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


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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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