Smoothing the $H_0$ tension with a dynamical dark energy model

Abstract

The discrepancy between Planck data and direct measurements of the current expansion rate $H_0$ and the matter fluctuation amplitude $S_8$ has become one of the most intriguing puzzles in cosmology nowadays. The $H_0$ tension has reached $4.2\sigma$ in the context of standard cosmology i.e $\Lambda$CDM. Therefore, explanations to this issue are mandatory to unveil its secrets. Despite its success, $\Lambda$CDM is unable to give a satisfying explanation to the tension problem. Unless some systematic errors might be hidden in the observable measurements, physics beyond the standard model of cosmology must be advocated. In this perspective, we study a phantom dynamical dark energy model as an alternative to $\Lambda$CDM in order to explain the aforementioned issues. This phantom model is characterised by one extra parameter, ${\Omega }_{pdde}$, compared to $\Lambda$CDM. We obtain a strong positive correlation between $H_0$ and ${\Omega }_{pdde}$, for all data combinations. Using Planck measurements together with BAO and Pantheon, we find that the $H_0$ and the $S_8$ tensions are $3\sigma$ and $2.6\sigma$, respectively. By introducing a prior on the absolute magnitude, $M_B$, of the SN Ia, the $H_0$ tension decreases to $2.27\sigma$ with $H_0=69.76_{-0.82}^{+0.75}$ km s${}^{-1}$ Mpc${}^{-1}$ and the $S_8$ tension reaches the value $2.37\sigma$ with $S_8=0.8269_{-0.012}^{+0.011}$.

arXiv comment11 pages, 4 figures

References in corpus (78)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The Cosmological Constant and Dark Energy
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• 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
• A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
• In the Realm of the Hubble tension $-$ a Review of Solutions
• 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 Pantheon+ Analysis: Cosmological Constraints
• Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Tensions between the Early and the Late Universe
• Early Dark Energy Can Resolve The Hubble Tension
• Information criteria for astrophysical model selection
• KiDS-450: Cosmological parameter constraints from tomographic weak gravitational lensing
• The Hubble Hunter's Guide
• Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
• New physics in light of the $H_0$ tension: an alternative view
• The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
• Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• Reconciling Planck with the local value of $H_0$ in extended parameter space
• KiDS+VIKING-450: Cosmic shear tomography with optical+infrared data
• Large Scale Structure as a Probe of Gravitational Slip
• Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension
• Dark Energy Anisotropic Stress and Large Scale Structure Formation
• Cosmic Microwave Background and Supernova Constraints on Quintessence: Concordance Regions and Target Models
• Aspects of the cosmological "coincidence problem"
• Does the Hubble constant tension call for new physics?
• First Cosmology Results using Type Ia Supernovae from the Dark Energy Survey: Constraints on Cosmological Parameters
• To H0 or not to H0?
• Likelihood Analysis of CMB Temperature and Polarization Power Spectra
• Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
• Baryon acoustic oscillations from the cross-correlation of Ly$\alpha$ absorption and quasars in eBOSS DR14
• Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z)\ge -1$ are tighter than those obtained in $\Lambda$CDM
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• On the use of the local prior on the absolute magnitude of Type Ia supernovae in cosmological inference
• Consistency tests of $\Lambda$CDM from the early integrated Sachs-Wolfe effect: Implications for early-time new physics and the Hubble tension
• Can Late Dark Energy Transitions Raise the Hubble constant?
• Constraining Dark Energy Dynamics in Extended Parameter Space
• Revisiting a negative cosmological constant from low-redshift data
• Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions
• Does Hubble Tension Signal a Breakdown in FLRW Cosmology?
• $H_0$ Tension, Phantom Dark Energy and Cosmological Parameter Degeneracies
• Holographic explanation of wide-angle power correlation suppression in the Cosmic Microwave Background Radiation
• Update on Coupled Dark Energy and the $H_0$ tension
• Dark Energy with Phantom Crossing and the $H_0$ tension
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Restoring cosmological concordance with early dark energy and massive neutrinos?
• Beyond six parameters: extending $\Lambda$CDM
• Dynamical dark energy after Planck CMB final release and $H_0$ tension
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• Dark sector interaction and the supernova absolute magnitude tension
• The impact of the cosmic variance on $H_0$ on cosmological analyses
• The little sibling of the big rip singularity
• Cosmological Bound on the QCD Axion Mass, Redux
• Late time interacting cosmologies and the Hubble constant tension
• Cosmological parameter inference with Bayesian statistics
• Constraining the Cosmology of the Phantom Brane using Distance Measures
• AIC, BIC, Bayesian evidence against the interacting dark energy model
• Cosmological constraints of phantom dark energy models
• Is the $H_0$ tension suggesting a 4th neutrino's generation?
• Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip
• Integral $F(R)$ Gravity and Saddle Point Condition as a Remedy for the $H_0$-tension
• Reconciling Hubble Constant Discrepancy from Holographic Dark Energy
• Is the Cosmological Coincidence a Problem?
• Cosmological perturbations in an effective and genuinely phantom dark energy Universe
• Cosmic infinity: A dynamical system approach
• The quantum realm of the "Little Sibling" of the Big Rip singularity
• Likelihood methods for CMB experiments
• Cosmological consequences of a scalar field with oscillating equation of state: A possible solution to the fine-tuning and coincidence problems
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Quantum behavior of the "Little Sibling" of the Big Rip induced by a three-form field
• How does an incomplete sky coverage affect the Hubble Constant variance?
• Linking little rip cosmologies with regular early universes

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• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
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• Multidimensionality of the Hubble tension: the roles of ${\Omega }_m$ and ${\omega }_c$
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• Testing the local void hypothesis using baryon acoustic oscillation measurements over the last twenty years
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• Fast Radio Bursts as probes of the late-time universe: a new insight on the Hubble tension
• Shape of Dark Energy: Constraining Its Evolution with a General Parametrization
• Revisiting CPL with sign-switching density: To cross or not to cross the NECB
• Observational constraints on the growth index parameters in $f(Q)$ gravity
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• A new parametrization of Hubble function and Hubble tension
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