DE models with combined $H_0\cdot r_d$ from BAO and CMB dataset and friends

Abstract

It has been theorized that Dynamical Dark Energy (DDE) could be a possible solution to the Hubble tension. To avoid the degeneracy between the Hubble parameter $H_0$ and the sound horizon scale $r_d$, in this article we use their multiplication as one parameter $c/\left(H_0{r}_d\right)$ and we use it to infer cosmological parameters for 6 different models - $\Lambda$CDM and 5 DDE parametrizations -- the Chevallier-Polarski-Linder (CPL), the Barboza-Alcaniz (BA), the Low correlation (LC), the Jassal-Bagla-Padmanabhan (JBP) and the Feng-Shen-Li-Li model. We choose a dataset that treats this combination as one parameter, that includes the Baryon Acoustic Oscillation (BAO) data $0.11\le z\le 2.40$ and additional points from the Cosmic Microwave Background (CMB) Peaks ($z\approx 1090$). To them, we add the marginalized Pantehon dataset and GRB dataset. We see that the tension is moved from $H_0$ and $r_d$ to $c/\left(H_0{r}_d\right)$ and ${\Omega }_m$. There is only one model that satisfies the Planck 2018 constraints on both parameters and this is LC with a huge error. The rest cannot fit into both constraints. $\Lambda$CDM is preferred with respect to the statistical measures.

15 pages, final version published in the Special Issue of Universe "Modified Gravity Approaches to the Tensions of $\Lambda$CDM"

References in corpus (36)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• In the Realm of the Hubble tension $-$ a Review of Solutions
• Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with LambdaCDM
• PolyChord: nested sampling for cosmology
• WMAP constraints on low redshift evolution of dark energy
• On the Hubble constant tension in the SNe Ia Pantheon sample
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space
• Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$
• A parametric model for dark energy
• Cosmology with gamma-ray bursts: I. The Hubble diagram through the calibrated $E_{\mathrm{p},\mathrm{i}}$ - $E_{\mathrm{iso}}$ correlation
• A combined analysis of the $H_0$ late time direct measurements and the impact on the Dark Energy sector
• Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry
• Figure of Merit for Dark Energy Constraints from Current Observational Data
• Revealing Intrinsic Flat $\Lambda$CDM Biases with Standardizable Candles
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• Hints of Early Dark Energy in Planck, SPT, and ACT data: new physics or systematics?
• Comparing early dark energy and extra radiation solutions to the Hubble tension with BBN
• Can dark energy be dynamical?
• Recombination-independent determination of the sound horizon and the Hubble constant from BAO
• Is cosmic acceleration proven by local cosmological probes?
• Constraints on reconstructed dark energy model from SN Ia and BAO/CMB observations
• Soundness of Dark Energy properties
• Revealing the effects of curvature on the cosmological models
• BAO angular scale at z_eff = 0.11 with the SDSS blue galaxies
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• A New Class of Parametrization for Dark Energy without Divergence
• Modelling and testing the equation of state for (Early) dark energy
• Early dark energy in $k$-essence
• Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues
• Constraining the dark energy models using Baryon Acoustic Oscillations: An approach independent of $H_0\cdot r_d$
• Machine Learning improved fits of the sound horizon at the baryon drag epoch
• Sources of $H_0$-tensions in dark energy scenarios
• Improving data-driven model-independent reconstructions and updated constraints on dark energy models from Horndeski cosmology
• Constraints from High-Precision Measurements of the Cosmic Microwave Background: The Case of Disintegrating Dark Matter with $\Lambda$ or Dynamical Dark Energy
• Low-Redshift Constraints on Covariant Canonical Gauge Theory of Gravity
• Tests of Standard Cosmology in Horava Gravity and Bayesian Evidence for a Closed Universe, and the Hubble Tension

Cited by in corpus (5)

• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Impact of Cosmology on Lorentz Invariance Violation Constraints from GRB Time-Delays
• Special Issue on Modified Gravity Approaches to the Tensions of $\Lambda$CDM: Goals and Highlights
• Probing for Lorentz Invariance Violation in Pantheon Plus Dominated Cosmology
• Statistical Nuances in BAO Analysis: Likelihood Formulations and Non-Gaussianities