Dynamics of Magnetized Black Holes in Anisotropic Matter Fields
Munisa Boltatoshova
1,*
,
Bakhtiyor Narzilloev
2
,
Ahmadjon Abdujabbarov
3,4,5
,
Bobomurat Ahmedov
1,2,3
1 Institute of Theoretical Physics, National University of Uzbekistan , Tashkent 100174, Uzbekistan
2 Institute for Advanced Studies, New Uzbekistan University , Movarounnahr str. 1, Tashkent 100000, Uzbekistan
3 School of Physics, Harbin Institute of Technology , Harbin 150001, People’s Republic of China
4 Tashkent State Technical University , Tashkent 100095, Uzbekistan
5 Institute of Nuclear Physics , Ulugbek 1, Tashkent 100214, Uzbekistan
Abstract
We study the dynamics of charged test particles around magnetized black holes with anisotropic matter fields. Using the Cho-Kim solution, we analyze the effects of the anisotropy parameter K, the state parameter ω, and an external magnetic field on the effective potential, orbital stability, and the innermost stable circular orbit (ISCO). Our results show that anisotropy shifts the ISCO outward, while magnetic coupling allows stable orbits closer to the horizon. The combined influence of anisotropy and magnetization reproduces Kerr-like orbital features, suggesting that such black holes may act as Kerr mimickers with observable astrophysical signatures.
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Cite this article
Boltatoshova, M., Narzilloev, B., Abdujabbarov, A. and Ahmedov, B., Dynamics of Magnetized Black Holes in Anisotropic Matter Fields, Turanian J. Vol. 1, No. 4 (010402), 2025