1 Introduction

For u(x,t):Ω× R + R, we consider the strongly damped wave equation on a bounded domain Ω in R 3 with smooth boundary:

u t t αΔ u t Δu+h( u t )+f(u)=g(x),
(1.1)

supplemented with the periodic boundary conditions and initial conditions

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

where the strongly damped coefficient α is a positive constant, the damped function h:RR is continuous, and the forcing term f:RR is a nonlinear term satisfying some growth conditions, g:ΩR is the external force.

When α=0, (1.1) reduces to a usual wave equation with nonlinear damping, which arises as an evolutionary mathematical model in various systems (cf. [1, 2]), for example: (i) modeling a continuous Josephson junction with specific h, g and f; (ii) modeling a hybrid system of nonlinear waves and nerve conduct; and (iii) modeling a phenomenon in quantum mechanics and which has been studied widely by using of the concept of global attractors; see, for example, [210] for the linear damping case, and [1118] for the nonlinear damping case. There are some results on the regularity in these papers; for example, in [7] the authors gave the dimensionality and related properties of the global attractor, and in [14], the authors presented a direct method to establish the optimal regularity of the attractor for the semilinear damped wave equation (when α=0 and h( u t )= u t ) with nonlinearity for the critical growth. But for α0, the case can be complex.

There is a large literature on the asymptotic behavior of solutions to (1.1), (1.2) (cf. [1, 1923]). For the strongly damped wave equations, [23] had proved the uniform boundedness of the global attractor for very strong damping in H 1 × L 2 and obtained an estimate of the upper bound of the Hausdorff dimension of an attractor for the strongly damped nonlinear wave equation (1.1). Furthermore, when h( u t )=0, Pata and Zelik in [21] had proved the existence of compact global attractors of optimal regularity, i.e., the compact global attractor on H 1 (Ω)× L 2 (Ω) is a bounded subset of H 2 × H 1 . The aim of this paper is to prove that the dynamical system associated with (1.1) possesses a compact global attractor in H 2 (Ω)× H 1 (Ω), i.e., we will prove that the global attractor A 1 in H 1 (Ω)× L 2 (Ω) is a compact set A 2 in H 2 (Ω)× H 1 (Ω). This implies that A 1 = A 2 .

The paper is organized as follows. In Section 2, we present the existence, uniqueness, and continuous dependence of solutions for problem (1.1), and we establish the existence of an absorbing set in H 1 (Ω)× L 2 (Ω). In Section 3, we prove the existence of the global attractor in H 1 (Ω)× L 2 (Ω). In Section 4, we establish the regularity of the attractor, i.e., that the global attractor is a compact subset in H 2 (Ω)× H 1 (Ω).

2 Preliminaries

We assume that g L 2 (Ω)=H, and H ˙ 1 = ( H ˙ 1 ) , with

H ˙ 1 = H 1 { u L 2 ( Ω ) ; Ω u ( x ) d x = 0 } ,

and the functions h, f satisfy the following conditions:

  1. (i)

    Let f(u) C 1 (R;R) satisfy:

    (1) The asymptotic sign condition

    lim sup | s | + f ( s ) s 0.
    (2.1)

    (2) Let F(s)= 0 s f(ρ)dρ, there exist constants c 1 , c 2 ,δ, C δ >0 such that

    ( f ( u ) , u ) c 1 Ω F(u)dxδ | u | 2 C δ |Ω|,
    (2.2)

    where | | 0 denotes the absolute value of the number in ℝ. We have

    | f (s)| c 2 ( 1 + | s | p ) with  { 0 p < , when  n = 1 , 2 , 0 p < 2 , when  n = 3 .
    (2.3)
  2. (ii)

    There exist two constants β 1 , β 2 0 such that

    h(0)=0,0< β 1 h (s) β 2 <+,sR.
    (2.4)

Let Au=Δu, then the system (1.1)-(1.2) is equivalent to the following initial value problem in H ˙ 1 (Ω)× L 2 (Ω):

{ Y ˙ = P Y + Q ( Y ) , x Ω , t > 0 , Y ( 0 ) = Y 0 = ( u 0 , u 1 ) T H ˙ × L 2 ,
(2.5)

where Y= ( u , u t ) T , Q(Y)= ( 0 , h ( u t ) f ( u ) + g ) T ,

P= ( 0 I A k A ) .

By the assumption (2.1)-(2.4), it is easy to check that the function Q(Y): H ˙ 1 × L 2 H ˙ 1 × L 2 is continuously differentiable and globally Lipschitz continuous with respect to Y. By the classical theory concerning the existence and uniqueness of the solutions of evolution differential equations (cf. [15]), we have the following lemma (see [23] for details).

Lemma 2.1 Consider the initial value problem (2.5) in H ˙ 1 × L 2 . If (2.1)-(2.4) hold, then, for any Y 0 H ˙ 1 × L 2 , there exists a unique continuous function Y()=Y(, Y 0 )C( R + ; H ˙ 1 × L 2 ) such that Y(0, Y 0 )= Y 0 and Y(t) satisfies the integral equation

Y(t, Y 0 )= e P t Y 0 + 0 t e P ( t τ ) Q ( Y ( τ ) ) dτ.

Y(t, Y 0 ) is called the mild solution of (2.5), and Y(t, Y 0 ) is jointly continuous in t and Y 0 , and

(u, u t )C ( R + ; H ˙ 1 ( Ω ) ) × [ C ( R + ; L 2 ( Ω ) ) L 2 ( ( 0 , T ) ; H ˙ 1 ( Ω ) ) ] , T >0.

For any t0, we can introduce a map

S(t): Y 0 =( u 0 , u 1 )(u, u t )=Y(t, Y 0 ),S(t): H ˙ 1 × L 2 H ˙ 1 × L 2 ,

where Y(t, Y 0 ) is the solution of (2.5), and then {S(t)|t0} is a continuous semigroup on H ˙ 1 × L 2 .

Consider the map G: H ˙ 1 × L 2 H ˙ 1 × L 2 defined as

G ( u ( t ) , u t ( t ) ) = e P t ( u 0 , u 1 )+ 0 t e P ( t τ ) ( 0 , g h ( u t ( τ ) ) f ( u ( τ ) ) ) dτ.
(2.6)

For some λ>0, let

A 1 =A+λI.
(2.7)

Let

( u , v ) = Ω u v d x , | u | = ( u , u ) 1 2 , u , v L 2 , ( ( u , v ) ) = Ω A 1 u v d x , u = ( ( u , u ) ) 1 2 , u , v H 1 ( Ω ) .

Obviously, A 1 is symmetric and positive definite, so we have the following Poincaré type inequality:

y λ |y|,y L 2 .
(2.8)

Let h 1 ( u t )=h( u t )αλ u t , then (1.1) can be written in the equivalent form

u t t +α A 1 u t + A 1 u+ h 1 ( u t )λu+f(u)=g,
(2.9)

and by (2.4), h 1 ( u t ) satisfies

h 1 (0)=0,αλ< β 1 h 1 (θ) β 2 <+,θR,
(2.10)

where β 1 = β 1 αλ, β 2 = β 2 αλ are two constants.

To construct an attractor for (1.1), we make the following assumptions. Let φ= ( u , v ) T , v= u t +ku, where k is chosen as

k= α λ + β 1 4 + 2 ( α λ + β 1 ) α + β 2 2 / λ 1 .
(2.11)

Equation (2.9) can be written as

φ t +H(φ)=F(φ),φ(0)= ( u 0 , v 0 = u 1 + k u 0 ) T ,t0,
(2.12)

where

F ( φ ) = ( 0 λ u f ( u ) + g ) , H ( φ ) = ( k u v A 1 u k ( α A 1 k ) u + ( α A 1 k ) v ) + ( 0 h 1 ( v k u ) ) .

We define a new weighted inner product and norm in E= H ˙ 1 × L 2 as

( φ , ψ ) E =μ ( ( u 1 , u 2 ) ) +( v 1 , v 2 ), φ E = ( φ , φ ) E 1 / 2 ,
(2.13)

for any φ= ( u 1 , v 1 ) T ,ψ= ( u 2 , v 2 ) T E, where μ is chosen as

μ= 4 + ( α λ + β 1 ) α + β 2 2 / λ 4 + 2 ( α λ + β 1 ) α + β 2 2 / λ ( 1 2 , 1 ) .
(2.14)

Obviously, the norm E in (2.13) is equivalent to the usual norm | | H ˙ 1 × L 2 in E.

Lemma 2.2 (see [23], Lemma 1)

For any φ= ( u , v ) T E, if

αλ< β 1 β 2 <+, β 2 | β 1 |+min { 1 / α , ( α λ + β 1 ) / 2 } ,
(2.15)

hold, then

( H ( φ ) , φ ) E σ φ E 2 + α 2 v 2 + β 1 2 | v | 2 σ φ E 2 + α λ + β 1 2 | v | 2 ,
(2.16)

where

σ= α λ + β 1 γ 1 + γ 1 γ 2 , γ 1 =4+(αλ+ β 1 )α+ β 2 2 λ , γ 2 =(αλ+ β 1 )α+ β 2 2 λ .
(2.17)

Proposition 2.1 The semigroup {S(t)|t0} possesses an absorbing set B H ˙ 1 × L 2 .

Proof Let φ= ( u , v ) T E be the solution of (2.12). Taking the inner product ( , ) E of (2.12) with φ, we have

( φ t ,φ)+ ( H ( φ ) , φ ) = ( F ( φ ) , φ )

and

1 2 d d t φ E 2 + ( H ( φ ) , φ ) E + ( f ( u ) , v ) λ(u,v)=(g,v).
(2.18)

By v= u t +ku, we have

( f ( u ) , v ) = ( f ( u ) , u t + k u ) = d d t Ω F(u)dx+k ( f ( u ) , u ) ,
(2.19)

by (2.18) and (2.19), we have

1 2 d d t [ φ E 2 + 2 Ω F ( u ) d x ] + ( H ( φ ) , φ ) E +k ( f ( u ) , u ) λ(u,v)=(g,v).
(2.20)

Let y(t)= φ E 2 +2 Ω F(u)dx+2 C δ |Ω| 1 4 φ E 2 0. By (2.15) and (2.2), there exists δ>0 such that

( H ( φ ) , φ ) E + k ( f ( u ) , u ) λ ( u , v ) σ φ E 2 + α λ + β 1 2 | v | 2 + k c 1 Ω F ( u ) d x + k δ | u | 2 k C δ | Ω | λ | u | | v | σ φ E 2 + α λ + β 1 2 | v | 2 + k c 1 Ω F ( u ) d x + k δ λ μ μ | u | 2 k C δ | Ω | λ 2 μ φ E 2 ( σ + k δ λ μ λ 2 μ ) φ E 2 + k c 1 Ω F ( u ) d x k C δ | Ω | + α λ + β 1 2 | v | 2 1 2 ρ y k ( C δ | Ω | + c 1 C δ | Ω | ) + α λ + β 1 2 | v | 2 ,
(2.21)

where ρ=min{k c 1 ,(σ+ k δ λ μ λ 2 μ )}. By (2.20) and (2.21),

d d t y + ρ y 2 k C δ | Ω | ( 1 + c 1 ) + 2 ( g , v ) ( α λ + β 1 ) | v | 2 2 k C δ | Ω | ( 1 + c 1 ) + 1 α λ + β 1 | g | 2 .
(2.22)

Using the Gronwall lemma, we have

φ ( t ) E 2 4y(0) e 2 ρ t +4 ( | g | 2 ( α λ + β 1 ) ρ + 2 k C δ | Ω | ( 1 + c 1 ) ρ ) .

Following [24] and [8], it follows from (2.1) that, for each κ>0, there is a constant C κ >0 such that, for each u L 2 (Ω),

( f ( u ) , u ) = Ω f(u)udxκ | u | 2 + C κ .
(2.23)

Note that (2.2) and (2.23) imply

c 1 Ω F ( u ) d x ( f ( u ) , u ) δ | u | 2 + C δ | Ω | κ | u | 2 + C κ δ | u | 2 + C δ | Ω | c ( 1 + | u | 2 ) .
(2.24)

For any bounded set B of E, where sup φ B φ E <r, if φ(0)B, there exists c 2 = c 2 (r)>0 such that y(0)= φ ( 0 ) E 2 +2 Ω F( u 0 )dx+2 C δ |Ω| c 2 . Therefore, for the solution φ(t)= ( u ( t ) , v ( t ) ) T of (2.12) with φ(0)B,

φ ( t ) E 2 4 c 2 (r) e 2 ρ t +4 ( | g | 2 ( α λ + β 1 ) ρ + 2 k C δ | Ω | ( 1 + c 1 ) ρ ) .

Taking

M 0 =8 ( | g | 2 ( α λ + β 1 ) ρ + 2 k C δ | Ω | ( 1 + c 1 ) ρ )

completes the proof. □

3 Existence of the global attractor in H ˙ 1 × L 2

Theorem 3.1 (see [[2], I.1.1])

Let {S(t)|t0} be a continuous semigroup on H ˙ 1 × L 2 that possesses an absorbing ball in H ˙ 1 × L 2 . Let us assume that, for any t0,

S(t)= S 1 (t)+ S 2 (t),

where:

  • For every bounded set B, there exists t 0 that depends on B, such that t t 0 S 1 (t)Bis relatively compact in H ˙ 1 × L 2 .

  • For every bounded set B,

    lim sup t ( sup θ B S 2 ( t ) θ H ˙ 1 × L 2 ) =0.

Then S ( t ) t 0 possesses a global attractor A that is compact in H ˙ 1 × L 2 .

Remark 3.1 (see [10])

We characterize such an attractor A as

A = { ( u 0 , u 1 ) H ˙ 1 × L 2 , ( u 0 n , u 1 n ) n B , ( t n ) , such that  S ( t n ) ( u 0 n , u 1 n ) ( u 0 , u 1 ) H ˙ 1 × L 2 0 } .

Theorem 3.2 The semigroup {S(t)|t0} possesses a global attractor A in H ˙ 1 × L 2 .

Proof We consider g ϵ C 0 and 0 1 g ϵ (x)dx=0 such that

| g g ϵ | L 2 <ϵ,
(3.1)

and we introduce the splitting (u,v)=( u 1 , v 1 )+( u 2 , v 2 )+( u 3 , v 3 ) where ( u 1 , v 1 ) satisfies

{ u 1 , t + k u 1 v 1 = 0 , v 1 , t + A 1 u 1 k ( α A 1 k ) u 1 + ( α A 1 k ) v 1 + h 1 ( v 1 k u 1 ) + f ( u ) λ u 1 = g ϵ , u 1 ( 0 ) = 0 , v 1 ( 0 ) = 0 ,
(3.2)

( u 2 , v 2 ) satisfies

{ u 2 , t + k u 2 v 2 = 0 , v 2 , t + A 1 u 2 k ( α A 1 k ) u 2 + ( α A 1 k ) v 2 + h 1 ( v 1 k u 1 + v 2 k u 2 ) h 1 ( v 1 k u 1 ) + f ( u 1 + u 2 ) f ( u 1 ) λ u 2 = g g ϵ , u 2 ( 0 ) = 0 , v 2 ( 0 ) = 0 ,
(3.3)

and ( u 3 , v 3 ) is the solution of

{ u 3 , t + k u 3 v 3 = 0 , v 3 , t + A 1 u 3 k ( α A 1 k ) u 3 + ( α A 1 k ) v 3 + h 1 ( v k u ) h 1 ( v 1 k u 1 + v 2 k u 2 ) + f ( u ) f ( u 1 + u 2 ) λ u 3 = 0 , u 3 ( 0 ) = u 0 , v 3 ( 0 ) = v 0 .
(3.4)

We now define the families of maps { S k 1 (t)|t0} and { S k 2 (t)|t0} in H ˙ 1 × L 2 , where

S k 1 (t)( u 0 , v 0 )= ( u 1 ( t ) , v 1 ( t ) ) + ( u 2 ( t ) , v 2 ( t ) ) , S k 2 (t)( u 0 , v 0 )= ( u 3 ( t ) , v 3 ( t ) ) .

First step: We prove that ( u 1 , v 1 ) is bounded in H 2 × H 1 . The system (3.2) can be written as

φ t 1 + H 1 ( φ 1 ) = F 1 ( φ 1 ) , φ 1 (0)= ( 0 , 0 ) T ,t0,
(3.5)

where

F 1 ( φ 1 ) = ( 0 f ( u 1 ) + λ u 1 + g ϵ ) , H 1 ( φ 1 ) = ( k u 1 v 1 A 1 u 1 k ( α A 1 k ) u 1 + ( α A 1 k ) v 1 + h ( v 1 k u 1 ) ) .
(3.6)

Similar to Proposition 2.1, we obtain

φ 1 E 2 1 ρ C ( | g ϵ | H 1 , λ , α , δ , κ , k , β 1 , β 2 ) = M 1 .
(3.7)

Now we multiply (3.2) by ( A 1 u 1 , A 1 v 1 ) and integrate on Ω to obtain

1 2 d d t A 1 1 2 φ 1 E 2 +σ A 1 1 2 φ 1 E 2 + α λ + β 1 2 | A 1 1 2 v 1 | 2 ( f ( u 1 ) + λ u 1 , A 1 v 1 ) +( g ϵ , A 1 v 1 ),
(3.8)

with

( f ( u 1 ) , A 1 v 1 ) = ( A 1 1 2 f ( u 1 ) , A 1 1 2 ( u 1 , t + k u 1 ) ) = d d t ( A 1 1 2 f ( u ) , A 1 1 2 u 1 ) + ( A 1 1 2 f ( u 1 ) u 1 , t , A 1 1 2 u 1 ) k ( A 1 1 2 f ( u ) , A 1 1 2 u 1 ) .

Then (3.8) can be rewritten as

1 2 d d t [ A 1 1 2 φ 1 E 2 + 2 ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) ] + σ A 1 1 2 φ 1 E 2 + k ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) α λ + β 1 2 | A 1 1 2 v 1 | 2 + ( A 1 1 2 f ( u 1 ) u 1 , t , A 1 1 2 u 1 ) + λ ( A 1 1 2 u 1 , A 1 1 2 v 1 ) + ( A 1 1 2 g ϵ , A 1 1 2 v 1 ) ,

i.e.,

1 2 d d t [ A 1 1 2 φ 1 E 2 + 2 ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) ] + ( σ λ 2 μ ) A 1 1 2 φ 1 E 2 + k ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) ( A 1 1 2 f ( u 1 ) u 1 , t , A 1 1 2 u 1 ) + A 1 1 2 g ϵ 2 ( α λ + β 1 ) ;
(3.9)

for the first term on the right-hand side of (3.9), we have

( A 1 1 2 f ( u 1 ) u 1 , t , A 1 1 2 u 1 ) c 3 | A 1 1 2 u 1 , t | | u 1 | 6 p | A 1 1 2 u 1 | 6 3 p c 3 | A 1 1 2 u 1 , t | | u 1 | H 1 p | A 1 1 2 u 1 | 2 p 2 | A 1 1 2 u 1 | p 2 c 3 λ p 2 4 | A 1 1 2 u 1 , t | | u 1 | H 1 p | A 1 u 1 | c 4 | A 1 u 1 | 2 + c 4 λ p 4 2 | A 1 1 2 u 1 , t | 2 | u 1 | H 1 2 p c 4 | A 1 u 1 | 2 + c 5 λ p 4 2 ( 1 + | u 1 | H 1 6 + | v 1 | H 1 6 ) c 6 A 1 1 2 φ 1 E 2 + c 5 λ p 4 2 ( 1 + | u 1 | H 1 6 + | v 1 | 6 ) .
(3.10)

By (3.9)-(3.10), we have

d d t [ A 1 1 2 φ 1 E 2 + 2 ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) ] + 2 ( σ λ 2 μ c 6 ) A 1 1 2 φ 1 E 2 + 2 k ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) 2 c 5 λ p 4 2 ( | u 1 | H 1 6 + | v 1 | 6 ) + A 1 1 2 g ϵ α λ + β 1 .
(3.11)

Let ϱ=min{σ λ 2 μ c 6 ,k}0, using the Gronwall lemma, we have

A 1 1 2 φ 1 E 2 + 2 ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) ( A 1 1 2 φ 1 ( 0 ) E 2 + 2 ( A 1 1 2 f ( u 1 ( 0 ) ) , A 1 1 2 u 1 ( 0 ) ) ) e 2 ϱ t + 2 c 5 λ p 4 2 0 t e 2 ϱ t ( | u 1 ( s ) | H 1 6 + | v 1 ( s ) | 6 ) d s + | A 1 1 2 g ϵ | ( α λ + β 1 ) ϱ 2 c 5 λ p 4 2 0 t e 2 ϱ t ( | u 1 ( s ) | H 1 6 + | v 1 ( s ) | 6 ) d s + | A 1 1 2 g ϵ | ( α λ + β 1 ) ϱ .

By (3.7), we have

A 1 1 2 φ 1 E 2 +2 ( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) 1 ρ ϱ C 3 ( | A 1 1 2 g ϵ | , λ , α , δ , κ , k , β 1 , β 2 ) .

Note that (3.2) implies that

( A 1 1 2 f ( u 1 ) , A 1 1 2 u 1 ) c 7 | A 1 1 2 u 1 | 2 + c 7 | A 1 1 2 u 1 | c 8 A 1 1 2 φ 1 E 2 .

Then we obtain

A 1 2 φ 1 E 2 1 ρ ϱ C 3 ( | A 1 1 2 g ϵ | , λ , α , δ , κ , k , β 1 , β 2 ) .
(3.12)

Proposition 2.1, (3.8), and (3.12) imply that ( u 1 , v 1 ) is bounded in H 2 × H 1 .

Second step: Let φ 2 =( u 2 , v 2 ); we will prove that there exists a K>0 independence on ϵ such that

φ 2 E Kϵ.

Multiplying (3.3) by ( u 2 , v 2 ), we thus obtain

1 2 d d t φ 2 E 2 + ( σ 2 λ μ ) φ 2 E 2 + α λ + β 1 2 | v 2 | 2 + ( f ( u 1 + u 2 ) f ( u 1 ) , v 2 ) | g g ϵ | | v 2 | .
(3.13)

For the last term on the left-hand side of (3.13), by (2.3), Proposition 2.1, and (3.7), there exists ξ such that

( f ( u 1 + u 2 ) f ( u 1 ) , v 2 ) = ( f ( u 1 + ξ u 2 ) u 2 , v 2 ) c 2 ( 1 + | u 1 | p + | u 2 | p ) | u 2 | | v 2 | c 11 ( M 0 , M 1 ) | u 2 | | v 2 | .
(3.14)

By the Gronwall and Poincaré inequalities,

φ 2 E 2 2 | g g ϵ | 2 ( 2 λ μ + c 11 ( M 0 , M 1 ) σ ) ( α λ + β 1 ) 8 ϵ 2 ( 2 λ μ + c 11 ( M 0 , M 1 ) σ ) ( α λ + β 1 ) .
(3.15)

By (3.12), (3.15), and the following lemma we see that { S k 1 (t)|t0} is compact in H ˙ 1 × L 2 .

Lemma 3.1 (see [25])

Let X be a complete metric space and A be a subset in X, such that

ϵ,A K ϵ +B ( 0 , C ( ϵ ) )

with lim ϵ 0 C(ϵ)=0 and K ϵ is compact in X, then A is compact in X.

Third step: Let φ 3 =( u 3 , v 3 ), by (3.4) and Lemma 2.2, we have

1 2 d d t φ 3 E 2 +σ φ 3 E 2 + α λ + β 1 2 | v 3 | 2 ( f ( u ) f ( u 1 + u 2 ) , v 3 ) +λ( u 3 , v 3 ).
(3.16)

For the right-hand side of (3.16), by (2.1), we have

( f ( u ) f ( u 1 + u 2 ) , v 3 ) + λ ( u 3 , v 3 ) c 13 | u 3 | | v 3 | + λ | u 3 | | v 3 | c 14 u 3 | v 3 | σ 2 φ 3 E 2 + ( c 14 2 2 σ μ σ 2 ) | v 3 | 2 .
(3.17)

Let c 14 < σ μ ( α λ + β 1 ) + σ 2 μ . Equations (3.16) and (3.17) lead to

φ 3 E 2 ( μ u 0 2 + | v 0 | 2 ) exp{σt}.
(3.18)

In other words we have

S(t)( u 0 , v 0 )0in  H ˙ 1 × L 2 ,
(3.19)

uniformly in bounded sets. Then from Theorem 3.1, (3.18), and the compactness of { S k 1 (t)|t0}, for the system (1.1) there exists a global attractor A in H ˙ 1 × L 2 .  □

Remark 3.2 It is easy to see that the semigroup

S k (t)= S k 1 (t)+ S k 2 (t): ( u 0 , v 0 = u 1 + k u 0 ) T ( u ( t ) , u t ( t ) + k u ( t ) ) T ,EE,

defined by (2.12) has the following relation with S(t):

S k (t)= R k S(t) R k ,
(3.20)

where R k is an isomorphism of E:

R k :{u, u t }{u, u t +ku}.

Since the semigroup { S k (t)|t0} defined by (1.1) possesses a global attractor A 0 E, by (3.19), {S(t)|t0} also possesses a global attractor A= R k A 0 .

4 Regularity of the attractor

In this section, we suppose that g L ˙ 2 and prove that the attractor is compact in H 2 × H 1 . Let ( u 0 , v 0 ) H ˙ 1 × L 2 . We set

S k (t)( u 0 , v 0 )= ( p ( t ) , q ( t ) ) + ( w ( t ) , ρ ( t ) ) ,t0,
(4.1)

where (p,q) is the solution of

{ p t + k p q = 0 , q t + A 1 p k ( α A 1 k ) p + ( α A 1 k ) q + h 1 ( q k p ) + f ( u ) λ u = g , p ( 0 ) = 0 , q ( 0 ) = 0 ,
(4.2)

(w,ρ) satisfies

{ w t + k w ρ = 0 , ρ t + A 1 w k ( α A 1 k ) w + ( α A 1 k ) ρ + h 1 ( v k u ) h 1 ( q k p ) = 0 , w ( 0 ) = u 0 , ρ ( 0 ) = v 0 .
(4.3)

We use Remark 3.1 to prove that A H 2 × H 1 . Let ( u 0 , v 0 )A. Let ( u 0 n , v 0 n )B and a sequence of a real numbers t n as n, such that

S k ( t n ) ( u 0 n , v 0 n ) ( u 0 , v 0 )in  H ˙ 1 × L 2  as n.
(4.4)

We also have

S k ( t n ) ( u 0 n , v 0 n ) = ( p n ( t n ) , q n ( t n ) ) + ( w n ( t n ) , ρ n ( t n ) ) ,nN.
(4.5)

We deduce from (3.12) and (3.20) that

( p n ( t n ) , q n ( t n ) ) H 2 × H 1 2 1 ρ ϱ C 3 ( | A 1 1 2 g ϵ | , λ , α , δ , κ , k , β 1 , β 2 )
(4.6)

and

( w n ( t n ) , ρ n ( t n ) ) H ˙ 1 × L 2 2 ( u 0 , v 0 ) H 1 × L 2 2 exp(2σ t n ).
(4.7)

From (4.6), we infer that there exist subsequences t n and ( u 0 n , v 0 n ), and ( p 0 , q 0 ) H 2 × H 1 such that

( p n ( t n ) , q n ( t n ) ) ( p 0 , q 0 ) weakly in  H 2 × H 1 .
(4.8)

From (4.4), (4.5), and (4.7), we have

( p n ( t n ) , q n ( t n ) ) ( u 0 , v 0 )in  H 1 × L 2 .
(4.9)

We conclude that ( u 0 , v 0 )=( p 0 , q 0 ) and then

A H 2 × H 1 .
(4.10)

In the following, we use the famous argument of [5] to show that the attractor A is actually a compact set in H 2 × H 1 .

Theorem 4.1 The semigroup {S(t)|t0} in H ˙ 1 × L 2 possesses a global attractor A which is compact subset of H 2 × H 1 .

Proof Multiplying (1.1) by ( A 1 u, A 1 v), we have

1 2 d d t [ μ A 1 1 2 u 2 + | A 1 1 2 v | 2 ] + σ ( μ A 1 1 2 u 2 + | A 1 1 2 v | 2 ) + α λ + β 1 2 | A 1 1 2 v | 2 = ( g , A 1 v ) ( f ( u ) λ u , A 1 v ) .
(4.11)

We put G(u,v)=μ A 1 1 2 u 2 + | A 1 1 2 v | 2 , K(u,v)= Ω [ A 1 1 2 g A 1 1 2 v(f(u)λu) A 1 v]dx α λ + β 1 2 | A 1 1 2 v | 2 , then we have

1 2 d d t G(u,v)+σG(u,v)=K(u,v),
(4.12)

this shows that

G(u,v)= e 2 σ t G( u 0 , v 0 )+2 0 t e 2 σ ( s t ) K(u,v)ds.
(4.13)

We consider a sequence ( a n , b n ) n N A, and we may assume that, up to a subsequence,

( a n , b n ) ( a , b ) weakly in  H 2 × H 1 , ( a n , b n ) ( a , b ) strongly in  H 1 × L 2 .

We want to prove the strong convergence of ( a n , b n ) in H 2 × H 1 ; this will give the compactness of A in H 2 × H 1 .

For a given T0 and up to subsequence extraction, we may assume that a.e. in t[0,T],

S ( t T ) ( a n , b n ) S ( t T ) ( a , b ) weakly in  H 2 × H 1 , S ( t T ) ( a n , b n ) S ( t T ) ( a , b ) strongly in  H 1 × L 2 .

Using (4.13) for ( u 0 , v 0 )=S(T)( a n , b n ), we have

G ( S ( t T ) ( a n , b n ) ) = e 2 σ t G ( S ( T ) ( a n , b n ) ) + 2 0 t e 2 σ ( s t ) K ( S ( s T ) ( a n , b n ) ) d s .
(4.14)

By the Lebesgue dominated convergence theorem, similar to (3.8)-(3.12), we have

0 t e 2 σ ( s t ) K ( S ( s T ) ( a n , b n ) ) ds 0 t e 2 σ ( s t ) K ( S ( s T ) ( a , b ) ) ds,
(4.15)

passing to the limit sup in (4.14) and taking t=T we have

lim n G ( a n , b n ) lim n e 2 σ T G ( S ( T ) ( a n , b n ) ) + 2 0 T e 2 σ ( s T ) K ( S ( s T ) ( a , b ) ) d s .
(4.16)

The last term of (4.16) follows from (4.14) for ( u 0 , v 0 )=S(T)(a,b) and t=T, and we have

I=2 0 T e 2 σ ( s T ) K ( S ( s T ) ( a , b ) ) ds=G(a,b) e 2 σ T G ( S ( T ) ( a , b ) ) .
(4.17)

We replace I in (4.16), we obtain

lim n G( a n , b n )G(a,b) e 2 σ T ( G ( S ( T ) ( a , b ) ) lim n G ( S ( T ) ( a n , b n ) ) ) .
(4.18)

It is a standard matter to prove

e 2 σ T ( G ( S ( T ) ( a , b ) ) lim n G ( S ( T ) ( a n , b n ) ) ) 0when T.
(4.19)

It follows from (4.18) that

lim n G( a n , b n )G(a,b) lim _ n G( a n , b n ).
(4.20)

This completes the proof of lemma. □