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Hawking Radiation as Tunneling for Extremal and Rotating Black Holes

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arxiv hep-th/0503081 v2 pith:CCKNB7PT submitted 2005-03-09 hep-th

Marco Angheben , Mario Nadalini , Luciano Vanzo , Sergio Zerbini This is my paper
classification hep-th
keywords blackextremaltunnelinghawkingholemethodradiationrotating
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The issue concerning semi-classical methods recently developed in deriving the conditions for Hawking radiation as tunneling, is revisited and applied also to rotating black hole solutions as well as to the extremal cases. It is noticed how the tunneling method fixes the temperature of extremal black hole to be zero, unlike the Euclidean regularity method that allows an arbitrary compactification period. A comparison with other approaches is presented.

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Cited by 3 Pith papers

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

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

    hep-th 2026-07 reject novelty 4.0 of 10

    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.

  2. Quantum-Corrected Thermodynamics, Dirac Perturbations, Geodesic Structure, and Topological Phases of Black Holes with Non-Minimal Logarithmic Coupling

    gr-qc 2026-07 reject novelty 4.0 of 10

    For the ln(R)F² black hole, a single coupling B is claimed to shrink the shadow and ISCO, alter Dirac quasinormal ringing, suppress Hawking luminosity, and set the sign of an effective pressure on the topological defect line.

  3. Alternative Derivations of Hawking Radiation

    gr-qc 2025-05 unverdicted novelty 2.0 of 10

    A review chapter that reproduces and compares the tunneling, anomaly, and Green's function derivations of Hawking radiation, recovering the Hawking temperature and noting open justifications.

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