Theorem 16.8.32.1CA975F04423 Let $\varphi _0,\varphi _1\in \mathrm{PSH}(X,\theta )_{>0}$. Then the following are equivalent:
8E345DA2D98AThere is a subgeodesic from $\varphi _0$ to $\varphi _1$;
5498C9F0BF2D$\varphi _0\sim _ P\varphi _1$.
1CA975F04423Theorem 16.8.32.1CA975F04423 Let $\varphi _0,\varphi _1\in \mathrm{PSH}(X,\theta )_{>0}$. Then the following are equivalent:
8E345DA2D98AThere is a subgeodesic from $\varphi _0$ to $\varphi _1$;
5498C9F0BF2D$\varphi _0\sim _ P\varphi _1$.
Proof. 2 $\implies $ 1. This follows from proposition 17.10.24.
1 $\implies $ 2. Let $(\varphi _ t)_{t\in (0,1)}$ be a subgeodesic from $\varphi _0$ to $\varphi _1$.
Step 1. We assume that $\varphi _0\geq \varphi _1$.
We first replace the given subgeodesic by the geodesic from $\varphi _0$ to $\varphi _1$. Note that the geodesic is necessarily a subgeodesic as well by 17.10.22.
Observe that $t\mapsto \varphi _ t$ is decreasing due to 17.10.28.
Let $\varphi _ t=\varphi _1$ for all $t>1$. Then by the gluing lemma 17.10.16, we find that $(\varphi _ t)_{t\geq 0}$ is a subgeodesic ray.
Next, we consider the Legendre transform
It follows from Kiselman's principle proposition 5.14.15 that $\Gamma _{\tau }\in \mathrm{PSH}(X,\theta )\cup \{ -\infty \} $. Note that for $\tau >0$, we clearly have $\Gamma _{\tau }\equiv -\infty $. On the other hand, for $\tau \leq 0$,
By Legendre inversion (cf. corollary 21.11.26), for $t>0$,
Fix a Kähler form $\omega $ on $X$. It follows from proposition 16.8.28 that for each $t>0$,
The right-hand side is independent of $t$. Here by adding $\omega $, we no longer have to worry about the possibility where $\Gamma _{\tau }$ has vanishing mass.
Write
By proposition 16.8.28 again, we find that
as well. So $\varphi _0\sim _ P \varphi _1$.
Step 2. We prove the general case.
Observe that $(\varphi _ t\lor \varphi _1)_{t\in (0,1)}$ is a subgeodesic from $\varphi _0\lor \varphi _1$ to $\varphi _1$. By Step 1,
Hence $\varphi _0\preceq _ P \varphi _1$ by 16.8.13. The converse is proved similarly. Hence 2 follows. $\square$
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