Near?horizon structure of escape zones of electrically charged particles around weakly magnetized rotating black hole: Case of oblique magnetosphere

We study the effects of large scale magnetic fields on dynamics charged particles near a rotating black hole. consider scenario in which initially neutral geodesic orbits equatorial plane become ionized, and hence they are destabilized by charging process. Fraction then accelerated out follow jet like trajectories with relativistic velocities. explore non axisymmetric systems field is inclined respect to hole spin. system numerically order locate zones escaping compute terminal escape velocity. By breaking axial symmetry we notice increasing fraction unbound allow for acceleration ultrarelativistic