Einstein--Weyl Spaces and Near-Horizon Geometry
arXiv:1610.08953 · doi:10.1088/1361-6382/aa5992
Abstract
We show that a class of solutions of minimal supergravity in five dimensions is given by lifts of three--dimensional Einstein--Weyl structures of hyper-CR type. We characterise this class as most general near--horizon limits of supersymmetric solutions to the five--dimensional theory. In particular, we deduce that a compact spatial section of a horizon can only be a Berger sphere, a product metric on or a flat three-torus. We then consider the problem of reconstructing all supersymmetric solutions from a given near--horizon geometry. By exploiting the ellipticity of the linearised field equations we demonstrate that the moduli space of transverse infinitesimal deformations of a near--horizon geometry is finite--dimensional.
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- Einstein manifolds with torsion and nonmetricity
- Schrödinger connection with selfdual nonmetricity vector in 2+1 dimensions
- An action principle for the Einstein-Weyl equations
- The Maxwell-Chern-Simons gravity and its cosmological implications
- Supersymmetric near-horizon geometry and Einstein-Cartan-Weyl spaces
- Uniqueness of the extremal Schwarzschild de Sitter spacetime
- Electrovacuum spacetime near an extreme horizon
- Moduli Spaces of Transverse Deformations of Near-Horizon Geometries
- Spinorial geometry, off-shell Killing spinor identities and higher derivative 5D supergravities
- Parallel spinors on Lorentzian Weyl spaces
- Uniqueness of extremal charged black holes in de Sitter
- Existence and Uniqueness of Near-Horizon Geometries for 5-Dimensional Black Holes
- Rigidity of the extremal Kerr-Newman horizon
- Solutions of D=4 Gauged Pseudo-Supergravity
- Recurrent Lorentzian Weyl spaces
- Lie point symmetries of near-horizon geometry equation