Gravitational radiation by a particle with nonzero orbital angular momentum falling into a Kerr black hole

Details Gravitational radiation by a particle with nonzero orbital angular momentum falling into a Kerr black hole Gravitational radiation by a particle with nonzero orbital angular momentum falling into a Kerr black hole

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phla...99...37k&link_type=abstract

Physics Letters A, Volume 99, Issue 1, p. 37-40.

Physics

12

Scientific paper

We have computed the energy of the gravitational waves induced by a particle with nonzero orbital angular momentum μLz plunging into a Kerr black hole in an equatorial plane. It is found that for the same |Lz| a corotating particle emits more energy than a counter-rotating one, which is due to the change of the frequency of the quasi-normal mode with the increase of the angular momentum of the black hole.

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