Kaehler geometry of black holes and gravitational instantons
Steffen Aksteiner, Bernardo Araneda

TL;DR
This paper derives a unified formula for the Kähler potential of various four-dimensional geometries, revealing relationships between black hole solutions, supergravity spacetimes, and complex structures through the Weyl double copy.
Contribution
It provides a closed-form expression for the Kähler potential of broad classes of geometries and uncovers new links between black hole solutions and complex geometric structures.
Findings
Kähler potentials for Schwarzschild and Kerr are related by a Newman-Janis shift
Supergravity black holes like Kerr-Sen are Hermitian but not conformal Kähler
Integrability conditions lead to the non-linear Weyl double copy
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.
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Taxonomy
TopicsAdvanced Differential Geometry Research · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
