Reconstruction of the muon production longitudinal profiles in extensive air showers

0581821 - FZÚ 2024 RIV FR eng C - Konferenční příspěvek (zahraniční konf.)
Kravka, A. - dos Santos, Eva M. Martins - Stadelmaier, Maximilian Klaus - Yushkov, Alexey
Reconstruction of the muon production longitudinal profiles in extensive air showers.
EPJ Web of Conferences. Vol. 283. Les Ulis: E D P Science, 2023 - (De Mitri, I.; Barbato, F.; Boncioli, D.; Evoli, C.; Pagliaroli, G.; Salamida, F.), č. článku 05009. ISSN 2100-014X.
[International symposium on Ultra High Energy Cosmic Rays (UHECR) /6./. L'Aquila (IT), 03.10.2022-07.10.2022]
Grant CEP: GA ČR(CZ) GM21-02226M
Institucionální podpora: RVO:68378271
Klíčová slova: muon production depth * Extensive Air Showers
Obor OECD: Astronomy (including astrophysics,space science)
https://www.epj-conferences.org/articles/epjconf/pdf/2023/09/epjconf_uhecr2023_05009.pdf

Muons produced in extensive air showers have large decay lengths and small radiative energy losses, enabling a large fraction of them to reach surface and underground detector arrays while keeping relevant information about the hadronic interactions that occurred high in the atmosphere. We can relate a muon's arrival time and position at the detector to its production distance/depth. The total delay of muons with respect to the shower plane is primarily due to their geometric path and energy, which we call the geometric and kinematic delays, respectively. We are currently working on improving the current kinematic delay parameterizations using Deep Neural Networks for muons arriving at surface and underground detector arrays. We aim to reconstruct the longitudinal profile of muons for future arrays of buried scintillator detectors at energies from around the second knee to the ankle of the cosmic ray spectrum, where there is an overlap with the nominal energies at the LHC.
Trvalý link: https://hdl.handle.net/11104/0349977