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Thermodynamics and Quasinormal Modes of the Dymnikova Black Hole in Higher Dimensions
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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.
Forward citations
Cited by 3 Pith papers
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Null geodesics, causal structure, and matter accretion in Lorentzian-Euclidean black holes
In the Lorentzian-Euclidean black hole, photons and massive particles are claimed to be unable to cross the event horizon, making the spacetime geodesically complete and avoiding the central singularity.
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Dymnikova Black Hole Tidal Forces
In the Dymnikova regular black hole, both radial and angular tidal forces remain finite and change sign inside the horizons, and freely falling dust turns around before reaching the regular center.
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Bonanno-Reuter regular black hole: quasi-resonances, grey-body factors and absorption cross-sections of a massive scalar field
Damping of massive scalar quasinormal modes decreases with field mass in the Bonanno-Reuter black hole, and grey-body factors shift to higher frequencies.
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