If the gravitino is sufficiently light and stable it will behave as an
effective massless neutrino species at the time of nucleosynthesis. D
epending on the temperature at which it decouples from the thermal bat
h in the early universe, the gravitino mass will be bounded by the pri
mordial He-4 abundance, Assuming a conservative estimate that the numb
er of neutrino families, N-nu < 3.6, superlight gravitinos with a mass
m(3/2) less than or similar to 10(-6) eV are ruled out, This bound is
weaker than previous estimates because the Goldstino annihilation cro
ss section was overestimated.