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Exact interpolation between Fick and Cattaneo diffusion in relativistic kinetic theory

Lorenzo Gavassino

Abstract

We construct a family of exactly solvable relativistic kinetic theories in $1+1$ dimensions whose hydrodynamic sector continuously interpolates between Fick's and Cattaneo's laws of diffusion. The interpolation is controlled by a single parameter $a\in[0,1]$, which tunes the microscopic scattering dynamics from infinitely soft but infinitely frequent scatterings ($a=0$), reproducing standard diffusion, to maximally hard but finite-rate scatterings ($a=1$), yielding hyperbolic Cattaneo-type transport. For intermediate values of $a$, the dynamics combines frequent weak scatterings with rare strong randomizing events, providing a concrete microscopic realization of mixed diffusive-telegraphic behavior. Remarkably, the full quasinormal mode spectrum can be obtained analytically for all $a$. This allows us to track explicitly how purely diffusive modes continuously deform into damped propagating modes as the collision structure is varied.

Exact interpolation between Fick and Cattaneo diffusion in relativistic kinetic theory

Abstract

We construct a family of exactly solvable relativistic kinetic theories in dimensions whose hydrodynamic sector continuously interpolates between Fick's and Cattaneo's laws of diffusion. The interpolation is controlled by a single parameter , which tunes the microscopic scattering dynamics from infinitely soft but infinitely frequent scatterings (), reproducing standard diffusion, to maximally hard but finite-rate scatterings (), yielding hyperbolic Cattaneo-type transport. For intermediate values of , the dynamics combines frequent weak scatterings with rare strong randomizing events, providing a concrete microscopic realization of mixed diffusive-telegraphic behavior. Remarkably, the full quasinormal mode spectrum can be obtained analytically for all . This allows us to track explicitly how purely diffusive modes continuously deform into damped propagating modes as the collision structure is varied.

Paper Structure

This paper contains 14 sections, 29 equations, 4 figures.

Figures (4)

  • Figure 1: Dispersion relations $\omega=-i\mathfrak{D}k^2$ and $\omega=-i\mathfrak{D}(k^2-\omega^2)$ for Fick (blue) and Cattaneo (red) diffusion, respectively, as obtained from the corresponding kinetic theories. Left panel: Frequency plotted as a function of imaginary $k$. The Fick branch terminates at $|\mathfrak{Im}k|=(2\mathfrak{D})^{-1}$, beyond which the information current associated with the mode \ref{['ansatz']} diverges, rendering the mode unphysical (the particle density itself diverges at $|\mathfrak{Im}k|=\mathfrak{D}^{-1}$). By contrast, the Cattaneo branches extend to arbitrarily large $|k|$. As expected, none of the curves enter the region $\mathfrak{Im}\omega<|\mathfrak{Im}k|$ (shaded), where the modes would become unstable under Lorentz boosts GavassinoBounds2023myj. Right panel: Frequency plotted as a function of real $k$. Both Fick and Cattaneo branches extend over the full real axis. In the Cattaneo case, $i\mathfrak{D}\omega$ develops an imaginary part (red dashed) for $|k|>(2\mathfrak{D})^{-1}$, indicating the onset of propagating behavior Pu2010BAGGIOLI20201GavassinoGENERIC:2022isg. In both cases, one finds $\mathfrak{Im}\omega\leq 0$, consistent with linear stability.
  • Figure 2: Hydrodynamic dispersion relation $\omega(k)$ of the Fokker-Planck-Anderson-Witting kinetic theory \ref{['interpuls']} for imaginary wave number and various values of the parameter $a$ (see equation \ref{['parameterization']}). Left panel: As $a$ increases (orange: $a=1/5$, brown: $a=2/3$, red: $a=0.98$), the dispersion relation interpolates continuously between Fick’s law (upper dashed curve), with $\mathfrak{D}=\tau/4$, and Cattaneo’s law (lower dashed curve), with $\mathfrak{D}=\tau$. Throughout this deformation, the continuous spectrum remains fixed and occupies the region $i\omega\geq -|ik|+1/\tau$ (yellow shading). Consistently with causality HellerBounds2022ejwGavassinoDistrubingMoving:2026klp, none of the branches enters the unstable region $\mathfrak{Im}\omega<|\mathfrak{Im}k|$ (red shading). Right panel: For $a<2/3$, the hydrodynamic branch merges with the continuous spectrum at a finite value $(ik\tau)_{\text{max}}$, beyond which it ceases to exist. In particular, at $a=0$ one recovers Fick’s law, which is defined only for $|\mathfrak{Im}(k\tau)|<2$. As $a$ increases, $(ik\tau)_{\text{max}}$ grows monotonically and diverges as $a\to 2/3$, signaling the transition to the Cattaneo regime, where the dispersion relation extends over the entire imaginary axis.
  • Figure 3: Left panel: Non-propagating branch of the discrete dispersion relation $\omega(k)$ of the interpolating kinetic theory \ref{['interpuls']} for real wavenumber and various values of the parameter $a$ (blue: $a=0.5$, brown: $a=0.9$, orange: $a=0.99$, red: $a=0.999$). As $a$ increases, the curve interpolates continuously between the parabolic Fick geometry and the circular Cattaneo geometry. The non-propagating modes, characterized by $i\omega\in\mathbb{R}$, are obtained by setting $\lambda_1=r-is$ and $\lambda_2=r+is$ with $r>0$ and exploring the corresponding parametric curve $(k(r),\omega(r))$ over the interval $1/2<r\le (2\sqrt{1-a})^{-1}$. For all $a<1$, $\chi$ spans the entire imaginary axis, and the curves extend to arbitrarily large $|k|$. In the limit $a\to 1$, the branch approaches a circle of radius $1$, together with a vertical half-line emerging from $(k\tau,i\omega\tau)=(0,1)$. This additional line is absent in the Cattaneo theory ($a\equiv 1$) and reflects an exchange-of-limits issue. If one fixes $r\in[1/2+\varepsilon,(2\sqrt{1-a})^{-1}]$ with $\varepsilon>0$ and then sends $a\to1$, only the Cattaneo circle survives. If instead $a$ is fixed and $r\to1/2$, then $s$ diverges and the wavefunction $\psi(p)$ becomes highly oscillatory (see right panel for an explicit example). In this ultraviolet regime, the diffusive Fokker-Planck term \ref{['FokkerPLanck']} dominates, even when the momentum diffusivity $\nu$ is small, causing the mode to decay on a timescale much shorter than $\tau$. For the same reason, the continuous spectrum is given by \ref{['continuousspectrumaless1']} for all $a<1$, while it collapses to $\pm ik+1/\tau$ at $a=1$: arbitrarily oscillatory states are always damped by the Fokker-Planck term at finite $1-a$. Right panel: Real part of the effective wavefunction $\psi(p)$ corresponding to $a=0.9$ and $r=1/2+0.0001$, illustrating the highly oscillatory ultraviolet behavior near the endpoint $r=1/2$.
  • Figure 4: Real (blue) and imaginary (red) parts of the dispersion relations $i\omega(k)$ for real $k$, including both the non-propagating branch (cf. figure \ref{['fig:NonPropagating']}) and the propagating branches, shown for representative values of $a$. A pair of propagating modes bifurcates from the continuous spectrum, where the latter occupies the region $\mathfrak{Re}\,(i\omega)\ge 1/\tau$ (yellow shading) and $\mathfrak{Im}\,(i\omega)=\pm k$ (black dashed), at a finite value of $k$. For $a<a_{\text{critical}}\approx 0.87$, this pair persists up to $k\to\infty$. For $a\ge a_{\text{critical}}$, the propagating modes are absorbed by the non-propagating branch at the forward tilt point and subsequently reemerge at the backward tilt point (note that $a_{\text{critical}}$ is the value of $a$ at which the non-propagating dispersion relation ceases to be single-valued). In the Cattaneo limit, only the branch emanating from the backward tilt point remains.