  The application of holographic principle in very early time is studied. The
consideration of the principle in the late-time evolution will be a good
motivation to study its role at the time of inflation. Since the length scale
is expected to be small during inflation, the resulted energy density form the
holographic principle is expected to be large enough to drive inflation. The
entropy of the system is the main part of the holographic principle, in which
modifying entropy will leads to a modified energy density. Here, instead of the
original entropy, we are going to apply a modified entropy, known as Tsallis
entropy which includes quantum corrections. The length scale is assumed to be
GO length scale. Finding an analytical solution for the model, the slow-roll
parameters, scalar spectral index, and tensor-to-scalar ratio are calculated.
Comparing the result, with Planck $r-n_s$ diagram, we could find a parametric
space for the constants of the model. Then, a correspondence between the
holographic dark energy and the scalar field is constructed, and the outcome
potentials are investigated.
