$f(T)$ gravity after DESI Baryon Acoustic Oscillation and DES Supernovae 2024 data

Abstract

In this work, we investigate new constraints on $f(T)$ gravity using the recent Baryon Acoustic Oscillation (BAO) data released by the Dark Energy Spectroscopic Instrument (DESI) and the Type Ia supernovae (SNIa) catalog from the full 5-years of the Dark Energy Survey Supernova Program (DES-SN5YR). The $f(T)$ cosmological models considered are characterised by power law late-time accelerated expansion. Our results show that the combination DESI BAO +$r_d$ CMB Planck suggests a Bayesian preference for late-time $f(T)$ cosmological models over $\Lambda$CDM, obtaining a value of $H_0=68.3_{-3.5}^{+3.0}$[km/s/Mpc] in agreement with SH0ES collaboration, however, due to a bigger uncertainty.

5 pages, 3 tables and 1 figure. Version accepted in Journal of High Energy Astrophysics 2024

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• A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
• Model-agnostic assessment of dark energy after DESI DR1 BAO
• Quintessence and phantoms in light of DESI 2025
• The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae
• Modified gravity realizations of quintom dark energy after DESI DR2
• Impacts of dark energy on weighing neutrinos after DESI BAO
• Newest measurements of Hubble constant from DESI 2024 BAO observations
• Empirical Validation: Investigating the ${\Lambda }_s$CDM Model with new DESI BAO Observations
• A short review on Quintom dark energy theory
• Testing Gauss-Bonnet Gravity with DESI BAO Data
• Probing dynamical embeddings in a five-dimensional spacetime in light of DESI BAO
• Constraining nonminimal f(T) gravity from Primordial Nucleosynthesis to Late-Universe observations
• Phantom Crossing with Quintom Models
• Chaplygin and Polytropic gases Teleparallel Robertson-Walker $F(T)$ gravity solutions
• Electromagnetic Sources Teleparallel Robertson--Walker $F(T)$-Gravity Solutions