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Information in black hole radiation. (English) Zbl 0972.83567

Summary: If black hole formation and evaporation can be described by an \(S\)-matrix, information would be expected to come out in black hole radiation. An estimate shows that it may come out initially so slowly, or else be so spread out, that it would never show up in an analysis perturbative in \(M_{\text{Planck}}/M\), or in \(1/N\) for two-dimensional dilatonic black holes with a large number \(N\) of minimally coupled scalar fields.

MSC:

83C57 Black holes
83C47 Methods of quantum field theory in general relativity and gravitational theory
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References:

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