Massive vector particles tunneling from black holes influenced by the generalized uncertainty principle

TL;DR

This paper investigates how quantum gravity effects, modeled by the generalized uncertainty principle, influence the tunneling of massive vector particles from black holes, leading to modified temperature behaviors and potential black hole remnants.

Contribution

It introduces a model incorporating the generalized uncertainty principle to analyze massive vector particle tunneling from black holes, revealing quantum gravity corrections and remnant formation.

Findings

Quantum gravity decelerates black hole temperature increase.

Corrected temperatures depend on particle mass and angular momentum.

Black holes can stop radiating and form remnants near the Planck mass.

Abstract

This study considers the generalized uncertainty principle, which incorporates the central idea of large extra dimensions, to investigate the processes involved when massive spin-1 particles tunnel from Reissner-Nordstrom and Kerr black holes under the effects of quantum gravity. For the black hole, the quantum gravity correction decelerates the increase in temperature. Up to $\mathcal{O}(\frac{1}{M_f^2})$, the corrected temperatures are affected by the mass and angular momentum of the emitted vector bosons. In addition, the temperature of the Kerr black hole becomes uneven due to rotation. When the mass of the black hole approaches the order of the higher dimensional Planck mass $M_f$, it stops radiating and yields a black hole remnant.