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Quantum gas unlocks the secrets of the universe's birth ⚡ экспресс

Original: "Expansion-contraction duality breaking in a Planck-scale sensitive cosmological quantum simulator"
Ultracold atoms become a miniature model of the cosmos to reveal hidden ripples left over from the Big Bang.
Abstract

Imagine that ripples on water could tell us about the birth of the universe. Physicists have created an analogue of cosmic ripples in a cloud of supercooled atoms and saw how invisible quantum 'whispers' can alter the large-scale picture. Could a handful of atoms shed light on the mysteries of the Big Bang?

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To peer 14 billion years into the past, you don’t need a telescope—just a cloud of atoms chilled to near absolute zero. In the Bose–Einstein condensate state, discovered by Bose and Einstein, atoms merge into a giant synchronized wave. By tuning magnetism, scientists turn this wave into a tiny “pond” that models spacetime right after the Big Bang—complete with its ripples of primordial inhomogeneities. The key discovery: when the “pond” expands (like our universe), small ripples vanish without a trace, and when it contracts, large ones disappear. This “Planckian damping” breaks symmetry: contrary to expectations, ripples are not the same at all scales. This effect is a direct consequence of spacetime ceasing to be smooth at the smallest scales (where curvature plays a role). For the first time, a lab trick allows us to distinguish the inflationary theory of Alan Guth from other scenarios and peek beyond the Standard Model without giant accelerators. The temperature of this “cosmos” is a hundred million times lower than the interstellar void: the slightest heat would destroy the entire simulation.

🎯 The gas is cooled to a few billionths of a degree above absolute zero—so cold that even the cosmic microwave background, cooled after the Big Bang, feels hot.

Scientists
Alan GuthAndrei LindeGeorges LemaîtreJames PeeblesAdam RiessBrian Schmidt
Tags
big bang expansion of the universe spacetime curvature Standard Model
Laws
Friedmann equationsHubble's lawNoether's theoremEinstein field equationsPlanck's lawequivalence principle
Original: arXiv:2506.02719v3 · CC BY · bridge42worlds