Thermodynamics and Quasinormal Modes of the Dymnikova Black Hole in Higher Dimensions

TL;DR

This paper explores the thermodynamics and quasinormal modes of higher-dimensional Dymnikova black holes, providing insights into their stability and characteristic oscillations within Einstein's theory.

Contribution

It introduces the analysis of thermodynamic properties and quasinormal modes of Dymnikova black holes in higher dimensions, extending previous work to a new class of solutions.

Findings

Thermodynamic parameters indicate stability regions.

Calculated quasinormal modes using WKB approximation.

Identified characteristic oscillation frequencies of the black holes.

Abstract

In this study, we investigate the thermodynamic properties and quasinormal modes of Dymnikova black holes within the context of higher dimensions in Einstein's general theory of relativity. We calculate the thermodynamic parameters, including the Hawking temperature and heat capacity, which allowed us to investigate the black hole's stability. Lastly the quasinormal modes with the WKB formula were calculated.