Dynamical Analysis of Attractor Behavior in Constant Roll Inflation
  There has been considerable recent interest in a new class of non-slow roll
inflationary solutions known as \textit{constant roll} inflation. Constant roll
solutions are a generalization of the ultra-slow roll (USR) solution, where the
first Hubble slow roll parameter $\epsilon$ is small, but the second Hubble
slow roll parameter $\eta$ is not. While it is known that the USR solutions
represent dynamical transients, there has been some disagreement in literature
about whether or not large-$\eta$ constant roll solutions are attractors or are
also a class of transient solutions. In this paper we show that the
large-$\eta$ constant roll solutions do in fact represent transient solutions
by performing stability analysis on the exact analytic (large-$\eta$) constant
roll solutions.
