Speaker
Amani Bemsa Bouasla
(University of Badji Mokhtar Annaba)
Description
High-energy atmospheric muons are the prevalent events detected by deep under-water/ice neutrino telescopes. Understanding their properties at sea level is crucial for accurately interpreting the observed signals. We present in this work results for the calculation of the flux and charge ration of atmospheric muons at sea level above 100 GeV. We use the Monte Carlo code CORSIKA for our calculations, along with several advanced hadronic interaction models. We compare the obtained results with experimental data and recent relevant studies.
Authors
Amani Bemsa Bouasla
(University of Badji Mokhtar Annaba)
Prof.
Reda Attallah
(University of Badji Mokhtar Annaba)