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https://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 |
DOI: | 10.1364/OE.20.008329 |
Published version: | http://dx.doi.org/10.1364/oe.20.008329 |
Appears in Collections: | Aurora harvest 5 IPAS publications |
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