Scattering Amplitudes and Conservative Binary Dynamics at $O(G^5)$ without Self-Force Truncation

Fuente: arXiv
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Main Authors: Bern, Zvi, Herrmann, Enrico, Roiban, Radu, Ruf, Michael S., Smirnov, Alexander V., Smith, Sid, Zeng, Mao
Format: Preprint
Published: 2025
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author Bern, Zvi
Herrmann, Enrico
Roiban, Radu
Ruf, Michael S.
Smirnov, Alexander V.
Smith, Sid
Zeng, Mao
author_facet Bern, Zvi
Herrmann, Enrico
Roiban, Radu
Ruf, Michael S.
Smirnov, Alexander V.
Smith, Sid
Zeng, Mao
contents We compute the complete potential-graviton contributions to the conservative radial action and scattering angle for two non-spinning bodies in general relativity, accurate through fifth order in Newton's constant and including second-order self-force (2SF) effects. The calculation is carried out in the scattering-amplitude framework, combining the double copy, effective field theory, and multi-loop integration techniques based on integration by parts and differential equations. To address a major computational bottleneck, we develop improved integration-by-parts algorithms that render calculations at this order tractable. The post-Minkowskian amplitude is presented as a series expansion, following the strategy used earlier in maximal supergravity. For the first self-force sector, which involves only polylogarithmic functions, we also provide a closed-form analytic expression. For the second self-force sector, as in earlier supergravity work, we find nontrivial cancellations among contributions related to integrals supported on Calabi-Yau geometry.
format Preprint
id arxiv_https___arxiv_org_abs_2512_23654
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Scattering Amplitudes and Conservative Binary Dynamics at $O(G^5)$ without Self-Force Truncation
Bern, Zvi
Herrmann, Enrico
Roiban, Radu
Ruf, Michael S.
Smirnov, Alexander V.
Smith, Sid
Zeng, Mao
High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
We compute the complete potential-graviton contributions to the conservative radial action and scattering angle for two non-spinning bodies in general relativity, accurate through fifth order in Newton's constant and including second-order self-force (2SF) effects. The calculation is carried out in the scattering-amplitude framework, combining the double copy, effective field theory, and multi-loop integration techniques based on integration by parts and differential equations. To address a major computational bottleneck, we develop improved integration-by-parts algorithms that render calculations at this order tractable. The post-Minkowskian amplitude is presented as a series expansion, following the strategy used earlier in maximal supergravity. For the first self-force sector, which involves only polylogarithmic functions, we also provide a closed-form analytic expression. For the second self-force sector, as in earlier supergravity work, we find nontrivial cancellations among contributions related to integrals supported on Calabi-Yau geometry.
title Scattering Amplitudes and Conservative Binary Dynamics at $O(G^5)$ without Self-Force Truncation
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2512.23654