Shadow of a rotating traversable wormhole

By P. Nedkova, Vassil K. Tinchev, S. Yazadjiev. 2013

141 citations recorded by the source corpus.

We explore the shadow of a 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.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a5a4b105e4db694680ef773cb808f6442fd0418b

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. O. Tsupko
2. V. Perlick
3. G. Bisnovatyi-Kogan
4. M. Werner
5. A. Rogers
6. Sushant G. Ghosh
7. Rahul Kumar

In Nuclear and High Energy Physics

1. O. Tsupko
2. V. Perlick
3. G. Bisnovatyi-Kogan
4. Sushant G. Ghosh
5. Rahul Kumar

Citations in the corpus

• Calculating black hole shadows: Review of analytical studies (2021, background): “[151], so the shadow can be calculated analytically.”