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arXiv · 1405.4155

Self-force driven motion in curved spacetimes

Alessandro D. A. M. Spallicci·P. Ritter·S. Aoudia
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Abstract

We adopt the Dirac-Detweiler-Whiting radiative and regular effective field in curved spacetime. Thereby, we derive straightforwardly the first order perturbative correction to the geodesic of the background in a covariant form, for the extreme mass ratio two-body problem. The correction contains the self-force contribution and a background metric dependent term.

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Alessandro D. A. M. Spallicci, P. Ritter, S. Aoudia. 2014-05-16. Self-force driven motion in curved spacetimes. https://arxiv.org/abs/1405.4155

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