Some Bianchi Type I Viscous Fluid Cosmological Models with a Variable Cosmological Constant |
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Authors: | Anirudh Pradhan Purnima Pandey |
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Institution: | (1) Department of Mathematics, Hindu Post-graduate College, Zamania, 232 331 Ghazipur, U.P., India |
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Abstract: | Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant are investigated in which the
expansion is considered only in two direction i.e. one of the Hubble parameter
is zero. The viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density whereas the coefficient
of shear viscosity is considered as constant in first case whereas in other case it is taken as proportional to scale of expansion
in the model. The cosmological constant Λ is found to be positive and is a decreasing function of time which is supported
by results from recent supernovae Ia observations. Some physical and geometric properties of the models are also discussed. |
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Keywords: | Cosmology Bianchi type I universe Viscous fluid models Variable cosmological constant |
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