A general ODE numerical method for polarized photon transport in Kerr-Newman spacetime shows that increasing black hole charge compresses and distorts EVPA structures on photon-ring scales.
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Polarized Radiative Transfer of Kerr-Newman Black Hole
A general ODE numerical method for polarized photon transport in Kerr-Newman spacetime shows that increasing black hole charge compresses and distorts EVPA structures on photon-ring scales.