Quintom potentials from quantum cosmology using the FRW cosmological model
arXiv:1305.1640 · doi:10.1007/s10773-013-1565-8
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.
Latex2e, 10 pages, 1 figure