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Magnetized Emergent Universe with Null Radiation Flow

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Abstract

In this paper, we study the Bianchi type-I cosmological model in a different basic form incorporating with null radiation flow with the perfect fluid in the presence as well as absence of a source free magnetic field. A set of new exact solutions of Einstein field equations are obtained in both the cases. We observe that the emergent universe model with null radiation flow approaches to de-sitter universe at late time obeying the same rate of expansion in presence and absence of the magnetic field.

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Authors and Affiliations

  1. Department of Mathematics, Netaji Subhas Institute of Technology, University of Delhi, Sector 3, Dwarka, New Delhi, 110078, India

    J. K. Singh & Sarita Rani

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  1. J. K. Singh
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  2. Sarita Rani
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Correspondence to Sarita Rani.

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Singh, J.K., Rani, S. Magnetized Emergent Universe with Null Radiation Flow. Int J Theor Phys 55, 232–240 (2016). https://doi.org/10.1007/s10773-015-2655-6

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  • DOI: https://doi.org/10.1007/s10773-015-2655-6

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