Journal articles
Self-force driven motion in curved spacetime
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.
Keywords :
motion
general relativity
Cited literature [7 references]
https://hal-insu.archives-ouvertes.fr/insu-01257754
Contributor : Nathalie Pothier <>
Submitted on : Tuesday, January 19, 2016 - 9:44:27 AM
Last modification on : Tuesday, April 28, 2020 - 10:38:05 AM
Document(s) archivé(s) le : Friday, November 11, 2016 - 9:24:06 AM
Contributor : Nathalie Pothier <>
Submitted on : Tuesday, January 19, 2016 - 9:44:27 AM
Last modification on : Tuesday, April 28, 2020 - 10:38:05 AM
Document(s) archivé(s) le : Friday, November 11, 2016 - 9:24:06 AM
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1405.4155v1.pdf
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Distributed under a Creative Commons Attribution - NonCommercial - NoDerivatives 4.0 International License
