English

A Study of Dirac Fermionic Dark Matters

High Energy Physics - Phenomenology 2013-08-28 v3 Cosmology and Nongalactic Astrophysics

Abstract

We study pure weak eigenstate Dirac fermionic dark matters (DM). We consider WIMP with renormalizable interaction. According to results of direct searches and the nature of DM (electrical neutral and being a pure weak eigenstate), the quantum number of DM is determined to be I3=Y=0I_3=Y=0. There are only two possible cases: either DM has non-vanishing weak isospin (I0I\neq 0) or it is an isosinglet (I=0). In the first case, the Sommerfeld enhancement is sizable for large II, producing large χ0χ0ˉVV\chi^0\bar{\chi^0}\to VV rates. In particular, we obtain large χχˉW+W\chi\bar\chi\to W^+ W^- cross section, which is comparable to the latest bounds from indirect searches and mχm_\chi is constrained to be larger than few hundred GeV to few TeV. It is possible to give correct relic density with mχm_\chi higher than these lower bounds. In the second case, to couple DM to standard model (SM) particles, a SM-singlet vector mediator XX is required from renormalizability and the SM gauge quantum numbers. To satisfy the latest bounds of direct searches and to reproduce the DM relic density at the same time, resonant enhancement in DM annihilation diagram is needed. Thus, the masses of DM and the mediator are related. Furthermore, this model is not sufficient to explain the deviation in muon g2g-2.

Keywords

Cite

@article{arxiv.1305.7008,
  title  = {A Study of Dirac Fermionic Dark Matters},
  author = {Chun-Khiang Chua and Ron-Chou Hsieh},
  journal= {arXiv preprint arXiv:1305.7008},
  year   = {2013}
}

Comments

17 pages, 6 figures, version to appear in Phys. Rev. D

R2 v1 2026-06-22T00:24:59.751Z