The estimations of scalar products of vector fields and their norms play a significant role in proving the solvability of mathematical physics problems. Many researches are devoted to the study of estimates of the norms of vector functions in different functional spaces [1-4]. But in the most cases such estimations require the homogeneous areas when their parameters don’t depend on space coordinates [5,6].

For inhomogeneous areas we suggest using estimations of scalar products of vector fields for the mathematical physics problems. In the publications [7-10] some L_p-estimations of scalar product of vector fields in the limited areas were obtained and was investigated the possibility of their application to study the solvability of different problems of electromagnetic theory.

It is natural to study problem formulations in non-homogeneous unbounded domains for most problems of mathematical physics. In the publications [11,12] we proved L₂-estimations of scalar products of vector fields in unlimited areas.

The paper is dedicated to solvability of a stationary set of Maxwell equations in the whole space, based on the proved L_p-estimations of scalar product in the weighted functional spaces.

Let be an open subset of space (particularly).

Let be a Banach space of functions, summable with power, where a norm is

Let be a Banach space of vector-functions,

where (), with a norm

.

Let and be Banach spaces

with norms

respectively.

We denote by and the closures of the set of test vector-functions in and, respectively.

The following estimates for scalar products of vector fields in the bounded star-shaped domain with the regular boundary were obtaned in [8,9,11].

Lemma 2.1. Let,. There exists a constant, that for any and

Lemma 2.2. Let,. There exists a constant, that for any ,

Lemma 2.3. Let,. There exists a constant, that for any and

The main result of this paper is a proof of similar estimates for.

Let. For each and we define Banach spaces of vector-functions:

with the corresponding norms

,

.

For [12] these spaces are defined as:

The main result of the current article is Theorem 3.1. Let, , ,. Then there exists a positive constant , which does not depend on vector-functions and, and the inequality

is correct.

In proving Theorem 3.1 the following statement is used.

Lemma 3.2 [7]. Let be an open set in (particularly,) star-shaped on. Then the following identities are true for all and each function

Let, ,. Then the identities (2) and (3) are equivalent to

Proof (Theorem 3.1). Let. Let and be smooth vector-functions on

Let denote a closed solid sphere with radius centered at the origin and with the boundary. Consider the integral

where is a function of scalar argument

We use the representation (3) for the vector-function in the integral (6)

For the first of resulting integrals () we use a vector field relation

and then we invoke the Gauss-Ostrogradsky theorem and use the fact that when. So

or passing to spherical coordinates the operator

We estimate the first integral. Applying Hölder’s inequality to we get

then

Applying Hölder’s inequality to the second inner integral, we have:

We can write the estimation as

It is obvious that if an expression , then

Let us estimate the integral. It is evident the the

, where

Applying Hölder’s inequality several times, we get

The following estimation is obvious

Hense

then when.

Next we construct an estimation for integral. We apply Hölder’s inequality to.

So, we get an estimation for:

We use Hölder’s inequality for the second integral again.

Let’s estimate the following integral

Denote and consider

When (i.e.), then

and, respectively

If we get

At last, when, then

Thus, we obtain

and therefore

Bringing together the constructed estimates, we derive the following inequality for integral (6)

where

Going to the limit for in the last inequality, we will obtain estimation (1).

Note, that for the theorem may be proved similarly using the Equivalence (2).

As an example of using the estimations proved in Section 3, we will consider a problem of determining the magnetic field stretch in the whole space with a bounded conducting subdomain.

Stationary electromagnetic field is described by the set of stationary Maxwell’s equations

Here. The conductivity of the atmosphere is denoted as. Let denotes a bounded open star-shaped subset of defined by conditions

Functions are permeability and permittivity. They satisfy the following conditions

The is a vector-function of the external electromotive force, which is asumed given and satisfying the condition

Function equals zero for almost all .

We introduce the necessary functional spaces

Denote. It is readily proved that this functional space will be Hilbert space relatively to scalar product

We name the solution of the Problem (7)-(10) the functions, and satisfying condition for almost all.

The validity of (10) implies the distibution for all defined by the formula

Equation (7) in conducting subdomain will be

and in nonconducting subdomain () it becomes an identity.

Multiplying the last equation by, , integrating along, and using or

.

It becomes obvious that the problem of determining the stationary magnetic field can be formulated as follows:

Determine vector-function satisfying the integral identity

for all functions.

We need the following statement to prove the theorem of solvability (Theorem 4.2) for the Problem (14).

Lemma 4.1 (Lax-Milgram [13]). Let be a Hilbert space over the field of real numbers. Let be a symmetric bilinear bounded coercive form,—linear bounded functional. Then there exists a unique element satisfying the equality

for all.

Theorem 4.2 (Solvability of the Problem (14)). Let

satisfy (11), (12), and

for almost all. Then the solution of the generalized Problem (14) exists and is unique.

Proof. Let’s verify the conditions of the Lax-Milgram lemma.

Let us denote

Obviously, is a bilinear and symmetric form. The finiteness is easily proved by condition (11):

Using the Cauchy-Bunyakovsky-Schwarz inequality, we obtain

Let’s show coercivity of the form.

Whereas thus for each, i.e. the vector-function satisfies estimation

The following notation is used. Let’s use Estimation (1)

Since, the last summand is zero. Then using the Hölder’s inequality, we obtain

Hense

where. The estimates show the coercivity of the bilinear form, because

Now we verify the conditions for functional. The linearity is obvious. Let’s show the finiteness using the Cauchy-Bunyakovsky-Schwarz inequality

Thus, all the constraints of the Lax-Milgram lemma are satisfied, and the solution of the Problem (14) exists and is unique.

Remark. The solvability of the studied problem is also true when is a positive-definite tensor. The scheme of the proof is similar to Theorem 4.2.

Let satifies relation (14) for all . Let’s show that other indefinite functions will be defined in from equaitons (7)-(10) as values depending on.

We determine function in the conductivity area by equality

Let. Let’s extend by zero in. According to the Lax-Milgram lemma there is the unique function, which for each satisfies the equality

Then and as, then. Therefore we obtain that

This shows that.

The function is defined by relation (13) as shown above.

The paper was devoted to the proof of L_p-estimation of vector fields in weighted functional spaces. Also we discussed a solvability of the problem of determinig the magnetic field stretch in the whole space. The proof of solvability is based on the proved estimation.

This work was supported by Analytical Departmental Program “Highschool scientific potential growth” (2009- 2011) Russian Ministry of Education and Science (reg. no. 2.1.1/3927), Federal Target Program “Scientific and Scientific-Pedagogical Personnel of Innovative Russia” (2009-2013) (project NK-13P-13) and RFBR Grant (project 09-01-97019-r_povolzhie_a).