http://arxiv.org/abs/1405.4155
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.
A. Spallicci, P. Ritter and S. Aoudia
Mon, 19 May 14
1/45
Comments: To appear in Int. J. Geom. Meth. Mod. Phys