Canonical Ensemble Model for the Black Hole Quantum Tunneling Radiation

TL;DR

This paper introduces a canonical ensemble model for black hole quantum tunneling radiation, analyzing emission spectra, probability distributions, and entropy to explore information flow from black holes.

Contribution

It presents a novel canonical ensemble framework for black hole radiation, linking quantum tunneling, entropy, and information transfer mechanisms.

Findings

Derived probability distribution function for emission shells

Analyzed the statistical significance of black hole radiation spectrum

Discussed the mechanism of information flow from black holes

Abstract

In this paper, a canonical ensemble model for the black hole quantum tunneling radiation is introduced. With this model the probability distribution function corresponding to the emission shell is calculated. Comparing with this function, the statistical significance of the quantum tunneling radiation spectrum of black holes is investigated. Moreover, by calculating the entropy of the emission shell, a discussion about the mechanism of information flowing out from the black hole is given too.