Quantum corrected thermodynamics of nonlinearly charged BTZ black holes in massive gravity's rainbow
arXiv:2111.06935 · doi:10.1142/S0217732321501583
Abstract
In this paper, we consider three-dimensional massive gravity's rainbow and obtain black hole solutions in three different cases of Born-Infeld, logarithmic, and exponential theories of nonlinear electrodynamics. We discuss the horizon structure and geometrical properties. Then, we study thermodynamics of these models by considering the first-order quantum correction effects, which appears as a logarithmic term in the black hole entropy. We discuss such effects on the black hole stability and phase transitions. We find that, due to the quantum corrections, the second-order phase transition happens in Born-Infeld and logarithmic models. We obtain the modified first law of black hole thermodynamics in the presence of logarithmic corrections.
19 pages, 8 figures
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- Thermodynamics of Einstein-Euler-Heisenberg Black Holes with Thermal Fluctuations and Nonlinear Electromagnetic Fields
- Three-dimensional energy-dependent -metric: black hole solutions
- Strong gravitational lensing by black hole in F(R) Euler Heisenberg Gravity's Rainbow