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arXiv · 1612.04743

Stationary $D=4$ Black Holes in Supergravity: The Issue of Real Nilpotent Orbits

Daniele Ruggeri·Mario Trigiante
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Abstract

The complete classification of the nilpotent orbits of ${\rm SO}(2,2)^2$ in the representation ${\bf (2,2,2,2)}$, achieved in \cite{Dietrich:2016ojx}, is applied to the study of multi-center, asymptotically flat, extremal black hole solutions to the STU model. These real orbits provide an intrinsic characterization of regular single-center solutions, which is invariant with respect to the action of the global symmetry group ${\rm SO}(4,4)$, underlying the stationary solutions of the model, and provide stringent regularity constraints on multi-centered solutions. The known \emph{almost-BPS} and \emph{composite non-BPS} solutions are revisited in this setting. We systematically provide, for the relevant ${\rm SO}(2,2)^2$-nilpotent orbits of the global Noether charge matrix, regular representatives thereof. This analysis unveils a composition law of the orbits according to which those containing regular multi-centered solutions can be obtained as combinations of specific single-center orbits defining the constituent black holes. Some of the ${\rm SO}(2,2)^2$-orbits of the total Noether charge matrix are characterized as "intrinsically singular" in that they cannot contain any regular solution.

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Daniele Ruggeri, Mario Trigiante. 2016-12-14. Stationary $D=4$ Black Holes in Supergravity: The Issue of Real Nilpotent Orbits. https://doi.org/10.1002/prop.201700007

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