Warm Inflation in the light of Swampland Criteria
  Warm Inflation seems to be the most befitting single-field slow-roll
inflation scenario in the context of the recently proposed Swampland Criteria.
We investigate the constraints these Swampland Criteria impose on Warm
Inflation parameters and show that Warm Inflation is in accordance with both
the current cosmological observations and the proposed Swampland Criteria in
both weak and strong dissipative regimes depending on the value of the
parameter $c$ which limits the slope of the inflaton potential according to the
criteria.
