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Thermodynamic geometric analysis of conventional black holes under f(R) gravity

2021/12/13 by Wen-Xiang Chen, Chen, Wen-Xiang, Y. G. Zheng +3
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc)

paper · pdf · doi:10.48550/arxiv.2112.06718

openalex publication_date 2021/12/13 · openalex created_date 2022/07/19 · openalex updated_date 2026/07/28

Abstract

In this article, we consider a conventional black hole under f(R) gravity. Due to the small fluctuations around the equilibrium state, we have summarized the expression of the modified thermodynamic entropy of this black hole. At the same time, we also studied the geometric thermodynamics (GTD) of black holes, and studied the adaptability of the curvature scalar of the geometric thermodynamics method to the phase transition point of the black hole. In addition, we also studied the influence of the modified parameters on the thermodynamic behavior of black holes.

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