期刊
JOURNAL OF PLASMA PHYSICS
卷 87, 期 1, 页码 -出版社
CAMBRIDGE UNIV PRESS
DOI: 10.1017/S0022377821000040
关键词
astrophysical plasmas
资金
- European Research Council [267841, 695008]
- FCT (Portugal) grant [PTDC-FIS-PLA-2940-2014, SFRH/IF/01635/2015]
This study demonstrates that the Weibel or current filamentation instability can result in circularly polarized radiation, with the level of circular polarization increasing with the initial plasma magnetization and saturating at around 13% when the magnetization exceeds 0.05. Additionally, it is shown that this effect requires an ion-electron mass ratio greater than unity.
We show that the Weibel or current filamentation instability can lead to the emission of circularly polarized radiation. Using particle-in-cell simulations and a radiation post-processing numerical algorithm, we demonstrate that the level of circular polarization increases with the initial plasma magnetization, saturating at similar to 13% when the magnetization, given by the ratio of magnetic energy density to the electron kinetic energy density, is larger than 0.05. Furthermore, we show that this effect requires an ion-electron mass ratio greater than unity. These findings, which could also be tested in currently available laboratory conditions, show that the recent observation of circular polarization in gamma-ray burst afterglows could be attributed to the presence of magnetized current filaments driven by the Weibel or current filamentation instability.
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