Pseudo Nambu-Goldstone Boson DM with Linear Symmetry Breaking: Revisited

In this work, we revisit pseudo Nambu Goldstone boson (pNGB) DM model where global $U(1)$ dark symmetry is spontaneously broken as well as explicitly with broken by with linear symmetry breaking, focusing on the dark matter mass range in $500 {\rm GeV} \lesssim m_{\rm DM} \lesssim O(10)$ TeV. This model is interesting not only in its own in the context of pNGB DM, but also in the context of cosmological collider signatures from heavy particle mass regime without Boltzmann suppressions, $H \lesssim m_{\rm heavy} \lesssim 60 H$, through the chemical potential type interaction. After imposing perturbative unitarity, perturbativity, correct thermal relic density and constraints from colliders and (in)direct detection experiments, we find that pNGB DM mass is allowed up to $\sim 1 (10)$ TeV for the dark Higgs mass $m_{H_2} = 1 (100)$ TeV for the Higgs-dark Higgs mixing $\sin θ= 0.1$. We also consider the case where global $U(1)$ dark symmetry is not spontaneously broken, where DM is no longer pNGB. In this case, DM and dark Higgs masses are nearly degenerate in the range of a few TeV $\lesssim m_{{\rm DM}, H_2} \lesssim \sim 70$ TeV. Low mass region for pNGB DM and $H_2$ could be directly probed in colliders or indirect DM detections, whereas the heavy mass regime could be probed through the non-Gaussianity at the level of $f_{\rm NL} \sim O(0.01-10)$ if $H$ is as low as $O(1-10)$ TeV.

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