Kawamura, Seiji and Zucker, Michael E. (1994) Mirror-orientation noise in a Fabry-Perot interferometer gravitational wave detector. Applied Optics, 33 (18). pp. 3912-3918. ISSN 0003-6935 http://resolver.caltech.edu/CaltechAUTHORS:20120221-142610247
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The influence of angular mirror-orientation errors on the length of a Fabry-Perot resonator is analyzed geometrically. Under conditions in which dominant errors are static or vary slowly over time, the analysis permits a simple prediction of the spectrum of short-term cavity length fluctuations resulting from mirror-orientation noise. The resulting model is applicable to the design of mirror control systems for the Laser Interferometer Gravitational-Wave Observatory, which will monitor separations between mirrored surfaces of suspended inertial test bodies as a way to measure astrophysical gravitational radiation. The analysis is verified by measuring the response of the Laser Interferometer Gravitational- Wave Observatory's 40-m interferometer test-bed to the rotation of its mirrors.
|Additional Information:||© 1994 Optical Society of America. Received 11 January 1993; revised manuscript received 12 October 1993. We thank all those who contributed to the construction and improvement of the interferometer, and we are grateful for the continuing support of LIGO science, engineering, and administrative staff. We are especially grateful to J. Chapsky for designing the improved control electronics and to A. Gillespie, F. Raab, R. Spero, and S. Whitcomb for their assistance in measuring and analyzing the data and preparing the manuscript. Our work is supported by National Science Foundation grant PHY-9210038.|
|Subject Keywords:||Fabry-Perot, cavity, gravitational wave, interferometer, alignment|
|Official Citation:||Seiji Kawamura and Michael E. Zucker, "Mirror-orientation noise in a Fabry-Perot interferometer gravitational wave detector," Appl. Opt. 33, 3912-3918 (1994) http://www.opticsinfobase.org/abstract.cfm?URI=ao-33-18-3912|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Tony Diaz|
|Deposited On:||22 Feb 2012 00:23|
|Last Modified:||26 Dec 2012 14:51|
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