Runaway potentials in warm inflation satisfying the swampland
  conjectures
  The runaway potentials, which do not possess any critical points, are viable
potentials which befit the recently proposed de Sitter swampland conjecture
very well. In this work, we embed such potentials in the warm inflation
scenario motivated by quantum field theory models generating a dissipation
coefficient with a dependence cubic in the temperature. It is demonstrated that
such models are able to remain in tune with the present observations and they
can also satisfy all the three Swampland conjectures, namely the Swampland
Distance conjecture, the de Sitter conjecture and the Transplackian Censorship
Conjecture, simultaneously. These features make such models viable from the
point of view of effective field theory models in quantum gravity and string
theory, away from the Swampland.
