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Freese, K. and Lewis, M. (2002) Cardassian expansion: A model in which the universe is flat, matter dominated, and accelerating. Physics Letters B, 540, 1. doi:10.1016/S0370-2693(02)02122-6

has been cited by the following article:

• TITLE: Bianchi type-VIo Universe with wet dark fluid

  AUTHORS: Raghavendra Chaubey

  KEYWORDS: Cosmological Models; Wet Dark Fluid; Cosmological Parameters

  JOURNAL NAME: Natural Science, Vol.3 No.10, October 21, 2011

  ABSTRACT: 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.