Constraints on $f(T)$ Cosmology with Pantheon+

Abstract

$f(T)$ cosmology has shown promise in explaining aspects of cosmic evolution. In this work, we analyze constraints on leading models of $f(T)$ gravity in the context of the recently released Pantheon+ data set, together with comparisons with previous releases. We also consider other late-time data sets including cosmic chronometers and baryonic acoustic oscillation data. Our main result is that we find that the different $f(T)$ models under investigation connect to a variety of Hubble constant, which may help alleviate the cosmic tension on this parameter.

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Cited by in corpus (16)

• Late-Time constraints on Interacting Dark Energy: Analysis independent of $H_0$, $r_d$ and $M_B$
• $f(T)$ gravity after DESI Baryon Acoustic Oscillation and DES Supernovae 2024 data
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• Growth of structures using redshift space distortion in $f(T)$ Cosmology
• Prospects of constraining $f(T)$ gravity with the third-generation gravitational-wave detectors
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• Phase space analysis of Bianchi III Universe with $f(R,T)$ gravity theory
• White Dwarf Envelops and Temperature Corrections in Exponential $f(T)$ Gravity