Content
- Ultrahigh-energy cosmic rays: Single particle propagation and efficient nuclei-photon interaction modeling
- Galactic cosmic rays: Complex magnetic field models (coherent + turbulent), ensemble averaged transport (grid based and stochastic differential equations), nuclei-nuclei interaction
- Source physics: Non-linear time evolution of energy spectra, tabulated interactions rates, matrix methods
- From simulation to physics values: Re-weighting, normalization, comparison with observables
- Kursleiter/in: Lukas Merten
- Kursleiter/in: Julia Tjus
Semester: SoSe 2024