Large-scale cryogenic gravitational wave telescope

Kazuaki Kuroda*, Masatake Ohashi, Shinji Miyoki, Daisuke Tatsumi, Shuichi Sato, Hideki Ishizuka, Masa Katsu Fujimoto, Seiji Kawamura, Ryutaro Takahashi, Toshitaka Yamazaki, Koji Arai, Mitsuhiro Fukushima, Koichi Waseda, Souichi Telada, Akitoshi Ueda, Takakazu Shintomi, Akira Yamamoto, Toshikazu Suzuki, Yoshio Saito, Tomiyoshi HaruyamaNobuaki Sato, Kimio Tsubono, Keita Kawabe, Masaki Ando, Ken Ichi Ueda, Hitoki Yoneda, Mitsuru Musha, Norikatsu Mio, Shigenori Moriwaki, Akito Araya, Nobuyuki Kanda, Mike E. Tobar

*この研究の対応する著者

研究成果: Article査読

117 被引用数 (Scopus)

抄録

We present here the Large-scale Cryogenic Gravitational wave Telescope (LCGT) project which is aimed to improve the sensitivity of the existing gravitational wave projects by ten times. LCGT is the project constructing the km-scale gravitational wave detector in Japan succeeding the TAMA project, which adopts cryogenic mirrors with a higher power laser. We are planing to build it in an underground site in Kamioka mine. If its target sensitivity is attained, we will be able to catch a few events per month.

本文言語English
ページ(範囲)557-579
ページ数23
ジャーナルInternational Journal of Modern Physics D
8
5
出版ステータスPublished - 1999 10月
外部発表はい

ASJC Scopus subject areas

  • 数理物理学
  • 天文学と天体物理学
  • 宇宙惑星科学

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