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arXiv · 1112.4821

Self-consistent orbital evolution of a particle around a Schwarzschild black hole

Peter Diener·Ian Vega·Barry Wardell·Steven Detweiler
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Abstract

The motion of a charged particle is influenced by the self-force arising from the particle's interaction with its own field. In a curved spacetime, this self-force depends on the entire past history of the particle and is difficult to evaluate. As a result, all existing self-force evaluations in curved spacetime are for particles moving along a fixed trajectory. Here, for the first time, we overcome this long-standing limitation and present fully self-consistent orbits and waveforms of a scalar charged particle around a Schwarzschild black hole.

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Peter Diener, Ian Vega, Barry Wardell, Steven Detweiler. 2012-09-27. Self-consistent orbital evolution of a particle around a Schwarzschild black hole. https://doi.org/10.1103/physrevlett.108.191102

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