Anomalous diffusion of the cosmic rays: steady-state solution

Simple item page
dc.creatorLagutin, A. A.
dc.creatorMakarov, V. V.
dc.creatorTyumentsev, A. G.
dc.date2001-07-14
dc.date.accessioned2026-07-07T01:59:18Z
dc.date.available2026-07-07T01:59:18Z
dc.descriptionWe consider the propagation of galactic cosmic rays in the fractal interstellar medium. Steady state solution of the fractional diffusion equation, describing cosmic ray propagation, is found. We show that the exponent of the steady state spectrum turns out to be equal to the exponent of the cosmic ray spectrum above the "knee", that is approximately equal to 3.1.
dc.description3 pages; Proc. of the 27th ICRC
dc.identifierhttps://arxiv.org/abs/astro-ph/0107253
dc.identifierhttp://arxiv.org/abs/astro-ph/0107253
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3060
dc.subjectAstrophysics
dc.titleAnomalous diffusion of the cosmic rays: steady-state solution
dc.typetext

Files

Collections

arXiv