Navier-Stokes equation

ScientificConcept

A complex fluid dynamics equation recently solved computationally by AI models, disrupting the mathematics community.


First Mentioned

9/13/2026, 4:51:37 AM

Last Updated

9/20/2026, 6:40:54 PM

Research Retrieved

9/13/2026, 4:59:31 AM

Summary

The Navier-Stokes equations are a system of partial differential equations that describe the motion of viscous fluids, developed by Claude-Louis Navier and George Gabriel Stokes between 1822 and 1850, with independent contributions from Siméon Denis Poisson. These equations express momentum balance for Newtonian fluids, incorporating mass conservation and the relationship between pressure, temperature, and density through an equation of state. They are derived from Newton's second law applied to fluid motion, assuming fluid stress is a combination of viscous forces and pressure, thus detailing viscous flow and generalizing the Euler equations for inviscid flow. The Navier-Stokes equations hold significant importance in science and engineering, aiding in the design of aircraft and cars, studying blood flow, designing power stations, and analyzing pollution. They are also fundamental to magnetohydrodynamics when coupled with Maxwell's equations. In pure mathematics, the existence and smoothness of solutions to these equations in three-dimensional space is a Millennium Prize Problem, with a claimed counterexample announced by OpenAI in September 2026, though it awaits independent verification and has sparked a priority dispute. OpenAI has also claimed to have used massive compute to solve the Navier-Stokes equation, raising concerns about data leakage and proprietary prompt ingestion.

Research Data
Extracted Attributes
    Navier–Stokes equations

    The Navier–Stokes equations ( nav-YAY STOHKS) describe the motion of viscous fluids. This system of partial differential equations was named after Claude-Louis Navier and George Gabriel Stokes, who developed them over a few decades of progressive work, from 1822 (Navier) to 1842–1850 (Stokes). Siméon Denis Poisson independently achieved the same results. The Navier–Stokes equations mathematically express momentum balance for Newtonian fluids and make use of the conservation of mass. They are sometimes accompanied by an equation of state relating pressure, temperature and density. They arise from applying Newton's second law to fluid motion, together with the assumption that the stress in the fluid is the sum of a diffusing viscous term (proportional to the gradient of velocity) and a pressure term—hence describing viscous flow. The Navier–Stokes equations generalize the Euler equations which only consider inviscid flow. The Navier–Stokes equations are of great scientific and engineering interest because they may be used to model a wide variety of scenarios. In their full or simplified forms, they can assist in the design of aircraft and cars, the study of blood flow, the design of power stations, the analysis of pollution, and many other problems. Coupled with Maxwell's equations, they comprise the fundamentals of magnetohydrodynamics. The Navier–Stokes equations are also of great interest to pure mathematics. The Navier–Stokes existence and smoothness problem concerns whether they have smooth (meaning infinitely differentiable) or bounded solutions in three-dimensional Euclidean space, as opposed to a breakdown with unbounded solutions. This is one of seven Millennium Prize Problems, notable open mathematics problems for which the Clay Mathematics Institute offered $1 million prizes in 2000 for correct solutions. In September 2026, OpenAI announced a claimed counterexample to the existence and smoothness problem. The announcement was followed by a priority dispute, and the claimed counterexample has yet to be independently verified.

    Web Search Results
    • Navier–Stokes existence and smoothness - Wikipedia

      The Navier–Stokes equations are a set of partial differential equations that describe the motion of fluids. They are given by: {\displaystyle {\frac {\partial \mathbf {v} }{\partial t}}+(\mathbf {v} \cdot \nabla )\mathbf {v} =-{\frac {1}{\rho }}\nabla p+\nu \nabla ^{2}\mathbf {v} +\mathbf {f} } {\displaystyle \nabla \cdot \mathbf {v} =0} where {\displaystyle \mathbf {v} (x,t)} is the velocity field of the fluid, {\displaystyle p(x,t)} is the pressure, {\displaystyle \rho } is the density, {\displaystyle \nu } is the kinematic viscosity, and {\displaystyle \mathbf {f} (x,t)} is an external force. The first equation is known as the momentum equation, and the second equation is known as the continuity equation.

    • Navier-Stokes Equation - an overview

      Then, in consideration of the continuity equation, Navier-Stokes equation is written in the following form: (3.204)$\mathit{\rho} \left(\right. \frac{\mathit{\partial} u}{\mathit{\partial} t} + \mathit{u} \frac{\mathit{\partial} u}{\mathit{\partial} x} + \mathit{v} \frac{\mathit{\partial} u}{\mathit{\partial} y} + \mathit{w} \frac{\mathit{\partial} u}{\mathit{\partial} z} \left.\right) = - \frac{\mathit{\partial} p}{\mathit{\partial} x} + \frac{\mathit{\partial} \mathit{\sigma}_{\mathit{x}}}{\mathit{\partial} x} + \frac{\mathit{\partial} \mathit{\tau}_{\mathit{yx}}}{\mathit{\partial} y} + \frac{\mathit{\partial} \mathit{\tau}_{\mathit{zx}}}{\mathit{\partial} z} + \mathit{F}_{\mathit{x}} ,$ [...] (3.198)$\frac{\mathit{\partial} \mathit{\rho} w}{\mathit{\partial} t} + \frac{\mathit{\partial} \mathit{\rho} w u}{\mathit{\partial} x} + \frac{\mathit{\partial} \mathit{\rho} w v}{\mathit{\partial} y} + \frac{\mathit{\partial} \mathit{\rho} w w}{\mathit{\partial} z} = - \frac{\mathit{\partial} p}{\mathit{\partial} z} + \frac{\mathit{\partial} \mathit{\tau}_{\mathit{xz}}}{\mathit{\partial} x} + \frac{\mathit{\partial} \mathit{\tau}_{\mathit{yz}}}{\mathit{\partial} y} + \frac{\mathit{\partial} \mathit{\sigma}_{\mathit{z}}}{\mathit{\partial} z} + \mathit{F}_{\mathit{z}} .$ The basic equation for viscous fluid flow, called Navier-Stokes equation, are the aforementioned equations coupled with the continuity equation. [...] The general form (vector form) of the Navier–Stokes equation is (1.36)$\rho \frac{\partial \mathbf{\mathit{V}}}{\partial t} + \rho \mathbf{\mathit{V}} \cdot \nabla \mathbf{\mathit{V}} = - \nabla P + \mu \nabla^{2} \mathbf{\mathit{V}} + \rho g$ where $\rho$ is density, $t$ is time, $\mathbf{\mathit{V}}$ is fluid velocity, $P$ is normal pressure on fluid element surfaces, $\mu$ is viscosity and $g$ is gravity. Table 1.4 shows the Navier–Stokes equation in rectangular and cylindrical coordinates. Table 1.4. Navier–Stokes Equation for Incompressible Fluids in Rectangular and Cylindrical Coordinates Rectangular Coordinates: _x_ direction:

    • Navier–Stokes equations - Wikipedia

      The incompressible Navier–Stokes equations with uniform density and viscosity and conservative external field is the fundamental equation of hydraulics. The domain for these equations is commonly a 3 or fewer dimensional Euclidean space, for which an orthogonal coordinate reference frame is usually set to explicit the system of scalar partial differential equations to be solved. In 3-dimensional orthogonal coordinate systems are 3: Cartesian, cylindrical, and spherical. Expressing the Navier–Stokes vector equation in Cartesian coordinates is quite straightforward and not much influenced by the number of dimensions of the euclidean space employed, and this is the case also for the first-order terms (like the variation and convection ones) also in non-cartesian orthogonal coordinate [...] Navier–Stokes momentum equation (convective form) ![{\displaystyle \rho {\frac {\mathrm {D} \mathbf {u} }{\mathrm {D} t}}=\rho \left({\frac {\partial \mathbf {u} }{\partial t}}+(\mathbf {u} \cdot \nabla )\mathbf {u} \right)=-\nabla p+\nabla \cdot \left(\mu \left[\nabla \mathbf {u} +(\nabla \mathbf {u} )^{\mathsf {T}}-{\tfrac {2}{3}}(\nabla \cdot \mathbf {u} )\mathbf {I} \right]\right)+\nabla [\zeta (\nabla \cdot \mathbf {u} )]+\rho \mathbf {a} .}]( in index notation, the equation can be written as Navier–Stokes momentum equation (index notation) [...] {\displaystyle {\frac {D\mathbf {u} }{Dt}}=-{\frac {1}{\rho }}\nabla p+\nu \,\nabla ^{2}\mathbf {u} +\left({\tfrac {1}{3}}\nu +\xi \right)\,\nabla (\nabla \cdot \mathbf {u} )+\mathbf {a} .} where {\textstyle {\frac {\mathrm {D} }{\mathrm {D} t}}} is the material derivative. {\textstyle \nu ={\frac {\mu }{\rho }}} is the shear kinematic viscosity and {\textstyle \xi ={\frac {\zeta }{\rho }}} is the bulk kinematic viscosity. The left-hand side changes in the conservation form of the Navier–Stokes momentum equation. By bringing the operator on the flow velocity on the left side, one also has: Navier–Stokes momentum equation with uniform shear and bulk viscosities (convective form)

    • What is... the Navier-Stokes equation?

      So what is the Navier Stokes problem? What are the Navier Stokes equations? What's the Oiler equation? And what problem are we trying to solve here? The Navier Stokes equation or Navier Stokes problem is a fundamental problem in fluid dynamics in mathematics because it asks a very fundamental question. If you take the equations, the simplified equations we use to model the motion of ordinary fluids in space in 3D space. Then those equations give you solutions. And the question is do those solutions stay smooth for all time or there could be a finite time where those solutions become not smooth where there is a singularity where the velocity becomes infinite. Let me try to explain this in more concrete terms with actual mathematical equations. So we're going to be talking about what we

    • Navier-Stokes Equations in Fluid Dynamics | Fundamental and Theoretical Fluid Dynamics | Fluid Mechanics and Thermal Engineering | Applied sciences | Topics | Nature Index

      The Navier–Stokes equations form the cornerstone of modern fluid dynamics, describing the motion of viscous, incompressible fluids through a set of nonlinear partial differential equations. At their heart lies the balance of momentum, combining inertial forces, pressure gradients and viscous diffusion. These equations capture phenomena ranging from laminar flow in microfluidic channels to turbulent currents in the atmosphere and oceans. Solutions may be smooth and unique under certain conditions, yet the problem of global regularity in three dimensions remains one of the great mathematical challenges. Analytical approaches often employ functional frameworks such as Sobolev or Besov spaces, while numerical methods rely on discretisation schemes and stability criteria. In practice, the