Abstract
Bianchi type-III cosmological model of universe filled with dark energy from a wet dark fluid (WDF) in presence and absence of magnetic field is investigated in general theory of relativity. We assume that F 12 is the only non-vanishing component of F ij . We obtain exact solutions to the field equations using the condition that expansion is proportional to the shear scalar i.e. (B=C n). The physical behavior of the model is discussed with and without magnetic field. We conclude that universe model do not approach isotropy through the evolution of the universe.
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Adhav, K.S., Dawande, M.V., Thakare, R.S. et al. Bianchi Type-III Magnetized Wet Dark Fluid Cosmological Model in General Relativity. Int J Theor Phys 50, 339–348 (2011). https://doi.org/10.1007/s10773-010-0530-z
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DOI: https://doi.org/10.1007/s10773-010-0530-z