On the Thermal Regeneration Rate for Light Gravitinos in the Early Universe
arXiv:hep-ph/9505438 · doi:10.1016/0927-6505(96)00006-0
Abstract
We investigate the light gravitino regeneration rate in the early Universe in models based on supergravity. Motivated by a recent claim by Fischler, we evaluate finite-temperature effects on the gravitino regeneration rate due to the hot primordial plasma for a wide range of the supersymmetry-breaking scale . We find that thermal corrections to the gravitino pole mass and to the Goldstino coupling are negligible for a wide range of temperatures, thereby justifying the extension of the equivalence theorem for the helicity-1/2 gravitino and Goldstino to a hot primordial plasma background. Utilizing the Braaten-Pisarski resummation method, the helicity-1/2 gravitino regeneration rate is found to be up to a calculable, model-dependent numerical factor. We review the implications of this regeneration rate for supergravity cosmology, focusing in particular on scenaria for baryogenesis.
REVTEX 32 pages, two encapsulated ps figure files
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