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All timelike supersymmetric solutions of N=2, D=4 gauged supergravity coupled to abelian vector multiplets

Sergio L. Cacciatori, Dietmar Klemm, Diego S. Mansi, Emanuele Zorzan

TL;DR

This work provides a complete timelike-classification of supersymmetric solutions in four-dimensional ${\cal N}=2$ gauged supergravity with abelian vector multiplets using spinorial geometry. It reveals a generalized holonomy constraint ${\rm GL}((8-N)/2,\mathbb{C})\ltimes (N/2)\mathbb{C}^{(8-N)/2}$ and shows the spacetime is a U$(1)$-holonomy fibration over a three-dimensional base with torsion, guiding the construction of novel AdS$_4$ BPS black holes with nontrivial scalar profiles. In the timelike sector with U$(1)$ FI gauging and no hypermultiplets, the Killing spinor equations yield a linear system that fixes scalars and fluxes, resulting in a metric of the form $ds^2 = -4|b|^2 (dt+\sigma)^2 + |b|^{-2}(dz^2 + e^{2\Phi} dw d\bar{w})$ and a 3D base with reduced holonomy. The analysis sets the stage for exploring attractor phenomena and extensions to more general gaugings, hypermultiplets, and non-Abelian vector sectors in AdS backgrounds.

Abstract

The timelike supersymmetric solutions of N=2, D=4 gauged supergravity coupled to an arbitrary number of abelian vector multiplets are classified using spinorial geometry techniques. We show that the generalized holonomy group for vacua preserving N supersymmetries is GL((8-N)/2,C) $\ltimes$ N/2 C^((8-N)/2) $\subseteq$ GL(8,R), where N=0,2,4,6,8. The spacetime turns out to be a fibration over a three-dimensional base manifold with U(1) holonomy and nontrivial torsion. Our results can be used to construct new supersymmetric AdS black holes with nontrivial scalar fields turned on.

All timelike supersymmetric solutions of N=2, D=4 gauged supergravity coupled to abelian vector multiplets

TL;DR

This work provides a complete timelike-classification of supersymmetric solutions in four-dimensional gauged supergravity with abelian vector multiplets using spinorial geometry. It reveals a generalized holonomy constraint and shows the spacetime is a U-holonomy fibration over a three-dimensional base with torsion, guiding the construction of novel AdS BPS black holes with nontrivial scalar profiles. In the timelike sector with U FI gauging and no hypermultiplets, the Killing spinor equations yield a linear system that fixes scalars and fluxes, resulting in a metric of the form and a 3D base with reduced holonomy. The analysis sets the stage for exploring attractor phenomena and extensions to more general gaugings, hypermultiplets, and non-Abelian vector sectors in AdS backgrounds.

Abstract

The timelike supersymmetric solutions of N=2, D=4 gauged supergravity coupled to an arbitrary number of abelian vector multiplets are classified using spinorial geometry techniques. We show that the generalized holonomy group for vacua preserving N supersymmetries is GL((8-N)/2,C) N/2 C^((8-N)/2) GL(8,R), where N=0,2,4,6,8. The spacetime turns out to be a fibration over a three-dimensional base manifold with U(1) holonomy and nontrivial torsion. Our results can be used to construct new supersymmetric AdS black holes with nontrivial scalar fields turned on.

Paper Structure

This paper contains 13 sections, 169 equations, 2 tables.