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

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.

Two columns, 8 pages, 4 figures, matches published version

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Cited by in corpus (4)

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• Telling tails and quasi-resonances in the vicinity of Dymnikova regular black hole
• Field Sources for $f(R,R_{\mu \nu })$ Black-Bounce Solutions: The Case of K-Gravity
• Gravitational quasinormal modes of Dymnikova black holes