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• W3105449119 startingPage "022101" @default.
• W3105449119 abstract "The role of the Weibel instability is investigated for the first time in the context of the large-scale magnetic reconnection problem. A late-time evolution of magnetic reconnection in relativistic pair plasmas is demonstrated by particle-in-cell simulations. In the outflow regions, powerful reconnection jets pile up the magnetic fields and then a contact discontinuity appears there. Further downstream, it is found that the two-dimensional extension of the relativistic Weibel instability generates electromagnetic fields, which are comparable to the antiparallel or piled-up fields. In a microscopic viewpoint, the instability allows the plasma’s multiple interactions with the discontinuity. In a macroscopic viewpoint, the instability leads to rapid expansion of the current sheet and then the reconnection jet front further propagates into the downstream. Possible application to the three-dimensional case is briefly discussed." @default.
• W3105449119 created "2020-11-23" @default.
• W3105449119 creator A5040102378 @default.
• W3105449119 creator A5052497233 @default.
• W3105449119 date "2008-02-01" @default.
• W3105449119 modified "2023-10-17" @default.
• W3105449119 title "The role of the Weibel instability at the reconnection jet front in relativistic pair plasma reconnection" @default.
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• W3105449119 doi "https://doi.org/10.1063/1.2836623" @default.
• W3105449119 hasPublicationYear "2008" @default.
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