On the Moduli Space of non-BPS Attractors for N=2 Symmetric Manifolds

Abstract

We study the ``flat'' directions of non-BPS extremal black hole attractors for N=2, d=4 supergravities whose vector multiplets' scalar manifold is endowed with homogeneous symmetric special Kahler geometry. The non-BPS attractors with non-vanishing central charge have a moduli space described by real special geometry (and thus related to the d=5 parent theory), whereas the moduli spaces of non-BPS attractors with vanishing central charge are certain Kahler homogeneous symmetric manifolds. The moduli spaces of the non-BPS attractors of the corresponding N=2, d=5 theories are also indicated, and shown to be rank-1 homogeneous symmetric manifolds.

1+11 pages, 4 Tables

References in corpus (5)

• N=8 non-BPS Attractors, Fixed Scalars and Magic Supergravities
• Non-supersymmetric Black Holes and Topological Strings
• Black-Hole Attractors in N=1 Supergravity
• One entropy function to rule them all
• Attractor Horizon Geometries of Extremal Black Holes

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• d=4 Black Hole Attractors in N=2 Supergravity with Fayet-Iliopoulos Terms
• Non-BPS Attractors in 5d and 6d Extended Supergravity
• Attractors with Vanishing Central Charge
• Attractors in Black
• Moduli Stabilization, Large-Volume dS Minimum Without anti-D3-Branes, (Non-)Supersymmetric Black Hole Attractors and Two-Parameter Swiss Cheese Calabi-Yau's
• Separation of Attractors in 1-modulus Quantum Corrected Special Geometry
• Black Holes in Supergravity: the non-BPS Branch