Gravitational wave background from coalescing compact stars in eccentric orbits

Details Gravitational wave background from coalescing compact stars in eccentric orbits Gravitational wave background from coalescing compact stars in eccentric orbits

2001-06-18

arxiv.org/abs/astro-ph/0106299v1

Mon.Not.Roy.Astron.Soc. 327 (2001) 531

Astronomy and Astrophysics

Astrophysics

6 pages, 7 figures

Scientific paper

10.1046/j.1365-8711.2001.04732.x

Stochastic gravitational wave background produced by a stationary coalescing population of binary neutron stars in the Galaxy is calculated. This background is found to constitute a confusion limit within the LISA frequency band up to a limiting frequency $\NUlim{}\sim 10^{-3}$ Hz, leaving the frequency window $\sim 10^{-3}$--$10^{-2}$ Hz open for the potential detection of cosmological stochastic gravitational waves and of signals involving massive black holes out to cosmological distances.

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