Abstract
The analytical solutions for the quasi-Keplerian motion under the generally parameterized post-Newtonian force are derived in the Brumberg–Damour–Deruelle representation. The solutions are formulated in terms of the orbital energy and angular momentum. The achieved results can be applied to not only the motion of a test particle but also the relative motion of a binary system in a broad spectrum of gravitation theories.
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The authors would like to thank the anonymous reviewer for providing useful suggestions to promote the quality of this paper.
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This work was supported in part by the National Natural Science Foundation of China (Grant Nos. 11973025 and 11947404).
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Yang, B., Lin, W. Quasi-Keplerian motion under the generally parameterized post-Newtonian force. Gen Relativ Gravit 52, 49 (2020). https://doi.org/10.1007/s10714-020-02700-3
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DOI: https://doi.org/10.1007/s10714-020-02700-3