On Thermodynamics of Kerr Black Hole-Reference-Cited by-同舟云学术

On Thermodynamics of Kerr Black Hole

Published:2023-06-21 Issue:8 Volume:535 Page:
ISSN:0003-3804
Container-title:Annalen der Physik
language:en
Short-container-title:Annalen der Physik

Author:

Ulhoa Sérgio Costa¹²,dos Santos Alesandro Ferreira³^ORCID,Spaniol Ednardo Paulo⁴⁵,Khanna Faqir Chand⁶

Affiliation:

1. International Center of Physics Instituto de Física Universidade de Brasília Brasília Distrito Federal 70910‐900 Brazil

2. Canadian Quantum Research Center 204‐3002 32 Ave Vernon BC V1T 2L7 Canada

3. Instituto de Física Universidade Federal de Mato Grosso Cuiabá Mato Grosso 78060‐900 Brazil

4. Centro Universitário de Brasília UniCEUB Brasília DF 70790‐075 Brazil

5. UDF Centro Universitário and Centro Universitário de Brasília UniCEUB Brasília DF 70390‐045 Brazil

6. Department of Physics and Astronomy University of Victoria 3800 Finnerty Road Victoria Victoria British Columbia V8P 5C2 Canada

Abstract

AbstractThe gravitational Stefan–Boltzmann law is considered for the Kerr black hole in the weak‐field limit. The energy‐momentum tensor predicted by teleparallelism equivalent to general relativity is used in the thermo field dynamics formalism to thermalize the field. A temperature‐dependent gravitational pressure is obtained. Regions of divergent heat capacity are observed. According to Landau theory, it allows the existence of distinct phases around the Kerr black hole.

Publisher

Wiley

Subject

General Physics and Astronomy

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1002/andp.202300173

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