Moduli space of supersymmetric solitons and black holes in five dimensions
arXiv:1712.07092 · doi:10.1007/s00220-018-3215-8
Abstract
We determine all asymptotically flat, supersymmetric and biaxisymmetric soliton and black hole solutions to five dimensional minimal supergravity. In particular, we show that the solution must be a multi-centred solution with a Gibbons-Hawking base. The proof involves combining local constraints from supersymmetry with global constraints for stationary and biaxisymmetric spacetimes. This reveals that the horizon topology must be one of S^3, S^1 x S^2 or a lens space L(p,1), thereby providing a refinement of the allowed horizon topologies. We construct the general smooth solution for each possible rod structure. We find a large moduli space of black hole spacetimes with noncontractible 2-cycles for each of the allowed horizon topologies. In the absence of a black hole we obtain a classification of the known `bubbling' soliton spacetimes.
v2: 43 pages, 5 figures, references added, typos fixed, minor clarifications, expanded discussion of physical parameters. v3: clarified statement of theorem 4 (results unchanged, update made after publication)
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- On the uniqueness of supersymmetric AdS black holes with toric symmetry
- Uniqueness of the extremal Schwarzschild de Sitter spacetime
- Supersymmetric black holes with a single axial symmetry in five dimensions
- On the nonexistence of a vacuum black lens
- New thermodynamic identities for five-dimensional black holes
- A classification of supersymmetric Kaluza-Klein black holes with a single axial symmetry
- Five-dimensional electrostatic black holes in a background field
- Lower bound for angular momenta of microstate geometries in five dimensions
- N=4 Near-Horizon Geometries in D=11 Supergravity
- Bubbling saddles of the gravitational index