  In an alternative mechanism recently proposed, adiabatic cosmological
perturbations are generated at the decay of the inflaton field due to small
fluctuations of its coupling to matter. This happens whenever the coupling is
governed by the vacuum expectation value of another field, which acquires
fluctuations during inflation. We discuss generalization and various possible
implementations of this mechansim, and present some specific particle physics
examples. In many cases the second field can start oscillating before
perturbations are imprinted, or survive long enough so to dominate over the
decay products of the inflaton. The primordial perturbations will then be
modified accordingly in each case.
