Thermodynamics of de Sitter black hole in massive gravity
Yu-Bo Ma, Ren Zhao, Shuo Cao

TL;DR
This paper explores the thermodynamic properties of de Sitter black holes in massive gravity, revealing universal entropy characteristics and emphasizing the importance of thermodynamic quantities in stability analysis.
Contribution
It introduces a thermodynamic framework for de Sitter black holes in massive gravity and demonstrates the universal form of entropy similar to Reissner-Nordstrom-de Sitter space.
Findings
Entropy matches that of Reissner-Nordstrom-de Sitter space
Thermodynamic quantities influence stability and evolution
Provides a foundation for understanding de Sitter thermodynamics
Abstract
In this paper, by taking de Sitter space-time as a thermodynamic system, we study the equivalent thermodynamic quantities of de Sitter black hole in massive gravity, and furthermore obtain the equivalent thermodynamic quantities of the space-time. Our results show that the entropy of this type of space-time takes the same form as that in Reissner-Nordstrom-de Sitter space-time, which lays a solid foundation for deeply understanding the universal thermodynamic characteristics of de Sitter space-time in the future. Moreover, our analysis indicates that the equivalent thermodynamic quantities and relevant parameters play a very important role, especially in the investigation of the stability and evolution of de Sitter space-time.
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