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15.35 Exponential equations for an individual densityC3635E28D6B1

C3635E28D6B1

We return to the Hermitian background $h$ and a fixed nonzero density $0\leq f\in L^1(\mathrm{d}V)$, and consider, for $\lambda >0$, the exponential equation

A708922257FB 15.35.1
\begin{equation} \mathrm{MA}^{\mathrm{ext}}_ h(u)=\mathrm{e}^{\lambda u}f\, \mathrm{d}V, \qquad u\in \mathrm{PSH}(X,h). \end{equation}

A solution is a function $u\in \mathrm{PSH}(X,h)$ satisfying (15.35.1), and an exponential subsolution at exponent $\lambda $ is a function $s\in \mathrm{PSH}(X,h)$ with $\mathrm{MA}^{\mathrm{ext}}_ h(s)\geq \mathrm{e}^{\lambda s}f\, \mathrm{d}V$. For the truncations $f_ k=\min (f,k)$, theorem 14.19.3 gives continuous solutions $u_ k$ of the truncated equations, and these decrease as $k$ increases. Strict domination shows that every exponential subsolution is a common lower bound for the $u_ k$. Hence, as soon as one subsolution exists, the decreasing limit is not identically $-\infty $, and theorem 15.34.2 shows that it solves (15.35.1); it is the greatest subsolution. A positive threshold $b_ h(f)$ provides exponential subsolutions for every exponent, and the normalized greatest solutions then recover $b_ h(f)$ as $\lambda \downarrow 0$.

Theorem 15.35.2.9016C2906071 Fix $\lambda >0$, and suppose that (15.35.1) has an exponential subsolution $s\in \mathrm{PSH}(X,h)$. For $k\geq 1$, let $u_ k$ be the continuous solution of

\[ \mathrm{MA}_ h(u_ k)=\mathrm{e}^{\lambda u_ k}f_ k\, \mathrm{d}V, \qquad f_ k=\min (f,k), \]

given by theorem 14.19.3. Then $u_ k$ decreases to a solution $u_\lambda $ of (15.35.1), and $\mathrm{MA}^{\mathrm{ext}}_ h(u_\lambda )$ has finite mass. Moreover, $u_\lambda $ is the greatest exponential subsolution: every exponential subsolution $v$ at exponent $\lambda $ satisfies $v\leq u_\lambda $. In particular, $u_\lambda $ is the greatest solution of (15.35.1).

Proof. Since $f_ k\leq f_{k+1}$, lemma 14.19.28 gives $u_{k+1}\leq u_ k$.

We first show that every exponential subsolution $v$ lies below each $u_ k$. Let $t>0$. On the set $\{ u_ k<v-t\} $,

\[ \mathrm{MA}_ h(u_ k)=\mathrm{e}^{\lambda u_ k}f_ k\, \mathrm{d}V \leq \mathrm{e}^{-\lambda t}\mathrm{e}^{\lambda v}f\, \mathrm{d}V \leq \mathrm{e}^{-\lambda t}\mathrm{MA}^{\mathrm{ext}}_ h(v-t). \]

Since $u_ k$ is bounded, $P_{h/2}(u_ k)\geq \inf _ Xu_ k$ is not identically $-\infty $, and $v-t\preceq u_ k$. Strict domination, theorem 15.2.2, therefore gives $u_ k\geq v-t$. Letting $t\downarrow 0$ gives $u_ k\geq v$.

In particular $s\leq u_ k\leq u_1$ for every $k$, so the decreasing limit $u_\lambda \geq s$ is not identically $-\infty $ and belongs to $\mathrm{PSH}(X,h)$. By lemma 5.29.19, $u_ k\to u_\lambda $ in capacity. Choose a constant $A\geq \sup _ Xu_1$. The nonpositive functions $u_ k-A$ satisfy

\[ \mathrm{MA}^{\mathrm{ext}}_ h(u_ k-A)=\mathrm{e}^{\lambda (u_ k-A)}\, \mathrm{e}^{\lambda A}f_ k\, \mathrm{d}V, \]

and $\mathrm{e}^{\lambda A}f_ k\to \mathrm{e}^{\lambda A}f$ in $L^1(\mathrm{d}V)$. Theorem 15.34.2, applied with $\mu =\mathrm{d}V$ and constant exponents, shows that $\mathrm{MA}^{\mathrm{ext}}_ h(u_\lambda )$ is finite and that $u_\lambda $ solves (15.35.1). Finally, every exponential subsolution lies below all $u_ k$, hence below $u_\lambda $, which is itself a subsolution. $\square$

Being the greatest subsolution, $u_\lambda $ does not depend on the approximation used to construct it. The equation may have other, smaller solutions with different singularities. If $f\in L^ p$ for some $p>1$, the continuous solution of theorem 14.19.3 is a subsolution and therefore lies below $u_\lambda $. Thus $u_\lambda $ is bounded, and bounded exponential comparison (corollary 14.19.12) shows that it coincides with the continuous solution.

Corollary 15.35.3.B2672237F244 Suppose $b=b_ h(f)>0$. Then (15.35.1) has a greatest solution $u_\lambda $ for every $\lambda >0$. If $v\in \mathrm{PSH}(X,h)$ satisfies $\sup _ Xv=0$ and $\mathrm{MA}^{\mathrm{ext}}_ h(v)\geq bf\, \mathrm{d}V$, then

\[ u_\lambda \geq v+\lambda ^{-1}\log b. \]

Put

\[ M_\lambda =\sup _ Xu_\lambda ,\qquad v_\lambda =u_\lambda -M_\lambda ,\qquad c_\lambda =\mathrm{e}^{\lambda M_\lambda }. \]

Then, as $\lambda \downarrow 0$,

\[ c_\lambda \longrightarrow b_ h(f),\qquad \mathrm{e}^{\lambda u_\lambda }f\longrightarrow b_ h(f)f \quad \text{in }L^1(\mathrm{d}V). \]

Proof. By theorem 15.28.4, a function $v$ as in the statement exists. Since $v\leq 0$, the function $s=v+\lambda ^{-1}\log b$ satisfies

\[ \mathrm{MA}^{\mathrm{ext}}_ h(s)\geq bf\, \mathrm{d}V \geq \mathrm{e}^{\lambda s}f\, \mathrm{d}V, \]

so it is an exponential subsolution. Theorem 15.35.2 gives the greatest solution $u_\lambda $ and the bound $u_\lambda \geq s$; in particular, $c_\lambda \geq b$.

Set $g_\lambda =\mathrm{e}^{\lambda v_\lambda }f$. By lemma 5.44.5, applied to the finite measure $f\, \mathrm{d}V$, we have $g_\lambda \to f$ in $L^1$ as $\lambda \downarrow 0$. Each $g_\lambda $ is nonzero, since $v_\lambda $ is finite almost everywhere. The equation for $u_\lambda $ reads $\mathrm{MA}^{\mathrm{ext}}_ h(v_\lambda )=c_\lambda g_\lambda \, \mathrm{d}V$, so theorem 15.28.4, applied to the density $g_\lambda $, gives

\[ c_\lambda \leq b_ h(g_\lambda ). \]

The upper semicontinuity of the threshold (theorem 15.32.1) therefore gives

\[ b\leq \liminf _{\lambda \downarrow 0}c_\lambda \leq \limsup _{\lambda \downarrow 0}c_\lambda \leq b_ h(f)=b. \]

This proves $c_\lambda \to b$. Since $\mathrm{e}^{\lambda u_\lambda }f=c_\lambda g_\lambda $ and $g_\lambda \to f$ in $L^1$, it also proves $\mathrm{e}^{\lambda u_\lambda }f\to bf$ in $L^1$. $\square$

Since $\mathrm{MA}^{\mathrm{ext}}_ h(v_\lambda )=\mathrm{e}^{\lambda u_\lambda }f\, \mathrm{d}V$, the Monge–Ampère measures of the normalized greatest solutions converge in total variation to $b_ h(f)f\, \mathrm{d}V$. This answers the questions about the scalar and the measure raised in section 15.34; the potentials $v_\lambda $ themselves are harder to control. Under positive lower mass, corollary 15.37.32 shows that every $L^1$-convergent sequence $v_{\lambda _ j}$ with $\lambda _ j\downarrow 0$ converges in capacity to a solution of $\mathrm{MA}^{\mathrm{ext}}_ h(v)=b_ h(f)f\, \mathrm{d}V$. For $L^ p$ data with $p>1$, proposition 15.20.1 gives uniform precompactness. In both cases, convergence of the whole family $(v_\lambda )$ requires that all its cluster limits coincide. This holds when the dual problem for $f^{1/n}$ over Gauduchon currents, studied in section 12.10, has a smooth strictly positive maximizer: the whole family then converges uniformly (corollary 12.10.13). If the maximizer is smooth and semipositive, and strictly positive outside a proper analytic set, proposition 12.10.20 gives $L^1$ convergence of the whole family and a fixed lower barrier, and corollary 12.10.31 strengthens this to uniform convergence for $L^ p$ data with $p>1$.

For a general positive threshold, the corollary gives the lower bound

\[ v_\lambda \geq v-\lambda ^{-1}\log (c_\lambda /b_ h(f)) \]

for every normalized threshold subsolution $v$. The next subsection estimates the scalar error $\log (c_\lambda /b_ h(f))$ when $f^{1/n}$ can be approximated by bounded functions in the norm of $\mathcal D_ h$. When $b_ h(f)=0$, theorem 15.35.2 still applies whenever an exponential subsolution exists; examples are constructed in 15.35.7.

15.35.4 An error bound for the scalar limit36B99A272B8F

Suppose that $f^{1/n}$ belongs to the space $\mathcal D_ h^0$ of 15.32.7. The uniform tail condition of proposition 15.32.9 then gives a rate for the convergence $c_\lambda \to b_ h(f)$ in corollary 15.35.3. Split the root $p=f^{1/n}$ at a height $K$. On $\{ p\leq K\} $, the error $p(1-\mathrm{e}^{\lambda v/n})$ of the damped root has norm $O(K\lambda )$ in $\mathcal D_ h$, uniformly over normalized potentials $v$, while on $\{ p>K\} $ it is bounded by the tail of $p$, which is small in that norm. Optimizing over $K$ gives a modulus valid for every normalized potential.

Proposition 15.35.5.AC5E6031A12C Let $0\leq p\in \mathcal D_ h^0$ be nonzero, and put $f=p^ n$, $R=\rho _ h(p)$ and $b=R^{-n}=b_ h(f)$. There is a constant $C_ h$, depending only on $h$ and $\mathrm{d}V$, such that the function

\[ \eta _ p(\lambda )=\inf _{K>0} \left(\| p\mathbf1_{\{ p>K\} }\| _{\mathcal D_ h}+C_ hK\lambda \right) \]

tends to zero as $\lambda \downarrow 0$ and satisfies

747F5A0D1221 15.35.6
\begin{equation} \big \| p(1-\mathrm{e}^{\lambda v/n})\big \| _{\mathcal D_ h} \leq \eta _ p(\lambda ) \qquad \bigl (v\in \mathrm{PSH}(X,h),\ \sup _ Xv=0\bigr ). \end{equation}

Let $u_\lambda $, $v_\lambda $ and $c_\lambda $ be the greatest exponential solutions and their normalizations from corollary 15.35.3. If $\eta _ p(\lambda )<R$, then

\[ b\leq c_\lambda \leq \bigl (R-\eta _ p(\lambda )\bigr )^{-n} \]

and

\begin{align*} \big \| \mathrm{MA}^{\mathrm{ext}}_ h(v_\lambda ) -bf\, \mathrm{d}V\big \| _{\mathrm{TV}} & \leq (c_\lambda -b)\| p\| _{L^ n}^{n} +nb\| p\| _{L^ n}^{n-1}\eta _ p(\lambda ). \end{align*}

If $p\in L^ r$ for some finite $r>n$, the same bounds hold with $\eta _ p(\lambda )$ replaced by $C_{h,r}\| p\| _{L^ r}\lambda $, where $C_{h,r}$ depends only on $h$, $\mathrm{d}V$ and $r$. In particular, for each such $p$ the scalar and total-variation errors are $O(\lambda )$.

Proof. By lemma 5.26.2, normalized $h$-plurisubharmonic functions are uniformly bounded in every $L^ s$ with $s<+\infty $. By (15.32.8) with $r=2n$, their norms $\| v\| _{\mathcal D_ h}$ are therefore uniformly bounded; let $C_ h$ be $1/n$ times this bound. Let $v$ be normalized and $K>0$. On $\{ p\leq K\} $ we have

\[ 0\leq p(1-\mathrm{e}^{\lambda v/n}) \leq K\lambda (-v)/n, \]

since $1-\mathrm{e}^{-x}\leq x$ for $x\geq 0$, while on $\{ p>K\} $ we use the bound $p(1-\mathrm{e}^{\lambda v/n})\leq p$. The monotonicity of $\| \cdot \| _{\mathcal D_ h}$ and the triangle inequality give

\[ \big \| p(1-\mathrm{e}^{\lambda v/n})\big \| _{\mathcal D_ h} \leq \| p\mathbf1_{\{ p>K\} }\| _{\mathcal D_ h}+C_ hK\lambda , \]

and taking the infimum over $K$ proves (15.35.6). By proposition 15.32.9, and since the $L^ n$ tails of $p$ tend to zero, $\| p\mathbf1_{\{ p>K\} }\| _{\mathcal D_ h}\to 0$ as $K\to \infty $. Choosing $K$ first and then letting $\lambda \downarrow 0$ shows that $\eta _ p(\lambda )\to 0$.

Now set $q_\lambda =p\, \mathrm{e}^{\lambda v_\lambda /n}$, so that $q_\lambda ^ n=g_\lambda =\mathrm{e}^{\lambda v_\lambda }f$, with $g_\lambda $ as in the proof of corollary 15.35.3. Since $0\leq q_\lambda \leq p$ and $\rho _ h(p-q_\lambda )\leq \eta _ p(\lambda )$ by (15.35.6), the triangle inequality and monotonicity give

\[ R-\eta _ p(\lambda )\leq \rho _ h(q_\lambda )\leq R. \]

The same proof gives $b\leq c_\lambda \leq b_ h(g_\lambda )=\rho _ h(q_\lambda )^{-n}$, which yields the scalar bound. For the measures, the factorization of $p^ n-q_\lambda ^ n$ gives $0\leq p^ n-q_\lambda ^ n\leq np^{n-1}(p-q_\lambda )$, and Hölder's inequality implies

\[ \| f-g_\lambda \| _{L^1} \leq n\| p\| _{L^ n}^{n-1}\| p-q_\lambda \| _{L^ n} \leq n\| p\| _{L^ n}^{n-1}\eta _ p(\lambda ). \]

Since $\mathrm{MA}^{\mathrm{ext}}_ h(v_\lambda )=c_\lambda g_\lambda \, \mathrm{d}V$, the identity $c_\lambda g_\lambda -bf=(c_\lambda -b)g_\lambda -b(f-g_\lambda )$, together with $\| g_\lambda \| _{L^1}\leq \| f\| _{L^1}=\| p\| _{L^ n}^ n$, proves the total-variation bound.

Finally, suppose $p\in L^ r$ with $n<r<+\infty $, and choose $n<s<r$. By (15.32.8) with exponent $s$, and since $\| \cdot \| _{L^ n}\leq \| \cdot \| _{L^ s}$, we have $\| \cdot \| _{\mathcal D_ h}\leq (1+C_ s)\| \cdot \| _{L^ s}$. Hölder's inequality and lemma 5.26.2 then give, for every normalized $v$,

\[ \| p(-v)\| _{\mathcal D_ h} \leq (1+C_ s)\| p(-v)\| _{L^ s} \leq (1+C_ s)\| p\| _{L^ r}\| v\| _{L^{rs/(r-s)}} \leq nC_{h,r}\| p\| _{L^ r}. \]

Since $0\leq 1-\mathrm{e}^{\lambda v/n}\leq \lambda (-v)/n$, the left side of (15.35.6) is therefore at most $C_{h,r}\| p\| _{L^ r}\lambda $, and the two estimates above can be repeated with this bound in place of $\eta _ p(\lambda )$. For $\lambda $ so small that $C_{h,r}\| p\| _{L^ r}\lambda \leq R/2$, the function $t\mapsto (R-t)^{-n}$ has bounded derivative on $[0,R/2]$, so the scalar error $c_\lambda -b$, and hence the total-variation error, is $O(\lambda )$. $\square$

For a general $p\in \mathcal D_ h^0$ the modulus $\eta _ p(\lambda )$ tends to zero, but we do not know whether it is $O(\lambda )$. Combined with the lower bound $v_\lambda \geq v-\lambda ^{-1}\log (c_\lambda /b)$ for normalized threshold subsolutions $v$, the proposition gives

\[ 0\leq \lambda ^{-1}\log (c_\lambda /b) \leq -\frac n\lambda \log \bigl (1-\eta _ p(\lambda )/R\bigr ), \]

which stays bounded as $\lambda \downarrow 0$ when $\eta _ p(\lambda )=O(\lambda )$, in particular for $p\in L^ r$ with $r>n$; root tails alone do not give such a bound. Even when a uniform lower barrier for $v_\lambda $ is available, passing to the limit in capacity requires the singularity-type or lower-mass hypotheses of a continuity theorem. The proposition estimates only scalars and measures; when the lower mass vanishes, it does not give an exact equation at the threshold.

15.35.7 Exponential equations at zero threshold49C07144356F

When $b_ h(f)=0$, no positive multiple of $f\, \mathrm{d}V$ is dominated by a Monge–Ampère measure. An exponential subsolution $s$ only needs $\mathrm{MA}^{\mathrm{ext}}_ h(s)\geq \mathrm{e}^{\lambda s}f\, \mathrm{d}V$, however, and the factor $\mathrm{e}^{\lambda s}$ is small where $s$ is very negative. A density concentrating near the pole of a singular potential can therefore admit exponential subsolutions although its threshold vanishes. We construct such densities on the products of section 15.30.

We keep the notation of that section: $X=X_0\times Y$ with $Y=\mathbb P^ k$, the background $H=h_0+\kappa $, the constants $N$, $C$ and $V_0$, the probability volume form $\mu =V_0^{-1}h_0^ m\wedge \kappa ^ k$ with density $R=\mu /\mathrm{d}V$, and the potential $u_\alpha $ with density $q_\alpha $ from lemma 15.30.1, for a fixed $0<\alpha <1$. On $Y\setminus \{ o\} $ put $L=1-\psi \geq 1$, so that $u_\alpha =1-L^\alpha $, and $t=\mathrm e^{1-L}$. As functions of $L$, define

\[ a=\alpha L^{\alpha -1},\qquad Q=t+(1-t)a,\qquad D=t(1-a)+(1-t)\alpha (1-\alpha )L^{\alpha -2}, \]
\[ W=kQ^{k-1}D,\qquad B_\tau =q_\alpha \mathrm e^{\tau (L^\alpha -1)}\quad (\tau >0),\qquad b_0=(1-\alpha )^ k. \]

Here $Q$ is the function $Q(r)$ of lemma 15.30.1, written in terms of $L$, and $D=-\mathrm{d}Q/\mathrm{d}L$. The weight $B_\tau $ is chosen so that $\mathrm e^{\tau u_\alpha }B_\tau =q_\alpha $ off $o$.

Lemma 15.35.8.C9E4D8D9901A As functions of $L$,

\[ q_\alpha =Q^{k-1}D\, \mathrm e^{k(L-1)},\qquad q_\alpha \geq b_0, \]

and $W(L)\sim k\alpha ^ k(1-\alpha )L^{-1-k(1-\alpha )}$ as $L\to +\infty $. For every $\tau >0$, $\mathrm e^{\tau (L^\alpha -1)}W(L)\to +\infty $ as $L\to +\infty $. In particular, $B_\tau \kappa ^ k$ has infinite mass on every punctured neighborhood of $o$.

Proof. In the notation of the proof of lemma 15.30.1, $t=r/(1+r)$ and $s(r)=L$. Since the mass of $q_\alpha \kappa ^ k$ on $\{ r_1<r<r_2\} $ is $Q(r_2)^ k-Q(r_1)^ k$, this measure has radial distribution $-\mathrm{d}(Q^ k)/\mathrm{d}L=W(L)\, \mathrm{d}L$. The Fubini–Study measure $\kappa ^ k$ corresponds to $Q=t$, so its radial distribution is $k\mathrm e^{-k(L-1)}\mathrm{d}L$. Both measures are invariant under the unitary group of the chart, so $q_\alpha $ is the ratio of the two distributions, which is the stated formula. The lower bound $q_\alpha \geq b_0$ follows from $\kappa +\mathrm{dd}^{\mathrm{c}}u_\alpha \geq (1-\alpha )\kappa $ off $o$. As $L\to +\infty $, $t$ tends to zero exponentially, so $Q\sim \alpha L^{\alpha -1}$ and $D\sim \alpha (1-\alpha )L^{\alpha -2}$; this gives the asymptotics of $W$. Consequently,

\[ \log \bigl (\mathrm e^{\tau (L^\alpha -1)}W(L)\bigr )=\tau L^\alpha -[1+k(1-\alpha )]\log L+O(1)\longrightarrow +\infty , \]

and the mass of $B_\tau \kappa ^ k$ on $\{ L>T\} $, which equals $\int _ T^\infty \mathrm e^{\tau (L^\alpha -1)}W(L)\, \mathrm{d}L$, is infinite for every $T$. $\square$

Theorem 15.35.9.8FF7FBD67552 Let $f\geq 0$ be a nonzero integrable function on $X$, and put $F=f/R$.

  1. If $\lambda >0$ and $F\leq AB_\lambda $ almost everywhere for a constant $A>0$, then

    \[ s_\lambda =u_\alpha +\lambda ^{-1}\log (CV_0/A) \]

    is an exponential subsolution at exponent $\lambda $, of mass $CV_0$, and the equation $\mathrm{MA}^{\mathrm{ext}}_ H(u)=\mathrm{e}^{\lambda u}f\, \mathrm{d}V$ has a greatest solution, whose mass is finite and positive.

  2. Suppose that $F$ is locally essentially bounded on $X\setminus (X_0\times \{ o\} )$ and

    \[ \lim _{T\to +\infty }\operatorname *{ess\, sup}_{x\in X_0,\ L(y)>T} \frac{\log ^+(F(x,y)/q_\alpha (y))}{L(y)^\alpha }=0, \]

    where $\log ^+r=\log \max (1,r)$ for $r\geq 0$. Then the hypothesis of (1), and hence its conclusion, holds for every $\lambda >0$.

Proof. (1) By theorem 15.30.3, $\mathrm{MA}^{\mathrm{ext}}_ H(u_\alpha )=CV_0q_\alpha \mu $. Off the pole fiber $X_0\times \{ o\} $ we have $\mathrm e^{\lambda u_\alpha }B_\lambda =q_\alpha $ and $f\, \mathrm{d}V=F\mu \leq AB_\lambda \mu $, hence

\[ \mathrm e^{\lambda s_\lambda }f\, \mathrm dV \leq (CV_0/A)\mathrm e^{\lambda u_\alpha }AB_\lambda \mu =CV_0q_\alpha \mu =\mathrm{MA}^{\mathrm{ext}}_ H(s_\lambda ), \]

and both measures vanish on the pole fiber. Thus $s_\lambda $ is an exponential subsolution, and its mass is $CV_0$, since adding a constant does not change the Monge–Ampère measure. Theorem 15.35.2 now gives the greatest solution $u$ and the finiteness of its mass. The mass $\int _ X\mathrm{e}^{\lambda u}f\, \mathrm{d}V$ is positive because $u$ is finite almost everywhere and $f$ has positive integral.

(2) Fix $\lambda >0$. By hypothesis, there is $T$ such that $F/q_\alpha \leq \mathrm e^{(\lambda /2)L^\alpha }$ almost everywhere on $\{ L>T\} $. Since $\mathrm e^{(\lambda /2)L^\alpha }\leq \mathrm e^{\lambda }\mathrm e^{\lambda (L^\alpha -1)}$ for $L\geq 1$, we have $F\leq \mathrm e^{\lambda }B_\lambda $ there. On the complement $\{ L\leq T\} $, which is compact and disjoint from the pole fiber, $F$ is essentially bounded, while $B_\lambda \geq q_\alpha \geq b_0>0$. Increasing the constant, we obtain $F\leq AB_\lambda $ almost everywhere on $X$. $\square$

Theorem 15.35.10.092A98EE953D Let $F_ j$, $j\geq 1$, be smooth strictly positive probability densities on $X_0$ with respect to $\mathrm dV_0=V_0^{-1}h_0^ m$, whose normalization scalars on $X_0$, relative to $h_0$ and $\mathrm dV_0$, satisfy $c_{h_0}(F_ j)\leq 2^{-2j}/C$. There are smooth strictly positive probability densities $g_ j$ on $Y$ with respect to $\kappa ^ k$ such that the probability densities

\[ f_ j=RF_ jg_ j,\qquad f=\sum _{j\geq 1}2^{-j}f_ j \]

on $X$ satisfy $c_ H(f_ j)\leq 2^{-2j}$ and $b_ H(f)=0$. The function $f$ is finite everywhere, smooth off the pole fiber $X_0\times \{ o\} $, has integral one and is bounded below by a positive constant. For every $\lambda >0$, the equation $\mathrm{MA}^{\mathrm{ext}}_ H(u)=\mathrm{e}^{\lambda u}f\, \mathrm{d}V$ has an exponential subsolution and a greatest solution, of finite mass, and every solution is unbounded.

Proof. Put $w_ j=2^{-j}$ and $M_ j=\max _{X_0}F_ j$.

Step 1: a smooth baseline. Fix $C^ j$ norms $\| \cdot \| _{C^ j}$ on $X_0$, computed in a fixed finite atlas, so that they increase with $j$. Choose $0<\varepsilon _ j\leq 1/2$ with

\[ w_ j\varepsilon _ jM_ j\leq b_0 2^{-j-2},\qquad w_ j\varepsilon _ j\| F_ j\| _{C^ j}\leq 2^{-j}. \]

Then $E=\sum _ jw_ j\varepsilon _ jF_ j$ converges in every $C^ l$ norm, so $E$ is smooth on $X_0$, and $0<E\leq b_0/4$.

Step 2: bumps escaping to the pole. Choose a smooth function $\chi :\mathbb R\to [0,1]$, supported in $[0,1]$, positive on $(0,1)$ and flat at $0$ and $1$. Starting with $T_0=0$, choose inductively $T_ j\geq 2$ with $T_ j>T_{j-1}+2$ and

\[ Z_ j=\int _{T_ j}^{T_ j+1}\chi (L-T_ j) \mathrm e^{(L^\alpha -1)/j}W(L)\, \mathrm dL \geq 2w_ jM_ j. \]

This is possible because, by lemma 15.35.8 with $\tau =1/j$, the factor $\mathrm e^{(L^\alpha -1)/j}W(L)$ is uniformly large on sufficiently distant intervals. On the annulus $\{ T_ j\leq L\leq T_ j+1\} $ put $\beta _ j=\chi (L-T_ j)B_{1/j}/Z_ j$, extend $\beta _ j$ by zero, and set $g_ j=\varepsilon _ j+(1-\varepsilon _ j)\beta _ j$. Since $\chi $ is flat at the endpoints, $\beta _ j$ is smooth; it vanishes near $o$ and near the hyperplane $\{ L=1\} $. Its integral against $\kappa ^ k$ is one, so $g_ j$ is a smooth strictly positive probability density with respect to $\kappa ^ k$. Moreover,

\[ w_ jM_ j(1-\varepsilon _ j)\beta _ j\leq B_{1/j}/2. \]

Step 3: the scalars $c_ H(f_ j)$. By theorem 14.2.1 on $Y$, there is a smooth $\phi _ j$ with $\kappa +\mathrm{dd}^{\mathrm{c}}\phi _ j>0$ and $(\kappa +\mathrm{dd}^{\mathrm{c}}\phi _ j)^ k=g_ j\kappa ^ k$; the scalar is one because both sides have mass one. On $X_0$, the same theorem gives a smooth $v_ j$ with $h_0+\mathrm{dd}^{\mathrm{c}}v_ j>0$ and $(h_0+\mathrm{dd}^{\mathrm{c}}v_ j)^ m=c_{h_0}(F_ j)F_ j\, \mathrm dV_0$. Since only one term of the binomial expansion survives for dimensional reasons,

\[ (H+\mathrm{dd}^{\mathrm{c}}(v_ j+\phi _ j))^ N =C c_{h_0}(F_ j)F_ jg_ j\mu =C c_{h_0}(F_ j)f_ j\, \mathrm dV. \]

Uniqueness of the scalar gives $c_ H(f_ j)=C c_{h_0}(F_ j)\leq 2^{-2j}$.

Step 4: properties of $f$. By Tonelli's theorem, $\int _ Xf\, \mathrm dV=\sum _ jw_ j=1$. The density of $f\, \mathrm{d}V$ with respect to $\mu $ is

\[ F=f/R=\sum _ jw_ jF_ jg_ j=E+\sum _ jw_ j(1-\varepsilon _ j)F_ j\beta _ j. \]

The annuli are disjoint and escape to the pole, so only finitely many bumps meet any compact subset of $Y\setminus \{ o\} $; hence $F$, and therefore $f$, is smooth off the pole fiber. On the pole fiber all bumps vanish and $F=E$, so $f$ is finite everywhere. Also $f\geq w_1f_1\geq \frac12\min _ Xf_1>0$. If $\mathrm{MA}^{\mathrm{ext}}_ H(u)\geq af\, \mathrm{d}V$ with $a>0$, then $\mathrm{MA}^{\mathrm{ext}}_ H(u)\geq aw_ jf_ j\, \mathrm{d}V$, and lemma 15.27.1 gives

\[ aw_ j\leq c_ H(f_ j)\leq 2^{-2j},\quad \text{that is,}\quad a\leq 2^{-j}, \quad \text{for every }j. \]

This is impossible, so $b_ H(f)=0$ by theorem 15.28.4.

Step 5: exponential subsolutions. Fix $\lambda >0$, and choose $J$ with $1/j\leq \lambda $ for $j\geq J$. Since $L^\alpha -1\geq 0$, we have $B_{1/j}\leq B_\lambda $ for these $j$. As the bumps have disjoint supports, Step 2 bounds their total contribution $\sum _{j\geq J}w_ j(1-\varepsilon _ j)F_ j\beta _ j$ by $B_\lambda /2$. The baseline satisfies $E\leq b_0/4\leq B_\lambda /4$, because $B_\lambda \geq q_\alpha \geq b_0$. The remaining finitely many bumps are bounded by the constant

\[ K_\lambda =\max _ Y\sum _{j<J}w_ j(1-\varepsilon _ j)M_ j\beta _ j, \]

and $K_\lambda \leq (K_\lambda /b_0)B_\lambda $. Hence $F\leq A_\lambda B_\lambda $ with $A_\lambda =3/4+K_\lambda /b_0$, and theorem 15.35.9 gives the exponential subsolution $u_\alpha +\lambda ^{-1}\log (CV_0/A_\lambda )$ and the greatest solution. Finally, a bounded solution $u$ would satisfy $\mathrm{MA}^{\mathrm{ext}}_ H(u)\geq \mathrm{e}^{\lambda \inf _ Xu}f\, \mathrm{d}V$, a positive scaled subsolution, contradicting $b_ H(f)=0$. Hence every solution is unbounded. $\square$

The density just constructed also satisfies the criterion in part (2) of theorem 15.35.9: on the $j$th annulus, $F/q_\alpha \leq 1/4+\frac12\mathrm e^{(L^\alpha -1)/j}$, and away from all annuli the ratio is at most $1/4$. Approaching the pole through the annuli forces $j\to \infty $, so the required limit is zero. Since $b_ H(f)=0$, proposition 15.28.7 also shows that $f$ belongs to no $L^ p$ with $p>1$.

Densities $F_ j$ as in the theorem exist whenever $v_-(h_0)=0$, by theorem 12.15.4, theorem 12.2.3. For instance, on the elliptic threefold, theorem 12.19.1 gives smooth functions $v_\ell $ with $h_0+\mathrm{dd}^{\mathrm{c}}v_\ell >0$ and masses $\delta _\ell =\int _{X_0}(h_0+\mathrm{dd}^{\mathrm{c}}v_\ell )^3\to 0$. The probability densities $F_\ell =(h_0+\mathrm{dd}^{\mathrm{c}}v_\ell )^3/(\delta _\ell \, \mathrm dV_0)$ satisfy $c_{h_0}(F_\ell )=\delta _\ell $ by uniqueness of the scalar, and a subsequence with $\delta _{\ell _ j}\leq 2^{-2j}/C$ gives the required densities. Thus the construction applies to this threefold times $\mathbb P^ k$ for every $k\geq 1$. With the balanced metric of proposition 12.19.18, $V_0=24\pi $, so the explicit subsolutions have mass $CV_0$, equal to $96\pi $ on the fourfold ($k=1$) and $240\pi $ on the fivefold ($k=2$). These values concern the subsolutions; the greatest solutions have their own finite positive masses.

In this construction the projective components $g_ j$ are chosen after the densities $F_ j$, to fit them. We do not know whether the exponential equation is solvable for every prescribed concentration family of this kind, and we have no necessary criterion for solvability at zero threshold.

15.35.11 Solvable exponents and collapse at zero threshold4B9655E85450

We return to a general Hermitian form $h$ on $X$ and a nonzero density $0\leq f\in L^1(\mathrm dV)$. Let $\Lambda _ h(f)$ be the set of exponents $\lambda >0$ for which (15.35.1) has a solution. By theorem 15.35.2, $\lambda \in \Lambda _ h(f)$ if and only if the equation has an exponential subsolution at exponent $\lambda $.

Proposition 15.35.12.B2DB6BD3AC4D If $\lambda _0\in \Lambda _ h(f)$, then $[\lambda _0,+\infty )\subset \Lambda _ h(f)$. Consequently, $\Lambda _ h(f)$ is empty, or equals $(a,+\infty )$ for some $a\geq 0$, or equals $[a,+\infty )$ for some $a>0$. If $b_ h(f)>0$, then $\Lambda _ h(f)=(0,+\infty )$.

Proof. Let $u$ be a solution at $\lambda _0$, and put $s=u-\max (0,\sup _ Xu)$. Then $s\leq \min (u,0)$, so for $\lambda \geq \lambda _0$,

\begin{align*} \mathrm{MA}^{\mathrm{ext}}_ h(s) & =\mathrm e^{\lambda _0u}f\, \mathrm dV\\ & \geq \mathrm e^{\lambda _0s}f\, \mathrm dV \geq \mathrm e^{\lambda s}f\, \mathrm dV. \end{align*}

Thus $s$ is an exponential subsolution at every $\lambda \geq \lambda _0$, and theorem 15.35.2 gives a solution. Hence $\Lambda _ h(f)$ contains $[\lambda _0,+\infty )$ together with each of its points $\lambda _0$. A nonempty subset of $(0,+\infty )$ with this property is determined by its infimum $a$ and by whether $a$ belongs to it, which gives the stated forms. If $b_ h(f)>0$, corollary 15.35.3 gives $\Lambda _ h(f)=(0,+\infty )$. $\square$

Proposition 15.35.13.C791D4F48DEC Suppose $b_ h(f)=0$. Let $\lambda _ j>0$ decrease to zero, and let $u_ j$ be any solution of (15.35.1) at exponent $\lambda _ j$. Put

\[ M_ j=\sup _ Xu_ j,\qquad v_ j=u_ j-M_ j,\qquad c_ j=\mathrm e^{\lambda _ jM_ j}. \]

Then

\begin{gather*} c_ j\longrightarrow 0,\qquad \lambda _ jM_ j\longrightarrow -\infty ,\\ \| \mathrm{MA}^{\mathrm{ext}}_ h(u_ j)\| _{\mathrm{TV}} =\| \mathrm{MA}^{\mathrm{ext}}_ h(v_ j)\| _{\mathrm{TV}} \longrightarrow 0. \end{gather*}

Moreover, $\mathrm e^{\lambda _ ju_ j}\to 0$ uniformly on $X$, where the exponential is zero on the pole set, and $u_ j\to -\infty $ uniformly, that is, $\sup _ Xu_ j\to -\infty $.

Proof. Set $g_ j=\mathrm e^{\lambda _ jv_ j}f$. By lemma 5.44.5, applied to the finite non-pluripolar measure $f\, \mathrm dV$, $g_ j\to f$ in $L^1$; each $g_ j$ is nonzero, since $v_ j$ is finite almost everywhere. Since the Monge–Ampère measure is unchanged by adding constants,

\[ \mathrm{MA}^{\mathrm{ext}}_ h(v_ j)=c_ jg_ j\, \mathrm dV, \qquad \text{hence}\qquad 0<c_ j\leq b_ h(g_ j) \]

by theorem 15.28.4. The upper semicontinuity of the threshold, theorem 15.32.1, gives $\limsup _ jc_ j\leq b_ h(f)=0$. Since $0\leq g_ j\leq f$, the total masses are at most $c_ j\| f\| _{L^1}$ and tend to zero. Moreover $\lambda _ jM_ j=\log c_ j\to -\infty $, and $0\leq \mathrm e^{\lambda _ ju_ j}\leq \mathrm e^{\lambda _ jM_ j}=c_ j$. Finally, once $\lambda _ j<1$ and $\log c_ j<0$, we have $M_ j=\lambda _ j^{-1}\log c_ j\leq \log c_ j$, so $M_ j\to -\infty $. $\square$

For the density of theorem 15.35.10, solutions exist for every positive exponent, so the collapse applies as $\lambda \downarrow 0$ to every choice of solutions, in particular to the greatest ones. By contrast, the subsolutions of theorem 15.35.9 keep the mass $CV_0$ for every exponent, while the masses of the solutions above them tend to zero: on a nonclosed background, the order of two potentials does not give an order of their total Monge–Ampère masses. Whether the normalized potentials converge in capacity, and which equation a normalized cluster limit satisfies at exponent zero, are not decided by this argument. Positive endpoints of $\Lambda _ h(f)$ are governed instead by the compactness criterion below.

15.35.14 Positive endpoints and one-sided limits44A2CB44D7CB

For $\lambda \in \Lambda _ h(f)$, write $U_\lambda $ for the greatest solution given by theorem 15.35.2. When the exponents stay above a fixed $\tau >0$, the solution of a bounded truncated equation at exponent $\tau $ is a common upper barrier for all subsolutions. Together with the maximality of greatest solutions, this barrier gives an order estimate between $U_{\lambda _1}$ and $U_{\lambda _2}$, which controls the positive endpoint of $\Lambda _ h(f)$ and the limits of $U_\lambda $ from the right.

Lemma 15.35.15.A9F34BD594E1 For every $\tau >0$, there is a nonnegative $t_\tau \in \mathrm{PSH}(X,h)\cap C(X)$ such that every exponential subsolution at an exponent $\lambda \geq \tau $ lies below $t_\tau $. Put $K_\tau =\sup _ Xt_\tau $. If $\tau \leq \lambda _1\leq \lambda _2$ belong to $\Lambda _ h(f)$, then

\[ U_{\lambda _2}\geq U_{\lambda _1} -K_\tau \frac{\lambda _2-\lambda _1}{\lambda _2}. \]

Consequently, $\lambda \mapsto U_\lambda +K_\tau \log (\lambda /\tau )$ is nondecreasing on $\Lambda _ h(f)\cap [\tau ,+\infty )$.

Proof. Set $q=\min (f,1)$, a nonzero bounded density. By theorem 14.19.3, there is a continuous $w\in \mathrm{PSH}(X,h)$ with $\mathrm{MA}_ h(w)=\mathrm e^{\tau w}q\, \mathrm dV$. Put $t_\tau =w+\max (0,-\inf _ Xw)$. Then $t_\tau \geq 0$ and $t_\tau \geq w$, so for $\lambda \geq \tau $,

\[ \mathrm{MA}_ h(t_\tau )=\mathrm e^{\tau w}q\, \mathrm dV \leq \mathrm e^{\lambda t_\tau }f\, \mathrm dV. \]

Let $u$ be an exponential subsolution at an exponent $\lambda \geq \tau $, and let $\epsilon >0$. On $\{ t_\tau <u-\epsilon \} $,

\[ \mathrm{MA}_ h(t_\tau ) \leq \mathrm e^{\lambda (u-\epsilon )}f\, \mathrm dV \leq \mathrm e^{-\lambda \epsilon } \mathrm{MA}^{\mathrm{ext}}_ h(u-\epsilon ). \]

The bounded function $t_\tau $ satisfies $P_{h/2}(t_\tau )\not\equiv -\infty $, and $u-\epsilon \preceq t_\tau $. Thus theorem 15.2.2 gives $t_\tau \geq u-\epsilon $, and letting $\epsilon \downarrow 0$ gives $t_\tau \geq u$.

For the order estimate, put $\delta =K_\tau (\lambda _2-\lambda _1)/\lambda _2$. By the first part, $U_{\lambda _1}\leq t_\tau \leq K_\tau $, so $(\lambda _2-\lambda _1)U_{\lambda _1}\leq \lambda _2\delta $, that is, $\lambda _1U_{\lambda _1}\geq \lambda _2(U_{\lambda _1}-\delta )$. Since the Monge–Ampère measure is unchanged by adding constants,

\begin{align*} \mathrm{MA}^{\mathrm{ext}}_ h(U_{\lambda _1}-\delta ) & =\mathrm e^{\lambda _1U_{\lambda _1}}f\, \mathrm dV\\ & \geq \mathrm e^{\lambda _2(U_{\lambda _1}-\delta )}f\, \mathrm dV. \end{align*}

Thus $U_{\lambda _1}-\delta $ is an exponential subsolution at $\lambda _2$, and the maximality of $U_{\lambda _2}$ gives $U_{\lambda _2}\geq U_{\lambda _1}-\delta $. Finally, $1-x^{-1}\leq \log x$ for $x\geq 1$; with $x=\lambda _2/\lambda _1$ this gives $\delta \leq K_\tau \log (\lambda _2/\lambda _1)$, which proves the monotonicity. $\square$

Proposition 15.35.16.9E30269224CD Suppose $\Lambda _ h(f)\ne \varnothing $ and $a=\inf \Lambda _ h(f)>0$. Then $a\in \Lambda _ h(f)$ if and only if there are exponents $\lambda _ j>a$ decreasing to $a$ and solutions $u_ j$ at exponent $\lambda _ j$ with $\inf _ j\sup _ Xu_ j> -\infty $.

If $a\notin \Lambda _ h(f)$, then every sequence of solutions $u_ j$ at exponents $\lambda _ j>a$ decreasing to $a$ satisfies

\begin{gather*} \sup _ Xu_ j\longrightarrow -\infty ,\qquad \mathrm e^{\lambda _ ju_ j}\longrightarrow 0\ \text{uniformly on }X,\\ \| \mathrm{MA}^{\mathrm{ext}}_ h(u_ j)\| _{\mathrm{TV}} \longrightarrow 0, \end{gather*}

where the exponential is zero on the pole sets.

Proof. Suppose first that $a\in \Lambda _ h(f)$, let $u_ a$ be a solution at $a$, and put $s=u_ a-\max (0,\sup _ Xu_ a)$. As in the proof of proposition 15.35.12, $s$ is an exponential subsolution at every $\lambda \geq a$, so $U_\lambda \geq s$. Hence the greatest solutions at any exponents $\lambda _ j\downarrow a$ have suprema at least $\sup _ Xs>-\infty $.

Conversely, let $\lambda _ j$ and $u_ j$ be as in the statement. The lemma with $\tau =a$ gives the common upper bound $u_ j\leq K_ a$. Write $M_ j=\sup _ Xu_ j$. After extraction, $M_ j\to M\in \mathbb R$ and, by theorem 5.25.2, $u_ j-M_ j\to v$ in $L^1$ for some $v\in \mathrm{PSH}(X,h)$. Then $u_ j\to u=v+M$ in $L^1$ and, after a further extraction, almost everywhere. Since $a\leq \lambda _ j\leq \lambda _1$, $u_ j\leq K_ a$ and $K_ a\geq 0$, the densities $\mathrm e^{\lambda _ ju_ j}f$ are bounded by $\mathrm e^{\lambda _1K_ a}f$, and dominated convergence gives

\[ \mathrm e^{\lambda _ ju_ j}f\longrightarrow \mathrm e^{au}f \quad \text{in }L^1(\mathrm dV). \]

Lemma 15.28.3 now gives $\mathrm{MA}^{\mathrm{ext}}_ h(u)\geq \mathrm e^{au}f\, \mathrm dV$. Thus $u$ is an exponential subsolution at $a$, and theorem 15.35.2 gives a solution at $a$.

Finally, suppose $a\notin \Lambda _ h(f)$, and let $u_ j$ be solutions at exponents $\lambda _ j\downarrow a$. If $\sup _ Xu_ j$ did not tend to $-\infty $, a subsequence would satisfy the condition just shown to imply $a\in \Lambda _ h(f)$. Hence $M_ j\to -\infty $. Once $M_ j<0$, since $\lambda _ j\geq a>0$,

\[ 0\leq \mathrm e^{\lambda _ ju_ j}\leq \mathrm e^{\lambda _ jM_ j}\leq \mathrm e^{aM_ j} \longrightarrow 0, \]

and the total mass $\int _ X\mathrm e^{\lambda _ ju_ j}f\, \mathrm dV$ is at most $\mathrm e^{aM_ j}\| f\| _{L^1}$. $\square$

Proposition 15.35.17.B1974D837A1A For every $a\in \Lambda _ h(f)$, the greatest solutions satisfy

\[ U_\lambda \longrightarrow U_ a \quad \text{in }L^1\text{ and in capacity}\quad (\lambda \downarrow a), \]

and their Monge–Ampère measures converge in total variation to $\mathrm e^{aU_ a}f\, \mathrm dV$.

Proof. Let $K=K_ a$ be the constant of the lemma with $\tau =a$, and let $\lambda _ j>a$ decrease to $a$. By the lemma, the functions

\[ V_ j=U_{\lambda _ j}+K\log (\lambda _ j/a) \]

decrease and satisfy $V_ j\geq U_ a$. Their limit $V$ therefore belongs to $\mathrm{PSH}(X,h)$ and satisfies $V\geq U_ a$. Dominated convergence between the integrable bounds $U_ a$ and $V_1$ gives $V_ j\to V$ in $L^1$, and lemma 5.29.19 gives convergence in capacity. Since the added constants tend to zero, $U_{\lambda _ j}\to V$ in both senses.

The nonpositive functions $U_{\lambda _ j}-K$ satisfy

\[ \mathrm{MA}^{\mathrm{ext}}_ h(U_{\lambda _ j}-K)=\mathrm e^{\lambda _ j(U_{\lambda _ j}-K)}\, \mathrm e^{\lambda _ jK}f\, \mathrm dV, \]

and $\mathrm e^{\lambda _ jK}f\to \mathrm e^{aK}f$ in $L^1$. Theorem 15.34.2 therefore gives $\mathrm{MA}^{\mathrm{ext}}_ h(V)=\mathrm e^{aV}f\, \mathrm dV$, together with total-variation convergence of the measures $\mathrm{MA}^{\mathrm{ext}}_ h(U_{\lambda _ j})$. Hence $V$ is a solution at $a$, so $V\leq U_ a$ by maximality, while $V\geq U_ a$ by construction. Thus $V=U_ a$. Since every sequence of exponents converging to $a$ from above has a decreasing subsequence, this proves the assertions. $\square$

The corrected order also controls approach from the left. The limit solves the equation at the limiting exponent; maximality gives an inequality with the greatest solution there, but does not force equality.

Proposition 15.35.18.0535F55900CB Suppose $\Lambda _ h(f)\ne \varnothing $, and put $a_0=\inf \Lambda _ h(f)$. For every $a>a_0$, there is $L_ a\in \mathrm{PSH}(X,h)$ such that

\[ U_\lambda \longrightarrow L_ a \quad \text{in }L^1\text{ and in capacity}\quad (\lambda \uparrow a). \]

It satisfies

\[ L_ a\leq U_ a,\qquad \mathrm{MA}^{\mathrm{ext}}_ h(L_ a)=\mathrm e^{aL_ a}f\, \mathrm dV. \]

The equation measures converge in total variation to this finite measure. The left limit is independent of the auxiliary exponent and of the cofinal sequence used to construct it.

Proof. Choose $\tau \in \Lambda _ h(f)$ with $0<\tau <a$; the upper-interval property gives such a choice. Put $K=K_\tau $ from lemma 15.35.15 and

\[ V_\lambda =U_\lambda +K\log (\lambda /\tau ) \qquad (\lambda \in \Lambda _ h(f),\ \lambda \geq \tau ). \]

This family is increasing. For a sequence $\lambda _ j\uparrow a$ with $\tau \leq \lambda _ j<a$, its members lie between the integrable potentials $V_\tau $ and $V_ a$. The upper-envelope construction in section 5.40 gives

\[ V^-_ a=\left(\sup _{\tau \leq \lambda <a}V_\lambda \right)^* =\left(\lim _ jV_{\lambda _ j}\right)^*\in \mathrm{PSH}(X,h). \]

Indeed cofinality and the order give the same pointwise supremum for every such sequence. Regularization changes it only on a pluripolar set. Dominated convergence between the integrable bounds gives $L^1$ convergence to $V^-_ a$, and lemma 5.29.19 gives convergence in capacity. Since the added constants converge, set

\[ L_ a=V^-_ a-K\log (a/\tau ). \]

Then $U_{\lambda _ j}\to L_ a$ in both topologies and $L_ a\leq U_ a$; the latter inequality survives regularization because $V_ a$ is upper semicontinuous.

The potentials $U_{\lambda _ j}-K$ and their limit $L_ a-K$ are nonpositive. Apply theorem 15.34.2 with exponents tending to $a>0$ and densities $\mathrm e^{\lambda _ jK}f\to \mathrm e^{aK}f$ in $L^1$. It proves the exact equation and total-variation convergence.

Every sequence approaching $a$ from the left has a cofinal increasing subsequence. If potential convergence in either topology, or total-variation convergence of the equation measures, failed, a sequence staying outside a fixed neighbourhood of the proposed limit would therefore have an increasing subsequence, contrary to the preceding argument. This proves the full left limit and measure convergence. Repeating the construction with another $\tau $ gives the same $L^1$ limit; canonical quasi-plurisubharmonic representatives that agree almost everywhere agree everywhere. Thus the auxiliary choice does not change $L_ a$. $\square$

Proposition 15.35.19.5E68200DBADD Suppose $\Lambda _ h(f)\ne \varnothing $, put $a_0=\inf \Lambda _ h(f)$, and let $L_ a$ be the left limit of proposition 15.35.18. The set

\[ D=\{ a>a_0:L_ a\ne U_ a\} \]

is at most countable. At every $a>a_0$ with $a\notin D$, the greatest solutions are continuous in $L^1$ and in capacity as $\lambda \to a$, and their equation measures converge in total variation to $\mathrm e^{aU_ a}f\, \mathrm dV$.

Proof. Fix $a_0<\alpha <\beta $, choose an admitted $0<\tau <\alpha $, and use the corrected family $V_\lambda $ from the preceding proof on $[\alpha ,\beta ]$. Its integrals

\[ I(\lambda )=\int _ XV_\lambda \, \mathrm dV \]

form a finite bounded increasing real function. For $a\in (\alpha ,\beta ]$, the left-limit proposition gives

\[ I(a)-I(a-)=\int _ X(U_ a-L_ a)\, \mathrm dV. \]

If $L_ a\ne U_ a$, this quantity is positive: the integrable nonnegative difference cannot vanish almost everywhere without equality of the canonical potentials. For any finite ordered collection of such points, the sum of their jumps is at most $I(\beta )-I(\alpha )$. Consequently there are only finitely many jumps at least $1/m$ for each positive integer $m$, and at most countably many positive jumps. A countable cover by intervals with rational endpoints inside $(a_0,+\infty )$ proves the assertion about $D$.

If $a\notin D$, the left limit is $U_ a$, and proposition 15.35.17 supplies the same right limit in both topologies and for the equation measures. Splitting an arbitrary approaching sequence into its two sides proves the stated two-sided convergence. $\square$

Whether an actual jump occurs, or all left limits equal the greatest solution, remains undecided. An intrinsic criterion on $f$ and the existence or nonexistence of a positive excluded endpoint remain separate questions. These one-sided limits concern greatest solutions at positive exponents; they do not identify limits of arbitrary solutions with other singularities or supply a zero-exponent limit.

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