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Optical design of the proposed Australian International Gravitational Observatory
Pablo Barriga, Muzammil A. Arain, Guido Mueller, Chunnong Zhao, and David G. Blair »View Author Affiliations
1School of Physics, The University of Western Australia, Crawley, WA 6009
2Department of Physics, University of Florida, Gainesville, FL32611, USA
*Corresponding author: pbarriga@cyllene.uwa.edu.au
Optics Express, Vol. 17, Issue 4, pp. 2149-2165 (2009)
http://dx.doi.org/10.1364/OE.17.002149
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Abstract
Marginally stable power recycling cavities are being used by nearly all interferometric gravitational wave detectors. With stability factors very close to unity the frequency separation of the higher order optical modes is smaller than the cavity bandwidth. As a consequence these higher order modes will resonate inside the cavity distorting the spatial mode of the interferometer control sidebands. Without losing generality we study and compare two designs of stable power recycling cavities for the proposed 5 kilometer long Australian International Gravitational Observatory (AIGO), a high power advanced interferometric gravitational wave detector. The length of various optical cavities that form the interferometer and the modulation frequencies that generate the control sidebands are also selected.
© 2009 Optical Society of America
OCIS Codes
(120.0120) Instrumentation, measurement, and metrology : Instrumentation, measurement, and metrology
(120.2230) Instrumentation, measurement, and metrology : Fabry-Perot
(120.3180) Instrumentation, measurement, and metrology : Interferometry
(350.4600) Other areas of optics : Optical engineering
ToC Category:
Instrumentation, Measurement, and Metrology
History
Original Manuscript: November 13, 2008
Revised Manuscript: December 13, 2008
Manuscript Accepted: December 17, 2008
Published: February 2, 2009
Citation
Pablo Barriga, Muzammil A. Arain, Guido Mueller, Chunnong Zhao, and David G. Blair, "Optical design of the proposed Australian International Gravitational
Observatory," Opt. Express 17, 2149-2165 (2009)
http://www.opticsinfobase.org/oe/abstract.cfm?URI=oe-17-4-2149
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- L. Ju, S. Gras, C. Zhao, J. Degallaix, D. G. Blair, "Multiple modes contributions to parametric instabilities in advanced laser ineterferometer gravitational wave detectors," Phys. Lett. A 354, 360-365, (2006). [CrossRef]
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