Non-Thermal Corrections to Hawking Radiation Versus the Information Paradox

Abstract

We provide a model-independent argument indicating that for a black hole of entropy N the non-thermal deviations from Hawking radiation, per each emission time, are of order 1/N, as opposed to exp(-N). This fact abolishes the standard a priory basis for the information paradox.

5 pages, Latex

References in corpus (3)

• Black holes as mirrors: quantum information in random subsystems
• Black Hole Macro-Quantumness
• Black Holes as Critical Point of Quantum Phase Transition

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