Gravitino thermal production revisited
Helmut Eberl, Ioannis D. Gialamas, Vassilis C. Spanos

TL;DR
This paper recalculates the gravitino production rate in the early universe, correcting previous errors and providing a new formula to estimate its abundance based on reheating temperature.
Contribution
It introduces a revised calculation of gravitino production, including previously overlooked processes, and offers a practical formula for cosmological applications.
Findings
Gravitino production rate is revised downward by nearly 10%.
New processes contributing to gravitino production are identified.
A convenient formula for gravitino abundance as a function of reheating temperature is provided.
Abstract
We calculate the gravitino production rate, computing its one-loop thermal self-energy. Gravitino production processes that do not result through thermal cuts of its self-energy, have been identified and taken into account. Correcting analytical errors and numerical approximations in the previous calculations, we present our result. This deviates from the latest estimation by almost 10%. More importantly, we provide a convenient formula, for calculating the gravitino production rate and its thermal abundance, as a function of the reheating temperature of the Universe.
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