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4. Connections with algebraic geometry [02BN]

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4. Connections with algebraic geometry

The consequences of Theorem 1.1, for the relation between algebro-geometric and differential geometric limits, could be summarised by saying that things work out in the way that one might at first sight guess at. As we have mentioned before, the proofs of many of the statements, given Theorem 1.1, have been outlined by Tian in [23]. Thus we view this Section, broadly speaking, as an opportunity to attempt a careful exposition of the material.

4.1. Proof of Theorem 2

Lemma 4.1.

There are numbers NkN_{k}, depending only on n,c,V,kn,c,V,k, such that for any XX in 𝒦⁑(n,c,V){\mathcal{K}}(n,c,V) we have dim​H0​(X,Lk)≀Nk+1{\rm dim}H^{0}(X;L^{k})\leq N_{k}+1.

We work in the rescaled metric. Given Ο΅>0\epsilon>0 we can choose a maximal set of points xix_{i} in XX such that the distance between any two is at least Ο΅\epsilon. Then the 2​ϡ2\epsilon balls with these centres cover XX and the Ο΅/2\epsilon/2 balls are disjoint. Consider the evaluation map

ev:H0​(X,Lk)→⨁Lxik.{\rm ev}:H^{0}(X;L^{k})\rightarrow\bigoplus L^{k}_{x_{i}}.

We first show that if Ο΅\epsilon is sufficiently small then this map is injective. For if it is not injective there is a holomorphic section ss with L2,β™―L^{2,\sharp} norm 11 vanishing at all the xix_{i}. Since the 2​ϡ2\epsilon balls cover we get β€–sβ€–Lβˆžβ‰€2​K1​ϡ\|s\|_{L^{\infty}}\leq 2K_{1}\epsilon. This gives a contradiction to β€–sβ€–L2​♯=1\|s\|_{L^{2\sharp}}=1 if Ο΅\epsilon is small enough. On the other hand since the Ο΅/2\epsilon/2 balls are disjoint the non-collapsing condition gives an upper bound on the number of the points xix_{i} which completes the proof.

In fact the estimate one gets by this argument is

Nk+1=24​n​K12​n​Vn+1​n!c​πn​kn2,N_{k}+1=\frac{2^{4n}K_{1}^{2n}V^{n+1}n!}{c\pi^{n}}k^{n^{2}},

which is very poor compared with the asymptotics we know that dim​H0​(X,Lk)∼(2​π)βˆ’n​V​kn{\rm dim}H^{0}(X,L^{k})\sim(2\pi)^{-n}Vk^{n} for a fixed XX, as kβ†’βˆžk\rightarrow\infty.

For our purposes there is no loss of generality in supposing that the k0k_{0} of Theorem 1.1 is 11. Then the sections of LkL^{k} define a regular map of XX for all kk. Suppose we choose isometric embeddings

Ο•k:H0​(X,Lk)βˆ—β†’β„‚Nk+1,\phi_{k}:H^{0}(X;L^{k})^{*}\rightarrow\mbox{${\mathbb{C}}$}^{N_{k}+1},

using the L2L^{2} norm on the left hand side and the fixed standard Hermitian form on the right. Then we get projective varieties

V⁑(X,Ο•k)βŠ‚β„‚β„™Nk,V(X,\phi_{k})\subset\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N_{k}},

and holomorphic maps

Tk:Xβ†’V⁑(X,Ο•k).T_{k}:X\rightarrow V(X,\phi_{k}).

Of course TkT_{k} depend on the choice of Ο•k\phi_{k} which is arbitrary, but any two choices differ by the action of the unitary group U⁑(Nk+1)U(N_{k}+1). The fact that this group is compact will mean that in the end the choice of Ο•k\phi_{k} will not be important. Soon we will reduce to the case when TT is generically 1-1 but we do not need to assume that yet, so TkT_{k} could map to a variety of dimension less than nn or be a multiple cover of an nn-dimensional variety. In any case we get, by straightforward arguments, a fixed upper bound on the degree of V⁑(X,Ο•k)V(X,\phi_{k}) (depending on k,n,Vk,n,V).

By standard general principles there is a system of morphisms of projective varieties, for integer Ξ»\lambda,

fΞ»:V⁑(X,ϕλ​k)β†’V⁑(X,Ο•k),f_{\lambda}:V(X,\phi_{\lambda k})\rightarrow V(X,\phi_{k}),

with fλ​μ=fλ∘fΞΌf_{\lambda\mu}=f_{\lambda}\circ f_{\mu} and fλ​Tλ​k=Tk.f_{\lambda}T_{\lambda k}=T_{k}.

Now we bring in the crucial lower bound provided by Theorem 1.

Lemma 4.2.

Taking k0=1k_{0}=1, the map T1:Xβ†’V⁑(X,Ο•1)T_{1}:X\rightarrow V(X,\phi_{1}) has derivative bounded by K1​bβˆ’1K_{1}b^{-1} where bb is the lower bound in Theorem 1.1 and K1K_{1} is the constant in the first derivative estimate.

Here we are referring to the β€œoperator norm” of the derivative, regarded as a map from the tangent space of XX at a point, with the given metric gg, to the tangent space of β„‚β„™N1\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N_{1}} with the standard Fubini-Study metric.

The proof of the Lemma comes directly from the definitions. Given a point x∈Xx\in X we can choose an orthonormal basis of sections s0,s1,…,sNs_{0},s_{1},\dots,s_{N} with si​(x)=0s_{i}(x)=0 for i>0i>0 and |s0​(x)|=Bβ‰₯b|s_{0}(x)|=B\geq b. There is no loss of generality in supposing that Ο•1\phi_{1} maps the dual basis to the first N+1N+1 basis vectors in β„‚N1+1\mbox{${\mathbb{C}}$}^{N_{1}+1}. Fix a unitary isomorphism of the fibre LxL_{x} with β„‚{\mathbb{C}}. Then the derivative of each sis_{i}, for i>0i>0 can be regarded as an element of the cotangent space of XX at xx. Identifying the tangent space of β„‚β„™N1\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N_{1}} at (1,0,…,0)(1,0,\dots,0) with β„‚N1\mbox{${\mathbb{C}}$}^{N_{1}} in the standard way, the derivative of TT at xx is represented by

Bβˆ’1​(βˆ‚s1,…,βˆ‚sN,…,0),B^{-1}(\partial s_{1},\dots,\partial s_{N},\dots,0),

and the lemma follows.

Using Lemma 3.1 we get similar universal bounds on the derivatives of all maps TkT_{k}, for suitable constants which we do not need to keep track of.

Now suppose that XiX_{i} is a sequence in 𝒦⁑(n,c,v){\mathcal{K}}(n,c,v) with Gromov-Hausdorff limit a polarised limit space X∞X_{\infty}. For each fixed kk we choose Ο•k,i\phi_{k,i} so we have a sequence of projective varieties V⁑(Xi,Ο•k,i)V(X_{i},\phi_{k,i}) of bounded dimension and degree. By standard results we can, choosing a subsequence suppose that for each kk these converge in the algebro-geometric sense to a limit WkW_{k}. (More precisely, we can suppose that for each kk the V⁑(Xi,Ο•k,i)V(X_{i},\phi_{k,i}) have fixed degree and dimension and converge as points in the Chow variety parametrising algebraic cycles of that type. Then we take WkW_{k} to be the corresponding algebraic set.) It follows easily from the compactness of U⁑(Nk+1)U(N_{k}+1) that WkW_{k} is independent, up to projective unitary transformations, of the choice of maps Ο•k,i\phi_{k,i}.

Lemma 4.3.

After perhaps passing to a subsequence of the XiX_{i}, for each kk the maps Tk:Xiβ†’V⁑(Xi,Ο•k)T_{k}:X_{i}\rightarrow V(X_{i},\phi_{k}) extend by continuity to a continuous map Tk:Xβˆžβ†’WkT_{k}:X_{\infty}\rightarrow W_{k}, holomorphic on X∞regX^{{\rm reg}}_{\infty}.

More precisely what we mean is that we suppose we have fixed metrics on the XiβŠ”X∞X_{i}\sqcup X_{\infty} then for all Ο΅>0\epsilon>0 we can find Ξ΄>0\delta>0 so that the distance in the projective space between Tk​(y),Tk​(y)T_{k}(y),T_{k}(y) is less than Ο΅\epsilon if d⁑(x,y)<Ξ΄d(x,y)<\delta.

The proof of the Lemma is very easy using the equicontinuity of the maps TkT_{k} on the XiX_{i}. The limit map TkT_{k} on X∞X_{\infty} is unique up to unitary transformations preserving WkW_{k} and the possible existence of such maps is the only reason that we may need to pass to a subsequence.

In the next subsection we will collect some further analytical results which will give a much clearer view of the situation. Then we return to discuss the relation between X∞X_{\infty} and the WkW_{k} further in subsection 4.3.

4.2. More analysis

Recall that we have a uniform C0C^{0} estimate (Prop. 2.1) for holomorphic sections of Lkβ†’XL^{k}\rightarrow X, for any XX in 𝒦⁑(n,c,V){\mathcal{K}}(n,c,V). We will now extend this to a polarised limit space X∞X_{\infty}.

Lemma 4.4.

If ss is a bounded holomorphic section of LkL^{k} over X∞r​e​gX_{\infty}^{reg} then

β€–sβ€–Lβˆžβ‰€K0​‖sβ€–L2,β™―.\|s\|_{L^{\infty}}\leq K_{0}\|s\|_{L^{2,\sharp}}.

Here of course we are writing Lkβ†’X∞regL^{k}\rightarrow X^{{\rm reg}}_{\infty} for the limiting line bundle and we are defining the L2,β™―L^{2,\sharp} norm with the rescaled metric.

We prove the Lemma by contradiction. The argument is very similar to our main construction in Section 3. Suppose there is a holomorphic section ss with β€–sβ€–L2,β™―=1,β€–sβ€–L∞=B\|s\|_{L^{2,\sharp}}=1,\|s\|_{L^{\infty}}=B and there is a point p∈X∞regp\in X^{{\rm reg}}_{\infty} with |s⁑(p)|=K0+Ξ»|s(p)|=K_{0}+\lambda for some Ξ»>0\lambda>0. Choose a neighbourhood DD of pp which lies inside X∞X_{\infty}. There is some constant CC so that an estimate like that in (H3) of Property (H) holds. The singular set in X∞X_{\infty} has Hausdorff codimension strictly bigger than 22 so by the argument of Prop. 3.5 we can construct a cut-off function Ξ²\beta equal to 11 over DD and with β€–βˆ‡Ξ²β€–L2\|\nabla\beta\|_{L^{2}} as small as we like. In particular we can make this much smaller than λ​Bβˆ’1​Cβˆ’1\lambda B^{-1}C^{-1}. When ii is large we can choose maps Ο‡i\chi_{i} from a neighbourhood of the support of Ξ²\beta into XiX_{i} and lifts Ο‡^i\hat{\chi}_{i} so that the structures match up as closely as we please. Transport β​s\beta s by these maps to a section of Lkβ†’XiL^{k}\rightarrow X_{i} and adjust to get a holomorphic section sis_{i} just as in Section 3. Then when ii is large enough we see that sis_{i} contradicts Prop. 2.1, by arguments just like those in Section 3.

Now we define H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}) to be the space of bounded holomorphic sections over the regular part. Let SβŠ‚β„S\subset\mbox{${\mathbb{R}}$} be the set

S={0,1,1/2,1/3,1/4,…​1/i​…},S=\{0,1,1/2,1/3,1/4,\dots 1/i\dots\},

and for integers jj let SjβŠ‚SS_{j}\subset S be the subset {0,jβˆ’1,(j+1)βˆ’1​…}\{0,j^{-1},(j+1)^{-1}\dots\}. We are regarding SS as a topological space, so any sequence tending to zero would do equally well. Let

𝒳=⨆i=1,2,…,∞Xi.{\mathcal{X}}=\bigsqcup_{i=1,2,\dots,\infty}X_{i}.

Thus there is a map of sets Ο€:𝒳→S\pi:{\mathcal{X}}\rightarrow S which takes XiX_{i} to iβˆ’1i^{-1} for i=1,β€¦β€‹βˆži=1,\dots\infty. The distance functions on XiβŠ”X∞X_{i}\sqcup X_{\infty} define a natural topology on 𝒳{\mathcal{X}} such that Ο€\pi is continuous.

Now let

β„‹=⨆i=1,2,…,∞H0​(Xi,Lk),{\mathcal{H}}=\bigsqcup_{i=1,2,\dots,\infty}H^{0}(X_{i},L^{k}),

taking the above definition in the case i=∞i=\infty. There is an obvious map of sets Ο–:β„‹β†’S\varpi:{\mathcal{H}}\rightarrow S. We put a topology on β„‹{\mathcal{H}} by saying that sections are close if they are close when compared by maps Ο‡i,Ο‡^i\chi_{i},\hat{\chi}_{i}, as above.

Lemma 4.5.

For sufficiently large jj the restriction of Ο–:β„‹β†’S\varpi:{\mathcal{H}}\rightarrow S to SjβŠ‚SS_{j}\subset S is a vector bundle.

(Note that this is for fixed kk: for different values of kk one might a priori have to take different values of jj.)

The proof uses much the same construction as in Lemma 4.6. The content of the statement is that, for large enough ii, we can define linear isomorphisms

Qi:H0​(X∞,Lk)β†’H0​(Xi,Lk)Q_{i}:H^{0}(X_{\infty},L^{k})\rightarrow H^{0}(X_{i},L^{k})

such that Qi​(s)Q_{i}(s) tends to ss as iβ†’βˆži\rightarrow\infty, in the sense above. We choose a family of compactly supported cut-off functions Ξ²i\beta_{i} on X∞regX^{{\rm reg}}_{\infty} with the following properties.

  • β€’

    The compact sets Ξ²iβˆ’1​(1)\beta_{i}^{-1}(1) give an exhaustion of X∞regX_{\infty}^{{\rm reg}};

  • β€’

    The support of Ξ²i\beta_{i} is contained in the domain of a map Ο‡i\chi_{i} under which the structures compare with a small error Ξ·i\eta_{i} with Ξ·iβ†’0\eta_{i}\rightarrow 0 as iβ†’βˆži\rightarrow\infty;

  • β€’

    β€–βˆ‡Ξ²iβ€–L2,β™―β†’0\|\nabla\beta_{i}\|_{L^{2,\sharp}}\rightarrow 0 as iβ†’βˆži\rightarrow\infty. In particular β€–βˆ‡Ξ²iβ€–L2,β™―\|\nabla\beta_{i}\|_{L^{2,\sharp}} can be taken very small compared with K0βˆ’1K_{0}^{-1}.

Then for any holomorphic section s∈H0​(X∞,Lk)s\in H^{0}(X_{\infty},L^{k}) we transport Ξ²i​s\beta_{i}s to XiX_{i} using Ο‡i\chi_{i} and project to get an element Qi​(s)∈H0​(Xi,Lk)Q_{i}(s)\in H^{0}(X_{i},L^{k}) in the familiar way. Our standard argument shows that Qi​(s)Q_{i}(s) can be made as close as we please to ss by taking ii large. In particular this shows that QiQ_{i} is injective, for large ii. (Note that the point of establishing Lemma 4.4 first is that the bounds we require on β€–βˆ‡Ξ²iβ€–\|\nabla\beta_{i}\| do not depend on ss, but only on K0K_{0}.) To prove surjectivity we argue by contradiction. If QiQ_{i} is not surjective we can find si∈H0​(Xi,Lk)s_{i}\in H^{0}(X_{i},L^{k}) of L2,β™―L^{2,\sharp} norm 11 and L2,β™―L^{2,\sharp}-orthogonal to the image of QiQ_{i}. Passing to a subsequence and taking a limit as iβ†’βˆži\rightarrow\infty we get a section s∞∈H0​(X∞,Lk)s_{\infty}\in H^{0}(X_{\infty},L^{k}). The C0C^{0} estimate shows that s∞s_{\infty} has L2,β™―L^{2,\sharp} norm 11 and we easily get a contradiction to the fact that sis_{i} is orthogonal to Qi​(s∞)Q_{i}(s_{\infty}) for all ii.

Our reason for formulating things in this way is that it is natural to consider families Ο€:𝒳→B\pi:{\mathcal{X}}\rightarrow B over a general base. Here we want the fibres of Ο€\pi to be either smooth manifolds in 𝒦⁑(n,c,V){\mathcal{K}}(n,c,V) or polarised Gromov-Hausdorff limits of such, and we want the topology on 𝒳{\mathcal{X}} to be compatible with the Gromov-Hausdorff distance in an obvious way. It is not hard to set up the definitions and the proof of Lemma 4.5 shows that, if BB is connected, there is a β€œdirect image” which is a vector bundle over BB. However there does not seem much point in developing the theory in detail since in the end, after we have proved Theorem 1.2, this construction can be obtained from the standard algebraic geometry direct image.

We now turn to the problem of separating points.

Proposition 4.6.

Suppose X∞X_{\infty} is a polarised limit space and ρ>0\rho>0. We can find a kk such that if p1,p2∈X∞p_{1},p_{2}\in X_{\infty} are points with d⁑(p1,p2)>ρd(p_{1},p_{2})>\rho then the map Tk:Xβˆžβ†’β„‚β„™NkT_{k}:X_{\infty}\rightarrow\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N_{k}} takes p1,p2p_{1},p_{2} to distinct points in β„‚β„™Nk\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N_{k}}.

The proof is a small extension of our main argument in Section 3. By a compactness argument, it suffices to find a kk which works for a fixed pair of distinct points p1,p2p_{1},p_{2}. We choose a sequence XiX_{i} from 𝒦⁑(n,c,V){\mathcal{K}}(n,c,V) converging to X∞X_{\infty}. We can find a sequence kΞ½β†’βˆžk_{\nu}\rightarrow\infty such that rescaling X∞X_{\infty} by kΞ½\sqrt{k_{\nu}} at each of the points we get convergence to tangent cones C⁑(Y1),C⁑(Y2)C(Y_{1}),C(Y_{2}) and we construct U1,U2U_{1},U_{2} etc. in each case. We then choose kk so that we get maps Ο‡s:Usβ†’Xi\chi_{s}:U_{s}\rightarrow X_{i} as in Section 3. Clearly we can also suppose that Ο‡1​(U1),Ο‡2​(U2)\chi_{1}(U_{1}),\chi_{2}(U_{2}) are disjoint. (For this we will need to take k\sqrt{k} large compared with Οβˆ’1\rho^{-1}.) Then we get holomorphic sections s1,s2s_{1},s_{2} of Lkβ†’XiL^{k}\rightarrow X_{i} with fixed L2,β™―L^{2,\sharp} norm and such that |si|β‰₯1/2|s_{i}|\geq 1/2 say at points close to pip_{i}. Consider the section s1s_{1} at points in XiX_{i} close to the image of Ο‡2\chi_{2}. Recall that s1=Οƒ1βˆ’Ο„1s_{1}=\sigma_{1}-\tau_{1} where Οƒ1\sigma_{1} vanishes on the image of Ο‡2\chi_{2} and the L2,β™―L^{2,\sharp} norm of Ο„1\tau_{1} can be made as we please by our original choice of parameters. Let uβˆ—βˆˆDβŠ‚U2u_{*}\in D\subset U_{2} be the base point. Since Ο„1\tau_{1} is holomorphic over Ο‡2​(D)\chi_{2}(D) the size of Ο„1​(Ο‡2​(uβˆ—))\tau_{1}(\chi_{2}(u_{*})) can be controlled by the L2L^{2} norm of Ο„1\tau_{1} over Ο‡2​(D)\chi_{2}(D). Thus by a suitable choice of original parameters (depending only on knowledge of Y1,Y2Y_{1},Y_{2}) we can arrange that |s1​(x)|=|Ο„1​(x)|≀1/100|s_{1}(x)|=|\tau_{1}(x)|\leq 1/100, say, for points xx close to Ο‡2​(uβˆ—)\chi_{2}(u_{*}). Taking the limit as iβ†’βˆži\rightarrow\infty we get sections s1,s2∈H0​(X∞,Lk)s_{1},s_{2}\in H^{0}(X_{\infty},L^{k}) with |si​(pi)|β‰₯1/2|s_{i}(p_{i})|\geq 1/2 and |si​(pj)|≀1/100|s_{i}(p_{j})|\leq 1/100 for iβ‰ ji\neq j.

Proposition 4.7.

Given a compact set KβŠ‚X∞regK\subset X_{\infty}^{{\rm reg}} we can find an integer m⁑(K)m(K) such that for kβ‰₯m⁑(K)k\geq m(K), any point x∈Kx\in K and any tangent vector vv at xx there is a holomorphic section s∈H0​(X∞,Lk)s\in H^{0}(X_{\infty},L^{k}) with s⁑(x)=0s(x)=0 and the derivative of ss along vv not zero.

This is another straightforward application of the HΓΆrmander technique.

4.3. Recap

We can go back to the discussion of (4.1) and state things in a much clearer way. For a given kk we can suppose that all the spaces H0​(Xi,Lk)H^{0}(X_{i},L^{k}) have the same dimension and identify them with H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}) as in Lemma 4.5. In the usual way, the sections in H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}) define a holomorphic map from X∞regX^{{\rm reg}}_{\infty} to ℙ⁑(H0​(X∞,Lk)βˆ—)\mbox{${\mathbb{P}}$}(H^{0}(X_{\infty},L^{k})^{*}). We fix a basis in H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}) so that we can say that we map to β„‚β„™N\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N}. The same argument as in lemma 4.2 gives a bound on the derivative of this map so it has a unique continuous extension to X∞X_{\infty}. Pulling back the hyperplane bundle by this map (in the case k=1k=1) defines an extension of the line bundle LL to X∞X_{\infty} (at this stage, as a topological bundle). Theorem (1.1) implies that the original metric on LL is uniformly equivalent to the metric pulled back from the hyperplane bundle. The convergence of the maps Tk:Xiβ†’β„‚β„™NT_{k}:X_{i}\rightarrow\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N} to Tk:Xβˆžβ†’β„‚β„™NT_{k}:X_{\infty}\rightarrow\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N} over the regular part is completely clear because of the way we chose our identifications of H0​(Xi,Lk),H0​(X∞,Lk)H^{0}(X_{i},L^{k}),H^{0}(X_{\infty},L^{k}). The algebraic set WkW_{k} is the image Tk​(X∞)T_{k}(X_{\infty}). It is also clear that we have a system of morphisms fΞ»:Wk​λ→Wkf_{\lambda}:W_{k\lambda}\rightarrow W_{k} such that fλ​μ=fλ∘fΞΌf_{\lambda\mu}=f_{\lambda}\circ f_{\mu} and

Tk=fλ∘Tk​λ:Xβˆžβ†’Wk.T_{k}=f_{\lambda}\circ T_{k\lambda}:X_{\infty}\rightarrow W_{k}.

(The morphism fΞ»f_{\lambda} can be viewed as induced by the linear map which is the transpose of sλ​(H0​(X∞,Lk))β†’H0​(X∞,Lλ​k)s^{\lambda}(H^{0}(X_{\infty},L^{k}))\rightarrow H^{0}(X_{\infty},L^{\lambda k}) composed with the inverse of the Veronese map.)

Suppose we have any collection of sets WkW_{k}, for integers kβ‰₯1k\geq 1, and maps fΞ»:Wk​λ→Wkf_{\lambda}:W_{k\lambda}\rightarrow W_{k} with fλ​μ=fλ∘fΞΌf_{\lambda\mu}=f_{\lambda}\circ f_{\mu}. Then we can form the limit set Wβ†βŠ‚Ξ k​WkW_{\leftarrow}\subset\Pi_{k}W_{k} given by sequences (w1,w2,…)(w_{1},w_{2},\dots) such that fλ​(wk​λ)=wkf_{\lambda}(w_{k\lambda})=w_{k} for all k,Ξ»k,\lambda. If we have another set X∞X_{\infty} and maps Tk:Xβˆžβ†’WkT_{k}:X_{\infty}\rightarrow W_{k} compatible with the fΞ»f_{\lambda} then we get an induced map from X∞X_{\infty} to W←W_{\leftarrow}. In our situation, Proposition 4.6 implies that this map is a bijection so what we know at this stage is that we can recover the Gromov-Haussdorf limit algebro-geometrically (at least as a set) in this way.

It is interesting to compare this with [10], [11] where the first-named author made a different attack on the same kind of problem. This attack was made in the absence of Theorem 1.1, and the cost of that absence was that one got a system like the fΞ»f_{\lambda} but only of rational maps (or β€œweb of descendants” in the language of [10]). The core of the problem was that, without something like Theorem 1.1, one does not know that the WkW_{k} are irreducible. This difficulty is also explained by Tian in [23]. The construction of [10] should probably best be thought of as an attempt to define the Gromov-Hausdorff limit as a β€œlimit” of algebraic sets or schemes (in the sense of lim←{\rm lim}\leftarrow) in this fashion. (From a more algebraic point of view the limiting process we conceive of here is related to considering rings that are not finitely generated.) But, having now Theorem 1.1, we can take a simpler and more direct path (in the context of manifolds satisfying the hypotheses (1.1),(1.2)). However it seem likely that related ideas on the algebraic side may play a role in the future in the study of constant scalar curvature KΓ€hler metrics (lacking (1.1), (1.2)). In this direction, see the recent work of Szekelyhidi [20].

4.3.1. Completion of proof of Theorem 1.2

Lemma 4.8.

For each kk, the algebraic set WkW_{k} is irreducible.

This is crucial, as we indicated above, but the proof is easy. The set X∞regX^{{\rm reg}}_{\infty} is dense in X∞X_{\infty} so its image is dense in WkW_{k}. Thus we can choose a point x0∈X∞regx_{0}\in X^{{\rm reg}}_{\infty} so that Tk​(x0)T_{k}(x_{0}) lies in a unique component UU of WkW_{k}. Suppose there is a point ww in WkW_{k} which is not in UU. Then we can find a polynomial PP of degree Ξ»\lambda say so that PP vanishes on UU but not at ww. Regarding PP as a section of a line bundle we can suppose |P⁑(w)|=1|P(w)|=1. Now PP also defines holomorphic sections Οƒi\sigma_{i} of Lλ​kL^{\lambda k} over XiX_{i} for each ii (including i=∞i=\infty) which satisfy a fixed L∞L^{\infty} bound (because of the equivalence of the metrics on the line bundle). By construction the section Οƒβˆž\sigma_{\infty} vanishes in a neighbourhood of x0x_{0} and so by analytic continuation and the fact that the regular set is dense and connected it vanishes identically. It follows from the L∞L^{\infty} bound on Οƒi\sigma_{i}, the general estimate of (2.1) and convergence on compact subsets of the regular set that β€–Οƒiβ€–L∞\|\sigma_{i}\|_{L^{\infty}} tends to 00 as iβ†’βˆži\rightarrow\infty. But this contradicts the fact that |P⁑(w)|=1|P(w)|=1 (again using the equivalence of the two metrics on LkL^{k}).

(Notice that in this proof we do use the fact that X∞regX_{\infty}^{{\rm reg}} has an analytic, not just C2,αC^{2,\alpha}, structure.)

Recall that we have compatible maps Tk:Xβˆžβ†’WkT_{k}:X_{\infty}\rightarrow W_{k} and fΞ»:Wλ​kβ†’Wkf_{\lambda}:W_{\lambda k}\rightarrow W_{k}. Proposition (4.8) implies that the TkT_{k} asymptotically separate points, in the sense that the induced map from X∞X_{\infty} to lim←Wk\lim_{\leftarrow}W_{k} is injective. What we want to show now is that in fact there is some fixed kk for which this is true.

Lemma 4.9.

We can find a kk so that all fibres of Tk→WkT_{k}\rightarrow W_{k} are finite.

First we can plainly use Proposition 4.6 to arrange that TkT_{k} is generically 1-1, i.e. so that the fibre Tkβˆ’1​(w)T_{k}^{-1}(w) is a single point for a generic w∈Wkw\in W_{k}. As usual we may as well suppose that this happens for k=1k=1 and hence for all kk. Thus all maps fΞ»:Wλ​kβ†’Wkf_{\lambda}:W_{\lambda k}\rightarrow W_{k} are also generically 1βˆ’11-1. Our main theorem 1.1 and the first derivative estimate imply that there is a number r>0r>0 so that for any Xβˆˆπ’¦β‘(n,c,V)X\in{\mathcal{K}}(n,c,V) and any point x∈Xx\in X there is a holomorphic section of LL which does not vanish on the ball of radius rr about xx. The argument extends easily to the limit space X∞X_{\infty} and H0​(X∞,L)H^{0}(X_{\infty},L). Choose kk in accordance with Proposition 4.6 taking ρ=r/2\rho=r/2 say. Thus if p1,p2p_{1},p_{2} are two points in the same fibre F=Tkβˆ’1​(w)F=T_{k}^{-1}(w) of Tk:Xβˆžβ†’WkT_{k}:X_{\infty}\rightarrow W_{k} the distance between them is less r/2r/2. In other words the fibre FF is contained in the r/2r/2 ball about p1p_{1}, so there is a section s∈H0​(X∞,L)s\in H^{0}(X_{\infty},L) of LL which does not vanish on FF. By construction, FF maps by Tk​λT_{k\lambda} onto FΞ»=fΞ»βˆ’1​(w)F_{\lambda}=f_{\lambda}^{-1}(w) for any fΞ»:Wλ​kβ†’Wkf_{\lambda}:W_{\lambda k}\rightarrow W_{k}. The section sλ​k∈H0​(X∞,Lλ​k)s^{\lambda k}\in H^{0}(X_{\infty},L^{\lambda k}) defines one component of Tk​λT_{k\lambda} so the fact that ss does not vanish on FF implies that FΞ»F_{\lambda} lies in the corresponding affine subspace. Since FΞ»F_{\lambda} is a compact algebraic set it must be finite. Thus all maps fΞ»:Wk​λ→Wkf_{\lambda}:W_{k\lambda}\rightarrow W_{k} have finite fibres. Let N⁑(w)N(w) be the number of local irreducible components of WkW_{k} at ww. Since fΞ»f_{\lambda} is generically 1-1 the number of points in fΞ»βˆ’1​(w)f_{\lambda}^{-1}(w) is at most N⁑(w)N(w). It follows then the number of points in Tkβˆ’1​(w)T_{k}^{-1}(w) is also finite, and in fact bounded by N⁑(w)N(w).

Proposition 4.10.

We can find a kk so that TkT_{k} is injective.

As usual we may as well suppose that the value of kk in the previous Lemma is 11. Thus T1:Xβˆžβ†’W1βŠ‚β„‚β„™N1T_{1}:X_{\infty}\rightarrow W_{1}\subset\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N_{1}} has finite fibres. For any given point w1∈W1w_{1}\in W_{1} we can find a kk such that T1βˆ’1​(w1)T_{1}^{-1}(w_{1}) is mapped injectively to WkW_{k} by TkT_{k}. It is clear then there is a decomposition of W1W_{1} into a finite number of quasi-projective subvarieties ZΞ±Z_{\alpha} such that T1βˆ’1​(ZΞ±)T_{1}^{-1}(Z_{\alpha}) is a disjoint union of a number nΞ±n_{\alpha} of copies of ZΞ±Z_{\alpha}. Pick points zα∈ZΞ±z_{\alpha}\in Z_{\alpha}. If for some Ξ±\alpha some TkT_{k} separates the points T1βˆ’1​(zΞ±)T_{1}^{-1}(z_{\alpha}) then it is clear that TkT_{k} separates points in T1βˆ’1​(z)T_{1}^{-1}(z) for generic z∈ZΞ±z\in Z_{\alpha}. Now the Proposition follows from a simple induction argument, using induction on the maximal dimension of a ZΞ±Z_{\alpha} with nΞ±>1n_{\alpha}>1 and the number of components ZΞ±Z_{\alpha} with this maximal dimension.

We have now achieved our main goalβ€”the central statement in Theorem 1.2. We have a continuous bijection Tk:Xβˆžβ†’WkT_{k}:X_{\infty}\rightarrow W_{k} which is a homeomorphism, since the spaces are compact. As usual we may as well suppose that this kk is 11, so all TkT_{k} are homeomorphisms.

Recall that we denote the differential geometric singular set, the complement of X∞regX_{\infty}^{{\rm reg}} by Ξ£\Sigma. Let SkβŠ‚WkS_{k}\subset W_{k} denote the algebro-geometric singular set.

Lemma 4.11.

We can choose kk so that Tkβˆ’1T_{k}^{-1} maps SkS_{k} to Ξ£\Sigma.

Of course it is equivalent to say that TkT_{k} maps X∞regX_{\infty}^{{\rm reg}} to smooth points of WkW_{k}. The proof is similar to that of the previous Lemma. It follows from Proposition 4.7 that for any given compact subset KβŠ‚X∞regK\subset X_{\infty}^{{\rm reg}} we can choose kk so that TkT_{k} maps KK into the smooth points of WkW_{k}. On the other hand the singular set S1S_{1} has a finite number of irreducible components. If there is a component which meets T1​(X∞reg)T_{1}(X_{\infty}^{{\rm reg}}) we choose one of maximal dimension, say VV. Thus there is a point x∈X∞regx\in X_{\infty}^{{\rm reg}} with T1​(x)∈VT_{1}(x)\in V. We apply Proposition 4.7 with K={x}K=\{x\} to find a kk such that Tk​(x)T_{k}(x) lies in the smooth set of WkW_{k}. Then it is clear that the number of irreducible components of SkS_{k} is strictly less than for S1S_{1}, and the proof is completed by induction.

As usual we can suppose that the kk in Lemma 4.11 is 1. In the next subsection we will show that, at least for KΓ€hler-Einstein limits, the singular sets match up but we do not need to use this fact.

Lemma 4.12.

We can choose a kk such that WkW_{k} is a normal variety.

Suppose W1W_{1} is not normal. Let Ξ½:W^1β†’W1\nu:\hat{W}_{1}\rightarrow W_{1} be the normalisation. Thus Ξ½\nu is a bijection outside the singular set S1S_{1} of W1W_{1}. It is a general fact that the pull back β„’=Ξ½βˆ—β€‹(π’ͺ​(1)){\mathcal{L}}=\nu^{*}({\mathcal{O}}(1)) is an ample line bundle on W^1\hat{W}_{1}, so we can choose kk such that sections of β„’k{\mathcal{L}}^{k} define a projective embedding of W^1\hat{W}_{1} in β„™{\mathbb{P}} say. The map T1:X∞regβ†’W1T_{1}:X_{\infty}^{{\rm reg}}\rightarrow W_{1} maps into the smooth part and so lifts to T^1:X∞regβ†’W^1\hat{T}_{1}:X_{\infty}^{{\rm reg}}\rightarrow\hat{W}_{1}. Clearly the pull back of β„’{\mathcal{L}} to X∞r​e​gX_{\infty}^{reg} by this map is identified with our polarising bundle LL. Moreover, Theorem 1 implies that the metrics on the bundle agree up to a bounded factor. So the sections of β„’k{\mathcal{L}}^{k} over W^1\hat{W}_{1} define bounded sections of LkL^{k} over X∞r​e​gX_{\infty}^{reg} that is, elements of H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}). Write UβŠ‚H0​(X∞,Lk)U\subset H^{0}(X_{\infty},L^{k}) for the image of this map from H0​(W^1,β„’k)H^{0}(\hat{W}_{1},{\mathcal{L}}^{k}). These sections define a map Ξ±\alpha from X∞regX_{\infty}^{{\rm reg}} to β„™{\mathbb{P}} and the definitions mean that this is just the composite of T^\hat{T} with the above projective embedding of W^1\hat{W}_{1}. The subspace UU contains the kth. powers of sections in H0​(X∞,L)H^{0}(X_{\infty},L) which uniformly generate the fibres, so we have a first derivative estimate on the map Ξ±\alpha. Hence Ξ±\alpha extends to a Lipschitz map, which we also call Ξ±\alpha, from X∞X_{\infty} to β„™{\mathbb{P}} with image W^1\hat{W}_{1}. Let ZZ be the intersection of smooth part of W^1\hat{W}_{1} with α⁑(Ξ£)\alpha(\Sigma). The Lipschitz bound implies that the Hausdorff dimension of ZZ is at most 2​nβˆ’42n-4 and it follows that any local holomorphic function defined on the complement of ZZ extends holomorphically over ZZ [18]. This means that H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}) can be identified with bounded holomorphic sections of the hyperplane bundle over the smooth part of W^1\hat{W}_{1}. But it is a basic general fact about a normal variety that its structure sheaf can be defined by bounded holomorphic functions on the smooth part. So the subspace UU is in fact the whole of H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}). Thus Ξ±\alpha is exactly TkT_{k} and WkW_{k} is W^1\hat{W}_{1}, and hence normal.

To complete the story we have

Lemma 4.13.

If W1W_{1} is normal then WkW_{k} is the embedding of W1W_{1} defined by sections of π’ͺ⁑(k){\mathcal{O}}(k).

This follows from the same argument as above.

We have now almost completed the proof of Theorem 1.2. For any given polarised limit space X∞X_{\infty} we can choose a kk so that H0​(X∞,Lk)H^{0}(X_{\infty},L^{k}) represents X∞X_{\infty} as a normal variety and if XiX_{i} is a sequence converging to XiX_{i} in the Gromov-Hausdorff sense we can choose a convergent sequence of embeddings. (Notice that the only reason for passing to a subsequence in the statement of Theorem 1.2 is that we can have different polarisations on the same Riemannian limit space.) The last point is to show that there is a single k1k_{1} which works for all X∞X_{\infty}. But this follows from Gromov compactness and the easy fact that if kk has the desired property for X∞X_{\infty} it does also for all limit spaces sufficiently close to X∞X_{\infty}, in the Gromov-Hausdorff sense.

To spell out a little more the consequences of Theorem 1.2, observe that now that we are considering embeddings the degree of WW is determined by k1k_{1} and VV. So (for theoretical purposes) we can operate in a fixed quasi projective Chow variety 𝒯{\mathcal{T}} parameterising normal nn-dimensional subvarieties of the given degree in a suitable large projective space β„‚β„™N\mbox{${\mathbb{C}}$}\mbox{${\mathbb{P}}$}^{N}. β€œAlgebro-geometric convergence” of XiX_{i} to X∞X_{\infty} means convergence in 𝒯{\mathcal{T}}. There is a universal variety 𝒰→𝒯{\mathcal{U}}\rightarrow{\mathcal{T}} and by general facts ([14], Theorem 9.11) this is a flat family. So we see that if XiX_{i} converge to X∞X_{\infty} in the Gromov-Hausdorff sense then XiX_{i} and W=X∞W=X_{\infty} can be realised as fibres in a flat family. So, for example, the Hilbert polynomials of XiX_{i} and W=X∞W=X_{\infty} are the same.

There are different ways of going about the proofs of Theorem 1.2. We mention one elegant alternative, based on a result from the thesis of Chi Li [15], Prop. 7. This in turn depends upon results of Siu and Skoda. For XX in 𝒦⁑(n,c,V){\mathcal{K}}(n,c,V) let RXR_{X} be the graded ring

RX=⨁kH0​(X,Lk).R_{X}=\bigoplus_{k}H^{0}(X;L^{k}).

Then from standard theory we know that RXR_{X} is finitely generated and X=Proj⁑(RX)X={\rm Proj}(R_{X}). Assuming the lower bound in Theorem 1.1, Li proves an effective form of finite generation in the sense that if Οƒi\sigma_{i} is an orthonormal basis in the finite dimensional space ⨁j=0(n+2)​k0H0​(X,Lj)\bigoplus_{j=0}^{(n+2)k_{0}}H^{0}(X,L^{j}) then the Οƒi\sigma_{i} generate RXR_{X} and for each kk there is a number BkB_{k} such that any element of L2L^{2} norm 11 in H0​(X,Lk)H^{0}(X,L^{k}) can be expressed as a polynomial in the Οƒi\sigma_{i} with co-efficients bounded by BkB_{k}. It follows easily that for a polarised limit space X∞X_{\infty} the graded ring

RX∞=⨁kH0​(X∞,Lk)R_{X_{\infty}}=\bigoplus_{k}H^{0}(X_{\infty};L^{k})

is finitely generated. Then we can immediately define the algebraic variety WW as Proj⁑(RX∞){\rm Proj}(R_{X_{\infty}}). Of course there is still some work to do in checking the properties of WW.

4.4. Further results

We will now restrict attention to the case when X∞X_{\infty} is the limit of KΓ€hler-Einstein manifolds Xiβˆˆπ’¦β‘(n,c,V)X_{i}\in{\mathcal{K}}(n,c,V) with Ricci curvature +1, -1/2 or 0. We suppose that L=KXβˆ’1L=K_{X}^{-1} or KX2K_{X}^{2} in the first and second situations and in the third situation we suppose that the manifolds are Calabi-Yau, so we have fixed holomorphic nn forms Θi\Theta_{i} over XiX_{i} with Θi∧Θ¯i\Theta_{i}\wedge\overline{\Theta}_{i} the volume form. For brevity we just call this β€œthe KΓ€hler-Einstein case”.

Proposition 4.14.

In the KΓ€hler-Einstein case the map T:Xβˆžβ†’WT:X_{\infty}\rightarrow W takes the differential geometric limit singular set to the algebro-geometric singular set.

Proof.

The argument in the previous subsection implies that TT maps the smooth set in X∞X_{\infty} to the regular set in WW. So we need to show that if T⁑(p)T(p) is a smooth point of WW, then the limit metric on X∞X_{\infty} is also smooth at pp. Denote by Ο‰i\omega_{i} the KΓ€hler-Einstein metric on XiX_{i}, and Ο‰iβ€²\omega_{i}^{\prime} the induced Fubini-Study metric. Then we have Ο‰iβ€²=Ο‰i+βˆ’1β€‹βˆ‚βˆ‚Β―β€‹Ο•i\omega_{i}^{\prime}=\omega_{i}+\sqrt{-1}\partial\bar{\partial}\phi_{i} with Ο•i=kβˆ’1​log⁑ρk​(Ο‰i)\phi_{i}=k^{-1}\log\rho_{k}(\omega_{i}). By our main Theorem 1.1 and Proposition 2.1 there is a constant C1>0C_{1}>0 such that |Ο•i|Lβˆžβ‰€C1|\phi_{i}|_{L^{\infty}}\leq C_{1} for all ii. Also by arguments similar to the proof of Lemma 4.3 we see that there is a constant C2>0C_{2}>0 such that for all ii we have |βˆ‡Ο‰iΟ•i|Lβˆžβ‰€C2|\nabla_{\omega_{i}}\phi_{i}|_{L^{\infty}}\leq C_{2}, and Ο‰i′≀C2​ωi\omega_{i}^{\prime}\leq C_{2}\omega_{i}. Now write R​i​c​(Ο‰iβ€²)=λ​ωiβ€²+βˆ’1β€‹βˆ‚βˆ‚Β―β€‹hiRic(\omega_{i}^{\prime})=\lambda\omega_{i}^{\prime}+\sqrt{-1}\partial\bar{\partial}h_{i}, where Ξ»\lambda is 11, βˆ’12-\frac{1}{2} or 00. So with suitable normalization of hih_{i} we have the equation

(4.1) Ο‰in=ehi+λ​ϕi​ωiβ€²n.\omega_{i}^{n}=e^{h_{i}+\lambda\phi_{i}}\omega_{i}^{\prime n}.

Then it is not hard to see that ∫Xihi2​ωiβ€²n≀C3\int_{X_{i}}h_{i}^{2}\omega_{i}^{\prime n}\leq C_{3} for some constant C3>0C_{3}>0. Now for any pp in Wr​e​gW^{reg}, we choose a small neighborhood B⁑(p,Ξ΄)βŠ‚Wr​e​gB(p,\delta)\subset W^{reg}. Then there are corresponding points pi∈Xip_{i}\in X_{i}, such that B⁑(pi,Ξ΄)B(p_{i},\delta) converges smoothly to B⁑(p,Ξ΄)B(p,\delta) in ℂ​ℙNk\mathbb{C}\mathbb{P}^{N_{k}}. By standard elliptic estimate we see that |hi|C1​(B⁑(pi,Ξ΄/2),Ο‰iβ€²)|h_{i}|_{C^{1}(B(p_{i},\delta/2),\omega_{i}^{\prime})} is uniformly bounded. Then by (4.1) there is a C4>0C_{4}>0 such that C4βˆ’1​ωi≀ωi′≀C4​ωiC_{4}^{-1}\omega_{i}\leq\omega_{i}^{\prime}\leq C_{4}\omega_{i} in B⁑(pi,Ξ΄/2)B(p_{i},\delta/2). Thus |βˆ‡Ο‰iβ€²Ο•i|Lβˆžβ€‹(B⁑(pi,Ξ΄/2))≀C4​|βˆ‡Ο‰iΟ•i|Lβˆžβ€‹(B⁑(pi,Ξ΄/2))≀C4​C2|\nabla_{\omega_{i}^{\prime}}\phi_{i}|_{L^{\infty}(B(p_{i},\delta/2))}\leq C_{4}|\nabla_{\omega_{i}}\phi_{i}|_{L^{\infty}(B(p_{i},\delta/2))}\leq C_{4}C_{2}. Then in B⁑(pi,Ξ΄/2)B(p_{i},\delta/2) with respect to the metric Ο‰iβ€²\omega_{i}^{\prime}, the right hand side of (4.1) has a uniform C1C^{1} bound. Therefore we can apply the Evans-Krylov theory(see for example [3]) to conclude that |Ο•i||\phi_{i}| has a uniform C2,Ξ±C^{2,\alpha} bound in B⁑(pi,Ξ΄/4)B(p_{i},\delta/4). Then standard arguments show that all covariant derivatives of Ο•i\phi_{i}(with respect to Ο‰iβ€²\omega_{i}^{\prime}) are uniformly bounded, so the KΓ€hler-Einstein metrics Ο‰i\omega_{i} converge smoothly in a neighborhood of pp.

∎

Proposition 4.15.

In the KΓ€hler-Einstein case, the algebro-geometric limit WW has log-terminal singularities.

Proof.

By general theory, what the statement really means is that for any singular point xx in WW, there is a neighborhood UU, and a nowhere zero holomorphic nn form Θ\Theta on Wr​e​g∩UW^{reg}\cap U with ∫Wr​e​g∩UΘ∧Θ¯<∞\int_{W^{reg}\cap U}\Theta\wedge\overline{\Theta}<\infty. We first consider the cases L=KX2L=K_{X}^{2} and KXβˆ’1K_{X}^{-1}. Previous discussion has shown that for any xx, there is a neighborhood UU of xx, an integer k>0k>0, a constant C>0C>0, and a section ss of LkL^{k} over Xβˆžβˆ–Ξ£=Wr​e​gX_{\infty}\setminus\Sigma=W^{reg} with Cβˆ’1≀‖s⁑(x)β€–2≀CC^{-1}\leq\|s(x)\|^{2}\leq C for x∈Wr​e​g∩Ux\in W^{reg}\cap U. Here the norm is taken with respect to the KΓ€hler-Einstein metric. When L=KX2L=K_{X}^{2}, we define Θ=(sβŠ—sΒ―)12​k\Theta=(s\otimes\overline{s})^{\frac{1}{2k}}, then

∫Wr​e​g∩UΘ∧Θ¯=∫Wr​e​g∩Uβ€–sβ€–1k​𝑑v​o​l≀C12​k​V​o​l​(W).\int_{W^{reg}\cap U}\Theta\wedge\overline{\Theta}=\int_{W^{reg}\cap U}\|s\|^{\frac{1}{k}}dvol\leq C^{\frac{1}{2k}}Vol(W).

When L=βˆ’KXL=-K_{X}, we define Θ=(sβˆ—βŠ—sβˆ—Β―)1k\Theta=(s^{*}\otimes\overline{s^{*}})^{\frac{1}{k}}, where sβˆ—s^{*} is the dual section of ss. So β€–sβˆ—β€–=β€–sβ€–βˆ’1\|s^{*}\|=\|s\|^{-1}. Then

∫Wr​e​g∩UΘ∧Θ¯=∫Wr​e​g∩Uβ€–sβˆ—β€–2k​𝑑v​o​l≀Cβˆ’1k​V​o​l​(W).\int_{W^{reg}\cap U}\Theta\wedge\overline{\Theta}=\int_{W^{reg}\cap U}\|s^{*}\|^{\frac{2}{k}}dvol\leq C^{-\frac{1}{k}}Vol(W).

In the Calabi-Yau case, since Θi\Theta_{i} has norm one, we easily see that there is a limit holomorphic volume form Θ\Theta on Xβˆžβˆ–Ξ£=Wr​e​gX_{\infty}\setminus\Sigma=W^{reg} with norm one. Then ∫Wr​e​gΘ∧Θ¯=V​o​l​(W).\int_{W^{reg}}\Theta\wedge\overline{\Theta}=Vol(W). ∎

Remark 4.16.

From the uniform bound of the KΓ€hler potentials Ο•i\phi_{i}, it is not hard to see that the KΓ€hler forms Ο‰i\omega_{i} converge to a singular KΓ€hler-Einstein metric Ο‰βˆž\omega_{\infty} on WW in the sense of [12].

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