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

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4 November 2025

  • curlast 13:5713:57, 4 November 2025 EllaGreenaway6 talk changes 5,572 bytes +5,572 Created page with "<br>Electron-scale Kelvin-Helmholtz instabilities (ESKHI) are found in several astrophysical scenarios. Naturally ESKHI is topic to a background magnetic field, but an analytical dispersion relation and an accurate progress fee of ESKHI underneath this circumstance are long absent, as former MHD derivations aren't applicable within the relativistic regime. We present a generalized dispersion relation of ESKHI in relativistic magnetized shear flows, with few assumptions...."
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