Particle dynamics around an electrically charged Kiselev black hole embedded in quintessence

TL;DR

This paper introduces a new charged black hole solution in quintessence, analyzing charged particle orbits and periapsis shifts, revealing conditions for prograde and retrograde precession.

Contribution

It presents an electric generalization of the Kiselev black hole embedded in quintessence and studies charged particle dynamics around it.

Findings

Uncharged particles exhibit always prograde periapsis shifts.

Charged particles can have retrograde periapsis shifts under certain conditions.

The stability of circular orbits is analyzed in the new spacetime.

Abstract

We introduce and study a new solution describing a static, spherically symmetric and electrically charged black hole embedded in a charged quintessence fluid, which corresponds to an electric generalization of the Kiselev geometry. We derive the effective potential and analyze the various types of orbits followed by charged particles. A special attention is given to circular orbits and their stability. We found that for uncharged particles the periapsis shifts for bounded orbits is always prograde. However, for charged test particles the periapsis shifts can become retrograde in some cases.