نوع مقاله : مقاله پژوهشی کامل
عنوان مقاله English
نویسندگان English
Modeling extensive air showers and obtaining high-energy cosmic rays' origin information depends on the description of hadronic interactions (in the energy range of LHC collisions and more). Diffraction events in hadronic interactions are expected to be well-effective in observables of extensive air showers and affect shower characteristics profile since it provides a different way of transferring energy to the atmosphere. In particular, in this research, the maximum depth and the maximum number of secondary particles of extensive air showers with diffractive events have been measured. The results obtained from this article, predicts slower shower distribution, an increase in the maximum depth and a decrease in the maximum number of particles in the presence of diffractive interactions.
کلیدواژهها English
