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

First Author: Bell A

Attributed to: Astrophysics at Oxford 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1906.12240

Publication URI: https://arxiv.org/abs/1906.12240

Type: Other