Detailed Information on Publication Record
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
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
Singapore
Confidentiality degree
není předmětem státního či obchodního tajemství
References:
RIV identification code
RIV/47813059:19630/22:A0000190
Organization unit
Institute of physics in Opava
UT WoS
000763026800010
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.
Změněno: 1/2/2023 13:26, Mgr. Pavlína Jalůvková
Abstract
V originále
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.