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
References in corpus (14)
- The Pantheon+ Analysis: Cosmological Constraints
- Modified teleparallel gravity: inflation without inflaton
- Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
- Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated - correlation
- New models and Big Bang Nucleosynthesis constraints in gravity
- Late-time cosmology with phantom dark-energy in gravity
- Data reconstruction of the dynamical connection function in cosmology
- Black hole solutions in scalar-tensor symmetric teleparallel gravity
- Testing Dark Energy Models with Gamma-Ray Bursts Calibrated from the Observational Data through a Gaussian Process
- Testing -Free f(Q) Cosmology
- Modelling the Accelerating Universe with Gravity: Observational Consistency
- Energy condition bounds on model parameters in a curved FLRW universe
- How different connections in flat FLRW geometry impact energy conditions in theory?
- Cosmological dynamics and observational constraints on a viable non-metric gravity model
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- Reconstructing dark energy with model independent methods after DESI DR2 BAO
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- A generic dynamical system formulation for Bianchi-I cosmology with isotropic fluid in gravity
- Addressing the tension through matter with pressure and no early dark energy
- Accelerating behavior from dynamical system analysis parameters
- Updated Cosmological Constraints from 2D BAO Measurements: A New Compilation and Comparison with DESI DR2
- Modified cosmology through generalized mass-to-horizon entropy: observational constraints from DESI DR2 BAO data
- Viability of general relativity and modified gravity cosmologies using high-redshift cosmic probes
- A Unified Dynamical Systems Framework for Cosmology in Gravity: Generic Features Beyond the Coincident Gauge
- Gamma-Ray Bursts Calibrated by Using Artificial Neural Networks from the Pantheon+ Sample
- Observational constraints on the modified cosmology inspired by string T-duality
- Insights in cosmology: the relevance of the connection