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• W2078161625 abstract "It has long been thought that the sensitivity of laser interferometric gravitational-wave detectors is limited by the free-mass standard quantum limit, unless radical redesigns of the interferometers or modifications of their input/output optics are introduced. Within a fully quantum-mechanical approach we show that in a second-generation interferometer composed of arm cavities and a signal recycling cavity, e.g., the LIGO-II configuration, (i) quantum shot noise and quantum radiation-pressure-fluctuation noise are dynamically correlated, (ii) the noise curve exhibits two resonant dips, (iii) the Standard Quantum Limit can be beaten by a factor of 2, over a frequency range Delta f/f sim 1, but at the price of increasing noise at lower frequencies." @default.
• W2078161625 created "2016-06-24" @default.
• W2078161625 creator A5004437377 @default.
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• W2078161625 date "2001-07-30" @default.
• W2078161625 modified "2023-09-25" @default.
• W2078161625 title "Quantum noise in second generation, signal-recycled laser interferometric gravitational-wave detectors" @default.
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• W2078161625 doi "https://doi.org/10.1103/physrevd.64.042006" @default.
• W2078161625 hasPublicationYear "2001" @default.
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