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• W2020191570 abstract "Einstein field equations with the cosmological constant is considered in the presence of bulk viscosity in a Bianchi type-I universe. Solutions of the field equations are obtained by assuming the following conditions: the bulk viscosity is proportional to the expansion scalar ξ ∝ θ; the expansion scalar is proportional to shear scalar θ ∝ σ; and Λ is proportional to the Hubble parameter Λ ∝ H. The corresponding interpretations of the cosmological solutions are also discussed." @default.
• W2020191570 created "2016-06-24" @default.
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• W2020191570 date "2011-09-01" @default.
• W2020191570 modified "2023-09-26" @default.
• W2020191570 title "Bianchi Type-I String Cosmological Model with Bulk Viscosity and Time-Dependent Λ term" @default.
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• W2020191570 doi "https://doi.org/10.1088/0256-307x/28/9/090401" @default.
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