Rotating thin-shell wormhole from glued Kerr spacetimes
arXiv:1101.5281 · doi:10.1134/S0202289311020149
Abstract
We construct a model of a rotating wormhole made by cutting and pasting two Kerr spacetimes. As a result, we obtain a rotating thin-shell wormhole with exotic matter at the throat. Two candidates for the exotic matter are considered: (i) a perfect fluid; (ii) an anisotropic fluid. We show that a perfect fluid is unable to support a rotating thin-shall wormhole. On the contrary, the anisotropic fluid with the negative energy density can be a source for such a geometry.
8 pages, 3 figures, accepted for publication in Gravitation and Cosmology
References in corpus (12)
- Traversable wormholes: Some simple examples
- Traversable wormholes from surgically modified Schwarzschild spacetimes
- Stability of Chaplygin gas thin-shell wormholes
- Plane symmetric thin-shell wormholes: solutions and stability
- Cylindrical thin-shell wormholes
- Thin-shell wormholes in dilaton gravity
- Thin-shell wormholes with a generalized Chaplygin gas
- Stability of thin-shell wormholes supported by ordinary matter in Einstein-Maxwell-Gauss-Bonnet gravity
- Thin-shell wormholes in Brans-Dicke gravity
- Thin-shell wormholes associated with global cosmic strings
- Slowly rotating scalar field wormholes: the second order approximation
- Once again on thin-shell wormholes in scalar-tensor gravity
Cited by in corpus (13)
- Wormholes versus black holes: quasinormal ringing at early and late times
- I-Love-Q relations for a gravastar and the approach to the black-hole limit
- Rotating Thin-Shell Wormhole
- Stable thin-shell wormholes with a Chaplygin gas in Einstein-Maxwell-Gauss-Bonnet gravity
- Vacuum decays around spinning black holes
- Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes
- On a Particular Thin-shell Wormhole
- Quantum Corrected Schwarzschild Thin Shell Wormhole
- Dynamics of test particles in thin-shell wormhole spacetimes
- Wormhole solutions in the presence of nonlinear Maxwell field
- Thin-shell wormholes in 2+1-dimensional Einstein-Scalar Theory
- Gravitational Waves by Perturbation of a Slowly Rotating Thin-Shell Wormhole
- Stability of Thin Shell and Wormhole Configurations: Schwarzschild, Schwarzschild -- (Anti-) de Sitter, and FLRW Spacetimes