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.
Implication of neutrino backgrounds on the reach of next generation dark matter direct detection experiments,
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
citation-role summary
background 1
citation-polarity summary
fields
hep-ph 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
background 1representative citing papers
citing papers explorer
-
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.