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2.2. The model space [03GI]

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2.2. The model space

Consider a 22-torus 𝕋2\mathbb{T}^{2} with a flat metric of area AA and let U=𝕋x,y2×ℝz>0U=\mathbb{T}^{2}_{x,y}\times\mathbb{R}_{z>0}, where we have fixed a choice of an orthogonal frame {e1,e2}\{e_{1},e_{2}\} on 𝕋2\mathbb{T}^{2} such that g𝕋2=A⁡(e12+e22)g_{\mathbb{T}^{2}}=A(e_{1}^{2}+e_{2}^{2}). Let V⁡(z)=2​π​b​zAV(z)=\frac{2\pi bz}{A} for a positive integer b>0b>0. Fixing a connection form θ\theta such that d​θ=2​π​bA​dvol𝕋2d\theta=\frac{2\pi b}{A}{\rm dvol}_{\mathbb{T}^{2}}, the corresponding hyperkähler Gibbons-Hawking metric gg is given by

(2.19) g=2​π​b​zA​(g𝕋2+d​z2)+A2​π​b​z​θ2.\displaystyle g=\frac{2\pi bz}{A}(g_{\mathbb{T}^{2}}+dz^{2})+\frac{A}{2\pi bz}\theta^{2}.

The Gibbons-Hawking space (𝔐,g)(\mathfrak{M},g) has one complete end as z→∞z\rightarrow\infty and one incomplete end as z→0z\rightarrow 0. Moreover, for each z0>0z_{0}>0, the level set {z=z0}\{z=z_{0}\} is a Heisenberg nilmanifold Nilb3⁡(ϵ,τ)\Nil^{3}_{b}(\epsilon,\tau) with a z0z_{0}-dependent left-invariant metric, where τ\tau denotes the modulus of our flat 22-torus in the upper half-plane and A=ϵ2​τ2A=\epsilon^{2}\tau_{2} as in Section 2.1. Making the substitution z=(3/2)​s2/3z=(3/2)s^{2/3}, and then scaling appropriately, the Gibbons-Hawking metric gg takes the form

(2.20) ds2+s2/3g𝕋2+s−2/3(A3​π​bθ)2.\displaystyle ds^{2}+s^{2/3}g_{\mathbb{T}^{2}}+s^{-2/3}\Big(\frac{A}{3\pi b}\theta\Big)^{2}.

In this form, it is easy to see that the volume growth is ∼s4/3\sim s^{4/3} and that |Rm|∼s−2|{\Rm}|\sim s^{-2} as s→∞s\rightarrow\infty. One can also show using the Chern-Gauss-Bonnet formula that the L2L^{2} norm of Rm\Rm is finite.

Note that if we had instead taken b=0b=0, the Gibbons-Hawking metric would be the product of ℝ\mathbb{R} with a flat 33-torus, i.e., the type of geometry known as ALH geometry in the literature.

View the flat torus 𝕋2\mathbb{T}^{2} as an elliptic curve EE of modulus τ\tau with respect to the complex structure JJ defined by J​e1=e2Je_{1}=e_{2}. Then there is exactly one gg-parallel complex structure J0J_{0} on the total space 𝔐\mathfrak{M} that makes the projection map to EE holomorphic. This choice of complex structure realizes 𝔐\mathfrak{M} as an open subset of the total space of a degree bb holomorphic line bundle LL over EE (more precisely, as a tubular neighborhood of the zero section of LL with the zero section removed). The Ricci-flat Kähler form with respect to J0J_{0} is then given by (see Proposition 3.1)

(2.21) ω0=23​i​∂∂¯​(−log⁡|ξ|h2)3/2,\omega_{0}=\frac{2}{3}i\partial\bar{\partial}(-{\log|\xi|}_{h}^{2})^{3/2},

where hh is a hermitian metric on LL whose curvature form is a multiple of the flat Kähler form on EE, and where the tautological section ξ\xi cuts out the zero section of LL. This is an example of the Calabi construction, and we call the corresponding metric a Calabi model metric of degree bb. We will discuss this construction (in all dimensions) in more detail in Section 3. In complex dimension 22, the Gibbons-Hawking ansatz actually recovers the Calabi ansatz for all degree bb holomorphic line bundles over EE. Indeed, any two such line bundles differ by a degree 0 line bundle and Pic0⁡(E)=H1​(E,𝒪E)/H1​(E,ℤ)\Pic^{0}(E)=H^{1}(E,\mathcal{O}_{E})/H^{1}(E,\mathbb{Z}); on the other hand, the gauge equivalence classes of flat connections are parametrized by H1​(E,ℝ)/H1​(E,ℤ)H^{1}(E,\mathbb{R})/H^{1}(E,\mathbb{Z}).

A very convenient property for our purposes is that if we do change the connection 11-form θ\theta by a flat connection, then the associated Gibbons-Hawking metric (2.19) actually only changes by a diffeomorphism (although this diffeomorphism necessarily breaks the S1S^{1}-bundle structure on 𝔐\mathfrak{M}). To see this, fix any choice of θ\theta such that d​θ=2​π​bA​dvolEd\theta=\frac{2\pi b}{A}\dvol_{E}. Note that we can always arrange by parallel transport in the zz-direction that the d​zdz-component of θ\theta vanishes. Then we only need to consider the case that θ\theta gets changed by the pullback (under the projection 𝔐→πU→E\mathfrak{M}\stackrel{{\scriptstyle\pi}}{{\to}}U\to E) of a parallel 11-form η\eta on EE. Write η=v​⌟​dvolE\eta=v\,\lrcorner\,\dvol_{E}, where vv is a parallel vector field on EE. Let v^\hat{v} be the θ\theta-horizontal lift of vv to 𝔐\mathfrak{M} and let f^s\hat{f}_{s} be the 11-parameter group of diffeomorphisms generated by v^\hat{v}, which covers a 11-parameter group of translations on EE. Then

(2.22) dd​s​(f^s∗​θ)=v^​⌟​f^s∗​(d​θ)+d⁡(v^​⌟​f^s∗​θ)=2​π​bA​(v^​⌟​π∗​(dvolE))=2​π​bA​π∗​η,\displaystyle\begin{split}\frac{d}{ds}(\hat{f}_{s}^{*}\theta)&=\hat{v}\,\lrcorner\,\hat{f}_{s}^{*}(d\theta)+d(\hat{v}\,\lrcorner\,\hat{f}_{s}^{*}\theta)=\frac{2\pi b}{A}(\hat{v}\,\lrcorner\,\pi^{*}({\rm dvol}_{E}))=\frac{2\pi b}{A}\pi^{*}\eta,\end{split}

using the fact that d​f^s|x​(v^|x)=v^|f^s​(x)d\hat{f}_{s}|_{x}(\hat{v}|_{x})=\hat{v}|_{\hat{f}_{s}(x)} for all x∈𝔐x\in\mathfrak{M}. Thus,

(2.23) f^s∗​θ=θ+2​π​b​sA​π∗​η.\hat{f}_{s}^{*}\theta=\theta+\frac{2\pi bs}{A}\pi^{*}\eta.

This shows that any two possible choices of θ\theta with vanishing d​zdz-component differ by the translation action of EE on itself, lifted to 𝔐\mathfrak{M}, and then the corresponding hyperkähler metrics (2.19) are clearly isometric as well. We note that with the particular choice θ=θb\theta=\theta_{b} from (2.12), these diffeomorphisms can be written down explicitly as follows: for all p,q∈ℝp,q\in\mathbb{R}, the mapping

(2.24) φ⁡(x,y,t,z)=(x−q,y+p,t+p​x,z)\displaystyle\varphi(x,y,t,z)=(x-q,y+p,t+px,z)

descends to a diffeomorphism of Nilb3​(ϵ,τ)x,y,t×ℝz{\rm Nil}^{3}_{b}(\epsilon,\tau)_{x,y,t}\times\mathbb{R}_{z} which satisfies

(2.25) φ∗​θb=θb+2​π​bA​(p​d​x+q​d​y).\displaystyle\varphi^{*}\theta_{b}=\theta_{b}+\frac{2\pi b}{A}(pdx+qdy).
Remark 2.4.

The above observations reflect the fact that EE acts transitively by pullback on its own Picb{\rm Pic}^{b} for b>0b>0 (for instance, a holomorphic line bundle of degree 11 on EE is uniquely isomorphic to 𝒪E​(x)\mathcal{O}_{E}(x) for some point x∈Ex\in E). Moreover, the total spaces of all degree b>0b>0 holomorphic line bundles on EE are actually biholomorphic as complex manifolds. All of this is false in the classical ALH case b=0b=0. In particular, for b=0b=0 the above parameters p,qp,q are actual moduli of the metric, corresponding to flat metrics on 𝕋3\mathbb{T}^{3} that do not split isometrically as S1×𝕋2S^{1}\times\mathbb{T}^{2}.

The Calabi construction provides the model at infinity of the Tian-Yau metrics in our context. These metrics will also be studied in more detail in Section 3. Note that every Tian-Yau metric comes with its own preferred choice of a connection form θ\theta determined by the Chern connection of the normal bundle of the compactifying divisor. The above gauge fixing construction then allows us to choose a new coordinate system at infinity that identifies this θ\theta with the standard connection form θb\theta_{b} (see the proof of Proposition 3.1 and also equation (6.6)).

Remark 2.5.

We can choose a different gg-parallel complex structure J1J_{1} on 𝔐\mathfrak{M} such that J1​θ=z​d​xJ_{1}\theta=zdx. With respect to J1J_{1} we can view 𝔐\mathfrak{M} as a holomorphic elliptic fibration over a punctured disc in ℂ\mathbb{C}. The monodromy of this fibration is given by the matrix

(2.26) [1b01]∈SL⁡(2,ℤ).\begin{bmatrix}1&b\\ 0&1\end{bmatrix}\in\SL(2,\mathbb{Z}).

See [Sco83] for more details. This gives a different compactified model for 𝔐\mathfrak{M} where the compactifying divisor is a singular fiber of Kodaira type IbI_{b}. The J1J_{1}-Kähler form of our hyperkähler model metric is then given by an appropriate semi-flat ansatz [GSVY90, GW00], and provides the model at infinity for the gravitational instantons with volume growth ∼r4/3\sim r^{4/3} and curvature decay ∼r−2\sim r^{-2} constructed in [Hei12]. We will pursue this observation further in [HSVZ], connecting the complete hyperkähler metrics of [TY90] and of [Hei12] by global hyperkähler rotations.

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