• Cosmic acceleration and stability of cosmological models in extended teleparallel gravity

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    • Keywords


      Locally rotationally symmetric Bianchi type-I space–time; modified holographic Ricci dark energy; $f (T )$ gravity; stability factor.

    • Abstract


      In this paper,we study themodel 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.

    • Author Affiliations



      1. Department of Mathematics, Indira Gandhi Mahavidyalaya, Ralegaon 445 402, India
      2. Department of Mathematics, Sant Gadge Baba Amravati University, Amravati 444 602, India
    • Dates

  • Pramana – Journal of Physics | News

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