Radiation-reaction-induced evolution of circular orbits of particles around Kerr Black Holes

Details Radiation-reaction-induced evolution of circular orbits of particles around Kerr Black Holes Radiation-reaction-induced evolution of circular orbits of particles around Kerr Black Holes

1995-12-08

arxiv.org/abs/gr-qc/9512018v1

Phys.Rev. D53 (1996) 4319-4326

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

23 pages. Revtex 3.0. Inquiries to danielk@tapir.caltech.edu

Scientific paper

10.1103/PhysRevD.53.4319

It is demonstrated that, in the adiabatic approximation, non-Equatorial circular orbits of particles in the Kerr metric (i.e. orbits of constant Boyer-Lindquist radius) remain circular under the influence of gravitational radiation reaction. A brief discussion is given of conditions for breakdown of adiabaticity and of whether slightly non-circular orbits are stable against the growth of eccentricity.

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