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arxiv: gr-qc/0212103 · v2 · submitted 2002-12-25 · 🌀 gr-qc

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Gravitational self-force on a particle orbiting a Kerr black hole

Leor Barack , Amos Ori
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classification 🌀 gr-qc
keywords gravitationalkerrblackholemethodparticleregularizationself-force
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We present a practical method for calculating the gravitational self-force, as well as the electromagnetic and scalar self forces, for a particle in a generic orbit around a Kerr black hole. In particular, we provide the values of all the regularization parameters needed for implementing the (previously introduced) {\it mode-sum regularization} method. We also address the gauge-regularization problem, as well as a few other issues involved in the calculation of gravitational radiation-reaction in Kerr spacetime.

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Cited by 1 Pith paper

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  1. All-order structure of static gravitational interactions and the seventh post-Newtonian potential

    hep-th 2026-04 unverdicted novelty 6.0

    A closed formula computes static post-Newtonian corrections at arbitrary odd orders in gravity, yielding the explicit seventh post-Newtonian potential that matches an independent diagrammatic method.