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16.16 Real Hessian bounds for Kähler envelopes20C85925F87F

20C85925F87F

A bounded metric Laplacian bounds the complex Hessian of a potential, by positivity, but the full real Hessian also contains the $(2,0)$ and $(0,2)$ parts, and bounding these requires a different argument. We now show that, for a Kähler background, the envelope of a finite minimum of $C^{1,1}$ obstacles is again $C^{1,1}$ (theorem 16.16.7). The main step is an a priori bound for the full real Hessian of the solutions of the penalized equation (lemma 16.16.1), obtained from the maximum principle applied to the largest eigenvalue of the real Hessian. Differentiating this eigenvalue twice produces positive third-derivative terms, and we keep them: they absorb the negative term that comes from differentiating its logarithm.

We first recall the covariant Hessian of a Riemannian metric. Let $g$ be a smooth Riemannian metric on $X$. For smooth vector fields $Y,Z,W$ on an open set $U\subset X$ let $\mathcal K_{Y,Z}(W)$ be the right side of the Koszul formula

\begin{align*} 2g(\nabla _ YZ,W)={}& Y\, g(Z,W)+Z\, g(Y,W)-W\, g(Y,Z)\\ & +g([Y,Z],W)-g([Y,W],Z)-g([Z,W],Y). \end{align*}

If $W$ is replaced by $\phi W$ for a smooth function $\phi $, the terms of $\mathcal K_{Y,Z}(\phi W)$ containing derivatives of $\phi $ cancel in pairs, so $\mathcal K_{Y,Z}(\phi W)=\phi \, \mathcal K_{Y,Z}(W)$. In a chart, therefore, $\mathcal K_{Y,Z}(W)=\sum _ sW^ s\mathcal K_{Y,Z}(\partial _ s)$, and since $g$ is nondegenerate there is a unique smooth vector field $\nabla _ YZ$ satisfying the Koszul formula for all $W$; by uniqueness, the vector fields obtained in different charts agree on overlaps. This is the Levi-Civita connection of $g$. Replacing $Y$ or $Z$ by $\phi Y$ or $\phi Z$ in the formula, the terms containing derivatives of $\phi $ cancel, respectively add up to $2(Y\phi )g(Z,W)$, so $\nabla _{\phi Y}Z=\phi \nabla _ YZ$ and $\nabla _ Y(\phi Z)=(Y\phi )Z+\phi \nabla _ YZ$; and interchanging $Y$ and $Z$ changes the right side by $-2g([Y,Z],W)$, so $\nabla _ YZ-\nabla _ ZY=[Y,Z]$.

In coordinates, with $g_{uv}=g(\partial _ u,\partial _ v)$, the Koszul formula for coordinate vector fields gives $\nabla _{\partial _ u}\partial _ v=\sum _ t\Gamma ^ t_{uv}\partial _ t$, where the Christoffel symbols are determined by $\sum _ tg_{st}\Gamma ^ t_{uv}=\frac12(\partial _ ug_{vs}+\partial _ vg_{us}-\partial _ sg_{uv})$; they are symmetric in $u$ and $v$ and vanish at a point where the first derivatives of the $g_{uv}$ vanish. For a smooth function $b$, the covariant Hessian $\nabla ^2b(Y,Z)=Y(Zb)-(\nabla _ YZ)b$ is, by these rules, given in coordinates by

\[ \nabla ^2b(Y,Z)=\sum _{u,v}Y^ uZ^ v\Bigl (\partial _ u\partial _ vb-\sum _ t\Gamma ^ t_{uv}\partial _ tb\Bigr ). \]

Hence $\nabla ^2b$ is a symmetric bilinear form on each tangent space, and at a point where the first derivatives of the metric vanish it is the matrix of second derivatives of $b$. If $g'$ is another smooth Riemannian metric, the difference $\nabla '_ YZ-\nabla _ YZ$ is linear over smooth functions in $Y$ and in $Z$, by the rules above, so the two covariant Hessians of $b$ differ by a smooth tensor applied to $\mathrm db$. For a $C^1$ function $b$ the same coordinate formula, with distributional second derivatives, defines the weak covariant Hessian.

Recall that a function is of class $C^{1,1}$ if it is $C^1$ and its first derivatives are locally Lipschitz in smooth real coordinates (proposition 2.8.5). On the compact manifold $X$ we measure such a function by the supremum norms of its value, its gradient and its weak covariant Hessian with respect to a fixed smooth Riemannian metric; the sum of these three norms is its $C^{1,1}$ norm.

The two descriptions agree: the first derivatives of a $C^1$ function are locally Lipschitz exactly when its weak second derivatives are locally bounded. Indeed, if a first derivative $\partial _ af$ is Lipschitz with constant $M$ on a coordinate ball, its difference quotients in a direction $e_ b$ are bounded by $M$; pairing them with a test function $\varphi $ and passing to the limit gives $|\langle \partial _ b\partial _ af,\varphi \rangle |\leq M\int |\varphi |\, \mathrm dx$. By corollary 2.8.2(1), $\partial _ b\partial _ af$ is therefore a bounded function, with $|\partial _ b\partial _ af|\leq M$. Conversely, by proposition 2.8.5, a continuous function whose weak second derivatives are bounded by $M$ on a ball has a gradient that is Lipschitz on this ball with constant $2nM$, the real dimension being $2n$. The Christoffel symbols of a metric and the derivatives of coordinate changes are bounded on compact subsets of the charts, and they multiply only first derivatives, so different smooth metrics give equivalent $C^{1,1}$ norms. In the applications below, the $C^1$ property of the envelope will be known in advance from proposition 16.14.9.

Lemma 16.16.1.C8D21E3D949A Let $\kappa $ be a Kähler form on $X$, and let $g_0$ be a smooth Riemannian metric on $X$ with Levi-Civita connection $\nabla $. Let $B>0$, and let $f$ be a smooth real function such that

\[ \| f\| _\infty +\| \nabla f\| _\infty \leq B, \qquad \nabla ^2f\leq Bg_0 \]

as real quadratic forms, and for $\beta >0$ let $a_\beta $ be the solution of (16.15.8) given by theorem 16.15.20. Then there are constants $\beta _0$ and $C$, depending only on $B$ and on the fixed geometry ($X$, $\kappa $ and $g_0$), such that

\[ \| a_\beta \| _\infty +\| \nabla a_\beta \| _\infty +\| \nabla ^2a_\beta \| _\infty \leq C \qquad (\beta \geq \beta _0). \]

Proof. Step 1 reduces to a metric defined by $\kappa $ and collects the bounds for $a_\beta $ and its gradient. Steps 2 and 3 apply the maximum principle to the logarithm of the largest eigenvalue of $\nabla ^2a_\beta $, corrected by functions of the gradient and of $a_\beta $, and Step 4 absorbs the negative term with third derivatives.

Step 1: reductions and first bounds. Any two smooth Riemannian metrics on $X$ are uniformly equivalent, and, as observed before the lemma, the Hessians of a function for the two metrics differ by a bounded tensor applied to its gradient. Changing $g_0$ therefore changes $B$ and the constants only by factors depending on the two metrics, and we may assume that $g_0$ is the following Riemannian metric defined by $\kappa $. In local holomorphic coordinates write $\kappa =\frac{\mathrm i}{2\pi }k_{i\bar j}\, \mathrm dz_ i\wedge \mathrm d\bar z_ j$, so that $k$ is the coefficient matrix of $2\pi \kappa $ as in section 16.15, and let $g_0=2\operatorname{Re}(k_{i\bar j}\, \mathrm dz_ i\otimes \mathrm d\bar z_ j)$; this is $2\pi $ times the Riemannian metric $\kappa (\cdot ,J\cdot )$, where $J$ is the complex structure. At the center of normal coordinates for $\kappa $, given by lemma 16.15.3, we have $k_{i\bar j}=\delta _{ij}$ and $\mathrm dk=0$; hence the Christoffel symbols of $g_0$ vanish and $g_0=2\sum _ i(\mathrm dx_ i^2+\mathrm dy_ i^2)$. Comparing coordinate derivatives at such a point, we obtain for every smooth function $b$

FA70E3BD3873 16.16.2
\begin{equation} \operatorname {tr}_{g_0}\nabla ^2b=2D_ kb, \qquad D_ kb=k^{i\bar j}b_{i\bar j}. \end{equation}

In particular the upper bound for $\nabla ^2f$ gives $D_ kf\leq nB$.

Write $a=a_\beta $, $G=(k_{i\bar j}+a_{i\bar j})$ and $D_ G=G^{i\bar j}\partial _ i\partial _{\bar j}$; thus $G$ is the matrix denoted $g$ in section 16.15. We apply lemma 16.15.7 with $\kappa $ also as the measuring metric. It bounds $|a|$ by $\| f\| _\infty $ and, for all sufficiently large $\beta $, bounds $\operatorname {tr}_ kG$ in terms of $B$ and the fixed geometry. Since $G>0$ and $\operatorname {tr}_ kG$ is bounded, all coefficients of $G$, and hence of the complex Hessian of $a$, are bounded; in particular the metric Laplacian $La$ for the fixed Kähler form $\omega $, which is a constant multiple of the trace of $\mathrm{dd}^{\mathrm{c}}a$ with respect to $\omega $ (lemma 10.2.12), is uniformly bounded. Fix $p>2n$. By proposition 16.14.9, $\| a\| _{W^{2,p}(X)}\leq C(\| La\| _{L^ p}+\| a\| _{L^ p})$ is uniformly bounded, and Morrey's inequality (lemma 2.9.16), applied in the charts defining the norm to the first derivatives of the products of $a$ with the cutoff functions, bounds $\nabla a$ uniformly. From now on $C$ denotes a constant depending only on these bounds, on $B$ and on the fixed geometry; it may increase from line to line, but it never depends on $\beta $.

Step 2: the auxiliary function. Let $\ell $ be the largest eigenvalue of the real covariant Hessian $\nabla ^2a$ with respect to $g_0$. By (16.16.2), the sum of all eigenvalues is $2D_ ka=2\operatorname {tr}_ kG-2n\geq -2n$. Since each eigenvalue is at most $\ell $, it is at least $-2n-(2n-1)\ell $; hence every eigenvalue of $\nabla ^2a$ has absolute value at most $2n(\max \{ \ell ,0\} +1)$. It therefore suffices to bound $\ell $ from above, and we do so by the maximum principle. Put

\[ s=|\partial a|_ k^2,\quad S=\sup _ Xs,\quad \tau =(1+2\sup _ X|\partial f|_ k^2)^{-1},\quad \eta (s)=-\frac\tau 2\log (1+S-s). \]

Then $S\leq C$, the number $\tau \in (0,1]$ has a uniform positive lower bound, and since $0\leq s\leq S$,

D5B65BED5E46 16.16.3
\begin{equation} \frac{\tau }{2(1+S)}\leq \eta '\leq \frac\tau 2, \qquad \eta ''=\frac{2(\eta ')^2}{\tau }\geq 2(\eta ')^2. \end{equation}

For a constant $A>0$ to be chosen later, consider the function $Q=\log \ell +\eta (s)-Aa$ on the open set $\{ \ell >0\} $. If this set is empty, then $\ell \leq 0$ and there is nothing to prove. Otherwise, since $a$ and $\eta (s)$ are bounded, $Q$ tends to $-\infty $ where $\ell $ tends to zero, so by compactness of $X$ it attains its maximum at some point $x_0$ with $\ell (x_0)>0$. For the same reason a uniform bound for $\ell (x_0)$ bounds $\ell $ on all of $X$. We may therefore assume that $\ell (x_0)\geq 1$, and that $\ell (x_0)$ exceeds any uniform threshold used below.

Choose normal coordinates for $\kappa $ at $x_0$ in which $G(x_0)$ is diagonal, with diagonal entries $r_ i>0$: by lemma 16.15.3, applied to $k$ in one of finitely many fixed charts that contains $x_0$ in a fixed compact subset, and followed by a unitary change of coordinates that diagonalizes $G(x_0)$, there are such coordinates in which the derivatives of $k$ of every fixed order at $x_0$ are bounded independently of $x_0$. Since $\sum _ ir_ i=\operatorname {tr}_ kG\leq C$, we have $r_ i\leq C$, hence $r_ i^{-1}\geq c$ for a uniform $c>0$. Write $T=\sum _ ir_ i^{-1}$; thus $T\geq c$. Take a $g_0$-orthonormal basis $V_1,\ldots ,V_{2n}$ of the real tangent space at $x_0$ consisting of eigenvectors of $\nabla ^2a(x_0)$, with $V_1$ belonging to the eigenvalue $\ell (x_0)$, and extend these vectors to the chart as vector fields with constant real coordinate coefficients.

The largest eigenvalue $\ell $ may be multiple and need not be smooth, so we perturb the Hessian. Let $B_0$ be the symmetric bilinear form with constant coefficients in this chart which at $x_0$ is the $g_0$-orthogonal projection onto $V_1^\perp $, that is, $B_0(Y,Z)=g_0(PY,PZ)$ at $x_0$ for this projection $P$, and set

\[ \Phi =g_0^{-1}(\nabla ^2a-B_0). \]

The form $B_0$ is positive semidefinite everywhere in the chart. Hence the largest eigenvalue $\lambda _1(\Phi )$ of $\Phi $ is at most $\ell $, and it equals $\ell $ at $x_0$. Denote the eigenvalues of $\Phi $ at $x_0$ by $\lambda =\ell (x_0),\lambda _2,\ldots ,\lambda _{2n}$, with eigenvectors $V_1,\ldots ,V_{2n}$. For $\alpha >1$, $\lambda _\alpha $ is the Hessian eigenvalue belonging to $V_\alpha $ minus one, so $\lambda -\lambda _\alpha \geq 1$. In particular $\lambda _1(\Phi )$ is a smooth function near $x_0$. Indeed, $\lambda $ is a simple root of the characteristic polynomial of $\Phi (x_0)$, so by the implicit function theorem the characteristic polynomial of $\Phi $ has, near $x_0$, exactly one root close to $\lambda $, and this root depends smoothly on the point; it equals $\lambda _1(\Phi )$, which is continuous as the maximum of $(\nabla ^2a-B_0)(Y,Y)$ over $g_0$-unit vectors $Y$, and it is a simple eigenvalue. The smooth function $\widehat Q=\log \lambda _1(\Phi )+\eta (s)-Aa$ satisfies $\widehat Q\leq Q\leq Q(x_0)=\widehat Q(x_0)$, so it has a local maximum at $x_0$.

Step 3: the inequality at the maximum point. From now on all quantities are evaluated at $x_0$. Write $a_{V_\alpha V_\gamma }=\nabla ^2a(V_\alpha ,V_\gamma )$, a smooth function near $x_0$, and define the nonnegative quantities

\begin{align*} U& =2\sum _{i,\alpha >1} \frac{|\partial _ i a_{V_\alpha V_1}|^2}{r_ i\lambda (\lambda -\lambda _\alpha )},& R& =\sum _{p,q}\frac{|V_1G_{p\bar q}|^2}{r_ pr_ q\lambda },\\ N& =\sum _ i\frac{|\partial _ i a_{V_1V_1}|^2}{r_ i\lambda ^2},& K& =\sum _{i,p}\frac{|a_{ip}|^2+|a_{i\bar p}|^2}{r_ i}. \end{align*}

We first compute $D_ G\log \lambda _1(\Phi )$, keeping the third-derivative terms. Let $M(t)$ be a smooth family of real symmetric matrices, and let $\lambda (t)$ be a simple eigenvalue with unit eigenvector $V_1$ at $t=0$, the other eigenvalues being $\lambda _\alpha $ with orthonormal eigenvectors $V_\alpha $. Then

\[ \lambda '=\langle M'V_1,V_1\rangle ,\qquad \lambda ''=\langle M''V_1,V_1\rangle +2\sum _{\alpha >1} \frac{|\langle M'V_1,V_\alpha \rangle |^2}{\lambda -\lambda _\alpha }. \]

Indeed, near $t=0$ the simple eigenvalue $\lambda (t)$ is a smooth function of $t$, by the implicit function theorem applied to the characteristic polynomial, and the columns of the adjugate matrix of $\lambda (t)I-M(t)$, which has rank one, span the eigenspace; normalizing a column that does not vanish at $t=0$ gives a smooth unit eigenvector $y(t)$ with $y(0)=\pm V_1$, and we may take the sign $+$. Differentiate the eigenvector equation $M(t)y(t)=\lambda (t)y(t)$. Pairing with $V_1$ gives the first formula, and pairing with $V_\alpha $ shows that the derivative of the eigenvector has component $\langle M'V_1,V_\alpha \rangle /(\lambda -\lambda _\alpha )$ along $V_\alpha $, and it has no component along $V_1$, because $|y(t)|=1$. Differentiating the identity $\lambda '(t)=\langle M'(t)y(t),y(t)\rangle $, where $y(t)$ is the normalized eigenvector with $y(0)=V_1$, and substituting these components gives the second formula.

We apply these formulas to the symmetric matrix $M$ with entries $(\nabla ^2a-B_0)(e_\alpha ,e_\gamma )$, where $e_1,\ldots ,e_{2n}$ is the $g_0$-orthonormal frame obtained from the constant vector fields $V_1,\ldots ,V_{2n}$ by the Gram–Schmidt process; $M$ has the same eigenvalues as $\Phi $. The frame depends smoothly on the point, equals $V_1,\ldots ,V_{2n}$ at $x_0$, and its first derivatives vanish at $x_0$, because those of $g_0$ do. We differentiate along the real coordinate directions and use $\partial _ i\partial _{\bar i}=\frac14(\partial _{x_ i}^2+\partial _{y_ i}^2)$. Since $B_0$ is constant, the first derivatives of $M$ at $x_0$ are those of the functions $\nabla ^2a(V_\alpha ,V_\gamma )$. In the second derivatives, the second derivatives of the frame multiply $\nabla ^2a-B_0$, which is bounded by $C(\lambda +1)$; after weighting with $r_ i^{-1}$ and summing they contribute at most $C\lambda T$. Since $|\partial _ ib|^2=\frac14(|\partial _{x_ i}b|^2+|\partial _{y_ i}b|^2)$ for a real function $b$, we obtain

\[ D_ G\lambda _1(\Phi )\geq 2\sum _{i,\alpha >1} \frac{|\partial _ i a_{V_\alpha V_1}|^2}{r_ i(\lambda -\lambda _\alpha )} +\sum _ i r_ i^{-1}V_1V_1G_{i\bar i}-C\lambda T. \]

Here the middle term comes from $\sum _ ir_ i^{-1}\partial _ i\partial _{\bar i}a_{V_1V_1}$ after commuting derivatives, and we check that this commutation costs at most $C\lambda T$. In real coordinates $a_{V_1V_1}=V_1V_1a-\Gamma ^ t_{uv}V_1^ uV_1^ v\partial _ ta$, where the Christoffel symbols $\Gamma $ of $g_0$ vanish at $x_0$. When we apply $\partial _ i\partial _{\bar i}$, the term containing third derivatives of $a$ is multiplied by $\Gamma (x_0)=0$; the remaining terms are a first derivative of $\Gamma $ times a second derivative of $a$, or a second derivative of $\Gamma $ times a first derivative of $a$. By the Hessian and gradient bounds above they are at most $C(\lambda +1)$. Moreover $\partial _ i\partial _{\bar i}V_1V_1a=V_1V_1a_{i\bar i}=V_1V_1G_{i\bar i}-V_1V_1k_{i\bar i}$, and the derivatives of the fixed matrix $k$ are bounded. Summing with the weights $r_ i^{-1}$ gives an error at most $C\lambda T$, and no third derivative of $a$ enters it.

Next we use the equation. Taking logarithms in (16.15.8) gives $\log \det G=\log \det k+\beta (a-f)$. Differentiating twice along $V_1$ and using $\partial (G^{-1})=-G^{-1}(\partial G)G^{-1}$, we obtain at $x_0$

\[ \sum _ i r_ i^{-1}V_1V_1G_{i\bar i} =\sum _{p,q}\frac{|V_1G_{p\bar q}|^2}{r_ pr_ q} +V_1V_1\log \det k+\beta (\lambda -f_{V_1V_1}). \]

Here we used that at the center of normal coordinates directional and covariant second derivatives agree, so that $V_1V_1a=\lambda $ and $V_1V_1f=f_{V_1V_1}$. If $\lambda \geq 2\max \{ 1,\sup _{X,|Y|_{g_0}=1}f_{YY}\} $, which is a uniform threshold because $\nabla ^2f\leq Bg_0$, the last term is at least $\beta \lambda /2$. The term $V_1V_1\log \det k$ is bounded, hence at least $-CT$ because $T\geq c$. By the first variation formula, $\partial _ i\lambda _1(\Phi )=\partial _ i a_{V_1V_1}$ at $x_0$. Since $D_ G\log \lambda _1=\lambda ^{-1}D_ G\lambda _1-\sum _ ir_ i^{-1}|\partial _ i\lambda _1|^2/\lambda ^2$, we conclude that

\[ D_ G\log \lambda _1(\Phi )\geq U+R-N-CT+\beta /2. \]

Next we differentiate the logarithmic equation once and apply the product rule to $s=k^{p\bar q}a_ pa_{\bar q}$. At $x_0$,

\[ \partial _ i\partial _{\bar i}s=\sum _ p\bigl (|a_{pi}|^2+|a_{p\bar i}|^2\bigr ) +2\operatorname{Re}\sum _ pa_{\bar p}\, \partial _ pa_{i\bar i} +(\partial _ i\partial _{\bar i}k^{p\bar q})a_ pa_{\bar q}. \]

The last term involves only the bounded gradient. In the middle term the third derivatives occur only in the contraction $\sum _ ir_ i^{-1}\partial _ pa_{i\bar i}=\partial _ p\log \det G=\beta (a_ p-f_ p)$, because $\mathrm dk(x_0)=0$; so we need no estimate for third derivatives. Weighting with $r_ i^{-1}$ and summing, we get

\[ D_ Gs\geq K-CT +2\beta \operatorname{Re}\sum _ p a_{\bar p}(a_ p-f_ p) \geq K-CT+\beta s-\beta |\partial f|_ k^2. \]

Also $D_ Ga=\sum _ ir_ i^{-1}(r_ i-1)=n-T$. At the local maximum $x_0$ we have $D_ G\widehat Q\leq 0$, where

\[ D_ G\widehat Q=D_ G\log \lambda _1(\Phi )+\eta 'D_ Gs +\eta ''\sum _ i\frac{|s_ i|^2}{r_ i}-AD_ Ga. \]

Since $0<\eta '\leq \frac12$ and $\eta '|\partial f|_ k^2\leq \frac\tau 2\sup _ X|\partial f|_ k^2\leq \frac14$, the three preceding estimates yield

E052CD3153AF 16.16.4
\begin{equation} 0\geq U+R-N+\eta 'K +\eta ''\sum _ i\frac{|s_ i|^2}{r_ i} +(A-C_0)T-An+\beta \eta 's+\beta /4, \end{equation}

where $C_0$ is a uniform constant that does not depend on $A$.

Step 4: absorption of the third-order term. It remains to absorb the negative term $-N$ completely. Fix $0<\varepsilon <1/2$, to be chosen below, and assume that $\lambda \geq C/\varepsilon ^2$. Let $J$ be the complex structure of $X$, and define a $(1,0)$-vector $W$ and real numbers $\mu _\alpha $ by

\[ W=(V_1-\mathrm iJV_1)/\sqrt2 =\sum _ q\nu _ q\partial _ q,\qquad JV_1=\sum _{\alpha >1}\mu _\alpha V_\alpha . \]

Since $k(x_0)$ is the identity, $\sum _ q|\nu _ q|^2=g_0(V_1,V_1)=1$; since $JV_1$ is a $g_0$-unit vector orthogonal to $V_1$, also $\sum _{\alpha >1}\mu _\alpha ^2=1$. The coefficients $\nu _ q,\mu _\alpha $, and $J$ itself, are constant in our coordinate system.

Writing $V_1=\sqrt2\, \overline W-\mathrm iJV_1$ in the outer derivative of $\partial _ ia_{V_1V_1}$, we obtain

AADD4CDBAE91 16.16.5
\begin{equation} \partial _ i a_{V_1V_1} =\sqrt2\sum _ q\overline\nu _ q V_1G_{i\bar q} -\mathrm i\sum _{\alpha >1}\mu _\alpha \partial _ i a_{V_1V_\alpha }+E_ i, \qquad |E_ i|\leq C. \end{equation}

Indeed, the third coordinate derivatives of the scalar function $a$ commute, and $\partial _ i\overline W=\sum _ q\overline\nu _ q\partial _ i\partial _{\bar q}$. Replacing coordinate second derivatives by covariant ones before the last differentiation introduces only first derivatives of $\Gamma $ times the bounded gradient of $a$, since $\Gamma (x_0)=0$; and the derivatives of the fixed matrix $k$ are bounded. Thus the error $E_ i$ involves only the gradient bound.

We use twice the inequality $|b+c|^2\leq (1+t)|b|^2+(1+t^{-1})|c|^2$, $t>0$. First take $t=\varepsilon /(1-2\varepsilon )$ to separate $E_ i$; then $(1-2\varepsilon )(1+t)=1-\varepsilon $ and $(1-2\varepsilon )(1+t^{-1})\leq \varepsilon ^{-1}$, so the contribution of $E_ i$ to $(1-2\varepsilon )N$ is at most $CT/(\varepsilon \lambda ^2)\leq T$. Then take $t=\varepsilon $ for the two principal terms (with the factor $1+\varepsilon $ on the second one). This gives

\begin{align*} (1-2\varepsilon )N\leq {}& (1-\varepsilon )(1+\varepsilon ^{-1}) \sum _ i\frac{2|\sum _ q\overline\nu _ q V_1G_{i\bar q}|^2}{r_ i\lambda ^2}\\ & +(1-\varepsilon ^2) \sum _ i\frac{|\sum _{\alpha >1}\mu _\alpha \partial _ i a_{V_1V_\alpha }|^2}{r_ i\lambda ^2}+T. \end{align*}

By the weighted Cauchy–Schwarz inequality and $\sum _ qr_ q|\nu _ q|^2\leq C$, the first line is at most $CR/(\varepsilon \lambda )\leq R$. For the second line the Cauchy–Schwarz inequality and $\sum _{\alpha >1}\mu _\alpha ^2=1$ give

\[ \left|\sum _{\alpha >1}\mu _\alpha \partial _ i a_{V_1V_\alpha }\right|^2 \leq \left(\lambda -\sum _{\alpha >1}\lambda _\alpha \mu _\alpha ^2\right) \sum _{\alpha >1} \frac{|\partial _ i a_{V_1V_\alpha }|^2}{\lambda -\lambda _\alpha }. \]

To bound the first factor we use the positivity of $G$. Since the Hessian eigenvalue of $V_\alpha $ is $\lambda _\alpha +1$ (this is where the perturbation by $B_0$ enters) and $\partial \bar\partial a(W,\overline W)=\frac12\bigl (a_{V_1V_1}+a_{JV_1JV_1}\bigr )$ at $x_0$, we have

\[ 0<G(W,\overline W) =1+\tfrac 12\left(\lambda + \sum _{\alpha >1}(\lambda _\alpha +1)\mu _\alpha ^2\right). \]

Thus $\lambda -\sum _{\alpha >1}\lambda _\alpha \mu _\alpha ^2\leq 2\lambda +3$. If $\lambda \geq 3/(2\varepsilon ^2)$, then $(1-\varepsilon ^2)(2\lambda +3)\leq 2\lambda $, so the second line is at most $U$. Finally, the critical point equation for $\widehat Q$ at $x_0$ reads

\[ \frac{\partial _ i a_{V_1V_1}}\lambda =Aa_ i-\eta 's_ i. \]

Together with $|b+c|^2\leq 2|b|^2+2|c|^2$ and $4\varepsilon <2$, it bounds the remaining part of $N$:

\[ 2\varepsilon N\leq 4\varepsilon A^2\sum _ i\frac{|a_ i|^2}{r_ i}+2(\eta ')^2\sum _ i\frac{|s_ i|^2}{r_ i}. \]

Combining the three bounds, we obtain

25C8519515AD 16.16.6
\begin{equation} N\leq U+R+T+4\varepsilon A^2\sum _ i\frac{|a_ i|^2}{r_ i} +2(\eta ')^2\sum _ i\frac{|s_ i|^2}{r_ i}. \end{equation}

Now choose $A=C_0+3$, after enlarging $C_0$ so that it is positive, and $\varepsilon =[4A^2(S+1)]^{-1}<1/2$. Both choices are uniform, and so are the thresholds for $\lambda $ used above. By (16.16.3), the $\eta ''$ term of (16.16.4) absorbs the last term of (16.16.6), and $4\varepsilon A^2\sum _ i|a_ i|^2/r_ i\leq sT/(S+1)\leq T$. Substituting (16.16.6) into (16.16.4) and dropping its nonnegative $\beta $ terms, we get

\[ 0\geq \eta 'K+T-An. \]

By the lower bound for $\eta '$ in (16.16.3) and $r_ i^{-1}\geq c$, this bounds every $a_{ip}$ and $a_{i\bar p}$ at $x_0$, and hence every real second derivative of $a$ there; at $x_0$ these coincide with the covariant ones. Thus $\lambda =\ell (x_0)$ is uniformly bounded, either by the thresholds assumed above or by this estimate. As observed at the beginning, the maximum property of $Q$ then bounds $\ell $ everywhere, and the lower bound for the trace bounds the remaining eigenvalues of $\nabla ^2a$. This proves the lemma. $\square$

Theorem 16.16.7.4B6432E0991B Let $\kappa $ be a Kähler form on $X$, let $r\geq 1$ be an integer, and let $f_1,\ldots ,f_ r$ be real $C^{1,1}$ functions on $X$. Then the envelope

\[ P_\kappa \bigl (\min _{1\leq j\leq r}f_ j\bigr ) \]

is $C^{1,1}$. Its $C^{1,1}$ norm is bounded by a constant depending only on the fixed geometry and on a common bound for the $C^{1,1}$ norms of the obstacles.

Proof. First let $r=1$, and suppose that $f=f_1$ is smooth. By lemma 16.16.1, the solutions $a_\beta $ have uniformly bounded values, gradients and full real Hessians for $\beta \geq \beta _0$, and by proposition 16.15.21 they converge uniformly to $P_\kappa (f)$. The limit $P_\kappa (f)$ is therefore continuous, and by the same proposition it has bounded metric Laplacian; hence it belongs to $C^{1,\alpha }(X)$ by proposition 16.14.9, and in particular it is $C^1$.

We now pass to the limit in the Hessian bounds. For a smooth vector field $Y$, the function $\nabla ^2a_\beta (Y,Y)=YYa_\beta -(\nabla _ YY)a_\beta $ is obtained from $a_\beta $ by a second-order differential operator. Since $a_\beta \to P_\kappa (f)$ uniformly, $\nabla ^2a_\beta (Y,Y)\to \nabla ^2P_\kappa (f)(Y,Y)$ in the sense of distributions, where the right side is the weak covariant Hessian, and for every nonnegative test function $\varphi $ we obtain $|\langle \nabla ^2P_\kappa (f)(Y,Y),\varphi \rangle |\leq C\int |Y|_{g_0}^2\varphi $. By corollary 2.8.2(1), the weak quadratic components $\nabla ^2P_\kappa (f)(Y,Y)$ are bounded functions, with $|\nabla ^2P_\kappa (f)(Y,Y)|\leq C|Y|_{g_0}^2$ almost everywhere; by polarization, so are all components of the weak covariant Hessian.

The gradient is treated in the same way: $Ya_\beta \to YP_\kappa (f)$ in the sense of distributions, and $|Ya_\beta |\leq C|Y|_{g_0}$; since $YP_\kappa (f)$ is continuous, pairing with nonnegative test functions of integral one supported in small balls about a point shows that $|YP_\kappa (f)|\leq C|Y|_{g_0}$ everywhere, so $|\nabla P_\kappa (f)|_{g_0}\leq C$. In a chart, the weak second derivatives of $P_\kappa (f)$ differ from the components of its weak covariant Hessian by the Christoffel symbols times its first derivatives, so they are bounded on compact subsets of the chart. Hence $P_\kappa (f)$ is $C^{1,1}$, by proposition 2.8.5, and the bounds just proved show that its $C^{1,1}$ norm is bounded by a constant depending only on the fixed geometry and on the constant $B$ of lemma 16.16.1 for $f$.

Now let the $f_ j$ be arbitrary $C^{1,1}$ functions. Using convolution in finitely many charts and a smooth partition of unity, we obtain smooth functions $f_{j,\rho }$ that converge to $f_ j$ in $C^1$ as $\rho \to 0$ and have uniformly bounded covariant Hessians. Indeed, the second derivatives of such a partitioned convolution are the cutoffs times the convolutions of the bounded weak second derivatives of $f_ j$, plus terms that involve only the values and first derivatives of the local convolutions; all of these are uniformly bounded. For $\delta >0$ put

\[ F_{\rho ,\delta }=-\delta \log \sum _ j \mathrm e^{-f_{j,\rho }/\delta }, \qquad p_ j=\frac{\mathrm e^{-f_{j,\rho }/\delta }}{\sum _ k\mathrm e^{-f_{k,\rho }/\delta }}. \]

The weights $p_ j$ are positive with sum one, $\min _ jf_{j,\rho }-\delta \log r\leq F_{\rho ,\delta }\leq \min _ jf_{j,\rho }$, and the gradient of $F_{\rho ,\delta }$ is the convex combination $\sum _ jp_ j\nabla f_{j,\rho }$. For every real tangent vector $Y$ the chain rule gives

\begin{align*} \nabla ^2F_{\rho ,\delta }(Y,Y) & =\sum _ jp_ j\nabla ^2f_{j,\rho }(Y,Y)\\ & \quad -\frac1\delta \left(\sum _ jp_ j(\mathrm df_{j,\rho }(Y))^2 -\left(\sum _ jp_ j\mathrm df_{j,\rho }(Y)\right)^2\right)\\ & \leq C|Y|_{g_0}^2, \end{align*}

because the term in parentheses is a variance and hence nonnegative. Let $\rho ,\delta \to 0$ with $\delta \log r\leq 1$. Then the smooth obstacles $F_{\rho ,\delta }$ have uniformly bounded values and gradients and a uniform upper bound for their Hessians, although their Hessians have no uniform lower bound as $\delta \to 0$; this is why lemma 16.16.1 uses only an upper bound. Since the smooth case bounds the $C^{1,1}$ norm of the envelope in terms of the fixed geometry and the constant $B$ of that lemma, the envelopes $P_\kappa (F_{\rho ,\delta })$ have uniformly bounded $C^{1,1}$ norms. The obstacles converge uniformly to $\min _ jf_ j$, so the envelopes converge uniformly to $P_\kappa (\min _ jf_ j)$ by the stability estimate of proposition 16.11.4(4). The limit is $C^1$ by theorem 16.15.24, since $C^{1,1}$ functions have bounded metric Laplacian. The same passage to the limit as in the smooth case, with the smooth functions $a_\beta $ replaced by the $C^{1,1}$ functions $P_\kappa (F_{\rho ,\delta })$, whose gradients and weak covariant Hessians are bounded by a uniform constant, now proves the theorem, together with the bound for the norm. $\square$

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