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Bianchi type-III minimally interacting holographic dark energy model with linearly varying deceleration parameter in Brans-Dicke theory

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Abstract

In this paper, we study the minimally interacting fields; matter and holographic dark energy components in Bianchi type-III space-time in the frame work of Brans-Dicke (Phys. Rev. 125:961, 1961) scalar-tensor theory of gravitation. We present a Bianchi type-III holographic dark energy model with the help of linearly varying deceleration parameter proposed by Akarsu and Dereli (Int. J. Theor. Phys. 51:612, 2012). Some physical and kinematical properties of the model are also discussed.

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Correspondence to D. R. K. Reddy.

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Kiran, M., Reddy, D.R.K. & Rao, V.U.M. Bianchi type-III minimally interacting holographic dark energy model with linearly varying deceleration parameter in Brans-Dicke theory. Astrophys Space Sci 360, 54 (2015). https://doi.org/10.1007/s10509-015-2563-5

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  • DOI: https://doi.org/10.1007/s10509-015-2563-5

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