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Bianchi Type-III Magnetized Wet Dark Fluid Cosmological Model in General Relativity

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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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Authors and Affiliations

  1. Department of Mathematics, S.G.B. Amravati University, Amravati, 444 602, India

    K. S. Adhav, M. V. Dawande, R. S. Thakare & R. B. Raut

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  1. K. S. Adhav
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  2. M. V. Dawande
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  3. R. S. Thakare
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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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