Modeling the Saturation of the Bell Instability Using Hybrid Simulations

The nonresonant streaming instability (Bell instability) plays a pivotal role in the acceleration and confinement of cosmic rays (CRs), yet the exact mechanism responsible for its saturation and the magnitude of the final amplified magnetic field have not been assessed from first principles. Using a...

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Autors principals:	Georgios Zacharegkas, Damiano Caprioli, Colby Haggerty, Siddhartha Gupta, Benedikt Schroer
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2024-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Cosmic rays Galactic cosmic rays Particle astrophysics Cosmic ray sources High-energy cosmic radiation High energy astrophysics
Accés en línia:	https://doi.org/10.3847/1538-4357/ad3960
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