CLIO Cryogenic Laser Interferometer Observatory

Details CLIO Cryogenic Laser Interferometer Observatory CLIO Cryogenic Laser Interferometer Observatory

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.3073m&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

Cryogenic Laser Interferometer Observatory (CLIO) is now constructed to demonstrate two of three features of Large-scale Cryogenic Gravitational wave telescope (LCGT), that are to utilize low seismic and stable environment in the Kamioka mine and sapphire mirrors at low temperature for thermal noise reduction. CLIO has a locked Fabry-Perot configuration equipp ed with ring mode cleaners for laser frequency stabilization and the cryogenic vacuum and cooling system using refrigerators to cool the sapphire mirrors at 20 K. The noise level of CLIO is designed to sync√ onize with the thermal noise √ sapphire mirrors which hr of -19 -20 varies from 3 × 10 m/ Hz at 300 K to 2 × 10 m/ Hz at 20 K around 100 Hz.

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