In Kerr black holes the gravitational spin Hall effect produces a helicity-dependent shift of the critical impact parameter that is linear in spin parameter chi and scales as 1/omega, appearing as a cos phi modulation of the shadow edge.
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Helicity-dependent corrections to black-hole shadows from the gravitational spin Hall effect
In Kerr black holes the gravitational spin Hall effect produces a helicity-dependent shift of the critical impact parameter that is linear in spin parameter chi and scales as 1/omega, appearing as a cos phi modulation of the shadow edge.