National Library of Energy BETA

Sample records for high school physics

  1. Secretary Chu Recalls Garden City High School Physics Teacher | Department

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

    of Energy Recalls Garden City High School Physics Teacher Secretary Chu Recalls Garden City High School Physics Teacher September 30, 2010 - 12:00am Addthis As part of President Obama's new initiative to recruit teachers, U.S. Energy Secretary Steven Chu is featured in a Public Service Announcement (PSA) video recalling how his high school physics teacher inspired him to pursue a career in science. In the PSA, Secretary Chu shares how his teacher, Mr. Thomas Miner, changed his approach to

  2. PPPL now offering SUMMER high school internship! | Princeton Plasma Physics

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

    Lab PPPL now offering SUMMER high school internship! April 3, 2015 Apply by May 30! The Princeton Plasma Physics Laboratory is pleased to announce that applications are now open for internships for high school rising seniors for the SUMMER of 2015! Please click here for more information.

  3. High School Semester-Long Internship | Princeton Plasma Physics Lab

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

    Semester-Long Internship Dr. Arturo Dominguez mentors a student on RGDX. Internship opportunities during the school year are avaialble for highly motivated high school students at PPPL! The spring internship application is open September 1 through November 30. The fall internship application is open February 1 through April 30. High School Semester Internship Application PPPL's Science Education department offers a limited number of internship positions for outstanding high school seniors

  4. High School Summer Internship | Princeton Plasma Physics Lab

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

    Summer Internship Internship opportunities for the summer of 2017 are available for highly motivated high school students at PPPL! High School Summer Internship Application - Applications are open Thanksgiving through January 31! PPPL's Science Education department offers a limited number of internship positions for outstanding high school graduating seniors during the summer. This paid internship offers students the chance to work on a project with a member of our research or engineering staff.

  5. 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-

  6. High Energy Physics

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

    High Energy Physics High Energy Physics Investigating the field of high energy physics ... Through the Office of High Energy Physics (HEP), Los Alamos conducts research in particle ...

  7. High School Internship Program

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

    High School Internship Program High School Internship Program Point your career towards Los Alamos Lab: work with the best minds on the planet in an inclusive environment that is rich in intellectual vitality and opportunities for growth. Contact Program Manager Scott Robbins Student Programs (505) 667-3639 Email Program Coordinator Brenda Montoya Student Programs (505) 667-4866 Email Opportunities for Northern New Mexico high school seniors The High School Internship Program provides qualified

  8. High School Science Bowl

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

    High School Science Bowl High School Science Bowl WHEN: Feb 07, 2015 8:00 AM - 4:00 PM WHERE: Highland High School 4700 Coal Ave SE, Albuquerque, USA CATEGORY: Community INTERNAL: Calendar Login Event Description The Science Bowl is a Jeopardy-like event for high school and middle school students who have a strong interest in mathematics and science. The competition is in the form of a round robin in the morning and double elimination after lunch. Teams consist of four students and one optional

  9. Students from Smoky Hill High School Triumph in Colorado High School

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

    Science Bowl - News Releases | NREL Students from Smoky Hill High School Triumph in Colorado High School Science Bowl February 11, 2006 Golden, Colo. - For the fifth year in a row, students from Smoky Hill High School won top honors at the Colorado High School Science Bowl. In the final round of rapid-fire questions and answers about physics, math, biology, astronomy, chemistry, computers and the earth sciences, Smoky Hill High School from Aurora was victorious over D'Evelyn High School from

  10. High energy physics

    SciTech Connect (OSTI)

    Kernan, A.; Shen, B.C.; Ma, E.

    1997-07-01

    This proposal is for the continuation of the High Energy Physics program at the University of California at Riverside. In hadron collider physics the authors will complete their transition from experiment UA1 at CERN to the DZERO experiment at Fermilab. On experiment UA1 their effort will concentrate on data analysis at Riverside. At Fermilab they will coordinate the high voltage system for all detector elements. They will also carry out hardware/software development for the D0 muon detector. The TPC/Two-Gamma experiment has completed its present phase of data-taking after accumulating 160 pb{sup {minus}}1 of luminosity. The UC Riverside group will continue data and physics analysis and make minor hardware improvement for the high luminosity run. The UC Riverside group is participating in design and implementation of the data acquisition system for the OPAL experiment at LEP. Mechanical and electronics construction of the OPAL hadron calorimeter strip readout system is proceeding on schedule. Data analysis and Monte Carlo detector simulation efforts are proceeding in preparation for the first physics run when IEP operation comenses in fall 1989.

  11. FSU High Energy Physics

    SciTech Connect (OSTI)

    Prosper, Harrison B.; Adams, Todd; Askew, Andrew; Berg, Bernd; Blessing, Susan K.; Okui, Takemichi; Owens, Joseph F.; Reina, Laura; Wahl, Horst D.

    2014-12-01

    The High Energy Physics group at Florida State University (FSU), which was established in 1958, is engaged in the study of the fundamental constituents of matter and the laws by which they interact. The group comprises theoretical and experimental physicists, who sometimes collaborate on projects of mutual interest. The report highlights the main recent achievements of the group. Significant, recent, achievements of the group’s theoretical physicists include progress in making precise predictions in the theory of the Higgs boson and its associated processes, and in the theoretical understanding of mathematical quantities called parton distribution functions that are related to the structure of composite particles such as the proton. These functions are needed to compare data from particle collisions, such as the proton-proton collisions at the CERN Large Hadron Collider (LHC), with theoretical predictions. The report also describes the progress in providing analogous functions for heavy nuclei, which find application in neutrino physics. The report highlights progress in understanding quantum field theory on a lattice of points in space and time (an area of study called lattice field theory), the progress in constructing several theories of potential new physics that can be tested at the LHC, and interesting new ideas in the theory of the inflationary expansion of the very early universe. The focus of the experimental physicists is the Compact Muon Solenoid (CMS) experiment at CERN. The report, however, also includes results from the D0 experiment at Fermilab to which the group made numerous contributions over a period of many years. The experimental group is particularly interested in looking for new physics at the LHC that may provide the necessary insight to extend the standard model (SM) of particle physics. Indeed, the search for new physics is the primary task of contemporary particle physics, one motivated by the need to explain certain facts, such as the

  12. Theoretical High Energy Physics

    SciTech Connect (OSTI)

    Christ, Norman H.; Weinberg, Erick J.

    2014-07-14

    we provide reports from each of the six faculty supported by the Department of Energy High Energy Physics Theory grant at Columbia University. Each is followed by a bibliography of the references cited. A complete list of all of the publications in the 12/1/2010-04/30/2014 period resulting from research supported by this grant is provided in the following section. The final section lists the Ph.D. dissertations based on research supported by the grant that were submitted during this period.

  13. High Energy Physics and Nuclear Physics Network Requirements...

    Office of Scientific and Technical Information (OSTI)

    Technical Report: High Energy Physics and Nuclear Physics Network Requirements Citation Details In-Document Search Title: High Energy Physics and Nuclear Physics Network ...

  14. Princeton High School and Grover Middle School Win Top Prizes at Regional

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

    Science Bowls | Princeton Plasma Physics Lab Princeton High School and Grover Middle School Win Top Prizes at Regional Science Bowls Princeton Plasma Physics Laboratory Hosts Competitions February 27, 2012 Tweet Widget Google Plus One Share on Facebook Thomas Grover Middle School took home the top prize Feb. 24 during the middle school Science Bowl® competition at the U.S. Department of Energy's Princeton Plasma Physics Laboratory (PPPL). Grover team members (from left) are Coach Rae

  15. High School Science Bowl | The Ames Laboratory

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

    High School Science Bowl January 28, 2017 A Competition Like No Other The Iowa Regional High School Science Bowl is an opportunity for Iowa's top science and math students to face-off in an intense question and answer format where contestants are quizzed on their knowledge of math and a range of science disciplines including biology, chemistry, Earth and space science, physics and energy. Iowa's Regional competition is hosted by the U.S. Department of Energy's Ames Laboratory and Iowa State

  16. High School football | Y-12 National Security Complex

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

    High School football High School football Fancy footwork at High School football practice

  17. High School Students Gear Up for Battle of the Brains

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

    Pueblo Pueblo Centennial High School Pueblo Central High School Pueblo South High School Other areas Granada High School - Granada Grand Junction High School - Grand Junction Lewis ...

  18. High Performance Schools Policy

    Broader source: Energy.gov [DOE]

    The Executive Order also requires that the New Jersey Economic Development Authority establish a subsidiary corporation, The New Jersey Schools Construction Corporation (SCC), to be responsible...

  19. Jefferson Lab hosts 19 schools for Virginia Regional High School...

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

    Feb. 10, to compete in the Virginia Regional High School Science Bowl. Nineteen teams, representing high schools from across the region are participating in this year's...

  20. High Energy Physics

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

    Administration | (NNSA) High Energy Density Laboratory Plasmas Program Steady advances in increasing the energy, power, and brightness of lasers and particle beams and advances in pulsed power systems have made possible the exploration of matter at extremely high energy density in the laboratory. Exciting new experimental regimes are being realized by exploiting the scientific capabilities of existing ICF Office facilities, as well as the relevant Department of Defense (DoD) and university

  1. Local High School Students Tour NERSC

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

    Local High School Students Tour NERSC Local High School Students Tour NERSC Outreach educates students about careers in scientific computing February 17, 2015 Oaktech-bashor.jpg...

  2. Theoretical High Energy Physics | Argonne National Laboratory

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

    Research Accelerator Technology ATLAS at the LHC Cosmology & Astrophysics Instrumentation Precision Muon Physics Neutrino Physics Theoretical High Energy Physics Theoretical High Energy Physics Theoretical High Energy Physics Much of the work of high-energy physics concentrates on the interplay between theory and experiment. The theory group of Argonne's High Energy Physics Division performs high-precision calculations of Standard Model processes, interprets experimental data in terms of

  3. West Windsor-Plainsboro South High School & William Annin Middle School

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

    Virginia win N.J. Regional Science Bowl at PPPL | Princeton Plasma Physics Lab

    West Windsor-Plainsboro South High School & William Annin Middle School win N.J. Regional Science Bowl at PPPL Top science whizzes will go to national contest in Washington, D.C. By Jeanne Jackson DeVoe February 23, 2016 Tweet Widget Google Plus One Share on Facebook The West Windsor-Plainsboro South High School team buzzes in an answer as they compete against Millburn High School in Round 12 of the New

  4. Mira Loma High School and Hopkins Junior High School from California...

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

    Junior High School from California Win U.S. Department of Energy National Science Bowl Mira Loma High School and Hopkins Junior High School from California Win U.S. Department of ...

  5. High Energy Physics Division, ANL Lattice QCD

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

    Energy Physics Division, ANL Lattice QCD in extreme environments D. K. Sinclair (HEP, Argonne) J. B. Kogut (Physics, Illinois) D. ... At large I and high temperature we observe ...

  6. Coal Study Guide - High School | Department of Energy

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

    High School Coal Study Guide - High School Coal Study Guide - High School (658.82 KB) More Documents & Publications Coal Study Guide - Middle School Coal Study Guide for Elementary School Fossil Energy Today - First Quarter, 2011

  7. Oklahoma Center for High Energy Physics (OCHEP)

    SciTech Connect (OSTI)

    S. Nandi; M.J. Strauss; J. Snow; F. Rizatdinova; B. Abbott; K. Babu; P. Gutierrez; C. Kao; A. Khanov; K.A. Milton; H. Neaman; H. Severini, P. Skubic

    2012-02-29

    areas ranging from the search for new phenomena at the Fermilab Tevatron and the CERN Large Hadron Collider to theoretical modeling, computer simulation, detector development and testing, and physics analysis. OCHEP faculty members participating on the D0 collaboration at the Fermilab Tevatron and on the ATLAS collaboration at the CERN LHC have made major impact on the Standard Model (SM) Higgs boson search, top quark studies, B physics studies, and measurements of Quantum Chromodynamics (QCD) phenomena. The OCHEP Grid computing facility consists of a large computer cluster which is playing a major role in data analysis and Monte Carlo productions for both the D0 and ATLAS experiments. Theoretical efforts are devoted to new ideas in Higgs bosons physics, extra dimensions, neutrino masses and oscillations, Grand Unified Theories, supersymmetric models, dark matter, and nonperturbative quantum field theory. Theory members are making major contributions to the understanding of phenomena being explored at the Tevatron and the LHC. They have proposed new models for Higgs bosons, and have suggested new signals for extra dimensions, and for the search of supersymmetric particles. During the seven year period when OCHEP was partially funded through the DOE EPSCoR implementation grant, OCHEP members published over 500 refereed journal articles and made over 200 invited presentations at major conferences. The Center is also involved in education and outreach activities by offering summer research programs for high school teachers and college students, and organizing summer workshops for high school teachers, sometimes coordinating with the Quarknet programs at OSU and OU. The details of the Center can be found in http://ochep.phy.okstate.edu.

  8. UPR/Mayaguez High Energy Physics

    SciTech Connect (OSTI)

    Mendez, Hector

    2014-10-31

    Puerto Rico-Rio Piedras (Carlos Malca). The students H. Moreno and C. Malca has been directly supervised by Dr. Mendez and S. Santiesteban supervised by Dr. Ramirez. During the last 13 years, our group have graduated 23 MS students on experimental High Energy Physics data analysis and applied hardware techniques. Most of the students have been supported by DOE grants, included this grant. Since 2001, Dr. Mendez have directly supervised eleven students, Dr. Ramirez three students and the former PI (Dr. Lopez) nine students. These theses work are fully documented in the group web page (http://charma.uprm.edu). The High Energy Physics group at Mayaguez is small and presently consists of three Physics faculty members, the Senior Investigators Dr. Hector Mendez (Professor) and Dr. Juan Eduardo Ramirez (Professor), and Dr. Sudhir Malik who was just hired in July 2014. Dr. Ramirez is in charge of the UPRM Tier-3 computing and will be building the network bandwidth infrastructure for the campus, while Dr. Mendez will continues his effort in finishing the heavy quark physics data analysis and moving to work on SUSY analysis for the 2015 data. Our last grant application in 2012 was awarded only for 2013-2014. As a result our postdoc position was lost last month of March. Since then, we have hired Dr. Malik as a new faculty in order to reinforce the group and to continue our efforts with the CMS experiment. Our plan is to hire another junior faculty in the next two years to strengthen the HEP group even further. Dr. Mendez continues with QuarkNet activities involving an ever larger group of high school physics teachers from all around Puerto Rico.

  9. Fossil Fuels Study Guide - High School | Department of Energy

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

    Fuels Study Guide - High School Fossil Fuels Study Guide - High School Fossil Fuels Study Guide - High School (63.66 KB) More Documents & Publications Coal Study Guide for ...

  10. Students from Pueblo Centennial High School Triumph in Colorado High School

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

    Science Bowl - News Releases | NREL Students from Pueblo Centennial High School Triumph in Colorado High School Science Bowl February 3, 2007 Photo of students holding a High School Science Bowl banner. (From left) Pueblo Centennial's Jesse Hovis, Lisa Marquez, Mitch Montoya, Meara Christian, Jay Mead (coach) and Benjamin Pacheco hold their trophy and banner after winning the 2007 High School Science Bowl at Dakota Ridge High School in Littleton, Colo. Students from Pueblo Centennial High

  11. National Nuclear Physics Summer School (NNPSS) 2011

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

    National Network for Manufacturing Innovation National Network for Manufacturing Innovation Image of Energy Department's Assistant Secretary David Danielson standing at podium speaking in front of workshop participants. The National Network for Manufacturing Innovation (NNMI) is an interagency initiative made up of public/private partnerships devoted to manufacturing excellence. Under the NNMI, each institute will bring together innovative manufacturers, university engineering schools, community

  12. Natural Gas Study Guide - High School | Department of Energy

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

    Natural Gas Study Guide - High School Natural Gas Study Guide - High School (434.33 KB) More Documents & Publications Natural Gas Study Guide - Middle School Fossil Fuels Study ...

  13. Energy Design Guidelines for High Performance Schools: Hot and...

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

    Design Guidelines for High Performance Schools: Hot and Humid Climates Energy Design Guidelines for High Performance Schools: Hot and Humid Climates School districts around the...

  14. High School Internship Program Recruitment Calendar

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

    Recruitment Calendar High School Internship Program Recruitment Calendar Point your career towards Los Alamos Lab: work with the best minds on the planet in an inclusive environment that is rich in intellectual vitality and opportunities for growth. Program Coordinator Brenda Montoya Student Programs (505) 667-4866 Email Local high school campus visits Winter-Spring 2016 "All visits have been completed for the 2016-2017 academic year." High school Contact Campus visit date Capital High

  15. High Energy Physics | Argonne National Laboratory

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

    Accelerator Technology Taking collider physics to higher energies More ATLAS at the LHC Colliding protons to learn about universal forces More Cosmology & Astrophysics Looking at the dawn and evolution of the universe More Instrumentation Innovative detectors for next-generation experiments More Precision Muon Physics Muons as a probe for new physics More Neutrino Physics Studying the elusive, but second most abundant particle in the universe More Theoretical High Energy Physics Motivating

  16. NREL: News - High School Students Gear Up for Battle of the Brains

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

    Eaglecrest High School (two teams) George Washington High School (two teams) Grand Junction High School Gunnison High School (two teams) Highlands Ranch High School (two ...

  17. High School Rules, Forms, and Resources | U.S. DOE Office of...

    Office of Science (SC) Website

    Resources National Science Bowl (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Strategies...

  18. News Media invited to cover Feb. 12 Virginia Regional High School Science

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

    Bowl at Jefferson Lab; 22 teams competing | Jefferson Lab Feb. 12 Virginia Regional High School Science Bowl at Jefferson Lab; 22 teams competing World Year of Physics News Media invited to cover Feb. 12 Virginia Regional High School Science Bowl at Jefferson Lab; 22 teams competing February 7, 2005 The Department of Energy's Jefferson Lab in Newport News, Va., is hosting this year's Virginia Regional High School Science Bowl on Saturday, Feb. 12. Twenty-two teams, representing high schools

  19. Local High School Students Tour NERSC

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

    Local High School Students Tour NERSC Local High School Students Tour NERSC Outreach educates students about careers in scientific computing February 17, 2015 Oaktech-bashor.jpg Jon Bashor, computing sciences' communications manager, gives students an inside look at supercomputing. Last week, two groups of students from East Bay high schools descended on the Oakland Scientific Facility to learn more about supercomputing and networking. On Wednesday, Feb. 11, 30 students from a computer science

  20. High School Co-op Program Recruitment Calendar

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

    Salazar Wed, Feb 18 Mesa Vista High School Mark Richmond TBD New Mexico School for the Arts Acacia McCombs Wed, Mar 4 Pecos High School Emily Ortiz Mon, Mar 2 Peasco High School...

  1. Precision Crystal Calorimeters in High Energy Physics

    ScienceCinema (OSTI)

    Ren-Yuan Zhu

    2010-01-08

    Precision crystal calorimeters traditionally play an important role in high energy physics experiments. In the last two decades, it faces a challenge to maintain its precision in a hostile radiation environment. This paper reviews the performance of crystal calorimeters constructed for high energy physics experiments and the progress achieved in understanding crystal?s radiation damage as well as in developing high quality scintillating crystals for particle physics. Potential applications of new generation scintillating crystals of high density and high light yield, such as LSO and LYSO, in particle physics experiments is also discussed.

  2. Mira Loma High School and Hopkins Junior High School from California Win

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

    U.S. Department of Energy National Science Bowl | Department of Energy Mira Loma High School and Hopkins Junior High School from California Win U.S. Department of Energy National Science Bowl Mira Loma High School and Hopkins Junior High School from California Win U.S. Department of Energy National Science Bowl May 4, 2009 - 12:00am Addthis WASHINGTON, DC - High school and middle school teams from California won the 2009 U.S. Department of Energy (DOE) National Science Bowl® today at the

  3. High School Students | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Students National Science Bowl (NSB) NSB Home About High School High School Students High School Coaches High School Regionals Middle School Attending the National Finals ...

  4. PARTICIPATION IN HIGH ENERGY PHYSICS

    SciTech Connect (OSTI)

    White, Christopher

    2012-12-20

    This grant funded experimental and theoretical activities in elementary particles physics at the Illinois Institute of Technology (IIT). The experiments in which IIT faculty collaborated included the Daya Bay Reactor Neutrino Experiment, the MINOS experiment, the Double Chooz experiment, and FNAL E871 - HyperCP experiment. Funds were used to support summer salary for faculty, salary for postdocs, and general support for graduate and undergraduate students. Funds were also used for travel expenses related to these projects and general supplies.

  5. High School Academic Competition - Double Elimination | U.S....

    Office of Science (SC) Website

    NSB Home About High School Middle School Attending National Event Volunteers 2015 ... School Double Elimination Top Teams for 2015 News Media WDTS Home Contact Information ...

  6. Thomas Jefferson High School for Science & Technology Wins...

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

    School, Richmond, Takes Second NEWPORT NEWS, Va., Feb. 27, 2010 - The Thomas Jefferson High School for Science and Technology from Alexandria beat out St. Christopher's School...

  7. High Energy Physics Research at Louisiana Tech

    SciTech Connect (OSTI)

    Sawyer, Lee; Greenwood, Zeno; Wobisch, Marcus

    2013-06-28

    The goal of this project was to create, maintain, and strengthen a world-class, nationally and internationally recognized experimental high energy physics group at Louisiana Tech University, focusing on research at the energy frontier of collider-based particle physics, first on the D� experiment and then with the ATLAS experiment, and providing leadership within the US high energy physics community in the areas of jet physics, top quark and charged Higgs decays involving tau leptons, as well as developing leadership in high performance computing.

  8. Computing in high-energy physics

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

    Mount, Richard P.

    2016-05-31

    I present a very personalized journey through more than three decades of computing for experimental high-energy physics, pointing out the enduring lessons that I learned. This is followed by a vision of how the computing environment will evolve in the coming ten years and the technical challenges that this will bring. I then address the scale and cost of high-energy physics software and examine the many current and future challenges, particularly those of management, funding and software-lifecycle management. Lastly, I describe recent developments aimed at improving the overall coherence of high-energy physics software.

  9. Research in High Energy Physics. Final report

    SciTech Connect (OSTI)

    Conway, John S.

    2013-08-09

    This final report details the work done from January 2010 until April 2013 in the area of experimental and theoretical high energy particle physics and cosmology at the University of California, Davis.

  10. High school interns opt for research over relaxation | Princeton Plasma

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

    Physics Lab High school interns opt for research over relaxation By Constance Kaita August 27, 2013 Tweet Widget Google Plus One Share on Facebook Rising senior Maya Moten from Somerset, N.J, left, and mentor Sophia Gershman, a research collaborator in the Science Education department, work on an experiment investigating small bright sparks in gas bubbles inside liquids to better understand the way fluids respond to high voltages. (Photo by Photo by Elle Starkman, PPPL Office of

  11. Oil Study Guide - High School | Department of Energy

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

    High School Oil Study Guide - High School Oil Study Guide - High School (602.29 KB) More Documents & Publications EIS-0165: DRAFT ENVIRONMENTAL IMPACT STATEMENT 2009 SPR Report to Congress Fossil Energy Today - First Quarter, 2012

  12. DC High School Science Bowl Regionals

    Broader source: Energy.gov [DOE]

    This event is the Washington, D.C. High School Regional competition for the US National Science Bowl. The regional competition is run by the Office of Economic Impact and Diversity, and the...

  13. AEC and Oak Ridge High School

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

    what happened. The Atomic Energy Commission spent 3,000,000 to build a new state- of-the-art high school in Oak Ridge in a very central and special location. This was done at a...

  14. About 900 High School Students, Educators Attend Third Annual...

    Energy Savers [EERE]

    About 900 High School Students, Educators Attend Third Annual DOE Science Alliance About 900 High School Students, Educators Attend Third Annual DOE Science Alliance September 28, ...

  15. Thomas Jefferson High School for Science & Technology National...

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

    Thomas Jefferson High School for Science & Technology National Science Bowl Champion Thomas Jefferson High School for Science & Technology National Science Bowl Champion May 2,...

  16. Modoc High School Space Heating Low Temperature Geothermal Facility...

    Open Energy Info (EERE)

    High School Space Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Modoc High School Space Heating Low Temperature Geothermal Facility Facility Modoc...

  17. Cedarville Elementary & High School Space Heating Low Temperature...

    Open Energy Info (EERE)

    Cedarville Elementary & High School Space Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Cedarville Elementary & High School Space Heating Low...

  18. Henley High School Space Heating Low Temperature Geothermal Facility...

    Open Energy Info (EERE)

    Henley High School Space Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Henley High School Space Heating Low Temperature Geothermal Facility Facility...

  19. Cotulla High School Space Heating Low Temperature Geothermal...

    Open Energy Info (EERE)

    Cotulla High School Space Heating Low Temperature Geothermal Facility Jump to: navigation, search Name Cotulla High School Space Heating Low Temperature Geothermal Facility...

  20. Spring high school internship application is open | Princeton...

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

    Spring high school internship application is open September 4, 2015 Apply by November 30 The application for PPPL's spring high school internship is open Click here for more...

  1. Watauga High School Wind Energy Project | Open Energy Information

    Open Energy Info (EERE)

    Energy Project Jump to: navigation, search Name Watauga High School Wind Energy Project Facility Watauga High School Sector Wind energy Facility Type Community Wind Facility Status...

  2. Thomas Jefferson High School takes regional Science Bowl competition...

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

    Science Bowl Results: Thomas Jefferson High School for Science and Technology The Thomas Jefferson High School for Science and Technology Science Bowl 2005 team includes (front...

  3. High energy physics at UC Riverside

    SciTech Connect (OSTI)

    1997-07-01

    This report discusses progress made for the following two tasks: experimental high energy physics, Task A, and theoretical high energy physics, Task B. Task A1 covers hadron collider physics. Information for Task A1 includes: personnel/talks/publications; D0: proton-antiproton interactions at 2 TeV; SDC: proton-proton interactions at 40 TeV; computing facilities; equipment needs; and budget notes. The physics program of Task A2 has been the systematic study of leptons and hadrons. Information covered for Task A2 includes: personnel/talks/publications; OPAL at LEP; OPAL at LEP200; CMS at LHC; the RD5 experiment; LSND at LAMPF; and budget notes. The research activities of the Theory Group are briefly discussed and a list of completed or published papers for this period is given.

  4. Advanced Analysis Methods in High Energy Physics

    SciTech Connect (OSTI)

    Pushpalatha C. Bhat

    2001-10-03

    During the coming decade, high energy physics experiments at the Fermilab Tevatron and around the globe will use very sophisticated equipment to record unprecedented amounts of data in the hope of making major discoveries that may unravel some of Nature's deepest mysteries. The discovery of the Higgs boson and signals of new physics may be around the corner. The use of advanced analysis techniques will be crucial in achieving these goals. The author discusses some of the novel methods of analysis that could prove to be particularly valuable for finding evidence of any new physics, for improving precision measurements and for exploring parameter spaces of theoretical models.

  5. High Energy Physics | Argonne National Laboratory

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

    News & Events Upcoming Events Press Releases Feature Stories In the News Videos Downloads About HEP at Work Career Opportunities Staff Directory About HEP at Work Career Opportunities Staff Directory Argonne National Laboratory High Energy Physics Research Facilities Capabilities Initiatives Publications News & Events Accelerator Technology Taking collider physics to higher energies More ATLAS at the LHC Colliding protons to learn about universal forces More Cosmology & Astrophysics

  6. Thomas Jefferson High School for Science & Technology Snaps Up...

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

    Beach Schools Take 2nd, 3rd Place High School Science Bowl 1st Place The Thomas Jefferson High School for Science and Technology team from Alexandria poses with its first-place...

  7. Discharge Physics of High Power Impulse Magnetron Sputtering...

    Office of Scientific and Technical Information (OSTI)

    Discharge Physics of High Power Impulse Magnetron Sputtering Citation Details In-Document Search Title: Discharge Physics of High Power Impulse Magnetron Sputtering High power ...

  8. COMPILATION OF CURRENT HIGH ENERGY PHYSICS EXPERIMENTS

    SciTech Connect (OSTI)

    Wohl, C.G.; Kelly, R.L.; Armstrong, F.E.; Horne, C.P.; Hutchinson, M.S.; Rittenberg, A.; Trippe, T.G.; Yost, G.P.; Addis, L.; Ward, C.E.W.; Baggett, N.; Goldschmidt-Clermong, Y.; Joos, P.; Gelfand, N.; Oyanagi, Y.; Grudtsin, S.N.; Ryabov, Yu.G.

    1981-05-01

    This is the fourth edition of our compilation of current high energy physics experiments. It is a collaborative effort of the Berkeley Particle Data Group, the SLAC library, and nine participating laboratories: Argonne (ANL), Brookhaven (BNL), CERN, DESY, Fermilab (FNAL), the Institute for Nuclear Study, Tokyo (INS), KEK, Serpukhov (SERP), and SLAC. The compilation includes summaries of all high energy physics experiments at the above laboratories that (1) were approved (and not subsequently withdrawn) before about April 1981, and (2) had not completed taking of data by 1 January 1977. We emphasize that only approved experiments are included.

  9. Indiana University High Energy Physics, Task A

    SciTech Connect (OSTI)

    Brabson, B.; Crittenden, R.; Dzierba, A.; Hanson, G.; Martin, H.; Marshall, T.; Mir, R.; Mouthuy, T.; Ogren, H.; Rust, D.; Teige, S.; Zieminska, D.; Zieminski, A.

    1991-01-01

    This report discusses research in High Energy Physics under the following experiments: Meson spectroscopy at BNL; dimuon production at FNAL; the DO collider experiment at FNAL; the Mark II experiment at SLC and PEP; the OPAL experiment at CERN; and the superconducting supercollider.

  10. Central High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Northwestern High School Wind Project

  11. Lewistown High Schools Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Northwestern High School Wind Project

  12. Luray High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Northwestern High School Wind Project

  13. Forest City High School Wind Farm | Open Energy Information

    Open Energy Info (EERE)

    High School Energy Purchaser Forest City Community School District Location Forest City IA Coordinates 43.266011, -93.653378 Show Map Loading map... "minzoom":false,"mappings...

  14. High School Academic Competition - Double Elimination | U.S....

    Office of Science (SC) Website

    Science Bowl Winners Past National Science Bowl Photos and Videos National Science Bowl Logos High School Middle School Attending National Event Volunteers 2015 Competition Results...

  15. Students from Smoky Hill High School Triumph in Colorado Science Bowl -

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

    News Releases | NREL Students from Smoky Hill High School Triumph in Colorado Science Bowl February 7, 2004 Golden, Colo. - Students from Smoky Hill High School won top honors today at the Colorado Science Bowl for the third year in a row. In the final round of rapid-fire questions and answers about physics, math, biology, astronomy, chemistry, computers and the earth sciences, Smoky Hill High School was victorious over Pueblo Centennial High School. Thirty-nine student teams from across the

  16. Students from Smoky Hill High School Triumph in Colorado Science Bowl -

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

    News Releases | NREL Students from Smoky Hill High School Triumph in Colorado Science Bowl February 12, 2005 Golden, Colo. - Students from Smoky Hill High School won top honors at the Colorado Science Bowl today for the fourth year in a row. In the final round of rapid-fire questions and answers about physics, math, biology, astronomy, chemistry, computers and the earth sciences, Smoky Hill High School team #2 from Aurora was victorious over Smoky Hill High School team #1. Thirty-six student

  17. Frontiers for Discovery in High Energy Density Physics

    SciTech Connect (OSTI)

    Davidson, R. C.; Katsouleas, T.; Arons, J.; Baring, M.; Deeney, C.; Di Mauro, L.; Ditmire, T.; Falcone, R.; Hammer, D.; Hill, W.; Jacak, B.; Joshi, C.; Lamb, F.; Lee, R.; Logan, B. G.; Melissinos, A.; Meyerhofer, D.; Mori, W.; Murnane, M.; Remington, B.; Rosner, R.; Schneider, D.; Silvera, I.; Stone, J.; Wilde, B.; Zajc. W.

    2004-07-20

    The report is intended to identify the compelling research opportunities of high intellectual value in high energy density physics. The opportunities for discovery include the broad scope of this highly interdisciplinary field that spans a wide range of physics areas including plasma physics, laser and particle beam physics, nuclear physics, astrophysics, atomic and molecular physics, materials science and condensed matter physics, intense radiation-matter interaction physics, fluid dynamics, and magnetohydrodynamics

  18. High School Co-op Program Salary Structure

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

    Salary Structure High School Co-op Program Salary Structure Point your career towards Los Alamos Lab: work with the best minds on the planet in an inclusive environment that is rich in intellectual vitality and opportunities for growth. Contact Student Programs (505) 667-4866 Email High school internship program salary structure Program Description Yearly Hourly High school intern High school senior $21,320/yr $10.25/hr Post HS graduate High school graduate (limited to 90-day appointment)

  19. Sandia California Regional Middle and High School Science Bowl winners |

    National Nuclear Security Administration (NNSA)

    National Nuclear Security Administration | (NNSA) Regional Middle and High School Science Bowl winners Thursday, March 3, 2016 - 2:00pm San Ramon's Dougherty Valley High School won the high school division for the third year in a row. More than 240 students and 48 teams competed in the Sandia California Regional Science Bowls at Las Positas College, in Livermore, California. Hopkins Junior High School (Fremont, California) and Dougherty Valley High School (San Ramon, California) defended

  20. Past High School National Science Bowl Winners (1991 - 2014)...

    Office of Science (SC) Website

    ... Team members: Nirjar (Juny) Sridhara, Tom Zavisca, Michael Hsia, Jay Moore, Lee Cochran, Hugh C. Smith (COACH) Prize: Trip to the International School of Physics in Sydney, ...

  1. High Technology School-to-Work Program at Argonne

    ScienceCinema (OSTI)

    None

    2013-04-19

    Argonne's High Technology School-to-Work Program for Chicago Public School Students. Supported by the Illinois Department of Commerce and Economic Opportunity, Chicago Public Schools, Argonne National Laboratory and the City of Chicago.

  2. Thomas Jefferson High School for Science & Technology Wins Virginia

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

    Regional Science Bowl; St. Christopher's School, Richmond, Takes Second | Jefferson Lab Wins Virginia Regional Science Bowl; St. Christopher's School, Richmond, Takes Second Thomas Jefferson High School for Science & Technology Wins Virginia Regional Science Bowl; St. Christopher's School, Richmond, Takes Second NEWPORT NEWS, Va., Feb. 27, 2010 - The Thomas Jefferson High School for Science and Technology from Alexandria beat out St. Christopher's School from Richmond, 54-44, in the

  3. West Windsor-Plainsboro High School South wins regional Science Bowl at

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

    PPPL | Princeton Plasma Physics Lab West Windsor-Plainsboro High School South wins regional Science Bowl at PPPL A dramatic ending to High School Bowl sends local team to nationals By Jeanne Jackson DeVoe February 25, 2013 Tweet Widget Google Plus One Share on Facebook Next stop Washington DC: Members of the West Windsor-Plainsboro High School South team pose after winning the New Jersey Regional Science Bowl at the Princeton Plasma Physics Laboratory on Feb. 23. From left to right: Coach

  4. Basic Research Needs for High Energy Density Laboratory Physics

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

    National Laboratory. Basic Research Needs for High Energy Density Laboratory Physics Report of the Workshop on High Energy Density Laboratory Physics Research Needs November ...

  5. Discharge Physics of High Power Impulse Magnetron Sputtering...

    Office of Scientific and Technical Information (OSTI)

    Discharge Physics of High Power Impulse Magnetron Sputtering Citation Details In-Document Search Title: Discharge Physics of High Power Impulse Magnetron Sputtering You are ...

  6. NERSC's Brian Friesen Helps Cray Surprise an Inquisitive High School

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

    Student NERSC's Brian Friesen Helps Cray Surprise an Inquisitive High School Student NERSC's Brian Friesen Helps Cray Surprise an Inquisitive High School Student May 23, 2016 friesenschoolsurprise Brian Friesen (second from left), Christy Adkinson (middle) and Hugo Villanueva (second from right) with school officials at the John F. Kennedy Middle College High School. Image: Cray About a month ago, Hugo Villanueva of John F. Kennedy Middle College High School in Southern California was trying

  7. Students from Smoky Hill High School Triumph in Colorado Science Bowl -

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

    News Releases | NREL Students from Smoky Hill High School Triumph in Colorado Science Bowl February 8, 2003 Golden, CO. - Students from Smoky Hill High School won top honors at the Colorado Science Bowl today at the Colorado School of Mines. In the final round of rapid-fire questions and answers about physics, math, biology, astronomy, chemistry, computers and the earth sciences, students from Smoky Hill High School team #2 were victorious over their peers, Smoky Hill team #3. At the end of

  8. High-precision arithmetic in mathematical physics

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

    Bailey, David H.; Borwein, Jonathan M.

    2015-05-12

    For many scientific calculations, particularly those involving empirical data, IEEE 32-bit floating-point arithmetic produces results of sufficient accuracy, while for other applications IEEE 64-bit floating-point is more appropriate. But for some very demanding applications, even higher levels of precision are often required. Furthermore, this article discusses the challenge of high-precision computation, in the context of mathematical physics, and highlights what facilities are required to support future computation, in light of emerging developments in computer architecture.

  9. High Energy Physics and Nuclear Physics Network Requirements

    SciTech Connect (OSTI)

    Dart, Eli; Bauerdick, Lothar; Bell, Greg; Ciuffo, Leandro; Dasu, Sridhara; Dattoria, Vince; De, Kaushik; Ernst, Michael; Finkelson, Dale; Gottleib, Steven; Gutsche, Oliver; Habib, Salman; Hoeche, Stefan; Hughes-Jones, Richard; Ibarra, Julio; Johnston, William; Kisner, Theodore; Kowalski, Andy; Lauret, Jerome; Luitz, Steffen; Mackenzie, Paul; Maguire, Chales; Metzger, Joe; Monga, Inder; Ng, Cho-Kuen; Nielsen, Jason; Price, Larry; Porter, Jeff; Purschke, Martin; Rai, Gulshan; Roser, Rob; Schram, Malachi; Tull, Craig; Watson, Chip; Zurawski, Jason

    2014-03-02

    The Energy Sciences Network (ESnet) is the primary provider of network connectivity for the U.S. Department of Energy (DOE) Office of Science (SC), the single largest supporter of basic research in the physical sciences in the United States. In support of SC programs, ESnet regularly updates and refreshes its understanding of the networking requirements needed by instruments, facilities, scientists, and science programs that it serves. This focus has helped ESnet to be a highly successful enabler of scientific discovery for over 25 years. In August 2013, ESnet and the DOE SC Offices of High Energy Physics (HEP) and Nuclear Physics (NP) organized a review to characterize the networking requirements of the programs funded by the HEP and NP program offices. Several key findings resulted from the review. Among them: 1. The Large Hadron Collider?s ATLAS (A Toroidal LHC Apparatus) and CMS (Compact Muon Solenoid) experiments are adopting remote input/output (I/O) as a core component of their data analysis infrastructure. This will significantly increase their demands on the network from both a reliability perspective and a performance perspective. 2. The Large Hadron Collider (LHC) experiments (particularly ATLAS and CMS) are working to integrate network awareness into the workflow systems that manage the large number of daily analysis jobs (1 million analysis jobs per day for ATLAS), which are an integral part of the experiments. Collaboration with networking organizations such as ESnet, and the consumption of performance data (e.g., from perfSONAR [PERformance Service Oriented Network monitoring Architecture]) are critical to the success of these efforts. 3. The international aspects of HEP and NP collaborations continue to expand. This includes the LHC experiments, the Relativistic Heavy Ion Collider (RHIC) experiments, the Belle II Collaboration, the Large Synoptic Survey Telescope (LSST), and others. The international nature of these collaborations makes them heavily

  10. Thomas Jefferson High School for Science & Technology Wins Feb...

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

    Warwick High Wins Math and Science Challenges Thomas Jefferson High School for Science & Technology Wins Feb. 5 Virginia Science Bowl; Warwick High Wins Math and Science ...

  11. Thomas Jefferson High School for Science & Technology wins...

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

    at the Virginia Regional High School Science Bowl was the team from the Thomas Jefferson High School for Science and Technology from Alexandria, Va. Pictured from left to right is...

  12. Virginia Regional High School Science Bowl | Jefferson Lab

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

    several high schools join the competition for the first time, and as the Thomas Jefferson High School for Science & Technology team, Alexandra, works to defend its six-year run as...

  13. UNIVERSITY OF ARIZONA HIGH ENERGY PHYSICS PROGRAM (Technical...

    Office of Scientific and Technical Information (OSTI)

    The High Energy Physics Group at the University of Arizona has conducted forefront research in elementary particle physics. Our theorists have developed new ideas in lattice QCD, ...

  14. Rube Goldberg 2013 - Hoffman Estates High School | Argonne National

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

    Laboratory Rube Goldberg 2013 - Hoffman Estates High School Share Topic Community Education Rube Goldberg Machine Contest

  15. Valley wins 2016 High School Science Bowl | The Ames Laboratory

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

    Valley wins 2016 High School Science Bowl Championship bracket results News Release First Place - Valley High School (from left) Coach Nathan Speichinger, Gabe Mintzer, Arjun Ganga, Guowei Qi, Jacob Bedia, Luke Rustin, Ames Laboratory Director Adam Schwartz. Second Place - Dubuque Wahlert High School Front (l-r) Natalie Hoy, Sam Hoelscher, Zoe Hermsen; back (l-r) Coach Tom Stierman, Andrew Wagner, Miguel Sanchez, Ames Laboratory Director Adam Schwartz. Third Place - Marshalltown High School

  16. Jefferson Lab hosts 19 schools for Virginia Regional High School Science

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

    Bowl on Feb. 10 | Jefferson Lab hosts 19 schools for Virginia Regional High School Science Bowl on Feb. 10 Jefferson Lab hosts 19 schools for Virginia Regional High School Science Bowl on Feb. 10 January 30, 2007 Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 10, to compete in the Virginia Regional High School Science Bowl. Nineteen teams, representing high schools from across the region are participating in this

  17. University of Oklahoma - High Energy Physics

    SciTech Connect (OSTI)

    Skubic, Patrick L.

    2013-07-31

    The High Energy Physics program at the University of Oklahoma, Pat Skubic, Principal Investigator, is attempting to understand nature at the deepest level using the most advanced experimental and theoretical tools. The four experimental faculty, Brad Abbott, Phil Gutierrez, Pat Skubic, and Mike Strauss, together with post-doctoral associates and graduate students, are finishing their work as part of the D0 collaboration at Fermilab, and increasingly focusing their investigations at the Large Hadron Collidor (LHC) as part of the ATLAS Collaboration. Work at the LHC has become even more exciting with the recent discovery by ATLAS and the other collaboration, CMS, of the long-sought Higgs boson, which plays a key role in generating masses for the elementary constituents of matter. Work of the OUHEP group has been in the three areas of hardware, software, and analysis. Now that the Higgs boson has been discovered, completing the Standard Model of fundamental physics, new efforts will focus on finding hints of physics beyond the standard model, such as supersymmetry. The OUHEP theory group (Kim Milton, PI) also consists of four faculty members, Howie Baer, Chung Kao, Kim Milton, and Yun Wang, and associated students and postdocs. They are involved in understanding fundamental issues in formulating theories of the microworld, and in proposing models that carry us past the Standard Model, which is an incomplete description of nature. They therefore work in close concert with their experimental colleagues. One also can study fundamental physics by looking at the large scale structure of the universe; in particular the ``dark energy'' that seems to be causing the universe to expand at an accelerating rate, effectively makes up about 3/4 of the energy in the universe, and yet is totally unidentified. Dark energy and dark matter, which together account for nearly all of the energy in the universe, are an important probe of fundamental physics at the very shortest distances

  18. SUPPORT FOR HU CFRT SUMMER HIGH SCHOOL FUSION WORKSHOP

    SciTech Connect (OSTI)

    Punjabi, Alkesh

    2010-02-09

    Nine summer fusion science research workshops for minority and female high school students were conducted at the Hampton University Center for Fusion Research and Training from 1996 to 2005. Each workshop was of the duration of eight weeks. In all 35 high school students were mentored. The students presented 28 contributed papers at the annual meetings of the American Physical Society Division of Plasma Physics. These contributed papers were very well received by the plasma physics and fusion science research community. The students won a number of prestigious local, state, and national honors, awards, prizes, and scholarships. The notable among these are the two regional finalist positions in the 1999 Siemens-Westinghouse Science and Technology Competitions; 1st Place U.S. Army Award, 2006; 1st Place U.S. Naval Science Award, 2006; Yale Science and Engineering Association Best 11th Grade Project, 2006; Society of Physics Students Book Award, 2006; APS Corporate Minority Scholarship and others. This workshop program conducted by the HU CFRT has been an exemplary success, and served the minority and female students exceptionally fruitfully. The Summer High School Fusion Science Workshop is an immensely successful outreach activity conducted by the HU CFRT. In this workshop, we train, motivate, and provide high quality research experiences to young and talented high school scholars with emphasis on under-represented minorities and female students in fusion science and related areas. The purpose of this workshop is to expose minority and female students to the excitement of research in science at an early stage in their academic lives. It is our hope that this may lead the high school students to pursue higher education and careers in physical sciences, mathematics, and perhaps in fusion science. To our knowledge, this workshop is the first and only one to date, of fusion science for under-represented minorities and female high school students at an HBCU. The faculty

  19. Southeastern Regional Vocational Technical High School | Open...

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  20. Students from Grand Junction High School Triumph in Colorado...

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

    Grand Junction High School Triumph in Colorado Science Bowl For more information contact: e:mail: Public Affairs Golden, Colo., Feb. 12, 2000 - Students from Grand Junction High ...

  1. High School Teams Compete in Science Bowl

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

    Teams from Across Colorado Compete in Science Bowl For more information contact: e:mail: Public Affairs Golden, Colo., Feb. 23, 1998 — On the surfaces of which three planets would you weigh more than you do on Earth? How many molecules are in two moles of sulfur trioxide? High school students from across Colorado will face such questions as they test their mental agility in the 1998 Colorado Science Bowl Feb. 28 at Metropolitan State College in Denver. More than 40 teams will compete in this

  2. Energy Design Guidelines for High Performance Schools: Tropical Island Climates

    SciTech Connect (OSTI)

    2004-11-01

    Design guidelines outline high performance principles for the new or retrofit design of K-12 schools in tropical island climates. By incorporating energy improvements into construction or renovation plans, schools can reduce energy consumption and costs.

  3. DOE SC Exascale Requirements Review: High Energy Physics

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

    Review: High Energy Physics Bethesda Hyatt, June 10, 2015 Jim Siegrist Associate Director for High Energy Physics Office of Science, U.S. Department of Energy HEP Computing and ...

  4. Lakewood High School Wins Colorado Science Bowl - News Releases | NREL

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

    Lakewood High School Wins Colorado Science Bowl Lakewood School Heads to Washington D.C. to Challenge for National Title January 26, 2013 Students from Lakewood High School Team 1 won the Colorado High School Science Bowl today. They will go on to the 23rd National Science Bowl in Washington D.C., Apr. 25-29, where they will compete for the national title against more than 400 students from 70 high schools. The U.S. Department of Energy (DOE) began the Science Bowl tradition in 1991 as a way to

  5. Fairview High School Wins Colorado Science Bowl - News Releases | NREL

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

    Fairview High School Wins Colorado Science Bowl Boulder School Heads to Washington D.C. to Challenge for National Title January 29, 2011 Golden, CO., Jan. 29, 2011 - Students from Fairview High School Team 1 won the Colorado High School Science Bowl today. They will go on to the 21st National Science Bowl in Washington D.C. on Apr. 28 - May 2, where they will compete for the national title against more than 450 students from 68 high schools. The U.S. Department of Energy (DOE) began the Science

  6. (The physics of highly charged ions)

    SciTech Connect (OSTI)

    Phaneuf, R.A.

    1990-10-12

    The Fifth International Conference on the Physics of Highly Charged Ions drew more than 200 participants, providing an excellent overview of this growing field. Important technical developments and experimental results in electron-ion collisions were reported. The merging of fast ion beams from accelerators or storage rings with advanced high-intensity electron-beam targets has yielded data of unprecedented quality on radiative and dielectronic recombination, providing stringent tests of theory. Long-awaited technical innovations in electron-impact excitation measurements were also reported. The level of activity in multicharged ion-surface interactions has increased. More sophisticated experimental studies of the neutralization process have shown the inadequacy of previously accepted mechanisms, and theoretical activity in this area is just being initiated. The IAEA meetings addressed atomic and molecular data needs for fusion research, with ITER providing a key focus. Such data are especially critical to modeling and diagnostics of the edge plasma. The ALADDIN data base system has been universally accepted and has streamlined the exchange of numerical data among data centers and the fusion community. The IAEA continues to play a pivotal role in the identification of data needs, and in the coordination of data compilation and research activities for fusion applications.

  7. Category:Wind for Schools High School Curricula | Open Energy...

    Open Energy Info (EERE)

    School Curricula" The following 39 files are in this category, out of 39 total. Air Density Lab.pdf Air Density Lab.pdf 240 KB Anemometer activity.docx Anemometer activity.docx...

  8. West Windsor-Plainsboro High School South wins regional Science Bowl at

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

    PPPL | Princeton Plasma Physics Lab West Windsor-Plainsboro High School South wins regional Science Bowl at PPPL By Jeanne Jackson DeVoe February 25, 2013 Tweet Widget Google Plus One Share on Facebook Next stop Washington DC: Members of the West Windsor-Plainsboro High School South team pose after winning the New Jersey Regional Science Bowl at the Princeton Plasma Physics Laboratory on Feb. 23. From left to right: Coach Sunila Sharma, Arnav Sood, Chaitanya Asawa, Team Captain Alexander

  9. UPR/Mayaguez High Energy Physics

    SciTech Connect (OSTI)

    López, Angel M.

    2015-10-27

    For the period of sixteen years covered by this report (June 1, 1997 - July 31, 2013) the High Energy Physics Group at the University of Puerto Rico’s Mayaguez Campus (UPRM) carried out an extensive research program that included major experiments at Fermi National Accelerator Laboratory (Fermilab), the Cornell Electron-positron Collider and CERN. In particular, these were E831 (FOCUS) at Fermilab, CLEOc at Cornell and the Compact Muon Solenoid (CMS) at the Large Hadron Collider (LHC) at CERN. The group’s history is one of successful execution and growth. Beginning with one faculty researcher in 1985, it eventually included four faculty researchers, one post-doctoral research associate, two undergraduates and as many as six graduate students at one time working on one of the experiments that discovered the Higgs boson. Some of this expansion was due to the group’s leveraging of funds from the Department of Energy’s core grant to attract funds from National Science Foundation programs not targeted to high energy physics. Besides the group’s research productivity, its other major contribution was the training of a large number of MS students who later went on to successful technical careers in industry as well as academia including many who obtained PhD degrees at US universities. In an attempt to document this history, this final report gives a general description of the Group’s work prior to June 1, 2010, the starting date for the last grant renewal period. Much more detail can, of course, be found in the annual reports submitted up to that date. The work during the last grant period is discussed in detail in a separate section. To summarize the group’s scientific accomplishments, one can point to the results of the experiments. Both FOCUS and CLEOc were designed to carry out precise measurements of processes involving the heavy quarks, charm and bottom. Heavy quarks are particularly interesting because, due to their mass, theoretical calculations

  10. High School Students Gear Up for Battle of the Brains - News Releases |

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

    NREL High School Students Gear Up for Battle of the Brains February 6, 2006 Golden, Colo. - The next generation of scientists, mathematicians and engineers will test their mental agility in the U.S. Department of Energy's (DOE) Colorado Science Bowl on Feb. 11 at the Colorado School of Mines in Golden. Forty teams from across Colorado will compete in this rapid-fire question-and-answer tournament, which focuses on physics, math, biology, astronomy, chemistry, computers, general science and

  11. Media Advisory - Virginia Regional High School Science Bowl | Jefferson Lab

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

    High School Science Bowl Media Advisory - Virginia Regional High School Science Bowl What: Virginia Regional High School Science Bowl When: Saturday, Feb. 1, 2014. Round robin competition runs from 9 a.m. - noon. The double elimination, semi-final and finalist rounds run from 1:30 - ~ 5 p.m. Awards presentations will be made immediately after the final round. Where: CEBAF Center Auditorium, Thomas Jefferson National Accelerator Facility, 12000 Jefferson Avenue, Newport News, Va. 23606 Details:

  12. Lakewood High School Teacher Recognized for Introduction of Renewable

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

    Energy Curriculum - News Releases | NREL Lakewood High School Teacher Recognized for Introduction of Renewable Energy Curriculum November 17, 2005 Golden, Colo. - Students taking technology classes at Lakewood High School this semester are learning about more than construction, technical theater and computer aided drafting (CAD); they are learning about energy issues within their community. Matthew Brown, technology teacher at Lakewood High School, started a new course this year that

  13. Research Projects in Renewable Energy for High School Student

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

    PROJECTS IN RENEWABLE ENERGY FOR HIGH SCHOOL STUDENTS National Renewable Energy Laboratory Education Programs 1617 Cole Blvd. Golden, CO 80401 Tel: (303) 275-3044 Home page: http:...

  14. High School Students Gear Up for Battle of the Brains

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

    Students from Grand Junction High School placed first in last year's regional competition. DOE began the National Science Bowl 11 years ago to help stimulate interest in science ...

  15. University of Denver High School Teacher Recognized for Commitment...

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

    University of Denver High School (DUHS), walks the talk when it comes to sustainability. ... renewable energy and for being an advocate of sustainability in the community. ...

  16. Video: Mira Loma High School Named Science Bowl Grand Champion

    Broader source: Energy.gov [DOE]

    Today, Mira Loma High School won the 2014 National Science Bowl at the National Building Museum in Washington, D.C.

  17. Thomas Jefferson High School for Science & Technology wins...

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

    Regional Science Bowl. Winning the daylong academic competition was the Thomas Jefferson High School for Science and Technology, from Alexandria, Va. Following in second place was...

  18. DOE SC Exascale Requirements Review: High Energy Physics

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

    SC Exascale Requirements Review: High Energy Physics Bethesda Hyatt, June 10, 2015 Jim Siegrist Associate Director for High Energy Physics Office of Science, U.S. Department of Energy HEP Computing and Data Challenges * What's new? * In May 2014, the U.S. particle physics community updated its vision for the future - The P5 (Particle Physics Project Prioritization Panel) report presents a strategy for the next decade and beyond that enables discovery and maintains our position as a global leader

  19. DOE - NNSA/NFO -- Nevada Science Bowl - HIGH SCHOOL

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

    High School NNSA/NFO Language Options U.S. DOE/NNSA - Nevada Field Office Nevada Science Bowl - High School February 3-4, 2017 On behalf of the National Nuclear Security Administration Nevada Field Office (NNSA/NFO), we are pleased to announce the 2017 Nevada Science Bowl for high school competition will take place February 3-4, 2017 at the National Atomic Testing Museum (NATM) and Vegas PBS. We would be honored to have your school field a team for this event. REGISTRATION INFORMATION

  20. DOE - NNSA/NFO -- Science Bowl - High School Registration

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

    Nevada High School Science Bowl Registration NNSA/NFO Language Options U.S. DOE/NNSA - Nevada Field Office Welcome to the 26th Annual Nevada High School Science Bowl! February 3-4, 2017 Registration is due on December 14, 2016 Thirty-two teams from high schools in California, Nevada, and Utah are welcome to participate in this round robin - double-elimination competition. Monetary awards are given to the first through ninth place teams for use in their school's mathematics/science departments.

  1. Large Scale Computing and Storage Requirements for High Energy Physics

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

    Large Scale Computing and Storage Requirements for High Energy Physics HEPFrontcover.png Large Scale Computing and Storage Requirements for High Energy Physics An HEP / ASCR / NERSC Workshop November 12-13, 2009 Report Large Scale Computing and Storage Requirements for High Energy Physics, Report of the Joint HEP / ASCR / NERSC Workshop conducted Nov. 12-13, 2009 https://www.nersc.gov/assets/HPC-Requirements-for-Science/HEPFrontcover.png Goals This workshop was organized by the Department of

  2. DOE New Jersey Regional High School Science Bowl *NO LECTURE* | Princeton

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

    Plasma Physics Lab 1, 2015, 9:00am to 4:00pm Science Education Lab-wide DOE New Jersey Regional High School Science Bowl *NO LECTURE* Contact Information Coordinator(s): Deedee Ortiz-Arias, Science Education Department Program Administraor dortiz@ppl.gov Host(s): Dr. Andrew Zwicker, Science Education Department Head azwicker@pppl.gov

  3. DOE New Jersey Regional High School Science Bowl! NO SCIENCE ON SATURDAY

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

    LECTURE | Princeton Plasma Physics Lab 2, 2014 (All day) Science On Saturday DOE New Jersey Regional High School Science Bowl! NO SCIENCE ON SATURDAY LECTURE DUE TO THE NEW JERSEY REGIONAL SCIENCE BOWL COMPETITION, THERE WILL BE NO SCIENCE ON SATURDAY LECTURE TODAY.

  4. High energy physics advisory panel`s subpanel on vision for the future of high-energy physics

    SciTech Connect (OSTI)

    Not Available

    1994-05-01

    This report was requested by the Secretary of Energy to (1) define a long-term program for pursuing the most important high-energy physics goals since the termination of the Superconducting Super Collider (SSC) project, (2) assess the current US high-energy physics program, and (3) make recommendations regarding the future of the field. Subjects on which recommendations were sought and which the report addresses were: high-energy physics funding priorities; facilitating international collaboration for future construction of large high-energy physics facilities; optimizing uses of the investment made in the SSC; how to encourage displaced scientists and engineers to remain in high-energy physics and to attract young scientists to enter the field in the future. The report includes a description of the state of high-energy physics research in the context of history, a summary of the SSC project, and documentation of the report`s own origins and development.

  5. Energy Design Guidelines for High Performance Schools: Arctic and Subarctic Climates

    SciTech Connect (OSTI)

    2004-11-01

    Energy Design Guidelines for High Performance Schools book detailing DOE's EnergySmart Schools Program for Arctic Climates.

  6. NJ Regional Middle School Science Bowl | Princeton Plasma Physics...

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

    competition in Washington, D.C. The Science Bowl is a double elimination contest with oral question and answer rounds in the fields of chemistry, biology, physics, astronomy and...

  7. High Performance Green Schools Planning Grants

    Broader source: Energy.gov [DOE]

    In addition to planning grant opportunities, the Department of Education offers an additional reimbursement to schools that build or renovate to LEED silver or higher, or achieve two or more...

  8. Participation in High Energy Physics at the University of Chicago

    SciTech Connect (OSTI)

    Martinec, Emil J.

    2013-06-27

    This report covers research at the University of Chicago in theoretical high energy physics and its connections to cosmology, over the period Nov. 1, 2009 to April 30, 2013. This research is divided broadly into two tasks: Task A, which covers a broad array of topics in high energy physics; and task C, primarily concerned with cosmology.

  9. High Energy Physics Organization Chart | Argonne National Laboratory

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

    Career Opportunities Staff Directory About HEP at Work Career Opportunities Staff Directory Argonne National Laboratory High Energy Physics Research Facilities Capabilities Initiatives Publications News & Events News & Events Upcoming Events Press Releases Feature Stories In the News Videos Downloads High Energy Physics Organization Chart PDF icon Org Chart 08-04-16.pdf

  10. Princeton University High Energy Physics Research

    SciTech Connect (OSTI)

    Marlow, Daniel R.

    2015-06-30

    This is the Final Report on research conducted by the Princeton Elementary Particles group over the approximately three-year period from May 1, 2012 to April 30, 2015. The goal of our research is to investigate the fundamental constituents of matter, their fields, and their interactions; to understand the properties of space and time; and to study the profound relationships between cosmology and particle physics. During the funding period covered by this report, the group has been organized into a subgroup concentrating on the theory of particles, strings, and cosmology; and four subgroups performing major experiments at laboratories around the world: CERN, Daya Bay, Gran Sasso as well as detector R\\&D on the Princeton campus. Highlights in of this research include the discovery of the Higgs Boson at CERN and the measurement of $\\sin^22\\theta_{13}$ by the Daya Bay experiment. In both cases, Princeton researchers supported by this grant played key roles.

  11. High energy physics in cosmic rays

    SciTech Connect (OSTI)

    Jones, Lawrence W.

    2013-02-07

    In the first half-century of cosmic ray physics, the primary research focus was on elementary particles; the positron, pi-mesons, mu-mesons, and hyperons were discovered in cosmic rays. Much of this research was carried out at mountain elevations; Pic du Midi in the Pyrenees, Mt. Chacaltaya in Bolivia, and Mt. Evans/Echo Lake in Colorado, among other sites. In the 1960s, claims of the observation of free quarks, and satellite measurements of a significant rise in p-p cross sections, plus the delay in initiating accelerator construction programs for energies above 100 GeV, motivated the Michigan-Wisconsin group to undertake a serious cosmic ray program at Echo Lake. Subsequently, with the succession of higher energy accelerators and colliders at CERN and Fermilab, cosmic ray research has increasingly focused on cosmology and astrophysics, although some groups continue to study cosmic ray particle interactions in emulsion chambers.

  12. 2016 Middle School Science Bowl | Princeton Plasma Physics Lab

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

    Middle School Science Bowl View larger image 16 PR 0219 271 View larger image 16 PR 0220 090 View larger image MSSci Bowl Winner William Annin 1 F View larger image Princeton Charter 264 View larger image Princeton Charter 278 View larger image Princeton Charter Witherspoon 229 View larger image Second Place Princeton Charter 313 View larger image Third Place Witherspoon 312 View larger image William Annin 261 View larger image 16 PR 0219 037 View larger image 16 PR 0219 072 View larger image 16

  13. Thomas Jefferson High School for Science & Technology National Science

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

    Bowl® Champion | Department of Energy Thomas Jefferson High School for Science & Technology National Science Bowl® Champion Thomas Jefferson High School for Science & Technology National Science Bowl® Champion May 2, 2005 - 12:40pm Addthis WASHINGTON, DC -- "The Incompleteness Theorem" was the answer to a question on mathematics that today clinched the 2005 National Science Bowl® championship for the Thomas Jefferson High School for Science & Technology team from

  14. Tabu search techniques for large high-school timetabling problems

    SciTech Connect (OSTI)

    Schaerf, A.

    1996-12-31

    The high-school timetabling problem consists in assigning all the lectures of a high school to the time periods in such a way that no teacher (or class) is involved in more than one lecture at a time and other side constraints are satisfied. The problem is NP-complete and is usually tackled using heuristic methods. This paper describes a solution algorithm (and its implementation) based on Tabu Search. The algorithm interleaves different types of moves and makes use of an adaptive relaxation of the hard constraints. The implementation of the algorithm has been successfully experimented in some large high schools with various kinds of side constraints.

  15. Atomic physics with highly charged ions

    SciTech Connect (OSTI)

    Richard, P.

    1991-08-01

    This report discusses: One electron outer shell processes in fast ion-atom collisions; role of electron-electron interaction in two-electron processes; multi-electron processes at low energy; multi-electron processes at high energy; inner shell processes; molecular fragmentation studies; theory; and, JRM laboratory operations.

  16. New high power linacs and beam physics

    SciTech Connect (OSTI)

    Wangler, T.P.; Gray, E.R.; Nath, S.; Crandall, K.R.; Hasegawa, K.

    1997-08-01

    New high-power proton linacs must be designed to control beam loss, which can lead to radioactivation of the accelerator. The threat of beam loss is increased significantly by the formation of beam halo. Numerical simulation studies have identified the space-charge interactions, especially those that occur in rms mismatched beams, as a major concern for halo growth. The maximum-amplitude predictions of the simulation codes must be subjected to independent tests to confirm the validity of the results. Consequently, the authors compare predictions from the particle-core halo models with computer simulations to test their understanding of the halo mechanisms that are incorporated in the computer codes. They present and discuss scaling laws that provide guidance for high-power linac design.

  17. Precision Timing Calorimeter for High Energy Physics

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

    Anderson, Dustin; Apresyan, Artur; Bornheim, Adolf; Duarte, Javier; Pena, Cristian; Ronzhin, Anatoly; Spiropulu, Maria; Trevor, Jason; Xie, Si

    2016-04-01

    Here, we present studies on the performance and characterization of the time resolution of LYSO-based calorimeters. Results for an LYSO sampling calorimeter and an LYSO-tungsten Shashlik calorimeter are presented. We also demonstrate that a time resolution of 30 ps is achievable for the LYSO sampling calorimeter. Timing calorimetry is described as a tool for mitigating the effects due to the large number of simultaneous interactions in the high luminosity environment foreseen for the Large Hadron Collider.

  18. Fourth International Conference on High Energy Density Physics

    SciTech Connect (OSTI)

    Beg, Farhat

    2015-01-06

    The Fourth International Conference on High Energy Density Physics (ICHED 2013) was held in Saint Malo, France, at the Palais du Grand Large on 25-28 June 2013 (http://web.luli.polytechnique.fr/ICHED2013/). This meeting was the fourth in a series which was first held in 2008. This conference covered all the important aspects of High Energy Density Physics including fundamental topics from strong-field physics to creating new states of matter (including radiation-dominated, high-pressure quantum and relativistic plasmas) and ultra-fast lattice dynamics on the timescale of atomic transitions.

  19. Daniel Wright Junior High School Wins First Place In Hydrogen...

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

    Daniel Wright Junior High School Wins First Place In Hydrogen Fuel Cell Car Contest National "Battle of the Brains" continues June 23-24 at the University of Denver June 23, 2006 ...

  20. Alternative Fuels Data Center: Missouri High School Students...

    Alternative Fuels and Advanced Vehicles Data Center [Office of Energy Efficiency and Renewable Energy (EERE)]

    Missouri High School Students Get Hands-On Training With Biodiesel See how students in Fenton, Missouri, are learning to convert waste vegetable oil into biodiesel and put it into ...

  1. High School Co-op Program Salary Structure

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

    Salary Structure High School Co-op Program Salary Structure Point your career towards Los Alamos Lab: work with the best minds on the planet in an inclusive environment that is...

  2. Secretary Chu Announces Middle and High School Finalists Set...

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

    in the 2012 National Science Bowl in Washington, D.C. Secretary Chu Announces Middle and High School Finalists Set to Compete in the 2012 National Science Bowl in Washington, ...

  3. West Windsor-Plainsboro South High School & William Annin...

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

    ... More information is available on the NSB website: http:www.science.energy.govwdtsnsb. The contest brought 32 high school teams to PPPL from as far away as Brooklyn and ...

  4. Sandia Energy - Successful Conclusion of SSLS EFRC's High School...

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

    were between their junior and senior years of high school, and had strong backgrounds math and science. Our interns participated in a wide range of activities: ES&H courses,...

  5. JCESR introduces high school students to the future of battery...

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

    JCESR introduces high school students to the future of battery science By Robyn Henderson ... of energy storage and how battery science is improving our world both today and tomorrow. ...

  6. Southeastern visits local high school | Department of Energy

    Energy Savers [EERE]

    Southeastern visits local high school Southeastern visits local high school May 10, 2013 - 11:54am Addthis Southeastern employee, Dale Jett, uses a power system mockup to explain how power is distributed to homes. Southeastern employee, Dale Jett, uses a power system mockup to explain how power is distributed to homes. Southeastern employee, Sonya Hulme, describes the Power Marketing Administations and the ares that each one supports. Southeastern employee, Sonya Hulme, describes the Power

  7. Media Advisory - Virginia Regional High School Science Bowl | Jefferson Lab

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

    27, 2010. Round robin competition runs from 9 a.m. - noon. The double elimination, semi-final and finalist rounds run from 1:30 - 5 p.m. Awards presentations will be made immediately after the final round. Where: CEBAF Center Auditorium, Thomas Jefferson National Accelerator Facility, 12000 Jefferson Avenue, Newport News, Va. Details: Twenty teams, representing high schools from across the state are participating in this annual, academic competition. Catch the excitement as several high schools

  8. Thomas Jefferson High School for Science & Technology wins Virginia

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

    Regional Science Bowl | Jefferson Lab wins Virginia Regional Science Bowl Thomas Jefferson High School for Science & Technology wins Virginia Regional Science Bowl February 8, 2003 Hundreds of the brightest young minds in the commonwealth came together at the Department of Energy's Jefferson Lab today to compete in the Virginia Regional Science Bowl. Winning the daylong academic competition was the Thomas Jefferson High School for Science and Technology, from Alexandria, Va. Following in

  9. Thomas Jefferson High School for Science and Technology from Alexandria

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

    Wins 2002 Virginia Regional Science Bowl | Jefferson Lab and Technology from Alexandria Wins 2002 Virginia Regional Science Bowl Thomas Jefferson High School for Science and Technology from Alexandria Wins 2002 Virginia Regional Science Bowl February 14, 2002 NEWPORT NEWS, VA - Some of the brightest young minds in the state came together at Jefferson Lab on Saturday, Feb. 9, to compete in the Virginia Regional Science Bowl. Twenty teams, representing high schools from across the Commonwealth

  10. Thomas Jefferson High School takes regional Science Bowl competition at

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

    JLab for 4th year running | Jefferson Lab takes regional Science Bowl competition at JLab for 4th year running Science Bowl Results: Thomas Jefferson High School for Science and Technology The Thomas Jefferson High School for Science and Technology Science Bowl 2005 team includes (front row, left to right): Coach Sharon Baker, Charlotte Seid, Sam Lederer and Lisa Marrone, and (back row, l. to r.): Matthew Isakowitz and Logan Kearsley. Photos by Steve Gagnon, JLab Science Education Thomas

  11. Hotchkiss High School Seniors Recognized for Renewable Energy Project -

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

    News Releases | NREL Hotchkiss High School Seniors Recognized for Renewable Energy Project April 10, 2006 Golden, Colo. - The U.S. Department of Energy's National Renewable Energy Laboratory (NREL) presented a special Renewable Energy Award to Christopher Snow and Alexander Farinell from Hotchkiss High School, Hotchkiss, Colo., at the 51st Colorado Science and Engineering Fair (CSEF) on April 6. The award is sponsored by NREL's corporate partners, Midwest Research Institute (MRI) and

  12. Conference shows high school girls their scientific future | Argonne

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

    National Laboratory J'Tia Taylor (left), a nonproliferation technical specialist in Argonne's Nuclear Engineering Division, speaks with event attendees. Click to enlarge. J'Tia Taylor (left), a nonproliferation technical specialist in Argonne's Nuclear Engineering Division, speaks with event attendees. Click to enlarge. Conference shows high school girls their scientific future By Justin H.S. Breaux * April 7, 2014 Tweet EmailPrint ARGONNE, Ill. - Nearly 400 high school girls from the

  13. Final Report. Research in Theoretical High Energy Physics

    SciTech Connect (OSTI)

    Greensite, Jeffrey P.; Golterman, Maarten F.L.

    2015-04-30

    Grant-supported research in theoretical high-energy physics, conducted in the period 1992-2015 is briefly described, and a full listing of published articles result from those research activities is supplied.

  14. We Have a Winner - DC High School Regional Science Bowl Competition...

    Office of Environmental Management (EM)

    We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday ...

  15. Poudre High School From Fort Collins , Colorado Wins U.S. Department...

    Energy Savers [EERE]

    ... East Brunswick, New Jersey Edwin O. Smith High School, Storrs, Connecticut Homestead ... North Dakota Southside High School, Fort Smith, Arkansas Texas Academy of Mathematics and ...

  16. PV Solar Site Assessment (Milwaukee High School)

    Broader source: Energy.gov [DOE]

    The purpose of this assessment is to provide site-specific information on how a solar electric (also referred to as a photovoltaic, or PV) system would perform at your location, including information on estimated physical size, rated output, energy production, costs, financial incentives and mounting options. Site assessors are required to present unbiased information and may not recommend contractors or products.

  17. Experimental And Theoretical High Energy Physics Research At UCLA

    SciTech Connect (OSTI)

    Cousins, Robert D.

    2013-07-22

    This is the final report of the UCLA High Energy Physics DOE Grant No. DE-FG02- 91ER40662. This report covers the last grant project period, namely the three years beginning January 15, 2010, plus extensions through April 30, 2013. The report describes the broad range of our experimental research spanning direct dark matter detection searches using both liquid xenon (XENON) and liquid argon (DARKSIDE); present (ICARUS) and R&D for future (LBNE) neutrino physics; ultra-high-energy neutrino and cosmic ray detection (ANITA); and the highest-energy accelerator-based physics with the CMS experiment and CERN’s Large Hadron Collider. For our theory group, the report describes frontier activities including particle astrophysics and cosmology; neutrino physics; LHC interaction cross section calculations now feasible due to breakthroughs in theoretical techniques; and advances in the formal theory of supergravity.

  18. CERN and high energy physics, the grand picture

    ScienceCinema (OSTI)

    None

    2011-10-06

    The lecture will touch on several topics, to illustrate the role of CERN in the present and future of high-energy physics: how does CERN work? What is the role of the scientific community, of bodies like Council and SPC, and of international cooperation, in the definition of CERN's scientific programme? What are the plans for the future of the LHC and of the non-LHC physics programme? What is the role of R&D; and technology transfer at CERN?

  19. High Energy Physics at Tufts University Final Report

    SciTech Connect (OSTI)

    Goldstein, Gary R.; Oliver, William P.; Napier, Austin; Gallagher, Hugh R.

    2012-07-18

    In this Final Report, we the researchers of the high energy physics group at Tufts University summarize our works and achievements in three frontier areas of elementary particle physics: (i) Neutrino physics at the Intensity Frontier, (ii) Collider physics at the Energy Frontier, and (iii) Theory investigations of spin structure and quark-gluon dynamics of nucleons using quantum chromodynamics. With our Neutrino research we completed, or else brought to a useful state, the following: Data-taking, physics simulations, physics analysis, physics reporting, explorations of matter effects, and detector component fabrication. We conducted our work as participants in the MINOS, NOvA, and LBNE neutrino oscillation experiments and in the MINERvA neutrino scattering experiment. With our Collider research we completed or else brought to a useful state: Data-taking, development of muon system geometry and tracking codes, software validation and maintenance, physics simulations, physics analysis, searches for new particles, and study of top-quark and B-quark systems. We conducted these activities as participants in the ATLAS proton-proton collider experiment at CERN and in the CDF proton-antiproton collider experiment at Fermilab. In our Theory research we developed QCD-based models, applications of spin phenomenology to fundamental systems, fitting of models to data, presenting and reporting of new concepts and formalisms. The overarching objectives of our research work have always been: 1) to test and clarify the predictions of the Standard Model of elementary particle physics, and 2) to discover new phenomena which may point the way to a more unified theoretical framework.

  20. Thomas Jefferson High School for Science & Technology Snaps Up Virginia

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

    Science Bowl Championship; Virginia Beach Schools Take 2nd, 3rd Place | Jefferson Lab Snaps Up Virginia Science Bowl Championship; Virginia Beach Schools Take 2nd, 3rd Place Thomas Jefferson High School for Science & Technology Snaps Up Virginia Science Bowl Championship; Virginia Beach Schools Take 2nd, 3rd Place High School Science Bowl 1st Place The Thomas Jefferson High School for Science and Technology team from Alexandria poses with its first-place trophy after the competition.

  1. Compilation of current high-energy physics experiments

    SciTech Connect (OSTI)

    Wohl, C.G.; Kelly, R.L.; Armstrong, F.E.

    1981-05-01

    This is the fourth edition of the compilation of current high energy physics experiments. It is a collaborative effort of the Berkeley Particle Data Group, the SLAC library, and nine participating laboratories: Argonne (ANL), Brookhaven (BNL), CERN, DESY, Fermilab (FNAL), the Institute for Nuclear Study, Tokyo (INS), KEK, Serpukhov (SERP), and SLAC. The compilation includes summaries of all high energy physics experiments at the above laboratories that (1) were approved (and not subsequently withdrawn) before about April 1981, and (2) had not completed taking of data by 1 January 1977. Only approved experiments are included.

  2. Theoretical Research in Cosmology, High-Energy Physics and String Theory

    SciTech Connect (OSTI)

    Ng, Y Jack; Dolan, Louise; Mersini-Houghton, Laura; Frampton, Paul

    2013-07-29

    The research was in the area of Theoretical Physics: Cosmology, High-Energy Physics and String Theory

  3. High Energy Physics at the University of Illinois

    SciTech Connect (OSTI)

    Liss, Tony M.; Thaler, Jon J.

    2013-07-26

    This is the final report for DOE award DE-FG02-91ER40677 (“High Energy Physics at the University of Illinois”), covering the award period November 1, 2009 through April 30, 2013. During this period, our research involved particle physics at Fermilab and CERN, particle physics related cosmology at Fermilab and SLAC, and theoretical particle physics. Here is a list of the activities described in the final report: * The CDF Collaboration at the Fermilab Tevatron * Search For Lepton Flavor Violation in the Mu2e Experiment At Fermilab * The ATLAS Collaboration at the CERN Large Hadron Collider * the Study of Dark Matter and Dark Energy: DES and LSST * Lattice QCD * String Theory and Field Theory * Collider Phenomenology

  4. Papillion-LaVista South High School Wind Project | Open Energy...

    Open Energy Info (EERE)

    - Northwestern High School Wind Project

  5. High schools compete for Nevada Science Bowl title | National Nuclear

    National Nuclear Security Administration (NNSA)

    Security Administration | (NNSA) High schools compete for Nevada Science Bowl title Monday, February 15, 2016 - 3:37pm NNSA Blog The winner of the 2016 Nevada Science Bowl was the team from Reno's Davidson Academy of Nevada. From left: Matthew Bauer, Rinik Kumar, Haydn Bradstreet, Paolo Adajar, Eric Liu, and Coach Brett Guisti. While sports fans across the U.S. prepared for last weekend's game day, 160 Nevada high school students went head-to-head in a different kind of competition.

  6. Laboratory for Nuclear Science. High Energy Physics Program

    SciTech Connect (OSTI)

    Milner, Richard

    2014-07-30

    High energy and nuclear physics research at MIT is conducted within the Laboratory for Nuclear Science (LNS). Almost half of the faculty in the MIT Physics Department carry out research in LNS at the theoretical and experimental frontiers of subatomic physics. Since 2004, the U.S. Department of Energy has funded the high energy physics research program through grant DE-FG02-05ER41360 (other grants and cooperative agreements provided decades of support prior to 2004). The Director of LNS serves as PI. The grant supports the research of four groups within LNS as “tasks” within the umbrella grant. Brief descriptions of each group are given here. A more detailed report from each task follows in later sections. Although grant DE-FG02-05ER41360 has ended, DOE continues to fund LNS high energy physics research through five separate grants (a research grant for each of the four groups, as well as a grant for AMS Operations). We are pleased to continue this longstanding partnership.

  7. An Experimental and Theoretical High Energy Physics Program

    SciTech Connect (OSTI)

    Shipsey, Ian

    2012-07-31

    The Purdue High Energy Physics Group conducts research in experimental and theoretical elementary particle physics and experimental high energy astrophysics. Our goals, which we share with high energy physics colleagues around the world, are to understand at the most fundamental level the nature of matter, energy, space and time, and in order to explain the birth, evolution and fate of the Universe. The experiments in which we are currently involved are: CDF, CLEO-c, CMS, LSST, and VERITAS. We have been instrumental in establishing two major in-house facilities: The Purdue Particle Physics Microstructure Detector Facility (P3MD) in 1995 and the CMS Tier-2 center in 2005. The research efforts of the theory group span phenomenological and theoretical aspects of the Standard Model as well as many of its possible extensions. Recent work includes phenomenological consequences of supersymmetric models, string theory and applications of gauge/gravity duality, the cosmological implications of massive gravitons, and the physics of extra dimensions.

  8. DOE's NJ HIGH SCHOOL SCIENCE BOWL | Princeton Plasma Physics...

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

    at PPPL, adult visitors must show a government-issued photo I.D. - for example, a passport or a driver's license. Non-U.S. citizens must show a government-issued photo I.D.,...

  9. 2016 High School Science Bowl | Princeton Plasma Physics Lab

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

    2016 GreenGov Symposium (Washington, D.C.) 2016 GreenGov Symposium (Washington, D.C.) September 8, 2016 9:00AM to 5:00PM EDT The 2016 GreenGov Symposium will bring together senior Administration officials and Federal sustainability stakeholders to discuss the executive order, Planning for Federal Sustainability in the Next Decade. The purpose is to discuss strategies to green the fleet, improve water management, reduce greenhouse gas (GHG) emissions, increase energy efficiency and renewable

  10. Highlighting High Performance: Blackstone Valley Regional Vocational Technical High School; Upton, Massachusetts

    SciTech Connect (OSTI)

    Not Available

    2006-10-01

    This brochure describes the key high-performance building features of the Blackstone Valley High School. The brochure was paid for by the Massachusetts Technology Collaborative as part of their Green Schools Initiative. High-performance features described are daylighting and energy-efficient lighting, indoor air quality, solar energy, building envelope, heating and cooling systems, and water conservation. Energy cost savings are also discussed.

  11. Program to enrich science and mathematics experiences of high school students through interactive museum internships

    SciTech Connect (OSTI)

    Reif, R.J.; Lock, C.R.

    1998-11-01

    This project addressed the problem of female and minority representation in science and mathematics education and in related fields. It was designed to recruit high school students from under-represented groups into a program that provided significant, meaningful experiences to encourage those young people to pursue careers in science and science teaching. It provided role models for those students. It provided experiences outside of the normal school environment, experiences that put the participants in the position to serve as role models themselves for disadvantaged young people. It also provided encouragement to pursue careers in science and mathematics teaching and related careers. In these respects, it complemented other successful programs to encourage participation in science. And, it differed in that it provided incentives at a crucial time, when career decisions are being made during the high school years. Further, it encouraged the pursuit of careers in science teaching. The objectives of this project were to: (1) provide enrichment instruction in basic concepts in the life, earth, space, physical sciences and mathematics to selected high school students participating in the program; (2) provide instruction in teaching methods or processes, including verbal communication skills and the use of questioning; (3) provide opportunities for participants, as paid student interns, to transfer knowledge to other peers and adults; (4) encourage minority and female students with high academic potential to pursue careers in science teaching.

  12. Alabama High School Regional Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Alabama High School Regional Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Alabama High School Regional Science Bowl

  13. Alaska High School Regional Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Alaska High School Regional Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Alaska High School Regional Science Bowl

  14. BPA Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    BPA Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals BPA Regional High School Science Bowl Print

  15. Booz Allen Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Booz Allen Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Booz Allen Regional High School

  16. Chicago High School Regional Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Chicago High School Regional Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Chicago High School Regional Science Bowl

  17. Colorado Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Colorado Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Colorado Regional High School

  18. Eastern Nebraska High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Eastern Nebraska High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Eastern Nebraska High School Science Bowl

  19. El Paso Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    El Paso Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals El Paso Regional High School Science Bowl

  20. Georgia Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Georgia Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Georgia Regional High School Science Bowl

  1. Hawaii Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Hawaii Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Hawaii Regional High School Science Bowl

  2. Illinois Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Illinois Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Illinois Regional High School

  3. Indiana Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Indiana Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Indiana Regional High School Science Bowl

  4. Iowa Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Iowa Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Iowa Regional High School Science Bowl Print

  5. Kansas Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Kansas Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Kansas Regional High School Science Bowl

  6. LADWP Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    LADWP Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals LADWP Regional High School Science Bowl Print

  7. Maine Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Maine Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Maine Regional High School Science Bowl Print

  8. Maryland Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Maryland Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Maryland Regional High School

  9. Michigan Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Michigan Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Michigan Regional High School

  10. Minnesota Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Minnesota Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Minnesota Regional High School

  11. Missouri Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Missouri Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Missouri Regional High School

  12. Montana Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Montana Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Montana Regional High School Science Bowl

  13. NYC Regional SHPE High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) NYC Regional SHPE High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals NYC Regional SHPE High School

  14. Nevada Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Nevada Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Nevada Regional High School Science Bowl

  15. New Jersey Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) New Jersey Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals New Jersey Regional High School

  16. Northeast Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Northeast Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Northeast Regional High School

  17. Oklahoma Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Oklahoma Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Oklahoma Regional High School

  18. Pantex Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Pantex Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Pantex Regional High School Science Bowl

  19. Redding Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Redding Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Redding Regional High School Science Bowl

  20. SLAC Regional High School Science Bowl| U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    SLAC Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals SLAC Regional High School Science Bowl Print

  1. SWPA Regional High School Science Bowl | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    SWPA Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals SWPA Regional High School Science Bowl Print

  2. Sacramento Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Sacramento Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Sacramento Regional High School

  3. Tennessee Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Tennessee Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Tennessee Regional High School

  4. Virginia Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Virginia Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Virginia Regional High School

  5. Summer High School Program Fosters Diversity in Science

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

    The Introductory College Level Experience in Microbiology (iCLEM) program provides Bay Area high school students with valuable hands-on experience in the lab and guidance for continuing a career in science. The students are hosted by the Joint BioEnergy Institute.

  6. High School Students Gear Up for Battle of the Brains

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

    Feb. 17, 1999 — What is the maximum distance an electron can travel in a nanosecond? Which planet has a moon almost as big as the planet itself? High school students from across Colorado will face such questions as they test their mental agility in the U.S. Department of Energy's (DOE) 1999 Denver Regional Science Bowl Feb. 27 at the Colorado School of Mines in Golden. More than 20 student teams from rural communities to metropolitan areas across the state will compete in this rapid-fire

  7. The Office of High Energy Physics Announces the Launch of Its...

    Office of Science (SC) Website

    Community Resources News Archives 2013 The Office of High Energy Physics Announces the Launch of Its New Accelerator R&D Stewardship Webpages High Energy Physics (HEP) HEP ...

  8. A novel zirconium K{alpha} imager for high energy density physics...

    Office of Scientific and Technical Information (OSTI)

    for high energy density physics research Citation Details In-Document Search Title: A novel zirconium Kalpha imager for high energy density physics research We report on the ...

  9. High Energy Physics Advisory Panel October 1-2, 2015 | U.S. DOE...

    Office of Science (SC) Website

    High Energy Physics Advisory Panel October 1-2, 2015 High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings Previous Meetings 2015 HEPAP Membership ChargesReports Charter...

  10. Media Advisory - Virginia Regional High School Science Bowl | Jefferson Lab

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

    7, 2009. Round robin competition runs from 9 a.m. - noon. The double elimination, semi-final and finalist rounds run from 1:30 - 5 p.m. Awards presentations will be made immediately after the final round. Where: CEBAF Center Auditorium, Thomas Jefferson National Accelerator Facility, 12000 Jefferson Avenue, Newport News, Va. Details: Twenty-two teams, representing high schools from across the state are participating in this annual, academic competition. Catch the excitement as several high

  11. Cherry Creek High School Wins Colorado Science Bowl - News Releases | NREL

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

    (NNSA) Chernobyl Nuclear Accident Chernobyl Nuclear Accident Chernobyl, Ukraine A catastrophic nuclear accident occurs at Chernobyl Reactor #4 in the then Soviet Republic of Ukraine

    Cherry Creek High School Wins Colorado Science Bowl Greenwood Village School Heads to Washington D.C. to Challenge for National Title January 28, 2012 Golden, Colo., Jan. 28, 2012 - Students from Cherry Creek High School won the Colorado High School Science Bowl today. The school will go on to the 22nd

  12. Design and operation of the high energy physics information server

    SciTech Connect (OSTI)

    Dingbaum, J.J.; Martin, D.E.

    1994-12-31

    HEPIC an information {open_quotes}center of centers{close_quotes} for the HEP community, is a 24 hour online location where a HEP researcher can start her/his search for information. Operated by the HEP Network Research Center, HEPIC is accessible via WWW, gopher, anonymous FTP, DECnet, and AFS. This paper describes HEPIC`s design and future plans, and the HEPNRC`s efforts to collect information and link high energy physics researchers world-wide.

  13. Media Advisory - Virginia Regional High School Science Bowl | Jefferson Lab

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

    4, 2012. Round robin competition runs from 9 a.m. - noon. The double elimination, semi-final and finalist rounds run from 1:30 - ~ 5 p.m. Awards presentations will be made immediately after the final round. Where: CEBAF Center Auditorium, Thomas Jefferson National Accelerator Facility, 12000 Jefferson Avenue, Newport News, Va. 23606 Details: Teams from 22 high schools from across the commonwealth are participating in this annual, academic competition. Catch the excitement as local teams from

  14. Media Advisory - Virginia Regional High School Science Bowl | Jefferson Lab

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

    5, 2011. Round robin competition runs from 9 a.m. - noon. The double elimination, semi-final and finalist rounds run from 1:30 - 5 p.m. Awards presentations will be made immediately after the final round. Where: CEBAF Center Auditorium, Thomas Jefferson National Accelerator Facility, 12000 Jefferson Avenue, Newport News, Va. Details: Twenty-three teams, representing high schools from across the state are participating in this annual, academic competition. Catch the excitement as Patrick Henry

  15. Centauri High School Teacher Honored as Colorado Outstanding Biology

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

    Cement (2010 MECS) Cement (2010 MECS) Manufacturing Energy and Carbon Footprint for Cement Sector (NAICS 327310) Energy use data source: 2010 EIA MECS (with adjustments) Footprint Last Revised: February 2014 View footprints for other sectors here. Manufacturing Energy and Carbon Footprint Cement (126.44 KB) More Documents & Publications MECS 2006 - Cement Glass and Glass Products (2010 MECS) Textiles Teacher

    Centauri High School Teacher Honored as Colorado Outstanding Biology Teacher

  16. High School Co-op Program Selection Process

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

    Selection Process High School Co-op Program Selection Process Point your career towards Los Alamos Lab: work with the best minds on the planet in an inclusive environment that is rich in intellectual vitality and opportunities for growth. Contact Student Programs (505) 665-0987 Email Student selection process Once all application materials are submitted, they will be reviewed for program eligibility. Students who meet the minimum program requirements will have their application materials posted

  17. High School Academic Competition - Double Elimination | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Double Elimination National Science Bowl® (NSB) NSB Home About Regional Competitions National Finals Attending the National Finals 2016 Competition Results Middle School Round Robin Middle School Double Elimination Middle School Electric Car High School Round Robin High School Double Elimination Top Teams for 2016 Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal

  18. High School Academic Competition - Round Robin | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Round Robin National Science Bowl® (NSB) NSB Home About Regional Competitions National Finals Attending the National Finals 2016 Competition Results Middle School Round Robin Middle School Double Elimination Middle School Electric Car High School Round Robin High School Double Elimination Top Teams for 2016 Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000

  19. State College Area High School From State College, PA Wins DOE...

    Office of Environmental Management (EM)

    College Area High School From State College, PA Wins DOE's National Science Bowl State College Area High School From State College, PA Wins DOE's National Science Bowl May 1, ...

  20. National Science Bowl Update: Teams from North Carolina and California to Compete for High School Championship

    Office of Energy Efficiency and Renewable Energy (EERE)

    The field of high school finalists in the Department of Energy (DOE) National Science Bowl has narrowed once more, and now only two high school teams remain in the competition.

  1. We Have a Winner- DC High School Regional Science Bowl Competition Held Last Saturday

    Broader source: Energy.gov [DOE]

    As part of the National Science Bowl, more than 9,500 high school students take place in 70 high school regional competitions around the United States and Puerto Rico.  The winners of these regions...

  2. Connecticut Regional High School Science Bowl| U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Connecticut Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Connecticut Regional High

  3. Kern County Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Kern County Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Kern County Regional High

  4. Long Island Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Long Island Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Long Island Regional High

  5. Mississippi Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Mississippi Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Mississippi Regional High

  6. North Dakota Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) North Dakota Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals North Dakota Regional High

  7. Puerto Rico Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Puerto Rico Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Puerto Rico Regional High

  8. South Dakota Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) South Dakota Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals South Dakota Regional High

  9. Thomas Jefferson High School for Science & Technology Takes 2015 Virginia

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

    Science Bowl | Jefferson Lab Takes 2015 Virginia Science Bowl Thomas Jefferson High School for Science & Technology Takes 2015 Virginia Science Bowl 2014 Virginia High School Science Bowl The team from Thomas Jefferson High School for Science and Technology, Alexandria, swept through the Virginia Regional High School Science Bowl undefeated on Feb. 7. The team of (back row, left to right) Matthew Barbano, Tiger Zhang and Janice Ong, and (front, l. to r.) Franklyn Wang and Ross Dempsey

  10. **NO SCIENCE ON SATURDAY TODAY** NJ Regional High School Science Bowl |

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

    Princeton Plasma Physics Lab 3, 2013, 8:00am Science Education Lab-wide Event **NO SCIENCE ON SATURDAY TODAY** NJ Regional High School Science Bowl Teams of students are invited to participate in the Department of Energy's National Science Bowl Competition. Each year PPPL hosts the New Jersey Regional Science Bowl which decides which teams from the local area can continue onto the national competition in Washington, D.C. The Science Bowl is a double elimination contest with oral question and

  11. High School Academic Competition - Round Robin | U.S. DOE Office...

    Office of Science (SC) Website

    ... 0 0 0 0 0 0 0 9 5. North Allegheny Senior High School 2 2 2 2 2 2 2 2 16 4 6. Edwin O. Smith High School 0 2 2 2 0 2 2 1 11 1 7. Stevens High School 0 2 0 2 0 0 2 0 6 5 8. BASIS DC ...

  12. Physics

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

    Group (PDG) Organizations American Institute of Physics (AIP) American Physical Society (APS) Institute of Physics (IOP) SPIE - International society for optics and photonics Top...

  13. REPORT OF RESEARCH ACCOMPLISHMENTS AND FUTURE GOALS HIGH ENERGY PHYSICS

    SciTech Connect (OSTI)

    Wise, Mark B.; Kapustin, Anton N.; Schwarz, John Henry; Carroll, Sean; Ooguri, Hirosi; Gukov, Sergei; Preskill, John; Hitlin, David G.; Porter, Frank C.; Patterson, Ryan B.; Newman, Harvey B.; Spiropulu, Maria; Golwala, Sunil; Zhu, Ren-Yuan

    2014-08-26

    Caltech High Energy Physics (HEP) has a broad program in both experimental and theoretical physics. We are known for our creativity and leadership. The future is uncertain and we strive to be involved in all the major areas of experimental and theoretical HEP physics so no matter where the important discoveries occur we are well positioned to play an important role. An outstanding group of postdoctoral scholars, graduate students, staff scientists, and technical and administrative personnel support our efforts in experimental and theoretical physics. The PI’s on this grant are involved in the following program of experimental and theoretical activities: I) EXPERIMENTAL PHYSICS Our CMS group, led by Harvey Newman and Maria Spiropulu, has played a key role in the discovery and interpretation of the Higgs boson and in searches for new physics. They have important hardware responsibilities in both ECAL and HCAL and are also involved in the upgrades needed for the High Luminosity LHC. Newman's group also develops and operates Grid-based computing, networking, and collaborative systems for CMS and the US HEP community. The charged lepton (Mu2e) and quark BaBar flavor physics group is led by David Hitlin and Frank Porter. On Mu2e they have been instrumental in the design of the calorimeter. Construction responsibilities include one third of the crystals and associated readout as well as the calibration system. They also will have responsibility for a major part of the online system software. Although data taking ceased in 2008 the Caltech BaBar group is active on several new forefront analyses. The neutrino group is led by Ryan Patterson. They are central to NOvA's core oscillation physics program, to calibration, and to detector readiness being responsible for the production and installation of 12,000 APD arrays. They have key roles in neutrino appearance and disappearance analysis in MINOS and MINOS+. Sunil Golwala leads the dark matter direct detection effort. Areas

  14. Stratton Middle and High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  15. Ponderosa High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  16. Skyline High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  17. Shelley High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  18. Eudora High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  19. USD 376 Sterling High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  20. Walsh High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  1. Santa Fe Trail High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  2. Diller-Odell High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  3. James Buchanan High School Wind Turbine | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  4. Watauga High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  5. Rigby High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  6. Mullen High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  7. Northwestern High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  8. Florence High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  9. Loup City High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  10. Grassfield High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  11. Nederland High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  12. USD 393 Solomon High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  13. North Wilkes Middle and High School Wind Project | Open Energy...

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  14. Burlington High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  15. USD 375 Circle High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  16. USD 345 Seaman High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  17. Clover Hill High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  18. Avery County High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  19. Ferndale High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  20. Concordia High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  1. Alleghany High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  2. Mt. Edgecumbe High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  3. Jefferson West High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  4. Pretty Prairie High School Wind Project | Open Energy Information

    Open Energy Info (EERE)

    - Yankton School District Wind Project

  5. High School Regionals | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    High School Regionals National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us Regional Competitions High School Regionals Print Text Size: A A A FeedbackShare Page

  6. High School Sample Questions | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    High School Sample Questions National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us Rules, Forms, and Resources High School Sample Questions Print Text Size: A A

  7. Greater Cincinnati Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Greater Cincinnati Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Greater

  8. Inland Northwest Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Inland Northwest Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Inland Northwest

  9. Los Angeles JPL Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Los Angeles JPL Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Los Angeles JPL

  10. New York Capital District High School Regional Science Bowl | U.S. DOE

    Office of Science (SC) Website

    Office of Science (SC) New York Capital District High School Regional Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School

  11. North Carolina Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Carolina Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals North Carolina Regional

  12. Pacific Northwest Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Pacific Northwest Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Pacific

  13. Sandia/Las Positas Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Sandia/Las Positas Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Sandia/Las

  14. Savannah River Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Savannah River Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Savannah River

  15. South Central Ohio Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) South Central Ohio Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals South Central

  16. South Florida Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) South Florida Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals South Florida

  17. U.S. Virgin Islands Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) U.S. Virgin Islands High School Regional Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals U.S. Virgin

  18. Washington, DC Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Washington, DC Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Washington, DC

  19. West Kentucky Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) West Kentucky Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals West Kentucky

  20. West Virginia Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) West Virginia Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals West Virginia

  1. Western Nebraska Regional High School Science Bowl | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) Western Nebraska Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Western Nebraska

  2. High-Efficiency Solar Cell Concepts: Physics, Materials, and Devices

    SciTech Connect (OSTI)

    Mascarenhas, A.; Francoeur, S.; Seong, M. J.; Fluegel, B.; Zhang, Y.; Wanlass, M. W.

    2005-01-01

    Over the past three decades, significant progress has been made in the area of high-efficiency multijunction solar cells, with the effort primarily directed at current-matched solar cells in tandem. The key materials issues here have been obtaining semiconductors with the required bandgaps for sequential absorption of light in the solar spectrum and that are lattice matched to readily available substrates. The GaInP/GaAs/Ge cell is a striking example of success achieved in this area. Recently, several new approaches for high-efficiency solar cell design have emerged, that involve novel methods for tailoring alloy bandgaps, as well as alternate technologies for hetero-epitaxy of III-V's on Si. The advantages and difficulties expected to be encountered with each approach will be discussed, addressing both the materials issues and device physics whilst contrasting them with other fourth-generation solar cell concepts.

  3. Thomas Jefferson High School for Science & Technology Wins Feb. 5 Virginia

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

    Science Bowl; Warwick High Wins Math and Science Challenges | Jefferson Lab Wins Feb. 5 Virginia Science Bowl; Warwick High Wins Math and Science Challenges Thomas Jefferson High School for Science & Technology Wins Feb. 5 Virginia Science Bowl; Warwick High Wins Math and Science Challenges fellowship The Thomas Jefferson High School for Science and Technology, Alexandria, won the Feb. 5 Virginia Regional High School Science Bowl. Pictured, left to right, are Coach Sharon Webb; Alexander

  4. Research in High Energy Physics at Duke University

    SciTech Connect (OSTI)

    Kotwal, Ashutosh V.; Goshaw, Al; Kruse, Mark; Oh, Seog; Scholberg, Kate; Walter, Chris

    2013-07-29

    This is the Closeout Report for the research grant in experimental elementary particle physics, carried out by the Duke University High Energy Physics (HEP) group. We re- port on physics results and detector development carried out under this grant, focussing on the recent three-year grant period (2010 to 2013). The Duke HEP group consisted of seven faculty members, two senior scientists, #12;ve postdocs and eight graduate students. There were three thrusts of the research program. Measurements at the energy frontier at CDF and ATLAS were used to test aspects of elementary particle theory described by the Stan- dard Model (SM) and to search for new forces and particles beyond those contained within the SM. The neutrino sector was explored using data obtained from a large neutrino detector located in Japan, and R & D was conducted on new experiments to be built in the US. The measurements provided information about neutrino masses and the manner in which neutri- nos change species in particle beams. Two years ago we have started a new research program in rare processes based on the Mu2E experiment at Fermilab. This research is motivated by the search for the #22; ! e transition with unprecedented sensitivity, a transition forbidden in the standard model but allowed in supersymmetric and other models of new physics. The high energy research program used proton and antiproton colliding beams. The experiments were done at the Fermilab Tevatron (proton-antiproton collisions at a center of mass energy of 1.96 TeV) and at the CERN Large Hadron Collider (proton-proton collisions at 7-8 TeV). The neutrino program used data obtained from the Super-Kamiokande detec- tor. This water-#12;lled Cherenkov counter was used to detect and measure the properties of neutrinos produced in cosmic ray showers, and from neutrino beams produced from acceler- ators in Japan. The Mu2E experiment will use a special stopped muon beam to be built at Fermilab.

  5. Research in High Energy Physics at Duke University

    SciTech Connect (OSTI)

    Goshaw, Alfred; Kotwal, Ashutosh; Kruse, Mark; Oh, Seog; Scholberg, Kate; Walter, Chris

    2013-07-29

    This is the Closeout Report for the research grant in experimental elementary particle physics, carried out by the Duke University High Energy Physics (HEP) group. We re- port on physics results and detector development carried out under this grant, focussing on the recent three-year grant period (2010 to 2013). The Duke HEP group consisted of seven faculty members, two senior scientists, five postdocs and eight graduate students. There were three thrusts of the research program. Measurements at the energy frontier at CDF and ATLAS were used to test aspects of elementary particle theory described by the Stan- dard Model (SM) and to search for new forces and particles beyond those contained within the SM. The neutrino sector was explored using data obtained from a large neutrino detector located in Japan, and R & D was conducted on new experiments to be built in the US. The measurements provided information about neutrino masses and the manner in which neutri- nos change species in particle beams. Two years ago we have started a new research program in rare processes based on the Mu2E experiment at Fermilab. This research is motivated by the search for the #22;{mu} {yields} e transition with unprecedented sensitivity, a transition forbidden in the standard model but allowed in supersymmetric and other models of new physics. The high energy research program used proton and antiproton colliding beams. The experiments were done at the Fermilab Tevatron (proton-antiproton collisions at a center of mass energy of 1.96 TeV) and at the CERN Large Hadron Collider (proton-proton collisions at 7-8 TeV). The neutrino program used data obtained from the Super-Kamiokande detector. This water-filled Cherenkov counter was used to detect and measure the properties of neutrinos produced in cosmic ray showers, and from neutrino beams produced from acceler- ators in Japan. The Mu2E experiment will use a special stopped muon beam to be built at Fermilab.

  6. High School Students Compete in Solar-Powered Bike Race

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

    Compete in Solar-Powered Bike Race For more information contact: e:mail: Public Affairs Golden, Colo., April 23, 1998 — Photo opportunity: Media are invited to cover the workshop and solar-powered bicycle race designed to give students hands-on learning experiences with renewable energy technologies. What: The Colorado Solar BikeRayce is a competition for high school students to race solar-powered bikes that they design and build. The event will prepare the teams for the national Solar

  7. High School Academic Competition - Round Robin | U.S. DOE Office...

    Office of Science (SC) Website

    ... Team 1 2 3 4 5 6 7 8 Total Points DTC Rank 1. University Preparatory School 0 0 2 2 0 0 0 4 4 2. E.O. Smith High School 2 2 2 2 2 2 2 14 3 3. Los Alamos High School 2 0 2 2 0 2 2 ...

  8. High energy physics program at Texas A and M University

    SciTech Connect (OSTI)

    Not Available

    1991-10-01

    The Texas A M experimental high energy physics program continued to reach significant milestones in each of its research initiatives during the course of the past year. We are participating in two major operating experiments, CDF and MACRO. In CDF, the Texas A M group has spearheaded the test beam program to recalibrate the Forward Hadron Calorimeter for the upcoming CDF data run, as well as contributing to the ongoing analysis work on jets and b-quarks. In MACRO, we have assisted in the development of the final version of the wave form digitizing system being implemented for the entire scintillator system. The construction of the first six supermodules of the detector has been completed and all six are currently taking data with streamer chambers while four have the completed scintillator counter system up and running. We have built and tested prototypes of a liquid-scintillator fiber calorimeter system, in which internally reflecting channels are imbedded in a lead matrix and filled with liquid scintillator. This approach combines the performance features of fiber calorimetry and the radiation hardness of liquid scintillator, and is being developed for forward calorimetry at the SSC. The microstrip chamber is a new technology for precision track chambers that offers the performance required for future hadron colliders. The theoretical high energy physics program has continued to develop during the past funding cycle. We have continued the study of their very successful string-derived model that unifies all known interactions; flipped SU(5), which is the leading candidate for a TOE. Work has continued on some generalizations of the symmetries of string theory, known as W algebras. These are expected to have applications in two-dimensional conformal field theory, two-dimensional extensions of gravity and topological gravity and W-string theory.

  9. Future Accelerator Challenges in Support of High-Energy Physics

    SciTech Connect (OSTI)

    Zisman, Michael S.; Zisman, M.S.

    2008-05-03

    Historically, progress in high-energy physics has largely been determined by development of more capable particle accelerators. This trend continues today with the imminent commissioning of the Large Hadron Collider at CERN, and the worldwide development effort toward the International Linear Collider. Looking ahead, there are two scientific areas ripe for further exploration--the energy frontier and the precision frontier. To explore the energy frontier, two approaches toward multi-TeV beams are being studied, an electron-positron linear collider based on a novel two-beam powering system (CLIC), and a Muon Collider. Work on the precision frontier involves accelerators with very high intensity, including a Super-BFactory and a muon-based Neutrino Factory. Without question, one of the most promising approaches is the development of muon-beam accelerators. Such machines have very high scientific potential, and would substantially advance the state-of-the-art in accelerator design. The challenges of the new generation of accelerators, and how these can be accommodated in the accelerator design, are described. To reap their scientific benefits, all of these frontier accelerators will require sophisticated instrumentation to characterize the beam and control it with unprecedented precision.

  10. High-Performance Computing Modeling Advances Accelerator Science for High-Energy Physics

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

    Amundson, James; Macridin, Alexandru; Spentzouris, Panagiotis

    2014-11-01

    The development and optimization of particle accelerators are essential for advancing our understanding of the properties of matter, energy, space and time. Particle accelerators are complex devices whose behavior involves many physical effects on multiple scales. Therefore, advanced computational tools utilizing high-performance computing (HPC) are essential for accurately modeling them. In the past decade, the DOE SciDAC program has produced such accelerator-modeling tools, which have beem employed to tackle some of the most difficult accelerator science problems. In this article we discuss the Synergia beam-dynamics framework and its applications to high-intensity particle accelerator physics. Synergia is an accelerator simulation packagemorecapable of handling the entire spectrum of beam dynamics simulations. We present the design principles, key physical and numerical models in Synergia and its performance on HPC platforms. Finally, we present the results of Synergia applications for the Fermilab proton source upgrade, known as the Proton Improvement Plan (PIP).less

  11. High-Performance Computing Modeling Advances Accelerator Science for High-Energy Physics

    SciTech Connect (OSTI)

    Amundson, James; Macridin, Alexandru; Spentzouris, Panagiotis

    2014-11-01

    The development and optimization of particle accelerators are essential for advancing our understanding of the properties of matter, energy, space and time. Particle accelerators are complex devices whose behavior involves many physical effects on multiple scales. Therefore, advanced computational tools utilizing high-performance computing (HPC) are essential for accurately modeling them. In the past decade, the DOE SciDAC program has produced such accelerator-modeling tools, which have beem employed to tackle some of the most difficult accelerator science problems. In this article we discuss the Synergia beam-dynamics framework and its applications to high-intensity particle accelerator physics. Synergia is an accelerator simulation package capable of handling the entire spectrum of beam dynamics simulations. We present the design principles, key physical and numerical models in Synergia and its performance on HPC platforms. Finally, we present the results of Synergia applications for the Fermilab proton source upgrade, known as the Proton Improvement Plan (PIP).

  12. High-pressure stability relations, crystal structures, and physical...

    Office of Scientific and Technical Information (OSTI)

    ... Country of Publication: United States Language: English Subject: 37 INORGANIC, ORGANIC, PHYSICAL AND ANALYTICAL CHEMISTRY; ANTIFERROMAGNETISM; CRYSTAL STRUCTURE; EXCHANGE ...

  13. Physics

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

    Physics Physics Print Because a large proportion of ALS experiments are "physics" experiments, it's useful to separate them into two categories - one focused on Materials/Condensed Matter, and this one, with a dual focus on AMO (atomic, molecular, and optical) physics and accelerator physics. Light sources such as the ALS have opened up research frontiers that may hold the answers to fundamental questions about structure and dynamics in AMO physics. The advanced spectroscopies that

  14. High-Z Non-Equilibrium Physics and Bright X-ray Sources with...

    Office of Scientific and Technical Information (OSTI)

    Technical Report: High-Z Non-Equilibrium Physics and Bright X-ray Sources with New Laser Targets Citation Details In-Document Search Title: High-Z Non-Equilibrium Physics and ...

  15. High Energy Physics Advisory Panel August 2012 Meeting | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) High Energy Physics Advisory Panel August 2012 Meeting High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings Previous Meetings 2016 HEPAP Membership Charges/Reports Charter .pdf file (44KB) HEP Committees of Visitors Federal Advisory Committees HEP Home Meetings High Energy Physics Advisory Panel August 2012 Meeting Print Text Size: A A A FeedbackShare Page Agenda High Energy Physics Advisory Panel Hilton Hotel 1750 Rockville Pike Rockville, Maryland August 27-28, 2012

  16. National Best Practices Manual for Building High Performance Schools

    Office of Energy Efficiency and Renewable Energy (EERE)

    The Best Practices Manual was written as a part of the promotional effort for EnergySmart Schools, provided by the US Department of Energy, to educate school districts around the country about energy efficiency and renewable energy.

  17. National Best Practices Manual for Building High Performance Schools

    SciTech Connect (OSTI)

    2007-10-01

    The Best Practices Manual was written as a part of the promotional effort for EnergySmart Schools, provided by the US Department of Energy, to educate school districts around the country about energy efficiency and renewable energy.

  18. Physics

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

    Physics Print Because a large proportion of ALS experiments are "physics" experiments, it's useful to separate them into two categories - one focused on Materials/Condensed Matter, and this one, with a dual focus on AMO (atomic, molecular, and optical) physics and accelerator physics. Light sources such as the ALS have opened up research frontiers that may hold the answers to fundamental questions about structure and dynamics in AMO physics. The advanced spectroscopies that have been

  19. High Energy Physics at the University of Illinois

    SciTech Connect (OSTI)

    Neubauer, Mark; Errede, Steve; Gollin, George; Thaler, Jon; El-Khadra, Aida; Willenbrock, Scott; Leigh, Robert; Pitts, Kevin

    2013-04-01

    Experimental and theoretical research in elementary particle physics and astronomy at the University of Illinois Urbana-Champaign is presented via a series of reprints of published papers.

  20. Thomas Jefferson High School for Science & Technology wins the Virginia

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

    Regional Science Bowl | Jefferson Lab #38; Technology wins the Virginia Regional Science Bowl Thomas Jefferson High School for Science & Technology wins the Virginia Regional Science Bowl February 15, 2006 TJHSST Finishing in first place at the Virginia Regional High School Science Bowl was the team from the Thomas Jefferson High School for Science and Technology from Alexandria, Va. Pictured from left to right is Coach Sharon Webb, Charlotte Seid, Daniel Schafer, Lisa Marrone, Neel

  1. Twenty High School Teams Compete in Virginia Regional Science Bowl Being

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

    Held At Jefferson Lab | Jefferson Lab Twenty High School Teams Compete in Virginia Regional Science Bowl Being Held At Jefferson Lab Media Advisory: Twenty High School Teams Compete in Virginia Regional Science Bowl Being Held At Jefferson Lab February 7, 2002 The Department of Energy's Thomas Jefferson National Accelerator Facility (Jefferson Lab) in Newport News, Va., is hosting this year's Virginia Regional Science Bowl on February 9, 2002. Twenty teams, representing high schools from

  2. 2010 DOE National Science Bowl® Photos - Campbell High School...

    Office of Science (SC) Website

    Campbell High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past National ...

  3. 2010 DOE National Science Bowl® Photos - Onate High School ...

    Office of Science (SC) Website

    Onate High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past National ...

  4. 2010 DOE National Science Bowl® Photos - C.M. Russell High School...

    Office of Science (SC) Website

    C.M. Russell High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past ...

  5. 2010 DOE National Science Bowl® Photos - LaFayette High School...

    Office of Science (SC) Website

    LaFayette High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past ...

  6. 2010 DOE National Science Bowl® Photos - Lexington High School...

    Office of Science (SC) Website

    Lexington High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past ...

  7. 2010 DOE National Science Bowl® Photos - Farmingdale High School...

    Office of Science (SC) Website

    Farmingdale High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past ...

  8. 2010 DOE National Science Bowl® Photos - Palo Alto High School...

    Office of Science (SC) Website

    Palo Alto High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past ...

  9. 2010 DOE National Science Bowl® Photos - Shasta High School...

    Office of Science (SC) Website

    Shasta High School National Science Bowl (NSB) NSB Home About National Science Bowl Contacts Regional Science Bowl Coordinators National Science Bowl FAQ's Alumni Past National ...

  10. Colorado Regional High School Science Bowl | U.S. DOE Office...

    Office of Science (SC) Website

    Beginning 5 weeks prior to the event and space permitting, second registered teams will be approved to participate. Competition Location Dakota Ridge High School 13399 W Coal Mine ...

  11. D.C. Middle and High School Students Get a Chance to Experience...

    Office of Environmental Management (EM)

    to Experience the Regional Science Bowl Competition Setting D.C. Middle and High School Students Get a Chance to Experience the Regional Science Bowl Competition Setting March ...

  12. Poudre High School From Fort Collins , Colorado Wins U.S. Department of

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

    Energy National Science Bowl® | Department of Energy Poudre High School From Fort Collins , Colorado Wins U.S. Department of Energy National Science Bowl® Poudre High School From Fort Collins , Colorado Wins U.S. Department of Energy National Science Bowl® April 30, 2007 - 12:45pm Addthis WASHINGTON, DC - Poudre High School from Fort Collins, Colorado won the 2007 U.S. Department of Energy (DOE) National Science Bowl® for high school students today at the National 4-H Youth Conference

  13. Twenty Teams to Compete in Virginia High School Science Bowl on Feb. 7 |

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

    Jefferson Lab Twenty Teams to Compete in Virginia High School Science Bowl on Feb. 7 The final match of the 2014 Virginia High School Science Bowl pitted Warwick High School, Newport News, against Thomas Jefferson High School for Science and Technology, Alexandria, the long-standing Virginia Science Bowl champs. The team from TJHSST won the day and advanced to the national finals. A number of teams that didn't make it into the semi-finals participated in the Stay All Day design and

  14. High School Students Begin Battle for Trip to the National Science Bowl -

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

    News Releases | NREL High School Students Begin Battle for Trip to the National Science Bowl January 29, 2009 Proving that they know more about science than some adults will be a cinch for approximately 160 Colorado high school students who will showcase their science and math knowledge at the Colorado Science Bowl on Saturday, January 31, at Dakota Ridge High School. The U.S. Department of Energy began the science bowl tradition nearly 20 years ago as a way to encourage high school students

  15. Jefferson Lab Hosts 20 Teams for High School Science Bowl on Feb. 2 |

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

    Jefferson Lab High School Science Bowl on Feb. 2 Jefferson Lab Hosts 20 Teams for High School Science Bowl on Feb. 2 NEWPORT NEWS, Va., Jan. 25, 2008 - Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 2, to compete in the Virginia Regional High School Science Bowl. Twenty teams, representing high schools from across the region are registered for this year's academic competition. The National Science Bowl®

  16. Jefferson Lab Hosts 22 Teams for High School Science Bowl on Feb. 7 |

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

    Jefferson Lab 2 Teams for High School Science Bowl on Feb. 7 Jefferson Lab Hosts 22 Teams for High School Science Bowl on Feb. 7 NEWPORT NEWS, Va., Feb. 2, 2009 - Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 7, to compete in the Virginia Regional High School Science Bowl. Twenty-two teams, representing high schools from across the region, are registered for this year's academic competition. The National Science

  17. Jefferson Lab hosts 23 teams for Virginia High School Science Bowl on Feb.

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

    11 | Jefferson Lab hosts 23 teams for Virginia High School Science Bowl on Feb. 11 Jefferson Lab Hosts 23 teams for Virginia High School Science Bowl on Feb. 11 February 3, 2006 Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 11, to compete in the Virginia Regional High School Science Bowl. Twenty-three teams, representing high schools from across the region are participating in this year's academic competition.

  18. Nineteen Teams to Compete in Virginia Regional High School Science Bowl on

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

    Feb. 6 | Jefferson Lab Nineteen Teams to Compete in Virginia Regional High School Science Bowl on Feb. 6 The final match of the 2015 Virginia Regional High School Science Bowl pitted Langley High School, McLean, against Thomas Jefferson High School for Science and Technology, Alexandria. The team from TJHSST won the day and advanced to the national finals. Teams that didn't make it into the semi-finals participated in the Stay All Day design and engineering challenge. Pictured are photos

  19. High Performance Computing Modeling Advances Accelerator Science for High-Energy Physics

    SciTech Connect (OSTI)

    Amundson, James; Macridin, Alexandru; Spentzouris, Panagiotis

    2014-07-28

    The development and optimization of particle accelerators are essential for advancing our understanding of the properties of matter, energy, space, and time. Particle accelerators are complex devices whose behavior involves many physical effects on multiple scales. Therefore, advanced computational tools utilizing high-performance computing are essential for accurately modeling them. In the past decade, the US Department of Energy's SciDAC program has produced accelerator-modeling tools that have been employed to tackle some of the most difficult accelerator science problems. The authors discuss the Synergia framework and its applications to high-intensity particle accelerator physics. Synergia is an accelerator simulation package capable of handling the entire spectrum of beam dynamics simulations. Our authors present Synergia's design principles and its performance on HPC platforms.

  20. High Performance Computing Modeling Advances Accelerator Science for High-Energy Physics

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

    Amundson, James; Macridin, Alexandru; Spentzouris, Panagiotis

    2014-07-28

    The development and optimization of particle accelerators are essential for advancing our understanding of the properties of matter, energy, space, and time. Particle accelerators are complex devices whose behavior involves many physical effects on multiple scales. Therefore, advanced computational tools utilizing high-performance computing are essential for accurately modeling them. In the past decade, the US Department of Energy's SciDAC program has produced accelerator-modeling tools that have been employed to tackle some of the most difficult accelerator science problems. The authors discuss the Synergia framework and its applications to high-intensity particle accelerator physics. Synergia is an accelerator simulation package capable ofmore » handling the entire spectrum of beam dynamics simulations. Our authors present Synergia's design principles and its performance on HPC platforms.« less

  1. Large Scale Computing and Storage Requirements for High Energy Physics

    SciTech Connect (OSTI)

    Gerber, Richard A.; Wasserman, Harvey

    2010-11-24

    The National Energy Research Scientific Computing Center (NERSC) is the leading scientific computing facility for the Department of Energy's Office of Science, providing high-performance computing (HPC) resources to more than 3,000 researchers working on about 400 projects. NERSC provides large-scale computing resources and, crucially, the support and expertise needed for scientists to make effective use of them. In November 2009, NERSC, DOE's Office of Advanced Scientific Computing Research (ASCR), and DOE's Office of High Energy Physics (HEP) held a workshop to characterize the HPC resources needed at NERSC to support HEP research through the next three to five years. The effort is part of NERSC's legacy of anticipating users needs and deploying resources to meet those demands. The workshop revealed several key points, in addition to achieving its goal of collecting and characterizing computing requirements. The chief findings: (1) Science teams need access to a significant increase in computational resources to meet their research goals; (2) Research teams need to be able to read, write, transfer, store online, archive, analyze, and share huge volumes of data; (3) Science teams need guidance and support to implement their codes on future architectures; and (4) Projects need predictable, rapid turnaround of their computational jobs to meet mission-critical time constraints. This report expands upon these key points and includes others. It also presents a number of case studies as representative of the research conducted within HEP. Workshop participants were asked to codify their requirements in this case study format, summarizing their science goals, methods of solution, current and three-to-five year computing requirements, and software and support needs. Participants were also asked to describe their strategy for computing in the highly parallel, multi-core environment that is expected to dominate HPC architectures over the next few years. The report includes

  2. Physics

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

    Physics Physics Our science answers questions about the nature of the universe and delivers solutions for national security concerns. Contact Us Division Leader David Meyerhofer Deputy Division Leader Scott Wilburn Division Office (505) 667-4117 For more than 70 years-from the Manhattan Project to today-Physics Division researchers have been performing groundbreaking fundamental and applied research. For more than 70 years-from the Manhattan Project to today-Physics Division researchers have

  3. Langston University - High Energy Physics (LU-HEP)

    SciTech Connect (OSTI)

    Snow, Dr., Joel

    2012-08-13

    This final report is presented by Langston University (LU) for the project entitled "Langston University High Energy Physics" (LUHEP) under the direction of principal investigator (PI) and project director Professor Joel Snow. The project encompassed high energy physics research performed at hadron colliders. The PI is a collaborator on the DZero experiment at Fermi National Accelerator Laboratory in Batavia, IL, USA and the ATLAS experiment at CERN in Geneva, Switzerland and was during the entire project period from April 1, 1999 until May 14, 2012. Both experiments seek to understand the fundamental constituents of the physical universe and the forces that govern their interactions. In 1999 as member of the Online Systems group for Run 2 the PI developed a cross-platform Python-based, Graphical User Interface (GUI) application for monitoring and control of EPICS based devices for control room use. This served as a model for other developers to enhance and build on for further monitoring and control tasks written in Python. Subsequently the PI created and developed a cross-platform C++ GUI utilizing a networked client-server paradigm and based on ROOT, the object oriented analysis framework from CERN. The GUI served as a user interface to the Examine tasks running in the D\\O\\ control room which monitored the status and integrity of data taking for Run 2. The PI developed the histogram server/control interface to the GUI client for the EXAMINE processes. The histogram server was built from the ROOT framework and was integrated into the D\\O\\ framework used for online monitoring programs and offline analysis. The PI developed the first implementation of displaying histograms dynamically generated by ROOT in a Web Browser. The PI's work resulted in several talks and papers at international conferences and workshops. The PI established computing software infrastructure at LU and U. Oklahoma (OU) to do analysis of DZero production data and produce simulation data

  4. View from Washington: Perspectives on future high energy physics

    SciTech Connect (OSTI)

    Krebs, M.

    1997-03-01

    This is a talk by Martha Krebs (director of energy research at the U.S. Department of Energy). Funding priorities and the current budget constraints at the Department of Energy are discussed. {copyright} {ital 1997 American Institute of Physics.}

  5. Calling Science Stars in Middle and High Schools | Department...

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

    2010 Science Bowl national champions: North Carolina School of Science and Mathematics from Durham, NC | Department of Energy Photo | Public Domain | 2010 Science Bowl national...

  6. National Best Practices Manual for Building High Performance Schools (Revised)

    SciTech Connect (OSTI)

    Not Available

    2007-10-01

    The Best Practices Manual was written as a part of the promotional effort for EnergySmart Schools, provided by the US Department of Energy, to educate school districts around the country about energy efficiency and renewable energy. Written specifically for architects and engineers, The Best Practices Manual is designed to help those who are responsible for designing or retrofitting schools, as well as their project managers. This manual will help design staff make informed decisions about energy and environmental issues important to the school systems and communities.

  7. High Energy Physics: Report of research accomplishments and future goals, FY 1988

    SciTech Connect (OSTI)

    Barish, B C; Stone, E C; Ames, C A

    1987-07-10

    This report discusses high energy physics research in the following areas: Research in elementary particle physics; QCD phenomenology; lattice gauge theory; Mark III; MARK J and Mark II/SLC.

  8. State College Area High School From State College, PA Wins DOE's National

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

    Science Bowl® | Department of Energy College Area High School From State College, PA Wins DOE's National Science Bowl® State College Area High School From State College, PA Wins DOE's National Science Bowl® May 1, 2006 - 10:34am Addthis WASHINGTON , DC - State College Area High School from State College, Pennsylvania, today won the Department of Energy's (DOE) National Science Bowl®. Teams representing 65 schools from across the United States competed in this "Science Jeopardy"

  9. Twenty-three Teams to Compete in Virginia High School Science Bowl |

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

    Jefferson Lab Twenty-three Teams to Compete in Virginia High School Science Bowl Twenty-three Teams to Compete in Virginia High School Science Bowl NEWPORT NEWS, Va., Jan. 30, 2014 - Some of the brightest young minds in the Commonwealth will meet at the U.S. Department of Energy's Jefferson Lab on Saturday, Feb. 1, to compete in the Virginia Regional High School Science Bowl. Teams from 23 schools are registered for this year's academic competition. The National Science Bowl tournament -

  10. University of Texas Rio Grande Valley Regional High School Science Bowl |

    Office of Science (SC) Website

    U.S. DOE Office of Science (SC) University of Texas Rio Grande Valley Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us

  11. Experimental High Energy Physics Brandeis University Final Report

    SciTech Connect (OSTI)

    Blocker, Craig A.; Bensinger, James; Sciolla, Gabriella; Wellenstein, Hermann

    2013-07-26

    During the past three years, the Brandeis experimental particle physics group was comprised of four faculty (Bensinger, Blocker, Sciolla, and Wellenstein), one research scientist, one post doc, and ten graduate students. The group focused on the ATLAS experiment at LHC. In 2011, the LHC delivered 5/fb of pp colliding beam data at a center-of-mass energy of 7 TeV. In 2012, the center-of-mass energy was increased to 8 TeV, and 20/fb were delivered. The Brandeis group focused on two aspects of the ATLAS experiment -- the muon detection system and physics analysis. Since data taking began at the LHC in 2009, our group actively worked on ATLAS physics analysis, with an emphasis on exploiting the new energy regime of the LHC to search for indications of physics beyond the Standard Model. The topics investigated were Z' -> ll, Higgs -> ZZ* -. 4l, lepton flavor violation, muon compositeness, left-right symmetric theories, and a search for Higgs -> ee. The Brandeis group has for many years been a leader in the endcap muon system, making important contributions to every aspect of its design and production. During the past three years, the group continued to work on commissioning the muon detector and alignment system, development of alignment software, and installation of remaining chambers.

  12. The Office of High Energy Physics Announces the Launch of Its New

    Office of Science (SC) Website

    Accelerator R&D Stewardship Webpages | U.S. DOE Office of Science (SC) Featured Content » 2013 » The Office of High Energy Physics Announces the Launch of Its New Accelerator R&D Stewardship Webpages High Energy Physics (HEP) HEP Home About Research Facilities Science Highlights Benefits of HEP Funding Opportunities Advisory Committees Community Resources Featured Content 2016 2015 2014 2013 2012-2008 Reports Contact Information High Energy Physics U.S. Department of Energy

  13. High Energy Physics Advisory Panel August 12, 2016 | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) August 12, 2016 High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings Previous Meetings 2016 HEPAP Membership Charges/Reports Charter .pdf file (44KB) HEP Committees of Visitors Federal Advisory Committees HEP Home Meetings High Energy Physics Advisory Panel August 12, 2016 Print Text Size: A A A FeedbackShare Page DOE Logo NSF Logo U.S Department of Energy and the National Science Foundation Agenda .pdf file (191KB) High Energy Physics Advisory Panel Teleconference

  14. High Energy Physics Division semiannual report of research activities, July 1, 1994--December 31, 1994

    SciTech Connect (OSTI)

    Wagner, R.; Schoessow, P.; Talaga, R.

    1995-04-01

    This report describes the research conducted in the High Energy Physics Division of Argonne National Laboratory during the period of July 1, 1994--December 31, 1994. Topics covered here include experimental and theoretical particle physics, advanced accelerator physics, detector development, and experimental facilities research. Lists of division publications and colloquia are included.

  15. High School Science Bowl Coaching Information | The Ames Laboratory

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

    don't delay. Schools whose applications are received after the roster is filled will be placed on a waiting list. Hints, tips and tricks: Registration opens October 1, 11:00 AM....

  16. West Windsor-Plainsboro High School South wins regional Science...

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

    For senior Alexander Clifton, the team's captain, whose middle school team went to the nationals when he was in eighth grade, it was a sweet victory. The team had come in second in ...

  17. West Windsor-Plainsboro High School South wins regional Science...

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

    ... For senior Alexander Clifton, the team's captain, whose middle school team went to the nationals when he was in eighth grade, it was a sweet victory. The team had come in second in ...

  18. Thomas Jefferson High School for Science & Technology National...

    Energy Savers [EERE]

    The team also won a research trip to Alaska, three Computer Based Laboratories and 1,000 for their school's science department. The team has won the national championship for four ...

  19. Jefferson Lab hosts 22 teams for Virginia High School Science Bowl on Feb.

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

    12 | Jefferson Lab hosts 22 teams for Virginia High School Science Bowl on Feb. 12 Science Bowl Click above for print version (tiff) of the Jefferson Lab Science Bowl logo. Jefferson Lab hosts 22 teams for Virginia High School Science Bowl on Feb. 12 February 1, 2005 Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 12, to compete in the Virginia Regional High School Science Bowl. Twenty-two teams, representing high

  20. High Energy Physics Advisory Panel (HEPAP) Homepage | U.S. DOE Office of

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

    Science (SC) HEPAP Home High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings 2016 HEPAP Membership Charges/Reports Charter .pdf file (44KB) HEP Committees of Visitors Federal Advisory Committees HEP Home Print Text Size: A A A FeedbackShare Page P5 Final Report Building for Discovery The Particle Physics Project Prioritization Panel (P5), a subpanel of the High Energy Physics Advisory Panel (HEPAP), has now completed its Report, a ten-year strategic plan for high energy physics in

  1. Yale High Energy Physics Research: Precision Studies of Reactor Antineutrinos

    SciTech Connect (OSTI)

    Heeger, Karsten M.

    2014-09-13

    This report presents experimental research at the intensity frontier of particle physics with particular focus on the study of reactor antineutrinos and the precision measurement of neutrino oscillations. The experimental neutrino physics group of Professor Heeger and Senior Scientist Band at Yale University has had leading responsibilities in the construction and operation of the Daya Bay Reactor Antineutrino Experiment and made critical contributions to the discovery of non-zero$\\theta_{13}$. Heeger and Band led the Daya Bay detector management team and are now overseeing the operations of the antineutrino detectors. Postdoctoral researchers and students in this group have made leading contributions to the Daya Bay analysis including the prediction of the reactor antineutrino flux and spectrum, the analysis of the oscillation signal, and the precision determination of the target mass yielding unprecedented precision in the relative detector uncertainty. Heeger's group is now leading an R\\&D effort towards a short-baseline oscillation experiment, called PROSPECT, at a US research reactor and the development of antineutrino detectors with advanced background discrimination.

  2. Thomas Jefferson High School for Science & Technology Takes 2015...

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

    physics and energy use to chemistry, geology, plant biology, cellular physiology and ... a team trophy, individual medals and the regional banner that the team will carry to ...

  3. Twenty-one high school teams compete in Virginia Regional Science Bowl

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

    hosted by Jefferson Lab | Jefferson Lab Twenty-one high school teams compete in Virginia Regional Science Bowl hosted by Jefferson Lab MEDIA ADVISORY: Twenty-one high school teams compete in Virginia Regional Science Bowl hosted by Jefferson Lab February 4, 2003 The Department of Energy's Thomas Jefferson National Accelerator Facility (Jefferson Lab) in Newport News, Va., is hosting this year's Virginia Regional Science Bowl on Saturday, February 8, 2003. Twenty-one teams, representing high

  4. La Cueva High School team takes top award in 23rd New Mexico Supercomputing

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

    Challenge 23rd New Mexico Supercomputing Challenge La Cueva High School team takes top award in 23rd New Mexico Supercomputing Challenge The team, Ari Echt-Wilson, Eli Echt-Wilson, and Justin Sanchez also won the CHECS Teamwork and Cray High Performance Computing awards. April 23, 2013 Justin Sanchez of Albuquerque La Cueva High School during the finalist team judging at the New Mexico Supercomputing Challenge expo and awards ceremony at Los Alamos National Laboratory. The styrofoam balls

  5. High Energy Physics: Report of research accomplishments and future goals, FY 1992

    SciTech Connect (OSTI)

    1991-09-05

    This report discusses high energy physics research in the following areas: Research in theoretical physics; phenomenology; experimental computer facility at Caltech; Beijing BES; MACRO; CLEO II; SLD; L3 at LEP; the B Factory R & D Program; SSC GEM Detector; and a high resolution barium fluoride calorimeter for the SSC.

  6. UVA experimental and high energy physics. Final grant report

    SciTech Connect (OSTI)

    Cox, B.

    1999-10-07

    The period 1992--1997 was a mixture of frustrations and of accomplishments for the UVa HEP group. The experimental HEP group began this period with the completion of a truncated run of Experiment E771 at Fermilab in 1992. This experiment was designed to measure the cross section for beauty production in 800 GeV/c pN interactions. It succeeded in this goal as well as in obtaining one of the best limits on FCNC in charm decays by setting an upper limit on D{sup 0} {r_arrow} {mu}{sup +}{mu}{sup {minus}}. In addition, they were able to measure {Psi}, {Psi}, {chi}{sub 1},{chi}{sub 2} and upsilon production. Three UVa PhD theses have resulted from this experiment (as well as 12 other PhD's at other institutions). At the same time, the UVa experimental group was vigorously pursuing the goal of studying CP violation in B production. This took the form of a proposal to the SSC for a super fixed target facility, the SFT, which would focus on studies of B mesons. B. Cox was the spokesman of this experiment that had over thirty institutions. This proposal EOI-14 had a good reception by the SSC PAC. A R and D activity to prove the technique of crystal channeling was undertaken to prove the accelerator aspects of this proposal. This activity, known as E853 or CEX at Fermilab, resulted in proof of the crystal channeling technique as viable for the extraction of 20 TeV beam at the SSC. In addition to this activity, the UVa group investigated many other aspects of B physics at the SSC. They were among the leaders of the 1993 Snowmass meeting on B Physics at Hadronic Accelerators. The UVa HEP group worked vigorously on developing the ideas for B physics at the SSC, as evidenced by the many different studies listed in the publication list given, up to the very day the SSC was terminated by an act of Congress.

  7. High School Girls Honored for Math, Science Achievements at Sandia National Laboratory

    Broader source: Energy.gov [DOE]

    Now in its 23rd year, the Math and Science Awards program is sponsored by the Sandia Women’s Connection. This year’s event honored more students, with the addition of four high schools in Oakland, Calif., and included recognition of the students by federal and state officials. Teachers from 15 high schools in Livermore, Dublin, Pleasanton, Tracy, Manteca and Oakland nominated high school juniors whom they deemed outstanding in math and science, so the students can include the award on college and scholarship applications.

  8. Jefferson Lab Hosts High School Science Bowl on Feb. 27 | Jefferson Lab

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

    27 Jefferson Lab Hosts High School Science Bowl on Feb. 27 Please note the date change from Feb. 6 to Saturday, Feb. 27 NEWPORT NEWS, Va., Feb. 5, 2010 - Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 27, to compete in the Virginia Regional High School Science Bowl. Teams from 20 high schools from across the region are registered for this year's academic competition. The National Science Bowl tournament - sponsored by

  9. Jefferson Lab Hosts High School Science Bowl on Feb. 4 | Jefferson Lab

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

    4 Jefferson Lab Hosts High School Science Bowl on Feb. 4 NEWPORT NEWS, Va., Jan. 31. , 2012 - Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 4, to compete in the Virginia Regional High School Science Bowl. Teams from 22 high schools from across the region are registered for this year's academic competition. The National Science Bowl tournament - sponsored by the U.S. Department of Energy since 1991 - is an annual

  10. Jefferson Lab Hosts High School Science Bowl on Feb. 5 | Jefferson Lab

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

    5 Jefferson Lab Hosts High School Science Bowl on Feb. 5 NEWPORT NEWS, Va., Feb. 2, 2011 - Some of the brightest young minds in the Commonwealth will meet at the Department of Energy's Jefferson Lab on Saturday, Feb. 5, to compete in the Virginia Regional High School Science Bowl. Teams from 23 high schools from across the region are registered for this year's academic competition. The National Science Bowl tournament - sponsored by the U.S. Department of Energy since 1991 - is an annual

  11. Experimental High Energy Physics Research: Direct Detection of Dark Matter

    SciTech Connect (OSTI)

    Witherell, Michael S.

    2014-10-02

    The grant supported research on an experimental search for evidence of dark matter interactions with normal matter. The PI carried out the research as a member of the LUX and LZ collaborations. The LUX research team collected a first data set with the LUX experiment, a large liquid xenon detector installed in the Sanford Underground Research Facility (SURF). The first results were published in Physical Review Letters on March 4, 2014. The journal Nature named the LUX result a scientific highlight of the year for 2013. In addition, the LZ collaboration submitted the full proposal for the Lux Zeplin experiment, which has since been approved by DOE-HEP as a second-generation dark matter experiment. Witherell is the Level 2 manager for the Outer Detector System on the LUX-Zeplin experiment.

  12. High energy physics advisory panel`s composite subpanel for the assessment of the status of accelerator physics and technology

    SciTech Connect (OSTI)

    1996-05-01

    In November 1994, Dr. Martha Krebs, Director of the US Department of Energy (DOE) Office of Energy Research (OER), initiated a broad assessment of the current status and promise of the field of accelerator physics and technology with respect to five OER programs -- High Energy Physics, Nuclear Physics, Basic Energy Sciences, Fusion Energy, and Health and Environmental Research. Dr. Krebs asked the High Energy Physics Advisory Panel (HEPAP) to establish a composite subpanel with representation from the five OER advisory committees and with a balance of membership drawn broadly from both the accelerator community and from those scientific disciplines associated with the OER programs. The Subpanel was also charged to provide recommendations and guidance on appropriate future research and development needs, management issues, and funding requirements. The Subpanel finds that accelerator science and technology is a vital and intellectually exciting field. It has provided essential capabilities for the DOE/OER research programs with an enormous impact on the nation`s scientific research, and it has significantly enhanced the nation`s biomedical and industrial capabilities. Further progress in this field promises to open new possibilities for the scientific goals of the OER programs and to further benefit the nation. Sustained support of forefront accelerator research and development by the DOE`s OER programs and the DOE`s predecessor agencies has been responsible for much of this impact on research. This report documents these contributions to the DOE energy research mission and to the nation.

  13. Calloway Middle School Honored at DOE National Science Bowl, Lone Oak Competes Among High Schools

    Broader source: Energy.gov [DOE]

    PADUCAH, KY – Calloway County Middle School won the Civility Award and was named one of the top six battery-powered model car design teams at the Department of Energy’s National Science Bowl in Washington, D.C.

  14. Santa Monica High School From Santa Monica, Calif. Wins U.S....

    Energy Savers [EERE]

    Wins U.S. Department of Energy National Science Bowl Santa Monica High School From Santa Monica, Calif. Wins U.S. Department of Energy National Science Bowl May 5, 2008 - ...

  15. OSTIblog Articles in the high school Topic | OSTI, US Dept of...

    Office of Scientific and Technical Information (OSTI)

    high school Topic Where Do New Scientists Come From? by Philip Ellis 07 Feb, 2013 in ... Thus the reality is that "new" scientists come from the general public fortuitously, and ...

  16. Thomas Jefferson High School Wins Virginia Science Bowl for 7th...

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

    NEWPORT NEWS, Va., Feb. 20, 2008 - The Thomas Jefferson High School for Science and Technology team pummeled its competition at the Virginia Regional Science Bowl held Feb. 2 at...

  17. NREL: News - Students From Smoky Hill High School Triumph in...

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

    In the final round of rapid-fire questions and answers about physics, math, biology, ... the National Science Bowl 12 years ago to help stimulate interest in science and math. ...

  18. High School Students Gear Up for Battle of the Brains - News Releases |

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

    NREL High School Students Gear Up for Battle of the Brains February 3, 2003 Golden, CO. - In what part of the chloroplast is carbon fixed during the Calvin cycle? Yellow fever is transmitted by what genus of mosquito? High school students from across Colorado will face such questions as they test their mental agility in the U.S. Department of Energy's (DOE) Colorado Science Bowl on Feb. 8 at the Colorado School of Mines in Golden. Thirty-nine teams from across the state will compete in this

  19. High School Students Gear Up for Battle of the Brains - News Releases |

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

    NREL High School Students Gear Up for Battle of the Brains January 30, 2004 Golden, Colo. - The Andes Mountains of South America were formed at what kind of margin? How many prime numbers are there between 30 and 60? High school students from across Colorado will face such questions as they test their mental agility in the U.S. Department of Energy's (DOE) Colorado Science Bowl on Feb. 7 at the Colorado School of Mines in Golden. Forty teams will compete in this rapid-fire

  20. Manzano High School student wins top award in 22nd New Mexico

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

    Supercomputing Challenge Manzano High School student wins Supercomputing Challenge Manzano student wins top award in 22nd New Mexico Supercomputing Challenge Jordan Medlock wins for his computer algorithm. April 24, 2012 Jordan Medlock Jordan Medlock Contact Steve Sandoval Communications Office (505) 665-9206 Email LOS ALAMOS, New Mexico, April 24, 2012-Jordan Medlock of Albuquerque's Manzano High School took the top prize in the 22nd New Mexico Supercomputing Challenge for his computer

  1. D.C. Middle and High School Students Get a Chance to Experience the

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

    Regional Science Bowl Competition Setting | Department of Energy D.C. Middle and High School Students Get a Chance to Experience the Regional Science Bowl Competition Setting D.C. Middle and High School Students Get a Chance to Experience the Regional Science Bowl Competition Setting March 26, 2014 - 1:07pm Addthis Annie Whatley Annie Whatley Deputy Director, Office of Minority Education and Community Development Have you ever heard of the Washington, D.C. regional science bowl competition?

  2. US Department of Energy High School Student Supercomputing Honors Program: A follow-up assessment

    SciTech Connect (OSTI)

    Not Available

    1987-01-01

    The US DOE High School Student Supercomputing Honors Program was designed to recognize high school students with superior skills in mathematics and computer science and to provide them with formal training and experience with advanced computer equipment. This document reports on the participants who attended the first such program, which was held at the National Magnetic Fusion Energy Computer Center at the Lawrence Livermore National Laboratory (LLNL) during August 1985.

  3. Portsmouth Site Tour Focuses on Potential Careers for High School Graduates

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

    | Department of Energy Portsmouth Site Tour Focuses on Potential Careers for High School Graduates Portsmouth Site Tour Focuses on Potential Careers for High School Graduates July 28, 2016 - 12:20pm Addthis A teachers group organized by the Buckeye Hills Career Center prepares for a driving tour of the Portsmouth Site. A teachers group organized by the Buckeye Hills Career Center prepares for a driving tour of the Portsmouth Site. Area teachers talk with officials at the Portsmouth Site

  4. DIAGNOSTICS FOR ION BEAM DRIVEN HIGH ENERGY DENSITY PHYSICS EXPERIMENTS

    SciTech Connect (OSTI)

    Bieniosek, F.M.; Henestroza, E.; Lidia, S.; Ni, P.A.

    2010-01-04

    Intense beams of heavy ions are capable of heating volumetric samples of matter to high energy density. Experiments are performed on the resulting warm dense matter (WDM) at the NDCX-I ion beam accelerator. The 0.3 MeV, 30-mA K{sup +} beam from NDCX-I heats foil targets by combined longitudinal and transverse neutralized drift compression of the ion beam. Both the compressed and uncompressed parts of the NDCX-I beam heat targets. The exotic state of matter (WDM) in these experiments requires specialized diagnostic techniques. We have developed a target chamber and fielded target diagnostics including a fast multi-channel optical pyrometer, optical streak camera, laser Doppler-shift interferometer (VISAR), beam transmission diagnostics, and high-speed gated cameras. We also present plans and opportunities for diagnostic development and a new target chamber for NDCX-II.

  5. High Frequency Physics-Based Earthquake System Simulations | Argonne

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

    Leadership Computing Facility Ground motion simulations reveal regions at risk of strong shaking during a possible magnitude-8 earthquake on the San Andreas fault Ground motion simulations reveal regions at risk of strong shaking during a possible magnitude-8 earthquake on the San Andreas fault. For the CyberShake project, reciprocal simulations of all known possible quakes are combined to estimate the total probabilistic hazard for California. Geoffrey Ely, Argonne National Laboratory High

  6. High School Girls Honored for Math, Science Achievements

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

    School Girls Honored for Math, Science Achievements - 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 Defense Waste

  7. RF physics of ICWC discharge at high cyclotron harmonics

    SciTech Connect (OSTI)

    Lyssoivan, A.; Van Eester, D.; Wauters, T.; Vervier, M.; Van Schoor, M.; Bobkov, V.; Rohde, V.; Schneider, P.; Douai, D.; Kogut, D.; Kreter, A.; Möller, S.; Philipps, V.; Sergienko, G.; Moiseenko, V.; Noterdaeme, J.-M.; Collaboration: TEXTOR Team; ASDEX Upgrade Team

    2014-02-12

    Recent experiments on Ion Cyclotron Wall Conditioning (ICWC) performed in tokamaks TEXTOR and ASDEX Upgrade with standard ICRF antennas operated at fixed frequencies but variable toroidal magnetic field demonstrated rather contrasting parameters of ICWC discharge in scenarios with on-axis fundamental ion cyclotron resonance (ICR) for protons,ω=ω{sub H+}, and with its high cyclotron harmonics (HCH), ω=10ω{sub cH+}⋅ HCH scenario: very high antenna coupling to low density RF plasmas (P{sub pl}≈0.9P{sub RF-G}) and low energy Maxwellian distribution of CX hydrogen atoms with temperature T{sub H}≈350 eV. Fundamental ICR: lower antenna-plasma coupling efficiency (by factor of about 1.5 times) and generation of high energy non-Maxwellian CX hydrogen atoms (with local energy E{sub ⊥H} ≥1.0 keV). In the present paper, we analyze the obtained experimental results numerically using (i) newly developed 0-D transport code describing the process of plasma production with electron and ion collisional ionization in helium-hydrogen gas mixture and (ii) earlier developed 1-D Dispersion Relation Solver accounting for finite temperature effects and collision absorption mechanisms for all plasma species in addition to conventionally examined Landau/TTPM damping for electrons and cyclotron absorption for ions. The numerical study of plasma production in helium with minor hydrogen content in low and high toroidal magnetic fields is presented. The investigation of the excitation, conversion and absorption of plasma waves as function of B{sub T}-field suggests that only fast waves (FW) may give a crucial impact on antenna coupling and characteristics of the ICWC discharge using standard poloidally polarized ICRF antennas designed to couple RF power mainly to FW. The collisional (non-resonant) absorption by electrons and ions and IC absorption by resonant ions of minor concentration in low T{sub e} plasmas is studied at fundamental ICR and its high harmonics.

  8. High Energy Physics Advisory Panel April 6-7, 2015 | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) April 6-7, 2015 High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings Previous Meetings 2016 HEPAP Membership Charges/Reports Charter .pdf file (44KB) HEP Committees of Visitors Federal Advisory Committees HEP Home Meetings High Energy Physics Advisory Panel April 6-7, 2015 Print Text Size: A A A FeedbackShare Page DOE Logo NSF Logo U.S Department of Energy and the National Science Foundation Agenda .pdf file (95KB) High Energy Physics Advisory Panel Washington Marriott

  9. High Energy Physics Advisory Panel December 9-11, 2015 | U.S. DOE Office of

    Office of Science (SC) Website

    Science (SC) December 9-11, 2015 High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings Previous Meetings 2016 HEPAP Membership Charges/Reports Charter .pdf file (44KB) HEP Committees of Visitors Federal Advisory Committees HEP Home Meetings High Energy Physics Advisory Panel December 9-11, 2015 Print Text Size: A A A FeedbackShare Page DOE Logo NSF Logo U.S Department of Energy and the National Science Foundation Agenda .pdf file (86KB) High Energy Physics Advisory Panel Newport

  10. High Energy Physics Advisory Panel March 31 - April 1, 2016 | U.S. DOE

    Office of Science (SC) Website

    Office of Science (SC) March 31 - April 1, 2016 High Energy Physics Advisory Panel (HEPAP) HEPAP Home Meetings Previous Meetings 2016 HEPAP Membership Charges/Reports Charter .pdf file (44KB) HEP Committees of Visitors Federal Advisory Committees HEP Home Meetings High Energy Physics Advisory Panel March 31 - April 1, 2016 Print Text Size: A A A FeedbackShare Page DOE Logo NSF Logo U.S Department of Energy and the National Science Foundation Agenda .pdf file (81KB) High Energy Physics

  11. HIGH ENERGY DENSITY PHYSICS EXPERIMENTS WITH INTENSE HEAVY ION BEAMS

    SciTech Connect (OSTI)

    Henestroza, E.; Leitner, M.; Logan, B.G.; More, R.M.; Roy, P.K.; Ni, P.; Seidl, P.A.; Waldron, W.L.; Barnard, J.J.

    2010-03-16

    The US heavy ion fusion science program has developed techniques for heating ion-beam-driven warm dense matter (WDM) targets. The WDM conditions are to be achieved by combined longitudinal and transverse space-charge neutralized drift compression of the ion beam to provide a hot spot on the target with a beam spot size of about 1 mm, and pulse length about 1-2 ns. As a technique for heating volumetric samples of matter to high energy density, intense beams of heavy ions are capable of delivering precise and uniform beam energy deposition dE/dx, in a relatively large sample size, and the ability to heat any solid-phase target material. Initial experiments use a 0.3 MeV K+ beam (below the Bragg peak) from the NDCX-I accelerator. Future plans include target experiments using the NDCX-II accelerator, which is designed to heat targets at the Bragg peak using a 3-6 MeV lithium ion beam. The range of the beams in solid matter targets is about 1 micron, which can be lengthened by using porous targets at reduced density. We have completed the fabrication of a new experimental target chamber facility for WDM experiments, and implemented initial target diagnostics to be used for the first target experiments in NDCX-1. The target chamber has been installed on the NDCX-I beamline. The target diagnostics include a fast multi-channel optical pyrometer, optical streak camera, VISAR, and high-speed gated cameras. Initial WDM experiments will heat targets by compressed NDCX-I beams and will explore measurement of temperature and other target parameters. Experiments are planned in areas such as dense electronegative targets, porous target homogenization and two-phase equation of state.

  12. HIGH ENERGY DENSITY PHYSICS EXPERIMENTS WITH INTENSE HEAVY ION BEAMS

    SciTech Connect (OSTI)

    Bieniosek, F.M.; Henestroza, E.; Leitner, M.; Logan, B.G.; More, R.M.; Roy, P.K.; Ni, P.; Seidl, P.A.; Waldron, W.L.; Barnard, J.J.

    2008-08-01

    The US heavy ion fusion science program has developed techniques for heating ion-beam-driven warm dense matter (WDM) targets. The WDM conditions are to be achieved by combined longitudinal and transverse space-charge neutralized drift compression of the ion beam to provide a hot spot on the target with a beam spot size of about 1 mm, and pulse length about 1-2 ns. As a technique for heating volumetric samples of matter to high energy density, intense beams of heavy ions are capable of delivering precise and uniform beam energy deposition dE/dx, in a relatively large sample size, and the ability to heat any solid-phase target material. Initial experiments use a 0.3 MeV K+ beam (below the Bragg peak) from the NDCX-I accelerator. Future plans include target experiments using the NDCX-II accelerator, which is designed to heat targets at the Bragg peak using a 3-6 MeV lithium ion beam. The range of the beams in solid matter targets is about 1 micron, which can be lengthened by using porous targets at reduced density. We have completed the fabrication of a new experimental target chamber facility for WDM experiments, and implemented initial target diagnostics to be used for the first target experiments in NDCX-1. The target chamber has been installed on the NDCX-I beamline. The target diagnostics include a fast multi-channel optical pyrometer, optical streak camera, VISAR, and high-speed gated cameras. Initial WDM experiments will heat targets by compressed NDCX-I beams and will explore measurement of temperature and other target parameters. Experiments are planned in areas such as dense electronegative targets, porous target homogenization and two-phase equation of state.

  13. Ion Desorption Stability in Superconducting High Energy Physics Proton Colliders

    SciTech Connect (OSTI)

    Turner, W.C.

    1995-05-29

    of the diagonal uncoupled feedback loops are first order in the ion desorption coefficients whereas the gains of the off diagonal coupled feedback loops are second and higher order. For this reason it turns out that in practical cases stability is dominated by the uncoupled diagonal elements and the inverse of the largest first order closed loop gain is a useful estimate of the margin of stability. In contrast to the case of a simple cold beam tube, the stability condition for a beam screen does not contain the desorption coefficient for physisorbed molecules, even when the screen temperature is low enough that there is a finite surface density of them on the screen surface. Consequently there does not appear to be any particular advantage to operating the beam screen at high enough temperature to avoid physisorption. Numerical estimates of ion desorption stability are given for a number of cases relevant to LHC and all of the ones likely to be encountered were found to be stable. The most important case, a I % transparency beam screen at {approx}4.2 K, was found to have a stability safety margin of approximately thirty determined by ion desorption of CO. Ion desorption of H{sub 2} is about a factor of eighty less stringent than CO. For these estimates the beam tube surface was assumed to be solvent cleaned but otherwise untreated, for example by a very high temperature vacuum bakeout or by glow discharge cleaning.

  14. Exploration of Plasma Jets Approach to High Energy Density Physics. Final report

    SciTech Connect (OSTI)

    Chen, Chiping

    2013-08-26

    High-energy-density laboratory plasma (HEDLP) physics is an emerging, important area of research in plasma physics, nuclear physics, astrophysics, and particle acceleration. While the HEDLP regime occurs at extreme conditions which are often found naturally in space but not on the earth, it may be accessible by colliding high intensity plasmas such as high-energy-density plasma jets, plasmoids or compact toroids from plasma guns. The physics of plasma jets is investigated in the context of high energy density laboratory plasma research. This report summarizes results of theoretical and computational investigation of a plasma jet undergoing adiabatic compression and adiabatic expansion. A root-mean-squared (rms) envelope theory of plasma jets is developed. Comparison between theory and experiment is made. Good agreement between theory and experiment is found.

  15. Used MRI magnets get a second chance at life in high-energy physics...

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

    high-energy and nuclear physics experiments. The two new magnets have a strength of 4 Tesla, not as strong as the newest generation of MRI magnets but ideal for benchmarking ...

  16. High-Z Non-Equilibrium Physics and Bright X-ray Sources with...

    Office of Scientific and Technical Information (OSTI)

    X-ray Sources with New Laser Targets Citation Details In-Document Search Title: High-Z Non-Equilibrium Physics and Bright X-ray Sources with New Laser Targets You are ...

  17. High Energy Physics (HEP) Homepage | U.S. DOE Office of Science (SC)

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

    Programs » HEP Home High Energy Physics (HEP) HEP Home About Research Facilities Science Highlights Benefits of HEP Funding Opportunities Advisory Committees Community Resources Contact Information High Energy Physics U.S. Department of Energy SC-25/Germantown Building 1000 Independence Ave., SW Washington, DC 20585 P: (301) 903-3624 F: (301) 903-2597 E: Email Us More Information » Intermediate Neutrino Research Program Awards ANNIE External link and PROSPECT External link will investigate the

  18. Accelerator physics and technology challenges of very high energy hadron colliders

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

    Shiltsev, Vladimir D.

    2015-08-20

    High energy hadron colliders have been in the forefront of particle physics for more than three decades. At present, international particle physics community considers several options for a 100 TeV proton–proton collider as a possible post-LHC energy frontier facility. The method of colliding beams has not fully exhausted its potential but has slowed down considerably in its progress. This article briefly reviews the accelerator physics and technology challenges of the future very high energy colliders and outlines the areas of required research and development towards their technical and financial feasibility.

  19. Special Colloquium : Looking at High Energy Physics from a gender studies perspective

    ScienceCinema (OSTI)

    None

    2011-04-25

    Human actors, workplace cultures and knowledge production: Gender studies analyse the social constructions and cultural representations of gender. Using methods and tools from the humanities and social science, we look at all areas, including the natural sciences and technology, science education and research labs. After a short introduction to gender studies, the main focus of my talk will be the presentation of selected research findings on gender and high energy physics. You will hear about an ongoing research project on women in neutrino physics and learn about a study on the world of high energy physicists characterised by "rites of passage" and "male tales" told during a life in physics. I will also present a study on how the HEP community communicates, and research findings on the naming culture in HEP. Getting to know findings from another field on your own might contribute to create a high energy physics culture that is fair and welcoming to all genders.

  20. La Cueva High School team takes top award in 24th New Mexico Supercomputing

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

    Challenge 24th New Mexico Supercomputing Challenge La Cueva High School team takes top award in 24th New Mexico Supercomputing Challenge Eli Echt-Wilson and Albert Zuo from La Cueva High in Albuquerque won the top award at the 24th New Mexico Supercomputing Challenge. April 22, 2014 Albert Zuo, left, and Eli Echt-Wilson of Albuquerque La Cueva High School with their poster. They won the top award at the 24th New Mexico Supercomputing Challenge at Los Alamos National Laboratory. Albert Zuo,

  1. Biomass Company Sets Up Shop in High School Lab

    Broader source: Energy.gov [DOE]

    Unlike most biotechnology students who have to go to a research facility to see scientists in action, those at Greeneville High just need to turn their heads.

  2. Thomas Jefferson High School for Science & Technology Wins Feb...

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

    Wins Feb. 5 Virginia Science Bowl; Warwick High Wins Math and Science Challenges ... in science, technology, engineering and math among our nation's youth," Tyler said. "It ...

  3. Indiana University High Energy Physics, Task A. Technical progress report, 1992--1993

    SciTech Connect (OSTI)

    Brabson, B.; Crittenden, R.; Dzierba, A.

    1993-10-01

    This report discusses research at Indians University on the following high energy physics experiments: A search for mesons with unusual quantum numbers; hadronic states produced in association with high-mass dimuons; FNAL E740 (D0); superconducting super collider; and OPAL experiment at CERN.

  4. (The 25th international conference on high-energy physics at Singapore)

    SciTech Connect (OSTI)

    Plasil, F.

    1990-08-17

    The traveler attended the 25th International Conference on High-Energy Physics in Singapore, August 1--8, 1990. The conference was dominated by results from the new LEP accelerator at CERN. The precision of the data from LEP is impressive, and all results are consistent with the standard model. No new physics'' has emerged at LEP. The traveler presented a talk on CERN/SPS WA80 results and had several interesting, private discussions on both L* and WA80 topics.

  5. Texas A&M Regional High School Science Bowl | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Texas A&M Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About Regional Competitions Rules, Forms, and Resources High School Regionals Middle School Regionals National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us High School Regionals Texas A&M Regional High

  6. Physics Teachers Workshop

    ScienceCinema (OSTI)

    Huggins, DaNel; Calhoun, John; Palmer, Alyson; Thorpe, Steve; Vanderveen, Anne;

    2013-05-28

    INL is looking for the nation's top high school physics teachers to attend our July workshop in Idaho Falls. Participants get to learn from nuclear researchers, tour facilities including a research reactor and interact with peers from across the country. You can learn more about INL projects at http://www.facebook.com/idahonationallaboratory

  7. Physics Teachers Workshop

    SciTech Connect (OSTI)

    Huggins, DaNel; Calhoun, John; Palmer, Alyson; Thorpe, Steve; Vanderveen, Anne

    2011-01-01

    INL is looking for the nation's top high school physics teachers to attend our July workshop in Idaho Falls. Participants get to learn from nuclear researchers, tour facilities including a research reactor and interact with peers from across the country. You can learn more about INL projects at http://www.facebook.com/idahonationallaboratory

  8. Solar Energy Education. Renewable energy activities for junior high/middle school science

    SciTech Connect (OSTI)

    Not Available

    1985-01-01

    Some basic topics on the subject of solar energy are outlined in the form of a teaching manual. The manual is geared toward junior high or middle school science students. Topics include solar collectors, solar water heating, solar radiation, insulation, heat storage, and desalination. Instructions for the construction of apparatus to demonstrate the solar energy topics are provided. (BCS)

  9. About 900 High School Students, Educators Attend Third Annual DOE Science Alliance

    Broader source: Energy.gov [DOE]

    PIKETON, OH – The U.S. Department of Energy (DOE) welcomed about 900 high school juniors and educators for its third annual Science Alliance, a science fair that took place September 25-26, 2012, at the Portsmouth Gaseous Diffusion Plant.

  10. Discussing spent nuclear fuel in high school classrooms: addressing public fears through early education

    SciTech Connect (OSTI)

    Winkel, S.; Sullivan, J.; Jones, S.; Sullivan, K.; Hyland, B.; Pencer, J.; Colton, A.

    2013-07-01

    The Inreach program combines the Deep River Science Academy (DRSA) 'learning through research' approach with state of the art communication technology to bring scientific research to high school classrooms. The Inreach program follows the DRSA teaching model where a university student tutor works on a research project with scientific staff at AECL's Chalk River Laboratories. Participating high school classes are located across Canada. The high school students learn about the ongoing research activities via weekly web conferences. In order to engage the students and encourage participation in the conferences, themed exercises linked to the research project are provided to the students. The DRSA's Inreach program uses a cost-effective internet technology to reach a wide audience, in an interactive setting, without anyone leaving their desks or offices. An example Inreach research project is presented here: an investigation of the potential of the Canadian supercritical water cooled reactor (SCWR) concept to burn transuranic elements (Np, Pu, Am, Cm) to reduce the impact of used nuclear fuel. During this project a university student worked with AECL (Atomic Energy of Canada Limited) researchers on technical aspects of the project, and high school students followed their progress and learned about the composition, hazards, and disposition options for used nuclear fuel. Previous projects included the effects of tritium on cellular viability and neutron diffraction measurement of residual stresses in automobile engines.

  11. Characterization of spatially resolved high resolution x-ray spectrometers for high energy density physics and light source experiments

    SciTech Connect (OSTI)

    Hill, K. W. Bitter, M.; Delgado-Aparacio, L.; Efthimion, P.; Pablant, N. A.; Lu, J.; Beiersdorfer, P.; Chen, H.; Magee, E.

    2014-11-15

    A high resolution 1D imaging x-ray spectrometer concept comprising a spherically bent crystal and a 2D pixelated detector is being optimized for diagnostics of small sources such as high energy density physics (HEDP) and synchrotron radiation or x-ray free electron laser experiments. This instrument is used on tokamak experiments for Doppler measurements of ion temperature and plasma flow velocity profiles. Laboratory measurements demonstrate a resolving power, E/ΔE of order 10 000 and spatial resolution better than 10 μm. Initial tests of the high resolution instrument on HEDP plasmas are being performed.

  12. Status of networking for high energy physics in the United States

    SciTech Connect (OSTI)

    Kunz, P.F.

    1985-06-01

    Networks are used extensively for High Energy Physics in the United States. Although the networks have grown in an ad hoc manner with connections typically being made to satisfy the needs of one detector group, they now encompass to large fraction of the US HEP community in one form or another. This paper summarizes the current status and experience with networks.

  13. Recent results of high p(T) physics at the CDF II

    SciTech Connect (OSTI)

    Tsuno, Soushi; /Okayama U.

    2005-02-01

    The Tevatron Run II program has been in progress since 2001. The CDF experiment has accumulated roughly five times as much data as did Run I, with much improved detectors. Preliminary results from the CDF experiment are presented. The authors focus on recent high p{sub T} physics results in the Tevatron Run II program.

  14. Report of the Interagency Task Force on High Energy Density Physics

    SciTech Connect (OSTI)

    2007-08-01

    Identifies the needs for improving Federal stewardship of specific aspects of high energy density physics, particularly the study of high energy density plasmas in the laboratory, and strengthening university activities in this latter discipline. The report articulates how HEDP fits into the portfolio of federally funded missions and includes agency actions to be taken that are necessary to further this area of study consistent with Federal priorities and plans, while being responsive to the needs of the scientific community.

  15. Large-x connections of nuclear and high-energy physics

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

    Accardi, Alberto

    2013-11-20

    I discuss how global QCD fits of parton distribution functions can make the somewhat separated fields of high-energy particle physics and lower energy hadronic and nuclear physics interact to the benefit of both. I review specific examples of this interplay from recent works of the CTEQ-Jefferson Lab collaboration, including hadron structure at large parton momentum and gauge boson production at colliders. Particular attention is devoted to quantifying theoretical uncertainties arising in the treatment of large partonic momentum contributions to deep inelastic scattering observables, and to discussing the experimental progress needed to reduce these.

  16. Monochromatic radiography of high energy density physics experiments on the MAGPIE generator

    SciTech Connect (OSTI)

    Hall, G. N. Burdiak, G. C.; Suttle, L.; Stuart, N. H.; Swadling, G. F.; Lebedev, S. V.; Smith, R. A.; Patankar, S.; Suzuki-Vidal, F.; Grouchy, P. de; Harvey-Thompson, A. J.; Bennett, M.; Bland, S. N.; Pickworth, L.; Skidmore, J.

    2014-11-15

    A monochromatic X-ray backlighter based on Bragg reflection from a spherically bent quartz crystal has been developed for the MAGPIE pulsed power generator at Imperial College (1.4 MA, 240ns) [I. H. Mitchell et al., Rev. Sci. Instrum. 67, 1533 (2005)]. This instrument has been used to diagnose high energy density physics experiments with 1.865 keV radiation (Silicon He-?) from a laser plasma source driven by a ?7 J, 1 ns pulse from the Cerberus laser. The design of the diagnostic, its characterisation and performance, and initial results in which the instrument was used to radiograph a shock physics experiment on MAGPIE are discussed.

  17. Proceedings of the workshop on opportunities for atomic physics using slow, highly-charged ions

    SciTech Connect (OSTI)

    Not Available

    1987-01-01

    The study of atomic physics with highly-charged ions is an area of intense activity at the present time because of a convergence of theoretical interest and advances in experimental techniques. The purpose of the Argonne ''Workshop on Opportunities for Atomic Physics Using Slow, Highly-Charged Ions'' was to bring together atomic, nuclear, and accelerator physicists in order to identify what new facilities would be most useful for the atomic physics community. The program included discussion of existing once-through machines, advanced ion sources, recoil ion techniques, ion traps, and cooler rings. One of the topics of the Workshop was to discuss possible improvement to the ANL Tandem-Linac facility (ATLAS) to enhance the capability for slowing down ions after they are stripped to a high-charge state (the Accel/Decel technique). Another topic was the opportunity for atomic physics provided by the ECR ion source which is being built for the Uranium Upgrade of ATLAS. 18 analytics were prepared for the individual papers in this volume.

  18. Santa Monica High School From Santa Monica, Calif. Wins U.S. Department of Energy National Science Bowl®

    Broader source: Energy.gov [DOE]

    WASHINGTON, DC - The U.S. Department of Energy (DOE) today announced that Santa Monica High School from Santa Monica, Calif. is the winner of the 2008 DOE National Science Bowl®.  Santa Monica High...

  19. Plasma physics and related challenges of millimeter-wave-to-terahertz and high power microwave generation

    SciTech Connect (OSTI)

    Booske, John H.

    2008-05-15

    Homeland security and military defense technology considerations have stimulated intense interest in mobile, high power sources of millimeter-wave (mmw) to terahertz (THz) regime electromagnetic radiation, from 0.1 to 10 THz. While vacuum electronic sources are a natural choice for high power, the challenges have yet to be completely met for applications including noninvasive sensing of concealed weapons and dangerous agents, high-data-rate communications, high resolution radar, next generation acceleration drivers, and analysis of fluids and condensed matter. The compact size requirements for many of these high frequency sources require miniscule, microfabricated slow wave circuits. This necessitates electron beams with tiny transverse dimensions and potentially very high current densities for adequate gain. Thus, an emerging family of microfabricated, vacuum electronic devices share many of the same plasma physics challenges that are currently confronting 'classic' high power microwave (HPM) generators including long-life bright electron beam sources, intense beam transport, parasitic mode excitation, energetic electron interaction with surfaces, and rf air breakdown at output windows. The contemporary plasma physics and other related issues of compact, high power mmw-to-THz sources are compared and contrasted to those of HPM generation, and future research challenges and opportunities are discussed.

  20. P24 Plasma Physics Summer School 2012 Los Alamos National Laboratory Summer lecture series for students

    SciTech Connect (OSTI)

    Intrator, Thomas P.; Bauer, Bruno; Fernandez, Juan C.; Daughton, William S.; Flippo, Kirk A.; Weber, Thomas; Awe, Thomas J.; Kim, Yong Ho

    2012-09-07

    This report covers the 2012 LANL summer lecture series for students. The lectures were: (1) Tom Intrator, P24 LANL: Kick off, Introduction - What is a plasma; (2) Bruno Bauer, Univ. Nevada-Reno: Derivation of plasma fluid equations; (3) Juan Fernandez, P24 LANL Overview of research being done in p-24; (4) Tom Intrator, P24 LANL: Intro to dynamo, reconnection, shocks; (5) Bill Daughton X-CP6 LANL: Intro to computational particle in cell methods; (6) Kirk Flippo, P24 LANL: High energy density plasmas; (7) Thom Weber, P24 LANL: Energy crisis, fission, fusion, non carbon fuel cycles; (8) Tom Awe, Sandia National Laboratory: Magneto Inertial Fusion; and (9) Yongho Kim, P24 LANL: Industrial technologies.

  1. Summer Schools

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

    Program Offices Energy Security Council New Mexico Consortium Coordination Office Postdoc Program Students/Internships Centers, Institutes Center for Nonlinear Studies Engineering Institute Information Science & Technology Institute Center for Space and Earth Science Institute for Materials Science Seaborg Institute Summer Schools Engineering Institute Institute of Geophysics, Planetary Physics, Signatures Events NSEC » Summer Schools Summer Schools Offering various 8 to 12-week programs

  2. High energy-density physics: From nuclear testing to the superlasers

    SciTech Connect (OSTI)

    Campbell, E.M.; Holmes, N.C.; Libby, S.B.; Remington, B.A.; Teller, E.

    1995-10-20

    We describe the role for the next-generation ``superlasers`` in the study of matter under extremely high energy density conditions, in comparison to previous uses of nuclear explosives for this purpose. As examples, we focus on three important areas of physics that have unresolved issues which must be addressed by experiment: Equations of state, hydrodynamic mixing, and the transport of radiation. We will describe the advantages the large lasers will have in a comprehensive experimental program.

  3. High School Academic Competition - Round Robin | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Round Robin National Science Bowl® (NSB) NSB Home About Regional Science Bowl Coordinators Alumni Historical Information - National Finals National Science Bowl Logos Regional Competitions National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us 2013 Competition Results High School Academic

  4. High School Academic Competition - Round Robin | U.S. DOE Office of Science

    Office of Science (SC) Website

    (SC) Round Robin National Science Bowl® (NSB) NSB Home About Regional Science Bowl Coordinators Alumni Historical Information - National Finals National Science Bowl Logos Regional Competitions National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 E: Email Us 2014 Competition Results High School Academic

  5. Past High School National Science Bowl Winners (1991 - 2014) | U.S. DOE

    Office of Science (SC) Website

    Office of Science (SC) High School National Science Bowl Winners (1991 - 2015) National Science Bowl® (NSB) NSB Home About Regional Science Bowl Coordinators Alumni Historical Information - National Finals National Science Bowl Logos Regional Competitions National Finals Volunteers Key Dates Frequently Asked Questions News Media Contact Us WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585

  6. Thomas Jefferson High School Wins Virginia Science Bowl for 7th Year

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

    Running | Jefferson Lab Wins Virginia Science Bowl for 7th Year Running NEWPORT NEWS, Va., Feb. 20, 2008 - The Thomas Jefferson High School for Science and Technology team pummeled its competition at the Virginia Regional Science Bowl held Feb. 2 at Jefferson Lab. The team finished the day winning all of its matches. This marked the seventh time since Jefferson Lab has been hosting this annual event that the Thomas Jefferson team, from Alexandria, took the regional title. Eighteen teams

  7. US/Japan Cooperation in High Energy Physics. Review of activities, 1988--1993

    SciTech Connect (OSTI)

    Not Available

    1993-11-16

    The objective of the Implementing Arrangement was to further the energy programs of both countries by establishing a framework for cooperation in the field of high energy physics, including research, accelerator and detector instrumentation research and development, the fabrication and subsequent use of new experimental devices and facilities, and related joint efforts as may be mutually agreed. Over the years, this cooperation has been very effective and has strengthened the overall collaborative efforts and the understanding between our nations and their citizens. It has demonstrated to the world our ability to work together to attack difficult problems. High Energy Physics goes across national borders; the bond is clearly intellectual and common ground is shared for the benefit of all in a most effective manner. This review covers the activities conducted under the aegis of the US/Japan Committee for Cooperation in High Energy Physics during the past five years (1988--1993). This was the second such US review of the US/Japan cooperative activities; the first was held in 1987.

  8. Proceedings of RIKEN BNL Research Center Workshop: Progress in High-pT Physics at RHIC

    SciTech Connect (OSTI)

    Bazilevsky, A.; Bland, L.; Vogelsang, W.

    2010-03-17

    This volume archives the presentations at the RIKEN BNL Research Center workshop 'Progress in High-PT Physics at RHIC', held at BNL in March 2010. Much has been learned from high-p{sub T} physics after 10 years of RHIC operations for heavy-ion collisions, polarized proton collisions and d+Au collisions. The workshop focused on recent progress in these areas by both theory and experiment. The first morning saw review talks on the theory of RHIC high-p{sub T} physics by G. Sterman and J. Soffer, and on the experimental results by M. Tannenbaum. One of the most exciting recent results from the RHIC spin program is the first observation of W bosons and their associated single-spin asymmetry. The new preliminary data were reported on the first day of our workshop, along with a theoretical perspective. There also were detailed discussions on the global analysis of polarized parton distributions, including the knowledge on gluon polarization and the impact of the W-data. The main topic of the second workshop day were single-transverse spin asymmetries and their analysis in terms of transverse-momentum dependent parton distributions. There is currently much interest in a future Drell-Yan program at RHIC, thanks to the exciting physics opportunities this would offer. This was addressed in some of the talks. There also were presentations on the latest results on transverse-spin physics from HERMES and BELLE. On the final day of the workshop, the focus shifted toward forward and small-x physics at RHIC, which has become a cornerstone of the whole RHIC program. Exciting new data were presented and discussed in terms of their possible implications for our understanding of strong color-field phenomena in QCD. In the afternoon, there were discussions of nuclear parton distributions and jet observables, among them fragmentation. The workshop was concluded with outlooks toward the near-term (LHC, JLab) and longer-term (EIC) future. The workshop has been a great success. We had

  9. Final Report for Research in High Energy Physics (University of Hawaii)

    SciTech Connect (OSTI)

    Browder, Thomas E.

    2013-08-31

    Here we present a final report for the DOE award for the University of Hawaii High Energy Physics Group (UHHEPG) for the period from December 1, 2009 to May 31, 2013 (including a period of no-cost extension). The high energy physics (HEP) group at the University of Hawaii (UH) has been engaged in experiments at the intensity frontier studying flavor physics (Task A: Belle, Belle-II and Task B: BES) and neutrinos (Task C: SuperK, LBNE, Double Chooz, DarkSide, and neutrino R\\&D). On the energy frontier, new types of pixel detectors were developed for upgrades of the ATLAS experiment at the LHC (Task D). On the cosmic frontier, there were investigations of ultra high-energy neutrino astrophysics and the highest energy cosmic rays using special radio detection techniques (Task E: AMBER, ANITA R\\&D) and results of the analysis of ANITA data. In addition, we have developed new types of sophisticated and cutting edge instrumentation based on novel ``oscilloscope on a chip'' electronics (Task F). Theoretical physics research (Task G) is phenomenologically oriented and has studied experimental consequences of existing and proposed new theories relevant to the energy, cosmic and intensity frontiers. The senior investigators for proposal were T. E. Browder (Task A), F. A. Harris (Task B), P. Gorham (Task E), J. Kumar (Task G), J. Maricic (Task C), J. G. Learned (Task C), S. Pakvasa (Task G), S. Parker (Task D), S. Matsuno (Task C), X. Tata (Task G) and G. S. Varner (Tasks F, A, E).

  10. HIGH-RESOLUTION OBSERVATIONS AND THE PHYSICS OF HIGH-VELOCITY CLOUD A0

    SciTech Connect (OSTI)

    Verschuur, Gerrit L.

    2013-04-01

    The neutral hydrogen structure of high-velocity cloud A0 (at about -180 km s{sup -1}) has been mapped with a 9.'1 resolution. Gaussian decomposition of the profiles is used to separately map families of components defined by similarities in center velocities and line widths. About 70% of the H I gas is in the form of a narrow, twisted filament whose typical line widths are of the order of 24 km s{sup -1}. Many bright features with narrow line widths of the order of 6 km s{sup -1}, clouds, are located in and near the filament. A third category with properties between those of the filament and clouds appears in the data. The clouds are not always co-located with the broader line width filament emission as seen projected on the sky. Under the assumption that magnetic fields underlie the presence of the filament, a theorem is developed for its stability in terms of a toroidal magnetic field generated by the flow of gas along field lines. It is suggested that the axial magnetic field strength may be derived from the excess line width of the H I emission over and above that due to kinetic temperature by invoking the role of Alfven waves that create what is in essence a form of magnetic turbulence. At a distance of 200 pc the axial and the derived toroidal magnetic field strengths in the filament are then about 6 {mu}G while for the clouds they are about 4 {mu}G. The dependence of the derived field strength on distance is discussed.

  11. Novel high-energy physics studies using intense lasers and plasmas

    SciTech Connect (OSTI)

    Leemans, Wim P.; Bulanov, Stepan; Esarey, Eric; Schroeder, Carl

    2015-06-29

    In the framework of the project “Novel high-energy physics studies using intense lasers and plasmas” we conducted the study of ion acceleration and “flying mirrors” with high intensity lasers in order to develop sources of ion beams and high frequency radiation for different applications. Since some schemes of laser ion acceleration are also considered a good source of “flying mirrors”, we proposed to investigate the mechanisms of “mirror” formation. As a result we were able to study the laser ion acceleration from thin foils and near critical density targets. We identified several fundamental factors limiting the acceleration in the RPA regime and proposed the target design to compensate these limitations. In the case of near critical density targets, we developed a concept for the laser driven ion source for the hadron therapy. Also we studied the mechanism of “flying mirror” generation during the intense laser interaction with thin solid density targets. As for the laser-based positron creation and capture we initially proposed to study different regimes of positron beam generation and positron beam cooling. Since the for some of these schemes a good quality electron beam is required, we studied the generation of ultra-low emittance electron beams. In order to understand the fundamental physics of high energy electron beam interaction with high intensity laser pulses, which may affect the efficient generation of positron beams, we studied the radiation reaction effects.

  12. 12.6 keV Kr K-alpha X-ray Source For High Energy Density Physics...

    Office of Scientific and Technical Information (OSTI)

    Kr K-alpha X-ray Source For High Energy Density Physics Experiments A high contrast 12.6 keV Kr Kalpha source has been demonstrated on the petawatt-class Titan laser facility. ...

  13. [High Energy Physics Program at the University of Alabama. Final report

    SciTech Connect (OSTI)

    Baksay, L.; Busenitz, J.K.

    1993-10-01

    The High Energy Physics group at University of Alabama is a member of the L3 collaboration studying e+e{minus} collisions near the Z{degree} pole at the LEP accelerator at CERN. About 2 million Z{degree} events have been accumulated and the experiment has been prolific in publishing results on the Z resonance parameters, the Z couplings to all leptons and quarks with mass less than half the Z mass, searches for new particles and interactions, and studies of strong interactions and/or weak charged current decays of the quarks and leptons abundantly produced in Z decays. The group is contributing to data analysis as well as to detector hardware. In particular, the authors are involved in a major hardware upgrade for the experiment, namely the design, construction and commissioning of a Silicon Microvertex Detector (SMD) which has successfully been installed for operation during the present grant period. The authors present here a report on their recent L3 activities and their plans for the next grant period of twelve months (April 1, 1994--March 31, 1995). Their main interests in data analysis are in the study of single photon final states and the physics made more accessible by the SMD, such as heavy flavor physics. Their hardware efforts continue to be concentrated on the high precision capacitive and optical alignment monitoring systems for the SMD and also includes gas monitoring for the muon system. They are also planning to participate in the coming upgrade of the L3 detector.

  14. BES-HEP Connections: Common Problems in Condensed Matter and High Energy Physics, Round Table Discussion

    SciTech Connect (OSTI)

    Fradkin, Eduardo; Maldacena, Juan; Chatterjee, Lali; Davenport, James W

    2015-02-02

    On February 2, 2015 the Offices of High Energy Physics (HEP) and Basic Energy Sciences (BES) convened a Round Table discussion among a group of physicists on ‘Common Problems in Condensed Matter and High Energy Physics’. This was motivated by the realization that both fields deal with quantum many body problems, share many of the same challenges, use quantum field theoretical approaches and have productively interacted in the past. The meeting brought together physicists with intersecting interests to explore recent developments and identify possible areas of collaboration.... Several topics were identified as offering great opportunity for discovery and advancement in both condensed matter physics and particle physics research. These included topological phases of matter, the use of entanglement as a tool to study nontrivial quantum systems in condensed matter and gravity, the gauge-gravity duality, non-Fermi liquids, the interplay of transport and anomalies, and strongly interacting disordered systems. Many of the condensed matter problems are realizable in laboratory experiments, where new methods beyond the usual quasi-particle approximation are needed to explain the observed exotic and anomalous results. Tools and techniques such as lattice gauge theories, numerical simulations of many-body systems, and tensor networks are seen as valuable to both communities and will likely benefit from collaborative development.

  15. Software Aspects of IEEE Floating-Point Computations for Numerical Applications in High Energy Physics

    ScienceCinema (OSTI)

    None

    2011-10-06

    Floating-point computations are at the heart of much of the computing done in high energy physics. The correctness, speed and accuracy of these computations are of paramount importance. The lack of any of these characteristics can mean the difference between new, exciting physics and an embarrassing correction. This talk will examine practical aspects of IEEE 754-2008 floating-point arithmetic as encountered in HEP applications. After describing the basic features of IEEE floating-point arithmetic, the presentation will cover: common hardware implementations (SSE, x87) techniques for improving the accuracy of summation, multiplication and data interchange compiler options for gcc and icc affecting floating-point operations hazards to be avoided About the speaker Jeffrey M Arnold is a Senior Software Engineer in the Intel Compiler and Languages group at Intel Corporation. He has been part of the Digital->Compaq->Intel compiler organization for nearly 20 years; part of that time, he worked on both low- and high-level math libraries. Prior to that, he was in the VMS Engineering organization at Digital Equipment Corporation. In the late 1980s, Jeff spent 2½ years at CERN as part of the CERN/Digital Joint Project. In 2008, he returned to CERN to spent 10 weeks working with CERN/openlab. Since that time, he has returned to CERN multiple times to teach at openlab workshops and consult with various LHC experiments. Jeff received his Ph.D. in physics from Case Western Reserve University.

  16. Software Aspects of IEEE Floating-Point Computations for Numerical Applications in High Energy Physics

    SciTech Connect (OSTI)

    2010-05-11

    Floating-point computations are at the heart of much of the computing done in high energy physics. The correctness, speed and accuracy of these computations are of paramount importance. The lack of any of these characteristics can mean the difference between new, exciting physics and an embarrassing correction. This talk will examine practical aspects of IEEE 754-2008 floating-point arithmetic as encountered in HEP applications. After describing the basic features of IEEE floating-point arithmetic, the presentation will cover: common hardware implementations (SSE, x87) techniques for improving the accuracy of summation, multiplication and data interchange compiler options for gcc and icc affecting floating-point operations hazards to be avoided About the speaker Jeffrey M Arnold is a Senior Software Engineer in the Intel Compiler and Languages group at Intel Corporation. He has been part of the Digital->Compaq->Intel compiler organization for nearly 20 years; part of that time, he worked on both low- and high-level math libraries. Prior to that, he was in the VMS Engineering organization at Digital Equipment Corporation. In the late 1980s, Jeff spent 2 years at CERN as part of the CERN/Digital Joint Project. In 2008, he returned to CERN to spent 10 weeks working with CERN/openlab. Since that time, he has returned to CERN multiple times to teach at openlab workshops and consult with various LHC experiments. Jeff received his Ph.D. in physics from Case Western Reserve University.

  17. Theoretical Physics

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

    HEP Theoretical Physics Understanding discoveries at the Energy, Intensity, and Cosmic Frontiers Get ... HEP Theory at Los Alamos The Theoretical High Energy Physics group at ...

  18. Physics perspectives of heavy-ion collisions at very high energy

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

    Chang, Ning-bo; Cao, ShanShan; Chen, Bao-yi; Chen, Shi-yong; Chen, Zhen-yu; Ding, Heng-Tong; He, Min; Liu, Zhi-quan; Pang, Long-gang; Qin, Guang-you; et al

    2016-01-15

    We expect heavy-ion collisions at very high colliding energies to produce a quark-gluon plasma (QGP) at the highest temperature obtainable in a laboratory setting. Experimental studies of these reactions can provide an unprecedented range of information on properties of the QGP at high temperatures. We also report theoretical investigations of the physics perspectives of heavy-ion collisions at a future high-energy collider. These include initial parton production, collective expansion of the dense medium, jet quenching, heavy-quark transport, dissociation and regeneration of quarkonia, photon and dilepton production. Here, we illustrate the potential of future experimental studies of the initial particle production andmore » formation of QGP at the highest temperature to provide constraints on properties of strongly interaction matter.« less

  19. Highly ionized physical vapor deposition plasma source working at very low pressure

    SciTech Connect (OSTI)

    Stranak, V.; Herrendorf, A.-P.; Drache, S.; Hippler, R.; Cada, M.; Hubicka, Z.; Tichy, M.

    2012-04-02

    Highly ionized discharge for physical vapor deposition at very low pressure is presented in the paper. The discharge is generated by electron cyclotron wave resonance (ECWR) which assists with ignition of high power impulse magnetron sputtering (HiPIMS) discharge. The magnetron gun (with Ti target) was built into the single-turn coil RF electrode of the ECWR facility. ECWR assistance provides pre-ionization effect which allows significant reduction of pressure during HiPIMS operation down to p = 0.05 Pa; this is nearly more than an order of magnitude lower than at typical pressure ranges of HiPIMS discharges. We can confirm that nearly all sputtered particles are ionized (only Ti{sup +} and Ti{sup ++} peaks are observed in the mass scan spectra). This corresponds well with high plasma density n{sub e} {approx} 10{sup 18} m{sup -3}, measured during the HiPIMS pulse.

  20. High Performance Computing and Storage Requirements for Nuclear Physics: Target 2017

    SciTech Connect (OSTI)

    Gerber, Richard; Wasserman, Harvey

    2015-01-20

    In April 2014, NERSC, ASCR, and the DOE Office of Nuclear Physics (NP) held a review to characterize high performance computing (HPC) and storage requirements for NP research through 2017. This review is the 12th in a series of reviews held by NERSC and Office of Science program offices that began in 2009. It is the second for NP, and the final in the second round of reviews that covered the six Office of Science program offices. This report is the result of that review

  1. Massachusetts Institute of Technology New Trend in High Energy Physics, Alushta, Ukraine, Sep. 6, 2011

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

    9/06/2011 Teppei Katori, MIT 1 Teppei Katori for the MiniBooNE collaboration Massachusetts Institute of Technology New Trend in High Energy Physics, Alushta, Ukraine, Sep. 6, 2011 MiniBooNE, a neutrino oscillation experiment at Fermilab Outline 1. Introduction 2. Neutrino beam 3. Events in the detector 4. Cross section model 5. Neutrino oscillation result 6. Anti-neutrino oscillation result 7. Outlook 09/06/2011 Teppei Katori, MIT 2 Teppei Katori for the MiniBooNE collaboration Massachusetts

  2. High-energy physics detector MicroBooNE sees first accelerator-born

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

    neutrinos MicroBooNE sees first accelerator-born neutrinos High-energy physics detector MicroBooNE sees first accelerator-born neutrinos The principal purpose of the detector is to confirm or deny the existence of a hypothetical particle known as the sterile neutrino. November 2, 2015 An accelerator-born neutrino candidate, spotted with the MicroBooNE detector. Image courtesy Fermilab. An accelerator-born neutrino candidate, spotted with the MicroBooNE detector. Image courtesy Fermilab.

  3. Health hazard evaluation report HETA 92-108-2247, Montpelier High School, Montpelier, Vermont

    SciTech Connect (OSTI)

    Crandall, M.S.; Wilcox, T.G.

    1992-08-01

    On January 8, 1992, the National Institute for Occupational Safety and Health (NIOSH), received a request for a hazard evaluation from Senator Patrick Leahy's office in Montpelier, Vermont. The request was for NIOSH to evaluate the indoor environmental quality at the Montpelier High School, particularly with regard to new carpets installed there. On March 4, 1992, NIOSH investigators interviewed teachers and collected air samples for 4-phenylcyclohexene (4-PC) and other volatile organic chemicals (VOCs). Air samples were collected in classrooms and administrative offices which were carpeted. Other yearly remodeling activities, such as painting classrooms and applying a sealant to the gymnasium floor, had been done at the same time the carpet was installed. Energy-saving and fire code modifications to the school over time had altered the effectiveness of the designed ventilation system. Based on the medical interviews and environmental information, it appeared that there was a temporal relationship between the yearly remodeling of the school and the symptoms reported by the teachers. Ventilation system improvements and the use of low emitting building materials and furnishings are recommended.

  4. OSTIblog Articles in the high school Topic | OSTI, US Dept of Energy Office

    Office of Scientific and Technical Information (OSTI)

    of Scientific and Technical Information high school Topic Where Do New Scientists Come From? by Philip Ellis 07 Feb, 2013 in Science Communications Photo of Jack Andraka from his Twitter feed When we think of scientists, most of us picture professionals working in labs or in university settings. But how did these people get to become scientists? They were born into the world like everyone else and could have selected from a myriad different career paths. The evidence does not suggest that

  5. La Vida Robot - High School Engineering Program Combats Engineering Brain Drain

    ScienceCinema (OSTI)

    Cameron, Allan; Fredi, Lajvardi

    2009-09-01

    Carl Hayden High School has built an impressive reputation with its robotics club. At a time when interest in science, math and engineering is declining, the Falcon Robotics club has young people fired up about engineering. Their program in underwater robots (MATE) and FIRST robotics is becoming a national model, not for building robots, but for building engineers. Teachers Fredi Lajvardi and Allan Cameron will present their story (How kids 'from the mean streets of Phoenix took on the best from M.I.T. in the national underwater bot championship' - Wired Magazine, April 2005) and how every student needs the opportunity to 'do real engineering.'

  6. Linking Automated Data Analysis and Visualization with Applications in Developmental Biology and High-Energy Physics

    SciTech Connect (OSTI)

    Ruebel, Oliver

    2009-12-01

    Knowledge discovery from large and complex collections of today's scientific datasets is a challenging task. With the ability to measure and simulate more processes at increasingly finer spatial and temporal scales, the increasing number of data dimensions and data objects is presenting tremendous challenges for data analysis and effective data exploration methods and tools. Researchers are overwhelmed with data and standard tools are often insufficient to enable effective data analysis and knowledge discovery. The main objective of this thesis is to provide important new capabilities to accelerate scientific knowledge discovery form large, complex, and multivariate scientific data. The research covered in this thesis addresses these scientific challenges using a combination of scientific visualization, information visualization, automated data analysis, and other enabling technologies, such as efficient data management. The effectiveness of the proposed analysis methods is demonstrated via applications in two distinct scientific research fields, namely developmental biology and high-energy physics.Advances in microscopy, image analysis, and embryo registration enable for the first time measurement of gene expression at cellular resolution for entire organisms. Analysis of high-dimensional spatial gene expression datasets is a challenging task. By integrating data clustering and visualization, analysis of complex, time-varying, spatial gene expression patterns and their formation becomes possible. The analysis framework MATLAB and the visualization have been integrated, making advanced analysis tools accessible to biologist and enabling bioinformatic researchers to directly integrate their analysis with the visualization. Laser wakefield particle accelerators (LWFAs) promise to be a new compact source of high-energy particles and radiation, with wide applications ranging from medicine to physics. To gain insight into the complex physical processes of particle

  7. Closeout Report: Experimental High Energy Physics Group at the University of South Alabama

    SciTech Connect (OSTI)

    Jenkins, Charles M; Godang, Romulus

    2013-06-25

    The High Energy Physics group at the University of South Alabama has been supported by this research grant (DE-FG02-96ER40970) since 1996. One researcher, Dr. Merrill Jenkins, has been supported on this grant during this time worked on fixed target experiments at the Fermi National Accelerator Laboratory, west of Chicago, Illinois. These experiments have been E-705, E-771, E-871 (HyperCP) and E-921 (CKM) before it was canceled for budgetary reasons. After the cancellation of CKM, Dr. Jenkins joined the Compact Muon Solenoid (CMS) experiment as an associate member via the High Energy Physics Group at the Florida State University. A second, recently tenured faculty member, Dr. Romulus Godang joined the group in 2009 and has been supported by this grant since then. Dr. Godang is working on the BaBaR experiment at SLAC and has joined the Belle-II experiment located in Japan at KEK. According to the instructions sent to us by our grant monitor, we are to concentrate on the activities over the last three years in this closeout report.

  8. US Heavy Ion Beam Research for High Energy Density Physics Applications and Fusion

    SciTech Connect (OSTI)

    Davidson, R.C.; Logan, B.G.; Barnard, J.J.; Bieniosek, F.M.; Briggs, R.J.; et al.

    2005-09-19

    Key scientific results from recent experiments, modeling tools, and heavy ion accelerator research are summarized that explore ways to investigate the properties of high energy density matter in heavy-ion-driven targets, in particular, strongly-coupled plasmas at 0.01 to 0.1 times solid density for studies of warm dense matter, which is a frontier area in high energy density physics. Pursuit of these near-term objectives has resulted in many innovations that will ultimately benefit heavy ion inertial fusion energy. These include: neutralized ion beam compression and focusing, which hold the promise of greatly improving the stage between the accelerator and the target chamber in a fusion power plant; and the Pulse Line Ion Accelerator (PLIA), which may lead to compact, low-cost modular linac drivers.

  9. A novel zirconium K{alpha} imager for high energy density physics research

    SciTech Connect (OSTI)

    Akli, K. U.; Jiang, S.; Storm, M. S.; Krygier, A.; Freeman, R. R.; Sanchez del Rio, M.; Stephens, R. B.; Pereira, N. R.; Baronova, E. O.; Theobald, W.; Ping, Y.; McLean, H. S.; Patel, P. K.; Key, M. H.

    2011-12-15

    We report on the development and characterization of a zirconium K{alpha} imager for high energy density physics research. The imager consists of a spherically bent quartz crystal operating at 15.7 keV photon energy. We compare the performance of the imager in terms of integrated reflectivity (R{sub int}) and temperature dependent collection efficiency ({eta}{sub Te}) to that of the widely used Cu K{alpha} imager. Our collisional-radiative simulations show that the new imager can be reliably used up to 250 eV plasma temperature. Monte Carlo simulations show that for a 25 {mu}m thick tracer layer of zirconium, the contribution to K{alpha} production from photo-pumping is only 2%. We present, for the first time, 2D spatially resolved images of zirconium plasmas generated by a high intensity short pulse laser interacting with Zr solid targets.

  10. Neutrino Oscillation Physics

    SciTech Connect (OSTI)

    Kayser, Boris

    2012-06-01

    To complement the neutrino-physics lectures given at the 2011 International School on Astro Particle Physics devoted to Neutrino Physics and Astrophysics (ISAPP 2011; Varenna, Italy), at the 2011 European School of High Energy Physics (ESHEP 2011; Cheila Gradistei, Romania), and, in modified form, at other summer schools, we present here a written description of the physics of neutrino oscillation. This description is centered on a new way of deriving the oscillation probability. We also provide a brief guide to references relevant to topics other than neutrino oscillation that were covered in the lectures. Neutrinos and photons are by far the most abundant elementary particles in the universe. Thus, if we would like to comprehend the universe, we must understand the neutrinos. Of course, studying the neutrinos is challenging, since the only known forces through which these electrically-neutral leptons interact are the weak force and gravity. Consequently, interactions of neutrinos in a detector are very rare events, so that very large detectors and intense neutrino sources are needed to make experiments feasible. Nevertheless, we have confirmed that the weak interactions of neutrinos are correctly described by the Standard Model (SM) of elementary particle physics. Moreover, in the last 14 years, we have discovered that neutrinos have nonzero masses, and that leptons mix. These discoveries have been based on the observation that neutrinos can change from one 'flavor' to another - the phenomenon known as neutrino oscillation. We shall explain the physics of neutrino oscillation, deriving the probability of oscillation in a new way. We shall also provide a very brief guide to references that can be used to study some major neutrino-physics topics other than neutrino oscillation.

  11. The Ultimate Structure of Matter: The High Energy Physics Program from the 1950s through the 1980s

    DOE R&D Accomplishments [OSTI]

    1990-02-01

    This discusses the following topics in High Energy Physics: The Particle Zoo; The Strong and the Weak; The Particle Explosion; Deep Inside the Nucleon; The Search for Unity; Physics in Collision; The Standard Model; Particles and the Cosmos; and Practical Benefits.

  12. BELLE High Energy Physics Experiment at the KEK B-factory: Data and Physics Results for CPV, Rare, DKM, 5S, Charm, Tau, and New Particles

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

    Belle is a high-energy physics (HEP) experiment that began in 1999 at the KEK B-factory in Japan under the direction of the International Belle Collaboration. The Collaboration was formed around the common interest of clarifying a long standing physics puzzle, that of CP violation. The goal of the experiments was to make a definitive test of the Standard Models predictions for CP violations in the decays of B mesons. The original Belle experiment verified the KM theory, leading to a Nobel prize in 2008 for Kobayashi and Maskawa. Belle II Collaboration is now working on additional discoveries.

  13. Courses on Beam Physics

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

    a foundation course on accelerator physics and associated technologies. The US-CERN-Japan-Russia Joint Accelerator School The purpose of the US-CERN-Japan-Russia joint school...

  14. Association between Electronic Cigarette Use and Asthma among High School Students in South Korea

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

    Cho, Jun Ho; Paik, Samuel Y.

    2016-03-04

    Little is known about health outcomes related to electronic cigarette (EC) use, despite its growing popularity. The aim of this study is to investigate the association between EC use and asthma. The study design is a cross-sectional study. A total of 35,904 high school students were included as the final study population. The presence of asthma was based on a student’s self-reported doctor diagnosis of asthma in the past 12 months. Results showed prevalence rates of asthmatics in ‘current EC users’ (n = 2,513), ‘former EC users’ (n = 2,078), and ‘never EC users’ (n = 31,313), were 3.9% (nmore » = 98), 2.2% (n = 46) and 1.7% (n = 530), respectively. Comparing ‘current EC’ users with ‘never EC’ users, the unadjusted OR for asthma was 2.36 (95% CI: 1.89–2.94). In order to control for the effect of conventional cigarette (CC) smoking, after stratifying the subjects by the three CC smoking categories (never CC, former CC, and current CC), within the ‘never CC’ category, the unadjusted OR for asthma for ‘current EC’ users was 3.41 (95% CI: 1.79–6.49), and the adjusted OR was 2.74 (95% CI: 1.30–5.78). Severe asthma was reflected by the number of days absent from school due to asthma symptoms; current EC users had the highest adjusted OR for severe asthma compared to ‘never EC’ users. In conclusion, when compared to a reference population of high school students in South Korea, EC users have an increased association with asthma and are more likely to have had days absent from school due to severe asthma symptoms. In conclusion, the results indicate that EC use may be a risk factor for asthma. The results may be useful in developing a scientific basis for the evaluation of a potential health hazard by EC.« less

  15. Performance of bent-crystal x-ray microscopes for high energy density physics research

    SciTech Connect (OSTI)

    Schollmeier, Marius S.; Geissel, Matthias; Shores, Jonathon E.; Smith, Ian C.; Porter, John L.

    2015-05-29

    We present calculations for the field of view (FOV), image fluence, image monochromaticity, spectral acceptance, and image aberrations for spherical crystal microscopes, which are used as self-emission imaging or backlighter systems at large-scale high energy density physics facilities. Our analytic results are benchmarked with ray-tracing calculations as well as with experimental measurements from the 6.151 keV backlighter system at Sandia National Laboratories. Furthermore, the analytic expressions can be used for x-ray source positions anywhere between the Rowland circle and object plane. We discovered that this enables quick optimization of the performance of proposed but untested, bent-crystal microscope systems to find the best compromise between FOV, image fluence, and spatial resolution for a particular application.

  16. Performance of bent-crystal x-ray microscopes for high energy density physics research

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

    Schollmeier, Marius S.; Geissel, Matthias; Shores, Jonathon E.; Smith, Ian C.; Porter, John L.

    2015-05-29

    We present calculations for the field of view (FOV), image fluence, image monochromaticity, spectral acceptance, and image aberrations for spherical crystal microscopes, which are used as self-emission imaging or backlighter systems at large-scale high energy density physics facilities. Our analytic results are benchmarked with ray-tracing calculations as well as with experimental measurements from the 6.151 keV backlighter system at Sandia National Laboratories. Furthermore, the analytic expressions can be used for x-ray source positions anywhere between the Rowland circle and object plane. We discovered that this enables quick optimization of the performance of proposed but untested, bent-crystal microscope systems to findmore » the best compromise between FOV, image fluence, and spatial resolution for a particular application.« less

  17. Searches for New Physics Using High Mass Dimuons at the CDF II Experiment

    SciTech Connect (OSTI)

    Karagoz Unel, Muge

    2004-12-01

    This work describes the measurement of inclusive jets cross section in the D0 experiment. This cross section is computed as a function of jet transverse momentum, in several rapidity intervals. This quantity is sensitive to the proton structure and is crucial for the determination of parton distribution functions (PDF), essentially for the gluon at high proton momentum fraction. The measurement presented here gives the first values obtained for Tevatron Run II for the cross section in several rapidity intervals, for an integrated luminosity of 143 pb{sup -1}. The results are in agreement, within the uncertainties, with theoretical Standard Model predictions, showing no evidence for new physics. This work points out the aspects of the detector which need better understanding to reach Run I precision and to constrain the PDFs.

  18. The impact of Hall physics on magnetized high energy density plasma jets

    SciTech Connect (OSTI)

    Gourdain, P.-A.; Seyler, C. E.; Atoyan, L.; Greenly, J. B.; Hammer, D. A.; Kusse, B. R.; Pikuz, S. A.; Potter, W. M.; Schrafel, P. C.; Shelkovenko, T. A.

    2014-05-15

    Hall physics is often neglected in high energy density plasma jets due to the relatively high electron density of such jets (n{sub e} ∼ 10{sup 19} cm{sup −3}). However, the vacuum region surrounding the jet has much lower densities and is dominated by Hall electric field. This electric field redirects plasma flows towards or away from the axis, depending on the radial current direction. A resulting change in the jet density has been observed experimentally. Furthermore, if an axial field is applied on the jet, the Hall effect is enhanced and ignoring it leads to serious discrepancies between experimental results and numerical simulations. By combining high currents (∼1 MA) and magnetic field helicity (15° angle) in a pulsed power generator such as COBRA, plasma jets can be magnetized with a 10 T axial field. The resulting field enhances the impact of the Hall effect by altering the density profile of current-free plasma jets and the stability of current-carrying plasma jets (e.g., Z-pinches)

  19. Final Technical Report for "High Energy Physics at The University of Iowa"

    SciTech Connect (OSTI)

    Mallik, Usha; Meurice, Yannick; Nachtman, Jane; Onel, Yasar; Reno, Mary

    2013-07-31

    Particle Physics explores the very fundamental building blocks of our universe: the nature of forces, of space and time. By exploring very energetic collisions of sub-nuclear particles with sophisticated detectors at the colliding beam accelerators (as well as others), experimental particle physicists have established the current theory known as the Standard Model (SM), one of the several theoretical postulates to explain our everyday world. It explains all phenomena known up to a very small fraction of a second after the Big Bang to a high precision; the Higgs boson, discovered recently, was the last of the particle predicted by the SM. However, many other phenomena, like existence of dark energy, dark matter, absence of anti-matter, the parameters in the SM, neutrino masses etc. are not explained by the SM. So, in order to find out what lies beyond the SM, i.e., what conditions at the earliest fractions of the first second of the universe gave rise to the SM, we constructed the Large Hadron Collider (LHC) at CERN after the Tevatron collider at Fermi National Accelerator Laboratory. Each of these projects helped us push the boundary further with new insights as we explore a yet higher energy regime. The experiments are extremely complex, and as we push the boundaries of our existing knowledge, it also requires pushing the boundaries of our technical knowhow. So, not only do we pursue humankind’s most basic intellectual pursuit of knowledge, we help develop technology that benefits today’s highly technical society. Our trained Ph.D. students become experts at fast computing, manipulation of large data volumes and databases, developing cloud computing, fast electronics, advanced detector developments, and complex interfaces in several of these areas. Many of the Particle physics Ph.D.s build their careers at various technology and computing facilities, even financial institutions use some of their skills of simulation and statistical prowess. Additionally, last

  20. Very High-Temperature Reactor (VHTR) Proliferation Resistance and Physical Protection (PR&PP)

    SciTech Connect (OSTI)

    Moses, David Lewis

    2011-10-01

    This report documents the detailed background information that has been compiled to support the preparation of a much shorter white paper on the design features and fuel cycles of Very High-Temperature Reactors (VHTRs), including the proposed Next-Generation Nuclear Plant (NGNP), to identify the important proliferation resistance and physical protection (PR&PP) aspects of the proposed concepts. The shorter white paper derived from the information in this report was prepared for the Department of Energy Office of Nuclear Science and Technology for the Generation IV International Forum (GIF) VHTR Systems Steering Committee (SSC) as input to the GIF Proliferation Resistance and Physical Protection Working Group (PR&PPWG) (http://www.gen-4.org/Technology/horizontal/proliferation.htm). The short white paper was edited by the GIF VHTR SCC to address their concerns and thus may differ from the information presented in this supporting report. The GIF PR&PPWG will use the derived white paper based on this report along with other white papers on the six alternative Generation IV design concepts (http://www.gen-4.org/Technology/systems/index.htm) to employ an evaluation methodology that can be applied and will evolve from the earliest stages of design. This methodology will guide system designers, program policy makers, and external stakeholders in evaluating the response of each system, to determine each system's resistance to proliferation threats and robustness against sabotage and terrorism threats, and thereby guide future international cooperation on ensuring safeguards in the deployment of the Generation IV systems. The format and content of this report is that specified in a template prepared by the GIF PR&PPWG. Other than the level of detail, the key exception to the specified template format is the addition of Appendix C to document the history and status of coated-particle fuel reprocessing technologies, which fuel reprocessing technologies have yet to be deployed

  1. Topics in nuclear and radiochemistry for college curricula and high school science programs

    SciTech Connect (OSTI)

    Not Available

    1990-01-01

    The concern with the current status and trends of nuclear chemistry and radiochemistry education in academic institutions was addressed in a recent workshop. The 1988 workshop considered the important contributions that scientist with nuclear and radiochemistry backgrounds have made and are continuing to make to other sciences and to various applied fields. Among the areas discussed were environmental studies, life sciences, materials science, separation technology, hot atom chemistry, cosmochemistry, and the rapidly growing field of nuclear medicine. It is intent of the organizer and participants of this symposium entitled Topics in Nuclear and Radiochemistry for College Curricula and High School Science Program'' to provide lecture material on topics related to nuclear and radiochemistry to educators. It is our hope that teachers, who may or may not be familiar with the field, will find this collections of articles useful and incorporate some of them into their lectures.

  2. Colorado School Earns Return Trip to National Science Bowl |...

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

    After a full day answering rapid-fire questions in physics, math, astronomy, chemistry, ... Bowl in 1991 as a way to encourage high school students to explore math and science. ...

  3. 12.6 keV Kr K-alpha X-ray Source For High Energy Density Physics...

    Office of Scientific and Technical Information (OSTI)

    12.6 keV Kr K-alpha X-ray Source For High Energy Density Physics Experiments Citation Details In-Document Search Title: 12.6 keV Kr K-alpha X-ray Source For High Energy Density...

  4. QCD Thermodynamics at High Temperature Peter Petreczky Large Scale Computing and Storage Requirements for Nuclear Physics (NP),

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

    QCD Thermodynamics at High Temperature Peter Petreczky Large Scale Computing and Storage Requirements for Nuclear Physics (NP), Bethesda MD, April 29-30, 2014 NY Center for Computational Science 2 Defining questions of nuclear physics research in US: Nuclear Science Advisory Committee (NSAC) "The Frontiers of Nuclear Science", 2007 Long Range Plan "What are the phases of strongly interacting matter and what roles do they play in the cosmos ?" "What does QCD predict for

  5. Middle School Rules, Forms, and Resources | U.S. DOE Office of...

    Office of Science (SC) Website

    Resources National Science Bowl (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms,...

  6. MCRUNJOB: A High energy physics workflow planner for grid production processing

    SciTech Connect (OSTI)

    Graham, Gregory E.

    2004-08-26

    McRunjob is a powerful grid workflow manager used to manage the generation of large numbers of production processing jobs in High Energy Physics. In use at both the DZero and CMS experiments, McRunjob has been used to manage large Monte Carlo production processing since 1999 and is being extended to uses in regular production processing for analysis and reconstruction. Described at CHEP 2001, McRunjob converts core metadata into jobs submittable in a variety of environments. The powerful core metadata description language includes methods for converting the metadata into persistent forms, job descriptions, multi-step workflows, and data provenance information. The language features allow for structure in the metadata by including full expressions, namespaces, functional dependencies, site specific parameters in a grid environment, and ontological definitions. It also has simple control structures for parallelization of large jobs. McRunjob features a modular design which allows for easy expansion to new job description languages or new application level tasks.

  7. Reactor Physics Measurements and Benchmark Specifications for Oak Ridge Highly Enriched Uranium Sphere (ORSphere)

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

    Marshall, Margaret A.

    2014-11-04

    In the early 1970s Dr. John T. Mihalczo (team leader), J.J. Lynn, and J.R. Taylor performed experiments at the Oak Ridge Critical Experiments Facility (ORCEF) with highly enriched uranium (HEU) metal (called Oak Ridge Alloy or ORALLOY) in an effort to recreate GODIVA I results with greater accuracy than those performed at Los Alamos National Laboratory in the 1950s. The purpose of the Oak Ridge ORALLOY Sphere (ORSphere) experiments was to estimate the unreflected and unmoderated critical mass of an idealized sphere of uranium metal corrected to a density, purity, and enrichment such that it could be compared with themore » GODIVA I experiments. Additionally, various material reactivity worths, the surface material worth coefficient, the delayed neutron fraction, the prompt neutron decay constant, relative fission density, and relative neutron importance were all measured. The critical assembly, material reactivity worths, the surface material worth coefficient, and the delayed neutron fraction were all evaluated as benchmark experiment measurements. The reactor physics measurements are the focus of this paper; although for clarity the critical assembly benchmark specifications are briefly discussed.« less

  8. Reactor Physics Measurements and Benchmark Specifications for Oak Ridge Highly Enriched Uranium Sphere (ORSphere)

    SciTech Connect (OSTI)

    Marshall, Margaret A.

    2014-11-04

    In the early 1970s Dr. John T. Mihalczo (team leader), J.J. Lynn, and J.R. Taylor performed experiments at the Oak Ridge Critical Experiments Facility (ORCEF) with highly enriched uranium (HEU) metal (called Oak Ridge Alloy or ORALLOY) in an effort to recreate GODIVA I results with greater accuracy than those performed at Los Alamos National Laboratory in the 1950s. The purpose of the Oak Ridge ORALLOY Sphere (ORSphere) experiments was to estimate the unreflected and unmoderated critical mass of an idealized sphere of uranium metal corrected to a density, purity, and enrichment such that it could be compared with the GODIVA I experiments. Additionally, various material reactivity worths, the surface material worth coefficient, the delayed neutron fraction, the prompt neutron decay constant, relative fission density, and relative neutron importance were all measured. The critical assembly, material reactivity worths, the surface material worth coefficient, and the delayed neutron fraction were all evaluated as benchmark experiment measurements. The reactor physics measurements are the focus of this paper; although for clarity the critical assembly benchmark specifications are briefly discussed.

  9. Physics of (very) high energy e/sup +/-e/sup -/ colliders

    SciTech Connect (OSTI)

    Peskin, M.E.

    1984-10-01

    I review the physics capabilities of e/sup +/e/sup -/ colliders of hundred GeV to TeV center-of-mass energies, emphasizing issues relevant to the physics of symmetry breaking in the weak interactions. 24 references.

  10. Engineering the CernVM-Filesystem as a High Bandwidth Distributed Filesystem for Auxiliary Physics Data

    SciTech Connect (OSTI)

    Dykstra, D.; Bockelman, B.; Blomer, J.; Herner, K.; Levshina, T.; Slyz, M.

    2015-12-23

    A common use pattern in the computing models of particle physics experiments is running many distributed applications that read from a shared set of data files. We refer to this data is auxiliary data, to distinguish it from (a) event data from the detector (which tends to be different for every job), and (b) conditions data about the detector (which tends to be the same for each job in a batch of jobs). Relatively speaking, conditions data also tends to be relatively small per job where both event data and auxiliary data are larger per job. Unlike event data, auxiliary data comes from a limited working set of shared files. Since there is spatial locality of the auxiliary data access, the use case appears to be identical to that of the CernVM- Filesystem (CVMFS). However, we show that distributing auxiliary data through CVMFS causes the existing CVMFS infrastructure to perform poorly. We utilize a CVMFS client feature called 'alien cache' to cache data on existing local high-bandwidth data servers that were engineered for storing event data. This cache is shared between the worker nodes at a site and replaces caching CVMFS files on both the worker node local disks and on the site's local squids. We have tested this alien cache with the dCache NFSv4.1 interface, Lustre, and the Hadoop Distributed File System (HDFS) FUSE interface, and measured performance. In addition, we use high-bandwidth data servers at central sites to perform the CVMFS Stratum 1 function instead of the low-bandwidth web servers deployed for the CVMFS software distribution function. We have tested this using the dCache HTTP interface. As a result, we have a design for an end-to-end high-bandwidth distributed caching read-only filesystem, using existing client software already widely deployed to grid worker nodes and existing file servers already widely installed at grid sites. Files are published in a central place and are soon available on demand throughout the grid and cached locally on the

  11. A new variable-resolution associative memory for high energy physics

    SciTech Connect (OSTI)

    Annovi, A.; Amerio, S.; Beretta, M.; Bossini, E.; Crescioli, F.; Dell'Orso, M.; Giannetti, P.; Hoff, J.; Liu, T.; Magalotti, D.; Piendibene, M.; Sacco, I.; Schoening, A.; Soltveit, H. K.; Stabile, A.; Tripiccione, R.; Liberali, V.; Vitillo, R.; Volpi, G.

    2011-07-01

    We describe an important advancement for the Associative Memory device (AM). The AM is a VLSI processor for pattern recognition based on Content Addressable Memory (CAM) architecture. The AM is optimized for on-line track finding in high-energy physics experiments. Pattern matching is carried out by finding track candidates in coarse resolution 'roads'. A large AM bank stores all trajectories of interest, called 'patterns', for a given detector resolution. The AM extracts roads compatible with a given event during detector read-out. Two important variables characterize the quality of the AM bank: its 'coverage' and the level of fake roads. The coverage, which describes the geometric efficiency of a bank, is defined as the fraction of tracks that match at least one pattern in the bank. Given a certain road size, the coverage of the bank can be increased just adding patterns to the bank, while the number of fakes unfortunately is roughly proportional to the number of patterns in the bank. Moreover, as the luminosity increases, the fake rate increases rapidly because of the increased silicon occupancy. To counter that, we must reduce the width of our roads. If we decrease the road width using the current technology, the system will become very large and extremely expensive. We propose an elegant solution to this problem: the 'variable resolution patterns'. Each pattern and each detector layer within a pattern will be able to use the optimal width, but we will use a 'don't care' feature (inspired from ternary CAMs) to increase the width when that is more appropriate. In other words we can use patterns of variable shape. As a result we reduce the number of fake roads, while keeping the efficiency high and avoiding excessive bank size due to the reduced width. We describe the idea, the implementation in the new AM design and the implementation of the algorithm in the simulation. Finally we show the effectiveness of the 'variable resolution patterns' idea using simulated

  12. Stimulated scattering in laser driven fusion and high energy density physics experiments

    SciTech Connect (OSTI)

    Yin, L. Albright, B. J.; Rose, H. A.; Montgomery, D. S.; Kline, J. L.; Finnegan, S. M.; Bergen, B.; Bowers, K. J.; Kirkwood, R. K.; Milovich, J.

    2014-09-15

    In laser driven fusion and high energy density physics experiments, one often encounters a k?{sub D} range of 0.15?

  13. Saturday Morning Physics at Texas A&M University

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

    Registration Program Schedule Contact Us Directions Previous Programs Follow us on facebook. Spring 2016 Program Learn about exciting developments in Modern Physics, this year focusing on the fundamentals and forefront research in nuclear and high-energy physics as well as quantum optics. An event series for Texas High-School Students to go on a journey of discovering how physics can help us understand nature! Eleventh Year Running! Earn a certificate for sustained attendance! View the program

  14. High energy physics program at Texas A&M University. Final report, April 1, 1990--March 31, 1991

    SciTech Connect (OSTI)

    Not Available

    1992-12-01

    The Texas A&M experimental high energy physics program has been supported since its inception by DOE Contract DE-AS05-81ER40039. During that period we established a viable experimental program at a university which before this time had no program in high energy physics. In 1990, the experimental program was augmented with a program in particle theory. In the accompanying final report, we outline the research work accomplished during the final year of this contract and the program being proposed for consideration by the Department of Energy for future grant support. Some of the particular areas covered are: Collider detector at Fermilab program; the TAMU MACRO program; SSC R&D program; SSC experimental program; and theoretical physics program.

  15. U.C. Davis high energy particle physics research: Technical progress report -- 1990

    SciTech Connect (OSTI)

    NONE

    1990-12-31

    Summaries of progress made for this period is given for each of the following areas: (1) Task A--Experiment, H1 detector at DESY; (2) Task C--Experiment, AMY detector at KEK; (3) Task D--Experiment, fixed target detectors at Fermilab; (4) Task F--Experiment, PEP detector at SLAC and pixel detector; (5) Task B--Theory, particle physics; and (6) Task E--Theory, particle physics.

  16. Applications of Robust, Radiation Hard AlGaN Optoelectronic Devices in Space Exploration and High Energy Density Physics

    SciTech Connect (OSTI)

    Sun, K.

    2011-05-04

    This slide show presents: space exploration applications; high energy density physics applications; UV LED and photodiode radiation hardness; UV LED and photodiode space qualification; UV LED AC charge management; and UV LED satellite payload instruments. A UV LED satellite will be launched 2nd half 2012.

  17. Spearfish High School, Sparfish, South Dakota solar energy system performance evaluation, September 1980-June 1981

    SciTech Connect (OSTI)

    Howard, B.D.

    1981-01-01

    Spearfish High School in South Dakota contains 43,000 square feet of conditioned space. Its active solar energy system is designed to supply 57% of the space heating and 50% of the hot water demand. The system is equipped with 8034 square feet of flat plate collectors, 4017 cubic feet of rock bin sensible heat storage, and auxiliary equipment including 8 heat pumps, 6 of which are solar supplied and instrumented, air conditioning units, and natural-gas-fired boilers. Performance data are given for the system including the solar fraction, solar savings ratio, conventional fuel savings, system performance factor and solar system coefficient of performance. Insolation, solar energy utilization and operation data are also given. The performance of the collector, storage, domestic hot water and space heating subsystems, the operating energy, energy savings, and weather conditions are also evaluated. Appended are a system description, performance evaluation techniques and equations, site history, long-term weather data, sensor technology, and typical monthly data. (LEW)

  18. Using the automata processor for fast pattern recognition in high energy physics experiments—A proof of concept

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

    Michael H. L. S. Wang; Cancelo, Gustavo; Green, Christopher; Guo, Deyuan; Wang, Ke; Zmuda, Ted

    2016-06-25

    Here, we explore the Micron Automata Processor (AP) as a suitable commodity technology that can address the growing computational needs of pattern recognition in High Energy Physics (HEP) experiments. A toy detector model is developed for which an electron track confirmation trigger based on the Micron AP serves as a test case. Although primarily meant for high speed text-based searches, we demonstrate a proof of concept for the use of the Micron AP in a HEP trigger application.

  19. Using the automata processor for fast pattern recognition in high energy physics experiments. A proof of concept

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

    Michael H. L. S. Wang; Cancelo, Gustavo; Green, Christopher; Guo, Deyuan; Wang, Ke; Zmuda, Ted

    2016-06-25

    Here, we explore the Micron Automata Processor (AP) as a suitable commodity technology that can address the growing computational needs of pattern recognition in High Energy Physics (HEP) experiments. A toy detector model is developed for which an electron track confirmation trigger based on the Micron AP serves as a test case. Although primarily meant for high speed text-based searches, we demonstrate a proof of concept for the use of the Micron AP in a HEP trigger application.

  20. PROCEEDINGS OF RIKEN BNL RESEARCH CENTER WORKSHOP, VOLUME 57, HIGH PT PHYSICS AT RHIC, DECEMBER 2-6, 2003

    SciTech Connect (OSTI)

    Kretzer, Stefan; Venugopalan, Raju; Vogelsang, Werner

    2004-02-18

    The AuAu, dAu, and pp collision modes of the RHIC collider at BNL have led to the publication of exciting high p{perpendicular} particle production data. There have also been two physics runs with polarized protons, and preliminary results on the double-spin asymmetry for pion production had been presented very recently. The ontological questions behind these measurements are fascinating: Did RHIC collisions create a Quark-Gluon-Plasma phase and did they verify the Color Glass Condensate as the high energy limit of QCD? Will the Spin Crisis finally be resolved in terms of gluon polarization and what new surprises are we yet to meet for Transverse Spin? Phenomena related to sub-microscopic questions as important as these call for interpretations that are footed in solid theory. At large p{perpendicular}, perturbative concepts are legitimately expected to provide useful approaches. The corresponding hard parton dynamics are, in several ways, key to unraveling the initial or final state and collisional phase of hard scattering events in vacuum as well as in hot or cold nuclear matter. Before the advent of RHIC data, a RIKEN-BNL workshop had been held at BNL in March 1999 on ''Hard Parton Physics in High Energy Nuclear Collisions''. The 2003 workshop on ''High p{perpendicular} Physics at RHIC'' was a logical continuation of this previous workshop. It gave the opportunity to revisit the 1999 expectations in the light of what has been found in the meantime and, at the same time, to critically discuss the underlying theoretical concepts. We brought together theorists who have done seminal work on the foundations of parton phenomenology in field theory, with theorists and experimentalists who are presently working on RHIC phenomenology. The participants were both from a high-energy physics and nuclear physics background and it remains only to be said here that this chemistry worked perfectly and the workshop was a great success.

  1. Alternative Fuel School Buses Earn High Marks: Reprint from Alternative Fuel News, Vol. 5, No. 3

    SciTech Connect (OSTI)

    Not Available

    2002-11-01

    A two-page article on school buses that run on alternative fuels including biodiesel and compressed natural gas. Reprinted from Alternative Fuel News, published by the Clean Cities Program of DOE.

  2. Energy Design Guidelines for High Performance Schools: Cold and Humid Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  3. Energy Design Guidelines for High Performance Schools: Temperate and Humid Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  4. Energy Design Guidelines for High Performance Schools: Hot and Dry Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  5. Energy Design Guidelines for High Performance Schools: Hot and Humid Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  6. Energy Design Guidelines for High Performance Schools: Temperate and Mixed Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  7. Energy Design Guidelines for High Performance Schools: Cool and Dry Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  8. Energy Design Guidelines for High Performance Schools: Cool and Humid Climates

    SciTech Connect (OSTI)

    2002-06-01

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  9. Energy Design Guidelines for High Performance Schools: Hot and Humid Climates

    Office of Energy Efficiency and Renewable Energy (EERE)

    School districts around the country are finding that the smart energy choices can help them save money and provide healthier, more effective learning environments. By incorporating energy improvements into their construction or renovation plans,

  10. Middle School Science Bowl

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

    2015 February Middle School Science Bowl Middle School Science Bowl WHEN: Feb 28, 2015 8:00 AM - 4:00 PM WHERE: Highland High School 4700 Coal Ave SE, Albuquerque, NM...

  11. The University of Virginia Experimental and Theoretical High Energy Physics Closeout Report

    SciTech Connect (OSTI)

    Principal Investigator: Harry B. Thacker

    2012-08-13

    The work covered in this report includes a joint project on using gauge-gravity duality to discover qualitatively new results on jet quenching in strongly-coupled QCD-like plasmas. Other topics addressed by the theoretical work include jet stopping and energy loss in weakly-coupled plasmas, perturbative QCD amplitudes, AdS/CMT, dynamical electroweak symmetry breaking with a heavy fourth generation, electroweak-scale #23;{nu}{sub R} model, vacuum topological structure and chiral dynamics in strongly coupled gauge theory. Effort committed to the CMS experiment is reported, particularly the management, maintenance, operation and upgrade of the CMS electromagnetic detector (ECAL). Activities in various physics analyses including Supersymmetry, Higgs, Top, and QCD analyses are reported. Physics projects covering wide areas of physics at the LHC are reported. CY2010 saw the accumulation of a data sample corresponding to approximately 36 pb{sup -1}; in CY 2011 the data sample swelled to more than 5 fb{sup -1}. The UVa CMS analysis efforts are focused on this large 2011 data sample in a suite of crucial measurements and searches. KTeV physics activities are reported. Efforts are reported pertaining to several experiments, including: HyperCP, CKM, MIPP, D?, NO#23;{nu}A, and Mu2e.

  12. Capabilities for measuring physical and chemical properties of rocks at high pressure

    SciTech Connect (OSTI)

    Durham, W.B.

    1990-01-01

    The Experimental Geophysics Group of the Earth Sciences Department at Lawrence Livermore National Laboratory (LLNL) has experimental equipment that measures a variety of physical properties and phase equilibria and kinetics on rocks and minerals at extreme pressures (to 500 GPa) and temperatures (from 10 to 2800 K). These experimental capabilities are described in this report in terms of published results, photographs, and schematic diagrams.

  13. DOE Closeout Report from SUNY Albany High Energy Physics to Department of Energy Office of Science.

    SciTech Connect (OSTI)

    Ernst, Jesse; Jain, Vivek

    2014-08-15

    A report from the SUNY Albany Particle Physics Group summarizing our activities on the ATLAS experiment at the Large Hadron Collider. We summarize our work: on data analysis projects, on efforts to improve detector performance, and on service work to the experiment.

  14. Physics Division News

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

    PADSTE » ADEPS » Physics » Physics Division News Physics Division News Discover more about the wide-ranging scope of Physics Division science and technology. Contact Us ADEPS Communications Email Physics Flash An electronic newsletter featuring interviews with Physics Division staff and news of awards and the latest research published in peer-reviewed journals. Physics Flash archive Focus on Physics Focus on Proton Radiography (pdf) High Energy Physics: LBNE, HAWC (pdf) Nuclear Physics:

  15. High Resolution RANS NLH Study of Stage 67 Tip Injection Physics

    SciTech Connect (OSTI)

    Matheson, Michael A

    2014-01-01

    Numerical prediction of the Stage 67 transonic fan stage employing wall jet tip injection flow control and study of the physical mechanisms leading to stall suppression and stability enhancement afforded by endwall recirculation/injection is the focus of this paper. Reynolds averaged Navier-Stokes computations were used to perform detailed analysis of the Stage 67 configuration experimentally tested at NASA s Glenn Research Center in 2004. Time varying prediction of the stage plus recirculation and injection flowpath were performed utilizing the Nonlinear Harmonic approach. Significantly higher grid resolution per passage was achieved than what has been generally employed in prior reported numerical studies of spike stall phenomena in transonic compressors. This paper focuses on characterizing the physics of spike stall embryonic stage phenomena and the impact of tip injection, resulting in experimentally and numerically demonstrated stall suppression

  16. Status Report of the DPHEP Study Group: Towards a Global Effort for Sustainable Data Preservation in High Energy Physics

    SciTech Connect (OSTI)

    Akopov, Zaven; Amerio, Silvia; Asner, David; Avetisyan, Eduard; Barring, Olof; Beacham, James; Bernardi, Gregorio; Bethke, Siegfried; Boehnlein, Amber; Brooks, Travis; Browder, Thomas; Brun, Rene; Cartaro, Concetta; Cattaneo, Marco; Chen, Gang; Corney, David; Cranmer, Kyle; Culbertson, Ray; Dallmeier-Tiessen, Sunje; Denisov, Dmitri

    2013-03-27

    Data from high-energy physics (HEP) experiments are collected with significant financial and human effort and are mostly unique. An inter-experimental study group on HEP data preservation and long-term analysis was convened as a panel of the International Committee for Future Accelerators (ICFA). The group was formed by large collider-based experiments and investigated the technical and organisational aspects of HEP data preservation. An intermediate report was released in November 2009 addressing the general issues of data preservation in HEP. This paper includes and extends the intermediate report. It provides an analysis of the research case for data preservation and a detailed description of the various projects at experiment, laboratory and international levels. In addition, the paper provides a concrete proposal for an international organisation in charge of the data management and policies in high-energy physics.

  17. Search for new physics in high pT like-sign dilepton events at CDF II

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

    Aaltonen, T.

    2011-10-25

    We present a search for new physics in events with two high pT leptons of the same electric charge, using data with an integrated luminosity of 6.1 fb-1. The observed data are consistent with standard model predictions. We set 95% C.L. lower limits on the mass of doubly-charged scalars decaying to like-sign dileptons, mH±± > 190 - 245 GeV/c2, depending on the decay mode and coupling.

  18. Research in high energy physics. Progress report, 1 July 1993--30 June 1994

    SciTech Connect (OSTI)

    Rosen, J.; Block, M.; Buchholz, D.

    1994-07-01

    Progress on Task A centered around data analysis. E835 is now approved. It will extend E760 studies, exploring new charmonium states and featuring an upgraded detector system plus operation at 4--6 times higher luminosity. Results are given on E760 analysis. Task B has 10 papers that have either appeared in print, or have been prepared for publication. They break down into four categories; experimental physics, theoretical physics, and computer computational techniques. They are described here along with an exciting new experimental proposal to use Da{Phi}ne, the {Phi} factory that is being constructed at Frascati National Laboratory. Progress for Task C which includes participating in the D0 project at TeV I, and the photoproduction experiment, E687, at TeV II is given. While Northwestern is not participating in the top quark physics group at D0, they have been involved in the data analysis and the discussions that led to the limits on the top quark mass. Task D comprises the shared services for the Northwestern DOE contract. This includes the maintenance and operation of all computers within the HEP group. The projects supported by Task D during the past year are given. Task E progress was to resolve the apparent conflict between EMC, SMC, and SLAC results on nucleon structure functions and Bjorken sum rules. Task F covered research in hadronic decay of the tau, thermal field theory, plasma effects in astrophysics, and heavy quarkonium. Task G covers E665, a general purpose muon scattering experiment which can detect both the scattered muon and most charged and neutral hadrons produced in the forward region. The Northwest group has collaborated very closely in the past year with the Harvard group on analyses of structure functions and vector meson production in the 1991 data sample.

  19. Basic physical and chemical information needed for development...

    Office of Scientific and Technical Information (OSTI)

    (i.e., statistical physics and physical kinetics in the language of the Landau school). ... Country of Publication: United States Language: English Subject: 73 NUCLEAR PHYSICS AND ...

  20. High Energy Theory Workshops and Visitors at the Michigan Center for Theoretical Physics FY14

    SciTech Connect (OSTI)

    Pierce, Aaron T.

    2014-04-01

    The workshop was held from September 23-25, 2013 on the University of Michigan campus. Local organizers were Dragan Huterer, Katherine Freese, and Heidi Wu (University of Michigan). Marilena Lo Verde (University of Chicago) also served as an external organizer. This workshop sought to gather experimentalists and theorists to discuss and define directions in cosmology research after the 1st year release of Planck data. The workshop included 35 invited (non-U-M) cosmologists, most of them relatively junior. The workshop was notable for spirited discussion of various theoretical ideas and experimental developments, and particularly on how one could test theory with ongoing and future experiments. In our follow-up poll, 95% of participants reported that interactions with other participants at the workshop may lead to further collaboration. Most participants (again about 95%) reported that they are very satisfied with the quality of the program, information they received, and the logistical support. Slides are available on line at: http://www.umich.edu/~mctp/SciPrgPgs/events/2013/CAP13/program.html. The YHET visitor program invited weekly young visitors to the University of Michigan campus to present their work. This year 23 participants came under the program. Slides are available on line for talks when applicable: http://mctp.physics.lsa.umich.edu/brown-bag-seminar-history/winter 2014 and http://mctp.physics.lsa.umich.edu/brown-bag-seminar-history/fall-2013.

  1. Combined Modular Pumped Hydro Energy Storage Plus Solar PV Proposal for Rio Rancho High School, New Mexico

    SciTech Connect (OSTI)

    Bibeault, Mark Leonide

    2015-08-25

    This is a proposal to locate a combined Modular Pumped Hydro (MPH) Energy Storage plus PV solar facility at Rio Rancho High School, NM. The facility will functionally provide electricity at night derived from renewable solar energy. Additionally the facility will provide STEM related educational opportunities for students and staff of the school, public community outreach, and validation of an energy storage approach applicable for the Nation (up to 1,000,000 kWh per installation). The proposal will summarize the nature of electricity, why energy storage is useful, present the combined MPH and solar PV production design, present how the actual design will be built and operated in a sustainable manner, how the project could be funded, and how the project could be used in STEM related activities.

  2. High Energy Density Physics and Applications with a State-of-the-Art Compact X-Pinch

    SciTech Connect (OSTI)

    Beg, Farhat N

    2013-08-14

    Recent advances in technology has made possible to create matter with extremely high energy density (energy densities and pressure exceeding 1011 J/m3 and 1 Mbar respectively). The field is new and complex. The basic question for high energy density physics (HEDP) is how does matter behave under extreme conditions of temperature, pressure, density and electromagnetic radiation? The conditions for studying HEDP are normally produced using high intensity short pulse laser, x-rays, particle beams and pulsed power z-pinches. Most of these installations occupy a large laboratory floor space and require a team consisting of a large number of scientists and engineers. This limits the number of experiments that can be performed to explore and understand the complex physics. A novel way of studying HEDP is with a compact x-pinch in university scale laboratory. The x-pinch is a configuration in which a pulsed current is passed through two or more wires placed between the electrodes making the shape of the letter ‘X’. Extreme conditions of magnetic field (> 200 MGauss for less than 1 ns), temperature (1 keV) and density (~ 1022 cm-3) are produced at the cross-point, where two wires make contact. Further, supersonic jets are produced on either side of the cross-point. The physics of the formation of the plasma at the cross-point is complex. It is not clear what role radiation plays in the formation of high energy density plasma (>> 1011 J/m3) at the cross-point. Nor it is understood how the supersonic jets are formed. Present numerical codes do not contain complex physics that can take into account some of these aspects. Indeed, a comprehensive experimental study could answer some of the questions, which are relevant to wide-ranging fields such as inertial confinement fusion, astrophysical plasmas, high intensity laser plasma interactions and radiation physics. The main aim of the proposal was to increase the fundamental understanding of high energy density physics and

  3. Optical coatings of variable refractive index and high laser-resistance from physical-vapor-deposited perfluorinated amorphous polymer

    DOE Patents [OSTI]

    Chow, Robert; Loomis, Gary E.; Thomas, Ian M.

    1999-01-01

    Variable index optical single-layers, optical multilayer, and laser-resistant coatings were made from a perfluorinated amorphous polymer material by physical vapor deposition. This was accomplished by physically vapor depositing a polymer material, such as bulk Teflon AF2400, for example, to form thin layers that have a very low refractive index (.about.1.10-1.31) and are highly transparent from the ultra-violet through the near infrared regime, and maintain the low refractive index of the bulk material. The refractive index can be varied by simply varying one process parameter, either the deposition rate or the substrate temperature. The thus forming coatings may be utilized in anti-reflectors and graded anti-reflection coatings, as well as in optical layers for laser-resistant coatings at optical wavelengths of less than about 2000 nm.

  4. Optical coatings of variable refractive index and high laser-resistance from physical-vapor-deposited perfluorinated amorphous polymer

    DOE Patents [OSTI]

    Chow, R.; Loomis, G.E.; Thomas, I.M.

    1999-03-16

    Variable index optical single-layers, optical multilayer, and laser-resistant coatings were made from a perfluorinated amorphous polymer material by physical vapor deposition. This was accomplished by physically vapor depositing a polymer material, such as bulk Teflon AF2400, for example, to form thin layers that have a very low refractive index (ca. 1.10--1.31) and are highly transparent from the ultra-violet through the near infrared regime, and maintain the low refractive index of the bulk material. The refractive index can be varied by simply varying one process parameter, either the deposition rate or the substrate temperature. The thus forming coatings may be utilized in anti-reflectors and graded anti-reflection coatings, as well as in optical layers for laser-resistant coatings at optical wavelengths of less than about 2000 nm. 2 figs.

  5. Minnesota Regional Science Bowl for Middle School Students |...

    Office of Science (SC) Website

    Minnesota Regions Minnesota Regional Science Bowl for Middle School Students National Science Bowl (NSB) NSB Home About High School Middle School Middle School Students Middle ...

  6. Natural Gas Study Guide - Middle School | Department of Energy

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

    Middle School Natural Gas Study Guide - Middle School Natural Gas Study Guide - Middle School (246.85 KB) More Documents & Publications Natural Gas Study Guide - High School What ...

  7. D.C. Middle and High School Students Get a Chance to Experience...

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

    country to compete in a fast-paced question and answer format being tested on a range of science disciplines including biology, chemistry, Earth science, physics, energy and math. ...

  8. Middle School Students | U.S. DOE Office of Science (SC)

    Office of Science (SC) Website

    Students National Science Bowl (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Attending the National Finals ...

  9. Plasma Physics

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

    plasma physics Plasma Physics Almost all of the observable matter in the universe is in the plasma state. Formed at high temperatures, plasmas consist of freely moving ions and free electrons. They are often called the "fourth state of matter" because their unique physical properties distinguish them from solids, liquids and gases. Plasma densities and temperatures vary widely, from the cold gases of interstellar space to the extraordinarily hot, dense cores of stars and inside a

  10. Theoretical Physics

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

    HEP Theoretical Physics Understanding discoveries at the Energy, Intensity, and Cosmic Frontiers Get Expertise Rajan Gupta (505) 667-7664 Email Bruce Carlsten (505) 667-5657 Email HEP Theory at Los Alamos The Theoretical High Energy Physics group at Los Alamos National Laboratory is active in a number of diverse areas of research. Their primary areas of interest are in physics beyond the Standard Model, cosmology, dark matter, lattice quantum chromodynamics, neutrinos, the fundamentals of

  11. High Energy Theory Workshops and Visitors at the Michigan Center for Theoretical Physics FY15

    SciTech Connect (OSTI)

    Pierce, Aaron T.

    2015-09-18

    The String theory workshop was held from March 4-7, 2015 on the University of Michigan campus. Local organizers were Gordon Kane and Aaron Pierce. Piyush Kumar (Yale), Jim Halverson (KITP), Bobby Acharya (ICTP) and Sven Krippendorf (Oxford) served as external organizers.The meeting focused on the status of work to project 10 or 11 dimensional string/M theories onto our 4 spacetime dimensions (compactification). The workshop had 31 participants, half from outside the U.S. Participants were encouraged to focus on predictions for recent and forthcoming data, particularly for Higgs physics and LHC and dark matter, rather than on the traditional approach of embedding the Standard Model particles and forces. The Higgs boson sympoosium was locally organized by James Wells (chair), Aaron Pierce and Jianming Qian. Additional input in the early stages by Stefan Pokorski (Warsaw) who was unable to attend in the end. The workshop consistent of 22 talks from experts around the world, both theoretical and experimental. Experimentalists summarized the current state of knowledge of the Higgs boson and its varients. The theory talks ranged from technical calculations of Standard Model processes to speculative novel ideas. The YHET visitor program invited weekly young visitors to the University of Michigan campus to present their work. This year 24 participants came under the program, with 17 of them receiving at least partial support for their visits.

  12. High energy physics research. Final report, October 1, 1969--December 31, 1990

    SciTech Connect (OSTI)

    1995-05-01

    The goal of this research was to understand the fundamental constituents of matter and their interactions. First, a brief history of the high energy research at Princeton University is presented. Next, the extensive research covered in this 21 year period is summarized. Finally, a list of all publications issued during this period is presented.

  13. Atomic physics with highly charged ions. Progress report, FY 1989--91

    SciTech Connect (OSTI)

    Richard, P.

    1991-08-01

    This report discusses: One electron outer shell processes in fast ion-atom collisions; role of electron-electron interaction in two-electron processes; multi-electron processes at low energy; multi-electron processes at high energy; inner shell processes; molecular fragmentation studies; theory; and, JRM laboratory operations.

  14. Search for new physics in high pT like-sign dilepton events at CDF II

    SciTech Connect (OSTI)

    Aaltonen, T.

    2011-10-25

    We present a search for new physics in events with two high pT leptons of the same electric charge, using data with an integrated luminosity of 6.1 fb-1. The observed data are consistent with standard model predictions. We set 95% C.L. lower limits on the mass of doubly-charged scalars decaying to like-sign dileptons, mH > 190 - 245 GeV/c2, depending on the decay mode and coupling.

  15. physics-based-html

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

    Physics-based High-Resolution Numerical Modeling of Bridge Foundation Scour

  16. Preliminary Physics Motivation and Engineering Design Assessment of the National High Power Torus

    SciTech Connect (OSTI)

    Robert D. Woolley

    2009-06-11

    In April 2006, Dr. Ray Orbach, Director of the DOE Office of Science, challenged the fusion community to "propose a new facility... which will put the U.S. at the lead in world fusion science." Analysis of the gaps between expected ITER performance and the requirements of a demonstration power plant (Demo) pointed to the critical and urgent need to develop fusion-relvant plasma-material interface (PMI) solutions consistent with sustained high plasma performance. A survey of world fusion program indicated that present and planned experimental devices do not advance the PMI issue beyond ITER, and a major dedicated experimental facility is warranted. Such a facility should provide the flexibility and access needed to solve plasma boundary challenges related to divertor heat flux and particle exhaust while also developing methods to minimize hydrogenic isotope retention and remaining compatible with high plasma performance.

  17. HepSim: A Repository with Predictions for High-Energy Physics Experiments

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

    Chekanov, S. V.

    2015-01-01

    A file repository for calculations of cross sections and kinematic distributions using Monte Carlo generators for high-energy collisions is discussed. The repository is used to facilitate effective preservation and archiving of data from theoretical calculations and for comparisons with experimental data. The HepSim data library is publicly accessible and includes a number of Monte Carlo event samples with Standard Model predictions for current and future experiments. The HepSim project includes a software package to automate the process of downloading and viewing online Monte Carlo event samples. Data streaming over a network for end-user analysis is discussed.

  18. Physics of laser fusion. Volume IV. The future development of high-power solid-state laser systems

    SciTech Connect (OSTI)

    Emmett, J.L.; Krupke, W.F.; Trenholme, J.B.

    1982-11-01

    Solid state lasers, particularly neodymium glass systems, have undergone intensive development during the last decade. In this paper, we review solid state laser technology in the context of high-peak-power systems for inertial confinement fusion. Specifically addressed are five major factors: efficiency, wavelength flexibility, average power, system complexity, and cost; these factors today limit broader application of the technology. We conclude that each of these factors can be greatly improved within current fundamental physical limits. We further conclude that the systematic development of new solid state laser madia, both vitreous and crystalline, should ultimately permit the development of wavelength-flexible, very high average power systems with overall efficiencies in the range of 10 to 20%.

  19. Final Report for Research in High Energy Physics at the University of Pennsylvania for the period ending April 30, 2012

    SciTech Connect (OSTI)

    Williams, Hugh H.; Balasubramanian, V.; Bernstein, G.; Beier, E. W.; Cvetic, M.; Gladney, L.; Jain, B.; Klein, J.; Kroll, J.; Lipeles, E.; Ovrut, B.; Thomson, E.

    2015-07-23

    The University of Pennsylvania elementary particle physics/particle cosmology group, funded by the Department of Energy Office of Science, participates in research in high energy physics and particle cosmology that addresses some of the most important unanswered questions in science. The research is divided into five areas. Energy Frontier - We participate in the study of proton-proton collisions at the Large Hadron Collider in Geneva, Switzerland using the ATLAS detector. The University of Pennsylvania group was responsible for the design, installation, and commissioning of the front-end electronics for the Transition Radiation Tracker (TRT) and plays the primary role in its maintenance and operation. We play an important role in the triggering of ATLAS, and we have made large contributions to the TRT performance and to the study and identification of electrons, photons, and taus. We have been actively involved in searches for the Higgs boson and for SUSY and other exotic particles. We have made significant contributions to measurement of Standard Model processes such as inclusive photon production and WW pair production. We also have participated significantly in R&D for upgrades to the ATLAS detector. Cosmic Frontier - The Dark Energy Survey (DES) telescope will be used to elucidate the nature of dark energy and the distribution of dark matter. Penn has played a leading role both in the use of weak gravitational lensing of distant galaxies and the discovery of large numbers of distant supernovae. The techniques and forecasts developed at Penn are also guiding the development of the proposed Large Synoptic Survey Telescope (LSST).We are also developing a new detector, MiniClean, to search for direct detection of dark matter particles. Intensity Frontier - We are participating in the design and R&D of detectors for the Long Baseline Neutrino Experiment (now DUNE), a new experiment to study the properties of neutrinos. Advanced Techology R&D - We have an extensive

  20. REPORT OF RESEARCH ACTIVITIES FOR THE YEARS 2000 - 2003; HIGH ENERGY PHYSICS GROUP; SOUTHERN METHODIST UNIVERSITY; EXPERIMENTAL TASK A AND THEORY TASK B

    SciTech Connect (OSTI)

    Dr. Ryszard Stroynowski

    2003-07-01

    The experimental program in High Energy Physics at SMU was initiated in 1992. Its main goal is the search for new physics phenomena beyond the Standard Model (SSC, LHC) and the study of the properties of heavy quarks and leptons (CLEO, BTeV).