Effect of the inner horizon on the black hole thermodynamics: Reissner–Nordström black hole and Kerr black hole

DOI10.1142/S0217732321501777zbMath1487.83105arXiv2107.11193OpenAlexW3192490012MaRDI QIDQ5067278

G. E. Volovik

Publication date: 1 April 2022

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2107.11193

zbMATH Keywords

entropyHawking radiationblack holeinner horizon

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Measures of information, entropy (94A17) Stochastic integral equations (60H20)

Related Items (3)

Thermodynamics of multi-horizon spacetimes ⋮ Hawking temperature of black holes with multiple horizons ⋮ Replica trick calculation for entanglement entropy of static black hole spacetimes

Cites Work

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• On the Kerr quantum area spectrum
• Universal Area Product Formulas for Rotating and Charged Black Holes in Four and Higher Dimensions
• Evaporating black-to-white hole
• Singularities in Reissner–Nordström black holes
• Hawking Radiation As Tunneling

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