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Revisiting Buchdahl transformations: New static and rotating black holes in vacuum, double copy, and hairy extensions

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arxiv 2404.12194 v2 pith:KPEKNOYH submitted 2024-04-18 gr-qc hep-th

classification gr-qchep-th
keywords buchdahlblackcopydoubletransformationseinstein-scalarextendsextensions
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This paper investigates Buchdahl transformations within the framework of Einstein and Einstein-Scalar theories. Specifically, we establish that the recently proposed Schwarzschild-Levi-Civita spacetime can be obtained by means of a Buchdahl transformation of the Schwarschild metric along the spacelike Killing vector. The study extends Buchdahl's original theorem by combining it with the Kerr-Schild representation. In doing so, we construct new vacuum-rotating black holes in higher dimensions which can be viewed as the Levi-Civita extensions of the Myers-Perry geometries. Furthermore, it demonstrates that the double copy scheme within these new generated geometries still holds, providing an example of an algebraically general double copy framework. In the context of the Einstein-Scalar system, the paper extends the corresponding Buchdahl theorem to scenarios where a static vacuum seed configuration, transformed with respect to a spacelike Killing vector, generates a hairy black hole spacetime. We analyze the geometrical features of these spacetimes and investigate how a change of frame, via conformal transformations, leads to a new family of black hole spacetimes within the Einstein-Conformal-Scalar system.

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Cited by 2 Pith papers

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  1. Charged Kerr--Levi-Civita geometries in Einstein--Maxwell and low-energy heterotic string theory

    gr-qc 2026-08 conditional novelty 6.0 of 10

    Exact rotating charged Kerr-Levi-Civita solutions are constructed by Ernst inversion and by Hassan-Sen charging, with no exterior Ernst zeros or azimuthal closed timelike curves in the Einstein-Maxwell case and a Lamb...

  2. Extremal Kerr-Schild Form

    gr-qc 2024-11 conditional novelty 5.0 of 10

    A non-extremal black hole can be written exactly as its extremal limit plus a linear-in-mass term built from a single null vector, for a wide class of known solutions.

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