Deformed and twisted black holes with NUTs
arXiv:1511.02536 · doi:10.1088/0264-9381/33/11/115016
Abstract
We construct a new class of vacuum black hole solutions whose geometry is deformed and twisted by the presence of NUT charges. The solutions are obtained by `unspinning' the general Kerr-NUT-(A)dS spacetimes, effectively switching off some of their rotation parameters. The resulting geometry has a structure of warped space with the Kerr-like Lorentzian part warped to a Euclidean metric of deformed and/or twisted sphere, with the deformation and twist characterized by the `Euclidean NUT' parameters. In the absence of NUTs, the solution reduces to a well known Kerr-(A)dS black hole with several rotations switched off. New geometries inherit the original symmetry of the Kerr-NUT-(A)dS family, namely, they possess the full Killing tower of hidden and explicit symmetries. As expected, for vanishing NUT, twist, and deformation parameters, the symmetry is further enlarged.
22 pages
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Cited by in corpus (7)
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- Separation of Maxwell equations in Kerr-NUT-(A)dS spacetimes
- NUT-like and near-horizon limits of Kerr-NUT-(A)dS spacetimes
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