2019/06/20 by Xiao Yan Chew, Vladimir Dzhunushaliev, Vladimir Folomeev +2 · 1 citation
Physics and Astronomy · #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.100.044019
published as Phys. Rev. D 100, 044019 (2019) · 13 pages, 6 figures
arxiv created 2019/06/20 · arxiv updated 2019/08/21
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.