Production of high-energy gravitinos during preheating

We present a new technique for the calculation of helicity $\pm 1\mathrm{/}2$ gravitino production during preheating. It is based on the equivalence between goldstinos and helicity $\pm 1\mathrm{/}2$ gravitinos at high energies. The problem is thus reduced to the standard (Majorana) fermion production after inflation. Comparison with the results obtained in the unitary gauge is also presented.