial and metal-enriched plasmas (as well as some optically-thick cooling models), radiation transport, cosmological expansion, and models for star formation and feedback in a cosmological context. In addition to explaining the algorithms implemented, we present solutions for a wide range of test problems, demonstrate the code's parallel performance, and discuss the Enzo collaboration's code development methodology.

  14. On Numerical Considerations for Modeling Reactive Astrophysical Shocks

    SciTech Connect (OSTI)

    Papatheodore, Thomas L [ORNL] [ORNL; Messer, Bronson [ORNL] [ORNL

    2014-01-01T23:59:59.000Z

    Simulating detonations in astrophysical environments is often complicated by numerical approximations to shock structure. A common prescription to ensure correct detonation speeds (and associated quantities) is to prohibit burning inside the numerically broadened shock (Fryxell et al. 1989). We have performed a series of simulations to verify the efficacy of this approximation and to understand how resolution and dimensionality might affect its use. Our results show that, in one dimension, prohibiting burning in the shock is important wherever the carbon burning length is not resolved, in keeping with the results of Fryxell et al. (1989). In two dimensions, we find that the prohibition of shock burning effectively inhibits the development of cellular structure for all but the most highly-resolved cases. We discuss the possible impacts this outcome may have on sub-grid models and detonation propagation in Type Ia supernovae.

  15. COSMOS: A Radiation-Chemo-Hydrodynamics Code for Astrophysical Problems

    E-Print Network [OSTI]

    Peter Anninos; P. Chris Fragile; Stephen D. Murray

    2003-03-10T23:59:59.000Z

    We have developed a new massively-parallel radiation-hydrodynamics code (Cosmos) for Newtonian and relativistic astrophysical problems that also includes radiative cooling, self-gravity, and non-equilibrium, multi-species chemistry. Several numerical methods are implemented for the hydrodynamics, including options for both internal and total energy conserving schemes. Radiation is treated using flux-limited diffusion. The chemistry incorporates 27 reactions, including both collisional and radiative processes for atomic hydrogen and helium gases, and molecular hydrogen chains. In this paper we discuss the equations and present results from test problems carried out to verify the robustness and accuracy of our code in the Newtonian regime. An earlier paper presented tests of the relativistic capabilities of Cosmos.

  16. COSMOS A Radiation-Chemo-Hydrodynamics Code for Astrophysical Problems

    E-Print Network [OSTI]

    Anninos, P; Murray, S D; Anninos, Peter; Murray, Stephen D.

    2003-01-01T23:59:59.000Z

    We have developed a new massively-parallel radiation-hydrodynamics code (Cosmos) for Newtonian and relativistic astrophysical problems that also includes radiative cooling, self-gravity, and non-equilibrium, multi-species chemistry. Several numerical methods are implemented for the hydrodynamics, including options for both internal and total energy conserving schemes. Radiation is treated using flux-limited diffusion. The chemistry incorporates 27 reactions, including both collisional and radiative processes for atomic hydrogen and helium gases, and molecular hydrogen chains. In this paper we discuss the equations and present results from test problems carried out to verify the robustness and accuracy of our code in the Newtonian regime. An earlier paper presented tests of the relativistic capabilities of Cosmos.

  17. Astrophysical Dynamics 1999/2000: Merging Research and Education

    E-Print Network [OSTI]

    Alessandro B. Romeo

    2000-06-09T23:59:59.000Z

    The workshop `Astrophysical Dynamics 1999/2000' followed a homonymous advanced research course, and both activities were organized by me. In this opening paper of the proceedings book, I describe them and document their strong impact on the academic life of the local institutions. The advanced research course was open to graduate students, senior researchers, and motivated under-graduate students with good background in physics and mathematics. The course covered several multi-disciplinary issues of modern research on astrophysical dynamics, and thus also of interest to physicists, mathematicians and engineers. The major topic was gas dynamics, viewed in context with stellar dynamics and plasma physics. The course was complemented by parallel seminars on hot topics given by experts in such fields, and open to a wide scientific audience. In particular, I gave a friendly introduction to wavelets, which are becoming an increasingly powerful tool not only for processing signals and images but also for analysing fractals and turbulence, and which promise to have important applications to dynamical modelling of disc galaxies. The workshop was open to a wide scientific audience. The workshop with published proceedings book was, as a matter of fact, the innovative form of exam that I proposed for the advanced research course. The contributions were refereed and their quality is high on average, exceptionally high in a few cases. The advanced research course and the workshop all together produced great enthusiasm in the students and welcomed the participation of a hundred different people, which means an order of magnitude more than an average graduate course at Chalmers University of Technology and G\\"oteborg University.

  18. Accelerator & Fusion Research Division: 1993 Summary of activities

    SciTech Connect (OSTI)

    Chew, J.

    1994-04-01T23:59:59.000Z

    The Accelerator and Fusion Research Division (AFRD) is not only one of the largest scientific divisions at LBL, but also the one of the most diverse. Major efforts include: (1) investigations in both inertial and magnetic fusion energy; (2) operation of the Advanced Light Source, a state-of-the-art synchrotron radiation facility; (3) exploratory investigations of novel radiation sources and colliders; (4) research and development in superconducting magnets for accelerators and other scientific and industrial applications; and (5) ion beam technology development for nuclear physics and for industrial and biomedical applications. Each of these topics is discussed in detail in this book.

  19. Environmental Research Division technical progress report, January 1984-December 1985

    SciTech Connect (OSTI)

    Not Available

    1986-05-01T23:59:59.000Z

    Technical progress in the various research and assessment activities of Argonne National Laboratory's Environmental Research Division is reported for the period 1984 to 1985. Textual, graphic, and tabular information is used to briefly summarize (in separate chapters) the work of the Division's Atmospheric Physics, Environmental Effects Research, Environmental Impacts, Fundamental Molecular Physics and Chemistry, and Waste Management Programs. Information on professional qualifications, awards, and outstanding professional activities of staff members, as well as lists of publications, oral presentations, special events organized, and participants in educational programs, are provided in appendices at the end of each chapter.

  20. Studies into the Molecular Basis of Chloroplast Division

    E-Print Network [OSTI]

    Smith, Aaron Gene

    2012-07-16T23:59:59.000Z

    proteins have been identified that are negative regulators of cell division under certain conditions. UgtP acts as an inhibitor of cell division in nutrient rich media by destabilizing interactions between FtsZ protofilaments and is downregulated under... non-nutrient rich media conditions (50). During DNA damage in E. coli, SulA is expressed as part of the SOS response and inhibits assembly of new Z- rings and promotes disassembly of active Z-rings (51-54). The critical concentration of Fts...

  1. Nuclear astrophysics studies with ultra-peripheral heavy-ion collisions

    E-Print Network [OSTI]

    C. A. Bertulani

    2009-12-17T23:59:59.000Z

    I describe in very simple terms the theoretical tools needed to investigate ultra-peripheral nuclear reactions for nuclear astrophysics purposes. For a more detailed account, see arXiv:0908.4307.

  2. Applying petroleum geophysics to astrophysics: Quantitative 4D seismic study of the solar interior

    E-Print Network [OSTI]

    Crawford, Ian

    Applying petroleum geophysics to astrophysics: Quantitative 4D seismic study, is to a significant extent based on tomographic methods developed in geophysics. The proposed time-lapse seismic methods developed in petroleum geophysics offer the next

  3. A Search for Astrophysical Burst Signals at the Sudbury Neutrino Observatory

    E-Print Network [OSTI]

    B. Aharmim; S. N. Ahmed; A. E. Anthony; N. Barros; E. W. Beier; A. Bellerive; B. Beltran; M. Bergevin; S. D. Biller; K. Boudjemline; M. G. Boulay; B. Cai; Y. D. Chan; D. Chauhan; M. Chen; B. T. Cleveland; G. A. Cox; X. Dai; H. Deng; J. A. Detwiler; M. DiMarco; M. D. Diamond; P. J. Doe; G. Doucas; P. -L. Drouin; F. A. Duncan; M. Dunford; E. D. Earle; S. R. Elliott; H. C. Evans; G. T. Ewan; J. Farine; H. Fergani; F. Fleurot; R. J. Ford; J. A. Formaggio; N. Gagnon; J. TM. Goon; K. Graham; E. Guillian; S. Habib; R. L. Hahn; A. L. Hallin; E. D. Hallman; P. J. Harvey; R. Hazama; W. J. Heintzelman; J. Heise; R. L. Helmer; A. Hime; C. Howard; M. Huang; P. Jagam; B. Jamieson; N. A. Jelley; M. Jerkins; K. J. Keeter; J. R. Klein; L. L. Kormos; M. Kos; C. Kraus; C. B. Krauss; A. Krueger; T. Kutter; C. C. M. Kyba; R. Lange; J. Law; I. T. Lawson; K. T. Lesko; J. R. Leslie; I. Levine; J. C. Loach; R. MacLellan; S. Majerus; H. B. Mak; J. Maneira; R. Martin; N. McCauley; A. B. McDonald; S. R. McGee; M. L. Miller; B. Monreal; J. Monroe; B. G. Nickel; A. J. Noble; H. M. O'Keeffe; N. S. Oblath; R. W. Ollerhead; G. D. Orebi Gann; S. M. Oser; R. A. Ott; S. J. M. Peeters; A. W. P. Poon; G. Prior; S. D. Reitzner; K. Rielage; B. C. Robertson; R. G. H. Robertson; M. H. Schwendener; J. A. Secrest; S. R. Seibert; O. Simard; J. J. Simpson; D. Sinclair; P. Skensved; T. J. Sonley; L. C. Stonehill; G. Tesic; N. Tolich; T. Tsui; R. Van Berg; B. A. VanDevender; C. J. Virtue; B. L. Wall; D. Waller; H. Wan Chan Tseung; D. L. Wark; P. J. S. Watson; J. Wendland; N. West; J. F. Wilkerson; J. R. Wilson; J. M. Wouters; A. Wright; M. Yeh; F. Zhang; K. Zuber

    2013-09-04T23:59:59.000Z

    The Sudbury Neutrino Observatory (SNO) has confirmed the standard solar model and neutrino oscillations through the observation of neutrinos from the solar core. In this paper we present a search for neutrinos associated with sources other than the solar core, such as gamma-ray bursters and solar flares. We present a new method for looking for temporal coincidences between neutrino events and astrophysical bursts of widely varying intensity. No correlations were found between neutrinos detected in SNO and such astrophysical sources.

  4. Indirect methods of determination of the asymptotic normalization coefficients and their application for nuclear astrophysics

    SciTech Connect (OSTI)

    Yarmukhamedov, R. [Institute of Nuclear Physics, Academy of Sciences of Uzbekistan, 100214 Tashkent (Uzbekistan)

    2014-05-09T23:59:59.000Z

    The basic methods of the determination of asymptotic normalization coefficient for A+a?B of astrophysical interest are briefly presented. The results of the application of the specific asymptotic normalization coefficients derived within these methods for the extrapolation of the astrophysical S factors to experimentally inaccessible energy regions (E ? 25 keV) for the some specific radiative capture A(a,?)B reactions of the pp-chain and the CNO cycle are presented.

  5. The Trojan Horse method for nuclear astrophysics: Recent results on resonance reactions

    SciTech Connect (OSTI)

    Cognata, M. La; Pizzone, R. G. [Laboratori Nazionali del Sud, Istituto Nazionale di Fisica Nucleare, Catania (Italy); Spitaleri, C.; Cherubini, S.; Romano, S. [Dipartimento di Fisica e Astronomia, Università di Catania, Catania, Italy and Laboratori Nazionali del Sud, Istituto Nazionale di Fisica Nucleare, Catania (Italy); Gulino, M.; Tumino, A. [Kore University, Enna, Italy and Laboratori Nazionali del Sud, Istituto Nazionale di Fisica Nucleare, Catania (Italy); Lamia, L. [Dipartimento di Fisica e Astronomia, Università di Catania, Catania (Italy)

    2014-05-09T23:59:59.000Z

    Nuclear astrophysics aims to measure nuclear-reaction cross sections of astrophysical interest to be included into models to study stellar evolution and nucleosynthesis. Low energies, < 1 MeV or even < 10 keV, are requested for this is the window where these processes are more effective. Two effects have prevented to achieve a satisfactory knowledge of the relevant nuclear processes, namely, the Coulomb barrier exponentially suppressing the cross section and the presence of atomic electrons. These difficulties have triggered theoretical and experimental investigations to extend our knowledge down to astrophysical energies. For instance, indirect techniques such as the Trojan Horse Method have been devised yielding new cutting-edge results. In particular, I will focus on the application of this indirect method to resonance reactions. Resonances might dramatically enhance the astrophysical S(E)-factor so, when they occur right at astrophysical energies, their measurement is crucial to pin down the astrophysical scenario. Unknown or unpredicted resonances might introduce large systematic errors in nucleosynthesis models. These considerations apply to low-energy resonances and to sub-threshold resonances as well, as they may produce sizable modifications of the S-factor due to, for instance, destructive interference with another resonance.

  6. Engineering Physics and Mathematics Division progress report for period ending December 31, 1994

    SciTech Connect (OSTI)

    Sincovec, R.F.

    1995-07-01T23:59:59.000Z

    This report provides a record of the research activities of the Engineering Physics and Mathematics Division for the period January 1, 1993, through December 31, 1994. This report is the final archival record of the EPM Division. On October 1, 1994, ORELA was transferred to Physics Division and on January 1, 1995, the Engineering Physics and Mathematics Division and the Computer Applications Division reorganized to form the Computer Science and Mathematics Division and the Computational Physics and Engineering Division. Earlier reports in this series are identified on the previous pages, along with the progress reports describing ORNL`s research in the mathematical sciences prior to 1984 when those activities moved into the Engineering Physics and Mathematics Division.

  7. Policy Flash 2014-27 Implementation of Division D, Titles III...

    Energy Savers [EERE]

    Appropriations Act, 2014,Pub. L. No. 113-76. (AL) 2014-04 and (FAL) 2014-01 revised Policy Flash 2014-27 Implementation of Division D, Titles III and V, and Division E, Title...

  8. Policy Flash 2013-53 Implementation of Division F, Title I, II...

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

    53 Implementation of Division F, Title I, II, III AL 2013-06 and FAL 2013-04 Policy Flash 2013-53 Implementation of Division F, Title I, II, III AL 2013-06 and FAL 2013-04...

  9. Regulatory pathways controlling cell division after DNA damage in Caulobacter crescentus

    E-Print Network [OSTI]

    Modell, Joshua Wexler

    2013-01-01T23:59:59.000Z

    All cells must coordinate DNA replication with cell division in order to faithfully propagate whole chromosomes to daughter cells. During episodes of DNA damage, cells often delay division until the lesions have been ...

  10. Cognitive Issues in Upper-Division Electricity & Magnetism Steven J. Pollock

    E-Print Network [OSTI]

    Colorado at Boulder, University of

    interventions ­at the upper division. Keywords: physics education research, course reform, electricityCognitive Issues in Upper-Division Electricity & Magnetism Steven J. Pollock and Stephanie V. Chasteen* * Science Education Initiative, University of Colorado, Boulder, CO 80309, USA Department

  11. A DNA Damage-Induced, SOS-Independent Checkpoint Regulates Cell Division in Caulobacter crescentus

    E-Print Network [OSTI]

    Modell, Joshua W.

    Cells must coordinate DNA replication with cell division, especially during episodes of DNA damage. The paradigm for cell division control following DNA damage in bacteria involves the SOS response where cleavage of the ...

  12. Policy Flash 2014-27 Implementation of Division D, Titles III...

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

    7 Implementation of Division D, Titles III and V, and Division E, Title VII of the Consolidated Appropriations Act, 2014,Pub. L. No. 113-76. (AL) 2014-04 and (FAL) 2014-01 revised...

  13. AL 2015-04 - Implementation of Division D, Title III and Title...

    Energy Savers [EERE]

    AL 2015-04 - Implementation of Division D, Title III and Title V, and Division E, Title Title VII of the Consolidated and Further Continuing Appropriations Act, 2015, Pub. L....

  14. Instrumentation and Controls Division progress report, July 1, 1990--June 30, 1992. Volume 2

    SciTech Connect (OSTI)

    Not Available

    1993-01-01T23:59:59.000Z

    This report contains the following information from the Instrumentation and Controls Division of Oak Ridge National Laboratory: supplementary activities; seminars; publications and presentations; scientific and professional activities, achievements, and awards; and division organization charts.

  15. Instrumentation and Controls Division progress report, July 1, 1990--June 30, 1992

    SciTech Connect (OSTI)

    Not Available

    1993-01-01T23:59:59.000Z

    This report contains the following information from the Instrumentation and Controls Division of Oak Ridge National Laboratory: supplementary activities; seminars; publications and presentations; scientific and professional activities, achievements, and awards; and division organization charts.

  16. Oklahoma Cooperative Extension Service Division of Agricultural Sciences and Natural Resources

    E-Print Network [OSTI]

    Balasundaram, Balabhaskar "Baski"

    E-1014 Oklahoma Cooperative Extension Service Division of Agricultural Sciences and Natural Resources Oklahoma State University E-1014 Oklahoma Cooperative Extension Service Division of Agricultural Sciences and Natural Resources Oklahoma State University Habitat Evaluation Guide for the Lesser Prairie

  17. RESEARCH ACTIVITIES Division of Heat and Power Technology

    E-Print Network [OSTI]

    Kazachkov, Ivan

    Euro Necessary space Rig in use: 45m2 (9mx5m), storage: ca 14 m2 (7mx2m) General application Experimental to high subsonic operation Application for industry Testing of aerodynamic damping of blade rows Turbine - Division of Heat and Power Technology Object Cold Flow Test Turbine Brand name ABB STAL design

  18. DIVISION OF SOCIAL SCIENCES PROCESS TO BE FOLLOWED FOR CONSIDERING

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    DIVISION OF SOCIAL SCIENCES PROCESS TO BE FOLLOWED FOR CONSIDERING UC PRESIDENT'S POSTDOCTORAL CALL for proposals for the UC President's and Chancellor's Postdoctoral Fellows Hiring Incentive. It is expected that the investigation of Postdoctoral Fellows through this recruitment program will be handled

  19. ENVIRONMENT, SAFETY, HEALTH, AND QUALITY DIVISION Chapter 24: Training

    E-Print Network [OSTI]

    Wechsler, Risa H.

    ENVIRONMENT, SAFETY, HEALTH, AND QUALITY DIVISION Chapter 24: Training Minimum Training November 2013 URL: http://www-group.slac.stanford.edu/esh/eshmanual/references/trainingReqMinimum.pdf 1 Purpose The purpose of these requirements is to ensure that everyone has the minimum training necessary

  20. ENVIRONMENT, SAFETY, HEALTH, AND QUALITY DIVISION Chapter 24: Training

    E-Print Network [OSTI]

    Wechsler, Risa H.

    ENVIRONMENT, SAFETY, HEALTH, AND QUALITY DIVISION Chapter 24: Training Badging Procedure Product ID: http://www-group.slac.stanford.edu/esh/eshmanual/references/trainingProcedBadging.pdf 1 Purpose that indicates their minimum environment, safety, and health (ESH) training. It covers obtaining a SLAC

  1. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT SMART GRID INFORMATION ASSURANCE report, Smart Grid Information Assurance and Security Technology Assessment was prepared on the following RD&D program areas: · Buildings EndUse Energy Efficiency · Energy Innovations Small Grants

  2. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT Integrated CHP Company, California Air Resource Board, U.S. Department of Energy, Integrated CHP Systems Corporation Integrated CHP Using UltraLow NOx Supplemental Firing is the final report for the Integrated CHP Using Ultra

  3. UC ACADEMIC SENATE SANTA CRUZ DIVISION Committee on Educational Policy

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    UC ACADEMIC SENATE SANTA CRUZ DIVISION Committee on Educational Policy Policy on the Appointment to an undergraduate student appointed in the capacity of a Teaching Assistant. The Committee on Educational Policy to oversee the work of this appointment in compliance with CEP's policy. 2. What General Education

  4. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    the aircraft off the ground for each mission. i #12;PREFACE The California Energy Commission Energy Research/Agricultural/Water End-Use Energy Efficiency · Renewable Energy Technologies · Transportation California AutonomousEnergy Research and Development Division FINAL PROJECT REPORT CALIFORNIA AUTONOMOUS UNMANNED AERIAL

  5. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Energy Research and Development Division FINAL PROJECT REPORT RWE SCHOTT SOLAR Energy Commission Prepared by: RWE Schott Solar, Inc #12; PREPARED BY: Primary Author(s): Miles C on the following RD&D program areas: · Buildings EndUse Energy Efficiency · Energy Innovations Small Grants

  6. Energy Research and Development Division FINAL PROJECT REPORT

    E-Print Network [OSTI]

    Franco Program Area Lead Energy-Related Environmental Research Linda Spiegel Office Manager Energy on the following RD&D program areas: · Buildings EndUse Energy Efficiency · Energy Innovations Small Grants Energy Research and Development Division FINAL PROJECT REPORT AIRQUALITY IMPACTS OF HEAT

  7. Radiological Control Manual Environment, Safety, Health, and Quality Division

    E-Print Network [OSTI]

    Wechsler, Risa H.

    ............................................................................................................................................8 128 Facility Modifications and Radiological Design ConsiderationsRadiological Control Manual Environment, Safety, Health, and Quality Division SLAC-I-720-0A05Z-001 and published by ESHQ Publishing Document Title: Radiological Control Manual Original Publication Date: 1

  8. School and Community Psychology Division of Theoretical and

    E-Print Network [OSTI]

    Berdichevsky, Victor

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    E-Print Network [OSTI]

    Acquisition Services Management (ASM) Division Subcontracts, ASM-SUB P.O. Box 1663, Mail Stop D447-trace of itself while running. Question/Issue 3 This question is on the three codes described in the Trinity Capability Improvement codes on the Cielo system is shown at different node counts. What is the memory

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    E-Print Network [OSTI]

    Acquisition Services Management (ASM) Division Subcontracts, ASM-SUB P.O. Box 1663, Mail Stop D447 that the 'Base case' shall be run with "no OpenMP" threads or "any existing APIs in the codes which exploit SNAP, or MILC codes without using the OpenMP enabling compiler flag. I can provide details of the code

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    E-Print Network [OSTI]

    directly from the sun because harvesting solar energy using photovoltaic technologiesEnergy Research and Development Division FINAL PROJECT REPORT REPORT ON ROUTE TO SCALEUP OF POLYMER Energy Commission Prepared by: California Solar Energy Collaborative(CSEC) University of California Davis

  12. EU Guide v 2d January 20141 Finance Division

    E-Print Network [OSTI]

    de Gispert, Adrià

    EU Guide v 2d January 20141 Finance Division Procurement Services The EU Directives on Public purchasing practice and especially where funders require it as part of their grant conditions. In exceptional Andrew Reid (goods and services) or the Director of Estate Management and Building Services (property

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    E-Print Network [OSTI]

    Kreinovich, Vladik

    Towards Reliable Sub­Division of Geological Areas: Interval Approach David D. Coblentz 1;2 , Vladik difficult to produce a reliable subdivision. The subdivision of a geological zone into segments is often, and often, we do not have a statistically sufficient amount of thoroughly analyzed geological samples

  14. Towards Reliable SubDivision of Geological Areas: Interval Approach

    E-Print Network [OSTI]

    Kreinovich, Vladik

    Towards Reliable Sub­Division of Geological Areas: Interval Approach David D. Coblentz 1;2 , Vladik Difficult to Produce a Reliable Subdivision The subdivision of a geological zone into segments is often the area, and often, we do not have a statistically sufficient amount of thoroughly analyzed geological

  15. Energy and Environmental Systems Division's publications publications 1968-1982

    SciTech Connect (OSTI)

    none,

    1982-03-01T23:59:59.000Z

    Books, journal articles, conference papers, and technical reports produced by the Energy and Environmental Systems Division of Argonne National Laboratory are listed in this bibliography. Subjects covered are energy resources (recovery and use); energy-efficient technology; electric utilities, and environments. (MCW)

  16. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT RANKING AND PRIORITIZING THE DEPLOYMENT OF COMMUNITY- SCALE ENERGY MEASURES BASED ON THEIR INDIRECT EFFECTS IN CALIFORNIA'S CLIMATE ZONES MARCH 2013 CEC-500-2013-122 ALTOSTRATUS Prepared for: California Energy Commission Prepared by

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  18. Energy Research and Development Division FINAL PROJECT REPORT

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  19. Energy Research and Development Division FINAL PROJECT REPORT

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  20. Energy Research and Development Division FINAL PROJECT REPORT

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  1. Energy Research and Development Division FINAL PROJECT REPORT

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  2. Energy Research and Development Division FINAL PROJECT REPORT

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  3. Energy Research and Development Division FINAL PROJECT REPORT

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  4. Energy Research and Development Division FINAL PROJECT REPORT

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  5. Energy Research and Development Division FINAL PROJECT REPORT

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  6. Energy Research and Development Division FINAL PROJECT REPORT

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  8. Energy Research and Development Division FINAL PROJECT REPORT

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  9. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT ENERGY INNOVATIONS: California Energy Commission Prepared by: San Diego State Research Foundation #12; Prepared by: Primary-1858 (619) 594-1900 Contract Number: 500-98-014 Prepared for: California Energy Commission Raquel E. Kravitz

  10. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT LIFECYCLE ENERGY: California Energy Commission Prepared by: University of California, Berkeley Department of Civil-1712 510-642-7300 Contract Number: 500-02-004 Work Authorization MR-048 Prepared for: California Energy

  11. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT TIME OF USE WATER METER IMPACTS · Transportation Time-of-Use Water Meter Impacts on Customer Water Use is the final report for the Time of Use This report was prepared as the result of work sponsored by the California Energy Commission. It does

  12. Accomplishments of the Alaska Region's Habitat Conservation Division

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    -Stevens Fishery Conservation and Management Act, Fish and Wildlife Coordination Act, National Environmental Policy and conservation of Essential Fish Habitat (EFH) through fishery management, and environmental review of nonAccomplishments of the Alaska Region's Habitat Conservation Division in Fiscal Year 2006

  13. Post Retirement Employment Form Division of Human Resources

    E-Print Network [OSTI]

    Meyers, Steven D.

    Post Retirement Employment Form Division of Human Resources Phone (813)974-2970 / Fax (813)974-5227 / SVC 2172 Questions (813) 974-2970 Human Resources / Employment Center Rev. 02/2012 In accordance with the Post Retirement Employment Policy, this form is required for instances of retiree re-employment

  14. MATH AND COMPUTER SCIENCE DIVISION 2001-2003 CATALOG UPDATE

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    Gering, Jon C.

    1 MATH AND COMPUTER SCIENCE DIVISION 2001-2003 CATALOG UPDATE Changes effective 2002-2003 COMPUTER REQUIREMENTS FOUNDATIONS CS 100 Computer Science Seminar 1 CS 180 Foundations of Computer Science I 3 CS 185 Foundations of Computer Science II 3 CS 285 Foundations of Computer Science III 3 CS 310 Data Structures

  15. ALASKA DEPARTMENT OF LABOR & WORKFORCE DEVELOPMENT Division of Workers' Compensation

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    115512, Juneau AK 99811-5512 REPORT OF OCCUPATIONAL INJURY OR ILLNESS AWCB Case Number (Division Use Only # 38. Give Details of How Injury or Illness Happened 39. Injury / Illness Due to Machine / Product Failure? YES NO 40. Mechanical Guard / Safeguards Provided? YES NO 41. List Any Machine / Substance

  16. Division of Economics and Business Working Paper Series

    E-Print Network [OSTI]

    data of wind generation and emissions from plants in ERCOT (Texas), CAISO (California), and MISO (UpperDivision of Economics and Business Working Paper Series Emissions savings from wind power generation: Evidence from Texas, California and the Upper Midwest Daniel T. Kaffine Brannin J. McBee Jozef

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    ORNL/TM-1999/157 ENERGY DIVISION Aluminum R&D for Automotive Uses And the Department of Energy .............................................................................................. 6 3. ROLE OF ALUMINUM IN FUTURE AUTOMOTIVE USES........................................... 7 4. COST's Role S.W. Hadley S. Das J.W. Miller March 2000 Prepared for the Office of Advanced Automotive

  18. Division of Administration and Finance Facilities Planning and Construction

    E-Print Network [OSTI]

    Bittner, Eric R.

    Division of Administration and Finance Facilities Planning and Construction News Release the construction fence into the Entrance 6 roadway to accommodate new landscaping and site work for the Cougar will be present to assist with traffic flow during construction work hours, typically 7 a.m. to 5 p.m., Monday

  19. Division of Economics and Business Working Paper Series

    E-Print Network [OSTI]

    ;1 Introduction Thermal electricity from fossil sources generates CO2 emissions as a by-product, and car- bon and fuel. The costs of emitting CO2 are thus passed through to the ultimate "polluters", i.e. the consumersDivision of Economics and Business Working Paper Series Carbon content of electricity futures

  20. Physics division. Progress report for period ending September 30, 1996

    SciTech Connect (OSTI)

    Ball, S.J. [ed.

    1997-04-01T23:59:59.000Z

    This report covers the research and development activities of the Physics Division for the 1995 and 1996 fiscal years, beginning October 1, 1994, and ending September 30, 1996. The activities of the Division continue to be concentrated in the areas of experimental nuclear physics, experimental atomic physics, and theoretical nuclear and atomic physics. In addition, there are smaller programs in plasma diagnostics and data compilation and evaluation. During the period of this report, there has been considerable success in bringing the Holifield Radioactive Ion Beam Facility (HRIBF) into routine operation. The budgets of the nuclear physics portion of the Division have increased each year in nearly all areas, and several new members have been added to the Division research and development staff. On August 30, 1996, the HRIBF successfully accelerated its first radioactive ion beams, {sup 69}As and {sup 70}As. Prior to this, the heart of the facility, the RIB injector system, was completed, including installation of a remote handling system for the target/ion source assembly. Target and ion source development is likely to be the technical key to success of the HRIBF. We have expanded our efforts in those development areas. Of special note is the development of highly permeable composite targets which have now been shown to allow release of difficult-to-produce radioactive ions such as {sup 17,18}F. A summary of the HRIBF work is provided in Chapter 1, along with supporting activities of the Joint Institute for Heavy Ion Research.

  1. Accelerator and Fusion Research Division 1989 summary of activities

    SciTech Connect (OSTI)

    Not Available

    1990-06-01T23:59:59.000Z

    This report discusses the research being conducted at Lawrence Berkeley Laboratory's Accelerator and Fusion Research Division. The main topics covered are: heavy-ion fusion accelerator research; magnetic fusion energy; advanced light source; center for x-ray optics; exploratory studies; high-energy physics technology; and bevalac operations.

  2. Oklahoma State University Division of Agricultural Sciences and Natural Resources

    E-Print Network [OSTI]

    Balasundaram, Balabhaskar "Baski"

    E-979 Oklahoma State University Division of Agricultural Sciences and Natural Resources Oklahoma. Bartholomew Big Game Biologist Oklahoma Department of Wildlife Conservation White-tailed Deer Habitat-Soil Conservation Service (now NRCS) in Oklahoma. The authors greatly appreciate Dr. Teels' efforts in initiating

  3. Algebra -The Euclidean Division Algorithm 30 March 2010

    E-Print Network [OSTI]

    Banaji,. Murad

    Algebra - The Euclidean Division Algorithm 30 March 2010 19:10 Lessons - Tanya Page 1 #12;Algebra - Base Representation 30 March 2010 19:26 Lessons - Tanya Page 2 #12;Algebra - Base Representation Exam Examples 30 March 2010 19:45 Lessons - Tanya Page 3 #12;Algebra - Partial Fractions 02 April 2010 09

  4. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT COMPENSATION CEC5002013114 Prepared for: California Energy Commission Prepared by: Stratus Consulting Inc. #12-04-025 Prepared for: California Energy Commission Joe O'Hagan Contract Manager Linda Spiegel Office Manager Energy

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    Energy Research and Development Division FINAL PROJECT REPORT THE ICHTHYOPLANKTON OF KING HARBOR, REDONDO BEACH, CALIFORNIA 19742006 APRIL 2008 CEC5002013053 Prepared for: California Energy Angeles, CA 90041 Contract Number: 500-04-025 Prepared for: California Energy Commission Joseph O

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    Energy Research and Development Division FINAL PROJECT REPORT ADVANCED CHARACTERIZATION OF WIND RESOURCES IN SELECTED FOCUS AREAS OF CALIFORNIA Prepared for: California Energy Commission Prepared by: AWS-06-024 Prepared for: California Energy Commission Mike Kane Contract Manager Linda Spiegel Office Manager Energy

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    Energy Research and Development Division FINAL PROJECT REPORT DEVELOPMENT OF STEAM for: California Energy Commission Prepared by: University of California #12; PREPARED BY: Primary-781-5791 951-781-5790 (fax) Contract Number: 500-09-008 Prepared for: California Energy Commission David

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    Energy Research and Development Division FINAL PROJECT REPORT REDUCTIONS IN URBAN OUTDOOR WATER USE-2013-152 Prepared for: California Energy Commission Prepared by: University of California #12;PREPARED BY: Primary of California, Los Angeles Contract Number: PIR-08-005 Prepared for: California Energy Commission Joseph O

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    Energy Research and Development Division FINAL PROJECT REPORT CALIFORNIA TRANSMISSION CONGESTION ASSESSMENT DECEMBER 2007 CEC-500-2011-007 Prepared for: California Energy Commission Prepared by: Electric Pasadena, CA Contract Number: BOA-142 Prepared for: California Energy Commission Jamie Patterson Contract

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    Energy Research and Development Division FINAL PROJECT REPORT AN ECONOMIC ANALYSIS OF SIX DAIRY DIGESTER SYSTEMS IN CALIFORNIA Volume 2 MARCH 2013 CEC-500-2014-001-V2 Prepared for: California Energy: California Energy Commission Abolghasem Edalati Contract Manager Linda Spiegel Office Manager Energy

  11. Energy Research and Development Division FINAL PROJECT REPORT

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  12. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT LIFE-CYCLE ASSESSMENT AND URBAN SUSTAINABILITY OCTOBER 2010 CEC-500-2013-129 Prepared for: California Energy Commission Prepared by: University for: California Energy Commission Erik Stokes Contract Manager Linda Spiegel Office Manager Energy

  13. Energy Research and Development Division FINAL PROJECT REPORT

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    Energy Research and Development Division FINAL PROJECT REPORT COMMERCE ENERGY BIOGAS/PV MINIGRID in California APRIL 2012 CEC-500-2013-127 Prepared for: California Energy Commission Prepared by: CH2MHill #12 Number: 500-00-036 Prepared for: California Energy Commission Zhiqin Zhang Contract Manager Linda Spiegel

  14. Division of Residential and Campus Communities Review Interim Report

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    Botea, Adi

    Division of Residential and Campus Communities Review Interim Report December 2013 As stressed in the University's strategic plan ANU by 2020, the residential experience is a key aspect of the holistic ANU experience of all students by providing a richer residential experience for on-campus students and more

  15. Department of Natural Resources Division of Oil, Gas and Mining

    E-Print Network [OSTI]

    Tipple, Brett

    . The division will continue to work with companies involved in energy development, government agencies of the population within Utah. Worldwide and regional commodity prices have historically been the most significant of few states with this incentive.) 2. Half-price day-use access for seniors who choose not to purchase

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  17. ENVIRONMENT, SAFETY & HEALTH DIVISION Chapter 19: Personal Protective Equipment

    E-Print Network [OSTI]

    Wechsler, Risa H.

    : http://www-group.slac.stanford.edu/esh/eshmanual/references/PPEQuickstart.pdf 1 Who needs to know about from the Environment, Safety, and Health (ESH) Division, and workers must be trained or informed appropriate ESH Manual chapter. SLAC is responsible for providing PPE to its employees, Stanford University

  18. ENVIRONMENT, SAFETY & HEALTH DIVISION Chapter 0: About This Manual

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    Wechsler, Risa H.

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    Edison Taylor Engineering The New York Times TRACO University of California, Berkeley UniversityEnergy Research and Development Division FINAL PROJECT REPORT HIGH PERFORMANCE BUILDING FAÃ?ADE SOLUTIONS NOVEMBER 2009 CEC-500-2012-049 Prepared for: California Energy Commission Prepared by: Lawrence

  20. Decision and Information Sciences Division Information Sciences Group CCyybbeerr SSeeccuurriittyy

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    Kemner, Ken

    in industry (e.g., gas, oil, electric, water) to monitor and control remote equipment from a central facilityDecision and Information Sciences Division Information Sciences Group CCyybbeerr SSeeccuurriittyy Network analysis and cyber security lab Introduction In today's environment, it is essential to assure