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

Authors

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

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Issue

2018: Proceedings of the 36th Samahang Pisika ng Pilipinas Physics Conference

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.

Article ID

SPP-2018-PB-46

Section

Poster Session B (Complex Systems, Simulations, and Theoretical Physics)

Published

2018-05-29

How to Cite

[1]

MCT Perez and MFI 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://proceedings.spp-online.org/article/view/SPP-2018-PB-46.