Abstract
In this work, I consider the logarithmic-corrected and the power-law corrected versions of the holographic dark energy (HDE) model in the non-flat FRW universe filled with a viscous Dark Energy (DE) interacting with Dark Matter (DM). I propose to replace the infra-red cut-off with the inverse of the Ricci scalar curvature R. I obtain the equation of state (EoS) parameter ω Λ , the deceleration parameter q and the evolution of energy density parameter \(\varOmega_{D}'\) in the presence of interaction between DE and DM for both corrections. I study the correspondence of the logarithmic entropy corrected Ricci Dark Dnergy (LECRDE) and power-law entropy corrected Ricci Dark Energy (PLECRDE) models with the the Modified Chaplygin Gas (MCG) and some scalar fields including tachyon, K-essence, dilaton and quintessence. I also make comparisons with previous results.
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Pasqua, A. Power-law and logarithmic entropy-corrected Ricci viscous dark energy and dynamics of scalar fields. Astrophys Space Sci 346, 531–543 (2013). https://doi.org/10.1007/s10509-013-1464-8
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DOI: https://doi.org/10.1007/s10509-013-1464-8