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  QND measurements for future gravitational-wave detectors

Chen, Y., Danilishin, S. L., Khalili, F. Y., & Müller-Ebhardt, H. (2011). QND measurements for future gravitational-wave detectors. General Relativity and Gravitation, 43(2), 671-694. doi:10.1007/s10714-010-1060-y.

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0910.0319 (Preprint), 514KB
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 Creators:
Chen, Yanbei, Author           
Danilishin, Stefan L., Author
Khalili, Farid Ya., Author
Müller-Ebhardt, Helge1, Author           
Affiliations:
1Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 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.

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 Dates: 2009-10-012011
 Publication Status: Issued
 Pages: 21 pages, 6 figures, 1 table
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Title: General Relativity and Gravitation
Source Genre: Journal
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Publ. Info: Dordrecht, etc. : Kluwer Academic Publishers [etc.]
Pages: - Volume / Issue: 43 (2) Sequence Number: - Start / End Page: 671 - 694 Identifier: ISSN: 0001-7701
CoNE: https://pure.mpg.de/cone/journals/resource/954925263179