Charged particle and epicyclic motions around 4D Einstein-Gauss-Bonnet black hole immersed in an external magnetic field

被引:51
|
作者
Shaymatov, Sanjar [1 ,2 ,3 ,4 ]
Vrba, Jaroslav [5 ]
Malafarina, Daniele [6 ]
Ahmedov, Bobomurat [2 ,3 ,4 ]
Stuchlik, Zdenek [5 ]
机构
[1] Zheijiang Univ Technol, Inst Theoret Phys & Cosmol, Hangzhou 310023, Peoples R China
[2] Ulugh Beg Astron Inst, Astron St 33, Tashkent 100052, Uzbekistan
[3] Natl Univ Uzbekistan, Tashkent 100174, Uzbekistan
[4] Tashkent Inst Irrigat & Agr Mechanizat Engineers, Kori Niyoziy 39, Tashkent 100000, Uzbekistan
[5] Silesian Univ Opava, Inst Phys Opava, Res Ctr Theoret Phys & Astrophys, Bezrucovo Namesti 13, CZ-74601 Opava, Czech Republic
[6] Nazarbayev Univ, Dept Phys, Kabanbay Batyr 53, Nur Sultan 010000, Kazakhstan
来源
关键词
QUASI-PERIODIC OSCILLATIONS; GRAVITATIONAL COLLAPSE; ELECTROMAGNETIC-FIELDS; ORBITAL RESONANCE; NEUTRON-STAR; MODEL; GRAVITY; ACCELERATION; ENERGETICS; SIGNATURE;
D O I
10.1016/j.dark.2020.100648
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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. (c) 2020 Elsevier B.V. All rights reserved.
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页数:10
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