Quantum gas unlocks the secrets of the universe's birth ✛ ✎

Original: "Expansion-contraction duality breaking in a Planck-scale sensitive cosmological quantum simulator"
arXiv:2506.02719v3 · 2025-06-03 · arXiv non-exclusive · independent analysis · 1 min
Ultracold atoms become a miniature model of the cosmos to reveal hidden ripples left over from the Big Bang.

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.

k^2 W_k = a^2 \lambda_{pl}^{-2} F^2(k \lambda_{pl} / a)
Dispersion relation for perturbation modes: the square of the wavenumber times the power spectrum depends on the Planck length λ_pl, which is set by the trap width. This shows how laboratory parameters relate to the quantum-gravity scale.
Scientists
Alan GuthAlexander FriedmannAndrei LindeGeorges LemaîtreJames PeeblesAdam Riess
Concepts
planck time non singular cosmology cosmological bounce quantum simulation cosmology quantum fluctuation inflation double slit experiment cosmological simulation contraction cosmic bubble nucleation inflaton cosmological constant quantum Hall effect planck scale planck mass quantum ripples quantum vacuum fluctuations bubble collision