  If the reheating temperature at the end of inflation is low, of order 10 MeV,
then dark matter produced through ultraviolet freeze-in has a large direct
detection cross section. We study such a scenario in which dark matter is
hadrophilic. This leads to dark matter-nucleon scattering cross sections of
interest for near-future experiments for dark matter masses in the range of 100
keV-100 MeV. We explore how these predictions vary if reheating is
non-instantaneous.
