  Recently a mechanism was proposed whereby the primordial density
perturbations are generated at the end of inflation. We continue the analysis
of the proposed model of this mechanism and calculate the maximum extent to
which the density perturbations produced via this model can dominate over those
of the standard inflationary paradigm. In addition, we provide a
straightforward variation of this model which allows for greater amplification
of the density perturbations. Finally, we show that a variation in the
implementation of the original model results in significant non-gaussianities
in the resulting spectrum of density perturbations. The level of
non-gaussianities can be made to saturate the current observational bound.
