Radiation of Quantized Black Hole

TL;DR

This paper explores the quantized surface of black holes, deriving their entropy, horizon spectrum, and radiation characteristics, aligning quantum properties with classical thermodynamics.

Contribution

It determines the horizon spectrum structure, calculates the Barbero-Immirzi parameter, and models black hole radiation spectrum consistent with quantum gravity theories.

Findings

Maximum entropy proportional to surface area in classical limit

Discrete radiation spectrum fits Wien profile

Total thermal radiation intensity calculated

Abstract

The maximum entropy of a quantized surface is demonstrated to be proportional to the surface area in the classical limit. The general structure of the horizon spectrum and the value of the Barbero-Immirzi parameter are found. The discrete spectrum of thermal radiation of a black hole fits naturally the Wien profile. The natural widths of the lines are very small as compared to the distances between them. The total intensity of the thermal radiation is calculated.