Advanced interferometry, quantum optics and optomechanics in gravitational wave detectors

Currently operating laser interferometric gravitational wave detectors are limited by quantum noise above a few hundred Hertz. Detectors that will come on line in the next decade are predicted to be limited by quantum noise over their entire useful frequency band (from 10 Hz to 10 kHz). Further sens...

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Published inLaser & photonics reviews Vol. 5; no. 5; pp. 677 - 696
Main Authors McClelland, D.E., Mavalvala, N., Chen, Y., Schnabel, R.
Format Journal Article
LanguageEnglish
Published Berlin WILEY-VCH Verlag 01.09.2011
WILEY‐VCH Verlag
Wiley-VCH
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Summary:Currently operating laser interferometric gravitational wave detectors are limited by quantum noise above a few hundred Hertz. Detectors that will come on line in the next decade are predicted to be limited by quantum noise over their entire useful frequency band (from 10 Hz to 10 kHz). Further sensitivity improvements will, therefore, rely on using quantum optical techniques such as squeezed state injection and quantum non‐demolition, which will, in turn, drive these massive mechanical systems into quantum states. This article reviews the principles behind these optical and quantum optical techniques and progress toward there realization. Currently operating laser interferometric gravitational wave detectors are limited by quantum noise above a few hundred Hertz. Detectors that will come on line in the next decade are predicted to be limited by quantum noise over their entire useful frequency band (from 10 Hz to 10 kHz). Further sensitivity improvements will, therefore, rely on using quantum optical techniques such as squeezed state injection and quantum nondemolition, which will, in turn, drive these massive mechanical systems into quantum states.
Bibliography:ArticleID:LPOR201000034
Deutsche Forschungsgemeinschaft - No. Centre for Quantum Engineering and Space-Time Research (QUEST)
istex:C581F82FD3BA86B673C29DBBDE2DB89609C7F132
ark:/67375/WNG-J6P42M10-V
Australian Research Council
National Science Foundation
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SourceType-Scholarly Journals-1
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ISSN:1863-8880
1863-8899
1863-8899
DOI:10.1002/lpor.201000034