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4.2.2. Kähler potentials [052B]

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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).

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