<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Millennium Prize on Nam Le</title><link>https://blog.namln.org/en/tags/millennium-prize/</link><description>Recent content in Millennium Prize on Nam Le</description><generator>Hugo</generator><language>en-US</language><lastBuildDate>Fri, 29 May 2026 00:00:00 +0000</lastBuildDate><atom:link href="https://blog.namln.org/en/tags/millennium-prize/index.xml" rel="self" type="application/rss+xml"/><item><title>Navier–Stokes Existence and Smoothness</title><link>https://blog.namln.org/en/posts/navier-stokes-existence-smoothness/</link><pubDate>Fri, 29 May 2026 00:00:00 +0000</pubDate><guid>https://blog.namln.org/en/posts/navier-stokes-existence-smoothness/</guid><description>&lt;p&gt;The motion of a viscous incompressible fluid is described by the Navier–Stokes
equations, first written down by Claude-Louis Navier in 1822 and given their modern
form by George Gabriel Stokes. Whether smooth solutions to these equations can
always be continued for all time (or whether they can spontaneously develop a
singularity at some finite time) is one of the deepest open problems in mathematics,
and one of the seven &lt;a href="https://www.claymath.org/millennium-problems/"&gt;Clay Millennium Prize Problems&lt;/a&gt;,
carrying a 1,000,000$ prize for a solution.&lt;/p&gt;
&lt;div style="padding:10px 14px; border:2px solid dodgerblue; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:dodgerblue; font-weight:bold;"&gt;Problem (Clay Millennium Prize, Fefferman 2000)&lt;/span&gt;
&lt;p&gt;Let $u_0 : \mathbb{R}^3 \to \mathbb{R}^3$ be a smooth divergence-free vector field.
Does there exist a smooth solution $u(x,t)$, $p(x,t)$ to the 3D incompressible
Navier–Stokes equations
$$\partial_t u + (u \cdot \nabla)u - \nu\Delta u + \nabla p = 0, \qquad \nabla \cdot u = 0,
\qquad u(\cdot,0) = u_0$$
defined for all $t &amp;gt; 0$ and satisfying $\int_{\mathbb{R}^3}|u(x,t)|^2,dx &amp;lt; C$
for all $t \geq 0$? A solution or a counterexample (a smooth $u_0$ for which no
such smooth solution exists) both qualify for the prize.&lt;/p&gt;
&lt;/div&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="the-equations-and-their-scaling"&gt;
 The Equations and Their Scaling&lt;span class="heading__anchor"&gt; &lt;a href="#the-equations-and-their-scaling"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;Compared to the Euler equations (which describe inviscid flow), the Navier–Stokes
equations add the viscous term $\nu\Delta u$, where $\nu &amp;gt; 0$ is the kinematic
viscosity. This term dissipates energy and regularises the flow locally. The central
tension is that the nonlinear term $(u\cdot\nabla)u$ can concentrate energy at
small spatial scales faster than viscosity can diffuse it away.&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;Scaling symmetry.&lt;/strong&gt; The Navier–Stokes equations are invariant under the rescaling
$$u(x,t) \mapsto \lambda u(\lambda x,, \lambda^2 t), \qquad
p(x,t) \mapsto \lambda^2 p(\lambda x,, \lambda^2 t).$$
A norm is &lt;em&gt;critical&lt;/em&gt; (or &lt;em&gt;scale-invariant&lt;/em&gt;) if it is preserved by this rescaling.
The critical norm in $L^p(\mathbb{R}^3)$ is $L^3$, since
$|\lambda u(\lambda\cdot)| _{L^3} = |u| _{L^3}$.
The energy norm $|u| _{L^2}$ is &lt;em&gt;subcritical&lt;/em&gt;: it scales as $\lambda^{1/2}|u| _{L^2}$,
which shrinks under the rescaling $\lambda \to \infty$ (i.e., zoom into small
scales). This mismatch is the core of the difficulty: global energy control does
not prevent concentration at arbitrarily small scales.&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;2D global regularity.&lt;/strong&gt; In two dimensions the scaling is different: the enstrophy
$|\nabla u|_{L^2}^2$ is scale-invariant and is controlled by the energy. Global
regularity in 2D follows from this enstrophy estimate, a fact known since the 1960s.
In 3D no analogous critical quantity is controlled globally, and the problem is open.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="the-hierarchy-of-known-results"&gt;
 The Hierarchy of Known Results&lt;span class="heading__anchor"&gt; &lt;a href="#the-hierarchy-of-known-results"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;h3 class="heading" id="lerayhopf-weak-solutions-1934"&gt;
 Leray–Hopf Weak Solutions (1934)&lt;span class="heading__anchor"&gt; &lt;a href="#lerayhopf-weak-solutions-1934"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;div style="padding:10px 14px; border:2px solid #27ae60; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#27ae60; font-weight:bold;"&gt;Theorem (Leray 1934, Hopf 1951)&lt;/span&gt;
&lt;p&gt;For any $u_0 \in L^2(\mathbb{R}^3)$ divergence-free, there exists a global
&lt;em&gt;weak solution&lt;/em&gt; $u \in L^\infty(0,\infty;, L^2) \cap L^2(0,\infty;, H^1)$
satisfying the energy inequality
$$|u(t)| _{L^2}^2 + 2\nu\int _0^t |\nabla u| _{L^2}^2, ds \leq |u_0| _{L^2}^2.$$&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;Leray&amp;rsquo;s construction, via a compactness argument on regularised equations, produces
a solution that is globally defined but potentially not smooth, and the term &amp;ldquo;weak&amp;rdquo;
refers to the fact that the equations are satisfied only in an integral (distributional)
sense, not pointwise. The energy inequality is the only bound available globally.
Whether Leray–Hopf solutions are unique, or whether they are the same as smooth
solutions when the initial data is smooth, is unknown.&lt;/p&gt;
&lt;h3 class="heading" id="partial-regularity-the-ckn-theorem"&gt;
 Partial Regularity: The CKN Theorem&lt;span class="heading__anchor"&gt; &lt;a href="#partial-regularity-the-ckn-theorem"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;The best known result limiting the size of potential singularities is the following.&lt;/p&gt;
&lt;div style="padding:10px 14px; border:2px solid #27ae60; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#27ae60; font-weight:bold;"&gt;Theorem (Caffarelli–Kohn–Nirenberg, 1982)&lt;/span&gt;
&lt;p&gt;For any &lt;em&gt;suitable weak solution&lt;/em&gt; to the 3D Navier–Stokes equations, the set of
space-time singular points has &lt;em&gt;parabolic Hausdorff dimension at most 1&lt;/em&gt;. In
particular, at any given time the spatial singular set has Hausdorff dimension
at most $\dfrac{1}{2}$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;A &amp;ldquo;suitable weak solution&amp;rdquo; is a weak solution satisfying a local energy inequality.
The CKN theorem proves that singularities, if they exist, cannot fill a curve or
surface: they can occupy at most a set of dimension one in space-time. This is the
most quantitative partial regularity result available and was simplified by Lin
(1998). Scheffer (1977) had earlier shown singular times have Hausdorff dimension
at most $\dfrac{1}{2}$.&lt;/p&gt;
&lt;h3 class="heading" id="conditional-regularity-ladyzhenskayaprodiserrin"&gt;
 Conditional Regularity: Ladyzhenskaya–Prodi–Serrin&lt;span class="heading__anchor"&gt; &lt;a href="#conditional-regularity-ladyzhenskayaprodiserrin"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;div style="padding:10px 14px; border:2px solid #27ae60; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#27ae60; font-weight:bold;"&gt;Theorem (Ladyzhenskaya 1967, Prodi 1959, Serrin 1962)&lt;/span&gt;
&lt;p&gt;If a weak solution additionally satisfies $u \in L^r(0,T;, L^s(\mathbb{R}^3))$
with $\dfrac{2}{r} + \dfrac{3}{s} = 1$ and $3 &amp;lt; s \leq \infty$, then $u$ is
smooth on $(0,T]$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;The condition $\dfrac{2}{r} + \dfrac{3}{s} = 1$ is precisely the scale-invariant
line in the $(r,s)$ plane: membership in any of these spaces implies regularity.
The family ranges from $(r,s)=(\infty, 3)$ (critical $L^3$ control in space,
uniform in time) to $(r,s)=(2,\infty)$ (square-integrable $L^\infty$ control in
time). These are &lt;em&gt;conditional&lt;/em&gt; results: they do not prove that a weak solution
lies in such a space, only that if it does, it must be smooth.&lt;/p&gt;
&lt;h3 class="heading" id="the-critical-endpoint-escauriazasereginšverák"&gt;
 The Critical Endpoint: Escauriaza–Seregin–Šverák&lt;span class="heading__anchor"&gt; &lt;a href="#the-critical-endpoint-escauriazaseregin%c5%a1ver%c3%a1k"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;div style="padding:10px 14px; border:2px solid #27ae60; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#27ae60; font-weight:bold;"&gt;Theorem (Escauriaza–Seregin–Šverák, 2003)&lt;/span&gt;
&lt;p&gt;If $u$ is a Leray–Hopf weak solution with $\sup _{t \in [0,T^*)} |u(\cdot,t)| _{L^3(\mathbb{R}^3)} &amp;lt; \infty$,
then $u$ can be extended as a smooth solution past $T^*$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;The endpoint case $s=3$ of the LPS family is the critical one: $L^3(\mathbb{R}^3)$
is exactly the scale-invariant norm for Navier–Stokes. The ESS proof is substantially
harder than the subcritical cases; it uses a compactness argument to reduce to a
smooth, backwards self-similar solution and then invokes a backwards uniqueness
theorem for parabolic equations to rule it out.&lt;/p&gt;
&lt;h3 class="heading" id="taos-quantitative-criterion"&gt;
 Tao&amp;rsquo;s Quantitative Criterion&lt;span class="heading__anchor"&gt; &lt;a href="#taos-quantitative-criterion"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;div style="padding:10px 14px; border:2px solid #27ae60; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#27ae60; font-weight:bold;"&gt;Theorem (Tao, 2019)&lt;/span&gt;
&lt;p&gt;If a smooth finite-energy solution first becomes singular at time $T^*$, then
$$\limsup_{t \uparrow T^*}
\dfrac{|u(\cdot,t)| _{L^3(\mathbb{R}^3)}}{\bigl(\log\log\log\tfrac{1}{T^*-t}\bigr)^c}
= \infty$$
for some absolute constant $c&amp;gt;0$. In particular, the critical $L^3$ norm must blow
up at least as fast as a triple-logarithm in $(T^*-t)^{-1}$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;Tao&amp;rsquo;s result is the first &lt;em&gt;supercritical&lt;/em&gt; regularity criterion for Navier–Stokes:
it gives quantitative information about the blowup rate that goes (by a triple
logarithm) beyond what scaling alone can detect. The proof quantifies the
compactness arguments in the ESS proof, replacing each use of a compactness method
by an explicit Carleman inequality, and propagates lower bounds for the vorticity
across dyadic annuli. The triple-exponential dependence in Tao&amp;rsquo;s bound has since
been localised and sharpened by Barker–Prange (2021) and others.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="the-supercriticality-problem"&gt;
 The Supercriticality Problem&lt;span class="heading__anchor"&gt; &lt;a href="#the-supercriticality-problem"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;The fundamental analytical obstruction is that Navier–Stokes is &lt;em&gt;supercritical&lt;/em&gt;
with respect to the only globally controlled norm ($L^2$): the energy.&lt;/p&gt;
&lt;p&gt;Define the &lt;em&gt;critical regularity index&lt;/em&gt; as the Sobolev exponent $s$ such that
$\dot{H}^s(\mathbb{R}^3)$ is scale-invariant. For Navier–Stokes, $s = 1/2$. The
energy controls $\dot{H}^0 = L^2$ (subcritical), and regularity theory requires
control at $\dot{H}^1$ (critical viscous norm) or $L^3$ (critical Lebesgue norm).
There is a &lt;em&gt;regularity gap&lt;/em&gt; between what is globally available ($L^2$) and what
is needed ($L^3$ or $\dot{H}^1$). Every known approach to closing this gap runs
into the same obstruction: the nonlinearity can create structure at arbitrarily
small scales that the subcritical $L^2$ bound cannot see.&lt;/p&gt;
&lt;p&gt;Tao (2016) made this gap precise by constructing an &lt;em&gt;averaged&lt;/em&gt; Navier–Stokes system, where the bilinear nonlinearity $(u\cdot\nabla)u$ is replaced by a carefully designed convex average of related nonlinearities, for which finite-time blowup
can be rigorously proved. This construction does not produce a counterexample to the true Navier–Stokes equations, but it demonstrates that the specific algebraic structure of the nonlinearity is load-bearing: any proof of global regularity must use something specific about $(u\cdot\nabla)u$ that is not shared by its averages.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="research-directions"&gt;
 Research Directions&lt;span class="heading__anchor"&gt; &lt;a href="#research-directions"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;h3 class="heading" id="1-improving-the-quantitative-blowup-rate"&gt;
 1. Improving the Quantitative Blowup Rate&lt;span class="heading__anchor"&gt; &lt;a href="#1-improving-the-quantitative-blowup-rate"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;Tao&amp;rsquo;s triple-logarithmic rate is the sharpest known lower bound on blowup of the
critical $L^3$ norm. Scaling considerations suggest that the true rate, if blowup
occurs, should be much faster; conjecturally $|u|_{L^3} \sim (T^*-t)^{-\delta}$
for some $\delta &amp;gt; 0$, analogous to Type I blowup in nonlinear heat equations. The
gap between the triple-logarithmic lower bound and the conjectured power-law rate
represents the frontier of quantitative regularity theory. Closing even part of this
gap, for instance establishing a single-logarithmic or power-of-log lower bound,
would require new ideas beyond Carleman estimates.&lt;/p&gt;
&lt;h3 class="heading" id="2-type-i-vs-type-ii-blowup"&gt;
 2. Type I vs. Type II Blowup&lt;span class="heading__anchor"&gt; &lt;a href="#2-type-i-vs-type-ii-blowup"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;A blowup is called &lt;em&gt;Type I&lt;/em&gt; if the scale-invariant norm $|u(\cdot,t)|_{L^3}$
grows no faster than $O((T^&lt;em&gt;-t)^{-1/2})$ near $T^&lt;/em&gt;$. It is &lt;em&gt;Type II&lt;/em&gt; otherwise.
For the Navier–Stokes equations, ruling out Type I blowup would be a significant
advance: all self-similar singularities (where $u(x,t) = (T^*-t)^{-1/2}U(x/(T^*-t)^{1/2})$)
are of Type I, and several results (including work of Ružička and Seregin) already
rule them out under mild additional assumptions. Whether all Type I blowup can be
excluded, leaving only the less structured Type II, is open.&lt;/p&gt;
&lt;h3 class="heading" id="3-uniqueness-of-weak-solutions"&gt;
 3. Uniqueness of Weak Solutions&lt;span class="heading__anchor"&gt; &lt;a href="#3-uniqueness-of-weak-solutions"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;Leray–Hopf weak solutions exist globally, but they may not be unique. This is a
separate, equally deep question: even if all smooth solutions extend globally, one
must also ask whether weak solutions coincide with smooth ones when started from
smooth data. Recent work of Buckmaster and Vicol (2019) showed that weak solutions
below the Ladyzhenskaya–Prodi–Serrin threshold are indeed non-unique, using
convex integration techniques developed for the Euler equations (De Lellis–Székelyhidi).
Whether Leray–Hopf solutions with the energy inequality are unique is still open
and is perhaps the central problem in the weak solution theory.&lt;/p&gt;
&lt;h3 class="heading" id="4-self-similar-and-discretely-self-similar-solutions"&gt;
 4. Self-Similar and Discretely Self-Similar Solutions&lt;span class="heading__anchor"&gt; &lt;a href="#4-self-similar-and-discretely-self-similar-solutions"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;Self-similar solutions of the form $u(x,t) = (T^*-t)^{-1/2} U(x/(T^*-t)^{1/2})$
satisfy a nonlinear elliptic system for the profile $U$. Several non-existence
theorems show that backward self-similar solutions with certain integrability must
be trivial (Nečas–Ružička–Šverák, 1996). The case of &lt;em&gt;discretely&lt;/em&gt; self-similar
solutions, where $u(x,t) = \lambda u(\lambda x, \lambda^2 t)$ for a fixed
$\lambda \neq 1$, is less understood and was recently revisited. Whether the
set of self-similar profiles that could appear as blowup limits is empty is not known.&lt;/p&gt;
&lt;h3 class="heading" id="5-computer-assisted-proofs-via-rigorous-numerics"&gt;
 5. Computer-Assisted Proofs via Rigorous Numerics&lt;span class="heading__anchor"&gt; &lt;a href="#5-computer-assisted-proofs-via-rigorous-numerics"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;The Chen–Hou approach to Euler singularities (2025) used a computer-assisted proof
framework: construct a numerical approximate profile, then verify its stability
rigorously using interval arithmetic. For Navier–Stokes the presence of viscosity
complicates such an approach (the profile is dissipated rather than transported),
but the same framework (dynamical rescaling plus nonlinear stability verification) might in principle detect or rule out singularities in specific axi-symmetric geometries. Applying and adapting the Hou group&amp;rsquo;s methods to the viscous problem
is an active direction.&lt;/p&gt;
&lt;h3 class="heading" id="6-the-zero-viscosity-limit-and-eulernavierstokes-connection"&gt;
 6. The Zero-Viscosity Limit and Euler–Navier–Stokes Connection&lt;span class="heading__anchor"&gt; &lt;a href="#6-the-zero-viscosity-limit-and-eulernavierstokes-connection"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;As $\nu \to 0$, Navier–Stokes formally converges to Euler. The precise relationship
is subtle: in the presence of boundaries (Prandtl layers) or after a potential Euler
singularity, the zero-viscosity limit can fail to hold in strong norms. If Euler
develops a finite-time singularity at time $T^*_E$ from smooth data (as Chen–Hou
suggest for bounded domains), then for small $\nu$ the Navier–Stokes solution must
either also develop a near-singularity or be regularised by viscosity before $T^*_E$.
Whether viscosity is always sufficient to regularise an Euler singularity, or whether
a Navier–Stokes singularity can arise from a nearby Euler one, is entirely open.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="references"&gt;
 References&lt;span class="heading__anchor"&gt; &lt;a href="#references"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;ol&gt;
&lt;li&gt;Fefferman, C. L. (2000). Existence and smoothness of the Navier–Stokes equation. Clay Mathematics Institute Millennium Prize Problems. &lt;a href="https://www.claymath.org/wp-content/uploads/2022/06/navierstokes.pdf"&gt;https://www.claymath.org/wp-content/uploads/2022/06/navierstokes.pdf&lt;/a&gt;&lt;/li&gt;
&lt;li&gt;Leray, J. (1934). Sur le mouvement d&amp;rsquo;un liquide visqueux emplissant l&amp;rsquo;espace. &lt;em&gt;Acta Mathematica&lt;/em&gt;, &lt;strong&gt;63&lt;/strong&gt;, 193–248.&lt;/li&gt;
&lt;li&gt;Hopf, E. (1951). Über die Anfangswertaufgabe für die hydrodynamischen Grundgleichungen. &lt;em&gt;Mathematische Nachrichten&lt;/em&gt;, &lt;strong&gt;4&lt;/strong&gt;(1–6), 213–231.&lt;/li&gt;
&lt;li&gt;Caffarelli, L., Kohn, R., &amp;amp; Nirenberg, L. (1982). Partial regularity of suitable weak solutions of the Navier–Stokes equations. &lt;em&gt;Communications on Pure and Applied Mathematics&lt;/em&gt;, &lt;strong&gt;35&lt;/strong&gt;(6), 771–831.&lt;/li&gt;
&lt;li&gt;Ladyzhenskaya, O. A. (1967). On uniqueness and smoothness of generalized solutions to the Navier–Stokes equations. &lt;em&gt;Zapiski Nauchnykh Seminarov LOMI&lt;/em&gt;, &lt;strong&gt;5&lt;/strong&gt;, 169–185.&lt;/li&gt;
&lt;li&gt;Escauriaza, L., Seregin, G. A., &amp;amp; Šverák, V. (2003). $L_{3,\infty}$-solutions of the Navier–Stokes equations and backward uniqueness. &lt;em&gt;Russian Mathematical Surveys&lt;/em&gt;, &lt;strong&gt;58&lt;/strong&gt;(2), 211–250.&lt;/li&gt;
&lt;li&gt;Tao, T. (2019). Quantitative bounds for critically bounded solutions to the Navier–Stokes equations. arXiv:1908.04958. Published in &lt;em&gt;Nine Mathematical Challenges&lt;/em&gt;, AMS, 2021, pp. 149–193.&lt;/li&gt;
&lt;li&gt;Tao, T. (2016). Finite time blowup for an averaged three-dimensional Navier–Stokes equation. &lt;em&gt;Journal of the American Mathematical Society&lt;/em&gt;, &lt;strong&gt;29&lt;/strong&gt;(3), 601–674.&lt;/li&gt;
&lt;li&gt;Buckmaster, T. &amp;amp; Vicol, V. (2019). Nonuniqueness of weak solutions to the Navier–Stokes equation. &lt;em&gt;Annals of Mathematics&lt;/em&gt;, &lt;strong&gt;189&lt;/strong&gt;(1), 101–144.&lt;/li&gt;
&lt;li&gt;Barker, T. &amp;amp; Prange, C. (2021). Localized quantitative estimates and potential blow-up rates for the Navier–Stokes equations. &lt;em&gt;Communications in Mathematical Physics&lt;/em&gt;, &lt;strong&gt;385&lt;/strong&gt;, 717–792.&lt;/li&gt;
&lt;/ol&gt;</description></item></channel></rss>