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Liouville Theorems Above the Critical $9/2$ Threshold for Stationary Navier-Stokes Equations

Published 7 Apr 2026 in math.AP | (2604.06527v1)

Abstract: We establish new Liouville-type theorems for the stationary Navier--Stokes equations in R<sup>3\mathbb{R}<sup>3. A central open problem in this context is whether the classical L<sup>9/2(R<sup>3)L<sup>{9/2}(\mathbb{R}<sup>3) condition of G.~Galdi can be relaxed. In this note we show that this global integrability requirement can indeed be weakened. More precisely, we prove that triviality already follows under assumptions of the form uL<sup>9/2</sup>+ε()(R<sup>3)u \in L<sup>{9/2</sup> + \varepsilon(\cdot)}(\mathbb{R}<sup>3), where $\varepsilon(\cdot)&gt;0$. As a consequence, we obtain a localized Liouville theorem: it is sufficient to impose this integrability condition only at infinity, with no additional assumptions on the behavior of uu inside a compact set. This highlights that the mechanism enforcing triviality is purely asymptotic. Our approach relies on a general uniqueness result in the framework of Lebesgue spaces with variable exponents, which naturally captures the coexistence of different integrability regimes across the domain.

Summary

  • The paper proves a new Liouville theorem showing that stationary Navier–Stokes solutions in \(\dot H^1(\mathbb R^3)\) are trivial under a variable-exponent condition \(u\in L^{9/2+\varepsilon(\cdot)}\), where \(\varepsilon(x)\to0\) at infinity.
  • The proof uses localized energy estimates, variable-exponent Hölder inequalities, annular decay, and Riesz-transform bounds to make both diffusion and nonlinear pressure remainders vanish without frequency decompositions or smallness assumptions.
  • The result demonstrates that integrability is needed only outside an arbitrary compact set, while the critical \(L^{9/2}\) case and the broader \(\dot H^1\) uniqueness problem remain open.

This paper establishes new Liouville-type theorems for the stationary Navier–Stokes equations

Δu+uablau+P=0,u=0-\Delta u + u\cdot abla u + \nabla P = 0, \qquad \nabla\cdot u = 0

in R3\mathbb{R}^3, weakening the classical global integrability hypothesis uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3) due to Galdi to a variable-exponent condition uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3), where ε(x)0\varepsilon(x) \to 0 as x|x|\to\infty. The main conceptual contribution is a demonstration that the rigidity mechanism enforcing triviality is purely asymptotic: integrability need only be controlled at infinity, with no assumptions on uu inside an arbitrarily large compact set.

Background and the open problem

The motivating question, raised by Galdi and Seregin, asks whether every solution uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3) vanishing at infinity must be identically zero. Existence of nontrivial solutions in (H˙1,H˙1/2)(\dot{H}^1, \dot{H}^{1/2}) is known (via Lemarié-Rieusset's construction), but uniqueness in this class remains open, so additional decay or integrability hypotheses are needed to force triviality.

Prior results form a hierarchy of relaxations of Galdi's L9/2L^{9/2} condition:

  • Chae–Wolf: the logarithmic refinement R3\mathbb{R}^30 suffices.
  • Lerner: it suffices that only the low-frequency projection R3\mathbb{R}^31 belongs to R3\mathbb{R}^32.
  • Kozono–Terasawa–Wakasugi, extended by Seregin–Wang: a smallness condition on the weak-R3\mathbb{R}^33 norm relative to R3\mathbb{R}^34 suffices.
  • Chae: R3\mathbb{R}^35 implies triviality; Seregin: R3\mathbb{R}^36 with R3\mathbb{R}^37 implies triviality.

The present work departs from all of these by working entirely in physical space with variable exponents, requiring no frequency decomposition and no smallness assumption.

Main results

The central uniqueness theorem is formulated in the variable-exponent Lebesgue space R3\mathbb{R}^38, defined via the Luxemburg norm associated with the modular R3\mathbb{R}^39.

Theorem (general criterion). Let uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)0 and let uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)1 solve the stationary system. Suppose uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)2 satisfies: (i) uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)3 on uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)4; (ii) uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)5 is continuous, radially decreasing, and uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)6 everywhere; (iii) uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)7 for uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)8, with uL9/2(R3)u \in L^{9/2}(\mathbb{R}^3)9. If uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)0, then uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)1.

Two concrete corollaries follow immediately:

  • Explicit exponent theorem (uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)2): with uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)3 for uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)4 and uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)5 for uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)6, membership uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)7 forces uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)8. Note that uL92+ε()(R3)u \in L^{\frac{9}{2}+\varepsilon(\cdot)}(\mathbb{R}^3)9 near the origin, so the hypothesis coincides exactly with what Sobolev embedding already provides on bounded sets, while decaying toward the critical value ε(x)0\varepsilon(x) \to 00 at infinity at a quantified rate ε(x)0\varepsilon(x) \to 01.
  • Localized Liouville theorem: the same conclusion holds if the variable-exponent condition is imposed only on ε(x)0\varepsilon(x) \to 02, since the interior contribution is covered automatically by ε(x)0\varepsilon(x) \to 03. Since ε(x)0\varepsilon(x) \to 04 is arbitrary, no assumption whatsoever is made on ε(x)0\varepsilon(x) \to 05 inside any fixed compact set — the paper's strongest qualitative claim, namely that triviality is enforced purely by asymptotic behavior.

Method of proof

The argument follows the classical energy/localization scheme: testing the equation against ε(x)0\varepsilon(x) \to 06 with a standard cut-off yields

ε(x)0\varepsilon(x) \to 07

where ε(x)0\varepsilon(x) \to 08 collects the cut-off Laplacian term and ε(x)0\varepsilon(x) \to 09 the convective and pressure terms. Triviality follows once both remainder terms vanish as x|x|\to\infty0.

The technical core lies in estimating these remainders using variable-exponent Hölder inequalities on annuli x|x|\to\infty1. Three lemmas drive the asymptotics:

  1. Since x|x|\to\infty2 is continuous, radially decreasing, and approaches x|x|\to\infty3 at rate x|x|\to\infty4, the essential supremum satisfies x|x|\to\infty5.
  2. Consequently x|x|\to\infty6, and hence x|x|\to\infty7.
  3. For any x|x|\to\infty8, one has x|x|\to\infty9.

Combining these with Lemma showing uu0 (a dominated-convergence argument on the modular), both uu1 and uu2 vanish. The pressure term is handled via the Riesz-transform representation uu3 together with boundedness of Riesz transforms on uu4 for globally log-Hölder exponents uu5 — a point verified directly for the exponents considered here. This last point is significant: earlier variable-exponent Liouville results (Chamorro–Vergara-Hermosilla) used discontinuous exponents on infinite-measure regions, where Riesz transform boundedness fails, forcing simultaneous hypotheses on uu6 and uu7. The log-Hölder framework here removes that restriction, allowing conditions on the velocity alone.

The proof concludes with uu8, hence uu9 by Sobolev embedding.

Limitations and open questions

Several caveats should be noted plainly. First, the result does not resolve the original Problem of Galdi–Seregin: the exponent uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)0 still exceeds the critical threshold everywhere, and the rate of approach uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)1 is quantified; whether pure uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)2, or even weaker asymptotic conditions, suffice remains open. Second, the theorem requires uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)3 in the decay condition (iii), a constraint tied to the specific scaling of the estimates rather than an obviously sharp requirement. Third, the argument relies on regularity of uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)4 obtained from uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)5 (via Galdi's Theorem X.1.1), which holds here because uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)6; extensions to rougher solution classes are not addressed. Finally, the paper leaves open whether the Sobolev embedding information uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)7 can be upgraded to a global condition implying triviality in uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)8 — the remark in the introduction notes this would immediately settle the problem but "remains an open problem."

Conclusion

The paper proves that the classical uH˙1(R3)u \in \dot{H}^1(\mathbb{R}^3)9 Liouville threshold for stationary Navier–Stokes in (H˙1,H˙1/2)(\dot{H}^1, \dot{H}^{1/2})0 can be relaxed to a spatially varying integrability condition approaching (H˙1,H˙1/2)(\dot{H}^1, \dot{H}^{1/2})1 from above at infinity, and — more strikingly — that this condition need only hold outside an arbitrary compact set. The mechanism is shown to be purely asymptotic, and the variable-exponent framework with log-Hölder continuity provides the functional analytic tool that makes a velocity-only formulation possible. The precise boundary between these hypotheses and the full (H˙1,H˙1/2)(\dot{H}^1, \dot{H}^{1/2})2 conjecture remains unresolved.

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