Quintessence with Yukawa Interaction

Abstract

We consider a quintessence model for dark energy interacting with dark matter via a Yukawa interaction. To put constraints on this model we use the CMB measurements from the Planck satellite together with BAO, SNIa and $H_0$ data. We conclude that this is a viable model and an appropriate scalar potential can favor the interacting scenario.

10 pages, 6 figures, 3 tables. We fixed a bug in our numerical implementation and redid all the analysis. As a result: the previous divergent behavior at low multipoles is now absent; there is now more room for larger values of the interaction; the interaction become more favorable using low redshift measurements; the interaction become more plausible to help alleviating the coincidence problem

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Cited by in corpus (29)

• Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
• Non-minimal dark sector physics and cosmological tensions
• Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions
• Constraints on interacting dark energy models from Planck 2015 and redshift-space distortion data
• Listening to the sound of dark sector interactions with gravitational wave standard sirens
• Evidence for interacting dark energy from BOSS
• Unveiling dark fifth forces with linear cosmology
• Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn
• Analytic study of the effect of dark energy-dark matter interaction on the growth of structures
• J-PAS: forecasts on interacting dark energy from baryon acoustic oscillations and redshift-space distortions
• Coupled quintessence and the impossibility of an interaction: a dynamical analysis study
• Dynamical analysis for a vector-like dark energy
• Fractional Dark Matter decay: cosmological imprints and observational constraints
• Metastable dark energy
• Interacting quintessence in light of Generalized Uncertainty Principle: Cosmological perturbations and dynamics
• The BINGO Project VII: Cosmological Forecasts from 21cm Intensity Mapping
• Fractional dark energy
• Can Conformal and Disformal Couplings Between Dark Sectors Explain the EDGES 21cm Anomaly?
• The Dark Sector Cosmology
• A note on interacting holographic dark energy with a Hubble-scale cutoff
• Cosmological perturbations and dynamical analysis for interacting quintessence
• Testing a quintessence model with Yukawa interaction from cosmological observations and N-body simulations
• Two-dimensional Yukawa interaction driven by a nonlocal-Proca quantum electrodynamics
• Constraints on interacting dark energy revisited: implications for the Hubble tension
• Interacting Scalar fields: Dark matter and early dark energy
• Disentangling modified gravity from a dark force with gravitational redshift
• Comparing the motion of dark matter and standard model particles on cosmological scales
• Probing the independence within the dark sector in the fluid approximation
• Exploring the evolution of structure growth in the universe with field-fluid interactions through dynamical stability analysis