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    Gravity as a deformed topological gauge theory

    Jean Thibaut* and Serge Lazzarini†

    • *Contact author: jthibaut@cpt.univ-mrs.fr
    • †Contact author: serge.Lazzarini@cpt.univ-mrs.fr

    Phys. Rev. D 113, 024007 – Published 6 January, 2026

    DOI: https://doi.org/10.1103/83y2-g7jt

    Abstract

    We describe gauge theories that allow one to retrieve a large class of gravitational theories, including MacDowell-Mansouri gravity and its topological extension to loop quantum gravity via the Pontryagin characteristic class involving the Nieh-Yan term. Considering symmetric spaces parametrized by mutations allows one to naturally obtain a bare cosmological constant that in particular cases gives rise to a positive effective cosmological constant while having an anti–de Sitter (AdS) spacetime. Two examples are studied, Lorentzian geometry (including dS and AdS spacetimes) and Lorentz × Weyl geometry. In the latter case, we prove that adding a term dependent on torsion and dilations makes the equations of motion exhibit a secondary source for curvature in addition to the usual energy-momentum tensor. This additional source is expressed in terms of the spin density of matter, torsion, and their variations. Finally, we show that the gauge+matter actions constructed from invariant polynomials are asymptotically topological if one assumes a vanishing bare cosmological constant together with gauge and matter fields having compact support.

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