Wormholes with tuned throat parameters can produce the same shadow and silhouette radii as Schwarzschild black holes but yield brighter accretion disk images dominated by Doppler boosting rather than gravitational redshift.
Exact gravitational lens equation in spherically symmetric and static spacetimes,
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Image of a wormhole with an arbitrary throat profile
Wormholes with tuned throat parameters can produce the same shadow and silhouette radii as Schwarzschild black holes but yield brighter accretion disk images dominated by Doppler boosting rather than gravitational redshift.