Book 4A

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Course 4Book 4A: Function Spaces and Sobolev SpacesChapter 10

Sobolev Embeddings and Critical Exponents

Scaling, embeddings, Rellich compactness, and how compactness fails at the critical exponent.

28 min read · Updated Oct 2, 2026

Read with Brezis, chapter 9, the sections on Sobolev inequalities (Gagliardo–Nirenberg–Sobolev, Morrey, the case p=np = n) and on compact embeddings (Rellich–Kondrachov); Evans §5.6–5.7 is a good second voice. Start with this chapter's scaling section, which predicts every exponent before it is proved.

In this chapter · 8 sections
  1. 10.1Why bubbles are round
  2. 10.2Scaling first
  3. 10.3The Gagliardo–Nirenberg–Sobolev inequality
  4. 10.3.1Sobolev inequalities are isoperimetric inequalities
  5. 10.4Morrey's inequality
  6. 10.5Rellich–Kondrachov: compactness restored
  7. 10.6Failure at the critical exponent
  8. 10.7History
  9. 10.8Exercises

A Sobolev function has derivatives in LpL^p. What does that say about the function itself? This chapter's theorems answer exactly. If p<np < n, the function is in Lp∗L^{p^*} for a larger exponent p∗=npn−pp^* = \frac{np}{n - p} (Gagliardo–Nirenberg–Sobolev). If p>np > n, it is Hölder continuous (Morrey). And on a bounded domain or a closed manifold, the embedding into LqL^q is compact for every q<p∗q < p^* (Rellich–Kondrachov), which is the theorem that finally restores compactness to the analysis of PDE, completing the spectral theorem of 4A.7 Compact Operators and Spectra and the Poincaré inequality of 4A.9 Sobolev Spaces.

All the exponents can be predicted before anything is proved, by dimensional analysis: an inequality that holds for all functions on Rn\mathbb{R}^n must be unchanged when the functions are rescaled, and that pins down the exponent. This is thread S at its most effective, and it also explains the chapter's last theme. At the critical exponent p∗p^* the inequality is scale-invariant, and compactness fails, because a function can concentrate into a tall narrow bubble without changing either side. Loss of compactness by concentration, repaired by rescaling, is the mechanism of singularity analysis in Ricci flow.

By the end of this chapter you will be able to:

  • derive the Sobolev exponents by scaling, and place any space Wk,pW^{k,p} on the "Sobolev number line" k−n/pk - n/p;
  • state and use the Gagliardo–Nirenberg–Sobolev and Morrey inequalities, and prove the former in the plane;
  • explain the equivalence between the L1L^1 Sobolev inequality and the isoperimetric inequality;
  • prove the Rellich–Kondrachov theorem for H01H^1_0, and use it to finish the Dirichlet spectral theorem;
  • show that compactness fails at the critical exponent by concentration, and explain how rescaling repairs it.

Why bubbles are round

In the world Model The isoperimetric inequality

A soap bubble encloses a fixed volume of air, and surface tension pulls its film to the least area that can enclose it. The result is a sphere, because among all shapes of a given volume the sphere has the smallest surface area: the isoperimetric inequality. In three dimensions, a region of volume VV has surface area at least (36π)1/3V2/3(36\pi)^{1/3}V^{2/3}, with equality only for balls. For volume 11, a sphere has area 4.844.84, a cube 66. In the plane, a region of area AA has perimeter at least 2πA2\sqrt{\pi A}; for area 11, a disc has perimeter 3.543.54, a square 44.

Small water droplets on a surface are nearly spherical caps for the same reason, until gravity competes with surface tension. The competition is measured by the Bond number Bo=ρgL2/σ\mathrm{Bo} = \rho gL^2/\sigma (density, gravity, size, surface tension). It is a ratio of energies that scale differently with size: surface energy like L2L^2, gravitational energy like L4L^4. Below the capillary length σ/ρg\sqrt{\sigma/\rho g}, about 2.72.7 mm for water, surface tension wins and drops are round; well above it, gravity flattens them into puddles. A scaling argument, comparing how two energies change with size, predicts the shape. This chapter does the same for function spaces.

Herbert Federer and Wendell Fleming, and independently Vladimir Maz'ya, showed in 1960 that the isoperimetric inequality and the L1L^1 Sobolev inequality are the same statement, with the same best constant: the first is the second applied to (approximations of) the indicator function of a region (Theorem 10.2). Sobolev inequalities are isoperimetric inequalities for functions.

Scaling first

Suppose an inequality ∥u∥Lq(Rn)≤C∥∇u∥Lp(Rn)\|u\|_{L^q(\mathbb{R}^n)} \leq C\|\nabla u\|_{L^p(\mathbb{R}^n)} held for all smooth compactly supported uu. Replace uu by uλ(x)=u(λx)u_\lambda(x) = u(\lambda x). By the scaling rules of 3A.5 Product Measures and Change of Variables,

∥uλ∥q=λ−n/q∥u∥q,∥∇uλ∥p=λ1−n/p∥∇u∥p.\|u_\lambda\|_q = \lambda^{-n/q}\|u\|_q, \qquad \|\nabla u_\lambda\|_p = \lambda^{1 - n/p}\|\nabla u\|_p.

So the inequality says λ−n/q∥u∥q≤Cλ1−n/p∥∇u∥p\lambda^{-n/q}\|u\|_q \leq C\lambda^{1-n/p}\|\nabla u\|_p for every λ>0\lambda > 0. Unless the powers of λ\lambda agree, letting λ→0\lambda \to 0 or ∞\infty forces u=0u = 0. So the only possible exponent is given by

−nq=1−np,that is,q=p∗=npn−p(p<n).-\frac nq = 1 - \frac np, \qquad\text{that is,}\qquad q = p^* = \frac{np}{n - p} \quad (p < n).

For p=2p = 2 in dimension 33, p∗=6p^* = 6; in dimension nn, 2∗=2nn−22^* = \frac{2n}{n-2}. The exponent comes from dimensions alone, before any analysis.

The same bookkeeping organises everything: assign to Wk,pW^{k,p} the number k−npk - \frac np ("derivatives minus dimension over integrability"), and to the Hölder space Cm,αC^{m,\alpha} the number m+αm + \alpha. Sobolev's theorems say that a space embeds in the spaces with smaller numbers: W1,pW^{1,p} (number 1−np1 - \frac np) in Lp∗L^{p^*} (number −np∗=1−np-\frac{n}{p^*} = 1 - \frac np, equal), and in C0,1−n/pC^{0, 1 - n/p} when 1−np>01 - \frac np > 0 (Figure 10.1). Embeddings into spaces with strictly smaller numbers are compact on bounded domains; the borderline ones are not.

Figure 10.1. The Sobolev number line. Each space sits at k−n/pk - n/p (Sobolev) or m+αm + \alpha (Hölder). A space embeds into any space at the same point or to its left (with the LpL^p-type restrictions of the theorems); embeddings strictly to the left are compact on bounded domains, and points to the right of 00 consist of continuous functions. Examples shown are for n=2n = 2 or 33.

The Gagliardo–Nirenberg–Sobolev inequality

Theorem 10.1 Gagliardo–Nirenberg–Sobolev

For 1≤p<n1 \leq p < n there is C=C(n,p)C = C(n, p) such that for all u∈W1,p(Rn)u \in W^{1,p}(\mathbb{R}^n),

∥u∥Lp∗(Rn)≤C ∥∇u∥Lp(Rn),p∗=npn−p.\|u\|_{L^{p^*}(\mathbb{R}^n)} \leq C\,\|\nabla u\|_{L^p(\mathbb{R}^n)}, \qquad p^* = \frac{np}{n - p}.

We prove the key case p=1p = 1 in the plane, where the idea is visible, and then explain the rest.

Proof. Case n=2n = 2, p=1p = 1, p∗=2p^* = 2. By density take uu smooth with compact support. For each point, integrating ∂1u\partial_1u along the horizontal line and ∂2u\partial_2u along the vertical line through it,

∣u(x1,x2)∣≤∫R∣∇u(t,x2)∣ dt=:g2(x2),∣u(x1,x2)∣≤∫R∣∇u(x1,s)∣ ds=:g1(x1).|u(x_1, x_2)| \leq \int_{\mathbb{R}}|\nabla u(t, x_2)|\,dt =: g_2(x_2), \qquad |u(x_1, x_2)| \leq \int_{\mathbb{R}}|\nabla u(x_1, s)|\,ds =: g_1(x_1).

Multiply: ∣u(x)∣2≤g1(x1) g2(x2)|u(x)|^2 \leq g_1(x_1)\,g_2(x_2). The right side is a product of a function of x1x_1 and a function of x2x_2, so by Tonelli (3A.5 Product Measures and Change of Variables)

∫R2∣u∣2≤∫g1(x1) dx1∫g2(x2) dx2=∥∇u∥12.\int_{\mathbb{R}^2}|u|^2 \leq \int g_1(x_1)\,dx_1\int g_2(x_2)\,dx_2 = \|\nabla u\|_1^2.

So ∥u∥2≤∥∇u∥1\|u\|_2 \leq \|\nabla u\|_1.

General nn, p=1p = 1. The same idea, bounding ∣u∣|u| by the integral of ∣∇u∣|\nabla u| along the line through xx in each of the nn coordinate directions, gives ∣u∣n/(n−1)≤∏igi1/(n−1)|u|^{n/(n-1)} \leq \prod_i g_i^{1/(n-1)} with each gig_i independent of xix_i; integrating one variable at a time with Hölder's inequality ("Gagliardo's lemma") gives ∥u∥n/(n−1)≤∥∇u∥1\|u\|_{n/(n-1)} \leq \|\nabla u\|_1 (Evans §5.6.1).

General p<np < n. Apply the p=1p = 1 case to ∣u∣γ|u|^\gamma for a suitable γ>1\gamma > 1, and use Hölder on ∫∣u∣γ−1∣∇u∣\int|u|^{\gamma-1}|\nabla u|; the choice γ=p(n−1)n−p\gamma = \frac{p(n-1)}{n-p} makes the exponents match (Exercise 10.6).

On a bounded domain, the same holds for u∈W01,p(Ω)u \in W^{1,p}_0(\Omega) (extend by zero), and for all of W1,p(Ω)W^{1,p}(\Omega) on a C1C^1 domain with ∥u∥W1,p\|u\|_{W^{1,p}} on the right (extend, 4A.9 Sobolev Spaces). Since Ω\Omega has finite measure, Lp∗(Ω)⊆Lq(Ω)L^{p^*}(\Omega) \subseteq L^q(\Omega) for every q≤p∗q \leq p^* (3A.7 Lᵖ Spaces and Jensen’s Inequality), so W1,p(Ω)↪Lq(Ω)W^{1,p}(\Omega) \hookrightarrow L^q(\Omega) for 1≤q≤p∗1 \leq q \leq p^*.

Sobolev inequalities are isoperimetric inequalities

Theorem 10.2 Sobolev implies isoperimetry

If ∥u∥n/(n−1)≤C∥∇u∥1\|u\|_{n/(n-1)} \leq C\|\nabla u\|_1 for all u∈Cc∞(Rn)u \in C_c^\infty(\mathbb{R}^n), then every bounded region EE with smooth boundary satisfies

∣E∣(n−1)/n≤C⋅Area(∂E).|E|^{(n-1)/n} \leq C\cdot\mathrm{Area}(\partial E).

Proof. Let uεu_\varepsilon be 11 on EE, 00 at distance more than ε\varepsilon from EE, and decreasing linearly in the distance to EE in between. Then ∥uε∥n/(n−1)≥∣E∣(n−1)/n\|u_\varepsilon\|_{n/(n-1)} \geq |E|^{(n-1)/n}, and ∣∇uε∣=1ε|\nabla u_\varepsilon| = \frac1\varepsilon on the shell of width ε\varepsilon around EE, whose volume is about ε⋅Area(∂E)\varepsilon\cdot\mathrm{Area}(\partial E). So ∥∇uε∥1→Area(∂E)\|\nabla u_\varepsilon\|_1 \to \mathrm{Area}(\partial E) as ε→0\varepsilon \to 0. (uεu_\varepsilon is Lipschitz, not smooth; mollify, or use density in W1,1W^{1,1}.)

The converse also holds, with the same constant, via the coarea formula, which writes ∫∣∇u∣\int|\nabla u| as the integral over tt of the areas of the level sets {u=t}\{u = t\} (Federer–Fleming; Maz'ya). The best constant is the isoperimetric one, C=(nωn1/n)−1C = \big(n\omega_n^{1/n}\big)^{-1}, attained (in the limit) by balls. This equivalence is the cleanest instance of a principle that recurs in geometry: an analytic inequality for all functions encodes a geometric inequality for all regions. On a Riemannian manifold, Sobolev constants are controlled by isoperimetric constants, and both are controlled by curvature and volume (9B.2 Volume Comparison).

Morrey's inequality

When p>np > n the number 1−np1 - \frac np is positive, and the functions are continuous.

Theorem 10.3 Morrey

For n<p≤∞n < p \leq \infty there is C=C(n,p)C = C(n, p) such that every u∈W1,p(Rn)u \in W^{1,p}(\mathbb{R}^n) has a representative with

∣u(x)−u(y)∣≤C ∣x−y∣1−n/p ∥∇u∥Lpandsup⁡∣u∣≤C∥u∥W1,p.|u(x) - u(y)| \leq C\,|x - y|^{1 - n/p}\,\|\nabla u\|_{L^p} \quad\text{and}\quad \sup|u| \leq C\|u\|_{W^{1,p}}.

Idea of the proof (Evans §5.6.2). For smooth uu, the average of ∣u(y)−u(x)∣|u(y) - u(x)| over a ball B(x,r)B(x, r) is bounded by C∫B(x,r)∣∇u(y)∣∣x−y∣n−1 dyC\int_{B(x,r)}\frac{|\nabla u(y)|}{|x - y|^{n-1}}\,dy (integrate ∇u\nabla u along rays from xx). By Hölder, that is at most C∥∇u∥p(∫B(x,r)∣x−y∣−(n−1)qdy)1/qC\|\nabla u\|_p\big(\int_{B(x,r)}|x - y|^{-(n-1)q}dy\big)^{1/q}, which is finite exactly when (n−1)q<n(n - 1)q < n, that is p>np > n, and then it equals Cr1−n/p∥∇u∥pCr^{1 - n/p}\|\nabla u\|_p. Comparing u(x)u(x) and u(y)u(y) through the average over a ball containing both, of radius ∣x−y∣|x - y|, gives the Hölder estimate. In one dimension it is 4A.9 Sobolev Spaces's Hölder bound.

At the borderline p=np = n, functions need not be bounded (log⁡log⁡(1+1/∣x∣)\log\log(1 + 1/|x|) in H1(R2)H^1(\mathbb{R}^2), 4A.5 The Fourier Transform); they are exponentially integrable instead (Trudinger, 1967), and they lie in every LlocqL^q_{\mathrm{loc}} with q<∞q < \infty.

For higher derivatives the inequalities iterate. Wk,p↪LqW^{k,p} \hookrightarrow L^q with 1q=1p−kn\frac1q = \frac1p - \frac kn when kp<nkp < n, and Wk,p↪Cm,αW^{k,p} \hookrightarrow C^{m,\alpha} when k−np>m+αk - \frac np > m + \alpha with 0<α<10 < \alpha < 1 (and in borderline cases with care). This is what lets smoothness be proved one derivative at a time in L2L^2 and converted to classical derivatives at the end: a function in Hk(Rn)H^k(\mathbb{R}^n) for every kk is smooth.

Rellich–Kondrachov: compactness restored

Theorem 10.4 Rellich–Kondrachov

Let Ω\Omega be a bounded open set in Rn\mathbb{R}^n with C1C^1 boundary, or a closed Riemannian manifold, and 1≤p<n1 \leq p < n. Then the embedding W1,p(Ω)↪Lq(Ω)W^{1,p}(\Omega) \hookrightarrow L^q(\Omega) is compact for every 1≤q<p∗1 \leq q < p^*. If p≥np \geq n it is compact for every q<∞q < \infty (and into continuous functions if p>np > n). The same holds for W01,p(Ω)W^{1,p}_0(\Omega) on any bounded open Ω\Omega.

Here is a complete proof in the case used most, H01(Ω)↪L2(Ω)H^1_0(\Omega) \hookrightarrow L^2(\Omega), which is Arzelà–Ascoli (2B.5 Uniform Convergence and Arzelà–Ascoli) in disguise.

Proof. Let (uk)(u_k) be bounded in H01(Ω)H^1_0(\Omega), ∥uk∥H1≤M\|u_k\|_{H^1} \leq M; extend by zero to functions in H1(Rn)H^1(\mathbb{R}^n) supported in the bounded set Ωˉ\bar\Omega.

Step 1: mollification costs little. For smooth uu and the mollifier ϕε\phi_\varepsilon of 3A.8 Convolution and Mollifiers, u(x−y)−u(x)=−∫01∇u(x−ty)⋅y dtu(x - y) - u(x) = -\int_0^1\nabla u(x - ty)\cdot y\,dt, so by Minkowski's integral inequality ∥u(⋅−y)−u∥2≤∣y∣ ∥∇u∥2\|u(\cdot - y) - u\|_2 \leq |y|\,\|\nabla u\|_2, and averaging over yy against ϕε\phi_\varepsilon,

∥u∗ϕε−u∥2≤ε ∥∇u∥2≤εM.\|u * \phi_\varepsilon - u\|_2 \leq \varepsilon\,\|\nabla u\|_2 \leq \varepsilon M.

By density this holds for every uku_k.

Step 2: for fixed ε\varepsilon, the mollified family is compact. The functions uk∗ϕεu_k * \phi_\varepsilon are supported in a fixed compact set (the ε\varepsilon-neighbourhood of Ωˉ\bar\Omega), uniformly bounded (∣uk∗ϕε∣≤∥uk∥2∥ϕε∥2|u_k * \phi_\varepsilon| \leq \|u_k\|_2\|\phi_\varepsilon\|_2), and uniformly Lipschitz (∣∇(uk∗ϕε)∣≤∥uk∥2∥∇ϕε∥2|\nabla(u_k * \phi_\varepsilon)| \leq \|u_k\|_2\|\nabla\phi_\varepsilon\|_2). By Arzelà–Ascoli a subsequence converges uniformly, hence in L2L^2 on the bounded support.

Step 3: diagonal argument. Take ε=1,12,13,…\varepsilon = 1, \tfrac12, \tfrac13, \ldots, extracting successively, and take the diagonal subsequence (vj)(v_j). For any ε=1m\varepsilon = \frac1m, ∥vi−vj∥2≤2εM+∥vi∗ϕε−vj∗ϕε∥2\|v_i - v_j\|_2 \leq 2\varepsilon M + \|v_i * \phi_\varepsilon - v_j * \phi_\varepsilon\|_2, and the last term tends to 00. So (vj)(v_j) is Cauchy in L2L^2.

Step 1 is where the derivative bound is used: it says that, uniformly over the family, the functions are close to their own smoothed versions, so they can't oscillate on scales below ε\varepsilon. That is exactly the oscillation escape of 2B.3 Compactness being ruled out by a derivative bound. Escape to infinity is ruled out by the bounded domain. And concentration is ruled out by working below the critical exponent: Exercise 10.8 shows each of the three hypotheses is needed.

Now the deferred proofs can be completed. The solution operator GG of the Dirichlet problem maps L2L^2 boundedly into H01H^1_0, which embeds compactly in L2L^2; so GG is compact, and the spectral theorem of 4A.7 Compact Operators and Spectra gives the Dirichlet eigenfunctions. The mean-zero Poincaré inequality of 4A.9 Sobolev Spaces follows by the contradiction–compactness argument of its rehearsal. And on a closed manifold, Perelman's λ(g)\lambda(g) is attained.

Failure at the critical exponent

At q=p∗q = p^* the embedding W1,p↪Lp∗W^{1,p} \hookrightarrow L^{p^*} is continuous but never compact, even on a bounded domain. Fix u∈Cc∞(B1)u \in C_c^\infty(B_1) with u≠0u \neq 0, take p=2p = 2 and n≥3n \geq 3, and let

uk(x)=k(n−2)/2 u(kx).u_k(x) = k^{(n-2)/2}\,u(kx).

By the scaling rules of 3A.5 Product Measures and Change of Variables (Exercise 10.9), ∥∇uk∥2=∥∇u∥2\|\nabla u_k\|_2 = \|\nabla u\|_2 and ∥uk∥2∗=∥u∥2∗\|u_k\|_{2^*} = \|u\|_{2^*} for every kk: the critical norms don't notice the rescaling. The functions are supported in B1/kB_{1/k}, so uk→0u_k \to 0 almost everywhere and weakly in H01(B1)H^1_0(B_1) (4A.6 Weak Convergence and the Direct Method). If a subsequence converged in L2∗L^{2^*}, its limit would have to be 00, contradicting ∥uk∥2∗=∥u∥2∗≠0\|u_k\|_{2^*} = \|u\|_{2^*} \neq 0. The mass concentrates into a bubble at the origin: escape to vertical infinity (3A.3 The Lebesgue Integral), now in a form that is invisible to the critical norms.

Figure 10.2. Concentrating bubbles uk(x)=k(n−2)/2u(kx)u_k(x) = k^{(n-2)/2}u(kx) in dimension n=3n = 3 (radial profiles, computed for k=1,2,4,8k = 1, 2, 4, 8). The critical norms ∥∇uk∥2\|\nabla u_k\|_2 and ∥uk∥6\|u_k\|_6 are the same for every kk, yet uk→0u_k \to 0 at every point except the origin. No subsequence converges in L6L^6: compactness is lost by concentration.

The remedy is the one the template of 2B.3 Compactness always uses: normalise by rescaling. If a sequence concentrates at a point at scale 1k\frac1k, undo the concentration by vk(y)=k−(n−2)/2uk(y/k)v_k(y) = k^{-(n-2)/2}u_k(y/k); the rescaled sequence no longer concentrates, and a limit can be extracted from it. Pierre-Louis Lions's concentration–compactness principle (1984) makes this systematic: a bounded sequence in a critical space either converges, or loses mass in finitely many concentrating bubbles, each of which, rescaled, converges to a non-trivial limit, or escapes to infinity. Thierry Aubin and Richard Schoen used these ideas to solve the Yamabe problem (finding a conformal metric of constant scalar curvature), whose difficulty is exactly that it lives at the critical Sobolev exponent.

Where this goes Concentration, rescaling and the singularities of Ricci flow

The bubble picture is the template for singularity analysis. When a Ricci flow develops a singularity, curvature concentrates in small regions, as the bubbles concentrate ∣u∣2∗|u|^{2^*}. Hamilton's blow-up procedure (11B.4 Singularities) rescales the flow by the curvature at points of concentration, so that curvature becomes of size 11, and extracts a limit flow by his compactness theorem (11B.3 Compactness of Ricci Flows). As with bubbles, the rescaled limit is non-trivial and models the singularity; the work is in showing that nothing else can escape, and that is where Perelman's noncollapsing enters (12A.4 κ-Noncollapsing).

Sobolev inequalities themselves also reappear along the flow. Qi S. Zhang (2007) and Rugang Ye proved that a Sobolev inequality, with a scalar-curvature correction term, holds uniformly along Ricci flow on a closed manifold, as a consequence of Perelman's entropy monotonicity; and a uniform Sobolev inequality implies a lower bound on the volume of balls, a form of noncollapsing (Exercise 10.11). The logarithmic Sobolev inequality of 6A.10 Entropy, Information and Diffusion, which is what Perelman's W\mathcal{W}-entropy encodes, is a limiting, dimension-free relative of the Sobolev inequality (Beckner and Pearson made one precise version of this in 1998).

History

Sergei Sobolev proved his embedding theorem in 1938, by potential estimates. Emilio Gagliardo (1958) and Louis Nirenberg (1959) gave the elementary proof by integration along lines used above, which also handles p=1p = 1. Charles Morrey proved his Hölder estimate in 1938–40. Franz Rellich proved the compactness theorem in 1930 and Vladimir Kondrachov extended it in 1945. The equivalence with the isoperimetric inequality is due to Federer and Fleming and to Maz'ya, both in 1960; the sharp constants for p>1p > 1 were found by Thierry Aubin and Giorgio Talenti in 1976. Neil Trudinger's exponential integrability at p=np = n dates from 1967, Lions's concentration–compactness from 1984, and the solution of the Yamabe problem was completed by Schoen in 1984.

Recall Where we stand

Scaling forces the Sobolev exponent p∗=npn−pp^* = \frac{np}{n-p} and organises all embeddings on the line k−n/pk - n/p. Gagliardo–Nirenberg–Sobolev gives W1,p↪Lp∗W^{1,p} \hookrightarrow L^{p^*} for p<np < n; with p=1p = 1 it is equivalent to the isoperimetric inequality. Morrey gives Hölder continuity for p>np > n. On bounded domains and closed manifolds, Rellich–Kondrachov makes the embeddings into LqL^q, q<p∗q < p^*, compact, which completes the Dirichlet spectral theorem and the mean-zero Poincaré inequality. At the critical exponent compactness fails by concentrating bubbles, and rescaling recovers a limit: the model for singularity analysis. 4A.11 Hölder Spaces measures smoothness by Hölder exponents, the spaces in which elliptic and parabolic regularity is sharp.

Exercises

Exercise 10.5 Exponents by scaling

Use scaling to find the only possible qq in each inequality on Rn\mathbb{R}^n: (a) ∥u∥q≤C∥∇2u∥2\|u\|_q \leq C\|\nabla^2u\|_2 (two derivatives); (b) ∥u∥∞≤C∥∇u∥pθ∥u∥q1−θ\|u\|_\infty \leq C\|\nabla u\|_p^\theta\|u\|_q^{1-\theta} for given p>np > n, qq and unknown θ\theta; (c) the Nash inequality ∥u∥22+4/n≤C∥∇u∥22∥u∥14/n\|u\|_2^{2 + 4/n} \leq C\|\nabla u\|_2^2\|u\|_1^{4/n}: check that both sides scale the same way.

Solution

(a) −nq=2−n2-\frac nq = 2 - \frac n2, so q=2nn−4q = \frac{2n}{n-4} for n>4n > 4. (b) 0=θ(1−np)+(1−θ)(−nq)0 = \theta(1 - \frac np) + (1 - \theta)(-\frac nq), so θ=n/q1−n/p+n/q\theta = \frac{n/q}{1 - n/p + n/q}. (c) Under u(λx)u(\lambda x): left λ−n2(2+4n)=λ−n−2\lambda^{-\frac n2(2 + \frac4n)} = \lambda^{-n-2}; right λ2−nλ−n⋅4n=λ−n−2\lambda^{2-n}\lambda^{-n\cdot\frac4n} = \lambda^{-n-2}.

Exercise 10.6 From p=1p = 1 to general pp

Assuming ∥v∥n/(n−1)≤∥∇v∥1\|v\|_{n/(n-1)} \leq \|\nabla v\|_1, apply it to v=∣u∣γv = |u|^\gamma and use Hölder on ∫γ∣u∣γ−1∣∇u∣\int\gamma|u|^{\gamma-1}|\nabla u| to get ∥u∥p∗≤C∥∇u∥p\|u\|_{p^*} \leq C\|\nabla u\|_p, with γ=p(n−1)n−p\gamma = \frac{p(n-1)}{n-p}.

Exercise 10.7 Comparing shapes

For area 11, compare the perimeters of a disc, a square and an equilateral triangle, and check them against 2π2\sqrt\pi. For volume 11, compare the surface areas of a ball and a cube with (36π)1/3(36\pi)^{1/3}.

Solution

Disc 2π≈3.5452\sqrt\pi \approx 3.545; square 44; triangle ≈4.559\approx 4.559. Ball (36π)1/3≈4.836(36\pi)^{1/3} \approx 4.836; cube 66.

Exercise 10.8 Each hypothesis is needed

Show that the embedding H1↪L2H^1 \hookrightarrow L^2 is not compact (a) on Rn\mathbb{R}^n, using translates u(x−ke1)u(x - ke_1) of one bump; (b) for H1(Ω)H^1(\Omega) when Ω\Omega is a bounded domain with a sufficiently sharp outward cusp (state, don't prove); (c) into L2∗L^{2^*}, using the bubbles. In terms of 2B.3 Compactness's three escapes, which escape does each failure use?

Solution

(a) Escape to infinity: the translates are bounded in H1H^1, converge weakly to 00, and stay at L2L^2 distance 2∥u∥2\sqrt2\|u\|_2 apart. (b) Bad boundaries let functions concentrate at the cusp tip (a missing-point phenomenon); this is why some boundary regularity is assumed. (c) Concentration at a point.

Exercise 10.9 The bubble norms

For uk(x)=k(n−2)/2u(kx)u_k(x) = k^{(n-2)/2}u(kx) on Rn\mathbb{R}^n, verify ∥∇uk∥2=∥∇u∥2\|\nabla u_k\|_2 = \|\nabla u\|_2 and ∥uk∥2∗=∥u∥2∗\|u_k\|_{2^*} = \|u\|_{2^*} using 3A.5 Product Measures and Change of Variables's change of variables, and show ∥uk∥2=k−1∥u∥2→0\|u_k\|_2 = k^{-1}\|u\|_2 \to 0. So the bubbles converge to 00 in L2L^2 (as Rellich predicts) but not in L2∗L^{2^*}.

Exercise 10.10 Morrey's exponent

Check that ∣x∣α|x|^\alpha near 00 lies in W1,pW^{1,p} for p>np > n exactly when α>1−np\alpha > 1 - \frac np (4A.9 Sobolev Spaces), and is Hölder continuous with exponent α\alpha. Deduce that the Hölder exponent 1−np1 - \frac np in Morrey's inequality can't be improved.

Exercise 10.11 Rehearsal: a Sobolev inequality prevents collapsing

On a complete Riemannian manifold of dimension n≥3n \geq 3, suppose (∫∣u∣2∗)2/2∗≤A∫∣∇u∣2\big(\int|u|^{2^*}\big)^{2/2^*} \leq A\int|\nabla u|^2 for every Lipschitz uu with compact support in a ball B(x,r0)B(x, r_0). Let V(r)=vol B(x,r)V(r) = \mathrm{vol}\,B(x, r). Testing with u=(r−d(x,⋅))+u = (r - d(x, \cdot))_+ for r≤r0r \leq r_0 (so u≥r/2u \geq r/2 on B(x,r/2)B(x, r/2) and ∣∇u∣≤1|\nabla u| \leq 1), show

(r2)2V(r2)(n−2)/n≤A V(r).\Big(\frac r2\Big)^2V\Big(\frac r2\Big)^{(n-2)/n} \leq A\,V(r).

Iterating from small rr (where V(r)≈ωnrnV(r) \approx \omega_nr^n), deduce V(r)≥c(n,A) rnV(r) \geq c(n, A)\,r^n for r≤r0r \leq r_0. So a uniform Sobolev inequality implies that balls are κ-noncollapsed, with κ\kappa depending only on the Sobolev constant. In 12A.4 κ-Noncollapsing Perelman's μ\mu-functional plays the role of a logarithmic Sobolev constant, and the noncollapsing proof has this shape.

Solution

∥u∥2∗2≥((r2)2∗V(r2))2/2∗=(r2)2V(r2)(n−2)/n\|u\|_{2^*}^2 \geq \big((\frac r2)^{2^*}V(\frac r2)\big)^{2/2^*} = (\frac r2)^2V(\frac r2)^{(n-2)/n}, and ∫∣∇u∣2≤V(r)\int|\nabla u|^2 \leq V(r). Setting V(r)=arrnV(r) = a_r r^n, the inequality becomes ar≥c ar/2(n−2)/na_r \geq c\,a_{r/2}^{(n-2)/n} with c=14A⋅2−(n−2)c = \frac{1}{4A}\cdot2^{-(n-2)}; iterating, ar≥c1+θ+θ2+⋯ar/2mθma_r \geq c^{1 + \theta + \theta^2 + \cdots}a_{r/2^m}^{\theta^m} with θ=n−2n<1\theta = \frac{n-2}{n} < 1, and ar/2mθm→1a_{r/2^m}^{\theta^m} \to 1 because ar/2m→ωn>0a_{r/2^m} \to \omega_n > 0. So ar≥c1/(1−θ)=cn/2a_r \geq c^{1/(1-\theta)} = c^{n/2}, a positive constant depending only on nn and AA.

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