The status of LCGT

被引:66
作者
Kuroda, K [1 ]
机构
[1] Univ Tokyo, ICRR, Kashiwa, Chiba 2778582, Japan
关键词
D O I
10.1088/0264-9381/23/8/S27
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The current status of LCGT is described. The physical target of LCGT is to detect every year at least one event of gravitational wave signal produced at the coalescence of a binary neutron star. To attain this objective, LCGT is built underground by adopting cryogenic mirrors with a high power laser. To assure the reliable detection, two independent sets of interferometers are installed in a common vacuum system.
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页码:S215 / S221
页数:7
相关论文
共 17 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]  
ADHIKARI R, 2005, 4 TAMA S OS JAP
[3]   Stable operation of a 300-m laser interferometer with sufficient sensitivity to detect gravitational-wave events within our galaxy [J].
Ando, M ;
Arai, K ;
Takahashi, R ;
Heinzel, G ;
Kawamura, S ;
Tatsumi, D ;
Kanda, N ;
Tagoshi, H ;
Araya, A ;
Asada, H ;
Aso, Y ;
Barton, MA ;
Fujimoto, MK ;
Fukushima, M ;
Futamase, T ;
Hayama, K ;
Horikoshi, G ;
Ishizuka, H ;
Kamikubota, N ;
Kawabe, K ;
Kawashima, N ;
Kobayashi, Y ;
Kojima, Y ;
Kondo, K ;
Kozai, Y ;
Kuroda, K ;
Matsuda, N ;
Mio, N ;
Miura, K ;
Miyakawa, O ;
Miyama, SM ;
Miyoki, S ;
Moriwaki, S ;
Musha, M ;
Nagano, S ;
Nakagawa, K ;
Nakamura, T ;
Nakao, K ;
Numata, K ;
Ogawa, Y ;
Ohashi, M ;
Ohishi, N ;
Okutomi, S ;
Oohara, K ;
Otsuka, S ;
Saito, Y ;
Sasaki, M ;
Sato, S ;
Sekiya, A ;
Shibata, M .
PHYSICAL REVIEW LETTERS, 2001, 86 (18) :3950-3954
[4]  
ASO Y, 2002, THESIS U TOKYO
[5]   Seismic isolation by mechanical filters at very low frequencies [J].
Bougleux, E ;
Braccini, S ;
Bradaschia, C ;
Casciano, C ;
Cella, G ;
Dattilo, V ;
DeSalvo, R ;
Di Virgilio, A ;
Feng, GT ;
Fidecaro, F ;
Frasconi, F ;
Gaddi, A ;
Giazotto, A ;
Holloway, L ;
La Penna, P ;
Losurdo, G ;
Malik, S ;
Palla, F ;
Passaquieti, R ;
Raffaelli, F ;
Stanga, R ;
Valentini, R ;
Vicere, A .
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 1998, 409 (1-3) :480-483
[6]  
DANZMANN K, 1994, M PLANK I QUANTENOPT, P190
[7]   The cosmic coalescence rates for double neutron star binaries (vol 601, pg L179, 2004) [J].
Kalogera, V ;
Kim, C ;
Lorimer, DR ;
Burgay, M ;
D'Amico, N ;
Possenti, A ;
Manchester, RN ;
Lyne, AG ;
Joshi, BC ;
McLaughlin, MA ;
Kramer, M ;
Sarkissian, JM ;
Camilo, F .
ASTROPHYSICAL JOURNAL, 2004, 614 (02) :L137-L138
[8]  
KANDA N, 2004, LCGT COLL M
[9]   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
[10]   Current status of large-scale cryogenic gravitational wave telescope [J].
Kuroda, K ;
Ohashi, M ;
Miyoki, S ;
Uchiyama, T ;
Ishitsuka, H ;
Yamamoto, K ;
Kasahara, K ;
Fujimoto, MK ;
Kawamura, S ;
Takahashi, R ;
Yamazaki, T ;
Arai, K ;
Tatsmui, D ;
Ueda, A ;
Fukushima, M ;
Sato, S ;
Nagano, S ;
Tsunesada, Y ;
Zhu, ZH ;
Shintomi, T ;
Yamamoto, A ;
Suzuki, T ;
Saito, Y ;
Haruyama, T ;
Sato, N ;
Higashi, Y ;
Tomaru, T ;
Tsubono, K ;
Ando, M ;
Takamori, A ;
Numata, K ;
Aso, Y ;
Ueda, KI ;
Yoneda, H ;
Nakagawa, K ;
Musha, M ;
Mio, N ;
Moriwaki, S ;
Somiya, K ;
Araya, A ;
Kanda, N ;
Telada, S ;
Tagoshi, H ;
Nakamura, T ;
Sasaki, M ;
Tanaka, T ;
Oohara, K ;
Takahashi, H ;
Miyakawa, O ;
Tobar, ME .
CLASSICAL AND QUANTUM GRAVITY, 2003, 20 (17) :S871-S884