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A modified holographic Ricci dark energy model in $f(R, T)$ theory of gravity
D. D. PAWAR R. V. MAPARI P. K. AGRAWAL
Volume 40 Issue 2 April 2019 Article ID 0013
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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.
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Author Affiliations
D. D. PAWAR1 R. V. MAPARI2 P. K. AGRAWAL1
- School of Mathematical Sciences, Swami Ramanand Teerth Marathwada University, Nanded 431606, India.
- Department of Mathematics, Govt. Vidarbha Institute of Science and Humanities, Amravati 444604, India.
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Dates
- Published
- 16 April 2019
- Manuscript received
- 5 September 2018
- Accepted
- 22 February 2019
- Final version published online
- 19 March 2019
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Journal of Astrophysics and Astronomy
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