Cosmic ray acceleration to ultrahigh energy in radio galaxies
The origin of ultrahigh energy cosmic rays (UHECRs) is an open question. In this proceeding, we first review the general physical requirements that a source must meet for acceleration to 10-100 EeV, including the consideration that the shock is not highly relativistic. We show that shocks in the bac...
| Κύριοι συγγραφείς: | , , , |
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| Μορφή: | Journal article |
| Έκδοση: |
EDP Sciences
2019
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