2022
			
	    
	
	
    Quasi-periodic oscillation around regular Bardeen black holes in 4D Einstein-Gauss-Bonnet gravity
RAYIMBAEV, Javlon; Dilshodbek BARDIEV; Ahmadjon ABDUJABBAROV; Yunus TURAEV; Zdeněk STUCHLÍK et. al.Basic information
Original name
Quasi-periodic oscillation around regular Bardeen black holes in 4D Einstein-Gauss-Bonnet gravity
	Authors
RAYIMBAEV, Javlon; Dilshodbek BARDIEV (860 Uzbekistan, belonging to the institution); Ahmadjon ABDUJABBAROV; Yunus TURAEV and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution)
			Edition
 International Journal of Modern Physics D, 2022, 0218-2718
			Other information
Language
English
		Type of outcome
Article in a journal
		Field of Study
10308 Astronomy
		Country of publisher
Singapore
		Confidentiality degree
is not subject to a state or trade secret
		References:
Impact factor
Impact factor: 2.200
			RIV identification code
RIV/47813059:19630/22:A0000190
		Organization unit
Institute of physics in Opava
			UT WoS
000763026800010
		EID Scopus
2-s2.0-85126610871
		Keywords in English
Modified gravity; quasi-periodic oscillations; Einstein Gauss Bonnet; regular black holes; nonlinear electrodynamics
		Tags
Tags
International impact, Reviewed
		Links
GA19-03950S, research and development project. 
			
				
				Changed: 1/2/2023 13:26, Mgr. Pavlína Jalůvková
				
		Abstract
In the original language
In this paper, we explore the dynamics of test particles in spacetime around regular Bardeen black holes (BHs) in the novel four-dimensional Einstein-Gauss-Bonnet (4D EGB) theory. First, we analyze properties of the spacetime around the Bardeen BH with respect to the Gauss-Bonnet (GB) coupling parameter a, and we show the range of values of the BH charge and the parameter a that horizon exists as alpha/M-2 is an element of (-0.15869, 1) and g/M is an element of (0,0.886247), respectively. We also investigate the effects of the magnetic charge of the regular BH on innermost stable circular orbits (ISCOs) radius and efficiency of energy release from infalling test particles to the regular Bardeen BH in 4D EGB gravity. Moreover, fundamental frequencies such as Keplerian and harmonic oscillations are also studied with the applications of quasi-periodic oscillations (QP0s) where we proposed a method to test gravity theories through data from astrophysical observations of twin-peak QPOs in relativistic precession (RP) model. Finally, we show the dependence of the distance from the central BH to the orbit where twin-peak QPOs shine from the spin of Kerr BH, magnetic charge of Bardeen and Reissner-Nordstrom (RN) BHs, and GB coupling parameter.