A recent analysis of the Supernova Ia data claims a 'marginal' ($\sim3\sigma$) 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 $\Delta(\textAIC)\sim30$.

Haridasu, B., Lukovic, V., D'Agostino, R., Vittorio, N. (2017). Strong evidence for an accelerating Universe. ASTRONOMY & ASTROPHYSICS, 600, L1 [10.1051/0004-6361/201730469].

Strong evidence for an accelerating Universe

VITTORIO, NICOLA
2017-01-01

Abstract

A recent analysis of the Supernova Ia data claims a 'marginal' ($\sim3\sigma$) 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 $\Delta(\textAIC)\sim30$.
2017
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
astro-ph.CO; astro-ph.CO
http://arxiv.org/abs/1702.08244v1
Haridasu, B., Lukovic, V., D'Agostino, R., Vittorio, N. (2017). Strong evidence for an accelerating Universe. ASTRONOMY & ASTROPHYSICS, 600, L1 [10.1051/0004-6361/201730469].
Haridasu, B; Lukovic, V; D'Agostino, R; Vittorio, N
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/179534
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