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  Double Neutron Star Binaries: A “Foreground” Source for the Gravitational-Wave Stochastic Background

Allen, B. (2011). Double Neutron Star Binaries: A “Foreground” Source for the Gravitational-Wave Stochastic Background. Progress of Theoretical Physics, Supplement, 190, 316-321. doi:10.1143/PTPS.190.316.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-10AC-D Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-10AD-B
Genre: Journal Article

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 Creators:
Allen, Bruce1, Author              
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1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24011              

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 Abstract: Cosmological sources of gravitational wave backgrounds can be hidden by “foreground” sources: signals produced recently by normal astrophysical sources. Here, we briefly examine one such foreground source: the signals produced by the inspiral of Double Neutron Star (DNS) binaries. We do simple estimates of the spectrum and statistical properties of the resulting foreground, and discuss when the signals might be removable and when they form a central-limit-theorem confusion noise.

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 Dates: 2011
 Publication Status: Published in print
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 Identifiers: DOI: 10.1143/PTPS.190.316
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Title: Progress of Theoretical Physics, Supplement
Source Genre: Journal
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Publ. Info: Kyoto, Japan : Kyoto University.
Pages: - Volume / Issue: 190 Sequence Number: - Start / End Page: 316 - 321 Identifier: ISSN: 0375-9687
CoNE: /journals/resource/954925525801