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    Gravitational energy-momentum pseudotensor in f(Q) nonmetric gravity

    Salvatore Capozziello1,2,3,*, Maurizio Capriolo4,†, and Gaetano Lambiase4,5,‡

    • *Contact author: capozziello@na.infn.it
    • Contact author: mcapriolo@unisa.it
    • Contact author: glambiase@unisa.it

    Phys. Rev. D 113, 044017 – Published 6 February, 2026

    DOI: https://doi.org/10.1103/1kvt-vvcf

    Abstract

    We derive the affine tensor associated with the energy and momentum densities of both gravitational and matter fields, the complex pseudotensor, for f(Q) nonmetric gravity, the straightforward extension of the symmetric teleparallel equivalent of general relativity (STEGR), characterized by a flat, torsion-free, nonmetric connection. The local conservation of energy-momentum complex on shell is satisfied through a continuity equation. An important analogy is pointed out between gravitational pseudotensor of teleparallel f(T) gravity, in the Weitzenböck gauge, and the same object of symmetric teleparallel f(Q) gravity, in the coincident gauge. Furthermore, we perturb the gravitational pseudotensor ταλ in the coincident gauge up to the second order in the metric perturbation, obtaining a useful expression for the power carried by the related gravitational waves. We also present an application of the gravitational pseudotensor, determining the gravitational energy density of a Schwarzschild spacetime in STEGR gravity, adopting the concident gauge. Finally, analyzing the conserved quantities on manifolds, the Stokes theorem can be formulated for generic affine connections.

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