  A matter bouncing entropy-corrected cosmological model has been suggested.
The model allows only positive curvature with negative pressure and no
violation of the null energy condition. The result obtained in this paper is
supported by some recent theoretical works where the combination of positive
spatial curvature and vacuum energy leads to non-singular bounces with no
violation of the null energy condition. An important feature of the current
model is that evolutions of the cosmic pressure, energy density and equation of
state parameter are independent of the values of the prefactors $\alpha$ and
$\beta$ in the corrected entropy-area relation. The validity of the classical
and the new nonlinear energy conditions has been discussed. The cosmographic
parameters have been analyzed
