Strong evidence for an accelerating universe

Abstract

A recent analysis of the Supernova Ia data claims a 'marginal' ($\sim 3\sigma$) evidence for a cosmic acceleration. This result has been complemented with a non-accelerating $R_h=ct$ cosmology, which was presented as a valid alternative to the $\Lambda$CDM model. In this paper, we use the same analysis to show that a non-marginal evidence for acceleration is actually found. We compare the standard Friedmann models to the $R_h=ct$ cosmology by complementing SN Ia data with the Baryon Acoustic Oscillations, Gamma Ray Bursts and Observational Hubble datasets. We also study the power-law model which is a functional generalisation of $R_h=ct$. We find that the evidence for late-time acceleration is beyond refutable at a 4.56$\sigma$ confidence level from SN Ia data alone, and at an even stronger confidence level ($5.38\sigma$) from our joint analysis. Also, the non-accelerating $R_h=ct$ model fails to statistically compare with the $\Lambda$CDM having a $\Delta (\text{AIC})\sim 30$.

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Cited by in corpus (4)

• Extended Gravity Cosmography
• Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$
• Apparent cosmic acceleration from type Ia supernovae
• Reconstruction of $f(R)$ gravity models for an accelerated universe using Raychaudhuri equation