Swampland, Axions and Minimal Warm Inflation
  Warm inflation has been noted previously as a possible way to implement
inflationary models compatible with the dS swampland bounds. But often in these
discussions the heat bath dynamics is kept largely unspecified. We point out
that the recently introduced Minimal Warm Inflation of arXiv:1910.07525, where
an axionic coupling of the inflaton leads to an explicit model for the thermal
bath, yields models of inflation that can easily fit cosmological observations
while satisfying de Sitter swampland bounds, as well as the swampland distance
bound and trans-Planckian censorship.
