Please use this identifier to cite or link to this item:
|Scopus||Web of Science®||Altmetric|
|Title:||Gingin high optical power test facility|
|Citation:||Journal of Physics: Conference Series (Print Edition), 2006; 32(1):368-373|
|Publisher:||Institute of Physics Publishing|
|C. Zhao, D.G. Blair, P. Barriga, J. Degallaix, J-C Dumas, Y. Fan, S. Gras, L. Ju, B. Lee, S. Schediwy, Z. Yan, D.E. McClelland, S.M. Scott, M.B. Gray, A.C. Searle, S. Gossler, B.J.J. Slagmolen, J. Dickson, K. McKenzie, C. Mow-Lowry, A. Moylan, D. Rabeling, J. Cumpston, K. Wette, J. Munch, P.J. Veitch, D. Mudge, A. Brooks, and D. Hosken|
|Abstract:||The Australian Consortium for Gravitational Wave Astronomy (ACIGA) in collaboration with LIGO is developing a high optical power research facility at the AIGO site, Gingin, Western Australia. Research at the facility will provide solutions to the problems that advanced gravitational wave detectors will encounter with extremely high optical power. The problems include thermal lensing and parametric instabilities. This article will present the status of the facility and the plan for the future experiments.|
|Description:||Copyright © Institute of Physics and IOP Publishing Limited 2006.|
|Appears in Collections:||Physics publications|
Environment Institute publications
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.