A Statistical Derivation of Bekenstein-Hawking Entropy for Schwarzschild Black Holes

TL;DR

This paper derives the Bekenstein-Hawking entropy for Schwarzschild black holes using a holographic phase space and an ideal bosonic gas model, emphasizing a 2D system perspective consistent with black hole thermodynamics.

Contribution

It introduces a holographic principle-based derivation of black hole entropy assuming an ideal bosonic gas inside the phase space, aligning black hole behavior with a 2D system.

Findings

Derivation of Bekenstein-Hawking entropy using holographic phase space

Black hole modeled as a 2D system with equation of state P=ρ

Supports black hole thermodynamics through microscopic statistical approach

Abstract

A microscopic derivation of the Bekenstein-Hawking entropy for the Schwarzschild black hole was presented earlier by using a non-trivial phase space. It was argued that the Schwarzschild black hole behaves like a 1D quantum mechanical system. In this paper, we show that if we assume the phase space to obey the holographic principle and take the microscopic particles inside the quantum gravitational system to be ideal bosonic gas, we can derive the Bekenstein-Hawking entropy. The assumption of the phase space to follow the holographic principle such that the Schwarzschild black hole behaves as a 2D system is very much in the spirit of our understanding of black holes than their behavior as a 1D system. However, the argument suggests that the black hole be treated as a system with the equation of state $P=\rho$.