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Stochastic Electron Acceleration in Shell-Type Supernova Remnants

We study the stochastic electron acceleration by fast mode waves in the turbulent downstream of weakly magnetized collisionless astrophysical shocks. The acceleration is most efficient in a dissipative layer, and the model characteristics are determined by the shock speed, density, magnetic field, and turbulence decay length. The model explains observations of shell-type supernova remnants RX J1713.7-3946 and J0852.0-4622 and can be tested by observations in hard X-rays with the HXMT and NuSTAR or gamma-rays with the GLAST.

preprint2008arXivOpen access
Siming LiuZhong-Hui FanChristopher L. FryerJian-Min WangHui Li
astro-ph
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Open access5 authors1 topic
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Siming LiuZhong-Hui FanChristopher L. FryerJian-Min WangHui Li

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