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Global existence of weak solutions to a class of higher-order nonlinear evolution equations

  • This paper deals with the initial boundary value problem for a class of n-dimensional higher-order nonlinear evolution equations that come from the viscoelastic mechanics and have no positive definite energy. Through the analysis of functionals containing higher-order energy of motion, a modified potential well with positive depth is constructed. Then, using the potential well method, and Galerkin method, it has been shown that when the initial data starts from the stable set, there exists a global weak solution to such an evolution problem.

    Citation: Li-ming Xiao, Cao Luo, Jie Liu. Global existence of weak solutions to a class of higher-order nonlinear evolution equations[J]. Electronic Research Archive, 2024, 32(9): 5357-5376. doi: 10.3934/era.2024248

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  • This paper deals with the initial boundary value problem for a class of n-dimensional higher-order nonlinear evolution equations that come from the viscoelastic mechanics and have no positive definite energy. Through the analysis of functionals containing higher-order energy of motion, a modified potential well with positive depth is constructed. Then, using the potential well method, and Galerkin method, it has been shown that when the initial data starts from the stable set, there exists a global weak solution to such an evolution problem.



    In this paper, we study the following initial boundary value problem for n-dimensional higher-order nonlinear wave equations with dispersive and dissipative terms:

    utt(x,t)+ut(x,t)+(1)KΔKu(x,t)+(1)KΔKut(x,t)+(1)KΔKutt(x,t)=f(u(x,t)),(x,t)U×[0,T), (1.1)
    u(x,0)=u0(x), ut(x,0)=u1(x),xU, (1.2)
    Dαu(x,t)=0 for any 0|α|K1,(x,t)U×[0,T), (1.3)

    where URn is a bounded domain with sufficiently smooth boundary U, K=1,2,3,, Dα=|α|xα11xα22xαnn means multi-index derivative operator, α=(α1,α2,,αn) is multi-index of nonnegative integers αi(i=1,2,,n), |α|=α1+α2++αn,u0(x)HK0(U) and u1(x)HK0(U). Moreover,

    f(u)=|u|p1u (1.4)

    with p>1 satisfying:

    1<p<+ when Kn2;  1<pnn2K when K<n2. (1.5)

    Problems (1.1)–(1.3) come from viscoelastic mechanics. As K=1, the nonlinear evolution equation

    uttuxxuxxtt=f(u)

    describes the propagation of longitudinal strain waves in a slender elastic rod [1,2]. Similar equations containing a strong damping term uxxt appear in the framework of the Mooney–Rivlin viscoelastic solids of second grade (see [3]). Concerning the higher-dimensional equation

    uttΔuΔutΔutt=f(u),  xU,  t>0, (1.6)

    a unique existence result of a global strong solution for the initial boundary problem of Eq (1.6) was proved in [4] under some assumptions on f(u) for the positive definite energy. Xu et al. [5] also proved that the global strong solution of Eq (1.6) decays to zero exponentially as the time approaches infinity by using the multiplier method for the positive definite energy.

    In [6], Gazzola and Squassina considered the initial boundary value problem of the following equation with both strong and weak damping terms

    uttΔuωΔut+μut=|u|p2u  in  U×(0,T), (1.7)

    where T>0,ω0 and μ>ωλ1 (λ1 is the first eigenvalue of the operator Δ under homogeneous Dirichlet boundary condition). They got the global existence of solutions with initial data in the potential well, which was first introduced by Sattinger (see [7]). Moreover, they proved the finite time blow up for solutions starting in the unstable set and constructed the high energy initial data for which the solution blows up. In [8], Lian and Xu also obtained the global well-posedness of equation uttΔuωΔut+μut=uln|u|.

    In [9], Xu and Yang studied the following nonlinear wave equation with dispersive–dissipative terms and weak damping

    uttΔuΔutΔutt+ut=|u|p1u. (1.8)

    Using the technique of [6] and the concavity method, Xu and Yang derived a sufficient condition on the initial data with arbitrarily positive initial energy such that the corresponding local solution of Eq (1.8) blows up in a finite time. However, the global existence of weak solutions and strong solutions for Eq (1.8) is still open.

    As K=2, Eq (1.1) represents the elastic plate equation with dispersive and dissipative effects [10,11]. In [12], Xu et al. studied the global well-posedness of the initial boundary value problem for a class of fourth-order wave equations with a nonlinear damping term and a nonlinear source term, which was introduced to describe the dynamics of a suspension bridge. By the potential well method, in [13] Lin et al. derived global weak solutions and global strong solutions of the initial boundary value problem for a class of damped nonlinear evolutional equations

    uttΔu+Δ2uαΔut=f(u), xU,t>0.

    Up to now, there is no result on the existence of global solutions to the initial boundary value problem for the nonlinear wave equation, including dispersive term utt, dissipative term ut and ut.

    Fourth-order equation models with the main part utt+Δ2u+ containing weak and strong damping terms such as ut,f(ut),Δut and nonlinear strain ni=1xiσi(uxi) also attract a lot of attention (see [14,15,16,17,18]). A recent work by Lian et al. (see [19]) considered the solutions of the following equation

    utt+Δ2uΔu+ni=1xiσi(uxi)Δut+|ut|r1ut=f(u),  (x,t)U×(0,). (1.9)

    The global existence, asymptotic behavior, and blow-up of solutions for subcritical initial energy and critical initial energy of Eq (1.9) were obtained, and the blow-up of solutions in finite time for the positive initial energy case was also proved.

    As K>2, Problems (1.1)–(1.3) also appear in physics. For example, when n=2 and K=4, Eq (1.1) can represent the model of two-dimensional quasicrystal elasticity with dispersive and dissipative effect; when n=3 and K=6, Eq (1.1) represents the model of three-dimensional quasicrystal elasticity with dispersive and dissipative effect (see [20]). As mentioned above, Eq (1.1) has an important physical background, while the mathematical achievements for the arbitrary higher order wave equation with both dispersive and dissipative terms (for any positive integer K1) are scarce. So the aim of the present paper is to establish a global existence result of weak solutions to such an evolution problem.

    Motivated by previous papers [6,8,13], we shall use the potential well theory to establish conditions under which the initial boundary value problems (1.1)–(1.3) have global weak solutions. This method proposed by Sattinger (see [7,21]) and its improvements (see [22,23,24,25]) allow us to consider the hyperbolic equations without positive definite energy. For example, concerning about Eq (1.7) in [6], in the framework of the potential well method, a Nehari manifold N, a stable set W (potential well) and an unstable set V (outside the potential well), should be introduced, and the mountain pass energy level d (also known as potential well depth) can be characterized as

    d=infuN(12u21p+1up+1p+1).

    However, when dealing with the present models with higher-order dispersive term ΔKutt, higher-order energy of motion KutL2(U) should be contained in energy functionals. This work brings complicated construction of potential well W, and consequently a detailed computational formula of the modified potential well depth d is needed.

    Therefore, in Section 2, we present some notations and definitions for the energy functionals, modified potential well W, and modified potential well depth d. Then we concentrate on the detailed equivalent definition of d and prove that d>0.

    In Section 3, using the potential well method and Galerkin method, we construct a global weak solution to the evolution Problems (1.1)–(1.3) when the initial data stars from stable set W.

    There are also interesting problems for further studies.

    1) As K=1, the blow-up property of corresponding local solution, has been derived in [12], whereas the uniqueness of solution, vacuum isolation of solutions and decay or blow-up properties of solutions are still open for dispersive–dissipative models with any arbitrary higher-order K.

    2) The Cauchy problem of such kinds of higher-order evolution equations has not been of concerned so far.

    3) It is well worth considering some important physical properties and physical structures in numerical analysis, such as positivity preservation, maximum principle [26], long-term behavior [27], and singular solutions.

    Let us give some explanations for constraint (1.5) of exponent p. Note that 2=2nn2K is the critical Sobolev exponent for q in the embedding HK0(U)Lq(U) (see [28]); it follows from (1.5) that HK0(U)Lp+1(U), hence the following functionals I(u),J(u), and E(t) introduced in (2.1),(2.2), and (2.4) should be well defined. Furthermore, by assumption (1.5), we can control the L2 norm of the nonlinear term (1.4) by using Sobolev embedding HK0(U)L2p(U). It will lead to global existence results for the nonlinear ordinary differential systems (3.7) and (3.8) associated to Problems (1.1)–(1.3) when the Galerkin method is applied.

    We denote by q the Lq(U) norm for 1q, by the L2(U) norm, and by k,p the Wk,p(U) norm. Let

    Z={u(x,t) in L(0,T;HK0(U)) and ut(x,t) in L(0,T;HK0(U))}.

    For any 0<t<T, we define functionals I,J:ZR by

    I(u)=Ku2+Kut2up+1p+1,   p>1 (2.1)

    and

    J(u)=12Ku2+12Kut21p+1up+1p+1,   p>1. (2.2)

    We define the potential well depth (also the mountain pass value of J) as

    d=inf0<t<T,uZ,Ku2+Kut20(supa0J(au)). (2.3)

    The energy functional E:ZR is defined by

    E(u)=12ut2+12Ku2+12Kut(x,t)2ΩF(u(x,t))dx, (2.4)

    where F(u)=u0f(s)ds.

    We introduce the modified Nehari manifold (for Nehari manifold we refer to [29] and [30]) as

    N={uZ|I(u)=0  and  Ku2+Kut20}.

    Finally, for any 0<t<T the modified potential well is defined as

    W={uZ| I(u)>0,J(u)<d}{0}. (2.5)

    Theorem 2.1. The depth of the potential well (denoted by d in (2.3)) can also be characterized as

    d=inf0<t<T,uNJ(u).

    In order to prove Theorem 2.1, we introduce the following two lemmas.

    Lemma 2.1. If 0<t<T,uZandKu2+Kut20, we have

    (i) Lima+J(au)=, Lima0J(au)=0.

    (ii) There exists a unique positive number ˜a=˜a(u) such that dJ(au)da|a=˜a=0.

    (iii) When a=˜a, d2J(au)da2<0.

    (iv) J(au) increases with a as 0a˜a; J(au) decreases with a as ˜aa<+.

    Proof. (i) is true because

    J(au)=a22Kut2+a22Ku2ap+1p+1up+1p+1,   p>1. (2.6)

    Calculate

    dJ(au)da=aKut2+aKu2apup+1p+1. (2.7)

    Solving dJ(au)da=0, there is an unique solution

    ˜a=(Kut2+Ku2)1p1up+1p1p+1. (2.8)

    (ii) is true as Kut2+Ku20.

    In order to obtain (iii), substitute (2.8) into the expression

    d2J(au)da2=Kut2+Ku2ap1pup+1p+1

    gives

    d2J(au)da2|a=˜a=(Kut2+Ku2)˜ap1(1p)<0.

    At last, from (2.7) and (2.8), we have

    dJ(au)da=up+1p+1a(˜ap1ap1).

    Hence dJ(au)da>0 as 0<a<˜a and dJ(au)da<0 as ˜a<a<+. So (iv) is true.

    Lemma 2.2. If 0<t<T,uZ and Kut2+Ku20, J(αu)=supa0J(au) is equivalent to I(αu)=0.

    Proof. Since

    I(αu)=α2Kut2+α2Ku2αp+1up+1p+1,

    ˜a in (2.8) coincides with the solution to equation I(αu)=0. From Lemma 2.1 (iv), J(αu)=supa0J(au).

    Conversely, if J(αu)=supa0J(au), Lemma 2.1 gives α=˜a in (2.8), then

    I(αu)=˜a2Kut2+˜a2Ku2˜ap+1up+1p+1=0.

    Proof of Theorem 2.1: By Lemma 2.1, the depth of potential well (see (2.3)) should be

    d=inf0<t<T,uZ,Ku2+Kut20(supa0J(au))=inf0<t<T,uZ,Ku2+Kut20J(˜au). (2.9)

    Let w=˜au then from Lemma 2.2 we have d=infJ(w), where the infimum is taken for all t(0,T) and all functions wZ satisfying that I(u) attains 0 on (0,T) with Ku2+Kut20, which means wN.

    The proof of Theorem 2.1 is completed.

    Lemma 2.3. As p>1 satisfies (1.5), a computational formula for the potential well depth is

    d=1κΛκ. (2.10)

    Here

    κ=2(p+1)p1 (2.11)

    and

    Λ2=supt(0,T),uZKut2+Ku20u2p+1Kut2+Ku2. (2.12)

    Moreover,

    d1κSκp+1>0,

    where Sp+1 is the best Sobolev constant for the embedding HK0(U)Lp+1(U), i.e.,

    Sp+1=supuHK0(U){0}up+1Ku.

    Proof. As the process of proof in Theorem 2.1, substituting (2.8) into the computation of J(au) (see (2.6)) we obtain

    J(˜au)=˜a22(|Kut2+Ku2)˜ap+1p+1up+1p+1=˜a22(|Kut2+Ku2)˜a2p+1˜ap1up+1p+1=˜a22(|Kut2+Ku2)˜a2p+1(Kut2+Ku2)up+1p+1up+1p+1=(121p+1)˜a2(Kut2+Ku2)=p12(p+1)(Kut2+Ku2u2p+1)p+1p1.

    Value of κ and Λ in (2.11),(2.12) gives

    sup0<t<T,uZ,Ku2+Kut20(u2p+1Kut2+Ku2)p+1p1=Λ2(p+1)p1=Λκ.

    Therefore

    d=inf0<t<T,uZ,Ku2+Kut20J(˜au)=1sup0<t<T,uZ,Ku2+Kut201J(˜au)=1κΛκ.

    Furthermore,

    Λ2sup0<t<T,uZ,Ku2+Kut20u2p+1Ku2S2p+1.

    It follows that

    d1κSκp+1>0.

    Lemma 2.4. If J(u)d, then I(u)>0 is equivalent to

    0<Kut2+Ku2<Λκ.

    Proof. From (2.1) and (2.2), the following equality holds:

    J(u)=1p+1I(u)+1κ(Kut2+Ku2). (2.13)

    Since d=1κΛκ where κ=2(p+1)p1, for I(u)>0 and J(u)d we have

    0<Kut2+Ku2<Λκ.

    Conversely, if

    Kut2+Ku2<Λκ, (2.14)

    then

    Λκ(Kut2+Ku2)<1.

    By value of Λ in (2.12),

    1>Λκ(p1)2(Kut2+Ku2)p12=Λp+1(Kut2+Ku2)p12up+1p+1(Kut2+Ku2)p+12(Kut2+Ku2)p12=up+1p+1(Kut2+Ku2)1.

    Hence

    up+1p+1<Kut2+Ku2.

    Thus I(u)=Ku2+Kut2up+1p+1>0.

    We denote the inner product in L2(U) by

    (u,v)=Uu(x)v(x)dx. (3.1)

    A continuous linear functional defined on the locally convex linear topological space D(0,T) is called the "distribution" or the "generalized function" (see [31], Chapter 8). We denote the space of generalized functions on (0,T) by D(0,T).

    Definition 3.1. For T>0, if the function u(x,t)Z satisfies:

    1) for any v(x)HK0(U) and for almost t[0,T),

    (ut,v)+t0(Ku,Kv)dτ+(Ku,Kv)+(Kut,Kv)+(u,v)=t0(f(u),v)dτ+(u1,v)+(Ku0,Kv)+(Ku1,Kv)+(u0,v). (3.2)

    2) u(x,0)=u0(x) in HK0(U) and ut(x,0)=u1(x) in L2(U).

    Then we call u=u(x,t) a global weak solution to Problems (1.1)–(1.3).

    For u0HK0(U) and u1HK0(U), we introduce the following initial functionals:

    E(0)=12u1(x)2+12Ku0(x)2+12Ku1(x)2UF(u0(x))dx, (3.3)
    J(0)=12Ku0(x)2+12Ku1(x)21p+1u0(x)p+1p+1, (3.4)
    I(0)=Ku1(x)2+Ku0(x)2u0(x)p+1p+1. (3.5)

    Theorem 3.1. If T>0, f(s)=|s|p1s where p satisfies (1.5) and E(0)<d, there exists a global weak solution to Problems (1.1)–(1.3) as long as I(0)>0, J(0)<d for u0HK0(Ω) and u1HK0(Ω). Moreover, for any 0t<T, uW.

    Let {ωk(x)}(k=1,2,3,) be a complete orthogonal basis in H2K(Ω)HK0(Ω), which solves the following eigenvalue system

    (1)KΔKωk=λkωk, Dαωk|U=0, 0|α|K1.

    It is also a complete orthonormal basis for L2(U) and a complete orthogonal basis for HK0(U). (see [32,33]).

    Based on the Galerkin method, an approximate solution to Problems (1.1)–(1.3) can be constructed by

    um(x,t)=mk=1gkm(t)ωk(x), m=1,2,3,, (3.6)

    where um(x,t) satisfies a system of nonlinear ordinary differential equations

     (ωk,umtt)+(ωk,(1)KΔKum)+(ωk,(1)KΔKumt)+(ωk,(1)KΔKumtt)+(ωk,umt)=(ωk(x),f(um(x,t))) (3.7)

    with initial values

    gkm(0)=akm and gkm(0)=bkm (3.8)

    for k=1,2,,m.

    Since u0(x)HK0(U) and u1(x)HK0(U), when m+ there exist akm and bkm (k=1,2,,m) such that

    um(x,0)=mk=1akmωk(x)u0(x) in HK0(U), (3.9)
    umt(x,0)=mk=1bkmωk(x)u1(x) in HK0(U). (3.10)

    Notice that f(s)=|s|p1s(p>1) is locally Lipschitz continuous with respect to s. According to classical existence theory for nonlinear ordinary differential equations (see [34], corollary 1.1.1), systems (3.7) and (3.8) with initial data satisfying (3.9) and (3.10) have a local solution um(x,t) for each m. In order to extend it to a global solution on [0,T), we will make priori estimates of um(x,t)(m=1,2,).

    Multiplying by gkm(t) on both sides of (3.7) and summing up from k=1 to k=m, we obtain

    (mj=1ωk(x)gkm(t),umtt)+(mk=1ωk(x)gkm(t),(1)KΔKum)+(mk=1ωk(x)gkm(t),(1)KΔKumt)+(mk=1ωk(x)gkm(t),(1)KΔKumtt)+(mk=1ωk(x)gkm(t),umt)=(mk=1ωk(x)gkm(t),f(um)).

    That is,

    (umt,umtt)+(umt,(1)KΔKum)+(umt,(1)KΔKumt)+(umt,(1)KΔKumtt)+(umt,umt)=(umt,f(um)).

    Integrating the above equality by parts with respect to x,

    12ddtumt2+12ddtKum2+Kumt2+12ddtKumt2+umt2(f(um),umt)=0.

    Let F(um)=um0f(s)ds, calculation

    ddtUF(um)dx=UddtF(um)dx=Uf(um)umtdx=(f(um),umt)

    gives that

    ddt(12umt2+12Kum2+12Kumt2UF(um)dx)+Kumt2+umt2=0. (3.11)

    Let Em(t)=E(um), from (2.4) we have

    Em(t)=12umt2+12Kum2+12Kumt2UF(um)dx (3.12)

    and

    Em(0)=12umt(x,0)2+12Kum(x,0)2+12Kumt(x,0)2UF(um(x,0))dx. (3.13)

    Integrating (3.11) with respect to t on (0,t) for 0t<T gives

    Em(t)+t0Kumτ(x,τ)2dτ+t0umτ(x,τ)2dτ=Em(0), 0t<T. (3.14)

    It concludes that

    Em(t)Em(0),0t<T. (3.15)

    First, we claim that there exists N1>0 such that

    I(um)(0)>0 and J(um)(0)<d for all m>N1. (3.16)

    From (3.9), (3.10), and (1.5), using Sobolev imbedding theorem we find Kum(x,0) converges to Ku0(x), um(x,0)p+1p+1 converges to u0(x)p+1p+1 and Kumt(x,0) converges to Ku1(x) as m+. Therefore, when m tends to +,

    I(um)(0)=Kum(x,0)2+Kumt(x,0)2um(x,0)p+1p+1

    converges to I(0) and

    J(um)(0)=12Mum(x,0)2+12Kumt(x,0)21p+1um(x,0)p+1p+1

    converges to J(0).

    Since I(0)>0 and J(0)<d, we conclude that I(um)(0)>0 and J(um)(0)<d for sufficiently large integer m, which implies (3.16).

    Next we prove that UF(um(x,0))dx converges to UF(u0(x))dx when m increases to +.

    By mean value theorem of integral, there exists ξ(m) between u0(x) and um(x,0) such that

    F(um(x,0))F(u0(x))=um(x,0)u0(x)f(s)ds=f(ξ(m))(um(x,0)u0(x)),

    hence

    |U(F(um(x,0))F(u0(x)))dx||ξ(m)|pp+1pum(x,0)u0(x)p+1.

    Under condition (1.5) of p, HK0(U) is embedded in Lp+1(U). Since um(x,0) converges to u0(x) in HK0(U) as m increases to + (see (3.9)), um(x,0)u0(x)p+10 as m+ and |ξ(m)|pp+1p is uniformly bounded for m=1,2,. So we arrive at

    UF(um(x,0))dxUF(u0(x))dx(m+). (3.17)

    By (3.9),(3.10), and (3.17), Em(0) in (3.13) converges to

    12(u12+Ku02+Ku12)UF(u0)dx,

    that is,

    Em(0)E(0),m+. (3.18)

    Since E(0)<d, there exists N2>0 satisfying Em(0)<d for all m>N2.

    Recalling |f(u)|=|u|p, a control of F(u)=u0f(s)ds is

    0F(u)1p+1|u|p+1,

    then

    1p+1U|u|p+1dxUF(u)dx. (3.19)

    Combining with (3.19), it follows from (2.2),(3.12) that

    Em(t)J(um)+12umt2,0t<T.

    Therefore, from (3.14) we have

    Em(0)t0Kumτ(x,τ)2dτ+Em(t)t0Kumτ(x,τ)2dτ+J(um)+12umt2,0t<T. (3.20)

    Hence

    J(um(x,t))<d for all t(0,T) and m>N2. (3.21)

    In what follows, we prove that um(x,t)W for sufficiently large integer m. Set m>max{N1,N2} and T>0, if there exists t0=t0(m)(0,T) such that um(x,t) attains W at t=t0, then I(um)(t0)=0 with Kum(x,t0)+Kumt(x,t0)0 or J(um)(t0)=d.

    Inequality (3.21) means J(um)(t0)=d is impossible; on the other hand, by Theorem 2.1 we find J(um)(t0)d, which also contradicts (3.21). Therefore, when m is large enough and 0<t<T, um(x,t) always stays in W. That is, I(um)>0 and J(um)<d.

    Substituting

    J(um(x,t))=p12(p+1)(Kum2+Kumt2)+1p+1I(um(x,t)) (3.22)

    into (3.20), we obtain

    p12(p+1)(Kum2+Kumt2)+1p+1I(um(x,t))+12umt2<d

    and

    t0Kumτ(x,τ)2dτ<d,0<t<T. (3.23)

    Since I(um)>0, when sufficiently large m we have the estimates

    Kum2+Kumt2<κd (3.24)

    and

    umt2<2d,0<t<T. (3.25)

    Inequality (3.24) shows umHK0(U) and umtHK0(U) are uniformly bounded for m=1,2,. Consequently um and um are also uniformly bounded for m=1,2,.

    From (1.5), the Sobolev space HK0(U) is embedded in Lp+1(U) and L2p(U). Thus ump+1 and f(um)2=um2p2p are also uniformly bounded for m=1,2,.

    When 0<t<T,

    |(ωk(x),f(um))|ωk(x)f(um)=f(um)

    should be uniformly bounded for m=1,2,, where {ωk(x)}+k=1 is a complete orthonormal basis in L2(Ω) with ωi(x)=1 (i=1,2,).

    Now we conclude that there exist global solutions

    gkm(t),k=1,2,3,,m

    to problems (3.7) and (3.8) on [0,T), according to classical theory of nonlinear ordinary differential system (see [34]).

    Let q=p+1p and QT=U×[0,T). It follows from

    |f(u)|q=|u|pq=|u|p+1

    that

    {f(um)}+m=1 is uniformly bounded in L(0,T;Lq(U)). (3.26)

    Furthermore,

    {f(um)}+m=1 is uniformly bounded  in Lq(QT). (3.27)

    By (3.24) there exists a subsequence of {um(x,t)}+m=1 (still denoted by {um(x,t)}+m=1), a function u(x,t) satisfying the following two:

    um(x,t) converges to u(x,t) in L(0,T;HK0(U)) weakly-star as m increases to+, (3.28)
    umt(x,t) converges to ut(x,t) in L(0,T;HK0(U)) weakly-star as m increases to+. (3.29)

    By (3.26), there exists another subsequence of {um(x,t)}+m=1 (still denoted by {um(x,t)}+m=1 again), a function X(x,t) satisfy that

    f(um(x,t)) converges to X(x,t) in L(0,T;Lq(U)) weakly-star as m increases to+. (3.30)

    By (3.25), {um(x,t)}+m=1 is uniformly bounded in H1(QT). Since H1(QT) is compactly imbedded into L2(QT), there exists a subsequence of {um(x,t)}+m=1 (still denoted by {um(x,t)}+m=1) such that

    um(x,t) converges to u(x,t) in L2(QT) as m increases to +,

    and then

    um(x,t) converges to u(x,t) in QT almost everywhere as m increases to +.

    Moreover,

    f(um(x,t)) converges to f(u(x,t)) in QT almost everywhere as m increases to +,

    because f(s)=|s|p1s is continuous.

    On the other hand, f(um(x,t)) is bounded in Lq(QT) from (3.27), according to J. L. Lions' Lemma ([35], Lemma 1.3) we find

    f(um(x,t)) weakly converges to f(u(x,t)) in Lq(QT) as m increases to +. (3.31)

    For 0t<T, integrating by parts with respect to x and integrating with respect to t from 0 to t on both sides of (3.7), we obtain

     (ωk,umt)+t0(Kωk,Kum)dt+(Kωk,Kum)+(Kωk,Kumt,)+(ωk,um)=t0(ωk,f(um),)dt+(ωk,umt(x,0),)+(Kωk(x),Kum(x,0),)                         +(Kωk(x),Kumt(x,0))+(ωk(x),um(x,0)),  k=1,2,3,.

    Let m+, we obtain

     (ωk,ut)+t0(Kωk,Ku)dt+(Kωk,Ku)+(Kωk,Kut)+(ωk,u)=t0(ωk,f(u))dt+(ωk,u1)+(Kωk,Ku0)+(Kωk,Ku1)+(ωk,u0),k=1,2,3,.

    Since {ωk(x)}+k=1 is a complete orthogonal basis in HK0(U), the above equality still holds if we replace ωk by arbitrary vHK0(U).

    According to Lemma 1.2 in [35], it can be deduced from (3.28) and (3.29) that um(x,t)C(0,T;HM0(U)), u(x,t)C(0,T;HK0(U)). Then

    um(x,0)u(x,0) in HK0(U) weakly-star  as m+.

    On the other hand, from (3.9) we see that um(x,0) strongly converges to u0(x) in HK0(U) as m increases to +, so

    u(x,0)=u0(x) in HK0(U).

    Next, we will verify ut(x,0)=u1(x) in L2(U). Integrating by parts with respect to x on both sides of (3.7), we get

     (umtt,ωk)+(Kumtt,Kωk)=(f(um),ωk)(Kum,Kωk)(Kumt,Kωk)(umt,ωk), k=1,2,3,,m. (3.32)

    By (3.28)–(3.30), when m+, for k=1,2,3,,

    (f(um),ωk)(X,ωk) in L(0,T) weakly-star, (3.33)
    (Kum,Kωk)(Ku,Kωk) in L(0,T) weakly-star, (3.34)
    (Kumt,Kωk)(Kut,Kωk) in L(0,T) weakly-star, (3.35)
    (umt,ωk)(ut,ωk) in L(0,T) weakly-star. (3.36)

    So the right side in (3.32) converges to (X,ωk)(Ku,Kωk)(Kut,Kωk)(ut,ωk) in L(0,T) weakly-star as m+, which means that the left side of (3.32) is also convergent in L(0,T) weakly-star.

    Moreover, by (3.36) and (3.35) when m+, for k=1,2,3,

    (umt,ωk)(ut,ωk) in D(0,T)

    and

    (Kumt,Kωk)(Mut,Mωk) in D(0,T).

    Furthermore, when m+, for k=1,2,3,,

    (umtt,ωk)(utt,ωk) in D(0,T)

    and

    (Kumtt,Kωk)(Kutt,Kωk) in D(0,T).

    Hence the left side in (3.32) converges to (utt,ωk)+(Kutt,Kωk) in D(0,T), and then it converges to the same limit in L(0,T) weakly-star by the uniqueness of limit.

    From the above discussions, for k=1,2,

    (ut,ωk)+(Kut,Kωk)L(0,T)

    and

    (utt,ωk)+(Kutt,Kωk)L(0,T).

    Again, using Lemma 1.2 in [35], for k=1,2, we have

    (umt,ωk)+(Kumt,Kωk)C(0,T;R)

    and

    (ut,ωk)+(Kut,Kωk)C(0,T;R).

    Therefore, when m+, for k=1,2,

    (umt(x,0),ωk(x))+(Kumt(x,0),Kωk(x))(ut(x,0),ωk(x))+(Kut(x,0),Kωk(x)).

    On the other hand, from (3.10) when m+, for k=1,2,

    (umt(x,0),ωk(x))+(Kumt(x,0),Kωk(x))(u1,ωk)+(Ku1,Kωk).

    By uniqueness of limit, for k=1,2,

    (ut(x,0),ωk(x))+(Kut(x,0),Kωk(x))=(u1,ωk)+(Ku1,Kωk).

    Integrating by parts with respect to x,

    (ut(x,0),ωk(x))+(ut(x,0),(1)KΔKωk(x))=(u1,ωk)+(u1,(1)KΔKωk),  for k=1,2,.

    It follows that

    (ut(x,0),ωk(x))+(ut(x,0),λkωk(x))=(u1,ωk)+(u1,λkωk)  for k=1,2,.

    Equivalently,

    (1+λk)(ut(x,0)u1(x),ωk(x))=0  for k=1,2,.

    Since all eigenvalues λk>0 (k=1,2,) (see Theorem 7.23 in [32]), there should be

    (ut(x,0)u1(x),ωk(x))=0  for k=1,2,.

    Thus, we have ut(x,0)u1(x)=0 in L2(U), that is, ut(x,0)=u1(x) in L2(U).

    We finally have a global weak solution u(x,t)L(0,T;HK0(U)) with ut(x,t)L(0,T;HK0(U)) to Problems (1.1)–(1.3).

    The process will be an analogue as in Step 2.

    We denote the inner product in L(0,T;L2(U)) by

    [u(,t),v(,t)]=t0(u(,τ),v(,τ))dτ,   0t<T.

    Making an inner product in L2(U) by ut on both sides of (1.1), we obtain

     (ut,utt)+(ut,(1)KΔKu)+(ut,(1)KΔKut)+(ut,(1)KΔKutt)+(ut,ut)=(ut,f(u))   in D(0,T).

    Integrating by parts with respect to x, we obtain

    12ddtut2+ut2+12ddtKu2+Kut2+12ddtKut2=ddtUF(u)dx.

    Integrating with respect to t from 0 to t (0<t<T), we have

    12ut2+[ut,ut]+12Ku2+12Kut2+[Kut,Kut]UF(u)dx=12u1(x)2+12Ku0(x)2+12Ku1(x)2UF(u0)dx.

    That is,

    E(t)+[Kut,Kut]+[ut,ut]=E(0).

    Hence

    E(t)E(0)  for 0t<T.

    Similar to (3.20), by some computations we obtain

    12ut2+J(u)E(t)E(0)  for 0t<T.

    Since E(0)<d,

    J(u)<d  for 0t<T. (3.37)

    If there exists t0(0,T) such that uW for 0t<t0 and u attains W at t=t0, then the nontrivial solution uZ satisfies that J(u)(t0)=d or I(u)(t0)=0 with Kut(x,t0)+Ku(x,t0)0.

    Inequality (3.37) implies that J(u)(t0)=d is impossible. On the other hand, if u(x,t)Z satisfies that I(u)(t0)=0 and Kut(x,t0)+Ku(x,t0)0, that is u(x,t0)N, from Theorem 2.1 we should have that J(u)(t0)d, which is also in contradiction with (3.37). So we conclude that u(x,t)W for 0t<T.

    The proof of Theorem 3.1 is completed.

    The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.

    This work is supported by Teaching Team Project, Guangdong Provincial Department of Education 2018 (No. 99161010120) and Guangdong Provincial NSF under Grants 2018A030313546.

    The authors declare there are no conflicts of interest.



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