Reaction force of gravitational radiation in an effective-one-body theory based on the post-Minkowskian approximation

被引:0
|
作者
Sun, Manman [1 ,2 ]
Chen, Shuai [1 ,2 ]
He, Xiaokai [3 ]
Jing, Jiliang [1 ,2 ]
机构
[1] Hunan Normal Univ, Key Lab Low Dimens Quantum Struct & Quantum Contr, Minist Educ, Dept Phys, Changsha 410081, Hunan, Peoples R China
[2] Hunan Normal Univ, Synerget Innovat Ctr Quantum Effects & Applicat, Changsha 410081, Hunan, Peoples R China
[3] Hunan First Normal Univ, Sch Math & Computat Sci, Changsha 410205, Peoples R China
来源
EUROPEAN PHYSICAL JOURNAL C | 2021年 / 81卷 / 09期
基金
中国国家自然科学基金;
关键词
ROTATING BLACK-HOLE; CIRCULAR ORBIT; NEWTONIAN EXPANSION; GENERAL RELATIVITY; PARTICLE; WAVES; MOTION; PERTURBATIONS; EQUATIONS; FIELD;
D O I
10.1140/epjc/s10052-021-09626-3
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
Effective-one-body (EOB) theory based on the post-Newtonian (PN) approximation presented by Buonanno and Damour plays an important role in the analysis of gravitational wave signals. Based on the post-Minkowskian (PM) approximation, Damour introduced another novel EOB theory which will lead to theoretically improved versions of the EOB conservative dynamics and might be useful in the upcoming era of high signal-to-noise-ratio gravitational-wave observations. Using the 2PM effective metric obtained by us recently, in this paper we study the radiation reaction force experienced by the particle with the help of the energy-loss-rate, which is an important step to construct the EOB theory based on the PM approximation.
引用
收藏
页数:10
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