2D radiative PIC simulations show multi-sheet reconnection in relativistic pair plasma evolving into Kolmogorov-like turbulence that provides secondary particle acceleration while keeping the high-energy spectrum steep.
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Radiative PIC simulations of relativistic pair plasma: multiple interacting current sheets and turbulent evolution
2D radiative PIC simulations show multi-sheet reconnection in relativistic pair plasma evolving into Kolmogorov-like turbulence that provides secondary particle acceleration while keeping the high-energy spectrum steep.