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    • Fulltext

       

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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

       
      Published
      16 April 2019
      Manuscript received
      5 September 2018
      Accepted
      22 February 2019
      Final version published online
      19 March 2019

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

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