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3 Moduli space of holomorphic curves [0495]

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3 Moduli space of holomorphic curves

The theme of this Chapter is the bordism currents produced from the (n+1)(n+1)-dimensional universal family over the (n−1)(n-1)-dimensional moduli spaces of holomorphic curves. This theme unifies the search for the Floer theoretic obstructions, and the problem of extending the Solomon functional to the derived Fukaya category setting. One of our central techniques is integration over the moduli spaces, to prove both identities and inequalities. The primary setting of this Chapter is exact graded compact Lagrangians inside Calabi-Yau Stein manifolds, with occasional comments on the compact Calabi-Yau case.

The Floer theoretic obstructions are necessary conditions to the existence of special Lagrangians in the exact and almost calibrated setting. We will give a large number of a priori heuristic principles to place very stringent constraints on what kind of obstructions we are looking for, then prove the Floer theoretic obstructions under the extra hypotheses of automatic transversality and a positivity condition (cf. section 3.5), and then compare our picture to Joyce’s proposal on Bridgeland stability (cf. section 3.6). The converse direction, in search of sufficient conditions for the existence of special Lagrangians, will be laid out in Chapter 5.

We also present two perspectives on extending the Solomon functional to unobstructed Lagrangians within the same Db​F​u​k​(X)D^{b}Fuk(X) class. The more elementary perspective (cf. section 3.2) works only in the exact setting, and implies the first variation formula under Hamiltonian isotopies in a rather straightforward manner. The second perspective (cf. section 3.7) represents the Solomon functional as an integral over the moduli space of holomorphic curves, which we hope can be generalized to the compact Calabi-Yau setting. Section 3.8 contains more applications of the moduli integral technique.

Remark 3.1.

The two assumptions of automatic transversality (which roughly means that no perturbation of almost complex structure is needed, cf. section 3.3) and the positivity condition (cf. section 3.4) will feature prominently in the major results of this Chapter. Correspondingly, we will not dwell on the detail of the perturbation schemes aimed at overcoming the transversality issues, which are painstakingly carried out in [7][81][82][14][15]. The expert readers may convert to their favourite schemes as they prefer. For more on our clockwise conventions such as gradings and signs, which differ from many symplectic texts, see the Appendix.

3.1 Lotay-Pacini picture revisited

From a Floer theoretic perspective, the main insight of Lotay and Pacini (cf. section 2.9) is that given two Lagrangians L,L′L,L^{\prime} decorated with suitable brane structures, one should look for a family of holomorphic curves with boundary on LL and L′L^{\prime}, which pass through any generic point of LL and L′L^{\prime}. In their formal picture, such families are called ‘geodesics’. What Lotay and Pacini did not provide is a good existence criterion for their geodesics. Now, even though we will soon specialize to a much simpler setting, we wish to explain how their geodesics fit into the Thomas-Yau-Joyce picture.

In the setup of Bridgeland stability, the central charge is defined as a homomorphism from the Grothendieck group of a triangulated category to ℂ\mathbb{C}, which factorizes through a finitely generated lattice, viewed as a numerical Grothendieck group. In view of the application to special Lagrangians, the triangulated category is Db​F​u​k​(X)D^{b}Fuk(X), and the numerical Grothendieck group should be a subgroup of the homology group modulo torsion Hn​(X,ℤ)/torsH_{n}(X,\mathbb{Z})/\text{tors}. In particular,

  • •

    If two Lagrangian branes L,L′L,L^{\prime} define the same object in Db​F​u​k​(X)D^{b}Fuk(X), then this picture predicts them to lie in the same homology class in Hn​(X)H_{n}(X).

  • •

    If L1→L→L2→L1​[1]L_{1}\to L\to L_{2}\to L_{1}[1] is a distinguished triangle, then [L1]+[L2]=[L][L_{1}]+[L_{2}]=[L] in Hn​(X)H_{n}(X).

This means Floer theory must provide a bordism current between L,L′L,L^{\prime} (resp. LL and L1∪L2L_{1}\cup L_{2}), namely an (n+1)(n+1)-dimensional integration current 𝒞\mathcal{C} with ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} (resp. ∂𝒞=L−L1−L2\partial\mathcal{C}=L-L_{1}-L_{2}).4242 42 The boundary of integration currents do not detect contributions from supports of small enough dimension. In this respect they are similar to pseudocycles, although when we generalize to Lagrangians with very weak regularity later, the language of currents may be more natural. In Floer theory, cycles are constructed from moduli spaces of holomorphic curves and evaluation maps, so this current 𝒞\mathcal{C} should come from families of holomorphic curves, possibly with highly sophisticated perturbations and virtual techniques. This suggests the Lotay-Pacini geodesics, construed in this homological sense, should be part of the Fukaya category foundation necessary for the Thomas-Yau-Joyce program.

High brow viewpoint

The claim that the KK-theory of the derived Fukaya category of a symplectic Calabi-Yau manifold (exact with suitable convexity at infinity, or compact) factorizes through homology Hn​(X)H_{n}(X) modulo torsion seems well known to symplectic topology experts, although a precise reference seems rather difficult to find. We now sketch a high brow viewpoint explained to the author by P. Seidel and S. Rezchikov, and will later explain in more detail a more pedestrian approach in the exact setting. The claim is a formal consequence of the existence of maps

K0​(Db​F​u​k​(X))→c​h0H​H0​(Db​F​u​k​(X))K_{0}(D^{b}Fuk(X))\xrightarrow{ch_{0}}HH_{0}(D^{b}Fuk(X))
H​H0​(Db​F​u​k​(X))→O​CQ​Hn​(X,Λn​o​v)≃Hn​(X)⊗Λn​o​v.HH_{0}(D^{b}Fuk(X))\xrightarrow{OC}QH^{n}(X;\Lambda_{nov})\simeq H_{n}(X)\otimes\Lambda_{nov}.

Here H​H0​(Db​F​u​k​(X))HH_{0}(D^{b}Fuk(X)) is the Hochschild homology in degree zero. The first map sends the K-theory class of an unobstructed Lagrangian brane LL (compact, graded, oriented, with spin and bounding cochain structure) to the unit 1L∈H​F0​(L,L)→H​H0​(Db​F​u​k​(X))1_{L}\in HF^{0}(L,L)\to HH_{0}(D^{b}Fuk(X)); the well definition of this map is an essentially algebraic fact. Suppose L,L′L,L^{\prime} are isomorphic in Db​F​u​k​(X)D^{b}Fuk(X), then there are closed morphisms α∈C​F0​(L,L′)\alpha\in CF^{0}(L,L^{\prime}) and β∈C​F0​(L′,L)\beta\in CF^{0}(L^{\prime},L) whose derived category compositions are equal to 1L∈H​F0​(L,L)1_{L}\in HF^{0}(L,L) and 1L′∈H​F0​(L′,L′)1_{L^{\prime}}\in HF^{0}(L^{\prime},L^{\prime}) in cohomology. The Hochschild differential of β⊗α\beta\otimes\alpha exhibits 1L−1L′1_{L}-1_{L^{\prime}} as a coboundary in the Hochschild chain complex, so 1L=1L′1_{L}=1_{L^{\prime}} in H​H0​(Db​F​u​k​(X))HH_{0}(D^{b}Fuk(X)). Some additional calculation shows the compatibility with distinguished triangles.

The second map is a special case of the open-closed string map, and in general requires working over the Novikov field. One then needs the claim that 1L1_{L} is sent to the homology class [L]∈Hn​(X)[L]\in H_{n}(X), without quantum correction. The intuitive meaning of the open-closed string map is to consider holomorphic discs with boundary on LL with an unconstrained boundary marked point, and find the cycle in XX traced out by an interior marked point. The claim amounts to saying that the only contribution comes from constant maps. Unfortunately, the author is unable to locate a general reference. Granted this claim, we would get by composition a map from K0​(Db​F​u​k​(X))K_{0}(D^{b}Fuk(X)) to Hn​(X,Λn​o​v)H_{n}(X;\Lambda_{nov}) which sends the K-theory class of LL to the homology class [L][L].

3.1.1 The exact embedded Lagrangian case

We specialize to the setting of Stein manifolds, and all Lagrangians are assumed to be exact, graded and compact, and in particular carry an orientation (cf. the Appendix for some basic Floer theory). The local systems have holonomy in ℝ\mathbb{R}, ℚ\mathbb{Q} or ℤ\mathbb{Z}. We consider two transverse embedded Lagrangians L,L′L,L^{\prime} in the same derived Fukaya category class. By definition, we have closed morphisms α∈C​F0​(L,L′)\alpha\in CF^{0}(L,L^{\prime}) and β∈C​F0​(L′,L)\beta\in CF^{0}(L^{\prime},L); we sometimes view the Lagrangian intersections in β\beta as degree nn outputs. Morever, in terms of the product structure on cohomology

{H​F0​(L,L′)⊗H​F0​(L′,L)→H​F0​(L′,L′),H​F0​(L′,L)⊗H​F0​(L,L′)→H​F0​(L,L),\begin{cases}HF^{0}(L,L^{\prime})\otimes HF^{0}(L^{\prime},L)\to HF^{0}(L^{\prime},L^{\prime}),\\ HF^{0}(L^{\prime},L)\otimes HF^{0}(L,L^{\prime})\to HF^{0}(L,L),\end{cases}

the composition α∘β=1L′\alpha\circ\beta=1_{L^{\prime}} and β∘α=1L\beta\circ\alpha=1_{L}. These conditions completely characterize isomorphism in Db​F​u​k​(X)D^{b}Fuk(X). Our goal is to explain

Proposition 3.1.

There is a bordism current 𝒞\mathcal{C} such that ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} in the sense of currents.

The bordism current will be constructed from universal families of (perturbed) holomorphic strips with boundary on LL and L′L^{\prime}, and with ends at α\alpha and β\beta (meaning that the ends of the strip converge to intersection points of L,L′L,L^{\prime} of degree 00 and nn respectively, and α,β\alpha,\beta encode the weighting factors to the contribution of these intersection points). We will assume all the usual transversality assumptions in Floer theory are satisfied, so the compactified moduli space ℳ⁡(α,β)/ℝ¯\overline{\mathcal{M}(\alpha,\beta)/\mathbb{R}} of perturbed holomorphic strips up to domain translation is a smooth manifold with boundary and corners, of dimension (n−1)(n-1). The notation really stands for a formal sum of many moduli spaces, coming from the summands of α,β\alpha,\beta. The universal family is fibred over this moduli space ℳ⁡(α,β)/ℝ¯\overline{\mathcal{M}(\alpha,\beta)/\mathbb{R}}, whose fibres are the solutions to the Cauchy-Riemann equation (with domain dependent perturbations of the almost complex structure), which we call perturbed holomorphic curves. The fibres over the boundary of the moduli space are broken holomorphic curves. The orientation on the universal family is induced from the complex orientation on Σ\Sigma and the orientation on the moduli space, up to an extra minus sign (cf. Example 6.2 for conventions). Upon evaluation to XX we obtain an (n+1)(n+1)-dimensional current 𝒞\mathcal{C}.

Remark 3.2.

If the Fukaya category is defined over ℤ\mathbb{Z}, then all the weighting factors to the various universal families are all integers, and 𝒞\mathcal{C} is naturally an integral current. If we use Fukaya categories over ℚ\mathbb{Q} or ℝ\mathbb{R} instead, then 𝒞\mathcal{C} is only guaranteed to be a finite ℚ\mathbb{Q} (resp. ℝ\mathbb{R}) linear combination of integral currents.

Our main task is to understand the boundary of 𝒞\mathcal{C}. There are two sources of boundaries:

  • •

    The holomorphic curves themselves have boundary along L∪L′L\cup L^{\prime}. This boundary contribution is always supported on L∪L′L\cup L^{\prime}.

  • •

    The compactified moduli spaces have boundary due to holomorphic strip breaking.

In schematic notation, the boundary of the moduli space is described by

∂(ℳ⁡(α,β)/ℝ¯)=⋃rℳ⁡(α,r)/ℝ¯×ℳ⁡(r,β)/ℝ¯.\partial(\overline{\mathcal{M}(\alpha,\beta)/\mathbb{R}})=\bigcup_{r}\overline{\mathcal{M}(\alpha,r)/\mathbb{R}}\times\overline{\mathcal{M}(r,\beta)/\mathbb{R}}. (16)

Here rr can range from all intersection points of degree between 11 and n−1n-1. The notation ℳ⁡(α,β)/ℝ\mathcal{M}(\alpha,\beta)/\mathbb{R} stands for a weighted sum of moduli spaces, with weighting coming from the holonomy factors of the local systems.

Next comes a crucial observation. Although 2≤deg⁡r≤n−22\leq\deg r\leq n-2 give rise to boundaries of the moduli space ℳ⁡(α,β)/ℝ¯\overline{\mathcal{M}(\alpha,\beta)/\mathbb{R}}, their contributions to ∂𝒞\partial\mathcal{C} are contained in the universal families associated to ℳ⁡(α,r)/ℝ¯\overline{\mathcal{M}(\alpha,r)/\mathbb{R}} and ℳ⁡(r,β)/ℝ¯\overline{\mathcal{M}(r,\beta)/\mathbb{R}}. These smaller moduli spaces have dimension at most n−3n-3, and the corresponding universal families have dimension at most n−1n-1. By rectifiability considerations, the nn-dimensional current ∂𝒞\partial\mathcal{C} cannot receive contributions from at most (n−1)(n-1)-dimensional supports, so such disc breakings do not contribute to ∂𝒞\partial\mathcal{C}.

Now for deg⁡r=1\deg r=1, the moduli spaces ℳ⁡(α,r)/ℝ¯\overline{\mathcal{M}(\alpha,r)/\mathbb{R}} are zero dimensional, so their presence merely amounts to some counting factors. The condition for α\alpha to be closed in C​F0​(L,L′)CF^{0}(L,L^{\prime}) is equivalent to the weighted count of ℳ⁡(α,r)/ℝ¯\overline{\mathcal{M}(\alpha,r)/\mathbb{R}} being zero. This weighted sum appears as the coefficient of the nn-dimensional current defined by the universal family over ℳ⁡(r,β)/ℝ¯\overline{\mathcal{M}(r,\beta)/\mathbb{R}}. Thus we see that r∈C​F1​(L,L′)r\in CF^{1}(L,L^{\prime}) does not contribute to ∂𝒞\partial\mathcal{C}. Similarly, the condition for β\beta to be closed in C​F0​(L′,L)CF^{0}(L^{\prime},L) implies that r∈C​F1​(L′,L)r\in CF^{1}(L^{\prime},L) (alternatively viewed as degree n−1n-1 intersections from LL to L′L^{\prime}) does not contribute to ∂𝒞\partial\mathcal{C}. In summary, ∂𝒞\partial\mathcal{C} must be an integration cycle supported on L∪L′L\cup L^{\prime}.

Since ∂𝒞\partial\mathcal{C} is itself the boundary of a current, it must be closed. This explains why ∂𝒞\partial\mathcal{C} is a constant linear combination of the integration cycle of LL and L′L^{\prime}, instead of some nontrivial function times these cycles. The constant coefficients can be pinned down by counting the number of holomorphic strips passing through a given generic point on LL (resp. L′L^{\prime}), and the choice of the generic point does not matter. Such counts are precisely the geometric interpretation of the Floer product H​F0​(L,L′)⊗H​F0​(L′,L)→H​F0​(L′,L′),HF^{0}(L,L^{\prime})\otimes HF^{0}(L^{\prime},L)\to HF^{0}(L^{\prime},L^{\prime}), and H​F0​(L′,L)⊗H​F0​(L,L′)→H​F0​(L,L)HF^{0}(L^{\prime},L)\otimes HF^{0}(L,L^{\prime})\to HF^{0}(L,L) (cf. Example 6.1). When the moduli space orientations are taken into account, we obtain ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} (cf. Example 6.2 for an exposition on signs).

Remark 3.3.

(Homological uniqueness of the bordism current) Some auxiliary perturbation data goes into the construction of 𝒞\mathcal{C} due to the need to ensure transversality. If we fix L,L′L,L^{\prime}, but change the domain dependent almost complex structures, then the difference of two bordism currents 𝒞−𝒞′\mathcal{C}-\mathcal{C}^{\prime} has zero boundary in the sense of currents. Recall that Stein manifolds have the homotopy type of a CW complex of dimension ≤n\leq n, and thus Hk​(X)=0H_{k}(X)=0 for k≥n+1k\geq n+1, so 𝒞−𝒞′\mathcal{C}-\mathcal{C}^{\prime} must be the boundary of an (n+2)(n+2)-dimensional current. For an alternative viewpoint, this (n+2)(n+2)-dimensional current can be concretely provided by parametrized families of pseudoholomorphic curves (cf. Remark 3.5).

3.1.2 Immersed case

Still working in the exact setting, we now allow (L,b),(L′,b′)(L,b),(L^{\prime},b^{\prime}) to be unobstructed immersed Lagrangians with transverse self intersections. Assume they intersect transversally, and define isomorphic objects in Db​F​u​k​(X)D^{b}Fuk(X). We now wish to explain why Proposition 3.1 should continue to hold even in the immersed setting, without delving too deep into the specifics of the perturbation schemes and transversality issues. For some background on the immersed Floer theory, see the Appendix 6.2.

The isomorphism condition gives us closed morphisms α∈C​F0​(L,L′)\alpha\in CF^{0}(L,L^{\prime}) and β∈C​F0​(L′,L)\beta\in CF^{0}(L^{\prime},L) whose cohomological compositions give the identities. At the chain level,

m2b,b′​(β,α)=1L−m1b​(γ),m2b′,b​(α,β)=1L′+m1b′​(γ′)m_{2}^{b,b^{\prime}}(\beta,\alpha)=1_{L}-m_{1}^{b}(\gamma),\quad m_{2}^{b^{\prime},b}(\alpha,\beta)=1_{L^{\prime}}+m_{1}^{b^{\prime}}(\gamma^{\prime})

where 1L,1L′1_{L},1_{L^{\prime}} stand for the geometric units (represented by a sum of local maximum points of Hamiltonian functions on L,L′L,L^{\prime} respectively), and γ,γ′\gamma,\gamma^{\prime} are elements in C​F−1​(L,L)CF^{-1}(L,L), C​F−1​(L′,L′)CF^{-1}(L^{\prime},L^{\prime}) respectively. Notice in the almost calibrated case, γ,γ′\gamma,\gamma^{\prime} would be both zero, since there are no self intersections of degree −1-1.

As before, the bordism current shall be constructed from the universal family of (perturbed) holomorphic curves with boundary on LL and L′L^{\prime}. But instead of working only with holomorphic strips, we need holomorphic polygons with corners not only at intersection points in α,β\alpha,\beta, but also at points in b,b′b,b^{\prime}. In addition to the holomorphic strip moduli space ℳ⁡(α,β)/ℝ\mathcal{M}(\alpha,\beta)/\mathbb{R}, we also need the moduli space of polygons ℳ⁡(b,…​b,α,b′,…​b′,β)\mathcal{M}(b,\ldots b,\alpha,b^{\prime},\ldots b^{\prime},\beta), and ℳ⁡(b,…,b,γ)\mathcal{M}(b,\ldots,b,\gamma), ℳ⁡(b′,…​b′,γ′)\mathcal{M}(b^{\prime},\ldots b^{\prime},\gamma^{\prime}). The notation here is a shorthand for a weighted sum of many moduli spaces of polygons. Since the bounding cochain elements have Floer degrees one, these moduli spaces all have dimension n−1n-1. The energy of the polygons satisfies the topological formula (66), so by the Novikov positivity requirement of bounding cochains, there is a uniform a priori energy bound once α,β,γ,γ′\alpha,\beta,\gamma,\gamma^{\prime} are given, whence there are in fact only finitely many moduli spaces involved. Each moduli space provides a universal family of holomorphic curves, and the sum of all the contributions defines an (n+1)(n+1)-dimensional current 𝒞\mathcal{C}. For sign conventions, see the Appendix 6.2, and Example 6.2.

The boundary of 𝒞\mathcal{C} comes from two sources: the boundary of the individual holomorphic curves which lie on L∪L′L\cup L^{\prime}, and the boundary of the compactified moduli spaces. In the exact setting, there are no sphere bubbles. As in the embedded case, for support dimension reasons, the boundaries of the compactified moduli space that can contribute to ∂𝒞\partial\mathcal{C}, is caused by curve breaking into two pieces arising in 00 and n−2n-2 dimensional moduli spaces. The cancellation of these contributions is very similar to the standard argument for the Floer differential to square to zero (cf. the Appendix 6.2):

  • •

    For breakings at a nodal point mapping to C​F1​(L,L′)CF^{1}(L,L^{\prime}) (resp. C​F1​(L′,L)CF^{1}(L^{\prime},L)), the contributions vanish due to the closedness condition m1b,b′​(α)=0m_{1}^{b,b^{\prime}}(\alpha)=0 (resp. the closedness of β\beta).

  • •

    For breakings at degree 2 self intersection point on LL (resp. L′L^{\prime}), the contributions vanish due to the Mauer-Cartan equation on bb (resp. b′b^{\prime}).

  • •

    A new way of disc breaking/splitting, is at a degree zero self intersection rr on LL (the L′L^{\prime} case being entirely similar). The discs of ℳ⁡(b,…​b,α,b′,…​b′,β)\mathcal{M}(b,\ldots b,\alpha,b^{\prime},\ldots b^{\prime},\beta) can break into a virtual dimension zero disc with input at b,…,α,b′,…​β,b,…​bb,\ldots,\alpha,b^{\prime},\ldots\beta,b,\ldots b and output at rr, and a virtual dimension n−1n-1 disc with input corners at b,…​b,rb,\ldots b,r. On the other hand, the discs of ℳ⁡(b,…,b,γ)\mathcal{M}(b,\ldots,b,\gamma) can break into a virtual dimension zero disc with input at b,…,γ,b,…​bb,\ldots,\gamma,b,\ldots b and output at rr, and a virtual dimension n−1n-1 disc with input corners at b,…​b,rb,\ldots b,r. These two effects cancel out.

After the cancellation of all moduli space boundaries, the only contributions ∂𝒞\partial\mathcal{C} are supported in L∪L′L\cup L^{\prime}. As in the embedded case, ∂𝒞\partial\mathcal{C} is locally a constant multiple of the underlying cycles of L,L′L,L^{\prime}. The interpretation of the geometric unit pins down ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} as in the embedded case.

Example 3.2.

If LL and L′L^{\prime} are disjoint Lagrangian branes which both define the zero object in Db​F​u​k​(X)D^{b}Fuk(X), then α,β\alpha,\beta are both zero, and 𝒞\mathcal{C} comes entirely from the γ,γ′\gamma,\gamma^{\prime} contributions. Of course, zero Lagrangian objects have zero homology class, which cannot happen in the almost calibrated case.

Remark 3.4.

If there are degree −2-2 self intersections of LL, then the choice of γ\gamma is only unique up to m1bm_{1}^{b} of some element in C​F−2​(L,L)CF^{-2}(L,L). The corresponding choice of 𝒞\mathcal{C} would be ambiguous by the boundary of an (n+2)(n+2)-dimensional integration current. As a closely related issue, our conditions on α,β\alpha,\beta are merely cohomological, so in general we can adjust α\alpha and β\beta by coboundary terms, which would affect 𝒞\mathcal{C} also by the boundary of an (n+2)(n+2) dimensional current. If we impose L,L′L,L^{\prime} to be almost calibrated, then there are no C​F−1​(L,L′)CF^{-1}(L,L^{\prime}) elements to begin with, and these phenomena do not happen.

On the other hand, 𝒞\mathcal{C} still depends on the choice of local systems and bounding cochains, which may contribute nontrivial holonomy factors. Gauge equivalent choices affect 𝒞\mathcal{C} by the boundary of an (n+2)(n+2)-dimensional current. One may naturally ask:

Question 3.

Up to gauge equivalence of bounding cochains and local systems, is there an optimal representative of 𝒞\mathcal{C}?

Question 4.

Given an exact isotopy with surgery between LL and L′L^{\prime} among unobstructed Lagrangians, is there a preferred choice of 𝒞\mathcal{C} (cf. Question 2)?

Distinguished triangles

In our convention, an immersed Lagrangian can be made up of several connected components. A prototypical situation is when L′L^{\prime} is the union of two immersed Lagrangians L1L_{1} and L2L_{2}, with some degree one intersections in C​F1​(L2,L1)CF^{1}(L_{2},L_{1}) arising as part of the bounding cochain data of L′L^{\prime}. When the brane structure is taken into account, we can view L′L^{\prime} as a twisted complex built from L1,L2L_{1},L_{2} (with bounding cochains b1,b2b_{1},b_{2} suppressed in the notation) and a closed morphism γ∈C​F1​(L2,L1)=C​F0​(L2​[−1],L1)\gamma\in CF^{1}(L_{2},L_{1})=CF^{0}(L_{2}[-1],L_{1}). Inside Db​F​u​k​(X)D^{b}Fuk(X),

L≃L′≃((L2,b2)γ(L1,b1)).L\simeq L^{\prime}\simeq\left(\begin{matrix}(L_{2},b_{2})&\\ \gamma&(L_{1},b_{1})\end{matrix}\right).

We have a distinguished triangle

L2​[−1]→𝛾L1→Cone​(γ)→L2,L_{2}[-1]\xrightarrow{\gamma}L_{1}\to\text{Cone}(\gamma)\xrightarrow{}L_{2},

and L≃L′≃Cone​(γ)L\simeq L^{\prime}\simeq\text{Cone}(\gamma). Rotating the triangles, we get another distinguished triangle

L1→L→L2→𝛾L1​[1].L_{1}\to L\to L_{2}\xrightarrow{\gamma}L_{1}[1].

The bordism current between LL and L′L^{\prime} is an (n+1)(n+1)-dimensional integration current, with ∂𝒞=L−L1−L2.\partial\mathcal{C}=L-L_{1}-L_{2}. In particular, this explains that the Grothendieck group of Db​F​u​k​(X)D^{b}Fuk(X) should factorize through Hn​(X)H_{n}(X).

Here is a more geometric perspective on the bordism currents arising from distinguished triangles, which is very close to Thomas and Yau’s original viewpoint, where the fundamental phenomenon is Lagrangian breaking. In the simplest case, we can imagine LL is isomorphic in Db​F​u​k​(X)D^{b}Fuk(X) to the Lagrangian connected sum L1​#​L2L_{1}\#L_{2} (beware our convention for L1​#​L2L_{1}\#L_{2} is the same as Thomas-Yau [65] but different from many symplectic texts), so that we can construct a bordism current between LL and L1​#​L2L_{1}\#L_{2}. Now when L1​#​L2L_{1}\#L_{2} deforms, the Lagrangian handle part can shrink, and in the limit L1​#​L2L_{1}\#L_{2} can break into two components L1∪L2L_{1}\cup L_{2} (cf. Example 2.12). The bordism current between LL and L1∪L2L_{1}\cup L_{2} should simply be the limit of the sequence of bordism currents. This picture illustrates that even when the topology of the Lagrangians can change under non-smooth convergence, the bordism currents should persist in a continuous way.

One can proceed with the case of many Lagrangians, namely we take the immersed Lagrangian L′L^{\prime} to be the twisted complex (cf. the Appendix section 6.2)

((LN,bN)bN,N−1(LN−1,bN−1)…bN,1bN−1,1…b2,1(L1,b1)).\left(\begin{matrix}(L_{N},b_{N})&&\\ b_{N,N-1}&(L_{N-1},b_{N-1})&\\ \ldots\\ b_{N,1}&b_{N-1,1}&\ldots&b_{2,1}&(L_{1},b_{1})\end{matrix}\right). (17)

In this case, assuming LL is isomorphic to L′L^{\prime} in Db​F​u​k​(X)D^{b}Fuk(X), the bordism current between LL and L′L^{\prime} amounts to a bordism current between LL and L1∪L2​…∪LNL_{1}\cup L_{2}\ldots\cup L_{N}.

This multi-Lagrangian situation is built out of many distinguished triangles: for 1≤k≤N1\leq k\leq N, let ℰk\mathcal{E}_{k} be the immersed Lagrangian L1∪…∪LkL_{1}\cup\ldots\cup L_{k} corresponding to the twisted complex

((Lk,bk)bk,k−1(Lk−1,bk−1)…bk,1bk−1,1…b2,1(L1,b1)).\left(\begin{matrix}(L_{k},b_{k})&&\\ b_{k,k-1}&(L_{k-1},b_{k-1})&\\ \ldots\\ b_{k,1}&b_{k-1,1}&\ldots&b_{2,1}&(L_{1},b_{1})\end{matrix}\right). (18)

Then (suppressing bounding cochains in the notation) we have a sequence in Db​F​u​k​(X)D^{b}Fuk(X),

0=ℰ0→ℰ1→…→ℰN≃L,0=\mathcal{E}_{0}\to\mathcal{E}_{1}\to\ldots\to\mathcal{E}_{N}\simeq L,

with distinguished triangles

ℰi−1→ℰi→Li→ℰi−1​[1].\mathcal{E}_{i-1}\to\mathcal{E}_{i}\to L_{i}\to\mathcal{E}_{i-1}[1].

The morphism from LiL_{i} to ℰi−1\mathcal{E}_{i-1} comes from bi,jb_{i,j} for j<ij<i. This setup should be reminiscent of Harder-Narasimhan decompositions (4), although at this stage we have not yet brought in stability conditions, which shall be discussed further in section 3.6.

3.2 Solomon functional revisited

Let (X,ω,Ω)(X,\omega,\Omega) be an almost Calabi-Yau Stein manifold, and LL be an exact Lagrangian brane, with ∫LIm​(e−i​θ^​Ω)=0\int_{L}\text{Im}(e^{-i\hat{\theta}}\Omega)=0 for some suitable θ^∈(−π2,π2)\hat{\theta}\in(-\frac{\pi}{2},\frac{\pi}{2}). Our goal is to suggest how the Solomon functional may be well defined without the universal cover issue, and extended beyond a given exact isotopy class. Both issues are essential for the variational approach to the Thomas-Yau conjecture, see Chapter 5.

Homological nature of the Solomon functional

Write the Liouville 1-form as λ\lambda, so d​λ=ωd\lambda=\omega, and the potential of the immersed Lagrangian LL as fLf_{L}, so d​fL=λ|Ldf_{L}=\lambda|_{L}. We consider the potential as part of the brane data, so adding a constant to fLf_{L} is viewed as a different Lagrangian brane. We shall consider a path of such Lagrangians LtL_{t}, with associated Hamiltonian functions hth_{t}, so there is a preferred way to parallel transport fLf_{L}, as recalled below.

Lemma 3.3.
∫01dt∫LthtIm(e−i​θ^Ω)=∫LtfLtIm(e−i​θ^Ω)|t=0t=1−∫∪tLtλ∧Im(e−i​θ^Ω).\int_{0}^{1}dt\int_{L_{t}}h_{t}\text{Im}(e^{-i\hat{\theta}}\Omega)=\int_{L_{t}}f_{L_{t}}\text{Im}(e^{-i\hat{\theta}}\Omega)|^{t=1}_{t=0}-\int_{\cup_{t}L_{t}}\lambda\wedge\text{Im}(e^{-i\hat{\theta}}\Omega). (19)
Proof.

Let XtX_{t} be the Hamiltonian vector field along LtL_{t} associated to hth_{t}, namely d​ht=ω⁡(Xt,⋅)dh_{t}=\omega(X_{t},\cdot). We calculate the time derivative of fLtf_{L_{t}}: along LtL_{t}

ℒX​λ=ιX​d​λ+d⁡(ιX​λ)=ιX​ω+d⁡(ιX​λ)=d⁡(ht+ιX​λ),\mathcal{L}_{X}\lambda=\iota_{X}d\lambda+d(\iota_{X}\lambda)=\iota_{X}\omega+d(\iota_{X}\lambda)=d(h_{t}+\iota_{X}\lambda),

so there is a preferred parallel transport of fLf_{L} along the path LtL_{t},

∂tfLt=ht+ιX​λ.\partial_{t}f_{L_{t}}=h_{t}+\iota_{X}\lambda.

Hence

∂t∫LtfLt​Im​(e−i​θ^​Ω)=∫Lt(ht+ιX​λ)​Im​(e−i​θ^​Ω)+∫LtfLt​ℒX​Im​(e−i​θ^​Ω).\partial_{t}\int_{L_{t}}f_{L_{t}}\text{Im}(e^{-i\hat{\theta}}\Omega)=\int_{L_{t}}(h_{t}+\iota_{X}\lambda)\text{Im}(e^{-i\hat{\theta}}\Omega)+\int_{L_{t}}f_{L_{t}}\mathcal{L}_{X}\text{Im}(e^{-i\hat{\theta}}\Omega).

Now by the Cartan formula and the closedness of Ω\Omega,

ℒX​Im​(e−i​θ^​Ω)=d​ιX​Im​(e−i​θ^​Ω),\mathcal{L}_{X}\text{Im}(e^{-i\hat{\theta}}\Omega)=d\iota_{X}\text{Im}(e^{-i\hat{\theta}}\Omega),

so after integration by part,

∫LtfLtℒXIm(e−i​θ^Ω)=−∫Ltdft∧ιXIm(e−i​θ^Ω)=−∫Ltλ∧ιXIm(e−i​θ^Ω).\int_{L_{t}}f_{L_{t}}\mathcal{L}_{X}\text{Im}(e^{-i\hat{\theta}}\Omega)=-\int_{L_{t}}df_{t}\wedge\iota_{X}\text{Im}(e^{-i\hat{\theta}}\Omega)=-\int_{L_{t}}\lambda\wedge\iota_{X}\text{Im}(e^{-i\hat{\theta}}\Omega).

Combining the above,

∂t∫LtfLt​Im​(e−i​θ^​Ω)=∫Ltht​Im​(e−i​θ^​Ω)+∫LtιX​(λ∧Im​(e−i​θ^​Ω)).\partial_{t}\int_{L_{t}}f_{L_{t}}\text{Im}(e^{-i\hat{\theta}}\Omega)=\int_{L_{t}}h_{t}\text{Im}(e^{-i\hat{\theta}}\Omega)+\int_{L_{t}}\iota_{X}(\lambda\wedge\text{Im}(e^{-i\hat{\theta}}\Omega)).

Integrating in tt gives the result. ∎

We observe that by the Kähler condition ω∧Ω=0\omega\wedge\Omega=0, so

d⁡(λ∧Im​(e−i​θ^​Ω))=ω∧Im​(e−i​θ^​Ω)=0.d(\lambda\wedge\text{Im}(e^{-i\hat{\theta}}\Omega))=\omega\wedge\text{Im}(e^{-i\hat{\theta}}\Omega)=0.

This means the term ∫∪tLtλ∧Im(e−i​θ^Ω)\int_{\cup_{t}L_{t}}\lambda\wedge\text{Im}(e^{-i\hat{\theta}}\Omega) is a homological quantity, in the sense that we can replace ∪tLt\cup_{t}L_{t} by any compactly supported (n+1)(n+1)-current 𝒞\mathcal{C} with ∂𝒞=L1−L0\partial\mathcal{C}=L_{1}-L_{0}, which would automatically satisfy [𝒞−∪tLt]=0∈Hn+1(X)[\mathcal{C}-\cup_{t}L_{t}]=0\in H_{n+1}(X), since Hn+1​(X)=0H_{n+1}(X)=0 for Stein manifolds. In particular, this explains Solomon’s theorem that his functional is invariant under Hamiltonian deformations of the path of Lagrangians. The advantage of our homological interpretation is to allow more general currents 𝒞\mathcal{C}, which in particular can come from families of holomorphic curves.

Proposed extension of the Solomon functional

Taking the homological interpretation of (19) as starting point, a natural way to extend the Solomon functional is to make use of the bordism current 𝒞\mathcal{C} between an unobstructed Lagrangian LL and a fixed unobstructed reference Lagrangian L0L_{0}. We have ∂𝒞=L−L0\partial\mathcal{C}=L-L_{0} as currents, and 𝒞\mathcal{C} comes from the universal family of holomorphic curves. Our proposed formula is

𝒮⁡(L)=∫LfL​Im​(e−i​θ^​Ω)−∫L0fL0​Im​(e−i​θ^​Ω)−Im​∫𝒞λ∧e−i​θ^​Ω.\mathcal{S}(L)=\int_{L}f_{L}\text{Im}(e^{-i\hat{\theta}}\Omega)-\int_{L_{0}}f_{L_{0}}\text{Im}(e^{-i\hat{\theta}}\Omega)-\text{Im}\int_{\mathcal{C}}\lambda\wedge e^{-i\hat{\theta}}\Omega. (20)

A few conceptual points are in order:

  • •

    We emphasize that this depends not only on the underlying Lagrangian, but also on the potential fLf_{L}.

  • •

    There is no need to pass to any universal cover in the space of Lagrangians, as in Solomon’s work (cf. section 2.8).

  • •

    The topology of LL is no longer fixed, and in particular the Hamiltonian isotopy class may change.

  • •

    We view (20) as a unification of the very different viewpoints of Solomon and Lotay-Pacini. In section 2.10 we suggested that this extended Solomon functional may be relevant for quantum tunneling amplitudes between the branes L0L_{0} and LL.

  • •

    Suppose we vary the Lagrangian LL within a 1-parameter exact isotopy family of unobstructed Lagrangians LtL_{t}. The bordism currents 𝒞t\mathcal{C}_{t} between LtL_{t} and L0L_{0} satisfy

    𝒞t2=𝒞t1+∪t1≤t≤t2Lt modulo exact (n+1)-dim currents,\mathcal{C}_{t_{2}}=\mathcal{C}_{t_{1}}+\cup_{t_{1}\leq t\leq t_{2}}L_{t}\text{ modulo exact $(n+1)$-dim currents},

    then the computation in Lem 3.3 proves the first variation formula for the Solomon functional

    dd​t​𝒮​(Lt)=∫Ltht​Im​(e−i​θ^​Ω)\frac{d}{dt}\mathcal{S}(L_{t})=\int_{L_{t}}h_{t}\text{Im}(e^{-i\hat{\theta}}\Omega) (21)

    which is of course the defining feature of the Solomon functional. Consequently, the formula (20) extends Solomon’s definition in our exact setting, and fixes the multivaluedness problem (i.e. the need to pass to universal covers) in Solomon’s work.

Change of reference Lagrangian

The definition of the Solomon functional depends on the reference Lagrangian L0L_{0}, and we write 𝒮L0​(L)\mathcal{S}_{L_{0}}(L) when we wish to emphasize this dependence. The following feature of the Solomon functional resembles the Donaldson functional in the HYM context (cf. (9)):

Proposition 3.4.

Under the change of reference Lagrangians,

𝒮L0​(L)=𝒮L0′​(L)+𝒮L0​(L0′).\mathcal{S}_{L_{0}}(L)=\mathcal{S}_{L_{0}^{\prime}}(L)+\mathcal{S}_{L_{0}}(L_{0}^{\prime}). (22)
Proof.

We shall use the homological nature of the Solomon functional and the fact that Hn+1​(X)=0H_{n+1}(X)=0. We pick 𝒞1,𝒞2,𝒞3\mathcal{C}_{1},\mathcal{C}_{2},\mathcal{C}_{3} such that

∂𝒞1=L−L0′,∂𝒞2=L0′−L0,∂𝒞3=L−L0.\partial\mathcal{C}_{1}=L-L_{0}^{\prime},\quad\partial\mathcal{C}_{2}=L_{0}^{\prime}-L_{0},\quad\partial\mathcal{C}_{3}=L-L_{0}.

Then 𝒞1+𝒞2\mathcal{C}_{1}+\mathcal{C}_{2} is homologous to 𝒞3\mathcal{C}_{3}, so we can replace 𝒞3\mathcal{C}_{3} by 𝒞1+𝒞2\mathcal{C}_{1}+\mathcal{C}_{2} to compute 𝒮L0​(L)\mathcal{S}_{L_{0}}(L), whence (22) follows. ∎

Remark 3.5.

A more Floer theoretic argument that 𝒞1+𝒞2\mathcal{C}_{1}+\mathcal{C}_{2} is homologous to 𝒞3\mathcal{C}_{3}, which does not appeal to Hn+1​(X)=0H_{n+1}(X)=0 directly, can be sketched as follows. We assume L0,L0′,LL_{0},L_{0}^{\prime},L are three unobstructed Lagrangians mutually isomorphic in Db​F​u​k​(X)D^{b}Fuk(X), and H​F−1​(L0,L0)=0HF^{-1}(L_{0},L_{0})=0. Of course, the self Floer cohomologies of L0,L0′,LL_{0},L_{0}^{\prime},L are all isomorphic, and H​F−1=0HF^{-1}=0 is a necessary condition if the Db​F​u​k​(X)D^{b}Fuk(X) class admits any almost calibrated representative at all. We consider α∈C​F0​(L0,L0′),β∈C​F0​(L0′,L),γ∈C​F0​(L,L0)\alpha\in CF^{0}(L_{0},L_{0}^{\prime}),\beta\in CF^{0}(L_{0}^{\prime},L),\gamma\in CF^{0}(L,L_{0}) representing the generators of H​F0HF^{0}, such that at the level of Floer cohomology

γ∘β∘α=1L0,α∘γ∘β=1L0′,β∘α∘γ=1L.\gamma\circ\beta\circ\alpha=1_{L_{0}},\quad\alpha\circ\gamma\circ\beta=1_{L_{0}^{\prime}},\quad\beta\circ\alpha\circ\gamma=1_{L}.

For simplicity we first assume almost calibratedness, so that C​F−1=0CF^{-1}=0, and there is no ambiguity for these generators. Notice the compositions β∘α,γ∘β,α∘γ\beta\circ\alpha,\gamma\circ\beta,\alpha\circ\gamma provide generators of H​F0​(L0,L)HF^{0}(L_{0},L), H​F0​(L0′,L0)HF^{0}(L_{0}^{\prime},L_{0}), H​F0​(L,L0′)HF^{0}(L,L_{0}^{\prime}). Consider the nn-dimensional moduli spaces ℳ~\tilde{\mathcal{M}} of holomorphic discs with corners at α,β,γ\alpha,\beta,\gamma and the self intersection points corresponding to the bounding cochains. The corresponding universal family 𝒞~\tilde{\mathcal{C}} provides an (n+2)(n+2)-dimensional current, whose boundary comes from disc bubbling and disc breaking. Most of the boundary contributions are eliminated by the Mauer-Cartan equation of the bounding cochains, the closedness of α,β,γ\alpha,\beta,\gamma, and support dimension reasons, and only three boundary contributions survive. These are the (n+1)(n+1)-dimensional bordism currents between L0,L0′L_{0},L_{0}^{\prime} (resp. L0′,LL_{0}^{\prime},L and L,L0L,L_{0}) constructed from the universal family of holomorphic curves associated to the generators α,−γ∘β\alpha,-\gamma\circ\beta (resp. β,−α∘γ\beta,-\alpha\circ\gamma and γ,β∘α\gamma,\beta\circ\alpha). We can identify these as 𝒞2,𝒞1,−𝒞3\mathcal{C}_{2},\mathcal{C}_{1},-\mathcal{C}_{3}. The upshot is that Floer theory explicitly provides the (n+2)(n+2)-dimensional current that exhibits the homological relation between 𝒞1+𝒞2\mathcal{C}_{1}+\mathcal{C}_{2} and 𝒞3\mathcal{C}_{3}.

In general without assuming almost calibratedness, then C​F−1CF^{-1} can be nonzero. Then we need some extra nn-dimensional moduli spaces to account for the non-uniqueness of cohomological representatives of H​F0HF^{0}, an issue quite similar to section 3.1.2. A subtle new issue is that the moduli space ℳ~\tilde{\mathcal{M}} receives new boundary contributions involving the m3bm_{3}^{b} products (this shorthand notation indicates the presence of bounding cochain elements, cf. (73)) of α,β,γ\alpha,\beta,\gamma. The three cyclic permutations of α,β,γ\alpha,\beta,\gamma produce three m3bm_{3}^{b} products, which are elements in C​F−1​(L0,L0),C​F−1​(L0′,L0′)CF^{-1}(L_{0},L_{0}),CF^{-1}(L_{0}^{\prime},L_{0}^{\prime}) and C​F−1​(L,L)CF^{-1}(L,L) respectively, and the (n−1)(n-1)-dimensional moduli of polygons with one corner at the C​F−1CF^{-1} intersections and the other corners at bounding cochain elements contribute to ∂𝒞~\partial\tilde{\mathcal{C}}. Now by the A∞A_{\infty} relation, and the closedness of α,β,γ\alpha,\beta,\gamma,

m1b​(m3b​(γ,β,α))+m2b​(γ,m2b​(β,α))−m2b​(m2b​(γ,β),α)=0.m_{1}^{b}(m_{3}^{b}(\gamma,\beta,\alpha))+m_{2}^{b}(\gamma,m_{2}^{b}(\beta,\alpha))-m_{2}^{b}(m_{2}^{b}(\gamma,\beta),\alpha)=0.

Writing m2b​(γ,m2b​(β,α))=1L0+m1b​(δ1)m_{2}^{b}(\gamma,m_{2}^{b}(\beta,\alpha))=1_{L_{0}}+m_{1}^{b}(\delta_{1}) and m2b​(m2b​(γ,β),α)=1L0+m1b​(δ2)m_{2}^{b}(m_{2}^{b}(\gamma,\beta),\alpha)=1_{L_{0}}+m_{1}^{b}(\delta_{2}), we see m3b​(γ,β,α)+δ1−δ2m_{3}^{b}(\gamma,\beta,\alpha)+\delta_{1}-\delta_{2} is m1bm_{1}^{b}-closed, so by the assumption that H​F−1​(L0,L0)=0HF^{-1}(L_{0},L_{0})=0, it is in fact −m1b​(ϵ1)-m_{1}^{b}(\epsilon_{1}) for some ϵ1∈C​F−2​(L0,L0)\epsilon_{1}\in CF^{-2}(L_{0},L_{0}). We can then produce an nn-dimensional moduli space, from polygons with a corner at ϵ1\epsilon_{1}, and other corners at the bounding cochain elements. Completely analogously, one can produce two other nn-dimensional moduli spaces from ϵ2∈C​F−2​(L0′,L0′)\epsilon_{2}\in CF^{-2}(L_{0}^{\prime},L_{0}^{\prime}) and ϵ3∈C​F−2​(L,L)\epsilon_{3}\in CF^{-2}(L,L). Combining the (n+2)(n+2)-dimensional universal families over the nn-dimensional moduli spaces, results in an explicit bordism current between 𝒞1+𝒞2\mathcal{C}_{1}+\mathcal{C}_{2} and 𝒞3\mathcal{C}_{3}.

3.3 Automatic transversality

In our later applications, it is not enough to just have a bordism current between Lagrangians L,L′L,L^{\prime} constructed from perturbed pseudoholomorphic curves. Two additional conditions are desirable: automatic transversality and positivity condition. These are natural properties of the highly idealized picture of Lotay and Pacini (cf. section 2.9), but may seem rather strong for Floer theorists.

In this section we discuss various sufficient conditions for automatic transversality, which intuitively means that the bordism current 𝒞\mathcal{C} is constructed without perturbing the integrable complex structure. This requires that the (extended) linearized Cauchy-Riemann operator is surjective, namely the moduli space is regular. The next section will discuss the positivity condition. Complex integrability and the existence of holomorphic volume form Ω\Omega will be assumed throughout. All holomorphic curves are assumed to be nonconstant.

  • •

    (Automatic transversality) There exist a finite collection of (n−1)(n-1)-dimensional smooth moduli spaces of holomorphic curves u:Σ→Xu:\Sigma\to X with respect to the integrable complex structure, constructed from the inputs in C​F0​(L,L′)CF^{0}(L,L^{\prime}), C​F0​(L′,L)≃C​Fn​(L,L′)∨CF^{0}(L^{\prime},L)\simeq CF^{n}(L,L^{\prime})^{\vee} and the bounding cochain data as in section 3.1, such that by taking the weighted sum of the (n+1)(n+1)-dimensional universal families of holomorphic curves, we obtain a current 𝒞\mathcal{C} with ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime}. This bordism current 𝒞\mathcal{C} agrees with the bordism currents constructed from generically perturbed almost complex structures, up to the boundary of an (n+2)(n+2)-dimensional current.

    Morever, considering the boundary of holomophic curves ∂Σ\partial\Sigma varying in the (n−1)(n-1) dimensional regular moduli spaces, we obtain nn-dimensional universal families, sweeping out the cycle L−L′L-L^{\prime}; we require the evaluation map from these nn-dimensional universal family to L∪L′L\cup L^{\prime} to be immersions, except at the corner points of ∂Σ\partial\Sigma mapping to the Lagrangian intersections, where the failure of immersion is ‘minimal’ (see below for details). We say that the bordism current 𝒞\mathcal{C} consists purely of ‘automatically transverse curves’.

  • •

    (Automatic transversality, weak version) We can allow certain holomorphic curves u:Σ→Xu:\Sigma\to X arising in (n−1)(n-1)-virtual dimensional moduli spaces, which are not automatically transverse, subject to the following requirements on these extra bad curves:

    1. 1.

      When virtual perturbation theory is taken into account, ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} still holds.

    2. 2.

      At any such bad curve u:Σ→Xu:\Sigma\to X, given any n−1n-1 first order deformation vector fields, the 1-form Ω⁡(⋅,v1,…​vn)\Omega(\cdot,v_{1},\ldots v_{n}) restricted to Σ\Sigma vanishes identically. Intuitively, this means Ω\Omega vanishes identically on the Zariski tangent space of the universal family at u:Σ→Xu:\Sigma\to X. As a caveat, these Zariski tangent spaces may be higher dimensional.

    3. 3.

      The boundary evaluation u:∂Σ→L∪L′u:\partial\Sigma\to L\cup L^{\prime} for all such bad holomorphic curves is contained in some subset of L∪L′L\cup L^{\prime} of Hausdorff dimension ≤n−1\leq n-1. As such, at almost every point on L∪L′L\cup L^{\prime}, only automatically transverse curves pass through it.

    4. 4.

      The Solomon functional can be computed by integrating only on the part of 𝒞\mathcal{C} consisting of automatically transverse curves.

The automatic transversality assumption should be viewed as a higher dimensional generalization of the fact that on Riemann surfaces, the nontrivial holomorphic polygons are immersions up to the boundary (cf. [69, Section 13 (b)]. The intuition for the weak version is that we sometimes need extra holomorphic curves to maintain ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime}, but for questions related to the Solomon functional and the boundary evaluation to the Lagrangians, these extra curves do not contribute.

Index theory preliminary

For a pseudoholomorphic polygon u:Σ→Xu:\Sigma\to X with inputs at p1,…​pkp_{1},\ldots p_{k} and an output at qq, arranged in clockwise order, the index is deg⁡q−∑1kdeg⁡pk\deg q-\sum_{1}^{k}\deg p_{k}, where the degree convention is (63). The index amounts to a Maslov number computation, and an alternative topological description is as follows: take a section ss of the complex line bundle Λn​T​M→Σ\Lambda^{n}TM\to\Sigma, which restricts on ∂Σ\partial\Sigma to a section of the real line bundle Λn​T​L\Lambda^{n}TL. (When several Lagrangians are involved, it is understood that T​LTL refers to the appropriate Lagrangian on the portion of ∂Σ\partial\Sigma.) We assume ss has isolated zeros up to the boundary and the corner (aka. strip like ends). We may also regard ss as a function Ω⁡(s)\Omega(s) on the polygon, by contraction with Ω\Omega. Then

Index=2​∑(interior zeros)+∑(boundary zeros)+∑(excess corner zeros)+n.\text{Index}=2\sum(\text{interior zeros})+\sum(\text{boundary zeros})+\sum(\text{excess corner zeros})+n. (23)

Here the order of zeros is computed from winding numbers, and for general sections ss may take positive and negative values. At a corner where ∂Σ\partial\Sigma passes from L+L_{+} to L−L_{-} in the clockwise direction, we can put the tangent spaces T​L±⊂T​XTL_{\pm}\subset TX into the standard form respecting the complex structure

L+=ℝn,L−=(ei​ϕ1,…​ei​ϕn)​ℝn,0<ϕi<π,T​X=ℝn⊗ℂ,L_{+}=\mathbb{R}^{n},\quad L_{-}=(e^{i\phi_{1}},\ldots e^{i\phi_{n}})\mathbb{R}^{n},\quad 0<\phi_{i}<\pi,\quad TX=\mathbb{R}^{n}\otimes\mathbb{C}, (24)

so if Ω⁡(s)∼zα\Omega(s)\sim z^{\alpha} in the complex coordinate of the upper half plane model, the excess vanishing order at the corner is 1π​(α−∑1nϕi)\frac{1}{\pi}(\alpha-\sum_{1}^{n}\phi_{i}). Formula (23) is equivalent to the standard index formula by a topological version of the Cauchy residue formula.

3.3.1 Automatically transverse cases

Holomorphic strip

We first consider the holomorphic strip case with input pp and output qq, and the integrability of the complex structure will be important. The first order deformations of the holomorphic strips Σ\Sigma are given by holomorphic sections of T​X|ΣTX|_{\Sigma}, which takes boundary value in T​LTL over ∂Σ\partial\Sigma, and decays at the corners.

Lemma 3.5.

If v1,…​vnv_{1},\ldots v_{n} are first order deformation vector fields, then either Ω⁡(v1,…​vn)=0\Omega(v_{1},\ldots v_{n})=0 everywhere on Σ\Sigma, or we must have deg⁡q−deg⁡p≥n\deg q-\deg p\geq n, and when the equality holds then Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}) only vanishes at the ends with excess vanishing order zero.

Proof.

We have a section of Λn​T​X|Σ\Lambda^{n}TX|_{\Sigma} given by v1∧…​vnv_{1}\wedge\ldots v_{n}, which takes boundary value in Λn​T​L\Lambda^{n}TL on ∂Σ\partial\Sigma. Since v1,…​vnv_{1},\ldots v_{n} are all holomorphic, so must be the function Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}). Assume this function is not identically zero. By holomorphicity, the zeros are isolated. We claim that the order of zeros must be nonnegative everywhere. This is clear for the interior and the boundary points. We analyze the ends of the strip as the origin in the upper half plane model with holomorphic coordinate zz, putting T​L±TL_{\pm} in the standard form at the corner point. The deformation vector field has the leading asymptote

vk=(ak​1zϕ1/π,…,ak​nzϕn/π)+O(z),k=1,2,…n,v_{k}=(a_{k1}z^{\phi_{1}/\pi},\ldots,a_{kn}z^{\phi_{n}/\pi})+O(z),\quad k=1,2,\ldots n,

hence

Ω⁡(v1,…​vn)=z(∑ϕk)/π​(det(ak​j)+o⁡(1)),\Omega(v_{1},\ldots v_{n})=z^{(\sum\phi_{k})/\pi}(\det(a_{kj})+o(1)),

and the excess vanishing order is nonnegative. By the index formula (23), the index deg⁡q−deg⁡p≥n\deg q-\deg p\geq n, and when equality is achieved all vanishing orders must be zero. In particular det(ak​j)≠0\det(a_{kj})\neq 0 at the corners. ∎

Corollary 3.6.

(Automatic transversality, strip case) Suppose deg⁡q−deg⁡p=n\deg q-\deg p=n. If v1,…​vnv_{1},\ldots v_{n} are ℝ\mathbb{R}-linearly independent at some point on ∂Σ\partial\Sigma away from the two corners, then v1,…​vnv_{1},\ldots v_{n} span the space of all first order deformations, the obstruction space vanishes, and the moduli space is smooth at u:Σ→Xu:\Sigma\to X. Morever, the holomorphic strip is an immersion up to the boundary.

Proof.

Since v1,…​vnv_{1},\ldots v_{n} are ℝ\mathbb{R}-linearly independent at a point on ∂Σ\partial\Sigma, they span T​LTL at the point, so Ω⁡(v1,…​vn)≠0\Omega(v_{1},\ldots v_{n})\neq 0. By the Lemma above v1,…​vnv_{1},\ldots v_{n} are pointwise complex linearly independent as sections of the holomorphic vector bundle T​XTX over Σ\Sigma, so any holomorphic first order deformation can be written as

v=f1​v1+…​fn​vn.v=f_{1}v_{1}+\ldots f_{n}v_{n}.

The functions f1,…​fnf_{1},\ldots f_{n} are holomorphic on Σ\Sigma up to boundary, and even up to corners due to det(ak​j)≠0\det(a_{kj})\neq 0. Now subtracting a constant linear combination of v1,…​vnv_{1},\ldots v_{n}, we can ensure vv vanishes at any chosen point on ∂Σ\partial\Sigma. Then Ω⁡(v,v2,…​vn)\Omega(v,v_{2},\ldots v_{n}) has a zero, so must be identically zero by the above Lemma, whence f1=0f_{1}=0 identically. Similar all fk=0f_{k}=0, so v=0v=0. This proves that v1,…​vnv_{1},\ldots v_{n} span all first order deformations. Since the index is nn, and the first order deformation space is nn-dimensional, we must have vanishing obstruction space.

There is a special deformation vector field from ℝ\mathbb{R} translation. The nonvanishing result then implies that the holomorphic strip is an immersion up to boundary. At the corners, the holomorphic strip is to leading order

(a1​zϕ1/π+O⁡(z),…​an​zϕn/π+O⁡(z)),ak≠0,∀k,|z|≪1.(a_{1}z^{\phi_{1}/\pi}+O(z),\ldots a_{n}z^{\phi_{n}/\pi}+O(z)),\quad a_{k}\neq 0,\forall k,\quad|z|\ll 1.

By det(ak​j)≠0\det(a_{kj})\neq 0, this translation vector field cannot be O⁡(z)O(z) at the corner, so for at least one choice of kk, we have ak≠0a_{k}\neq 0. We say the failure of immersion at the corner is ‘minimal’. ∎

Holomorphic polygon

We now move on to holomorphic polygons with k+1k+1 corner points for k≥2k\geq 2. The extended linearized Cauchy-Riemann equation (cf. [69, Chapter 9]) involves a vector field v∈C∞​(Σ,u∗​T​X)v\in C^{\infty}(\Sigma,u^{*}TX) decaying at the ends, and ρ∈Ω0,1​(Σ,T​Σ)\rho\in\Omega^{0,1}(\Sigma,T\Sigma) representing a tangent vector of the Stasheff associahedron (i.e. the deformation of Riemann surface structure on the domain Σ\Sigma), satisfying

∂¯​v+12​JX∘d​u∘ρ=0.\bar{\partial}v+\frac{1}{2}J_{X}\circ du\circ\rho=0.

where JXJ_{X} is the complex structure on XX. Here ρ\rho can be taken to be compactly supported, so ∂¯​v=0\bar{\partial}v=0 near the corners. It immediately follows that

Lemma 3.7.

Given first order deformation vector fields v1,…​vn−1v_{1},\ldots v_{n-1}, then the (1,0)-form Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) on Σ\Sigma is holomorphic.

Remark 3.6.

Adding vector fields on Σ\Sigma valued in T​ΣT\Sigma to v1,…​vn−1v_{1},\ldots v_{n-1} does not affect Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) as a 1-form on Σ\Sigma. Thus this 1-form is insensitive to how one represents the Riemann surface structures on the abstract polygon.

We impose that the input at one of the kk corners maps to an intersection point in C​F0​(L,L′)CF^{0}(L,L^{\prime}), and the other inputs map to degree one self intersections of LL or L′L^{\prime}. The output maps to q∈C​F∗​(L,L′)q\in CF^{*}(L,L^{\prime}).

Proposition 3.8.

(Automatic transversality, polygon case) Suppose v1,…​vn−1v_{1},\ldots v_{n-1} are linearly independent first order deformation vector fields. Either Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) vanishes identically as a 1-form on Σ\Sigma, or we must have deg⁡q≥n\deg q\geq n, and when the equality holds then Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) only vanishes at corners. In this case, all first order defomation vector fields are spanned by v1,…​vn−1v_{1},\ldots v_{n-1}, the holomorphic polygon u:Σ→Xu:\Sigma\to X is an immersion up to the boundary, the obstruction of the extended linearized operator vanishes, and the moduli space is smooth at u:Σ→Xu:\Sigma\to X.

Proof.

By viewing the domain of the polygon as a strip with extra boundary punctures, we produce a holomorphic vector field vnv_{n} as the ℝ\mathbb{R}-translation vector field. However, unlike in the strip case, at the degree one self intersection corners vnv_{n} does not typically have the required decay to be admitted as a deformation vector field. Indeed, by thinking about such a corner point as the origin in the upper half plane model of Σ\Sigma with local coordinate zz, then z​vnzv_{n} decays at the corner, but not necessarily vnv_{n} itself.

Now v1∧…​vnv_{1}\wedge\ldots v_{n} is a section of Λn​T​X\Lambda^{n}TX with boundary value on Λn​T​L\Lambda^{n}TL, and Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}) is a holomorphic function on Σ\Sigma. We assume from now on that it is not identically zero. The index of the ordinary Cauchy-Riemann operator is

deg⁡q−∑1kdeg⁡pk=deg⁡q−k+1.\deg q-\sum_{1}^{k}\deg p_{k}=\deg q-k+1.

Invoking (23) this is computable from the vanishing orders of Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}):

deg⁡q−k+1=2​∑(interior zeros)+∑(boundary zeros)+∑(corner zeros)+n.\deg q-k+1=2\sum(\text{interior zeros})+\sum(\text{boundary zeros})+\sum(\text{corner zeros})+n.

The interior and boundary vanishing orders are non-negative. Since the vkv_{k} are holomorphic near the corners without correction, the proof of Lemma 3.5 shows that the excess vanishing order at the C​F0​(L,L′)CF^{0}(L,L^{\prime}) corner and the qq corner are both non-negative. At the degree one self intersection corners, the excess vanishing order of Ω⁡(v1,…​vn−1,z​vn)\Omega(v_{1},\ldots v_{n-1},zv_{n}) is nonnegative by the same previous arguments, so Ω⁡(v1,…​vn−1,vn)\Omega(v_{1},\ldots v_{n-1},v_{n}) itself has excess vanishing order ≥−1\geq-1. Hence deg⁡q−k+1≥n−k+1,\deg q-k+1\geq n-k+1, namely deg⁡q≥n\deg q\geq n.

When the equality is achieved, then all bounds are saturated. In particular, Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}) can only vanish at the corners, so u:Σ→Xu:\Sigma\to X is an immersion up to boundary. At the corners, the same arguments in Corollary 3.6 shows the failure of immersion is minimal.

If vv is the deformation vector field corresponding to an arbitrary kernel element of the extended linearized operator, then after subtracting off a constant linear combination of v1,…​vn−1v_{1},\ldots v_{n-1}, we may assume vv is tangent to Σ\Sigma at any chosen point on ∂Σ\partial\Sigma. The same argument in Corollary 3.6 shows vv is tangent to the image of Σ\Sigma. The immersion property allows us to lift vv to the domain Σ\Sigma. There is no room to deform the complex structure of Σ\Sigma, nor is there any automorphism of Σ\Sigma, so in fact vv vanishes identically. This shows that v1,…​vn−1v_{1},\ldots v_{n-1} span all first order deformations. But deg⁡q=n\deg q=n implies that the index of the extended linearized operator is

deg⁡q−∑1kpk+k−2=n−1\deg q-\sum_{1}^{k}p_{k}+k-2=n-1

Thus the cokernel dimension is zero, namely the obstruction space vanishes. Consequently, the moduli space of such holomorphic polygons is smooth. ∎

Remark 3.7.

Using the Floer degree formula (63), the asymptotic behaviour of Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}) at the corners can be extracted from the above proof: at the C​F0​(L,L′)CF^{0}(L,L^{\prime}) corner point pp

Ω⁡(v1,…​vn)=ap​z(θL′−θL)​(p)/π​(1+O⁡(z)),ap≠0,arg⁡ap=θL​(p)modπ​ℤ.\Omega(v_{1},\ldots v_{n})=a_{p}z^{(\theta_{L^{\prime}}-\theta_{L})(p)/\pi}(1+O(z)),\quad a_{p}\neq 0,\quad\arg a_{p}=\theta_{L}(p)\mod\pi\mathbb{Z}.

At the degree one self intersections pl∈C​F1​(L+,L−)p_{l}\in CF^{1}(L_{+},L_{-}) on LL or L′L^{\prime},

Ω⁡(v1,…​vn)=al​z(θL−−θL+)​(pl)/π​(1+O⁡(z)),al≠0,arg⁡al=θL+​(pl)modπ​ℤ.\Omega(v_{1},\ldots v_{n})=a_{l}z^{(\theta_{L_{-}}-\theta_{L_{+}})(p_{l})/\pi}(1+O(z)),\quad a_{l}\neq 0,\quad\arg a_{l}=\theta_{L_{+}}(p_{l})\mod\pi\mathbb{Z}.

At the degree nn output qq,

Ω⁡(v1,…​vn)=aq​z(θL−θL′)​(q)/π​(1+O⁡(z)),aq≠0,arg⁡aq=θL′​(q)modπ​ℤ.\Omega(v_{1},\ldots v_{n})=a_{q}z^{(\theta_{L}-\theta_{L^{\prime}})(q)/\pi}(1+O(z)),\quad a_{q}\neq 0,\quad\arg a_{q}=\theta_{L^{\prime}}(q)\mod\pi\mathbb{Z}.

Weighted Sobolev space with exponential growth

We now discuss solutions to linearized Cauchy-Riemann equations in weighted Sobolev spaces W1,2;μW^{1,2;\mu} (cf. [70, section 2]). These spaces agree with their unweighted counterparts along the strip like input ends, but at the strip like output end s≫0s\gg 0, a vector field v∈Wl,2;μv\in W^{l,2;\mu} means that exp⁡(−μ​s)​v\exp(-\mu s)v lies in Wl,2W^{l,2}. Generally we choose μ\mu to avoid a discrete set of indicial values. The main point of these weighted Sobolev spaces is that they allow for holomorphic vector fields with prescribed exponential growth along the output end, which is conceptually similar to allowing for meromorphic functions in Riemann surface theory. If we think of the strip like end qq as the infinity (resp. the origin) in the upper half plane model of Σ\Sigma, then the natural coodinate is z=eπ⁡(s+i​t)z=e^{\pi(s+it)} (resp. z=e−π⁡(s+i​t)z=e^{-\pi(s+it)}), and the exponential growth o⁡(eμ​s)o(e^{\mu s}) becomes o⁡(|z|μ/π)o(|z|^{\mu/\pi}) (resp. o(|z|−μ/π)o(|z|^{-\mu/\pi}).

For larger μ\mu more vector fields are included in the Sobolev space, and the index increases by one each time μ\mu crosses an indicial value (counted with multiplicity). In our problem, the indicial values are

ϕ1+π​ℤ,ϕ2+π​ℤ,…,ϕn+π​ℤ,\phi_{1}+\pi\mathbb{Z},\quad\phi_{2}+\pi\mathbb{Z},\ldots,\phi_{n}+\pi\mathbb{Z},

where ϕ1,…​ϕn\phi_{1},\ldots\phi_{n} are the characterizing angles at the Lagrangian intersection point qq at the output end. Then the index for the linearized Cauchy-Riemann operator W1,2;μ→L2,μW^{1,2;\mu}\to L^{2,\mu} is

deg⁡q−∑1kdeg⁡pi+number of indicial values between 0 and μ,\deg q-\sum_{1}^{k}\deg p_{i}+\text{number of indicial values between $0$ and $\mu$}, (25)

where kk is the number of input ends. In particular, for holomorphic strips with deg⁡p=deg⁡q\deg p=\deg q (resp. deg⁡q−deg⁡p=1\deg q-\deg p=1), then the index for μ=π\mu=\pi is equal to nn (resp. n+1n+1). In contrast, the ordinary index (for the μ=0\mu=0 case) is zero, and the moduli space obtained by taking ℝ\mathbb{R}-quotient has virtual dimension −1-1 (resp. zero). There are in fact sufficient conditions to rule out the negative dimension moduli spaces, and constrain the zero dimensional moduli spaces:

Lemma 3.9.

In the holomorphic strip case, assume v1,…​vnv_{1},\ldots v_{n} are in the kernel of the linearized Cauchy-Riemann operator on W1,2;μ=πW^{1,2;\mu=\pi}, such that Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}) does not vanish identically. Then deg⁡q−deg⁡p≥1\deg q-\deg p\geq 1. When the equality is achieved, the holomorphic strip is an immersion up to the boundary with minimal vanishing at the corner, and the zero dimensional moduli space is regular.

Proof.

We modify the proof of Lemma 3.5 and Cor. 3.6. We think of the corner qq as the origin in the upper half plane model. Without loss of generality vnv_{n} is the ℝ\mathbb{R}-translation vector field of the holomorphic strip. Then the leading order asymptotic is

vk=(ak​1zϕ1/π−1,…,ak​nzϕn/π−1)+O(1),k=1,2,…n−1,v_{k}=(a_{k1}z^{\phi_{1}/\pi-1},\ldots,a_{kn}z^{\phi_{n}/\pi-1})+O(1),\quad k=1,2,\ldots n-1,

and

vn=(an​1​zϕ1/π,…,an​n​zϕn/π)+O⁡(z).v_{n}=(a_{n1}z^{\phi_{1}/\pi},\ldots,a_{nn}z^{\phi_{n}/\pi})+O(z).

hence

Ω⁡(v1,…​vn)=z(∑ϕk)/π−n+1​(det(ak​j)+o⁡(1)),\Omega(v_{1},\ldots v_{n})=z^{(\sum\phi_{k})/\pi-n+1}(\det(a_{kj})+o(1)),

The excess vanishing order is ≥1−n\geq 1-n, where negative order stands for poles. By the index formula (23) for the ordinary linearized Cauchy-Riemann equation, we have

deg⁡q−deg⁡p≥1−n+n=1,\deg q-\deg p\geq 1-n+n=1,

and equality forces Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}) to have no interior zero, no boundary zero, minimal zero at pp, and det(ak​j)≠0\det(a_{kj})\neq 0 at qq. The argument in Cor. 3.6 shows v1,…​vn,vnzv_{1},\ldots v_{n},\frac{v_{n}}{z} span the real vector space of first order deformations in W1,2;πW^{1,2;\pi}. In particular, the only first order deformation which decays at qq is the ℝ\mathbb{R}-translation vector field. Thus the cokernel to the ordinary linearized Cauchy-Riemann operator vanishes, and the moduli space is regular. ∎

A very analogous statement holds in the polygon case, and is left to the reader:

Lemma 3.10.

In the holomorphic polygon case, assume v1,…​vn−1v_{1},\ldots v_{n-1} are in the kernel of the extended linearized Cauchy-Riemann operator on W1,2;μ=πW^{1,2;\mu=\pi}, such that Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) does not vanish identically as a 1-form on Σ\Sigma. Then deg⁡q−∑1kdeg⁡pk+k−2≥0\deg q-\sum_{1}^{k}\deg p_{k}+k-2\geq 0. When the equality is achieved, the holomorphic polygon is an immersion up to the boundary with minimal vanishing at the corner, and the zero dimensional moduli space of holomorphic polygons is regular at u:Σ→Xu:\Sigma\to X.

A similar statement applies to teardrop curves:

Lemma 3.11.

(Regularity of teardrops) Let u:Σ→Xu:\Sigma\to X be a teardrop curve with a unique output qq and no input ends. Assume v1,…​vn−1v_{1},\ldots v_{n-1} are in the kernel of the linearized Cauchy-Riemann operator on W1,2;μ=πW^{1,2;\mu=\pi}, such that Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) does not vanish identically as a 1-form on Σ\Sigma. Then deg⁡q≥2\deg q\geq 2. When the equality is achieved, the teardrop curve is an immersion up to the boundary with minimal vanishing at the corner, and the kernel of the ordinary Cauchy-Riemann operator is spanned as a real vector space by the Möbius vector fields on Σ\Sigma fixing the qq corner, and the cokernel vanishes.

Proof.

We modify the proof of Lemma 3.9. We think of the corner qq as the origin in the upper half plane model, and take vnv_{n} instead to be the Möbius vector field z2∂zz^{2}\partial_{z} on Σ\Sigma. This has one higher order of vanishing:

vn=(an​1​zϕ1/π+1,…​an​n​zϕn/π+1)+O⁡(z2).v_{n}=(a_{n1}z^{\phi_{1}/\pi+1},\ldots a_{nn}z^{\phi_{n}/\pi+1})+O(z^{2}).

This leads to

Ω⁡(v1,…​vn)=z(∑ϕk)/π−n+2​(det(ak​j)+o⁡(1)),\Omega(v_{1},\ldots v_{n})=z^{(\sum\phi_{k})/\pi-n+2}(\det(a_{kj})+o(1)),

so the excess vanishing order at qq is ≥2−n\geq 2-n. The index of the ordinary linearized Cauchy-Riemann operator is

deg⁡q=2​∑(interior zeros)+∑(boundary zeros)+∑(excess corner zeros)+n,\deg q=2\sum(\text{interior zeros})+\sum(\text{boundary zeros})+\sum(\text{excess corner zeros})+n,

whence deg⁡q≥2\deg q\geq 2.

When the equality is achieved, then there is no interior or boundary zero, and det(ak​j)≠0\det(a_{kj})\neq 0 at the corner, hence the immersion claim. The argument in Cor. 3.6 shows that v1,…​vn,vnz,vnz2v_{1},\ldots v_{n},\frac{v_{n}}{z},\frac{v_{n}}{z^{2}} span the real vector space of first order deformations in W1,2;πW^{1,2;\pi}. In particular, the only first order deformation which decays at qq are spanned by vnv_{n} and z−1​vnz^{-1}v_{n}, namely the Möbius generators. Since the index of the ordinary Cauchy-Riemann operator is two, the cokernel must have dimension zero, namely the obstruction vanishes. ∎

The above lemma describes the optimal case for teardrop curves. Such deg⁡q=2\deg q=2 teardrop curves arise in isolated zero dimensional moduli spaces after taking the A​u​t​(D2,q)Aut(D^{2},q) quotient, and the counting contribution to m0m_{0} are ±1\pm 1 depending on the spin structure and the orientation issues.

Structure of linearized Cauchy-Riemann equation

Let Σ\Sigma be a holomorphic polygon with k≥0k\geq 0 input ends pip_{i}, and one output end at qq. The case k=0k=0 corresponds to teardrops, and k=1k=1 corresponds to strips. We consider the ordinary linearized Cauchy-Riemann operator in weighted Sobolev spaces W1,2;μW^{1,2;\mu}, to classify the structure of the first order deformation theory. As usual, the complex structure is integrable. Since ∂¯\bar{\partial} is elliptic, its cokernel in L2L^{2} is finite dimensional, represented by holomorphic 1-forms on Σ\Sigma, which must have finite order of vanishing at qq. For large enough μ\mu, the dual space L2;−μL^{2;-\mu} for L2;μL^{2;\mu} imposes an exponential decay condition O⁡(e−μ​s)O(e^{-\mu s}) at qq, so the cokernel evantually vanishes for μ≫1\mu\gg 1. Then the kernel dimension in W1,2;μW^{1,2;\mu} is equal to the index, computed by (25). For convenience, we use μ∈π​ℕ\mu\in\pi\mathbb{N}, which avoids the indicial values. Then

dim(ker⁡∂¯⊂W1,2;μ)=deg⁡q−∑1kdeg⁡pi+n​μπ.\dim(\ker\bar{\partial}\subset W^{1,2;\mu})=\deg q-\sum_{1}^{k}\deg p_{i}+\frac{n\mu}{\pi}. (26)

It is convenient to view the domain Σ\Sigma of the holomorphic polygon as the upper half plane with coordinate zz, with corners pip_{i} on the real line and qq at infinity.

Lemma 3.12.

If v∈ker⁡∂¯⊂W1,2;μv\in\ker\bar{\partial}\subset W^{1,2;\mu}, then v=f​wv=fw for some real coefficient polynomial function ff on the upper half plane, such that ww is nonvanishing on ℝ∖{p1,…​pk}\mathbb{R}\setminus\{p_{1},\ldots p_{k}\}, and vanishes minimally at pip_{i} (meaning ww is indivisible by z−piz-p_{i}).

Proof.

If vv vanishes at any boundary point aa on ℝ∖{p1,…​pk}\mathbb{R}\setminus\{p_{1},\ldots p_{k}\}, or if vv vanishes at pip_{i} beyond minimal order, then vz−a\frac{v}{z-a} (resp. vz−pi\frac{v}{z-p_{i}}) is also a first order deformation with the same T​LTL boundary condition, subject to the growth constraints at infinity. Since the kernel dimension is finite, the divisions can only happen a finite number of times, producing the polynomial ff. ∎

Let p∈∂Σ≃∂ℍp\in\partial\Sigma\simeq\partial\mathbb{H}, and let KK be the maximal number depending on pp, such that there exist ℝ\mathbb{R}-linearly independent v1,…​vK∈ker⁡∂¯v_{1},\ldots v_{K}\in\ker\bar{\partial}, satisfying

  • •

    In case pp is not a corner point, then v1​(p),…,vK​(p)v_{1}(p),\ldots,v_{K}(p) are ℝ\mathbb{R}-linearly independent vectors,

  • •

    In case p=pip=p_{i} is a corner point, then the nonzero elements in the ℝ\mathbb{R}-span of v1,…​vKv_{1},\ldots v_{K} are vector fields vanishing minimally at pp.

Lemma 3.13.

Any v∈ker⁡∂¯⊂W1,2;μv\in\ker\bar{\partial}\subset W^{1,2;\mu} is of the form g1​v1+…​gK​vKg_{1}v_{1}+\ldots g_{K}v_{K} for some real coefficient rational functions g1,…​gKg_{1},\ldots g_{K}, nonsingular at pp.

Proof.

Without loss of generality p=0p=0. Let w0w_{0} be any first order deformation. By the maximality of KK, we can choose real numbers aia_{i}, such that the first order deformation w0−∑1Kai​viw_{0}-\sum_{1}^{K}a_{i}v_{i} vanishes at zero, so w0−∑1Kai​1​vi=zk1​w1w_{0}-\sum_{1}^{K}a_{i1}v_{i}=z^{k_{1}}w_{1} for some first order deformation w1w_{1} which is nonzero at the origin. Finite dimensionality means this process can be repeated for only a finite number of times:

{w0=∑ai​1​vi+zk1​w1,w1=∑ai​2​vi+zk2​w2,…wN−1=∑ai​N​vi+zkN​wN.\begin{cases}w_{0}=\sum a_{i1}v_{i}+z^{k_{1}}w_{1},\\ w_{1}=\sum a_{i2}v_{i}+z^{k_{2}}w_{2},\\ \ldots\\ w_{N-1}=\sum a_{iN}v_{i}+z^{k_{N}}w_{N}.\end{cases}

We choose the smallest NN such that v1,…​vK,w0,…​wNv_{1},\ldots v_{K},w_{0},\ldots w_{N} are ℝ\mathbb{R}-linearly dependent as vector fields; notice v1,…​vKv_{1},\ldots v_{K} are linearly independent, so N≥0N\geq 0. We then get a linear relation

f0​(z)​wN=∑1Kfi​(z)​vi,f_{0}(z)w_{N}=\sum_{1}^{K}f_{i}(z)v_{i},

where f0,…​fKf_{0},\ldots f_{K} are polynomials, and f0​(0)≠0f_{0}(0)\neq 0. This implies the claim. ∎

We can also apply a Möbius transform to make the output end qq lie at the origin. The growth condition translates to o(|z|−μ/π)o(|z|^{-\mu/\pi}) at zero. Let KK be maximal, such that there are ℝ\mathbb{R}-linearly independent vector fields z−μ/πv1,…,z−μ/πvK∈ker∂¯⊂W1,2;μz^{-\mu/\pi}v_{1},\ldots,z^{-\mu/\pi}v_{K}\in\ker\bar{\partial}\subset W^{1,2;\mu}, and any nonzero element in the ℝ\mathbb{R}-span of v1,…​vKv_{1},\ldots v_{K} vanishes mimimally at q=0q=0. As a caveat, this does not assume v1,…​vKv_{1},\ldots v_{K} satisfy the growth constraints at infinity to lie in ker⁡∂¯⊂W1,2;μ\ker\bar{\partial}\subset W^{1,2;\mu}. Minor adaptions give

Lemma 3.14.

Any v∈ker⁡∂¯⊂W1,2;μv\in\ker\bar{\partial}\subset W^{1,2;\mu} is of the form z−μ/π(g1v1+…gKvK)z^{-\mu/\pi}(g_{1}v_{1}+\ldots g_{K}v_{K}) for some real coefficient rational functions g1,…​gKg_{1},\ldots g_{K}, nonsingular at qq.

Corollary 3.15.

The number KK is independent of the boundary and corner points on ∂Σ\partial\Sigma.

We view the boundary ∂Σ≃ℙ1​(ℝ)\partial\Sigma\simeq\mathbb{P}^{1}(\mathbb{R}). By the above lemmas, there is a real algebraic vector bundle ℰ\mathcal{E} of rank KK over ℙ1​(ℝ)\mathbb{P}^{1}(\mathbb{R}) such that v1,…​vKv_{1},\ldots v_{K} provide the basis of local sections. By Grothendieck’s classification of vector bundles,

Proposition 3.16.

ℰ≃⊕1K𝒪(ni)\mathcal{E}\simeq\oplus_{1}^{K}\mathcal{O}(n_{i}) for some ni∈ℤn_{i}\in\mathbb{Z}.

Since the rank KK is nondecreasing in μ\mu, it evantually stabilizes for μ≫0\mu\gg 0. Since around any given point, the same choice of v1,…​vKv_{1},\ldots v_{K} is valid for all large μ\mu, the algebraic vector bundle ℰ\mathcal{E} is independent of μ≫0\mu\gg 0. The elements of ker⁡∂¯⊂W1,2;μ\ker\bar{\partial}\subset W^{1,2;\mu} can be interpreted as global sections of ℰ⊗𝒪⁡(μπ)\mathcal{E}\otimes\mathcal{O}(\frac{\mu}{\pi}). Thus for all large μ\mu,

dim(ker⁡∂¯⊂W1,2;μ)=dimΓ⁡(ℙ1​(ℝ),ℰ⊗𝒪⁡(μπ))=K⁡(μπ+1)+∑1Kni.\dim(\ker\bar{\partial}\subset W^{1,2;\mu})=\dim\Gamma(\mathbb{P}^{1}(\mathbb{R}),\mathcal{E}\otimes\mathcal{O}(\frac{\mu}{\pi}))=K(\frac{\mu}{\pi}+1)+\sum_{1}^{K}n_{i}. (27)

Contrasting with the index formula (26),

Corollary 3.17.

The rank K=nK=n, and the degree ∑1nni=deg⁡q−∑1kdeg⁡pi−n\sum_{1}^{n}n_{i}=\deg q-\sum_{1}^{k}\deg p_{i}-n.

The structure of ℰ≃⊕1K𝒪(ni)\mathcal{E}\simeq\oplus_{1}^{K}\mathcal{O}(n_{i}) provides meromorphic sections v1,…​vnv_{1},\ldots v_{n} which are a basis of local sections on ℝ⊂ℙ1​(ℝ)\mathbb{R}\subset\mathbb{P}^{1}(\mathbb{R}), and have excess vanishing orders n1,…​nnn_{1},\ldots n_{n} at qq. Consider the function Ω⁡(v1,…​vn)\Omega(v_{1},\ldots v_{n}). By construction, it has no boundary zero, and its excess corner vanishing order is ∑1nni\sum_{1}^{n}n_{i}. Comparing with the index formula (23),

deg⁡q−∑1kpi=2​∑(interior zeros)+∑ni+n.\begin{split}\deg q-\sum_{1}^{k}p_{i}=2\sum(\text{interior zeros})+\sum n_{i}+n.\end{split}

Since all interior vanishing orders are nonnegative by holomorphicity,

Corollary 3.18.

We have Ω⁡(v1,…​vn)≠0\Omega(v_{1},\ldots v_{n})\neq 0 in the interior of Σ\Sigma.

The significance is that the algebraic vector bundle structure on ℰ→ℙ1​(ℝ)\mathcal{E}\to\mathbb{P}^{1}(\mathbb{R}) now extends over the entire Σ\Sigma. The v1,…​vnv_{1},\ldots v_{n} now provide the basis of local sections for the vector bundle u∗​T​X|Σu^{*}TX|_{\Sigma}. One upshot is that an algebraic structure arises on u∗​T​X→Σu^{*}TX\to\Sigma from solving the Cauchy-Riemann equation with Lagrangian boundary:

(u∗TX,u∗TL)≃(⊕1n𝒪(ni),natural real structure).(u^{*}TX,u^{*}TL)\simeq(\oplus_{1}^{n}\mathcal{O}(n_{i}),\text{natural real structure}). (28)

In contrast, the Lagrangians are only assumed to be smooth, not necessarily real analytic.

To analyze obstructions, Serre duality motivates us to consider the dualized cokernel to the ordinary (unweighted, unextended) linearized Cauchy-Riemann operator. A dualized cokernel element η\eta is represented by a holomorphic 1-forms in Ω1,0​(Σ,u∗​T∗​X)\Omega^{1,0}(\Sigma,u^{*}T^{*}X) with L2L^{2} integrablity, and its T∗​XT^{*}X factor lies in the annilator of the T​LTL boundary condition. Equivalently, for all test vector fields v∈W1,2​(Σ,T​X,T​L)v\in W^{1,2}(\Sigma,TX,TL),

∫Σ⟨∂¯​v∧η⟩=0,\int_{\Sigma}\langle\bar{\partial}v\wedge\eta\rangle=0,

where ⟨,⟩\langle,\rangle is the pairing of T​XTX with T∗​XT^{*}X, and the wedge takes care of the forms on Σ\Sigma. In the canonical form (28), this dualized cokernel is isomorphic to Γ(ℝℙ1,⊕1n𝒪(−2−ni)).\Gamma(\mathbb{RP}^{1},\oplus_{1}^{n}\mathcal{O}(-2-n_{i})). In particular,

Corollary 3.19.

In the teardrop curve case k=0k=0, the strip case k=1k=1 and the triangle case k=2k=2, the vanishing of cokernel is equivalent to ni≥−1n_{i}\geq-1 for all ii.

For k≥3k\geq 3 the deformation of the holomorphic polygons is governed instead by the extended Cauchy-Riemann equation, since the punctured Riemann surface structure on Σ\Sigma is allowed to vary. The dualized cokernel of the extended Cauchy-Riemann operator, is the subspace of the dualized cokernel of the ordinary Cauchy-Riemann operator, which pairs trivially with JX∘d​u∘ρJ_{X}\circ du\circ\rho for any ρ\rho representing some tangent vector of the Stasheff associahedron.

Hamiltonian deformations and transversality

We now consider the parametrized moduli space of holomorphic curves over the infinite dimensional space of Hamiltonian deformations for the Lagrangian LL. Infinitesimally around a holomorphic curve Σ\Sigma, we have a Hamiltonian vector field XHX_{H} defined by ω⁡(XH,⋅)=d​H\omega(X_{H},\cdot)=dH, viewed as a T​XTX-valued vector field over Σ\Sigma. We are interested in whether the Hamiltonian deformation kills the cokernel of the ordinary Cauchy-Riemann operator. This question was first addressed by Oh [64]. The following account follows a similar strategy but differs in details.

Recall the ordinary Cauchy-Riemann operator maps W1,2​(Σ,u∗​T​X,u∗​T​L)W^{1,2}(\Sigma,u^{*}TX,u^{*}TL) to L2​(Σ,u∗​T​X⊗T∗(1,0)​Σ)L^{2}(\Sigma,u^{*}TX\otimes T^{*(1,0)}\Sigma). The effect of Hamiltonian deformation is to enlarge the domain of the ∂¯\bar{\partial} operator, by including the vector fields XHX_{H} for all the allowed Hamiltonians HH. The question is to analyze the pairing of ∂¯​XH\bar{\partial}X_{H} with the dualized cokernel elements.

Proposition 3.20.

Let u:Σ→Xu:\Sigma\to X be a holomorphic disc which is immersed near some point z0∈∂Σz_{0}\in\partial\Sigma with the boundary injectivity property u|∂Σ−1​(u⁡(z0))={z0}u|_{\partial\Sigma}^{-1}(u(z_{0}))=\{z_{0}\}. Let η\eta be a nonzero dualized cokernel element for the ordinary linearized Cauchy-Riemann operator. Then there is a Hamiltonian HH supported in any prescribed small ball on XX containing u⁡(z0)u(z_{0}), such that ∫Σ⟨∂¯​XH∧η⟩≠0\int_{\Sigma}\langle\bar{\partial}X_{H}\wedge\eta\rangle\neq 0.

Proof.

Since η\eta is a holomorphic 1-form valued in u∗​T∗​Xu^{*}T^{*}X, Stokes theorem gives

∫Σ⟨∂¯​XH∧η⟩=∫∂Σ⟨XH,η⟩,\int_{\Sigma}\langle\bar{\partial}X_{H}\wedge\eta\rangle=\int_{\partial\Sigma}\langle X_{H},\eta\rangle,

where ⟨,⟩\langle,\rangle stands for the pairing between T​XTX and T∗​XT^{*}X. On ∂Σ\partial\Sigma, we can write η=ω⁡(⋅,Y)​d​s\eta=\omega(\cdot,Y)ds for some vector field YY valued in u∗​T​Xu^{*}TX, and ss is any local coordinate on ∂Σ\partial\Sigma. The cokernel element condition implies ω⁡(v,Y)=0\omega(v,Y)=0 for any v∈u∗​T​Lv\in u^{*}TL, so YY must in fact be valued in the Lagrangian subbundle u∗​T​Lu^{*}TL. Thus

∫∂Σ⟨XH,η⟩=∫∂Σω⁡(XH,Y)​𝑑s=∫∂Σd​H​(Y)​𝑑s.\int_{\partial\Sigma}\langle X_{H},\eta\rangle=\int_{\partial\Sigma}\omega(X_{H},Y)ds=\int_{\partial\Sigma}dH(Y)ds.

We suppose for contradiction, that this pairing vanishes identically for any HH supported in the prescribed ball.

By the holomorphicity of η\eta, its zeros are isolated, so without loss of generality YY does not vanish in the local portion of ∂Σ\partial\Sigma where uu is injective and immersed. Suppose first that YY is not tangent to the image of Σ\Sigma. Then we find some local function hh on a small ball in XX with d​h​(Y)=1dh(Y)=1 and h=0h=0 on the local portion of ∂Σ\partial\Sigma, and another cutoff function h2≥0h_{2}\geq 0 with d​h2​(Y)=0dh_{2}(Y)=0 along ∂Σ\partial\Sigma, supported in a small ball. Taking H=h​h2H=hh_{2}, then

∫∂Σd​H​(Y)​𝑑s=∫∂Σh2​𝑑s≠0.\int_{\partial\Sigma}dH(Y)ds=\int_{\partial\Sigma}h_{2}ds\neq 0.

This contradiction shows YY is tangent to the image of Σ\Sigma in the local portion of ∂Σ\partial\Sigma. We can write Y=f∂sY=f\partial_{s} for some local function ff. Then requiring

∫∂ΣdH(Y)ds=∫∂Σf∂sHds=−∫∂ΣH∂sfds\int_{\partial\Sigma}dH(Y)ds=\int_{\partial\Sigma}f\partial_{s}Hds=-\int_{\partial\Sigma}H\partial_{s}fds

for any compactly supported local function HH, implies that ff is constant in the local portion of ∂Σ\partial\Sigma. Thus up to multiplying by a nonzero constant, locally

Y=∂u∂s​d​s,η=ω⁡(⋅,∂u∂s)​d​s.Y=\frac{\partial u}{\partial s}ds,\quad\eta=\omega(\cdot,\frac{\partial u}{\partial s})ds. (29)

We now produce holomorphic vector fields on Σ\Sigma. For holomorphic strips or polygons with k+1≥3k+1\geq 3 corners, we select one input end as pp, and call the output qq as usual, and represent Σ\Sigma as a strip with k−1k-1 boundary punctures. This perspective provides a natural translation vector field ∂u∂s\frac{\partial u}{\partial s}, which have exponential decay along the p,qp,q ends, but may not be L2L^{2} near the other k−1k-1 ends. Instead, by thinking about the k−1k-1 ends as the origin in the upper half plane model, we see

∂u∂s=O⁡(|z|α−1),α=min⁡{ϕ1/π,…​ϕn/π}\frac{\partial u}{\partial s}=O(|z|^{\alpha-1}),\quad\alpha=\min\{\phi_{1}/\pi,\ldots\phi_{n}/\pi\}

for the characterizing angles ϕ1,…​ϕn\phi_{1},\ldots\phi_{n} at the Lagrangian intersection point. The T(1,0)​XT^{(1,0)}X part of 2​JX​∂u∂s2J_{X}\frac{\partial u}{\partial s} is JX​∂u∂s+−1​∂u∂sJ_{X}\frac{\partial u}{\partial s}+\sqrt{-1}\frac{\partial u}{\partial s}. Contracting this with the T∗(1,0)​X⊗T∗(1,0)​ΣT^{*(1,0)}X\otimes T^{*(1,0)}\Sigma part of η\eta yields a 1-form on Σ\Sigma

ζ=η⁡(JX​∂u∂s+−1​∂u∂s)\zeta=\eta(J_{X}\frac{\partial u}{\partial s}+\sqrt{-1}\frac{\partial u}{\partial s})

which is also holomorphic, with boundary value along Σ\Sigma

ζ=ω⁡(JX​∂u∂s+−1​∂u∂s,Y)​d​s=ω⁡(JX​∂u∂s,Y)​d​s.\zeta=\omega(J_{X}\frac{\partial u}{\partial s}+\sqrt{-1}\frac{\partial u}{\partial s},Y)ds=\omega(J_{X}\frac{\partial u}{\partial s},Y)ds. (30)

Here ω⁡(∂u∂s,Y)=0\omega(\frac{\partial u}{\partial s},Y)=0 since both vectors satisfy the T​LTL boundary condition. Notably, the boundary condition of ζ\zeta is real valued. In the upper half plane model, the Schwartz reflection principle allows us to extend ζ\zeta meromorphically over ℂ​ℙ1\mathbb{CP}^{1}.

At any of the k−1k-1 ends, since η∈L2\eta\in L^{2}, we know by holomorphicity |η|=O⁡(|z|α)|\eta|=O(|z|^{\alpha}), so ζ=O⁡(|z|2​α−1)\zeta=O(|z|^{2\alpha-1}) in the upper half plane model, hence has no pole. At the p,qp,q ends, by the decay of the holomorphic ∂u∂s\frac{\partial u}{\partial s} and η\eta, we likewise infer that ζ\zeta has no pole in the upper half plane model. In conclusion, the extension of ζ\zeta over ℂ​ℙ1\mathbb{CP}^{1} has no pole, so must in fact vanish. However, by (29)(30), on a local portion of ∂Σ\partial\Sigma

ζ=ω⁡(JX​∂u∂s,∂u∂s)​d​s≠0.\zeta=\omega(J_{X}\frac{\partial u}{\partial s},\frac{\partial u}{\partial s})ds\neq 0.

This contradiction proves the Proposition in the k≥1k\geq 1 case.

Finally, for the teardrop curve case k=0k=0, we replace the holomorphic vector field ∂u∂s\frac{\partial u}{\partial s} by the Möbius vector fields vanishing at the corner, and the rest of the arguments are entirely similar. ∎

The upshot is that by the Sard-Smale theorem, provided we can always ensure ‘somewhere boundary injectivity’ for any holomorphic disc in a given moduli space, then generic Hamiltonian perturbation would be able to achieve regularity for the moduli space.

Remark 3.8.

In the exact setting there is no closed holomorphic curve. The failure of ‘somewhere boundary injectivity’ is often associated with multiple cover issues, namely u:Σ→Xu:\Sigma\to X may decompose into several domain components, each of which factorizes through a somewhere boundary injective holomorphic disc (cf. [50] for the case of Lagrangian boundary with no corners).

In the simplest case, if uu factorizes through another disc, then the corner points would be repeated several times on ∂Σ\partial\Sigma. This phenomenon does not happen for the curves appearing in the bordism current 𝒞\mathcal{C}, which involve only one corner at C​F0​(L,L′)CF^{0}(L,L^{\prime}) and one corner at C​F0​(L′,L)CF^{0}(L^{\prime},L). Nor does this occur for teardrop curves, which have only one corner at a degree two self intersection point. This raises hope that the failure of ‘somewhere boundary injectivity’ may be highly nongeneric, or in certain situations can be ruled out altogether.

Further comments on automatic transversality

We now comment on the gap between what we proved and the (weak version of) automatic transversality that we will later assume.

  1. 1.

    Prop. 3.8, Lemma 3.5 and Cor. 3.6 establish the dichotomy for holomorphic discs u:Σ→Xu:\Sigma\to X arising in virtual dimension n−1n-1 moduli spaces, that either uu is automatically transverse, or Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) vanishes for any (n−1)(n-1) first order deformation vectors. This argument does not establish unperturbed regularity for the lower dimensional moduli spaces, so it is not completely clear if complex structure perturbations can be removed in the arguments for ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} in section 2.9.

  2. 2.

    For the bad curves, Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) vanishes identically as a 1-form on Σ\Sigma, so at any point on the boundary, v1,…​vn−1v_{1},\ldots v_{n-1} and the tangent vector to ∂Σ\partial\Sigma are ℝ\mathbb{R}-linearly dependent. Suppose for the moment that the moduli spaces are regular, then the boundary evaluation to L∪L′L\cup L^{\prime} for the bad curves arise in Hausdorff dimension at most n−1n-1. Morever, since the Solomon functional is defined through ∫𝒞λ∧Ω\int_{\mathcal{C}}\lambda\wedge\Omega, and Ω\Omega vanishes around the bad curves, smoothness assumptions imply that the bad curves cannot contribute.

    When regularity assumptions are dropped, one needs to appeal to virtual techniques, so these conclusions require further justification. One problem is that the standard virtual perturbation techniques based on Kuranishi structures do not necessarily produce virtual cycles inside the original moduli spaces, but only inside their small neighbourhoods. This perturbation step destroys the identical vanishing of Ω\Omega, by a small amount corresponding to the size of the perturbation. As one shrinks the size of the perturbations, one needs uniform mass bound on the virtual chains to justify that the integral contribution to ∫𝒞λ∧Ω\int_{\mathcal{C}}\lambda\wedge\Omega from the bad curves actually converges to zero.

  3. 3.

    Alternatively, one can hope to replace Lagrangians by arbitrarily small Hamiltonian perturbations to achieve transversality. This is mostly adequate for our purpose, except that one needs to justify the ‘somewhere boundary injectivity’ property (cf. Remark 3.8).

3.4 Positivity condition

The (n−1)(n-1)-dimensional moduli spaces contributing to the bordism current come with orientation signs and weighting factors. The positivity condition (i.e. no cancellation of signs) means that around any automatically transverse curves, if the first order deformations v1,…​vn−1v_{1},\ldots v_{n-1} form an oriented basis of the moduli space, and v0v_{0} be a clockwise ordered vector field on ∂Σ\partial\Sigma, then upon boundary evaluation v0∧…​vn−1v_{0}\wedge\ldots v_{n-1} agrees with the orientation of L−L′L-L^{\prime}. For the other holomorphic curves, the question of orientation does not arise, because the boundary evaluation maps have degenerate differentials everywhere on ∂Σ\partial\Sigma.

The positivity condition forbids two curves passing through a generic point with the evaluation maps contributing opposite signs. Such a requirement is geometric rather than homological, and if we go beyond the almost calibrated case, it also depends on the choice of the generators α∈C​F0​(L,L′)\alpha\in CF^{0}(L,L^{\prime}) and β∈C​F0​(L′,L)\beta\in CF^{0}(L^{\prime},L), rather than only their classes in H​F0HF^{0}.

Question 5.

Given two unobstructed Lagrangian objects L,L′L,L^{\prime} which are isomorphic in Db​F​u​k​(X)D^{b}Fuk(X). When can we make gauge choices for the local systems and the bounding cochain data, and choices of the Floer cohomology group generators, such that the bordism current 𝒞\mathcal{C} produced from the universal family of holomorphic curves satisfies the positivity condition?

The positivity condition will arise in the applications as follows. We will write various quantities as integrals over the (n−1)(n-1)-dimensional moduli spaces of holomorphic curves, and the positivity condition would in each case imply the pointwise positivity of the integrand. In the mirror analogy, this corresponds to the pointwise positivity of curvature integrands, which features for instance in the proof that the Hermitian Yang-Mills equation implies the semistability of bundles (cf. section 2.5).

Morse theory analogy

The intuition of the positivity condition can be explained through the following analogy with Morse theory. Given a compact oriented manifold MM with a Morse-Smale function HH, then

  • •

    The degree zero (resp. nn) elements in the Morse cochain complex are generated by the local maxima (resp. local minima) of HH whose unstable submanifolds (resp. stable submanifolds) have preferred orientations.

  • •

    The fundamental class 1∈H0​(M)1\in H^{0}(M) is represented by the sum of the local maxima with the preferred orientation. Similarly with the generator of Hn​(M)H^{n}(M).

  • •

    A generic point on MM lies on exactly one Morse flowlines which starts with one local maximum point and ends on one local minimum point. More formally, if we construct the universal family of Morse flowlines that start with some local maximum and ends on some local minimum, the evaluation map would sweep out the fundamental cycle of MM as an nn-dimensional current, without any cancellation effect.

Now for simplicity, if we start with an embedded Lagrangian brane LL, and preform a small generic Hamiltonian deformation ϕH​(L)\phi_{H}(L), then the Floer cohomology H​F∗​(L,ϕH​(L))HF^{*}(L,\phi_{H}(L)) is computed as the Morse cohomology, so the Morse theory statements above would imply the positivity condition at least in such special cases. The intuition is that if the Lagrangian L′L^{\prime} (together with its brane structure) is a sufficiently small deformation of LL, then we expect the positivity condition to hold for the bordism current between LL and L′L^{\prime}.

Positivity for individual moduli spaces

In general the bordism current 𝒞\mathcal{C} receives contributions from many (n−1)(n-1)-dimensional moduli spaces of holomorphic curves. We now focus on one moduli space by fixing the choice of the Lagrangian intersections p1,…​pk,qp_{1},\ldots p_{k},q and the homotopy type of u:Σ→Xu:\Sigma\to X, and consider a connected open subset of the moduli space which contains only automatically transverse curves. We observe:

  • •

    For a fixed automatically transverse holomorphic curve u:Σ→Xu:\Sigma\to X, along ∂Σ\partial\Sigma between any two successive corners, by the nowhere vanishing of Ω⁡(⋅,v1,…​vn)\Omega(\cdot,v_{1},\ldots v_{n}), the Jacobian of the boundary evaluation map cannot change sign. That is, either the orientation of the universal family agrees with the orientation of LL (resp. −L′-L^{\prime}) along u:∂Σ→Lu:\partial\Sigma\to L at every point along the boundary portion of ∂Σ\partial\Sigma, or the two orientations disagree at every point.

  • •

    The Lagrangians are graded by assumption, and the orientations are canonically determined by e−i​θ​Ωe^{-i\theta}\Omega. The corner behaviour (cf. Remark 3.7) implies that at the degree one self intersections, e−i​θ​Ω​(⋅,v1,…​vn−1)e^{-i\theta}\Omega(\cdot,v_{1},\ldots v_{n-1}) does not change sign. On the other hand, at the C​F0​(L,L′)CF^{0}(L,L^{\prime}) and the C​F0​(L′,L)CF^{0}(L^{\prime},L) ends along ∂Σ\partial\Sigma, the 1-form e−i​θ​Ω​(⋅,v1,…​vn−1)e^{-i\theta}\Omega(\cdot,v_{1},\ldots v_{n-1}) changes orientation sign. Thus at a fixed automatically transverse curve, the orienation of the universal family and L−L′L-L^{\prime} either completely agree along every point of ∂Σ\partial\Sigma, or completely disagree.

  • •

    As we deform among automatically transverse curves, the orientation signs cannot change. Thus either all these holomorphic curves contribute positively to ∂𝒞\partial\mathcal{C}, or they all contribute negatively.

The above discussion also suggests the limitation of the positivity condition: if we encounter a holomorphic curve in the moduli space, which is not automatically transverse, then it is possible to switch orientation signs. For arbitrary exact immersed Lagrangians, it seems unreasonable to expect the positivity condition, and it is conceivable that counterexamples may arise from hh-principle constructions. Whether counterexamples occur for more restrictive Lagrangians seems less clear, and we leave the following sample questions as food for thought:

Question 6.

How does the positivity condition behave under exact isotopy with surgery?

Question 7.

Are there examples of exact Calabi-Yau manifolds such that the positivity condition is satisfied for bordism currents between all exact, almost calibrated, unobstructed immersed Lagrangians equipped with suitable brane structures? What if the Lagrangians are quantitatively almost calibrated (cf. (3))?

Remark 3.9.

If the Fukaya category is defined over ℤ\mathbb{Z}, we can require all holonomy factors to be integer valued. The positivity condition requires all the contributions to ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} to have the same orientation sign. This has the amusing consequence that all holonomy factors associated with (n−1)(n-1)-dimensional moduli spaces contributing to 𝒞\mathcal{C}, must in fact all be +1+1. Intuitively, this means there is a unique such holomorphic curve through any generic point of LL, and the boundary evaluation of universal family to LL is transverse.

3.5 Floer theoretic obstructions

General features of obstruction conditions

Our goal is to look for obstructions to the existence of special Lagrangians within given Db​F​u​k​(X)D^{b}Fuk(X) classes, which is the ‘easy direction’ of the conjectural stability condition. Before specializing to a technically oversimplified setup, we first explain the features we expect from these obstructions, which may hold in much more general contexts. The mirror analogy (cf. our discussion on the μ\mu-stability in section 2.5) suggests:

  • •

    The obstructions are associated to certain positivity of signs, which essentially depend on the integrability of Kähler geometry.

  • •

    The quantity involved in the obstruction can be expressed as an integral over a moduli space of worldsheet instantons (i.e. holomorphic curves), and its sign comes from a pointwise positivity of the integrand on the moduli space.

  • •

    The input from Floer theory is associated to a distinguished triangle in Db​F​u​k​(X)D^{b}Fuk(X), or possible generalisations to several Lagrangians.

  • •

    The role of the holomorphic volume form enters via cohomological integrals.

  • •

    There is no need for the complex Monge-Ampère equation. Only the almost Calabi-Yau condition is needed.

Furthermore, out of the many moduli spaces that may arise in Floer theory, we will only make use of certain (n−1)(n-1)-dimensional moduli spaces of holomorphic curves, whose associated (n+1)(n+1)-dimensional universal family provides bordism currents between the nn-dimensional Lagrangians. Here are some a priori reasons why we restrict attention to these:

  • •

    The holomorphic volume form is naturally integrated over nn-cycles. This explains the dimension.

  • •

    We need bordism currents canonically associated to the distinguished triangles. In Floer theory, the A∞A_{\infty}-structure only becomes an invariant when considered as a whole, and individual A∞A_{\infty} products are not invariants, so invariance constrains how moduli spaces can enter into stability conditions. As mentioned in section 3.1, the existence of the bordism current is the geometric manifestation of linear relations in the zeroth Hochschild homology H​H0HH_{0} of the Fukaya category, which contains important invariant information.

  • •

    From a variational viewpoint which will be discussed more fully in Chapter 5, it is desirable to extend Floer theory to Lagrangians with much weaker regularity, in the varifold and current sense. We shall explain there that most of Floer cohomologies and A∞A_{\infty} products cannot be expected to pass to the limit when the Lagrangians degenerate in such weak topologies, and we hope that the bordism currents we use are among the few pieces of Floer theory that may be well behaved under rather severe degenerations of Lagrangians.

These requirements are very stringent. We notice two other features:

  • •

    We shall crucially rely on the almost calibrated condition.

  • •

    When we test the stability of LL via the distinguished triangle L1→L→L2→L1​[1]L_{1}\to L\to L_{2}\to L_{1}[1], we do not wish to assume L1L_{1} or L2L_{2} is special Lagrangian. In our view, stability conditions should be expressed in Floer theoretic terms, without a priori knowledge of what special Lagrangians there are inside a given almost Calabi-Yau manifold.

The Floer theoretic obstruction condition

The following Floer theoretic obstruction will crucially require complex integrability and the almost calibrated condition. Assume L1→L→L2→𝛾L1​[1]L_{1}\to L\to L_{2}\xrightarrow{\gamma}L_{1}[1] be a distinguished triangle of unobstructed exact immersed Lagrangian branes with bounding cochains, such that L1,L,L2L_{1},L,L_{2} are all almost calibrated, and all intersections are transverse. In other words, the Lagrangian brane LL is isomorphic in Db​F​u​k​(X)D^{b}Fuk(X) to the immersed Lagrangian corresponding to the twisted complex (cf. section 3.1, 6.2)

L′≃((L2,b2)γ(L1,b1)).L^{\prime}\simeq\left(\begin{matrix}(L_{2},b_{2})&\\ \gamma&(L_{1},b_{1})\end{matrix}\right).

We obtain a bordism current 𝒞\mathcal{C} with ∂𝒞=L−L′=L−L1−L2\partial\mathcal{C}=L-L^{\prime}=L-L_{1}-L_{2}. In our generality, the domains of L1,L2,LL_{1},L_{2},L may have many connected components.

Theorem 3.21.

(Floer theoretic obstruction) Assume the automatic transversality and the positivity condition hold for the bordism current 𝒞\mathcal{C}. Assume the destabilizing condition

θ^1=arg∫L1Ω>θ^2=arg∫L2Ω.\hat{\theta}_{1}=\arg\int_{L_{1}}\Omega>\hat{\theta}_{2}=\arg\int_{L_{2}}\Omega.

Then the Lagrangian phase angle of LL has a lower bound on its oscillation:

supLθL≥θ^1,infLθL≤θ^2,\sup_{L}\theta_{L}\geq\hat{\theta}_{1},\quad\inf_{L}\theta_{L}\leq\hat{\theta}_{2}, (31)

and morever the J-volume of LL (cf. section 2.9) has a nontrivial lower bound

VolJ​(L)=∫Le−i​θ​Ω≥|∫L1Ω|+|∫L2Ω|.\text{Vol}_{J}(L)=\int_{L}e^{-i\theta}\Omega\geq|\int_{L_{1}}\Omega|+|\int_{L_{2}}\Omega|. (32)
Proof.

At a holomorphic polygon Σ\Sigma in the universal family 𝒞\mathcal{C}, denote v1,…​vn−1v_{1},\ldots v_{n-1} as the first order deformation vector fields representing an oriented basis of tangent vectors to the moduli space. In the special case of holomorphic strips, the moduli space refers to the ℝ\mathbb{R}-translation quotient. We noted in section 3.3 that Ω⁡(⋅,v1,…,vn−1)\Omega(\cdot,v_{1},\ldots,v_{n-1}) restricts to a holomorphic 1-form on Σ\Sigma, so can be written as the differential of a holomorphic function FF by the simply connectedness of Σ\Sigma:

d​F=Ω⁡(⋅,v1,…,vn−1).dF=\Omega(\cdot,v_{1},\ldots,v_{n-1}). (33)

The corners on Σ\Sigma are arranged in clockwise order with the following possibilities:

  • •

    In the primary case, we encounter some degree one self intersections on LL from bounding cochains, a corner p∈C​F0​(L,L2)p\in CF^{0}(L,L_{2}), some degree one self intersections on L2L_{2}, a corner rr from γ∈C​F1​(L2,L1)\gamma\in CF^{1}(L_{2},L_{1}), some degree one self intersections on L1L_{1}, and a corner at q∈C​F0​(L1,L)q\in CF^{0}(L_{1},L). Notice the Lagrangian boundary follows L,L2,L1L,L_{2},L_{1} in clockwise order, and we cannot go reversely from L1L_{1} to L2L_{2} instead.

  • •

    In the secondary cases, the boundary data may miss either L1L_{1} or L2L_{2}. For instance, we may encounter some degree one intersections on LL, a corner p∈C​F0​(L,L2)p\in CF^{0}(L,L_{2}), some degree one intersections on L2L_{2} and a corner at q∈C​F0​(L2,L)q\in CF^{0}(L_{2},L). The Lagrangian boundary follows L,L2L,L_{2} in clockwise order. The alternative possibility of Lagrangian boundary along LL and L1L_{1} is entirely similar.

In all cases, there is precisely one corner pp at C​F0​(L,L′)CF^{0}(L,L^{\prime}) and a corner qq at C​F0​(L′,L)CF^{0}(L^{\prime},L). We can normalize F⁡(q)=0F(q)=0 to fix the constant. In the primary case, there is a corner r∈C​F1​(L2,L1)r\in CF^{1}(L_{2},L_{1}), which is absent in the secondary cases. In general, the bordism current 𝒞\mathcal{C} receives contributions from many moduli spaces, and all three cases may arise depending on the generators of H​F0​(L,L′)HF^{0}(L,L^{\prime}) and H​F0​(L′,L)HF^{0}(L^{\prime},L).

We can now define complex valued volume forms on the (n−1)(n-1) dimensional moduli spaces of holomorphic curves. Recall v1,…​vn−1v_{1},\ldots v_{n-1} represent the tangent vectors to the moduli spaces, and the holomorphic function FF depends on v1∧…​vn−1v_{1}\wedge\ldots v_{n-1}. In the primary case, we define

{Ω~L​(v1,…​vn−1)=F⁡(p),Ω~L1​(v1,…​vn−1)=F⁡(r),Ω~L2​(v1,…​vn−1)=F⁡(p)−F⁡(r).\begin{cases}\tilde{\Omega}_{L}(v_{1},\ldots v_{n-1})=F(p),\\ \tilde{\Omega}_{L_{1}}(v_{1},\ldots v_{n-1})=F(r),\\ \tilde{\Omega}_{L_{2}}(v_{1},\ldots v_{n-1})=F(p)-F(r).\end{cases}

In the secondary cases, if the Lagrangian boundary lies on LL and L1L_{1}, then

{Ω~L​(v1,…​vn−1)=F⁡(p),Ω~L1​(v1,…​vn−1)=F⁡(p),Ω~L2​(v1,…​vn−1)=0.\begin{cases}\tilde{\Omega}_{L}(v_{1},\ldots v_{n-1})=F(p),\\ \tilde{\Omega}_{L_{1}}(v_{1},\ldots v_{n-1})=F(p),\\ \tilde{\Omega}_{L_{2}}(v_{1},\ldots v_{n-1})=0.\end{cases}

If the Lagrangian boundary lies on LL and L2L_{2}, then

{Ω~L​(v1,…​vn−1)=F⁡(p),Ω~L1​(v1,…​vn−1)=0,Ω~L2​(v1,…​vn−1)=F⁡(p).\begin{cases}\tilde{\Omega}_{L}(v_{1},\ldots v_{n-1})=F(p),\\ \tilde{\Omega}_{L_{1}}(v_{1},\ldots v_{n-1})=0,\\ \tilde{\Omega}_{L_{2}}(v_{1},\ldots v_{n-1})=F(p).\end{cases}

The values of FF should be understood as the integral of d​FdF on the appropriate portions of ∂Σ\partial\Sigma. The key point is that since ∂𝒞\partial\mathcal{C} sweeps out the cycle L−L1−L2L-L_{1}-L_{2}, we can write the period integrals as integrals on the (n−1)(n-1)-dimensional moduli spaces of holomorphic curves:

∫LΩ=∫ℳΩ~L,∫LiΩ=∫ℳΩ~Li,i=1,2.\int_{L}\Omega=\int_{\mathcal{M}}\tilde{\Omega}_{L},\quad\int_{L_{i}}\Omega=\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}},\quad i=1,2. (34)

where ℳ\mathcal{M} is a shorthand for the weighted sum over contributions from all the (n−1)(n-1)-dimensional moduli spaces involved in the construction of 𝒞\mathcal{C}, cf. the Appendex 6.2.

Recall the positivity condition means that if v0v_{0} stands for a clockwise oriented tangent vector on ∂Σ\partial\Sigma, then v0∧v1​…∧vn−1v_{0}\wedge v_{1}\ldots\wedge v_{n-1} agrees with the orientation on LL, and is opposite to the orientation on L′L^{\prime}. The nonvanishing of v0∧v1​…∧vn−1v_{0}\wedge v_{1}\ldots\wedge v_{n-1} is a consequence of the immersion property from the automatic transversality (cf. Cor. 3.6, Prop. 3.8). The almost calibrated condition implies that Re​Ω>0\text{Re}\Omega>0 on the Lagrangians with respect to the orientation on LL and L′L^{\prime}. Thus

Claim 3.22.

(Monotonicity) Clockwise along ∂Σ\partial\Sigma, the function Re ​F\text{Re }F is increasing on the LL boundary portion, but decreasing on the L′=L1∪L2L^{\prime}=L_{1}\cup L_{2} boundary portion. In particular,

0=Re ​F​(q)≤Re ​F≤Re ​F​(p).0=\text{Re }F(q)\leq\text{Re }F\leq\text{Re }F(p).

More intrinsically, the real part of the complex volume forms on the moduli spaces are nonnegative.

The holomorphic function FF maps Σ\Sigma into a bounded region in the complex plane. The behaviour at the corners is specified in Remark 3.7. Since each vertical line intersects ∂F⁡(Σ)⊂ℂ\partial F(\Sigma)\subset\mathbb{C} at ≤2\leq 2 points by the monotonicity claim above, the boundary and corner local behaviours imply that

Claim 3.23.

(Image curve) The image F⁡(Σ)⊂ℂF(\Sigma)\subset\mathbb{C} lies above its L′L^{\prime} boundary portion, and below its LL boundary portion.

We turn to the proof of the Lagrangian phase angle inequality (31). For each curve that contributes nontrivially to Ω~L\tilde{\Omega}_{L}, by the monotonicity claim we can find a unique point r′r^{\prime} on the LL boundary of ∂Σ\partial\Sigma, such that

{Re F(r′)=Re F(r),primary case,r′=q,secondary case, boundary on L and L2,r′=p,secondary case, boundary on L and L1.\begin{cases}\text{Re }F(r^{\prime})=\text{Re }F(r),\quad&\text{primary case},\\ r^{\prime}=q,\quad&\text{secondary case, boundary on $L$ and $L_{2}$},\\ r^{\prime}=p,\quad&\text{secondary case, boundary on $L$ and $L_{1}$}.\end{cases}

From the image curve claim, we always have Im​F​(r′)≥Im​F​(r)\text{Im}F(r^{\prime})\geq\text{Im}F(r) in the primary case. Integrating over the moduli space of holomorphic curves,

Re​∫ℳF⁡(r′)=Re​∫ℳΩ~L1=Re​∫L1Ω,Im​∫ℳF⁡(r′)≥Im​∫ℳΩ~L1=Im​∫L1Ω.\text{Re}\int_{\mathcal{M}}F(r^{\prime})=\text{Re}\int_{\mathcal{M}}\tilde{\Omega}_{L_{1}}=\text{Re}\int_{L_{1}}\Omega,\quad\text{Im}\int_{\mathcal{M}}F(r^{\prime})\geq\text{Im}\int_{\mathcal{M}}\tilde{\Omega}_{L_{1}}=\text{Im}\int_{L_{1}}\Omega.

We now introduce two almost everywhere defined functions χA1,χA2\chi_{A_{1}},\chi_{A_{2}} on LL. The recipe is that at any generic point P∈LP\in L, if an automatically transverse holomorphic curve in the universal family passes through PP on the boundary portion of ∂Σ\partial\Sigma joining qq to r′r^{\prime} (resp. r′r^{\prime} to pp), then it gives an additive contribution to χA1​(P)\chi_{A_{1}}(P) (resp. χA2​(P)\chi_{A_{2}}(P)) equal to the weighting factor of the curve. Intuitively χA1,χA2\chi_{A_{1}},\chi_{A_{2}} should be understood as the characteristic functions of weighted subsets A1,A2⊂LA_{1},A_{2}\subset L. The positivity condition gives χAi≥0\chi_{A_{i}}\geq 0, and ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime} gives χA1+χA2=1\chi_{A_{1}}+\chi_{A_{2}}=1. Intuitively A1,A2A_{1},A_{2} give a (weighted) partition of LL.

The moduli space integrals now have target space interpretations:

∫ℳF(r′)=∫LχA1Ω=:∫A1Ω,∫ℳF(p)−F(r′)=∫LχA2Ω=:∫A2Ω.\int_{\mathcal{M}}F(r^{\prime})=\int_{L}\chi_{A_{1}}\Omega=:\int_{A_{1}}\Omega,\quad\int_{\mathcal{M}}F(p)-F(r^{\prime})=\int_{L}\chi_{A_{2}}\Omega=:\int_{A_{2}}\Omega.

Since LL is homologous to L1+L2L_{1}+L_{2}, we have ∫LΩ=∫L1Ω+∫L2Ω\int_{L}\Omega=\int_{L_{1}}\Omega+\int_{L_{2}}\Omega. Whence

Claim 3.24.

There is a weighted partition L=A1+A2L=A_{1}+A_{2} such that

Re​∫AiΩ=Re​∫LiΩ>0,Im​∫A2Ω≤Im​∫L2Ω,Im​∫A1Ω≥Im​∫L1Ω.\text{Re}\int_{A_{i}}\Omega=\text{Re}\int_{L_{i}}\Omega>0,\quad\text{Im}\int_{A_{2}}\Omega\leq\text{Im}\int_{L_{2}}\Omega,\quad\text{Im}\int_{A_{1}}\Omega\geq\text{Im}\int_{L_{1}}\Omega.

Consequently arg∫A2Ω≤arg∫L2Ω=θ^2\arg\int_{A_{2}}\Omega\leq\arg\int_{L_{2}}\Omega=\hat{\theta}_{2} and arg∫A1Ω≥arg∫L1Ω=θ^1\arg\int_{A_{1}}\Omega\geq\arg\int_{L_{1}}\Omega=\hat{\theta}_{1}, so in particular infLθL≤θ^2\inf_{L}\theta_{L}\leq\hat{\theta}_{2} and supLθL≥θ^1\sup_{L}\theta_{L}\geq\hat{\theta}_{1}.

Finally we deal with the J-volume lower bound (32). By the triangle inequality,

∫Le−i​θ​Ω=∫L|Ω|=∫A1|Ω|+∫A2|Ω|≥|∫A1Ω|+|∫A2Ω|.\int_{L}e^{-i\theta}\Omega=\int_{L}|\Omega|=\int_{A_{1}}|\Omega|+\int_{A_{2}}|\Omega|\geq|\int_{A_{1}}\Omega|+|\int_{A_{2}}\Omega|.

The RHS is at least |∫L1Ω|+|∫L2Ω||\int_{L_{1}}\Omega|+|\int_{L_{2}}\Omega|, due to an elementary numerical fact:

Lemma 3.25.

Let z,wz,w be complex numbers, with fixed real parts 0<Re​(z)<Re​(w)0<\text{Re}(z)<\text{Re}(w). Then as a function of Im​(z)\text{Im}(z), the function |z|+|w−z||z|+|w-z| is decreasing when arg⁡z≤arg⁡w\arg z\leq\arg w, and increasing when arg⁡z≥arg⁡w\arg z\geq\arg w.

This concludes the proof of (32). ∎

A few remarks are in order to clarify the relevance to special Lagrangian geometry:

Remark 3.10.

Recall that for LL to be a special Lagrangian, then its phase angle is constant, and its J-volume is

VolJ​(L)=|∫LΩ|<|∫L1Ω|+|∫L2Ω|,\text{Vol}_{J}(L)=|\int_{L}\Omega|<|\int_{L_{1}}\Omega|+|\int_{L_{2}}\Omega|,

using the triangle inequality, the homological relation [L]=[L1+L2]∈Hn​(X)[L]=[L_{1}+L_{2}]\in H_{n}(X) and the assumption that θ^1>θ^2\hat{\theta}_{1}>\hat{\theta}_{2}. Thus the conclusion of the theorem is a quantitative obstruction for LL to be special Lagrangian. In section 3.6 we will discuss the relation to Joyce’s LMCF program and the Bridgeland stability condition.

Remark 3.11.

If L1,L2L_{1},L_{2} are actually special Lagrangians, then the phase angle bounds (31) would be evident from the Floer degree formula (63) applied to the intersection points L∩L′L\cap L^{\prime}. One main feature of the theorem is that we do not need a priori knowledge on the existence of special Lagrangians, and the holomorphic volume form enters the obstruction criterion only through cohomological information.

Variant: twisted complex case

The Floer theoretic obstruction for distinguished triangles can be easily generalized to involve many Lagrangians. Let L′L^{\prime} be an exact immersed Lagrangian with bounding cochain built from the data of a twisted complex (17). We assume LL is isomorphic to L′L^{\prime} in Db​F​u​k​(X)D^{b}Fuk(X), so we obtain a bordism current 𝒞\mathcal{C} with ∂𝒞=L−L′=L−∑1NLi\partial\mathcal{C}=L-L^{\prime}=L-\sum_{1}^{N}L_{i}. As before, all Lagrangians are assumed to be almost calibrated, and all intersections are transverse.

Theorem 3.26.

(Floer theoretic obstruction, multiple Lagrangian case) Assume the automatic transversality and the positivity condition hold for the bordism current 𝒞\mathcal{C}. Assume the destabilizing condition

θ^1>θ^2>…>θ^N,θ^i=arg∫LiΩ.\hat{\theta}_{1}>\hat{\theta}_{2}>\ldots>\hat{\theta}_{N},\quad\hat{\theta}_{i}=\arg\int_{L_{i}}\Omega.

Then the Lagrangian phase angle of LL has a lower bound on its oscillation:

supLθL≥θ^1,infLθL≤θ^N,\sup_{L}\theta_{L}\geq\hat{\theta}_{1},\quad\inf_{L}\theta_{L}\leq\hat{\theta}_{N}, (35)

and morever the J-volume of LL has a nontrivial lower bound

VolJ​(L)=∫Le−i​θ​Ω≥∑1N|∫LiΩ|.\text{Vol}_{J}(L)=\int_{L}e^{-i\theta}\Omega\geq\sum_{1}^{N}|\int_{L_{i}}\Omega|. (36)
Proof.

Since most parts of the proof are identical to the distinguished triangle case, we will only sketch the main difference.

The Lagrangian boundaries on ∂Σ\partial\Sigma are arranged in the clockwise order as L,LN,LN−1,…​L1L,L_{N},L_{N-1},\ldots L_{1}. We construct the holomorphic function FF as in (33), and use it to produce complex valued volume forms on the (n−1)(n-1)-dimensional moduli spaces, such that for any m=1,…​Nm=1,\ldots N,

∫LΩ=∫ℳΩ~L,∫LiΩ=∫ℳΩ~Li,i=1,2,…N.\int_{L}\Omega=\int_{\mathcal{M}}\tilde{\Omega}_{L},\quad\int_{L_{i}}\Omega=\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}},\quad i=1,2,\ldots N.

As before, the real part of these complex volume forms are all non-negative, as a consequence of the positivity condition. The claim on the image curve F⁡(Σ)F(\Sigma) holds verbatim. Similarly to the distinguished triangle case, we produce nonnegatively weighted subsets A1,…​AN⊂LA_{1},\ldots A_{N}\subset L with L=∑AiL=\sum A_{i}, such that

Re​∫AmΩ=Re​∫LmΩ>0,Im​∑1m∫AiΩ≥Im​∑1m∫LiΩ,∫LΩ=∑1N∫LiΩ.\text{Re}\int_{A_{m}}\Omega=\text{Re}\int_{L_{m}}\Omega>0,\quad\text{Im}\sum_{1}^{m}\int_{A_{i}}\Omega\geq\text{Im}\sum_{1}^{m}\ \int_{L_{i}}\Omega,\quad\int_{L}\Omega=\sum_{1}^{N}\int_{L_{i}}\Omega. (37)

This implies

arg∫A1Ω≥arg∫L1Ω,arg∫ANΩ≤arg∫LNΩ,\arg\int_{A_{1}}\Omega\geq\arg\int_{L_{1}}\Omega,\quad\arg\int_{A_{N}}\Omega\leq\arg\int_{L_{N}}\Omega,

whence the phase inequality (35).

The J-volume can be bounded below by

VolJ​(L)=∫L|Ω|=∑1N∫Ai|Ω|≥∑1N|∫AiΩ|≥∑1N|∫LiΩ|.\text{Vol}_{J}(L)=\int_{L}|\Omega|=\sum_{1}^{N}\int_{A_{i}}|\Omega|\geq\sum_{1}^{N}|\int_{A_{i}}\Omega|\geq\sum_{1}^{N}|\int_{L_{i}}\Omega|.

The last step uses the purely numerical Lemma 3.27 below. ∎

Lemma 3.27.

Let z1,…​zNz_{1},\ldots z_{N} be complex numbers, and a1,…​aNa_{1},\ldots a_{N} be fixed complex numbers with positive real parts, such that arg⁡a1>arg⁡a2>…>arg⁡aN\arg a_{1}>\arg a_{2}>\ldots>\arg a_{N}. Assume

Re​(zi)=Re​(ai),Im​∑1mzi≥Im​∑1mai,∑1Nzi=∑1Nai.\text{Re}(z_{i})=\text{Re}(a_{i}),\quad\text{Im}\sum_{1}^{m}z_{i}\geq\text{Im}\sum_{1}^{m}a_{i},\quad\sum_{1}^{N}z_{i}=\sum_{1}^{N}a_{i}.

Then ∑1N|zi|≥∑1N|ai|\sum_{1}^{N}|z_{i}|\geq\sum_{1}^{N}|a_{i}|.

Proof.

We argue by induction. The N=2N=2 case is implied by Lemma 3.25. In general, we view ∑1N|zi|\sum_{1}^{N}|z_{i}| as a function of the imaginary parts of z1,…​zNz_{1},\ldots z_{N} subject to the constraints. Clearly this function achieves its minimum for some (zi)(z_{i}). If z1=a1z_{1}=a_{1}, then we can conclude by induction. Otherwise Im​z1>Im​a1\text{Im}z_{1}>\text{Im}a_{1}. If arg⁡z2<arg⁡z1\arg z_{2}<\arg z_{1}, then we can fix z1+z2z_{1}+z_{2} and decrease ∑12|zi|\sum_{1}^{2}|z_{i}| by Lemma 3.25, which would contradict minimality. Proceding with this argument, we are forced to have

arg⁡z1≤arg⁡z2≤…≤arg⁡zN,\arg z_{1}\leq\arg z_{2}\leq\ldots\leq\arg z_{N},

whence

arg∑1Nzi≥argz1>arga1>arg∑1Nai\arg\sum_{1}^{N}z_{i}\geq\arg z_{1}>\arg a_{1}>\arg\sum_{1}^{N}a_{i}

which contradicts ∑1Nzi=∑1Nai\sum_{1}^{N}z_{i}=\sum_{1}^{N}a_{i}. ∎

What if we relax the positivity condition?

We now discuss a weaker version that does not require the positivity condition on holomorphic curves. This amounts to dropping pointwise positivity of the integrand for the moduli space integral, which breaks some parts of our mirror analogy.

As in Theorem 3.21, we consider L′L^{\prime} built from two immersed Lagrangians L1,L2L_{1},L_{2}, and LL fits into the distinguished triangle. All Lagrangians are almost calibrated, and all intersections are transverse. We classify the automatically transverse holomorphic curves (cf. Cor. 3.6, Prop. 3.8) into ±\pm types according to whether the boundary evalation to LL agrees with the orientation on LL or its opposite. The complex volume forms Ω~Li\tilde{\Omega}_{L_{i}} on the moduli space can be split into the sum of two parts according to whether u:Σ→Xu:\Sigma\to X is of ±\pm types:

Ω~Li=Ω~Li++Ω~Li−,∫ℳΩ~Li=∫LiΩ.\tilde{\Omega}_{L_{i}}=\tilde{\Omega}_{L_{i}}^{+}+\tilde{\Omega}_{L_{i}}^{-},\quad\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}=\int_{L_{i}}\Omega.

In particular the signed measure Re​Ω~Li\text{Re}\tilde{\Omega}_{L_{i}} is decomposed into its positive and negative parts, and Re​∫ℳΩ~Li−≤0\text{Re}\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}^{-}\leq 0. We define

θ^i+=arg∫ℳΩ~Li+,θ^i−=arg(−∫ℳΩ~Li−),i=1,2.\hat{\theta}_{i}^{+}=\arg\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}^{+},\quad\hat{\theta}_{i}^{-}=\arg(-\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}^{-}),\quad i=1,2.

Here θ^i−\hat{\theta}_{i}^{-} is only defined when ∫ℳΩ~Li−\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}^{-} is nonzero, namely the case not covered already by the positivity condition.

Theorem 3.28.

(Floer theoretic obstruction, relaxing positivity condition) Assume the automatic transversality holds for the bordism current 𝒞\mathcal{C} between LL and L′L^{\prime}. Then the Lagrangian phase angle of LL has a lower bound on its oscillation:

supLθL≥max⁡{θ^1+,θ^1−},infLθL≤min⁡{θ^2+,θ^2−}.\sup_{L}\theta_{L}\geq\max\{\hat{\theta}_{1}^{+},\hat{\theta}_{1}^{-}\},\quad\inf_{L}\theta_{L}\leq\min\{\hat{\theta}_{2}^{+},\hat{\theta}_{2}^{-}\}.
Proof.

We will only sketch the modifications. The positivity conditition enters through the monotonicity claim 3.22. Once we drop this, we would allow holomophic discs u:Σ→Xu:\Sigma\to X that sweep out parts of L∪L′L\cup L^{\prime} with the reversed orientation. For such curves, claim 3.22 is modified to

Claim 3.29.

Clockwise along ∂Σ\partial\Sigma, the function Re ​F\text{Re }F is decreasing on the LL boundary portion, but increasing on the L′=L1∪L2L^{\prime}=L_{1}\cup L_{2} boundary portion. In particular,

0=Re ​F​(q)≥Re ​F≥Re ​F​(p).0=\text{Re }F(q)\geq\text{Re }F\geq\text{Re }F(p).

More intrinsically, the real part of the complex volume forms on the moduli spaces at such u:Σ→Xu:\Sigma\to X are nonpositive.

The corresponding claim 3.23 is modified to

Claim 3.30.

The image F⁡(Σ)⊂ℂF(\Sigma)\subset\mathbb{C} lies below its L′L^{\prime} boundary portion, and above its LL boundary portion.

At almost every point on L∪L′L\cup L^{\prime}, only automatically transverse holomophic curves pass through it, since by assumption the boundary evaluation of the other holomorphic curves is contained in some subset of L∪L′L\cup L^{\prime} with Hausdorff dimension ≤n−1\leq n-1. According to the ±\pm types of the automatically transverse curves, we decompose the weighted characteristic functions χAi\chi_{A_{i}} on LL into its positive and negative parts χAi+≥0\chi_{A_{i}^{+}}\geq 0 and χAi−≤0\chi_{A_{i}^{-}}\leq 0.

Then upon integration over the moduli space,

Re∫LχAi+Ω=Re∫ℳΩ~Li+≥0,Re∫LχAi−Ω=Re∫ℳΩ~Li−≤0,Im∫LχA2+Ω≤Im∫ℳΩ~L2+,Im∫LχA1+Ω≥Im∫ℳΩ~L1+,Im∫LχA2−Ω≥Im∫ℳΩ~L2−,Im∫LχA1−Ω≤Im∫ℳΩ~L1−.\begin{split}&\text{Re}\int_{L}\chi_{A_{i}^{+}}\Omega=\text{Re}\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}^{+}\geq 0,\quad\text{Re}\int_{L}\chi_{A_{i}^{-}}\Omega=\text{Re}\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}^{-}\leq 0,\\ &\text{Im}\int_{L}\chi_{A_{2}^{+}}\Omega\leq\text{Im}\int_{\mathcal{M}}\tilde{\Omega}_{L_{2}}^{+},\quad\text{Im}\int_{L}\chi_{A_{1}^{+}}\Omega\geq\text{Im}\int_{\mathcal{M}}\tilde{\Omega}_{L_{1}}^{+},\\ &\text{Im}\int_{L}\chi_{A_{2}^{-}}\Omega\geq\text{Im}\int_{\mathcal{M}}\tilde{\Omega}_{L_{2}}^{-},\quad\text{Im}\int_{L}\chi_{A_{1}^{-}}\Omega\leq\text{Im}\int_{\mathcal{M}}\tilde{\Omega}_{L_{1}}^{-}.\end{split}

In particular

arg∫LχA2+Ω≤θ^2+,arg(−∫LχA2−Ω)≤θ^2−,\arg\int_{L}\chi_{A_{2}^{+}}\Omega\leq\hat{\theta}_{2}^{+},\quad\arg(-\int_{L}\chi_{A_{2}^{-}}\Omega)\leq\hat{\theta}_{2}^{-},

and

arg∫LχA1+Ω≥θ^1+,arg(−∫LχA1−Ω)≥θ^1−.\arg\int_{L}\chi_{A_{1}^{+}}\Omega\geq\hat{\theta}_{1}^{+},\quad\arg(-\int_{L}\chi_{A_{1}^{-}}\Omega)\geq\hat{\theta}_{1}^{-}.

Now χAi+≥0\chi_{A_{i}^{+}}\geq 0 and χAi−≤0\chi_{A_{i}^{-}}\leq 0, and the special case where χAi−=0\chi_{A_{i}^{-}}=0 almost everywhere is already covered by the positivity condition. The Theorem follows. ∎

Remark 3.12.

In the special case where L1,L2L_{1},L_{2} are special Lagrangians of phase θ^1,θ^2\hat{\theta}_{1},\hat{\theta}_{2}, then clearly θ^i±=θ^i\hat{\theta}_{i}^{\pm}=\hat{\theta}_{i}. The conclusion in this case can be deduced easily from Floer degree considerations at Lagrangian intersections, similar to section 2.2.

Remark 3.13.

Recall θ^i=arg∫LiΩ\hat{\theta}_{i}=\arg\int_{L_{i}}\Omega. The caveat is that max⁡{θ^i±}\max\{\hat{\theta}_{i}^{\pm}\} and min⁡{θ^i±}\min\{\hat{\theta}_{i}^{\pm}\} do not quite control θ^i\hat{\theta}_{i}, so the above Theorem 3.28 does not imply the phase angle inequality (31). In this sense the conclusion of Theorem 3.28 is weaker than Theorem 3.21, illustrating the power of the positivity condition.

On the other hand, we will heuristically argue in section 3.6 that in the Thomas-Yau-Joyce picture, once we assume the existence of Joyce’s Bridgeland stability condition, the phase angle inequality (31) can be deduced without the positivity condition in Theorem 3.21.

We think it is very interesting to either prove the positivity condition as a consequence of the other assumptions, or to find another Floer theoretic argument for (31) that requires neither the positivity condition, nor the a priori knowledge of special Lagrangian representatives.

3.6 Towards a Bridgeland stability condition

Joyce’s proposal and Bridgeland stability condition revisited

We now seek a better appreciation of the Bridgeland stability aspect of Joyce’s proposal (cf. section 2.1). To specify the Bridgeland stability condition on Db​F​u​k​(X)D^{b}Fuk(X), we need the central charge Z⁡(L)=∫LΩZ(L)=\int_{L}\Omega, and all the subcategories 𝒫⁡(ϕ0<ϕ<ϕ1)\mathcal{P}(\phi_{0}<\phi<\phi_{1}) for any interval (ϕ0,ϕ1)(\phi_{0},\phi_{1}). Joyce’s proposal [41] strongly suggests two claims:

  • •

    If an unobstructed Lagrangian brane LL has phase angle function θ∈(π​ϕ0,π​ϕ1)\theta\in(\pi\phi_{0},\pi\phi_{1}), then LL defines an object in the subcategory 𝒫⁡(ϕ0<ϕ<ϕ1)\mathcal{P}(\phi_{0}<\phi<\phi_{1}) generated by all stable objects with ϕ0<ϕ<ϕ1\phi_{0}<\phi<\phi_{1}. This claim is because the infinite time limit of the LMCF should provide the stable objects which generate LL, and by the monotonicity of the Lagrangian angle (cf. section 4.1 below), we can predict a priori θ∈(π​ϕ0,π​ϕ1)\theta\in(\pi\phi_{0},\pi\phi_{1}) for all these stable objects.

  • •

    Any object in 𝒫⁡(ϕ0<ϕ<ϕ1)\mathcal{P}(\phi_{0}<\phi<\phi_{1}) can be generated by unobstructed Lagrangian branes with phase angle function θ∈(π​ϕ0,π​ϕ1)\theta\in(\pi\phi_{0},\pi\phi_{1}).

Thus one can simply define 𝒫⁡(ϕ0<ϕ<ϕ1)\mathcal{P}(\phi_{0}<\phi<\phi_{1}) to be the subcategory of the derived Fukaya category (suitably enlarged to allow for immersed and singular objects) generated by all unobstructed Lagrangian branes LL with θ∈(π​ϕ0,π​ϕ1)\theta\in(\pi\phi_{0},\pi\phi_{1}), and then reconstruct 𝒫⁡(ϕ′)\mathcal{P}(\phi^{\prime}) as the intersection of all 𝒫⁡(ϕ0<ϕ<ϕ1)\mathcal{P}(\phi_{0}<\phi<\phi_{1}) for all ϕ0<ϕ′<ϕ1\phi_{0}<\phi^{\prime}<\phi_{1}. Such a definition would make the Thomas-Yau proposal nearly tautological, and the difficult part of Joyce’s proposal is to verify this indeed defines a Bridgeland stability. In fact, by the discussions in section 2.1, 2.2, the only formidable part is the Harder-Narasimhan decomposition, for which Joyce’s LMCF provides the conjectural mechanism.

There are two primary applications of the Thomas-Yau-Joyce proposal to keep in mind:

  • •

    The existence of special Lagrangians is important for geometric measure theory. A definition of stability conditions along the above lines is too tautological to be useful.

  • •

    Defining special Lagrangian DT invariants is important for mirror symmetry (cf. section 2.4). Knowing the existence of a Bridgeland stability condition on Db​F​u​k​(X)D^{b}Fuk(X) is of great theoretic significance in view of Kontsevich and Soibelman’s framework [46][47], but without a more Floer theoretic characterization it would lack computability.

Thus even if Joyce’s conjectures can be proved along the lines in [41], it is still desirable to have a Floer theoretic characterization of the Bridgeland stability condition. We first revisit Theorem 3.21 in the light of the Thomas-Yau-Joyce conjectural picture, but without assuming the automatic transversality and positivity condition.

Conjecture 3.31.

Suppose we have almost calibrated exact Lagrangian objects L1,L2,LL_{1},L_{2},L, fitting into a distinguished triangle L1→L→L2→L1​[1]L_{1}\to L\to L_{2}\to L_{1}[1], and satisfies the destabilizing condition

θ^1=arg∫L1Ω>θ^2=arg∫L2Ω.\hat{\theta}_{1}=\arg\int_{L_{1}}\Omega>\hat{\theta}_{2}=\arg\int_{L_{2}}\Omega.

Then the phase angle inequality (31) follows. In particular, the derived category class of LL admits no special Lagrangian representative.

Proof.

(Heuristic) Consider the Harder-Narasimhan decomposition (4) of L1L_{1}:

0=ℰ0→ℰ1→…→ℰN=L1,0=\mathcal{E}_{0}\to\mathcal{E}_{1}\to\ldots\to\mathcal{E}_{N}=L_{1},

fitting into the distinguished triangles

ℰi−1→ℰi→Li′→ℰi−1​[1],\mathcal{E}_{i-1}\to\mathcal{E}_{i}\to L_{i}^{\prime}\to\mathcal{E}_{i-1}[1],

where Li′L_{i}^{\prime} represents an object in 𝒫⁡(ϕi)\mathcal{P}(\phi_{i}), with ϕ1>ϕ2​…>ϕN\phi_{1}>\phi_{2}\ldots>\phi_{N}. Since by assumption L1L_{1} is almost calibrated, we have L1∈𝒫⁡(−12<ϕ<12)L_{1}\in\mathcal{P}(-\frac{1}{2}<\phi<\frac{1}{2}), hence −12<ϕi<12-\frac{1}{2}<\phi_{i}<\frac{1}{2}. Since the central charges satisfy

Z⁡(L1)=∑1NZ⁡(Li′),arg⁡Z⁡(Li)=π​ϕi,Z(L_{1})=\sum_{1}^{N}Z(L_{i}^{\prime}),\quad\arg Z(L_{i})=\pi\phi_{i},

we must have θ^1≤π​ϕ1\hat{\theta}_{1}\leq\pi\phi_{1}. The conjectural description of the Bridgeland stability condition requires that Li′L_{i}^{\prime} has a special Lagrangian representative with constant Lagrangian phase π​ϕi\pi\phi_{i}. A weaker requirement which suffices for us is that there exists a representative Li′L_{i}^{\prime} with Lagrangian angle function θLi′\theta_{L_{i}^{\prime}} satisfying the oscillation bound |θLi′−π​ϕi|<ϵ|\theta_{L_{i}^{\prime}}-\pi\phi_{i}|<\epsilon for any given ϵ>0\epsilon>0. It is expected that this flexibility allows one to assume sufficient smoothness on the Lagrangian.

By combining the distinguished triangles, we obtain a new distinguished triangle

L1′→L→L′′→L1′​[1].L_{1}^{\prime}\to L\to L^{\prime\prime}\to L_{1}^{\prime}[1].

Here L1′,L,L′′L_{1}^{\prime},L,L^{\prime\prime} are all almost calibrated. Suppose for contradiction that supLθL<θ^1\sup_{L}\theta_{L}<\hat{\theta}_{1}. Then supLθL<π​ϕ1\sup_{L}\theta_{L}<\pi\phi_{1}, and we can arrange supLθL<infL1′θL1′\sup_{L}\theta_{L}<\inf_{L_{1}^{\prime}}\theta_{L_{1}^{\prime}}. The Floer degree formula (63) implies C​F0​(L1′,L)=0CF^{0}(L_{1}^{\prime},L)=0, and in particular H​F0​(L1′,L)=0HF^{0}(L_{1}^{\prime},L)=0. The distinguished triangle splits: L′′≃L⊕L1′​[1]L^{\prime\prime}\simeq L\oplus L_{1}^{\prime}[1]. Since L′′L^{\prime\prime} is almost calibrated, it lies in 𝒫⁡(−12<ϕ<12)\mathcal{P}(-\frac{1}{2}<\phi<\frac{1}{2}), and so must L1′​[1]L_{1}^{\prime}[1]. But L1′∈𝒫⁡(ϕ1)L_{1}^{\prime}\in\mathcal{P}(\phi_{1}) implies L1′​[1]∈𝒫⁡(ϕ1+1)L_{1}^{\prime}[1]\in\mathcal{P}(\phi_{1}+1). Since ϕ1+1>12\phi_{1}+1>\frac{1}{2}, we know 𝒫⁡(ϕ1+1)∩𝒫⁡(−12<ϕ<12)=∅\mathcal{P}(\phi_{1}+1)\cap\mathcal{P}(-\frac{1}{2}<\phi<\frac{1}{2})=\emptyset, contradiction. This proves supLθL≥θ^1\sup_{L}\theta_{L}\geq\hat{\theta}_{1}, subject to the conjectural existence of the Bridgeland stability condition.

A very similar argument, beginning with the Harder-Narasimhan decomposition of L2L_{2}, would show infLθL≤θ^2\inf_{L}\theta_{L}\leq\hat{\theta}_{2}. ∎

Remark 3.14.

In the above argument, once we achieved C​F0​(L1′,L)=0CF^{0}(L_{1}^{\prime},L)=0, there is a different way to proceed. We reinterpret the distinguished triangle L1′→L→L′′→L1′​[1]L_{1}^{\prime}\to L\to L^{\prime\prime}\to L_{1}^{\prime}[1] as an isomorphism in Db​F​u​k​(X)D^{b}Fuk(X) between LL and a twisted complex built from L1′∪L′′L_{1}^{\prime}\cup L^{\prime\prime}. This would give rise to a bordism current constructed from the universal family of holomorphic curves, with ∂𝒞=L−L1′−L′′\partial\mathcal{C}=L-L_{1}^{\prime}-L^{\prime\prime}. However, C​F0​(L1′,L)=0CF^{0}(L_{1}^{\prime},L)=0 implies that no holomorphic curve contributing to 𝒞\mathcal{C} passes from L1′L_{1}^{\prime} to LL in the clockwise direction of ∂Σ\partial\Sigma. The twisted complex structure on L1′∪L′′L_{1}^{\prime}\cup L^{\prime\prime} forbids the passage from L1′L_{1}^{\prime} to L′′L^{\prime\prime} in the clockwise direction of ∂Σ\partial\Sigma. Thus if the holomorphic curve has any boundary portion on L1′L_{1}^{\prime}, its entire boundary would lie on L1′L_{1}^{\prime}, which cannot happen in the almost calibrated setting.

This motivates the following definition, whose precise meaning depends on the conjectural enlargement of the derived Fukaya category by incorporating singular Lagrangian objects:

Definition 3.32.

Let LL be an almost calibrated exact Lagrangian brane representing a class in the (suitably enlarged) derived Fukaya category. Suppose for any almost calibrated exact Lagrangian objects L1,L2L_{1},L_{2} fitting into a distinguished triangle L1→L→L2→L1​[1]L_{1}\to L\to L_{2}\to L_{1}[1], we always have

θ^1=arg∫L1Ω≤θ^2=∫L2Ω,resp. θ^1=arg∫L1Ω<θ^2=∫L2Ω,\hat{\theta}_{1}=\arg\int_{L_{1}}\Omega\leq\hat{\theta}_{2}=\int_{L_{2}}\Omega,\quad\text{resp. }\hat{\theta}_{1}=\arg\int_{L_{1}}\Omega<\hat{\theta}_{2}=\int_{L_{2}}\Omega,

then we say LL is Thomas-Yau semistable (resp. strictly stable). If LL fails to be Thomas-Yau semistable, we say it is Thomas-Yau unstable.

We have attributed this definition to Thomas-Yau [65][66], since it is in their spirit that stability conditions should be Floer theoretic conditions to be tested on the distinguished triangles, and that one should restrict attention only to almost calibrated Lagrangians. We now argue that if Joyce’s conjectural Bridgeland stability exists with its expected properties, then its semistable objects should agree with Thomas-Yau semistability.

Conjecture 3.33.

An almost calibrated exact Lagrangian brane LL defines a semistable object in Db​F​u​k​(X)D^{b}Fuk(X) under Joyce’s Bridgeland stability, if and only if it is Thomas-Yau semistable.

Proof.

(Heuristic) If the derived category class of LL is semistable in Joyce’s sense, then we can choose an optimal representative which is a special Lagrangian, or at least has phase oscillation arbitrarily small. By conjecture 3.31, we cannot have any destabilizing distinguished triangle, i.e. LL is Thomas-Yau semistable.

Conversely, if LL is not a semistable object in Joyce’s sense, then from its Harder-Narasimhan decomposition we can produce a destabilizing distinguished triangle L1→L→L2→L1​[1]L_{1}\to L\to L_{2}\to L_{1}[1], with almost calibrated L1,L2L_{1},L_{2}, which violates Thomas-Yau semistability. ∎

Having discussed the semistable objects, it is interesting to see what Joyce’s LMCF picture suggests about the Harder-Narasimhan decomposition.

Conjecture 3.34.

Assume further that the Kähler metric on XX is Calabi-Yau. Suppose LL is an almost calibrated exact Lagrangian brane in Db​F​u​k​(X)D^{b}Fuk(X), with Harder-Narasimhan decomposition (4)

0=ℰ0→ℰ1→…→ℰN=L,0=\mathcal{E}_{0}\to\mathcal{E}_{1}\to\ldots\to\mathcal{E}_{N}=L,

fitting into the distinguished triangles

ℰi−1→ℰi→Li→ℰi−1​[1],\mathcal{E}_{i-1}\to\mathcal{E}_{i}\to L_{i}\to\mathcal{E}_{i-1}[1],

such that Li∈𝒫⁡(ϕi)L_{i}\in\mathcal{P}(\phi_{i}) with ϕ1>…>ϕN\phi_{1}>\ldots>\phi_{N}. We have θ^i=πϕi=arg∫LiΩ\hat{\theta}_{i}=\pi\phi_{i}=\arg\int_{L_{i}}\Omega. Then the phase angle inequality (35) and the volume lower bound (36) hold.

Proof.

(Heuristic) In Joyce’s conjectural program, the Harder-Narasimhan decomposition is constructed by running the LMCF (Lt)(L_{t}) starting from the unobstructed Lagrangian LL, and take the infinite time limit (6) to obtain the limiting special Lagrangians L1,…,LNL_{1},\ldots,L_{N} with angles θ^1>θ^2>…>θ^N\hat{\theta}_{1}>\hat{\theta}_{2}>\ldots>\hat{\theta}_{N}, assuming L1,…​LNL_{1},\ldots L_{N} have enough regularity to be admitted as objects of Db​F​u​k​(X)D^{b}Fuk(X). It is expected that L1,…​LNL_{1},\ldots L_{N} generate LL in Db​F​u​k​(X)D^{b}Fuk(X) via (4).

A basic feature of LMCF in Calabi-Yau manifolds is that the Lagrangian angle satisfies a heat equation (cf. section 4.1), so supLtθ\sup_{L_{t}}\theta is nonincreasing in time (resp. infLtθ\inf_{L_{t}}\theta is nondecreasing). Comparing the initial time with the infinite time limit, this suggests supθL≥θ^1\sup\theta_{L}\geq\hat{\theta}_{1} and infθL≤θ^N\inf\theta_{L}\leq\hat{\theta}_{N}.

Morever, if the ambient metric is Calabi-Yau, then LMCF is a special case of mean curvature flow, so the volume functional decreases in time. This monotonicity is not affected by the surgeries in Joyce’s LMCF. Thus

Vol​(L)≥∑1NVol​(Li)=∑1N|Z⁡(Li)|=∑1N|∫LiΩ|.\text{Vol}(L)\geq\sum_{1}^{N}\text{Vol}(L_{i})=\sum_{1}^{N}|Z(L_{i})|=\sum_{1}^{N}|\int_{L_{i}}\Omega|.

Under the Calabi-Yau metric, the volume of the Lagrangian LL agrees with the JJ-volume:

Vol​(L)=∫Le−i​θ​Ω=∫L|Ω|.\text{Vol}(L)=\int_{L}e^{-i\theta}\Omega=\int_{L}|\Omega|.

so (36) follows. ∎

Remark 3.15.

Analogously in the context of HYM connections, if a holomorphic bundle EE is unstable, then its Harder-Narasimhan decomposition provides a lower bound on the Yang-Mills energy of any Chern connection on EE compatible with ∂¯E\bar{\partial}_{E}, which improves the topological energy bound. This type of phenomenon is common in Kähler geometry, for instance it also happens in the context of K-stability. These topics are covered in the introduction of [30].

In conclusion, Joyce’s conjectural picture suggests that if a Lagrangian object is unstable, then it satisfies certain angle and volume inequalities which quantitatively forbids it to be a special Lagrangian, and these obstructions detect the features of the Harder-Narasimhan decomposition. This should be compared with Theorem 3.26, which contains the main features of the obstructions, but makes no a priori reference to the LMCF or special Lagrangian representatives. The cost is that Theorem 3.21 and 3.26 require the positivity condition as an extra hypothesis.

Almost calibrated case: categorical predictions of the Joyce picture

A complete characterization of Bridgeland stability conditions on a triangulated category, known since the inception of the subject [13, Prop 5.3], is that 𝒫⁡(ϕ0<ϕ≤ϕ0+1)\mathcal{P}(\phi_{0}<\phi\leq\phi_{0}+1) defines an abelian subcategory (‘the heart of a bounded tt-structure’), and the central charge function on this abelian subcategory satisfies the Harder-Narasimhan condition.

In the Thomas-Yau-Joyce picture, 𝒫⁡(−12<ϕ≤12)\mathcal{P}(-\frac{1}{2}<\phi\leq\frac{1}{2}) essentially is the same as the subcategory of almost calibrated Lagrangians, if we assume there is no special Lagrangian of phase π2\frac{\pi}{2}, which holds as long as the discrete set of values of Ω\Omega-periods on Hn​(X,ℤ)H_{n}(X,\mathbb{Z}) miss the phase angle π2\frac{\pi}{2}. Then this picture would predict almost calibrated Lagrangians to form an abelian category, which morever generate the entire derived Fukaya category using the shift operator. Morally, this is asserting that there are sufficiently many almost calibrated Lagrangians, which is evidently very deep since constructing geometric Lagrangian objects is known to be a difficult problem in symplectic topology. Another deep prediction of the existence of Bridgeland stability condition [41, conjecture 3.6], is that the derived Fukaya category Db​F​u​k​(X)D^{b}Fuk(X) (after incorporating immersed and singular Lagrangians with local systems) is automatically idempotent complete, so agrees with Dπ​F​u​k​(X)D^{\pi}Fuk(X). These predictions, if correct, are very interesting structural results on the Fukaya category, but at the moment they are controversial.

In Chapter 5, we will set up a variational framework to find special Lagrangian representatives of Db​F​u​k​(X)D^{b}Fuk(X) classes under the assumption of Thomas-Yau semistability. By restricting only to the subcategory of almost calibrated Lagrangians, our program evades these difficult structural claims on the entire Db​F​u​k​(X)D^{b}Fuk(X). It would thus not have the same strength as the Joyce program, nor is it subject to the same falsification criteria.

3.7 Moduli integral formula for the Solomon functional

3.7.1 Moduli integral formula for the Solomon functional

Assuming automatic transversality, we can rewrite the Solomon functional (20) as a moduli space integral in terms of the notations introduced in section 3.5. Let u:Σ→Xu:\Sigma\to X be a holomorphic polygon, with first order deformation vector fields v1,…​vn−1v_{1},\ldots v_{n-1}, so we can define a holomorphic function FF via (33). In clockwise order on ∂Σ\partial\Sigma, we encounter the degree one intersections on LL, an intersection p∈C​F0​(L,L0)p\in CF^{0}(L,L_{0}), the degree one self intersections on L0L_{0}, and an intersection q∈C​F0​(L0,L)q\in CF^{0}(L_{0},L). As before, we fix the additive constant by F⁡(q)=0F(q)=0.

In the following calculation, we will use the complex orientation on Σ\Sigma, and the counterclockwise orientation on ∂Σ\partial\Sigma. The Solomon functional contains a term −∫𝒞λ∧Im(e−i​θ^Ω).-\int_{\mathcal{C}}\lambda\wedge\text{Im}(e^{-i\hat{\theta}}\Omega). Now −∫𝒞λ∧Ω-\int_{\mathcal{C}}\lambda\wedge\Omega can be expressed as an integral of the following (n−1)(n-1)-form over the (n−1)(n-1)-dimensional moduli spaces ℳ\mathcal{M} of holomorphic curves:

∫Σλ∧Ω⁡(⋅,v1,…​vn−1)=∫Σλ∧𝑑F.\int_{\Sigma}\lambda\wedge\Omega(\cdot,v_{1},\ldots v_{n-1})=\int_{\Sigma}\lambda\wedge dF.

Notice that since u:Σ→Xu:\Sigma\to X is a holomorphic curve and Ω\Omega is an (n,0)(n,0)-form, adjusting viv_{i} by a vector field tangent to Σ\Sigma does not change this integrand, and all viv_{i} must hit Ω\Omega instead of the 1-form λ\lambda. After integration by part,

∫Σλ∧𝑑F=∫ΣF​𝑑λ−∫∂ΣF​λ=∫ΣF​ω−∫∂ΣF​λ.\int_{\Sigma}\lambda\wedge dF=\int_{\Sigma}Fd\lambda-\int_{\partial\Sigma}F\lambda=\int_{\Sigma}F\omega-\int_{\partial\Sigma}F\lambda.

The Solomon functional contains another two terms ∫LfL​Im​(e−i​θ^​Ω)\int_{L}f_{L}\text{Im}(e^{-i\hat{\theta}}\Omega) and −∫L0fL0Im(e−i​θ^Ω)-\int_{L_{0}}f_{L_{0}}\text{Im}(e^{-i\hat{\theta}}\Omega). Now ∫LfL​Ω\int_{L}f_{L}\Omega can be expressed as an integral of the following (n−1)(n-1)-form over the moduli spaces ℳ\mathcal{M}:

−∫∂Σ∩LfLΩ(⋅,v1,…vn−1)=−∫∂Σ∩LfLdF.-\int_{\partial\Sigma\cap L}f_{L}\Omega(\cdot,v_{1},\ldots v_{n-1})=-\int_{\partial\Sigma\cap L}f_{L}dF.

The abused notation ∂Σ∩L\partial\Sigma\cap L means the part of ∂Σ\partial\Sigma mapping to LL instead of L0L_{0}. Similarly −∫L0fL0Ω-\int_{L_{0}}f_{L_{0}}\Omega is the moduli space integral of the (n−1)(n-1)-form

−∫∂Σ∩L0fL0Ω(⋅,v1,…vn−1)=−∫∂Σ∩L0fL0dF.-\int_{\partial\Sigma\cap L_{0}}f_{L_{0}}\Omega(\cdot,v_{1},\ldots v_{n-1})=-\int_{\partial\Sigma\cap L_{0}}f_{L_{0}}dF.

The extra minus sign comes from the fact that ∂𝒞\partial\mathcal{C} sweeps out the cycle −L0-L_{0} instead of L0L_{0}.

Combining all the three contributions, the Solomon functional is the moduli space integral with integrand

ℐ=Im​∫Σe−i​θ^​F​ω−Im​∫∂Σ∩Le−i​θ^​d​(fL​F)−Im​∫∂Σ∩L0e−i​θ^​d​(fL0​F).\mathcal{I}=\text{Im}\int_{\Sigma}e^{-i\hat{\theta}}F\omega-\text{Im}\int_{\partial\Sigma\cap L}e^{-i\hat{\theta}}d(f_{L}F)-\text{Im}\int_{\partial\Sigma\cap L_{0}}e^{-i\hat{\theta}}d(f_{L_{0}}F).

The last two terms involve total derivatives, so can be integrated along boundary segments between the corner points, to yield

−Im∫∂Σ∩Le−i​θ^d(fLF)−Im∫∂Σ∩L0e−i​θ^d(fL0F)=Im​∑all cornerse−i​θ^​F​f|−+,\begin{split}&-\text{Im}\int_{\partial\Sigma\cap L}e^{-i\hat{\theta}}d(f_{L}F)-\text{Im}\int_{\partial\Sigma\cap L_{0}}e^{-i\hat{\theta}}d(f_{L_{0}}F)\\ &=\text{Im}\sum_{\text{all corners}}e^{-i\hat{\theta}}Ff|^{+}_{-},\end{split} (38)

where f|−+f|^{+}_{-} stands for the difference of the potentials fL+−fL−f_{L_{+}}-f_{L-} at a Lagrangian intersection point, such that ∂Σ\partial\Sigma moves from L+L_{+} to L−L_{-} in the clockwise direction. In the more general framework of Floer theory with Novikov coefficients, f|−+f|^{+}_{-} have the interpretation as the Novikov exponents of these intersection points. The bounding cochain elements have f|−+≥0f|^{+}_{-}\geq 0, while p∈C​F0​(L,L0),q∈C​F0​(L0,L)p\in CF^{0}(L,L_{0}),q\in CF^{0}(L_{0},L) may have negative Novikov exponents.

Proposition 3.35.

(Moduli space integral formula) The Solomon functional 𝒮⁡(L)\mathcal{S}(L) is the integral of the following complex valued volume form over the (n−1)(n-1)-dimensional moduli spaces of holomorphic curves:

𝒮⁡(L)=∫ℳℐ,ℐ=Im​∫Σe−i​θ^​F​ω+Im​∑all cornerse−i​θ^​F​f|−+.\mathcal{S}(L)=\int_{\mathcal{M}}\mathcal{I},\quad\mathcal{I}=\text{Im}\int_{\Sigma}e^{-i\hat{\theta}}F\omega+\text{Im}\sum_{\text{all corners}}e^{-i\hat{\theta}}Ff|^{+}_{-}. (39)
Remark 3.16.

The normalization F⁡(q)=0F(q)=0 is convenient, but changing FF by a constant along Σ\Sigma does not affect ℐ\mathcal{I}, due to the energy identity

∫Σω+∑all cornersf|−+=0.\int_{\Sigma}\omega+\sum_{\text{all corners}}f|^{+}_{-}=0.
Remark 3.17.

We have focused the discussion on the holomorphic curves with boundary on both LL and L0L_{0}, which are the only curves relevant for the bordism current 𝒞\mathcal{C} in the almost calibrated case. In general we need also curves involving corners at C​F−1​(L,L)CF^{-1}(L,L) or C​F−1​(L0,L0)CF^{-1}(L_{0},L_{0}), and the formula (39) takes into account all these contributions.

3.7.2 Change of reference Lagrangians formula revisited

We now revisit Prop. 3.4 from the moduli space integral perspective, which we expect is better suited for generalization to compact Calabi-Yau settings. All transversality requirements of moduli spaces will be assumed, and in this sense the calculations below are formal.

In Remark 3.5 we sketched that under the extra assumption H​F−1​(L0,L0)=0HF^{-1}(L_{0},L_{0})=0, there is an (n+2)(n+2)-dimensional universal family 𝒞~\tilde{\mathcal{C}} over some nn-dimensional moduli ℳ~\tilde{\mathcal{M}}, such that the boundary of C~\tilde{C} has three (n+1)(n+1)-dimensional contributions, corresponding up to sign to the three bordism currents 𝒞1,𝒞2,𝒞3\mathcal{C}_{1},\mathcal{C}_{2},\mathcal{C}_{3} between L0,L0′,LL_{0},L_{0}^{\prime},L, which are in turn the universal families over the (n−1)(n-1)-dimensional moduli spaces ℳi\mathcal{M}_{i} for i=1,2,3i=1,2,3. Here ℳi\mathcal{M}_{i} can be viewed as certain boundary strata of the compactification of ℳ~\tilde{\mathcal{M}}. The integrand ℐ\mathcal{I} naturally makes sense as an (n−1)(n-1)-form on ℳ~\tilde{\mathcal{M}}, and restricts naturally to ℳi\mathcal{M}_{i}. The change of reference formula (22) amounts to

∫ℳ3ℐ=∫ℳ1ℐ+∫ℳ2ℐ.\int_{\mathcal{M}_{3}}\mathcal{I}=\int_{\mathcal{M}_{1}}\mathcal{I}+\int_{\mathcal{M}_{2}}\mathcal{I}. (40)

Our strategy is to use Stokes formula on the moduli spaces. As usual, the holonomy weighting factors will be suppressed in the moduli integral notations. Then (40) reduces to the two claims:

Claim 3.36.

The nn-form d​ℐ=0d\mathcal{I}=0 over the moduli space ℳ~\tilde{\mathcal{M}}.

Claim 3.37.

The Stokes boundary term is

∫ℳ~𝑑ℐ=∫ℳ1ℐ+∫ℳ2ℐ−∫ℳ3ℐ.\int_{\tilde{\mathcal{M}}}d\mathcal{I}=\int_{\mathcal{M}_{1}}\mathcal{I}+\int_{\mathcal{M}_{2}}\mathcal{I}-\int_{\mathcal{M}_{3}}\mathcal{I}.

We first explain Claim 3.36. First, we calculate the derivatives of FF. Let y1,…​yny_{1},\ldots y_{n} be local coordinates on ℳ~\tilde{\mathcal{M}}, so ∂∂yi\frac{\partial}{\partial y_{i}} can be identified as first order deformations of holomorphic curves. The local coordiates on Σ\Sigma are denoted as s,ts,t. We can write F=∑Fi​(−1)i−1​d​y1∧…d​yi⌢…​d​ynF=\sum F_{i}(-1)^{i-1}dy_{1}\wedge\ldots\stackrel{{\scriptstyle\mbox{\large$\frown$}}}{{dy_{i}}}\ldots dy_{n}, such that along Σ\Sigma,

∂sFi=(−1)i−1Ω(∂∂s,∂∂y1,…∂∂yi⌢,…∂∂yn),∂tFi=(−1)i−1Ω(∂∂t,∂∂y1,…∂∂yi⌢,…).\partial_{s}F_{i}=(-1)^{i-1}\Omega(\frac{\partial}{\partial s},\frac{\partial}{\partial y_{1}},\ldots\stackrel{{\scriptstyle\mbox{\large$\frown$}}}{{\frac{\partial}{\partial y_{i}}}},\ldots\frac{\partial}{\partial y_{n}}),\quad\partial_{t}F_{i}=(-1)^{i-1}\Omega(\frac{\partial}{\partial t},\frac{\partial}{\partial y_{1}},\ldots\stackrel{{\scriptstyle\mbox{\large$\frown$}}}{{\frac{\partial}{\partial y_{i}}}},\ldots).

The holomorphic volume form satisfies d​Ω=0d\Omega=0, whence

∑i=1n∂s∂iFi=∂s(Ω⁡(∂∂y1,…,∂∂yn)),∑i=1n∂t∂iFi=∂t(Ω⁡(∂∂y1,…,∂∂yn)).\sum_{i=1}^{n}\partial_{s}\partial_{i}F_{i}=\partial_{s}(\Omega(\frac{\partial}{\partial y_{1}},\ldots,\frac{\partial}{\partial y_{n}})),\quad\sum_{i=1}^{n}\partial_{t}\partial_{i}F_{i}=\partial_{t}(\Omega(\frac{\partial}{\partial y_{1}},\ldots,\frac{\partial}{\partial y_{n}})).

Notice Ω⁡(∂∂y1,…,∂∂yn)\Omega(\frac{\partial}{\partial y_{1}},\ldots,\frac{\partial}{\partial y_{n}}) vanishes at the corners due to the decay of the first order deformation vector fields, and comparing with the additive normalization convention on FF, we find

∑i=1n∂iFi=Ω⁡(∂∂y1,…,∂∂yn).\sum_{i=1}^{n}\partial_{i}F_{i}=\Omega(\frac{\partial}{\partial y_{1}},\ldots,\frac{\partial}{\partial y_{n}}). (41)

In particular, at all the corner points ∑i∂iFi=0\sum_{i}\partial_{i}F_{i}=0. The term f|−+f|^{+}_{-} at the corners are independent of the moduli space parameters, so the only contribution to d​ℐd\mathcal{I} comes from the Im​∫Σe−i​θ^​F​ω\text{Im}\int_{\Sigma}e^{-i\hat{\theta}}F\omega term in formula (39).

We calculate

∑i=1n∂i∫ΣFi​ω=∫Σ∑i∂iFi​ω+∫Σ∑iFi​∂iω.\sum_{i=1}^{n}\partial_{i}\int_{\Sigma}F_{i}\omega=\int_{\Sigma}\sum_{i}\partial_{i}F_{i}\omega+\int_{\Sigma}\sum_{i}F_{i}\partial_{i}\omega.

Here ∂iω\partial_{i}\omega is the Lie derivative of the symplectic form ω\omega with respect to the vector field ∂∂yi\frac{\partial}{\partial y_{i}}, which by Cartan’s formula is

∂iω=d⁡(ω⁡(∂∂yi,⋅))+ι∂∂yi​d​ω=d⁡(ω⁡(∂∂yi,⋅)).\partial_{i}\omega=d(\omega(\frac{\partial}{\partial y_{i}},\cdot))+\iota_{\frac{\partial}{\partial y_{i}}}d\omega=d(\omega(\frac{\partial}{\partial y_{i}},\cdot)).

Thus

∫Σ∑iFi​∂iω=∫∂Σ∑iFi​ω​(∂∂yi,⋅)−∫Σ∑id​Fi∧ω⁡(∂∂yi,⋅).\int_{\Sigma}\sum_{i}F_{i}\partial_{i}\omega=\int_{\partial\Sigma}\sum_{i}F_{i}\omega(\frac{\partial}{\partial y_{i}},\cdot)-\int_{\Sigma}\sum_{i}dF_{i}\wedge\omega(\frac{\partial}{\partial y_{i}},\cdot).

Notice that ∂Σ\partial\Sigma and ∂∂yi\frac{\partial}{\partial y_{i}} are both tangent to the Lagrangian boundary, so the ∂Σ\partial\Sigma integrand vanishes. We are left with

∑i=1n∂i∫ΣFi​ω=∫Σ∑i∂iFi​ω−∫Σ∑id​Fi∧ω⁡(∂∂yi,⋅)=∫ΣΩ(∂∂y1,…,∂∂yn)ω+∑i(−1)i−1ω(∂∂yi,⋅)∧Ω(⋅,∂∂y1,…∂∂yi⌢,…∂∂yn).\begin{split}&\sum_{i=1}^{n}\partial_{i}\int_{\Sigma}F_{i}\omega=\int_{\Sigma}\sum_{i}\partial_{i}F_{i}\omega-\int_{\Sigma}\sum_{i}dF_{i}\wedge\omega(\frac{\partial}{\partial y_{i}},\cdot)\\ =&\int_{\Sigma}\Omega(\frac{\partial}{\partial y_{1}},\ldots,\frac{\partial}{\partial y_{n}})\omega+\sum_{i}(-1)^{i-1}\omega(\frac{\partial}{\partial y_{i}},\cdot)\wedge\Omega(\cdot,\frac{\partial}{\partial y_{1}},\ldots\stackrel{{\scriptstyle\mbox{\large$\frown$}}}{{\frac{\partial}{\partial y_{i}}}},\ldots\frac{\partial}{\partial y_{n}}).\end{split}

Here we used the definition of FiF_{i} via ∂sFi,∂tFi\partial_{s}F_{i},\partial_{t}F_{i}, and the formula (41) for ∑i∂iFi\sum_{i}\partial_{i}F_{i}. We contract the identity ω∧Ω=0\omega\wedge\Omega=0 with ∂∂y1,…,∂∂yn\frac{\partial}{\partial y_{1}},\ldots,\frac{\partial}{\partial y_{n}}. When two ∂∂yi\frac{\partial}{\partial y_{i}} hit ω\omega, the Ω\Omega term will be contracted only (n−2)(n-2) times, which produces a (2,0)(2,0)-form vanishing identically on the holomorphic curve Σ\Sigma. When at most one ∂∂yi\frac{\partial}{\partial y_{i}} hits ω\omega, we obtain the above integrand. In effect, the integrand vanishes identically:

∑i=1n∂i∫ΣFi​ω=0,\sum_{i=1}^{n}\partial_{i}\int_{\Sigma}F_{i}\omega=0,

which then implies d​ℐ=0d\mathcal{I}=0.

We next explain Claim 3.37. In general, the compactified moduli space has many boundary strata corresponding to disc bubbling and disc splitting.

Claim 3.38.

Only the boundary strata corresponding to gluing holomorphic curves with virtual dimension 00 and n−1n-1, can have nonzero contributions to the Stokes boundary term.

To see this, we need to understand how ℐ\mathcal{I} (and notably FF) behaves near the boundary of the moduli space. Recall that when the holomorphic disc is degenerating to several disc components, then under transversality conditions, the cokernel of the extended linearized Cauchy-Riemann operator vanishes, and for small fixed gluing parameters, the kernel elements (i.e. first order deformations) are up to small perturbation obtained by gluing the kernel elements from the degenerate disc components. The perturbation effect tends to zero as we approach the moduli space boundary. Now the kernel elements from different disc components have essentially disjoint supports, so unless we have at least (n−1)(n-1) kernel elements supported on one disc component such that Ω⁡(⋅,v1,…​vn−1)\Omega(\cdot,v_{1},\ldots v_{n-1}) does not vanish identically, we will have d​F=0dF=0 for the moduli boundary strata, so that F=constF=\text{const} along Σ\Sigma, whence ℐ=0\mathcal{I}=0 by Remark 3.16. This shows Claim 3.38. We comment that this phenomenon is closely related to the fact that many moduli boundary strata do not contribute to the boundary of the bordism current 𝒞\mathcal{C} due to support reasons (cf. section 3.1).

On the boundary strata, the only contributions to the integral ℐ\mathcal{I} come from the (n−1)(n-1)-dimensional moduli spaces. The role of the holomorphic curves of virtual dimension zero, is to provide the counting factors, in a manner entirely analogous to section 3.1.2. Most contributions cancel out due to the Mauer-Cartan equation on the bounding cochains, and the closedness of the H​F0HF^{0} generators. The remaining contributions produce the RHS in Claim 3.37.

3.7.3 First variation formula revisited

We now explain how to semi-heuristically understand the first variation formula (21) as a consequence of Prop. 3.4, from the perspective of the moduli space integral formula (39). We hope this viewpoint is better suited for generalization to compact Calabi-Yau settings.

Suppose we are given a 1-parameter exact isotopy of unobstructed exact immersed Lagrangians LtL_{t}, and we wish to calculate dd​t​𝒮L0′​(Lt)\frac{d}{dt}\mathcal{S}_{L_{0}^{\prime}}(L_{t}) at t=0t=0. The change of reference Lagrangian formula (cf. Prop. 3.4) allows us to replace 𝒮L0′​(Lt)\mathcal{S}_{L_{0}^{\prime}}(L_{t}) by 𝒮L0​(Lt)\mathcal{S}_{L_{0}}(L_{t}). The Lagrangian LtL_{t} for |t|≪1|t|\ll 1 is approximately the graph of t​d​htdh in T∗​L0T^{*}L_{0} (understood in an immersed sense), for the Hamiltonian function h=ht|t=0h=h_{t}|_{t=0} on L0L_{0}. The holomorphic discs between LtL_{t} and L0L_{0} for |t|≪1|t|\ll 1 have small energy of order O⁡(|t|)O(|t|), and are locally approximated by Morse trajectories of hh. Write XhX_{h} as the Hamiltonian vector field, namely ω⁡(Xh,⋅)=d​h\omega(X_{h},\cdot)=dh, then

dd​t|t=0∫ΣFω=∫∂Σ∩L0Fω(⋅,Xh)=−∫∂Σ∩L0Fdh.\frac{d}{dt}|_{t=0}\int_{\Sigma}F\omega=\int_{\partial\Sigma\cap L_{0}}F\omega(\cdot,X_{h})=-\int_{\partial\Sigma\cap L_{0}}Fdh.

Now we examine ∑all cornersF​f|−+\sum_{\text{all corners}}Ff|^{+}_{-} for very small tt. The Lagrangian intersections come in two types:

  • •

    The corners p∈C​F0​(Lt,L0)p\in CF^{0}(L_{t},L_{0}) and q∈C​F0​(L0,Lt)q\in CF^{0}(L_{0},L_{t}) correspond to the local extrema of the Hamiltonian hh.

  • •

    Any self intersection pip_{i} between two local sheets L+,L−L_{+},L_{-} of L0L_{0} can be paired with a very nearby self intersection of pitp_{i}^{t} between two sheets L+t,L−tL_{+}^{t},L_{-}^{t} of LtL_{t}. The bounding cochain on LtL_{t} is thus induced from the bounding cochain on L0L_{0}.

At the intersection points p,qp,q,

{f|−+​(q)=fL0​(q)−fLt​(q)=−t​h​(q)+O⁡(t2),f|−+​(p)=fLt​(p)−fL0​(p)=t​h​(p)+O⁡(t2).\begin{cases}f|^{+}_{-}(q)=f_{L_{0}}(q)-f_{L_{t}}(q)=-th(q)+O(t^{2}),\\ f|^{+}_{-}(p)=f_{L_{t}}(p)-f_{L_{0}}(p)=th(p)+O(t^{2}).\end{cases}

The self intersections are usually not important here, because the smallness of energy prevents their appearance on ∂Σ\partial\Sigma, unless f|−+​(pit)=O⁡(|t|)f|^{+}_{-}(p_{i}^{t})=O(|t|), and f|−+​(pi)=0f|^{+}_{-}(p_{i})=0, which is a rather nongeneric situation. When the self intersections do appear, the evolution of the potential under exact isotopy gives

(fL+t−fL−t)​(pit)=(fL+−fL−)​(pi)+∫0t(h+,τ−h−,τ)​(piτ)​𝑑τ=f|−+​(pi)+t​h|−+​(pi)+O⁡(t2),(f_{L_{+}^{t}}-f_{L_{-}^{t}})(p_{i}^{t})=(f_{L_{+}}-f_{L_{-}})(p_{i})+\int_{0}^{t}(h_{+,\tau}-h_{-,\tau})(p_{i}^{\tau})d\tau=f|^{+}_{-}(p_{i})+th|^{+}_{-}(p_{i})+O(t^{2}),

where h±h_{\pm} keeps track of the hamiltonian on the different sheets of L0L_{0}. Thus

f|−+​(pit)=fL−t​(pit)−fL+t​(pit)=−f|−+​(pi)−t​h|−+​(pi)+O⁡(t2).f|^{+}_{-}(p_{i}^{t})=f_{L_{-}^{t}}(p_{i}^{t})-f_{L_{+}^{t}}(p_{i}^{t})=-f|^{+}_{-}(p_{i})-th|^{+}_{-}(p_{i})+O(t^{2}).

Here we have a tricky sign reversal, because if L+L_{+} and L−L_{-} are clockwise ordered on ∂Σ\partial\Sigma, then L+tL_{+}^{t} and L−tL_{-}^{t} are counterclockwise ordered. In summary,

dd​t|t=0​∑all cornersF​f|−+​(t)=limt→0{−F​h​(q)+F​h​(p)−∑L0−self intersection cornersF​h|−+​(pi)}.\frac{d}{dt}|_{t=0}\sum_{\text{all corners}}Ff|^{+}_{-}(t)=\lim_{t\to 0}\{-Fh(q)+Fh(p)-\sum_{L_{0}-\text{self intersection corners}}Fh|^{+}_{-}(p_{i})\}.

Combining the above, and integrating by parts,

dd​t|t=0​(∫ΣF​ω+∑all cornersF​f|−+​(t))=limt→0{−F​h​(q)+F​h​(p)−∑L0−cornersF​h|−+​(pi)−∫∂Σ∩L0F​dh}=limt→0{∫∂Σ∩L0h​dF}.\begin{split}&\frac{d}{dt}|_{t=0}\left(\int_{\Sigma}F\omega+\sum_{\text{all corners}}Ff|^{+}_{-}(t)\right)\\ &=\lim_{t\to 0}\{-Fh(q)+Fh(p)-\sum_{L_{0}-\text{corners}}Fh|^{+}_{-}(p_{i})-\int_{\partial\Sigma\cap L_{0}}Fdh\}\\ &=\lim_{t\to 0}\{\int_{\partial\Sigma\cap L_{0}}hdF\}.\end{split}

Observe that for very small tt, as the holomorphic curves vary in the (n−1)(n-1)-dimensional moduli spaces ℳ\mathcal{M}, under the counterclockwise sign convention for ∂Σ\partial\Sigma, the boundary evaluation of ∂Σ∩L0\partial\Sigma\cap L_{0} sweeps out the cycle L0L_{0} (beware of the sign!), and any generic point on L0L_{0} is swept out precisely once due to the Morse theory limiting description. Consequently, the moduli space integral

limt→0∫ℳ{∫∂Σ∩L0h​𝑑F}=∫L0h​Ω,\lim_{t\to 0}\int_{\mathcal{M}}\{\int_{\partial\Sigma\cap L_{0}}hdF\}=\int_{L_{0}}h\Omega,

hence

dd​t|t=0​∫ℳ(∫ΣF​ω+∑all cornersF​f|−+​(t))=∫L0h​Ω.\frac{d}{dt}|_{t=0}\int_{\mathcal{M}}\left(\int_{\Sigma}F\omega+\sum_{\text{all corners}}Ff|^{+}_{-}(t)\right)=\int_{L_{0}}h\Omega.

By the moduli integral formula (39) of the Solomon functional,

dd​t|t=0​𝒮​(Lt)=dd​t|t=0​∫ℳℐ=∫L0h​Im​(e−i​θ^​Ω).\frac{d}{dt}|_{t=0}\mathcal{S}(L_{t})=\frac{d}{dt}|_{t=0}\int_{\mathcal{M}}\mathcal{I}=\int_{L_{0}}h\text{Im}(e^{-i\hat{\theta}}\Omega).

This recovers the first variation formula (21).

3.7.4 Speculations on compact Calabi-Yau manifolds

Floer theoretic foundations are much more complicated beyond the exact setting, and the foundations concerning the open-closed string map in the immersed Fukaya category setting are not fully written out in the literature. Nonetheless, due to the interest of the topic, we shall offer some speculations about how the Solomon functional formula (39) generalizes to the compact almost Calabi-Yau setting. Our local systems will have coefficients in ℝ,ℚ\mathbb{R},\mathbb{Q}, i.e. the parallel transport in the local system have only Novikov exponent zero components. This convention is somewhat more restrictive than [7][81][82].

Remark 3.18.

In Joyce’s LMCF, bounding cochains and local systems can be created ex nihilo during the flow, but in all the mechanisms the author is aware of, the flow preserves the above class of local systems.

First, we recall the role of Novikov coefficients in Floer theory. All Floer cochain spaces C​F∗CF^{*} are modules over the Novikov field

Λ={∑iaiTλi:λi∈ℝ,λ1<λ2<…→+∞},\Lambda=\{\sum_{i}a_{i}T^{\lambda_{i}}:\quad\lambda_{i}\in\mathbb{R},\lambda_{1}<\lambda_{2}<\ldots\to+\infty\},

and ai∈ℚa_{i}\in\mathbb{Q} or ℝ\mathbb{R} depending on the coefficient field choice.4343 43 We do not know if the Fukaya category can be defined over integers in general. One should not confuse the coefficients aia_{i} with the Novikov exponents λi\lambda_{i}. Typically aia_{i} are rational numbers related to counting, while λi\lambda_{i} are real numbers related to the energy. There are a few conventions to define A∞A_{\infty}-operations. Let LL be a compact immersed Lagrangian with transverse self intersections. In the Morse model [81], the self Floer cochain space C​F∗​(L,L)CF^{*}(L,L) is generated by the Morse critical points on LL, and the ordered self intersections (twisted by local system hom and orientation factors as usual). The Fukaya A∞A_{\infty}-algebra is a collection of Novikov-multilinear operations

mk:C​F∗​(L,L)⊗…​C​F∗​(L,L)→C​F∗​(L,L)​[2−k]m_{k}:CF^{*}(L,L)\otimes\ldots CF^{*}(L,L)\to CF^{*}(L,L)[2-k]

defined by counting holomorphic treed discs u:Σ→Xu:\Sigma\to X (cf. [81, Definition 3.1]), weighted by the holonomy and orientation factors, and an energy factor TE⁡(u)T^{E(u)}. Very roughly, the domain Σ\Sigma have surface parts (which consist of discs, and spheres attached to them), and tree parts connecting the disc boundaries. Then uu is a holomorphic map with Lagrangian boundary on the surface parts, and Morse gradient flowlines on the tree parts. The role of C​F∗CF^{*} elements is to specify the limiting behaviour of the Morse flowlines, and the Lagrangian self intersections on ∂Σ\partial\Sigma. The energy E⁡(u)=∫ΣωE(u)=\int_{\Sigma}\omega is the sum of ∫u∗​ω\int u^{*}\omega on all the surface parts of Σ\Sigma.

A nontrivial fact is that (after complicated perturbation schemes, or virtual techniques) this gives rise to a curved A∞A_{\infty}-algebra structure [81]. The most important new feature, absent in the exact case, is that the disc bubbling can occur at points of LL, which are not necessarily self intersection points. The domain disc splits into two discs, attached at a boundary node. This phenomenon is compensated by considering two discs joined by a gradient flowline segment, whose length shrinks to zero, producing the same nodal discs in the degeneration limit. With the appropriate weights and orientations taken into account, these two effects would cancel algebraically. On the other hand, the length parameter of the tree parts can tend to infinity, causing the Morse gradient flow line to break, a phenomenon which contributes to the boundary of the one dimensional moduli spaces, reflected algebraically in the A∞A_{\infty}-relations.

Similar to the exact immersed case (cf. Appendix 6.2), the bounding cochains are b∈C​F1​(L,L)b\in CF^{1}(L,L) elements satisfying the nonnegative Novikov exponent requirement, and the Mauer-Cartan equation

m0+m1​(b)+m2​(b,b)+…=0.m_{0}+m_{1}(b)+m_{2}(b,b)+\ldots=0.

Generally speaking, the sum is infinite, but after truncating the Novikov series at any given high energy, only finitely many terms appear due to Gromov compactness, so the sum makes formal sense. As usual, the Lagrangian with bounding cochain structures are called unobstructed.

The framework for setting up the Fukaya algebra of a single immersed Lagrangian, also assigns meanings to Floer cohomologies between two immersed Lagrangians with bounding cochain structures. Suppose α∈C​F0​(L,L′)\alpha\in CF^{0}(L,L^{\prime}) and β∈C​F0​(L′,L)\beta\in CF^{0}(L^{\prime},L) represent elements in H​F0​(L,L′)HF^{0}(L,L^{\prime}) and H​F0​(L′,L)HF^{0}(L^{\prime},L) whose cohomological compositions are the identities. The α,β\alpha,\beta are in generally represented by infinite series in the Novikov variable TT, where some Novikov exponents may be negative, and may bot be bounded above, but at least they are bounded from below depending on α,β\alpha,\beta. We now speculate that there is a bordism current 𝒞\mathcal{C} with ∂𝒞=L−L′\partial\mathcal{C}=L-L^{\prime}, constructed from the universal families of treed holomorphic discs over the (n−1)(n-1)-dimensional moduli spaces ℳ\mathcal{M}. The monomial summands of α,β\alpha,\beta and the bounding cochain elements prescribe the corners of the treed holomorphic discs, and monomials with different Novikov exponents are viewed as independent contributions to ℳ\mathcal{M} and 𝒞\mathcal{C}. Beyond the almost calibrated case, one would also need to incorporate degree −1-1 self intersections as usual. We think the moduli spaces that contribute to 𝒞\mathcal{C} would satisfy the Novikov exponent condition

∫Σω+∑all cornersNovikov exponent=0.\int_{\Sigma}\omega+\sum_{\text{all corners}}\text{Novikov exponent}=0. (42)

Here the corners include the monomial summands of α,β\alpha,\beta (or the degree −1-1 self intersections as appropriate), and the bounding cochains at the degree one self intersections/Morse critical points of L,L′L,L^{\prime}. Since all Novikov exponents at the bounding cochains are non-negative (not so at α,β\alpha,\beta, and the degree −1-1 self intersections!), this condition would impose an energy upper bound on the holomorphic treed discs depending on α,β\alpha,\beta, whence only finitely many moduli spaces contribute to the bordism current.

Remark 3.19.

The Novikov exponents correspond to f|−+f|^{+}_{-} in the exact case. While in the exact case (42) is an automatic consequence of the energy identity (66), in general it is an extra condition on the moduli spaces. It sits well with the fact that the geometric unit has zero Novikov exponent.

Now the moduli space integral formula (39) formally makes sense almost verbatim, ignoring all virtual perturbation nuances. For first order deformations v1,…​vn−1v_{1},\ldots v_{n-1} of the holomorphic treed discs, we can define FF on the domain Σ\Sigma via the 1-form d​F=Ω⁡(⋅,v1,…​vn−1)dF=\Omega(\cdot,v_{1},\ldots v_{n-1}). On the surface parts of Σ\Sigma, we would obtain a holomorphic function FF by complex integrability as usual (which must be constant on the holomorphic sphere components by the Liouville theorem), while on the tree parts, there is no obstruction for the 1-form to be exact. Next, we replace the appearance of f|−+f|^{+}_{-} in (39) by the Novikov exponents of the monomial summands at the corners, to define the moduli integrand ℐ\mathcal{I}. The term ∫ΣF​ω\int_{\Sigma}F\omega is understood to only involve integration on the surface parts of Σ\Sigma. The Solomon functional 𝒮⁡(L)\mathcal{S}(L) still has the form ∫ℳℐ\int_{\mathcal{M}}\mathcal{I}. Notice that adding a constant to FF would not change the moduli integrand ℐ\mathcal{I}, thanks to (42).

In the absence of the Lagrangian potential, the Novikov exponents of α,β\alpha,\beta are no longer canonically fixed. Suppose we replace α\alpha by Tμ​αT^{\mu}\alpha, and β\beta by T−μ​βT^{-\mu}\beta, for some μ∈ℝ\mu\in\mathbb{R}. This would affect the moduli integrand ℐ\mathcal{I}, by the amount

μ​Im​{e−i​θ^​(F⁡(p)−F⁡(q))},\mu\text{Im}\{e^{-i\hat{\theta}}(F(p)-F(q))\},

where p,qp,q stand for the components of α,β\alpha,\beta. By analogy with the exact case, we expect

Im​(e−i​θ^​∫ℳF⁡(p)−F⁡(q))=Im​(e−i​θ^​∫LΩ)=0,\text{Im}\left(e^{-i\hat{\theta}}\int_{\mathcal{M}}F(p)-F(q)\right)=\text{Im}\left(e^{-i\hat{\theta}}\int_{L}\Omega\right)=0,

whence 𝒮⁡(L)\mathcal{S}(L) is independent of μ\mu.

Once the foundations are in place, we expect

Conjecture 3.39.

Fix a compact almost Calabi-Yau manifold XX. The Solomon functional is well defined for graded immersed unobstructed Lagrangians in the same Db​F​u​k​(X)D^{b}Fuk(X) class of a reference Lagrangian L0L_{0}, satisfying

  • •

    The change of reference Lagrangian formula (22) holds,

  • •

    Gauge equivalent bounding cochains give rise to the same functional,

  • •

    Cohomologous choices of H​F0HF^{0} generators α,β\alpha,\beta give rise to the same functional,

  • •

    The first variation formula (21) holds for any 1-parameter exact isotopy of unobstructed Lagrangians.

The slogan is that Floer theory should fix the multivaluedness problem of the Solomon functional (cf. section 2.8). As a more technical observation, once the change of reference Lagrangian formula (22) is established, one can remove the assumption for LL to be transverse to L0L_{0}, using a perturbation L0′L_{0}^{\prime} of L0L_{0}.

3.8 More applications of moduli space integrals

We collect a number of further topics involving the moduli space integral technique. Sections 3.8.2 and 3.8.3 are applications of the moduli integral formula (39) for the Solomon functional.

3.8.1 Lotay-Pacini convexity

Lotay and Pacini proved the convexity of their JJ-functional (cf. Prop. 2.13) through rather heavy calculations, so it is instructive to see that in the Calabi-Yau case, this result has a much simpler conceptual argument.

We interpret their ‘geodesic’ as a bordism current 𝒞\mathcal{C} between two Lagrangians L,L′L,L^{\prime}, constructed from universal families of holomorphic curves, such that automatic transversality and the positivity condition hold. In their highly idealized setting, only holomorphic strips Σ≃ℝs×[0,1]t\Sigma\simeq\mathbb{R}_{s}\times[0,1]_{t} appear in the construction of 𝒞\mathcal{C}. We define the holomorphic function FF as usual. The 1-parameter family of totally real submanifolds is given by the constant tt-coordinate slices 𝒞t\mathcal{C}_{t} of 𝒞\mathcal{C}, whose JJ-volume functional is expressible through moduli space integrals

VolJ​(𝒞t)=∫𝒞t|Ω|=∫ℳ∫ℝs×{t}|∂F∂s|​𝑑s.\text{Vol}_{J}(\mathcal{C}_{t})=\int_{\mathcal{C}_{t}}|\Omega|=\int_{\mathcal{M}}\int_{\mathbb{R}_{s}\times\{t\}}|\frac{\partial F}{\partial s}|ds.

Since FF is holomorphic, so is ∂F∂s\frac{\partial F}{\partial s}, whence |∂F∂s||\frac{\partial F}{\partial s}| is subharmonic, which combined with the exponential decay at s→±∞s\to\pm\infty implies the convexity of the function in tt

∫ℝs×{t}|∂F∂s|​𝑑s.\int_{\mathbb{R}_{s}\times\{t\}}|\frac{\partial F}{\partial s}|ds.

Thus VolJ​(𝒞t)\text{Vol}_{J}(\mathcal{C}_{t}) is convex as a function of tt, as Lotay and Pacini observed.

3.8.2 Lower bound of the Solomon functional

The theme of Chapter 5 will be on the variational approach to find special Lagrangians by minimizing the Solomon functional in a fixed derived category class. As an important motivation, special Lagrangians are formal local minimizers of the Solomon functional under Hamiltonian deformations (cf. section 2.8). In fact we can do better under the automatic transversality and the positivity condition:

Proposition 3.40.

(‘special Lagrangians are minimizers’) Suppose L0L_{0} is an exact immersed special Lagrangian of phase θ^∈(−π2,π2)\hat{\theta}\in(-\frac{\pi}{2},\frac{\pi}{2}), with unobstructed bounding cochain structure. Let LL be an almost calibrated, exact, immersed Lagrangian in the same Db​F​u​k​(X)D^{b}Fuk(X) class, which intersects L0L_{0} transversely. Suppose the bordism current 𝒞\mathcal{C} with ∂𝒞=L−L0\partial\mathcal{C}=L-L_{0} satisfies automatic transversality and the positivity condition. Then 𝒮⁡(L)≥𝒮⁡(L0)\mathcal{S}(L)\geq\mathcal{S}(L_{0}).

Proof.

The incline angle of the tangent vector to F⁡(∂Σ)⊂ℂF(\partial\Sigma)\subset\mathbb{C} is equal to the Lagrangian angle modulo π​ℤ\pi\mathbb{Z}. Since L0L_{0} is a special Lagrangian, along the L0L_{0} boundary portion arg⁡F=θ^\arg F=\hat{\theta}. Thus Im​(e−i​θ^​F)=0\text{Im}(e^{-i\hat{\theta}}F)=0 at p,qp,q and the self intersections on L0L_{0}. The Solomon functional integrand simplifies to

Im​∫Σe−i​θ^​F​ω+∑L-self intersections on ∂ΣIm​(e−i​θ^​F)​fL|−+.\text{Im}\int_{\Sigma}e^{-i\hat{\theta}}F\omega+\sum_{\text{$L$-self intersections on $\partial\Sigma$}}\text{Im}(e^{-i\hat{\theta}}F)f_{L}|^{+}_{-}.

By the almost calibrated assumption on L,L0L,L_{0}, and the positivity condition, we obtain Claim 3.23, namely F⁡(Σ)F(\Sigma) lies above its L0L_{0} boundary,

Im​(e−i​θ^​F)≥0on ​Σ.\text{Im}(e^{-i\hat{\theta}}F)\geq 0\quad\text{on }\Sigma.

Morever, the Novikov positivity requirement for the bounding cochain on LL says that fL|−+≥0f_{L}|^{+}_{-}\geq 0 at the degree one self intersections on ∂Σ∩L\partial\Sigma\cap L. Thus the Solomon functional integrand is nonnegative, which implies 𝒮⁡(L)≥0=𝒮⁡(L0)\mathcal{S}(L)\geq 0=\mathcal{S}(L_{0}). ∎

Remark 3.20.

Suppose we drop the positivity condition, then the key step Im​(e−i​θ^​F)≤0\text{Im}(e^{-i\hat{\theta}}F)\leq 0 would break down, so the above proof of Prop. 3.40 would be invalidated. However, the conclusion may still be true (cf. section 5.7.1).

3.8.3 Bounded part of the Solomon functional

Let L,L0L,L_{0} be both exact, immersed Lagrangians with unobstructed bounding cochain structures, lying in the same Db​F​u​k​(X)D^{b}Fuk(X) class, such that all intersections are transverse. Assume the bordism current 𝒞\mathcal{C} with ∂𝒞=L−L0\partial\mathcal{C}=L-L_{0} satisfies automatic transversality and the positivity condition. We consider L0L_{0} as a fixed reference Lagrangian, while LL can vary. We wish to find uniform a priori bound on certain parts of the Solomon functional, under natural conditions on LL.

We shall assume:

  • •

    (Quantitative almost calibratedness) Both LL and L0L_{0} have Lagrangian phase angles within [−π2+ϵ,π2−ϵ][-\frac{\pi}{2}+\epsilon,\frac{\pi}{2}-\epsilon] for some fixed small constant ϵ\epsilon.

  • •

    (Potential clustering, cf. Lemma 6.3) The immersed Lagrangian LL can be represented by a twisted complex (17) built from the immersed Lagrangians L1,…​LNL_{1},\ldots L_{N}, such that the oscillation of the Lagrangian potentials have uniform bounds

    supLifLi−infLifLi≤A,\sup_{L_{i}}f_{L_{i}}-\inf_{L_{i}}f_{L_{i}}\leq A,

    while for any i>ji>j,

    supLjfLj≤infLifLi.\sup_{L_{j}}f_{L_{j}}\leq\inf_{L_{i}}f_{L_{i}}.

    Without loss of generality, we also assume supL0fL0−infL0fL0≤A\sup_{L_{0}}f_{L_{0}}-\inf_{L_{0}}f_{L_{0}}\leq A for the fixed Lagrangian L0L_{0}.

Proposition 3.41.

(Uniform energy bound) Under the potential clustering assumption, all holomorphic polygons u:Σ→Xu:\Sigma\to X with boundary on LL and L0L_{0} contributing to 𝒞\mathcal{C} have uniformly bounded energy independent of LL:

E⁡(u)=∫Σu∗​ω≤A⁡(N+1),E(u)=\int_{\Sigma}u^{*}\omega\leq A(N+1),

and along ∂Σ\partial\Sigma the degree one self intersections of L0,L1,…​LNL_{0},L_{1},\ldots L_{N} arising from the bounding cochains satisfy a uniform bound

∑i∑bifLi|−+​(bi)≤A⁡(N+1).\sum_{i}\sum_{b_{i}}f_{L_{i}}|^{+}_{-}(b_{i})\leq A(N+1).
Proof.

We consider holomorphic polygons whose boundary ∂Σ\partial\Sigma encounters in the clockwise order intersections in pN−1∈C​F1​(LN,LN−1),…p_{N-1}\in CF^{1}(L_{N},L_{N-1}),\ldots, p1∈C​F1​(L2,L1)p_{1}\in CF^{1}(L_{2},L_{1}), p0∈C​F0​(L1,L0)p_{0}\in CF^{0}(L_{1},L_{0}), pN∈C​F0​(L0,LN)p_{N}\in CF^{0}(L_{0},L_{N}), juxaposed possibly by more degree one self intersections bib_{i} of LiL_{i}. The notation here does not constrain the number of self intersections of LiL_{i} that can occur on ∂Σ\partial\Sigma. The topological energy formula (66) expresses E⁡(u)E(u) in terms of the Lagrangian potentials at the intersections

E⁡(u)+∑i∑bifLi|−+​(bi)=fLN​(pN)−fL0​(pN)+∑i=0N−1(fLi−fLi+1)​(pi)=fL0​(p0)−fL0​(pN)+∑i=1N(fLi​(pi)−fLi​(pi−1))≤(N+1)​A.\begin{split}&E(u)+\sum_{i}\sum_{b_{i}}f_{L_{i}}|^{+}_{-}(b_{i})\\ &=f_{L_{N}}(p_{N})-f_{L_{0}}(p_{N})+\sum_{i=0}^{N-1}(f_{L_{i}}-f_{L_{i+1}})(p_{i})\\ &=f_{L_{0}}(p_{0})-f_{L_{0}}(p_{N})+\sum_{i=1}^{N}(f_{L_{i}}(p_{i})-f_{L_{i}}(p_{i-1}))\\ &\leq(N+1)A.\end{split}

By the Novikov positivity requirement of the bounding cochains fLi|−+​(bi)≥0f_{L_{i}}|^{+}_{-}(b_{i})\geq 0, and the energy of the holomorphic curve is also positive, so they are individually bounded.

More generally, the polygons may miss some of the Lagrangians in L1,…​LNL_{1},\ldots L_{N}, but cannot reverse the order of the Lagrangians. This amounts to using a smaller effective value NN, and the same argument implies the energy bound. ∎

We now consider the holomorphic function FF as before. Recall by Claim 3.22 we have 0≤Re ​(F)≤Re ​F​(p)0\leq\text{Re }(F)\leq\text{Re }F(p), where pp is the intersection point in C​F0​(L,L0)CF^{0}(L,L_{0}). In fact F⁡(Σ)F(\Sigma) must be contained in a triangular region determined by Re ​F​(p)\text{Re }F(p):

Lemma 3.42.

(Wedge region bound) Under the quantitative almost calibrated hypothesis, we have |arg⁡F|≤π2−ϵ|\arg F|\leq\frac{\pi}{2}-\epsilon, or equivalently |Im​(F)|≤(cot⁡ϵ)​Re ​(F).|\text{Im}(F)|\leq(\cot\epsilon)\text{Re }(F). In particular |F|≤1sin⁡ϵ​Re ​F≤1sin⁡ϵ​Re ​F​(p).|F|\leq\frac{1}{\sin\epsilon}\text{Re }F\leq\frac{1}{\sin\epsilon}\text{Re }F(p).

Proof.

The incline angle of the tangent vector of F⁡(∂Σ)F(\partial\Sigma) is equal to the Lagrangian angle mod π​ℤ\pi\mathbb{Z}. Together with Claim 3.22 this implies |arg⁡F|≤π2−ϵ|\arg F|\leq\frac{\pi}{2}-\epsilon on the ∂Σ\partial\Sigma, whence the same bound holds on Σ\Sigma by the maximum principle for holomorphic functions. ∎

We now introduce an elementary functional

𝒮¯​(L)=Im​(∑1N(supLifLi)​e−i​θ^​∫LiΩ)−(supL0fL0)​Im​(e−i​θ^​∫L0Ω).\bar{\mathcal{S}}(L)=\text{Im}\left(\sum_{1}^{N}(\sup_{L_{i}}f_{L_{i}})e^{-i\hat{\theta}}\int_{L_{i}}\Omega\right)-(\sup_{L_{0}}f_{L_{0}})\text{Im}(e^{-i\hat{\theta}}\int_{L_{0}}\Omega). (43)

As in section 3.5, we introduce complex valued volume form Ω~Li\tilde{\Omega}_{L_{i}} on the (n−1)(n-1)-dimensional moduli spaces of holomorphic curves, whose core properties are

Re Ω~Li≥0,∫ℳΩ~Li=∫LiΩ,i=0,1,…N.\text{Re }\tilde{\Omega}_{L_{i}}\geq 0,\quad\int_{\mathcal{M}}\tilde{\Omega}_{L_{i}}=\int_{L_{i}}\Omega,\quad i=0,1,\ldots N. (44)

Thus the elementary functional is also a moduli space integral, with integrand

Im​∑1N(e−i​θ^​Ω~Lj)​supfLj−Im​(e−i​θ^​Ω~L0)​supfL0.\text{Im}\sum_{1}^{N}(e^{-i\hat{\theta}}\tilde{\Omega}_{L_{j}})\sup f_{L_{j}}-\text{Im}(e^{-i\hat{\theta}}\tilde{\Omega}_{L_{0}})\sup f_{L_{0}}. (45)

We decompose the Solomon functional into 𝒮¯​(L)\bar{\mathcal{S}}(L) and 𝒮​(L)−𝒮¯​(L)\mathcal{S}(L)-\bar{\mathcal{S}}(L).

Theorem 3.43.

(Bounded part of the Solomon functional) Under the quantitative almost calibratedness and the potential clustering assumption, and all the standing assumptions of this section, there is a uniform a priori bound independent of LL,

|𝒮⁡(L)−𝒮¯​(L)|≤A⁡(4​N+2)sin⁡ϵ​∫L0Re ​Ω.|\mathcal{S}(L)-\bar{\mathcal{S}}(L)|\leq\frac{A(4N+2)}{\sin\epsilon}\int_{L_{0}}\text{Re }\Omega.
Proof.

We analyze the moduli space integrand (39) of the Solomon functional. Applying the uniform energy bound and the wedge region bound, the first term is bounded by

|Im​∫Σe−i​θ^​F​ω|≤∫Σ|F|​ω≤Re​(F​(p))sin⁡ϵ​∫Σω≤Re​(F​(p))sin⁡ϵ​A​(N+1).|\text{Im}\int_{\Sigma}e^{-i\hat{\theta}}F\omega|\leq\int_{\Sigma}|F|\omega\leq\frac{\text{Re}(F(p))}{\sin\epsilon}\int_{\Sigma}\omega\leq\frac{\text{Re}(F(p))}{\sin\epsilon}A(N+1).

More intrinsically F⁡(p)F(p) defines the complex valued volume form Ω~L0\tilde{\Omega}_{L_{0}} on the moduli space, hence

|Im​∫Σe−i​θ^​F​ω|≤1sin⁡ϵ​A​(N+1)​Re​(Ω~L0).|\text{Im}\int_{\Sigma}e^{-i\hat{\theta}}F\omega|\leq\frac{1}{\sin\epsilon}A(N+1)\text{Re}(\tilde{\Omega}_{L_{0}}). (46)

The other two terms in (39) are rewritten as a sum of contributions from intersection points in (38). As in Prop. 3.41, we consider holomorphic polygons whose boundary ∂Σ\partial\Sigma encounters in the clockwise order pN−1∈C​F1​(LN,LN−1),…p_{N-1}\in CF^{1}(L_{N},L_{N-1}),\ldots, p1∈C​F1​(L2,L1)p_{1}\in CF^{1}(L_{2},L_{1}), p=p0∈C​F0​(L1,L0)p=p_{0}\in CF^{0}(L_{1},L_{0}), q=pN∈C​F0​(L0,LN)q=p_{N}\in CF^{0}(L_{0},L_{N}) juxaposed possibly by more degree one self intersections bib_{i} of LiL_{i}. (The other cases, where ∂Σ\partial\Sigma misses some Lagrangians, can be handled completely similarly.) We first deal with these extra self intersections. Using the wedge region bound, and the Novikov positivity requirement,

|Im​∑i∑bie−i​θ^​F​fLi|−+​(bi)|≤∑i∑bi|F⁡(bi)|​fLi|−+​(bi)≤Re​(F​(p))sin⁡ϵ​∑i∑bifLi|−+​(bi).|\text{Im}\sum_{i}\sum_{b_{i}}e^{-i\hat{\theta}}Ff_{L_{i}}|^{+}_{-}(b_{i})|\leq\sum_{i}\sum_{b_{i}}|F(b_{i})|f_{L_{i}}|^{+}_{-}(b_{i})\leq\frac{\text{Re}(F(p))}{\sin\epsilon}\sum_{i}\sum_{b_{i}}f_{L_{i}}|^{+}_{-}(b_{i}).

By Lemma 3.41, we have

|Im​∑i∑bie−i​θ^​F​fLi|−+​(bi)|≤1sin⁡ϵ​A​(N+1)​Re​(Ω~L0).|\text{Im}\sum_{i}\sum_{b_{i}}e^{-i\hat{\theta}}Ff_{L_{i}}|^{+}_{-}(b_{i})|\leq\frac{1}{\sin\epsilon}A(N+1)\text{Re}(\tilde{\Omega}_{L_{0}}). (47)

We are left with the contributions of p0,p1,…​pNp_{0},p_{1},\ldots p_{N} to (38):

Im​∑0N−1e−i​θ^​F​(fLj+1−fLj)​(pj).\text{Im}\sum_{0}^{N-1}e^{-i\hat{\theta}}F(f_{L_{j+1}}-f_{L_{j}})(p_{j}).

If we replace fLif_{L_{i}} by its supremum value supLifLi\sup_{L_{i}}f_{L_{i}} for all i=0,1,…​Ni=0,1,\ldots N, the new expression would be

Im​∑0N−1e−i​θ^​F​(pj)​(supfLj+1−supfLj)=Im​∑1Ne−i​θ^​supfLj​(F⁡(pj−1)−F⁡(pj))−Im​(e−i​θ^​F​(p)​supfL0)\begin{split}&\text{Im}\sum_{0}^{N-1}e^{-i\hat{\theta}}F(p_{j})(\sup f_{L_{j+1}}-\sup f_{L_{j}})\\ =&\text{Im}\sum_{1}^{N}e^{-i\hat{\theta}}\sup f_{L_{j}}(F(p_{j-1})-F(p_{j}))-\text{Im}(e^{-i\hat{\theta}}F(p)\sup f_{L_{0}})\end{split}

which is more intrinsically the integrand (45) of the elementary functional. Using the potential clustering assumption and the wedge region bound lemma, the error of replacing the potentials by supLjfLj\sup_{L_{j}}f_{L_{j}} can be bounded by

2​A​∑1N|F⁡(pj)|≤2​A​N​Re​(F​(p))sin⁡ϵ=2​A​Nsin⁡ϵ​Re​(Ω~L0).2A\sum_{1}^{N}|F(p_{j})|\leq 2AN\frac{\text{Re}(F(p))}{\sin\epsilon}=\frac{2AN}{\sin\epsilon}\text{Re}(\tilde{\Omega}_{L_{0}}). (48)

Now (46)(47)(48) are upper bounds on the three contributions to the difference between the Solomon functional integrand (39) and the elementary functional integrand. Their sum is bounded by

A⁡(4​N+2)sin⁡ϵ​Re​(Ω~L0),\frac{A(4N+2)}{\sin\epsilon}\text{Re}(\tilde{\Omega}_{L_{0}}),

so after integration on the moduli space,

|𝒮⁡(L)−𝒮¯​(L)|≤A⁡(4​N+2)sin⁡ϵ​∫L0Re ​Ω|\mathcal{S}(L)-\bar{\mathcal{S}}(L)|\leq\frac{A(4N+2)}{\sin\epsilon}\int_{L_{0}}\text{Re }\Omega

as required. ∎

Remark 3.21.

In section 5.2 below we will deduce the potential clustering and an upper bound on NN as consequences of almost quantitative calibratedness, and very mild conditions on the ambient manifold XX. In section 5.5 the boundedness of |𝒮−𝒮¯||\mathcal{S}-\bar{\mathcal{S}}| will be essential for relating the asymptote of the Solomon functional to stability conditions.

Remark 3.22.

In Kähler geometry, it is often useful to decompose natural functionals into two parts. For instance, the K-energy functional can be decomposed into an entropy part and a pluripotential part [17, section 2.4], which is important in the study of constant scalar curvature Kähler metrics.

Remark 3.23.

We suggested in section 2.10 that the Solomon functional is essentially the logarithm of the tunneling amplitude between Lagrangian branes. Pushing forth with this physics analogy, we may regard the elementary functional as a semiclassical approximation,4444 44 The elementary functional is proportional to the period integrals over the cycles LiL_{i}, which may be regarded as coming from integration over the moduli of constant maps. Such integrals are regarded as more classical then those involving nontrivial holomorphic curves. and 𝒮−𝒮¯\mathcal{S}-\bar{\mathcal{S}} as quantum fluctuation effects. Our main assertion then becomes that quantitative almost calibratedness with some extra hypotheses imply the a priori bound on the quantum fluctuation effects. The author is not aware of previous suggestions in the physics literature, but Jake Solomon’s formal Riemannian picture in section 2.8 may offer partial explanations for the relevance of the almost calibrated condition.

What if we relax the positivity condition?

Suppose we drop the positivity condition on the bordism current, but keep all the other assumptions. Then the key difference is that for holomorphic curves contributing negatively to ∂𝒞\partial\mathcal{C}, we need to replace Claim 3.22 by Claim 3.29, and Claim 3.23 by Claim 3.30. Correspondingly, all appearance of Re ​F​(p)\text{Re }F(p) is replaced by its absolute value. Then the conclusion in Theorem 3.43 is replaced by

|𝒮⁡(L)−S¯​(L)|≤A⁡(4​N+2)sin⁡ϵ​∫ℳ|Re ​Ω~L0|.|\mathcal{S}(L)-\bar{S}(L)|\leq\frac{A(4N+2)}{\sin\epsilon}\int_{\mathcal{M}}|\text{Re }\tilde{\Omega}_{L_{0}}|. (49)

The problem is that the RHS is no longer a manefestedly a priori bounded quantity.

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