Low-redshift constraints on covariant canonical Gauge theory of gravity

Constraints on the Covariant Canonical Gauge Gravity (CCGG) theory from low-redshift cosmology are studied. The formulation extends Einstein's of General Relativity (GR) by a quadratic Riemann-Cartan term in Lagrangian, controlled "deformation" parameter. In Friedman universe this leads to an additional geometrical stress energy and promotes, due necessary presence torsion, cosmological constant time-dependent function. MCMC analysis combined data sets Type Ia Supernovae, Cosmic Chronometers Baryon Acoustic Oscillations yields fit that is well comparable with $\Lambda$CDM results. modifications implied CCGG approach turn out be subdominant cosmology. However, non-zero spatial curvature deformation parameter shown consistent observations.