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4.2. Kähler geometry [051X]

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4.2. Kähler geometry

A key feature in the analysis in Kähler geometry is that we can describe the geometry in terms of a single potential function. This has led to a vast simplification of formulae in Kähler geometry as compared to more general Riemannian geometric setting, and it also has allowed various techniques from PDE and several complex variables, etc to be exploited.

The goal of this subsection is to derive a formulae for the Kähler potential for our Kähler manifold (ℳ,ω,Ω)(\mathcal{M},\omega,\Omega). This is one of the most crucial observations in this paper.

In Section 4.2.1 we will identify the underlying complex manifold of the family of Kähler metrics constructed in the Section 4.1 as a family of open subsets of a fixed complex manifold. In Section 4.2.2 we derive a formula for the Kähler potential.

4.2.1. The underlying complex manifold

We define the following holomorphic line bundles on DD

(4.85) L+≡L−⊗k+,L−≡L⊗k−.L_{+}\equiv L^{-\otimes k_{+}},\ L_{-}\equiv L^{\otimes k_{-}}.

Denote by 𝒩0\mathcal{N}^{0} the hypersurface in the total space of L+⊕L−L_{+}\oplus L_{-} defined by the equation

(4.86) ζ+⊗ζ−=SH​(x),\zeta_{+}\otimes\zeta_{-}=S_{H}(x),

where ζ±\zeta_{\pm} denotes points on the fibers of L±L_{\pm} over x∈Dx\in D. Since HH is smooth, 𝒩0\mathcal{N}^{0} is also smooth, and the submanifold

(4.87) ℋ≡{ζ+=ζ−=0}\mathcal{H}\equiv\{\zeta_{+}=\zeta_{-}=0\}

is naturally isomorphic to HH. The fixed hermitian metric on LL then induces hermitian metrics on L±L_{\pm}, which yields the norm functions on L±L_{\pm}:

(4.88) r±​(ζ±)≡‖ζ±‖.r_{\pm}(\zeta_{\pm})\equiv\|\zeta_{\pm}\|.

Then by the projection of 𝒩0\mathcal{N}^{0} to L±L_{\pm} we may also view r±r_{\pm} as functions on 𝒩0\mathcal{N}^{0}.

There is a natural holomorphic volume form on 𝒩0\mathcal{N}^{0} given by

(4.89) Ω𝒩0≡−12​(d​ζ+ζ+−d​ζ−ζ−)∧ΩD\Omega_{\mathcal{N}^{0}}\equiv\frac{\sqrt{-1}}{2}(\frac{d\zeta_{+}}{\zeta_{+}}-\frac{d\zeta_{-}}{\zeta_{-}})\wedge\Omega_{D}

where ΩD\Omega_{D} means the pull-back of ΩD\Omega_{D} to 𝒩0\mathcal{N}^{0} and for simplicity of notation we shall omit the pull-back notation when the meaning is clear from the context. The expression on the right hand side of (4.89) should be understood in the following sense: after choosing a local holomorphic frame σ\sigma of LL, ζ±\zeta_{\pm} becomes local holomorphic functions on L±L_{\pm}, and one can check the definition does not depend on the choice of σ\sigma. It is not hard to show using the defining equation of 𝒩0\mathcal{N}^{0} that Ω𝒩0\Omega_{\mathcal{N}^{0}} is a well-defined holomorphic volume form on 𝒩0\mathcal{N}^{0} and is nowhere vanishing.

There is a natural ℂ∗\mathbb{C}^{*} action on 𝒩0\mathcal{N}^{0} given by

(4.90) λ.(ζ+,ζ−)≡(λ−1​ζ+,λ​ζ−),λ∈ℂ∗.\lambda.(\zeta_{+},\zeta_{-})\equiv(\lambda^{-1}\zeta_{+},\lambda\zeta_{-}),\ \ \lambda\in\mathbb{C}^{*}.

and we denote by

(4.91) ξ𝒩0≡−1(−ζ+∂ζ++ζ−∂ζ−)\xi_{\mathcal{N}^{0}}\equiv\sqrt{-1}(-\zeta_{+}\partial_{\zeta_{+}}+\zeta_{-}\partial_{\zeta_{-}})

the corresponding holomorphic vector field (the choice of coefficients is made so that the real part of ξ𝒩0\xi_{\mathcal{N}^{0}} is twice the real vector field generated by the induced S1S^{1} action, as in (4.84)). One checks that

(4.92) ξ𝒩0​⌟​Ω𝒩0=ΩD\xi_{\mathcal{N}^{0}}\lrcorner\ \Omega_{\mathcal{N}^{0}}=\Omega_{D}
Proposition 4.8.

There is a holomorphic embedding Φ:(ℳ,Ω)→𝒩0\Phi:(\mathcal{M},\Omega)\rightarrow\mathcal{N}^{0} as a relatively compact open subset containing 𝒫\mathcal{P}, such that the following holds

  1. (1)

    Φ\Phi commutes with the projection maps to DD.

  2. (2)

    Φ∗​Ω𝒩0=Ω.\Phi^{*}\Omega_{\mathcal{N}^{0}}=\Omega.

  3. (3)

    d​Φ​(ξ1,0)=ξ𝒩01,0d\Phi(\xi^{1,0})=\xi^{1,0}_{\mathcal{N}^{0}}. In particular, Φ\Phi maps 𝒫\mathcal{P} isomorphically onto ℋ\mathcal{H}.

Remark 4.8.1.

From this we can say DD is indeed the GIT quotient of 𝒩0\mathcal{N}_{0}, and we have a variation of GIT that leads to the birational map between L+−1L_{+}^{-1} and L−L_{-}.

Proof.

We define

(4.93) {ℳ−≡ℳ∗∖π−1​(H×[0,∞))ℳ+≡ℳ∗∖π−1​(H×(∞,0]).\begin{cases}\mathcal{M}_{-}\equiv{\mathcal{M}^{*}}\setminus\pi^{-1}(H\times[0,\infty))\\ \mathcal{M}_{+}\equiv{\mathcal{M}^{*}}\setminus\pi^{-1}(H\times(\infty,0]).\end{cases}

On ℳ−\mathcal{M}_{-} we can trivialize the U⁡(1)U(1) connection −−1​Θ-\sqrt{-1}\Theta along the zz direction so that the zz component Θz\Theta_{z} vanishes identically. Denote by Θ|z\Theta|_{z} the restriction of Θ\Theta to the slice D×{z}D\times\{z\} for z<0z<0 and to (D∖H)×{z}(D\setminus H)\times\{z\} for z≥0z\geq 0. From (4.33) we see that that curvature form of −−1​Θ|z-\sqrt{-1}\Theta|_{z} is given by −−1∂zω~-\sqrt{-1}\partial_{z}\tilde{\omega}.

By Section 3.4, we have

(4.94) ∂zω~|z=T−=k−​ωD+ϵT\partial_{z}\tilde{\omega}|_{z=T_{-}}=k_{-}\omega_{D}+\epsilon_{T}

and

(4.95) [∂zω~]|z=T−=k−​[ωD]∈H2​(D,ℝ).[\partial_{z}\tilde{\omega}]|_{z=T_{-}}=k_{-}[\omega_{D}]\in H^{2}(D;\mathbb{R}).

Since b1​(D)=0b_{1}(D)=0, we may assume ℳ|z=T−\mathcal{M}|_{z=T_{-}} embeds into L−L_{-}, as the unit circle bundle defined by another hermitian metric ∥⋅∥∼2\|\cdot\|_{\sim}^{2} which differs from the fixed metric by ϵT\epsilon_{T}, and the connection 1-form −−1​Θ|T−-\sqrt{-1}\Theta|_{T_{-}} agrees with the restriction of the Chern connection form. Denote by r~−\tilde{r}_{-} the norm function on L−L_{-} corresponding to the new hermitian metric, then we have

(4.96) log⁡r~−=log⁡r−+ϵT\log\tilde{r}_{-}=\log r_{-}+\epsilon_{T}

Furthermore, we may extend −−1​Θ|T−-\sqrt{-1}\Theta|_{T_{-}} naturally to the complement of the zero section 𝟎L−{\bf 0}_{L_{-}} in L−L_{-}, via the fiberwise projection, and the resulting 1-form coincides with −1​r~−−1​J−​d​r~−\sqrt{-1}\tilde{r}_{-}^{-1}J_{-}d\tilde{r}_{-}, where J−J_{-} denotes the complex structure on L−L_{-}.

Now we define a map Φ−:ℳ∗−→L−∖𝟎L−\Phi_{-}:{\mathcal{M}^{*}}_{-}\rightarrow L_{-}\setminus{\bf 0}_{L_{-}} where 𝟎L−{\bf 0}_{L_{-}} denotes the zero section in L−L_{-}. First at z=T−z=T_{-} we define Φ−\Phi_{-} to be the natural inclusion map as above, multiplied by eA−e^{A_{-}} for some constant A−A_{-} to be determined later. Then using the trivialization of the U⁡(1)U(1) bundle ℳ∗−{\mathcal{M}^{*}}_{-} along the zz direction and the natural scaling map on L−L_{-}, we extend the map to the whole ℳ∗−{\mathcal{M}^{*}}_{-} by setting

(4.97) r~−=eA−−∫T−zh⁡(u)​𝑑u\tilde{r}_{-}=e^{A_{-}-\int_{T_{-}}^{z}h(u)du}

Then Φ−\Phi_{-} clearly commutes with the projection maps to DD, so Φ−∗​α=α\Phi_{-}^{*}\alpha=\alpha for any 11-form α\alpha which is a pull-back from DD. Since

(4.98) ∂zΘ|z=dDc​h=−JD​dD​h\partial_{z}\Theta|_{z}=d_{D}^{c}h=-J_{D}d_{D}h

we have

(4.99) r~−−1​Φ−∗​d​r~−=−h​𝑑z−∫T−z𝑑u∧dD​h=−h​𝑑z−JD​(Θ|z−Θ|T−),\tilde{r}_{-}^{-1}\Phi_{-}^{*}d\tilde{r}_{-}=-hdz-\int_{T_{-}}^{z}du\wedge d_{D}h=-hdz-J_{D}(\Theta|_{z}-\Theta|_{T_{-}}),

noticing that Θ|z−Θ|T−\Theta|_{z}-\Theta|_{T_{-}} is a 1-form pulled-back from DD. So

(4.100) r~−−1​Φ−∗​(d​r~−+−1​J−​d​r~−)=−h​d​z−−1​Θ|z−−1​(Θ|T−−Θ|z)−JD​(Θ|z−ΘT−)\tilde{r}_{-}^{-1}\Phi_{-}^{*}(d\tilde{r}_{-}+\sqrt{-1}J_{-}d\tilde{r}_{-})=-hdz-\sqrt{-1}\Theta|_{z}-\sqrt{-1}(\Theta|_{T_{-}}-\Theta|_{z})-J_{D}(\Theta|_{z}-\Theta_{T_{-}})

is a (1,0)(1,0) form on ℳ∗−{\mathcal{M}^{*}}_{-}.

Notice by definition locally

(4.101) r~−2=|ζ−|2⋅‖σ‖∼2\tilde{r}_{-}^{2}=|\zeta_{-}|^{2}\cdot\|\sigma\|_{\sim}^{2}

so

(4.102) d​ζ−ζ−=d​r~−r~−+−1​J−​d​r~−r~−+∂Dlog⁡|σ|2\frac{d\zeta_{-}}{\zeta_{-}}=\frac{d\tilde{r}_{-}}{\tilde{r}_{-}}+\sqrt{-1}J_{-}\frac{d\tilde{r}_{-}}{\tilde{r}_{-}}+\partial_{D}\log|\sigma|^{2}

Therefore we obtain

(4.103) Φ−∗​ΩL−=Ω\Phi_{-}^{*}\Omega_{L_{-}}=\Omega

where

(4.104) ΩL−≡−−1​d​ζ−ζ−∧ΩD\Omega_{L_{-}}\equiv-\sqrt{-1}\frac{d\zeta_{-}}{\zeta_{-}}\wedge\Omega_{D}

is a natural holomorphic volume form on L−∖𝟎L−L_{-}\setminus{\bf 0}_{L_{-}}. In particular Φ−\Phi_{-} is a holomorphic embedding. Also, we have

(4.105) dΦ−(ξ1,0)=−1ζ−∂ζ−d\Phi_{-}(\xi^{1,0})=\sqrt{-1}\zeta_{-}\partial_{\zeta_{-}}

is the natural holomorphic vector field on L−L_{-}.

Since hh is positive we see that the image of Φ−\Phi_{-} is bounded in L−L_{-}. Since ℳ∖ℳ−\mathcal{M}\setminus\mathcal{M}_{-} is of complex codimension one, by the removable singularity theorem for bounded holomorphic functions, Φ−\Phi_{-} extends to a holomorphic map on the entire ℳ\mathcal{M}.

Similarly we get a holomorphic embedding

(4.106) Φ+:ℳ+→L+\Phi_{+}:\mathcal{M}_{+}\rightarrow L_{+}

with

(4.107) r~+=eA+−∫zT+h⁡(u)​𝑑u\tilde{r}_{+}=e^{A_{+}-\int_{z}^{T_{+}}h(u)du}

for a constant A+A_{+} to be determined. Again Φ+\Phi_{+} extends to a holomorphic map on ℳ\mathcal{M}.

Together we obtain

(4.108) Φ≡(Φ+,Φ−):ℳ→L+⊕L−\Phi\equiv(\Phi_{+},\Phi_{-}):\mathcal{M}\rightarrow L_{+}\oplus L_{-}

which is an embedding on ℳ∖𝒫\mathcal{M}\setminus\mathcal{P}. It commutes with projections maps to DD and satisfies

(4.109) dΦ(ξ1,0)=−1(ζ−∂ζ−−ζ+∂ζ+).d\Phi(\xi^{1,0})=\sqrt{-1}(\zeta_{-}\partial_{\zeta_{-}}-\zeta_{+}\partial_{\zeta_{+}}).

Now we show that with appropriate choice of A±A_{\pm}, Φ\Phi maps ℳ\mathcal{M} into 𝒩0\mathcal{N}^{0}. First we notice that by (4.109),

(4.110) detΦ≡Φ+⊗Φ−:ℳ∖(H×(−∞,∞))→L+⊗L−\det\Phi\equiv\Phi_{+}\otimes\Phi_{-}:\mathcal{M}\setminus(H\times(-\infty,\infty))\rightarrow L_{+}\otimes L_{-}

has image lying on a non-zero holomorphic section, say S~\tilde{S}, of L⊗k=L+⊗L−L^{\otimes k}=L_{+}\otimes L_{-} over D∖HD\setminus H. By definition since hh is positive we know the the image of Φ\Phi is bounded in L+⊕L−L_{+}\oplus L_{-}, with respect to the norm r~±\tilde{r}_{\pm}, so S~\tilde{S} is a bounded section of L⊗kL^{\otimes k} with respect to the norm r~≡r~+⊗r~−\tilde{r}\equiv\tilde{r}_{+}\otimes\tilde{r}_{-}, hence again by removable singularity theorem for bounded holomorphic functions it extends to a holomorphic section on the entire DD. By our assumption that [H][H] is isomorphic to LL, we see HH is exactly the zero locus of S~\tilde{S}, so there is a constant CC such that

(4.111) S~=C⋅SH.\tilde{S}=C\cdot S_{H}.

Multiplying Φ−\Phi_{-} by an element in S1S^{1} we may assume CC is a positive real number. Now

(4.112) log⁡C=1∫DωDn−1​∫log⁡‖S~​‖ωDn−1−1∫DωDn−1​∫log‖​SH‖​ωDn−1\log C=\frac{1}{\int_{D}\omega_{D}^{n-1}}\int\log\|{\tilde{S}}\|\omega_{D}^{n-1}-\frac{1}{\int_{D}\omega_{D}^{n-1}}\int\log\|S_{H}\|\omega_{D}^{n-1}

The second term is a constant independent of TT. For the first term, by definition we have

(4.113) −log⁡‖S~‖=∫T−T+h​𝑑z−(A−+A+)+ϵT.-\log\|\tilde{S}\|=\int_{T_{-}}^{T_{+}}hdz-(A_{-}+A_{+})+\epsilon_{T}.

By (4.14)

(4.114) ∫T−T+∫h​ωDn−1\displaystyle\int_{T_{-}}^{T_{+}}\int h\omega_{D}^{n-1} =\displaystyle= ∫T−T+T2−n​∫D(T​ωD+ψ)n−1​𝑑z+T−1​B¯T\displaystyle\int_{T_{-}}^{T_{+}}T^{2-n}\int_{D}(T\omega_{D}+\psi)^{n-1}dz+T^{-1}\underline{B}_{T}
(4.115) =\displaystyle= 1n​∫DωDn−1​(1k−−1k+)​(T2−1)+T−1​B¯T\displaystyle\frac{1}{n}\int_{D}\omega_{D}^{n-1}(\frac{1}{k_{-}}-\frac{1}{k_{+}})(T^{2}-1)+T^{-1}\underline{B}_{T}

So we get that

(4.116) −log⁡C=1n​(1k−−1k+)​(T2−1)−(A−+A+)+1∫DωDn−1​∫log⁡‖SH‖+T−1​B¯T-\log C=\frac{1}{n}(\frac{1}{k_{-}}-\frac{1}{k_{+}})(T^{2}-1)-(A_{-}+A_{+})+\frac{1}{\int_{D}\omega_{D}^{n-1}}\int\log\|S_{H}\|+T^{-1}\underline{B}_{T}

Setting C=1C=1 gives one condition on A−A_{-} and A+A_{+}. For our later purposes we shall need additionally that

(4.117) k−​A−=k+​A+k_{-}A_{-}=k_{+}A_{+}

Together these determine A−A_{-} and A+A_{+} as

(4.118) A−≡1n​k−​(T2−1)−−k+2​(k−−k+)​1∫DωDn−1​∫log⁡‖SH‖+T−1​B¯TA_{-}\equiv\frac{1}{nk_{-}}(T^{2}-1)-\frac{-k_{+}}{2(k_{-}-k_{+})}\frac{1}{\int_{D}\omega_{D}^{n-1}}\int\log\|S_{H}\|+T^{-1}\underline{B}_{T}
(4.119) A+≡1−n​k+​(T2−1)−k−2​(k−−k+)​1∫DωDn−1​∫log⁡‖SH‖+T−1​B¯TA_{+}\equiv\frac{1}{-nk_{+}}(T^{2}-1)-\frac{k_{-}}{2(k_{-}-k_{+})}\frac{1}{\int_{D}\omega_{D}^{n-1}}\int\log\|S_{H}\|+T^{-1}\underline{B}_{T}

Then we can make Φ\Phi maps ℳ\mathcal{M} into 𝒩0\mathcal{N}^{0}.

It is easy to check that Φ\Phi satisfies (1), (2), (3) in the statement of the Proposition. It then follows from (2) that Φ\Phi is a holomorphic embedding also across 𝒫\mathcal{P}. This finishes the proof of Proposition.

∎

Remark 4.8.2.

In the case b1​(D)≠0b_{1}(D)\neq 0, from the proof we can make the same conclusion except the holomorphic line bundles L+L_{+} and L−L_{-} can not be prescribed as isomorphic to the powers on the given holomorphic line bundle LL. Instead, as can be seen in the above proof, they are determined by the restriction of ∂zω~​(z)\partial_{z}\tilde{\omega}(z) on the two ends. However, as pointed in Remark 4.3.2, we always have L+=L−⊗k+⊗ℱL_{+}=L^{-\otimes k_{+}}\otimes\mathcal{F} and L−=L⊗k−⊗ℱ−1L_{-}=L^{\otimes k_{-}}\otimes\mathcal{F}^{-1} for some holomorphic line bundle ℱ\mathcal{F} on DD with c1​(ℱ)=0c_{1}(\mathcal{F})=0. In particular the tensor product L+⊗L−L_{+}\otimes L_{-} is always isomorphic to LkL^{k}. The freedom of ℱ\mathcal{F} corresponds exactly to the choice of the connection 1-form Θ\Theta in the construction of ℳ∗\mathcal{M}^{*}.

For our purpose later, we list a few more results here. First we shall need to compare the function zz with the norm r−r_{-} and r+r_{+} near each end. Given C>0C>0 fixed, then by (4.16) we have

(4.120) {−logr−=1n​k−T2−n(T+k−z)n−A−+ϵT+ϵ(z),z≤−C;−logr+=−1n​k+T2−n(T+k+z)n−A++ϵT+ϵ(z),z≥C.\begin{cases}-\log r_{-}=\frac{1}{nk_{-}}T^{2-n}(T+k_{-}z)^{n}-A_{-}+\epsilon_{T}+\epsilon(z),\ \ z\leq-C;\\ -\log r_{+}=-\frac{1}{nk_{+}}T^{2-n}(T+k_{+}z)^{n}-A_{+}+\epsilon_{T}+\epsilon(z),\ \ z\geq C.\end{cases}

by noticing that for example

(4.121) ∫T−zϵ⁡(z)​𝑑z=ϵT+ϵ⁡(z),z≤−C.\int_{T_{-}}^{z}\epsilon(z)dz=\epsilon_{T}+\epsilon(z),z\leq-C.

So we have

(4.122) {(T+k−​z)n=Tn−2​n​k−​(A−−log⁡r−+ϵT+ϵ⁡(z))(T+k+​z)n=−Tn−2​n​k+​(A+−log⁡r−+ϵT+ϵ⁡(z))\begin{cases}(T+k_{-}z)^{n}=T^{n-2}nk_{-}(A_{-}-\log r_{-}+\epsilon_{T}+\epsilon(z))\\ (T+k_{+}z)^{n}=-T^{n-2}nk_{+}(A_{+}-\log r_{-}+\epsilon_{T}+\epsilon(z))\end{cases}

For our analysis later we also give a description of the behavior of the metric ω\omega when we restrict to the region |z|≥1|z|\geq 1. From the asymptotics of ω~\tilde{\omega} and hh we know the metric is asymptotic to the Calabi model space in Section 2.2. Locally on DD we fix holomorphic coordinates {w1,⋯,wn−1}\{w_{1},\cdots,w_{n-1}\} and choose a holomorphic trivialization of LL as before, then we obtain fiber holomorphic coordinates ζ±\zeta_{\pm} on L±L_{\pm}. Denote

(4.123) ω±,c​y​l≡∑i≥1−1​d​wi∧d​w¯i+−1​d​ζ±∧d​ζ¯±|ζ±|2\omega_{\pm,cyl}\equiv\sum_{i\geq 1}\sqrt{-1}dw_{i}\wedge d\bar{w}_{i}+\frac{\sqrt{-1}d\zeta_{\pm}\wedge d\bar{\zeta}_{\pm}}{|\zeta_{\pm}|^{2}}

the local cylindrical type metrics on L±L_{\pm} respectively. Then we have

Lemma 4.9.

On |z|≥1|z|\geq 1, we have

(4.124) C−1​T(n−2)​(1−n)n​(T+k±​z)1−n​ω±,c​y​l≤ω≤C​T2−nn​(T+k±​z)⋅ω±,c​y​lC^{-1}T^{\frac{(n-2)(1-n)}{n}}(T+k_{\pm}z)^{1-n}\omega_{\pm,cyl}\leq\omega\leq CT^{\frac{2-n}{n}}(T+k_{\pm}z)\cdot\omega_{\pm,cyl}

and for all k≥1k\geq 1, there exists mk,Ckm_{k},C_{k} such that

(4.125) |∇ω±,c​y​lkω|ω±,c​y​l≤Ck​(T2−nn​(T+k±​z))mk.|\nabla^{k}_{\omega_{\pm,cyl}}\omega|_{\omega_{\pm,cyl}}\leq C_{k}(T^{\frac{2-n}{n}}(T+k_{\pm}z))^{m_{k}}.
Proof.

Consider the case z≤−1z\leq-1. Since

(4.126) d​ζ−ζ−=d​r−r−+−1​J​d​r−r−=−h​d​z+ϵT−−1​J​h​d​z\frac{d\zeta_{-}}{\zeta_{-}}=\frac{dr_{-}}{r_{-}}+\sqrt{-1}J\frac{dr_{-}}{r_{-}}=-hdz+\epsilon_{T}-\sqrt{-1}Jhdz

The result then easily follows from the asymptotics of hh (4.16) and ω~\tilde{\omega} (3.349). ∎

Finally we need to understand the boundary of the shape of the level set r±=Cr_{\pm}=C under the projection to D×ℝD\times\mathbb{R}, for a fixed C>0C>0 and for TT large. First we have the formula

Lemma 4.10.

We have

(4.127) A−−∫T−0h⁡(u)​𝑑u=12​log⁡‖SH‖+BTA_{-}-\int_{T_{-}}^{0}h(u)du=\frac{1}{2}\log{\|S_{H}\|}+B_{T}
(4.128) A++∫T+0h⁡(u)​𝑑u=12​log⁡‖SH‖+BTA_{+}+\int_{T_{+}}^{0}h(u)du=\frac{1}{2}\log{\|S_{H}\|}+B_{T}
Proof.

We denote

(4.129) h^−=A−−∫T−0h⁡(u)​𝑑u−12​log⁡‖SH‖.\hat{h}_{-}=A_{-}-\int_{T_{-}}^{0}h(u)du-\frac{1}{2}\log\|S_{H}\|.

By the Poincaré-Lelong equation we have

(4.130) dD​dDc​log⁡‖SH‖2=4​π​δH−(k−−k+)​ωD,d_{D}d_{D}^{c}\log{\|S_{H}\|}^{2}=4\pi\delta_{H}-(k_{-}-k_{+})\omega_{D},

where δH\delta_{H} denotes the current of integration along HH. By directly taking derivatives and use (2.13) we obtain that outside HH,

(4.131) dDdDc(∫0T−h(z)dz)=∫0T−dDdDch(z)dz=∫0T−−∂z2ω~(z)dz=−∂zω~|z=T−+∂zω~|z=0d_{D}d_{D}^{c}(\int_{0}^{T_{-}}h(z)dz)=\int_{0}^{T_{-}}d_{D}d_{D}^{c}h(z)dz=\int_{0}^{T_{-}}-\partial_{z}^{2}\tilde{\omega}(z)dz=-\partial_{z}\tilde{\omega}|_{z=T_{-}}+\partial_{z}\tilde{\omega}|_{z=0}

By (3.349) and (3.381), the right hand side is given by −12​(k−−k+)​ωD+ϵT-\frac{1}{2}(k_{-}-k_{+})\omega_{D}+\epsilon_{T}. Now using the asymptotics of hh near PP in (4.17), one sees that h^−\hat{h}_{-} is bounded near HH. So the following current equation holds globally on DD

(4.132) dD​dDc​h^−=ϵTd_{D}d_{D}^{c}\hat{h}_{-}=\epsilon_{T}

Now

(4.133) ∫Dh^−​ωDn−1=A−​∫DωDn−1+∫D∫0T−h​ωDn−1​𝑑z=BT\int_{D}\hat{h}_{-}\omega_{D}^{n-1}=A_{-}\int_{D}\omega_{D}^{n-1}+\int_{D}\int_{0}^{T_{-}}h\omega_{D}^{n-1}dz=B_{T}

So by standard elliptic regularity we get the conclusion for h^−\hat{h}_{-}. The proof for the other equation is similar. ∎

Since for |z|≤1|z|\leq 1 we have h⁡(z)=T+12​r+O′​(r)+O⁡(T−1)h(z)=T+\frac{1}{2r}+O^{\prime}(r)+O(T^{-1}), we easily see that in a fixed distance (with respect to ωD\omega_{D}) away from HH, r±≤Cr_{\pm}\leq C is equivalent to BT⋅T−1∓z≥0B_{T}\cdot T^{-1}\mp z\geq 0. Now we fix a point in HH and as before consider the coordinate chart (y,y¯,w2′,⋯,w¯n−1′)(y,\bar{y},w_{2}^{\prime},\cdots,\bar{w}_{n-1}^{\prime}) on DD centered at this point. Then we have

Proposition 4.11.

In this chart we have

(4.134) log⁡r−\displaystyle\log r_{-} =−T​z+12​log⁡(r−z)+BT,\displaystyle=-Tz+\frac{1}{2}\log(r-z)+B_{T},
(4.135) log⁡r+\displaystyle\log r_{+} =T​z+12​log⁡(r+z)+BT.\displaystyle=Tz+\frac{1}{2}\log(r+z)+B_{T}.
Proof.

By the previous Lemma,

(4.136) A−−∫T−zh⁡(u)=12​log⁡‖SH‖+BT+∫z0h⁡(u)​𝑑uA_{-}-\int_{T_{-}}^{z}h(u)=\frac{1}{2}\log{\|S_{H}\|}+B_{T}+\int_{z}^{0}h(u)du

When |z|≤1|z|\leq 1, if we are in the above chart, then

(4.137) ∫0zh⁡(u)​𝑑u=BT+T​z+12​(log⁡(r+z)−log⁡|y|)\int_{0}^{z}h(u)du=B_{T}+Tz+\frac{1}{2}(\log(r+z)-\log|y|)

Since log⁡‖SH‖=log⁡|y|+BT\log{\|S_{H}\|}=\log|y|+B_{T}, it follows that

(4.138) log⁡r−=BT−T​z+12​log⁡(r−z)\log r_{-}=B_{T}-Tz+\frac{1}{2}\log(r-z)

Similarly we get the estimate for log⁡r+\log r_{+}.

∎

Corollary 4.11.1.

The following hold:

  1. (1)

    Let C>0C>0 be fixed, then for TT large, r−≤Cr_{-}\leq C implies z≥−34​T−1​log⁡Tz\geq-\frac{3}{4}T^{-1}\log T.

  2. (2)

    Let c>0c>0 be fixed. Then for TT large if r≤c​T−1​log⁡Tr\leq cT^{-1}\log T for some c<1/2c<1/2, then

    log⁡r−≤−12​(12−c)​log⁡T.\log r_{-}\leq-\frac{1}{2}(\frac{1}{2}-c)\log T.
  3. (3)

    Let C≥1C\geq 1 be fixed, then for TT large, z≥−Cz\geq-C implies log⁡r−≤(C+1)​T\log r_{-}\leq(C+1)T

Proof.

The first two items are easy consequences of the previous Lemma. For the last item we simply notice that for C≥1C\geq 1,

(4.139) ∫−C−1h⁡(u)​𝑑u=∫−C−1(T2−n​(T+k−​u)n−1+ϵ⁡(u))​𝑑u≤C​T.\int_{-C}^{-1}h(u)du=\int_{-C}^{-1}(T^{2-n}(T+k_{-}u)^{n-1}+\epsilon(u))du\leq CT.

∎

4.2.2. Kähler potentials

We look for an S1S^{1} invariant function ϕ\phi on ℳ\mathcal{M} satisfying the equation

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

We write

(4.141) d​ϕ=dD​ϕ+ϕz​d​zd\phi=d_{D}\phi+\phi_{z}dz

where as before dD​ϕd_{D}\phi is the differential along DD direction and ϕz=∂zϕ\phi_{z}=\partial_{z}\phi is the derivative along zz direction. Then

(4.142) dc​ϕ=dDc​ϕ+ϕz​h−1​Θ,d^{c}\phi=d^{c}_{D}\phi+\phi_{z}h^{-1}\Theta,

and

(4.143) d​dc​ϕ=dD​dDc​ϕ+d​z∧(dDc​ϕz)+d⁡(ϕz​h−1)∧Θ+ϕz​h−1​(∂zω~−d​z∧dDc​h)dd^{c}\phi=d_{D}d_{D}^{c}\phi+dz\wedge(d^{c}_{D}\phi_{z})+d(\phi_{z}h^{-1})\wedge\Theta+\phi_{z}h^{-1}(\partial_{z}\tilde{\omega}-dz\wedge d_{D}^{c}h)

Since

(4.144) Tn−2n​ω=π∗​ω~+d​z∧Θ,T^{\frac{n-2}{n}}\omega=\pi^{*}\tilde{\omega}+dz\wedge\Theta,

we see (4.140) is equivalent to the system of equations

(4.145) {ω~=T​ωD+dD​dDc​ϕ+ϕz​h−1​∂zω~dDc​ϕz−ϕz​h−1​dDc​h=0d⁡(ϕz​h−1)=d​z.\begin{cases}\tilde{\omega}=T\omega_{D}+d_{D}d^{c}_{D}\phi+\phi_{z}h^{-1}\partial_{z}\tilde{\omega}\\ d_{D}^{c}\phi_{z}-\phi_{z}h^{-1}d_{D}^{c}h=0\\ d(\phi_{z}h^{-1})=dz.\end{cases}

To solve these (apparently overdetermined) equations, we first notice that the last equation in (4.145) is equivalent to

(4.146) ϕz​h−1=z+C\phi_{z}h^{-1}=z+C

for a constant CC. So we obtain 22 2 In the case when n=2n=2 for the classical Gibbons-Hawking ansatz this formula was derived by the authors together with Hans-Joachim Hein in the office of the first author at Stony Brook in the Fall of 2017.

(4.147) ϕ⁡(z)=∫z0z(u+C)​h​𝑑u+ϕ⁡(z0)\phi(z)=\int_{z_{0}}^{z}(u+C)hdu+\phi(z_{0})

for a function ϕ⁡(z0)\phi(z_{0}) on DD.

The second equation of (4.145) then holds automatically, and the first equation also follows after taking ∂z\partial_{z}. So in order for ϕ\phi defined in (4.147) to satisfy (4.145), it suffices that at a fixed z=T+z=T_{+} the following holds

(4.148) T​ωD+dD​dDc​ϕ=ω~−(T++C)​∂zω~T\omega_{D}+d_{D}d^{c}_{D}\phi=\tilde{\omega}-(T_{+}+C)\partial_{z}\tilde{\omega}

Comparing the cohomology class of both sides yields that CC must be zero. Then we can solve ϕ⁡(T+)\phi(T_{+}) uniquely up to addition of a constant. After fixing a choice of ϕ⁡(T+)\phi(T_{+}) we may define ϕ\phi by

(4.149) ϕ⁡(z)=∫T+zu​h​𝑑u+ϕ⁡(T+)\phi(z)=\int_{T_{+}}^{z}uhdu+\phi(T_{+})

and we can view it as either a function on QTQ_{T} or an S1S^{1} invariant function on ℳ\mathcal{M}.

Proposition 4.12.

The function ϕ\phi is smooth on ℳ∗{\mathcal{M}^{*}}, and C3,αC^{3,\alpha} on ℳ\mathcal{M} (in the smooth topology as defined in Section 4.1), and satisfies (4.140).

Remark 4.12.1.

The regularity is indeed C4,αC^{4,\alpha} in local holomorphic coordinates.

Proof.

By definition ϕ\phi is smooth on QT∖H×(−∞,0]Q_{T}\setminus H\times(-\infty,0]. Using (4.17) it is easy to see that ϕ\phi extends to a continuous function on QTQ_{T}. Hence for all fixed zz, the following equation holds in the sense of currents on DD

(4.150) T​ωD+dD​dDc​ϕ​(z)=ω~​(z)−z​∂zω~​(z).T\omega_{D}+d_{D}d_{D}^{c}\phi(z)=\tilde{\omega}(z)-z\partial_{z}\tilde{\omega}(z).

Elliptic regularity then implies that ϕ\phi is smooth on each slice {z}×D\{z\}\times D for z≠0z\neq 0. Now for z≤0z\leq 0 we can write

(4.151) ϕ⁡(z)=∫T−zu​h​𝑑u+ϕ⁡(T−).\phi(z)=\int_{T_{-}}^{z}uhdu+\phi(T_{-}).

We then see that ϕ\phi is indeed smooth on QT∖PQ_{T}\setminus P. Over the S1S^{1} fibration ℳ\mathcal{M}, we know ϕ\phi is globally continuous, and it is smooth and satisfies the equation (4.140) on ℳ∗{\mathcal{M}^{*}}. Now again by standard theory on pluri-subharmonic functions we conclude the current equation holds on ℳ\mathcal{M}. Since we know ω\omega is C2,αC^{2,\alpha} in local holomorphic coordinates on ℳ\mathcal{M}, elliptic regularity gives that ϕ\phi is in C4,αC^{4,\alpha} in local holomorphic coordinates. This implies that ϕ\phi is C3,αC^{3,\alpha} in the smooth topology we defined, since we know the holomorphic coordinate functions are C3,αC^{3,\alpha}. ∎

Remark 4.12.2.

As a by-product we can also recover the formula of the Calabi model metric in terms of Kähler potentials as mentioned in Section 2.2. In this case as in (2.30) we take ω~=z​ωD\tilde{\omega}=z\omega_{D} and h=zn−1h=z^{n-1}. Then we can write

(4.152) ω~=d​dc​ϕ\tilde{\omega}=dd^{c}\phi

with

(4.153) ϕ=∫0zun​𝑑u=1n+1​zn+1\phi=\int_{0}^{z}u^{n}du=\frac{1}{n+1}z^{n+1}

To match with the formula for Calabi ansatz in (2.32), we notice that zn+1=(−log⁡|ξ|)2z^{n+1}=(-\log|\xi|)^{2}, and there is a factor of n2\frac{n}{2} due to the normalization of the Calabi-Yau equation and that d​dc=2​−1​∂∂¯dd^{c}=2\sqrt{-1}\partial\bar{\partial}.

Remark 4.12.3.

Notice the argument above does not essentially require the compactness of DD, except to solve the equation (4.150) on one slice. Using similar idea can get the expression of the Taub-NUT metric on ℂ2\mathbb{C}^{2} in terms of Kähler potentials, as mentioned in Section 2.3. Here we take DD to be ℂ\mathbb{C} with the standard flat structure, and

(4.154) ω~​(z)=−12​V​d​y∧d​y¯;h=V,\tilde{\omega}(z)=\frac{\sqrt{-1}}{2}Vdy\wedge d\bar{y};\ \ \ \ h=V,

with

(4.155) V=12​r+T.V=\frac{1}{2r}+T.

Suppose we want to find ϕ\phi with

(4.156) ω=d​dc​ϕ,\omega=dd^{c}\phi,

then we first have

(4.157) ϕ⁡(z)−ϕ⁡(0)=∫0z(12​r+T)​𝑑u=12​r−12​|y|+T2​z2\phi(z)-\phi(0)=\int_{0}^{z}(\frac{1}{2r}+T)du=\frac{1}{2}r-\frac{1}{2}|y|+\frac{T}{2}z^{2}

The equation (4.150) for z=0z=0 becomes

(4.158) 4​∂y∂y¯ϕ⁡(0)=ω~​(0)=12​|y|+T4\partial_{y}\partial_{\bar{y}}\phi(0)=\tilde{\omega}(0)=\frac{1}{2|y|}+T

and a solution is given by

(4.159) ϕ⁡(0)=12​|y|+T4​|y|2\phi(0)=\frac{1}{2}|y|+\frac{T}{4}|y|^{2}

So we get

(4.160) ϕ=12​r+T2​z2+T4​|y|2.\phi=\frac{1}{2}r+\frac{T}{2}z^{2}+\frac{T}{4}|y|^{2}.

In terms of the u1,u2u_{1},u_{2} coordinates we get

(4.161) ϕ=14​(|u1|2+|u2|2)+T8​(|u1|4+|u2|4).\phi=\frac{1}{4}(|u_{1}|^{2}+|u_{2}|^{2})+\frac{T}{8}(|u_{1}|^{4}+|u_{2}|^{4}).

This agrees with formula (7.61) up to a constant 22, again caused by the fact that d​dc=2​−1​∂∂¯dd^{c}=2\sqrt{-1}\partial\bar{\partial}.

Notice from the above discussion we know for each fixed zz, ϕ⁡(z)\phi(z) is uniquely determined up to a constant on DD by the equation

(4.162) T​ωD+dD​dDc​ϕ​(z)=ω~​(z)−z​∂zω~​(z),T\omega_{D}+d_{D}d^{c}_{D}\phi(z)=\tilde{\omega}(z)-z\partial_{z}\tilde{\omega}(z),

and the integration formula (4.149) exactly gives a coherent way of fixing all the constants for each zz, so the overall freedom in only up to a global constant. 33 3 maybe more geometric explanation if we have time

Notice by (3.349) we have for z≫1z\gg 1,

(4.163) ω~​(z)−z​∂zω~​(z)−T​ωD=ψ⁡(z)−z​∂zψ⁡(z)=ϵ⁡(z)\tilde{\omega}(z)-z\partial_{z}\tilde{\omega}(z)-T\omega_{D}=\psi(z)-z\partial_{z}\psi(z)=\epsilon(z)

Standard elliptic estimate allows us to find a solution ϕ⁡(T+)\phi(T_{+}) which is ϵT\epsilon_{T}. By (4.16) we obtain that for z≥Cz\geq C

(4.164) ϕ⁡(z)=C++T2−n​k+−2​[(k+​z+T)n+1n+1−T​(k+​z+T)nn]\phi(z)=C_{+}+T^{2-n}k_{+}^{-2}[\frac{(k_{+}z+T)^{n+1}}{n+1}-\frac{T(k_{+}z+T)^{n}}{n}]

where

(4.165) C+=ϵT+ϵ⁡(z)−T2−n​k+−2​[1n+1​T(n+1)​(n−2)n−1n​Tn−2]C_{+}=\epsilon_{T}+\epsilon(z)-T^{2-n}k_{+}^{-2}[\frac{1}{n+1}T^{\frac{(n+1)(n-2)}{n}}-\frac{1}{n}T^{n-2}]

For the other end z≤−Cz\leq-C, similarly we have

(4.166) ϕ⁡(z)−ϕ⁡(T−)=C−+T2−n​k−−2​[(k−​z+T)n+1n+1−T​(k−​z+T)nn]\phi(z)-\phi(T_{-})=C_{-}+T^{2-n}k_{-}^{-2}[\frac{(k_{-}z+T)^{n+1}}{n+1}-\frac{T(k_{-}z+T)^{n}}{n}]

where

(4.167) C−=ϵT+ϵ⁡(z)+T2−n​k−−2​[1n+1​T(n+1)​(n−2)n−1n​Tn−2]C_{-}=\epsilon_{T}+\epsilon(z)+T^{2-n}k_{-}^{-2}[\frac{1}{n+1}T^{\frac{(n+1)(n-2)}{n}}-\frac{1}{n}T^{n-2}]

To understand ϕ⁡(T−)\phi(T_{-}) we need the following

Lemma 4.13.

We have

(4.168) ϕ⁡(T−)=ϵT+T−1​B¯T\phi(T_{-})=\epsilon_{T}+T^{-1}\underline{B}_{T}
Proof.

We have ϕ⁡(T−)=ϕ⁡(T+)−Ψ,\phi(T_{-})=\phi(T_{+})-\Psi, where

(4.169) Ψ=∫T−T+z​h​𝑑z.\Psi=\int_{T_{-}}^{T_{+}}zhdz.

Away from HH we have

(4.170) dDdDcΨ=∫T−T+zdDdDchdz=−∫T−T+z∂z2ω~dzd_{D}d_{D}^{c}\Psi=\int_{T_{-}}^{T_{+}}zd_{D}d_{D}^{c}hdz=-\int_{T_{-}}^{T_{+}}z\partial_{z}^{2}\tilde{\omega}dz

Integration by parts we get

(4.171) dDdDcΨ=(−z∂zω~+ω~)|T−T+=ϵTd_{D}d_{D}^{c}\Psi=(-z\partial_{z}\tilde{\omega}+\tilde{\omega})|^{T_{+}}_{T_{-}}=\epsilon_{T}

Notice since there is a factor zz in the integrand we do not get residue term at z=0z=0. Notice Ψ\Psi is continuous on DD, and the right hand side is smooth on DD, so elliptic regularity implies that Ψ\Psi is indeed smooth on DD, and the equation holds globally on DD.

On the other hand, we have

(4.172) ∫DΨ​ωDn−1=∫T−T+z​∫Dh​ωDn−1​𝑑z\int_{D}\Psi\omega_{D}^{n-1}=\int_{T_{-}}^{T_{+}}z\int_{D}h\omega_{D}^{n-1}dz

Using (4.14)

∫DΨ​ωDn−1∫DωDn−1=\displaystyle\frac{\int_{D}\Psi\omega_{D}^{n-1}}{\int_{D}\omega_{D}^{n-1}}= T2−n​k+−2​[(k+​z+T)n+1n+1−T​(k+​z+T)nn]\displaystyle T^{2-n}k_{+}^{-2}[\frac{(k_{+}z+T)^{n+1}}{n+1}-\frac{T(k_{+}z+T)^{n}}{n}]
(4.173) −T2−n​k−−2​[(k−​z+T)n+1n+1−T​(k−​z+T)nn]+T−1​B¯T,\displaystyle-T^{2-n}k_{-}^{-2}[\frac{(k_{-}z+T)^{n+1}}{n+1}-\frac{T(k_{-}z+T)^{n}}{n}]+T^{-1}\underline{B}_{T},

where we used the definition of T−T_{-} and T+T_{+}. (4.171) and (4.173) together yield the conclusion. ∎

Now we investigate (4.166).

(4.174) ϕ⁡(z)−ϕ⁡(T−)=C−+T2−n​k−−2​[(k−​z+T)n+1n+1−T​(k−​z+T)nn]+ϵT+O⁡(T−1)\phi(z)-\phi(T_{-})=C_{-}+T^{2-n}k_{-}^{-2}[\frac{(k_{-}z+T)^{n+1}}{n+1}-\frac{T(k_{-}z+T)^{n}}{n}]+\epsilon_{T}+O(T^{-1})

We first notice that by (4.120)

(4.175) −T3−n​k−−2​(k−​z+T)nn=Tk−​(log⁡r−−A−+ϵT+ϵ⁡(z))+ϵT-T^{3-n}k_{-}^{-2}\frac{(k_{-}z+T)^{n}}{n}=\frac{T}{k_{-}}(\log r_{-}-A_{-}+\epsilon_{T}+\epsilon(z))+\epsilon_{T}

We may also write by definition

(4.176) ωD=−1k−​d​dc​log⁡r−\omega_{D}=-\frac{1}{k_{-}}dd^{c}\log r_{-}

So when z≤−Cz\leq-C, we have

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

with

(4.178) ϕ−≡1n+1​nn+1n​k−−n−1n​(A−+ϵT+ϵ⁡(z)−log⁡r−)n+1n−T2n​k−−1​A−+ϵT+T2n​ϵ​(z)\phi_{-}\equiv\frac{1}{n+1}n^{\frac{n+1}{n}}k_{-}^{-\frac{n-1}{n}}(A_{-}+\epsilon_{T}+\epsilon(z)-\log r_{-})^{\frac{n+1}{n}}-T^{\frac{2}{n}}k_{-}^{-1}A_{-}+\epsilon_{T}+T^{\frac{2}{n}}\epsilon(z)

Similarly for z≥Cz\geq C, we have

(4.179) T​π∗​ωD+d​dc​ϕ=d​dc​ϕ+,T\pi^{*}\omega_{D}+dd^{c}\phi=dd^{c}\phi_{+},

with

(4.180) ϕ+≡1n+1​nn+1n​(−k+)−n−1n​(A++ϵT+ϵ⁡(z)−log⁡r+)n+1n−T2n​k+−1​A++ϵT+T2n​ϵ​(z).\phi_{+}\equiv\frac{1}{n+1}n^{\frac{n+1}{n}}(-k_{+})^{-\frac{n-1}{n}}(A_{+}+\epsilon_{T}+\epsilon(z)-\log r_{+})^{\frac{n+1}{n}}-T^{\frac{2}{n}}k_{+}^{-1}A_{+}+\epsilon_{T}+T^{\frac{2}{n}}\epsilon(z).

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