Black hole evolution

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Abstract

Black hole formation and evaporation is studied in the semiclassical approximation in simple 1+1-dimensional models, with emphasis on issues related to Hawking's information paradox. Exact semiclassical solutions are described and questions of boundary conditions and vacuum stability are discussed. The validity of the semiclassical approximation has been called into question in the context of the information puzzle. A different approach, where black hole evolution is assumed to be unitary, is described. It requires unusual causal properties and kinematic behavior of matter that may be realized in string theory.

Original languageEnglish
Pages (from-to)245-275
Number of pages31
JournalNuclear Physics B (Proceedings Supplements)
Volume41
Issue number1-3
DOIs
Publication statusPublished - Apr 1995

Bibliographical note

Funding Information: *Supported in part by NSF grant No. PHY89-04035.

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