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Quasi-periodic solutions for the incompressible Navier-Stokes equations with nonlocal diffusion

  • This paper studied the incompressible Navier-Stokes (NS) equations with nonlocal diffusion on Td(d2). Driven by a time quasi-periodic force, the existence of time quasi-periodic solutions in the Sobolev space was established. The proof was based on the decomposition of the unknowns into the spatial average part and spatial oscillating one. The former were sought under the Diophantine non-resonance assumption, and the latter by the contraction mapping principle. Moreover, by constructing suitable time weighted function space and using the Banach fixed point theorem, the asymptotic stability of quasi-periodic solutions and the exponential decay of perturbation were proved.

    Citation: Shuguan Ji, Yanshuo Li. Quasi-periodic solutions for the incompressible Navier-Stokes equations with nonlocal diffusion[J]. Electronic Research Archive, 2023, 31(12): 7182-7194. doi: 10.3934/era.2023363

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  • This paper studied the incompressible Navier-Stokes (NS) equations with nonlocal diffusion on Td(d2). Driven by a time quasi-periodic force, the existence of time quasi-periodic solutions in the Sobolev space was established. The proof was based on the decomposition of the unknowns into the spatial average part and spatial oscillating one. The former were sought under the Diophantine non-resonance assumption, and the latter by the contraction mapping principle. Moreover, by constructing suitable time weighted function space and using the Banach fixed point theorem, the asymptotic stability of quasi-periodic solutions and the exponential decay of perturbation were proved.



    Consider the following incompressible Navier-Stokes (NS) system with nonlocal diffusion

    {tu+(Δ)αu+p=uu+εf(ωt,x),u=0, (1.1)

    where the variables xTd=Rd/(2πZ)d(d2),tR. The field u(x,t) and scalar p(x,t) represent the velocity and pressure of fluid at point (x,t), respectively. The nonlocal operator (Δ)α with α(0,1) is defined by the Fourier transform on the torus

    (Δ)αu=kZd|k|2αˆu(k)eikx.

    The parameter ε is a small positive constant, and the time-dependent external force f(Tν,Td) is quasi-periodic with frequency ω=(ω1,,ων)Rν.

    The incompressible NS system with nonlocal diffusion describes the fluid motion with internal friction interaction [1], and corresponds a stochastic representation given in terms of stochastic differential equations driven by Lévy processes [2,3]. It has received increasing attention over the past few decades, and many interesting results have been established in several works [2,4,5,6,7,8,9,10]. For instance, see [4,5] for the global well-posedness, [6] for the regularity theory of Caffarelli-Kohn-Nirenberg and [8,9] for the ill-posedness of weak solutions.

    Concerning the time periodic solutions of system (1.1) with α=1, we refer the readers to [11,12,13,14,15] for the bounded domain cases, and to [16,17,18,19,20,21,22] for the unbounded domain cases. Serrin [11] proved the existence of time periodic solutions based on the solvability and stability of an initial value problem. Kozono and Nakao [16] converted the original time periodic problem into a mild formulation, and then established the existence and uniqueness of solutions by the Lp-Lq estimates of an associated semigroup and Kato iteration. Based on the decomposition of unknowns into a steady part and a purely periodic part, Kyed [17,18] derived the maximal regularity of the linearized problem and then established the unique existence of solutions for the nonlinear problem. Galdi, jointly with his collaborators [19,20,21], handled the scenario of flow around a rigid body, which moved or rotated in a prescribed periodic manner.

    Recently, Montalto [23] obtained the existence and stability of quasi-periodic solutions for incompressible NS equations on Td(d2). Some authors have applied the normal form method and celebrated the Kolmogorov-Arnold-Moser (KAM) theory to the NS and Euler equations (α=0), and obtained several intriguing results [24,25,26]. Baldi and Montalto [24] proved the existence of quasi-periodic solutions for Euler equations on T3. Montalto [25] considered the inviscid limit problem for the quasi-periodic solutions to the NS equations on T2. Berti, Hassainia and Masmoudi [26] proved the existence of vortex patches close to the Kirchhoff ellipses. In addition, Crouseilles and Faou [27] constructed an explicit quasi-periodic solution with compact support on T2, and a generalized version of the higher dimension was established in [28].

    However, regarding the time periodic problem for the general case of α(0,1), to the best of our knowledge there are few results available in the literature. Motivated by the works above, we would like to extend the results in [23] to system (1.1) and obtain the existence of quasi-periodic solutions near zero for α[1/2,1). It is worth mentioning that the remained case of solutions near zero for α(0,1/2) is hard to handle, which is due to the lack of the sufficient smoothing effect to control the nonlinear convection type term uu. Nevertheless, the issues considered in the present paper do not involve the small divisor problem due to the presence of dissipation.

    On one hand, to seek the quasi-periodic solutions uω(t):=U(ωt,x), pω(t):=P(ωt,x) of system (1.1), it suffices to solve the following equations:

    {ωφU+(Δ)αU+UU+P=εf(φ,x),U=0, (1.2)

    then one can decompose system (1.2) as a spatial averaged part and an oscillating one,

    ωφU0(φ)=εf0(φ) (1.3)

    and

    ωφUp+(Δ)αUp=P((UpUp)+εfp). (1.4)

    Here, the terms independent of x appear in the nonlinear term vanishes due to U=0. The first equation (1.3) could be solved under the assumption that the frequency ω is Diophantine, i.e., for some γ(0,1),

    |ω|γ||ν,Zν{0}. (1.5)

    The existence for the second equation (1.4) is obtained by means of the contraction mapping principle, provided that ε is suitably small. The main results are stated as follows.

    Theorem 1.1 (Existence). Let ν1, d2 and α[1/2,1), and let σ>ν/2, s>d/2+1 and Nmax{σ+ν,σ+s2α} be real numbers. Assume that f(ωt,x)CN(Tν×Td;Rd) is a time-dependent quasi-periodic function with Diophantine frequency ω and satisfies

    Tν×Tdf(φ,x)dxdφ=0, (1.6)

    then there exists a positive constant ε0 such that if εε0, system (1.1) admit time quasi-periodic solutions

    uω(t,x)=U(ωt,x)C(Tν;Hs)C1(Tν;Hs2α),pω(t,x)=P(ωt,x)C(Tν;Hs).

    Moreover,

    Tν×TdU(φ,x)dxdφ=0 (1.7)

    and

    UCφHsxC1φHs2αxCε,PCφHsxCε. (1.8)

    In particular, if f satisfies

    Tdf(φ,x)dx=0,φTν, (1.9)

    then the above conclusion holds for ωRν, and

    TdU(φ,x)dx=0,φTν.

    Remark 1.2. If we look for the quasi-periodic solutions near a constant vector ζRd satisfying a suitable assumption, a similar statement may be obtained for α(0,1) by the normal form method and KAM method. Precisely, solutions are written as

    u(t,x)=ζ+w(t,x),

    where w=0.

    Remark 1.3. It is easy to see that if U0(φ) is the solution of Eq (1.3), then U0+C(CRd) is also a solution of Eq (1.3). In this paper, we choose the zero order term as zero.

    On the other hand, let u(t,x)=uω(t,x)+v(t,x) and p(t,x)=pω(t,x)+q(t,x) be the perturbed quasi-periodic solutions. The asymptotic stability of quasi-periodic solutions uω(t,x), pω(t,x) can be investigated by studying the global existence of solutions for the following initial value problem

    {tv+(Δ)αv+q=uωvvuωvv,v=0, (1.10)

    with initial datum

    v0(x)=v(0,x). (1.11)

    By constructing time-weighted function space, we prove the global existence of small solutions by the Banach fixed point theorem. As a by product, we present the exponential decay estimates of the perturbation v.

    We state the asymptotic stability of quasi-periodic solutions as follows.

    Theorem 1.4 (Asymptotic stability). Let α(1/2,1), β(0,1) and the assumptions of Theorem 1.1 hold. Suppose that u0=u(0,x)Hs and

    Td(u0uω(0))dx=0. (1.12)

    Put

    E1=u0uω(0)Hs,

    then there exists a positive constant δ1 such that if E1δ1, the problems (1.10) and (1.11) have a unique global solution (v,q)C([0,),Hs). Moreover,

    Td(uuω)dx=0,t0, (1.13)

    and

    (uuω)(t)HsCE1eβt,(ppω)(t)HsCE1eβt,t0. (1.14)

    The paper is organized as follows. In Section 2, we give some function spaces and useful lemmas. Then, in Section 3, we prove the existence of time quasi-periodic solutions which have the same oscillation frequency with the f(ωt,x). Finally, the asymptotic stability of time quasi-periodic solutions obtained in Section 3 discussed in Section 4.

    This section collects some notations, function space and useful lemmas.

    We introduce some notations and function spaces used in this paper. For mN, let Zm0:=Zm{0}. Let P denote the Leray projection operator on solenoidal vector fields. We denote a generic positive constant by C. For any vectors u=(u1,u2,,ud) and v=(v1,v2,,vd), uv=(uivj)1i,jd represents the matrix-valued tensor product of u and v.

    For any u(x)L2(Td), one can expand it by the Fourier series [29]

    u(x)=kZdˆu(k)eixk,

    where the Fourier coefficients are given by

    ˆu(k)=1(2π)dTdu(x)eixkdx.

    Let π0 be the orthogonal projection operator defined by

    π0u(x):=1(2π)dTdu(x)dx=ˆu(0).

    For any s0,σ0, Hs=Hs(Td) is the standard Sobolev space with the norm

    uHs(Td)=(kZd(1+|k|2)s2|ˆu(k)|2)12.

    And let ˙Hs=˙Hs(Td) be the corresponding Sobolev space with the norm

    u˙Hs(Td)=(kZd|k|s|ˆu(k)|2)12.

    For any u(φ,x)L2(Tν;L2(Td)), one can expand it as

    u(φ,x)=ZνkZdˆu(,k)eiφeixk,

    where the Fourier coefficients are

    ˆu(,k)=1(2π)ν+dTdTνu(φ,x)eiφeixkdφdx.

    The function space Hσ,s=Hσ(Tν;Hs) is defined by

    Hσ,s={uL2(Tν;L2(Td))|uHσφHsx<+},

    where

    uHσφHsx=(ZνkZd(1+||2)σ2(1+|k|2)s2|ˆu(,k)|2)12.

    For an interval I and a Banach space X, Cm(I;X) denotes the space of m-times continuously differentiable functions on I with values in X. One can also define Cm(Tν,X) in a similar way.

    Lemma 2.1. Let σ>ν/2, ι0, then Hσ+ι(Tν) is compactly imbedded in Cι(Tν) and

    uCιCuHσ+ι.

    Note that Hs(Td) is a Banach algebra whenever s>d/2. The result below readily follows.

    Lemma 2.2. Let σ>ν/2, s>d/2, then one can get

    uvHsxuHsxvHsx (2.1)

    for u(x),v(x)Hs(Td), and

    uvHσφHsxuHσφHsxvHσφHsx (2.2)

    for u(φ,x),v(φ,x)Hσ(Tν;Hs(Td)).

    This section is devoted to establishing the existence of quasi-periodic solutions that have the same oscillation frequency as f for system (1.1).

    Proof. First, for Eq (1.3), by (1.6) we have

    U0(φ)=Zν0εˆf(,0)iωeiφ.

    Clearly, U0=0 and

    Tν×TdU0(φ)dxdφ=Td×TνU0(φ)dφdx=0.

    From the Diophantine condition (1.5) and the Hölder inequality, it follows that

    U0(φ)Hσφεγ1f0Hσ+νφCεγ1fHσ+νφH0x. (3.1)

    Next, for Eq (1.4), we would justify the solvability by the contraction mapping principle in the setting Hσ(Tν;Hs(Td)) with σ>ν/2, s>d/2+1. To this end, define the following function space

    Xσ,s={uHσ(Tν;Hs(Td)):u=0,π0u=0,uX<},

    where

    uX:=uHσφHsx.

    Let

    Lω:=ωφ+(Δ)α:Xσ+1,s+2αXσ,s.

    Owing to the operator Lω as invertible on Xσ,s, define the mapping

    T(u):=L1ωP(εfpuu), (3.2)

    where

    L1ωg(φ,x)=ZνkZd0ˆg(,k)iω+|k|2αeiφeikx.

    Now, it suffices to verify that the mapping T is a strict contraction on some closed ball in Xσ,s. Define the function space

    XR=Xσ,sR:={uXσ,s:uXR}.

    where R is a positive constant that will be determined later. For any uXσ,s, a direct calculation shows that

    L1ωu(φ,x)2HσφHs+2αxCZνkZd0(1+||2)σ|k|2(s+2α)|ˆu(,k)|2|iω+|k|2α|2CZνkZd0(1+||2)σ|k|2s|ˆu(,k)|2Cu2HσφHsx, (3.3)

    where we have used the equivalence of uHσφHsx and uHσφ˙Hsx, then for any uXR, it is easy to check that

    TνTdT(u)dxdφ=0andT(u)=0.

    From (3.3), Lemma 2.2 and the Sobolev embedding theorem, it follows that

    T(u)HσφHsx=L1ωP(εfpuu)HσφHsxC(εfpuu)HσφHs2αxCεfpHσφHs2αx+CuuHσφHs+12αxCεfCN+Cu2HσφHs+12αxC1ε+C2u2HσφHsx. (3.4)

    Taking R=4C1ε yields

    T(u)X2C1εR, (3.5)

    whenever ε1/(16C1C2). Moreover, for any u1,u2XR, from (3.2), (3.4) and Lemma 2.2, we have

    T(u1)T(u2)HσφHsxC2u1(u1u2)+u2(u1u2)HσφHs+12αxC2(u1HσφHsx+u2HσφHsx)u1u2HσφHsx2C2Ru1u2HσφHsx.

    Noting that R=4C1ε and ε1/(16C1C2), it gives us

    T(u1)T(u2)(t)X12u1u2X. (3.6)

    Combining (3.5) and (3.6), we arrive at T as a strict contraction from XR to XR. Thus, there exists a unique fixed point in XR of the mapping T, which is a unique time quasi-periodic solution Up of (1.4).

    Finally, we end the proof with the regularity of solution U=U0+Up. By Lemma 2.1, we have

    UCφHsxRCε.

    For the C1 regularity with respect to φ, from (1.3) and (1.4), it follows that

    φU0HσφCεf0HσφCε

    and

    φUpHσφHs2αC(Δ)αUp+P((UpUp)+εfp)HσφHs2αCUpHσφHs+CUp2HσφHs+CεfpHσφHs2αCε,

    hence,

    UC1φHs2αxCε.

    For the pressure P,

    PCφHsxCPHσφHsxCΔ1((UU)+εf)HσφHsxCU2HσφHsx+εfHσφHs1xCε.

    On the whole, we conclude that u(ωt,x)=U(φ,x) and p(ωt,x)=P(φ,x) are solutions of system (1.1) and satisfy the desired properties (1.7) and estimates (1.8). For the particular case of f satisfying (1.9), Eq (1.3) only admits a trivial solution U0=CRd and the verification of Eq (1.4) is similar with the above one. We omit here for simplification. The whole proof of Theorem 1.1 is completed.

    In this section, we prove the asymptotic stability of quasi-periodic solutions.

    Lemma 4.1. Let α[1/2,1),s0. Assume u0˙Hs satisfies π0u0=0, then it holds that

    et(Δ)αu0˙Hsetu0˙Hs,t>0. (4.1)

    Let 1s0s+1 and β(0,1), then for g˙Hs+1s0 satisfying π0g=0, it holds that

    et(Δ)αg˙HsCts02α(1β)s02αeβtg˙Hs+1s0,t>0. (4.2)

    Proof. We only prove (4.2). From Parseval's equality and the basic property of rapidly decaying functions, one can get

    et(Δ)αg2˙Hs=kZd0|k|2(s+1)e2t|k|2α|ˆg(k)|2=kZd0e2tβ|k|2α|k|2(s+1s0)|k|2s0e2t(1β)|k|2α|ˆg(k)|2e2βt(t(1β))s0αkZd0|k|2(s+1s0)|ˆg(k)|2×(t(1β)|k|α)2s0αe2t(1β)|k|2αCe2βt(t(1β))s0αkZd0|k|2(s+1s0)|ˆg(k)|2=Ce2βt(t(1β))s0αg2˙Hs+1s0.

    The lemma is proved.

    Denote

    B(u,v):=t0e(tτ)(Δ)αP(uv)(τ)dτ. (4.3)

    Lemma 4.2. Let α(1/2,1), β(0,1) and s>d/2. There holds that

    supt0eβtB(u,v)HsC3supt0eβtvHssupt0uHs, (4.4)
    supt0eβtB(u,v)HsC3supt0vHssupt0eβtuHs (4.5)

    and

    supt0eβtB(v,v)HsC3(supt0eβtvHs)2, (4.6)

    for u,vC([0,);Hs) and supt0eβtvHs<.

    Proof. Since the proof of (4.4) and (4.5) are similar, we only prove the former. If 0<t1, by (4.2) with s0=1 and Lemma 2.1, we have

    B(u,v)HsCt0e(tτ)(Δ)α(uv)(τ)Hs+1dτCt0eβ(tτ)(tτ)12α(1β)12α(uv)(τ)HsdτCeβtsupt0eβtvHssupt0uHs10τ12αdτCeβtsupt0eβtvHssupt0uHs.

    If t>1, we decompose the integral as

    t0e(tτ)(Δ)α(uv)(τ)Hs+1dτ=t10()dτ+tt1()dτ=:J1+J2.

    By changing variables, one can treat J2 similarly with the case 0<t1. For the term J1, from the Sobolev imbedding inequality and (4.2) with s0=s+1, it follows that

    J1t10(tτ)s+12α(1β)s+12αeβ(tτ)(uv)(τ)L2dτCeβtsupt0eβtvHssupt0uHst1τs+12αdτCeβtsupt0eβtvHssupt0uHs.

    Since eβt1 for any t0, the estimates (4.6) can be proved in a similar way. The lemma is proved.

    Now we turn back to the proof of Theorem 1.4.

    Proof. Note that

    q=(Δ)1((uωv+vuω+vv))

    and, therefore, we mainly focus on the unknown v(t,x) in the following. Due to Duhamel's principle, one can deduce that

    v=et(Δ)αv0t0e(tτ)(Δ)αP(vuω+uωv+vv)(τ)dτ.

    Therefore, define the following mapping

    Mv=et(Δ)αv0t0e(tτ)(Δ)αP(uωv+vuω+vv)(τ)dτ:=V0+B(uω,v)+B(v,uω)+B(v,v), (4.7)

    where B(,) is defined in (4.3). For 0<β<1 and s>d/2, define the following functional space

    YR:={uC([0,);Hs(Td)):uYR},

    where

    uY:=supt0eβtuHs.

    For the linear term, from (4.1) we get

    supt0eβtV0Hssupt0e(β1)tv0Hsv0Hs. (4.8)

    For the Duhamel integral terms, applying Lemma 4.2, one can get

    B(uω,v)+B(v,uω)Hs4C1C3eβtεvY, (4.9)

    and

    B(v,v)HsC3eβtv2Y. (4.10)

    Combining (4.8)–(4.10) yields

    MvYE1+4C1C3εvY+C3v2Y.

    Taking R=4E1, one can obtain

    MvY2E1R, (4.11)

    provided that E11/(32C3) and εmin{1/(16C1C2),1/(8C1C3)}. For any v1,v2YR, let vδ=v1v2, and we get

    M(v1)M(v2)Hst0e(tτ)(Δ)αP(uωvδ+vδuω)(τ)dτHs+t0e(tτ)(Δ)αP(v1vδ+vδv2)(τ)dτHsB(uω,vδ)Hs+B(vδ,uω)Hs+B(v1,vδ)Hs+B(vδ,v1)Hs.

    Applying Lemma 4.2 again, one can get

    M(v1)M(v2)Y4C1C3εv1v2Y+2C3Rv1v2Y34v1v2Y, (4.12)

    provided that E11/(32C3) and εmin{1/(16C1C2),1/(8C1C3)}. Combining estimates (4.11) and (4.12), one can see that map M is a strict contraction. We then obtain that there exists a unique fixed point v of the map M in YR, which is the unique solution of problems (1.10) and (1.11). Therefore, we conclude that the quasi-periodic solution in Theorem 1.1 is asymptotically stable. Moreover,

    uuωHs=vHsCE1eβt.

    This completes the proof of Theorem 1.4.

    The authors declare they have not used Artificial Intelligence (AI) tools in the creation of this article.

    This work is supported partially by NSFC Grants (12225103, 12071065 and 11871140) and the National Key Research and Development Program of China (2020YFA0713602 and 2020YFC1808301).

    The authors declare there is no conflicts of interest.



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