Journal
ASTROPHYSICS AND SPACE SCIENCE
Volume 346, Issue 1, Pages 233-236Publisher
SPRINGER
DOI: 10.1007/s10509-013-1418-1
Keywords
Bulk viscous fluid; Wet dark fluid; Cosmological model; General relativity
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In this paper, we have constructed a five dimensional LRS Bianchi type I cosmological model with wet dark fluid (WDF) in general relativity with the matter field described as bulk viscosity. It is found that in presence of bulk viscosity an inflationary effective stiff fluid cosmological model is obtained, whereas in absence of bulk viscosity the wet dark fluid degenerate to stiff fluid. Some physical and geometrical properties of the model are also discussed.
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