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Cosmic acceleration and stability of cosmological models in extended teleparallel gravity

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Abstract

In this paper, we study the model of f(T) gravity in the presence of dark matter and modified holographic Ricci dark energy (MHRDE) in locally rotationally symmetric (LRS) Bianchi type-I space–time. To achieve a physically realistic solution of the field equations, we have considered volumetric power and exponential expansion laws. We plot the corresponding cosmological parameters for dark energy components in terms of redshift; thereafter we investigate the accelerated expansion of the Universe. The physical and geometrical parameters of the models are also discussed in detail. The Statefinder diagnostic pair and jerk parameter are analysed to characterise completely different phases of the Universe.

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Acknowledgements

The authors are very much grateful to the honourable referees and the editor for the illuminating suggestions that have significantly improved our work in terms of research quality and presentation.

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Authors and Affiliations

  1. Department of Mathematics, Indira Gandhi Mahavidyalaya, Ralegaon, 445 402, India

    A Y Shaikh & S V Gore

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

    S D Katore

Authors
  1. A Y Shaikh
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  2. S V Gore
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  3. S D Katore
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Corresponding author

Correspondence to S V Gore.

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Shaikh, A.Y., Gore, S.V. & Katore, S.D. Cosmic acceleration and stability of cosmological models in extended teleparallel gravity. Pramana - J Phys 95, 16 (2021). https://doi.org/10.1007/s12043-020-02048-y

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  • DOI: https://doi.org/10.1007/s12043-020-02048-y

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