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.
Agol,The Effects of Magnetic Fields, Absorption, and Relativity on the Polarization of Accretion Disks around Supermassive Black Holes, Ph.D
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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.