Gravitational-wave emission during captures in black-hole clusters

Details Gravitational-wave emission during captures in black-hole clusters Gravitational-wave emission during captures in black-hole clusters

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..930p&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, Sept.-Oct. 1975, p. 930-936. In Russian.

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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