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.
https://hal-insu.archives-ouvertes.fr/insu-01257754
Contributeur : Nathalie Pothier
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Soumis le : mardi 19 janvier 2016 - 09:44:27
Dernière modification le : jeudi 7 février 2019 - 17:22:48
Document(s) archivé(s) le : vendredi 11 novembre 2016 - 09:24:06
Alessandro D. A. M. Spallicci, Patxi Ritter, Sofiane Aoudia. Self-force driven motion in curved spacetime. International Journal of Geometric Methods in Modern Physics, World Scientific Publishing, 2014, 11 (8), pp.1450072. 〈10.1142/S0219887814500728〉. 〈insu-01257754〉
