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    Charged black hole surrounded by a galactic halo in a de Sitter universe

    R. A. Konoplya1,*, Z. Stuchlík1,†, and A. Zhidenko1,2,‡

    • 1Research Centre for Theoretical Physics and Astrophysics, Institute of Physics, Silesian University in Opava, Bezručovo náměstí 13, CZ-74601 Opava, Czech Republic
    • 2Centro de Matemática, Computação e Cognição (CMCC), Universidade Federal do ABC (UFABC), Rua Abolição, CEP: 09210-180, Santo André, SP, Brazil

    • *Contact author: roman.konoplya@gmail.com
    • †Contact author: zdenek.stuchlik@physics.slu.cz
    • ‡Contact author: olexandr.zhydenko@ufabc.edu.br

    Phys. Rev. D 112, 083014 – Published 6 October, 2025

    DOI: https://doi.org/10.1103/l33g-6hlr

    Abstract

    Assuming a sufficiently general form for the matter distribution function of a galactic halo, we have derived solutions to the Einstein-Maxwell equations describing a charged black hole embedded in such a halo, while also allowing for a nonzero cosmological constant. These solutions generalize our earlier results for neutral black holes in asymptotically flat spacetime. As specific realizations of the general distribution, we consider the Hernquist, Navarro-Frenk-White, Burkert, Taylor-Silk, and Moore halo profiles, thereby capturing a broad range of astrophysically motivated scenarios.

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