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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| Formato: | Artigo |
| Idioma: | English |
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IOP Publishing
2023-01-01
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| Colecção: | The Astrophysical Journal |
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| Acesso em linha: | https://doi.org/10.3847/1538-4357/ad00b1 |