Non-perturbative correction on the black hole geometry
General Relativity and Quantum Cosmology
2024-03-14 v1 High Energy Astrophysical Phenomena
High Energy Physics - Theory
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.
Cite
@article{arxiv.2403.07972,
title = {Non-perturbative correction on the black hole geometry},
author = {Behnam Pourhassan and Hoda Farahani and Farideh Kazemian and İzzet Sakallı and Sudhaker Upadhyay and Dharm Veer Singh},
journal= {arXiv preprint arXiv:2403.07972},
year = {2024}
}
Comments
19 pages, 24 captioned figures, published in Physics of the Dark Universe