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Interferometer Configurations

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. http://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
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/978-3-319-03792-9_3DOIArticle
https://link.springer.com/chapter/10.1007%2F978-3-319-03792-9_3PublisherArticle
Additional Information:© 2014 Springer International Publishing Switzerland. 06 March 2014.
Group:LIGO
Record Number:CaltechAUTHORS:20170622-075759340
Persistent URL:http://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:22 Jun 2017 17:47

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