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|Title:||The impact of upconverted scattered light on advanced interferometric gravitational wave detectors|
|Citation:||Optics Express, 2012; 20(8):8329-8336|
|Publisher:||Optical Soc Amer|
|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|
|Appears in Collections:||IPAS publications|
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