Progress in gravitational wave detection

Details Progress in gravitational wave detection Progress in gravitational wave detection

Sep 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pabei..23..195c&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 23, No. 3, p. 195 - 204 (2005)

Astronomy and Astrophysics

Astrophysics

Astrophysics, Gravitational Wave, Review, Gravitational Wave Telescope

Scientific paper

General theory of Einstein's relativity predicts the existence of gravitational wave when mass is accelerated. However, no material has direct effect when the gravitational wave passes. Therefore, gravitational wave can only be detected indirectly. The effort in gravitational wave detection was started in the 60s of last century by using a huge cylinder of aluminum. This paper introduced all the relevant projects in the gravitational wave detection. These projects include Weber's bar, Laser interferometer Gravitational wave Detector (LGD), Laser Interferometer Gravitational wave Observatory (LIGO), GEO600, VIRGO, TAMA300, Advanced LIGO, Large scale Cryogenic Gravitational wave Telescope (LCGO), and Laser Interferometer Space Antenna (LISA).

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