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R E S E A R C H

Open Access

Boundary value problems for modified

Helmholtz equations and applications

Longfei Gu and Zunwei Fu

*

*Correspondence:

[email protected]

Department of Mathematics, Linyi University, Linyi, Shandong 276005, P.R. China

Abstract

We investigate factorizations of modified Helmholtz equations in Clifford algebra

Cl(V3,3). Using the method of fundamental solutions for modified Helmholtz equations and Clifford calculus, we obtain some integral representation theorem in Clifford analysis. The boundedness of singular integral operators in Hölder space is given. Moreover, we establish solvability conditions of Riemann type problems for modified Helmholtz equations in Clifford analysis. As applications, we solve a kind of singular integral equations. The explicit representation of the solution is also given.

MSC: 30G35

Keywords: Clifford algebra; Riemann type problem; Hölder space; modified Helmholtz equations

1 Introduction

As we know, the Helmholtz equations can be regarded as a generalization of the Sturm-Liouville equation to higher dimensions. The research on the Helmholtz equationsu±

κu=  has drawn the attention of some physicists and mathematicians, we refer to [–

]. Using a new transform method, Fokas, ben-Avraham and Antipov translate some im-portant boundary value problems for linear and for integral nonlinear partial differential equations in physical plane to the corresponding modified Helmholtz equations. Novel integral representations for the solution of the Helmholtz and the modified Helmholtz equations formulated in the interior of a convex polygon are presented. These representa-tions provide the basis for the development of certain analytical and numerical techniques for diffusion-limited coalescence, see [–] for more details. This article focuses on mod-ified Helmholtz equations in Clifford analysis.

The Clifford approach is a powerful mathematical tool for the treatment of partial differ-ential equations in higher dimensions, see [–, , –]. Maxwell’s equations in physics are the fundamental equations of electromagnetism and are recast into Helmholtz equa-tions by using the Clifford approach, which is different from the vector calculus method. The electric and magnetic fields are treated together, both encoded as bi-vector into one part of a four-dimensional Clifford number in Clifford approach; we mention here [, – ]. It is natural to consider boundary value problems theory for Helmholtz equations and modified Helmholtz equations in higher dimensions, for instance, Riemann type prob-lems, Dirichlet type probprob-lems, and so on. Besides the pure mathematical interest, these results are necessary for concrete problems in physics and engineering [, ]. In [],

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mann type problems for Helmholtz equations in the framework of Clifford algebraCl(Vn,)

are considered. Based on some ideas from [], Riemann type problems for Helmholtz equations in Hermitian Clifford analysis are studied in []. However, to the best of our knowledge, some boundary value problems for modified Helmholtz equations and their applications in integral equations in the framework of Clifford algebra Cl(Vn,n) (n≥)

have not been considered. The main motivation is that the modified Helmholtz opera-tor has been exactly facopera-torized by means of the so-called±κ-Dirac operators (κ> )i.e., κ= (D+κ)(Dκ) in the Clifford algebraCl(V,).

In this article, motivated by [, ], in the framework of Clifford algebraCl(V,), we obtain second order generalized integral representations and solve some Dirichlet type problems for modified Helmholtz equations. We define some integral operators which are the generalization of classical Cauchy type integral operators, Teodorescu operators in Clifford analysis, and we study some properties of them. Finally, we study Riemann type problems for modified Helmholtz equations and give some applications.

2 Preliminaries

LetV,be an -dimensional real linear space with basis{e,e,e},Cl(V,) be the Clifford algebra overV,and the -dimensional real linear space with basis

eA,A={l, . . . ,lr} ∈PN, ≤l<· · ·<lr≤

,

where N stands for the set{, , } andPN denotes the family of all order-preserving subsets ofNin the above way. Now denotee∅byeandel···lrbyeAforA={l, . . . ,lr} ∈PN. The product onCl(V,) is defined by

⎧ ⎪ ⎨ ⎪ ⎩

eAeB= (–)n((AB)\N)(–)P(A,B)eAB, ifA,BPN,

λμ=A,BPNλAμBeAeB, ifλ=

APNλAeA,

μ=BPNμBeB,

(.)

wheren(A) is the cardinal number of the setA, the numberP(A,B) =jBP(A,j),P(A,j) =

n{i,iA,i>j}, the symmetric difference setABis order-preserving in the above way, and λA∈Ris the coefficient of theeA-component of the Clifford numberλ. It follows from the

multiplication rule above thateis the identity element written now as  and, in particular,

e

i = , ifi= , , ,

eiej= –ejei, if ≤i<j≤.

(.)

ThusCl(V,) is a real linear, associative, but non-commutative algebra. An involution is defined by

eA= (–)

n(A)(n(A)+)

eA, ifAPN, λ=APNλAeA, ifλ=

APNλAeA.

(.)

In view of the multiplication rule (.) and the definition of the involution (.), it is easy to check that

ei=ei, ifi= , , , ,

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The norm of λis defined byλ= (APN|λA|)

. Throughout this article, suppose

is an open bounded non-empty subset ofR with a Lyapunov boundary, denote

+=,–=R\. We now introduce the Dirac operatorD=i=ei∂∂xi. In particular, we haveDD=whereis the Laplacian overR. A functionu:Cl(V,) is said to

be left monogenic if it satisfies the equationD[u](x) =  for each x. A similar definition can be given for right monogenic functions. Elementary properties of the Dirac operators and left monogenic functions can be found in [, , –].

The elliptic partial differential operatorH= (κ), forκ> , corresponds to the

mod-ified Helmholtz equation:

Hu=κu= , (.)

which has as fundamental solution the function

Ex,κ= e

κx

πx. (.)

We defined the operators,Lκas follows:

Lκu=Du+κu, L–κu=Duκu.

By the multiplication rule on Clifford algebraCl(V,), the modified Helmholtz equation may be written as

LκLκu=LκLκu= .

Denote

K(x, y,κ) =  π

y– x

y– x +

κ(y – x)

y– x +

κ

y– x

eκy–x, (.)

K∗(x, y,κ) =

 π

y– x

y– x +

κ(y – x)

y– x –

κ

y– x

eκy–x, (.)

where y – x =i=(yixi)ei. It is clear thatK(x, y,κ) andK∗(x, y,κ) are fundamental

solutions of= 

i=ei∂∂yi+κandLκ= 

i=ei∂∂yiκ, respectively.

3 Integral representation formulas and some properties of generalized Cauchy integral operators

Letbe an open bounded nonempty subset ofRwith a Lyapunov boundary,u(x) =

AeAuA(x), whereuA(x) are real functions.u(x) is called a Hölder continuous functions

onif the following condition is satisfied:

u(x) –u(x)=

A

uA(x) –uA(x)

 

Cx– xα,

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Denote by (,Cl(V,)) the set of Hölder continuous functions with values in

Cl(V,) on (the Hölder exponent isα,  <α< ). Define the norm ofuin (,

Cl(V,)) as

u(α,)=u∞+uα, (.)

whereu∞:=supx∈∂u(x),:=supx,x∈

x=x

u(x)–u(x)

x–xα .

Lemma .[] The Hölder space Hα(,Cl(V,))is a Banach space with norm(.).

Lemma . Let f,gC(,Cl(V,))C(,Cl(V,)).Then

f dσyg=

[f]Lκg dV+

fL–κ[g]dV=

[f]L–κg dV+

fLκ[g]dV.

Proof From Stokes’ theorem in Clifford analysis in [], the results can be directly proved.

Theorem . If uC(,Cl(V,))C(,Cl(V,)) where is an open bounded nonempty subset ofRwith a Lyapunov boundary,then

K∗(x, y,κ)yu(y) +

 π

eκy–x

y– xy[u](y)

–  π

eκy–x

y– xH[u](y)dV=

u(x), x,

, x∈R\, (.)

where K∗(x, y,κ)is as in(.).

Proof Let x∈R\. Using Lemma ., we get

 π

eκy–x

y– xH[u](y)dV

=  π

eκy–x

y– xy[u](y) –  π

eκy–x y– x

LκLκ[u](y)dV

=  π

eκy–x

y– xy[u](y) +

K∗(x, y,κ)[u](y)dV

=  π

eκy–x

y– xy[u](y) +

K∗(x, y,κ)yu(y).

Then the left-hand side of (.) apparently equals zero.

Now, let xand taker>  such thatB(x,r)⊂. Invoking the previous case, we may then write

(\B(x,r))

K∗(x, y,κ)yu(y) +

 π

(\B(x,r)) eκy–x

y– yy[u](y)

–  π

\B(x,r) eκy–x

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Here we take the limits for r→. As regards the weak singularity of eκy–xy–x, the third term of (.) yields

lim

r→

\B(x,r) eκy–x

y– xH[u](y)dV=

eκy–x

y– xH[u](y)dV. (.)

Furthermore we write

(\B(x,r))

K∗(x, y,κ)yu(y) +

 π

(\B(x,r)) eκy–x

y– xy[u](y)

=

K∗(x, y,κ)yu(y) +

 π

eκy–x

y– xy[u](y)

∂B(x,r)

K∗(x, y,κ)yu(y) –

 π

∂B(x,r) eκy–x

y– xy[u](y). (.)

We denote

(x)

∂B(x,r)

K∗(x, y,κ)yu(y) +

 π

∂B(x,r) eκy–x

y– xy[u](y). (.)

It follows from the Stokes formula that

(x) =e

κr

πr

B(x,r)

u(y)dV+κe

κr

πr

B(x,r) u(y)dV

+ e

κr

πr

B(x,r)

(y – x)D[u](y)dV+κe

κr

πr

B(x,r)

(y – x)D[u](y)dV

+e

κr

πr

B(x,r)

[u](y)dV. (.)

Applying the Lebesgue differentiation theorem, we have

lim

r→(x) =u(x). (.)

Combining (.) with (.)-(.), we get the desired result.

Theorem . If uC(,Cl(V,))∩ C(,Cl(V,)) where is an open bounded nonempty subset ofRwith a Lyapunov boundary,then

K(x, y,κ)yu(y) +

 π

eκy–x

y– xyL–κ[u](y)

–  π

eκy–x

y– xH[u](y)dV=

u(x), x,

, x∈R\, (.)

where K(x, y,κ)is as in(.).

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Corollary . If uC(,Cl(V,)) C(,Cl(V,)) where is an open bounded nonempty subset ofRwith a Lyapunov boundary∂and H[u] =LκL–κ[u] = in,then

K(x, y,κ)dσyu(y) +

 π

eκy–x

y– xyL–κ[u](y) =

u(x), x,

, x∈R\, (.)

where K(x, y,κ)is as in(.).

Corollary . If uC(,Cl(V

,))∩C(,Cl(V,)) where is an open bounded nonempty subset ofRwith a Lyapunov boundaryand H[u] =L–

κLκ[u] = in,then

K∗(x, y,κ)dσyu(y) +

 π

eκy–x

y– xy[u](y) =

u(x), x,

, x∈R\, (.)

where K∗(x, y,κ)is as in(.).

Corollary . Let f(x)Cc(,Cl(V,)).The solution of the following Dirichlet boundary value problem:

⎧ ⎪ ⎨ ⎪ ⎩

Hu=f, in,

[u] = , on∂,

u= , on∂,

(.)

is

u(x) = –  π

eκy–x

y– xf(y)dV. (.)

Proof By Theorem ., the solution of (.) is formulated as

u(x) =

K∗(x, y,κ)yu(y) +

 π

eκy–x

y– xy[u](y)

–  π

eκy–x

y– xH[u](y)dV, (.)

since[u] =  andu=  on, the result follows.

Using Theorem ., we also have the following result which can be similarly proved to Corollary ..

Corollary . Let f(x)C

c(,Cl(V,)).The solution of the Dirichlet boundary value

problem

⎧ ⎪ ⎨ ⎪ ⎩

Hu=f, in,

L–κ[u] = , on∂,

u= , on∂,

(.)

is

u(x) = –  π

eκy–x

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Next, we introduce the following generalized Teodorescu operatorsT±κ, the generalized Cauchy integral operatorsF±κ, and the generalized Cauchy singular integral operators

κ:

Tκ[u](x)

K∗(x, y,κ)u(y)dV, x, (.)

T–κ[u](x)

K(x, y,κ)u(y)dV, x, (.)

Fκ[u](x)

K∗(x, y,κ)dσyu(y), x∈R\, (.)

F–κ[u](x)

K(x, y,κ)dσyu(y), x∈R\, (.)

Sκ[u](x)

K∗(x, y,κ)dσyu(y), x, (.)

S–κ[u](x)

K(x, y,κ)dσyu(y), x, (.)

whereκ≥,u(,Cl(V

,)).

Lemma .[] Letbe an open nonempty bounded subset ofRwith a Lyapunov bound-ary∂,u(,Cl(V,)),  <α.Then

lim xx∈

x

Fκ[u](x) =

u(x)

 + 

Sκ[u](x), (.)

lim x→x∈

x∈R\

Fκ[u](x) = –

u(x)

 + 

Sκ[u](x), (.)

lim xx∈

x

F–κ[u](x) =

u(x)

 + 

S–κ[u](x), (.)

lim x→x∈

x∈R\

F–κ[u](x) = –

u(x)

 + 

S–κ[u](x). (.)

Theorem . Letbe an open bounded non-empty subset ofRwith a Lyapunov bound-ary∂,uC(,Cl(V,))C(,Cl(V,)).Then forx,

Tκ[u](x) =u(x). (.)

Proof Step . Becauseu(x) has its compact supportsupp[u], we have

Tκ[u](x) = –

K∗(x, y,κ)u(y)dV

= –

RK∗(x, y,

κ)u(y)dV

= –

RK∗(x, y + x,

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In view ofu(x) having a compact support, the operator acting on Tκ[u](x) may be interchanged with integration. Thus we get

Tκ[u](x) = –lim

r→

R\B(,r)

i= ei

∂xi

K∗(x, y + x,κ)u(y + x)

+κK∗(x, y + x,κ)u(y + x)

dV

= –lim

r→

R\B(,r)

i=

eiK∗(x, y + x,κ)

∂xi

u(y + x)

+κK∗(x, y + x,κ)u(y + x)

dV

= –lim

r→

R\B(,r)

i=

eiK∗(x, y + x,κ)

∂yi

u(y + x)

+κK∗(x, y + x,κ)u(y + x)

dV

= –lim

r→

R\B(,r)

i= ei

∂yi

K∗(x, y + x,κ)u(y + x)

dV.

Using the Stokes formula, we conclude that

Tκ[u](x) =lim

r→

y=r

yK∗(x, y + x,κ)u(y + x)

=lim

r→

y=r

yK∗(x, y + x,κ)

u(y + x) –u(x)

+lim

r→

y=r

yK∗(x, y + x,κ)u(x)

=lim

r→

 π

y=r

y

y

y +

κy

y–

κ

y

eκyu(x)

=lim

r→

eκr

πr

yr

dV+κe

κr

πr

yr

dV

u(x)

=u(x). (.)

Thus we have proved that (.) follows for anyu(x)C

c(,Cl(V,)).

Step . We prove that (.) holds for anyu(x)C(,Cl(V,)). We take a neighborhood V of x such that xV , a real-valued functionC∞() such that|V=  and

supp. Then

u(x) =u+u( –) :=u(x) +u(x).

It is obvious thatu(x)C

c(,Cl(V,)),u(x)C(,Cl(V,)) andu|V=u,u|V = .

Following step , we obtain

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Sinceu(x) equals zero inV, we get

Tκ[u](x) =

K∗(x, y,κ)u(y)dV

=

\V

K∗(x, y,κ)u(y)dV

= . (.)

It follows from (.) and (.) that

Tκ[u](x) =u(x). (.)

Because x is taken arbitrarily in, the result follows.

Corresponding to Theorem ., we have the following theorem.

Theorem . Letbe an open bounded non-empty subset ofRwith a Lyapunov bound-ary∂,uC(,Cl(v,))C(,Cl(V,)).Then forx,

L–κT–κ[u](x) =u(x). (.)

In the following, we need to consider Hölder’s boundedness of the singular integral op-eratorsS±κ. It is necessary to solve the following boundary value problems in Clifford analysis.

Theorem . Let be an open nonempty bounded subset of R with a Lyapunov boundary . Then the generalized Cauchy integral operator Sκ: (,Cl(V,)) →

(,Cl(V,))defined by(.)is bounded,i.e.

Sκ[u](α,)Cu(α,), (.)

where C=max{C

πη

–α(||+  –α) +C,

C(||+η+η)

π η +

κ(Cη+C||)

η }and||denotes the

surface area of.

Proof For x, we have

Sκ[u](x)=  π

y– x

y– x+

κ(y – x)

y– x–

κ

y– x

eκy–xdσ yu(y)

≤ 

π

κ(y – x)

y– xe

κy–xdσ yu(y)

+  π

κ

y– xe

κy–xdσ yu(y)

+  π

y– x

y– xe

κy–xdσ yu(y)

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Sinceis Lyapunov boundary, the normal vector n is continuous on. Therefore, we can choose  <η≤ such that for the scalar product

n(x); n(y)≥

 (.)

for all x, ywithy– xη. It is enough to consider the case ofy– xbeing suffi-ciently small such that the set∂L{y:y– xη}is connected for each x. Then the condition (.) implies that∂Lcan be bijective into the tangent plane toat the point x. Using polar coordinates (r,ω) in the tangent plane with origin in x, for any

u(,Cl(V

,)), we arrive at

L

κ(y – x)

y– xe

κy–xdσ yu(y)

κCu

∂L

y– xdS≤π κCuη

dr

= π κCηu∞, (.)

whereC,Cdenote nonnegative constants which are independent ofu. Here we use the facts thatx– yr, that the surface element

dS= r dr dω

(n(x), x(y)) (.)

can be estimated with the aid of (.) bydS≤r dr dω, and that the projection∂Linto the tangent plane is contained in the interior of the sphere of radiusηand center x. Fur-thermore,

\Lκy(y – x)– xe

κy–xdσ yu(y)

≤π κCu

\∂L

η–dS

≤π κCuη–||, (.)

where||is the surface area of. Inequalities (.) with (.) imply

JκCη

+κC||

η u∞. (.)

Using a similar method to the proof ofJ, we obtain

JκCη

+κC||

η u∞. (.)

Now we estimateJ. Combiningu(,Cl(V,)) with

 π

y– x

y– xy=

, for x,

we have

J≤ 

π

y– x

y– xy

eκy–xu(y) –u(x)

+  π

y– x

y– xy

u(x)eκy–xu(x)

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Cuα  π

y– x–αdS+C  πu∞

y– xdS+u∞

C

π

\∂L

y– x–αdS+

∂L

y– x–αdS

+Cπ

\∂L

y– xdS+

∂L

y– xdS

u∞+u

C

π

η–α||+ η

–α

 –α

+

C

π

η–||+η+ u∞. (.)

Combining (.), (.), (.), and (.), we get

Sκ[u]

C

πη

–α

||+   –α

uα

+

C(||+η+η)

π η +

κ(Cη+C||)

η

u∞, (.)

whereC,C,Cdenote nonnegative constants which are independent ofu.

On the other hand, for x, x∈, it is enough to consider the case ofx– xbeing

sufficiently small. It is obvious that

eκy–xiu(y)Hα×,Cl(V,), i= , ,

and

y– xeκy–xiu(y)Hα×,Cl(V

,)

, i= , .

Applying some properties of the Hilbert transform in Clifford analysis (see [, , , ]) and the weak singularity of yy–x–x andy–x, we conclude

Sκ[u](x) –Sκ[u](x)≤Cx– xα, (.)

whereCis a nonnegative constant independent of xand x. It follows from (.) and

(.) that

Sκ[u](α,)Cu(α,),

whereC=max{C

πη

–α(||+  –α) +C,

C(||+η+η)

π η +

κ(Cη+C||)

η }. The proof is

com-plete.

Remark . By the same technique we obtain the following result that the generalized Cauchy integral operatorS–κ:(,Cl(V,)) →(,Cl(V,)) defined by (.) is

bounded.

Remark . We assumeu(,Cl(V

,)). All integrals are understood in the

Rie-mann integral sense in Lemma . and Theorem .. Now, letLp(,Cl(V

,)), ≤p<∞

be the space of all Clifford algebra valued functions, whosepth power is Lebesgue inte-grable in. IfuLp(,Cl(V,)) then one has to understandF

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and the necessary changes can be easily made. For instance, the limits exist almost every-where onwith respect to the surface Lebesgue measure in Lemma .. Using classical Calderón-Zygmund theory, anLpformulation of Theorem . holds.

In the framework of Clifford algebraCl(V,), we come back to the modified Helmholtz equation (κ)[u](x) = , x. By Theorem ., Theorem ., Theorem ., and Theorem ., we have the following theorem.

Theorem . Suppose thatis an open nonempty bounded subset ofRwith a Lyapunov boundary∂,f,gC(,Cl(V,))∩C(,Cl(V,)),L–κ[f] = and Lκ[g] = in.Then

the function u(x)is determined by

u(x) =Tκ[f](x) +g(x) (.)

or

u(x) =T–κ[g](x) +f(x). (.)

Conversely,suppose u(x)C(,Cl(V

,))and u(x)is a solution of the modified Helmholtz equation.Then u may be represented by(.)or(.),where L–κ[f] = and Lκ[g] = 

in.

4 Some boundary value problems for modified Helmholtz equations and its application

We consider the following Riemann type problem now:

⎧ ⎪ ⎪ ⎪ ⎨ ⎪ ⎪ ⎪ ⎩

Hu= , inR\,

u+(x) =u(x)f(x) +g

(x), x,

[u]+(x) =[u]–(x)A+g(x), x,

limx→∞u(x) = ,

(.)

whereAis any invertible Clifford constant.g(x),g(x), andf(x) are Clifford value func-tions in(,Cl(V,)),  <α< ,H=κ,κ. We establish solvability conditions

of the Riemann type problem (.).

Theorem . Suppose f(x),g(x),g(x)(,Cl(V,)),  <α< ,and f(x)satisfies the

following condition:

 –f(x)(α,)< 

C+ , (.)

where C is a positive constant mentioned in Theorem..Then there exists a unique so-lution to the Riemann type problem(.).

Proof CombiningH[u](x) =L–κ[[u]](x) =  andu(∞) = , we easily checkL–κ[u](x) =  andω(∞) = . Letω(x) =[u](x). Then

(13)

holds. Furthermore, we obtain

ω(x) = ∂K(x, y,κ)dσyg(y), x

+,

∂K(x, y,κ)dσyg(y)A

–, x. (.)

Let

u(x) =

 π

eκy–x

y–x dσyg(y), x

+,

 π

eκy–x

y–x dσyg(y)A–, x–.

(.)

It is easy to see that

[uu](x) = , x∈R\. (.)

Denoteu(x) –u(x) :=ϕ(x), x∈R\, applying the transmission condition

u+(x) =u(x)f(x) +g(x), x,

we have

ϕ+(x) =ϕ(x)f(x) +g(x), x, (.)

where

g(x) =g(x) –ω

eκy–x

y– xdσyg(y) +ω

eκy–x

y– xdσyg(y)A

–f(x).

It is clear thatg(x)(,Cl(V,)),  <α< . We haveϕ() = . Combining (.) with (.), we have

[ϕ] = , inR\,

ϕ+(x) =ϕ(x)f(x) +g(x), x,ϕ(∞) = . (.)

We only need to consider the existence of solutions to (.). The solution to this problem may be written in the form

ϕ(x) =

K∗(x, y,κ)dσyϕ(y), (.)

whereϕ(y) is a Hölder continuous function to be determined on. Using Lemma .,

(.) can be reduced to an equivalent singular integral equation forϕ,

ϕ(x) =

ϕ(x)

 –

K∗(x, y,κ)dσyϕ(y)

 –f(x)+g(x). (.)

We set

()(x) =

ϕ(x) – (Sκϕ)(x)

( –f(x))

(14)

For anyω,ω∈(,Cl(V,)),

–(α,)≤ ω–ω(α,) –f(α,)( +C). (.)

From (.), the integral operatorT is a contraction operator mapping the Banach space

(,Cl(V

,)) into itself. Then the operatorThas a unique fixed point. Thus there exists

a unique solution to (.). The proof is finished.

Remark . In the above Theorem ., the existence and uniqueness of solutions of the Riemann type problem for the modified Helmholtz equation with variable coefficienti.e.,

f(x)(,Cl(V,)) is illustrated. Particularly, whenf(x) is just an invertible Clifford constant, for the boundary value problem (.) there exists a unique solution. Moreover, we have obtained an explicit representation of solutions in [].

As applications, using Lemma . and the results of the boundary value problem, we consider two kinds of singular integral equations and obtain their explicit representations of solutions.

Theorem . Consider the singular integral equation:

u(x)A+ 

K∗(x, y,κ)yu(y)B=f(x), x⊂R, (.)

where f(x)(,Cl(V,)),B is a non-zero Clifford constant,A+B and AB are

in-vertible Clifford constants,and(A+B)–and(AB)–are invertible elements,respectively.

Then:

. Ifu(x)(,Cl(V

,))is a solution to(.),and

F∗(x) =

K∗(x, y,κ)yu(y), x∈R\, (.)

then

F+(x) =F–(x)·(AB)(A+B)–+f(x)(A+B)–, x (.)

and

lim

x→∞F∗(x) = . (.)

. AssumeF∗(x)is solution of Riemann type problem(.)andLκ[F∗](x) = ,

x∈R\,F+(x),F–(x)(,Cl(V

,)).Let

u(x) =F+(x) –F–(x).

Thenu(x)is the solution of the singular equation(.)u(x)(,Cl(V,)).

Proof . Using Lemma ., we have

F+(x) =u(x)  +

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F+(x) = –u(x)  +

K∗(x, y,κ)yu(y). (.)

Combining (.) with (.), we get

F+(x) –F–(x)A+F+(x) +F–(x)B=f(x) (.)

i.e.,

F+(x) =F–(x)·(AB)(A+B)–+f(x)(A+B)–, x. (.)

It is clear thatF(∞) = . The result follows.

. In view of Theorem . and Remark ., we obtain

F∗(x) =

K∗(x, x,κ)yu(y). (.)

By Lemma ., we get

F+(x) =u(x)  +

K∗(x, y,κ)yu(y), (.)

F–(x) = –u(x)  +

K∗(x, y,κ)yu(y). (.)

Combining (.), (.), and (.), the result follows.

Theorem . The singular integral equation(.)is solvable in Hα(,Cl(V

,))and the solution may be represented by the following formula:

u(x) = f(x)

(A+B)–+ (AB)–

+

K∗(x, y,κ)yf(y)

(A+B)–– (AB)–, x. (.)

Proof In view of Theorem ., we consider the following Riemann boundary value prob-lem:

⎧ ⎪ ⎨ ⎪ ⎩

[F] = , inR\,

F+(x) =F–(x)·(AB)(A+B)–+f(x)(A+B)–, x,

F(∞) = .

(.)

We have

F(x) =

K∗(x, y,κ)yf(y)(A+B)–, x+,

∂K∗(x, y,κ)yf(y)(AB)–, x–.

(.)

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Remark . When A= , the singular integral equation (.) is solvable in (,

Cl(V,)) and the solution may be represented by the following formula:

u(x) = 

K∗(x, y,κ)yf(y)B–, x.

The following theorems can be similarly proved as Theorem . and Theorem ..

Theorem . Consider the singular integral equation:

u(x)C+ 

K(x, y,κ)yu(y)D=f(x), x⊂R, (.)

where f(x)(,Cl(V,)),D is a non-zero Clifford constant,C+D and CD are

in-vertible Clifford constants,and(C+D)–and(CD)–are invertible elements,respectively. Then:

. Ifu(x)(,Cl(V

,))is a solution to(.),set

F(x) =

K(x, y,κ)yu(y), x∈R\. (.)

Then

F+(x) =F–(x)·(AB)(A+B)–+f(x)(A+B)–, x (.)

and

lim

x→∞F(x) = . (.)

. Conversely,ifF(x)is solution of Riemann type problem(.)andL–κ[F](x) = , x∈R\,F+(x),F–(x)(,Cl(V

,)).Let

u(x) =F+(x) –F–(x).

Thenu(x)is the solution of singular equation(.),u(x)(,Cl(V,)).

Theorem . The singular integral equation(.)is solvable in Hα(,Cl(V,))and the

solution may be represented by the following formula:

u(x) = f(x)

(C+D)–+ (CD)–

+

K(x, y,κ)yf(y)

(C+D)–– (CD)–, x.

Remark . When C= , the singular integral equation (.) is solvable in (,

Cl(V,)) and the solution may be represented by the following formula:

u(x) = 

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Competing interests

The authors declare that they have no competing interests.

Authors’ contributions

All authors contributed equally to the manuscript and typed, read, and approved the final manuscript.

Acknowledgements

The authors cordially thank the referees for their careful reading and helpful comments. This work was partially supported by NNSF of China (Nos. 11401287 and 11271175), the AMEP and DYSP of Linyi University.

Received: 6 September 2015 Accepted: 12 November 2015

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