Vacuum-compatible vibration isolation stack for an interferometric gravitational wave detector TAMA300

被引:23
|
作者
Takahashi, R [1 ]
Kuwahara, F
Majorana, E
Barton, MA
Uchiyama, T
Kuroda, K
Araya, A
Arai, K
Takamori, A
Ando, M
Tsubono, K
Fukushima, M
Saito, Y
机构
[1] Natl Astron Observ, Tokyo 1818588, Japan
[2] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan
[3] KEK High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan
[4] Univ Tokyo, Earthquake Res Inst, Bunkyo Ku, Tokyo 1130032, Japan
[5] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
来源
REVIEW OF SCIENTIFIC INSTRUMENTS | 2002年 / 73卷 / 06期
关键词
D O I
10.1063/1.1473225
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
Interferometric gravitational wave detectors require a large degree of vibration isolation. For this purpose, a multilayer stack constructed of rubber and metal blocks is suitable, because it provides isolation in all degrees of freedom at once. In TAMA300, a 300 m interferometer in Japan, long-term dimensional stability and compatibility with an ultrahigh vacuum environment of about 10(-6) Pa are also required. To keep the interferometer at its operating point despite ground strain and thermal drift of the isolation system, a thermal actuator was introduced. To prevent the high outgassing rate of the rubber from spoiling the vacuum, the rubber blocks were enclosed by gas-tight bellows. Using these techniques, we have successfully developed a three-layer stack which has a vibration isolation ratio of more than 10(3) at 300 Hz with control of drift and enough vacuum compatibility. (C) 2002 American Institute of Physics.
引用
收藏
页码:2428 / 2433
页数:6
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