  We discuss the construction of wave packets resulting from the solutions of a
class of Wheeler-DeWitt equations in Robertson-Walker type cosmologies. We
present an ansatz for the initial conditions which leads to a unique
determination of the expansion coefficients in the construction of the wave
packets with probability distributions which, in an interesting contrast to
some of the earlier works, agree well with all possible classical paths. The
possible relationship between these initial conditions and signature transition
in the context of classical cosmology is also discussed.
