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Thermodynamic Topology of Quantum RN Black Holes (2405.04541v2)

Published 25 Apr 2024 in physics.gen-ph

Abstract: This paper presents a comprehensive exploration of the thermodynamics of black holes, focusing on foundational concepts such as free energy, entropy, and topological numbers, alongside a detailed examination of quantum RN black holes. By extending the discussion to encompass the symmetry groups SO(2), SO(3)/SO(2), and SO(3) within the framework of (f(R)) gravity, the paper offers a nuanced understanding of black hole physics. Key insights include the pivotal role of free energy and entropy in understanding the thermodynamic properties of black holes, the significance of topological numbers in determining thermodynamic stability and phase transitions, and the implications of quantum mechanics and (f(R)) gravity on traditional thermodynamic concepts. This exploration not only enriches our theoretical knowledge of black holes but also sets the stage for future empirical investigations, marking a pivotal contribution to our ongoing quest to decipher the universe's mysteries.

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References (5)
  1. Wu, Shan-Ping and Shao-Wen Wei. “Thermodynamical Topology of Quantum BTZ Black Hole.”(2024). arXiv preprint arXiv:2403.14167.
  2. Chen, Wenxiang, Junxian Li, and Jingyi Zhang. “Calculating the Hawking Temperatures of Conventional Black Holes in the f (R) Gravity Models with the RVB Method.” arXiv preprint arXiv:2210.09062 (2022).
  3. Mihalis Dafermos and Jonathan Luk. The interior of dynamical vacuum black holes I: The C0superscript𝐶0C^{0}italic_C start_POSTSUPERSCRIPT 0 end_POSTSUPERSCRIPT-stability of the Kerr Cauchy horizon. 102017.
  4. Caravelli, Francesco, and Leonardo Modesto. “Holographic effective actions from black holes.” Physics Letters B 702.4 (2011): 307-311.
  5. Chen, Wen-Xiang. “Exploring the Dynamics of Mass Inflation: Implications for Cauchy Horizon Stability and Black Hole Physics in General Relativity and f⁢(R)𝑓𝑅f(R)italic_f ( italic_R ) Gravity.” arXiv preprint arXiv:2402.18097 (2024).
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