Turbulence-driven magnetic reconnection in the corona of NGC 1068 accelerates protons to ~10^14 eV, producing neutrinos via pp interactions that match IceCube data while gamma rays are attenuated by pair production.
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A Turbulence-Driven Magnetic Reconnection Model for the High-Energy Neutrino Emission from NGC 1068
Turbulence-driven magnetic reconnection in the corona of NGC 1068 accelerates protons to ~10^14 eV, producing neutrinos via pp interactions that match IceCube data while gamma rays are attenuated by pair production.