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        A Riemann-Hilbert Approach to the Harry-Dym Equation on the Line?

        2016-06-09 03:34:26YuXIAOEnguiFAN

        Yu XIAO Engui FAN

        1 Introduction

        The following nonlinear partial differential equation

        is known as the Harry-Dym equation(see[1]).This equation was obtained by Harry Dym and Martin Kruskal as an evolution equation solvable by a spectral problem based on the string equation instead of the Schr?dinger equation.The Harry-Dym equation plays an important role in the study of the Saffman-Taylor problem which describes the motion of a two-dimensional interface between a viscous and a nonviscousfluid(see[2]).The Harry-Dym equation shares many of the properties typical of the soliton equations.It is a completely integrable equation which can be solved by the inverse scattering transform(see[3]).It has a bi-Hamiltonian structure(see[4]),an in finite number of conservation laws and in finitely many symmetries(see[5]),and has reciprocal Backlund transformations to the KdV equation(see[6]).The Harry-Dym equation has been solved by different methods such as the inversing scattering method(see[3]),the B¨acklund transformation technique(see[7]),and the straightforward method(see[8]).Especially,Wadati obtained the one-cusp soliton solution(see[3])

        by using inverse scattering transformation.

        The main aim of this paper is to develop the inversing scattering method,based on a Riemann-Hilbert problem for solving nonlinear integrable systems,which has further developed and applied many equations with initial value problems on the line(see[9–11])and initial boundary value problems on the half line(see[12–17]).In this paper,we consider the initial value problem of the Harry-Dym equation

        where the q0(x)is a smoothly real-valued function and decays as|x|→ ∞.The organization of the paper is as follows.In the following Section 2,we perform the spectral analysis of the associated Lax pair for the Harry-Dym equation.In Section 3,we formulate the main Riemann-Hilbert problem associated with the initial value problem(1.2).In Section 4,we obtain the one-cusp soliton solution in terms of the Riemann-Hilbert problem,which has a similar,but not the same,form constructed by the inverse scattering method(see[3]).

        2 Spectral Analysis

        2.1 A Lax pair

        In general,the matrix Riemann-Hilbert problem is defined in the λ plane and has explicit(x,t)dependence,while for the Harry-Dym equation(1.2),we need to construct a new matrix Riemann-Hilbert problem with explicit(y,t)dependence,where y(x,t)is a function unknown from the initial value condition.For this purpose,we make a transformation

        and(1.2)can be expressed by

        Then the initial value problem(1.2)is transformed into

        It was shown that(1.2)admits the following Lax pair(see[3]):

        Making a transformation then the Lax pair(2.2)can be written in the matrix form

        where

        Further,by the gauge transformations

        we have

        where

        It is clear that as|x|→ ∞,U(x,t)→ 0 and V(x,t,λ)→ 0.We define a real-valued function y(x,t)by

        It is obvious that

        The conservation law

        implies that

        Extending the column vector φ to be a 2×2 matrix and letting

        then μ solves

        which can be written in the full derivative form

        where

        and[σ3,μ]= σ3μ ? μσ3.As|x| → ∞,→ 0.The lax pair in(2.5)is very convenient for dedicated solutions via the integral Volterra equation,which is also what we study in the following paper.

        Remark 2.1 By the representation of M,N and U,V in(2.3)and(2.4)respectively,wefind that ψx,ψtand φx,φthave no singularity in λ =0.Therefore,φ has no real singularity in λ=0.

        2.2 Eigenfunctions

        We define two eigenfunctions μ±of(2.5)as the solutions of the following two Volterra integral equations in the(x,t)plane:

        where I is a 2×2 identity matrix,andacts on a 2×2 matrix A bySince the integrated expression is independent of the path of integration,we choose the particular initial points of integration to be parallel to the x-axis and obtain that for μ+and μ?,

        De fine the following sets:

        Since for any fixed t,yx=ρ(x,t)>0,y(x,t)is an increasing function of x for fixed t.As x?x?<0,y(x,t)?y(x?,t)<0;as x?x?>0,y(x,t)?y(x?,t)>0.We can deduce that the second column vectors of μ+and μ?are bounded and analytic for λ ∈ C provided that λ belongs to D1and D2,respectively.We denote these vectors with superscripts(1),(2)to indicate the domains of their boundedness.Then

        For any x and t,the following conditions are satisfied:

        2.3 Spectral functions

        For λ ∈ R,the eigenfunctions μ+,μ?being the solution of the system of differential equations(2.5)are related by a matrix independent of(x,t).We define the spectral function by

        From(2.5),we get

        Sincethe μ±(x,t,λ)have the relations:

        The spectral function s(λ)can be written as

        From the(2.9),det(s(λ))=1.Equations(2.8)–(2.9)imply that a(λ)and b(λ)have the following properties:

        (1)a(λ)is analytic in D1and continuous for λ ∈

        (2)b(λ)is continuous for λ ∈ R.

        (3)

        (4)a(λ)=1+O,λ→∞,λ∈D1.

        (5)b(λ)=O??,λ→∞,λ∈R.

        2.4 Residue conditions

        We assume that a(λ)has N simple zerosin the upper half plane.These eigenvalues are purely imaginary.The second column of(2.8)is

        For(2.9)and(2.13),it yields

        where we have used that both sides are well defined and analytic in D1to extend the above relation toHence,if a(λj)=0,the,are linearly dependent vectors for each x and t,i.e.,there exist constants bj?=0 such that

        Recalling the symmetries in(2.10),wefind

        Consequently,the residues

        where

        Remark 2.2 There is the relation of μ±that the s(λ)is the scattering matrix for the one-dimensional Sch?dinger equation:

        via the Liouville transformation:

        Therefore,in terms of the spectral problem of the Schr?dinger equation,we deduce that a(λ)has only pure imaginary part of simple poles in the upper plane.

        3 The Riemann-Hilbert Problem

        3.1 A Riemann-Hilbert problem for(x,t)

        We now solve the initial value problem for(2.1)on the line,and the solution can be expressed in terms of a 2×2 matrix Riemann-Hilbert problem.Let M(x,t,λ)be defined by

        and let the M satisfy the jump condition:

        where

        These definitions imply

        and

        This contour of the Riemann-Hilbert problem is the real axis.

        The jump matrix J(x,t,λ),and the spectral a(λ)and b(λ)are dependent on the y(x,t),while y(x,t)doesn’t involve initial data.Therefore,this Riemann-Hilbert problem can not be formulated in terms of initial data alone.In order to overcome this problem,we will reconstruct a new jump matrix by changing

        where y is a new scale.Then we can transform this Riemann-Hilbert problem into the Riemann-Hilbert problem parametrized by(y,t).

        3.2 A Riemann-Hilbert problem for(y,t)

        Theorem 3.1 Let q0(x),x∈R be a smooth function and decay as|x|→ ∞.Moreover 1+q0(x)>0.Define the,ρ0and y0(x)as follows:

        Let μ+(x,0,λ)and μ?(x,0,λ)be the unique solution of the Volterra linear integral equation(2.5)evaluated at t=0 withDe fine a(λ),b(λ),Cjby

        and

        here and here after([A]1[A]2)denotes the first(second)column of a 2×2 matrix A.We assume that a(λ)has N simple zerosin the upper half plane and is pure imaginary.Then

        (1)a(λ)is defined for k ∈and analytic in D1.

        (2)b(λ)is defined for λ ∈ R.

        (4)a(λ)=1+O,λ→∞,λ∈D1.

        (5)b(λ)=O??,λ→∞,λ∈R.

        Suppose that there exists a uniquely solution q(x,t)of(1.2)with initial data q0(x)such thathas sufficient smoothness and decays for t>0.Then q(x,t)is given in the parametric form by

        and the function x(y,t)is defined by

        where m(y,t)and M(y,t,λ)is the unique solution of the following Riemann-Hilbert problem:

        (1)

        is a sectionally meromorphic function.

        (2)

        where J(y)(y,t,λ)is defined by

        (3)

        (4)The possible simple poles of the first column of M+(y,t,λ)occur at λ = λj,j=1,···,N,and the possible simple poles of the second column of M?(y,t,λ)occur at λ =,j=1,···,N.The associated residues are given by

        Proof Assume that μ(x,t)is the solution of equation(2.5),and its asymptotic expansion is

        into the x-part of(2.5),where μ(1)(x,t), μ(2)(x,t)and μ(3)(x,t)are 2×2 matrices,dependent on x,t.By considering the terms of O(1),We get

        By construction of the new Riemann-Hilbert problem about(y,t,λ),we can deduce that

        Then

        (3.13)can be expressed in terms of y=y(x,t).Indeed,using=ρ,then(3.15)becomes

        As|y|→ ∞,ρ(y,t)→ 1,by the evaluation of(3.16),we get

        Therefore

        As|x|→ ∞,|y|→∞ and=ρ>0,

        Remark 3.1 It follows from the symmetries(2.10)that the solution M(y,t,λ)of the Riemann-Hilbert problem in Theorem 3.1 has the symmetries:

        4 Soliton Solution

        The solitons correspond to the spectral data{a(λ),b(λ),Cj}for which b(λ)vanishes identically.In this case,the jump matrix J(y)(y,t,λ)in the(3.9)is the identity matrix and the Riemann-Hilbert problem of Theorem 3.1 consists of finding a meromorphic function M(y,t,λ)satisfying(3.10)and the residue conditions(3.11)–(3.12).From(3.10)–(3.11),we get

        For the symmetries(3.17),(4.1)can be written as

        Letbecomes

        Solving this algebraic system for M12(y,t,λj),M22(y,t,λj),n=1,···,N,and substituting them into(4.1)provide an explicit expression for the[M(y,t,λ)]1.In terms of the symmetries(3.17),we can get M12(y,t,λ),which solves the Riemann-Hilbert problem.Then

        Therefore,the N soliton solution q(x,t)is expressed by the(3.7).

        4.1 The one-soliton solution

        In this section,we derive an explicit formula for the one-soliton solution,which arises when a(λ)has a pure imaginary λ1of simple zero.Letting N=1 in(4.3),from the the symmetries of(2.10),we can deduce thatand thenSince the b1is a real constant,wefind that C1=?C1,and thus C1is pure imaginary.Making use of the symmetries of(3.17),we can obtain

        Then

        Substituting this result into(4.3),we get

        Let λ1=iε, ε >0,and in order to conveniently study the properties of the one soliton solution,we choose C1= ±2iε.When C1= ?2iε,substituting both parameters into(4.4),it comes into being that

        Then

        where the arctanhx is the inverse function of tanhx.Furthermore,

        The solution q(x,t)in(3.7)can be transformed into

        Letting α(y,t)=earctanhe?2(εy?4ε3t),wefind that Lnα(y,t)=arctanhe?2(εy?4ε3t),and then

        i.e.,

        We deduce

        (4.7)can be written as

        Substituting y with x,(4.8)becomes

        whereThen(4.9)can be varied as(1+q(x,t)?1=cosh2(?εx+4ε3t?εγ(x,t)),and hence the one soliton solution q(x,t)has a singularity at the peak of the soliton,the so-called cusp soliton.

        When λ1=iε and C1=2iε,the corresponding one soliton solution q(x,t)of(1.2)can be expressed as

        where

        Remark 4.1 In this paper,we use the Riemann-Hilbert approach to obtain the solution q(x,t)of(1.2)expressed by(4.9)–(4.10).While[3]applies the inverse scattering method to get the solution q(x,t).If ε= κ (κ in[3],to the one soliton solution,when C1= ?2iε,the expression of the solution in both papers is similar,identical with ?εx+4ε3t in the

        and κx?4κ3t in the tanh?4(κx?4κ3t?κx0+ε+)in[3]).There is a different point about the expression of the one soliton solution in the two papers,i.e.,one is dependent of the?εγ(x,t)of x and the other is?κx0+ε+of x.

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