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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| Format: | Article |
| Language: | English |
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SpringerOpen
2024-10-01
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| Series: | Journal of High Energy Physics |
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| 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]. |
| format | Article |
| id | doaj-art-322a42d5d5214a5293fc688ab7da8233 |
| institution | OA Journals |
| issn | 1029-8479 |
| language | English |
| publishDate | 2024-10-01 |
| publisher | SpringerOpen |
| record_format | Article |
| series | Journal of High Energy Physics |
| 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 |