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.
Chung,Composite flavon-higgs models,Physical Review D104(2021) 095011
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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.