Bertotti-Robinson Geometry and Supersymmetry
The role of Bertotti-Robinson geometry in the attractor mechanism of extremal black holes is described for the case of N = 2 supersymmetry. Its implication for a model-independent derivation of the Bekenstein-Hawking entropy formula is discussed.
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Lenguaje: | eng |
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1997
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Acceso en línea: | http://cds.cern.ch/record/319252 |