Black Holes and Critical Points in Moduli Space
As we have seen, the d = 4, N = 2 ungauged SUGRAs have two types of geometries: the s-t geometry and the moduli space geometry. In this section, mainly following the seminal paper  of Ferrara, Gibbons, and Kallosh, (see also ) we will consider the fundamental interplay between these two geometries, especially in relation with the attractor mechanism.
KeywordsBlack Hole Modulus Space Lagrangian Density Extreme Black Hole Attractor Point
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