Super-Eddington AGN funnels accelerate hadrons by reconnection; pγ on disk photons yields 10–100 TeV neutrinos while winds absorb the gamma-ray counterpart, with NGC 7469 as a worked example.
Astroparticle Physics 177, 103214
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Neutrinos from super-Eddington Seyfert galaxies
Super-Eddington AGN funnels accelerate hadrons by reconnection; pγ on disk photons yields 10–100 TeV neutrinos while winds absorb the gamma-ray counterpart, with NGC 7469 as a worked example.