Twisted sectors in three-dimensional gravity

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Twisted sectors in three-dimensional gravity

Twisted sectors –solutions to the equations of motion with nontrivial monodromies– of three dimensional Euclidean gravity are studied. We argue that upon quantization this new sector of the theory provides the necessary (and no more) degrees of freedom to account for the Bekenstein-Hawking entropy of three-dimensional black holes. PACS: 04.70.Dy; 04.60.Kz

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ژورنال

عنوان ژورنال: Physical Review D

سال: 1999

ISSN: 0556-2821,1089-4918

DOI: 10.1103/physrevd.60.104022