On the interacting dark energy scenarios $-$ the case for Hubble constant tension

Abstract

The Hubble constant $H_0$ is one of the important cosmological parameters measuring the expansion rate of our universe at present moment. Over the last couple of years, $H_0$ has created an enormous amount of debates interests in the astrophysical and cosmological communities for its different estimations at many standard deviations by different observational surveys. The recent estimation of $H_0$ from the cosmic microwave background observations by Planck within the $\Lambda$-Cold Dark Matter ($\Lambda$CDM) paradigm is in tension with $\gtrsim 5\sigma$ confidence with SH0ES (Supernovae and $H_0$ for the Equation of State of dark energy) collaboration. As a result, revision of the standard $\Lambda$CDM model has been suggested in various ways in order to examine whether such scenarios can solve this $H_0$ tension. Among the list of the proposed cosmological scenarios, in this chapter we focus on a generalized cosmological theory in which the dark components of the universe, namely, Dark Matter (DM) and Dark Energy (DE) are allowed to interact with each other in a non-gravitational way, widely known as the Interacting DE or Coupled DE scenarios. These interacting scenarios have received magnificent attention in the scientific community for their appealing consequences. Specifically, in the context of $H_0$ tension, it has been observed that the interacting DE scenarios can lead to higher values of the Hubble constant ($H_0$) value, and consequently, the tension on $H_0$ can be either alleviated or solved. In this chapter we review various interacting DE scenarios and their roles in alleviating the $H_0$ tension.

Invited chapter for the edited book "Hubble Constant Tension" (Eds. E. Di Valentino and D. Brout, Springer Singapore) of the Springer Series in Astrophysics and Cosmology; published

References in corpus (41)

• 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
• Challenges for $\Lambda$CDM: An update
• Planck evidence for a closed Universe and a possible crisis for cosmology
• Large-scale instability in interacting dark energy and dark matter fluids
• Indications of a late-time interaction in the dark sector
• Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data
• Cosmologies with Energy Exchange
• Effects of the interaction between dark energy and dark matter on cosmological parameters
• Probing the interaction between dark matter and dark energy in the presence of massive neutrinos
• Gauss-Bonnet Quintessence: Background Evolution, Large Scale Structure and Cosmological Constraints
• Dark sector interaction: a remedy of the tensions between CMB and LSS data
• Interacting models may be key to solve the cosmic coincidence problem
• Toward a solution of the coincidence problem
• Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry
• KiDS+VIKING-450 and DES-Y1 combined: Mitigating baryon feedback uncertainty with COSEBIs
• Interacting models of soft coincidence
• A new interacting two fluid model and its consequences
• Novel approach towards the large-scale stable Interacting Dark-Energy models and their Astronomical Bounds
• 2021-$H_0$ Odyssey: Closed, Phantom and Interacting Dark Energy Cosmologies
• Interacting Dark Energy in a closed universe
• Disformal couplings and the dark sector of the universe
• Interacting quintessence from a variational approach Part II: derivative couplings
• Cosmological Evolution of Quintessence and Phantom with a New Type of Interaction in Dark Sector
• Thermodynamics second law and $\omega =-1$ crossing(s) in interacting holographic dark energy model
• Searching for dark matter - dark energy interactions: going beyond the conformal case
• Covariantizing the interaction between dark energy and dark matter
• Testing coupled dark energy models with their cosmological background evolution
• A Consistent View of Interacting Dark Energy from Multiple CMB Probes
• In search of the dark matter dark energy interaction: a kinematic approach
• Post-$Planck$ constraints on interacting vacuum energy
• Coupled and uncoupled early dark energy, massive neutrinos and the cosmological tensions
• First Cosmological Constraints on Dark Energy from the Radial Baryon Acoustic Scale
• Coupled dark energy with perturbed Hubble expansion rate
• Cosmological constraints on coupled dark energy
• A cosmographic analysis of holographic dark energy models
• Probing the sign-changeable interaction between dark energy and dark matter with current observations
• Theoretical and observational bounds on some interacting vacuum energy scenarios
• IWDM: The fate of an interacting non-cold dark matter $-$ vacuum scenario
• Evidence for horizon-scale power from CMB polarization
• On sign-changeable interaction in FLRW cosmology

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• No rungs attached: A distance-ladder free determination of the Hubble constant through type II supernova spectral modelling
• Reconciling $S_8$: Insights from Interacting Dark Sectors
• III. Interacting Dark Energy: Summary of Models, Pathologies, and Constraints
• Do we need wavelets in the late Universe?
• II. Non-Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• I. Linear Interacting Dark Energy: Analytical Solutions and Theoretical Pathologies
• Testing Gauss-Bonnet Gravity with DESI BAO Data
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• Background dynamics and observational constraints of flat and non-flat $\Lambda (t)$CDM models from $H(z)$ and DESI DR2 BAO measurements