pith. sign in

arxiv: 1504.00504 · v2 · pith:VKDNRNKQnew · submitted 2015-04-02 · ✦ hep-ph · hep-ex

Probing Bino-Gluino Coannihilation at the LHC

classification ✦ hep-ph hep-ex
keywords coannihilationbino-gluinodarkmatterscenariosusyabundanceactually
0
0 comments X
read the original abstract

It has been widely known that bino-like dark matter in the supersymmetric (SUSY) theories in general suffers from over-production. The situation can be drastically improved if gluinos have a mass slightly heavier than the bino dark matter as they reduce the dark matter abundance through coannihilation. In this work, we consider such a bino-gluino coannihilation scenario in high-scale SUSY models, which can be actually realized when the squark-mass scale is less than 100-1000 TeV. We study the prospects for exploring this bino-gluino coannihilation scenario at the LHC. We show that the searches for long-lived colored particles with displaced vertices offer a strong tool to test this scenario in collider experiments.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.