Charged Particles Orbiting a Magnetized Black Hole Immersed in Quintessential Matter
Vitalie Lungu, Marina-Aura Dariescu, Cristian Stelea

TL;DR
This paper introduces an exact solution for a magnetized black hole in quintessence, analyzing charged particle dynamics and trajectories near stable orbits using perturbative methods.
Contribution
It presents a new exact magnetized black hole solution in quintessence and studies charged particle motion, including approximate solutions for perturbed circular orbits.
Findings
Different types of particle trajectories are discussed.
Perturbative analysis of small oscillations near stable orbits.
Trajectory shape depends on gravitational and quintessence forces.
Abstract
A new exact magnetized solution describing a Kiselev black hole immersed in a magnetic field is used for studying the dynamics of charged particles. Different types of trajectories are discussed. In the particular case of a weak magnetic field, we employ a first-order perturbative approach to analyze the perturbed circular orbits near the minimum of the effective potential. We obtain an approximate solution for the bounded equatorial trajectory subjected to small radial and latitudinal oscillations. The shape of the trajectory localized near the stable circular orbit depends on the relation between the attractive gravitational force and the repulsive quintessence contribution.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsExperimental and Theoretical Physics Studies · Astrophysical Phenomena and Observations · Relativity and Gravitational Theory
