Schwarzschild geodesics from scattering amplitudes to all orders in G N

Abstract The dynamics of the leading self-force (0SF) order, corresponding to the geodesic motion of a light body in the exact background of a heavy body, are explicitly derived for the first time using a flat space scattering amplitude-based approach. This is achieved by utilising the cubic formula...

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Main Authors: Stavros Mougiakakos, Pierre Vanhove
Format: Article
Language:English
Published: SpringerOpen 2024-10-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP10(2024)152
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author Stavros Mougiakakos
Pierre Vanhove
author_facet Stavros Mougiakakos
Pierre Vanhove
author_sort Stavros Mougiakakos
collection DOAJ
description Abstract The dynamics of the leading self-force (0SF) order, corresponding to the geodesic motion of a light body in the exact background of a heavy body, are explicitly derived for the first time using a flat space scattering amplitude-based approach. This is achieved by utilising the cubic formulation of Einstein’s general relativity coupled to the effective worldline action of massive point particles, which was employed to derive the Schwarzschild black hole metric in [1].
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spelling doaj-art-322a42d5d5214a5293fc688ab7da82332025-08-20T02:31:17ZengSpringerOpenJournal of High Energy Physics1029-84792024-10-0120241011110.1007/JHEP10(2024)152Schwarzschild geodesics from scattering amplitudes to all orders in G NStavros Mougiakakos0Pierre Vanhove1Laboratoire Univers et Théories, Observatoire de Paris, Université PSL, Université Paris Cité, CNRSInstitut de Physique Théorique, Université Paris-Saclay, CEA, CNRSAbstract The dynamics of the leading self-force (0SF) order, corresponding to the geodesic motion of a light body in the exact background of a heavy body, are explicitly derived for the first time using a flat space scattering amplitude-based approach. This is achieved by utilising the cubic formulation of Einstein’s general relativity coupled to the effective worldline action of massive point particles, which was employed to derive the Schwarzschild black hole metric in [1].https://doi.org/10.1007/JHEP10(2024)152Effective Field TheoriesClassical Theories of GravityBlack Holes
spellingShingle Stavros Mougiakakos
Pierre Vanhove
Schwarzschild geodesics from scattering amplitudes to all orders in G N
Journal of High Energy Physics
Effective Field Theories
Classical Theories of Gravity
Black Holes
title Schwarzschild geodesics from scattering amplitudes to all orders in G N
title_full Schwarzschild geodesics from scattering amplitudes to all orders in G N
title_fullStr Schwarzschild geodesics from scattering amplitudes to all orders in G N
title_full_unstemmed Schwarzschild geodesics from scattering amplitudes to all orders in G N
title_short Schwarzschild geodesics from scattering amplitudes to all orders in G N
title_sort schwarzschild geodesics from scattering amplitudes to all orders in g n
topic Effective Field Theories
Classical Theories of Gravity
Black Holes
url https://doi.org/10.1007/JHEP10(2024)152
work_keys_str_mv AT stavrosmougiakakos schwarzschildgeodesicsfromscatteringamplitudestoallordersingn
AT pierrevanhove schwarzschildgeodesicsfromscatteringamplitudestoallordersingn