Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification (2019)

First Author: Bell A

Attributed to: Astrophysics at Oxford 2019-2022 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stz1805

Publication URI: http://dx.doi.org/10.1093/mnras/stz1805

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2