Self-force driven motion in curved spacetime
| Autor: | Sofiane Aoudia, Alessandro D. A. M. Spallicci, Patxi Ritter |
|---|---|
| Přispěvatelé: | Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Mathématiques - Analyse, Probabilités, Modélisation - Orléans (MAPMO), Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft |
| Jazyk: | angličtina |
| Rok vydání: | 2014 |
| Předmět: |
Physics
Quantum field theory in curved spacetime Physics and Astronomy (miscellaneous) Geodesic Maxwell's equations in curved spacetime FOS: Physical sciences General Relativity and Quantum Cosmology (gr-qc) Stationary spacetime General Relativity and Quantum Cosmology Mathematics of general relativity Classical mechanics [SDU]Sciences of the Universe [physics] motion general relativity Hamilton–Jacobi–Einstein equation Background independence Theoretical motivation for general relativity |
| Zdroj: | International Journal of Geometric Methods in Modern Physics International Journal of Geometric Methods in Modern Physics, World Scientific Publishing, 2014, 11 (8), pp.1450072. ⟨10.1142/S0219887814500728⟩ |
| ISSN: | 0219-8878 |
| Popis: | 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. To appear in Int. J. Geom. Meth. Mod. Phys |
| Databáze: | OpenAIRE |
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