Einstein-Maxwell-Anti-de-Sitter spinning solitons
arXiv:1602.06990 · doi:10.1016/j.physletb.2016.04.004
Abstract
Electrostatics on global Anti-de-Sitter (AdS) spacetime is sharply different from that on global Minkowski spacetime. It admits a multipolar expansion with everywhere regular, finite energy solutions, for every multipole moment except the monopole (arXiv:1507.04370). A similar statement holds for global AdS magnetostatics. We show that everywhere regular, finite energy, electric plus magnetic fields exist on AdS in three distinct classes: with non-vanishing total angular momentum ; with vanishing but non-zero angular momentum density, ; with vanishing and . Considering backreaction, these configurations remain everywhere smooth and finite energy, and we find, for example, Einstein-Maxwell-AdS solitons that are globally - Type I - or locally (but not globally) - Type II - spinning. This backreaction is considered first perturbatively, using analytical methods and then non-perturbatively, by constructing numerical solutions of the fully non-linear Einstein-Maxwell-AdS system. The variation of the energy and total angular momentum with the boundary data is explicitly exhibited for one example of a spinning soliton.
15 pages, 3 figures
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- Static Einstein-Maxwell Magnetic Solitons and Black Holes in an Odd Dimensional AdS Spacetime
- AdS magnetized solutions in minimal gauged supergravity
- Gravitational systems in asymptotically anti-de Sitter space-times