Trans-Planckian censorship and other swampland bothers addressed in warm
  inflation
  The implications of the recently proposed Trans-Planckian censorship
conjecture (TCC) are analyzed in the context of warm inflation. It is found
that for a single-stage accelerated expansion the constraints imposed by the
censorship are roughly the same as for cold inflation. Next, we study how a
two-stage inflationary expansion with an intermediate radiation-dominated era
can alleviate the bounds imposed by the censorship. For a demonstrative toy
model we found $r<10^{-23}$, but can be $r<10^{-5}$ for a weaker form of TCC
for the later stages of expansion, while still satisfying the other swampland
conditions.
