Emission of gravitational waves accompanying the coalescence of black holes

Details Emission of gravitational waves accompanying the coalescence of black holes Emission of gravitational waves accompanying the coalescence of black holes

Apr 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976sva....19..565p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 52, Sept.-Oct. 1975, p. 930-936.) Soviet Astronomy, vol. 19, no. 5, 1976, p. 565-568. Translati

Astronomy and Astrophysics

Astrophysics

Black Holes (Astronomy), Gravitational Waves, Star Clusters, Stellar Radiation, Astrophysics, Galactic Nuclei, Gravitational Collapse, Neutron Stars

Scientific paper

A qualitative picture of gravitational emission during the coalescence of two black holes is calculated. It is found that a sequence of gravitational-radiation bursts is characteristic of such a process and that the collision parameters may be determined, in principle, from the ratio of the time intervals between subsequent bursts. The frequency of such events is obtained as a function of the time between subsequent bursts and as a function of the total number of bursts on the assumption that black-hole clusters serve as the sources of the gravitational radiation.

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