Using higher moments of air-shower depth distributions, the authors project that the full Pierre Auger dataset could reject the EPOS and Sibyll hadronic models at high confidence.
We denote theselectedeventsas {( ˜Ei, ˜Xmax,i, δ˜Xmax,i)}ℓ, with i = 1,
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Ultra High Energy Cosmic Rays versus Models of High Energy Hadronic Interactions
Using higher moments of air-shower depth distributions, the authors project that the full Pierre Auger dataset could reject the EPOS and Sibyll hadronic models at high confidence.