Ellis Wormholes in Anti-De Sitter Space
2021
We construct traversable wormholes with anti-de Sitter asymptotics supported by a phantom field. These wormholes are massless and symmetric with respect to reflection of the radial coordinate $$\eta \rightarrow - \eta $$
. Their circumferential radius decreases monotonically from radial infinity to their single throat. Analogous to their asymptotically flat counterparts, these anti-de Sitter wormholes possess an unstable radial mode.
Keywords:
- Correction
- Source
- Cite
- Save
- Machine Reading By IdeaReader
90
References
0
Citations
NaN
KQI