Vajente, Gabriele (2014) Interferometer Configurations. In: Advanced Interferometers and the Search for Gravitational Waves. Astrophysics and Space Science Library. Vol.404. Springer , Cham, Switzerland, pp. 57-95. ISBN 978-3-319-03791-2. https://resolver.caltech.edu/CaltechAUTHORS:20170622-075759340
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Abstract
Gravitational waves induce a differential strain between free-falling test masses. The most sensitive instruments to measure this kind of effect are laser interferometers. This chapter introduces the working principles of the different optical configuration that were and will be used in gravitational wave detectors: Michelson interferometer, Fabry-Perot resonant cavity, power and signal recycling techniques. Advanced detectors will feature high power levels, therefore the important issue of radiation pressure effects is addressed. Finally, a brief introduction to the topic of diffraction limited beams and high order transverse electromagnetic modes is included.
Item Type: | Book Section | |||||||||
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Additional Information: | © 2014 Springer International Publishing Switzerland. 06 March 2014. | |||||||||
Group: | LIGO | |||||||||
Series Name: | Astrophysics and Space Science Library | |||||||||
DOI: | 10.1007/978-3-319-03792-9_3 | |||||||||
Record Number: | CaltechAUTHORS:20170622-075759340 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20170622-075759340 | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 78455 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | Ruth Sustaita | |||||||||
Deposited On: | 22 Jun 2017 17:47 | |||||||||
Last Modified: | 15 Nov 2021 17:40 |
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