For a rotating hairy black hole, thin-disk flux, temperature, luminosity, and ray-traced images deviate increasingly from Kerr as spin grows, especially in the inner disk.
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Thin Accretion Disk Around Rotating Hairy Black Hole: Radiative Property and Optical Appearance
For a rotating hairy black hole, thin-disk flux, temperature, luminosity, and ray-traced images deviate increasingly from Kerr as spin grows, especially in the inner disk.