2023
DOI: 10.1103/physrevd.107.062004
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Measurement of hadron production in πC interactions at 158 and 350GeV

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Cited by 5 publications
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“…Muons propagate with minimal energy loss in the atmosphere, nearly undecayed, and eventually reach the Earth's surface. Based on the highest-energy cosmic ray data observed so far, the Pierre Auger Observatory (Aab et al 2015(Aab et al , 2016a and Telescope Array (Aab et al 2017) indicated a significant discrepancy in the muon number within extensive air showers (EAS) compared to the data predicted by the hadronic interaction models using in detectors like LHC (Adriani et al 2016) and SPS (Adhikary et al 2023a). Hadronic interaction models such as Sibyll-2.1 (Ahn et al 2009), QGSJetII-04 (Ostapchenko 2011), and EPOS-LHC (Pierog et al 2015) are proposed after further development and adjustment to the data.…”
mentioning
confidence: 99%
“…Muons propagate with minimal energy loss in the atmosphere, nearly undecayed, and eventually reach the Earth's surface. Based on the highest-energy cosmic ray data observed so far, the Pierre Auger Observatory (Aab et al 2015(Aab et al , 2016a and Telescope Array (Aab et al 2017) indicated a significant discrepancy in the muon number within extensive air showers (EAS) compared to the data predicted by the hadronic interaction models using in detectors like LHC (Adriani et al 2016) and SPS (Adhikary et al 2023a). Hadronic interaction models such as Sibyll-2.1 (Ahn et al 2009), QGSJetII-04 (Ostapchenko 2011), and EPOS-LHC (Pierog et al 2015) are proposed after further development and adjustment to the data.…”
mentioning
confidence: 99%