English

Composite Dark Sectors

High Energy Physics - Phenomenology 2015-06-02 v2 Cosmology and Nongalactic Astrophysics

Abstract

We introduce a new paradigm in Composite Dark Sectors, where the full Standard Model (including the Higgs boson) is extended with a strongly-interacting composite sector with global symmetry group G\mathcal{G} spontaneously broken to HG\mathcal{H}\subset \mathcal{G}. We show that, under well-motivated conditions, the lightest neutral pseudo Nambu-Goldstone bosons are natural dark matter candidates for they are protected by a parity symmetry not even broken in the electroweak phase. These models are characterized by only two free parameters, namely the typical coupling gDg_D and the scale fDf_D of the composite sector, and are therefore very predictive. We consider in detail two minimal scenarios, SU(3)/[SU(2)×U(1)]SU(3)/[SU(2)\times U(1)] and [SU(2)2×U(1)]/[SU(2)×U(1)][SU(2)^2\times U(1)]/[SU(2)\times U(1)], which provide a dynamical realization of the Inert Doublet and Triplet models, respectively. We show that the radiatively-induced potential can be computed in a five-dimensional description with modified boundary conditions with respect to Composite Higgs models. Finally, the dark matter candidates are shown to be compatible, in a large region of the parameter space, with current bounds from dark matter searches as well as electroweak and collider constraints on new resonances.

Keywords

Cite

@article{arxiv.1504.00332,
  title  = {Composite Dark Sectors},
  author = {Adrian Carmona and Mikael Chala},
  journal= {arXiv preprint arXiv:1504.00332},
  year   = {2015}
}

Comments

20 pages, 5 figures; v2; references added and Figure 4 corrected; matches published version in JHEP

R2 v1 2026-06-22T09:08:18.170Z