- 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.
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- Peer review status:
- Peer reviewed
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- Oxford University Press Publisher's website
- Monthly Notices of the Royal Astronomical Society Journal website
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- Copyright holder:
- Bell et al.
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- © 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
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