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Volume 2010, Article ID 636140,47pages doi:10.1155/2010/636140

Research Article

Weak Solutions of a Stochastic Model for Two-Dimensional Second Grade Fluids

P. A. Razafimandimby

1

and M. Sango

1, 2

1Department of Mathematics and Applied Mathematics, University of Pretoria, Pretoria 0002, South Africa

2School of Mathematics, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540, USA

Correspondence should be addressed to P. A. Razafimandimby,paulrazafi@gmail.com Received 3 July 2009; Accepted 28 February 2010

Academic Editor: Robert Finn

Copyrightq2010 P. A. Razafimandimby and M. Sango. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

We initiate the investigation of a stochastic system of evolution partial differential equations modelling the turbulent flows of a second grade fluid filling a bounded domain ofR2. We establish the global existence of a probabilistic weak solution.

1. Introduction

The study of turbulence either in Newtonian flows or Non-Newtonian flows is one of the greatest unsolved and still not well-understood problem in contemporary applied sciences.

For indepth coverage of the deep and fascinating investigations undertaken in this field, the abundant wealth of results obtained, and remarkable advances achieved we refer to the monographs in 1–4 and references therein. The hypothesis relating the turbulence to the “randomness of the background field” is one of the motivations of the study of stochastic version of equations governing the motion of fluids flows. The introduction of random external forces of noise type reflectssmallirregularities that give birth to a new random phenomenon, making the problem more realistic. Such approach in the mathematical investigation for the understanding of the turbulence phenomenonwas pioneered by Bensoussan and Temam in 5 where they studied the Stochastic Navier-Stokes Equation SNSE excited by random forces. Since then, stochastic partial differential equations and stochastic models of fluid dynamics have been the object of intense investigations which have generated several important results. We refer, for instance, to6–22. Similar investigations for Non-Newtonian fluids have almost not been undertaken except in very few work; we refer, for instance, to 23–25 for some computational studies of stochastic models of polymeric

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fluids. It is worth to note that in the Non-Newtonian case the study of stochastic models is relevant not only for the analytical approach to turbulent flows but also for practical needs related to the physics of the corresponding fluids2.

In the present work, we initiate the mathematical analysis for the stochastic model of incompressible second grade fluids. An incompressible fluid of second grade with a velocity fielduis a special example of a differential Rivlin-Ericksen fluid. It was shown in26that its stress tensorTis given by

T−p1 νA1α1A2α2A21, 1.1

wherepis the scalar pressure field,νis the kinematic viscosity, andA1 andA2are the first two Rivlin-Ericksen tensors defined by

A1 ∂ui

∂xj

i,j

∂uj

∂xi

i,j

,

A2 DA1

Dt A1

∂ui

∂xj

i,j

∂uj

∂xi

i,j

A1,

1.2

whereD/Dtdenotes the material derivative. The constantsα1andα2represent the normal stress moduli. The incompressibility requires that

divu0. 1.3

Taking into account some thermodynamical aspects, Dunn and Fosdick proved in27that the kinematic viscosityνmust be nonnegative. In addition, they found that the free energy must be a quadratic function of A1. This implies in particular that the Clausius-Duhem inequality is satisfied and the Helmholtz free energy is minimum at equilibrium if and only if

α1α20, α1 ≥0. 1.4

In what follows we assume thatα1α >0 andν >0. We also refer to28,29for more recent works concerning those conditions.

Those thermodynamical conditions imply that the stress tensorTcan be written in the following form:

T−p1 νA1α

∂tA11 2A1

LLT

−1 2

LLT A1

, 1.5

where

L ∂ui

∂xj

i,j

. 1.6

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We can check that

divT−∇pνΔuα∂Δu

∂t α

curlΔu×u

u·Δu1 4|A1|2

. 1.7

For a given external forcefthe dynamical equation for a second grade fluid is

∂u

∂t curlu×u∇ 1

2|u|2

divTf. 1.8

Making use of the latter equation and 1.7, we obtain the system of partial differential equations

∂tu−αΔuνΔucurlu−αΔu×u∇Pf, divu0,

1.9

where

Ppα

u·Δu1 4|A1|

1

2|u|2 1.10

is the modified pressure. For a given connected and bounded domainDofR2and finite time horizon0, Twe complete the above system with the initial value

u0 u0 inD, 1.11

and the Dirichlet boundary value condition

u0 on∂D×0, T. 1.12

The interest in the investigation of problem1.9arises from the fact that it is an admissible model of slow flow fluids. Furthermore, once the above thermodynamical compatibility conditions are satisfied “the second grade fluid has general and pleasant properties such as boundedness, stability, and exponential decay”see again27. It also can be taken as a generalization of the Navier-Stokes EquationNSE. Indeed they reduce to NSE whenα0;

moreover recent work30shows that it is a good approximation of the NSE. See also31–36 for interesting discussions to their relationship with other fluid models.

Due to the above nice properties, the mathematical analysis of the second grade fluid has attracted many prominent researchers in the deterministic case. The first relevant analysis was done by Ouazar in his 1981 thesis; together with Cioranescu, they published the related result in 37, 38. Their method was based on the Galerkin approximation scheme involving a priori estimates for the approximating solutions using a special basis consisting of eigenfunctions corresponding to the scalar product associated with the operator curlu−αΔu. They proved global existence and uniqueness without restriction on the initial

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data for the two-dimensional case. Cioranescu and Girault 39, as well as Bernard 40 extended this method to the three dimensional case; global existence was obtained with some reasonable restrictions on the initial data. For another approach to global existence using Schauder’s fixed point technics, we refer to41and some relevant references therein.

As already mentioned, in this work we propose a stochastic version of the problem 1.9,1.11-1.12. More precisely, we assume that a connected and bounded open setD of R2with boundary∂Dof classC3, a finite time horizon0, T, and a nonrandom initial value u0are given. We consider the problem

duαΔu −νΔucurlu−αΔu×u∇PdtFu, tdtGu, tdW inD×0, T,

divu0 in D×0, T, u0 in ∂D×0, T,

u0 u0 inD,

1.13

where u u1, u2 and P represent the random velocity and pressure, respectively. The system is to be understood in the Ito sense. It is the equation of motion of an incompressible second grade fluid driven by random external forcesFu, tand Gu, tdW, where W is a Rm-valued standard Wiener process.

As far as we know, this paper is the first dealing with the stochastic version of the equation governing the motion of a second grade fluid filling a connected and bounded domainD of R2. Consequently, we could by no means exhaust the mathematical analysis of the problem; many questions are still open but we hope that this pioneering work will find its applications elsewhere. We limited ourselves to the discussion of a global existence result of a probabilistic weak solution in the two-dimensional case. In forthcoming papers we will address other questions such as the existence probabilistic strong solutions under more stringent conditions, the uniqueness of those solutions, and their behaviour whenα → 0. It should be noted that solving this problem is not easy even in the deterministic case, the nature of the nonlinearities being one of the main difficulties in addition to the complex structure of the equations. Besides the obstacles encountered in the deterministic case, the introduction of the noise termGu, tdWin the stochastic version induces the appearance of expressions that are very hard to control when proving some crucial estimates. Overcoming these problems will require a-tour-de force in the work.

The rest of the paper is organized as follows. InSection 2, we give some notations, necessary background of probabilistic or analytical nature. Section 3 is devoted to the formulation of the hypotheses and the main result. We introduce a Galerkin approximation of the problem and derive crucial a priori estimates for its solution inSection 4; a compactness result is also derived. We prove the main result inSection 5.

2. Notations and Preliminaries

Let us start with some informationsabout some functional spaces needed in this work. LetD be an open subset ofR2, let 1≤ p ≤ ∞, and letkbe a nonnegative integer. We consider the well-known Lebesgue and Sobolev spacesLpDandWk,pD, respectively. Whenp2, we writeWk,2D HkD. We denote byW0k,pDthe closure inWk,pDofCc Dthe space

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of infinitely differentiable function with compact support inD. Ifp 2, we denoteW0k,pD byH0kD. We assume that the Hilbert spaceH01Dis endowed with the scalar product

u, v

D

∇u· ∇v dx2

i1 D

∂u

∂xi

∂v

∂xidx, 2.1

where∇is the gradient operator. The norm·generated by this scalar product is equivalent to the usual norm ofW1,2DinH01D. If the domainD is smooth enough and bounded, then for anymandpsuch thatmp >2 the embedding

Wjm,pWj,q 2.2

is compact for any 1≤q≤ ∞. More Sobolev embedding theorems can be found in42and references therein.

Next we define some probabilistic evolution spaces necessary throughout the paper.

Let Ω,F,Ft0≤t≤T,P be a given stochastic basis; that is,Ω,F,P is complete probability space andFt0≤t≤T is an increasing sub-σ-algebras of Fsuch thatF0 contains everyP-null subset ofΩ. For any reflexive separable real Banach spaceXendowed with the norm · X, for anyp ≥1,Lp0, T;Xis the space ofX-valued measurable functionsudefined on0, T such that

uLp0,T;X T

0

upXdt 1/p

<∞. 2.3

For anyr, p ≥ 1 we denote byLpΩ,P;Lr0, T;Xthe space of processesu uω, twith values inXdefined onΩ×0, Tsuch that

1uis measurable with respect toω, tand, for eacht,uisFtmeasurable, 2ut, ωXfor almost allω, tand

uLpΩ,P;Lr0,T;X

⎝E T

0

urXdt p/r

1/p

<∞, 2.4

where E denotes the mathematical expectation with respect to the probability measureP.

Whenr∞, we write

uLpΩ,P;L0,T;X

Eess sup

0≤t≤TupXdt 1/p

<∞. 2.5

Next we give some compactness results of probabilistic nature due to Prokhorov and Skorokhod. Let us considerΩas a separable and complete metric space andFits Borelσ- field. A familyPkof probability measures onΩ,Fis relatively compact if every sequence of

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elements ofPkcontains a subsequencePkjwhich converges weakly to a probability measure P; that is, for anyφbounded and continuous function onΩ,

φωdPkjdω−→ φωdPdω. 2.6

The familyPkis said to be tight if, for anyε >0, there exists a compact setKε⊂Ωsuch that PKε≥1−ε, for everyP∈Pk.

We frequently use the following two theorems. We refer to43for their proofs.

Theorem 2.1see Prokhorov. The familyPkis relatively compact if and only if it is tight.

Theorem 2.2see Skorokhod. For any sequence of probability measuresPkonΩwhich converges to a probability measureP, there exist a probability spaceΩ,F,Pand random variablesXk,Xwith values inΩsuch that the probability law ofXk(resp.,X) isPk(resp.,P) and limk→ ∞XkXP-a.s.

We proceed now with the definitions of additional spaces frequently used in this work.

In what follows we denote byXthe space ofR2-valued functions such that each component belongs toX. A simply-connected bounded domainDwith boundary of classC3is given. We introduce the spaces

V

u∈Cc 2 such that divu0 , Vclosure ofV inH1D, Hclosure ofV inL2D.

2.7

We denote by·,·and| · |the inner product and the norm induced by the inner product and the norm inL2DonH, respectively. The inner product and the norm induced by that of H10DonVare denoted respectively by ·,· and · . In the spaceV, the latter norm is equivalent to the norm generated by the following scalar productsee, e.g.,37

u, vV u, v αu, v, for anyu, v∈V. 2.8

We also introduce the following space:

W

u∈Vsuch that curlu−αΔuL2D

. 2.9

The following lemma tells us that the norm generated by the scalar product

u, vW u, vV curlu−αΔu,curlv−αΔv, 2.10

is equivalent to the usualH3D-norm onW. Its proof can be found, for example, in37,39.

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Lemma 2.3. The following (algebraic and topological) identity holds:

WW, 2.11

where

W

v∈H3Dsuch that divv0 and v|∂D 0

. 2.12

Moreover, there is a positive constantCsuch that

|v|2H3DC

|v|2V|curlv−αΔv|2

, 2.13

for anyv∈W.

By this lemma we can endow the spaceWwith norm| · |Wwhich is generated by the scalar product2.10.

From now on, we identify the space V with its dual space V via the Riesz representation, and we have the Gelfand chain

W⊂V⊂W , 2.14

where each space is dense in the next one and the inclusions are continuous.

The following inequalities will be used frequently.

Lemma 2.4. For anyu∈W,v∈W, andw∈Wone has

|curlu−αΔu×v, w| ≤C|u|H3|v|V|w|W. 2.15

One also has

|curlu−αΔu×u, w| ≤C|u|2V|w|W, 2.16

for anyu∈Wandw∈W.

Proof. We introduce the well-known trilinear formbused in the study of the Navier-Stokes equation by setting

bu, v, w 2

i,j1 D

ui

∂vj

∂xiwjdx. 2.17

We give the following identity whose proof can be found in37,40. This equation is valid for any smoothsolenoidalfunctionsΦ, v, andwas

curlΦ×v, w bv,Φ, w−bw,Φ, v. 2.18

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We derive from this that for anyu∈W,v∈W, andw∈W

|curlu−αΔu×v, w| ≤C|v|L2D|∇u−αΔu|L2D|w|LD, 2.19

where H ¨older’s inequality was used. The Sobolev embedding2.2and the equivalence of the norms| · |Wand| · |3HDimply2.15.

By2.18we deduce

curlu−αΔu×u, w bu, u, wαbu,Δu, w αbw,Δu, u. 2.20

With the help of integration by parts and using the fact thatuandware elements ofWwe derive that

bu,Δu, w 2

j1

b ∂u

∂xj, w, ∂u

∂xj

2

i1

b

u,∂w

∂xj, ∂u

∂xj

, 2.21

bw,Δu, u 2

j1

b ∂w

∂xj, u, ∂u

∂xj

. 2.22

We use these results to derive the following estimate. For any elementsu∈Vandw∈L4D, we obtain by H ¨older’s inequality

|bu, u, w| ≤C|u|L4Du|w|L4D. 2.23

And since the spaceVandWare, respectively, continuously embedded inL4DandV, then

|bu, u, w| ≤C|u|2V|w|W. 2.24

We also have

|bu,Δu, w| ≤ |∇w|LD

2 j1

∂u

∂xj

2

L2D

|u|L4D

2

j1

∂w

∂xj

2

L4D

1/2

2

j1

∂u

∂xj

2

L2D

1/2

.

2.25

We derive from this and the Sobolev embedding2.2that

|bu,Δu, w| ≤C|u|2V|w|W. 2.26

By an analogous argument we have

|bw,Δu, u| ≤C|w|W|u|2V. 2.27

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The estimates2.20,2.24–2.27yield

|curlu−αΔu×u, w| ≤C|u|2V|w|W, 2.28

for anyu∈Wandw∈W. This completes the proof of the lemma.

Next we give some results on which most of the proofs in forthcoming sections rely.

We start by stating a theorem on solvability of the “generalized Stokes equations”

vαΔv∇qf inD, divv0 in D,

v0 on∂D.

2.29

By a solution of this system we mean a functionv∈Vwhich satisfies v, h αv, h

f, h

, 2.30

for anyh∈V.

The proof of the following result can be derived from an adaptation of the results obtained by Solonnikov in44,45.

Theorem 2.5. LetDbe a connected, bounded open set ofRn n≥ 2with boundary∂Dof classCl and letfbe a function inHl,l1. Then2.29has a unique solutionv. Moreover iffis an element ofV,v∈Hl2∩V, and the following hold:

v, hV v, h,

|v|WCf

V, 2.31

for anyh∈V.

Next we formulate Aubin-Lions’s compactness theorem; its proof can be found in46.

Theorem 2.6. LetX, B, Y be three Banach spaces such that the following embedding is continuous:

XBY. 2.32

Moreover, assume that the embeddingXBis compact, then the setFconsisting of functionsvLq0, T;B, 1q≤ ∞, such that

sup

0≤h≤1 t2

t1

|vthvt|pYdt−→0, ash−→0, 2.33

for any 0< t1< t2< T, is compact inLp0, T;Bfor anyp.

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Last but not least we present the famous Kolmogorov- ˇCentsov continuity criterion for stochastic processes. We refer to47,48for its proof and some of its extension.

Theorem 2.7see Kolmogorv- ˇCentsov. Suppose that a real-valued processX {Xt, 0≤tT} on a probability spaceΩ,Psatisfies the condition

E|XthXt|γCh, 0≤t, hT, 2.34

for some positive constantsγ, β, andC. Then there exists a continuous modificationX {Xt, 0≤tT}ofX, which is locally H¨older continuous with exponentκ∈0, β/γ.

3. Hypotheses and the Main Result

We state on our problem the following.

3.1. Hypotheses 1We assume that

F:V×0, T−→V 3.1

is continuous in both variables.We also assume that, for anyt∈0, Tand anyv∈V

|Fv, t|VC1|v|V. 3.2

2We also define a nonlinear operatorGas follows:

G:V×0, T−→Vm 3.3

is continuous in both variables.We require that, for anyt∈0, T, Gv, tsatisfy

|Gv, t|V⊗mC1|v|V. 3.4

3.2. Statement of the Main Theorem

We introduce the concept of solution of the problem1.13that is of interest to us.

Definition 3.1. By a solution of the problem1.13, we mean a system Ω,F,P,Ft, W, u

, 3.5

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where

1 Ω,F,Pis a complete probability space;Ftis a filtration onΩ,F,P, 2Wtis anm-dimensionalFtstandard Wiener process,

3for a.e.t,utLpΩ,P;L0, T;W∩LpΩ,P;L0, T;V, 2≤p <∞, 4for almost allt,utisFtmeasurable,

5P-a.s the following integral equation of It ˆo type holds:

ut−u0, vV t

0

νu, v curlus−αΔus×u, vds

t

0

Fus, s, vds t

0

Gus, s, vdWs

3.6

for anyt∈0, Tandv∈W.

Remark 3.2. In the above definition the quantityt

0Gus, s, vdWsshould be understood as:

t 0

Gus, s, vdWs m

k1 t 0

Gkus, s, vdWks, 3.7

whereGkandWkdenote thekth component ofGandW, respectively.

Now we state our main result.

Theorem 3.3. Assume thatu0 ∈W; assume also that all the assumptions, namely,3.2and3.4, on the operatorsF, G are satisfied; then the problem1.13has a solution in the sense of the above definition. Moreover, almost surely the paths of the processuareW-valued weakly continuous.

4. Auxiliary Results

In this section we derive crucial a priori estimates from the Galerkin approximation. They will serve as a toolkit for the proof ofTheorem 3.3.

4.1. The Approximate Solution

The following statement is a consequence of the spectral theorem for self-adjoint compact operator stated in49. The injection of WintoVis compact. LetIbe the isomorphism of W onto W, then the restriction of I toVis a continuous compact operator into itself. Thus, there exists a sequenceeiof elements of Wwhich forms an orthonormal basis inW, and an orthogonal basis inV.

This sequence verifies:

for any v∈W v, eiWλiv, eiV, 4.1 whereλi1> λi >0,i1,2, . . . .

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We have the following important result due to39about the regularity of theei-s.

Lemma 4.1. LetDbe a bounded, simply-connected open set ofR2with a boundary of classC3, then the eigenfunctions of 4.1belong toH4D.

We consider the subset WN Spane1, . . . , eN ⊂ W and we look for a finite- dimensional approximation of a solution of our problem as a vectoruN ∈ WN that can be written as the Fourier series:

uNt N

i1

ciNteix. 4.2

Let us consider a complete probabilistic systemΩ,F,P,Ft, Wsuch that the filtration{Ft} satisfies the usual condition and W is anm-dimensional standard Wiener process taking values inRm. We requireuNto satisfy the following system:

d uN, ei

Vν uN, ei

dtb

uN, uN, ei

dtαb

uN,ΔuN, ei

dtαb

ei,ΔuN, uN dt

F t, uN

, ei

dt

G t, uN

, ei

dW,

4.3

whereuN0 as the orthogonal projection ofu0in the spaceWNis given as uN0

oruN0

−→u0 strongly inV 4.4

as N → ∞. The Fourier coefficients ciN in 4.2 are solutions of a system of stochastic ordinary differential equations which satisfy the conditions of the existence theorem of Skorokhod 50 see also47. Therefore the sequence of functionsuN exists at least on a short interval0, TN. Global existence will follow from a priori estimates foruN.

4.2. A Priori Estimates

From now onCis a constant depending only on the data, and may change from one line to the next one. We start by proving the following lemma.

Lemma 4.2. For anyN1 one has

Esup

0≤t≤T

uNt2

V<∞. 4.5

One also has

Esup

0≤t≤T

uNt2

W<∞. 4.6

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Proof. From now on we denote by|v|the quantity|curlv−αΔv|for anyv∈ W. For any integerM≥1 we introduce the stopping time

τM

⎧⎨

⎩ inf

0≤t;uNt

VuNt

M

∞ if

0≤t;uNt

VuNt

M

∅. 4.7 We will use a modification of the argument used in7.

For any 0≤ stτM,t ∈0, TN, we may apply It ˆo’s formulasee, e.g.,7,12for φuNs, eiV uNs, ei2Vto4.3and obtain

uNs, ei

2

V2

s 0

uNr, ei

V

ν

uNr, ei

b

uNr, uNr−αΔuNr, ei

dr

2

s 0

uNr, ei

V

−αb

ei,ΔuNr, uNr

F r, uN

, ei

dr

s

0

G

r, uN , ei

dW s

0

uNr, ei

V

G

r, uN , ei

2

dr.

4.8

We note that |uN|2V N

i1λiuN, ei2V. Then, multiplying by λi the above equation and summing overifrom 1 toNgive us

uNs2

V

s 0

uN2dr uN0 2

V2

s 0

F

r, uN , uN

drN

i1

λi s 0

Gr, uN, ei

2 dr

2

s 0

G

r, uN , uN

dW,

4.9

where we have used the fact thatbuN, uN, uN 0.

We obtain from4.9that uNs2

V

s 0

uNr, uNr

dr ≤uN0 2

VN

i1

λi s 0

G

uNr, r , ei

2 dr

2

s 0

F

uNr, r

, uNrdr

2

s 0

G

uNr, r

, uNr dW

,

4.10

for any 0≤stτM,t∈0, TN. For anyu∈Vwe have

|u| ≤ Pu, 4.11

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wherePis the so called Poincar´e’s constant. The last inequality implies that

F

uNs, s

, uN≤ P2uNF

uNs, s. 4.12

We also mention that

P2α−1

|v|2V≤ v2≤α−1|v|2V, for any v∈V. 4.13

From the former equation and this one we find

F

uNs, s

, uNs≤2CP2 α

1uNs2

V

. 4.14

To find a uniform estimate for the corrector termN

i1λiGuNs, ei2is not straightforward;

this is the difficulty already mentioned in the introduction. Since the corrector term is explicitly written as function depending on the scalar productinL2D ·,·and theei-s form an orthonormal basisresp., orthogonal basisofWresp,V, then the usual Bessel’s inequalitysee, e.g.,6does not apply anymore. To circumvent this difficulty we consider the following generalized Stokes equation:

GαΔG∇qG

uNs, s inD, divG0 in D,

G0 on∂D,

4.15

for anys∈0, T. ByTheorem 2.5,4.15has a solutionGinW⊗mwhen∂Dis of classC3and GuNs, s∈V⊗m. Moreover, there exists a positive constantC0such that

G

H3D⊗mC0G

uNs, s

V⊗m, 4.16

andG, e iV GuNs, s, eifor anyi≥1.

Since the norms|·|H3Dand|·|Ware equivalent onW, then there exists another positive constantCsuch that

G

W⊗mCC0G

uNs, s

V⊗m. 4.17

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Equation4.17implies thatGdepends continuously on the dataGuNs, s. Therefore, we note the aboveGasGu Ns, s. We find from4.17that

N i1

λi

G

uNs, s , ei

2 N

i1

λi

G

uNs, s , ei

2

V

N

i1

1 λi

G

uNs, s , ei

2

W.

4.18

We deduce from this that N i1

1 λi

G

uNs, s , ei

2 W ≤ 1

λ1

GuNs, s2

W⊗m. 4.19

By4.17and the assumption onG, we have N

i1

λi

G

uNs, s , ei

2

C

1uNs2

V

. 4.20

Collecting this information, we obtain from4.10that uNs2

V

s 0

uNr2dr

CC

s 0

uNr2

Vdr2 s

0

G

uNr, r

, uNr dW

.

4.21

Taking the sup over stτM in both sides of this inequality and passing to the mathematical expectation in the resulting relation and finally applying Burkh ¨older-Davis- Gundy’s inequalitysee, e.g.,48to the stochastic term, we get

Esup

s≤t∧τM

uNs2

V2νE t∧τM

0

uNs2ds

CCE t∧τM

0

uNs2

Vds2C1E t∧τM

0

GuNs, s, uNs2 ds

1/2

.

4.22

Now, we estimate

γ E t∧τM

0

G

uNs, s

, uNs2 ds

1/2

. 4.23

(16)

With the same argument that we have used for the term|FuNs, s, uNs|, we have

γCE

⎣sup

s≤t∧τM

uNs

V t∧τM

0

G

uNs, s2

V×mds 1/2

. 4.24

Byε-Young’s inequality

γCεE sup

s≤t∧τM

uNs2

VCεE t∧τM

0

GuNs, s2

V×mds 4.25

Using the assumption onGone has

γCεEsup

s≤t∧τM

uNs2

VCεE t∧τM

0

1uNs2

V

. 4.26

With convenient choice ofε1−2C1 1/2, the estimates4.22and4.26allow us to write

Esup

s≤t∧τM

uNs2

V4νE t∧τM

0

uNs2dsCCE t∧τM

0

uNs2

Vds. 4.27

We derive from this and Gronwall’s inequality that

E sup

0≤s≤t∧τM

uNs2

VC. 4.28

We recall the following relationship which is very important in the sequel:

λi

G

uNs, s , ei

G

uNs, s , ei

W, i≥1, 4.29

whereGu Ns, sis the solution inWofGS.

To alleviate notation, we only writeuNwhen we meanuN·. Let us set

φ uN

−νΔuNcurl

uNαΔuN

×uNF uN, t

. 4.30

ByLemma 4.1,φuN∈H1D. We have

d uN, ei

V φ

uN , ei

dt

G uN, t

, ei

dW. 4.31

(17)

ByTheorem 2.5a solutionvN∈Wof the following system exists:

vNαΔvN∇qφ uN

inD, divvN 0 inD,

vN0 on∂D.

4.32

Moreover,

vN, ei

V φ

uN , ei

, 4.33

for anyi. Thus,

d uN, ei

V φ

uN , ei

dtd

uN, ei

V vN, ei

Vdt

G uN, t

, ei

dW.

4.34

The following follows by multiplying the latter equation byλi and using the relationship 4.1:

d uN, ei

W vN, ei

Wdtλi

G

uN, t , ei

dW. 4.35

Recalling4.29, we obtain

d uN, ei

W vN, ei

Wdt G

uN, t , ei

WdW. 4.36

Now applying the It ˆo’s formulasee, e.g.,7toϕuN, eiW uN, ei2W, we have

d uN, ei

2

W2 uN, ei

W

vN, ei

Wdt G

uN, t , ei

2

Wdt2 uN, ei

W

G uN, t

, ei

WdW.

4.37 Summing both sides of the last equation from 1 toNyields

duN2

W2

uN, vN

WdtN

i1

G uN, t

, ei

2

Wdt2 G

uN, t , uN

WdW. 4.38

(18)

Using the definition of| · |Wand the scalar product·,·W, we can rewrite the above equation in the form

d# uN2

VuN2

$ 2

vN, uN

V curl

vNαΔvN curl

uNαΔuN dt

2 curl

G uN, t

αΔG uN, t

,curl

uNαΔuN dW

N

i1

λ2i G

uN, t , ei

2 Vdt2

G uN, t

, uN

VdW.

4.39

In view ofRemark 3.2, we have to make the convention that in the sequel

curl G

uN, t ,curl

uNαΔuNdW dt m

k1

curl

Gk

uN, t

,curl

uNαΔuNdWk

dt .

4.40

Using the definition ofvNandG, we obtain

d# uN2

VuN2

$ 2

φ uN

, uN

curl φ

uN ,curl

uNαΔuN dt

N

i1

λ2i

GuN, t, ei

2 dt2

G uN, t

, uN dW

2 curl

G uN, t

,curl

uNαΔuN dW.

4.41

With the help of4.9,4.41can be rewritten in the following way:

duN2

2 curlφ

uN ,curl

uNαΔuN dt

2 curl

G uN, t

,curl

uNαΔuN

dWN

i1

λiλ2i G

uN, t , ei

2 dt.

4.42

We infer from the definition ofφuNthat curlφ

uN

−νcurl

ΔuNF uN, t

curl curl

uNαΔuN

×uN

. 4.43

In taking advantage of the dimension we get curl

curl

uNαΔuN

×uN

uN· ∇ curl

uNαΔuN

. 4.44

(19)

This yields

uN· ∇ curl

uNαΔuN

νcurl

ΔuNF uN, t

,curl

uNαΔuN

curlφ uN

,curl

uNαΔuN .

4.45

Owing toLemma 4.1we readily check that

uN· ∇ β, β

0, 4.46

whereβcurluNαΔuN. Consequently,

ν curl ΔuN

,curl

uNαΔuN

curl F

uN, t ,curl

uNαΔuN

curlφ uN

,curl

uNαΔuN .

4.47

Or equivalently ν α

uN

ν α

curluNα νcurl

F uN, t

,curl

uNαΔuN

curlφ

uN ,curl

uNαΔuN .

4.48

We derive from4.42and the last equation that d

dt uN2

α

uN2

−2ν α

curluN α νcurl

F uN, t

,curl

uNαΔuN

N

i1

λiλ2i G

uN, t , ei

2

2 curl

G uN, t

,curl

uNαΔuNdW dt .

4.49

We argue as before in considering the stopping timeτM. We derive from4.49that uNs2

s

0

α

uNr2

N

i1

λiλ2i G

uNr, r , ei

2 dr

s

0

α

# curl

uNr

α νcurl

F

uNr, r ,curl

uNr−αΔuNr$ dr

2

s 0

curl

G

uNr, r ,curl

uNr−αΔuNr W.

4.50

(20)

Hence, uNs2

s

0

α

uNr2

drN

i1

λiλ2i

s 0

G

uNr, r , ei

2 dr

≤uN0 2

s

0

α

curl

uNruNr

s

0

2curl F

uNr, ruNr

dr 2

s

0

curl

G

uNr, r ,curl

uNr−αΔuNr dW

.

4.51

Taking the supremum over stτM in the last estimate, and taking the mathematical expectation in the resulting relation yields

Esup

s≤t∧τM

uNs2

E t∧τM

0

α

uNs2

dsN

i1

λiλ2i E t∧τM

0

G

uNs, s , ei

2 ds

≤uN0 2

E t∧τM

0

α

curl

uNsuNs

E t∧τM

0

2curl F

uNs, suNs

ds 2Esup

s≤t∧τM

s∧τM

0

curl

G

uNs, s ,curl

uNs−αΔuNs dW

.

4.52

For anyε1≥0 andε2≥0, we have Esup

s≤t∧τM

uNs2

E t∧τM

0

α

uNs2

dsN

i1

λiλ2i E t∧τM

0

G

uNs, s , ei

2

ds

≤uN0 2

E t∧τM

0

αε1

curl

uNs2 2 ε2

curl F

uNs, s2

ds

2Esup

s≤t∧τM

s∧τM

0

curl

G

uNs, s ,curl

uNs−αΔuNs dW

2νε1

α2 t∧τM

0

uNs2

ds.

4.53

We chooseε1 1/4 andε2 ν/4αand we deduce from the last inequality the following estimate,

E sup

s≤t∧τM

uNs2

E t∧τM

0

ν α

uNs2

dsN

i1

λiλ2i E t∧τM

0

G

uNs, s , ei

2

ds

≤uN0 2

E t∧τM

0

αε1

curl

uNs2ν

curl F

uNs, s2

ds

2E sup

s≤t∧τM

s∧τM

0

curl

G

uNs, s ,curl

uNs−αΔuNs dW

.

4.54

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