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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.
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.
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 , and that its 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 with is continuous into with ;
- prove improved regularity, with , for data;
- prove instant smoothing for data by weighted energy estimates, and explain the compatibility conditions needed for smoothness up to ;
- 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 law.
Drug release from a polymer film
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 holds a uniform initial concentration, the drug diffuses with coefficient , and both faces are perfect sinks. The concentration solves the heat equation on with zero boundary values, and separation of variables (6B.4 Green’s Functions, Separation of Variables and Transforms) gives the fraction released by time exactly:
(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
the square-root-of-time law. At late times only the slowest eigenmode survives, and the remaining fraction decays like , exponentially at the rate of the first Dirichlet eigenvalue (6A.3 The Heat Equation on ℝⁿ's energy decay). Pharmaceutical scientists plot release against to test whether it is diffusion-controlled; Takeru Higuchi's 1961 analysis of drug release from ointments, which gives a 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: , where is a space such as or . For a Banach space , is the space of (strongly measurable) functions with
with the usual modification for ; is the space of continuous with the sup norm. Integrals of -valued functions are Bochner integrals, defined as limits of integrals of simple functions exactly as in 3A.3 The Lebesgue Integral; they satisfy and commute with bounded linear maps (Evans, appendix E.5). A function is the weak derivative of if for every scalar test function , the definition of 4A.9 Distributions and Weak Derivatives with vector values.
Let be bounded, , and the dual of , with the pairing ; via , , and
each inclusion continuous with dense image. A weak solution of a parabolic equation lies in with (6A.7 Parabolic Regularity). The next theorem says such a function is better than it looks.
Let with . Then, after modification on a set of times of measure zero, , the function is absolutely continuous with
and , with depending only on .
Proof. Smoothing in time. Extend to a slightly larger interval by reflection, and ; the extension still has its weak derivative in (reflection reverses the sign of the derivative and creates no jump). Let be a mollifier in and for , . Then is smooth in with values in , in and in (mollification converges in of vector-valued functions as for scalar ones, 3A.8 Convolution and Mollifiers).
The identity for smooth functions. For , classically, since . Integrating between and ,
Uniform convergence. Apply this to in place of :
The integral is at most . Since in , for almost every we have in along a subsequence; fix such an . Then the right side tends to uniformly in , so is Cauchy in , and its limit, a continuous function, agrees with for almost every . That is the modification.
The identity in the limit. Pass to the limit in the integrated identity for : for all . An integral of an function is absolutely continuous, with derivative equal to the integrand almost everywhere (3A.6 Modes of Convergence and Differentiation).
The bound. Choose with (some time is at most the average). Then for every , , which gives the estimate.
The theorem is the rigorous form of "multiply by and integrate", the first move of every energy estimate, for functions that are not smooth. Its key structural point is the Gelfand triple : 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
be symmetric and uniformly elliptic with smooth coefficients independent of , , and its bilinear form, so that (6A.6 Weak Solutions and Elliptic Regularity). The problem is
with smooth. 6A.7 Parabolic Regularity constructed the weak solution as a limit of Galerkin approximations in the span of the first eigenfunctions of (for a symmetric we may use its own eigenfunctions, orthonormal in and orthogonal for ).
If and , then the weak solution satisfies and , with
Proof. Test with the time derivative. For the Galerkin approximation, multiply the -th equation by and sum over :
Since is symmetric and does not depend on , . By Cauchy's inequality . So
Integrate from to : . Now is the projection of onto the span of , and since the are -orthogonal, . With ,
These bounds pass to the weak limit (4A.7 Weak Convergence and the Direct Method, lower semicontinuity of norms), giving the and bounds for and .
Elliptic regularity at each time. For almost every , the weak formulation says for all : is the weak solution of the elliptic problem , with right side in . Global regularity for elliptic equations on smooth domains (6A.6 Weak Solutions and Elliptic Regularity) gives . Square and integrate in .
The idea is the parabolic counterpart of the elliptic bootstrap: one more time derivative tested gives one more space derivative, through the elliptic equation at each time. Repeating, with time derivatives of the equation:
If , for , and the compatibility conditions of order hold, then for , with estimates. If and are smooth and the compatibility conditions of all orders hold, then (Evans, section 7.1.3, Theorems 6 and 7).
The compatibility conditions say that the time derivatives of at , which the equation computes from the data (, , , and so on), must vanish on , because there for all time. For the heat equation with , the first condition is on , the next is on , and so on. If they fail, the solution is still smooth for but not up to the corner : for the drug-release problem, where the initial concentration is but the boundary value is , the solution has a singularity at the corners at , which is exactly what produces the law.
Instant smoothing for rough data
Away from , 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.
Let and . Then for ,
In particular .
Proof. We argue with Galerkin approximations (all identities below hold for them, and the inequalities pass to the limit). First: test with : ; integrate. Second: test with : , so is non-increasing; then
Integrating from and using the first identity, . Third: differentiate the equation in ; solves the same equation, so , and
the last equality from the second step. Integrating from to , .
Each step is the previous one applied to a time derivative, with one more power of as a weight: and are bounded by . Combined with elliptic regularity at each time (), this gives for every and every , with : the solution is in for , with the rate per derivative that parabolic scaling demands (6A.3 The Heat Equation on ℝⁿ). For the time derivatives the same holds, so .
Maximum principles and Harnack. The pointwise theory of 6A.5 Maximum Principles applies to classical solutions of 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 ; 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 , so weak limits of approximate solutions are solutions. For a nonlinear term, such as , weak convergence is not enough: if weakly, need not converge to (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.
Let be Banach spaces, with the inclusion compact and continuous and injective. Then for every there is with
Proof. Contradiction–compactness (2B.3 Compactness). If not, for some there are with ; normalise so that . Then , and . By compactness a subsequence converges in to some , with . Since is continuous, in too, so , and by injectivity : a contradiction.
We use it with , , . The inclusion is compact by Rellich (4A.11 Sobolev Embeddings and Critical Exponents), and the inclusion 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).
Let be bounded in , with bounded in . Then a subsequence converges strongly in .
Proof. Step 1: compactness in . By Theorem 11.1, the are continuous into and uniformly in . So for each the set is bounded in , hence precompact in . And the are equicontinuous into :
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 , hence in .
Step 2: upgrading to . By Ehrling's lemma at each time, squared and integrated,
where bounds the norms. For the subsequence of Step 1 the last term tends to , so for every : the subsequence is Cauchy in .
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 can oscillate wildly in time, like , and functions with bounded time derivatives can oscillate in space.
Let be Lipschitz with constant , and consider on , on , . The Galerkin approximations satisfy for , a system of ODEs with Lipschitz right side, solvable for all time. Testing with , and using ,
so by Gronwall is bounded in , and as in 6A.7 Parabolic Regularity is bounded in . By Aubin–Lions a subsequence converges strongly in to some (and weakly in , with ). Strong convergence handles the nonlinearity: . So is a weak solution. Uniqueness follows by testing the difference of two solutions with : , 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.
Everything here works on a closed Riemannian manifold, with replaced by 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 ; 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.
Functions of time with values in and derivatives in are continuous into , with : the rigorous energy identity, proved by mollifying in time. Testing with and using elliptic regularity at each time gives improved regularity for data; differentiating in time gives higher regularity, up to only under compatibility conditions. Weighted energies prove instant smoothing with the parabolic rate per derivative. Ehrling's lemma and the Aubin–Lions lemma turn spatial bounds plus time-derivative bounds into strong compactness in , which lets Galerkin's method pass nonlinear terms to the limit. Diffusion out of a slab releases mass like early and approaches equilibrium like 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
For on with and : (a) show ; (b) integrate to get the remaining mass and the formula for in the opening box, using ; (c) derive the early-time law from the half-space solution : show that the flux out of one face is , so the total released by both faces up to time is , and divide by .
Solution
(a) The sine coefficients of on are , which is for odd . (b) for odd , so the remaining mass is , equal to at . (c) Near a face, at early times, the concentration is approximately ( at the face, inside), so , so the flux out is , and per face.
For the heat equation on with zero boundary values and , compute and from the series, and verify the first identity of Proposition 11.4.
Solution
and , so . Adding gives .
On , take . Show that , and that is a constant independent of (find it). Conclude that the bound cannot be improved in its dependence on .
Solution
, , . With , , maximised at with value . So for each some data (with ) nearly attain .
For the heat equation on with at both ends and , show that if is up to the corners, then ; and if is in and in up to the corners, then also . What happens to near for ?
Solution
Continuity at the corner gives . If is continuous up to the corner, then for (as ), so ; but , so . For , near the corner , whose -derivative is , unbounded near (along it is of size ).
(a) Let with a fixed . Show is bounded in but has no subsequence converging strongly in . Which hypothesis of Aubin–Lions fails? (b) Let on , independent of . Show but there is no strongly convergent subsequence in . Which hypothesis fails?
Solution
(a) . But weakly in while , so no subsequence converges strongly (the only possible limit is ). The time derivative is unbounded. (b) is unbounded; the spatial bound fails, and without strong convergence.
On a closed manifold with a fixed metric, let a tensor satisfy , where (a quadratic reaction term, as for the curvature under Ricci flow, 11A.2 How Curvature Evolves). (a) Show, by testing with and integrating by parts, that . (b) Deduce that as long as , grows at most like , and 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 to the derivative.
Solution
(a) and on a closed manifold; . (b) Dropping the gradient term, , so Gronwall gives the exponential bound. Integrating the full inequality over , , which is bounded.
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