Email this article Particle acceleration and magnetic field amplification in supernova shells: A nonlinear Monte Carlo model
- Authors: Bykov A.M.1, Osipov S.M.1, Ellison D.2
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Affiliations:
- Ioffe Institute
- North Carolina State University
- Issue: Vol 81, No 4 (2017)
- Pages: 431-433
- Section: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185033
- DOI: https://doi.org/10.3103/S1062873817040116
- ID: 185033
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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.
About the authors
A. M. Bykov
Ioffe Institute
Author for correspondence.
Email: byk@astro.ioffe.ru
Russian Federation, St. Petersburg, 194021
S. M. Osipov
Ioffe Institute
Email: byk@astro.ioffe.ru
Russian Federation, St. Petersburg, 194021
D. Ellison
North Carolina State University
Email: byk@astro.ioffe.ru
United States, Raleigh, NC, 27695
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