Magnetized Black Hole as an Accelerator of Charged Particle

Astrophysical accretion processes near the black hole candidates, such as active galactic nuclei (AGN), X-ray binary (XRB), and other astrophysical sources, are associated with high-energetic emission of radiation relativistic particles outflows (winds or jets). It is widely believed that magnetic field plays a very important role to explain high energetic in vicinity those sources. In present research note, we propose embedded an asymptotically uniform field. We investigate dynamic motion charged weakly magnetized hole. show that, presence field, radius innermost stable circular orbits (ISCO) for particle located close hole’s horizon. The fundamental frequencies, Keplerian epicyclic frequencies split into two parts due analog Zeeman effect. orbital velocity measured by local observer has been computed external also analytical expression four-acceleration orbiting around holes. Finally, determine intensity radiating accelerating