Wormhole: The Birth of a Black Hole ✎ express

Original: "Wormhole Dynamics: Nonlinear Collapse and Gravitational-Wave Emission"
· Nikita M. Shirokov
arXiv:2604.00071 · 2026-03-31 · arXiv non-exclusive · independent analysis · 1 min
Physicists simulated the collapse of an unstable wormhole and produced gravitational waves.

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A wormhole is a hypothetical tunnel that shortens the path between distant corners of the universe, like a soap bubble stretched between two points. To keep the bubble's walls from closing, a special film is needed — matter with negative pressure, akin to dark energy. But this support isn't eternal: remove half the film, and the bubble bursts.

Physicists tested this scenario on a computer. They simulated how, as the support weakens, the wormhole collapses, giving birth to a black hole. Meanwhile, the swallowed matter doesn't vanish without a trace: it's ejected back in a powerful burst, like spray from a burst balloon. The disturbance ripples through space as gravitational waves, racing at the speed of light.

A signal from a wormhole of a thousand solar masses, a million light-years away, is still too faint for today's detectors. But future gravitational antennas like the Einstein Telescope will be able to catch this "echo." And then we will hear how, for a moment, space turns into a punctured bubble.

The term 'wormhole' was coined by physicist John Wheeler in 1957, though the idea itself traces back to Einstein and Rosen.

In 'Interstellar,' the wormhole near Saturn was held open by invisible matter. Remove it, and the tunnel would collapse, just as in the physicists' models.

Scientists
Albert EinsteinBarry BarishKip ThorneRichard FeynmanRussell HulseHenri Poincaré
Concepts
wormhole resonance gravitational wave echoes gravitational collapse black hole echo black hole ringdown throat Wormhole critical collapse starobinsky inflation inspiral pulsar glitch black hole ringdown overtones inflationary gravitational waves