Soft-haired Kerr black holes show rotated, dilated, drifting images and an image memory effect when soft hair changes via waves, with the effect scaling with the large black hole's mass and spin.
Andrianov and et al., Simulations of M87 and Sgr A* imaging with the Millimetron Space Observatory on near-Earth orbits , MNRAS 500 (2021) 4866 [2006.10120]
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Torn accretion disks around Kerr black holes erode the inner shadow and create bifurcated, crescent, and multi-ring shadow features driven by sub-disk discontinuities and outer tilt angle.
Accretion disk images in hybrid metric-Palatini gravity show scalar-field-dependent deviations from GR in temperature, brightness, and secondary ring structure.
citing papers explorer
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Shaving off soft hairs and the black hole image memory effect
Soft-haired Kerr black holes show rotated, dilated, drifting images and an image memory effect when soft hair changes via waves, with the effect scaling with the large black hole's mass and spin.
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Reshaping the inner shadow of a Kerr black hole by a torn accretion disk
Torn accretion disks around Kerr black holes erode the inner shadow and create bifurcated, crescent, and multi-ring shadow features driven by sub-disk discontinuities and outer tilt angle.
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Images of the accretion disk in Hybrid metric-Palatini gravity
Accretion disk images in hybrid metric-Palatini gravity show scalar-field-dependent deviations from GR in temperature, brightness, and secondary ring structure.