Quasiperiodic Oscillations, Quasinormal Modes and Shadows of Bardeen-Kiselev Black Holes

TL;DR

This paper explores the properties, particle dynamics, oscillations, and shadows of Bardeen-Kiselev black holes, revealing how their unique features influence observable phenomena like QPOs and quasinormal modes.

Contribution

It provides a comprehensive analysis of Bardeen-Kiselev black holes, including their geometrical properties, particle orbits, oscillation frequencies, and shadow characteristics, which were not extensively studied before.

Findings

Degeneracy between Kerr spin and magnetic charge at specific parameters.

Relationship between shadow radius and quasinormal mode frequencies.

Analysis of quasiperiodic oscillations and innermost stable circular orbits.

Abstract

In this article, we study the particle dynamics around a static and spherically symmetric Bardeen-Kiselev black hole (BK BH) which is a solution of the Einstein-non-linear Maxwell field equations along with a quintessential field. We discuss its essential geometrical properties such as scalar invariants and size of innermost stable circular orbits. Dynamics of test particles around the BH is also studied. Moreover, we also computed the fundamental frequencies of a test particle orbiting the BH in a slightly perturbed orbit. Further, the degeneracy relations between the spin of rotating Kerr BH and magnetic charge of the BK BH at the values of the quintessential parameter $\omega_q=-1/3$ and in terms of the same values of innermost stable circular orbits (ISCOs) radius, energy efficiency, twin-peaks quasiperiodic oscillations (QPOs) frequencies and impact parameter for photon are also discussed in detail. Finally, we have investigated the relationship between the shadow radius and the real part of the quasinormal mode (QNM) frequency.