In this paper, we study the initial boundary value problem for a class of fractional p-Laplacian Kirchhoff type diffusion equations with logarithmic nonlinearity. Under suitable assumptions, we obtain the extinction property and accurate decay estimates of solutions by virtue of the logarithmic Sobolev inequality. Moreover, we discuss the blow-up property and global boundedness of solutions.
Citation: Peng Shi, Min Jiang, Fugeng Zeng, Yao Huang. Initial boundary value problem for fractional p-Laplacian Kirchhoff type equations with logarithmic nonlinearity[J]. Mathematical Biosciences and Engineering, 2021, 18(3): 2832-2848. doi: 10.3934/mbe.2021144
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In this paper, we study the initial boundary value problem for a class of fractional p-Laplacian Kirchhoff type diffusion equations with logarithmic nonlinearity. Under suitable assumptions, we obtain the extinction property and accurate decay estimates of solutions by virtue of the logarithmic Sobolev inequality. Moreover, we discuss the blow-up property and global boundedness of solutions.
In this paper, we study the extinction and the blow-up for the following fractional p-Laplacian Kirchhoff type equations with logarithmic nonlinearity.
{ut+M(‖u‖p)(−Δ)spu=λ|u|r−2uln|u|−β|u|q−2u,in Ω×(0,T),u(0)=u0,in Ω,u=0,on ∂Ω×(0,T), | (1.1) |
where
‖u‖=(∬Q|u(x)−u(y)|p|x−y|N+spdxdy)1p, |
Q=R2N∖(CΩ×CΩ), CΩ=RN∖Ω, Ω⊂RN (N>2s) is a bounded domain with Lipschitz boundary, s∈(0,1), 1<p<2, 1<q≤2, r>1, λ, β>0, (−Δ)sp is the fractional p-Laplacian operator and satisfies
(−Δ)spu(x)=2limγ→0+∫RN∖Bγ(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, Bγ(x)⊂RN is the ball with center x and radius γ. u0(x)∈L∞(Ω)∩Ws,p0(Ω) is a nonzero non-negative function, where L∞(Ω) and Ws,p0(Ω) are Lebesgue space and fractional Sobolev space respectively, which will be given in section 2. M(⋅) is a Kirchhoff function with the following assumptions
(M1) 0<s<1,M(τ):=a+bθτθ−1 for τ∈R+0:=[0,+∞) (a>0,b≥0 are two constants), θ≥1;
(M2) M:R+0→R+0∖{0} is continuous and there exits m0≥0 such M(τ)≥m0 for all τ≥0.
It is worth pointing out that the interest in studying problems like (1.1) relies not only on mathematical purposes, but also on their significance in real models. For example, in the study of biological populations, we can use u(x,t) to represent the density of the population at x at time t, the term (−Δ)spu represents the diffusion of density, μ|u|q−2u represents the internal source and λ|u|r−2uln|u| denotes external influencing factors. For more practical applications of problems like (1.1), please refer to the studies [1,2,3].
Compared with integer-order equations, it is very difficult to study the problem (1.1), which contains both non-local terms (including fractional p-Laplacian operators and Kirchhoff functions) and logarithmic nonlinearity. For the fractional order theory, we refer the readers to the studies [4,5,6]. In [7,8], the authors use Sobolev space and Nehari manifold to study the existence of solutions for fractional equations. In [9,10], the solutions for fractional equations are discussed by virtue of Nehari manifold and fibrillation diagram. By using different methods from above, the properties of the solutions for such partial differential equations are considered by the method of variational principle and topological theory in the the literature [11,12,13]. Moreover, the authors prefer to use potential well theory, Galerkin approximation and Nehari manifold method to prove the existence of solutions, decay estimation and blow-up, we refer the reader to the literature [14,15,16].
Existence, extinction and blow-up of solutions are three important topics which regard parabolic problems; in particular, the study of extinction properties has made great progress in recent years. In [17], Liu considered the following initial boundary value problem for the fractional p-Laplacian equation
ut−div(|∇u|p−2∇u)+βuq=λur, x∈Ω, t>0, | (1.2) |
where 1<p<2, q≤1 and r,λ,β>0. By employing the differential inequality and comparison principle, they obtained the extinction and the non-extinction of weak solutions. In [18], Sarra Toualbia et al. considered the following initial boundary value problem of a nonlocal heat equations with logarithmic nonlinearity
ut−div(|∇u|p−2∇u)=|u|p−2ulog|u|−∮Ω|u|p−2ulog|u|dx, x∈Ω, t>0, | (1.3) |
where p∈(2,+∞). By using the logarithmic Sobolev inequality and potential well method, they obtained decay, blow-up and non-extinction of solutions. In [19], Xiang and Yang studied the first initial boundary value problem of the following fractional p-Kirchhoff type
ut+M([u]ps,p)(−Δ)spu=λ|u|r−2u−μ|u|q−2u, (x,t)∈Ω×(0,∞), | (1.4) |
where M:[0,∞)→(0,∞) is a continuous function, 0<s<1<p<2, 1<q≤2, r>1, λ,μ>0. Under suitable assumptions, they proved the extinction and non-extinction of solutions and perfected the Gagliardo-Nirenberg inequality. For more information on the extinction properties of the solution, please refer to the studies [20,21,22,23].
Inspired by the above works, we overcome the research difficulties of logarithmic nonlinearity, p-Laplace operator and Kirchhoff coefficients in problem (1.1) based on the potential well theory, Nehari manifold and differential inequality methods, we give the extinction and the blow-up properties of solutions. In addition, we give the global boundedness of the solution by appropriate assumptions. To the best of our knowledge, it is the first result in the literature to investigate the extinction and blow-up of solutions for fractional p-Laplacian Kirchhoff type with logarithmic nonlinearity.
In order to introduce our main results, we first give some related definitions and sets.
Definition 1.1(Weak solution). A function u(x,t) is said to be a weak solution of problem (1.1), if (x,t)∈Ω×[0,T), u∈Lp(0,T;Ws,p0(Ω))∩C(0,T;L2(Ω)), ut∈L2(0,T;L2(Ω)), u(x,0)=u0(x)∈Ws,p0(Ω), for all v∈Ws,p0(Ω), t∈(0,T), the following equation holds
∫Ωutvdx+M(‖u‖p)⟨u,v⟩=λ∫Ωv|u|r−2uln|u|dx−β∫Ωv|u|q−2udx, |
where
⟨u,v⟩=∬Q|u(x)−u(y)|p−2(u(x)−u(y))(v(x)−v(y))|x−y|N+spdxdy. |
Definition 1.2(Extinction of solutions). Let u(t) be a weak solution of problem (1.1). We call u(t) an extinction if there exists T>0 such that u(x,t)>0 for all t∈(t,T) and u(x,t)≡0 for all t∈[T,+∞).
Define the following two functionals on Ws,p0(Ω)
E(u)=1pa‖u‖p+1pb‖u‖θp−λ1r∫Ω|u|rln|u|dx+λ1r2∫Ω|u|rdx+β1q∫Ω|u|qdx, | (1.5) |
I(u)=a‖u‖p+θb‖u‖θp−λ∫Ω|u|rln|u|dx+β‖u‖qq. | (1.6) |
Let
Z={u∈Lp(0,T;Ws,p0(Ω))∩C(0,T;L2(Ω)),ut∈L2(0,T;L2(Ω))}. |
Remark 1 Since u∈Z, 1<p<2, M(⋅) is a continuous function and
∫Ω|u|rln|u|dx≤1σ‖u‖r+σr+σ≤1σCr+σr+σ‖u‖r+σ, |
where 0<σ<p∗s−r, then we can claim that E(u) and I(u) are well-defined in Ws,p0(Ω). Further, by arguing essentially as in [24], one can prove the that
u↦∫Ω|u|rln|u|dx |
is continuous from Ws,p0(Ω) to R. It follows that E(u) and I(u) are continuous.
Define some sets as follows
W:={u∈Ws,p0(Ω) | I(u)>0, E(u)<h}∪{0}, | (1.7) |
V:={u∈Ws,p0(Ω) | I(u)<0, E(u)<h}, | (1.8) |
the mountain pass level
h:=infu∈NE(u), | (1.9) |
the Nehari manifold
N:={u∈Ws,p0(Ω)∖{0} | I(u)=0}. | (1.10) |
Moreover, we define
N+:={u∈Ws,p0(Ω) | I(u)>0}, | (1.11) |
N−:={u∈Ws,p0(Ω) | I(u)<0}. | (1.12) |
Let λ1 be the first eigenvalue of the problem
(−Δ)spu=λ|u|p−2u in Ω, u|RN∖Ω=0, | (1.13) |
and ϕ(x)>0 a.e. in Ω be the eigenfunction corresponding to the eigenvalue λ1>0, ϕ(x)∈L∞(Ω) and ‖ϕ‖L∞(Ω)≤1.
First, we give some results satisfying I(u0)>0 and q=2.
Theorem 1.1 Assume that I(u0)>0, r=p and q=2. Let m0 be as in assumption (M2), and let
l:=2N−(s+N)psp, P1:=m0λ1L(p,Ω)+ln(R), P2:=λ1m0lpp−1[λ1L(p,Ω)+ln(R)](p+l−1)p−1, |
where L(p,Ω) and R are given in Lemma 2.1 and Lemma 2.5. Then, there exist positive constants C1, C2, T1 and T2 such that
(ⅰ) If λ<λ1P1, then the weak solution of (1.1) vanishes in the sense of ‖⋅‖2 as t→+∞.
(ⅱ) If 2N/(N+2s)<p<2 and λ<λ1P1 or 1<p≤2N/(N+2s) and λ<P2, then the nonnegative solutions of (1.1) vanish in finite time, and
{‖u‖2≤[(‖u0‖2−p2+C1β)e(p−2)βt−C1β]12−p,t∈[0,T1),‖u‖2≡0,t∈[T1,∞), |
for 2N/(N+2s)<p<2, and
{‖u‖l+1≤[(‖u0‖2−pl+1+C2β)e(p−2)βt−C2β]12−p,t∈[0,T2),‖u‖l+1≡0,t∈[T2,∞), |
for 1<p<2N/(N+2s).
Theorem 1.2 Assume that I(u0)>0, 0<σ≤p∗s−r, r>p and q=2. Let m0 be as in assumption (M2), and let
P3:=max{m0L(r,Ω)Rr−p+εΦ,βΦεr(ϑ1−1)p−r(1−ϑ1)}, P4:=max{m0lppε1(p+l−1)p,βεr2(1−ϑ2)p−r2(1−ϑ2)1}, |
where
Φ=ln(R)|Ω|s1−rs1Cr(1−ϑ1)p∗s, p∗s=NpN−sp, s1=2ϑ1+p∗s(1−ϑ1),ϑ1=2(r−p)r(2−p), r2=p(l+r+σ−1)l+p−1, |
Cp∗s is the best constant of embedding from Ws,p0(Ω) to Lp∗s(Ω), L(p,Ω) and R are given in Lemma 2.1 and Lemma 2.5, and ε,ε1>0 are two constants. Then, there exist positive constants C4, C5, C6, C7, T3 and T4 such that the non-negative weak solution of problem (1.1) vanishes in finite time and
{‖u‖2≤[(‖u0‖2−pl+1+C5C4)e(p−2)C4t−C5C4]12−p,t∈[0,T3),‖u‖2≡0,t∈[T3,∞), |
for 2N/(N+2s)≤p<2, λ<P3, and
{‖u‖l+1≤[(‖u0‖2−pl+1+C6C7)e(p−2)C7t−C6C7]12−p,t∈[0,T4),‖u‖l+1≡0,t∈[T4,∞), |
for 1<p<2N/(N+2s), λ<P4.
Secondly, we give some results satisfying I(u0)>0 and q<2.
Theorem 1.3 Assume that I(u0)>0, p=r, l1>l≥1 and 1<q<2. Let m0 be as in assumption (M2), and let
P5:=λ1m0l1pp−1[λ1L(p,Ω)+ln(R)](p+l1−1)p−1, |
where L(p,Ω) and R are given in Lemma 2.1 and Lemma 2.5. If 2N/(N+2s)<p<2 with λ<λ1P1 or 1<p≤2N/(N+2s) with λ<P5, then the non-negative weak solution of problem (1.1) vanishes in finite time for any non-negative initial data.
Theorem 1.4 Assume that I(u0)>0, l1>l≥1, r≤2 and 1<q<2. Let m0 be as in assumption (M2), and let
P6:=max{m0L(r,Ω)Rr−p,βε(1−ϑ4)r4p−(1−ϑ4)r43C(ϑ4−1)r4p∗sRr4−rln(R)|Ω|2−r2}, P7:=1Cβε(ϑ3−1)r3(1−ϑ3)−(p+l1−1)2C(ϑ3−1)pr3p+l1−1p∗s, |
ϑ3=[(q+l1−1)p∗s−(l1+1)p](p+l1−1)[(q+l1−1)p∗s−(p+l1−1)p](l1+1), ϑ4=(p∗s−2)p(p∗s−q)2, C=1eσ|Ω|1−r5l1+1Cr5l1+1Rr5−r3, |
r3=(q+l1−1)(p+l1−1)ϑ3(p+l1−1)+(q+l1−1)(1−ϑ3), r4=qpq(1−ϑ4)+ϑ4p, r5=l1+r+σ−1, |
and ε2, ε3>0 are two constants. If 2N/(N+2s)<p<2 with λ<P6 or 1<p≤2N/(N+2s) with λ<P7, then the non-negative weak solution of problem (1.1) vanishes in finite time for any non-negative initial data.
Finally, we discuss the global boundedness and blow up of weak solutions.
Theorem 1.5 Let u(x,t) be the weak solution of problem (1.1).
(ⅰ) If E(u0)<0, r=p>q and θ=1, then the weak solution u(x,t) blows up at +∞;
(ⅱ) If 0<E(u0)≤h and I(u0)≥0, then the weak solution u(x,t) is globally bounded.
The rest of the paper is organized as follows. In Section 2, we give some related spaces and lemmas. In Section 3, we give the proof process for the main results of problem (1.1).
In order to facilitate the proof of the main results, we start this section by introducing some symbols and Lemmas that will be used throughout the paper.
In this section, we assume that 0<s<1<p<2 and Ω∈RN (N>2s) is a bounded domain with Lipschitz boundary. We denote by ‖u‖i (i≥1) the norm of Lebesgue space Li(Ω). Let Ws,p(Ω) be the linear space of Lebesgue measurable functions u from RN to R such that the restriction to Ω of any function u in Ws,p(Ω) belongs to Lp(Ω) and
∬Q|u(x)−u(y)|p|x−y|N+spdxdy<∞, |
where Q=R2N∖(CΩ×CΩ), CΩ=RN∖Ω. The space Ws,p(Ω) is equipped with the norm
‖u‖Ws,p(Ω)=(‖u‖pp+∬Q|u(x)−u(y)|p|x−y|N+spdxdy)1p. |
We further give a closed linear subspace
Ws,p0(Ω)={u∈Ws,p(Ω)|u(x)=0 a.e. in RN∖Ω}. |
As shown in [19], it can be concluded that
‖u‖=(∬Q|u(x)−u(y)|p|x−y|N+spdxdy)1p |
is an equivalent norm of Ws,p0(Ω).
Next we give the necessary Lemmas.
Lemma 2.1 ([25]) Let u∈Ws,p0(Ω)∖{0}. Then
∫Ω|u|pln|u|dx≤L(p,Ω)‖u‖p+ln(‖u‖)∫Ω|u|pdx, |
where L(p,Ω):=|Ω|ep+1e(p∗s−p)Cp∗sp∗s, Cp∗s is the best constant of embedding from Ws,p0(Ω) to Lp∗s(Ω).
Lemma 2.2 ([26]) Let y(t) be a non-negative absolutely continuous function on [T0,+∞) satisfying
dydt+αyk+βy≤0, t≥0, y(0)≥0, |
where α,β>0 are constants and k∈(0,1). Then
{y(t)≤[(y1−k(T0)+αβ)e(k−1)β(t−T0)−αβ]11−k,t∈[T0,T∗),y(t)≡0,t∈[T∗,+∞), |
where T∗=1(1−k)βln(1+βαy1−k(T0)).
Lemma 2.3 ([27]) Suppose that β∗≥0, N>sp≥1, and 1≤r≤q≤(β∗+1)p∗s, then for u such that |u|β∗u∈Ws,p0(Ω), we have
‖u‖q≤C1−ϑβ∗+1p∗s‖u‖ϑr‖|u|β∗u‖1−ϑβ∗+1, |
with ϑ=[(β∗+1)p∗s−q]r[(β∗+1)p∗s−r]q, where Cp∗s is the embedding constant for Ws,p0(Ω)↪Lp∗s(Ω).
Lemma 2.4 ([19]) Let 1<p<∞ and g:R→R be an increasing function. Define
G(t)=∫t0g′(τ)1pdτ, t∈R |
then
|a−b|p−2(a−b)(g(a)−g(b))≥|G(a)−G(b)|p for all a,b∈R. |
Lemma 2.5 Assume that (M1) holds. Let u∈Ws,p0(Ω)∖{0}, 0<σ≤p∗s−r. We have
(ⅰ) if 0<‖u‖≤R, then I(u)>0;
(ⅱ) if I(u)≤0, then ‖u‖>R,
where
R=(aσλCr+σr+σ)1r+σ−p, |
Cr+σ is the embedding constant for Ws,p0(Ω)↪Lr+σ(Ω).
Proof. Since u∈Ws,p0(Ω)∖{0}, and
σln|u(x)|<|u(x)|σ for a.e.x∈Ω. |
Then by the definition of I(u), we obtain
I(u)=a‖u‖p+θb‖u‖θp+β‖u‖qq−λ∫Ω|u|rln|u|dx>a‖u‖p+θb‖u‖θp+β‖u‖qq−λ1σ‖u‖r+σr+σ≥a‖u‖p−λ1σ‖u‖r+σr+σ≥(a−λ1σCr+σr+σ‖u‖r+σ−p)‖u‖p, |
where Cr+σ is the embedding constant for Ws,p0(Ω)↪Lr+σ(Ω).
We can get
I(u)>(a−λ1σCr+σr+σ‖u‖r+σ−p)‖u‖p. | (2.1) |
If 0<‖u‖≤R, then it follows from the definition of R that
a−λ1σCr+σr+σ‖u‖r+σ−p≥0, |
thus (ⅰ) holds.
If I(u)≤0, by (1.12), we have
a−λ1σCr+σr+σ‖u‖r+σ−p<0, |
thus (ⅱ) holds.
Lemmas 2.6 is similar to [28,Lemmas 9], so we ignore its proof.
Lemma 2.6 ([28]) Assume that E(u0)≤h, then the sets N+ and N− are both invariant for u(t), i.e, if u0∈N− (resp. u0∈N+), then u(t)∈N− (resp. u(t)∈N+) for all t∈[0,T).
Lemma 2.7 ([29]) Let α be positive. Then
tpln(t)≤1eαtp+α, for all p,t>0. |
In this section, we prove that the main results of problem (1.1).
Proof of Theorem 1.1
(1) Taking v=u in Definition 1.1, we obtain
12ddt∫Ωu2dx+M(‖u‖p)‖u‖p=λ∫Ω|u|pln|u|dx−β∫Ωu2dx. | (3.1) |
By Lemma 2.1, Lemma 2.5 and Lemma 2.6, we obtain
12ddt∫Ωu2dx+(m0−λL(p,Ω)−λλ1ln(R))‖u‖p+β∫Ωu2dx≤0. |
Since λ<λ1P1, we get
12ddt∫Ωu2dx+β∫Ωu2dx≤0. |
thus
‖u(⋅,t)‖22≤‖u0‖22e−2βt. |
which implies that ‖u(⋅,t)‖2→0 as t→+∞.
(2) We consider first the case 2N/(N+2s)<p<2 with λ<λ1P1. By (3.1) and Lemma 2.1, Lemma 2.5 and Lemma 2.6, we have
12ddt‖u‖22+(m0−λλ1(λ1L(p,Ω)+ln(R)))‖u‖p+β‖u‖22≤0. | (3.2) |
Using Hölder's inequality and the fractional Sobolev embedding theorem, we have
‖u‖2≤|Ω|12−N−spNp‖u‖NpN−sp≤Cp∗s|Ω|12−N−spNp‖u‖, | (3.3) |
where Cp∗s>0 is the embedding constant. By (3.2), (3.3) and λ<λ1P1, we obtain
12ddt‖u‖22+C1‖u‖p2+β‖u‖22≤0, | (3.4) |
where
C1=C−pp∗s|Ω|N−spN−P2(m0−λλ1(λ1L(p,Ω)+ln(R)))>0. | (3.5) |
Setting y(t)=‖u(⋅,t)‖22, y(0)=‖u0(⋅)‖22, by Lemma 2.2, we obtain
{‖u‖2≤[(‖u0‖2−p2+C1β)e(p−2)βt−C1β]12−p,t∈[0,T1),‖u‖2≡0,t∈[T1,∞), |
where
T1=1(2−p)βln(1+βC1‖u0‖2−p2). | (3.6) |
Next, we consider the case 1<p≤2N/(N+2s) and λ<λ1P2. Taking ν=ul in Definition 1.1, where l=2N−(s+N)psp≥1, by Lemma 2.1, Lemma 2.4, Lemma 2.5 and Lemma 2.6, we obtain
1l+1ddt‖u‖l+1l+1+G‖up+l−1p‖p+β‖u‖l+1l+1≤0, | (3.7) |
where G=(m0lpp(p+l−1)p−λpL(p,Ω)p+l−1−λpln(R)λ1(p+l−1)). By the very choice of l and the fractional Sobolev embedding theorem, we have
‖u‖p+l−1pl+1=(∫Ωup+l−1p⋅NpN−spdx)N−spNp≤Cp∗s‖up+l−1p‖. | (3.8) |
Hence,
1l+1ddt‖u‖l+1l+1+C2‖u‖p+l−1l+1+β‖u‖l+1l+1≤0, | (3.9) |
where
C2=C−pp∗S(m0lpp(p+l−1)p−λpL(p,Ω)p+l−1−λpln(R)λ1(p+l−1)), | (3.10) |
since λ<P2, then C2>0. Setting y(t)=‖u(⋅,t)‖l+1, y(0)=‖u0(⋅)‖l+1, by Lemma 2.2, we obtain
{‖u‖l+1≤[(‖u0‖2−pl+1+C2β)e(p−2)βt−C2β]12−p,t∈[0,T2),‖u‖l+1≡0,t∈[T2,∞), |
where
T2=1(2−p)βln(1+βC2‖u0‖2−pl+1). | (3.11) |
The proof is completed.
Proof of Theorem 1.2
We consider first the case p<r<2 and 2N/(N+2s)<p<2. Taking ν=u in Definition 1.1, we have
12ddt‖u‖22+M(‖u‖p)‖u‖p=∫Ω|u|rln|u|dx−β‖u‖22. | (3.12) |
By Lemma 2.1, Lemma 2.5 and Lemma 2.6, we obtain
12ddt‖u‖22+M(‖u‖p)‖u‖p≤λL(r,Ω)‖u‖r+λln(R)‖u‖rr−β‖u‖22. | (3.13) |
Using Hölder's inequality and the interpolation inequality, the fractional Sobolev embedding theorem and Young inequality, we can easily obtain (see [19])
‖u‖rr≤|Ω|s1−rs1‖u‖rs1≤|Ω|s1−rs1Cr(1−ϑ1)p∗s(ε‖u‖p+εr(ϑ1−1)p−r(1−ϑ1)‖u‖22), | (3.14) |
where s1>r, ϑ1∈(0,1), ε>0 and
s1=2ϑ1+p∗s(1−ϑ1), ϑ1=2(r−p)r(2−p). |
By (3.13) and (3.14), we have
12ddt‖u‖22+C3‖u‖p+C4‖u‖22≤0, | (3.15) |
where
C3=m0−λL(r,Ω)Rr−p−λεln(R)|Ω|s1−rs1Cr(1−ϑ1)p∗s, | (3.16) |
C4=β−λln(R)|Ω|s1−rs1Cr(1−ϑ1)p∗sεr(ϑ1−1)p−r(1−ϑ1). | (3.17) |
Since 2N/(N+2s)<p<2 and λ<P3, by the fractional embedding theorem and (3.3), we obtain
12ddt‖u‖22+C5‖u‖p2+C4‖u‖22≤0, | (3.18) |
and C3>0,C4>0, where
C5=C3C−pp∗s|Ω|N−spN−P2. | (3.19) |
Similar to the Theorem 1.1, one can prove the that
{‖u‖2≤[(‖u0‖2−pl+1+C5C4)e(p−2)C4t−C5C4]12−p,t∈[0,T3),‖u‖2≡0,t∈[T3,∞), |
where
T3=1(2−p)C4ln(1+C4C5‖u0‖2−p2). | (3.20) |
When 1<p≤2N/(N+2s), p<r≤2 and λ<P4. Taking ν=ul (l=2N−sp−Npsp≥1) in Definition 1.1, by Lemma 2.4 and Lemma 2.7, we obtain
1l+1ddt‖u‖l+1l+1+m0lpp(p+l−1)p‖ul+p−1p‖p≤λ1eσ‖u‖l+r+σ−1l+r+σ−1−β‖u‖l+1l+1 | (3.21) |
further, we have
1l+1ddt‖ul+p−1p‖r1r1+m0lpp(p+l−1)p‖ul+p−1p‖p≤λ1eσ‖ul+p−1p‖r2r2−β‖ul+p−1p‖r1r1 | (3.22) |
where r1=p(l+1)l+p−1, r2=p(l+r+σ−1)l+p−1. Note that, since r1<p∗s, by the Hölder's inequality and the fractional Sobolev embedding theorem, we have
‖ul+p−1p‖pr1≤|Ω|(p∗s−r1)pr1p∗s‖ul+p−1p‖pp∗s≤|Ω|(p∗s−r1)pr1p∗sCpp∗s‖ul+p−1p‖p. | (3.23) |
Using the same discussion as above, one can conclude that
‖ul+p−1p‖r2r2≤|Ω|s2−r2s2Cr2(1−ϑ2)p∗s(ε1‖ul+p−1p‖p+εr2(ϑ2−1)p−r2(1−ϑ2)1‖ul+p−1p‖r1r1), | (3.24) |
where s2>r2, ϑ2∈(0,1), ε1>0 and
s2=r1ϑ2+p∗s(1−ϑ2), ϑ2=r1(r2−p)r2(r1−p). |
Combining (3.22)-(3.24) and λ<P4, we obtain
1l+1ddt‖ul+p−1p‖r1r1+C6‖ul+p−1p‖pr1+C7‖ul+p−1p‖r1r1≤0, | (3.25) |
and C6>0, C7>0, where
C6=(m0lpp(l+p−1)p−λε11eσCr2(1−ϑ2)p∗s|Ω|s2−r2s2)|Ω|(r1−p∗s)pr1p∗sC−pp∗s, | (3.26) |
C7=β−λ1eσ|Ω|s2−r2s2Cr2(1−ϑ2)p∗sεr2(ϑ2−1)p−r2(1−ϑ2)1. | (3.27) |
Using Lemma 2.2 and a direct calculation, we have
{‖u‖l+1≤[(‖u0‖2−pl+1+C6C7)e(p−2)C7t−C6C7]12−p,t∈[0,T4),‖u‖l+1≡0,t∈[T4,∞), |
where
T4=1(2−p)C7ln(C7C6‖u0‖2−pl+1+1). | (3.28) |
The proof is completed.
Proof of Theorem 1.3
We consider first the case 2N/(N+2s)<p<2 with λ<λ1P1. Taking v=u in Definition 1.1, we obtain
12ddt∫Ωu2dx+M(‖u‖p)‖u‖p=λ∫Ω|u|pln|u|dx−β∫Ωuqdx. | (3.29) |
Note that ‖u‖p≥λ1‖u‖pp and by Lemma 2.1, Lemma 2.5 and Lemma 2.6, we have
12ddt‖u‖22+(m0−λλ1(λ1L(p,Ω)+ln(R)))‖u‖p+β‖u‖qq≤0. | (3.30) |
By (3.3) and β>0 and λ<λ1P1, we obtain
12ddt‖u‖22+C8‖u‖p2≤0, | (3.31) |
where
C8=C−pp∗s|Ω|2(N−sp)−Np2N(m0−λλ1(λ1L(p,Ω)+ln(R)))>0. | (3.32) |
By a direct calculation, we obtain
{‖u‖2≤[(‖u0‖2−p2+C8(p−2)t]12−p,t∈[0,T5),‖u‖2≡0,t∈[T5,∞), |
where
T5=1(2−p)C8‖u0‖2−p2. | (3.33) |
Next, we consider the case 1<p≤2N(N+2s) with λ<P2. Multiplying (1.1) by ul1 (l1>l≥1) and integrating, by Lemma 2.1, Lemma 2.4, Lemma 2.5 and Lemma 2.6, we obtain
1l1+1ddt‖u‖l1+1l1+1+G1‖up+l1−1p‖p+β‖u‖q+l1−1q+l1−1≤0, | (3.34) |
where G1=(m0l1pp(p+l1−1)p−λpL(p,Ω)p+l1−1−λpln(R)λ1(p+l1−1)). By Lemma 2.3, we obtain
‖u‖l1+1≤C(1−ϑ3)pp+l1−1p∗s‖up+l1−1p‖(1−ϑ3)pp+l1−1‖u‖ϑ3q+l1−1, | (3.35) |
where
ϑ3=[(q+l1−1)p∗s−(l1+1)p](p+l1−1)[(q+l1−1)p∗s−(p+l1−1)p](l1+1). |
By the choice of l1, we have 0<ϑ3<1. Hence, using the Young inequality, for every r3>0 and ε2>0, we obtain
‖u‖r3l1+1≤C(1−ϑ3)pr3p+l1−1p∗s(ε2‖up+l1−1p‖p+ε(1−ϑ3)r3(1−ϑ3)r3−(p+l1−1)2‖u‖ϑ3r3(p+l1−1)(p+l1−1)−(1−ϑ3)r3q+l1−1). | (3.36) |
We now choose
r3=(q+l1−1)(p+l1−1)ϑ3(p+l1−1)+(q+l1−1)(1−ϑ3), |
and we notice that ϑ3r3(p+l1−1)(p+l1−1)−(1−ϑ3)r3=q+l1−1. That means
‖u‖r3l1+1≤C(1−ϑ3)pr3p+l1−1p∗s(ε2‖up+l1−1p‖p+ε(1−ϑ3)r3(1−ϑ3)r3−(p+l1−1)2‖u‖q+l1−1q+l1−1). | (3.37) |
We choose
ε2=[1β(m0l1pp(p+l1−1)p−λpL(p,Ω)p+l1−1−λpln(R)λ1(p+l1−1))](1−ϑ3)r3−(p+l1−1)−(p+l1−1). |
By (3.34) and (3.37) and λ<P5, we obtain
1l1+1ddt‖u‖l1+1l1+1+C9‖u‖r3l1+1≤0, |
where
C9=C(ϑ3−1)pr3p+l1−1p∗sβ[1β(m0l1pp(p+l1−1)p−λpL(p,Ω)p+l1−1−λpln(R)λ1(p+l1−1))](ϑ3−1)r3−(p+l1−1), |
and C9>0, which implies that
{‖u‖l1+1≤[‖u0‖l1+1−r3l1+1+(r3−l1−1)C9t]1l1+1−r3,t∈[0,T6),‖u‖l1+1≡0,t∈[T6,∞), |
where
T6=1(l1+1−r3)C9‖u0‖l1+1−r3l1+1. |
The proof is completed.
Proof of Theorem 1.4
We consider first the case r<2. When 2N/(N+2)<p<2, multiplying (1.1) by u, we obtain
12ddt∫Ωu2dx+M(‖u‖p)‖u‖p=λ∫Ω|u|rln|u|dx−β∫Ωuqdx. | (3.38) |
Similar to the Theorem 1.2, we obtain
12ddt‖u‖22+(m0−λL(r,Ω)Rr−p)‖u‖p≤λln(R)|Ω|2−r2‖u‖r2−β‖u‖qq. | (3.39) |
Taking β∗=0 in Lemma 2.3, we have
‖u‖2≤‖u‖(1−ϑ4)p∗s‖u‖ϑ4q≤C(1−ϑ4)p∗S‖u‖(1−ϑ4)‖u‖ϑ4q, | (3.40) |
where ϑ4=(p∗s−2)p(p∗s−q)2. Then, taking into account that ϑ4∈(0,1), we can apply Young's inequality: for every r4>0 and ε3>0, we have
‖u‖r42≤C(1−ϑ4)r4p∗s(ε3‖u‖p+ε(ϑ4−1)r4p−(1−ϑ4)r43‖u‖ϑ4r4pp−r4(1−ϑ4)q). | (3.41) |
Taking
r4=qpq(1−ϑ4)+ϑ4p, |
then ϑ4r4pp−k2(1−ϑ4)=q. By (3.39), (3.41), Lemma 2.5 and λ<P6, and let ε3=(m0−λL(r,Ω)Rr−pβ)p−(1−ϑ4)r4p, we obtain
12ddt‖u‖22+C10‖u‖r2≤0, | (3.42) |
where
C10=βε(1−ϑ4)r4p−(1−ϑ4)r43C(ϑ4−1)r4p∗sRr4−r−λln(R)|Ω|2−r2>0, |
which implies that our result holds.
When 1<p≤2N/(N+2s), we multiply (1.1) by ul1 (l1>l≥1), by Lemma 2.4 and Lemma 2.7, we obtain
1l1+1ddt‖u‖l1+1l1+1+m0l1pp(p+l1−1)p‖ul1+p−1p‖p≤λ1eσ‖u‖r5r5−β‖u‖q+l1−1q+l1−1, | (3.43) |
where r5=l1+r+σ−1. Using the Holder inequality and (3.37), and we choose
ε2=[m0l1ppβ(p+l1−1)p]p+l1−1+(1−ϑ3)r3p+l1−1, |
then, we have
1l1+1ddt‖u‖l1+1l1+1+βε(ϑ3−1)r3(1−ϑ3)r3−(p+l1−1)2C(ϑ3−1)pr3p+l1−1p∗s‖u‖r3l1+1≤λ1eσ|Ω|1−r5l1+1‖u‖r5l1+1, | (3.44) |
for 0<σ<2−r. After performing some simple calculations, we finally obtain
1l1+1ddt‖u‖l1+1l1+1+C11‖u‖r3l1+1≤0, | (3.45) |
where
C11=βε(ϑ3−1)r3(1−ϑ3)r3−(p+l1−1)2C(ϑ3−1)pr3p+l1−1p∗s−λC, C=1eσ|Ω|1−r5l1+1Cr5l1+1Rr5−r3. |
Note that λ<P7, then C11>0, which implies that
{‖u‖l1+1≤[‖u0‖l1+1−r3l1+1+(r3−l1−1)C11t]1l1+1−r3,t∈[0,T7),‖u‖l1+1≡0,t∈[T7,∞), |
where
T7=1(l1+1−r3)C11‖u0‖l1+1−r3l1+1. |
The proof is completed.
Proof of Theorem 1.5
(ⅰ) By the definition of E(u) and I(u), we obtain
E(u)=1pI(u)+1pb(1−θ)‖u‖θp+β(p−q)qp‖u‖qq+λ1p2‖u‖pp. | (3.46) |
Choosing ν=ut in Definition 1.1, we have
∫Ωututdx=−M(‖u‖p)⟨u,ut⟩+λ∫Ωut|u|r−2uln|u|dx−β∫Ωut|u|q−2udx. | (3.47) |
Note that
ddtE(u)=1pddt(a‖u‖p+b‖u‖θp)−λ∫Ω|u|r−2uutln|u|dx+β∫Ω|u|q−2uutdx. | (3.48) |
By (3.47) and (3.48), we obtain
ddtE(u)+∫Ωututdx=0, |
which implies that
E(u)=E(u0)−∫t0‖uτ‖22dτ. | (3.49) |
Setting Γ(t)=12∫Ω|u(x,t)|2dx, then we have
Γ′(t)=∫Ωutudx=−I(u). | (3.50) |
By (3.46) and (3.49) and (3.50), we obtain
Γ′(t)=−pE(u)+b(1−θ)‖u‖θp+1qβ(p−q)‖u‖qq+λ1p‖u‖pp=−pE(u0)+b(1−θ)‖u‖θp+1qβ(p−q)‖u‖qq+λ1p‖u‖pp+p∫t0‖uτ‖22dτ. |
Since p>q, then 1qμ(p−q)‖u‖qq>0, we obtain
Γ′(t)≥−pE(u0)>0. |
By a simple calculation, we get
‖u‖22≥−2pE(u0)t+2‖u0‖22, for all t>0, |
which implies that our result holds.
(ⅱ) Here, we only prove the case of E(u0)<h, and the proof of E(u0)=h is similar. Choosing ν=u in Definition 1.1, we have
12ddt‖u‖22+M(‖u‖p)‖u‖p=∫Ω|u|rln|u|dx−β‖u‖qq, | (3.51) |
namely
12ddt‖u‖22+I(u)=0. | (3.52) |
Next, taking ν=ut in Definition 1.1 and integrating with respect to time from 0 to t, we have
∫t0‖uτ‖22dx+E(u(t))=E(u0)<h,for t>0. | (3.53) |
We claim that u(x,t)∈W for any t>0. If it is false, there exists a t0∈R+0∖{0} such that u(t0)∈∂W, which implies
I(u(x,t0))=0 or E(u(x,t0))=h. |
From (3.53), E(u(t0))=h is not true. So u(t0)∈N, then by the definition of h in (1.9), we have E(u(t0))≥h, which also contradicts with (3.53). Hence, u(t0)∈W. By (3.52) and u(t)∈W for all t>0, we obtain
‖u‖22≤‖u0‖22. |
Remark 2 Compared with problem (1.4), we not only discuss the extinction of weak solutions of problem (1.1) with logarithmic nonlinearity, but also prove that the weak solutions are globally bounded and blow up at infinity.
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 potential conflict of interests.
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