Cosmic Ray Transport with Magnetic Focusing and the "Telegraph" model
Mikhail Malkov, Roald Sagdeev

TL;DR
This paper rigorously analyzes cosmic ray transport models, demonstrating that the telegraph equation does not naturally arise from the Chapman-Enskog expansion and is unphysical during the initial relaxation period.
Contribution
The study clarifies the mathematical origin of the telegraph term, showing it is not inherent to cosmic ray transport and only appears as an unphysical artifact during early relaxation.
Findings
No second order time derivative (telegraph term) emerges in proper asymptotic expansion.
The telegraph term is only relevant during a short initial relaxation period.
The telegraph solution introduces unphysical singularities during this period.
Abstract
Cosmic rays (CR), constrained by scattering on magnetic irregularities, are believed to propagate diffusively. But a well-known defect of diffusive approximation whereby some of the particles propagate unrealistically fast has directed interest towards an alternative CR transport model based on the "telegraph" equation. However, its derivations often lack rigor and transparency leading to inconsistent results. We apply the classic Chapman-Enskog method to the CR transport problem. We show that no "telegraph" (second order time derivative) term emerges in any order of a proper asymptotic expansion with systematically eliminated short time scales. Nevertheless, this term may formally be\emph{ converted} from the \emph{fourth} order hyper-diffusive term of the expansion. But, both the telegraph and hyperdiffusive terms may only be important for a short relaxation period associated with…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Dark Matter and Cosmic Phenomena · Atmospheric Ozone and Climate
