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 $F=f/R$.
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.
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.
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