The Motion of the Charged Particles in the Field of Rotating Charged Black Holes and Naked Singularities. II. The Motion in the Equatorial Plane
Abstract
The motion in the equatorial plane is discussed in three cases which exhibit well the interaction of charged particles and KerrNewman 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).
 Publication:

Bulletin of the Astronomical Institutes of Czechoslovakia
 Pub Date:
 June 1989
 Bibcode:
 1989BAICz..40..133B
 Keywords:

 Black Holes (Astronomy);
 Charged Particles;
 Particle Motion;
 Relativistic Particles;
 Angular Momentum;
 Computational Astrophysics;
 Electromagnetic Fields;
 Astrophysics