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Five Dimensional Bulk Viscous String Cosmological Models in Saez and Ballester Theory of Gravitation

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Abstract

LRS Bianchi type-I bulk viscous string cosmological models are obtained in scalar tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). It is shown that cosmic string does not survive for ρ+λ=0 whereas it survives for the equations of state ρ=(1+ω)λ (Takabayasi string) and ρ=λ (Geometric string). Some physical and geometrical properties of the exhibited model are discussed.

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Acknowledgement

The authors would like to convey their sincere thanks to the anonymous reviewers for their useful comments and suggestions for the improvement of the paper.

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Authors and Affiliations

  1. Department of Mathematics, Birla Institute of Technology & Science-Pilani, K.K. Birla, Goa Campus, Zuarinagar, Goa, 403726, India

    G. C. Samanta

  2. Department of Physics, Gandhi Institute for Technological Advancement, Bhubaneswar, 752054, India

    S. K. Biswal

  3. Department of Mathematics, Birla Institute of Technology & Science-Pilani, Hyderabad Campus, Hyderabad, 500078, India

    P. K. Sahoo

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  1. G. C. Samanta
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  3. P. K. Sahoo
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Correspondence to P. K. Sahoo.

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Samanta, G.C., Biswal, S.K. & Sahoo, P.K. Five Dimensional Bulk Viscous String Cosmological Models in Saez and Ballester Theory of Gravitation. Int J Theor Phys 52, 1504–1514 (2013). https://doi.org/10.1007/s10773-012-1470-6

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  • DOI: https://doi.org/10.1007/s10773-012-1470-6

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