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Hawking Radiation as Tunneling through the Quantum Horizon

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arxiv hep-th/0505266 v2 pith:CNJO3EUV submitted 2005-05-31 hep-th astro-phgr-qc

Hawking Radiation as Tunneling through the Quantum Horizon

classification hep-th astro-phgr-qc
keywords blackradiationspectrumtermstunnelingariseblack-holecalculated
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Quantum Scattering in Schwarzschild Spacetime: Hawking Radiation and Black Hole Atmospheres

    hep-th 2026-07 reject novelty 4.0

    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.