Circular orbit frequencies of a charged particle around a weakly magnetized rotating black hole

  • Marc Christian Tolentino Perez National Institute of Physics, University of the Philippines Diliman
  • Michael Francis Ian Vega, II National Institute of Physics, University of the Philippines Diliman

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.

Published
2018-05-29
How to Cite
[1]
M. C. Perez and M. F. I. Vega. Circular orbit frequencies of a charged particle around a weakly magnetized rotating black hole, Proceedings of the Samahang Pisika ng Pilipinas 36, SPP-2018-PB-46 (2018). URL: https://paperview.spp-online.org/proceedings/article/view/SPP-2018-PB-46.
Section
Poster Session B (Complex Systems, Simulations, and Theoretical Physics)