PreprintCC BY 4.0arXiv
Radiative losses from unbound orbits at quadratic order in spin from MPM formalism
Abstract
We study the spinning two-body system in the aligned spin case for hyperboliclike motions computing all radiative losses (at the 2PN absolute accuracy and including spin-squared corrections) using the MPM formalism and generalizing previous results valid at linear order in spin [Phys. Rev. D \textbf{108}, no.6, 064049 (2023)]. Leading PM order results are checked against existing literature, whereas higher-order PM results (within the 2PN accuracy) are new with this work. As a by-product of our general results we analyze the spinning situation which supports radial fall (at 2PN and including spin-squared accuracy level contributions), showing that as soon as the PN accuracy increases deviations from radial fall appear necessarily.
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BibTeX
@misc{bini2026radiative,
title = {{Radiative losses from unbound orbits at quadratic order in spin from MPM formalism}},
author = {Donato Bini and Giorgio Di Russo},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.20185},
eprint = {2609.20185},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.20185},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Radiative losses from unbound orbits at quadratic order in spin from MPM formalism
AU - Donato Bini
AU - Giorgio Di Russo
PY - 2026
DA - 2026/09/01
PB - arXiv
DO - 10.48550/arxiv.2609.20185
UR - https://arxiv.org/abs/2609.20185
AB - We study the spinning two-body system in the aligned spin case for hyperboliclike motions computing all radiative losses (at the 2PN absolute accuracy and including spin-squared corrections) using the MPM formalism and generalizing previous results valid at linear order in spin [Phys. Rev. D \textbf{108}, no.6, 064049 (2023)]. Leading PM order results are checked against existing literature, whereas higher-order PM results (within the 2PN accuracy) are new with this work. As a by-product of our general results we analyze the spinning situation which supports radial fall (at 2PN and including spin-squared accuracy level contributions), showing that as soon as the PN accuracy increases deviations from radial fall appear necessarily.
ER -