Production of high-energy gravitinos during preheating

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We present a new technique for the calculation of helicity $\pm 1/2$ gravitino production during preheating. It is based on the equivalence between goldstinos and helicity $\pm 1/2$ 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.
4 pages, LaTeX, uses moriond.sty. Talk given at XXXVth Recontres de Moriond "Energy Densities in the Universe", Les Arcs, France, January 22-29, 2000

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