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

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..586..787k&link_type=abstract

RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP Conference Proceedings, Volume 586, pp. 787-792 (2001).

Statistics

Neutron Stars, Background Radiations, Spectroscopic Binaries, Close Binaries, Star Counts, Distribution, And Statistics

Scientific paper

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 νlim~10-3 Hz, leaving the frequency window ~10-3-10-2 Hz open for the potential detection of cosmological stochastic GW. .

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