2025/12/11 by Richard A. Davison, Davison, Richard A., Andre Pinheiro +1 · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #FOS: Physical sciences #High Energy Physics - Theory (hep-th) #Quantum Electrodynamics and Casimir Effect
paper · pdf · doi:10.48550/arxiv.2512.10905
openalex publication_date 2025/12/11 · openalex created_date 2025/12/13 · openalex updated_date 2026/07/28
We study the dynamics of an isotropic, planar AdS black hole charged under a pair of two-form gauge potentials. We prove that long wavelength, small amplitude perturbations of this state are governed by the relativistic theory of viscoelastic hydrodynamics. We use this effective theory to identify instabilities in certain regions of parameter space, and show that the dominant instability is always driven by fluctuations of an incoherent density of the higher-form charge. The spacetime we study also arises as a solution to gravity coupled to a pair of massless scalar fields, where part of its dynamics is governed by a simpler effective theory of heat diffusion. We derive this simpler description directly from viscoelastic hydrodynamics, demonstrating that the heat diffusion mode is the collective excitation of the viscoelastic fluid under no-flux boundary conditions.