Emergence of Calabi-Yau manifolds in high-precision black hole scattering

Fuente: arXiv
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Autores principales: Driesse, Mathias, Jakobsen, Gustav Uhre, Klemm, Albrecht, Mogull, Gustav, Nega, Christoph, Plefka, Jan, Sauer, Benjamin, Usovitsch, Johann
Formato: Preprint
Publicado: 2024
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author Driesse, Mathias
Jakobsen, Gustav Uhre
Klemm, Albrecht
Mogull, Gustav
Nega, Christoph
Plefka, Jan
Sauer, Benjamin
Usovitsch, Johann
author_facet Driesse, Mathias
Jakobsen, Gustav Uhre
Klemm, Albrecht
Mogull, Gustav
Nega, Christoph
Plefka, Jan
Sauer, Benjamin
Usovitsch, Johann
contents Using the worldline quantum field theory formalism, we compute the radiation-reacted impulse, scattering angle, radiated energy and recoil of a classical black hole (or neutron star) scattering event at fifth post-Minkowskian and sub-leading self-force orders (5PM-1SF). This state-of-the-art four-loop computation employs advanced integration-by-parts and differential equation technology, and is considerably more challenging than the conservative 5PM-1SF counterpart. As compared with the conservative 5PM-1SF, in the radiation sector Calabi-Yau three-fold periods appear and contribute to the radiated energy and recoil observables. We give an extensive exposition of the canonicalization of the differential equations and provide details on boundary integrations, Feynman rules, and integration-by-parts strategies. Comparisons to numerical relativity are also performed.
format Preprint
id arxiv_https___arxiv_org_abs_2411_11846
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Emergence of Calabi-Yau manifolds in high-precision black hole scattering
Driesse, Mathias
Jakobsen, Gustav Uhre
Klemm, Albrecht
Mogull, Gustav
Nega, Christoph
Plefka, Jan
Sauer, Benjamin
Usovitsch, Johann
High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Algebraic Geometry
Using the worldline quantum field theory formalism, we compute the radiation-reacted impulse, scattering angle, radiated energy and recoil of a classical black hole (or neutron star) scattering event at fifth post-Minkowskian and sub-leading self-force orders (5PM-1SF). This state-of-the-art four-loop computation employs advanced integration-by-parts and differential equation technology, and is considerably more challenging than the conservative 5PM-1SF counterpart. As compared with the conservative 5PM-1SF, in the radiation sector Calabi-Yau three-fold periods appear and contribute to the radiated energy and recoil observables. We give an extensive exposition of the canonicalization of the differential equations and provide details on boundary integrations, Feynman rules, and integration-by-parts strategies. Comparisons to numerical relativity are also performed.
title Emergence of Calabi-Yau manifolds in high-precision black hole scattering
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Algebraic Geometry
url https://arxiv.org/abs/2411.11846