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Particle acceleration and magnetic field amplification in supernova shells: A nonlinear Monte Carlo model

  • Proceedings of the 34th National Conference on Cosmic Rays
  • Published:
Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

A nonlinear model of particle spectra and nonadiabatic magnetic field amplification in supernova shells is presented. The effect super-diffusive particle propagation in the vicinity of a shock wave has on the spectra of accelerated particles and magnetic field fluctuations is studied in a Monte Carlo simulation.

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Author information

Authors and Affiliations

  1. Ioffe Institute, Russian Academy of Sciences, St. Petersburg, 194021, Russia

    A. M. Bykov & S. M. Osipov

  2. North Carolina State University, Raleigh, NC, 27695, USA

    D. Ellison

Authors
  1. A. M. Bykov
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  2. S. M. Osipov
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  3. D. Ellison
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Corresponding author

Correspondence to A. M. Bykov.

Additional information

Original Russian Text © A.M. Bykov, S.M. Osipov, D. Ellison, 2017, published in Izvestiya Rossiiskoi Akademii Nauk, Seriya Fizicheskaya, 2017, Vol. 81, No. 4, pp. 468–470.

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Bykov, A.M., Osipov, S.M. & Ellison, D. Particle acceleration and magnetic field amplification in supernova shells: A nonlinear Monte Carlo model. Bull. Russ. Acad. Sci. Phys. 81, 431–433 (2017). https://doi.org/10.3103/S1062873817040116

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  • DOI: https://doi.org/10.3103/S1062873817040116

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