Journal article
Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
- Abstract:
- We show that the energy required to turbulently amplify magnetic field during cosmic ray (CR) acceleration by shocks extracts energy from the CR and steepens the CR energy spectrum.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Version of record, pdf, 346.1KB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/stz1805
Authors
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 488*
- Issue:
- 2
- Pages:
- 2466-2472
- Publication date:
- 2019-07-22
- Acceptance date:
- 2019-06-27
- DOI:
- EISSN:
-
1365-2966
- ISSN:
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0035-8711
- Keywords:
- Pubs id:
-
pubs:1024147
- UUID:
-
uuid:9c1bf3cf-0c07-4e94-9d18-7424b4f68f7f
- Local pid:
-
pubs:1024147
- Source identifiers:
-
1024147
- Deposit date:
-
2019-06-28
Terms of use
- Copyright holder:
- Bell et al
- Copyright date:
- 2019
- Notes:
- © 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
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