THE MOTION OF PARTICLES IN THE BOUND NON-GEODESIC ORBITS AROUND COMPACT GRAVITATING OBJECTS IMMERSED IN AN EXTERNAL MAGNETIC FIELD
Keywords:
Black hole, angular momentum, Kerr-Newman, energyAbstract
This paper analyzes the motion of particles in bound, i.e., confined, non-geodesic orbits in the presence of an external magnetic field around compact gravitational objects — in particular, neutron stars and black holes. The work studies the dynamical properties of particle trajectories formed as a result of the interaction of electromagnetic and gravitational forces. The influence of the magnetic field intensity and the mass and rotational speed of the compact object on the stability of the orbit is also considered. The results of the analysis are of great importance in understanding the role of charged particles in the formation of astrophysical disks, relic radiations or jets. This research serves to further deepen modern theoretical models in relativistic astrophysics and cosmic plasma dynamics.
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