paper

Testing Non-Coincident -gravity with DESI DR2 BAO and GRBs

arXiv:2504.11132 · doi:10.1016/j.dark.2025.101993

Abstract

We consider the -theory for the description of dark energy with a non-trivial connection defined in the non-coincident gauge. The resulting field equations form a two-scalar-field, quintom-like gravitational model. For the power-law model , we construct an analytic expression for the dynamical evolution of dark energy, which depends on the parameter . We constrain this dark energy model using the the baryon acoustic oscillations from DESI DR2, and gamma-ray bursts. The cosmological data provides . The -model challenges the CDM by providing a smaller value for . Although the Akaike Information Criterion indicates that the two cosmological models fit the data from the Pantheon+, the cosmic chronometers and the baryonic acoustic oscillators in a similar way, when the gamma-ray bursts are introduced there is weak evidence in favor of the -theory.

8 pages, 4 figures, version accepted for publication in Physics of the Dark Universe

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