Direct measurement of the scattered light effect on the sensitivity in TAMA300

被引：9

作者：

Takahashi, R ^{[1
]}

Arai, K

Kawamura, S

Smith, MR

机构：

[1] Natl Astron Observ, Tokyo 1818588, Japan

[2] CALTECH, Pasadena, CA 91125 USA

来源：

PHYSICAL REVIEW D | 2004年 / 70卷 / 06期

关键词：

D O I：

10.1103/PhysRevD.70.062003

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Laser interferometer gravitational wave detectors need vacuum tubes through which the laser beams pass. The light scattered from the arm cavity mirrors will make multiple reflections from the inside wall of the polished tube back onto the mirrors causing phase noise on the interferometer output beam. The TAMA300 has two 300 m length arms enclosed by vacuum tubes. By vibrating one of the tubes of the TAMA300, we directly observed the effect of the scattered light on the displacement sensitivity. It was found that a tube vibration amplitude of 5.6 mum at 776.5 Hz increased the mirror displacement noise by 1.2x10(-17) m. This noise level is consistent with the calculated noise due to the scattered light effect.

引用

页码：062003 / 1

页数：4

共 8 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] 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

[3] 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

[4] 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

[5] Vacuum system design for the 300m gravitational wave laser interferometer in Japan (TAMA300) [J].

Saito, Y ;

Matuda, N ;

Ogawa, Y ;

Horikoshi, G .

VACUUM, 1996, 47 (6-8) :609-611

[6] Application of diamond-like Carbon (DLC) coatings for gravitational wave detectors [J].

Takahashi, R ;

Saito, Y ;

Sato, Y ;

Kubo, T ;

Tomaru, T ;

Tokunari, M ;

Sumiya, T ;

Takasugi, K ;

Naito, Y .

VACUUM, 2004, 73 (02) :145-148

[7] Present status of large-scale cryogenic gravitational wave telescope [J].

Uchiyama, T ;

Kuroda, K ;

Ohashi, M ;

Miyoki, S ;

Ishitsuka, H ;

Yamamoto, K ;

Hayakawa, H ;

Kasahara, K ;

Fujimoto, MK ;

Kawamura, S ;

Takahashi, R ;

Yamazaki, T ;

Arai, K ;

Tatsumi, D ;

Ueda, A ;

Fukushima, M ;

Sato, 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 ;

Numata, K ;

Aso, Y ;

Ueda, KI ;

Yoneda, H ;

Nakagawa, K ;

Musha, M ;

Mio, N ;

Moriwaki, S ;

Somiya, K ;

Araya, A ;

Takamori, A ;

Kanda, N ;

Telada, S ;

Tagoshi, H ;

Nakamura, T ;

Sasaki, M ;

Tanaka, T ;

Ohara, KI ;

Takahashi, H ;

Nagano, S ;

Miyakawa, O .

CLASSICAL AND QUANTUM GRAVITY, 2004, 21 (05) :S1161-S1172

[8] Scattered light noise in gravitational wave interferometric detectors: Coherent effects [J].

Vinet, JY ;

Brisson, V ;

Braccini, S .

PHYSICAL REVIEW D, 1996, 54 (02) :1276-1286

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