Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/69885
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Type: Journal article
Title: The impact of upconverted scattered light on advanced interferometric gravitational wave detectors
Author: Ottaway, D.
Fritschel, P.
Waldman, S.
Citation: Optics Express, 2012; 20(8):8329-8336
Publisher: Optical Soc Amer
Issue Date: 2012
ISSN: 1094-4087
1094-4087
Statement of
Responsibility: 
David J Ottaway, Peter Fritschel, and Samuel J. Waldman
Abstract: Second generation gravitational wave detectors are being installed in a number of locations globally. These long-baseline, Michelson interferometers increase the sensitivity between 10 and 40 Hz by many orders of magnitude compared with first generation instruments. Control of non-linear noise coupling from scattered light fields is critical to achieve low frequency performance. In this paper we investigate the requirements on the attenuation of scattered light using a novel time-domain analysis and two years of seismic data from the LIGO Livingston Observatory.
Rights: © 2012 Optical Society of America
RMID: 0020118496
DOI: 10.1364/OE.20.008329
Appears in Collections:IPAS publications

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