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Bianchi Type-V Dark Energy Model in a Scalar-Tensor Theory of Gravitation

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Abstract

A spatially homogeneous and anisotropic Bianchi type-V universe with variable equation of state (EoS) parameter and constant deceleration parameter is obtained in a scalar-tensor theory of gravitation proposed by Saez and Ballester (Phys. Lett. A 113:467, 1986). The physical and kinematical properties of the universe have been discussed.

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Authors and Affiliations

  1. Department of Basic Science and Humanities, GMR Institute of Technology, Rajam, 532127, Andhra Pradesh, India

    R. L. Naidu & B. Satyanarayana

  2. Department of Science and Humanities, M. V. G. R. College of Engineering, Vizainagaram, Andhra Pradesh, India

    D. R. K. Reddy

Authors
  1. R. L. Naidu
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  2. B. Satyanarayana
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  3. D. R. K. Reddy
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Correspondence to R. L. Naidu.

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Naidu, R.L., Satyanarayana, B. & Reddy, D.R.K. Bianchi Type-V Dark Energy Model in a Scalar-Tensor Theory of Gravitation. Int J Theor Phys 51, 1997–2002 (2012). https://doi.org/10.1007/s10773-012-1078-x

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  • DOI: https://doi.org/10.1007/s10773-012-1078-x

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