  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.
