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Charged Particles Orbiting a Magnetized Black Hole Immersed in Quintessential Matter

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arxiv 2405.14420 v3 pith:5XVST7AL submitted 2024-05-23 gr-qc

Vitalie Lungu , Marina-Aura Dariescu , Cristian Stelea This is my paper · ORCID
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keywords blackchargedcircularfieldholeimmersedmagneticmagnetized
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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.

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  1. Magnetising de Sitter and Anti-de Sitter spacetimes

    gr-qc 2026-07 conditional novelty 5.5 of 10

    A Harrison-type map plus fluid rescaling produces spherical Melvin analogues of dS and AdS that reduce to ordinary (A)dS when the magnetic field vanishes.

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