Particle acceleration and magnetic field amplification in supernova shells: A nonlinear Monte Carlo model
- 作者: Bykov A.M.1, Osipov S.M.1, Ellison D.2
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隶属关系:
- Ioffe Institute
- North Carolina State University
- 期: 卷 81, 编号 4 (2017)
- 页面: 431-433
- 栏目: 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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详细
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.
作者简介
A. Bykov
Ioffe Institute
编辑信件的主要联系方式.
Email: byk@astro.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021
S. Osipov
Ioffe Institute
Email: byk@astro.ioffe.ru
俄罗斯联邦, St. Petersburg, 194021
D. Ellison
North Carolina State University
Email: byk@astro.ioffe.ru
美国, Raleigh, NC, 27695
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