ScalingStacks

Proof. [03GX]

Original official author HTML, exact retained edition. Historical TeX conversion verdicts remain unchanged. Cited-edition alignment and mathematical self-containment are not assessed.

Complete original source context · Original author HTML

Proof.

One can prove using an argument due to Donaldson that items (a) and (b) are equivalent. The point is that ΩX\Omega_{X} uniquely determines JXJ_{X} because JXJ_{X} is determined by knowing the subspace ΛJX1,0⊂Λℂ1​X\Lambda^{1,0}_{J_{X}}\subset\Lambda^{1}_{\mathbb{C}}X, and we have ΛJX1,0​X=ker​T\Lambda^{1,0}_{J_{X}}X={\rm ker}\,T, where T:Λℂ1​X→Λℂn+1​XT:\Lambda^{1}_{\mathbb{C}}X\to\Lambda^{n+1}_{\mathbb{C}}X is the ℂ\mathbb{C}-linear map defined by T​α=ΩX∧αT\alpha=\Omega_{X}\wedge\alpha. See Lemma 2.14 in [CH13] for details.

Item (b) can be proved by following the steps of a similar estimate in the asymptotically conical case in Section 2.2 of [CH15]. Fix any background hermitian metric gg on MM. Via gg-orthogonal projection, the holomorphic normal bundle L=ND=T1,0​M|D/T1,0​DL=N_{D}=T^{1,0}M|_{D}/T^{1,0}D is naturally isomorphic to the gg-orthogonal complement (T1,0​D)⟂⊂T1,0​M(T^{1,0}D)^{\perp}\subset T^{1,0}M as a C∞C^{\infty} complex line bundle, and the gg-normal exponential map defines a diffeomorphism from a neighborhood of the zero section in (T1,0​D)⟂(T^{1,0}D)^{\perp} to a neighborhood of DD in MM. Let Φ\Phi be the composition of these two maps. Then Φ\Phi is a diffeomorphism from a neighborhood of the zero section in LL to a neighborhood of DD in MM, and the restriction of Φ\Phi to the zero section is IdD{\rm Id}_{D}. Note that Φ\Phi is almost never holomorphic, but in generic situations Φ\Phi will be one of the “most holomorphic” diffeomorphisms between tubular neighborhoods of DD in LL and in MM. In any case, Φ\Phi turns out to be good enough to obtain the asymptotics (3.13).

Fix a point on DD. Let (z1,…,zn−1,w)(z_{1},\ldots,z_{n-1},w) be local holomorphic coordinates on MM centered at this point such that DD is locally cut out by w=0w=0. Then (z1,…,zn−1,w)(z_{1},\ldots,z_{n-1},w) may also be viewed as local holomorphic coordinates on LL corresponding to the normal vector w⁡(∂∂w+T1,0​D)∈Lw(\frac{\partial}{\partial w}+T^{1,0}D)\in L based at the point (z1,…,zn−1,0)∈D(z_{1},\ldots,z_{n-1},0)\in D. In these coordinates we may write

(3.16) ΩX\displaystyle\Omega_{X} =(f⁡(z)w+g⁡(z,w))​d​z1∧…∧d​zn−1∧d​w,\displaystyle=\biggl(\frac{f(z)}{w}+g(z,w)\biggr)dz_{1}\wedge\ldots\wedge dz_{n-1}\wedge dw,
(3.17) Ω𝒞\displaystyle\Omega_{\mathcal{C}} =f⁡(z)w​d​z1∧…∧d​zn−1∧d​w,\displaystyle=\frac{f(z)}{w}dz_{1}\wedge\ldots\wedge dz_{n-1}\wedge dw,

where f,gf,g are local holomorphic functions with f⁡(z)≠0f(z)\neq 0 for all zz. In order to compare Φ∗​ΩX\Phi^{*}\Omega_{X} to Ω𝒞\Omega_{\mathcal{C}}, we define new C∞C^{\infty} complex coordinates (z1′,…,zn−1′,w)(z_{1}^{\prime},\ldots,z_{n-1}^{\prime},w) on MM by

(3.18) zi′​(z,w)=zi−ai​(z)​w,where​ai​(z)=∂(zi∘Φ)∂w|(z,0).\displaystyle z_{i}^{\prime}(z,w)=z_{i}-a_{i}(z)w,\ \text{where}\ a_{i}(z)=\frac{\partial(z_{i}\circ\Phi)}{\partial w}\biggr|_{(z,0)}.

Using the fact that d​Φd\Phi is complex linear at w=0w=0 and that Φ∗​(∂∂w)=∂∂w+∑ai​(z)​∂∂zi\Phi_{*}(\frac{\partial}{\partial w})=\frac{\partial}{\partial w}+\sum a_{i}(z)\frac{\partial}{\partial z^{i}} at w=0w=0, it is easy to check that these new coordinates satisfy

(3.19) Φ∗​d​zi′=d​zi​and​Φ∗​d​w=d​w​at​w=0.\displaystyle\Phi^{*}dz_{i}^{\prime}=dz_{i}\ \text{and}\ \Phi^{*}dw=dw\ \text{at}\ w=0.

By Taylor expansion, it follows directly from this that

(3.20) Φ∗​zi′=zi+Ai​w2+Bi​w​w¯+Ci​w¯2​and​Φ∗​w=w+A​w2+B​w​w¯+C​w¯2\displaystyle\Phi^{*}z_{i}^{\prime}=z_{i}+A_{i}w^{2}+B_{i}w\overline{w}+C_{i}\overline{w}^{2}\ \text{and}\ \Phi^{*}w=w+Aw^{2}+Bw\overline{w}+C\overline{w}^{2}

with smooth functions Ai,Bi,CiA_{i},B_{i},C_{i} and A,B,CA,B,C. We now express the coordinates (z,w)(z,w) in (3.16) in terms of (z′,w)(z^{\prime},w) using (3.18), and then use (3.20) to compare Φ∗​ΩX\Phi^{*}\Omega_{X} to Ω𝒞\Omega_{\mathcal{C}}. The first step yields

(3.21) ΩX=f⁡(z′)w​d​z1′∧…∧d​zn−1′∧d​w+Υ∧d​w,\displaystyle\Omega_{X}=\frac{f(z^{\prime})}{w}dz_{1}^{\prime}\wedge\ldots\wedge dz_{n-1}^{\prime}\wedge dw+\Upsilon\wedge dw,

where Υ\Upsilon extends to a smooth complex (n−1)(n-1)-form on a neighborhood of DD in MM. Then

(3.22) Φ∗​ΩX−Ω𝒞=(A′+B′​w¯w+C′​w¯2w2)​(Υ′∧d​w)+(A′′+B′′​w¯w+C′′​w¯2w2)​(Υ′′∧d​w¯)+(w​Θ′+w¯​Θ′′+w¯2w​Θ′′′)1+A​w+B​w¯+C​w¯2w+Φ∗​Υ∧(d​w+w​ϕ′+w¯​ϕ′′),\displaystyle\begin{split}&\Phi^{*}\Omega_{X}-\Omega_{\mathcal{C}}\\ =&\frac{(A^{\prime}+B^{\prime}\frac{\overline{w}}{w}+C^{\prime}\frac{\overline{w}^{2}}{w^{2}})(\Upsilon^{\prime}\wedge dw)+(A^{\prime\prime}+B^{\prime\prime}\frac{\overline{w}}{w}+C^{\prime\prime}\frac{\overline{w}^{2}}{w^{2}})(\Upsilon^{\prime\prime}\wedge d\overline{w})+(w\Theta^{\prime}+\overline{w}\Theta^{\prime\prime}+\frac{\overline{w}^{2}}{w}\Theta^{\prime\prime\prime})}{1+Aw+B\overline{w}+C\frac{\overline{w}^{2}}{w}}\\ &+\Phi^{*}\Upsilon\wedge(dw+w\phi^{\prime}+\overline{w}\phi^{\prime\prime}),\end{split}

where A′,B′,C′,A′′,B′′,C′′,Υ′,Υ′′,Θ′,Θ′′,Θ′′′,ϕ′,ϕ′′A^{\prime},B^{\prime},C^{\prime},A^{\prime\prime},B^{\prime\prime},C^{\prime\prime},\Upsilon^{\prime},\Upsilon^{\prime\prime},\Theta^{\prime},\Theta^{\prime\prime},\Theta^{\prime\prime\prime},\phi^{\prime},\phi^{\prime\prime} extend to smooth complex functions, (n−1)(n-1)-forms, nn-forms, and 11-forms on a neighborhood of DD in LL, respectively. The reason for writing the right-hand side of (3.22) in this way is that a smooth complex nn-form is small with respect to g𝒞g_{\mathcal{C}} if it either contains an explicit factor of ww or w¯\overline{w} in front, or if it splits off a wedge factor of d​wdw or d​w¯d\overline{w}. Unfortunately the right-hand side of (3.22) is not smooth at the divisor but all non-smooth terms are due to factors of w¯/w\overline{w}/w, which satisfy the same estimates as smooth functions.

It remains to prove appropriate estimates on |∇g𝒞kF|g𝒞|\nabla^{k}_{g_{\mathcal{C}}}F|_{g_{\mathcal{C}}} for all k≥0k\geq 0, where FF is either a smooth function on a neighborhood of DD in LL, or F=w¯/wF=\overline{w}/w. To begin, note that

(3.23) |∇g𝒞kzi|g𝒞\displaystyle|\nabla_{g_{\mathcal{C}}}^{k}z_{i}|_{g_{\mathcal{C}}} =O⁡(1)​for all​k≥0,\displaystyle=O(1)\ \text{for all}\ k\geq 0,
(3.24) |w|\displaystyle|w| =O⁡(e−12​zn),|∇g𝒞kw|g𝒞=O⁡(e−(12−ϵ)​zn)​for all​k≥1,ϵ>0,\displaystyle=O(e^{-\frac{1}{2}z^{n}}),\ |\nabla_{g_{\mathcal{C}}}^{k}w|_{g_{\mathcal{C}}}=O(e^{-(\frac{1}{2}-\epsilon)z^{n}})\ \text{for all}\ k\geq 1,\epsilon>0,
(3.25) |w−1|\displaystyle|w^{-1}| =O⁡(e12​zn),|∇g𝒞kw−1|g𝒞=O⁡(e(12+ϵ)​zn)​for all​k≥1,ϵ>0.\displaystyle=O(e^{\frac{1}{2}z^{n}}),\ |\nabla_{g_{\mathcal{C}}}^{k}w^{-1}|_{g_{\mathcal{C}}}=O(e^{(\frac{1}{2}+\epsilon)z^{n}})\ \text{for all}\ k\geq 1,\epsilon>0.

Here the bound |zi|=O⁡(1)|z_{i}|=O(1) is clear, and the bounds |w±1|=O⁡(e∓12​zn)|w^{\pm 1}|=O(e^{\mp\frac{1}{2}z^{n}}) follow from the definition of the moment map z=(−log⁡|ξ|h2)1/nz=(-{\log|\xi|_{h}^{2}})^{1/n} together with the fact that |ξ|h2=|w|2​e−ϕ|\xi|_{h}^{2}=|w|^{2}e^{-\phi} with ϕ\phi independent of w,w¯w,\overline{w}. The higher derivative bounds in (3.23)–(3.25) follow from these pointwise bounds by using elliptic estimates for holomorphic functions on a Kähler manifold of C∞C^{\infty} bounded geometry (these estimates apply here because g𝒞g_{\mathcal{C}} is Ricci-flat Kähler of bounded curvature). Note that the ϵ\epsilon-terms in (3.24)–(3.25) are necessary because the sup of |w||w| over a g𝒞g_{\mathcal{C}}-ball of radius 1 is O⁡(|w|1−ϵ)O(|w|^{1-\epsilon}) for every ϵ>0\epsilon>0 but is not O⁡(|w|)O(|w|), unlike on a cylinder ℂw∗×D\mathbb{C}^{*}_{w}\times D with model metric |d​log⁡w|2+gD|d\log w|^{2}+g_{D}.

We now prove by induction that for all smooth functions FF on a neighborhood of DD in LL,

(3.26) |F|=O⁡(1),|∇g𝒞kF|g𝒞=O⁡(eϵ​zn)​for all​k≥1,ϵ>0.|F|=O(1),\ |\nabla_{g_{\mathcal{C}}}^{k}F|_{g_{\mathcal{C}}}=O(e^{\epsilon z^{n}})\ \text{for all}\ k\geq 1,\epsilon>0.

Indeed, the pointwise bound is clear, and for k≥1k\geq 1 we apply ∇g𝒞k−1\nabla_{g_{\mathcal{C}}}^{k-1} to the expansion

(3.27) d​F=∂F∂w​d​w+∂F∂w¯​d​w¯+∑i=1n−1∂F∂zi​d​zi+∑i=1n−1∂F∂z¯i​d​z¯i,dF=\frac{\partial F}{\partial w}dw+\frac{\partial F}{\partial\overline{w}}d\overline{w}+\sum_{i=1}^{n-1}\frac{\partial F}{\partial z_{i}}dz_{i}+\sum_{i=1}^{n-1}\frac{\partial F}{\partial\overline{z}_{i}}d\overline{z}_{i},

using the inductive hypothesis to control ∇g𝒞k−1\nabla_{g_{\mathcal{C}}}^{k-1} of the partials of FF on the right-hand side and using (3.23)–(3.24) to control ∇g𝒞k−1\nabla_{g_{\mathcal{C}}}^{k-1} of d​zi,d​z¯i,d​w,d​w¯dz_{i},d\overline{z}_{i},dw,d\overline{w}. This proves (3.26). By using (3.24)–(3.25) we can then prove in a similar manner that

(3.28) |w¯w|=O⁡(1),|∇g𝒞k(w¯w)|g𝒞=O⁡(eϵ​zn)​for all​k≥1,ϵ>0.\displaystyle\left|\frac{\overline{w}}{w}\right|=O(1),\ \left|\nabla^{k}_{g_{\mathcal{C}}}\left(\frac{\overline{w}}{w}\right)\right|_{g_{\mathcal{C}}}=O(e^{\epsilon z^{n}})\ \text{for all}\ k\geq 1,\epsilon>0.

Taken together, (3.26) and (3.28) allow us to estimate all contributions to (3.22) in all CkC^{k} norms with respect to g𝒞g_{\mathcal{C}}, proving item (b).

To prove item (c), notice that in local coordinates ξ=(z1,…,zn−1,w)∈L\xi=(z_{1},\ldots,z_{n-1},w)\in L as above,

(3.29) Φ∗​|S|hM2=(1+G)​|ξ|h2=(1+G)​|w|2​e−ϕ\Phi^{*}|S|^{2}_{h_{M}}=(1+G)|\xi|^{2}_{h}=(1+G)|w|^{2}e^{-\phi}

with smooth real-valued locally defined functions GG and ϕ\phi, where GG vanishes at w=0w=0 and ϕ\phi does not depend on w,w¯w,\overline{w}. Notice that G=F​w+F​w¯G=Fw+\overline{Fw} for some smooth complex-valued locally defined function FF. This structure of the Φ∗​JX\Phi^{*}J_{X}-Kähler potential of Φ∗​ωX\Phi^{*}\omega_{X}, together with (3.24), (3.26), and item (a), makes it possible to prove that for all k≥0,ϵ>0k\geq 0,\epsilon>0,

(3.30) |∇g𝒞k(Φ∗​ωX−ω𝒞)|g𝒞=O⁡(e−(12−ϵ)​zn).|\nabla^{k}_{g_{\mathcal{C}}}(\Phi^{*}\omega_{X}-\omega_{\mathcal{C}})|_{g_{\mathcal{C}}}=O(e^{-(\frac{1}{2}-\epsilon)z^{n}}).

Similarly by Theorem 3.3 we get for some δ¯>0\underline{\delta}>0 depending on δ0\delta_{0} that for all k≥0k\geq 0,

(3.31) |∇g𝒞k(Φ∗​ωT​Y−Φ∗​ωX)|g𝒞=O⁡(e−δ¯​zn/2).|\nabla^{k}_{g_{\mathcal{C}}}(\Phi^{*}\omega_{TY}-\Phi^{*}\omega_{X})|_{g_{\mathcal{C}}}=O(e^{-\underline{\delta}z^{n/2}}).

This completes the proof of item (c). ∎

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