Thermodynamic geometry of black holes in f(R) gravity
Abstract
In this paper, we consider three types (static, static charged and rotating charged) of black holes in f(R) gravity. We study the thermodynamical behavior, stability conditions and phase transition of these black holes. It will be shown that, the number and type of phase transition points are related to different parameters, which shows the dependency of stability conditions to these parameters. Also, we extended our study to different thermodynamic geometry methods (Ruppeiner, Weinhold and GTD). Next, we investigate the compatibility of curvature scalar of geothermodynamic methods with phase transition points of the above balck holes. In addition, we point out the effect of different values of spacetime parameters on stability conditions of mentioned black holes.
Keywords
Cite
@article{arxiv.1605.00767,
title = {Thermodynamic geometry of black holes in f(R) gravity},
author = {Saheb Soroushfar and Reza Saffari and Negin Kamvar},
journal= {arXiv preprint arXiv:1605.00767},
year = {2016}
}
Comments
45 figures,35 pages