TL;DR
This paper investigates W-boson and trident production in high-energy neutrino observatories, revealing their significant impact on neutrino interactions, attenuation, and detection signals, which are crucial for interpreting cosmic neutrino data.
Contribution
It provides the first comprehensive analysis of W-boson and trident production effects at TeV--PeV energies in neutrino observatories, highlighting their importance over previous assumptions.
Findings
W-boson production dominates neutrino interactions at high energies.
Cross sections can be up to 14% of charged-current deep-inelastic scattering.
Attenuation in Earth increases by up to 15%, affecting neutrino flux.
Abstract
Detecting TeV--PeV cosmic neutrinos provides crucial tests of neutrino physics and astrophysics. The statistics of IceCube and the larger proposed IceCube-Gen2 demand calculations of neutrino-nucleus interactions subdominant to deep-inelastic scattering, which is mediated by weak-boson couplings to nuclei. The largest such interactions are W-boson and trident production, which are mediated instead through photon couplings to nuclei. In a companion paper [1], we make the most comprehensive and precise calculations of those interactions at high energies. In this paper, we study their phenomenological consequences. We find that: (1) These interactions are dominated by the production of on-shell W-bosons, which carry most of the neutrino energy, (2) The cross section on water/iron can be as large as 7.5%/14% that of charged-current deep-inelastic scattering, much larger than the quoted…
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