We consider the free boundary problem for the plasma-vacuum interface in ideal compressible magnetohydrodynamics (MHD). In the plasma region, the flow is governed by the usual compressible MHD equations, while in the vacuum region we consider the Maxwell system for the electric and the magnetic fields, in order to investigate the well-posedness of the problem, in particular in relation with the electric field in vacuum. At the free interface, driven by the plasma velocity, the total pressure is continuous and the magnetic field on both sides is tangent to the boundary. Under suitable stability conditions satisfied at each point of the plasma- vacuum interface, we derive a basic a priori estimate for solutions to the linearized problem in the Sobolev space H^1_tan with conormal regularity. The proof follows by a suitable secondary symmetrization of the Maxwell equations in vacuum and the energy method. An interesting novelty is represented by the fact that the interface is characteristic with variable multiplicity, so that the problem requires a different number of boundary conditions, depending on the direction of the front velocity (plasma expansion into vacuum or viceversa). To overcome this difficulty, we recast the vacuum equations in terms of a new variable which makes the interface characteristic of constant multiplicity. In particular, we don’t assume that plasma expands into vacuum.

Stability of the linearized MHD-Maxwell free interface problem

CATANIA, Davide;D'ABBICCO, Marcello;SECCHI, Paolo
2014-01-01

Abstract

We consider the free boundary problem for the plasma-vacuum interface in ideal compressible magnetohydrodynamics (MHD). In the plasma region, the flow is governed by the usual compressible MHD equations, while in the vacuum region we consider the Maxwell system for the electric and the magnetic fields, in order to investigate the well-posedness of the problem, in particular in relation with the electric field in vacuum. At the free interface, driven by the plasma velocity, the total pressure is continuous and the magnetic field on both sides is tangent to the boundary. Under suitable stability conditions satisfied at each point of the plasma- vacuum interface, we derive a basic a priori estimate for solutions to the linearized problem in the Sobolev space H^1_tan with conormal regularity. The proof follows by a suitable secondary symmetrization of the Maxwell equations in vacuum and the energy method. An interesting novelty is represented by the fact that the interface is characteristic with variable multiplicity, so that the problem requires a different number of boundary conditions, depending on the direction of the front velocity (plasma expansion into vacuum or viceversa). To overcome this difficulty, we recast the vacuum equations in terms of a new variable which makes the interface characteristic of constant multiplicity. In particular, we don’t assume that plasma expands into vacuum.
2014
Ateneo di appartenenza
PE1_12 Mathematical physics
PE1_11 Theoretical aspects of partial differential equations
PE1_8 Analysis
PE1_20 Application of mathematics in sciences
Esperti anonimi
Inglese
Internazionale
STAMPA
13
6
2407
2443
37
Ideal compressible magneto-hydrodynamics; Maxwell equations; plasma-vacuum interface; characteristic free boundary; nonuniformly characteristic boundary
MIUR (compresi PRIN FIRB,FISR)
no
3
info:eu-repo/semantics/article
262
Catania, Davide; D'Abbicco, Marcello; Secchi, Paolo
1 Contributo su Rivista::1.1 Articolo in rivista
none
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11379/407906
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