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Holographic dissipative space-time supersolids

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arxiv 2304.02534 v2 pith:M7Z6FQFM submitted 2023-04-05 hep-th cond-mat.quant-gas

Holographic dissipative space-time supersolids

classification hep-th cond-mat.quant-gas
keywords phaseholographicinternalmethodsmodelspace-timespatialsuperfluid
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Driving a system out of equilibrium enriches the paradigm of spontaneous symmetry breaking, which could then take place not only in space but also in time. The interplay between temporal and spatial symmetries, as well as symmetries from other internal degrees of freedom, can give rise to novel nonequilibrium phases of matter. In this study, we investigate a driven-dissipative superfluid model using holographic methods and reveal the existence of a space-time supersolid (STS) phase which concomitantly breaks the time translation, spatial translation, and the internal U(1) symmetry. The holographic methods naturally include finite temperature effects, which enables us to explore the complex phase diagram of this model and observe a cascade of out-of-equilibrium phase transitions from the STS phase to a synchronized superfluid phase, and finally to a normal fluid phase, by increasing the temperature.

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  1. Quantum Mpemba effect in holography

    hep-th 2026-07 conditional novelty 5.0

    In a holographic superfluid, quenching from stronger symmetry breaking relaxes faster to equilibrium, with the slowest decay mode suppressed and the second mode amplified.