Non-Hydrodynamic Solutions to the linear Density-dependent BGK equation
Florian Kogelbauer
TL;DR
This work investigates the linear density-dependent BGK equation in $d$ dimensions to distinguish hydrodynamic and non-hydrodynamic regimes. It combines spectral analysis of the BGK operator with an explicit Laplace–Fourier solution to obtain a time-domain formula for the macroscopic density, revealing a critical wave number $k_c = \frac{1}{\tau}\sqrt{\frac{\pi}{2}}$ that separates regimes. For $|k|<k_c$ the macroscopic dissipation follows Chapman--Enskog scaling, yielding $\Delta[\hat{\rho}](k,t,\tau) \sim \tau |k|^2$ as $\tau\to0$, while for $|k|\ge k_c$ the dynamics are governed by the essential spectrum and produce a dissipation $\Delta[\hat{\rho}](k,t,\tau) \sim \frac{Z'(\hat{\zeta}_\beta)}{\tau}$ (with $\beta=\tau|k|$ and $Z(\hat{\zeta}_\beta)=i\beta$), causing a $1/\tau$ divergence. These results demonstrate non-hydrodynamic exact solutions and highlight the nonuniform nature of hydrodynamic limits, with implications for how Closures and reduced-order models may fail to capture certain fast kinetic fluctuations.
Abstract
We prove the existence of non-hydrodynamic solutions to the linear density-dependent BGK equation in $d$ dimensions. Specifically, we show the existence of an initial condition for any Knudsen number $τ$ for which the dissipation rate of the macroscopic mass density diverges $\sim 1/τ$. Our results rely on a detailed spectral analysis of the linear BGK operator, an explicit solution formula for the time-dependent problem using a combination of Fourier series with the Laplace transform and subsequent contour integration arguments from complex analysis.
