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    Double Wick rotations between symmetries of Taub-NUT, near-horizon extreme Kerr, and swirling spacetimes

    Aimeric Colléaux1,*, Ivan Kolář1,†, and Tomáš Málek2,‡

    • *Contact author: aimeric.colleaux@matfyz.cuni.cz
    • †Contact author: ivan.kolar@matfyz.cuni.cz
    • ‡Contact author: malek@math.cas.cz

    Phys. Rev. D 112, 124040 – Published 11 December, 2025

    DOI: https://doi.org/10.1103/y6sl-b6x4

    Abstract

    We explicitly show that certain four-dimensional infinitesimal group actions with three-dimensional orbits are related by double Wick rotations. In particular, starting with the symmetries of the spherical/hyperbolic/planar Taub-NUT spacetimes, one can obtain symmetries of the near-horizon extreme Kerr (NHEK) geometry or swirling universe by complex analytic continuations of coordinates. Similarly, the static spherical/hyperbolic/planar symmetries (i.e., symmetries of the Schwarzschild spacetime and other A-metrics) are mapped to symmetries of the B-metrics (or Melvin spacetime). All these mappings are theory independent—they constitute relations among symmetries themselves, and, hence among the classes of symmetry-invariant metrics and electromagnetic field strengths, rather than among specific solutions. Consequently, finding, e.g., vacuum Taub-NUT–type solutions in a given gravitational theory automatically yields vacuum NHEK- or swirling-type solutions of that theory, with a possible extension to the electromagnetic case.

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