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21.13.31 Partial Okounkov bodies962BB5F87752

There are some canonical choices of smooth flags in the toric setting.

Since $X$ is smooth and projective, we can choose a full-dimensional cone $\sigma $ in $\Sigma $ with rays $\rho _1,\ldots ,\rho _ n\in \sigma (1)$ such that $u_{\rho _1},\ldots ,u_{\rho _ n}$ form a basis of $N$. Define

\[ Y_ i=D_{\rho _1}\cap \cdots \cap D_{\rho _ i},\quad i=1,\ldots ,n. \]

Then $Y_{\bullet }$ is a smooth flag on $X$. Let

1EA0A3B6C7EA 21.13.32
\begin{equation} \Phi \colon M\rightarrow \mathbb {Z}^ n,\quad m\mapsto \left(\langle m-m_{\sigma },u_{\rho _1} \rangle ,\dots ,\langle m-m_{\sigma },u_{\rho _ n} \rangle \right). \end{equation}

Then $\Phi $ is an isomorphism of lattices. It induces an $\mathbb {Z}$-affine isomorphism

\[ \Phi _{\mathbb {R}}\colon M_{\mathbb {R}}\rightarrow \mathbb {R}^ n. \]

Proposition 21.13.33.0ED70BB2A7D0 We have

35302703CBCC 21.13.34
\begin{equation} k^{-1}\nu _{Y_{\bullet }}\left(\mathrm{H}^0(X,L^ k)^{\times } \right)=\Phi _{\mathbb {R}} \left(P_{D}\cap k^{-1}M\right) \end{equation}

for any $k\in \mathbb {Z}_{>0}$. In particular,

12.28
\begin{equation} \Delta _{Y_{\bullet }}(L)=\Phi _{\mathbb {R}}(P_ D). \end{equation}
Recall that $\Delta _{Y_{\bullet }}(L)\subseteq \mathbb {R}^ n$ is the Okounkov body defined in definition 19.4.8.

Proof. We first reduce to the case where $D|_{U_{\sigma }}=0$. In fact, replacing $D$ by $D+\operatorname{div}\chi ^{m_{\sigma }}$ would result in changing $P_ D$ to $P_ D-m_{\sigma }$. So in view of (21.13.6), we may assume that $D|_{U_{\sigma }}=0$ and hence $m_{\sigma }=0$.

Fix $k\in \mathbb {Z}_{>0}$. Let $s\in \mathrm{H}^0(X,L^ k)$ be a non-zero toric eigen-section, say $\chi ^ m$ for some $m\in kP_ D\cap M$. The zero-divisor of $s$ on $U_{\sigma }$ is given by

\[ \sum _{i=1}^ n \langle m, u_{\rho _ i} \rangle D_{\rho _ i}, \]

see [Proposition 4.1.2, CLS11]. Therefore,

\[ \nu _{Y_{\bullet }}(s)=\Bigl (\langle m, u_{\rho _1} \rangle ,\dots ,\langle m, u_{\rho _ n} \rangle \Bigr )=\Phi (m). \]

Conversely, every section of $L^ k$ is a finite linear combination of such characters. In the coordinates on $U_{\sigma }$ determined by $u_{\rho _1},\ldots ,u_{\rho _ n}$, the Okounkov valuation of a non-zero linear combination is the lexicographically first exponent among the characters with non-zero coefficient. Hence arbitrary sections give no valuations beyond the right-hand side of (21.13.34), and (21.13.34) follows. $\square$

Example 21.13.35.74A6D2D50F46 Let us continue the example of $\mathbb {P}^2$ in example 21.13.12. We use the same notations. Take $\sigma _1$ as our reference cone, and $\rho _1=\sigma _5$, $\rho _2=\sigma _6$. Then

\[ Y_1=\Bigl \{ [X_0:0:X_2]:(X_0,X_2)\neq (0,0) \Bigr \} ,\quad Y_2=\Bigl \{ [X_0:0:0]:X_0\neq 0\Bigr \} . \]

The map $\Phi $ is given by

\[ \Phi (m_1,m_2)=(m_1,m_2). \]

In this case, we see easily

\[ \Delta _{Y_{\bullet }}\left(\mathcal{O}_{\mathbb {P}^2}(1)\right)=P_ D \]

is the polytope in 21.13.14.

Example 21.13.36.BB6FCAD03597 Let us continue the example of $\mathrm{Bl}_{0}\mathbb {P}^2$ in example 21.13.15. This time, let us take $\sigma _1'$ as our reference cone and $\rho _1=\sigma _5$, $\rho _2=\sigma _7$. Then $Y_1$ is just the strict transform of the line $\{ [X_0:0:X_2]:X_0X_2\neq 0\} $ in $\mathbb {P}^2$, while $Y_2$ is the point $Y_1\cap E$, where $E$ is the exceptional divisor.

In this case, the map $\Phi $ is given by

\[ \Phi (m_1,m_2)=(m_1,m_1+m_2). \]

We find that

\[ \Delta _{Y_{\bullet }}\left(\mathrm{Bl}_{0}\mathbb {P}^2,\pi ^*\mathcal{O}_{\mathbb {P}^2}(1)\right) \]

is the polytope in 21.13.37.

Mathematical diagram from the source
51BA09C1565221.13.37 The Okounkov body $\Delta _{Y_{\bullet }}(\mathrm{Bl}_{0}\mathbb {P}^2,\pi ^*\mathcal{O}_{\mathbb {P}^2}(1))$.

Note that it differs from the polytope in example 21.13.35.

Lemma 21.13.38.FCDBEF4DBD54 Let $\varphi \in \mathrm{PSH}_{\mathrm{tor}}(X,\theta )$ and assume that $\theta _{\varphi }$ is a Kähler current. Then $\varphi $ admits a quasi-equisingular approximation $(\varphi _ j)_ j$ with the following additional properties:

  1. FE65BEEFF2E3

    $\varphi _ j\in \mathrm{PSH}_{\mathrm{tor}}(X,\theta )$ and $\theta _{\varphi _ j}$ is a Kähler current for all $j\geq 1$;

  2. 5EC471277960

    for each $j\geq 1$, there are $q_ j\in \mathbb Z_{>0}$ and toric eigen-sections

    \[ s_{j,1},\ldots ,s_{j,a_ j}\in \mathrm{H}^0(X,L^{q_ j}) \]

    such that

    \[ \varphi _ j=\frac{1}{q_ j}\log \sum _{\ell =1}^{a_ j}|s_{j,\ell }|_{h^{q_ j}}^2+\mathcal O(1). \]

Proof. Apply Demailly's Bergman-kernel approximation theorem [Theorem 13.21, Dem12] to the singular Hermitian metric $h\exp (-\varphi )$ on $L$. Since $\theta _{\varphi }$ is a Kähler current, the theorem applies to the Hilbert spaces

\[ \mathrm{H}^0\bigl (X,L^ q\otimes \mathcal I(q\varphi )\bigr ) \]

for $q\gg 1$, endowed with the $L^2$-norm induced by $h^ q\exp (-q\varphi )$ and a fixed Kähler volume form. The usual decreasing extraction in Demailly's construction gives a quasi-equisingular approximation; taking $q$ sufficiently large at each step ensures that the approximants still have Kähler Chern currents.

It remains to note that this construction is compatible with the torus action. Indeed, both $h$ and $\varphi $ are $T_ c$-invariant, hence the above Hilbert spaces and their $L^2$-inner products are $T_ c$-invariant. Since $T_ c$ is compact and abelian, each of these finite-dimensional Hilbert spaces admits an orthonormal basis consisting of toric eigen-sections. With such a basis, the corresponding Bergman potential has the displayed form and is $T_ c$-invariant. This proves the lemma. $\square$

Theorem 21.13.39.8F3CCCDB83EC Let $\varphi \in \mathrm{PSH}_{\mathrm{tor}}(X,\theta )_{>0}$. Then

3FD1A27C837D 21.13.40
\begin{equation} \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi )\Bigr )=\Delta _{Y_{\bullet }}(\theta ,\varphi ). \end{equation}

In particular,

04CC3F6E758B 21.13.41
\begin{equation} n!\operatorname{vol}\Delta (\theta ,\varphi )=\operatorname{vol}\theta _{\varphi }. \end{equation}
In particular, once $D$ is fixed, the Newton body $\Delta (\theta ,\varphi )$ depends only on the current $\theta _{\varphi }$, not on the specific choices of $h$, $\varphi $ and $s_ D$. It makes sense to write
\[ \Delta \left(\theta _{\varphi }\right)=\Delta (\theta ,\varphi ). \]

A generalization of (21.13.41) to mixed volumes will be proved in theorem 21.13.84.

Proof. We first reduce to the case where $D|_{U_{\sigma }}=0$. In fact, changing $D$ to $D+\operatorname{div}\chi ^{m_{\sigma }}$ would result in changing $F_{\theta }$ to $F_{\theta }-m_{\sigma }$. Hence, $F_{\varphi }$ changes to $F_{\varphi }-m_{\sigma }$. Therefore, $\Delta (\theta ,\varphi )$ becomes $\Delta (\theta ,\varphi )-m_{\sigma }$. Taking (21.13.6) into consideration, we may assume that $m_{\sigma }=0$.

Step 1. We first reduce to the case where $\theta _{\varphi }$ is a Kähler current.

By 13.13.47, we can find $\psi \in \mathrm{PSH}(X,\theta )$ such that $\psi \leq \varphi $ and $\theta _{\psi }$ is a Kähler current. Taking the average along $T_ c$, we may assume that $\psi $ is $T_ c$-invariant.

For each $t\in (0,1)$, we let

\[ \varphi _ t=(1-t)\psi +t\varphi . \]

Suppose that Kähler current case is known. Then we get

\[ \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi _ t)\Bigr )=\Delta _{Y_{\bullet }}(\theta ,\varphi _ t) \]

for any $t\in (0,1)$. It follows from theorem 21.11.56 that

\[ \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi )\Bigr )\supseteq \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi _ t)\Bigr )= \Delta _{Y_{\bullet }}(\theta ,\varphi _ t) \]

for any $t\in (0,1)$. Thanks to theorem 19.4.30, we have

\[ \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi )\Bigr )\supseteq \Delta _{Y_{\bullet }}(\theta ,\varphi ). \]

Comparing the volumes of both sides using proposition 21.13.28, (19.4.20), and the $\mathcal{I}$-goodness of toric singularities example 18.1.56, we find that

\[ n!\operatorname{vol}\Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi )\Bigr )=\int _ X \theta _{\varphi }^ n=\operatorname{vol}\theta _{\varphi }=n!\operatorname{vol}\Delta _{Y_{\bullet }}(\theta ,\varphi ). \]

In particular, we conclude (21.13.40).

Step 2. We handle the case where $\theta _{\varphi }$ is a Kähler current.

Let $(\varphi _ j)_ j$ be the quasi-equisingular approximation given by 21.13.38.

Now assume that the result is known for each $\varphi _ j$. Then

\[ \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi _ j)\Bigr )=\Delta _{Y_{\bullet }}(\theta ,\varphi _ j). \]

In particular, thanks to proposition 19.4.28,

\[ \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi )\Bigr )\subseteq \Delta _{Y_{\bullet }}(\theta ,\varphi _ j) \]

for each $j\geq 1$. It follows from theorem 19.4.30 that

\[ \Phi _{\mathbb {R}}\Bigl ( \Delta (\theta ,\varphi )\Bigr )\subseteq \Delta _{Y_{\bullet }}(\theta ,\varphi ). \]

Comparing the volumes of both sides using proposition 21.13.28, (19.4.20), and example 18.1.56, we conclude (21.13.40).

Step 3. It remains to prove the assertion for the analytic approximants appearing in Step 2.

By 21.13.38, these approximants may be chosen in the form

\[ \varphi =\frac{1}{q}\log \sum _{i=1}^ a |s_ i|_{h^ q}^2+\mathcal O(1), \]

where $q\in \mathbb Z_{>0}$ and $s_1,\ldots ,s_ a\in \mathrm{H}^0(X,L^ q)$ are toric eigen-sections.

Let $m_1,\ldots ,m_ a\in qP_ D\cap M$ be the lattice points corresponding to $s_1,\ldots ,s_ a$.

Observe that

\[ \begin{aligned} \Delta (\theta ,\varphi ) =& \overline{\nabla F_{\varphi }(N_{\mathbb {R}})}\\ =& \left\{ m\in M_{\mathbb {R}} : F_{\varphi }(n)-\langle m,n \rangle \textup{ is bounded from below} \right\} \\ =& \left\{ m\in M_{\mathbb {R}}: q^{-1}\log \sum _{i=1}^ a \mathrm{e}^{\langle m_ i,n\rangle }-\langle m,n\rangle \textup{ is bounded below in } n \right\} \\ =& q^{-1}\mathrm{Conv}\{ m_1,\ldots ,m_ a\} , \end{aligned} \]

where we have applied (21.13.23) on the second line and 21.11.62 on the third line. Since $m_1,\ldots ,m_ a\in qP_ D$, the preceding formula also shows that

\[ \Delta (\theta ,\varphi )\subseteq P_ D. \]

Thus, if $m\in k\Delta (\theta ,\varphi )\cap M$, then $m\in kP_ D\cap M$, and $\chi ^ m$ indeed determines a global section of $L^ k$.

In particular, by the same separation argument as in 21.11.60, for any $k\in \mathbb {Z}_{>0}$ and any $m\in k\Delta (\theta ,\varphi )\cap M$, we have

\[ |\chi ^ m|^2 \mathrm{e}^{-k\varphi } \]

is bounded from above on $T(\mathbb {C})$. In other words, the section $s$ of $L^ k$ corresponding to $m$ satisfies

\[ s\in \mathrm{H}^0\left(X,L^ k\otimes \mathcal{I}_{\infty }(k\varphi )\right). \]

Therefore,

\[ \nu _{Y_{\bullet }}(s)=\Phi (m)\in k\Delta _ k(\theta ,\varphi ), \]

where $\Delta _ k$ is defined in section 19.4. Hence,

\[ \Phi \Bigl (k\Delta (\theta ,\varphi )\cap M\Bigr )\subseteq k\Delta _ k(\theta ,\varphi ). \]

Letting $k\to \infty $ and applying theorem 19.4.41, we find that

\[ \Phi _{\mathbb {R}}\Bigl (\Delta (\theta ,\varphi )\Bigr ) \subseteq \Delta _{Y_{\bullet }}(\theta ,\varphi ). \]

Comparing the volumes of both sides using proposition 21.13.28 and (19.4.20), we conclude that the equality holds and (21.13.40) follows. $\square$

The following two consequences are both due to Yi Yao.

Corollary 21.13.42.B202075FB15E Let $E$ be a $T$-invariant prime divisor on $X$ corresponding to a ray $\rho \in \Sigma (1)$. Then for any $\varphi \in \mathrm{PSH}_{\mathrm{tor}}(X,\theta )_{>0}$, we have

\[ \nu (\varphi ,E)=\inf \left\{ \langle m-m_{\rho },u_{\rho }\rangle : m\in \Delta (\theta ,\varphi ) \right\} . \]

Proof. This follows immediately from theorem 21.13.39 and theorem 19.4.51. In fact, since $X$ is projective and smooth, there is always a $T$-invariant smooth flag $Y_{\bullet }$ with $Y_1=E$. $\square$

This result seems new even in the ample setting. Intuitively, after taking theorem 21.13.45 into consideration as well, in the ample case the generic Lelong number $\nu (\varphi ,E)$ is the rescaled “distance” from $\Delta (\theta ,\varphi )$ to the facet of $P_ D$ corresponding to $E$.2

Corollary 21.13.43.C521E79AA7F6 Let $Y\subseteq X$ be a $T$-invariant subvariety corresponding to a cone $\sigma $ in $\Sigma $, and let $\varphi \in \mathrm{PSH}_{\mathrm{tor}}(X,\theta )_{>0}$. Then the following are equivalent:

  1. 29543A48DCD3

    $\nu (\varphi ,Y)=0$;

  2. 132682CA7C05

    there is a point $m\in \Delta (\theta ,\varphi )$ such that $\langle m-m_{\rho },u_{\rho }\rangle =0$ for any $\rho \in \sigma (1)$;

  3. 9F273D9DD37A

    we have

    \[ \Delta (\theta ,\varphi )\cap Q_{\sigma } \neq \varnothing . \]
Recall that $Q_{\sigma }$ is defined in (21.13.7).

Proof. 2 $\iff $ 3. This follows from the definition of $Q_{\sigma }$ in (21.13.7).

1 $\iff $ 2. Let $\rho _1,\ldots ,\rho _ r$ be the rays of $\sigma $. Up to replacing $D$ by a translation, we may assume that $m_{\sigma }=0$. Hence, we may take $m_{\rho _ i}=0$ for all $i$.

Let $\pi \colon Z\rightarrow X$ be the blow-up of $X$ along $Y$. See [Page 132, CLS11] for the basic properties of the toric blow-up. Take the divisor $\pi ^*D$ on $Z$. We choose the pull-back metric $\pi ^*h$ on $\pi ^*L$. Then $F_{\pi ^*\theta }$ can be taken as $\pi ^*F_{\theta }$ by (21.13.23). It follows that $\Delta (\theta ,\varphi )=\Delta (\pi ^*\theta ,\pi ^*\varphi )$. On the other hand, the ray corresponding to the exceptional divisor $E$ is generated by $u_{\rho _1}+\cdots +u_{\rho _ r}$. Since $X$ is smooth, this vector is primitive.

Recall that the support function of $\pi ^*D$ is the same as the support function of $D$, see [Proposition 6.2.7, CLS11]. In particular, we can take the Cartier datum $m_{\rho }=m_{\sigma } \mod M(\rho )$, where $\rho $ is the ray corresponding to $E$.

It follows from corollary 21.13.42 and 5.16.17 that

6C720B821C17 21.13.44
\begin{equation} \nu (\varphi ,Y)=\nu (\pi ^*\varphi ,E)= \inf \left\{ \langle m-m_{\sigma },u_{\rho _1}+\cdots +u_{\rho _ r}\rangle :m\in \Delta (\theta ,\varphi )\right\} . \end{equation}

Our assertion follows in view of (21.13.5). $\square$

It follows from (21.13.44) that

\[ \nu (\varphi ,Y)\geq \sum _{i=1}^ r \nu (\varphi ,E_ i), \]

where the $E_ i$'s are the prime divisors corresponding to the rays of $\sigma $. This inequality seems to be new as well.

The following consequence of theorem 21.13.39 is the key to the development of the toric pluripotential theory.

Theorem 21.13.45.1293B87EF09F We have

188F0AD7B28C 21.13.46
\begin{equation} F_{V_{\theta }}\in \mathcal{E}^{\infty }(N_{\mathbb {R}},P_ D).{}^{\href{#sgpt-a0000102047}{3}}\end{equation}

In particular,

82B62A741230 21.13.47
\begin{equation} \int _ X \theta _{V_{\theta }}^ n=n!\operatorname{vol}P_ D. \end{equation}
Recall that $\mathcal{E}^{\infty }$ is defined in definition 21.11.41. The equation (21.13.46) says
83935CB0C416 21.13.48
\begin{equation} F_{V_{\theta }}-\operatorname{Supp}_{P_ D} \textup{ is bounded}. \end{equation}

In particular,

6DBC736A41CF 21.13.49
\begin{equation} \Delta (\theta ,V_{\theta })=P_ D \end{equation}

and hence the Newton bodies $\Delta (\theta ,\varphi )$ are all contained in $P_ D$.

Proof. Taking $\varphi =V_{\theta }$ in theorem 21.13.39, we find

\[ \Phi _{\mathbb {R}}\left( \Delta (\theta ,V_{\theta })\right)=\Delta _{Y_{\bullet }}(\theta ,V_{\theta })=\Delta _{Y_{\bullet }}(L)=\Phi _{\mathbb {R}}(P_ D), \]

where we applied proposition 21.13.33 in the last equality. Therefore, (21.13.49) follows. In particular, (21.13.47) follows from proposition 21.13.28.

Next we prove (21.13.48). Take a smooth function $\chi \colon N_{\mathbb {R}}\rightarrow [0,1]$ so that

  1. 37909700D0C1

    $\operatorname{Supp}\chi $ is compact;

  2. C1605365568C

    $\chi \equiv 1$ on a neighbourhood of $0$.

Fix a $T_ c$-invariant volume form $\mu $ on $T(\mathbb {C})$. Then $(\operatorname{Trop}^*\chi )\mu $ can be regarded as a $T_ c$-invariant smooth non-negative measure on $X$. After choosing a suitable normalizing constant $C>0$, there is a unique solution

F3EAEAF94235 21.13.50
\begin{equation} \theta _{\varphi }^ n=C\left(\operatorname{Trop}^*\chi \right)\mu ,\quad \sup _ X \varphi =0,\quad \varphi \in \mathcal{E}^{\infty }(X,\theta ). \end{equation}

This is proved in [Theorem B, BEGZ10]. The uniqueness of $\varphi $ further guarantees its $T_ c$-invariance. Since $\varphi $ has minimal singularities, $F_{\varphi }\sim F_{V_{\theta }}$. Next, using proposition 21.13.28, the Monge–Ampère equation (21.13.50) implies

\[ \operatorname{MA}_{\mathbb {R}}\left(F_{\varphi }\right)=C \chi \operatorname{Trop}_*\mu . \]

It follows from the regularity theorem [Theorem 2.19, BB13] and (21.13.49) that $F_{\varphi }\sim \operatorname{Supp}_{P_ D}$. Hence, (21.13.48) follows. $\square$

In particular, thanks to corollary 21.13.42,

70B4F53FBB2E 21.13.51
\begin{equation} \nu (V_{\theta },E)=\min \left\{ \langle m-m_{\rho },u_{\rho }\rangle : m\in P_ D \right\} . \end{equation}

As an interesting consequence of (21.13.51), we have a geometric description of the divisorial Zariski decomposition in the toric setting: The negative part of $D$ is given by

\[ \sum _{\rho \in \Sigma (1)} \min \left\{ \langle m-m_{\rho },u_{\rho }\rangle : m\in P_ D \right\} D_{\rho }. \]

A prime divisor $D_{\rho }$ appears in the negative part if and only if the corresponding condition

\[ \langle m,u_{\rho } \rangle \geq -a_{\rho } \]

is redundant in defining $P_ D$ by (21.13.2). The modified nef part of $D$ is the $\mathbb {Q}$-divisor obtained after removing these redundancies.

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