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      Permanent link:
      https://www.ias.ac.in/article/fulltext/joaa/040/02/0013

    • 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

       

      D. D. PAWAR1 R. V. MAPARI2 P. K. AGRAWAL1

      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

       
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