Black Hole Did Not Destroy Quantum Entanglement express

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

📄 Showing the "Simple" version — "Popular" is not ready yet. Add it to favorites to help prioritize it.

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 BekensteinWilliam WoottersJohn Stewart BellFritz ZwickyErwin Schrödinger
Concepts
maximal quantum entanglement schwarzschild black hole black hole information paradox hawking area law absolute zero bell states Hawking area theorem greenberger horne zeilinger state schwarzschild metric quantum vacuum event horizon stability Bose-Einstein condensate entanglement protection low temperature information loss cryogenic temperature thermal equilibrium third law of thermodynamics remnant no-hair theorem