Hints of the tension in uncorrelated Baryon Acoustic Oscillations dataset
arXiv:2111.07907 · doi:10.1142/9789811269776_0151
Abstract
Baryon Acoustic Oscillations (BAO) datasets use very precise measurements of the spatial distribution of large-scale structures as a distance ladder to help constrain cosmological parameters. In a recent article \cite{Benisty:2020otr}, we combined 17 uncorrelated BAO measurements in the effective redshift range with the Cosmic Chronometers data, the Pantheon Type Ia supernova and the Hubble Diagram of Gamma Ray Bursts and Quasars to obtain that the CDM model fit infers for the Hubble constant: and for the sound horizon distance: . Beyond the CDM model we test CDM and wCDM and we get , accordingly. In this proceeding we present elaborate on our findings and we compare them to other recent results in the literature.
12 pages, 3 tables, 3 figures. To appear in the proceedings of the Sixteenth Marcel Grossmann Meeting - MG16, July 5-10, 2021
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