Rotating black hole shadows in 4D Einstein-Gauss-Bonnet gravity shrink with increasing coupling parameter α, grow more asymmetric with spin a, and remain consistent with EHT data.
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Visual Characteristics of a Rotating Black Hole in $4$D Einstein-Gauss-Bonnet Gravity with Thin Accretion Disk Under EHT Constraints
Rotating black hole shadows in 4D Einstein-Gauss-Bonnet gravity shrink with increasing coupling parameter α, grow more asymmetric with spin a, and remain consistent with EHT data.