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A Heavy-metal Scenario of Ultra-high-energy Cosmic Rays

  • Authors: Jakub Vícha, Alena Bakalová, Ana L. Müller, Olena Tkachenko, Maximilian K. Stadelmaier

Jakub Vícha et al 2025 The Astrophysical Journal Letters 986 .

  • Provider: AAS Journals

Caption: Figure 4.

Top left panel: the muon number obtained by direct measurements at Auger (A. Aab et al. 2020a, 2021) compared to the predictions with and without the application of ΔXmax. Note that in case of the SIBYLL 2.3d model, only the predictions at energy 1019 eV were at our disposal. Top right panel: the ratio of the muon signal in the data and the signal predicted from air-shower simulations with (filled markers) and without (open markers) application of ΔXmax. The results from A. Abdul Halim et al. (2024a) are displayed by triangles. Bottom panels: the Xmax distribution of Auger data (A. Aab et al. 2014a) compared to the prediction for the heavy-metal scenario (Gauss × exp.) using QGSJET II-04 + ΔXmax (left) and SIBYLL 2.3d + ΔXmax (right) in the energy bin 1018.0−18.5 eV. For visualization purposes, the fits to the tail of the predicted Xmax distributions (Λη), corrected for detector acceptance, are shown.

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