Rotating wormhole solutions with a complex phantom scalar field
arXiv:1906.08742 · doi:10.1103/PhysRevD.100.044019
Abstract
We consider rotating wormhole solutions supported by a complex phantom scalar field with a quartic self-interaction, where the phantom field induces the rotation of the spacetime. The solutions are regular and asymptotically flat. A subset of solutions describing static but not spherically symmetric wormholes is also obtained.
13 pages, 6 figures