Hawking Radiation as Tunneling through the Quantum Horizon
Michele Arzano, A. J. M. Medved, Elias C. Vagenas
Abstract
Planck-scale corrections to the black-hole radiation spectrum in the Parikh-Wilczek tunneling framework are calculated. The corrective terms arise from modifications in the expression of the surface gravity in terms of the mass-energy of the black hole-emitted particle system. The form of the new spectrum is discussed together with the possible consequences for the fate of black holes in the late stages of evaporation.
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