Final state radiation from high and ultrahigh energy neutrino interactions
Ryan Plestid, Bei Zhou

TL;DR
This paper investigates how final state radiation from charged leptons produced in high-energy neutrino interactions affects detection and measurement, with implications for neutrino telescopes, flavor identification, and collider experiments.
Contribution
It provides a detailed analysis of the impact of final state radiation on neutrino detection, flux measurements, and collider physics, emphasizing the need to include these effects in future analyses.
Findings
Final state radiation can increase detectable energy by up to 20%.
It affects flavor measurements and tau neutrino energy estimates.
Impacts the extraction of strange quark PDFs at the LHC's Forward Physics Facility.
Abstract
Charged leptons produced by high-energy and ultrahigh-energy neutrinos have a substantial probability of emitting prompt internal bremsstrahlung . This can have important consequences for neutrino detection. We discuss observable consequences at high- and ultrahigh-energy neutrino telescopes and the Large Hadron Collider's Forward Physics Facility. Logarithmic enhancements can be substantial (e.g., ) when either the charged lepton's energy or the rest of the cascade is measured. We comment on final state radiation's impacts on measuring the inelasticity distribution, flux ratio, throughgoing muons, and double-bang signatures for high-energy neutrino observation. Furthermore, for ultrahigh-energy neutrino observation, we find that final state radiation increases the overall detectable energy by as much as 20\%,…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies · Neutrino Physics Research
