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Black Hole Did Not Destroy Quantum Entanglement ⚡ экспресс

Original: "Complete freezing of initially maximal entanglement in Schwarzschild black hole"
arXiv:2602.11586 · 2026-02-12 · CC BY 4.0 · ⏱ 1 min · General Relativity Quantum Physics
Physicists have found a state where entanglement doesn't die even near a black hole.
Abstract

Against expectations, near a black hole, the special quantum link between particles does not break down, but stays unchanged at any temperature. As if a dance of four partners remained perfectly synchronized, even when it becomes unbearably hot around. So black holes, it turns out, might be not destroyers, but keepers of quantum secrets.

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Fragile as ice in a furnace, quantum entanglement usually perishes from the slightest heat. Near a black hole, where space is twisted by Einstein's gravity and Hawking radiation Hawking's heats things up, any bond should be destroyed. But physicists found an exception. They took four specially prepared particles (a cluster state) and placed them near a black hole of Schwarzschild Schwarzschild. Force carrier particles (bosons) predictably lost their connection. But matter particles (fermions, like electrons) behaved differently: their entanglement remained exactly the same as it was at the start. Even as the black hole heated up, the bond did not weaken — it was maximal and unchanged.

This was called 'complete freezing': gravity doesn't destroy the bond, it preserves it.

This promises quantum communication and computation in space, where ordinary entanglement perishes from radiation and curved spacetime. The resilience of fermions opens the way to reliable information transfer even near massive objects. While the black hole evaporates and accumulates entropy (disorder), this does not affect the quartet.

🎯 The temperature of large black holes is billionths of a degree above absolute zero, yet even this tiny heating usually destroys quantum effects.

Scientists
Stephen HawkingJacob BekensteinAlbert EinsteinFritz ZwickyVera RubinBernhard Riemann
Tags
black hole spacetime curvature entropy
Laws
second law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropyEinstein field equationsBoltzmann distribution
Original: arXiv:2602.11586 · CC BY 4.0 · bridge42worlds