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Wormholes Without Exotic Matter ⚡ экспресс

Original: "Traversable Wormholes with Non-Exotic Matter: The Role of Higher Curvature Corrections"
arXiv:2605.18376 · 2026-05-18 · CC BY 4.0 · ⏱ 1 min · General Relativity
A new theory of gravity frees wormholes from the need for exotic matter—just rethink the geometry of space.
Abstract

In an extended theory of gravity, f(R,□R), where the action includes the d’Alembertian of the curvature scalar (□R), scientists explored the possibility of traversable wormholes. By deriving field equations for a static spherical wormhole, they showed that higher-order corrections contribute effectively to the energy-momentum tensor, reducing the need for exotic matter or eliminating it entirely. It's like an arch that holds itself up by its shape, without extra supports. The findings suggest that quantum corrections to general relativity could make wormholes physically possible.

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A wormhole is a tunnel through the fabric of spacetime, an idea expanded by John Wheeler and Kip Thorne. Just as a mountain passage tends to cave in, the throat of a wormhole wants to snap shut. Normally, it's propped open with exotic matter that has negative energy—a substance that pushes space apart, like dark energy. Only we don't have any.

Now, researchers have revisited gravity. Instead of hunting for nonexistent material, they tweaked the equations, adding extra spacetime curvature. Think of an arch bridge: to keep a span from falling, you could prop it with beams you lack, or you can design the arch's curve so it holds itself. Here, the geometry of space is the support. The math checks out: a traversable wormhole (a cousin of black holes) works without exotic matter, and the forces inside are no stronger than Earth's gravity. Sci-fi portals become a far-future engineering challenge.

🎯 Physicist John Wheeler coined the term "wormhole," comparing spacetime to an apple a worm bores through.

🎬 In the movie Interstellar, a wormhole let the heroes cross the galaxy in an instant.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesStephen HawkingJacob Bekenstein
Tags
spacetime curvature black hole dark energy
Laws
Friedmann equationsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsequivalence principle
Original: arXiv:2605.18376 · CC BY 4.0 · bridge42worlds