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Neutrino Interactions at Ultrahigh Energies
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abstract
We report new calculations of the cross sections for deeply inelastic neutrino-nucleon scattering at neutrino energies between $10^{9}\ev$ and $10^{21}\ev$. We compare with results in the literature and assess the reliability of our predictions. For completeness, we briefly review the cross sections for neutrino interactions with atomic electrons, emphasizing the role of the $W$-boson resonance in $\bar{\nu}_{e}e$ interactions for neutrino energies in the neighborhood of $6.3\pev$. Adopting model predictions for extraterrestrial neutrino fluxes from active galactic nuclei, gamma-ray bursters, and the collapse of topological defects, we estimate event rates in large-volume water \v{C}erenkov detectors and large-area ground arrays.
Forward citations
Cited by 5 Pith papers
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Little Red Dots as Hidden Neutrino Sources
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Four, One, and None: Quantifying the Ultra-High-Energy Neutrino Anomaly Across ANITA-IV, KM3NeT, and IceCube
A joint three-detector analysis finds that ANITA-IV's four events and KM3NeT's 220 PeV event cannot be reconciled with IceCube's silence under any Standard Model diffuse or transient flux, leaving a 5.9-7.9σ anomaly.
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Using a line-of-sight transport formalism, the paper finds a 3.1 sigma tension between the KM3NeT ultra-high-energy event and IceCube non-observation under a diffuse power-law flux, with stronger tension for steady po...
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