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LRS Bianchi Type-I Dark Energy Cosmological Model in Brans-Dicke Theory of Gravitation

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Abstract

Bianchi type-I dark energy model with variable equation of state (EoS) parameter is presented in a scalar-tensor theory of gravitation proposed by Brans and Dicke (Phys. Rev. 124:925, 1961). To get a determinate solution of the field equations we will take the help of special law of variation for Hubble’s parameter presented by Bermann (Nuovo Cimento B. 74:182, 1983) which yields a dark energy cosmological model with negative constant deceleration parameter. It is observed that this dark energy cosmological model always represents an accelerated and expanding universe and also consistent with the recent observations of type-Ia supernovae. Some physical and geometrical properties of the model are also discussed.

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Authors and Affiliations

  1. Department of Applied Mathematics, Andhra University, Visakhapatnam, A.P., India

    V. U. M. Rao, M. Vijaya Santhi & G. Sree Devi Kumari

  2. Department of Mathematics, GITAM University, Visakhapatnam, A.P., India

    T. Vinutha

Authors
  1. V. U. M. Rao
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  2. M. Vijaya Santhi
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  3. T. Vinutha
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  4. G. Sree Devi Kumari
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Correspondence to V. U. M. Rao.

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Rao, V.U.M., Vijaya Santhi, M., Vinutha, T. et al. LRS Bianchi Type-I Dark Energy Cosmological Model in Brans-Dicke Theory of Gravitation. Int J Theor Phys 51, 3303–3310 (2012). https://doi.org/10.1007/s10773-012-1210-y

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  • DOI: https://doi.org/10.1007/s10773-012-1210-y

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