Composite Dark Sectors

TL;DR

This paper proposes a new class of composite dark matter models where the Standard Model is extended with a strongly-interacting sector, predicting natural dark matter candidates protected by symmetries, and compatible with current experimental bounds.

Contribution

Introduction of a novel framework for composite dark sectors with minimal parameters, providing explicit models and detailed phenomenological analysis.

Findings

Dark matter candidates are stable due to parity symmetry.

Models are compatible with current dark matter search constraints.

The potential can be computed using a five-dimensional approach.

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 $\mathcal{G}$ spontaneously broken to $\mathcal{H}\subset \mathcal{G}$. 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 $g_D$ and the scale $f_D$ of the composite sector, and are therefore very predictive. We consider in detail two minimal scenarios, $SU(3)/[SU(2)\times U(1)]$ and $[SU(2)^2\times U(1)]/[SU(2)\times U(1)]$, 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.