Book 6B

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Course 6Book 6B: Linear PDE: Characteristics, Waves and RegularityChapter 11

Linear Parabolic Equations in Full

Galerkin existence, energy estimates, regularity in space and time, and parabolic Harnack inequalities.

43 min read · Updated Oct 23, 2026

Read with Evans, Partial Differential Equations, section 5.9.2 (spaces involving time) and section 7.1 (second-order parabolic equations: weak solutions, existence, regularity, maximum principles); Jost, section 5.3 (the initial boundary value problem for the heat equation); Taylor I, §6.1 ("The heat equation and wave equation on bounded domains"). 6A.7 Parabolic Regularity proved Galerkin existence; this chapter proves the time-continuity theorem it used, the regularity theorems, a smoothing estimate, and the Aubin–Lions compactness lemma, and applies them to a nonlinear equation.

In this chapter · 7 sections
  1. 11.1Drug release from a polymer film
  2. 11.2Functions of time with values in a Banach space
  3. 11.3Improved regularity
  4. 11.4Instant smoothing for rough data
  5. 11.5Compactness in time: the Aubin–Lions lemma
  6. 11.6History
  7. 11.7Exercises
  8. ↗Free resources

6B.10 Harmonic Coordinates and the Regularity of Metrics ended with the Ricci–DeTurck flow, a parabolic system with diagonal principal part, and with the remark that its theory is the theory of linear parabolic equations applied component by component. 6A.7 Parabolic Regularity built weak solutions of parabolic equations by Galerkin's method and stated, without proof, two facts it needed: that such a solution is continuous in time with values in L2L^2, and that its L2L^2 norm is differentiable with the obvious formula. It also stated that solutions are as smooth as the data allow. This chapter proves these facts and develops the rest of the Hilbert-space theory of linear parabolic equations, Evans's section 7.1 in full: improved regularity by testing with the time derivative, higher regularity by differentiating in time, instant smoothing by weighted energies, and finally the compactness lemma of Aubin and Lions, which is what makes the Galerkin method work for nonlinear equations.

Two points of view run side by side. The energy method works with integrals: test the equation with the solution, or its derivative, or a weighted version, integrate by parts, and use Gronwall's inequality. The spectral method expands in eigenfunctions, which gives explicit formulas when the operator does not depend on time. The energy method is more general and is the one that extends to nonlinear and geometric problems; the spectral method is the one to compute with. The chapter's anchor, drug release from a polymer film, uses both.

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

  • work with Banach-space-valued functions of time, and prove that u∈L2(0,T;H01)u \in L^2(0, T; H^1_0) with u′∈L2(0,T;H−1)u' \in L^2(0, T; H^{-1}) is continuous into L2L^2 with ddt∥u∥2=2⟨u′,u⟩\frac{d}{dt}\|u\|^2 = 2\langle u', u\rangle;
  • prove improved regularity, u∈L2(0,T;H2)∩L∞(0,T;H01)u \in L^2(0, T; H^2)\cap L^\infty(0, T; H^1_0) with u′∈L2(0,T;L2)u' \in L^2(0, T; L^2), for H01H^1_0 data;
  • prove instant smoothing for L2L^2 data by weighted energy estimates, and explain the compatibility conditions needed for smoothness up to t=0t = 0;
  • prove Ehrling's lemma and the Aubin–Lions compactness lemma, and use them to solve a semilinear equation by Galerkin's method;
  • compute short-time and long-time behaviour of diffusion out of a slab, and explain the t\sqrt t law.

Drug release from a polymer film

In the world In use The square-root-of-time law

Many controlled-release medicines, skin patches and drug-eluting coatings on stents work by diffusion: the drug is dissolved in a polymer film and diffuses out through its surface. In the simplest model, a film of thickness LL holds a uniform initial concentration, the drug diffuses with coefficient DD, and both faces are perfect sinks. The concentration solves the heat equation on (0,L)(0, L) with zero boundary values, and separation of variables (6B.4 Green’s Functions, Separation of Variables and Transforms) gives the fraction released by time tt exactly:

MtM∞=1−8π2∑k odd1k2e−k2π2Dt/L2\frac{M_t}{M_\infty} = 1 - \frac{8}{\pi^2}\sum_{k\text{ odd}}\frac{1}{k^2}e^{-k^2\pi^2Dt/L^2}

(Exercise 11.8). Two regimes appear. At early times each face behaves like the face of a half-space, where the concentration profile is the self-similar error function of 6A.1 What a PDE Is, and the released fraction grows like

MtM∞≈4DtπL2:\frac{M_t}{M_\infty} \approx 4\sqrt{\frac{Dt}{\pi L^2}}:

the square-root-of-time law. At late times only the slowest eigenmode survives, and the remaining fraction decays like 8π2e−π2Dt/L2\frac{8}{\pi^2}e^{-\pi^2Dt/L^2}, exponentially at the rate of the first Dirichlet eigenvalue (6A.3 The Heat Equation on ℝⁿ's energy decay). Pharmaceutical scientists plot release against t\sqrt t to test whether it is diffusion-controlled; Takeru Higuchi's 1961 analysis of drug release from ointments, which gives a t\sqrt t law for a related moving-front problem, is one of the most cited papers in the field. Real formulations swell, erode and have drug loads above solubility, so the simple model is a reference case, not a description of every product.

Functions of time with values in a Banach space

A solution of a parabolic equation is, at each time, a function of space: t↦u(t)∈Xt \mapsto u(t) \in X, where XX is a space such as L2(U)L^2(U) or H01(U)H^1_0(U). For a Banach space XX, Lp(0,T;X)L^p(0, T; X) is the space of (strongly measurable) functions u:[0,T]→Xu : [0, T] \to X with

∥u∥Lp(0,T;X)=(∫0T∥u(t)∥Xp dt)1/p<∞,\|u\|_{L^p(0,T;X)} = \Big(\int_0^T\|u(t)\|_X^p\,dt\Big)^{1/p} < \infty,

with the usual modification for p=∞p = \infty; C([0,T];X)C([0, T]; X) is the space of continuous uu with the sup norm. Integrals of XX-valued functions are Bochner integrals, defined as limits of integrals of simple functions exactly as in 3A.3 The Lebesgue Integral; they satisfy ∥∫u∥≤∫∥u∥\|\int u\| \leq \int\|u\| and commute with bounded linear maps (Evans, appendix E.5). A function v∈L1(0,T;X)v \in L^1(0, T; X) is the weak derivative u′u' of u∈L1(0,T;X)u \in L^1(0, T; X) if ∫0Tϕ′(t)u(t) dt=−∫0Tϕ(t)v(t) dt\int_0^T\phi'(t)u(t)\,dt = -\int_0^T\phi(t)v(t)\,dt for every scalar test function ϕ∈Cc∞(0,T)\phi \in C_c^\infty(0, T), the definition of 4A.9 Distributions and Weak Derivatives with vector values.

Let UU be bounded, H01=H01(U)H^1_0 = H^1_0(U), L2=L2(U)L^2 = L^2(U) and H−1H^{-1} the dual of H01H^1_0, with the pairing ⟨⋅,⋅⟩\langle\cdot, \cdot\rangle; via f↦(v↦∫fv)f \mapsto (v \mapsto \int fv), L2⊂H−1L^2 \subset H^{-1}, and

H01⊂L2⊂H−1,H^1_0 \subset L^2 \subset H^{-1},

each inclusion continuous with dense image. A weak solution of a parabolic equation lies in L2(0,T;H01)L^2(0, T; H^1_0) with u′∈L2(0,T;H−1)u' \in L^2(0, T; H^{-1}) (6A.7 Parabolic Regularity). The next theorem says such a function is better than it looks.

Theorem 11.1 Continuity in time

Let u∈L2(0,T;H01)u \in L^2(0, T; H^1_0) with u′∈L2(0,T;H−1)u' \in L^2(0, T; H^{-1}). Then, after modification on a set of times of measure zero, u∈C([0,T];L2)u \in C([0, T]; L^2), the function t↦∥u(t)∥L22t \mapsto \|u(t)\|_{L^2}^2 is absolutely continuous with

ddt∥u(t)∥L22=2⟨u′(t),u(t)⟩for almost every t,\frac{d}{dt}\|u(t)\|_{L^2}^2 = 2\langle u'(t), u(t)\rangle \quad\text{for almost every } t,

and max⁡0≤t≤T∥u(t)∥L2≤C(∥u∥L2(0,T;H01)+∥u′∥L2(0,T;H−1))\max_{0\leq t\leq T}\|u(t)\|_{L^2} \leq C\big(\|u\|_{L^2(0,T;H^1_0)} + \|u'\|_{L^2(0,T;H^{-1})}\big), with CC depending only on TT.

Proof. Smoothing in time. Extend uu to a slightly larger interval (−σ,T+σ)(-\sigma, T + \sigma) by reflection, u(−t)=u(t)u(-t) = u(t) and u(T+t)=u(T−t)u(T + t) = u(T - t); the extension still has its weak derivative in L2(H−1)L^2(H^{-1}) (reflection reverses the sign of the derivative and creates no jump). Let ηε\eta_\varepsilon be a mollifier in tt and uε=ηε∗uu_\varepsilon = \eta_\varepsilon * u for t∈[0,T]t \in [0, T], ε<σ\varepsilon < \sigma. Then uεu_\varepsilon is smooth in tt with values in H01H^1_0, uε→uu_\varepsilon \to u in L2(0,T;H01)L^2(0, T; H^1_0) and uε′=ηε∗u′→u′u_\varepsilon' = \eta_\varepsilon * u' \to u' in L2(0,T;H−1)L^2(0, T; H^{-1}) (mollification converges in LpL^p of vector-valued functions as for scalar ones, 3A.8 Convolution and Mollifiers).

The identity for smooth functions. For uεu_\varepsilon, ddt∥uε(t)∥2=2(uε′,uε)=2⟨uε′,uε⟩\frac{d}{dt}\|u_\varepsilon(t)\|^2 = 2(u_\varepsilon', u_\varepsilon) = 2\langle u_\varepsilon', u_\varepsilon\rangle classically, since uε′∈H01⊂L2u_\varepsilon' \in H^1_0 \subset L^2. Integrating between ss and tt,

∥uε(t)∥2=∥uε(s)∥2+2∫st⟨uε′,uε⟩ dτ.\|u_\varepsilon(t)\|^2 = \|u_\varepsilon(s)\|^2 + 2\int_s^t\langle u_\varepsilon', u_\varepsilon\rangle\,d\tau.

Uniform convergence. Apply this to uε−uδu_\varepsilon - u_\delta in place of uεu_\varepsilon:

∥uε(t)−uδ(t)∥2=∥uε(s)−uδ(s)∥2+2∫st⟨uε′−uδ′,uε−uδ⟩ dτ.\|u_\varepsilon(t) - u_\delta(t)\|^2 = \|u_\varepsilon(s) - u_\delta(s)\|^2 + 2\int_s^t\langle u_\varepsilon' - u_\delta', u_\varepsilon - u_\delta\rangle\,d\tau.

The integral is at most 2∥uε′−uδ′∥L2(H−1)∥uε−uδ∥L2(H01)→02\|u_\varepsilon' - u_\delta'\|_{L^2(H^{-1})}\|u_\varepsilon - u_\delta\|_{L^2(H^1_0)} \to 0. Since uε→uu_\varepsilon \to u in L2(0,T;L2)L^2(0, T; L^2), for almost every ss we have uε(s)→u(s)u_\varepsilon(s) \to u(s) in L2L^2 along a subsequence; fix such an ss. Then the right side tends to 00 uniformly in tt, so (uε)(u_\varepsilon) is Cauchy in C([0,T];L2)C([0, T]; L^2), and its limit, a continuous function, agrees with uu for almost every tt. That is the modification.

The identity in the limit. Pass to the limit in the integrated identity for uεu_\varepsilon: ∥u(t)∥2=∥u(s)∥2+2∫st⟨u′,u⟩ dτ\|u(t)\|^2 = \|u(s)\|^2 + 2\int_s^t\langle u', u\rangle\,d\tau for all s,ts, t. An integral of an L1L^1 function is absolutely continuous, with derivative equal to the integrand almost everywhere (3A.6 Modes of Convergence and Differentiation).

The bound. Choose ss with ∥u(s)∥2≤1T∫0T∥u∥2≤CT∥u∥L2(H01)2\|u(s)\|^2 \leq \frac1T\int_0^T\|u\|^2 \leq \frac CT\|u\|_{L^2(H^1_0)}^2 (some time is at most the average). Then for every tt, ∥u(t)∥2≤∥u(s)∥2+2∥u′∥L2(H−1)∥u∥L2(H01)\|u(t)\|^2 \leq \|u(s)\|^2 + 2\|u'\|_{L^2(H^{-1})}\|u\|_{L^2(H^1_0)}, which gives the estimate.

The theorem is the rigorous form of "multiply by uu and integrate", the first move of every energy estimate, for functions that are not smooth. Its key structural point is the Gelfand triple H01⊂L2⊂H−1H^1_0 \subset L^2 \subset H^{-1}: the time derivative lives in a big space, the solution in a small one, and their pairing makes sense in the middle.

Improved regularity

For the rest of the chapter, let

Lu=−∑i,j∂j(aij(x)∂iu)+c(x)uLu = -\sum_{i,j}\partial_j\big(a^{ij}(x)\partial_iu\big) + c(x)u

be symmetric and uniformly elliptic with smooth coefficients independent of tt, c≥0c \geq 0, and B[u,v]B[u, v] its bilinear form, so that B[u,u]≥θ∥u∥H012B[u, u] \geq \theta\|u\|_{H^1_0}^2 (6A.6 Weak Solutions and Elliptic Regularity). The problem is

ut+Lu=f  in U×(0,T],u=0  on ∂U×[0,T],u=g  at t=0,u_t + Lu = f \ \text{ in } U\times(0, T], \qquad u = 0 \ \text{ on } \partial U\times[0, T], \qquad u = g \ \text{ at } t = 0,

with ∂U\partial U smooth. 6A.7 Parabolic Regularity constructed the weak solution as a limit of Galerkin approximations umu_m in the span of the first mm eigenfunctions w1,…,wmw_1, \ldots, w_m of LL (for a symmetric LL we may use its own eigenfunctions, orthonormal in L2L^2 and orthogonal for BB).

Theorem 11.2 Improved regularity

If g∈H01(U)g \in H^1_0(U) and f∈L2(0,T;L2(U))f \in L^2(0, T; L^2(U)), then the weak solution satisfies u∈L2(0,T;H2(U))∩L∞(0,T;H01(U))u \in L^2(0, T; H^2(U))\cap L^\infty(0, T; H^1_0(U)) and u′∈L2(0,T;L2(U))u' \in L^2(0, T; L^2(U)), with

sup⁡0≤t≤T∥u(t)∥H01+∥u∥L2(0,T;H2)+∥u′∥L2(0,T;L2)≤C(∥g∥H01+∥f∥L2(0,T;L2)).\sup_{0\leq t\leq T}\|u(t)\|_{H^1_0} + \|u\|_{L^2(0,T;H^2)} + \|u'\|_{L^2(0,T;L^2)} \leq C\big(\|g\|_{H^1_0} + \|f\|_{L^2(0,T;L^2)}\big).

Proof. Test with the time derivative. For the Galerkin approximation, multiply the kk-th equation (um′,wk)+B[um,wk]=(f,wk)(u_m', w_k) + B[u_m, w_k] = (f, w_k) by dmk ′(t)d_m^k\,'(t) and sum over kk:

∥um′∥L22+B[um,um′]=(f,um′).\|u_m'\|_{L^2}^2 + B[u_m, u_m'] = (f, u_m').

Since BB is symmetric and does not depend on tt, B[um,um′]=12ddtB[um,um]B[u_m, u_m'] = \frac12\frac{d}{dt}B[u_m, u_m]. By Cauchy's inequality (f,um′)≤12∥f∥2+12∥um′∥2(f, u_m') \leq \frac12\|f\|^2 + \frac12\|u_m'\|^2. So

∥um′∥2+ddtB[um,um]≤∥f∥2.\|u_m'\|^2 + \frac{d}{dt}B[u_m, u_m] \leq \|f\|^2.

Integrate from 00 to tt: ∫0t∥um′∥2+B[um(t),um(t)]≤B[um(0),um(0)]+∫0T∥f∥2\int_0^t\|u_m'\|^2 + B[u_m(t), u_m(t)] \leq B[u_m(0), u_m(0)] + \int_0^T\|f\|^2. Now um(0)u_m(0) is the projection of gg onto the span of w1,…,wmw_1, \ldots, w_m, and since the wkw_k are BB-orthogonal, B[um(0),um(0)]≤B[g,g]≤C∥g∥H012B[u_m(0), u_m(0)] \leq B[g, g] \leq C\|g\|_{H^1_0}^2. With B[u,u]≥θ∥u∥H012B[u, u] \geq \theta\|u\|_{H^1_0}^2,

sup⁡t∥um(t)∥H012+∫0T∥um′∥2dt≤C(∥g∥H012+∥f∥L2(L2)2).\sup_t\|u_m(t)\|_{H^1_0}^2 + \int_0^T\|u_m'\|^2dt \leq C\big(\|g\|_{H^1_0}^2 + \|f\|_{L^2(L^2)}^2\big).

These bounds pass to the weak limit (4A.7 Weak Convergence and the Direct Method, lower semicontinuity of norms), giving the L∞(H01)L^\infty(H^1_0) and L2(L2)L^2(L^2) bounds for uu and u′u'.

Elliptic regularity at each time. For almost every tt, the weak formulation says B[u(t),v]=(f(t)−u′(t),v)B[u(t), v] = (f(t) - u'(t), v) for all v∈H01v \in H^1_0: u(t)u(t) is the weak solution of the elliptic problem Lu(t)=f(t)−u′(t)Lu(t) = f(t) - u'(t), with right side in L2L^2. Global H2H^2 regularity for elliptic equations on smooth domains (6A.6 Weak Solutions and Elliptic Regularity) gives ∥u(t)∥H2≤C(∥f(t)∥L2+∥u′(t)∥L2+∥u(t)∥L2)\|u(t)\|_{H^2} \leq C\big(\|f(t)\|_{L^2} + \|u'(t)\|_{L^2} + \|u(t)\|_{L^2}\big). Square and integrate in tt.

The idea is the parabolic counterpart of the elliptic bootstrap: one more time derivative tested gives one more space derivative, through the elliptic equation Lu=f−u′Lu = f - u' at each time. Repeating, with time derivatives of the equation:

Theorem 11.3 Higher regularity (statement)

If g∈H2m+1(U)g \in H^{2m+1}(U), dkfdtk∈L2(0,T;H2m−2k(U))\frac{d^kf}{dt^k} \in L^2(0, T; H^{2m-2k}(U)) for k=0,…,mk = 0, \ldots, m, and the compatibility conditions of order mm hold, then dkudtk∈L2(0,T;H2m+2−2k)\frac{d^ku}{dt^k} \in L^2(0, T; H^{2m+2-2k}) for k=0,…,m+1k = 0, \ldots, m + 1, with estimates. If gg and ff are smooth and the compatibility conditions of all orders hold, then u∈C∞(U‾×[0,T])u \in C^\infty(\overline U\times[0, T]) (Evans, section 7.1.3, Theorems 6 and 7).

The compatibility conditions say that the time derivatives of uu at t=0t = 0, which the equation computes from the data (g0=gg_0 = g, g1=f(0)−Lg0g_1 = f(0) - Lg_0, g2=f′(0)−Lg1g_2 = f'(0) - Lg_1, and so on), must vanish on ∂U\partial U, because u=0u = 0 there for all time. For the heat equation with f=0f = 0, the first condition is g=0g = 0 on ∂U\partial U, the next is Δg=0\Delta g = 0 on ∂U\partial U, and so on. If they fail, the solution is still smooth for t>0t > 0 but not up to the corner ∂U×{0}\partial U\times\{0\}: for the drug-release problem, where the initial concentration is 11 but the boundary value is 00, the solution has a singularity at the corners at t=0t = 0, which is exactly what produces the t\sqrt t law.

Instant smoothing for rough data

Away from t=0t = 0, no compatibility is needed: parabolic equations smooth rough data instantly. The weighted energy method proves it with nothing but the equation, in the spirit of Bernstein's estimate (6A.7 Parabolic Regularity), but with integrals instead of maxima.

Proposition 11.4 Weighted energy estimates

Let f=0f = 0 and g∈L2(U)g \in L^2(U). Then for 0<t≤T0 < t \leq T,

∥u(t)∥L22+2∫0tB[u,u] ds=∥g∥L22,t B[u(t),u(t)]≤12∥g∥L22,t2∥u′(t)∥L22≤C∥g∥L22.\|u(t)\|_{L^2}^2 + 2\int_0^tB[u, u]\,ds = \|g\|_{L^2}^2, \qquad t\,B[u(t), u(t)] \leq \frac12\|g\|_{L^2}^2, \qquad t^2\|u'(t)\|_{L^2}^2 \leq C\|g\|_{L^2}^2.

In particular ∥u(t)∥H01≤Ct∥g∥L2\|u(t)\|_{H^1_0} \leq \frac{C}{\sqrt t}\|g\|_{L^2}.

Proof. We argue with Galerkin approximations (all identities below hold for them, and the inequalities pass to the limit). First: test with uu: 12ddt∥u∥2+B[u,u]=0\frac12\frac{d}{dt}\|u\|^2 + B[u, u] = 0; integrate. Second: test with u′u': ∥u′∥2+12ddtB[u,u]=0\|u'\|^2 + \frac12\frac{d}{dt}B[u, u] = 0, so B[u,u]B[u, u] is non-increasing; then

ddt(t B[u,u])=B[u,u]+tddtB[u,u]=B[u,u]−2t∥u′∥2≤B[u,u].\frac{d}{dt}\big(t\,B[u, u]\big) = B[u, u] + t\frac{d}{dt}B[u, u] = B[u, u] - 2t\|u'\|^2 \leq B[u, u].

Integrating from 00 and using the first identity, tB[u(t),u(t)]≤∫0tB[u,u]≤12∥g∥2tB[u(t), u(t)] \leq \int_0^tB[u, u] \leq \frac12\|g\|^2. Third: differentiate the equation in tt; v=u′v = u' solves the same equation, so ddt∥v∥2=−2B[v,v]≤0\frac{d}{dt}\|v\|^2 = -2B[v, v] \leq 0, and

ddt(t2∥v∥2)≤2t∥v∥2=2t∥u′∥2=B[u,u]−ddt(tB[u,u]),\frac{d}{dt}\big(t^2\|v\|^2\big) \leq 2t\|v\|^2 = 2t\|u'\|^2 = B[u, u] - \frac{d}{dt}\big(tB[u, u]\big),

the last equality from the second step. Integrating from 00 to tt, t2∥u′(t)∥2≤∫0tB[u,u] ds−tB[u(t),u(t)]≤12∥g∥2t^2\|u'(t)\|^2 \leq \int_0^tB[u, u]\,ds - tB[u(t), u(t)] \leq \frac12\|g\|^2.

Each step is the previous one applied to a time derivative, with one more power of tt as a weight: tkB[∂tk−1u,∂tk−1u]t^kB[\partial_t^{k-1}u, \partial_t^{k-1}u] and tk+1∥∂tku∥2t^{k+1}\|\partial_t^ku\|^2 are bounded by Ck∥g∥2C_k\|g\|^2. Combined with elliptic regularity at each time (L∂tku=−∂tk+1uL\partial_t^ku = -\partial_t^{k+1}u), this gives u(t)∈H2k(U)u(t) \in H^{2k}(U) for every kk and every t>0t > 0, with ∥u(t)∥H2k≤Ckt−k∥g∥L2\|u(t)\|_{H^{2k}} \leq C_kt^{-k}\|g\|_{L^2}: the solution is C∞C^\infty in xx for t>0t > 0, with the rate t−1/2t^{-1/2} per derivative that parabolic scaling demands (6A.3 The Heat Equation on ℝⁿ). For the time derivatives the same holds, so u∈C∞(U‾×(0,T])u \in C^\infty(\overline U\times(0, T]).

Maximum principles and Harnack. The pointwise theory of 6A.5 Maximum Principles applies to classical solutions of ut+Lu=0u_t + Lu = 0 with smooth coefficients, and by the regularity just proved, to every weak solution at positive times: the weak and strong maximum principles hold, and a non-negative solution is either identically zero or positive everywhere at later times. For smooth coefficients, Evans (section 7.1.4) proves the parabolic Harnack inequality by a Li–Yau type estimate for log⁡u\log u; for measurable coefficients it is Moser's theorem (6B.9 De Giorgi–Nash–Moser).

Compactness in time: the Aubin–Lions lemma

Galerkin's method for a linear equation needs only weak convergence: the equation is linear in uu, so weak limits of approximate solutions are solutions. For a nonlinear term, such as f(u)f(u), weak convergence is not enough: if um⇀uu_m \rightharpoonup u weakly, f(um)f(u_m) need not converge to f(u)f(u) (4A.7 Weak Convergence and the Direct Method, the oscillation examples). One needs strong convergence in some norm, and in space-time the source of strong convergence is a compactness lemma that combines a bound on spatial regularity with a bound on the time derivative. It starts from an inequality between three spaces.

Lemma 11.5 Ehrling's lemma

Let X0⊂X⊂X1X_0 \subset X \subset X_1 be Banach spaces, with the inclusion X0↪XX_0 \hookrightarrow X compact and X↪X1X \hookrightarrow X_1 continuous and injective. Then for every ε>0\varepsilon > 0 there is CεC_\varepsilon with

∥v∥X≤ε∥v∥X0+Cε∥v∥X1for all v∈X0.\|v\|_X \leq \varepsilon\|v\|_{X_0} + C_\varepsilon\|v\|_{X_1} \qquad\text{for all } v \in X_0.

Proof. Contradiction–compactness (2B.3 Compactness). If not, for some ε\varepsilon there are vk∈X0v_k \in X_0 with ∥vk∥X>ε∥vk∥X0+k∥vk∥X1\|v_k\|_X > \varepsilon\|v_k\|_{X_0} + k\|v_k\|_{X_1}; normalise so that ∥vk∥X0=1\|v_k\|_{X_0} = 1. Then ∥vk∥X>ε\|v_k\|_X > \varepsilon, and ∥vk∥X1<1k∥vk∥X≤Ck→0\|v_k\|_{X_1} < \frac1k\|v_k\|_X \leq \frac Ck \to 0. By compactness a subsequence converges in XX to some vv, with ∥v∥X≥ε\|v\|_X \geq \varepsilon. Since X↪X1X \hookrightarrow X_1 is continuous, vk→vv_k \to v in X1X_1 too, so ∥v∥X1=0\|v\|_{X_1} = 0, and by injectivity v=0v = 0: a contradiction.

We use it with X0=H01X_0 = H^1_0, X=L2X = L^2, X1=H−1X_1 = H^{-1}. The inclusion H01↪L2H^1_0 \hookrightarrow L^2 is compact by Rellich (4A.11 Sobolev Embeddings and Critical Exponents), and the inclusion L2↪H−1L^2 \hookrightarrow H^{-1} is also compact: it is the adjoint of the first, and adjoints of compact operators on Hilbert spaces are compact (4A.8 Compact Operators and Spectra).

Theorem 11.6 The Aubin–Lions lemma

Let (um)(u_m) be bounded in L2(0,T;H01)L^2(0, T; H^1_0), with (um′)(u_m') bounded in L2(0,T;H−1)L^2(0, T; H^{-1}). Then a subsequence converges strongly in L2(0,T;L2)L^2(0, T; L^2).

Proof. Step 1: compactness in C([0,T];H−1)C([0, T]; H^{-1}). By Theorem 11.1, the umu_m are continuous into L2L^2 and sup⁡t∥um(t)∥L2≤M\sup_t\|u_m(t)\|_{L^2} \leq M uniformly in mm. So for each tt the set {um(t)}\{u_m(t)\} is bounded in L2L^2, hence precompact in H−1H^{-1}. And the umu_m are equicontinuous into H−1H^{-1}:

∥um(t)−um(s)∥H−1=∥∫stum′∥H−1≤∣t−s∣1/2∥um′∥L2(H−1)≤M′∣t−s∣1/2.\|u_m(t) - u_m(s)\|_{H^{-1}} = \Big\|\int_s^tu_m'\Big\|_{H^{-1}} \leq |t - s|^{1/2}\|u_m'\|_{L^2(H^{-1})} \leq M'|t - s|^{1/2}.

By the Arzelà–Ascoli theorem for functions with values in a metric space (2B.5 Uniform Convergence and Arzelà–Ascoli; the proof is the same diagonal argument over a countable dense set of times), a subsequence converges in C([0,T];H−1)C([0, T]; H^{-1}), hence in L2(0,T;H−1)L^2(0, T; H^{-1}).

Step 2: upgrading to L2(L2)L^2(L^2). By Ehrling's lemma at each time, squared and integrated,

∥um−uk∥L2(0,T;L2)≤ε∥um−uk∥L2(0,T;H01)+Cε∥um−uk∥L2(0,T;H−1)≤2Bε+Cε∥um−uk∥L2(0,T;H−1),\|u_m - u_k\|_{L^2(0,T;L^2)} \leq \varepsilon\|u_m - u_k\|_{L^2(0,T;H^1_0)} + C_\varepsilon\|u_m - u_k\|_{L^2(0,T;H^{-1})} \leq 2B\varepsilon + C_\varepsilon\|u_m - u_k\|_{L^2(0,T;H^{-1})},

where BB bounds the L2(H01)L^2(H^1_0) norms. For the subsequence of Step 1 the last term tends to 00, so lim sup⁡m,k∥um−uk∥L2(L2)≤2Bε\limsup_{m,k}\|u_m - u_k\|_{L^2(L^2)} \leq 2B\varepsilon for every ε\varepsilon: the subsequence is Cauchy in L2(0,T;L2)L^2(0, T; L^2).

The lemma's message: spatial compactness (a bound in a compactly embedded space) plus control of time oscillation (a bound on the time derivative, even in a weak norm) gives compactness in space-time. Neither alone suffices: functions bounded in L2(H01)L^2(H^1_0) can oscillate wildly in time, like sin⁡(mt)ϕ(x)\sin(mt)\phi(x), and functions with bounded time derivatives can oscillate in space.

Example 11.7 A semilinear equation by Galerkin and compactness

Let F:R→RF : \mathbb{R}\to\mathbb{R} be Lipschitz with constant KK, and consider ut−Δu=F(u)u_t - \Delta u = F(u) on U×(0,T]U\times(0, T], u=0u = 0 on ∂U\partial U, u(0)=g∈L2u(0) = g \in L^2. The Galerkin approximations umu_m satisfy (um′,wk)+(∇um,∇wk)=(F(um),wk)(u_m', w_k) + (\nabla u_m, \nabla w_k) = (F(u_m), w_k) for k≤mk \leq m, a system of ODEs with Lipschitz right side, solvable for all time. Testing with umu_m, and using ∣F(s)∣≤∣F(0)∣+K∣s∣|F(s)| \leq |F(0)| + K|s|,

12ddt∥um∥2+∥∇um∥2≤∥F(um)∥∥um∥≤C(1+∥um∥2),\frac12\frac{d}{dt}\|u_m\|^2 + \|\nabla u_m\|^2 \leq \|F(u_m)\|\|u_m\| \leq C(1 + \|u_m\|^2),

so by Gronwall umu_m is bounded in L∞(L2)∩L2(H01)L^\infty(L^2)\cap L^2(H^1_0), and as in 6A.7 Parabolic Regularity um′u_m' is bounded in L2(H−1)L^2(H^{-1}). By Aubin–Lions a subsequence converges strongly in L2(L2)L^2(L^2) to some uu (and weakly in L2(H01)L^2(H^1_0), with um′⇀u′u_m' \rightharpoonup u'). Strong convergence handles the nonlinearity: ∥F(um)−F(u)∥L2(L2)≤K∥um−u∥L2(L2)→0\|F(u_m) - F(u)\|_{L^2(L^2)} \leq K\|u_m - u\|_{L^2(L^2)} \to 0. So uu is a weak solution. Uniqueness follows by testing the difference ww of two solutions with ww: 12ddt∥w∥2≤K∥w∥2\frac12\frac{d}{dt}\|w\|^2 \leq K\|w\|^2, and Gronwall. The same scheme, with more work in the estimates, proves existence of weak solutions of the Navier–Stokes equations in three dimensions (Leray 1934, Hopf 1951), where uniqueness remains famously open.

Where this goes Energy methods on manifolds and along flows

Everything here works on a closed Riemannian manifold, with H01H^1_0 replaced by H1(M)H^1(M) and no boundary conditions (9B.7 The Heat Equation on a Manifold); the eigenfunction expansion of the heat equation there is the spectral picture of 6B.15 Spectral Theory and Heat Trace Asymptotics. Along the Ricci flow the metric, and so the inner products, change in time, and energy identities pick up extra terms from ∂tg=−2Ric⁡\partial_tg = -2\operatorname{Ric}; Perelman's monotonicity formulas are energy identities of exactly this kind, for the conjugate heat equation coupled to the flow (12A.2 Ricci Flow as a Gradient Flow). The Aubin–Lions mechanism, spatial bounds plus time-derivative bounds, is how weak solutions of geometric flows (harmonic map flow in 6C.7 Harmonic Maps and Their Heat Flow, Ricci flow through singularities in 12C.9 After Perelman) are obtained as limits of approximations.

History

Jacques-Louis Lions developed the Hilbert-space theory of evolution equations, with Gelfand triples and Bochner spaces, in the 1950s and 1960s; his book with Enrico Magenes (1968–70) and his 1969 book on nonlinear problems systematised it, including the compactness lemma he proved with Jean-Pierre Aubin (Aubin's paper is from 1963). Gunnar Ehrling's lemma dates from 1954. Jean Leray constructed weak solutions of the Navier–Stokes equations in 1934 and Eberhard Hopf extended the construction to bounded domains in 1951. Takeru Higuchi's paper on drug release appeared in 1961; John Crank's The Mathematics of Diffusion (1956, second edition 1975) collected the solutions used in the release calculation.

Recall Where we stand

Functions of time with values in H01H^1_0 and derivatives in H−1H^{-1} are continuous into L2L^2, with ddt∥u∥2=2⟨u′,u⟩\frac{d}{dt}\|u\|^2 = 2\langle u', u\rangle: the rigorous energy identity, proved by mollifying in time. Testing with u′u' and using elliptic regularity at each time gives improved regularity for H01H^1_0 data; differentiating in time gives higher regularity, up to t=0t = 0 only under compatibility conditions. Weighted energies tkB[∂tk−1u,∂tk−1u]t^kB[\partial_t^{k-1}u, \partial_t^{k-1}u] prove instant smoothing with the parabolic rate t−1/2t^{-1/2} per derivative. Ehrling's lemma and the Aubin–Lions lemma turn spatial bounds plus time-derivative bounds into strong compactness in L2(L2)L^2(L^2), which lets Galerkin's method pass nonlinear terms to the limit. Diffusion out of a slab releases mass like t\sqrt t early and approaches equilibrium like e−λ1te^{-\lambda_1t} late. 6B.12 Unique Continuation and Backward Uniqueness proves that, for all their smoothing, parabolic equations never forget completely: solutions are determined by their values at one time, and elliptic solutions by their values on any open set.

Exercises

Exercise 11.8 The release curve

For ut=Duxxu_t = Du_{xx} on (0,L)(0, L) with u(0,t)=u(L,t)=0u(0, t) = u(L, t) = 0 and u(x,0)=1u(x, 0) = 1: (a) show u=∑k odd4kπsin⁡kπxLe−k2π2Dt/L2u = \sum_{k\text{ odd}}\frac{4}{k\pi}\sin\frac{k\pi x}{L}e^{-k^2\pi^2Dt/L^2}; (b) integrate to get the remaining mass and the formula for MtM∞\frac{M_t}{M_\infty} in the opening box, using ∑k odd1k2=π28\sum_{k\text{ odd}}\frac{1}{k^2} = \frac{\pi^2}{8}; (c) derive the early-time law from the half-space solution erfc⁡(x2Dt)\operatorname{erfc}\big(\frac{x}{2\sqrt{Dt}}\big): show that the flux out of one face is DπDt\frac{D}{\sqrt{\pi Dt}}, so the total released by both faces up to time tt is 4Dtπ4\sqrt{\frac{Dt}{\pi}}, and divide by M∞=LM_\infty = L.

Solution

(a) The sine coefficients of 11 on (0,L)(0, L) are 2L∫0Lsin⁡kπxLdx=2kπ(1−(−1)k)\frac2L\int_0^L\sin\frac{k\pi x}{L}dx = \frac{2}{k\pi}(1 - (-1)^k), which is 4kπ\frac{4}{k\pi} for odd kk. (b) ∫0Lsin⁡kπxLdx=2Lkπ\int_0^L\sin\frac{k\pi x}{L}dx = \frac{2L}{k\pi} for odd kk, so the remaining mass is 8Lπ2∑k odd1k2e−k2π2Dt/L2\frac{8L}{\pi^2}\sum_{k\text{ odd}}\frac{1}{k^2}e^{-k^2\pi^2Dt/L^2}, equal to LL at t=0t = 0. (c) Near a face, at early times, the concentration is approximately u=erf⁡(x2Dt)u = \operatorname{erf}\big(\frac{x}{2\sqrt{Dt}}\big) (00 at the face, 11 inside), so ux(0,t)=1πDtu_x(0, t) = \frac{1}{\sqrt{\pi Dt}}, so the flux out is Dux=DπDt=DπtDu_x = \frac{D}{\sqrt{\pi Dt}} = \sqrt{\frac{D}{\pi t}}, and ∫0tDπsds=2Dtπ\int_0^t\sqrt{\frac{D}{\pi s}}ds = 2\sqrt{\frac{Dt}{\pi}} per face.

Exercise 11.9 The energy identity for the heat equation

For the heat equation on (0,π)(0, \pi) with zero boundary values and g=∑bksin⁡kxg = \sum b_k\sin kx, compute ∥u(t)∥2\|u(t)\|^2 and 2∫0t∥∇u∥22\int_0^t\|\nabla u\|^2 from the series, and verify the first identity of Proposition 11.4.

Solution

∥u(t)∥2=π2∑bk2e−2k2t\|u(t)\|^2 = \frac\pi2\sum b_k^2e^{-2k^2t} and ∥∇u∥2=π2∑k2bk2e−2k2t\|\nabla u\|^2 = \frac\pi2\sum k^2b_k^2e^{-2k^2t}, so 2∫0t∥∇u∥2=π2∑bk2(1−e−2k2t)2\int_0^t\|\nabla u\|^2 = \frac\pi2\sum b_k^2(1 - e^{-2k^2t}). Adding gives π2∑bk2=∥g∥2\frac\pi2\sum b_k^2 = \|g\|^2.

Exercise 11.10 The rate is sharp

On (0,π)(0, \pi), take g=sin⁡Nxg = \sin Nx. Show that ∥u(t)∥H01=∥∇u(t)∥=π/2 Ne−N2t\|u(t)\|_{H^1_0} = \|\nabla u(t)\| = \sqrt{\pi/2}\,Ne^{-N^2t}, and that sup⁡Nt Ne−N2t\sup_N\sqrt t\,Ne^{-N^2t} is a constant independent of tt (find it). Conclude that the bound ∥u(t)∥H01≤Ct∥g∥\|u(t)\|_{H^1_0} \leq \frac{C}{\sqrt t}\|g\| cannot be improved in its dependence on tt.

Solution

u=e−N2tsin⁡Nxu = e^{-N^2t}\sin Nx, ∥∇u∥=Ne−N2tπ/2\|\nabla u\| = Ne^{-N^2t}\sqrt{\pi/2}, ∥g∥=π/2\|g\| = \sqrt{\pi/2}. With s=Nts = N\sqrt t, t Ne−N2t=se−s2\sqrt t\,Ne^{-N^2t} = se^{-s^2}, maximised at s=12s = \frac{1}{\sqrt2} with value 12e\frac{1}{\sqrt{2e}}. So for each tt some data (with N≈(2t)−1/2N \approx (2t)^{-1/2}) nearly attain 12et∥g∥\frac{1}{\sqrt{2et}}\|g\|.

Exercise 11.11 Compatibility conditions

For the heat equation on (0,1)(0, 1) with u=0u = 0 at both ends and u(x,0)=g(x)u(x, 0) = g(x), show that if uu is C2C^2 up to the corners, then g(0)=g(1)=0g(0) = g(1) = 0; and if uu is C4C^{4} in xx and C2C^2 in tt up to the corners, then also g′′(0)=g′′(1)=0g''(0) = g''(1) = 0. What happens to utu_t near (0,0)(0, 0) for g≡1g \equiv 1?

Solution

Continuity at the corner gives g(0)=u(0,0)=0g(0) = u(0, 0) = 0. If utu_t is continuous up to the corner, then ut(0,t)=0u_t(0, t) = 0 for t>0t > 0 (as u(0,t)=0u(0, t) = 0), so ut(0,0)=0u_t(0, 0) = 0; but ut=uxxu_t = u_{xx}, so g′′(0)=0g''(0) = 0. For g≡1g \equiv 1, near the corner u≈erf⁡(x2t)u \approx \operatorname{erf}\big(\frac{x}{2\sqrt t}\big), whose tt-derivative is −x2πt3/2e−x2/4t-\frac{x}{2\sqrt\pi t^{3/2}}e^{-x^2/4t}, unbounded near (0,0)(0, 0) (along x=tx = \sqrt t it is of size t−1t^{-1}).

Exercise 11.12 Why both bounds are needed

(a) Let um(x,t)=sin⁡(mt)ϕ(x)u_m(x, t) = \sin(mt)\phi(x) with a fixed ϕ∈H01\phi \in H^1_0. Show (um)(u_m) is bounded in L2(0,T;H01)L^2(0, T; H^1_0) but has no subsequence converging strongly in L2(L2)L^2(L^2). Which hypothesis of Aubin–Lions fails? (b) Let um(x,t)=sin⁡(mx)u_m(x, t) = \sin(mx) on (0,π)(0, \pi), independent of tt. Show um′=0u_m' = 0 but there is no strongly convergent subsequence in L2(L2)L^2(L^2). Which hypothesis fails?

Solution

(a) ∥um∥L2(H01)2=∥ϕ∥H012∫0Tsin⁡2(mt)dt≤T∥ϕ∥H012\|u_m\|_{L^2(H^1_0)}^2 = \|\phi\|_{H^1_0}^2\int_0^T\sin^2(mt)dt \leq T\|\phi\|^2_{H^1_0}. But sin⁡(mt)⇀0\sin(mt) \rightharpoonup 0 weakly in L2(0,T)L^2(0, T) while ∫sin⁡2(mt)→T2\int\sin^2(mt) \to \frac T2, so no subsequence converges strongly (the only possible limit is 00). The time derivative mcos⁡(mt)ϕm\cos(mt)\phi is unbounded. (b) ∥sin⁡mx∥H01=mπ/2\|\sin mx\|_{H^1_0} = m\sqrt{\pi/2} is unbounded; the spatial bound fails, and sin⁡mx⇀0\sin mx \rightharpoonup 0 without strong convergence.

Exercise 11.13 Rehearsal: an integral estimate for a tensor heat equation

On a closed manifold with a fixed metric, let a tensor TT satisfy ∂tT=ΔT+Q(T)\partial_tT = \Delta T + Q(T), where ∣Q(T)∣≤C∣T∣2|Q(T)| \leq C|T|^2 (a quadratic reaction term, as for the curvature under Ricci flow, 11A.2 How Curvature Evolves). (a) Show, by testing with TT and integrating by parts, that ddt∫∣T∣2=−2∫∣∇T∣2+2∫⟨Q(T),T⟩≤−2∫∣∇T∣2+2Csup⁡∣T∣∫∣T∣2\frac{d}{dt}\int|T|^2 = -2\int|\nabla T|^2 + 2\int\langle Q(T), T\rangle \leq -2\int|\nabla T|^2 + 2C\sup|T|\int|T|^2. (b) Deduce that as long as sup⁡∣T∣≤K\sup|T| \leq K, ∫∣T∣2\int|T|^2 grows at most like e2CKte^{2CKt}, and ∫0t∫∣∇T∣2\int_0^t\int|\nabla T|^2 is bounded. Integral estimates of this kind, combined with the Moser iteration of 6B.9 De Giorgi–Nash–Moser, are one way to control curvature along geometric flows; along the Ricci flow the volume form also changes, which adds a term −∫R∣T∣2-\int R|T|^2 to the derivative.

Solution

(a) ddt∫∣T∣2=2∫⟨ΔT+Q(T),T⟩\frac{d}{dt}\int|T|^2 = 2\int\langle\Delta T + Q(T), T\rangle and ∫⟨ΔT,T⟩=−∫∣∇T∣2\int\langle\Delta T, T\rangle = -\int|\nabla T|^2 on a closed manifold; ∣⟨Q(T),T⟩∣≤C∣T∣3≤Csup⁡∣T∣ ∣T∣2|\langle Q(T), T\rangle| \leq C|T|^3 \leq C\sup|T|\,|T|^2. (b) Dropping the gradient term, ddt∫∣T∣2≤2CK∫∣T∣2\frac{d}{dt}\int|T|^2 \leq 2CK\int|T|^2, so Gronwall gives the exponential bound. Integrating the full inequality over [0,t][0, t], 2∫0t∫∣∇T∣2≤∫∣T(0)∣2+2CK∫0t∫∣T∣22\int_0^t\int|\nabla T|^2 \leq \int|T(0)|^2 + 2CK\int_0^t\int|T|^2, which is bounded.

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