1. Introduction
We consider a free boundary problem for a viscous compressible magnetohydrodynamics motion in domain , bounded by a free surface The motion interacts with an electromagnetic field located in . Moreover, is bounded by a fixed boundary B. Hence, and .
In
Figure 1, we present the two-dimensional section of the considered problem.
In
, the magnetohydrodynamic motion of viscous compressible barotropic fluid is described by the following system of equations:
where
is the velocity of the fluid,
is the density,
is the magnetic field,
is the electric field,
is the external force field, and
are Cartesian coordinates.
Since the fluid is considered barotropic, we have
and
is the strain tensor of the form
where
and
are positive viscosity coefficients, and
is the Kroneker delta, which is such that
for
and
for
.
Moreover,
is the constant magnetic permeability;
is the constant electric conductivity. For system (
1), the following initial and boundary conditions are prescribed:
where
is the unit vector outward to
and normal to
and
is the stress magnetic field tensor of the form
The boundary condition (4)
1 implies the compatibility condition
where
, and
is a tangent vector to
. In
, we have a motionless dielectric gas under the constant pressure
.
Therefore, we only have an electromagnetic field described by the system of equations
where
is the constant magnetic permeability and
is the constant electric conductivity.
For system (
7), the following initial and boundary conditions are prescribed:
where
are tangent vectors to
B.
Problems (1)–(8) are composed of two problems. For a given
, we have the following problem for
v and
:
Furthermore, for a given
v, we have the following problem for
and
:
where
and
Problem (
10) is not complete because electromagnetic fields in
and
interact through the free surface
. The general transmission conditions are formulated in Lemma 1.1 in [
1]. Recalling them, we have
where
are arbitrary non-vanishing constants,
is the unit normal vector to
, and
are tangent to
.
Eliminating the electric fields from (
10), we obtain for any
the following problem:
where
are tangent vectors to
B, and the transmission condition (
11) takes the form
In this paper, we prove the local existence of solutions to problems (10), (12), and (13). We prove it by the method of successive approximations described in problems (53) and (54).
The existence is proved in the Sobolev–Slobodetskii spaces defined in
Section 2.1. We use the Besov-type spaces to describe more precisely the initial and boundary traces. Moreover, we are able to prove the local existence of solutions with sharp regularity with the lowest possible regularity that is necessary to handle the nonlinearity of the problem. To describe the main result precisely, we need to describe the following quantities:
We define Lagrangian coordinates in
and
as the initial data for the Cauchy problems (see (
49)):
Solving the equation, we get
where
However, to define the Lagrangian coordinate
, we need
in
. Since we do not have it, we construct
in
as a solution to the problem (see (47))
Since
is unknown, we construct it as a solution to the following elliptic problem (see (48)):
Now, we formulate the main result.
Theorem 1. Assume that , , , , , and . Assume that and , where is a smooth function, , . Assume that , and , , , and , where , , and is defined by (47).
Then, for sufficiently small t, there exists a local solution to problems (9), (12), and (13) such that , , and .
Now, we describe the proof of this theorem. Since the free boundary problem is considered, we need to use the Lagrangian coordinates.
In , there is no velocity, so we introduce velocity in as a solution to problem (47).
Hence, we have in and in . Hence, an evolution of the free surface and domains , is described by the relation between Eulerian and Lagrangian coordinates.
The Lagrangian coordinates in
and
are introduced in (
49) and (
50).
Expressing problems (9) and (12) in the Lagrangian coordinates yields problems (
51) and (
52). To show the existence of solutions to problems (
51) and (
52), we construct a method of successive approximations described by problems (53) and (54).
Problem (53) is linear with respect to
and nonlinear in
,
. In
Section 4, we derive the inequality
where
,
, and
is an increasing positive function.
To derive estimate (
18), we have to examine the operator
where
and
are given and
is a solution. To obtain an estimate for the quantity
we need the Hölder continuity of
and appropriate partition of unity, which helps to derive an estimate for (
20). This difficulty follows from the compressibility of the considered problem.
To formulate problem (
52), we need Lagrangian coordinates in
, so we construct
by problem (47). We describe the quantities (see expressions (
14) to (
17)) introduced prior in Theorem 1. Problem (
54) is a linear problem for
and
and nonlinear with respect to
and
,
, with appropriate initial and boundary conditions and the transmission condition. It is a very complicated problem.
The existence and estimate for
,
are derived by the regularizer technique. The method can be found in [
2]. Estimates of nonlinear terms containing
,
, and
can be derived in the same way as in
Section 4. Therefore, we have
where
.
From (18) and (21) and
t being sufficiently small, we have
The above estimate and the standard estimates for differences imply the existence of the solutions described in Theorem 1.
The free boundary problems for incompressible and compressible magnetohydrodynamics were developed by P. Kacprzyk between 2003 and 2015 (see the references in [
2]). The technique developed by P. Kacprzyk is based on the energy method. A more advanced technique developed in [
1,
2] for incompressible magnetohydrodynamics potentiates proving the existence of solutions with the lowest possible regularity for the considered nonlinear problem. The technique in this paper requires the results of V.A. Solonnikov (see the references in [
2]). The mathematical motivation of the considered problem is that it is an open problem. Physically, it means that the magnetohydrodynamic fluid is kept in a bounded domain by the electromagnetic field. Hence, the fusion problem has a physical motivation.
3. Method of Successive Approximations
Let be given.
Definition 1. The Lagrangian coordinates in are initial data to the Cauchy problem Hence, the domain
is defined by
where
.
In free boundary problems in hydrodynamics, the free boundary at any time is built up from the same fluid particles as at time because is tangent to .
To formulate problem (12) in Lagrangian coordinates, we have to introduce them in artificially because there is no velocity in . For this purpose, we need
Definition 2. Let be defined in . Then, we construct in as a solution to the parabolic problem Since
is unknown, we construct it as a solution to the following elliptic problem
A proof of the existence of solutions to (47) is similar to the proof from [
8], where parabolic system (47) with the slip boundary conditions was considered. Having
constructed by problems (47) and (48), we can introduce Lagrangian coordinates
as the Cauchy data to the problems
Then,
where
Expressing problems (9) and (12) in Lagrangian coordinates yields
and
where
in
in
, and
.
Moreover, any operator with subscript means that it contains the transformed gradient , and any operator with subscript ξ contains derivatives with respect to ξ.
To prove the existence of local solutions to problems (
51) and (
52), we apply the following method of successive approximations. Let
be given. Then,
where
. Let
, be given.
Then,
are solutions to the problem
where
in
,
in
, and
6. Conclusions
The aim of this paper is to prove the local existence of solutions to the system of compressible magnetohydrodynamics described in (1)–(8). The considered problem is naturally divided as follows:
- (1)
A given implies v in .
- (2)
A given v implies .
Problem (1), which has the form (
9), determines
in terms of
. Problem (2) is equivalent to (12), where
can be calculated in terms of v. problem (12) describes
in
and
in
, which are coupled by the transmission conditions (
13).
We use the Lagrangian coordinates because the free boundary problems are considered. Unfortunately, in
, there is no velocity, so it is constructed artificially as a solution to problem (2). Applying Lagrangian coordinates in (9) and (12), we obtain problems (
51) and (
52), respectively. Since problems (
51) and (
52) are very complicated, we use the method of successive approximations to prove the existence of the solutions. The method of successive approximations is described in problems (53) and (54). First, we examine (53). It is a linear parabolic system for
- the
-step of the approximations with the r.h.s. dependent on
.
We have three difficulties:
- (1)
the coefficients of the main part of the parabolic system are variable: they depend on ρ;
- (2)
the solvability of a linear parabolic system with constant coefficients in -Besor spaces;
- (3)
estimating
in terms of
, where
are defined in
Section 2.4.
The second difficulty is solved in [
8]. To overcome the first difficulty, we need an appropriate partition of unity to locally define the parabolic system with a constant coefficient. This is conducted at the beginning of
Section 4. In the second part of
Section 4, we derive the estimate
Since we use the
-Besov space, the proof of (
135) is difficult.
To solve problem (
54), we first have to consider the linear problem (
43). We can solve (
43) via the regularizer technique. For this purpose, we need an appropriate partition of unity (see
Section 2.2.1). The problem is considered in [
2], where applying the regularizer technique yields
Using the form of
described in (
54), we prove
where
are defined in
Section 2.4. To prove (
137), we use the same methods as applied in the proof of (
135).
From (
135) and (
137), we obtain, for sufficiently small time, the estimate
where data means initial data and forcing.
Next, for sufficiently small t, we show that differences converge to zero as n tends to ∞.
Hence, the method of successive approximations establishes Theorem 1.