English

Colored Dark Matter

High Energy Physics - Phenomenology 2019-02-04 v3 Cosmology and Nongalactic Astrophysics Nuclear Theory

Abstract

We explore the possibility that Dark Matter is the lightest hadron made of two stable color octet Dirac fermions Q{\cal Q}. The cosmological DM abundance is reproduced for MQ12.5M_{\cal Q}\approx 12.5 TeV, compatibly with direct searches (the Rayleigh cross section, suppressed by 1/MQ61/M_{\cal Q}^6, is close to present bounds), indirect searches (enhanced by QQ+QˉQˉQQˉ+QQˉ{\cal Q}{\cal Q}+\bar{\cal Q}\bar{\cal Q}\to {\cal Q}\bar{\cal Q}+{\cal Q}\bar{\cal Q} recombination), and with collider searches (where Q{\cal Q} manifests as tracks, pair produced via QCD). Hybrid hadrons, made of Q\cal Q and of SM quarks and gluons, have large QCD cross sections, and do not reach underground detectors. Their cosmological abundance is 10510^5 times smaller than DM, such that their unusual signals seem compatible with bounds. Those in the Earth and stars sank to their centers; the Earth crust and meteorites later accumulate a secondary abundance, although their present abundance depends on nuclear and geological properties that we cannot compute from first principles.

Keywords

Cite

@article{arxiv.1801.01135,
  title  = {Colored Dark Matter},
  author = {Valerio De Luca and Andrea Mitridate and Michele Redi and Juri Smirnov and Alessandro Strumia},
  journal= {arXiv preprint arXiv:1801.01135},
  year   = {2019}
}

Comments

36 pages, 7 figures. v3: improved computation of the relic abundance; revised estimate of the indirect detection cross section

R2 v1 2026-06-22T23:35:48.125Z