Interacting modified holographic Ricci dark energy model and statefinder diagnosis in flat universe

Abstract

In this work we have considered the modified holographic Ricci dark energy interacting with dark matter through a non-gravitational coupling. We took three phenomenological forms for the interaction term $Q$ in the model, where in general $Q$ is proportional to the Hubble parameter and densities of the dark sectors, ${\rho }_{de}+{\rho }_m,{\rho }_m$ and ${\rho }_{de}$ respectively. We have obtained analytical solutions for the three interacting models, and studied the evolutions of equations of state parameter, deceleration parameter. The results are compared with the observationally constrained values for the best parameters of the model. We have also done the statefinder analysis of the model to discriminate the model from other standard models. In general we have shown that the model is showing a de Sitter type behavior in the far future of the evolution of the universe.

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Cited by in corpus (7)

• Bulk viscous matter and recent acceleration of the Universe
• Scalar perturbations in cosmological models with dark energy - dark matter interaction
• A Dynamical System Analysis of Holographic Dark Energy Models with Different IR Cutoff
• Holographik, the k-essential approach to interactive models with modified holographic Ricci dark energy
• Viscous extended holographic Ricci dark energy in the framework of standard Eckart theory
• Bayesian Comparison of Interacting Modified Holographic Ricci Dark Energy Scenarios
• Bayesian analysis of running holographic Ricci dark energy