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5 The Mukai-Umemura manifold and its deformations [02AK]

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5 The Mukai-Umemura manifold and its deformations

The first part of this section gives an account, not aimed at algebraic geometry specialists, of a very interesting family of Fano 33-folds, following Mukai. The basic references are [22], [23], but there are also many other relevant papers in the algebraic geometry literature. Then we go on to discuss the existence of Kahler-Einstein metrics on some manifolds in this family.

5.1 Mukai’s construction

We start with a 77-dimensional complex vector space VV and write G​r3​(V)Gr_{3}(V) for the Grassmann manifold of 3-dimensional subspaces of VV. So G​r3​(V)Gr_{3}(V) has dimension 3.(7−3)=123.(7-3)=12. A form Ω∈Λ2​(V∗)\Omega\in\Lambda^{2}(V^{*}) defines a subset ZΩ⊂G​r3​(V)Z_{\Omega}\subset Gr_{3}(V) consisting of the 33-planes PP such that Ω|P\Omega|_{P} vanishes. In other language we consider the tautological rank 3 vector bundle U→G​r3​(V)U\rightarrow Gr_{3}(V); the form Ω\Omega defines a section sΩs_{\Omega} of Λ2​U∗\Lambda^{2}U^{*} with zero set ZΩZ_{\Omega}. For generic Ω\Omega this zero set is a smooth subvariety of codimension 33. Now let Ω1,Ω2,Ω3\Omega_{1},\Omega_{2},\Omega_{3} be three such forms and consider

X=ZΩ1∩ZΩ2∩ZΩ3⊂G​r3​(V).X=Z_{\Omega_{1}}\cap Z_{\Omega_{2}}\cap Z_{\Omega_{3}}\subset Gr_{3}(V).

Of course this only depends on the 33-plane Π\Pi in Λ2​V∗\Lambda^{2}V^{*} spanned by the Ωi\Omega_{i}, so we may sometimes write XΠX_{\Pi}. Obviously there is a Zariski-open subset 𝒰{\cal U} in the Grassmannian G​r3​(Λ2​V∗)Gr_{3}(\Lambda^{2}V^{*}) of 33-planes Π\Pi such that XΠX_{\Pi} is a smooth subvariety of dimension 12−3.3=312-3.3=3. This set 𝒰{\cal U} is non-empty, as we will see later. The group S​L​(V)SL(V) acts on the whole construction and obviously different subspaces Π\Pi which lie in the same S​L​(V)SL(V) orbit define isomorphic manifolds XΠX_{\Pi}, so we get a set of equivalence classes of manifolds constructed in this way, parametrised by the quotient 𝒰/S​L​(V){\cal U}/SL(V). (Mukai shows further that this parametrisation is effective: i.e. XΠ1X_{\Pi_{1}} is isomorphic to XΠ2X_{\Pi_{2}} if and only if Π1,Π2\Pi_{1},\Pi_{2} lie in the same S​L​(V)SL(V) orbit. Moreover, he shows that all “prime Fano 33-folds of genus 12” arise in this way.)

We compute the canonical bundle KXK_{X} of the variety X=XΠX=X_{\Pi} for some Π∈𝒰\Pi\in{\cal U}. We have

Λ2​U∗=U⊗H\Lambda^{2}U^{*}=U\otimes H

where HH is the ample line bundle Λ3​U∗\Lambda^{3}U^{*}. So, writing det\det for the the top exterior power of a vector bundle, we have

detΛ2​U∗=H⊗2.\det\Lambda^{2}U^{*}=H^{\otimes 2}.

The tangent bundle of the Grassmannian at a 33-plane P⊂VP\subset V can be identified with P∗⊗V/PP^{*}\otimes V/P. So

detT​G​r3=H⊗7.\det TGr_{3}=H^{\otimes 7}.

Now since the tangent bundle of XX is the kernel of a surjective map from T​G​r3​(V)TGr_{3}(V) to Λ2​U∗⊕Λ2​U∗⊕Λ2​U∗\Lambda^{2}U^{*}\oplus\Lambda^{2}U^{*}\oplus\Lambda^{2}U^{*} we have

KX−1=detT​X=H⊗(7−3.2)=H.K_{X}^{-1}=\det TX=H^{\otimes(7-3.2)}=H.

Thus XX is a Fano manifold. The sections of HH over G​r3Gr_{3} give the Plucker embedding

G​r3​(V)→𝐏⁡(Λ3​V)=𝐏34Gr_{3}(V)\rightarrow{\bf P}(\Lambda^{3}V)={\bf P}^{34}

For any 33-form A∈Λ3​V∗A\in\Lambda^{3}V^{*} we get a hyperplane section YA⊂G​r3​(V)Y_{A}\subset Gr_{3}(V) which just consists of the 33-planes PP such A|P=0A|_{P}=0. By definition this occurs if PP is in XX and AA is in the image of the wedge product map Π⊗V∗→Λ3​V∗\Pi\otimes V^{*}\rightarrow\Lambda^{3}V^{*}. We expect this map to have an image of dimension 7.3=217.3=21 in which case the image of the composite

X→G​r3​(V)→𝐏34X\rightarrow Gr_{3}(V)\rightarrow{\bf P}^{34}

lies in a linear subspace 𝐏34−21=𝐏13{\bf P}^{34-21}={\bf P}^{13}. Certainly this map is defined by sections of KX−1K_{X}^{-1}, we will see later that H0​(X,KX−1)H^{0}(X,K_{X}^{-1}) has dimension 1414 and that this embedding is that given by the anticanonical system.

To make this more concrete we show now that XX is a rational variety; that is, we construct an explicit parametrisation of a dense open set in XX. Suppose we have a pair of 33-dimensional subspaces P0,Q0⊂VP_{0},Q_{0}\subset V with P0∩Q0=0P_{0}\cap Q_{0}=0. We ask what 33-planes PP in the 66-dimensional subspace P0⊕Q0P_{0}\oplus Q_{0} lie in XX. In matrix notation, we can write the restriction of a form Ω\Omega to P0⊕Q0P_{0}\oplus Q_{0} as

(σA−ATτ)\left(\begin{array}[]{cc}\sigma&A\\ -A^{T}&\tau\end{array}\right)

Now consider the 33-dimensional subspaces PP which arise as the graphs of linear maps M:P0→Q0M:P_{0}\rightarrow Q_{0}. The condition becomes

σ+MT​τ​M+(A​M−(A​M)T)=0.\sigma+M^{T}\tau M+(AM-(AM)^{T})=0. (33)

So our three forms Ωi\Omega_{i} give us three triples Ai,σi,τiA_{i},\sigma_{i},\tau_{i} and we have three equations of the form (33) to solve to find a point of XX. We have 99 unknowns: the entries of the matrix MM. The left hand side of (33) takes values in the 33-dimensional space of skew symmetric 3×33\times 3 matrices so we obtain a total of 3.3=93.3=9 equations in these 99 unknowns and we expect a finite number of solutions. These equations are quadratic and one can solve them explicitly, to see that there are generically two solutions. However it is easier to suppose that we are in the case when P0P_{0} itself lies in XX. This means that all the τi\tau_{i} are zero, so the equations (33) become linear. Generically this system of 99 linear equations in 99 unknowns is nondegerate and there is a unique solution. Now suppose we have found one point P0P_{0} in XX and consider the space of 66-planes in VV which contain P0P_{0}. This is a copy of projective 33-space 𝐏3{\bf P}^{3}. Given a point in 𝐏3{\bf P}^{3}, that is to say a 6 dimensional subspace EE of VV, we choose a complementary subspace to write is as E=P0⊕Q0E=P_{0}\oplus Q_{0}. Then we can proceed as above and, by solving linear equations, find the points of X∩G​r3​(E)X\cap Gr_{3}(E). Generically there is just one, PEP_{E} say, different from the original P0P_{0}. Conversely for any P′∈XP^{\prime}\in X the sum P⊕P′P\oplus P^{\prime} lies in a 66-dimensional subspace. Of course there will be various exceptional cases, but the upshot is that we get a birational map from 𝐏3{\bf P}^{3} to XX which takes a subspace EE containing P0P_{0} to PEP_{E}.

We now consider a special manifold in this family. Take the vector space VV to be the sixth symmetric power s6s^{6} of the fundamental representation of S​L​(2,𝐂)SL(2,{\bf C}). Then Λ2​V∗=Λ2​s6\Lambda^{2}V^{*}=\Lambda^{2}s^{6} decomposes into distinct irreducible representations

Λ2​s6=s10⊕s6⊕s2.\Lambda^{2}s^{6}=s^{10}\oplus s^{6}\oplus s^{2}.

The s2s^{2} summand is a 33-plane Π0\Pi_{0} invariant under S​L​(2,𝐂)SL(2,{\bf C}), so there is a natural S​L​(2,𝐂)SL(2,{\bf C}) action on the corresponding variety, the Mukai-Umemura manifold, X0=XΠ0X_{0}=X_{\Pi_{0}}. We will see below that X0X_{0} admits a Kahler-Einstein metric. The representation s6s^{6} has a standard invariant symmetric form (,)(\ ,\ ) and the inclusion s2→Λ2​s6s^{2}\rightarrow\Lambda^{2}s^{6} is just the map from the Lie algebra of S​L​(2,𝐂)SL(2,{\bf C}) given by the action on s6s^{6}. This comes down to saying that a 33-plane PP is in X0X_{0} if and only if

(δ​p,q)=0(\delta p,q)=0 (34)

for all p,q∈Pp,q\in P and δ∈𝔰​𝔩2\delta\in\mathfrak{s}\mathfrak{l}_{2}. Notice that the action of S​L​(2,𝐂)SL(2,{\bf C}) on all the spaces involved actually factors through P​S​L​(2,𝐂)PSL(2,{\bf C}).

Identify the projectivisation of the fundamental representation s1=𝐂2s^{1}={\bf C}^{2} with the standard round sphere and fix an icosahedron, which can be regarded as a set of 12 vertices in in this sphere. Thus we get a symmetry group Γ⊂S​O​(3)⊂P​S​L​(2,𝐂)\Gamma\subset SO(3)\subset PSL(2,{\bf C}) of order 6060. There is a simple way to see that the 77-dimensional representation s6s^{6} of P​S​L​(2,𝐂)PSL(2,{\bf C}) becomes reducible when restricted to Γ\Gamma. There are 66 pairs of antipodal vertices and for each such pair p,p¯p,\overline{p} we have a 11-dimensional subspace consisting of polynomials which vanish to order 33 at p,p¯p,\overline{p}. The sum of these 66 subspaces is obviously invariant under Γ\Gamma and is a proper subspace of s6s^{6} since it has codimension at least 11. A little calculation shows that this invariant subspace is of dimension 33 and satisfies the criterion (34). So this subspace gives a point P0P_{0} in X0X_{0} fixed by Γ\Gamma. On the other hand the stabiliser of P0P_{0} is obviously not the whole of S​O​(3)SO(3) and, since there is no finite subgroup of S​O​(3)SO(3) strictly larger than Γ\Gamma, the stabiliser must be exactly Γ\Gamma.

Now go back to the wedge product P0∧V∗→Λ3​V∗P_{0}\wedge V^{*}\rightarrow\Lambda^{3}V^{*}. In terms of representations this is an S​L​(2,𝐂)SL(2,{\bf C})-map

s2⊗s6→Λ3​s6.s^{2}\otimes s^{6}\rightarrow\Lambda^{3}s^{6}.

It is an exercise in representation theory to show that

Λ3​s6=s12⊕s8⊕s6⊕s4⊕s2⊕s0⊕s0.\Lambda^{3}s^{6}=s^{12}\oplus s^{8}\oplus s^{6}\oplus s^{4}\oplus s^{2}\oplus s^{0}\oplus s^{0}.

So comparing with

s2⊗s6=s8⊕s6⊕s4⊕s2⊕s0s^{2}\otimes s^{6}=s^{8}\oplus s^{6}\oplus s^{4}\oplus s^{2}\oplus s^{0}

we see that the embedding X0⊂G​r3​(V)⊂𝐏⁡(Λ3​V)X_{0}\subset Gr_{3}(V)\subset{\bf P}(\Lambda^{3}V) gives rise to an S​L​(2,𝐂)SL(2,{\bf C})-equivariant embedding

X0→𝐏⁡(s0⊕s12).X_{0}\rightarrow{\bf P}(s^{0}\oplus s^{12}). (35)

In other words, by our identification of the anticanonical bundle K−1K^{-1} we have

H0​(X0,K−1)=s0⊕s12,H^{0}(X_{0},K^{-1})=s^{0}\oplus s^{12},

as a representation of S​L​(2,𝐂)SL(2,{\bf C}).In particular, there is an S​L​(2,𝐂)SL(2,{\bf C})-invariant section σ\sigma of K−1K^{-1}. Explicitly, if we identify Λ3​s6\Lambda^{3}s^{6} with Λ4​s6\Lambda^{4}s^{6} then σ\sigma corresponds to the 44-form on V=s6V=s^{6} defined as follows. We choose any orthonormal basis Ω1,Ω2,Ω3\Omega_{1},\Omega_{2},\Omega_{3} of P0P_{0} and write down the 44-form

∗σ=Ω12+Ω22+Ω32.*\sigma=\Omega_{1}^{2}+\Omega_{2}^{2}+\Omega_{3}^{2}.

In this way, we get another description of the manifold X0X_{0}. Our point P0∈X0P_{0}\in X_{0} cannot lie in the zero set of σ\sigma (since its orbit is 33-dimensional). So, in the embedding (35), we have

P0=[1,v0]∈𝐏⁡(𝐂⊕s12).P_{0}=[1,v_{0}]\in{\bf P}({\bf C}\oplus s^{12}).

Thus v0v_{0} is an element of s12s^{12} whose stabiliser in P​S​L​(2,𝐂)PSL(2,{\bf C}) is exactly Γ\Gamma.Now there is an obvious element of the projective space 𝐏⁡(s12){\bf P}(s^{12}) with stabiliser Γ\Gamma, just the configuration of vertices of the icosahedron, regarded as an element of the symmetric product. Since Γ\Gamma is a perfect group it must act trivially on the corresponding line in s12s^{12}, so we get a vector in s12s^{12} with stabiliser Γ\Gamma. It is easy to see that, up to a multiple, this in the only element of s12s^{12} with stabiliser Γ\Gamma, and thus we have identified v0v_{0}. Then we can simply define X0X_{0} to be the closure in 𝐏⁡(𝐂⊕s12){\bf P}({\bf C}\oplus s^{12}) of the P​S​L​(2,𝐂)PSL(2,{\bf C})-orbit of v0v_{0} in s12s^{12}. (Here we are regarding the vector space s12s^{12} as being a subset of the projective space 𝐏⁡(𝐂⊕s12){\bf P}({\bf C}\oplus s^{12}) in the familiar way.)

In this description, the intersection of X0X_{0} with the hyperplane at infinity

D=𝐏⁡(s12)⊂𝐏⁡(𝐂⊕s12),D={\bf P}(s^{12})\subset{\bf P}({\bf C}\oplus s^{12}),

is, by definition, the zero set of the invariant section σ\sigma of K−1K^{-1}. Consider a 11-parameter subgroup λt\lambda_{t} in P​S​L​(2,𝐂)PSL(2,{\bf C}). Thus we have a pair of distinct point z+,z−z_{+},z_{-} such that when tt is large positive the map λt\lambda_{t} contracts most of the sphere to a small neighbourhood of z+z_{+}, and when tt is large negative to a small neighbourhood of z−z_{-}. If y1,…​y12y_{1},\dots y_{12} is any configuration of distinct points it is not hard to see that the limit as t→∞t\rightarrow\infty of

λt​(y¯)=(λt​(y1),λt​(y2​…​λt​(y12))CLOSE\lambda_{t}(\underline{y})=\left(\lambda_{t}(y_{1}),\lambda_{t}(y_{2}\dots\lambda_{t}(y_{12})\right)

in the symmetric product 𝐏⁡(s12){\bf P}(s^{12}) is either 12​z+=(z+,z+,…,z+)12z_{+}=(z_{+},z_{+},\dots,z_{+}) (in the generic case) or 11​z++z−=(z+,…,z+,z−)11z_{+}+z_{-}=(z_{+},\dots,z_{+},z_{-}) (in the case when one of the yiy_{i} is z−z_{-}). Using this, Mukai and Umemura show that the divisor at infinity DD consists precisely of the union of points of the form 12​z+12z_{+} or 11​z++z−11z_{+}+z_{-} in 𝐏⁡(s12){\bf P}(s^{12}). It is easy to identify this geometrically. The points of the form 12​z+12z_{+} make up the rational normal curve in 𝐏⁡(s12){\bf P}(s^{12}). Our divisor DD is the surface swept out by the lines in 𝐏⁡(s12){\bf P}(s^{12}) tangent to the rational normal curve. As a set we can identify DD with 𝐏1×𝐏1{\bf P}^{1}\times{\bf P}^{1}: we just map (z+,z−)∈𝐏1×𝐏1(z_{+},z_{-})\in{\bf P}^{1}\times{\bf P}^{1} to 11​z++z−∈D11z_{+}+z_{-}\in D. But the surface DD is singular and a more precise statement is that the map above is a holomorphic map ν:𝐏1×𝐏1→D\nu:{\bf P}^{1}\times{\bf P}^{1}\rightarrow D which is the normalisation of DD. The singular set of DD is the image of the diagonal in 𝐏1×𝐏1{\bf P}^{1}\times{\bf P}^{1}, and it is easy to check that the singularity has the form of a cusp transverse to the diagonal. That is to say, we can choose local co-ordinates z1​z2,z3z_{1}z_{2},z_{3} in X0X_{0} around a singular point of DD such that DD is defined by the equation z12=z23z_{1}^{2}=z_{2}^{3}.

We now have a rather explicit description of X0X_{0}, as the compactification of P​S​L​(2,𝐂)/ΓPSL(2,{\bf C})/\Gamma formed by adjoining the divisor DD. We can use this to compute the action of P​S​L​(2,𝐂)PSL(2,{\bf C}) on all of the spaces of sections H0​(X0,K−p)H^{0}(X_{0},K^{-p}). For the pull back ν∗​(K−1)\nu^{*}(K^{-1}) is isomorphic to the line bundle 𝒪⁡(11,1){\cal O}(11,1) over 𝐏1×𝐏1{\bf P}^{1}\times{\bf P}^{1}. We can regard the structure sheaf of DD as a subsheaf of that of 𝐏1×𝐏1{\bf P}^{1}\times{\bf P}^{1}. From the local model of the singularity along the diagonal one sees that the quotient can be identified with sections of 𝒪⁡(2){\cal O}(2) along the diagonal. This means that H0​(D,K−p|D)H^{0}(D,K^{-p}|_{D}) is the kernel of a map H0​(𝐏1×𝐏1,𝒪⁡(11​p,p))→H0​(𝐏1,𝒪⁡(12​p−2))H^{0}({\bf P}^{1}\times{\bf P}^{1};{\cal O}(11p,p))\rightarrow H^{0}({\bf P}^{1};{\cal O}(12p-2)). As representations of P​S​L​(2,𝐂)PSL(2,{\bf C}) this is a map

s11​p⊗sp→s12​p−2.s^{11p}\otimes s^{p}\rightarrow s^{12p-2}.

Now

s11​p⊗sp=s12​p+s12​p−2​…⊕s10​ps^{11p}\otimes s^{p}=s^{12p}+s^{12p-2}\dots\oplus s^{10p}

and the map above is just the projection to the second factor. So

H0​(D,K−p|D)=s12​p⊕s12​p−4⊕s12​p−6​…⊕s10​p+2⊕s10​p.H^{0}(D;K^{-p}|_{D})=s^{12p}\oplus s^{12p-4}\oplus s^{12p-6}\dots\oplus s^{10p+2}\oplus s^{10p}.

Then the exact cohomology sequence of

0→K−(p−1)→K−p→K−p|D→00\rightarrow K^{-(p-1)}\rightarrow K^{-p}\rightarrow K^{-p}|_{D}\rightarrow 0

together with Kodaira vanishing on X0X_{0} gives

H0​(X0,K−p)=H0​(X0,K−(p−1))⊕s12​p⊕s12​p−4​…​s10​p,H^{0}(X_{0},K^{-p})=H^{0}(X_{0},K^{-(p-1)})\oplus s^{12p}\oplus s^{12p-4}\dots s^{10p},

and inductively we get a description of each H0​(X0,K−p)H^{0}(X_{0},K^{-p}). Thus

H0​(X0,K−1)=s0⊕s12,H^{0}(X_{0},K^{-1})=s^{0}\oplus s^{12},
H0​(X0,K−2)=s0⊕s12⊕s24⊕s20.H^{0}(X_{0},K^{-2})=s^{0}\oplus s^{12}\oplus s^{24}\oplus s^{20}.

For p≥6p\geq 6 we get multiplicities: H0​(X0,K−6)H^{0}(X_{0},K^{-6}) contains two copies of s60s^{60}. This illustrates the difference with the multiplicity-free case discussed above. (Although since the multiplicities are small until pp becomes quite large, once is tempted to think of X0X_{0} as being “close” to multiplicity-free. )

5.2 Topological and symplectic picture

We will now get another explicit picture of X0X_{0}, taking the point of view of symplectic geometry. Recall that all Kahler metrics in the cohomology class c1​(X0)c_{1}(X_{0}) define equivalent symplectic structures, so we have a well-defined symplectic manifold (X0,ω)(X_{0},\omega) with an S​O​(3)SO(3)-action. Thus we have an equivariant moment map

μ:X0→𝐑3=Lie​(S​O​(3))∗.\mu:X_{0}\rightarrow{\bf R}^{3}={\rm Lie}(SO(3))^{*}.

whose image is clearly a ball in 𝐑3{\bf R}^{3}. We can understand the structure of this moment map by restricting to a subgroup S1⊂S​O​(3)S^{1}\subset SO(3), say that corresponding to the x1x_{1}-axis in 𝐑3{\bf R}^{3}. Then the Hamiltonian HH for this circle action on X0X_{0} is the composite of μ\mu with projection to the x1x_{1}-axis. The critical points of HH are the fixed points of the circle action and we can find these explicitly. We can suppose that our circle subgroups corresponds to the standard action of

(λ1/200λ−1/2),\left(\begin{array}[]{cc}\lambda^{1/2}&0\\ 0&\lambda^{-1/2}\end{array}\right),

acting on 𝐂7{\bf C}^{7} with weights λ3,…​λ−3\lambda^{3},\dots\lambda^{-3}. We write eie_{i} for the basis vector belonging to the weight λi\lambda^{i}. This induces an action on the Grassmannian G​r3​(V)Gr_{3}(V) whose fixed points are just invariant 33-dimensional subspaces of 𝐂7{\bf C}^{7} and these are just the spans Pi​j​k=⟨ei,ej,ek⟩P_{ijk}=\langle e_{i},e_{j},e_{k}\rangle for distinct i,j,ki,j,k. By checking the 35 different cases, or otherwise, one finds that the only Pi​j​kP_{ijk} which satisfy the criterion (34) to lie in X0X_{0} are P123,P023,P0−2−3,P−1−2−3P_{123},P_{023},P_{0-2-3},P_{-1-2-3}. There is an action of the Weyl group {±1}\{\pm 1\} on the whole situation which commutes, up to sign, with the circle action, takes HH to −H-H and takes Pi​j​kP_{ijk} to P−i−j−kP_{-i-j-k}. So there are four fixed points of the circle action but to analyse the local structure around them it suffices to consider the two cases P123,P023P_{123},P_{023}. Notice that, by considering HH as a Morse function we immediately see that X0X_{0} has the same additive homology as 𝐂𝐏3{\bf C}{\bf P}^{3}. Notice also that the value of HH at a critical point is just given by the weight of the action on the fibre of K−1K^{-1} over this point, which is just i+j+ki+j+k at Pi​j​kP_{ijk}.

We next compute the weights of the circle action on the tangent spaces at the fixed points. This is similar to the calculation of the canonical bundle. At a fixed point the tangent space T​X0TX_{0}, viewed as a representation of S1S^{1}, can be written as the formal difference

T​G​r3​(V)−(Λ2​U∗⊗Lie⁡(S​O​(3))).TGr_{3}(V)-\left(\Lambda^{2}U^{*}\otimes{\rm Lie}(SO(3))\right).

Computing the weights of these two terms and subtracting we find that the weights of the action on the tangent space at P123P_{123} are (1,2,3)(1,2,3) and on the tangent space at P023P_{023} are (1,−1,5)(1,-1,5). In either case the orbit of the fixed point is a copy of S​O​(3)/S1=S2SO(3)/S^{1}=S^{2} in X0X_{0} and the weight 11 in the action on T​X0TX_{0} just corresponds to the tangent space of this orbit. The weights normal to the orbit are (2,3)(2,3) in the case of P123P_{123} and (−1,5)(-1,5) in the case of P023P_{023}.

With these calculations we can get a good picture of the map μ\mu. Write Σ,Σ′\Sigma,\Sigma^{\prime} for the orbits of P123P_{123} and P023P_{023} respectively. Then μ\mu restricts to an S​O​(3)SO(3)-equivariant equivalence between Σ\Sigma and the sphere of radius 1+2+3=61+2+3=6 in 𝐑3{\bf R}^{3} and between Σ′\Sigma^{\prime} and the sphere of radius 0+2+3=50+2+3=5. The image of μ\mu is the ball of radius 66 and the critical values of μ\mu are precisely these two spheres. So μ\mu is a fibration away from these spheres. For x¯∈𝐑3\underline{x}\in{\bf R}^{3}, write Fx¯F_{\underline{x}} for the preimage μ−1​(x¯)\mu^{-1}(\underline{x}). If |x¯|≠5,6|\underline{x}|\neq 5,6 the fibre Fx¯F_{\underline{x}} is a 33-manifold. If also |x¯|>0|\underline{x}|>0 then this 33-manifold has a natural circle action defined by the circle subgroup of S​O​(3)SO(3) fixing x¯\underline{x}. When x¯=0\underline{x}=0 the fibre has an S​O​(3)SO(3) action. As x¯\underline{x} varies in 𝐑3{\bf R}^{3} the fibre only “changes”—in the obvious sense—when |x¯||\underline{x}| crosses the special values 5,65,6. Thus we understand the full topological picture if we understand the changes in the fibre as x¯\underline{x} moves along the positive x1x_{1}-axis, say. Let V⊂X0V\subset X_{0} be the pre-image by μ\mu of the positive x1x_{1}-axis. This is a smooth 44-manifold, with a circle action, and the fibres Fx¯F_{\underline{x}}, for x¯\underline{x} on the axis, are the level sets of the Hamiltonian HH, restricted to VV. Then we have the usual Morse-theory description of these changes, from the Hessian of HH on VV, which is determined by the weights of the circle action. As x¯\underline{x} moves across the point (6,0,0)(6,0,0) the situation is modelled by the level sets

2​|z1|2+3​|z3|2=ϵ,2|z_{1}|^{2}+3|z_{3}|^{2}=\epsilon,

for (z1,z2)∈𝐂2(z_{1},z_{2})\in{\bf C}^{2}, with the circle action of weight (2,3)(2,3). Thus the fibre changes from the empty set to a 33-sphere with an action given by these weights. As x¯\underline{x} moves across the point (5,0,0)(5,0,0) the situation is modelled, locally, by the level sets

−|z1|2+5​|z2|2=ϵ,-|z_{1}|^{2}+5|z_{2}|^{2}=\epsilon,

with the circle action of weight (−1,5)(-1,5). The effect on the fibres is to perform a “Dehn surgery” on an S1S^{1}-orbit. Thus the fibres Fx¯F_{\underline{x}} for |x¯|<5|\underline{x}|<5 are obtained by performing this surgery on a knot Γ⊂S3\Gamma\subset S^{3}. Now Γ\Gamma is a free orbit of the (2,3)(2,3) action so it is the (2,3)(2,3) “torus knot” which is just a trefoil. To nail down the Dehn surgery completely we need to specify a framing of the knot but this is determined by the fact that the linking number of a nearby orbit with Γ\Gamma is the weight 55, from which one concludes that the framing is +1+1. This is a well-known description of the Poincaré homology sphere (the result of +1+1-surgery on a trefoil), and ties in with our previous discussion since the fibre F0F_{0} is the S​O​(3)SO(3)-orbit S​O​(3)/ΓSO(3)/\Gamma. (Another way of expressing this is that the fibres Fx¯F_{\underline{x}} are Seifert-fibred 33-manifolds: for 5<|x¯|<65<|\underline{x}|<6 we have two multiple fibres with multiplicity (2,3)(2,3) and the surgery across |x¯|=5|\underline{x}|=5 introduces another multiple fibre with multiplicity 55, so for |x¯|<5|\underline{x}|<5 we get the Seifert manifold with multiplicities (2,3,5)(2,3,5), which is another well-known description of the Poincaré manifold.)

It is interesting to match this picture up with the algebro-geometric description. This illustrates the general theory of Kirwan [19]. The 22-sphere Σ\Sigma at which |μ||\mu| attains its maximal value 66 is a holomorphic sphere in X0X_{0}: it is just the rational normal curve in our divisor D⊂𝐏⁡(s12)D\subset{\bf P}(s^{12}). The other sphere Σ′\Sigma^{\prime} is not holomorphic. It is a critical manifold for the function |μ|2|\mu|^{2} on X0X_{0} and the divisor DD appears as the associated “ascending set”: the closure of the set of points which flow to Σ′\Sigma^{\prime} under the decreasing gradient flow of |μ|2|\mu|^{2}. In our description of DD as S2×S2S^{2}\times S^{2} the holomorphic curve Σ\Sigma is the diagonal and Σ′\Sigma^{\prime} is the “anti-diagonal”consisting of pairs of antipodal points. One can also see the cusp singularity in DD, transverse to Σ\Sigma, from the weights (2,3)(2,3) of the circle action on the normal bundle.

Notice that if we write 𝐂𝐏3=𝐏⁡(s3){\bf C}{\bf P}^{3}={\bf P}(s^{3}), for the 44-dimensional representation s3s^{3} of S​U​(2)SU(2), the moment map μ:𝐂𝐏3→𝐑3\mu:{\bf C}{\bf P}^{3}\rightarrow{\bf R}^{3} for the action gives a description of 𝐂𝐏3{\bf C}{\bf P}^{3} very similar to that above. In this case μ−1​(0)\mu^{-1}(0) is S​O​(3)/HSO(3)/H where H⊂S​O​(3)H\subset SO(3) is the group of symmetries of an equilateral triangle, and we see this 33-manifold described as the Seifert fibration with multiple fibres (2,2,3)(2,2,3).

5.3 Deformations

Here we study the deformations of Mukai’s construction about the special solution X0X_{0}. Recall that a manifold in this family is specified by a 33-plane in Λ2​𝐂7\Lambda^{2}{\bf C}^{7}. We start with the 33-plane s2⊂Λ2​s6=s10⊕s6⊕s2s^{2}\subset\Lambda^{2}s^{6}=s^{10}\oplus s^{6}\oplus s^{2}. The tangent space of the Grassmannian at this point is given by the linear maps from s2s^{2} to the complementary subspace s10⊕s6s^{10}\oplus s^{6}, that is (using the fact that all these representations are isomorphic to their duals)

T​G​r3​(Λ2​𝐂7)=(s10⊕s6)⊗s2=s12⊕2​s8⊕s6⊕s4.TGr_{3}(\Lambda^{2}{\bf C}^{7})=(s^{10}\oplus s^{6})\otimes s^{2}=s^{12}\oplus 2s^{8}\oplus s^{6}\oplus s^{4}.

The action of the group S​L​(𝐂7)=S​L​(s6)SL({\bf C}^{7})=SL(s^{6}) gives a linear map

𝔰​𝔩​(7)→T​G​r3​(Λ2​𝐂7),\mathfrak{s}\mathfrak{l}(7)\rightarrow TGr_{3}(\Lambda^{2}{\bf C}^{7}),

which we know has kernel the Lie algebra 𝔰​𝔩​(2)\mathfrak{s}\mathfrak{l}(2) of the stabiliser. Now the Lie algebra of G​L​(𝐂7)=G​L​(s6)GL({\bf C}^{7})=GL(s^{6}) is

s6⊗s6=s12⊕s10⊕s8⊕s6⊕s4⊕s2⊕s0s^{6}\otimes s^{6}=s^{12}\oplus s^{10}\oplus s^{8}\oplus s^{6}\oplus s^{4}\oplus s^{2}\oplus s^{0}

so the Lie algebra of S​L​(s6)SL(s^{6}) is s12⊕…​s2s^{12}\oplus\dots s^{2}. It is clear then that the quotient of the tangent space by the tangent space to the orbit is just s8s^{8}, as a representation of P​S​L​(2,𝐂)PSL(2,{\bf C}). By general theory there is an equivariant slice: a P​S​L​(2,𝐂)PSL(2,{\bf C}) equivariant embedding jj from a neighbourhood of 00 in s8s^{8} into G​r3​(Λ2)Gr_{3}(\Lambda^{2}), mapping 00 to our fixed subspace s2s^{2}, such that two points j⁡(p),j⁡(q)j(p),j(q) in the same S​L​(7)SL(7) orbit if and only p,qp,q are in the same P​S​L​(2)PSL(2) orbit. In fact, although we do not really need this, what we are describing is the versal deformation of X0X_{0}, so H1​(T​X0)=s8H^{1}(TX_{0})=s^{8}, as a representation of P​S​L​(2,𝐂)PSL(2,{\bf C}).

One can gain a lot of insight from this simple calculation. The structure of the orbits of P​S​L​(2,𝐂)PSL(2,{\bf C}) on s8s^{8} (or any sps^{p}) is a standard example in Geometric Invariant Theory. There are five cases

  1. 1.

    The trivial orbit {0}\{0\}.

  2. 2.

    The orbits of polynomials having no zero of multiplicity ≥4\geq 4. These are closed in s8s^{8}.

  3. 3.

    The orbit of polynomials having two distinct zeros, each of multiplicity four. This orbit is closed and each point in it has stabiliser 𝐂∗⊂P​S​L​(2,𝐂){\bf C}^{*}\subset PSL(2,{\bf C}).

  4. 4.

    The orbits of polynomials having a zero of multiplicity four and other zeros each of multiplicity less than four. These orbits are not closed but there closure contains the orbit of type (3).

  5. 5.

    The orbits of polynomials having a zero of multiplicity ≥5\geq 5. these are not closed and contain 00 in their closure.

This is the source of the famous example of Tian of Fano manifolds without Kahler-Einstein (or Ricci soliton) metrics [31]. Tian shows that the manifolds corresponding to any P​S​L​(2,𝐂)PSL(2,{\bf C}) orbit of type (5) cannot have such metrics. Tian’s general results also show the same for the manifolds corresponding to orbits of type (4). Tian’s results are of course deep and difficult but we note now that a weaker statement is rather obviously true. For this we need to recall some background.

In general, the linearisation of the Kahler-Einstein equations on a complex manifold ZZ at a solution ω0\omega_{0} is given by the self-adjoint operator Δ+1\Delta+1 and, much as we have seen in Section 3, the kernel of this can be identified with the Lie algebra of the isometry group GG of ω0\omega_{0}. Suppose we have a GG-equivariant deformation of Z0Z_{0}: i.e. a complex manifold 𝒵{\cal Z} with a GG-action, an action of GG on a ball B⊂𝐂mB\subset{\bf C}^{m} and a GG-equivariant submersion π:𝒵→B\pi:{\cal Z}\rightarrow B. In this situation we automatically get “local actions” of the complexified group GcG^{c} on 𝒵{\cal Z} and BB, compatible with π\pi. The standard “Kuranishi method”, which depends only on the formal properties of the situation, yields the following structure (after possibly restricting to a smaller ball BB).

  • •

    A GG-invariant family of Kahler metrics ωt\omega_{t} on the fibres Zt=π−1​(t)Z_{t}=\pi^{-1}(t) such that ωt\omega_{t} is isometric to ωt′\omega_{t^{\prime}} if and only if tt and t′t^{\prime} are in the same GG-orbit.

  • •

    A smooth map ν:B→𝔤∗\nu:B\rightarrow\mathfrak{g}^{*}, equivariant for the action of GG on BB and the co-adjoint action on 𝔤∗\mathfrak{g}^{*}, such that ωt\omega_{t} is Kahler-Einstein if and only if ν⁡(t)=0\nu(t)=0.

Now in this general situation we can see that, if the GG-action on BB is non-trivial the map ν\nu cannot be identically zero. For if t,t′t,t^{\prime} are in the same orbit of the local GcG^{c} action on BB then ZtZ_{t} and Zt′Z_{t^{\prime}} are isomorphic complex manifolds. But if ν⁡(t)\nu(t) and ν⁡(t′)\nu(t^{\prime}) both vanish then ωt\omega_{t} and ωt′\omega_{t^{\prime}} are Kahler-Einstein and, by the uniqueness of the Kahler-Einstein solution, they must be isometric and this only happens if t,t′t,t^{\prime} are in the same GG-orbit. Thus what we see from this elementary argument is that as we deform Z0Z_{0} in the smooth family ZtZ_{t} we cannot deform the metric ω0\omega_{0} in a smooth family of Kahler-Einstein metrics, for all small tt. Tian’s much stronger result is that if the Futaki invariant of Z0Z_{0} vanishes (say), and if 00 lies in the closure of the the GcG^{c}-orbit of a point t∈Bt\in B then ZtZ_{t} does not admit any Kahler-Einstein metric at all. This is an example of the “jumping of structures” phenomenon discussed in Section 1: there are arbitrarily small deformations of Z0Z_{0} which are equivalent to a different structure ZtZ_{t}.

Returning to our special case of the Mukai-Umemura manifold, we can see conversely that there are some deformations of X0X_{0} which do admit Kahler-Einstein metrics. The general theory of these “obstruction maps” ν\nu is being developed by T. Brönnle, in his Ph.D thesis, but in this special case we can make some simple deductions from symmetry arguments. Let pp be a point in s8s^{8} which is fixed by a subgroup J⊂S​O​(3)J\subset SO(3). Then JJ acts on 𝐑3=𝔰​𝔲​(2){\bf R}^{3}=\mathfrak{s}\mathfrak{u}(2) and if ν\nu is any equivariant map from s8s^{8} to 𝐑3{\bf R}^{3} then JJ must fix ν⁡(p)\nu(p). So if the origin is the only point in 𝐑3{\bf R}^{3} fixed by JJ then we must have ν⁡(p)=0\nu(p)=0. Consider, for example,

p=C⁡(z4−α​w4)​(w4−α​z4),p=C(z^{4}-\alpha w^{4})(w^{4}-\alpha z^{4}),

with any α,C∈𝐂\alpha,C\in{\bf C}. This is fixed by a dihedral group JJ of order 88 which has the desired property, so we see that the deformations corresponding such elements of s8s^{8} admit Kahler-Einstein metrics, for small CC. For α,C≠0\alpha,C\neq 0 the element pp has a discrete stabiliser in S​O​(3)SO(3) and it follows that the corresponding metrics have discrete isometry groups. But then the deformation theory implies that all small deformations of these manifolds admit Kahler-Einstein metrics. So we conclude that there is a non-empty open set in 𝒰{\cal U} where the manifolds admit Kahler-Einstein metrics.

Taking α=0\alpha=0 above we get a special family of deformations, admitting Kahler-Einstein metrics, where we can take J=O⁡(2)⊂S​O​(3)J=O(2)\subset SO(3). It follows that the corresponding manifolds have a 𝐂∗{\bf C}^{*}-action. We can see this family of manifolds explicitly as follows. Fix the action on 𝐂7{\bf C}^{7} with weights λ3,…,λ−3\lambda^{3},\dots,\lambda^{-3} as usual. Then we want to look at 33-dimensional subspaces Π\Pi of Λ2​𝐂7\Lambda^{2}{\bf C}^{7} preserved by the action and we just consider those on which the action has weights 1,0−11,0-1. Now the weight 11-subspace of λ2\lambda^{2} has a basis e3∧e−2,e2∧e−1,e1∧e0e_{3}\wedge e_{-2},e_{2}\wedge e_{-1},e_{1}\wedge e_{0} and our space Π\Pi must contain a vector

u=u3,−2​e3∧e−2+u2,−1​e2∧e−1+u1,0​e1∧e0,u=u_{3,-2}e_{3}\wedge e_{-2}+u_{2,-1}e_{2}\wedge e_{-1}+u_{1,0}e_{1}\wedge e_{0},

for scalars u3,−2u_{3,-2} etc. Similarly Π\Pi must contain a vector

v=v1,−1​e1∧e−1+v2,−2​e2∧e−2+v3,−3​e3∧e−3v=v_{1,-1}e_{1}\wedge e_{-1}+v_{2,-2}e_{2}\wedge e_{-2}+v_{3,-3}e_{3}\wedge e_{-3}

and a vector

w=w−3,2​e−3∧e2+w−2,1​e−2∧e1+w−1,0​e−1∧e0.w=w_{-3,2}e_{-3}\wedge e_{2}+w_{-2,1}e_{-2}\wedge e_{1}+w_{-1,0}e_{-1}\wedge e_{0}.

The vector space Π\Pi is determined by these three vectors u,v,wu,v,w. The coefficients are not unique. We could change u,v,wu,v,w to μ1​u,μ2​v,μ3​w\mu_{1}u,\mu_{2}v,\mu_{3}w. Also we could change our basis vectors eie_{i} to λi​ei\lambda_{i}e_{i} to give an equivalent 33-plane. This would change the coefficients, for example u3,−2u_{3,-2} would change to λ3​λ−2​u3,−2\lambda_{3}\lambda_{-2}u_{3,-2}. However the expression

τ=u3,−2​w−3,2​v1,−1u2,−1​w−2,1​v3,−3\tau=\frac{u_{3,-2}w_{-3,2}v_{1,-1}}{u_{2,-1}w_{-2,1}v_{3,-3}}

is invariant under all these changes and gives a “modulus” for this family. The Mukai-Umemura manifold has τ=1\tau=1. When τ\tau is close to 11 we have seen that the corresponding manifold admits a Kahler-Einstein metric. It seems likely that this true for all τ\tau but, as far the author is aware, this is not known. It seems an interesting test case for future developments in the existence theory.

5.4 The α\alpha-invariant

In this subsection we establish the fact used above, that the Mukai-Umemura manifold has a Kahler-Einstein metric11 1 This material appeared in the preprint A note on the α\alpha-invariant of the Mukai-Umemura 3-fold arxiv DG 07114357., which is . For this we appeal to the theory of the α\alpha-invariant, developed by Tian [30]. We begin by recalling the definition. Let ZZ be a Fano manifold on which a compact group GG acts by holomorphic automorphisms and fix a GG-invariant Kahler metric ω0\omega_{0} in the cohomology class −c1​(KZ)-c_{1}(K_{Z}). Let 𝒫{\cal P} be the set of GG-invariant Kahler potentials ψ\psi on XX such that ωψ=ω0+i​∂∂¯​ψ>0\omega_{\psi}=\omega_{0}+i\partial\overline{\partial}\psi>0 and maxZ⁡ψ=0\max_{Z}\psi=0. Thus 𝒫{\cal P} can be identified with the set of all GG-invariant Kahler metrics in the given Kahler class. Let A⊂𝐑A\subset{\bf R} be the set defined by the condition that β∈A\beta\in A if there exists a Cβ∈𝐑C_{\beta}\in{\bf R} such that

∫Ze−β​ψ​d​μ0≤Cβ,\int_{Z}e^{-\beta\psi}d\mu_{0}\leq C_{\beta},

for all ψ∈𝒫\psi\in{\cal P}. Here d​μ0d\mu_{0} is the volume form defined by the fixed metric ω0\omega_{0}. Then Tian sets

αG​(Z)=sup{β:β∈A},\alpha_{G}(Z)=\sup\{\beta:\beta\in A\},

and shows that this does not depend on the choice of ω0\omega_{0}. He shows that αG​(Z)\alpha_{G}(Z) is always strictly positive and that if αG​(Z)>nn+1\alpha_{G}(Z)>\frac{n}{n+1} then ZZ has a Kahler-Einstein metric. What we really show in this subsection is that if we take the Mukai-Umemura manifold XX with the action of S​O​(3)SO(3) then,

Theorem 3

The α\alpha-invariant αS​O​(3)​(X0)\alpha_{SO(3)}(X_{0}) is 5/65/6.

So, since 5/6>3/45/6>3/4, Tian’s theory proves the existence of a Kahler-Einstein metric. We should say straightaway that this is not really a new result. Alessio Corti has explained to the author that, given the facts above, it can be obtained from the more general theories of [13]. But our argument is extremely simple and fits well into the general framework of this article.

We will only write down the proof that α≥5/6\alpha\geq 5/6, which is what is relevant to Corollary 1. The proof that α=5/6\alpha=5/6 is an easy extension of this.

Lemma 2

There is an M∈𝐑M\in{\bf R} such that

∫Zψ​d​μ0≥−M\int_{Z}\psi\ d\mu_{0}\geq-M

for all ψ∈𝒫\psi\in{\cal P}.

This is a step in Tian’s proof that α>0\alpha>0 and we repeat his argument. If ψ∈𝒫\psi\in{\cal P} we have

Δ0​ψ=2​Λ​(i​∂∂¯​ψ)≥−2​n.\Delta_{0}\psi=2\Lambda(i\partial\overline{\partial}\psi)\geq-2n.

Let KK be the Green’s function for Δ0\Delta_{0}, so that for all functions ff on ZZ

f(x)=−∫ZK(x,y)(Δ0f)(y)dμ0(y)+1V∫f(y)dμ0(y),f(x)=-\int_{Z}K(x,y)(\Delta_{0}f)(y)d\mu_{0}(y)+\frac{1}{V}\int f(y)d\mu_{0}(y),

where VV is the volume of the manifold. With our sign conventions, KK is bounded below and, since we can change KK by the addition of a constant without affecting the identity, we may suppose that K≥0K\geq 0. While KK is singular along the diagonal it is integrable in each variable. Let xx be the point where ψ\psi vanishes. Then applying the Green’s identity to ψ\psi we have

∫Zψ(y)dμ0(y)=V∫ZK(x,y)Δ0ψdμ0(y)≥−2nV∫ZK(x,y)dμ0(y).\int_{Z}\psi(y)d\mu_{0}(y)=V\int_{Z}K(x,y)\Delta_{0}\psi d\mu_{0}(y)\geq-2nV\int_{Z}K(x,y)d\mu_{0}(y).

So we can take

M=2​n​V​max⁡∫Zx⁡K⁡(x,y)​d​μ0​(y).M=2nV\max_{x}\int_{Z}K(x,y)d\mu_{0}(y).

For the rest of this section we work with the Mukai-Umemura manifold, which we denote by XX. Let σ\sigma be the S​O​(3)SO(3)-invariant section of the anticanonical bundle K−1K^{-1} cutting out the divisor DD. There is a Hermitian metric on this line bundle such that the curvature of the associated unitary connection is −i​ω0-i\omega_{0}. Set

f0=−log⁡(|σ|2).f_{0}=-\log\left(|\sigma|^{2}\right).

This is a smooth function on X∖DX\setminus D and i​∂∂¯​f0=ω0i\partial\overline{\partial}f_{0}=\omega_{0}.

Lemma 3

For any β<56\beta<\frac{5}{6} the function exp⁡(β​f0)\exp(\beta f_{0}) is integrable.

This is also standard. The integral in question is

∫Z|σ|−2​β​d​μ0.\int_{Z}|\sigma|^{-2\beta}d\mu_{0}.

By what we know about the singlarities of DD, we can reduce to considering the integrals

∫B|z2−w3|−2​β,\int_{B}|z^{2}-w^{3}|^{-2\beta},

where BB is the unit ball in 𝐂2{\bf C}^{2} and z,wz,w are complex co-ordinates. Let TT be the linear map T⁡(z,w)=(z/8,w/4)T(z,w)=(z/8,w/4) and for r≥1r\geq 1 set

Ωr=Tr​(B)∖Tr−1​(B).\Omega_{r}=T^{r}(B)\setminus T^{r-1}(B).

Set

Ir=∫Ωr|z2−w3|−2​β.I_{r}=\int_{\Omega_{r}}|z^{2}-w^{3}|^{-2\beta}.

The substitution (z′,w′)=T⁡(z,w)(z^{\prime},w^{\prime})=T(z,w) shows that

Ir+1=2(12​β−10)​Ir.I_{r+1}=2^{(12\beta-10)}I_{r}.

Thus ∑rIr\sum_{r}I_{r} is finite if β<5/6\beta<5/6 and the union of the Ωr\Omega_{r} cover B4∖{0}B^{4}\setminus\{0\}.

Now we give the main proof. Let x0∈Xx_{0}\in X be the point with stabiliser Γ\Gamma. We identify S​O​(3)SO(3)-invariant functions on X∖DX\setminus D with Γ\Gamma-invariant functions on M=P​S​L​(2,𝐂)/S​O​(3)M=PSL(2,{\bf C})/SO(3) as in (4.2). The function f0f_{0} on x∖Dx\setminus D corresponds to a convex function ϕ0\phi_{0} on M=P​S​L​(2,𝐂)/S​O​(3)M=PSL(2,{\bf C})/SO(3) which is an “admissible potential” in the language of (4.2). For any other admissible potential ϕ\phi the difference ϕ−ϕ0\phi-\phi_{0} corresponds to ψ\psi, restricted to X∖DX\setminus D. The normalisation that max⁡ψ=0\max\psi=0 becomes the condition that sup​ϕ−ϕ0=0{\rm sup}\ \phi-\phi_{0}=0, and in particular ϕ≤ϕ0\phi\leq\phi_{0}.

Let P0∈MP_{0}\in M be the identity coset. It is the unique point fixed by the action of Γ\Gamma. Any admissible potential function ϕ\phi on MM is proper and bounded below so achieves a minimum in MM. By the convexity and Γ\Gamma-invariance this minimum must occur at P0P_{0}. Set ϕ⁡(P0)=−b\phi(P_{0})=-b. Then the inequality ϕ0≥−b\phi_{0}\geq-b translates back into the statement that ψ≥f0−b\psi\geq f_{0}-b. So

∫Ze−β​ψ​d​μ0≤eb​β​∫Zf0−β​d​μ0.\int_{Z}e^{-\beta\psi}d\mu_{0}\leq e^{b\beta}\int_{Z}f_{0}^{-\beta}d\mu_{0}.

By Lemma 1, it suffices to obtain an upper bound on bb. Let BB be the geodesic ball in MM centred on P0P_{0}, of radius 11 say, and let a¯\overline{a} be the maximum value of ϕ0\phi_{0} on BB, so for any ϕ\phi we have ϕ≤a¯\phi\leq\overline{a} on BB. Convexity along geodesics emanating from P0P_{0} implies that

ϕ⁡(Q)≤−b+(a¯+b)​dist​(Q,P0),\phi(Q)\leq-b+(\overline{a}+b)\ {\rm dist}(Q,P_{0}),

for any point QQ in BB. In particular, on the ball 12​B\frac{1}{2}B of radius 1/21/2 about P0P_{0} we have ϕ≤(a¯−b)/2\phi\leq(\overline{a}-b)/2.

Take the inverse image in P​S​L​(2,𝐂)PSL(2,{\bf C}) of the ball 12​B\frac{1}{2}B and map this to XX by g→g⁡(x0)g\rightarrow g(x_{0}). The image obviously contains a neighbourhood NN of x0x_{0} and on NN we have ψ≤a¯−b2+f0\psi\leq\frac{\overline{a}-b}{2}+f_{0}. Then Lemma 1 implies that bb cannot be very large. In fact, if the minimum of f0f_{0} on NN is a¯\underline{a}, we have ψ≤(a¯2−a¯)−b2\psi\leq(\frac{\overline{a}}{2}-\underline{a})-\frac{b}{2} on NN, so

−M≤∫Nψ​d​μ0≤((a¯2−a¯)−b2)​Vol​(N),-M\leq\int_{N}\psi\ d\mu_{0}\leq((\frac{\overline{a}}{2}-\underline{a})-\frac{b}{2}){\rm Vol}(N),

hence

b≤(a¯−2​a¯)+2​MVol⁡(N)b\leq(\overline{a}-2\underline{a})+\frac{2M}{{\rm Vol}(N)}

where MM is as in Lemma 1. This completes the proof of Theorem 3.

Notice that the same argument can be applied in the toric case, when the polytope PP has a group Γ\Gamma of symmetries, as discussed in (4.2). We should suppose that Γ\Gamma has a unique fixed point in PP: then the proof proceeds exactly as before. The analogue of Lemma 1 holds with β<1\beta<1 since the local models for the zeros of ss are fp​(z1,…,zn)=0f_{p}(z_{1},\dots,z_{n})=0 where fp​(z1,…,zn)=z1​…​zpf_{p}(z_{1},\dots,z_{n})=z_{1}\dots z_{p} and |fp|−2​β|f_{p}|^{-2\beta} is locally integrable for β<1\beta<1. the conclusion is that the α\alpha-invariant in this case is 11. which is a theorem of Batyrev and Selinova [4]. Song gave another proof in [26], and showed conversely that for polytopes which do not have such a symmetry group the α\alpha-invariant never exceeds n/n+1n/n+1. The fact that such toric manifolds nevertheless have Kahler-Einstein metrics illustrates the point that Tian’s α\alpha-invariant criterion is sufficient but not necessary.

Original mathematics by the credited authors. Source-backed reader collection; mathematical self-containment is not assessed.