Research article Special Issues

Decay estimate and blow-up for fractional Kirchhoff wave equations involving a logarithmic source

  • This paper was dedicated to researching a class of fractional Kirchhoff wave models involving a logarithmic source and strong damping term. We have proven the local existence and uniqueness of weak solutions through combining contraction mapping theory with Faedo-Galerkin's method. Based on the framework of a potential well and under suitable conditions, an exponential decay estimate of global weak solutions was established. Finally, the result of the finite time blow-up was obtained.

    Citation: Aihui Sun, Hui Xu. Decay estimate and blow-up for fractional Kirchhoff wave equations involving a logarithmic source[J]. AIMS Mathematics, 2025, 10(6): 14032-14054. doi: 10.3934/math.2025631

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  • This paper was dedicated to researching a class of fractional Kirchhoff wave models involving a logarithmic source and strong damping term. We have proven the local existence and uniqueness of weak solutions through combining contraction mapping theory with Faedo-Galerkin's method. Based on the framework of a potential well and under suitable conditions, an exponential decay estimate of global weak solutions was established. Finally, the result of the finite time blow-up was obtained.



    Fractional differential equations can better describe practical problems than classical differential equations. This has attracted the interest and attention of many scholars to the fractional p-Laplacian (Δ)sp [1,2,3,4,5]. The fractional 2-Laplacian operator of the form (Δ)s(p=2) was first mentioned in physics when observing the Levy steady-state diffusion process, and later it was also used to depict abnormal plasma diffusion, fluid dynamics, and stochastic analysis [6,7,8]. Not only for mathematical purposes, but also for their importance in practical models, this paper will investigate the Kirchhoff-type wave models involving logarithmic nonlinearity and the fractional Laplacian operator as follows:

    {utt+M([u]2s)(Δ)su+(Δ)sut=|u|k2uln|u|,xΩ,t>0;%(x,t)Ω×R+;u(x,0)=u0(x),ut(x,0)=u1(x),xΩ;u(x,t)=0,xRNΩ,t0, (1.1)

    where, among them, (Δ)s(s(0,1)) is the fractional Laplacian operator satisfying

    (Δ)su(x)=2limε0+RNBε(x)u(x)u(y)|xy|2s+Ndy.

    The Kirchhoff term M(ψ)=a+ψθ1 is a function that satisfies local Lipschitz continuity, a>0, 1θ<2s2, where

    2s={+,ifN2s,2NN2s,ifN>2s,

    is the critical exponent of the fractional Sobolev embedding inequality. If ψ=ψ(t), we impose the following assumption on M(ψ):

    ddtM[ψ(t)]CM[ψ(t)]. (1.2)

    Moreover, ΩRN(N1) is a bounded domain and the boundary Ω is the smooth and nonlinear index 2θ<k2s.

    Recently, the research on Kirchhoff-type equations [9,10] has received widespread attention. This kind of problem develops a major effect in the applications of nonlinear elasticity, electrorheological fluid, and image restoration [11,12]. It is meaningful to investigate the nonexistence, existence, blow-up, extinction, and decay estimation of its solutions. Kirchhoff [13] first introduced the following equation:

    ρhutt+δut={P0+Eh2LL0(ux(x,t))2dx}2ux2+f,t0,0xL,

    where u denotes lateral displacement, δ denotes the resistance modulus, ρ denotes mass density, h represents the cross-section area, P0 denotes initial axial tension, L is the length, E is Young's modulus, and f represents external force. Since then, many researchers have become concerned with this kind of equation and have had excellent research results. In particular, many literatures have been devoted to discussing the Kirchhoff equation as follows:

    utt+g(ut)M(u2)Δu=f(u), (1.3)

    where f(u) is a nonlinear function that satisfies appropriate conditions and M0 is a local Lipschitz function. When g(ut)=Δut, Wu and Tsai [14] made a profound study for Problem (1.3), where they found the upper bound of the blow-up time of solutions by the direct energy method. Yang and Han [15] also discussed Problem (1.3), through the Banach fixed point theorem, where they proved uniqueness as well as local existence of weak solutions. Then, through constructing a potential well, the lifespan of solutions with arbitrary initial energy was established. When g(ut) is the non-linear dissipation term |ut|m1ut or the linear dissipation term ut, Ono studied Problem (1.3) involving f(u)=|u|pu in [16,17], when the initial energy is negative, and proved the finite time blow-up. In addition, when the initial energy was positive, he provided sufficient conditions for the finite time blow-up of the solutions. More research on the problems of Kirchhoff-type can be found in references [18,19,20,21,22].

    In 2017, Pan et al. [23] investigated the degenerate fractional Kirchhoff-type hyperbolic problems as follows:

    utt+[u]2(θ1)s(Δ)su=|u|p1u.

    Combining the potential wells theorem with the Galerkin method, they proved the global existence. Moreover, the vacuum isolating phenomenon and blow-up properties also were acquired. Additionally, the study of logarithmic source has a long history, appearing in different modules of physics [24].

    Inspired by the above works, we investigate Problem (1.1) involving the fractional the Laplacian operator strong damping and logarithmic source, which is the first work that takes into account the blow-up property and decay estimate of weak solutions of Problem (1.1). We not only overcome the difficulty of logarithmic nonlinearity, but also deal with the fractional Laplacian operator. This work is extremely meaningful.

    The structure of this article is as follows: In Section 2, we introduce important lemmas and basic definitions. In addition, potential wells and their properties are provided. Next, the local existence and uniqueness of the weak solutions are proved. Then we gain the global existence of weak solutions and establish an exponential decay estimate in Section 4. Finally, the finite time blow-up of the solutions is obtained.

    We introduce some symbols, lemmas, and basic definitions in this section. For convenience, we define the Lk(Ω) norm through k(1k). First, some definitions of Sobolev space are reviewed, which can be found in [25].

    Let the fractional exponent s(0,1), Hs(RN) be the fractional Sobolev space satisfying

    Hs(RN)={uL2(RN):u(x)u(y)|xy|s+N2L2(RN×RN)} (2.1)

    equipped with the norm

    uHs(RN)=(RN×RN|u(x)u(y)|2|xy|2s+Ndxdy+u2L2(RN))12. (2.2)

    We denote space O=C(Ω)×C(Ω)RN where C(Ω)=RNΩ, and then denote Q=(RN×RN)O. From nonlocal characteristics, we define the space

    W={uL2(RN):Q|u(x)u(y)|2|xy|2s+Ndxdy<}. (2.3)

    Let W0={uW:u(x,t)=0,xC(Ω)}, which is a closed linear space, and W0W. Moreover, [u]s is the Gagliardo seminorm satisfying

    [u]s=(Q|u(x)u(y)|2|xy|2s+Ndxdy)12. (2.4)

    From the results of [26], it can be concluded that [u]s is equivalent to the norm of W0, and it is clear that the main space W0 is a Hilbert space. Moreover, we denote the inner product in L2 as (,), the inner product in W0 as (,)W0, and the dual product of W0 in Y0 as ,W0. Y0 is the dual space of W0.

    For uW0, we denote the main energy functional of this paper:

    E(t)=12ut22+a2u2W0+12θu2θW01kΩ|u|kln|u|dx+1k2ukk. (2.5)

    In addition, we define the potential energy functional

    J(u)=a2u2W0+12θu2θW01kΩ|u|kln|u|dx+1k2ukk, (2.6)

    and Nehari functional

    I(u)=au2W0+u2θW0Ω|u|kln|u|dx. (2.7)

    By direct computation, we have

    E(t)=J(u)+12ut22, (2.8)

    and

    J(u)=a(k2)2ku2W0+k2θ2θku2θW0+1kI(u). (2.9)

    We also define the depth of the potential well and the Nehari manifold, respectively, as

    d=infuNJ(u), (2.10)
    N={uW0{0},I(u)=0}.

    Further, we will introduce the sets

    W+={uW0|I(u)>0}{0},
    W={uW0|I(u)<0}.

    In this paper, to avoid confusion, we simply write u(x,t) as u(t) sometimes. Next, we give some definitions.

    Definition 2.1. The function u=u(x,t) is a weak solution of Problem (1.1) on Ω×[0,T], supposing that

    uC([0,T];W0)C1([0,T];L2(Ω))C2([0,T];Y0)

    and utL2(0,T;W0) satisfying u(0)=u0,ut(0)=u1, and it holds that

    utt,ϕW0+M([u]2s)(u,ϕ)W0+(ut,ϕ)W0=(|u|k2uln|u|,ϕ),

    for arbitrary ϕW0, where the inner product

    (u,v)W0=Q(u(x)u(y))(v(x)v(y))|xy|2s+Ndxdy.

    Definition 2.2. Let u(x,t) be a weak solution of Problem (1.1), and if the maximal existence time Tmax is finite and

    limtTmax(t0u2W0dt+u22)=+,

    we say that u(x,t) blows up in finite time.

    Lemma 2.1. Let uW0{0}, and we have

    (i)limλ+J(λu)=, limλ0+J(λu)=0;

    (ii)J(λu) is decreasing when λ(λ,+), and increasing when λ(0,λ);

    (iii)I(λu)<0 when λ(λ,+), and I(λu)>0 when λ(0,λ).

    Proof. By (2.6), we have

    J(λu)=aλ22u2W0+λ2θ2θu2θW0λkk2lnλukkλkkΩ|u|kln|u|dx+λkk2ukk,

    so the conclusion of (i) is obviously valid. For the derivation of the above formula, we can obtain

    ddλJ(λu)=λk1lnλukkλk1Ω|u|kln|u|dx+aλu2W0+λ2θ1u2θW0=λ(λk2lnλukkλk2Ω|u|kln|u|dx+au2W0+λ2θ2u2θW0).

    Let

    g(λ)=λk2(lnλukkΩ|u|kln|u|dx+λ2θku2θW0),

    and since k>2θ and θ1, we can obtain

    limλ0g(λ)=0andlimλ+g(λ)=. (2.11)

    Further, we have

    g(λ)=λk3[2u2θW0(θ1)λ2θk(k2)ukklnλ(k2)Ω|u|kln|u|dxukk]λk3h(λ),

    where

    h(λ)=2u2θW0(θ1)λ2θk(k2)ukklnλ(k2)Ω|u|kln|u|dxukk,

    which, together with k>2θ2 and θ1, gives us limλ+h(λ)= and limλ0h(λ)=+. Taking the derivative of h(λ), we obtain

    h(λ)=2u2θW0(k2θ)(θ1)λ2θk(k2)ukkλ<0.

    So we infer that there is a unique λ0 that satisfies h(λ)|λ=λ0=0, which means that

    g(λ){<0,λ0<λ<+,=0,λ=λ0,>0,0<λ<λ0. (2.12)

    Combining (2.11) and (2.12), there is a unique λ1 that satisfies g(λ)|λ=λ1=0. Then we can get that there is a λ>λ1 satisfying au2W0+g(λ)=0, which means that ddλJ(λu)|λ=λ=0, ddλJ(λu) is negative on (λ,+), and ddλJ(λu) is positive on (0,λ). Therefore, it can be seen that the conclusion of (ii) is valid. By (2.6) and (2.7), we have

    I(λu)=λddλJ(λu){<0,λ<λ<+,=0,λ=λ,>0,0<λ<λ.

    Thus, the conclusion of (iii) holds. We have completed the proof of the properties of J(λu).

    Lemma 2.2. [27] Suppose that μ is a positive constant. We can get

    |ΨklnΨ|(ek)1,if0<Ψ<1,

    and

    ΨklnΨ(eμ)1Ψk+μ,ifΨ1,

    where e is a natural constant.

    Lemma 2.3. [28] For r[1,2s] and uW0, there is a constant C0(N,r,s)>0 that gives us

    urC0uW0.

    Lemma 2.4. [29] Assume that W is a Banach space, and if fLk(0,T;W),ftLk(0,T;W), then when the value is transformed in a suitable set of measure zero in [0,T], f is a continuous injection from [0,T] onto W.

    Lemma 2.5. [30] Assume that (X,d) is a complete metric space, F:XX, and for any x,yX, we have

    d(F(x),F(y))δd(x,y),

    for some constant 0<δ<1. Then F has a unique fixed point ˉxX such that F(ˉx)=ˉx.

    Lemma 2.6. Assume that u(x,t) is a weak solution of Problem (1.1), so the energy functional E(t) is non-increasing about t.

    Proof. We multiply the first equation of (1.1) by ut and integrate it on Ω×[0,t), we can get

    12ddtut22+a2ddtu2W0+12θddtu2θW0+ut2W0=1kddtΩ|u|kln|u|dx1k2ddtukk,

    namely,

    t0uτ2W0dτ+E(t)=E(0). (2.13)

    Deriving E(t) about t, and we get

    E(t)=uτ2W00.

    Therefore, the proof of the properties of E(t) has been completed.

    Lemma 3.1. For any 22θ<k2s, T>0, uH=C([0,T];W0)C1([0,T];L2(Ω)), there is a unique

    vC([0,T];W0)C1([0,T];L2(Ω))C2([0,T];Y0)

    such that

    {vtt+M([u]2s)(Δ)sv+(Δ)svt=|u|k2uln|u|,xΩ,t>0;u(x,0)=u0(x),ut(x,0)=u1(x),xΩ;u(x,t)=0,xRNΩ,t0. (3.1)

    Proof. (i) Proof of the existence.

    According to literature [31], there is an eigenfunction sequence {ej}jC0(Ω) of fractional Laplacian operators, which is a completed orthogonal basis of W0 and is an orthonormal basis in L2(Ω). λj>0 is defined as the corresponding eigenvalue satisfying (Δ)sej=λjej. Taking Wm=Span{e1,,em} and constructing the approximate solutions

    vm(x,t)=mj=1ej(x)hmj(t),

    for every ηWm and t0, satisfies the equations

    {Ω[¨vm+M([u]2s)(Δ)svm+(Δ)s˙vm|u|k2uln|u|]ηdx=0,vm(0)=um0=mj=1(Ωu0ejdx)eju0inW0asm,˙vm(x)=um1=mj=1(Ωu1ejdx)eju1inL2(Ω)asm. (3.2)

    For j=1,,m, we make η=ej in the first equation in (3.2), and {hmj}mj=1 satisfies the Cauchy equations

    {¨hmj(t)=Fj(t,hm1(t),hm2(t),,hmm(t)),hmj(0)=Ωu0ejdx,˙hmj(0)=Ωu1ejdx,

    where

    Fj=λjhmj(t)M([u]2s)λj˙hmj(t)+Ωej(x)|u|k2uln|u|dx,

    which is a linear ordinary differential equation about hmj. On the basis of Peano's theorem, a local solution hmjC1[0,T] has been obtained for the Cauchy problem mentioned above.

    Now, we take η=ej and multiply two sides of the first equation (3.2) by ˙hmnj(t), and then sum over j from 1 to m to get

    ddtvmt22+ddt[M([u]2s)vm2W0]+2vmτ2W0=2Ωvmt|u|k2uln|u|dx+vm2W0ddt[M([u]2s)].

    We integrate the above equation on [0,t] to get

    vmt22+M([u]2s)vm2W0+2t0vmτ2W0dτ=u122+M([u0]2s)um02W0+t0vm2W0ddt[M([u]2s)]dτ+2t0Ωvmτ|u|k2uln|u|dxdτ. (3.3)

    Recalling uH, we see that uW0 is bounded. Through the definition and assumption of function M(m), we arrive at

    t0vm2W0ddt[M([u]2s)]dτt0CM([u]2s)vm2W0dτ=t0C(a+u2(θ1)W0)vm2W0dτC1t0vm2W0dτ. (3.4)

    Among them, C1 is a positive number that only depends on T. Then we estimate the integral containing a logarithmic source on the right side of (3.3). Through Hölder's inequality, we can obtain

    2t0Ωvmτ|u|k2uln|u|dxdτ2t0(Ω|vmτ|2NN2sdx)N2s2N(Ω||u|k2uln|u||2NN+2sdx)N+2s2Ndτ2t0vmτ2NN2s|u|k2uln|u|2NN+2sdτ. (3.5)

    So next we deal with the term vmt2NN+2s in (3.5). According to Lemma 2.3, we have

    vmt2NN2sC0(N,s)vmtW0. (3.6)

    Then let Ω1={xΩ||un(x)|<1}, Ω2={xΩ||un(x)|1}. Combining Lemmas 2.2 and 2.3, here we choose 0<μ2NN2sp, and then we can obtain

    |u|k2uln|u|2NN+2s2NN+2s=Ω1||u|k2uln|u||2NN+2sdx+Ω2||u|k2uln|u||2NN+2sdxΩ1||u|k1ln|u||2NN+2sdx+Ω2||u|μln|u||u|k1+μ|2NN+2sdx[e(k1)]2NN+2s|Ω|+(eμ)2NN+2su2N(k1+μ)N+2s2N(k1+μ)N+2s[e(k1)]2NN+2s|Ω|+(eμ)2NN+2sC2N(k1+μ)N+2s0u2N(k1+μ)N+2sW0, (3.7)

    so we can obtain

    t0|u|k2uln|u|22NN+2sdt([e(k1)]2NN+2s|Ω|+(eμ)2NN+2sC2N(k1+μ)N+2s0C2N(k1+μ)N+2s)N+2sNT=C2T, (3.8)

    where C2=([e(k1)]2NN+2s|Ω|+(eμ)2NN+2sC2N(k1+μ)N+2s0C2N(k1+μ)N+2s)N+2sN.

    Utilizing Young's inequality, then combining (3.6) and (3.8), (3.5) can be written as

    2t0Ωvmτ|u|k2uln|u|dxdτ2t0C0vmtW0|u|k2uln|u|2NN+2sdτt0C20|u|k2uln|u|22NN+2sdτ+t0vmτ2W0dτC20C2T+t0vmτ2W0dτ. (3.9)

    Due to the convergence of um0 and um1, from (3.3), (3.4), and (3.9), we arrive at

    vmt22+M([u]2s)vm2W0+t0vmτ2W0dτu122+M([u0]2s)um02W0+C20C2T+C1t0vm2W0dτ=˜C+C1t0vm2W0dτ, (3.10)

    where ˜C=u122+M([u0]2s)um02W0+C20C2T>0 is independent of m. According to the definition of Kirchhoff function M(m), we have

    avm2W0M([u]2s)vm2W0. (3.11)

    Combining (3.10) and (3.11), we have

    avm2W0˜C+C1t0vm2W0dτ. (3.12)

    Making use of the Gronwall inequality, we get

    vm2W0˜CaeC1at, (3.13)

    and integrating (3.13) on [0,t], we arrive at

    t0vm2W0dτ˜CC1(eC1at1). (3.14)

    We substitute (3.14) into (3.10) to get

    vmt22+M([u]2s)vm2W0+t0vmτ2W0dτ˜CC1(eC1at1)+˜CCT, (3.15)

    where CT is a normal number that depends on T. From (3.15), we get

    vmvweaklystarinL(0,T;W0), (3.16)
    vmtvtweaklyinL2(0,T;W0), (3.17)
    vmtvtweaklystarinL(0,T;L2(Ω)). (3.18)

    By (3.16), (3.17), and the Aubin-Lions-Simon lemma [32], we can obtain

    vmvstronglyinC([0,T],L2(Ω)).

    Therefore, vm(x,0) makes sense, vm(x,0)v(x,0)inL2(Ω), and vm(x,0)=um0(x)u0(x)inW0. Thus, v(x,0)=u0(x).

    Furthermore, dividing the two sides of the first equation in (3.2) by ηW0, we have

    vmtt,ηηW0=(vt,η)W0M([u]2s)(v,η)W0+(|u|k2uln|u|,η)ηW0. (3.19)

    By the H¨older inequality, (3.7), and (3.15), we get

    vmtt,ηηW0CT. (3.20)

    For ηW0{0}, upper bounds are simultaneously taken on both sides of Eq (3.20), and we have

    vmttY0CT, (3.21)

    namely

    vmttvttweaklystarinL(0,T;Y0). (3.22)

    Combining vtL(0,T;L2(Ω)) and vttL(0,T;Y0), through Lemma 2.4, we get

    vtC([0,T],Y0).

    Thus vmt(x,0) is meaningful and vmt(x,0)vt(x,0)inY0. Owing to vmt(x,0)=um1(x)u1(x) in L2(Ω), we have that vt(x,0)=u1(x). We have completed the proof of the existence.

    (ii) Proof of the uniqueness.

    Assuming Problem (1.1) has two solutions v1 and v2 with the same starting conditions, substituting them into Problem (3.1), and then, by subtracting the obtained two equations, we can get

    (v1v2)tt+M([u]2s)(Δ)s(v1v2)+(Δ)s(v1v2)t=0. (3.23)

    Multiplying (3.23) by v1tv2t and integrating on Ω×(0,T), we get

    12v1tv2t22+12M([u]2s)v1v22W0+t0v1τv2τ2W0dτ=0.

    Obviously, this equality immediately yields v1v2. This completes the proof.

    Based on the above lemma, we obtain the following theorem.

    Theorem 3.1. Let u0W0, u1L2(Ω), and 22θ<k2s. Then there is a T>0 that gives Problem (1.1) with a unique local solution u(x,t) on [0,T] satisfying

    uC([0,T];W0)C1([0,T];L2(Ω))C2([0,T];Y0).

    Proof. For a given T>0, we think over the important space H=C([0,T];W0)C1([0,T];L2(Ω)) which has the following norm:

    u2H=max0tT(au(t)2W0+ut(t)22).

    Let R2=M([u0]2s)u02W0+u122, and then we denote

    MT={uH:ut(0)=u1,u(0)=u0,uHR}.

    We first prove that MT is a complete metric space. Let {un} be the Cauchy-Schwarz sequence in MT. Thus, for any ε>0, there exists με such that if n,mμε, then

    unum2H=max0tT(unum2W0+unum22)ε,

    and by the completeness of L2(Ω) and W0, there exist uL2(Ω) such that umu in L2(Ω) and uW0 such that umu in W0 when m, namely

    unu2H=max0tT(unu2W0+unu22)ε.

    Therefore, MT is a complete metric space.

    Next, using the conclusion of Lemma 3.1, we denote v=Φ(u) for any uMT as the unique solution to Problem (3.1). We will prove the mapping Φ is a contraction mapping satisfying Φ(MT)MT. We multiply the first equation of the Problem (3.1) with vt and integrate it on Ω×(0,t), and we obtain

    vt22+M([u]2s)v2W0+2t0vτ2W0dτ=u122+M([u0]2s)u02W0+t0ddt[M([u]2s)]v2W0dτ+2t0Ωvτ|u|k2uln|u|dxdτ. (3.24)

    Using a calculation method similar to the processes in (3.5) and (3.7), we find

    2t0Ωvτ|u|k2uln|u|dxdτ2t0vτ2NN2s|u|k2uln|u|2NN+2sdτt0C202|u|k2uln|u|22NN+2sdτ+2t0vτ2W0dτC20T2{(eμ)2NN+2s(C20R2a)N(k1+μ)N+2s+[e(k1)]2NN+2s|Ω|}N+2sN+2t0vτ2W0dτ. (3.25)

    Then by a similar computation to that of (3.4) and (3.14), we can derive that

    t0v2W0ddt[M([u]2s)]dτ˜C(eC1aT1). (3.26)

    Combining (3.25) and (3.26), (3.24) becomes

    vt22+M([u]2s)v2W0R2+˜C(eC1aT1)+C20T2{(eμ)2NN+2s(C20R2a)N(k1+μ)N+2s+[e(k1)]2NN+2s|Ω|}N+2sN.

    Further,

    v2H=vt22+av2W0vt22+M([u]2s)v2W0R2+˜C(eC1aT1)+C20T2{(eμ)2NN+2s(C20R2a)N(k1+μ)N+2s+[e(k1)]2NN+2s|Ω|}N+2sN.

    So we can choose a T>0 to make it small enough so that v2HR2.

    Next, we will prove that Φ is a contraction mapping. Let v1=Φ(w1), v2=Φ(w2) where w1,w2MT. Then if v=v1v2, v satisfies

    {vtt+M([w1]2s)(Δ)sv+(Δ)svt=+|w1|k2w1ln|w1||w2|k2w2ln|w2|[M([w1]2s)M([w2]2s)](Δ)sv2,xΩ,t>0;v(x,0)=vt(x,0)=0,xΩ;v(x,t)=0,xRNΩ,t0.

    We will multiply the first equation of the above problem by vt, and then integrate on Ω×(0,t), and we have

    vt22+M([w1]2s)v2W0+2t0vτ2W0dτt0ddt[M([w1]2s)]v2W0dτ+2t0Ω|M([w1]2s)M([w2]2s)|(Δ)sv2vτdxdτ+2t0Ω(|w1|k2w1ln|w1||w2|k2w2ln|w2|)vτdxdτ. (3.27)

    Next, we estimate the terms on the right side of (3.27) one by one. First, by performing calculations similar to (3.4), we obtain

    t0ddt[M([w1]2s)]v2W0dτt0CM([w1]2s)v2W0dτCt0[M([w1]2s)v2W0+vτ22]dτ. (3.28)

    Due to the function M(m) being locally Lipschitz continuous, we arrive at

    2t0Ω|M([w1]2s)M([w2]2s)|(Δ)sv2vτdxdτ=2t0Ω|M([w1]2s)M([w2]2s)[w1]2s[w2]2s||[w1]2s[w2]2s|(Δ)sv2vτdxdτ2CLt0Ω|w12W0w22W0|(Δ)sv2vτdxdτ=2CL|w1W0+w2W0||w1W0w2W0|t0Ω(Δ)sv2vτdxdτ2CL|w1W0+w2W0|w1w2W0t0Ω(Δ)sv2vτdxdτ.

    Next we use Young's inequality and Hölder's inequality to obtain

    2t0Ω|M([w1]2s)M([w2]2s)|(Δ)sv2vτdxdτ2CL|w1W0+w2W0|w1w2W0t0v2W0vτW0dτ4CLRaw1w2W0t0v2W0vτW0dτ(4CLRaw1w2W0)24t0v22W0dτ+t0vτ2W0dτ4C2LR4a2Tw1w22W0+t0vτ2W0dτ4C2LR4a3Tw1w22H+t0vτ2W0dτ. (3.29)

    Similarly, taking advantage of the Lipschitz continuity of f(x)=|x|k2xln|x| in R+R+, and from Lemma 2.3, we can see that

    2t0Ω(|w1|k2w1ln|w1||w2|k2w2ln|w2|)vtdxdτ=2t0Ω(f(w1)f(w2)w1w2)(w1w2)vtdxdτ2˜CLt0w1w22vt2dτ2˜CLC20t0w1w2W0vtW0dτ(2˜CLC20w1w2W0)2T4+t0vt2W0dτ˜C2LC40aTw1w22H+t0vt2W0dτ. (3.30)

    Substitute (3.28)–(3.30) into (3.27), and we can infer that

    vt22+M([w1]2s)v2W0+2t0vτ2W0dτCt0[M([w1]2s)v2W0+vτ22]dτ+(4C2LR4a3T+˜C2LC40aT)w1w22H.

    Applying the Gronwall inequality to the above inequality, we have

    vt22+M([w1]2s)v2W0(4C2LR4a3T+˜C2LC40aT)(1+CTeCT)w1w22H.

    We can take T>0 to make it small enough so that

    (4C2LR4a3T+˜C2LC40aT)(1+CTeCT)<1,

    and we conclude that there exists δ(0,1) satisfying

    Φ(w1)Φ(w2)H=v2Hδw1w2H.

    Therefore, the above processes make certain the existence of weak solutions.

    First of all, we will prove the invariance of the set W+.

    Lemma 4.1. Let u be the solution to Problem (1.1). In the case of u0W+, u1L2(Ω), and 0<E(0)<d, then for all t0, we have u(t)W+.

    Proof. First, according to Lemma 2.6, we can get E(t)E(0)<d. Next, we will prove through the method of contradiction that there is a minimum time t(0,Tmax) that satisfies u(t)W+, i.e., I(u(t))>0 for t[0,t) and I(u(t))=0. From (2.8), (2.9), and (2.13), we have

    0<12ut(t)22+a(k2)2pu(t)2W0+k2θ2θku(t)2θW0+t0uτ(t)2W0dτ=E(0)<d,

    which means that u(t)0 and ut(t)0. Thus according to (2.10), we get

    d>E(0)E(t)J(u(t))infuNJ(u)=d,

    which is not valid. Hence, we obtain u(t)W+.

    Theorem 4.1. Let u0W0, u1L2(Ω), and 22θ<k2s. If E(0)d, I(u0)>0, and then Problem (1.1) possesses a global weak solution uL(0,+;W0) and utL(0,+;L2(Ω))L2(0,+;W0). In addition, if

    E(0){d,a(k2)2p(aeμCp+μ0)2k+μ2}andI(u0)>0,

    there exist positive constants κ and γ so that E(t) satisfies the exponential decay estimate for t0 as follows:

    E(t)κeγt.

    Proof. We will prove the global existence and decay estimate.

    Step 1. Global existence.

    We will divide into two cases to prove the global existence.

    Case 1: I(u0)>0 and E(0)<d

    First of all, we need to declare that for the cases where E(0)<d and I(u0)>0, we have:

    (i) If I(u0)>0 and E(0)<0, this contradicts (2.8) and (2.9).

    (ii) If I(u0)>0 and E(0)=0, by (2.8) and (2.9), it is evident that u00 and u10, which is an ordinary situation.

    As a result, we only need to think about the cases where 0<E(0)<d and I(u0)>0.

    From Lemma 4.1, we can see that u(t)W+, which means that I(u(t))>0. Combining (2.5), (2.9), and (2.13), we get

    1kI(u)+12ut22+a(k2)2ku2W0+k2θ2θku2θW0+t0uτ2W0dτ=E(0)<d,

    namely

    12ut22+a(k2)2ku2W0+k2θ2θku2θW0+t0uτ2W0dτ<E(0)<d. (4.1)

    The right end of Eq (4.1) is a constant unrelated to t. This estimate enables us to take Tmax=+. As a consequence, we are able to get that Problem (1.1) has a unique global weak solution u(t).

    Case 2: I(u0)>0 and E(0)=d

    Above all, we can select a sequence {θn}n=1(0,1) satisfying limnθn=1. Next we think about the problem as follows:

    {utt+M([u]2s)(Δ)su+(Δ)sut=|u|k2uln|u|,xΩ,t>0;%(x,t)Ω×R+;u(x,0)=u0n=θnu0(x),ut(x,0)=u1n=θnu1(x),xΩ,%(x,t)(RNΩ)×R+0;u(x,t)=0,xRNΩ,t0.

    We claim that I(u0n)>0 and 0<E(u0n)<d. In fact, from I(u0)>0 and θn(0,1), we get

    I(u0n)=θknΩ|u0|kln|u0|dx+aθ2nu2W0+θ2θnu2θW0θknlnθnu0kkθknΩ|u0|kln|u0|dx+aθ2nu2W0+θ2θnu2θW0θknI(u0)>0.

    On the other hand, combining the above inequality and Lemma 2.1, we have

    ddθnJ(θnu0)=1θnI(u0n)>0,

    which indicates that J(θnu0) is strictly increasing relative to θn and

    J(u0n)=J(θnu0)<J(u0).

    Further, we have

    0<E(u0n,u1n)=J(u0n)+12u1n22<J(u0)+12u122=E(0)=d.

    Since u0nu0 and u1nu1 as n+, we are able to get that there is a global weak solution u(t) to the above problem through a method similar to Case 1.

    Step 2. Decay estimate.

    We establish an exponential energy decay estimate of Problem (1.1) when I(u0)>0 as well as E(0){d,a(k2)2p(aeμCp+μ0)2k+μ2}.

    It follows from (4.1) that

    u2W02kE(0)a(k2). (4.2)

    Next, we define an auxiliary function as follows:

    K(t)=εΩutudx+ε2u2W0+E(t),

    where ε>0 will be specified later. Through Lemma 4.1, we get I(u(t))>0. Then by (2.5), (2.8), and (2.9), we obtain

    E(t)>12ut22+a(k2)2ku2W0+k2θ2θku2θW0>0. (4.3)

    Next, utilizing Young's inequality, and combining (4.3) and Lemma 2.3, we arrive at

    K(t)ε2u22+ε2u2W0+ε2ut22+E(t)ε2ut22+(εC202+ε2)u2W0+E(t)εE(t)+(εC202+ε2)2ka(k2)E(t)+E(t)η2E(t), (4.4)

    and

    K(t)ε4ξut22+ε2u2W0εξu22+E(t)ε4ξut22+(ε2εξC20)u2W0+E(t). (4.5)

    Taking ξ small enough such that ξ12C20, then we can obtain

    K(t)ε4ξu2W0+E(t)ε2ξE(t)+E(t),

    and we fix ξ and choose a sufficiently small normal number ε such that ε<2δ, so (4.4) can be written as

    K(t)[1ε(2ξ)1]E(t)=η1E(t). (4.6)

    Combining (4.4) and (4.6), it is easy to conclude that L(t) is equivalent to E(t), because there exist two constants η1>0 and η2>0 about ε satisfying

    η1E(t)K(t)η2E(t),fort0. (4.7)

    Next, we derive K(t) about t and choose 0<M<2θ. From (2.5) and Lemma 2.3, we arrive at

    K(t)=E(t)+ε(u,utt)+ε(u,ut)W0+εut22=ut2W0+ε(Ω|u|kln|u|dxau2W0u2θW0)+εut22=εME(t)ut2W0+(εM2+ε)ut22+(aεM2aε)u2W0+(εM2θε)u2θW0+(εεMk)Ω|u|kln|u|dx+εMk2ukkεME(t)+(εM2+ε1C20)ut22+(aεM2aε)u2W0+(εεMk)Ω|u|kln|u|dx+εMk2ukk. (4.8)

    Next we will estimate each term of (4.8). For the term ukk, by (4.2), we obtain

    ukkCk0ukW0=Ck0uk2W0u2W0Ck0(2kE(0)a(k2))k22u2W0. (4.9)

    From (4.3) and Lemmas 2.2 and 2.3, for the logarithmic source term, we have

    Ω|u|kln|u|dxΩ2|u|k1eμ|u|μdx1eμuk+μk+μCk+μ0eμuk+μW0Ck+μ0eμ(2kE(0)a(k2))k+μ22u2W0, (4.10)

    where μ satisfies 0<μ<2sk. Substituting (4.9) and (4.10) into (4.8), we can derive that

    K(t)εME(t)+(εM2+ε1C20)ut22+(aεM2aε)u2w0+(εεMk)Ck+μ0eμ[2kE(0)a(k2)]k+μ22u2w0+εMCk0k2[2kE(0)a(k2)]k22=εME(t)+(εM2+ε1C20)ut22+ε{aM2a+Ck+μ0eμ[2pE(0)a(p2)]k+μ22Ck+μ0Mkeμ[2kE(0)a(k2)]k+μ22+Ck0Mk2[2kE(0)a(k2)]k22}u2w0, (4.11)

    where we require E(0){d,a(k2)2k(aeμCk+μ0)2k+μ2} such that

    Ck+μ0eμ[2kE(0)a(k2)]k+μ22aCk+μ0eμ[2kda(k2)]k+μ22a<0.

    Now, we choose a small enough M to make

    aM2a+Ck+μ0eμ[2kE(0)a(k2)]k+μ22+Ck0Mk2[2kE(0)a(k2)]k22<0. (4.12)

    We fix M and then select a sufficiently small ε to make

    εM2+ε1C20<0. (4.13)

    Through (4.11)–(4.13), we arrive at

    K(t)εME(t). (4.14)

    Further, by (4.7), let γ=εMη2 and (4.14) becomes

    K(t)γK(t). (4.15)

    Eventually, by integrating (4.15) with (0,t), we can infer that K(t)K(0)eγt, and combining with (4.7), we can get

    0<E(t)κeγt,t>0,

    where κ=L(0)η1.

    First, we will prove the invariance of the set W.

    Lemma 5.1. Let u(x,t) be a weak solution to Problem (1.1). Assuming u0W and E(0)<d, for all t0, we have u(t)W. In addition, we have the following inequality:

    d<a(k2)2ku2W0+k2θ2θku2θW0. (5.1)

    Proof. It follows from u0W that I(u0)<0. Next, we discuss it in two situations.

    When E(0)0, from (2.8) and (2.9), we arrive at

    E(t)=12ut22+1kI(u)+a(k2)2ku2W0+k2θ2θku2θW0<E(0)0<d,

    which means that I(u(t))<0, i.e., u(t)W.

    When 0<E(0)<d, by (2.13), we have

    0<E(t)+t0uτ2W0dτ=E(0)<d, (5.2)

    which implies that u(x,t)0. For t[0,Tmax), we prove that I(u(t))<0. If not, there is a t1(0,Tmax) to make u(t1)W, i.e., I(u(t1))=0 and I(u(t))<0, t[0,t1). Looking back at (2.10), it is obvious that

    E(0)E(t1)J(u(t1))infuNJ(u)=d,

    which is opposite to (5.2). Therefore, for t[0,Tmax], we get u(t)W.

    By Lemma 2.1, due to I(u(t))<0, there is a λ<1 satisfying I(λu(t))=0, and combining with (2.9) gives

    dJ(λu)=1kI(λu)+a(k2)2kλ2u2W0+k2θ2θkλ2θu2θW0=a(k2)2kλ2u2W0+k2θ2θkλ2θu2θW0<a(k2)2ku2W0+k2θ2θku2θW0.

    Therefore, Lemma 4.1 is proven.

    Theorem 5.1. Let 22θ<k2s, u0W, and u1L2(Ω). Assuming E(0)<d, the solution of Problem (1.1) blows up in finite time.

    Proof. First of all, by E(0)<d, u0W, and Lemma 4.1, we get uW, which means that I(u)<0.

    We will prove that u(t) blows up in finite time. If this is not established, we assume the global existence of u, i.e., Tmax=+. For any T0>0, we define the positive function

    Q(t)=(T0t)u02W0t0u2W0dτ+u22.

    We calculate the first-order and second-order derivatives of Q(t), respectively, as

    Q(t)=u2W0+2(u,ut)u02W0=2t0(u,uτ)W0dτ+2(u,ut), (5.3)

    and

    Q(t)=2ut22+2(u,ut)W0+2(u,utt)=2ut222I(u)>0. (5.4)

    Through direct calculation, we arrive at

    Q(t)Q(t)k+24[Q(t)]2=Q(t)(2ut222I(u))+(k+2){Φ(t)[Q(t)(Tt)u02W0](t0uτ2W0dτ+ut22)}, (5.5)

    where the definition of ψ(t) is as follows:

    ψ(t)=(t0u2W0dτ+u22)(t0uτ2W0dτ+ut22)[t0(u,uτ)W0dτ+(u,ut)]2.

    Using Hölder's inequality and the Cauchy-Schwarz inequality, for any t(0,T0), it is clear that ψ(t)0.

    Further, (5.5) becomes

    Q(t)Q(t)k+24[Q(t)]2Q(t)(2ut222I(u))(k+2)[Q(t)(Tt)u02W0](t0uτ2W0dτ+ut22)Q(t)[2ut222I(u)(k+2)(t0uτ2W0dτ+ut22)]=Q(t)[kut222I(u)(k+2)t0uτ2W0dτ]=Q(t)φ(t), (5.6)

    where φ(t)=kut222I(u)(k+2)t0uτ2W0dτ. Moreover, by (2.5), (2.13), and (5.1), we have

    φ(t)=2kE(t)+a(k2)u2W0+(kθ2)u2θW0+2kukk(k+2)t0uτ2W0dτ2kE(0)+2kt0uτ2W0dτ+a(k2)u2W0+(kθ2)u2θW0+2kukk(k+2)t0uτ2W0dτ=2kE(0)+(k2)t0uτ2W0dτ+a(k2)u2W0+(kθ2)u2θW0+2kukk2kd2kE(0)+(k2)t0uτ2W0dτ+2kukk. (5.7)

    Since E(0)<d, we can get φ(t)>0. The combination of (5.6) and (5.7) means that for all t[0,T0],

    Q(t)Q(t)k+24[Q(t)]2>0.

    Let

    q(t):=Q(t)k24,

    and then we arrive at

    q(t)=(k241)(k24)Q(t)k242[Q(t)]2Q(t)k24Q(t)k241={Q(t)Q(t)k+24[Q(t)]2}(k24)Q(t)k242<0.

    As a result, it can be obtained that

    limtT0q(t)=0,

    namely

    limtT0Q(t)=+.

    Therefore, the hypothesis does not hold. We have completed the proof.

    We have investigated the initial boundary value problem that includes the fractional laplacian operator, strong damping term, and logarithmic source. To our knowledge, Kirchhoff proposed groundbreaking work on Kirchhoff-type problems, and we consider Problem (1.1), which has not been studied before. We proved the local existence by the contraction mapping principle and Faedo-Galerkin's method, namely, Theorem 3.1. Furthermore, global existence and properties of decay and blow-up when the initial value meets certain conditions are obtained, namely, Theorems 4.1 and 5.1. In future work, we will attempt to study the qualitative analysis of some interesting new models.

    A. H. Sun: Methodology, writing–original draft, writing–review and editing; H. Xu: Methodology, writing–original draft. Both of authors have read and approved the final version of the manuscript for publication.

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

    The authors would like to thank the editors and the anonymous referees for their careful reading and helpful suggestions which led to an improvement of this paper.

    The authors declare that there is no conflict of interests regarding the publication of this paper.



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