The need for more and more accurate gravitational wave templates requires taking into account all possible contributions to the emission of gravitational radiation from a binary system. Therefore, working within a multipolar-post-Minkowskian framework to describe the gravitational wave field in terms of the source multipole moments, the dominant instantaneous effects should be supplemented by hereditary contributions arising from nonlinear interactions between the multipoles. The latter effects are referred to as tails being described in terms of integrals depending on the past history of the source. We compute higher-order tail (i.e., tail-of-tail and tail-squared) contributions to both energy and angular momentum fluxes and their averaged values along hyperboliclike orbits at the leading post-Newtonian approximation, using harmonic coordinates and working in the Fourier domain. Due to the increasing level of accuracy recently achieved in the determination of the scattering angle in a two-body system by several complementary approaches, the knowledge of these terms will provide useful information to compare results from different formalisms.
Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting
Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order
Momentum recoil in the relativistic two-body problem: higher-order tails
在描述相对论性两体相互作用时，除了由于引力辐射的发射而导致的能量和角动量损失的影响外，还必须考虑线性动量的损失，这是系统质心反冲的原因。我们计算高阶尾（即，尾尾和尾平方）的贡献的线性动量通量的非自旋双星系统沿双曲线或椭圆形轨道。相应的轨道平均值在其领先的后牛顿近似下进行评估，使用调和坐标并在傅立叶域中工作。最后给出了沿双曲轨道的大偏心率（或大角动量）展开式和沿椭圆轨道的小偏心率展开式。因此，我们完成了先前的分析，重点是能量和角动量损失[Phys. Rev. D \textbf{104}，no.10，104020（2021）]，提供了有用的砖型结果，例如，用于高精度地确定经历散射过程的两个物体的辐射脉冲。
Quantum fluxes and $\langle\hatΦ^2\rangle$ for a non-minimally coupled scalar field: ringdown and tail on approaching the polar Kerr inner horizon
Technion（以色列理工学院）；Max Planck Institute for Mathematics in Sciences (MiS)（马克斯·普朗克科学促进研究所数学研究所）；Princeton University（普林斯顿大学）；Institut für Theoretische Physik, Universität Leipzig（莱比锡大学理论物理研究所）；University College Dublin（都柏林大学学院）；Centro Brasileiro de Pesquisas Físicas (CBPF)（巴西物理学研究中心）
Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN
Adiabatic evolution of asymmetric binaries on generic orbits with new fundamental fields I: characterization of gravitational wave fluxes
Gran Sasso Science Institute (GSSI)（格兰萨索科学研究所）；INFN, Laboratori Nazionali del Gran Sasso（意大利国家核物理研究所，格兰萨索国家实验室）；Dipartimento di Fisica, Sapienza Università di Roma（罗马智慧大学物理系）；Dipartimento di Fisica, Università di Pisa（比萨大学物理系）；INFN, Sezione di Roma（意大利国家核物理研究所罗马分部）；School of Mathematics and Statistics, University College Dublin（都柏林大学学院数学与统计学院）；INFN, Sezione di Pisa（意大利国家核物理研究所比萨分部）；School of Mathematical Sciences & School of Physics and Astronomy, University of Nottingham（诺丁汉大学数学科学学院与物理与天文学院）；Nottingham Centre of Gravity, University of Nottingham（诺丁汉大学引力研究中心）
Lorentz Covariant Supertranslation Frames for the Angular Momentum Aspect
School of Physics, Institute for Research in Fundamental Sciences (IPM)（基础科学研究所物理学院）；Center for Cosmology and Particle Physics, Department of Physics, New York University（纽约大学物理系宇宙学与粒子物理中心）
Waveforms and fluxes: Towards a self-consistent effective one body waveform model for nonprecessing, coalescing black-hole binaries for third generation detectors
Towards ultrarelativistic scattering near the light ring: asymptotic divergence of gravitational-wave fluxes
GReCO, Institut d’Astrophysique de Paris, UMR 7095, CNRS & Sorbonne Université（巴黎天体物理学研究所）；Centre national d’études spatiales (CNES)（法国国家空间研究中心）；School of Mathematical Sciences and STAG Research Centre, University of Southampton（南安普顿大学数学与STAG研究中心）；Queen Mary University of London（伦敦玛丽女王大学）
Conservative binary dynamics from gravitational tail emission processes
Universidade Federal do Rio Grande do Norte（北里奥格兰德联邦大学）；UNESP - Universidade Estadual Paulista（圣保罗州立大学）；Université de Genève（日内瓦大学）；ICTP South American Institute for Fundamental Research（国际理论物理研究所南美基础研究所）
Resummation of Universal Tails in Gravitational Waveforms
Center for Theoretical Physics, Massachusetts Institute of Technology（麻省理工学院理论物理中心）；The NSF AI Institute for Artificial Intelligence and Fundamental Interactions（美国国家科学基金会人工智能基础相互作用研究所）；Department of Physics, Princeton University（普林斯顿大学物理系）；Institut des Hautes Études Scientifiques（高等科学研究所）
