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Large-time behavior of a two-scale semilinear

reaction-diffusion system for concrete sulfatation

Citation for published version (APA):

Aiki, T., & Muntean, A. (2013). Large-time behavior of a two-scale semilinear reaction-diffusion system for concrete sulfatation. (CASA-report; Vol. 1314). Technische Universiteit Eindhoven.

Document status and date: Published: 01/01/2013

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EINDHOVEN UNIVERSITY OF TECHNOLOGY

Department of Mathematics and Computer Science

CASA-Report 13-14 May 2013

Large-time behavior of a two-scale semilinear reaction-diffusion system for concrete sulfatation

by

T. Aiki, A. Muntean

Centre for Analysis, Scientific computing and Applications Department of Mathematics and Computer Science

Eindhoven University of Technology P.O. Box 513

5600 MB Eindhoven, The Netherlands ISSN: 0926-4507

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Large-time behavior of a two-scale semilinear reaction-diffusion

system for concrete sulfatation

Toyohiko Aiki‡ and Adrian Muntean?

Department of Mathematics, Faculty of Science, Japan Women’s University

2-8-1 Mejirodai, Bunkyo-ku, Tokyo 112-8681, Japan. e-mail: aikit@fc.jwu.ac.jp

?CASA - Centre for Analysis, Scientific computing and Applications, Institute for

Complex Molecular Systems (ICMS), Department of Mathematics and Computer Science, Eindhoven University of Technology, The Netherlands. e-mail:

a.muntean@tue.nl

Abstract

We study the large-time behavior of (weak) solutions to a two-scale reaction-diffusion system coupled with a nonlinear ordinary differential equations modeling the partly dissipative corrosion of concrete (/cement)-based materials with sulfates. We prove that as t → ∞ the solution to the original two-scale system converges to the corresponding two-scale stationary system. To obtain the main result we make use essentially of the theory of evolution equations governed by subdifferential operators of time-dependent convex functions developed combined with a series of two-scale energy-like time-independent estimates.

1

Introduction

1.1

Organization of the paper

We study the large time behavior of a two-scale reaction-diffusion system modeling the evolution of the sulfatation reaction in concrete-based materials; see [FM13] for a rigorous derivation of the system by periodic homogenization [a direct application of two-scale convergence principles [All92, Ngu89] and multiscale analysis of PDEs posed in perforated domains [HJ91]]. To fix ideas, let us only mention here that the sulfatation reaction attacks aggressively unsaturated porous media, where the H2S air-water transfer and

bacteria interplay together in the presence of heat. This is precisely the case of most sewer pipes or of marble monuments in countries like Brazil, Japan, USA, Italy, etc.; see e.g. [BR96, ADDN04] and references cited therein. More engineering details on this scenario can be found e.g. in [GMSR09].

To show that as t → ∞ the solution to the original two-scale reaction-diffusion system converges to the corresponding two-scale stationary system, we proceed as follows:

In the subsequent sections, we present the setting of the two-scale model equations (Section 1.2), give a brief outlook on the literature that inspired us to working in such framework of multiple spatial scales (Section 1.3), and finally, we delimitate the aim of the paper (Section 1.4). The main technical assumptions behind our results together with

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the weak solvability of the problem are collected in Section 2 and Section 3, respectively. The bulk of the paper is Section 4 – the proof of our main main result - Theorem 2.6 - a characterization of the solution behavior at large times.

1.2

Two-scale model equations

Let us consider Ω and Y to be connected and bounded domains in IR3, Γi ⊂ ∂Y , i = 1, 2, 3,

∂Y = Γ1∪ Γ2∪ Γ3, and Γ1, Γ2 and Γ3 are disjoint. Also, ∂Ω = ΓD∪ ΓN and ΓD∩ ΓN = ∅.

Simplifying the scenario analyzed in [FMA12], we consider here the following system of partial differential equations coupled with one ordinary differential equation for T > 0: ∂tw1− ∇y · (d1∇yw1) = −ψ(w1 − γw2) in (0, T ) × Ω × Y, (1) ∂tw2− ∇y · (d2∇yw2) = ψ(w1− γw2) in (0, T ) × Ω × Y, (2) ∂tw3− ∇ · (d3∇w3) = −α Z Γ2 hw3− w2dγy in (0, T ) × Ω, (3) ∂tw4 = η(w1, w4) on (0, T ) × Ω × Γ1. (4)

The system is equipped with the initial conditions

wi(0, ·, ·) = wi0 in Ω × Y, i = 1, 2, w3(0, ·) = w30 in Ω, w4(0, ·, ·) = w40 on Ω × Γ1, (5)

while the boundary conditions are                d1∇yw1· νy = −η(w1, w4) on (0, T ) × Ω × Γ1, d1∇yw1· νy = 0 on (0, T ) × Ω × (Γ2 ∪ Γ3), d2∇yw2· νy = 0 on (0, T ) × Ω × (Γ1 ∪ Γ3), d2∇yw2· νy = α(hw3− w2 on (0, T ) × Ω × Γ2, d3∇w3· ν(x) = 0 on (0, T ) × ΓN, w3 = w3D on (0, T ) × ΓD, (6)

where w1 = w1(t, x, y) denotes the concentration of H2SO4 in (0, T ) × Ω × Y , w2 =

w2(t, x, y) the concentration of H2S aqueous species in (0, T ) × Ω × Y , w3 = w3(t, x) the

concentration of H2S gaseous species in (0, T ) × Ω and w4 = w4(t, x, y) of gypsum

con-centration on (0, T ) × Ω × Γ1 and η is the reaction rate of gypsum. ∇ without subscript

denotes the differentiation w.r.t. macroscopic variable x, while ∇y is the respective

dif-ferential operators w.r.t. the micro-variable y, ν and νy are outward normal vectors on

∂Ω and ∂Y , respectively.

By α we denote the rate of the reaction taking place on the interface Γ2, h is Henry’s

constant (see [BC66] for an extensive review on Henry’s law), d1, d2 and d3 are diffusion

coefficients, ψ is a continuous function on IR and γ is a positive constant. The microscale and macroscale are connected together via the right-hand side of (3) and via the micro-macro boundary condition (6)4.

1.3

Comments on related PDE systems with multiple scales

structure

Promoted initatially by G. I. Barenblatt and his co-workers (see e.g. [BZK60] and ref-erences cited therein), the research on fissured media-like equations in particular and on

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double-porosity models in general has attracted an increasing interest on the mathemat-ical analysis side especially on what pseudo-parabolic equations and nonlinear parabolic equations posed on multiple spatial scales are concerned; the focus being mostly on well-posedness aspects; see the original work of R.E Showalter and collaborators [BS85, HS90, SW91, CS95] which was a source of inspiration for later developments by M. B¨ohm and S. A. Meier ([MB08, Mei08, MM08, MM10]) and J. Escher and D. Treutler ([ET12, Tre12]). Mathematical tools employed range from a fine use of strong solutions (exploiting the semigroup structure of the problem), fixed-point arguments in Bochner spaces, energy methods for parabolic equations as well as weak-convergence type methods (particularly the two-scale convergence put in the periodic homogenization context).

For a classification of two-scale PDE systems based on the used micro-macro trans-mission condition, we refer the reader to the chapter written by R. E. Showalter in U. Hornung’s book [Hor97]. Furthermore, the reader will discover therein that the concept of balance equations on two-scales (or on a distributed array of microstructures) can be used as a stand alone modeling tool, not necessarily in the context of averaging techniques.

1.4

Aim of this paper

Very much in line with older results by Friedman, Knabner, and Tzavaras (compare [FT87, FK92]), the interest of this paper lies on the large-time asymptotics of the two-scale system (1)–(4) endowed with the initial conditions (5) and the boundary conditions (6).

In this special context of multiple spatial scales, we need to cope with two main specific difficulties:

(i) Due to the presence of the microscale (here denoted by Y ) and evolution equations posed at that level, memory effects are inherently present; see e.g. [Ant93]. The question is here twofold: How strong are such memory effects and to which extent can they affect the lifespan of the coupled PDE system?

(ii) As micro-macro transmission condition we impose a nonlinear Henry’s law, therefore particular care is needed while treating two-scale traces of Sobolev functions; see e.g. [MNR10].

It is worth noting that the large-time behavior is not only the most interesting mathe-matical question that one would pose at this stage, but also it is the most relevant one from the practical point of view – an estimate on the lifespan of the material [forced to confront, for instance, evolving free boundaries [AM10, AM13], potential clogging of the pores, and self-healing [ZACV13]] is the holy grail of the materials science.

For our problem (1)–(6), we basically show that the large-time behavior of the active concentrations is well described by the solution of the corresponding stationary system; see Theorem 2.6. In the rest of the paper, we prepare a suitable mathematical framework and then prove the large-time asymptotics for this multiscale reaction-diffusion scenario in a rigorous manner.

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2

Assumptions and main results

To keep notation simple, we put

X := {z ∈ H1(Ω) : z = 0 on ΓD}, H := L2(Ω × Y ) × L2(Ω × Y ) × L2(Ω),

V := L2(Ω; H1(Y )) × L2(Ω; H1(Y )) × X, K(T ) := W1,2(0, T ; L2(Ω × Γ1)) for T > 0,

(u, v)H := (u1, v1)L2(Ω×Y )+ γ(u2, v2)L2(Ω×Y )+ γh(u3, v3)L2(Ω)

for u := (u1, u2, u3), v := (v1, v2, v3) ∈ H.

Assumption 2.1 (A1) For i = 1, 2, di ∈ L∞(Ω×Y ) and d3 ∈ L∞(Ω) such that di(x, y) ≥

d0

i for a.e. (x, y) ∈ Ω × Y , where d0i is a positive constant, and d3(x) ≥ d03 for a.e. x ∈ Ω,

where d0

3 is a positive constant.

(A2) η(r1, r2) := R(r1)Q(r2) for r1, r2 ∈ IR, where R and Q are locally Lipschitz

continuous functions such that R0 ≥ 0 and Q0 ≤ 0 a.e. on IR and

R(r1) :=

 positive if r1 > 0,

0 otherwise, Q(r2) :=

 positive if r2 < βmax,

0 otherwise,

where βmax is a positive constant.

(A3) The function ψ is increasing and locally Lipschitz continuous on IR with ψ(0) = 0. (A4) wD 3 ∈ L2loc([0, ∞); H2(Ω))∩W 1,2 loc([0, ∞); L2(Ω))∩L ∞ +((0, ∞)×Ω) with ∇wD3 ·ν = 0 on (0, ∞) × ΓN. (A5) wi0 ∈ L2(Ω; H1(Y )) ∩ L∞+(Ω × Y ) for i = 1, 2, w30 ∈ H1(Ω) ∩ L∞+(Ω), w30− wD 3 (0, ·) ∈ X, and w40∈ L∞+(Ω × Γ1).

Note that in (A4) and (A5) we define L∞+(Ω0) := L∞(Ω0) ∩ {u : u ≥ 0 on Ω0} for a domain Ω0.

Next, we denote the two-scale problem (1)–(6) by TP(R, Q, ψ) and give a definition of a solution to TP(R, Q, ψ) as follows:

Definition 2.2 We call the multiplet (w1, w2, w3, w4) a solution to TP(R, Q, ψ) on [0, T ],

T > 0, if (S1) ∼ (S5) hold: (S1) w1, w2 ∈ W1,2(0, T ; L2(Ω × Y )) ∩ L∞(0, T ; L2(Ω; H1(Y ))) ∩ L∞((0, T ) × Ω × Y ), w3 ∈ W1,2(0, T ; L2(Ω)) ∩ L∞((0, T ) × Ω), w3− w3D ∈ L∞(0, T ; X), w4 ∈ W1,2(0, T ; L2(Ω × Γ1)) ∩ L∞((0, T ) × Ω × Γ1). (S2) Z Ω×Y ∂tw1v1dxdy + Z Ω×Y d1∇yw1· ∇yv1dxdy + Z Ω×Γ1 Q(w4)R(w1)v1dxdγy = − Z Ω×Y

ψ(w1− γw2)v1dxdy for v1 ∈ L2(Ω; H1(Y )) a.e. on [0, T ].

(S3) Z Ω×Y ∂tw2v2dxdy + Z Ω×Y d2∇yw2· ∇yv2dxdy − α Z Ω×Γ2 (hw3− w2)v2dxdγy

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= Z

Ω×Y

ψ(w1− γw2)v2dxdy for v2 ∈ L2(Ω; H1(Y )) a.e. on [0, T ].

(S4) Z Ω ∂tw3v3dx + Z Ω d3∇w3· ∇v3dx = −α Z Ω×Γ2 (hw3− w2)v3dxdγy for v3 ∈ X a.e. on [0, T ]. (S5) (4) and (5) hold.

Moreover, the multiplet (w1, w2, w3, w4) is called a solution of TP(R, Q, ψ) on [0, ∞),

if it is a solution of TP(R, Q, ψ) on [0, T ] for any T > 0.

These two Theorems are concerned with the well-posedness of TP(R, Q, ψ).

Theorem 2.3 (Uniqueness) Assume (A1) ∼ (A5), then there exists at most one solution of TP(R, Q, ψ).

Theorem 2.4 (Global existence of solutions to TP(R, Q, ψ)) Assume (A1) ∼ (A5), then there exists a solution (w1, w2, w3, w4) of TP(R, Q, ψ) on [0, ∞). Moreover, it holds that

(i) w1(t), w2(t) ≥ 0 a.e. in Ω × Y , w3(t) ≥ 0 a.e. in Ω and w4(t) ≥ 0 a.e. on Ω × Γ1

for t ≥ 0.

(ii) w1(t) ≤ M1, w2(t) ≤ M2 a.e. in Ω × Y , w3(t) ≤ M3 a.e. in Ω and w4(t) ≤ M4

a.e. on Ω × Γ1 for t ≥ 0, where M1 =

max{|w10|L∞(Ω×Y ), γ|w20|L(Ω×Y ), γh|w30|L(Ω), γh|wD

3 |L∞((0,∞)×Ω)}, M2 = 1

γM1, M3 =

1

hM2, and M4 = max{βmax, |w40|L∞(Ω×Γ1)}.

Remark 2.1 In [FMA12], we consider the system consisting in the equations (3) and (4) and prove its well-posedness (see Theorem 4.3 and Theorem 4.4 in [FMA12]):

∂tw1− ∇y· (d1∇yw1) = −f1(w1) + f2(w2) in (0, T ) × Ω × Y,

∂tw2− ∇y· (d2∇yw2) = f1(w1) − f2(w2) in (0, T ) × Ω × Y,

where f1 and f2 are continuous functions on IR. It is easy to see that Theorems 2.3 and 2.4

can cover the well-posedness of TP(R, Q, f1−f2) in case f1(r) = a1[r]+ and f2(r) = a2[r]+

for r ∈ IR, where a1 and a2 are positive constants. In fact, Let ψ(r) = a1(r) for r ∈ IR and

γ = a2

a1. Then, by Theorem 2.4, the solution (w1, w2, w3, w4) of TP(R, Q, ψ) satisfies that

• w1 and w2 are nonnegative;

• ψ(w1− γw2) = f1(w1) − f2(w2).

To be able to study the large time behavior of the solution, we need the additional condition (A6) on the boundary data.

(A6) wD 3 ∈ L ∞(0, ∞; H1(Ω)), ∂ twD3 ∈ L1((0, ∞) × Ω) ∩ L2((0, ∞) × Ω), ∂tw3D − ∇d3∇wD3 ∈ L ∞(0, ∞; L1(Ω)), ∂ t(∂twD3 − ∇d3∇w3D) ∈ L1((0, ∞) × Ω).

Clearly, under (A6) we have: w3D(t) → wD3∞ in L2(Ω) and weakly in H1(Ω) as t → ∞. Also, in order to give a statement on the large time behavior we introduce the following

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stationary problem SP(w4∞, w3∞D ) for given functions w4∞ and wD3∞. In this problem

unknown functions are w1∞, w2∞ and w3∞ such that

−∇y· (d1∇yw1∞) = −ψ(w1∞− γw2∞) in Ω × Y, −∇y· (d2∇yw2∞) = ψ(w1∞− γw2∞) in Ω × Y, −∇ · (d3∇w3∞) = −α Z Γ2 hw3∞− w2∞dγy in Ω, d1∇yw1∞· νy = −η(w1, w4∞) on Ω × Γ1, d1∇yw1∞· νy = 0 on Ω × (Γ2∪ Γ3), d2∇yw2∞· νy = 0 on Ω × (Γ1∪ Γ3), d2∇yw2∞· νy = α(hw3∞− w2∞ on Ω × Γ2, d3∇w3∞· ν(x) = 0 on ΓN, w3∞ = wD3∞ on ΓD.

Definition 2.5 We say that the triplet (w1∞, w2∞, w3∞) is a solution of SP(w4∞, wD3∞),

if the following conditions hold: wi∞ ∈ L2(Ω; H1(Y )) ∩ L∞(Ω × Y ), i = 1, 2, w3∞− wD3∞∈

X ∩ L∞(Ω), Z Ω×Y d1∇yw1∞· ∇yv1dxdy + Z Ω×Γ1 Q(w4∞)R(w1∞)v1dxdγy = − Z Ω×Y ψ(w1∞− γw2∞)v1dxdy for v1 ∈ L2(Ω, H1(Y )), Z Ω×Y d2∇yw2∞· ∇yv2dxdy − α Z Ω×Γ2 (hw3∞− w2∞)v2dxdγy = Z Ω×Y ψ(w1∞− γw2∞)v2dxdy for v2 ∈ L2(Ω, H1(Y )), Z Ω d3∇w3∞· ∇v3dx + α Z Ω×Γ2 (hw3∞− w2∞)v3dxdγy = 0 for v3 ∈ X.

Theorem 2.6 (Large-time behavior) Assume (A1) ∼ (A6) and let (w1, w2, w3, w4) be a

solution of TP(R, Q, ψ) on [0, ∞). Then it holds that w4(t) → w4∞ in L1(Ω × Γ1) as

t → ∞ for some w4∞ ∈ L∞(Ω × Γ1), and ∂tw4 ∈ L1((0, ∞) × Ω × Γ1) and there exists a

sequence {tn} with tn→ ∞ as n → ∞ such that

w(tn) → w∞ weakly in H as n → ∞,

for some w∞ ∈ H, and w∞ is a solution of SP(w4∞, w3∞D ), where w = (w1, w2, w3).

Moreover, if (ψ(r) − ψ(r0))(r − r0) ≥ µ|r − r0|p+1 for r, r0 ∈ IR, where µ > 0 and p ≥ 1,

then SP(w4∞, wD3∞) has at most one solution and

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3

Well-posedness of TP(R, Q, ψ)

The aim of this section is to show the existence and uniqueness of a solution to TP(R, Q, ψ) on [0, T ] for any T > 0.

First, we consider the following auxiliary problem AP(w4) for given w4 ∈ K(T ):

∂tw1− ∇y · (d1∇yw1) = −ψ(w1 − γw2) in (0, T ) × Ω × Y, (8) ∂tw2− ∇y · (d2∇yw2) = ψ(w1− γw2) in (0, T ) × Ω × Y, (9) ∂tw3− ∇ · (d3∇w3) = −α Z Γ2 hw3− w2dγy in (0, T ) × Ω, (10) wi(0) = wi0 in Ω × Y for i = 1, 2, and w3(0) = w03 in Ω, (11) d1∇yw1· νy = −η(w1, w4) on (0, T ) × Ω × Γ1, (12) d1∇yw1· νy = 0 on (0, T ) × Ω × (Γ2∪ Γ3), (13) d2∇yw2· νy = 0 on (0, T ) × Ω × (Γ1∪ Γ3), (14) d2∇yw2· νy = α(hw3− w2  on (0, T ) × Ω × Γ2, (15) d3∇w3· ν(x) = 0 on (0, T ) × ΓN, w3 = wD3 on (0, T ) × ΓD. (16)

From now on, we solve the above problem AP(w4) by using the theory of evolution

equations governed by subdifferential operators of time-dependent convex functions (see [Yam76] and[Ken81]). To apply this theory, we first define a function ϕt(w4, ·) on H for

t ∈ [0, T ], wD

3 satisfying (A4) and w4 ∈ L2(Ω × Γ1) as follows:

ϕt(w4, u) =                  1 2 Z Ω×Y d1|∇yu1|2dxdy + Z Ω×Γ1 Q(w4) ˆR(u1)dxdγy + γ 2 Z Ω×Y d2|∇yu2|2dxdy + Z Ω×Y ˆ

ψ(u1− γu2)dxdy +

γα 2 Z Ω×Γ2 |h(u3+ w3D(t)) − u2|2dxdγy +γh 2 Z Ω d3|∇u3|2dx if u = (u1, u2, u3) ∈ V, ∞ otherwise,

where ˆR and ˆψ are primitives of R and ψ with ˆR(0) = 0 and ˆψ(0) = 0, respectively. Moreover, we can prove the following Lemma in a straightforward manner:

Lemma 3.1 Let t ∈ [0, T ]. If (A1) ∼ (A4) hold, Q is Lipschitz continuous and bounded on IR, R and ψ are Lipschitz continuous on IR and w4 ∈ K(T ), then ϕt(w4, ·) is proper,

l.s.c. and convex on H for t ∈ [0, T ] and D(ϕt(w

4, ·)) = V and ∂ϕt(w4, u) is single

valued, where D(ϕt(w4, ·)) denotes the effective domain of ϕt(w4, ·). Moreover, u ∈ H

and u∗ = ∂ϕt(w4, u) is equivalent to u∗ = (u∗1, u ∗ 2, u ∗ 3) ∈ H and (u∗1, v1)L2(Ω×Y ) = Z Ω×Y d1∇yu1· ∇yv1dxdy + Z Ω×Γ1 Q(w4)R(u1)v1dxdγy + Z Ω×Y

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(u∗2, v2)L2(Ω×Y ) = Z Ω×Y d2∇yu2· ∇yv2dxdy − α Z Ω×Γ2 (h(u3+ wD3 (t)) − u2)v2dxdγy − Z Ω×Y

ψ(u1− γu2)v2dxdy for v2 ∈ L2(Ω, H1(Y )),

(u∗3, v3)L2(Ω) = Z Ω d3∇u3· ∇v3dx + α Z Ω×Γ2 (h(u3+ w3D(t)) − u2)v3dxdγy for v3 ∈ X.

The next Lemma is concerned with the continuity property of ϕt with respect to t.

Lemma 3.2 Let T > 0. If (A1) ∼ (A5) hold, R and Q are Lipschitz continuous and bounded on IR, ψ is Lipschitz continuous on IR and w4 ∈ K(T ), then for any r > 0 there

exists br ∈ W1,2(0, T ) such that for 0 ≤ s ≤ t ≤ T and u ∈ V with |u|H ≤ r it holds that

ϕt(w4(t), u) − ϕs(w4(s), u) ≤ |br(t) − br(s)|(1 + |ϕs(w4(s), u)|).

Accordingly, by the theory of evolution equations developed cf. [Ken81] and by Lemma 3.2, we can deduce the solvability of the following problem.

Lemma 3.3 Let T > 0. If (A1) ∼ (A5) hold, R and Q are Lipschitz continuous and bounded on IR, ψ is Lipschitz continuous on IR and w4 ∈ K(T ), then for any u0 ∈ V there

exists one and only u ∈ W1,2(0, T ; H) such that ϕ(·)(w4(·), u(·)) ∈ L∞(0, T ) and

d

dtu(t) + ∂ϕ

t(w

4(t), u(t)) = f (t) in H for t ∈ [0, T ] and u(0) = u0, (17)

where f (t) = (0, 0, −∂twD3 (t) + ∇d3∇w3D(t)) for t ∈ [0, T ].

Lemma 3.1 and Lemma 3.3 guarantee the existence of a solution of AP(w4).

Lemma 3.4 Let T > 0. If (A1) ∼ (A5) hold, R and Q are Lipschitz continuous and bounded on IR, ψ is Lipschitz continuous on IR and w4 ∈ K(T ), then AP(w4) has a unique

solution w = (w1, w2, w3) on [0, T ]. Precisely speaking, w1, w2 ∈ W1,2(0, T ; L2(Ω × Y )) ∩

L∞(0, T ; L2(Ω; H1(Y ))), w3 ∈ W1,2(0, T ; L2(Ω)), w3− w3D ∈ L∞(0, T ; X), (8) ∼ (16) hold

in the usual sense.

Proof. By putting u0 = (w10, w20, w30− wD3 (0)) we see that u0 ∈ V . Then on account

of Lemma 3.3 there exists u = (u1, u2, u3) satisfying (17). Hence, by putting w1 = u1,

w2 = u2 and w3 = u3+ wD3 it is clear that the assertion of this proposition is true. 2

Now, we show a proof of Theorem 2.4 by applying the fixed point argument in case Q, R and ψ are Lipschitz continuous.

Proposition 3.5 Let T > 0. If (A1) ∼ (A5) hold, R and Q are Lipschitz continuous and bounded on IR, ψ is Lipschitz continuous on IR, then TP(R, Q, ψ) has a unique solution on [0, T ].

(12)

Proof. Let T > 0. By Lemma 3.4 for w4 ∈ K(T ) these exists one and only one solution

(w1, w2, w3) ∈ W1,2(0, T ; H) of AP(w4). Then we can define a mapping ΛT in the following

way: ΛT : K(T ) → K(T ) is given by

(ΛTw4)(t) = w04+

Z t

0

η(w1(τ ), w4(τ ))dτ for t ∈ [0, T ].

Obviously, this mapping is well-defined. From now on we shall show that ΛT is a

contrac-tion mapping for small T > 0.

Let w4(1), w4(2) ∈ K(T ), w(1) = (w(1) 1 , w (1) 2 , w (1) 3 ) and w(2) = (w (2) 1 , w (2) 2 , w (2) 3 ) be solutions

of AP(w4(1)) and AP(w4(2)), respectively, and put w4 = w (1)

4 − w

(2)

4 , w = w(1) − w(2) =

(w1, w2, w3). It from (8) follows that

∂tw1− ∇y · (d1∇yw1) = −ψ(w (1) 1 − γw (1) 2 ) + ψ(w (2) 1 − γw (2) 2 ) in (0, T ) × Ω × Y. By multiplying it by w1 we have 1 2 d dt|w1| 2 L2(Ω×Y )+ Z Ω×Y d1|∇yw1|2dxdy + Z Ω×Γ1 (Q(w4(1))R(w1(1)) − Q(w(2)4 )R(w(2)1 ))w1dxdγy = − Z Ω×Y (ψ(w(1)1 − γw(1)2 ) − ψ(w1(2)− γw2(2)))w1dxdy a.e. on [0, T ]. (18)

Similarly to (18), we see that γ 2 d dt|w2| 2 L2(Ω×Y )+ γ Z Ω×Y d2|∇yw2|2dxdy = γα Z Ω×Γ2 (hw3− w2)w2dxdγy +γ Z Ω×Y (ψ(w1(1)− γw(1)2 ) − ψ(w1(2)− γw2(2)))w2dxdy a.e. on [0, T ], and γh 2 d dt|w3| 2 L2(Ω)+ γh Z Ω d3|∇w3|2dx = −γhα Z Ω×Γ2 (hw3− w2)w3dxdγy a.e. on [0, T ].

Since (A2) implies that R is increasing on IR, we obtain Z Ω×Γ1 (Q(w(1)4 )R(w1(1)) − Q(w(2)4 )R(w(2)1 ))w1dxdγy ≥ − Z Ω×Γ1 |Q(w(1)4 ) − Q(w4(2))||R(w(2)1 )||w1|dxdγy a.e. on [0, T ].

Accordingly, it holds that 1 2 d dt|w| 2 H + d01 Z Ω×Y |∇yw1|2dxdy + γd02 Z Ω×Y |∇yw2|2dxdy + γhd03 Z Ω |∇w3|2dx

(13)

≤ Z Ω×Γ1 |Q(w4(1)) − Q(w(2)4 )||R(w(2)1 )||w1|dxdγy − Z Ω×Y (ψ(w1(1)− γw2(1)) − ψ(w1(2)− γw(2)2 ))(w1 − γw2)dxdy ≤ CQ|R|L∞(IR) Z Ω |w1|L2 1)|w4|L2(Γ1)dx ≤ CYCQ|R|L∞(IR) Z Ω (|∇yw1|L2(Y )+ |w1|L2(Y ))|w4|L2 1)dx ≤ d 0 1 2 Z Ω |∇yw1|2L2(Y )dx + 1 2 Z Ω |w1|2L2(Y )dx + C0 Z Ω |w4|2L2 1)dx a.e. on [0, T ],

where CQis a Lipschitz constant of Q, C0 = (2d10 1

+12)(CYCQ|R|L∞(IR))2 and CY is a positive

constant such that

|z|L2

1) ≤ CY|z|H1(Ω) for z ∈ H

1(Y ). (19)

From these inequalities, it follows that 1 2 d dt|w| 2 H + d0 1 2 Z Ω×Y |∇yw1|2dxdy + γd02 Z Ω×Y |∇yw2|2dxdy + γhd03 Z Ω |∇w3|2dxdy ≤ C0 Z Ω |w4|2L2 1)dx + 1 2 Z Ω |w1|2L2(Y )dx ≤ C1( Z Ω |w4|2L2 1)dx + |w| 2 H) a.e. on [0, T ],

where C1 = C0+12. Then by applying Gronwall’s inequality we obtain

1 2|w(t)| 2 H + Z t 0 (d 0 1 2|∇yw1| 2 L2(Ω×Y )+ γd02|∇yw2|2L2(Ω×Y )+ γhd03|∇w3|2L2(Ω))dτ ≤ C2 Z t 0 |w4|2L2(Ω×Γ 1)dτ for t ∈ [0, T ], (20)

where C2 is a positive constant. This shows that

|∂t(Λw (1) 4 ) − ∂t(Λw (2) 4 )|L2(0,T ;L2(Ω×Γ 1)) ≤ |R(w1(1))Q(w(1)4 ) − R(w1(2))Q(w(2)4 )|L2(0,T ;L2(Ω×Γ 1)) ≤ CR|Q|L∞(IR)|w1|L2(0,T ;L2(Ω×Γ 1))+ CQ|R|L∞(IR)|w4|L2(0,T ;L2(Ω×Γ1))) ≤ (1 + CY)CR|Q|L∞(IR)|w1|L2(0,T ;L2(Ω;H1(Y )))+ CQ|R|L(IR)|w4|L2(0,T ;L2(Ω×Γ 1))) ≤ C3|w4|L2(0,T ;L2(Ω×Γ 1)) ≤ C3| Z t 0 ∂τw4dτ |L2(0,T ;L2(Ω×Γ 1)) ≤ C3T |∂tw4|L2(0,T ;L2(Ω×Γ 1)), (21)

where CR is a Lipschitz constant of R and C3 is a positive constant depending only on

C2. Moreover, by using (21) we have

|Λw(1)4 − Λw(2)4 |L2(0,T ;L2(Ω×Γ 1)) ≤ | Z t ∂t(Λw (1) 4 − Λw (2) 4 )dτ |L2(0,T ;L2(Ω×Γ 1))

(14)

≤ T |∂t(Λw (1) 4 ) − ∂t(Λw (2) 4 )|L2(0,T ;L2(Ω×Γ 1)) ≤ C4T2|∂tw4|L2(0,T ;L2(Ω×Γ 1)),

where C4 is a positive constant.

Hence, if T1 is sufficiently small, then ΛT1 is a contraction mapping. Namely, Banach’s

fixed point theorem shows that TP(R, Q, ψ) has a solution on [0, T1]. Furthermore, the

choice of T1 is independent of initial values so that we conclude that TP(R, Q, ψ) has a

solution on [0, T ].

The uniqueness of a solution is a direct consequence of the Banach’s fixed point

the-orem. 2

Lemma 3.6 Let T > 0 and assume that (A1) ∼ (A5) hold, R and Q are Lipschitz continuous and bounded on IR, ψ is Lipschitz continuous on IR. If (w1, w2, w3, w4) is a

solution of TP(R, Q, ψ) on [0, T ], then it holds that

0 ≤ wi ≤ Mi a.e. on (0, T ) × Ω × Y for i = 1, 2,

0 ≤ w3 ≤ M3 a.e. on (0, T ) × Ω, and 0 ≤ w4 ≤ M4 a.e. on (0, T ) × Ω × Γ1,

where Mi is the positive constant defined in Theorem 2.4 for each i = 1, 2, 3, 4.

The proof of this lemma is quite similar to that of [FMA12, Theorem 4.4] so that we omit a proof of Lemma 3.6.

By using Proposition 3.5 and Lemma 3.6, we can now prove Theorem 2.3 and Theorem 2.4.

Sketch of the proofs of Theorem 2.3 and Theorem 2.4. First, for m > 0 we put

Rm(r) =  R(m) for r > m, R(r) otherwise, Qm(r) =    Q(m) for r > m, Q(r) for 0 ≤ r ≤ m, Q(0) otherwise, and ψm(r) =    ψ(m) for r > m, ψ(r) for 0 ≤ r ≤ m, ψ(−m) otherwise.

Then, Proposition 3.5 implies that TP(Rm, Qm, ψm) has a solution (w1m, w2m, w3m, w4m)

on [0, T ] for any T > 0. Moreover, on account of Lemma 3.6 we can choose a positive constant m > 0 such that Rm(w1m) = R(w1m), Qm(w1m) = Q(w1m) and ψm(w1m −

γw2m) = ψ(w1m− γw2m), since Mi is independent of m for each i = 1, 2, 3, 4. This shows

the conclusion of Theorem 2.4. Moreover, the uniqueness of a solution of TP(R, Q, ψ) is a direct consequence of Proposition 3.5. 2

4

The quest of the large-time behavior

To prove Theorem 2.6, throughout this section we always assume (A1) ∼ (A5) and (A6), and denote a solution of TP(R, Q, ψ) on [0, ∞) by (w1, w2, w3, w4). Clearly, by putting

(15)

f := ∂twD3 − ∇d3∇w3D there exists f∞ ∈ L

(Ω) such that f (t) → f

∞ in L1(Ω) as

t → ∞. Also, let m0 = max{M1, M2, M3, M4}. Then for some m1 ≥ m0 it holds that

Rm1(z1) = R(z1), ψm1(z1−γz2) = ψ(z1−γz2) for z = (z1, z2, z3) ∈ U (m0), where U (m0) =

{z = (z1, z2, z3) ∈ H|0 ≤ z1 ≤ m0, 0 ≤ z2 ≤ m0 a.e. on Ω × Y, 0 ≤ z3 ≤ m0 a.e. on Ω}.

Moreover, for simplicity, we write R, Q and ψ as Rm1, Qm1 and ψm1, respectively, in this

section, and set

`1 = R(M1), `2 = |Q(w4)|L∞((0,∞)×Ω×Γ

1), `3 = ˆR(M1), `4 = sup{|Q

0

(r)| : |r| ≤ m0|}.

First, we show the convergence of w4(t) as t → ∞.

Lemma 4.1 w4(t) converges to some function w4∞ ∈ L∞(Ω × Γ1) in L1(Ω × Γ1) as

t → ∞, 0 ≤ w4∞ ≤ m0 a.e. on Ω × Γ1, and

∂tw4 ∈ L1(0, ∞; L1(Ω × Γ1)) ∩ L2(0, ∞; L2(Ω × Γ1)). (22)

Proof. By (A2) it is obvious that ∂tw4 = η(w1, w4) ≥ 0 a.e. on (0, ∞) × Ω × Γ1. Then

Lemma 3.6 and the Lebesgue monotone convergence theorem imply that w4(t) → w4∞ in

L1(Ω × Γ1) as t → ∞, where w4∞ ∈ L∞(Ω × Γ1).

It is easy to see that

Z T 0 Z Ω×Γ1 |∂tw4|dxdγydt = Z T 0 Z Ω×Γ1 ∂tw4dxdγydt = Z Ω×Γ1 (w4(T ) − w04)dxdγy for T > 0, and Z T 0 Z Ω×Γ1 |∂tw4|2dxdγydt ≤ `1`2 Z T 0 Z Ω×Γ1 |∂tw4|dxdγydt for T > 0.

Then these estimates lead to (22). 2

Now, we provide uniform estimates on the time derivative of solutions. Lemma 4.2 It holds that

∂tw1, ∂tw2 ∈ L2(0, ∞; L2(Ω × Y )), ∂tw˜3 ∈ L2(0, ∞; L2(Ω)),

w1, w2 ∈ L∞(0, ∞; L2(Ω; H1(Y ))), ˜w3 ∈ L∞(0, ∞; X),

where ˜w3 = w3− wD3 .

Proof. By multiplying (1) by ∂tw1, we can obtain

Z Ω×Y |∂tw1|2dxdy + 1 2 d dt Z Ω×Y d1|∇yw1|2dxdy + d dt Z Ω×Γ1 Q(w4) ˆR(w1)dxdγy = − Z Ω×Y ψ(w1 − γw2)∂tw1dxdy + Z Ω×Γ Q0(w4)∂tw4R(wˆ 1)dxdγy a.e. on [0, ∞).

(16)

Next, we multiply (2) by γ∂tw2. Then we see that γ Z Ω×Y |∂tw2|2dxdy + γ 2 d dt Z Ω×Y d2|∇yw2|2dxdy +γα Z Ω×Γ2 (w2− h( ˜w3+ w3D))∂tw2dxdγy = γ Z Ω×Y ψ(w1 − γw2)∂tw2dxdy a.e. on [0, ∞). Easily, we have ∂tw˜3− ∇d3∇ ˜w3 = −α Z Γ2 h( ˜w3 + wD3 ) − w2dγy− f a.e. on (0, ∞) × Ω,

where f = ∂tw3D− ∇d3∇wD3 . Here, we multiply it by γh∂tw˜3 and observe that

γh Z Ω |∂tw˜3|2dx + γh 2 d dt Z Ω d3|∇ ˜w3|2dx = −αγh Z Ω×Γ2 (h( ˜w3+ w3D) − w2)∂tw˜3dxdγy − γh Z Ω f ∂tw˜3dx = −αγh Z Ω×Γ2 (h( ˜w3+ w3D) − w2)(∂tw˜3+ ∂twD3 )dxdγy +αγh Z Ω×Γ2 (h( ˜w3+ w3D) − w2)∂twD3 dxdγy− γh d dt Z Ω f ˜w3dx + γh Z Ω ∂tf ˜w3dx

a.e. on [0, ∞). By adding these equations we obtain Z Ω×Y |∂tw1|2dxdy + γ Z Ω×Y |∂tw2|2dxdy + γh Z Ω |∂tw˜3|2dx +1 2 d dt Z Ω×Y d1|∇yw1|2dxdy + γ Z Ω×Y d2|∇yw3|2dxdy + γh Z Ω d3|∇ ˜w3|2dx  +d dt Z Ω×Γ1 Q(w4) ˆR(w1)dxdγy+ γα d dt Z Ω×Γ2 |w2− h( ˜w3+ wD3 )| 2 dxdγy +d dt Z Ω×Y ˆ ψ(w1− γw2)dxdy = Z Ω×Γ1 Q0(w4)∂tw4R(wˆ 1)dxdγy+ αγh Z Ω×Γ2 (h( ˜w3+ wD3 ) − w2)∂wD3 dxdγy (23) −γhd dt Z Ω f ˜w3dx + γh Z Ω ∂tf ˜w3dx (=: 4 X i=1 Ii(·)) a.e. on [0, ∞). Since I1(t) ≤ `3`4 Z Ω×Γ1 |∂tw4(t)|dxdγy for a.e. t ≥ 0,

(17)

it holds that I1 ∈ L1(0, ∞). It is clear that I2 = αγh Z Ω×Γ2 (hw3− w2)∂tw3Ddxdγy ≤ αγh(hM3+ M2) Z Ω×Γ2 |∂tw3D|dxdγy a.e. on [0, ∞)

so that I2 ∈ L1(0, ∞). Also, we see that

Z t 0 I3(τ )dτ = γh(− Z Ω f (t) ˜w3(t)dx + Z Ω f (0)(w30+ wD3 (0))dx) ≤ B1 for t ≥ 0,

where B1 is a positive constant, and

I4(t) ≤ γh(M3+ |wD3 |L∞((0,∞)×Ω))

Z

|∂tf (t)|dx for t ≥ 0

so that I4 ∈ L∞(0, ∞). Hence, we have proved this lemma. 2

To describe the large-time behavior of the solution, we introduce the following nota-tions: We put w(t) := (w1(t), w2(t), w3(t)) ∈ H for t ≥ 0,

ω(w0) =  z ∈ H

w(tn) → z weakly in H as n → ∞ for some sequence {tn}

with tn→ ∞ as n → ∞  , where w0 = (w10, w20, w30), ϕt1(u) = ϕt(w4(t), u) − γh Z Ω f (t)u3dx for u = (u1, u2, u3) ∈ H, ϕ∞1 (u) =                    1 2 Z Ω×Y d1|∇yu1|2dxdy + Z Ω×Γ1 Q(w4∞) ˆR(u1)dxdγy+ γ 2 Z Ω×Y d2|∇yu2|2dxdy + Z Ω×Y ˆ

ψ(u1− γu2)dxdy +

γα 2 Z Ω×Γ2 |h(u3+ wD3∞) − u2|2dxdγy +γh 2 Z Ω d3|∇u3|2dx − γh Z Ω f∞u3dx if u = (u1, u2, u3) ∈ V, ∞ otherwise, and F (ϕ∞1 ) = {z ∈ H|ϕ∞1 (z) = min u∈Hϕ ∞ 1 (u)}.

Clearly, the similar results to Lemma 3.1 hold for ϕ∞1 . Here, we note that w satisfies (S2), (S3) and (S4) if and only if ˜w = (w1, w2, ˜w3) with ˜w3 = w3− w3D is a solution of the

following evolution equation:

˜

(18)

Moreover, since by Theorem 2.4 {w(t)}t≥0 is bounded in H, there exist a sequence

{tn} with tn→ ∞ as n → ∞ and w∞ = (w1∞, w2∞, w3∞) ∈ U (m0) such that

w(tn) → w∞ weakly in H as n → ∞,

that is, w∞ ∈ ω(w0).

The next Lemma guarantees the existence of a solution to SP(w4∞, wD3∞).

Lemma 4.3 w∞∈ F (ϕ∞1 ) and w∞ is a solution of SP(w4∞, w3∞D ).

Proof. By integrating (23) over [s, t] with 0 ≤ s ≤ t we have

ϕt1( ˜w(t)) − ϕs1( ˜w(s)) + Z t s |∂tw|˜2Hdτ ≤ 4 X i=1 Z t s Iidτ for 0 ≤ s ≤ t,

where ˜w = (w1, w2, ˜w3). It is obvious that the function t → ϕt1( ˜w(t)) +

Rt 0 |∂tw|˜ 2 Hdτ − P4 i=1 Rt 0Iidτ is non-increasing on [0, ∞) and ϕ t

1( ˜w(t))) ≥ 0 for t ≥ 0. Then by Lemma

4.2 we see that limt→∞ϕt1( ˜w(t)) exists so that we can put q0 = limt→∞ϕt1( ˜w(t))) ≥ 0.

Next, we show that

ϕ∞1 ( ˜w∞) ≤ lim inf

n→∞ ϕ

tn

1 ( ˜w(tn)), (25)

where ˜w∞ = (w1∞, w2∞, w3∞− w3∞D ). In fact, we observe that for each n

|ϕ∞ 1 ( ˜w(tn)) − ϕt1n( ˜w(tn))| ≤ Z Ω×Γ1 |Q(w4∞) ˆR(w1(tn)) − Q(w4(tn)) ˆR(w1(tn))|dxdγy +γα 2 Z Ω×Γ2 ||h( ˜w3(tn) + wD3∞) − w2(tn)|2− |h( ˜w3(tn) + w3D(tn)) − w2(tn))|2|dxdγy +h Z Ω |(f∞− f (tn)) ˜w3(tn)|dx ≤ `3`4 Z Ω×Γ1 |w4∞− w4(tn)|dxdγy + h Z Ω |f∞− f (tn)|| ˜w3(tn)|dx +γα 2 Z Ω×Γ2 |h(w3∞D − w3D(tn))(2h ˜w3(tn) + h(w3D(tn) + wD3∞) − 2w2(tn))|dxdγy.

Then, for some positive constant C5, we obtain:

|ϕ∞1 ( ˜w(tn)) − ϕt1n( ˜w(tn))| ≤ C5 Z ∞ tn ( Z Ω×Γ1 |∂tw4|dxdγy+ Z Ω×Γ2 |∂twD3 |dxdγy + Z Ω |∂tf |dx)dt for n so that lim n→∞(ϕ ∞ 1 ( ˜w(tn)) − ϕt1n( ˜w(tn))) = 0. (26)

Hence, we see that

lim inf n→∞ ϕ tn 1 ( ˜w(tn)) ≥ lim inf n→∞ (ϕ tn 1 ( ˜w(tn)) − ϕ∞1 ( ˜w(tn)) + lim inf n→∞ ϕ ∞ 1 ( ˜w(tn)) ≥ ϕ∞1 ( ˜w∞).

(19)

Thus (25) is true. Moreover, it is clear that ϕ∞1 ( ˜w∞) ≤ q0 so that ˜w∞∈ V .

Based on Lemma 4.2, we can take a subsequence {t0n} with t0

n → ∞ as n → ∞ such

that

n ≤ t0n≤ n + 1 for each n and ∂tw(t˜ 0n) → 0 in H as n → ∞. (27)

Let z ∈ V . Similarly to (26), we can prove that ϕt0n

1 (z) → ϕ ∞ 1 (z) as n → ∞. Also, by (24) we have (− ˜wt(t0n), z − w(t 0 n))H = (∂ϕ t0n 1 (w(t 0 n)), z − ˜w(t 0 n))H ≤ ϕt0n 1 (z) − ϕ t0n 1 ( ˜w(t 0 n)) for each n.

By letting n → ∞ in the above inequality, we obtain 0 ≤ ϕ∞1 (z) − q0 for any z ∈ V . This

shows that q0 = min ϕ∞, that is, and ˜w∞ ∈ F (ϕ∞1 ). Moreover, we see that 0 = ∂ϕ∞( ˜w∞).

Hence, Lemma 3.1 together with w∞∈ U (m0) implies the conclusion of this Lemma. 2

The next Lemma guarantees the uniqueness of solutions to SP(w4∞, wD3∞).

Lemma 4.4 If (ψ(r) − ψ(r0))(r − r0) ≥ µ|r − r0|p+1 for r, r0 ∈ IR, where µ > 0 and p ≥ 1,

then SP(w4∞, w3∞D ) has at most one solution.

Proof. Let w(1)∞(:= (w1(1), w2(1), w3(1))) and w(2)∞(:= (w1(2), w2(2), w(2)3 )) be solutions of

SP(w4∞, w3∞D ) and w (1)

∞ − w∞(2) = (w1∞, w2∞, w3∞).

By Definition 2.5 we see that

0 = Z Ω×Y d1|∇yw1∞|2dxdy + Z Ω×Γ1 Q(w4∞)(R(w (1) 1 ) − R(w (2) 1 ))w1∞dxdγy + Z Ω×Y (ψ(w1(1)− γw2(1)) − ψ(w1(2)− γw(2)2 ))(w1∞− γw2∞)dxdy +γ Z Ω×Y d2|∇yw2∞|2dxdy + αγ Z Ω×Γ2 |hw3∞− w2∞|2dxdγy + αγ Z Ω d3|∇w3∞|2dx.

Using of the monotonicity of R and ψ, we obtain ∇w3∞ = 0 a.e. on Ω. Since w3∞ = 0

a.e. on ΓD, we obtain w3∞ = 0 a.e. on Ω. Accordingly, we have w2 = 0 a.e. on

Ω × Γ2. Immediately, we infer that w2 = 0 a.e. on Ω × Y . Moreover, it follows that

R

Ω×Y d1|∇yw1∞|

2dxdy + µR

Ω×Y |w1∞ − γw2∞|

p+1dxdy = 0. This implies the uniqueness

of a solution of the stationary problem. 2 Now, we accomplish the proof of Theorem 2.6.

Proof of Theorem 2.6.

Considering the above arguments, it is sufficient to show (7). Let {t0n} be a sequence satisfying (27). First, we observe that

(∂ϕt0n 1 ( ˜w(t 0 n)) − ∂ϕ ∞ 1 ( ˜w∞), ˜w(t0n) − ˜w∞)H ≥ Z Ω×Y d1|∇y(w1(t0n) − w1∞)|2dxdy + Z Ω×Γ (Q(w4(t0n))R(w1(t0n)) − Q(w4∞)R(w1∞))(w1(t0n) − w1∞)dxdγy

(20)

+µ Z Ω×Y |(w1(t0n) − w1∞) − γ(w2(t0n) − w2∞)|p+1dxdy +γ Z Ω×Y d2|∇y(w2(t0n) − w2∞)|2dxdy +αγ Z Ω×Γ2 |h( ˜w3(t0n) − ˜w3∞) − (w2(t0n) − w2∞)|2dxdγy +αγh Z Ω×Γ2 (wD3 (t0n) − wD3∞){(w2(tn0 ) − w2∞) − h( ˜w3(t0n) − ˜w3∞)}dxdγy +γh Z Ω d3|∇( ˜w3(t0n) − ˜w3∞)|2dx + γh Z Ω (f (t0n) − f∞)( ˜w3(t0n) − ˜w3∞)dx =: 8 X i=1 Jin for each n.

For each n, it is easy to see that

J1n+ J4n+ J7n ≥ d0 1 Z Ω×Y |∇y(w1(t0n) − w∞)|2dxdy + γd02 Z Ω×Y |∇y(w2(t0n) − w2∞)|2dxdy +γhd03 Z Ω |∇( ˜w3(t0n) − ˜w3∞)|2dx, and J2n ≥ Z Ω×Γ1 (Q(w4(t0n)) − Q(w4∞))R(w1∞)(w1(t0n) − w1∞)dxdγy.

On the other hand, we have

(∂ϕt0n 1 ( ˜w(t 0 n)) − ∂ϕ ∞ 1 ( ˜w∞), ˜w(t 0 n) − ˜w∞)H = (− ˜wt(t0n), ˜w(t 0 n) − ˜w∞)H for each n. (28) Then we obtain d01 Z Ω×Y |∇y(w1(t0n) − w∞)| 2dxdy + γd0 2 Z Ω×Y |∇y(w2(t0n) − w2∞)|2dxdy +αγd03 Z Ω |∇( ˜w3(t0n) − ˜w3∞)|2dx +µ Z Ω×Y |(w1(t0n) − w1∞) − γ(w2(t0n) − w2∞)|p+1dxdy +αγ Z Ω×Γ2 |h( ˜w3(t0n) − ˜w3∞) − (w2(t0n) − w2∞)|2dxdγy

≤ E(t0n) + | ˜wt(t0n)|H| ˜w(t0n) − ˜w∞|H for each n, (29)

where

E(t) = Z

Ω×Γ1

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+αγh Z Ω×Γ2 (w3D(t0n) − w3∞D ){(w2(tn0) − w2∞) − h( ˜w3(t0n) − ˜w3∞)}dxdγy +γh Z Ω |f (t) − f∞|| ˜w3(t) − ˜w3∞|dx for t ≥ 0.

By letting n → ∞ in the above inequality, we infer that ˜w3(t0n) → ˜w3∞in X, w2(t0n) → w2∞

and w1(t0n) → w1∞ in L2(Ω; H1(Y )) as n → ∞. In particular, ˜w(t0n) → ˜w∞ in H as

n → ∞.

From (28), it follows that

−(∂ϕt 1( ˜w(t)) − ∂ϕ ∞ 1 ( ˜w∞), ˜w(t) − ˜w∞)H = 1 2 d dt| ˜w(t) − ˜w∞| 2 H for a.e. t ≥ 0.

Then, similarly to (29), we can show that 1

2 d

dt| ˜w(t) − ˜w∞|

2

H ≤ E(t) for a.e. t ≥ 0.

By integrating it over [t0n, t] with t0n≤ t ≤ t0

n+ 2 for n, we have 1 2| ˜w(t) − ˜w∞| 2 H ≤ 1 2| ˜w(t 0 n) − ˜w∞| 2 H + Z t0n+2 t0 n E(τ )dτ. (30)

By the assumption (A6) and Lemma 4.1 for any ε > 0 we can take a positive integer N1

such that 1 2| ˜w(t 0 n) − ˜w∞| 2 H < 1

2ε for n ≥ N1 and E(t) < 1

4ε for t ≥ N1.

Then for t ≥ N1+ 1 there exists a positive integer n ≥ N1 such that n + 1 ≤ t ≤ n + 2.

In this case we see that n ≤ t0n ≤ n + 1 ≤ t ≤ n + 2 ≤ t0

n+ 2. Hence, on account of (30)

we infer that 12| ˜w(t) − ˜w∞|2H < ε for t ≥ N1 + 1. This is the conclusion of this theorem.

Thus we have proved Theorem 2.6. 2

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