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Axially Symmetric Cosmological Model with Bulk Stress in Saez-Ballester Theory of Gravitation

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Abstract

An Axially symmetric non-static space time is considered in presence of bulk stress in scalar tensor theory formulated by Saez and Ballester (Phys. Lett. A113, 467 1985). For solving the field equations, relation between metric potential and shear velocity is proportional to scale expansion are used. Also various physical and geometrical properties of the model have been discussed.

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Acknowledgments

We are grateful to the referee for his/her valuable comments which we found very essential and useful in revising the paper.

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Authors and Affiliations

  1. Department of Mathematics, R.D.I.K. and K.D. College, Badnera - Amravati, India

    V. G. Mete

  2. Department of Mathematics, Shri. Dr. R.G. Rathod Arts and Science College, Murtizapur Dist., Akola, India

    A. S. Nimkar

  3. Department of Mathematics, J.D.Patil Sangludkar Mahavidyalaya, Daryapur, Dist. Amravati, India

    V. D. Elkar

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  1. V. G. Mete
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  2. A. S. Nimkar
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  3. V. D. Elkar
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Correspondence to V. G. Mete.

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Mete, V.G., Nimkar, A.S. & Elkar, V.D. Axially Symmetric Cosmological Model with Bulk Stress in Saez-Ballester Theory of Gravitation. Int J Theor Phys 55, 412–420 (2016). https://doi.org/10.1007/s10773-015-2675-2

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  • DOI: https://doi.org/10.1007/s10773-015-2675-2

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