Proposition 17.16.29.A3E893F6A601 The pullback $\pi ^*v_ t$ is the full Hermitian Perron segment and is stationary under all smooth fixed-endpoint variations. Its distance and action are
17.16.28 Explicit basic geodesics and singular potentials1DFB5A5992AD
Diagonal projective automorphisms give smooth nonconstant geodesics. For real $a_0,\ldots ,a_{n-1}$, set
The family is spatially nonconstant when the $a_ j$ are not all equal.
Proof. On the strip, the holomorphic map $F([z],s)=[\mathrm e^{a_0s/2}z_0:\cdots :\mathrm e^{a_{n-1}s/2}z_{n-1}]$ satisfies $\operatorname {pr}_ Y^*\kappa +\mathrm{dd}^{\mathrm{c}}V=F^*\kappa $. The imaginary-time phases are unitary, so $V$ depends only on $\operatorname{Re}s$. This form has rank $d$, strictly positive spatial slices, and zero $(d+1)$st power. The classical bounded Kähler Dirichlet uniqueness identifies it with the base Perron segment; proposition 17.16.16, proposition 17.16.22 give the full segment and its stationarity.
For $x_ j=|z_ j|^2/\sum |z_ j|^2$, the initial velocity is $\sum _ ja_ jx_ j$. A standard complex Gaussian vector has independent exponential squared coordinates, and its projective direction has distribution $\kappa ^ d$. Dividing those coordinates by their sum gives the uniform simplex distribution, with moments
The smooth distance formula and (17.16.20) give the claimed squared distance; the action is half of it. $\square$
For instance, $n=3$ and $(a_0,a_1,a_2)=(1,-1,0)$ give squared distance one and action $1/2$.
The completed space also contains potentials with different ordinary singularity types. Put $o=[1:0:\cdots :0]\in Y$ and
with the canonical value $v_ a(o)=-\infty $.
Proposition 17.16.30.9355B610E2C3 Every $v_ a$ has non-pluripolar mass one, and
At equality its squared energy diverges logarithmically. The pullback has mass $2n$ and pole set $\pi ^{-1}(o)$. If $0<a<b<d/(d+2)$, the two pullbacks have different ordinary singularity types and finite positive $d_ B$ distance.
Proof. In the chart $z_0=1$, write $s=\log |z'|^2$, $L=\log (1+\mathrm e^ s)$, $P=\mathrm e^ s/(1+\mathrm e^ s)$, and $T=1+L-s\geq 1$. The local potential $\Phi =L+1-T^ a$ has derivative
Both $A$ and $A'$ are positive, so the radial complex Hessian is positive. Its bounded-above local potential extends plurisubharmonically across $o$ by lemma 5.24.7. The function extends smoothly across the hyperplane at infinity. Its bounded plurisubharmonic truncations decrease to a nontrivial canonical potential: near $o$, $|v_ a|=O((1-s)^ a)$ is integrable against radial smooth volume $O(\mathrm e^{ds})\, \mathrm ds$.
The radial mass flux is $Q(s)=A(s)^ d$. Its sphere coefficient is one, since $\mathrm d^{\mathrm c}\log |z'|^2$ integrates to one on the Hopf circle and $\mathrm{dd}^{\mathrm{c}}\log |z'|^2$ induces mass-one Fubini–Study on $\mathbb P^{d-1}$. Stokes on an annulus gives mass $Q(s_2)-Q(s_1)$. Since $Q(-\infty )=0$ and $Q(+\infty )=1$, finite-level locality and annular exhaustion give non-pluripolar mass one. The pole has no atom, and smoothness gives no mass on the hyperplane at infinity.
As $s\to -\infty $,
The squared energy therefore converges exactly when $2a-d(1-a)<0$. At equality the integrand has order $T^{-1}$, giving logarithmic divergence. All other compact regions have smooth potentials and measures. Fiber integration gives the pullback assertions. Finally, $v_ a-v_ b=T^ b-T^ a\to +\infty $ at $o$, so mutual bounded comparison fails. Both points lie in the completed metric space and are distinct, giving finite positive distance. $\square$
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