Published March 7, 2004 | Version v1
Journal article

Experimental measurements of coating mechanical loss factors

  • 1. Institute for Gravitational Research, Department of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ (United Kingdom)
  • 2. Edward L Ginzton Laboratory, Stanford University, Stanford, CA 94305-4088 (United States)
  • 3. LIGO Livingston Observatory, Livingston, Louisiana, 70754 (United States)
  • 4. LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)
  • 5. Centre for Nondestructive Evaluation, Institute for Physical Research and Technology, Iowa State University, Ames, IA 50011 (United States)
  • 6. Department of Physics, Hobart and William Smith Colleges, Geneva, New York, 14456 (United States)

Description

All current gravitational wave detectors use test masses coated with alternating layers of two different dielectric materials to form highly reflective mirrors. The thermal noise from mechanical dissipation associated with such coatings may be significant for future detectors such as advanced LIGO. We have measured the mechanical dissipation of a number of types of coatings formed from SiO2 (silica) and Ta2O5 (tantala). The frequency dependence of the dissipation has been determined, taking into account the contribution of thermoelastic loss

Availability note (English)

Available online at http://stacks.iop.org/0264-9381/21/S1059/cqg4_5_101.pdf or at the Web site for the journal Classical and Quantum Gravity (ISSN 1361-6382) http://www.iop.org/

Additional details

Publishing Information

Journal Title
Classical and Quantum Gravity
Journal Volume
21
Journal Issue
5
Journal Page Range
p. S1059-S1065
ISSN
0264-9381
CODEN
CQGRDG

Conference

Title
5. Edoardo Amaldi conference on gravitational waves
Dates
6-11 Jul 2003
Place
Tirrenia (Italy)