Absorption of Fermionic Dark Matter via the Scalar Portal

Abstract

The absorption of fermionic dark matter has recently been studied as a signature for the direct detection of dark matter. We construct the first UV completion of the scalar effective operator associated with this signature. We calculate the constraints on the model and demonstrate there is viable parameter space which can be probed by a next-generation experiment such as XLZD. We also consider the cosmological history of our model and show that the correct relic abundance can be obtained via freeze-out in the dark sector. However, within this minimal model, we find that the absorption signal is highly suppressed in the parameter space that yields the correct relic abundance.

arXiv comment11 pages, 8 figures. v2: stellar/SN bounds updated, journal version

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Cited by in corpus (1)

• The Non-Relativistic Effective Field Theory Of Dark Matter-Electron Interactions