English

Distinctive signals of frustrated dark matter

High Energy Physics - Phenomenology 2022-09-27 v2 Cosmology and Nongalactic Astrophysics

Abstract

We study a renormalizable model of Dirac fermion dark matter (DM) that communicates with the Standard Model (SM) through a pair of mediators -- one scalar, one fermion -- in the representation (6,1,43)(\boldsymbol{6},\boldsymbol{1}, \tfrac{4}{3}) of the SM gauge group SU(3)c×SU(2)L×U(1)Y\text{SU}(3)_{\text{c}} \times \text{SU}(2)_{\text{L}} \times \text{U}(1)_Y. While such assignments preclude direct coupling of the dark matter to the Standard Model at tree level, we examine the many effective operators generated at one-loop order when the mediators are heavy, and find that they are often phenomenologically relevant. We reinterpret dijet and pair-produced resonance and jets+ETmiss\text{jets} + E_{\text{T}}^{\text{miss}} searches at the Large Hadron Collider (LHC) in order to constrain the mediator sector, and we examine an array of DM constraints ranging from the observed relic density ΩχhPlanck2\Omega_{\chi} h^2_{\text{Planck}} to indirect and direct searches for dark matter. Tree-level annihilation, available for DM masses starting at the TeV scale, is required in order to produce ΩχhPlanck2\Omega_{\chi} h^2_{\text{Planck}} through freeze-out, but loops -- led by the dimension-five DM magnetic dipole moment -- are nonetheless able to produce signals large enough to be constrained, particularly by the XENON1T experiment. In some benchmarks, we find a fair amount of parameter space left open by experiment and compatible with freeze-out. In other scenarios, however, the open space is quite small, suggesting a need for further model-building and/or non-standard cosmologies.

Keywords

Cite

@article{arxiv.2205.06824,
  title  = {Distinctive signals of frustrated dark matter},
  author = {Linda M. Carpenter and Taylor Murphy and Tim M. P. Tait},
  journal= {arXiv preprint arXiv:2205.06824},
  year   = {2022}
}

Comments

37 pages, 19 figures. Updated to resemble JHEP Version of Record