Catastrophic Production of Slow Gravitinos
Edward W. Kolb, Andrew J. Long, and Evan McDonough

TL;DR
This paper investigates the catastrophic gravitational production of slow gravitinos in cosmological spacetimes, revealing divergences linked to vanishing sound speed and discussing implications for effective field theories and string theory UV completions.
Contribution
It uncovers conditions leading to divergent gravitino production, analyzes supergravity models' behavior, and proposes the Gravitino Swampland Conjecture connecting to string theory.
Findings
Catastrophic gravitino production occurs for masses below the Hubble rate.
UV cutoff dominates the produced particle spectrum, indicating EFT breakdown.
Some supergravity models avoid the catastrophe, others do not.
Abstract
We study gravitational particle production of the massive spin- Rarita-Schwinger field, and its close relative, the gravitino, in FRW cosmological spacetimes. For masses lighter than the value of the Hubble expansion rate after inflation, , we find catastrophic gravitational particle production, wherein the number of gravitationally produced particles is divergent, caused by a transient vanishing of the helicity-1/2 gravitino sound speed. In contrast with the conventional gravitino problem, the spectrum of produced particles is dominated by those with momentum at the UV cutoff. This suggests a breakdown of effective field theory, which might be cured by new degrees of freedom that emerge in the UV. We study the UV completion of the Rarita-Schwinger field, namely , , supergravity. We reproduce known results for models with a single superfield and…
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