  Cyclic models of the universe have the advantage of avoiding initial
conditions problems related to postulating any sort of beginning in time. To
date, the only known viable examples of cyclic models have been ekpyrotic. In
this paper, we show that the recently proposed anamorphic scenario can also be
made cyclic. The key to the cyclic completion is a classically stable,
non-singular bounce. Remarkably, even though the bounce construction was
originally developed to connect a period of contraction with a period of
expansion both described by Einstein gravity, we show here that it can
naturally be modified to connect an ordinary contracting phase described by
Einstein gravity with a phase of anamorphic smoothing. The paper will present
the basic principles and steps in constructing cyclic anamorphic models.
