TL;DR
This paper explores a singlet-extended 2 Higgs doublet model that can naturally accommodate pseudo-Nambu-Goldstone dark matter, satisfying various experimental constraints and potentially explaining observed astrophysical and collider excesses.
Contribution
It demonstrates the viability of pNG dark matter within the S2HDM framework using a genetic algorithm to identify parameter regions consistent with all constraints.
Findings
S2HDM can reproduce the observed dark matter relic abundance.
The model can potentially explain galactic center and antiproton excesses.
A Higgs boson around 96 GeV may account for LEP and CMS excesses.
Abstract
We investigate a possible realization of pseudo-Nambu-Goldstone (pNG) dark matter in the framework of a singlet-extended 2 Higgs doublet model (S2HDM). pNG dark matter gained attraction due to the fact that direct-detection constraints can be avoided naturally because of the momentum-suppressed scattering cross sections, whereas the relic abundance of dark matter can nevertheless be accounted for via the usual thermal freeze-out mechanism. We confront the S2HDM with a multitude of theoretical and experimental constraints, paying special attention to the theoretical limitations on the scalar potential, such as vacuum stability and perturbativity. In addition, we discuss the complementarity between constraints related to the dark matter sector, on the one hand, and to the Higgs sector, on the other hand. In our numerical discussion we explore the Higgs funnel region with dark matter…
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