A necessary condition of potential blowup for the Navier–Stokes system in half-space

Assuming that T is a potential blow up time for the Navier–Stokes system in R 3 + , we show that the norm of the velocity ﬁeld in the Lorenz space L 3 , q with q < ∞ goes to ∞ as time t approaches T .


Introduction
The question that is addressed in the paper is as follows. Let us consider the initial boundary value problem for the Navier in . It is assumed that the initial velocity field v 0 is smooth, compactly supported, and divergence free in , i.e., v 0 belongs to the space C ∞ 0,0 ( ), and that is a domain in R 3 with sufficiently smooth boundary. Here, Our main aim is to study whether or not the velocity field v blows up in a finite time, in other words, whether or not there exists a finite time T > 0 such that There is a huge number of papers dedicated to this problem. Among them the most relevant to us are the following papers. In the first place, one should mention the classical Leray necessary conditions for T to be a blowup time: (1.5) for any 0 < t < T , for all s > 3, and for a positive constant c s depending only on s. Estimates (1.5) have been proven by Leray [11] for = R 3 and then by Giga [5] for a wide class of domains including a half space and bounded domains with sufficiently smooth boundaries. However, there is an interesting marginal case s = 3, in which no estimate of type (1.5) is known. In papers [3,14,17], it has been shown that lim sup Recent progress has been made in establishing the validity of (1.6) for other critical spaces. We refer to X , consisting of measurable functions acting on domains in R 3 , as critical if for u ∈ X such that u λ (x) = λu(λx) we have u λ X = u X . In [15,28], it was shown that when X is the non endpoint Lorentz space with q finite L 3,q (R 3 ) condition (1.6) remains to be true. Recently, Gallagher et al. proved in [4] that (1.6) holds for X =Ḃ −1+ 3 holds true? In [21] it is proven that this holds for = R 3 and X ( ) = L 3 (R 3 ) using the theory of local energy solutions in [10], in addition to ideas developed in [19,20]. The aim of the paper is to prove Theorem 1.1 Let = R 3 + . Let v : Q + → R 3 be a Leray-Hopf solution to (1.2)-(1.3), with initial data v 0 ∈ C ∞ 0,0 ( ). Suppose 3 q < ∞. Let T be a blow-up time. Then it necessarily holds that Before commenting further let us define the Lorentz spaces. For a measurable function f : → R define: Given a measurable subset ⊂ R n , the Lorentz space L p,q ( ), with p ∈]0, ∞[, q ∈]0, ∞], is the set of all measurable functions g on such that the quasinorm g L p,q ( ) is finite. Here: It is well known that for p ∈]0, ∞[, q 1 ∈]0, ∞] and q 2 ∈]0, ∞] with q 1 q 2 we have the following embedding L p,q 1 → L p,q 2 and the inclusion is known to be strict. Roughly speaking, the second index of Lorentz spaces gives information regarding nature of logarithmic bumps. For example, for any 1 > β > 0, q > 3 we have It should be stressed that, at the time of writing, (1.7) is open for the critical norm L 3,∞ ( ) that contains |x| −1 . Furthermore, uniqueness of weak Leray-Hopf solutions in the space L ∞ (0, T ; L 3,∞ ( )) remains open. We mention that interior regularity results, that have smallness condition on L ∞ (L 3,∞ ) norm, have been obtained in [8,9,12], for example. We would like to emphasise that to prove Theorem 1.1, a different approach is used to that of the whole space. Though we focus on the half space, this also provides an alternative to the proof given for the whole space in [21].
The main difficulty in attempts to prove Theorem 1.1 is as follows. The proof of this statement, for q = 3, in the case = R 3 consists of two big parts: rescaling, leading to a certain class of ancient solutions to the Navier-Stokes equations, and a Liouville type theorem for those solutions based on the backward uniqueness. The second part at least conceptually works in the case of a half space R 3 + as well while the first one does not. The reason is that the rescaling and the limiting procedure in the case of the whole space R 3 give the special type of the so-called local energy ancient solutions to the Navier-Stokes that coincide with Lemarie-Rieusset solutions to the Cauchy problem for the Navier-Stokes equations on some finite time interval. Those solutions have been introduced by Lemarie-Rieusset [10], see also for some definitions in [7]. Unfortunately, an analogue of Lemarie-Rieusset solutions for a half space is not known yet. In fact, this is an interesting open problem. In this paper, we are able to work without Lemarie-Rieusset type solutions in half space to get a local energy ancient solution to which a Liouville type theorem based on backward uniqueness is applicable. In comparison to [21], our approach doesn't require a notion of local energy solution, since we get all desired properties for the ancient solution directly from a priori estimates associated to the blow up procedure. Those ideas can be used for the construction of a global in time solution, for non energy initial data that is contained in the sum of certain Lesbesgue spaces, that applies in R 3 and is extendible to other unbounded domains with boundaries. Further developments in this direction will be published elsewhere. 1

Preliminaries
In this section, we will introduce notation that will be repeatedly used throughout the rest of the paper. For spatial domains and space time domains, we will make use of the following notation: For ⊂ R 3 , mean values of integrable functions are denoted as follows For, ⊂ R 3 , the space [C ∞ 0,0 ( )] L s ( ) is defined to be the closure of with respect to the L s ( ) norm. If X is a Banach space with norm · X , then L s (a, b; X ), a < b, will denote the usual Banach space of strongly measurable Xvalued functions f (t) on ]a, b[ such that the norm for s ∈ [1, ∞[, and with the usual modification if s = ∞. With this notation, we will define We define the following Sobolev spaces with the mixed norm: The analogues definitions for the above Sobolev spaces hold when the space-time domain is replaced by Q −T,0 .

A priori estimates
First we begin by stating and proving a simple (but important) fact about Lorentz spaces concerning a decomposition. This will be formulated as a Lemma. Analogous statement is Lemma II.I proven by Calderon [2]. Lemma 3.1 Take 1 < t < r < s ∞, and suppose that g ∈ L r,∞ ( ). For any N > 0, we let g N − := gχ |g| N and g N + := g − g N − . Then if s < ∞ and g N − L ∞ ( ) N , and

2)
Moreover for = R 3 or R 3 + , if g ∈ L r, p ( ) with 1 p ≤ ∞ and div g = 0 in weak sense (also g 3 (x , 0) = 0 for half space in weak sense), then g = g 1 + g 2 where and Proof Proof of decomposition (3.1), (3.2) can be found in [13]. Given g, satisfying assumptions of the lemma, we can find g 1 − and g 1 + . We then can use the Helmoltz-Weyl decomposition g 1 − = g 1 + ∇q 1 where g 1 belongs to the required space with the estimate The same is true for the second counterpart. So, we have Using properties of harmonic functions and the above global integrability of ∇q 1 and ∇q 2 , we conclude that ∇(q 1 + q 2 ) = 0. From this, from estimates (3.1), (3.2), and embedding L r, p ( ) into L r,∞ ( ), we derive the required estimates (3.3) and (3.4).
Let us consider a sufficiently smooth solution u and p to the Navier-Stokes system in the space-time strip Q + −2,0 = R 3 + ×] − 2, 0[ to the following initial boundary value problem: Suppose that The key observation for Lorentz spaces is as follows. From Lemma 3.1 (along with fact embedding into weak L 3 ) we may decompose: We then decompose u = v 1 + v 2 where v 1 and p 1 solve the linear problem Below we give some relevant estimates for the linear problem. We note that the cases k = 0, 1 and 10 3 l < ∞ follow from [27, Theorem 3.1]. The case l = ∞ can be obtained directly by using Solonnikov estimates for the Green function in half-space, see [26]. The relevant estimates are ( 10 3 l ∞, k = 0, 1, . . .): It is then seen that: The second counterpart of u satisfies the non-linear system The standard energy approach to the second system gives Next, let us consequently evaluate terms on the right hand side of the energy identity. For the first term, we have The second term can be treated as follows: Applying the known multiplicative inequality to the second factor in the right hand side of the latter bound, we find Letting and using the Young inequality, we find Next, elementary arguments lead to the inequality So, Using (3.9) and (3.11), it is easily seen that sup −2<t<0 From these estimates and from the multiplicative inequality, one can deduce that v 2 with any s ∈ [2, 10 3 ]. Moreover, Using (3.10) and (3.12), one can decompose Here, Using (3.12) and multiplicative inequalities, one can readily verify that Using (3.10) we see that Finally, using (3.12) and (3.10) we see that Putting everything together we have Let us fix a smooth cut-off function χ(t) so that χ(t) = 1 if −3/2 < t < 1 and χ(t) = 0 if −2 < t < −7/4. Then, we may split χ u and χ p in the following way: Our main tool here is the coercive estimates of the linear theory for the Stokes system developed in [25] when space and time exponents are the same and subsequently in [6,24] for unequal space time exponents. In particular, using (3.14) and (3.18)- (3.20) it follows from that and ∂ t u 3 In what follows, we are going to use the following Poincare type inequalities: 9 20 dt; dt. (3.27) All the formulae are valid provided B(x 0 , R) ⊂ R 3 + . They are also valid if we replace B(x 0 , R) with semi-balls B + (x 0 , R) assuming that x 03 = 0.

Passage to the limit
Suppose that we have a sequence of sufficiently smooth functions u (n) and p (n) defined in the domain Q + −2,0 = R 3 + ×]−2, 0[ that are solutions to the following initial boundary value problem: It is supposed also that Moreover, for any R > 0, the limits pair u and p satisfies the local energy inequality Proof Obviously, we may assume, without loss of generality, that (4.4) follows from (3.14) . Moreover, the limit function obeys the estimate u L 10/3 (Q + −2,0 ) < ∞. (4.11) By known compact embeddings we infer, that there exists a subsequence (denoted here by the original sequence) such that the following holds for any a > 0: (4.14) Using the above, along with the fact u (n) is bounded in L 10 3 (Q + −2,0 ), we can deduce (4.6). Now, let us treat the pressure p (n) , using the decomposition of the previous section Then, using (3.22)-(3.24) and (3.25)-(3.27), we can justify (4.7) and (4.8).
Since functions u (n) and p (n) satisfy the local energy inequality, i.e., we can find (4.9) by passing to the limits and taking into account (4.6) and (4.7).

Rescaling: scenario I
Let us go back to our original problem (1.1)-(1.3).
We assume that T > 0 is a blowup time. Theorem 1.1 can be proven ad absurdum. Suppose that there exists a sequence t n ↑ T such that then T is NOT a blowup time.
It is known that there exists a global weak Leray-Hopf solution (energy solution) to initial boundary value problem (1.1)-(1.3). This solution coincides with v on the interval ]0, T [ and that is why we are going to denote it still by v. Arguments similar to used in the previous section show that for every > 0 there exists R 1 ( ) > 0 such that So, by the definition of blowup time T , there should be a singular point Now let us focus on the first case, which will be referred to as 'Scenario I'. The case x 03 > 0 will be referred to as 'Scenario II'. We know from [16,18] that it must be for all 0 < a < a 0 , for some positive a 0 , and for some universal constant ε.
In this scenario, our rescaling will be as follows: where x = λ n y, t = T + λ 2 n s, λ n = T − t n 2 So, sufficiently smooth solutions u (n) and p (n) satisfy (4.1)-(4.3) with u (n) 0 (y) = λ n v(λ n y, t n ). Hence, Without loss of generality, we may assume . So, all assumptions and statements of Propositions 4.1 and 4.2 hold for u (n) and p (n) and for their limits u and p.
First examine the profile. Let us recall the known fact that The identification is as follows, if f ∈ L s , p (R 3 + ) and g ∈ L s, p (R 3 + ): Now, we mention that our assumption that v : R 3 + ×]0, ∞[→ R 3 is a weak Leray Hopf solution implies that v can be adjusted on some set of time of Lebesgue measure zero such that v(·, t) ∈ L 2 (R 3 + ). Moreover, for any ϕ(x) ∈ C ∞ 0 (R 3 + ) the following functional is continuous in time on [0, ∞[: Our assumption that v(·, t n ) L 3,q (R 3 + ) M implies by O'Neil's inequality that for ϕ ∈ C ∞ 0 (R 3 ): .
Hence, the weak-continuity implies . This implies, from the aforementioned facts regarding Lorentz spaces, that Now, we shall show that Indeed, it follows from (4.12)-(4.14) that |u(x, 0)|dx.
Using generalized Holder inequality for Lorentz spaces (along with scale invariance), it is not so difficult to show λ n a)) .

Rescaling: scenario II
Recall that 'Scenario II' refers to the case x 03 > 0 for the singular point at blowup time T . Here, the scaling is x = x 0 + λ n y. So, we replace R 3 + with R 3 h = {y = (y , y 3 ) ∈ R : y 3 > h} with h = h n = −x 03 /λ n .
In the case, sufficiently smooth functions u (n) and p (n) are a solution to the following initial boundary value problem: |u| 2 (∂ t ϕ 2 + ϕ 2 ) + u · ∇ϕ 2 (|u| 2 + 2 p)dxds (6.6) for all −3/2 < t 0 − R 2 < t ≤ t 0 ≤ 0, for all x 0 ∈ R 3 , and for all ϕ ∈ The proof of Proposition 6.1 goes along the lines of the proof of Proposition 4.1 with minor modifications. Scenario II can then be ruled out in the same way as in [21]. We would like to stress that a major simplification in Scenario II, compared with Scenario I, is related to showing non-triviality of the limit solution. In the interior case we may follow the local pressure decomposition used in [21] one of which is harmonic and the other satisfies a coercive estimate. Interior properties of harmonic functions are essential in the use of this decomposition for showing non-triviality of the limit function. In the boundary case of Scenario I the same decomposition doesn't apply. Instead, in order to show non-triviality, one uses a local decomposition of the velocity and pressure together with estimates for the Stokes system near the boundary as described in Scenario I.