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

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    SYSNO ASEP0599956
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleRevisiting Buchdahl transformations: new static and rotating black holes in vacuum, double copy, and hairy extensions
    Author(s) Barrientos, José (MU-W) SAI, ORCID, RID
    Cisterna, A. (CL)
    Hassaine, M. (CL)
    Oliva, J. (CL)
    Article number1011
    Source TitleEuropean Physical Journal C. - : Springer - ISSN 1434-6044
    Roč. 84, č. 10 (2024)
    Number of pages16 s.
    Publication formPrint - P
    Languageeng - English
    CountryDE - Germany
    Keywordsblack holes ; mathematical transformations ; black-hole spacetimes
    Subject RIVBA - General Mathematics
    OECD categoryParticles and field physics
    Method of publishingOpen access
    Institutional supportMU-W - RVO:67985840
    UT WOS001330673600010
    EID SCOPUS85206219473
    DOI https://doi.org/10.1140/epjc/s10052-024-13383-4
    AnnotationThis 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.
    WorkplaceMathematical Institute
    ContactJarmila Štruncová, struncova@math.cas.cz, library@math.cas.cz, Tel.: 222 090 757
    Year of Publishing2025
    Electronic addresshttps://doi.org/10.1140/epjc/s10052-024-13383-4
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