English

Light-Gravitino Production at Hadron Colliders

High Energy Physics - Phenomenology 2009-08-25 v2

Abstract

We consider the production of gravitinos (G~\widetilde G) in association with gluinos (g~\tilde g) or squarks (q~\tilde q) at hadron colliders, including the three main sub-processes: qqˉ>g~G~q \bar q -> \tilde g\widetilde G, qg>q~G~qg -> \tilde q\widetilde G, and gg>g~G~gg -> \tilde g\widetilde G. These channels become enhanced to the point of being observable for sufficiently light gravitino masses (mG~<104eVm_{\widetilde G} < 10^{-4} eV), as motivated by some supersymmetric explanations of the CDF eeγγ+ET,missee\gamma\gamma+ E_{T,miss} event. The characteristic signal of such events would be monojets, as opposed to dijets obtained in the more traditional supersymmetric process ppˉ>g~g~p \bar p -> \tilde g\tilde g. Searches for such events at the Tevatron can impose lower limits on the gravitino mass. In the Appendix, we provide a complete set of Feynman rules for gravitino interactions used in our calculation.

Keywords

Cite

@article{arxiv.hep-ph/9707331,
  title  = {Light-Gravitino Production at Hadron Colliders},
  author = {Jaewan Kim and Jorge L. Lopez and D. V. Nanopoulos and Raghavan Rangarajan and A. Zichichi},
  journal= {arXiv preprint arXiv:hep-ph/9707331},
  year   = {2009}
}

Comments

25 pages, including 8 figures. Typeset in LaTex2e. Replaced with corrected figures, and some minor rewrites

R2 v1 2026-07-22T14:38:18.326Z