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Existence and Smoothness of the Navier-Stokes Equation
Source of package cmi.navier_stokes · claymath.org/wp-content/uploads/2022/06/navierstokes.pdf
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- urn:org:cmi:navier-stokes#treatise
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| URI | Type | documentHash | Retrieved |
|---|---|---|---|
| https://www.claymath.org/wp-content/uploads/2022/06/navierstokes.pdf | text/plain; charset=utf-8 | sha256:4784ff5ad4b227c37b8f42cb743d95fd9903bd11eb141e604818feb0d5e908e0 | 2026-09-17T00:00:00Z |
Fragments — 18
ckn-intro · defn
en · official · sha256:9336a13df97aa5ec1a143a1453f633d442474b82fb0050b875b8b81f0645aee2
Scheffer [7] applied ideas from geometric measure theory to prove a partial regularity theorem for suitable weak solutions of the Navier-Stokes equations. Caffarelli-Kohn-Nirenberg [2] improved Scheffer's results, and F.-H. Lin [6] simplified the proofs of the results in Caffarelli-Kohn-Nirenberg [2]. The partial regularity theorem of [2], [6] concerns a parabolic analogue of the Hausdorff dimension of the singular set of a suitable weak solution of Navier-Stokes. Here, the singular set of a weak solution u consists of all points (x_o,t_o) in R^3 x R such that u is unbounded in every neighborhood of (x_o,t_o).ckn-theorem · lemma · referenced by: 1
en · official · sha256:c8615dfc0535f06fd425853049f9ebea9a355f9fe49965682782c3af2f0283d6
The main results of [2], [6] may be stated roughly as follows. Theorem. (A) Let u be a weak solution of the Navier-Stokes equations, satisfying suitable growth conditions. Let E be the singular set of u. Then P_1(E) = 0. (B) Given a divergence-free vector field u_o(x) and a force f(x,t) satisfying (4) and (5), there exists a weak solution of Navier-Stokes (1), (2), (3) satisfying the growth conditions in (A). In particular, the singular set of u cannot contain a spacetime curve of the form {(x,t) in R^3 x R: x = phi(t)}. This is the best partial regularity theorem known so far for the Navier-Stokes equation.Referencing norms: names-caffarelli-kohn-nirenberg-1982
decay-conditions-4-5 · defn · referenced by: 1
en · official · sha256:20daae86b55b08e8845299d2a51621095b123b11e15c831c2cf8c47a41c0f1a0
Equation (1) is just Newton's law f=ma for a fluid element subject to the external force f=(f_i(x,t))_{1<=i<=n} and to the forces arising from pressure and friction. Equation (2) just says that the fluid is incompressible. For physically reasonable solutions, we want to make sure u(x,t) does not grow large as |x| -> infinity. Hence, we will restrict attention to forces f and initial conditions u_o that satisfy |d^alpha_x u_o(x)| <= C_{alpha K}(1+|x|)^{-K} on R^n, for any alpha and K, (4); and |d^alpha_x d^m_t f(x,t)| <= C_{alpha m K}(1+|x|+t)^{-K} on R^n x [0,infinity), for any alpha, m, K, (5).Referencing norms: defines-decay-conditions
equations-1-2-3 · defn · referenced by: 1
en · official · sha256:a824600228a8063d957ccb7860a72a1587d95b359affb2176a214ba6ab2bda99
The Navier-Stokes equations are then given by (d/dt)u_i + sum_{j=1}^n u_j (d u_i/d x_j) = nu*Delta(u_i) - (d p/d x_i) + f_i(x,t) (x in R^n, t >= 0), (1); div u = sum_{i=1}^n (d u_i/d x_i) = 0 (x in R^n, t >= 0), (2); with initial conditions u(x,0) = u_o(x) (x in R^n), (3).Referencing norms: defines-equations
leray-note · defn · referenced by: 1
en · official · sha256:bc5a2f7485912852de329fceae77869226b76f92a46406449428130e553ef44a
Starting with Leray [5], important progress has been made in understanding weak solutions of the Navier-Stokes equations. Leray in [5] showed that the Navier-Stokes equations (1), (2), (3) in three space dimensions always have a weak solution (p,u) with suitable growth properties. Uniqueness of weak solutions of the Navier-Stokes equation is not known.Referencing norms: names-leray-1934
partial-results · defn · referenced by: 1
en · official · sha256:5ae011cf79adfafbd9e635a8e11cee7559a7440fea03cfeedabb635bbd62a956
In two dimensions, the analogues of assertions (A) and (B) have been known for a long time (Ladyzhenskaya [4]), also for the more difficult case of the Euler equations. This gives no hint about the three-dimensional case, since the main difficulties are absent in two dimensions. In three dimensions, it is known that (A) and (B) hold provided the initial velocity u_o satisfies a smallness condition. For initial data u_o(x) not assumed to be small, it is known that (A) and (B) hold (also for nu=0) if the time interval [0,infinity) is replaced by a small time interval [0,T), with T depending on the initial data. For a given initial u_o(x), the maximum allowable T is called the "blowup time." Either (A) and (B) hold, or else there is a smooth, divergence-free u_o(x) for which (1), (2), (3) have a solution with a finite blowup time. For the Navier-Stokes equations (nu>0), if there is a solution with a finite blowup time T, then the velocity (u_i(x,t))_{1<=i<=3} becomes unbounded near the blowup time.Referencing norms: names-ladyzhenskaya-2d
periodic-force-decay-9 · defn
en · official · sha256:86f09b52246331732907ba2498ecc6644d271e44d82194cf3f06a89c05663bdf
In place of (4) and (5), we assume that u_o is smooth and that |d^alpha_x d^m_t f(x,t)| <= C_{alpha m K}(1+|t|)^{-K} on R^3 x [0,infinity), for any alpha, m, K, (9).periodic-setup-8 · defn · referenced by: 1
en · official · sha256:c81dc9ebd5668337c24004cc89b81e5d431919a06eb765c5fd429e3ec3bc55d5
Alternatively, to rule out problems at infinity, we may look for spatially periodic solutions of (1), (2), (3). Thus, we assume that u_o(x), f(x,t) satisfy u_o(x+e_j) = u_o(x), f(x+e_j,t) = f(x,t) for 1 <= j <= n (e_j = j-th unit vector in R^n), (8).Referencing norms: defines-periodic-setup
physically-reasonable-6-7 · defn · referenced by: 1
en · official · sha256:268c2dfa3f7c44478be64ed1d285b8d703ebd017031b0550e435bad2f4c98395
We accept a solution of (1), (2), (3) as physically reasonable only if it satisfies p, u in C-infinity(R^n x [0,infinity)), (6); and integral over R^n of |u(x,t)|^2 dx < C for all t >= 0 (bounded energy), (7).Referencing norms: defines-physically-reasonable-r3
physically-reasonable-torus-10-11 · defn · referenced by: 1
en · official · sha256:402e16d80a3dec5777ab6bdbc22c16b8e298a92130f1fc9ff21ebfa3505c6c68
We then accept a solution of (1), (2), (3) as physically reasonable if it satisfies u(x,t) = u(x+e_j,t) on R^3 x [0,infinity) for 1 <= j <= n, (10); and p, u in C-infinity(R^n x [0,infinity)), (11).Referencing norms: defines-physically-reasonable-torus
problem-intro · defn
en · official · sha256:88e54f969e9dfb60bf45da6cbcdac7a5c445047c44edc2ecc9d3f0dd51ec3f12
A fundamental problem in analysis is to decide whether such smooth, physically reasonable solutions exist for the Navier-Stokes equations. To give reasonable leeway to solvers while retaining the heart of the problem, we ask for a proof of one of the following four statements.setup · defn
en · official · sha256:4ebfc476c2526209d72430f55ca1f18e953418959ac1493c82efe06e92429efb
The Euler and Navier-Stokes equations describe the motion of a fluid in R^n (n = 2 or 3). These equations are to be solved for an unknown velocity vector u(x,t) = (u_i(x,t))_{1<=i<=n} in R^n and pressure p(x,t) in R, defined for position x in R^n and time t >= 0. We restrict attention here to incompressible fluids filling all of R^n.statement-a · lemma · referenced by: 3
en · official · sha256:a5a4fd9bcca3359185acc5c38c48819eb2c6e7352c2953d36b6fb5a07458ad80
(A) Existence and smoothness of Navier-Stokes solutions on R^3. Take nu > 0 and n = 3. Let u_o(x) be any smooth, divergence-free vector field satisfying (4). Take f(x,t) to be identically zero. Then there exist smooth functions p(x,t), u_i(x,t) on R^3 x [0,infinity) that satisfy (1), (2), (3), (6), (7).Referencing norms: NsStatementA, a-identifies-ns, source-asserts-a
statement-b · lemma · referenced by: 3
en · official · sha256:c544b48bbef171506c5721782610879e79fbdf434187b7b868f57c4a769bd743
(B) Existence and smoothness of Navier-Stokes solutions in R^3/Z^3. Take nu > 0 and n = 3. Let u_o(x) be any smooth, divergence-free vector field satisfying (8); we take f(x,t) to be identically zero. Then there exist smooth functions p(x,t), u_i(x,t) on R^3 x [0,infinity) that satisfy (1), (2), (3), (10), (11).Referencing norms: NsStatementB, b-identifies-ns, source-asserts-b
statement-c · lemma · referenced by: 3
en · official · sha256:d15b6ab7951163b99617f35acf92e044f18e691263dd2e8e69db7c2fc95eda11
(C) Breakdown of Navier-Stokes solutions on R^3. Take nu > 0 and n = 3. Then there exist a smooth, divergence-free vector field u_o(x) on R^3 and a smooth f(x,t) on R^3 x [0,infinity), satisfying (4), (5), for which there exist no solutions (p,u) of (1), (2), (3), (6), (7) on R^3 x [0,infinity).Referencing norms: NsStatementC, c-identifies-ns, source-asserts-c
statement-d · lemma · referenced by: 3
en · official · sha256:a303c9e04ed321e872746256b5b52e61d1f4bbba4c5af23122c3abc6847f745e
(D) Breakdown of Navier-Stokes Solutions on R^3/Z^3. Take nu > 0 and n = 3. Then there exist a smooth, divergence-free vector field u_o(x) on R^3 and a smooth f(x,t) on R^3 x [0,infinity), satisfying (8), (9), for which there exist no solutions (p,u) of (1), (2), (3), (10), (11) on R^3 x [0,infinity).Referencing norms: NsStatementD, d-identifies-ns, source-asserts-d
terms-def · defn
en · official · sha256:14aa4d292fd311ea8e80ab3877c828ebc1f9d56f8942ba35f4273e87a3d37e88
Here, u_o(x) is a given, C-infinity divergence-free vector field on R^n, f_i(x,t) are the components of a given, externally applied force (e.g. gravity), nu is a positive coefficient (the viscosity), and Delta = sum_{i=1}^n (d^2/d x_i^2) is the Laplacian in the space variables. The Euler equations are equations (1), (2), (3) with nu set equal to zero.title · defn · referenced by: 5
en · official · sha256:9f2830e575377bd2c7075a55939c430d0caf841c1eb5d2b3c9f2bb49351e89fb
EXISTENCE AND SMOOTHNESS OF THE NAVIER-STOKES EQUATIONReferencing norms: CmiNavierStokesSource, a-classified, classified_as_millennium_problem, defines_notion, names_historical_result
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