Tunneling Analysis Under the Influences of Einstein-Gauss-Bonnet Black Holes Gravity Theory

TL;DR

This paper investigates how quantum gravity effects influence tunneling radiation and Hawking temperature of charged black holes within Einstein-Gauss-Bonnet gravity, revealing non-thermal remnants and modifications to black hole thermodynamics.

Contribution

It introduces a semiclassical tunneling analysis of W-bosons in Einstein-Gauss-Bonnet black holes, highlighting quantum gravity's impact on radiation and temperature corrections.

Findings

Quantum gravity effects cause non-thermal radiation remnants.

Modified Hawking temperature depends on quantum corrections.

Graphical analysis shows temperature deviations due to quantum effects.

Abstract

We consider an equation of motion for Glashow-Weinberg-Salam model and apply the semiclassical Hamilton-Jacobi process and WKB approximation in order to compute the tunneling probability of W-bosons in the background of electromagnetic field to analyze the quantum gravity effects of charged black hole(BH) in Einstein-Gauss-Bonnet gravity theory. After this, we examine the quantum gravity influences on the generalized Lagrangian field equation. We make clear that quantum gravity effects leave the remnants on the tunneling radiation becomes non-thermal. Moreover, we analyze the graphical behavior of quantum gravity influences on corrected Hawking temperature for spin-$1$ particles for charged BHs.