Impacts of Generalized Uncertainty Principle on Black Hole Thermodynamics and Salecker-Wigner Inequalities
A. Tawfik (MTI U., Cairo & Egyptian Ctr. Theor. Phys., Cairo & WLCAPP)

TL;DR
This paper explores how the Generalized Uncertainty Principle (GUP) influences black hole thermodynamics and lifetime, suggesting GUP prevents complete evaporation and implies the existence of black hole remnants.
Contribution
It introduces a GUP-based analysis of black hole thermodynamics and lifetime, highlighting the prevention of total evaporation and the potential for black hole remnants.
Findings
GUP prevents black hole from complete evaporation.
Black hole remnants are implied where specific heat vanishes.
Modified lifetime depends on black hole mass and GUP effects.
Abstract
We investigate the impacts of Generalized Uncertainty Principle (GUP) proposed by some approaches to quantum gravity such as String Theory and Doubly Special Relativity on black hole thermodynamics and Salecker-Wigner inequalities. Utilizing Heisenberg uncertainty principle, the Hawking temperature, Bekenstein entropy, specific heat, emission rate and decay time are calculated. As the evaporation entirely eats up the black hole mass, the specific heat vanishes and the temperature approaches infinity with an infinite radiation rate. It is found that the GUP approach prevents the black hole from the entire evaporation. It implies the existence of remnants at which the specific heat vanishes. The same role is played by the Heisenberg uncertainty principle in constructing the hydrogen atom. We discuss how the linear GUP approach solves the entire-evaporation-problem. Furthermore, the black…
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