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arXiv · 0912.0107

Mirror thermal noise in laser interferometer gravitational wave detectors operating at room and cryogenic temperature

Janyce Franc·Nazario Morgado·Raffaele Flaminio·Ronny Nawrodt·Iain Martin·Liam Cunningham·Alan Cumming·Sheila Rowan·James Hough
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Abstract

Mirror thermal noise is and will remain one of the main limitations to the sensitivity of gravitational wave detectors based on laser interferometers. We report about projected mirror thermal noise due to losses in the mirror coatings and substrates. The evaluation includes all kind of thermal noises presently known. Several of the envisaged substrate and coating materials are considered. The results for mirrors operated at room temperature and at cryogenic temperature are reported.

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Janyce Franc, Nazario Morgado, Raffaele Flaminio, Ronny Nawrodt, Iain Martin, Liam Cunningham, Alan Cumming, Sheila Rowan, James Hough. 2009-12-01. Mirror thermal noise in laser interferometer gravitational wave detectors operating at room and cryogenic temperature. https://arxiv.org/abs/0912.0107

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