Charged Massive Particle's Tunneling From Charged Non-Rotating Micro Black Hole

TL;DR

This paper investigates how natural cutoffs affect the tunneling process and luminosity of charged massive particles emitted from charged non-rotating micro black holes within the Hawking radiation framework.

Contribution

It introduces the effects of minimal length, momentum, and maximal momentum cutoffs via a generalized uncertainty principle on black hole tunneling and luminosity calculations.

Findings

Natural cutoffs modify tunneling probabilities.

Luminosity is affected by the generalized uncertainty principle.

Energy and charge conservation are incorporated in the analysis.

Abstract

In the tunneling framework of Hawking radiation, charged massive particle's tunneling in charged non-rotating TeV-Scale black hole is investigated. To this end, we consider natural cutoffs as a minimal length, a minimal momentum, and a maximal momentum through a generalized uncertainty principle. We focus on the role played by these natural cutoffs on the luminosity of charged non-rotating micro black hole by taking into account the full implications of energy and charge conservation as well as the back- scattered radiation.