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Entropy and black hole horizons
The standard approach of counting the number of eigenmodes of N scalar fields near the horizon is used as a basis to provide a simple statistical mechanical derivation of the black hole entropy in two and four dimensions. The Bekenstein formula S={A\ov 4G\h} and the two-dimensional entropy S=2M/\l\h...
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| Lenguaje: | eng |
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1995
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| Acceso en línea: | https://dx.doi.org/10.1016/0370-2693(95)01020-Q http://cds.cern.ch/record/284235 |