The angular size of a dust wormhole's shadow in a closed Friedmann universe first decreases, then increases with observation time, following a power-law relation in the wormhole size.
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Gravitational lensing by Lema\^{\i}tre-Tolman-Bondi wormholes in a Friedmann universe
The angular size of a dust wormhole's shadow in a closed Friedmann universe first decreases, then increases with observation time, following a power-law relation in the wormhole size.