Thermodynamics and Quasinormal Modes of the Dymnikova Black Hole in Higher Dimensions
arXiv:2404.02818 · doi:10.1016/j.aop.2024.169833
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.
arXiv commentTwo columns, 8 pages, 4 figures, matches published version
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