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MPM形式论下自旋二次阶非束缚轨道的辐射损失

Radiative losses from unbound orbits at quadratic order in spin from MPM formalism

Donato Bini, Giorgio Di Russo

arXiv 2609.20185首次发表:更新:

发表机构

Istituto per le Applicazioni del Calcolo “M. Picone,” CNR; School of Fundamental Physics and Mathematical Sciences, Hangzhou Institute for Advanced Study, UCAS(意大利国家研究委员会计算应用研究所; 杭州高等研究院基础物理与数学学院,中国科学院大学)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

本研究利用MPM形式论计算了自旋双体系统在2PN精度下的辐射损失,推广至自旋平方阶,并发现高精度下径向下落偏差必然出现。

AI 中文摘要

我们研究了自旋双体系统在对齐自旋情形下的双曲型运动,利用MPM形式论计算了所有辐射损失(达到2PN绝对精度并包含自旋平方修正),推广了先前仅适用于自旋线性阶的结果[Phys. Rev. D \ extbf{108}, no.6, 064049 (2023)]。领先PM阶的结果与现有文献进行了核对,而更高阶PM结果(在2PN精度内)则是本工作的新贡献。作为我们一般结果的副产品,我们分析了支持径向下落的旋转情形(在2PN精度并包含自旋平方阶贡献),表明随着PN精度的提高,径向下落的偏差必然出现。

英文摘要

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.

Comments17 pages, no figures

论文原文

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