J 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

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.