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Journal Article

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

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons40518

Allen,  Bruce
Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society;

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Fulltext (public)

PTPS-190-316.pdf
(Any fulltext), 252KB

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Citation

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.


Cite as: http://hdl.handle.net/11858/00-001M-0000-000F-10AC-D
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.