Technology developments for ACIGA high power test facility for advanced interferometry

Date

2005

Authors

Barriga, P.
Barton, M.
Blair, D.
Brooks, A.
Burman, R.
Burston, R.
Chin, E.
Chow, J.
Coward, D.
Cusack, B.

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Journal article

Citation

Classical and Quantum Gravity, 2005; 22(10):S199-S208

Statement of Responsibility

P Barriga, M Barton, D G Blair, A Brooks, R Burman, R Burston, E J Chin, J Chow, D Coward, B Cusack, G de Vine, J Degallaix, J C Dumas, M Feat, S Gras, M Gray, M Hamilton, D Hosken, E Howell, J S Jacob, L Ju, T L Kelly, B H Lee, C Y Lee, K T Lee, A Lun, D E McClelland, K McKenzie, C Mow-Lowry, A Moylan, D Mudge, J Munch, D Rabeling, D Reitze, A Romann, S Schediwy, S M Scott, A Searle, B S Sheard, B J J Slagmolen, P Veitch, J Winterflood, A Woolley, Z Yan and C Zhao

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Abstract

The High Optical Power Test Facility for Advanced Interferometry has been built by the Australian Consortium for Interferometric Gravitational Astronomy north of Perth in Western Australia. An 80 m suspended cavity has been prepared in collaboration with LIGO, where a set of experiments to test suspension control and thermal compensation will soon take place. Future experiments will investigate radiation pressure instabilities and optical spring effects in a high power optical cavity with ~200 kW circulating power. The facility combines research and development undertaken by all consortium members, whose latest results are presented.

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Copyright © Institute of Physics and IOP Publishing Limited 2005.

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