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4.5. Perturbation of complex structures [0539]

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4.5. Perturbation of complex structures

In Section 4.2 we have identified the underlying complex manifold of our family of C2,αC^{2,\alpha} Kähler metrics (ℳT,ωT)(\mathcal{M}_{T},\omega_{T}). In our gluing argument in Section 7.3 we shall need to perturb the complex structure. This section is devoted to the estimate of error caused by such a perturbation.

Under the holomorphic embedding of ℳT\mathcal{M}_{T} into 𝒩0\mathcal{N}^{0} defined in Section 4.2, ΩT\Omega_{T} is identified with the standard holomorphic volume form Ω𝒩0\Omega_{\mathcal{N}^{0}}.

Fix C>0C>0, and let 𝒱\mathcal{V} be the open neighborhood of 𝒫\mathcal{P} in 𝒩0\mathcal{N}^{0} defined by {r+<C,r−<C}\{r_{+}<C,r_{-}<C\}. Fix a smooth Kähler metric ω𝒩0\omega_{\mathcal{N}^{0}} on 𝒩0\mathcal{N}^{0}. Suppose now that we have a family of complex structures JT′J_{T}^{\prime} on 𝒱\mathcal{V} with holomorphic volume forms ΩT′\Omega_{T}^{\prime} satisfying for all k≥0k\geq 0,

(4.320) sup𝒙∈𝒱|∇ω𝒩0k(ΩT′−Ω𝒩0)​(𝒙)|ω𝒩0≤ϵ¯T2.\sup_{\bm{x}\in\mathcal{V}}|\nabla^{k}_{\omega_{\mathcal{N}^{0}}}(\Omega_{T}^{\prime}-\Omega_{\mathcal{N}^{0}})(\bm{x})|_{\omega_{\mathcal{N}^{0}}}\leq\underline{\epsilon}_{T^{2}}.

We also assume there is a deformation of the form π∗​ωD\pi^{*}\omega_{D} over 𝒱\mathcal{V} to ωD,T\omega_{D,T}, which is a closed (1,1)(1,1) form with respect JT′J_{T}^{\prime}, and satisfies that for all k≥0k\geq 0

(4.321) sup𝒙∈𝒱|∇ω𝒩0k(ωD,T−π∗​ωD)​(𝒙)|ω𝒩0≤ϵ¯T2.\sup_{\bm{x}\in\mathcal{V}}|\nabla^{k}_{\omega_{\mathcal{N}^{0}}}(\omega_{D,T}-\pi^{*}\omega_{D})(\bm{x})|_{\omega_{\mathcal{N}^{0}}}\leq\underline{\epsilon}_{T^{2}}.

Let ϕ\phi be the Kähler potential defined in (4.149). Then we define the new family of closed forms on 𝒱\mathcal{V}

(4.322) Tn−2n​ωT′≡T​ωD,T+d​JT′​d​ϕ.T^{\frac{n-2}{n}}\omega_{T}^{\prime}\equiv T\omega_{D,T}+dJ_{T}^{\prime}d\phi.
Proposition 4.24.

For TT sufficiently large, the above (ωT′,ΩT′)(\omega_{T}^{\prime},\Omega_{T}^{\prime}) defines a family of C1,αC^{1,\alpha} Kähler structures on 𝒱\mathcal{V}, satisfying for all fixed α∈(0,1)\alpha\in(0,1), δ,μ,ν∈ℝ\delta,\mu,\nu\in\mathbb{R}, we have

(4.323) |ΩT′−ΩT|Cδ,μ,ν2,α​(𝒱)\displaystyle|\Omega_{T}^{\prime}-\Omega_{T}|_{C^{2,\alpha}_{\delta,\mu,\nu}(\mathcal{V})} =ϵ¯T2,\displaystyle=\underline{\epsilon}_{T^{2}},
(4.324) |ωT′−ωT|Cδ,μ,ν1,α​(𝒱)\displaystyle|\omega_{T}^{\prime}-\omega_{T}|_{C^{1,\alpha}_{\delta,\mu,\nu}(\mathcal{V})} =ϵ¯T2.\displaystyle=\underline{\epsilon}_{T^{2}}.

We first reduce the estimate to a local form. Choose finitely many holomorphic charts (Uβ,w1,⋯,wn−1)(U_{\beta},w_{1},\cdots,w_{n-1}) in DD of the form {|w1|<1,⋯,|wn−1|<1}\{|w_{1}|<1,\cdots,|w_{n-1}|<1\}, such that the smaller charts given by Vβ={|w1|<1/2,⋯,|wn−1|<1/2}V_{\beta}=\{|w_{1}|<1/2,\cdots,|w_{n-1}|<1/2\} also cover DD. We may also assume if a UβU_{\beta} intersects HH, then it is centered at some p∈Hp\in H, i.e. wi​(p)=0w_{i}(p)=0 for all ii, and also HH is defined by w1=0w_{1}=0 in this chart. We may further assume in each UβU_{\beta} the line bundle LL has a holomorphic trivialization σβ\sigma_{\beta}, under which we may view ζ±\zeta_{\pm} as local holomorphic functions on 𝒩0\mathcal{N}^{0}, and 𝒱∩π−1​(Uβ)\mathcal{V}\cap\pi^{-1}(U_{\beta}) is locally defined by |ζ±|<C​|σL|−|k±||\zeta_{\pm}|<C|\sigma_{L}|^{-|k_{\pm}|}. These then give an open cover of 𝒱\mathcal{V} by 𝒱∩π−1​(Vβ)\mathcal{V}\cap\pi^{-1}(V_{\beta}), and it suffices to prove the estimates in each such open set.

We shall work with one β\beta such that Uβ∩H≠∅U_{\beta}\cap H\neq\emptyset. The other case can be proved similarly. For such β\beta in π−1​(Uβ)\pi^{-1}(U_{\beta}), by definition of 𝒩0\mathcal{N}^{0}, we get the equation

(4.325) ζ+⋅ζ−=w1​F​(w1,⋯,wn−1)\zeta_{+}\cdot\zeta_{-}=w_{1}F(w_{1},\cdots,w_{n-1})

for a non-zero holomorphic function FF. So without loss of generality we may assume ζ+,ζ−,w2,⋯,wn−1\zeta_{+},\zeta_{-},w_{2},\cdots,w_{n-1} are holomorphic coordinates on π−1​(Uβ)\pi^{-1}(U_{\beta}).

We first prove (4.323). The hypothesis implies that

(4.326) ΩT′−ΩT=Gi1​…​in​ei1∧…∧ein,\Omega_{T}^{\prime}-\Omega_{T}=G_{i_{1}\ldots i_{n}}e_{i_{1}}\wedge\ldots\wedge e_{i_{n}},

where each eje_{j} is one of d​ζ±,d​ζ¯±,d​wj,d​w¯j​(j≥2)d\zeta_{\pm},d\bar{\zeta}_{\pm},dw_{j},d\bar{w}_{j}(j\geq 2), and Gi1​…​inG_{i_{1}\ldots i_{n}} is a smooth function in ζ±,ζ¯±,wj,w¯j​(j≥2)\zeta_{\pm},\bar{\zeta}_{\pm},w_{j},\bar{w}_{j}(j\geq 2) and its kk-th derivative over 𝒱\mathcal{V} with respect to the fixed metric ω𝒩0\omega_{\mathcal{N}^{0}} is bounded by ϵ¯T2\underline{\epsilon}_{T^{2}} for all kk. Since a holomorphic function is automatically harmonic with respect to any Kähler metric, we have

(4.327) ΔωT​ζ±=ΔωT​wj=0.\Delta_{\omega_{T}}\zeta_{\pm}=\Delta_{\omega_{T}}w_{j}=0.

By Corollary 4.11.1, Item (1), we know 𝒱\mathcal{V} is contained in the region |z|≤1|z|\leq 1. Also notice by the discussion in Section 4.3 there is a constant C>1C>1 such that for each 𝒙∈𝒱∩π−1​(Vβ)\bm{x}\in\mathcal{V}\cap\pi^{-1}(V_{\beta}), the ball BC−1​𝔰​(𝒙)​(𝒙)B_{C^{-1}\mathfrak{s}(\bm{x})}(\bm{x}) is contained in π−1(Uβ)∩{|z|≤2}\pi^{-1}(U_{\beta})\cap\{|z|\leq 2\}. Again by Corollary 4.11.1, Item (3) on π−1(Uβ)∩{|z|≤2}\pi^{-1}(U_{\beta})\cap\{|z|\leq 2\}, we have

(4.328) |ζ±|≤C​r±≤C​e3​T.|\zeta_{\pm}|\leq Cr_{\pm}\leq Ce^{3T}.

Now applying Proposition 4.22 to every 𝒙∈𝒱∩π−1​(Vβ)\bm{x}\in\mathcal{V}\cap\pi^{-1}(V_{\beta}) we obtain

(4.329) |ζ±|Cδ,μ,ν3,α​(𝒱)≤C|ζ±|C0δ,μ,ν(π−1(Uβ)∩{|z|≤1})≤Ce3​T.|\zeta_{\pm}|_{C^{3,\alpha}_{\delta,\mu,\nu}(\mathcal{V})}\leq C|\zeta_{\pm}|_{C^{0}_{\delta,\mu,\nu}(\pi^{-1}(U_{\beta})\cap\{|z|\leq 1\})}\leq Ce^{3T}.

Similarly, since on UβU_{\beta} we have |wj|<1|w_{j}|<1, we get for j=2,⋯,n−1j=2,\cdots,n-1,

(4.330) |wj|Cδ,μ,ν3,α​(𝒱)≤|wj|C0δ,μ,ν(π−1(Uβ)∩{|z|≤1})≤C.|w_{j}|_{C^{3,\alpha}_{\delta,\mu,\nu}(\mathcal{V})}\leq|w_{j}|_{C^{0}_{\delta,\mu,\nu}(\pi^{-1}(U_{\beta})\cap\{|z|\leq 1\})}\leq C.

Then using the chain rule and induction we get that

(4.331) |Gi1⋯in|Cδ,ν,μ3,α​(𝒱)=ϵ¯T2⋅Ce3​T=ϵ¯T2.|G_{i_{1}\cdots i_{n}}|_{C^{3,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}=\underline{\epsilon}_{T^{2}}\cdot Ce^{3T}=\underline{\epsilon}_{T^{2}}.

So

(4.332) |ΩT′−ΩT|Cδ,μ,ν2,α​(𝒱)=ϵ¯T2.|\Omega_{T}^{\prime}-\Omega_{T}|_{C^{2,\alpha}_{\delta,\mu,\nu}(\mathcal{V})}=\underline{\epsilon}_{T^{2}}.

Notice the complex structure JT′J_{T}^{\prime} is pointwise determined by the holomorphic nn form ΩT′\Omega_{T}^{\prime} algebraically, we get

(4.333) |JT′−JT|Cδ,ν,μ2,α​(𝒱)=ϵ¯T2.|J_{T}^{\prime}-J_{T}|_{C^{2,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}=\underline{\epsilon}_{T^{2}}.

Now to prove (4.324), we write

(4.334) ωT′=ωT+T⁡(ωD,T−π∗​ωD)+d⁡((JT′−JT)​d​ϕ).\omega_{T}^{\prime}=\omega_{T}+T(\omega_{D,T}-\pi^{*}\omega_{D})+d((J_{T}^{\prime}-J_{T})d\phi).

By assumption, and the above discussion, using (4.329) we get

(4.335) |ωD,T−π∗ω|C2,αδ,ν,μ(π−1(Uβ)∩{|z|≤1})=ϵ¯T2|\omega_{D,T}-\pi^{*}\omega|_{C^{2,\alpha}_{\delta,\nu,\mu}(\pi^{-1}(U_{\beta})\cap\{|z|\leq 1\})}=\underline{\epsilon}_{T^{2}}

It is also easy to see

(4.336) |V1⋅V2|Cδ,ν,μ2,α​(𝒱)≤Tm​|V1|Cδ,ν,μ2,α​(𝒱)|​V2|Cδ,ν,μ2,α​(𝒱),|V_{1}\cdot V_{2}|_{C^{2,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}\leq T^{m}|V_{1}|_{C^{2,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}|V_{2}|_{C^{2,\alpha}_{\delta,\nu,\mu}(\mathcal{V})},

for some m>0m>0 independent of V1V_{1} and V2V_{2}. So (4.324) is a consequence of the following

Lemma 4.25.
(4.337) |ϕ|Cδ,ν,μ3,α​(𝒱)≤eC​T.|\phi|_{C^{3,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}\leq e^{CT}.
Proof.

Since by construction

(4.338) Tn−2n​ω=T​π∗​ωD+d​dc​ϕ.T^{\frac{n-2}{n}}\omega=T\pi^{*}\omega_{D}+dd^{c}\phi.

We have

(4.339) ΔT2​n−2n​ω​ϕ=n−T⋅TrT2​n−2n​ω⁡π∗​ωD.\Delta_{T^{\frac{2n-2}{n}}\omega}\phi=n-T\cdot\Tr_{T^{\frac{2n-2}{n}}\omega}\pi^{*}\omega_{D}.

Since π∗​ωD\pi^{*}\omega_{D} is smooth on 𝒱\mathcal{V} and ω\omega is parallel, again the above discussion gives that

(4.340) |TrT2​n−2n​ω⁡π∗​ωD|Cδ,ν,μ1,α​(𝒱)≤eC​T.|\Tr_{T^{\frac{2n-2}{n}}\omega}\pi^{*}\omega_{D}|_{C^{1,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}\leq e^{CT}.

So by Proposition 4.22 we get that

(4.341) |ϕ|Cδ,ν,μ3,α​(𝒱)≤eC​T+C|ϕ|C0δ,ν,μ(π−1(Uβ)∩{|z|≤1}).|\phi|_{C^{3,\alpha}_{\delta,\nu,\mu}(\mathcal{V})}\leq e^{CT}+C|\phi|_{C^{0}_{\delta,\nu,\mu}(\pi^{-1}(U_{\beta})\cap\{|z|\leq 1\})}.

To bound the right hand side we use the formula

(4.342) ϕ=∫T+zu​h​(u)​𝑑u+ϕ⁡(T+)=∫T+0u​h​(u)​𝑑u+ϕ⁡(T+)+∫0zu​h​(u)​𝑑u.\phi=\int_{T_{+}}^{z}uh(u)du+\phi(T_{+})=\int_{T_{+}}^{0}uh(u)du+\phi(T_{+})+\int_{0}^{z}uh(u)du.

Hence

(4.343) ϕ=T2​z2+12​r+BT+O⁡(1),\phi=\frac{T}{2}z^{2}+\frac{1}{2}r+B_{T}+O(1),

which gives

(4.344) |ϕ|C0δ,ν,μ(π−1(Uβ)∩{|z|≤1})≤O(Tm)|\phi|_{C^{0}_{\delta,\nu,\mu}(\pi^{-1}(U_{\beta})\cap\{|z|\leq 1\})}\leq O(T^{m})

for some m>0m>0. The conclusion then follows. ∎

Remark 4.25.1.

In principle, it is possible to obtain more refined estimates with respect to the higher order weighted norms of ζ±\zeta_{\pm} and ϕ\phi by more direct calculation. The above argument using weighted Schauder estimates avoids the lengthy computations, and it suffices for our purpose since in our setting the error caused by complex structure perturbation is at the scale e−C​T2e^{-CT^{2}} while the weighted analysis in the region {|z|≤1}\{|z|\leq 1\} only introduces at most eC​Te^{CT} error. It is also possible to improve the estimates by working on a scale much smaller than the regularity scale, but again that is not needed for our applications in this paper.

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