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Gravitational wave background from coalescing compact stars in eccentric orbits

V. B. Ignatiev·A. G. Kuranov·K. A. Postnov·M. E. Prokhorov
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Abstract

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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V. B. Ignatiev, A. G. Kuranov, K. A. Postnov, M. E. Prokhorov. 2001-06-18. Gravitational wave background from coalescing compact stars in eccentric orbits. https://doi.org/10.1046/j.1365-8711.2001.04732.x

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