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Black Hole Solutions as Topological Thermodynamic Defects

Shao-Wen Wei, Yu-Xiao Liu, and Robert B. Mann
Phys. Rev. Lett. 129, 191101 – Published 31 October 2022

Abstract

In this Letter, employing the generalized off-shell free energy, we treat black hole solutions as defects in the thermodynamic parameter space. The results show that the positive and negative winding numbers corresponding to the defects indicate the local thermodynamical stable and unstable black hole solutions, respectively. The topological number defined as the sum of the winding numbers for all the black hole branches at an arbitrary given temperature is found to be a universal number independent of the black hole parameters. Moreover, this topological number only depends on the thermodynamic asymptotic behaviors of the black hole temperature at small and large black hole limits. Different black hole systems are characterized by three classes via this topological number. This number could help us in better understanding the black hole thermodynamics and, further, shed new light on the fundamental nature of quantum gravity.

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  • Received 12 August 2022
  • Accepted 10 October 2022

DOI:https://doi.org/10.1103/PhysRevLett.129.191101

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Shao-Wen Wei1,2,*, Yu-Xiao Liu1,2,†, and Robert B. Mann3,‡

  • 1Lanzhou Center for Theoretical Physics, Key Laboratory of Theoretical Physics of Gansu Province, School of Physical Science and Technology, Lanzhou University, Lanzhou 730000, People’s Republic of China
  • 2Institute of Theoretical Physics and Research Center of Gravitation, Lanzhou University, Lanzhou 730000, People’s Republic of China
  • 3Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada

  • *Corresponding author. weishw@lzu.edu.cn
  • Corresponding author. liuyx@lzu.edu.cn
  • Corresponding author. rbmann@uwaterloo.ca

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Issue

Vol. 129, Iss. 19 — 4 November 2022

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