Freeze-in, early matter domination, and fast-expanding cosmologies keep many WIMP models within reach of next-generation direct detection experiments at the neutrino floor.
A prominent example is a DM candidate charged under SU (2)L with mass be- low 1 TeV, which would satisfy these requirements due to its enhanced annihilation cross-section
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Beyond the Veil: Charting WIMP Territories at the Neutrino Floor
Freeze-in, early matter domination, and fast-expanding cosmologies keep many WIMP models within reach of next-generation direct detection experiments at the neutrino floor.