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Random attractors for stochastic plate equations with memory in unbounded domains

  • Xiao Bin Yao EMAIL logo
Published/Copyright: December 31, 2021

Abstract

In this paper, we investigate the dynamics of stochastic plate equations with memory in unbounded domains. More specifically, we obtain the uniform time estimates for solutions of the problem. Based on the estimates above, we prove the existence and uniqueness of random attractors in unbounded domains.

MSC 2010: 35B40; 35B41; 37L55; 35R60

1 Introduction

Let ( Ω , , P ) be the standard probability space, where Ω = { ω C ( R , R ) : ω ( 0 ) = 0 } , is the Borel σ -algebra induced by the compact open topology of Ω , and P is the Wiener measure on ( Ω , ) . There is a classical group { θ t } t R acting on ( Ω , , P ) , which is defined by

θ t ω ( ) = ω ( + t ) ω ( t ) , for all ω Ω , t R ,

then ( Ω , , P , { θ t } t R ) is an ergodic parametric dynamical system.

Considering the following non-autonomous stochastic plate equation with memory and multiplicative noise in unbounded domain R n :

(1.1) u t t + Δ 2 u + h ( u t ) + 0 μ ( s ) Δ 2 ( u ( t ) u ( t s ) ) d s + λ u + f ( x , u ) = g ( x , t ) + ε u d w d t

with the initial value conditions

(1.2) u ( x , τ ) = u 0 ( x ) , u t ( x , τ ) = u 1 ( x ) ,

where x R n , t > τ with τ R , λ > 0 and ε are constants, μ is the memory kernel, h ( u t ) is a nonlinear damping term, f is a given interaction term, g is a given function satisfying g L loc 2 ( R , H 1 ( R n ) ) , and w is a two-sided real-valued Wiener process on a probability space. The stochastic equation (1.1) is understood in the sense of Stratonovich’s integration.

Many studies have been carried out regarding the dynamics of a variety of systems related to equation (1.1). For example, if the random term is vanished, μ = 0 and g ( x , t ) = g ( x ) , then (1.1) changes into a deterministic autonomous plate equation. The existence and uniqueness of the global attractor of the corresponding dynamical system were investigated in [1,2,3, 4,5,6, 7,8,9, 10,11]; besides, the uniform attractor of the dynamical system generated by the non-autonomous plate equation was obtained in [12].

For the stochastic case, if μ = 0 and the forcing term g ( x , t ) = g ( x ) , then the existence of a random attractor of (1.1)–(1.2) in bounded domain has been established in [13,14, 15,16]; if μ 0 , the existence of random attractors for plate equations with memory and additive noise in bounded domain was considered in [17,18]. Recently, in the unbounded domain, the authors investigated the asymptotic behavior for stochastic plate equation driven by different noises (see [19,20, 21,22] for details).

However, studies on the stochastic plate equation with memory still lack. Motivated by the literature above, we investigate the asymptotic behaviors for stochastic plate equation driven by multiplicative noise in unbounded domains in this paper. More precisely, compared to [19,20, 21,22], we have the memory effects. The main features of our work are summarized as follows.

  1. Note that Sobolev embeddings are no longer compact in unbounded domains. It leads to a major difficulty for us to prove the asymptotic compactness of solutions by standard method. To overcome this difficulty, we refer to [23,24] which provide uniform estimates on the far-field values of solutions.

  2. There is no applicable compact embedding property in the “history” space. In this case, we solve it with the help of a useful result in [25]. For our purpose, we introduce a new variable and an extended Hilbert space. Moreover, we still need uniform estimates of solutions in higher regular space due to the memory term.

  3. The influence of multiplicative noise and additive noise on the solutions of plate equations is quite different. When dealing with random attractors of a stochastic equation, we often transform the stochastic equation into a deterministic one with random parameters. If the equation is driven by additive noise, then the transformation does not change the structure of the original equation. Therefore, one can obtain all necessary uniform estimates of solutions, and then get the existence of random attractors for additive noise with any intensity (see, e.g., [20]). However, if the plate equation is driven by multiplicative noise, then there are several additional terms appearing after the equation is transformed (see ( 3.12 ) 2 in Section 3). These additional terms involve the unknown variable u and have great effect on the way to derive uniform estimates of solutions. This is the reason why, in this paper, we only study the existence of random attractors for the stochastic equation (1.1) when the intensity ε of the multiplicative noise is sufficiently small.

  4. In this manuscript, φ 0 E , so we cannot obtain the higher order estimate by using the classical energy method. To this end, we split the system into a linear system and a zero initial data nonlinear system. The energy of the linear system decays to 0, while the energy of nonlinear system is bounded in higher regular space. Then we can use this property to deduce the compactness.

In the next section, we recall some notations and results regarding random attractors for non-autonomous stochastic equations. We then define a continuous cocycle for equation (1.1) and derive necessary uniform estimates in Sections 3 and 4, respectively. Finally, we prove the existence of random attractors in Section 5.

Throughout the paper, the letters c and c i ( i = 1 , 2 , ) are generic positive constants which do not depend on ε .

2 Preliminaries

In this section, we present some definitions and known results regarding pullback attractors of non-autonomous random dynamical systems from [26,27].

Definition 2.1

Let θ : R × Ω Ω be a ( ( R ) × , ) -measurable mapping. We say ( Ω , , P , θ ) is a parametric dynamical system if θ ( 0 , ) is the identity on Ω , θ ( s + t , ) = θ ( t , ) θ ( s , ) for all t , s R , and P θ ( t , ) = P for all t R .

Definition 2.2

Let K : R × Ω 2 X be a set-valued mapping with closed nonempty images. We say K is measurable with respect to in Ω if the mapping ω Ω d ( x , K ( τ , ω ) ) is ( , ( R ) ) -measurable for every fixed x X and τ R .

Definition 2.3

A mapping Φ : R + × R × Ω × X X is called a continuous cocycle on X over R and ( Ω , , P , { θ t } t R ) if for all τ R , ω Ω , and t , s R + , the following conditions (1)–(4) are satisfied:

  1. Φ ( , τ , , ) : R + × Ω × X X is ( ( R + ) × × ( X ) , ( X ) ) -measurable;

  2. Φ ( 0 , τ , ω , ) is the identity on X ;

  3. Φ ( t + s , τ , ω , ) = Φ ( t , τ + s , θ s ω , ) Φ ( s , τ , ω , ) ;

  4. Φ ( t , τ , ω , ) : X X is continuous.

Hereafter, we assume Φ is a continuous cocycle on X over R and ( Ω , , P , { θ t } t R ) , and D is the collection of some families of nonempty bounded subsets of X parameterized by τ R and ω Ω :

D = { D = { D ( τ , ω ) X : D ( τ , ω ) , τ R , ω Ω } } .

Definition 2.4

Let B = { B ( τ , ω ) : τ R , ω Ω } be a family of nonempty subsets of X . For every τ R , ω Ω , let

Ω ( B , τ , ω ) = r 0 t r Φ ( t , τ t , θ t ω , B ( τ t , θ t ω ) ) ¯ .

Then the family { Ω ( B , τ , ω ) : τ R , ω Ω } is called the Ω -limit set of B and is denoted by Ω ( B ) .

Definition 2.5

Let D be a collection of some families of nonempty subsets of X and K = { K ( τ , ω ) : τ R , ω Ω } D . Then K is called a D -pullback absorbing set for Φ if for all τ R and ω Ω and for every B D , there exists T = T ( B , τ , ω ) > 0 such that

Φ ( t , τ t , θ t ω , B ( τ t , θ t ω ) ) K ( τ , ω ) for all t T .

If, in addition, K ( τ , ω ) is closed in X and is measurable in ω with respect to , then K is called a closed measurable D -pullback absorbing set for Φ .

Definition 2.6

Let D be a collection of some families of nonempty subsets of X . Then Φ is said to be D -pullback asymptotically compact in X if for all τ R and ω Ω , the sequence

{ Φ ( t n , τ t n , θ t n ω , x n ) } n = 1 has a convergent subsequence in X

whenever t n , and x n B ( τ t n , θ t n ω ) with { B ( τ , ω ) : τ R , ω Ω } D .

Definition 2.7

Let D be a collection of some families of nonempty subsets of X and A = { A ( τ , ω ) : τ R , ω Ω } D . Then A is called a D -pullback attractor for Φ if the following conditions (1)–(3) are fulfilled: for all t R + , τ R and ω Ω ,

  1. A ( τ , ω ) is compact in X and is measurable in ω with respect to ;

  2. A is invariant, that is,

    Φ ( t , τ , ω , A ( τ , ω ) ) = A ( τ + t , θ t ω ) ;

  3. For every B = { B ( τ , ω ) : τ R , ω Ω } D ,

    lim t d ( Φ ( t , τ t , θ t ω , B ( τ t , θ t ω ) ) , A ( τ , ω ) ) = 0 .

Proposition 2.8

Let D be an inclusion-closed collection of some families of nonempty subsets of X , and Φ be a continuous cocycle on X over R and ( Ω , , P , { θ t } t R ) . If Φ is D -pullback asymptotically compact in X and Φ has a closed measurable D -pullback absorbing set K in D , then Φ has a unique D -pullback attractor A in D which is given by, for each τ R and ω Ω ,

A ( τ , ω ) = Ω ( K , τ , ω ) = D D Ω ( B , τ , ω ) .

3 Cocycles for stochastic plate equation

In this section, we outline some basic settings about (1.1)–(1.2) and show that it generates a continuous cocycle in E = H 2 × L 2 × R μ , 2 .

Let Δ denote the Laplace operator in R n , A = Δ 2 and D ( A ) = H 4 ( R n ) . We can define the powers A r of A for r R . The space V r = D A r 4 is a Hilbert space with the following inner product and norm:

( u , v ) r = A r 4 u , A r 4 v , r = A r 4 u , u , v V r .

In particular, V 0 = L 2 ( R n ) , V 1 = H 1 ( R n ) , V 2 = H 2 ( R n ) .

For brevity, the notation ( , ) for L 2 -inner product will also be used for the notation of duality pairing between dual spaces.

Following Dafermos [28], we introduce a Hilbert “history” space R μ , 2 = L μ 2 ( R + , V 2 ) with the inner product

( η 1 , η 2 ) μ , 2 = 0 μ ( s ) ( Δ η 1 ( s ) , Δ η 2 ( s ) ) d s , η 1 , η 2 R μ , 2 ,

and new variables

η ( x , t , s ) = u ( x , t ) u ( x , t s ) , ( x , s ) R n × R + , t 0 .

By differentiation we have

η t ( x , t , s ) = η s ( x , t , s ) + u t ( x , t ) , ( x , s ) R n × R + , t 0 .

Denote E = H 2 × L 2 × R μ , 2 , with the Sobolev norm

(3.1) y H 2 × L 2 × R μ , 2 = ( v 2 + u 2 + Δ u 2 + η μ , 2 ) 1 2 , for y = ( u , v , η ) E .

Let ξ = u t + δ u , where δ is a small positive constant whose value will be determined later. Substituting u t = ξ δ u into (1.1) we find

(3.2) d u d t + δ u = ξ , d ξ d t δ ξ + ( λ + δ 2 + A ) u + h ( ξ δ u ) + 0 μ ( s ) A η ( s ) d s + f ( x , u ) = g ( x , t ) + ε u d w d t , η t + η s = u t ,

with the initial value conditions

(3.3) u ( x , τ ) = u 0 ( x ) , ξ ( x , τ ) = ξ 0 ( x ) , η ( x , τ , s ) = η 0 ( x , s ) = u ( x , τ ) u ( x , τ s ) ,

where ξ 0 ( x ) = u 1 ( x ) + δ u 0 ( x ) , x R n , s R + .

Assumption I

Assume that the memory kernel function μ C 1 ( R + ) L 1 ( R + ) , nonlinear functions h C 1 ( R ) and f C 1 ( R ) satisfy the following conditions:

  1. s R + and some ϖ > 0 .

    (3.4) μ ( s ) 0 , μ ( s ) + ϖ μ 0 ,

    note that (3.4) implies m 0 = def μ L 1 ( R + ) = 0 μ ( s ) d s > 0 .

  2. Let F ( x , u ) = 0 u f ( x , s ) d s for x R n and u R , there exist positive constants c i ( i = 1 , 2 , 3 , 4 ), such that

    (3.5) f ( x , u ) c 1 u p + ϕ 1 ( x ) , ϕ 1 L 2 ( R n ) ,

    (3.6) f ( x , u ) u c 2 F ( x , u ) ϕ 2 ( x ) , ϕ 2 L 1 ( R n ) ,

    (3.7) F ( x , u ) c 3 u p + 1 ϕ 3 ( x ) , ϕ 3 L 1 ( R n ) ,

    (3.8) f u ( x , u ) β , f x ( x , u ) ϕ 4 ( x ) , ϕ 4 L 2 ( R n ) ,

    where β > 0 , 1 p n + 4 n 4 . Note that (3.5) and (3.6) imply

    (3.9) F ( x , u ) c ( u 2 + u p + 1 + ϕ 1 2 + ϕ 2 ) .

  3. There exist two constants β 1 , β 2 such that

    (3.10) h ( 0 ) = 0 , 0 < β 1 h ( v ) β 2 < .

By (3.4), the space R μ , r = L μ 2 ( R + , V r ) ( r R ) is a Hilbert space of V r -valued functions on R + with the inner product and norm:

( η 1 , η 2 ) μ , r = 0 μ ( s ) A r 4 η 1 ( s ) , A r 4 η 2 ( s ) d s , η μ , r 2 = 0 μ ( s ) A r 4 η ( s ) , A r 4 η ( s ) d s , η , η 1 , η 2 V r ,

and on R μ , r , the linear operator s has domain

D ( s ) = { η H μ 1 ( R + , V r ) : η ( 0 ) = 0 } , where H μ 1 ( R + , V r ) = { η : η ( s ) , s η L μ 2 ( R + , V r ) } .

To study the dynamical behavior of problem (3.2), we need to convert problem (3.2) into a deterministic system with a random parameter. We now introduce an Ornstein-Uhlenbeck process given by the Brownian motion. Put

(3.11) z ( θ t ω ) = z ( t , ω ) = δ 0 e δ s ( θ t ω ) ( s ) d s ,

which is called the Ornstein-Uhlenbeck process and solves the Itô equation d z + δ z d t = d ω , z ( ) = 0 .

From [30], it is known that the random variable z ( ω ) is a stationary, ergodic, and tempered stochastic process, and there is a θ t -invariant set Ω ˜ Ω of full P measure such that z ( θ t ω ) is continuous in t for every ω Ω ˜ . For convenience, we shall simply write Ω ˜ as Ω .

To show that problem (3.2) generates a cocycle, we let

v ( x , t ) = ξ ( x , t ) ε u ( x , t ) z ( θ t ω ) ,

then (3.2) can be rewritten as the equivalent system with random coefficients but without multiplicative noise

(3.12) d u d t + δ u v = ε u z ( θ t ω ) , d v d t δ v + ( λ + δ 2 + A ) u + 0 μ ( s ) A η ( s ) d s + f ( x , u ) = g ( x , t ) h ( v + ε u z ( θ t ω ) δ u ) ε ( v 3 δ u + ε u z ( θ t ω ) ) z ( θ t ω ) , η t + η s = u t ,

with the initial value conditions

(3.13) u ( x , τ ) = u 0 ( x ) , v ( x , τ ) = v 0 ( x ) , η ( x , τ , s ) = η 0 ( x , s ) = u ( x , τ ) u ( x , τ s ) ,

where v 0 ( x ) = ξ 0 ( x ) ε u 0 ( x ) z ( θ t ω ) , x R n , s R + .

The well-posedness of the deterministic problems (3.12)–(3.13) in H 2 × L 2 × R μ , 2 can be established by standard methods as in [29,30,31], more precisely, under conditions (3.4)–(3.8) and (3.10), for every ω Ω , τ R and ( u 0 , v 0 , η 0 ) E , we can obtain the following lemma:

Lemma 3.1

Put φ ( t + τ , τ , θ τ ω , φ 0 ) = ( u ( t + τ , τ , θ τ ω , u 0 ) , v ( t + τ , τ , θ τ ω , v 0 ) , η ( t + τ , τ , θ τ ω , η 0 , s ) ) , where φ 0 = ( u 0 , v 0 , η 0 ) , and let conditions (3.4)–(3.8) and (3.10) hold. Then for every ω Ω , τ R and φ 0 E ( R n ) , problem (3.12)–(3.13) has a unique ( , ( H 2 ( R n ) ) × ( L 2 ( R n ) ) × ( R μ , 2 ) ) -measurable solution φ ( , τ , ω , φ 0 ) C ( [ τ , ) , E ( R n ) ) with φ ( τ , τ , ω , φ 0 ) = φ 0 , φ ( t , τ , ω , φ 0 ) E ( R n ) being continuous in φ 0 with respect to the usual norm of E ( R n ) for each t > τ . Moreover, for every ( t , τ , ω , φ 0 ) R + × R × Ω × E ( R n ) , the mapping

(3.14) Φ ( t , τ , ω , φ 0 ) = φ ( t + τ , τ , θ τ ω , φ 0 )

generates a continuous cocycle from R + × R × Ω × E ( R n ) to E ( R n ) over R and ( Ω , , P , { θ t } t R ) .

Introducing the homeomorphism P ( θ t ω ) ( u , v , η ) = ( u , v + z ( θ t ω ) , η ) , ( u , v , η ) E ( R n ) with an inverse homeomorphism P 1 ( θ t ω ) ( u , v , η ) = ( u , v z ( θ t ω ) , η ) . Then, the transformation

(3.15) Φ ˜ ( t , τ , ω , ( u 0 , ξ 0 , η 0 ) ) = P ( θ t ω ) Φ ( t , τ , ω , ( u 0 , v 0 , η 0 ) ) P 1 ( θ t ω )

generates a continuous cocycle with (3.2)–(3.3) over R and ( Ω , , P , { θ t } t R ) .

Note that these two continuous cocycles are equivalent. By (3.15), it is easy to check that Φ ˜ has a random attractor provided Φ possesses a random attractor. Then, we only need to consider the continuous cocycle Φ .

Assumption II

We assume that σ , δ , ε , and g ( x , t ) satisfy the following conditions:

(3.16) σ = 1 2 min δ , δ 1 2 m 0 δ ϖ , ϖ 4 , δ c 2 ,

(3.17) δ > 0 satisfies λ + δ 2 β 2 δ > 0 , β 1 > 5 δ + β 2 δ ( λ + δ 2 β 2 δ ) ,

(3.18) ε < min 4 δ ( γ 2 γ 3 + γ 1 ) ϖ + 2 4 δ ( γ 2 γ 3 + γ 1 ) 2 ϖ 2 + π δ ϖ ( 2 σ γ 2 ϖ + 8 σ γ 2 m 0 ) ( 2 ϖ + 8 m 0 ) γ 2 π , 4 δ ( γ 2 γ 3 + 1 ) ϖ + 2 4 δ ( γ 2 γ 3 + 1 ) 2 ϖ 2 + π δ ϖ ( 2 σ γ 2 ϖ + 8 σ γ 2 m 0 ) ( 2 ϖ + 8 m 0 ) γ 2 π ,

where γ 1 = max 1 , c 1 c 3 1 2 , γ 2 = 1 + 1 λ + δ 2 β 2 δ , γ 3 = 3 2 δ + 1 2 β 2 + ( β 2 β 1 ) δ + 1 . Moreover,

(3.19) 0 e σ s g ( , τ + s ) 1 2 d s < , τ R ,

and

(3.20) lim k 0 e σ s x k g ( x , τ + s ) 2 d x d s = 0 , τ R ,

where denotes the absolute value of real number in R .

Given a bounded nonempty subset B of E , we write B = sup ϕ B ϕ E . Let D = { D ( τ , ω ) : τ R , ω Ω } be a family of bounded nonempty subsets of E such that for every τ R , ω Ω ,

(3.21) lim s e σ s D ( τ + s , θ s ω ) E 2 = 0 .

Let D be the collection of all such families, that is,

(3.22) D = { D = { D ( τ , ω ) : τ R , ω Ω } : D satisfies ( 3.21 ) } .

4 Uniform estimates of solutions

In this section, we derive a series of uniform estimates for solutions of problems (3.12)–(3.13).

We define a new norm E by

(4.1) Y E = ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η μ , 2 ) 1 2 , for Y = ( u , v , η ) E .

It is easy to check that E is equivalent to the usual norm H 2 × L 2 × R μ , 2 in (3.1).

First we show that the cocycle Φ has a pullback D -absorbing set in D .

Lemma 4.1

Under Assumptions I and II, for every τ R , ω Ω , D = { D ( τ , ω ) : τ R , ω Ω } D , there exists T = T ( τ , ω , D ) > 0 such that for all t T the solution of problem (3.12)–(3.13) satisfies

φ ( τ , τ t , θ τ ω , φ 0 ) E 2 R ( τ , ω ) ,

and R ( τ , ω ) is given by

(4.2) R ( τ , ω ) = M 0 e 2 0 s σ γ 1 ε z ( θ r ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ r ω ) 2 + γ 3 ε z ( θ t ω ) d r ( g ( , s + τ ) 2 + ε z ( θ s ω ) ) d s ,

where M is a positive constant independent of τ , ω , D , and ε .

Proof

Taking the inner product of ( 3.12 ) 2 with v in L 2 ( R n ) , we get

(4.3) 1 2 d d t v 2 ( δ ε z ( θ t ω ) ) v 2 + ( λ + δ 2 ) ( u , v ) + ( A u , v ) + 0 μ ( s ) ( A η ( s ) , v ) d s + ( f ( x , u ) , v ) = ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) ( u , v ) ( h ( v + ε u z ( θ t ω ) δ u ) , v ) + ( g ( x , t ) , v ) .

By ( 3.12 ) 1 , we have

(4.4) v = u t ε u z ( θ t ω ) + δ u .

It follows from (3.10) and Lagrange’s mean value theorem that

(4.5) ( h ( v + ε u z ( θ t ω ) δ u ) , v ) = ( h ( v + ε u z ( θ t ω ) δ u ) h ( 0 ) , v ) = ( h ( ϑ ) ( v + ε u z ( θ t ω ) δ u ) , v ) β 1 v 2 ( h ( ϑ ) ( ε u z ( θ t ω ) δ u ) , v ) β 1 v 2 + β 2 ε z ( θ t ω ) u v + h ( ϑ ) δ ( u , v ) ,

where ϑ is between 0 and v + ε u z ( θ t ω ) δ u .

By (3.10) and (4.4), we know

(4.6) h ( ϑ ) δ ( u , v ) = h ( ϑ ) δ ( u , u t ε u z ( θ t ω ) + δ u ) β 2 δ 1 2 d d t u 2 + β 2 δ 2 u 2 β 1 δ ε z ( θ t ω ) u 2 .

Substituting (4.4) into the third and fourth terms on the left-hand side of (4.3), we find that

(4.7) ( u , v ) = ( u , u t ε u z ( θ t ω ) + δ u ) 1 2 d d t u 2 + δ u 2 ε z ( θ t ω ) u 2

and

(4.8) ( A u , v ) = ( Δ u , Δ v ) = ( Δ u , Δ u t ε z ( θ t ω ) Δ u + δ Δ u ) 1 2 d d t Δ u 2 + δ Δ u 2 ε z ( θ t ω ) Δ u 2 .

Using the Cauchy-Schwarz inequality and Young’s inequality, we have

(4.9) ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) ( u , v ) + β 2 ε z ( θ t ω ) u v = ( 3 δ ε z ( θ t ω ) ε 2 z 2 ( θ t ω ) ) ( u , v ) + β 2 ε z ( θ t ω ) u v ( 3 δ ε z ( θ t ω ) + ε 2 z ( θ t ω ) 2 ) u v + β 2 ε z ( θ t ω ) u v = ( ( 3 δ + β 2 ) ε z ( θ t ω ) + ε 2 z ( θ t ω ) 2 ) u v 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 z ( θ t ω ) 2 ( u 2 + v 2 ) ,

(4.10) ( g , v ) g v g 2 2 ( β 1 δ ) + β 1 δ 2 v 2 .

Let F ˜ ( x , u ) = R n F ( x , u ) d x . Then for the last term on the left-hand side of (4.3) we have

(4.11) ( f ( x , u ) , v ) = ( f ( x , u ) , u t ε z ( θ t ω ) u + δ u ) = d d t F ˜ ( x , u ) + δ ( f ( x , u ) , u ) ε z ( θ t ω ) ( f ( x , u ) , u ) .

From (3.5) and (3.7), we obtain

(4.12) ε z ( θ t ω ) ( f ( x , u ) , u ) c 1 ε z ( θ t ω ) R n u γ + 1 d x + ε z ( θ t ω ) ϕ 1 2 + ε z ( θ t ω ) u 2 c 1 c 3 1 ε z ( θ t ω ) R n ( F ( x , u ) + ϕ 3 ) d x + ε z ( θ t ω ) ϕ 1 2 + ε z ( θ t ω ) u 2 c 1 c 3 1 ε z ( θ t ω ) F ˜ ( x , u ) + c ε z ( θ t ω ) + ε z ( θ t ω ) u 2 .

A direct calculation deduces that

(4.13) 0 μ ( s ) ( A η ( s ) , v ) d s = 0 μ ( s ) ( Δ 2 η ( s ) , v ) d s = 0 μ ( s ) ( Δ η ( s ) , Δ ( u t ε u z ( θ t ω ) + δ u ) ) d s = 0 μ ( s ) ( Δ η ( s ) , Δ u t ) d s ε z ( θ t ω ) 0 μ ( s ) ( Δ η ( s ) , Δ u ) d s + δ 0 μ ( s ) ( Δ η ( s ) , Δ u ) d s .

Using ( 3.12 ) 3 , then integrating by parts with respect to s , we get

(4.14) 0 μ ( s ) ( Δ η ( s ) , Δ u t ) d s 1 2 d d t η μ , 2 2 + ϖ 2 η μ , 2 2 .

Using Young’s inequality, we have

(4.15) ε z ( θ t ω ) 0 μ ( s ) ( Δ η ( s ) , Δ u ) d s ϖ 8 η μ , 2 2 2 m 0 ε 2 ϖ z ( θ t ω ) 2 Δ u 2

and

(4.16) δ 0 μ ( s ) ( Δ η ( s ) , Δ u ) d s ϖ 8 η μ , 2 2 2 m 0 δ 2 ϖ Δ u 2 .

Combining with (4.14)–(4.16) and (4.13), we get

(4.17) 0 μ ( s ) ( A η ( s ) , v ) d s 1 2 d d t η μ , 2 2 + ϖ 4 η μ , 2 2 2 m 0 ε 2 ϖ z ( θ t ω ) 2 Δ u 2 2 m 0 δ 2 ϖ Δ u 2 .

Substitute (4.5)–(4.17) into (4.3) and together with (3.6) to obtain

(4.18) 1 2 d d t ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η μ , 2 2 + 2 F ˜ ( x , u ) ) + δ ( v 2 + ( λ + δ 2 β 2 δ ) u 2 ) + δ 1 2 m 0 δ ϖ Δ u 2 + ϖ 4 η μ , 2 2 + δ c 2 F ˜ ( x , u ) 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 z ( θ t ω ) 2 ( u 2 + v 2 ) + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 Δ u 2 + ε z ( θ t ω ) ( v 2 + ( λ + δ 2 β 1 δ ) u 2 + Δ u 2 ) + ε z ( θ t ω ) u 2 + 3 δ β 1 2 v 2 + g 2 2 ( β 1 δ ) + c 1 c 3 1 ε z ( θ t ω ) F ˜ ( x , u ) + c ε z ( θ t ω ) 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 ( u 2 + v 2 + Δ u 2 ) + γ 1 ε z ( θ t ω ) ( v 2 + ( λ + δ 2 β 1 δ ) u 2 + Δ u 2 + 2 F ˜ ( x , u ) ) + ε z ( θ t ω ) u 2 + c ( g 2 + ε z ( θ t ω ) ) ,

where γ 1 = max 1 , c 1 c 3 1 2 .

Choosing δ small enough such that 1 2 m 0 δ ϖ > 0 , then let σ = 1 2 min δ , δ 1 2 m 0 δ ϖ , ϖ 4 , δ c 2 , we get

(4.19) 1 2 d d t ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η μ , 2 2 + 2 F ˜ ( x , u ) ) σ γ 1 ε z ( θ t ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 + γ 3 ε z ( θ t ω ) × ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η μ , 2 2 + 2 F ˜ ( x , u ) ) + c ( g 2 + ε z ( θ t ω ) ) ,

where γ 2 = 1 + 1 λ + δ 2 β 2 δ , γ 3 = 3 2 δ + 1 2 β 2 + ( β 2 β 1 ) δ + 1 .

Denote

(4.20) ϱ ( τ , ω ) = σ γ 1 ε z ( θ t ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 + γ 3 ε z ( θ t ω ) .

Using the Gronwall inequality to integrate (4.19) over ( τ t , τ ) with t 0 , we get

(4.21) v ( τ , τ t , ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , ω , u 0 ) 2 + Δ u ( τ , τ t , ω , u 0 ) 2 + η ( τ , τ t , ω , η 0 , s ) μ , 2 2 + 2 F ˜ ( x , u ( τ , τ t , ω , u 0 ) ) ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 τ τ t ϱ ( s , ω ) d s + c τ t τ e 2 τ s ϱ ( r , ω ) d r ( g ( , s ) 2 + ε z ( θ s ω ) ) d s .

Replacing ω by θ τ ω in the above we obtain, for every t R + , τ R , and ω Ω ,

(4.22) v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , θ τ ω , u 0 ) 2 + Δ u ( τ , τ t , θ τ ω , u 0 ) 2 + η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 + 2 F ˜ ( x , u ( τ , τ t , θ τ ω , u 0 ) ) ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 τ τ t ϱ ( s τ , ω ) d s + c τ t τ e 2 τ s ϱ ( r τ , ω ) d r ( g ( , s ) 2 + ε z ( θ s τ ω ) ) d s ,

then

(4.23) v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , θ τ ω , u 0 ) 2 + Δ u ( τ , τ t , θ τ ω , u 0 ) 2 + η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 + 2 F ˜ ( x , u ( τ , τ t , θ τ ω , u 0 ) ) ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 0 t ϱ ( s , ω ) d s + c t 0 e 2 0 s ϱ ( r , ω ) d r ( g ( , s + τ ) 2 + ε z ( θ s ω ) ) d s .

Since z ( θ t ω ) is stationary and ergodic, from (3.11) and the ergodic theorem we can get

(4.24) lim t 1 t t 0 z ( θ r ω ) d r = E ( z ( θ r ω ) ) = 1 π δ ,

(4.25) lim t 1 t t 0 z ( θ r ω ) 2 d r = E ( z ( θ r ω ) 2 ) = 1 2 δ .

By (4.24)–(4.25), there exists T 1 ( ω ) > 0 such that for all t T 1 ( ω ) ,

(4.26) t 0 z ( θ r ω ) d r < 2 π δ t , t 0 z ( θ r ω ) 2 d r < 1 δ t .

Next we show that for any s T 1

(4.27) e 2 0 s ϱ ( r , ω ) d r e σ s .

By using the two inequalities in (4.26), we have

(4.28) 0 s σ γ 1 ε z ( θ r ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ r ω ) 2 + γ 3 ε z ( θ r ω ) d r > σ s ε 2 γ 1 π δ s γ 2 1 2 ε 2 + 2 m 0 δ 2 ϖ 1 δ + γ 3 ε 2 π δ s = γ 2 δ 1 2 ε 2 + 2 m 0 ε 2 ϖ s 2 π δ [ γ 3 γ 2 + γ 1 ] ε s + σ s .

In order to have the inequality in (4.27) valid, we need

0 s σ γ 1 ε z ( θ r ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ r ω ) 2 + γ 3 ε z ( θ r ω ) d r σ 2 s .

Since s T 1 , then it requires that

γ 2 δ 1 2 ε 2 + 2 m 0 ε 2 ϖ + 2 π δ [ γ 3 γ 2 + γ 1 ] ε σ 2 < 0 .

Solving this quadratic inequality, ε needs to satisfy (3.18) as we have assumed in Assumption II.

Since z ( θ t ω ) is tempered, by (3.19) and (4.27), we see that the following integral is convergent:

(4.29) R 1 2 ( τ , ω ) = c 0 e 2 0 s ϱ ( r , ω ) d r ( g ( , s + τ ) 2 + ε z ( θ s ω ) ) d s .

Note that (3.9) implies

(4.30) R n F ( x , u 0 ) d x c ( 1 + u 0 2 + u 0 H 2 p + 1 ) .

Since D D and ( u 0 , v 0 , η 0 ) D ( τ t , θ t ω ) , for all t T 1 , we get from (4.29) and (4.30) that

(4.31) ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 0 t ϱ ( s , ω ) d s c e σ t ( 1 + v 0 2 + u 0 H 2 2 + u 0 H 2 p + 1 + η 0 μ , 2 2 ) c e σ t ( 1 + D ( τ t , θ t ω ) 2 + D ( τ t , θ t ω ) p + 1 ) 0 , as t + .

From (4.1), (4.23), (4.29), and (4.31), there exists T 2 = T 2 ( τ , ω , D ) T 1 such that for all t T 2 ,

φ ( τ , τ t , θ τ ω , φ 0 ) E 2 c R 1 2 ( τ , ω ) ,

thus the proof is completed.□

The following lemma will be used to show the uniform estimates of solutions as well as to establish pullback asymptotic compactness.

Lemma 4.2

Under Assumptions I and II, for every τ R , ω Ω , D = { D ( τ , ω ) : τ R , ω Ω } D , there exists T = T ( τ , ω , D ) > 0 such that for all t T , s [ t , 0 ] , the solution of problem (3.12)–(3.13) satisfies

φ ( τ + s , τ t , θ τ ω , φ 0 ) E 2 R ( τ , ω ) e 2 s 0 ϱ ( r , ω ) d r ,

where ( u 0 , v 0 , η 0 ) D ( τ t , θ t ω ) , M is a positive constant independent of τ , ω , D , and ε , and R ( τ , ω ) is a specific random variable.

Proof

Similar to (4.23), integrating (4.19) over ( τ t , τ + s ) with t 0 and s [ t , 0 ] , we get

(4.32) v ( τ + s , τ t , ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ + s , τ t , ω , u 0 ) 2 + Δ u ( τ + s , τ t , ω , u 0 ) 2 + η ( τ + s , τ t , ω , η 0 , s ) μ , 2 2 + 2 F ˜ ( x , u ( τ + s , τ t , ω , u 0 ) ) ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 τ + s τ t ϱ ( r t , ω ) d r + c τ t τ + s e 2 τ + s ζ ϱ ( r τ , ω ) d r ( g ( , ζ ) 2 + ε z ( θ ζ τ ω ) ) d ζ ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 s t ϱ ( r , ω ) d r + c t s e 2 s ζ ϱ ( r , ω ) d r ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ .

For the last integral term on the right-hand side of (4.32), we have

(4.33) c t s e 2 s ζ ϱ ( r t , ω ) d r ( 1 + g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ = c t T 1 e 2 s ζ ϱ ( r , ω ) d r + T 1 s e 2 s ζ ϱ ( r , ω ) d r ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ c e 2 s 0 ϱ ( r , ω ) d r t T 1 e 2 0 ζ ϱ ( r , ω ) d r ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ

+ c e 2 s 0 ϱ ( r , ω ) d r T 1 0 e 2 0 ζ ϱ ( r , ω ) d r ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ c e 2 s 0 ϱ ( r , ω ) d r t T 1 e σ ζ ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ + c e 2 s 0 ϱ ( r , ω ) d r T 1 0 e 2 0 ζ ϱ ( r , ω ) d r ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ e 2 s 0 ϱ ( r , ω ) d r R 2 ( ε , τ , ω ) ,

where

R 2 ( τ , ω ) = c 0 e σ ζ ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ + c T 1 0 e 2 0 ζ ϱ ( r , ω ) d r ( g ( , ζ + τ ) 2 + ε z ( θ ζ ω ) ) d ζ .

As in (4.31), we find that there exists T 3 = T 3 ( τ , ω , D ) T 1 such that for all t T 3 ,

(4.34) ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 s t ϱ ( r , ω ) d r c e 2 s 0 ϱ ( r , ω ) d r e 2 0 t ϱ ( r , ω ) d r ( v 0 2 + ( λ + δ 2 β 2 δ ) u 0 2 + Δ u 0 2 + η 0 μ , 2 2 + 2 F ˜ ( x , u 0 ) ) e 2 s 0 ϱ ( r , ω ) d r R 2 ( τ , ω ) .

It follows from (4.32)–(4.34) and (4.30) that, for all t T 3 , s [ t , 0 ] , and ε satisfying (3.18),

(4.35) v ( τ + s , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ + s , τ t , θ τ ω , u 0 ) 2 + Δ u ( τ + s , τ t , θ τ ω , u 0 ) 2 + η ( τ + s , τ t , ω , η 0 , s ) μ , 2 2 2 e 2 s 0 ϱ ( r , ω ) d r R 2 ( τ , ω ) .

The proof is completed.□

Next, we will give higher order estimates for φ ( ε ) .

Lemma 4.3

Under Assumptions I and II, for every τ R , ω Ω , D = { D ( τ , ω ) : τ R , ω Ω } D , there exists T = T ( τ , ω , D ) > 0 such that for all t T the solution of problem (3.12)–(3.13) satisfies

A 1 4 φ ( τ , τ t , θ τ ω , φ 0 ) E 2 R ( τ , ω ) ,

and R ( τ , ω ) is given by

(4.36) R ( τ , ω ) = R 3 2 ( ε , τ , ω ) + c e σ t A 1 4 v 0 2 + A 1 4 u 0 2 + A 3 4 u 0 2 ,

where ( u 0 , v 0 , η 0 ) D ( τ t , θ t ω ) , c is a positive constant independent of τ , ω , D , and ε , and R 3 ( τ , ω ) is a specific random variable.

Proof

Taking the inner product of ( 3.12 ) 2 with A 1 2 v in L 2 ( R n ) , we find that

(4.37) 1 2 d d t A 1 4 v 2 ( δ ε z ( θ t ω ) ) A 1 4 v 2 + ( λ + δ 2 ) u , A 1 2 v + A u , A 1 2 v + 0 μ ( s ) A η ( s ) , A 1 2 v d s + ( f ( x , u ) , A 1 2 v ) = ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) u , A 1 2 v ( h ( v + ε u z ( θ t ω ) δ u ) , A 1 2 v ) + g ( x , t ) , A 1 2 v .

Similar to the proof of Lemma 4.1, we have the following estimates:

(4.38) h ( v + ε u z ( θ t ω ) δ u ) , A 1 2 v = h ( v + ε u z ( θ t ω ) δ u ) h ( 0 ) , A 1 2 v = h ( ϑ ) ( v + ε u z ( θ t ω ) δ u ) , A 1 2 v β 1 A 1 4 v 2 h ( ϑ ) ( ε u z ( θ t ω ) δ u ) , A 1 2 v β 1 A 1 4 v 2 + β 2 ε z ( θ t ω ) A 1 4 u A 1 4 v + h ( ϑ ) δ u , A 1 2 v ,

(4.39) h ( ϑ ) δ u , A 1 2 v = h ( ϑ ) δ u , A 1 2 u t ε z ( θ t ω ) A 1 2 u + δ A 1 2 u β 2 δ 1 2 d d t A 1 4 u 2 + β 2 δ 2 A 1 4 u 2 β 1 δ ε z ( θ t ω ) A 1 4 u 2 ,

(4.40) u , A 1 2 v = u , A 1 2 u t ε z ( θ t ω ) A 1 2 u + δ A 1 2 u 1 2 d d t A 1 4 u 2 + δ A 1 4 u 2 ε z ( θ t ω ) A 1 4 u 2 ,

(4.41) ( A u , A 1 2 v ) = A u , A 1 2 u t ε z ( θ t ω ) A 1 2 u + δ A 1 2 u 1 2 d d t A 3 4 u 2 + δ A 3 4 u 2 ε z ( θ t ω ) A 3 4 u 2 ,

(4.42) ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) u , A 1 2 v + β 2 ε z ( θ t ω ) A 1 4 u A 1 4 v = ( 3 δ ε z ( θ t ω ) ε 2 z 2 ( θ t ω ) ) u , A 1 2 v + β 2 ε z ( θ t ω ) A 1 4 u A 1 4 v ( 3 δ ε z ( θ t ω ) + ε 2 z ( θ t ω ) 2 ) A 1 4 u A 1 4 v + β 2 ε z ( θ t ω ) A 1 4 u A 1 4 v = ( ( 3 δ + β 2 ) ε z ( θ t ω ) + ε 2 z ( θ t ω ) 2 ) A 1 4 u A 1 4 v 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 z ( θ t ω ) 2 A 1 4 u 2 + A 1 4 v 2 ,

(4.43) g , A 1 2 v g 1 A 1 4 v g 1 2 2 ( β 1 δ ) + β 1 δ 2 A 1 4 v 2 ,

(4.44) 0 μ ( s ) A η ( s ) , A 1 2 v d s 1 2 d d t A 1 4 η μ , 2 2 + ϖ 4 A 1 4 η μ , 2 2 2 m 0 ε 2 ϖ z ( θ t ω ) 2 A 3 4 u 2 2 m 0 δ 2 ϖ A 3 4 u 2 .

For the last term on the left-hand side of (4.37), by (3.8), we have

(4.45) f ( x , u ) , A 1 2 v = R n x f ( x , u ) A 1 4 v d x R n u f ( x , u ) A 1 4 u A 1 4 v d x R n x f ( x , u ) A 1 4 v d x + β R n A 1 4 u A 1 4 v d x R n η 4 A 1 4 v d x + β R n A 1 4 u A 1 4 v d x η 4 A 1 4 v + β A 1 4 u A 1 4 v c + δ + β 2 2 δ ( λ + δ 2 β 2 δ ) A 1 4 v 2 + 1 2 δ ( λ + δ 2 β 2 δ ) A 1 4 u 2 .

Substitute (4.38)–(4.45) into (4.37) and together with (3.17) to obtain

(4.46) 1 2 d d t A 1 4 v 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 2 + A 3 4 u 2 + A 1 4 η μ , 2 2 + σ A 1 4 v 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 2 + A 3 4 u 2 + A 1 4 η μ , 2 2 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 A 1 4 u 2 + A 1 4 v 2 + A 3 4 u 2 + ε z ( θ t ω ) A 1 4 v 2 + ( λ + δ 2 β 1 δ ) A 1 4 u 2 + A 3 4 u 2 + A 1 4 η μ , 2 2 + g 1 2 2 ( β 1 δ ) .

Then

(4.47) 1 2 d d t A 1 4 v 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 2 + A 3 4 u 2 + A 1 4 η μ , 2 2 σ ε z ( θ t ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 + γ 3 ε z ( θ t ω ) × A 1 4 v 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 2 + A 3 4 u 2 + A 1 4 η μ , 2 2 + g 1 2 2 ( β 1 δ ) .

Let us denote

(4.48) ϱ 1 ( τ , ω ) = σ ε z ( θ t ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 + γ 3 ε z ( θ t ω ) .

Using the Gronwall inequality to integrate (4.47) over ( τ t , τ ) with t 0 , we get

(4.49) A 1 4 v ( τ , τ t , ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) A 1 4 u ( τ , τ t , ω , u 0 ) 2 + A 3 4 u ( τ , τ t , ω , u 0 ) 2 + A 1 4 η ( τ , τ t , ω , η 0 , s ) μ , 2 2 A 1 4 v 0 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 0 2 + A 3 4 u 0 2 + A 1 4 η 0 μ , 2 2 e 2 τ τ t ϱ 1 ( s , ω ) d s + c τ t τ e 2 τ s ϱ 1 ( r , ω ) d r g ( , s ) 1 2 d s .

Replacing ω by θ τ ω in (4.49), for every t R + , τ R , and ω Ω ,

(4.50) A 1 4 v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) A 1 4 u ( τ , τ t , θ τ ω , u 0 ) 2 + A 3 4 u ( τ , τ t , θ τ ω , u 0 ) 2 + A 1 4 η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 A 1 4 v 0 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 0 2 + A 3 4 u 0 2 + A 1 4 η 0 μ , 2 2 e 2 τ τ t ϱ 1 ( s τ , ω ) d s + c τ t τ e 2 τ s ϱ 1 ( r τ , ω ) d r g ( , s ) 1 2 d s ,

then

(4.51) A 1 4 v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) A 1 4 u ( τ , τ t , θ τ ω , u 0 ) 2 + A 3 4 u ( τ , τ t , θ τ ω , u 0 ) 2 + A 1 4 η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 A 1 4 v 0 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 0 2 + A 3 4 u 0 2 + A 1 4 η 0 μ , 2 2 e 2 0 t ϱ 1 ( s , ω ) d s + c t 0 e 2 0 s ϱ 1 ( r , ω ) d r g ( , s + τ ) 1 2 d s .

Next we show that for any s T 1

(4.52) e 2 0 s ϱ 1 ( r , ω ) d r e σ s .

In fact, using the two inequalities in (4.26), we have

0 s σ ε z ( θ r ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ r ω ) 2 + γ 3 ε z ( θ r ω ) d r > σ s ε 2 π δ s γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ 1 δ + γ 3 ε 2 π δ s = γ 2 δ 1 2 ε 2 + 2 m 0 ε 2 ϖ s 2 π δ [ γ 3 γ 2 + 1 ] ε s + σ s .

In order to have the inequality in (4.52) valid, we need

0 s σ ε z ( θ r ω ) γ 2 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ r ω ) 2 + γ 3 ε z ( θ r ω ) d r σ 2 s .

Since s T 1 , then it requires that

γ 2 δ 1 2 ε 2 + 2 m 0 ε 2 ϖ + 2 π δ [ γ 3 γ 2 + 1 ] ε σ 2 < 0 .

Solving this quadratic inequality, ε needs to satisfy (3.18).

By (3.19) and (4.52), we see that the following integral is convergent:

(4.53) R 3 2 ( τ , ω ) = c 0 e 2 0 s ϱ 1 ( r , ω ) d r g ( , s + τ ) 1 2 d s .

For all t T 1 , we get from (4.52) that

(4.54) A 1 4 v 0 2 + ( λ + δ 2 β 2 δ ) A 1 4 u 0 2 + A 3 4 u 0 2 + A 1 4 η 0 μ , 2 2 e 2 0 t Γ 1 ( s , ω ) d s c e σ t A 1 4 v 0 2 + A 1 4 u 0 2 + A 3 4 u 0 2 + A 1 4 η 0 μ , 2 2 .

From (4.1), (4.51), (4.53), and (4.54), there exists T 4 = T 4 ( τ , ω , D ) T 1 such that for all t T 4 ,

(4.55) A 1 4 φ ( τ , τ t , θ τ ω , φ 0 ) E 2 R 3 2 ( τ , ω ) + c e σ t A 1 4 v 0 2 + A 1 4 u 0 2 + A 3 4 u 0 2 + A 1 4 η 0 μ , 2 2 .

Thus, the proof is completed.□

In what follows, we derive uniform estimates on the tails of solutions when x and t approach infinity. These estimates will be used to overcome the difficulty caused by non-compactness in unbounded domains and are crucial for proving the pullback asymptotic compactness of the cocycle.

Lemma 4.4

Under Assumptions I and II, for every η > 0 , τ R , ω Ω , D = { D ( τ , ω ) : τ R , ω Ω } D , there exists T = T ( τ , ω , D , η ) > 0 , K = K ( τ , ω , η ) 1 such that for all t T , k K , the solutions of problems (3.12)–(3.13) satisfy

(4.56) φ ( τ , τ t , θ τ ω , φ 0 ) E ( R n B k ) 2 η ,

where for k 1 , B k = { x R n : x k } and R n B k is the complement of B k .

Proof

Take a smooth function ρ , such that 0 ρ 1 for s R , and

(4.57) ρ ( s ) = 0 , if 0 s 1 , 1 , if s 2 ,

and there exist constants μ 1 , μ 2 , μ 3 , μ 4 such that ρ ( s ) μ 1 , ρ ( s ) μ 2 , ρ ( s ) μ 3 , ρ ( s ) μ 4 for s R . Taking the inner product of ( 3.12 ) 2 with ρ x 2 k 2 v in L 2 ( R n ) , we obtain

(4.58) 1 2 d d t R n ρ x 2 k 2 v 2 d x ( δ ε z ( θ t ω ) ) R n ρ x 2 k 2 v 2 d x + R n 0 μ ( s ) A η ( s ) ρ x 2 k 2 v d s d x + ( λ + δ 2 ) R n ρ x 2 k 2 u v d x + R n ( A u ) ρ x 2 k 2 v d x + R n ρ x 2 k 2 f ( x , u ) v d x = ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) R n ρ x 2 k 2 u v d x R n ρ x 2 k 2 ( h ( v + ε u z ( θ t ω ) δ u ) ) v d x + R n ρ x 2 k 2 g ( x , t ) v d x .

First, by (3.10), similar to (4.5), we have

(4.59) R n ρ x 2 k 2 ( h ( v + ε u z ( θ t ω ) δ u ) ) v d x = R n ρ x 2 k 2 ( h ( v + ε u z ( θ t ω ) δ u ) h ( 0 ) ) v d x β 1 R n ρ x 2 k 2 v 2 d x + h ( ϑ ) δ R n ρ x 2 k 2 u v d x + β 2 ε z ( θ t ω ) R n ρ x 2 k 2 u v d x .

Taking (4.59) into (4.58), we have

(4.60) 1 2 d d t R n ρ x 2 k 2 v 2 d x ( δ ε z ( θ t ω ) β 1 ) R n ρ x 2 k 2 v 2 d x + R n 0 μ ( s ) A η ( s ) ρ x 2 k 2 v d s d x + ( λ + δ 2 h ( ϑ ) δ ) R n ρ x 2 k 2 u v d x + R n ( A u ) ρ x 2 k 2 v d x + R n ρ x 2 k 2 f ( x , u ) v d x

ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) R n ρ x 2 k 2 u v d x + R n ρ x 2 k 2 g ( x , t ) v d x + β 2 ε z ( θ t ω ) R n ρ x 2 k 2 u v d x .

For the fourth term on the left-hand side of (4.60), we have

(4.61) ( λ + δ 2 h ( ϑ ) δ ) R n ρ x 2 k 2 u v d x = ( λ + δ 2 h ( ϑ ) δ ) R n ρ x 2 k 2 u d u d t + δ u ε u z ( θ t ω ) d x = ( λ + δ 2 h ( ϑ ) δ ) R n ρ x 2 k 2 1 2 d d t u 2 + ( δ ε z ( θ t ω ) ) u 2 d x ( λ + δ 2 β 2 δ ) 1 2 d d t R n ρ x 2 k 2 u 2 d x + δ R n ρ x 2 k 2 u 2 d x ( λ + δ 2 + β 2 δ ) ε z ( θ t ω ) R n ρ x 2 k 2 u 2 d x .

For the fifth term on the left-hand side of (4.60), we have

(4.62) R n ( A u ) ρ x 2 k 2 v d x = R n ( A u ) ρ x 2 k 2 d u d t + δ u ε u z ( θ t ω ) d x = R n ( Δ 2 u ) ρ x 2 k 2 d u d t + δ u ε z ( θ t ω ) u d x = R n ( Δ u ) Δ ρ x 2 k 2 d u d t + δ u ε z ( θ t ω ) u d x = R n ( Δ u ) 2 k 2 ρ x 2 k 2 + 4 x 2 k 4 ρ x 2 k 2 d u d t + δ u ε z ( θ t ω ) u + 2 2 x k 2 ρ x 2 k 2 d u d t + δ u ε z ( θ t ω ) u + ρ x 2 k 2 Δ d u d t + δ u ε z ( θ t ω ) u d x k < x < 2 k 2 μ 1 k 2 + 4 μ 2 x 2 k 4 ( Δ u ) v d x k < x < 2 k 4 μ 1 x k 2 ( Δ u ) ( v ) d x + 1 2 d d t R n ρ x 2 k 2 Δ u 2 d x + δ R n ρ x 2 k 2 Δ u 2 d x ε z ( θ t ω ) R n ρ x 2 k 2 Δ u 2 d x R n 2 μ 1 + 8 μ 2 k 2 ( Δ u ) v d x R n 4 2 μ 1 k ( Δ u ) ( v ) d x + 1 2 d d t R n ρ x 2 k 2 Δ u 2 d x + δ R n ρ x 2 k 2 Δ u 2 d x ε z ( θ t ω ) R n ρ x 2 k 2 Δ u 2 d x

μ 1 + 4 μ 2 k 2 ( Δ u 2 + v 2 ) 4 2 μ 1 k Δ u v + 1 2 d d t R n ρ x 2 k 2 Δ u 2 d x + δ R n ρ x 2 k 2 Δ u 2 d x ε z ( θ t ω ) R n ρ x 2 k 2 Δ u 2 d x μ 1 + 4 μ 2 k 2 ( Δ u 2 + v 2 ) 2 2 μ 1 k ( Δ u 2 + v 2 ) + 1 2 d d t R n ρ x 2 k 2 Δ u 2 d x ( ε z ( θ t ω ) δ ) R n ρ x 2 k 2 Δ u 2 d x .

For the sixth term on the left-hand side of (4.60), we have

(4.63) R n ρ x 2 k 2 f ( x , u ) v d x = R n ρ x 2 k 2 f ( x , u ) d u d t + δ u ε z ( θ t ω ) u d x = d d t R n ρ x 2 k 2 F ( x , u ) d x + δ R n ρ x 2 k 2 f ( x , u ) u d x ε z ( θ t ω ) R n ρ x 2 k 2 f ( x , u ) u d x .

By (3.6), we see that

(4.64) R n ρ x 2 k 2 f ( x , u ) u d x c 2 R n ρ x 2 k 2 F ( x , u ) d x + R n ρ x 2 k 2 ϕ 2 ( x ) d x .

On the other hand, by (3.5) and (3.7),

(4.65) ε z ( θ t ω ) R n ρ x 2 k 2 f ( x , u ) u d x c ε z ( θ t ω ) R n ρ x 2 k 2 F ( x , u ) d x + c ε z ( θ t ω ) R n ρ x 2 k 2 u 2 d x + c ε z ( θ t ω ) R n ρ x 2 k 2 ( ϕ 1 2 + ϕ 3 ) d x .

Similar to (4.9) and (4.10) in Lemma 4.1, we get

(4.66) ε z ( θ t ω ) ( 3 δ ε z ( θ t ω ) ) R n ρ x 2 k 2 u v d x + β 2 ε z ( θ t ω ) R n ρ x 2 k 2 u v d x 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 z ( θ t ω ) 2 R n ρ x 2 k 2 ( u 2 + v 2 ) d x .

(4.67) R n ρ x 2 k 2 g ( x , t ) v d x 1 2 ( β 1 δ ) R n ρ x 2 k 2 g ( x , t ) 2 d x + β 1 δ 2 R n ρ x 2 k 2 v 2 d x .

For the third term on the left-hand side of (4.60), we have

(4.68) R n 0 μ ( s ) A η ( s ) ρ x 2 k 2 v d s d x = R n 0 μ ( s ) A η ( s ) ρ x 2 k 2 d u d t + δ u ε u z ( θ t ω ) d s d x = R n 0 μ ( s ) Δ η ( s ) Δ ρ x 2 k 2 d u d t + δ u ε u z ( θ t ω ) d s d x = R n 0 μ ( s ) Δ η ( s ) 2 k 2 ρ x 2 k 2 + 4 x 2 k 4 ρ x 2 k 2 d u d t + δ u ε u z ( θ t ω ) + 2 2 x k 2 ρ x 2 k 2 d u d t + δ u ε u z ( θ t ω ) + ρ x 2 k 2 Δ d u d t + δ u ε u z ( θ t ω ) d s d x k < x < 2 k 2 μ 1 k 2 + 4 μ 2 x 2 k 4 0 μ ( s ) Δ η ( s ) v d s d x k < x < 2 k 4 μ 1 x k 2 0 μ ( s ) Δ η ( s ) v d s d x + R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u t d s d x + δ R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u d s d x ε R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u z ( θ t ω ) d s d x 2 μ 1 + 8 μ 2 k 2 R n 0 μ ( s ) Δ η ( s ) v d s d x 4 2 μ 1 k R n 0 μ ( s ) Δ η ( s ) v d s d x + R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u t d s d x + δ R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u d s d x ε R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u z ( θ t ω ) d s d x .

Using Young’s inequality, we get

(4.69) 2 μ 1 + 8 μ 2 k 2 R n 0 μ ( s ) Δ η ( s ) v d s d x μ 1 + 4 μ 2 k 2 ( η μ , 2 2 + m 0 v 2 ) ,

and

(4.70) 4 2 μ 1 k R n 0 μ ( s ) Δ η ( s ) v d s d x 2 2 μ 1 k ( η μ , 2 2 + m 0 v 2 ) .

Integrating by parts with respect to s and using (3.4), we obtain

(4.71) R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u t d s d x = R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ ( η t + η s ) d s d x 1 2 d d t R n ρ x 2 k 2 η ( s ) μ , 2 2 d x + ϖ 2 R n ρ x 2 k 2 η ( s ) μ , 2 2 d x ,

(4.72) δ R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u d s d x ϖ 8 R n ρ x 2 k 2 η ( s ) μ , 2 2 d x 2 m 0 δ 2 ϖ R n ρ x 2 k 2 Δ u 2 d x ,

(4.73) ε R n 0 μ ( s ) Δ η ( s ) ρ x 2 k 2 Δ u z ( θ t ω ) d s d x ϖ 8 R n ρ x 2 k 2 η ( s ) μ , 2 2 d x 2 m 0 ε 2 ϖ R n ρ x 2 k 2 Δ u 2 z ( θ t ω ) 2 d x .

Then it follows from (4.60)–(4.73) that

(4.74) 1 2 d d t R n ρ x 2 k 2 ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η ( s ) μ , 2 2 + 2 F ( x , u ) ) d x + δ R n ρ x 2 k 2 ( v 2 + ( λ + δ 2 β 2 δ ) u 2 ) d x + δ 1 2 m 0 δ ϖ R n ρ x 2 k 2 Δ u 2 d x + ϖ 4 R n ρ x 2 k 2 η ( s ) μ , 2 2 d x + δ c 2 R n ρ x 2 k 2 F ( x , u ) d x c ( Δ u 2 + v 2 + v 2 + η ( s ) μ , 2 2 ) + 1 2 ( 3 δ + β 2 ) ε z ( θ t ω ) + 1 2 ε 2 + 2 m 0 ε 2 ϖ z ( θ t ω ) 2 × R n ρ x 2 k 2 ( u 2 + v 2 + Δ u 2 ) d x + c R n ρ x 2 k 2 g ( x , t ) 2 d x + c ε z ( θ t ω ) R n ρ x 2 k 2 F ( x , u ) d x + c ε z ( θ t ω ) R n ρ x 2 k 2 u 2 d x + c ε z ( θ t ω ) R n ρ x 2 k 2 ( ϕ 1 2 + ϕ 3 ) d x + c R n ρ x 2 k 2 ϕ 2 ( x ) d x + ε z ( θ t ω ) R n ρ x 2 k 2 ( v 2 + ( λ + δ 2 β 1 δ ) u 2 + Δ u 2 ) d x .

Since that ϕ 1 L 2 ( R n ) , ϕ 2 , ϕ 3 L 1 ( R n ) , for given η > 0 , there exists K 0 = K 0 ( η ) 1 such that for all k K 0 ,

(4.75) c R n ρ x 2 k 2 ( ϕ 1 2 + ϕ 2 + ϕ 3 ) d x = c x k ρ x 2 k 2 ( ϕ 1 2 + ϕ 2 + ϕ 3 ) d x c x k ( ϕ 1 2 + ϕ 2 + ϕ 3 ) d x η .

Using the expression (4.20), we conclude from (4.74) that

(4.76) 1 2 d d t R n ρ x 2 k 2 ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η ( s ) μ , 2 2 + 2 F ( x , u ) ) d x ϱ ( t , ω ) R n ρ x 2 k 2 ( v 2 + ( λ + δ 2 β 2 δ ) u 2 + Δ u 2 + η ( s ) μ , 2 2 + 2 F ( x , u ) ) d x + c ( Δ u 2 + v 2 + v 2 + η ( s ) μ , 2 2 ) + c R n ρ x 2 k 2 g ( x , t ) 2 d x + η ( 1 + ε z ( θ t ω ) ) .

Integrating (4.76) over ( τ t , τ ) for t R + and τ R , we get

(4.77) R n ρ x 2 k 2 ( v ( τ , τ t , ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , ω , u 0 ) 2 ) d x + R n ρ x 2 k 2 ( Δ u ( τ , τ t , ω , u 0 ) 2 + η ( τ , τ t , ω , η 0 , s ) μ , 2 2 + 2 F ( x , u ( τ , τ t , ω , u 0 ) ) ) d x e 2 τ τ t ϱ ( μ , ω ) d μ R n ρ x 2 k 2 ( v 0 ( x ) 2 + ( λ + δ 2 β 2 δ ) u 0 ( x ) 2 ) d x + e 2 τ τ t ϱ ( μ , ω ) d μ R n ρ x 2 k 2 ( Δ u 0 ( x ) 2 + η 0 ( s ) μ , 2 2 + 2 F ( x , u 0 ( x ) ) ) d x + c τ t τ e 2 τ s ϱ ( μ , ω ) d μ R n ρ x 2 k 2 g ( x , s ) 2 d s d x + η τ t τ e 2 τ s ϱ ( μ , ω ) d μ ( 1 + ε z ( θ s ω ) ) d s + c τ t τ e 2 τ s ϱ ( μ , ω ) d μ ( Δ u ( s , τ t , ω , u 0 ) 2 + v ( s , τ t , ω , v 0 ) 2 ) d s + c τ t τ e 2 τ s ϱ ( μ , ω ) d μ ( v ( s , τ t , ω , u 0 ) 2 + η ( s , τ t , ω , η 0 , s ) μ , 2 2 ) d s .

Replacing ω by θ τ ω in (4.77), for every t R + , τ R , and ω Ω ,

(4.78) R n ρ x 2 k 2 ( v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , θ τ ω , u 0 ) 2 ) d x + R n ρ x 2 k 2 ( Δ u ( τ , τ t , θ τ ω , u 0 ) 2 + η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 + 2 F ( x , u ( τ , τ t , θ τ ω , u 0 ) ) ) d x e 2 τ τ t ϱ ( μ τ , ω ) d μ R n ρ x 2 k 2 ( v 0 ( x ) 2 + ( λ + δ 2 β 2 δ ) u 0 ( x ) 2 ) d x + e 2 τ τ t ϱ ( μ τ , ω ) d μ R n ρ x 2 k 2 ( Δ u 0 ( x ) 2 + η 0 ( s ) μ , 2 2 + 2 F ( x , u 0 ( x ) ) ) d x + c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ R n ρ x 2 k 2 g ( x , s ) 2 d s d x + η τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( 1 + ε z ( θ s τ ω ) ) d s + c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( Δ u ( s , τ t , θ τ ω , u 0 ) 2 + v ( s , τ t , θ τ ω , v 0 ) 2 ) d s + c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( v ( s , τ t , θ τ ω , u 0 ) 2 + η ( s , τ t , θ τ ω , η 0 , s ) μ , 2 2 ) d s e 2 0 t ϱ ( μ , ω ) d μ ( v 0 ( x ) 2 + ( λ + δ 2 β 2 δ ) u 0 ( x ) 2 + Δ u 0 ( x ) 2 + η 0 ( s ) μ , 2 2 + 2 F ˜ ( x , u 0 ( x ) ) ) d x + c t 0 e 2 0 s ϱ ( μ , ω ) d μ R n ρ x 2 k 2 g ( x , s + τ ) 2 d s d x + η t 0 e 2 0 s ϱ ( μ , ω ) d μ ( 1 + ε z ( θ s ω ) ) d s + c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( Δ u ( s , τ t , θ τ ω , u 0 ) 2 + v ( s , τ t , θ τ ω , v 0 ) 2 ) d s + c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( v ( s , τ t , θ τ ω , u 0 ) 2 + η ( s , τ t , θ τ ω , η 0 , s ) μ , 2 2 ) d s .

It is similar to (4.31), for an arbitrarily given η > 0 , there exists T = T ( τ , ω , D , η ) such that for all t T ,

(4.79) e 2 0 t ϱ ( μ , ω ) d μ ( v 0 ( x ) 2 + ( λ + δ 2 β 2 δ ) u 0 ( x ) 2 + Δ u 0 ( x ) 2 + η 0 ( s ) μ , 2 2 + 2 F ˜ ( x , u 0 ( x ) ) ) d x η .

For the fourth and fifth terms on the right-hand side of (4.78), by Lemmas 4.1 and 4.3, for all t max { T 2 , T 4 } ,

(4.80) c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( Δ u ( s , τ t , θ τ ω , u 0 ) 2 + v ( s , τ t , θ τ ω , v 0 ) 2 ) d s + c τ t τ e 2 τ s ϱ ( μ τ , ω ) d μ ( v ( s , τ t , θ τ ω , u 0 ) 2 + η ( s , τ t , θ τ ω , η 0 , s ) μ , 2 2 ) d s η ( R 1 2 ( ε , τ , ω ) + R 3 2 ( ε , τ , ω ) ) .

For the second term on the right-hand side of (4.78), there exists K 1 = K 1 ( τ , ω ) 1 such that for all k K 1 , by (4.27), we get

(4.81) 0 e 2 0 s ϱ ( μ , ω ) d μ R n ρ x 2 k 2 g ( x , s + τ ) 2 d s d x T 1 e 2 0 s ϱ ( μ , ω ) d μ x k g ( x , s + τ ) 2 d s d x + T 1 0 e 2 0 s ϱ ( μ , ω ) d μ x k g ( x , s + τ ) 2 d s d x T 1 e σ s x k g ( x , s + τ ) 2 d s d x + e c T 1 0 e σ s x k g ( x , s + τ ) 2 d s d x ,

where c > 0 is a random variable independent of τ R and D D .

Therefore, by (3.20) there exists K 2 ( τ , ω ) K 1 such that for all k K 2 , we obtain

(4.82) c 0 e 2 0 s ϱ ( μ , ω ) d μ R n ρ x 2 k 2 g ( x , s + τ ) 2 d s d x e c 0 e σ s x k g ( x , s + τ ) 2 d s d x η .

Let

(4.83) R 4 2 ( τ , ω ) = 0 e 2 0 s ϱ ( μ , ω ) d μ ( 1 + ε z ( θ s ω ) ) d s ,

by (4.27), we know that the integral of (4.83) is convergent.

Together with (4.78)–(4.82), we have

(4.84) R n ρ x 2 k 2 ( v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , θ τ ω , u 0 ) 2 ) d x + R n ρ x 2 k 2 ( Δ u ( τ , τ t , θ τ ω , u 0 ) 2 + η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 ) + 2 F ( x , u ( τ , τ t , θ τ ω , u 0 ) ) d x 2 η ( 1 + R 1 2 ( τ , ω ) + R 3 2 ( τ , ω ) + R 4 2 ( τ , ω ) ) .

It follows from (4.30) and (4.84) that there exists K 3 = K 3 ( τ , ω ) K 2 , such that for all k K 3 , t max { T 2 , T 4 } ,

x 2 k ρ x 2 k 2 ( v ( τ , τ t , θ τ ω , v 0 ) 2 + ( λ + δ 2 β 2 δ ) u ( τ , τ t , θ τ ω , u 0 ) 2 ) d x + R n ρ x 2 k 2 ( Δ u ( τ , τ t , θ τ ω , u 0 ) 2 + η ( τ , τ t , θ τ ω , η 0 , s ) μ , 2 2 ) d x 3 η ( 1 + R 1 2 ( τ , ω ) + R 3 2 ( τ , ω ) + R 4 2 ( τ , ω ) ) ,

which implies (4.56).□

In order to obtain the precompactness of the solutions for (3.12)–(3.13) in bounded domain B 2 k later, we decompose φ = ( u , v , η ) of (3.12)–(3.13) into φ = φ L + φ N , where φ L = ( u L , ξ L , η L ) T and φ N = ( u N , v N , η N ) T solve, respectively,

(4.85) d u L d t + δ u L = ξ L , d ξ L d t δ ξ L + h ( u t ) h ( u N , t ) + ( λ + δ 2 + A ) u L + 0 μ ( s ) A η L ( s ) d s = 0 , η L , t + η L , s = u L , t , u L ( x , τ ) = u 0 ( x ) , ξ L ( x , τ ) = ξ 0 ( x ) , η L ( x , τ , s ) = η 0 ( x , s ) = u L ( x , τ ) u L ( x , τ s )

and

(4.86) d u N d t + δ u N = v N + ε u z ( θ t ω ) , d v N d t δ v N + h ( u N , t ) + ( λ + ε 2 + A ) u N + 0 μ ( s ) A η N ( s ) d s + f ( x , u ) = g ( x , t ) + ε ( v 3 δ u + ε u z ( θ t ω ) ) , η N , t + η N , s = u N , t , u N ( x , τ ) = 0 , v N ( x , τ ) = 0 , η N ( x , τ , s ) = 0 .

For the solutions of equations (4.85) and (4.86), by Lemmas 4.1 and 4.3, we can easily get the following estimates and regularity results, respectively.

Lemma 4.5

Assume that (3.4) and (3.10) hold. Then for any ( u L , ξ L , η L ) T of the solution of (4.85) satisfies

(4.87) φ L ( τ , τ t , θ τ ω , φ L , 0 ) E 2 0 , when t .

Lemma 4.6

Under Assumptions I and II, for every τ R , ω Ω , D = { D ( τ , ω ) : τ R , ω Ω } D , there exists T = T ( τ , ω , D ) > 0 such that for all t T the solution of problem (4.86) satisfies

A 1 4 φ N ( τ , τ t , θ τ ω , φ N , 0 ) E 2 R 3 ( τ , ω ) ,

where R 3 ( τ , ω ) is a random variable.

5 Random attractors

In this section, we prove existence and uniqueness of D -pullback attractors for the stochastic system (3.12)–(3.13). First we also need the following results to prove the asymptotic compactness about memory term as well as the existence of random attractors.

Lemma 5.1

[25] Let X 0 , X , X 1 be three Banach spaces such that X 0 X X 1 , the first injection being compact. Let Y L μ 2 ( R + , X ) satisfy the following hypotheses:

  1. Y is bounded in L μ 2 ( R + , X 0 ) H μ 1 ( R + , X 1 ) ;

  2. sup η Y η ( s ) X 2 K 0 , s R + for some K 0 > 0 .

Then Y is relatively compact in L μ 2 ( R + , X ) .

Note that for any τ R , ω Ω , t m 0 ,

(5.1) η N ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) = u N ( τ , τ t m , θ τ ω , u N , 0 ( θ t m ω ) ) u N ( τ s , τ t m , θ τ + s ω , u N , 0 ( θ t m + s ω ) ) , s t , u N ( τ , τ t m , θ τ ω , u N , 0 ( θ t m ω ) ) , s t

and

(5.2) η N , s ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) ) = u N , t ( τ s , τ t m , θ τ + s ω , u N , 0 ( θ t m + s ω ) ) , s t , 0 , s t .

Then from Lemma 4.6 and (5.2), it follows that

(5.3) max { η N , s ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) μ , 1 2 , η N ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) μ , 3 2 } 2 R 3 ( τ , ω ) , s 0 ,

which implies that { η N ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) } m = 1 is bounded in L μ 2 ( R + , V 3 ) H μ 1 ( R + , V 1 ) . For brevity, we denote B ˆ ( τ , ω ) = { η N ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) } m = 1 . Again, by Lemmas 4.1, Lemma 4.6, and (5.1), we have

(5.4) sup η B ˆ ( τ , ω ) , s 0 Δ η ( s ) 2 = sup t m 0 sup η 0 ( θ t m ω ) D ( τ t m , θ t m ω ) Δ η N ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) 2 2 R 1 ( τ , ω ) .

Thus, by (3.4) and (5.4), it follows that for any η B ˆ ( τ , ω ) ,

(5.5) η ( s ) μ , 2 2 = 0 + μ ( s ) Δ η ( s ) 2 d s 2 R 1 ( τ , ω ) 0 + e δ s d s 2 R 1 ( τ , ω ) δ ,

which shows that { η N ( τ , τ t m , θ τ ω , η N , 0 ( θ t m ω ) , s ) } m = 1 L μ 2 ( R + , H 2 ( B 2 k 1 ) ) is a bounded subset. By Lemma 4.5 and 5.1, we know that the sequence { η ( τ , τ t m , θ τ ω , η 0 ( θ t m ω ) , s ) } m = 1 is compact in L μ 2 ( R + , H 2 ( B 2 k 1 ) ) .

Then we apply the lemmas shown in Section 4 to prove the asymptotic compactness of solutions of (3.12)–(3.13) in E .

Lemma 5.2

Under Assumptions I and II, for every τ R , ω Ω , the sequence of solutions of (3.12)–(3.13), { φ ( τ , τ t m , θ τ ω , φ 0 , n ) } m = 1 has a convergent subsequence in E whenever t m and φ 0 , n D ( τ t m , θ t m ω ) with D D .

Proof

By Lemma 4.4, for every ζ > 0 , there exist k 0 = k 0 ( τ , ω , ζ ) 1 and m 2 = m 2 ( τ , ω , D , ζ ) m 1 such that for all m m 1 ,

(5.6) φ ( τ , τ t , θ τ ω , φ 0 , n ) E ( R n B k 0 ) 2 ζ ,

By Lemma 4.6, there exist k 1 = k 1 ( τ , ω ) k 0 , such that

A 1 4 u N ( τ , τ t m , θ τ ω , u N , 0 ( θ t m ω ) H 2 ( B 2 k 1 ) 2 + A 1 4 v N ( τ , τ t m , θ τ ω , v N , 0 ( θ t m ω ) L 2 ( B 2 k 1 ) 2 R 3 ( τ , ω ) ,

which along with the compact embedding H 3 ( B 2 k 1 ) × H 1 ( B 2 k 1 ) H 2 ( B 2 k 1 ) × L 2 ( B 2 k 1 ) , we know the sequences { ( u N ( τ , τ t m , θ τ ω , u N , 0 ( θ t m ω ) ) , v N ( τ , τ t m , θ τ ω , v N , 0 ( θ t m ω ) ) ) } m = 1 are precompact in H 2 ( B 2 k 1 ) × L 2 ( B 2 k 1 ) . By Lemma 4.5, we deduce that the sequences { ( u ( τ , τ t m , θ τ ω , u 0 ( θ t m ω ) ) , v ( τ , τ t m , θ τ ω , v 0 ( θ t m ω ) ) ) } m = 1 are precompact in H 2 ( B 2 k 1 ) × L 2 ( B 2 k 1 ) . In addition, the sequences { η ( τ , τ t m , θ τ ω , η 0 ( θ t m ω ) , s ) } m = 1 are precompact in L μ 2 ( R + , H 2 ( B 2 k 1 ) ) . Thus, { φ ( τ , τ t m , θ τ ω , φ 0 , n ) } m = 1 is precompact in E ( B 2 k 1 ) , this together with (5.6) implies { φ ( τ , τ t m , θ τ ω , φ 0 , n ) } m = 1 has a convergent subsequence in E ( R n ) .□

Since Lemma 4.1 implies a pullback D -absorbing set for Φ , and Φ ε is pullback D -asymptotically compact in E from Lemma 5.2, we immediately get the following existence theorem by Proposition 2.1.

Theorem 5.3

Under Assumptions I and II, the cocycle Φ generated by the stochastic plate equation (3.12)–(3.13) has a unique pullback D -attractor A = { A ( τ , ω ) : τ R , ω Ω } D in the space E .

  1. Funding information: This work was supported by the NSFC No. (12161071), Key projects of university level planning in Qinghai Nationalities University grant (2021XJGH01), and Scientific Research Innovation Team in Qinghai Nationalities University.

  2. Conflict of interest: Author states no conflict of interest.

References

[1] A. R. A. Barbosaa and T. F. Ma , Long-time dynamics of an extensible plate equation with thermal memory, J. Math. Anal. Appl. 416 (2014), 143–165. 10.1016/j.jmaa.2014.02.042Search in Google Scholar

[2] A. Kh Khanmamedov , A global attractor for the plate equation with displacement-dependent damping, Nonlinear Anal. 74 (2011), 1607–1615. 10.1016/j.na.2010.10.031Search in Google Scholar

[3] A. Kh. Khanmamedov , Existence of global attractor for the plate equation with the critical exponent in an unbounded domain, Appl. Math. Lett. 18 (2005), 827–832. 10.1016/j.aml.2004.08.013Search in Google Scholar

[4] A. Kh Khanmamedov , Global attractors for the plate equation with a localized damping and a critical exponent in an unbounded domain, J. Differ. Equ. 225 (2006), 528–548. 10.1016/j.jde.2005.12.001Search in Google Scholar

[5] T. T. Liu and Q. Z. Ma , Time-dependent attractor for plate equations on Rn , J. Math. Anal. Appl. 479 (2019), 315–332. 10.1016/j.jmaa.2019.06.028Search in Google Scholar

[6] M. A. J. Silva and T. F. Ma , Long-time dynamics for a class of Kirchhoff models with memory, J. Math. Phys. 54 (2013), 021505. 10.1063/1.4792606Search in Google Scholar

[7] H. Wu , Long-time behavior for a nonlinear plate equation with thermal memory, J. Math. Anal. Appl. 348 (2008), 650–670. 10.1016/j.jmaa.2008.08.001Search in Google Scholar

[8] H. B. Xiao , Asymptotic dynamics of plate equations with a critical exponent on unbounded domain, Nonlinear Anal. 70 (2009), 1288–1301. 10.1016/j.na.2008.02.012Search in Google Scholar

[9] L. Yang and C. K. Zhong , Global attractor for plate equation with nonlinear damping, Nonlinear Anal. 69 (2008), 3802–3810. 10.1016/j.na.2007.10.016Search in Google Scholar

[10] G. C. Yue and C. K. Zhong , Global attractors for plate equations with critical exponent in locally uniform spaces, Nonlinear Anal. 71 (2009), 4105–4114. 10.1016/j.na.2009.02.089Search in Google Scholar

[11] J. Zhou , Global existence and blow-up of solutions for a Kirchhoff type plate equation with damping, Appl. Math. Comput. 265 (2015), 807–818. 10.1016/j.amc.2015.05.098Search in Google Scholar

[12] L. Yang and C. K. Zhong , Uniform attractor for non-autonomous plate equations with a localized damping and a critical nonlinearity, J. Math. Anal. Appl. 338 (2008), 1243–1254. 10.1016/j.jmaa.2007.06.011Search in Google Scholar

[13] T. T. Liu and Q. Z. Ma , Time-dependent asymptotic behavior of the solution for plate equations with linear memory, Discrete Contin. Dyn. Syst. Ser. B 23 (2018), 4595–4616. 10.3934/dcdsb.2018178Search in Google Scholar

[14] T. T. Liu and Q. Z. Ma , The existence of time-dependent strong pullback attractors for non-autonomous plate equations, Chinese J. Contemp. Math. 2 (2017), 101–118. Search in Google Scholar

[15] W. J. Ma and Q. Z. Ma , Attractors for the stochastic strongly damped plate equations with additive noise, Electron. J. Differ. Equ. 111 (2013), 1–12. Search in Google Scholar

[16] Q. Z. Ma and W. J. Ma . Asymptotic behavior of solutions for stochastic plate equations with strongly damped and white noise, J. Northwest Norm. Univ. Nat. Sci. 50 (2014), 6–17. Search in Google Scholar

[17] X. Y. Shen and Q. Z. Ma , The existence of random attractors for plate equations with memory and additive white noise, Korean J. Math. 24 (2016), 447–467. 10.11568/kjm.2016.24.3.447Search in Google Scholar

[18] X. Y. Shen and Q. Z. Ma , Existence of random attractors for weakly dissipative plate equations with memory and additive white noise, Comput. Math. Appl. 73 (2017), 2258–2271. 10.1016/j.camwa.2017.03.009Search in Google Scholar

[19] X. B. Yao , Q. Z. Ma , and T. T. Liu , Asymptotic behavior for stochastic plate equations with rotational inertia and Kelvin-Voigt dissipative term on unbounded domains, Discrete Contin. Dyn. Syst. Ser. B 24 (2019), 1889–1917. 10.3934/dcdsb.2018247Search in Google Scholar

[20] X. B. Yao and X. Liu , Asymptotic behavior for non-autonomous stochastic plate equation on unbounded domains, Open Math. 17 (2019), 1281–1302. 10.1515/math-2019-0092Search in Google Scholar

[21] X. B. Yao , Existence of a random attractor for non-autonomous stoc- hastic plate equations with additive noise and nonlinear damping on Rn , Bound. Value Probl. 2020 (2020), 49, https://doi.org/10.1186/s13661-020-01346-z. Search in Google Scholar

[22] X. B. Yao , Random attractors for non-autonomous stochastic plate equations with multiplicative noise and nonlinear damping, AIMS Math. 5 (2020), 2577–2607. 10.3934/math.2020169Search in Google Scholar

[23] B. Wang and X. Gao , Random attractors for wave equations on unbounded domains, Discr. Contin. Dyn. Syst. 2009 (2009), 800–809. Search in Google Scholar

[24] Z. Wang , S. Zhou , and A. Gu , Random attractor for a stochastic damped wave equation with multiplicative noise on unbounded domains, Non. Anal. RWA 12 (2011), 3468–3482. 10.1016/j.nonrwa.2011.06.008Search in Google Scholar

[25] V. Pata and A. Zucchi , Attractors for a damped hyperbolic equation with linear memory, Adv. Math. Sci. Appl. 11 (2001), 505–529. Search in Google Scholar

[26] B. Wang , Sufficient and necessary criteria for existence of pullback attractors for non-compact random dynamical systems, J. Differ. Equ. 253 (2012), 1544–1583. 10.1016/j.jde.2012.05.015Search in Google Scholar

[27] B. Wang , Existence and upper semicontinuity of attractors for stochastic equations with deterministic non-autonomous terms, Stoch. Dyn. 14 (2014), no. 4, 1450009, https://doi.org/10.1142/S0219493714500099. Search in Google Scholar

[28] C. M. Dafermos , Asymptotic stability in viscoelasticity, Arch. Ration. Mech. Anal. 37 (1970), 297–308. 10.1007/BF00251609Search in Google Scholar

[29] A. Pazy , Semigroup of Linear Operators and Applications to Partial Differential Equations, Springer-Verlag, New York, 1983. 10.1007/978-1-4612-5561-1Search in Google Scholar

[30] J. Duan , K. Lu , and B. Schmalfuss , Invariant manifolds for stochastic partial differential equations, Ann. Probab. 31 (2003), 2109–2135. 10.1214/aop/1068646380Search in Google Scholar

[31] R. Temam , Infinite Dimensional Dynamical Systems in Mechanics and Physics, Springer-Verlag, New York, 1998. 10.1007/978-1-4612-0645-3Search in Google Scholar

Received: 2021-04-15
Accepted: 2021-08-11
Published Online: 2021-12-31

© 2021 Xiao Bin Yao, published by De Gruyter

This work is licensed under the Creative Commons Attribution 4.0 International License.

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