2 research outputs found

    Interacting Two Fluid Viscous Dark Energy Cosmological Models in Bianchi Type II Universe

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    In this paper, we present a class of solutions of Barber’s second self creation field equations describing two fluid models of the universe in locally rotationally symmetric Bianchi type II universe filled with the barotropic fluid and bulk viscous dark energy fluid. Exact solutions of the field equations are obtained for non-interacting and interacting two fluid models. The Physical behavior of the model has been discussed

    Magnetized Anisotropic Dark Energy Bianchi Type III Cosmological Models in Brans-Dicke Theory of Gravitation

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    We investigate the spatially homogeneous Bianchi Type III cosmological models with magnetized anisotropic dark energy fluid in the scalar tensor theory of gravitation proposed by Brans-Dicke [1]. The solutions of the models are obtained by volumetric exponential expansion, power law expansion and power law relation between scalar field and scale factor ‘a’. The physical aspects of the dark energy models are discussed
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