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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Black hole shadows in a Dehnen-(1,4,5/2) dark matter halo with quintessence grow with halo density, scale radius, and dark energy parameters, with intensity more sensitive to dark energy and radius more sensitive to dark matter.
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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.
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Shadows and photon spheres of static black holes embedded in a Dehnen-(1,4,5/2)-type dark matter halo with a quintessential field
Black hole shadows in a Dehnen-(1,4,5/2) dark matter halo with quintessence grow with halo density, scale radius, and dark energy parameters, with intensity more sensitive to dark energy and radius more sensitive to dark matter.