LIP Lisboa

Multiparticle production with SIBYLL in extensive air showers

by Felix Riehn (Karlsruhe Institut of Technology)

Portugal
Description
The measurement of ultra-high energy cosmic rays can only be done indirectly through the detection of extensive air showers. The development of such air showers is driven by the interactions of hadrons in the atmosphere. In order to extract the properties of the primary cosmic ray from the measurement of the air shower the cascade of hadron interactions taking place in the atmosphere have to be modeled. One of the models commonly used for the simulation of the processes of hadronic multiparticle production in extensive air showers is SIBYLL. One aspect of this talk will be the presentation of the development of the model based on data provided by the LHC experiments. Since the LHC only covers proton interactions on the order of 10 TeV but interactions in air showers encompass a much broader range of energies and projectiles the presentation will further focus on the qualitative assessment of the remaining uncertainty in the interpretation of the air shower measurements due to the hadronic models.
Slides