In three WIMP models, blind spots and loop corrections keep spin-independent scattering below current bounds and, in parts of parameter space, below the neutrino floor, while satisfying thermal relic density.
Snowmass2021 cosmic frontier dark matter direct detection to the neutrino fog,
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WIMPs Below the Radar: Blind Spots and Benchmarks Beyond the Neutrino Floor
In three WIMP models, blind spots and loop corrections keep spin-independent scattering below current bounds and, in parts of parameter space, below the neutrino floor, while satisfying thermal relic density.