Status of Japanese gravitational wave detectors

被引：25

作者：

Arai, K. ^{[1
]}

Takahashi, R. ^{[1
]}

Tatsumi, D. ^{[1
]}

Izumi, K. ^{[2
]}

Wakabayashi, Y. ^{[10
]}

Ishizaki, H. ^{[1
]}

Fukushima, M. ^{[1
]}

Yamazaki, T. ^{[1
]}

Fujimoto, M-K ^{[1
]}

Takamori, A. ^{[9
]}

Tsubono, K. ^{[8
]}

DeSalvo, R. ^{[7
]}

Bertolini, A. ^{[5
]}

Marka, S. ^{[6
]}

Sannibale, V. ^{[7
]}

Uchiyama, T. ^{[3
]}

Miyakawa, O. ^{[3
]}

Miyoki, S. ^{[3
]}

Agatsuma, K. ^{[3
]}

Saito, T. ^{[3
]}

Ohashi, M. ^{[3
]}

Kuroda, K. ^{[3
]}

Nakatani, I. ^{[3
]}

Telada, S. ^{[11
]}

Yamamoto, K. ^{[5
]}

Tomaru, T. ^{[4
]}

Suzuki, T. ^{[4
]}

Haruyama, T. ^{[4
]}

Sato, N. ^{[4
]}

Yamamoto, A. ^{[4
]}

Shintomi, T. ^{[12
]}

机构：

[1] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[2] Univ Tokyo, Dept Astron, Bunkyo Ku, Tokyo 1130033, Japan

[3] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan

[4] High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan

[5] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-30167 Hannover, Germany

[6] Columbia Univ, New York, NY 10027 USA

[7] CALTECH, Pasadena, CA 91125 USA

[8] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

[9] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan

[10] Ochanomizu Univ, Grad Sch Humanities & Sci, Bunkyo Ku, Tokyo 1128610, Japan

[11] Natl Inst Adv Ind Sci & Technol, Tsukuba, Ibaraki 3058563, Japan

[12] Nihon Univ, Adv Res Inst Sci & Humanities, Chiyoda Ku, Tokyo 1020073, Japan

来源：

CLASSICAL AND QUANTUM GRAVITY | 2009年 / 26卷 / 20期

基金：

日本学术振兴会; 美国国家科学基金会;

关键词：

FREQUENCY STABILIZATION; AUTOMATIC ALIGNMENT; LASER; INTERFEROMETER; SYSTEM; EXTRACTION;

D O I：

10.1088/0264-9381/26/20/204020

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页数：9

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