Stability and existence of relativistic plasma--vacuum interfaces
Paolo Secchi, Yuri Trakhinin, Tao Wang

TL;DR
This paper analyzes the stability and local existence of solutions for relativistic plasma-vacuum interfaces governed by magnetohydrodynamics and Maxwell's equations, establishing conditions for linear stability and nonlinear well-posedness.
Contribution
It identifies a stability condition for relativistic plasma-vacuum interfaces and proves local-in-time existence and uniqueness of solutions in two dimensions.
Findings
Established a quantitative stability condition for the interface.
Proved linear stability in three dimensions under the stability condition.
Proved local-in-time existence and uniqueness in two dimensions.
Abstract
We consider the free boundary problem for relativistic plasma--vacuum interfaces in two and three spatial dimensions. The plasma flow is governed by the equations of ideal relativistic magnetohydrodynamics, while the vacuum magnetic and electric fields satisfy Maxwell's equations. The plasma and vacuum magnetic fields are tangential to the interface, which moves with the plasma flow. This yields a nonlinear, multidimensional hyperbolic problem with a free boundary that is characteristic of variable multiplicity. We identify a quantitative stability condition and establish the linear stability of three-dimensional relativistic plasma--vacuum interfaces in the sense that the variable-coefficient linearized problem satisfies energy estimates in anisotropic Sobolev spaces. In estimating tangential derivatives, we exploit an intrinsic cancellation effect to convert the boundary term into an…
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