The Dynamics of Very Special Black Holes

Abstract

We show that the moduli space of supersymmetric black holes that arise in the five-dimensional N=2 supergravity theory with any number of vector multiplets is a weak HKT manifold. The moduli metric is expressed in terms of a HKT potential which is determined by the associated very special geometry of the supergravity theory. As an example, we give explicitly the black hole moduli metric for the STU model.

16 pages, Phyzzx, minor changes, some more references have been added

References in corpus (1)

• Moduli space metric for maximally-charged dilaton black holes

Cited by in corpus (16)

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