The motion of the charged particles in the field of rotating charged black holes and naked singularities. II - The motion in the equatorial plane

Article

The motion of the charged particles in the field of rotating charged black holes and naked singularities. II - The motion in the equatorial plane

Bálek, V.; Bičák, J.; Stuchlík, Z.

Bull. Astron. Inst. Czechosl. 40(0), 133-165 (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).

Keywords

BLACK HOLES (ASTRONOMY), CHARGED PARTICLES, PARTICLE MOTION, RELATIVISTIC PARTICLES, ANGULAR MOMENTUM, COMPUTATIONAL ASTROPHYSICS, ELECTROMAGNETIC FIELDS

Institute authors

Bičák, Jiří

BibTeX

@article{UTF248,
  author        = {Bálek, V. and Bičák, J. and Stuchlík, Z.},
  title         = {{The motion of the charged particles in the field of rotating charged black holes and naked singularities. II - The motion in the equatorial plane}},
  journal       = {Bull. Astron. Inst. Czechosl.},
  volume        = {40},
  number        = {0},
  pages         = {133-165},
  year          = {1989},
}