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    • Keywords


      Bianchi types-V space-time; $f(R, T)$ theory of gravity; modified holographic Ricci dark energy; deceleration parameter.

    • Abstract


      In the present paper,we studied the Bianchi type-V cosmological model in the presence of $f (R, T)$ Theory of Gravity using modified Holographic Ricci Dark Energy. To compute dynamical cosmological parameters, we used the relation between pressure and energy density $p_{\Lambda} = ω_{\Lambda} ρ_{\Lambda}$. We have also discussed the physical and geometrical properties of the model in detail.

    • Author Affiliations



      1. School of Mathematical Sciences, Swami Ramanand Teerth Marathwada University, Nanded 431606, India.
      2. Department of Mathematics, Govt. Vidarbha Institute of Science and Humanities, Amravati 444604, India.
    • Dates

  • Journal of Astrophysics and Astronomy | News

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      Posted on January 27, 2016

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