The Shadow of a Rotating Traversable Wormhole

Understand

We explore the shadow of certain class of rotating traversable wormholes within classical general relativity.

• The images depend on the angular momentum of the wormhole, and the inclination angle of the observer.
• We compare the results with the case of the Kerr black hole.
• For small angular momenta the shadows for the two solutions are nearly identical, however with the increasing of the angular momentum they start to deviate considerably.