In this paper, we study the initial-boundary value problem for a class of fractional p-Laplacian Kirchhoff diffusion equation with logarithmic nonlinearity. For both subcritical and critical states, by means of the Galerkin approximations, the potential well theory and the Nehari manifold, we prove the global existence and finite time blow-up of the weak solutions. Further, we give the growth rate of the weak solutions and study ground-state solution of the corresponding steady-state problem.
Citation: Fugeng Zeng, Peng Shi, Min Jiang. Global existence and finite time blow-up for a class of fractional p-Laplacian Kirchhoff type equations with logarithmic nonlinearity[J]. AIMS Mathematics, 2021, 6(3): 2559-2578. doi: 10.3934/math.2021155
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In this paper, we study the initial-boundary value problem for a class of fractional p-Laplacian Kirchhoff diffusion equation with logarithmic nonlinearity. For both subcritical and critical states, by means of the Galerkin approximations, the potential well theory and the Nehari manifold, we prove the global existence and finite time blow-up of the weak solutions. Further, we give the growth rate of the weak solutions and study ground-state solution of the corresponding steady-state problem.
In this paper, we study the global existence and blow-up for the following nonlinear fractional p-Laplacian Kirchhoff diffusion equation.
{ut+M([u]ps,p)(−Δ)spu=|u|αp−2uln|u|,in Ω×(0,T),u(0)=u0,in Ω,u=0,on ∂Ω×(0,T), | (1.1) |
where s∈(0,1), 1<p<N/s (N is space latitude and satisfies N≥1), 1≤α<p∗s/p, p∗s=NpN−sp, Ω⊂RN is a bounded domain with Lipschitz boundary, [u]s,p is Gagliardo seminorm of u, (−Δ)sp is the fractional p-Laplacian operator and satisfies
(−Δ)spu(x)=2limβ→0+∫RN∖Bβ(x)|u(x)−u(y)|p−2(u(x)−u(y))|x−y|N+spdy, |
where u(x)∈C∞ and u(x) has compact support in Ω, Bβ(x)⊂RN is the set of spheres with x as the center and β as the radius. Let M(t)=a+btα−1(t≥1), where a and b are constants and satisfy a≥0, b>0, in this paper we let a=0, b=1, t=[u]ps,p, i.e. M([u]ps,p)=[u]αp−ps,p. Let Ω⊂RN be a bounded domain with Lipschitz boundary, and use ‖⋅‖r to denote the norm of Lebesgue space Lr(Ω), where r∈(0,+∞). In view of the idea from [1], we define linear space Ws,p(Ω) as a fractional Sobolev space and discuss in the fractional Sobolev space Ws,p0(Ω),
Ws,p0(Ω)={u∈Ws,p(Ω) | u(t)=0 a.e.in RN∖Ω}. |
The norm of space Ws,p(Ω) is defined as the following equation
‖u‖Ws,p=(‖u‖pp+∬R2N|u(x)−u(y)|p|x−y|N+spdxdy)1p. |
According to the research result from [2], it can be concluded that
[u]s,p=(∬R2N|u(x)−u(y)|p|x−y|N+spdxdy)1p. |
Kirchhoff-type problems have a wide range of applications in mathematics and physics. In recent years, many scholars have devoted themselves to the study of Kirchhoff-type problems and have achieved many results [3,4,5,6]. Moreover, readers who are interested in this knowledge can refer to [7,8,9,10,11,12,13,14,15]. The research on the fractional p-Laplacian operator equation also achieved some results, such as [16,17,18,19,20,21]. Detailed knowledge about fractional-order related theories and differential inequalities can refer to [22,23,24,25] and the parabolic equation with logarithmic nonlinearity can refer to [26,27,28].
Until now, many scholars have studied the fractional Laplacian problem. In [1], the authors studied the fractional Kirchhoff-type problem.
{ut+[u]2(θ−1)s(−Δ)su=|u|q−2uln|u|,(x,t)∈Ω×R+,u(x,t)=0,(x,t)∈(RN∖Ω)×R+,u(x,0)=u0(x),x∈Ω, | (1.2) |
where [u]s is the Gagliardo seminorm of u, let
[u]s=(∬R2N|u(x)−u(y)|2|x−y|N+2sdxdy)12, |
where s∈(0,1), q∈(2θ,2∗), θ∈[1,N/(N−2s)), N>2s, Ω⊂RN is a bounded domain with Lipschitz boundary. They use the variational principle, Nehari manifold and potential well method to study the finite time blow-up of the solution of the problem (1.2) and the sufficient conditions for the global existence.
In [2], the authors studied the following initial value problem:
M([u]ps,p)(−Δ)spu=h(x)|u|θp−2uln|u|+λ|u|q−2u,x∈Ω, | (1.3) |
where h(x) is a sign-changing function on Ω, λ is a positive parameter, M([u]ps,p)=[u]p(θ−1)s,p. By the method of the mountain pass lemma and Nehari manifold, the existence of the minimum energy solutions are obtained. For the steady-state equation, it is worth emphasizing that for the local minimum solution, Liu and Liao and Pan used a brand-new method in [29], and also obtained some properties of the corresponding equation.
In [3], the authors discuss the following equations
ut+M([u]2s)LKu=|u|p−2uln|u|,(x,t)∈Ω×(0,+∞), | (1.4) |
where LK is a nonlocal integro-differential operator. They used the Galerkin approximation method and the potential well to prove the existence of a global weak solution with subcritical and critical states. According to the differential inequality, the blow-up solution of the equation is given. At the same time, the lower bound of the solution of problem (1.4) and the existence of the ground state solution of the corresponding steady-state problem was discussed. More details for fractional Laplacian equations with logarithmic nonlinearity can refer to [30,31,32].
Inspired by the above references, we study problem (1.1). Compared with problem (1.2), we consider the case of 1<p<N/s and discuss the global existence and finite time blow-up of the solutions. If p=2 and 1<α<N/(N−2s), we can turn problem (1.1) into problem (1.2). Compared with problem (1.3) and (1.4), we study the global existence and finite time blow-up of the solutions for fractional p-Laplacian Kirchhoff type equation with logarthmic nonlinearity. By the methods of the variational principle and Nehari manifold, as well as combining with the relevant theories and properties of the fractional Sobolev space definition, we consider both E(u0)<h and E(u0)=h cases and prove the global existence and the finite time blow-up of the solution for problem (1.1), and discuss the growth rate of the weak solutions and study ground-state solution of the corresponding steady-state problem.
The rest of the paper is organized as follws. In Section 2, we give some related definitions and lemmas. In Section 3, we prove the global existence and the finite time blow-up of the solution with subcritical state E(u0)<h of the problem (1.1), at the same time, we give the growth rate of the solutions and study ground-state solution of the corresponding steady-state problem. In Section 4, we prove the global existence and the finite time blow-up of the solution with critical state E(u0)=h of the problem (1.1).
In this section, we give some related definitions and Lemmas needed to prove the conclusions later. First of all, we define
r(ϱ)=(eϱ(e−1)Dαp+ϱ∗)1ϱ, | (2.1) |
where D∗ is the best embedding constant for Ws,p0(Ω)↪Lαp+ϱ(Ω),ϱ∈(0,p∗s−αp).
The energy functional is
E(u)=1αp[u]αps,p−1αp∫Ω|u|αpln|u|dx+1(αp)2∫Ω|u|αpdx. | (2.2) |
The Nehari functional is
I(u)=[u]αps,p−∫Ω|u|αpln|u|dx. | (2.3) |
And then, we define some sets as follows:
W:={u(x)∈Ws,p0(Ω) | I(u(x))>0, E(u(x))<h}∪{0}, | (2.4) |
V:={u(x)∈Ws,p0(Ω) | I(u(x))<0, E(u(x))<h}, | (2.5) |
the mountain pass level
h:=infu(x)∈NE(u(x)), | (2.6) |
the Nehari manifold
N={u(x)∈Ws,p0(Ω) | I(u(x))=0, u(x)≠0}. | (2.7) |
Further, define the positive set and the negative sets as follows
N+={u(x)∈Ws,p0(Ω) | I(u(x))>0}. | (2.8) |
N−={u(x)∈Ws,p0(Ω) | I(u(x))<0}. | (2.9) |
From (2.2) and (2.3), we have
E(u)=1αpI(u)+1(αp)2∫Ω|u|αpdx, | (2.10) |
In order to facilitate the proof of the main results, next we give the necessary Lemmas and definitions.
Lemma 2.1 Let u∈Ws,p0(Ω) and [u]s,p≠0, ρ∈(0,+∞), then:
(ⅰ) limρ→0+E(ρu(x))=0, limρ→+∞E(ρu(x))=−∞;
(ⅱ) There is an unique value ρ∗, such that
ddρE(ρu(x))⏐ρ=ρ∗=0; |
(ⅲ) E(ρu(x)) is increasing on (0,ρ∗), decreasing on (ρ∗,+∞) and takes the maximum at ρ∗;
(ⅳ) I(ρu(x))>0 for all 0<ρ<ρ∗, I(ρu(x))<0 for all ρ>ρ∗ and I(ρ∗u(x))=0.
Proof. (ⅰ) According to the known definition of E(u(x)) on (2.2), i.e.
E(u(x))=1αp[u(x)]αps,p−1αp∫Ω|u(x)|αpln|u(x)|dx+1(αp)2∫Ω|u(x)|αpdx, |
we have
E(ρu(x))=1αpραp[u(x)]αps,p−1αpραp∫Ω|u(x)|αpln|u(x)|dx−1αpραp∫Ω|u(x)|αpln|ρ|dx+1(αp)2ραp∫Ω|u(x)|αpdx=ραp(1αp[u(x)]αps,p−1αp∫Ω|u(x)|αpln|u(x)|dx−1αp∫Ω|u(x)|αplnρ+1(αp)2∫Ω|u(x)|αpdx), |
we can conclude that (ⅰ) holds.
(ⅱ) Through simple calculations, we have
ddρE(ρu(x))=ραp−1([u(x)]αps,p−∫Ω|u(x)|αpln|u(x)|dx−lnρ∫Ω|u(x)|αpdx), | (2.11) |
therefore, (ⅱ) holds.
(ⅲ) By the result in (ⅱ), we have
ddρE(ρu(x))=ραp−1([u(x)]αps,p−∫Ω|u(x)|αpln|u(x)|dx−lnρ∫Ω|u(x)|αpdx)>0, 0<ρ<ρ∗, |
and
ddρE(ρu(x))=ραp−1([u(x)]αps,p−∫Ω|u(x)|αpln|u(x)|dx−lnρ∫Ω|u(x)|αpdx)<0, ρ∗<ρ<+∞, |
thus, (ⅲ) holds.
(ⅳ) According to the (2.11) and
I(ρu(x))=ραp[u(x)]αps,p−ραp∫Ω|u(x)|αpln|u(x)|dx−ραp∫Ω|u(x)|αplnρdx, |
thus
I(ρu(x))=ρddρE(ρu(x)), |
then, I(ρu(x))>0 for all 0<ρ<ρ∗, I(ρu(x))<0 for all ρ>ρ∗ and I(ρu(x))=0, (iv) holds.
Lemma 2.2 [1,2] If ϱ∈(0,p∗s−αp), then:
eϱlnt≤tϱ, 1≤t<+∞. |
Proof. Set g(t)=lnt−tϱeϱ, t∈[1,+∞). By a simple derivative calculation of the function, we get g′(t)=1t−1eϱtϱ−1 and let g′(t)=0, then t∗=e1ϱ. Obviously t∗ is the maximum point of function g(t), thus g(t)≤g( t∗)=0 for all t∈[1,+∞). This proves the above inequality.
Lemma 2.3 If ϱ∈(0,p∗s−αp). Let u∈Ws,p0(Ω) and [u]s,p≠0, we have
(ⅰ) If 0<[u]s,p<r(ϱ), then I(u)>0;
(ⅱ) If I(u)≤0, then [u]s,p≥r(ϱ).
Proof. By Lemma 2.2 and the definition of Nehari function I(u), we have
I(u)=[u]αps,p−∫Ω|u(x)|αpln|u(x)|dx>[u]αps,p−1ϱ∫Ω(|u|<1)|u(x)|αpln|u|ϱdx−∫Ω(|u|≥1)|u(x)|αpln|u|dx≥[u]αps,p−1ϱ∥u∥αp+ϱαp+ϱ−1eϱ∥u∥αp+ϱαp+ϱ≥[u]αps,p−1ϱDαp+ϱ∗[u]αp+ϱs,p−1eϱDαp+ϱ∗[u]αp+ϱs,p=[u]αps,p(1−e−1eϱDαp+ϱ∗[u]ϱs,p ), |
we can get
I(u)>[u]αps,p(1−e−1eϱDαp+ϱ∗[u]ϱs,p). |
If 0<[u]s,p<r(ϱ), then
1−e−1eϱDαp+ϱ∗[u]ϱs,p>0, |
thus (ⅰ) holds.
Similarly, assume I(u)≤0, i.e.
1−e−1eϱDαp+ϱ∗[u]ϱs,p≤0, |
thus (ⅱ) holds.
Lemma 2.4 [2] If s∈(0,1), 1<p<N/s holds, then the functionals E(u) and I(u) are well-defined and continuous on Ws,p0(Ω). Moreover, E(u)∈C1(Ws,p0(Ω),R), and I(u)=⟨E′(u),u⟩ for all u∈Ws,p0(Ω).
Proof. Since
∫Ω|u|αpln|u|dx≤1ϱ‖u‖αp+ϱαp+ϱ≤1ϱDαp+ϱ∗[u]αp+ϱs,p, |
where 1≤α<p∗s/p, then we can claim that E(u) and I(u) are well-defined in Ws,p0(Ω). Further, Similar to Lemma 2.3 in [2], one can prove the that E(u)∈C1(Ws,p0(Ω),R), and I(u)=⟨E′(u),u⟩ for all u∈Ws,p0(Ω).
Lemma 2.5 [33] Let s∈(0,1) and p∈[1,+∞) such that sp<N. Let q∈[1,p∗), Ω⊆RN be a bounded extension domain for Ws,p(Ω) and ζ be a bounded subset of Lp(Ω). Suppose that
supf∈ζ∫Ω∫Ω|f(x)−f(x)|p|x−y|N+spdxdy<+∞, |
then ζ is pre-compact in Lq(Ω).
Lemma 2.6 Let s∈(0,1), 1<p<N/s, α∈[1,p∗s/p), t∈[0,T), and assume that u(x,t) is the solution of problem (1.1), then
ddt‖u‖22=−2I(u). |
Proof. By the definition of the weak solution, we have
∫Ωutudx+[u](α−1)ps,p∬R2N|u(x)−u(y)|p−2(u(x)−u(y))2|x−y|N+spdxdy=∫Ωu|u|αp−2uln|u|dx. |
So
12‖u‖22=−[u]αps,p+∫Ω|u|αpln|u|dx=−([u]αps,p−∫Ω|u|αpln|u|dx). |
Thus, we obtain
ddt‖u‖22=−2I(u). |
Definition 2.1 A function u(x,t) is called a weak solution of problem (1.1), where (x,t)∈Ω×[0,T). If u∈L∞(0,T;Ws,p0(Ω)) and ut∈L2(0,T;L2(Ω)), for all v∈Ws,p0(Ω), t∈(0,T), the following equation holds
∫Ωutvdx+[u](α−1)ps,p∬R2N|u(x)−u(y)|p−2(u(x)−u(y))(v(x)−v(y))|x−y|N+spdxdy=∫Ωv|u|αp−2uln|u|dx, |
with u(x,0)=u0(x) in Ws,p0(Ω). Moreover, for 0≤t<T, the following inequality holds
∫t0‖ur‖22dr+E(u)≤E(u0). | (2.12) |
Definition 2.2 (Maximal existence time) Let u(t) be a solution of problem (1.1), we define the maximal existence time T of u(t) as follows:
(ⅰ) If u(t) exists for 0≤t<+∞, then T=+∞.
(ⅱ) If there exists a t0∈(0,+∞) such that u(t) exists for 0≤t<t0, but doesn't exist at t=t0, then T=t0.
Definition 2.3 (Finite time blow-up) Let u(x) be weak solution of problem (1.1), We call u(t) a blow-up in finite time if the maximal existence time T is finite and
limt→T−∫T0‖u‖22dr=+∞. |
In this section, we use Galerkin approximation, potential well theory, Nehari manifold to study the problem (1.1) the global existence of the solution, blow-up in finite time of the solution with subcritical state E(u0)<h of the problem (1.1). In addition, we discuss the growth rate of the weak solution. Finally, we also discuss the ground state solution of the corresponding steady-state problem.
Theorem 3.1 Let α∈[1,p∗s/p), 1<p<N/s. u0∈Ws,p0(Ω), If E(u0)<h and I(u0)>0, then problem (1.1) admits a global weak solution u(t)∈L∞(0,T;Ws,p0(Ω)),ut∈L2(0,T;L2(Ω)) and u(t)∈W for all t∈[0,+∞).
Proof. By the definition of the weak solution, we take a set of smooth functions η=ηk(x) (k=1,2,⋅⋅⋅) such that {ηk(x)}∞k=1 is the basis function of Ws,p0(Ω), and then construct a approximate solutions um(t) of problem (1.1) as follows:
um=m∑k=1dkm(t)ηk(x), k=1,2,⋅⋅⋅, |
i.e. um : [0,T)⟼Ws,p0(Ω), um∈span{η1,⋅⋅⋅ηm}, which satisfy
∫Ωumtηkdx+[um]αp−ps,p∬R2N|um(x)−um(y)|p−2(um(x)−um(y))(ηk(x)−ηk(y))|x−y|N+spdxdy=∫Ωηk|um|αp−2umln|um|dx | (3.1) |
and
um(x,0)=m∑k=1bkmηk(x)→u0 in Ws,p0(Ω), | (3.2) |
where bkm=(um(0),ηk) are given constants, k=1,2,⋅⋅⋅,m. we use (⋅,⋅) to represent the inner product in L2(Ω).
Multiplying (3.1) by d′km(t), then summing k from 0 to m, and finally integrating t from 0 to t, we get
∫t0‖umr‖22dr+E(um)=E(um(0)) 0≤t≤T. |
According to (3.2), we obtain dkm(0)=bkm. Noticing E(u0)<h, I(u0)>0, we have
limm→+∞(∫t0‖umr‖22dr+E(um))=limm→+∞E(um(0))<h, |
and
limm→+∞I(um(0))=I(u0)>0, |
then for a sufficiently large m, we can obtain
∫t0‖umr‖22dr+E(um)=E(um(0))<h, | (3.3) |
and
I(um(0))=I(u0)>0, |
due to W:={u∈Ws,p0(Ω) | I(u)>0, E(u)<h}∪{0}, thus um(x,0)∈W, this is true if m is big enough.
Let m→+∞, 0≤t≤T, we prove um(t)∈W. Arguing by contraction, we suppose um(t)∉W, for sufficiently large m, then exists a t0∈(0,T) satisfying um(t0) is on the boundary of ∂W, we have
I(um(t0))=0, u(t0)≠0, |
thus can get um(t0)∈N. And because h=infu∈NE(u) which yields E(um(t0))≥h, this is paradoxically. Then um(t0)∈W for m→+∞ and 0≤t≤T.
By (3.3) and
E(um)=1αpI(um)+1(αp)2∫Ω|um|αpdx, |
we can get
∫t0‖umr‖22dr+1(αp)2‖um‖αpαp<h. |
For sufficiently large m, it yields
1(αp)2‖um‖αpαp<h, 0≤t≤T, | (3.4) |
∫t0‖umr‖22dr<h, 0≤t≤T, | (3.5) |
‖uαp−2m‖q=‖um‖αpαp≤Cαp∗[u]αps,p<Cαp∗rαp(ϱ), 0≤t≤T, q=αpαp−2, | (3.6) |
where C∗ is the best embedding constant for Ws,p0(Ω)↪Lαp(Ω). Thus, we get T=+∞, um(t)∈W for sufficiently large m and 0≤t<+∞.
Next, we prove um(t)∈L∞(0,T;Ws,p0(Ω)) and ut∈L2(0,T;L2(Ω)). According to the (3.4) (3.5) and (3.6), we have ut∈L2(0,T;L2(Ω)), u(t)∈L∞(0,T;Ws,p0(Ω)). Based on the above proof, there exists a u and subsequence {un} and {um} such that
un⇀u weakly in L2(0,+∞;Ws,p0(Ω)), | (3.7) |
un⇀u weakly star in L∞(0,+∞;Ws,p0(Ω)), | (3.8) |
uαp−2n⇀uαp−2 weakly star in L∞(0,+∞;Lq(Ω)), | (3.9) |
un→u a.e. Ω, | (3.10) |
unt⇀u wealky in L2(0,+∞;L2(Ω)). | (3.11) |
By (3.7) and (3.11), we obtain
un⇀u strongly in L2(0,+∞;Lαp(Ω)), | (3.12) |
then |u|αp−2unln|un|→|u|αp−2uln|u| a.e. in Ω×(0,+∞).
Since un(t)∈W and
∫Ω|un(t)|un(t)|αp−2ln|un(t)||αpdx≤∫Ω(|un(x)|≤1)||un(t)|αp−1ln|un(t)||αpdx+∫Ω(|un(x)|>1)||un(t)|αp−1ln|un(t)||αpdx≤1(eαp−e)αp|Ω|+(1eϱ)αp‖un‖(αp+ϱ−1)αp(αp+ϱ−1)αp≤1(eαp−e)αp|Ω|+(S(αp+ϱ−1)∗eϱ)αp[un](αp+ϱ−1)αps,p≤1(eαp−e)αp|Ω|+(S(αp+ϱ−1)∗eϱ)αpr(αp+ϱ−1)αp(ϱ), |
where S∗ is the imbedding constant for Ws,p0(Ω)↪L(αp+ϱ−1)αp(Ω), which implies
|u|αp−2unln|un|→|u|αp−2uln|u| weakly star in L∞(0,+∞; Lαp(Ω)). | (3.13) |
In (3.1), we take a fixed k, let m=n→+∞, then there is
∫Ωutηkdx+[u]αp−ps,p∬R2N|u(x)−u(y)|p−2(u(x)−u(y))(ηk(x)−ηk(y))|x−y|N+spdxdy=∫Ωηk|u|αp−2uln|u|dx |
and
∫Ωutvdx+[u]αp−ps,p∬R2N|u(x)−u(y)|p−2(u(x)−u(y))(v(x)−v(y))|x−y|N+spdxdy=∫Ωv|u|αp−2uln|u|dx, |
where v∈Ws,p0(Ω), t∈(0,+∞), and by (3.2) gives u(x,0)=u0(x) in Ws,p0(Ω).
Finally, we prove the following inequality
∫t0‖ur‖22dr+E(u)≤E(u0). |
In order to achieve the above result, we first consider
∫Ω|um|αpln|um|dx−∫Ω|u|αpln|u|dx≤0. |
Since ϱlns≤sϱ, s∈(0,+∞), ϱ>0, we have
∫Ω|um|αpln|um|dx−∫Ω|u|αpln|u|dx≤|∫Ω(|um|αpln|um|+uum|um|αp−2ln|um|−uum|um|αp−2ln|um|−|u|αpln|u|)dx|≤∫Ω|(um−u)um|um|αp−2ln|um||dx+|∫Ωu(um|um|αp−2ln|um|−u|u|αp−2ln|u|)dx|=‖um−u‖αp1ϱ‖um‖αp+ϱ−1αp+ϱ−1+|∫Ωu(um|um|αp−2−u|u|αp−2ln|u|)dx|→0 (m→+∞). |
By the weak lower semicontinuity and the above inequality, we obtain
E(u0)+1αp∫Ω|u|αpln|u|dx=lim infm→+∞(E(um(0))+1αp∫Ω|um|αpln|um|dx)=lim infm→+∞(E(um)+1αp∫Ω|um|αpln|um|dx+∫t0‖umr‖22dr)=lim infm→+∞(1αp[um]αps,p+1(αp)2‖um‖αpαp+∫t0‖umr‖22dr)≥lim infm→+∞1αp[um]αps,p+lim infm→+∞1(αp)2‖um‖αpαp+lim infm→+∞∫t0‖umr‖22dr≥1αp[u]αps,p+1(αp)2∫Ω|u|αpdx+∫t0‖ur‖22dr, |
which implies that the following inequality holds
∫t0‖ur‖22dr+E(u)≤E(u0). |
Theorem 3.2. Assume that α∈[1,p∗s/p), 1<p<N/s hold, and if u0∈Ws,p0(Ω), E(u(0))<h, I(u(0))<0, u(t) is the weak solution of problem (1.1), then u(t) blows up in a finite time T (T>0) and satisfies the following equation
limt→T∫t0‖u‖22dr=+∞. |
In addition, if E(u0)≤0, then the solution u(t) of problem (1.1) also satisfies
‖u‖22≥(1M(t))2αp−2, |
where M(t)=‖u0‖2−αp22−4αp−2t|Ω|2−αp2(αp)−1.
Proof. Let u(t) be weak solution of problem (1.1), and E(u0)<h, I(u0)<0, we first define
Q(t):=∫t0‖u‖22dr, |
then, we obtain
Q′(t)=‖u‖22, |
and
Q″(t)=2(u,ut)=−2I(u). | (3.14) |
By (2.12), (3.14)and the following equation
E(u)=1αpI(u)+1(αp)2‖u‖αpαp, |
we can get
Q″(t)=−2I(u)≥2αp∫t0‖u‖22dr+2αp‖u‖αpαp−2αpE(u0). | (3.15) |
Due to
∫t0(ur,u)dr=12∫t0ddt‖u‖22dr=12(‖u‖2−‖u0‖2), |
square both sides of the above equation, we have
(∫t0(ur,u)dr)2=14((Q′(t))2−2‖u0‖22Q′(t)+‖u0‖42). | (3.16) |
By (3.15), (3.16) and the Schwartz's inequality, we can get
Q″(t)Q(t)−2αp(∫t0(ur,u)dr)2≥2αp∫t0‖ur‖22dr∫t0‖u‖22−2αp(∫t0(ur,u)dr)2+2αp‖u‖αpαpQ(t)−2αpE(u0)Q(t), |
i, e.
Q″(t)Q(t)−αp2(Q′(t))2≥2αp(∫t0‖ur‖22dr∫t0‖u‖22dr−(∫t0(ur,u)dr)2)+2αp‖u‖αpαpQ(t)−2αpE(u0)Q(t)−αpQ′(t)‖u0‖22+αp2‖u0‖42≥2αp‖u‖αpαp Q(t)−2αpE(u0)Q(t)−αpQ′(t)‖u0‖22+αp2‖u0‖42≥2αp‖u‖αpαp Q(t)−2αpE(u0)Q(t)−αpQ′(t)‖u0‖22. |
Now, we discuss the two cases E(u0)≤0, and 0<E(u0)<h.
(a) If E(u0)≤0, then
Q″(t)Q(t)−αp2(Q′(t))2≥2αp‖u‖αpαp Q(t)−αpQ′(t)‖u0‖22. | (3.17) |
Due to I(u)<0 for all t∈[0,T), so Q″(t)=−2I(u)>0, Q′(t)>Q′(0)=‖u0‖22>0. Then for all δ∈[0,t−t0), where t0≥0,t≥t0 and Q′(t)>0, further we obtain
Q(t)≥δQ′(t0)>δQ′(0). | (3.18) |
Moreover, we construct the following functional
f(t)=∫t0∫Ω|u(x,r)|2dxdr+(T−t)∫Ω|u0|2dx, 0≤t<T. |
By simple calculation and Lemma 5, we have
f′(t)=∫Ω|u(x,t)|2dx−∫Ω|u0|2dx, |
and
f″(t)=2(ut,u)=−2I(u). |
Since I(u)<0, thus
f″(t)=2(ut,u)=−2I(u)>0. |
By (2.10), (2.12) and Holder's inequality, we obtain
f″(t)=−2αpE(u(t))+2αp‖u(t)‖αpαp≥2αp∫t0∥ur(r)∥22dr+2αp‖u(t)‖αpαp−2αpE(u0)≥2αp‖u(t)‖αpαp≥2αp|Ω|2−αp2‖u(t)‖αp2=2αp|Ω|2−αp2(γ(t))αp2, |
where γ(t)=f′(t)+∫Ω|u0|2dx, and γ′(t)≥2(αp)−1|Ω|2−αp2(γ(t))αp2, by the differential inequality, we obtain
‖u‖22≥(1M(t))2αp−2, | (3.19) |
where M(t)=‖u0‖2−αp22−4αp−2t|Ω|2−αp2(αp)−1. By (3.18) (3.19), for sufficiently large t, we have
Q″(t)Q(t)−αp2(Q′(t))2>0. |
(b) If 0<E(u0)<h, by (3.18), αp>2 and Holder's inequality, then for a sufficiently large time t, we have
Q″(t)Q(t)−αp2(Q′(t))2≥2αp‖u‖αpαp Q(t)−2αpE(u0)Q(t)−αpQ′(t)‖u0‖22=(1αp‖u‖αpαp Q(t)−2αpE(u0)Q(t))+(1αp‖u‖αpαpQ(t)−αpQ′(t)‖u0‖22)≥((1αpQ′(t)−2αpE(u0))Q(t))+(1αp‖u‖αpαpQ(t)−αpQ′(t)‖u0‖22)≥((1αpQ′(t)−2αpE(u0))Q(t))+(1αp|Ω|2−αp2‖u(t)‖αp2Q(t)−αpQ′(t)‖u0‖22)>0. |
It implies for a sufficiently large time t, there exists a finite time T>0 such that
limt→T−Q(t)=+∞. |
Theorem 3.3 If α∈[1,p∗s/p), 1<p<N/s hold, then there exists a v∈N that satisfies the equation E(v)=limu∈NE(u)=h, and v is the ground state solution of the following steady-state problem
{M([u]ps,p)(−Δ)spu=|u|αp−2uln|u|,x∈Ω,u=0,x∈RN∖Ω. |
Proof. By the definition of h in (2.6), due to u∈N, I(u)=0, we have
h=infu∈NE(u)=infu∈N{1αpI(u)+1(αp)2∫Ω|u|αpdx}=infu∈N{1(αp)2‖u‖αpαp}. |
Let {un} be a minimizing sequence, where {un}⊂N and limn→+∞E(un)=h, then
E(un)=1(αp)2‖un‖αpαp=h. |
Since α∈[1,p∗s/p), 1<p<N/s, it implies that {un} is bound in Ws,p0(Ω).
According to the above discussion, there exists a subsequence of {un}. For the convenience, we still use {un} to represent the subsequence, and further obtain
un⇀v weakly in Ws,p0(Ω), |
un⇀v strongly in Lαp(Ω), |
un→v a.e. in Ω. |
By Sobolev embedding theorem and logarithmic inequality, we have
∫Ω∗|un|αpln|un|dx=−∫Ω∗(|un|<1)|un|αpln|un|dx+∫Ω∗(|un|≥1)|un|αpln|un|dx≤1αpe|Ω∗|+1ϱe‖un‖αp+ϱαp+ϱ≤1αpe|Ω∗|+1ϱeDαp+ϱ∗[un]αp+ϱαp+ϱ, |
where Ω∗⊂Ω is a measurable subset, thus we can get that |un|αpln|un| is uniformly bound. By integral convergence theorem and |un|αpln|un|→|v|αpln|v| a.e. in Ω, we have
limn→+∞∫Ω|un|αpln|un|dx→∫Ω|v|αpln|v|dx. | (3.20) |
By Lemma 2.3(ii) and {un}⊂N, I(un)=0, we can get
0<r(ϱ)≤[un]αp=(∫Ω|un|αpln|un|dx)1αp. |
In other words
0 < \int_\Omega|v|^{\alpha p}\ln|v|dx, |
thus, we can conclude that v\neq0.
According to (ii) of Lemma 2.1 , there exists a \rho^* > 0 satifying \rho^*v\in\mathcal{N}, \ I(\rho^*v) = 0 , i.e.
I(\rho^*v) = (\rho^*)^{\alpha p}[v]^{\alpha p}_{s, p}-(\rho^*)^{\alpha p}\int_\Omega |v|^{\alpha p}\ln|v|dx-(\rho^*)^{\alpha p}\ln{\rho^*}\int_\Omega |v|^{\alpha p}dx = 0. |
Let
b(\rho): = I(\rho v) = (\rho)^{\alpha p}[v]^{\alpha p}_{s, p}-(\rho)^{\alpha p}\int_\Omega |v|^{\alpha p}\ln|v|dx-(\rho)^{\alpha p}\ln{\rho}\int_\Omega |v|^{\alpha p}dx = 0, |
by (iii) of Lemma 2.1 and taking I(v) < 0 , [u(x)]^{\alpha p}_{s, p} < \int_\Omega|u|^{\alpha p}\ln|u(x)|dx , we can be sure that 0 < \rho^* < 1.
Then by the definition of h , the weak lower semicontinuity and (3.20), we obtain
h = \lim\limits_{n\rightarrow+\infty}\inf E(u_n)\geq E(v), |
and
h = \lim\limits_{n\rightarrow+\infty}\{\frac{1}{(\alpha p)^2}\|u_n\|^{\alpha p}_{\alpha p} \}\geq\lim\limits_{n\rightarrow+\infty}\inf \|u_n\|^{\alpha p}_{\alpha p}\geq \frac{1}{(\alpha p)^2}\|v\|^{\alpha p}_{\alpha p}. |
By simply calculating, we can get
E(\rho^*v) = \big(\frac{1}{\alpha p}\big)^2(\rho^*)^{\alpha p}\|v\|^{\alpha p}_{\alpha p} < \big(\frac{1}{\alpha p}\big)^2\|v\|^{\alpha p}_{\alpha p}. |
This contradicts our definition of E(\rho^*v)\geq h , so we can conclude I(v) = 0, \ h = E(v) = \inf\limits_{u\in\mathcal{N}}E(u).
Next, we prove v is the ground state solution of the steady-state problem. From the above proof, we obtain E(v) = h, \ I(v) = 0. By the theory of Lagrange multipliers, there exists \xi\in\mathbb{R} such that
E^{'}(v)-\xi I^{'}(v) = 0, |
so we have
\xi\langle I^{'}(v), v\rangle = \langle E^{'}(v), v\rangle = I(v) > 0. |
Since I(v) = [v]^{\alpha p}_{\alpha p}-\int_\Omega|v|^{\alpha p}\ln|v|dx, then there is
I^{'}(v) = {\alpha p}[v]^{\alpha p-1}_{\alpha p}-{\alpha p}\int_\Omega|v|^{\alpha p-1}\ln|v|dx-\int_\Omega|v|^{\alpha p-1}dx. |
Thus
\xi\langle I^{'}(v), v\rangle = \alpha p[v]^{\alpha p}-{\alpha p}\int_\Omega|v|^{\alpha p}\ln|v|dx-\int_\Omega|v|^{\alpha p}dx. |
Note that I(v) = 0, \ [v]^{\alpha p}_{s, p} = \int_\Omega|v|^{\alpha p}\ln|v|dx , then
\xi\langle I^{'}(v), v\rangle = \alpha p[v]^{\alpha p}-{\alpha p}\int_\Omega|v|^{\alpha p}\ln|v|dx-\int_\Omega|v|^{\alpha p}dx = -\int_\Omega|v|^{\alpha p}dx < 0, |
thus, \xi = 0, \ E^{'}(v) = 0. We get that v is the ground state solution of the steady-state problem.
In this section, we will discuss the global existence and the finite time blow-up of weak solutions of problem (1.1) in the critical initial energy state (E(u_0) = h) .
Theorem 4.1 Assume that p\in(1, N/s), \ \alpha\in[1, p^*_s/p), \ u_0\in W^{s, p}_0(\Omega) and E(u_0) = h, \ I(u_0)\geq0 hold, then problem (1.1) admits a global weak solution u(t)\in L^\infty(0, T; W^{s, p}_0(\Omega)), \ u_t\in L^2(0, T; L^2(\Omega)) and u(t)\in \overline{W} for all t\in[0, +\infty).
Proof. We take a function \rho_m which satisfies \rho_m > 0 and \lim\limits_{n\rightarrow+\infty}\rho_m = 1 . Let u(x, 0) = u_{0m}(x) = \rho_mu_0(x), x\in\Omega , for the following equations
\begin{equation} \left\{ \begin{array}{@{}l@{\quad}l} u_{t}+M([u]^{p}_{s, p})(-\Delta)^{s}_{p}u = |u|^{\alpha{p}-2}u\ln{|u|} , \; \; \; \; &\text{in} \ \Omega\times(0, T), \\ u(x, 0) = u_{0m}(x) = \rho_mu_0, \; \; \; \; &\text{in} \ \Omega, \\ u = 0, \; \; \; \; &\text{in} \ \partial{\Omega}\times(0, T).\\ \end{array}\right. \end{equation} | (4.1) |
Since E(u_0) = h , it implies [u_0]_{s, p}\neq0. By Lemma (2.1) and I(u_0)\geq0, 0 < \rho_m < 1 , we obtain
[u_0]^{\alpha p}_{s, p}\geq\int_\Omega|u_0|^{\alpha p}\ln|u_0|dx, |
and
(\rho)^{\alpha p}\ln{\rho}\int_\Omega |u_0|^{\alpha p}dx < 0. |
By (iv) of lemma 2.1 \big(\rho_m\frac{d}{d\rho_m}E(\rho_mu_0) = I(\rho_mu_0) \big) and
\begin{split} I(\rho u_0) = &\rho^{\alpha p}[u_0]^{\alpha p}_{s, p}-\rho^{\alpha p}\int_\Omega |u_0|^{\alpha p}\ln|u_0|dx-\rho^{\alpha p}\ln{\rho}\int_\Omega |u_0|^{\alpha p}dx\\ > &\rho^{\alpha p}[u_0]^{\alpha p}_{s, p}-\rho^{\alpha p}\int_\Omega |u_0|^{\alpha p}\ln|u_0|dx\\ = &\rho^{\alpha p}\big([u_0]^{\alpha p}_{s, p}-\int_\Omega |u_0|^{\alpha p}\ln|u_0|dx\big)\\ \geq&0, \end{split} |
we have I(\rho_mu_0) > 0. (i.e. \rho_m\frac{d}{d\rho_m}E(\rho_mu_0) = I(\rho_mu_0) > 0 ). Then E(\rho_m u(x)) is monotonically increasing on (0, \rho^*) , we can get
E(u_{0m}) = E(\rho_mu_0) < E(u_0) = h. |
From Theorem 3.1, it follows that for each m , the above problem (4.1) admits a global weak solution u_m(t) , where u_m(t)\in L^\infty(0, +\infty; W^{s, p}_0(\Omega)), \ u_{mt}\in L^{2}(0, +\infty; L^2(\Omega)), moreover u_m(t)\in W for all t\in[0, +\infty) and satisfying
\begin{split} \int_\Omega u_{mt}\varphi dx+ &[u_m]^{\alpha p-p}_{s, p}\iint_{R^{2N}}\frac{|u_m(x)-u_m(y)|^{p-2}(u_m(x)-u_m(x)(\varphi(x)-\varphi(y))}{|x-y|^{N+sp}}dxdy\\ = &\int_\Omega \varphi |u_m|^{\alpha p-2} u_m\ln|u_m|dx, \ \ \ \ \ \ (\forall\ \varphi \in W^{s, p}_0(\Omega)\ , \ t > 0), \\ \end{split} |
in addition
\begin{equation} \int^t_0\|u_{mr}\|^2_2dr+E(u_m(t)) = E(u_{0m}) < h. \end{equation} | (4.2) |
By (4.2) and the following equation
E(u_m(t)) = \frac{1}{\alpha p}I(u_m(t))+\frac{1}{(\alpha p)^2}\int_\Omega |u_m(t)|^{\alpha p}dx, |
we have
\int^t_0\|u_{mr}\|^2_2dr+\frac{1}{(\alpha p)^2}\|u_m\|^{\alpha p}_{\alpha p} < h. |
The remainder of the proof is similar to that in the proof of Theorem 3.1.
Theorem 4.2 Let u(t) be the weak solution of problem (1.1), assume that p\in(1, N/s), \ \alpha\in[1, p^*_s/p), \ u_0\in W^{s, p}_0(\Omega) and E(u_0) = h, \ I(u_0) < 0 hold, then u(t) blows up in a finite time T_*.
Proof. If T_* = +\infty , taking Y(t) = \int^t_0\|u\|^2_2dr, we have
Y^{'}(t) = \|u\|^2_2, |
and
\begin{equation} Y^{''}(t) = 2(u, u_t) = -2I(u). \end{equation} | (4.3) |
By (2.12), (4.3) and the following equation
E(u) = \frac{1}{\alpha p}I(u)+\frac{1}{(\alpha p)^2}\int_\Omega|u|^{\alpha p}dx, |
we can get
\begin{equation} Y^{''}(t) = -2I(u)\geq2{\alpha p}\int^t_0\|u\|^2_2dr+\frac{2}{\alpha p}\|u\|^{\alpha p}_{\alpha p}-2{\alpha p}h. \end{equation} | (4.4) |
Since
\int^t_0(u_r, u)dr = \frac{1}{2}\int^t_0\frac{d}{dt}\|u\|^2_2dr = \frac{1}{2}(\|u\|^2_2-\|u_0\|^2_2), |
squaring both sides of the above equation, we have
\begin{equation} \Big(\int^t_0(u_r, u)dr\Big)^2 = \frac{1}{4}\Big((Y^{'}(t))^2-2\|u_0\|^2_2Y^{'}(t)+\|u_0\|^4_2\Big). \end{equation} | (4.5) |
By (4.4), (4.5) and the Schwartz's inequality, we can get
\begin{split} Y^{''}&(t)Y(t)-2{\alpha p}\Big(\int^t_0(u_r, u)dr\Big)^2\\ &\geq2{\alpha p}\int^t_0\|u_r\|^2_2dr\int^t_0\|u\|^2_2-2{\alpha p}\Big(\int^t_0(u_r, u)dr\Big)^2+\frac{2}{\alpha p}Y(t)\int_\Omega|u|^{\alpha p}dx-2{\theta p}hY(t), \\ \end{split} |
i, e.
\begin{split} Y^{''}&(t)Y(t)-\frac{\alpha p}{2}(Y^{'}(t))^2\\ &\geq2{\alpha p}\Big(\int^t_0\|u_r\|^2_2dr\int^t_0\|u\|^2_2dr-\big(\int^t_0(u_r, u)dr\big)^2\Big)+\frac{2}{\alpha p}Y(t)\int_\Omega|u|^{\alpha p}dx\\ &-2{\alpha p}hY(t)-{\alpha p}Y^{'}(t)\|u_0\|^2_2+\frac{\alpha p}{2}\|u_0\|^4_2\\ &\geq\frac{2}{\alpha p} Y(t)\int_\Omega|u|^{\alpha p}dx-2{\alpha p}hY(t)-{\alpha p}Y^{'}(t)\|u_0\|^2_2\\ & = \big(\frac{1}{\alpha p}Y(t)\int_\Omega|u|^{\alpha p}dx-2{\alpha p}hY(t)\big)+\big(\frac{1}{\alpha p}Y(t)\int_\Omega|u|^{\alpha p}dx-{\alpha p}Y^{'}(t)\|u_0\|^2_2\big) \end{split} |
Due to I(u) < 0 for all t\in[0, T) , so Y{''}(t) = -2I(u) > 0 , Y^{'}(t) > Y^{'}(0) = \|u_0\|^2_2 > 0 . For all \delta\in[0, t-t_0), where t_0\geq0, t\geq t_0 and Y^{'}(t) > 0, we obtain
\begin{equation} Y(t)\geq\delta Y^{'}(t_0) > \delta Y^{'}(0). \end{equation} | (4.6) |
Taking |u| > 1 and noting that {\alpha p} > 2, we have
\begin{equation} \frac{1}{\alpha p}\int_\Omega|u|^{\alpha p}dx-2{\alpha p}h > \frac{1}{\alpha p}\int_\Omega|u|^{2}dx-2{\alpha p}h > \frac{1}{\alpha p}\int_\Omega|u_0|^{2}dx-2{\alpha p}h. \end{equation} | (4.7) |
Moreover, by Holder's inequality, we have
\begin{equation} \|u(t)\|^{\alpha p}_{\alpha p}\geq|\Omega|^{\frac{2-\alpha p}{2}}\|u(t)\|^{\alpha p}_2. \end{equation} | (4.8) |
By (4.6), (4.7), (4.8), for sufficiently large t , it implies that
\frac{1}{\alpha p}Y(t)\int_\Omega|u|^{\alpha p}dx-2{\alpha p}hY(t) > 0, |
and
\frac{1}{\alpha p}Y(t)\int_\Omega|u|^{\alpha p}dx-{\alpha p}Y^{'}(t)\|u_0\|^2_2 > 0. |
So
Y^{''}(t)Y(t)-\frac{\alpha p}{2}(Y^{'}(t))^2 > 0, |
which gives
\big(Y^{-b}(t)\big)^{''} = \frac{-b}{Y^{b+2}(t)}\big(Y(t)Y^{''}(t)-(b+1)(Y^{'}(t)^2)\big)\leq0, \ \ \ b = \frac{\alpha p-2}{2}. |
It implies for a sufficiently large time t , there exists a finite time T_* such that
\lim\limits_{t\rightarrow T_*}Y^{-b}(t) = 0, |
and
\lim\limits_{t\rightarrow T_*}Y(t) = +\infty. |
This is contradictory to our assumption that T_* = +\infty.
Remark 1 . Theorems 3.1 and 4.1 show that E(u_0)\leq h and I(u_0) > 0 holds, then problem (1.1) admits a global weak solution u(t)\in L^\infty\big(0, T; W^{s, p}_0(\Omega)\big), \ u_t\in L^2\big(0, T; L^2(\Omega)\big) and u(t)\in W for all t\in[0, +\infty).
Remark 2 . One can see from Theorems 3.2 and 4.2 that blow-up of the weak solutions can always occur if E(u_0)\leq h, \ I(u_0) < 0 holds.
In this work, we study the initial-boundary value problem for a class of fractional p -Laplace Kirchhoff diffusion equation with logarithmic nonlinearity. For both subcritical and critical states, by means of the Galerkin approximations, the potential well theory and the Nehari manifold, we prove the global existence and finite time blow-up of the weak solutions. Further, we give the growth rate of the weak solutions and study ground-state solution of the corresponding steady-state problem. Compared with problem (1.2), we consider the case of 1 < p < N/s and discuss the global existence and finite time blow-up of the solutions. Compared with problem (1.3) and (1.4), we study the well-posedness of the solution for the fractional p-Laplacian Kirchhoff type evolution equation with logarithmic nonlinearity.
This research was supported by the Project for Young Talents Growth of Guizhou Provincial Department of Education under(Grant No.Ky[2017]133), and by the project of Guizhou Minzu University under (Grant No.16yjrcxm002 and No.GZMU[2019]YB04).
The authors declare no conflict of interest.
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