The Wheeler-DeWitt equation for a Robertson-Walker closed universe fil
led with an SU(2) Yang-Mills spatially uniform field is separable; we
are then led to impose on the wave function the usual rules for a quan
tum bound system: square integrability and orthogonality. We investiga
te the correspondence principle for large gravitational quantum number
s. The classical probability depends on the gauge chosen for the time,
and we examine lapse functions of the form N = N(alpha) (having in mi
nd cosmic time and conformal time). The correspondence principle holds
for these gauges if the differential representation of the momentum i
s gauge-dependent. This gives a prescription for the ordering of opera
tors in the Wheeler-DeWitt equation. We also discuss the measure in th
e minisuperspace needed to ensure invariance of matrix elements of gau
ge-invariant operators.