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Dynamics of plate equations with time delay driven by additive noise in \(\mathbb{R}^{n}\)
Journal of Inequalities and Applications volume 2023, Article number: 68 (2023)
Abstract
This paper is concerned with the asymptotic behavior of solutions for plate equations with delay blurred by additive noise in \(\mathbb{R}^{n}\). First, we obtain the uniform compactness of pullback random attractors of the problem, then derive the upper semicontinuity of the attractors.
1 Introduction
Delays in differential systems are used for mathematical modeling in many applications to describe the dynamics influenced by events from the past. It is known that differential equations with delay appears in physics, biology, and other disciplines, and the time delay is considered in the model of the systems [7, 12]. In particular, these equations are applied to mathematical modeling in many applications to describe the dynamics influenced by events from the past, see [15, 16, 18]. Most noteworthy is that the attractors of deterministic differential equations with a time delay have been studied in [11], while the stochastic case has been studied in [6, 29].
This paper is concerned with the following plate equations with time delay blurred by additive noise in \(\mathbb{R}^{n}\):
where \(\tau \in \mathbb{R}\), \(x\in \mathbb{R}^{n}\), \(s\in [-\rho ,0]\), \(\epsilon \in (0, 1]\), α, λ are positive constants, the time delay \(\rho >0\) is a constant, the conditions F, f are satisfied (see Sect. 3), \(g(x,\cdot )\in L^{2}_{\mathrm{loc}}(\mathbb{R}, L^{2}(\mathbb{R}^{n}))\), \(h\in H^{2}(\mathbb{R}^{n})\) and \(\phi \in C([\tau -\rho , \tau ], H^{2}(\mathbb{R}^{n}))\), W is a two-side real-value Wiener process on a complete probability space that will be specified later.
For the deterministic case, many authors obtained the existence of global attractors in [2, 8–10, 30–33, 40]. For the stochastic case, Ma and Shen investigated the existence of random attractors for plate equations in bounded domains in [14, 19, 20]. Moreover, in the entire space, Yao obtained the existence of random attractors for plate equations in [34–39]. Wang investigated the global existence as well as long-term dynamics for a wide class of lattice plate equations on the entire integer set with nonlinear damping driven by infinite-dimensional nonlinear noise in [27].
For the case \(\rho \equiv 0\) in (1.1), we derived the existence of results in [35]. However, as far as we know, there is little literature dealing with stochastic time-delay plate equations. Also, in [28], Wang and Ma studied the existence of pullback attractors for the nonautonomous suspension-bridge equation with time delay.
Motivated by the literature above, we study the dynamics of the delay plate equations. The main features of the work are summarized as follows: (i) We prove that (1.1) generates random dynamical systems; (ii) We show the existence of random attractors for (1.1); (iii) We obtain the convergence of random attractors for (1.1) as \(\rho \rightarrow 0\) or \(\epsilon \rightarrow 0\). A major difficulty in the proof process is to prove the existence random attractors for (1.1), the reason for this is that Sobolev embeddings are no longer compact. To overcome this, we use the uniform estimates and the splitting technique ([26]).
This paper is organized as follows. In the next section, we recall some basic concepts on the theory of random dynamical systems. We then prove an abstract result for the upper semicontinuity of random attractors for stochastic delay equations. In Sect. 3, we establish the continuous random dynamical system for (1.1). Some necessary estimates are given in Sect. 4. We then prove the existence of pullback attractors for (1.1) in Sect. 5. In Sects. 6 and 7, we further prove the upper semicontinuity of attractors when \(\epsilon \rightarrow 0\) and \(\rho \rightarrow 0\).
2 Mathematical setting and notation
Now, we recall some notations and propositions on the theory of random dynamical systems, the reader is referred to [1, 3, 4, 13, 17, 21–24].
Denote \((\Omega ,\mathcal{F},\mathbb{P})\) as the probability space and for \(t\in \mathbb{R}\), \(\omega \in \Omega \),
Let \((X, \|\cdot \|_{X})\) be a separable Hilbert space, and let \((\Omega ,\mathcal{F},\mathbb{P},\{\theta _{t}\}_{t\in \mathbb{R} })\) be an ergodic metric dynamical system
Proposition 2.1
([24])
Let \(\mathcal{D}\) be an inclusion closed collection of some families of nonempty subsets of X, and Φ be a continuous cocycle on X over \((\Omega ,\mathcal{F},\mathbb{P},\{\theta _{t}\}_{t\in \mathbb{R} })\). Then, Φ has a unique \(\mathcal{D}\)-pullback random attractor \(\mathcal{A}\) in \(\mathcal{D}\) if Φ is \(\mathcal{D}\)-pullback asymptotically compact in X and Φ has a closed measurable \(\mathcal{D}\)-pullback absorbing set K in \(\mathcal{D}\).
We denote by \(C_{X}\) the space \(C([-\rho ,0],X)\) with the sup-norm
Denote by \((Y,\|\cdot \|)\) a Banach space that satisfies that the injection \(X \subset Y\) is continuous, we also denote by \(C_{X,Y}\) the Banach space \(C_{X}\cap C^{1}([-\rho ,0],Y)\) with the norm \(\|\cdot \|_{C_{X,Y}}\)
Denote −Δ the Laplace operator, \(A=\Delta ^{2}\) and the Hilbert spaces \(V_{r} = D(A^{\frac{r}{4}})\) endowed with inner product and norm
In particular, \(V_{0}=L^{2}(\mathbb{R}^{n})\), \(V_{2}=H^{2}(\mathbb{R}^{n})\).
3 Random dynamical system
In this section, we discuss the assumptions on F, f, and g and define a continuous cocycle in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) for (1.1). Assume \(F(x,\cdot )\in C^{2}(\mathbb{R}), f, g\) satisfy the following conditions:
Let \(\widetilde{F}(r,x)=\int _{0}^{r}F(s,x)\,ds\) for \(x\in \mathbb{R}^{n}\) and \(s\in \mathbb{R}\),
where \(\varpi , l_{f}>0\), \(1\leq p\leq \frac{n+4}{n-4}\) and \(c_{i}>0\). It follows from (3.1) and (3.2) that
Assume g satisfies
which implies that
where σ is a positive constant.
For \(Y=(u,v)^{\top}\in C_{V_{2},V_{0}}(\mathbb{R}^{n})\), set
In addition, we see that \(\|\cdot \|_{C_{V_{2},V_{0}}}(\mathbb{R}^{n})\) is equivalent to \(\|\cdot \|_{C_{V_{2},V_{0}}(\mathbb{R}^{n})}\) in (2.1).
Let \(\xi =\partial _{t}u+\delta u\), for \(x\in \mathbb{R}^{n}\), \(s\in [-\rho ,0]\), hence problem (1.1) is equivalent to
Let \(z(\theta _{t}\omega )=hy(\theta _{t}\omega )\), where y satisfies
From [5], we know that for every \(\omega \in \Omega \), \(y(\theta _{t}\omega )\) is continuous.
Let \(z(\theta _{t}\omega )=hy(\theta _{t}\omega )\). We have the following lemma on \(z(\theta _{t}\omega )\):
Lemma 3.1
([32])
For \(\forall \varepsilon >0\), there exists a random variable \(\chi :\Omega \rightarrow \mathbb{R}^{+}\), such that for \(\forall t\in \mathbb{R}\), \(\omega \in \Omega \),
where
Denote \(v(t)=\xi (t)-\epsilon z(\theta _{t}\omega )\), then (3.10) is equivalent to
For given \(\tau \in \mathbb{R}\), \(\omega \in \Omega \), and \(\phi \in C_{V_{2}}(\mathbb{R}^{n})\), \(\psi \in C_{V_{0}}(\mathbb{R}^{n})\), a solution of (3.11) will be written as \((u(\cdot ,\tau ,\omega ,\phi ),v(\cdot , \tau ,\omega ,\psi ))\). As usual, the segments of \(u(\cdot ,\tau ,\omega ,\phi )\) and \(v(\cdot ,\tau ,\omega ,\psi )\) on \([t-\rho , t]\) are written as \(u^{t}(\cdot ,\tau ,\omega ,\phi )\) and \(v^{t}(\cdot ,\tau ,\omega ,\psi )\), respectively; that is,
Under conditions (3.1)–(3.5), for \(\tau \in \mathbb{R}\), \(\omega \in \Omega \), and \(\phi \in C_{V_{2}}(\mathbb{R}^{n})\), \(\psi \in C_{V_{0}}(\mathbb{R}^{n})\), problem (3.11) has a unique continuous solution \((u(\cdot ,\tau ,\omega ,\phi ),v(\cdot , \tau ,\omega ,\psi )):[ \tau -\rho ,\infty ]\rightarrow C_{V_{2},V_{0}}(\mathbb{R}^{n})\), and the segment \(u_{t}(\cdot ,\tau ,\omega ,\phi )\) of u is \((\mathcal{F},~\mathcal{B}(C_{V_{2}}(\mathbb{R}^{n})))\)-measurable in \(\omega \in \Omega \) and continuous with respect to ϕ in \(C_{V_{2}}(\mathbb{R}^{n})\); the segment \(v_{t}(\cdot ,\tau ,\omega ,\psi )\) of v is \((\mathcal{F},~\mathcal{B}(C_{V_{0}}(\mathbb{R}^{n})))\)-measurable in \(\omega \in \Omega \) and continuous with respect to ψ in \(C_{V_{0}}(\mathbb{R}^{n})\).
Define \(\Phi :\mathbb{R}^{+}\times \mathbb{R}\times \Omega \times C_{V_{2},V_{0}}( \mathbb{R}^{n})\rightarrow C_{V_{2},V_{0}}(\mathbb{R}^{n})\) by
where \((t,\tau ,\omega ,(\phi ,\psi ))\in \mathbb{R}^{+}\times \mathbb{R} \times \Omega \times C_{V_{2},V_{0}}(\mathbb{R}^{n})\), \(u_{t+\tau}(s,\tau ,\theta _{-\tau}\omega ,\phi )=u(t+\tau +s,\tau , \theta _{-\tau}\omega ,\phi )\) for \(s\in [-\rho ,0]\); \(v_{t+\tau}(s,\tau ,\theta _{-\tau}\omega ,\psi )=v(t+\tau +s,\tau , \theta _{-\tau}\omega ,\psi )\) for \(s\in [-\rho ,0]\). Then, Φ is a continuous cocycle on \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) over \((\Omega ,\mathcal{F},\mathbb{P},\{\theta _{t}\}_{t\in \mathbb{R} })\).
Let \(D=\{D(\tau ,\omega )\subseteq C_{V_{2},V_{0}}(\mathbb{R}^{n}):\tau \in \mathbb{R}, \omega \in \Omega \}\) be a family of bounded nonempty subsets of \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) satisfying
where \(\|D(\tau -t,\theta _{-t}\omega )\|_{C_{V_{2},V_{0}}(\mathbb{R}^{n})}= \sup_{(u,v)\in D(\tau -t,\theta _{-t}\omega )}\|(u,v)\|_{C_{V_{2},V_{0}}( \mathbb{R}^{n})}\). Let \(\mathcal{D}\) be the set of all families \(D=\{D(\tau ,\omega )\subseteq C_{V_{2},V_{0}(\mathbb{R}^{n})}:\tau \in \mathbb{R}, \omega \in \Omega \}\) that satisfies (3.13).
For later purposes, we assume \(\delta \in (0,1)\) satisfies
In addition,
Under (3.15), assume σ satisfies
4 Uniform estimates
We will obtain some necessary estimates of solutions for (3.11) in this section.
Lemma 4.1
Assume that (3.1)–(3.5), (3.7), (3.14), and (3.16) hold. Then, for \(\forall \varsigma ,\tau \in \mathbb{R}\), \(\omega \in \Omega \), and \(D=\{D(\tau ,\omega ):\tau \in \mathbb{R},\omega \in \Omega \}\in \mathcal{D}\), there exists \(T=T(\tau ,\omega ,D,\varsigma )>0\) such that for \(\forall t\geq T\),
where \(Y_{0}=(\phi ,\psi )^{\top}\in D(\tau -t,\theta _{-t}\omega )\) and M is a positive constant independent of τ, ω, D, and ϵ, but dependent on λ, σ, α, and δ.
Proof
Taking the inner product with (3.11)2 by v in \(L^{2}(\mathbb{R}^{n})\), we obtain
By simple calculation, we can obtain the following estimates for the right-hand side of (4.2):
By (3.2) we obtain
From (3.1) and (3.3), we obtain
From (3.5), we have
Equations (4.3)–(4.11), together with (4.2), imply
and together with (3.16) we obtain
Substituting τ by \(\tau -t\), and integrating (4.13) between \([\tau -t,\iota +s]\), we obtain
Note that
By (4.14), (4.15), and (3.16) we obtain
Combination of Lemma 3.1 and (3.7) implies that
Equation (3.6) yields
We can deduce that
which together with (3.3), (4.16), and (4.17) yields (4.1). □
Let ρ be a smooth function on \(\mathbb{R}^{+}\) such that \(0\leq \rho (s)\leq 1\) for all \(s\in \mathbb{R}^{+}\), and
For every \(k\in \mathbb{N}\), let
We also assume that for all \(x\in \mathbb{R}^{n}\) and \(k\in \mathbb{N}\), \(|\nabla \rho _{k}|\leq \frac{1}{k}c_{4}\), \(|\Delta \rho _{k}|\leq \frac{1}{k}c_{5}\), \(|\Delta \nabla \rho _{k}|\leq \frac{1}{k}c_{6}\), \(|\Delta ^{2}\rho _{k}|\leq \frac{1}{k}c_{7}\), where \(c_{4}\), \(c_{5}\), \(c_{6}\), and \(c_{7}\) are positive constants independent of k.
Given \(k\geq 1\), denote \(\mathbb{H}_{k}=\{x\in \mathbb{R}^{n}:|x|< k\}\) and \(\mathbb{R}^{n}\setminus \mathbb{H}_{k}\) the complement of \(\mathbb{H}_{k}\).
Lemma 4.2
Suppose (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. Then, for \(\forall \tau \in \mathbb{R}\), \(s\in [-\rho ,0]\), \(\omega \in \Omega \), there exist \(\widetilde{R}=\widetilde{R}(\tau ,\omega ,\varepsilon )\geq 1\) and \(T=T(\tau ,\omega ,D,\varepsilon )>0\), such that for \(\forall k\geq \widetilde{R}\), \(t\geq T\),
Proof
Multiplying (3.11)2 with \(\rho _{k}(x)v\), we have
For the terms on the right-hand side of (4.20), using Young’s inequality and the interpolation inequality
we have
From (3.5) we deduce that
Then, it follows from (4.20)–(4.30) and (3.16) that
Multiplying (4.31) by \(e^{\sigma t}\) and integrating between \(\tau -t\) and \(\tau +s\), then substituting ω by \(\theta _{-\tau}\omega \) and rearranging, we obtain
Since \((\phi ,\psi )^{\top}\in D(\tau -t,\theta _{-t}\omega )\in \mathcal{D}\) together with (3.6) we know that there exists \(\widetilde{T_{1}}=\widetilde{T_{1}}(\tau ,\varepsilon ,\omega ,D)>0\), such that for \(\forall t>\widetilde{T_{1}}\),
From Lemma 4.1, there are \(\widetilde{T_{2}}=\widetilde{T_{2}}(\tau ,\varepsilon ,\omega ,D)>0\) and \(\widetilde{R_{1}}=\widetilde{R_{1}}(\varepsilon ,\omega ,D)>1\), such that for \(\forall t>\widetilde{T_{2}}\), \(k>\widetilde{R_{1}}\),
By Lemma 3.1, there are \(\widetilde{T_{3}}=\widetilde{T_{3}}(\varepsilon ,\omega )>0\), \(\widetilde{R_{2}}=\widetilde{R_{2}}(\varepsilon ,\omega )>1\), such that for \(\forall t>\widetilde{T_{3}}\), \(k>\widetilde{R_{2}}\),
By (3.8), there exists \(\widetilde{R_{3}}=\widetilde{R_{3}}(\tau ,\varepsilon )>1\), such that for \(\forall k>\widetilde{R_{3}}\),
Letting \(\widetilde{R}=\max \{\widetilde{R_{1}},\widetilde{R_{2}}, \widetilde{R_{3}}\}\), \(\widetilde{T}=\max \{\widetilde{T_{1}},\widetilde{T_{2}}, \widetilde{T_{3}}\}\), together with (4.32)–(4.36), for \(\forall t>\widetilde{T}\), \(k>\widetilde{R}\), we obtain
which together with (3.3) implies (4.19). □
For \(\forall x\in \mathbb{R}^{n}\) and \(k\geq 1\), denote
where \(\widehat{\rho _{k}}=1-\rho _{k}\). Then, for \(k\geq 1\), \(x\in \mathbb{R}^{n}\setminus \mathbb{H}_{k}\), we have \(\widehat{u}(t,\tau ,\omega ,\widehat{\phi})=\widehat{v}(t,\tau , \omega ,\widehat{\psi})=0\). In addition, there is some constant \(c>0\) independent of \(k\geq 1\), such that \(\|\widehat{u}\|_{H^{2}(\mathbb{R}^{n})}\leq c \|u\|_{H^{2}( \mathbb{R}^{n})}\), \(\|\widehat{v}\|_{L^{2}(\mathbb{R}^{n})}\leq c \|v\|_{L^{2}( \mathbb{R}^{n})}\). Accordingly, together with (3.11) and (4.38), we obtain
Considering the eigenvalue problem
it is easy to see that eigenfunctions \(\{e_{i}\}_{i\in \mathbb{N}}\) and eigenvalues \(\{\lambda _{i}\}_{i\in \mathbb{N}}\) of (4.40) satisfy:
For given n, assume \(X_{n}=\operatorname{span}\{e_{1},\ldots ,e_{n}\}\), \(P_{n}:L^{2}(\mathbb{H}_{k})\rightarrow X_{n}\).
Lemma 4.3
Suppose (3.1)–(3.5), (3.7), (3.14), and (3.16) hold. Then, for \(\forall \omega \in \Omega \), \(\tau \in \mathbb{R}\), \(s\in [-\rho ,0]\), \(D= \{D(\tau ,\omega ):\tau \in \mathbb{R},\omega \in \Omega \}\in \mathcal{D}\), there exists \(\widehat{R}=\widehat{R}(\tau ,\omega ,\varepsilon )\geq 1\), \(\widehat{T}=\widehat{T}(\tau ,\omega ,D,\varepsilon )>0\), \(N=N(\tau , \omega ,\varepsilon )>0\), such that for \(\forall t\geq \widehat{T}\), \(n\geq N\), \(k\geq \widehat{R}\),
Proof
Denote \(\widehat{u}_{n,2}=(I-P_{n})\widehat{u}\), \(\widehat{u}_{n,1}=P_{n} \widehat{u}\), \(\widehat{v}_{n,2}=(I-P_{n})\widehat{v}\), \(\widehat{v}_{n,1}=P_{n} \widehat{v} \). Multiplying (4.39)1 with \(I-P_{n}\), we obtain
Multiplying (4.39)2 with \(I-P_{n}\) then taking the inner product with \(\widehat{v}_{n,2}\) in \(L^{2}(\mathbb{H}_{k})\), we have
For the right-hand side of (4.43), by simple calculation, we obtain the following estimates
From (3.1), choosing \(\theta =\frac{n(p-1)}{4(p+1)}\), we obtain
It follows from the Cauchy inequality and Young’s inequality that
Therefore, by (3.16), (4.43)–(4.52), and the fact \(\eta _{1}\in L^{2}(\mathbb{R}^{n})\), \(\lambda _{n}\rightarrow \infty \), there are \(\widehat{N}_{1}=\widehat{N}_{1}(\varepsilon )>0\), \(\widehat{R}_{1}= \widehat{R}_{1}(\varepsilon )>0\) such that for \(\forall n>\widehat{N}_{1}\), \(k>\widehat{R}_{1}\),
Using a similar calculation with (4.14) and (4.15), and combining with (3.16) we have that
Since \((\widehat{\phi},\widehat{\psi})^{\top}\in D(\tau -t,\theta _{-t} \omega )\in \mathcal{D}\), then there are \(\widehat{T}_{1}=\widehat{T}_{1}(\tau ,\varepsilon ,D,\omega )>0\), \(\widehat{R}_{1}=\widehat{R}_{1}(\tau ,\varepsilon ,\omega )>1\), such that for \(t>\widehat{T}_{1}\), \(k>\widehat{R}_{1}\)
From (3.7), there exists \(\widehat{N}=\widehat{N}(\tau ,\varepsilon ,\omega )>0\), such that for \(\forall n>\widehat{N}\)
From Lemma 4.1, there are \(\widehat{T}_{2}=\widehat{T}_{2}(\tau ,\varepsilon ,D,\omega )>0\), \(\widehat{R}_{2}(\tau ,\varepsilon ,\omega )>1\), such that for \(\forall t>\widehat{T}_{2}\), \(k>\widehat{R}_{2}\),
By Lemma 4.1, there is \(\widehat{T}_{3}=\widehat{T}_{3}(\tau ,\varepsilon ,D,\omega )>0\), for \(\forall t>\widehat{T}_{3}\)
which together with (4.54)–(4.57) gives the desired result (4.41). □
5 Existence of random attractors
In this section, we establish the existence and uniqueness of random attractors for problem (3.11). We can easily obtain the existence of random absorbing sets of Φ from Lemma 4.1.
Lemma 5.1
Suppose (3.1)–(3.5), (3.7), (3.14), and (3.16) hold. Then, for \(\forall \epsilon \in (0,1]\), \(\omega \in \Omega \), \(\tau \in \mathbb{R}\), the cocycle Φ has a random absorbing set \(K_{\epsilon}=\{K_{\epsilon}(\tau ,\omega ):\tau \in \mathbb{R}, \omega \in \Omega \}\in \mathcal{D}\) as
with \(Y=(u,v)^{\top}\) and
Next, we establish the asymptotic compactness of the cocycle Φ in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\).
Lemma 5.2
Suppose (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. Then, the cocycle Φ is \(\mathcal{D}\)-pullback asymptotically compact in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\).
Proof
For \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \) and \(D=\{D(\tau ,\omega ):\tau \in \mathbb{R},\omega \in \Omega \}\in \mathcal{D}\), we will prove that the sequence \(\{Y_{\tau}(\cdot , \tau -t_{n},\theta _{-\tau}\omega ,Y_{0,n})\}\) has a convergent subsequence in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) whenever \(t_{n}\rightarrow \infty \) and \(Y_{0,n}\in D(\tau -t_{n},\theta _{-\tau}\omega )\).
From Lemma 4.1, \(\{Y_{\tau}(\cdot , \tau -t_{n},\theta _{-\tau}\omega ,Y_{0,n})\}\) is bounded in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\); which means that for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \), there is \(\widehat{N}_{1}=\widehat{N}_{1}(\tau ,\omega ,D)>0\) for \(\forall n>\widehat{N}_{1}\),
In addition, from Lemma 4.2 we know that there are \(k_{1}=k_{1}(\tau ,\varepsilon ,\omega )>0\), \(\widehat{N}_{2}= \widehat{N}_{2}(\tau ,D,\varepsilon , \omega )>0\), for \(\forall n\geq \widehat{N}_{2}\) and fixed \(s\in [-\rho ,0]\),
From Lemma 4.3, there exist \(N=N(\tau ,\varepsilon ,\omega )>0\), \(k_{2}=k_{2}(\tau ,\varepsilon ,\omega )\geq k_{1}\), \(\widehat{N}_{3}= \widehat{N}_{3}(\tau ,D,\varepsilon ,\omega )>0\), for \(\forall n\geq \widehat{N}_{3}\) and fixed \(s\in [-\rho ,0]\),
By (4.38) and (5.2), we see that \(\{P_{N}\widehat{Y}(\tau +s, \tau -t_{n},\theta _{-\tau}\omega , \widehat{Y}_{0,n})\}\) is bounded in \(P_{N}H^{2}(\mathbb{H}_{2k_{2}})\times L^{2}(\mathbb{H}_{2k_{2}})\), together with (5.4) we find \(\{\widehat{Y}(\tau +s, \tau -t_{n},\theta _{-\tau}\omega , \widehat{Y}_{0,n})\}\) is precompact in \(H^{2}(\mathbb{H}_{2k_{2}})\times L^{2}(\mathbb{H}_{2k_{2}})\).
Note that \(\widehat{\rho _{k_{2}}}=1\) for \(|x|\leq \frac{k_{2}}{2}\). By (4.38), we obtain \(\{Y(\tau +s, \tau -t_{n},\theta _{-\tau}\omega ,Y_{0,n})\}\) is precompact in \(H^{2}(\mathbb{H}_{k_{2}})\times L^{2}(\mathbb{H}_{k_{2}})\), which together with (5.3) shows the precompactness of this sequence in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) for fixed \(s\in [-\rho ,0]\). □
As an immediate consequence of Proposition 2.1, Lemma 5.1, and Lemma 5.2, we have
Theorem 5.1
Assume that (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. Then, for every \(\epsilon \in (0,1]\), the continuous cocycle Φ associated with (3.11) has a unique \(\mathcal{D}\)-pullback attractor \(\mathcal{A}_{\epsilon}=\{\mathcal{A}_{\epsilon}(\tau ,\omega ):\tau \in \mathbb{R},\omega \in \Omega \}\in \mathcal{D}\) in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\).
6 Upper semicontinuity of attractors as \(\epsilon \rightarrow 0\)
In this section, we establish the upper semicontinuity of random attractors of the plate Eq. (3.11) with delay driven by additive noise when \(\epsilon \rightarrow 0\). We write the solution and the corresponding cocycle of (3.11) as \(u^{\epsilon}\), \(v^{\epsilon}\) and \(\Phi _{\epsilon}\), respectively.
In Sect. 5, we obtained that \(\Phi _{\epsilon}\) has a \(\mathcal{D}\)-pullback attractor \(\mathcal{A}_{\epsilon}\in \mathcal{D}\) in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) and random absorbing set \(K_{\epsilon}=\{K_{\epsilon}(\tau ,\omega ):\tau \in \mathbb{R}, \omega \in \Omega \}\) with \(K_{\epsilon}(\tau ,\omega )\subseteq K(\tau ,\omega )\) for all \(\epsilon \in (0,1]\), where for every \(\tau \in \mathbb{R}\), \(\omega \in \Omega \),
and
where \(Y=(u,v)^{\top}\).
From Lemma 5.1 we know for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \),
As \(\epsilon =0\), the problem (3.11) reduces to a deterministic one:
Accordingly, by Theorem 5.1 the cocycle \(\Phi _{0}\) generated by (6.2) has a unique random attractor \(\mathcal{A}_{0}=\{\mathcal{A}_{0}(\tau ):\tau \in \mathbb{R}\}\in \mathcal{D}_{0}\) in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\) and a random absorbing set \(K_{0}=\{K_{0}(\tau ):\tau \in \mathbb{R}\}\), where
and
where
Note that \(R_{0}(\tau )\) corresponds to the number \(R_{\epsilon}(\tau ,\omega )\) given by (5.1) with \(\epsilon = 0\). From Lemma 5.1 and (6.3) and (6.4) we have that for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \),
Now, we will establish the convergence of the solutions of (3.11) as \(\epsilon \rightarrow 0\) to obtain the upper semicontinuity of the \(\mathcal{D}\)-pullback attractor \(\mathcal{A}_{\epsilon}\).
Lemma 6.1
Let \(Y^{\epsilon}=(u^{\epsilon},v^{\epsilon})\) and \(Y=(u,v)\) be the solutions of (3.11) and (6.2) with initial values \(Y^{\epsilon}_{0}=(\phi ^{\epsilon},\psi ^{\epsilon})\) and \(Y_{0}=(\phi ,\widehat{\psi })\), respectively. Assume that (3.1)–(3.5) and (3.14) hold. If \(\lim_{\epsilon \rightarrow 0}(\phi ^{\epsilon},\psi ^{ \epsilon})=(\phi ,\widehat{\psi })\in C_{V_{2},V_{0}}(\mathbb{R}^{n})\), for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \), \(T>0\), \(t\in [\tau ,\tau +T]\),
Proof
Let \((u^{\epsilon}(t,\tau ,\omega ,\phi ^{\epsilon}),v^{\epsilon}(t, \tau ,\omega ,\psi ^{\epsilon}) )\) be the solution of (3.11) and \(\tilde{u}=u^{\epsilon}-u\), \(\tilde{v}=v^{\epsilon}-v\). Then, by (3.11) and (6.2) we have
Taking the inner product of (6.7)2 with ṽ, we obtain
By (3.4), we obtain
From (3.5), we have
which together with (6.7)–(6.9) gives
Integrating (6.10) between τ and t we obtain
Note that
Thus, for \(\forall t\in [\tau ,\tau +T]\), from (6.11), (6.12), and (3.9) we have that
Accordingly, for \(\forall t\in [\tau ,\tau +T]\), we obtain
Hence, if \(\lim_{\epsilon \rightarrow 0}(\phi ^{\epsilon},\psi ^{ \epsilon})=(\phi ,\widehat{\psi })\in C_{V_{2},V_{0}}(\mathbb{R}^{n})\), then
and hence by (6.13), for \(\forall t\in [\tau ,\tau +T]\),
which implies (6.6). □
Now, we establish the uniform compactness of \(\mathcal{A}_{\epsilon}\) in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\).
Lemma 6.2
Suppose (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. Then, for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \), \(\bigcup_{0<\epsilon \leq 1} \mathcal{A}_{\epsilon}(\tau , \omega )\) is precompact in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\).
Proof
Given \(\epsilon \in (0,1]\). First, from (6.4), Lemma 4.2, and the invariance of \(\mathcal{A}_{\epsilon}(\tau , \omega )\), we know that for \(\forall \epsilon >0, \tau \in \mathbb{R}\), \(\omega \in \Omega \), there is \(r_{0}=r_{0}(\omega ,\varepsilon )\geq 1\) such that
Secondly, from (6.1), Lemma 5.2, Lemma 4.3, and the invariance of \(\mathcal{A}_{\epsilon}(\tau , \omega )\), we know that there exists \(k_{1}=k_{1}(\omega ,\varepsilon )\geq k_{0}\) such that for \(\forall k\geq k_{1}\), the set \(\bigcup_{0<\epsilon \leq 1}\mathcal{A}_{\epsilon}(\tau , \omega )\) is precompact in \(C_{V_{2},V_{0}}(\mathbb{H}_{k})\), which together with (6.16) implies that \(\bigcup_{0<\epsilon \leq 1}\mathcal{A}_{\epsilon}(\tau , \omega )\) is precompact in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\). □
Now, we are ready to prove the upper semicontinuity of the \(\mathcal{A}_{\epsilon}\) as \(\epsilon \rightarrow 0\). In fact, it is an immediate consequence of Theorem 3.2 in [25] based on (6.5) and Lemmas 6.1 and 6.2.
Theorem 6.1
Assume that (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. Then, for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \),
7 Upper semicontinuity of attractors as \(\rho \rightarrow 0\)
In this section, we establish the upper semicontinuity of random attractors of the plate Eq. (3.11) when the delay ρ approaches zero for a fixed \(\epsilon \in (0,1]\). We write the solution and the corresponding cocycle of (3.11) as \(u^{\rho}\), \(v^{\rho}\) and \(\Phi ^{\rho}\), respectively.
For given \(\tau \in \mathbb{R}\), \(\omega \in \Omega \), denote
where \(R^{\rho}(\tau ,\omega )\) is equal to the right-hand side of (5.1). From (7.1) and Lemma 5.1 we know that, for all \(\rho \in (0,1]\), \(K^{\rho}=\{K^{\rho}(\tau ,\omega ):\tau \in \mathbb{R},\omega \in \Omega \}\) is a \(\mathcal{D}\)-pullback absorbing set of \(\Phi ^{\rho}\) in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\). In addition, for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \), \(\Phi ^{\rho}\) has a \(\mathcal{D}\)-pullback attractor \(\mathcal{A}^{\rho}\in \mathcal{D}\) in \(C_{V_{2},V_{0}}(\mathbb{R}^{n})\),
As \(\rho =0\), the stochastic delay system (3.11) becomes a stochastic system without delay given by
Accordingly, by Theorem 5.1 the cocycle \(\Phi ^{0}\) generated by (7.3) is readily verified to admit a unique \(\mathcal{D}^{0}\)-pullback attractor \(\mathcal{A}^{0}=\{\mathcal{A}^{0}(\tau ,\omega ):\tau \in \mathbb{R}, \omega \in \Omega \}\in \mathcal{D}^{0}\) in \(H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})\) and a \(\mathcal{D}^{0}\)-pullback absorbing set \(K^{0}=\{K^{0}(\tau ,\omega ):\tau \in \mathbb{R},\omega \in \Omega \}\), where
and
with \(R^{0}(\tau ,\omega )\) given by the right-hand side of (5.1).
From (7.1) and (7.4), we see that for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \),
Lemma 7.1
Suppose \(Y^{\rho}=(u^{\rho},v^{\rho})^{\top}\) and \(Y=(u,v)^{\top}\) are the solutions of (3.11) and (7.3) with initial values \(Y^{\rho}_{0}=(\phi ^{\rho},\psi ^{\rho})^{\top}\) and \(Y_{0}=(\phi ,\psi )^{\top}\), respectively. Assume that (3.1)–(3.5) and (3.14) hold. If \(\lim_{\rho \rightarrow 0}\sup_{-\rho \leq s\leq 0}\| Y^{ \rho}_{0}(s)-Y_{0}\|_{H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})}=0\), then for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \), \(T>0\), \(t\in [\tau , \tau +T]\),
Proof
For \(\forall s\in [-\rho ,0]\), \(t\geq \tau \), let \(\widehat{v}=v^{\rho}(t+s)-v(t)\) and \(\widehat{u}=u^{\rho}(t+s)-u(t)\), where \(v^{\rho }=\partial _{t}u^{\rho }+\delta u^{\rho }-\epsilon z(\theta _{t} \omega )\) and \(v =\partial _{t}u +\delta u -\epsilon z(\theta _{t}\omega )\) with \(\psi ^{\rho}(s)=\partial _{t}\phi ^{\rho}(s)+\delta \phi ^{\rho}(s)- \epsilon z(\theta _{t}\omega )\) and \(\psi (s)=\partial _{t}\phi (s)+\delta \phi (s)-\epsilon z(\theta _{t} \omega )\).
By (3.11) and (7.3) we see that for \(t>\tau -s\) and \(s\in [-\rho ,0]\),
Taking the inner product of (7.7) with v̂, then
From (3.4), we obtain
By (3.5), we obtain
which along with (7.7)–(7.9) implies
Integrating (7.10) over \((\tau -s,t)\) with \(t\in [\tau ,\tau +T]\), we obtain that
Note that
Thus, for \(\forall t\in [\tau ,\tau +T]\) with \(t>\tau -s\), from (7.11), (7.12), and (3.9) we have that
From Lemma 3.1, given \(\eta >0\), there is \(\rho _{1}\in (0,1]\) for \(\forall \rho \leq \rho _{1}\), \(s\in [-\rho ,0]\), \(r\in [\tau ,\tau +T]\),
By \(\lim_{\rho \rightarrow 0}\int ^{\tau +2\rho}_{\tau}\|u(r, x)- \phi \|^{2}\,dr=0\), we see for \(\forall \rho \leq \rho _{2}\), there is \(\rho _{2}\leq \rho _{1}\) such that
Note that u is uniformly continuous from \([\tau ,\tau +1+T]\) to \(H^{2}(\mathbb{R}^{n})\), and we obtain that there is \(\rho _{3}\leq \rho _{2}\) such that for \(\forall \rho \leq \rho _{3}\), \(r\in [\tau ,\tau +T]\),
Since \(g\in L^{2}_{\mathrm{loc}}(\mathbb{R},L^{2}(\mathbb{R}^{n}))\) one obtains that
which implies that there is \(\rho _{4}\leq \rho _{3}\) such that for \(\forall \rho \leq \rho _{4}\), \(s\in [-\rho ,0]\),
It follows from (7.13)–(7.18) that
Accordingly, we have
In addition,
which together with (7.16) shows that there is \(\rho _{5}\leq \rho _{4}\) such that for \(\forall \rho \leq \rho _{5}\), \(s\in [-\rho ,0]\),
It follows from (7.20) and (7.21) that for \(\forall \rho \leq \rho _{5}\), \(t\in [\tau ,\tau +T]\) with \(t>\tau -s\) and \(s\in [-\rho ,0]\),
For \(t\in [\tau ,\tau -s]\), we set \(r=t-\tau \). Thus, we have \(\tau -\rho \leq t+s\leq \tau \), \(t=r+\tau \). One can easily obtain that there is \(\rho _{6}\leq \rho _{5}\) such that for \(\forall \rho \leq \rho _{6}\), \(t\in [\tau ,\tau -s]\),
Hence, by (7.22) and (7.23) we obtain that
which gives (7.6). □
Lemma 7.2
Suppose (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. If \(\rho _{n}\rightarrow 0\), \(Y_{n}\in \mathcal{A}^{\rho _{n}}(\tau , \omega )\), then there exists a subsequence \(\{Y_{n_{m}}\}\) of \(\{Y_{n}\}\) and \(Y\in H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})\) such that
where \(Y=(u,v)^{\top}\).
Proof
Denote \(\{t_{n}\}^{\infty}_{n=1}\) as a sequence and \(t_{n}\rightarrow \infty \), \(n\rightarrow \infty \). By the invariance of \(\mathcal{A}^{\rho _{n}}\), there is \(\widehat{Y}_{n}\in \mathcal{A}^{\rho _{n}}(\tau -t_{n},\theta _{-t_{n}} \omega )\) such that
By (7.2), we have \(\widehat{Y}_{n}\in K^{\rho _{n}}(\tau -t_{n},\theta _{-t_{n}}\omega )\). By the uniform estimates obtained in Sect. 5, one can verify:
(i) \(\Phi ^{\rho _{n}} (t_{n},\tau -t_{n},\theta _{-t_{n}}\omega , \widehat{Y}_{n})(0)\) is precompact in \(H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})\).
(ii) For given \(\forall \eta >0\), there is \(N_{1}\geq 1\) such that for \(\forall n\geq N_{1}\), \(s\in [-\rho _{n}, 0]\),
From (i) we see that there is \(Y\in H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})\) such that
Thus, there is \(N_{2}\geq N_{1}\) such that for \(\forall n\geq N_{2}\),
together with (ii), for \(\forall n\geq N_{2}\) and \(s\in [-\rho _{n}, 0]\), we have
which along with (7.25) implies (7.24). □
Finally, we will prove the upper semicontinuity of \(\mathcal{A}^{\rho}\) as \(\rho \rightarrow 0\).
Theorem 7.1
Assume that (3.1)–(3.5), (3.7), (3.8), (3.14), and (3.16) hold. Then, for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \),
where \(d_{H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})}\) is defined for \(\forall E\subseteq C_{V_{2},V_{0}}(\mathbb{R}^{n})\), \(S\subseteq H^{2}( \mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})\) as
Proof
Let \(Y^{\rho _{n}}_{0}\in C_{V_{2},V_{0}}(\mathbb{R}^{n})\) and \(Y_{0}\in H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})\) with \(\sup_{-\rho _{n}\leq s\leq 0}\| Y^{\rho _{n}}_{0}(s)- Y_{0} \|_{H^{2}(\mathbb{R}^{n})\times L^{2}(\mathbb{R}^{n})}\rightarrow 0\) as \(n\rightarrow \infty \), \(\rho _{n}\rightarrow 0\). We have from Lemma 7.1 that for \(\forall \tau \in \mathbb{R}\), \(\omega \in \Omega \), \(t\geq \tau \),
By (7.4), (7.5), (7.29), and Lemma 7.2 we obtain (7.28) from Theorem 2.1 in [29] immediately. □
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The work was supported by the NSFC (Nos. 12161071 and 11961059).
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Yao, X. Dynamics of plate equations with time delay driven by additive noise in \(\mathbb{R}^{n}\). J Inequal Appl 2023, 68 (2023). https://doi.org/10.1186/s13660-023-02950-0
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DOI: https://doi.org/10.1186/s13660-023-02950-0
MSC
- 37B55
- 35B41
- 60H15
Keywords
- Dynamics
- Uniform compactness
- Time delay
- Entire space
- Additive noise