Solar neutrino fluxes from dark matter annihilation differ by up to five to six orders of magnitude between the non-linear and linear Higgs portal models at high DM mass, which could discriminate the two frameworks.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
hep-ph 1years
2025 1verdicts
REJECT 1representative citing papers
citing papers explorer
-
Dark Matter signals in solar neutrinos fluxes as probe of non-linear symmetry breaking
Solar neutrino fluxes from dark matter annihilation differ by up to five to six orders of magnitude between the non-linear and linear Higgs portal models at high DM mass, which could discriminate the two frameworks.