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Sobolev Spaces

The idea of a Sobolev space is to differentiate weakly. A function u∈L2u \in L^2 need not have a classical derivative, but there may be a v∈L2v \in L^2 with

∫u φ′=−∫v φfor all φ∈Cc∞,\int u\,\varphi' = -\int v\,\varphi \quad \text{for all } \varphi \in C_c^\infty,

and if such vv exists it is the weak derivative of uu, written u′=vu' = v. Integration by parts is the definition rather than a theorem. The Sobolev space Wk,pW^{k,p} collects the functions whose weak derivatives up to order kk are in LpL^p, and for p=2p = 2 the space Hk=Wk,2H^k = W^{k,2} is a Hilbert space.

The reason PDE theory lives here is that PDEs are equations in derivatives, and the natural objects on which derivatives behave well are these spaces. Weak formulations turn differential equations into variational ones, the Lax–Milgram theorem; proved in the fundamental theorems page; gives existence and uniqueness, and elliptic regularity then promotes weak solutions to classical ones. Sobolev spaces are the language in which that promotion is stated.

The weak derivative is the derivative that integration by parts can see. Consider the function u(x)=∣x∣u(x) = |x| on (−1,1)(-1, 1): it has no derivative at 00, but its distributional derivative is the function v=sign⁡(x)v = \operatorname{sign}(x), because ∫−11∣x∣φ′(x) dx=−∫−11sign⁡(x)φ(x) dx\int_{-1}^{1} |x|\varphi'(x)\,dx = -\int_{-1}^{1}\operatorname{sign}(x)\varphi(x)\,dx for every test function; the kink integrates out. And vv is itself weakly differentiable, with v′=2δ0v' = 2\delta_0; the Dirac delta, not a function. So ∣x∣∈H1|x| \in H^1 but ∣x∣∉H2|x| \notin H^2.

That example carries the whole subject: each derivative costs one order of regularity, and the Sobolev scale is exactly the bookkeeping of how much smoothness is left after differentiating. Whether a boundary value problem has a classical solution becomes the question of whether enough orders of regularity survive, and the embedding theorems are the tool that answers it.

Definition. For k∈Nk \in \mathbb{N} and 1≤p≤∞1 \leq p \leq \infty,

Wk,p(Ω)={u∈Lp(Ω):Dαu∈Lp(Ω) for all ∣α∣≤k},∥u∥Wk,p=(∑∣α∣≤k∥Dαu∥Lpp)1/p,W^{k,p}(\Omega) = \big\{u \in L^p(\Omega) : D^\alpha u \in L^p(\Omega) \text{ for all } |\alpha| \leq k\big\}, \qquad \|u\|_{W^{k,p}} = \Big(\sum_{|\alpha| \leq k} \|D^\alpha u\|_{L^p}^p\Big)^{1/p},

where DαuD^\alpha u is the weak derivative and α\alpha ranges over multi-indices. For p=2p = 2 write HkH^k; the norm comes from the inner product ⟨u,v⟩Hk=∑∣α∣≤k⟨Dαu,Dαv⟩\langle u, v\rangle_{H^k} = \sum_{|\alpha| \le k} \langle D^\alpha u, D^\alpha v\rangle.

Theorem (completeness). Wk,p(Ω)W^{k,p}(\Omega) is a Banach space, and Hk(Ω)H^k(\Omega) is a Hilbert space.

Proof. The map u↦(Dαu)∣α∣≤ku \mapsto (D^\alpha u)_{|\alpha| \leq k} embeds Wk,pW^{k,p} isometrically into the product (Lp)N(L^p)^{N}, NN the number of multi-indices. The product is Banach, so it suffices to show the image is closed. Let un→uu_n \to u in Wk,pW^{k,p}; then Dαun→vαD^\alpha u_n \to v_\alpha in LpL^p for each α\alpha. For any test function φ\varphi, the definition of the weak derivative and LpL^p convergence give

∫u Dαφ=lim⁡n∫unDαφ=(−1)∣α∣lim⁡n∫Dαun φ=(−1)∣α∣∫vα φ,\int u\, D^\alpha\varphi = \lim_n \int u_n D^\alpha\varphi = (-1)^{|\alpha|}\lim_n \int D^\alpha u_n\, \varphi = (-1)^{|\alpha|} \int v_\alpha\, \varphi,

so vαv_\alpha is the weak derivative DαuD^\alpha u, and u∈Wk,pu \in W^{k,p} with Dαu=vαD^\alpha u = v_\alpha. Hence the image is closed. ■\blacksquare

The only analysis in the proof is that LpL^p limits commute with integration against a fixed test function, which is Hölder’s inequality. Completeness is otherwise pure functional analysis, and it is what licenses using the Banach and Hilbert space theorems; the open mapping theorem, uniform boundedness, Lax–Milgram; on spaces of functions.

Cc∞C_c^\infty is dense. In Wk,p(Ω)W^{k,p}(\Omega) for 1≤p<∞1 \leq p < \infty, the smooth compactly supported functions are dense (Meyers–Serrin). This is worth stating because its failure at p=∞p = \infty and its dependence on Ω\Omega at the boundary are the two places the theory surprises people. It means "Wk,pW^{k,p}" is not a bigger, stranger space than smooth functions; it is their completion, and every element is approximable.

Theorem (Poincaré). Let Ω⊂Rn\Omega \subset \mathbb{R}^n be bounded in some direction, and u∈W01,2(Ω)u \in W_0^{1,2}(\Omega); the closure of Cc∞(Ω)C_c^\infty(\Omega) in H1H^1. Then

∥u∥L2≤CΩ ∥∇u∥L2.\|u\|_{L^2} \leq C_\Omega\, \|\nabla u\|_{L^2}.

Proof for Ω=(0,L)\Omega = (0, L) in one dimension. For u∈Cc∞(0,L)u \in C_c^\infty(0, L) and x∈(0,L)x \in (0,L),

u(x)=∫0xu′(s) ds,u(x) = \int_0^x u'(s)\,ds,

since uu vanishes at the endpoints. Squaring and applying Cauchy–Schwarz,

∣u(x)∣2≤(∫0x12 ds)(∫0x∣u′(s)∣2ds)≤L ∥u′∥L22.|u(x)|^2 \leq \Big(\int_0^x 1^2\,ds\Big)\Big(\int_0^x |u'(s)|^2 ds\Big) \leq L\, \|u'\|_{L^2}^2.

Integrating over x∈(0,L)x \in (0,L): ∥u∥L22≤L2∥u′∥L22\|u\|_{L^2}^2 \leq L^2\|u'\|_{L^2}^2, so CΩ=LC_\Omega = L works. The case of general u∈W01,2u \in W_0^{1,2} follows by density. ■\blacksquare

The proof is two lines, and it is worth noticing what the two hypotheses do. Vanishing at the boundary is what made the fundamental theorem applicable; for the constant function u=1u = 1, which has ∥∇u∥=0\|\nabla u\| = 0, the inequality is false, and constants are exactly the elements of H1H^1 removed by the W01,2W_0^{1,2} condition. And boundedness of Ω\Omega is what made LL finite; Poincaré fails on unbounded domains for the same reason, and its repair there requires a weight or a spectral gap.

Poincaré is the Poincaré inequality of the spectral theory of the Laplacian: applied to −Δ-\Delta with Dirichlet conditions, it says the first eigenvalue λ1≥CΩ−2>0\lambda_1 \geq C_\Omega^{-2} > 0, which is why the Laplacian’s spectrum is discrete and why solutions of the heat equation decay.

Theorem (Sobolev embedding). Let Ω⊂Rn\Omega \subset \mathbb{R}^n be bounded with smooth boundary. Then

Wk,p(Ω)↪Lq(Ω)where1q=1p−kn,q<∞,W^{k,p}(\Omega) \hookrightarrow L^q(\Omega) \quad\text{where}\quad \frac{1}{q} = \frac{1}{p} - \frac{k}{n}, \qquad q < \infty,

and if 1p−kn<0\frac{1}{p} - \frac{k}{n} < 0, then Wk,p↪C0,αW^{k,p} \hookrightarrow C^{0,\alpha} with α=k−n/p\alpha = k - n/p.

Proof for the sharpest case in one dimension, W1,2(0,L)↪C0W^{1,2}(0,L) \hookrightarrow C^0. For u∈C∞u \in C^\infty and x,y∈(0,L)x, y \in (0,L),

∣u(x)−u(y)∣=∣∫yxu′(s) ds∣≤∣x−y∣  ∥u′∥L2,|u(x) - u(y)| = \Big|\int_y^x u'(s)\,ds\Big| \leq \sqrt{|x - y|}\;\|u'\|_{L^2},

by Cauchy–Schwarz. So uu is Hölder continuous with exponent 1/21/2 and constant ∥u′∥L2\|u'\|_{L^2}. For the sup norm, fix any x0x_0:

∣u(x)∣≤∣u(x0)∣+L ∥u′∥L2,|u(x)| \leq |u(x_0)| + \sqrt{L}\,\|u'\|_{L^2},

and averaging over x0x_0 gives ∣u(x0)∣≤L−1/2∥u∥L2|u(x_0)| \leq L^{-1/2}\|u\|_{L^2} for some choice, so

∥u∥∞≤L−1/2∥u∥L2+L ∥u′∥L2≤C ∥u∥H1.\|u\|_\infty \leq L^{-1/2}\|u\|_{L^2} + \sqrt{L}\,\|u'\|_{L^2} \leq C\,\|u\|_{H^1}.

Density of C∞C^\infty in H1H^1 extends the inequality, and a uniform limit of continuous functions is continuous, giving the embedding. ■\blacksquare

The two-dimensional statement 1q=12−12=0\frac{1}{q} = \frac{1}{2} - \frac{1}{2} = 0 is the borderline, and the theorem correctly refuses to say H1(R2)↪L∞H^1(\mathbb{R}^2) \hookrightarrow L^\infty: it embeds into every LqL^q for q<∞q < \infty and not into L∞L^\infty. The standard counterexample family is uϵ(x)=log⁡log⁡(∣x∣−1)u_\epsilon(x) = \log\log(|x|^{-1}) truncated near 00, whose H1H^1 norm stays bounded while its supremum tends to infinity. That borderline is exactly where Φ24\Phi^4_2‘s renormalisation lives, as in the stochastic PDE page: the critical dimension is the one where the embedding into L∞L^\infty fails.

4. Rellich–Kondrachov: where compactness comes from

Section titled “4. Rellich–Kondrachov: where compactness comes from”

Theorem (Rellich–Kondrachov). With Ω\Omega bounded and smooth, W1,2(Ω)↪↪L2(Ω)W^{1,2}(\Omega) \hookrightarrow\hookrightarrow L^2(\Omega): the embedding is compact, meaning bounded sets in H1H^1 have subsequences converging in L2L^2.

Proof idea. Boundedness in H1H^1 bounds the L2L^2 norms of both uu and ∇u\nabla u. The gradient bound gives an equicontinuity-type estimate after averaging: convolution with a mollifier ρδ\rho_\delta satisfies

∥u∗ρδ−u∥L2≤δ ∥∇u∥L2,\|u * \rho_\delta - u\|_{L^2} \leq \delta\,\|\nabla u\|_{L^2},

uniformly for uu in a bounded set, while {u∗ρδ}\{u * \rho_\delta\} is bounded and equi-uniformly-continuous in L∞L^\infty for fixed δ\delta. The Arzelà–Ascoli theorem then gives a uniformly convergent subsequence of the mollified family, and letting δ→0\delta \to 0 along a diagonal subsequence extracts an L2L^2- convergent subsequence of the original. ■\blacksquare

This is the only source of compactness in the theory, and it is what makes the Dirichlet Laplacian have a discrete spectrum: an operator with compact resolvent has eigenvalues marching to infinity, and Rellich–Kondrachov is the compactness of the resolvent. The heat kernel’s decay, the convergence of spectral approximations, and the existence of eigenfunction bases all trace back here.

The pipeline that solves a PDE is now complete:

  1. Weak solution. Lax–Milgram gives u∈H01(Ω)u \in H_0^1(\Omega) with a(u,v)=⟨f,v⟩a(u, v) = \langle f, v\rangle for all vv; existence, uniqueness, continuous dependence.
  2. Improved integrability. Sobolev embedding turns H1H^1 control into LqL^q control, so the solution is a function with integrable powers.
  3. Interior regularity. Difference quotients, controlled uniformly using the equation, show u∈Hloc2u \in H^2_{\mathrm{loc}} and by iteration u∈Hlocmu \in H^m_{\mathrm{loc}} for every mm when ff is smooth.
  4. Classical solution. Sobolev embedding with mm large enough makes uu continuous, then C1C^1, then C2C^2; at which point the weak equation holds pointwise and uu is a classical solution.

Each arrow is a theorem; none is optional. Step 3 is the elliptic regularity that the Hodge theory page uses as a black box to put smooth representatives on de Rham classes, and step 4’s threshold m>n/2+jm > n/2 + j for CjC^j regularity is the Sobolev embedding theorem again, with nn the dimension.

  • Confusing weak and classical derivatives. A weak derivative is an equivalence class defined by integration by parts; it may fail to exist even where a pointwise derivative exists, and it may exist where no classical derivative does. ∣x∣|x| is the standard example in both directions.
  • Applying Poincaré without the boundary condition. Constants have zero gradient. On H1H^1 rather than W01,2W_0^{1,2}, add ∥u∥L2\|u\|_{L^2} to the right side, or quotient out constants.
  • Reading the embedding theorem at the borderline. When 1p=kn\frac{1}{p} = \frac{k}{n} the embedding into L∞L^\infty fails; into every finite qq it holds. The failure is not a weakness of the method but the critical case, and it is where renormalisation appears.
  • Assuming Cc∞C_c^\infty is dense in every Sobolev space on every domain. For Wk,pW^{k,p} with p=∞p = \infty it is false, and for domains with bad boundaries the closure can be a strict subspace (W01,pW_0^{1,p} rather than W1,pW^{1,p}), which is a boundary condition in disguise.
  • Expecting Sobolev functions to be continuous. H1H^1 functions in one dimension are continuous; that is the embedding; but in two dimensions they need not be, and in nn dimensions a Wk,pW^{k,p} function is continuous only when k>n/pk > n/p. The whole subject is the bookkeeping of that threshold.