On special optical modes and thermal issues in advanced gravitational wave interferometric detectors

DOI10.12942/lrr-2009-5zbMath1215.83013OpenAlexW2050538931WikidataQ36274810 ScholiaQ36274810MaRDI QIDQ533828

Jean-Yves Vinet

Publication date: 9 May 2011

Published in: Living Reviews in Relativity (Search for Journal in Brave)

Full work available at URL: https://eudml.org/doc/233621

Mathematics Subject Classification ID

Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar dynamics (85A05) Gravitational waves (83C35)

Related Items (3)

Interferometer techniques for gravitational-wave detection ⋮ Gravitational wave detection by interferometry (ground and space) ⋮ Gravitational-wave data analysis. Formalism and sample applications: the Gaussian Case

Cites Work

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• Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes
• Thermal noise in interferometric gravitational wave detectors due to dielectric optical coatings
• Mirror thermal noise in flat-beam cavities for advanced gravitational wave interferometers
• The dependence of test-mass thermal noises on beam shape in gravitational-wave interferometers
• Irreversibility and Generalized Noise

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