期刊
LASER & PHOTONICS REVIEWS
卷 5, 期 5, 页码 677-696出版社
WILEY-V C H VERLAG GMBH
DOI: 10.1002/lpor.201000034
关键词
Gravitational waves; quantum optics; opto-mechanics
资金
- Australian Research Council
- National Science Foundation
- Deutsche Forschungsgemeinschaft through the Centre for Quantum Engineering and Space-Time Research, QUEST
- Direct For Mathematical & Physical Scien
- Division Of Physics [1068772] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Physics [0757058] Funding Source: National Science Foundation
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.
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