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Emergent Scenario in Anisotropic Universe

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Abstract

In this work, we have considered that the anisotropic universe is filled with normal matter and phantom field (or tachyonic field). We have chosen the exponential forms of scale factors a and b in such a way that there is no singularity for evolution of the anisotropic universe. Here we have shown that the emergent scenario is possible for open, closed or flat universe if the universe contains phantom field or tachyonic field or phantom tachyonic field. From recently developed statefinder parameters, the behaviour of different stages of the evolution of the emergent universe have been generated.

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Authors and Affiliations

  1. Department of Mathematics, Seacom Engineering College, Howrah, 711 302, India

    Shuvendu Chakraborty

  2. Department of Mathematics, Bengal Engineering and Science University, Shibpur, Howrah, 711 103, India

    Ujjal Debnath

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  1. Shuvendu Chakraborty
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  2. Ujjal Debnath
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Correspondence to Ujjal Debnath.

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Chakraborty, S., Debnath, U. Emergent Scenario in Anisotropic Universe. Int J Theor Phys 50, 80–87 (2011). https://doi.org/10.1007/s10773-010-0495-y

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  • DOI: https://doi.org/10.1007/s10773-010-0495-y

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