J 2020

Dynamics of magnetized particles around 4-D Einstein Gauss-Bonnet black hole

ABDUJABBAROV, Ahmadjon, Javlon RAYIMBAEV, Bobur TURIMOV and Farruh ATAMUROTOV

Basic information

Original name

Dynamics of magnetized particles around 4-D Einstein Gauss-Bonnet black hole

Authors

ABDUJABBAROV, Ahmadjon (860 Uzbekistan), Javlon RAYIMBAEV, Bobur TURIMOV (860 Uzbekistan, belonging to the institution) and Farruh ATAMUROTOV

Edition

Physics of the Dark Universe, 2020, 2212-6864

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10308 Astronomy

Country of publisher

Netherlands

Confidentiality degree

není předmětem státního či obchodního tajemství

References:

URL

RIV identification code

RIV/47813059:19630/20:A0000056

Organization unit

Institute of physics in Opava

DOI

http://dx.doi.org/10.1016/j.dark.2020.100715

UT WoS

000595916100036

Keywords in English

Einstein Gauss-Bonnet gravity; Magnetized particles; Magnetic field; Center-of-mass energy

Tags

, FÚ2020, RIV21, SGS12-2019, UF

Tags

International impact, Reviewed
Změněno: 22/4/2021 14:12, RNDr. Jan Hladík, Ph.D.

Abstract

V originále

In this paper, we have investigated the dynamics of magnetized particles around 4-D Einstein Gauss-Bonnet black hole immersed in an external asymptotically uniform magnetic field. We have shown that the magnetic interaction parameter responsible for circular orbits decreases for negative values of the Gauss-Bonnet parameter alpha and the range where magnetized particle's stable circular orbits are allowed increases for the positive values of the parameter alpha. The study of the collisions of magnetized, charged and neutral particles has shown that the center-of-mass energy of the particles increases in the presence of positive Gauss-Bonnet parameter. Finally, we show how the magnetic interaction and Gauss-Bonnet parameter may mimic the effect of rotation of the Kerr black hole giving the same ISCO radius for magnetized particles. Detailed analysis of the ISCO show that spin of Kerr black hole cannot be mimicked by the effects of magnetic interaction and the Gauss-Bonnet parameters when alpha < -4.37 and the spin parameter a > 0.237.
Displayed: 24/12/2024 03:32