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Lasers and optics: looking towards third generation gravitational wave detectors

Mavalvala, Nergis; McClelland, David; Mueller, Guido; Reitze, D; Schnabel, Roman; Willke, B

Description

Third generation terrestrial interferometric gravitational wave detectors will likely require significant advances in laser and optical technologies to reduce two of the main limiting noise sources: thermal noise due to mirror coatings and quantum noise arising from a combination of shot noise and radiation pressure noise. Increases in laser power and possible changes of the operational wavelength require new high power laser sources and new electro-optic modulators and Faraday isolators....[Show more]

CollectionsANU Research Publications
Date published: 2011
Type: Journal article
URI: http://hdl.handle.net/1885/53178
Source: General Relativity and Gravitation
DOI: 10.1007/s10714-010-1023-3

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