Simulations show the Lorentz violation parameter l alters black hole inner shadow shape from elliptical to D-shaped, changes polarization patterns, and affects angular velocity in thin accretion disks.
Shadow and Deflection Angle of Rotating Black Holes in Perfect Fluid Dark Matter with a Cosmological Constant
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Probing Observable Features of Lorentz violation in Low-Energy Ho\v{r}ava Gravity with Accretion Disk Images of Black Hole
Simulations show the Lorentz violation parameter l alters black hole inner shadow shape from elliptical to D-shaped, changes polarization patterns, and affects angular velocity in thin accretion disks.