Super-Eddington black-hole winds colliding with broad-line-region clouds could produce detectable neutrino fluxes with weak electromagnetic counterparts.
Exploring accretion disk physics and black hole growth with regular monitoring of ultrafast active galactic nucleus winds
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Super-Accreting Active Galactic Nuclei as Neutrino Sources
Super-Eddington black-hole winds colliding with broad-line-region clouds could produce detectable neutrino fluxes with weak electromagnetic counterparts.