A New Estimation of the Merging Binary Black Holes Detection Rate

Details A New Estimation of the Merging Binary Black Holes Detection Rate A New Estimation of the Merging Binary Black Holes Detection Rate

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..686..285l&link_type=abstract

THE ASTROPHYSICS OF GRAVITATIONAL WAVE SOURCES. AIP Conference Proceedings, Volume 686, pp. 285-288 (2003).

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Gravitational Radiation, Magnetic Fields, And Other Observations, Black Holes, Cataclysmic Binaries, Symbiotic Stars

Scientific paper

The binary relativistic stars merge rate in the Universe is determined mostly by the evolutionary scenario of the binary stars. Some of the unknown parameters of this scenario can be estimateted by the comparison of population synthesis predictions with the actually observed galactic population. We performed the Scenario Machine simulations with a revised scenario model and obtained that the lower estimate of the binary black hole merger rate should be ~ 7 times higher than was given before.

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