After the Fluid: Subexponential Decay in AdS$_4$

Fuente: arXiv
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Main Authors: Crump, John R. V., Santos, Jorge E.
Format: Preprint
Published: 2026
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author Crump, John R. V.
Santos, Jorge E.
author_facet Crump, John R. V.
Santos, Jorge E.
contents We study the late-time behaviour of nonlinear perturbations of Schwarzschild-AdS$_4$ black branes and show that real-analytic initial data generically enter a regime controlled by the large-$k$ tail of the quasinormal mode spectrum $\{ω_{k\,n}\}$. Using the asymptotic scaling $\mathrm{Im}\,ω_{k\,n} \sim k^{-1/5}$ of the planar AdS$_4$ black brane, we derive a universal prediction that boundary observables decay in a stretched-exponential manner, specifically as $\exp(-c\, t^{5/6})$ up to a mild polynomial prefactor. Fully nonlinear numerical evolutions employing Fourier spectral and discontinuous Galerkin methods confirm this behaviour for small black holes and show consistent scaling - after suppressing long-lived low-$k$ modes - for larger ones. These results indicate that stretched-exponential decay with exponent $5/6$ is a robust feature of AdS$_4$ gravitational dynamics with real-analytic data, arising from geometric-optics physics rather than hydrodynamic modes.
format Preprint
id arxiv_https___arxiv_org_abs_2605_18978
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle After the Fluid: Subexponential Decay in AdS$_4$
Crump, John R. V.
Santos, Jorge E.
High Energy Physics - Theory
General Relativity and Quantum Cosmology
We study the late-time behaviour of nonlinear perturbations of Schwarzschild-AdS$_4$ black branes and show that real-analytic initial data generically enter a regime controlled by the large-$k$ tail of the quasinormal mode spectrum $\{ω_{k\,n}\}$. Using the asymptotic scaling $\mathrm{Im}\,ω_{k\,n} \sim k^{-1/5}$ of the planar AdS$_4$ black brane, we derive a universal prediction that boundary observables decay in a stretched-exponential manner, specifically as $\exp(-c\, t^{5/6})$ up to a mild polynomial prefactor. Fully nonlinear numerical evolutions employing Fourier spectral and discontinuous Galerkin methods confirm this behaviour for small black holes and show consistent scaling - after suppressing long-lived low-$k$ modes - for larger ones. These results indicate that stretched-exponential decay with exponent $5/6$ is a robust feature of AdS$_4$ gravitational dynamics with real-analytic data, arising from geometric-optics physics rather than hydrodynamic modes.
title After the Fluid: Subexponential Decay in AdS$_4$
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2605.18978