Three component model of cosmic ray spectra from 10 GeV to 100 PeV

2006/01/31 by В. И. Зацепин, V. I. Zatsepin, N. V. Sokolskaya · 5 citations
Physics and Astronomy · #Air shower #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Atmosphere (unit) #COSMIC cancer database #Cosmic ray #Dark Matter and Cosmic Phenomena #Energy spectrum #Flux (metallurgy) #Meteorology #Neutrino Physics Research #Particle (ecology) #Physics #Spectral line #Supernova #Ultra-high-energy cosmic ray #astro-ph

paper · pdf · doi:10.1051/0004-6361:20065108

Revised version accepted for publication in Astronomy and Astrophysics, 5 pages, 6 figures, aa.cls

openalex publication_date 2006/08/04 · arxiv created 2006/08/24 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.A model to describe cosmic ray spectra in the energy region from 1010 to 1017 eV is suggested based on the assumption that Galactic cosmic ray flux is a mixture of fluxes accelerated by shocks from nova and supernova of different types.

Citations

• A single source of cosmic rays in the range - eV

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• The DArk Matter Particle Explorer mission
• Pion decay model of the Tibet-ASγ PeV gamma-ray signal