We derive a special of scalar field quintom potential using the isotropic flat Friedmann-Robertson-Walker cosmological model from canonical quantum cosmology under determined conditions in the evolution of our universe, using the Bohmian formalism. We obtain a family of potentials corresponding to the most probable to study the inflation phenomenon. Also we present exact solutions to the Wheeler-DeWitt equations in closed form.
This content is only available via PDF.
© 2012 American Institute of Physics.
2012
American Institute of Physics
You do not currently have access to this content.