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Wormhole Shadow: Sharp Angles When Rotating ⚡ экспресс

Original: "On the Cuspy Structure of Rotating Wormhole Shadows"
· Peng Cheng, Ruo-Fan Xu, Peng Zhao
arXiv:2602.14182 · 2026-02-15 · CC BY 4.0 · ⏱ 1 min · General Relativity High Energy
A wormhole’s rotation turns its shadow into something like a gear — with sharp teeth instead of a smooth circle.
Abstract

Scientists studied what the silhouette (shadow) of a rotating wormhole — a hypothetical tunnel through space — looks like. It turns out its shape can change from smooth to pointy, with 'ears', depending on the wormhole's properties. Imagine a telescope capturing such an 'eared' shadow — and we realize it's a wormhole, not a black hole.

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A wormhole is a tunnel through space, connecting distant regions of the Universe. Its shadow against a bright gas background was long thought to be as round as that of a black hole. But for a rotating wormhole (one you could actually traverse), the shape of the shadow might be surprising: the edge becomes jagged, like a gear.

A black hole's shadow stays circular even at furious rotation. A wormhole behaves differently.

If light passing through its throat is strongly 'stretched' (shifting in color toward red), then rotation causes the shadow to develop sharp protrusions. Researchers found a critical threshold: as soon as this stretching reaches a certain value, the shadow abruptly acquires teeth.

Such a 'jagged' silhouette is a key for future telescopes. If instead of a smooth shadow astronomers see a structure with notches, it would point not to a black hole, but to a wormhole.

🎯 Wormholes haven't been discovered yet, but Einstein's equations allow for their existence — just like black holes once were.

🎬 In Interstellar, the journey through a wormhole happened without its shadow — too bad: perhaps it would have looked like a gear.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole spacetime curvature photometry
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsStefan–Boltzmann lawequivalence principle
Original: arXiv:2602.14182 · CC BY 4.0 · bridge42worlds