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Wormhole on a quantum chip ⚡ экспресс

Original: "Quantum simulation of traversable-wormhole-inspired quantum teleportation in a chaotic binary sparse SYK model"
arXiv:2604.10090 · 2026-04-11 · CC BY · ⏱ 1 min · HEP Theory Quantum Physics
Physicists simulated a traversable wormhole on a noisy quantum processor and observed a key signature of teleportation.
Abstract

Scientists used a quantum computer to transmit information through a kind of wormhole, harnessing the chaos of many particles. It's as if two ends of the universe connected for a moment. Despite the noise, they spotted a key characteristic: signal asymmetry. Will this bring us closer to unraveling quantum gravity?

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Physicists found out: to open a wormhole, you have to shake it hard. Not literally — but on a quantum chip, they simulated a system of 8 particles, so chaotic and entangled that it turned into a vibrating hologram of a black hole. The theory of Susskind and Kitaev came to life in a real, though noisy, processor: the stronger the system's jitter, the clearer the tunnel emerges.

A signal was sent through this virtual funnel. It passed through, but came out with different intensity: the positive impulse passed differently than the negative one. Exactly how a real traversable wormhole would behave. The equipment's noise didn't erase the picture, but only confirmed it — for teleportation, internal shaking is exactly what's needed.

The main surprise: the same math describes any black hole as a holographic projector. All infalling information doesn't disappear, but is sort of recorded on its surface — like on a trembling film. Now physicists have a miniature proving ground for testing such ideas, which John Preskill dreamed of.

🎯 The idea that gravity can emerge from entanglement is called the holographic principle — as if our three-dimensional world is projected from a flat surface.

🎬 In Interstellar, the wormhole was meant for people, and here — for signals, but the principle is the same.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
spacetime curvature black hole entropy
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2604.10090 · CC BY · bridge42worlds