LARGE-SCALE CRYOGENIC GRAVITATIONAL WAVE TELESCOPE
LARGE-SCALE CRYOGENIC GRAVITATIONAL WAVE TELESCOPE
复制标题
大型低温引力波望远镜
DOI：
10.1142/s0218271899000390
复制
发表时间：
1999
影响因子：
2.2
通讯作者：
Michael E. Tobar
中科院分区：
文献类型：
--
作者：
K. Kuroda;M. Ohashi;S. Miyoki;D. Tatsumi;S. Sato;H. Ishizuka;M. Fujimoto;S. Kawamura;R. Takahashi;T. Yamazaki;K. Arai;M. Fukushima;K. Waseda;S. Telada;A. Ueda;T. Shintomi;A. Yamamoto;Toshikazu Suzuki;Yoshio Saito;T. Haruyama;N. Sato;K. Tsubono;K. Kawabe;M. Ando;K. Ueda;H. Yoneda;M. Musha;N. Mio;S. Moriwaki;A. Araya;N. Kanda;Michael E. Tobar
我们在这里介绍了大型低温引力波望远镜（LCGT）项目，该项目旨在将现有引力波项目的灵敏度提高十倍。LCGT是继TAMA计划之后在日本建造千米级引力波探测器的计划，它采用了带有更高功率激光器的低温反射镜。我们计划在神冈矿的地下建造它。如果它的目标灵敏度达到，我们将能够捕捉到每月几个事件。
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.