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Interpretation of Fluxes of Cosmic-Ray Nuclei and Electrons within a Nonclassical Diffusion Model

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

A new scenario of the formation of observed ultrahigh-energy cosmic-ray electron/positron and nuclei spectra is discussed within a nonclassical (superdiffusion) model of particle propagation in highly inhomogeneous interstellar and intergalactic media. It is shown that the proposed scenario provides a consistent description of data from highly precise satellite measurements, ground-based hybrid EAS arrays, and Cherenkov telescopes using the spectra of leptons and nuclei, and the mass composition of cosmic rays in the super- and ultrahigh ranges of energy.

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Funding

The work is supported by the the Russian Science Foundation (grant no. 23-72-00057).

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Authors and Affiliations

  1. Altai State University, 656049, Barnaul, Russia

    A. A. Lagutin, N. V. Volkov & R. I. Raikin

Authors
  1. A. A. Lagutin
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  2. N. V. Volkov
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  3. R. I. Raikin
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Corresponding author

Correspondence to A. A. Lagutin.

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The authors declare that they have no conflicts of interest.

Additional information

Translated by E. Bondareva

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Lagutin, A.A., Volkov, N.V. & Raikin, R.I. Interpretation of Fluxes of Cosmic-Ray Nuclei and Electrons within a Nonclassical Diffusion Model. Bull. Russ. Acad. Sci. Phys. 87, 878–883 (2023). https://doi.org/10.3103/S1062873823702635

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  • DOI: https://doi.org/10.3103/S1062873823702635

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