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Institute of Theoretical Physics · Faculty of Mathematics and Physics, Charles University

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Article

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

Colléaux, A.; Kolář, J.; Málek, T.

Phys. Rev. D 112(12), 124040 (2025)

doi ↗ arXiv:2509.22309 ↗ link ↗

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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BibTeX

@article{UTF1049,
  author        = {Colléaux, A. and Kolář, J. and Málek, T.},
  title         = {{Double Wick rotations between symmetries of Taub-NUT, near-horizon extreme Kerr, and swirling spacetimes}},
  journal       = {Phys. Rev. D},
  volume        = {112},
  number        = {12},
  pages         = {124040},
  year          = {2025},
  month         = {12},
  doi           = {10.1103/y6sl-b6x4},
  eprint        = {2509.22309},
  archivePrefix = {arXiv},
  url           = {https://doi.org/10.1103/y6sl-b6x4},
}