AGN evolution produces the IceCube neutrino spectral break through superposition of contributions from active and post-active phases, with host galaxies acting as efficient cosmic-ray reservoirs.
The blazar PKS 0605-085 as the origin of the KM3-230213A neutrino event
2 Pith papers cite this work. Polarity classification is still indexing.
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Phenomenological study predicting incomplete tau polarization at FASER2, observable neutrino and muon trident processes, and contributions to hadron structure from IceCube neutrino events.
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Does the spectral break in the IceCube diffuse neutrino spectrum originate from AGN evolution?
AGN evolution produces the IceCube neutrino spectral break through superposition of contributions from active and post-active phases, with host galaxies acting as efficient cosmic-ray reservoirs.
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Lepton interactions from GeV to EeV
Phenomenological study predicting incomplete tau polarization at FASER2, observable neutrino and muon trident processes, and contributions to hadron structure from IceCube neutrino events.