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DOI : https://doi.org/10.32628/CSEIT1953116

Stability of

𝑳 βˆ’

periodic equilibrium solutions of Navier-Stokes equations on

infinite strip

S. Khabid

LaΓ’youne Higher School of Technology, Ibn Zohr University, Morocco E-mail : [email protected]

ABSTRACT

In this paper, we assume that a smooth equilibrium solution π‘ˆ0, 𝑝0 of Navier-Stokes equations is given on an infinite strip Ξ© = 𝐼𝑅 Γ—] βˆ’1

2, 1

2[, the problem of stability that arises in the infinite plate (Ξ© = 𝐼𝑅

2Γ—] βˆ’1 2,

1 2[) disappears in our case using the same tools in [7].

Keywords : Navier-Stokes equations, Fourier series, Stability, Regularity

I. Notations and Preliminaries

For

𝒳, 𝒴

Banach spaces,

βˆ₯. βˆ₯

𝒳

, βˆ₯. βˆ₯

𝒴

are their

respective norms.

𝐿(𝒳, 𝒴)

is the space of bounded

operators from

𝒳

to

𝒴

with

βˆ₯ 𝑇 βˆ₯

the operator

norm.

For

𝐴

a linear operator on

𝒳

and

𝐸 βŠ† 𝒳

a

subspace,

𝐴|

𝐸

is the restriction of

𝐴

to

𝐸

.

For any

Ω, 𝐻

𝑝

(Ξ©)

is the Sobolev space of functions

having square integrable derivatives up to order

𝑝

with

(. , . )

𝑝

and

βˆ₯. βˆ₯

𝐻𝑝(Ξ©)

the usual scalar product

and norm on

𝐻

𝑝

(Ξ©)

.We set

β„’

2

(Ω) = 𝐻

0

(Ξ©)

and

βˆ₯. βˆ₯

𝐻𝑝

=βˆ₯. βˆ₯

𝐻𝑝(Ξ©)

and extend this notation to vectors

and set :

βˆ₯ 𝑒 βˆ₯

β„’22

=βˆ₯ 𝑒

1

βˆ₯

β„’22

+βˆ₯ 𝑒

2

βˆ₯

β„’22

where

𝑒 = (𝑒

1

, 𝑒

2

) ∈ (β„’

2

(Ξ©))

2

, Likewise with the

Sobolev norms. The scalar product on

(𝐻

𝑝

(Ξ©))

2

is

〈. , . βŒͺ

𝑝

, with :

βŒ©π‘’, 𝑣βŒͺ

𝑝

= βˆ‘

2

𝑖=1

(𝑒

𝑖

, 𝑣

𝑖

)

𝑝

, 𝑒

𝑖

, 𝑣

𝑖

∈ 𝐻

𝑝

(Ξ©)

where

𝑒 = (𝑒

1

, 𝑒

2

), 𝑣 = (𝑣

1

, 𝑣

2

)

and we set

〈. , . βŒͺ = 〈. , . βŒͺ

0

.

𝐢

𝑝

(Ξ©

Μ…)

is the space of functions

𝑝

times

continously differentiable on

Ξ©

Μ…

and

𝐢

0𝑝

(Ξ©

Μ…)

is the

space of functions

𝑓 ∈ 𝐢

𝑝

(Ξ©

Μ…)

with supp

𝑓

compact.

II. Introduction

Consider the Navier-Stokes equation on an infinite strip Ξ© = IR Γ—] βˆ’1

2, 1 2[: βˆ‚U

βˆ‚t = Ξ½Ξ”U βˆ’ (U. βˆ‡)U + βˆ‡p + f, div U = 0 (1) Where U = (u1, u2) satisfies Dirichlet boundary conditions at y = Β±1/2, p is the pressure, Ξ½ kinematic viscosity and f a time independent outer force.

We assume that a smooth equilibrium solution

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We can study The stability of U0= (u1, u2), p0 against small perturbations under two aspects: (i) The perturbations are L -periodic in x. (ii)The perturbations are in (β„’2(Ξ©))2.

The relation between (i) and (ii) is the mathematical tools used by physicists in connection with Schrâdinger equations with periodic potentials [4]. We will use the same tools used before like the direct integrals (see [1] , [4] , [7]) and the Θ-Periodic functions (ie. generalisation of periodic function).

To discuss the stability of U0, p0 with respect to various classes of perturbations we replace U, p in ( 1) by U0+ v, p0+ Ο€ and we use that U0, p0 is an equilibrium solution of ( 1), Whereby it is supposed that v satisfy the same Dirichlet boundary conditions. By a straightforward computation we obtain:

{ βˆ‚v

βˆ‚t = Ξ½Ξ”v βˆ’ (u0. βˆ‡)v βˆ’ (v. βˆ‡)u0βˆ’ (v. βˆ‡)v βˆ’ βˆ‡Ο€

div v = 0, v/ βˆ‚Ξ© = 0 (2)

Now let’s put this problem in a functional analytic frame.

Set V = {f ∈ (H01(Ξ©))2, div f = 0}andE = V (β„’2(Ξ©))2

,

and 𝒫 the orthogonal projection onto E

We apply 𝒫 to the both sides of (2) we get:

βˆ‚tv = (As+ 𝒫T0)v + 𝒫N(v) (3)

Where As is the Stokes operator defined by:

f ∈ D(AS) iff {f ∈ (H

2(Ω) ∩ H 0

1(Ξ©))2, div f = 0 ASf = ν𝒫Δf, βˆ€f ∈ D(AS)

T0 the linear operator defined by

T0f = βˆ’(u0. βˆ‡)f βˆ’ (f. βˆ‡)u0, βˆ€f ∈ (H1(Ξ©) ∩ H01(Ξ©))2. N is no-linear operator defined on E by N(v) = βˆ’(v. βˆ‡)v and let B = As+ 𝒫T0.

Proposition 2.1 [7]

E = {v ∈ L2(Ξ©), div v = 0\v βŠ₯ βˆ‡p, βˆ€p ∈ H1(Ξ©)}

Remark 1

EβŠ₯βŠƒ {βˆ‡Ο†, Ο† ∈ H1(Ξ©)}

We have Ο€ ∈ H1(Ξ©) then according to the previous remark βˆ‡Ο€ ∈ EβŠ₯, and on the other hand we have for all v ∈ E, βˆ‚tv ∈ E. cause βˆ‚t commute with v.

Proposition 2.2

AS is selfadjoint and ≀ βˆ’Ξ΅ for some Ξ΅ > 0, and exists c > 0 such if ASv = f for v ∈ D(AS) and f ∈ E, then β€–vβ€–H2(Ξ©)≀ cβ€–fβ€–L2(Ξ©) (βˆ—)

Proof

We have 〈ASv, vβŒͺ ≀ βˆ’Ξ½ c(Ξ©)β€–vβ€–L2

2 , where c(Ξ©) is the PoincarΓ© constant, then it suffice to take Ξ΅ =c(Ξ©)Ξ½ . βŒ©βˆ’ASv, vβŒͺ β‰₯ Ξ΅β€–vβ€–L2 so β€–ASvβ€–L2β‰₯ β€–vβ€–L2 which

implies AS is injective .

Finaly, AS is bijective from D(AS) to Im(AS).

Corollary 1

T0 is relatively bounded with respect to AS ie : for all Ξ΄ > 0 there is KΞ΄> 0 such that:

β€–T0uβ€–L2≀ Ξ΄β€–ASuβ€–L2+ KΞ΄β€–uβ€–L2 , βˆ€u ∈ D(AS)

Proof

Set A operator on L2(Ξ©) such that (Au)

i= Ξ”ui for all u in D(A) with D(A) = (H2(Ξ©) ∩ H

0

1(Ξ©))2, i = 1,2.

Ξ© bounded in the direction π‘œπ‘¦βƒ—βƒ—βƒ—βƒ— then according to the PoincarΓ© inequality A is bounded ie: there is a constant cβ€² > 0 such that:

β€–Auβ€–L2≀ cβ€²β€–uβ€–H2(Ξ©) , for all u ∈ D (A)

Since A ≀ βˆ’Ξ΅ for some Ξ΅ > 0 then (βˆ’A)12 is well

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For all Ξ΄ > 0 exists KΞ΄> 0 such that:

According to (*) of the proposition 2.2 there is c > 0

such that:

According to proposition 2.2 we have A is selfadjoint and β‰₯ Ξ΄ for some Ξ΄ > 0. example the quadratic forms theory in [4]) that:

D (A12) = H01(Ξ©), βˆ₯ A (****) with the proposition 2.2 to obtain:

βˆ‘ equivalents independently to Ξ», and defined by :

β€–fβ€–Ξ³ = β€–BΞ»

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equilibrium solution of (3) stable in the sense of Ljapounov.

Theorem 1 [5]

1. If Οƒ(B) βŠ† {Ξ»/Re(Ξ») ≀ βˆ’Ξ΄} for some Ξ΄ > 0 then v = 0 is stable in the sense of Ljapounov of (3),

2. If Re(Ξ») > 0 for some Ξ» ∈ Οƒ(B) then v = 0 is unstable in the sense of Ljapounov of (3)

Since the source of the difficulties is the singularity of the Stokes operator then we will focus on it using the same theory. This theory, well established in the case of SchrΓΆdinger equations with periodic potentials [4] extends to the stokes operators which occur in Navier-Stokes and related equations, but the corresponding theory is now more involved, see [7] where the three dimensional case (3d) is treated. The Stokes operators which appear in connection with (1), either 2d or 3d, are of the form:

AsU = ν𝒫ΔU. (4)

U is the argument on which the operator acts, while

𝒫 is the orthogonal projection onto the space of divergence free fields. Three cases are of interest: (a) U ∈ (H2(Ξ©) ∩ H01(Ξ©))2, div U = 0.

(b) U is periodic in the unbounded space direction. (c) U is Floquet-periodic in the unbounded space direction.

Case (b) subsumes under case (c) [2]; case (a) is handled in [6]. There is a spectral formulas relation between the cases (a) and (c), well known in case of the SchrΓΆdinger equations with periodic potentials. In the 3d-case however, these spectral formulas associated with (2) are more complicated than in the SchrΓΆdinger case due to the appearance of singularities [7]. The purpose of this paper is to show that in the 2d-case these singularities are disappear and that the spectral formulas associated with (2) have the same results as in the SchrΓΆdinger equations case. To this effect we study first the most important special, ie. U = 0. We have to perform estimates

similar to those in [7]. In our estimates, which are considerably simpler, singularities do not appear.

How to exploit this fact so as to obtain the mentioned spectral formulas is the outlined in subsequent section.

III. 𝚯-Periodic function

We fix a period 𝐿 > 0 , set 𝑄𝐿=]0, 𝐿[ and 𝑄 = 𝑄𝐿×] βˆ’

1 2,

1

2[, for some small πœ– > 0 we put π‘€πœ–=] βˆ’ πœ–, 2πœ‹ + πœ–[ with 𝑀 = [0,2πœ‹] (π‘€πœ– is a neighbourhood of 𝑀) .

And let π‘€Μ‡πœ–be π‘€πœ–minus the numbers 0 and 2πœ‹. We define a Θ-Periodic function (Floquet-periodic function):

For Θ in π‘€πœ– ; 𝑓 ∈ 𝐢Θ 𝑝

(𝑄) if 𝑓 ∈ 𝐢𝑝(𝑄) and 𝑓(π‘₯ + 𝑗𝐿, 𝑦) = π‘’π‘–π‘—Ξ˜π‘“(π‘₯, 𝑦), 𝑗 ∈ 𝑍𝑍, (π‘₯, 𝑦) ∈ Ξ©, with 𝑖2= βˆ’1 we define the functional spaces :

π»Ξ˜π‘(𝑄) is the set of 𝑓 ∈ β„’2(𝑄) such that lim

𝑛→+∞βˆ₯ π‘“π‘›βˆ’ 𝑓 βˆ₯𝐻𝑝= 0 for some sequence (𝑓𝑛)π‘›βˆˆ 𝐼 𝑁 ∈ 𝐢Θ

𝑝 (𝑄)

We also let ℒ𝑔2be the subspace of β„’2(𝑄) containing the elements 𝑓 such that 𝑓(π‘₯, βˆ’π‘¦) = 𝑓(π‘₯, 𝑦) π‘Ž. 𝑒.

Likewise with ℒ𝑒2and 𝑓(π‘₯, βˆ’π‘¦) = βˆ’π‘“(π‘₯, 𝑦) π‘Ž. 𝑒 Finaly, we put

𝐿2= (β„’2)2, 𝐿 𝑔 2 = β„’

𝑔2Γ— ℒ𝑒2and ℒ𝑒2 = ℒ𝑒2Γ— ℒ𝑔2

It’s easy to prove that :

𝐿2= 𝐿 𝑔 2 βŠ• 𝐿

𝑒 2

IV.Fourier series

We consider the eigenvalue problem: 𝑦" + πœ†π‘¦ = 0 on

] βˆ’12,12[ with Neumann resp. Dirichlet boundary conditions.

In the first case we have a complete orthonormal (C.O.N) system in β„’2(𝑄):

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πœ‘2π‘˜+1= (βˆ’1)π‘˜βˆš2 sin((2π‘˜ + 1)πœ‹π‘¦)) for π‘˜ β‰₯ 0

Λ𝑝= 𝑝2πœ‹2 is an eigenvalue associated to πœ‘π‘, πœ‘2π‘˜ is even, πœ‘2π‘˜+1 odd and morever πœ‘π‘(1/2) = √2 for 𝑝 β‰₯ 1.

And in other case we have a (C.O.N) system given by

βˆšΞ›π‘πœ“π‘= πœ‘β€²π‘ where πœ“β€²π‘= βˆ’βˆšΞ›π‘πœ‘π‘ for 𝑝 β‰₯ 1. Since parity in 𝑦 will be important we introduce notations:

πœŽπ‘˜ = πœ‘2π‘˜+1, πœπ‘˜ = πœ“2π‘˜+1, πœ†π‘˜ = Ξ›2π‘˜+1, π‘˜ β‰₯ 0, and πœŒπ‘˜= πœ‘2π‘˜, πœ‹π‘˜ = πœ“2π‘˜ for π‘˜ β‰₯ 1, πœ‘0= 1 and πœ‡π‘˜ = πœ†2π‘˜ And for Θ ∈ π‘€πœ– we set: 𝛼̂ = (2πœ‹π›Ό + Θ)πΏβˆ’1, 𝛼 ∈ β„€ and 𝑒𝛼= 𝑒𝑖𝛼̂π‘₯.

We have a characterization of spaces 𝐻Θ,01 , 𝐻Θ1, 𝐻Θ2 with the Fourier series :

Let 𝑓 ∈ β„’2(𝑄) have Fourier series : 𝑓 = βˆ‘ 𝑓𝛼,π‘–πœ‘π‘– = βˆ‘ 𝑓̃𝛼,π‘–πœ“π‘–

With respect to {π‘’π›Όπœ‘π‘–} resp {π‘’π›Όπœ“π‘–}.

Proposition 4.1 (a) 𝑓 ∈ 𝐻Θ1iff

βˆ‘ (𝛼̂2+ Ξ›

𝑖)|𝑓𝛼,𝑖|2< ∞ (b) 𝑓 ∈ 𝐻Θ,01 iff

βˆ‘ (𝛼̂2+ Ξ›

𝑖)|𝑓̃𝛼,𝑖|2< ∞.

For the proof see [7].

We have the characterization of space 𝐻Θ2too :

Proposition 4.2

Let 𝑓 ∈ β„’2(𝑄) satisfy βˆ‘ (𝛼̂2+ Ξ›

𝑖)2|𝑓𝛼,𝑖|2< ∞. then 𝑓 ∈ 𝐻Θ2and :

βˆ₯ 𝑓 βˆ₯𝐻22≀ 𝐢(βˆ‘ (𝛼̂2+ Λ𝑖)2|𝑓𝛼,𝑖|2)

for a 𝐢 independent of Θ ∈ π‘€πœ–. Likewise with βˆ‘ (𝛼̂2+ Λ𝑖)2|𝑓̃𝛼,𝑖|2. For the proof see [7].

V. Main theorem

Our aim is to prove: Theorem 2

(π‘Ž) There is 𝐢 > 0 as follows: If π‘ˆ ∈ π‘‘π‘œπ‘š(𝐴𝑠(Θ)) ∩ 𝐸Θ

𝑔

and 𝐴𝑠(Θ)π‘ˆ = 𝑓 for some Θ ∈ π‘€πœ–, 𝑓 ∈ 𝐸Θ

𝑔

then π‘ˆ ∈ (𝐻Θ2)2 and β€–π‘ˆβ€–π»Β²β‰€ 𝐢‖𝑓‖ℒ²

βˆ₯ π‘ˆ βˆ₯𝐻2≀ 𝐢 βˆ₯ 𝑓 βˆ₯𝐿2.

(𝑏) Under the conditions π‘ˆ ∈ π‘‘π‘œπ‘š(𝐴𝑠(Θ)) ∩ πΈΞ˜π‘’ or π‘ˆ ∈ π‘‘π‘œπ‘š(𝐴𝑠(Θ)) ∩ 𝐸Θ the assertion (π‘Ž) holds.

Proposition 5.1

If 𝑓 ∈ 𝐻Θ1 has Fourier series βˆ‘π›Ό,𝑗 π‘Žπ›Ό,π‘—π‘’π›ΌπœŽπ‘— then βˆ‘π‘—|π‘Žπ›Ό,𝑗| ≀ ∞ and 𝑓 ∈ 𝐻Θ,01 iff βˆ‘π‘—π‘Žπ›Ό,𝑗 = 0, 𝛼 in β„€

For the proof of the proposition 5.1 see [7].

We need also the proposition 6.12 used in [7] page 115:

We recall πœ†π‘˜=

(2π‘˜+1)2

πœ‹2 :

Proposition 5.2 There are 𝛀0, 𝛀1 such that for 𝑠 β‰₯ 0: (i) Ξ“0(1 + 𝑠)βˆ’3≀ βˆ‘ (πœ†π‘˜+ 𝑠2)βˆ’2≀ Ξ“1(1 + 𝑠)βˆ’3 (ii) βˆ‘ (πœ†π‘˜+ 𝑠2)βˆ’1≀ Ξ“1(1 + 𝑠)βˆ’1

(iii)βˆ‘ πœ†π‘˜βˆ’1(πœ†

π‘˜+ 𝑠2)βˆ’2≀ Ξ“1(1 + 𝑠)βˆ’4 (iv)βˆ‘ πœ†π‘˜(πœ†π‘˜+ 𝑠2)βˆ’2≀ Ξ“1(1 + 𝑠)βˆ’1

VI.Proof of the main theorem

Since in the first part of the proof factor π›ΌΜ‚βˆ’1 appear which later cancel, it is advantagious to assume first

Θ ∈ π‘€Μ‡πœ–.

We take π‘ˆ = (𝐴, 𝐡) ∈ (𝐻Θ,01 ) ∩ 𝐿𝑔2 such that d𝑖𝑣 π‘ˆ = 0.

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π‘ˆ is a weak solution of 𝐴𝑠(Θ)π‘ˆ = 𝑓 for 𝑓 ∈ 𝐸Θ if and certain equations for the Fourier coefficients

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|𝐼𝑗|2≀ using Proposition 5.1 that there is a Θ βˆ’independent

𝐢2such that :

As indicated, due to the fact that the singularity Θ = 0 resp. Θ = 2πœ‹ drops out in the computations presented in the previous section, the spectral theory, carried out for dimension 𝑑 = 3 in [7] is simplified

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for such 𝑣 we set 𝐴𝑆(pπ‘’π‘Ÿ)𝑣 = πœˆπ’«pπ‘’π‘ŸΞ”π‘£, π‘€β„Žπ‘’π‘Ÿπ‘’ 𝒫pπ‘’π‘Ÿ is the orthogonal projection from β„’2(𝑄)2 onto 𝐸

pπ‘’π‘Ÿ. With this definition, 𝐴𝑠(pπ‘’π‘Ÿ) is selfadjoint on 𝐸pπ‘’π‘Ÿ. Finally, we need corresponding objects defined on the whole strip Ξ© = 𝐼𝑅 Γ—] βˆ’1

2, 1

2[. Thus 𝐸 is the β„’Β² βˆ’closure of 𝑓 ∈ 𝐻1(Ξ©) Γ— 𝐻

01(Ξ©) such that div 𝑓 = 0,

𝑓 ∈ dπ‘œπ‘š(𝐴𝑆) 𝑖𝑓𝑓 𝑓 ∈ (𝐻2(Ξ©) ∩ 𝐻01(Ξ©))2 π‘Žπ‘›π‘‘ 𝑑𝑖𝑣 𝑓 = 0,

and for such 𝑓 we set 𝐴𝑆𝑓 = πœˆπ’«Ξ”π‘“.

For elements 𝑓 ∈ dπ‘œπ‘š(𝐴𝑆), the operator 𝑇 acts again via (18). Under these conditions, the operators

𝐺 = 𝐴𝑆+ 𝒫𝑇, 𝐺Θ = 𝐴𝑆(Θ) + π’«Ξ˜π‘‡, 𝐺pπ‘’π‘Ÿ = 𝐴𝑆(pπ‘’π‘Ÿ) + 𝒫pπ‘’π‘Ÿπ‘‡

all become holomorphic semigroup generators on

𝐸, 𝐸Θ, 𝐸pπ‘’π‘Ÿ respectively. The spectral formulas, announced above now are:

(22)1 𝜎(𝐴𝑆+ 𝒫𝑇) = (β‹ƒΜ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Μ…Ξ˜βˆˆ[0,2πœ‹] (𝐴𝑆(Θ) + π’«Ξ˜π‘‡))

(22)2 𝜎(𝐴𝑆+ 𝒫𝑇) = ⋃ Θ∈[0,2πœ‹]

(𝐴𝑆(Θ) + π’«Ξ˜π‘‡).

These formulas correspond to formulas (*), (**) in [7], page. 169. While (22)1 looks the same as (*) in [7], (22)2 is definitely simpler; it implies in particular that if πœ† ∈ 𝜎(𝐴𝑆(pπ‘’π‘Ÿ) + 𝒫pπ‘’π‘Ÿπ‘‡) then πœ† ∈ 𝜎(𝐴𝑆+ 𝒫𝑇), a statement which cannot be asserted in dimension

𝑑 = 3 as can be seen from formula (**) in [7]. The proof of (22)2 is based on the computations in the present section 5, which entails that the singularities which arise in dimension 𝑑 = 3 in [7], drop out. The detailed verification of this claim is treated by a careful examination of the arguments in [7], a task within the scope of this paper.

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[2]. K.KirchgΓ€ssner, H.KielhΓΆfer, Stability and bifurcation in fluid dynamics, Rocky mountain J. of Math. Vol. 3, no. 2, 275-318 (1973). [3]. Pazy, A., Semigroupes of linear operators and

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