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12.14 Positive volume without bignessE4AB7B03C20D

E4AB7B03C20D

By corollary 12.2.4, every big background has positive volume. For a closed nef class on a compact Kähler manifold the converse also holds: the volume is then $\int _ X\theta ^ n$, and a closed nef class with positive top self-intersection is big. We now show that the converse fails for nonclosed nef backgrounds, even on a projective manifold: such a background can have positive volume without containing a Kähler current. In the example, the coefficient of a fiber direction vanishes at one point of the base. A radial potential on the base compensates for this vanishing, and the determinant of the resulting current bounds every Gauduchon quotient from below. Bigness, on the other hand, is excluded by pairing with a closed semipositive form concentrated near the vanishing point.

Throughout this section fix an integer $m\geq 2$, and put $n=m+1$, $t=(m-1)/m$ and $B=\mathbb P^ m$. Give $B$ and $\mathbb P^1$ their Fubini–Study forms $\omega $ and $w$, normalized by $\int _ B\omega ^ m=\int _{\mathbb P^1}w=1$. On $B$ define

\[ x([Z_0:\cdots :Z_ m])= \frac{\sum _{j=1}^ m|Z_ j|^2}{\sum _{j=0}^ m|Z_ j|^2}, \qquad a=x/t,\qquad p=[1:0:\cdots :0]. \]

Thus $x$ is a smooth function on $B$ with values in $[0,1]$; it vanishes only at $p$ and equals one on the hyperplane $\{ Z_0=0\} $. On $X=B\times \mathbb P^1$, with pullbacks understood, set

\[ h=\omega +w,\qquad \mu =\omega ^ m\wedge w, \qquad \theta =\omega +a w. \]

For $\epsilon >0$ put

71973446DB97 12.14.1
\begin{equation} H_\epsilon =m\int _0^1\frac{y^{m-1}}{y/t+\epsilon }\, \mathrm{d}y. \end{equation}

Lemma 12.14.2.C0A6E438A11D There are smooth real functions $\varphi _\epsilon $ on $B$ such that $A_\epsilon =\omega +\mathrm{dd}^{\mathrm{c}}\varphi _\epsilon >0$ and

471F6FE31EB0 12.14.3
\begin{equation} A_\epsilon ^ m=\frac{\omega ^ m}{H_\epsilon (a+\epsilon )}. \end{equation}

As $\epsilon \downarrow 0$ they converge uniformly to a bounded continuous function $\varphi \in \mathrm{PSH}(B,\omega )$ that is smooth on $B\setminus \{ p\} $. On $B\setminus \{ p\} $ the current $A=\omega +\mathrm{dd}^{\mathrm{c}}\varphi $ is a smooth strictly positive form satisfying

C34D8558189E 12.14.4
\begin{equation} A^ m=a^{-1}\omega ^ m. \end{equation}

Moreover $H_\epsilon \to 1$ as $\epsilon \downarrow 0$.

Proof. In the affine chart $Z_0=1$, write $s=|z|^2$. Then $x=s/(1+s)$ and $\omega =\mathrm{dd}^{\mathrm{c}}\log (1+s)$. Polar integration gives

8523C0528005 12.14.5
\begin{equation} \int _ B b(x)\omega ^ m=m\int _0^1 b(y)y^{m-1}\, \mathrm{d}y \end{equation}

for every integrable function $b$ on $[0,1]$, since the normalized radial density of $\omega ^ m$ in the variable $s$ is $m s^{m-1}(1+s)^{-m-1}\, \mathrm{d}s$. In particular $\int _ B a^{-1}\omega ^ m=mt/(m-1)=1$, and monotone convergence in (12.14.1) gives $H_\epsilon \to 1$.

Define $q_\epsilon \geq 0$ and $\varphi _\epsilon $ on $[0,1]$ by

\[ q_\epsilon (x)^ m=\frac m{H_\epsilon } \int _0^ x\frac{y^{m-1}}{y/t+\epsilon }\, \mathrm{d}y, \qquad \varphi _\epsilon (x)=\int _0^ x \frac{q_\epsilon (y)-y}{y(1-y)}\, \mathrm{d}y. \]

Near zero,

\[ q_\epsilon (x)=x\left(\frac m{H_\epsilon } \int _0^1\frac{u^{m-1}}{xu/t+\epsilon }\, \mathrm{d}u\right)^{1/m}, \]

so $q_\epsilon $ is $x$ times a smooth positive function; moreover $q_\epsilon (1)=1$. Hence both apparent singularities of $\varphi _\epsilon '$, at $0$ and at $1$, are removable, and $\varphi _\epsilon $ is smooth on $[0,1]$. Composing with the smooth function $x$ gives a smooth function on $B$, again denoted $\varphi _\epsilon $.

To compute $A_\epsilon $, recall that for a local potential of the form $F(s)$, with $q=sF'(s)$, the complex Hessian has the tangential eigenvalue $q/s$, of multiplicity $m-1$, and the radial eigenvalue $\mathrm{d}q/\mathrm{d}s$. For $F_\epsilon =\log (1+s)+\varphi _\epsilon (x)$ one finds $sF_\epsilon '=q_\epsilon (x)$. Differentiating the integral defining $q_\epsilon $ shows that both eigenvalues are positive, also at $s=0$ by the smooth factorization above. Their product relative to the Fubini–Study determinant is

\[ \frac{A_\epsilon ^ m}{\omega ^ m} =\frac{q_\epsilon ^{m-1}q_\epsilon '}{x^{m-1}} =\frac1{H_\epsilon (a+\epsilon )}. \]

At a point of the hyperplane $\{ Z_0=0\} $, the smooth form $A_\epsilon $ is semipositive, as a limit of the positive matrices in the affine chart. Since the determinant just computed extends there with a strictly positive value, every eigenvalue is positive. This proves strict positivity on all of $B$ and (12.14.3).

We now pass to the limit. For $x>0$, $q_\epsilon (x)$ tends to $x^ t$. To bound $q_\epsilon $ uniformly, note that $q_\epsilon ^ m$ is the distribution function of the probability density $\frac{m}{H_\epsilon }\frac{y^{m-1}}{y/t+\epsilon }$ on $[0,1]$. Relative to the probability density $my^{m-1}$, this density has a decreasing weight; relative to $(m-1)y^{m-2}$, its weight is proportional to $y/(y+t\epsilon )$ and hence increasing. If one probability density on $[0,1]$ has a decreasing weight relative to another, its average weight on $[0,x]$ is at least one and its distribution function is the larger of the two; an increasing weight reverses the inequality. Consequently

\[ x^ m\leq q_\epsilon (x)^ m\leq x^{m-1}, \qquad \text{that is,}\qquad x\leq q_\epsilon (x)\leq x^ t. \]

The function

\[ \varphi (x)=\int _0^ x\frac{y^ t-y}{y(1-y)}\, \mathrm{d}y \]

is bounded and continuous on $[0,1]$, since $t>0$, and smooth on $(0,1]$; its derivative extends smoothly at one. The integrable function $(y^ t-y)/[y(1-y)]$ dominates the derivatives of the functions $\varphi _\epsilon $, so dominated convergence gives uniform convergence $\varphi _\epsilon \to \varphi $ on $B$. Distributional convergence shows that $A$ is a closed positive current. On each coordinate chart, a smooth local potential of $\omega $ plus $\varphi $ is a uniform limit of the corresponding plurisubharmonic functions built with $\varphi _\epsilon $, including at $p$. Hence $\varphi $ is $\omega $-plurisubharmonic. Off $p$, the limit $q=x^ t$ gives

\[ \frac{A^ m}{\omega ^ m} =\frac{(x^ t)^{m-1}t x^{t-1}}{x^{m-1}}=\frac tx=\frac1a. \]

Smoothness of $\varphi $ off $p$ and the same determinant argument at the hyperplane $\{ Z_0=0\} $ prove (12.14.4). $\square$

Theorem 12.14.6.ECAB6BFB33FD The background $\theta $ on $X$ is smooth, semipositive, nef and nonclosed. It is not big, but

3D231D52B18A 12.14.7
\begin{equation} \lambda _\mu (\theta )=n^{1/n},\qquad \mathcal V_\mu (\theta )=n. \end{equation}

For $\theta _\epsilon =\omega +(a+\epsilon )w$, one has

\[ \mathcal V_\mu (\theta _\epsilon )=\frac n{H_\epsilon }, \]

and the smooth positive metrics

F9FEC7FAC55E 12.14.8
\begin{equation} \gamma _\epsilon =(a+\epsilon )^{-1/m} \bigl (A_\epsilon +(a+\epsilon )w\bigr ) \end{equation}

are balanced and minimize the defining quotient at $\theta _\epsilon $.

Proof. The coefficient $a$ is nonnegative, and $\theta +\eta h>0$ for every $\eta >0$; this proves semipositivity and nefness. Since $a$ is nonconstant, $\mathrm{d}\theta =\mathrm{d}a\wedge w\ne 0$.

Suppose that $\theta +\mathrm{dd}^{\mathrm{c}}v\geq \delta h$ for a quasi-plurisubharmonic function $v$ and some $\delta >0$. Choose a nonzero smooth function $f\geq 0$ on $B$ supported in $\{ a<\delta \} $. Its pullback $S=f\omega ^ m$ is a smooth semipositive $(m,m)$-form, closed because it has top degree on the base. Positivity and distributional Stokes would give

\[ 0\leq \int _ X(\theta +\mathrm{dd}^{\mathrm{c}}v-\delta h)\wedge S =\int _ B f(a-\delta )\omega ^ m<0. \]

This contradiction shows that $\theta $ is not big, since every Hermitian form on $X$ dominates a positive multiple of $h$.

For the lower bound on the volume, pull back the bounded potential $\varphi $ of lemma 12.14.2. The positive current $\Omega =A+a w=\theta +\mathrm{dd}^{\mathrm{c}}\varphi $ is a smooth strictly positive form off $Z=\{ p\} \times \mathbb P^1$, where

\[ \Omega ^ n=n a A^ m\wedge w=n\mu . \]

Let $\gamma $ be a Gauduchon metric. Since $\varphi $ is bounded, distributional Stokes lets us replace $\theta $ by $\Omega $ in the numerator of its quotient. The set $Z$ has zero smooth volume and $\Omega \wedge \gamma ^{n-1}$ is a positive measure, so the pointwise arithmetic–geometric mean inequality off $Z$ gives

\[ \int _ X\theta \wedge \gamma ^{n-1} \geq n^{1/n}\int _ X (\mu /\gamma ^ n)^{1/n}\gamma ^ n =n^{1/n}D_\mu (\gamma ). \]

This lower bound holds for every test in definition 12.2.1; no power of the current $\Omega $ along $Z$ is needed.

For the upper bound, put $c_\epsilon =n/H_\epsilon $ and $\Omega _\epsilon =A_\epsilon +(a+\epsilon )w=\theta _\epsilon +\mathrm{dd}^{\mathrm{c}}\varphi _\epsilon $. Then $\Omega _\epsilon ^ n=c_\epsilon \mu $. The metrics in (12.14.8) satisfy

\[ T_\epsilon =\gamma _\epsilon ^ m =(a+\epsilon )^{-1}A_\epsilon ^ m +m A_\epsilon ^{m-1}\wedge w. \]

The first term has top degree on the base and the second is a product of closed forms, so $T_\epsilon $ is closed; that is, $\gamma _\epsilon $ is balanced, and in particular Gauduchon. Smooth Stokes and (12.14.5) give

\[ \int _ X\theta _\epsilon \wedge T_\epsilon =c_\epsilon \int _ X(a+\epsilon )^{-1}\mu =n, \qquad D_\mu (\gamma _\epsilon )=c_\epsilon ^{m/n}H_\epsilon , \]

so the quotient of $\gamma _\epsilon $ at $\theta _\epsilon $ equals $c_\epsilon ^{1/n}$. The same arithmetic–geometric mean argument, applied to the smooth representative $\Omega _\epsilon $, bounds every Gauduchon quotient at $\theta _\epsilon $ below by $c_\epsilon ^{1/n}$. This proves that $\gamma _\epsilon $ minimizes, and gives the formula for $\mathcal V_\mu (\theta _\epsilon )$. Since $\theta \leq \theta _\epsilon $, the metrics $\gamma _\epsilon $, used as tests for $\theta $, also give $\lambda _\mu (\theta )\leq c_\epsilon ^{1/n}$. Letting $\epsilon \downarrow 0$ proves (12.14.7). By theorem 12.11.1, this value is also the limit of the volumes of the Hermitian perturbations $\theta +\epsilon h$. $\square$

The value $n$ refers to the probability measure $\mu $ fixed above, but positivity holds for every smooth positive probability measure by proposition 12.15.1. Thus positive volume does not characterize bigness for nonclosed nef backgrounds, even on a projective manifold. The construction needs $m\geq 2$, so that $t>0$ and the endpoint potential is bounded; it says nothing about surfaces, or about closed nef classes on general compact complex manifolds.

12.14.9 Volume tests and threshold testsB51E860FD3F7

Two quotients are formed from the same pairing $\int _ X\theta \wedge \gamma ^{n-1}$. The volume quotient divides it by the determinant integral $D_\mu (\gamma )$, whereas the linear threshold $\kappa _ h(\theta )$ of corollary 11.6.2 divides it by the trace $\int _ Xh\wedge \gamma ^{n-1}$. This threshold is positive exactly when $\theta $ is big, and we call it the bigness threshold; for the pseudoeffective but nonbig background $\theta $ of theorem 12.14.6 it vanishes. The same metrics can approach both infima, but need not do so. In the radial model, the volume-minimizing metrics approach the bigness threshold only in dimension three, while a second family of smooth balanced metrics approaches it in every dimension by concentrating on the fiber over $p$.

Keep the data of theorem 12.14.6, and put

\[ T_\epsilon =\gamma _\epsilon ^ m,\qquad I_\epsilon =\int _ B(a+\epsilon )^{-2}\omega ^ m, \qquad M_\epsilon =m+I_\epsilon /H_\epsilon , \qquad g_\epsilon =M_\epsilon ^{-1/m}\gamma _\epsilon . \]

Write $Z=\{ p\} \times \mathbb P^1$. Its integration current $[Z]$ satisfies $\int _ Zh=1$ and annihilates $\theta $, since $\theta |_ Z=a(p)w=0$.

Proposition 12.14.10.0E9506DB4E70 The metrics $g_\epsilon $ are balanced, satisfy $\int _ Xh\wedge g_\epsilon ^ m=1$, and

662BE6BF9C61 12.14.11
\begin{equation} \int _ X\theta \wedge g_\epsilon ^ m =\frac{n-\epsilon I_\epsilon /H_\epsilon }{M_\epsilon }, \qquad D_\mu (g_\epsilon ) =\frac{(n/H_\epsilon )^{m/n}H_\epsilon }{M_\epsilon }. \end{equation}

Their volume quotients tend to $n^{1/n}$ as $\epsilon \downarrow 0$. If $n=3$, then $g_\epsilon ^2$ converges weakly to $[Z]$, and

F4D7155E150D 12.14.12
\begin{equation} \int _ X\theta \wedge g_\epsilon ^2 \sim \frac6{\log (1/\epsilon )}, \qquad D_\mu (g_\epsilon ) \sim \frac{2\, 3^{2/3}}{\log (1/\epsilon )}. \end{equation}

If $n\geq 4$, put $M_0=m+(m-1)^2/[m(m-2)]$. Then

\[ \int _ X\theta \wedge g_\epsilon ^ m\longrightarrow \frac n{M_0}>0, \qquad D_\mu (g_\epsilon )\longrightarrow \frac{n^{m/n}}{M_0}>0. \]

Thus this family approaches the bigness threshold, which is zero, exactly when $n=3$.

Proof. By the power formula in the proof of theorem 12.14.6 and (12.14.3),

\[ T_\epsilon =\frac{\omega ^ m}{H_\epsilon (a+\epsilon )^2} +mA_\epsilon ^{m-1}\wedge w. \]

Since $A_\epsilon $ is cohomologous to $\omega $, closed Stokes gives $\int _ B\omega \wedge A_\epsilon ^{m-1}=1$. Consequently the two terms have $h$-traces $I_\epsilon /H_\epsilon $ and $m$, which proves the trace normalization of $g_\epsilon ^ m=T_\epsilon /M_\epsilon $. Subtracting $\epsilon w$ from $\theta _\epsilon $ subtracts $\epsilon I_\epsilon /H_\epsilon $ from the pairing $\int _ X\theta _\epsilon \wedge T_\epsilon =n$. Rescaling $\gamma _\epsilon $ by $M_\epsilon ^{-1/m}$ divides both the linear pairing and $D_\mu $ by $M_\epsilon $, proving (12.14.11).

Polar integration gives

\[ I_\epsilon =m t^2\int _0^1 \frac{x^{m-1}}{(x+t\epsilon )^2}\, \mathrm{d}x. \]

When $m=2$, put $q=\epsilon /2$. Direct integration yields

\[ I_\epsilon =\tfrac 12\left(\log \frac{1+q}{q} +\frac q{1+q}-1\right), \qquad H_\epsilon =1-q\log \frac{1+q}{q}. \]

Hence $I_\epsilon \sim \tfrac 12\log (1/\epsilon )$ and $\epsilon I_\epsilon \to 0$. Since $H_\epsilon \to 1$, the asymptotics in (12.14.12) follow from (12.14.11).

For the weak limit when $n=3$, note that the mixed positive term $2A_\epsilon \wedge w$ has $h$-trace two; divided by $M_\epsilon \to \infty $, it tends weakly to zero. The horizontal probability measure

\[ I_\epsilon ^{-1}(a+\epsilon )^{-2}\omega ^2 \]

on $B$ concentrates at $p$: outside any fixed neighborhood of $p$ its unnormalized density stays bounded, while $I_\epsilon \to \infty $. For a smooth $(1,1)$-test form on $X$, integration along the fibers $\{ b\} \times \mathbb P^1$ gives a smooth function on $B$. The convergence of these probability measures to the Dirac mass at $p$ therefore shows that the horizontal term of $g_\epsilon ^2$ converges to $[Z]$, because its coefficient $I_\epsilon /(H_\epsilon M_\epsilon )$ tends to one.

For $m\geq 3$, monotone convergence instead gives

\[ I_\epsilon \longrightarrow m t^2\int _0^1x^{m-3}\, \mathrm{d}x =\frac{(m-1)^2}{m(m-2)}. \]

In both cases $\epsilon I_\epsilon \to 0$. Using $H_\epsilon \to 1$ in (12.14.11) proves the remaining limits, including that of the volume quotients. $\square$

For $n\geq 4$ the metrics $g_\epsilon $ still minimize the perturbed volumes, and their quotients converge to $\lambda _\mu (\theta )$, but their normalized pairings with $\theta $ stay bounded away from zero. This does not contradict nonbigness: the bigness threshold is approached by a different family.

Proposition 12.14.13.F8EA88FD522E For every $n\geq 3$ there are smooth balanced metrics $b_\rho $, $0<\rho <1$, with

\[ \int _ Xh\wedge b_\rho ^ m=1,\qquad b_\rho ^ m\rightharpoonup [Z],\qquad \int _ X\theta \wedge b_\rho ^ m\longrightarrow 0, \qquad D_\mu (b_\rho )\longrightarrow 0 \]

as $\rho \downarrow 0$.

Proof. Choose a nonzero smooth function $f_\rho \geq 0$ on $B$, supported in $\{ x<\rho \} $ and normalized by $\int _ Bf_\rho \omega ^ m=1$. The form

F8E2395BD557 12.14.14
\begin{equation} \Gamma _\rho =\frac{f_\rho \omega ^ m+\rho h^ m}{1+n\rho } \end{equation}

is smooth, strictly positive and closed: the first summand has top degree on the base, and $h$ is Kähler. The positive-root construction in the proof of theorem 11.6.1 gives a unique smooth metric $b_\rho $ with $b_\rho ^ m=\Gamma _\rho $, and $b_\rho $ is balanced because $\Gamma _\rho $ is closed. Since $\int _ Xh^{m+1}=n$, its $h$-trace is one.

Put $C_\theta =\int _ X\theta \wedge h^ m$. Since $a<\rho /t$ on the support of $f_\rho $,

\[ 0\leq \int _ X\theta \wedge \Gamma _\rho \leq \frac{\rho /t+\rho C_\theta }{1+n\rho }\longrightarrow 0. \]

The lower bound in the proof of theorem 12.14.6 gives $D_\mu (b_\rho )\leq n^{-1/n}\int _ X\theta \wedge \Gamma _\rho $, so the determinant integrals also tend to zero. The probability measures $f_\rho \omega ^ m$ converge to the Dirac mass at $p$ because their supports shrink to that point. Fiber integration, as in the preceding proof, gives the current limit $[Z]$, while the term $\rho h^ m$ tends to zero. $\square$

Thus the normalized current $[Z]$ is a weak limit of smooth balanced metrics normalized by their $h$-traces. It annihilates $\theta $, and its determinant-weighted measure vanishes by proposition 12.34.2. The two families give explicit instances of the separation between the volume and threshold denominators described in proposition 24.3.2, without any general smoothing result for Gauduchon currents.

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