Dymnikova Black Hole Surrounded by Quintessence

TL;DR

This paper studies a Dymnikova black hole surrounded by quintessence, analyzing its thermodynamics, geodesics, shadows, and quasinormal modes, revealing how quintessence influences stability, temperature, and observable properties.

Contribution

It introduces a detailed analysis of a Dymnikova black hole in a quintessential field, highlighting the effects on thermodynamics, light trajectories, shadows, and mode damping, which were not previously explored.

Findings

Quintessence modifies Hawking temperature and phase transitions.

Black hole shadows are sensitive to quintessence parameters.

Quintessence enhances damping of scalar quasinormal modes.

Abstract

The Dymnikova black hole (BH) is a regular solution that interpolates between a de Sitter core near the origin and a Schwarzschild-like behavior at large distances. In this work, we investigate the properties of a Dymnikova BH immersed in a quintessential field, characterized by the state parameter $\omega$ and a normalization constant $c$. We explore the thermodynamic behavior, null geodesics, scalar quasinormal modes and shadow profiles for this model. Our analysis shows that the presence of quintessence alters the Hawking temperature and specific heat, leading to parameter-dependent phase transitions. The null geodesics and corresponding black hole shadows are also found to be sensitive to the model parameters, especially $\omega$ and $c$. This sensitivity influences light deflection and shadow size. Furthermore, we compute the scalar quasinormal modes and observe that quintessence tends to enhance the damping of the modes, indicating greater stability under perturbations.