Some Anisotropic Dark Energy model in Five Dimensional Bianchi Type-V Space-time

Abstract

Five dimensional Bianchi type-V space-time has been considered with the introduction of four different skewness parameters along spatial directions to quantify the deviation of pressure from isotropy. We have assumed that the four skewness parameters are time dependent to study the anisotropic nature of the dark energy which has the dynamical energy density. For the phantom model it is found that the Universe achieves the flatness. The physical properties of the Universe has also been discussed in this paper.