  We consider inflationary scenarios of the supersymmetric quantum cosmology of
FRLW models with a scalar field. We use the superfield formalism with a
superpotential for the scalar superfield. The probability amplitude solution of
the supersymmetric Wheeler-DeWitt equation, gives a probability density from
which we can compute mean trajectories that can be parametrized by the scalar.
By suitable choices of the superpotential, the resulting evolutions of the
scale factor correspond to consistent inflationary scenarios. We show the
acceleration, the resulting $e$-folds and the horizon for several
superpotentials.
