English

Direct Detection of Non-Chiral Dark Matter

High Energy Physics - Phenomenology 2009-09-17 v2

Abstract

Direct detection experiments rule out fermion dark matter that is a chiral representation of the electroweak gauge group. Non-chiral real, complex and singlet representations, however, provide viable fermion dark matter candidates. Although any one of these candidates will be virtually impossible to detect at the LHC, it is shown that they may be detected at future planned direct detection experiments. For the real case, an irreducible radiative coupling to quarks may allow a detection. The complex case in general has an experimentally ruled out tree-level coupling to quarks via Z-boson exchange. However, in the case of two SU(2)_L doublets, a higher dimensional coupling to the Higgs can suppress this coupling, and a remaining irreducible radiative coupling may allow a detection. Singlet dark matter could be detected through a coupling to quarks via Higgs exchange. Since all non-chiral dark matter can have a coupling to the Higgs, at least some of its mass can be obtained from electroweak symmetry breaking, and this mass is a useful characterization of its direct detection cross-section.

Keywords

Cite

@article{arxiv.0710.1668,
  title  = {Direct Detection of Non-Chiral Dark Matter},
  author = {Rouven Essig},
  journal= {arXiv preprint arXiv:0710.1668},
  year   = {2009}
}

Comments

22 pages, 3 figures. References added. Minor corrections to match published version

R2 v1 2026-06-21T09:28:44.879Z