Geometry.Net - the online learning center
Home  - Basic_H - High Energy & Nuclear Physics
e99.com Bookstore
  
Images 
Newsgroups
Page 6     101-114 of 114    Back | 1  | 2  | 3  | 4  | 5  | 6 
A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z  

         High Energy & Nuclear Physics:     more books (100)
  1. Proceedings of the 30th International Conference on High Energy Physics, Osaka, Japan, 27 July - 2 August 2000 by Japan) International Conference on High Energy Physics 2000 (Osaka, C. S. Lim, et all 2001-06
  2. Introduction to High Energy Physics by Donald H. Perkins, 2000-04-24
  3. A Modern Introduction to Particle Physics (High Energy Physics) by Fayyazuddin, Riazuddin, 2000-09-29
  4. Particle and Astroparticle Physics (Series in High Energy Physics, Cosmology and Gravitation) by Utpal Sarkar, 2007-12-03
  5. Hadronic Probes and Nuclear Interactions (AIP Conference Proceedings)
  6. High-Energy-Density Physics: Fundamentals, Inertial Fusion, and Experimental Astrophysics (Shock Wave and High Pressure Phenomena) by R. Paul Drake, 2006-06-02
  7. High Energy Astrophysics: Volume 1, Particles, Photons and their Detection (High Energy Astrophysics) by Malcolm S. Longair, 1992-03-27
  8. High-Energy Particle Diffraction (Theoretical and Mathematical Physics) by Vincenzo Barone, Enrico Predazzi, 2002-04-08
  9. Lectures on high energy physics delivered at the Sixth Summer Meeting of Nuclear Physicists, July - August 1961. by B., editor. JASIC, 1961
  10. An Introduction to the Physics of High Energy Accelerators (Wiley Series in Beam Physics and Accelerator Technology) by D. A. Edwards, M. J. Syphers, 1992-11
  11. Instrumentation in High Energy Physics (Advanced Series on Directions in High Energy Physics)
  12. Nuclei, Neutrons, and Energy: Proceedings of the VIII International School on Nuclear Physics, Neutron Physics, and Nuclear Energy by W. Andrejtscheff, Chr V. Christov, 1988-10
  13. Introduction to Nuclear And Particle Physics by C. Bromberg, A Das, et all 2006-08-25
  14. Techniques and Concepts of High-Energy Physics II (Nato a S I Series Series B, Physics) by Thomas Ferbel, 1983-09-01

101. High Energy & Nuclear Physics Directorate
high energy and nuclear physics at BNL comprises the ColliderAccelerator Department (including the NASA Space Radiation Laboratory, NSRL), the physics
http://www.bnl.gov/henp/
BNL: Departments Science Newsroom Administration ... Directory search
Site Details HENP Home HENP Program Advisory Committee NASA Radiobiology Program Directorate Orgs Physics Department Collider-Accelerator Dept. Instrumentation Division Superconducting Magnet Division RHIC Links RHIC/AGS Proposal Submission Procedure RHIC Planning Documents Can't View PDFs?
High Energy and Nuclear Physics at BNL comprises the Collider-Accelerator Department (including the NASA Space Radiation Laboratory, NSRL), the Physics Department, the Instrumentation Division, and the Superconducting Magnet Division. (See department/division descriptions , pdf) Links to department/division web pages may be found to the left.
HENP Program Advisory Committee
NOTE on PDFs: If your browser displays a blank page for any pdf document, either: 1) copy the file to your computer and then display it with Acrobat; or 2) configure your local Acrobat reader to display in a separate window. This is an Adobe/Microsoft incompatibility problem, for which there is as yet no more elegant fix. Full details
Reference Documents
Decadal Planning for RHIC Experiments
BRAHMS PHENIX Phobos STAR ... Detector Advisory Committee Report
Other RHIC Documents

102. Samuel Aronson Named Associate Laboratory Director For High Energy And Nuclear P
“The high energy and nuclear physics Directorate has had a long and productive tradition at the Laboratory, with many important discoveries and the
http://www.bnl.gov/bnlweb/pubaf/pr/PR_display.asp?prID=05-40

103. High Energy And Nuclear Physics
The Office of high energy and nuclear physics is a $1 billion per year basic research program that provides new insights into the nature of energy and
http://www.nersc.gov/news/greenbook/nersc3/node10.html
National Energy Research Scientific Computing Center A DOE Office of Science User Facility
at Lawrence Berkeley National Laboratory
Home About HPC Users ... Projects
NERSC 3 Greenbook
Next: Lattice Field Theory Up: Representative Energy Research Scientific Previous: Representative Energy Research Scientific
High Energy and Nuclear Physics
The Office of High Energy and Nuclear Physics is a $1 billion per year basic research program that provides new insights into the nature of energy and matter and operates large world-class scientific facilities for the nation and the international community. High energy and nuclear physics research is conducted by over 3,000 researchers and over 1,000 graduate students from over 100 universities and the National Laboratories. High Energy and Nuclear Physics are concerned with understanding of matter and space-time at the fundamental level. There are many unanswered questions:
  • Why is the electron lighter than the proton?
  • Why is there more matter than antimatter in the universe?
  • What was matter like in the early moments of the universe?

104. NERSC 2000 Annual Report: Science Highlights: High Energy And Nuclear Physics
Biological and Environmental Research Fusion energy Sciences high energy and nuclear physics Advanced Scientific Computing Research and Other Projects
http://www.nersc.gov/news/annual_reports/annrep00/sh_HENP_01.html
Annual Report
TABLE OF CONTENTS
YEAR IN REVIEW SCIENCE HIGHLIGHTS SCIENCE HIGHLIGHTS:
HIGH ENERGY AND NUCLEAR PHYSICS Phenomenology with O a ) Improved Lattice QCD Director's
Perspective
YEAR IN REVIEW Computational Science BOOMERANG Data, Analyzed at NERSC, Reveals Flat Universe Systems and Service IBM SP Launched Ahead of Schedule with Million-Hour Bonus for Users ... Deb Agarwal Named One of "Top 25 Women of the Web" SCIENCE HIGHLIGHTS Basic Energy Sciences Biological and Environmental Research Fusion Energy Sciences High Energy and Nuclear Physics ... Advanced Scientific Computing Research and Other Projects
A fit of the form c V = c V + c V ) to extract the improvement constant for the vector current. The pole term is an artifact of lattice discretization, and resolved in our calculation. Rajan Gupta, Tanmoy Bhattacharya, and Weonjong Lee, Los Alamos National Laboratory
Stephen Sharpe, University of Washington

105. THE 2002 EUROPEAN SCHOOL OF HIGH-ENERGY PHYSICS
The tenth European School of highenergy physics will be hosted by the NESTOR N. Ellis (CERN); E. Floratos (University of Athens and nuclear physics
http://physicschool.web.cern.ch/PhysicSchool/2002/Welcome.html
The 2002 European School of High-Energy Physics
Pylos, Greece
25 August - 7 September 2002
The 2002 European School of High-Energy Physics (formerly the CERN-JINR School of Physics) will be organized jointly by the European Organization for Nuclear Research (CERN) , Geneva, Switzerland, and the Joint Institute for Nuclear Research (JINR) , Dubna, Russia, together with the NESTOR Institute for Deep Sea Research, Technology, and Neutrino Astroparticle Physics, Pylos, Greece. The basic aim of the School is to teach various aspects of high-energy physics, but especially theoretical physics, to young experimental physicists, mainly from the Member States of CERN and of JINR. The Schools of Physics are designed to give a survey of up-to-date information, rather than to be a training course. Reading lists and an outline of each of the lecture courses will be sent to the selected students in late Spring 2002 together with their letters of acceptance.
Date and Place of the School Accommodation Scientific Programme Discussion Sessions ... Poster for the School (Poster)

Date and place of the School
The tenth European School of High-Energy Physics will be hosted by the NESTOR Institute in Pylos, Greece, from Sunday 25th August to Saturday 7th September 2002.

106. BNL HET & NT PAGE
high energy, Lattice Gauge, and nuclear Theory Groups at Brookhaven National Theory high energy/RIKEN and nuclear/RIKEN Particle physics seminars
http://thy.phy.bnl.gov/
High Energy, Lattice Gauge, and Nuclear Theory Groups at Brookhaven National Laboratory.

107. The Office Of Science - Home Page
nuclear energy and Science for the 21st Century Atoms for Peace Plus 50 October 22, high energy physics nuclear physics - Workforce Development for
http://www.science.doe.gov/
Contact Web Publishing Inventory Site Map Privacy Policy
FirstGov for Science
Relief for Researchers Affected by Hurricane Katrina Letter from Dr. Raymond L. Orbach, Director of the Office of Science, to the science community In Memory of John N. Bahcall Tribute to Dr. John N. Bahcall by Dr. Raymond L. Orbach, Director, Office of Science Solar Energy Workshop Report DOE Outlines Research Needed to Improve Solar Energy Technologies Basic Research Needs for Solar Energy Utilization
Report of the Basic Energy Sciences Workshop on Solar Energy Utilization,
April 18-21, 2005 Rice Genome Sequence International Rice Genome Sequence Effort Completed Multiscale Mathematics Awards New DOE Program Funds $20 Million for Mathematics Research FY 2005 Multiscale Mathematics Research Awards Lawrence Livermore Researchers Capture Four Awards for Industrial Innovation Call for Proposals for High Performance Computing Resources Energy Department Seeks Proposals to Use Scientific Computing Resources at Lawrence Berkeley, Oak Ridge National Laboratories

108. Partice Theory Department
in the Henryk Niewodniczanski Instutute of nuclear physics, Cracow, Poland, network HPRNCT-2000-00149 Particle physics Phenomenology at high energy
http://hpjmiady.ifj.edu.pl/
Department of the Particle Theory
in the Henryk Niewodniczanski Instutute of Nuclear Physics Cracow Poland
Our address is now "MAIN SITE!!!"
tel (secretariat): +48.12.662 8010 fax: +48.12.662.8012 Department Head: Maciej Skrzypek Physicists: We are participating in the 5-th Framework network HPRN-CT-2000-00149 Particle Physics Phenomenology at High Energy Colliders together with the particle theory groups at University of Silesia and Warsaw University From Jul 1, 2004 we participate also in Marie Curie Actions Human resources and mobility Research Programme FP6 : Framework Programme 6, contract MTKD-CT-2004-510126, see the web page `Calculational Tools and Methods for Physics at Large Hadron Collider' , for details and job vacancies which we offer; `how to apply' Our Polish Funding Agency KBN We organize anually Cracow Epiphany Conference on Partice Physics and Astrophysics Our resources (old ones, see individual home pages for the actual versions):
PAPERS
PROGRAMS Collaborating PhD students : Other collaborators, other links:

109. The Nuclear Weapon Archive - A Guide To Nuclear Weapons
nuclear Data Center of the Japan Atomic energy Research Institute (JAERI). This is an excellent source of nuclear physics data also.
http://nuclearweaponarchive.org/
The Nuclear Weapon Archive
A Guide to Nuclear Weapons
If we fight a war and win it with H-bombs, what history will remember is not
the ideals we were fighting for but the methods we used to accomplish them.
These methods will be compared to the warfare of Genghis Khan who ruthlessly
killed every last inhabitant of Persia.
Hans A. Bethe ...And these atomic bombs which science burst upon the world that night were strange even to the men who used them.
H. G. Wells, The World Set Free
About This Site
Archive Charter Archive History Notable Quotes About the Graphics Used ... Credits and Thanks A "sister site" relationship has been established with Gregory Walker's Trinity Site . Greg and I are actively collaborating to provide the broadest variety of nuclear weapon information, in the most convenient form that we can. The two sites each have a different focus. The Nuclear Weapon Archive provides current information, technical data, and informative write-ups. The Trinity Site focuses on historical information, especially reproductions of public domain documents.
Latest Site Updates
17 August 2003
  • Site is retitled The Nuclear Weapon Archive with its own domain.

110. Institute Of Physics - About The Institute Of Physics
high energy Particle physics higher Education History of physics The Institute of physics undertakes to provide administrative support,
http://about.iop.org/IOP/Groups/
Divisions and Groups
Divisions
The Divisions act as forums for reviewing research and development in their respective field of physics. Each Division comprises several Subject Groups coming within its area of interest and in collaboration with those Groups organises an annual or biennial conference. Through the Divisional Affairs Committee the Divisions are invited by the Engineering and Physical Sciences Research Council (EPSRC) to comment on the its Business Plans for Physics and Materials. There are currently five Divisions: Groups
The Subject Groups are concerned with the specialist subject areas of physics, the Professional Groups with the application of physics in research, development and manufacture across a wide range of disciplines. In addition to arranging meetings and conferences, the majority of Groups produce regular newsletters keeping their members in touch with the latest developments in their field and providing information on relevant meetings organised by other bodies. Some Subject Groups make bursaries available to help students attend conferences. Several of the Groups are organised jointly with other societies with similar interests.

111. Basic Nuclear Science Information
In fact, nuclear fusion reactions are responsible for the energy output of most high energy electrons, protons, and complex nuclei can be produced in a
http://www.lbl.gov/abc/Basic.html
ABC's of Nuclear Science
Nuclear Structure Radioactivity Alpha Decay Beta Decay ... Antimatter
Nuclear Structure
An atom consists of an extremely small, positively charged nucleus surrounded by a cloud of negatively charged electrons . Although typically the nucleus is less than one ten-thousandth the size of the atom, the nucleus contains more than 99.9% of the mass of the atom! Nuclei consist of positively charged protons and electrically neutral neutrons held together by the so-called strong or nuclear force. This force is much stronger than the familiar electrostatic force that binds the electrons to the nucleus, but its range is limited to distances on the order of a few x10 meters.
The number of protons in the nucleus, Z, is called the atomic number . This determines what chemical element the atom is. The number of neutrons in the nucleus is denoted by N . The atomic mass of the nucleus, A, is equal to Z + N . A given element can have many different isotopes, which differ from one another by the number of neutrons contained in the nuclei. In a neutral atom, the number of electrons orbiting the nucleus equals the number of protons in the nucleus. Since the electric charges of the proton and the electron are +1 and-1 respectively (in units of the proton charge), the net charge of the atom is zero. At present, there are 112 known elements which range from the lightest, hydrogen, to the recently discovered and yet to-be-named element 112. All of the elements heavier than uranium are man made. Among the elements are approximately 270 stable isotopes, and more than 2000 unstable isotopes.

112. Imagine The Universe! Dictionary
Laboratory for high energy Astrophysics, located at NASA s Goddard Space Flight Center. A unit of energy used to describe nuclear warheads.
http://imagine.gsfc.nasa.gov/docs/dictionary.html
What's New
Site Map

NASA Homepage

Search:
... Feedback
Imagine the Universe! Dictionary
Please allow the whole page to load before you start searching for an entry. Otherwise, errors will occur. A B C D ... Z (Note - Greek letters are written out by name - alpha, beta etc.)
A
accretion
Accumulation of dust and gas onto larger bodies such as stars, planets and moons. accretion disk
A relatively flat sheet of gas and dust surrounding a newborn star, a black hole, or any massive object growing in size by attracting material. active galactic nuclei (AGN)
A class of galaxies which spew massive amounts of energy from their centers, far more than ordinary galaxies. Many astronomers believe supermassive black holes may lie at the center of these galaxies and power their explosive energy output.
angstrom
A unit of length equal to 0.00000001 centimeters. This may also be written as 1 x 10 cm (see scientific notation angular momentum
A quantity obtained by multiplying the mass of an orbiting body by its velocity and the radius of its orbit. According to the conservation laws of physics, the angular momentum of any orbiting body must remain constant at all points in the orbit, i.e., it cannot be created or destroyed. If the orbit is elliptical the radius will vary. Since the mass is constant, the velocity changes. Thus planets in elliptical orbits travel faster at perihelion and more slowly at aphelion . A spinning body also possesses spin angular momentum.

113. Institute Of Nuclear Physics - NCSR Demokritos
The Institute of nuclear physics is working within the National Research Center Demokritos since 1987.
http://www.inp.demokritos.gr/

114. CHEP 01
The summary for this English page contains characters that cannot be correctly displayed in this language/character set.
http://www.ihep.ac.cn/~chep01/

A  B  C  D  E  F  G  H  I  J  K  L  M  N  O  P  Q  R  S  T  U  V  W  X  Y  Z  

Page 6     101-114 of 114    Back | 1  | 2  | 3  | 4  | 5  | 6 

free hit counter