PoS - Proceedings of Science
Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - CRI - Cosmic Ray Indirect
A Kinetic Study of the Saturation of the Bell Instability
G. Zacharegkas*, D. Caprioli, C. Haggerty and S. Gupta
Full text: pdf
Pre-published on: July 04, 2021
Published on: March 18, 2022
The nonresonant cosmic ray instability, predicted by Bell (2004), is thought to play an important role in the acceleration and confinement of cosmic rays (CR) close to supernova remnants. Despite its importance, the exact mechanism responsible for the saturation of the instability has not been determined, and there is no first-principle prediction for the amplitude of the saturated magnetic field.
Using a survey of self-consistent hybrid simulations (with kinetic ions and fluid electrons), we study the non-linear evolution of the Bell instability as a function of the parameters of the CR population.
We find that saturation is achieved when the magnetic pressure in the amplified field is comparable to the initial CR momentum flux.
DOI: https://doi.org/10.22323/1.395.0483
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