On Fluctuations of Cosmic Rays in the Galaxy with Random Supernova Outbursts

Physics

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Scientific paper

The random nature of cosmic ray (CR) sources leads to the fluctuations of CR intensity in space and time. We calculate the expected fluctuations in a flathalo diffusion model for particles with energies from 1 to 103 TeV. The data on CR spectrum and anisotropy, and the astronomical data on supernova remnants, the potential sources of CRs, can be used to constrain the value of CR diffusion coefficient and its dependence on energy.

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