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Cited by 476

The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.

Black Hole Entropy from Conformal Field Theory in Any Dimension

Open access
Carlip, S.·1999·Physical Review Letters

Abstract

Restricted to a black hole horizon, the ``gauge'' algebra of surface deformations in general relativity contains a Virasoro subalgebra with a calculable central charge. The fields in any quantum theory of gravity must transform accordingly, i.e., they must admit a conformal field theory description. Applying Cardy's formula for the asymptotic density of states, I use this result to derive the Bekenstein-Hawking entropy. This method is universal---it holds for any black hole, and requires no details of quantum gravity---but it is also explicitly statistical mechanical, based on counting microscopic states.

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Metadata

Authors
Carlip, S.
Venue
Physical Review Letters
Published
1999-04-05
Volume
82
Issue
14
Pages
2828-2831
ISSN
  • 0031-9007 (ISSN-L)
  • 1079-7114
OpenAlex
W2082823875
Cited by
476
References
4
FWCI
19.65
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Black Hole Entropy from Conformal Field Theory in Any Dimension. https://app.cochat.ai/papers/10.1103/physrevlett.82.2828
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Carlip, S. (1999). Black Hole Entropy from Conformal Field Theory in Any Dimension. Physical Review Letters. https://doi.org/10.1103/physrevlett.82.2828

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