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.

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

References in corpus (8)

• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
• Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2
• 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
• Neutrinos and dark energy after Planck and BICEP2: data consistency tests and cosmological parameter constraints
• Parametrised modified gravity and the CMB Bispectrum

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