http://arxiv.org/abs/1412.0863
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 Alfv\’enic turbulence which in turn determines the scattering and diffusion of particles.
V. Zirakashvili
Wed, 3 Dec 14
44/60
Comments: 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