A survey of recent studies concerning the extreme properties of Morris-Thorne wormholes
Peter K.F. Kuhfittig

TL;DR
This survey reviews recent research on the extreme properties of Morris-Thorne wormholes, focusing on the necessity of exotic matter, alternative gravity theories, and the potential implications for a multiply-connected universe.
Contribution
It compiles and analyzes various approaches to understanding the high radial tension in wormholes, including modified gravity and the role of exotic matter, offering a comprehensive overview of current challenges and theories.
Findings
Exotic matter is typically required to sustain wormholes but may be minimized.
Modified gravity theories like $f(R)$ can eliminate the need for exotic matter.
High radial tension remains a key challenge in wormhole physics.
Abstract
It has been known for a long time that Morris-Thorne wormholes can only be held open by violating the null energy condition, which can be expressed in the form , where is the radial tension. Matter that violates this condition is usually referred to as "exotic." For any wormhole having a moderately-sized throat, the radial tension is equal to that at the center of a massive neutron star. Attributing this outcome to exotic matter seems reasonable enough, but it ignores the fact that exotic matter was introduced for a completely different reason. Moreover, its problematical nature suggests that the amount of exotic matter be held to a minimum, but this would make the high radial tension harder to explain. If the amount is infinitely small, this explanation breaks down entirely. By invoking modified gravity, the need for exotic matter at the throat could…
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Taxonomy
TopicsCosmology and Gravitation Theories · Geophysics and Gravity Measurements · Pulsars and Gravitational Waves Research
