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.
Can we overcome the neutrino floor at high masses?,
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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.