Post-Keplerian motion in Reissner-Nordstrom spacetime

被引：8
|
作者：
Yang, Bo [1 ]
Lin, Wenbin [1 ,2 ]
机构：
[1] Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Sichuan, Peoples R China
[2] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China
来源：
GENERAL RELATIVITY AND GRAVITATION | 2019年 / 51卷 / 09期
基金：
中国国家自然科学基金;
关键词：
Post-Newtonian approximations; (post-)Keplerian parameters; Reissner-Nordstrom spacetime; GRAVITATIONAL-RADIATION; NEWTONIAN MOTION; BINARY-SYSTEMS; ORBITS; PULSAR; WAVES;
D O I：
10.1007/s10714-019-2597-z
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the analytical post-Newtonian solutions for the test particle's motion in the Reissner-Nordstrom spacetime. The solutions are formulated in the Wagoner-Will representation, the Epstein-Haugan representation, the Brumberg representation, and the Damour-Deruelle representation, respectively. The relations between the (post-)Keplerian parameters in different representations, as well as their relations to the orbital energy and angular momentum are also provided.
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页数：10
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