Abstract
We study in this article a class of homogeneous, but anisotropic cosmological models in which shear viscosity is included. Within the matter content we consider a component (the quintessence component) determined by the baryotropic equations of state, $p=\ensuremath{\alpha}\ensuremath{\rho},$ with $\ensuremath{\alpha}<0.$ We establish conditions under which a closed axisymmetrical cosmological model may look flat at low redshift.
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