Double Neutron Star Binaries : A "Foreground" Source for the Gravitational-Wave Stochastic Background(Chapter VI: Gravitational waves,Cosmology-The Next Generation-)

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概要

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• 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.

• 2011-10-31

著者

• Allen Bruce

  Albert-einstein-institut Max-planck-institut Fur Gravitationsphysik:university Of Wisconsin-milwauke

• ALLEN Bruce

  Albert-Einstein-Institut, Max-Planck-Institut fur Gravitationsphysik:University of Wisconsin-Milwaukee

関連論文

• Double Neutron Star Binaries : A "Foreground" Source for the Gravitational-Wave Stochastic Background(Chapter VI: Gravitational waves,Cosmology-The Next Generation-)

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