Numerical images of thick accretion flows around Konoplya-Zhidenko black holes show outer bright rings from higher-order light paths and inner dark regions from the event horizon, with lower polarization in those rings and parameter-dependent asymmetry.
First sagittarius a* event horizon telescope results. i. the shadow of the supermassive black hole in the center of the milky way,
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Horizon-scale intensity and polarization images of rotating Konoplya-Zhidenko black holes with thick accretion flows
Numerical images of thick accretion flows around Konoplya-Zhidenko black holes show outer bright rings from higher-order light paths and inner dark regions from the event horizon, with lower polarization in those rings and parameter-dependent asymmetry.