  We study the formation of structure for a universe that undergoes a recent
loitering phase. We compare the nonlinear mass distribution to that in a
standard, matter dominated cosmology. The statistical aspects of the clustered
matter are found to be robust to changes in the expansion law, an exception
being that the peculiar velocities are lower by a factor of $\sim 3$ in the
loitering model. Further, in the loitering scenario, nonlinear growth of
perturbation occurs more recently ($z\sim 3-5$) than in the matter dominated
case. Differences in the high redshift appearances of the two models will
result but observable consequences depend critically on the chosen form, onset
and duration of the loitering phase.
