The Quasi-Keplerian Motion of the Charged Test Particle in Reissner-Nordstrom Spacetime under the Wagoner-Will-Epstein-Haugan Representation

被引：2
作者：
Yang, Bo [1 ,2 ,3 ]
Jiang, Chunhua [1 ,2 ]
He, Guansheng [1 ,2 ]
Lin, Wenbin [1 ,2 ,4 ]
机构：
[1] Univ South China, Sch Math & Phys, Hengyang 421001, Peoples R China
[2] Hunan Key Lab Math Modeling & Sci Comp, Hengyang 421001, Peoples R China
[3] Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
[4] Southwest Jiaotong Univ, Sch Phys Sci & Technol, Chengdu 610031, Peoples R China
来源：
SYMMETRY-BASEL | 2022年 / 14卷 / 12期
基金：
中国国家自然科学基金;
关键词：
quasi-Keplerian; Reissner-Nordstrom spacetime; post-Newtonian approximation; BINARY; PULSAR; LIGHT; FIELD;
D O I：
10.3390/sym14122661
中图分类号：
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号：
07 ; 0710 ; 09 ;
摘要：
We present the post-Newtonian solution for the quasi-Keplerian motion of a charged test particle in the field of Reissner-Nordstrom 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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页数：9
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