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Cosmic Ray Acceleration in Supernova Remnants with Nonuniform Density Distribution

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

Abstract

A study is performed of the acceleration of cosmic rays by shock waves propagating in bubbles of hot rarefied gas created by the stellar wind of supernova progenitors. Spectra of accelerated particles produced in type Ib/c supernova remnants are determined.

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Funding

This work was partially supported by the Russian Foundation for Basic Research, project no. 19-02-00043.

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Authors and Affiliations

  1. Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Russian Academy of Sciences, 108840, Moscow, Russia

    V. N. Zirakashvili & V. S. Ptuskin

Authors
  1. V. N. Zirakashvili
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  2. V. S. Ptuskin
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Corresponding author

Correspondence to V. N. Zirakashvili.

Additional information

Translated by T. Sokolova

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Zirakashvili, V.N., Ptuskin, V.S. Cosmic Ray Acceleration in Supernova Remnants with Nonuniform Density Distribution. Bull. Russ. Acad. Sci. Phys. 85, 366–368 (2021). https://doi.org/10.3103/S1062873821040407

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  • DOI: https://doi.org/10.3103/S1062873821040407

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