Composite Scalar Dark Matter
Michele Frigerio, Alex Pomarol, Francesco Riva, Alfredo Urbano
TL;DR
This work investigates a light scalar dark matter candidate η arising as a pseudo Nambu-Goldstone boson in a TeV-scale composite sector with an SO(6)/SO(5) symmetry breaking pattern. The Higgs is also a composite pNGB, and η interacts with the Standard Model through derivative couplings fixed by symmetry and explicit $U(1)_η$ breaking, controlled by four parameters $f$, $\,\lambda$, $c_t$, and $c_b$. The authors compute the relic density via the Boltzmann equation, analyze Higgs-width and coupling constraints from LHC, and compare to dark-matter direct-detection bounds, finding three predictive mass regions for viable DM: near the Higgs resonance at $m_η \approx m_h/2$, a heavier region $m_η \approx 100$–$500$ GeV dominated by derivative interactions, and a light region disfavored by theory and collider bounds. The model is highly predictive, tying EWSB and DM phenomenology, and will be decisively tested by upcoming direct-detection experiments and LHC precision Higgs measurements.
Abstract
We show that the dark matter (DM) could be a light composite scalar $η$, emerging from a TeV-scale strongly-coupled sector as a pseudo Nambu-Goldstone boson (pNGB). Such state arises naturally in scenarios where the Higgs is also a composite pNGB, as in $O(6)/O(5)$ models, which are particularly predictive, since the low-energy interactions of $η$ are determined by symmetry considerations. We identify the region of parameters where $η$ has the required DM relic density, satisfying at the same time the constraints from Higgs searches at the LHC, as well as DM direct searches. Compositeness, in addition to justify the lightness of the scalars, can enhance the DM scattering rates and lead to an excellent discovery prospect for the near future. For a Higgs mass $m_h\simeq 125$ GeV and a pNGB characteristic scale $f \lesssim 1$ TeV, we find that the DM mass is either $m_η\simeq 50-70$ GeV, with DM annihilations driven by the Higgs resonance, or in the range 100-500 GeV, where the DM derivative interaction with the Higgs becomes dominant. In the former case the invisible Higgs decay to two DM particles could weaken the LHC Higgs signal.
