Current Status of CLIO for the Detection of Gravitational Waves

Details Current Status of CLIO for the Detection of Gravitational Waves Current Status of CLIO for the Detection of Gravitational Waves

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ebhe.conf..377a&link_type=abstract

ENERGY BUDGET IN THE HIGH ENERGY UNIVERSE . Proceedings of the International Workshop. Held 22-24 February 2006 in Kashiwa, Japa

Physics

Scientific paper

The CLIO is a 100 m baseline cryogenic laser interferometer for the detection of the gravitational waves, which is under construction in Kamioka mine, Japan. This is for the investigation the technical feasibility for the Large-scale Cryogenic Gravitational wave Telescope (LCGT), which is planned to be constructed in the same Kamioka mine with 30 times longer baseline than the CLIO. We successfully operated CLIO, whose three mirrors were cooled around 20K, as a gravitational wave detector using a locked Fabry-Perot control scheme.

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