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6. Construction of the approximate hyperkähler triple [03IH]

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6. Construction of the approximate hyperkähler triple

In this section, we will obtain a closed manifold ℳ\mathcal{M} by gluing two pieces of hyperkähler Tian-Yau spaces with a neck region which satisfies appropriate topological balancing condition, such that ℳ\mathcal{M} has the same homological invariants as the K3⁡3\K 3 surface (see Proposition 6.6). Moreover, we will construct a closed definite triple 𝝎ℳ\bm{\omega}^{\mathcal{M}} on ℳ\mathcal{M} which is very close to an SU⁡(2){\rm{SU}}(2)-structure. This will be perturbed to a hyperkähler triple 𝝎HK\bm{\omega}^{\HK} in Section 9.

First, we briefly describe the geometry of the Tian-Yau spaces (Xb−4,gb−)(X_{b_{-}}^{4},g_{b_{-}}) and (Xb+4,gb+)(X_{b_{+}}^{4},g_{b_{+}}) for fixed b±∈{1,…,9}b_{\pm}\in\{1,\ldots,9\}. Denote by Nilb±3\Nil^{3}_{b_{\pm}} the Heisenberg nilpotent 33-manifolds with deg⁡(Nilb±3)=b±\deg(\Nil^{3}_{b_{\pm}})=b_{\pm}. It follows from Proposition 3.1 and Corollary 3.6 that there exists a coordinate system on the end of the Tian-Yau spaces (Xb±4,gb±)(X_{b_{\pm}}^{4},g_{b_{\pm}})

(6.1) Φ±T​Y:[ζ0±,∞)×Nilb±3→Xb±4,\displaystyle\Phi^{TY}_{\pm}:[\zeta_{0}^{\pm},\infty)\times\Nil^{3}_{b_{\pm}}\rightarrow X_{b_{\pm}}^{4},

such that

(6.2) (Φ±T​Y)∗​gb±\displaystyle(\Phi^{TY}_{\pm})^{*}g_{b_{\pm}} =V±​(g𝕋2+d​z±2)+V±−1​θb±2+O⁡(e−δ¯±​z±),\displaystyle=V_{\pm}(g_{\mathbb{T}^{2}}+dz_{\pm}^{2})+V_{\pm}^{-1}\theta_{b_{\pm}}^{2}+O(e^{-\underline{\delta}_{\pm}z_{\pm}}),

as z±→∞z_{\pm}\to\infty, and the area of each 22-torus fiber 𝕋2\mathbb{T}^{2} is A−A_{-} and A+A_{+} respectively. Moreover, the harmonic potential V±V_{\pm} admits the expansion in coordinates

(6.3) V±=2​πA±​b±​z±+c±,V_{\pm}=\frac{2\pi}{A_{\pm}}b_{\pm}z_{\pm}+c_{\pm},

as z±→∞z_{\pm}\to\infty, and θb±\theta_{b_{\pm}} is the fixed connection 11-form on the model space satisfying

(6.4) d​θb±=2​π​b±A±​dvol𝕋2.d\theta_{b_{\pm}}=\frac{2\pi b_{\pm}}{A_{\pm}}\dvol_{\mathbb{T}^{2}}.

From now on, we rescale the above Tian-Yau metrics such that the above 22-tori have the common area AA, which we assume satisfies 12≤A≤1\frac{1}{2}\leq A\leq 1. We are free to make the following assumptions

(6.5) c±\displaystyle c_{\pm} =0,\displaystyle=0,
(6.6) θb±\displaystyle\theta_{b_{\pm}} =2​π​b±A​(d​t−x​d​y).\displaystyle=\frac{2\pi b_{\pm}}{A}(dt-xdy).

The normalization (6.5) can be arranged by applying a translation in the z±z_{\pm} coordinates (since b±≠0b_{\pm}\neq 0 by assumption). The normalization (6.6) can be arranged using the discussion of gauge transformations given in Section 2.

Notice that, we have fixed a scale of the space such that the slope of the above linear functions are uniquely determined. In our gluing construction, for fixed parameters T−>0T_{-}>0 and T+>0T_{+}>0, we choose the cutoff region in Xb±4X_{b_{\pm}}^{4},

(6.7) Xb−4​(T−)\displaystyle X_{b_{-}}^{4}(T_{-}) ≡Xb−4∖((T−,+∞)×Nilb−3)\displaystyle\equiv X_{b_{-}}^{4}\setminus\Big((T_{-},+\infty)\times\Nil_{b_{-}}^{3}\Big)
(6.8) Xb+4​(T−)\displaystyle X_{b_{+}}^{4}(T_{-}) ≡Xb+4∖((T+,+∞)×Nilb+3).\displaystyle\equiv X_{b_{+}}^{4}\setminus\Big((T_{+},+\infty)\times\Nil_{b_{+}}^{3}\Big).

6.1. The neck region: a doubly periodic analogue of the Ooguri-Vafa metric

Given m0∈ℤ+m_{0}\in\mathbb{Z}_{+}, the neck region (𝒩m04,gG​H)(\mathcal{N}_{m_{0}}^{4},g_{GH}) is obtained from a Gibbons-Hawking space based on 𝕋2×ℝ\mathbb{T}^{2}\times\mathbb{R} with m0m_{0} monopole points. The Gibbons-Hawking metric is determined by a harmonic function on 𝕋2×ℝ\mathbb{T}^{2}\times\mathbb{R}. Notice that, the topology of K3⁡3\K 3 requires

(6.9) m0=b−+b+.m_{0}=b_{-}+b_{+}.

Consider the flat cylinder (𝕋2×ℝ,g0)(\mathbb{T}^{2}\times\mathbb{R},g_{0}) and denote by 𝒫m0≡{p1,…,pm0}⊂𝕋2×ℝ\mathcal{P}_{m_{0}}\equiv\{p_{1},\ldots,p_{m_{0}}\}\subset\mathbb{T}^{2}\times\mathbb{R} a finite set of monopoles, let V∞V_{\infty} be the Green’s function from Corollary 2.7, which satisfies

(6.10) −Δg0​V∞=2​π​∑m=1m0δpm.-\Delta_{g_{0}}V_{\infty}=2\pi\sum\limits_{m=1}^{m_{0}}\delta_{p_{m}}.

In the gluing procedure, we need to modify the above Green’s function V∞V_{\infty} such that the metric on the neck matches up with the metric of the Tian-Yau parts. For this purpose, we analyze the asymptotic behavior of V∞V_{\infty} at the two ends of the neck region. By Corollary 2.7, there are bounded harmonic functions h+h_{+} and h−h_{-} on 𝕋2×ℝ\mathbb{T}^{2}\times\mathbb{R} such that

(6.11) V∞​(z)={π⁡(b−+b+)A​z+β−+h−,z≪−1,−π⁡(b−+b+)A​z+β++h+,z≫1,\displaystyle V_{\infty}(z)=\begin{cases}\frac{\pi(b_{-}+b_{+})}{A}z+\beta_{-}+h_{-},&z\ll-1,\\ -\frac{\pi(b_{-}+b_{+})}{A}z+\beta_{+}+h_{+},&z\gg 1,\end{cases}

and h±h_{\pm} satisfy the asymptotic behavior h±​(𝒙)=O⁡(e−ϵ0​|z⁡(𝒙)|)h_{\pm}(\bm{x})=O(e^{-\epsilon_{0}|z(\bm{x})|}).

For fixed β>0\beta>0, we define a new harmonic function on 𝕋2×ℝ\mathbb{T}^{2}\times\mathbb{R},

(6.12) Vβ​(z)≡V∞​(z)+k​z+βV_{\beta}(z)\equiv V_{\infty}(z)+kz+\beta

such that the metric on the neck can be glued with the metric on the Tian-Yau space. First, we need to match the slopes, that is, the slope parameter kk should be chosen as

(6.13) k=π⁡(b−−b+)A.\displaystyle k=\frac{\pi(b_{-}-b_{+})}{A}.

Then near to the two ends of the neck region, the harmonic function VβV_{\beta} can be written as

(6.14) Vβ​(z)={2​π​b−A​z+β−+β+h−,z≪−1,−2​π​b+A​z+β++β+h+,z≫1.\displaystyle V_{\beta}(z)=\begin{cases}\frac{2\pi b_{-}}{A}z+\beta_{-}+\beta+h_{-},&z\ll-1,\\ -\frac{2\pi b_{+}}{A}z+\beta_{+}+\beta+h_{+},&z\gg 1.\end{cases}

Using this potential, we next define the neck metric through the Gibbons-Hawking ansatz. Letting 𝒫m0\mathcal{P}_{m_{0}} denote the set of monopole points, we note that H2​((𝕋2×ℝ)∖𝒫m0,ℤ)H^{2}((\mathbb{T}^{2}\times\mathbb{R})\setminus\mathcal{P}_{m_{0}},\mathbb{Z}) has dimension m0+1m_{0}+1 with generators being small spheres around the monopole points, and any torus of the form 𝕋2×{z′}\mathbb{T}^{2}\times\{z^{\prime}\} where z′z^{\prime} is any value of zz for which there are no monopole points. It is easy to see that the 22-form 12​π∗d​Vβ\frac{1}{2\pi}*dV_{\beta} attains integer values on these cycles, which implies that the cohomology class [12​π∗d​Vβ][\frac{1}{2\pi}*dV_{\beta}] lies in the image of the natural inclusion

(6.15) H2​((𝕋2×ℝ)∖𝒫m0,ℤ)↪H2​((𝕋2×ℝ)∖𝒫m0,ℝ).\displaystyle H^{2}((\mathbb{T}^{2}\times\mathbb{R})\setminus\mathcal{P}_{m_{0}},\mathbb{Z})\hookrightarrow H^{2}((\mathbb{T}^{2}\times\mathbb{R})\setminus\mathcal{P}_{m_{0}},\mathbb{R}).

Therefore, we let 𝒩m04\mathcal{N}_{m_{0}}^{4} be the total space of the S1S^{1}-bundle over (𝕋2×ℝ)∖𝒫m0(\mathbb{T}^{2}\times\mathbb{R})\setminus\mathcal{P}_{m_{0}} corresponding to the class [12​π∗d​Vβ][\frac{1}{2\pi}*dV_{\beta}], completed by adding finitely many points corresponding to 𝒫m0\mathcal{P}_{m_{0}}. Choose a connection 11-form θ\theta on 𝒩m0\mathcal{N}_{m_{0}} so that

(6.16) dθ=∗dVβ.\displaystyle d\theta=*dV_{\beta}.

Then applying the Gibbons-Hawking construction to VβV_{\beta}, we obtain a smooth hyperkähler triple 𝝎N\bm{\omega}^{N} over 𝒩m04\mathcal{N}_{m_{0}}^{4}, which induces an incomplete hyperkähler metric over the part in 𝕋2×ℝ\mathbb{T}^{2}\times\mathbb{R} where VβV_{\beta} is strictly positive.

For parameters T−>0T_{-}>0 and T+>0T_{+}>0, we define,

(6.17) 𝒩m04(−T−,T+)≡π−1(U∩{−T−<z<T+}),\mathcal{N}_{m_{0}}^{4}(-T_{-},T_{+})\equiv\pi^{-1}\big(U\cap\{-T_{-}<z<T_{+}\}\big),

where π:𝒩m04→U≡(𝕋2×ℝ)∖𝒫m0\pi:\mathcal{N}_{m_{0}}^{4}\rightarrow U\equiv(\mathbb{T}^{2}\times\mathbb{R})\setminus\mathcal{P}_{m_{0}} is the bundle projection.

Proposition 6.1.

There is a diffeomorphism

(6.18) Φ−N:(−T−,−T−+1,)×Nilb−3(ϵ,τ)→𝒩m04(−T−,−T−+1),\displaystyle\Phi^{N}_{-}:(-T_{-},-T_{-}+1,)\times\Nil^{3}_{b_{-}}(\epsilon,\tau)\rightarrow\mathcal{N}_{m_{0}}^{4}(-T_{-},-T_{-}+1),

which preserves the zz-coordinate, such that

(6.19) (Φ−N)∗​θ=θb−+O⁡(e−δN​T−),(\Phi^{N}_{-})^{*}\theta=\theta_{b_{-}}+O(e^{-\delta_{N}T_{-}}),

as T−→∞T_{-}\rightarrow\infty. Similarly, there is a diffeomorphism

(6.20) Φ+N:(T+−1,T+)×Nil−b+3⁡(ϵ,τ)→𝒩m04​(T+−1,T+),\displaystyle\Phi^{N}_{+}:(T_{+}-1,T_{+})\times\Nil^{3}_{-b_{+}}(\epsilon,\tau)\rightarrow\mathcal{N}_{m_{0}}^{4}(T_{+}-1,T_{+}),

which preserves the zz-coordinate, such that

(6.21) (Φ+N)∗​θ=θ−b++O⁡(e−δN​T+),(\Phi^{N}_{+})^{*}\theta=\theta_{-b_{+}}+O(e^{-\delta_{N}T_{+}}),

as T+→∞T_{+}\rightarrow\infty. Furthermore, there exist triples of 11-forms on the ends of the neck such that

(6.22) (Φ−N)∗​𝝎N−𝝎b−=d⁡(𝒂−N)\displaystyle(\Phi^{N}_{-})^{*}\bm{\omega}^{N}-\bm{\omega}_{b_{-}}=d(\bm{a}^{N}_{-})
(6.23) (Φ+N)∗​𝝎N−𝝎−b+=d⁡(𝒂+N),\displaystyle(\Phi^{N}_{+})^{*}\bm{\omega}^{N}-\bm{\omega}_{-b_{+}}=d(\bm{a}^{N}_{+}),

with

(6.24) |∇k𝒂±N|≤C​e−δN​|z|\displaystyle|\nabla^{k}\bm{a}^{N}_{\pm}|\leq Ce^{-\delta_{N}|z|}

for any integer k≥0k\geq 0 and ϵ>0\epsilon>0, where δN>0\delta_{N}>0 is a uniform constant in Proposition 3.4, 𝛚b−\bm{\omega}_{b_{-}} and 𝛚−b+\bm{\omega}_{-b_{+}} are the hyperkähler triples on the corresponding Calabi model spaces.

Proof.

We just deal with the negative end of the neck, the positive end is similar. Let

(6.25) U−={p∈(𝕋2×ℝ)∖{p1,…,pm0}|−∞<z<−T−/2}.\displaystyle U_{-}=\{p\in(\mathbb{T}^{2}\times\mathbb{R})\setminus\{p_{1},\dots,p_{m_{0}}\}\ |\ -\infty<z<-T_{-}/2\}.

Note that U−U_{-} deformation retracts to 𝕋2\mathbb{T}^{2}, so H2​(U−,ℤ)=ℤH^{2}(U_{-},\mathbb{Z})=\mathbb{Z}. The neck is a circle bundle over U=(𝕋2×ℝ)∖{p1,…,pm0}U=(\mathbb{T}^{2}\times\mathbb{R})\setminus\{p_{1},\dots,p_{m_{0}}\}, and call the restriction to U−U_{-} by 𝒩U−\mathcal{N}_{U_{-}}. Note this bundle has Euler number b−b_{-}.

Over U−U_{-} there exists another S1S^{1}-bundle explicitly identified with an open subset of the model space

(6.26) 𝒩b−=(−∞,−T−+1,)×Nilb−3(ϵ,τ),\displaystyle\mathcal{N}_{b_{-}}=(-\infty,-T_{-}+1,)\times\Nil^{3}_{b_{-}}(\epsilon,\tau),

with connection form θb−\theta_{b_{-}}, which has curvature form −2​π​b−A​d​x∧d​y-\frac{2\pi b_{-}}{A}dx\wedge dy, so this bundle also has Euler number b−b_{-}. From the exponential sheaf sequence, H1​(U−,ℰ∗)≅H2​(U−,ℤ)H^{1}(U_{-},\mathcal{E}^{*})\cong H^{2}(U_{-},\mathbb{Z}), so there exists a bundle equivalence

(6.27) H:𝒩b−→𝒩U−\displaystyle H:\mathcal{N}_{b_{-}}\rightarrow\mathcal{N}_{U_{-}}

which covers the identity map on the base, and such that the pullback bundle H∗​𝒩U−=𝒩b−H^{*}\mathcal{N}_{U_{-}}=\mathcal{N}_{b_{-}}. The 11-forms H∗​θH^{*}\theta and θb−\theta_{b_{-}} are therefore both connection forms on 𝒩b−\mathcal{N}_{b_{-}}. Note that

(6.28) d(H∗θ)=H∗dθ=H∗(∗dV)=∗dVβ,\displaystyle d(H^{*}\theta)=H^{*}d\theta=H^{*}(*dV)=*dV_{\beta},

and

(6.29) d​θb−=−2​π​b−A​d​x∧d​y.\displaystyle d\theta_{b_{-}}=-\frac{2\pi b_{-}}{A}dx\wedge dy.

From the asymptotics on VβV_{\beta} in (6.14), we have

(6.30) d⁡(H∗​θ−θb−)=O⁡(eδ′​z),\displaystyle d(H^{*}\theta-\theta_{b_{-}})=O(e^{\delta^{\prime}z}),

as z→−∞z\rightarrow-\infty. By same method from the proof of Lemma 3.7, we conclude that

(6.31) d⁡(H∗​θ−θb−)=d​a,\displaystyle d(H^{*}\theta-\theta_{b_{-}})=da,

where a=O⁡(eδ′​z)a=O(e^{\delta^{\prime}z}), as z→−∞z\to-\infty. Therefore

(6.32) d⁡(H∗​θ−θ~b−)=0\displaystyle d(H^{*}\theta-\tilde{\theta}_{b_{-}})=0

where θ~b−=θb−+a\tilde{\theta}_{b_{-}}=\theta_{b_{-}}+a. Since H∗​θH^{*}\theta and θ~b−\tilde{\theta}_{b_{-}} are two connections with the same curvature form, and since H1​(U−,ℝ)≅H1​(𝕋2,ℝ)≅ℝ⊕ℝH^{1}(U_{-},\mathbb{R})\cong H^{1}(\mathbb{T}^{2},\mathbb{R})\cong\mathbb{R}\oplus\mathbb{R}, we conclude that

(6.33) H∗​θ−θ~b−=d​f+p​d​x+q​d​y,\displaystyle H^{*}\theta-\tilde{\theta}_{b_{-}}=df+pdx+qdy,

for some function f:U−→ℝf:U_{-}\rightarrow\mathbb{R}, and constants p,q∈ℝp,q\in\mathbb{R}.

Next, there exists a gauge transformation, that is, a mapping G:𝒩b−→𝒩b−G:\mathcal{N}_{b_{-}}\rightarrow\mathcal{N}_{b_{-}}, covering the identity map, given by fiber rotation by ei​fe^{if}, so that

(6.34) G∗​H∗​θ−θ~b−=p​d​x+q​d​y.\displaystyle G^{*}H^{*}\theta-\tilde{\theta}_{b_{-}}=pdx+qdy.

Then, by the discussion in Subsection 2.2, there exists a mapping R:𝒩b−→𝒩b−R:\mathcal{N}_{b_{-}}\rightarrow\mathcal{N}_{b_{-}} which is the lift of a rotation on the torus, so that R∗​θb−=θb−−p​d​x−q​d​yR^{*}\theta_{b_{-}}=\theta_{b_{-}}-pdx-qdy. Pulling back (6.34),

(6.35) R∗​G∗​H∗​θ−R∗​θ~b−=R∗​(p​d​x+q​d​y).\displaystyle R^{*}G^{*}H^{*}\theta-R^{*}\tilde{\theta}_{b_{-}}=R^{*}(pdx+qdy).

Since RR covers a rotation on the torus, the right hand side is invariant under RR, so this can be rewritten as

(6.36) R∗​G∗​H∗​θ−θb−′=0,\displaystyle R^{*}G^{*}H^{*}\theta-\theta_{b_{-}}^{\prime}=0,

where θb−′=θb−+O⁡(eδ​z)\theta_{b_{-}}^{\prime}=\theta_{b_{-}}+O(e^{\delta z}) as z→−∞z\rightarrow-\infty. Then we define Φ−N=H∘G∘R\Phi^{N}_{-}=H\circ G\circ R. The zz coordinate is not affected because HH and GG both cover the identity map, and RR covers a rotation on the torus.

Next, it follows from (6.19) that the leading terms of the hyperkähler triple on the neck agree with the model hyperkähler triple for z≪0z\ll 0 (note we can allow VV to become negative, the triple is still defined). The same method from the proof of Lemma 3.7 then yields (6.22).

∎

6.2. The attaching maps and constraints

We next define the “attaching maps” which will be used to construct the manifold ℳ\mathcal{M}. Let

(6.37) D​Z−=Φ−T​Y​((T−,T−+1)×Nilb−3)⊂Xb−4,\displaystyle DZ_{-}=\Phi^{TY}_{-}\Big((T_{-},T_{-}+1)\times\Nil^{3}_{b_{-}}\Big)\subset X_{b_{-}}^{4},

using the above coordinates on the end of Xb−4X_{b_{-}}^{4}. Define

(6.38) Ψ−:D​Z−→𝒩m04\displaystyle\Psi_{-}:DZ_{-}\rightarrow\mathcal{N}_{m_{0}}^{4}

by Ψ−​(Φ−T​Y)−1​(z−,p)=Φ−N​(z−−2​T−,p)\Psi_{-}(\Phi^{TY}_{-})^{-1}(z_{-},p)=\Phi^{N}_{-}(z_{-}-2T_{-},p).

Simlarly, let

(6.39) D​Z+=Φ−T​Y​((T+,T++1)×Nilb+3)⊂Xb+4,\displaystyle DZ_{+}=\Phi^{TY}_{-}\Big((T_{+},T_{+}+1)\times\Nil^{3}_{b_{+}}\Big)\subset X_{b_{+}}^{4},

using the above coordinates on the end of Xb+4X_{b_{+}}^{4}. Define

(6.40) Ψ+:D​Z+→𝒩m04\displaystyle\Psi_{+}:DZ_{+}\rightarrow\mathcal{N}_{m_{0}}^{4}

be defined by Ψ+​(Φ+T​Y)−1​(z+,p)=Φ+N​(2​T+−z+,ψ⁡(p))\Psi_{+}(\Phi^{TY}_{+})^{-1}(z_{+},p)=\Phi^{N}_{+}(2T_{+}-z_{+},\psi(p)), where ψ+:Nilb+3→Nil−b+3\psi_{+}:\Nil^{3}_{b_{+}}\rightarrow\Nil^{3}_{-b_{+}} is the diffeomorphism given by

(6.41) ψ⁡(x,y,t)=(−x,−y,−t).\displaystyle\psi(x,y,t)=(-x,-y,-t).

We obtain the manifold ℳ\mathcal{M} by gluing the pieces together using the attaching maps:

(6.42) ℳ≡Xb−4​(T−+1)​⋃Ψ−𝒩m04​(−T−,T+)​⋃Ψ+Xb+4​(T++1).\mathcal{M}\equiv X_{b_{-}}^{4}(T_{-}+1)\bigcup_{\Psi_{-}}\mathcal{N}_{m_{0}}^{4}(-T_{-},T_{+})\bigcup_{\Psi_{+}}X_{b_{+}}^{4}(T_{+}+1).

The manifold ℳ\mathcal{M} carries an orientation compatible with both Tian-Yau pieces, and we will fix this orientation in the following.

Next, we want the potentials to agree up to the constant term in the damage zones after identifying the corresponding regions by the attaching maps. On D​Z−DZ_{-} we have

(6.43) Ψ−∗​Vβ\displaystyle\Psi_{-}^{*}V_{\beta} =2​πA​b−​(z−−2​T−)+β−+β\displaystyle=\frac{2\pi}{A}b_{-}(z_{-}-2T_{-})+\beta_{-}+\beta
(6.44) =2​πA​b−​z−+(−2​πA​b−​(2​T−)+β−+β),\displaystyle=\frac{2\pi}{A}b_{-}z_{-}+\Big(-\frac{2\pi}{A}b_{-}(2T_{-})+\beta_{-}+\beta\Big),

which we want to equal to the leading terms of V−V_{-}, so we must have

(6.45) 0=−2​πA​b−​(2​T−)+β−+β.\displaystyle 0=-\frac{2\pi}{A}b_{-}(2T_{-})+\beta_{-}+\beta.

Similarly, on the other damage zone D​Z+DZ_{+} we have

(6.46) Ψ+∗​Vβ\displaystyle\Psi_{+}^{*}V_{\beta} =−2​πA​b+​(2​T+−z+)+β++β\displaystyle=-\frac{2\pi}{A}b_{+}(2T_{+}-z_{+})+\beta_{+}+\beta
(6.47) =2​πA​b+​z++(−2​πA​b+​(2​T+)+β++β),\displaystyle=\frac{2\pi}{A}b_{+}z_{+}+\Big(-\frac{2\pi}{A}b_{+}(2T_{+})+\beta_{+}+\beta\Big),

which we want to equal to the leading terms of V+V_{+}, so we must have

(6.48) 0=−2​πA​b+​(2​T+)+β++β.\displaystyle 0=-\frac{2\pi}{A}b_{+}(2T_{+})+\beta_{+}+\beta.
Remark 6.2.

If both b+=0b_{+}=0 and b−=0b_{-}=0, then there is no constraint. This is the already known ALH⁡#​ALH\ALH\#\ALH gluing [CC16], so we do not need to analyze this case further.

To summarize: the gluing procedure requires

(6.49) 4​π​b±A⋅T±\displaystyle\frac{4\pi b_{\pm}}{A}\cdot T_{\pm} =β±+β.\displaystyle=\beta_{\pm}+\beta.

Immediately, the above constraints give 11 free parameter β>0\beta>0. So T−>0T_{-}>0 and T+>0T_{+}>0 are completely determined by β>0\beta>0 in the case b−>0b_{-}>0 and b+>0b_{+}>0, i.e.,

(6.50) T±\displaystyle T_{\pm} =A⁡(β+β±)4​π​b±.\displaystyle=\frac{A(\beta+\beta_{\pm})}{4\pi b_{\pm}}.
Remark 6.3.

We emphasize that we are fixing all the other gluing parameters so that only β\beta varies. We will prove some effective estimates in Section 8 and Section 9 which give uniform etimates for the linearized gluing operator ℒ\mathscr{L} (defined in Section 1.3) and for sufficiently large β≫1\beta\gg 1. We also note that the estimates are unifrom as long as other parameters vary in compact sets.

6.3. Gluing definite triples and topology of ℳ\mathcal{M}

We have hyperkähler triples

(6.51) 𝝎−≡(ω1−,ω2−,ω3−)​ on ​Xb−4,𝝎N≡(ω1N,ω2N,ω3N)​ on ​𝒩m04​(−T−,T+),𝝎+≡(ω1+,ω2+,ω3+)​ on ​Xb+4.\displaystyle\begin{split}\bm{\omega}^{-}&\equiv(\omega_{1}^{-},\omega_{2}^{-},\omega_{3}^{-})\ \mbox{ on }X_{b_{-}}^{4},\\ \bm{\omega}^{N}&\equiv(\omega_{1}^{N},\omega_{2}^{N},\omega_{3}^{N})\ \mbox{ on }\mathcal{N}_{m_{0}}^{4}(-T_{-},T_{+}),\\ \bm{\omega}^{+}&\equiv(\omega_{1}^{+},\omega_{2}^{+},\omega_{3}^{+})\ \mbox{ on }X_{b_{+}}^{4}.\end{split}

We assume that ω1\omega_{1} is the Kähler form with respect to which the tori are holomorphic on all three pieces. Next, we will glue these triples in the damage zones D​Z−DZ_{-} and D​Z+DZ_{+}, to get a definite triple on ℳ\mathcal{M}. In this section, we show that we can moreover obtain a closed definite triple, which is also very close to an SU⁡(2){\rm{SU}}(2)-structure.

Proposition 6.4.

There exist smooth triples of 11-forms 𝐚±∈Ω1​(D​Z±)⊗ℝ3\bm{a}^{\pm}\in\Omega^{1}(DZ_{\pm})\otimes\mathbb{R}^{3} satisfying

(6.52) 𝝎±+d​𝒂±=Ψ±∗​𝝎N​ in ​D​Z±,\displaystyle\bm{\omega}^{\pm}+d\bm{a}^{\pm}=\Psi_{\pm}^{*}\bm{\omega}^{N}\mbox{ in }DZ_{\pm},

such that for any k∈ℕk\in\mathbb{N},

(6.53) |∇k𝒂±|≤Ck​e−δ​z±​ in ​D​Z±,\displaystyle|\nabla^{k}\bm{a}^{\pm}|\leq C_{k}e^{-\delta z_{\pm}}\mbox{ in }DZ_{\pm},

where δ>0\delta>0 and Ck>0C_{k}>0 are uniform constants independent of β\beta.

Proof.

This follows upon combining Lemma 3.7 and Proposition 6.1. ∎

Let ϕ±\phi_{\pm} be cutoff functions such that

(6.54) ϕ±={0 for ​z±≤T±1 for ​z±≥T±+1.\displaystyle\phi_{\pm}=\begin{cases}0&\mbox{ for }z_{\pm}\leq T_{\pm}\\ 1&\mbox{ for }z_{\pm}\geq T_{\pm}+1\\ \end{cases}.

Then we define

(6.55) 𝝎ℳ={𝝎− on ​Xb−4​(T−),𝝎−+d⁡(ϕ−​𝒂−) on ​Xb−4​(T−,T−+1),𝝎N on ​𝒩m04​(−T−+1,T+−1),𝝎++d⁡(ϕ+​𝒂+) on ​Xb+4​(T+,T++1),𝝎+ on ​Xb+4​(T+).\displaystyle\bm{\omega}^{\mathcal{M}}=\begin{cases}\bm{\omega}^{-}&\mbox{ on }X_{b_{-}}^{4}(T_{-}),\\ \bm{\omega}^{-}+d\big(\phi_{-}\bm{a}^{-}\big)&\mbox{ on }X_{b_{-}}^{4}(T_{-},T_{-}+1),\\ \bm{\omega}^{N}&\mbox{ on }\mathcal{N}_{m_{0}}^{4}(-T_{-}+1,T_{+}-1),\\ \bm{\omega}^{+}+d\big(\phi_{+}\bm{a}^{+}\big)&\mbox{ on }X_{b_{+}}^{4}(T_{+},T_{+}+1),\\ \bm{\omega}^{+}&\mbox{ on }X_{b_{+}}^{4}(T_{+}).\\ \end{cases}
Corollary 6.5.

The triple 𝛚ℳ\bm{\omega}^{\mathcal{M}} is a closed definite triple on ℳ\mathcal{M}. Furthermore, for any k∈ℕk\in\mathbb{N}, there is some constant Ck>0C_{k}>0 independent of the gluing parameter β>0\beta>0 such that

(6.56) ‖Q𝝎−Id‖Ck​(ℳ)≤Ck​e−δq​β,\displaystyle\|Q_{\bm{\omega}}-\Id\|_{C^{k}(\mathcal{M})}\leq C_{k}e^{-\delta_{q}\beta},

where δq>0\delta_{q}>0 is a uniform constant independent of β\beta and Q𝛚=(Qi​j)Q_{\bm{\omega}}=(Q_{ij}) is defined by

(6.57) 12​ωi∧ωj=Qi​j​dvol𝝎ℳ.\frac{1}{2}\omega_{i}\wedge\omega_{j}=Q_{ij}\dvol_{\bm{\omega}^{\mathcal{M}}}.

Here the norm is measured with respect to gβg_{\beta}, the Riemannian metric associated to 𝛚ℳ\bm{\omega}^{\mathcal{M}}.

Proof.

This follows from Proposition 6.1 and Proposition 6.4. ∎

We next analyze some topological properties of the manifold ℳ\mathcal{M}. Note that we do not yet know that ℳ\mathcal{M} is diffeomorphic to the K3⁡3\K 3 surface.

Proposition 6.6.

The compact oriented manifold ℳ\mathcal{M} has the following topological properties:

(6.58) b1​(ℳ)=0,χ⁡(ℳ)=24,b2+​(ℳ)=3,b2−​(ℳ)=19.\displaystyle b_{1}(\mathcal{M})=0,\ \chi(\mathcal{M})=24,\ b_{2}^{+}(\mathcal{M})=3,\ b_{2}^{-}(\mathcal{M})=19.
Proof.

We write the manifold ℳ\mathcal{M} as the union of open sets U∪VU\cup V, where

(6.59) U=𝒩m04​(−T−,T+),V=Xb−​(T−+1)⊔Xb+​(T−+1),\displaystyle U=\mathcal{N}_{m_{0}}^{4}(-T_{-},T_{+}),\ V=X_{b_{-}}(T_{-}+1)\sqcup X_{b_{+}}(T_{-}+1),

where Xb±=Qb±∖𝕋2X_{b_{\pm}}=Q_{b_{\pm}}\setminus\mathbb{T}^{2}, m0=b−+b+m_{0}=b_{-}+b_{+}, with Qb±Q_{b_{\pm}} a del Pezzo surface of degree b±b_{\pm}. Clearly, U∩VU\cap V deformation retracts onto Nilb−3⊔Nilb+3\Nil_{b_{-}}^{3}\sqcup\Nil_{b_{+}}^{3}.

Next, we claim that the de Rham cohomology H1​(Xb±)=0H^{1}(X_{b_{\pm}})=0. To see this, we use the long exact sequence of a pair in de Rham cohomology

(6.60) ⋯→Hck​(Qb±∖𝕋2)→Hk​(Qb±)→Hk​(𝕋2)→ϕHck+1​(Qb±∖𝕋2)→⋯,\displaystyle\cdots\rightarrow H^{k}_{c}(Q_{b_{\pm}}\setminus\mathbb{T}^{2})\rightarrow H^{k}(Q_{b_{\pm}})\rightarrow H^{k}(\mathbb{T}^{2})\xrightarrow{\phi}H^{k+1}_{c}(Q_{b_{\pm}}\setminus\mathbb{T}^{2})\rightarrow\cdots,

see [Spi79, Chapter 11]. Since H3​(Qb±)=0H^{3}(Q_{b_{\pm}})=0, (6.60) yields an exact sequence

(6.61) …→H2​(Qb±)→i∗H2​(𝕋2)→Hc3​(Qb±∖𝕋2)→0.\displaystyle\dots\rightarrow H^{2}(Q_{b_{\pm}})\xrightarrow{i^{*}}H^{2}(\mathbb{T}^{2})\rightarrow H^{3}_{c}(Q_{b_{\pm}}\setminus\mathbb{T}^{2})\rightarrow 0.

Here the mapping i∗:H2​(Qb±)→H2​(𝕋2)i^{*}:H^{2}(Q_{b_{\pm}})\rightarrow H^{2}(\mathbb{T}^{2}) is just the pullback under inclusion, which is dual to the mapping on homology i∗:H2​(𝕋2,ℝ)→H2​(Qb±,ℝ)i_{*}:H_{2}(\mathbb{T}^{2};\mathbb{R})\rightarrow H_{2}(Q_{b_{\pm}};\mathbb{R}). Since 𝕋2\mathbb{T}^{2} is a complex submanifold of a Kähler manifold, this latter mapping is injective, so the mapping i∗i^{*} is surjective, and by Poincaré duality we conclude that

(6.62) H1​(Qb±∖𝕋2)≅Hc3​(Qb±∖𝕋2)=0.\displaystyle H^{1}(Q_{b_{\pm}}\setminus\mathbb{T}^{2})\cong H^{3}_{c}(Q_{b_{\pm}}\setminus\mathbb{T}^{2})=0.

Since we just showed that H1​(Xb±)=0H^{1}(X_{b_{\pm}})=0, the Mayer-Vietoris sequence in cohomology for the pair {U,V}\{U,V\} yields an exact sequence

(6.63) 0→H1​(ℳ)→H1​(𝒩m0)→i∗H1​(Nilb−3⊔Nilb+3)≅H1​(Nilb−3)⊕H1​(Nilb+3).\displaystyle 0\rightarrow H^{1}(\mathcal{M})\rightarrow H^{1}(\mathcal{N}_{m_{0}})\xrightarrow{i^{*}}H^{1}(\Nil_{b_{-}}^{3}\sqcup\Nil_{b_{+}}^{3})\cong H^{1}(\Nil_{b_{-}}^{3})\oplus H^{1}(\Nil_{b_{+}}^{3}).

The mapping i∗i^{*} is the pullback under inclusion of the two nilmanifold fibers of the neck at each end. We claim that this mapping is injective. To see this, let 𝒫m0≡{p1,…,pm0}\mathcal{P}_{m_{0}}\equiv\{p_{1},\ldots,p_{m_{0}}\} denote the monopole points in B=𝕋2×(−T−,T+)B=\mathbb{T}^{2}\times(-T_{-},T_{+}), where m0=b−+b+m_{0}=b_{-}+b_{+}. Then there are p~j∈𝒩m04\tilde{p}_{j}\in\mathcal{N}_{m_{0}}^{4} such that 𝒩m04∖𝒫~m0\mathcal{N}_{m_{0}}^{4}\setminus\widetilde{\mathcal{P}}_{m_{0}} is a circle bundle over B∖𝒫m0B\setminus\mathcal{P}_{m_{0}},

(6.64) S1⟶𝒩m04∖𝒫~m0→𝜋B∖𝒫m0.\displaystyle S^{1}\longrightarrow\mathcal{N}_{m_{0}}^{4}\setminus\widetilde{\mathcal{P}}_{m_{0}}\xrightarrow{\ \pi\ }B\setminus\mathcal{P}_{m_{0}}.

The Gysin sequence of (6.64) begins with

(6.65) 0→H1​(B∖𝒫m0)→π∗H1​(𝒩m04∖𝒫~m0)→⋯\displaystyle 0\rightarrow H^{1}(B\setminus\mathcal{P}_{m_{0}})\xrightarrow{\pi^{*}}H^{1}(\mathcal{N}_{m_{0}}^{4}\setminus\widetilde{\mathcal{P}}_{m_{0}})\rightarrow\cdots

It is easy to see inclusion induces an isomorphism H1​(B∖𝒫m0)≅H1​(B)≅ℝ⊕ℝH^{1}(B\setminus\mathcal{P}_{m_{0}})\cong H^{1}(B)\cong\mathbb{R}\oplus\mathbb{R}, and similarly, H1​(𝒩m04∖𝒫~m0)≅H1​(𝒩m04)H^{1}(\mathcal{N}_{m_{0}}^{4}\setminus\widetilde{\mathcal{P}}_{m_{0}})\cong H^{1}(\mathcal{N}_{m_{0}}^{4}). Then (6.65) becomes

(6.66) 0→span​{d​x,d​y}→π∗H1​(𝒩m04)→⋯\displaystyle 0\rightarrow\mbox{span}\{dx,dy\}\xrightarrow{\pi^{*}}H^{1}(\mathcal{N}_{m_{0}}^{4})\rightarrow\cdots

Together with Proposition 2.3, and the exact sequence (6.63), we conclude that i∗​π∗​d​xi^{*}\pi^{*}dx and i∗​π∗​d​yi^{*}\pi^{*}dy are both nontrivial and are linearly independent in H1​(Nilb−3⊔Nilb+3)H^{1}(\Nil^{3}_{b_{-}}\sqcup\Nil^{3}_{b_{+}}), so i∗i^{*} is injective as claimed. Then (6.63) implies that b1​(ℳ)=0b_{1}(\mathcal{M})=0. Since ℳ\mathcal{M} is a compact orientable 44-manifold, Poincaré duality also implies that b3​(ℳ)=0b_{3}(\mathcal{M})=0.

Next, it follows from the fibration (6.64) that χ⁡(𝒩m04∖𝒫~m0)=0\chi(\mathcal{N}_{m_{0}}^{4}\setminus\widetilde{\mathcal{P}}_{m_{0}})=0, and therefore

(6.67) χ⁡(𝒩m04)=#​ of monopole points =m0=b−+b+.\displaystyle\chi(\mathcal{N}_{m_{0}}^{4})=\#{\mbox{ of monopole points }}=m_{0}=b_{-}+b_{+}.

For a Tian-Yau space, it follows that

(6.68) χ⁡(Xb4)=χ⁡(Qb∖𝕋2)=χ⁡(Qb)−χ⁡(𝕋2)=χ⁡(Qb),\displaystyle\chi(X_{b}^{4})=\chi(Q_{b}\setminus\mathbb{T}^{2})=\chi(Q_{b})-\chi(\mathbb{T}^{2})=\chi(Q_{b}),

where QbQ_{b} is a degree bb del Pezzo surface, so

(6.69) χ⁡(Xb4)=χ⁡(Qb∖𝕋2)=12−b\displaystyle\chi(X_{b}^{4})=\chi(Q_{b}\setminus\mathbb{T}^{2})=12-b

Note also that χ⁡(Nilb−3)=χ⁡(Nilb+3)=0\chi(\Nil_{b_{-}}^{3})=\chi(\Nil_{b_{+}}^{3})=0 since it is an orientable 3-manifold. Then we have

(6.70) χ⁡(ℳ)=χ⁡(Xb−4)+χ⁡(𝒩)+χ⁡(Xb+4)=(12−b−)+(b++b−)+(12−b+)=24.\displaystyle\chi(\mathcal{M})=\chi(X_{b_{-}}^{4})+\chi(\mathcal{N})+\chi(X_{b_{+}}^{4})=(12-b_{-})+(b_{+}+b_{-})+(12-b_{+})=24.

Since we have shown above that b1​(ℳ)=b3​(ℳ)=0b_{1}(\mathcal{M})=b_{3}(\mathcal{M})=0, this proves that b2​(ℳ)=22b_{2}(\mathcal{M})=22.

Next, as we constructed in (6.55) the approximate definite triple 𝝎ℳ≡(ω1,ω2,ω3)\bm{\omega}^{\mathcal{M}}\equiv(\omega_{1},\omega_{2},\omega_{3}), which are everywhere non-zero self-dual 2-forms forming a basis of Λ+2\Lambda^{2}_{+} at every point. This implies the bundle Λ+2​(ℳ)\Lambda^{2}_{+}(\mathcal{M}) is a trivial rank 33 bundle. Also, ω1\omega_{1} being non-zero everywhere means that there is an almost complex structure (ω1/|ω1|\omega_{1}/|\omega_{1}| is a unit norm self-dual 2-form, which is equivalent to an orthogonal almost complex structure). By Corollary 6.5, for β≫1\beta\gg 1, the rank 2 subbundle V⊂Λ02V\subset\Lambda^{2}_{0}, given by the orthogonal complement of ω1/|ω1|\omega_{1}/|\omega_{1}| is trivial. Then 0=c1​(V⊗ℂ)=c1​(T​ℳ,J)20=c_{1}(V\otimes\mathbb{C})=c_{1}(T\mathcal{M},J)^{2}, and the Hirzebruch signature theorem implies that

(6.71) 2​χ​(ℳ)+3​τ​(ℳ)=∫ℳc12=0,\displaystyle 2\chi(\mathcal{M})+3\tau(\mathcal{M})=\int_{\mathcal{M}}c_{1}^{2}=0,

from which it follows that τ⁡(ℳ)=−16\tau(\mathcal{M})=-16. Therefore, b2+​(ℳ)=3b_{2}^{+}(\mathcal{M})=3 and b2−​(ℳ)=19b_{2}^{-}(\mathcal{M})=19.

∎

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