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Rayleigh-Taylor and Richtmyer-Meshkov Instabilities in Relativistic Hydrodynamic Jets

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Figure

Figure 1. Schematic picture of the jet propagating through the ambient medium (see Figure 1 in Ref
Figure 2. Snapshots of the 2D spatial distribution of the density in the 3D calculation for the propagation of the relativistic jet throughthe uniform ambient medium when t = 2000
Figure 3.Three-dimensional density map of the jet-externalmedium system in the half simulation box modeling the radiallyoscillating motion of the jet when t = 0, 150, and 200.
Figure 4. Time evolution of the volume-averaged azimuthal ve-locity |vθ|ave defined by Equation (4).

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