Description
The origin of high-energy cosmic rays remains one of the biggest mysteries in astrophysics. Mass reconstruction of the primary cosmic ray is essential for pinpointing potential sources. In this study, we utilize hadronic interaction models—EPOS, SIBYLL, and QGSJET—to simulate extensive air showers. By analyzing the resulting observables, we aim to establish a robust method for distinguishing between different primary cosmic rays, thereby advancing our understanding of their origins.
| Talk category | data science (contact d.huppenkothen@uva.nl) |
|---|---|
| Preference for a talk or poster | Poster |
