Detailed Information on Publication Record
2020
Charged particle and epicyclic motions around 4D Einstein-Gauss-Bonnet black hole immersed in an external magnetic field
SHAYMATOV, Sanjar, Jaroslav VRBA, Daniele MALAFARINA, Bobomurat AHMEDOV, Zdeněk STUCHLÍK et. al.Basic information
Original name
Charged particle and epicyclic motions around 4D Einstein-Gauss-Bonnet black hole immersed in an external magnetic field
Authors
SHAYMATOV, Sanjar, Jaroslav VRBA (203 Czech Republic, belonging to the institution), Daniele MALAFARINA, Bobomurat AHMEDOV (860 Uzbekistan) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution)
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:
RIV identification code
RIV/47813059:19630/20:A0000057
Organization unit
Institute of physics in Opava
UT WoS
000595916100011
Keywords in English
Einstein-Gauss-Bonnet (EGB) black hole
Tags
International impact, Reviewed
Změněno: 26/4/2022 18:52, Mgr. Pavlína Jalůvková
Abstract
V originále
We investigate particle motion in the vicinity of a 4D Einstein-Gauss-Bonnet (EGB) black hole immersed in external asymptotically uniform magnetic field. It is well known that magnetic fields can strongly affect charged particle motion in the black hole vicinity due to the Lorenz force. We find that the presence of the Gauss-Bonnet (GB) coupling gives rise to a similar effect, reducing the radius of the innermost stable circular orbit (ISCO) with respect to the purely relativistic Schwarzschild black hole. Further, we consider particle collisions in the black hole vicinity to determine the center of mass energy and show that this energy increases with respect to the Schwarzschild case due to the effect of the GB term. Finally, we consider epicyclic motion and its frequencies and resonance as a mean to test the predictions of the model against astrophysical observations. In particular we test which values of the parameters of the theory best fit the 3:2 resonance of high-frequency quasi-periodic oscillations in three low-mass X-ray binaries.