A modified holographic Ricci dark energy model in $f(R, T)$ theory of gravity
D. D. PAWAR R. V. MAPARI P. K. AGRAWAL
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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.
D. D. PAWAR1 R. V. MAPARI2 P. K. AGRAWAL1
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December 2019
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