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- W2158366861 abstract "Bianchi type I magnetized cosmological models in the presence of a bulk viscous fluid are investigated. The source of the magnetic field is due to an electric current produced along the x-axis. The distribution consists of an electrically neutral viscous fluid with an infinite electrical conductivity. The coefficient of bulk viscosity is assumed to be a power function of mass density. The cosmological constant Λ is found to be positive and is a decreasing function of time which is supported by results from recent supernovae observations. The behaviour of the models in the presence and the absence of magnetic field are also discussed." @default.
- W2158366861 created "2016-06-24" @default.
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- W2158366861 date "2003-08-01" @default.
- W2158366861 modified "2023-10-10" @default.
- W2158366861 title "BIANCHI TYPE I ANISOTROPIC MAGNETIZED COSMOLOGICAL MODELS WITH VARYING Λ" @default.
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- W2158366861 doi "https://doi.org/10.1142/s0218271803003761" @default.
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