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Classical limit of the relativistic Vlasov-Maxwell-Landau system

Chuqi Cao, Ling-Bing He, Yuanjie Lei, Qinghua Xiao

TL;DR

The paper rigorously justifies the non-relativistic (classical) limit of the relativistic Vlasov-Maxwell-Landau system to the Vlasov-Poisson-Landau system in a periodic box by establishing uniform-in-$c$ coercivity for the relativistic collision operator, introducing a weighted energy framework to counteract weak field dissipation, and proving global well-posedness independent of $c$. It formalizes a $c^{-1}$ expansion up to order three, showing that the leading-order dynamics recover the VPL system while higher-order terms satisfy controlled, decaying equations. The main results include global existence and uniform energy bounds for the RVML system, a precise $O(1/c)$ convergence rate to VPL, and the convergence of the self-consistent magnetic field to a fixed background, clarifying the Maxwell-to-Poisson reduction in the presence of collisions. This work advances the mathematical understanding of kinetic limits with self-consistent fields and highlights how collisional damping interacts with long-range electromagnetic effects in singular limits.

Abstract

The physical essence of the non-relativistic limit, from the relativistic Vlasov-Maxwell-Landau system to the Vlasov-Poisson-Landau system, lies in the transition from finite-speed electromagnetic waves to instantaneous Coulomb interactions, and from relativistic to Newtonian particle dynamics. We rigorously justify this limit (mathematically corresponding to the light speed $c \to \infty$) in a periodic box via three key technical advances: establishing a uniform-in-$c$ coercivity estimate for the relativistic Landau collision operator, constructing a novel weighted energy functional to overcome the weakening dissipation of the electromagnetic field at large $c$, and proving a corresponding global well-posedness result.

Classical limit of the relativistic Vlasov-Maxwell-Landau system

TL;DR

The paper rigorously justifies the non-relativistic (classical) limit of the relativistic Vlasov-Maxwell-Landau system to the Vlasov-Poisson-Landau system in a periodic box by establishing uniform-in- coercivity for the relativistic collision operator, introducing a weighted energy framework to counteract weak field dissipation, and proving global well-posedness independent of . It formalizes a expansion up to order three, showing that the leading-order dynamics recover the VPL system while higher-order terms satisfy controlled, decaying equations. The main results include global existence and uniform energy bounds for the RVML system, a precise convergence rate to VPL, and the convergence of the self-consistent magnetic field to a fixed background, clarifying the Maxwell-to-Poisson reduction in the presence of collisions. This work advances the mathematical understanding of kinetic limits with self-consistent fields and highlights how collisional damping interacts with long-range electromagnetic effects in singular limits.

Abstract

The physical essence of the non-relativistic limit, from the relativistic Vlasov-Maxwell-Landau system to the Vlasov-Poisson-Landau system, lies in the transition from finite-speed electromagnetic waves to instantaneous Coulomb interactions, and from relativistic to Newtonian particle dynamics. We rigorously justify this limit (mathematically corresponding to the light speed ) in a periodic box via three key technical advances: establishing a uniform-in- coercivity estimate for the relativistic Landau collision operator, constructing a novel weighted energy functional to overcome the weakening dissipation of the electromagnetic field at large , and proving a corresponding global well-posedness result.

Paper Structure

This paper contains 46 sections, 36 theorems, 369 equations.

Key Result

Proposition 1.1

Assume that $F^{\infty}_{\pm,0}(x,p)=\mu^{\infty}(p)+\sqrt{\mu^{\infty}(p)}f^{\infty}_{\pm,0}(x,p)\geq0$ and $[f^{\infty}_{\pm,0}(x,p),E^{\infty}_0(x)]$ satisfies conservation laws cons-VPL0. There exists a sufficiently small constant $\overline{M} > 0$ such that if $\mathcal{E}^{\infty}_{2,2}(0)\le

Theorems & Definitions (76)

  • Remark 1.1
  • Remark 1.2
  • Proposition 1.1
  • Remark 1.3
  • Theorem 1.1: Global existence of the RVML system
  • Remark 1.4: Smallness and Uniformity
  • Remark 1.5: Decay Properties
  • Remark 1.6: Conservation Laws
  • Remark 1.7: Function Space Differences
  • Remark 1.8: Global Well-posedness Framework
  • ...and 66 more