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Disconnecting a Traversable Wormhole: Universal Quench Dynamics in Random Spin Models

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arxiv 2009.00277 v1 pith:L72AH4SH submitted 2020-09-01 cond-mat.quant-gas cond-mat.dis-nncond-mat.str-elhep-th

classification cond-mat.quant-gascond-mat.dis-nncond-mat.str-elhep-th
keywords gravityquantumdynamicsdifferentphysicsfieldquenchsystems
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Understanding strongly interacting quantum matter and quantum gravity are both important open issues in theoretical physics, and the holographic duality between quantum field theory and gravity theory nicely brings these two topics together. Nevertheless, direct connections between gravity physics and experimental observations in quantum matter are still rare. Here we utilize the gravity physics picture to understand quench dynamics experimentally observed in a class of random spin models realized in several different quantum systems, where the dynamics of magnetization are measured after the external polarization field is suddenly turned off. Two universal features of the magnetization dynamics, namely, a slow decay described by a stretched exponential function and an oscillatory behavior, are respectively found in different parameter regimes across different systems. This work addresses the issues of generic conditions under which these two universal features can occur, and we find that a natural answer to this question emerges in the gravity picture. By the holographic duality bridged by a model proposed by Maldacena and Qi, the quench dynamics after suddenly turning off the external polarization field is mapped to disconnecting an eternal traversable wormhole. Our studies show that insight from gravity physics can help unifying different experiments in quantum systems.

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  1. Hot wormholes and chaos dynamics in a two-coupled SYK model

    hep-th 2025-01 conditional novelty 6.0 of 10

    First numerical Lyapunov exponents for the unstable hot wormhole phase of the two-coupled SYK model, obtained via cooling and periodic-driving protocols.

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