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    Locally rotationally symmetric spacetimes of type II in f(Q) gravity

    Fabrizio Esposito1,2,*, Sante Carloni1,2,3,†, and Stefano Vignolo1,2,‡

    • *Contact author: fabrizio.esposito01@edu.unige.it
    • †Contact author: sante.carloni@unige.it
    • ‡Contact author: stefano.vignolo@unige.it

    Phys. Rev. D 112, 044051 – Published 26 August, 2025

    DOI: https://doi.org/10.1103/17rf-2368

    Abstract

    We investigate the 1+1+2 covariant formalism in the presence of nonmetricity. Focusing on locally rotationally symmetric spacetimes, we show how nonmetricity affects all the kinematic quantities involved in the covariant 1+1+2 decomposition. We apply the resulting geometrical framework to study both homogeneous solutions and static spherically symmetric solutions in the context of f(Q) gravity. We obtain sufficient conditions for homogeneous solutions with flat spatial hypersurfaces and Schwarzschild-de Sitter type solutions in the 1+1+2 formalism. We also explore an elementary gravastar solution utilizing covariant junction conditions.

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