“…Let consider the matter of a perfect fluid (WRS) n spacetime with isotropic pressure p, energy density σ, and velocity vector ρ is given by (X, ρ) = µ(X) for all X. Also, we know that there is no unique value of Lagrangian, therefore we assume that L m = −p and using (5) we turn up T(U, V) = p (U, V) + (σ + p)η(U)η(V), (33) where (ρ, ρ) = −1. Using (33), we can easily obtain the variation of stress energy in the following form…”