Linear Tearing Growth and Onset of Relativistic Magnetic Reconnection in the Presence of Shear Flows and a Guide Field
This paper utilizes kinetic particle-in-cell simulations and a newly developed numerical solver to demonstrate that both shear flows and guide fields delay the onset of relativistic magnetic reconnection by slowing the linear tearing instability, with high flow shear eventually triggering a transition to Kelvin-Helmholtz instability.