Bertotti-Robinson Geometry and Supersymmetry
arXiv:hep-th/9701163
Abstract
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.
13 pages, figures, uses procsla,epsf,epsfig; Talk given at the 12th Italian Conference on General Relativity and Gravitational Physics, Rome, September 1996