Gravity as a deformed topological gauge theory
Abstract
We describe gauge theories which allow to retrieve a large class of gravitational theories, including, MacDowell-Mansouri gravity and its topological extension to Loop Quantum Gravity via the Pontrjagin characteristic class involving the Nieh-Yan term. Considering symmetric spaces parametrized by mutations allows to naturally obtain a bare cosmological constant which in particular cases gives rise to a positive effective cosmological constant while having an AdS spacetime. Two examples are studied, Lorentzian geometry (including dS and AdS spacetimes) and LorentzWeyl geometry. In the latter case we prove 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.
Keywords
Cite
@article{arxiv.2403.05284,
title = {Gravity as a deformed topological gauge theory},
author = {J. Thibaut and S. Lazzarini},
journal= {arXiv preprint arXiv:2403.05284},
year = {2026}
}