Interster

An Interster is a hypothetical stellar object that exists entirely within a wormhole, its mass-energy contributing to the stability and maintenance of the wormhole itself. Unlike a star viewed through a wormhole, which would be a distinct object on the "other side," an Interster is the wormhole.

Conceptual Underpinnings:

The concept arises from theoretical physics, specifically in the context of exotic matter and traversable wormholes. Maintaining a wormhole requires negative mass-energy density, a concept that challenges our understanding of known physics. An Interster proposes a scenario where a star-like entity, composed perhaps of exotic matter or existing in a state governed by unknown physical laws, provides this necessary negative energy density. Its gravitational effects would actively counteract the natural tendency of the wormhole to collapse.

Theoretical Properties:

• Location: Located entirely within the throat of the wormhole.
• Composition: Hypothetical, possibly composed of exotic matter or matter in an unknown state.
• Stability: Its mass-energy distribution is crucial for maintaining the wormhole's traversability.
• Observable Characteristics: Direct observation from outside the wormhole would be impossible, as the Interster is the wormhole. Indirect observation might be possible by analyzing gravitational lensing or other effects on light and matter passing nearby.
• Formation: The formation mechanism is purely speculative, requiring conditions drastically different from those observed in our universe.

Scientific Status:

The Interster remains a purely theoretical construct. No observational evidence supports its existence, and its theoretical feasibility depends on the validity of currently unproven or debated physics. It is primarily a thought experiment exploring the potential connection between stellar objects and wormhole physics.