Self-Supporting Wormholes in Four Dimensions with Scalar Field
arXiv:2204.08178 · doi:10.1140/epjc/s10052-023-11789-0
Abstract
In this paper, we investigated the space-time obtained by quotients of the space-time. Further quotient with specific is considered. Taking up to the first-order perturbation in metric, we estimated the backreaction of the matter field on space-time geometry. We can calculate the stress-energy tensor's expected value by pulling it back onto the covering space. The average null energy becomes negative when the suitable boundary condition is chosen, resulting in a traversable wormhole.
References in corpus (7)
- Achronal averaged null energy condition
- A holographic proof of the averaged null energy condition
- Behind the geon horizon
- Wormholes in Einstein-scalar-Gauss-Bonnet theories with a scalar self-interaction potential
- Novel traversable wormhole in General Relativity and Einstein-Scalar-Gauss-Bonnet theory supported by nonlinear electrodynamics
- Anti-de Sitter Quotients: When Are They Black Holes?
- Symmetric wormholes in Einstein-vector-Gauss-Bonnet theory