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K. Freese and M. Lewis, “Cardassian Expansion: A Model in which the Universe is Flat, Matter Dominated, and Accelerating,” Physical Letters B, Vol. 540, No. 1-2, 2002, pp. 1-8. doi:10.1016/S0370-2693(02)02122-6

has been cited by the following article:

• TITLE: Bianchi Type- III and Kantowski-Sachs Universes with wet Dark Fluid

  AUTHORS: Raghavendra Chaubey

  KEYWORDS: Cosmological Universe, Cosmological Parameters, Wet Dark Fluid

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.1 No.2, July 1, 2011

  ABSTRACT: The Bianchi type- III and Kantowski-Sachs (KS) Universes 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 ρ=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 =1/3have been also analysed.