Turbulent Diffusion of the Particles within Pulsar Wind Nebulae

A turbulent diffusion model is presented to account for the energy and spatial diffusion of the particles within pulsar wind nebulae (PWNe), with the assumption that the energy injected from the pulsar into the nebula is split between the turbulence waves and electrons/positrons. In the model, the m...

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Bibliographic Details
Main Authors: Fang-Wu Lu, Bo-Tao Zhu, Wen Hu, Li Zhang
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ace0c2