http://arxiv.org/abs/2210.07575
In the sub-TeV regime, the most widely used hadronic interaction models disagree significantly in their predictions of particle spectra from cosmic ray induced air showers. We investigate the nature and impact of model uncertainties, focussing on air shower primaries with energies around the transition between high and low energy hadronic interaction models, where the dissimilarities are largest and which constitute the bulk of the interactions in air showers.
M. Schmelling, &. Pastor-Gutiérrez, H. Schorlemmer, et. al.
Mon, 17 Oct 22
51/56
Comments: Proceedings of the 51 International Symposium on Multiparticle Dynamics (ISMD2022)
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