Generalised Uncertainty Principle, Remnant Mass and Singularity Problem in Black Hole Thermodynamics
Rabin Banerjee, Sumit Ghosh

TL;DR
This paper introduces a new GUP consistent with string theory, analyzes its effects on black hole thermodynamics, and shows that black hole evaporation halts at a remnant mass, addressing the singularity issue.
Contribution
It derives a novel GUP and applies it to black hole thermodynamics, providing insights into remnant formation and singularity resolution.
Findings
Black hole evaporation stops at a finite remnant mass
Corrections to the mass-temperature relation are derived
The approach helps bypass the singularity problem in black hole physics
Abstract
We have derived a new Generalised Uncertainty Principle (GUP) based on certain general assumptions. This GUP is consistent with predictions from string theory. It is then used to study Schwarzschild black hole thermodynamics. Corrections to the mass-temperature relation, area law and heat capacity are obtained. We find that the evaporation process stops at a particular mass, referred as the remnant mass. This is instrumental in bypassing the well known singularity problem that occurs in a semiclassical approach.
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