Abstract
In this paper we study FRW bulk viscous cosmology in presence of modified cosmic Chaplygin gas. We obtain generalized Friedmann equations due to bulk viscosity and modified cosmic Chaplygin gas. Then, we calculate time-dependent energy density and discuss Hubble expansion parameter.
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Saadat, H., Pourhassan, B. FRW bulk viscous cosmology with modified cosmic Chaplygin gas. Astrophys Space Sci 344, 237–241 (2013). https://doi.org/10.1007/s10509-012-1301-5
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DOI: https://doi.org/10.1007/s10509-012-1301-5