The transition from galactic to extragalactic cosmic rays

dc.creatorStanev, Todor
dc.date2006-11-20
dc.date.accessioned2026-07-07T10:36:36Z
dc.date.available2026-07-07T10:36:36Z
dc.descriptionWe discuss the region of transition between galactic and extragalactic cosmic rays. The exact shapes and compositions of these two components contains information about important parameters of powerful astrophysical sources and the conditions in extragalactic space. Several types of experimental data, including the exact shape of the ultrahigh energy cosmic rays, their chemical composition and their anisotropy, and the fluxes of cosmogenic neutrinos have to be included in the solution of this problem.
dc.description6 pages, 3 figures, written in LaTeX, to be published in the Proceedings of the NOW 2006 workshop
dc.identifierhttps://arxiv.org/abs/astro-ph/0611633
dc.identifierhttp://arxiv.org/abs/astro-ph/0611633
dc.identifierNucl.Phys.Proc.Suppl.168:252-257,2007
dc.identifierdoi:10.1016/j.nuclphysbps.2007.02.021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180110
dc.subjectAstrophysics
dc.titleThe transition from galactic to extragalactic cosmic rays
dc.typetext

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