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Kantowski-Sacks Bulk Viscous String Cosmological Models in the Presence of Zero-Mass Scalar Fields

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Abstract

The Kantowski-Sachs cosmological solutions of massive strings have been studied in the presence of zero-mass scalar field coupled with bulk viscosity. It is assumed that the coefficient of bulk viscosity is a power function of energy density of massive strings. Further we have considered the cosmological parameter as a function of cosmic time. We obtained the general solution of the field equations in polynomial and exponential forms respectively. The behaviors of these models are also discussed in the presence as well as in the absence of bulk.

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Acknowledgements

The authors are grateful to the anonymous referee for his constructive comments which improve the quality of this paper.

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Authors and Affiliations

  1. GITAM School of Int’l Business, GITAM University, Visakhapatnam, 530045, India

    R. Venkateswarlu

  2. Vignan’s Institute of Engineering for Women, Visakhapatnam, 530046, India

    J. Satish

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Correspondence to R. Venkateswarlu.

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Venkateswarlu, R., Satish, J. Kantowski-Sacks Bulk Viscous String Cosmological Models in the Presence of Zero-Mass Scalar Fields. Int J Theor Phys 53, 1879–1895 (2014). https://doi.org/10.1007/s10773-013-1990-8

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