Notes about Noise in Gravitational Wave Antennas Created by Cosmic Rays

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dc.creatorBraginsky, V. B.
dc.creatorRyazhskaya, O. G.
dc.creatorVyatchanin, S. P.
dc.date2005-09-15
dc.date.accessioned2026-07-07T11:26:18Z
dc.date.available2026-07-07T11:26:18Z
dc.descriptionThermodynamical fluctuations of temperature in mirrors may produce surface fluctuations not only through thermal expansion in mirror body but also through thermal expansion in mirror coating. We analyze the last "surface" effect which can be larger than the first "volume" one due to larger thermal expansion coefficient of coating material and smaller effective volume. In particular, these fluctuations may be important in laser interferometric gravitational antennae.
dc.description9 pages, LaTex
dc.identifierhttps://arxiv.org/abs/gr-qc/0509058
dc.identifierhttp://arxiv.org/abs/gr-qc/0509058
dc.identifierPhys.Lett.A350:1-4,2006
dc.identifierdoi:10.1016/j.physleta.2005.09.073
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195783
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNotes about Noise in Gravitational Wave Antennas Created by Cosmic Rays
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