  We study inflation in a random multifield potential, using techniques
developed by Marsh et al. The potential is a function of a large number of
fields, and we choose parameters so that inflation only occurs in regions where
the potential is accidentally flat. Using an improved estimate for the dynamics
of eigenvalue repulsion, we are able to describe the steepening of the
potential as inflation progresses. We provide suggestive arguments, but not a
proof, that the resulting scalar power spectrum generically disagrees with
observations. We also point out two problematic aspects of the model: there is
no well-defined probability distribution for the gradient of the potential, and
the evolution of the potential over small distances in field space is
unphysical.
