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The quasi-Keplerian motion in regular Bardeen spacetime

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成果类型:
期刊论文
作者:
Li, Jie;Yang, Bo;Wang, Yu;Lin, Wenbin
通讯作者:
Yang, B
作者机构:
[Lin, Wenbin; Li, Jie; Yang, Bo] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
[Yang, Bo] Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China.
[Wang, Yu] Univ Rome, ICRA Dip Fis, Ple Aldo Moro 5, I-00185 Rome, Italy.
[Wang, Yu] INAF Osservatorio Astron Abruzzo, Via M Maggini Snc, I-64100 Teramo, Italy.
通讯机构:
[Yang, B ] U
Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China.
Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China.
语种:
英文
关键词:
Bardeen black hole;Quasi-Keplerian motion;Post-Newtonian approximation;Perihelion precession
期刊:
General Relativity and Gravitation
ISSN:
0001-7701
年:
2023
卷:
55
期:
10
页码:
1-12
基金类别:
The authors would like to thank Prof. Remo Ruffini for helpful discussions. This work was supported in part by the National Natural Science Foundation of China (Grant Nos. 12247157, 12303079 and 11973025), and Scientific Research Fund of Hunan Provincial Education Department (Grant No. 22B0446). Thanks in part for the support of the postdoctoral program of purple Mountain Observatory, Chinese Academy of Sciences.
机构署名:
本校为第一且通讯机构
院系归属:
数理学院
摘要:
We present the second post-Newtonian solution for the quasi-Keplerian motion of a test particle in the gravitational field of Bardeen black hole. This solution is formulated in terms of energy and angular momentum of the particle, as well as the black hole’s magnetic charge. The leading effects of the magnetic charge on the test particle’s orbit and motion including perihelion precession are displayed explicitly. In particular, it is shown that the magnetic charge does not have effects on the orbital period when the second post-Newtonian orde...

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