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  Heating by optical absorption and the performance of interferometric gravitational-wave detectors

Winkler, W., Danzmann, K., Rüdiger, A., & Schilling, R. (1991). Heating by optical absorption and the performance of interferometric gravitational-wave detectors. Physical Review A, 44(11), 7022-7036. doi:10.1103/PhysRevA.44.7022.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5CAF-4 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0013-5CB0-F
Genre: Journal Article

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372218.pdf (Publisher version), 3MB
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 Creators:
Winkler, Walter1, Author              
Danzmann, Karsten1, Author              
Rüdiger, Albrecht1, Author              
Schilling, Roland1, Author              
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1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, escidoc:24010              

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 Abstract: The ultimate sensitivity of interferometric gravitational-wave detectors requires extremely high light powers sensing the separation of test masses. Absorption of light at the optical components causes wave-front distortions via the thermally deformed substrates or via thermal lensing. The performance of thermally distorted interferometers is treated quantitatively, and the two schemes for increasing the optical path, the delay-line and Fabry-Pérot methods, are compared.

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 Dates: 1991-12
 Publication Status: Published in print
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Title: Physical Review A
Source Genre: Journal
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Pages: - Volume / Issue: 44 (11) Sequence Number: - Start / End Page: 7022 - 7036 Identifier: ISSN: 1094-1622