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In this work, we examine the cosmological characteristics of the Power LawEntropy Corrected Holographic Dark Energy (PLECHDE) model with infrared (IR)cut-off, which is determined by the curvature parameter $k$, the timederivative of $H$, and the average radius of the Ricci scalar curvature $R$,which varies with the Hubble parameter $H$ squared. We obtain the decelerationparameter $q$ and the Equation of State (EoS) parameter of Dark Energy (DE)$\omega_D$. Additionally, we derive the Hubble parameter $H$ and the scalefactor $a$ expressions as functions of the cosmic time $t$. Additionally, weexamine the limiting scenario that pertains to a flat Dark Dominated Universe.Furthermore, we establish a correspondence between the DE model considered andsome scalar fields, in particular the Generalized Chaplygin Gas, the ModifiedChaplygin Gas, the Modified Variable Chaplygin Gas, the New Modified ChaplyginGas, the Viscous Generalized Chaplygin Gas, the Dirac-Born-Infeld, theYang-Mills, and the Non Linear Electrodynamics scalar field models.

Reconstruction schemes of scalar field models for the Power Law Entropy Corrected Holographic Dark Energy model with Ricci scalar cut-off