Circular orbit frequencies of a charged particle around a weakly magnetized rotating black hole
Abstract
We investigate the orbital frequencies of circular non-geodesic orbits of a charged particle in the equatorial plane of a weakly magnetized Kerr black hole. For future-directed prograde orbits, isofrequency pairs of orbits with different radii are found to occur when the orbital motions of the charged particles are oppositely aligned to their azimuthal angular momentum L > 0. The number of isofrequency is numerically observed to increase with both the magnetic field parameter and black hole's spin.
Downloads
Issue
Building bridges and exploring frontiers
6-9 June 2018, Puerto Princesa City
Please visit the activity webpage for SPP2018 for more information on this year's conference.