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   Home / Science / Astronomy / Observatories / Gravitational Waves
 
   See Also
   Web Sites
  • AURIGA - Ultracryogenic gravitational wave detector experiment at Legnaro National Laboratories, Italy.
    axln01.lnl.infn.it
  • Australian Consortium for Interferometric Gravitational Astronomy - ACIGA is intended to undertake research and development aimed at improving the performance of present laser interferometer gravitational wave detectors through advanced designs to ultimate limits set by mechanics, quantum mechanics, lasers and optics; and to transfer this into practical designs that can be used in production of commercial products.
    www.anu.edu.au/Physics/ACIGA
  • Australian International Gravitational Research Center - Gravity wave group at University of Western Australia.
    www.gravity.uwa.edu.au
  • Chilling Mirrors with Light - Applied to gravitational wave detectors.
    www.aip.org/enews/physnews/1999/split/pnu450-1.htm
  • GEO 600 - A UK-German project aiming at the direct detection of gravitational waves by means of a laser interferometer of 600 m armlength.
    www.geo600.uni-hannover.de
  • Gravity Wave Analysis From LIGO Prototype - Physics News Update.
    www.aip.org/enews/physnews/1999/split/pnu442-1.htm
  • ICRR Group - Gravitational wave group in Japan.
    www.icrr.u-tokyo.ac.jp/gr/gr.html
  • Laser Interferometer Gravitational-Wave Observatory (LIGO) - U.S. facility dedicated to the detection of cosmic gravitational waves and the harnessing of these waves for scientific research.
    www.ligo.caltech.edu
  • Laser Interferometer Gravitational-Wave Observatory (LIGO) - Livingston Observatory.
    www.ligo-la.caltech.edu
  • Laser Interferometer Gravitational-Wave Observatory (LIGO) - Hanford Observatory.
    www.ligo-wa.caltech.edu
  • Laser Interferometer Space Antenna (LISA) - An ESA space mission to detect and observe gravitational waves from massive black holes and galactic binary stars in the frequency range 10-4 to 10-1 hz. Useful measurements in this frequency range cannot be made on the ground because of the unshieldable background of local gravitational noise.
    www.estec.esa.nl/spdwww/future/html/lisa.htm
  • Laser Interferometer Space Antenna -- LISA - Universität Hannover site. Includes information about the project as well as the text of reports based on it.
    www.lisa.uni-hannover.de
  • Laser Interferometer Space Antenna -- LISA - NASA site. Project that will attempt to detect gravitational waves. General and technical information.
    lisa.jpl.nasa.gov
  • Listen to the Universe - Simulated sounds of gravitational waves created by spiraling binary systems.
    www.people.cornell.edu/pages/sd68/ligo/inspiral.html
  • Ripples in Curvature - Transparencies of a talk by Patrick Brady, included are sound files of compact coalescing binaries.
    www.lsc-group.phys.uwm.edu/~patrick/work/talks/itp.html
  • Rome Group - Rome Gravitational Wave Experiment.
    www.roma1.infn.it/rog/rogmain.html
  • TAMA - A five-year (1995-2000) project involving almost all gravity physics researchers in Japan. It adopts a Fabry-Perot Michelson Interferometer (FPMI) with recycling. The aim of this project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur by chance within our local group of galaxies.
    tamago.mtk.nao.ac.jp
  • The Virgo Project - Collaboration between Italian and French research teams for the realization of an interferometric gravitational wave detector.
    www.virgo.infn.it
  • Tsubono Group - 300-m arm-length Fabry-Perot laser interferometer.
    t-munu.phys.s.u-tokyo.ac.jp/welcome_e.html
  • Washington University Gravity Group - WUGRAV, contains large collection of gravity links.
    wugrav.wustl.edu
  • WUGRAV Movies - Computer simulated movies of colliding neutron stars, gravitational waves propagation; click on top image for newest movies.
    wugrav.wustl.edu/Movies

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