TURIMOV, Bobur, Madina BOBOQAMBAROVA, Bobomurat AHMEDOV and Zdeněk STUCHLÍK. Distinguishable feature of electric and magnetic charged black hole Acceleration of charged particle in Reissner-Nordstrom spacetime. European Physical Journal Plus. DE - Spolková republika Německo, 2022, vol. 137, No 2, p. "222-1"-"222-11", 11 pp. ISSN 2190-5444. Available from: https://dx.doi.org/10.1140/epjp/s13360-022-02390-7.
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Basic information
Original name Distinguishable feature of electric and magnetic charged black hole Acceleration of charged particle in Reissner-Nordstrom spacetime
Authors TURIMOV, Bobur, Madina BOBOQAMBAROVA, Bobomurat AHMEDOV (860 Uzbekistan) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition European Physical Journal Plus, DE - Spolková republika Německo, 2022, 2190-5444.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Germany
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/22:A0000223
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1140/epjp/s13360-022-02390-7
UT WoS 000753876000001
Keywords in English Reissner-Nordstrom black holes; charged test particles;Keplerian and Larmor frequencies
Tags , RIV23
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 1/2/2023 10:45.
Abstract
Obviously, from the geometrical point of view, it is impossible to distinguish the electrically and magnetically charged Reissner-Nordstrom 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 (sigma(e), sigma(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.
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