English

Dark Freeze-out Cogenesis

High Energy Physics - Phenomenology 2022-03-08 v2 Cosmology and Nongalactic Astrophysics

Abstract

We propose a new mechanism where a multi-component dark sector generates the observed dark matter abundance and baryon asymmetry and thus addresses the coincidence between the two. The thermal freeze-out of dark matter annihilating into meta-stable dark partners sets the dark matter relic abundance while providing the out-of-equilibrium condition for baryogenesis. The meta-stable state triggers baryon asymmetry production by its decay well after the freeze-out and potentially induces a period of early matter domination before its decay. The dark matter and baryon abundances are related through number conservation within the dark sector (cogenesis). The "coincidence" is a natural outcome with GeV- to TeV-scale symmetric dark matter and the dark sector's interactions with the Standard Model quarks. We present a UV-complete model and explore its phenomenological predictions, including dark matter direct detection signals, LHC signatures of new massive particles with color charges and long-lived particles with displaced vertices, dark matter-induced nucleon conversions, (exotic) dark matter indirect detection signals, and effects on the cosmological matter power spectrum. As a side result, we provide a novel analytical treatment for dark sector freeze-out, which may prove useful in the study of related scenarios.

Keywords

Cite

@article{arxiv.2112.10784,
  title  = {Dark Freeze-out Cogenesis},
  author = {Xiaoyong Chu and Yanou Cui and Josef Pradler and Michael Shamma},
  journal= {arXiv preprint arXiv:2112.10784},
  year   = {2022}
}

Comments

31 pages, 13 figures, 1 appendix. References and minor comments added, conclusions unchanged, matches published version

R2 v1 2026-06-24T08:25:10.675Z