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Navier–Stokes Existence and Smoothness

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millennium-navier-stokes Β· source

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Statement

The divergence βˆ‡β‹…v\nabla \cdot v of a vector field v:Rnβ†’Rnv : \mathbb{R}^n \to \mathbb{R}^n at a point xx, computed as the trace of the Jacobian matrix.

In coordinates, βˆ‡β‹…v=βˆ‘iβˆ‚vi/βˆ‚xi\nabla \cdot v = \sum_i \partial v_i / \partial x_i.

This is available as the notation βˆ‡β¬ v. If v is not differentiable at x, then fderiv is the zero map, so this definition has the corresponding junk value 00.

A function f:Rn→αf : \mathbb{R}^n \to \alpha is 1-periodic if it is periodic in each coordinate with period 11, i.e. f(x+ei)=f(x)f(x + e_i) = f(x) for each unit vector eie_i. This captures functions on the nn-torus Rn/Zn\mathbb{R}^n/\mathbb{Z}^n.

Basic conditions on initial velocity field for the Navier-Stokes equations in nn-dimensional space.

The initial velocity must be:

  • Divergence-free (incompressibility condition: βˆ‡β‹…u0=0\nabla \cdot u_0 = 0)
  • Smooth (C∞C^\infty)

These conditions apply regardless of spatial dimension.

The initial velocity field is divergence-free (equation 2). This is the incompressibility constraint for the fluid.

The initial velocity field is smooth (C∞C^\infty in all variables).

Initial velocity conditions for the Navier-Stokes problem on all of Rn\mathbb{R}^n.

In addition to being smooth and divergence-free, the velocity must decay faster than any polynomial at spatial infinity (condition 4 in Fefferman's paper).

This condition ensures the velocity field has finite energy and reasonable behavior as βˆ₯xβˆ₯β†’βˆž\lVert x \rVert \to \infty.

All derivatives of uβ‚€ decay faster than any polynomial (condition 4). For any derivative order mm and any decay rate KK, there exists a constant CC such that βˆ₯βˆ‚mu0(x)βˆ₯≀C/(1+βˆ₯xβˆ₯)K\lVert \partial^m u_0(x) \rVert \le C/(1+\lVert x \rVert)^K.

Initial velocity conditions for the periodic Navier-Stokes problem on Rn/Zn\mathbb{R}^n/\mathbb{Z}^n.

The velocity must be smooth, divergence-free, and 1-periodic in each coordinate (condition 8, part 1 in Fefferman's paper).

The initial velocity is 1-periodic in each direction (condition 8, part 1).

The basic smoothness condition on the external forcing term.

The force f(x,t)f(x,t) must be smooth (C∞C^\infty) in both space and time variables for tβ‰₯0t \ge 0.

The force is smooth on RnΓ—[0,∞)\mathbb{R}^n \times [0,\infty).

Force conditions for the Navier-Stokes problem on all of Rn\mathbb{R}^n.

The force must be smooth and decay faster than any polynomial in both space and time (condition 5 in Fefferman's paper).

All derivatives of f decay faster than any polynomial in space and time (condition 5). For any derivative order mm and any decay rate KK, there exists CC such that βˆ₯βˆ‚x,tmf(x,t)βˆ₯≀C/(1+βˆ₯xβˆ₯+t)K\lVert \partial^m_{x,t} f(x,t) \rVert \le C/(1+\lVert x \rVert+t)^K for tβ‰₯0t \ge 0.

Force conditions for the periodic Navier-Stokes problem on Rn/Zn\mathbb{R}^n/\mathbb{Z}^n.

The force must be smooth, 1-periodic in space, and decay in time (conditions 8, part 1 and 9 in Fefferman's paper).

The force is 1-periodic in space for all times tβ‰₯0t \ge 0 (condition 8, part 1).

All derivatives of f decay faster than any polynomial in time (condition 9).

A solution (v, p) to the Navier-Stokes equations in n-dimensional space with viscosity Ξ½\nu, initial velocity u0u_0, and external force ff.

This structure captures the core requirements for a solution:

  1. The velocity and pressure satisfy the Navier-Stokes PDE (equation 1)
  2. The velocity remains divergence-free for all time (equation 2)
  3. The initial condition is satisfied (equation 3)
  4. The solution is smooth (C∞C^\infty) for all time tβ‰₯0t \ge 0 (equations 6, 11)

The Navier-Stokes equation (equation 1): βˆ‚v/βˆ‚t+(vβ‹…βˆ‡)v=Ξ½Ξ”vβˆ’βˆ‡p+f\partial v/\partial t + (v \cdot \nabla)v = \nu\Delta v - \nabla p + f.

Incompressibility constraint (equation 2): βˆ‡β‹…v=0\nabla \cdot v = 0 for all xx and tβ‰₯0t \ge 0.

Initial condition (equation 3): v(x,0)=u0(x)v(x,0) = u_0(x) for all xx.

The velocity field is smooth (C∞C^\infty) on RnΓ—[0,∞)\mathbb{R}^n \times [0,\infty) (conditions 6, 11).

The pressure field is smooth (C∞C^\infty) on RnΓ—[0,∞)\mathbb{R}^n \times [0,\infty) (conditions 6, 11).

A solution to the Navier-Stokes equations on all of Rn\mathbb{R}^n with appropriate decay and energy bounds.

In addition to the basic solution properties, we require:

  • The velocity is in L2L^2 at each time tβ‰₯0t \ge 0 (finite kinetic energy)
  • The total energy remains bounded for all time (condition 7)

The velocity is square-integrable at each time tβ‰₯0t \ge 0 (condition 7).

The kinetic energy ∫βˆ₯v(x,t)βˆ₯2 dx\int \lVert v(x,t) \rVert^2\,dx remains uniformly bounded for all time (condition 7), where the integral is the Lebesgue integral.

A solution to the Navier-Stokes equations on the nn-torus Rn/Zn\mathbb{R}^n/\mathbb{Z}^n.

The velocity must be 1-periodic in each spatial direction for all times (condition 10). The pressure is also required to be 1-periodic, following the errata appended to the Clay problem statement.

The velocity is 1-periodic in space for all times tβ‰₯0t \ge 0 (condition 10).

The pressure is 1-periodic in space for all times tβ‰₯0t \ge 0 (Clay errata).

(A) Existence and smoothness of Navier–Stokes solutions on ℝ³.

Metadata
  • Subjects: partial differential equations

Formal statement (Lean 4)

theorem navier_stokes_existence_and_smoothness_R3 (nu : ℝ) (hnu : nu > 0)
    (uβ‚€ : ℝ³ β†’ ℝ³) (huβ‚€ : InitialVelocityConditionDecay uβ‚€) :
    βˆƒ v p, NavierStokesExistenceAndSmoothnessRn nu uβ‚€ (f := 0) v p := by
  sorry

sorry is the open goal β€” a proof that compiles against mathlib settles this.

Related open statements (3)

navier_stokes_existence_and_smoothness_periodic

(B) Existence and smoothness of Navier–Stokes solutions in ℝ³/β„€Β³.

theorem navier_stokes_existence_and_smoothness_periodic (nu : ℝ) (hnu : nu > 0)
    (uβ‚€ : ℝ³ β†’ ℝ³) (huβ‚€ : InitialVelocityConditionPeriodic uβ‚€) :
    βˆƒ v p, NavierStokesExistenceAndSmoothnessPeriodic nu uβ‚€ (f := 0) v p := by
  sorry

navier_stokes_breakdown_R3

(C) Breakdown of Navier–Stokes solutions on ℝ³.

theorem navier_stokes_breakdown_R3 (nu : ℝ) (hnu : nu > 0) :
    βˆƒ (uβ‚€ : ℝ³ β†’ ℝ³) (f : ℝ³ β†’ ℝ β†’ ℝ³),
    InitialVelocityConditionDecay uβ‚€ ∧ ForceConditionDecay f ∧
    Β¬ (βˆƒ v p, NavierStokesExistenceAndSmoothnessRn nu uβ‚€ f v p) := by
  sorry

navier_stokes_breakdown_periodic

(D) Breakdown of Navier–Stokes Solutions on ℝ³/β„€Β³.

theorem navier_stokes_breakdown_periodic (nu : ℝ) (hnu : nu > 0) :
    βˆƒ (uβ‚€ : ℝ³ β†’ ℝ³) (f : ℝ³ β†’ ℝ β†’ ℝ³),
    InitialVelocityConditionPeriodic uβ‚€ ∧ ForceConditionPeriodic f ∧
    Β¬ (βˆƒ v p, NavierStokesExistenceAndSmoothnessPeriodic nu uβ‚€ f v p) := by
  sorry

Provenance

  • statement: google-deepmind/formal-conjectures (Apache-2.0), FormalConjectures/Millenium/NavierStokes.lean

Prize status

unsolved

Official page

https://www.claymath.org/millennium/navier-stokes-equation/

Research program

millennium_prize

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