In this paper we have studied five-dimensional Bianchi type-V spacetime in the f (R,T) theory. To solve Einstein’s field equations, we have assumed that the Hubble parameter is inversely proportional toݎ ℎݐ power of the scale factor i.e.
H 1/r. We have obtained a singular model for r 0, non-singular model for r=0. The physical behavior of the models has also been discussed using some physical parameters.
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K. K. ; A. Singh, "Higher Dimensional Bianchi V Models in f (R,T) Theory with Perfect Fluid Distribution", Journal of Ultra Scientist of Physical Sciences, Volume 35, Issue 6, Page Number 54-67, 2023Copy the following to cite this URL:
K. K. ; A. Singh, "Higher Dimensional Bianchi V Models in f (R,T) Theory with Perfect Fluid Distribution", Journal of Ultra Scientist of Physical Sciences, Volume 35, Issue 6, Page Number 54-67, 2023Available from: https://www.ultrascientist.org/paper/1583/