Heinert, D.; Craig, K.; Grote, H.; Hild, S.; Lück, H.; Nawrodt, R.; Simakov, D.A.; Vasilyev, D.V.; Vyatchanin, S.P.; Wittel, H.
(College Park, MD : American Physical Society, 2014)
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 ...