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

  • A. M. BykovEmail author
  • S. M. Osipov
  • D. Ellison
Proceedings of the 34th National Conference on Cosmic Rays
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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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Copyright information

© Allerton Press, Inc. 2017

Authors and Affiliations

  1. 1.Ioffe InstituteRussian Academy of SciencesSt. PetersburgRussia
  2. 2.North Carolina State UniversityRaleighUSA

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