Quasinormal modes in charged fluids at complex momentum
Aron Jansen, Christiana Pantelidou
TL;DR
We investigate the convergence of relativistic hydrodynamics in charged fluids within holography by combining nonperturbative spectral-curve analysis with high-order small-$k$ perturbations in $AdS_{d+1}$ RN black-brane backgrounds. The study shows a finite radius of convergence at zero charge for all hydrodynamic channels, while approaching extremality drives the radius to zero for shear and sound (diffusion can remain finite). Pole skipping is analyzed via Matsubara frequencies and chaos points, revealing a complex, charge-dependent structure that does not universally constrain the convergence radius. Across $d=3,4$, the perturbative and spectral-curve methods agree quantitatively, clarifying previous neutral-versus-charged results and highlighting the distinct roles of different pole-collision mechanisms.
Abstract
We investigate the convergence of relativistic hydrodynamics in charged fluids, within the framework of holography. On the one hand, we consider the analyticity properties of the dispersion relations of the hydrodynamic modes on the complex frequency and momentum plane and on the other hand, we perform a perturbative expansion of the dispersion relations in small momenta to a very high order. We see that the locations of the branch points extracted using the first approach are in good quantitative agreement with the radius of convergence extracted perturbatively. We see that for different values of the charge, different types of pole collisions set the radius of convergence. The latter turns out to be finite in the neutral case for all hydrodynamic modes, while it goes to zero at extremality for the shear and sound modes. Furthermore, we also establish the phenomenon of pole-skipping for the Reissner-Nordstrom black hole, and we find that the value of the momentum for which this phenomenon occurs need not be within the radius of convergence of hydrodynamics.
