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ACIGA's high optical power test facility

Ju, Li; Aoun, M; Barriga, P; Blair, David Gerald; Brooks, A; Burman, R; Burston, R; Chin, X; Chin, E J; Lee, C Y; Coward, D; Cusack, B J; De Vine, Glenn; Degallaix, J; Dumas, J-C; Garoi, Florin; Gras, S; Gray, Malcolm; Hosken, David; Howell, E; Jacob, J S; Kelly, Theresa-Lan; Lee, B L; Lee, K T; Lun, T; McClelland, David; Mow-Lowry, C; Mudge, D; Munch, Jesper; Schediwy, S; Scott, Susan M; Searle, Antony; Sheard, B; Slagmolen, Bram; Veitch, Peter John; Winterflood, J; Woolley, A; Yan, Z; Zhao, Chunnong

Description

Advanced laser interferometer detectors utilizing more than 100 W of laser power and with ∼106 W circulating laser power present many technological problems. The Australian Consortium for Interferometric Gravitational Astronomy (ACIGA) is developing a h

CollectionsANU Research Publications
Date published: 2004
Type: Journal article
URI: http://hdl.handle.net/1885/87180
Source: Classical and Quantum Gravity
DOI: 10.1088/0264-9381/21/5/077

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