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arXiv 2006.16772physics.ins-det
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低温干涉型引力波探测器分子层光损耗研究

The optical loss study of molecular layer for a cryogenic interferometric gravitational-wave detector

Satoshi Tanioka, Kunihiko Hasegawa, Yoichi Aso

摘要:

引力波的探测使我们对宇宙有了深刻的了解。为了增加可探测的引力波源的数量,未来的几个引力波探测器将使用低温反射镜。然而,最近的研究表明,真空室内的残余气体分子粘附在低温镜面上,并形成随时间增长的分子层。不断生长的分子层在反射镜中引入了额外的光学损耗,这会降低检测器的性能。本文从理论上估算了低温运行的引力波探测器中分子层的光损耗。根据光损耗的估算结果,讨论了低温引力波探测器的性能。

英文摘要:

The detection of gravitational-waves provides us with a deep insight into the universe. In order to increase the number of detectable gravitational-wave sources, several future gravitational-wave detectors will operate with cryogenic mirrors. Recent studies, however, showed residual gas molecules inside the vacuum chamber adhere to the cryogenic mirror surface and form a molecular layer which grows with time. The growing molecular layer introduces an additional optical loss in the mirror which can decrease the detector's performance. We theoretically estimate the optical loss by the molecular layer in a cryogenically operated gravitational-wave detector. The impacts on a cryogenic gravitational-wave detector is discussed based on the results of optical loss estimation.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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