Towards the bounce inflationary gravitational wave
  In bounce inflation scenario, the inflation is singularity-free, while the
advantages of inflation are reserved. We analytically calculate the power
spectrum of its primordial gravitational waves (GWs), and show a universal
result including the physics of the bounce phase. The spectrum acquires a
cutoff at large scale, while the oscillation around the cutoff scale is quite
drastic, which is determined by the details of bounce. Our work highlights that
the primordial GWs at large scale may encode the physics of the bounce ever
happened at about $\sim 60$ efolds before inflation.
