A method to estimate the primary mass of ultrahigh-energy Cosmic Rays from measurements of the depth of the shower maximum and the muon content

0581825 - FZÚ 2024 RIV GB eng J - Článek v odborném periodiku
Stadelmaier, Maximilian Klaus
A method to estimate the primary mass of ultrahigh-energy Cosmic Rays from measurements of the depth of the shower maximum and the muon content.
Astrophysical Journal. Roč. 946, č. 2 (2023), č. článku 100. ISSN 0004-637X. E-ISSN 1538-4357
Grant CEP: GA MŠMT(CZ) EF18_053/0016627
Institucionální podpora: RVO:68378271
Klíčová slova: cosmic radiation: UHE * nucleus: massm muon * mass spectrum * air
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 4.9, rok: 2022
Způsob publikování: Open access

The origin and mass composition of ultrahigh-energy cosmic rays is one of the big open questions of modern physics. Estimating the mass of ultrahigh-energy cosmic rays always involves the comparison of data with simulations using hadronic interaction models. The state-of-the-art hadronic interaction models, however, fail to agree with each other on the expected depths of the shower maxima, and on the average number of muons produced in air showers initiated by the same primary particles. Thus the interpretation of data in terms of the primary masses of cosmic rays differs depending on which hadronic interaction model is considered as a reference. Good agreement, however, can be found in the implications from hadronic interaction models in the prediction of the change of the average depth of the shower maximum and in the relative change in the number of produced muons as a function of the nuclear mass of the primary cosmic ray.
Trvalý link: https://hdl.handle.net/11104/0349978