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11.1 Torsion and the variation of mass7B453010B5B8

7B453010B5B8

Throughout this chapter, $\omega $ is a Hermitian form on $X$. If $\omega $ were closed, Stokes' theorem would make the total Monge–Ampère mass $\int _ X(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n$ independent of the potential $u$. For a nonclosed Hermitian form this invariance can fail. Integration by parts expresses the mass of a smooth potential as a polynomial whose coefficients pair the potential with the complex Hessians of the powers of $\omega $, and polarization shows that the vanishing of these Hessians is also necessary for invariance. When they do not vanish, even smooth potentials of the same singularity type can have different masses, and the usual global comparison principle fails. The masses may nevertheless remain bounded, and whether they do depends only on the manifold, not on the chosen Hermitian form.

11.1.1 Integration by parts with a nonclosed formFD6E63098594

Integration by parts moves the complex Hessian of a function onto the form against which it is integrated. When that form is a power of a nonclosed $(1,1)$-form, its complex Hessian contains, besides the complex Hessian of the form itself, a quadratic term in its exterior derivative.

Lemma 11.1.2.3B0A8DD950AD For a smooth real function $f$ and a smooth form $T$ of bidegree $(n-1,n-1)$,

\[ \int _ X\mathrm{dd}^{\mathrm{c}}f\wedge T=\int _ X f\mathrm{dd}^{\mathrm{c}}T. \]

Proof. Since $\mathrm d^{\mathrm c}f$ is a one-form, $\mathrm{d}(\mathrm d^{\mathrm c}f\wedge T)=\mathrm{dd}^{\mathrm{c}}f\wedge T-\mathrm d^{\mathrm c}f\wedge \mathrm{d}T$, and Stokes' theorem gives the first equality in

\[ \int _ X\mathrm{dd}^{\mathrm{c}}f\wedge T =\int _ X\mathrm d^{\mathrm c}f\wedge \mathrm{d}T =\int _ X f\mathrm{dd}^{\mathrm{c}}T. \]

For the second, recall that the integral of $\mathrm d^{\mathrm c}\sigma $ vanishes for every form $\sigma $ of total degree $2n-1$, by Stokes' theorem for $\partial $ and $\bar\partial $. We apply this to $\sigma =f\, \mathrm{d}T$ and use $\mathrm d^{\mathrm c}\mathrm{d}=-\mathrm{d}\mathrm d^{\mathrm c}$. $\square$

Lemma 11.1.3.BF56C7366FC6 For a smooth real $(1,1)$-form $\theta $ and an integer $q\geq 1$,

\[ \mathrm{dd}^{\mathrm{c}}(\theta ^ q) =q\, \theta ^{q-1}\wedge \mathrm{dd}^{\mathrm{c}}\theta +q(q-1)\, \theta ^{q-2}\wedge \mathrm{d}\theta \wedge \mathrm d^{\mathrm c}\theta , \]

where the second term is omitted when $q=1$.

Proof. For $q=1$ there is nothing to prove. For $q\geq 2$, since $\theta $ has even degree, $\mathrm d^{\mathrm c}(\theta ^ q)=q\, \theta ^{q-1}\wedge \mathrm d^{\mathrm c}\theta $. Applying $\mathrm{d}$ and using again that $\theta ^{q-1}$ has even degree, we obtain

\[ \mathrm{d}\mathrm d^{\mathrm c}(\theta ^ q) =q(q-1)\, \theta ^{q-2}\wedge \mathrm{d}\theta \wedge \mathrm d^{\mathrm c}\theta +q\, \theta ^{q-1}\wedge \mathrm{d}\mathrm d^{\mathrm c}\theta . \]
$\square$

Thus the quadratic torsion term $\mathrm{d}\omega \wedge \mathrm d^{\mathrm c}\omega $ can make the higher powers of $\omega $ fail to be $\mathrm{dd}^{\mathrm{c}}$-closed even when $\mathrm{dd}^{\mathrm{c}}\omega =0$. The mass expansion below involves the complex Hessians of all these powers separately.

11.1.4 The mass polynomialCA97FF13B1BB

For a smooth real function $u$ on $X$, write $\omega _ u=\omega +\mathrm{dd}^{\mathrm{c}}u$, and set

\[ \mathcal H_\omega =\{ u\in C^\infty (X,\mathbb R):\omega +\mathrm{dd}^{\mathrm{c}}u>0\} , \qquad \mathrm M_\omega (u)=\int _ X(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n. \]

The set $\mathcal H_\omega $ of smooth strictly $\omega $-plurisubharmonic functions is convex and open in the $C^2$ topology, while the mass $\mathrm M_\omega (u)$ is defined for every smooth real $u$. Expanding it along a smooth direction gives a polynomial whose nonconstant coefficients detect the complex Hessians of the powers of the background.

Theorem 11.1.5.2B3316345A4A For every smooth real function $u$,

EB2FF7F930E4 11.1.6
\begin{equation} \mathrm M_\omega (u)=\int _ X\omega ^ n+ \sum _{k=1}^{n-1}\binom nk \int _ X u(\mathrm{dd}^{\mathrm{c}}u)^{k-1}\wedge \mathrm{dd}^{\mathrm{c}}(\omega ^{n-k}). \end{equation}

Proof. Expand $(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n$ by the binomial theorem. The term with $k=n$ integrates to zero, since it is exact:

\[ (\mathrm{dd}^{\mathrm{c}}u)^ n=\mathrm{d}\bigl (\mathrm d^{\mathrm c}u\wedge (\mathrm{dd}^{\mathrm{c}}u)^{n-1}\bigr ). \]

For $1\leq k\leq n-1$, apply lemma 11.1.2 with $f=u$ and $T=(\mathrm{dd}^{\mathrm{c}}u)^{k-1}\wedge \omega ^{n-k}$. Since both $\mathrm{d}$ and $\mathrm d^{\mathrm c}$ annihilate $\mathrm{dd}^{\mathrm{c}}u$,

\[ \mathrm{dd}^{\mathrm{c}}T=(\mathrm{dd}^{\mathrm{c}}u)^{k-1}\wedge \mathrm{dd}^{\mathrm{c}}(\omega ^{n-k}), \]

which gives the $k$th term of (11.1.6). When $n=1$, the sum is empty and the mass is constant. $\square$

If every $\mathrm{dd}^{\mathrm{c}}(\omega ^ j)$ with $1\leq j\leq n-1$ vanishes, (11.1.6) shows that the mass is constant. Conversely, varying the potential in several independent directions recovers each of these forms by polarization.

Theorem 11.1.7 (Chiose).FB90FC741F25 Assume $n\geq 2$. The following conditions are equivalent:

  1. $\int _ X(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n$ is independent of $u\in \mathcal H_\omega $;

  2. $\mathrm{dd}^{\mathrm{c}}(\omega ^ j)=0$ for $1\leq j\leq n-1$;

  3. $\mathrm{dd}^{\mathrm{c}}\omega =0$ and $\mathrm{d}\omega \wedge \mathrm d^{\mathrm c}\omega =0$.

They are also equivalent to the condition that $\int _ X(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n$ be the same for all bounded $\omega $-plurisubharmonic functions $u$, where $(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n$ is the Bedford–Taylor product of section 5.28. Under these conditions the common mass is $\int _ X\omega ^ n$.

Proof. Step 1: the first condition implies the second. Let $u$ be a smooth real function. For $|t|$ small, $tu$ belongs to $\mathcal H_\omega $ for both signs of $t$, so the polynomial $t\mapsto \int _ X(\omega +t\mathrm{dd}^{\mathrm{c}}u)^ n$ is constant on an interval and its nonconstant coefficients vanish. For $1\leq j\leq n-1$ this gives

\[ \int _ X\omega ^ j\wedge (\mathrm{dd}^{\mathrm{c}}u)^{n-j}=0. \]

Replace $u$ by a linear combination of $n-j$ smooth real functions $u_1,\ldots ,u_{n-j}$ and compare the coefficients of the monomial in which every parameter appears once. We obtain

\[ \int _ X\omega ^ j\wedge \mathrm{dd}^{\mathrm{c}}u_1\wedge \cdots \wedge \mathrm{dd}^{\mathrm{c}}u_{n-j}=0. \]

Integrating by parts in the first factor and using that $u_1$ is arbitrary, we obtain the pointwise identity

\[ \mathrm{dd}^{\mathrm{c}}(\omega ^ j)\wedge \mathrm{dd}^{\mathrm{c}}u_2\wedge \cdots \wedge \mathrm{dd}^{\mathrm{c}}u_{n-j}=0 \]

for every choice of the remaining functions. At a given point, the complex Hessians of these functions can be prescribed arbitrarily: multiply a quadratic polynomial in a coordinate chart by a cutoff function equal to one near that point. Since the identity is multilinear, we may complexify it and use the quadratic monomials $z_ a\bar z_ b$. Wedge products of their complex Hessians give all coordinate forms of the complementary bidegree, and pairing with these forms shows that every coefficient of $\mathrm{dd}^{\mathrm{c}}(\omega ^ j)$ vanishes. When $j=n-1$ there are no remaining factors, and the same conclusion follows directly from the arbitrariness of $u_1$. This proves the second condition.

Step 2: the remaining equivalences for smooth potentials. The second condition implies the first by theorem 11.1.5. For $n\geq 3$, the identities for $j=1,2$ and lemma 11.1.3 give $\mathrm{dd}^{\mathrm{c}}\omega =0$ and

\[ 0=\mathrm{dd}^{\mathrm{c}}(\omega ^2)=2\omega \wedge \mathrm{dd}^{\mathrm{c}}\omega +2\mathrm{d}\omega \wedge \mathrm d^{\mathrm c}\omega , \]

so the second condition implies the third. For $n=2$, the second condition is $\mathrm{dd}^{\mathrm{c}}\omega =0$, while $\mathrm{d}\omega \wedge \mathrm d^{\mathrm c}\omega $ vanishes for degree reasons; the implication is again immediate. Conversely, lemma 11.1.3 derives all the identities of the second condition from the third.

Step 3: bounded potentials. Assume the first condition and let $u$ be a bounded $\omega $-plurisubharmonic function. By theorem 5.32.1, there are uniformly bounded functions $u_ j\in \mathcal H_\omega $ decreasing to $u$. Their masses all equal $\int _ X\omega ^ n$, and the continuity of the bounded products of section 5.28 along such sequences passes this common value to the limit. Conversely, every element of $\mathcal H_\omega $ is a bounded $\omega $-plurisubharmonic function, so constancy for bounded potentials implies the first condition. The zero potential shows that the common mass is $\int _ X\omega ^ n$. $\square$

In particular, a closed background has invariant mass. Under the equivalent conditions above, (11.1.6) even gives $\mathrm M_\omega (u)=\int _ X\omega ^ n$ for every smooth real $u$, not only for $u\in \mathcal H_\omega $. In dimension one the mass is always $\int _ X\omega $.

Mass invariance can also hold in a nonclosed background. In theorem 12.18.15, a pluriclosed metric with nonzero exterior derivative satisfies all the lower-power identities above. Those identities fix its bounded-potential mass, even though a family of scalar perturbations can have its least relative eigenvalue tend to zero.

The first variation of the mass involves only the complex Hessian of the power $\omega _ u^{n-1}$ of the perturbed form.

Proposition 11.1.8.5C29873687ED For smooth real functions $u,v$ on $X$,

0B024E0A2A47 11.1.9
\begin{equation} \left.\frac{\mathrm{d}}{\mathrm{d}t}\right|_{t=0}\mathrm M_\omega (u+tv) =n\int _ X v\mathrm{dd}^{\mathrm{c}}(\omega _ u^{n-1}). \end{equation}

If $\mathrm M_\omega $ is constant on $\mathcal H_\omega $, then $\mathrm{dd}^{\mathrm{c}}(\omega _ u^{n-1})=0$ for every $u\in \mathcal H_\omega $.

Proof. Since $\mathrm M_\omega (u+tv)$ is a polynomial in $t$, its derivative at $t=0$ is

\[ n\int _ X\mathrm{dd}^{\mathrm{c}}v\wedge \omega _ u^{n-1}, \]

and lemma 11.1.2 turns this into the right-hand side of (11.1.9). For the second assertion, fix $u\in \mathcal H_\omega $. For every smooth real direction $v$, the segment $u+tv$ lies in $\mathcal H_\omega $ when $|t|$ is sufficiently small, so the right-hand side of (11.1.9) vanishes for all smooth real $v$. Hence the smooth top-degree form $\mathrm{dd}^{\mathrm{c}}(\omega _ u^{n-1})$ vanishes. $\square$

Corollary 11.1.10.2C05FFD39C6D If $n=2$, then for every smooth real function $u$ on $X$,

\[ \mathrm M_\omega (u)=\int _ X\omega ^2+2\int _ Xu\mathrm{dd}^{\mathrm{c}}\omega . \]

Consequently, $\mathrm M_\omega $ is constant on $\mathcal H_\omega $ if and only if $\mathrm{dd}^{\mathrm{c}}\omega =0$.

Proof. The formula is the case $n=2$ of (11.1.6), and it shows that $\mathrm{dd}^{\mathrm{c}}\omega =0$ implies constancy. Conversely, if the mass is constant, proposition 11.1.8 at $u=0$ gives $\mathrm{dd}^{\mathrm{c}}\omega =0$. $\square$

The identity $\mathrm{dd}^{\mathrm{c}}(\omega ^{n-1})=0$ makes the first variation vanish at $u=0$; Hermitian forms satisfying it are the Gauduchon metrics of section 11.3. On a surface this identity already gives mass invariance. In dimension three, however, (11.1.6) reads

\[ \mathrm M_\omega (u)=\int _ X\omega ^3 +3\int _ Xu\mathrm{dd}^{\mathrm{c}}(\omega ^2) +3\int _ Xu\mathrm{dd}^{\mathrm{c}}u\wedge \mathrm{dd}^{\mathrm{c}}\omega . \]

Vanishing of $\mathrm{dd}^{\mathrm{c}}(\omega ^2)$ removes the linear term, while $\mathrm{dd}^{\mathrm{c}}\omega $ still governs the quadratic term. Thus stationarity of the mass at one potential must be distinguished from its invariance on $\mathcal H_\omega $; an explicit example is given in example 11.23.5.

11.1.11 Mass variation on a complex torusD4D9C4F87D5D

By corollary 11.1.10, the mass on a surface varies precisely through the pairing $2\int _ Xu\mathrm{dd}^{\mathrm{c}}\omega $ of the potential with the complex Hessian of the background. A product of elliptic curves gives an explicit background and a family of smooth potentials for which this pairing is nonzero.

Example 11.1.12.F336FEED9D87 Let $X=(\mathbb C/(\mathbb Z+\mathrm i\mathbb Z))^2$. For $j=1,2$, let $z_ j=x_ j+\mathrm i y_ j$ be the standard coordinates on the universal cover $\mathbb C^2$, with $x_ j,y_ j$ real, and put

\[ \beta _ j=\frac{\mathrm i}{2\pi }\, \mathrm{d}z_ j\wedge \mathrm{d}\bar z_ j. \]

The forms $\beta _ j$ descend to $X$. For a real parameter $t$, define

\[ b(x_1)=2+\cos (2\pi x_1),\qquad \omega =\beta _1+b(x_1)\beta _2,\qquad u_ t=t\cos (2\pi x_1). \]

Since $1\leq b\leq 3$, the form $\omega $ is Hermitian. It is not closed, because $\mathrm{d}\omega =\mathrm{d}b\wedge \beta _2$ is not identically zero.

For a function $f$ of $x_1$ alone, one has $\mathrm{dd}^{\mathrm{c}}f=(f''/4)\beta _1$, where the prime denotes differentiation in $x_1$. Hence

\[ \omega _{u_ t} =\bigl (1-\pi ^2t\cos (2\pi x_1)\bigr )\beta _1+b\beta _2>0 \quad \text{if}\quad |t|<\pi ^{-2}. \]

Writing $B=\int _ X\beta _1\wedge \beta _2>0$, we have

914CB776FFB8 11.1.13
\begin{equation} \mathrm M_\omega (u_ t)=(4-\pi ^2t)B. \end{equation}

Indeed,

\[ \omega _{u_ t}^2 =2\bigl (1-\pi ^2t\cos (2\pi x_1)\bigr ) \bigl (2+\cos (2\pi x_1)\bigr )\beta _1\wedge \beta _2, \]

and over a period the average of $\cos (2\pi x_1)$ is zero while that of its square is $1/2$.

Although the complex torus is Kähler, the background $\omega $ chosen above is not closed, and this already allows the mass to vary. On non-Kähler manifolds even an upper bound for the mass can fail; the Hopf manifolds of section 23.1 give examples.

Corollary 11.1.14.0C9AAEBBC04C In general, the total Monge–Ampère mass is not determined by the ordinary singularity type or by the multiplier ideals, even among smooth strictly $\omega $-plurisubharmonic potentials.

Proof. The potentials $u_ t$ of example 11.1.12 are smooth on the compact manifold $X$, so any two of them differ by a bounded function and have the same singularity type in the sense of section 5.33. For the same reason, their multiplier ideals are the structure sheaf for every positive multiple of the weight. By (11.1.13), their masses differ. $\square$

11.1.15 Comparison and mass invarianceB5345EE28748

The global comparison principle of Kähler geometry compares the Monge–Ampère measures of two potentials on the set where one lies below the other. Adding a constant to a potential leaves its Monge–Ampère measure unchanged, and after a large constant shift this set becomes the whole manifold. Such an inequality would therefore compare total masses, and the varying mass of example 11.1.12 rules it out.

Proposition 11.1.16.2A8C104899E8 Suppose that every pair $u,v\in \mathcal H_\omega $ satisfies

F5F2F7988675 11.1.17
\begin{equation} \int _{\{ u<v\} }\omega _ v^ n \leq \int _{\{ u<v\} }\omega _ u^ n. \end{equation}

Then $\mathrm M_\omega $ is constant on $\mathcal H_\omega $.

Proof. Fix $u,v\in \mathcal H_\omega $. By compactness there is a constant $C$ such that $u<v+C$ everywhere. Since $\omega _{v+C}=\omega _ v$, applying (11.1.17) to $u$ and $v+C$ gives $\mathrm M_\omega (v)\leq \mathrm M_\omega (u)$. Exchanging the roles of $u$ and $v$ gives the opposite inequality. $\square$

Corollary 11.1.18.9578EA44189A The inequality (11.1.17) does not hold for every Hermitian form on a compact complex manifold.

Proof. Let $X$, $\omega $, $u_ t$ and $B=\int _ X\beta _1\wedge \beta _2$ be as in example 11.1.12. For $-\pi ^{-2}<t<0$, set $u=0$ and $v=u_ t+C$ with $C>|t|$. Then $\{ u<v\} =X$, but

\[ \int _ X\omega _ v^2=(4-\pi ^2t)B>4B=\int _ X\omega _ u^2. \]

Thus this pair violates (11.1.17). $\square$

The modified comparison principle of theorem 14.19.6 compensates for the derivatives of the background. Conversely, under the equivalent conditions of theorem 11.1.7, the ordinary comparison principle holds for bounded potentials, by 14.25.3.

11.1.19 Uniform mass boundsD29B5BFF0A9A

Although the mass varies, it may remain bounded. Set

\[ \overline{\mathrm v}_{\mathrm{sm}}(\omega )=\sup _{u\in \mathcal H_\omega }\mathrm M_\omega (u)\in (0,+\infty ], \]

the supremum of the masses of smooth strictly $\omega $-plurisubharmonic potentials. Comparing two Hermitian forms and rescaling the potentials shows that the finiteness of this supremum depends only on $X$.

Proposition 11.1.20.682711871907 If $\eta $ is another Hermitian form and $\omega \leq C\eta $ for a constant $C>0$, then

\[ \overline{\mathrm v}_{\mathrm{sm}}(\omega )\leq C^ n\overline{\mathrm v}_{\mathrm{sm}}(\eta ). \]

In particular, finiteness of $\overline{\mathrm v}_{\mathrm{sm}}$ is independent of the Hermitian form.

Proof. Let $u\in \mathcal H_\omega $. Since $C\eta +\mathrm{dd}^{\mathrm{c}}u\geq \omega +\mathrm{dd}^{\mathrm{c}}u>0$, the function $u/C$ belongs to $\mathcal H_\eta $. The top exterior power is monotone on positive $(1,1)$-forms: for positive Hermitian matrices $A\leq B$, all eigenvalues of $A^{-1/2}BA^{-1/2}$ are at least one, so $\det A\leq \det B$. Applying this pointwise gives

\[ \int _ X(\omega +\mathrm{dd}^{\mathrm{c}}u)^ n \leq C^ n\int _ X\bigl (\eta +\mathrm{dd}^{\mathrm{c}}(u/C)\bigr )^ n \leq C^ n\overline{\mathrm v}_{\mathrm{sm}}(\eta ). \]

Taking the supremum over $u$ proves the inequality. Since any two Hermitian forms on the compact manifold $X$ are comparable in both directions, the last assertion follows. $\square$

The smooth supremum considered here is also the upper mass over all bounded $\omega $-plurisubharmonic potentials: proposition 13.14.15 proves this using approximation by smooth strict potentials and continuity of bounded products. In section 13.14, we then pass to unbounded truncations. By corollary 13.14.19, finiteness of this common supremum is equivalent to finiteness of the extended non-pluripolar mass of every $\omega $-plurisubharmonic potential.

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