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Cosmic ray acceleration at oblique shocks

Abstract:
We show that the diffusion approximation breaks down for particle acceleration at oblique shocks with velocities typical of young supernova remnants. Higher order anisotropies flatten the spectral index at quasi-parallel shocks and steepen the spectral index at quasi-perpendicular shocks. We compare the theory with observed spectral indices. © 2011 The Authors Monthly Notices of the Royal Astronomical Society © 2011 RAS.
Publication status:
Published

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Publisher copy:
10.1111/j.1365-2966.2011.19571.x

Authors

More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atomic & Laser Physics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Author


Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
418
Issue:
2
Pages:
1208-1216
Publication date:
2011-12-01
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
pubs:194615
UUID:
uuid:5ee03ad1-8614-4593-8f82-2d3079af6d90
Local pid:
pubs:194615
Source identifiers:
194615
Deposit date:
2012-12-19
ARK identifier:

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