Radiation-reaction correction to scattering binary dynamics at the Next-to-Leading Post-Newtonian Order

Fuente: arXiv
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Main Authors: Bini, Donato, Geralico, Andrea, Aliberti, Sara Rufrano
Format: Preprint
Published: 2025
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author Bini, Donato
Geralico, Andrea
Aliberti, Sara Rufrano
author_facet Bini, Donato
Geralico, Andrea
Aliberti, Sara Rufrano
contents We compute the next-to-leading-order radiation-reaction modification to the harmonic coordinate quasi-Keplerian parametrization of the binary dynamics, the two bodies undergoing a scattering process. The solution for the radiation-reaction corrections to the orbital parameters is examined both in the time domain and in the frequency domain. The knowledge of the radiation-reaction corrected orbit is a key ingredient for the calculation of the fractional 3.5PN corrections to the radiative losses as well as to the radiative multipole moments needed to build up the waveform at the same accuracy.
format Preprint
id arxiv_https___arxiv_org_abs_2509_17853
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Radiation-reaction correction to scattering binary dynamics at the Next-to-Leading Post-Newtonian Order
Bini, Donato
Geralico, Andrea
Aliberti, Sara Rufrano
General Relativity and Quantum Cosmology
We compute the next-to-leading-order radiation-reaction modification to the harmonic coordinate quasi-Keplerian parametrization of the binary dynamics, the two bodies undergoing a scattering process. The solution for the radiation-reaction corrections to the orbital parameters is examined both in the time domain and in the frequency domain. The knowledge of the radiation-reaction corrected orbit is a key ingredient for the calculation of the fractional 3.5PN corrections to the radiative losses as well as to the radiative multipole moments needed to build up the waveform at the same accuracy.
title Radiation-reaction correction to scattering binary dynamics at the Next-to-Leading Post-Newtonian Order
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2509.17853