Cosmic Rays below<i>Z</i> = 30 in a Diffusion Model: New Constraints on Propagation Parameters
Cosmic Rays below<i>Z</i> = 30 in a Diffusion Model: New Constraints on Propagation Parameters
Cosmic-ray nuclei fluxes are expected to be measured with high precision in the near future. For instance, high-quality data on the antiproton component could give important clues about the nature of the astronomical dark matter. A very good understanding of the different aspects of cosmic-ray propagation is therefore necessary. In …