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• W1983638247 abstract "The locally rotationally symmetric Bianchi type-II magnetized string cosmological model with bulk viscous fluid is investigated. The magnetic field is due to an electric current produced along the x-axis. Thus the magnetic field is in the y-z plane and F23 is the only non-vanishing component of electromagnetic field tensor Fij. To obtain the deterministic model in terms of cosmic time t, we have assumed the condition ξθ=const, where ξ is the coefficient of bulk viscosity and θ is the expansion in the model." @default.
• W1983638247 created "2016-06-24" @default.
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• W1983638247 date "2011-08-01" @default.
• W1983638247 modified "2023-10-14" @default.
• W1983638247 title "Locally Rotationally Symmetric Bianchi Type-II Magnetized String Cosmological Model with Bulk Viscous Fluid in General Relativity" @default.
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• W1983638247 doi "https://doi.org/10.1088/0256-307x/28/8/089802" @default.
• W1983638247 hasPublicationYear "2011" @default.
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