An f(T) model with m ≈ 0.91 and n ≈ 0.69, stable under dynamical analysis, reproduces the observed cosmic expansion when fitted to recent BAO, Hubble, and supernova datasets.
Cosmographic bounds on the cosmological deceleration–acceleration transition redshift inf(R) gravity,
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Cosmological Parameters in $f(T)$ Gravity: Theoretical and Observational Analysis
An f(T) model with m ≈ 0.91 and n ≈ 0.69, stable under dynamical analysis, reproduces the observed cosmic expansion when fitted to recent BAO, Hubble, and supernova datasets.