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Quiver algebras as Fukaya categories

Ivan Smith Ivan Smith, Centre for Mathematical Sciences, University of Cambridge, England.
Abstract.

We embed triangulated categories defined by quivers with potential arising from ideal triangulations of marked bordered surfaces into Fukaya categories of quasi-projective 3-folds associated to meromorphic quadratic differentials. Together with previous results, this yields non-trivial computations of spaces of stability conditions on Fukaya categories of symplectic six-manifolds.

The author was partially supported by grant ERC-2007-StG-205349 from the European Research Council.

1. Introduction

A marked bordered surface (𝕊,𝕄)(\mathbb{S},\mathbb{M}) comprises a compact, connected oriented surface 𝕊\mathbb{S}, perhaps with non-empty boundary, together with a non-empty set 𝕄𝕊\mathbb{M}\subset\mathbb{S} of marked points, such that every boundary component of 𝕊\mathbb{S} contains at least one marked point. We always assume that (𝕊,𝕄)(\mathbb{S},\mathbb{M}) is not a sphere with fewer than five marked points. An ideal triangulation of (𝕊,𝕄)(\mathbb{S},\mathbb{M}) gives rise, via work of Labardini-Fragoso [32], to a quiver with potential. The CY3 -triangulated category 𝒟(𝕊,𝕄){\mathcal{D}}(\mathbb{S},\mathbb{M}) of finite-dimensional modules over the corresponding Ginzburg algebra depends only on the underlying data (𝕊,𝕄)(\mathbb{S},\mathbb{M}). This paper embeds these categories, under mild hypotheses on (𝕊,𝕄)(\mathbb{S},\mathbb{M}), into Fukaya categories of quasi-projective 3-folds. The 3-folds are the total spaces of affine conic fibrations over 𝕊\mathbb{S}; whilst these spaces have not appeared previously in the literature, they are close cousins of those studied in [8]. Together with the main results of [5], we therefore obtain computations of spaces of stability conditions on (distinguished subcategories of) Fukaya categories of symplectic six-manifolds.

We work over an algebraically closed field kk of characteristic zero. For much of the paper, we take kk to be the single variable Novikov field (with formal parameter qq),

(1.1) Λ={ciqmi|ci,mi,limimi=+}\Lambda_{\mathbb{C}}\ =\ \left\{\sum c_{i}q^{m_{i}}\ \big{|}\ c_{i}\in\mathbb{C},\,m_{i}\in\mathbb{R},\,\lim_{i\rightarrow\infty}m_{i}=+\infty\right\}

which is algebraically closed by [15, Lemma 13.1].

1.1. Surfaces and differentials

Let (𝕊,𝕄)(\mathbb{S},\mathbb{M}) be a marked bordered surface. An ideal triangulation TT of 𝕊\mathbb{S} with vertices at 𝕄\mathbb{M} has an associated quiver with potential (Q(T),W(T))(Q(T),W(T)), which can be defined over any algebraically closed field kk. The construction is indicated schematically in the case where TT is non-degenerate in Figure 1 and Equation (2.2), and defined more generally in [32]. There is a triangulated CY3 category 𝒟(T){\mathcal{D}}(T) of finite type (i.e. cohomologically finite) over kk defined by the Ginzburg algebra construction [19]; this has a distinguished heart, equivalent to the category of finite-dimensional modules for the complete Jacobi algebra of the quiver with potential (Q(T),W(T))(Q(T),W(T)). Results of Keller-Yang and Labardini-Fragoso imply that 𝒟(T){\mathcal{D}}(T) depends up to quasi-isomorphism only on the underlying marked bordered surface (𝕊,𝕄)(\mathbb{S},\mathbb{M}). We write 𝒟(𝕊,𝕄){\mathcal{D}}(\mathbb{S},\mathbb{M}) for any category in this equivalence class.

A meromorphic quadratic differential ϕ\phi on a Riemann surface SS has an associated marked bordered surface (𝕊,𝕄)(\mathbb{S},\mathbb{M}). The surface 𝕊\mathbb{S} is obtained as the real blow-up of SS at poles of ϕ\phi of order 3\geqslant 3; the distinguished tangent directions of the horizontal foliation of ϕ\phi define boundary marked points in 𝕄\mathbb{M}, and poles of order 2\leqslant 2 define the punctures (interior marked points) 𝕄\operatorname{\mathbb{P}}\subset\mathbb{M}. We will write Pol(ϕ)\mathrm{Pol}(\phi) for the set of poles, and Poli(ϕ)\mathrm{Pol}_{\geqslant i}(\phi), Pol=2(ϕ)\mathrm{Pol}_{=2}(\phi) for poles of constrained or specified orders. For qPol(ϕ)q\in\mathrm{Pol}(\phi) let ord(q)ord(q) denote the order of the corresponding pole.

All quadratic differentials considered in this paper have simple zeroes.

Let Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M}) denote the complex orbifold parametrizing equivalence classes of pairs comprising a Riemann surface SS and a meromorphic quadratic differential ϕ\phi with simple zeroes whose associated marked bordered surface is diffeomorphic to (𝕊,𝕄)(\mathbb{S},\mathbb{M}). This has an open dense subset Quad(𝕊,𝕄)0\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0} of pairs where the differential ϕ\phi has poles of order exactly 22 at \operatorname{\mathbb{P}}, or equivalently for which the flat metric defined by ϕ\phi is complete. There is an unramified 2||:12^{|\operatorname{\mathbb{P}}|}:1 cover Quad±(𝕊,𝕄)0Quad(𝕊,𝕄)0\operatorname{Quad}^{\pm}(\mathbb{S},\mathbb{M})_{0}\rightarrow\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0} whose points are signed meromorphic differentials, meaning that we fix a choice of sign of the residue of the differential ϕ\phi at each double pole; the cover extends as a ramified cover Quad±(𝕊,𝕄)Quad(𝕊,𝕄)\operatorname{Quad}^{\pm}(\mathbb{S},\mathbb{M})\rightarrow\operatorname{Quad}(\mathbb{S},\mathbb{M}).

1.2. The threefolds

Fix a signed complete differential (S,ϕ)Quad±(𝕊,𝕄)0(S,\phi)\in\operatorname{Quad}^{\pm}(\mathbb{S},\mathbb{M})_{0}. Denote by MM the divisor pPol(ϕ)ord(p)/2p\sum_{p\in\mathrm{Pol}(\phi)}\lceil ord(p)/2\rceil p on SS, where α\lceil\alpha\rceil denotes the smallest integer greater than or equal to α\alpha, and write

(1.2) M=M=2+M3M=M_{=2}+M_{\geqslant 3}

corresponding to the obvious decomposition Pol(ϕ)=Pol=2Pol3\mathrm{Pol}(\phi)=\mathrm{Pol}_{=2}\amalg\mathrm{Pol}_{\geqslant 3}. Take a rank two holomorphic vector bundle VV on SS with det(V)=KS(M)\det(V)=K_{S}(M). We perform an elementary modification of the vector bundle Sym2(V)\mathrm{Sym}^{2}(V) at each double pole pp of ϕ\phi, to obtain a rank three bundle WW fitting into a short exact sequence

0WSym2(V)𝒪M=20.0\longrightarrow W\longrightarrow\mathrm{Sym}^{2}(V)\longrightarrow\mathcal{O}_{M_{=2}}\longrightarrow 0.

We then remove from SS all poles of ϕ\phi of order 3\geqslant 3.

The determinant map det:Sym2(V)KS(M)2\det\colon\mathrm{Sym}^{2}(V)\longrightarrow K_{S}(M)^{\otimes 2} restricts to a quadratic map detW\det_{W} on the bundle WW which is rank one at points of M=2SM_{=2}\subset S. The threefold

Yϕ={detWπϕ=0}W|SPol3(ϕ)Y_{\phi}=\big{\{}{\det}_{W}-\pi^{*}\phi=0\big{\}}\subset W|_{S-\mathrm{Pol}_{\geqslant 3}(\phi)}

is an affine conic fibration over SPol3(ϕ)S-\mathrm{Pol}_{\geqslant 3}(\phi), with nodal fibres over the zeroes of ϕ\phi, fibres singular at infinity over the double poles, and empty fibres over higher order poles. The topology of the fibre over a double pole pp depends on the choice of elementary modification. A choice of line in the fibre of VV at pp determines a distinguished elementary modification, with the property that the resulting fibre of YϕY_{\phi} at pp is isomorphic to the disjoint union of two planes p,+2p,2\mathbb{C}^{2}_{p,+}\amalg\mathbb{C}^{2}_{p,-}. We will always consider elementary modifications with this property.

1.3. The result

We fix a linear Kähler form on (W𝒪)\mathbb{P}(W\oplus\mathcal{O}). This induces a Kähler form ω\omega on YϕY_{\phi}. A Moser-type argument, see Lemma 3.17, shows that (having fixed the parameters determining the cohomology class of the Kähler form appropriately) the symplectic manifold underlying YϕY_{\phi} depends up to isomorphism only on the pair (𝕊,𝕄)(\mathbb{S},\mathbb{M}). YϕY_{\phi} has vanishing first Chern class, and ϕ\phi determines a distinguished homotopy class η(ϕ)\eta(\phi) of trivialisation of the canonical bundle of YϕY_{\phi}.

When 𝕊\partial\mathbb{S}\neq\emptyset, the Kähler form ω\omega is exact, and YϕY_{\phi} has a well-defined exact Fukaya category (Yϕ)\mathcal{F}(Y_{\phi}), which may be constructed over any field kk, see [47]. More generally, we will consider Lagrangian submanifolds LYϕL\subset Y_{\phi} with the following property: there is an almost complex structure JLJ_{L} on YϕY_{\phi}, taming the symplectic form and co-inciding with the given integrable structure at infinity, for which LL bounds no JLJ_{L}-holomorphic disk and does not meet any JLJ_{L}-holomorphic sphere. For ease of notation, we will refer to such (L,JL)(L,J_{L}) as strictly unobstructed. When 𝕊\mathbb{S} is closed, YϕY_{\phi} has a strictly unobstructed Fukaya category (which we again denote by) (Yϕ)\mathcal{F}(Y_{\phi}), now defined over the Novikov field Λ\Lambda_{\mathbb{C}}. This version of the Fukaya category appears, for instance, in [2] and [49]. The strictly unobstructed hypothesis rules out bubbling of holomorphic disks, which simplifies the technical construction of (Yϕ)\mathcal{F}(Y_{\phi}), see [49, Sections 3b, 3c] for a detailed discussion under slightly weaker hypotheses.

Let YY be a symplectic manifold with well-defined Fukaya category (Y)\mathcal{F}(Y). For each bH2(Y;2)b\in H^{2}(Y;\mathbb{Z}_{2}), there is a category (Y;b)\mathcal{F}(Y;b), the bb-twisted strictly unobstructed Fukaya category, which for b=0b=0 recovers the category considered previously. Objects of (Y;b)\mathcal{F}(Y;b) are closed oriented graded strictly unobstructed Lagrangians LL, which are equipped with a relative spin structure111In other words, b|L=w2(TL)b|_{L}=w_{2}(TL) and we fix a trivialisation of ξBTL\xi_{B}\oplus TL over the 2-skeleton of LL, where ξbY\xi_{b}\rightarrow Y is the unique real 2-plane bundle with w1(ξb)=0w_{1}(\xi_{b})=0 and w2(ξb)=bw_{2}(\xi_{b})=b., relative to the background class bb. The choice of background class bH2(Y;2)b\in H^{2}(Y;\mathbb{Z}_{2}) serves to change the signs with which holomorphic polygons contribute to the AA_{\infty}-operations μd\mu^{d}_{\mathcal{F}}, and can be seen as fixing a particular coherent orientation scheme for the Fukaya category; compare to [47, Section 11 & Remark 12.1].

Each category (Yϕ;b)\mathcal{F}(Y_{\phi};b) is a \mathbb{Z}-graded AA_{\infty}-category, linear over the appropriate field kk. Let 𝒟𝒞{\mathcal{D}}\,\mathcal{C} denote the cohomological category H0(Tw𝒞)H^{0}(\mathrm{Tw}\,\mathcal{C}) of the category of twisted complexes over an AA_{\infty}-category 𝒞\mathcal{C}.

Now consider the threefold YϕSY_{\phi}\rightarrow S. For each pMSp\in M\subset S, the fibre π1(p)\pi^{-1}(p) is reducible. Let +,p2\mathbb{C}^{2}_{+,p} denote one component of this fibre. We fix the background class b0H2(Yϕ;2)b_{0}\in H^{2}(Y_{\phi};\mathbb{Z}_{2}) represented by the locally finite cycle

(1.3) b0=pM=2p,+2H4lf(Yϕ;2)H2(Yϕ;2)b_{0}=\sum_{p\in M_{=2}}\mathbb{C}^{2}_{p,+}\ \in H_{4}^{\operatorname{lf}}(Y_{\phi};\mathbb{Z}_{2})\cong H^{2}(Y_{\phi};\mathbb{Z}_{2})

given by (either) one of the components of the reducible fibre at each point of Pol=2(ϕ)\mathrm{Pol}_{=2}(\phi), or equivalently each point of \operatorname{\mathbb{P}}. The class is non-trivial by Lemma 3.11. Different choices of cycle representative for b0b_{0} are related by monodromy by Lemma 3.12.

Theorem 1.1.

Let (𝕊,𝕄)(\mathbb{S},\mathbb{M}) be a marked bordered surface, with 𝕄\mathbb{M}\neq\emptyset. Suppose either

  1. (1)

    𝕊\mathbb{S} is closed, g(𝕊)>0g(\mathbb{S})>0, |𝕄|3|\mathbb{M}|\geqslant 3, and k=Λk=\Lambda_{\mathbb{C}}; or

  2. (2)

    𝕊\partial\mathbb{S}\neq\emptyset, and 𝕊\mathbb{S} is not a sphere with fewer than five punctures.

There is a kk-linear fully faithful embedding 𝒟(𝕊,𝕄)𝒟(Yϕ;b0).{\mathcal{D}}(\mathbb{S},\mathbb{M})\hookrightarrow{\mathcal{D}}\mathcal{F}(Y_{\phi};b_{0}).

The untwisted Fukaya category (Yϕ)\mathcal{F}(Y_{\phi}), which differs from (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}) by certain signs, is different, and is discussed in Section 5.4.

One drawback of Theorem 1.1 is that it does not give a symplectic characterisation of the image of the embedding 𝒟(𝕊,𝕄)𝒟(Yϕ;b0){\mathcal{D}}(\mathbb{S},\mathbb{M})\hookrightarrow{\mathcal{D}}\mathcal{F}(Y_{\phi};b_{0}). There is an obvious candidate for such a characterisation, which we now explain.

Any embedded path γ:[0,1]S\gamma:[0,1]\rightarrow S, with end-points distinct zeroes of ϕ\phi and otherwise disjoint from the zeroes and poles of ϕ\phi, defines a Lagrangian 3-sphere LγYϕL_{\gamma}\subset Y_{\phi}, fibred over the arc γΣ\gamma\subset\Sigma via Donaldson’s “matching cycle” construction [47, III, Section 16g]. The matching spheres LγL_{\gamma} are exact if 𝕊,\partial\mathbb{S}\neq\emptyset, and strictly unobstructed (with JLJ_{L} the canonical complex structure on YϕY_{\phi}) when 𝕊\mathbb{S} is closed and g(𝕊)>0g(\mathbb{S})>0. A Lagrangian sphere is relatively spin for any choice of background class bb, hence equipped with a grading defines a Lagrangian brane in (Yϕ;b)\mathcal{F}(Y_{\phi};b). A non-degenerate ideal triangulation TT of SS defines a full subcategory 𝒜(T;b)(Yϕ;b)\mathcal{A}(T;b)\subset\mathcal{F}(Y_{\phi};b), generated by the matching spheres associated to the edges of the cellulation dual to TT. Theorem 1.1 is proved by showing that 𝒟𝒜(T;b0)𝒟(T){\mathcal{D}}\mathcal{A}(T;b_{0})\simeq{\mathcal{D}}(T) for particularly well-behaved triangulations TT. Since the category 𝒟(T){\mathcal{D}}(T) does not depend on TT, it follows that 𝒟𝒜(T;b0){\mathcal{D}}\mathcal{A}(T;b_{0}) also depends only on the pair (𝕊,𝕄)(\mathbb{S},\mathbb{M}), up to triangulated equivalence.

Let 𝒦(Yϕ;b0)(Yϕ;b0)\mathcal{K}(Y_{\phi};b_{0})\subset\mathcal{F}(Y_{\phi};b_{0}) be the full AA_{\infty}-subcategory generated by Lagrangian matching spheres. This manifestly depends only on the pair (𝕊,𝕄)(\mathbb{S},\mathbb{M}). It seems likely that 𝒟(𝕊,𝕄)𝒟𝒦(Yϕ;b0){\mathcal{D}}(\mathbb{S},\mathbb{M})\simeq{\mathcal{D}}\mathcal{K}(Y_{\phi};b_{0}). We outline one tentative approach to proving that, which amounts to proving that 𝒜(T;b0)\mathcal{A}(T;b_{0}) generates 𝒦(Yϕ;b0)\mathcal{K}(Y_{\phi};b_{0}), in Section 4.9, but elaborating the details of that sketch would be a substantial task. Going further, it seems likely that all Lagrangian spheres in YϕY_{\phi} are quasi-isomorphic to matching spheres (the result is proved in special cases in [2, 50]), in which case the category 𝒟𝒦(Yϕ;b0){\mathcal{D}}\mathcal{K}(Y_{\phi};b_{0}) would be a symplectic invariant of YϕY_{\phi}, carrying an action of the subgroup of π0Symp(Yϕ)\pi_{0}\mathrm{Symp}(Y_{\phi}) preserving the class b0H2(Yϕ;2)b_{0}\in H^{2}(Y_{\phi};\mathbb{Z}_{2}). The question of whether the embedding 𝒦(Yϕ;b0)(Yϕ;b0)\mathcal{K}(Y_{\phi};b_{0})\hookrightarrow\mathcal{F}(Y_{\phi};b_{0}) itself split-generates is also open, though here there seems to be less evidence either way. We hope to return to these questions elsewhere.

The imposed condition 𝕄\mathbb{M}\neq\emptyset gives a substantial simplication since holomorphic polygons are constrained for grading considerations that do not pertain when ϕ\phi is globally holomorphic, cf. Remarks 3.22 and 4.15. The constraint on the number of punctures |𝕄|3|\mathbb{M}|\geqslant 3 when 𝕊\mathbb{S} is closed arises from a similar constraint in work of Geiss, Labardini-Fragoso and Schröer [18], who study the action of right equivalences on potentials on the quivers Q(T)Q(T), cf. Theorem 2.1. We conjecture that, for a closed surface 𝕊\mathbb{S} of genus g(𝕊)>0g(\mathbb{S})>0, Theorem 1.1 holds under the weaker hypothesis |𝕄|>1|\mathbb{M}|>1. (Once-punctured surfaces are special: not every pair of signed ideal triangulations are related by pops and flips, and when g=1g=1 the analogue of Theorem 2.1 is actually false, cf. [18].)

One can relax the strict unobstructedness hypothesis at the cost of invoking the deep obstruction theory of [14] in the construction of (Yϕ;b)\mathcal{F}(Y_{\phi};b). If 𝕊\mathbb{S} is closed and g(𝕊)=0g(\mathbb{S})=0 then YϕY_{\phi} may contain rational curves, so only the more complicated construction is available. This is the reason for the genus constraint in the first part of Theorem 1.1.

Remark 1.2.

The elementary modifications appearing in the specific construction of YϕY_{\phi} play a definite role in reproducing 𝒟(𝕊,𝕄){\mathcal{D}}(\mathbb{S},\mathbb{M}), which seems somewhat less natural from the viewpoint of the symplectic topology of the original bordered surface (𝕊,𝕄)(\mathbb{S},\mathbb{M}), not least because of the CY3 property. The particular choice of elementary modification that we employ was motivated by two considerations: first, to yield the Calabi-Yau property of Lemma 3.5, and second, to ensure the non-vanishing of a certain count of local holomorphic sections over discs centred on double poles in Lemma 4.10. (The latter result would fail if instead one took the threefold YϕY_{\phi} to have smooth, nodal, higher multiplicity or empty fibres over the double poles, and also accounts for the appearance of the twisting class b0b_{0}.) At a more technical level, the appearance of a reducible fibre whose components are exchanged by the local monodromy of the family of threefolds obtained by allowing the residue at a double pole to wind once around the origin, cf. Lemma 3.12, fits well with the appearance of “signed” quadratic differentials in [5, Section 6.2].

1.4. Context

In many cases, the paper [5] computes the space of stability conditions on the category 𝒟(𝕊,𝕄){\mathcal{D}}(\mathbb{S},\mathbb{M}) in terms of moduli spaces of quadratic differentials. If either 𝕊\mathbb{S} is closed with g(𝕊)>0g(\mathbb{S})>0 and with at least two punctures, or 𝕊\partial\mathbb{S}\neq\emptyset and 𝕊\mathbb{S} is not a sphere with fewer than six punctures, there is a connected component StabΔ(𝕊,𝕄)\operatorname{Stab}_{\Delta}(\mathbb{S},\mathbb{M}) of Stab(𝒟(𝕊,𝕄))\operatorname{Stab}({\mathcal{D}}(\mathbb{S},\mathbb{M})) and a subgroup AutΔ\mathrm{Aut}_{\Delta} of autoequivalences which preserve this component modulo those which act trivially upon it, with

StabΔ(𝕊,𝕄)/AutΔQuad(𝕊,𝕄)\operatorname{Stab}_{\Delta}(\mathbb{S},\mathbb{M})/\mathrm{Aut}_{\Delta}\ \cong\ \operatorname{Quad}_{\heartsuit}(\mathbb{S},\mathbb{M})

where Quad(𝕊,𝕄)\operatorname{Quad}_{\heartsuit}(\mathbb{S},\mathbb{M}) has the same coarse moduli space as Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M}) but additional orbifolding along the incomplete locus, see [5] for details. This gives a non-trivial computation of the space of stability conditions on (a subcategory of) the Fukaya category of a symplectic six-manifold, and enables one to understand the Donaldson-Thomas invariants of these categories.

One can construct a complex (3,0)-form Ω\Omega on YϕY_{\phi} with the following property: if the path γΣ\gamma\subset\Sigma is a saddle connection for ϕ\phi, the associated matching sphere LγL_{\gamma} is special, i.e. Ω\Omega has constant phase on LγL_{\gamma}. (We are not working with the Ricci-flat metric, so these are not strictly special in the traditional sense.) There are similarly Ω\Omega-special Lagrangian submanifolds S1×S2S^{1}\times S^{2} of YϕY_{\phi} associated to homotopically non-trivial closed geodesics for the flat metric defined by ϕ\phi. Theorem 1.4 of [5] implies that the Donaldson-Thomas invariants of YϕY_{\phi}, defined with respect to the stability condition associated to ϕ\phi, count such special Lagrangian submanifolds, the existence and numerics of which are therefore governed by the Joyce-Song and Kontsevich-Soibelman wall-crossing formulae [24, 30]. This confirms, in this special case, a long-standing expectation of Joyce and others.

It is natural to conjecture that moduli spaces of holomorphic quadratic differentials with simple zeroes arise as spaces of stability conditions (modulo autoequivalences) on the Fukaya categories of the local threefolds of [8] (see Equation 3.1). However, these categories do not appear to admit descriptions in terms of quivers, and different techniques would be required to analyse them and the corresponding spaces of stability conditions.

1.5. Higher rank

The threefolds YϕY_{\phi} are associated to meromorphic maps of Riemann surfaces into the versal deformation space of the A1A_{1}-surface singularity 2/2\mathbb{C}^{2}/\mathbb{Z}_{2}. There are also local threefolds associated to meromorphic maps to the versal deformation spaces of other ADE singularities: in the case of a holomorphic map, the relevant threefolds are studied in [8, 55]. Already for the A2A_{2}-surface, however, the geometry is substantially more complicated, and the relationship to stability conditions rather less clear.

The natural data required to write down a quasi-projective Calabi-Yau threefold fibred over a Riemann surface SS in the AnA_{n}-case is a tuple comprising (perhaps meromorphic) sections of KSiK_{S}^{\otimes i} for 2in2\leqslant i\leqslant n. For instance, when n=2n=2 and supposing one is working with holomorphic rather than meromorphic differentials, one takes a vector bundle V=L1L2V=L_{1}\oplus L_{2} with det(V)KSdet(V)\cong K_{S}, and considers the hypersurface

(1.4) {(x,y,z)L13L23L1L2|xy+z3=ϕz+ψ}\left\{(x,y,z)\in L_{1}^{3}\oplus L_{2}^{3}\oplus L_{1}L_{2}\ |\ xy+z^{3}=\phi\cdot z+\psi\right\}

where ϕH0(KS2)\phi\in H^{0}(K_{S}^{\otimes 2}) and ψH0(KS3)\psi\in H^{0}(K_{S}^{\otimes 3}). For generic choices of (ϕ,ψ)(\phi,\psi) this is a smooth Calabi-Yau, the total space of a Lefschetz fibration over SS, with generic fibre the Milnor fibre of 2/3\mathbb{C}^{2}/\mathbb{Z}_{3} (symplectically, the plumbing of two copies of TS2T^{*}S^{2}).

However, the moduli space of such data – a complex structure on 𝕊\mathbb{S} and a tuple of differentials – has dimension smaller than the dimension of the space of stability conditions on the corresponding category, or more mundanely smaller than the rank of H3H_{3} of the associated threefold (compare to Remark 3.15). This is a familiar problem: whilst one expects spaces of complex structures on a symplectic Calabi-Yau to embed into the space of stability conditions on the Fukaya category, there is no reason to expect that embedding to be onto an open subset. The fortunate accident in the A1A_{1}-case is that Teichmüller space has the same dimension as the space of quadratic differentials. At least for AnA_{n}-fibred threefolds, it seems natural following [33] to expect the “higher Teichmüller space”, i.e. Hitchin’s contractible component [22] of the variety of flat SL(n,)\mathbb{P}SL(n,\mathbb{R})-connections, to play a role in resolving this discrepancy.

Finally, we note that computations in [17] indicate that the CY3 -categories arising in higher rank (even when one restricts to meromorphic differentials) are appreciably more complicated; whereas the Donaldson-Thomas invariants of the categories studied in this paper are always +1+1 or 2-2, cf. [5], and non-vanishing only for primitive classes, in the higher rank case one expects there are classes [γ][\gamma] for which the DT-invariants (conjecturally related to counts of special Lagrangian submanifolds in the corresponding threefold) in class k[γ]k[\gamma] grow exponentially with kk. The symplectic topology of (1.4) is the subject of work in progress by the author.

1.6. Standing assumptions

The arguments for the two cases of Theorem 1.1 are rather similar. For definiteness, for the rest of the paper we consider the (more complicated) case when 𝕊\mathbb{S} is closed, leaving the required modifications for the case with non-empty boundary to the interested reader.

In the closed case all the marked points 𝕄=𝕊\mathbb{M}=\operatorname{\mathbb{P}}\subset\mathbb{S} are punctures. To avoid transversality issues arising from rational curves and their multiple covers, we also exclude the (interesting) case of threefolds fibring over the 2-sphere. Therefore the discrete topological data will henceforth be indexed by a pair (𝕊,𝕄)(\mathbb{S},\mathbb{M}) with g(𝕊)>0g(\mathbb{S})>0 and #𝕄>0\#\mathbb{M}>0.

Acknowledgements. Tom Bridgeland was originally to be a co-author; his influence is pervasive. I am indebted to Daniel Labardini-Fragoso for explanations of his joint work with Geiss and Schröer [18], on which we rely essentially. Thanks also to Mohammed Abouzaid, Bernhard Keller, Yankl Lekili, Andy Neitzke, Oscar Randal-Williams, Tony Scholl, Paul Seidel, Balazs Szendroi and Richard Thomas for helpful conversations; Abouzaid and Seidel provided assistance with a crucial sign computation. Finally, I am grateful to the anonymous referee for suggesting many improvements to the exposition.

2. Background

2.1. Quivers with potential

Let QQ be a quiver, specified by sets of vertices and arrows Q0Q_{0}, Q1Q_{1}, and source and target maps s,t:Q1Q0s,t\colon Q_{1}\to Q_{0}. We write kQkQ for the path algebra of QQ over the field kk, and kQ^\widehat{kQ} for the completion of kQkQ with respect to path length. A potential on QQ is an element WkQ^W\in\widehat{kQ} of the closure of the subspace of kQ^\widehat{kQ} spanned by all cyclic paths in QQ of length 2\geqslant 2. A potential is called reduced if it lies in the closure of the subspace spanned by cycles of length 3\geqslant 3.

We say that two potentials WW and WW^{\prime} are cyclically equivalent if WWW-W^{\prime} lies in the closure of the subspace generated by differences a1asa2asa1a_{1}\ldots a_{s}-a_{2}\ldots a_{s}a_{1}, where a1asa_{1}\ldots a_{s} is a cycle in the path algebra. WW and WW^{\prime} are right-equivalent if there is an automorphism ϕ:kQ^kQ^\phi:\widehat{kQ}\rightarrow\widehat{kQ} of the completed path algebra which fixes the zero-length paths and such that ϕ(W)\phi(W) and WW^{\prime} are cyclically equivalent. Following [18], we say WW and WW^{\prime} are weakly right equivalent if WW and tWtW^{\prime} are right-equivalent, for some invertible scalar tkt\in k^{*}.

Consider minimal AA_{\infty} categories 𝒞\mathcal{C} whose objects SiS_{i} are indexed by the vertices of QQ, and such that, as a graded vector space

Hom𝒞(Si,Sj)=kδijVij[1]Vji[2]kδij[3],\mathrm{Hom}_{\mathcal{C}}(S_{i},S_{j})=k^{\delta_{ij}}\oplus V^{*}_{ij}[-1]\oplus V_{ji}[-2]\oplus k^{\delta_{ij}}[-3],

where VijV_{ij} is the space with basis consisting of arrows in QQ connecting vertex ii to vertex jj. There is an obvious non-degenerate pairing

,:Hom𝒞(Si,Sj)×Hom𝒞(Sj,Si)k[3].\langle-,-\rangle\colon\mathrm{Hom}_{\mathcal{C}}(S_{i},S_{j})\times\mathrm{Hom}_{\mathcal{C}}(S_{j},S_{i})\to k[-3].

Thus, if we define

cn(fn,,f1)=fn,mn1(fn1,,f1),c_{n}(f_{n},\cdots,f_{1})=\langle f_{n},m_{n-1}(f_{n-1},\cdots,f_{1})\rangle,

an AA_{\infty} product of degree 2(n1)2-(n-1),

mn1:Hom𝒞(Sjn1,Sjn)Hom𝒞(Sj1,Sj2)Hom𝒞(Sj1,Sjn),m_{n-1}\colon\mathrm{Hom}_{\mathcal{C}}(S_{j_{n-1}},S_{j_{n}})\otimes\cdots\otimes\mathrm{Hom}_{\mathcal{C}}(S_{j_{1}},S_{j_{2}})\longrightarrow\mathrm{Hom}_{\mathcal{C}}(S_{j_{1}},S_{j_{n}}),

is equivalently described by a linear map of degree n-n

(2.1) cn:Hom𝒞(Sjn,Sj1)Hom𝒞(Sjn1,Sjn)Hom𝒞(Sj1,Sj2)k.c_{n}\colon\mathrm{Hom}_{\mathcal{C}}(S_{j_{n}},S_{j_{1}})\otimes\mathrm{Hom}_{\mathcal{C}}(S_{j_{n-1}},S_{j_{n}})\cdots\otimes\mathrm{Hom}_{\mathcal{C}}(S_{j_{1}},S_{j_{2}})\longrightarrow k.

Let us insist that 𝒞\mathcal{C} is cyclic as an AA_{\infty} category, meaning that the tensors cnc_{n} are cyclically invariant in the graded sense. If we further insist that the AA_{\infty} structure on 𝒞\mathcal{C} is strictly unital then the whole structure is determined by the elements cn(fn,,f1)c_{n}(f_{n},\cdots,f_{1}) when all the fif_{i} have degree 1. For background on this construction, see [43].

Let WW be a reduced potential on QQ. Decomposing the potential into homogeneous pieces, and cyclically symmetrising, we obtain linear maps

Wn:Vjn,j1Vjn1,jnVj1,j2k.W_{n}\colon V^{*}_{j_{n},j_{1}}\otimes V^{*}_{j_{n-1},j_{n}}\otimes\cdots\otimes V^{*}_{j_{1},j_{2}}\longrightarrow k.

Setting cn=Wnc_{n}=W_{n} gives a well-defined AA_{\infty} category 𝒞(Q,W)\mathcal{C}(Q,W). Define 𝒟(Q,W){\mathcal{D}}(Q,W) to be the homotopy category of the category of twisted complexes over 𝒞(Q,W)\mathcal{C}(Q,W)

𝒟(Q,W)=H0(Tw(𝒞(Q,W)).{\mathcal{D}}(Q,W)=H^{0}(\operatorname{Tw}(\mathcal{C}(Q,W)).

The associated graded category of 𝒟(Q,W){\mathcal{D}}(Q,W) contains 𝒞\mathcal{C} as a full subcategory.

The same category 𝒟(Q,W){\mathcal{D}}(Q,W) admits an alternative (Koszul dual) description in terms of the derived category of a dg algebra A(Q,W)A(Q,W) called the complete Ginzburg algebra (see for instance [30, Theorem 9] or [26, Section 5]). To define it, first double QQ, adding a dual edge aa^{*} for each aQa\in Q, and then add loops tit_{i} based at each vertex ii of QQ. The resulting quiver QQ^{*} has a grading given by

deg(x)=0;deg(x)=1;deg(t)=2.\deg(x)=0;\quad\deg(x^{*})=-1;\quad\deg(t)=-2.

Let A(Q,W)A(Q,W) be the completion of the path algebra kQ^\widehat{kQ^{*}} as a graded algebra, with respect to the ideal generated by the arrows of QQ^{*}. There is a unique continuous differential dd satisfying

d(t)=aQ1ei[a,a]ei,d(a)=aW,d(a)=0.d(t)=\sum_{a\in Q_{1}}e_{i}\cdot[a,a^{*}]\cdot e_{i},\quad d(a^{*})=\partial_{a}W,\quad d(a)=0.

Thus A(Q,W)A(Q,W) is a dg algebra. The category 𝒟(Q,W){\mathcal{D}}(Q,W) can then be equivalently described as the full subcategory of the derived category of the dg algebra A(Q,W)A(Q,W) consisting of finite-dimensional modules. By a general result of Keller and Van den Bergh [27], this description shows that 𝒟(Q,W){\mathcal{D}}(Q,W) is a CY3 triangulated category.

Keller and Yang [28, Lemma 2.9] showed that if WW and WW^{\prime} are right-equivalent potentials, they have isomorphic complete Ginzburg algebras, and hence yield equivalent categories 𝒟(Q,W)𝒟(Q,W){\mathcal{D}}(Q,W)\simeq{\mathcal{D}}(Q,W^{\prime}). Ladkani [34, Proposition 2.7], see also [18, Lemma 8.5], showed that the same conclusion holds when WW and WW^{\prime} are only weakly right-equivalent. Indeed, there is a natural kk^{*}-action on the set of minimal AA_{\infty}-structures on the category 𝒞\mathcal{C}, where λk\lambda\in k^{*} acts by rescaling the operation mnm_{n} by λn2\lambda^{n-2}. AA_{\infty}-structures related by the kk^{*}-action are AA_{\infty}-equivalent even though not gauge-equivalent in the usual sense (the required equivalence does not act by the identity on cohomology but by a multiple of the Euler vector field). The potentials WW and tWtW on QQ give rise to AA_{\infty}-categories 𝒞(Q,W)\mathcal{C}(Q,W) and 𝒞(Q,tW)\mathcal{C}(Q,tW) which are related by the kk^{*}-action. Since AA_{\infty}-equivalences induce equivalences on categories of twisted complexes by [47, Lemma 3.20], the category 𝒟(Q,W){\mathcal{D}}(Q,W) depends only on the weak right equivalence class of WW.

The fact that A(Q,W)A(Q,W) is concentrated in non-positive degrees implies [28, Lemma 5.2] that 𝒟(Q,W){\mathcal{D}}(Q,W) is equipped with a canonical bounded t-structure, whose heart 𝒜(Q,W)\mathcal{A}(Q,W) is equivalent to the category of nilpotent representations of the completed Jacobian algebra

J(Q,W)=H0(A(Q,W))=kQ^/(aW:aQ1).J(Q,W)=H^{0}(A(Q,W))=\widehat{kQ}\big{/}(\partial_{a}W:a\in Q_{1}).

In particular, 𝒜(Q,W)𝒟(Q,W)\mathcal{A}(Q,W)\subset{\mathcal{D}}(Q,W) is a finite-length heart. Since it admits a bounded t-structure, the category 𝒟(Q,W){\mathcal{D}}(Q,W) is split-closed, i.e. agrees with its own idempotent completion, see [35].

2.2. Quivers from triangulated surfaces

Suppose again that 𝕊\mathbb{S} is a closed oriented surface of genus g(𝕊)>0g(\mathbb{S})>0, now equipped with a non-empty set of d2d\geqslant 2 marked points 𝕄𝕊\mathbb{M}\subset\mathbb{S}.

By a non-degenerate ideal triangulation of (𝕊,𝕄)(\mathbb{S},\mathbb{M}) we mean a triangulation of 𝕊\mathbb{S} whose vertex set is precisely 𝕄\mathbb{M}, and in which every vertex has valency at least 33 (this implies that every triangle has three distinct edges). A signed triangulation is a triangulation equipped with a function

ϵ:𝕄{±1}.\epsilon:\mathbb{M}\rightarrow\{\pm 1\}.

We can associate a quiver with potential (Q(T),W(T,ϵ))(Q(T),W(T,\epsilon)) to a signed non-degenerate triangulation TT as follows.

Refer to caption
Figure 1. Quiver associated to a triangulation

The quiver Q(T)Q(T) has vertices at the midpoints of the edges of TT, and is obtained by inscribing a small clockwise 3-cycle inside each face of TT, as in Figure 1. There are two obvious systems of cycles in Q(T)Q(T), namely a clockwise 3-cycle T(f)T(f) in each face ff, and an anticlockwise cycle C(p)C(p) of length at least 3 encircling each point p𝕄p\in\mathbb{M}. Define a potential

(2.2) W(T,ϵ)=fT(f)pϵ(p)C(p).W({T},\epsilon)=\sum_{f}T(f)-\sum_{p}\epsilon(p)C(p).

When ϵ1\epsilon\equiv 1 we will sometimes omit it from the notation.

Consider the derived category of the completed Ginzburg algebra of the quiver with potential (Q(T),W(T,ϵ))(Q(T),W(T,\epsilon)) over kk, and let 𝒟(T,ϵ){\mathcal{D}}(T,\epsilon) be the full subcategory consisting of modules with finite-dimensional cohomology. As a special case of the discussion of Section 2.1, this is a CY3 triangulated category of finite type over kk, and comes equipped with a canonical t-structure, whose heart 𝒜(T,ϵ)𝒟(T,ϵ)\mathcal{A}(T,\epsilon)\subset{\mathcal{D}}(T,\epsilon) is equivalent to the category of finite-dimensional modules for the completed Jacobi algebra of (Q(T),W(T,ϵ))(Q(T),W(T,\epsilon)).

Suppose two non-degenerate ideal triangulations TiT_{i} are related by a flip, in which the diagonal of a quadilateral is replaced by its opposite diagonal. The resulting quivers with potential (Q(Ti),W(Ti,ϵ))(Q(T_{i}),W(T_{i},\epsilon)) (in which the signing is unchanged) are related by a mutation at the vertex corresponding to the edge being flipped. It follows from general results of Keller and Yang [28] that there exist distinguished kk-linear triangulated equivalences Φ±:𝒟(T1,ϵ)𝒟(T2,ϵ)\Phi_{\pm}\colon{\mathcal{D}}(T_{1},\epsilon)\cong{\mathcal{D}}({T}_{2},\epsilon).

Labardini-Fragoso [32] extended the above definitions so as to encompass a larger class of signed ideal triangulations (ones containing self-folded triangles, in which two of the three edges co-incide; in this case there may be punctures of valency one, and the mutation operation can change the signing). He moreover proved that flips also induce right-equivalences in this more general context. There is another operation on signed ideal triangulations, which involves changing the signing at a given puncture without changing the triangulation, and a corresponding “pop” equivalence which relates the associated categories. Under our hypothesis on (𝕊,𝕄)(\mathbb{S},\mathbb{M}) that d=|𝕄|2d=|\mathbb{M}|\geqslant 2, any two of these more general signed ideal triangulations are related by a finite chain of flips and pops. It follows that up to kk-linear triangulated equivalence, the category 𝒟(T,ϵ){\mathcal{D}}(T,\epsilon) is independent of the chosen triangulation and of the choice of signing; see [5, Sections 8 & 9] for a more detailed discussion. We denote by 𝒟(𝕊,𝕄){\mathcal{D}}(\mathbb{S},\mathbb{M}) any triangulated category in this quasi-equivalence class.

Given the quiver Q(T)Q(T), one can define a CY3 category by taking any potential on Q(T)Q(T), not necessarily the potential W(T,ϵ)W(T,\epsilon) described above. We will say that two potentials W1W_{1} and W2W_{2} are disjoint if no cycle occuring in W1W_{1} is cyclically equivalent to a cycle appearing in W2W_{2}. The following result is due to Geiss, Labardini-Fragoso and Schröer [18].

Theorem 2.1.

Let TT be a triangulation of (𝕊,𝕄)(\mathbb{S},\mathbb{M}) which contains no self-folded triangles or loops and in which every vertex has valency at least 4. Suppose that the associated quiver Q(T)Q(T) contains no double arrows. Any two potentials on Q(T)Q(T) of the form

(2.3) fT(f)pλpC(p)+W\sum_{f}T(f)-\sum_{p}\lambda_{p}C(p)+W^{\prime}

(for scalars λp0\lambda_{p}\neq 0 and WW^{\prime} disjoint from the T(f)T(f) and C(p)C(p)) are weakly right equivalent.

Geiss, Labardini-Fragoso and Schröer furthermore prove that every pair (𝕊,𝕄)(\mathbb{S},\mathbb{M}) with g(𝕊)>0g(\mathbb{S})>0 and with |𝕄|3|\mathbb{M}|\geqslant 3 admits some triangulation TT which satisfies the hypotheses, i.e. which contains no self-folded triangle or loop, in which every vertex has valency at least 4, and for which the associated quiver has no double arrow. (In the case when 𝕊\mathbb{S} has non-empty boundary, the same result holds without further hypotheses on the number of punctures.) The proof of Theorem 2.1 involves a delicate, iterative construction of a suitable right-equivalence by hand, obtained as an infinite composition of equivalences which, to first approximation, increase the minimal length of any cycle appearing in the remainder term WW^{\prime}; the actual proof is more complicated than this suggests.

For our purposes, these results yield a finite-determinacy theorem for AA_{\infty}-structures on the total endomorphism algebra of the category 𝒞\mathcal{C} of Section 2.1 in the special case (Q,W)=(Q(T),W(T,ϵ))(Q,W)=(Q(T),W(T,\epsilon)). Considering the description of the category 𝒟(Q,W){\mathcal{D}}(Q,W) as a category of twisted complexes over an AA_{\infty}-algebra given in Section 2.1, Theorem 2.1 implies in particular that different choices of scalars {λp}p\{\lambda_{p}\}_{p\in\operatorname{\mathbb{P}}} for the potential (2.3) yield equivalent categories 𝒟(Q,W){\mathcal{D}}(Q,W), whilst AA_{\infty}-products encoded by the “remainder” term WW^{\prime} can be gauged away.

2.3. Quadratic differentials and flat metrics

Let (S,ϕ)(S,\phi) denote a pair comprising a Riemann surface SS and meromorphic quadratic differential ϕ\phi with poles of order precisely 2 at the points of a divisor MSM\subset S comprising dd reduced points, and with simple zeroes. Thus, the marked bordered surface associated to (S,ϕ)(S,\phi) is diffeomorphic to (𝕊,𝕄)(\mathbb{S},\mathbb{M}). Let ZerϕS\mathrm{Zer}_{\phi}\subset S denote the set of zeroes, so

|Zerϕ|= 4g(S)4+2|M|.|\mathrm{Zer}_{\phi}|\,=\,4g(S)-4+2|M|.

At a point of S\{MZerϕ}S\backslash\{M\cup\mathrm{Zer}_{\phi}\} there is a distinguished local co-ordinate zz with respect to which

ϕ(z)=dzdz.\phi(z)\,=\,dz\otimes dz.

This local co-ordinate is uniquely defined up to changes z±z+constantz\mapsto\pm z+constant. At simple zeroes, respectively double poles, there is a canonical co-ordinate with respect to which

(2.4) ϕ(z)={zdz2atsimplezeroes;mdz2z2atdoublepoles,wherem.\phi(z)\,=\ \begin{cases}z\,dz^{\otimes 2}\quad\mathrm{at\ simple\ zeroes};\\ m\,\frac{dz^{\otimes 2}}{z^{2}}\quad\mathrm{at\ double\ poles,\ where}\ m\in\mathbb{C}^{*}.\end{cases}

We refer to the value mm in the second case as the residue at the double pole.

The surface S\MS\backslash M inherits a flat metric |ϕ|2|\phi|^{2} with singularities; at each pZerϕp\in\mathrm{Zer}_{\phi}, the metric has a cone angle of 3π3\pi. The length element of the metric is defined by

ϕ(w)dw\sqrt{\phi(w)}dw

in an arbitrary local parameter ww, so the length of a curve γS\M\gamma\subset S\backslash M is given by

|γ|ϕ=γ|ϕ(w)|1/2|dw|.|\gamma|_{\phi}\ =\ \int_{\gamma}\,|\phi(w)|^{1/2}\,|dw|.

This is well-defined for curves passing through zeroes of ϕ\phi, but diverges to infinity for curves through double poles. The area of the flat surface

S|ϕ(w)|𝑑xdy\int_{S}\,|\phi(w)|\,dx\wedge dy

is infinite, since a neighbourhood of each point of MM is isometric to a semi-infinite flat cylinder of circumference 2π|m|2\pi|m|, with mm as in Equation 2.4.

The differential ϕH0(KS(M)2)\phi\in H^{0}(K_{S}(M)^{\otimes 2}) defines a horizontal foliation of S\MS\backslash M, given by the lines along which arg(ϕ)=0arg(\phi)=0. In the natural local co-ordinate, the horizontal foliation is given by lines Im(z)=constant\operatorname{Im}(z)=constant. The local trajectory structure at a zero shows the horizontal foliation is not transversely orientable. The natural S1S^{1}-action by rotation, ϕeiθϕ\phi\mapsto e^{i\theta}\phi, does not change the underlying flat surface, but changes which in the circle of foliations defined by argϕ(z)=constant\arg\,\phi(z)=constant is regarded as horizontal.

A saddle connection is a finite length maximal horizontal trajectory. Any such has both end-points at (not necessarily distinct) zeroes of ϕ\phi.

2.4. WKB triangulations

Suppose the quadratic differential ϕ\phi is complete and saddle-free, meaning that it has no finite-length maximal horizontal trajectory. It then defines a canonical isotopy class of triangulation of SS with vertices at MM, called the WKB-triangulation, see [5, Section 10]. There is a dual “Lagrangian cellulation”, with trivalent vertices the zeroes of ϕ\phi and which has exactly one face for each point of MM.

In general, the WKB-triangulation may contain self-folded triangles. Given a quadratic differential ψ\psi whose associated WKB-triangulation contains a self-folded triangle, there is an edge in the Lagrangian cellulation which goes from a zero to itself. The quiver prescription of Labardini-Fragoso differs in this case [32]. For simplicity we will restrict attention to the non-degenerate case:

Lemma 2.2.

For every g>0g>0 and d>0d>0 there is a complete saddle-free differential whose associated WKB-triangulation contains no self-folded triangles. If d>3d>3 one can assume that the triangulation satisfies the further hypotheses of Theorem 2.1. Every edge of the dual cellulation then has distinct end-points.

Proof.

According to [11, Corollary 3.9], any ideal triangulation can be transformed via a sequence of flips to a non-degenerate triangulation (one containing no self-folded triangles), whilst [18] constructs non-degenerate triangulations satisfying the hypotheses of Theorem 2.1 whenever d>3d>3. Any non-degenerate triangulation TT has an associated bipartite quadrilation T~\tilde{T}, whose vertices are the vertices of TT together with the mid-points of all faces of TT, and which has three edges for each face of TT, which join the vertices of that face to its centre, see Figure 2. Section 4.9 of [5] shows that any quadrilation of the marked surface (𝕊,𝕄)(\mathbb{S},\mathbb{M}) may be realised as the “horizontal strip decomposition” of a quadratic differential ϕ\phi, meaning that ϕ\phi has double poles at the vertices of TT, zeroes at the additional (necessarily trivalent) vertices of T~\tilde{T}, and that the edges of T~\tilde{T} are exactly the trajectories of ϕ\phi which contain a zero. It follows that the non-degenerate triangulation obtained in [18] is realised as a WKB triangulation. The final statement is an immediate consequence of non-degeneracy. ∎

Refer to caption
Figure 2. The quadrilation associated to a triangulation

For brevity, we will call a triangulation as provided by Lemma 2.2 a non-degenerate WKB triangulation.

3. Threefolds

We now associate quasi-projective Calabi-Yau 3-folds to meromorphic quadratic differentials. By way of motivation, if (S,ψ)(S,\psi) comprises a Riemann surface of genus g2g\geqslant 2 and a holomorphic quadratic differential ψ\psi on SS, there is a quasi-projective 3-fold which is a Lefschetz fibration over SS, namely

(3.1) Yψ={(q1,q2,q3)KS3|q12+q22+q32=ψ}Tot(KS3).Y^{\prime}_{\psi}\ =\ \left\{(q_{1},q_{2},q_{3})\in K_{S}^{\oplus 3}\,|\,q_{1}^{2}+q_{2}^{2}+q_{3}^{2}=\psi\right\}\ \subset\mathrm{Tot}(K_{S}^{\oplus 3}).

This is Calabi-Yau, and its geometry (Abel-Jacobi map, cycle theory etc) have elegant interpretations in terms of geometry on SS, see [8]. Our spaces are cousins of these, adapted to the case of meromorphic differentials.

3.1. Elementary modification

Let SS be a closed Riemann surface of genus g1g\geqslant 1, equipped with a reduced divisor MM comprising d=|M|d=|M| points. Fix a rank two holomorphic vector bundle

VSwith an isomorphismη:det(V)KS(M)V\rightarrow S\qquad\textrm{with an isomorphism}\ \eta:\det(V)\cong K_{S}(M)

The determinant defines a fibrewise quadratic map

(3.2) det:S2(V)KS(M)2.\det:S^{2}(V)\rightarrow K_{S}(M)^{\otimes 2}.

Consider an elementary modification of the symmetric square S2(V)S^{2}(V) along MM, fitting into a short exact sequence of sheaves

(3.3) 0WS2Vα(ιM)0.0\rightarrow W\longrightarrow S^{2}V\stackrel{{\scriptstyle\alpha}}{{\longrightarrow}}(\iota_{M})_{*}\mathbb{C}\rightarrow 0.
Lemma 3.1.

WW is locally free of rank 33, and c1(W)=3KS+2PD[M]c_{1}(W)=3K_{S}+2\mathrm{PD}[M].

Proof.

The sheaf WW is torsion-free on a smooth curve, hence locally free. The first Chern class is given by the Whitney sum formula. ∎

Elementary modifications along MM are not unique, but depend on the choice of α\alpha in (3.3). It will be important for us to choose the elementary modification compatibly with the quadratic map (3.2).

Lemma 3.2.

There is an elementary modification WW as above with the property that for each xMx\in M, the induced map

det:WKS(M)2\det:W\rightarrow K_{S}(M)^{\otimes 2}

has fibre 22Wx\mathbb{C}^{2}\amalg\mathbb{C}^{2}\subset W_{x} over any non-zero point of KS(M)x2K_{S}(M)^{\otimes 2}_{x}.

Proof.

The statement is obviously local at a given xMx\in M. Let xx be defined by an equation ff. Near xx we fix a trivialisation S2V𝒪𝒪𝒪S^{2}V\cong\mathcal{O}\oplus\mathcal{O}\oplus\mathcal{O} in which S2VS^{2}V is spanned by holomorphic sections a,b,ca,b,c with respect to which the determinant map is given by the fibrewise quadratic

(a,b,c)abc2.(a,b,c)\mapsto ab-c^{2}.

Such a local basis of sections arises naturally from a choice of local basis of sections s,ss,s^{\prime} for VV near xx, with a=ssa=s\otimes s, b=ssb=s^{\prime}\otimes s^{\prime} and c=ss+ssc=s\otimes s^{\prime}+s^{\prime}\otimes s. The proof of Lemma 3.1 implies there is an elementary modification WW which is spanned by local holomorphic sections (fa,b,c)(fa,b,c), and the determinant map on WW is then given by

(fa)bc2.(fa)b-c^{2}.

At xx, where f=0f=0, the fibre det1(y)={c2=y}Wx\det^{-1}(y)=\{c^{2}=-y\}\subset W_{x} is isomorphic to the disjoint union of two planes {c=±y}3\{c=\pm\sqrt{-y}\}\subset\mathbb{C}^{3}, provided y0y\neq 0. ∎

Note that a choice of complex line \ell in the fibre VpV_{p} of VV at pp, equivalently of a parabolic structure on VV at pp, induces an elementary modification as in Lemma 3.2, where the subspace WpS2VpW_{p}\subset S^{2}V_{p} is identified with the quadratic forms on VpV_{p}^{*} vanishing on the annihilator of Vp\ell\subset V_{p}.

3.2. A quasiprojective Calabi-Yau 3-fold

Let ϕH0(KS(M)2)\phi\in H^{0}(K_{S}(M)^{\otimes 2}) be a meromorphic quadratic differential on SS with simple zeroes and a pole of order exactly 22 at each xMx\in M. Define the hypersurface

Yϕ={detWπϕ=0}WY_{\phi}=\{det_{W}-\pi^{*}\phi=0\}\subset W

inside the total space of the vector bundle WW. We shall write

Xϕ(W𝒪)X_{\phi}\subset\mathbb{P}(W\oplus\mathcal{O})

for the fibrewise projective completion of YϕY_{\phi}. Being fibred in quadrics, this is the zero-locus of a section of πKS(M)2(2)(W𝒪)\pi^{*}K_{S}(M)^{\otimes 2}(2)\rightarrow\mathbb{P}(W\oplus\mathcal{O}), where π:(W𝒪)S\pi:\mathbb{P}(W\oplus\mathcal{O})\to S denotes projection.

The previous description of the determinant map detW\det_{W} shows that the natural map XϕSX_{\phi}\rightarrow S is a fibration by projective quadrics, with generic fibre 1×1\mathbb{P}^{1}\times\mathbb{P}^{1}, nodal fibres over zeroes of ϕ\phi, and reducible fibre 2l2\mathbb{P}^{2}\cup_{l}\mathbb{P}^{2} at each point of MM, i.e. the union of two planes joined along a line ll. The locus of reducible quadrics has codimension >1>1 in the space of all quadric hypersurfaces in 3\mathbb{P}^{3}, so a generic one-parameter family of quadrics would have no such singular fibres. The singular fibre 2l2\mathbb{P}^{2}\cup_{l}\mathbb{P}^{2} is not locally smoothable (i.e. not the 0-fibre of a smooth three-fold 𝒳D\mathcal{X}\rightarrow D); an infinitesimal smoothing is determined by a section of the tensor product νl/2νl/2𝒪(2)\nu_{l/\mathbb{P}^{2}}^{*}\otimes\nu_{l/\mathbb{P}^{2}}^{*}\cong\mathcal{O}(-2) of the normal bundles to the normal crossing locus ll in the two components of the singular fibre.

Lemma 3.3.

XϕX_{\phi} has two isolated singularities at infinity (i.e. in the complement of YϕXϕY_{\phi}\subset X_{\phi}) over each point of MSM\subset S, which are 3-fold ordinary double points. These are the only singularities of XϕX_{\phi}.

Proof.

Away from MM, the map XϕSX_{\phi}\rightarrow S is a Lefschetz fibration, and smoothness of the total space is clear. Given the description of the determinant map in Lemma 3.2, a local model for the behaviour near the singular fibres over MM is given by a neighbourhood of the (δ=0)(\delta=0) fibre in the quadric pencil

(3.4) {x2δyz=ϕ(δ)t2}[x:y:z:t]3×δ;ϕ(δ)0δ\left\{x^{2}-\delta yz=\phi(\delta)t^{2}\right\}\ \subset\ \mathbb{P}^{3}_{[x:y:z:t]}\times\mathbb{C}_{\delta};\qquad\phi(\delta)\neq 0\,\forall\,\delta

The subspace {t=1}\{t=1\} defines the vector bundle W(W𝒪)W\subset\mathbb{P}(W\oplus\mathcal{O}) in the given trivialisation, and by hypothesis the holomorphic function ϕ(δ)\phi(\delta) vanishes away from MM. Without loss of generality, we can suppose ϕ(0)=1\phi(0)=1. Under projection to the second factor δ\mathbb{C}_{\delta}, the 0-fibre is {x2=t2}\{x^{2}=t^{2}\} which is a union of two planes, whose line of intersection {x=0=t}\{x=0=t\} lies in the hyperplane at infinity Π={t=0}\Pi=\{t=0\}. The complement of Π\Pi is the affine variety

{x2δyz=ϕ(δ)}4.\left\{\,x^{2}-\delta yz=\phi(\delta)\,\right\}\ \subset\ \mathbb{C}^{4}.

Under the projection to the plane δ\mathbb{C}_{\delta}, this has generic fibre an affine conic TS2T^{*}S^{2}, and these degenerate at δ=0\delta=0 to a singular fibre 22\mathbb{C}^{2}\amalg\mathbb{C}^{2}. The singularities of the total space of (3.4) are the points

y=1, 0{x2ϕ(δ)t2=δz}andz=1, 0{x2ϕ(δ)t2=δy}y=1,\,0\in\{x^{2}-\phi(\delta)t^{2}=\delta z\}\qquad\textrm{and}\ z=1,\,0\in\{x^{2}-\phi(\delta)t^{2}=\delta y\}

in the given affine charts {y=1}\{y=1\} respectively {z=1}\{z=1\}, which since ϕ\phi is locally non-vanishing are both 3-fold ordinary double points. ∎

Corollary 3.4.

YϕY_{\phi} is smooth.

Proof.

Removing the section of 𝒪(1)\mathcal{O}_{\mathbb{P}}(-1) defining the divisor Δ=Xϕ\Yϕ\Delta_{\infty}=X_{\phi}\backslash Y_{\phi} at infinity removes the line ll from each reducible fibre, hence removes all the nodes. ∎

The quasi-projective variety YϕY_{\phi} comes with a natural projection map π:YϕS\pi:Y_{\phi}\rightarrow S.

  • The generic fibre of π\pi is a smooth affine quadric {abc2=t}\{ab-c^{2}=t\} with t0t\neq 0, abstractly diffeomorphic to the cotangent bundle TS2T^{*}S^{2};

  • At a zero pp of ϕ\phi, π1(p)\pi^{-1}(p) is defined by the quadratic {abc2=0}3\{ab-c^{2}=0\}\subset\mathbb{C}^{3}, which has an isolated nodal singularity;

  • At a point xMx\in M, recalling that by hypothesis ϕ(x)=t0\phi(x)=t^{\prime}\neq 0, the fibre π1(x)\pi^{-1}(x) is given by an affine quadric {c2=t}3\{c^{2}=t^{\prime}\}\subset\mathbb{C}^{3}, a disjoint union of two planes.

Lemma 3.5.

YϕY_{\phi} has holomorphically trivial canonical bundle, hence c1(Yϕ)c_{1}(Y_{\phi}) = 0. The choice of isomorphism η:det(V)KS(M)2\eta:\det(V)\rightarrow K_{S}(M)^{\otimes 2} defines a canonical homotopy class of trivialisation of the canonical bundle KYϕK_{Y_{\phi}}.

Proof.

Consider the 3\mathbb{P}^{3}-bundle π:=(W𝒪)S\pi:\mathbb{P}=\mathbb{P}(W\oplus\mathcal{O})\rightarrow S. The determinant map

det:S2(V)KS(M)2det:S^{2}(V)\rightarrow K_{S}(M)^{\otimes 2}

restricted to WS2(V)W\subset S^{2}(V) is fibrewise quadratic, hence can be viewed as an element of the space of global sections π(KS(M)2)(2)\pi^{*}(K_{S}(M)^{\otimes 2})(2), which pushes forward to give

Γ(S2(W𝒪)πKS(M)2).\Gamma\,\big{(}S^{2}(W\oplus\mathcal{O})^{*}\otimes\pi^{*}K_{S}(M)^{\otimes 2}\big{)}.

The projective completion XϕX_{\phi} has canonical class KX=KKS(M)2(2)K_{X}=K_{\mathbb{P}}K_{S}(M)^{\otimes 2}(2). Since

(3.5) K=det(W𝒪)(4)πKSK_{\mathbb{P}}=det(W^{*}\oplus\mathcal{O})(-4)\otimes\pi^{*}K_{S}

and there is an isomorphism η~:det(W)KS(M)3(M)\tilde{\eta}:det(W^{*})\rightarrow K_{S}(M)^{\otimes-3}(M), one sees

KX=𝒪(2).K_{X}=\mathcal{O}_{\mathbb{P}}(-2).

The quasi-projective subvariety YϕXϕY_{\phi}\subset X_{\phi} is the complement of the section of 𝒪(1)\mathcal{O}_{\mathbb{P}}(1) at infinity, and the square of that section is a canonical divisor on XϕX_{\phi}. The last statement follows from (3.5) since η\eta induces η~\tilde{\eta}. ∎

Lemma 3.6.

There is a nowhere zero holomorphic volume form κϕ\kappa_{\phi} on YϕY_{\phi}.

Proof.

Up to rescaling, there is a unique section of 𝒪(1)\mathcal{O}_{\mathbb{P}}(1) vanishing on the divisor Δ\Delta_{\infty} at infinity, and since KXϕ=𝒪(2)K_{X_{\phi}}=\mathcal{O}_{\mathbb{P}}(-2), the complement YϕY_{\phi} admits a canonical holomorphic volume form up to scale. ∎

Remark 3.7.

The form κϕ\kappa_{\phi} has poles of order 2 at infinity. For a heuristic discussion of the relevance of the pole order being 2\geqslant 2 to constructions of stability conditions on the Fukaya category starting from pairs comprising a complex structure and such a non-vanishing volume form, see [31, Section 7.3].

3.3. Resolution

The 3-fold ordinary double point

{z02+z12+z22+z32=0}4\{z_{0}^{2}+z_{1}^{2}+z_{2}^{2}+z_{3}^{2}=0\}\subset\mathbb{C}^{4}

admits two distinct small resolutions, in which the singular point is replaced by a smooth 1\mathbb{P}^{1} with normal bundle 𝒪(1)𝒪(1)\mathcal{O}(-1)\oplus\mathcal{O}(-1). The resolutions are obtained by collapsing either one of the two rulings of the exceptional divisor 1×1\mathbb{P}^{1}\times\mathbb{P}^{1} resulting from blowing up the singularity; the passage from one resolution to the other is the simplest example of a 3-fold flop.

Lemma 3.8.

There is a projective small resolution χ:X^ϕXϕ\chi:\hat{X}_{\phi}\rightarrow X_{\phi}.

Proof.

Blow-ups of projective varieties are necessarily projective. Let X^ϕ\hat{X}_{\phi} be given by blowing up a Weil divisor comprising exactly one component 2Hxπ1(x)\mathbb{P}^{2}\cong H_{x}\subset\pi^{-1}(x) of each reducible fibre, xMx\in M. Such a Weil divisor contains all of the nodes, hence the blow-up is a small resolution. See [7], [52] for further discussion. ∎

Let Δ^X^ϕ\hat{\Delta}_{\infty}\subset\hat{X}_{\phi} be the total transform of ΔXϕ\Delta_{\infty}\subset X_{\phi}.

Refer to caption
Figure 3. Reducible degenerations of a quadric surface with smooth total space. The divisor Δ^\hat{\Delta}_{\infty} is marked in bold (sum of components with multiplicity one); small resolution curves are labelled EE.
Lemma 3.9.

The divisor Δ^X^ϕ\hat{\Delta}_{\infty}\subset\hat{X}_{\phi} is smooth, and supports an effective anticanonical divisor.

Proof.

There are two possible models for the singular fibre of X^ϕS\hat{X}_{\phi}\rightarrow S over a point of MM, depending on whether the small resolution curves lie in the same or distinct components of the fibre. Either the generic fibre 1×1\mathbb{P}^{1}\times\mathbb{P}^{1} degenerates to a union of two first Hirzebruch surfaces meeting along a fibre; or it degenerates to a copy of the blow-up of 2\mathbb{P}^{2} at two distinct points p,qp,q, meeting a second copy of 2\mathbb{P}^{2} along the curve which is the proper transform of the line between p,qp,q, see Figure 3. More explicitly, the local model given by the rightmost of the degenerations of Figure 3 can be obtained by taking the trivial fibration (1×1)×D(\mathbb{P}^{1}\times\mathbb{P}^{1})\times D and blowing up a point ((q,q),0)((q,q),0) lying on the diagonal of the central fibre. The two models are related by flopping one of the (1,1)(-1,-1)-curves EE. In either case, Δ^\hat{\Delta}_{\infty} is a conic bundle over SS with Lefschetz-type singularities, hence the total space of the divisor is smooth. Since X^ϕXϕ\hat{X}_{\phi}\rightarrow X_{\phi} is crepant and ΔXϕ\Delta_{\infty}\subset X_{\phi} supports an effective anticanonical divisor on XϕX_{\phi}, by Lemma 3.5, the last statement holds. ∎

Lemma 3.10.

Δ^C0\hat{\Delta}_{\infty}\cdot C\geqslant 0 for every rational curve 1CΔ^X^ϕ\mathbb{P}^{1}\cong C\subset\hat{\Delta}_{\infty}\subset\hat{X}_{\phi}.

Proof.

Inside XϕX_{\phi}, the divisor at infinity is a conic bundle over SS, with an integrable complex structure for which projection to SS is holomorphic. Since g(S)>0g(S)>0, any rational curve in Δ\Delta_{\infty} is contained in a fibre of projection, hence is a rational curve in some quadric surface in 3\mathbb{P}^{3}. Any such curve is in the homology class of some multiple of a line in 3\mathbb{P}^{3}, hence deforms inside the 3\mathbb{P}^{3}-fibre, and meets Δ\Delta_{\infty} strictly positively.

The small resolution r:X^ϕXϕr:\hat{X}_{\phi}\rightarrow X_{\phi} contracts, for each point xMx\in M, two smooth 1\mathbb{P}^{1}’s with normal bundle 𝒪(1)𝒪(1)\mathcal{O}(-1)\oplus\mathcal{O}(-1). For such a curve EE, the intersection EΔ^=0E\cdot\hat{\Delta}_{\infty}=0; indeed, KX^ϕ=rKXϕ=r(2Δ)=2Δ^K_{\hat{X}_{\phi}}=r^{*}K_{X_{\phi}}=r^{*}(-2\Delta_{\infty})=-2\hat{\Delta}_{\infty}, but the canonical class is trivial near a (1,1)(-1,-1)-curve. The result for a general C=1Δ^C=\mathbb{P}^{1}\subset\hat{\Delta}_{\infty} then follows by linearity; the coefficient of a line in the homology class of CC must be non-negative by considering the area (with respect to a suitable Kähler form, see Section 3.5 below) of the image of CC after blowing down. ∎

At a double pole of ϕ\phi, there is a canonical local complex co-ordinate on SS in which a quadratic differential can be expressed as

ϕ=mdz2z2.\phi=m\,\frac{dz^{\otimes 2}}{z^{2}}.

We refer to mm\in\mathbb{C}^{*} as the residue of ϕ\phi at the double pole.

For each pMSp\in M\subset S, the fibre π1(p)\pi^{-1}(p) is reducible. Let +,p2\mathbb{C}^{2}_{+,p} denote one component of this fibre.

Lemma 3.11.

The divisors +,p2\mathbb{C}^{2}_{+,p} are linearly independent in H2(Yϕ;2)H4lf(Y;2)H^{2}(Y_{\phi};\mathbb{Z}_{2})\cong H_{4}^{lf}(Y;\mathbb{Z}_{2}).

Proof.

By considering intersections with the small resolution curves, the dd divisors defined by taking one component of each reducible fibre are linearly independent in H2(X^ϕ;)H^{2}(\hat{X}_{\phi};\mathbb{Z}); general properties of small resolutions [52] further imply that b2(X^ϕ)=b2(Xϕ)+db_{2}(\hat{X}_{\phi})=b_{2}(X_{\phi})+d. YϕY_{\phi} is the complement of a smooth divisor Δ^X^ϕ\hat{\Delta}_{\infty}\subset\hat{X}_{\phi}, by Lemma 3.9. The complex surface Δ^\hat{\Delta}_{\infty} is a ruled surface over SS, with fibres comprising a chain of 3 rational curves over each point of MM and smooth fibres elsewhere. Mayer-Vietoris gives an exact sequence with 2\mathbb{Z}_{2}-coefficients

(3.6) 0H2(X^ϕ)H2(Yϕ)H2(Δ^)H2(U(Δ^))00\rightarrow H^{2}(\hat{X}_{\phi})\rightarrow H^{2}(Y_{\phi})\oplus H^{2}(\hat{\Delta}_{\infty})\rightarrow H^{2}(\partial U(\hat{\Delta}_{\infty}))\rightarrow 0

with U(Δ^)\partial U(\hat{\Delta}_{\infty}) the smooth five-manifold which is the circle normal bundle to Δ^X^ϕ\hat{\Delta}_{\infty}\subset\hat{X}_{\phi}. The Gysin sequence for the cohomology of this five-manifold shows the map

H2(Δ^)H2(U(Δ^))H^{2}(\hat{\Delta}_{\infty})\rightarrow H^{2}(\partial U(\hat{\Delta}_{\infty}))

is a surjective map 22+2d21+2d\mathbb{Z}_{2}^{2+2d}\rightarrow\mathbb{Z}_{2}^{1+2d} with rank one kernel spanned by the Euler class. The group H2(X^ϕ)H^{2}(\hat{X}_{\phi}) has rank 2+d2+d, and dimension counting shows that H2(Yϕ)H^{2}(Y_{\phi}) has rank 1+d1+d and that the map between them in (3.6) has full rank. It follows that the components of the reducible fibres in H2(X^ϕ)H^{2}(\hat{X}_{\phi}) are linearly independent in the image. ∎

Lemma 3.12.

Consider a loop γ\gamma of quadratic differentials {ϕt}tS1\{\phi_{t}\}_{t\in S^{1}} on SS with the property that the residue at a given double pole pSp\in S has winding number +1+1 about 0. Let f:𝒳S1f:\mathcal{X}\rightarrow S^{1} denote the corresponding family of relative quadrics, with fibre XϕtX_{\phi_{t}} over ϕt\phi_{t}. The monodromy of ff on H(Xϕ1)H_{*}(X_{\phi_{1}}) exchanges the homology classes of the two components of the reducible singular fibre π1(p)Xϕ1\pi^{-1}(p)\subset X_{\phi_{1}}.

Proof.

In the local model {x2δyz=ϕ(δ)t2}\{x^{2}-\delta yz=\phi(\delta)t^{2}\} of Equation (3.4), consider a family of differentials ϕθ\phi_{\theta} with ϕθ(0)=eiθ\phi_{\theta}(0)=e^{i\theta}. The components of the fibre over δ=0\delta=0 of the affine piece YϕθY_{\phi_{\theta}} are given by {x=±eiθ/2t}\{x=\pm e^{i\theta/2}t\}, which are exchanged by the monodromy corresponding to varying θ\theta in [0,2π][0,2\pi].∎

Since the choice of small resolution X^ϕ\hat{X}_{\phi} depends on a choice of component of the reducible fibre along which to blow up, there is no obvious universal family of small resolutions over any such loop γ\gamma in the space of quadratic differentials. A universal family of small resolutions does exist over the space Quad±(𝕊,𝕄)0\operatorname{Quad}^{\pm}(\mathbb{S},\mathbb{M})_{0} of signed complete differentials introduced in the Introduction.

3.4. Topology

We consider the algebraic topology of the threefold YϕY_{\phi}.

Lemma 3.13.

If π:YϕS\pi:Y_{\phi}\rightarrow S is the natural projection and DpSD_{p}\subset S is a small disk encircling a pole pM=Pol(ϕ)p\in M=\mathrm{Pol}(\phi), then π1(Dp)Yϕ\pi^{-1}(D_{p})\subset Y_{\phi} is simply connected, and has reduced homology groups

H2(π1(Dp))2;H3(π1(Dp)).H_{2}(\pi^{-1}(D_{p}))\cong\mathbb{Z}^{2};\quad H_{3}(\pi^{-1}(D_{p}))\cong\mathbb{Z}.
Proof.

Via the right side of Figure 3, a neighbourhood of the reducible fibre at a point of MM is described topologically as follows. Let u:1×1×11u:\mathbb{P}^{1}\times\mathbb{P}^{1}\times\mathbb{P}^{1}\rightarrow\mathbb{P}^{1} denote the third projection. Let H(1)3H\subset(\mathbb{P}^{1})^{3} be a divisor which is a smooth conic in every fibre of uu over 1\{0}\mathbb{P}^{1}\backslash\{0\}, but meets the 0-fibre of uu in a union of two lines. Let ZZ denote the blow-up of 1×1×1\mathbb{P}^{1}\times\mathbb{P}^{1}\times\mathbb{P}^{1} at the unique intersection point of those two lines, and let WZW\subset Z denote the divisor which is the proper transform of u1()Hu^{-1}(\infty)\cup H. Then π1(Dp)Z\W\pi^{-1}(D_{p})\simeq Z\backslash W, and hence H(π1(Dp))Hct6(Z\W)=H6(Z,W)H_{*}(\pi^{-1}(D_{p}))\cong H^{6-*}_{ct}(Z\backslash W)=H^{6-*}(Z,W). The computation is then straightforward. ∎

The Lemma implies that YϕY_{\phi} contains homotopically non-trivial 2-spheres which are not contained in a fibre of projection to SS, which is one source of delicacy in the subsequent construction of its Fukaya category.

Lemma 3.14.

H3(Yϕ;)H_{3}(Y_{\phi};\mathbb{Z}) has rank 6g6+3d6g-6+3d; the intersection form has kernel of rank dd.

Proof.

Let YϕopY_{\phi}^{op} denote π1(S\pDp)\pi^{-1}(S\backslash\cup_{p}D_{p}), with DpD_{p} a small disk enclosing pMp\in M and no other critical point of ϕ\phi. A Mayer-Vietoris argument and (the proof of) Lemma 3.13 implies H3(Yϕ)H3(Yϕop)H_{3}(Y_{\phi})\cong H_{3}(Y^{op}_{\phi}). We now apply the Leray-Serre spectral sequence to the projection YϕopS\MY^{op}_{\phi}\rightarrow S\backslash M. The monodromy in R2πR^{2}\pi_{*}\mathbb{Z} of a projective fibration of quadric surfaces can be canonically identified with the monodromy in R0πR^{0}\pi_{*}\mathbb{Z} of the associated double covering of Riemann surfaces, see e.g. [41]. Let CSC\rightarrow S be the double cover branched at the zeroes of ϕ\phi, and C0CC^{0}\subset C the preimage in CC of S\MS\backslash M. We next identify the 2-dimensional homology of an affine quadric with the anti-invariant 0-dimensional homology of the corresponding pair of points. Then

H3(Yϕop;)H1(S\M;R2π)H1(C0;).H_{3}(Y^{op}_{\phi};\mathbb{Z})\ \cong\ H_{1}(S\backslash M;R^{2}\pi_{*}\mathbb{Z})\ \cong\ H_{1}(C^{0};\mathbb{Z})^{-}.

The last group was computed by Riemann-Hurwitz in [5, Lemma 2.2], and has rank 6g6+3d6g-6+3d. Matching paths in SS between zeroes of ϕ\phi define circles γC0\gamma\subset C^{0} and 3-spheres LγYϕL_{\gamma}\subset Y_{\phi}, cf. Section 3.7 below. By considering a basis of either group associated to matching paths of a cellulation of SS, one sees that the intersection forms ,C0\langle\bullet,\bullet\rangle_{C^{0}} and ,Yϕ\langle\bullet,\bullet\rangle_{Y_{\phi}} agree, which means that the kernel of the intersection form can be computed on C0C^{0}. The last statement then follows from [5, Section 2]. ∎

Remark 3.15.

The space of stability conditions Stab(𝒟𝒞)\operatorname{Stab}({\mathcal{D}}\mathcal{C}) on any triangulated category 𝒞\mathcal{C} is locally homeomorphic to Hom(K0(𝒞),)\mathrm{Hom}_{\mathbb{Z}}(K^{0}(\mathcal{C}),\mathbb{C}). The K0K^{0}-group of the CY3 category 𝒟(Q,W){\mathcal{D}}(Q,W) defined by a quiver with potential is freely generated by the vertices of the quiver, and for the quivers Q(T)Q(T) arising from ideal triangulations of (𝕊,𝕄)(\mathbb{S},\mathbb{M}), the number of vertices is 6g6+3d6g-6+3d. On the other hand, for any symplectic manifold Y2nY^{2n} for which the Fukaya category is well-defined and bH2(Y;2)b\in H^{2}(Y;\mathbb{Z}_{2}), there is always a natural homomorphism

K0((Y;b))Hn(Y;)K^{0}(\mathcal{F}(Y;b))\longrightarrow H_{n}(Y;\mathbb{Z})

which associates to a Lagrangian submanifold its homology class (note we have not passed to split-closures). From Lemma 3.14 and Theorem 1.1 one can show that this map is an isomorphism for YϕY_{\phi} if one restricts to the K0K^{0}-group of the subcategory 𝒜(T;b0)(Yϕ;b0)\mathcal{A}(T;b_{0})\subset\mathcal{F}(Y_{\phi};b_{0}) introduced after Theorem 1.1. It is interesting to compare this to Abouzaid’s computation [1] for K0((Σg))K^{0}(\mathcal{F}(\Sigma_{g})), with Σg\Sigma_{g} a closed surface of genus g2g\geqslant 2.

3.5. Symplectic forms

The divisor ΔXϕ\Delta_{\infty}\subset X_{\phi} is relatively ample over SS, and its pullback Δ^X^ϕ\hat{\Delta}_{\infty}\subset\hat{X}_{\phi} is relatively nef, and relatively ample over S\MS\backslash M. Fix a Hermitian metric \|\cdot\| in 𝒪(Δ^)\mathcal{O}(\hat{\Delta}_{\infty}) for which the curvature form iFiF_{\nabla} is a semipositive (1,1)(1,1)-form. Denote by tt the section of 𝒪X^ϕ(Δ^)\mathcal{O}_{\hat{X}_{\phi}}(\hat{\Delta}_{\infty}) defining the divisor at infinity. The 2-form

(3.7) ωv=ddc(logt2)\omega_{v}=-dd^{c}(log\|t\|^{2})

is weakly plurisubharmonic and vertically non-degenerate over S\MS\backslash M; for each xS\(MZerϕ)x\in S\backslash(M\cup\mathrm{Zer}_{\phi}) the fibre (π1(x),ωv)(\pi^{-1}(x),\omega_{v}) is a finite type Stein manifold, symplectomorphic to a Stein subdomain of the cotangent bundle (TS2,dpdq)(T^{*}S^{2},dp\wedge dq). In particular, the fibres of YϕY_{\phi} over SMS-M have contact type at infinity.

Fix an area form ωS\omega_{S} on SS of total area d=|M|d=|M|. The class [π1(pt)]+λΔ[\pi^{-1}(pt)]+\lambda\Delta_{\infty} lies in the interior of the ample cone of XϕX_{\phi} for any λ>0\lambda>0, and the form

λωv+πωS\lambda\omega_{v}+\pi^{*}\omega_{S}

is symplectic away from the small resolution curves {Ei}X^ϕ\{E_{i}\}\subset\hat{X}_{\phi}. Recall that χ:X^ϕXϕ\chi:\hat{X}_{\phi}\rightarrow X_{\phi} is the blow-up of a (not necessarily connected) Weil divisor HMXϕH_{M}\subset X_{\phi} which passes through all the ordinary double points. Flopping the small resolution curves appropriately, we can ensure that the pullback HX^ϕH\subset\hat{X}_{\phi} of HMH_{M} meets every EiE_{i} strictly positively. Direct consideration of the blow-up, cf. the proof of [52, Theorem 2.9], implies that

(3.8) ωres=λωv+πωS+δσH\omega_{res}=\lambda\omega_{v}+\pi^{*}\omega_{S}+\delta\sigma_{H}

is a Kähler form on X^ϕ\hat{X}_{\phi}, where σH\sigma_{H} is a 2-form Poincaré dual to HMH_{M}, pointwise positive on each of the EiE_{i}, and δ>0\delta>0 is sufficiently small.

Lemma 3.16.

Let γ:[0,1]S(MZerϕ)\gamma:[0,1]\rightarrow S-(M\cup\mathrm{Zer}_{\phi}) be a C1C^{1}-smooth embedded path. For any λ>0\lambda>0, there is a well-defined symplectic parallel transport map for π:YϕS\pi:Y_{\phi}\rightarrow S over γ\gamma, which induces an exact symplectomorphism of the fibres π1(γ(i))\pi^{-1}(\gamma(i)), i=0,1i=0,1 over the end-points.

Proof.

Since by hypothesis γ\gamma avoids MM, and the perturbing form σH\sigma_{H} can be chosen to be supported near the preimage of MM, it suffices to work with the form λωv+πωS\lambda\omega_{v}+\pi^{*}\omega_{S}, which in turn defines the same symplectic connection as ωv\omega_{v}.

Let DSMD\subset S-M be a small disk. Local parallel transport maps for Xϕ|DDX_{\phi}|_{D}\rightarrow D are clearly well-defined since the map is proper, but it is not obvious that these preserve the divisor at infinity and hence restrict to give maps on YϕY_{\phi}. One can appeal to a relative version of Moser’s theorem to deform the parallel transport vector fields so that they preserve the divisor at infinity, or one can estimate the horizontal vector fields on the open part directly. With respect to the vertical Kähler metric on YϕY_{\phi} induced by \|\cdot\|, the horizontal lift of the vector zTD\partial_{z}\in TD is

(3.9) z=ππ2\partial_{z}^{\sharp}\ =\ \frac{\nabla\pi}{\|\nabla\pi\|^{2}}

since

Dπ(z)=Dπ(π)π2=1andz,v=Dπ(v)π2=0forvTvt(Xϕ)|D=ker(dπ).D\pi(\partial_{z}^{\sharp})=\frac{D\pi(\nabla\pi)}{\|\nabla\pi\|^{2}}=1\qquad\textrm{and}\ \langle\partial_{z}^{\sharp},v\rangle=\frac{D\pi(v)}{\|\nabla\pi\|^{2}}=0\quad\textrm{for}\ v\in T^{vt}(X_{\phi})|_{D}=\mathrm{ker}(d\pi).

Over DD, the divisor Δ\Delta_{\infty} is smooth, irreducible and of multiplicity 11. Choose local co-ordinates 𝐱\bf{x} near a point 0Δ0\in\Delta_{\infty} with

Δ=t1(0)={x1=0};π(x)=xn\Delta_{\infty}=t^{-1}(0)=\{x_{1}=0\};\ \pi(\textbf{x})=x_{n}

and write =eσ||\|\cdot\|=e^{\sigma}|\cdot| as a multiple of the standard metric, for some locally bounded positive function σ\sigma. Then ωres=ddch\omega_{res}=dd^{c}h for a Kähler potential

h=logt2=log|t|2σh=-log\|t\|^{2}=-log|t|^{2}-\sigma

and

|zh|=|π,σ|π2+2|t||t,π|π2|t|2const.|π||\partial_{z}^{\sharp}\cdot h|=\frac{|\langle\nabla\pi,\nabla\sigma\rangle|}{\|\nabla\pi\|^{2}}+\frac{2|t|\,|\langle\nabla t,\nabla\pi\rangle|}{\|\nabla\pi\|^{2}\,|t|^{2}}\ \leqslant\ \frac{const.}{|\pi|}

which ensures integrability of the horizontal vector field on YϕY_{\phi} itself. ∎

The parallel transport maps are not compactly supported, but the image under parallel transport along γ\gamma of any closed exact Lagrangian submanifold of π1(γ(0))\pi^{-1}(\gamma(0)) is well-defined up to compactly supported Hamiltonian isotopy inside π1(γ(1))\pi^{-1}(\gamma(1)). One can slightly generalise the story to allow parallel transport along vanishing paths γ0\gamma_{0} which end at a zero of ϕ\phi, i.e. critical point of the Lefschetz fibration π|π1(SM)\pi|_{\pi^{-1}(S-M)}. In particular, there are well-defined Lefschetz thimbles associated to such paths, in the usual way; see [45] for details.

3.6. Universal families

Recall from the Introduction the finite 2d2^{d}-fold cover

(3.10) Quad±(𝕊,𝕄)0Quad(𝕊,𝕄)0\operatorname{Quad}^{\pm}(\mathbb{S},\mathbb{M})_{0}\longrightarrow\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0}

of signed quadratic differentials. Geometrically on SS, one interprets the sign at pp as a choice of residue ±βpϕ\pm\int_{\beta_{p}}\sqrt{\phi}, where βp\beta_{p} is a small loop encircling pp on SS. The unbranched cover (3.10) extends to Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M}) as a branched cover, with isotropy group 2s\mathbb{Z}_{2}^{s} over differentials with ss simple poles.

Both Quad(𝕊,𝕄)0\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0} and its finite cover are complex analytic orbifolds, excluding a handful of exceptional cases where there is a non-trivial generic isotropy group; when g(𝕊)>0g(\mathbb{S})>0 this only occurs if g(𝕊)=1g(\mathbb{S})=1 and |𝕄|=1|\mathbb{M}|=1, when differentials have generic 2\mathbb{Z}_{2}-stabiliser. One can also consider framed quadratic differentials QuadΓ(𝕊,𝕄)0\operatorname{Quad}^{\Gamma}(\mathbb{S},\mathbb{M})_{0} in which one fixes a framing of the group H3(Yϕ)H_{3}(Y_{\phi}). A framed quadratic differential determines a signed differential, see [5], and QuadΓ(𝕊,𝕄)0\operatorname{Quad}^{\Gamma}(\mathbb{S},\mathbb{M})_{0} is smooth. We will view the choice of sign at a double pole which enters into a signed differential as a choice of component +,x2π1(x)Yϕ\mathbb{C}^{2}_{+,x}\subset\pi^{-1}(x)\subset Y_{\phi} of the reducible fibre over xx (making this association canonical will not be required in the sequel). There is then a universal smooth family

(3.11) 𝒳^QuadΓ(𝕊,𝕄)0\widehat{\mathcal{X}}\rightarrow\operatorname{Quad}^{\Gamma}(\mathbb{S},\mathbb{M})_{0}

of small resolutions over framed quadratic differentials.

Lemma 3.17.

For any fixed λ>0\lambda>0 and δ>0\delta>0 sufficiently small, the symplectic six-manifold (Y,ω)(Y,\omega) underlying (Yϕ,ωresλ,δ)(Y_{\phi},\omega_{res}^{\lambda,\delta}) depends up to symplectic diffeomorphism only on the underlying smooth data (𝕊,𝕄)(\mathbb{S},\mathbb{M}).

Proof.

Fix λ>0\lambda>0 and δ>0\delta>0 sufficiently small. Note ωresλ,δ\omega_{res}^{\lambda,\delta} is Kähler on X^ϕ\hat{X}_{\phi} for every ϕ\phi. The period map on QuadΓ(𝕊,𝕄)0\operatorname{Quad}^{\Gamma}(\mathbb{S},\mathbb{M})_{0} equips that space with a flat Kähler structure, cf. [5, Theorem 1], and there is a Kähler form on the total space of 𝒳^QuadΓ(𝕊,𝕄)0\widehat{\mathcal{X}}\rightarrow\operatorname{Quad}^{\Gamma}(\mathbb{S},\mathbb{M})_{0} which restricts to ωres\omega_{res} on each fibre. Since both varieties Δ^X^ζ\hat{\Delta}_{\infty}\subset\hat{X}_{\zeta} are smooth for every ζ\zeta, we can now apply a relative version of Moser’s theorem (or an argument as in Lemma 3.16) to the universal family (3.11) to symplectically identify the complements X^ζ\Δ^=Yζ\hat{X}_{\zeta}\backslash\hat{\Delta}_{\infty}=Y_{\zeta} for different ζ\zeta. ∎

To simplify notation, we will write ω\omega or ωλ\omega_{\lambda} to denote a symplectic (Kähler) form on YϕY_{\phi} induced as above by the ample divisor [π1(pt)]+λΔ[\pi^{-1}(pt)]+\lambda\Delta_{\infty} on XϕX_{\phi}.

3.7. Lagrangian spheres

The general fibre of (Yϕ,ω)(Y_{\phi},\omega) is a finite type Stein manifold, symplectomorphic to a disk cotangent subbundle DTS2TS2DT^{*}S^{2}\subset T^{*}S^{2}, equipped with the restriction of the canonical symplectic form. A well-known theorem of Hind [21] asserts that there is a unique Lagrangian 2-sphere in TS2T^{*}S^{2} up to Hamiltonian isotopy. That uniqueness leads to various constructions of 3-dimensional Lagrangian submanifolds in YϕY_{\phi}.

Pick a path γ:[0,1]S\gamma:[0,1]\rightarrow S with {γ(0),γ(1)}Zerϕ\{\gamma(0),\gamma(1)\}\subset\mathrm{Zer}_{\phi}, γ(0)γ(1)\gamma(0)\neq\gamma(1), and with γ|(0,1)S\{MZerϕ}\gamma|_{(0,1)}\subset S\backslash\{M\cup\mathrm{Zer}_{\phi}\}. We require the tangent vector of γ\gamma to be non-trivial at each end-point.

Lemma 3.18.

Such a γ\gamma defines a Lagrangian sphere LγYϕL_{\gamma}\subset Y_{\phi}, well-defined up to Hamiltonian isotopy.

Proof.

Suppose ϕ0\phi_{0} is a meromorphic quadratic differential with a zero of multiplicity two at a point pSp\in S. The corresponding 3-fold

Yϕ0={detW=πϕ0}Y_{\phi_{0}}\ =\ \{det_{W}=\pi^{*}\phi_{0}\}

is given locally by a family of quadrics

{abc2=t2}|t|<ε3×t\{ab-c^{2}=t^{2}\}_{|t|<\varepsilon}\subset\mathbb{C}^{3}\times\mathbb{C}_{t}

which has a 3-fold ordinary double point at the origin. The sphere LγYϕL_{\gamma}\subset Y_{\phi} arises as a vanishing cycle for the associated nodal degeneration corresponding to a path of quadratic differentials from ϕ\phi to ϕ0\phi_{0} for which two simple zeroes of ϕ\phi coalesce to a double zero along γ\gamma. The sphere is well-defined up to Hamiltonian isotopy by a Moser-type argument, starting from the fact that the stratum of quadratic differentials with one double zero (and all other zeroes simple) is connected. ∎

The path γ\gamma defines a matching cycle LγYϕL_{\gamma}^{\prime}\subset Y_{\phi}, fibred over the arc γ\gamma via Donaldson’s construction, cf. [47, Section 16] and [4]. In general, the matching cycle construction requires a perturbation of the symplectic connexion over γ\gamma and thus of ω\omega, which may in general change its cohomology class (pulling back a non-trivial multiple of the area class on SS). To avoid this issue, we impose additional symmetry.

Lemma 3.19.

Given any open subset MUSM\subset U\subset S, there is a Hamiltonian isotopy hth_{t}, 0t10\leqslant t\leqslant 1 and h0=idh_{0}=\mathrm{id}, of YϕY_{\phi} for which h1(Lγ)h_{1}(L_{\gamma}) fibres over γ\gamma for every matching path γSU\gamma\subset S-U.

Proof.

There is a distinguished trivialisation of 𝒪(M)\mathcal{O}(M) over S\MS\backslash M. Pick a spin structure on SS viewed as a square root KS12K_{S}^{\frac{1}{2}} of the canonical bundle. We may then suppose that the original vector bundle VS\MV\rightarrow S\backslash M is a direct sum of line bundles

V=KS12KS12=KS122.V=K_{S}^{\frac{1}{2}}\oplus K_{S}^{\frac{1}{2}}=K_{S}^{\frac{1}{2}}\otimes\mathbb{C}^{2}.

Then there is a canonical action of SU(2)SU(2) by bundle automorphisms of V|SMV|_{S-M}, hence of S2VS^{2}V, and the determinant map is SU(2)SU(2)-equivariant. Since S2VS^{2}V and WW are isomorphic over S\MS\backslash M, the same holds for the determinant map on WW. It follows that, for ϕH0(KS(M)2)\phi\in H^{0}(K_{S}(M)^{\otimes 2}), the hypersurface

(3.12) det1(ϕ)Wdet^{-1}(\phi)\subset W

has a holomorphic SU(2)SU(2)-action fibrewise over S\MS\backslash M (which does not extend to the total space of YϕY_{\phi}). Away from π1(U)\pi^{-1}(U), the Kähler form on WW and hence YϕY_{\phi} can be made SU(2)SU(2)-invariant (in fact the SU(2)SU(2)-action factors through SO(3)SO(3)).

The SO(3)SO(3) action on any fibre TS2D<μ(S2)=π1(x)T^{*}S^{2}\supset D^{<\mu}(S^{2})=\pi^{-1}(x) is the canonical action induced by rotations of S2S^{2}. Since the action is fibrewise, symplectic parallel transport maps are SO(3)SO(3)-equivariant, which in turn means that the vanishing cycles for arbitrary matching paths contained in S\US\backslash U are SO(3)SO(3)-invariant Lagrangian spheres in TS2T^{*}S^{2}. However, there is a unique such sphere (any one is an orbit of the action, so distinct ones would be disjoint). Therefore, for the invariant symplectic form, the matching cycle LγL_{\gamma}^{\prime} can be constructed without perturbing the symplectic connection. The Hamiltonian isotopy hth_{t} of the Lemma arises from interpolating a given symplectic form with one which is SO(3)SO(3)-invariant over S\US\backslash U. ∎

The previous construction of a Hamiltonian representative for LγL_{\gamma} fibred over γ\gamma depends on choices; fortunately, we will not need to carry this out in families. A choice of orientation for the vanishing cycle in the fibre and of the matching path in SS defines an orientation of the Lagrangian LγL_{\gamma}.

3.8. Lagrangian cylinders

Consider a loop σS\sigma\subset S encircling a point xMx\in M. Each fibre π1(y)\pi^{-1}(y) for yσy\in\sigma contains a Lagrangian 2-sphere, unique up to Hamiltonian isotopy. In particular, if one parallel transports a given 2-sphere Vπ1(σ(0))V\subset\pi^{-1}(\sigma(0)) around σ\sigma, the resulting monodromy image hσ(V)h_{\sigma}(V) is Hamiltonian isotopic to VV, and co-incident with VV if the symplectic form is SO(3)SO(3)-invariant over σ\sigma as in the previous section. This constructs a Lagrangian submanifold LσYϕL_{\sigma}\subset Y_{\phi} fibred over σ\sigma.

Lemma 3.20.

LσS1×S2.L_{\sigma}\cong S^{1}\times S^{2}.

Proof.

We claim the monodromy around xMx\in M is Hamiltonian isotopic to the identity. The smooth projective 3-fold X^ϕS\hat{X}_{\phi}\rightarrow S has singular fibre a union of two rational surfaces meeting along a smooth curve C1C\cong\mathbb{P}^{1}, cf. Lemma 3.8. This is a Morse-Bott Lefschetz degeneration of the generic smooth fibre 1×1\mathbb{P}^{1}\times\mathbb{P}^{1}, so the monodromy is a fibred Dehn twist in the vanishing cycle [39]. In this case, the isotropic fibres of the vanishing cycle are circles in 1\mathbb{P}^{1}, so the fibred Dehn twist is Hamiltonian isotopic to the identity. ∎

It will be helpful to be more explicit. We keep the previous notation.

Lemma 3.21.

Let Γ\Gamma be defined by

(3.13) Γ={x,peiθ/2,qeiθ/2,δ=eiθ}0θ2π\Gamma=\left\{x\in\mathbb{R},\,p\in e^{-i\theta/2}\mathbb{R},\,q\in e^{-i\theta/2}\mathbb{R},\,\delta=e^{i\theta}\right\}_{0\leqslant\theta\leqslant 2\pi}

inside the affine variety

𝒳={x2+δ(p2+q2)=1}4.\mathcal{X}\ =\ \{\,x^{2}+\delta(p^{2}+q^{2})=1\,\}\subset\mathbb{C}^{4}.

There is a symplectic structure ω𝒳\omega_{\mathcal{X}} on 𝒳\mathcal{X}, compatible with the standard complex structure, for which Γ\Gamma is Lagrangian, and a symplectic embedding of an open subset of the preimage of {|δ|=1}(𝒳,ω𝒳)\{|\delta|=1\}\subset(\mathcal{X},\omega_{\mathcal{X}}) into (Yϕ,ω)(Y_{\phi},\omega) taking Γ\Gamma to LσL_{\sigma}.

Proof.

After flattening the Hermitian metric on the vector bundle WW to look like a product near MM, and deforming ϕ\phi through smooth sections to be constant over a small neighbourhood of MM, one obtains the following symplectic (but not holomorphic) local model for a neighbourhood of a reducible fibre of YϕY_{\phi}. Consider

3×{[x:y:z:t],δ|x2δyz=t2}withωFSωstd\mathbb{P}^{3}\times\mathbb{C}\ \supset\ \left\{\,[x:y:z:t],\delta\,\big{|}\,x^{2}-\delta yz=t^{2}\,\right\}\qquad\textrm{with}\ \omega_{FS}\oplus\omega_{std}

and the hyperplane section Π={t=0}\Pi=\{t=0\}. The subspace living over some small ball 0Bδδ0\in B_{\delta}\subset\mathbb{C}_{\delta} embeds into XϕX_{\phi}, with the local fibration given by projection π\pi to the δ\delta-plane, and a symplectic model for YϕY_{\phi} near a double pole of ϕ\phi is the affine complement of Π\Pi,

(3.14) 3×{x2δyz=1}.\mathbb{C}^{3}\times\mathbb{C}\ \supset\ \left\{\,x^{2}-\delta yz=1\,\right\}.

A unitary change of co-ordinates and conformal rescaling gives the hypersurface

𝒳={x2+δ(p2+q2)=1}4\mathcal{X}\ =\ \{\,x^{2}+\delta(p^{2}+q^{2})=1\,\}\subset\mathbb{C}^{4}

which we equip with the restriction of the standard flat symplectic structure, scaled in the δ\delta-direction so BδB_{\delta} contains the unit circle. We deform the standard symplectic form ω3ωδ\omega_{\mathbb{C}^{3}}\oplus\omega_{\delta} by deforming ωδ\omega_{\delta} to a form ωδ\omega_{\delta}^{\prime} which coincides with the form (1/r)drdθ(1/r)\,dr\wedge d\theta in a small open neighbourhood of the unit circle. Since this co-incides with the usual form rdrdθr\,dr\,d\theta on S1S^{1}, a sufficiently small such perturbation will still tame the standard integrable complex structure. There is an antiholomorphic involution

(x,p,q,δ)(x¯,δp¯,δq¯,1/δ¯)(x,p,q,\delta)\mapsto(\bar{x},\overline{\delta p},\overline{\delta q},1/\overline{\delta})

which preserves 𝒳\mathcal{X} and reverses the sign of the deformed symplectic form on the submanifold 𝒳|{|δ|=1}\mathcal{X}|_{\{|\delta|=1\}}. The fixed locus therefore defines a Lagrangian submanifold

Γ={x,peiθ/2,qeiθ/2,δ=eiθ}0θ2π\Gamma=\left\{x\in\mathbb{R},\,p\in e^{-i\theta/2}\mathbb{R},\,q\in e^{-i\theta/2}\mathbb{R},\,\delta=e^{i\theta}\right\}_{0\leqslant\theta\leqslant 2\pi}

as given in the Lemma. This is an S2S^{2}-bundle over the unit δ\delta-circle; since it is globally Lagrangian, the 2-sphere fibres are preserved by parallel transport by [47, Lemma 16.3], which implies that Γ=Lσ\Gamma=L_{\sigma} for σ\sigma a parametrization of the unit δ\delta-circle. ∎

3.9. WKB collections of spheres

Fix a complete saddle-free quadratic differential ϕ\phi which defines a non-degenerate WKB triangulation in the sense of Lemma 2.2. Lemma 3.18 associates to every edge of the dual cellulation a Lagrangian sphere, which gives a collection of n=6g6+3dn=6g-6+3d Lagrangian spheres {Le}Yϕ\{L_{e}\}\subset Y_{\phi}. We will call such a collection a WKB collection of Lagrangian spheres.

We remark that if the differential ψ\psi yielded a WKB triangulation TT which contained a self-folded triangle, the dual cellulation would contain an edge with goes from a zero to itself, and the matching sphere construction would yield an immersed Lagrangian sphere in YψY_{\psi}. The quiver prescription of Labardini-Fragoso then involves replacing this immersed sphere with an embedded replacement, as in Figure 4. In any case, the situation covered by Lemma 2.2 will suffice in this paper.

Refer to caption
Figure 4. A self-folded triangle, its enclosing triangle, and matching spheres (dotted). On the left, one sphere would be immersed; the right shows its embedded WKB replacement.

Saddle-free differentials form chambers which are separated by walls on which, in the simplest instance, there is a unique saddle connection; the corresponding triangulations differ by a flip, and the Lagrangian cellulations and WKB collections differ as in Figure 5, assuming the WKB triangulations are non-degenerate on both sides of the wall.

Refer to caption
Figure 5. Lagrangian cellulations differing by a flip

Note that the Lagrangians LeL_{e}, LfL_{f} for two distinct edges may meet at two points, cf. Figure 6. In this case, the union of the two matching paths γeγf\gamma_{e}\cup\gamma_{f} is necessarily a homotopically non-trivial loop, by the uniqueness of geodesic representatives for homotopy classes in complete flat surfaces, see [54].

Refer to caption
Figure 6. WKB Lagrangians {L,K,P}\{L,K,P\} in the case g=1g=1, d=1d=1
Remark 3.22.

A holomorphic quadratic differential ψ\psi on SS has 4g44g-4 zeroes. There is no trivalent cellulation of SS with vertices the zeroes of ψ\psi, for reasons of Euler characteristic (trivalence implies the number of faces would be zero). Thus, there is no direct analogue of the Lagrangian cellulation for the 3-fold YψY^{\prime}_{\psi} of Equation (3.1).

3.10. Gradings

Let (Z,ω)(Z,\omega) be a symplectic manifold with 2c1(Z)=02c_{1}(Z)=0, so that ZZ has trivial bicanonical bundle KZ2𝒪K_{Z}^{\otimes 2}\cong\mathcal{O}, where KZK_{Z} is defined with respect to any compatible almost complex structure. The space of possible homotopy classes of trivialisation of KZ2K_{Z}^{\otimes 2} is given by H1(Z;)H^{1}(Z;\mathbb{Z}). Pick a quadratic volume form ΘH0(KZ2)\Theta\in H^{0}(K_{Z}^{\otimes 2}) giving the trivialisation. Θ\Theta defines a map from the Lagrangian Grassmannian to the circle

α:GrLag(Z)S1,Λη(v1vn)2|η(v1vn)2|,Λ=vjTZz.\alpha:Gr_{Lag}(Z)\rightarrow S^{1},\quad\Lambda\mapsto\frac{\eta(v_{1}\wedge\ldots\wedge v_{n})^{2}}{|\eta(v_{1}\wedge\ldots\wedge v_{n})^{2}|},\ \Lambda=\langle v_{j}\rangle\subset TZ_{z}.

For any LZL\subset Z there is an induced map αL:LS1\alpha_{L}:L\rightarrow S^{1} and a grading of LZL\subset Z is given by a phase function α~L:L\tilde{\alpha}_{L}:L\rightarrow\mathbb{R} with exp(2iπα~L)=αLexp(2i\pi\tilde{\alpha}_{L})=\alpha_{L}. If L~\tilde{L}, L~\tilde{L}^{\prime} are graded Lagrangians, any isolated transverse intersection point pp of LL and LL^{\prime} acquires an absolute Maslov index i(L~,L~;p)i(\tilde{L},\tilde{L}^{\prime};p)\in\mathbb{Z}.

Example 3.23.

Suppose LL^{\prime} is the graph of an exact one-form dfdf in TLT^{*}L, and ff is Morse with an isolated critical point at 0. Equip LL with the constant trivial phase function. There is a distinguished choice of grading on LL^{\prime} compatible with the canonical isotopy from LL^{\prime} to LL via graphs of εdf\varepsilon df, and with respect to this grading, i(L~,L~;0)i(\tilde{L},\tilde{L}^{\prime};0) is given by the Morse index of 0 as a critical point of ff.

The Lagrangian submanifolds LγL_{\gamma} admit gradings with respect to the holomorphic volume form κϕ\kappa_{\phi} of Lemma 3.6, since they are simply-connected.

Since ϕ\phi equips the surface SS with a flat metric with singularities, a curve γ:[0,1]SM\gamma:[0,1]\rightarrow S-M has a well-defined phase at each point with γ(t)Zerϕ\gamma(t)\not\in\mathrm{Zer}_{\phi}. Recall that γ\gamma is a geodesic for the ϕ\phi-metric precisely if this phase is constant on each connected component of γ1(S\Zerϕ)\gamma^{-1}(S\backslash\mathrm{Zer}_{\phi}), and any primitive saddle connection for ϕ\phi is a geodesic.

Lemma 3.24.

There is a volume form κ~ϕ\tilde{\kappa}_{\phi} homotopic to κϕ\kappa_{\phi} with the property that the phase function of the matching sphere LγYϕL_{\gamma}\subset Y_{\phi}, computed with respect to κ~ϕ\tilde{\kappa}_{\phi}, is equal to the ϕ\phi-phase of the curve γS\gamma\subset S. In particular, saddle connections define Lagrangian 3-spheres of constant phase.

Proof.

Away from a neighbourhood MUSM\subset U\subset S we have a holomorphic SU(2)SU(2)-action on YϕY_{\phi} fixing the divisor at infinity, hence the associated holomorphic volume form is SU(2)SU(2)-invariant in this subset. It follows that the phase function on a matching sphere LeL_{e} is SO(3)SO(3)-invariant, where SO(3)SO(3) rotates the S2S^{2}-fibres, hence defines a function on the underlying matching path γe\gamma_{e}. We claim that this function co-incides with the phase of γe\gamma_{e} in the ϕ\phi-metric.

The result is local, so after passing to a cover of SS we can reduce to the case where γ\gamma is an arc in the base of a Lefschetz fibration with fibres given by affine quadrics. An explicit formula for the phase can then be obtained from the Poincaré residue theorem, compare to [56, Section 6] or [29, Section 5e]. In particular, for the local model

3,(z1,z2,z3)zi2=t\mathbb{C}^{3}\rightarrow\mathbb{C},\qquad(z_{1},z_{2},z_{3})\mapsto\sum z_{i}^{2}=t

equation (6.3) of [56] asserts that the phase function associated to Θ=dz1dz2dz3\Theta=dz_{1}\wedge dz_{2}\wedge dz_{3} at any tangent vector to the Lefschetz thimble defined by a path γ(t)\gamma(t), and projecting to γ(t)t\gamma^{\prime}(t)\partial_{t}, has phase γ(t)t\gamma^{\prime}(t)\sqrt{t}, i.e. that Θ\Theta pushes forward to the one-form tdt\sqrt{t}\,dt. Thus Θ2\Theta^{\otimes 2} defines a quadratic differential tdt2t\,dt^{\otimes 2} on the tt-plane with a simple zero. ∎

The previous Lemma can be used to fix the phase of κϕ\kappa_{\phi} uniquely.

4. Floer theory

4.1. Almost complex structures

The manifold (Yϕ,ω)(Y_{\phi},\omega) is not convex or of contact type at infinity, because the divisor Δ\Delta_{\infty} is not ample. Lemma 3.10 nonetheless gives good control on holomorphic curve theory in YϕY_{\phi}.

Definition 4.1.

Let 𝒥ϕ\mathcal{J}_{\phi} denote the space of almost complex structures on YϕY_{\phi} which

  1. (1)

    tame the symplectic form ω\omega;

  2. (2)

    make projection YϕSY_{\phi}\rightarrow S holomorphic;

  3. (3)

    co-incide outside a compact set with the restriction of the integrable complex structure from the crepant resolution X^ϕ\hat{X}_{\phi}.

Lemma 4.2.

For J𝒥ϕJ\in\mathcal{J}_{\phi} there is no non-constant JJ-holomorphic map 1Yϕ\mathbb{P}^{1}\rightarrow Y_{\phi}, and if LγYϕL_{\gamma}\subset Y_{\phi} is a matching sphere, then LγL_{\gamma} bounds no JJ-holomorphic disk.

Proof.

Since projection YϕSY_{\phi}\rightarrow S is holomorphic and g(S)>0g(S)>0, the first statement follows. The same argument implies that any JJ-holomorphic disk with boundary on LγL_{\gamma} is contained in a fibre of the projection YϕSY_{\phi}\rightarrow S, but the intersection of LγL_{\gamma} with any fibre it meets is exact. ∎

A pseudoholomorphic disk denotes the solution to a perturbed Cauchy-Riemann equation

(4.1) (duγXH)0,1= 0(du-\gamma\otimes X_{H})^{0,1}\,=\,0

defined on a disk with boundary punctures and Lagrangian boundary conditions Ljint(A)L_{j}\subset int(A), where γΩ1(D)\gamma\in\Omega^{1}(D) is a 1-form and XHX_{H} the Hamiltonian vector field of a Hamiltonian function H:X^ϕH:\hat{X}_{\phi}\rightarrow\mathbb{R} which vanishes to order at least 2 on the divisor Δ^\hat{\Delta}_{\infty}. The (0,1)(0,1)-part of the 1-form is taken with respect to a family of almost complex structures induced by a mapping of the domain of uu into 𝒥ϕ\mathcal{J}_{\phi}. Note that the map u:D𝒥ϕu:D\rightarrow\mathcal{J}_{\phi} has the property that u(t)u(t) is some fixed integrable structure J0J_{0} near Δ\Delta_{\infty}. In local co-ordinates Equation 4.1 has the form

su+Ju(z)tuγ(t)Ju(z)XH(u,t)= 0.\partial_{s}u+J_{u(z)}\partial_{t}u-\gamma(\partial_{t})\cdot J_{u(z)}\cdot X_{H}(u,t)\,=\,0.

Since XH0X_{H}\equiv 0 near Δ\Delta_{\infty} and Ju(z)J_{u(z)} is constant near infinity, outside a relatively compact subset UU whose interior contains all the {Lj}\{L_{j}\}, Equation 4.1 reduces to the usual unperturbed holomorphic curve equation.

Lemma 4.3.

Let {L1,,Lk}Yϕ\{L_{1},\ldots,L_{k}\}\subset Y_{\phi} be compact Lagrangian submanifolds, and suppose uju_{j} is a sequence of pseudoholomorphic disks with uniformly bounded energy and with boundary on jLj\cup_{j}L_{j}. Then the uju_{j} are contained in some compact subset of YϕY_{\phi}.

Proof.

Suppose the conclusion of the Lemma fails. By Gromov compactness in the smooth variety X^ϕ\hat{X}_{\phi}, some subsequence of the uju_{j} converges to a curve uu_{\infty} in X^ϕ\hat{X}_{\phi} which has non-trivial intersection with the divisor Δ^\hat{\Delta}_{\infty}. Since the Cauchy-Riemann equation is unperturbed near infinity, the image of uu_{\infty} must meet Δ^\hat{\Delta}_{\infty} locally positively, except for components contained inside the divisor. More precisely, positivity of intersections applied to the principal component of the stable curve limit means that this limit curve must contain at least one bubble component which is a rational curve in Δ^\hat{\Delta}_{\infty} with strictly negative intersection with Δ^\hat{\Delta}_{\infty}. No such curves exist by Lemma 3.10. ∎

4.2. Fukaya category generalities

The strictly unobstructed Fukaya categories occuring in this paper belong to a technically manageable regime. The relevant transversality theory is encompassed by material in [47, 49], to which we defer for essentially all details of the construction.

Let (Y,ω)(Y,\omega) be a symplectic manifold which admits a class of taming almost complex structures 𝒥Y\mathcal{J}_{Y} which satisfy the first conclusion of Lemma 4.2. We only consider strictly unobstructed Lagrangian submanifolds, and suppose furthermore that the conclusion of Lemma 4.3 is valid. (A quasi-projective variety YY admitting a compactification as in Lemma 3.10 is the most relevant source of examples.) For ach bH2(Y;2)b\in H^{2}(Y;\mathbb{Z}_{2}) there is a \mathbb{Z}-graded AA_{\infty}-category (Y;b)\mathcal{F}(Y;b), linear over Λ\Lambda_{\mathbb{C}}, called the strictly unobstructed (bb-twisted) Fukaya category. Objects of (Y;b)\mathcal{F}(Y;b) are Lagrangian branes LYL\subset Y, namely:

  • LYL\subset Y is a closed oriented Lagrangian submanifold;

  • JL𝒥YJ_{L}\in\mathcal{J}_{Y} is an almost complex structure for which LL bounds no JLJ_{L}-holomorphic disk and meets no JLJ_{L}-holomorphic sphere;

  • LL carries a relative spin structure, relative to the class bb;

  • LL is graded, see Section 3.10.

Morphisms in (Y;b)\mathcal{F}(Y;b) are given by the Floer cochain complex (CF(L,L),μ1)(CF^{*}(L,L^{\prime}),\mu^{1}), which is freely generated by intersection points of LL and LL^{\prime} if they intersect transversely. More properly, index theory and the choice of gradings on LL, LL^{\prime} associate to any isolated transverse intersection point xLLx\in L\pitchfork L^{\prime} an abstract one-dimensional Λ\Lambda_{\mathbb{C}}-vector space orx\mathrm{or}_{x}, see [47, Section 11h], and the Floer complex

CF(L,L)=xorx.CF^{*}(L,L^{\prime})\ =\ \oplus_{x}\,\mathrm{or}_{x}.

There are higher order chain-level operations which comprise a collection of maps

(4.2) μd:CF(Ld1,Ld)CF(L0,L1)CF(L0,Ld)[2d]\mu_{\mathcal{F}}^{d}:CF(L_{d-1},L_{d})\otimes\cdots\otimes CF(L_{0},L_{1})\rightarrow CF(L_{0},L_{d})[2-d]

of degree 2d2-d, for d1d\geqslant 1, with μ1\mu_{\mathcal{F}}^{1} being the aforementioned differential and μ2\mu_{\mathcal{F}}^{2} the holomorphic triangle product. The {μd}\{\mu^{d}_{\mathcal{F}}\} have matrix coefficients which are defined by counting holomorphic disks with (d+1)(d+1)-boundary punctures, whose arcs map to the Lagrangian submanifolds (L0,,Ld)(L_{0},\ldots,L_{d}) in cyclic order and which converge in strip-like end co-ordinates at the punctures to intersection points. The moduli spaces of disks are naturally oriented relative to the orientation lines occuring in (4.2) (in a manner which depends on the choice of bb), so the count of pseudo-holomorphic disks is a signed count. The count of a disk uu is weighted by the symplectic area quωq^{\int_{u}\omega}, with qq the Novikov parameter.

The construction of the operations μd\mu^{d}_{\mathcal{F}} is rather involved, and we defer to [49, Section 3] for details; in particular, the coefficients μd(xd1,,x0)\mu^{d}(x_{d-1},\ldots,x_{0}) depend on additional perturbation data (𝒦,𝒥)(\mathcal{K},\mathcal{J}) (choices of Hamiltonian functions, domain-dependent almost complex structures, strip-like ends etc; these choices in part overcome the difficulty that a Lagrangian is never transverse to itself). The coefficients are not individually well-defined (the μk\mu^{k} are not chain maps), but the entire structure is invariant up to a suitable notion of quasi-isomorphism. Hamiltonian isotopic Lagrangian submanifolds, equipped with brane data compatible with the isotopy, define quasi-isomorphic objects of (Y;b)\mathcal{F}(Y;b).

We denote by Tw(Y;b)\operatorname{Tw}\,\mathcal{F}(Y;b) the category of twisted complexes over (Y;b)\mathcal{F}(Y;b), and by Twπ(Y;b)\operatorname{Tw}^{\pi}\,\mathcal{F}(Y;b) its idempotent completion. The corresponding cohomological categories are denoted 𝒟(Y;b){\mathcal{D}}\mathcal{F}(Y;b) and 𝒟π(Y;b){\mathcal{D}}^{\pi}\mathcal{F}(Y;b).

We record one particular fact for later.

Lemma 4.4.

Let bH2(Y;2)b\in H^{2}(Y;\mathbb{Z}_{2}) be supported by a locally finite cycle FbYF_{b}\subset Y disjoint from a collection of spin Lagrangian submanifolds {Li}0ik\{L_{i}\}_{0\leqslant i\leqslant k}. Suppose the LiL_{i} are pairwise transverse, and fix intersection points xiCF(Li,Li+1)x_{i}\in CF(L_{i},L_{i+1}) with cyclic indices. If a rigid holomorphic disk uu contributes to the coefficient μ(Y)k(xk1,,x0)\mu^{k}_{\mathcal{F}(Y)}(x_{k-1},\ldots,x_{0}) with value κ\kappa, then it contributes to the same coefficient in (Y;b)\mathcal{F}(Y;b) with coefficient (1)dκ(-1)^{d}\cdot\kappa, where d=uFbd=u\cdot F_{b} is the algebraic intersection number of the disk with the cycle FbF_{b}.

Proof.

See [14, Vol. II, Proposition 8.1.16]. Since FbLi=F_{b}\cap L_{i}=\emptyset, each of the spin Lagrangians LiL_{i} is also relatively spin relative to bb. Note that two Hamiltonian isotopic representatives for LL in YY each lying in Y\FbY\backslash F_{b}, which define quasi-isomorphic objects of (Y;b)\mathcal{F}(Y;b), may not be Hamiltonian isotopic in Y\FbY\backslash F_{b}. The trace on LL of the isotopy with the cycle FbF_{b} defines a 11-cycle in LL, Poincaré dual to a class in H2(L;2)H^{2}(L;\mathbb{Z}_{2}) which twists its relative spin structure compatibly with the change in intersection number with FbF_{b} of some given element in π2(Y,L)\pi_{2}(Y,L). ∎

If one encounters Lagrangians in some convenient geometric position (clean Morse-Bott intersections, matching cycles in a Lefschetz fibration) it is often useful to compute without perturbing them. Given a finite set of Lagrangians {Lj}\{L_{j}\} which meet pairwise transversely, one can define the corresponding Fukaya category subject to this constraint, but the stucture coefficients are obtained from (virtual) counts of more general objects called pearly trees, see [48, Section 7] and [51, Section 4].

First, one defines CF(Li,Li)=CMorse(fi)CF^{*}(L_{i},L_{i})=C^{*}_{Morse}(f_{i}) for a fixed Morse function fi:Lif_{i}:L_{i}\rightarrow\mathbb{R} (Morse-Smale for an underlying Riemannian metric). An abstract pearly tree is a planar tree Γ2\Gamma\subset\mathbb{R}^{2} with one infinite incoming and several infinite outgoing edges, and d0d\geqslant 0 finite-length internal edges, vertices of valence at least 3, the connected components of the complement 2\Γ\mathbb{R}^{2}\backslash\Gamma being labelled by Lagrangians LjL_{j}. A holomorphic pearly tree comprises a collection of pseudoholomorphic disks and gradient flow-lines, satisfying obvious incidence and compatibility conditions; gradient flowlines arise when computing a higher product μk(xk1,,x0)\mu^{k}(x_{k-1},\ldots,x_{0}) for which some inputs xiCF(Li,Li)x_{i}\in CF^{*}(L_{i},L_{i}), see Figure 7.

Refer to caption
Figure 7. An abstract planar tree, and associated pearly configuration

There are two important situations in which one can avoid pearls for purposes of computing a coefficient of (4.2).

  1. (1)

    If adjacent boundary conditions {Li,Li+1}\{L_{i},L_{i+1}\} (with cyclic indices) are always pairwise transverse, in particular never co-incide, there are no pearly contributions to this particular coefficient of μk\mu^{k}. This relies on an important theorem due to Sheridan [51, Proposition 4.6]: moduli spaces of pearls can be made regular by generic choices of consistent perturbation data, and in the regular case pearls with dd internal edges form a stratum of real codimension dd. Therefore for isolated regular pearls, there are no internal (finite length Morse) edges of the underlying planar tree.

  2. (2)

    If there is exactly one adjacent pair of co-incident Lagrangians Li=Li+1L_{i}=L_{i+1}, and the corresponding input or output xiHF(Li,Li)H(Li)x_{i}\in HF^{*}(L_{i},L_{i})\cong H^{*}(L_{i}) is the class of top degree, then one can count pseudoholomorphic polygons which are smooth at the given corner but have an incidence condition, passing through a fixed generic point qLiq\in L_{i} Poincaré dual to xix_{i}. Compare to [48, Section 7].

The choice of b0b_{0} as background class is relevant in Lemma 4.11, but much of the discussion in the next sections applies to the categories (Y;b)\mathcal{F}(Y;b) uniformly. We will sometimes omit the background class bH2(Yϕ;2)b\in H^{2}(Y_{\phi};\mathbb{Z}_{2}) from our notation when it plays no role.

4.3. Grading the WKB algebra

Now return to the 3-fold YϕY_{\phi}. Any Lagrangian matching sphere is strictly unobstructed and admits a unique spin structure. Since LL bounds no holomorphic disks, the cohomology H(CF(L,L))H(L)H(CF^{*}(L,L))\cong H^{*}(L), equipped with its classical AA_{\infty}-structure.

Given a finite collection of Lagrangian spheres {Le}Yϕ\{L_{e}\}\subset Y_{\phi}, and a choice of bH2(Yϕ;2)b\in H^{2}(Y_{\phi};\mathbb{Z}_{2}), there is an associated total morphism AA_{\infty}-algebra

(4.3) 𝒜=𝒜b=e,eHF(Le,Le)\mathcal{A}=\mathcal{A}_{b}=\oplus_{e,e^{\prime}}HF(L_{e},L_{e^{\prime}})

Theorem 1.1 involves computing the AA_{\infty}-algebra 𝒜=𝒜(T;b0)\mathcal{A}=\mathcal{A}(T;b_{0}), where the indices eTe\in T are indexed by edges of a non-degenerate triangulation TT and correspond to a WKB-collection of Lagrangian spheres, and identifying it with the corresponding Ginzburg potential algebra (i.e. with the total endomorphism algebra of the category 𝒞\mathcal{C} considered in Section 2.1).

Lemma 3.19 implies that each LeL_{e} can be taken to fibre over the path γe\gamma_{e}, and hence it suffices to compute the Floer theory amongst such a collection of fibred matching spheres. By projecting to SS, pseudoholomorphic disks are then constrained by the Riemann mapping theorem. Collections of matching spheres don’t lie in general position (there are triple intersections at vertices of the Lagrangian cellulation), so in principle one must define 𝒜\mathcal{A} via pearls, but the remarks at the end of Section 4.2 imply that in the case at hand the consequences are fairly benign.

Consider the Lagrangian submanifolds {Le}\{L_{e}\} which are matching spheres for the edges of the Lagrangian cellulation (dual to a non-degenerate WKB triangulation). Any two distinct Lagrangians Le,LfL_{e},L_{f} are either disjoint or meet at either one or two isolated points, lying over trivalent vertices of the cellulation (the nodal points of a fibre of π\pi lying over a zero of ϕ\phi).

Lemma 4.5.

The LeL_{e} admit gradings for which

  • the algebra 𝒜=e,eHF(Le,Le)\mathcal{A}=\oplus_{e,e^{\prime}}HF^{*}(L_{e},L_{e^{\prime}}) is concentrated in degrees 030\leqslant\ast\leqslant 3;

  • the isolated intersection points have absolute Maslov index +1+1 clockwise and +2+2 anticlockwise, cf. Figure 8.

Refer to caption
Figure 8. A point contributes to CF2(L,K)CF^{2}(L,K) and CF1(K,L)CF^{1}(K,L).
Proof.

The groups HF(L,L)H(S3)HF^{*}(L,L)\cong H^{*}(S^{3}) carry their natural grading, and by Poincaré duality HF(L,L)HF3(L,L)HF^{*}(L,L^{\prime})\cong HF^{3-*}(L^{\prime},L) for any L,LL,L^{\prime}, so it suffices to determine the grading of an isolated intersection point lying over a zero of ϕ\phi. The Lagrangian matching paths of a WKB-type Lagrangian cellulation are realised by geodesics for the ϕ\phi-metric on SS, so the Lagrangians are locally given by transversely intersecting special Lagrangian thimbles.

More explicitly, working locally near a simple zero of the quadratic differential ϕ\phi, we consider the three straight arcs of the associated vertical foliation, which form the terminals of a trivalent vertex. (Comparing to Figure 5, the leaves of the horizontal foliation at a zero fall into the double poles at the centres of the three cells adjacent to the zero, and the edges of the Lagrangian cellulation are given, locally near the zero, by leaves of the vertical foliation.) Each of the arcs defines by parallel transport a Lagrangian disk in the 3-fold YϕY_{\phi}, and Lemma 3.24 implies these all have identical phase. There are Darboux co-ordinates in which these three Lagrangians are given by linear subspaces 3,eiπ/33\mathbb{R}^{3},e^{i\pi/3}\mathbb{R}^{3} and e2iπ/333e^{2i\pi/3}\mathbb{R}^{3}\subset\mathbb{C}^{3}. (Note the quadratic volume form Θ=(dz1dz2dz3)2\Theta=(dz_{1}\wedge dz_{2}\wedge dz_{3})^{\otimes 2} is invariant under rotation by π/3\pi/3, just as the quadratic volume form on SS, locally given by tdt2t\,dt^{\otimes 2} with t=zj2t=\sum z_{j}^{2}, is locally invariant under rotation by 2π/32\pi/3.)

L=eiπ/33L^{\prime}=e^{i\pi/3}\mathbb{R}^{3} is the graph of the differential of a function over L=3L=\mathbb{R}^{3} with an isolated minimum, so a Morse critical point of index 0. Therefore, for the grading on LL^{\prime} compatible with the obvious rotation isotopy back to LL, the absolute index would be zero by Example 3.23. The phase function αLπ/2\alpha_{L^{\prime}}\equiv\pi/2 differs from the phase function compatible with that isotopy by the constant function 11, hence the index of the intersection point is +1+1. (An alternative for the last step is to use non-vanishing of the triangle product, Lemma 4.9 below, to show that since the absolute indices are symmetric under rotation of Figure 8 by 2π/32\pi/3, they must all equal +1+1.) ∎

The local Morse-theoretic description of an isolated intersection xx of WKB spheres L,LL,L^{\prime} given above also yields preferred isomorphisms orxk\mathrm{or}_{x}\cong k between the orientation lines and the ground field, coming from preferred trivialisations det(Dx)k\det(D_{x})\cong k for the determinant line of a ¯\mathrm{\overline{\partial}}-operator on a half-plane with linear Lagrangian boundary conditions which rotate by π/3\pi/3. Via these trivialisations, Lemma 4.5 shows that the WKB algebra is isomorphic, as a graded vector space, to the total morphism algebra of the category 𝒞\mathcal{C} introduced in Section 2.1.

4.4. First constraints on polygons

Let {Le}\{L_{e}\} be matching spheres which are edges of a non-degenerate WKB cellulation. Appealing to [47, Lemma 2.1], we can take the AA_{\infty}-structure on the algebra 𝒜\mathcal{A} from (4.3) to be strictly unital.

Lemma 4.6.

Let k3k\geqslant 3. If the product

μk:HF(Lk1,Lk)HF(L0,L1)HF(L0,Lk)[2k]\mu^{k}:HF^{*}(L_{k-1},L_{k})\otimes\cdots\otimes HF^{*}(L_{0},L_{1})\rightarrow HF^{*}(L_{0},L_{k})[2-k]

is non-zero, then either L0LkL_{0}\neq\operatorname{L}_{k} and all inputs have degree 11, or L0=LkL_{0}=L_{k}, exactly one input has degree 22 and all others have degree 11.

Proof.

Lemma 4.5 implies that the degree 0 subalgebra of the WKB algebra is spanned by the units eiHF0(Li,Li)e_{i}\in HF^{0}(L_{i},L_{i}) of the constituent WKB spheres. It follows that since the AA_{\infty}-structure is strictly unital, none of the inputs to a non-trivial operation μk\mu^{k} with k3k\geqslant 3 has degree 0. Hence every input has degree 1\geqslant 1, whilst μk\mu^{k} has degree 2k2-k. Since 𝒜\mathcal{A} is concentrated in degrees 030\leqslant\ast\leqslant 3, it follows that no input can have degree 33, and at most one input can have degree 22. Moreover, there is an input of degree 22 if and only if the output has degree 33, which is possible only if L0L_{0} and LkL_{k} co-incide. ∎

Lemma 4.7.

The second case of Lemma 4.6 does not occur.

Proof.

Working with pearls, we take a Morse model CF(L,L)=CMorse(L)CF^{*}(L,L)=C^{*}_{Morse}(L) for self Floer cochains; without loss of generality, for each WKB sphere we can take a perfect Morse function so the Floer cochain group has rank 2. If there is a degree two input to the product in Lemma 4.6, the output is in the rank one space CF3(L0,L0)CF^{3}(L_{0},L_{0}), which means that the holomorphic disk should pass through the stable manifold for the gradient flow of the maximum of the Morse function on L0L_{0}. Therefore this marked point is unconstrained, and hence no non-constant disk can be rigid. It follows from the proof of Lemma 4.9 below that constant polygons contribute non-trivially to μ2\mu^{2} but not to μk\mu^{k} for k3k\geqslant 3. ∎

According to [13, Theorem 1.1], over Λ\Lambda_{\mathbb{C}} the Fukaya category can always be taken both cyclic and strictly unital, and Lemma 4.7 would also follow formally from that fact, compare to Section 2.1. A helpful consequence of the previous result is that one can compute the Fukaya category using pseudoholomorphic disks rather than pearly trees. Note that these results do not imply that all the {Li}\{L_{i}\} in (4.2) are pairwise distinct for the corresponding operation to be non-trivial, see Figure 9 for an example.

Refer to caption
Figure 9. A polygon contributing to μ5\mu^{5} in the universal cover when g(S)=1,|M|=1g(S)=1,|M|=1; note the holomorphic disk maps onto S=T2S=T^{2}.

The boundary of any holomorphic polygon contributing to μk\mu^{k} defines a (not necessarily embedded) parametrized closed path in the graph on the surface SS formed by the edges of the Lagrangian cellulation. Inputs of degree 11 correspond to turning clockwise in the graph defined by the cellulation edges, and inputs of degree 22 correspond to turning anticlockwise, along the boundary of the disk; it is simplest to see this by lifting the disk to the universal cover, given by pulling back the fibration π:YϕS\pi:Y_{\phi}\rightarrow S to the universal cover of SS, where the Lagrangian cellulation edges give rise to a trivalent planar graph. Lemma 4.6 implies that there is at most one anticlockwise turn.

Example 4.8.

Suppose LL and KK meet transversely at a single point. The unique closed path of length 22 gives rise to the product

(4.4) HF1(L,K)HF2(K,L)HF3(K,K)HF^{1}(L,K)\otimes HF^{2}(K,L)\rightarrow HF^{3}(K,K)

which is non-trivial by Poincaré duality.

4.5. Constant triangles

Let L0,L1,L2ZL_{0},L_{1},L_{2}\subset Z be three graded Lagrangian submanifolds, intersecting pairwise transversely at a point pp. There is a constant holomorphic triangle uu with boundary conditions (anticlockwise ordered) L0,L1,L2L_{0},L_{1},L_{2}. Let DuD_{u} be the linearized operator at uu, i.e. the ¯\bar{\partial}-operator on the trivial vector bundle with fibre TZpTZ_{p} over a disk with three boundary punctures, with boundary values in TL0,pTL_{0,p}, TL1,pTL_{1,p}, TL2,pTL_{2,p}. The index formula for such operators [47, Proposition 11.13] implies that

(4.5) index(Du)=i(L~0,L~2;p)i(L~0,L~1;p)i(L~1,L~2;p).\mathrm{index}\,(D_{u})=i(\tilde{L}_{0},\tilde{L}_{2};p)-i(\tilde{L}_{0},\tilde{L}_{1};p)-i(\tilde{L}_{1},\tilde{L}_{2};p).

We now return to the situation (and notation) arising in the proof of Lemma 4.5. We label the linear Lagrangians 3,eiπ/33\mathbb{R}^{3},e^{i\pi/3}\mathbb{R}^{3} and e2iπ/333e^{2i\pi/3}\mathbb{R}^{3}\subset\mathbb{C}^{3} by L0L_{0}, L2π/3L_{2\pi/3} and L4π/3L_{4\pi/3}, corresponding to the slopes in the complex plane of the arcs over which they fibre in the model Lefschetz fibration

p:3,(z1,z2,z3)z12+z22+z32.p:\mathbb{C}^{3}\rightarrow\mathbb{C},\quad(z_{1},z_{2},z_{3})\mapsto z_{1}^{2}+z_{2}^{2}+z_{3}^{2}.

For the zero phase functions of Lemma 4.5, the indices appearing in (4.5) are

i(L~0,L~2π/3;p)=2;i(L~0,L~4π/3;p)=1;i(L~4π/3,L~2π/3;p)=1,i(\tilde{L}_{0},\tilde{L}_{2\pi/3};p)=2;\ i(\tilde{L}_{0},\tilde{L}_{4\pi/3};p)=1;\ i(\tilde{L}_{4\pi/3},\tilde{L}_{2\pi/3};p)=1,

so the constant triangle has index 0 and can in principle contribute non-trivially to the product in the algebra 𝒜b\mathcal{A}_{b}.

Lemma 4.9.

The constant holomorphic triangle at a trivalent zero contributes exactly +1+1 to a non-trivial multiplication

μ2:HF1(L4π/3,L2π/3)HF1(L0,L4π/3)HF2(L0,L2π/3).\mu^{2}_{\mathcal{F}}:HF^{1}(L_{4\pi/3},L_{2\pi/3})\otimes HF^{1}(L_{0},L_{4\pi/3})\ \longrightarrow\ \ HF^{2}(L_{0},L_{2\pi/3}).
Proof.

The local model splits into a direct sum of 3 copies of the geometry given by 3 real lines in \mathbb{C} passing through the origin.

Case 2: indexDu=0\mathrm{index}\,D_{u}=0L0L_{0}L1L_{1}L2L_{2}L0L_{0}L2L_{2}L1L_{1}Case 1: indexDu=1\mathrm{index}\,D_{u}=-1
Figure 10. Indices of constant holomorphic triangles

The regularity of the constant triangle uu is then standard, provided the Lagrangians are taken in the appropriate order. For a constant triangle uu in \mathbb{C} contributing to a product

HF(L1,L2)HF(L0,L1)HF(L0,L2)HF^{*}(L_{1},L_{2})\otimes HF^{*}(L_{0},L_{1})\longrightarrow HF^{*}(L_{0},L_{2})

the indices are as given in Figure 10 (consider perturbing the three lines to create a non-trivial triangle in \mathbb{C}, which is either holomorphic or antiholomorphic depending on the cyclic order of the boundary conditions). ∎

Constant triangles and Poincaré duality do not always completely determine the algebra structure in 𝒜\mathcal{A}; there may be additional products if some of the cells of the Lagrangian cellulation are themselves triangles.

4.6. Holomorphic disks on totally real cylinders

Constant holomorphic triangles provide the cubic terms in the superpotential associated to a triangulated surface arising from the “inscribed triangles” of Labardini-Fragoso’s quiver prescription for a potential [32], see (2.2) and Figure 1. The higher order terms of the potential arise from higher order AA_{\infty}-products in 𝒜\mathcal{A}. En route to computing these, it will be helpful to study a simpler local model involving the Lagrangian cylinder of Section 3.8.

Recall the totally real model S1×S2Γ4S^{1}\times S^{2}\cong\Gamma\subset\mathbb{C}^{4} for the Lagrangian cylinder given in (3.13). We will consider holomorphic sections D4D\rightarrow\mathbb{C}^{4} with this boundary condition.

Lemma 4.10.

In the notation of Lemma 3.21, there are exactly two rigid holomorphic sections of π:𝒳D\pi:\mathcal{X}\rightarrow D with boundary condition on Γ\Gamma, and all other moduli spaces of sections are empty.

Proof.

Consider a section D𝒳D\rightarrow\mathcal{X} of π\pi. Since 𝒳4\mathcal{X}\subset\mathbb{C}^{4}, each co-ordinate projection defines a holomorphic map DD\rightarrow\mathbb{C}. In the xx co-ordinate this is a map from the unit disk DδD_{\delta} to \mathbb{C} which takes the boundary circle to the real line; any such is constant, so in fact the non-trivial geometry takes place in the 2\mathbb{C}^{2}-bundle over the disk with co-ordinates p,qp,q. In each of these factors, the total space of the fibrewise Lagrangian of Equation 3.13 over the boundary circle defines a Möbius band, for instance

p,δ2{δ=eiθ,peiθ/2}\mathbb{C}^{2}_{p,\delta}\ \supset\ \left\{\,\delta=e^{i\theta},p\in e^{-i\theta/2}\mathbb{R}\,\right\}

Consider a holomorphic section of π\pi in this factor. This defines a map zv(z)z\mapsto v(z) on the disk with the property that v(z)z1/2v(z)\in z^{-1/2}\mathbb{R} for zS1z\in S^{1}. [45, Lemma 2.16] shows that the only holomorphic maps u:Du:D\rightarrow\mathbb{C} satisfying u(z)z1/2u(z)\in z^{1/2}\mathbb{R} on S1S^{1} are

u:zcz+c¯for  somec,u:z\ \mapsto\ cz+\bar{c}\quad\textrm{for \ some}\ c\in\mathbb{C},

Therefore if vv is a holomorphic section of π\pi, then zv(z)=cz+c¯zv(z)=cz+\bar{c}, but then v(z)=(c+c¯z)v(z)=(c+\frac{\bar{c}}{z}) is meromorphic with a pole, unless c=0c=0. It follows that the only holomorphic sections of π\pi with boundary condition Γ\Gamma are the constant sections

x(δ)=±1;p(δ)=0=q(δ).x(\delta)=\pm 1;\ p(\delta)=0=q(\delta).

Since the sections are constant, they are both regular. ∎

We equip Γ\Gamma with the unique spin structure which is bounding in the circle factor. The moduli space of holomorphic sections of π:𝒳D\pi:\mathcal{X}\rightarrow D with boundary on Γ\Gamma inherits a canonical orientation. (More precisely, we are interested in the space of sections with a single boundary marked point, which has a natural evaluation map to Γ\Gamma.) Note that this spin structure is in particular a relative spin structure relative to the class b0b_{0} of (1.3), since b0|Γ=0{b_{0}}|_{\Gamma}=0. The choice of background class bH2(Yϕ;2)b\in H^{2}(Y_{\phi};\mathbb{Z}_{2}) enters the computation of 𝒜(T;b)\mathcal{A}(T;b) at the following point.

Lemma 4.11.

The two rigid sections of Lemma 4.10 contribute to the moduli space of sections with opposite signs, with respect to the trivial background class b=0b=0, and with the same sign, relative to the background class b=b0b=b_{0}.

Proof.

We return to the local model of Lemma 3.21, and the affine variety {x2+δ(p2+q2)=1}4\{x^{2}+\delta(p^{2}+q^{2})=1\}\subset\mathbb{C}^{4}. There is a holomorphic involution ι\iota of the model given by xxx\mapsto-x, ppp\mapsto-p. This acts fibrewise, preserves the Lagrangian Γ\Gamma, and exchanges the two holomorphic sections. The involution preserves the orientation of Γ\Gamma, which implies that the sections count with the same respectively opposite signs (for the trivial background class) depending on whether or not the involution does or does not preserve the stable trivialisation of the Lagrangian boundary condition along the sections determined by the spin structure on Γ\Gamma, cf. [14, Proof of Theorem 8.1.1]. We claim that the involution does not preserve this stable framing.

Fix a model S1×S22×3=5S^{1}\times S^{2}\subset\mathbb{R}^{2}\times\mathbb{R}^{3}=\mathbb{R}^{5}, with the bounding spin structure. Let (x,y,z)(x,y,z) denote co-ordinates on the 3\mathbb{R}^{3}-factor. There is a natural parametrisation S1×S2ΓS^{1}\times S^{2}\rightarrow\Gamma taking (eiθ,(x,y,z))(e^{i\theta},(x,y,z)) to

(eiθ,(x,eiθ/2(cos(θ/2)y+sin(θ/2)z),eiθ/2(sin(θ/2)ycos(θ/2)z)=(eiθ,(x,p,q)).(e^{i\theta},(x,e^{-i\theta/2}(\cos(\theta/2)y+\sin(\theta/2)z),e^{-i\theta/2}(\sin(\theta/2)y-\cos(\theta/2)z)=(e^{i\theta},(x,p,q)).

The involution ι\iota acts fibrewise on the S2S^{2}-factor of S1×S2S^{1}\times S^{2} by reversing the sign of xx and reflecting the circle in the (y,z)(y,z)-plane along an axis of angle θ/2\theta/2. Altogether, this means we act by the generator of π1(SO(3))\pi_{1}(SO(3)) and hence of π1(SO(5))\pi_{1}(SO(5)). Put differently, the boundary values x=±1,p=0=qx=\pm 1,p=0=q of the holomorphic sections, viewed as S1S^{1}-submanifolds of Γ\Gamma, have an obvious “constant” framing (constant in a twisted parametrisation) from the tangent spaces to the (p,q)(p,q)-plane. These “constant” framings are exchanged by the involution, but are not simultaneously compatible with a choice of spin structure on Γ\Gamma. Indeed, Γ\Gamma is really the mapping torus of a rotation by π\pi on S2S^{2}, and the two holomorphic sections have boundary values coming from the two rotation fixed points. Homotoping the monodromy to the identity rotates the tangent spaces at the fixed points by π\pi in opposite directions, hence can bring only one of the two “constant” framings to the framing induced by the fixed spin structure. The upshot is that the two sections contribute with opposite signs to the moduli space oriented with respect to the trivial background class.

Note that b0b_{0} is supported by a locally finite cycle HH disjoint from the Lagrangian Γ\Gamma. The two holomorphic sections of Lemma 4.10 each hit one of the two components of the reducible fibre over the local point of MM, hence exactly one of them intersects HH, so turning on the background class b0b_{0} changes the sign of exactly one of the disks by Lemma 4.4. ∎

Remark 4.12.

After twisting by b0b_{0}, the boundary values of the sections of Lemma 4.10 sweep the 1-cycle

𝔪0(S1×S2)=±2[σ]0H1(S1×S2),\mathfrak{m}_{0}(S^{1}\times S^{2})=\pm 2[\partial\sigma]\neq 0\in H_{1}(S^{1}\times S^{2}),

which is not the restriction of any central element of QH(M;b0)QH^{*}(M;b_{0}). Therefore a Lagrangian cylinder LσL_{\sigma} has obstructed b0b_{0}-twisted Floer cohomology, and does not define an object of (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}), even if one enlarges the category to allow unobstructed branes in the sense of [14] rather than just weakly exact Lagrangian submanifolds.

4.7. Nonconstant polygons

Fix a finite collection {L0,,Lk}\{L_{0},\ldots,L_{k}\} of matching spheres LiYϕL_{i}\subset Y_{\phi} arranged cyclically, bounding an open subset of SS containing a unique double pole of ϕ\phi. The Lagrangians meet at a sequence of intersection points xj=LjLj+1x_{j}=L_{j}\pitchfork L_{j+1} for 0jk0\leqslant j\leqslant k (with Lk+1L0L_{k+1}\equiv L_{0} by definition). Appealing to Lemma 4.5, we may suppose that xjx_{j} has Maslov index 11. Let x¯k\bar{x}_{k} denote the dual Maslov index 2 intersection point which is a generator of HF2(L0,Lk)HF^{2}(L_{0},L_{k}).

Lemma 4.13.

If the {Lj}1jk\{L_{j}\}_{1\leqslant j\leqslant k} are pairwise distinct, the coefficient of κ\kappa in the product

μ(Y;b)k(xk1,,x0)=κx¯k\mu^{k}_{\mathcal{F}(Y;b)}(x_{k-1},\ldots,x_{0})\ =\ \kappa\,\bar{x}_{k}

is well-defined; it is independent of the auxiliary choices made in constructing the Fukaya category.

Proof.

Recall that the construction of the Fukaya category relies on additional perturbation data (𝒦,𝒥)(\mathcal{K},\mathcal{J}) of Hamiltonian deformations, domain-dependent almost complex structures or Morse-Smale pairs made universally over moduli spaces of stable disks or pearly trees. As in [47, Section 10e], two different choices of that auxiliary data (𝒦i,𝒥i)(\mathcal{K}_{i},\mathcal{J}_{i}), i=1,2i=1,2, for defining the AA_{\infty}-operations can be related by a continuation AA_{\infty}-functor 𝒢=(𝒢i)i1\mathcal{G}=(\mathcal{G}^{i})_{i\geqslant 1} between the resulting Fukaya categories i\mathcal{F}_{i}. Given a configuration of WKB Lagrangians, 𝒢1\mathcal{G}^{1} (the action on morphism groups) is necessarily the identity, whilst μi1\mu^{1}_{\mathcal{F}_{i}} also vanishes on CF(Li,Lj)CF(L_{i},L_{j}) (defining self-Floer cochains using perfect Morse functions). The AA_{\infty}-functor equations then imply that

(4.6) μ2k(xk1,,x0)+i<k,jμ2i(xk1,,𝒢j(xi+j,,xi),xi1,,x1))=\displaystyle\mu^{k}_{\mathcal{F}_{2}}(x_{k-1},\ldots,x_{0})+\sum_{i<k,j}\mu^{i}_{\mathcal{F}_{2}}(x_{k-1},\ldots,\mathcal{G}^{j}(x_{i+j},\ldots,x_{i}),x_{i-1},\ldots,x_{1}))\ =
𝒢1(μ1k(xk1,,x0))+j,i<k±𝒢j(xk1,,μ1i(xi+j,,xj),,x0))\displaystyle\mathcal{G}^{1}(\mu^{k}_{\mathcal{F}_{1}}(x_{k-1},\ldots,x_{0}))+\sum_{j,i<k}\pm\mathcal{G}^{j}(x_{k-1},\ldots,\mu^{i}_{\mathcal{F}_{1}}(x_{i+j},\ldots,x_{j}),\ldots,x_{0}))

The higher products μj\mu^{j}_{\mathcal{F}} amongst the {xi}\{x_{i}\} all vanish for 2<j<k2<j<k, since any contributing holomorphic disk would not have boundary defining a closed curve in the WKB-graph. That immediately implies the μk\mu^{k}-product is invariant under 𝒢\mathcal{G}. ∎

Note that the hypothesis that the {Li}1ik\{L_{i}\}_{1\leqslant i\leqslant k} are pairwise distinct can be weakened to the hypothesis that no cyclic subchain {Li,,Li+j}{L0,,Lk}\{L_{i},\ldots,L_{i+j}\}\subset\{L_{0},\ldots,L_{k}\} arises as the ordered boundary of any non-trivial element of π2(Yϕ,jLj)\pi_{2}(Y_{\phi},\cup_{j}L_{j}). Since holomorphic disks lift uniquely to unramified covers, it would also be sufficient to realise either of these hypotheses after pullback to a covering space, as in Figure 9.

Suppose one has a Lefschetz fibration p:XBp:X\rightarrow B and a finite collection of k+1k+1 cyclically ordered weakly exact matching spheres {Kj}X\{K_{j}\}\subset X which enclose a disk containing no critical points of pp. Suppose that the Lagrangians {Kj}\{K_{j}\} are pairwise distinct, and have the obvious affine AkA_{k}-intersection graph. Let yjKjKj+1y_{j}\in K_{j}\pitchfork K_{j+1} denote the intersection points, for 0jk0\leqslant j\leqslant k with cyclic indices. The following is well-known, and reflects the existence of a relation between the classes [Kj]K0((X))[K_{j}]\in K^{0}(\mathcal{F}(X)).

Lemma 4.14.

If eK0HF0(K0,K0)e_{K_{0}}\in HF^{0}(K_{0},K_{0}) denotes the unit,

(4.7) μk+1(yk,,y0)=±eK0.\mu^{k+1}(y_{k},\ldots,y_{0})=\pm e_{K_{0}}.
Proof.

The coefficient of eK0e_{K_{0}} in the output is well-defined by Lemma 4.13. An iterated application of the long exact triangle in Floer cohomology expresses KkK_{k} as a twisted complex on {K0,,Kk1}\{K_{0},\ldots,K_{k-1}\}, and the non-triviality of (4.7) follows from the Maurer-Cartan equation for the differential in that complex. ∎

Remark 4.15.

Suppose ψ\psi is a holomorphic quadratic differential, and consider a cycle of matching spheres in the 3-fold YψY^{\prime}_{\psi} of (3.1) enclosing a disk with no critical points of ψ\psi, hence in the configuration of the previous Lemma. The non-vanishing of this higher product implies that i=0k|yi|+1k=0\sum_{i=0}^{k}|y_{i}|+1-k=0, which precludes |yi|=1|y_{i}|=1 for every ii. It follows that (Yψ;b)\mathcal{F}(Y^{\prime}_{\psi};b) is not described by a quiver with potential of WKB-type. Compare to Remark 3.22.

The higher product of (4.7) counts disks with k+1k+1 punctures, which extend smoothly across the output puncture but are constrained at the corresponding marked point on the boundary of the disk to pass through a generic point pK0p\in K_{0}, the minimum of the Morse function used to define CF(K0,K0)CF^{*}(K_{0},K_{0}). In particular, consider the moduli space (yk1,,y0)\mathcal{M}_{\ast}(y_{k-1},\ldots,y_{0}) of Maslov zero holomorphic polygons with kk punctures at the given intersection points, and one boundary marked point on the boundary interval between the first and last inputs. The AA_{\infty}-relations then imply that for generic JJ, \mathcal{M}_{\ast} is a closed manifold of dimension n=dim(Kj)n=\dim_{\mathbb{R}}(K_{j}). There is an evaluation map

(4.8) ev:(yk1,,y0)K0ev_{\ast}:\mathcal{M}_{\ast}(y_{k-1},\ldots,y_{0})\longrightarrow K_{0}

which is transverse for generic choices of perturbation data, and Lemma 4.14 implies that

(4.9) evhas degree±1.ev_{\ast}\ \textrm{has degree}\ \pm 1.
Lemma 4.16.

For background class b0b_{0}, the contribution to the multiplication

μ(Y;b0)k:HF1(Lk1,Lk)HF1(L0,L1)HF2(L0,Lk)\mu^{k}_{\mathcal{F}(Y;b_{0})}:HF^{1}(L_{k-1},L_{k})\otimes\cdots\otimes HF^{1}(L_{0},L_{1})\ \longrightarrow\ HF^{2}(L_{0},L_{k})

from holomorphic disks which project to a single WKB cell with multiplicity one is non-trivial.

Proof.

We are essentially in the situation of Lemma 4.13, bearing in mind the remark after that Lemma. Note that our standing hypotheses imply that |𝕄|>1|\mathbb{M}|>1, so the number of faces of the Lagrangian cellulation associated to a non-degenerate WKB triangulation is at least 2. In particular, given any face of the cellulation, there is at least one boundary edge γ\gamma on that face which occurs exactly once in the boundary, separating two distinct embedded open faces on the surface SS. (This need not be true when |𝕄|=1|\mathbb{M}|=1, see Figure 9.)

Following a well-known strategy going back at least to [45], we then apply a degeneration and gluing argument to the situation depicted on the left of Figure 11, which is a schematic for a polygon RR of matching spheres encircling a double pole in SS.

Refer to caption
Figure 11. Bubbling off sections of the local model near a double pole

There is a Lagrangian boundary condition fibred over the dashed circle, and Lemma 4.11 asserts that the algebraic count of isolated holomorphic sections over this inner disk DlocD_{loc} is non-vanishing. There is a degeneration of the restriction of the fibration to this WKB cell, indicated on the right of Figure 11, to a pair of fibrations over disks with boundary marked points, namely the local model and the trivial fibration over a polygon RtrivR_{triv} encircling no singular fibres. In this degeneration, we push the double pole towards an edge γ\gamma which occurs only once on the boundary on the given polygon, so the degeneration on the surface is locally schematically well depicted by Figure 11. The gluing theorem [45, Proposition 2.14] implies that

(4.10) 0(R)p+q=2p(Dloc,e)×Lq(Rtriv,e)\mathcal{M}^{0}(R)\ \cong\ \amalg_{p+q=2}\mathcal{M}^{p}(D_{loc},e)\times_{L}\mathcal{M}^{q}(R_{triv},e)

where i\mathcal{M}^{i} denotes the ii-dimensional component of a space of holomorphic sections over the relevant domain, eγe\in\gamma is the boundary marked point on the fibrations after degeneration, and the fibre product is taken over evaluation into the Lagrangian 2-sphere L=Lγπ1(e)π1(e)L=L_{\gamma}\cap\pi^{-1}(e)\subset\pi^{-1}(e). The evaluation maps are transverse for generic J𝒥ϕJ\in\mathcal{J}_{\phi}, see e.g. [36, Proposition 3.4.2]. On the right of Equation 4.10, we have computed already that p(Dloc,e)\mathcal{M}^{p}(D_{loc},e) is trivial except for p=0p=0; on the other hand, Lemma 4.14 and (4.9) imply that the evaluation map M2(Rtriv,e)M^{2}(R_{triv},e) sweeps LL with multiplicity 1. The fibre-product is therefore non-empty; the moduli space on the left of Equation 4.10 is cobordant to two (transversely cut out) isolated points.

Since the two holomorphic sections contribute to 0(Dloc,e)\mathcal{M}^{0}(D_{loc},e) with the same sign by Lemma 4.11, given our choice of background class b0b_{0}, the holomorphic polygons contribute to μk\mu^{k} with the same sign.∎

If the conic fibres of YϕSY_{\phi}\rightarrow S over points in MM had a different topological type (smooth, Lefschetz singularities, higher multiplicity, empty etc), or if we took b=0b=0, it seems the analogue of Lemma 4.16 would not hold.

4.8. Summary

Fix a non-degenerate triangulation TT of 𝕊\mathbb{S} which satisfies the conditions of Theorem 2.1. Denote by 𝒞(T)=𝒞(Q(T),W(T))\mathcal{C}(T)=\mathcal{C}(Q(T),W(T)) the associated Ginzburg category from Section 2.1, for the trivial signing ϵ1\epsilon\equiv 1. Via Lemma 2.2, pick a meromorphic quadratic differential ϕH0(KS(M)2)\phi\in H^{0}(K_{S}(M)^{\otimes 2}) whose associated WKB triangulation is TT. Let {Le}\{L_{e}\} denote the corresponding WKB Lagrangian spheres, graded as in Lemmas 4.9 and 4.16, and denote by 𝒜b0\mathcal{A}_{b_{0}} the total morphism algebra e,fHF(Le,Lf)\oplus_{e,f}HF^{*}(L_{e},L_{f}) in the category (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}).

Theorem 4.17.

Suppose |𝕄|3|\mathbb{M}|\geqslant 3. The AA_{\infty}-algebra 𝒜b0\mathcal{A}_{b_{0}} is quasi-isomorphic to 𝒞(T)\mathcal{C}(T).

Proof.

We begin by recalling the discussion from the end of Section 4.3. The AA_{\infty}-algebra 𝒜b0=𝒜\mathcal{A}_{b_{0}}=\mathcal{A} is the total morphism algebra of an AA_{\infty}-category over Λ\Lambda_{\mathbb{C}} whose objects are the Lagrangians LeL_{e}, which correspond one-to-one with the vertices of the quiver Q(T)Q(T). From Lemma 4.5 we know that each LeL_{e} has Floer cohomology isomorphic as a graded algebra to H(S3)H^{*}(S^{3}), and the morphisms between the different LeL_{e} are based by the arrows in the quiver Q(T)Q(T), graded as in the construction of the category 𝒞(T)\mathcal{C}(T) in Section 2.1. Thus, as graded vector spaces, 𝒜𝒞(T)\mathcal{A}\cong\mathcal{C}(T) are isomorphic.

Floer theory equips 𝒜\mathcal{A} with an AA_{\infty}-structure which, by homological perturbation, we can take to be minimal and strictly unital. The structure coefficients of this AA_{\infty}-structure count holomorphic polygons with boundary conditions the LeL_{e}, weighted by their symplectic areas. Lemmas 4.6 and 4.7, together with Poincaré duality as in Example 4.8, imply that in the notation of Equation 2.1 the only non-trivial multiplications mn1m_{n-1} in 𝒜\mathcal{A} with n3n\geqslant 3 are exactly those recorded by the corresponding cyclic degree n-n maps cnc_{n}, i.e. the AA_{\infty}-structure is in fact cyclic. It follows that the AA_{\infty}-structure on 𝒜\mathcal{A} may be encoded by the terms of a reduced potential WW on Q(T)Q(T).

Lemma 4.9 implies that there is a non-trivial multiplication m2m_{2} in 𝒜\mathcal{A}, and hence non-trivial cubic term in the potential WW, for each isolated intersection point of a triple of Lagrangians LeL_{e}; indeed, the corresponding Floer product counts a constant disc (of area zero) with co-efficient +1+1. Such isolated triple intersections exactly correspond to the clockwise 3-cycles T(f)T(f) for the faces ff of the triangulation TT, and show that the potential W=fT(f)+W′′W=\sum_{f}T(f)+W^{\prime\prime}, where by definition W′′W^{\prime\prime} is disjoint from fT(f)\sum_{f}T(f). More prosaically, disjointness asserts that none of the oriented 3-cycles corresponding to the oriented triangular faces of Q(T)Q(T) centred on vertices of TT occur in W′′W^{\prime\prime} (each triangular face of Q(T)Q(T) defines three such 3-cycles, pairwise cyclically equivalent).

Lemma 4.16 implies that there are further non-trivial multiplications mkm_{k} in 𝒜\mathcal{A} for each (k+1)(k+1)-dimensional face of the WKB Lagrangian cellulation on SS defined by ϕ\phi. The corresponding coefficients ck+1c_{k+1} in the potential WW are exactly the (anticlockwise-oriented) cycles C(p)C(p) occuring in the quiver Q(T)Q(T) (cf. Figure 1). In the notation of Lemma 4.13, Lemma 4.16 implies that the Floer product μk(xk1,,x0)\mu^{k}(x_{k-1},\ldots,x_{0}) is a non-zero multiple of x¯k\bar{x}_{k}, where the multiple depends on the symplectic area of the polygons occuring in Lemma 4.16 and the orientation (relative to the orientation lines associated to intersection points) of that moduli space: we have established (via Lemma 4.11) that the two holomorphic sections which contribute to the given product count with the same sign, hence cannot cancel, but have not pinned down that sign. At this stage, we may therefore write the potential WW as

(4.11) W=fT(f)pλpC(p)+WW=\sum_{f}T(f)-\sum_{p}\lambda_{p}C(p)+W^{\prime}

where we sum over the faces respectively vertices of Q(T)Q(T), where λp=±2quωΛ\lambda_{p}=\pm 2q^{\int_{u}\omega}\in\Lambda_{\mathbb{C}}^{*} records the area and orientation of the holomorphic discs uu of Lemma 4.16, and where WW^{\prime} is disjoint from the various cycles T(f)T(f) and C(p)C(p). Since [ω]H2(Yϕ,eLe)H0(S,eγe)[\omega]\in H^{2}(Y_{\phi},\cup_{e}L_{e})\cong H^{0}(S,\cup_{e}\gamma_{e}) (with the isomorphism arising from the Leray-Serre spectral sequence of the projection map), the choice of symplectic form not only determines but is essentially equivalent to a choice of (non-zero) scalar coefficients λp\lambda_{p} above.

At this point, we have determined the AA_{\infty}-structure constants which arise either from constant holomorphic polygons or from polygons which project to a single face of the WKB cellulation of SS with multiplicity one. In general there will be additional polygons, for instance those which project to a single cell with higher multiplicity (corresponding to powers C(p)jC(p)^{j} of the cycles C(p)C(p)) or to the union of two adjacent cells (corresponding to a concatenation C(p)C(q)C(p)C(q)), which give rise to the terms in WW^{\prime}. Rather than determining these by hand, we appeal to finite determinacy, via the work of Geiss, Labardini-Fragoso and Schröer. Equation 4.11 shows that the potential WW governing the AA_{\infty}-structure on 𝒜\mathcal{A} is exactly of the form given in Equation 2.3. By Theorem 2.1, we infer that the potential WW is weakly right-equivalent to W(T)W(T), which shows that 𝒜𝒞(T)\mathcal{A}\simeq\mathcal{C}(T) are AA_{\infty}-quasi-isomorphic as required. ∎

We should point out that analogous finite determinacy arguments have been used to pin down AA_{\infty}-structures in symplectic topology elsewhere, going back at least to Seidel’s [48].

Since the quiver category 𝒞(T)\mathcal{C}(T) is independent, up to derived equivalence, on the particular WKB triangulation TT, one can infer the same result for the subcategories Tw𝒜b0\operatorname{Tw}\mathcal{A}_{b_{0}} of (Y;b0)\mathcal{F}(Y;b_{0}) generated by the Lagrangians coming from different cellulations (strictly, provided those cellulations come from triangulations satisfying the hypotheses of Theorem 2.1). Since 𝒟(T)=H0Tw(𝒞(T)){\mathcal{D}}(T)=H^{0}\operatorname{Tw}(\mathcal{C}(T)) is idempotent complete, Theorem 4.17 then implies that

Twπ𝒜b0Tw𝒜b0.\operatorname{Tw}^{\pi}\mathcal{A}_{b_{0}}\ \simeq\ \operatorname{Tw}\,\mathcal{A}_{b_{0}}.

Since 𝒜b0\mathcal{A}_{b_{0}} is tautologically a subcategory of the Fukaya category (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}), on passing to twisted complexes and then cohomology we see that 𝒟(𝒞(T))𝒟(Yϕ;b0){\mathcal{D}}(\mathcal{C}(T))\hookrightarrow{\mathcal{D}}\mathcal{F}(Y_{\phi};b_{0}), which completes the proof of (the first case of) Theorem 1.1 as stated in the Introduction.

4.9. Generation

Fix a non-degenerate triangulation TT. This subsection outlines one approach to proving that 𝒜(T;b0)\mathcal{A}(T;b_{0}) generates the subcategory 𝒦(Yϕ;b0)(Yϕ;b0)\mathcal{K}(Y_{\phi};b_{0})\subset\mathcal{F}(Y_{\phi};b_{0}) generated by all matching spheres. This sketch falls far short of a proof, but it seems worth including in part because one sees the Harder-Narasimhan filtration of a matching sphere with respect to the stability condition determined by ϕ\phi emerge as a natural ingredient in the argument.

There are two pieces of background for the sketch. Let LL and LL^{\prime} denote two matching spheres which meet transversely once, at a vertex pp of the cellulation. Consider the Lagrange surgery L#LL\#L^{\prime} of LL and LL^{\prime} at pp, which is equivalently given by taking the Dehn twist of LL^{\prime} about LL. (There are two local surgeries, corresponding to the positive and negative Dehn twists; here we are taking pHF1(L,L)p\in HF^{1}(L,L^{\prime}), a morphism from LL to LL^{\prime}.) Seidel’s theorem [45] yields a distinguished triangle in 𝒦(Yϕ;b)\mathcal{K}(Y_{\phi};b)

(4.12) L\textstyle{L\ignorespaces\ignorespaces\ignorespaces\ignorespaces}L\textstyle{L^{\prime}\ignorespaces\ignorespaces\ignorespaces\ignorespaces}L#L\textstyle{L\#L^{\prime}\ignorespaces\ignorespaces\ignorespaces\ignorespaces}[1]\scriptstyle{[1]}

This gives a long exact sequence of Floer cohomology groups in YϕY_{\phi}

HF(L′′,L)μ2(p,)HF(L′′,L)HF(L′′,L#L)\cdots\rightarrow HF(L^{\prime\prime},L)\xrightarrow{\mu^{2}(p,\cdot)}HF(L^{\prime\prime},L^{\prime})\rightarrow HF(L^{\prime\prime},L\#L^{\prime})\rightarrow\cdots

for any third Lagrangian submanifold L′′(Y;b)L^{\prime\prime}\in\mathcal{F}(Y;b), and shows the Lagrange surgery L#LL\#L^{\prime} is generated by the two constituent Lagrangians LL and LL^{\prime}.

The second piece of background concerns Floer theory for immersed Lagrangians [3]. Consider a closed saddle trajectory γ0\gamma_{0} for ϕ\phi of phase θ\theta, going from a zero to itself. If we assume that the residue of ϕ\phi at each double pole does not belong to eiθ<0e^{i\theta}\mathbb{R}_{<0}, then γ0\gamma_{0} forms one boundary component of a ring domain, the other boundary of which is a union of straight arcs also of phase θ\theta (the hypothesis on the residues rules out the degenerate case in which the other boundary component collapses onto a double pole). The closed saddle γ0\gamma_{0} defines an immersed Lagrangian 3-sphere Lγ0YϕL_{\gamma_{0}}\hookrightarrow Y_{\phi}. Despite being immersed, this has well-defined Floer cohomology (indeed Lγ0L_{\gamma_{0}} is still strictly unobstructed, i.e. bounds no holomorphic disks, so this is straightforward), and

HF(Lγ0,Lγ0)H(S3)k2HF(L_{\gamma_{0}},L_{\gamma_{0}})\cong H^{*}(S^{3})\oplus k^{\oplus 2}

where the second summand arises from the node of Lγ0L_{\gamma_{0}}.

The suggested route to generation of 𝒦(Yϕ;b0)\mathcal{K}(Y_{\phi};b_{0}) by 𝒜(T;b0)\mathcal{A}(T;b_{0}) has three ingredients.

Step 1. Let γ0\gamma_{0} be as above, and suppose for simplicity that both boundaries of the ring domain containing γ0\gamma_{0} are composed of a single saddle (this is true for generic ϕ\phi, compare to the discussion of hat-proportional saddles in [5, Section 5]).

Refer to caption
Figure 12. A non-degenerate ring domain with a pair of arcs α,β\alpha,\beta.

Let α,β\alpha,\beta be two ϕ\phi-geodesics inside the ring domain bound by γ0\gamma_{0}, as in Figure 12, defining embedded matching spheres LαL_{\alpha}, LβL_{\beta} in YϕY_{\phi} with

HF(Lα,Lβ)kxkyHF(L_{\alpha},L_{\beta})\cong k\langle x\rangle\oplus k\langle y\rangle

where {x,y}\{x,y\} denote the zeroes on the boundary of the ring domain and xx belongs to γ0\gamma_{0}. It seems natural to conjecture that the immersed sphere is quasi-isomorphic to the cone

(4.13) Lγ0(LαyLβ).L_{\gamma_{0}}\simeq(L_{\alpha}\stackrel{{\scriptstyle y}}{{\longrightarrow}}L_{\beta}).

This is a version of (4.12), in a setting where the surgery is unobstructed but immersed (in particular cannot be interpreted in terms of a Dehn twist). One roundabout approach to a proof of (4.13) would appeal to known results on homological mirror symmetry for the 3-dimensional affine A2A_{2}-singularity, which provides a local model for two spherical objects having a two-dimensional space of extensions, cf. the discussion of the representation theory of the quiver (J1) in [5, Section 11].

Step 2. The existence theorem for geodesics in flat surfaces implies that a given matching path γS\gamma\subset S is homotopic to a concatenation of ϕ\phi-geodesics γγj0γjk\gamma\simeq\gamma_{j_{0}}\ast\cdots\ast\gamma_{j_{k}}, where each γji\gamma_{j_{i}} is embedded in its interior (hence is either a geodesic matching path or a closed geodesic from a zero to itself). Given the correspondence between geodesics and stable objects [5, Theorem 1.4], this decomposition should reflect the Harder-Narasimham filtration of LγL_{\gamma} in the stability condition associated to ϕ\phi, and (especially in light of [56]) there are obvious potential connections to mean curvature flow. In particular, one expects that LγLγj0,,LγjkL_{\gamma}\in\langle L_{\gamma_{j_{0}}},\ldots,L_{\gamma_{j_{k}}}\rangle, where \langle\cdots\rangle denotes the extension-closed subcategory generated by the given objects. An inductive argument might reduce that claim to the special cases of the surgery exact triangle discussed above.

Step 3. At this point, one would know that any Lagrangian matching sphere is generated by the subset of matching spheres coming from ϕ\phi-geodesics. An embedded ϕ\phi-geodesic τ\tau of phase θ\theta occurs as one of the WKB-Lagrangians for the cellulation associated to ei(θ+δ)ϕe^{-i(\theta+\delta)}\phi, for sufficiently small δ\delta, compare to [5, Figure 32]. If the triangulation TT^{\prime} associated to this rotated differential is non-degenerate, it is immediate from Theorem 1.1 and the fact that 𝒟(T)𝒟(T){\mathcal{D}}(T)\simeq{\mathcal{D}}(T^{\prime}) that LτL_{\tau} is generated by the category 𝒜(T;b0)\mathcal{A}(T;b_{0}) associated to the triangulation TT defined by ϕ\phi itself.

However, if ei(θ+δ)ϕe^{-i(\theta+\delta)}\phi has a triangulation TT^{\prime} with self-folded triangles, this is more delicate. To conclude that 𝒜(T;b0)\mathcal{A}(T;b_{0}) generates 𝒦(Yϕ;b0)\mathcal{K}(Y_{\phi};b_{0}), at least by this method, one would need further to introduce the algebras 𝒜(T;b0)\mathcal{A}(T^{\prime};b_{0}) for arbitrary, not necessarily non-degenerate triangulations TT^{\prime}, and to prove that 𝒜(T;b0)𝒟(T)\mathcal{A}(T^{\prime};b_{0})\simeq{\mathcal{D}}(T^{\prime}) in this wider setting. Note in particular that any such argument would seem to hinge on an extension of the results of [18] to this more general setting. Assuming that such an extension had been carried out, however, one could then conclude the desired generation: LγL_{\gamma} would be generated by geodesics, geodesics arise as WKB-Lagrangians for some triangulation, and all the subcategories of (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}) associated to triangulations would be quasi-equivalent.

5. Miscellany

5.1. Higher order poles

Suppose we have a marked bordered surface (𝕊,𝕄)(\mathbb{S},\mathbb{M}) with 𝕊\partial\mathbb{S}\neq\emptyset, arising from a quadratic differential ϕ\phi on a Riemann surface SS with a non-empty set of poles of order 3\geqslant 3. We construct the 3-fold YϕS\Pol3(ϕ)Y_{\phi}\rightarrow S\backslash\mathrm{Pol}_{\geqslant 3}(\phi) as indicated in the Introduction.

The preceding arguments need only minimal changes to yield the second case of Theorem 1.1. The locally free sheaf WW now has first Chern class 3KS+2M=2+3M33K_{S}+2M_{=2}+3M_{\geqslant 3}, in the notation of (1.2). The proof of Lemma 3.5 then implies that the projective completion XϕX_{\phi} has canonical class 𝒪(2)π(M3)\mathcal{O}_{\mathbb{P}}(-2)\otimes\pi^{*}(-M_{\geqslant 3}), which again means that after removing Δπ1(M3)\Delta_{\infty}\cup\pi^{-1}(M_{\geqslant 3}) the open 3-fold YϕY_{\phi} is a smooth Calabi-Yau222Since the coefficients in the divisor M3=pPol3(ϕ)ord(p)/2pM_{\geqslant 3}=\sum_{p\in\mathrm{Pol}_{\geqslant 3}(\phi)}\lceil ord(p)/2\rceil p are all 2\geqslant 2, the holomorphic volume form κϕ\kappa_{\phi} again has poles of order at least 2 at infinity.. It is moreover affine, and one can work with a symplectic structure which is exact and contact type at infinity, which obviates the need to control rational curves via intersection theory at infinity.

Lemma 3.14 changes. We now view the differential ϕ\phi as a section of the bundle KS(M)2K_{S}(M)^{\otimes 2}, where the divisor M=pPol(ϕ)ord(p)/2pM=\sum_{p\in\mathrm{Pol}(\phi)}\lceil ord(p)/2\rceil p, which means ϕ\phi has simple zeroes at odd order poles, and hence the local system R2πR^{2}\pi_{*}\mathbb{Z} picks up monodromy at odd order poles. The identification of H3(Yϕ;)H_{3}(Y_{\phi};\mathbb{Z}) with the anti-invariant homology of a spectral double cover goes through only if that cover is branched at both zeroes and odd order poles. The upshot is that H3(Yϕ;)H_{3}(Y_{\phi};\mathbb{Z}) is now free of rank

n=6g6+pPol(ϕ)(ord(p)+1).n=6g-6+\sum_{p\in\mathrm{Pol}(\phi)}(ord(p)+1).

Lemma 3.11 carries over unchanged. The construction of symplectic forms, matching spheres, and the grading of the WKB algebra, were all essentially local arguments on SS, as were the computations of the contribution of constant holomorphic triangles and non-constant polygons covering WKB cells with multiplicity one. At this stage, one sees that the AA_{\infty}-structure on the WKB algebra 𝒜\mathcal{A} is given by a potential of the shape W(T,ϵ)+WW(T,\epsilon)+W^{\prime} as before. Finally, the crucial result Theorem 2.1 of Geiss, Labardini-Fragoso and Schröer also holds in the non-empty boundary case (with no further constraints on the number of punctures), which enables one to conclude the proof as before.

Example 5.1.

Consider (𝕊,𝕄)(\mathbb{S},\mathbb{M}) to be an annulus with pp respectively qq marked points on the two boundary components. This corresponds to differentials on 1\mathbb{P}^{1} with poles of order p+2p+2 and q+2q+2 and n=p+qn=p+q simple zeroes. The quiver QQ is a non-cyclic orientation of the affine An1A_{n-1}-Dynkin diagram, with trivial potential. The Lagrangian spheres of a WKB collection form a cycle of nn matching spheres encircling the origin; the vanishing of the potential reflects the fact that the threefold fibres over \mathbb{C}^{*}, and there are no non-constant holomorphic polygons (by the maximum principle applied in \mathbb{C}^{*}). Note that the poles of the holomorphic volume form and resulting grading of the endomorphism algebra of the WKB collection depend on the decomposition n=p+qn=p+q. Compare to [5, Section 12.3].

5.2. Simple poles

Whilst one can construct the triangulated category associated to (𝕊,𝕄)(\mathbb{S},\mathbb{M}) by starting with a non-degenerate ideal triangulation defined by a point ϕ\phi of the open stratum Quad(𝕊,𝕄)0Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0}\subset\operatorname{Quad}(\mathbb{S},\mathbb{M}), the space of stability conditions on 𝒟𝒦((𝕊,𝕄);b)){\mathcal{D}}\mathcal{K}((\mathbb{S},\mathbb{M});b)) is (an orbifolded version of) the larger space Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M}) in which the differentials may acquire simple poles by having zeroes collide with double poles. The universal family 𝒴Quad(𝕊,𝕄)0\mathcal{Y}\rightarrow\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0} of threefolds (which exists locally) does not extend to Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M}) as a locally trivial fibre bundle. In any extension of the universal family there must be a non-trivial degeneration of YϕY_{\phi} when ϕ\phi acquires a simple pole, to account for the non-triviality of the monodromy action on H2(Yϕ;2)H^{2}(Y_{\phi};\mathbb{Z}_{2}) described in Lemma 3.12, which exchanges components of the reducible fibre.

Return to the local model

{a2δbc=ϕ(δ)t2}[a,b,c,t]3×δ\{a^{2}-\delta\,bc=\phi(\delta)t^{2}\}\subset\mathbb{P}^{3}_{[a,b,c,t]}\times\mathbb{C}_{\delta}

for the neighbourhood of the reducible fibre {a2t2=0}3×{0}\{a^{2}-t^{2}=0\}\subset\mathbb{P}^{3}\times\{0\} inside XϕX_{\phi}, where ϕH0(KS(M)2)\phi\in H^{0}(K_{S}(M)^{\otimes 2}) has a double pole at δ=0S\delta=0\in S and ϕ(0)=1\phi(0)=1. Suppose instead that we have a differential ϕ0\phi_{0} with ϕ0(0)=0\phi_{0}(0)=0, so the quadratic differential ϕ0\phi_{0} has a simple pole at the corresponding point of SS. The corresponding 3-fold

Xϕ0={a2=δ(bc+t2}3×δX_{\phi_{0}}\ =\ \{a^{2}=\delta(bc+t^{2}\}\subset\mathbb{P}^{3}\times\mathbb{C}_{\delta}

has a multiple fibre {a2=0}\{a^{2}=0\}, and is singular along a smooth conic curve {a=0=δ,bc+t2=0}\{a=0=\delta,\,bc+t^{2}=0\}. The transversal singularity is a surface ordinary double point.

It is tempting to associate to a quadratic differential ϕ0\phi_{0} with a simple pole at pMp\in M a smooth 3-fold

Yϕ0SY_{\phi_{0}}\rightarrow S

with fibre T2T^{*}\mathbb{R}\mathbb{P}^{2}, with multiplicity 2, over pp. For suitable symplectic forms, there is a Lagrangian 3Yϕ0\mathbb{R}\mathbb{P}^{3}\subset Y_{\phi_{0}}, fibred by a Morse-Bott function over an arc from a zero to pp (the vanishing cycle of the zero converges at pp to the 2\mathbb{R}\mathbb{P}^{2} Bott minimum). The two Lagrangian spheres depicted on the right side of Figure 4, which should persist in the category defined by ϕ0\phi_{0} since this does not change in passing from Quad(𝕊,𝕄)0\operatorname{Quad}(\mathbb{S},\mathbb{M})_{0} to Quad(𝕊,𝕄)\operatorname{Quad}(\mathbb{S},\mathbb{M}), would now be realised by this 3\mathbb{R}\mathbb{P}^{3}, equipped with either the trivial or the non-trivial spin structure or equivalently 2\mathbb{Z}_{2}-valued local system. It would be interesting to find a model (of this or another form) for the “locally trivial family of categories” over a point of the incomplete locus.

5.3. No poles

Let SS be a Riemann surface of genus 2\geqslant 2. Consider again the 3-fold YψY^{\prime}_{\psi} from (3.1) associated to a holomorphic quadratic differential ψ\psi on SS with distinct zeroes. This has a fibrewise compactification which is a Lefschetz fibration over SS with generic fibre 1×1\mathbb{P}^{1}\times\mathbb{P}^{1}. According to [53, Corollary 4.9], there is an equivalence of 2\mathbb{Z}_{2}-graded split-closed categories

(5.1) Dπ(1×1)λ=0Dπ(S0)D^{\pi}\mathcal{F}(\mathbb{P}^{1}\times\mathbb{P}^{1})_{\lambda=0}\ \simeq\ D^{\pi}\mathcal{F}(S^{0})

between the nilpotent summand of the Fukaya category of the even-dimensional quadric, i.e. that corresponding to the zero eigenvalue of quantum product with the first Chern class, and the Fukaya category of a pair of points (both categories are semisimple). The paper [53] works over \mathbb{C}, but the argument underlying the equivalence of (5.1) (which uses the computation of a certain Gromov-Witten invariant counting sections of a Lefschetz fibration with fibre 1×1\mathbb{P}^{1}\times\mathbb{P}^{1} and some elementary deformation theory) goes through over any algebraically closed characteristic zero field. Starting from this, one can show in the spirit of [53, Section 5] that, over the Novikov field Λ\Lambda_{\mathbb{C}}, the 2\mathbb{Z}_{2}-graded category underlying (Yψ)\mathcal{F}(Y^{\prime}_{\psi}) admits a formal deformation which is split-closed derived equivalent to the 2\mathbb{Z}_{2}-graded Fukaya category (C)\mathcal{F}(C) of the spectral cover CSC\rightarrow S, i.e. the double cover of SS branched at the zeroes of ψ\psi.

That equivalence takes the matching sphere LγL_{\gamma} considered in this paper to the obvious circle lying over γ\gamma in the double covering CC. An essential simple closed curve σS\sigma\subset S defines a Lagrangian (S1×S2)Yψ(S^{1}\times S^{2})\subset Y^{\prime}_{\psi} and a disjoint union of two circles in CC. The ring structures on the Floer cohomologies of these objects is different (only one has a non-trivial degree zero idempotent), which suggests that the deformation of categories from Dπ(Yψ)D^{\pi}\mathcal{F}(Y^{\prime}_{\psi}) to Dπ(C)D^{\pi}\mathcal{F}(C) induced by the compactification of the fibres is non-trivial.

5.4. The untwisted category

For each bH2(Yϕ;2)b\in H^{2}(Y_{\phi};\mathbb{Z}_{2}) there is a total morphism algebra 𝒜(T;b)=e,fTHF(Le,Lf)\mathcal{A}(T;b)=\oplus_{e,f\in T}HF^{*}(L_{e},L_{f}) associated to a collection of Lagrangian matching spheres indexed by edges of a non-degenerate triangulation TT. The quasi-isomorphism type of this algebra will depend on the choice of bb, even though its idempotent pieces HF(Le,Le)HF(L_{e},L_{e}) do not. Theorem 1.1 concerns the case b=b0b=b_{0} and the twisted Fukaya category (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}), and it is natural to consider the untwisted category (Yϕ)\mathcal{F}(Y_{\phi}) corresponding to taking b=0b=0.

Lemma 4.11 determined the signs with which the two rigid disks with boundary on Γ\Gamma contribute to their moduli space. These discs cancelled in the category (Yϕ)\mathcal{F}(Y_{\phi}). Therefore, the category 𝒟(𝒜(T;0)){\mathcal{D}}(\mathcal{A}(T;0)) is obtained by replacing the potential of (2.2) by its first term fT(f)\sum_{f}T(f), killing the higher AA_{\infty}-products; alternatively, it arises if one constructs the threefold YϕY_{\phi} by removing the conic fibres over all poles of ϕ\phi, and not just those of order >2>2. This category is drastically different to 𝒟(𝒜;b0){\mathcal{D}}(\mathcal{A};b_{0}), see the example considered in Section 5.5.

Moreover, in contrast to Remark 4.12, the Lagrangian cylinder LσS1×S2L_{\sigma}\cong S^{1}\times S^{2} does define an object of the untwisted category (Yϕ)\mathcal{F}(Y_{\phi}) if one allows unobstructed branes. The category (Yϕ)\mathcal{F}(Y_{\phi}) cannot be generated by matching spheres: the Lagrangian cylinder LσL_{\sigma} can be deformed through non-Hamiltonian deformations (shrinking the loop σ\sigma) to be disjoint from any given matching path in SMS-M, but (in the untwisted category) still with non-trivial Floer cohomology.

5.5. An example

Consider a differential on 1\mathbb{P}^{1} with poles of order 22 and 44; this case was considered in [5, Section 12]. The relevant quiver has two vertices and no arrows, and the category 𝒦((𝕊,𝕄);b0)\mathcal{K}((\mathbb{S},\mathbb{M});b_{0}) is generated by two Lagrangian spheres L1,L2L_{1},L_{2} with HF(L1,L2)={0}HF(L_{1},L_{2})=\{0\}. All objects are isomorphic to direct sums of shifts of the LiL_{i}. These objects are depicted on the left of Figure 13, where the black dot denotes the double pole and the higher order pole lies at 1\infty\in\mathbb{C}\mathbb{P}^{1}.

Refer to caption
Figure 13. The generators of (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}), and a non-isotopic sphere defining an equivalent object.

The vanishing of Floer cohomology relies on the choice of the non-trivial background class, which ensures the two rigid disks which project onto the obvious region bound by these arcs count with the same sign: the differential

(5.2) :CF(L1,L2)=k[1]k[2]k[1]k[2]=CF(L1,L2)\partial:CF^{*}(L_{1},L_{2})=k[1]\oplus k[2]\rightarrow k[1]\oplus k[2]=CF^{*}(L_{1},L_{2})

maps the degree one generator to a non-trivial multiple of the degree two generator.

On the other hand, there are infinitely many pairwise non-Hamiltonian isotopic Lagrangian spheres in YϕY_{\phi}, distinguished in the split-closed twisted Fukaya category Twπ(Yϕ)\operatorname{Tw}^{\pi}\mathcal{F}(Y_{\phi}) by the rank of Floer cohomology with the non-compact Lefschetz thimble dotted in the right of Figure 13 (with background class b=0b=0 the differential in (5.2) vanishes, and spherical objects can then arise from non-trivial twisted complexes based on the LiL_{i}). Turning on the background class b0b_{0} collapses all of these distinct objects onto shifts of L1L_{1} and L2L_{2} (direct sums are excluded by considering the rank of self Floer cohomology). Therefore isomorphism in the category (Yϕ;b0)\mathcal{F}(Y_{\phi};b_{0}) is very far from implying Hamiltonian isotopy.

5.6. Open directions

It is natural to wonder if [5] and Theorem 1.1 have applications to the classical symplectic topology of YϕY_{\phi}, or to representation theory. The results established so far fall slightly short of what seems to be required, although there are several obvious avenues for further study.

There are natural representations (the first defined by parallel transport)

(5.3) π1(Quad±(𝕊,𝕄)0)π0Symp(Yϕ;b0)Auteq𝒟(Yϕ;b0)/[2]\pi_{1}(\operatorname{Quad}^{\pm}(\mathbb{S},\mathbb{M})_{0})\longrightarrow\pi_{0}\,\mathrm{Symp}(Y_{\phi};b_{0})\longrightarrow\mathrm{Auteq}\,{\mathcal{D}}\mathcal{F}(Y_{\phi};b_{0})/\langle[2]\rangle

where the middle term refers to mapping classes preserving b0H2(Yϕ;2)b_{0}\in H^{2}(Y_{\phi};\mathbb{Z}_{2}) and where on the right we quotient by the square of the shift functor. It follows from results of [5] that if the space of stability conditions StabΔ(𝕊,𝕄)\operatorname{Stab}_{\Delta}(\mathbb{S},\mathbb{M}) studied there is simply-connected, then the first arrow is injective: but simple-connectivity of StabΔ(𝕊,𝕄)\operatorname{Stab}_{\Delta}(\mathbb{S},\mathbb{M}) is currently unknown (see however [40] for progress in this direction).

When 𝕊\partial\mathbb{S}\neq\emptyset one can kill the fundamental group of YϕY_{\phi} by subcritical handle attachments at infinity, to obtain symplectic six-manifolds which are simply-connected but admit symplectomorphisms of positive Floer-theoretic entropy, and which have subgroups of autoequivalences of the Fukaya category which surject onto mapping class groups. This may be of some interest, since whilst such examples are known, they are not yet terribly numerous.

In another direction, the second map of (5.3) does surject onto the quotient of the subgroup of autoequivalences which preserve StabΔ(𝕊,𝕄)\operatorname{Stab}_{\Delta}(\mathbb{S},\mathbb{M}) by those which act trivially (“negligible” autoequivalences in the terminology of [5]). There are many situations in which autoequivalences of derived Fukaya categories have no geometric origin, i.e. do not arise from symplectomorphisms, see e.g. [2].

Finally, the existence of a smooth compactification divisor Δ^\hat{\Delta}_{\infty} for YϕY_{\phi} gives rise to a spectral sequence computing symplectic cohomology SH(Yϕ)SH^{*}(Y_{\phi}), see [46]. That in turn leads to conjectural bounds on the ranks of the Hochschild cohomology groups of the Ginzburg algebra A(Q,W)A(Q,W) which might be of independent interest. It would be instructive, in this vein, to relate the wrapped Fukaya category of YϕY_{\phi} to the derived category of all (not necessarily finite-dimensional) modules over the complete Ginzburg algebra.

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