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A rapidly expanding Bose-Einstein condensate: an expanding universe in the lab

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

We study the dynamics of a supersonically expanding ring-shaped Bose-Einstein condensate both experimentally and theoretically. The expansion redshifts long-wavelength excitations, as in an expanding universe. After expansion, energy in the radial mode leads to the production of bulk topological excitations -- solitons and vortices -- driving the production of a large number of azimuthal phonons and, at late times, causing stochastic persistent currents. These complex nonlinear dynamics, fueled by the energy stored coherently in one mode, are reminiscent of a type of "preheating" that may have taken place at the end of inflation.

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2026 2

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UNVERDICTED 2

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representative citing papers

Collective excitations in quantum gravity condensates

gr-qc · 2026-05-18 · unverdicted · novelty 6.0

Collective excitations analogous to phonons are derived in quantum gravity condensates within a group field theory model, yielding leading beyond-mean-field corrections to emergent Friedmann dynamics.

Laboratory rivers extremize friction and are cosmological analogues

physics.geo-ph · 2026-05-14 · unverdicted · novelty 6.0

River cross-sectional profiles satisfy the Friedmann equation for an Anti-de Sitter universe; the associated action extremizes friction and dissipation, and the extremum is a maximum by second variation analysis.

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Showing 2 of 2 citing papers.

  • Collective excitations in quantum gravity condensates gr-qc · 2026-05-18 · unverdicted · none · ref 110 · internal anchor

    Collective excitations analogous to phonons are derived in quantum gravity condensates within a group field theory model, yielding leading beyond-mean-field corrections to emergent Friedmann dynamics.

  • Laboratory rivers extremize friction and are cosmological analogues physics.geo-ph · 2026-05-14 · unverdicted · none · ref 22 · internal anchor

    River cross-sectional profiles satisfy the Friedmann equation for an Anti-de Sitter universe; the associated action extremizes friction and dissipation, and the extremum is a maximum by second variation analysis.