NGC 1068's IceCube neutrinos are attributed to non-thermal particle acceleration in the black hole corona, with coronal parameters derived from a millimeter excess and a testable MeV gamma-ray prediction.
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On the Origin of High Energy Neutrinos from NGC 1068: The Role of Non-Thermal Coronal Activity
NGC 1068's IceCube neutrinos are attributed to non-thermal particle acceleration in the black hole corona, with coronal parameters derived from a millimeter excess and a testable MeV gamma-ray prediction.