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

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.

7 pages,3 figures, version accepted for publication in New Astronomy

References in corpus (3)

• Exact Hawking Radiation of Scalars, Fermions, and Bosons Using the Tunneling Method Without Back-Reaction
• Tunneling of Massive Vector Particles from Types of BTZ-like Black Holes
• Tunneling Under the Influence of Quantum Gravity in Black Rings

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