English

Slow and Safe Gravitinos

High Energy Physics - Theory 2021-06-16 v1 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology

Abstract

It has been argued that supergravity models of inflation with vanishing sound speeds, csc_s, lead to an unbounded growth in the production rate of gravitinos. We consider several models of inflation to delineate the conditions for which cs=0c_s = 0. In models with unconstrained superfields, we argue that the mixing of the goldstino and inflatino in a time-varying background prevents the uncontrolled production of the longitudinal modes. This conclusion is unchanged if there is a nilpotent field associated with supersymmetry breaking with constraint S2=0{\bf S^2} =0, i.e. sgoldstino-less models. Models with a second orthogonal constraint, S(ΦΦˉ)=0{\bf S(\Phi-\bar{\Phi})} =0, where Φ\bf{\Phi} is the inflaton superfield, which eliminates the inflatino, may suffer from the over-production of gravitinos. However, we point out that these models may be problematic if this constraint originates from a UV Lagrangian, as this may require using higher derivative operators. These models may also exhibit other pathologies such as cs>1c_s > 1, which are absent in theories with the single constraint or unconstrained fields.

Keywords

Cite

@article{arxiv.2104.03749,
  title  = {Slow and Safe Gravitinos},
  author = {Emilian Dudas and Marcos A. G. Garcia and Yann Mambrini and Keith A. Olive and Marco Peloso and Sarunas Verner},
  journal= {arXiv preprint arXiv:2104.03749},
  year   = {2021}
}

Comments

12 pages

R2 v1 2026-06-24T00:57:48.675Z