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17.13 Ross–Witt Nyström correspondenceC9D15D724069

C9D15D724069

Let $X$ be a connected compact Kähler manifold of dimension $n$ and $\theta $ be a smooth closed real $(1,1)$-form on $X$ representing a big cohomology class. Fix a model potential $\phi \in \mathrm{PSH}(X,\theta )_{>0}$.

proposition 17.12.16 allows us to talk about the Legendre transforms of test curves in the expected way.

The general definition of the Legendre transform definition 21.11.22 can be translated as follows:

Definition 17.13.1.2105331E66C7 Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. We define its Legendre transform as the map $\Gamma ^*\colon (0,\infty )\rightarrow \mathrm{PSH}(X,\theta )$ given by

22C9794122C8 17.13.2
\begin{equation} \Gamma ^*_ t=\sup _{\tau \in \mathbb {R}} \left(t\tau + \Gamma _{\tau }\right){}^{\href{#sgpt-a0000073394}{1}}. \end{equation}

Thanks to 17.12.3, (17.13.2) can be equivalently written as
\[ \Gamma ^*_ t=\sup _{\tau <\Gamma _{\max }} \left(t\tau + \Gamma _{\tau }\right)=\sup _{\tau \leq \Gamma _{\max }} \left(t\tau + \Gamma _{\tau }\right). \]

It is sometimes handy to define

1824FEE5F9FF 17.13.3
\begin{equation} \Gamma ^*_0\coloneqq \phi \end{equation}

at $t=0$. But it is important to remember that, with this convention, (17.13.2) is not true at $t=0$ in general.

Remark 17.13.4.ABB931E35703 Here we do not discuss the case $t<0$ because its behavior is straightforward: take $x\in X$; if $\Gamma _{\tau }(x)=-\infty $ for all $\tau <\Gamma _{\max }$, then $\Gamma _ t^*(x)=-\infty $; otherwise, $\Gamma _ t^*(x)=\infty $.

The information about $t>0$ suffices to characterize $\Gamma $.

Proposition 17.13.5.1F48BF7602CA Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. Then

24A2034A1287 17.13.6
\begin{equation} \Gamma _{\tau }=\inf _{t>0} \left(\Gamma ^*_ t-t\tau \right) \end{equation}

for all $\tau \in \mathbb {R}$.

Due to our convention (17.13.3), in (17.13.6) we may equivalently take $t\geq 0$.

Proof. Fix $x\in X$. We want to establish (17.13.6) at $x$. We distinguish two cases. First suppose that $\Gamma _{\tau }(x)=-\infty $ for all $\tau <\Gamma _{\max }$ and hence all $\tau \in \mathbb {R}$. In this case, we have $\Gamma _ t^*(x)=-\infty $ for all $t>0$. Therefore, (17.13.6) follows trivially.

Otherwise, by 17.13.4, we know that $\Gamma ^*_ t(x)=\infty $ for all $t<0$. The relative interior of the domain of $t\mapsto \Gamma ^*_ t(x)$ is contained in $(0,\infty )$. Therefore, (17.13.6) follows from theorem 21.11.24, proposition 17.12.16. $\square$

In definition 17.13.1, we made the nontrivial claim that $\Gamma ^*_ t\in \mathrm{PSH}(X,\theta )$ for all $t>0$. Let us prove this.

Lemma 17.13.7.BC74B8EA334F Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. Then $\Gamma ^*_ t\in \mathrm{PSH}(X,\theta )$ for all $t>0$. In fact, $\Gamma ^*$ is upper semicontinuous as a function of $X\times (0,\infty )$.

Proof. We first observe that for each $x\in X$, we have

\[ \Gamma _ t^*(x)\leq t\Gamma _{\max }<\infty . \]

Let $R=\{ a+\mathrm{i}b\in \mathbb {C}:a>0,b\in \mathbb {R}\} $. We consider

\[ F\colon X\times R\rightarrow [-\infty ,\infty ),\quad (x,a+\mathrm{i}b)\mapsto \Gamma _ a^*(x). \]

Let $\pi \colon X\times R\rightarrow X$ be the natural projection. Observe that the upper semicontinuous regularization $G$ of $F$ is $\pi ^*\theta $-psh by proposition 5.14.2. It suffices to show that $F=G$. We let

\[ E\coloneqq \left\{ (x,z)\in X\times R: F(x,z)<G(x,z) \right\} . \]

We want to argue that $E=\varnothing $. Since $F$ is invariant under translations in the imaginary direction of $R$, the same is true for its upper semicontinuous regularization $G$. So $E$ can be written as $B\times \mathrm{i}\mathbb {R}$ for some set $B\subseteq X\times (0,\infty )$. Since $E$ is a pluripolar set by proposition 5.14.5, it has zero Lebesgue measure. Hence, $B$ has zero Lebesgue measure. For each $x\in X$, write

\[ B_ x=\left\{ t\in (0,\infty ): (x,t)\in B \right\} . \]

By Fubini's theorem, $B_ x$ has vanishing $1$-dimensional Lebesgue measure for all $x\in X\setminus Z$, where $Z\subseteq X$ is a subset of measure $0$. We may assume that $Z\supseteq \{ \Gamma _{\Gamma _{\max }}=-\infty \} $ so that for $x\in X\setminus Z$, $\Gamma ^*_ t(x)\neq -\infty $ for all $t>0$.

For any $x\in X\setminus Z$, both $t\mapsto F(x,t)$ and $G(x,t)$ are convex functions with values in $\mathbb {R}$ on $(0,\infty )$. They agree almost everywhere, hence everywhere by their continuity. It follows that for $x\in X\setminus Z$, we have $B_ x=\varnothing $.

By proposition 17.13.5, for any $x\in X$, we have

\[ \Gamma _{\tau }(x)=\inf _{t>0} (F(x,t)-t\tau ),\quad \tau <\Gamma _{\max }. \]

On the other hand, let

DBF41B839C63 17.13.8
\begin{equation} \chi _{\tau }(x)=\inf _{t>0} (G(x,t)-t\tau ),\quad \tau < \Gamma _{\max },\quad x\in X. \end{equation}

By Kiselman's principle proposition 5.14.15, $\chi _{\tau }\in \mathrm{PSH}(X,\theta )$. But on $X\setminus Z$, we already know that $\Gamma _{\tau }=\chi _{\tau }$ for all $\tau <\Gamma _{\max }$. By proposition 5.14.6,

\[ \Gamma _{\tau }=\chi _{\tau },\quad \tau <\Gamma _{\max }. \]

Now we conclude that $F(x,t)=G(x,t)$ by corollary 21.11.26. $\square$

Corollary 17.13.9.4B87EF03E3EA Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. Then $\Gamma ^*_ t\in \mathcal{E}(X,\theta ;\phi )$ for all $t>0$.

Proof. Fix $t>0$. We already know that $\Gamma ^*_ t\in \mathrm{PSH}(X,\theta )$ by 17.13.7. It suffices to show that

\[ \Gamma ^*_ t\sim _ P \phi . \]

From (17.13.2) and proposition 16.8.28, we know that

\[ \Gamma ^*_ t\sim _ P \operatorname *{sup}_{\tau <\Gamma _{\max }}{}\! {}^{*} \Gamma _{\tau }=\phi . \]

This completes the proof. $\square$

Lemma 17.13.10.C6092031D5B3 Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. Then

\[ \sup _ X \Gamma _ t^*=t\Gamma _{\max } \]

for all $t>0$.

In particular, $t\mapsto \Gamma ^*_ t-t\Gamma _{\max }$ is a decreasing function in $t>0$.

Proof. Since $\Gamma _{\tau }\leq 0$ for all $\tau <\Gamma _{\max }$, we have

\[ \sup _ X \Gamma _ t^*\leq t\Gamma _{\max } \]

for all $t>0$. Conversely, for each $\tau <\Gamma _{\max }$,

\[ \sup _ X\Gamma _ t^*\geq \sup _ X(t\tau +\Gamma _{\tau })=t\tau . \]

Letting $\tau \to \Gamma _{\max }$ gives the reverse inequality. The final assertion follows directly from the formula

\[ \Gamma _ t^*-t\Gamma _{\max }=\sup _{\tau <\Gamma _{\max }}\Bigl (\Gamma _\tau -t(\Gamma _{\max }-\tau )\Bigr ). \]

This completes the proof. $\square$

Lemma 17.13.11.9C6538C4298E Given $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$, we have $\Gamma ^*\in \mathcal{R}(X,\theta ;\phi )$.

See definition 17.10.38 for the notation $\mathcal{R}(X,\theta ;\phi )$.

Proof. It follows from 17.13.7, (17.13.2) and proposition 5.14.2 that the restriction of $\Gamma ^*$ to each compact subinterval of $(0,\infty )$ is a subgeodesic. By corollary 17.13.9, for any $t>0$, $\Gamma ^*_ t\in \mathcal{E}(X,\theta ;\phi )$.

First observe that as $t\to 0+$, we have

E5C60BE9B124 17.13.12
\begin{equation} \Gamma _ t^*\xrightarrow {L^1}\phi . \end{equation}

By 17.13.10 and proposition 5.17.3, it suffices to show each $L^1$-cluster point $\psi \in \mathrm{PSH}(X,\theta )$ of $\Gamma _ t^*$ as $t\to 0$ is equal to $\phi $.

To see this, first observe that by (17.13.2), for any fixed $t>0$,

\[ \Gamma _ t^*\leq t\Gamma _{\max }+\phi . \]

Therefore, $\psi \leq \phi $. On the other hand, for any fixed $\tau <\Gamma _{\max }$, by (17.13.2), we have

\[ \Gamma ^*_ t\geq \Gamma _{\tau }+t\tau \]

for any $t>0$. So $\psi \geq \Gamma _{\tau }$ almost everywhere and hence everywhere by proposition 5.14.6. It follows that $\psi \geq \phi $. Therefore, $\psi =\phi $.

Assume that $\Gamma ^*$ is not a geodesic ray. Then we can find $0\leq a<b$ such that $(\Gamma ^*_ t)_{t\in (a,b)}$ differs from the geodesic $(\eta _ t)_{t\in (a,b)}$ from $\Gamma ^*_ a$ to $\Gamma ^*_ b$. The existence of $(\eta _ t)_ t$ is guaranteed by proposition 17.10.24. We consider the subgeodesic $(\ell _ t)_{t>0}$ given by $\ell _ t=\eta _ t$ for $t\in (a,b)$ and $\ell _ t=\Gamma ^*_ t$ otherwise. Note that $\ell $ is a subgeodesic due to the gluing lemma 17.10.16.

Consider the Legendre transform

\[ \Gamma '_{\tau }=\inf _{t>0} (\ell _ t-t\tau ),\quad \tau \in \mathbb {R}. \]

Then $\Gamma '_{\tau }\geq \Gamma _{\tau }$ and $\Gamma '_{\tau }\in \mathrm{PSH}(X,\theta )\cup \{ -\infty \} $ by proposition 5.14.15 for all $\tau \in \mathbb {R}$.

We claim that

BD13D6DEBB93 17.13.13
\begin{equation} \Gamma '_{\tau }\leq \Gamma _{\tau }+(b-a)(\Gamma _{\max }-\tau ),\quad \tau \in \mathbb {R}. \end{equation}

Observe that $\Gamma '_{\tau }\equiv -\infty $ when $\tau >\Gamma _{\max }$ by 17.13.10. Thus it suffices to consider $\tau \leq \Gamma _{\max }$. Put

\[ C_{\tau }\coloneqq (b-a)(\Gamma _{\max }-\tau )\geq 0. \]

For any $s\in [a,b]$, the monotonicity of $t\mapsto \Gamma _ t^*-t\Gamma _{\max }$ from 17.13.10 gives

\[ \Gamma _ b^*-b\tau \leq \Gamma _ s^*-s\tau +C_{\tau }. \]

Since $\ell _ b=\Gamma _ b^*$, we get

\[ \Gamma '_{\tau }\leq \Gamma _ b^*-b\tau \leq \Gamma _ s^*-s\tau +C_{\tau },\quad s\in [a,b]. \]

For $s\notin [a,b]$, we have $\ell _ s=\Gamma _ s^*$, hence

\[ \Gamma '_{\tau }\leq \Gamma _ s^*-s\tau \leq \Gamma _ s^*-s\tau +C_{\tau }. \]

Taking the infimum over all $s>0$ gives

\[ \Gamma '_{\tau }\leq \Gamma _{\tau }+C_{\tau }. \]

Therefore, (17.13.13) follows. In particular, for any $\tau <\Gamma _{\max }$, we have $\Gamma '_{\tau }\sim \Gamma _{\tau }$. Moreover, $\sup _ X\ell _ t\leq t\Gamma _{\max }$ for all $t>0$: this is clear outside $(a,b)$ from 17.13.10, and on $(a,b)$ it follows from the convexity of subgeodesics applied to the geodesic $(\eta _ t)_{t\in (a,b)}$. Hence, for $\tau <\Gamma _{\max }$,

\[ \sup _ X(\ell _ t-t\tau )\leq t(\Gamma _{\max }-\tau ). \]

Letting $t\to 0+$ gives $\Gamma '_{\tau }\leq 0$. It follows from the fact that $\Gamma _{\tau }$ is a model potential that $\Gamma _{\tau }=\Gamma '_{\tau }$ for all $\tau <\Gamma _{\max }$. Therefore, by theorem 21.11.24, we have $\Gamma ^*_ t=\ell _ t$ for all $t>0$, which is a contradiction. $\square$

Given $\ell \in \mathcal{R}(X,\theta ;\phi )$, define its Legendre transform

10B32891AA98 17.13.14
\begin{equation} \ell ^*_{\tau }\coloneqq \inf _{t>0} (\ell _ t-t\tau ),\quad \tau \in \mathbb {R}. \end{equation}

Lemma 17.13.15.7B83BD1D5FB9 Given $\ell \in \mathcal{R}(X,\theta ;\phi )$, then $\ell ^*=(\ell ^*_\tau )_{\tau <\sup _ X \ell _1}\in \mathrm{TC}(X,\theta ;\phi )$.

Proof. Note that it follows from proposition 5.14.15 that $\ell ^*_{\tau }\in \mathrm{PSH}(X,\theta )\cup \{ -\infty \} $ for all $\tau \in \mathbb {R}$. It is clear that $\mathbb {R}\ni \tau \mapsto \ell ^*_{\tau }$ is a decreasing and concave function.

By proposition 17.10.39,

\[ \sup _ X\ell _ t= t\sup _ X \ell _1 \quad \forall t\geq 0. \]

Set $C=\sup _ X\ell _1$. By proposition 17.10.39, $\sup _ X(\ell _ t-Ct)=0$ for all $t>0$. For each $x$ outside a pluripolar set, the function $t\mapsto \ell _ t(x)-Ct$ is convex on $(0,\infty )$ and bounded above by $0$, hence it is decreasing. By proposition 5.14.6, the same monotonicity holds as an inequality of $\theta $-psh functions. Thus $(\ell _ t-Ct)_{t>0}$ is a decreasing net in $\mathrm{PSH}(X,\theta )$.

Its infimum is not identically $-\infty $, since the family is normalized by $\sup _ X(\ell _ t-Ct)=0$ and is compact in $L^1$ by proposition 5.17.3. Therefore

\[ \ell ^*_{C}=\inf _{t>0}(\ell _ t-Ct)\in \mathrm{PSH}(X,\theta ) \]

by proposition 5.14.2.

On the other hand, for $\tau >\sup _ X \ell _1$, the same argument shows that

\[ \ell ^*_{\tau }\equiv -\infty . \]

Therefore, $\ell ^*_{\tau }\in \mathrm{PSH}(X,\theta )$ if and only if $\tau \leq \ell ^*_{\max }\coloneqq \sup _ X \ell _1$.

We claim that $(\ell ^*_{\tau })_{\tau <\ell ^*_{\max }}$ is a test curve. We first observe that for $\tau <\ell ^*_{\max }$, we have

\[ \ell ^*_{\tau }\leq \ell _1-\tau \sim _ P \phi . \]

Therefore,

5BF1777D23C2 17.13.16
\begin{equation} \ell ^*_{\tau }\preceq _ P \phi ,\quad \forall \tau <\ell ^*_{\max }. \end{equation}

Also observe that for any $\tau \leq \ell ^*_{\max }$ and any $t>0$, we have

\[ \sup _ X \ell ^*_{\tau }\leq \sup _ X \ell _ t-t\tau =\ell ^*_{\max }t-t\tau . \]

Letting $t\to 0+$, we find that for any $\tau \leq \ell ^*_{\max }$, we have

6F01D0840C12 17.13.17
\begin{equation} \sup _ X \ell ^*_{\tau }\leq 0. \end{equation}

Fix $\tau <\ell ^*_{\max }$. We want to argue that

59C9610616F1 17.13.18
\begin{equation} P_{\theta }\left[\ell ^*_{\tau }\right]=\ell ^*_{\tau }. \end{equation}

First we claim that for any $C>0$, we have

25F16D030FA9 17.13.19
\begin{equation} (\ell ^*_{\tau }+C)\land \phi =(\ell ^*_{\tau }+C)\land V_{\theta }. \end{equation}

The $\leq $ direction is trivial. We argue the reverse inequality, which reduces to

\[ \phi \geq (\ell ^*_{\tau }+C)\land V_{\theta }. \]

Since $\phi $ is model and $(\ell ^*_{\tau }+C)\land V_{\theta }\leq 0$, it suffices to show that

\[ \phi \succeq _ P (\ell ^*_{\tau }+C)\land V_{\theta }, \]

which follows from (17.13.16). Therefore, (17.13.19) is established. Thanks to (17.13.17), we have the obvious inequality

\[ (\ell ^*_{\tau }+C)\land V_{\theta }\geq \ell ^*_{\tau } \]

for any $C>0$. Therefore, in order to prove (17.13.18), it remains to argue that for any $C>0$,

CBA3E07AB082 17.13.20
\begin{equation} (\ell ^*_{\tau }+C)\land \phi \leq \ell ^*_{\tau }. \end{equation}

For this purpose, let us consider the following geodesics: For any $M>0$ and $t\in [0,1]$, let

\[ \ell ^{1,M}_ t= \ell _{tM}-tM\tau ,\quad \ell ^{2,M}_ t= (\ell ^*_{\tau }+C)\land \phi -Ct. \]

It is clear that at $t=0,1$, we have $\ell ^{2,M}_ t\leq \ell ^{1,M}_ t$. Hence, the same holds for all $t\in [0,1]$. In particular, for any fixed $s\in (0,1]$, we have

\[ (\ell ^*_{\tau }+C)\land \phi -Cs\leq \ell _{sM}-sM\tau \]

for all $M>0$. Taking infimum with respect to $M>0$, we find

\[ (\ell ^*_{\tau }+C)\land \phi -Cs\leq \ell ^*_{\tau }. \]

Since $s\in (0,1]$ is arbitrary, we conclude (17.13.20).

Finally, we check the condition at $-\infty $. Set

\[ \psi \coloneqq \operatorname *{sup}_{\tau <\ell ^*_{\max }}{}\! {}^{*}\ell ^*_{\tau }. \]

The family $(\ell ^*_{\tau })_{\tau <\ell ^*_{\max }}$ is locally uniformly bounded from above, so $\psi \in \mathrm{PSH}(X,\theta )$. Thanks to corollary 17.10.9, outside a pluripolar set, the function $t\mapsto \ell _ t(x)$ is a finite closed convex function on $[0,\infty )$ with value $\phi (x)$ at $t=0$. Applying the one-variable Legendre duality gives

\[ \psi (x)=\adjustlimits \sup _{\tau <\ell ^*_{\max }}\inf _{t>0}\bigl (\ell _ t(x)-t\tau \bigr )=\ell _0(x)=\phi (x)\quad \textup{quasi-everywhere}. \]

Hence $\psi =\phi $ by proposition 5.14.6. In particular, $\ell ^*_{-\infty }=\phi $ has positive mass. $\square$

Theorem 17.13.21.B28F0A28CB3E The Legendre transform in definition 17.13.1 is a bijection

6D5BA4827FF5 17.13.22
\begin{equation} \mathrm{TC}(X,\theta ;\phi )\xrightarrow {\sim } \mathcal{R}(X,\theta ;\phi ). \end{equation}

Moreover, this bijection restricts to the following bijections:

AE510D6D0C2F 17.13.23
\begin{equation} \mathrm{TC}^1(X,\theta ;\phi )\xrightarrow {\sim } \mathcal{R}^1(X,\theta ;\phi ),\quad \mathrm{TC}^{\infty }(X,\theta ;\phi )\xrightarrow {\sim } \mathcal{R}^{\infty }(X,\theta ;\phi ). \end{equation}

For any $\Gamma \in \mathrm{TC}^1(X,\theta ;\phi )$, we have

4884EC5C8FA9 17.13.24
\begin{equation} \mathbf{E}^{\phi }(\Gamma )=\mathbf{E}^{\phi }(\Gamma ^*). \end{equation}
Recall that the two energy functionals in (17.13.24) are defined in (17.12.12) and definition 17.10.82 respectively.

The correspondence (17.13.22) will be referred to as the Ross–Witt Nyström correspondence.

To appreciate this result, just consider the simple case where $\theta $ is a Kähler form and $\phi =0$. In this case, elements in $\mathcal{R}^{\infty }(X,\theta )$ are rays of bounded potentials, while elements in $\mathrm{TC}^{\infty }(X,\theta )$ are rays of singular potentials. This result establishes a bridge between the pluripotential theory of regular potentials and that of singular potentials!

Proof. Step 1. We first establish (17.13.22).

It follows from 17.13.11 that the forward map is well-defined. The inverse map is given by (17.13.14). We show that the inverse map is also well-defined. Given $\ell \in \mathcal{R}(X,\theta ;\phi )$, we know from 17.13.15 that $\ell ^*\in \mathrm{TC}(X,\theta ;\phi )$. We need to show that $\ell ^*\in \mathrm{TC}(X,\theta ;\phi )$.

The equality $\ell ^*_{-\infty }=\phi $ was proved in 17.13.15. Therefore, $\ell ^*\in \mathrm{TC}(X,\theta ;\phi )$ as expected.

The two operations are inverse to each other thanks to corollary 21.11.26. Hence, (17.13.22) is established.

Step 2. Next we consider the bounded situation. Namely, we want to establish the second half of (17.13.23).

Suppose that $\Gamma \in \mathrm{TC}^{\infty }(X,\theta ;\phi )$. Take $\tau _0\in \mathbb {R}$ so that $\Gamma _{\tau }=\phi $ for all $\tau \leq \tau _0$. It follows from (17.13.2) that

\[ \Gamma _ t^*\geq \phi +t\tau _0 \]

for all $t>0$. Therefore, $\Gamma ^*_ t\sim \phi $ for all $t>0$ and hence $\Gamma ^*\in \mathcal{R}^{\infty }(X,\theta ;\phi )$.

Conversely, suppose that $\ell \in \mathcal{R}^{\infty }(X,\theta ;\phi )$. Thanks to proposition 17.10.37, there is a constant $C>0$ such that

\[ \ell _ t\geq \phi -Ct. \]

Therefore, according to (17.13.14), we have

\[ \ell ^*_{\tau }\geq \inf _{t>0} \Bigl ( \phi -(C+\tau )t \Bigr )=\phi \]

if $\tau \leq -C$. Therefore, $\ell ^*_{\tau }=\phi $ for all $\tau \leq -C$.

Step 3. We establish (17.13.24) and the first half of (17.13.23).

Step 3.1. We reduce to the case where $\Gamma _{\max }=0$.

Suppose that we define

\[ \Gamma '_{\tau }=\Gamma _{\tau +\Gamma _{\max }},\quad \forall \tau <0. \]

Then $\Gamma '\in \mathrm{TC}(X,\theta ;\phi )$ as well and for all $t>0$,

\[ \Gamma '^*_ t=\sup _{\tau <0} \left( t\tau +\Gamma '_{\tau } \right)=\sup _{\tau <\Gamma _{\max }} \left( t\tau +\Gamma _{\tau } \right)-t\Gamma _{\max }=\Gamma ^*_ t-t\Gamma _{\max }. \]

Therefore,

\[ \mathbf{E}^{\phi }\left(\Gamma '^*\right)=\mathbf{E}^{\phi }\left(\Gamma ^*\right)-\Gamma _{\max }\int _ X \theta _{\phi }^ n. \]

by (16.5.13). Using (17.12.12), we also have

\[ \begin{aligned} \mathbf{E}^{\phi }(\Gamma ')=& \int _{-\infty }^0 \left( \int _ X \theta _{\Gamma '_{\tau }}^ n-\int _ X \theta _{\phi }^ n \right)\, \mathrm{d}\tau \\ =& \int _{-\infty }^{\Gamma _{\max }}\left( \int _ X \theta _{\Gamma _{\tau }}^ n-\int _ X \theta _{\phi }^ n \right)\, \mathrm{d}\tau \\ =& \mathbf{E}^{\phi }(\Gamma )-\Gamma _{\max }\int _ X \theta _{\phi }^ n. \end{aligned} \]

Therefore, it suffices to establish (17.13.24) for $\Gamma '$ in place of $\Gamma $.

Step 3.2. We assume that $\Gamma _{\max }=0$ and $\Gamma \in \mathrm{TC}^{\infty }(X,\theta ;\phi )$. We prove (17.13.24).

For $N\in \mathbb {Z}_{>0}$, $M \in \mathbb {Z}$, we introduce the following:

\[ \Gamma ^{*,N,M}_ t \coloneqq \max _{\substack {k \in \mathbb {Z} \\ k \leq M}} \left(\Gamma _{k/2^ N} + tk/2^ N\right)\in \mathcal{E}^{\infty }(X,\theta ;\phi ),\quad t>0. \]

We first claim that for all $t>0$, $N\in \mathbb {Z}_{>0}$ and $M\in \mathbb {Z}_{<0}$,

1C55A624E61E 17.13.25
\begin{equation} \frac{t}{2^ N} \int _ X \theta ^ n_{\Gamma _{(M+1)/2^ N}}\leq E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,M+1}\right)-E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,M}\right)\leq \frac{t}{2^ N} \int _ X \theta ^ n_{\Gamma _{M/2^ N}}. \end{equation}

Assuming this, let us prove (17.13.24).

Fixing $N$, let $M=\lfloor 2^{N}\Gamma _{\min }\rfloor $. Recall that $\Gamma _{\min }$ is defined in (17.12.11). Then repeated applications of (17.13.25) yield

\[ \sum _{j=M+1}^0 \frac{t}{2^ N} \int _ X \theta ^ n_{\Gamma _{j/2^ N}}\leq E^{\phi }_{\theta }\left(\Gamma _ t^{*,N,0}\right)-E^{\phi }_{\theta }\left(\Gamma _ t^{*,N,M}\right)\leq \sum _{j=M}^{-1} \frac{t}{2^ N} \int _ X \theta ^ n_{\Gamma _{j/2^ N}}. \]

Since $M \leq 2^{N}\Gamma _{\min }$, we have

\[ \Gamma ^{*,N,M}_ t =\phi +t M/2^ N. \]

Using (16.5.13), we can continue to write

\[ \sum _{j=M+1}^0 \frac{t}{2^ N} \left(\int _ X \theta ^ n_{\Gamma _{j/2^ N}} - \int _ X \theta ^ n_{\phi }\right)\leq E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,0}\right)\leq \sum _{j=M}^{-1} \frac{t}{2^ N} \left(\int _ X \theta ^ n_{\Gamma _{j/2^ N}} - \int _ X \theta ^ n_{\phi }\right). \]

We now notice that we have Riemann sums on both the left and right of the above inequality. Moreover, as $N\to \infty $, the potentials $\Gamma _ t^{*,N,0}$ increase to $\Gamma _ t^*$, hence their energies converge to $E^\phi _\theta (\Gamma _ t^*)$ by proposition 16.5.37. Using proposition 17.12.9, it is possible to let $N \to \infty $ and obtain

85E0D04C585D 17.13.26
\begin{equation} E_{\theta }^{\phi }(\Gamma _ t^{*})=t\mathbf{E}^{\phi }(\Gamma ) \end{equation}

So (17.13.24) follows as desired.

It remains to argue (17.13.25). Fix $t>0$, $N\in \mathbb {Z}_{>0}$ and $M\in \mathbb {Z}$. By proposition 16.5.36,

877135CB19C2 17.13.27
\begin{equation} \begin{aligned} \int _ X \left(\Gamma _ t^{*,N,M+1}-\Gamma _ t^{*,N,M}\right)\, \theta ^ n_{\Gamma _ t^{*,N,M+1}}\leq & E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,M+1}\right)-E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,M}\right)\\ \leq & \int _ X \left(\Gamma _ t^{*,N,M+1}-\Gamma _ t^{*,N,M}\right)\, \theta ^ n_{\Gamma _ t^{*,N,M}}. \end{aligned} \end{equation}

Clearly $\Gamma _ t^{*,N,M+1} \geq \Gamma _ t^{*,N,M}$. Moreover, since $\mathbb {R}\ni \tau \mapsto \Gamma _{\tau }+t\tau $ is concave, we notice that

\[ U_ t \coloneqq \left\{ \Gamma ^{*,N,M+1}_ t>\Gamma ^{*,N,M}_ t\right\} = \left\{ \Gamma _{(M+1)/2^ N} + 2^{-N}t >\Gamma _{M/2^ N}\right\} , \]

and on $U_ t$ we have

23E6778F003A 17.13.28
\begin{equation} \Gamma _ t^{*,N,M+1} = \Gamma _{(M+1)/2^ N} + t (M+1)/2^{N},\quad \Gamma _ t^{*,N,M} = \Gamma _{M/2^ N} + t M /2^{N}. \end{equation}

We also note that $U_ t$ is $\mathcal{F}$-open by corollary 5.15.19. So from the lower bound in (17.13.27), we have

\[ \begin{aligned} E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,M+1}\right)-E_{\theta }^{\phi }\left(\Gamma _ t^{*,N,M}\right)\geq & \int _{U_ t} \left(\Gamma _ t^{*,N,M+1}-\Gamma _ t^{*,N,M}\right)\, \theta ^ n_{\Gamma _ t^{*,N,M+1}}\\ = & \int _{U_ t} \left(\Gamma _{(M+1)/2^ N}-\Gamma _{M/2^ N}+t2^{-N}\right)\, \theta ^ n_{\Gamma _{(M+1)/2^ N}}\\ \geq & \int _{\left\{ \Gamma _{(M+1)/2^ N}=0\right\} }t2^{-N}\, \theta ^ n_{\Gamma _{(M+1)/2^ N}}, \end{aligned} \]

where on the second line, we applied (17.13.28) and proposition 13.11.4, on the third line, we applied the fact that $\theta _{\Gamma _{(M+1)/2^ N}}^ n$ is supported on the set (cf. theorem 16.3.12)

\[ \left\{ \Gamma _{(M+1)/2^ N}=0\right\} \subseteq U_ t\cap \left\{ \Gamma _{M/2^ N}=0\right\} . \]

When $(M+1)/2^ N=0$, we use proposition 16.4.3 to see that $P_\theta [\Gamma _0]=\Gamma _0$, since $\Gamma _0$ is the decreasing limit of the model potentials $\Gamma _\tau $ as $\tau \nearrow 0$. Thus theorem 16.3.12 applies to this endpoint as well.

We have deduced the first inequality in (17.13.25). Next, we apply the upper bound part in (17.13.27) and compute similarly

\[ \begin{aligned} E_{\theta }^{\phi }(\Gamma _ t^{*,N,M+1})-E_{\theta }^{\phi }(\Gamma _ t^{*,N,M})\leq & \int _ X \left(\Gamma _ t^{*,N,M+1}-\Gamma _ t^{*,N,M}\right)\, \theta ^ n_{\Gamma _ t^{*,N,M}}\\ =& \int _{U_ t} \left(\Gamma _{(M+1)/2^ N}-\Gamma _{M/2^ N}+t2^{-N}\right)\, \theta ^ n_{\Gamma _{M/2^ N}}\\ \leq & \int _{\{ \Gamma _{M/2^ N}=0\} \cap U_ t}\left(\Gamma _{(M+1)/2^ N}+t2^{-N}\right)\, \theta ^ n_{\Gamma _{M/2^ N}} \\ \leq & \int _{\{ \Gamma _{M/2^ N}=0\} \cap U_ t} t2^{-N}\, \theta ^ n_{\Gamma _{M/2^ N}}. \end{aligned} \]

We conclude the latter half of (17.13.25).

Step 3.3. We assume that $\Gamma _{\max }=0$. Now $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$ only.

For each $\epsilon >0$, we introduce $\Gamma ^{\epsilon }\in \mathrm{TC}^{\infty }(X,\theta ;\phi )$ as follows:

  1. 1E08B0569766

    Let $\Gamma ^{\epsilon }_{\max }=0$, and

  2. 70863808F7A7

    we set

    \[ \Gamma ^{\epsilon }_{\tau }= \begin{cases} \phi ,& \textup{if }\tau \leq -\epsilon ^{-1};\\ P_{\theta }\left[ (1+\epsilon \tau )\Gamma _{\tau }-\epsilon \tau \phi \right],& \textup{if }\tau \in \left(-\epsilon ^{-1},0\right). \end{cases} \]

The concavity and monotonicity in $\tau $ follow from proposition 16.4.2. The value at $-\infty $ is $\phi $. Moreover, $\Gamma ^\epsilon _\tau =\phi $ for $\tau \leq -\epsilon ^{-1}$, so $\Gamma ^\epsilon \in \mathrm{TC}^\infty (X,\theta ;\phi )$.

It follows from corollary 16.9.38 and corollary 16.9.14 that for each $\tau <0$, the potentials $\Gamma ^{\epsilon }_{\tau }$ decrease to $\Gamma _{\tau }$ as $\epsilon \searrow 0$. Applying proposition 16.4.4, we have

\[ \lim _{\epsilon \to 0+} \int _ X \left(\theta +\mathrm{dd}^{\mathrm{c}}\Gamma ^{\epsilon }_{\tau }\right)^ n=\int _ X \left(\theta +\mathrm{dd}^{\mathrm{c}}\Gamma _{\tau }\right)^ n \]

for all $\tau <0$. Hence, by the monotone convergence theorem and Step 3.2, we find

DBCF50A40C12 17.13.29
\begin{equation} \mathbf{E}^{\phi }(\Gamma )=\lim _{\epsilon \to 0+}\mathbf{E}^{\phi }(\Gamma ^{\epsilon })=\lim _{\epsilon \to 0+}\mathbf{E}^{\phi }(\Gamma ^{\epsilon *})=\lim _{\epsilon \to 0+} E_{\theta }^{\phi }(\Gamma ^{\epsilon *}_1), \end{equation}

where the last equality follows from (17.13.26). Furthermore, according to proposition 21.11.36, we have

\[ \Gamma ^*_ t=\inf _{\epsilon >0} \Gamma ^{\epsilon *}_ t \]

for all $t>0$. Note that we do not have to take the closure of the right-hand side since it is automatically upper semicontinuous in $t$.

Now suppose that $\Gamma \in \mathrm{TC}^1(X,\theta ;\phi )$. Then by (17.13.29), as $\epsilon \to 0+$, $(\Gamma _ t^{\epsilon *})_{\epsilon }$ is a decreasing Cauchy net in $\mathcal{E}^1(X,\theta ;\phi )$ and hence by theorem 17.10.63 for each $t>0$,

\[ E_{\theta }^{\phi }\left(\Gamma ^*_ t\right)=\lim _{\epsilon \to 0+}E_{\theta }^{\phi }\left(\Gamma ^{\epsilon ,*}_ t\right)=t\mathbf{E}^{\phi }(\Gamma )>-\infty , \]

where we have applied (17.13.26) and (17.13.29). Hence, $\Gamma ^*\in \mathcal{R}^1(X,\theta ;\phi )$. Moreover, (17.13.24) follows.

Conversely, suppose that $\Gamma ^*\in \mathcal{R}^1(X,\theta ;\phi )$. Then (17.13.29) implies that

\[ \mathbf{E}^{\phi }(\Gamma )=\lim _{\epsilon \to 0+} E_{\theta }^{\phi }\left(\Gamma ^{\epsilon *}_1\right) \geq E_{\theta }^{\phi }\left(\Gamma ^*_1\right)>-\infty . \]

Hence, $\Gamma \in \mathrm{TC}^1(X,\theta ;\phi )$. $\square$

Remark 17.13.30.E10A1DEDC7AF One could also consider geodesic rays emanating from another potential $\Phi \in \mathcal{E}(X,\theta ;\phi )$. In this case, one can show that these geodesic rays are in bijection with $\Phi $-twisted test curves: In definition 17.12.1, we replace 2 by the following condition:

\[ P_{\theta }\left[\Gamma _{\tau }\right](\Phi )=\Gamma _{\tau }. \]

Furthermore, we require that $\Gamma _{-\infty }=\Phi $.

The above results equally work in the twisted setting. The proofs are almost identical to the untwisted case.

Corollary 17.13.31.82AB68443E01 Let $\ell \in \mathcal{R}(X,\theta ;\phi )$. Then $\sup _ X \ell _ t=\ell ^*_{\max }t$ for any $t\geq 0$.

In particular, $\ell _ t-\ell ^*_{\max }t$ is a decreasing function of $t\geq 0$.

Example 17.13.32.E2332A16AF00 Let us see what the test curve in example 17.12.13 corresponds to under the Ross–Witt Nyström correspondence. Fix $\varphi \in \mathrm{PSH}(X,\theta )$. We claim that

D50F33814868 17.13.33
\begin{equation} \ell ^{\varphi }=\Gamma ^{\varphi *}, \end{equation}

where $\ell ^{\varphi }$ is as in example 17.10.92. We may assume that $\varphi \leq 0$ since both sides are invariant after adding a constant to $\varphi $.

We first prove the easy direction $\ell ^{\varphi }\geq \Gamma ^{\varphi *}$, which is equivalent to $\ell ^{\varphi *}\geq \Gamma ^{\varphi }$. Since $\ell ^{\varphi *}$ is a test curve, the latter is equivalent to

\[ \ell ^{\varphi *}_{\tau }\geq (1+\tau )\varphi -\tau V_{\theta } \]

for all $\tau \in (-1,0)$. By Legendre duality, this is equivalent to

F5A9BEF8F7BA 17.13.34
\begin{equation} \ell ^{\varphi }_ t\geq \sup _{\tau \in (-1,0)} \Bigl ((1+\tau )\varphi -\tau V_{\theta }+t\tau \Bigr )=\varphi \lor (V_{\theta }-t) \end{equation}

for all $t>0$.

Using the notations of example 17.10.92, we find easily that

\[ \ell ^{\varphi ,C}_ t\geq \varphi \lor (V_{\theta }-t) \]

for any $C>0$ and $t\in [0,C]$, since it holds at $t=0$ and $t=C$. Letting $C\to \infty $, we find (17.13.34). Therefore, $\ell ^{\varphi }\geq \Gamma ^{\varphi *}$ follows.

In order to prove the equality in (17.13.33), it suffices to show that the two sides have the same energy, as a consequence of (17.10.84). So we compute

\[ \begin{aligned} \mathbf{E}\left(\Gamma ^{\varphi *}\right)=& \mathbf{E}\left(\Gamma ^{\varphi }\right)\\ =& \int _{-1}^0 \left(\int _ X \theta _{(1+\tau )\varphi -\tau V_{\theta }}^ n-\int _ X \theta _{V_{\theta }}^ n\right)\, \mathrm{d}\tau \\ =& \sum _{j=0}^{n} \binom {n}{j} \int _ X \theta _{\varphi }^{j}\wedge \theta _{V_{\theta }}^{n-j} \int _0^1 \tau ^ j (1-\tau )^{n-j}\, \mathrm{d}\tau -\int _ X \theta _{V_{\theta }}^ n\\ =& \sum _{j=0}^{n} \binom {n}{j}\frac{j!(n-j)!}{(n+1)!} \int _ X \theta _{\varphi }^{j}\wedge \theta _{V_{\theta }}^{n-j}-\int _ X \theta _{V_{\theta }}^ n\\ =& \mathbf{E}(\ell ^{\varphi }), \end{aligned} \]

where in the second line we used proposition 16.3.10, in the fourth line we used the value of the $\beta $-function2, and the last line is just (17.10.94).

The multiplier ideal sheaves of a test curve can be characterized using the corresponding geodesic ray in a very simple manner.

Proposition 17.13.35 (He–Testorf–Wang).E6915C7339CD Let $\ell \in \mathcal{R}(X,\theta ;\phi )$. Given any $\tau <\ell ^*_{\max }$ and $x\in X$, we have

DA238F3ECC6F 17.13.36
\begin{equation} \mathcal{I}\left(\ell ^*_{\tau }\right)_{x}=\left\{ f\in \mathcal{O}_{X,x}: |f|^2\int _0^{\infty } \exp (-\ell _ t+t\tau )\, \mathrm{d}t \textup{ is integrable near }x \right\} . \end{equation}

Proof. Fix $x\in X$, $\tau <\ell ^*_{\max }$ and $f\in \mathcal{O}_{X,x}$. Fix a Kähler form $\omega $ on $X$.

Step 1. We first assume that $f$ lies in the right-hand side of (17.13.36).

Given any $y\in X$, it follows from (17.13.14) that there is $t_0>0$ with

\[ \ell ^*_{\tau }(y)+1\geq \ell _{t_0}(y)-t_0\tau . \]

Observe that $t\mapsto \ell _ t-t\ell ^*_{\max }$ is decreasing in $t$ by corollary 17.13.31, it follows that for $t\in [t_0,t_0+1]$, we have

\[ \ell ^*_{\tau }(y)+1-t_0(\ell ^*_{\max }-\tau )\geq \ell _{t_0}(y)-t_0\ell ^*_{\max }\geq \ell _{t}(y)-t\ell ^*_{\max }. \]

Since $\tau < \ell ^*_{\max }$ and $t_0\geq t-1$, we deduce that

77E18B7AC795 17.13.37
\begin{equation} \ell ^*_{\tau }(y)+1+\ell ^*_{\max }-\tau \geq \ell _{t}(y)-t\tau ,\quad t\in [t_0,t_0+1]. \end{equation}

Take a sufficiently small open neighborhood $U$ of $x$ such that

\[ \int _ U |f|^2\int _0^{\infty } \exp (-\ell _ t+t\tau )\, \mathrm{d}t\, \omega ^ n<\infty . \]

Applying (17.13.37), we deduce that

\[ \int _ U |f|^2\exp \left(-\ell ^*_{\tau }\right)\, \omega ^ n<\infty . \]

Therefore, $f\in \mathcal{I}(\ell ^*_{\tau })_ x$.

Step 2. Assume that $f\in \mathcal{I}(\ell ^*_{\tau })_ x$.

It follows from the strong openness theorem theorem 5.16.21 (cf. (17.12.5)) that $f\in \mathcal{I}(\ell ^*_{\tau +\epsilon })_ x$ for some small enough $\epsilon >0$ with $\tau +\epsilon <\ell ^*_{\max }$. Take a sufficiently small open neighborhood $U$ of $x$ such that

\[ \int _ U |f|^2 \exp \left(-\ell ^*_{\tau +\epsilon }\right)\, \omega ^ n<\infty . \]

We compute

\[ \begin{aligned} \int _ U |f|^2\int _0^{\infty } \exp \left(-\ell _ t+t\tau \right)\, \mathrm{d}t\, \omega ^ n\leq & \int _ U |f|^2\int _0^{\infty } \exp \left(-\ell ^*_{\tau +\epsilon }-t\epsilon \right)\, \mathrm{d}t\, \omega ^ n\\ =& \frac{1}{\epsilon }\int _ U |f|^2\exp \left(-\ell ^*_{\tau +\epsilon }\right)\, \omega ^ n\\ <& \infty . \end{aligned} \]

Therefore, $f$ lies in the right-hand side of (17.13.36). $\square$

The masses of potentials on a test curve can also be expressed in terms of the corresponding geodesic ray.

Proposition 17.13.38 (Hisamoto).3746B0074A79 Let $\ell \in \mathcal{R}(X,\theta ;\phi )$. Given any $\tau <\ell ^*_{\max }$, we have

16A5FF346A3B 17.13.39
\begin{equation} \int _ X \left(\theta +\mathrm{dd}^{\mathrm{c}}\ell ^*_{\tau }\right)^ n=\int _{\{ \dot{\ell }_0\geq \tau \} } \theta _{\phi }^ n. \end{equation}
Here $\dot{\ell }_0$ denotes the right-derivative of $\ell _ t$ with respect to $t$ at $t=0$. It is well-defined quasi-everywhere by corollary 17.10.9, and hence the right-hand side of (17.13.39) makes sense, even though $\{ \dot{\ell }_0\geq \tau \} $ is not well-defined.

Proof. Fix $\tau <\ell ^*_{\max }$. We first observe that it suffices to show that

0893138962D7 17.13.40
\begin{equation} \int _{\left\{ \dot{\ell }_0\geq \tau \right\} } \theta _{\phi }^ n=\int _{\left\{ \ell ^*_{\tau }=\phi \right\} } \theta _{\phi }^ n. \end{equation}

Assuming (17.13.40) for the moment. By theorem 17.13.21, $\ell ^*\in \mathrm{TC}(X,\theta ;\phi )$. In particular, $\ell ^*_\tau $ is a model potential and

\[ \ell ^*_\tau \leq \ell ^*_{-\infty }=\phi . \]

Since $\phi $ is model as well, proposition 16.3.41 gives

\[ \theta ^ n_{\ell ^*_{\tau }}=\mathds {1}_{\left\{ \ell ^*_{\tau }=0\right\} }\, \theta ^ n,\quad \theta ^ n_{\phi }=\mathds {1}_{\{ \phi =0\} }\, \theta ^ n. \]

Since $\ell ^*_{\tau }\leq \phi \leq 0$, we have

\[ \mathds {1}_{\left\{ \ell ^*_{\tau }=\phi \right\} }\, \theta _{\phi }^ n =\mathds {1}_{\left\{ \ell ^*_{\tau }=\phi =0\right\} }\, \theta ^ n =\mathds {1}_{\left\{ \ell ^*_{\tau }=0\right\} }\, \theta ^ n =\theta ^ n_{\ell ^*_{\tau }}. \]

Therefore, (17.13.39) follows from (17.13.40).

In order to prove (17.13.40), it suffices to show that

7F6505CF081C 17.13.41
\begin{equation} \left\{ \dot{\ell }_0\geq \tau \right\} =\left\{ \ell ^*_{\tau }=\phi \right\} \quad \textup{outside a pluripolar set}. \end{equation}

Take $x\in X$ so that $(\ell _ t(x))_{t\geq 0}$ is finite and right-differentiable at $t=0$. Note that this condition holds quasi-everywhere. Suppose that $\ell ^*_{\tau }(x)=\phi (x)$. Then

\[ \dot{\ell }_0(x)=\inf _{t>0} \frac{\ell _ t(x)-\phi (x)}{t}\geq \inf _{t>0} \frac{\ell ^*_{\tau }(x)+t\tau -\phi (x)}{t}=\tau . \]

Therefore, the $\supseteq $ direction in (17.13.41) follows. Conversely, suppose that $\dot{\ell }_0(x)\geq \tau $, then

\[ \ell ^*_{\tau }(x)=\inf _{t>0} \left(\ell _ t(x)-t\tau \right)\geq \inf _{t>0} \left(\phi (x)+t\dot{\ell }_0(x)-t\tau \right)\geq \phi (x). \]

Together with $\ell ^*_\tau \leq \phi $, this gives $\ell ^*_\tau (x)=\phi (x)$. Therefore, the $\subseteq $ direction in (17.13.41) follows as well. $\square$

Corollary 17.13.42.F147312B98B3 Let $\ell \in \mathcal{R}^1(X,\theta ;\phi )$. Then $\dot{\ell }_0\in L^1(X,\theta _{\phi }^ n)$ and

DA97CC2A78DC 17.13.43
\begin{equation} \mathbf{E}^{\phi }(\ell )=\int _ X \dot{\ell }_0\, \theta _{\phi }^ n. \end{equation}

In particular, for every $t\geq 0$,

\[ E_{\theta }^{\phi }(\ell _ t)=t\int _ X \dot{\ell }_0\, \theta _{\phi }^ n. \]

Proof. Set $\Gamma =\ell ^*$. By theorem 17.13.21, we have $\Gamma \in \mathrm{TC}^1(X,\theta ;\phi )$ and

\[ \mathbf{E}^{\phi }(\ell )=\mathbf{E}^{\phi }(\Gamma ). \]

By proposition 17.13.38, for every $\tau <\ell ^*_{\max }$,

\[ \int _ X \theta _{\Gamma _{\tau }}^ n=\int _{\{ \dot{\ell }_0\geq \tau \} } \theta _{\phi }^ n. \]

Hence (17.12.12) gives

\[ \mathbf{E}^{\phi }(\ell ) =\ell ^*_{\max }\int _ X \theta _{\phi }^ n-\int _{-\infty }^{\ell ^*_{\max }} \int _{\{ \dot{\ell }_0<\tau \} }\theta _{\phi }^ n\, \mathrm{d}\tau . \]

For $\tau >\ell ^*_{\max }$, we have $\ell ^*_{\tau }\equiv -\infty $ by 17.13.15. Then (17.13.40) shows that

\[ \int _{\{ \dot{\ell }_0\geq \tau \} }\theta _{\phi }^ n=0. \]

The layer-cake formula therefore gives (17.13.43). The final assertion follows from proposition 17.10.65, since $E_{\theta }^{\phi }(\ell _0)=E_{\theta }^{\phi }(\phi )=0$. $\square$

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