Classical corrections to black hole entropy in $d$ dimensions: a rear window to quantum gravity?
Martin Blaschke, Zden\v{e}k Stuchl\'ik, Filip Blaschke, Petr, Blaschke

TL;DR
This paper derives logarithmic corrections to black hole entropy in arbitrary dimensions using a classical, non-calculus approach, suggesting potential insights into quantum gravity without detailed quantum theories.
Contribution
It presents a simple, calculus-free derivation of entropy corrections for black holes, applicable in any dimension, and proposes a classical perspective to explore quantum gravity properties.
Findings
Logarithmic corrections to black hole entropy derived
Method avoids negative entropy issues for small black holes
Classical approach hints at quantum gravity insights
Abstract
We provide a simple derivation of the corrections for Schwarzschild and Schwarzschild-Tangherlini black hole entropy without knowing the details of quantum gravity. We will follow Bekenstein, Wheeler and Jaynes ideas, using summations techniques without calculus approximations, to directly find logarithmic corrections to well-known entropy formula for black holes. Our approach is free from pathological behaviour giving negative entropy for small values of black hole mass . With the aid of Universality principle we will argue that this purely classical approach could open a window for exploring properties of quantum gravity.
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