The behaviour of quantum metric perturbations produced during inflatio
n is considered at the stage after the second Hubble radius crossing.
It is shown that the classical correlation between amplitude and momen
tum of a perturbation mode, previously shown to emerge in the course o
f an effective quantum-to-classical transition, is maintained for a. s
ufficiently long time, and we present the explicit form it takes using
the Wigner function. We further show with a simple diffraction experi
ment that quantum interference, non-expressible in terms of a classica
l stochastic description of the perturbations, is essentially suppress
ed. Rescattering of the perturbations leads to a comparatively slow de
cay of this correlation and to a complete stochastization of the syste
m.