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2.2. Bi-polyhedral Kähler affine structures [03EQ]

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2.2. Bi-polyhedral Kähler affine structures

We will be interested in a very special types of integral Kähler affine structures. These structures arise in the metric limits of Calabi-Yau hypersurfaces and complete intersections in toric varieties.

Definition.

An integral affine structure on YY is polyhedral if there is an nn-dimensional polyhedral complex PP, a collection of disjoint open sets {Uα}\{U_{\alpha}\}, whose closures cover YY, i.e. Y=⋃U¯αY=\bigcup\overline{U}_{\alpha}, and a continuous map ϕ:Y→P\phi:Y\to P, which provides an affine homeomorphism of each UαU_{\alpha} with the interior of some nn-dimensional face of PP. We say that the pair ({Uα},P)(\{U_{\alpha}\},P) realizes the polyhedral affine structure if PP is minimal, which, in particular, means that there is a bijection between open sets {Uα}\{U_{\alpha}\} and nn-dimensional cells of PP.

Definition.

An integral Kähler affine structure on YY is bi-polyhedral (bi-PIKAS for short) if there is a bipartite covering {Uα,Vβ}\{U_{\alpha},V_{\beta}\} of YY and two polyhedral complexes P,P^P,\hat{P} such that ({Uα},P)(\{U_{\alpha}\},P) and ({Vβ},P^)(\{V_{\beta}\},\hat{P}) provide polyhedral realizations of the underlying affine structure and its dual, respectively. We say that the bi-polyhedral Kähler affine structure is of type ({Uα,Vβ},P,P^)(\{U_{\alpha},V_{\beta}\},P,\hat{P}).

The bi-polyhedral property imposes very severe restrictions on the compatibility between Riemannian metric and affine structure. In particular, Hess⁡Kα∈ℒl​o​c1​(ℝn)\operatorname{Hess}K_{\alpha}\in\mathcal{L}^{1}_{loc}(\mathbb{R}^{n}) and the Cauchy-Schwartz inequality implies that the metric completion of YY can be identified with PP or P^\hat{P}. This endows both polyhedral complexes with (isomorphic) structures of complete metric spaces.

Next we want to show the existence of bi-PIKAS on Σ\D{\Sigma\backslash D}. Recall from [HZ02] that Σ\D{\Sigma\backslash D} has a bipartite covering by open sets UvU_{v} and VwV_{w}. Also, given vectors λ,ν\lambda,\nu in the interiors of the respective secondary cones SC⁡(S),SC⁡(T)\operatorname{SC}(S),\operatorname{SC}(T) with λ⁡(0)=ν⁡(0)=0\lambda(0)=\nu(0)=0 we can define the polytopes

Δλ∨={n∈ℝd:⟨m,n⟩+λ⁡(m)≤0​ for all ​m∈Δℤ},\displaystyle\Delta^{\vee}_{\lambda}=\{n\in\mathbb{R}^{d}\ :\ \langle m,n\rangle+\lambda(m)\leq 0\text{ for all }m\in\Delta_{\mathbb{Z}}\},
Δν={m∈(ℝd)∗:⟨m,n⟩+ν⁡(n)≤0​ for all ​n∈Δℤ∨}.\displaystyle{\Delta_{\nu}}=\{m\in(\mathbb{R}^{d})^{*}\ :\ \langle m,n\rangle+\nu(n)\leq 0\text{ for all }n\in\Delta^{\vee}_{\mathbb{Z}}\}.

In the future we will abbreviate the type of a bi-polyhedral integral Kähler affine structure on Σ\D{\Sigma\backslash D} by simply (λ,ν)(\lambda,\nu) having fixed the covering ({Uv,Vw})(\{U_{v},V_{w}\}).

In order to specify a bi-PIKAS of type (λ,ν)(\lambda,\nu) on Σ\D{\Sigma\backslash D} we will provide the following data. A Legendre dual pair of convex functions Φ,Φ^\Phi,\hat{\Phi} on Δλ∨,Δν\Delta^{\vee}_{\lambda},{\Delta_{\nu}}, respectively, smooth on each strata of the respective polytope. (This implies that the Hessians of both Φ,Φ^\Phi,\hat{\Phi} are positive along the strata.) Then the restrictions of Φ\Phi to the facets of Δλ∨\Delta^{\vee}_{\lambda} serve as potentials for the metric along UvU_{v}. For future use we will prove that it is possible to choose these functions consistently in λ\lambda and ν\nu.

Definition.

Suppose, for each pair (λ,ν)∈SC⁡(S)×SC⁡(T)(\lambda,\nu)\in\operatorname{SC}(S)\times\operatorname{SC}(T) we have a bi-polyhedral Kähler affine structure on Σ\D{\Sigma\backslash D} of type (λ,ν)(\lambda,\nu), which varies continuously with (λ,ν)(\lambda,\nu) in the Hausdorff topology of metric structures on Σ\Sigma. We call such a family projective if:

  • •

    For any linear functions l∈ℝd,l∨∈(ℝd)∗l\in\mathbb{R}^{d},\ l^{\vee}\in(\mathbb{R}^{d})^{*}, the bi-PIKAS for (λ+l,ν+l∨)∈SC⁡(S)×SC⁡(T)(\lambda+l,\nu+l^{\vee})\in\operatorname{SC}(S)\times\operatorname{SC}(T) have the same underlying Kähler affine structure.

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    The bi-PIKAS for (ϵ−1​λ,ϵ​ν)(\epsilon^{-1}\lambda,\epsilon\nu) differs from the bi-PIKAS for (λ,ν)(\lambda,\nu) by the ϵ\epsilon-rescaling

    (yα′,y^α′,Kα′​(yα′),K^α′​(y^α′),gi​j)=(ϵ−1​yα,ϵ​y^α,Kα​(ϵ​yα′),K^α​(ϵ−1​y^α′),ϵ2​gi​j)(y^{\prime}_{\alpha},\hat{y}^{\prime}_{\alpha},K^{\prime}_{\alpha}(y^{\prime}_{\alpha}),\hat{K}^{\prime}_{\alpha}(\hat{y}^{\prime}_{\alpha}),g_{ij})=(\epsilon^{-1}y_{\alpha},\epsilon\hat{y}_{\alpha},K_{\alpha}(\epsilon y^{\prime}_{\alpha}),\hat{K}_{\alpha}(\epsilon^{-1}\hat{y}^{\prime}_{\alpha}),\epsilon^{2}g_{ij})

Note here that adding global linear functions to the potentials Φ,Φ^\Phi,\hat{\Phi} will induce translations of the polytopes Δν,Δλ∨{\Delta_{\nu}},\Delta^{\vee}_{\lambda}. Though giving different bi-PIKAS (as we defined them) this will have no effect on the underlying Kähler affine structures (the latter will be canonically equivalent).

Another important observation is that rescaling the data for bi-PIKAS will provide the same metric on Σ\D{\Sigma\backslash D}, though different affine structures.

Proposition 2.1.

There are Legendre dual functions Φ:Δλ∨→ℝ\Phi\colon\Delta^{\vee}_{\lambda}\rightarrow\mathbb{R} and Φ^:Δν→ℝ\hat{\Phi}\colon{\Delta_{\nu}}\rightarrow\mathbb{R} that define a projective family of bi-PIKAS on Σ\D{\Sigma\backslash D}.

Proof.

First, we choose a smooth function with positive Hessian on Δλ−β∨\Delta_{\lambda-\beta}^{\vee} whose gradients stay in Δν−β\Delta_{\nu-\beta}, and cover Δν−2​β\Delta_{\nu-2\beta}.

[Uncaptioned image][Uncaptioned image]

Figure 1:   The domain for the first step.    The set of gradients.

As a second step, we need a continuous strictly convex function ν~\tilde{\nu} on β​Δ∨\beta\Delta^{\vee} that is an approximation of the function ν\nu with the following properties.

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    ν~\tilde{\nu} is piecewise smooth.

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    Hess⁡ν~>0\operatorname{Hess}\tilde{\nu}>0 on the smooth pieces.

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    The gradients along cone⁡τ\operatorname{cone}\tau belong to a neighborhood of the corresponding vertex in Δν{\Delta_{\nu}} that are pairwise disjoint, and do not meet the β\beta neighborhood of the barycenter of Δν{\Delta_{\nu}}.

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    For a vertex w∈Tw\in T, the ww-directional derivatives equal −ν⁡(w)-\nu(w) in the star neighborhood of β​w\beta w in the barycentric subdivision of β​T\beta T.

[Uncaptioned image]

Figure 2: The set of gradients of ν~\tilde{\nu}.

We obtain a convex function on (ℝd)∗(\mathbb{R}^{d})^{*} if we consider the lower hull of the (d+1d+1)-dimensional Minkowski sum of graphs of the two functions.

Finally, we want to obtain a function that is smooth along the strata. As explained in § 3.2, we convolute with a kernel that depends on the position x∈Δλ∨x\in\Delta^{\vee}_{\lambda} as follows. Consider the quadratic form

Q⁡(x)=∑v∈SQv​(x)​ where ​Qv​(x)=1ρv​(x)​v2Q(x)=\sum_{v\in S}Q_{v}(x)\ \text{ where }\ Q_{v}(x)=\frac{1}{\rho_{v}(x)}v^{2}

This quadratic form is non-degenerate because the vv’s span (ℝd)∗(\mathbb{R}^{d})^{*}. It has a dominant summand if xx is close to a facet. Now our kernel will be a normalized e1−Q⁡(x)e^{1-Q(x)}. Its support – the ellipsoid given by Q⁡(x)≤1Q(x)\leq 1 – depends on the position as sketched in the figure.

[Uncaptioned image]

Figure 3: The support of the mollifier.

The obtained function will have a positive Hessian along the strata, so that the Legendre dual function will be smooth along its corresponding strata. ∎

The metric completion of Σ\D{\Sigma\backslash D} can be identified with Σ\Sigma and endowed with the structure of a compact metric space via the bi-polyhedral homeomorphisms ϕ,ϕ^\phi,\hat{\phi}:

Σ\textstyle{\Sigma\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}ϕ\scriptstyle{\phi}ϕ^\scriptstyle{\hat{\phi}}∂Δλ∨\textstyle{\partial\Delta^{\vee}_{\lambda}}∂Δν\textstyle{\partial{\Delta_{\nu}}}

Throughout the paper we will often identify points in Σ\Sigma, ∂Δλ∨\partial\Delta^{\vee}_{\lambda} and ∂Δν\partial{\Delta_{\nu}} by means of these homeomorphisms when there is no confusion.

We can realize the affine coordinates yy on UvU_{v} and VwV_{w} explicitly as taking values in the following (affine) subspaces and quotients of ℝd\mathbb{R}^{d}:

y⁡(q)∈ℝvd​(λ⁡(v)):={n∈ℝd:⟨v,n⟩+λ⁡(v)=0},q∈Uv,\displaystyle y(q)\in\mathbb{R}^{d}_{v}(\lambda(v)):=\{n\in\mathbb{R}^{d}\ :\ \langle v,n\rangle+\lambda(v)=0\},\quad q\in U_{v},
y⁡(q)∈ℝd/w,q∈Vw,\displaystyle y(q)\in\mathbb{R}^{d}/w,\quad q\in V_{w},

and the transition maps are given by the obvious projections ℝvd​(λ⁡(v))→ℝd/w\mathbb{R}^{d}_{v}(\lambda(v))\to\mathbb{R}^{d}/w. Then the affine monodromy along a primary loop (v0​w0​v1​w1)(v_{0}w_{0}v_{1}w_{1}) is given by (cf. [HZ02, Lemma 2.4]):

(1) n↦n+[⟨v1,n⟩+λ⁡(v1)]​(w1−w0),n∈ℝvd​(λ⁡(v)).n\mapsto n+[\langle v_{1},n\rangle+\lambda(v_{1})](w_{1}-w_{0}),\quad n\in\mathbb{R}^{d}_{v}(\lambda(v)).

To describe the full polarization class of a bi-PIKAS of type (λ,ν)(\lambda,\nu) on Σ\D{\Sigma\backslash D} we consider the representation of (SL⁡(d−1,ℤ)⋉ℝd−1)⋉Affd−1(\operatorname{SL}(d-1,\mathbb{Z})\ltimes\mathbb{R}^{d-1})\ltimes\operatorname{Af{}f}_{d-1} in ℝd⊕ℝ\mathbb{R}^{d}\oplus\mathbb{R}. The dual space is identified with (ℝd)∗⊕ℝ(\mathbb{R}^{d})^{*}\oplus\mathbb{R}. For the charts UvU_{v} and VwV_{w} we set

Uv:p=(01),k=(kv0),q=(v,0),l=(0,1),\displaystyle U_{v}:\ p=\left(\begin{array}[]{c}0\\ 1\end{array}\right),\ k=\left(\begin{array}[]{c}k_{v}\\ 0\end{array}\right),\ q=(v,0),\ l=(0,1),
Vw:p=(w0),k=(01),q=(0,1),l=(lw,0),\displaystyle V_{w}:\ p=\left(\begin{array}[]{c}w\\ 0\end{array}\right),\ k=\left(\begin{array}[]{c}0\\ 1\end{array}\right),\ q=(0,1),\ l=(l_{w},0),

where we have chosen integral elements lw∈(ℤd)∗l_{w}\in(\mathbb{Z}^{d})^{*} and kv∈ℤdk_{v}\in\mathbb{Z}^{d} such that ⟨lw,w⟩=1\langle l_{w},w\rangle=1 and ⟨v,kv⟩=1\langle v,k_{v}\rangle=1. Then for Uv∩VwU_{v}\cap V_{w} the cocycle transformation gv​w:ℝd⊕ℝ→ℝd⊕ℝg_{vw}:\mathbb{R}^{d}\oplus\mathbb{R}\to\mathbb{R}^{d}\oplus\mathbb{R} is given by:

(ns)↦(n′−[1+ν⁡(w)]​⟨lw,n′⟩​w+s​w⟨v,n⟩),\left(\begin{array}[]{c}n\\ s\end{array}\right)\mapsto\left(\begin{array}[]{c}n^{\prime}-\left[1+\nu(w)\right]\langle l_{w},n^{\prime}\rangle w+sw\\ \langle v,n\rangle\end{array}\right),

where n′=n−⟨v,n⟩​[1+λ⁡(v)]​kvn^{\prime}=n-\langle v,n\rangle\left[1+\lambda(v)\right]k_{v}. The cocycle {gv​w}\{g_{vw}\} represents the polarization class which we will denote by [λ,ν][\lambda,\nu].

Then the monodromy representation π1​(Σ\D)→GL⁡(ℝd⊕ℝ)\pi_{1}({\Sigma\backslash D})\to\operatorname{GL}(\mathbb{R}^{d}\oplus\mathbb{R}) along a primary loop (v0​w0​v1​w1)(v_{0}w_{0}v_{1}w_{1}) is given by

(ns)↦(ns)+α⁡(n)​(w1−w0ν⁡(w1)−ν⁡(w0)),\left(\begin{array}[]{c}n\\ s\end{array}\right)\mapsto\left(\begin{array}[]{c}n\\ s\end{array}\right)+\alpha(n)\left(\begin{array}[]{c}w_{1}-w_{0}\\ \nu(w_{1})-\nu(w_{0})\end{array}\right),

where α⁡(n)=v1​(n)+λ⁡(v1)​v0​(n)−[1+λ⁡(v)]​v1​(kv0)​v0​(n)\alpha(n)=v_{1}(n)+\lambda(v_{1})v_{0}(n)-[1+\lambda(v)]v_{1}(k_{v_{0}})v_{0}(n). Considering this transformation on the quotient by the last coordinate and using kv0k_{v_{0}} to identify 𝔸d−1={⟨v,n⟩=1}\mathbb{A}^{d-1}=\{\langle v,n\rangle=1\} with ℝvd(λ(v))={⟨v,n⟩+λ(v)=0}\mathbb{R}^{d}_{v}(\lambda(v))=\{\langle v,n\rangle+\lambda(v)=0\} via

n↦n−⟨v,n⟩​[1+λ⁡(v)]​kv,\displaystyle n\mapsto n-\langle v,n\rangle\left[1+\lambda(v)\right]k_{v},

we recover the above affine monodromy on ℝvd​(λ⁡(v))\mathbb{R}^{d}_{v}(\lambda(v)).

Following through the above calculation shows that the converse is also true: any bi-polyhedral Kähler affine structure on Σ\D{\Sigma\backslash D} in the class [λ,ν][\lambda,\nu] is, in fact, of type (λ,ν)(\lambda,\nu).

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