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Article

Global Existence and Decay Estimates for a Viscoelastic Petrovsky–Kirchhoff-Type Equation with a Delay Term

by
Noureddine Sebih
1,†,
Abdelhamid Mohammed Djaouti
2,*,†,
Chafi Boudekhil
1,† and
Ashraf Al-Quran
2,†
1
Department of Mathematics, University Djilali Liabes of Sidi-Bel-Abbes, Sidi Bel Abbes 22000, Algeria
2
Department of Mathematics and Statistics, Faculty of Sciences, King Faisal University, Hofuf 31982, Saudi Arabia
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Axioms 2024, 13(12), 869; https://doi.org/10.3390/axioms13120869
Submission received: 14 October 2024 / Revised: 22 November 2024 / Accepted: 9 December 2024 / Published: 13 December 2024

Abstract

:
In this paper, we consider a viscoelastic Kirchhoff equation with a delay term in the internal feedback. By using the Faedo–Galerkin approximation method, we prove the well posedness of the global solutions. Introducing suitable energy, we prove the general uniform decay results.

1. Introduction

In this paper, we investigate the global existence and uniform decay rate of the energy for solutions to the nonlinear viscoelastic Kirchhoff problem with a delay term in the internal feedback
| u ( x , t ) | ρ u ( x , t ) + Δ 2 u ( x , t ) Δ u ( x , t ) M Ω | u ( x , t ) | 2 d x Δ u ( x , t ) 0 t h ( t s ) Δ 2 u ( x , s ) d s + μ 1 g ( u ( x , t ) ) + μ 2 g ( u ( x , t τ ) ) = 0 , x Ω , t > 0 ,
u ( x , t ) = u ( x , t ) n = 0 , x Ω , t > 0 ,
u ( x , 0 ) = u 0 ( x ) , u ( x , 0 ) = u 1 ( x ) , x Ω ,
u ( x , t τ ) = f 0 ( x , t τ ) , x Ω , t ( 0 , τ ) ,
where Ω is a bounded domain in R n with smooth boundary Ω ; n represents the outward normal derivative on Ω ; ρ , μ 1 , and μ 2 are three positive real numbers; M C 1 ( R + ) ; h is a positive non-increasing function defined on R + which represents the kernel of the memory term; and g is an odd non-decreasing function of the class C 1 ( R ) which represents the internal feedback.
In the absence of the delay term, many authors have investigated problem (1) and proved the stability, instability, and the exponential decaying energy of the system under suitable assumptions; see, for example, [1,2,3,4,5,6]. In paper [1], the authors considered a related problem with strong damping. Liu and Zuazua in [7] investigated the decay rates for dissipative wave equations
u ( x , t ) Δ u ( x , t ) + g ( u ( x , t ) ) = 0 ,
where the authors proved the global existence of solutions and established asymptotic behavior.
| u ( x , t ) | ρ u ( x , t ) Δ u ( x , t ) Δ u ( x , t ) 0 t h ( t s ) Δ u ( x , s ) d s γ Δ u t ( x , t ) = 0 .
They obtained the global existence result for γ > 0 and the uniform exponential decay of the energy for γ > 0 . Lately, the decay result has been extended by [5] to the case γ = 0 .
Messaoudi and Tatar in [4] studied the following problem:
| u ( x , t ) | ρ u ( x , t ) Δ u ( x , t ) Δ u ( x , t ) 0 t h ( t s ) Δ u ( x , s ) d s = b | u ( x , t ) | p 2 u ( x , t ) .
By introducing a new functional and using a potential well method, they obtained the global existence of solutions and the uniform decay of the energy, where the initial data are stable in a suitable set. In paper [8], Alabau-Boussouira, Cannarsa and Sforza studied the general second order integrodifferential evolution equations with semilinear source terms
u ( x , t ) + A u ( x , t ) 0 t β ( t s ) A u ( x , s ) d s = F ( u ( x , t ) ) .
The authors obtained the global well-posedness of the IBVP to the equation and established the decay property of energy. Han and Wang proved in [3] the global existence and the uniform decay for the following nonlinear viscoelastic equation with damping:
| u ( x , t ) | ρ u ( x , t ) Δ u ( x , t ) Δ u ( x , t ) 0 t h ( t s ) Δ u ( x , s ) d s + u ( x , t ) = 0 .
Wu in [9] proved semilar results of [3] with the nonlinear damping conditions. On the other hand, for ρ = 0 , Peyravi [10] investigated the initial boundary value problem for a nonlinear viscoelastic Petrovsky wave equation
u t t ( x , t ) + Δ 2 u ( x , t ) 0 t g ( t s ) Δ 2 u ( x , s ) d s Δ u t ( x , t ) Δ u t t ( x , t ) + | u t ( x , t ) | m 1 u t ( x , t ) = | u ( x , t ) | p 1 u ( x , t ) .
Also, the author established the general decay result and the global existence of the solutions. In a recent work [11], Zhang and Ouyang looked into the following nonlinear viscoelastic equation with nonlinear damping and source term
| u t ( x , t ) | ρ u t t ( x , t ) Δ u ( x , t ) + α | u t ( x , t ) | p 2 u t ( x , t ) + 0 t g ( t s ) Δ u ( x , s ) d s = | u ( x , t ) | q 2 u ( x , t ) .
They obtained the global existence and optimal decay as well as the blow-up result. It is well known that delay effects often arise in many practical problems because these phenomena depend not only on the present state but also on the past history of the system. In recent years, the behavior of solutions for PDEs with time delay effects has become an active area of research; see [12,13,14,15,16,17] and the references therein. Datko proved in [12] that a small delay in a boundary control is a source of instability. To stabilize a system involving delay terms, additional control terms will be necessary. In [14], Nicaise and Pignotti considered the following wave equation with a linear damping and delay term inside the domain
u t t ( x , t ) Δ u ( x , t ) + μ 1 u t ( x , t ) + μ 2 u t ( x , t τ ) = 0 .
The stability was proved in the case 0 < μ 1 < μ 2 . Later, this result was extended by Benaissa and Louhibi [18] to the case where the source term and delay term are nonlinear. Kirane and Said Houari in [19] investigated the following linear viscoelastic wave equation with a linear damping and delay term:
u t t ( x , t ) Δ u ( x , t ) + 0 t g ( t s ) Δ u ( x , s ) d s + μ 1 u t ( x , t ) + μ 2 u t ( x , t τ ) = 0 .
They showed that its energy was exponentially decaying when 0 < μ 2 < μ 1 . In [20], the authors studied the results of [19] with a delay term in the non-linear internal feedback. They proved the global existence and uniform decay rates for the energy provided that the relaxation function decays exponentially. For the plate equation with a time delay term, Park considered in [16] the problem
u t t ( x , t ) + Δ 2 u ( x , t ) M ( u ( t ) 2 ) Δ u ( x , t ) + σ ( t ) 0 t g ( t s ) Δ u ( x , s ) d s + a 0 u t ( x , t ) + a 1 u t ( x , t τ ) = 0 ,
which can be considered an extensive weak viscoelastic plate equation with a linear time delay term. The author obtained a general decay result of energy by using suitable energy and Lyapunov functionals. Yang in [17] studied the initial boundary value problem of the Euler–Bernoulli viscoelastic equation with a delay term in the internal feedback
u t t ( x , t ) + Δ 2 u ( x , t ) 0 t g ( t s ) Δ 2 u ( x , s ) d s + μ 1 u t ( x , t ) + μ 2 u t ( x , t τ ) = 0 .
A global existence and uniform decay rates for the energy were proved. Recently, ref. [13] showed the energy decay of solutions for the following nonlinear viscoelastic equation with a time delay term in the internal feedback
u t t ( x , t ) + Δ 2 u ( x , t ) d i v F ( u ( x , t ) ) σ ( t ) 0 t g ( t s ) Δ 2 u ( x , s ) d s + μ 1 | u t ( x , t ) | m 1 u t ( x , t ) + μ 2 | u t ( x , t τ ) | m 1 u t ( x , t τ ) = 0 .
Motivated by the above work, we intend to study the global existence of weak solutions and to prove the uniform exponential decay of energy for problem (1)–(4). To our knowledge, the global existence and exponential rate of energy decay for system (1)–(4) have not been studied. The main contributions of this paper are the following:
  • We proved the global existence of weak solutions by using Lemma 1, Lemma 2, and the Faedo–Galerkin method.
  • To obtain the exponential decay estimates, we used a perturbed energy method.
Our paper is organized as follows. In Section 2, we present the assumptions and main results. In Section 3, we prove our main results.

2. Assumptions and Main Result

Let us consider the Hilbert space L 2 ( Ω ) endowed with the inner product ( , ) and the corresponding norm · 2 . We also consider the Sobolev space H 0 2 ( Ω ) endowed with the scalar product
( u , v ) H 0 2 ( Ω ) = ( Δ u , Δ v ) ,
and Δ u = i = 1 i = n 2 u 2 x i .
We define for all 1 p < , . p the L p ( Ω ) norm where
u p p = Ω | u ( x ) | p d x .
In particular, we write . instead of . 2 when p = 2 .
We introduce as in [14] a new variable
z ( x , ϱ , t ) = u t ( x , t τ ϱ ) , x Ω , ϱ ( 0 , 1 ) , t > 0 .
Then, we have
τ z t ( x , ϱ , t ) + z ϱ ( x , ϱ , t ) = 0 .
Therefore, problem (1)–(4) is equivalent to
| u ( x , t ) | ρ u ( x , t ) + Δ 2 u ( x , t ) Δ u ( x , t ) M ( u 2 ) Δ u ( x , t ) 0 t h ( t s ) Δ 2 u ( x , s ) d s + μ 1 g ( u ( x , t ) ) + μ 2 g ( z ( x , 1 , t ) ) = 0 ,
τ z t ( x , ϱ , t ) + z ϱ ( x , ϱ , t ) = 0 , x Ω , ϱ ( 0 , 1 ) , t > 0 ,
z ( x , 0 , t ) = u ( x , t ) , x Ω , t > 0 ,
u ( x , t ) = u ( x , t ) n = 0 , x Ω , t > 0 ,
u ( x , 0 ) = u 0 ( x ) , u ( x , 0 ) = u 1 ( x ) , x Ω ,
z ( x , ϱ , 0 ) = f 0 ( x , ϱ τ ) , x Ω , ϱ ( 0 , 1 ) .
To state and prove our result, we assume the following hypothesis:
(A1)
Assume that ρ satisfies
0 < ρ 2 n 2 if n 3 , 0 < ρ < if n = 1 , 2 .
(A2)
Assume that M C 1 ( R + ) satisfies
m 0 > 0 , M ( λ ) m 0 , λ 0 . γ , δ , M ( λ ) δ λ γ , λ 0 . α , β , | M ( λ ) | β λ α , λ 0 .
(A3)
The kernel function h : R + ( 0 , + ) is a bounded C 1 function such that
1 0 h ( s ) d s = β 1 > 0 ,
and we assume that there exists a positive constant ζ satisfying
h ( t ) ζ h ( t ) , t 0 .
(A4)
g : R R is an odd non-decreasing function of class C 1 such that there exist c 1 , α 1 , and α 2 positive constants, satisfying
| g ( s ) | c 1 , s R , α 1 s g ( s ) G ( s ) α 2 s g ( s ) , s R ,
where G ( s ) = 0 s g ( t ) d t , lim s + g ( s ) = + and α 2 μ 2 α 1 μ 1 .
First, we state some lemmas which will be used in the next sections.
Lemma 1
([2]). For h C 1 ( [ 0 , + ) , R ) and φ C 1 ( 0 , T ; L 2 ( Ω ) ) , we have
Ω 0 t h ( t s ) φ ( x , s ) φ ( x , t ) d s d x = 1 2 h ( t ) φ ( t ) 2 + 1 2 ( h φ ) ( t ) + 1 d 2 d t 0 t h ( s ) d s φ ( t ) 2 ( h φ ) ( t ) ,
where ( h φ ) ( t ) = 0 t h ( t s ) φ ( s ) φ ( t ) 2 d s .
Remark 1.
For φ ( x , t ) , a function defined on ( 0 , T ) with values in a space L 2 ( Ω ) , the space of functions depends only on x.When we write just φ ( t ) , we mean that φ ( t ) is an element of L 2 ( Ω ) , namely, the function x φ ( x , t ) . We note that φ ( x , t ) = d φ ( x , t ) d t , | φ ( x , t ) | is the absolute value of φ ( x , t ) , and
| | φ ( t ) | | = Ω | φ ( x , t ) | 2 d x 1 2 .
Lemma 2
([21]). Let Φ be a convex function of class C 1 ( R ) . The Legendre transformation of Φ is defined as follows
Φ * ( s ) = sup t R ( s t Φ ( t ) ) .
If Φ is an odd and lim s + Φ ( s ) = + , then
Φ * ( s ) = s ( Φ ) 1 ( s ) Φ ( Φ ) 1 ( s ) , s R ,
and satisfies the inequality
s t Φ * ( s ) + Φ ( t ) , s , t R .
The energy associated with problem (5)–(10) is given by
E ( t ) = 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + 1 2 Δ u ( t ) 2 2 + 1 2 u ( t ) 2 + 1 2 M ^ ( u ( t ) 2 ) 1 2 0 t h ( s ) d s Δ u ( t ) 2 + 1 2 ( h Δ u ) ( t ) + ξ Ω 0 1 G ( z ( x , ϱ , t ) ) d ϱ d x ,
where M ^ ( λ ) = 0 λ M ( t ) d t and ξ is a positive constant such that
τ μ 2 ( 1 α 1 ) α 1 < ξ < τ μ 1 α 2 μ 2 α 2 .
Remark 2.
If ρ satisfies hypotheses (A1), then we have the embedding H 0 1 ( Ω ) L 2 ( ρ + 1 ) ( Ω ) and H 0 2 ( Ω ) H 0 1 ( Ω ) . By the Poincaré inequality, we have the Sobolev embedding inequality
u 2 ( ρ + 1 ) C s 1 u , u C s 2 Δ u , u C s 3 Δ u , for u H 0 2 ( Ω ) ,
where C s 1 , C s 2 , a n d C s 3 are embedding constants. In what follows, we use C s to denote a generic embedding constant, and C i ( i N ) represent different positive constants.
From hypothesis (A3), the energy associate in ( 11 ) is positive. Moreover, the kernel of the memory function h also decays exponentially. The assumption in (A4) for the function g is a sufficient condition to guarantee the global existence and exponential decay of energy for problem (1)–(4). Finally, the hypothesis of positive constant ξ in ( 11 ) implies that θ 1 > 0 and θ 2 > 0 .
Theorem 1.
Let u 0 H 0 2 ( Ω ) H 3 ( Ω ) , u 1 H 0 2 ( Ω ) and f 0 H 0 1 ( Ω , H 1 ( 0 , 1 ) ) satisfy the compatibility condition f ( · , 0 ) = u 1 . Assume that(A1)–(A4)hold. Then, (5)–(10) admits a weak solution
u L ( [ 0 , ) ; H 0 2 ( Ω ) H 3 ( Ω ) ) , u L ( [ 0 , ) ; H 0 2 ( Ω ) ) , u L 2 ( [ 0 , ) ; H 0 1 ( Ω ) ) .
z L ( [ 0 , ) ; H 0 1 ( Ω × ( 0 , 1 ) ) ) , z L ( [ 0 , ) ; L 2 ( Ω × ( 0 , 1 ) ) ) ,
G ( z ( x , ϱ , t ) ) L ( [ 0 , ) ; L 1 ( Ω × ( 0 , 1 ) ) ) .
Moreover, if E ( 0 ) is positive and bounded, then for every t 0 > 0 , there exist positive constants k and K such that the energy defined by Lemma 1 possesses the following decay:
E ( t ) K e k t , t t 0 .

3. Proof of the Main Result

We will divide the proof into two steps: in the first step, we will use the Faedo–Galerkin method to prove the existence of global solutions, where the second step is devoted to proving the uniform decay of the energy by the perturbed energy method.
  • Step 1. Existence of weak solutions.
Let T > 0 be fixed and let ( w i ) i N * be an orthogonal basis of H 3 ( Ω ) H 0 2 ( Ω ) , with w i being the eigenfunctions of the bi-Laplacian operator subject to the boundary condition
Δ 2 w i = λ i w i , in Ω , w i = w i n = 0 , in Ω .
By the linear elliptic operator theory described in [22], we have w j H m ( Ω ) H 0 2 ( Ω ) , m N . Now, we denote by W k = span { w 1 , w 2 , . . . , w k } the subspace generated by the first k vectors of the basis ( w i ) i N * . By normalization, we obtain w i = 1 . Now, we define for 1 i k the sequence as follows: φ i ( x , 0 ) = w i ( x ) . Then, we may extend φ i ( x , 0 ) by φ i ( x , ϱ ) over L 2 ( Ω × ( 0 , 1 ) ) and denote Z k as the space generated by φ 1 , . . . , φ k . For any given integer k, we consider the approximate solution ( u k , z k )
u k ( x , t ) = i = 1 k g i k ( t ) w i ( x ) , z k ( x , ϱ , t ) = i = 1 k h i k ( t ) φ i ( x , ϱ ) ,
which satisfies
( | u k ( t ) | ρ u k ( t ) , w i ) + ( Δ u k ( t ) , Δ w i ) + ( u k ( t ) , w i ) + M ( u k ( t ) 2 ) ( u k ( t ) , w i ) 0 t h ( t s ) ( Δ u k ( s ) , Δ w i ) d s + μ 1 ( g ( u k ( t ) ) , w i ) + μ 2 ( g ( z k ( . , 1 , t ) ) , w i ) = 0 , z k ( x , 0 , t ) = u k ( x , t ) ,
( τ z k t ( ϱ , t ) + z k ϱ ( ϱ , t ) , φ i ( ϱ ) ) L 2 ( Ω ) = 0 ,
u k ( 0 ) = u 0 k , u k ( 0 ) = u 1 k , z k ( 0 ) = z 0 k ,
where i = 1 , k ¯
u 0 k = i = 1 k ( u 0 , w i ) w i , u 1 k = i = 1 k ( u 1 , w i ) w i , z 0 k = i = 1 k ( f 0 , φ i ) L 2 ( Ω × ( 0 , 1 ) ) φ i ,
and for k +
u 0 k u 0 in H 0 2 ( Ω ) H 3 ( Ω ) , u 1 k u 1 in H 0 2 ( Ω ) , z 0 k f 0 in H 0 1 ( Ω , H 1 ( 0 , 1 ) ) .
Taking account of assumption (A1), H 0 1 ( Ω ) L 2 ( ρ + 1 ) ( Ω ) , then u k ( t ) L 2 ( ρ + 1 ) ( Ω ) , | u k ( t ) | ρ L 2 ( ρ + 1 ) ρ ( Ω ) and w i L 2 ( Ω ) , from the generalized Hölder inequality, the nonlinear term in (13)
( | u k ( t ) | ρ u k ( t ) , w i ) = Ω | u k ( x , t ) | ρ u k ( x , t ) w i ( x ) d x u k ( t ) 2 ( ρ + 1 ) ρ u k ( t ) 2 ( ρ + 1 ) w i ,
makes sense. According to the standard of ordinary differential equations theory, the finite dimensional problem (13)–(15) has a solution ( g i k , h i k ) defined on [ 0 , t k ) . Then, we can obtain an approximate solution u k and z k of (13)–(15) in W k and Z k , respectively, over [ 0 , t k ) . Moreover, the solution can be extended to [ 0 , T ] for any given T by the first estimates below. Now, we derive the first estimate. Multiplying (13) by g i k ( t ) and summing with respect to i, we conclude that
d d t 1 ρ + 2 u k ( t ) ρ + 2 ρ + 2 + 1 2 Δ u k ( t ) 2 + 1 2 u k ( t ) 2 + 1 2 M ^ ( u k ( t ) 2 ) 0 t h ( t s ) ( Δ u k ( s ) , Δ u k ( t ) ) d s + μ 1 Ω u k ( x , t ) g ( u k ( x , t ) ) d x + μ 2 Ω u k ( x , t ) g ( z k ( x , 1 , t ) ) d x = 0 .
Applying Lemma 1 with φ = Δ u k , (17) become
d d t [ 1 ρ + 2 u k ( t ) ρ + 2 ρ + 2 + 1 2 Δ u k ( t ) 2 + 1 2 u k ( t ) 2 + 1 2 M ^ ( u k ( t ) 2 ) 1 2 0 t h ( s ) d s Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) ] = μ 1 Ω u k ( x , t ) g ( u k ( x , t ) ) d x μ 2 Ω u k ( x , t ) g ( z k ( x , 1 , t ) ) d x 1 2 h ( t ) Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) .
We multiply Equation (14) by ξ g ( z ( x , ϱ , t ) ) and integrate over Ω × ( 0 , 1 ) , and we obtain
ξ Ω 0 1 z k t ( x , ϱ , t ) g ( z k ( x , ϱ , t ) ) d ϱ d x = ξ τ Ω 0 1 z k ϱ ( x , ϱ , t ) g ( z k ( x , ϱ , t ) ) d ρ d x = ξ τ Ω 0 1 ϱ G ( z k ( x , ϱ , t ) ) d ϱ d x .
Hence,
ξ d d t Ω 0 1 G ( z k ( x , ϱ , t ) ) d ϱ d x = ξ τ Ω G ( z k ( x , 1 , t ) ) d x + ξ τ Ω G ( u k ( x , t ) ) d x .
Combining (18) and (19), we obtain
E k ( t ) = μ 1 Ω u k ( x , t ) g ( u k ( x , t ) ) d x μ 2 Ω u k ( x , t ) g ( z k ( x , 1 , t ) ) d x 1 2 h ( t ) Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) ξ τ Ω G ( z k ( x , 1 , t ) ) d x + ξ τ Ω G ( u k ( x , t ) ) d x .
From assumption (A4), we know that G is a convex function of class C 2 , G = g is an odd and lim s + G ( s ) = + , then by Lemma 2, we deduce
G * ( s ) = s g 1 ( s ) G ( g 1 ( s ) ) , s R .
Applying these equalities with s = g ( z k ( x , 1 , t ) ) , we obtain
G * ( g ( z k ( x , 1 , t ) ) ) = z k ( x , 1 , t ) g ( z k ( x , 1 , t ) ) G ( z k ( x , 1 , t ) ) .
By using inequality in Lemma 2 together with (A4) for s = g ( z k ( x , 1 , t ) ) , t = u k ( x , t ) , G is an even function, and we obtain
u k ( x , t ) g ( z k ( x , 1 , t ) ) G * ( g ( z k ( x , 1 , t ) ) ) + G ( u k ( x , t ) ) = z k ( x , 1 , t ) g ( z k ( x , 1 , t ) ) G ( z k ( x , 1 , t ) ) + G ( u k ( x , t ) ) ( 1 α 1 ) z k ( x , 1 , t ) g ( z k ( x , 1 , t ) ) + α 2 u k g ( u k ) .
From (20), (21) and assumption (A4), we have
E k ( t ) 1 2 h ( t ) Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) μ 1 ξ α 2 τ μ 2 α 2 Ω u k ( x , t ) g ( u k ( x , t ) ) d x ξ α 1 τ μ 2 + μ 2 α 1 Ω z k ( x , 1 , t ) g ( z k ( x , 1 , t ) ) d x .
Integrating (22) over ( 0 , t ) and using assumption (A3), we conclude that
E k ( t ) + θ 1 0 t Ω u k ( x , t ) g ( u k ( x , t ) ) d x + θ 2 0 t Ω z k ( x , 1 , t ) g ( z k ( x , 1 , t ) ) d x C 1 ,
where
θ 1 = μ 1 ξ α 2 τ μ 2 α 2 , θ 2 = ξ α 1 τ μ 2 + μ 2 α 1 ,
and C 1 is a positive constant depending only on u 0 H 0 2 ( Ω ) , u 1 H 0 1 ( Ω ) and f 0 L 2 ( Ω × ( 0 , 1 ) ) . Noting (A2), (A3), and (23), we obtain the first estimate
u k ( t ) ρ + 2 ρ + 2 + Δ u k ( t ) 2 + u k ( t ) 2 + u k ( t ) 2 + ( h Δ u k ) ( t ) + ξ Ω 0 1 G ( z k ( x , ϱ , t ) ) d ϱ d x + 0 t Ω u k ( x , s ) g ( u k ( x , s ) ) d x d s + 0 t Ω z k ( x , 1 , s ) g ( z k ( x , 1 , s ) ) d x d s C 2 ,
where C 2 is a positive constant depending only on u 0 H 0 2 ( Ω ) , u 1 H 0 1 ( Ω ) , f 0 L 2 ( Ω × ( 0 , 1 ) ) , m 0 , β 1 , ξ , τ , θ 1 and θ 2 .
It follows from (24) that
u k is uniformly bounded in L ( 0 , T ; H 0 2 ( Ω ) ) ; u k is uniformly bounded in L ( 0 , T ; H 0 1 ( Ω ) ) ; G ( z k ( x , ρ , t ) ) is uniformly bounded in L ( 0 , T ; L 1 ( Ω × ( 0 , 1 ) ) ) ; u k g ( u k ) is uniformly bounded in L 1 ( Ω × ( 0 , T ) ) ; z k ( . , 1 , . ) g ( z k ( . , 1 , . ) ) is uniformly bounded in L 1 ( Ω × ( 0 , T ) ) ) .
Then, we derive the second estimate. Substituting w i by Δ w i in (13), multiplying by g i k and then summing with respect to i, it holds that
1 2 d d t Δ u k ( t ) 2 + Δ u k ( t ) 2 Ω | u k ( x , t ) | ρ u k ( x , t ) Δ u k ( x , t ) d x + μ 1 Ω | u k ( x , t ) | 2 g ( u k ( x , t ) ) d x + μ 2 Ω g ( z k ( x , 1 , t ) ) u k ( x , t ) z k ( x , 1 , t ) d x 0 t h ( t s ) Ω Δ u k ( x , s ) Δ u k ( x , t ) d x d s + Ω M ( u k ( t ) 2 ) Δ u k ( x , t ) Δ u k ( x , t ) d x = 0 .
Using Lemma 1 with φ = Δ u k , we have
1 2 d d t 1 0 t h ( s ) d s Δ u k ( t ) 2 + Δ u k ( t ) 2 + M ( u k ( t ) 2 ) Δ u k ( t ) 2 + h Δ u k ( t ) Ω | u k ( x , t ) | ρ u k ( x , t ) Δ u k ( x , t ) d x M ( u k ( t ) 2 ) Δ u k ( t ) 2 ( u k ( t ) , u k ( t ) ) + μ 1 Ω | u k ( x , t ) | 2 g ( u k ( x , t ) ) d x + μ 2 Ω g ( z k ( x , 1 , t ) ) u k z k ( x , 1 , t ) d x = 1 2 h ( t ) Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) .
Substituting φ i by Δ φ i in (14), multiplying by h i k , summing with respect to i, and integrating over ϱ ( 0 , 1 ) , it follows that
τ 2 d d t z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + 1 2 z k ( . , 1 , t ) 2 1 2 u k ( t ) 2 = 0 .
Using Green’s formula, we obtain
Ω | u k ( x , t ) | ρ u k ( x , t ) Δ u k ( x , t ) d x = d d t Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x
Ω | u k ( x , t ) | ρ u k ( x , t ) u k ( x , t ) d x .
Combining (25)–(27), we obtain
1 2 d d t [ 1 0 t h ( s ) d s Δ u k ( t ) 2 + Δ u k ( t ) 2 + M ( u k ( t ) 2 ) Δ u k ( t ) 2 + h Δ u k ( t ) + 2 Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + τ z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 ] + 1 2 z k ( . , 1 , t ) 2 + μ 1 Ω | u k ( x , t ) | 2 g ( u k ( x , t ) ) d x = Ω | u k ( x , t ) | ρ u k ( x , t ) u k ( x , t ) d x μ 2 Ω g ( z k ( x , 1 , t ) ) u k z k ( x , 1 , t ) d x + 1 2 u k ( t ) 2 + M ( u k ( t ) 2 ) Δ u k ( t ) 2 ( u k ( t ) , u k ( t ) ) 1 2 h ( t ) Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) .
From Young’s inequality, we have, for all η > 0 , that
a b η a 2 + b 2 4 η , where a , b ( 0 , + ) .
With assumption (A2) and (24), and using Young’s inequality with η = 1 / 2 , we obtain
M ( u k ( t ) 2 ) Δ u k ( t ) 2 ( u k ( t ) , u k ( t ) ) M ( u k ( t ) 2 ) Δ u k ( t ) 2 u k u k ( t ) 1 2 M ( u k ( t ) 2 ) 2 Δ u k ( t ) 4 u k ( t ) 2 + 1 2 u k ( t ) 2 1 2 β 2 u k ( t ) 4 α + 2 Δ u k ( t ) 4 + C 2 2 β 2 C 2 2 α + 3 + C 2 2 .
From the generalized Hölder inequality and Sobolev embedding theorem H 0 2 ( Ω ) H 0 1 ( Ω ) L 2 ( ρ + 1 ) ( Ω ) , we obtain
Ω | u k ( x , t ) | ρ u k ( x , t ) u k ( x , t ) d x u k ( t ) 2 ( ρ + 1 ) ρ u k ( t ) 2 ( ρ + 1 ) u k ( t ) C s ρ + 1 u k ( t ) ρ Δ u k ( t ) u k ( t ) .
From Young’s inequality and (24), we deduce
Ω | u k ( x , t ) | ρ u k ( x , t ) u k ( x , t ) d x η u k ( t ) 2 + C s 2 ( ρ + 1 ) C 2 ρ 4 η Δ u k ( t ) 2 .
Similarly, Young’s inequality and assumption (A4) lead to
μ 2 Ω u k z k ( x , 1 , t ) g ( z k ( x , 1 , t ) ) η z k ( . , 1 , t ) 2 + ( μ 2 c 1 ) 2 C 2 4 η .
Taking into account (30) in (29) yields
1 2 d d t [ 1 0 t h ( s ) d s Δ u k ( t ) 2 + Δ u k ( t ) 2 + M ( u k ( t ) 2 ) Δ u k ( t ) 2 + h ( Δ u k ) ( t ) + 2 Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + τ z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 ] + ( 1 2 η ) z k ( . , 1 , t ) 2 + μ 1 Ω | u k ( x , t ) | 2 g ( u k ( x , t ) ) d x η u k ( t ) 2 + C s 2 ( ρ + 1 ) C 2 ρ 4 η Δ u k ( t ) 2 1 2 h ( t ) Δ u k ( t ) 2 + 1 2 ( h Δ u k ) ( t ) + C 2 ( η ) .
Multiplying (13) by g i k and summing with respect to i, it holds that
Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + u k ( t ) 2 = Ω u k ( x , t ) Δ 2 u k ( x , t ) d x + 0 t h ( t s ) Ω Δ u k ( x , s ) Δ u k ( x , t ) d x d s Ω M ( u k ( t ) 2 ) u k ( x , t ) u k ( x , t ) d x μ 1 Ω u k ( x , t ) g ( u k ( x , t ) ) d x μ 2 Ω u k ( x , t ) g ( z k ( x , 1 , t ) ) d x .
Differentiating (14) with respect to t, multiplying by h i k and summing with respect to i, it follows that
τ 2 d d t z k ( ϱ , t ) 2 + 1 2 d d ϱ z k ( ϱ , t ) 2 = 0 .
Integrating (32) with respect to ϱ ( 0 , 1 ) and summing with previous equation, we obtain that
Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + u k ( t ) 2 + τ 2 d d t z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + 1 2 z k ( 1 , t ) 2 = Ω u k ( x , t ) Δ 2 u k ( x , t ) d x + 0 t h ( t s ) Ω Δ u k ( x , s ) Δ u k ( x , t ) d x d s + 1 2 u k ( t ) 2 Ω M ( u k ( t ) 2 ) u k ( x , t ) u k ( x , t ) d x μ 1 Ω u k ( x , t ) g ( u k ( x , t ) ) d x μ 2 Ω u k ( x , t ) g ( z k ( x , 1 , t ) ) d x .
In what follows, we estimate the right-hand side in (33). Using Green’s formula and Young’s inequality, we obtain
Ω u k ( x , t ) Δ 2 u k ( x , t ) d x = Ω u k ( x , t ) Δ u k ( x , t ) d x η u k ( t ) 2 + 1 4 η Δ u k ( t ) 2 .
Applying the Cauchy–Schwarz inequality and Young’s inequality, we obtain from assumption (A2) and (24) that
Ω M ( u k ( t ) 2 ) u k ( t ) u k ( t ) d x δ u k ( t ) 2 γ + 1 u k ( t ) η u k ( t ) 2 + δ 2 C 2 2 γ + 1 4 η .
Similarly, we have
0 t h ( t s ) Ω Δ u k ( x , s ) Δ u k ( x , t ) d x d s η u k ( t ) 2 + 1 4 η Ω 0 t h ( t s ) | Δ u k ( x , s ) | d s 2 d x η u k ( t ) 2 + 1 4 η Ω 0 t h ( t s ) | Δ u k ( x , s ) Δ u k ( x , t ) | + | Δ u k ( x , t ) | d s 2 d x = η u k ( t ) 2 + 1 4 η I .
Applying Hölder’s and Young’s inequalities, we obtain
| I | 0 t h ( s ) d s 2 Δ u k ( t ) 2 + Ω 0 t h ( t s ) | Δ u k ( x , s ) Δ u k ( x , t ) | d s 2 d x + 2 Ω 0 t h ( t s ) | Δ u k ( x , s ) Δ u k ( x , t ) | d s 0 t h ( t s ) | Δ k u ( x , t ) | d s d x 2 0 t h ( s ) d s 2 Δ k u ( t ) 2 + 2 Ω 0 t h ( t s ) | Δ u k ( x , s ) Δ u k ( x , t ) | d s 2 d x . 2 ( 1 β 1 ) 2 Δ k u ( t ) 2 + 2 ( 1 β 1 ) ( h Δ u k ) ( t ) ,
then, we obtain the estimation
0 t h ( t s ) Ω Δ u k ( x , s ) Δ u k ( x , t ) d x d s η u k ( t ) 2 + ( 1 β 1 ) 2 2 η Δ k u ( t ) 2 + ( 1 β 1 ) 2 η ( h Δ u k ) ( t ) .
And also by Young’s inequality and the Sobolev embedding theorem, we obtain
μ 1 Ω u k ( x , t ) g ( u k ( x , t ) ) d x η C s 2 u k ( t ) 2 + μ 1 2 4 η Ω | g ( u k ( x , t ) ) 2 d x ,
μ 2 Ω u k ( x , t ) g ( z k ( x , 1 , t ) ) d x η C s 2 u k ( t ) 2 + μ 2 2 4 η Ω | g ( z k ( x , 1 , t ) ) | 2 d x .
Taking into account (34)–(38) in (33) yields
Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + 1 3 η 2 η C s 2 C s 2 2 u k ( t ) 2 + τ 2 d d t z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + 1 2 z k ( 1 , t ) 2 2 ( 1 β 1 ) 2 + 1 4 η Δ u k ( t ) 2 + μ 1 2 4 η Ω | g ( u k ) | 2 d x + μ 2 2 4 η Ω | g ( z k ( x , 1 , t ) ) | 2 d x + δ 2 C 2 2 γ + 1 4 η + 1 β 1 2 η ( h Δ u k ) ( t ) .
Thus from (31), (39), we obtain
1 2 d d t [ 1 0 t h ( s ) d s Δ u k ( t ) 2 + Δ u k ( t ) 2 + M ( u k ( t ) 2 ) Δ u k ( t ) 2 + ( h Δ u k ) ( t ) + τ z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + 2 Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + τ z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 ] + ( 1 2 η ) z k ( 1 , t ) 2 + μ 1 Ω | u k ( x , t ) | 2 g ( u k ( x , t ) ) d x + Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + 1 4 η 2 η C s 2 C s 2 2 u k ( t ) 2 + 1 2 z k ( 1 , t ) 2 2 ( 1 β 1 ) 2 + 1 4 η Δ u k ( t ) 2 + μ 1 2 4 η Ω | g ( u k ( x , t ) ) | 2 d x + μ 2 2 4 η Ω | g ( z k ( x , 1 , t ) ) | 2 d x + C s 2 ( ρ + 1 ) C 2 ρ 4 η Δ u k ( t ) 2 + 1 β 1 2 η ( h Δ u k ) ( t ) + 1 2 ( h Δ u k ) ( t ) 1 2 h ( t ) Δ u k ( t ) 2 + δ 2 C 2 2 γ + 1 4 η + C 2 ( η ) .
Using (A4), (24), and the mean value theorem, we obtain
Q T | g ( u k ( x , t ) ) | 2 d x d s = Q T | g ( u k ( x , t ) ) g ( 0 ) | | g ( u k ( x , t ) ) | d x d s c 1 Q T g ( u k ( x , t ) ) u k ( x , t ) d x d s c 1 C 2 ,
and Q T | g ( z k ( x , 1 , s ) ) | 2 d x d s c 1 C 2 , where Q T = Ω × ( 0 , T ) .
Integrating (40) over ( 0 , T ) , using (41), (42), and (A3), it yields
1 0 t h ( s ) d s Δ u k ( t ) 2 + Δ u k ( t ) 2 + M ( u k ( t ) 2 ) Δ u k ( t ) 2 + ( h Δ u k ) ( t ) + τ z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + 2 Ω | u k ( x , t ) | ρ | u k ( x , t ) | 2 d x + τ z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + ( 1 2 η ) 0 t z k ( . , 1 , s ) 2 d s + 0 t z k ( 1 , s ) 2 d s + 2 0 t Ω | u k ( x , s ) | ρ | u k ( x , s ) | 2 d x d s + 2 8 η 4 η C s 2 C s 2 0 t u k ( s ) 2 d s + 2 μ 1 0 t Ω | u k ( x , s ) | 2 g ( u k ( x , s ) ) d x d s 2 ( 1 β 1 ) 2 + 1 2 η 0 t Δ u k ( s ) 2 d s + μ 1 2 c 1 C 2 2 η + μ 2 2 c 1 C 2 2 η + C s 2 ( ρ + 1 ) C 2 ρ 2 η 0 t Δ u k ( s ) 2 d s + ( δ 2 C 2 2 γ + 1 + 4 C 2 ( η ) ) T 2 η + 1 β 1 η 0 t ( h Δ u k ) ( s ) d s + C 3 ,
where C 3 is a positive constant depending on u 0 H 3 H 0 2 ( Ω ) , u 1 H 0 2 , and f 0 H 0 1 ( Ω × ( 0 , 1 ) ) . Taking η to be suitably small in (43) and using Gronwall’s lemma, we obtain the second estimate,
Δ u k ( t ) 2 + Δ u k ( t ) 2 + z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + z k ( t ) L 2 ( Ω × ( 0 , 1 ) ) 2 + 0 t z k ( . , 1 , s ) 2 d s + 0 t u k ( s ) 2 d s + 0 t z k ( . , 1 , s ) 2 d s C 4 ,
where C 4 is a positive constant depending on u 0 H 3 H 0 2 ( Ω ) , u 1 H 0 1 , f 0 H 0 1 ( Ω × ( 0 , 1 ) ) , ρ , g ( 0 ) , m 0 , β 1 , τ , and T. Estimate (44) implies
u k is uniformly bounded in L ( 0 , T ; H 3 ( Ω ) H 0 2 ( Ω ) ) ; u k is uniformly bounded in L ( 0 , T ; H 0 2 ( Ω ) ) ; u k is uniformly bounded in L 2 ( 0 , T ; H 0 1 ( Ω ) ) ; z k is uniformly bounded in L ( 0 , T ; L 2 ( ( 0 , 1 ) ; H 0 1 ( Ω ) ) ) ; z k is uniformly bounded in L ( 0 , T ; L 2 ( Ω × ( 0 , 1 ) ) ) ; z k ( . , 1 , . ) is uniformly bounded in L 2 ( 0 , T ; H 0 1 ( Ω ) ) ; z k ( . , 1 , . ) is uniformly bounded in L 2 ( 0 , T ; L 2 ( Ω ) ) .
By (45) and z k ϱ = τ z k , then
z k is bounded in L ( 0 , T ; H 0 1 ( Ω × ( 0 , 1 ) ) ) .
Applying the Dunford–Pettis theorem, we infer that there exists a subsequence ( u j ) of ( u k ) and u such that
u k u weakly star in L ( 0 , T ; H 3 ( Ω ) H 0 2 ( Ω ) ) ,
u k u weakly star in L ( 0 , T ; H 0 2 ( Ω ) ) ,
u k u weakly in L 2 ( 0 , T ; H 0 1 ( Ω ) ) .
By Aubin’s lemma, it follows from (46)–(48) that there exists a subsequence of u j still denoted by u j such that
u j u strongly in L 2 ( 0 , T ; H 0 2 ( Ω ) ) ,
u j u strongly in L 2 ( 0 , T ; H 0 1 ( Ω ) ) ,
which implies u j u , Δ u j Δ u and u j u almost everywhere in Ω × ( 0 , T ) . Hence,
| u j | ρ u j | u | ρ u almost everywhere in Ω × ( 0 , T ) ,
M ( u j 2 ) Δ u j M ( u 2 ) Δ u almost everywhere in Ω × ( 0 , T ) .
On the other hand, by the Sobolev embedding theorem and the first estimate, this yields
| u j | ρ u j 2 L 2 ( 0 , T ; L 2 ( Ω ) ) = 0 T u j ( t ) 2 ( ρ + 1 ) 2 ( ρ + 1 ) d t c s 2 ( ρ + 1 ) 0 T u j ( t ) 2 2 ( ρ + 1 ) d t c s 2 ( ρ + 1 ) C 2 2 ( ρ + 1 ) T .
Thus, using (A2), (24), (41), (51), (52), and the Lions lemma ([23], p 12.), we derive
| u j | ρ u j | u | ρ u weakly in L 2 ( 0 , T ; L 2 ( Ω ) ) ,
M ( u j 2 ) Δ u j M ( u 2 ) Δ u weakly in L 2 ( 0 , T ; L 2 ( Ω ) ) ,
g ( u j ) g ( u ) weakly in L 2 ( 0 , T ; L 2 ( Ω ) ) .
Similarly, by applying the Dunford–Pettis theorem, we infer that there exists a subsequence ( z j ) of ( z k ) and z such that
z j z weakly star in L ( 0 , T ; H 0 1 ( Ω × ( 0 , 1 ) ) ) ,
z j z weakly star in L ( 0 , T ; L 2 ( Ω × ( 0 , 1 ) ) ) , z j ϱ z ϱ weakly in L 2 ( 0 , T ; L 2 ( Ω × ( 0 , 1 ) ) ) ,
z j ( . , 1 , . ) is bounded in L 2 ( 0 , T ; H 0 1 ( Ω ) ) , z j ( . , 1 , . ) is bounded in L 2 ( 0 , T ; L 2 ( Ω ) ) .
By Aubin’s lemma, it follows from (53), (54), (56), and (57) that there exists a subsequence of z j still denoted by z j and subsequence of z j ( . , 1 , . ) still denoted by z j ( . 1 , . ) such that
z j z strongly in L 2 ( 0 , T ; L 2 ( Ω × ( 0 , 1 ) ) ) ,
z j ( . , 1 , . ) z ( . , 1 , . ) strongly in L 2 ( 0 , T ; L 2 ( Ω ) ) .
Also by (42), (59), and Lion’s lemma, then
g ( z j ( . , 1 , . ) ) g ( z ( . , 1 , . ) ) weakly in L 2 ( 0 , T ; L 2 ( Ω ) ) .
Let D ( 0 , T ) be the space of C functions with compact support in ( 0 , T ) . Multiplying (13) and (14) by θ D ( 0 , T ) and integrating over ( 0 , T ) , it follows that
1 ρ + 1 0 T ( u k ( t ) ρ u k ( t ) , w i ) θ ( t ) d t + 0 T ( Δ u k ( t ) , Δ w i ) θ ( t ) d t + 0 T ( u k ( t ) , w i ) θ ( t ) d t + 0 T M ( u k ( t ) 2 ) ( u k ( t ) , w i ) θ ( t ) d t + 0 T 0 t h ( t s ) ( Δ u k ( t ) , w i ) θ ( t ) d s d t + μ 1 0 T ( g ( u k ( t ) ) , w i ) θ ( t ) d t + μ 2 0 T ( g ( z k ( . , 1 , t ) ) , w i ) θ ( t ) d t = 0 ,
and
τ 0 T ( z k , φ i ) L 2 ( Ω × ( 0 , 1 ) ) θ ( t ) d t + 0 T ( z k ϱ , φ i ) L 2 ( Ω × ( 0 , 1 ) ) θ ( t ) d t = 0 .
Noting that { w i } i = 1 is the basis of H 3 ( Ω ) H 0 2 ( Ω ) and { φ i } i = 1 is the basis of L 2 ( Ω × ( 0 , 1 ) ) , we can pass to the limit in (60) and (61) and obtain
| u | ρ u + Δ 2 u Δ u M ( u 2 ) Δ u 0 t h ( t s ) Δ 2 u ( s ) d s + μ 1 g ( u ) + μ 2 g ( z ( . , 1 , . ) ) = 0 , in L 2 ( 0 , T ; H 1 ( Ω ) ) ,
τ z + z ϱ = 0 , in L 2 ( 0 , T ; L 2 ( Ω × ( 0 , 1 ) ) ) ,
for arbitrary T > 0 . From (46), (47), (57), (58), and Lemma 3.3.7 in [22], we conclude u j ( 0 ) u ( 0 ) weakly in H 0 2 ( Ω ) , u j ( 0 ) u ( 0 ) weakly in H 0 1 ( Ω ) , and z j ( 0 ) z ( 0 ) weakly in L 2 ( Ω × ( 0 , 1 ) ) . Hence, by (16), we have u ( 0 ) = u 0 , u ( 0 ) = u 1 and z ( 0 ) = f 0 . Consequently, the global existence of weak solutions is established.
  • Step 2. Uniform decay of the energy.
To continue our proof, we need to introduce three new functionals
Φ ( t ) = 1 ρ + 1 Ω | u ( x , t ) | ρ u ( x , t ) u ( x , t ) d x + Ω u ( x , t ) u ( x , t ) d x .
Ψ ( t ) = Ω u ( x , t ) 0 t h ( t s ) ( u ( x , t ) u ( x , s ) ) d s d x 1 ρ + 1 Ω | u ( x , t ) | ρ u ( x , t ) 0 t h ( t s ) ( u ( x , t ) u ( x , s ) ) d s d x .
Υ ( t ) = Ω 0 1 e 2 τ ϱ G ( z ( x , ϱ , t ) ) d ϱ d x .
We set
F ( t ) = N E ( t ) + ϵ 1 Φ ( t ) + Ψ ( t ) + ϵ 2 Υ ( t ) ,
where N, ϵ 1 and ϵ 2 are suitable positive constants to be determined later.
Proposition 1.
There exist positive numbers k 0 and k 1 such that
k 0 E ( t ) F ( t ) k 1 E ( t ) .
Proof. 
Using (11), we obtain
| Υ ( t ) | 1 ξ E ( t ) .
Thanks to Young’s inequality and the Sobolev embedding theorem, we deduce
| Φ ( t ) | 1 ρ + 1 Ω | u ( x , t ) | ρ u ( x , t ) u ( x , t ) d x + Ω u ( x , t ) u ( x , t ) d x 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + ( ρ + 1 ) 1 ( ρ + 2 ) u ( t ) ρ + 2 ρ + 2 + 1 2 u ( t ) 2 + 1 2 u ( t ) 2 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + ( ρ + 1 ) 1 ( ρ + 2 ) C s ρ + 2 ( 2 E ( 0 ) / β 1 ) ρ / 2 u ( t ) 2 + 1 2 u ( t ) 2 + 1 2 u ( t ) 2 .
1 ρ + 1 Ω | u ( x , t ) | ρ u ( x , t ) 0 t h ( t s ) ( u ( x , t ) u ( x , s ) ) d s d x 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + ( ρ + 1 ) 1 ( ρ + 2 ) Ω 0 t h ( t s ) | u ( x , t ) u ( x , s ) | d s ρ + 2 d x 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + ( ρ + 1 ) 1 ( ρ + 2 ) 0 t h ( s ) d s ρ + 1 0 t h ( t s ) × Ω | u ( x , t ) u ( x , s ) | ρ + 2 d x d s 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + ( ρ + 1 ) 1 ( ρ + 2 ) ( 1 β 1 ) ρ + 1 × C s ρ + 2 ( 8 E ( 0 ) / β 1 ) ρ / 2 ( h Δ u ) ( t ) .
Thus, from (67), we obtain
Ψ ( t ) 1 2 u ( t ) 2 + ( 1 β 1 ) C s 2 2 ( h Δ u ) ( t ) + 1 ρ + 2 u ( t ) ρ + 2 ρ + 2 + ( ρ + 1 ) 1 ( ρ + 2 ) ( 1 β 1 ) ρ + 1 C s ρ + 2 ( 8 E ( 0 ) / β 1 ) ρ / 2 ( h Δ u ) ( t ) .
From (65), (66), (68), and the choice of ϵ 1 , ϵ 2 , and N, (64) can be established.
In order to obtain the exponential decay result of E ( t ) via (43), it is sufficient to prove that of F ( t ) . To this end, we need to estimate the derivative of F ( t ) first. Using (1), we obtain
Φ ( t ) = 1 ρ + 1 u ( t ) ρ + 2 ρ + 2 + u ( t ) 2 Δ u ( t ) 2 M ( u ( t ) 2 ) u ( t ) 2 + 0 t h ( t s ) ( Δ u ( s ) , Δ u ( t ) ) d s μ 1 Ω u ( x , t ) g ( u ( x , t ) ) d x μ 2 Ω u ( x , t ) g ( z ( x , 1 , t ) ) d x .
By the use of Young’s inequality and the Sobolev embedding theorem, we can estimate the right-hand side of (69) as follows:
Ω 0 t h ( t s ) Δ u ( x , t ) Δ u ( x , s ) d s d x Ω 0 t h ( t s ) | Δ u ( x , t ) | × ( | Δ u ( x , s ) Δ u ( x , t ) | + | Δ u ( x , t ) | ) d s d x 0 t h ( s ) Δ u ( t ) 2 d s + Ω 0 t h ( t s ) | Δ u ( x , t ) | | Δ u ( x , s ) Δ u ( x , t ) | d s d x ( 1 + η ) 0 t h ( s ) Δ u ( t ) 2 d s + 1 4 η ( h Δ u ) ( t ) ,
μ 1 Ω u ( x , t ) g ( u ( x , t ) ) d x μ 1 η C s 2 Δ u ( t ) 2 + μ 1 4 η g ( u ( t ) ) 2 ,
μ 2 Ω u g ( z ( x , 1 , t ) ) d x μ 2 η C s 2 Δ u ( t ) 2 + μ 2 4 η g ( z ( . , 1 , t ) ) 2 ,
where η > 0 . Here, and in the following, we use C s to represent the Poincaré constant. From (A3), (70)–(72), we obtain
Φ ( t ) 1 ρ + 1 u ( t ) ρ + 2 ρ + 2 + u ( t ) 2 1 ( 1 β 1 + 1 ) ( 1 + η ) ( μ 1 + μ 2 ) η C s 2 Δ u ( t ) 2 M ( u 2 ) u 2 + μ 1 4 η g ( u ( t ) ) 2 + μ 2 4 η g ( z ( 1 , t ) ) 2 + 1 4 η ( h Δ u ) ( t ) .
Taking the derivative of Ψ ( t ) , it follows from (6) that
Ψ ( t ) = 0 t h ( t s ) ( Δ u ( t ) , Δ u ( t ) Δ u ( s ) ) d s 0 t h ( t s ) ( u ( t ) , u ( t ) u ( s ) ) d s + Ω 0 t h ( t s ) M ( u 2 ) ( u ( t ) , u ( t ) u ( s ) ) d s d x Ω 0 t h ( t s ) Δ u ( s ) d s 0 t h ( t s ) ( Δ u ( t ) Δ u ( s ) ) d s d x + μ 1 Ω 0 t h ( t s ) ( u ( t ) u ( s ) ) g ( u ( t ) ) d s d x + μ 2 Ω 0 t h ( t s ) ( u ( t ) u ( s ) ) g ( z ( x , 1 , t ) ) d s d x 1 ρ + 1 0 t h ( t s ) ( | u ( t ) | ρ u ( t ) , u ( t ) u ( s ) ) d s 0 t h ( s ) u ( t ) 2 d s 1 ρ + 1 0 t h ( s ) u ( t ) ρ + 2 d s = I 1 + I 2 + I 3 + I 4 + I 5 + I 6 + I 7 0 t h ( s ) u ( t ) 2 d s 1 ρ + 1 0 t h ( s ) u ( t ) ρ + 2 d s .
In what follows, we estimate I 1 , . . . , I 7 in (74):
| I 1 | η Δ u ( t ) 2 + 1 β 1 4 η ( h Δ u ) ( t ) , η > 0 .
| I 2 | η u ( t ) 2 h ( 0 ) C s 2 4 η ( h Δ u ) ( t ) , η > 0 .
| I 3 | η ( 1 β 1 ) M ( u ( t ) 2 ) u ( t ) 2 + δ C s 2 4 η u ( t ) 2 γ ( h Δ u ) ( t ) η ( 1 β 1 ) M ( u ( t ) 2 ) u ( t ) 2 + δ C s 2 4 η ( 2 E ( 0 ) / m 0 ) γ ( h Δ u ) ( t ) .
For I 4 in (74), applying Hölder’s inequality and Young’s inequality, we obtain
| I 4 | η Ω 0 t h ( t s ) Δ u ( x , s ) d s 2 d x + 1 4 η Ω 0 t h ( t s ) ( Δ u ( x , t ) Δ u ( x , s ) ) d s 2 d x 2 η 0 t h ( s ) d s 2 Δ u ( t ) 2 + ( 2 η + 1 4 η ) 0 t h ( s ) d s ( h Δ u ) ( t ) , η > 0 .
By (A3), we obtain from (78) that
| I 4 | 2 η ( 1 β 1 ) 2 Δ u ( t ) 2 + ( 2 η + 1 4 η ) ( 1 β 1 ) ( h Δ u ) ( t ) , η > 0 .
Similarly,
| I 5 | μ 1 η g ( u ( t ) ) 2 + μ 1 ( 1 β 1 ) C s 2 4 η ( h Δ u ) ( t ) c 1 μ 1 η Ω u ( x , t ) g ( u ( x , t ) ) d x + μ 1 ( 1 β 1 ) C s 2 4 η ( h Δ u ) ( t ) , η > 0 .
| I 6 | μ 2 η g ( z ( . , 1 , t ) ) 2 + μ 2 ( 1 β 1 ) C s 2 4 η ( h Δ u ) ( t ) c 1 μ 2 η Ω z ( x , 1 , t ) g ( z ( x , 1 , t ) ) d x + μ 2 ( 1 β 1 ) C s 2 4 η ( h Δ u ) ( t ) , η > 0 .
| I 7 | η ρ + 1 u ( t ) 2 ( ρ + 1 ) 2 ( ρ + 1 ) h ( 0 ) C s 2 4 η ( ρ + 1 ) ( h Δ u ) ( t ) η C s 2 ( ρ + 1 ) ρ + 1 ( 2 E ( 0 ) ) ρ u ( t ) 2 h ( 0 ) C s 2 4 η ( ρ + 1 ) ( h Δ u ) ( t ) a 0 η ρ + 1 u ( t ) 2 h ( 0 ) C s 2 4 η ( ρ + 1 ) ( h Δ u ) ( t ) , η > 0 ,
where a 0 = C s 2 ( ρ + 1 ) ( 2 E ( 0 ) ) ρ . Combining (74)–(77) and (79)–(82) together, we arrive at
Ψ ( t ) 0 t h ( s ) d s ρ + 1 u ( t ) ρ + 2 ρ + 2 + η + a 0 η ρ + 1 0 t h ( s ) d s u ( t ) 2 + η 1 + 2 ( 1 β 1 ) 2 Δ u ( t ) 2 + c 1 μ 1 η Ω u ( x , t ) g ( u ( x , t ) ) d x + c 1 μ 2 η Ω z ( x , 1 , t ) g ( z ( x , 1 , t ) ) d x 2 η + 1 2 η + ( μ 1 + μ 2 ) C s 2 4 η ( 1 β 1 ) + δ C s 2 4 η ( 2 E ( 0 ) / m 0 ) γ ( h Δ u ) ( t ) ( ρ + 2 ) h ( 0 ) C s 2 4 ( ρ + 1 ) η ( h Δ u ) ( t ) , η > 0 .
Taking also the derivative of Υ ( t ) , it follows from (6) and (A4) that
Υ ( t ) = Ω 0 1 e 2 τ ϱ z ϱ ( x , ϱ , t ) g ( z ( x , ϱ , t ) ) = 1 τ Ω 0 1 ϱ ( e 2 τ ϱ G ( z ( x , ϱ , t ) ) ) + 2 τ e 2 τ ϱ G ( x , ϱ , t ) d ϱ d x = 1 τ Ω e 2 τ G ( z ( x , ϱ , t ) ) G ( u ( x , t ) ) d x 2 Υ ( t ) 2 Υ ( t ) + α 2 τ Ω u ( x , t ) g ( u ( x , t ) ) d x α 1 e 2 τ τ Ω z ( x , 1 , t ) g ( z ( x , 1 , t ) ) d x .
Then, we conclude from (63), (73), (83), and (84) that for any t t 0 > 0 ,
F ( t ) = N E ( t ) + ϵ Φ ( t ) + Ψ ( t ) + ϵ 2 Υ ( t ) h 0 ϵ ρ + 1 u ( t ) ρ + 2 ρ + 2 h 0 ϵ η 1 + a 0 ρ + 1 u ( t ) 2 ϵ η ( 1 β 1 ) M ^ ( u ( t ) 2 ) ϵ 1 ( 1 β 1 ) ( 1 + η ) ( μ 1 + μ 2 ) η C s 2 η ( 1 + 2 ( 1 β 1 ) 2 ) Δ u ( t ) 2
+ ϵ 4 η + 2 η + 1 2 η + ( μ 1 + μ 2 ) C s 2 4 η ( 1 β 1 ) + δ C s 2 4 η ( 2 E ( 0 ) / m 0 ) γ ( h Δ u ) ( t ) + N 2 ( ρ + 2 ) h ( 0 ) C s 2 4 ( ρ + 1 ) η ( h Δ u ) ( t ) N θ 1 ϵ 2 α 2 τ ϵ μ 1 c 1 4 η μ 1 c 1 η Ω u ( x , t ) g ( u ( x , t ) ) d x N θ 2 + ϵ 2 α 1 e 2 τ τ ϵ c 1 μ 2 4 η c 1 μ 2 η Ω z ( x , 1 , t ) g ( z ( x , 1 , t ) ) d x 2 ϵ 2 Υ ( t ) , η > 0 ,
where h 0 = 0 t 0 h ( s ) d s > 0 , guaranteed by (A3). At this stage, we take ϵ < h 0 and η to be sufficiently small such that
a 2 h 0 ϵ 1 η 1 + a 0 ρ + 1 > 0 , a 3 ϵ 1 η ( 1 β 1 ) > 0 ,
and a 4 ϵ 1 1 ( 1 β 1 ) ( 1 + η ) ( μ 1 + μ 2 ) η C s 2 η 1 + 2 ( 1 β 1 ) 2 > 0 .
Choosing ϵ 2 > ξ e 2 τ 2 for which
2 ϵ 2 Υ ( t ) ξ Ω 0 1 G ( z ( x , ϱ , t ) ) d x d ϱ .
As long as ϵ 1 , ϵ 2 and η are fixed, we choose N to be large enough such that
N θ 1 ϵ 2 α 2 τ ϵ 1 μ 1 c 1 4 η μ 1 c 1 η > 0 , N θ 2 + ϵ 2 α 1 e 2 τ τ ϵ 1 c 1 μ 2 4 η c 1 μ 2 η > 0 ,
and
a 5 ξ N 2 ( ρ + 2 ) h ( 0 ) C s 2 4 ( ρ + 1 ) η ϵ 4 η + 2 η + 1 2 η + ( μ 1 + μ 2 ) C s 2 4 η ( 1 β 1 ) + δ C s 2 4 η ( 2 E ( 0 ) / m 0 ) γ > 0 .
Then, applying assumption (A3) and (85), we deduce
F ( t ) a 1 u ( t ) ρ + 2 ρ + 2 a 2 u ( t ) 2 a 3 M ^ ( u ( t ) 2 ) a 4 Δ u ( t ) 2 a 5 ( h Δ u ) ( t ) ξ Ω 0 1 G ( z ( x , ϱ , t ) ) d x d ϱ , t t 0 ,
where a 1 = h 0 ϵ ρ + 1 . Then, (11) and (85) imply that there exists a positive constant M such that
F ( t ) M E ( t ) , t t 0 .
Combining (64) and (87), we infer
F ( t ) M k 1 F ( t ) , t t 0 .
Integrating (88) over ( t 0 , t ) , it follows that
F ( t ) F ( t 0 ) e M k 1 t , t t 0 .
Consequently, (12) can be obtained from (64) and (89). The proof is complete.
The rate of energy decay given by Theorem 1 is illustrated by the following example.

4. Example

Let h ( t ) = e A t with A > 1 and g ( s ) = s . Then, β 1 = 1 1 A , c 1 = 1 , α 1 = 1 2 and α 2 = 1 . For μ 1 = 1 , μ 2 = 1 4 , we obtain τ 4 ξ 3 τ 4 . Assuming max ( ϵ , ϵ 1 ) < h 0 , where h 0 = 0 t 0 h ( s ) d s and η sufficiently small, we have
h 0 ϵ 1 > η ( 1 + a 0 ρ + 1 ) , i . e . a 2 > 0 ,
ϵ 1 > η ( 1 β 1 ) , i . e . a 3 > 0 ,
and
β 1 > ( 1 β 1 ) + 5 4 C s 2 + 1 + 2 ( 1 β 1 ) 2 ϵ 1 η , i . e . a 4 > 0 .
As long as ϵ 1 , ϵ 2 , and η are fixed, we choose N to be large enough such that
N θ 1 ϵ 2 τ ϵ 1 4 η η > 0 , N θ 2 + ϵ 2 e 2 τ 2 τ ϵ 1 16 η η 4 > 0 ,
where a 5 > 0 . Finally, we put M = max ( ( ρ + 2 ) a 5 , 2 a 2 , 2 a 3 , 2 a 4 , 2 a 5 , ξ ) where a 1 = h 0 ϵ ρ + 1 , then ( 87 ) is satisfied and hence (12) yields
E ( t ) k 1 k 0 E ( t 0 ) e M k 1 t , t > t 0 .

5. Concluding Remarks

In this paper, we consider the Petrovsky–Kirchhoff-type equation with a delay term. Under suitable conditions for the initial energy, the relaxation function h ( · ) , and the nonlinear time delay term in the internal feedback g ( · ) , we prove the global existence of weak solutions and establish the uniform exponential decay of energy. The main contributions of this work are as follows:
  • We proved the global existence of weak solutions using Lemma 2 and the Faedo–Galerkin method.
  • We obtained exponential decay estimates by employing a perturbed energy method.
  • We found that the functions h ( · ) and g ( · ) are responsible for the decay rate of the energy functional and for the global existence of solutions.

Author Contributions

Writing—original draft, N.S., A.M.D., C.B. and A.A.-Q.; Supervision, A.M.D.; Funding acquisition, Supervision, A.A.-Q. All authors have read and agreed to the published version of the manuscript.

Funding

This work was supported by the Deanship of Scientific Research, Vice Presidency for Graduate Studies and Scientific Research, King Faisal University, Saudi Arabia. Project No. KFU242712.

Data Availability Statement

The original contributions presented in the study are included in the article, further inquiries can be directed to the corresponding author.

Conflicts of Interest

The authors declare no conflict of interest.

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Sebih, N.; Mohammed Djaouti, A.; Boudekhil, C.; Al-Quran, A. Global Existence and Decay Estimates for a Viscoelastic Petrovsky–Kirchhoff-Type Equation with a Delay Term. Axioms 2024, 13, 869. https://doi.org/10.3390/axioms13120869

AMA Style

Sebih N, Mohammed Djaouti A, Boudekhil C, Al-Quran A. Global Existence and Decay Estimates for a Viscoelastic Petrovsky–Kirchhoff-Type Equation with a Delay Term. Axioms. 2024; 13(12):869. https://doi.org/10.3390/axioms13120869

Chicago/Turabian Style

Sebih, Noureddine, Abdelhamid Mohammed Djaouti, Chafi Boudekhil, and Ashraf Al-Quran. 2024. "Global Existence and Decay Estimates for a Viscoelastic Petrovsky–Kirchhoff-Type Equation with a Delay Term" Axioms 13, no. 12: 869. https://doi.org/10.3390/axioms13120869

APA Style

Sebih, N., Mohammed Djaouti, A., Boudekhil, C., & Al-Quran, A. (2024). Global Existence and Decay Estimates for a Viscoelastic Petrovsky–Kirchhoff-Type Equation with a Delay Term. Axioms, 13(12), 869. https://doi.org/10.3390/axioms13120869

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