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Magnetized Particle Motion in γ-Spacetime in a Magnetic Field

Ahmadjon AbdujabbarovInstitute of Nuclear Physics, Ulughbek, Tashkent 100214, UzbekistanJavlon RayimbaevInstitute of Nuclear Physics, Ulughbek, Tashkent 100214, UzbekistanFarruh AtamurotovSchool of Computer and Information Engineering, Inha University in Tashkent, Tashkent 100170, UzbekistanBobomurat AhmedovPhysics Faculty, National University of Uzbekistan, Tashkent 100174, Uzbekistan
Galaxiesjournal2020en
ABI

Аннотация

In the present work we explored the dynamics of magnetized particles around the compact object in γ-spacetime in the presence of an external asymptotically-uniform magnetic field. The analysis of the circular orbits of magnetized particles around the compact object in the spacetime of a γ-object immersed in the external magnetic field has shown that the area of stable circular orbits of magnetized particles increases with the increase of γ-parameter. We have also investigated the acceleration of the magnetized particles near the γ-object and shown that the center-of-mass energy of colliding magnetized particles increases with the increase of γ-parameter. Finally, we have applied the obtained results to the astrophysical scenario and shown that the values of γ-parameter in the range of γ∈(0.5,1) can mimic the spin of Kerr black hole up to a≃0.85, while the magnetic interaction can mimic the γ-parameter at γ∈(0.8,1) and spin of a Kerr black hole up to a≃0.3.

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