Publication Date:
2014-08-08
Description:
Author(s): D. Heinert, K. Craig, H. Grote, S. Hild, H. Lück, R. Nawrodt, D. A. Simakov, D. V. Vasilyev, S. P. Vyatchanin, and H. Wittel Current gravitational-wave detectors rely on the use of Michelson interferometers. One crucial limitation of their sensitivity is the thermal noise of their optical components. Thus, for example, fluctuational deformations of the mirror surface are probed by a laser beam being reflected from the mir... [Phys. Rev. D 90, 042001] Published Thu Aug 07, 2014
Keywords:
Gravitational Experiment
Print ISSN:
0556-2821
Electronic ISSN:
1089-4918
Topics:
Physics
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