Electron-scale Kelvin-Helmholtz Instability In Magnetized Shear Flows: Revision history

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17 September 2025

  • curprev 13:2713:27, 17 September 2025TerranceCoward6 talk contribs 5,773 bytes +5,773 Created page with "<br>Electron-scale Kelvin-Helmholtz instabilities (ESKHI) are found in several astrophysical scenarios. Naturally ESKHI is subject to a background magnetic area, but an analytical dispersion relation and an correct growth rate of ESKHI below this circumstance are long absent, as former MHD derivations will not be applicable within the relativistic regime. We current a generalized dispersion relation of ESKHI in relativistic magnetized shear flows, with few assumptions. E..."