Cosmic ray propagation and interactions in the Galaxy
arXiv:1412.0863 · doi:10.1016/j.nuclphysbps.2014.10.012
Abstract
Cosmic ray propagation in the Galaxy is shortly reviewed. In particular we consider the self-consistent models of CR propagation. In these models CR streaming instability driven by CR anisotropy results in the Alfvénic turbulence which in turn determines the scattering and diffusion of particles.
6 pages, 3 figures, to appear in Nuclear Physics B, oral talk at the conference "Cosmic ray origin - beyond the standard models" San-Vito di Cadore, Italy, March 16-22, 2014