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|Title:||ACIGA's high optical power test facility|
de Vine, G.
|Citation:||Classical and Quantum Gravity, 2004; 21(5):S887-S893|
|Publisher:||IOP Publishing Ltd|
|L Ju, M Aoun, P Barriga, D G Blair, A Brooks, R Burman, R Burston, X T Chin, E J Chin, C Y Lee, D Coward, B Cusack, G de Vine, J Degallaix, J C Dumas, F Garoi, S Gras, M Gray, D Hosken, E Howell, J S Jacob, T L Kelly, B Lee, K T Lee, T Lun, D McClelland, C Mow-Lowry, D Mudge, J Munch, S Schediwy, S Scott, A Searle, B Sheard, B Slagmolen, P Veitch, J Winterflood, A Woolley, Z Yan and C Zhao|
|Abstract:||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 high power research facility in Gingin, north of Perth, Western Australia, which will test techniques for the next generation interferometers. In particular it will test thermal lensing compensation and control strategies for optical cavities in which optical spring effects and parametric instabilities may present major difficulties.|
|Description:||Copyright © Institute of Physics and IOP Publishing Limited 2004.|
|Appears in Collections:||Physics publications|
Environment Institute publications
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