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Microscopic derivation of the Bekenstein-Hawking entropy formula for non-extremal black holes
We derive the Bekenstein--Hawking entropy formula for four and five dimensional non-supersymmetric black holes (which include the Schwarzchild 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--Tei...
Autores principales: | Sfetsos, K, Skenderis, K |
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Lenguaje: | eng |
Publicado: |
1997
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0550-3213(98)00023-6 http://cds.cern.ch/record/338888 |
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