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Magnetized anisotropic Bianchi VI0 cosmology in Brans-Dicke gravity

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Abstract.

In this work, we present exact solutions of Brans-Dicke field equations with self-interacting potential U for the Bianchi type \( VI_{0}\) cosmological model filled with magnetized anisotropic matter contents. For this purpose, we use the variation law of the Hubble parameter and its resulting exponential as well as power law volumetric expansions. It is concluded that both the resulting models indicate expanding behavior of the universe with isotropic nature ( \( \delta \rightarrow 0\), \( \Delta\rightarrow 0\) in the presence of magnetized anisotropic fluid.

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Authors and Affiliations

  1. Department of Mathematics, University of the Punjab, Quaid-e-Azam Campus, 54590, Lahore, Pakistan

    M. Sharif & Imrana Shafique

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  1. M. Sharif
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  2. Imrana Shafique
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Correspondence to M. Sharif.

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Sharif, M., Shafique, I. Magnetized anisotropic Bianchi VI0 cosmology in Brans-Dicke gravity. Eur. Phys. J. Plus 129, 26 (2014). https://doi.org/10.1140/epjp/i2014-14026-2

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