  In this work, the PLECHDE model with Granda-Oliveros (G-O) IR-cutoff is
studied. The evolution of dark energy density, deceleration and EoS parameters
are calculated. I demonstrate that under a condition, our universe can
accelerate near the phantom barrier at present time. We calculate these
parameters also in PLECHDE at Ricci scale, when when $\alpha=2$ and $\beta=1$,
and at last a comparison between Ricci scale, G-O cutoff and non-corrected HDE
without matter field with G-O cutoff is done. The correspondence between this
model and some scalar field of dark energy models is established. By this
method, the evolutionary treatment of kinetic energy and potential for
quintessence, tachyon, K-essence and dilaton fields, are obtained. I show that
the results has a good compatibility with previous work in the limiting case of
flat, dark dominated and non corrected holographic dark energy.
