Publication date: Jun 1989
Abstract:
The motion in the equatorial plane is discussed in three cases which
exhibit well the interaction of charged particles and Kerr-Newman black
holes. These are: (1) the circular orbits of ultrarelativistic particles
with high specific charge; (2) the motion of charged particles with zero
angular momentum (where the interplay between the gravitational and
magnetic dragging can be seen in the simplest form); and (3) the motion
of charged particles with l = a x gamma (including all particles that
can hit the ring singularity and also the cases when the trajectories
can be given in terms of elementary functions).
Authors:
Balek, Vladimir; Bicak, Jiri; Stuchlik, Zdenek;