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Sample records for albert einstein distinguished

  1. Albert Einstein Distinguished Educator Fellowship Program accepting

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

    applications for 2017-2018 Albert Einstein Distinguished Educator Fellowship Program accepting applications for 2017-2018 Deadline for applying is Nov. 17, 2016, at 8 p.m. EST FOR IMMEDIATE RELEASE August 19, 2016 FY16-44 Chad Becker, Eddy Whitson and Kevin Fritts with EPA ENERGY STAR certificate WASHINGTON, D.C.-The U.S. Department of Energy's Albert Einstein Distinguished Educator Fellowship Program is now accepting applications for 2017-2018. The program provides a unique opportunity for

  2. Albert Einstein Distinguished Educator Fellowship Program accepting

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

    | National Nuclear Security Administration | (NNSA) Albert Einstein Alerts President Roosevelt of German Atomic Energy Program Albert Einstein Alerts President Roosevelt of German Atomic Energy Program Washington, DC Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions and the possibility that research might lead to developing powerful bombs. Einstein notes that Germany has stopped the sale of uranium and

  3. Albert Einstein Distinguished Educator Fellowship Act of 1994 in U.S.C. |

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

    Department of Energy Albert Einstein Distinguished Educator Fellowship Act of 1994 in U.S.C. Albert Einstein Distinguished Educator Fellowship Act of 1994 in U.S.C. CITE: 42USC7382 TITLE 42--THE PUBLIC HEALTH AND WELFARE CITE: 42USC7382a TITLE 42--THE PUBLIC HEALTH AND WELFARE CITE: 42USC7382b TITLE 42--THE PUBLIC HEALTH AND WELFARE CITE: 42USC7382c TITLE 42--THE PUBLIC HEALTH AND WELFARE CITE: 42USC7382d TITLE 42--THE PUBLIC HEALTH AND WELFARE CITE: 42USC7382e TITLE 42--THE PUBLIC HEALTH

  4. Energy Principles into High School Physics Dr. Ann Reimers, Albert Einstein Distinguished Educator Fellow

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

    Integrating a Holistic View of Energy Principles into High School Physics Dr. Ann Reimers, Albert Einstein Distinguished Educator Fellow Department of Energy -> UVa American Association of Physics Teachers Summer Meeting 2015 DOE Energy Literacy Framework 2 * Energy Literacy Framework is a guide to help energy educators teach energy from the natural to the social sciences. Also available in Spanish. http://energy.gov/eere/education/energy-literacy-essential-principles-and-fundamental-

  5. Zurek awarded Albert Einstein

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

    Zurek awarded Albert Einstein professorship prize July 30, 2010 LANL quantum theorist to serve as visiting professor at the University of Ulm LOS ALAMOS, New Mexico, July 30,...

  6. Zurek awarded Albert Einstein professorship prize

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

    Einstein professorship prize Zurek awarded Albert Einstein professorship prize Prize honors Ulm's connection with Albert Einstein, who was born in the city in 1879. July 30, 2010...

  7. Interviews in Washington, DC for Albert Einstein Fellowship Semi-Finalists

    Broader source: Energy.gov [DOE]

    Selected semi-finalists in the Albert Einstein Distinguished Educator Fellowship are invited to DC for interviews.

  8. OSTIblog Articles in the Albert Einstein Topic | OSTI, US Dept...

    Office of Scientific and Technical Information (OSTI)

    Albert Einstein Topic "The New Einsteins Will Be Scientists Who Share." by Kate Bannan 01 Nov, 2011 in Science Communications 4355 225px-Einstein1921portrait2.jpg "The New ...

  9. Albert Einstein Alerts President Roosevelt of German Atomic Energy Program

    National Nuclear Security Administration (NNSA)

    | National Nuclear Security Administration | (NNSA) Albert Einstein Alerts President Roosevelt of German Atomic Energy Program Albert Einstein Alerts President Roosevelt of German Atomic Energy Program Washington, DC Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions and the possibility that research might lead to developing powerful bombs. Einstein notes that Germany has stopped the sale of uranium and

  10. Albert Einstein Alerts President Roosevelt of German Atomic Energy...

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

    Atomic Energy Program Washington, DC Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions ...

  11. Albert Einstein Distinguished Educator Fellowship Program accepting...

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

    Deadline for applying is Nov. 19, 2015, at 8 p.m. EST FOR IMMEDIATE RELEASE Oct. 7, 2015 ... Program applications are due by Thurs., Nov. 19, 2015, at 8 p.m. EST and must be submitted ...

  12. Albert Einstein Distinguished Educator Fellowship (AEF) Program...

    Office of Science (SC) Website

    ... advising on policies that seek to improve K-12 education in the United States; Creating web-based science education tools; and Establishing and evaluating national and regional ...

  13. OSTIblog Articles in the Albert Einstein Topic | OSTI, US Dept of Energy

    Office of Scientific and Technical Information (OSTI)

    Office of Scientific and Technical Information Albert Einstein Topic "The New Einsteins Will Be Scientists Who Share." by Kate Bannan 01 Nov, 2011 in Science Communications 4355 225px-Einstein_1921_portrait2.jpg "The New Einsteins Will Be Scientists Who Share." Read more about 4355 In an October 29, 2011 Wall Street Journal article, "The New Einsteins Will Be Scientists Who Share," Dr. Michael Nielsenstated that networked science has the potential to speed up

  14. Albert Einstein - Hanford Site

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

    Alaska

    Decade Year-0 Year-1 Year-2 Year-3 Year-4 Year-5 Year-6 Year-7 Year-8 Year-9 1960's 65,817 99,303 149,647 1970's 217,854 228,172 222,905 223,288 229,963 253,227 269,111 373,791 596,834 732,990 1980's 893,759 943,059 1,084,732 1,164,602 1,206,370 1,343,553 1,375,054 1,694,870 1,933,047 1,965,013 1990's 2,053,324 2,378,896 2,625,713 2,778,341 3,085,900 3,369,904 3,373,584 3,380,950 3,378,848 3,362,082 2000's 3,529,394 3,427,779 3,477,438 3,578,305 3,644,084 3,642,948 3,205,751 3,479,290

  15. Manhattan Project: Einstein's Letter to Roosevelt

    Office of Scientific and Technical Information (OSTI)

    EINSTEIN'S LETTER TO ROOSEVELT Albert Einstein (with Leo Szilard) to President Franklin Roosevelt, August 2, 1939 Resources > Library Below are photographs of both pages of the ...

  16. Albert Carnesale | Department of Energy

    Energy Savers [EERE]

    Albert Carnesale About Us Albert Carnesale - Chancellor Emeritus and Professor, University of California, Los Angeles Albert Carnesale Albert Carnesale is Chancellor Emeritus and ...

  17. August 2, 1939: Einstein's Letter | Department of Energy

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

    , 1939: Einstein's Letter August 2, 1939: Einstein's Letter August 2, 1939: Einstein's Letter August 2, 1939 Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions and the possibility that research might lead to developing powerful bombs. Einstein notes that Germany has stopped the sale of uranium and German physicists are engaged in uranium research

  18. Albert Kang | Photosynthetic Antenna Research Center

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

    Albert Kang Albert Kang Albert Kang Graduate Student E-mail: h.kang@wustl.edu Website: Washington University in St. Louis Graduate Students

  19. Recommender Information | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Recommender Information Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Recommender...

  20. Distinguished Awards

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

    Distinguished Awards Distinguished Awards The Lab's mission is to develop and apply science and technology to ensure the safety, security, and reliability of the U.S. nuclear deterrent; reduce global threats; and solve other emerging national security and energy challenges. Contact Jenna L. Montoya (505) 665-4230 Email Without continual growth and progress, such words as improvement, achievement, and success have no meaning. ~ Benjamin Franklin Awards, peer recognition for Los Alamos National

  1. Centenarian Einstein

    ScienceCinema (OSTI)

    None

    2011-04-25

    Commémoration de A.Einstein avec 4 orateurs pour honnorer sa mémoire: le prof.Weisskopf parlera de l'homme de science engagé, Daniel Amati du climat de la physique aux années 1920, Sergio Fubini de l'heure scientifique d'A.Einstein et le prof.Berob(?)

  2. Einstein: His Impact on Accelerators; His Impact on theWorld

    SciTech Connect (OSTI)

    Sessler, A.

    2005-07-30

    The impact of the work of Albert Einstein on accelerator physics is described. Because of the limit of time, and also because the audience knows the details, the impact is described in broad strokes. Nevertheless, it is seen how his work has affected many different aspects of accelerator physics. In the second half of the talk, Albert Einstein's impact on the world will be discussed; namely his work on world peace (including his role as a pacifist, in the atomic bomb, and in arms control) and his efforts as a humanitarian (including his efforts on social justice, anti-racism, and civil rights).

  3. How to Apply | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    How to Apply Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Recommender Information...

  4. Albert "Al" J. Williams | Department of Energy

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

    Albert "Al" J. Williams About Us Albert "Al" J. Williams - President, Chevron Pipe Line Company (CPL) Albert “Al” J. Williams Albert (Al) J. Williams is president of Chevron Pipe Line Company (CPL), a wholly-owned subsidiary of Chevron Corporation, a role he assumed in May 2014. He is responsible for managing an extensive network of crude oil, natural gas and refined product pipelines, as well as storage facilities in North America. CPL also provides technical,

  5. Albert City, Iowa: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Albert City, Iowa: Energy Resources Jump to: navigation, search Equivalent URI DBpedia Coordinates 42.7819199, -94.9485993 Show Map Loading map... "minzoom":false,"mappingserv...

  6. Beyond Einstein

    SciTech Connect (OSTI)

    Primack, Joel

    2007-10-08

    The National Academy of Sciences was commissioned in 2006 to report on how to restart the Beyond Einstein program, which includes missions to understand dark energy, test general relativity, and observe gravity waves from merging supermassive black holes. This colloquium by one of the members of the recently released Academy study will explain the research strategy that the report proposes and its implications for continued U.S. participation in the exploration of the universe.

  7. Albert Lea, Minnesota: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Hide Map This article is a stub. You can help OpenEI by expanding it. Albert Lea is a city in Freeborn County, Minnesota. It falls under Minnesota's 1st...

  8. Fellows Central | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    The 2015-16 Albert Einstein Distinguished Educator fellows, who are placed in the Department of Energy, the National Science Foundation, the National Aeronautics and Space ...

  9. STEM Mentoring Café- Engaging Young Women in an Authentic Mentoring...

    Office of Environmental Management (EM)

    STEM Mentoring Caf- Engaging Young Women in an Authentic Mentoring Experience Melinda Higgins Albert Einstein Distinguished Educator Fellow, NASA Office of Education, ...

  10. ORISE: News Releases

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

    for 2016-2017 pilot program to research building to grid integration 10072015 Albert Einstein Distinguished Educator Fellowship Program accepting applications for...

  11. Scholten_abs_2012.pdf

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

    Scholarships and Fellowships Scholarships and Fellowships Energy Department Scholarships and Fellowships: Albert Einstein Distinguished Educator Fellowship Program The Albert Einstein Distinguished Educator Fellowship Act was signed into law in November 1994. The law gives the Department of Energy responsibility for administering the program of distinguished educator fellowships for elementary and secondary school mathematics and science teachers. Selected teachers spend eleven months in a

  12. Einstein for Everyone

    ScienceCinema (OSTI)

    Piccioni, Robert

    2014-06-25

    Young Einstein was a rebel who seemed doomed to fail. How did he overcome rejection to become the most famous scientist in history? We will discuss and explain all his theories in plain English and without math, and we will discover how Einstein's achievements impact our lives through DVDs, GPS, iPods, computers and green energy.

  13. Distinguished Alumni Award

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

    in 2003 as a Frederick Reines Distinguished Fellow and became a staff member in 2006. Chavez is a team leader at LANL and a project leader in the DOEDoD Joint Munitions Program. ...

  14. Additional Distinguished Awards

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

    Additional Distinguished Awards Additional Distinguished The Lab's mission is to develop and apply science and technology to ensure the safety, security, and reliability of the U.S. nuclear deterrent; reduce global threats; and solve other emerging national security and energy challenges. Contact Jenna L. Montoya (505) 665-4230 Email The atomic bomb made the prospect of future war unendurable. It has led us up those last few steps to the mountain pass; and beyond there is a different country. ~

  15. Zerkle wins Governor's Distinguished

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

    Zerkle wins Governor's Distinguished Public Service award October 29, 2009 Stimulus Project leader joins elite handful of outstanding LANL employees Los Alamos, New Mexico, OCTOBER 29, 2009-Carolyn E. Zerkle, leader of Los Alamos National Laboratory's Stimulus Project, has been named a 2009 winner of the Governor's New Mexico Distinguished Public Service Award.Zerkle is one of 10 recipients of the prestigious award, which recognizes outstanding contributions to public service and the improvement

  16. einstein.jpg | OSTI, US Dept of Energy Office of Scientific and Technical

    Office of Scientific and Technical Information (OSTI)

    Information einstein

  17. Eligibility | U.S. DOE Office of Science (SC)

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

    Eligibility Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Contact WDTS Home Eligibility Print Text Size: A A A FeedbackShare Page Eligibility for the Albert Einstein Distinguished Educator Fellowship Program requires that all applicants: Be a U.S. citizen at the time of applying (by the November 17, 2016 application deadline). Have a minimum of five

  18. DOE Cyber Distinguished Speaker Series

    Broader source: Energy.gov [DOE]

    Join us at the Department of Energy’s Cyber Distinguished Speaker Series on Wednesday, 13 January 2016, for an opportunity to expand your knowledge and awareness of today’s most pressing cyber issues.

  19. Einstein and Energy Efficiency: Making Homes Smarter (301) |...

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

    Einstein and Energy Efficiency: Making Homes Smarter (301) Einstein and Energy Efficiency: Making Homes Smarter (301) February 4...

  20. Einstein and the Daytime Sky - A

    Office of Scientific and Technical Information (OSTI)

    Einstein found how this relates to the reason the sky is blue. A B C D A. A path with a ... exist, we may, somewhat unconsciously, associate Einstein with the dark nighttime sky. ...

  1. Connecting the Classroom: Guiding Energy Educators | Department of Energy

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

    Connecting the Classroom: Guiding Energy Educators Connecting the Classroom: Guiding Energy Educators September 25, 2013 - 10:13am Addthis Josh Sneideman is an Albert Einstein Distinguished Educator Fellow and helps lead the Energy Department's Energy Literacy efforts. (Photo courtesy of Eco Organization) Josh Sneideman is an Albert Einstein Distinguished Educator Fellow and helps lead the Energy Department's Energy Literacy efforts. (Photo courtesy of Eco Organization) Daniel Boff Daniel Boff

  2. Entropic corrections to Einstein equations

    SciTech Connect (OSTI)

    Hendi, S. H. [Physics Department, College of Sciences, Yasouj University, Yasouj 75914 (Iran, Islamic Republic of); Research Institute for Astronomy and Astrophysics of Maragha (RIAAM), Maragha (Iran, Islamic Republic of); Sheykhi, A. [Research Institute for Astronomy and Astrophysics of Maragha (RIAAM), Maragha (Iran, Islamic Republic of); Department of Physics, Shahid Bahonar University, P.O. Box 76175-132, Kerman (Iran, Islamic Republic of)

    2011-04-15

    Considering the general quantum corrections to the area law of black hole entropy and adopting the viewpoint that gravity interprets as an entropic force, we derive the modified forms of Modified Newtonian dynamics (MOND) theory of gravitation and Einstein field equations. As two special cases we study the logarithmic and power-law corrections to entropy and find the explicit form of the obtained modified equations.

  3. He Said She Said: The Einstein and Energy Efficiency: Making...

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

    He Said She Said: The Einstein and Energy Efficiency: Making Homes Smarter (301) He Said She Said: The Einstein and Energy Efficiency: Making Homes Smarter (301) February 1...

  4. Einstein and Energy Efficiency: Making Homes Smarter (301) |...

    Energy Savers [EERE]

    Einstein and Energy Efficiency: Making Homes Smarter (301) Einstein and Energy Efficiency: Making Homes Smarter (301) Better Buildings Residential Network Peer Exchange Call ...

  5. Manhattan Project: Events Images

    Office of Scientific and Technical Information (OSTI)

    Scroll down to see each of these images individually. The images are: 1. Albert Einstein ... Albert Einstein and Leo Szilard Albert Einstein and Leo Szilard Painting of CP-1 going ...

  6. distinguished University of New Mexico alumni

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

    distinguished University of New Mexico alumni - Sandia Energy Energy Search Icon Sandia Home ... Stationary Power Energy Conversion Efficiency Solar Energy Wind Energy Water Power ...

  7. 2 Cornellians receive Distinguished Scholar Award > Archived...

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

    degradation mechanism in fuel cells, while Kayla was honored for her contribution in air-SEM system. The Distinguished Scholar Award, which is the most prestigious MAS student...

  8. Quantum theory and Einstein's general relativity

    SciTech Connect (OSTI)

    v. Borzeszkowski, H.; Treder, H.

    1982-11-01

    We dicusss the meaning and prove the accordance of general relativity, wave mechanics, and the quantization of Einstein's gravitation equations themselves. Firstly, we have the problem of the influence of gravitational fields on the de Broglie waves, which influence is in accordance with Einstein's weak principle of equivalence and the limitation of measurements given by Heisenberg's uncertainty relations. Secondly, the quantization of the gravitational fields is a ''quantization of geometry.'' However, classical and quantum gravitation have the same physical meaning according to limitations of measurements given by Einstein's strong principle of equivalence and the Heisenberg uncertainties for the mechanics of test bodies.

  9. Stability of the Einstein static universe in Einstein-Cartan theory

    SciTech Connect (OSTI)

    Atazadeh, K., E-mail: atazadeh@azaruniv.ac.ir [Department of Physics, Azarbaijan Shahid Madani University, Tabriz, 53714-161 (Iran, Islamic Republic of)

    2014-06-01

    The existence and stability of the Einstein static solution have been built in the Einstein-Cartan gravity. We show that this solution in the presence of perfect fluid with spin density satisfying the Weyssenhoff restriction is cyclically stable around a center equilibrium point. Thus, study of this solution is interesting because it supports non-singular emergent cosmological models in which the early universe oscillates indeterminately about an initial Einstein static solution and is thus past eternal.

  10. Celebrating Einstein A Series of Articles

    Office of Scientific and Technical Information (OSTI)

    But at that time Einstein found, in a newly-discovered physical law, a clue that there was more to light than the wave theory of those days seemed to suggest. Solid Cold - By the ...

  11. The Manhattan Project

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

    Ames, Iowa * Ames Laboratory History Grand Junction, Colorado, Site Top Key Events: August 2, 1939 -- Albert Einstein's Letter to President Franklin D. Roosevelt * Albert Einstein ...

  12. Was Einstein Right? A Centennial Assessment

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

    Was Einstein Right? A Centennial Assessment Clifford M. Will University of Florida March 30, 2016 4:00 p.m. - Wilson Hall, One West Einstein formulated general relativity 100 years ago. Although it is generally considered a great triumph, the theory's early years were characterized by conceptual confusion, empirical uncertanities and a lack of relevance to ordinary physics. But in recent decades, a remarkably diverse set of precision experiments has established it as the "standard

  13. Einstein's Biggest Blunder: A Cosmic Mystery Story

    ScienceCinema (OSTI)

    Krauss, Lawrence

    2010-09-01

    The standard model of cosmology built up over 20 years is no longer accepted as accurate. New data suggest that most of the energy density of the universe may be contained in empty space. Remarkably, this is exactly what would be expected if Einstein's cosmological constant really exists. If it does, its origin is the biggest mystery in physics and presents huge challenges for the fundamental theories of elementary particles and fields. Krauss explains Einstein's concept and describes its possible implications.

  14. Argonne announces 2015 Distinguished Fellows | Argonne National...

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

    EmailPrint The U.S. Department of Energy's Argonne National Laboratory has named Barry Smith, Charles Macal and Branko Ruscic as its 2015 Distinguished Fellows. The Argonne...

  15. Argonne Distinguished Fellows | Argonne National Laboratory

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

    Argonne Distinguished Fellows The Argonne Distinguished Fellow is the highest scientific/engineering rank at the laboratory, and this distinction is held by only a small fraction (approximately 3 percent) of the research staff. Staff members who achieve this rank have a widely recognized international reputation and have demonstrated exceptional achievements in science or engineering that are relevant to Argonne's core missions (e.g., seminal discoveries or advances that have broad influence and

  16. Zerkle wins Governor's Distinguished Public Service award

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

    Governor's Distinguished Public Service award Zerkle wins Governor's Distinguished Public Service award The award recognizes outstanding contributions to public service and the improvement of government at all levels by private citizens and government employees. October 29, 2009 Los Alamos National Laboratory sits on top of a once-remote mesa in northern New Mexico with the Jemez mountains as a backdrop to research and innovation covering multi-disciplines from bioscience, sustainable energy

  17. Argonne Distinguished Fellows | Argonne National Laboratory

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

    Argonne Distinguished Fellows Argonne's world-class scientists have achieved national and international recognition, including: Three Nobel Prizes, 119 R&D 100 Awards, More than 700 national and international awards and honors, and More than 800 patents. The Argonne Distinguished Fellow is the highest scientific/engineering rank at the laboratory, and this distinction is held by only a small fraction (approximately 3 percent) of the research staff. Staff members who achieve this rank have a

  18. Emergent Properties of the Bose-Einstein-Hubbard Condensate in...

    Office of Scientific and Technical Information (OSTI)

    Technical Report: Emergent Properties of the Bose-Einstein-Hubbard Condensate in UO2(+x) Citation Details In-Document Search Title: Emergent Properties of the Bose-Einstein-Hubbard ...

  19. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Persis Drell, Co-Chair; Albert Carnesale; Ram Shenoy;

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

    John Deutch, Co-Chair; Persis Drell, Co-Chair; Albert Carnesale; Ram Shenoy; Cherry Murray; Shirley Jackson; Dan Reicher; Martha Schlicher; Rafael Bras; Albert Carnesale; Dan Yergin; Deborah Jin; Michael McQuade; John Podesta Date and Time: 8:00 AM- 12:15 PM, December 3, 2013 Location: Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94550 Purpose: Meeting of the Secretary of Energy Advisory Board (SEAB) SEAB Staff: Amy Bodette, Designated Federal Officer; Karen

  20. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Chair; Arun Majumdar, Vice Chair; Rafael Bras; Albert Carnesale;

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

    Arun Majumdar, Vice Chair; Rafael Bras; Albert Carnesale; Deborah Jin; Paul Joskow (via teleconference); Michael McQuade; Richard Meserve; and Dan Reicher Date and Time: December 3, 2014, 9:00 AM - 12:15 PM MST Location: National Renewable Energy Laboratory (NREL) Education Center 15013 Denver West Parkway, Golden, CO Purpose: Meeting of the Secretary of Energy Advisory Board (SEAB) SEAB Staff: Karen Gibson, Designated Federal Officer; Corey Williams-Allen, Deputy Designated Federal Officer;

  1. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Chair; Frances Beinecke, Rafael Bras, Albert Carnesale, Deborah

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

    Chair; Frances Beinecke, Rafael Bras, Albert Carnesale, Deborah Jin, Paul Joskow, Steve Koonin, Michael McQuade, Richard Meserve, Cherry Murray, Dan Reicher, Ram Shenoy, Ellen Tauscher, Dan Yergin Date and Time: 11:30AM - 12:30PM ET, February 17, 2015 Location: Conference Call Purpose: Meeting of the Secretary of Energy Advisory Board (SEAB) SEAB Staff: Karen Gibson, Designated Federal Officer; Corey Williams-Allen, Deputy Designated Federal Officer; and Matthew Schaub, Deputy Director Meeting

  2. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Frances Beinecke; Albert Carnesale; Shirley Jackson;

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

    Beinecke; Albert Carnesale; Shirley Jackson; Deborah Jin; Paul Joskow; Steven Koonin; Arun Majumdar (via teleconference); Michael McQuade; Richard Meserve; Cherry Murray; Carmichael Roberts; Ram Shenoy; Martha Schlicher; Daniel Yergin; Date and Time: 9:00 AM- 12:15 PM, September 5, 2014 Location: U.S. Department of Energy Forrestal Building, 1000 Independence Avenue SW, Washington, D.C. 20585 Purpose: Meeting of the Secretary of Energy Advisory Board (SEAB) SEAB Staff: Karen Gibson, Designated

  3. Dark-dark solitons and modulational instability in miscible two-component Bose-Einstein condensates

    SciTech Connect (OSTI)

    Hoefer, M. A.; Chang, J. J.; Hamner, C.; Engels, P.

    2011-10-15

    We investigate the dynamics of two miscible superfluids experiencing fast counterflow in a narrow channel. The superfluids are formed by two distinguishable components of a trapped dilute-gas Bose-Einstein condensate (BEC). The onset of counterflow-induced modulational instability throughout the cloud is observed and shown to lead to the proliferation of dark-dark vector solitons. These solitons do not exist in single-component systems, exhibit intriguing beating dynamics, and can experience a transverse instability leading to vortex line structures. Experimental results and multidimensional numerical simulations are presented.

  4. Tomé wins Distinguished Scientist, Engineer Award

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

    Recipient of the 2013 Distinguished ScientistEngineer Award Tom wins Distinguished Scientist, Engineer Award The Minerals, Metals & Materials Society recognized Tom for his ...

  5. Live: DOE Cyber Distinguished Speaker Series | Department of...

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

    Live: DOE Cyber Distinguished Speaker Series Live: DOE Cyber Distinguished Speaker Series Live streaming video by Ustream HOW ACADEMIC INSTITUIONS ARE MEETING TODAY'S CYBER ...

  6. Dan Arvizu has had a long, distinguished

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

    Arvizu has had a long, distinguished career in advanced energy research and development, materials science, and technology commercialization. In 2015, he retired as the longest serving Director of the U.S. Department of Energy's National Renewable Energy Laboratory (NREL) in Golden, Colorado, where he is now Director Emeritus. He is also currently serving as a Precourt Energy Scholar at Stanford University. Prior to joining NREL, Arvizu was a chief technology officer with CH2M HILL Companies,

  7. UNCLASSIFIED Los Alamos Astrophysics Distinguished Seminar Series

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

    Los Alamos Astrophysics Distinguished Seminar Series Ryan Miranda Cornell University Sustained Dust Asymmetries At Dead Zone Edges in Protoplanetary Disks Thursday, July 21, 2016 2:00 PM - 3:00 PM T-DO Conf Room (TA-03, Building 123, Room 121) Abstract. Protoplanetary disks, consisting of gas and dust in orbit around a newly formed star, are the birthplaces of planetary systems. Several observations of transition disks, a class of protoplanetary disks in which the first stages of planet

  8. LLNL Distinguished Members of Technical Staff

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

    honors / dmts awards LLNL Distinguished Members of Technical Staff The Distinguised Members of Technical Staff (DMTS) classification, established in 2011, was created to serve as a career ladder for LLNL scientists and engineers within the Science & Engineering classification structure. It appropriately recognizes outstanding science and technology excellence with distinction and compensation while allowing the honored recipients to remain focused on delivering science and engineering

  9. Time Reversal of Bose-Einstein Condensates

    SciTech Connect (OSTI)

    Martin, J.; Georgeot, B.; Shepelyansky, D. L. [Laboratoire de Physique Theorique, Universite de Toulouse III, CNRS, 31062 Toulouse (France)

    2008-08-15

    Using Gross-Pitaevskii equation, we study the time reversibility of Bose-Einstein condensates (BEC) in kicked optical lattices, showing that in the regime of quantum chaos, the dynamics can be inverted from explosion to collapse. The accuracy of time reversal decreases with the increase of atom interactions in BEC, until it is completely lost. Surprisingly, quantum chaos helps to restore time reversibility. These predictions can be tested with existing experimental setups.

  10. Einstein and the Daytime Sky - B

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

    B. Effects of an uneven random distribution Einstein's work involved giving some greater mathematical precision to some recent ideas of the physicist Marian von Smoluchowski. Smoluchowski considered the significant effect that variations in a fluid's density can have on how light waves travel through the fluid. When a fluid, either gas or liquid, is compressed, its molecules get crowded into a smaller space, so the fluid becomes more dense. Since molecules constantly move about in random

  11. Extended Horava gravity and Einstein-aether theory

    SciTech Connect (OSTI)

    Jacobson, Ted

    2010-05-15

    Einstein-aether theory is general relativity coupled to a dynamical, unit timelike vector. If this vector is restricted in the action to be hypersurface orthogonal, the theory is identical to the IR limit of the extension of Horava gravity proposed by Blas, Pujolas and Sibiryakov. Hypersurface orthogonal solutions of Einstein-aether theory are solutions to the IR limit of this theory, hence numerous results already obtained for Einstein-aether theory carry over.

  12. Einstein and Energy Efficiency: Making Homes Smarter (301)

    Broader source: Energy.gov [DOE]

    Better Buildings Residential Network Peer Exchange Call Series: Einstein and Energy Efficiency: Making Homes Smarter (301), call slides and discussion summary.

  13. Possible Demonstration of a Polaronic Bose-Einstein(-Mott) Condensate...

    Office of Scientific and Technical Information (OSTI)

    Demonstration of a Polaronic Bose-Einstein(-Mott) Condensate in UO2(+x) by Ultrafast THz Spectroscopy and Microwave Dissipation Citation Details In-Document Search Title: Possible ...

  14. Super- and sub-Einstein intrinsic viscosities of spherical nanoparticl...

    Office of Scientific and Technical Information (OSTI)

    Super- and sub-Einstein intrinsic viscosities of spherical nanoparticles in concentrated low molecular weight polymer solutions Citation Details In-Document Search Title: Super- ...

  15. JLab, Hampton U. celebrate Einstein's love of music with special...

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

    available from Jack Liebeck's website JLab, Hampton U. celebrate Einstein's love of music with special event at CNU's Ferguson Center for the Arts April 11, 2005 The Department...

  16. Controlling phase separation of binary Bose-Einstein condensates...

    Office of Scientific and Technical Information (OSTI)

    Controlling phase separation of binary Bose-Einstein condensates via mixed-spin-channel Feshbach resonance Citation Details In-Document Search Title: Controlling phase separation ...

  17. Einstein and the Daytime Sky - D

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

    D. Fun with polarizers In one respect, Einstein's mathematical analysis (like Rayleigh's earlier one) proves quite accurate, in a way that's easy to demonstrate. This has to do with how the sky's scattered light is polarized. Try looking at a patch of clear sky through one lens of a pair of polarizing sunglasses while you rotate the lens. You'll notice that the sky looks brighter as you look through the lens in some positions, and darker when the lens is in other positions. If the sun is not far

  18. Metric redefinitions in Einstein-Aether theory

    SciTech Connect (OSTI)

    Foster, Brendan Z.

    2005-08-15

    'Einstein-Aether' theory, in which gravity couples to a dynamical, timelike, unit-norm vector field, provides a means for studying Lorentz violation in a generally covariant setting. Demonstrated here is the effect of a redefinition of the metric and 'aether' fields in terms of the original fields and two free parameters. The net effect is a change of the coupling constants appearing in the action. Using such a redefinition, one of the coupling constants can be set to zero, simplifying studies of solutions of the theory.

  19. Newton to Einstein dust to dust

    SciTech Connect (OSTI)

    Kopp, Michael; Uhlemann, Cora; Haugg, Thomas E-mail: cora.uhlemann@physik.lmu.de

    2014-03-01

    We investigate the relation between the standard Newtonian equations for a pressureless fluid (dust) and the Einstein equations in a double expansion in small scales and small metric perturbations. We find that parts of the Einstein equations can be rewritten as a closed system of two coupled differential equations for the scalar and transverse vector metric perturbations in Poisson gauge. It is then shown that this system is equivalent to the Newtonian system of continuity and Euler equations. Brustein and Riotto (2011) conjectured the equivalence of these systems in the special case where vector perturbations were neglected. We show that this approach does not lead to the Euler equation but to a physically different one with large deviations already in the 1-loop power spectrum. We show that it is also possible to consistently set to zero the vector perturbations which strongly constrains the allowed initial conditions, in particular excluding Gaussian ones such that inclusion of vector perturbations is inevitable in the cosmological context. In addition we derive nonlinear equations for the gravitational slip and tensor perturbations, thereby extending Newtonian gravity of a dust fluid to account for nonlinear light propagation effects and dust-induced gravitational waves.

  20. Radiation damping in Einstein-aether theory

    SciTech Connect (OSTI)

    Foster, Brendan Z.

    2006-05-15

    This work concerns the loss of energy of a material system due to gravitational radiation in Einstein-aether theory - an alternative theory of gravity in which the metric couples to a dynamical, timelike, unit-norm vector field. Derived to lowest post-Newtonian order are wave forms for the metric and vector fields far from a nearly Newtonian system and the rate of energy radiated by the system. The expressions depend on the quadrupole moment of the source, as in standard general relativity, but also contain monopolar and dipolar terms. There exists a one-parameter family of Einstein-aether theories for which only the quadrupolar contribution is present, and for which the expression for the damping rate is identical to that of general relativity to the order worked to here. This family cannot yet be declared observationally viable, since effects due to the strong internal fields of bodies in the actual systems used to test the damping rate have not yet been determined.

  1. Nonlinear interferometry with Bose-Einstein condensates

    SciTech Connect (OSTI)

    Tacla, Alexandre B. [Center for Quantum Information and Control, MSC 07-4220, University of New Mexico, Albuquerque, New Mexico 87131-0001 (United States); Boixo, Sergio [Institute for Quantum Information, California Institute of Technology, Pasadena, California 91125 (United States); Datta, Animesh [Clarendon Laboratory, Department of Physics, University of Oxford, OX1 3PU (United Kingdom); Shaji, Anil [School of Physics, Indian Institute of Science Education and Research, College of Engineering Trivandrum Campus, Thiruvananthapuram, Kerala 695016 (India); Caves, Carlton M. [Center for Quantum Information and Control, MSC 07-4220, University of New Mexico, Albuquerque, New Mexico 87131-0001 (United States); School of Mathematics and Physics, University of Queensland, Brisbane, Queensland 4072 (Australia)

    2010-11-15

    We analyze a proposed experiment [Boixo et al., Phys. Rev. Lett. 101, 040403 (2008)] for achieving sensitivity scaling better than 1/N in a nonlinear Ramsey interferometer that uses a two-mode Bose-Einstein condensate (BEC) of N atoms. We present numerical simulations that confirm the analytical predictions for the effect of the spreading of the BEC ground-state wave function on the ideal 1/N{sup 3/2} scaling. Numerical integration of the coupled, time-dependent, two-mode Gross-Pitaevskii equations allows us to study the several simplifying assumptions made in the initial analytic study of the proposal and to explore when they can be justified. In particular, we find that the two modes share the same spatial wave function for a length of time that is sufficient to run the metrology scheme.

  2. Neutron stars in Einstein-aether theory

    SciTech Connect (OSTI)

    Eling, Christopher; Jacobson, Ted; Miller, M. Coleman

    2007-08-15

    As current and future experiments probe strong gravitational regimes around neutron stars and black holes, it is desirable to have theoretically sound alternatives to general relativity against which to test observations. Here we study the consequences of one such generalization, Einstein-aether theory, for the properties of nonrotating neutron stars. This theory has a parameter range that satisfies all current weak-field tests. We find that within this range it leads to lower maximum neutron star masses, as well as larger surface redshifts at a particular mass, for a given nuclear equation of state. For nonrotating black holes and neutron stars, the innermost stable circular orbit is only slightly modified in this theory.

  3. Energy in the Einstein-aether theory

    SciTech Connect (OSTI)

    Eling, Christopher

    2006-04-15

    We investigate the energy of a theory with a unit vector field (the aether) coupled to gravity. Both the Weinberg and Einstein type energy-momentum pseudotensors are employed. In the linearized theory we find expressions for the energy density of the 5 wave modes. The requirement that the modes have positive energy is then used to constrain the theory. In the fully nonlinear theory we compute the total energy of an asymptotically flat spacetime. The resulting energy expression is modified by the presence of the aether due to the nonzero value of the unit vector at infinity and its 1/r falloff. The question of nonlinear energy positivity is also discussed, but not resolved.

  4. 225px-Einstein_1921_portrait2.jpg | OSTI, US Dept of Energy Office of

    Office of Scientific and Technical Information (OSTI)

    Scientific and Technical Information 225px-Einstein_1921_portrait2

  5. Generalized Einstein-Aether theories and the Solar System

    SciTech Connect (OSTI)

    Bonvin, Camille; Durrer, Ruth; Ferreira, Pedro G.; Zlosnik, Tom G.; Starkman, Glenn

    2008-01-15

    It has been shown that generalized Einstein-Aether theories may lead to significant modifications to the nonrelativistic limit of the Einstein equations. In this paper we study the effect of a general class of such theories on the Solar System. We consider corrections to the gravitational potential in negative and positive powers of distance from the source. Using measurements of the perihelion shift of Mercury and time delay of radar signals to Cassini, we place constraints on these corrections. We find that a subclass of generalized Einstein-Aether theories is compatible with these constraints.

  6. Governor's Distinguished CEBAF Professorship Awarded to JLab Chief

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

    Scientist | Jefferson Lab Governor's Distinguished CEBAF Professorship Awarded to JLab Chief Scientist Governor's Distinguished CEBAF Professorship Awarded to JLab Chief Scientist May 2, 2005 Washington, D.C. - Five Virginia universities unanimously approved the nomination of Anthony W. Thomas, Chief Scientist at the U.S. Department of Energy's Thomas Jefferson National Accelerator Facility (Jefferson Lab) in Newport News, Va., to a distinguished professorship at The College of William and

  7. Tomé wins Distinguished Scientist, Engineer Award

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

    Engineer Award October 29, 2012 Carlos Tom of LANL's Materials Science in Radiation and Dynamics Extremes is the recipient of the 2013 Distinguished ScientistEngineer Award ...

  8. Sandia Energy - Two CRF Papers Named "Distinguished" for 34th...

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

    Two CRF Papers Named "Distinguished" for 34th International Symposium on Combustion Home Energy Transportation Energy CRF Facilities Partnership News News & Events Research &...

  9. Cristal Jones-Harris | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Cristal Jones-Harris Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Cristal Jones-Harris Print Text Size: A A A FeedbackShare Page Cristal Jones-Harris Fellowship Placement: National Aeronautics and Space Administration Hometown: Sandy Springs, GA Cristal Jones-Harris, Ed.

  10. Donna Volkmann | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Donna Volkmann Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Donna Volkmann Print Text Size: A A A FeedbackShare Page Donna Volkmann Fellowship Placement: U.S. Department of Energy Hometown: Centreville, VA Donna Volkmann is a high school science teacher from James Madison

  11. Doug Baltz | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Doug Baltz Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Doug Baltz Print Text Size: A A A FeedbackShare Page Doug Baltz Fellowship Placement: National Science Foundation Hometown: Royal Oak, MI Douglas Baltz has been an AP Physics and STEM teacher for over 20 years at

  12. Jessica Mulhern | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Jessica Mulhern Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Jessica Mulhern Print Text Size: A A A FeedbackShare Page Jessica Mulhern Fellowship Placement: U.S. House of Representatives Hometown: Wall, NJ Jessica Mulhern taught high school biology at Wilde Lake High

  13. Joanna Hubbard | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Joanna Hubbard Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Joanna Hubbard Print Text Size: A A A FeedbackShare Page Joanna Hubbard Fellowship Placement: U.S. House of Representatives Hometown: Anchorage, AK Joanna Hubbard has taught Integrated Science 8 as part of a

  14. Michael Stone | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Michael Stone Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Michael Stone Print Text Size: A A A FeedbackShare Page Michael Stone Fellowship Placement: National Science Foundation Hometown: East Ridge, TN Michael Stone has taught at several high schools in Chattanooga,

  15. Sally Mitchell | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Sally Mitchell Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Sally Mitchell Print Text Size: A A A FeedbackShare Page Sally Mitchell Fellowship Placement: U.S. Department of Energy Hometown: Syracuse, NY Sally Mitchell is a high school chemistry teacher from East Syracuse

  16. Susan Kennedy | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Susan Kennedy Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Susan Kennedy Print Text Size: A A A FeedbackShare Page Susan Kennedy Fellowship Placement: National Aeronautics and Space Administration Hometown: Wallace, NC Susan Kennedy is a 13-year veteran high school teacher

  17. Teresa Sappington | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Teresa Sappington Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Current Fellows Teresa Sappington Print Text Size: A A A FeedbackShare Page Teresa Sappington Fellowship Placement: U.S. House of Representatives Hometown: Hattiesburg, MS Teresa Sappington teaches high school engineering at

  18. Joshua Sneideman | Department of Energy

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

    Joshua Sneideman About Us Joshua Sneideman - Albert Einstein Distinguished Educator Fellow Joshua Sneideman Joshua Sneideman is a middle school science teacher with 10 years of teaching experience. Prior to his Einstein Fellowship, he taught at a private school in Irvine, California. Sneideman has taught mathematics and science for fifth, sixth, seventh, and eighth grades. In addition to his recent role as grade level coordinator, he enjoys coaching varsity tennis and basketball. Sneideman has

  19. Key Dates | U.S. DOE Office of Science (SC)

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

    Key Dates Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Contact WDTS Home Key Dates Print Text Size: A A A FeedbackShare Page Key Dates for the 2017-2018 AEF Program Application process. On-line Application Opens August 17, 2016 Application Deadline 8:00pm EST November 17, 2016 Application Review 8 - 9 weeks Notification to Semi-Finalists [Travel

  20. Application Review and Selection Process | U.S. DOE Office of Science (SC)

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

    Application Review and Selection Process Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Recommender Information Application Review and Selection Process Key Dates Frequently Asked Questions Fellows Central Contact WDTS Home How to Apply Application Review and Selection Process Print Text Size: A A A FeedbackShare Page Application Eligibility and Compliance: To be considered for this program, an applicant must

  1. Contact | U.S. DOE Office of Science (SC)

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

    Contact Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Contact WDTS Home Contact Print Text Size: A A A FeedbackShare Page Name Email Address * Subject * Type of Inquiry or Feedback Eligibility Application System Question Application Requirements Choosing a Host Agency Letters of Recommendation Other * Comments max. 1000 characters Captcha Display another

  2. Soliton Creation During a Bose-Einstein Condensation

    SciTech Connect (OSTI)

    Damski, Bogdan; Zurek, Wojciech H.

    2010-04-23

    We use the stochastic Gross-Pitaevskii equation to study dynamics of Bose-Einstein condensation. We show that cooling into a Bose-Einstein condensate (BEC) can create solitons with density given by the cooling rate and by the critical exponents of the transition. Thus, counting solitons left in its wake should allow one to determine the critical exponents z and {nu} for a BEC phase transition. The same information can be extracted from two-point correlation functions.

  3. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Frances Beinecke, Rafael Bras, Albert Carnesale, John

    Office of Environmental Management (EM)

    U.S. Department of Energy (DOE) Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Frances Beinecke, Rafael Bras, Albert Carnesale, John Deutch, Shirley Ann Jackson, Paul Joskow, Steve Koonin, Arun Majumdar, Michael McQuade, Richard Meserve, Dan Reicher, Dan Yergin Date and Time: 2:00 - 2:45 PM, August 18, 2014 Location: Conference Call Purpose: Meeting of the Secretary of Energy Advisory Board (SEAB) SEAB Staff: Karen Gibson, Designated Federal Officer

  4. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Persis Drell, Co-Chair; Frances Beinecke; Albert

    Office of Environmental Management (EM)

    Summary Minutes of the U.S. Department of Energy (DOE) Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Persis Drell, Co-Chair; Frances Beinecke; Albert Carnesale; Shirley Jackson; Deborah Jin; Paul Joskow; Steven Koonin; Michael McQuade; Richard Meserve; Cherry Murray; Carmichael Roberts; Ram Shenoy; Martha Schlicher; Daniel Yergin Date and Time: 9:00 AM- 12:00 NOON, March 28, 2014 Location: U.S. Department of Energy Forrestal Building, 1000

  5. Distinguished Student Awards Paul Asare Agyapong, NEN-3, UGS...

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

    Distinguished Student Awards Paul Asare Agyapong, NEN-3, UGS, Technical Ty Brooks, C-IIAC, UGS, Technical Amy Jordan, EES-16, GRA, Technical Heather Hughes, IRM-CAS, GRA, ...

  6. Distinguished Hampton University Professor Joins Jefferson Lab As

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

    Experimental Hall Leader | Jefferson Lab Distinguished Hampton University Professor Joins Jefferson Lab As Experimental Hall Leader Distinguished Hampton University Professor Joins Jefferson Lab As Experimental Hall Leader Cynthia Keppel Cynthia Keppel has been named Group Leader of Jefferson Lab's Experimental Hall A. Keppel will begin her duties on July 1. NEWPORT NEWS, VA, May 9, 2012 - Cynthia Keppel, a Hampton University experimental physicist and winner of the 2011 Virginia Outstanding

  7. Distinguished Student Awards Paul Asare Agyapong, NEN-3, UGS, Technical

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

    Distinguished Student Awards Paul Asare Agyapong, NEN-3, UGS, Technical Ty Brooks, C-IIAC, UGS, Technical Amy Jordan, EES-16, GRA, Technical Heather Hughes, IRM-CAS, GRA, Administrative Alison Tamasi, C-NR, GRA, Technical Andrea Vargas, ITPMO, GRA, Administrative Naomi Wasserman, EES-14, UGS, Technical Distinguished Mentor Awards Joysree Aubrey, IAT-DO Alina Deshpande, DSA-3 Andrew Nelson, MST-7 Robert Robey, XCP-2 Information Technology Cody Jackson, "Evaluating Cyber Security Policies

  8. Tomé wins Distinguished Scientist, Engineer Award

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

    Recipient of the 2013 Distinguished Scientist/Engineer Award Tomé wins Distinguished Scientist, Engineer Award The Minerals, Metals & Materials Society recognized Tomé for his "long lasting contribution to the fundamental understanding of microstructure, properties and performance of structural materials for industrial applications." October 29, 2012 Carlos Tomé Carlos Tomé Carlos Tomé of LANL's Materials Science in Radiation and Dynamics Extremes is the recipient of the 2013

  9. DOE Cyber Distinguished Speaker Series | Department of Energy

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

    DOE Cyber Distinguished Speaker Series DOE Cyber Distinguished Speaker Series Featured Speaker: Dr. Winfried K. Hensinger Date: August 5, 2016 Time: 11:00 am - 12:00 pm Location: DOE Headquarters, Forrestal Auditorium, Washington, DC Winfried K. Hensinger.jpg Dr. Winfried Hensinger - Professor of Quantum Technologies, Ion Quantum Technology Group, Department of Physics and Astronomy, University of Sussex Winfried Hensinger obtained his undergraduate degree at the Ruprechts-Karls University in

  10. Distinguished Professionals to Serve as Collegiate Wind Competition Judges

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

    | Department of Energy Distinguished Professionals to Serve as Collegiate Wind Competition Judges Distinguished Professionals to Serve as Collegiate Wind Competition Judges May 12, 2016 - 3:52pm Addthis U.S. Department of Energy Collegiate Wind Competition organizers have announced the judges for the 2016 competition, which will take place May 24-25 at the American Wind Energy Association (AWEA) WINDPOWER conference in New Orleans, Louisiana. "The competition relies on the expertise of

  11. Bose-Einstein condensates of polaritons: Vortices and superfluidity |

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

    MIT-Harvard Center for Excitonics Bose-Einstein condensates of polaritons: Vortices and superfluidity May 10, 2011 at 3:00PM/36-428 Benoit Deveaud-Plédran Ecole Polytechnique Fédérale de Lausanne abstract: The idea of a possible Bose Einstein condensation in the solid state has been explored since the beginning of the sixties with the hope to get transition temperatures much more accessible than the temperatures needed for the condensation of atomic vapors (less than 1µK for Rubidium).

  12. Secretary of Energy Advisory Board Public Meeting Committee Members: John Deutch, Co-Chair; Frances Beinecke, Rafael Bras, Albert Carnesale, Shirley

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

    Shirley Ann Jackson, Deborah Jin, Paul Joskow, Arun Majumdar, Michael McQuade, Richard Meserve, Cherry Murray, Carmichael Roberts, Martha Schlicher, Ram Shenoy, Dan Yergin Date and Time: 11:00 - 11:35 AM, August 1, 2014 Location: Conference Call Purpose: Meeting of the Secretary of Energy Advisory Board (SEAB) SEAB Staff: Corey Williams-Allen, Deputy Designated Federal Officer Meeting Summary John Deutch, SEAB co-chair, opened the meeting at 11:00AM and asked Albert Carnesale, Task Force Chair,

  13. What Is the Largest Einstein Radius in the Universe?

    SciTech Connect (OSTI)

    Oguri, Masamune; Blandford, Roger D.

    2008-08-05

    The Einstein radius plays a central role in lens studies as it characterizes the strength of gravitational lensing. In particular, the distribution of Einstein radii near the upper cutoff should probe the probability distribution of the largest mass concentrations in the universe. Adopting a triaxial halo model, we compute expected distributions of large Einstein radii. To assess the cosmic variance, we generate a number of Monte-Carlo realizations of all-sky catalogues of massive clusters. We find that the expected largest Einstein radius in the universe is sensitive to parameters characterizing the cosmological model, especially {sigma}{sub s}: for a source redshift of unity, they are 42{sub -7}{sup +9}, 35{sub -6}{sup +8}, and 54{sub -7}{sup +12} arcseconds (errors denote 1{sigma} cosmic variance), assuming best-fit cosmological parameters of the Wilkinson Microwave Anisotropy Probe five-year (WMAP5), three-year (WMAP3) and one-year (WMAP1) data, respectively. These values are broadly consistent with current observations given their incompleteness. The mass of the largest lens cluster can be as small as {approx} 10{sup 15} M{sub {circle_dot}}. For the same source redshift, we expect in all-sky {approx} 35 (WMAP5), {approx} 15 (WMAP3), and {approx} 150 (WMAP1) clusters that have Einstein radii larger than 2000. For a larger source redshift of 7, the largest Einstein radii grow approximately twice as large. While the values of the largest Einstein radii are almost unaffected by the level of the primordial non-Gaussianity currently of interest, the measurement of the abundance of moderately large lens clusters should probe non-Gaussianity competitively with cosmic microwave background experiments, but only if other cosmological parameters are well-measured. These semi-analytic predictions are based on a rather simple representation of clusters, and hence calibrating them with N-body simulations will help to improve the accuracy. We also find that these 'superlens

  14. Sandia's Carol Adkins Named University of New Mexico Distinguished Alumna

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

    Carol Adkins Named University of New Mexico Distinguished Alumna - Sandia Energy Energy Search Icon Sandia Home Locations Contact Us Employee Locator Energy & Climate Secure & Sustainable Energy Future Stationary Power Energy Conversion Efficiency Solar Energy Wind Energy Water Power Supercritical CO2 Geothermal Natural Gas Safety, Security & Resilience of the Energy Infrastructure Energy Storage Nuclear Power & Engineering Grid Modernization Battery Testing Nuclear Energy

  15. Lynden Archer > James A. Friend Family Distinguished Professor

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

    Chemical and Biomolecular Engineering > Faculty Directory > The Energy Materials Center at Cornell Lynden Archer James A. Friend Family Distinguished Professor Chemical and Biomolecular Engineering Research Group Webpage laa25@cornell.edu Professor Archer received the Career Award from the National Science Foundation, 1996, Dupont Young Professor Award 1996-1999, 3M Company Non-Tenured Faculty Award 1995, and the George Armistead Faculty Fellowship 1999-2000. Lynden joined the Cornell

  16. Scalar field as a Bose-Einstein condensate?

    SciTech Connect (OSTI)

    Castellanos, Elas; Escamilla-Rivera, Celia; Macas, Alfredo; Nez, Daro E-mail: cescamilla@mctp.mx E-mail: nunez@nucleares.unam.mx

    2014-11-01

    We discuss the analogy between a classical scalar field with a self-interacting potential, in a curved spacetime described by a quasi-bounded state, and a trapped Bose-Einstein condensate. In this context, we compare the Klein-Gordon equation with the Gross-Pitaevskii equation. Moreover, the introduction of a curved background spacetime endows, in a natural way, an equivalence to the Gross-Pitaevskii equation with an explicit confinement potential. The curvature also induces a position dependent self-interaction parameter. We exploit this analogy by means of the Thomas-Fermi approximation, commonly used to describe the Bose-Einstein condensate, in order to analyze the quasi bound scalar field distribution surrounding a black hole.

  17. Second post-Newtonian approximation of Einstein-aether theory

    SciTech Connect (OSTI)

    Xie Yi; Huang Tianyi

    2008-06-15

    In this paper, second post-Newtonian approximation of Einstein-aether theory is obtained by Chandrasekhar's approach. Five parametrized post-Newtonian parameters in first post-Newtonian approximation are presented after a time transformation and they are identical with previous works, in which {gamma}=1, {beta}=1, and two preferred-frame parameters remain. Meanwhile, in second post-Newtonian approximation, a parameter, which represents third order nonlinearity for gravity, is zero--the same as in general relativity. For an application for future deep space laser ranging missions, we reduce the metric coefficients for light propagation in a case of N point masses as a simplified model of the Solar System. The resulting light deflection angle in second post-Newtonian approximation poses another constraint on the Einstein-aether theory.

  18. Princeton physicists share in excitement of gravitational waves Einstein

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

    predicted | Princeton Plasma Physics Lab Princeton physicists share in excitement of gravitational waves Einstein predicted By Catherine Zandonella, Office of the Dean for Research February 12, 2016 Tweet Widget Google Plus One Share on Facebook The collision of two black holes - an event detected for the first time ever by the Laser Interferometer Gravitational-Wave Observatory, or LIGO - is seen in this still from a computer simulation. (Image by SXS) The collision of two black holes - an

  19. Controllable scattering of vector Bose-Einstein solitons

    SciTech Connect (OSTI)

    Babarro, Judit; Paz-Alonso, Maria J.; Michinel, Humberto; Salgueiro, Jose R.; Olivieri, David N.

    2005-04-01

    We show the possibility of producing matter-wave switching devices by using Manakov interactions between vector matter-wave solitons using two-species Bose-Einstein condensates (BECs). Our results establish the experimental parameters for three interaction regimes in two-species BECs: symmetric and asymmetric splitting, down-switching, and up-switching. We have studied the dependence upon the initial conditions and the kind of interaction between the two matter-wave solitons.

  20. Controlling chaos in the Bose-Einstein condensate

    SciTech Connect (OSTI)

    Cong Fuzhong Wang Zhixia; Hua Hongtu; Pang Shichun; Tong Shouyu

    2012-03-15

    The spatial structure of the Bose-Einstein condensate (BEC) is investigated and spatially chaotic distributions of the condensates are revealed. By means of changing the s-wave scattering length with a Feshbach resonance, the chaotic behavior can be well controlled to enter into periodicity. Numerical simulation shows that there are different periodic orbits according to different s-wave scattering lengths only if the Lyapunov exponent of the system is negative.

  1. PPPL researchers combine quantum mechanics and Einstein's theory of

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

    special relativity to clear up puzzles in plasma physics | Princeton Plasma Physics Lab researchers combine quantum mechanics and Einstein's theory of special relativity to clear up puzzles in plasma physics By John Greenwald July 29, 2016 Tweet Widget Google Plus One Share on Facebook Graduate student Yuan Shi (Photo by Elle Starkman/Office of Communications) Graduate student Yuan Shi Gallery: Sketch of a pulsar, center, in binary star system (Photo credit: NASA Goddard Space Flight Center)

  2. PPPL researchers combine quantum mechanics and Einstein's theory of

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

    special relativity to clear up puzzles in plasma physics | Princeton Plasma Physics Lab researchers combine quantum mechanics and Einstein's theory of special relativity to clear up puzzles in plasma physics By John Greenwald July 29, 2016 Tweet Widget Google Plus One Share on Facebook Graduate student Yuan Shi (Photo by Elle Starkman/Office of Communications) Graduate student Yuan Shi Gallery: Sketch of a pulsar, center, in binary star system (Photo credit: NASA Goddard Space Flight Center)

  3. Princeton physicists share in excitement of gravitational waves Einstein

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

    predicted | Princeton Plasma Physics Lab Princeton physicists share in excitement of gravitational waves Einstein predicted By Catherine andonella, Office of the Dean for Research February 12, 2016 Tweet Widget Google Plus One Share on Facebook The collision of two black holes - an event detected for the first time ever by the Laser Interferometer Gravitational-Wave Observatory, or LIGO - is seen in this still from a computer simulation. (Image by SXS) The collision of two black holes - an

  4. Are black holes in alternative theories serious astrophysical candidates? The case for Einstein-dilaton-Gauss-Bonnet black holes

    SciTech Connect (OSTI)

    Pani, Paolo; Cardoso, Vitor

    2009-04-15

    It is generally accepted that Einstein's theory will get some as yet unknown corrections, possibly large in the strong-field regime. An ideal place to look for these modifications is in the vicinities of compact objects such as black holes. Here, we study dilatonic black holes, which arise in the framework of Gauss-Bonnet couplings and one-loop corrected four-dimensional effective theory of heterotic superstrings at low energies. These are interesting objects as a prototype for alternative, yet well-behaved gravity theories: they evade the 'no-hair' theorem of general relativity but were proven to be stable against radial perturbations. We investigate the viability of these black holes as astrophysical objects and try to provide some means to distinguish them from black holes in general relativity. We start by extending previous works and establishing the stability of these black holes against axial perturbations. We then look for solutions of the field equations describing slowly rotating black holes and study geodesic motion around this geometry. Depending on the values of mass, dilaton charge, and angular momentum of the solution, one can have differences in the innermost-stable-circular-orbit location and orbital frequency, relative to black holes in general relativity. In the most favorable cases, the difference amounts to a few percent. Given the current state-of-the-art, we discuss the difficulty of distinguishing the correct theory of gravity from electromagnetic observations or even with gravitational-wave detectors.

  5. Soliton-soliton scattering in dipolar Bose-Einstein condensates

    SciTech Connect (OSTI)

    Nath, R.; Santos, L.; Pedri, P.

    2007-07-15

    We analyze the scattering of bright solitons in dipolar Bose-Einstein condensates placed in unconnected layers. Whereas for short-range interactions unconnected layers are independent, a remarkable consequence of the dipole interaction is the appearance of nonlocal interlayer effects. In particular, we show that both for one- and two-dimensional solitons the interlayer interaction leads to an effective molecular potential between disconnected solitons, which induces a complex scattering physics between them, that includes inelastic fusion into soliton molecules, and strong inelastic resonances. In addition, contrary to the short-range interacting case, a two-dimensional soliton scattering is possible, in which inelastic spiraling occurs, resembling phenomena in photorefractive materials.

  6. Spectroscopic Test of Bose-Einstein Statistics for Photons

    SciTech Connect (OSTI)

    English, D.; Yashchuk, V. V.; Budker, D.

    2010-06-25

    Using Bose-Einstein-statistics-forbidden two-photon excitation in atomic barium, we have limited the rate of statistics-violating transitions, as a fraction {nu} of an equivalent statistics-allowed transition rate, to {nu}<4.0x10{sup -11} at the 90% confidence level. This is an improvement of more than 3 orders of magnitude over the best previous result. Additionally, hyperfine-interaction enabling of the forbidden transition has been observed, to our knowledge, for the first time.

  7. Dynamics of vortex dipoles in anisotropic Bose-Einstein condensates

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Goodman, Roy H.; Kevrekidis, P. G.; Carretero-González, R.

    2015-04-14

    We study the motion of a vortex dipole in a Bose-Einstein condensate confined to an anisotropic trap. We focus on a system of ODEs describing the vortices' motion, which is in turn a reduced model of the Gross-Pitaevskii equation describing the condensate's motion. Using a sequence of canonical changes of variables, we reduce the dimension and simplify the equations of motion. In this study, we uncover two interesting regimes. Near a family of periodic orbits known as guiding centers, we find that the dynamics is essentially that of a pendulum coupled to a linear oscillator, leading to stochastic reversals inmore » the overall direction of rotation of the dipole. Near the separatrix orbit in the isotropic system, we find other families of periodic, quasi-periodic, and chaotic trajectories. In a neighborhood of the guiding center orbits, we derive an explicit iterated map that simplifies the problem further. Numerical calculations are used to illustrate the phenomena discovered through the analysis. Using the results from the reduced system, we are able to construct complex periodic orbits in the original, PDE, mean-field model for Bose-Einstein condensates, which corroborates the phenomenology observed in the reduced dynamical equations.« less

  8. Dynamics of vortex dipoles in anisotropic Bose-Einstein condensates

    SciTech Connect (OSTI)

    Goodman, Roy H.; Kevrekidis, P. G.; Carretero-González, R.

    2015-04-14

    We study the motion of a vortex dipole in a Bose-Einstein condensate confined to an anisotropic trap. We focus on a system of ODEs describing the vortices' motion, which is in turn a reduced model of the Gross-Pitaevskii equation describing the condensate's motion. Using a sequence of canonical changes of variables, we reduce the dimension and simplify the equations of motion. In this study, we uncover two interesting regimes. Near a family of periodic orbits known as guiding centers, we find that the dynamics is essentially that of a pendulum coupled to a linear oscillator, leading to stochastic reversals in the overall direction of rotation of the dipole. Near the separatrix orbit in the isotropic system, we find other families of periodic, quasi-periodic, and chaotic trajectories. In a neighborhood of the guiding center orbits, we derive an explicit iterated map that simplifies the problem further. Numerical calculations are used to illustrate the phenomena discovered through the analysis. Using the results from the reduced system, we are able to construct complex periodic orbits in the original, PDE, mean-field model for Bose-Einstein condensates, which corroborates the phenomenology observed in the reduced dynamical equations.

  9. Graduate & Postdoctoral Opportunities | Department of Energy

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

    & Professional Development » Graduate & Postdoctoral Opportunities Graduate & Postdoctoral Opportunities The U.S. Department of Energy (DOE) and various other organizations and institutions offer fellowship opportunities across the country-from Washington, D.C., to Dayton, Ohio, to Golden, Colorado, and beyond-for students and faculty alike. Download a copy of our flyer that highlights some of the Graduate experiences available. DOE-Sponsored Albert Einstein Distinguished Educator

  10. Energy Literacy

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

    gov Energy Literacy I want to talk about building a sustainable energy future.... The United States is committed to taking action to meet the energy and climate challenge. Secretary Chu, December 6, 2010 Presenter: Matthew Inman Albert Einstein Distinguished Educator Fellow US Department of Energy, EERE-EEWD matthew.inman@ee.doe.gov 2 | Energy Education and Workforce Development eere.energy.gov Energy Literacy Energy Literacy Promote Energy Literacy The Department will actively participate in

  11. WDTS Budget | U.S. DOE Office of Science (SC)

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

    Budget Workforce Development for Teachers and Scientists (WDTS) WDTS Home About Organization Chart .pdf file (24KB) WDTS Budget WDTS Committees of Visitors Jobs Science Undergraduate Laboratory Internships (SULI) Community College Internships (CCI) Visiting Faculty Program (VFP) at DOE Laboratories DOE Office of Science Graduate Student Research (SCGSR) Program Albert Einstein Distinguished Educator Fellowship (AEF) Program DOE National Science Bowl® (NSB) STEM Resources Outreach Contact

  12. WDTS Committees of Visitors | U.S. DOE Office of Science (SC)

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

    Committees of Visitors Workforce Development for Teachers and Scientists (WDTS) WDTS Home About Organization Chart .pdf file (24KB) WDTS Budget WDTS Committees of Visitors Jobs Science Undergraduate Laboratory Internships (SULI) Community College Internships (CCI) Visiting Faculty Program (VFP) at DOE Laboratories DOE Office of Science Graduate Student Research (SCGSR) Program Albert Einstein Distinguished Educator Fellowship (AEF) Program DOE National Science Bowl® (NSB) STEM Resources

  13. EERE Internships and Fellowships | Department of Energy

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

    Internships and Fellowships EERE Internships and Fellowships There are plenty of opportunities for students, recent graduates, and others looking for internships, fellowships, and similar programs with the Office of Energy Efficiency and Renewable Energy (EERE) and U.S. Department of Energy (DOE). EERE's Student Volunteer Internship Program EERE offers exciting student volunteer internships throughout the year in its Washington, D.C., headquarters. Albert Einstein Distinguished Educator Program

  14. Upholding Dr. King's Dream and Inspiring the Next Generation Through STEM

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

    Education | Department of Energy Upholding Dr. King's Dream and Inspiring the Next Generation Through STEM Education Upholding Dr. King's Dream and Inspiring the Next Generation Through STEM Education January 27, 2015 - 12:56pm Addthis Upholding Dr. King’s Dream and Inspiring the Next Generation Through STEM Education Joshua Sneideman Joshua Sneideman Albert Einstein Distinguished Educator Fellow According to the Reverend Dr. Martin Luther King, Jr., "The function of education is

  15. 5 Energy Education Ideas to Spark Learning Beyond the Classroom |

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

    Department of Energy Energy Education Ideas to Spark Learning Beyond the Classroom 5 Energy Education Ideas to Spark Learning Beyond the Classroom August 4, 2015 - 12:01pm Addthis 5 Energy Education Ideas to Spark Learning Beyond the Classroom Joshua Sneideman Joshua Sneideman Albert Einstein Distinguished Educator Fellow Did you know energy is everywhere? Think about it: energy is clearly a physics concept, but is that all it is? Like turning off the lights when you leave home, our everyday

  16. Jobs | U.S. DOE Office of Science (SC)

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

    Jobs Workforce Development for Teachers and Scientists (WDTS) WDTS Home About Organization Chart .pdf file (24KB) WDTS Budget WDTS Committees of Visitors Jobs Science Undergraduate Laboratory Internships (SULI) Community College Internships (CCI) Visiting Faculty Program (VFP) at DOE Laboratories DOE Office of Science Graduate Student Research (SCGSR) Program Albert Einstein Distinguished Educator Fellowship (AEF) Program DOE National Science Bowl® (NSB) STEM Resources Outreach Contact

  17. K-12 Educators | U.S. DOE Office of Science (SC)

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

    STEM Resources » K-12 Educators Workforce Development for Teachers and Scientists (WDTS) WDTS Home About Science Undergraduate Laboratory Internships (SULI) Community College Internships (CCI) Visiting Faculty Program (VFP) at DOE Laboratories DOE Office of Science Graduate Student Research (SCGSR) Program Albert Einstein Distinguished Educator Fellowship (AEF) Program DOE National Science Bowl® (NSB) STEM Resources Undergraduate and Graduate Students K-12 Educators Outreach Contact

  18. Workforce Development for Teachers and Scientists (WDTS) Homepage | U.S.

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

    DOE Office of Science (SC) Programs » WDTS Home Workforce Development for Teachers and Scientists (WDTS) WDTS Home About Science Undergraduate Laboratory Internships (SULI) Community College Internships (CCI) Visiting Faculty Program (VFP) at DOE Laboratories DOE Office of Science Graduate Student Research (SCGSR) Program Albert Einstein Distinguished Educator Fellowship (AEF) Program DOE National Science Bowl® (NSB) STEM Resources Outreach Contact Information Workforce Development for

  19. Exact solutions with AdS asymptotics of Einstein and Einstein-Maxwell gravity minimally coupled to a scalar field

    SciTech Connect (OSTI)

    Cadoni, Mariano; Serra, Matteo; Mignemi, Salvatore

    2011-10-15

    We propose a general method for solving exactly the static field equations of Einstein and Einstein-Maxwell gravity minimally coupled to a scalar field. Our method starts from an ansatz for the scalar field profile, and determines, together with the metric functions, the corresponding form of the scalar self-interaction potential. Using this method we prove a new no-hair theorem about the existence of hairy black-hole and black-brane solutions and derive broad classes of static solutions with radial symmetry of the theory, which may play an important role in applications of the AdS/CFT correspondence to condensed matter and strongly coupled QFTs. These solutions include: (1) four- or generic (d+2)-dimensional solutions with planar, spherical or hyperbolic horizon topology; (2) solutions with anti-de Sitter, domain wall and Lifshitz asymptotics; (3) solutions interpolating between an anti-de Sitter spacetime in the asymptotic region and a domain wall or conformal Lifshitz spacetime in the near-horizon region.

  20. Method for distinguishing multiple targets using time-reversal acoustics

    DOE Patents [OSTI]

    Berryman, James G.

    2004-06-29

    A method for distinguishing multiple targets using time-reversal acoustics. Time-reversal acoustics uses an iterative process to determine the optimum signal for locating a strongly reflecting target in a cluttered environment. An acoustic array sends a signal into a medium, and then receives the returned/reflected signal. This returned/reflected signal is then time-reversed and sent back into the medium again, and again, until the signal being sent and received is no longer changing. At that point, the array has isolated the largest eigenvalue/eigenvector combination and has effectively determined the location of a single target in the medium (the one that is most strongly reflecting). After the largest eigenvalue/eigenvector combination has been determined, to determine the location of other targets, instead of sending back the same signals, the method sends back these time reversed signals, but half of them will also be reversed in sign. There are various possibilities for choosing which half to do sign reversal. The most obvious choice is to reverse every other one in a linear array, or as in a checkerboard pattern in 2D. Then, a new send/receive, send-time reversed/receive iteration can proceed. Often, the first iteration in this sequence will be close to the desired signal from a second target. In some cases, orthogonalization procedures must be implemented to assure the returned signals are in fact orthogonal to the first eigenvector found.

  1. Bose-Einstein condensation in liquid 4He under pressure

    SciTech Connect (OSTI)

    Glyde, Henry R; Omar Diallo, Souleymane; Azuah, Richard T; Kirichek, Oleg; Taylor, Jon W.

    2011-01-01

    We present neutron scattering measurements of Bose-Einstein condensation, the atomic momen- tum distribution and Final State effects in liquid 4He under pressure. The condensate fraction at low temperature is found to decrease from n0 = 7.25 0.75% at SVP (p 0) to n0 = 3.2 0.75% at pressure p = 24 bar. This indicates an n0 = 3.0% in the liquid at the liquid/solid co-existence line (p = 25.3 bar). The atomic momentum distribution n(k) has high occupation of low k states and differs significantly from a Gaussian (e.g. a classical n(k)). Both n(k) and the Final state function broaden with increasing pressure, reflecting the increased localization of the 4He in space under increased pressure.

  2. Eternal inflation and a thermodynamic treatment of Einstein's equations

    SciTech Connect (OSTI)

    Ghersi, José Tomás Gálvez; Geshnizjani, Ghazal; Shandera, Sarah; Piazza, Federico E-mail: ggeshnizjani@perimeterinstitute.ca E-mail: sshandera@perimeterinstitute.ca

    2011-06-01

    In pursuing the intriguing resemblance of the Einstein equations to thermodynamic equations, most sharply seen in systems possessing horizons, we suggest that eternal inflation of the stochastic type may be a fruitful phenomenon to explore. We develop a thermodynamic first law for quasi-de Sitter space, valid on the horizon of a single observer's Hubble patch and explore consistancy with previous proposals for horizons of various types in dynamic and static situations. We use this framework to demonstrate that for the local observer fluctuations of the type necessary for stochastic eternal inflation fall within the regime where the thermodynamic approach is believed to apply. This scenario is interesting because of suggestive parallels with black hole evaporation.

  3. Internal Josephson oscillations for distinct momenta Bose-Einstein condensates

    SciTech Connect (OSTI)

    Lim, Lih-King [Institute for Theoretical Physics, Utrecht University, Leuvenlaan 4, 3584 CE Utrecht (Netherlands); Laboratoire de Physique des Solides, CNRS UMR 8502, Universite Paris-Sud, F-91405 Orsay Cedex (France); Troppenz, T.; Morais Smith, C. [Institute for Theoretical Physics, Utrecht University, Leuvenlaan 4, 3584 CE Utrecht (Netherlands)

    2011-11-15

    The internal Josephson oscillations between an atomic Bose-Einstein condensate (BEC) and a molecular one are studied for atoms in a square optical lattice subjected to a staggered gauge field. The system is described by a Bose-Hubbard model with complex and anisotropic hopping parameters that are different for each species, i.e., atoms and molecules. When the flux per plaquette for each species is small, the system oscillates between two conventional zero-momentum condensates. However, there is a regime of parameters in which Josephson oscillations between a vortex-carrying atomic condensate (finite momentum BEC) and a conventional zero-momentum molecular condensate may be realized. The experimental observation of the oscillations between these qualitatively distinct BEC's is possible with state-of-the-art Ramsey interference techniques.

  4. Josephson effects in a Bose–Einstein condensate of magnons

    SciTech Connect (OSTI)

    Troncoso, Roberto E.; Núñez, Álvaro S.

    2014-07-15

    A phenomenological theory is developed, that accounts for the collective dynamics of a Bose–Einstein condensate of magnons. In terms of such description we discuss the nature of spontaneous macroscopic interference between magnon clouds, highlighting the close relation between such effects and the well known Josephson effects. Using those ideas, we present a detailed calculation of the Josephson oscillations between two magnon clouds, spatially separated in a magnonic Josephson junction. -- Highlights: •We presented a theory that accounts for the collective dynamics of a magnon-BEC. •We discuss the nature of macroscopic interference between magnon-BEC clouds. •We remarked the close relation between the above phenomena and Josephson’s effect. •We remark the distinctive oscillations that characterize the Josephson oscillations.

  5. Atomic quantum corrals for Bose-Einstein condensates

    SciTech Connect (OSTI)

    Xiong Hongwei [State Key Laboratory of Magnetic Resonance and Atomic and Molecular Physics, Wuhan Institute of Physics and Mathematics, Chinese Academy of Sciences, Wuhan 430071 (China); Kavli Institute for Theoretical Physics China, Chinese Academy of Sciences, Beijing 100190 (China); Wu Biao [Kavli Institute for Theoretical Physics China, Chinese Academy of Sciences, Beijing 100190 (China); International Center for Quantum Materials, Peking University, Beijing 100871 (China); Institute of Physics, Chinese Academy of Sciences, Beijing 100190 (China)

    2010-11-15

    We consider the dynamics of Bose-Einstein condensates in a corral-like potential. Compared to the electronic quantum corrals, the atomic quantum corrals have the advantages of allowing direct and convenient observation of the wave dynamics, together with adjustable interaction strength. Our numerical study shows that these advantages not only allow exploration of the rich dynamical structures in the density distribution but also make the corrals useful in many other aspects. In particular, the corrals for atoms can be arranged into a stadium shape for the experimental visualization of quantum chaos, which has been elusive with electronic quantum corrals. The density correlation is used to describe quantitatively the dynamical quantum chaos. Furthermore, we find that the interatomic interaction can greatly enhance the dynamical quantum chaos, for example, inducing a chaotic behavior even in circle-shaped corrals.

  6. Stabilization of ring dark solitons in Bose-Einstein condensates

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Wang, Wenlong; Kevrekidis, P. G.; Carretero-González, R.; Frantzeskakis, D. J.; Kaper, Tasso J.; Ma, Manjun

    2015-09-14

    Earlier work has shown that ring dark solitons in two-dimensional Bose-Einstein condensates are generically unstable. In this work, we propose a way of stabilizing the ring dark soliton via a radial Gaussian external potential. We investigate the existence and stability of the ring dark soliton upon variations of the chemical potential and also of the strength of the radial potential. Numerical results show that the ring dark soliton can be stabilized in a suitable interval of external potential strengths and chemical potentials. Furthermore, we also explore different proposed particle pictures considering the ring as a moving particle and find, wheremore » appropriate, results in very good qualitative and also reasonable quantitative agreement with the numerical findings.« less

  7. Stabilization of ring dark solitons in Bose-Einstein condensates

    SciTech Connect (OSTI)

    Wang, Wenlong; Kevrekidis, P. G.; Carretero-González, R.; Frantzeskakis, D. J.; Kaper, Tasso J.; Ma, Manjun

    2015-09-14

    Earlier work has shown that ring dark solitons in two-dimensional Bose-Einstein condensates are generically unstable. In this work, we propose a way of stabilizing the ring dark soliton via a radial Gaussian external potential. We investigate the existence and stability of the ring dark soliton upon variations of the chemical potential and also of the strength of the radial potential. Numerical results show that the ring dark soliton can be stabilized in a suitable interval of external potential strengths and chemical potentials. Furthermore, we also explore different proposed particle pictures considering the ring as a moving particle and find, where appropriate, results in very good qualitative and also reasonable quantitative agreement with the numerical findings.

  8. B-mode polarization in Einstein-aether theory

    SciTech Connect (OSTI)

    Nakashima, Masahiro; Kobayashi, Tsutomu

    2011-10-15

    We study how the dynamical vector degree of freedom in modified gravity affects the CMB B-mode polarization in terms of the Einstein-aether theory. In this theory, vector perturbations can be generated from inflation, which can grow on superhorizon scales in the subsequent epochs and thereby leaves imprints on the CMB B-mode polarization. We derive the linear perturbation equations in a covariant formalism, and compute the CMB B-mode polarization using the CAMB code modified so as to incorporate the effect of the aether vector field. We find that the amplitude of the B-mode signal from the aether field can be larger than the contribution from the inflationary gravitational waves for reasonable initial conditions and for a viable range of model parameters, in which perturbation modes propagate superluminally. We also give an analytic argument explaining the shape of the spectrum based on the tight coupling approximation.

  9. Generic features of Einstein-Aether black holes

    SciTech Connect (OSTI)

    Tamaki, Takashi; Miyamoto, Umpei

    2008-01-15

    We reconsider spherically symmetric black hole solutions in Einstein-Aether theory with the condition that this theory has identical parametrized post-Newtonian parameters as those for general relativity, which is the main difference from the previous research. In contrast with previous study, we allow superluminal propagation of a spin-0 Aether-gravity wave mode. As a result, we obtain black holes having a spin-0 'horizon' inside an event horizon. We allow a singularity at a spin-0 horizon since it is concealed by the event horizon. If we allow such a configuration, the kinetic term of the Aether field can be large enough for black holes to be significantly different from Schwarzschild black holes with respect to Arnowitt-Deser-Misner mass, innermost stable circular orbit, Hawking temperature, and so on. We also discuss whether or not the above features can be seen in more generic vector-tensor theories.

  10. Rapidity Dependence of Bose-Einstein Correlations at SPS energies

    SciTech Connect (OSTI)

    Kniege, Stefan

    2006-04-11

    This article is devoted to results on {pi}-{pi}--Bose-Einstein correlations in central Pb+Pb collisions measured by the NA49 experiment at the CERN SPS. Rapidity as well as transverse momentum dependences of the correlation lengths will be shown for collisions at 20A, 30A, 40A, 80A, and 158A GeV beam energy. Only a weak energy dependence of the radii is observed at SPS energies. The kt-dependence of the correlation lengths as well as the single particle mt-spectra will be compared to model calculations. The rapidity dependence is analysed in a range of 2.5 units of rapidity starting at the center of mass rapidity at each beam energy. The correlation lengths measured in the longitudinally comoving system show only a weak dependence on rapidity.

  11. Stability of the Einstein static universe in the presence of vacuum energy

    SciTech Connect (OSTI)

    Carneiro, Saulo; Tavakol, Reza

    2009-08-15

    The Einstein static universe has played a central role in a number of emergent scenarios recently put forward to deal with the singular origin of the standard cosmological model. Here we study the existence and stability of the Einstein static solution in the presence of vacuum energy corresponding to conformally invariant fields. We show that the presence of vacuum energy stabilizes this solution by changing it to a center equilibrium point, which is cyclically stable. This allows nonsingular emergent cosmological models to be constructed in which initially the Universe oscillates indefinitely about an initial Einstein static solution and is thus past eternal.

  12. Alumni Fellows | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Alumni Fellows Albert Einstein Distinguished Educator Fellowship (AEF) Program Einstein Fellowship Home Eligibility Benefits Obligations How to Apply Key Dates Frequently Asked Questions Fellows Central Current Fellows Alumni Fellows Official AEF Logos Contact WDTS Home Fellows Central Alumni Fellows Print Text Size: A A A FeedbackShare Page 2015-2016 | 2014-2015 | 2013-2014 | 2012-2013 | 2011-2012 | 2010-2011 | 2009-2010 | 2008-2009 | 2007-2008 | 2006-2007 | 2005-2006 | 2004-2005 | 2003-2004 |

  13. JLab, Hampton U. celebrate Einstein's love of music with special event at

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

    CNU's Ferguson Center for the Arts | Jefferson Lab JLab, Hampton U. celebrate Einstein's love of music with special event at CNU's Ferguson Center for the Arts Dr. Brian Foster and Jack Liebeck Dr. Brian Foster and Jack Liebeck. Photo by Richard Lea-Hair. More publicity photographs available from Jack Liebeck's website JLab, Hampton U. celebrate Einstein's love of music with special event at CNU's Ferguson Center for the Arts April 11, 2005 The Department of Energy's Jefferson Lab, in

  14. Einstein-aether theory with a Maxwell field: General formalism

    SciTech Connect (OSTI)

    Balakin, Alexander B.; Lemos, José P.S.

    2014-11-15

    We extend the Einstein-aether theory to include the Maxwell field in a nontrivial manner by taking into account its interaction with the time-like unit vector field characterizing the aether. We also include a generic matter term. We present a model with a Lagrangian that includes cross-terms linear and quadratic in the Maxwell tensor, linear and quadratic in the covariant derivative of the aether velocity four-vector, linear in its second covariant derivative and in the Riemann tensor. We decompose these terms with respect to the irreducible parts of the covariant derivative of the aether velocity, namely, the acceleration four-vector, the shear and vorticity tensors, and the expansion scalar. Furthermore, we discuss the influence of an aether non-uniform motion on the polarization and magnetization of the matter in such an aether environment, as well as on its dielectric and magnetic properties. The total self-consistent system of equations for the electromagnetic and the gravitational fields, and the dynamic equations for the unit vector aether field are obtained. Possible applications of this system are discussed. Based on the principles of effective field theories, we display in an appendix all the terms up to fourth order in derivative operators that can be considered in a Lagrangian that includes the metric, the electromagnetic and the aether fields.

  15. Primordial perturbations in Einstein-Aether and BPSH theories

    SciTech Connect (OSTI)

    Armendariz-Picon, Cristian; Sierra, Noela Fariña; Garriga, Jaume E-mail: noela@ffn.ub.es

    2010-07-01

    We study the primordial perturbations generated during a stage of single-field inflation in Einstein-aether theories. Quantum fluctuations of the inflaton and aether fields seed long wavelength adiabatic and isocurvature scalar perturbations, as well as transverse vector perturbations. Geometrically, the isocurvature mode is the potential for the velocity field of the aether with respect to matter. For a certain range of parameters, this mode may lead to a sizable random velocity of the aether within the observable universe. The adiabatic mode corresponds to curvature perturbations of co-moving slices (where matter is at rest). In contrast with the standard case, it has a non-vanishing anisotropic stress on large scales. Scalar and vector perturbations may leave significant imprints on the cosmic microwave background. We calculate their primordial spectra, analyze their contributions to the temperature anisotropies, and formulate some of the phenomenological constraints that follow from observations. These may be used to further tighten the existing limits on the parameters for this class of theories. The results for the scalar sector also apply to the extension of Hořava gravity recently proposed by Blas, Pujolàs and Sibiryakov.

  16. Atomic interactions in precision interferometry using Bose-Einstein condensates

    SciTech Connect (OSTI)

    Jamison, Alan O.; Gupta, Subhadeep; Kutz, J. Nathan

    2011-10-15

    We present theoretical tools for predicting and reducing the effects of atomic interactions in Bose-Einstein condensate (BEC) interferometry experiments. To address mean-field shifts during free propagation, we derive a robust scaling solution that reduces the three-dimensional Gross-Pitaevskii equation to a set of three simple differential equations valid for any interaction strength. To model the other common components of a BEC interferometer--condensate splitting, manipulation, and recombination--we generalize the slowly varying envelope reduction, providing both analytic handles and dramatically improved simulations. Applying these tools to a BEC interferometer to measure the fine structure constant, {alpha}[S. Gupta, K. Dieckmann, Z. Hadzibabic, and D. E. Pritchard, Phys. Rev. Lett. 89, 140401 (2002)], we find agreement with the results of the original experiment and demonstrate that atomic interactions do not preclude measurement to better than part-per-billion accuracy, even for atomic species with relatively large scattering lengths. These tools help make BEC interferometry a viable choice for a broad class of precision measurements.

  17. EINSTEIN'S SIGNATURE IN COSMOLOGICAL LARGE-SCALE STRUCTURE

    SciTech Connect (OSTI)

    Bruni, Marco; Hidalgo, Juan Carlos; Wands, David

    2014-10-10

    We show how the nonlinearity of general relativity generates a characteristic nonGaussian signal in cosmological large-scale structure that we calculate at all perturbative orders in a large-scale limit. Newtonian gravity and general relativity provide complementary theoretical frameworks for modeling large-scale structure in ?CDM cosmology; a relativistic approach is essential to determine initial conditions, which can then be used in Newtonian simulations studying the nonlinear evolution of the matter density. Most inflationary models in the very early universe predict an almost Gaussian distribution for the primordial metric perturbation, ?. However, we argue that it is the Ricci curvature of comoving-orthogonal spatial hypersurfaces, R, that drives structure formation at large scales. We show how the nonlinear relation between the spatial curvature, R, and the metric perturbation, ?, translates into a specific nonGaussian contribution to the initial comoving matter density that we calculate for the simple case of an initially Gaussian ?. Our analysis shows the nonlinear signature of Einstein's gravity in large-scale structure.

  18. Timeline of Events: 1938-1950 | Department of Energy

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

    38-1950 Timeline of Events: 1938-1950 August 2, 1939: Albert Einstein's Letter August 2, 1939: Albert Einstein's Letter With the help of Leo Szilard, Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions and the possibility that research might lead to developing powerful bombs. Read more July 16, 1945: Trinity July 16, 1945: Trinity Los Alamos scientists successfully test a plutonium implosion bomb. Read more

  19. Timeline__09_19_2013

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

    38-1950 Timeline of Events: 1938-1950 August 2, 1939: Albert Einstein's Letter August 2, 1939: Albert Einstein's Letter With the help of Leo Szilard, Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions and the possibility that research might lead to developing powerful bombs. Read more July 16, 1945: Trinity July 16, 1945: Trinity Los Alamos scientists successfully test a plutonium implosion bomb. Read more

  20. Observation of Fractional Stokes-Einstein Behavior in the Simplest Hydrogen-bonded Liquid

    SciTech Connect (OSTI)

    Herwig, Kenneth W; Molaison, Jamie J; Fernandez-Alonso, F.; Bermejo, F. J.; Turner, John F. C.; McLain, Sylvia E.

    2007-01-01

    Quasielastic neutron scattering has been used to investigate the single-particle dynamics of hydrogen fluoride across its entire liquid range at ambient pressure. For T > 230 K, translational diffusion obeys the celebrated Stokes-Einstein relation, in agreement with nuclear magnetic resonance studies. At lower temperatures, we find significant deviations from the above behavior in the form of a power law with exponent xi = -0.71+/-0.05. More striking than the above is a complete breakdown of the Debye-Stokes-Einstein relation for rotational diffusion. Our findings provide the first experimental verification of fractional Stokes-Einstein behavior in a hydrogen-bonded liquid, in agreement with recent computer simulations.

  1. Noether charges and black hole mechanics in Einstein-aether theory

    SciTech Connect (OSTI)

    Foster, Brendan Z.

    2006-01-15

    The Noether charge method for defining the Hamiltonian of a diffeomorphism-invariant field theory is applied to 'Einstein-aether' theory, in which gravity couples to a dynamical, timelike, unit-norm vector field. Using the method, expressions are obtained for the total energy, momentum, and angular momentum of an Einstein-aether space-time. The method is also used to discuss the mechanics of Einstein-aether black holes. The derivation of Wald, and Iyer and Wald, of the first law of black hole thermodynamics fails for this theory because the unit-vector is necessarily singular at the bifurcation surface of the Killing horizon. A general identity relating variations of energy and angular momentum to a surface integral at the horizon is obtained, but a thermodynamic interpretation, including a definitive expression for the black hole entropy, is not found.

  2. Generalized Bose-Einstein condensation in superconductivity and superfluidity

    SciTech Connect (OSTI)

    Llano, M. de

    2008-03-20

    Unification of the Bardeen, Cooper and Schrieffer (BCS) and the Bose-Einstein condensation (BEC) theories is surveyed in terms of a generalized BEC (GBEC) finite-temperature statistical formalism. A vital distinction is that Cooper pairs (CPs) are true bosons that may suffer a BEC since they obey BE statistics, in contrast with BCS pairs that are 'hard-core bosons' at best. A second crucial ingredient is the explicit presence of hole-pairs (2h) alongside the usual electron-pairs (2e). A third critical element (particularly in 2D where ordinary BEC does not occur) is the linear dispersion relation of CPs in leading order in the center-of-mass momentum (CMM) power-series expansion of the CP energy. The GBEC theory reduces in limiting cases to all five continuum (as opposed to 'spin') statistical theories of superconductivity, from BCS on one extreme to the BEC theory on the other, as well as to the BCS-Bose 'crossover' picture and the 1989 Friedberg-Lee BEC theory. It accounts for 2e- and 2h-CPs in arbitrary proportions while BCS theory can be deduced from the GBEC theory but allows only equal (50%-50%) BE condensed-mixtures of both kinds of CPs. As it yields the precise BCS gap equation for all temperatures as well as the precise BCS zero-temperature condensation energy for all couplings, it suggests that the BCS condensate is a BE condensate of a ternary mixture of kinematically independent unpaired electrons coexisting with equally proportioned weakly-bound zero-CMM 2e- and 2h-CPs. Without abandoning the electron-phonon mechanism in moderately weak coupling, and fortuituously insensitive to the BF interactions, the GBEC theory suffices to reproduce the unusually high values of T{sub c} (in units of the Fermi temperature T{sub F}) of 0.01-0.05 empirically found in the so-called 'exotic' superconductors of the Uemura plot, including cuprates, in contrast to the low values of T{sub c}/T{sub F}{<=}10{sup -3} roughly reproduced by BCS theory for conventional (mostly

  3. Quasispherical gravitational collapse in 5D Einstein-Gauss-Bonnet gravity

    SciTech Connect (OSTI)

    Ghosh, Sushant G.; Jhingan, S.

    2010-07-15

    We obtain a general five-dimensional quasispherical collapsing solutions of irrotational dust in Einstein gravity with the Gauss-Bonnet combination of quadratic curvature terms. These solutions are a generalization, to Einstein-Gauss-Bonnet gravity, of the five-dimensional quasispherical Szkeres like collapsing solutions in general relativity. It is found that the collapse proceeds in the same way as in the analogous spherical collapse, i.e., there exists regular initial data such that the collapse proceed to form naked singularities violating cosmic censorship conjecture. The effect of Gauss-Bonnet quadratic curvature terms on the formation and locations of the apparent horizon is deduced.

  4. Dark soliton interaction of spinor Bose-Einstein condensates in an optical lattice

    SciTech Connect (OSTI)

    Li Zaidong; Li Qiuyan . E-mail: lqy32@yahoo.com.cn

    2007-08-15

    We study the magnetic soliton dynamics of spinor Bose-Einstein condensates in an optical lattice which results in an effective Hamiltonian of anisotropic pseudospin chain. An equation of nonlinear Schroedinger type is derived and exact magnetic soliton solutions are obtained analytically by means of Hirota method. Our results show that the critical external field is needed for creating the magnetic soliton in spinor Bose-Einstein condensates. The soliton size, velocity and shape frequency can be controlled in practical experiment by adjusting the magnetic field. Moreover, the elastic collision of two solitons is investigated in detail.

  5. Browse by Discipline -- E-print Network Subject Pathways: --...

    Office of Scientific and Technical Information (OSTI)

    ... Biology, Albert Einstein College of Medicine, Yeshiva University Snell-Rood, Emilie C. (Emilie C. Snell-Rood) - Department of Ecology, Evolution, and Behavior, University of ...

  6. X-ray emission spectroscopy of bulk liquid water in "no-man's...

    Office of Scientific and Technical Information (OSTI)

    Radiation Research, Helmholtz-Zentrum Berlin fr Materialien und Energie GmbH, Albert-Einstein-Strae 15, 12489 Berlin, Germany, Institut fr Physik und Astronomie,...

  7. OSTI, US Dept of Energy, Office of Scientific and Technical Informatio...

    Office of Scientific and Technical Information (OSTI)

    Science Communications "Pure mathematics is, in its way, the poetry of logical ideas." Albert Einstein As you prepare your taxes, keep in mind that April is Mathematics...

  8. Russell Hulse, the First Binary Pulsar, and Science Education

    Office of Scientific and Technical Information (OSTI)

    pulsar - a twin star system that provides a rare natural laboratory in which to test Albert Einstein's prediction that moving objects emit gravitational waves, as well as other...

  9. Julian Schwinger and the Source Theory

    Office of Scientific and Technical Information (OSTI)

    he was awarded the academy's Nature of Light Prize. In 1951, Schwinger shared the first Albert Einstein Prize with mathematician Kurt Godel. The same year he received the...

  10. Converting Energy to Medical Progress

    Office of Scientific and Technical Information (OSTI)

    New York Robert M. Sharkey, Garden State Cancer Center, New Jersey Robert H. Singer, Albert Einstein College of Medicine, New York Suresh C. Srivastava, Brookhaven National...

  11. Secretary Chu's Remarks at the World Renewable Energy Forum Press...

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

    energy coupled with digital communication, management and manufacturing. A century ago, Albert Einstein showed the world that the mass of a particle has an intrinsic energy given...

  12. Manhattan Project: People

    Office of Scientific and Technical Information (OSTI)

    of California Scientists Bethe, Hans Chadwick, James Einstein, Albert Fermi, Enrico Feynman, Richard Franck, James Fuchs, Klaus Rotblat, Joseph Seaborg, Glenn T. Serber, Robert ...

  13. COLLOQUIUM: "The Usefulness of Useless Knowledge": The History...

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

    curiosity-driven research in the sciences and humanities. Diverse scholars including Albert Einstein, Erwin Panofsky, John von Neumann, J. Robert Oppenheimer, Freeman Dyson, Kurt...

  14. Faculty | Argonne National Laboratory

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

    live for today, hope for tomorrow. The important thing is not to stop questioning." - Albert Einstein Argonne is a place where scientists, engineers and reseachers immerse...

  15. Glenn Seaborg - Hanford Site

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

    For Students and Kids Hanford Fun Facts Classroom Projects Famous People of Hanford Albert Einstein Enrico Fermi Leslie Groves Franklin Matthias Gilbert Church Crawford...

  16. The History of the Light Bulb | Department of Energy

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

    pioneer Charles Proteus Steinmetz (center in light-colored suit) poses with Albert Einstein (immediate left) and other inventors at the RCA Brunswick, New Jersey,...

  17. Institute for Advanced Study Christine Di Bella Institute for...

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

    driven research in the sciences and humanities. Diverse schol- ars including Albert Einstein, Erwin Panofsky, John von Neu- mann, J. Robert Oppenheimer, Freeman Dyson,...

  18. Franklin Delano Roosevelt - Hanford Site

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

    For Students and Kids Hanford Fun Facts Classroom Projects Famous People of Hanford Albert Einstein Enrico Fermi Leslie Groves Franklin Matthias Gilbert Church Crawford...

  19. AE-LOMONOSOV0813.pptx

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

    013 1 Liquid Argon TPCs for future neutrino oscillaon experiments Antonio Ereditato Albert Einstein Center for Fundamental Physics (AEC) Laboratory for High Energy Physics...

  20. Visiting Faculty Program | Argonne National Laboratory

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

    from a new angle, requires creative imagination and marks real advance in science." -Albert Einstein Overview The Visiting Faculty Program (VFP) offers research opportunities for...

  1. Black hole solutions of dimensionally reduced Einstein-Gauss-Bonnet gravity with a cosmological constant

    SciTech Connect (OSTI)

    Melis, M.; Mignemi, S.

    2007-01-15

    We study the phase space of the spherically symmetric solutions of the system obtained from the dimensional reduction of the six-dimensional Einstein-Gauss-Bonnet action with a cosmological constant. We show that all the physical solutions have anti-de Sitter asymptotic behavior.

  2. Black hole solutions of dimensionally reduced Einstein-Gauss-Bonnet gravity

    SciTech Connect (OSTI)

    Mignemi, Salvatore

    2006-12-15

    We study the phase space of the spherically symmetric solutions of the system obtained from the dimensional reduction of the six-dimensional Einstein-Gauss-Bonnet action. We show that all the physically significant solutions are either asymptotically flat or asymptotically anti-de Sitter.

  3. Testing quantum superpositions of the gravitational field with Bose-Einstein condensates

    SciTech Connect (OSTI)

    Lindner, Netanel H.; Peres, Asher

    2005-02-01

    We consider the gravity field of a Bose-Einstein condensate in a quantum superposition. The gravity field then is also in a quantum superposition, which is in principle observable. Hence we have 'quantum gravity' far away from the so-called Planck scale.

  4. On-chip generation of Einstein-Podolsky-Rosen states with arbitrary symmetry

    SciTech Connect (OSTI)

    Grfe, Markus; Heilmann, Ren; Nolte, Stefan; Szameit, Alexander

    2015-05-04

    We experimentally demonstrate a method for integrated-optical generation of two-photon Einstein-Podolsky-Rosen states featuring arbitrary symmetries. In our setting, we employ detuned directional couplers to impose a freely tailorable phase between the two modes of the state. Our results allow to mimic the quantum random walk statistics of bosons, fermions, and anyons, particles with fractional exchange statistics.

  5. Method and apparatus for distinguishing actual sparse events from sparse event false alarms

    DOE Patents [OSTI]

    Spalding, Richard E.; Grotbeck, Carter L.

    2000-01-01

    Remote sensing method and apparatus wherein sparse optical events are distinguished from false events. "Ghost" images of actual optical phenomena are generated using an optical beam splitter and optics configured to direct split beams to a single sensor or segmented sensor. True optical signals are distinguished from false signals or noise based on whether the ghost image is presence or absent. The invention obviates the need for dual sensor systems to effect a false target detection capability, thus significantly reducing system complexity and cost.

  6. Vannevar Bush and Ernest Lawrence -- Two key individuals

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

    1939. This organization had been formed as a direct result of the letter Leo Szilard and Albert Einstein prepared and Einstein signed that was delivered to President Roosevelt by...

  7. Dark matter as a ghost free conformal extension of Einstein theory

    SciTech Connect (OSTI)

    Barvinsky, A.O.

    2014-01-01

    We discuss ghost free models of the recently suggested mimetic dark matter theory. This theory is shown to be a conformal extension of Einstein general relativity. Dark matter originates from gauging out its local Weyl invariance as an extra degree of freedom which describes a potential flow of the pressureless perfect fluid. For a positive energy density of this fluid the theory is free of ghost instabilities, which gives strong preference to stable configurations with a positive scalar curvature and trace of the matter stress tensor. Instabilities caused by caustics of the geodesic flow, inherent in this model, serve as a motivation for an alternative conformal extension of Einstein theory, based on the generalized Proca vector field. A potential part of this field modifies the inflationary stage in cosmology, whereas its rotational part at the post inflationary epoch might simulate rotating flows of dark matter.

  8. Uniform density static fluid sphere in Einstein-Gauss-Bonnet gravity and its universality

    SciTech Connect (OSTI)

    Dadhich, Naresh; Molina, Alfred; Khugaev, Avas

    2010-05-15

    In Newtonian theory, gravity inside a constant density static sphere is independent of spacetime dimension. Interestingly this general result is also carried over to Einsteinian as well as higher order Einstein-Gauss-Bonnet (Lovelock) gravity notwithstanding their nonlinearity. We prove that the necessary and sufficient condition for universality of the Schwarzschild interior solution describing a uniform density sphere for all n{>=}4 is that its density is constant.

  9. Controlling chaos in the Bose-Einstein condensate system of a double lattice

    SciTech Connect (OSTI)

    Wang Zhixia Ni Zhengguo; Cong Fuzhong; Liu Xueshen; Chen Lei

    2011-02-15

    We study the chaotic dynamics in the Bose-Einstein condensate (BEC) system of a double lattice. Chaotic space-time evolution is investigated for the particle number density in a BEC. By changing of the s-wave scattering length with a Feshbach resonance, the chaotic behavior can be well controlled to enter into periodicity. Numerical calculation shows that there is periodic orbit according to the s-wave scattering length only if the maximal Lyapunov exponent of the system is negative.

  10. Controlling chaos in a Bose-Einstein condensate loaded into a moving optical lattice potential

    SciTech Connect (OSTI)

    Wang Zhixia Zhang Xihe; Shen Ke

    2008-11-15

    The spatial structure of a Bose-Einstein condensate loaded into an optical lattice potential is investigated, and spatially chaotic distributions of the condensates are revealed. By means of changing of the s-wave scattering length with a Feshbach resonance, the chaotic behavior can be well controlled to enter into periodicity. Numerical simulation shows that there are different periodic orbits according to different s-wave scattering lengths only if the maximal Lyapunov exponent of the system is negative.

  11. Energy of Einstein's static universe and its implications for the ΛCDM cosmology

    SciTech Connect (OSTI)

    Mitra, Abhas

    2013-03-01

    The total Einstein energy (P{sub 0}) of a homogeneous and isotropic universe can be computed by using an appropriate superpotential (Rosen 1994) and also by a direct method (Mitra 2010). Irrespective of the physical significance of P{sub 0}, its eventual numerical value must be same in both the cases because both are derived from the same Einstein pseudo tensor and by employing the same coordinates. It follows then that the static isotropic and homogeneous universe, i.e., Einstein's static universe (ESU), must have an infinite radius and which tantamounts to a spatially flat case. The physical significance of this result is that the cosmological constant, Λ, is actually zero and ESU is the vacuous Minkowski spacetime. It is the same result which has recently been obtained in a completely independent manner (Mitra, Bhattacharyya and Bhatt 2013). Thus even though, mathematically, one can conceive of a static 3-sphere for the foundation of relativistic cosmology, physically, no such 3-sphere exists. On the other hand, the spatial section of the universe could essentially be an Euclidean space with local curvature spikes due to presence of lumpy matter. Since the ''Dark Energy'' is associated with Λ in the ΛCDM model, the result obtained here suggests that it is an artifact of departure of the lumpy and fractal universe from the ideal Friedmann Robertson Walker model (Jackson et al. 2012, Cowley et al. 2013)

  12. Entropy density of an adiabatic relativistic Bose-Einstein condensate star

    SciTech Connect (OSTI)

    Khaidir, Ahmad Firdaus; Kassim, Hasan Abu; Yusof, Norhasliza

    2015-04-24

    Inspired by recent works, we investigate how the thermodynamics parameters (entropy, temperature, number density, energy density, etc) of Bose-Einstein Condensate star scale with the structure of the star. Below the critical temperature in which the condensation starts to occur, we study how the entropy behaves with varying temperature till it reaches its own stability against gravitational collapse and singularity. Compared to photon gases (pressure is described by radiation) where the chemical potential, ? is zero, entropy of photon gases obeys the Stefan-Boltzmann Law for a small values of T while forming a spiral structure for a large values of T due to general relativity. The entropy density of Bose-Einstein Condensate is obtained following the similar sequence but limited under critical temperature condition. We adopt the scalar field equation of state in Thomas-Fermi limit to study the characteristics of relativistic Bose-Einstein condensate under varying temperature and entropy. Finally, we obtain the entropy density proportional to (?T{sup 3}-3T) which obeys the Stefan-Boltzmann Law in ultra-relativistic condition.

  13. BoseEinstein condensation versus DickeHeppLieb transition in an optical cavity

    SciTech Connect (OSTI)

    Piazza, Francesco; Strack, Philipp; Zwerger, Wilhelm

    2013-12-15

    We provide an exact solution for the interplay between BoseEinstein condensation and the DickeHeppLieb self-organization transition of an ideal Bose gas trapped inside a single-mode optical cavity and subject to a transverse laser drive. Based on an effective action approach, we determine the full phase diagram at arbitrary temperature, which features a bi-critical point where the transitions cross. We calculate the dynamically generated band structure of the atoms and the associated suppression of the critical temperature for BoseEinstein condensation in the phase with a spontaneous periodic density modulation. Moreover, we determine the evolution of the polariton spectrum due to the coupling of the cavity photons and the atomic field near the self-organization transition, which is quite different above or below the BoseEinstein condensation temperature. At low temperatures, the critical value of the DickeHeppLieb transition decreases with temperature and thus thermal fluctuations can enhance the tendency to a periodic arrangement of the atoms. -- Highlights: Atoms inside a driven cavity can undergo two transitions: self-organization and BEC. The phase diagram has four phases which coexist at a bi-critical point. Atomcavity coupling creates a dynamical lattice for the atoms. Finite temperature can enhance the tendency towards self-organization. We calculate the detailed spectrum of the polaritonic excitations.

  14. Distinguishability and chiral stability in solution: Effects of decoherence and intermolecular interactions

    SciTech Connect (OSTI)

    Han, Heekyung; Wardlaw, David M.; Frolov, Alexei M.

    2014-05-28

    We examine the effect of decoherence and intermolecular interactions (chiral discrimination energies) on the chiral stability and the distinguishability of initially pure versus mixed states in an open chiral system. Under a two-level approximation for a system, intermolecular interactions are introduced by a mean-field theory, and interaction between a system and an environment is modeled by a continuous measurement of a population difference between the two chiral states. The resultant equations are explored for various parameters, with emphasis on the combined effects of the initial condition of the system, the chiral discrimination energies, and the decoherence in determining: the distinguishability as measured by a population difference between the initially pure and mixed states, and the decoherence process; the chiral stability as measured by the purity decay; and the stationary state of the system at times long relative to the time scales of the system dynamics and of the environmental effects.

  15. Microsoft Word - Larsson, Mats - IMS Distinguished Lecture Series - Speaker Information.docx

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

    Mats Larsson Stockholm University Director of AlbaNova University Center Institute for Materials Science Distinguished Lecture Series Spontaneous Symmetry Breaking, Chirality, and Lev Landau and his Nobel Prize Date: Tuesday, January 19, 2016 Time: 2pm - 3pm Location: MSL Auditorium (TA-03 - Bldg 1698 - Room A103) Hosted By Alexander Balatsky Abstract The concept of spontaneous symmetry breaking has served physics well for almost a century, with ferromagnetism, superfluidity, and

  16. Thermodynamics of Taub-NUT/bolt-AdS black holes in Einstein-Gauss-Bonnet gravity

    SciTech Connect (OSTI)

    Khodam-Mohammadi, A.; Monshizadeh, M.

    2009-02-15

    We give a review of the existence of Taub-NUT/bolt solutions in Einstein Gauss-Bonnet gravity with the parameter {alpha} in six dimensions. Although the spacetime with base space S{sup 2}xS{sup 2} has a curvature singularity at r=N, which does not admit NUT solutions, we may proceed with the same computations as in the CP{sup 2} case. The investigation of thermodynamics of NUT/bolt solutions in six dimensions is carried out. We compute the finite action, mass, entropy, and temperature of the black hole. Then the validity of the first law of thermodynamics is demonstrated. It is shown that in NUT solutions all thermodynamic quantities for both base spaces are related to each other by substituting {alpha}{sup CP{sup k}}=[(k+1)/k]{alpha}{sup S{sup 2}}{sup xS{sup 2}}{sup x...S{sub k}{sup 2}}. So, no further information is given by investigating NUT solutions in the S{sup 2}xS{sup 2} case. This relation is not true for bolt solutions. A generalization of the thermodynamics of black holes to arbitrary even dimensions is made using a new method based on the Gibbs-Duhem relation and Gibbs free energy for NUT solutions. According to this method, the finite action in Einstein Gauss-Bonnet is obtained by considering the generalized finite action in Einstein gravity with an additional term as a function of {alpha}. Stability analysis is done by investigating the heat capacity and entropy in the allowed range of {alpha}, {lambda}, and N. For NUT solutions in d dimensions, there exists a stable phase at a narrow range of {alpha}. In six-dimensional bolt solutions, the metric is completely stable for B=S{sup 2}xS{sup 2} and is completely unstable for the B=CP{sup 2} case.

  17. Interaction of half-quantized vortices in two-component Bose-Einstein condensates

    SciTech Connect (OSTI)

    Eto, Minoru; Kasamatsu, Kenichi; Nitta, Muneto; Takeuchi, Hiromitsu; Tsubota, Makoto

    2011-06-15

    We study the asymptotic interaction between two half-quantized vortices in two-component Bose-Einstein condensates. When two vortices in different components are placed at distance 2R, the leading order of the force between them is found to be (lnR/{xi}-1/2)/R{sup 3}, in contrast to 1/R between vortices placed in the same component. We derive it analytically using the Abrikosov ansatz and the profile functions of the vortices, confirmed numerically with the Gross-Pitaevskii model. We also find that the short-range cutoff of the intervortex potential linearly depends on the healing length.

  18. Dynamical generation of phase-squeezed states in two-component Bose-Einstein condensates

    SciTech Connect (OSTI)

    Jin, G. R.; An, Y.; Yan, T.; Lu, Z. S. [Department of Physics, Beijing Jiaotong University, Beijing 100044 (China)

    2010-12-15

    As an ''input'' state of a linear (Mach-Zehnder or Ramsey) interferometer, the phase-squeezed state proposed by Berry and Wiseman exhibits the best sensitivity approaching to the Heisenberg limit [Phys. Rev. Lett. 85, 5098 (2000)]. Similar with the Berry and Wiseman's state, we find that two kinds of phase-squeezed states can be generated dynamically with atomic Bose-Einstein condensates confined in a symmetric double-well potential, which shows squeezing along spin operator S{sub y} and antisqueezing along S{sub z}, leading to subshot-noise phase estimation.

  19. Diffraction of a Bose-Einstein condensate in the time domain

    SciTech Connect (OSTI)

    Colombe, Yves; Mercier, Brigitte; Perrin, Helene; Lorent, Vincent

    2005-12-15

    We have observed the diffraction of a Bose-Einstein condensate of rubidium atoms on a vibrating mirror potential. The matter wave packet bounces back at normal incidence on a blue-detuned evanescent light field after a 3.6 mm free fall. The mirror vibrates at a frequency of 500 kHz with an amplitude of 3 nm. The atomic carrier and side bands are directly imaged during their ballistic expansion. The locations and the relative weights of the diffracted atomic wave packets are in very good agreement with the theoretical prediction of Henkel et al. [J. Phys. II 4, 1877 (1994)].

  20. Gluon transport equation with effective mass and dynamical onset of Bose–Einstein condensation

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Blaizot, Jean-Paul; Jiang, Yin; Liao, Jinfeng

    2016-05-01

    In this paper we study the transport equation describing a dense system of gluons, in the small scattering angle approximation, taking into account medium-generated effective masses of the gluons. We focus on the case of overpopulated systems that are driven to Bose–Einstein condensation on their way to thermalization. Lastly, the presence of a mass modifies the dispersion relation of the gluon, as compared to the massless case, but it is shown that this does not change qualitatively the scaling behavior in the vicinity of the onset.

  1. Five-dimensional black strings in Einstein-Gauss-Bonnet gravity

    SciTech Connect (OSTI)

    Kobayashi, Tsutomu; Tanaka, Takahiro

    2005-04-15

    We consider black-string-type solutions in five-dimensional Einstein-Gauss-Bonnet gravity. Numerically constructed solutions under static, axially symmetric and translationally invariant metric ansatz are presented. The solutions are specified by two asymptotic charges: mass of a black string and a scalar charge associated with the radion part of the metric. Regular black string solutions are found if and only if the two charges satisfy a fine-tuned relation, and otherwise the spacetime develops a singular event horizon or a naked singularity. We can also generate bubble solutions from the black strings by using a double Wick rotation.

  2. Stable Vortex-Bright-Soliton Structures in Two-Component Bose-Einstein Condensates

    SciTech Connect (OSTI)

    Law, K. J. H.; Kevrekidis, P. G.; Tuckerman, Laurette S.

    2010-10-15

    We report the numerical realization of robust two-component structures in 2D and 3D Bose-Einstein condensates with nontrivial topological charge in one component. We identify a stable symbiotic state in which a higher-dimensional bright soliton exists even in a homogeneous setting with defocusing interactions, due to the effective potential created by a stable vortex in the other component. The resulting vortex-bright-solitons, generalizations of the recently experimentally observed dark-bright solitons, are found to be very robust both in the homogeneous medium and in the presence of external confinement.

  3. Exploiting Soliton Decay and Phase Fluctuations in Atom Chip Interferometry of Bose-Einstein Condensates

    SciTech Connect (OSTI)

    Scott, R. G.; Judd, T. E.; Fromhold, T. M.

    2008-03-14

    We show that the decay of a soliton into vortices provides a mechanism for measuring the initial phase difference between two merging Bose-Einstein condensates. At very low temperatures, the mechanism is resonant, operating only when the clouds start in antiphase. But at higher temperatures, phase fluctuations trigger vortex production over a wide range of initial relative phase, as observed in recent experiments at MIT. Choosing the merge time to maximize the number of vortices created makes the interferometer highly sensitive to spatially varying phase patterns and hence atomic movement.

  4. Controlling soliton interactions in Bose-Einstein condensates by synchronizing the Feshbach resonance and harmonic trap

    SciTech Connect (OSTI)

    Zhang Xiaofei |; Yang Qin |; Zhang Jiefang; Chen, X. Z.; Liu, W. M.

    2008-02-15

    We present how to control interactions between solitons, either bright or dark, in Bose-Einstein condensates by synchronizing Feshbach resonance and harmonic trap. Our results show that as long as the scattering length is to be modulated in time via a changing magnetic field near the Feshbach resonance, and the harmonic trapping frequencies are also modulated in time, exact solutions of the one-dimensional nonlinear Schroedinger equation can be found in a general closed form, and interactions between two solitons are modulated in detail in currently experimental conditions. We also propose experimental protocols to observe the phenomena such as fusion, fission, warp, oscillation, elastic collision in future experiments.

  5. Swift Loss of Coherence of Soliton Trains in Attractive Bose-Einstein Condensates

    SciTech Connect (OSTI)

    Streltsov, Alexej I.; Cederbaum, Lorenz S.; Alon, Ofir E.

    2011-06-17

    Experiments on ultracold attractive Bose-Einstein condensates (BECs) have demonstrated that at low dimensions atomic clouds can form localized objects, propagating for long times without significant changes in their shapes and attributed to bright matter-wave solitons, which are coherent objects. We consider the dynamics of bright soliton trains from the perspective of many-boson physics. The fate of matter-wave soliton trains is actually to quickly lose their coherence and become macroscopically fragmented BECs. The death of the coherent matter-wave soliton trains gives birth to fragmented objects, whose quantum properties and experimental signatures differ substantially from what is currently assumed.

  6. Rectified motion of a Bose-Einstein condensate in a horizontally vibrating shallow optical lattice

    SciTech Connect (OSTI)

    Azizi, Y.; Valizadeh, A.

    2011-01-15

    We consider a Bose-Einstein condensate, described by the Gross-Pitaevskii equation, in a horizontally vibrating shallow optical lattice. We study the dynamics of a bright soliton using the collective coordinate approximation. We show that depending on the parameters, amplitude, and frequency of the vibration of the lattice, the phase space of the equation of motion for the soliton center of mass shows multistability. In the frequency locked regions, in which the soliton has a nonzero average velocity determined by the external frequency, the motion is quasiperiodic, and between the locked regions the soliton moves chaotically.

  7. Rotational fluxons of Bose-Einstein condensates in coplanar double-ring traps

    SciTech Connect (OSTI)

    Brand, J.; Haigh, T. J.; Zuelicke, U.

    2009-07-15

    Rotational analogs to magnetic fluxons in conventional Josephson junctions are predicted to emerge in the ground state of rotating tunnel-coupled annular Bose-Einstein condensates (BECs). Such topological condensate-phase structures can be manipulated by external potentials. We determine conditions for observing macroscopic quantum tunneling of a fluxon. Rotational fluxons in double-ring BECs can be created, manipulated, and controlled by external potentials in different ways than is possible in the solid-state system, thus rendering them a promising candidate system for studying and utilizing quantum properties of collective many-particle degrees of freedom.

  8. Collapses and Revivals of Bose-Einstein Condensates Formed in Small Atomic Samples

    SciTech Connect (OSTI)

    Wright, E.M.; Walls, D.F.; Garrison, J.C.

    1996-09-01

    The macroscopic wave function for atomic samples composed of a few thousand particles is shown to exhibit collapses and revivals on a few seconds time scale, while Bose-Einstein condensation remains in the form of off-diagonal long-range order in the one-particle reduced density matrix. A recently proposed measurement scheme which is sensitive to Bose-broken gauge symmetry, and hence to the macroscopic wave function, could be used to detect the collapses and revivals experimentally. {copyright} {ital 1996 The American Physical Society.}

  9. Post-Newtonian parameters and constraints on Einstein-aether theory

    SciTech Connect (OSTI)

    Foster, Brendan Z.; Jacobson, Ted

    2006-03-15

    We analyze the observational and theoretical constraints on ''Einstein-aether theory,'' a generally covariant theory of gravity coupled to a dynamical, unit, timelike vector field that breaks local Lorentz symmetry. The results of a computation of the remaining post-Newtonian parameters are reported. These are combined with other results to determine the joint post-Newtonian, vacuum-Cerenkov, nucleosynthesis, stability, and positive-energy constraints. All of these constraints are satisfied by parameters in a large two-dimensional region in the four-dimensional parameter space defining the theory.

  10. Einstein-aether theory, violation of Lorentz invariance, and metric-affine gravity

    SciTech Connect (OSTI)

    Heinicke, Christian; Baekler, Peter; Hehl, Friedrich W.

    2005-07-15

    We show that the Einstein-aether theory of Jacobson and Mattingly (J and M) can be understood in the framework of the metric-affine (gauge theory of) gravity (MAG). We achieve this by relating the aether vector field of J and M to certain post-Riemannian nonmetricity pieces contained in an independent linear connection of spacetime. Then, for the aether, a corresponding geometrical curvature-square Lagrangian with a massive piece can be formulated straightforwardly. We find an exact spherically symmetric solution of our model.

  11. Bose-Einstein condensation and superfluidity of magnetoexcitons in bilayer graphene

    SciTech Connect (OSTI)

    Berman, Oleg L.; Lozovik, Yurii E.; Gumbs, Godfrey

    2008-04-15

    We propose experiments to observe Bose-Einstein condensation and superfluidity of quasi-two-dimensional spatially indirect magnetoexcitons in two-layer graphene. The energy spectrum of collective excitations, the sound spectrum, and the effective magnetic mass of magnetoexcitons are presented in the strong magnetic field regime. The superfluid density n{sub S} and the temperature of the Kosterlitz-Thouless phase transition T{sub c} are shown to be increasing functions of the excitonic density n but decreasing functions of B and the interlayer separation D.

  12. Persistent currents in a circular array of Bose-Einstein condensates

    SciTech Connect (OSTI)

    Paraoanu, Gh.-S.

    2003-02-01

    A ring-shaped array of Bose-Einstein condensed atomic gases can display circular currents if the relative phase of neighboring condensates becomes locked to certain values. It is shown that, irrespective of the mechanism responsible for generating these states, only a restricted set of currents are stable, depending on the number of condensates, on the interaction and tunneling energies, and on the total number of particles. Different instabilities due to quasiparticle excitations are characterized, and possible experimental setups for testing the stability prediction are also discussed.

  13. Distinguishing neutrino mass hierarchies using dark matter annihilation signals at IceCube

    SciTech Connect (OSTI)

    Allahverdi, Rouzbeh; Dutta, Bhaskar; Ghosh, Dilip Kumar; Knockel, Bradley; Saha, Ipsita

    2015-12-01

    We explore the possibility of distinguishing neutrino mass hierarchies through the neutrino signal from dark matter annihilation at neutrino telescopes. We consider a simple extension of the standard model where the neutrino masses and mixing angles are obtained via the type-II seesaw mechanism as an explicit example. We show that future extensions of IceCube neutrino telescope may detect the neutrino signal from DM annihilation at the Galactic Center and inside the Sun, and differentiate between the normal and inverted mass hierarchies, in this model.

  14. How real-time cosmology can distinguish between different anisotropic models

    SciTech Connect (OSTI)

    Amendola, Luca; Bjlde, Ole Eggers; Valkenburg, Wessel; Wong, Yvonne Y.Y. E-mail: oeb@phys.au.dk E-mail: yvonne.y.wong@unsw.edu.au

    2013-12-01

    We present a new analysis on how to distinguish between isotropic and anisotropic cosmological models based on tracking the angular displacements of a large number of distant quasars over an extended period of time, and then performing a multipole-vector decomposition of the resulting displacement maps. We find that while the GAIA mission operating at its nominal specifications does not have sufficient angular resolution to resolve anisotropic universes from isotropic ones using this method within a reasonable timespan of ten years, a next-generation GAIA-like survey with a resolution ten times better should be equal to the task. Distinguishing between different anisotropic models is however more demanding. Keeping the observational timespan to ten years, we find that the angular resolution of the survey will need to be of order 0.1 ?as in order for certain rotating anisotropic models to produce a detectable signature that is also unique to models of this class. However, should such a detection become possible, it would immediately allow us to rule out large local void models.

  15. Unified Einstein-Virasoro Master Equation in the General Non-Linear Sigma Model

    SciTech Connect (OSTI)

    Boer, J. de; Halpern, M.B.

    1996-06-05

    The Virasoro master equation (VME) describes the general affine-Virasoro construction $T=L^abJ_aJ_b+iD^a \\dif J_a$ in the operator algebra of the WZW model, where $L^ab$ is the inverse inertia tensor and $D^a $ is the improvement vector. In this paper, we generalize this construction to find the general (one-loop) Virasoro construction in the operator algebra of the general non-linear sigma model. The result is a unified Einstein-Virasoro master equation which couples the spacetime spin-two field $L^ab$ to the background fields of the sigma model. For a particular solution $L_G^ab$, the unified system reduces to the canonical stress tensors and conventional Einstein equations of the sigma model, and the system reduces to the general affine-Virasoro construction and the VME when the sigma model is taken to be the WZW action. More generally, the unified system describes a space of conformal field theories which is presumably much larger than the sum of the general affine-Virasoro construction and the sigma model with its canonical stress tensors. We also discuss a number of algebraic and geometrical properties of the system, including its relation to an unsolved problem in the theory of $G$-structures on manifolds with torsion.

  16. Thermodynamics of rotating black branes in (n+1)-dimensional Einstein-Born-Infeld gravity

    SciTech Connect (OSTI)

    Dehghani, M. H.; Sedehi, H. R. Rastegar

    2006-12-15

    We construct a new class of charged rotating solutions of (n+1)-dimensional Einstein-Born-Infeld gravity with cylindrical or toroidal horizons in the presence of cosmological constant and investigate their properties. These solutions are asymptotically (anti)-de Sitter and reduce to the solutions of Einstein-Maxwell gravity as the Born-Infeld parameters goes to infinity. We find that these solutions can represent black branes, with inner and outer event horizons, an extreme black brane or a naked singularity provided the parameters of the solutions are chosen suitably. We compute temperature, mass, angular momentum, entropy, charge and electric potential of the black brane solutions. We obtain a Smarr-type formula and show that these quantities satisfy the first law of thermodynamics. We also perform a stability analysis by computing the heat capacity and the determinant of Hessian matrix of mass of the system with infinite boundary with respect to its thermodynamic variables in both the canonical and the grand-canonical ensembles, and show that the system is thermally stable in the whole phase space. Also, we find that there exists an unstable phase when the finite size effect is taken into account.

  17. Bose-Einstein Condensation and Bose Glasses in an S = 1 Organo-metallic quantum magnet

    SciTech Connect (OSTI)

    Zapf, Vivien

    2012-06-01

    I will speak about Bose-Einstein condensation (BEC) in quantum magnets, in particular the compound NiCl2-4SC(NH2)2. Here a magnetic field-induced quantum phase transition to XY antiferromagnetism can be mapped onto BEC of the spins. The tuning parameter for BEC transition is the magnetic field rather than the temperature. Some interesting phenomena arise, for example the fact that the mass of the bosons that condense can be strongly renormalized by quantum fluctuations. I will discuss the utility of this mapping for both understanding the nature of the quantum magnetism and testing the thermodynamic limit of Bose-Einstein Condensation. Furthermore we can dope the system in a clean and controlled way to create the long sought-after Bose Glass transition, which is the bosonic analogy of Anderson localization. I will present experiments and simulations showing evidence for a new scaling exponent, which finally makes contact between theory and experiments. Thus we take a small step towards the difficult problem of understanding the effect of disorder on bosonic wave functions.

  18. Strong field effects on binary systems in Einstein-aether theory

    SciTech Connect (OSTI)

    Foster, Brendan Z.

    2007-10-15

    'Einstein-aether' theory is a generally covariant theory of gravity containing a dynamical preferred frame. This article continues an examination of effects on the motion of binary pulsar systems in this theory, by incorporating effects due to strong fields in the vicinity of neutron star pulsars. These effects are included through an effective approach, by treating the compact bodies as point particles with nonstandard, velocity dependent interactions parametrized by dimensionless sensitivities. Effective post-Newtonian equations of motion for the bodies and the radiation damping rate are determined. More work is needed to calculate values of the sensitivities for a given fluid source; therefore, precise constraints on the theory's coupling constants cannot yet be stated. It is shown, however, that strong field effects will be negligible given current observational uncertainties if the dimensionless couplings are less than roughly 0.1 and two conditions that match the PPN parameters to those of pure general relativity are imposed. In this case, weak field results suffice. There then exists a one-parameter family of Einstein-aether theories with 'small-enough' couplings that passes all current observational tests. No conclusion can be reached for larger couplings until the sensitivities for a given source can be calculated.

  19. Distinguishing Supersymmetry From Universal Extra Dimensions or Little Higgs Models With Dark Matter Experiments

    SciTech Connect (OSTI)

    Hooper, Dan; Zaharijas, Gabrijela; /Fermilab

    2006-12-01

    There are compelling reasons to think that new physics will appear at or below the TeV-scale. It is not known what form this new physics will take, however. Although The Large Hadron collider is very likely to discover new particles associated with the TeV-scale, it may be difficult for it to determine the nature of those particles, whether superpartners, Kaluza-Klein modes or other states. In this article, we consider how direct and indirect dark matter detection experiments may provide information complementary to hadron colliders, which can be used to discriminate between supersymmetry, models with universal extra dimensions, and Little Higgs theories. We find that, in many scenarios, dark matter experiments can be effectively used to distinguish between these possibilities.

  20. Fluctuation statistics of mesoscopic Bose-Einstein condensates: Reconciling the master equation with the partition function to reexamine the Uhlenbeck-Einstein dilemma

    SciTech Connect (OSTI)

    Jordan, Andrew N.; Ooi, C. H. Raymond; Svidzinsky, Anatoly A.

    2006-09-15

    The atom fluctuation statistics of an ideal, mesoscopic, Bose-Einstein condensate are investigated from several different perspectives. By generalizing the grand canonical analysis (applied to the canonical ensemble problem), we obtain a self-consistent equation for the mean condensate particle number that coincides with the microscopic result calculated from the laser master equation approach. For the case of a harmonic trap, we obtain an analytic expression for the condensate particle number that is very accurate at all temperatures, when compared with numerical canonical ensemble results. Applying a similar generalized grand canonical treatment to the variance, we obtain an accurate result only below the critical temperature. Analytic results are found for all higher moments of the fluctuation distribution by employing the stochastic path integral formalism, with excellent accuracy. We further discuss a hybrid treatment, which combines the master equation and stochastic path integral analysis with results obtained based on the canonical ensemble quasiparticle formalism [Kocharovsky et al., Phys. Rev. A 61, 053606 (2000)], producing essentially perfect agreement with numerical simulation at all temperatures.

  1. Primordial massive gravitational waves from Einstein-Chern-Simons-Weyl gravity

    SciTech Connect (OSTI)

    Myung, Yun Soo; Moon, Taeyoon E-mail: tymoon@inje.ac.kr

    2014-08-01

    We investigate the evolution of cosmological perturbations during de Sitter inflation in the Einstein-Chern-Simons-Weyl gravity. Primordial massive gravitational waves are composed of one scalar, two vector and four tensor circularly polarized modes. We show that the vector power spectrum decays quickly like a transversely massive vector in the superhorizon limit z?0. In this limit, the power spectrum coming from massive tensor modes decays quickly, leading to the conventional tensor power spectrum. Also, we find that in the limit of m{sup 2}?0 (keeping the Weyl-squared term only), the vector and tensor power spectra disappear. It implies that their power spectra are not gravitationally produced because they (vector and tensor) are decoupled from the expanding de Sitter background, as a result of conformal invariance.

  2. Bose-Einstein Condensation of Magnons in Cs{sub 2}CuCl{sub 4}

    SciTech Connect (OSTI)

    Radu, T.; Wilhelm, H.; Luehmann, T.; Steglich, F.; Yushankhai, V.; Kovrizhin, D.; Coldea, R.; Tylczynski, Z.

    2005-09-16

    We report on results of specific heat measurements on single crystals of the frustrated quasi-2D spin-1/2 antiferromagnet Cs{sub 2}CuCl{sub 4} (T{sub N}=0.595 K) in external magnetic fields B<12 T and for temperatures T>30 mK. Decreasing B from high fields leads to the closure of the field-induced gap in the magnon spectrum at a critical field B{sub c}{approx_equal}8.51 T and a magnetic phase transition is clearly seen below B{sub c}. In the vicinity of B{sub c}, the phase transition boundary is well described by the power law T{sub c}(B){proportional_to}(B{sub c}-B){sup 1/{phi}}, with the measured critical exponent {phi}{approx_equal}1.5. These findings are interpreted as a Bose-Einstein condensation of magnons.

  3. Long-lived periodic revivals of coherence in an interacting Bose-Einstein condensate

    SciTech Connect (OSTI)

    Egorov, M.; Ivannikov, V.; Opanchuk, B.; Drummond, P.; Hall, B. V.; Sidorov, A. I. [ARC Centre of Excellence for Quantum-Atom Optics and Centre for Atom Optics and Ultrafast Spectroscopy, Swinburne University of Technology, Melbourne 3122 (Australia); Anderson, R. P. [ARC Centre of Excellence for Quantum-Atom Optics and Centre for Atom Optics and Ultrafast Spectroscopy, Swinburne University of Technology, Melbourne 3122 (Australia); School of Physics, Monash University, Victoria 3800 (Australia)

    2011-08-15

    We observe the coherence of an interacting two-component Bose-Einstein condensate (BEC) surviving for seconds in a trapped Ramsey interferometer. Mean-field-driven collective oscillations of two components lead to periodic dephasing and rephasing of condensate wave functions with a slow decay of the interference fringe visibility. We apply spin echo synchronous with the self-rephasing of the condensate to reduce the influence of state-dependent atom losses, significantly enhancing the visibility up to 0.75 at the evolution time of 1.5 s. Mean-field theory consistently predicts higher visibility than experimentally observed values. We quantify the effects of classical and quantum noise and infer a coherence time of 2.8 s for a trapped condensate of 5.5x10{sup 4} interacting atoms.

  4. Radiating black holes in Einstein-Yang-Mills theory and cosmic censorship

    SciTech Connect (OSTI)

    Ghosh, Sushant G.; Dadhich, Naresh

    2010-08-15

    Exact nonstatic spherically symmetric black-hole solutions of the higher dimensional Einstein-Yang-Mills equations for a null dust with Yang-Mills gauge charge are obtained by employing Wu-Yang ansatz, namely, HD-EYM Vaidya solution. It is interesting to note that gravitational contribution of Yang-Mills (YM) gauge charge for this ansatz is indeed opposite (attractive rather than repulsive) that of Maxwell charge. It turns out that the gravitational collapse of null dust with YM gauge charge admits strong curvature shell focusing naked singularities violating cosmic censorship. However, there is significant shrinkage of the initial data space for a naked singularity of the HD-Vaidya collapse due to presence of YM gauge charge. The effect of YM gauge charge on structure and location of the apparent and event horizons is also discussed.

  5. Thermodynamics of black holes in (n+1)-dimensional Einstein-Born-Infeld-dilaton gravity

    SciTech Connect (OSTI)

    Sheykhi, A.; Riazi, N.

    2007-01-15

    We construct a new class of (n+1)-dimensional (n{>=}3) black hole solutions in Einstein-Born-Infeld-dilaton gravity with Liouville-type potential for the dilaton field and investigate their properties. These solutions are neither asymptotically flat nor (anti)-de Sitter. We find that these solutions can represent black holes, with inner and outer event horizons, an extreme black hole, or a naked singularity provided the parameters of the solutions are chosen suitably. We compute the thermodynamic quantities of the black hole solutions and find that these quantities satisfy the first law of thermodynamics. We also perform a stability analysis and investigate the effect of dilaton on the stability of the solutions.

  6. Multiple dark-bright solitons in atomic Bose-Einstein condensates

    SciTech Connect (OSTI)

    Yan, D.; Kevrekidis, P. G.; Chang, J. J.; Hamner, C.; Engels, P.; Achilleos, V.; Frantzeskakis, D. J.; Carretero-Gonzalez, R.; Schmelcher, P.

    2011-11-15

    Motivated by recent experimental results, we present a systematic theoretical analysis of dark-bright-soliton interactions and multiple-dark-bright-soliton complexes in atomic two-component Bose-Einstein condensates. We study analytically the interactions between two dark-bright solitons in a homogeneous condensate and then extend our considerations to the presence of the trap. We illustrate the existence of robust stationary dark-bright-soliton ''molecules,'' composed of two or more solitons, which are formed due to the competition of the interaction forces between the dark- and bright-soliton components and the trap force. Our analysis is based on an effective equation of motion, derived for the distance between two dark-bright solitons. This equation provides equilibrium positions and characteristic oscillation frequencies of the solitons, which are found to be in good agreement with the eigenfrequencies of the anomalous modes of the system.

  7. Phonon Instability with Respect to Soliton Formation in Two-Dimensional Dipolar Bose-Einstein Condensates

    SciTech Connect (OSTI)

    Nath, R.; Santos, L.; Pedri, P.

    2009-02-06

    The partially attractive character of the dipole-dipole interaction leads to phonon instability in dipolar Bose-Einstein condensates, which is followed by collapse in 3D geometries. We show that in 2D, the nature of the post-instability dynamics is fundamentally different, due to the stabilization of 2D solitons. As a result, a transient gas of attractive solitons is formed, and collapse may be avoided. In the presence of an harmonic trap, the post-instability dynamics is characterized by a transient pattern formation followed by the creation of stable 2D solitons. This dynamics should be observable in ongoing experiments, allowing for the creation of stable 2D solitons for the first time ever in quantum gases.

  8. Dark soliton decay due to trap anharmonicity in atomic Bose-Einstein condensates

    SciTech Connect (OSTI)

    Parker, N. G.; Proukakis, N. P.; Adams, C. S.

    2010-03-15

    A number of recent experiments with nearly pure atomic Bose-Einstein condensates have confirmed the predicted dark soliton oscillations when under harmonic trapping. However, a dark soliton propagating in an inhomogeneous condensate has also been predicted to be unstable to the emission of sound waves. Although harmonic trapping supports an equilibrium between the coexisting soliton and sound, we show that the ensuing dynamics are sensitive to trap anharmonicities. Such anharmonicities can break the soliton-sound equilibrium and lead to the net decay of the soliton on a considerably shorter time scale than other dissipation mechanisms. Thus, we propose that small realistic modifications to existing experimental setups could enable the experimental observation of this decay channel.

  9. Dark soliton beats in the time-varying background of Bose-Einstein condensates

    SciTech Connect (OSTI)

    Wu Lei; Li Lu; Zhang Jiefang

    2009-07-15

    We investigate the dynamics of dark solitons in one-dimensional Bose-Einstein condensates. In the large particle limit, by introducing the lens-type transformation, we find that the macroscopic wave function evolves self-similarly when its initial profile strays from that of the equilibrium state, which provides a time-varying background for the propagation of dark solitons. The interaction of dark solitons with this kind of background is studied both analytically and numerically. We find that the center-of-mass motion of the dark soliton is deeply affected by the time-varying background, and the beating phenomena of dark soliton emerge when the intrinsic frequency of the dark soliton approaches that of the background. Lastly, we investigate the propagation of dark solitons in the freely expanding background.

  10. Feshbach-resonant Raman photoassociation in a Bose-Einstein condensate

    SciTech Connect (OSTI)

    Mackie, Matt; Phou, Pierre; Shinn, Mannix; Boyce, Heather; Katz, Lev

    2011-10-15

    We model the formation of stable heteronuclear molecules via pulsed Raman photoassociation of a two-component Bose-Einstein condensate near a strong Feshbach resonance, for both counterintuitive and intuitive pulse sequencing. Compared to lasers alone, weak Raman photoassociation is enhanced by as much as a factor of ten (five) for a counterintuitive (intuitive) pulse sequence, whereas strong Raman photoassociation is barely enhanced at all--regardless of pulse sequence. Stronger intra-atom, molecule, or atom-molecule collisions lead to an expected decrease in conversion efficiency, but stronger ambient inter-atom collisions lead to an unexpected increase in the efficiency of stable molecule production. Numerical results agree reasonably with an analytical approximation.

  11. Rayleigh surface wave interaction with the 2D exciton Bose-Einstein condensate

    SciTech Connect (OSTI)

    Boev, M. V.; Kovalev, V. M.

    2015-06-15

    We describe the interaction of a Rayleigh surface acoustic wave (SAW) traveling on the semiconductor substrate with the excitonic gas in a double quantum well located on the substrate surface. We study the SAW attenuation and its velocity renormalization due to the coupling to excitons. Both the deformation potential and piezoelectric mechanisms of the SAW-exciton interaction are considered. We focus on the frequency and excitonic density dependences of the SAW absorption coefficient and velocity renormalization at temperatures both above and well below the critical temperature of Bose-Einstein condensation of the excitonic gas. We demonstrate that the SAW attenuation and velocity renormalization are strongly different below and above the critical temperature.

  12. Chaotic behavior of three interacting vortices in a confined Bose-Einstein condensate

    SciTech Connect (OSTI)

    Kyriakopoulos, Nikos; Koukouloyannis, Vassilis; Skokos, Charalampos; Kevrekidis, Panayotis G.

    2014-06-01

    Motivated by recent experimental works, we investigate a system of vortex dynamics in an atomic Bose-Einstein condensate (BEC), consisting of three vortices, two of which have the same charge. These vortices are modeled as a system of point particles which possesses a Hamiltonian structure. This tripole system constitutes a prototypical model of vortices in BECs exhibiting chaos. By using the angular momentum integral of motion, we reduce the study of the system to the investigation of a two degree of freedom Hamiltonian model and acquire quantitative results about its chaotic behavior. Our investigation tool is the construction of scan maps by using the Smaller ALignment Index as a chaos indicator. Applying this approach to a large number of initial conditions, we manage to accurately and efficiently measure the extent of chaos in the model and its dependence on physically important parameters like the energy and the angular momentum of the system.

  13. Bose-Einstein condensates on tilted lattices: Coherent, chaotic, and subdiffusive dynamics

    SciTech Connect (OSTI)

    Kolovsky, Andrey R.; Gomez, Edgar A.; Korsch, Hans Juergen

    2010-02-15

    The dynamics of a (quasi-) one-dimensional interacting atomic Bose-Einstein condensate in a tilted optical lattice is studied in a discrete mean-field approximation, i.e., in terms of the discrete nonlinear Schroedinger equation. If the static field is varied, the system shows a plethora of dynamical phenomena. In the strong field limit, we demonstrate the existence of (almost) nonspreading states which remain localized on the lattice region populated initially and show coherent Bloch oscillations with fractional revivals in the momentum space (so-called quantum carpets). With decreasing field, the dynamics becomes irregular, however, still confined in configuration space. For even weaker fields, we find subdiffusive dynamics with a wave-packet width growing as t{sup 1/4}.

  14. Bose-Einstein condensation of triplons in Ba3Cr2O8

    SciTech Connect (OSTI)

    Jaime, Marcelo [Los Alamos National Laboratory; Kohama, Y [Los Alamos National Laboratory; Aczel, A [MCMASTER UNIV; Ninios, K [UNIV OF FL; Chan, H [UNIV OF FL; Balicas, L [NHMFL; Dabkowska, H [MCMASTER UNIV; Like, G [MCMASTER UNIV

    2009-01-01

    By performing heat capacity, magnetocaloric effect, torque magnetometry and force magnetometry measurements up to 33 T, we have mapped out the T-H phase diagram of the S = 1/2 spin dimer compound Ba{sub 3}Cr{sub 2}O{sub 8}. We found evidence for field-induced magnetic order between H{sub cl} = 12.52(2) T and H{sub c2} = 23.65(5) T, with the maximum transition temperature T{sub c} {approx} 2.7 K at H {approx} 18 T. The lower transition can likely be described by Bose-Einstein condensation of triplons theory, and this is consistent with the absence of any magnetization plateaus in our magnetic torque and force measurements. In contrast, the nature of the upper phase transition appears to be quite different as our measurements suggest that this transition is actually first order.

  15. Vacuum energy in Einstein-Gauss-Bonnet anti-de Sitter gravity

    SciTech Connect (OSTI)

    Kofinas, Georgios; Olea, Rodrigo

    2006-10-15

    A finite action principle for Einstein-Gauss-Bonnet anti-de Sitter gravity is achieved by supplementing the bulk Lagrangian by a suitable boundary term, whose form substantially differs in odd and even dimensions. For even dimensions, this term is given by the boundary contribution in the Euler theorem with a coupling constant fixed, demanding the spacetime to have constant (negative) curvature in the asymptotic region. For odd dimensions, the action is stationary under a boundary condition on the variation of the extrinsic curvature. A well-posed variational principle leads to an appropriate definition of energy and other conserved quantities using the Noether theorem, and to a correct description of black hole thermodynamics. In particular, this procedure assigns a nonzero energy to anti-de Sitter spacetime in all odd dimensions.

  16. Phase dynamics after connection of two separate Bose-Einstein condensates

    SciTech Connect (OSTI)

    Zapata, I.; Sols, F.; Leggett, A.J.

    2003-02-01

    We study the dynamics of the relative phase following the connection of the two independently formed Bose-Einstein condensates. Dissipation is assumed to be due to the creation of quasiparticles induced by a fluctuating condensate particle number. The coherence between different values of the phase, which is characteristic of the initial Fock state, is quickly lost after the net exchange of a few atoms has taken place. This process effectively measures the phase and marks the onset of a semiclassical regime in which the system undergoes Bloch oscillations around the initial particle number. These fast oscillations excite quasiparticles within each condensate and the system relaxes at a longer time scale until it displays low-energy, damped, Josephson plasma oscillations, eventually coming to a halt when the equilibrium configuration is finally reached.

  17. EinsteinCartan gravity, Asymptotic Safety, and the running Immirzi parameter

    SciTech Connect (OSTI)

    Daum, J.-E.; Reuter, M.

    2013-07-15

    In this paper we analyze the functional renormalization group flow of quantum gravity on the EinsteinCartan theory space. The latter consists of all action functionals depending on the spin connection and the vielbein field (co-frame) which are invariant under both spacetime diffeomorphisms and local frame rotations. In the first part of the paper we develop a general methodology and corresponding calculational tools which can be used to analyze the flow equation for the pertinent effective average action for any truncation of this theory space. In the second part we apply it to a specific three-dimensional truncated theory space which is parametrized by Newtons constant, the cosmological constant, and the Immirzi parameter. A comprehensive analysis of their scale dependences is performed, and the possibility of defining an asymptotically safe theory on this hitherto unexplored theory space is investigated. In principle Asymptotic Safety of metric gravity (at least at the level of the effective average action) is neither necessary nor sufficient for Asymptotic Safety on the EinsteinCartan theory space which might accommodate different universality classes of microscopic quantum gravity theories. Nevertheless, we do find evidence for the existence of at least one non-Gaussian renormalization group fixed point which seems suitable for the Asymptotic Safety construction in a setting where the spin connection and the vielbein are the fundamental field variables. -- Highlights: A functional RG equation for a first order formulation of gravity is constructed. The theory space constituted by tetrad and spin connection variables is explored. The RG equation is solved in a 3 dimensional truncation of theory space. The flow of Newtons constant, the cosmological constant and the Immirzi parameter is analyzed. Evidence for the nonperturbative renormalizability of the theory is found.

  18. EMPIRICAL DETERMINATION OF EINSTEIN A-COEFFICIENT RATIOS OF BRIGHT [Fe II] LINES

    SciTech Connect (OSTI)

    Giannini, T.; Antoniucci, S.; Nisini, B.; Lorenzetti, D.; Alcal, J. M.; Bacciotti, F.; Podio, L.; Bonito, R.; Stelzer, B.

    2015-01-01

    The Einstein spontaneous rates (A-coefficients) of Fe{sup +} lines have been computed by several authors with results that differ from each other by up to 40%. Consequently, models for line emissivities suffer from uncertainties that in turn affect the determination of the physical conditions at the base of line excitation. We provide an empirical determination of the A-coefficient ratios of bright [Fe II] lines that would represent both a valid benchmark for theoretical computations and a reference for the physical interpretation of the observed lines. With the ESO-Very Large Telescope X-shooter instrument between 3000 and 24700 , we obtained a spectrum of the bright Herbig-Haro object HH1. We detect around 100 [Fe II] lines, some of which with a signal-to-noise ratios ?100. Among these latter lines, we selected those emitted by the same level, whose dereddened intensity ratios are direct functions of the Einstein A-coefficient ratios. From the same X-shooter spectrum, we got an accurate estimate of the extinction toward HH1 through intensity ratios of atomic species, H I recombination lines and H{sub 2} ro-vibrational transitions. We provide seven reliable A-coefficient ratios between bright [Fe II] lines, which are compared with the literature determinations. In particular, the A-coefficient ratios involving the brightest near-infrared lines (?12570/?16440 and ?13209/?16440) are in better agreement with the predictions by the Quinet et al. relativistic Hartree-Fock model. However, none of the theoretical models predict A-coefficient ratios in agreement with all of our determinations. We also show that literature data of near-infrared intensity ratios better agree with our determinations than with theoretical expectations.

  19. Distinguishing Between Site Waste, Natural, and Other Sources of Contamination at Uranium and Thorium Contaminated Sites - 12274

    SciTech Connect (OSTI)

    Hays, David C.

    2012-07-01

    Uranium and thorium processing and milling sites generate wastes (source, byproduct, or technically enhanced naturally occurring material), that contain contaminants that are similar to naturally occurring radioactive material deposits and other industry wastes. This can lead to mis-identification of other materials as Site wastes. A review of methods used by the US Army Corps of Engineers and the Environmental Protection Agency to distinguish Site wastes from potential other sources, enhanced materials, and natural deposits, at three different thorium mills was conducted. Real case examples demonstrate the importance of understanding the methods of distinguishing wastes. Distinguishing between Site wastes and enhanced Background material can be facilitated by establishing and applying a formal process. Significant project cost avoidance may be realized by distinguishing Site wastes from enhanced NORM. Collection of information on other potential sources of radioactive material and physical information related to the potential for other radioactive material sources should be gathered and reported in the Historical Site Assessment. At a minimum, locations of other such information should be recorded. Site decision makers should approach each Site area with the expectation that non site related radioactive material may be present and have a process in place to distinguish from Site and non Site related materials. (authors)

  20. Women @ Energy: Félicie Albert

    Broader source: Energy.gov [DOE]

    "... I do something unique, and that every day I learn something new and different. I do experiments using intense lasers, including the National Ignition Facility, the biggest laser in the world. I work with a lot of talented people on challenging problems. When you work really hard on designing an experiment, the excitement when you get your first data and see that it works is an amazing feeling."

  1. August 2016 Project Dashboard | Department of Energy

    Energy Savers [EERE]

    , 1939: Einstein's Letter August 2, 1939: Einstein's Letter August 2, 1939: Einstein's Letter August 2, 1939 Albert Einstein writes President Franklin D. Roosevelt, alerting the President to the importance of research on nuclear chain reactions and the possibility that research might lead to developing powerful bombs. Einstein notes that Germany has stopped the sale of uranium and German physicists are engaged in uranium research the DOE Direct Final Rule as it relates to efficiency standards

  2. Jefferson Lab hosts World Year of Physics guest speaker Erich Vogt

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

    discussing Einstein - the Person and His Legacy | Jefferson Lab World Year of Physics guest speaker Erich Vogt discussing Einstein - the Person and His Legacy Erich Vogt Jefferson Lab hosts World Year of Physics guest speaker Erich Vogt discussing Einstein - the Person and His Legacy October 4, 2005 In this celebratory year for physics, the world is marking the 100th anniversary of Albert Einstein's "miraculous" contributions to physics. A few people still remember Einstein in his

  3. Theory of Bose-Einstein condensation and superfluidity of two-dimensional polaritons in an in-plane harmonic potential

    SciTech Connect (OSTI)

    Berman, Oleg L.; Lozovik, Yurii E.; Snoke, David W.

    2008-04-15

    Recent experiments have shown that it is possible to create an in-plane harmonic potential trap for a two-dimensional (2D) gas of exciton polaritons in a microcavity structure, and evidence has been reported of Bose-Einstein condensation of polaritons accumulated in this type of trap. We present here the theory of Bose-Einstein condensation (BEC) and superfluidity of the exciton polaritons in a harmonic potential trap. Along the way, we determine a general method for defining the superfluid fraction in a 2D trap, in terms of angular momentum representation. We show that in the continuum limit, as the trap becomes shallower, the superfluid fraction approaches the 2D Kosterlitz-Thouless limit, while the condensate fraction approaches zero, as expected.

  4. Symmetries of Einstein's field equations with a perfect fluid source as examples of Lie--Baecklund symmetries

    SciTech Connect (OSTI)

    Stephani, H.

    1988-07-01

    The framework of Lie--Baecklund (or generalized) symmetries is used to give a unifying view of some of the known symmetries of Einstein's field equations for the vacuum or perfect fluid case (with a ..mu.. = p or a ..mu..+3p = 0 equation of state). These symmetries occur if space-time admits one or two Killing vectors (orthogonal or parallel, respectively, to the four-velocity in the perfect fluid case).

  5. Elementary excitations and universal interaction in Bose-Einstein condensates at large scattering lengths

    SciTech Connect (OSTI)

    Sarjonen, R.; Saarela, M.; Mazzanti, F.

    2011-10-15

    We present a theoretical analysis of excitation modes in Bose-Einstein condensates of ultracold alkali-metal gases for large scattering lengths, showing clear deviations from the Bogoliubov prediction as seen by Papp et al.[Phys. Rev. Lett. 101, 135301 (2008)]. We construct the atom-atom interaction by deriving the T matrix of such systems from two coupled (open and closed) channels assuming that the Feshbach resonance dominates the latter. We calculate molecular bound-state energies as a function of the magnetic field and compare with available experiments. The s-wave phase shifts determine the local effective interaction with long-ranged repulsion and short-ranged attraction. We show that it becomes a universal function at large scattering lengths. Finally, we use this interaction to characterize the ground-state and elementary excitations of {sup 85}Rb, {sup 87}Rb, and {sup 23}Na gases. Good agreement with line shift experiments in {sup 85}Rb is achieved. We find that, at large scattering lengths, Bragg scattering experiments could directly measure the momentum dependence of the effective two-body potential.

  6. Cranked Hartree-Fock-Bogoliubov calculation for rotating Bose-Einstein condensates

    SciTech Connect (OSTI)

    Hamamoto, Nobukuni; Oi, Makito; Onishi, Naoki

    2007-06-15

    A rotating bosonic many-body system in a harmonic trap is studied with the three-dimensional cranked Hartree-Fock-Bogoliubov method at zero temperature, which has been applied to nuclear many-body systems at high spin. This method is a variational method extended from Hartree-Fock theory, which can treat the pairing correlations in a self-consistent manner. An advantage of this method is that a finite-range interaction between constituent particles can be used in the calculation, unlike the original Gross-Pitaevskii approach. To demonstrate the validity of our method, we present a calculation for a toy model--that is, a rotating system of ten bosonic particles interacting through the repulsive quadrupole-quadrupole interaction in a harmonic trap. It is found that the yrast states, the lowest-energy states for the given total angular momentum, do not correspond to the Bose-Einstein condensate, except for a few special cases. One such case is a vortex state, which appears when the total angular momentum L is twice the particle number N (i.e., L=2N)

  7. Observing the shadow of Einstein-Maxwell-Dilaton-Axion black hole

    SciTech Connect (OSTI)

    Wei, Shao-Wen; Liu, Yu-Xiao E-mail: liuyx@lzu.edu.cn

    2013-11-01

    In this paper, the shadows cast by Einstein-Maxwell-Dilaton-Axion black hole and naked singularity are studied. The shadow of a rotating black hole is found to be a dark zone covered by a deformed circle. For a fixed value of the spin a, the size of the shadow decreases with the dilaton parameter b. The distortion of the shadow monotonically increases with b and takes its maximal when the black hole approaches to the extremal case. Due to the optical properties, the area of the black hole shadow is supposed to equal to the high-energy absorption cross section. Based on this assumption, the energy emission rate is investigated. For a naked singularity, the shadow has a dark arc and a dark spot or straight, and the corresponding observables are obtained. These results show that there is a significant effect of the spin a and dilaton parameter b on these shadows. Moreover, we examine the observables of the shadow cast by the supermassive black hole at the center of the Milky Way, which is very useful for us to probe the nature of the black hole through the astronomical observations in the near future.

  8. Thermodynamics of rotating solutions in (n+1)-dimensional Einstein-Maxwell-dilaton gravity

    SciTech Connect (OSTI)

    Sheykhi, A.; Riazi, N.; Pakravan, J.; Dehghani, M. H.

    2006-10-15

    We construct a class of charged, rotating solutions of (n+1)-dimensional Einstein-Maxwell-dilaton gravity with cylindrical or toroidal horizons in the presence of Liouville-type potentials and investigate their properties. These solutions are neither asymptotically flat nor (anti)-de Sitter. We find that these solutions can represent black brane, with inner and outer event horizons, an extreme black brane or a naked singularity provided the parameters of the solutions are chosen suitably. We also compute temperature, entropy, charge, electric potential, mass and angular momentum of the black brane solutions, and find that these quantities satisfy the first law of thermodynamics. We find a Smarr-type formula and perform a stability analysis by computing the heat capacity in the canonical ensemble. We find that the system is thermally stable when the coupling constant between the dilaton and matter field {alpha}{<=}1, while for {alpha}>1 the system has an unstable phase. This shows that the dilaton field makes the solution unstable, while it is stable even in Lovelock gravity.

  9. Matter wave switching in Bose-Einstein condensates via intensity redistribution soliton interactions

    SciTech Connect (OSTI)

    Rajendran, S.; Lakshmanan, M.; Muruganandam, P.

    2011-02-15

    Using time dependent nonlinear (s-wave scattering length) coupling between the components of a weakly interacting two component Bose-Einstein condensate (BEC), we show the possibility of matter wave switching (fraction of atoms transfer) between the components via shape changing/intensity redistribution (matter redistribution) soliton interactions. We investigate the exact bright-bright N-soliton solution of an effective one-dimensional (1D) two component BEC by suitably tailoring the trap potential, atomic scattering length, and atom gain or loss. In particular, we show that the effective 1D coupled Gross-Pitaevskii equations with time dependent parameters can be transformed into the well known completely integrable Manakov model described by coupled nonlinear Schroedinger equations by effecting a change of variables of the coordinates and the wave functions under certain conditions related to the time dependent parameters. We obtain the one-soliton solution and demonstrate the shape changing/matter redistribution interactions of two and three-soliton solutions for the time-independent expulsive harmonic trap potential, periodically modulated harmonic trap potential, and kinklike modulated harmonic trap potential. The standard elastic collision of solitons occur only for a specific choice of soliton parameters.

  10. Three-dimensional stationary cyclic symmetric Einstein-Maxwell solutions; black holes

    SciTech Connect (OSTI)

    Garcia, Alberto A.

    2009-09-15

    From a general metric for stationary cyclic symmetric gravitational fields coupled to Maxwell electromagnetic fields within the (2 + 1)-dimensional gravity the uniqueness of wide families of exact solutions is established. Among them, all uniform electromagnetic solutions possessing electromagnetic fields with vanishing covariant derivatives, all fields having constant electromagnetic invariants F{sub {mu}}{sub {nu}}F{sup {mu}}{sup {nu}} and T{sub {mu}}{sub {nu}}T{sup {mu}}{sup {nu}}, the whole classes of hybrid electromagnetic solutions, and also wide classes of stationary solutions are derived for a third-order nonlinear key equation. Certain of these families can be thought of as black hole solutions. For the most general set of Einstein-Maxwell equations, reducible to three nonlinear equations for the three unknown functions, two new classes of solutions - having anti-de Sitter spinning metric limit - are derived. The relationship of various families with those reported by different authors' solutions has been established. Among the classes of solutions with cosmological constant a relevant place is occupied by the electrostatic and magnetostatic Peldan solutions, the stationary uniform and spinning Clement classes, the constant electromagnetic invariant branches with the particular Kamata-Koikawa solution, the hybrid cyclic symmetric stationary black hole fields, and the non-less important solutions generated via SL(2,R)-transformations where the Clement spinning charged solution, the Martinez-Teitelboim-Zanelli black hole solution, and Dias-Lemos metric merit mention.