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Spurious contribution to cosmic ray scattering calculations
Authors:A. Shalchi  H. Yan   A. Lazarian
Affiliation:Bartol Research Institute, University of Delaware, Newark, DE 19716, USA;Astronomy Department, University of Wisconsin–Madison, Madison, WI 53706, USA
Abstract:The quasi-linear theory for cosmic ray propagation is a well-known and widely accepted theory. In this paper, we discuss the different contributions to the pitch-angle Fokker–Planck coefficient from large and small scales for slab geometry using the damping model of dynamical turbulence. These examinations will give us a hint on the limitation range where the quasi-linear approximation is a good approximation.
Keywords:diffusion    turbulence    cosmic rays
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