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Bianchi Type-I Cosmological Model Filled with Viscous Fluid in a Modified Brans-Dicke Cosmology

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Abstract

Adding the cosmological term, which is assumed to be variable in Brans-Dicke theory we have discussed about a Bianchi type-I cosmological model filled with viscous fluid with free gravitational field of Petrov type-D. The effect of viscousity on various kinematical parameters has been discussed. Finally, this model has been transformed to the original form (1961) of Brans-Dicke theory including a variable cosmological term.

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Acknowledgements

We are very thankful to Prof. R.K. Prasad, Department of Mathematics, Veer Kunwar Singh University, Ara, Bihar for valuable discussions and corrections in the manuscript.

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Authors and Affiliations

  1. Department of Mathematics, Patna Science College, Patna, 800005, Bihar, India

    P. Rai & L. N. Rai

  2. School of Physics, Shri Mata Vaishno Devi University, Kakryal, Katra, 182320, J&K, India

    V. K. Singh

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  1. P. Rai
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  2. L. N. Rai
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  3. V. K. Singh
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Correspondence to P. Rai.

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Rai, P., Rai, L.N. & Singh, V.K. Bianchi Type-I Cosmological Model Filled with Viscous Fluid in a Modified Brans-Dicke Cosmology. Int J Theor Phys 51, 2127–2134 (2012). https://doi.org/10.1007/s10773-012-1092-z

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  • DOI: https://doi.org/10.1007/s10773-012-1092-z

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