Distinguishable feature of electric and magnetic charged black hole Acceleration of charged particle in Reissner–Nordström spacetime

Obviously, from the geometrical point of view, it is impossible to distinguish the electrically and magnetically charged Reissner–Nordström black holes. One way of describing the differences between these solutions is to study the dynamical motion of charged test particles in the vicinity of the cha...

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Bibliographic Details
Published inEuropean physical journal plus Vol. 137; no. 2
Main Authors Turimov, Bobur, Boboqambarova, Madina, Ahmedov, Bobomurat, Stuchlík, Zdeněk
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 10.02.2022
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Summary:Obviously, from the geometrical point of view, it is impossible to distinguish the electrically and magnetically charged Reissner–Nordström black holes. One way of describing the differences between these solutions is to study the dynamical motion of charged test particles in the vicinity of the charged black hole and explore the effects of the charge coupling parameters ( σ e , σ m ) on the instability of the circular orbits. On the other hand, it is also possible to investigate the fundamental frequencies, such as Keplerian, Larmor, and epicyclic frequencies of charged particles orbiting around a charged black hole. Lastly, we investigate the synchrotron radiation by charged particles accelerated by charged black hole and estimate the intensity of relativistic radiating charged particles. Finally, we comment on the possible utilization of our findings for the relativistic jets and magneto-hydrodynamical outflows.
ISSN:2190-5444
2190-5444
DOI:10.1140/epjp/s13360-022-02390-7