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Dynamics of Bianchi type-VI0 holographic dark energy models in general relativity and Lyra’s geometry

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Abstract

In this paper, we have studied the anisotropic and homogeneous Bianchi type-VI 0 Universe filled with dark matter and holographic dark energy components in the framework of general relativity and Lyra’s geometry. The Einstein’s field equations have been solved exactly by taking the expansion scalar (𝜃) in the model is proportional to the shear scalar (σ). Some physical and kinematical properties of the models are also discussed.

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Authors and Affiliations

  1. Department of Mathematics, Sant Gadge Baba Amravati University, Amravati, 444 602, India

    S D KATORE & D V KAPSE

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  1. S D KATORE
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  2. D V KAPSE
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Correspondence to D V KAPSE.

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KATORE, S.D., KAPSE, D.V. Dynamics of Bianchi type-VI0 holographic dark energy models in general relativity and Lyra’s geometry. Pramana - J Phys 88, 30 (2017). https://doi.org/10.1007/s12043-016-1338-z

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  • DOI: https://doi.org/10.1007/s12043-016-1338-z

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