<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Convex Integration on Nam Le</title><link>https://blog.namln.org/en/tags/convex-integration/</link><description>Recent content in Convex Integration 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/convex-integration/index.xml" rel="self" type="application/rss+xml"/><item><title>Navier–Stokes Regularity: The Uniqueness of Weak Solutions</title><link>https://blog.namln.org/en/posts/navier-stokes-weak-uniqueness/</link><pubDate>Fri, 29 May 2026 00:00:00 +0000</pubDate><guid>https://blog.namln.org/en/posts/navier-stokes-weak-uniqueness/</guid><description>&lt;p&gt;The &lt;a href="../navier-stokes-existence-smoothness"&gt;companion post on Navier–Stokes existence and smoothness&lt;/a&gt;
asked whether smooth solutions can break down in finite time. This post asks the
opposite question: when a solution is only weakly defined, satisfying the equations
in an integral sense rather than pointwise, is it uniquely determined by its initial
data? The answer, developed over the last two decades through a dramatic series of
results, is a resounding &lt;em&gt;no&lt;/em&gt; in many regimes. The frontier is now whether the
physically natural class of Leray–Hopf weak solutions retains uniqueness.&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;Question (Weak Uniqueness)&lt;/span&gt;
&lt;p&gt;Are Leray–Hopf weak solutions of the 3D incompressible Navier–Stokes equations
$$\partial_t u + (u\cdot\nabla)u - \nu\Delta u + \nabla p = 0, \qquad \nabla\cdot u = 0$$
uniquely determined by their initial data $u_0 \in L^2(\mathbb{R}^3)$?&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;The question is one of the most urgent open problems in the PDE theory of fluid
dynamics. It is logically independent of the blowup question: Leray–Hopf solutions
exist globally for all time regardless of whether smooth solutions break down. What
is not known is whether two Leray–Hopf solutions started from the same data must
coincide.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="nashs-h-principle-the-conceptual-ancestor"&gt;
 Nash&amp;rsquo;s h-Principle: The Conceptual Ancestor&lt;span class="heading__anchor"&gt; &lt;a href="#nashs-h-principle-the-conceptual-ancestor"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;The story begins not in fluid mechanics but in differential geometry. In 1954,
John Nash proved that any Riemannian manifold admits a $C^1$ isometric embedding
into Euclidean space, a result that contradicted the expectation, based on the rigid
behaviour of $C^2$ embeddings (Cauchy), that the metric should impose strong
constraints. The key insight is that $C^1$ embeddings are &lt;em&gt;flexible&lt;/em&gt;: one can
deform them by adding high-frequency oscillations that are invisible at the large
scale but locally produce any prescribed metric tensor.&lt;/p&gt;
&lt;p&gt;Gromov formulated this phenomenon as the &lt;em&gt;h-principle&lt;/em&gt;: for certain underdetermined
differential relations, the topological (homotopy-theoretic) obstructions are the
only ones, and any formal solution can be deformed into an actual solution. The
h-principle is a flexibility result: it says geometry is surprisingly unconstrained
below a critical regularity threshold.&lt;/p&gt;
&lt;p&gt;De Lellis and Székelyhidi recognised in the mid-2000s that the incompressible Euler
equations are formally analogous to Nash&amp;rsquo;s embedding problem. The Euler system is
underdetermined (more unknowns than equations), and one can attempt to construct
wild solutions by adding high-frequency oscillations. The crucial observation is that
the nonlinearity $u\otimes u$ in the Reynolds stress tensor plays the role of the
metric tensor in Nash&amp;rsquo;s problem.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="wild-euler-solutions"&gt;
 Wild Euler Solutions&lt;span class="heading__anchor"&gt; &lt;a href="#wild-euler-solutions"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;The first step was to show that the Euler equations possess infinitely many weak
solutions for given initial data.&lt;/p&gt;
&lt;div style="padding:10px 14px; border:2px solid #c0392b; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#c0392b; font-weight:bold;"&gt;Theorem (De Lellis–Székelyhidi, 2009–2013)&lt;/span&gt;
&lt;p&gt;For any divergence-free $u _0 \in L^2(\mathbb{T}^3)$ and any prescribed energy
profile $e(t) \in C^\infty([0,T])$ with $e(t) &amp;gt; |u _0| _{L^2}^2$ for all $t &amp;gt; 0$,
there exist infinitely many weak solutions $u \in C_t^0 L_x^2$ of the 3D Euler
equations with $u(\cdot,0) = u _0$ and $|u(\cdot,t)| _{L^2}^2 = e(t)$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;In particular, the Euler equations admit weak solutions that spontaneously gain or
lose kinetic energy for no reason: &lt;em&gt;wild solutions&lt;/em&gt;. The construction proceeds by
convex integration: one builds the solution iteratively, at each stage adding a
high-frequency perturbation (a &lt;em&gt;Beltrami wave&lt;/em&gt;) that corrects the error in the
momentum equation while staying nearly invisible in the velocity field.&lt;/p&gt;
&lt;p&gt;Earlier, Scheffer (1993) and Shnirelman (1997) had shown the existence of weak Euler
solutions with compact support in space-time: the fluid is at rest, then spontaneously
moves, then returns to rest; but their constructions were indirect. De Lellis and
Székelyhidi&amp;rsquo;s convex integration scheme gave the first systematic and quantitative
approach.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="onsagers-conjecture"&gt;
 Onsager&amp;rsquo;s Conjecture&lt;span class="heading__anchor"&gt; &lt;a href="#onsagers-conjecture"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;The De Lellis–Székelyhidi results raise an immediate question: at what regularity
does the fluid behaviour transition from flexible (wild, non-unique) to rigid
(energy-conserving, unique)? This is precisely what Lars Onsager conjectured in 1949.&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;Onsager's Conjecture (1949)&lt;/span&gt;
&lt;p&gt;For the 3D incompressible Euler equations, the threshold regularity for energy
conservation is the Hölder exponent $1/3$:&lt;/p&gt;
&lt;ul&gt;
&lt;li&gt;If $u \in C^{0,\alpha}$ with $\alpha &amp;gt; 1/3$, then every weak solution conserves
kinetic energy.&lt;/li&gt;
&lt;li&gt;For every $\alpha &amp;lt; 1/3$, there exist weak solutions in $C^{0,\alpha}$ that
dissipate energy.&lt;/li&gt;
&lt;/ul&gt;
&lt;/div&gt;
&lt;p&gt;The &lt;strong&gt;positive direction&lt;/strong&gt; (conservation above $1/3$) was proved by
Constantin–E–Titi (1994). The &lt;strong&gt;negative direction&lt;/strong&gt; (dissipation possible below
$1/3$) required much more work and was fully resolved only recently.&lt;/p&gt;
&lt;div style="padding:10px 14px; border:2px solid #c0392b; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#c0392b; font-weight:bold;"&gt;Theorem (Isett, 2018)&lt;/span&gt;
&lt;p&gt;For every $\alpha &amp;lt; 1/3$ there exist weak solutions $u \in C^{0,\alpha}(\mathbb{T}^3\times[0,T])$
of the 3D Euler equations that fail to conserve kinetic energy.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;Isett&amp;rsquo;s proof, published in the &lt;em&gt;Annals of Mathematics&lt;/em&gt; in 2018, was the culmination
of a decade of refinements of the De Lellis–Székelyhidi scheme. The key difficulty at
regularity exactly $1/3$ is that the high-frequency perturbations must be sized to
cancel the Reynolds stress error while staying in $C^{1/3-}$; this requires a
delicate interplay of oscillation and concentration (&lt;em&gt;intermittency&lt;/em&gt;). De Lellis,
Székelyhidi, Buckmaster, and Vicol also obtained solutions attaining any prescribed
energy profile in $C^{1/3-}$. Onsager&amp;rsquo;s conjecture is now a theorem.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="viscous-non-uniqueness-buckmastervicol"&gt;
 Viscous Non-Uniqueness: Buckmaster–Vicol&lt;span class="heading__anchor"&gt; &lt;a href="#viscous-non-uniqueness-buckmastervicol"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;Adapting the convex integration scheme from Euler to Navier–Stokes requires overcoming
the viscous term $\nu\Delta u$, which smooths out high-frequency oscillations. The
intermittent Beltrami waves used by Isett concentrate energy at sparse spatial sets,
reducing their interaction with the Laplacian. Buckmaster and Vicol exploited this
idea to bring convex integration into the viscous setting.&lt;/p&gt;
&lt;div style="padding:10px 14px; border:2px solid #c0392b; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#c0392b; font-weight:bold;"&gt;Theorem (Buckmaster–Vicol, 2019)&lt;/span&gt;
&lt;p&gt;There exist infinitely many weak solutions $u \in C_t^0 L_x^2(\mathbb{T}^3)$ of the
3D Navier–Stokes equations, belonging to the same regularity class as Leray–Hopf
solutions, that do not satisfy the global energy inequality. In particular, weak
solutions of 3D Navier–Stokes are not unique in the class $C_t^0 L_x^2$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;The Buckmaster–Vicol solutions, published in the &lt;em&gt;Annals of Mathematics&lt;/em&gt; &lt;strong&gt;189&lt;/strong&gt;
(2019), 101–144, are weak in both the PDE sense and the energy sense: they satisfy
the equations distributionally and have finite kinetic energy, but they can gain
energy spontaneously, violating the natural dissipation law $\partial _t|u| _{L^2}^2
\leq -2\nu|\nabla u| _{L^2}^2$.&lt;/p&gt;
&lt;p&gt;This non-uniqueness is striking but also limited: the Buckmaster–Vicol solutions
are not Leray–Hopf solutions, because Leray–Hopf solutions are required to satisfy
the &lt;em&gt;energy inequality&lt;/em&gt; $|u(t)| _{L^2}^2 \leq |u _0| _{L^2}^2$. Whether this
single additional constraint, that energy does not increase, suffices to restore
uniqueness is the open question.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="crossing-the-energy-barrier-albrittonbruécolombo"&gt;
 Crossing the Energy Barrier: Albritton–Brué–Colombo&lt;span class="heading__anchor"&gt; &lt;a href="#crossing-the-energy-barrier-albrittonbru%c3%a9colombo"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;The energy inequality distinguishing Leray–Hopf solutions from Buckmaster–Vicol wild
solutions seemed for a long time to be a genuine barrier to non-uniqueness. The
following result crossed this barrier, but required introducing an external force.&lt;/p&gt;
&lt;div style="padding:10px 14px; border:2px solid #c0392b; border-radius:6px; margin:16px 0;"&gt;
&lt;span style="color:#c0392b; font-weight:bold;"&gt;Theorem (Albritton–Brué–Colombo, 2022)&lt;/span&gt;
&lt;p&gt;There exists a body force $f \in L^1(0,T;, L^2(\mathbb{R}^3))$ and two distinct
Leray–Hopf weak solutions of the &lt;strong&gt;forced&lt;/strong&gt; 3D Navier–Stokes equations
$\partial_t u + (u\cdot\nabla)u - \nu\Delta u + \nabla p = f$ with the same initial
data $u_0 \equiv 0$ and the same force $f$.&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;Published in the &lt;em&gt;Annals of Mathematics&lt;/em&gt; &lt;strong&gt;196&lt;/strong&gt; (2022), 415–455, the proof uses a
completely different mechanism from convex integration. The key ingredient is an
&lt;em&gt;unstable&lt;/em&gt; background solution: using Vishik&amp;rsquo;s construction of spectrally unstable
steady states of the 2D Euler equations, Albritton–Brué–Colombo lift a 2D unstable
vortex ring to an axisymmetric 3D solution and embed it into the Navier–Stokes flow
via a self-similar change of variables. The force $f$ is chosen precisely to make
this background exactly solve the forced equations; the instability then allows two
different solutions to branch from the same initial data.&lt;/p&gt;
&lt;p&gt;The force is singular; it belongs to $L^1_t L^2_x$ but is not smooth, and is
concentrated near the initial time $t=0$. Whether the same non-uniqueness can be
achieved with a smooth or zero force is the remaining open problem.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="the-unforced-case-current-frontier"&gt;
 The Unforced Case: Current Frontier&lt;span class="heading__anchor"&gt; &lt;a href="#the-unforced-case-current-frontier"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;Non-uniqueness of Leray–Hopf solutions for the &lt;em&gt;unforced&lt;/em&gt; Navier–Stokes equations
remains open. The route to the unforced case requires finding a self-similar
background profile that solves the unforced equations exactly and has an unstable
eigenvalue, a far more demanding task than the forced case, where the profile can
be any divergence-free function.&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;Open Problem (Jia–Šverák Programme)&lt;/span&gt;
&lt;p&gt;Do there exist two distinct Leray–Hopf solutions of the 3D Navier–Stokes equations
with the same initial data and no external force?&lt;/p&gt;
&lt;/div&gt;
&lt;p&gt;Jia and Šverák (2013–2014) showed that non-uniqueness would follow from a spectral
assumption: if there exists a forward self-similar Navier–Stokes solution whose
linearised operator has an eigenvalue with positive real part, then Leray–Hopf
solutions are non-unique. Guillod and Šverák (2017) provided compelling numerical
evidence that such an unstable self-similar profile exists.&lt;/p&gt;
&lt;p&gt;In September 2025, Giri and Kwon posted a preprint (arXiv:2509.25116) claiming a
computer-assisted proof of the existence of an unstable self-similar profile for
the unforced equations, which, via the Jia–Šverák mechanism, would establish
non-uniqueness of Leray–Hopf solutions. The proof uses rigorous interval arithmetic
to verify the existence of an unstable eigenvalue. As of this writing the preprint
is under review by the community.&lt;/p&gt;
&lt;hr&gt;
&lt;h2 class="heading" id="the-regularity-threshold"&gt;
 The Regularity Threshold&lt;span class="heading__anchor"&gt; &lt;a href="#the-regularity-threshold"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h2&gt;&lt;p&gt;The accumulated results suggest the following picture of the
&lt;strong&gt;flexibility-rigidity dichotomy&lt;/strong&gt; for the Euler and Navier–Stokes equations.&lt;/p&gt;
&lt;table&gt;
	&lt;thead&gt;
			&lt;tr&gt;
					&lt;th&gt;Regularity class&lt;/th&gt;
					&lt;th&gt;Euler&lt;/th&gt;
					&lt;th&gt;Navier–Stokes&lt;/th&gt;
			&lt;/tr&gt;
	&lt;/thead&gt;
	&lt;tbody&gt;
			&lt;tr&gt;
					&lt;td&gt;$C^{0,\alpha}$, $\alpha &amp;lt; 1/3$&lt;/td&gt;
					&lt;td&gt;non-unique, dissipative (Isett 2018)&lt;/td&gt;
					&lt;td&gt;n/a&lt;/td&gt;
			&lt;/tr&gt;
			&lt;tr&gt;
					&lt;td&gt;$C^{0,\alpha}$, $\alpha &amp;gt; 1/3$&lt;/td&gt;
					&lt;td&gt;energy-conserving (Constantin–E–Titi 1994)&lt;/td&gt;
					&lt;td&gt;n/a&lt;/td&gt;
			&lt;/tr&gt;
			&lt;tr&gt;
					&lt;td&gt;$L^2$ (global energy inequality)&lt;/td&gt;
					&lt;td&gt;non-unique&lt;/td&gt;
					&lt;td&gt;&lt;strong&gt;open (unforced); non-unique forced (ABC 2022)&lt;/strong&gt;&lt;/td&gt;
			&lt;/tr&gt;
			&lt;tr&gt;
					&lt;td&gt;$L^\infty_t L^3_x$ (LPS regularity)&lt;/td&gt;
					&lt;td&gt;n/a&lt;/td&gt;
					&lt;td&gt;unique and smooth (ESS 2003)&lt;/td&gt;
			&lt;/tr&gt;
	&lt;/tbody&gt;
&lt;/table&gt;
&lt;p&gt;The Leray–Hopf class sits precisely at the boundary where uniqueness is expected
to break down but has not yet been proved to do so in the unforced case.&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-resolving-the-jiašverák-spectral-condition"&gt;
 1. Resolving the Jia–Šverák Spectral Condition&lt;span class="heading__anchor"&gt; &lt;a href="#1-resolving-the-jia%c5%a1ver%c3%a1k-spectral-condition"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;The most direct path to unforced Leray–Hopf non-uniqueness is to rigorously confirm
or refute the spectral condition of Jia–Šverák: find (or prove the nonexistence of)
a forward self-similar Navier–Stokes profile with an unstable linearised eigenvalue.
The 2025 Giri–Kwon computer-assisted preprint claims this is now done. If confirmed,
the consequence is striking: Leray&amp;rsquo;s 1934 existence theorem cannot be supplemented
by uniqueness, and the Navier–Stokes Cauchy problem is &lt;em&gt;ill-posed&lt;/em&gt; in the Leray–Hopf
class.&lt;/p&gt;
&lt;h3 class="heading" id="2-selection-principles-and-physical-solutions"&gt;
 2. Selection Principles and Physical Solutions&lt;span class="heading__anchor"&gt; &lt;a href="#2-selection-principles-and-physical-solutions"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;If Leray–Hopf solutions are indeed non-unique, a fundamental question becomes which
solution is the physically correct one, the one observed in experiments and computed
in simulations. Several selection criteria have been proposed:
the &lt;em&gt;vanishing viscosity&lt;/em&gt; limit of the Navier–Stokes solution as $\nu\to 0$ from
above, &lt;em&gt;entropy conditions&lt;/em&gt; analogous to those for hyperbolic conservation laws,
and &lt;em&gt;renormalisation group&lt;/em&gt; or &lt;em&gt;statistical ensemble&lt;/em&gt; approaches motivated by
turbulence theory. None of these has been rigorously validated as a selection
criterion that distinguishes a unique Leray–Hopf solution from the others.&lt;/p&gt;
&lt;h3 class="heading" id="3-sharp-regularity-thresholds-for-navierstokes"&gt;
 3. Sharp Regularity Thresholds for Navier–Stokes&lt;span class="heading__anchor"&gt; &lt;a href="#3-sharp-regularity-thresholds-for-navierstokes"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;For Euler, Onsager&amp;rsquo;s conjecture identifies $C^{1/3}$ as the sharp regularity
threshold for energy conservation. What is the analogous threshold for Navier–Stokes?
The Buckmaster–Vicol solutions are in $C_t^0 L_x^2$ (very rough), while the
Ladyzhenskaya–Prodi–Serrin class gives uniqueness. The precise exponent at which
uniqueness breaks down, if it does, is not known. Determining the sharp Sobolev
or Hölder regularity threshold for Navier–Stokes uniqueness, analogous to Onsager&amp;rsquo;s
$1/3$, is a central open problem.&lt;/p&gt;
&lt;h3 class="heading" id="4-uniqueness-for-axisymmetric-initial-data"&gt;
 4. Uniqueness for Axisymmetric Initial Data&lt;span class="heading__anchor"&gt; &lt;a href="#4-uniqueness-for-axisymmetric-initial-data"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;A natural restricted problem is whether Leray–Hopf solutions with axisymmetric,
swirl-free initial data are unique. Such data imposes a strong geometric constraint
that eliminates most of the degrees of freedom available to convex integration.
Partial results are known (e.g., global regularity for axisymmetric data without
swirl is not proved but no counterexamples exist), but uniqueness in this class
has not been established. If the Giri–Kwon instability is confirmed, understanding
whether the instability mechanism survives axisymmetric perturbations is an
immediate question.&lt;/p&gt;
&lt;h3 class="heading" id="5-stochastic-regularisation"&gt;
 5. Stochastic Regularisation&lt;span class="heading__anchor"&gt; &lt;a href="#5-stochastic-regularisation"&gt;#&lt;/a&gt;&lt;/span&gt;
&lt;/h3&gt;&lt;p&gt;There is a well-studied phenomenon, &lt;em&gt;regularisation by noise&lt;/em&gt;, in which adding
a stochastic forcing term to an ill-posed deterministic PDE restores well-posedness.
For the Navier–Stokes equations, Hofmanová–Zhu–Zhu (2023) showed non-uniqueness
persists even under multiplicative noise for certain body forces, by adapting the
Albritton–Brué–Colombo construction. Whether a generic stochastic perturbation
can restore uniqueness of Leray–Hopf solutions, and what the appropriate notion of
&amp;ldquo;generic&amp;rdquo; should be, is a rich open direction combining convex integration with stochastic
analysis.&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;Nash, J. (1954). $C^1$ isometric imbeddings. &lt;em&gt;Annals of Mathematics&lt;/em&gt;, &lt;strong&gt;60&lt;/strong&gt;(3), 383–396.&lt;/li&gt;
&lt;li&gt;De Lellis, C. &amp;amp; Székelyhidi, L. (2009). The Euler equations as a differential inclusion. &lt;em&gt;Annals of Mathematics&lt;/em&gt;, &lt;strong&gt;170&lt;/strong&gt;(3), 1417–1436.&lt;/li&gt;
&lt;li&gt;De Lellis, C. &amp;amp; Székelyhidi, L. (2013). Dissipative continuous Euler flows. &lt;em&gt;Inventiones Mathematicae&lt;/em&gt;, &lt;strong&gt;193&lt;/strong&gt;(2), 377–407.&lt;/li&gt;
&lt;li&gt;Constantin, P., E, W., &amp;amp; Titi, E. S. (1994). Onsager&amp;rsquo;s conjecture on the energy conservation for solutions of Euler&amp;rsquo;s equation. &lt;em&gt;Communications in Mathematical Physics&lt;/em&gt;, &lt;strong&gt;165&lt;/strong&gt;(1), 207–209.&lt;/li&gt;
&lt;li&gt;Isett, P. (2018). A proof of Onsager&amp;rsquo;s conjecture. &lt;em&gt;Annals of Mathematics&lt;/em&gt;, &lt;strong&gt;188&lt;/strong&gt;(3), 871–963.&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;Buckmaster, T. &amp;amp; Vicol, V. (2019). Convex integration and phenomenologies in turbulence. &lt;em&gt;EMS Surveys in Mathematical Sciences&lt;/em&gt;, &lt;strong&gt;6&lt;/strong&gt;(1–2), 1–88.&lt;/li&gt;
&lt;li&gt;Albritton, D., Brué, E., &amp;amp; Colombo, M. (2022). Non-uniqueness of Leray solutions of the forced Navier–Stokes equations. &lt;em&gt;Annals of Mathematics&lt;/em&gt;, &lt;strong&gt;196&lt;/strong&gt;(1), 415–455.&lt;/li&gt;
&lt;li&gt;Jia, H. &amp;amp; Šverák, V. (2014). Local-in-space estimates near initial time for weak solutions of the Navier–Stokes equations and forward self-similar solutions. &lt;em&gt;Inventiones Mathematicae&lt;/em&gt;, &lt;strong&gt;196&lt;/strong&gt;(1), 233–265.&lt;/li&gt;
&lt;li&gt;Giri, V. &amp;amp; Kwon, H. (2025). Nonuniqueness of Leray–Hopf solutions to the unforced incompressible 3D Navier–Stokes equation. arXiv:2509.25116.&lt;/li&gt;
&lt;/ol&gt;</description></item></channel></rss>