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Quasi-neutral limit of the Euler-Poisson and Euler-Monge-Ampère systems

Grégoire Loeper

TL;DR

The paper studies the quasi-neutral limit $\epsilon \to 0$ for two collisionless-fluid models, the pressureless Euler–Poisson system $EP_{\epsilon}$ and its fully nonlinear counterpart the Euler–Monge–Ampère system $EMA_{\epsilon}$, showing convergence to the incompressible Euler equations on the torus $\mathbb{T}^d$ ($d=2,3$) at large scales. For $EP_{\epsilon}$, using energy estimates and a reformulation with new unknowns $\beta_1$, $\rho_1$, and $\omega_1$ defined by $\nabla\cdot v = \epsilon \beta_1$, $\rho=1+\epsilon^2 \rho_1 = 1+\epsilon \Delta \phi$, $\nabla\times v = \omega = \bar{\omega} + \epsilon \omega_1$, they prove uniform bounds on $\epsilon^{-1}(v^{\epsilon}-\bar{v})$ and $\epsilon^{-2}(\rho^{\epsilon}-1)$ and convergence of the scaled perturbations to the incompressible limit; non-prepared data also converge. For $EMA_{\epsilon}$, they frame it as a penalized approximate geodesic problem on the group of volume-preserving maps, analyze the linearized Monge–Ampère operator and establish that small perturbations in density lead to controlled Hessians and quadratic remainder terms, and obtain energy estimates via a div–curl decomposition to prove convergence toward the Euler flow with non-prepared data also handled. The study highlights how fast oscillations from the electric coupling and the Monge–Ampère constraint interact with slow, incompressible modes to yield the quasi-neutral limit, providing rigorous justification for using incompressible Euler dynamics as large-scale limits of these models.

Abstract

This paper studies the pressureless Euler-Poisson system and its fully non-linear counterpart, the Euler-Monge-Amp\`ere system, where the fully non-linear Monge-Amp\`ere equation substitutes for the linear Poisson equation. While the first is a model of plasma physics, the second is derived as a geometric approximation to the Euler incompressible equations. Using energy estimates, convergence of both systems to the Euler incompressible equations is proved.

Quasi-neutral limit of the Euler-Poisson and Euler-Monge-Ampère systems

TL;DR

The paper studies the quasi-neutral limit for two collisionless-fluid models, the pressureless Euler–Poisson system and its fully nonlinear counterpart the Euler–Monge–Ampère system , showing convergence to the incompressible Euler equations on the torus () at large scales. For , using energy estimates and a reformulation with new unknowns , , and defined by , , , they prove uniform bounds on and and convergence of the scaled perturbations to the incompressible limit; non-prepared data also converge. For , they frame it as a penalized approximate geodesic problem on the group of volume-preserving maps, analyze the linearized Monge–Ampère operator and establish that small perturbations in density lead to controlled Hessians and quadratic remainder terms, and obtain energy estimates via a div–curl decomposition to prove convergence toward the Euler flow with non-prepared data also handled. The study highlights how fast oscillations from the electric coupling and the Monge–Ampère constraint interact with slow, incompressible modes to yield the quasi-neutral limit, providing rigorous justification for using incompressible Euler dynamics as large-scale limits of these models.

Abstract

This paper studies the pressureless Euler-Poisson system and its fully non-linear counterpart, the Euler-Monge-Amp\`ere system, where the fully non-linear Monge-Amp\`ere equation substitutes for the linear Poisson equation. While the first is a model of plasma physics, the second is derived as a geometric approximation to the Euler incompressible equations. Using energy estimates, convergence of both systems to the Euler incompressible equations is proved.

Paper Structure

This paper contains 20 sections, 17 theorems, 128 equations.

Key Result

Theorem 1.1

Let f be a weak solution of (3vma, 3mav, 3vmainit) (resp. of (3vma, 3pv, 3vmainit)) with finite energy, let (t,x)\rightarrow\bar{v}(t,x) be a smooth solution of the incompressible Euler equation (3euler) for t\in[0,T], and p(t,x) the corresponding pressure, let where E_{\epsilon}(t)=\epsilon^{-2} \int \rho |\nabla\phi|^2/2 (resp. E_{\epsilon}(t)=\epsilon^{-2} \int |\nabla\phi|^2/2 in the Poisson

Theorems & Definitions (18)

  • Theorem 1.1
  • Theorem 2.1
  • Lemma 2.2
  • Lemma 2.3
  • Corollary 2.4
  • Lemma 2.5
  • Proposition 2.6
  • Theorem 2.7
  • Theorem 3.1
  • Definition 3.2
  • ...and 8 more