Topology of supersymmetric N=1, D=4 supergravity horizons

Abstract

All supersymmetric N=1, D=4 supergravity horizons have toroidal or spherical topology, irrespective of whether the black hole preserves any supersymmetry.

17 pages, latex. Alterations to introduction and section 3.3

References in corpus (6)

• Near-horizon symmetries of extremal black holes
• A Higher Dimensional Stationary Rotating Black Hole Must be Axisymmetric
• Symmetries of Higher Dimensional Black Holes
• Almost BPS black holes
• On the `Stationary Implies Axisymmetric' Theorem for Extremal Black Holes in Higher Dimensions
• Geometry of all supersymmetric four-dimensional $\mathcal{N}=1$ supergravity backgrounds

Cited by in corpus (1)

• Spinorial geometry, horizons and superconformal symmetry in six dimensions