Salvage of Too Slow Gravitinos
Abstract
Gravitinos can inherit a non-relativistic dispersion relation while propagating in a background breaking both supersymmetry and Lorentz symmetry spontaneously. This is because the longitudinal mode velocity is controlled by the sound speed in the background. It was pointed out recently by Kolb, Long and McDonough that the production of gravitinos might diverge when this sound speed vanishes. We argue that in the framework of cosmological models with linearly spontaneously broken realised supersymmetry, where the physical fermions are combinations of the vacuum goldstino and the inflatino, the gravitino longitudinal mode has a relativistic dispersion relation and therefore avoids the catastrophic production. We illustrate this in some explicit examples.
Cite
@article{arxiv.2105.03784,
title = {Salvage of Too Slow Gravitinos},
author = {Ignatios Antoniadis and Karim Benakli and Wenqi Ke},
journal= {arXiv preprint arXiv:2105.03784},
year = {2022}
}
Comments
16 pages. This v2 matches the published version: one reference added and minor changes in the introduction