AstroWeb: Physics Resources

ALEPH Experiment (CERN)
http://alephwww.cern.ch/WWW/
APS - What's New?
Physics newsflashes by Bob Park, American Physical Society. If you wish to subscribe to What's New by e-mail, send a message to listserv@aps.org and in the body of the message say `sub whatsnew'.
http://www.aps.org/WN/
Albert-Ludwigs-Universität Freiburg - Fakultät für Physik (Univ. Freiburg-im-Breisgau)
http://hpfrs6.physik.uni-freiburg.de/
American Institute of Physics (AIP)
The American Institute of Physics (AIP) is a not-for-profit membership corporation chartered in New York State in 1931 for the purpose of promoting the advancement and diffusion of the knowledge of physics and its application to human welfare.
http://www.aip.org/
American Physical Society (APS)
On-line information includes the APS E-Print Archive Forum.
http://www.aps.org/
Argonne National Laboratory (ANL)
http://www.anl.gov/
Aspen Center for Physics (ACP)
The Aspen Center for Physics is a scientific organization which promotes organized research in physics, astrophysics and related fields through a program of individual and collaborative research, seminars, workshops and conferences and which promotes the education of the general public through public lectures and other activities.
http://andy.bu.edu/aspen/
Astronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES)
ANTARES is a project which aims at a large scale high energy cosmic neutrino water cherenkov detector.
http://antares.in2p3.fr/antares/
Atomic Line List
The atomic line list is a compilation of approximately 855,000 allowed, intercombination and forbidden atomic transitions with wavelengths in the range from 0.5 Å to 1000 µm. Its primary intention is to allow the identification of observed atomic absorption or emission features. The list is nearly complete for all ionization stages of all elements up to zinc. Transition probabilities are available for nearly 14% of the lines; they are mostly derived from Opacity Project data.
http://www.pa.uky.edu/~peter/atomic/
Basel Theoretical Nuclear/Particle Physics and Astrophysics Group (tNPA Uni Basel)
This is Quasar, the server of the theoretical Nuclear/Particle Physics and Astrophysics groups at the Dept. of Physics of the University of Basel, Switzerland. The server offers information on people, research topics, publications, and teaching as well as personal home pages and preprints. Research topics in astrophysics include nucleosynthesis, type I and II supernovae, nuclear astrophysics, nuclear physics far from stability, neutrino physics; other research interests are atomic physics and chaos. (For a full list, take a look at the server)!
http://quasar.physik.unibas.ch/
Brookhaven National Laboratory (BNL)
http://www.bnl.gov/
Brown University (High-Energy Physics Group)
http://www.het.brown.edu/
CERN Preprint Server
http://weblib.cern.ch/
CHIANTI: A database for astrophysical emission line spectroscopy (CHIANTI)
CHIANTI is a database that contains the most accurate data available for the calculation of emission line intensities as a function of both temperature and density. The database is essentially complete for wavelengths greater than 50 Angstroms and is to be extended to shorter wavelength. A library of IDL procedures is included.
http://wwwsolar.nrl.navy.mil/chianti.html
CLOUDY - Photoionization Simulation code (CLOUDY)
Cloudy is a large-scale Fortran code designed to simulate physical conditions in a broad range of astronomical plasmas, and predict its resulting spectrum. The Cloudy homepage provides pointers to the code and its documentation, along with related publications and activities.
http://www.pa.uky.edu/~gary/cloudy
INACTIVE LINK ? - 11 --- CMB Astrophysics Research Program (UC Berkeley, LBL)
Professor George Smoot's group conducts research on the early Universe using the cosmic microwave background radiation (CMB) and other astrophysical sources. These investigations are directed towards realizing a variety of science goals regarding CMB.
http://spectrum.lbl.gov/
California Institute of Technology Theoretical Particle Physics (CalTech)
http://www.theory.caltech.edu/
Center for Subatomic Research (CSR)
http://www.phys.ualberta.ca/
Centre Européen pour la Recherche Nucláaire (1) (CERN)
http://www1.cern.ch/
Centre de Physique Theorique (CPT)
Centre de Physique Theorique, Marseille, France.
http://www.cpt.univ-mrs.fr/
Centre de Physique des Particules de Marseille (CPPM)
[in French]
http://marwww.in2p3.fr/
Cornell University Theory Center
http://www.tc.cornell.edu/ctc.html
DELPHI experiment (CERN)
http://www1.cern.ch/Delphi/Welcome.html
Departamento de Física Teorica de la Universidad de Zaragoza (DFTUZ)
http://dftuz.unizar.es/
Deutsches Elektronen-Synchrotron (DESY)
http://www.desy.de/
Durham/RAL HEP Databases
http://cpt1.dur.ac.uk/HEPDATA
Dynamics of Astrophysical Discs
A six-month research programme (08 Jan - 03 Jul 98) at the Isaac Newton Institute for Mathematical Sciences, Cambridge, UK. The programme brought together experts from relevant areas in astrophysics and mathematicians and scientists familiar with appropriate analytic methods and numerical simulation techniques, including the solution of differential or integro-differential equations.
http://www.newton.cam.ac.uk/programs/old_progs/dad.html
Earth Observation Science group, Leicester University (EOS group)
Find out about the varied research projects and teaching activities of the EOS group at Leicester University. See the satellite image gallery, learn about the ATSR space-bourne instruments and read about the successful MSc course in Earth Observation Science.
http://www.le.ac.uk/physics/research/eos/
European Incoherent Scatter (EISCAT)
http://seldon.eiscat.no/
European Physical Society (EPS)
http://epswww.epfl.ch/
Exploration of the Earth's Magnetosphere
A collection of more than eighty linked files, forming a non-mathematical introduction to magnetism, plasmas, particles of space and their motion, and the study of the Earth's magnetic environment in space. Also covers the Sun and solar activity, magnetospheres of other planets, and amny other topics. the exposition follows a historical framework, and includes numerous historical side-excursions. Also includes a long review (more technical) "A Brief History of Magnetospheric Physics During the Space Age, an article "Birth of a Radiation Belt", a guide for teachers, a historical timeline, a question-and-answer collection and a template for a folded paper model of the magnetosphere.
http://www-spof.gsfc.nasa.gov/Education/Intro.html
Falling into a Black Hole
In which we fall into a black hole on a real free fall orbit. All distortions of images are real, both general relativistic from the gravitational bending of light, and special relativistic from the near light speed orbit. After you are done dying at the central singularity of the black hole, feel free to explore more about the Schwarzschild geometry, about wormholes, and about the collapse of a black hole.
http://casa.colorado.edu/~ajsh/schw.html
Fermilab
http://www.fnal.gov/
Fermilab Library
http://fnalpubs.fnal.gov/library/welcome.html
GALLEX
The GALLEX experiment was performed by an international collaboration headed by MPIK Heidelberg. GALLEX measured the solar neutrino flux produced inside the Sun by proton-proton fusion. As target for neutrino capture, a large amount (30 tons) of the rare element Gallium in form of an aqueous solution of Galliumtrichloride was used. To protect the detector from the interfering cosmic radiation one must go deep underground. Hence the experiment was carried out under the shielding of Italy's highest mountain outside the Alps, the Gran Sasso d'Italia in the Abruzzo region.
http://www.mpi-hd.mpg.de/kirsten/gallex.html
General Relativity around the world
http://jean-luc.ncsa.uiuc.edu/World/world.html
Gravity Probe B Relativity Mission (Stanford)
Gravity Probe B is the relativity gyroscope experiment being developed by NASA and Stanford University to test two extraordinary, unverified predictions of Albert Einstein's general theory of relativity. The experiment will check, very precisely, tiny changes in the direction of spin of four gyroscopes contained in an Earth satellite orbiting at 400-mile altitude directly over the poles. So free are the gyroscopes from disturbance that they will provide an almost perfect space-time reference system. They will measure how space and time are warped by the presence of the Earth, and, more profoundly, how the Earth's rotation drags space-time around with it. These effects, though small for the Earth, have far-reaching implications for the nature of matter and the structure of the Universe.
http://einstein.stanford.edu
HERMES Experiment
http://dxhra1.desy.de/
High Energy Gamma Ray Astronomy experiment (HEGRA)
The HEGRA experiment was constructed for investigations of cosmic rays (seen as extended air showers) at energies too high to be detectable by small satellite experiments. The HEGRA detector is sensitive in the energy range from 0.5-10.000 TeV and was designed with special emphasis on the detection of Gamma Rays. HEGRA is located at the Roque de los Muchachos Observatory on La Palma.
http://wpos6.uni-wuppertal.de:8080/
High Energy Physics Information Center (HEPIC)
http://www.hep.net/
High-Energy Physics Information (a resource list from CERN)
http://www.cern.ch/Physics/HEP.html
INTERBALL Exchange Information Server
This server provides the Interball and International scientific community with the means to access to Interball data processed at CNES Toulouse and to exchange files.
http://www-projet.cst.cnes.fr:8000/
Institut National de Physique Nucléaire et de Physique des Particules (IN2P3)
[in French]
http://info.in2p3.fr/
INACTIVE LINK ? - 15 --- Instituto de Astronomia y Fisica del Espacio (IAFE)
IAFE is an Institute devoted to the research in the areas of Astronomy, Solar Physics, Astrophysical Plasmas, Atomic Collisions and Relativistic Quantum Field Theories and Gravitation. Besides the Institute takes part in international interinstitutional instrumental projects. The objective of the Institute of Astronomy and Space Physics in Buenos-Aires, Argentina, is to constitute a multidisciplinary group of astronomers, physicists and engineers, whose work be centered on astrophysical problems not covered by other national institutions. Besides, through the requirements imposed by the non classical astronomical experiments, to carry on technological developements, mainly in the area of electronics, transferable to other sectors of the scientific-technological system of the country.
The Investigation Projects are: Astronomy, Solar Physics, Astrophysical Plasmas, Relativistic Quantum Field Theories and Gravitation, and Atomic Collisions.
http://www.iafe.uba.ar/
Instituto de Fisica de Cantabria (IFCA)
http://www.ifca.unican.es/
International Solar-Terrestrial Physics (ISTP)
The International Solar-Terrestrial Physics (ISTP) Science Initiative Home Page provides information on ISTP missions, campaigns, and activities.
http://www-istp.gsfc.nasa.gov/
Internet Pilot to Physics
Job announcements and deadlines - Conference deadlines - Physics News Flashes - Today in the history of physic - Physics Conference List - Announce a Conference - On-Line Discussion Forum - Market place for used equipment - Jobs on-line - Student Forum - Book Reviews and New Books.
http://physicsweb.org/TIPTOP/
Istituto di Fisica Cosmica e Applicazioni all'Informatica (IFCAI/CNR)
http://www.ifcai.pa.cnr.it/
Jicamarca Radio Observatory (Peru, radar, incoherent scatter)
Radar studies of the ionosphere and upper atmosphere.
http://dartagnan.ee.cornell.edu:8001/radar/jro/jicamarca.html
Kernfysisch Versneller Instituut (KVI)
http://kviexp.kvi.nl/
INACTIVE LINK ? - 23 --- Korean Physical Society (KPS)
http://www.kps.or.kr/welcomeeng.html
Kyiv Shevchenko University - Astronomy and Space physics department (Kiev, Ukraine)
Research interests: Host of annual Young Scientists Conference on Astronomy and Space Physics (YSC).
http://space.ups.kiev.ua/
Kyoto University - Department of Physics: Theoretical Astrophysics Group
Research on theoretical physics in the Universe at large from single star phenomena to whole universe, from quantum cosmology to present time astrophysical phenomena.
http://www-tap.scphys.kyoto-u.ac.jp/index-e.html
Laboratoire d'Annecy-le-vieux de Physique des Particules (LAPP)
http://wwwlapp.in2p3.fr/welcome-2-ag.html
Laboratoire de Gravitation et Cosmologie Relativistes (Paris)
Research area: Primordial Cosmology. General Relativity and its extensions. Gravitation and Interferometry. Atomic interferometry, atomic lasers. Relativistic Quantum Theories, Mathematical Physics. Relativistic Fluids and Astrophysics. Quasi-Cristalline and Amorphous Matter, Glass Theory. Foundations and History of Physical Theories.
http://www.gcr.jussieu.fr/eng_home.html
Laser Interferometer Space Antenna (LISA, Hannover Home Page)
http://www.lisa.uni-hannover.de/
Lawrence Berkeley Laboratory (LBL)
http://www.lbl.gov/
Lawrence Livermore National Laboratory (LLNL)
LLNL has developed world-class core competencies which are extending the frontiers of science and technology in many areas, including: defense systems science and technology, nuclear science and technology, high-performance computations, high-performance lasers, advanced sensors and instrumentation, energy science and technologies, environmental technologies, biology and biotechnology, including genomics, atmospheric science, large-scale science systems, precision manufacturing.
http://www.llnl.gov/
Lawrence Livermore National Laboratory - Physics Directorate (LLNL)
http://www-phys.llnl.gov/
Lecture Notes on General Relativity (University of Chicago)
http://ars-www.uchicago.edu/~carroll/notes/
Links to Relativistic Starflight (RFS)
This is a list of links to all known relativistic flight simulators. There are a variety of technologies in use.
http://ourworld.compuserve.com/homepages/anima/rfslink.htm
Los Alamos National Laboratory (LANL) - WWW
http://www.lanl.gov/external/welcome/
MIT Laboratory for Nuclear Science (LNS)
http://www-lns.mit.edu/
Max-Planck-Institut für Kernphysik
The Max-Planck-Institut für Kernphysik is located at Heidelberg, Germany. It was founded by Wolfgang Gentner as a research centre for nuclear physics in 1958. The present major research areas include nuclear and particle physics, space science, cosmic ray research and other topics.
http://www.mpi-hd.mpg.de/
Midcourse Space Experiment (MSX)
The MSX observatory is a Ballistic Missile Defense Organization project which offers major benefits for both the defense and civilian sectors. It was launched on a Delta II vehicle on April 24, 1996, into a 900 km, polar, near-Sun synchronous orbit. The spacecraft featured an advanced multispectral image capability to gather data on test targets and space background phenomena.
The infrared sensors operated at 11 to 12 degrees Kelvin by employing a solid hydrogen cryostat. The IR instruments span the range 4.2 - 26 microns. The focal plane array consists of five bands and the radiometer beam-size is more than 25 times smaller than IRAS. As a result, much greater spatial resolution than anything currently available has been obtained. The cryogen phase of the mission ended on 26 February 1997. During the ten month cryogen phase of the mission over 200 Giga Bytes of data on Celestial Backgrounds were obtained.
See the MSX Celestial Backgrounds Team Home Page for additional details.
http://scies.plh.af.mil:8600/
Nationaal Instituut voor Kernfysica en Hoge-Eenergie Fysica (NIKHEF)
http://www.nikhef.nl/
Nonproliferation and International Security (NIS/LANL)
The interests in astrophysics of the Astrophysics and Radiation Measurements Group (NIS-2) focus on gamma-ray bursts, x-ray binaries, accretion- and rotation-powered pulsars, neutron star dynamics, atomic processes in astrophysical sources, soft x-ray and EUV backgrounds, and EUV and soft x-ray transients such as flare stars.
An important mission of the group is to develop new types of optical, ultraviolet, x-ray and gamma-ray detectors for ground and space applications. The group has flown high-energy instruments on Pioneer Venus Orbiter, the ISEE-3 (ICE), P78-1, Vela satellites, and the Japanese satellite Ginga. The group is currently developing experiments for several scientific missions including the X-ray Multimirror Mission (XMM), High Energy Transient Explorer (HETE), MARS-96, and the MOXE all sky x-ray monitor on the Russian Spectrum X-Gamma satellite project, and is the lead institution operating the Array of Low Energy X-ray Imaging Sensors (ALEXIS) satellite and its wide field-of-view ultrasoft x-ray telescope array.
The group is actively participating in Compton Gamma Ray Observatory (CGRO) and Rossi X-ray Timing Explorer (RXTE) research through several guest investigator projects, and is also involved in establishing the growing-up Fenton Hill Observatory in the Jemez mountains, which includes an ultra-high-energy gamma-ray telescope, Milagro.
http://nis-www.lanl.gov/nis-projects/
Oak Ridge National Laboratory (ORNL)
http://www.phy.ornl.gov/
Ohio State University Astrophysics and Cosmology
People and Research in Astrophyiscs and Cosmology at Ohio State University.
http://www.physics.ohio-state.edu/~bbn/astro_theory.html
PhysicsEd
Collection of pointers to courses, multimedia documents, lesson plans, software, organizations, and other resources useful in the teaching/learning of Physics.
http://www-hpcc.astro.washington.edu/scied/physics.html
PhysicsWeb (The web site for physicists)
PhysicsWeb provides weekly news, patent news, webwatch, book reviews, jobs, events calendar, Physics World magazine and an extensive collection of physics related resources.
http://physicsweb.org/
Pierre Auger Project
The Auger Observatory is designed to detect and study cosmic rays around and above the GZK cutoff, i.e. at energies exceeding 1019 eV, with an unprecented quality and precision. Within our present knowledge, there is no standard explanation to the production and acceleration of any particle in the universe at such macroscopic energies. The Auger project is therefore the only answer the scientific community can propose to solve an astrophysical puzzle of more than 30 years.
http://www-lpnhep.in2p3.fr/auger/welcome.html
Radio Ice Cherenkov Experiment (RICE)
A prototype ultra-high energy neutrino detector/obervatory located at the South Pole. RICE consists of an array of radio antennas buried deep in the ice which detect coherent Cherenkov emission from electromagnetic cascades produced as a by product of ultra-high energy neutrino interactions.
http://kuhep4.phsx.ukans.edu/~iceman/
Raman Research Institute (RRI)
The Raman Research Institute has been active in the area of Astronomy/ Astrophysics research for over two decades. The observational programmes have focussed mainly on Radio Astronomy. The Institute has been involved in the construction and operation of several major radio telescopes. Scientists at the Institute observe with these telescopes, as well as many other facilities across the world.
http://www.rri.res.in/
Rome University Tor Vergata: Astrophysics (Tor Vergata astrophysics)
University of Rome " Tor Vergata" Physics Department, Astrophysics Group. Includes research activities and a guide to internet resources.
http://www.roma2.infn.it/astro/
Rutherford Appleton Laboratory (RAL)
http://www.rl.ac.uk/
Sandia National Laboratories
http://www.sandia.gov/
Space Plasma at RAL
http://sspg1.bnsc.rl.ac.uk/
Stanford Linear Accelerator Center (SLAC)
http://www-spires.slac.stanford.edu/highlighted.html
Stanford Public Information REtrieval System (SLAC-SPIRES)
A variety of SLAC's databases of interest to high-energy physics community is now made available via WWW, including: Preprints: HEP preprint database. Contains bibliographic summaries of more than 280,000 particle physics papers. Included are preprints, journal articles, technical reports, thesis, etc. Searchable by author, title, report number, institution, collaboration, and more. Find citations of your favorite author or article. View full postscript versions of selected preprints, read abstracts of bulletin-board papers. Need more help? Abstracts: Bulletin boards abstracts database. Useful in searching for recent physics bulletin board articles not yet covered by the HEP database. Find abstracts (and more!) of the articles posted today, yesterday, in the last seven days, week before that, or anytime.
http://www-spires.slac.stanford.edu/FIND/spires.html
University of California, Berkeley - Center for Particle Astrophysics (UCB - CfPA)
The CfPA located at the University of California, Berkeley was established in 1989 to conduct research in the new interdisciplinary field of particle astrophysics. We provide information on the Center's research, education and outreach efforts, workshops, seminars, publications, and a directory of members and visitors.
http://physics7.berkeley.edu/home.html
University of Cincinnati, Department of Physics (UC Physics)
The Department of Physics at the University of Cincinnati offers masters and Ph.D. degrees in Physics with an Astronomy Dissertation.
http://nimrod.phy.uc.edu/
University of Louisville - Moore Observatory
Moore Observatory is located in the Horner Wildlife Sanctuary near Louisville, KY. A computer-controlled 0.5 meter telescope, fiber optically coupled spectrograph, and wide field spectral imaging camera are used there to investigate physical processes in comets and low surface brightness emission nebulae. This resource describes the observatory and its environs, and provides a link to astrophysics research at the University of Louisville.
http://www.astro.louisville.edu/
University of Manchester. Department of Physics and Astronomy (UK)
Dept. of Physics & Astronomy including the astronomy group and NRAL.
http://www.ph.man.ac.uk/physics/
University of New Hampshire - Department of Physics
The Department of Physics at the University of New Hampshire has an extensive range of research including: space physics/astrophysics, nuclear physics, nonlinear dynamics and condensed matter.
http://www.physics.unh.edu/
University of Oklahoma - Physics and Astronomy Department
http://www.nhn.ou.edu/
University of Texas, Austin - Department of Physics
http://www.ph.utexas.edu/
Western Kentucky University - Physics and Astronomy Department
Home page for the astronomy group at Western Kentucky University and the Hardin Planetarium, in Bowling Green, Kentucky. The department is a collaborator in CASS: NASA University Research Center for Automated Space Science, along with Tennessee State University and South Carolina State University. Further links are provided for the Kentucky NASA EPSCoR program and the Kentucky Space Grant Consortium.
http://www.wku.edu/Dept/Academic/Ogden/Phyast/p0_.htm
Wilson Synchrotron Laboratory
http://w4.lns.cornell.edu/
Wright Nuclear Structure Laboratory (WNSL)
The astrophysics program centers on study of the nuclear reactions involved in the Stellar Hot CNO cycle.
http://wnsl.physics.yale.edu/
Wroclaw University, Institute of Theoretical Physics
http://www.ift.uni.wroc.pl/

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Please use the Astroweb submission form to request any addition or change to the Astroweb Database. This page was updated on: Tue 12 Oct 99