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      Spectrum and composition of galactic cosmic rays accelerated in supernova remnants

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          Abstract

          The spectra of high-energy protons and nuclei accelerated by supernova remnant shocks are calculated taking into account magnetic field amplification and Alfvenic drift for different types of SNRs during their evolution. The overall energy spectrum and elemental composition of cosmic rays after propagation through the Galaxy are found.

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          Journal
          0912.5172

          High energy astrophysical phenomena
          High energy astrophysical phenomena

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