Hints of the $H_0-r_d$ tension in uncorrelated Baryon Acoustic Oscillations dataset

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 $0.106\le z\le 2.36$ with the Cosmic Chronometers data, the Pantheon Type Ia supernova and the Hubble Diagram of Gamma Ray Bursts and Quasars to obtain that the $\Lambda$CDM model fit infers for the Hubble constant: $69.85\pm 1.27km/sec/Mpc$ and for the sound horizon distance: $146.1\pm 2.15Mpc$. Beyond the $\Lambda$CDM model we test ${\Omega }_k$CDM and wCDM and we get ${\Omega }_k=-0.076\pm 0.012$, $w=-0.989\pm 0.049$ accordingly. In this proceeding we present elaborate on our findings and we compare them to other recent results in the literature.

arXiv comment12 pages, 3 tables, 3 figures. To appear in the proceedings of the Sixteenth Marcel Grossmann Meeting - MG16, July 5-10, 2021

References in corpus (40)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• H0LiCOW XIII. A 2.4% measurement of $H_0$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes
• Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers
• Cosmological implications of baryon acoustic oscillation (BAO) measurements
• The Hubble Hunter's Guide
• Cosmology Intertwined II: The Hubble Constant Tension
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2
• Curvature tension: evidence for a closed universe
• The WiggleZ Dark Energy Survey: Improved Distance Measurements to z = 1 with Reconstruction of the Baryonic Acoustic Feature
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2
• Evolution of the $f{\sigma }_8$ tension with the Planck15/$\Lambda$CDM determination and implications for modified gravity theories
• Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future
• Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• General Cosmography Model with Spatial Curvature
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: galaxy clustering measurements in the low redshift sample of Data Release 11
• Acoustic scale from the angular power spectra of SDSS-III DR8 photometric luminous galaxies
• The length of the low-redshift standard ruler
• Cosmology Intertwined IV: The Age of the Universe and its Curvature
• A Lockdown Perspective on the Hubble Tension (with comments from the SH0ES team)
• Cosmology Intertwined I: Perspectives for the Next Decade
• Clustering and Halo Abundances in Early Dark Energy Cosmological Models
• H0 tension or T0 tension?
• Euclid: Forecast constraints on the cosmic distance duality relation with complementary external probes
• Combined analysis of Planck and SPTPol data favors the early dark energy models
• Phenomenology of the generalized cubic covariant Galileon model and cosmological bounds
• Self-interacting neutrinos: solution to Hubble tension versus experimental constraints
• Self-interacting dark matter from late decays and the $H_0$ tension
• Reaffirming the Cosmic Acceleration without Supernova and CMB
• Quintessential inflation and cosmological seesaw Mechanism: reheating and observational constraints
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• Special cases of the Multi-Measure Model -- understanding the prolonged inflation

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