The Bianchi type- VIo universe filled with dark energy from a wet dark fluid has been considered. A new equation of state for the dark energy component of the universe has been used. It is modeled on the equation of state p = γ ( ρ-ρ ﹡ ) which can describe a liquid, for example water. The exact solutions to the corresponding field equations are obtained in quadrature form. The solution for constant deceleration parameter have been studied in detail for power-law and exponential forms both. The case γ =0, γ =1, and γ =1/3 have been also analysed.
KeywordsCosmological ModelsWet Dark FluidCosmological Parameters
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