Non-perturbative correction on the black hole geometry

Abstract

In this paper, we use the holographic principle to obtain a modified metric of black holes that reproduces the exponentially corrected entropy. The exponential correction of the black hole entropy comes from non-perturbative corrections. It interprets as a quantum effect which affects black hole thermodynamics especially in the infinitesimal scales. Hence, it may affect black hole stability at the final stage. Then, we study modified thermodynamics due to the non-perturbative corrections and calculate thermodynamics quantities of several non-rotating black holes.

19 pages, 24 captioned figures, published in Physics of the Dark Universe

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Cited by in corpus (7)

• Thermodynamics of a newly constructed black hole coupled with nonlinear electrodynamics and cloud of strings
• Lorentz Symmetry Violation in Charged Black Hole Thermodynamics and Gravitational Lensing: Effects of the Kalb-Ramond Field
• Ayón--Beato--García black hole coupled with a cloud of strings: thermodynamics, shadows and quasinormal modes
• Thermodynamics of Einstein-Euler-Heisenberg Black Holes with Thermal Fluctuations and Nonlinear Electromagnetic Fields
• Black Holes in Lorentz-Violating Gravity: Thermodynamics, Geometry, and Particle Dynamics
• Exploring non-perturbative effects on quasi-topological black hole thermodynamics
• Phantom BTZ Black Holes: Thermal Properties Under Perturbative Corrections