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6.1. Framework of perturbation [054S]

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6.1. Framework of perturbation

The studies and applications of the implicit function theorem have been well developed in various contexts. We refer the readers to the book [KP13] for seeing the comprehensive discussions and the history of the whole methodology. For our practical and specific applications, we need the following quantitative version of implicit function theorem (Lemma 6.1), which is based on Banach contraction mapping principle.

To avoid confusions, we clarify several notations as follows:

  • •

    Let ℒ:𝔄→𝔅\mathscr{L}:\mathfrak{A}\to\mathfrak{B} be a bounded linear operator between normed linear spaces 𝔄\mathfrak{A} and 𝔅\mathfrak{B}, then the operator norm of ℒ\mathscr{L} is defined by

    (6.1) ∥ℒ∥o​p≡inf{M0∈ℝ+|∥ℒ(𝒗)∥𝔅≤M0⋅∥𝒗∥𝔄,∀𝒗∈𝔄}.\|\mathscr{L}\|_{op}\equiv\inf\Big\{M_{0}\in\mathbb{R}_{+}\Big|\ \|\mathscr{L}(\bm{v})\|_{\mathfrak{B}}\leq M_{0}\cdot\|\bm{v}\|_{\mathfrak{A}},\ \forall\bm{v}\in\mathfrak{A}\Big\}.
  • •

    We use the common notation 𝟎\bm{0} for the zero vector in every normed linear space.

Lemma 6.1 (Implicit function theorem).

Let ℱ:𝔄→𝔅\mathscr{F}:\mathfrak{A}\to\mathfrak{B} be a map between two Banach spaces such that for all 𝐯∈𝔄\bm{v}\in\mathfrak{A},

(6.2) ℱ⁡(𝒗)−ℱ⁡(𝟎)=ℒ⁡(𝒗)+𝒩⁡(𝒗),\mathscr{F}(\bm{v})-\mathscr{F}(\bm{0})=\mathscr{L}(\bm{v})+\mathscr{N}(\bm{v}),

where the operator ℒ:𝔄→𝔅\mathscr{L}:\mathfrak{A}\to\mathfrak{B} is linear and the operator 𝒩:𝔄→𝔅\mathscr{N}:\mathfrak{A}\to\mathfrak{B} satisfies 𝒩⁡(𝟎)=𝟎\mathscr{N}(\bm{0})=\bm{0}. Additionally we assume the following properties:

  1. (1)

    (Bounded inverse) ℒ:𝔄→𝔅\mathscr{L}:\mathfrak{A}\to\mathfrak{B} is an isomorphism and there is some constant CL>0C_{L}>0 such that

    (6.3) ‖ℒ−1‖o​p≤CL,\|\mathscr{L}^{-1}\|_{op}\leq C_{L},

    where ℒ−1\mathscr{L}^{-1} is the inverse of ℒ\mathscr{L}.

  2. (2)

    There exists a constant CN>0C_{N}>0 and there is some r0∈(0,12​CL​CN)r_{0}\in(0,\frac{1}{2C_{L}C_{N}}) satisfying the following:

    1. (a)

      (Controlled nonlinear error) for all 𝒗1,𝒗2∈Br0​(𝟎)¯⊂𝔄\bm{v}_{1},\bm{v}_{2}\in\overline{B_{r_{0}}(\bm{0})}\subset\mathfrak{A},

      (6.4) ‖𝒩⁡(𝒗1)−𝒩⁡(𝒗2)‖𝔅≤CN⋅r0⋅‖𝒗1−𝒗2‖𝔄.\|\mathscr{N}(\bm{v}_{1})-\mathscr{N}(\bm{v}_{2})\|_{\mathfrak{B}}\leq C_{N}\cdot r_{0}\cdot\|\bm{v}_{1}-\bm{v}_{2}\|_{\mathfrak{A}}.
    2. (b)

      (Controlled initial error) ℱ⁡(𝟎)\mathscr{F}(\bm{0}) is effectively controlled as follows,

      (6.5) ‖ℱ⁡(𝟎)‖𝔅≤r04​CL.\|\mathscr{F}(\bm{0})\|_{\mathfrak{B}}\leq\frac{r_{0}}{4C_{L}}.

Then the equation ℱ⁡(𝐱)=𝟎\mathscr{F}(\bm{x})=\bm{0} has a unique solution 𝐱∈Br0​(𝟎)\bm{x}\in B_{r_{0}}(\bm{0}) with the estimate

(6.6) ‖𝒙‖𝔄≤2​CL⋅‖ℱ⁡(𝟎)‖𝔅.\|\bm{x}\|_{\mathfrak{A}}\leq 2C_{L}\cdot\|\mathscr{F}(\bm{0})\|_{\mathfrak{B}}.
Remark 6.1.1.

In our applications, the constants CL>0C_{L}>0, CN>0C_{N}>0 and r0>0r_{0}>0 will be fixed as uniform constants (independent of T≫1T\gg 1). We will see this from the global linear and nonlinear estimates, which will be stated and proved in next subsections. With the specified weight parameters δ,μ,ν\delta,\mu,\nu, the error estimate in Proposition 4.23 in fact guarantees ‖ErrC​Y‖𝔅→0\|\mathrm{Err}_{CY}\|_{\mathfrak{B}}\to 0 as T→∞T\to\infty, which particularly implies ‖ℱ⁡(𝟎)‖𝔅→0\|\mathscr{F}(\bm{0})\|_{\mathfrak{B}}\to 0 and hence ℱ\mathscr{F} satisfies (b) of Item (2) in the above lemma.

To set up the perturbation problem in our setting, we define the Banach spaces

𝔖1\displaystyle\mathfrak{S}_{1} ≡{−1​∂∂¯​ϕ∈Ω1,1​(ℳT)|ϕ∈C2,α​(ℳT)​is​S1​-invariant and satisfies​∂ϕ∂n|∂ℳT=0},\displaystyle\equiv\Big\{\sqrt{-1}\partial\bar{\partial}\phi\in\Omega^{1,1}(\mathcal{M}_{T})\Big|\phi\in C^{2,\alpha}(\mathcal{M}_{T})\ \text{is}\ S^{1}\text{-invariant and satisfies}\ \frac{\partial\phi}{\partial n}\Big|_{\partial\mathcal{M}_{T}}=0\Big\},
(6.7) 𝔖2\displaystyle\mathfrak{S}_{2} ≡{f∈C0,α​(ℳT)|f​is​S1​-invariant and​∫ℳTf⋅ωTn=0}.\displaystyle\equiv\Big\{f\in C^{0,\alpha}(\mathcal{M}_{T})\Big|f\ \text{is}\ S^{1}\text{-invariant and}\ \int_{\mathcal{M}_{T}}f\cdot\omega_{T}^{n}=0\Big\}.

endowed with the weighted Hölder norms

(6.8) ‖−1​∂∂¯​ϕ‖𝔖1\displaystyle\|\sqrt{-1}\partial\bar{\partial}\phi\|_{\mathfrak{S}_{1}} ≡‖−1​∂∂¯​ϕ‖Cδ,ν+2,μ0,α​(Xt),\displaystyle\equiv\|\sqrt{-1}\partial\bar{\partial}\phi\|_{C_{\delta,\nu+2,\mu}^{0,\alpha}(X_{t})},
(6.9) ‖f‖𝔖2\displaystyle\|f\|_{\mathfrak{S}_{2}} ≡‖−1​∂∂¯​ϕ‖Cδ,ν+2,μ0,α​(Xt).\displaystyle\equiv\|\sqrt{-1}\partial\bar{\partial}\phi\|_{C_{\delta,\nu+2,\mu}^{0,\alpha}(X_{t})}.

Notice an S1S^{1} invariant function ϕ\phi on ℳT\mathcal{M}_{T} can be identified with a function on the quotient QTQ_{T}, and the Neumann boundary condition ∂ϕ∂n|∂ℳT=0\frac{\partial\phi}{\partial n}|_{\partial\mathcal{M}_{T}}=0 amounts to the condition ∂zϕ=0\partial_{z}\phi=0 on ∂QT\partial Q_{T}.

In this section, the weight parameters are specified as follows:

  1. (NP1)

    (Fix ν\nu) The parameters ν∈ℝ\nu\in\mathbb{R} is chosen such that

    (6.10) ν∈(−1,0).\displaystyle\nu\in(-1,0).

    In our context, Lemma 6.5 requires ν∈(−1,1)\nu\in(-1,1). To effectively apply Proposition 4.23, we need ν∈(−1,0)\nu\in(-1,0).

  2. (NP2)

    (Fix α\alpha) The Hölder order α∈(0,1)\alpha\in(0,1) is chosen sufficiently small such that

    (6.11) ν+α<0.\nu+\alpha<0.
  3. (NP3)

    (Fix δ\delta) δ>0\delta>0 is chosen such that

    (6.12) 0<δ<δN≡1n⋅(|k−|+|k+|)n⋅min⁡{δb,δe,λD},0<\delta<\delta_{N}\equiv\frac{1}{n\cdot(|k_{-}|+|k_{+}|)^{n}}\cdot\min\{\delta_{b},\delta_{e},\sqrt{\lambda_{D}}\},

    where ϵX>0\epsilon_{X}>0 is the constant in Theorem 5.2, λD\sqrt{\lambda_{D}} is in Lemma 6.7 (Liouville theorem on QQ), δb>0\delta_{b}>0 is in Proposition 5.14 (Liouville theorem on the Calabi space 𝒞n\mathcal{C}^{n} around the boundary of the neck), δe>0\delta_{e}>0 is in the error estimate Proposition 4.23.

  4. (NP4)

    (Fix μ\mu) The parameter μ\mu is fixed by

    (6.13) μ=(1−1n)​(ν+2+α).\mu=(1-\frac{1}{n})(\nu+2+\alpha).

    This condition guarantees that the weight function ρδ,ν,μ(α)\rho_{\delta,\nu,\mu}^{(\alpha)} with parameters specified as the above is uniformly bounded from below. This will be used in proving Proposition 6.4.

We first normalize the holomorphic volume form. For T≫1T\gg 1, starting with the C2,αC^{2,\alpha}-Kähler structure (ωT,ΩT)(\omega_{T},\Omega_{T}), we will solve the Calabi-Yau equation

(6.14) 1n!​(ωT+−1​∂∂¯​ϕ)n=(−1)n2​2−n⋅ΩT∧.Ω¯T.\frac{1}{n!}(\omega_{T}+\sqrt{-1}\partial\bar{\partial}\phi)^{n}=(\sqrt{-1})^{n^{2}}2^{-n}\cdot\Omega_{T}\wedge.\bar{\Omega}_{T}.

Notice that

(6.15) ∫ℳT(−1)n22n​ΩT∧Ω¯T\displaystyle\int_{\mathcal{M}_{T}}\frac{(\sqrt{-1})^{n^{2}}}{2^{n}}\Omega_{T}\wedge\bar{\Omega}_{T} =∫ℳTh⋅ωDn−1(n−1)!​𝑑z∧Θ=∫T−T+d​z​∫Dh​ωDn−1(n−1)!\displaystyle=\int_{\mathcal{M}_{T}}h\cdot\frac{\omega_{D}^{n-1}}{(n-1)!}dz\wedge\Theta=\int_{T_{-}}^{T_{+}}dz\int_{D}h\frac{\omega_{D}^{n-1}}{(n-1)!}

and

(6.16) ∫ℳTωTnn!=T2−n​∫ℳTω~​(z)n−1(n−1)!​𝑑z∧Θ=T2−n(n−1)!​∫T−T+d​z​∫Dω~​(z)n−1=C1​T2\displaystyle\int_{\mathcal{M}_{T}}\frac{\omega_{T}^{n}}{n!}=T^{2-n}\int_{\mathcal{M}_{T}}\frac{\tilde{\omega}(z)^{n-1}}{(n-1)!}dz\wedge\Theta=\frac{T^{2-n}}{(n-1)!}\int_{T_{-}}^{T_{+}}dz\int_{D}\tilde{\omega}(z)^{n-1}=C_{1}T^{2}

for some computable constant C1>0C_{1}>0. So by (4.14) we get

(6.17) ∫ℳT(−1)n22n​ΩT∧Ω¯T=(1+O⁡(T−2))​∫ℳTωTnn!.\int_{\mathcal{M}_{T}}\frac{(\sqrt{-1})^{n^{2}}}{2^{n}}\Omega_{T}\wedge\bar{\Omega}_{T}=(1+O(T^{-2}))\int_{\mathcal{M}_{T}}\frac{\omega_{T}^{n}}{n!}.

Now we replace ΩT\Omega_{T} by

(6.18) (∫ℳT(−1)n22n​ΩT∧ΩT¯∫ℳTωTnn!)−12​ΩT\Big(\frac{\int_{\mathcal{M}_{T}}\frac{(\sqrt{-1})^{n^{2}}}{2^{n}}\Omega_{T}\wedge\bar{\Omega_{T}}}{\int_{\mathcal{M}_{T}}\frac{\omega_{T}^{n}}{n!}}\Big)^{-\frac{1}{2}}\Omega_{T}

Then we have

(6.19) (−1)n22n​ΩT∧Ω¯T=(1+ErrC​Y)​ωTnn!\frac{(\sqrt{-1})^{n^{2}}}{2^{n}}\Omega_{T}\wedge\bar{\Omega}_{T}=(1+\mathrm{Err}_{CY})\frac{\omega_{T}^{n}}{n!}

where

(6.20) ∫ℳTErrC​Y​ωTn=0.\int_{\mathcal{M}_{T}}\mathrm{Err}_{CY}\omega_{T}^{n}=0.

Applying Proposition 4.23 and (6.13),

(6.21) ‖ErrC​Y‖Cδ,ν+2,μ0,α​(ℳT)=O⁡(Tν+α).\|\mathrm{Err}_{CY}\|_{C^{0,\alpha}_{\delta,\nu+2,\mu}(\mathcal{M}_{T})}=O(T^{\nu+\alpha}).

Let ℱ\mathscr{F} be the map sending every −1​∂∂¯​ϕ∈𝔖1\sqrt{-1}\partial\bar{\partial}\phi\in\mathfrak{S}_{1} to the function which satisfies

(6.22) ℱ⁡(−1​∂∂¯​ϕ)⋅ωTn≡(ωT+−1​∂∂¯​ϕ)n−ωTn​(1−ErrC​Y).\mathscr{F}(\sqrt{-1}\partial\bar{\partial}\phi)\cdot\omega_{T}^{n}\equiv(\omega_{T}+\sqrt{-1}\partial\bar{\partial}\phi)^{n}-\omega_{T}^{n}(1-\mathrm{Err}_{CY}).

Then (6.21) immediately tells us that

(6.23) ‖ℱ⁡(𝟎)‖𝔖2=O⁡(Tν+α).\|\mathscr{F}(\bm{0})\|_{\mathfrak{S}_{2}}=O(T^{\nu+\alpha}).
Lemma 6.2.

ℱ⁡(𝔖1)⊂𝔖2\mathscr{F}(\mathfrak{S}_{1})\subset\mathfrak{S}_{2}.

Proof.

This amounts to proving that

(6.24) ∫ℳTℱ⁡(−1​∂∂¯​ϕ)​ωTn=0.\int_{\mathcal{M}_{T}}\mathscr{F}(\sqrt{-1}\partial\bar{\partial}\phi)\omega_{T}^{n}=0.

By Stokes’ theorem,

(6.25) ∫ℳT(ωT+−1​∂∂¯​ϕ)n−∫ℳTωTn=∫∂ℳTγ,\int_{\mathcal{M}_{T}}(\omega_{T}+\sqrt{-1}\partial\bar{\partial}\phi)^{n}-\int_{\mathcal{M}_{T}}\omega_{T}^{n}=\int_{\partial\mathcal{M}_{T}}\gamma,

where γ\gamma is the sum of terms involving one factor dc​ϕd^{c}\phi and either d​dc​ϕdd^{c}\phi or ωT\omega_{T}. We claim that γ\gamma identically vanishes on ∂ℳT\partial\mathcal{M}_{T}. It suffices to show ∂t⌟​γ=0\partial_{t}\lrcorner\gamma=0. Since by assumption ϕ\phi is S1S^{1}-invariant, so we have ∂tϕ=0\partial_{t}\phi=0. By the Neumann boundary condition, we also have dcϕ(∂t)=0d^{c}\phi(\partial_{t})=0 on ∂ℳT\partial\mathcal{M}_{T}. This follows from the observation that J∂t=∇zJ\partial_{t}=\nabla z. Now

(6.26) ∂t⌟​ωT|∂ℳT\displaystyle\partial_{t}\lrcorner\omega_{T}|_{\partial\mathcal{M}_{T}} =d​z|∂ℳT=0,\displaystyle=dz|_{\partial\mathcal{M}_{T}}=0,
(6.27) ∂t⌟​d​dc​ϕ\displaystyle\partial_{t}\lrcorner dd^{c}\phi =ℒ∂t​(dc​ϕ)−d⁡(∂t⌟​dc​ϕ)=−d⁡(∂t⌟​dc​ϕ).\displaystyle=\mathcal{L}_{\partial_{t}}(d^{c}\phi)-d(\partial_{t}\lrcorner d^{c}\phi)=-d(\partial_{t}\lrcorner d^{c}\phi).

The last term vanishes on ∂ℳT\partial\mathcal{M}_{T} since dcϕ(∂t)=0d^{c}\phi(\partial_{t})=0 pointwise on ∂ℳT\partial\mathcal{M}_{T}. ∎

Now we are ready to state the main result in this section.

Theorem 6.3 (Existence of S1S^{1}-invariant Calabi-Yau metrics).

For each sufficiently large TT, there exists an S1S^{1}-invariant Calabi-Yau metric ωT,C​Y=ωT+−1​∂∂¯​ϕ\omega_{T,CY}=\omega_{T}+\sqrt{-1}\partial\bar{\partial}\phi for ϕ∈𝔖1\phi\in\mathfrak{S}_{1}, such that

(6.28) ‖−1​∂∂¯​ϕ‖𝔖1≤C0⋅Tν+α,\|\sqrt{-1}\partial\bar{\partial}\phi\|_{\mathfrak{S}_{1}}\leq C_{0}\cdot T^{\nu+\alpha},

where C0>0C_{0}>0 is a uniform constant independent of T≫1T\gg 1 and the weighted Hölder norm of 𝔖1\mathfrak{S}_{1} is defined in (6.8) for parameters ν\nu, α\alpha, δ\delta and μ\mu satisfying (6.10), (6.11), (6.12) and (6.13).

To prove Theorem 6.3, we decompose the map ℱ:𝔖1→𝔖2\mathscr{F}:\mathfrak{S}_{1}\to\mathfrak{S}_{2} as follows,

(6.29) ℱ⁡(−1​∂∂¯​ϕ)−ℱ⁡(𝟎)=ℒ⁡(−1​∂∂¯​ϕ)+𝒩⁡(−1​∂∂¯​ϕ),\mathscr{F}(\sqrt{-1}\partial\bar{\partial}\phi)-\mathscr{F}(\bm{0})=\mathscr{L}(\sqrt{-1}\partial\bar{\partial}\phi)+\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi),

for any −1​∂∂¯​ϕ∈𝔖1\sqrt{-1}\partial\bar{\partial}\phi\in\mathfrak{S}_{1}, where

(6.30) ℒ⁡(−1​∂∂¯​ϕ)\displaystyle\mathscr{L}(\sqrt{-1}\partial\bar{\partial}\phi) =Δ​ϕ,\displaystyle=\Delta\phi,
(6.31) 𝒩⁡(−1​∂∂¯​ϕ)⋅ωTn\displaystyle\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi)\cdot\omega_{T}^{n} =(ωT+−1​∂∂¯​ϕ)n−ωTn−n​ωTn−1∧−1​∂∂¯​ϕ.\displaystyle=(\omega_{T}+\sqrt{-1}\partial\bar{\partial}\phi)^{n}-\omega_{T}^{n}-n\omega_{T}^{n-1}\wedge\sqrt{-1}\partial\bar{\partial}\phi.

By the definition of the weight function and Lemma 4.20, we have the following nonlinear error estimate.

Lemma 6.4 (Nonlinear error estimate).

For any sufficiently large T≫1T\gg 1, let ℳT\mathcal{M}_{T} be the neck endowed with the C2,αC^{2,\alpha}-structure (ωT,ΩT)(\omega_{T},\Omega_{T}). Then there exists a constant CN>0C_{N}>0 independent of T≫1T\gg 1 such that for all

(6.32) ϱ∈(0,12)\varrho\in(0,\frac{1}{2})

and

(6.33) −1​∂∂¯​ϕ2∈Bϱ​(𝟎)¯⊂𝔖1,−1​∂∂¯​ϕ2∈Bϱ​(𝟎)¯⊂𝔖1,\sqrt{-1}\partial\bar{\partial}\phi_{2}\in\overline{B_{\varrho}(\bm{0})}\subset\mathfrak{S}_{1},\quad\sqrt{-1}\partial\bar{\partial}\phi_{2}\in\overline{B_{\varrho}(\bm{0})}\subset\mathfrak{S}_{1},

we have the pointwise estimate

(6.34) ‖𝒩⁡(−1​∂∂¯​ϕ1)−𝒩⁡(−1​∂∂¯​ϕ2)‖𝔖2≤CN⋅ϱ⋅‖−1​∂∂¯​(ϕ1−ϕ2)‖𝔖1.\displaystyle\|\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{1})-\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{2})\|_{\mathfrak{S}_{2}}\leq C_{N}\cdot\varrho\cdot\|\sqrt{-1}\partial\bar{\partial}(\phi_{1}-\phi_{2})\|_{\mathfrak{S}_{1}}.
Proof.

By definition,

(𝒩⁡(−1​∂∂¯​ϕ1)−𝒩⁡(−1​∂∂¯​ϕ2))⋅ω​(t)n\displaystyle\Big(\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{1})-\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{2})\Big)\cdot\omega(t)^{n}
(6.35) =\displaystyle= ∑k=2n(nk)⋅ω​(t)n−k∧((−1​∂∂¯​ϕ1)k−(−1​∂∂¯​ϕ2)k).\displaystyle\sum\limits_{k=2}^{n}\begin{pmatrix}n\\ k\end{pmatrix}\cdot\omega(t)^{n-k}\wedge\Big((\sqrt{-1}\partial\bar{\partial}\phi_{1})^{k}-(\sqrt{-1}\partial\bar{\partial}\phi_{2})^{k}\Big).

By the definition of the norm on 𝔖1\mathfrak{S}_{1}, we have

(6.36) ‖−1​∂∂¯​ϕ1‖Cδ,ν+2,μ0,α​(ℳT)≤ϱ,‖−1​∂∂¯​ϕ1‖Cδ,ν+2,μ0,α​(ℳT)≤ϱ.\|\sqrt{-1}\partial\bar{\partial}\phi_{1}\|_{C_{\delta,\nu+2,\mu}^{0,\alpha}(\mathcal{M}_{T})}\leq\varrho,\quad\|\sqrt{-1}\partial\bar{\partial}\phi_{1}\|_{C_{\delta,\nu+2,\mu}^{0,\alpha}(\mathcal{M}_{T})}\leq\varrho.

With μ\mu specified by (6.13), by Lemma 4.20, the weight function ρδ,ν+2,μ(α):ℳT→ℝ+\rho_{\delta,\nu+2,\mu}^{(\alpha)}:\mathcal{M}_{T}\to\mathbb{R}_{+} satisfies for any 𝒙∈ℳT\bm{x}\in\mathcal{M}_{T},

(6.37) ρδ,ν+2,μ(α)​(𝒙)≥1.\rho_{\delta,\nu+2,\mu}^{(\alpha)}(\bm{x})\geq 1.

This implies the following weight-free estimates,

(6.38) ‖−1​∂∂¯​ϕ1‖C0,α​(ℳT)≤C0⋅ϱand‖−1​∂∂¯​ϕ2‖C0,α​(ℳT)≤C0⋅ϱ,\|\sqrt{-1}\partial\bar{\partial}\phi_{1}\|_{C^{0,\alpha}(\mathcal{M}_{T})}\leq C_{0}\cdot\varrho\quad\text{and}\quad\|\sqrt{-1}\partial\bar{\partial}\phi_{2}\|_{C^{0,\alpha}(\mathcal{M}_{T})}\leq C_{0}\cdot\varrho,

where C0>0C_{0}>0 is a uniform constant independent of T≫1T\gg 1.

Since the L∞L^{\infty}-norm of the Kähler form ωT\omega_{T} is bounded by a uniform constant (independent of T≫1T\gg 1), so the above estimates imply the pointwise estimate for 𝒩\mathscr{N},

(6.39) |𝒩⁡(−1​∂∂¯​ϕ1)−𝒩⁡(−1​∂∂¯​ϕ2)|≤CN⋅ϱ⋅|−1​∂∂¯​(ϕ1−ϕ2)|,|\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{1})-\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{2})|\leq C_{N}\cdot\varrho\cdot|\sqrt{-1}\partial\bar{\partial}(\phi_{1}-\phi_{2})|,

where CN>0C_{N}>0 is a uniform constant independent of TT. Write the above in terms of the weighted norms, we have

(6.40) ‖𝒩⁡(−1​∂∂¯​ϕ1)−𝒩⁡(−1​∂∂¯​ϕ2)‖Cδ,ν+2,μ0,α​(ℳT)≤CN⋅ϱ⋅‖−1​∂∂¯​(ϕ1−ϕ2)‖Cδ,ν+2,μ0,α​(ℳT).\|\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{1})-\mathscr{N}(\sqrt{-1}\partial\bar{\partial}\phi_{2})\|_{C_{\delta,\nu+2,\mu}^{0,\alpha}(\mathcal{M}_{T})}\leq C_{N}\cdot\varrho\cdot\|\sqrt{-1}\partial\bar{\partial}(\phi_{1}-\phi_{2})\|_{C_{\delta,\nu+2,\mu}^{0,\alpha}(\mathcal{M}_{T})}.

The proof is done.

∎

To apply the implicit function theorem, we still need to prove the weighted linear estimate, which will be completed in the following subsections.

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