Quantum gravity corrections to the tunneling radiation of scalar particles

Abstract

The original derivation of Hawking radiation shows the complete evaporation of black holes. However, theories of quantum gravity predict the existence of the minimal observable length. In this paper, we investigate the tunneling radiation of the scalar particles by introducing quantum gravity effects influenced by the generalized uncertainty principle. The Hawking temperatures are not only determined by the properties of the black holes, but also affected by the quantum numbers of the emitted particles. The quantum gravity corrections slow down the increase of the temperatures. The remnants are found during the evaporation.

V1, 13 pages

References in corpus (6)

• Universality of Quantum Gravity Corrections
• Tunnelling, Temperature and Taub-NUT Black Holes
• Temporal contribution to gravitational WKB-like calculations
• Dirac particles tunneling from BTZ black hole
• Black hole thermodynamics with generalized uncertainty principle
• Remarks on remnants by fermions' tunnelling from black strings