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Diving inside holographic metals

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arxiv 2408.07748 v2 pith:D56XVJD3 submitted 2024-08-14 hep-th gr-qc

classification hep-thgr-qc
keywords cloudcollapseelectronfixedholographickasnernear-singularityneutral
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We investigate the gravitational dual of a fermionic field theory at finite temperature and charge density in two spatial dimensions, subject to a deformation by a relevant scalar operator. This makes a $(3+1)$-dimensional Einstein-Maxwell system coupled to a free fermion fluid, known as an electron cloud, undergo a holographic renormalization group flow. The inner (Cauchy) horizon is destroyed and the near-singularity metric instead adopts the form of a positive-$p_t$ Kasner cosmology, signaling the collapse of the Einstein-Rosen bridge. Previous studies have suggested that this collapse hinders direct probing of the singularity. Nonetheless, we propose and compute several CFT observables that characterize the interior and near-singularity geometries. These include the thermal $a$-function, which decays with a specific power of $p_t$ as nearly all CFT degrees of freedom are integrated out, and two-point correlators for neutral and charged operators, with the latter directly probing the singularity despite the positive-$p_t$. We also calculate characteristic velocities related to entanglement and complexity growth in the time-evolved thermofield double state, as well as the butterfly effect indicative of operator spreading. Notably, the deformed electron cloud features a Lifshitz IR fixed point and an additional Kasner trans-IR fixed point, absent in neutral RG flows.

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Cited by 2 Pith papers

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

  1. Non-Hermitian Holographic Flows to Little Rip Cosmologies

    hep-th 2026-07 conditional novelty 8.0 of 10

    A holographic model of a non-Hermitian PT-symmetric QFT produces black hole interiors that are isotropic Little Rip cosmologies, separated from standard Kasner behavior by a distinctive logarithmic signature in heavy-...

  2. Scrambling in charged hairy black holes and the Kasner interior

    hep-th 2025-01 conditional novelty 5.0 of 10

    In a charged hairy black hole, increasing the boundary deformation parameter lowers the Lyapunov exponent relative to surface gravity but can push it above the axion Reissner-Nordström value, and generally shortens th...

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