Observational constraints on $f(T)$ theory
Puxun Wu, Hongwei Yu

TL;DR
This paper investigates $f(T)$ gravity models as alternatives to dark energy for cosmic acceleration, analyzing their theoretical properties and observational constraints, and comparing their fit to data with the standard $\\Lambda$CDM model.
Contribution
It performs the first statefinder and $Om(z)$ diagnostics on specific $f(T)$ models and constrains them with recent observational data, highlighting differences from previous claims and the standard model.
Findings
Both models cannot cross the phantom divide line.
Observational data favor the $\\Lambda$CDM model over the $f(T)$ models.
Data suggest a phantom-like dark energy with Sne Ia alone, but quintessence-like with combined data.
Abstract
The theory, which is an extension of teleparallel, or torsion scalar , gravity, is recently proposed to explain the present cosmic accelerating expansion with no need of dark energy. In this Letter, we first perform the statefinder analysis and diagnostic to two concrete models, i.e., and , and find that a crossing of phantom divide line is impossible for both models. This is contrary to an existing result where a crossing is claimed for the second model. We, then, study the constraints on them from the latest Union 2 Type Ia Supernova (Sne Ia) set, the baryonic acoustic oscillation (BAO), and the cosmic microwave background (CMB) radiation. Our results show that at the 95% confidence level , for Model 1 and ,…
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