  We analyze the quantum supersymmetric cosmological FRW model with a scalar
field, with a conditional probability density and the scalar field identified
as time. The Hilbert space has a spinorial structure and there is only one
consistent solution, with a conserved probability density. The dynamics of the
scale factor is obtained from its mean value. The uncertainty relations are
fulfilled and the corresponding fluctuations are consistent with a
semiclassical Universe. We give two examples which turn out to have negative
potential.
