Polarization maps of direct images from scalar-hairy Kerr black holes exhibit dephasing in the polarization-vector twist (larger for weakly scalarized cases) and a reversal for vertical magnetic fields at high inclinations.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
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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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Polarized Equatorial Emission around Kerr Black Holes with Synchronized Scalar Hair. I. Direct images
Polarization maps of direct images from scalar-hairy Kerr black holes exhibit dephasing in the polarization-vector twist (larger for weakly scalarized cases) and a reversal for vertical magnetic fields at high inclinations.
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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.