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Holographic Schwinger-Keldysh effective field theories including a non-hydrodynamic mode

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arxiv 2411.16306 v2 pith:3PW2VB62 submitted 2024-11-25 hep-th cond-mat.str-elgr-qc

classification hep-thcond-mat.str-elgr-qc
keywords modeeffectivenon-hydrodynamicdynamicalfieldholographicincludingschwinger-keldysh
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We derive the Schwinger-Keldysh effective field theories for diffusion including the lowest non-hydrodynamic degree of freedom from holographic Gubser-Rocha systems. At low temperature the dynamical non-hydrodynamic mode could be either an IR mode or a slow mode, which is related to IR quantum critical excitations or encodes the information of all energy scales. This additional dynamical vector mode could be viewed as an ultraviolet sector of the diffusive hydrodynamic theory. We construct two different effective actions for each case and discuss their physical properties. In particular we show that the Kubo-Martin-Schwinger symmetry is preserved.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Comparison between Causal and Acausal Diffusion: a Schwinger-Keldysh Effective Field Theory Perspective

    hep-th 2025-06 conditional novelty 6.0 of 10

    One-loop real-time density correlations in causal diffusion reduce to known acausal results in the overdamped limit and yield a new universal scaling function in the underdamped limit.

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