In the present manuscript, we have constructed an anisotropic solution for spherically
symmetric space-time that satisfies Karmarkar's condition in the context of f (R, T) theory of
gravity where R and T represent the Ricci scalar and the trace of Energy-momentum tensor,
respectively. In order to achieve our goal, we chose a one of the gravitational potentials
having regular behavior and obtained a closed form of the solution. This expression of the
gravitational potential enables the embedding equation to be solved and the field equations …