Develops a numerical solver for relativistic linear tearing growth rates including motional E field and uses PIC simulations to demonstrate slowing by shear flows and guide fields with transition to KH instability at high shear.
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Linear Tearing Growth and Onset of Relativistic Magnetic Reconnection in the Presence of Shear Flows and a Guide Field
Develops a numerical solver for relativistic linear tearing growth rates including motional E field and uses PIC simulations to demonstrate slowing by shear flows and guide fields with transition to KH instability at high shear.