Scalar fields in an anisotropic closed universe
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 barotropic equations of state, p=α , with α < 0. We establish conditions under which a closed axisymmetrical cosmological model may look flat al low redshift.
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