We estimate the production of gravitinos during and after the end of a peri
od of warm inflation, a model in which radiation is produced continuously a
s the field rolls down the potential producing dissipation. We find that gr
avitino production is efficient for models in the strong dissipation regime
, with the result that standard nucleosynthesis is disrupted unless the mag
nitude of the inflaton potential is very small. Combining this with the con
straint from the thermal production of adiabatic density perturbations, we
find the dissipation rate must be extraordinarily strong, or that the poten
tial is very flat.