On the galactic origin of ultrahigh energy cosmic rays

Physics

Scientific paper

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Scientific paper

At the energy of 5×1018 -2×1019 eV the excess flux of particles by 4.2σ more has been detected than it is expected in the case of the isotropy from the Galaxy plane. The particle fluxes inside the definite radius around pulsars exceeding by > 3σ expected ones in the case of the isotropy are observed . The list of these pulsars is given. The problem of chemical composition of ultrahigh energy cosmic rays is discussed.

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