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.

Topics
Cosmological model, Quantum cosmology, Scalar field theory, Wheeler-DeWitt equation
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© 2012 American Institute of Physics.
2012
American Institute of Physics
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