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Optimal control of a viscous generalized θ-type dispersive equation with weak dissipation

  • Guobing Fan and Zhifeng Yang EMAIL logo
Published/Copyright: November 21, 2020

Abstract

In this paper, we investigate the problem for optimal control of a viscous generalized θ -type dispersive equation (VG θ -type DE) with weak dissipation. First, we prove the existence and uniqueness of weak solution to the equation. Then, we present the optimal control of a VG θ -type DE with weak dissipation under boundary condition and prove the existence of optimal solution to the problem.

MSC 2010: 35D40; 35Q53; 49J20; 49L25; 93C20

1 Introduction

In this paper, we investigate a viscous generalized θ -type dispersive equation (VG θ -type DE) with weak dissipation as follows:

(1.1) u t α 2 u x x t ε ( u u x x ) x x + k u x + ( a + b ) u u x + γ u x x x + λ ( u u x x ) = α 2 ( a u x u x x + b u u x x x ) ,

or

y t ε y x x + a u x y + b u y x + k u x + γ u x x x + λ y = 0 ,

where u = G y = + G ( x ξ ) y ( ξ ) d ξ , y = u u x x and G is chosen to be the Greens function for the Helmholtz operator 1 x 2 on the line. Here, k 0 , ε > 0 (viscous effect), λ > 0 (weakly dissipative effect) a , b > 0 and u = u ( x , t ) denotes the fluid velocity. The constants α 2 and γ c 0 are squares scales, and c 0 = g h ( c 0 = k ) is the linear wave speed for undisturbed water at rest at spatial infinity. (1.1) describing the unidirectional propagation of surface waves in a shallow water region was derived by the method of asymptotic analysis and a near-identity normal form transformation from water wave theory, combining the linear dispersive of the Korteweg-de Vries (KdV) equation with the nonlinear dispersion of the Camassa-Holm (CH) equation, as well as viscous effect and weakly dissipative effect. For simplicity, we assume that α = 1 .

When ε = 0 , α 0 and λ = 0 , (1.1) becomes the well-known KdV equation:

(1.2) u t + k u x + ( a + b ) u u x + γ u x x x = 0 .

Equation (1.2) describes unidirectional propagation of waves at the free surface of shallow water under the influence of gravity. u ( x , t ) represents the wave height above a flat bottom, x is proportional to distance in the direction of propagation and t is proportional to the elapsed time, see, e.g., [1]. The Cauchy problem and long-time behavior of the KdV equation have been studied extensively, see, e.g., [2,3,4].

When k = 0 , γ = 0 , a = 1 and λ = 0 , (1.1) becomes the following family of evolutionary 1 + 1 partial differential equations, see, e.g., [5]:

(1.3) y t + u x y convection + b u y x streching = ε y x x viscosity ,

which describes the balance between convection and stretching for small viscosity in the dynamics of 1-D nonlinear waves in fluids. In a recent study of soliton equations, it is found that (1.3) for ε = 0 and any b 1 is included in the family of shallow water equations at quadratic order accuracy that are asymptotically equivalent under Kodama transformations [5].

In the absence of viscous effect, i.e., ε = 0 , (1.3) reduces to the b-family of equations:

(1.4) y t + u x y + b u y x = 0 ,

which describes a one-dimensional version of active fluid transport. It was shown by Degasperis and Procesi [6] that (1.4) cannot satisfy the asymptotic integrability condition unless b = 2 or b = 3 , see, e.g., [5,6,7].

In the case of b = 2 in (1.4), (1.4) becomes the CH equation:

(1.5) y t + u x y + 2 u y x = 0 u t u x x t + 3 u u x = 2 u x u x x + u u x x x ,

which was derived by Camassa and Holm in [7] by approximating directly the Hamiltonian for Euler equations in the shallow water regime. It turns out that it is also a model for the propagation of nonlinear waves in cylindrical hyperelastic rods, see [1]. Recently, the CH equation(s) has been investigated in [818]. For initial data u 0 H s with s > 3 2 , they have established the well-posedness (including local and global well-posedness), breaking-waves (i.e., the solutions that remain bounded while its slope becomes unbounded in finite time), blow up and blow-up rate. We note that the advantage of the CH equation in comparison with the KdV equation lies in the fact that the CH equation has peak solitons and models wave breaking.

In the case of b = 3 in (1.4), (1.4) becomes the Degasperis-Procesi (DP):

(1.6) y t + u x y + 3 u y x = 0 u t u x x t + 4 u u x = 3 u x u x x + u u x x x ,

which has a similar form to CH Eq. (1.5). Degasperis, Holm and Hone [19] proved the formal integrability of DP Eq. (1.6) by constructing a Lax pair. They also showed that (1.6) has the bi-Hamiltonian structure and infinite sequence of conserved quantities to CH peakons. After (1.6) was derived, many contributions were devoted to its study, see [2023]. For example, Yin [21] established local well-posedness to (1.6) with initial data u 0 H s s > 3 2 on the line and precise blow-up scenario and blow-up result were derived. (1.6) can be regarded as a model for nonlinear shallow water dynamics and its asymptotic accuracy is the same for the CH equation. In [24], the authors showed that (1.5) can be obtained from the shallow water elevation by an approximate Kodama transformation.

Recently, Liu investigated the traveling wave solutions to a class of θ -type dispersive models of the form [25]

(1.7) ( 1 x 2 ) u t + ( 1 θ x 2 ) x u 2 2 = ( 1 4 θ ) x u x 2 2 u t u x x t + u u x = ( 1 θ ) u x u x x + θ u u x x x , 0 < θ < 1 ,

which were identified in his study of model equations for some dispersive schemes for approximating the Hopf equation. It is easy to see that (1.7) involves a convex combination of nonlinear terms u u x x x and u x u x x . Observing the coefficients of the peaked CH (1.5) and the DP (1.6), we note that in both models, the coefficient of u u x is equal to the coefficient of u x u x x plus the coefficient of u u x x x . That is, 3 = 2 + 1 , 4 = 3 + 1 . Recently, Lai and Wu [26] considered the following generalized equation:

(1.8) u t u x x t + ( a + b ) u u x = a u x u x x + b u u x x x ,

and established the global solutions and blow-up phenomena to (1.8).

In general, it is difficult to avoid energy dissipation mechanics in a real world. So it is reasonable to investigate the model with energy dissipation in propagation of nonlinear waves. For this reason, Zhang and co-workers [27,28,29] investigated how wave equation, Kein-Gordon equation and viscoelastic equation have to be modified to include the effect of dissipation and the influence of dissipation to the solution of the equation by using the perturbed energy method (see also [3032]). When ε = 0 , a = 2 , b = 1 , (1.1) becomes the weakly dissipative Dullin-Gottwald-Holm (DGH) equation as follows:

(1.9) u t u x x t + k u x + 3 u u x + γ u x x x + λ ( u u x x ) = 2 u x u x x + u u x x x ,

which describes that the unidirectional propagation of surface waves in a shallow water regime was derived by the method of asymptotic analysis and a near-identity normal form transformation from water wave theory, combining the linear dispersive of the KdV equation with the nonlinear dispersion of the CH equation, see, e.g., [1]. Weakly dissipative θ -type Eq. (1.8) and DP Eq. (1.6) have been investigated in [26] and [33,34], respectively. Wu and Yin [26] discussed the blow-up, blow-up rate and decay of solution to the weakly dissipative θ -type equation. Recently, Novruzov [35] considered blow-up phenomena the Cauchy problem for DGH Eq. (1.9) with weak dissipation and established certain conditions on the initial datum to guarantee that the corresponding positive strong solutions blow up in finite time. Later on, Zhang et al. [1] obtained the precise blow-up scenario and established some blow-up results for strong solutions, as well as the blow-up rate of the wave-breaking solutions to (1.9). This result complements the early one in the literature, such as [35].

To give a more comprehensive introduction, we shall present here some results concerning the control problems of nonlinear dispersive equations and other shallow water wave equations. For example, by adding a viscosity term to the equations, the optimal control problems with respect to the CH equation, the DP equation, the viscous weakly dispersive DP equation and the DGH equation are investigated in [36,37,38,39]. In [40], from the point of view of distributed control, Glass proved that the CH equation on the circle T is exact controllable, and he also obtained the global asymptotic stabilization result by means of an explicit stationary feedback law. In [41], Zhang investigated the optimal control of the Benjamin-Bona-Mahony (BBM) equation and showed that one can produce a water wave to match a desired water wave (called the desired state function) if the desired water wave is sufficiently small. By applying the analytical method, Sun [42,43] obtained the maximum principles of Pontryagin’s type for the viscous generalized CH equation and the viscous DGH equation, respectively. As for optimal control of other nonlinear dispersive equations, there are lots of contributions, such as [44,45,46,47,48,49,50].

In this paper, we present an optimal control problem for Eq. (1.1), which has never been studied until now. More precisely, we investigate the optimal control system

(1.10) min { J ( y , ω ) } = 1 2 C y z S 2 + δ 2 ω L 2 ( Q 0 ) 2 , y t ε y x x + a u x y + b u y x + k u x + γ u x x x + λ y = f + B ω , i n ( 0 , T ) × Ω , u = u x = u x x = 0 , o n ( 0 , T ) × Ω , y ( 0 , x ) = y 0 ( x ) H , i n Ω ,

where f + B ω L 2 ( 0 , T ; V ) , Ω = ( 0 , 1 ) and Q 0 Q = ( 0 , T ) × Ω in the L 2 sense. Our aim is to match the given desired state z by adjusting the body force f , ω is a control that belongs to the Hilbert space L 2 ( Q 0 ) with minimal energy, the first term in cost functional measures the physical objective, the second one is the size of the control, where δ > 0 plays the role of a weight.

Throughout the paper, the letter C denotes positive constant, which may change from line to line. Before proceeding to our analysis, we present some notations which will be used throughout the paper.

Let V = H 0 1 ( 0 , 1 ) , H = L 2 ( 0 , 1 ) , V = H 1 ( 0 , 1 ) and H = L 2 ( 0 , 1 ) be dual space, respectively. It is obvious that V is dense in H, and V H = H V with each embedding being dense. We supply V with the inner product ( φ , ψ ) V = ( φ x , ψ x ) H , φ , ψ V . The extended operator B ( L 2 ( Q 0 ) , L 2 ( V ) ) is given by

B v = v , v Q 0 , 0 , v Q \ Q 0 .

We also supply H with the inner product ( , ) H and the norm H and define u H m ( Ω ) = D m u H , where D m = m x m ( m = 0 , 1 , 2 , ) . A new space W ( 0 , T ; V ) is introduced as

W ( 0 , T ; V ) = { f : f L 2 ( 0 , T ; V ) , f t L 2 ( 0 , T ; V ) } ,

which is a Hilbert space endowed with a common inner product.

Remark 1.1

According to the value of two parameters, it is not difficult to see that (1.8) is a generalization of (1.7) and (1.8) includes (1.5) and (1.6). In fact, let a = 1 θ , b = θ , then a + b = 1 . If b = θ = 1 3 , a = 2 3 ( a = 2 b ), then by using transformation t θ t , (1.8) becomes (1.5). If b = θ = 1 4 , a = 3 4 ( a = 3 b ), then by using transformation t θ t , (1.8) becomes (1.6).

2 Existence and uniqueness of weak solution to VG θ -type DE with weak dissipation

In this section, we prove the existence of a weak solution for the following VG θ -type DE with weak dissipation

(2.1) y t ε y x x + a u x y + b u y x + k u x + γ u x x x + λ y = f + B ω , in ( 0 , T ) × Ω , u = u x = u x x = 0 , on ( 0 , T ) × Ω , y ( 0 , x ) = y 0 ( x ) H , in Ω ,

where f + B ω L 2 ( 0 , T ; V ) . To facilitate further on our analysis, we introduce definition of the weak solution of (2.1) in the space W ( 0 , T ; V ) as follows:

Definition 2.1

A function y ( x , t ) W ( 0 , T ; V ) is called a weak solution to (2.1), if

d d t ( y , ψ ) H + ε ( y x , ψ x ) H + a ( u x y , ψ ) H + b ( u y x , ψ ) H + k ( u x , ψ ) H + γ ( u x x x , ψ ) H + λ ( y , ψ ) H = ( f + B ω , ψ ) V , V

for all ψ V , a.e. t [ 0 , T ] and y 0 ( x ) = ϕ H .

Next, by using the Galerkin method [27,51,52] and a priori estimates, one can obtain the following theorem, which ensures the existence of a unique weak solution to (2.1). Now, we are in position to state the main result in this section.

Theorem 2.1

Let ϕ H , f + B ω L 2 ( 0 , T ; V ) . Then there exists a unique weak solution to (1.1) in the interval [ 0 , T ] .

Proof

Let { φ j } j = 1 be an orthonormal basis in the space H consisting of eigenfunctions of the operator x 2 , where φ j is the eigenfunction subject to the Dirichlet condition:

x 2 φ j = λ j φ j , in Ω , φ j = 0 , on Ω .

We also normalize φ j such that φ j H = 1 [53]. By the elliptic operator theory, φ j forms base functions in V . For n , we define the discrete ansatz space by V n = s p a n { φ 1 , φ 2 , , φ n } V . Let y n ( t ) = y n ( x , t ) = j = 1 n y j n φ j ( x ) with y n ( , 0 ) y 0 in H .

Next, we prove the existence of a unique weak solution to (2.1) by analyzing the limiting behavior of sequences of smooth functions u n and y n , where u n and y n are the solutions of the Cauchy problem as follows:

(2.2) y n , t ε y n , x x + a u n , x y n + b u n y n , x + k u n , x + γ u n , x x x + λ y n = f + B ω , in ( 0 , T ) × Ω , u n = u n , x = u n , x x = 0 , on ( 0 , T ) × Ω , y n ( 0 , x ) = y n , 0 ( x ) = ϕ H , in Ω .

By standard methods of differential equations [27], we prove the existence of a solution (2.2) on some interval [ 0 , t n ] , then, this solution can be extended to the whole interval [ 0 , T ] by using a priori estimates. That is, we will show that the solution is uniformly bounded as t n T . Thus, we divide our proof into four steps.

Step 1. We prove a uniform L 2 ( 0 , T ; V ) bound on a sequence { u n } . Taking the inner product of (2.2) with u n in Ω , we have

1 2 d d t ( u n 2 + u n , x 2 ) + ε ( u n , x 2 + u n , x x 2 ) + a 2 b 2 ( u n , x , u n , x 2 ) + λ ( u n 2 + u n , x 2 ) = ( f + B ω , u n ) V , V .

That is,

(2.3) 1 2 d d t ( u n 2 + u n , x 2 ) + ε ( u n , x 2 + u n , x x 2 ) a 2 b 2 ( u n , x , u n , x 2 ) + ( f + B ω , u n ) V , V ( λ > 0 ) .

First, we estimate the first term of the right hand side of (2.3) as follows:

(2.4) a 2 b 2 ( u n , x , u n , x 2 ) | a 2 b | 2 u n , x L u n , x 2 .

By the Sobolev embedding theorem ( H 1 L , H 2 H 1 ) and the Poincaré inequality, we get

(2.5) u n , x L C u n , x H 1 C u n H 2 C 1 u n , x x ,

where C , C 1 are constants.

By (2.4) and (2.5), we obtain

(2.6) a 2 b 2 ( u n , x , u n , x 2 ) | a 2 b | 2 C 1 u n , x x u n , x 2 .

Next, we estimate the second term of the right hand side of (2.3). Owing to f + B ω L 2 ( 0 , T ; V ) is a control item, there exists a constant M > 0 such that f + B ω L 2 ( 0 , T ; V ) M . Thus, we deduce

(2.7) | ( f + B ω , u n ) V , V | f + B ω V u n V C 2 M u n , x .

It follows from (2.3), (2.6), (2.7) and Young’s inequality that

1 2 d d t ( u n 2 + u n , x 2 ) + ε ( u n , x 2 + u n , x x 2 ) | a 2 b | 2 C 1 u n , x x u n , x 2 + C 2 M u n , x ε u n , x x 2 + | a 2 b | 2 C 1 2 4 ε u n , x 4 + ε u n 2 + C 2 2 M 2 ε ε ( u n , x x 2 + u n 2 ) + | a 2 b | 2 C 1 2 4 ε ( u n , x x 2 + u n 2 ) 2 + C 2 2 M 2 ε .

That is,

(2.8) d d t ( u n 2 + u n , x 2 ) | a 2 b | 2 C 1 2 2 ε ( u n , x x 2 + u n 2 ) 2 + 2 C 2 2 M 2 ε .

Therefore, by (2.8), we have

(2.9) u n 2 + u n , x 2 2 C 1 M | a 2 b | 2 C 1 tan | a 2 b | C 1 C 2 M ε t + C 3 M 1 2 ,

where t [ 0 , T ] , T < π ε 2 | a 2 b | C 1 C 2 M and

C 3 = arctan | a 2 b | C 1 ( u n , 0 2 + u n , x ( 0 ) 2 ) 2 C 2 M .

Based on the above analysis, we obtain u n M 1 and u n , x M 1 . By the Sobolev embedding theorem, we have

(2.10) u n L u n H 1 ( u n + u n , x ) C .

Step 2. Multiplying the first equation of (2.2) with u n , x x and integrating by parts with respect to x in Ω , we have

1 2 d d t ( u n , x 2 + u n , x x 2 ) + ε ( u n , x x 2 + u n , x x x 2 ) + λ ( u n , x 2 + u n , x x 2 ) = a + b 2 Ω ( u n , x ) 3 d x 2 a b 2 Ω u n , x ( u n , x x ) 2 d x + ( f + B ω , u n , x x ) V , V .

That is,

(2.11) 1 2 d d t ( u n V 2 + u n H 2 2 ) + ε ( u n H 2 2 + u n H 3 2 ) a + b 2 Ω ( u n , x ) 3 d x 2 a b 2 Ω u n , x ( u n , x x ) 2 d x + ( f + B ω , u n , x x ) V , V ( λ > 0 ) .

Next, we estimate each term of the right hand side of (2.11). Owing to the Sobolev embedding theorem, we deduce that

(2.12) a + b 2 Ω ( u n , x ) 3 d x | a + b | 2 u n , x L u n , x H 2 | a + b | 2 K 1 u n H 2 u n V 2 ,

(2.13) 2 a b 2 Ω u n , x ( u n , x x ) 2 d x | 2 a b | 2 u n , x L u n , x x H 2 | 2 a b | 2 K 2 u n H 2 3 ,

where K 1 , K 2 > 0 are embedding constants.

Owing to f + B ω L 2 ( 0 , T ; V ) is a control item, there exists a constant M > 0 such that f + B ω L 2 ( 0 , T ; V ) M . Thus, by the Sobolev embedding theorem, we deduce

(2.14) | ( f + B ω , u n , x x ) V , V | f + B ω V u n , x x V K 3 M u n H 3 ,

where K 3 > 0 is the embedding constant. It follows from (2.9), (2.11)–(2.14) and Young’s inequality that

1 2 d d t ( u n V 2 + u n H 2 2 ) + ε ( u n H 2 2 + u n H 3 2 ) | a + b | 2 K 1 M 1 2 u n H 2 + | 2 a b | 2 K 2 u n H 2 3 + K 3 M u n H 3 ε 2 u n H 2 2 + K 1 2 M 1 4 | a + b | 2 4 ε + ε 2 u n H 2 2 + K 2 2 | 2 a b | 2 4 ε u n H 2 4 + ε u n H 3 2 + K 3 2 M 2 ε .

Then, we have

d d t u n H 2 2 K 2 2 | 2 a b | 2 4 ε u n H 2 4 + K 1 2 M 1 4 | a + b | 2 4 ε + K 3 2 M 2 ε = M 2 2 u n H 2 4 + M 3 2 ,

where M 2 2 = K 2 2 | 2 a b | 2 4 ε , M 3 2 = K 1 2 M 1 4 | a + b | 2 4 ε + K 3 2 M 2 ε .

It follows from the aforementioned inequality that

(2.15) u n H 2 2 M 3 M 2 tan M 2 M t + arctan M 3 M 2 u 0 H 2 2 M 4 2 ,

where t [ 0 , T ] and T < π 2 M 2 M 3 .

Step 3. We prove a uniform L 2 ( 0 , T ; V ) bound on a sequence { y n } . Taking the inner product of (2.2) with y n in Ω , we have

(2.16) 1 2 d d t y n 2 + ε y n , x 2 + λ y n 2 = ( 2 a b ) ( u n , y n y n , x ) + ( f + B ω , y n ) V , V .

First, we estimate the first term of the right hand side of (2.16). It follows from (2.10), the Poincaré inequality and the Hölder inequality that

(2.17) | ( 2 a b ) ( u n , y n y n , x ) | | 2 a b | u n L | y n y n , x C | 2 a b | 2 ( y n 2 + y n , x 2 ) C | 2 a b | 2 ( C y n , x 2 + y n , x 2 ) C 4 y n , x 2 ,

where C 4 = C | 2 a b | 2 ( C + 1 ) .

Second, we estimate the second term of the right hand side of (2.16) in the following way:

(2.18) | ( f + B ω , y n ) V , V | f + B ω V y n V C 5 M y n , x .

It follows from (2.16), (2.17) and (2.18) that

(2.19) 1 2 d d t y n 2 + ε y n , x 2 C 4 y n , x 2 + C 5 M y n , x .

By (2.19) and Young’s inequality, we have

1 2 d d t y n 2 + ε y n , x 2 C 4 y n , x 2 + ( ε C 4 ) y n , x 2 2 + C 5 2 M 2 2 ( ε C 4 ) .

That is,

(2.20) d d t y n 2 + ( ε C 4 ) y n , x 2 C 5 2 M 2 ε C 4 ,

where ε C 4 > 0 . Integrating (2.20) with respect to t on [ 0 , T ] , we obtain

(2.21) 0 T y n , x 2 d t 1 ε C 4 C 5 2 M 2 T ε C 4 + y n , 0 2 M 5 2 .

Moreover, we deduce

(2.22) y n L 2 ( 0 , T ; V ) 2 = 0 T y n H 1 2 d t C 9 0 T y n , x d t M 6 2 .

On the other hand, it follows from (2.20) that

(2.23) d d t y n 2 C 5 2 M 5 2 ε C 4 .

Integrating (2.23) with respect to t on [ 0 , T ] , we obtain

(2.24) y n , x 2 C 5 2 M 5 2 T ε C 4 + y n , 0 2 M 7 2 .

Step 4. We prove a uniform L 2 ( 0 , T ; V ) bound on a sequence { y n , t } . By (2.2), (2.9), (2.10), (2.15) and the Sobolev embedding theorem, we have

(2.25) y n , t V ε y n V + a u n H y n V + b u n V y n H + k u n H + γ u n H 2 + λ y n H + f + B ω V ε y n V + a M 1 y n V + b C y n H + k M 1 + γ M 4 + λ y n H + C 5 M .

It follows from (2.25) that

(2.26) y n , t V 2 3 ( | k | M 1 + γ M 4 + C 5 M ) 2 + 3 ( ε + a M 1 ) 2 y n V 2 + ( 3 b 2 C 2 + λ ) y n H 2 .

Integrating (2.26) with respect to t on [ 0 , T ] , we have

y n , t L 2 ( 0 , T , V ) 2 [ 3 ( | k | M 1 + γ M 4 + C 5 M ) 2 + ( 3 b 2 C 2 + λ ) M 6 2 ] T + 3 ( ε + a M 1 ) 2 M 6 2 M 8 2 .

Observing the precious discussions, we have

  1. the sequence { y n } is bounded in L 2 ( 0 , T ; H ) as well as L 2 ( 0 , T ; V ) ;

  2. the sequence { y n , t } is bounded in L 2 ( 0 , T , V ) .

Therefore, by (i) and (ii), we obtain the boundedness of { y n } in W ( 0 , T ; V ) . Hence, by standard compactness arguments, we can know that there exists a weak limit y ( t , x ) to the subsequence of { y n } in W ( 0 , T ; V ) . Moreover, one concludes convergence of the subsequence of, again denoted by { y n } weak into W ( 0 , T ; V ) , weak-star in L ( 0 , T ; H ) and strong in L 2 ( 0 , T ; H ) to a function y ( t , x ) W ( 0 , T ; V ) . The uniqueness of weak solution can be easily derived by following ideas in [54].

This completes the proof of Theorem 2.1.□

Our next result describes weak solution can be controlled by the initial value and control item.

Theorem 2.2

Let ϕ H , f + B ω L 2 ( V ) . Then there exist two constants L 1 > 0 and L 2 > 0 , such that

y W ( V ) 2 2 L 1 [ ( ϕ H + f L ( V ) ) 2 + ω L 2 ( Q 0 ) 2 ] + L 2 ,

where

L 0 = 2 max { 1 , 2 C 0 , 2 C 0 M 8 } ,

L 1 = L 0 + 4 + 4 ( ε + a M 1 ) 2 C 0 + 8 ( b C + λ ) 2 T L 0

and

L 2 = 4 ( k M 1 + γ M 4 ) 2 T .

Proof

Multiplying the first equation of (2.1) by y and integrating by parts with respect to x in Ω , we have

(2.27) 1 2 d d t y H 2 + ε Ω y x 2 d x + λ y H 2 = ( 2 a b ) Ω u y y x d x + ( f + B ω , y ) V , V .

By Poincaré’s inequality and Sobolev embedding theorem, we obtain

(2.28) ( 2 a b ) Ω u y y x d x | 2 a b | u L y H y x H | 2 a b | 2 u L ( y H 2 + y x H 2 ) | 2 a b | 2 K 4 u V ( λ 1 y x H 2 + y x H 2 ) = | 2 a b | 2 K 4 ( λ 1 + 1 ) u V y x H 2 ,

where K 4 > 0 is the embedding constant and λ 1 > 0 is the Poincaré coefficient.

By using the same argument as in the proof of Theorem 2.1, we have

(2.29) u H M 1 , u V M 1 , u H 2 M 4 ,

where M 1 and M 4 are positive constants.

It follows from (2.28) and (2.29) that

(2.30) ( 2 a b ) Ω u y y x d x | 2 a b | 2 K 4 ( λ 1 + 1 ) M 1 y V 2 M 8 y V 2 ,

where M 8 = | 2 a b | 2 K 4 ( λ 1 + 1 ) M 1 .

Combining (2.27) with (2.30), we get

(2.31) 1 2 d d t y H 2 + ε Ω y x 2 d x ( f + B ω , y ) V , V + M 8 y V 2 .

Integrating (2.31) with respect to t on [ 0 , T ] , we have

1 2 y ( T ) H 2 1 2 ϕ H 2 + ε y L 2 ( V ) 2 0 T ( f + B ω , y ) V , V d t + M 8 y L 2 ( V ) 2 .

That is,

(2.32) 1 2 y ( T ) H 2 1 2 ϕ H 2 + ( ε M 8 ) y L 2 ( V ) 2 0 T ( f + B ω , y ) V , V d t ,

where ε > M 8 . By Hölder’s inequality and Young’s inequality, we have

(2.33) 0 T ( f + B ω , y ) V , V d t 0 T f + B ω V y V d t f + B ω L 2 ( V ) y L 2 ( V ) ε M 8 2 y L 2 ( V ) 2 + 1 2 ( ε M 8 ) f + B ω L 2 ( V ) 2 .

From (2.32) and (2.33), we have

(2.34) y L 2 ( V ) 2 1 ε M 8 ϕ H 2 + 1 ( ε M 8 ) 2 f + B ω L 2 ( V ) 2 max 1 ε M 8 , 1 ( ε M 8 ) 2 ( ϕ H + f + B ω L 2 ( V ) ) 2 C 0 ( ϕ H + f + B ω L 2 ( V ) ) 2 ,

where C 0 = max { 1 ε M 8 , 1 ( ε M 8 ) 2 } .

On the other hand, in view of (2.31), we get

1 2 d d t y H 2 ( f + B ω , y ) V , V + M 8 y V 2 .

Integrating the aforementioned inequality with respect to t and observing (2.34) yields

(2.35) y H 2 ϕ H 2 + 2 f + B ω L 2 ( V ) y L 2 ( V ) + 2 M 8 y L 2 ( V ) 2 2 f + B ω L 2 ( V ) C 0 ( ϕ H + f + B ω L 2 ( V ) ) + ϕ H 2 + 2 C 0 M 8 ( ϕ H + f + B ω L 2 ( V ) ) 2 L 0 ( ϕ H + f + B ω L 2 ( V ) ) 2 ,

where L 0 = 2 max { 1 , 2 C 0 , 2 C 0 M 8 } .

It follows from (2.1) and (2.29) that

(2.36) y t V ε y V + a u H y V + b u V y H + k u H + γ u H 2 + λ y H + f + B ω V ε y V + a M 1 y V + b C y H + k M 1 + γ M 4 + λ y H + f + B ω V ( ε + a M 1 ) y V + ( b C + λ ) y H + ( k M 1 + γ M 4 ) + f + B ω V .

It follows from (2.36) that

(2.37) y t V 2 4 ( ε + a M 1 ) 2 y V 2 + 4 ( b C + λ ) 2 y H 2 + 4 ( k M 1 + γ M 4 ) 2 + 4 f + B ω V 2 .

Integrating (2.37) with respect to t on [ 0 , T ] , we have

(2.38) y t L 2 ( V ) 2 4 ( ε + a M 1 ) 2 y L 2 ( V ) 2 + 4 ( b C + λ ) 2 0 T y H 2 d t + 4 ( k M 1 + γ M 4 ) 2 T + 4 f + B ω L 2 ( V ) 2 [ 4 + 4 ( ε + a M 1 ) 2 C 0 + 8 ( b C + λ ) 2 T L 0 ] ( ϕ H + f + B ω L 2 ( V ) ) 2 + 4 ( k M 1 + γ M 4 ) 2 T .

Taking into account (2.34) and (2.38), we have

y W ( V ) 2 = y L 2 ( V ) 2 + y t L 2 ( V ) 2 L 1 ( ϕ H + f + B ω L 2 ( V ) ) 2 + L 2 2 L 1 [ ( ϕ H + f L 2 ( V ) ) 2 + B ω L 2 ( V ) ) 2 ] + L 2 2 L 1 [ ( ϕ H + f L 2 ( V ) ) 2 + ω L 2 ( Q 0 ) 2 ] + L 2 ,

where

L 1 = L 0 + 4 + 4 ( ε + a M 1 ) 2 C 0 + 8 ( b C + λ ) 2 T L 0

and L 2 = 4 ( k M 1 + γ M 4 ) 2 T .

Thus, this completes the proof of Theorem 2.2.□

3 The distributed optima control of the VG θ -type DE with weak dissipation

In this section, we investigate the distributed optimal control associated with the VG θ -type DE with weak dissipation and prove the existence of optimal solution based on Lions’ theory [55].

Consider the following control system:

(3.1) min { J ( y , ω ) } = 1 2 C y z S 2 + δ 2 ω L 2 ( Q 0 ) 2 , y t ε y x x + a u x y + b u y x + k u x + γ u x x x + λ y = f + B ω , in ( 0 , T ) × Ω , u = u x = u x x = 0 , on ( 0 , T ) × Ω , y ( 0 , x ) = y 0 ( x ) = ϕ H , in Ω ,

where f + B ω L 2 ( 0 , T ; V ) , y = u u x x and ω is a control in L 2 ( Q 0 ) , C ( W ( 0 , T ; V ) , S ) is a given continuous observation operator, S is a real Hilbert space and

min { J ( y , ω ) } = 1 2 C y z S 2 + δ 2 ω L 2 ( Q 0 ) 2

is the performance index of tracking type. Here, z S is the desired state and δ > 0 is fixed.

The optimal control problem for the VG θ -type DE with weak dissipation is min { J ( y , ω ) } , where the optimal control pair ( y , ω ) satisfies (2.1) with the given initial value and boundary condition.

For convenience, let X = W ( 0 , T ; V ) × L 2 ( Q 0 ) , Y = L 2 ( 0 , T ; V ) × H and we define an operator E = E ( e 1 , e 2 ) : X Y given by

e 1 = ( Δ ) 1 [ y t ε y x x + a u x y + b u y x + k u x + γ u x x x + λ y ( f + B ω ) ] ,

e 2 = y ( x , 0 ) ϕ ( x ) ,

where Δ is an operator from V to V . Then we rewrite the optimal control problem in the following form:

min { J ( y , ω ) } , s . t . E ( y , ω ) = 0 .

The following theorem is presented to demonstrate the existence of the optimal control to the VG θ -type DE with weak dissipation. Now, we are in position to state our result in this section.

Theorem 3.1

There exists an optimal control solution ( y , ω ) to problem (2.39).

Proof

Let ( y , ω ) X satisfying E ( y , ω ) = 0 . Observing (2.39) and using Theorem 2.2, we get

J ( y , ω ) δ 2 ω L 2 ( Q 0 ) 2 0 , y W ( V ) , y i e l d s ω L 2 ( Q 0 ) .

Then, we have

(3.2) J ( y , ω ) a s ( y , ω ) X .

Note that the norm is weakly lower semicontinuous [56]; we deduce that J is weakly lower semicontinuous. Since J ( y , ω ) 0 , for all ( y , ω ) X , we conclude that there exists

(3.3) κ = inf { J ( y , ω ) | ( y , ω ) X , E ( y , ω ) = 0 } .

This implies the existence of a minimizing sequence { ( y n , ω n ) } n N in X such that

κ = lim n J ( y n , ω n ) , E ( y n , ω n ) = 0 , n N .

According to (3.2), there exists an element ( y n , ω n ) X such that, when n ,

(3.4) y n y , weakly y W ( 0 , T ; V ) ,

(3.5) ω n ω , weakly ω L 2 ( Q 0 ) .

From (3.4), we have

lim n 0 T ( y n , t ( t ) y t ( t ) , φ ( t ) ) V , V d t = 0 , φ ( t ) L 2 ( 0 , T ; V ) .

Since the fact that W ( 0 , T ; V ) is compactly embedded into L 2 ( 0 , T ; L ) [57] and W ( 0 , T ; V ) is continuously embedded C ( 0 , T ; H ) [54], we obtain that y n y strongly in L 2 ( 0 , T ; L ) and y n y strongly in C ( 0 , T ; H ) . Furthermore, we obtain that u n u strongly in C ( 0 , T ; H ) .

Owing to the sequence { y n } converges weakly and y n W ( 0 , T ; V ) is bounded [56], based on the embedding theorem, we obtain that y n L 2 ( 0 , T ; L ) is bounded. As a matter of fact, y n L 2 ( 0 , T ; L ) is also bounded, because y n y strongly in L 2 ( 0 , T ; L ) .

Thus, it follows from the Hölder inequality that

0 T Ω ( u n , x y n u x y ) φ d x d t = 0 T Ω ( u n , x y n u n , x y + u n , x y u x y ) φ d x d t 0 T Ω u n , x ( y n y ) φ d x d t + 0 T Ω ( u n , x u x ) y ) φ d x d t 0 T y n y L u n H φ V d t + 0 T y L u n u H φ V d t y n y L 2 ( 0 , T ; L ) u n C ( 0 , T ; H ) φ L 2 ( 0 , T ; V ) + y L 2 ( 0 , T ; L ) u n u C ( 0 , T ; H ) φ L 2 ( 0 , T ; V ) 0 , ( as n , φ L 2 ( 0 , T ; V ) ) .

Similarly, we have

0 T Ω ( u y u n y n ) φ x d x d t = 0 T Ω ( u y u n y + u n y u n y n ) φ x d x d t 0 T Ω ( u y u n y ) φ x d x d t + 0 T Ω ( u n y u n y n ) φ x d x d t 0 T y L u u n H φ V d t + 0 T y y n L u n H φ V d t y L 2 ( 0 , T ; L ) u u n C ( 0 , T ; H ) φ L 2 ( 0 , T ; V ) + y y n L 2 ( 0 , T ; L ) u n C ( 0 , T ; H ) φ L 2 ( 0 , T ; V ) 0 , ( as n , φ L 2 ( 0 , T ; V ) ) .

From (3.4), we obtain

0 T Ω ( k u n , x k u x ) φ d x d t 0 , n , φ L 2 ( 0 , T ; V ) ,

0 T Ω ( γ u n , x x x γ u x x x ) φ d x d t 0 , n , φ L 2 ( 0 , T ; V ) .

From (3.5), we obtain

0 T Ω ( B ω n B ω ) φ d x d t 0 , n , φ L 2 ( 0 , T ; V ) .

Based on the above discussion, we have e 1 ( y , ω ) = 0 . Also, using the fact that y W ( 0 , T ; V ) and y n y weakly in W ( 0 , T ; V ) , we have y ( 0 ) H and y n ( 0 ) y ( 0 ) weakly as n . Furthermore, we get

( y n ( 0 ) y ( 0 ) , φ ) 0 , n , φ H ,

which implies that e 2 ( y , ω ) = 0 .

Thus, we conclude that

E ( y , ω ) = 0 .

Therefore, there exists an optimal solution ( y , ω ) to problem (2.39). In the meantime, we can infer that there exists an optimal solution ( u , ω ) to the VG θ -type DE with weak dissipation owing to the relation u = ( 1 x 2 ) 1 y .

This completes the proof of Theorem 3.1.□

Acknowledgements

This work was supported by the Scientific Research Fund of Hunan Provincial Education Department under 17A029 and 18A440, the National Science Foundation of China under 11671128, the Science Research Project of Hengyang Normal University under 16D01, the Application-oriented Special Disciplines, and the Double First-Class University Project of Hunan Province under Xiangjiaotong [2018] 469.

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Received: 2019-09-06
Revised: 2020-05-08
Accepted: 2020-07-25
Published Online: 2020-11-21

© 2020 Guobing Fan and Zhifeng Yang, published by De Gruyter

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

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  86. Meromorphic exact solutions of the (2 + 1)-dimensional generalized Calogero-Bogoyavlenskii-Schiff equation
  87. Towards a homological generalization of the direct summand theorem
  88. A standard form in (some) free fields: How to construct minimal linear representations
  89. On the determination of the number of positive and negative polynomial zeros and their isolation
  90. Perturbation of the one-dimensional time-independent Schrödinger equation with a rectangular potential barrier
  91. Simply connected topological spaces of weighted composition operators
  92. Generalized derivatives and optimization problems for n-dimensional fuzzy-number-valued functions
  93. A study of uniformities on the space of uniformly continuous mappings
  94. The strong nil-cleanness of semigroup rings
  95. On an equivalence between regular ordered Γ-semigroups and regular ordered semigroups
  96. Evolution of the first eigenvalue of the Laplace operator and the p-Laplace operator under a forced mean curvature flow
  97. Noetherian properties in composite generalized power series rings
  98. Inequalities for the generalized trigonometric and hyperbolic functions
  99. Blow-up analyses in nonlocal reaction diffusion equations with time-dependent coefficients under Neumann boundary conditions
  100. A new characterization of a proper type B semigroup
  101. Constructions of pseudorandom binary lattices using cyclotomic classes in finite fields
  102. Estimates of entropy numbers in probabilistic setting
  103. Ramsey numbers of partial order graphs (comparability graphs) and implications in ring theory
  104. S-shaped connected component of positive solutions for second-order discrete Neumann boundary value problems
  105. The logarithmic mean of two convex functionals
  106. A modified Tikhonov regularization method based on Hermite expansion for solving the Cauchy problem of the Laplace equation
  107. Approximation properties of tensor norms and operator ideals for Banach spaces
  108. A multi-power and multi-splitting inner-outer iteration for PageRank computation
  109. The edge-regular complete maps
  110. Ramanujan’s function k(τ)=r(τ)r2(2τ) and its modularity
  111. Finite groups with some weakly pronormal subgroups
  112. A new refinement of Jensen’s inequality with applications in information theory
  113. Skew-symmetric and essentially unitary operators via Berezin symbols
  114. The limit Riemann solutions to nonisentropic Chaplygin Euler equations
  115. On singularities of real algebraic sets and applications to kinematics
  116. Results on analytic functions defined by Laplace-Stieltjes transforms with perfect ϕ-type
  117. New (p, q)-estimates for different types of integral inequalities via (α, m)-convex mappings
  118. Boundary value problems of Hilfer-type fractional integro-differential equations and inclusions with nonlocal integro-multipoint boundary conditions
  119. Boundary layer analysis for a 2-D Keller-Segel model
  120. On some extensions of Gauss’ work and applications
  121. A study on strongly convex hyper S-subposets in hyper S-posets
  122. On the Gevrey ultradifferentiability of weak solutions of an abstract evolution equation with a scalar type spectral operator on the real axis
  123. Special Issue on Graph Theory (GWGT 2019), Part II
  124. On applications of bipartite graph associated with algebraic structures
  125. Further new results on strong resolving partitions for graphs
  126. The second out-neighborhood for local tournaments
  127. On the N-spectrum of oriented graphs
  128. The H-force sets of the graphs satisfying the condition of Ore’s theorem
  129. Bipartite graphs with close domination and k-domination numbers
  130. On the sandpile model of modified wheels II
  131. Connected even factors in k-tree
  132. On triangular matroids induced by n3-configurations
  133. The domination number of round digraphs
  134. Special Issue on Variational/Hemivariational Inequalities
  135. A new blow-up criterion for the Nabc family of Camassa-Holm type equation with both dissipation and dispersion
  136. On the finite approximate controllability for Hilfer fractional evolution systems with nonlocal conditions
  137. On the well-posedness of differential quasi-variational-hemivariational inequalities
  138. An efficient approach for the numerical solution of fifth-order KdV equations
  139. Generalized fractional integral inequalities of Hermite-Hadamard-type for a convex function
  140. Karush-Kuhn-Tucker optimality conditions for a class of robust optimization problems with an interval-valued objective function
  141. An equivalent quasinorm for the Lipschitz space of noncommutative martingales
  142. Optimal control of a viscous generalized θ-type dispersive equation with weak dissipation
  143. Special Issue on Problems, Methods and Applications of Nonlinear analysis
  144. Generalized Picone inequalities and their applications to (p,q)-Laplace equations
  145. Positive solutions for parametric (p(z),q(z))-equations
  146. Revisiting the sub- and super-solution method for the classical radial solutions of the mean curvature equation
  147. (p,Q) systems with critical singular exponential nonlinearities in the Heisenberg group
  148. Quasilinear Dirichlet problems with competing operators and convection
  149. Hyers-Ulam-Rassias stability of (m, n)-Jordan derivations
  150. Special Issue on Evolution Equations, Theory and Applications
  151. Instantaneous blow-up of solutions to the Cauchy problem for the fractional Khokhlov-Zabolotskaya equation
  152. Three classes of decomposable distributions
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