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.
Reconstruction off(T)Gravity: Rip Cosmology, Finite-Time Future Singularities, and Thermodynamics
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.