Friedmann Cosmology with a Generalized Equation of State and Bulk Viscosity |
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Authors: | MENG Xin-He REN Jie HU Ming-Guang |
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Institution: | Department of Physics, Nankai University, Tianjin 300071, China |
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Abstract: | The universe content is considered as a non-perfect fluid with bulk viscosity and is described by a more general equation of state (endowed some deviation from the conventionally assumed cosmic perfect fluid model). We assume the bulk viscosity is a linear
combination of two terms: one is constant, and the other is
proportional to the scalar expansion θ=3\dot{a}/a. The
equation of state is described as
p=(γ-1)ρ+p0, where
p0 is a parameter. In this framework we demonstrate that this
model can be used to explain the dark energy dominated universe,
and different proper choices of the parameters may lead to three
kinds of fates of the cosmological evolution: no future
singularity, big rip, or Type-III singularity as presented in
S. Nojiri, S.D. Odintsov, and S. Tsujikawa, Phys. Rev. D
71 (2005) 063004]. |
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Keywords: | Friedmann cosmology equation of state bulk viscosity dark energy |
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