Thermoelastic dissipation in inhomogeneous media: loss measurements and displacement noise in coated test masses for interferometric gravitational wave detectors

M. M. Fejer, S. Rowan, G. Cagnoli, D. R. M. Crooks, A. Gretarsson, G. M. Harry, J. Hough, S. D. Penn, P. H. Sneddon, and S. P. Vyatchanin
Phys. Rev. D 70, 082003 – Published 22 October 2004

Abstract

The displacement noise in the test-mass mirrors of interferometric gravitational wave detectors is proportional to their elastic dissipation at the observation frequencies. In this paper, we analyze one fundamental source of dissipation in thin coatings, thermoelastic damping associated with the dissimilar thermal and elastic properties of the film and the substrate. We obtain expressions for the thermoelastic dissipation factor necessary to interpret resonant loss measurements, and for the spectral density of displacement noise imposed on a Gaussian beam reflected from the face of a coated mass. The predicted size of these effects is large enough to affect the interpretation of loss measurements, and to influence design choices in advanced gravitational wave detectors.

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  • Received 22 August 2003

DOI:https://doi.org/10.1103/PhysRevD.70.082003

©2004 American Physical Society

Authors & Affiliations

M. M. Fejer1, S. Rowan1,2, G. Cagnoli2, D. R. M. Crooks2, A. Gretarsson3, G. M. Harry4, J. Hough2, S. D. Penn6, P. H. Sneddon2, and S. P. Vyatchanin6

  • 1Edward L. Ginzton Laboratory, Stanford University, Stanford, California 94305, USA
  • 2IGR, Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ
  • 3LIGO Livingston Laboratory, 19100 LIGO Lane, Livingston, Louisiana 70754, USA
  • 4LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
  • 5Dept. of Physics, Hobart and William Smith Colleges, Geneva, New York 14456, USA
  • 6Physics Faculty, Moscow State University, Moscow 119899, Russia

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Issue

Vol. 70, Iss. 8 — 15 October 2004

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