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Black Hole Whisper-Changes the Quantum Rhythm ⚡ экспресс

Original: "Geometric Aharonov-Bohm phase effect around a black hole"
· Kaushlendra Kumar, Shahn Majid
arXiv:2605.28582 · 2026-05-27 · CC BY · ⏱ 1 min · General Relativity
Without even touching, a black hole can change the inner rhythm of a passing particle.
Abstract

What does particle motion near a black hole look like if we swap sharp trajectories for probability waves? It turns out that the wave's quantum phase experiences something like an invisible magnetic field — reshaping the whole flow of matter. Could gravity really 'entangle' particles without touching them?

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Spacetime flows like a river, and a black hole is a whirlpool. Particles in this flow are like waves with their own rhythm: alternating crests and troughs. It turns out the whirlpool shifts the wave's rhythm from a distance, without even sucking it in.

A similar effect was discovered by Aharonov and Bohm: an electron 'feels' a magnetic field without entering it — the field whisper-changes its wave.

Near a black hole, a quantum wave undergoes the same subtle shift, even though the particle doesn't cross the hole's edge. The role of the invisible field here is played by curved spacetime. Unexpectedly, the calculations yield the Raychaudhuri equation — it describes the expansion or contraction of matter in Einstein's theory.

This equation predicts the expansion of the universe, and now connects quantum 'ripples' of spacetime with large-scale gravity.

Thus gravity gains a quantum voice.

🎯 The Aharonov-Bohm effect, once dismissed as fantasy, now underlies detectors that can find metal buried in the ground without a single touch.

🎬 In the film 'Interstellar,' the black hole's gravity warps time; the new effect adds a layer: it also whisper-changes the quantum rhythm, as if sending particles a secret message.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole spacetime curvature
Laws
Hawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsequivalence principleno-hair theorem
Original: arXiv:2605.28582 · CC BY · bridge42worlds