Development of a light source with an injection-locked Nd:YAG laser and a ring-mode cleaner for the TAMA 300 gravitational-wave detector

被引：11

作者：

Nagano, S

Barton, MA

Ishizuka, H

Kuroda, K

Matsumura, S

Miyakawa, O

Miyoki, S

Tatsumi, D

Tomaru, T

Uchiyama, T

Ando, M

Arai, K

Kawabe, K

Ohishi, N

Takamori, A

Taniguchi, S

Tochikubo, K

Tsubono, K

Yamamoto, K

Fujimoto, MK

Fukushima, M

Kawamura, S

Kozai, Y

Miyama, S

Ohashi, M

Sato, S

Takahashi, R

Telada, S

Yamazaki, T

Mio, N

Moriwaki, S

Horikoshi, G

Kamikubota, N

Ogawa, Y

Saito, Y

Suzuki, T

Musha, M

Nakagawa, K

Ueda, A

Ueda, K

Araya, A

Kanda, N

Nakamura, T

Tanaka, T

Sasaki, M

Tagoshi, H

Futamase, T

Kawashima, N

Mizuno, E

Kojima, Y

机构：

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

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

[3] Natl Astron Observ, Tokyo 1818588, Japan

[4] Univ Tokyo, Dept Adv Mat Sci, Bunkyo Ku, Tokyo 1130033, Japan

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

[6] Univ Electrocommun, Inst Laser Sci, Chofu, Tokyo 1828585, Japan

[7] Univ Tokyo, Earthquake Res Inst, Tokyo 1130032, Japan

[8] Miyagi Univ Educ, Dept Phys, Sendai, Miyagi 9800845, Japan

[9] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan

[10] Osaka Univ, Dept Earth & Space Sci, Osaka 5600043, Japan

[11] Tohoku Univ, Inst Astron, Sendai, Miyagi 9808578, Japan

[12] Kinki Univ, Dept Phys, Osaka 5778502, Japan

[13] Inst Space & Astronaut Sci, Kanagawa 2290022, Japan

[14] Hiroshima Univ, Dept Phys, Hiroshima 7398526, Japan

[15] Tokyo Denki Univ, Chiyoda Ku, Tokyo 1018457, Japan

[16] Niigata Univ, Dept Phys, Niigata 9502102, Japan

[17] Tokai Univ, Div Precis Engn, Kanagawa 2591292, Japan

来源：

REVIEW OF SCIENTIFIC INSTRUMENTS | 2002年 / 73卷 / 05期

关键词：

D O I：

10.1063/1.1470230

中图分类号：

TH7 [仪器、仪表];

学科分类号：

0804 ; 080401 ; 081102 ;

摘要：

We have developed a light source suitable for laser interferometric gravitational-wave detectors. The developed light source has high power, TEM00 mode, linear polarization, high frequency stability, and low intensity noise. The light source with the quality is essential for attaining the goal sensitivity in the TAMA 300 and was found to be available for a observation run of a gravitational-wave detector. (C) 2002 American Institute of Physics.

引用

页码：2136 / 2142

页数：7

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