Abstract
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 order is considered.
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Acknowledgements
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.
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J. Li and B. Yang did the calculations. Y. Wang and W. Lin checked the calculation results. All authors participated in writing the manuscript text. The revisions were mainly done by B. Yang.
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Li, J., Yang, B., Wang, Y. et al. The quasi-Keplerian motion in regular Bardeen spacetime. Gen Relativ Gravit 55, 114 (2023). https://doi.org/10.1007/s10714-023-03166-9
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DOI: https://doi.org/10.1007/s10714-023-03166-9