- About this Journal ·
- Abstracting and Indexing ·
- Advance Access ·
- Aims and Scope ·
- Annual Issues ·
- Article Processing Charges ·
- Articles in Press ·
- Author Guidelines ·
- Bibliographic Information ·
- Citations to this Journal ·
- Contact Information ·
- Editorial Board ·
- Editorial Workflow ·
- Free eTOC Alerts ·
- Publication Ethics ·
- Reviewers Acknowledgment ·
- Submit a Manuscript ·
- Subscription Information ·
- Table of Contents
International Journal of Differential Equations
Volume 2013 (2013), Article ID 595819, 13 pages
Existence and Stability for the 3D Linearized Constant-Coefficient Incompressible Current-Vortex Sheets
Dipartimento di Matematica, Facoltà di Ingegneria, Università degli Studi di Brescia, Via Valotti 9, 25133 Brescia, Italy
Received 29 May 2012; Revised 21 December 2012; Accepted 27 December 2012
Academic Editor: Helge Holden
Copyright © 2013 Davide Catania. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
We consider the free boundary problem for current-vortex sheets in ideal incompressible magnetohydrodynamics. The problem of current-vortex sheets arises naturally, for instance, in geophysics and astrophysics. We prove the existence of a unique solution to the constant-coefficient linearized problem and an a priori estimate with no loss of derivatives. This is a preliminary result to the study of linearized variable-coefficient current-vortex sheets, a first step to prove the existence of solutions to the nonlinear problem.
1.1. The Eulerian Description
Let us consider the equations of magnetohydrodynamics (MHD) governing the motion of a perfectly conducting inviscid incompressible plasma in three-space dimension. In the case of a homogeneous plasma (i.e., the density is a positive constant), the equations in a dimensionless form read where, using for transposition, denotes the plasma velocity, is the magnetic field (in Alfvén velocity units), is the total pressure, and is the pressure. For smooth solutions, system (1) can be written in an equivalent form as
We are interested in weak solutions, in a suitable sense, to (1) that are smooth on either side of a smooth hypersurface in , where , , and that satisfy suitable jump conditions at each point of the front . For notational simplicity, we assume that the density is the same constant on either side of , so that we can take, with no loss of generality, . In physical applications, the two densities can be very different, but such a difference intervenes only at the boundary, and it is taken into account by the jump condition for the total pressure (see below), so it does not alter the mathematical techniques applied in this paper.
Let us set , where ; given any function , we set in and denote by the jump across .
We look for current-vortex sheets solutions, that is, smooth solutions of (2) in such that is a tangential discontinuity, namely, the plasma does not flow through the discontinuity front, and the magnetic field is tangent to , see, for example, Landau and Lifshitz ; thus, the boundary conditions take the form where denotes the outward unit normal on and denotes the velocity of propagation of the interface front . With the given parametrization of , an equivalent formulation of these jump conditions is with . Notice that the function describing the discontinuity front is part of the unknowns of the problem, that is, this is a free boundary problem.
Current-vortex sheets have various interesting applications in geophysics and astrophysics. For instance, an accepted model in the literature for the interface region between the unperturbed flows of the interstellar plasma and the supersonic solar wind plasma is given by a current-vortex sheet separating the interstellar plasma compressed at the bow shock from the solar wind plasma compressed at the termination shock, see Ruderman and Fahr  and references therein. This current-vortex sheet is called the heliopause and in some sense can be considered as the outer boundary of the solar system. Similarly, the boundary separating the shocked solar wind plasma from the plasma of the magnetosphere of planets equipped with an intrinsic magnetic field (such as the Earth, Jupiter …) is a current-vortex sheet called magnetopause.
In order to prove the local existence of solutions to the current-vortex sheets (nonlinear) problem (2), (4), and (5), it is useful to prove existence for the linearized problem and the strong stability, that is, an a priori estimate for the solutions with no loss of derivatives (see later on). We will perform a further simplification by assuming a linearization around a constant-coefficient basic state. This must be seen as a preliminary step before considering a linearization around a general variable-coefficient basic state, in order to prove existence, uniqueness and stability for the solution to problem (2), (4), and (5) without resorting to a Nash-Moser iteration. Such result would be a rigorous confirmation of the stabilizing effect of the magnetic field on Kelvin-Helmholtz instabilities, which is well known in astrophysics.
In the last years, there has been a renewed interest for the analysis of free interface problems in fluid dynamics, especially for the Euler equations in the vacuum and the water waves problem, see Coutand and Shkoller [3, 4] and the references thereinto. This fact has produced different methodologies for obtaining a priori estimates and the proof of the existence of solutions. If the interface moves with the velocity of fluid particles, a natural approach consists in the introduction of the Lagrangian coordinates that reduces the original problem to a new one on a fixed domain. This approach has been recently employed with success in a series of papers by Coutand and Shkoller on the incompressible and compressible Euler equations in the vacuum, see [3, 4]. However, this method seems hardly applicable to problem (2), (4), and (5).
For incompressible current-vortex sheets, the precise description of the region of weak stability is known, meaning that for states outside this region the problem is ill posed. In this region, Morando et al. , for the constant-coefficient linearized equations, have shown an a priori estimate for solutions with loss of regularity with respect to the data. In a subset of the region of weak stability, that is, under a more restrictive stability condition (i.e., (6), introduced in the following), Trakhinin  has shown a similar result with no loss of regularity for the solutions to the linearized problem with respect to the source terms, but with loss of derivatives with respect to the coefficients of the problem. Moreover, in a recent paper, Coulombel et al.  have shown that the same more restrictive stability condition is sufficient for an a priori estimate of solutions to the nonlinear problem with no loss of regularity (here, space periodicity is assumed). However, in all the previous cases, existence of the solution is missing. Let us note that we are looking for the existence and an a priori estimate with no loss of derivatives for the linearized incompressible current-vortex sheet problem. Reference  already provides an estimate with no loss of regularity in the constant-coefficient case, but such a loss manifests for variable coefficients, and existence is not proved. The main novelty of our paper is the existence result; however, we hope that it is possible to extend the techniques here used in order to obtain an a priori estimate with no loss of regularity even for the variable-coefficient linearized problem. We point out that the estimate in  is optimal, with no loss of derivatives, but refers to the nonlinear problem and does not help in proving existence for the linearized system.
In , Secchi and Trakhinin have established existence and stability for the linearized compressible plasma-vacuum (free boundary) problem. In that case, the interface separates a plasma region governed by the usual MHD equations from a vacuum region with pre-Maxwell dynamics for the magnetic field, as in the case of magnetic confinement in nuclear fusion processes. This work has been employed by Morando et al.  to obtain the analogous result for the incompressible problem. However, the techniques used in these papers cannot be easily adapted to current-vortex sheets, since they rely on a secondary symmetrization in the vacuum part that cancels problematic boundary terms and cannot be reproduced in plasma part.
In the present paper, we follow an approach different from the one of Coutand and Shkoller. To reduce our free boundary problem to the fixed domain, we consider a change of variables inspired from Lannes  and performed in Secchi and Trakhinin . The control of the function describing the free interface follows from a stability condition introduced by Trakhinin in , that is, the strong stability condition which implies in particular that is not the zero vector.
We use a compressible approximation and perform some changes of variables in order to obtain a symmetric hyperbolic problem with conditions in a more suitable form, so that we can apply the results by Lax and Phillips  and Secchi [13, 14] for maximally nonnegative linear symmetric hyperbolic systems with characteristic boundary of constant multiplicity. Another fundamental tool is the so-called secondary symmetrization, which is a linear combination of the equations of the hyperbolic system that allows a simplification of the border term necessary to obtain the a priori estimate (see Section 4). By exploiting such techniques, we obtain the existence of a unique solution to the incompressible current-vortex sheets free boundary problem linearized about a suitable constant-coefficient state and show that the solution satisfies a priori estimates with no loss of derivatives with respect to data. As mentioned above, this is a preliminary step in order to prove existence and stability for the current-vortex sheet nonlinear problem.
1.2. The Reference Domain
To avoid using local coordinate charts necessary for arbitrary geometries, and for simplicity, we will assume that the space domain occupied by the fluid is given by . We also set The moving discontinuity front is given by
1.3. An Equivalent Formulation in the Fixed Domain Ω
Lemma 1. Let be an integer. Then, for all and for all satisfying without loss of generality , there exists a function such that the function defines an -diffeomorphism of for all . Moreover, there holds
We set and we compute Now we may reduce the free boundary problem (2), (4), and (5) to a problem in the fixed domains by the change of variables (10). Let us set Then, the system (2), (4), and (5) can be reformulated on the fixed reference domains as In (15), we have set Notice that We warn the reader that the notation is used to denote the transpose of and has nothing to do with the time interval on which the smooth solution is sought; we hope that this does not create any confusion. Vectors are written in columns.
If we set , , and , problem (15) can be written in short form as where is the zero vector.
2. The Linearized Problem
2.1. Basic State
Let be such that and are constant vectors, , and We can then take , so that . Similarly, we determine all the “hat” functions as for the corresponding functions obtained for . Let us note, in particular, that , , , and . We assume that In particular, . Under these hypotheses, we have that the basic state is a solution of problem (15).
Moreover, we assume that the basic state satisfies This is the analogue of condition (6) and implies
2.2. Linearized Problem
The linearized equations for (15) are where , , , and are the unknowns. Here, we consider the source terms in order to make the system inhomogeneous.
If we omit and write explicitly the linearized equations, we get, in , The linearized boundary conditions are obtained in a similar way (let us recall that we are omitting ): on , where, as usual, if is a vector, we set , and moreover,.
2.3. Reduction to Homogeneous Boundary Conditions
Let , denote vector-valued functions which solve, respectively, the elliptic problems and set , = , and , where on and on (here, letters and represent different variables from the ones introduced in the original formulation (1)).
The equations in (25) can be recast in terms of : with new source terms , , with boundary conditions and initial data
3. Notations and Results
3.1. Function Spaces
We denote by the usual Sobolev space and by its norm, while is simply the norm of . We introduce a smooth odd function defined in such that for and for and set , and . For a multi-index , , we set , where is an integer number (see [14–17]).
If , defined on with values in , is such that for , we set where is the space of functions which are in together with the time derivatives up to order on , with values in . The spaces and are equipped with norms, respectively,
We define the same function spaces and norms for a general space domain in the same way; we write, for instance, to specify the domain that we are considering.
3.2. Main Result
Now, we are able to state the main theorem. We set and consider problem in , with boundary conditions on , and initial data where
Theorem 2. Assume that the constant basic state satisfies (20), (21), and (22), and moreover, assume that , on , and . Assume that , in , and on , where denotes the third component of vector . Finally, assume as well the compatibility conditions on :
Then there exists a unique solution to (34), (35), and (36) ( unique up to additive constants) such that , ( is the homogeneous Sobolev space), and ; in addition, for each , the following a priori estimate is satisfied, where is a positive constant.
Moreover, one has .
Remark 3. In order to consider the nonlinear problem, it might be useful to have higher regularity estimates, with no loss of derivatives, provided that data are sufficiently regular. The regularity can be obtained from the equations for and , which allow to improve the regularity for the normal derivatives. Taking further derivatives and proceeding as in the proof of Proposition 13, one can expect to get higher regularity. The details are postponed to a future paper.
As for the regularity assumption on , , see Section 4.5.
Note that in and on follow from (34), (35), and (36) and the assumptions of Theorem 2 and, in particular, from the validity of the restrictions of such equations at time . More precisely, we have the following result.
Proposition 4. Under the same assumptions of Theorem 2, the solution satisfies
Proof. If we take the divergence in the second equation in (34) and use in , we get
and hence in , since at time , we have on by assumption.
On the other hand, let us take just the third component of the second equation in where we have used and . If we substitute from the second equation into (35) and observe that , we deduce that in . Using the third equation in (38), which holds for , we conclude that in .
4.1. Hyperbolic Regularization
Here, the solution depends on but, in this moment, we will not use the more precise notation to denote the solution to the previous system (with suitable initial data). Let us note that, at least formally, if we project the system (45), (46), and (47) on the subspace of divergence-free functions, it converges, as , to system (34) projected on the same subspace; it is sufficient to multiply (45) by and take the limit. We will make this statement more precise in Section 4.7.
One can easily check that, as , this system converges to (34), at least formally. Moreover, the system is hyperbolic, since (omitting ) for each .
4.2. Secondary Symmetrization
More precisely, let us consider the system where will be chosen conveniently later on and (54) denotes the equation obtained by substituting (45) into (47), that is, We get where . This system is symmetric; indeed, the coefficient of is the singular term is given by and the remaining derivatives are included in where and denote, respectively, the identity and null matrix. All these matrices are symmetric, and the system can be recast as where each matrix is bounded in provided is bounded and , where if or , otherwise. Notice that .
Remark 5. The secondary symmetrization is inspired by [11, 19], which we refer to for further details. The main idea is to consider the following variant of (49), which takes into account the divergence constraint for the magnetic field where the matrix and the vector depend on the basic state. is then chosen in order to obtain , whose form is useful to get the energy a priori estimate, while is chosen to maintain the symmetry of the system. As pointed out in  (Remark 5), such a choice is related to the conservation of cross-helicity: . On the other hand, one main feature of the secondary symmetrization is that can be chosen widely arbitrarily, so that in the following we will be able to find a suitable which simplifies singular boundary terms in the a priori estimate.
The following lemma guarantees that, under our assumptions and a suitable choice of , the matrices are positive definite and (59) is symmetric hyperbolic.
Lemma 6. If then the symmetric matrices are positive definite.
Proof. Omitting “”, we have If that is to say, if then the matrix is positive definite.
Lemma 7. There exists such that, for each , the choice satisfies (61) and hence makes the matrices positive definite.
Let us remark that is a constant term independent of ; moreover, since , this choice of is the same as which will be useful in the following steps. Moreover, this choice is equivalent to In addition, we set which is always different from zero thanks to (23).
4.3. Boundary Conditions in Algebraic Form
The boundary conditions can be recast so that the space derivatives of the front function do not appear explicitly.
Lemma 8. The boundary conditions (35) imply, on , the boundary conditions and the front equation with
Proof. Condition (41) can be recast as
by hypothesis, we can obtain
By substituting in the second equation of (35), we get
Using the definition of and , we deduce the conditions The last condition can be recast as where
Recalling (68), we have The previous condition becomes and the lemma is proved.
4.4. Equivalence of Systems
Obviously, if is a solution to system (49) with boundary conditions (35), then it also satisfies system (59) with conditions (71) (we are assuming the same initial conditions); the converse holds true as well.
Proposition 9. If is a solution to system (59) with boundary conditions (71), then one can find a unique , so that is a solution to system (49) with boundary conditions (35) and the same initial conditions.
Proof. First, we prove that (49) is satisfied. Since (59) holds, then we have (51), (52), and (53). If we substitute (54) (47) + (45) into (52), we get (46) (47), and substituting this relation in (53), we deduce
thanks to (61), then we get (47) and consequently (46) (47) .
From (51), in order to prove (45), it is now sufficient to establish that , since we already know that (46) . With this aim, we substitute (51) into (47) and get Taking the divergence of the above equation, exploiting the assumption and the fact that , , are piecewise constant, and simplifying, we deduce that Since in by assumption on the initial data, we conclude that in , so that (45) from (51). Then (45), (46), and (47) are satisfied, which means that (49) holds.
Now, we have to prove (35). Condition on obviously holds, since we have the same condition in (71). We need to prove that there exists so that on . Given and , let us define as the solutions of Thus, for the completion of the proof of (35), it is sufficient to show that in . Proceeding as in the proof of Proposition 4, we first deduce in . Let us compute Since by (71), we obtain Thanks to (69), we have , and hence, Thus, we can take in , and (35) holds.
4.5. Existence of the Approximate Solution
Now, consider the system (59) with the boundary conditions (71) and the initial condition . This system can be written as where we have set and similarly for the other quantities; moreover, we set and so on. Notice that corresponds to the boundary conditions (71).
Let us note that, since , the condition on given by is automatically satisfied. Moreover, if we denote by the homonymous quantities in (91) evaluated at time and calculated in terms of the initial data, from the equations and the hypotheses on , , , we get the condition . Let us note that the hypothesis in , rather than simply in , is needed exactly here. We have the following result.
Proposition 10. There exists so that, for each , there exists a unique solution to problem (91); moreover, one has for each and a suitable .
Proof. The boundary matrix of system (91) is given by
where ). The matrix is singular with constant rank (indeed, is the null matrix) and, moreover, is maximally nonnegative for , that is to say,
for each (nonnegativity) and such a property does not hold in any other vector space properly containing (maximality). Indeed, we have
thanks to and on . Moreover, let us observe that both and have exactly one negative eigenvalue, so we have the same number of conditions defining and negative eigenvalues, that is, 2; this implies maximality.
Thus, we can apply the results in Lax and Phillips  (existence in , see as well Friedrichs  for the noncharacteristic case) and Secchi [13, 14] (regularity in ), and deduce the existence of a unique global solution to problem (91) such that (92) holds for each , provided is sufficiently small.
Remark 11. Let us note that, in the previous result, the smallness of is necessary in order to have positive definite.
We need to have a number of boundary conditions in (71), that is, defining , equal to the number of negative eigenvalues of , that is to say, , in order to have maximality.
Proof. Problem (91) with on is a different way to say that (59), (71), and (36) with are satisfied. Using Propositions 9 and 10, we get the result for . Let us note that, since and the normal component at the boundary is noncharacteristic, then the trace is in , as shown in Secchi [13, 14] and Shizuta . In particular, can be estimated using the other terms appearing in (45), so that we have
The same holds true for as well, for the same reason ( is obtained from (46)), and for , since is bounded (this follows from (54) proceeding similarly as in Proposition 4; note that, taking the divergence, the terms containing cancel together). Thus, from the transport equation (87), we find and This concludes the proof.
4.6. A Priori Energy Estimate Uniform in
Since estimate (96) depends on , we cannot use it when passing to the limit as . We can deduce the following a priori estimate for , which is an -estimate uniform in , useful to pass to the limit as . We recall that the choice makes positive definite, and hence, if we fix sufficiently small, there exists a suitable real number , so that for each .
Proposition 13. There exists , such that, for each , the a priori estimate holds for each and for a suitable independent of , where is the solution to problem (49), (35), and (36) and satisfies (87) with initial condition .
Proof. Let us take the scalar product of (59), which is equivalent to (49), with and integrate over (recall that ); integrating by parts the terms with spatial derivatives of , exploiting the fact that the coefficient matrices are constant, and recalling that the boundary matrix is given by , since , we get
where sum over is assumed. Let us note that, since the basic state is piecewise constant, then and are piecewise constant as well; thus,
in . Moreover,
thanks to the boundary conditions and , that hold in .
We deduce the equality For the left-hand side, integrating by parts in time and exploiting the symmetry of , we have By applying the Cauchy-Schwarz inequality in the right-hand side, we obtain and hence, by exploiting , Through a standard application of Grönwall’s lemma, we deduce that
In the same way, we can apply a tangential derivative to (59) and (35), take the scalar product with , and proceed as before to obtain
It remains to find an estimate for , where . If we apply to (59) and recall that , we get Testing by , summing up terms with plus and minus sign, and simplifying as before, we deduce that