Phase portraits for the motion of charged particles around a weakly magnetized rotating black hole
Abstract
We study the phase portraits of a charged particle orbiting around a weakly magnetized Kerr black hole. For prograde orbits in anti-Larmor motion, the center-saddle coalescence point approaches the event horizon as the spin a < 1/2 increases. For spin 1/2 ≤ a < 1, the coalescence point moves away from the horizon. Bound orbits are observed in the phase portraits having center and saddle fixed points which exist for b less than the coalescence point {rc, bc}.
Downloads
Published
Issue
Section
License
By submitting their manuscript to the Samahang Pisika ng Pilipinas (SPP) for consideration, the Authors warrant that their work is original, does not infringe on existing copyrights, and is not under active consideration for publication elsewhere.
Upon acceptance of their manuscript, the Authors further agree to grant SPP the non-exclusive, worldwide, and royalty-free rights to record, edit, copy, reproduce, publish, distribute, and use all or part of the manuscript for any purpose, in any media now existing or developed in the future, either individually or as part of a collection.
All other associated economic and moral rights as granted by the Intellectual Property Code of the Philippines are maintained by the Authors.
