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Tiny Universes: Why Their Secrets Are Elusive ⚡ экспресс

Original: "Baby universe as logical qubits: information recovery in random encoding"
· Takato Mori, Beni Yoshida
arXiv:2511.20747 · 2025-11-25 · CC BY 4.0 · ⏱ 1 min · HEP Theory Quantum Physics
Tiny universes are brimming with information, but no one can see it in its entirety — only scattered fragments.
Abstract

A baby universe in quantum gravity might not be empty but could hide a vast amount of information — like a locked room whose keys are shared among several people, but no single person has the full set. This is how scientists explain why information isn’t cloned and doesn’t disappear into a singularity. Could our own Universe be such a 'room with a secret'?

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According to one physical hypothesis, our voluminous world might be a projection from a flat surface. From such a Universe, tiny closed bubbles — baby universes — sometimes pinch off. For a long time, they were thought to be empty, devoid of internal diversity.

It turned out that the information inside them is scattered, like shards of a broken mirror. Each external observer sees only the reflection in their own shard — which means the degree of disorder is high, and the full picture is inaccessible to anyone. This explains why no one can peer into a black hole or grasp what's going on in curved spacetime during collapse.

Such a universe is a broken mirror, and each sees only their own shard.

This approach resolves old paradoxes like the disappearance of information. Hawking was the first to ponder these baby universes, while Maldacena and Susskind built a holographic model.

The most unexpected thing: the clump of matter that pinches off a baby universe itself becomes its first observer, setting one of countless shard arrangements.

🎯 The idea of tiny universes first emerged in Stephen Hawking's work, but was long considered mathematical exotica.

🎬 In science fiction, similar ideas play out in the movie 'Interstellar,' where other dimensions opened up behind a bookshelf.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
entropy black hole spacetime curvature big bang
Laws
Friedmann equationsHubble's lawsecond law of thermodynamicsHawking radiationgravitational lensingBekenstein-Hawking entropy
Original: arXiv:2511.20747 · CC BY 4.0 · bridge42worlds