Draft:Ground-based interferometric gravitational-wave detection
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Ground-based interferometric gravitational-wave detection refers to methods and devices used to detect gravitational waves based on interferometers built on the ground. Most of current gravitational wave observations have been made using these techniques; the first one was made in 2015 by the two LIGO detectors. The current major detectors are the two LIGO in the United States, Virgo in Italy and KAGRA in Japan, which are all part of the second generation of detectors; future projects include LIGO-India as part of the second generation, and the Einstein Telescope and Cosmic Explorer forming a third generation.
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Last edited by Thuiop (talk | contribs) 39 days ago. (Update) |