Gravity as a deformed topological gauge theory
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 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.