XENON1T solar axion and the Higgs boson emerging from the dark

Abstract

In a recent letter we proposed a new non-thermal mechanism of Dark Matter production based on vacuum misalignment, where both the Higgs boson and a very light pseudo-scalar η emerge from the Dark sector. In this letter, we identify the parameter space in a composite scenario where the light pseudo-scalar can be produced in the sun and explain the XENON1T excess in electron recoil data. The model's Dark Matter candidate has a mass around 50 TeV and out of range for Direct Detection. Testable predictions include Gravitational waves at frequencies in the Hz range from a cosmological phase transition, an exotic decay Z γ + inv. with rates 4 16 · 10-12 testable at a future Tera-Z collider, and an enhancement by 17 40 % of the branching ratio KL π0 + inv., not enough to explain the KOTO anomaly. All these predictions may be confirmed by future experiments.

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