Speaker
Mohamad Shalaby
(Perimeter Institute for Theoretical Physics)
Description
In this brief presentation, I will highlight several cosmic ray puzzles that arise from discrepancies between incredibly precise new observations and models used to approximate the observed spectra and abundances of various cosmic ray species. These models rely on advanced numerical techniques, yet significant differences remain. I will conclude by outlining my efforts to address the main sources of these disagreements.
External references
- 24100130
- 88844a04-fbc8-49f8-b70d-5062f5719fa0
