Nonsingular Phantom Cosmology in Five-Dimensional f(R, T) Gravity

We obtain exact solutions to the field equations for five-dimensional locally rotationally symmetric (LRS) Bianchi type-I spacetime in f(R,T) theory of gravity, where specifically, following three cases are considered: (i) f(R,T)=μ(R+T), (ii) f(R,T)=Rμ+RTμ2, and (iii) f(R,T)=R+μR2+μT, R T, respectively, Ricci scalar trace energy–momentum tensor. It is found that equation state (EOS) parameter w governed by μ involved expressions. fine-tune effect phantom energy model. However, we also restrict this a stable model universe.