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
C9D15D724069C9D15D724069
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
It is sometimes handy to define
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 $.
Proposition 17.13.5.1F48BF7602CA Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. Then
24A2034A1287
17.13.6
for all $\tau \in \mathbb {R}$.
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. $\square$
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
Let $R=\{ a+\mathrm{i}b\in \mathbb {C}:a>0,b\in \mathbb {R}\} $. We consider
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
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
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
On the other hand, let
DBF41B839C63
17.13.8
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,
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
From (17.13.2) and proposition 16.8.28, we know that
This completes the proof. $\square$
Lemma 17.13.10.C6092031D5B3 Let $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$. Then
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
for all $t>0$. Conversely, for each $\tau <\Gamma _{\max }$,
Letting $\tau \to \Gamma _{\max }$ gives the reverse inequality. The final assertion follows directly from the formula
This completes the proof. $\square$
Lemma 17.13.11.9C6538C4298E Given $\Gamma \in \mathrm{TC}(X,\theta ;\phi )$, we have $\Gamma ^*\in \mathcal{R}(X,\theta ;\phi )$.
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
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 $t>0$,
Therefore, $\psi \leq \phi $. On the other hand, for any fixed $\tau <\Gamma _{\max }$, by (17.13.2), we have
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
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
Observe that $\Gamma '_{\tau }\equiv -\infty $ when $\tau >\Gamma _{\max }$ by 17.13.10. Thus it suffices to consider $\tau \leq \Gamma _{\max }$. Put
For any $s\in [a,b]$, the monotonicity of $t\mapsto \Gamma _ t^*-t\Gamma _{\max }$ from 17.13.10 gives
Since $\ell _ b=\Gamma _ b^*$, we get
For $s\notin [a,b]$, we have $\ell _ s=\Gamma _ s^*$, hence
Taking the infimum over all $s>0$ gives
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 $\tau <\Gamma _{\max }$,
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
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,
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
by proposition 5.14.2.
On the other hand, for $\tau >\sup _ X \ell _1$, the same argument shows that
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
Therefore,
5BF1777D23C2
17.13.16
Also observe that for any $\tau \leq \ell ^*_{\max }$ and any $t>0$, we have
Letting $t\to 0+$, we find that for any $\tau \leq \ell ^*_{\max }$, we have
Fix $\tau <\ell ^*_{\max }$. We want to argue that
59C9610616F1
17.13.18
First we claim that for any $C>0$, we have
25F16D030FA9
17.13.19
The $\leq $ direction is trivial. We argue the reverse inequality, which reduces to
Since $\phi $ is model and $(\ell ^*_{\tau }+C)\land V_{\theta }\leq 0$, it suffices to show that
which follows from (17.13.16). Therefore, (17.13.19) is established. Thanks to (17.13.17), we have the obvious inequality
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
For this purpose, let us consider the following geodesics: For any $M>0$ and $t\in [0,1]$, let
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
for all $M>0$. Taking infimum with respect to $M>0$, we find
Since $s\in (0,1]$ is arbitrary, we conclude (17.13.20).
Finally, we check the condition at $-\infty $. Set
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
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
Moreover, this bijection restricts to the following bijections:
AE510D6D0C2F
17.13.23
For any $\Gamma \in \mathrm{TC}^1(X,\theta ;\phi )$, we have
4884EC5C8FA9
17.13.24
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
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
Therefore, according to (17.13.14), we have
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
Then $\Gamma '\in \mathrm{TC}(X,\theta ;\phi )$ as well and for all $t>0$,
Therefore,
by (16.5.13). Using (17.12.12), we also have
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:
We first claim that for all $t>0$, $N\in \mathbb {Z}_{>0}$ and $M\in \mathbb {Z}_{<0}$,
1C55A624E61E
17.13.25
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
Since $M \leq 2^{N}\Gamma _{\min }$, we have
Using (16.5.13), we can continue to write
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
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
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
and on $U_ t$ we have
23E6778F003A
17.13.28
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
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)
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
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:
1E08B0569766Let $\Gamma ^{\epsilon }_{\max }=0$, and
70863808F7A7we set
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
for all $\tau <0$. Hence, by the monotone convergence theorem and Step 3.2, we find
DBCF50A40C12
17.13.29
where the last equality follows from (17.13.26). Furthermore, according to proposition 21.11.36, we have
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 $t>0$,
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
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:
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 $t\geq 0$.
Proof. This follows from 17.13.10 and theorem 17.13.21. $\square$
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
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
for all $\tau \in (-1,0)$. By Legendre duality, this is equivalent to
F5A9BEF8F7BA
17.13.34
for all $t>0$.
Using the notations of example 17.10.92, we find easily that
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
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).
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
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
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
Since $\tau < \ell ^*_{\max }$ and $t_0\geq t-1$, we deduce that
77E18B7AC795
17.13.37
Take a sufficiently small open neighborhood $U$ of $x$ such that
Applying (17.13.37), we deduce that
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
We compute
Therefore, $f$ lies in the right-hand side of (17.13.36). $\square$
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
Proof. Fix $\tau <\ell ^*_{\max }$. We first observe that it suffices to show that
0893138962D7
17.13.40
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
Since $\phi $ is model as well, proposition 16.3.41 gives
Since $\ell ^*_{\tau }\leq \phi \leq 0$, we have
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
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
Therefore, the $\supseteq $ direction in (17.13.41) follows. Conversely, suppose that $\dot{\ell }_0(x)\geq \tau $, then
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
In particular, for every $t\geq 0$,
Proof. Set $\Gamma =\ell ^*$. By theorem 17.13.21, we have $\Gamma \in \mathrm{TC}^1(X,\theta ;\phi )$ and
By proposition 17.13.38, for every $\tau <\ell ^*_{\max }$,
Hence (17.12.12) gives
For $\tau >\ell ^*_{\max }$, we have $\ell ^*_{\tau }\equiv -\infty $ by 17.13.15. Then (17.13.40) shows that
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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