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Analog gravity: cold-atom simulation

If you cannot compute a system, perhaps you can build one. Cold-atom Bose–Einstein condensates obey the same equations as scalar-field dark matter — making them candidate laboratory analogs of wave dark matter and early-universe physics.

The analogy

A laboratory BEC is governed by the Gross–Pitaevskii equation (Topic 3.4) — the same nonlinear-Schrödinger physics that describes self-gravitating scalar-field dark matter on galactic scales. Solitons, interference, coherent nonlinear evolution: all appear in both. This makes cold atoms a candidate analog in which wave-dark-matter phenomenology could be probed in a lab rather than inferred from astrophysics.

Simulating the early universe

Jenkins et al. (2024) — the second frontier paper Sandro flagged — advance this programme by studying vacuum decay: false-vacuum bubble nucleation (figure), a relativistic early-universe process, realized in an ultracold potassium-41 condensate. They extend earlier classical treatments to include the quantum fluctuations of the analog vacuum, and show its fluctuation spectrum matches the relativistic field-theory result.

Worked example — what the analogy buys

Vacuum decay is a strongly non-perturbative, quantum process that is notoriously hard to simulate classically or observe cosmologically. A tabletop cold-atom system that reproduces its physics — bubble nucleation rates, fluctuation spectra — offers an experimental handle on scalar-field dynamics that FDM shares. It is empirical access to physics otherwise reachable only through simulation.

Analog gravity: a cold-atom condensate realizes false-vacuum bubble nucleation (Jenkins et al. 2024). The same Gross–Pitaevskii physics underlies fuzzy dark matter, making such platforms candidate lab analogs.

Relevance to fuzzy dark matter

The condensate physics is the same self-gravitating (or self-interacting) scalar-field dynamics FDM invokes. While Jenkins et al. target early-universe phase transitions rather than dark matter directly, the platform is among the few settings where wave-dark-matter phenomenology — solitons, coherence, nonlinear waves — might be studied experimentally.

Where it stands

Like the quantum-algorithm frontier, this is early and not FDM-specific. We catalogue it (survey §24.6) as an adjacent method whose maturation would enlarge a toolbox the wave problem is starved of — experimental, rather than computational, reach.

A false-vacuum bubble growing in the cold-atom analog — the process Jenkins et al. simulate.
In our research

This is the second frontier paper Sandro flagged (Jenkins et al. 2024, in our survey §24.6 and Papers tab). It connects through the shared Gross–Pitaevskii/nonlinear-Schrödinger physics (Topic 3.4) — cold atoms as a possible laboratory analog of the wave dynamics our codes simulate.

Key references
  • Jenkins et al. (2024), Analog vacuum decay from vacuum initial conditions, Phys. Rev. D 109, 023506 (arXiv:2307.02549).
  • Fialko et al. (2015), Fate of the false vacuum: cold-atom analog, EPL 110, 56001.
  • Pethick & Smith, Bose–Einstein Condensation in Dilute Gases.