arXiv · 1012.2120
Towards Cosmological Black Rings
Abstract
We classify all pseudo-supersymmetric near horizon geometries of extremal black holes in five dimensional de-Sitter supergravity coupled to vector multiplets. We find that there are three types of solution. The first type corresponds to the near-horizon geometry of extremal de Sitter BMPV black holes, and the spatial cross-section of the horizon is topologically S^3. The other two solutions cannot be embedded into the minimal de-Sitter supergravity theory, and correspond to near-horizon geometries for which the spatial cross-sections of the horizon are T^3 or S^1 * S^2.
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J. B. Gutowski, W. A. Sabra. 2010-12-09. Towards Cosmological Black Rings. https://doi.org/10.1007/jhep05(2011)020
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