Cosmic ray acceleration to ultrahigh energy in radio galaxies

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...

Bibliografski detalji
Glavni autori:	Matthews, J, Bell, A, Araudo, A, Blundell, K
Format:	Journal article
Izdano:	EDP Sciences 2019

Slični predmeti

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