Abstract
This paper deals with the fourth-order parabolic equation \(u_{t}+{\varDelta }^{2}u=u^{p(x)}\log u\) in a bounded domain, subject to homogeneous Navier boundary conditions. For subcritical and critical initial energy cases, we combine the Galerkin’s method with the generalized potential well method to prove the existence of global solutions. By the concavity arguments, we obtain the results about blow-up solutions. For super critical initial energy case, we use some ordinary differential inequalities to study the extinction of solutions. Moreover, extinction rate, blow-up rate and time, and decay estimate of solutions are discussed.
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1 Introduction
In this paper, we study the following fourth-order parabolic problem involving a variable exponent and logarithmic nonlinearity,
where \({\Omega }\subset \mathbb {R}^{n}\) is bounded with smooth boundary ∂Ω; \(u_{0}(x)\in {H_{0}^{2}}({\Omega })\) satisfies the compatibility conditions on the boundary in the trace sense; p(x) is Hölder-continuous in Ω, satisfying the Zhikov-Fan’s condition \(|p(x)-p(y)|\leq {Q}/{\log (1/|x-y|)}\) for x,y ∈Ω, |x − y| < δ, where constants Q > 0 and 0 < δ < 1. The problem (1.1) comes from the discussion on the properties of medical magnetic resonance images. Δ2u is the capillarity-driven surface diffusion term. The nonlinear source \(u^{p(x)}\log u\) describes some kinds of Gaussian noise, where the function u represents the random noise with respect to (x,t). The Navier boundary conditions are also referred to “stree-free” or “slip” boundary conditions. The term Δu is no longer subject to the zero-flux boundary condition whereas the image always satisfies the zero-flux boundary condition. For more information on background, the interested readers may refer to the works [18, 30]. There are little results about the singularity of solutions to the fourth-order parabolic equations with variable exponents. For the high-order equations with constant exponents, we referred the interested readers to the works [8, 12, 13, 20, 23, 25, 27, 31, 32]. For the second-order parabolic problems with variable exponents, the interested readers could find some results in the works [1, 2, 4,5,6,7, 10, 11, 14, 16, 17, 19, 22, 26, 28].
Philippin considered the following parabolic problem with coefficient of t in [21],
where the dimension n ≥ 2 and p is a positive constant. By using the Sobolev type inequalities and constructing auxiliary functions, they obtained some upper and lower bounds of blow-up time of (1.2).
Li and Liu in [15] studied the following parabolic problem involving logarithmic nonlinearity,
where constant \(2<q<2+\frac {4}{n}\). If \(\frac {1}{2}{\int \limits }_{\Omega } |{\varDelta } u_{0}|^{2} \mathrm {d}x \le \frac {1}{q}{\int \limits }_{\Omega } |u_{0}|^{q}\log |u_{0}| \mathrm {d}x-\frac {1}{q^{2}}{\int \limits }_{\Omega } |u_{0}|^{q} \mathrm {d}x\) and \( {\int \limits }_{\Omega } |{\varDelta } u_{0}|^{2} \mathrm {d}x > {\int \limits }_{\Omega } |u_{0}|^{q}\log |u_{0}| \mathrm {d}x \), then there exist global solutions of (1.3). If \(\frac {1}{2}{\int \limits }_{\Omega } |{\varDelta } u_{0}|^{2} \mathrm {d}x < \frac {1}{q}{\int \limits }_{\Omega } |u_{0}|^{q}\log |u_{0}| \mathrm {d}x-\frac {1}{q^{2}}{\int \limits }_{\Omega } |u_{0}|^{q} \mathrm {d}x\) and \( {\int \limits }_{\Omega } |{\varDelta } u_{0}|^{2} \mathrm {d}x < {\int \limits }_{\Omega } |u_{0}|^{q}\log |u_{0}| \mathrm {d}x \), then there exist blow-up solutions.
Qu, Zhou, and Liang in [24] employed the concavity method to study blow-up solutions of the fourth-order parabolic equation involving nonstandard growth conditions,
They proved that if (\({\mathscr{H}}\)) holds and \(\frac {1}{2}\|{\varDelta } u_{0}\|_{2}^{2} \leq {\int \limits }_{\Omega }\frac {1}{p(x)+1}u_{0}^{p(x)+1}\mathrm {d}x\), then the weak solutions of (1.4) blow up in the sense of \(\lim _{t\rightarrow T^{-} }{{\int \limits }_{0}^{t}}\|u\|_{2}^{2}\mathrm {d}\tau =+\infty \). Moreover, the bounds of blow-up time and rate are discussed.
Inspired by the works [9, 10, 15, 16, 21, 24, 28, 29], we would study the singular solutions to problem (1.1). We would use the sign of the difference between the energy functional and the potential depth to classify the initial energy into three subcases. Moreover, the asymptotic estimates are discussed also, which include the bounds of extinction rate, blow-up rate and time, and decay rate of weak solutions to problem (1.1). This paper is arranged as follows. In Section 2, we give the main results of the present paper. Moreover, we add Table 1 to show the optimal classification of the initial energy on the existence and nonexistence of singular solutions. Sections 3, 4, and 5 will be devoted to the subcritical, critical, and super critical cases, respectively.
2 Main Results
At the beginning, we give some preliminaries. The set
with the Luxemburg’s norm \(\|u\|_{p(x)}=\inf \{\lambda >0: {\int \limits }_{\Omega }\left | {u(x)}/{\lambda }\right |^{p(x)}\mathrm {d}x<1\}\), is a separable and uniformly convex Banach space. The following inequalities show the relation between ∥u∥p(x) and \(\mathcal {A}_{p(x)}(u)\) (see [3]), for all u ∈ Lp(x)(Ω), \({\min \limits } \left \{\|u\|_{p(x)}^{p^{-}},\|u\|_{p(x)}^{p^{+}} \right \}\leq \mathcal {A}_{p(x)}(u) \leq {\max \limits } \left \{\|u\|_{p(x)}^{p^{-}},\|u\|_{p(x)}^{p^{+}} \right \}\). We equip the Banach space \({H^{2}_{0}}({\Omega })\) with the norm \(\|u\|_{{H^{2}_{0}}}=\|{\varDelta } u\|_{2}\). There is the Sobolev embedding relationship \({H^{2}_{0}}({\Omega })\hookrightarrow L^{p^{+}+1}({\Omega })\hookrightarrow L^{p(x)+1}({\Omega })\), where
Let μ > 0 be small such that p(x) + μ ≤ p+ + μ < 4∗. We have
Suppose λ1 is the first eigenvalue of the clamped plate problem Δ2u − λu = 0 in Ω with ∂νu = ∂νΔu = 0 on ∂Ω, where ν denotes the unit outward normal vector. We have the following inequality \(\|u\|_{2}^{2}\leq \lambda _{1}^{-1}\|{\varDelta } u\|_{2}^{2}\). For all \(u\in {H_{0}^{2}}({\Omega })\), we give the following notations:
Define \(\mathcal {V}:= \left \{u\in {H_{0}^{2}}({\Omega }):I(u)<0, J(u)<d \right \}\), \( \mathcal {N}_{+} := \{u\in {H_{0}^{2}}({\Omega }):I(u)>0 \}\), and \(\mathcal {N}_{-} := \left \{u\in {H_{0}^{2}}({\Omega }):I(u)<0 \right \}\). Denote the sublevels of J as \( J^{s} := \left \{u\in {H_{0}^{2}}({\Omega }):J(u)< s \right \}\) and \(\mathcal {N}^{s}:=\mathcal {N}\cap J^{s}\neq \emptyset \) for ∀s > d. For all constant s > d, we define \(\lambda _{s} :=\inf \left \{\|u\|_{2}:u\in \mathcal {N}^{s}\right \}\) and \({\Lambda }_{s} :=\sup \left \{\|u\|_{2}:u\in \mathcal {N}^{s}\right \}\). Obviously, λs and Λs is non-increasing and non-decreasing with respect to s, respectively.
Now, we give the definition of weak solutions for problem (1.1), which could be proved by the standard procedure in [8].
Definition 2.1
Denote T be a positive constant. A function u is a weak solution of (1.1) if \(u\in L^{\infty }\left ((0,T);{H_{0}^{2}}({\Omega })\right )\) satisfies ut ∈ L2((0,T);L2(Ω)) and
and for any test function \(v\in L^{2}((0,T);{H_{0}^{2}}({\Omega }))\) and (⋅,⋅) as the inner product in L2(Ω). Moreover,
If u is a weak solution to (1.1) for every bounded T > 0, then we call it a weak global solution. \(\Box \)
2.1 Subcritical Initial Energy J(u 0) < d
Theorem 2.1
Let \(p(x)p^{\prime }(x)<4^{\ast }+1\) be in force and \(u_{0}\in {H_{0}^{2}}({\Omega })\). For J(u0) < d and I(u0) > 0, problem (1.1) has a global solution \(u\in L^{\infty }\left ((0,+\infty );{H_{0}^{2}}({\Omega })\right )\) with \(u_{t}\in L^{2}((0,+\infty );L^{2}({\Omega }))\) and \(u(t)\in \mathcal {W}\) for all \(0\leq t<+\infty \). Moreover, the weak solution is unique if it is bounded. Additionally, if J(u0) < d0 and I(u0) > 0, then \(\|u(t)\|_{2} \leq \|u_{0}\|_{2} \exp \{-\delta ^{\ast } t\}\) and
where positive constant \(d_{0}:=\frac {p^{-}-1}{2(p^{-}+1)}\left (\frac {\mathrm {e}\mu }{B^{p^{+}+1+\mu }}\right )^{\frac {2}{p^{-}-1+\mu }}\); B is defined in (2.2); Positive constants \(\delta ^{\ast } :=\lambda _{1} -\lambda _{1}\left ({J(u_{0})}/{d_{0}}\right )^{\frac {p^{-}-1+\mu }{2}}\) and
where M is a positive constant to be determined later.
Moreover, the energy functional J(u) decays in the following sense,
It could be tested that the radical functions in (2.8–2.10) make sense. In fact, since J(u0) < d0 and I(u0) > 0 and by (2.3), one could find out that J(u0) > 0.
Theorem 2.2
Let the variable exponent p(x) satisfies that
Assume u is a weak solution of problem (1.1) with
For 0 < J(u0) < d and I(u0) < 0, u blows up at some finite T satisfying \(\lim _{t\rightarrow T^{-} }{{\int \limits }_{0}^{t}}\|u\|_{2}^{2}\mathrm {d}\tau =+\infty \). Furthermore, \(T\leq \frac {2{\int \limits }_{0}^{t^{\ast }}\|u\|_{2}^{2} \mathrm {d}\tau }{(p^{-}-1) \|u(t^{\ast })\|_{2}^{2}}+t^{\ast }\), where \(t^{\ast }:=\sqrt {\frac {2\|u_{0}\|_{2}^{2}}{\lambda _{1} (p^{-}-1)(d-J(u_{0}))}}\).
2.2 Critical Initial Energy J(u 0) = d
Theorem 2.3
Let \(p(x)p^{\prime }(x)<4^{\ast }+1\) be in force and \(u_{0}\in {H_{0}^{2}}({\Omega })\). If J(u0) = d and I(u0) ≥ 0, then problem (1.1) admits a global weak solution \(u\in L^{\infty }((0,+\infty );{H_{0}^{2}}({\Omega }))\) with \(u_{t}\in L^{2}((0,+\infty );L^{2}({\Omega }))\) and \(u(t)\in \mathcal {\overline {W}}:=\mathcal {W}\cup \partial \mathcal {W}\) for \(0\leq t<+\infty \). In addition, the weak solution is unique if it is bounded.
Theorem 2.4
Let \(({\mathscr{H}})\) be in force. Assume u is a weak solution of problem (1.1) and the initial data satisfy (2.11). If J(u0) = d and I(u0) < 0, then there exists a finite time T such that u blows up in the sense of \( \lim _{t\rightarrow T^{-} }{{\int \limits }_{0}^{t}}\|u\|_{2}^{2}\mathrm {d}\tau =+\infty \). Furthermore, \(T\leq \frac {2{\int \limits }_{0}^{t^{\ast }}\|u\|_{2}^{2} \mathrm {d}\tau }{(p^{-}-1) \|u(t^{\ast })\|_{2}^{2}}+t^{\ast }\), where t∗ is determined by \( {\lambda _{1}} (p^{-}-1){{\int \limits }_{0}^{t}} \|u\|_{2}^{2} \mathrm {d}\tau >2(p^{-}+1)\|u_{0}\|^{2}_{2}\).
2.3 Super Critical Initial Energy J(u 0) > d
Theorem 2.5
Let \(({\mathscr{H}})\) be in force and J(u0) > d.
-
(i)
If \(u_{0}\in \mathcal {N}_{+} \) and \(\|u_{0}\|_{2}\leq \lambda _{J(u_{0})}\), the weak solution u of problem (1.1) in its \({H^{2}_{0}}\)-norm exists globally and \(u(t)\rightarrow 0\) as \(t\rightarrow +\infty \);
-
(ii)
If \(u_{0}\in \mathcal {N}_{-} \) and \(\|u_{0}\|_{2}\geq {\Lambda }_{J(u_{0})}\), the weak solution u of problem (1.1) in its \({H^{2}_{0}}\)-norm blows up in finite time.
For p(x) ≡ p, a positive constant, we give the following Theorem 2.6 to illustrate that there exists u0 such that J(u0) is arbitrary large, and the corresponding solution u(x,t) to problem (1.1) with u0 as initial datum blows up in finite time as well.
Theorem 2.6
Let p > 1 be in force. For any M > d, there exists \(u_{M}\in \mathcal {N}_{-}\) satisfying J(uM) = M and the weak solution u of problem (1.1) blows up in finite time.
2.4 Extinction or Non-extinction in Finite Time
The following result shows the extinction properties of weak solutions for 0 < p(x) < 1. Let p∗ be a positive constant satisfying p+ < p∗ < 1.
Theorem 2.7
If 0 < p− < p+ < p∗ < 1, and
then the weak solution u of (1.1) vanishes at T∗ and \(\frac {2}{{\lambda }_{1}(1-p^{\ast })}\leq T_{\ast }\leq \frac {-2|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\lambda _{1} \mathrm {e}(p^{\ast }-p^{+}) Y(0)}\). More precisely,
where \(T_{\ast }:=- {2\|u_{0}\|_{2}^{1-p^{\ast }}}/{Y(0)}\) and \( Y(0):=\left (1-p^{\ast }\right )\left [\frac {|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\mathrm {e}(p^{\ast }-p^{+})}-{\lambda }_{1}{\|u_{0}\|}_{2}^{1-p^{\ast }}\right ]<0\).
Corollary 2.1
Let 0 < p− < p+ < p∗ < 1 and (2.12) be in force. If J(u0) > d and I(u0) = 0, then the results of Theorem 2.7 hold.
In the following, we show a result on non-extinction of solutions.
Theorem 2.8
Let 0 < p− < p+ < p∗ < 1 and J(u0) < 0. The weak solution u of (1.1) does not vanish in finite time.
2.5 Remarks
We summarize the main results in the above three subsections. For convenience, we define some notations: “G.E.” means “Global existence”; “B.P.” means “Blow-up”; “N.E.” means “Non-extinction”; “E.” means “Extinction”; “Th.” means “Theorem”; “Cor.” means “Corollary”. We characterize the singularity of solutions by the help of Table 1.
The classification for the singularity of solutions is optimal with respect to the initial energy. In fact, Nehari energy I(u0)≠ 0 provided J(u0) < d. It was a pity that we have not solved the case where the energy J(u0) meets the potential depth.
3 Proof of Theorems 2.1–2.2
Lemma 3.1
The potential depth d > 0 which is defined in (2.5).
Proof
Fix any \(u\in \mathcal {N}\), we have I(u) = 0. Let μ > 0 be small that p(x) + μ < p+ + μ < 4∗. By \(x^{-\mu }\log x \leq (\mathrm {e}\mu )^{-1}\) for x ≥ 1, μ > 0 and \({H_{0}^{2}}({\Omega })\hookrightarrow L^{p(x)+1+\mu }({\Omega })\), one could obtain that
where Ω1 := {x ∈Ω : u ≥ 1}, Ω2 := {x ∈Ω : 0 < u < 1}, which implies \(\|{\varDelta } u\|_{2}\geq \left (\frac {\mathrm {e}\mu }{B^{p^{+}+1+\mu }}\right )^{\frac {1}{p^{-}-1+\mu }}\). Noticing that p− > 1, we have
Therefore, \(d\geq \frac {p^{-}-1}{2(p^{-}+1)}\left (\frac {\mathrm {e}\mu }{B^{p^{+}+1+\mu }}\right )^{\frac {2}{p^{-}-1+\mu }}>0\). □
Lemma 3.2
Let \(({\mathscr{H}})\) be in force and \(u\in {H_{0}^{2}}({\Omega })\).
-
(i)
If \(0\leq \|{\varDelta } u\|_{2}\leq r^{\ast } :=\left (\frac {\mathrm {e}\mu }{B^{p^{+}+1+\mu }}\right )^{\frac {1}{p^{-} -1+\mu }}\), then I(u) ≥ 0.
-
(ii)
If I(u) < 0, then ∥Δu∥2 > r∗.
-
(iii)
If I(u) = 0, then ∥Δu∥2 = 0 or ∥Δu∥2 ≥ r∗.
Proof
(i) By using the Sobolev’s inequality (3.1), we have
we have I(u) ≥ 0.
(ii) From I(u) < 0 and the Sobolev’s inequality (3.1), one could check that ∥Δu∥2 > r∗.
(iii) If ∥Δu∥2 = 0, then I(u) = 0. If I(u) = 0 and ∥Δu∥2≠ 0, then by the Sobolev’s inequality (3.1), we get ∥Δu∥2 ≥ r∗. □
Proof of Theorem 2.1.
Step 1. Global existence. We use the Galerkin’s approximation and a priori estimate. Let {ϕj(x)} be a system of orthogonal basis of \({H^{2}_{0}}({\Omega })\) and define \(u^{m}(x,t) ={\sum }_{j=1}^{m}{a_{j}^{m}}(t)\phi _{j}(x)\), m = 1,2,⋯, of (1.1) satisfying that
By the Peano’s theorem, (3.2, 3.3) have a local solution. Multiplying (3.2) by \(\frac {\mathrm {d}}{\mathrm {d}t}{a_{j}^{m}}(t)\), we have \( {{\int \limits }_{0}^{t}}\|u^{m}_{\tau }\|_{2}^{2}\mathrm {d}\tau +J(u^{m})=J(u^{m}(0)), \quad 0\leq t<+\infty \). Since \(u^{m}(x,0)\rightarrow u_{0}(x)\) in \({H^{2}_{0}}({\Omega })\), we have \(J(u^{m}(x,0))\rightarrow J(u_{0}(x))<d\), \(I(u^{m}(x,0))\rightarrow I(u_{0}(x))>0\). Thus, for large m, we have
and I(um(x,0)) > 0, which indicates that \(u^{m}(x,0)\in \mathcal {W}\) for sufficiently large m.
Next, we claim \(u^{m}(x,t)\in \mathcal {W}\) for sufficiently large m and any t ∈ [0,T]. By contradiction, there would exist a sufficiently large m and a constant t∗∈ (0,T] such that \(u^{m}(x,t_{\ast })\in {H_{0}^{2}}({\Omega })\setminus \{0\}\) and J(um(x,t∗)) = d or I(um(x,t∗)) = 0. In fact, the former case contradicts to (3.4), while the later one happens, we have J(um(x,t∗)) ≥ d, which also contradicts to (3.4). Hence, our claim is valid. Applying (2.3), (2.4), (3.4) and I(um(x,t)) > 0 for sufficiently large m, one could obtain
for large m and any \(0\leq t<+\infty \), which indicates that
Since \(p(x)p^{\prime }(x)<4^{\ast }+1\), we could choose μ > 0 sufficiently small that \((p(x)+\mu )p^{\prime }(x)<4^{\ast }+1\). Therefore, by embedding \({H_{0}^{2}}({\Omega })\hookrightarrow L^{(p(x)+\mu )p^{\prime }(x)}({\Omega })\), we get
where \(\psi ^{m}(x,t)=(u^{m})^{p(x)}\log (u^{m})\) and Ω1 := {x ∈Ω : um ≥ 1}, Ω2 := {x ∈Ω : 0 < um < 1} and the inequalities \(|x^{p^{-}}\log x|\leq (\mathrm {e}p^{-})^{-1}\) for 0 < x < 1 and \(x^{-\mu }\log x\leq (\mathrm {e}\mu )^{-1}\) for x ≥ 1 and μ > 0 are used.
By the uniform estimates (3.5–3.7), it was seen that the local solutions can be extended globally. Thus, there exist some u and a subsequence of {um} such that, for each T > 0, one could obtain that
as \(m\rightarrow +\infty \). Fix \(k\in \mathbb {N}\). In order to show the limit u in (3.8–3.10) is a weak solution of (1.1), one could find \(v\in C^{1}([0,T];{H_{0}^{2}}({\Omega }))\) of
where \(\{l_{j}(t)\}_{j=1}^{k}\) are arbitrarily given C1 functions. Choosing m ≥ k in (3.2) and multiplying (3.2) by lj(t), one could obtain
Let \(m\rightarrow +\infty \) in (3.12). By the convergence in (3.8–3.10), we deduce that
Since functions in (3.11) are dense in \(L^{2}((0,T);{H^{2}_{0}}({\Omega }))\), (3.13) holds for all \(v\in L^{2}((0,T);{H^{2}_{0}}({\Omega }))\). For arbitrariness of T > 0, one has \( (u_{t},v)+({\varDelta } u,{\varDelta } v)=\left (u^{p(x)}\log u,v\right )\) for a.e. t > 0. To prove (2.7), we first assume that u is smooth enough such that \(u_{t}\in L^{2}((0,T);{H^{2}_{0}}({\Omega }))\). Taking v = ut in (3.13) it is seen that (2.7) is true. By the density of \(L^{2}((0,T);{H^{2}_{0}}({\Omega }))\) in L2(Ω × (0,T)), we know (2.7) holds for weak solutions to problem (1.1). The global solutions of (1.1) is proved.
Step 2. Uniqueness of the bounded solution. We assume both u and v be bounded weak solutions to (1.1). For any \(\varphi \in {H^{2}_{0}}({\Omega })\), we have \( (u_{t},\varphi )+({\varDelta } u,{\varDelta } \varphi )=\left (u^{p(x)}\log u,\varphi \right )\) and \((v_{t},\varphi )+({\varDelta } v,{\varDelta } \varphi )=\left (v^{p(x)}\log v,\varphi \right )\). Subtracting the above two equalities, choosing \(\varphi =u-v\in {H^{2}_{0}}({\Omega })\) and integrating over (0,t) for any t > 0, we deduce that
Since φ(x,0) = 0, due to the boundedness of u and v, we have \( {\int \limits }_{\Omega }\varphi ^{2}(x,t)\mathrm {d}x\leq C{{\int \limits }_{0}^{t}}{\int \limits }_{\Omega }\varphi ^{2}(x,t)\mathrm {d}x\mathrm {d}t\), where C > 0 is a constant depending on p−, p+, and the bounds of u, v. By the Gronwall’s inequality, \({\int \limits }_{\Omega }\varphi ^{2}(x,t)\mathrm {d}x=0\). Hence, φ = 0 a.e. in \({\Omega }\times (0,+\infty )\) and the uniqueness of bounded solution follows.
Next, we consider the exponential decay of ∥u(t)∥2. Since \(u(t)\in \mathcal {W}\) for \(0\leq t<+\infty \), we have I(u(t)) ≥ 0. Then it follows from (2.7) and I(u(t)) ≥ 0 that
which, together with (2.2), implies
By the definition of d0 and (2.2, 3.1, 3.15), we obtain
Choosing v = u in (2.6) and combining (2.4) with (3.16), we have
Consequently, \(\|u(t)\|_{2}^{2}\leq \|u_{0}\|_{2}^{2} \exp \{-\delta t\}\), where constant \( \delta :=2\lambda _{1}\left [1-\left ({J(u_{0})}/{d_{0}}\right )^{\frac {p^{-}-1+\mu }{2}}\right ]\).
Finally, we consider the exponential decay of ∥Δu(t)∥2, ∥u(t)∥p(x)+ 1, and J(u(t)). By (2.4, 3.16), one could obtain
Define an auxiliary function \(L(t):=J(u(t))+\|u(t)\|_{2}^{2}\). Then by \(\|u\|_{2}^{2}\leq \lambda _{1}^{-1}\|{\varDelta } u\|_{2}^{2}\) and (3.14), we get
By (2.1), we have
Thus,
where \(M:=\max \limits \left \{D^{p^{+}+1}\left [\frac {2(p^{-}+1)}{p^{-}-1}J(u_{0})\right ]^{\frac {p^{-}-1}{2}}, D^{p^{+}+1}\left [\frac {2(p^{-}+1)}{p^{-}-1}J(u_{0})\right ]^{\frac {p^{+}-1}{2}}\right \}\). Moreover, it follows from (2.7) and \(\frac {\mathrm {d}}{\mathrm {d}t}\|u\|_{2}^{2}=-2I(u)\) that \(\frac {\mathrm {d}}{\mathrm {d}t}L(t)=-\|u_{t}\|_{2}^{2}-2I(u(t))\), which, together with (3.16, 3.17, 3.19), indicates that for any constant α > 0, one could obtain
Let
It follows from (3.18) that
which, together with the definition of L(t), implies
Finally, it follows from (2.1, 3.21) that
□
Proof of Theorem 2.2.
Step 1. Blow-up in finite time. Assume that u was a global weak solution to problem (1.1) for 0 < J(u0) < d, I(u0) < 0 and define \(M(t):={{\int \limits }_{0}^{t}}\|u\|_{2}^{2}\mathrm {d}\tau \) for t ≥ 0, one has \(M^{\prime }(t)=\|u\|_{2}^{2}\) and
Next, we claim I(u) < 0 for all t ∈ [0,T). In fact, if it was false, it follows there would exist a constant of first appearance t0 > 0 such that I(u(t0)) = 0 and I(u) < 0 for t ∈ [0,t0). From Lemma 3.2 (ii), we have ∥Δu(t)∥2 > r∗ > 0 for t ∈ [0,t0). By the continuity of ∥Δu(t)∥2 to t and Lemma 3.2 (iii), we get ∥Δu(t0)∥2 ≥ r∗ > 0. Hence, \(u(t_{0})\in \mathcal {N}\). Then it follows from (2.5) that J(u(t0)) ≥ d, which contradicts to (2.7). By computations, one has
By (2.7, 3.22, 3.23), one could obtain
Noticing that \( (M^{\prime }(t))^{2}=4\left ({{\int \limits }_{0}^{t}}{\int \limits }_{\Omega } u_{\tau } u\mathrm {d}x\mathrm {d}\tau \right )^{2}+2\|u_{0}\|^{2}_{2}M^{\prime }(t)-\|u_{0}\|^{4}_{2}\), we have
From \(M^{\prime \prime }(t)=-2I(u)\), we have \(M^{\prime \prime }(t)>0\) for t ≥ 0. Hence,
Since \(M^{\prime }(0)>0\), we have \(M(t)\geq M^{\prime }(0)t\). Therefore, for sufficiently large t ≥ t∗, one could obtain \( {\lambda _{1}}(p^{-}-1)M(t)>{2}(p^{-}+1)\|u_{0}\|^{2}_{2}\). Combining the above inequality and \(\|u_{0}\|_{2}^{2}>\frac {4(p^{-}+1)d}{\lambda _{1}(p^{-}-1)}>\frac {4(p^{-}+1)J(u_{0})}{\lambda _{1}(p^{-}-1)}\), we have
for sufficiently large t ≥ t∗. From (3.24), it follows with \(\alpha =\frac {p^{-}-1}{2}>0\) that
Integrating both sides of (3.25) over (t∗,t) with respect to t, M(t) cannot remain finite for all t > t∗, and therefore there is a contradiction.
Step 2. Upper bound of blow-up time. Taking J(λu) := j(λ), we have
It is noticed that j(λ) > 0 for small λ > 0, \(j(\lambda )\rightarrow -\infty \) for \(\lambda \rightarrow +\infty \) and j(λ) is continuous on \([0,+\infty )\) and differentiable on \((0,+\infty )\). Combining this facts, we imply that j(λ) attains its maximum value at some number λ∗ := λ∗(u).
By Fermat’s theorem, one has \(j^{\prime }(\lambda )=\lambda \|{\varDelta } u\|_{2}^{2}-{\int \limits }_{\Omega } {\lambda }^{p(x)}u^{p(x)+1}\log (\lambda u)\mathrm {d}x\). On the other hand, since \(j^{\prime }(\lambda )=\frac {1}{\lambda }I(\lambda u)\), we obtain I(λ∗u) = 0. Since
and p(x) > 1 for a.e. x ∈Ω, we derive that λ∗∈ (0,1) provided that I(u) < 0. And this implies
which in turn implies for all t ≥ 0 that \( {M^{\prime }(t) \geq } 2(p^{-}+1)(d-J(u_{0}))t\) and M(t) ≥(p− + 1)(d − J(u0))t2. Integrating both sides of (3.25) over (t∗,t) with respect to t, we obtain \( M(t)>\left [\frac {M^{1+\alpha }(t^{\ast })}{\alpha M^{\prime }(t^{\ast })(t^{\ast }-t)+M(t^{\ast })}\right ]^{\frac {1}{\alpha }}\), hence, \(t \leq \frac {2{\int \limits }_{0}^{t^{\ast }}\|u\|_{2}^{2} \mathrm {d}\tau }{(p^{-}-1)\|u(t^{\ast })\|_{2}^{2}}+t^{\ast }\). □
4 Proof of Theorems 2.3 and 2.5
Proof of Theorem 2.3.
Let λk = 1 − 1/k, k = 2,3,⋯. Consider
Noticing that \(u_{0}\in {H_{0}^{2}}({\Omega })\), λk ∈ (0,1), and I(u0) ≥ 0, we have
A simply computation shows
This implies that J(λku0) is strictly increasing with respect to λk. Hence, J(u0k) = J(λku0) < J(u0) = d. The remainder can be proved similarly to Theorem 2.1. □
Proof of Theorem 2.4.
Since J(u0) = d and I(u0) < 0, there exists a constant t0 > 0 such that J(u(x,t)) > 0 and I(u(x,t)) < 0 for 0 < t ≤ t0. Considering (ut,u) = −I(u), we have ut≢0 for 0 < t ≤ t0. Furthermore,
Taking t = t0 as the initial time, we will prove that I(u) < 0 for all t > t0. Otherwise, there must be a constant t1 > 0 such that I(u(t1)) = 0 and I(u) < 0 for t0 ≤ t < t1. From Lemma 3.2 (ii), we have ∥Δu(t)∥2 > r∗ > 0 for t ∈ [t0,t1). Then by continuity of ∥Δu(t)∥2 with respect to t and Lemma 3.2 (iii), we get ∥Δu(t1)∥2 ≥ r∗ > 0. Hence, \(u(t_{1})\in \mathcal {N}\). It follows from the definition of d that J(u(t1)) ≥ d, which contradicts to (4.1). Hence, I(u) < 0 for all t ≥ 0.
Similarly to the proof of Theorem 2.2, we get
Then from \(M^{\prime \prime }(t)=-2I(u)\), we have \(M^{\prime \prime }(t)>0\) for t ≥ 0. Since \(M^{\prime }(0)>0\), we have \(M(t)\geq M^{\prime }(0)t\). Therefore, for sufficiently large time t, we have \(\frac {\lambda _{1}}{2}(p^{-}-1)M(t)>(p^{-}+1)\|u_{0}\|^{2}_{2} \). By \(\|u_{0}\|_{2}>\tilde {C}\), we have \(\frac {\lambda _{1}}{2}(p^{-}-1)M^{\prime }(t)>2(p^{-}+1)J(u_{0})\). Consequently, there exists a suitably large constant t∗ such that for all t ≥ t∗, \( M^{\prime \prime }(t)M(t)-\frac {p^{-}+1}{2}(M^{\prime }(t))^{2}>0\). The other could be proved similarly to the ones of Theorem 2.2. □
5 Proof of Theorems 2.5 and 2.6
Lemma 5.1
Let \(({\mathscr{H}})\) be in force.
-
(i)
\(\text {dist}(0,\mathcal {N})>0\), \(\text {dist}(0,\mathcal {N}_{-})>0\).
-
(ii)
For any constant s > 0, the set \(J^{s}\cap \mathcal {N}_{+}\) is bounded in \({H_{0}^{2}}({\Omega })\).
Proof
(i) For any \(u\in \mathcal {N}\), by the definition of d, one could obtain
which yields that there exists a constant c0 > 0 such that
For any \(u\in \mathcal {N}_{-}\), we have ∥Δu∥2≠ 0. Let μ > 0 be small that p(x) + μ < p+ + μ < 4∗. By \(x^{-\mu }\log x\leq (\mathrm {e}\mu )^{-1}\) for x ≥ 1, μ > 0 and \({H_{0}^{2}}({\Omega })\hookrightarrow L^{p(x)+1+\mu }({\Omega })\), we have
where Ω1 := {x ∈Ω : u ≥ 1}, Ω2 := {x ∈Ω : 0 < u < 1}, which implies \(\|{\varDelta } u\|_{2}>\left (\frac {\mathrm {e}\mu }{B^{p^{+}+1+\mu }}\right )^{\frac {1}{p^{-}-1+\mu }}\). Therefore, \( \text {dist}(0,\mathcal {N}_{-})=\inf _{u\in \mathcal {N}_{-}}\|{\varDelta } u\|_{2}\geq \left (\frac {\mathrm {e}\mu }{B^{p^{+}+1+\mu }}\right )^{\frac {1}{p^{-}-1+\mu }}>0\).
(ii) For any \(u\in J^{s}\cap \mathcal {N}_{+}\), J(u) < s and I(u) > 0. Therefore,
which yields \(\|{\varDelta } u\|_{2}<\sqrt {\frac {2s(p^{-}+1)}{p^{-}-1}}\). □
Lemma 5.2
Let \(({\mathscr{H}})\) be in force. For any s > d, \(0<C_{1}\leq \lambda _{s}\leq {\Lambda }_{s}\leq C_{2}<+\infty \), where
\({\delta }_{\min \limits }(d)\) is a positive constant to be determined later; \(C_{2}:=\sqrt {\frac {2s(p^{-}+1)}{{\lambda }_{1}(p^{-}-1)}}\); β is the optimal constant in the Gagliardo-Nirenberg’s inequality
Proof
Firstly, we estimate the upper bound of Λs. For any \(u\in {\mathcal {N}}^{s}\), by the definition of functionals J(u) and I(u), we obtain
Therefore, (5.2) indicates that ∥u∥2 < C2. Hence, \({\Lambda }_{s}\leq C_{2}<+\infty \).
Next, we estimate the lower bound of λs. Let \(u\in {\mathcal {N}}^{s}\), then I(u) = 0 and J(u) < s. By (2.1), we obtain
Thus,
By \(x^{-\mu }\log x\leq (\mathrm {e}\mu )^{-1}\) for x ≥ 1, μ > 0, the continuous embedding \(L^{p^{+}+1+\mu }({\Omega })\hookrightarrow L^{p(x)+1+\mu }({\Omega })\) and (5.2), we could obtain
where \(\theta :=1+\frac {n}{2(p^{+}+1+\mu )}-\frac {n}{4}\in (0,1)\), one could obtain ∥u∥2 ≥ C1, which indicates λs ≥ C1 > 0. □
Lemma 5.3
Let p > 1. If J(u0) > d and \( \|u_{0}\|_{2}>\left [(1+|{\Omega }|)^{p+1}(p+1)^{2}J(u_{0})\right ]^{\frac {1}{p+1}}\), then the weak solution u of problem (1.1) blows up in finite time.
Proof
By the embedding Lp+ 1(Ω)↪L2(Ω), we have ∥u0∥2 ≤ (1 + |Ω|)∥u0∥p+ 1,
Therefore, I(u0) < 0, i.e., \(u_{0}\in {\mathcal {N}}_{-}\). Now, we only need to prove \({\|u_{0}\|}_{2}\geq {\Lambda }_{J(u_{0})}\). For any \(u\in {\mathcal {N}}_{J(u_{0})}\), i.e., I(u) = 0,J(u) < J(u0). Since
we have
i.e., \({\|u_{0}\|}_{2}>{\Lambda }_{J(u_{0})}\). This completes the proof of this lemma. □
Proof of Theorem 2.5.
Denote T(u0) be the maximal existence time of (1.1) with initial datum u0. If \(T(u_{0})=+\infty \), we denote the ω-limit set of u0 by \(\omega (u_{0})=\bigcap _{t\geq 0}\overline {\left \{u(s):s\geq t\right \}}^{{H_{0}^{2}}({\Omega })}\).
(i) Assume that \(u_{0}\in \mathcal {N}_{+}\) with \(\|u_{0}\|_{2}\leq \lambda _{J(u_{0})}\). We first claim that \(u(t)\in \mathcal {N}_{+}\) for all t ∈ [0,T(u0)). If not, there would exist a constant t0 ∈ (0,T(u0)) such that \(u(t)\in \mathcal {N}_{+}\) for t ∈ [0,t0) and \(u(t_{0})\in \mathcal {N}\). By \(I(u(t))=-{\int \limits }_{\Omega } u_{t}(x,t)u(x,t)\mathrm {d}x\), ut(x,t)≢0 for (x,t) ∈Ω× (0,t0). Recalling (2.7), J(u(t0)) < J(u0). Thus, \(u(t_{0})\in \mathcal {N}^{J(u_{0})}\). By the definition of \(\lambda _{J(u_{0})}\), we have
By I(u(t)) > 0 for t ∈ [0,t0) and \(\frac {\mathrm {d}}{\mathrm {d}t}\|u\|_{2}^{2}=-2I(u)\), we have \(\|u(t_{0})\|_{2}<\|u_{0}\|_{2}\leq \lambda _{J(u_{0})}\), which contradicts to (5.3). Therefore, our claim is true and we have \(u(t)\in J^{J(u_{0})}\) for all t ∈ [0,T(u0)). Lemma 5.1 (ii) shows that u(t) is bounded in \({H_{0}^{2}}({\Omega })\) for t ∈ [0,T(u0)), and the boundedness of \(\|u\|_{{H_{0}^{2}}({\Omega })}\) is dependent of t. Moreover, \(T(u_{0})=+\infty \). Let ω ∈ ω(u0). By (2.7) and \(\frac {\mathrm {d}}{\mathrm {d}t}\|u\|_{2}^{2}=-2I(u)\), one has \( \|\omega \|_{2}<\lambda _{J(u_{0})}\) and J(ω) < J(u0), which implies \(\omega (u_{0})\cap \mathcal {N}=\emptyset \). Hence, \(\omega (u_{0})=\left \{0\right \}\). Therefore, the weak solution u of (1.1) in its \({H^{2}_{0}}\)-norm exists globally and \(u(t)\rightarrow 0\) as \(t\rightarrow +\infty \).
(ii) Assume that \(u_{0}\in \mathcal {N}_{-}\) with \(\|u_{0}\|_{2}\geq {\Lambda }_{J(u_{0})}\). We claim that \(u(t)\in \mathcal {N}_{-}\) for all t ∈ [0,T(u0)). If not, there would exist a constant t0 ∈ (0,T(u0)) such that \(u(t)\in \mathcal {N}_{-}\) for t ∈ [0,t0) and \(u(t^{0})\in \mathcal {N}\). Similarly to case (i), one has J(u(t0)) < J(u0), which implies that \(u(t^{0})\in J^{J(u_{0})}\). Therefore, \(u(t^{0})\in \mathcal {N}^{J(u_{0})}\). According to the definition of \({\Lambda }_{J(u_{0})}\), we have
From \(\frac {\mathrm {d}}{\mathrm {d}t}\|u\|_{2}^{2}=-2I(u)\) and I(u(t)) < 0 for t ∈ [0,t0), we get \(\|u(t^{0})\|_{2}>\|u_{0}\|_{2}\geq {\Lambda }_{J(u_{0})}\), a contradiction to (5.4). Suppose \(T(u_{0})=+\infty \). For every ω ∈ ω(u0), by (2.7) and \(\frac {\mathrm {d}}{\mathrm {d}t}\|u\|_{2}^{2}=-2I(u)\), one has \( \|\omega \|_{2}>{\Lambda }_{J(u_{0})}\) and J(ω) < J(u0). Recalling \({\Lambda }_{J(u_{0})}\), we obtain \(\omega (u_{0})\cap \mathcal {N}=\emptyset \). Thus, \(\omega (u_{0})=\left \{0\right \}\), which contradicts to Lemma 5.1 (i). Hence, \(T(u_{0})<+\infty \). □
Proof of Theorem 2.6.
Assume that M > d and Ω1 and Ω2 are two arbitrary disjoint open subdomains of Ω. Assume that \(v\in Q({\Omega }_{1}):=\{u:u\in {H_{0}}^{2}({\Omega }_{1})\}\) is an arbitrary nonzero function and take α > 0 large enough such that
We fix such a number α > 0 and choose \(\mu \in Q({\Omega }_{2}):=\{u:u\in {H_{0}}^{2}({\Omega }_{2})\}\) satisfying M = J(μ) + J(αv). Extend v and μ to be 0 in Ω ∖Ω1 and Ω ∖Ω2. Set uM = αv + μ. Then M = J(αv + μ) = J(uM) and \(\|u_{M}\|_{2}>\|\alpha v\|_{2}>\left [(1+|{\Omega }|)^{1+p}(1+p)^{2}J(u_{M})\right ]^{\frac {1}{1+p}}\). By Lemma 5.3, \(u_{M}\in {\mathcal {N}}_{-}\) and the weak solution u of problem (1.1) blows up in finite time. □
6 Proof of Theorems 2.7 and 2.8
Lemma 6.1
Assume a nonnegative continuous φ(t) satisfies \( \varphi ^{\prime }(t)+2\lambda _{1}\varphi (t)\leq \frac {2|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\mathrm {e}(p^{\ast }-p^{+})}\varphi ^{\frac {p^{\ast }+1}{2}}(t)\), and \( \varphi (0)>\left [\frac {|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\lambda _{1} \mathrm {e}(p^{\ast }-p^{+})}\right ]^{\frac {2}{1-p^{\ast }}}\), where 0 < p− < p+ < p∗ < 1. There exists a constant T1 > 0 such that
where \(T_{1} :=- {2\varphi ^{\frac {1-p^{\ast }}{2}}(0)}/{\psi (0)}\), \(\frac {2}{{\lambda }_{1}(1-p^{\ast })}\leq T_{1}\leq \frac {-2|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\lambda _{1} \mathrm {e}(p^{\ast }-p^{+})\psi (0)}\), and
Proof
For simplicity, we denote \(M_{1}:=\frac {2|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\mathrm {e}(p^{\ast }-p^{+})}\), M2 := 2λ1. First, it is easy to observe that the following fact remains true. \( \varphi ^{\prime }(t)+M_{2}\varphi (t)\leq M_{1}\varphi ^{\frac {p^{\ast }+1}{2}}(t)\). Define \(H(t):=\varphi ^{\frac {1-p^{\ast }}{2}}(t)\). Then
Since ψ(0) < 0 and recalling the continuity of ψ(t), there exists a sufficiently small T0 > 0 such that
The estimates (6.2) and (6.3) indicate that \(H^{\prime }(t)\leq {\psi (0)}/{2}\), which implies that
Obviously, by the definition of H(t), we have (6.1). □
Lemma 6.2
Suppose constants p, α, β > 0 and h(t) be a nonnegative and absolutely continuous function satisfying \( h^{\prime }(t)+\alpha h^{p}(t)\geq \beta \), \(t\in (0,+\infty )\). Then there exists an estimate \( h(t)\geq \min \limits \left \{h(0),\left ({\beta }/{\alpha }\right )^{\frac {1}{p}}\right \}\).
In fact, the proof of this lemma can be similarly by ones for Lemma 3.2 in [17], where we use \( h^{\prime }(t)+\alpha h^{p}(t)\geq \beta \), \(t\in (0,+\infty )\) instead of \(h^{\prime }(t)+\alpha \max \limits \{h^{p}(t), h^{q}(t)\}\geq \beta \), \(t\in (0,+\infty )\). \(\Box \)
Proof of Theorem 2.7.
Multiplying the nonlinear equation in (1.1) by u and integrating it over Ω × (t,t + h) with h > 0 and then dividing the result by h yields
Let \(h\rightarrow 0^{+}\) in (6.4) and use the Lebesgue differentiation theorem. We have
where \( G(t):=\|u\|_{2}^{2}\). By \(x^{-\mu }\log x\leq (e\mu )^{-1}\) for x ≥ 1, μ ≥ 0 and Hölder inequality, we obtain
By using \(\|u\|_{2}^{2}\leq \lambda _{1}^{-1}\|{\varDelta } u\|_{2}^{2}\) and (6.5, 6.6), we have \( G^{\prime }(t)+2\lambda _{1}G(t)\leq \frac {|{\Omega }|^{\frac {1-p^{\ast }}{2}}}{\mathrm {e}(p^{\ast }-p^{+})}G^{\frac {p^{\ast }+1}{2}}(t)\). By Lemma 6.1 and the definition of G(t) above, we obtain (2.13). □
Proof of Theorem 2.8.
Let \(G(t):= {\int \limits }_{\Omega }u^{2}\mathrm {d}x\). According to the definition of J(u) and applying the results in Lemma, we have
Moreover, by \(x^{-\mu }\log x\leq (e\mu )^{-1}\) for x ≥ 1, μ > 0 and Hölder’s inequality, we obtain that
By (6.7, 6.8) and p− < 1, we have
By (6.9) and Lemma 6.2, we show \( G(t)\geq \min \limits \left \{G(0),\ \left ({\beta }/{\alpha }\right )^{\frac {2}{p^{\ast }+1}}\right \}\) with
□
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The authors would like to express their sincerely thanks to the Editor and the Reviewers for the constructive comments to improve this paper.
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This paper is supported by the Shandong Provincial Natural Science Foundation of China (ZR2021MA003, ZR2020MA020).
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Liu, B., Zhang, M. Classification of Singular Solutions in a Nonlinear Fourth-Order Parabolic Equation. J Dyn Control Syst 29, 455–474 (2023). https://doi.org/10.1007/s10883-022-09597-y
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DOI: https://doi.org/10.1007/s10883-022-09597-y