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17.3 Relative Monge–Ampère energyEC60D9ED3C42

EC60D9ED3C42

Fix a smooth closed real $(1,1)$-form $\theta $ whose class is big, and a model potential $\phi \in \mathrm{PSH}(X,\theta )$, that is, $P_\theta [\phi ]=\phi $ and $m=\int _ X\langle \theta _\phi ^ n\rangle >0$ (definition 16.21.1). In particular $\phi \leq 0$ and $\sup _ X\phi =0$. Recall from definition 13.9.3 that $\mathcal E(X,\theta ,\phi )$ consists of the potentials $u\preceq \phi $ with $\int _ X\langle \theta _ u^ n\rangle =m$. If $u_1,\ldots ,u_ n\in \mathcal E(X,\theta ,\phi )$, then

\[ \int _ X\langle \theta _{u_1}\wedge \cdots \wedge \theta _{u_ n}\rangle =m. \]

Indeed $P_\theta [u_ j]=P_\theta [\phi ]=\phi $ by proposition 16.22.14, and the singularity envelope preserves mixed masses by proposition 16.21.2.

Definition 17.3.1.8F92EE4FC37C Put

\[ \begin{aligned} \mathcal E^\infty (X,\theta ,\phi ) & =\{ u\in \mathrm{PSH}(X,\theta ):u\sim \phi \} ,\\ \mathcal E^1(X,\theta ,\phi ) & =\left\{ u\in \mathcal E(X,\theta ,\phi ): \int _ X|u-\phi |\, \mu _ u<\infty \right\} . \end{aligned} \]

The potentials in $\mathcal E^\infty (X,\theta ,\phi )$ have bounded difference from $\phi $, but they need not be bounded functions. The class $\mathcal E^1(X,\theta ,\phi )$ is the relative finite-energy class. For the potential $\phi =V_\theta $ with minimal singularities (definition 10.3.7) we omit the reference from these notations.

If $u\sim \phi $, then $\int _ X\langle \theta _ u^ n\rangle =m$ by corollary 13.8.8, and $|u-\phi |$ is bounded. Hence
\[ \mathcal E^\infty (X,\theta ,\phi )\subset \mathcal E^1(X,\theta ,\phi )\subset \mathcal E(X,\theta ,\phi ). \]

The potential $V_\theta $ is indeed a model potential: $P_\theta [V_\theta ]=V_\theta $ by proposition 16.21.2(4), and $\int _ X\langle \theta _{V_\theta }^ n\rangle =\operatorname {vol}(\{ \theta \} )>0$ by definition 13.9.1, proposition 13.9.2. For $\phi =V_\theta $, the class $\mathcal E^\infty (X,\theta )$ consists of the potentials with minimal singularities, and $\mathcal E(X,\theta )=\mathcal E(X,\theta ,V_\theta )$ is the class of potentials of full Monge–Ampère mass of definition 13.9.3. These classes of global potentials are not related to the local class $\mathcal E_0(B)$ of bounded functions on a ball in definition 7.11.1.

Definition 17.3.2.240EF1DE5889 For $u\in \mathcal E^\infty (X,\theta ,\phi )$ define

F19AAFA93177 17.3.3
\begin{equation} E_\theta ^\phi (u)=\frac1{n+1}\sum _{j=0}^ n \int _ X(u-\phi )\, \langle \theta _ u^ j\wedge \theta _\phi ^{n-j}\rangle . \end{equation}

All these integrals are finite, since the weight is bounded and every mixed measure has total mass $m$. For $\phi =V_\theta $ we write $E_\theta $.

Proposition 17.3.4.9086ABF36774 Let $u,v\in \mathcal E^\infty (X,\theta ,\phi )$ and put $u_ t=(1-t)u+tv$ for $0\leq t\leq 1$. Then

46190A7C1B2F 17.3.5
\begin{equation} \frac{\mathrm d}{\mathrm dt}E_\theta ^\phi (u_ t) =\int _ X(v-u)\, \mu _{u_ t}, \end{equation}

with one-sided derivatives at the endpoints, and

BC6BC1B194C2 17.3.6
\begin{equation} E_\theta ^\phi (v)-E_\theta ^\phi (u) =\frac1{n+1}\sum _{j=0}^ n\int _ X(v-u) \langle \theta _ v^ j\wedge \theta _ u^{n-j}\rangle . \end{equation}

In particular, the energy is increasing, and $E_\theta ^\phi (u+C)=E_\theta ^\phi (u)+Cm$ for every constant $C$.

Proof. Let $w\in \mathcal E^\infty (X,\theta ,\phi )$. For $0\leq r\leq 1$ the potential $\phi +r(w-\phi )=(1-r)\phi +rw$ again belongs to $\mathcal E^\infty (X,\theta ,\phi )$, and multilinearity gives

\[ \mu _{\phi +r(w-\phi )}=\sum _{j=0}^ n\binom nj r^ j(1-r)^{n-j}\langle \theta _ w^ j\wedge \theta _\phi ^{n-j}\rangle . \]

Since $\binom nj\int _0^1r^ j(1-r)^{n-j}\, \mathrm dr=1/(n+1)$, as one sees by integrating by parts $j$ times, we obtain

73519BE96F0E 17.3.7
\begin{equation} E_\theta ^\phi (w)=\int _0^1\int _ X(w-\phi )\, \mu _{\phi +r(w-\phi )}\, \mathrm dr. \end{equation}

Now put $h=v-u$ and $q_{r,t}=\phi +r(u_ t-\phi )$. Since $\theta _{q_{r,t}}=(1-r)\theta _\phi +r(1-t)\theta _ u+rt\theta _ v$, the measures $\mu _{q_{r,t}}$ are polynomials in $(r,t)$ whose coefficients are mixed measures of total mass $m$, and the weights $u_ t-\phi =(u-\phi )+th$ are bounded. All expressions below are therefore polynomials in $(r,t)$ with finite coefficients, and the derivatives are derivatives of polynomials. Identities between such polynomials of measures follow from the corresponding identities between polynomials in commuting variables $x,y,z$, by substituting the mixed measure $\langle \theta _\phi ^ a\wedge \theta _ u^ b\wedge \theta _ v^ c\rangle $ for the monomial $x^ ay^ bz^ c$; multilinearity shows that this substitution is compatible with the products occurring here. For instance, the identities $\partial _ t\ell ^ n=nr(z-y)\ell ^{n-1}$ and $\partial _ r\ell ^ n=n\bigl ((1-t)y+tz-x\bigr )\ell ^{n-1}$ for $\ell =(1-r)x+r(1-t)y+rtz$ give

25D7DD3C6946 17.3.8
\begin{equation} \partial _ t\mu _{q_{r,t}}=nr\, \mathrm{dd}^{\mathrm{c}}h\wedge \langle \theta _{q_{r,t}}^{n-1}\rangle ,\qquad \partial _ r\mu _{q_{r,t}}=n\, \mathrm{dd}^{\mathrm{c}}(u_ t-\phi )\wedge \langle \theta _{q_{r,t}}^{n-1}\rangle , \end{equation}

in the sense of (17.2.1). Differentiating (17.3.7) with $w=u_ t$ and using the first of these identities, we obtain

\[ \frac{\mathrm d}{\mathrm dt}E_\theta ^\phi (u_ t) =\int _0^1\left[\int _ Xh\, \mu _{q_{r,t}} +nr\int _ X(u_ t-\phi )\, \mathrm{dd}^{\mathrm{c}}h\wedge \langle \theta _{q_{r,t}}^{n-1}\rangle \right]\mathrm dr. \]

By theorem 17.2.5, applied to the bounded quasi-psh differences $u_ t-\phi $ and $h$, the second integral equals $\int _ Xh\, \mathrm{dd}^{\mathrm{c}}(u_ t-\phi )\wedge \langle \theta _{q_{r,t}}^{n-1}\rangle $, which is $\frac1n\partial _ r\int _ Xh\, \mu _{q_{r,t}}$ by the second identity. The integrand in $r$ is therefore $\partial _ r\bigl [r\int _ Xh\, \mu _{q_{r,t}}\bigr ]$, and since $q_{1,t}=u_ t$,

\[ \frac{\mathrm d}{\mathrm dt}E_\theta ^\phi (u_ t)=\int _ Xh\, \mu _{u_ t}. \]

This is (17.3.5). Integrating it from $t=0$ to $t=1$, and expanding $\mu _{u_ t}=\sum _ j\binom nj t^ j(1-t)^{n-j}\langle \theta _ v^ j\wedge \theta _ u^{n-j}\rangle $ with the same beta integrals, gives (17.3.6). If $u\leq v$, every term of the cocycle formula is nonnegative, so the energy is increasing. Every mixed measure has total mass $m$, so taking $v=u+C$ in the cocycle formula gives the last assertion. $\square$

Proposition 17.3.9.356D15D0C316 The energy is concave on $\mathcal E^\infty (X,\theta ,\phi )$, and for $u,v\in \mathcal E^\infty (X,\theta ,\phi )$,

26A7B21B6397 17.3.10
\begin{equation} \int _ X(v-u)\, \mu _ v \leq E_\theta ^\phi (v)-E_\theta ^\phi (u) \leq \int _ X(v-u)\, \mu _ u. \end{equation}

Moreover $|E_\theta ^\phi (v)-E_\theta ^\phi (u)|\leq m\sup |v-u|$, the supremum being taken over the common finite locus. If $\psi \in \mathrm{PSH}(X,\theta )$ and $\psi \sim \phi $, then the functional $E_\theta ^\psi $ defined by (17.3.3) with $\psi $ in place of $\phi $ satisfies

\[ E_\theta ^\psi (u)=E_\theta ^\phi (u)-E_\theta ^\phi (\psi ). \]

Proof. Let $u_ t=(1-t)u+tv$ and $h=v-u$. Then $\partial _ t\mu _{u_ t}=n\, \mathrm{dd}^{\mathrm{c}}h\wedge \langle \theta _{u_ t}^{n-1}\rangle $. Indeed, by multilinearity and (17.2.1), both sides expand into combinations of the mixed measures $\langle \theta _ u^ a\wedge \theta _ v^{n-a}\rangle $, obtained by substituting $\langle \theta _ u^ a\wedge \theta _ v^{n-a}\rangle $ for $y^ az^{n-a}$ in the two sides of the identity $\partial _ t((1-t)y+tz)^ n=n(z-y)((1-t)y+tz)^{n-1}$ in commuting variables $y,z$. Differentiating (17.3.5) once more, again as a polynomial in $t$, and using this identity, we obtain

\[ \frac{\mathrm d^2}{\mathrm dt^2}E_\theta ^\phi (u_ t) =n\int _ Xh\, \mathrm{dd}^{\mathrm{c}}h\wedge \langle \theta _{u_ t}^{n-1}\rangle \leq 0 \]

by lemma 17.2.7. Thus $t\mapsto E_\theta ^\phi (u_ t)$ is concave, and its derivative decreases from $\int _ Xh\, \mu _ u$ at $t=0$ to $\int _ Xh\, \mu _ v$ at $t=1$. Integrating the derivative over $[0,1]$ gives the tangent bounds (17.3.10). Since $\int _ X\langle \theta _{u_ t}^ n\rangle =m$, the first variation formula also gives $|E_\theta ^\phi (v)-E_\theta ^\phi (u)|\leq m\sup |v-u|$. Finally, the cocycle formula (17.3.6) applied to the pair $\psi ,u$ reads $E_\theta ^\phi (u)-E_\theta ^\phi (\psi )=E_\theta ^\psi (u)$. $\square$

We now extend the energy to all potentials that are at least as singular as $\phi $.

Definition 17.3.11.FC02DD85845C For $u\in \mathrm{PSH}(X,\theta )$ with $u\preceq \phi $ put

\[ E_\theta ^\phi (u)=\inf \{ E_\theta ^\phi (w):w\in \mathcal E^\infty (X,\theta ,\phi ),\ u\leq w\} . \]
The family on the right is nonempty, since $\phi +C$ belongs to it for large $C$; hence $E_\theta ^\phi (u)\in [-\infty ,\infty )$. Because the energy is increasing on $\mathcal E^\infty (X,\theta ,\phi )$, the new definition agrees with (17.3.3) there.

Proposition 17.3.12.92E951B4916A The extended energy is increasing, satisfies $E_\theta ^\phi (u+C)=E_\theta ^\phi (u)+Cm$, and

\[ E_\theta ^\phi (u)=\lim _{k\to \infty } E_\theta ^\phi (\max \{ u,\phi -k\} ), \]

where the limit exists in $[-\infty ,\infty )$.

Proof. If $u\leq u'$, every majorant of $u'$ in the definition is a majorant of $u$, so $E_\theta ^\phi (u)\leq E_\theta ^\phi (u')$. Translating majorants by a constant and using the shift formula on $\mathcal E^\infty (X,\theta ,\phi )$ gives the shift formula. The potentials $u_ k=\max \{ u,\phi -k\} $ belong to $\mathcal E^\infty (X,\theta ,\phi )$, decrease with $k$ and dominate $u$; hence $E_\theta ^\phi (u_ k)$ decreases and is bounded below by $E_\theta ^\phi (u)$. Conversely, let $w$ be any majorant in the definition, and choose $C$ with $w\geq \phi -C$. For $k\geq C$ both $u$ and $\phi -k$ lie below $w$, so $u_ k\leq w$ and $E_\theta ^\phi (u_ k)\leq E_\theta ^\phi (w)$. Letting $k\to \infty $ and taking the infimum over $w$ gives $\lim _ kE_\theta ^\phi (u_ k)\leq E_\theta ^\phi (u)$. $\square$

Proposition 17.3.13.69D86F9D2F90 Let $(u_ i)_{i\in I}$ be a decreasing net in $\mathrm{PSH}(X,\theta )$ with $u_ i\preceq \phi $, and suppose that $u=\inf _ iu_ i$ belongs to $\mathrm{PSH}(X,\theta )$. Then

\[ E_\theta ^\phi (u_ i)\downarrow E_\theta ^\phi (u). \]

Consequently the extended energy is concave on $\{ u\in \mathrm{PSH}(X,\theta ):u\preceq \phi \} $, and the set where it is finite is convex.

Proof. First let the net be a sequence $(u_ j)$. By monotonicity $E_\theta ^\phi (u_ j)$ decreases to a limit $L\geq E_\theta ^\phi (u)$. Let $w\in \mathcal E^\infty (X,\theta ,\phi )$ with $w\geq u$, and put $v_ j=\max \{ u_ j,w\} $. Then $v_ j$ decreases pointwise to $\max \{ u,w\} =w$. Since $u_ j\leq u_1\leq \phi +C$ and $w\geq \phi -C$ for some constant $C$, the differences $v_ j-w$ are uniformly bounded. The tangent bound (17.3.10) gives

\[ 0\leq E_\theta ^\phi (v_ j)-E_\theta ^\phi (w) \leq \int _ X(v_ j-w)\, \mu _ w\longrightarrow 0 \]

by bounded convergence. Since $E_\theta ^\phi (u_ j)\leq E_\theta ^\phi (v_ j)$, we get $L\leq E_\theta ^\phi (w)$, and taking the infimum over $w$ gives $L\leq E_\theta ^\phi (u)$.

For a general net, corollary 10.3.6 shows that $u_ i\to u$ in $L^1(X)$; its hypothesis holds because $\sup _ Xu_ i\geq \sup _ Xu>-\infty $. Choose indices $i_1\leq i_2\leq \cdots $ with $\| u_{i_ k}-u\| _{L^1}<1/k$. The decreasing pointwise limit $\tilde u$ of $(u_{i_ k})$ is a $\theta $-psh function by theorem 5.10.1, applied in charts after adding smooth local potentials of $\theta $, since it dominates $u$ and so is not identically $-\infty $. By monotone convergence, $\int _ X(\tilde u-u)\, \omega ^ n=\lim _ k\int _ X(u_{i_ k}-u)\, \omega ^ n=0$, so $\tilde u=u$ almost everywhere, hence everywhere. The sequence case gives $E_\theta ^\phi (u_{i_ k})\to E_\theta ^\phi (u)$. The net $E_\theta ^\phi (u_ i)$ is decreasing, so its limit is its infimum, which is at most $\lim _ kE_\theta ^\phi (u_{i_ k})=E_\theta ^\phi (u)$; the reverse inequality is monotonicity. (The selected indices need not be cofinal in $I$; this is why we compare infima.)

For concavity let $u,v\preceq \phi $ and $0<t<1$; we may assume that $E_\theta ^\phi (u)$ and $E_\theta ^\phi (v)$ are finite, since otherwise there is nothing to prove. The potentials $(1-t)\max \{ u,\phi -k\} +t\max \{ v,\phi -k\} $ belong to $\mathcal E^\infty (X,\theta ,\phi )$ and decrease to $(1-t)u+tv$ as $k\to \infty $. Concavity on $\mathcal E^\infty (X,\theta ,\phi )$ and decreasing continuity give

\[ E_\theta ^\phi ((1-t)u+tv) \geq (1-t)E_\theta ^\phi (u)+tE_\theta ^\phi (v). \]

In particular the finite locus of the energy is convex. $\square$

Theorem 17.3.14.69E7D1FEF207 For $u\in \mathrm{PSH}(X,\theta )$ with $u\preceq \phi $,

\[ E_\theta ^\phi (u)>-\infty \quad \Longleftrightarrow \quad u\in \mathcal E^1(X,\theta ,\phi ). \]

In particular, finite extended energy forces full mass relative to $\phi $. If $u\in \mathcal E^1(X,\theta ,\phi )$ and $u\leq \phi $, then

AE35DCCFE783 17.3.15
\begin{equation} \frac1{n+1}\int _ X(\phi -u)\, \mu _ u \leq -E_\theta ^\phi (u) \leq \int _ X(\phi -u)\, \mu _ u. \end{equation}

Proof. Both conditions are invariant under adding a constant to $u$, so we may assume $u\leq \phi $. Put $u_ k=\max \{ u,\phi -k\} $ and $A_ k=\{ u>\phi -k\} $. The potentials $u_ k$ belong to $\mathcal E^\infty (X,\theta ,\phi )$ and have mass $m$. Since $u_ k\leq \phi $, all terms in (17.3.3) are nonpositive, and keeping only the term $j=n$ gives

\[ \int _ X(\phi -u_ k)\mu _{u_ k}\leq (n+1)\bigl (-E_\theta ^\phi (u_ k)\bigr ). \]

Suppose that $E_\theta ^\phi (u)>-\infty $. Since $E_\theta ^\phi (u)\leq E_\theta ^\phi (u_ k)\leq E_\theta ^\phi (\phi )=0$, the right side is bounded by $C=-(n+1)E_\theta ^\phi (u)$. On $X\setminus A_ k$ the weight $\phi -u_ k$ equals $k$ outside a pluripolar set; on the plurifine open set $A_ k$ we have $u_ k=u$, so $\mu _{u_ k}=\mu _ u$ there by locality. Hence

\[ m-\mu _ u(A_ k)=\mu _{u_ k}(X\setminus A_ k)\leq C/k. \]

The sets $A_ k$ increase to the set where $u$ is finite, which carries $\mu _ u$, so $\int _ X\langle \theta _ u^ n\rangle \geq m$; since $u\leq \phi $, mass monotonicity (theorem 13.8.7) gives the reverse inequality, and therefore $u\in \mathcal E(X,\theta ,\phi )$. Locality also gives $\int _{A_ k}(\phi -u)\mu _ u\leq C$, and monotone convergence yields $\int _ X(\phi -u)\mu _ u\leq C$. This proves that $u\in \mathcal E^1(X,\theta ,\phi )$ and the first inequality in (17.3.15).

Conversely, suppose $u\in \mathcal E^1(X,\theta ,\phi )$, and let $I=\int _ X(\phi -u)\mu _ u<\infty $. The measures $\mu _{u_ k}$ and $\mu _ u$ have the same total mass $m$ and agree on $A_ k$, so $\mu _{u_ k}(X\setminus A_ k)=\mu _ u(X\setminus A_ k)$. Thus

\[ \int _ X(\phi -u_ k)\mu _{u_ k} =\int _ X\min \{ \phi -u,k\} \, \mu _ u\leq I. \]

The lower tangent bound in (17.3.10), applied to $u_ k$ and $\phi $, gives $E_\theta ^\phi (u_ k)\geq -I$. Letting $k\to \infty $ and using proposition 17.3.12, we obtain $E_\theta ^\phi (u)\geq -I>-\infty $, which is the second inequality in (17.3.15). The first inequality was proved above. $\square$

Example 17.3.16.6EAA0093766C Let $X$ be a compact Kähler curve, so $n=1$, and take $\theta =\omega $ and the reference $V_\omega =0$. For a smooth $\omega $-psh function $u$,

\[ E_\omega (u)=\int _ Xu\, \omega -\tfrac 12 \int _ X\mathrm du\wedge \mathrm d^{\mathrm c}u, \]

where $\mathrm d^{\mathrm c}$ is the real operator of (5.2.10), so that $\mathrm d\mathrm d^{\mathrm c}=\mathrm{dd}^{\mathrm{c}}$. Indeed, by definition $E_\omega (u)=\frac12\bigl (\int _ Xu\, \omega +\int _ Xu(\omega +\mathrm{dd}^{\mathrm{c}}u)\bigr )$, and Stokes' formula (lemma 13.5.2) gives $\int _ Xu\, \mathrm{dd}^{\mathrm{c}}u=-\int _ X\mathrm du\wedge \mathrm d^{\mathrm c}u$. Since $\mathrm du\wedge \mathrm d^{\mathrm c}u=\frac{\mathrm i}{2\pi }\partial u\wedge \bar\partial u$, the second term is a multiple of the classical Dirichlet energy of $u$.

The unbounded potential $u$ on $\mathbb P^1$ of example 16.22.12, which has full mass, also lies in $\mathcal E^1(\mathbb P^1,\omega )$. Away from its only pole $z=0$ the function $u$ is bounded, and $\mu _ u$ is a finite measure. Near the pole write $r=\log |z|^2$. If $G$ is a smooth function of one real variable, then $\bar\partial G(\log |z|^2)=G'(r)\, \mathrm d\bar z/\bar z$ and $\partial \bar\partial G(\log |z|^2)=G''(r)\, \mathrm dz\wedge \mathrm d\bar z/|z|^2$ on $\mathbb C\setminus \{ 0\} $; since $\mathrm i\, \mathrm dz\wedge \mathrm d\bar z=2\, \mathrm dA$, where $\mathrm dA$ is Lebesgue measure, we get $\mathrm{dd}^{\mathrm{c}}G(\log |z|^2)=\pi ^{-1}G''(r)|z|^{-2}\, \mathrm dA$, which in polar coordinates $z=\rho \mathrm e^{\mathrm i\vartheta }$, with $r=2\log \rho $, is $(2\pi )^{-1}G''(r)\, \mathrm dr\, \mathrm d\vartheta $.

The function $F$ of example 16.22.12 satisfies $F(r)=-\log (-r)$ for $r\leq r_0$, with $r_0$ sufficiently negative, and is therefore smooth there, with $F''(r)=r^{-2}$. On the punctured disc $\{ 0<|z|^2<\mathrm e^{r_0}\} $ the measure $\mu _ u$ is $\mathrm{dd}^{\mathrm{c}}F(\log |z|^2)$, and it does not charge the pole; hence the image of its restriction to $\{ |z|^2<\mathrm e^{r_0}\} $ under $z\mapsto \log |z|^2$ is $F''(r)\, \mathrm dr=r^{-2}\, \mathrm dr$ on $(-\infty ,r_0)$. Since $u-F(\log |z|^2)=-\log (1+|z|^2)$ is bounded near the pole, the finiteness of $\int |u|\, \mu _ u$ near the pole reduces, after the substitution $t=-r$, to

\[ \int _ a^\infty \frac{\log t}{t^2}\, \mathrm dt =\frac{\log a+1}{a}<\infty \qquad (a>1). \]

Hence $u$ is a potential of finite energy whose difference from the reference $V_\omega =0$ is unbounded.

Corollary 17.3.17.4DCEFD8869DD The classes $\mathcal E^\infty (X,\theta ,\phi )$, $\mathcal E^1(X,\theta ,\phi )$ and $\mathcal E(X,\theta ,\phi )$ are convex. If $u\in \mathcal E^1(X,\theta ,\phi )$, $v\in \mathrm{PSH}(X,\theta )$ and $u\leq v\preceq \phi $, then $v\in \mathcal E^1(X,\theta ,\phi )$.

Proof. Convex combinations of potentials with the same singularity type as $\phi $ have that singularity type. For $\mathcal E^1(X,\theta ,\phi )$, convexity follows from the concavity of the extended energy (proposition 17.3.13) and theorem 17.3.14. If $u,v\in \mathcal E(X,\theta ,\phi )$ and $0<t<1$, then $(1-t)u+tv\preceq \phi $, and by multilinearity $\mu _{(1-t)u+tv}$ is a combination of the mixed measures $\langle \theta _ u^ j\wedge \theta _ v^{n-j}\rangle $ with coefficients $\binom nj(1-t)^ jt^{n-j}$. Each of these measures has total mass $m$, as noted at the beginning of this section, so $\int _ X\langle \theta _{(1-t)u+tv}^ n\rangle =m$. The last assertion follows from the monotonicity of the extended energy and theorem 17.3.14. $\square$

Lemma 17.3.18.620127F44043 Let $u\in \mathcal E(X,\theta ,\phi )$, let $v\in \mathrm{PSH}(X,\theta )$ satisfy $v\preceq \phi $, and let $\gamma \colon X\to [-\infty ,\infty ]$ be a Borel function, for instance a $\theta $-psh function, with $\gamma \geq \max \{ u,v\} $. Then, allowing infinite values,

\[ \int _ X(\gamma -u)\mu _ v \leq 2\int _ X(\gamma -u)\mu _ u +2\int _ X(\gamma -v)\mu _ v. \]

Consequently, if $u,v,w_1,\ldots ,w_ n\in \mathcal E^1(X,\theta ,\phi )$, then

\[ \int _ X|u-v|\, \langle \theta _{w_1}\wedge \cdots \wedge \theta _{w_ n}\rangle <\infty . \]

Proof. For $t\geq 0$ we have

\[ \{ \gamma >u+2t\} \subset \{ \gamma >v+t\} \cup \{ v>u+t\} , \]

because $\gamma \leq v+t$ and $v\leq u+t$ imply $\gamma \leq u+2t$. The weights $\gamma -u$ and $\gamma -v$ are Borel functions with values in $[0,\infty ]$ on the complements of the pole sets of $u$ and $v$, respectively, and these pole sets carry no mass; the level sets above are taken on these complements. Since $u\in \mathcal E(X,\theta ,\phi )$ and $v-t\preceq \phi $, the comparison principle of proposition 16.25.4, applied with $p=n$ to $u$ and $v-t$, gives

\[ \mu _ v(\{ v>u+t\} )\leq \mu _ u(\{ v>u+t\} )+\int _ X\langle \theta _\phi ^ n\rangle -\int _ X\langle \theta _ u^ n\rangle =\mu _ u(\{ v>u+t\} ). \]

Integrating over level sets, we obtain

\[ \begin{split} \int _ X(\gamma -u)\mu _ v & \leq 2\int _0^\infty \mu _ v(\{ \gamma >v+t\} )\, \mathrm dt +2\int _0^\infty \mu _ u(\{ v>u+t\} )\, \mathrm dt\\ & \leq 2\int _ X(\gamma -v)\mu _ v+2\int _ X(\gamma -u)\mu _ u, \end{split} \]

where in the last step we used $(v-u)_+\leq \gamma -u$, which holds because $\gamma \geq \max \{ u,v\} $. All functions involved are nonnegative, so Tonelli's theorem applies without any integrability assumption.

For the second assertion, add constants to $u$ and $v$ so that $u,v\leq \phi $; this changes $|u-v|$ by at most a constant, and the mixed measure has finite mass $m$. Put $w=\frac1n\sum _ jw_ j$, which lies in $\mathcal E^1(X,\theta ,\phi )$ by corollary 17.3.17. By multilinearity, $\langle \theta _{w_1}\wedge \cdots \wedge \theta _{w_ n}\rangle \leq n^ n\mu _ w$. Choose $C$ with $w\leq \phi +C$ and apply the first assertion to $u$, $w$ and $\gamma =\phi +C$: its right side is finite because $u,w\in \mathcal E^1(X,\theta ,\phi )$. Hence $\phi -u$ is integrable for $\mu _ w$, and so for the mixed measure. The same holds for $\phi -v$, and $|u-v|\leq (\phi -u)+(\phi -v)$. $\square$

Proposition 17.3.19.98BD01BE1363 For $u,v\in \mathcal E^1(X,\theta ,\phi )$, the cocycle formula (17.3.6) and the tangent bounds (17.3.10) remain valid. In particular, (17.3.3) computes the extended energy on $\mathcal E^1(X,\theta ,\phi )$.

Proof. All mixed measures involved have total mass $m$, so both assertions are unchanged if constants are added to $u$ and $v$; we may therefore assume $u,v\leq \phi $. Put $u_ k=\max \{ u,\phi -k\} $ and $v_ k=\max \{ v,\phi -k\} $. Fix $0\leq j\leq n$ and write $\lambda _ k=\langle \theta _{u_ k}^ j\wedge \theta _{v_ k}^{n-j}\rangle $ and $\lambda =\langle \theta _ u^ j\wedge \theta _ v^{n-j}\rangle $. We show that

03F8F41E7068 17.3.20
\begin{equation} \int _ X(u_ k-v_ k)\lambda _ k\longrightarrow \int _ X(u-v)\lambda . \end{equation}

On the plurifine open set $A_ k=\{ u>\phi -k\} \cap \{ v>\phi -k\} $ the measures $\lambda _ k$ and $\lambda $ agree by locality, and $u_ k-v_ k=u-v$. By lemma 17.3.18, $|u-v|$ is $\lambda $-integrable. The sets $X\setminus A_ k$ decrease to the union of the pole sets of $u$, $v$ and $\phi $, which is pluripolar and therefore $\lambda $-null, so dominated convergence gives $\int _{X\setminus A_ k}|u-v|\lambda \to 0$. It remains to show that the integral of $|u_ k-v_ k|$ against $\lambda _ k$ over $X\setminus A_ k$ tends to zero.

For $z\in \{ u,v\} $ put $D_ k(z)=\{ z\leq \phi -k\} $, so that $X\setminus A_ k=D_ k(u)\cup D_ k(v)$. We claim that

474BE0C5FED2 17.3.21
\begin{equation} k\lambda _ k(D_ k(z))\leq 2^ n k\mu _ z(\{ z\leq \phi -k/2\} )\longrightarrow 0. \end{equation}

Consider $z=u$ and $j<n$, and put $q=(v_ k+\phi -k)/2$. Since $\phi -k\leq v_ k\leq \phi $, we have $q\leq \phi -k/2$ on $X$, and $u_ k=\phi -k\leq q$ on $D_ k(u)$. Moreover $\theta _{v_ k}\leq 2\theta _ q$, since $2\theta _ q-\theta _{v_ k}=\theta _\phi \geq 0$, so multilinearity gives $\lambda _ k\leq 2^{n-j}\langle \theta _{u_ k}^ j\wedge \theta _ q^{n-j}\rangle $. The potentials $q$ and $u_ k$ belong to $\mathcal E(X,\theta ,\phi )$, and the non-strict comparison principle of proposition 16.25.4, with $n-j$ factors $\theta _ q$ and the $j$ fixed factors $\theta _{u_ k}$, gives

\[ \lambda _ k(D_ k(u)) \leq 2^{n-j}\mu _{u_ k}(\{ u_ k\leq q\} ) \leq 2^{n-j}\mu _{u_ k}(\{ u\leq \phi -k/2\} ). \]

For $j=n$ the same bound holds directly, since then $\lambda _ k=\mu _{u_ k}$ and $D_ k(u)\subset \{ u\leq \phi -k/2\} $. The measures $\mu _{u_ k}$ and $\mu _ u$ have the same total mass and agree on $\{ u>\phi -k/2\} $ by locality, so the last mass equals $\mu _ u(\{ u\leq \phi -k/2\} )$. Since exchanging $u$ and $v$ and replacing $j$ by $n-j$ does not change $\lambda _ k$, the case $z=v$ follows from the case $z=u$. Finally,

\[ k\mu _ z(\{ z\leq \phi -k/2\} )\leq 2\int _{\{ z\leq \phi -k/2\} }(\phi -z)\mu _ z\longrightarrow 0 \]

because $\phi -z$ is $\mu _ z$-integrable. This proves (17.3.21).

Since $u_ k-\phi $ and $v_ k-\phi $ take values in $[-k,0]$, we have $|u_ k-v_ k|\leq k$, and (17.3.21) shows that the integral of $|u_ k-v_ k|$ against $\lambda _ k$ over $X\setminus A_ k$ tends to zero. This proves (17.3.20). Now pass to the limit in the cocycle formula for $u_ k,v_ k$: its left side converges to $E_\theta ^\phi (v)-E_\theta ^\phi (u)$ by proposition 17.3.12, and each term on the right converges by (17.3.20). The tangent bounds pass to the limit in the same way, using the terms $j=n$ and $j=0$. Taking $v=\phi $ in the cocycle formula gives the last assertion. $\square$

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