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4.1. Separation of variables on the model space [03H6]

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4.1. Separation of variables on the model space

We work with a Calabi model space π’ž\mathcal{C} with a smooth divisor DD defined as in Section 3. The Calabi metric is given by

(4.3) Ο‰π’ž=nn+1β€‹βˆ’1β€‹βˆ‚βˆ‚Β―β€‹(βˆ’log⁑|ΞΎ|h2)n+1n,\omega_{\mathcal{C}}=\frac{n}{n+1}\sqrt{-1}\partial\bar{\partial}(-\log|\xi|_{h}^{2})^{\frac{n+1}{n}},

which is well-defined for |ΞΎ|h<1|\xi|_{h}<1. In order to carry out separation of variables, we will study the local representation of the Laplace operator Ξ”π’ž\Delta_{\mathcal{C}} on π’ž\mathcal{C}.

We choose local holomorphic coordinates zΒ―={zi}i=1nβˆ’1\underline{z}=\{z_{i}\}_{i=1}^{n-1} on the smooth divisor DD, and fix a local holomorphic trivialization e0e_{0} of the line bundle LL with |e0|2=eβˆ’Οˆ|e_{0}|^{2}=e^{-\psi}, where ψ:D→ℝ\psi:D\to\mathbb{R} is a smooth function. So we get local holomorphic coordinates (zΒ―,w)≑(z1,…,znβˆ’1,w)(\underline{z},w)\equiv(z_{1},\ldots,z_{n-1},w) on π’ž\mathcal{C} by writing a point ΞΎβˆˆπ’ž\xi\in\mathcal{C} as ΞΎ=w​e0​(zΒ―)\xi=we_{0}(\underline{z}). Then |ΞΎ|h2=|w|2​eβˆ’Οˆ|\xi|_{h}^{2}=|w|^{2}e^{-\psi}. We may assume ψ⁑(0)=1\psi(0)=1, dβ€‹Οˆβ€‹(0)=0d\psi(0)=0 and βˆ’1β€‹βˆ‚βˆ‚Β―β€‹Οˆ=Ο‰0\sqrt{-1}\partial\bar{\partial}\psi=\omega_{0}. Let Ο€:π’žβ†’D\pi:\mathcal{C}\rightarrow D be the obvious projection map. Then we obtain

(4.4) Ο‰π’ž=(βˆ’log⁑|ΞΎ|h2)1n​ωD+1n​(βˆ’log⁑|ΞΎ|h2)1nβˆ’1β€‹βˆ’1​(d​wwβˆ’βˆ‚Οˆ)∧(d​wΒ―wΒ―βˆ’βˆ‚Β―β€‹Οˆ).\omega_{\mathcal{C}}=(-\log|\xi|^{2}_{h})^{\frac{1}{n}}\omega_{D}+\frac{1}{n}(-\log|\xi|_{h}^{2})^{\frac{1}{n}-1}\sqrt{-1}(\frac{dw}{w}-\partial\psi)\wedge(\frac{d\bar{w}}{\bar{w}}-\bar{\partial}\psi).

Let uu be a C2C^{2}-function in the Calabi space π’ž\mathcal{C}, the Laplacian at points in the fiber Ο€βˆ’1​(0)\pi^{-1}(0) is given by

(4.5) Ξ”π’žβ€‹u=(βˆ’log⁑|ΞΎ|h2)βˆ’1nβ€‹βˆ‘i=1nβˆ’1βˆ‚2uβˆ‚ziβ€‹βˆ‚zΒ―i+n​(βˆ’log⁑|ΞΎ|h2)βˆ’1n+1​|w|2β€‹βˆ‚2uβˆ‚wβ€‹βˆ‚wΒ―.\Delta_{\mathcal{C}}u=(-\log|\xi|^{2}_{h})^{-\frac{1}{n}}\sum_{i=1}^{n-1}\frac{\partial^{2}u}{\partial z_{i}\partial\bar{z}_{i}}+n(-\log|\xi|_{h}^{2})^{-\frac{1}{n}+1}|w|^{2}\frac{\partial^{2}u}{\partial w\partial\bar{w}}.

Now denote ϱ≑|ΞΎ|h\varrho\equiv|\xi|_{h}, then we can write

(4.6) w=ϱ​eψ2+βˆ’1​θ,w=\varrho e^{\frac{\psi}{2}+\sqrt{-1}\theta},

where βˆ‚ΞΈ\partial_{\theta} generates the natural S1S^{1}-rotation on the total space of LL. Then it is straightforward to check that

(4.7) βˆ‚Ο±βˆ‚w=Ο±2​w,βˆ‚ΞΈβˆ‚w=12β€‹βˆ’1​w,βˆ‚Ο±βˆ‚zi=βˆ’12Ο±βˆ‚ziψ,βˆ‚ΞΈβˆ‚zi=0\frac{\partial\varrho}{\partial w}=\frac{\varrho}{2w},\ \frac{\partial\theta}{\partial w}=\frac{1}{2\sqrt{-1}w},\frac{\partial\varrho}{\partial z_{i}}=-\frac{1}{2}\varrho\partial_{z_{i}}\psi,\frac{\partial\theta}{\partial z_{i}}=0

and

(4.8) |w|2β€‹βˆ‚2βˆ‚wβ€‹βˆ‚w¯​u=14​(Ο±2​uϱ​ϱ+ϱ​uΟ±+uθ​θ).|w|^{2}\frac{\partial^{2}}{\partial w\partial\bar{w}}u=\frac{1}{4}(\varrho^{2}u_{\varrho\varrho}+\varrho u_{\varrho}+u_{\theta\theta}).

For fixed r0∈(0,1)r_{0}\in(0,1), the level set Y2​nβˆ’1≑{Ο±=r0}Y^{2n-1}\equiv\{\varrho=r_{0}\} is equipped with the induced Riemannian metric given by

(4.9) h0=(βˆ’log⁑r02)1n​gD+1n​(βˆ’log⁑r02)1nβˆ’1​r02​(dβ€‹ΞΈβˆ’12​dcβ€‹Οˆ)βŠ—(dβ€‹ΞΈβˆ’12​dcβ€‹Οˆ).h_{0}=(-\log r_{0}^{2})^{\frac{1}{n}}g_{D}+\frac{1}{n}(-\log r_{0}^{2})^{\frac{1}{n}-1}r_{0}^{2}(d\theta-\frac{1}{2}d^{c}\psi)\otimes(d\theta-\frac{1}{2}d^{c}\psi).

Now we consider a smooth function Ο•βˆˆCβˆžβ€‹(Y2​nβˆ’1)\phi\in C^{\infty}(Y^{2n-1}) with

(4.10) β„’βˆ‚ΞΈβ€‹Ο•=βˆ’1​j​ϕ\mathcal{L}_{\partial_{\theta}}\phi=\sqrt{-1}j\phi

for some integer jj. Replacing Ο•\phi by ϕ¯\bar{\phi} if necessary we may assume jβ‰₯0j\geq 0. Then Ο•\phi is induced by a smooth section Ο•^\hat{\phi} of (Lβˆ—)βŠ—j(L^{*})^{\otimes j}. Precisely, if we locally write Ο•^​(zΒ―)=Φ⁑(zΒ―)​(e0​(zΒ―)βˆ—)βŠ—j\hat{\phi}(\underline{z})=\Phi(\underline{z})(e_{0}(\underline{z})^{*})^{\otimes j}, then

(4.11) ϕ⁑(zΒ―,w)=wj​Φ​(zΒ―)|Ο±=r0=r0j​ej⁑(ψ2+βˆ’1​θ)​Φ​(zΒ―).\phi(\underline{z},w)=w^{j}\Phi(\underline{z})|_{\varrho=r_{0}}=r_{0}^{j}e^{j(\frac{\psi}{2}+\sqrt{-1}\theta)}\Phi(\underline{z}).

Now let Ο•^\hat{\phi} be a non-zero eigen-section of the βˆ‚Β―\bar{\partial}-Laplace operator, i.e.

(4.12) Ξ”βˆ‚Β―β€‹Ο•^=Ξ»^​ϕ^.\Delta_{\bar{\partial}}\hat{\phi}=\hat{\lambda}\hat{\phi}.

By Kodaira-Nakano formula Ξ”βˆ‚Β―=Ξ”βˆ‚+j⁑(nβˆ’1)\Delta_{\bar{\partial}}=\Delta_{\partial}+j(n-1), so we have Ξ»^β‰₯j⁑(nβˆ’1)\hat{\lambda}\geq j(n-1). By a direct calculation, we get that on Ο€βˆ’1​(0)\pi^{-1}(0),

(4.13) βˆ‘i=1nβˆ’1βˆ‚2Ο•βˆ‚ziβ€‹βˆ‚zΒ―i=(βˆ’Ξ»^+j⁑(nβˆ’1)2)​ϕ.\sum_{i=1}^{n-1}\frac{\partial^{2}\phi}{\partial z_{i}\partial\bar{z}_{i}}=\Big(-\hat{\lambda}+\frac{j(n-1)}{2}\Big)\phi.

Moreover, by the local expression of h0h_{0} as in (4.9), one can directly check that on Ο€βˆ’1​(0)∩Y2​nβˆ’1\pi^{-1}(0)\cap Y^{2n-1},

(4.14) Ξ”h0​ϕ=(βˆ’log⁑r02)βˆ’1nβ€‹βˆ‘iβˆ‚2Ο•βˆ‚ziβ€‹βˆ‚zΒ―i+n​(βˆ’log⁑r02)βˆ’1n+1​r0βˆ’2​ϕθ​θ=((βˆ’log⁑r02)βˆ’1n​(βˆ’Ξ»^+j⁑(nβˆ’1)2)βˆ’j2​n​(βˆ’log⁑r02)βˆ’1n+1​r0βˆ’2)​ϕ.\displaystyle\begin{split}\Delta_{h_{0}}\phi&=(-\log r_{0}^{2})^{-\frac{1}{n}}\sum_{i}\frac{\partial^{2}\phi}{\partial z_{i}\partial\bar{z}_{i}}+n(-\log r_{0}^{2})^{-\frac{1}{n}+1}r_{0}^{-2}\phi_{\theta\theta}\\ &=\Big((-\log r_{0}^{2})^{-\frac{1}{n}}(-\hat{\lambda}+\frac{j(n-1)}{2})-j^{2}n(-\log r_{0}^{2})^{-\frac{1}{n}+1}r_{0}^{-2}\Big)\phi.\end{split}

Now suppose a smooth function u⁑(Ο±,z)u(\varrho,z) on the Calabi space π’ž\mathcal{C} is of the form u≑f⁑(Ο±)​ϕ​(y)u\equiv f(\varrho)\phi(y), where Ο•\phi is a function on Y2​nβˆ’1Y^{2n-1} satisfying (4.10) and (4.13). In polar coordinates, we obtain

Ξ”π’žβ€‹u\displaystyle\Delta_{\mathcal{C}}u =ϕ⁑(y)β‹…((βˆ’log⁑ϱ2)βˆ’1n​((βˆ’Ξ»^+j⁑(nβˆ’1)2)​fβˆ’nβˆ’12​ϱ​fΟ±)CLOSE\displaystyle=\phi(y)\cdot\Big((-\log\varrho^{2})^{-\frac{1}{n}}((-\hat{\lambda}+\frac{j(n-1)}{2})f-\frac{n-1}{2}{\varrho}f_{\varrho})
OPEN+n4​(βˆ’log⁑ϱ2)1βˆ’1n​(Ο±2​fϱ​ϱ+ϱ​fΟ±βˆ’j2​f))\displaystyle\ \ \ \ +\frac{n}{4}(-\log{\varrho}^{2})^{1-\frac{1}{n}}({\varrho}^{2}f_{{\varrho}{\varrho}}+{\varrho}f_{\varrho}-j^{2}f)\Big)
=ϕ⁑(y)β‹…(βˆ’log⁑ϱ2)βˆ’1n​(n4​(βˆ’log⁑ϱ2)​(Ο±2​fϱ​ϱ+ϱ​fΟ±βˆ’j2​f)CLOSE\displaystyle=\phi(y)\cdot(-\log\varrho^{2})^{-\frac{1}{n}}\Big(\frac{n}{4}(-\log{\varrho}^{2})({\varrho}^{2}f_{{\varrho}{\varrho}}+{\varrho}f_{\varrho}-j^{2}f)
(4.15) OPENβˆ’nβˆ’12​ϱ​fΟ±βˆ’(Ξ»^βˆ’j⁑(nβˆ’1)2)​f).\displaystyle\ \ \ \ -\frac{n-1}{2}{\varrho}f_{\varrho}-(\hat{\lambda}-\frac{j(n-1)}{2})f\Big).

Notice this formula is now independent of the choice of local holomorphic coordinates. So uu is harmonic if and only if

(4.16) n4​(βˆ’log⁑ϱ2)​(Ο±2​fϱ​ϱ+ϱ​fΟ±βˆ’j2​f)βˆ’nβˆ’12​ϱ​fΟ±βˆ’(Ξ»^βˆ’j⁑(nβˆ’1)2)​f=0.\frac{n}{4}(-\log{\varrho}^{2})(\varrho^{2}f_{{\varrho}{\varrho}}+\varrho f_{\varrho}-j^{2}f)-\frac{n-1}{2}{\varrho}f_{\varrho}-(\hat{\lambda}-\frac{j(n-1)}{2})f=0.

Denote z=(βˆ’log⁑ϱ2)1nz=(-\log\varrho^{2})^{\frac{1}{n}}, then we get

(4.17) fz​zβˆ’(n⁑(Ξ»^βˆ’j⁑(nβˆ’1)2)+j2​n24​zn)​znβˆ’2​f=0.f_{zz}-(n(\hat{\lambda}-\frac{j(n-1)}{2})+\frac{j^{2}n^{2}}{4}z^{n})z^{n-2}f=0.

In this section, we will also analyze the Poisson equation

(4.18) Ξ”π’žβ€‹u=v.\Delta_{\mathcal{C}}u=v.

Suppose now v≑΢⁑(Ο±)⋅ϕ⁑(y)v\equiv\zeta(\varrho)\cdot\phi(y), then the same separation of variables gives the following ODE

(4.19) fz​zβˆ’(n⁑(Ξ»^βˆ’j⁑(nβˆ’1)2)+j2​n24​zn)​znβˆ’2​f=znβˆ’1β‹…ΞΆ.f_{zz}-(n(\hat{\lambda}-\frac{j(n-1)}{2})+\frac{j^{2}n^{2}}{4}z^{n})z^{n-2}f=z^{n-1}\cdot\zeta.

We remark that a similar separation of variables was carried out in [KK10], but we will need stronger estimates on solutions in order to prove Theorem 4.3.

For our application we focus on the case n=2n=2. So the corresponding ODEs become

(4.20) fz​zβˆ’(Ξ»+j2​z2)​f=0f_{zz}-(\lambda+j^{2}z^{2})f=0

and

(4.21) fz​zβˆ’(Ξ»+j2​z2)​f=zβ‹…ΞΆ,f_{zz}-(\lambda+j^{2}z^{2})f=z\cdot\zeta,

where

(4.22) λ≑2​λ^βˆ’jβ‰₯j.\lambda\equiv 2\hat{\lambda}-j\geq j.

We have assumed jβ‰₯0j\geq 0 in the above discussion, but notice that the Laplace operator is a real operator, so the ODEs we get for jj and βˆ’j-j are the same. Denote z0≑(βˆ’log⁑r02)12z_{0}\equiv(-\log r_{0}^{2})^{\frac{1}{2}}, then we notice that each eigenvalue of Ξ”h0\Delta_{h_{0}} can be represented by

(4.23) Ξ›=Ξ»2​z0+2​z0β‹…j2r02.\Lambda=\frac{\lambda}{2z_{0}}+\frac{2z_{0}\cdot j^{2}}{r_{0}^{2}}.

With the above computations, we are ready to set up the ODE system. Now we fix some r0∈(0,1)r_{0}\in(0,1), and define (Y3,h0)(Y^{3},h_{0}) to be the level set {r=r0}\{r=r_{0}\} endowed with the induced Riemannian metric h0h_{0}. The above computations tell us that the eigenvalues of Y3Y^{3} is given by linear combinations of Ξ»^\hat{\lambda} and jj. Below we will parametrize our summation in terms of eigenvalues of (Y3,h0)(Y^{3},h_{0}) (counted with multiplicity), but we shall keep in mind that we have further split the eigenspaces of Ξ”h0\Delta_{h_{0}} according to the S1S^{1} action hence an eigenvalue is naturally written in terms of a linear combination of Ξ»^\hat{\lambda} and jj.

We denote by {Ξ›k}k=1∞\{\Lambda_{k}\}_{k=1}^{\infty} the spectrum of Ξ”h0\Delta_{h_{0}} and let {Ο†k}k=1∞\{\varphi_{k}\}_{k=1}^{\infty} be the eigenfunctions which are homogeneous under the S1S^{1} action and with

(4.24) βˆ’Ξ”h0​φk=Ξ›kβ‹…Ο†k.-\Delta_{h_{0}}\varphi_{k}=\Lambda_{k}\cdot\varphi_{k}.

In the above notations, one can compute that in the case n=2n=2,

(4.25) Ξ›k=Ξ»k2​z0+2​z0β‹…jk2r02.\Lambda_{k}=\frac{\lambda_{k}}{2z_{0}}+\frac{2z_{0}\cdot j_{k}^{2}}{r_{0}^{2}}.

First, we carry out separation of variables for harmonic functions on Ξ”π’ž\Delta_{\mathcal{C}}. Let uu be a harmonic function on the model space π’ž\mathcal{C}, namely,

(4.26) Ξ”π’žβ€‹u=0\Delta_{\mathcal{C}}u=0

For every fixed zz, we can write the L2L^{2}-expansion along the fiber Y3Y^{3},

(4.27) u⁑(z,π’š)=βˆ‘k=1∞uk​(z)β‹…Ο†k​(π’š).u(z,\bm{y})=\sum\limits_{k=1}^{\infty}u_{k}(z)\cdot\varphi_{k}(\bm{y}).

The above computations tell us that for each kβˆˆβ„€+k\in\mathbb{Z}_{+}, there are numbers jkβˆˆβ„•j_{k}\in\mathbb{N} and Ξ»kβ‰₯n​jk\lambda_{k}\geq nj_{k} such that the function uk​(z)u_{k}(z) satisfies the differential equation

(4.28) d2​uk​(z)d​z2βˆ’(jk2​z2+Ξ»k)​uk​(z)=0,zβ‰₯1.\frac{d^{2}u_{k}(z)}{dz^{2}}-(j_{k}^{2}z^{2}+\lambda_{k})u_{k}(z)=0,\ z\geq 1.

We also consider the Poisson equation

(4.29) Ξ”π’žβ€‹u=v.\Delta_{\mathcal{C}}u=v.

Take the L2L^{2}-expansion of vv in the direction of the cross section Y3Y^{3},

(4.30) v⁑(z,π’š)=βˆ‘k=1∞ξk​(z)β‹…Ο†k​(π’š),v(z,\bm{y})=\sum\limits_{k=1}^{\infty}\xi_{k}(z)\cdot\varphi_{k}(\bm{y}),

then the same procedure of separation of variables leads to a differential equation

(4.31) d2​uk​(z)d​z2βˆ’(jk2​z2+Ξ»k)​uk​(z)=ΞΎk​(z)β‹…z.\frac{d^{2}u_{k}(z)}{dz^{2}}-(j_{k}^{2}z^{2}+\lambda_{k})u_{k}(z)=\xi_{k}(z)\cdot z.

We end this subsection by giving a model example of the fiber Y3Y^{3}.

Example 4.4 (The spectrum of a Heisenberg manifold).

In our interested context, Y3Y^{3} is a Heisenberg nilpotent manifold. We consider a simple example that Y3≑H⁑(1,β„€)βˆ–H⁑(1,ℝ)Y^{3}\equiv H(1,\mathbb{Z})\setminus H(1,\mathbb{R}) with

(4.32) H(1,ℝ)≑{[1xt01y001]:x,y,tβˆˆβ„}.H(1,\mathbb{R})\equiv\left\{\begin{bmatrix}1&x&t\\ 0&1&y\\ 0&0&1\end{bmatrix}:\ x,y,t\in\mathbb{R}\right\}.

and

(4.33) H(1,β„€)≑{[1mp01n001]:m,n,pβˆˆβ„€}.H(1,\mathbb{Z})\equiv\left\{\begin{bmatrix}1&m&p\\ 0&1&n\\ 0&0&1\end{bmatrix}:\ m,n,p\in\mathbb{Z}\right\}.

In this case, Y3Y^{3} is a Heisenberg manifold of degree 11. As a 𝕋2\mathbb{T}^{2} bundle over S1S^{1}, its monodromy is given by (1101)∈SL⁑(2,β„€)(\begin{smallmatrix}1&1\\ 0&1\end{smallmatrix})\in\SL(2,\mathbb{Z}). So it is standard that the spectrum consists of two classes of eigenvalues

(4.34) 𝔗≑{4Ο€2(k2+β„“2)|k,β„“βˆˆβ„€}and𝔖≑{2Ο€|m|(2h+1+2Ο€|m|)|mβˆˆβ„€βˆ–{0},hβˆˆβ„•}.\mathfrak{T}\equiv\Big\{4\pi^{2}(k^{2}+\ell^{2})\Big|k,\ell\in\mathbb{Z}\Big\}\ and\ \mathfrak{S}\equiv\Big\{2\pi|m|(2h+1+2\pi|m|)\Big|m\in\mathbb{Z}\setminus\{0\},h\in\mathbb{N}\Big\}.

Detailed discussions can be found in [DS84] and [GW86]. So we can see that the above eigenvalues coincide with the form (4.25).

In the following subsections, we will analyze the convergence and regularity issues of the formal solutions (4.28) and (4.31).

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