Plasma oscillations within Israel-Stewart theory
Lorenzo Gavassino
TL;DR
The work shows that plasma oscillations predicted by a Drude-like kinetic model persist within Israel-Stewart magnetohydrodynamics when coupled to Maxwell equations, revealing that the nonhydrodynamic sector can describe genuine plasmons. Through the Onsager-Casimir principle, it is shown that uncharged kinetic theories at $k=0$ are purely relaxational due to PT symmetry, while coupling to the PT-odd electric field introduces an antisymmetric interaction that yields at most one pair of oscillatory nonhydrodynamic modes per spatial direction. A concrete bound is established: in a kinetic theory with $N$ non-equilibrium moments, at most two plasmons can exist, with all other modes remaining on the imaginary axis. The results broaden the predictive scope of Israel-Stewart MHD to timescales around the plasma period $\omega_p^{-1}$, clarifying its relevance for electromagnetic processes in metals, astrophysical plasmas, and possibly heavy-ion collision contexts, by linking the macroscopic relaxation dynamics to underlying plasmons via a thermodynamic symmetry framework.
Abstract
It is well known that, at zero wavenumber, the non-hydrodynamic frequencies of uncharged kinetic theory are purely imaginary. On the other hand, it was recently shown that, in resistive magnetohydrodynamics, the interplay between the Israel-Stewart relaxation equation and the Ampère-Maxwell law can give rise to a pair of oscillating non-hydrodynamic modes. In this work, we analyze this phenomenon in detail. We first demonstrate that these oscillatory modes are exact solutions of the Drude model, corresponding to ordinary plasma oscillations. We then invoke the Onsager-Casimir principle to explain that their oscillatory nature reflects the distinct PT-transformation properties of the degrees of freedom: the distribution function is even, while the electric field is odd. Finally, we establish that, in a kinetic theory of charged particles, there can be at most one such pair of oscillatory modes per spatial dimension, while all other modes still must sit on the imaginary axis.
