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- W4290635503 abstract "We obtain exact solutions to the field equations for 5 dimensional LRS Bianchi type-I spacetime in $f(R,T)$ theory of gravity where specifically the following three cases are considered: (i) $f(R,T)=mu(R+T)$, (ii) $f(R,T)=R mu + R T mu^2$ and (iii) $f(R,T)=R+mu R^2+mu T$ where $R$ and $T$ respectively the Ricci scalar and trace of the energy-momentum tensor. It is found that the equation of state (EOS) parameter $w$ is governed by the parameter $mu$ involved in the $f(R,T)$ expressions. We fine-tune the parameter $mu$ to obtain effect of phantom energy in the model, however we also restrict this parameter to obtain a stable model of the universe. It is noted that the model isotropizes at finite cosmic time." @default.
- W4290635503 created "2022-08-08" @default.
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- W4290635503 date "2022-08-08" @default.
- W4290635503 modified "2023-09-28" @default.
- W4290635503 title "Nonsingular phantom cosmology in Five Dimensional f(R,T) Gravity" @default.
- W4290635503 doi "https://doi.org/10.20944/preprints202208.0136.v1" @default.
- W4290635503 hasPublicationYear "2022" @default.
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