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Journal Article

Kähler geometry of black holes and gravitational instantons

MPS-Authors
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Aksteiner,  Steffen
Geometry and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Araneda,  Bernardo
Geometry and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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2207.10039.pdf
(Preprint), 154KB

PhysRevLett.130.161502.pdf
(Publisher version), 224KB

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Citation

Aksteiner, S., & Araneda, B. (2023). Kähler geometry of black holes and gravitational instantons. Physical Review Letters, 13(16): 161502. doi:10.1103/PhysRevLett.130.161502.


Cite as: https://hdl.handle.net/21.11116/0000-000A-C02C-C
Abstract
We obtain a closed formula for the Kaehler potential of a broad class of
four-dimensional Lorentzian or Euclidean conformal "Kaehler" geometries,
including the Plebanski-Demianski class and various gravitational instantons
such as Fubini-Study and Chen-Teo. We show that the Kaehler potentials of
Schwarzschild and Kerr are related by a Newman-Janis shift. Our method also
shows that a class of supergravity black holes, including the Kerr-Sen
spacetime, is Hermitian (but not conformal Kaehler). We finally show that the
integrability conditions of complex structures lead naturally to the
(non-linear) Weyl double copy, and we give new vacuum and non-vacuum examples
of this relation.