Ultra-High-Energy Cosmic Rays Accelerated by Magnetically Dominated Turbulence
Ultra-high-energy cosmic rays (UHECRs), particles characterized by energies exceeding 10 ^18 eV, are generally believed to be accelerated electromagnetically in high-energy astrophysical sources. One promising mechanism of UHECR acceleration is magnetized turbulence. We demonstrate from first princi...
Kaydedildi:
| Asıl Yazarlar: | , , |
|---|---|
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2024-01-01
|
| Seri Bilgileri: | The Astrophysical Journal Letters |
| Konular: | |
| Online Erişim: | https://doi.org/10.3847/2041-8213/ad955f |
| Etiketler: |
Etiket eklenmemiş, İlk siz ekleyin!
|