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Acoustic Black Holes Get Entangled Differently ⚡ экспресс

Original: "Entanglement entropy of an acoustic black hole"
arXiv:2605.30540 · 2026-05-28 · CC BY · ⏱ 1 min · Quantum Gases General Relativity
In an acoustic black hole, quantum entanglement fills the entire volume, not just the boundary.
Abstract

Researchers studied an acoustic black hole (a flow where sound gets trapped) and discovered that quantum entanglement inside it grows with volume, not surface area. Imagine cobwebs packing a whole ball, not just coating its shell. Why? It's all about paired sound waves born at the horizon.

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An acoustic black hole is a fluid flow faster than sound, so sound waves can't escape. The boundary—the surface where the flow speed reaches the speed of sound—spawns pairs of phonons: sound quanta, one flying away, the other plunging inward.

In a regular black hole, the amount of hidden information (entropy) is proportional to the horizon area—this idea was proposed by Jacob Bekenstein and Stephen Hawking.

Calculations show that the entropy of entanglement here depends on volume, not horizon area. Phonons throughout the interior are connected to each other—as if invisible strings weave through a waterfall, linking every drop to the others. Paradoxically, particles born at the boundary and forever separated by it retain a shared memory at any distance inside the flow.

Acoustic analogues of black holes were first proposed by William Unruh to study quantum effects without involving the complex geometry of curved spacetime.

🎯 If interstellar gas flowed around a massive object at supersonic speed, an acoustic black hole would form—and even the roar of a supernova couldn't escape.

🎬 In Fred Hoyle's novel 'The Black Cloud,' an intelligent gas cloud manipulates matter flows, resembling an acoustic analogue but without quantum effects.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole entropy spacetime curvature
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2605.30540 · CC BY · bridge42worlds