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Modified Renyi Holographic Dark Energy (MRHDE) in f(R, T) Theory of Gravity.
- Source :
-
Astrophysics . Dec2021, Vol. 64 Issue 4, p512-528. 17p. - Publication Year :
- 2021
-
Abstract
- In this work, we investigate the dynamics of Bianchi type VI0 space-time in the framework of f(R, T) theory of gravity where R stands for Ricci scalar and T stands for the trace of the stress energy-momentum tensor with Modified Renyi Holographic Dark Energy (MRHDE). With the specific choice of the functional f(R, T) = f1(R) + f2 (T) = μ1R+ μ2T where f1(R) and f2 (T) are arbitrary functions of R and T respectively and μ1 and μ2 are two parameters, we have obtained the exact solutions of the model by considering the energy density of MRHDE and by using a law of variation for the Hubble parameter H. It is found that our model leads to the accelerated expansion of the Universe. The EOS parameter ωDE > -1 DE indicates that our cosmological model behaves like a quintessence dark energy model which is consistent with the recent observations. A correspondence between MRHDE and quintessence dark energy is established. The quintessence dynamics of the potential and scalar field are reconstructed, which illustrates the late-time cosmic acceleration. All physical parameters are calculated and discussed graphically. [ABSTRACT FROM AUTHOR]
Details
- Language :
- English
- ISSN :
- 05717256
- Volume :
- 64
- Issue :
- 4
- Database :
- Academic Search Index
- Journal :
- Astrophysics
- Publication Type :
- Academic Journal
- Accession number :
- 153930158
- Full Text :
- https://doi.org/10.1007/s10511-021-09712-0