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Hawking Radiation as Tunneling through the Quantum Horizon
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Hawking Radiation as Tunneling through the Quantum Horizon
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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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Cited by 1 Pith paper
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Quantum Scattering in Schwarzschild Spacetime: Hawking Radiation and Black Hole Atmospheres
The paper derives a Bose-Einstein emission rate at the Hawking temperature and an atmosphere radius rAtm = 4 ln2 r_s from antibound poles of the Schwarzschild S-matrix, but the derivation is not self-consistent.
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