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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).
J. D. Bekenstein, “Black Holes and Entropy,” Phys. Rev. D 7
1973
Earlier work this paper cites.
S.W. Hawking, “Black Hole Explosions?”, Nature 248 (1974) 30; “Particle Creation by Black Holes”, Comm. Math. Phys. 43 (1975) 199
1975
Earlier work this paper cites.
S.W. Hawking, “The Unpredictability of Quantum Gravity”, Commun. Math. Phys. 87 (1982) 395-415
1982
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1993
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2007
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2014
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