Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
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.
| Главные авторы: | , , |
|---|---|
| Формат: | Journal article |
| Опубликовано: |
Oxford University Press
2019
|