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An Eulerian hyperbolic model for heat transfer derived via Hamilton's principle: analytical and numerical study

Firas Dhaouadi, Sergey Gavrilyuk

TL;DR

This paper develops a first-order Eulerian hyperbolic model for heat transfer in compressible flows derived from Hamilton's principle, with entropy evolution emerging as an Euler–Lagrange equation. It proves hyperbolicity via total-energy convexity and presents a Friedrichs symmetric form, revealing two wave families—acoustic and thermal—with the thermal fields capable of expansion shocks and compression fans. A relaxation mechanism links the model to Fourier's law asymptotically through $\tau = K c_V(\gamma-1) \rho^2 /( \varkappa^2 p)$, and a detailed Rankine–Hugoniot analysis shows nonexistence of contact discontinuities for $\varkappa\neq0$ and distinct Hugoniot branches. Numerical IMEX schemes corroborate the theoretical findings, showing agreement with Euler–Fourier in the long-wavelength limit and exposing nonclassical shock phenomena such as expansion shocks and shock splitting. The work provides a thermodynamically consistent, hyperbolic alternative to Fourier-based heat conduction with potential advantages for multidimensional curl-free discretizations.

Abstract

In this paper, we present a new model for heat transfer in compressible fluid flows. The model is derived from Hamilton's principle of stationary action in Eulerian coordinates, in a setting where the entropy conservation is recovered as an Euler--Lagrange equation. The governing system is shown to be hyperbolic. It is asymptotically consistent with the Euler equations for compressible heat conducting fluids, provided the addition of suitable relaxation terms. A study of the Rankine--Hugoniot conditions and the Clausius--Duhem inequality reveals that contact discontinuities cannot exist while expansion waves and compression fans are possible solutions to the governing equations. Evidence of these properties is provided on a set of numerical test cases.

An Eulerian hyperbolic model for heat transfer derived via Hamilton's principle: analytical and numerical study

TL;DR

This paper develops a first-order Eulerian hyperbolic model for heat transfer in compressible flows derived from Hamilton's principle, with entropy evolution emerging as an Euler–Lagrange equation. It proves hyperbolicity via total-energy convexity and presents a Friedrichs symmetric form, revealing two wave families—acoustic and thermal—with the thermal fields capable of expansion shocks and compression fans. A relaxation mechanism links the model to Fourier's law asymptotically through , and a detailed Rankine–Hugoniot analysis shows nonexistence of contact discontinuities for and distinct Hugoniot branches. Numerical IMEX schemes corroborate the theoretical findings, showing agreement with Euler–Fourier in the long-wavelength limit and exposing nonclassical shock phenomena such as expansion shocks and shock splitting. The work provides a thermodynamically consistent, hyperbolic alternative to Fourier-based heat conduction with potential advantages for multidimensional curl-free discretizations.

Abstract

In this paper, we present a new model for heat transfer in compressible fluid flows. The model is derived from Hamilton's principle of stationary action in Eulerian coordinates, in a setting where the entropy conservation is recovered as an Euler--Lagrange equation. The governing system is shown to be hyperbolic. It is asymptotically consistent with the Euler equations for compressible heat conducting fluids, provided the addition of suitable relaxation terms. A study of the Rankine--Hugoniot conditions and the Clausius--Duhem inequality reveals that contact discontinuities cannot exist while expansion waves and compression fans are possible solutions to the governing equations. Evidence of these properties is provided on a set of numerical test cases.
Paper Structure (29 sections, 1 theorem, 159 equations, 9 figures)

This paper contains 29 sections, 1 theorem, 159 equations, 9 figures.

Key Result

Theorem 1

Let $f(q_1,\cdots,q_n)$ be a convex function on a subset $\Omega\subset\mathbb{R_+}\times\mathbb{R}^{n-1}$. Then is also convex.

Figures (9)

  • Figure 1: log-linear plot of the real part of the phase velocities (Left) and log-log plot of the attenuation factors (Right) for both system of equations \ref{['eq:dissipative_hyp_heat_eq']} (Dashed lines) and system \ref{['eq:Euler-Fourier']} (Solid lines) as a function of the wavenumber $k$. Polytropic gas equation of state is used here with $\gamma=1.4$, $c_V=3/2$, $\rho_0=1$, $\eta_0=1$, $\varkappa=1$ and $K=0.1$.
  • Figure 2: Plot of the functions $\tilde{p}^+$ and $\tilde{p}^-$ as a function of $\tilde{v}$.
  • Figure 3: Plot of $\tilde{\Psi}^+$ (Left) and $\tilde{\Psi}^-$ (Right) as a function of $\tilde{v}$ for different values of $\tilde{\varkappa}$ that are $\varkappa_c= 1.0399...$, $\tilde{\varkappa}=0.8$ and $\tilde{\varkappa}=1.3$. $\gamma=2$. The dashed lines correspond to non-physical solutions that do not satisfy $\tilde{\Psi}\geq0$.
  • Figure 4: Schematic representation of the wave pattern in the $x-t$ plane, for the shock splitting solution. The shock propagates to the right, followed by a right facing compression fan. The Clausius-Duhem inequality is satisfied on the shock. The slope of the rightmost characteristic of the compression fan is equal to the velocity $\mathcal{D}_\star$ of a shock relating the right state to the $\star$ state.
  • Figure 5: Numerical Profiles at of the density (Left), velocity (middle) and pressure (Right) obtained after solving numerically the Euler equations supplemented with heat conduction for the initial condition \ref{['eq:IC_choctube']}. The solid line curves correspond to the numerical result at $t=0.2$ for different values of the heat conductivity $K=0$ (Blue), $K=10^{-3}$ (Red) and $K=10^{-2}$ (Green). The initial condition is plotted with black dashes lines. Here, $\gamma=1.4$ and $c_V =3/2$.
  • ...and 4 more figures

Theorems & Definitions (5)

  • Theorem 1
  • Remark
  • Remark
  • Definition
  • Remark