Exploring the effects of dark matter - dark energy interaction on cosmic evolution in viscous dark energy scenario

TL;DR

This paper investigates how interactions between dark matter and dark energy, combined with viscous dark energy effects, influence the Universe's evolution, using a generalized model and Bayesian analysis of supernova data.

Contribution

It introduces a generalized interacting dark energy model incorporating viscosity effects and performs a Bayesian analysis to constrain model parameters.

Findings

Viscous dark energy and dark matter interactions significantly affect cosmic expansion.

The model fits supernova data well, indicating the importance of viscosity and interaction effects.

Constraints on model parameters suggest deviations from standard $\\Lambda$CDM$.

Abstract

We explore the influence of interactions between dark matter (DM) and dark energy (DE) on the cosmic evolution of the Universe within a viscous dark energy (VDE) framework. Moving beyond traditional interacting dark energy (IDE) models, we propose a generalized IDE model adaptable to diverse IDE scenarios via IDE coupling parameters. In order to investigate deviations from $\Lambda$CDM across cosmic epochs by highlighting how viscous and the interactions between DM and DE impact cosmic density and expansion rates, we consider a model agnostic form of VDE. Eventually we perform a Bayesian analysis using the Union 2.1 Supernova Ia dataset and Markov Chain Monte Carlo (MCMC) sampling to obtain optimal values of model parameters. This comprehensive analysis provides insights about the interplay between viscous and IDE in shaping the Universe's expansion history.