Radiation-reaction-induced evolution of circular orbits of particles around Kerr Black Holes
arXiv:gr-qc/9512018 · doi:10.1103/PhysRevD.53.4319
Abstract
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.
23 pages. Revtex 3.0. Inquiries to [email protected]
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