Dark matter from a complex scalar singlet: the role of dark CP and other discrete symmetries

We study the case of a pseudo-scalar dark matter candidate which emerges from a complex scalar singlet, charged under a global U(1) symmetry, which is broken both explicitly and spontaneously. The pseudo-scalar is naturally stabilized by the presence of a remnant discrete symmetry: dark CP. We study and compare the phenomenology of several simplified models with only one explicit symmetry breaking term. We find that several regions of the parameter space are able to reproduce the observed dark matter abundance while respecting direct detection and invisible Higgs decay limits: in the resonances of the two scalars, featuring the known as forbidden or secluded dark matter, and through non-resonant Higgs-mediated annihilations. In some cases, combining different measurements would allow one to distinguish the breaking pattern of the symmetry. Moreover, this setup admits a light DM candidate at the sub-GeV scale. We also discuss the situation where more than one symmetry breaking term is present. In that case, the dark CP symmetry may be spontaneously broken, thus spoiling the stability of the dark matter candidate. Requiring that this does not happen imposes a constraint on the allowed parameter space. Finally, we consider an effective field theory approach valid in the pseudo-Nambu-Goldstone boson limit and when the U(1) breaking scale is much larger than the electroweak scale.

Automated summary

In this study, we investigate a pseudo-scalar dark matter candidate arising from a complex scalar singlet charged under a global U(1) symmetry, stabilized by a remnant discrete symmetry dark CP. By analyzing simplified models with explicit symmetry breaking terms, we find various regions in parameter space can reproduce observed dark matter abundance while respecting detection and decay limits. Furthermore, different measurements may help distinguish symmetry breaking patterns, with the possibility of a light dark matter candidate at the sub-GeV scale.