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Microscopic derivation of the Bekenstein-Hawking entropy formula for non-extremal black holes.(English)Zbl 0920.53048

Summary: We derive the Bekenstein-Hawking entropy formula for four- and five-dimensional non-supersymmetric black holes (which include the Schwarzschild ones) by counting microscopic states. This is achieved by first showing that these black holes are \(U\)-dual to the three-dimensional black hole of Banados-Teitelboim-Zanelli and then counting microscopic states of the latter following Carlip’s approach. Black holes higher than five dimensional are also considered. We discuss the connection of our approach to the \(D\)-brane picture.

MSC:

53Z05 Applications of differential geometry to physics
83C57 Black holes
83E30 String and superstring theories in gravitational theory

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This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.
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