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

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arxiv 2405.00608 v2 pith:ZWM4T4IG submitted 2024-05-01 astro-ph.CO gr-qc

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

classification astro-ph.CO gr-qc
keywords desiacousticbaryoncosmologicaldarkdataenergygravity
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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 $H_0= 68.3^{+3.0}_{-3.5}$[km/s/Mpc] in agreement with SH0ES collaboration, however, due to a bigger uncertainty.

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Cited by 3 Pith papers

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