Status of Japanese gravitational wave detectors
Status of Japanese gravitational wave detectors
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DOI：
10.1088/0264-9381/26/20/204020
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发表时间：
2009-10
影响因子：
3.5
通讯作者：
K. Arai;R. Takahashi;D. Tatsumi;K. Izumi;Yaka Wakabayashi;H. Ishizaki;M. Fukushima;T. Yamazaki;M. Fujimoto;A. Takamori;K. Tsubono;R. DeSalvo;A. Bertolini;S. Márka;V. Sannibale;T. Uchiyama;O. Miyakawa;S. Miyoki;K. Agatsuma;T. Saito;M. Ohashi;K. Kuroda;I. Nakatani;S. Telada;Kazuhiro Yamamoto;T. Tomaru;Toshikazu Suzuki;T. Haruyama;N. Sato;A. Yamamoto;T. Shintomi
中科院分区：
文献类型：
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作者：
K. Arai;R. Takahashi;D. Tatsumi;K. Izumi;Yaka Wakabayashi;H. Ishizaki;M. Fukushima;T. Yamazaki;M. Fujimoto;A. Takamori;K. Tsubono;R. DeSalvo;A. Bertolini;S. Márka;V. Sannibale;T. Uchiyama;O. Miyakawa;S. Miyoki;K. Agatsuma;T. Saito;M. Ohashi;K. Kuroda;I. Nakatani;S. Telada;Kazuhiro Yamamoto;T. Tomaru;Toshikazu Suzuki;T. Haruyama;N. Sato;A. Yamamoto;T. Shintomi
大型低温引力波望远镜（LCGT）计划作为日本未来引力波探测项目。神冈的一个地下矿井将建造一个 3 公里长的干涉仪。测试质量将采用低温蓝宝石镜面。为了演示 LCGT 技术，正在开发两种原型干涉仪 TAMA300 和 CLIO。本文介绍了 LCGT 项目和两个原型干涉仪的现状。
The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at Kamioka. Cryogenic sapphire mirrors are going to be employed for the test masses. For the demonstration of LCGT technologies, two prototype interferometers, TAMA300 and CLIO, are being developed. This paper describes the current status of the LCGT project and the two prototype interferometers.