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Advanced interferometry, quantum optics and optomechanics in gravitational wave detectors

MPG-Autoren
http://pubman.mpdl.mpg.de/cone/persons/resource/persons4285

Chen,  Y.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons40490

Schnabel,  R.
Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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LaserPhotoRev5_677.pdf
(beliebiger Volltext), 2MB

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Zitation

McClelland, D., Mavalvala, N., Chen, Y., & Schnabel, R. (2011). Advanced interferometry, quantum optics and optomechanics in gravitational wave detectors. Laser & Photonics Reviews, 5(5), 677-696. doi:10.1002/lpor.201000034.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-000F-0402-C
Zusammenfassung
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. This article reviews the principles behind these optical and quantum optical techniques and progress toward there realization.