Traversable Ghost Wormholes Explored
Analysis
This paper explores the theoretical possibility of 'ghost stars' within the framework of traversable wormholes. It investigates how these objects, characterized by arbitrarily small mass and negative energy density, might exist within wormhole geometries. The research highlights potential topological obstructions to their straightforward realization and provides a concrete example using a Casimir-like wormhole. The analysis of the Penrose-Carter diagram further illustrates the properties of the resulting geometry.
Key Takeaways
- •Investigates the connection between ghost-like configurations and traversable wormholes.
- •Analyzes the Hawking mass to understand the existence of ghost configurations.
- •Highlights topological obstructions to the straightforward realization of ghost configurations.
- •Provides a concrete example of a Casimir-like traversable wormhole.
- •Analyzes the Penrose-Carter diagram to illustrate the geometry's properties.
Reference
“The paper demonstrates that a Casimir-like traversable wormhole can be naturally constructed within this framework.”