2022
			
	    
	
	
    Distinguishable feature of electric and magnetic charged black hole Acceleration of charged particle in Reissner-Nordstrom spacetime
TURIMOV, Bobur; Madina BOBOQAMBAROVA; Bobomurat AHMEDOV and Zdeněk STUCHLÍKBasic 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
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
		References:
Impact factor
Impact factor: 3.400
			RIV identification code
RIV/47813059:19630/22:A0000223
		Organization unit
Institute of physics in Opava
			UT WoS
000753876000001
		EID Scopus
2-s2.0-85124911714
		Keywords in English
Reissner-Nordstrom black holes; charged test particles;Keplerian and Larmor frequencies
		Tags
International impact, Reviewed
		
				
				Changed: 1/2/2023 10:45, Mgr. Pavlína Jalůvková
				
		Abstract
In the original language
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.