The Korn–Lichtenstein Theorem and the Elliptic Canonical Form

Contents
  1. Statement
  2. From the canonical form to a Beltrami equation
  3. Normalizing the Beltrami coefficient
  4. The Cauchy and Beurling transforms
  5. The construction and the Jacobian

This appendix discharges the obligation recorded in Remark 14.14 of Partial Differential Equations: the elliptic branch of Proposition 14.13, the reduction of a second-order operator in two independent variables to the canonical form \(u_{\xi\xi}+u_{\eta\eta}\), under coefficients that are merely \(C^{1}\) and therefore only locally Hölder. The chapter's argument constructs the required complex first integral by complexifying the characteristic equation, which needs the coefficients to be real analytic; nothing in real ordinary differential equation theory replaces that step, because what is really being asked for is not a first integral of an ordinary equation at all but a solution of a first-order elliptic system in two variables — a Beltrami equation.

Four things are done below. First the reduction is made exact: the canonical form exists at a point if and only if a Beltrami equation with a coefficient of modulus bounded away from \(1\) has a local solution with non-vanishing Jacobian, and each of the equivalent formulations is derived from the previous one with nothing left implicit (From the canonical form to a Beltrami equation). Then the problem is normalized so that the Beltrami coefficient is as small as one pleases, in the Hölder norm and not merely in the supremum norm (Normalizing the Beltrami coefficient); this is where the Hölder hypothesis is spent, and it is what turns an existence problem into a convergent series. Then the singular-integral machinery is set out and the one deep estimate is stated precisely as a quoted theorem, with a remark saying exactly what is assumed and why this treatise does not prove it (The Cauchy and Beurling transforms). Finally the solution is constructed as an explicitly convergent Neumann series and the Jacobian is bounded below by hand (The construction and the Jacobian), which completes the proof.

Throughout, \(x\) and \(y\) are the two independent variables of the partial differential equation — not two spatial dimensions — and \(z = x+\ii y\), \(\bar z = x-\ii y\), with

\begin{equation}\tag{A13.1} \pp_{z} = \tfrac{1}{2}\bigl(\pp_{x}-\ii\,\pp_{y}\bigr)\ec\qquad \pp_{\bar z} = \tfrac{1}{2}\bigl(\pp_{x}+\ii\,\pp_{y}\bigr)\ec \end{equation}

so that \(\pp_{x} = \pp_{z}+\pp_{\bar z}\) and \(\pp_{y} = \ii\bigl(\pp_{z}-\pp_{\bar z}\bigr)\), and \(\nabla^{2} = 4\pp_{z}\pp_{\bar z}\). We write \(D_{\rho} = \set{z \in \C \mid \abs{z} < \rho}\), and for \(0 < \alpha < 1\)

\begin{equation}\tag{A13.2} [f]_{\alpha} = \sup_{z \neq w}\frac{\abs{f(z)-f(w)}}{\abs{z-w}^{\alpha}}\ec \end{equation}

\(C^{\alpha}\) denoting the functions with \([f]_{\alpha} < \infty\) and \(C^{k,\alpha}\) those whose derivatives up to order \(k\) lie in \(C^{\alpha}\).

Statement

Theorem A13.1 (Local canonical form for an elliptic operator with Hölder coefficients).

Let \(L u = a\,u_{xx} + 2b\,u_{xy} + c\,u_{yy} + \cdots\) be elliptic on a neighbourhood of \(P_{0}\), that is \(\Delta = b^{2}-ac < 0\) there, with \(a,b,c\) of class \(C^{\alpha}\) for some \(\alpha \in (0,1)\) — in particular whenever they are \(C^{1}\). Then there are a neighbourhood \(V\) of \(P_{0}\) and a map \((\xi,\eta) : V \longrightarrow \R^{2}\) of class \(C^{1,\alpha}\) whose Jacobian \(J_{0} = \xi_{x}\eta_{y}-\xi_{y}\eta_{x}\) is bounded away from \(0\) on \(V\), such that the transformed principal coefficients of Equation (14.12) satisfy

\begin{equation}\tag{A13.3} \tilde a = \tilde c = \delta\,J_{0} > 0\ec \qquad \tilde b = 0\ec \qquad \delta = \sqrt{ac-b^{2}}\ec \end{equation}

so that in the coordinates \((\xi,\eta)\) the principal part of \(L\) is \(\delta J_{0}\bigl(\pp_{\xi}^{2}+\pp_{\eta}^{2}\bigr)\), a positive multiple of the Laplacian. If in addition \(a,b,c \in C^{1,\alpha}\), the map is of class \(C^{2,\alpha}\) and the reduction is classical: the transformed operator is a genuine second-order operator with continuous coefficients, of the third form in Equation (14.10). Rests on Proposition 14.13, Definition 14.6 and Equation (14.6).

Two remarks fix what Theorem A13.1 does and does not claim, and the second is the reason the theorem is stated in two halves.

Remark A13.2 (Why the principal part is the whole claim at $C^{1}$).

The congruence Equation (14.6) that carries \(A\) to \(\tilde A\) involves the Jacobian \(J\) and nothing else, so it is meaningful for any \(C^{1}\) change of coordinates and is a pointwise statement of linear algebra. The extra term of Equation (14.7), by contrast, carries the second derivatives \(\pp_{i}\pp_{j}y^{a}\) of the change; a \(C^{1,\alpha}\) change does not have them, so for coefficients that are merely \(C^{\alpha}\) the transformed equation is not literally an equation with continuous first-order coefficients — the first-order remainder exists only as a distribution. Nothing is wrong with the reduction; what is wrong is the naive reading of what “the equation becomes \(u_{\xi\xi}+u_{\eta\eta}+\cdots\)” asserts. This is why the theorem separates the two statements, and why the second half buys the classical form with one extra derivative on the coefficients. The chapter's sentence that the conclusion of Proposition 14.13 “does hold at \(C^{1}\)” is correct in the first sense and should be read in it.

Remark A13.3.

There is no loss in assuming \(a > 0\). Ellipticity gives \(ac > b^{2} \ge 0\), so \(a\) and \(c\) are nonzero and of the same sign; replacing \(L\) by \(-L\), which changes no solution of \(Lu=f\) except by the sign of \(f\), makes both positive. The matrix \(A\) of Equation (14.11) is then positive definite, and \(\delta = \sqrt{ac-b^{2}} = \sqrt{\det A} > 0\) is continuous and bounded away from \(0\) near \(P_{0}\).

From the canonical form to a Beltrami equation

Proposition A13.4 (The complex characteristic equation).

Let \(\xi,\eta\) be real \(C^{1}\) functions near \(P_{0}\) and set \(\zeta = \xi + \ii\eta\). Then, with \(\tilde a,\tilde b,\tilde c\) the transformed principal coefficients of Equation (14.12),

\begin{equation}\tag{A13.4} a\,\zeta_{x}^{2} + 2b\,\zeta_{x}\zeta_{y} + c\,\zeta_{y}^{2} = \bigl(\tilde a - \tilde c\bigr) + 2\ii\,\tilde b\ep \end{equation}

Hence \(\tilde a = \tilde c\) and \(\tilde b = 0\) hold at a point if and only if \(\zeta\) satisfies the characteristic equation Equation (14.8) there, with the complex \(\nabla\zeta\) in place of \(\nabla\phi\). Rests on Equations (14.8) and (14.12).

Proof.

Derives Proposition A13.4. Expand, using \(\zeta_{x} = \xi_{x}+\ii\eta_{x}\) and \(\zeta_{y} = \xi_{y}+\ii\eta_{y}\):

\begin{equation*} a\zeta_{x}^{2} = a\bigl(\xi_{x}^{2}-\eta_{x}^{2}\bigr) + 2\ii a\,\xi_{x}\eta_{x}\ec \end{equation*}
\begin{equation*} 2b\,\zeta_{x}\zeta_{y} = 2b\bigl(\xi_{x}\xi_{y}-\eta_{x}\eta_{y}\bigr) + 2\ii b\bigl(\xi_{x}\eta_{y}+\eta_{x}\xi_{y}\bigr)\ec \end{equation*}
\begin{equation*} c\,\zeta_{y}^{2} = c\bigl(\xi_{y}^{2}-\eta_{y}^{2}\bigr) + 2\ii c\,\xi_{y}\eta_{y}\ep \end{equation*}

The real parts sum to \(\bigl(a\xi_{x}^{2}+2b\xi_{x}\xi_{y}+c\xi_{y}^{2}\bigr) -\bigl(a\eta_{x}^{2}+2b\eta_{x}\eta_{y}+c\eta_{y}^{2}\bigr) = \tilde a - \tilde c\) by Equation (14.12), and the imaginary parts sum to twice the polarisation \(a\xi_{x}\eta_{x}+b(\xi_{x}\eta_{y}+\eta_{x}\xi_{y})+c\xi_{y}\eta_{y} = \tilde b\).

Proposition A13.5 (The isothermal system).

Assume \(a>0\) and \(\Delta<0\), and write \(\delta = \sqrt{ac-b^{2}}>0\). A \(C^{1}\) pair \((\xi,\eta)\) satisfies the equation of Proposition A13.4 with the branch \(a\zeta_{x}+(b+\ii\delta)\zeta_{y}=0\) if and only if

\begin{equation}\tag{A13.5} \eta_{x} = -\frac{b\,\xi_{x}+c\,\xi_{y}}{\delta}\ec\qquad \eta_{y} = \frac{a\,\xi_{x}+b\,\xi_{y}}{\delta}\ep \end{equation}

For such a pair,

\begin{equation}\tag{A13.6} J_{0} = \xi_{x}\eta_{y}-\xi_{y}\eta_{x} = \frac{a\xi_{x}^{2}+2b\xi_{x}\xi_{y}+c\xi_{y}^{2}}{\delta} = \frac{\tilde a}{\delta}\ec \end{equation}

so \(J_{0} > 0\) exactly where \(\nabla\xi \neq 0\), and Equation (A13.3) holds there. Rests on Proposition A13.4 and Equation (14.11).

Proof.

Derives Proposition A13.5. The quadratic \(a t^{2}+2bt+c\) has the two roots \(t_{\pm} = \bigl(-b\pm\ii\delta\bigr)/a\), so \(a\zeta_{x}^{2}+2b\zeta_{x}\zeta_{y}+c\zeta_{y}^{2} = a\bigl(\zeta_{x}-t_{+}\zeta_{y}\bigr) \bigl(\zeta_{x}-t_{-}\zeta_{y}\bigr)\) and the equation of Proposition A13.4 holds if and only if one of the two factors vanishes. Take the factor \(\zeta_{x}-t_{-}\zeta_{y} = 0\), i.e.\ \(a\zeta_{x} + \bigl(b+\ii\delta\bigr)\zeta_{y} = 0\) (the other branch is the complex conjugate statement and produces \(\bar\zeta\)). Separating real and imaginary parts of \(a(\xi_{x}+\ii\eta_{x}) + (b+\ii\delta)(\xi_{y}+\ii\eta_{y}) = 0\),

\begin{equation}\tag{A13.7} a\xi_{x} + b\xi_{y} - \delta\eta_{y} = 0\ec \qquad a\eta_{x} + b\eta_{y} + \delta\xi_{y} = 0\ep \end{equation}

The first is the second half of Equation (A13.5). Substituting it into the second and using \(\delta^{2} = ac-b^{2}\), so that \(b^{2}+\delta^{2} = ac\),

\begin{equation*} a\eta_{x} = -\delta\xi_{y} - \frac{b\bigl(a\xi_{x}+b\xi_{y}\bigr)}{\delta} = -\frac{ab\,\xi_{x} + \bigl(b^{2}+\delta^{2}\bigr)\xi_{y}}{\delta} = -\frac{a\bigl(b\,\xi_{x}+c\,\xi_{y}\bigr)}{\delta}\ec \end{equation*}

and dividing by \(a \neq 0\) gives the first half. The steps are reversible, which is the “only if”.

For Equation (A13.6), substitute Equation (A13.5):

\begin{equation*} \xi_{x}\eta_{y}-\xi_{y}\eta_{x} = \frac{\xi_{x}\bigl(a\xi_{x}+b\xi_{y}\bigr) + \xi_{y}\bigl(b\xi_{x}+c\xi_{y}\bigr)}{\delta}\ec \end{equation*}

which is the displayed quadratic form. That form is \(\vect{v}\transpose A\,\vect{v}/\delta\) with \(\vect{v} = (\xi_{x},\xi_{y})\) and \(A\) the positive definite matrix of Equation (14.11) (Remark A13.3), so it is positive whenever \(\vect{v} \neq 0\) and zero otherwise. Finally Proposition A13.4 gives \(\tilde a = \tilde c\) and \(\tilde b = 0\), and Equation (A13.6) identifies \(\tilde a = \delta J_{0}\), which is Equation (A13.3).

Remark A13.6 (Why this is not an ordinary differential equation).

Eliminating \(\eta\) from Equation (A13.5) by the equality of mixed partials \(\pp_{y}\eta_{x} = \pp_{x}\eta_{y}\) gives, for \(\xi\) alone, the second-order equation in divergence form

\begin{equation}\tag{A13.8} \pp_{x}\!\left(\frac{a\,\xi_{x}+b\,\xi_{y}}{\delta}\right) + \pp_{y}\!\left(\frac{b\,\xi_{x}+c\,\xi_{y}}{\delta}\right) = 0\ec \end{equation}

whose principal part is again \(L\)'s. That is the exact sense in which the elliptic branch of Proposition 14.13 is circular if attacked head-on: putting an elliptic operator in canonical form is equivalent to solving an elliptic equation with the same principal part. The hyperbolic and parabolic branches escape this because there the two characteristic directions are real, so the corresponding first integrals come from Theorem 13.8 applied to a real ordinary differential equation, which needs no more than continuity and a Lipschitz condition. The complex route below breaks the circle by solving Equation (A13.8) not by elliptic theory but by inverting a constant-coefficient operator, \(\pp_{\bar z}\), and treating everything else as a perturbation.

Proposition A13.7 (Beltrami form).

With \(a>0\), \(\Delta<0\) and \(\delta = \sqrt{ac-b^{2}}\), the branch \(a\zeta_{x}+(b+\ii\delta)\zeta_{y}=0\) of Proposition A13.5 is exactly the Beltrami equation

\begin{equation}\tag{A13.9} \pp_{\bar z}\zeta = \mu\,\pp_{z}\zeta\ec\qquad \mu = -\frac{a-\delta+\ii b}{a+\delta-\ii b}\ec \end{equation}

and its coefficient satisfies

\begin{equation}\tag{A13.10} \abs{\mu}^{2} = \frac{\bigl(a-\delta\bigr)^{2}+b^{2}} {\bigl(a+\delta\bigr)^{2}+b^{2}} < 1\ec \end{equation}

with \(\mu = 0\) exactly where \(A\) is a positive multiple of the identity. Moreover the Jacobian of \(z \longmapsto \zeta\) is

\begin{equation}\tag{A13.11} J_{0} = \abs{\pp_{z}\zeta}^{2} - \abs{\pp_{\bar z}\zeta}^{2} = \bigl(1-\abs{\mu}^{2}\bigr)\,\abs{\pp_{z}\zeta}^{2}\ep \end{equation}

Rests on Proposition A13.5 and Equation (A13.1).

Proof.

Derives Proposition A13.7. Substitute \(\zeta_{x} = \pp_{z}\zeta+\pp_{\bar z}\zeta\) and \(\zeta_{y} = \ii\bigl(\pp_{z}\zeta-\pp_{\bar z}\zeta\bigr)\) from Equation (A13.1) into \(a\zeta_{x}+(b+\ii\delta)\zeta_{y}=0\) and use \((b+\ii\delta)\ii = -\delta+\ii b\):

\begin{equation*} \bigl(a-\delta+\ii b\bigr)\pp_{z}\zeta + \bigl(a+\delta-\ii b\bigr)\pp_{\bar z}\zeta = 0\ep \end{equation*}

The coefficient of \(\pp_{\bar z}\zeta\) has modulus squared \((a+\delta)^{2}+b^{2} > 0\) and never vanishes, so the equation may be solved for \(\pp_{\bar z}\zeta\), giving Equation (A13.9). Its modulus is Equation (A13.10), and \((a-\delta)^{2} < (a+\delta)^{2}\) because \(a\) and \(\delta\) are both positive; equality of the numerator with \(0\) requires \(b = 0\) and \(a = \delta = \sqrt{ac}\), i.e. \(a = c\) and \(b=0\).

For Equation (A13.11), write \(A_{1} = \zeta_{x}\) and \(B_{1} = \ii\zeta_{y}\), so that \(\pp_{z}\zeta = \tfrac12(A_{1}-B_{1})\) and \(\pp_{\bar z}\zeta = \tfrac12(A_{1}+B_{1})\). Then

\begin{equation*} \abs{\pp_{z}\zeta}^{2}-\abs{\pp_{\bar z}\zeta}^{2} = \tfrac14\left(\abs{A_{1}-B_{1}}^{2}-\abs{A_{1}+B_{1}}^{2}\right) = -\Re\bigl(\bar A_{1}B_{1}\bigr) = -\Re\bigl(\ii\,\bar\zeta_{x}\zeta_{y}\bigr) = \Im\bigl(\bar\zeta_{x}\zeta_{y}\bigr)\ec \end{equation*}

and \(\bar\zeta_{x}\zeta_{y} = (\xi_{x}-\ii\eta_{x})(\xi_{y}+\ii\eta_{y})\) has imaginary part \(\xi_{x}\eta_{y}-\eta_{x}\xi_{y} = J_{0}\). Inserting Equation (A13.9) gives the second equality.

Proposition A13.7 reduces Theorem A13.1 to a single question: does Equation (A13.9) have a local \(C^{1,\alpha}\) solution with \(\pp_{z}\zeta \neq 0\)? Note that Equation (A13.11) has already disposed of the Jacobian: because \(\abs{\mu}\) is bounded away from \(1\), a solution whose \(\pp_{z}\zeta\) does not vanish automatically has \(J_{0}\) bounded away from \(0\), and no separate argument is needed.

Normalizing the Beltrami coefficient

Lemma A13.8 (Affine normalization).

There is an invertible real linear change of the independent variables after which \(A(P_{0}) = \identity\), \(\delta(P_{0}) = 1\) and \(\mu(P_{0}) = 0\), the transformed coefficients being again of class \(C^{\alpha}\) and again elliptic. Rests on Proposition A13.7 and Theorem 14.8.

Proof.

Derives Lemma A13.8. \(A(P_{0})\) is symmetric and positive definite (Remark A13.3), so it factors as \(A(P_{0}) = S\,S\transpose\) with \(S\) real and invertible — take \(S = O\Lambda^{1/2}\) with \(A(P_{0}) = O\Lambda O\transpose\) its orthogonal diagonalization, the eigenvalues in \(\Lambda\) being positive. Change variables by \(\hat{\vect{x}} = S^{-1}\vect{x}\), whose Jacobian is the constant matrix \(J = S^{-1}\); by Equation (14.6) the new principal matrix is

\begin{equation}\tag{A13.12} \hat A = S^{-1}A\,\bigl(S^{-1}\bigr)\transpose\ec\qquad \hat A(P_{0}) = S^{-1}S\,S\transpose\bigl(S\transpose\bigr)^{-1} = \identity\ep \end{equation}

Congruence with a constant matrix preserves Hölder continuity and, by Theorem 14.8, ellipticity. At \(P_{0}\) one then has \(\hat a = \hat c = 1\), \(\hat b = 0\), \(\hat\delta = 1\), and Equation (A13.9) gives \(\mu(P_{0}) = -(1-1+0)/(1+1-0) = 0\). Since a composition of two changes of coordinates with non-vanishing Jacobians is again one, proving Theorem A13.1 for the normalized problem proves it in general.

Lemma A13.9 (Smallness after rescaling).

Assume the normalization of Lemma A13.8 and identify \(P_{0}\) with \(0 \in \C\). Fix once and for all a cutoff \(\chi \in C^{\infty}(\C)\) with \(0 \le \chi \le 1\), \(\chi = 1\) on \(\overline{D_{1}}\) and \(\chi = 0\) off \(D_{2}\). For \(r>0\) put

\begin{equation}\tag{A13.13} \nu_{r}(z) = \chi(z)\,\mu(rz)\ep \end{equation}

Then \(\nu_{r} \in C^{\alpha}(\C)\) vanishes off \(\overline{D_{2}}\), coincides with \(z \longmapsto \mu(rz)\) on \(\overline{D_{1}}\), satisfies \(\norm{\nu_{r}}_{\infty} \le \sup\abs{\mu} < 1\), and

\begin{equation}\tag{A13.14} \norm{\nu_{r}}_{\infty} + [\nu_{r}]_{\alpha} \le K\,r^{\alpha}\,[\mu]_{\alpha} \longrightarrow 0 \qquad (r \to 0^{+})\ec \end{equation}

with \(K\) depending only on \(\chi\) and \(\alpha\). If moreover \(a,b,c \in C^{1,\alpha}\), the same holds with the \(C^{1,\alpha}\) norm in place of the \(C^{\alpha}\) norm and \(r\) in place of \(r^{\alpha}\). Rests on Lemma A13.8 and Equation (A13.2).

Proof.

Derives Lemma A13.9. \(\mu\) is a rational function of \(a,b,\delta\) with non-vanishing denominator, hence of class \(C^{\alpha}\) on a neighbourhood of \(0\); shrink that neighbourhood to a disc \(D_{\rho}\) and take \(r < \rho/2\) so that \(rz \in D_{\rho}\) for \(z \in D_{2}\). Write \(\mu^{(r)}(z) = \mu(rz)\). Since \(\mu(0)=0\) by Lemma A13.8,

\begin{equation}\tag{A13.15} \abs{\mu^{(r)}(z)} = \abs{\mu(rz)-\mu(0)} \le [\mu]_{\alpha}\,\abs{rz}^{\alpha} \le [\mu]_{\alpha}\,(2r)^{\alpha} \qquad (z \in D_{2})\ec \end{equation}

and directly from Equation (A13.2), \([\mu^{(r)}]_{\alpha,D_{2}} = r^{\alpha}[\mu]_{\alpha}\). For the product with the cutoff, use \(\abs{\chi f(z)-\chi f(w)} \le \abs{\chi(z)}\abs{f(z)-f(w)} + \abs{f(w)}\abs{\chi(z)-\chi(w)}\), so that

\begin{equation}\tag{A13.16} [\chi f]_{\alpha} \le \norm{\chi}_{\infty}[f]_{\alpha} + \norm{f}_{\infty}[\chi]_{\alpha}\ec \end{equation}

which with Equation (A13.15) gives \([\nu_{r}]_{\alpha} \le r^{\alpha}[\mu]_{\alpha} + (2r)^{\alpha}[\mu]_{\alpha}[\chi]_{\alpha}\). Adding \(\norm{\nu_{r}}_{\infty} \le (2r)^{\alpha}[\mu]_{\alpha}\) gives Equation (A13.14) with \(K = 1+2^{\alpha}\bigl(1+[\chi]_{\alpha}\bigr)\). The bound \(\norm{\nu_{r}}_{\infty} \le \sup\abs{\mu} < 1\) is Equation (A13.10) and \(0\le\chi\le1\). Under the stronger hypothesis \(a,b,c \in C^{1,\alpha}\) one has \(\mu \in C^{1,\alpha}\) and \(\pp\mu^{(r)} = r\,(\pp\mu)(rz)\), so every seminorm entering the \(C^{1,\alpha}\) norm of \(\mu^{(r)}\) carries at least one factor \(r\), and the same product estimate applies.

Remark A13.10 (Where the Hölder hypothesis is spent).

Lemma A13.9 is the whole use made of the Hölder continuity of the coefficients, and it is worth seeing why mere continuity would not do. Continuity of \(\mu\) at \(P_{0}\) makes \(\norm{\nu_{r}}_{\infty}\) small, which is enough for an \(L^{p}\) theory but not for a Hölder one; what the exponent \(\alpha\) buys is the factor \(r^{\alpha}\) in Equation (A13.14), which makes the seminorm small as well and thereby turns the Neumann series of The construction and the Jacobian into a convergent series in the very space where the solution's regularity is measured. A zooming argument of this kind is available only because the Beltrami equation is invariant under \(z \longmapsto rz\): if \(\hat\zeta\) solves \(\pp_{\bar z}\hat\zeta = \mu^{(r)}\,\pp_{z}\hat\zeta\) on \(D_{1}\), then \(\zeta(w) = \hat\zeta(w/r)\) solves Equation (A13.9) on \(D_{r}\), both derivatives picking up the same factor \(1/r\), and the Jacobian is multiplied by the positive number \(r^{-2}\).

The Cauchy and Beurling transforms

Definition A13.11 (Cauchy and Beurling transforms).

For \(f\) continuous and vanishing outside a compact set put

\begin{equation}\tag{A13.17} Pf(z) = \frac{1}{\pi}\int_{\C}\frac{f(w)}{z-w}\,\dd A(w)\ec \qquad Tf(z) = -\frac{1}{\pi}\,\mathrm{p.v.}\!\int_{\C} \frac{f(w)}{(z-w)^{2}}\,\dd A(w)\ec \end{equation}

\(\dd A\) being the area element of the plane and the principal value meaning the limit of the integral over \(\abs{z-w} > \varepsilon\) as \(\varepsilon \to 0^{+}\). \(P\) is the Cauchy transform and \(T\) the Beurling transform. Rests on Equation (A13.1).

The integral defining \(Pf\) converges absolutely, the kernel \(\abs{z-w}^{-1}\) being integrable in the plane; the one defining \(Tf\) does not, and the principal value is not a notational convenience but the entire difficulty. The next lemma explains why \(P\) is the right object, and is the one part of the analytic package this treatise can prove outright, because it is the two-dimensional twin of Proposition 14.67.

Lemma A13.12 (Fundamental solution of $\pp_{\bar z}$).

In the sense of distributions on \(\C \cong \R^{2}\),

\begin{equation}\tag{A13.18} \nabla^{2}\!\left(\frac{1}{2\pi}\ln\abs{z}\right) = \delta\ec \qquad\text{and hence}\qquad \pp_{\bar z}\!\left(\frac{1}{\pi z}\right) = \delta\ep \end{equation}

Consequently \(Pf = \bigl(\pi z\bigr)^{-1} * f\) satisfies \(\pp_{\bar z}Pf = f\) distributionally. Rests on Proposition 14.67 and Equation (A13.1).

Proof.

Derives Lemma A13.12. Let \(G(z) = (2\pi)^{-1}\ln\abs{z}\), which is harmonic on \(\C \setminus \set{0}\) because \(\nabla^{2}\ln r = r^{-1}\pp_{r}(r\,\pp_{r}\ln r) = r^{-1}\pp_{r}(1)=0\) in plane polar coordinates. Let \(\varphi\) be a test function. Since \(\ln\abs{z}\) is integrable near the origin, \(\int G\nabla^{2}\varphi\,\dd A = \lim_{\varepsilon\to0^{+}}\int_{r>\varepsilon}G\nabla^{2}\varphi\,\dd A\). On \(r>\varepsilon\) apply Green's second identity Equation (14.41) with \(p=1\), \(u=\varphi\), \(v=G\); the term \(\varphi\nabla^{2}G\) vanishes, and the only boundary is the circle \(r=\varepsilon\), whose outward normal for the region \(r>\varepsilon\) points at the origin, so \(\pp_{\nu} = -\pp_{r}\) there. Hence

\begin{equation*} -\int_{r>\varepsilon}G\,\nabla^{2}\varphi\,\dd A = \oint_{r=\varepsilon} \left(-\varphi\,\pp_{r}G + G\,\pp_{r}\varphi\right)\dd s = -\frac{1}{2\pi\varepsilon}\oint_{r=\varepsilon}\varphi\,\dd s + \frac{\ln\varepsilon}{2\pi}\oint_{r=\varepsilon} \pp_{r}\varphi\,\dd s\ec \end{equation*}

using \(\pp_{r}G = (2\pi r)^{-1}\). The circle has length \(2\pi\varepsilon\), so the first term tends to \(-\varphi(0)\) by continuity of \(\varphi\) and the second is bounded by \(\varepsilon\abs{\ln\varepsilon}\sup\abs{\nabla\varphi} \to 0\). Thus \(\int G\nabla^{2}\varphi\,\dd A = \varphi(0)\), which is the first half of Equation (A13.18). For the second, note \(\nabla^{2} = 4\pp_{z}\pp_{\bar z}\) and \(\pp_{z}\ln\abs{z} = \pp_{z}\tfrac12\ln\bigl(z\bar z\bigr) = 1/(2z)\), so \(\delta = 4\pp_{\bar z}\pp_{z}G = 4\pp_{\bar z}\bigl(1/(4\pi z)\bigr) = \pp_{\bar z}\bigl(1/(\pi z)\bigr)\). Finally Equation (A13.17) is the convolution of \(f\) with \(1/(\pi z)\), and differentiating a convolution moves the derivative onto either factor.

Theorem A13.13 (Quoted: the Korn–Lichtenstein estimate for the Beurling transform).

Let \(0 < \alpha < 1\) and let \(f \in C^{\alpha}(\C)\) vanish outside \(\overline{D_{2}}\). Then:

  1. the principal value defining \(Tf\) in Equation (A13.17) exists at every point of \(\C\);

  2. \(Pf\) is continuously differentiable on \(\C\), with

    \begin{equation}\tag{A13.19} \pp_{\bar z}Pf = f\ec \qquad \pp_{z}Pf = Tf \end{equation}

    holding classically;

  3. \(Tf \in C^{\alpha}(\C)\) and

    \begin{equation}\tag{A13.20} \norm{Tf}_{\infty} + [Tf]_{\alpha} \le C_{\alpha}\,[f]_{\alpha}\ec \end{equation}

    with \(C_{\alpha}\) depending only on \(\alpha\);

  4. if in addition \(f \in C^{k,\alpha}\) for an integer \(k \ge 1\), then \(Tf \in C^{k,\alpha}\) and \(\norm{Tf}_{C^{k,\alpha}} \le C_{k,\alpha}\norm{f}_{C^{k,\alpha}}\).

Remark A13.14 (What is quoted here).

Theorem A13.13 is the only input of this section that is not proved, and it is worth being exact about its three parts. Part (ii) is half proved above: \(\pp_{\bar z}Pf = f\) is Lemma A13.12, and the Hölder hypothesis upgrades it from a distributional to a classical identity. Parts (i) and the second half of (ii) — that the singular integral converges and that it is the \(z\)-derivative of \(Pf\) — are the statement that differentiating the Newtonian-type potential \(Pf\) a second time is legitimate in the principal-value sense; the same question arises for the Newtonian potential of Proposition 14.67, where the chapter needed only one derivative and could avoid it. Part (iii) is the substantial content: it says the Beurling transform, a singular integral operator whose kernel \((z-w)^{-2}\) is exactly at the critical homogeneity for the plane, is bounded on Hölder spaces. That is the Korn–Lichtenstein inequality, proved for such kernels by Korn in 1914 and Lichtenstein in 1916 and placed in its general setting by the Calderón–Zygmund theory of singular integrals [Calderon:1952]; the standard modern account of the Beltrami equation built on it is Vekua's. The two original memoirs and Vekua's monograph are not entries of this bibliography, so those attributions are made in words; what the treatise does contain and does cite for the classical, real-analytic route is Courant and Hilbert [Courant:1962].

Why the estimate is not proved here is not a matter of length. Its proof requires the Calderón–Zygmund decomposition of a function relative to a cube, or an equivalent covering argument, and both rest on Lebesgue measure and on the maximal function; Real Analysis develops the Riemann integral only, and the Lebesgue theory these arguments belong to is not built anywhere in this book. Everything else in this section — the reduction of From the canonical form to a Beltrami equation, the normalization of Normalizing the Beltrami coefficient, the convergent series and the Jacobian bound of The construction and the Jacobian — is elementary once Equation (A13.20) is granted, and is carried out in full.

Remark A13.15 (The shape of the estimate).

Two features of Equation (A13.20) are used below and are worth isolating. First, the right-hand side involves only the seminorm \([f]_{\alpha}\), which is legitimate because \(f\) vanishes off \(\overline{D_{2}}\): every point of \(\overline{D_{2}}\) lies within distance \(4\) of a point where \(f\) vanishes, so \(\norm{f}_{\infty} \le 4^{\alpha}[f]_{\alpha}\), and \([\,\cdot\,]_{\alpha}\) is therefore a genuine norm on the space of such \(f\), complete because a \([\,\cdot\,]_{\alpha}\)-Cauchy sequence converges uniformly and its limit inherits the seminorm bound. Second, the left-hand side controls \(\norm{Tf}_{\infty}\) as well as \([Tf]_{\alpha}\), and the supremum bound is what will be needed to keep \(\pp_{z}\zeta\) away from zero.

The construction and the Jacobian

Proposition A13.16 (A convergent Neumann series).

Let \(\nu \in C^{\alpha}(\C)\) vanish off \(\overline{D_{2}}\) and set

\begin{equation}\tag{A13.21} \varepsilon_{\nu} = \left(\norm{\nu}_{\infty} + [\nu]_{\alpha}\right)C_{\alpha}\ec \end{equation}

with \(C_{\alpha}\) the constant of Equation (A13.20). If \(\varepsilon_{\nu} < 1\) then the series

\begin{equation}\tag{A13.22} h = \sum_{n=0}^{\infty}h_{n}\ec\qquad h_{0} = \nu\ec\qquad h_{n+1} = \nu\,T h_{n}\ec \end{equation}

converges in the space \(X\) of \(C^{\alpha}\) functions vanishing off \(\overline{D_{2}}\), and its sum is the unique element of \(X\) with

\begin{equation}\tag{A13.23} h = \nu\bigl(1 + Th\bigr)\ec\qquad [h]_{\alpha} \le \frac{[\nu]_{\alpha}}{1-\varepsilon_{\nu}}\ep \end{equation}

Rests on Theorem A13.13 and Equation (A13.2).

Proof.

Derives Proposition A13.16. Each \(h_{n}\) lies in \(X\): it is a product one of whose factors is \(\nu\), which vanishes off \(\overline{D_{2}}\), and it is Hölder because \(Th_{n-1}\) is, by Equation (A13.20). By the product estimate Equation (A13.16) applied to \(\nu\,Tg\) and then Equation (A13.20),

\begin{equation}\tag{A13.24} \bigl[\nu\,Tg\bigr]_{\alpha} \le \norm{\nu}_{\infty}\bigl[Tg\bigr]_{\alpha} + [\nu]_{\alpha}\norm{Tg}_{\infty} \le \left(\norm{\nu}_{\infty}+[\nu]_{\alpha}\right) \left(\norm{Tg}_{\infty}+\bigl[Tg\bigr]_{\alpha}\right) \le \varepsilon_{\nu}\,[g]_{\alpha} \end{equation}

for every \(g \in X\). Hence \([h_{n}]_{\alpha} \le \varepsilon_{\nu}^{\,n}[\nu]_{\alpha}\) by induction, and the series Equation (A13.22) is dominated term by term by a geometric series of ratio \(\varepsilon_{\nu}<1\). Since \([\,\cdot\,]_{\alpha}\) is a complete norm on \(X\) (Remark A13.15), the series converges there, with the bound stated in Equation (A13.23); the same domination and Lemma 13.6 give uniform convergence, so the sum may be rearranged and \(T\) applied term by term, \(T\) being bounded. Then

\begin{equation*} \nu\bigl(1+Th\bigr) = \nu + \nu\,T\!\left(\sum_{n\ge0}h_{n}\right) = h_{0} + \sum_{n\ge0}h_{n+1} = h\ec \end{equation*}

which is Equation (A13.23). Uniqueness: if \(h,h'\in X\) both satisfy it, then \([h-h']_{\alpha} = [\nu T(h-h')]_{\alpha} \le \varepsilon_{\nu}[h-h']_{\alpha}\) by Equation (A13.24), and \(\varepsilon_{\nu}<1\) forces \([h-h']_{\alpha}=0\), hence \(h=h'\) since both vanish off a compact set.

Proposition A13.17 (The solution and its Jacobian).

In the situation of Proposition A13.16, suppose in addition

\begin{equation}\tag{A13.25} \frac{C_{\alpha}[\nu]_{\alpha}}{1-\varepsilon_{\nu}} \le \frac{1}{2}\ep \end{equation}

Then \(\zeta(z) = z + Ph(z)\) is of class \(C^{1,\alpha}\) on \(\C\), solves \(\pp_{\bar z}\zeta = \nu\,\pp_{z}\zeta\) there, and satisfies

\begin{equation}\tag{A13.26} \abs{\pp_{z}\zeta} \ge \tfrac{1}{2}\ec\qquad J_{0} = \bigl(1-\abs{\nu}^{2}\bigr)\abs{\pp_{z}\zeta}^{2} \ge \tfrac14\left(1-\norm{\nu}_{\infty}^{2}\right) > 0\ep \end{equation}

Rests on Proposition A13.16, Theorem A13.13 and Equation (A13.11).

Proof.

Derives Proposition A13.17. By part (ii) of Theorem A13.13 applied to \(h \in X\),

\begin{equation}\tag{A13.27} \pp_{\bar z}\zeta = \pp_{\bar z}z + \pp_{\bar z}Ph = h\ec \qquad \pp_{z}\zeta = 1 + Th\ec \end{equation}

both continuous and Hölder by part (iii), so \(\zeta \in C^{1,\alpha}\). The Beltrami equation \(\pp_{\bar z}\zeta = \nu\,\pp_{z}\zeta\) reads, after Equation (A13.27), precisely \(h = \nu(1+Th)\), which is Equation (A13.23). For the Jacobian, Equation (A13.20) and Equation (A13.23) give

\begin{equation*} \norm{Th}_{\infty} \le C_{\alpha}[h]_{\alpha} \le \frac{C_{\alpha}[\nu]_{\alpha}}{1-\varepsilon_{\nu}} \le \frac12 \end{equation*}

by Equation (A13.25), so \(\abs{\pp_{z}\zeta} = \abs{1+Th} \ge 1 - \tfrac12 = \tfrac12\) everywhere. Equation (A13.11) then yields the second half of Equation (A13.26), and \(\norm{\nu}_{\infty}<1\) makes it strictly positive.

Proof of Theorem A13.1. Derives Theorem A13.1. By Remark A13.3 assume \(a>0\), and by Lemma A13.8 assume further that \(A(P_{0}) = \identity\) and \(\mu(P_{0})=0\), \(P_{0}\) being the origin of \(\C\); both reductions are linear changes of the independent variables with constant non-vanishing Jacobian, and composing them with the map constructed below gives the map of the theorem.

Let \(\nu_{r}\) be the cutoff coefficient of Lemma A13.9. By Equation (A13.14) both \(\varepsilon_{\nu_{r}}\) of Equation (A13.21) and the left-hand side of Equation (A13.25) are bounded by \(C_{\alpha}K r^{\alpha}[\mu]_{\alpha}\) times a constant, so choosing \(r\) small enough makes \(\varepsilon_{\nu_{r}} \le \tfrac12\) and Equation (A13.25) hold. Fix such an \(r\). Propositions A13.16 and A13.17 then produce \(\hat\zeta \in C^{1,\alpha}(\C)\) with \(\pp_{\bar z}\hat\zeta = \nu_{r}\pp_{z}\hat\zeta\) and Jacobian bounded below by a positive constant.

On \(\overline{D_{1}}\) one has \(\nu_{r}(z) = \mu(rz)\), so \(\zeta(w) = \hat\zeta(w/r)\) satisfies Equation (A13.9) on \(D_{r}\) by the scaling identity of Remark A13.10, with Jacobian multiplied by \(r^{-2}>0\) and hence still bounded away from \(0\). Set \(V = D_{r}\) and \((\xi,\eta) = (\Re\zeta,\Im\zeta)\), which is \(C^{1,\alpha}\). By Proposition A13.7 the pair satisfies the branch \(a\zeta_{x}+(b+\ii\delta)\zeta_{y}=0\) of the complex characteristic equation, so by Propositions A13.4 and A13.5 the transformed coefficients obey \(\tilde b = 0\) and \(\tilde a = \tilde c = \delta J_{0} > 0\), which is Equation (A13.3). The transformed principal part is therefore \(\tilde a\,u_{\xi\xi}+\tilde c\,u_{\eta\eta} = \delta J_{0}\bigl(u_{\xi\xi}+u_{\eta\eta}\bigr)\), as claimed.

For the last sentence of the theorem, suppose \(a,b,c\in C^{1,\alpha}\). Then \(\mu \in C^{1,\alpha}\), and by the last clause of Lemma A13.9 the quantity \(\norm{\nu_{r}}_{C^{1,\alpha}}\) is \(O(r)\). Running Proposition A13.16 in the space of \(C^{1,\alpha}\) functions vanishing off \(\overline{D_{2}}\) — legitimate because part (iv) of Theorem A13.13 bounds \(T\) there, and because the product estimate Equation (A13.16) has an evident \(C^{1,\alpha}\) counterpart obtained by applying it to \(f\) and to each \(\pp f\) — gives \(h \in C^{1,\alpha}\), hence \(\zeta \in C^{2,\alpha}\) by Equation (A13.27). The change of coordinates then has continuous second derivatives, the extra term of Equation (14.7) is an honest continuous first-order coefficient, and the transformed equation is the third canonical form of Equation (14.10) in the classical sense.

Remark A13.18 (What has been gained, and what the classical argument gives).

For real-analytic coefficients the chapter's own construction is available and is much cheaper: complexify \(y\), integrate the characteristic ordinary differential equation Equation (14.13) along the complex branch, and take real and imaginary parts. That argument produces an analytic \(\zeta\) and needs nothing beyond existence for an analytic ordinary differential equation — which is the Cauchy–Kovalevskaya theorem Theorem 14.22 in its simplest instance. What it cannot do is survive the loss of analyticity, because a complexified non-analytic coefficient has no meaning at all. The route taken here never complexifies the coefficients: it complexifies only the unknown, which turns one real second-order equation into one complex first-order equation, and then solves that by inverting the constant-coefficient operator \(\pp_{\bar z}\) and treating the variable-coefficient part as a small perturbation. The price is Theorem A13.13, and the gain is that \(C^{1}\) coefficients suffice — which matters because the coefficients of a physical equation are material properties, measured and interpolated, and are never analytic for any reason a physicist could give.

Remark A13.19.

The Korn–Lichtenstein Theorem and the Elliptic Canonical Form discharges the obligation stated in Remark 14.14 and completes the elliptic branch of Proposition 14.13 in Partial Differential Equations. Its consequence for the chapter is that the trichotomy of Equation (14.10) is a statement about all elliptic operators with \(C^{1}\) coefficients and not only about the real-analytic ones, so that the invariance of type proved in Theorem 14.8 is matched by an equally general normal form. One honest limitation survives and is stated in Remark A13.2: at \(C^{\alpha}\) coefficients the normal form is a statement about the principal part alone, and the classical form with continuous lower-order coefficients costs one more derivative. The single quoted input is Theorem A13.13, delimited in Remark A13.14.