The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation
We present the post-Newtonian solution for the quasi-Keplerian motion of a charged test particle in the field of Reissner-Nordström black hole under the Wagoner-Will-Epstein-Haugan representation. The explicit formulations for the charge effects on perihelion precession and the orbital period are ac...
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MDPI AG
2022-12-01
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Online Access: | https://www.mdpi.com/2073-8994/14/12/2661 |
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author | Bo Yang Chunhua Jiang Guansheng He Wenbin Lin |
author_facet | Bo Yang Chunhua Jiang Guansheng He Wenbin Lin |
author_sort | Bo Yang |
collection | DOAJ |
description | We present the post-Newtonian solution for the quasi-Keplerian motion of a charged test particle in the field of Reissner-Nordström 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. |
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issn | 2073-8994 |
language | English |
last_indexed | 2024-03-09T15:47:45Z |
publishDate | 2022-12-01 |
publisher | MDPI AG |
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series | Symmetry |
spelling | doaj.art-75ad6176b0d44b639ae3e2a7182bc4272023-11-24T18:20:58ZengMDPI AGSymmetry2073-89942022-12-011412266110.3390/sym14122661The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan RepresentationBo Yang0Chunhua Jiang1Guansheng He2Wenbin Lin3School of Mathematics and Physics, University of South China, Hengyang 421001, ChinaSchool of Mathematics and Physics, University of South China, Hengyang 421001, ChinaSchool of Mathematics and Physics, University of South China, Hengyang 421001, ChinaSchool of Mathematics and Physics, University of South China, Hengyang 421001, ChinaWe present the post-Newtonian solution for the quasi-Keplerian motion of a charged test particle in the field of Reissner-Nordström 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.https://www.mdpi.com/2073-8994/14/12/2661quasi-KeplerianReissner-Nordström spacetimepost-Newtonian approximation |
spellingShingle | Bo Yang Chunhua Jiang Guansheng He Wenbin Lin The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation Symmetry quasi-Keplerian Reissner-Nordström spacetime post-Newtonian approximation |
title | The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation |
title_full | The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation |
title_fullStr | The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation |
title_full_unstemmed | The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation |
title_short | The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordström Spacetime under the Wagoner-Will-Epstein-Haugan Representation |
title_sort | quasi keplerian motion of the charged test particle in reissner nordstrom spacetime under the wagoner will epstein haugan representation |
topic | quasi-Keplerian Reissner-Nordström spacetime post-Newtonian approximation |
url | https://www.mdpi.com/2073-8994/14/12/2661 |
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