Significant progress has been made in recent years on the development of gravitational wave detectors. Sources such as coalescing compact binary systems, low-mass X-ray binaries, stellar collapses and pulsars are all possible candidates for detection. The most promising design of gravitational wave detector uses test masses a long distance apart and freely suspended as pendulums on Earth or in drag-free craft in space. The main theme of this review is a discussion of the mechanical and optical principles used in the various long baseline systems being built around the world -- LIGO (USA), VIRGO (Italy/France), TAMA 300 (Japan) and GEO 600 (Germany/UK) -- and in LISA, a proposed space-borne interferometer.
Keywords: gravitational waves, laser interferometry
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Since a Living Reviews in Relativity article may evolve over time, please cite the access <date>, which uniquely identifies the version of the article you are referring to:
Sheila Rowan and James Hough,
"Gravitational Wave Detection by Interferometry (Ground and Space)",
Living Rev. Relativity 3, (2000), 3. URL (cited on <date>):
http://www.livingreviews.org/lrr-2000-3
ORIGINAL | http://www.livingreviews.org/lrr-2000-3 |
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Title | Gravitational Wave Detection by Interferometry (Ground and Space) |
Author | Sheila Rowan / James Hough |
Date | accepted 24 January 2000, published 29 June 2000 |
UPDATE | http://www.livingreviews.org/lrr-2011-5 |
Title | Gravitational Wave Detection by Interferometry (Ground and Space) |
Author | Matthew Pitkin / Stuart Reid / Sheila Rowan / James Hough |
Date | accepted 17 June 2011, published 11 July 2011 |
Changes | For the update the author list has changed to be Matthew Pitkin, Stuart Reid, Sheila Rowan and Jim Hough. There have been minor updates to Sections 1, 2 and 3; major updates to Sections 4 and 5; Section 6 has been renamed and includes entirely new material on the operation of, and results from, the first generation of gravitational wave detectors and upgrades that are under way; and Section 7 also includes major updates about the status of LISA. The number of references has increased from 110 to 324. |