Tunneling through the quantum horizon

Abstract

The emergence of quantum-gravity induced corrective terms for the probability of emission of a particle from a black hole in the Parikh-Wilczek tunneling framework is studied. It is shown, in particular, how corrections might arise from modifications of the surface gravity due to near horizon Planck-scale effects. Our derivation provides an example of the possible linking between Planck-scale departures from Lorentz invariance and the appearance of higher order quantum gravity corrections in the black-hole entropy-area relation.

8 pages, no figures, REVTeX. Extensively revised version. New title and modified paper structure. Main analysis unchanged. Some conclusions have been removed and will be discussed in a forthcoming work

References in corpus (5)

• Black hole entropy in Loop Quantum Gravity
• Hawking Radiation and Black Hole Thermodynamics
• A comment on black hole entropy or does Nature abhor a logarithm?
• A glimpse at the flat-spacetime limit of quantum gravity using the Bekenstein argument in reverse
• A follow-up to 'Does Nature abhor a logarithm?' (and apparently she doesn't)

Cited by in corpus (13)

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• Hawking radiation as tunneling from Gravity's rainbow
• Canonical entropy of three-dimensional BTZ black hole
• Hawking radiation as tunneling derived from Black Hole Thermodynamics through the quantum horizon
• Information loss and entropy conservation in quantum corrected Hawking radiation
• Back reaction, emission spectrum and entropy spectroscopy
• Tunneling across dilaton-axion black holes
• Charged Particles' Tunneling from Hot-NUT-Kerr-Newman-Kasuya Spacetime
• Logarithmic Entropy of Kehagias-Sfetsos black hole with Self-gravitation in Asymptotically Flat IR Modified Horava Gravity
• Radiation from Einstein-Gauss-Bonnet de Sitter Black Hole via Tunneling Process
• "Charged" Particle's Tunneling from Rotating Black Holes
• General Logarithmic Corrections to Bekenstein-Hawking Entropy