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.
arXiv comment6 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
References in corpus (9)
- Cosmic-ray propagation and interactions in the Galaxy
- Cosmic Ray Scattering and Streaming in Compressible Magnetohydrodynamic Turbulence
- The Structure of the Milky Way's Hot Gas Halo
- Wave damping by MHD turbulence and its effect upon cosmic ray propagation in the ISM
- Spectrum of cosmic rays, produced in supernova remnants
- Astrophysical hydromagnetic turbulence
- Propagation of galactic cosmic rays in the presence of self-generated turbulence
- The boron-to-carbon abundance ratio and Galactic propagation of cosmic radiation
- Induced Scattering and Two-Photon Absorption of Alfven Waves with Arbitrary Propagation Angles