Journal article
Electron acceleration by wave turbulence in a magnetized plasma
- Abstract:
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Astrophysical shocks are commonly revealed by the non-thermal emission of energetic electrons accelerated in situ1,2,3. Strong shocks are expected to accelerate particles to very high energies4,5,6; however, they require a source of particles with velocities fast enough to permit multiple shock crossings. While the resulting diffusive shock acceleration4 process can account for observations, the kinetic physics regulating the continuous injection of non-thermal particles is not well understoo...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Accepted manuscript, pdf, 255.7KB, Terms of use)
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(Preview, Accepted manuscript, pdf, 1.1MB, Terms of use)
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- Publisher copy:
- 10.1038/s41567-018-0059-2
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Bibliographic Details
- Publisher:
- Springer Nature
- Journal:
- Nature Physics More from this journal
- Volume:
- 14
- Pages:
- 475–479
- Publication date:
- 2018-03-12
- Acceptance date:
- 2018-01-25
- DOI:
- ISSN:
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1745-2481
Item Description
- Pubs id:
-
pubs:822570
- UUID:
-
uuid:b77e225b-7ae8-463d-a346-61a9138aac33
- Local pid:
-
pubs:822570
- Source identifiers:
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822570
- Deposit date:
-
2018-02-02
Terms of use
- Copyright holder:
- Rigby et al
- Copyright date:
- 2018
- Notes:
- This is the accepted manuscript version of the article. The final version is available online from Springer Nature at: https://doi.org/10.1038/s41567-018-0059-2
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