Combined velocity and magnetic shear in a relativistic pair plasma drives interacting Kelvin-Helmholtz and drift-kink instabilities that enhance dissipation and produce nonthermal particle acceleration.
The bulk-flow dynamic pressure can be obtained by subtracting Pij from Πij (i.e
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Dissipation and particle acceleration in astrophysical jets with velocity and magnetic shear: Interaction of Kelvin-Helmholtz and Drift-Kink Instabilities
Combined velocity and magnetic shear in a relativistic pair plasma drives interacting Kelvin-Helmholtz and drift-kink instabilities that enhance dissipation and produce nonthermal particle acceleration.