Thermodynamically allowed phantom cosmology with viscous fluid

Abstract

In this work we present an analysis of the phantom zone in a causal viscous cosmology from a thermodynamic point of view. In this description we consider a chemical potential and the approach of irreversible processes. We assume a flat universe filled with a single dissipative fluid described by a barotropic equation of state, $p=\omega \rho$. This model allows to construct a negative chemical potential for the phantom regime but also this construction allows us to have positive definite temperature and entropy.

9 pages, 3 figures. Accepted version in PRD

References in corpus (6)

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• Unified dark energy thermodynamics: varying w and the -1-crossing
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• Testing a nonlinear solution of the Israel-Stewart theory
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