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Fluffy Black Holes: The Flickering Tangle and the Paradox ⚡ экспресс

Original: "Entanglement islands, fuzzballs and stretched horizons"
arXiv:2605.08347 · 2026-05-08 · CC BY · ⏱ 1 min · HEP Theory General Relativity
In models of fuzzy black holes, information flickers like a knot on a tangled thread.
Abstract

Scientists studied how the fuzzball model (instead of a black hole) affects information preservation. Replace the event horizon with a reflective wall, and quantum “islands” of information may flicker, sparking a paradox. In more realistic models, islands often don’t appear. So is information inside a black hole there or not—like a mirage in a mirrored room?

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A black hole is usually depicted as an abyss with a point of no return. To save information—which quantum laws forbid from disappearing—physicists replaced that boundary with a fluffy tangle of microscopic strings. Infalling data gets permanently imprinted into its intertwined threads. Recently, the idea emerged of adding entropy islands inside the tangle—tiny regions where hidden information suddenly becomes visible, like a knot momentarily peeking out of tangled wool. But calculations show that depending on the structure of the tangle’s reflective surface, these islands behave capriciously. They flicker—appearing and then promptly falling back, as if someone is tugging the threads.

In reality, this would mean that information is sometimes saved, sometimes lost again, leaving the paradox unresolved.

In more precise models that account for spacetime curvature near the tangle, the islands don’t appear at all. The black hole securely hides its secrets, and the puzzle posed by Stephen Hawking and Jacob Bekenstein only deepens.

🎯 From the outside, this tangle looks exactly like an ordinary black hole. You can tell them apart only by quantum jitters near the horizon—so subtle that detecting them is currently impossible.

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:2605.08347 · CC BY · bridge42worlds