Abstract
In the present paper, we studied the Bianchi type-V cosmological model in the presence of \(f\left( {R,T} \right) \) Theory of Gravity using modified Holographic Ricci Dark Energy. To compute dynamical cosmological parameters, we used the relation between pressure and energy density \(p_\Lambda =\omega _\Lambda \rho _\Lambda \). We have also discussed the physical and geometrical properties of the model in detail.
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The authors are thankful to the anonymous referee for his/her constructive comments which helped to improve the quality of research paper.
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Pawar, D.D., Mapari, R.V. & Agrawal, P.K. A modified holographic Ricci dark energy model in f (R, T) theory of gravity. J Astrophys Astron 40, 13 (2019). https://doi.org/10.1007/s12036-019-9582-5
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DOI: https://doi.org/10.1007/s12036-019-9582-5