Abstract
Exact solutions of the field equations for a Bianchi type-I space-time, filled with a viscous fluid and cosmological constant, are obtained. We utilize the constancy of deceleration parameter to get singular and non-singular solutions. We investigate a number of solutions with constant and time-varying cosmological constant together with a linear relation between shear viscosity and expansion scalar. Due to dissipative processes, the mean anisotropy and shear of the model tend to zero at a faster rate.
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Singh, C.P., Kumar, S. Viscous fluid cosmology with a cosmological constant. Astrophys Space Sci 323, 407–414 (2009). https://doi.org/10.1007/s10509-009-0137-0
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DOI: https://doi.org/10.1007/s10509-009-0137-0