The model predicts a diffuse neutrino flux from AGN coronal current sheets that matches IceCube observations when the proton magnetization is fixed at 10^5.
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A hadronic model with two free parameters shows proton-photon interactions can supply enough pairs for observed coronal optical depths above a critical Eddington ratio, with neutrino luminosity scaling as L_X^2/L_Edd below and L_X above that threshold.
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Diffuse neutrino flux from coronal magnetospheric current sheets of accreting black holes
The model predicts a diffuse neutrino flux from AGN coronal current sheets that matches IceCube observations when the proton magnetization is fixed at 10^5.
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Neutrino and pair creation in reconnection-powered coronae of accreting black holes
A hadronic model with two free parameters shows proton-photon interactions can supply enough pairs for observed coronal optical depths above a critical Eddington ratio, with neutrino luminosity scaling as L_X^2/L_Edd below and L_X above that threshold.