Phantom Wormholes in (2+1)-dimensions
arXiv:1001.1243 · doi:10.1007/s10773-010-0263-z
Abstract
In this paper, we have constructed a (2+1)-dimensional wormhole using inhomogeneous and anisotropic distribution of phantom energy. We have determined the exact form of the equation of state of phantom energy that supports the wormhole structure. Interestingly, this equation of state is linear but variable one and is dependent only on the radial parameter of the model.
10 pages, 5 figures
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- General formalism for the stability of thin-shell wormholes in 2+1 dimensions
- Two-fluid evolving Lorentzian wormholes
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- Phantom evolving wormholes with big rip singularities
- (N+1)-dimensional Lorentzian evolving wormholes supported by polytropic matter
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- Thermodynamics of Evolving Lorentzian Wormhole at Apparent and Event Horizons
- Singularity free stars in (2+1) dimensions
- 2+1-dimensional wormhole from a doublet of scalar fields
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- Hypocycloidal throat for 2+1-dimensional thin-shell wormholes
- Three dimensional charged black holes in Gauss-Bonnet gravity
- Magnetic Morris-Thorne wormhole in 2+1-dimensions