Light asymmetric dark matter from new strong dynamics
Mads T. Frandsen, Subir Sarkar, Kai Schmidt-Hoberg
TL;DR
This work develops a mechanism to generate light asymmetric dark matter via two-scale strong dynamics linked to dynamical electroweak symmetry breaking. By introducing S1 and S2 sectors with scales $\Lambda_1$ and $\Lambda_2$ and a shared global $U(1)_{\mathrm{TB}}$, it shows how a dark baryon–like state and a GeV-scale ADM $\chi$ can inherit a common asymmetry through sphaleron processes, yielding $\Omega_\chi$ compatible with $\Omega_B$ through $\Omega_\chi = \frac{m_\chi \mathcal{N}_\chi}{m_B \mathcal{N}_B}\,\Omega_B$, with $m_\chi \approx 5$ GeV. Scale separation $\Lambda_1/\Lambda_2$ can be large, aided by four-fermion (gauged-NJL) interactions that lower the critical coupling $\alpha_c$ and extend the conformal window, enabling substantial separation while breaking EW at the correct scale. The model predicts testable phenomenology, including sizable self-interactions and potentially detectable spin-independent scattering cross-sections $\sigma \sim g_\chi^2 g_q^2 \frac{\mu^2}{m^4}$ for mediators with $m \sim 5$–$15$ GeV and $g_q \sim \Lambda_2/\Lambda_1 \lesssim 10^{-4}$, offering avenues for direct detection and collider signals from the technicolor sector.
Abstract
A ~5 GeV `dark baryon' with a cosmic asymmetry similar to that of baryons is a natural candidate for the dark matter. We study the possibility of generating such a state through dynamical electroweak symmetry breaking, and show that it can share the relic baryon asymmetry via sphaleron interactions, even though it has no electroweak interactions. The scattering cross-section on nucleons, estimated in analogy to QCD, is within reach of underground direct detection experiments.
