Gravitational radiation from a particle scattered by a non-rotating black hole

Details Gravitational radiation from a particle scattered by a non-rotating black hole Gravitational radiation from a particle scattered by a non-rotating black hole

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983phla...98..407o&link_type=abstract

Physics Letters A, Volume 98, Issue 8-9, p. 407-410.

Physics

10

Scientific paper

We have analyzed the gravitational radiation emitted by a particle of mass μ and angular momentum μLz [>4μ(GM/ itc2) c] scattered by a Schwarzschild black hole of mass M (>>μ). It is found that the quasi-normal mode is not excited even when the periastron approaches the limiting value 4 GM/c2. The total energy for Lz = 4.1 (GM/c2) c is 1.24 x 1 (μ/ M) c2, which is smaller than for Lz = 3.9 (GM/c2) c.

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