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    Efimov-like phonon production for an analog coasting universe in Bose-Einstein condensates

    Yunfei Xue1, Jiabin Wang2, Li Chen2,*, Chenwei Lv3,4,5,†, and Ren Zhang1,6,‡

    • 1MOE Key Laboratory for Nonequilibrium Synthesis and Modulation of Condensed Matter, Shaanxi Province Key Laboratory of Quantum Information and Quantum Optoelectronic Devices, School of Physics, Xi'an Jiaotong University, Xi'an 710049, China
    • 2Institute of Theoretical Physics, State Key Laboratory of Quantum Optics and Quantum Optics Devices, Shanxi University, Taiyuan 030006, China
    • 3Department of Physics, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong, China
    • 4The State Key Laboratory of Quantum Information Technologies and Materials, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong, China
    • 5New Cornerstone Science Laboratory, The Chinese University of Hong Kong, Shatin, New Territories, Hong Kong, China
    • 6Hefei National Laboratory, Hefei 230088, China

    • *Contact author: lchen@sxu.edu.cn
    • †Contact author: lcw205046@gmail.com
    • ‡Contact author: renzhang@xjtu.edu.cn

    Phys. Rev. A 114, 043310 – Published 22 October, 2026

    DOI: https://doi.org/10.1103/srl6-3v7v

    Abstract

    Efimov physics is characterized by discrete scale invariance and log-periodic observables. It emerges when an underlying continuous scale invariance is broken. While spatial Efimov physics has been extensively studied, realizing an analogous phenomenon associated with temporal scale invariance remains challenging because it requires a dynamical system that breaks time-translation symmetry while retaining time-scaling structure. Analog cosmology offers a powerful platform to address this challenge, bridging the domains of Efimov physics and cosmology. Here, we predict a temporal Efimov-like effect in an analog linearly expanding universe realized with a quasitwo-dimensional Bose-Einstein condensate. The invariance of phonon mode equations under time-scaling leads to particle production with two distinct dynamics: power-law growth and log-periodic oscillations, with the latter being the hallmark signature of Efimov-like discrete scale invariance. Furthermore, these dynamics map directly onto sub- and superhorizon cosmological modes. Our predictions can be tested through time-averaged measurements of the density-fluctuation spectrum Sk(t) in current experiments.

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