Japanese large-scale interferometers

K. Kuroda, M. Ohashi, S. Miyoki, H. Ishizuka, C. T. Taylor, K. Yamamoto, O. Miyakawa, M. K. Fujimoto, S. Kawamura, R. Takahashi, T. Yamazaki, K. Arai, D. Tatsumi, A. Ueda, Mitsuhiro Fukushima, S. Sato, T. Shintomi, A. Yamamoto, T. Suzuki, Y. SaitoT. Haruyama, N. Sato, Y. Higashi, T. Uchiyama, T. Tomaru, K. Tsubono, M. Ando, A. Takamori, K. Numata, K. I. Ueda, H. Yoneda, K. Nakagawa, M. Musha, N. Mio, S. Moriwaki, K. Somiya, A. Araya, N. Kanda, S. Telada, M. Sasaki, H. Tagoshi, T. Nakamura, T. Tanaka, K. Ohara

研究成果: Article査読

27 被引用数 (Scopus)

抄録

The objective of the TAMA 300 interferometer was to develop advanced technologies for kilometre scale interferometers and to observe gravitational wave events in nearby galaxies. It was designed as a power-recycled Fabry-Perot-Michelson interferometer and was intended as a step towards a final interferometer in Japan. The present successful status of TAMA is presented. TAMA forms a basis for LCGT (large-scale cryogenic gravitational wave telescope), a 3 km scale cryogenic interferometer to be built in the Kamioka mine in Japan, implementing cryogenic mirror techniques. The plan of LCGT is schematically described along with its associated R&D.

本文言語English
ページ(範囲)1237-1245
ページ数9
ジャーナルClassical and Quantum Gravity
19
7
DOI
出版ステータスPublished - 2002 4 7
外部発表はい

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

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