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Global conservative solutions for a modified periodic coupled Camassa-Holm system

  • Received: 01 April 2020 Revised: 01 July 2020 Published: 24 August 2020
  • Primary: 35A01, 35A02; Secondary: 35D30, 35G25, 35G25

  • In present paper, we deal with the behavior of a solution beyond the occurrence of wave breaking for a modified periodic Coupled Camassa-Holm system. By introducing a new set of independent and dependent variables, which resolve all singularities due to possible wave breaking, this evolution system is rewritten as a closed semilinear system. The local existence of the semilinear system is obtained as fixed points of a contractive transformation. Moreover, this formulation allows us to continue the solution after wave breaking, and gives a global conservative solution where the energy is conserved for almost all times. Returning to the original variables. We finally obtain a semigroup of global conservative solutions, which depend continuously on the initial data. Additionally, our results repair some gaps in the pervious work.

    Citation: Rong Chen, Shihang Pan, Baoshuai Zhang. Global conservative solutions for a modified periodic coupled Camassa-Holm system[J]. Electronic Research Archive, 2021, 29(1): 1691-1708. doi: 10.3934/era.2020087

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  • In present paper, we deal with the behavior of a solution beyond the occurrence of wave breaking for a modified periodic Coupled Camassa-Holm system. By introducing a new set of independent and dependent variables, which resolve all singularities due to possible wave breaking, this evolution system is rewritten as a closed semilinear system. The local existence of the semilinear system is obtained as fixed points of a contractive transformation. Moreover, this formulation allows us to continue the solution after wave breaking, and gives a global conservative solution where the energy is conserved for almost all times. Returning to the original variables. We finally obtain a semigroup of global conservative solutions, which depend continuously on the initial data. Additionally, our results repair some gaps in the pervious work.



    In this paper, we investigate the Cauchy problem of the modified periodic coupled Camassa-Holm system that has the following form:

    {mt+2mux+mxu+(mv)x+nvx=0,t>0, xR,nt+2nvx+nxv+(nu)x+mux=0,t>0, xR,m(0,x)=m0(x), n(0,x)=n0(x),t=0, xR,m(t,x)=m(t,x+1), n(t,x)=n(t,x+1),t>0, xR, (1)

    where m=uuxx and n=vvxx are periodic function respect to x. The system (1) is a generalization of the Camassa-Holm equation with peakon solitons in the form of a superposition of multipeakons which was firstly proposed by Fu and Qu in [13]. The well-posedness and blow-up solutions of periodic case for the system (1) were discussed by Fu et al. in [14]. In [30], the authors established the local well posedness and blow-up solutions in Besov spaces. The attractor, non-uniform dependence and persistence properties of the system (1) were discussed in [29,33]. Furthermore, Tian el at. in [28] investigated the global conservative and dissipative solutions of system (1) by tansforming it into an equivalent semilinear ODE system. However, there is gap in [28,31], i.e., the second derivative terms uxx and vxx appeared in the equivalent ODE system cannot be controlled by the H1(R) conservation law. This paper repair the gap in the following sections.

    It is known to us, when u=v and let ˜t=2t, system (1) can be degenerated to the famous Camassa-Holm equation:

    mt+2mux+mxu=0,m=uuxx. (2)

    The Camassa-Holm equation (2) was first implicitly contained in a bi-Hamiltonian generalization of the Korteweg-de Vries equation by Fuchssteiner and Fokas [15], and later deduced as a model for unidirectional propagation of shallow water over a flat bottom by Camassa and Holm [4]. Similar to the KdV equation, the Camassa-Holm equation has a bi-Hamilton structure [15,24], and is completely integrable [4,5,23]. The equation (2) not only holds an infinity of conservative laws, but also can be solved by its corresponding inverse scattering transform [2,9]. The solitary waves of equation (2) are solitons (i.e., it can keep their shape and velocity after interacted by the same type nonlinear wave). Compared to the KdV equation, the Camassa-Holm equation has many advantages, such as, it has both the finite time wave-breaking solutions (i.e. the solution keeps bounded but the slope becomes unbounded in finite time) and the global strong solutions [6,7,11,25]. The solitary wave solutions are peaked waves and a specific case was given in [4], it is not a classical solution because it has a peak at their crest. The local well-posedness of equation (2) with the inial data u0Hs,s>32 was studied in [1,7,25]. Many papers have investigated the weak solutions for the equation (2). Especially, in the non-periodic case, Bressan and Constantin in [3] has done many works, they developed a new method to investigate a conservative solution's semigroup. In the periodic case, Holden and Raynaud in [22] applied the semigroup theory to investigate the periodic Camassa-Holm equation, and proved its conservative solutions, depending continuously on the initial data, which can also construct a semigroup.

    Of course, the Camassa-Holm equation has many generalizations such as the modified two-component Camassa-Holm equation (M2CH) and the coupled Camassa-Holm equation. The M2CH equation was firstly introduced by Holm et al. in [21] as a modified version of the two-component Camassa-Holm equation (2CH) that was proposed by Constantin and Ivanov [10] in the context of shallow water theory. The M2CH equation is integrable and its form as follow;

    {mt+2mux+mxu+ρˉρx=0,ρt+(ρu)x=0,  (3)

    where m=uuxx. The equations (3) was testified that admits singular solutions in both of the variables m and ρ in [21]. The well-posedness, blow-up phenomena, Lipschitz metric and the global weak solution for the equations (3) were studied by Guan et al. in [17,18,19,20]. Tan et al. investigated the global conservative solutions for both of the periodic case and the non-periodic case in [26,27]. Guan proved the Cauchy problem of the M2CH with the initial data z0=(u0,ρ0)H1(R)×(H1W1,)) has a unique global conservative weak solution in [16].

    Inspired by [3,22,26,34,35], this paper mainly discusses the global conservative solutions of the modified periodic Camassa-Holm system. As is known to us, equations (1) is a system, so it's more difficult than the single one. Moreover, the interactions between u and v greatly increases the complexity of the research. To overcome these difficulties, we set the characteristics that completely different from the one used in [3,22,26]. Thus, the calculation is largely reduced. By introducing new variables, we transform the system (1) into a equivalent semilinear ODE system. Firstly, we get the global solutions of the equivalent semilinear ODE system. Then we get the global conservative solutions for the system (1) from the global solutions of the equivalent ODE system. Finally, we obtain a semigroup of the solutions depending continuously on inial data for the original system.

    The rest of this paper is organized as follows. Section 2 is the basic equation. In section 3, we get a equivalent semilinear system and the global solutions of the semilinear system. In section 4, we obtain the global conservative solution of the system (1) and construct a solution semigroup.

    Now, we reformulate the system (1). Let m=uuxx and n=vvxx. Note that G:=12sinh12cosh(x[x]12), xR, and (12x)1f=Gf for all fL2(R). Thus, we can rewrite system (1) as follow:

    {ut+(u+v)ux+P1+P2,x=0,t>0, xR,vt+(u+v)vx+Q1+Q2,x=0,t>0, xR,u(0,x)=u0(x), v(0,x)=v0(x),t=0, xR,u(t,x)=u(t,x+1), v(t,x)=v(t,x+1),t>0, xR, (4)

    where P1,P2,Q1,Q2 have the following form:

    {P1=G(uvx),P2=G(u2+12u2x+uxvx+12v212v2x),Q1=G(vux),Q2=G(v2+12v2x+uxvx+12u212u2x).

    According to the fact that the above representations, P1 and Q1 are symmetrical, P2 and Q2 are symmetrical, For convenience, we can set P1(u,v)=Q1(v,u)=G(uvx). So do P2 and Q2.

    In fact, for smooth solutions, differentiating the first and the second equations in (4) with respect to x, we get

    {uxt+u2x+uxvx+uuxx+vuxx+P1,x+P2(u2+12u2x+uxvx+12v212v2x)=0,vxt+v2x+uxvx+vvxx+uvxx+Q1,x+Q2(v2+12v2x+uxvx+12u212u2x)=0. (5)

    Multiplying the first and the second equations in (4) by u and v, and multiplying the first and the second equations in (5) by ux and vx, respectively, we get following conservation laws

    {(u22)t+(u2x2)t+(u2v+uu2x+vu2x+2uP22)x ux(v2+v2x)+vx(u2u2x)2+uP1+uxP1,x=0,(v22)t+(v2x2)t+(v2u+vv2x+uv2x+2vQ22)x      vx(u2+u2x)+ux(v2v2x)2+vQ1+vxQ1,x=0. (6)

    For regular solutions, using (6) and integrating by parts, it is clear that the total energy

    E(t)=S(u2+u2x+v2+v2x)dx

    is a constant in time. If u and v are smooth, from (4)-(6), it is not very hard to check that

    (u2+u2x+v2+v2x)t+((u+v)(u2+u2x+v2+v2x))x=(u32uP22uP1,x+v32vQ22vQ1,x)x. (7)

    Firstly, we introduce the space E1:

    E1={fH1loc(R)|f(θ+1)=f(θ)+1},

    and define the characteristics y:RE1,ty(t,) as the solution of

    yt(t,θ)=(u+v)(t,y(t,θ)). (8)

    In addition, we denote

    {U(t,θ)=u(t,y(t,θ)),V(t,θ)=v(t,y(t,θ),M(t,θ)=ux(t,y(t,θ),N(t,θ)=vx(t,y(t,θ), (9)

    and

    H(t,θ)=y(t,θ)y(t,0)(u2+u2x+v2+v2x)dx. (10)

    By (7) and (8), we get

    {dHdt=[(u32uP1,x2uP2+v32vQ1,x2vQ2)y]θ0,Hθ=[(u2+u2x+v2+v2x)y]yθ. (11)

    Using (10), the periodicity of u,v and yE1, we obtain

    H(t,θ+1)H(t,θ)=H(t,1)H(t,0).

    According to (11), it is very easy to prove that H(t,1)H(t,0) is a constant in time. Thus, we get that H(t,1)H(t,0)=H(0,1)H(0,0). For every t>0, H belongs to the vector space E defined as follow

    E={fH1loc(R)|f(θ+1)f(θ)=f(1)f(0)}.

    We define the norm fE=fH1[0,1] for E. For convenience, we will replace H1[0,1] by H1. Later, we will verify that E is complete.

    We derive formally a system equivalent to system (4). From the definition of the characteristics, it follows that

    {Ut(t,θ)=(P1P2,x)y(t,θ),Vt(t,θ)=(Q1Q2,x)y(t,θ),Mt(t,θ)=(M22N22+U2+V22P1,xP2)y(t,θ),Nt(t,θ)=(N22M22+V2+U22Q1,xQ2)y(t,θ). (12)

    Then, we get the explicit expression for Pi, Qi, Pi,x, Qi,x (i = 1, 2):

    {P1(u,v)=12sinh1210cosh(xy[xy]12)(u(t,y)vx(t,y))dy,P1,x(u,v)=12sinh1210sinh(xy[xy]12)(u(t,y)vx(t,y))dy,P2(u,v)=12sinh1210cosh(xy[xy]12)×(u2(t,y)+12u2x(t,y)+ux(t,y)vx(t,y)+12v2(t,y)12v2x(t,y))dy,P2,x(u,v)=12sinh1210sinh(xy[xy]12)×(u2(t,y)+12u2x(t,y)+ux(t,y)vx(t,y)+12v2(t,y)12v2x(t,y))dy,

    and Q1(u,v)=P1(v,u), Q1,x(u,v)=P1,x(v,u), Q2(u,v)=P2(v,u), Q2,x=P2,x(v,u).

    In the above formulae, we can perform the change of variables y=y(t,θ), and rewrite the convolution respect to θ. From (9), we get new expressions of Pi, Qi, Pi,x, Qi,x(i=1,2) with the new variable θ

    {P1(t,θ)=12(e1)10cosh(y(t,θ)y(t,θ))(UNyθ)(t,θ)dθ+1410exp(sgn(θθ)(y(θ)y(θ)))(UNyθ))(t,θ)dθ,P1,x(t,θ)=12(e1)10sinh(y(t,θ)y(t,θ))(UN)yθ)(t,θ)dθ1410sgn(θθ)exp(sgn(θθ)(y(θ)y(θ)))(UNyθ))(t,θ)dθ,P2(t,θ)=12(e1)10cosh(y(t,θ)y(t,θ))(Hθ+(U2+2MNN2)yθ)(t,θ)dθ+1410exp(sgn(θθ)(y(θ)y(θ)))×(Hθ+(U2+2MNN2)yθ)(t,θ)dθ,P2,x(t,θ)=12(e1)10sinh(y(t,θ)y(t,θ))(Hθ+(U2+2MNN2)yθ)(t,θ)dθ 1410sgn(θθ)exp(sgn(θθ)(y(θ)y(θ)))×(Hθ+(U2+2MNN2)yθ)(t,θ)dθ, (13)

    and

    {Q1(u(t,θ),v(t,θ))=P1(v(t,θ),u(t,θ)),Q1,x(u(t,θ),v(t,θ))=P1,x(v(t,θ),u(t,θ)),Q2(u(t,θ),v(t,θ))=P2(v(t,θ),u(t,θ)),Q2,x(u(t,θ),v(t,θ))=P2,x(v(t,θ),u(t,θ)). (14)

    Straight computation shows that

    {P1,θ=P1,xyθ, P1,xθ=UNyθ+P1yθ,P2,θ=P2,xyθ, P2,xθ=[Hθ+(U2+2MNN2)yθ]+P2yθ,Q1,θ=Q1,xyθ, Q1,xθ=VMyθ+Q1yθ,Q2,θ=Q2,xyθ, Q2,xθ=[Hθ+(V2+2MNM2)yθ]+Q2yθ. (15)

    From (8), (11)-(12) and (13)-(15), we obtain a new system which is equivalent to system (4). And the Cauchy problem of the new system can be rewritten with respect to the variables (y,U,V,M,N,H) in the following form

    {yt=U+V,Ut=P1P2,x,Vt=Q1Q2,x,Mt=M22N22+U2+V22P1,xP2,Nt=N22M22+V2+U22Q1,xQ2,Ht=(u32uP1,x2uP2+v32vQ1,x2vQ2)|θ0. (16)

    Differentiating (16) with respect to θ and utilizing (15), we have

    {yθt=Uθ+Vθ,Uθt=Hθ2+(U22+MNN2P1,xP2)yθ,  Vθt=Hθ2+(V22+MNM2Q1,xQ2)yθ,   Hθt=(3U22P2)Uθ+(3V22Q2)Vθ2(UP2,x+VQ2,x)yθ  2(MP1,x+UP1U2N+NQ1,x+VQ1V2M)yθ. (17)

    The system (17) is semilinear for the variables yθ, Uθ, Vθ and Hθ. By introducing the space H1per

    H1per={fH1loc(R)|f(θ+1)=f(θ)},

    with the norm fH1per=fH1[0,1], We define a linear map Φ: fH1per×R E as Φ:(σ,h) f=σ+hId.

    Lemma 3.1. The map Φ defined above is homeomorphism from H1per×R to E.

    It is clear that the space E is a Banach space, because the space H1per×R is a Banach space. Let's introduce η = yId and (σ,h) = σ+hId, i.e. h=H(t,1)H(t,0) and σ=HhId. Therefore, the system (16) is equivalent to

    {ηt=U+V,Ut=P1P2,x,Vt=Q1Q2,x,Mt=M22N22+U2+V22P1,xP2,Nt=N22M22+V2+U22Q1,xQ2,σt=(u32uP1,x2uP2+v32vQ1,x2vQ2)|θ0,ht=0. (18)

    In the next section, the well-posedness of system (18) will be proved as an ordinary differential equations in the Banach space W. Note that

    W=H1per×H1per×H1per×Lper×Lper×H1per×R.

    We have a bijection(η,U,V,M,N,σ,h) (y,U,V,M,N,H) from W to E1×H1per×H1per×Lper×Lper×E with y=η+Id and H=σ+hId.

    Theorem 3.2. Let ˉX = (ˉη,ˉU,ˉV,ˉM,ˉN,ˉρ,ˉh)W, there exists a T>0 depending only on ˉXW such that the system (18) has a unique solution in C1([0,T],E) with initial data ˉX.

    Proof. To prove the this theorem, the key step is to prove the Lipchitz continuity of the right side of system (18). We define the map ψ:WW

    ψ(X)=(U+V,P1P2,x,Q1Q2,x,M22N22+U2+V22P1,xP2,N22M22+V2+U22Q1,xQ2,(u32uP1,x2uP2+v32vQ1,x2vQ2)|θ0,0).

    Firstly, we testify that Pi, Qi, Pi,x, Qi,x are local Lipchitz continuous. Note that BM = {X=(η,U,V,M,N,σ,h)W| XWM}. Let X = (η,U,V,M,N,σ,h) and ˉX = (ˉη,ˉU,ˉV,ˉM,ˉN,ˉσ,ˉh) belong to BM. Then, we get that

    yL=Id+ηL1+CηH11+CM

    and ˉyL 1+CM. It is clear that coshx and sinhx are local Lipchitz continuous on {XR| |X|1+CM} where C is a constant that depends only on M, we yield

    |cosh(y(θ)y(θ))cosh(ˉy(θ)ˉy(θ))|C|y(θ)y(θ)ˉy(θ)+ˉy(θ)|CηˉηL,

    and

    |exp(sgn(θθ)(y(θ)y(θ))exp(sgn(θθ)(ˉy(θ)ˉy(θ))|CηˉηL,

    for all θ, θ in [0, 1]. Then, we have

    cosh(y(θ)y(θ))((Hθ+(U2+2MNN2)yθ))cosh(ˉy(θ)ˉy(θ))(¯Hθ+(ˉU2+2ˉMˉNˉN2)ˉyθ)LC(ηˉηL+UˉUL+VˉVL+MˉML2+NˉNL2+ηθ¯ηθL2+σθˉσθL2+|hˉh|)CXˉXW.

    So does exp(sgn(θθ)(y(θ)y(θ)))[Hθ+(U2+2MNN2)yθ]. Thus, we obtain that

    P2ˉP2LCXˉXW.

    The similar computation shows that

    P2,xˉP2,xLCXˉXW.

    Utilizing (15), we have

    P2,xθˉP2,xθL2C(XˉXW+P2ˉP2L)CXˉXW,

    and

    P2ˉP2L2C(XˉXW.

    In conclusion, the local Lipchitz continuity from W to H1per of P2 and P2,x has been proven, and so do P1, P1,x, Q1, Q1,x, Q2 and Q2,x. For above certify, it is easy to prove that ψ is locally Lipchitz continuous from W to W. Therefore, the theorem follows the standard theory of ordinary differential equations on Banach spaces.

    Now, we prove the existence of a global solution of system (18). As we all know that initial data is very significant to system (18), but, here, we will only consider a particular initial data that belong to

    W1=W1,per×W1,per×W1,per×Lper×W1,per×R.

    W1 is complete subspace of W. Let ˉXW1. We investigate the short time solution X = (η,U,V,M,N,σ, h) ([0,T],E) of system (18) given by Theorem 3.2. Because XC([0,T],W), Pi, Qi, Pi,x, Qi,x C([0,T],W), we now consider U, V, Pi, Qi, Pi,x, Qi,x as functions in C([0,T],H1per) and M,N in C([0,T],Lper). Then, for any fixed θ in R, we can solve the following system of ordinary differential equations in R4 given by

    {tα(t,θ)=β(t,θ)+γ(t,θ),tβ(t,θ)=ˉh+δ(t,θ)2+(U22+MNN2P1,xP2)(1+α(t,θ)),tγ(t,θ)=ˉh+δ(t,θ)2+(V22+MNM2Q1,xQ2)(1+α(t,θ)),tδ(t,θ)=(3U22P22P1,x+2V2)β(t,θ)+(3V22Q22Q1,x+2U2)γ(t,θ)2(UP2,x+UP1+VQ2,x+VQ1)(1+δ(t,θ)). (19)

    which is obtained by substituting ηθ,Uθ,Vθ and σθ in system (17) by α, β, γ and δ, respectively. We also replaced h(t) by h, hence h(t)=h for all t. Let

    S={θR||ˉUθ(θ)|ˉUθ(θ)L,|ˉVθ(θ)|ˉvθ(θ)L,|ˉηθ(θ)|ˉηθ(θ)L,
    |ˉσθ(θ)|ˉσθ(θ)L}.

    It is not very hard to check that meas(Sc)=0. For all θS, let

    (α(0,θ),β(0,θ),γ(0,θ),δ(0,θ))=(ˉηθ(θ),ˉUθ(θ),ˉvθ(θ),ˉσθ(θ)).

    For θSc, we take (α(0,θ),β(0,θ),γ(0,θ),δ(0,θ))=(0,0,0,0).

    Lemma 3.3. Given initial data

    ˉX=(ˉη,ˉU,ˉV,ˉM,ˉN,ˉσ,ˉh)[W1,per]3×[Lper]2×W1,per×R.

    Let X=(η,U,V,M,N,σ,h)C([0,T],W) be the solution of system (18) followed Theorem 3.2. Then

    XC1([0,T],[W1,per]3×[Lper]2×W1,per×R),

    and the functions α(t,θ),β(t,θ),γ(t,θ),δ(t,θ), which solve system (19) for any fixed θ with the specified initial data above, coincide for almost every θ and for all time with (ηθ,Uθ,Vθ,σθ), that is, for all t[0,T], for almost every θ,

    (α(t,θ),β(t,θ),γ(t,θ),δ(t,θ))=(ηθ(t,θ),Uθ(t,θ),Vθ(t,θ),σθ(t,θ)). (20)

    Proof. Firstly, let's introduce a key space Bper in which elements are bounded periodic functions with the norm fBper = supθ[0,1]|f(θ)|, clearly, this space is complete. According to the initial data conditions in the lemma, the solution for system (19) in space [Bper]4 can be defined as (α(t,θ),β(t,θ),γ(t, θ), δ(t,θ)). It is not very difficult to check that the solutions exists on the interval [0, T] on which (η,U,V,M,N,σ,h) is defined, since the system (19) is linear in (α,β,γ,δ). According system (18), we get that

    {ηθ(t,θ)=ˉηθ+t0(Uθ(τ,θ)+Vθ(τ,θ))dτ,Uθ(t,θ)=ˉUθ+t0(12(ˉh+δ(τ,θ))+(U22+MNN2P1,xP2)(1+α(τ,θ)))dτ,Vθ(t,θ)=ˉVθ+t0(12(ˉh+δ(τ,θ))+(V22+MNM2Q1,xQ2)(1+α(τ,θ)))dτ,σθ(t,θ)=ˉσθ+t0((3U22P22P1,x+2V2)β(τ,θ)+(3V22Q22Q1,x+2U2)γ(τ,θ)2(UP2,x+UP1+VQ2,x+VQ1)(1+δ(τ,θ)))dτ. (21)

    Since Bper imbeds in L2per, the integral form of system (19) holds in L2per sense. Now, we know that (α,β,γ,δ) and (ηθ,Uθ,Vθ,σθ) satisfy the linear system (19) with the same initial data in L2 sense on the interval [0,T]. By uniqueness, we get that

    (α(t),β(t),γ(t),δ(t))=(ηθ(t),Uθ(t),Vθ(t),σθ(t))

    in L2per on [0,T].

    Now, we give the initial data as follow

    {ˉU(θ)=ˉuˉy(θ),    ˉV(θ)=ˉvˉy(θ),ˉM(θ)=ˉuxˉy(θ),  ˉN(θ)=ˉvxˉy(θ),ˉH(θ)=ˉy(θ)0(ˉu2+ˉu2x+ˉv2+ˉv2x)dx,ˉy(θ)0(ˉu2+ˉu2x+ˉv2+ˉv2x)dx+ˉy(θ)=(1+ˉh)θ, (22)

    where ˉh=10(ˉu2+ˉu2x+ˉv2+ˉv2x)dx. By (22), we know that ˉy(θ) is continuous, strictly increasing. In the following work, we will testify that (ˉyId,ˉU,ˉV,ˉm,ˉN,ˉHˉhId,ˉh) belongs to G which is defined as follows.

    Definition 3.4. The set G is made up of all (η,U,V,M,N,σ,h)W such that

    {(η,U,V,M,N,σ,h)[W1,per]3×[Lper]2×W1,per×R,yθ0,Hθ0,yθ+Hθ0almost everywhere,yθHθ=U2y2θ+U2θ+V2y2θ+V2θalmost everywhere, (23)

    where y=η(θ)+θ, H(θ)=σ(θ)+hθ.

    We know that the initial data (ˉη,ˉU,ˉV,ˉM,ˉN,ˉσ,ˉh) belongs to G. We will certify that the solution of system (18) exists globally in time with any initial data in G.

    Lemma 3.5. Given the initial data ˉX=(ˉη,ˉU,ˉV,ˉM,ˉN,ˉσ,ˉh) in G. Let

    X(t)=(η(t),U(t),V(t),M(t),N(t),σ(t),h(t))

    be the local solution of system (18) in C([0,T],W) for some T>0, with the above initial data. Then

    (i) X(t) belongs to G for all t[0,T];

    (ii) almost every t[0,T], yθ(t,θ)>0 for almost every θ.

    Proof. (ⅰ) We continue to use S defined above. Therefore, from Lemma 3.3, the first one of (23) holds for all t[0,T] and XC1([0,T],W). We will prove that the second and third inequality of (23) hold for all θS. Fixed θS and dropped it in the notation without ambiguity. By system (17), we get

    (yθHθ)t=yθtHθ+yθHθt=(Uθ+Vθ)Hθ+yθ[(3U22P22P1,x+2V2)Uθ+(3V22Q22Q1,x+2U2)Vθ2(UP2,x+UP1+VQ2,x+VQ1)yθ],

    and on the other hand,

    (U2y2θ+U2θ+V2y2θ+V2θ)t=2UUtyθ+2U2yθyθt+2UθUθt+2VVtyθ+2V2yθyθt+2VθVθt=(Uθ+Vθ)Hθ+yθ[(3U22P22P1,x+2V2)Uθ+(3V22Q22Q1,x+2U2)Vθ2(UP2,x+UP1+VQ2,x+VQ1)yθ].

    It is not very difficult to check that (Myθ)t=(Uθ)t, ˉMˉyθ=ˉUθ, (Nyθ)t=(Vθ)t and ˉNˉyθ=ˉVθ. We can get that M(t,θ)yθ(t,θ)=Vθ(t,θ) for t[0,T], since the uniqueness of ordinary differential equation. Thus, (23) is defined. Now, we define t as follow

    t=sup{t[0.T]|yθ(t)0 for all t[0,t]}.

    If tT, we obtain

    yθ(t)=0

    for the continuity of yθ(t) on time. From (23), we get that Uθ(t)=Vθ(t)=0. Then, utilizing (17), we have

    yθt(t)=Uθ(t)+Vθ(t)=0.

    From system (17) and the fact yθ(t)=Uθ(t)+Vθ(t)=0, we can infer

    yθtt(t)=Uθt(t)+Vθt(t)=Hθ(t).

    If Hθ(t)=0, combining with (23), we can deduce that

    yθ(t)=Uθ(t)=Vθ(t)=Hθ(t)=0.

    This is a contradiction to the uniqueness of system (17). If Hθ(t)<0, then yθtt<0. Thus, yθ(t) is the strict maximum. This contradicts the definition of t. Hence Hθ(t)>0 implies that yθ(t) is the strict maximum. This contradicts the fact t<T. Therefore, we get yθ(t)0 for all t[0,T]. Let us certify that Hθ(t)0. This follows from (23) when yθ(t)>0. If yθ(t)=0 then as above, Hθ(t)<0 implies that yθ(t)=0 is the strict maximum. This contradicts the fact yθ(t)0 on [0,T]. Hence Hθ(t)0 on [0,T]. Now we have that yθ(t)+Hθ(t)0. If the equality holds, it then follows that yθ(t)=Uθ(t)=Vθ(t)=Hθ(t)=0. This contradicts the uniqueness of system (17) for ¯yθ>0.

    (ⅱ) Let

    A={(t,θ)[0,T]×R|yθ(t,θ)=0}.

    Fubini's theorem infers that

    meas(A)=Rmeas(Aθ)dθ=T0meas(At)dθ, (24)

    where

    Aθ={t[0,T]|yθ(t,θ)=0}, At={θR|yθ(t,θ)=0}.

    From the above proof, we know that for θA, the time points t satisfying yθ(t,θ)=0 are isolated. Thus, we have that meas(Aθ)=0. It follows from (24) and meas(Ac)=0 that

    meas(At)=0 for almost every t[0,T].

    We denote by K the set of times such that meas(At)>0, i.e.

    K={tR+|meas((A)t)>0}.

    Then, meas(K)=0. For all tKc, yθ>0 almost everywhere. Therefore, y(t,θ) in strictly increasing and invertible.

    Theorem 3.6. Given any ˉX=(ˉy,ˉU,ˉV,ˉM,ˉN,ˉH)G. Then the system (16) admits a global solution X(t)=(y(t),U(t),V(t),M(t),N(t),h(t)) in C1(R+,W) with the initial data ˉX=(ˉy,ˉU,ˉV,ˉM,ˉN,ˉH) and X(t)G for all tR+. Moreover, by equipping G with the topology inducted by the E-norm then the map D: G×R+G defined as

    Dt(ˉX)=X(t)

    is a continuous semigroup.

    Proof. Let us write (y,U,V,M,N,H) to denote η,U,V,M,N,σ,h with y=η+Id and H=σ+hId. Assuming (η,U,V,M,N,σ,h) be a solution of system (18) in C1(R+,W) with the initial data (ˉη,ˉU,ˉV,ˉM,ˉN,ˉσ,ˉh), we have

    supt[0,T)(η(t,.),U(t,.),V(t,.),M(t,.),N(t,.),σ(t,.),h(t,.))W<. (25)

    It is clear that h(t)=ˉh for all tR+. According to system (16) we get that H(t,0)=0. Because Hθ0, we obtain HLH(t,1)=ˉh. Hence, σL2ˉh, and supt[0,T)σL2ˉh. For θ and θ in [0, 1], we have that |y(θ)y(θ)|1 for yθ0 and y(1)y(0)=1. Thus, we claim that

    U2yθHθ, UθMHθ, V2yθHθ, VθNHθ. (26)

    Indeed, using (23), we obtain that yθ=0 which deduces Uθ=0. Thus, (26) holds if yθ=0. Othetwise, if yθ0, from (23), we have

    U2+U2θyθ+V2+V2θyθ=Hθ (27)

    and

    {UθMU2θyθ+M2yθ, UθNV2θyθ+N2yθ,VθNV2θyθ+N2yθ, VθMU2θyθ+M2yθ. (28)

    Utilizing (27)-(28), we get (26). From (13)-(22), we have that

    supt[0,T]ρiLCˉh, supt[0,T]ρi,xLCˉh,

    where the constant C is independent of t and the initial data. From system (18), we have following estimates

    supt[0,T]U(t)L,supt[0,T]V(t)L,supt[0,T]M(t)L,supt[0,T]N(t)L.

    For ηt=U+V, therefore

    supt[0,T]η(t)L.

    Now, we have certified that

    C1=supt[0,T]{U(t)L+V(t)L+M(t)L+N(t)L+ρ1L+ρ1,xL+ρ2L+ρ2,xL+ρ3L+ρ3,xL+ρ4L+ρ4,xL}

    is finite. Let

    Z(t)=yθ(t)L2+Uθ(t)L2+Vθ(t)L2+Hθ(t)L2.

    Since the system (17) is semilinear, we have that

    Z(t)=Z(0)+Ct0Z(τ)dτ,

    where C is only depend on C1. Applying Gronwall's inequality, we get (25). By the standard theorem of ordinary differential equation, we obtain that Dt is a continuous semigroup.

    In this section, we will investigate how to obtain a global conservative solution of system (4) from the global solution of system (17) with the initial variables (t,x). Let (y,U,V,M,N,H) be the global solution of system (17). Note that

    u(t,x)u(t,θ), v(t,θ)v(t,θ),  if y(t,θ)=x. (29)

    Theorem 4.1. Let (y,U,V,M,N,H) be a global solution of system (17). Then the pair function (u(t, x), v(t,x)) defined by (29) is the global solution to the system (4). Moreover, this solution (u,v) satisfies the following property:

    u(t,)2H1+v(t,)2H1=u(0,)2H1+v(0,)2H1,  a.e. t0. (30)

    Furthermore, let (ˉun,ˉvn) be a sequence of the initial data such that

    ˉunˉuH10, ˉvnˉvH10.

    Then the corresponding solutions (ˉun,ˉvn) converge to (u(t,x),v(t,x)) uniformly for all (t,x) in any bounded set.

    Proof. Firstly, what we have to do is to show that the definition of u and v make sense. Given x[0,1), if θ1θ2, x=y(t,θ1)=y(t,θ2), then

    yθ(θ)=0 in [θ1,θ2].

    We can obtain that Uθ=Vθ=0 in [θ1,θ2]. Therefore, U(θ1)=U(θ2), V(θ1)=V(θ2), and we can get that (u(t,x),v(t,x)) from the above definition is meaningful. It is clear that u(x+1)=u(x) and v(x+1)=v(x). Now we will certify uH1. Obviously, uL, which yields uL2. So does v. Next, we will show that ux,vxL2. From (23), we have

    10u2xdx=y1(1)y1(0)u2x(t,y(θ))yθdθ=10u2x(t,y(θ))yθdθ=θ[0,1]|yθUθyθdθ(H(1)H(0))=ˉh.

    It is similar to vx. Now, we testify the pair function (u,v) satisfied (4). Given ϕC(R+×R) with compact support. Let (y,U,V,M,N,H) be the solution of system (16), then

    R+×R[(u+v)ϕt+(u+v)(ux+vx)ϕ(t,x)]dxdt  =R+×R[(U+V)yθϕt+(U+V)(Uθ+Vθ)ϕ(t,Y)]dθdt. (31)

    Utilizing yt=U+V and yθt=Uθ=Vθ, we get

    [(U+V)yθϕy]t[(U+V)2]θ=(Ut+Vt)yθϕy+(U+V)yθϕ(U+V)(Uθ+Vθ)ϕ. (32)

    Integrating (32) over R+×R, using (23) and taking x=y(t,θ), we have that

    R+×R[(U+V)yθϕt+(U+V)(Uθ+Vθ)ϕ(t,Y)]dθdt=R+×R(Ut+Vt)yθyθϕdθdt=R+×R(P1P2,xQ1Q2,x)ϕ(t,x)dxdt=R+×R(P1P2,xQ1Q2,x)yθ(t,θ)ϕ(t,y(t,θ))dθdt. (33)

    By (31)-(33), we obtain the first two equation of system (4). When tKc, we have yθ(t,θ)>0 a.e. Utilizing (23), we obtain

    Hθ=U2yθ+Uθyθ+V2yθ+Vθyθ

    holds almost everywhere. By taking x=y(t,θ), we have

    10(u2(t,x)+u2x(t,x)+v2(t,x)+v2x(t,x))dx =10(u2(0,x)+u2x(0,x)+v2(0,x)+v2x(0,x))dx.

    Therefore, we get (30).

    Finally, let (ˉun,ˉvn) converge to (ˉu,ˉv) in H1×H1. From (22), it is not very hard to check that

    ˉynˉyL0, ˉUnˉUL0, ˉVnˉVL0,ˉHnˉHL0, ˉhnˉhL0.

    Now, we certify that

    ˉynθˉyθL20, ˉUnθˉUθL20, ˉVnθˉVθL20,ˉMnˉML20, ˉNnˉNL20.

    Let gn=u2n+u2nx+v2n+v2nx and g=u2+u2x+v2+v2x. From (22), we have that

    (1+h)(ˉyθˉynθ)=(gnyngy)ynθyθ+(hhn)yθ. (34)

    The first item on the right side of (34) can be written as follow

    (gnyngy)ynθyθ=(gnyngyn)ynθyθ+(gyngy)ynθyθ.

    Because 0yθ1+h, it follows that

    10|(gnyngy)ynθyθ|dθ(1+h)gngL1.

    Note that gL1. For any ε0, there exists a continuous function r such that gvL1ε. Then

    10|gygyn|ynθyθdθ10(|gyry|+|ryryn|)ynθyθdθ+10|ryngyn|ynθyθdθ.

    The first and third item tend to zero for the boundedness of ynθ,yθ and the arbitrariness of ε. The second item tends to zero by utilizing the dominated convergence theorem. Hence ˉynθˉyθ in L1. We finally obtain that ˉynθˉyθ in L2, because ynθ is bounded in L. From (22), we get ˉHnθˉHθ in L2,

    ˉMnˉM=ˉunxynˉuxy=ˉunxynˉuxyn+ˉuxynˉuxy.

    For ˉunxˉux in L, we know that

    10|ˉunxynˉuxyn|2dθˉunxˉux2L0.

    Given any ε>0, there exists a continuous function r(θ) such that

    10|ˉuxyr|2dθε. (35)

    Then

    ˉunxynˉuxy=ˉunxyy1ynˉuxy=ˉunxyy1ynry1yn+ry1ynr+rˉuxy.

    Utilizing (35), we have

    10|ˉuxyy1ynry1yn|2dθε,

    and

    10|rˉuxy|2dθε.

    According to dominated convergence theorem, we get

    10|ry1ynr|2dθ0.

    Thus, we have ˉMnˉM in L2. Similarly, ˉNnˉN in L2.

    According to (23), ˉUnˉUL0, ˉVnˉVL0, with MnM, ynθyθ in L2, we get UnθL2UθL2. So does VnθL2VθL2. What we only need to do to prove UnθUθ and VnθNθ in L2 is to show that for any continuous function Ψ with compact support, we have

    RUnθΨdθ=RunxynynθΨdθ=RunxΨy1ndx.

    Thus,

    limnRUnθΨdθ=RuxΨy1ndx=RUθΨdθ.

    Then, we obtain UnθUθ in L2. With the same calculation we have VnθVθ in L2. Now we have

    {yny in H1,UnU in H1,VnV in H1,HnH in H1,MnM in L2,NnN in L2. (36)

    Combining (16)-(17) and (36), we get

    ddt(Un(t)U(t)L+Vn(t)V(t)L+yn(t)y(t)L+Mn(t)M(t)L2+Nn(t)N(t)L2+Unθ(t)Uθ(t)L2+Vnθ(t)Vθ(t)L2+Hnθ(t)Hθ(t)L2+ynθ(t)yθ(t)L2)C(Un(t)U(t)L+Vn(t)V(t)L+yn(t)y(t)L+Mn(t)M(t)L2+Nn(t)N(t)L2+Unθ(t)Uθ(t)L2+Vnθ(t)Vθ(t)L2+Hnθ(t)Hθ(t)L2+ynθ(t)yθ(t)L2).

    According to Gronwall's inequality, we conclude that yny, UnU and VnV in L on any bounded time interval. This yields that

    un(t,x)u(t,x), vn(t,x)v(t,x),

    are uniformly Hölder continuous on any bounded time interval.

    Lastly, we shall certify that the solutions obtained in Theorem 4.1 construct a semigroup.

    Theorem 4.2. Given initial data (ˉu,ˉv)H1per×H1per. Let (u(t),v(t))=Ft(ˉu,ˉv) be the corresponding global solution of system (4) constructed in Theorem 4.1. Then the map F:H1per×H1per×[0,]H1per×H1per is semigroup.

    Proof. Fix (ˉu,ˉv)H1per×H1per and τ>0. For every t>0, what we need to do is prove

    Ft(Fτ(ˉu,ˉv))=Fτ+t(ˉu,ˉv).

    Let (y(τ,θ), U(τ,θ), V(τ,θ), M(τ,θ), N(τ,θ), H(τ,θ)) be the solution of system (16) with the initial data given by (22). For any time τ, we have the new initial data as follows

    ˆy(θ)0(u2+u2x+v2+v2x)dx+ˆy(θ)=(1+ˉh)θ, (37)

    and

    {ˆH(θ)=ˆy(θ)0(u2+u2x+v2+v2x)dx,ˆU(θ)=u(t,ˆy(t,θ)),  ˆV(θ)=v(t,ˆy(t,θ)),ˆM(θ)=ux(t,ˆy(t,θ)),ˆN(θ)=vx(t,ˆy(t,θ)). (38)

    Let (ˆy(t+τ,θ),ˆU(t+τ,θ),ˆV(t+τ,θ),ˆM(t+τ,θ),ˆN(t+τ,θ),ˆH(t+τ,θ)) be a solution of the system (16) with the initial data (37)-(38). We claim that

    (y(t+τ,θ),U(t+τ,θ),V(t+τ,θ),M(t+τ,θ),N(t+τ,θ),H(t+τ,θ))=(ˆy(t+τ,˜θ),ˆU(t+τ,˜θ),ˆV(t+τ,˜θ),ˆM(t+τ,˜θ),ˆN(t+τ,˜θ),ˆH(t+τ,˜θ)),

    where ˜θ is defined as ˆy(τ+t,˜θ)=y(τ+t,θ).

    Actually, the equality ˆy(τ+t,˜θ)=y(τ+t,θ) yields that

    ˆyθ(τ+t,˜θ)dθ=yθ(τ+t,θ)dθ. (39)

    Utilizing (39), we claim that

    Qi(τ+t,˜θ)=Qi(τ+t,θ(˜θ)), Qi,x(τ+t,˜θ)=Qi,x(τ+t,θ(˜θ)), i=1,2.

    For Pi,Pi,x(i = 1, 2), we can get the similar results. At the time τ, y(τ,θ)=ˆy(τ,ˆθ) implies that

    (y(τ,θ(ˆθ)),U(τ,θ(ˆθ)),V(τ,θ(ˆθ)),M(τ,θ(ˆθ)),N(τ,θ(ˆθ)),H(t+τ,θ))=(ˆy(τ,˜θ),ˆU(τ,˜θ),ˆV(τ,˜θ),ˆM(τ,˜θ),ˆN(τ,˜θ),ˆH(τ,˜θ)).

    Therefore, we get that (y(τ,θ(ˆθ)),U(τ,θ(ˆθ)),V(τ,θ(ˆθ)),M(τ,θ(ˆθ)),N(τ,θ(ˆθ)), H(t+τ,θ)) is a solution of system (16). Utilizing (29) and ˆy(τ+t,˜θ)=y(τ+t,θ), we obtain that the solution of the system (4) constructs a semigroup.

    The authors are very grateful to the anonymous reviewers and editors for their careful reading and useful suggestions, which greatly improved the presentation of the paper.

    The first author Chen is partially supported by Science and Technology Research Program of Chongqing Municipal Educational Commission. The third author Zhang is partially supported by the National Social Science Fund of China (No.19BJY077, No.18BJY093 and No.17CJY031), the National Natural Science Foud of China (No.71901044), Chongqing Social Science Planning Project (No.2018PY74), Science and Technology Project of Chongqing Education Commission(No.KJQN20180051 and No.KJQN201900537).



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    1. Byungsoo Moon, Orbital stability of periodic peakons for the generalized modified Camassa-Holm equation, 2021, 14, 1937-1632, 4409, 10.3934/dcdss.2021123
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