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Preprint submitted on 16 Feb 2018
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A non linear estimate on the life span of solutions of the three dimensional Navier-Stokes equations
Jean-Yves Chemin, Isabelle Gallagher
To cite this version:
Jean-Yves Chemin, Isabelle Gallagher. A non linear estimate on the life span of solutions of the three
dimensional Navier-Stokes equations. 2018. �hal-01690321v2�
A NON LINEAR ESTIMATE ON THE LIFE SPAN OF SOLUTIONS OF THE THREE DIMENSIONAL NAVIER-STOKES EQUATIONS
JEAN-YVES CHEMIN AND ISABELLE GALLAGHER
Abstract. The purpose of this article is to establish bounds from below for the life span of regular solutions to the incompressible Navier-Stokes system, which involve norms not only of the initial data, but also of nonlinear functions of the initial data. We provide examples showing that those bounds are significant improvements to the one provided by the classical fixed point argument. One of the important ingredients is the use of a scale-invariant energy estimate.
1. Introdution
In this article our aim is to give bounds from below for the life span of solutions to the incompressible Navier-Stokes system in the whole space R
3. We are not interested here in the regularity of the initial data: we focus on obtaining bounds from below for the life span associated with regular initial data. Here regular means that the initial data belongs to the intersection of all Sobolev spaces of non negative index. Thus all the solutions we consider are regular ones, as long as they exist.
Let us recall the incompressible Navier-Stokes system, together with some of its basic features. The incompressible Navier-Stokes system is the following:
(N S)
∂
tu − ∆u + u · ∇ u = −∇ p div u = 0 and u
|t=0= u
0,
where u is a three dimensional, time dependent vector field and p is the pressure, determined by the incompressibility condition div u = 0:
− ∆p = div(u · ∇ u) = X
1≤i,j≤3
∂
i∂
j(u
iu
j) .
This system has two fundamental properties related to its physical origin:
• scaling invariance
• dissipation of kinetic energy.
The scaling property is the fact that if a function u satisfies (N S) on a time interval [0, T ] with the initial data u
0, then the function u
λdefined by
u
λ(t, x)
def= λu(λ
2t, λx)
satisfies (N S) on the time interval [0, λ
−2T ] with the initial data λu
0(λ · ). This property is far from being a characteristic property of the system (N S). It is indeed satisfied by all systems of the form
(GN S)
∂
tu − ∆u + Q(u, u) = 0
u
|t=0= u
0with Q
i(u, u)
def= X
1≤j,k≤3
A
ij,k(D)(u
ju
k) where the A
ij,k(D) are smooth homogenenous Fourier multipliers of order 1. Indeed denoting by P the projection onto divergence free vector fields
P
def= Id − (∂
i∂
j∆
−1)
ij 1the Navier-Stokes system takes the form
∂
tu − ∆u + P div(u ⊗ u) = 0 u
|t=0= u
0,
which is of the type (GNS). For this class of systems, the following result holds. The definition of homogeneous Sobolev spaces ˙ H
sis recalled in the Appendix.
Proposition 1.1. Let u
0be a regular three dimensional vector field. A positive time T exists such that a unique regular solution to (GNS) exists on [0, T ]. Let T
⋆(u
0) be the maximal time of existence of this regular solution. Then, for any γ in the interval ]0, 1/2[, a constant c
γexists such that
(1) T
⋆(u
0) ≥ c
γk u
0k
−1 γ
H˙12 +2γ
.
In the case when γ = 1/4 for the particular case of (N S), this type of result goes back to the seminal work of J. Leray (see [8]). Let us point out that the same type of result can be proved for the L
3+1−6γ2γnorm.
Proof. This result is obtained by a scaling argument. Let us define the following function T
˙H12 +2γ
(r)
def= inf
T
⋆(u
0) , k u
0k
H˙12 +2γ= r .
We assume that at least one smooth initial data u
0develops singularites, which means exactly that T
⋆(u
0) is finite. Let us mention that this lower bound is in fact a minimum (see [10]).
Actually the function T
˙H12 +2γ
may be computed using a scaling argument. Observe that k u
0k
H˙12 +2γ= r ⇐⇒ k r
−2γ1u
0(r
−2γ1· ) k
H˙12 +2γ= 1 .
As we have T
⋆(u
0) = r
−γ1T
⋆r
−2γ1u
0(r
−2γ1· )
, we infer that T
˙H12 +2γ
(r) = r
−γ1T
˙H12 +2γ
(1) and thus that
T
⋆(u
0) ≥ c
γk u
0k
−1 γ
H˙12 +2γ
with c
γdef= T
˙H12 +2γ
(1) .
The proposition is proved. ✷
Now let us investigate the optimality of such a result, in particular concerning the norm appearing in the lower bound (1). Useful results and definitions concerning Besov spaces are recalled in the Appendix; the Besov norms of particular interest in this text are the ˙ B
∞,2−1norm which is given by
k a k
B˙−∞1,2def
= Z
∞0
k e
t∆a k
2L∞dt
12and the Besov norms ˙ B
−σ∞,∞for σ > 0 which are
k a k
B˙∞−σ,∞def
= sup
t>0
t
σ2k e
t∆a k
L∞.
It has been known since [6] that a smooth initial data in ˙ H
12(corresponding of course to the limit case γ = 0 in Proposition 1.1) generates a smooth solution for some time T > 0. Let us point out that in dimension 3, the following inequality holds
k a k
B˙∞−1,2. k a k
H˙12.
The norms ˙ B
∞,∞−σare the smallest norms invariant by translation and having a given scaling.
More precisely, we have the following result, due to Y. Meyer (see Lemma 9 in [9]).
2
Proposition 1.2. Let d ≥ 1 and let (E, k · k
E) be a normed space continuously included in S
′( R
d), the space of tempered distributions on R
d. Assume that E is stable by translation and by dilation, and that a constant C
0exists such that
∀ (λ, e) ∈ ]0, ∞ [ ×R
d, ∀ a ∈ E , k a(λ · − e) k
E≤ C
0λ
−σk a k
E. Then a constant C
1exists such that
∀ a ∈ E , k a k
B˙−α∞,∞≤ C
1k a k
E.
Proof. Let us simply observe that, as E is continuously included in S
′( R
d), a constant C exists such that for all a in E,
h a, e
−|·|2i ≤ C k a k
E.
Then by invariance by translation and dilation of E, we infer immediately that k e
t∆a k
L∞≤ C
1t
−σ2k a k
Ewhich proves the proposition. ✷
Now let us state a first improvement to Proposition 1.1 where the life span is bounded from below in terms of the ˙ B
∞,∞−1+2γnorm of the initial data.
Theorem 1.1. With the notations of Proposition 1.1, for any γ in the interval ]0, 1/2[, a constant c
′γexists such that
(2) T
⋆(u
0) ≥ T
FP,γ(u
0)
def= c
′γk u
0k
−1 γ
B˙∞−1+2γ,∞
.
This theorem is proved in Section 2; the proof relies on a fixed point theorem in a space included in the space of L
2in time functions, with values in L
∞.
Let us also recall that if a scaling 0 norm of a regular initial data is small, then the solution of (N S) associated with u
0is global. This a consequence of the Koch and Tataru theorem (see [7]) which can be translated as follows in the context of smooth solutions.
Theorem 1.2. A constant c
0exists such that for any regular initial data u
0satisfying k u
0k
BM O−1def
= sup
t>0
t
12k e
t∆u
0k
L∞+ sup
x∈R3 R>0
1 R
3Z
R2 0Z
B(x,R)
| e
t∆u
0(y) |
2dydt
12≤ c
0, the associate solution of (GN S) is globally regular.
Let us remark that
k u
0k
B˙∞−1,∞≤ k u
0k
BM O−1≤ k u
0k
B˙∞−1,2.
We shall explain in Section 2 how to deduce Theorem 1.2 from the Koch and Tataru theorem [7].
The previous results are valid for the whole class of systems (GN S). Now let us present the second main feature of the incompressible Navier-Stokes system, which is not shared by all systems under the form (GN S) as it relies on a special structure of the nonlinear term (which must be skew-symmetric in L
2): the dissipation estimate for the kinetic energy. For regular solutions of (N S) there holds
1 2
d
dt k u(t) k
2L2+ k∇ u(t) k
2L2= 0 which gives by integration in time
(3) ∀ t ≥ 0 , E u(t)
def= 1
2 k u(t) k
2L2+ Z
t0
k∇ u(t
′) k
L2dt
′= 1
2 k u
0k
2L2.
3
T. Tao pointed out in his paper [11] that the energy estimate is not enough to prevent possible singularities from appearing. Our purpose here is to investigate if this energy estimate can improve the lower bound (2) of the life span for regular initial data. We recall indeed that for smooth initial data, all Leray solutions — meaning solutions in the sense of distributions satisfying the energy inequality
(4) E u(t)
≤ 1 2 k u
0k
2L2coincide with the smooth solution as long as the latter exists.
What we shall use here is a rescaled version of the energy dissipation inequality in the spirit of [5], on the fluctuation w
def= u − u
Lwith u
L(t)
def= e
t∆u
0.
Proposition 1.3. Let u be a regular solution of (N S) associated with some initial data u
0. Then the fluctuation w satisfies, for any positive t
E w(t) t
14+ Z
t0
k w(t
′) k
2L2t
′32dt
′. Q
0Lexp k u
0k
2B˙∞−1,2with Q
0Ldef= Z
∞0
t
12k P (u
L·∇ u
L)(t) k
2L2dt . Our main result is then the following.
Theorem 1.3. There is a constant C > 0 such that the following holds. For any regular initial data of (N S),
(5) T
∗(u
0) > T
L(u
0)
def= C Q
0L−2k ∂
3u
0k
2B˙
−32
∞,∞
Q
0L+ q
Q
0LQ
1L−2exp − 4 k u
0k
2B˙∞−1,2,
with
Q
1Ldef= Z
∞0
t
32∂
32P (u
L· ∇ u
L) (t)
2L2
dt . The main two features of this result are that
• the statement involves non linear quantities associated with the initial data, namely norms of P (u
L· ∇ u
L);
• one particular (arbitrary) direction plays a specific role.
This theorem is proved in Section 4.
The following statement shows that the lower bound on T
∗(u
0) given in Theorem 1.3 is, for some classes of initial data, a significant improvement.
Theorem 1.4. Let (γ, η) be in ]0, 1/2[ × ]0, 1[. There is a constant C and a family (u
0,ε)
ε∈]0,1[of regular initial data such that with the notation of Theorems 1.1 and 1.3, T
FP(u
0,ε) = Cε
2| log ε |
−1γand T
L(u
0,ε) ≥ Cε
−2+η.
This theorem is proved in Section 5. The family (u
0,ε)
ε∈]0,1[is closely related to the family used in [3] to exhibit families of initial data which do not obey the hypothesis of the Koch and Tataru theorem and which nevertheless generate global smooth solutions. However it it too large to satisfy the assumptions of Theorem 2 in [3] so it is not known if the associate solution is global.
In the following we shall denote by C a constant which may change from line to line, and we shall sometimes write A . B for A ≤ CB .
4
2. Proof of Theorem 1.1
Let u
0be a smooth vector field and let us solve (GN S) by means of a fixed point method.
We define the bilinear operator B by (6) ∂
tB(u, v) − ∆B(u, v) = − 1
2 Q(u, v) + Q(v, u)
, and B(u, v) |
t=0= 0 . One can decompose the solution u to (GN S) into
u = u
L+ B (u, u) .
Resorting to the Littlewood-Paley decomposition defined in the Appendix, let us define for any real number γ and any time T > 0, the quantity
k f k
ETγdef
= sup
j∈Z
2
−j(1−2γ)k ∆
jf k
L∞([0,T]×R3)+ 2
2jk ∆
jf k
L1([0,T];L∞(R3)).
Using Lemma 2.1 of [2] it is easy to see that
k u
Lk
E∞γ. k u
0k
B˙−∞1+2γ,∞,
so Theorem 1.1 will follow from the fact that B maps E
Tγ× E
Tγinto E
Tγwith the following estimate:
(7) k B(u, v) k
ETγ≤ C
γT
γk u k
ETγk v k
ETγ.
So let us prove (7). Using again Lemma 2.1 of [2] along with the fact that the A
ik,ℓ(D) are smooth homogeneous Fourier multipliers of order 1, we have
k ∆
jB(u, v)(t) k
L∞. Z
t0
e
−c22j(t−t′)
2
j∆
ju(t
′) ⊗ v(t
′) + v(t
′) ⊗ u(t
′)
k
L∞dt
′.
We then decompose (component-wise) the product u ⊗ v following Bony’s paraproduct algo- rithm: for all functions a and b the support of the Fourier transform of S
j′+1a∆
j′b and S
j′b∆
j′a is included in a ball 2
j′B where B is a fixed ball of R
3, so one can write for some fixed con- stant c > 0
ab = X
2j′≥c2j
S
j′+1a∆
j′b + ∆
j′aS
j′b so thanks to Young’s inequality in time one can write
2
−j(1−2γ)k ∆
jB (u, v) k
L∞([0,T]×R3)+ 2
2jk ∆
jB(u, v ) k
L1([0,T];L∞(R3)). B
1j(u, v) + B
2j(u, v) with B
1j(u, v)
def= 2
2jγX
2j′≥max{c2j,T−12}
k S
j′+1u k
L∞([0,T]×R3)k ∆
j′v k
L1([0,T];L∞(R3))+ 2
2jγX
c2j≤2j′<T−12
k S
j′+1u k
L∞([0,T]×R3)k ∆
j′v k
L1([0,T];L∞(R3))and
B
2j(u, v)
def= 2
2jγX
2j′≥max{c2j,T−12}
k S
j′v k
L∞([0,T]×R3)k ∆
j′u k
L1([0,T];L∞(R3))+ 2
2jγX
c2j≤2j′<T−12
k S
j′v k
L∞([0,T]×R3)k ∆
j′u k
L1([0,T];L∞(R3)). (8)
In each of the sums over c2
j≤ 2
j′< T
−12we write
k f k
L1([0,T];L∞(R3))≤ T k f k
L∞([0,T]×R3) 5and we can estimate the two terms B
j1(u, v) and B
2j(u, v) in the same way: for ℓ ∈ { 1, 2 } there holds indeed
B
jℓ(u, v) ≤ k u k
EγTk v k
ETγ2
2jγX
2j′≥max{c2j,T−12}
2
−4j′γ+ T 2
2j(1−γ)X
c≤2j′ −j<(22jT)−12
2
2(j′−j)(1−2γ)≤ k u k
EγTk v k
ETγT
γ+ T 2
2j(1−γ)X
c≤2j′ −j<(22jT)−12
2
2(j′−j)(1−2γ).
Once noticed that
T 2
2j(1−γ)X
c≤2j′ −j<(22jT)−12
2
2(j′−j)(1−2γ)≤ 1
{22jT≤C}(T2
2j)
γ2
−2jγ. T
γthe estimate (7) is proved and Theorem 1.1 follows.
3. Proof of Theorem 1.2
As the solutions given by the Fujita-Kato theorem [6] and the Koch-Tataru theorem [7]
are unique in their own class, they are unique in the intersection and thus coincide as long as the Fujita-Kato solution exists. Thus Theorem 1.2 is a question of propagation of regularity, which is provided by the following lemma (which proves the theorem).
Lemma 3.1. A constant c
0exists which satisfies the following. Let u be a regular solution of (GN S) on [0, T [ associated with a regular initial data u
0such that
k u k
Kdef
= sup
t∈[0,T[
t
12k u(t) k
L∞≤ c
0. Then T
⋆(u
0) > T .
Proof. The proof is based on a paralinearization argument (see [2]). Observe that for any T less than T
⋆(u
0), u is a solution on [0, T [ of the linear equation
(P GN S)
∂
tv − ∆v + Q (u, v) = 0
v
|t=0= u
0with Q (u, v)
def= X
j∈Z
Q(S
j+1u, ∆
jv) + X
j∈Z
Q(∆
jv, S
ju) . In the same spirit as (6), let us define P B(u, v) by
(9) ∂
tP B(u, v) − ∆P B(u, v) = −Q (u, v) and P B(u, v) |
t=0= 0 . A solution of (P GN S) is a solution of
v = u
L+ P B(u, v) .
Let us introduce the space F
Tof continuous functions with values in ˙ H
12, which are elements of L
4([0, T ]; ˙ H
1), equipped with the norm
k v k
FTdef
= X
j∈Z
2
jk ∆
jv k
2L∞([0,T[;L2) 12+ k v k
L4([0,T[; ˙H1).
Notice that the first part of the norm was introduced in [4] and is a larger norm than the supremum in time of the ˙ H
12norm. Moreover there holds
k u
Lk
FT. k u
0k
H˙12. Let us admit for a while the following inequality:
(10) k P B(u, v) k
FT. k u k
Kk v k
FT.
6
Then it is obvious that if k u k
Kis small enough for some time [0, T [, the linear equation (P GN S) has a unique solution in F
T(in the distribution sense) which satisfies in particular, if c
0is small enough,
k v k
FT≤ C k u
0k
H˙12+ 1
2 k v k
FT. As u is a regular solution of (P GN S), it therefore satisfies
∀ t < T , k u k
L4([0,t]; ˙H1)≤ 2C k u
0k
H˙12which implies that T
⋆(u
0) > T , so the lemma is proved provided we prove Inequality (10).
Let us observe that for any j in Z ,
(11) ∂
t∆
jP B(u, v ) − ∆∆
jP B(u, v) = − ∆
jQ (u, v) . By definition of Q , we have
∆
jQ (u, v)(t) k
L2≤ X
j′∈Z
X
1≤i,k,ℓ≤3
∆
jA
ik,ℓ(D) S
j′+1u∆
j′v
L2+ ∆
jA
ik,ℓ(D) ∆
j′vS
j′u
L2. As A
ik,ℓ(D) are smooth homogeneous Fourier multipliers of order 1, we infer that for some fixed nonnegative integer N
0∆
jQ (u, v)(t) k
L2. 2
jX
j′≥j−N0
S
j′+1u(t)∆
j′v(t)
L2
+ ∆
j′v(t)S
j′u(t)
L2
. 2
jX
j′≥j−N0
k S
j′+1u(t) k
L∞k ∆
j′v(t) k
L2+ ∆
j′v(t) k
L2k S
j′u(t)
L∞. 2
jk u(t) k
L∞X
j′≥j−N0
k ∆
j′v(t) k
L2.
Using Relation (11) and the definition of the norm on F
T, we infer that k ∆
jP B(u, v)(t) k
L2≤
Z
t 0e
−c22j(t−t′)∆
jQ (u, v)(t
′) k
L2dt
′. 2
jZ
t 0e
−c22j(t−t′)k u(t
′) k
L∞X
j′≥j−N0
k ∆
j′v(t
′) k
L2dt
′. 2
jk u k
Kk v k
FTX
j′≥j−N0
c
j′2
−j′ 2
Z
t 0e
−c22j(t−t′)1
√ t
′dt
′,
where (c
j)
j∈Zdenotes a generic element of the sphere of ℓ
2( Z ). Thus we have, for all t less than T ,
2
j2k ∆
jP B (u, v)(t) k
L2. k u k
Kk v k
FTX
j′≥j−N0
c
j′2
−j′−j 2
Z
t 02
je
−c22j(t−t′)1
√ t
′dt
′.
Thanks to Young’s inequality, we have X
j′≥j−N0
c
j′2
−j′−j
2
. c
jand we deduce that
(12) 2
j2k ∆
jP B(u, v)(t) k
L2. c
jk u k
Kk v k
FTZ
t 02
je
−c22j(t−t′)1
√ t
′dt
′. As we have
Z
t 02
je
−c22j(t−t′)1
√ t
′dt
′. Z
t0
√ 1 t − t
′√ 1 t
′dt
′,
7
we infer finally that
(13) X
j∈Z
2
jk ∆
jP B(u, v) k
2L∞([0,T];L2). k u k
2Kk v k
2FT. Moreover returning to Inequality (12), we have
2
jk ∆
jP B(u, v) k
L4([0,T];L2). c
jk u k
Kk v k
FTZ
t 02
3j2e
−c22j(t−t′)1
√ t
′dt
′L4(R+)
. The Hardy-Littlewood-Sobolev inequality implies that
Z
t 02
3j2e
−c22j(t−t′)1
√ t
′dt
′L4(R+)
. 1 . Since thanks to the Minkowski inequality there holds
k P B(u, v) k
2L4([0,T]; ˙H1)≤ X
j∈Z
2
2jk ∆
jP B(u, v) k
2L4([0,T];L2),
together with Inequality (13) this concludes the proof of Inequality (10) and thus the proof
of Lemma 3.1. ✷
4. Proof of Theorem 1.3
The plan of the proof of Theorem 1.3 is the following: as previously we look for the solution of (N S) under the form
u = u
L+ w
where we recall that u
L(t) = e
t∆u
0. Moreover we recall that the solution u satisfies the energy inequality (4). By construction, the fluctuation w satisfies
(NSF) ∂
tw − ∆w + (u
L+ w) · ∇ w + w · ∇ u
L= − u
L· ∇ u
L− ∇ p , div w = 0 . Let us prove that the life span of w satisfies the lower bound (5). The first step of the proof consists in proving Proposition 1.3, stated in the introduction. This is achieved in Section 4.1.
The next step is the proof of a similar energy estimate on ∂
3w — note that contrary to the scaled energy estimate of Proposition 1.3, the next result is useful in general only locally in time. It is proved in Section 4.2.
Proposition 4.1. With the notation of Proposition 1.3 and Theorem 1.3, the fluctuation w satisfies the following estimate:
E ∂
3w
(t) .
Q
0Lt
12sup
t′∈(0,t)
k ∂
3w(t) k
4L2+ k ∂
3u
0k
2˙B
−32
∞,∞
+ q
Q
0LQ
1Lexp 2 k u
0k
2B˙∞,2−1. Combining both propositions, one can conclude the proof of Theorem 1.3. This is performed in Section 4.3.
4.1. The rescaled energy estimate on the fluctuation: proof of Proposition 1.3.
An L
2energy estimate on (NSF) gives 1
2 d
dt k w(t) k
2L2+ k∇ w(t) k
2L2= − X
1≤j,k≤3
Z
R3
w
j∂
ju
kLw
k(t, x)dx − P (u
L· ∇ u
L) w (t) .
¿From this, after an integration by parts and using the fact that the divergence of w is zero, we infer that
1 2
d dt
k w(t) k
2L2t
12+ k w(t) k
2L22t
32+ k∇ w(t) k
2L2t
12≤ k w(t) k
L2k u
L(t) k
L∞k∇ w(t) k
L2t
12+ k P (u
L· ∇ u
L)(t) k
L2k w(t) k
L2t
12·
8
Let us observe that
k P (u
L· ∇ u
L)(t) k
L2k w(t) k
L2t
12= t
14k P (u
L· ∇ u
L)(t) k
L2k w(t) k
L2t
34· Using a convexity inequality, we infer that
d dt
k w(t) k
2L2t
12+ k w(t) k
2L22t
32+ k∇ w(t) k
2L2t
12≤ k w(t) k
2L2k u
L(t) k
2L∞t
12+ t
12k u
L(t) · ∇ u
L(t) k
2L2. Thus we deduce that
d dt
k w(t) k
2L2t
12exp
− Z
t0
k u
L(t
′) k
2L∞dt
′+ exp
− Z
t0
k u
L(t
′) k
2L∞dt
′k w(t) k
2L22t
32+ k∇ w(t) k
2L2t
12≤ exp
− Z
t0
k u
L(t
′) k
2L∞dt
′t
12k P (u
L· ∇ u
L)(t) k
2L2, from which we infer by the definition of the ˙ B
∞,2−1norm and of Q
0Lthat
(14) ∀ t ≥ 0 , k w(t) k
2L2t
12+ Z
t0
k w(t
′) k
2L22t
′32+ k∇ w(t) k
2L2t
′12dt
′≤ Q
0Lexp k u
0k
2B˙−∞1,2.
Proposition 1.3 follows.
4.2. Proof of Proposition 4.1. Now let us investigate the evolution of ∂
3w in L
2. Applying the partial differentiation ∂
3to (NSF), we get
(15) ∂
t∂
3w − ∆∂
3w + (u
L+ w) · ∇ ∂
3w + ∂
3w · ∇ u
L= − ∂
3u
L· ∇ w − ∂
3w · ∇ w − w · ∇ ∂
3u
L− ∂
3(u
L· ∇ u
L) − ∇ ∂
3p .
The difficult terms to estimate are those which do not contain explicitly ∂
3w. So let us define (a)
def= − ∂
3u
L· ∇ w ∂
3w
L2
, (b)
def= − w · ∇ ∂
3u
L∂
3w)
L2and (c)
def= − ∂
3(u
L· ∇ u
L) ∂
3w
L2
.
The third term is the easiest. By integration by parts and using the Cauchy-Schwarz inequality along with (14) we have
Z
∞ 0(c)(t)dt = Z
∞0
Z
R3
∂
32P (u
L· ∇ u
L)(t, x)
· w(t, x)dxdt
≤ Z
∞0
t
32∂
32P (u
L· ∇ u
L)(t)
2L2dt
12Z
∞0
k w(t) k
2L2t
32dt
12≤ q
Q
0LQ
1Lexp 1
2 k u
0k
2B˙∞−1,2.
Now let us estimate the contribution of (a) and (b). By integration by parts, we get, thanks to the divergence free condition on u
L,
(a) = ∂
3u
L⊗ w ∇ ∂
3w
L2
and (b) = w ⊗ ∂
3u
L∇ ∂
3w)
L2.
The two terms can be estimated exactly in the same way since they are both of the form Z
R3
w(t, x)∂
3u
L(t, x) ∇ ∂
3w(t, x)dx .
9
We have Z
R3
w(t, x)∂
3u
L(t, x) ∇ ∂
3w(t, x)dx ≤ k w(t) k
L2k ∂
3u
L(t) k
L∞k∇ ∂
3w k
L2≤ 1
100 k∇ ∂
3w k
2L2+ 100 k w(t) k
2L2k ∂
3u
L(t) k
2L∞. The first term will be absorbed by the Laplacian. The second term can be understood as a source term. By time integration, we get indeed
Z
T0
k w(t) k
2L2k ∂
3u
L(t) k
2L∞dt ≤ Z
T0
k w(t) k
2L2t
32t
34k ∂
3u
L(t) k
L∞ 2dt
≤ k ∂
3u
0k
2B˙
−32
∞,∞
Z
∞ 0k w(t) k
2L2t
23dt , so it follows, thanks to Proposition 1.3, that
Z
T 0Z
R3
w(t, x)∂
3u
L(t, x) ∇ ∂
3w(t, x)dxdt ≤ 1 100
Z
T0
k∇ ∂
3w(t) k
2L2dt + C k ∂
3u
0k
2B˙−
32
∞,∞
Q
0Lexp k u
0k
2B˙−∞1,2.
The contribution of the quadratic term in (15) is estimated as follows: writing, for any func- tion a,
k a k
LphLqvdef
= Z
k a(x
1, x
2, · ) k
pLq(R)dx
1dx
21p, we have by H¨older’s inequality
Z
R3
∂
3w(t, x) · ∇ w(t, x)∂
3w(t, x)dx ≤ k ∂
3w(t) k
2L2vL4hk∇ w k
L∞v L2h≤ k ∂
3w(t) k
L2k∇
h∂
3w(t) k
L2k∇ w(t) k
1 2
L2
k∇ ∂
3w(t) k
1 2
L2
, where we have used the inequalities
(16) k a k
L∞v L2h. k ∂
3a k
1 2
L2
k a k
1 2
L2
and k a k
L2vL4h. k a k
1 2
L2
k∇
ha k
1 2
L2
with ∇
hdef= (∂
1, ∂
2). The first inequality comes from k a( · , x
3) k
2L2h= 1
2 Z
x3−∞
∂
3a( · , z) a( · , z)
L2h
dz
≤ 1 2
Z
R
k ∂
3a( · , z) k
L2hk a( · , z) k
L2hdz
≤ k ∂
3a k
L2k a k
L2while the second simply comes from the embedding ˙ H
h12⊂ L
4hand an interpolation. By Young’s inequality it follows that
Z
R3
∂
3w(t, x) · ∇ w(t, x)∂
3w(t, x)dx ≤ 1
100 k∇ ∂
3w k
2L2+ C k∇ w(t) k
2L2k ∂
3w(t) k
4L2≤ 1
100 k∇ ∂
3w(t) k
2L2+ sup
t′∈[0,t]
k ∂
3w(t
′) k
4L2t
12k∇ w(t) k
2L2t
12,
10