{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,12]],"date-time":"2025-10-12T01:39:13Z","timestamp":1760233153107,"version":"build-2065373602"},"reference-count":54,"publisher":"MDPI AG","issue":"12","license":[{"start":{"date-parts":[[2022,12,16]],"date-time":"2022-12-16T00:00:00Z","timestamp":1671148800000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0\/"}],"funder":[{"name":"National Natural Science Foundation of China","award":["12247157","11973025","12147208"],"award-info":[{"award-number":["12247157","11973025","12147208"]}]}],"content-domain":{"domain":[],"crossmark-restriction":false},"short-container-title":["Symmetry"],"abstract":"<jats:p>We present the post-Newtonian solution for the quasi-Keplerian motion of a charged test particle in the field of Reissner-Nordstr\u00f6m black hole under the Wagoner-Will-Epstein-Haugan representation. The explicit formulations for the charge effects on perihelion precession and the orbital period are achieved, which may be useful not only in the comparisons with astronomical observations but also in calculating the waveform of the gravitational wave from this kind of system.<\/jats:p>","DOI":"10.3390\/sym14122661","type":"journal-article","created":{"date-parts":[[2022,12,16]],"date-time":"2022-12-16T02:16:41Z","timestamp":1671157001000},"page":"2661","update-policy":"https:\/\/doi.org\/10.3390\/mdpi_crossmark_policy","source":"Crossref","is-referenced-by-count":2,"title":["The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordstr\u00f6m Spacetime under the Wagoner-Will-Epstein-Haugan Representation"],"prefix":"10.3390","volume":"14","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-7912-496X","authenticated-orcid":false,"given":"Bo","family":"Yang","sequence":"first","affiliation":[{"name":"School of Mathematics and Physics, University of South China, Hengyang 421001, China"},{"name":"Hunan Key Laboratory of Mathematical Modeling and Scientific Computing, Hengyang 421001, China"},{"name":"Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China"}]},{"given":"Chunhua","family":"Jiang","sequence":"additional","affiliation":[{"name":"School of Mathematics and Physics, University of South China, Hengyang 421001, China"},{"name":"Hunan Key Laboratory of Mathematical Modeling and Scientific Computing, Hengyang 421001, China"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-6145-0449","authenticated-orcid":false,"given":"Guansheng","family":"He","sequence":"additional","affiliation":[{"name":"School of Mathematics and Physics, University of South China, Hengyang 421001, China"},{"name":"Hunan Key Laboratory of Mathematical Modeling and Scientific Computing, Hengyang 421001, China"}]},{"given":"Wenbin","family":"Lin","sequence":"additional","affiliation":[{"name":"School of Mathematics and Physics, University of South China, Hengyang 421001, China"},{"name":"Hunan Key Laboratory of Mathematical Modeling and Scientific Computing, Hengyang 421001, China"},{"name":"School of Physical Science and Technology, Southwest Jiaotong University, Chengdu 610031, China"}]}],"member":"1968","published-online":{"date-parts":[[2022,12,16]]},"reference":[{"key":"ref_1","unstructured":"Weinberg, S. 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