  In this talk we present a new calculation of the gravitino production rate,
using its full one-loop corrected thermal self-energy, beyond the hard thermal
loop approximation. Gravitino production $2 \to 2$ processes, that are not
related to its self-energy have been taken properly into account. Our result,
compared to the latest estimation, differs by almost 10%. In addition, we
present a handy parametrization of our finding, that can be used to calculate
the gravitino thermal abundance, as a function of the reheating temperature.
