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Tilted Bianchi type-I wet dark fluid model in Saez and Ballester theory

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Abstract

Tilted Bianchi-I wet dark fluid cosmological model is investigated in Saez and Ballester scalar theory of gravitation. Background cosmologies are obtained for a constant deceleration parameter. We consider a linear relationship between the shear scalar and the expansion scalar. We have discussed some physical and geometrical properties of the models. In our models, equation of state of the dark energy is observed to behave like a cosmological constant at late times.

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Authors and Affiliations

  1. Department of Mathematics, Arba Minch University, P.O. Box-21, Arba Minch, Ethiopia

    S. K. Sahu & T. T. Tole

  2. Department of Mathematics, Kotebe Metropolitan University, P.O. Box-31248, Addis Ababa, Ethiopia

    M. Balcha

Authors
  1. S. K. Sahu
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  2. T. T. Tole
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  3. M. Balcha
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Correspondence to S. K. Sahu.

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Sahu, S.K., Tole, T.T. & Balcha, M. Tilted Bianchi type-I wet dark fluid model in Saez and Ballester theory. Indian J Phys 92, 813–818 (2018). https://doi.org/10.1007/s12648-017-1151-7

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  • DOI: https://doi.org/10.1007/s12648-017-1151-7

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