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Affine manifolds with singularities. [04I6]

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Affine manifolds with singularities.

When a Lagrangian fibration has singular fibres, its base is no longer an affine manifold but an affine manifold with singularities. These singularities can be a priori rather complicated. The topological properties described in §2 motivate the following:

Definition 3.6.

An (integral) affine manifold with singularities is a triple (B,Δ,𝒜)(B,\Delta,\mathscr{A}), where BB is a topological nn-dimensional manifold, Δ⊂B\Delta\subset B a set which is locally a finite union of locally closed submanifolds of codimension at least 22 and 𝒜\mathscr{A} is an (integral) affine structure on B0=B−ΔB_{0}=B-\Delta. A continuous map between (integral) affine manifolds with singularities

α:B→B′\alpha:B\rightarrow B^{\prime}

is (integral) affine if α−1​(B0′)∩B0\alpha^{-1}(B_{0}^{\prime})\cap B_{0} is dense in BB and the restriction α0=α|α−1​(B0′)∩B0\alpha_{0}=\alpha|_{\alpha^{-1}(B_{0}^{\prime})\cap B_{0}}:

α0:α−1​(B0′)∩B0→B0′\alpha_{0}:\alpha^{-1}(B_{0}^{\prime})\cap B_{0}\rightarrow B_{0}^{\prime}

is an (integral) affine map. We say that α\alpha is an (integral) affine isomorphism if α\alpha is an homeomorphism and α0\alpha_{0} is an (integral) affine isomorphism of (integral) affine manifolds.

From now on we restrict to dimension n=2n=2 or 33. Let (B,Δ,𝒜)(B,\Delta,\mathscr{A}) be an affine manifold with singularities and let (B0,𝒜)(B_{0},\mathscr{A}) be the corresponding affine manifold. Let X⁡(B0,𝒜)X(B_{0},\mathscr{A}) be the Lagrangian TnT^{n} bundle over B0B_{0} as introduced at the beginning of this section. We shall start imposing conditions on the singularities of the affine structure which, in particular, will imply that X⁡(B0,𝒜)X(B_{0},\mathscr{A}) is of the topological type described in §2, e.g. such that X⁡(B0,𝒜)X(B_{0},\mathscr{A}) will have semi-stable monodromy as in Theorem 2.11.

We start defining local models of integral affine manifolds with singularities. In dimension 2, the allowed behavior is described in the following:

Example 3.7 (The node).

We define an affine structure with singularities on B=ℝ2B=\mathbb{R}^{2}. Let Δ={0}\Delta=\{0\} and let (x1,x2)(x_{1},x_{2}) be the standard coordinates on BB. As the covering {Ui}\{U_{i}\} of B0=ℝ2−ΔB_{0}=\mathbb{R}^{2}-\Delta we take the following two sets

U1=ℝ2−{x2=0andx1≥0},U_{1}=\mathbb{R}^{2}-\{x_{2}=0\ \text{and}\ x_{1}\geq 0\},
U2=ℝ2−{x2=0andx1≤0}.U_{2}=\mathbb{R}^{2}-\{x_{2}=0\ \text{and}\ x_{1}\leq 0\}.

Denote by H+H^{+} the set {x2>0}\{x_{2}>0\} and by H−H^{-} the set {x2<0}\{x_{2}<0\}. Let TT be the matrix

T=(1011).T=\left(\begin{array}[]{cc}1&0\\ 1&1\end{array}\right). (6)

The coordinate maps ϕ1\phi_{1} and ϕ2\phi_{2} on U1U_{1} and U2U_{2} are defined as follows

ϕ1\displaystyle\phi_{1} =\displaystyle= Id\displaystyle\mathrm{Id}
ϕ2\displaystyle\phi_{2} =\displaystyle= {Idon​H¯+∩U2,(T−1)ton​H−\displaystyle\left\{\begin{array}[]{ll}\mathrm{Id}&\text{on}\ \bar{H}^{+}\cap U_{2},\\ (T^{-1})^{t}&\text{on}\ H^{-}\end{array}\right.

The atlas 𝒜={Ui,ϕi}i=1,2\mathscr{A}=\{U_{i},\phi_{i}\}_{i=1,2} is clearly an affine structure on B0B_{0}. It is easy to check that given a point b∈B0b\in B_{0}, we can chose a basis of Tb∗​B0T^{\ast}_{b}B_{0} with respect to which the holonomy representation ρ∗\rho^{\ast} sends the anti-clockwise oriented generator of π1​(B0)\pi_{1}(B_{0}) to the matrix TT.

In dimension 33 we have the following models.

Example 3.8 (The edge).

Let I⊆ℝI\subseteq\mathbb{R} be an open interval. Consider B=ℝ2×IB=\mathbb{R}^{2}\times I and Δ={0}×I\Delta=\{0\}\times I. On B0=(ℝ2−0)×IB_{0}=(\mathbb{R}^{2}-0)\times I we take the product affine structure between the affine structure on ℝ2−0\mathbb{R}^{2}-0 described in the previous example and the standard affine structure on II.

Example 3.9 (A variation).

In the previous example the discriminant locus Δ\Delta was a straight line. We can slightly perturb Δ\Delta so that it becomes a smooth curve. More precisely, let B=ℝ2×IB=\mathbb{R}^{2}\times I as before and consider a smooth function τ:I→ℝ\tau:I\rightarrow\mathbb{R}. Let

Δτ={(τ⁡(s),0,s),s∈I}⊂B\Delta_{\tau}=\{(\tau(s),0,s),s\in I\}\subset B

and define a covering {Ui}\{U_{i}\} of B0=B−ΔτB_{0}=B-\Delta_{\tau} to be

U1=(ℝ2×I)−{(x1,0,s)|x1≥τ⁡(s)},U_{1}=(\mathbb{R}^{2}\times I)-\{(x_{1},0,s)\ |\ x_{1}\geq\tau(s)\},
U2=(ℝ2×I)−{(x1,0,s)|x1≤τ⁡(s)}.U_{2}=(\mathbb{R}^{2}\times I)-\{(x_{1},0,s)\ |\ x_{1}\leq\tau(s)\}.

Now let H+={x2>0}H^{+}=\{x_{2}>0\} and H−={x2<0}H^{-}=\{x_{2}<0\}. Take the following matrix

T=(100110001)T=\left(\begin{array}[]{ccc}1&0&0\\ 1&1&0\\ 0&0&1\end{array}\right)

and define maps ϕj\phi_{j} on UjU_{j} to be

ϕ1\displaystyle\phi_{1} =\displaystyle= Id\displaystyle\mathrm{Id}
ϕ2\displaystyle\phi_{2} =\displaystyle= {Idon​H¯+∩U2,(T−1)ton​H−.\displaystyle\left\{\begin{array}[]{ll}\mathrm{Id}&\text{on}\ \bar{H}^{+}\cap U_{2},\\ (T^{-1})^{t}&\text{on}\ H^{-}.\end{array}\right.

Clearly 𝒜={Ui,ϕi}i=1,2\mathscr{A}=\{U_{i},\phi_{i}\}_{i=1,2} defines an affine structure on B0=B−ΔτB_{0}=B-\Delta_{\tau}. When τ=0\tau=0, this example coincides with the previous one. Notice that the curve (τ⁡(s),0,s)(\tau(s),0,s) is contained inside the 22-plane {x2=0}\{x_{2}=0\}, which can be viewed as an integral surface of the distribution spanned by the vectors in T​B0TB_{0} which are invariant with respect to the holonomy representation ρ\rho on T​B0TB_{0}. Two different curves give non-isomorphic singular affine structures, unless the curves can be taken one into the other via an integral affine transformation.

Example 3.10 (Positive vertex).

Take B=ℝ×ℝ2B=\mathbb{R}\times\mathbb{R}^{2}, with coordinates (x1,x2,x3)(x_{1},x_{2},x_{3}) and identify ℝ2\mathbb{R}^{2} with {0}×ℝ2\{0\}\times\mathbb{R}^{2}. Inside ℝ2\mathbb{R}^{2} consider the cone over three points:

Δ={x2=0,x3≤0}∪{x3=0,x2≤0}∪{x2=x3,x3≥0}.\Delta=\{x_{2}=0,\,x_{3}\leq 0\}\cup\{x_{3}=0,\,x_{2}\leq 0\}\cup\{x_{2}=x_{3},\,x_{3}\geq 0\}.

Now define closed sets in BB

R\displaystyle R =\displaystyle= ℝ×Δ,\displaystyle\mathbb{R}\times\Delta,
R+\displaystyle R^{+} =\displaystyle= ℝ≥0×Δ,\displaystyle\mathbb{R}_{\geq 0}\times\Delta,
R−\displaystyle R^{-} =\displaystyle= ℝ≤0×Δ,\displaystyle\mathbb{R}_{\leq 0}\times\Delta,

and consider the following cover {Ui}\{U_{i}\} of ℝ3−Δ\mathbb{R}^{3}-\Delta:

U1\displaystyle U_{1} =\displaystyle= ℝ3−R+,\displaystyle\mathbb{R}^{3}-R^{+},
U2\displaystyle U_{2} =\displaystyle= ℝ3−R−.\displaystyle\mathbb{R}^{3}-R^{-}.

It is clear that U1∩U2U_{1}\cap U_{2} has the following three connected components

V1\displaystyle V_{1} =\displaystyle= {x2<0,x3<0},\displaystyle\{x_{2}<0,\ x_{3}<0\},
V2\displaystyle V_{2} =\displaystyle= {x2>0,x2>x3},\displaystyle\{x_{2}>0,\ x_{2}>x_{3}\},
V3\displaystyle V_{3} =\displaystyle= {x3>0,x3>x2}.\displaystyle\{x_{3}>0,\ x_{3}>x_{2}\}.

Take two matrices

T1=(110010001),T2=(10−1010001).T_{1}=\left(\begin{array}[]{ccc}1&1&0\\ 0&1&0\\ 0&0&1\end{array}\right),\ \ \ T_{2}=\left(\begin{array}[]{ccc}1&0&-1\\ 0&1&0\\ 0&0&1\end{array}\right). (9)

Now on U1,U2U_{1},U_{2} we define coordinate maps ϕ1\phi_{1}, ϕ2\phi_{2} as follows

ϕ1\displaystyle\phi_{1} =\displaystyle= Id,\displaystyle\I,
ϕ2\displaystyle\phi_{2} =\displaystyle= {Idon​V¯1∩U2,T1−1on​V¯2∩U2T2on​V¯3∩U2\displaystyle\left\{\begin{array}[]{ll}\I&\text{on}\ \bar{V}_{1}\cap U_{2},\\ T_{1}^{-1}&\text{on}\ \bar{V}_{2}\cap U_{2}\\ T_{2}&\text{on}\ \bar{V}_{3}\cap U_{2}\end{array}\right.

Again we see that 𝒜={Ui,ϕi}i=1,2\mathscr{A}=\{U_{i},\phi_{i}\}_{i=1,2} gives an affine structure on B0=ℝ3−ΔB_{0}=\mathbb{R}^{3}-\Delta. One can compute that given a point b∈B0b\in B_{0} and closed paths g1g_{1}, g2g_{2} and g3g_{3} as in Figure 3, we can choose a basis of Tb∗​B0T^{\ast}_{b}B_{0} with respect to which the holonomy matrices satisfy ρ∗​(gj)=(Tj−1)t\rho^{\ast}(g_{j})=(T_{j}^{-1})^{t} for j=1,2,3j=1,2,3.

Example 3.11 (A variation).

In the previous example, Δ\Delta was a graph with three edges meeting in one vertex. All three edges were straight lines. In the spirit of Example 3.9 we can perturb each edge of Δ\Delta to a smooth curve starting at the vertex. Each straight edge of the previous example is contained in a 22-plane which is an integral plane of the distribution spanned by the vectors which are invariant with respect to the holonomy around that edge. For example, consider the edge E1={x1=x2=0,x3≤0}E_{1}=\{x_{1}=x_{2}=0,x_{3}\leq 0\} of Δ\Delta. Then E1E_{1} is contained inside the half plane, P1={x2=0,x3≤0}P_{1}=\{x_{2}=0,x_{3}\leq 0\}, whose tangent vectors are T1T_{1} invariant, where T1=ρ⁡(g1)T_{1}=\rho(g_{1}) is the holonomy of TB0T_{B_{0}} with respect to E1E_{1}. An analogous thing happens with the other two edges. The union of all three half planes gives RR. The new perturbed edges, Ej′E_{j}^{\prime}, must be curves inside the half planes PjP_{j}. More precisely, let τ\tau be a function on Δ\Delta which is the restriction of a smooth function defined on an open neighborhood of Δ\Delta, such that τ⁡(0)=0\tau(0)=0. If we let RR be as in the previous example, define

Δτ\displaystyle\Delta_{\tau} =\displaystyle= {(τ(q),q)∈ℝ×Δ}\displaystyle\{(\tau(q),q)\in\mathbb{R}\times\Delta\}
R+\displaystyle R^{+} =\displaystyle= {(x1,q)∈ℝ×Δ|x1≥τ⁡(q)}\displaystyle\{(x_{1},q)\in\mathbb{R}\times\Delta\ |x_{1}\geq\tau(q)\}
R−\displaystyle R^{-} =\displaystyle= {(x1,q)∈ℝ×Δ|x1≤τ⁡(q)}\displaystyle\{(x_{1},q)\in\mathbb{R}\times\Delta\ |x_{1}\leq\tau(q)\}

Now charts 𝒜={Ui,ϕi}i=1,2\mathscr{A}=\{U_{i},\phi_{i}\}_{i=1,2} on B−ΔτB-\Delta_{\tau} can be defined like in the previous example, but with these new definitions of R+R^{+} and R−R^{-}. It is clear that (B,Δτ,𝒜)(B,\Delta_{\tau},\mathscr{A}) defines an affine manifold with singularities. Two different choices of functions τ\tau define non-isomorphic integral affine manifolds with singularities, unless their graphs inside RR can be mapped one to the other via an integral affine map.

Example 3.12 (Negative vertex).

Let BB and Δ\Delta be as in Example 3.10. Clearly, ℝ2−Δ\mathbb{R}^{2}-\Delta has three connected components, which we denote C1,C2C_{1},C_{2} and C3C_{3}. Let C¯j=Cj∪∂Cj\bar{C}_{j}=C_{j}\cup\partial C_{j}. Viewing ℝ2\mathbb{R}^{2} embedded in BB as {0}×ℝ2\{0\}\times\mathbb{R}^{2}, consider the following three open subsets of B0B_{0}:

U1\displaystyle U_{1} =\displaystyle= ℝ3−(C¯2∪C¯3),\displaystyle\mathbb{R}^{3}-(\bar{C}_{2}\cup\bar{C}_{3}),
U2\displaystyle U_{2} =\displaystyle= ℝ3−(C¯1∪C¯3),\displaystyle\mathbb{R}^{3}-(\bar{C}_{1}\cup\bar{C}_{3}),
U3\displaystyle U_{3} =\displaystyle= ℝ3−(C¯1∪C¯2).\displaystyle\mathbb{R}^{3}-(\bar{C}_{1}\cup\bar{C}_{2}).

Let

V+\displaystyle V^{+} =\displaystyle= {x1>0},\displaystyle\{x_{1}>0\},
V−\displaystyle V^{-} =\displaystyle= {x1<0}.\displaystyle\{x_{1}<0\}.

Clearly Ui∩Uj=V+∪V−U_{i}\cap U_{j}=V^{+}\cup V^{-} when i≠ji\neq j. If T1T_{1} and T2T_{2} are as in (9), define the following coordinate charts on U1U_{1}, U2U_{2}, U3U_{3} respectively:

ϕ1\displaystyle\phi_{1} =\displaystyle= Id,\displaystyle\I,
ϕ2\displaystyle\phi_{2} =\displaystyle= {(T1−1)ton​V¯+∩U2Idon​V¯−∩U2\displaystyle\left\{\begin{array}[]{ll}(T_{1}^{-1})^{t}&\text{on}\ \bar{V}^{+}\cap U_{2}\\ \I&\text{on}\ \bar{V}^{-}\cap U_{2}\end{array}\right.
ϕ3\displaystyle\phi_{3} =\displaystyle= {Idon​V¯+∩U3(T2−1)ton​V¯−∩U3\displaystyle\left\{\begin{array}[]{ll}\I&\text{on}\ \bar{V}^{+}\cap U_{3}\\ (T_{2}^{-1})^{t}&\text{on}\ \bar{V}^{-}\cap U_{3}\end{array}\right.

We can check that the affine structure defined by these charts is such that, for fixed b∈B0b\in B_{0}, there exists a basis of Tb∗​B0T^{\ast}_{b}B_{0} with respect to which the holonomy representation is such that ρ∗​(gj)=Tj\rho^{\ast}(g_{j})=T_{j}, where gjg_{j} are as in Figure 3. In particular, the holonomy is given by the inverse transpose matrices of the holonomy in the previous example.

Example 3.13 (A variation).

Again, we can perturb the above example by replacing the straight edges of Δ\Delta with smooth curves starting at the origin. This time these curves have to be contained inside {0}×ℝ2\{0\}\times\mathbb{R}^{2}, which is the integral surface (containing Δ\Delta) of the distribution spanned by the ρ\rho-holonomy invariant vectors in T​B0TB_{0}. The perturbed Δ\Delta, which we could denote Δτ\Delta_{\tau}, still separates ℝ2\mathbb{R}^{2} in three connected components C1,C2C_{1},C_{2} and C3C_{3}. Then the definition of the affine structure carries through just like in the previous example and we denote it by 𝒜τ\mathscr{A}_{\tau}.

We are now ready to give a definition of the specific affine structures with singularities which we will consider.

Definition 3.14.

A 22-dimensional affine manifold with singularities (B,Δ,𝒜)(B,\Delta,\mathscr{A}) is said to be simple if Δ\Delta consists of a finite union of isolated points and a neighborhood of each p∈Δp\in\Delta is affine isomorphic to a neighborhood of 0∈ℝ20\in\mathbb{R}^{2} as in Example 3.7. We call p∈Δp\in\Delta a node. A 33-dimensional affine manifold with singularities (B,Δ,𝒜)(B,\Delta,\mathscr{A}) is simple if it satisfies:

  • (i)

    Δ\Delta is a trivalent graph;

  • (ii)

    a neighborhood of each vertex of Δ\Delta is affine isomorphic to a neighborhood of 0∈ℝ30\in\mathbb{R}^{3} in either Examples 3.10 or 3.11, in which case we call it a positive vertex; or to a neighborhood of 0∈ℝ30\in\mathbb{R}^{3} in either Examples 3.12 or 3.13, in which case we call it a negative vertex;

  • (iii)

    a neighborhood of each edge of the graph is affine isomorphic to a neighborhood of Δ\Delta in Example 3.8; or a neighborhood of Δτ\Delta_{\tau} in Example 3.9 for a suitable τ\tau.

The following is direct consequence of the above definition and Theorem 2.11:

Corollary 3.15.

Let (B,Δ,𝒜)(B,\Delta,\mathscr{A}) be a simple affine manifold with singularities and let (B0,𝒜)(B_{0},\mathscr{A}) be the underlying integral affine manifold. Then

f0:X⁡(B0,𝒜)→B0f_{0}:X(B_{0},\mathscr{A})\rightarrow B_{0}

is a TnT^{n} bundle with semi-stable monodromy as in Theorem 2.11. In particular, there is an 2​n2n-manifold XX and a topological semi-stable compactification X⁡(B0,𝒜)↪XX(B_{0},\mathscr{A})\hookrightarrow X. Furthermore, the topological fibration f:X→Bf:X\rightarrow B obtained is topologically simple.

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