Physics – High Energy Physics – High Energy Physics - Theory
Scientific paper
2008-06-13
Nucl.Phys.B812:343-401,2009
Physics
High Energy Physics
High Energy Physics - Theory
Replaced by final version to appear in Nuclear Physics B, Replacement has very minor changes, major results unchanged
Scientific paper
10.1016/j.nuclphysb.2008.10.023
We consider the geodesic motion on the symmetric moduli spaces that arise after timelike and spacelike reductions of supergravity theories. The geodesics correspond to timelike respectively spacelike $p$-brane solutions when they are lifted over a $p$-dimensional flat space. In particular, we consider the problem of constructing \emph{the minimal generating solution}: A geodesic with the minimal number of free parameters such that all other geodesics are generated through isometries. We give an intrinsic characterization of this solution in a wide class of orbits for various supergravities in different dimensions. We apply our method to three cases: (i) Einstein vacuum solutions, (ii) extreme and non-extreme D=4 black holes in N=8 supergravity and their relation to N=2 STU black holes and (iii) Euclidean wormholes in $D\geq 3$. In case (iii) we present an easy and general criterium for the existence of regular wormholes for a given scalar coset.
Bergshoeff Eric
Chemissany Wissam
Ploegh André
Riet Thomas Van
Trigiante Mario
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