Bounce from Inflation
  We construct a class of viable bouncing models that are conformally related
to cosmological inflation. There are three main difficulties in constructing
such a model: (i) A stable (attractor) solution, (ii) A non-singular bounce,
and (iii) to bypass the no-go theorem that states that simultaneously
maintaining the observational bounds on the tensor-to-scalar ratio and the
non-Gaussian scalar spectrum are not possible. We show that a non-minimal
coupling of the scalar field helps to bypass these difficulties and provides a
viable bouncing model with a naturally occurring reheating epoch briefly after
the bouncing phase.
