Fluffy Black Holes: The Flickering Tangle and the Paradox ✎ express

Original: "Entanglement islands, fuzzballs and stretched horizons"
arXiv:2605.08347 · 2026-05-08 · arXiv non-exclusive · independent analysis · 1 min
In models of fuzzy black holes, information flickers like a knot on a tangled thread.

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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
Jacob BekensteinStephen HawkingJohn Archibald WheelerFritz ZwickyKarl SchwarzschildSubrahmanyan Chandrasekhar
Concepts
event horizon stability area law black hole entropy inner horizon black hole echo Bekenstein-Hawking entropy apparent horizon horizon area