Current status of CLIO for detection of gravitational waves

T. Akutsu*, S. Miyoki, T. Uchiyama, K. Yamamoto, M. Ohashi, K. Kuroda, S. Kamagasako, N. Nakagawa, M. Tokunari, K. Kasahara, S. Telada, T. Tomaru, T. Suzuki, N. Sato, T. Shintomi, T. Haruyama, A. Yamamoto, D. Tatsumi, M. Ando, A. ArayaA. Takamori, S. Takemoto, H. Momose, H. Hayakawa, W. Morii, J. Akamatsu

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

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.

Original languageEnglish
Title of host publicationEnergy Budget in the High Energy Universe - Proceedings of the International Workshop
PublisherWorld Scientific Publishing Co. Pte Ltd
Pages377-381
Number of pages5
ISBN (Print)9812700102, 9789812700100
DOIs
StatePublished - 2007
EventInternational Workshop on Energy Budget in the High Energy Universe - Kashiwa, Japan
Duration: 2006/02/222006/02/24

Publication series

NameEnergy Budget in the High Energy Universe - Proceedings of the International Workshop

Conference

ConferenceInternational Workshop on Energy Budget in the High Energy Universe
Country/TerritoryJapan
CityKashiwa
Period2006/02/222006/02/24

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

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