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- W2024852898 abstract "The Bianchi type-III cosmological model for a cloud string in the presence of bulk viscosity and magnetic field are presented. To obtain the determinate model it is assumed that there is an equation of state ρ = kλ and the scalar of expansion is proportional to the shear scalar θσ, which leads to a relation between metric potentials B = mCn. The physical and geometric aspects of the model are also discussed. The model describes a shearing non-rotating continuously expanding universe with a big-bang start. In the absence of magnetic field, it reduces to the string model with bulk viscosity that was previously given in the literature." @default.
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- W2024852898 date "2006-06-28" @default.
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- W2024852898 title "Bianchi Type-III String Cosmological Model With Bulk Viscosity and Magnetic Field" @default.
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- W2024852898 doi "https://doi.org/10.1088/0256-307x/23/7/013" @default.
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