J 2022

Shadow and massless particles around regular Bardeen black holes in 4D Einstein Gauss-Bonnet gravity

RAYIMBAEV, Javlon, Dilshodbek BARDIEV, Temurbek MIRZAEV, Ahmadjon ABDUJABBAROV, Akram KHALMIRZAEV et. al.

Basic information

Original name

Shadow and massless particles around regular Bardeen black holes in 4D Einstein Gauss-Bonnet gravity

Authors

RAYIMBAEV, Javlon, Dilshodbek BARDIEV (860 Uzbekistan, belonging to the institution), Temurbek MIRZAEV, Ahmadjon ABDUJABBAROV and Akram KHALMIRZAEV

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:

URL

RIV identification code

RIV/47813059:19630/22:A0000229

Organization unit

Institute of physics in Opava

DOI

http://dx.doi.org/10.1142/S0218271822500559

UT WoS

000807421800003

Keywords in English

Black holes; magnetic fields; magnetized particles; relativistic stars; orbits

Tags

, RIV23, SGS-12-2019

Tags

International impact, Reviewed
Změněno: 1/2/2023 13:18, Mgr. Pavlína Jalůvková

Abstract

V originále

In this paper, we study dynamics of massless (photon and neutrino-like) particles in the spacetime of regular Bardeen black hole (BH) in novel four-dimensional Einstein-Gauss-Bonnet (4D EGB) theory. First, we have analyzed the hor properties of the spacetime of the Bardeen BH with respect to the Gauss-Bonnet (GB) coupling parameter alpha. Our detailed analysis has shown that the GB coupling parameter is limited by maximum and minimum values at, alpha is an element of (-0.15 divided by 1) and the extreme value of magnetic charge of the BH depends on the parameter alpha. We have explored motion of neutrino-like particles and photons around the Bardeen BH. We have also explored the possibility of mimicking cases of the spin of Kerr BH and charge of Reissner-Nordstrom BH by the Bardeen charge, providing the same values of impact parameter for photons corresponding to the BH shadow size. Finally, we have investigated spherically infalling accretion and shadow of the Bardeen BHs in 4D EGB theory.
Displayed: 2/11/2024 22:08