The Maximum Energy of Shock-accelerated Cosmic Rays

Identifying the accelerators of Galactic cosmic ray (CR) protons with energies up to a few PeV (10 ^15 eV) remains a theoretical and observational challenge. Supernova remnants (SNRs) represent strong candidates because they provide sufficient energetics to reproduce the CR flux observed at Earth. H...

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Bibliographic Details
Main Author: Rebecca Diesing
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad00b1