Quintom Potentials from Quantum Cosmology Using the FRW Cosmological Model

Abstract

We construct the quintom potential of dark energy models in the framework of spatially flat Friedmann-Robertson Walker universe in the inflationary epoch, using the Bohm like approach, known as amplitude-real-phase. We find some potentials for which the wave function of the universe is found analytically and we have obtained the classical trajectories in the inflation era. © 2013 Springer Science+Business Media New York.