QND measurements for future gravitational-wave detectors
arXiv:0910.0319 · doi:10.1007/s10714-010-1060-y
Abstract
Second-generation interferometric gravitational-wave detectors will be operating at the Standard Quantum Limit, a sensitivity limitation set by the trade off between measurement accuracy and quantum back action, which is governed by the Heisenberg Uncertainty Principle. We review several schemes that allows the quantum noise of interferometers to surpass the Standard Quantum Limit significantly over a broad frequency band. Such schemes may be an important component of the design of third-generation detectors.
22 pages, 6 figures, 1 table; In version 2, more tutorial information on quantum noise in GW interferometer and several new items into Reference list were added
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Cited by in corpus (25)
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- Quantum Measurement Theory in Gravitational-Wave Detectors
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- Realistic Filter Cavities for Advanced Gravitational Wave Detectors
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- Quantum correlations of light due to a room temperature mechanical oscillator for force metrology
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