Literature DB >> 22139282

Backscatter tolerant squeezed light source for advanced gravitational-wave detectors.

Sheon S Y Chua1, Michael S Stefszky, Conor M Mow-Lowry, Ben C Buchler, Sheila Dwyer, Daniel A Shaddock, Ping Koy Lam, David E McClelland.   

Abstract

We report on the performance of a dual-wavelength resonant, traveling-wave optical parametric oscillator to generate squeezed light for application in advanced gravitational-wave interferometers. Shot noise suppression of 8.6±0.8 dB was measured across the detection band of interest to Advanced LIGO, and controlled squeezing measured over 5900 s. Our results also demonstrate that the traveling-wave design has excellent intracavity backscattered light suppression of 47 dB and incident backscattered light suppression of 41 dB, which is a crucial design issue for application in advanced interferometers.
© 2011 Optical Society of America

Year:  2011        PMID: 22139282     DOI: 10.1364/OL.36.004680

Source DB:  PubMed          Journal:  Opt Lett        ISSN: 0146-9592            Impact factor:   3.776


  1 in total

1.  A squeezed light source operated under high vacuum.

Authors:  Andrew R Wade; Georgia L Mansell; Sheon S Y Chua; Robert L Ward; Bram J J Slagmolen; Daniel A Shaddock; David E McClelland
Journal:  Sci Rep       Date:  2015-12-14       Impact factor: 4.379

  1 in total

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