抄録
In the LCGT and CLIO projects for the interferometric gravitational wave detectors of Japan, the mirrors and a part of the suspension systems are cooled by cryocoolers to reduce the thermal noise. For the CLIO, extremely small vibration cryocoolers were specially developed by improving a commercial Gifford-McMahon type pulse tube cryocooler. We measured the vibration at the top of the suspension base in the CLIO interferometer while operating these cryocoolers. Although the seismic motion of 10-9(1 Hz/f)2 m/Hz1/2 at the site of the CLIO and LCGT in the Kamioka mine is 100-times smaller than that around Tokyo, these cryocoolers did not seriously increase the vibration. Consequently, a reduction of thermal noise by the cooled mirrors and suspension fibers using these cryocoolers is expected to be observed without any additional fluctuation disturbance due to the cryocoolers.
本文言語 | 英語 |
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ページ(範囲) | 418-423 |
ページ数 | 6 |
ジャーナル | Journal of Physics: Conference Series |
巻 | 32 |
号 | 1 |
DOI | |
出版ステータス | 出版済み - 2006/03/02 |
ASJC Scopus 主題領域
- 物理学および天文学一般