Uniqueness theorem for stationary black hole solutions of σ-models in five dimensions
arXiv:hep-th/0410059 · doi:10.1103/PhysRevD.70.084025
Abstract
We prove the uniqueness theorem for stationary self-gravitating non-linear σ-models in five-dimensional spacetime. We show that the Myers-Perry vacuum Kerr spacetime is the only maximally extended, stationary, axisymmetric, asymptotically flat solution having the regular rotating event horizon with constant mapping.
6 pages, Revtex, to be published in Phys.Rev.D15
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