What do the highest-energy cosmic-ray data suggest about possible new physics around 50 TeV?
Vasiliki Pavlidou, Theodore Tomaras

TL;DR
This paper proposes a new physics model around 50 TeV that explains ultra-high-energy cosmic-ray data by suggesting a change in particle interactions leading to increased shower multiplicity, challenging standard extrapolations.
Contribution
It introduces a minimal model predicting a new physics effect at 50 TeV that aligns with observed cosmic-ray shower data and suggests a high probability of detection at accelerators.
Findings
Model fits Auger data well
Predicts a high-energy threshold around 50 TeV
Indicates a light composition at highest energies
Abstract
The latest observations of extensive air showers (EAS) induced by ultra-high-energy cosmic rays (UHECR) appear to indicate, prima facie, a transition to heavy primaries at the highest energies. However, this interpretation, which is based on extrapolations of the Standard Model (SM) to ultra-LHC energies, is strained from both astrophysical and particle phenomenology perspectives. We consider the alternative that after some energy threshold, the first collision of the primary in the atmosphere results in a state, the decay of which leads to a considerably increased shower particle multiplicity, so that light-primary EAS appear heavy-like. We show that a minimal implementation of such a model yields predictions for the average EAS depth and shower-to-shower fluctuations that are consistent with each other, and an excellent fit to Auger data. If such an effect indeed takes place, we…
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