Japanese large-scale interferometers

被引:22
作者
Kuroda, K [1 ]
Ohashi, M
Miyoki, S
Ishizuka, H
Taylor, CT
Yamamoto, K
Miyakawa, O
Fujimoto, MK
Kawamura, S
Takahashi, R
Yamazaki, T
Arai, K
Tatsumi, D
Ueda, A
Fukushima, M
Sato, S
Shintomi, T
Yamamoto, A
Suzuki, T
Saito, Y
Haruyama, T
Sato, N
Higashi, Y
Uchiyama, T
Tomaru, T
Tsubono, K
Ando, M
Takamori, A
Numata, K
Ueda, KI
Yoneda, H
Nakagawa, K
Musha, M
Mio, N
Moriwaki, S
Somiya, K
Araya, A
Kanda, N
Telada, S
Sasaki, M
Tagoshi, H
Nakamura, T
Tanaka, T
Ohara, K
机构
[1] Univ Tokyo, Inst Cosm Ray Res, Kashiwa, Chiba 2778582, Japan
[2] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan
[3] High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan
[4] Univ Tokyo, Dept Phys, Tokyo 1130033, Japan
[5] Univ Electrocommun, Inst Laser Sci, Chofu, Tokyo 1828585, Japan
[6] Univ Tokyo, Dept Adv Mat Sci, Tokyo 1138656, Japan
[7] Univ Tokyo, Earthquake Res Inst, Tokyo 1130032, Japan
[8] Miyagi Univ Educ, Dept Phys, Sendai, Miyagi 9800485, Japan
[9] AIST, Natl Metrol Inst Japan, Tsukuba, Ibaraki 3058563, Japan
[10] Osaka Univ, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan
[11] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
[12] Niigata Univ, Fac Sci, Dept Phys, Niigata 9502102, Japan
关键词
D O I
10.1088/0264-9381/19/7/302
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 RD.
引用
收藏
页码:1237 / 1245
页数:9
相关论文
共 25 条
[1]   LIGO - THE LASER-INTERFEROMETER-GRAVITATIONAL-WAVE-OBSERVATORY [J].
ABRAMOVICI, A ;
ALTHOUSE, WE ;
DREVER, RWP ;
GURSEL, Y ;
KAWAMURA, S ;
RAAB, FJ ;
SHOEMAKER, D ;
SIEVERS, L ;
SPERO, RE ;
THORNE, KS ;
VOGT, RE ;
WEISS, R ;
WHITCOMB, SE ;
ZUCKER, ME .
SCIENCE, 1992, 256 (5055) :325-333
[2]   Current status of TAMA [J].
Ando, M .
CLASSICAL AND QUANTUM GRAVITY, 2002, 19 (07) :1409-1419
[3]   New signal extraction scheme with harmonic demodulation for power-recycled Fabry-Perot-Michelson interferometers [J].
Arai, K ;
Ando, M ;
Moriwaki, S ;
Kawabe, K ;
Tsubono, K .
PHYSICS LETTERS A, 2000, 273 (1-2) :15-24
[4]  
BRILLET A, 1998, P 2 AM C, P87
[5]  
DANZMANN K, 1994, M PLANK I QUANTENOPT, P190
[6]  
KURODA, 1997, P INT GRAV WAV SOURC, P100
[7]   Large-scale cryogenic gravitational wave telescope [J].
Kuroda, K ;
Ohashi, M ;
Miyoki, S ;
Tatsumi, D ;
Sato, S ;
Ishizuka, H ;
Fujimoto, MK ;
Kawamura, S ;
Takahashi, R ;
Yamazaki, T ;
Arai, K ;
Fukushima, M ;
Waseda, K ;
Telada, S ;
Ueda, A ;
Shintomi, T ;
Yamamoto, A ;
Suzuki, T ;
Saito, Y ;
Haruyama, T ;
Sato, N ;
Tsubono, K ;
Kawabe, K ;
Ando, M ;
Ueda, KI ;
Yoneda, H ;
Musha, M ;
Mio, N ;
Moriwaki, S ;
Araya, A ;
Kanda, N ;
Tobar, ME .
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 1999, 8 (05) :557-579
[8]  
MIO N, 2002, P 4 E AM C GRAV WAV, V19, P1647
[9]  
MIYAKAWA O, 2002, P 4 E AM C GRAV WAV, V19, P1555
[10]   Cryogenic contamination of an ultra-low loss mirror for cryogenic laser interferometric gravitational wave detector [J].
Miyoki, S ;
Uchiyama, T ;
Tomaru, T ;
Tatsumi, D ;
Ishizuka, H ;
Ohashi, M ;
Kuroda, K ;
Ueda, A ;
Suzuki, T ;
Sato, N ;
Haruyama, T ;
Yamamoto, A ;
Shintomi, T .
CRYOGENICS, 2000, 40 (01) :61-66