A new coupled three-form dark energy model and implications for the $H_0$ tension

Abstract

We propose a new coupled three-form dark energy model to relieve the Hubble tension in this paper. Firstly, by performing a dynamical analysis with the coupled three-form dark energy model, we obtain four fixed points, including a saddle point representing a radiation dominated Universe, a saddle point representing a matter dominated Universe, and two attractors representing two saturated de Sitter Universes. Secondly, by confronting the coupled three-form dark energy model and the $\Lambda$ cold dark matter model (the $\Lambda$CDM model) with cosmic microwave background (CMB), baryonic acoustic oscillations (BAO), Type Ia supernovae (SN Ia) observations, we obtain $H_0=67.8_{-0.6}^{+0.7}$($1\sigma$ level) km/s/Mpc for the coupled three-form dark energy model and $H_0=67.6_{-0.5}^{+0.5}$($1\sigma$ level) km/s/Mpc for the $\Lambda$CDM model, the former is in strong tension with the latest local measured $H_0$ value at $4.3\sigma$ confidence level, while the latter is in strong tension with the latest local measured $H_0$ value at $5.1\sigma$ level.

arXiv comment16 pages, 1 figure, 3 table. arXiv admin note: substantial text overlap with arXiv:2011.09160

References in corpus (39)

• 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
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Constraints on the redshift dependence of the dark energy potential
• A 6% measurement of the Hubble parameter at $z\sim 0.45$: direct evidence of the epoch of cosmic re-acceleration
• Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
• Early Dark Energy Can Resolve The Hubble Tension
• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• New physics in light of the $H_0$ tension: an alternative view
• Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
• Non-minimal dark sector physics and cosmological tensions
• Can interacting dark energy solve the $H_0$ tension?
• Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies
• New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75
• Evidence for massive neutrinos from CMB and lensing observations
• Quantifying discordance in the 2015 Planck CMB spectrum
• A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension
• Distance Priors from Planck Final Release
• Interacting dark energy with time varying equation of state and the $H_0$ tension
• Planck intermediate results. LI. Features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
• A Vacuum Phase Transition Solves $H_0$ Tension
• Planck Data Reconsidered
• Planck Constraints on Holographic Dark Energy
• Inflation and dark energy from three-forms
• Insensitivity of The Distance Ladder Hubble Constant Determination to Cepheid Calibration Modeling Choices
• Determining $H_0$ with Bayesian hyper-parameters
• How the Dark Energy Can Reconcile \textit{Planck} with Local Determination of the Hubble Constant
• Sterile neutrinos help reconcile the observational results of primordial gravitational waves from Planck and BICEP2
• Coupled three-form dark energy
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Testing interacting dark matter and dark energy model with cosmological data
• Measuring growth index in a universe with massive neutrinos: A revisit of the general relativity test with the latest observations
• Searching for sterile neutrinos in dynamical dark energy cosmologies
• Constraining light sterile neutrino mass with the BICEP2/Keck Array 2014 B-mode polarization data
• Parametrised modified gravity and the CMB Bispectrum
• A power-law coupled three-form dark energy model

Cited by in corpus (17)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
• Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension
• Exploring the $H_0$ tension and the evidence of dark sector interaction from 2D BAO measurements
• Dark sector interaction and the supernova absolute magnitude tension
• Late-transition vs smooth $H(z)$ deformation models for the resolution of the Hubble crisis
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• Late time interacting cosmologies and the Hubble constant tension
• Generalized Emergent Dark Energy Model and the Hubble Constant Tension
• A double take on early and interacting dark energy from JWST
• Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state
• On the dynamics of a dark sector coupling
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Hints of Neutrino Dark Matter scattering in the CMB? Constraints from the Marginalized and Profile Distributions
• Dissecting the $H_0$ and $S_8$ tensions with Planck + BAO + supernova type Ia in multi-parameter cosmologies
• Conditional variational autoencoders for cosmological model discrimination and anomaly detection in cosmic microwave background power spectra