Speaker
Mr
Arjen van Vliet
(DESY)
Description
Cosmic rays with energies up to 10^20 eV have been seen by the Pierre Auger Collaboration and other experiments. There are still many unanswered question concerning cosmic rays in this ultra-high-energy regime. For instance the measured structure of the flux, the incoming direction and the composition of the cosmic rays still bare question-marks. A possible explanation for these three problems, involving the interaction of these cosmic rays with the galactic magnetic field, will be presented in this talk.
Primary author
Mr
Arjen van Vliet
(DESY)
