Post-Keplerian motion in Reissner–Nordström spacetime

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成果类型：

期刊论文

作者：

Yang, Bo;Lin, Wenbin*

通讯作者：

Lin, Wenbin

作者机构：

[Lin, Wenbin; Yang, Bo] Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Sichuan, Peoples R China.

[Lin, Wenbin] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.

通讯机构：

[Lin, Wenbin] S

[Lin, Wenbin] U

Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Sichuan, Peoples R China.

Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.

语种：

英文

关键词：

(post-)Keplerian parameters;Post-Newtonian approximations;Reissner–Nordström spacetime

期刊：

General Relativity and Gravitation

ISSN：

0001-7701

年：

2019

卷：

期：

页码：

1-10

DOI：

10.1007/s10714-019-2597-z

基金类别：

We thank the reviewer for his/her constructive comments on promoting the quality of this paper. The author (W. Lin) would like to thank Prof. Remo Ruffini for inviting him to visit the ICRANet at Pescara where parts of this work were carried out. This research was supported in part by the National Natural Science Foundation of China (Grant Nos. 11647314 and 11847307).

机构署名：

本校为通讯机构

院系归属：

数理学院

摘要：

We present the analytical post-Newtonian solutions for the test particle’s motion in the Reissner–Nordström 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. © 2019, Springe...

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Post-Keplerian motion in Reissner–Nordström spacetime

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