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3 Gauge equivalence and moment maps [0583]

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3 Gauge equivalence and moment maps

In fact what Joyce is proposing to count is special Lagrangian spheres with flat line bundles on them (hence the otherwise anomalous dependence on the complex structure), while [T1] counts stable bundles (i.e. by Donaldson-Uhlenbeck-Yau, modulo the technicalities of polystable and non-locally-free sheaves, we count Hermitian-Yang-Mills connections; hence the dependence on the Kähler form). (Tyurin [Ty] was perhaps the first to suggest that the holomorphic Casson invariant should be related by mirror symmetry to the real Casson invariant (here the U⁡(1)U(1) Casson invariant) of SLag submanifolds.)

The link should be, of course, that we want to consider holomorphic connections on one side, up to complex gauge equivalence, and Lagrangians on the other side, up to hamiltonian isotopy, and in both cases we try to do this by picking distinguished representatives of equivalence classes by the usual method of symplectic reduction. Bringing in a Kähler structure on the complex side, we get a moment map for the gauge group action, whose zeros give the HYM equations. Dually, we would like to bring in the holomorphic 3-form on the symplectic (Kähler) side, and get a complex group to act. So again complexify by adding flat line bundles: consider the critical points of the functional ff of the last section, i.e. the space

𝒵={(L,A):L⊂WisLagrangian,AisaflatconnectiononL}\mathcal{Z}=\{(L,A)\,:\,L\subset W\mathrm{\ is\ Lagrangian,\ }A\mathrm{\ is\ a\ flat\ connection\ on\ }L\,\}

(not up to gauge equivalence). In fact consider this space on a Calabi-Yau manifold WW of any dimension nn. It has tangent space

T(L,A)​𝒵=Z1​(L)⊕Z1​(L)T_{(L,A)}\mathcal{Z}=Z^{1}(L)\oplus Z^{1}(L)

(Z1​(L)Z^{1}(L) denotes closed real one-forms on LL), the first being tangent to the space of flat connections, the second giving normal vector fields (by contracting with ω−1\omega^{-1}) preserving the Lagrangian condition. We have an obvious almost complex structure

J=(01−10).J=\left(\begin{array}[]{cc}0&1\\ -1&0\end{array}\right). (3.1)

Then the real group C∞​(L,ℝ)/ℝC^{\infty}(L;\mathbb{R})/\mathbb{R} acts as the Lie algebra to the group of gauge transformations on the flat line bundles (taking dd and adding to the connection) whose complexification C∞​(L,ℂ)/ℂC^{\infty}(L;\mathbb{C}\,)/\mathbb{C}\, acts complex linearly: the imaginary part C∞​(L,ℝ)/ℝC^{\infty}(L;\mathbb{R})/\mathbb{R} acts by hamiltonian deformations through the normal vector field

h↦d​h​ ​_∣ω−1.h\mapsto dh{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1}.

Unfortunately, without using a metric this vector field is only defined up to the addition of tangent vector fields to LL; the map (2.2) is really a map to (TW|L)/TL(TW\arrowvert_{L})/TL which we have lifted to TW|LTW\arrowvert_{L} using the metric. (Equivalently we can extend hh to a first formal neighbourhood of LL in different ways to get a different vector field.) How we pick this alters how we carry the flat connection along with LL, and how the almost complex structure (3.1) acts. For instance suppose we are in the rather artificial case of LL being transverse to an SYZ TnT^{n}-fibration. Then we can carry LL and the flat connection up the fibres and identify the functions C∞​(L)C^{\infty}(L) from Lagrangian to Lagrangian using the projection. Thus the group remains constant as LL moves (effectively what we are doing is extending functions from LL to a neighbourhood of LL in WW by pulling up along the SYZ fibres). This does not work when LL branches over the base of such a fibration. One can instead use the metric to define normal vector fields, but then identifying the Lie algebra C∞​(L)C^{\infty}(L) with a fixed C∞​(L0)C^{\infty}(L_{0}) for all LL becomes difficult.

This problem is perhaps not so surprising – the moment the Lagrangian has branching over the base of an SYZ fibration simple explicit correspondences between Lagrangians and vector bundles (such as [LYZ]) also break down due to our ignoring important holomorphic disc instanton corrections that appear in the physics. For instance recent work of Fukaya, Oh, Ohta and Ono [FO3], surveyed in [Fu1], show these provide the obstructions mirror to those of deformations of holomorphic bundles [T2] – one should not in general consider all (S)Lags (which are unobstructed) as mirror to holomorphic bundles, but only those whose Floer cohomology (whose definition involves holomorphic discs) is well defined.

However, what is clear is the totality of the group action, even if identifying individual elements causes problems, and this is all we really need. For instance in the K​3K3 (or T4T^{4}) case one can get the same total group orbit, with a genuine fixed group acting, by hyperkähler rotating a construction due to Donaldson [D]. The end result is that one considers parametrised Lagrangian embeddings ff from a Riemann surface LL into the K​3K3 such that the pullback of ReΩ\,\Omega is a fixed symplectic form on LL. Then the group of exact symplectomorphisms of

(L,f∗​Re​Ω)(L,f^{*}\mathrm{Re\,}\Omega)

provide a symmetry group of the space of maps ff, which also carries a natural Kähler structure. Complexified orbits give hamiltonian deformations, and the moment map is m⁡(f)=f∗​Im​Ωm(f)=f^{*}\,\mathrm{Im}\,\Omega. The connection with our construction is that after fixing a line bundle η\eta and connection with curvature f∗​Re​Ωf^{*}\mathrm{Re\,}\Omega, an infinitesimal symplectomorphism ϕ\phi induces a flat connection, via parallel transport and pull back, on the bundle η⊗ϕ∗​η∗\eta\otimes\phi^{*}\eta^{*}. Globally the action is different (this action has non-zero Lie bracket, for instance, and a fixed group) but the total group orbit and the moment map (see below) are the same.

In general it is clear that the problem of identifying the group for different embeddings of LL should be resolved by working with the space of maps from a fixed L0L_{0} to WW, and enlarging the group by including diffeomorphisms of L0L_{0}, giving a semi-direct product of Diff(L0)(L_{0}) and U⁡(1)U(1) gauge transformations on L0L_{0}. Then the moment map for the diffeomorphism part of the total group would be the Lagrangian condition as in [D], and the problems we are encountering would come from the fact that the group is a semi-direct product and not a product, so that we cannot separate the two out and divide by them separately, as in effect we have been trying to do. Unfortunately, I have not found the correct formulation of the problem, but it is not so important for follows.

So we shall not worry too much about whether the complex structure defined above is integrable, the group is fixed, or the symplectic structure below is closed. In 1 complex dimension it is trivial, in 2 we can use Donaldson’s picture, and in 3 dimensions we could either try to use an abstract SYZ fibration to deform and identify Lagrangians transverse to it, or take everything in this section as motivation for finding the stability condition for Lagrangians of the next section.

Fix a homology class of Lagrangians and multiply Ω\Omega by a unit norm complex number so that ∫LIm​Ω=0\int_{L}\,\mathrm{Im}\,\Omega=0. We induce a symplectic structure on 𝒵\mathcal{Z} from JJ and the following metric on the tangent space

⟨a,b⟩=∫La∧((b​ ​_∣ω−1)​ ​_∣Im​Ω),\langle a,b\rangle=\int_{L}a\wedge((b{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1}){\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\,\mathrm{Im}\,\Omega),

for a,ba,\,b closed 1-forms. A computation in local coordinates shows this is symmetric in aa and bb; in fact it can be written as

∫La∧(b~ _∣ReΩ)=∫Lcosθ(a∧∗b),\int_{L}a\wedge(\widetilde{b}{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\mathrm{\,Re\,}\Omega)=\int_{L}\cos\theta\,(a\wedge*b), (3.2)

where ~\,\widetilde{\ }\, is the isomorphism T∗​L→T​LT^{*}L\to TL set up by the induced metric on LL, Ω|L=ei​θvolL\Omega\arrowvert_{L}=e^{i\theta}\mathrm{vol}_{L}, and volL the Riemannian volume form on LL induced by the Ricci-flat metric. Thus for Lagrangians with θ∈(−π/2,π/2)\theta\in(-\pi/2,\pi/2), i.e. those for which ReΩ\,\Omega restricts to a nowhere vanishing volume form on LL and so are not too far from being SLag (θ≡0\theta\equiv 0), this gives a non-degenerate metric.

The symplectic form is invariant under the group action, and formally the moment map is indeed m⁡(L,A)=Im​Ωm(L,A)=\,\mathrm{Im}\,\Omega in the dual Ωn​(L)0\Omega^{n}(L)_{0} of the Lie algebra (i.e. nn-forms on LL with integral zero). This follows from the computation

X​∫Lh​Im​Ω=∫Lh​d​(X​ ​_∣Im​Ω)=∫L𝑑h∧((σ​ ​_∣ω−1)​ ​_∣Im​Ω),X\int_{L}h\,\mathrm{Im}\,\Omega=\int_{L}h\,d\,(X{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\,\mathrm{Im}\,\Omega)=\int_{L}dh\wedge((\sigma{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1}){\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\,\mathrm{Im}\,\Omega),

where X=σ​ ​_∣ω−1X=\sigma{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1} is a normal vector field to the Lagrangian LL down which we compute the derivative of the hamiltonian ∫Lh​Im​Ω=⟨m⁡(L,A),h⟩\int_{L}h\,\mathrm{Im}\,\Omega=\langle m(L,A),h\rangle for the infinitesimal action of hh. Here have extended hh to a first-order neighbourhood of L⊂WL\subset W so that it is constant in the direction of X=σ​ ​_∣ω−1X=\sigma{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1}. Then the right hand side of the above equation is the pairing using the symplectic form of d​hdh and σ\sigma, as required.

Infinitesimally we can see the moment map interpretation very easily, and fitting naturally with the mirror bundle point of view. Deformations of holomorphic connections AA modulo complex gauge equivalence are given by a ker∂¯A\,\bar{\partial}_{A}/im∂¯A\,\bar{\partial}_{A}  first cohomology group, related to deformations ker∂¯A∩\,\bar{\partial}_{A}\,\cap ker∂¯A∗\,\bar{\partial}_{A}^{*} of the HYM equations (modulo unitary gauge transformations) via Hodge theory, with the moment map equation providing the d∗=0d^{*}=0 slice to the imaginary part of the linearised group action. Similarly, deformations of Lagrangians are given by closed 1-forms kerd:Ω1​(L,ℝ)→Ω2​(L,ℝ)\,d:\,\Omega^{1}(L;\mathbb{R})\to\Omega^{2}(L;\mathbb{R}), so that dividing by hamiltonian deformations we get

H1​(L)=ker​d/im​d.H^{1}(L)=\mathrm{ker}\,d/\mathrm{im}\,d.

If instead of dividing we impose the special condition, we get a kerd∗\,d^{*} slice

H1​(L)=ker​d∩ker​d∗,H^{1}(L)=\mathrm{ker}\,d\cap\mathrm{ker}\,d^{*},

to the (imaginary) deformations (real deformations are given by changing the flat U⁡(1)U(1) connection that can be incorporated into this).

A symplectic example

To motivate a guess at the correct definition of stability for Lagrangians, we expand on an example of Lawlor and Joyce ([J] Sections 6 and 7, building on work of [Ha], [L]; see also a similar example in [SV] that is studied in [TY]), explaining its relevance to mirror symmetry, and giving a simple example in algebraic geometry that mirrors it.

First define the pointwise phase θ\theta of a submanifold LL: we may write

Ω|L=ei​θvol\Omega\arrowvert_{L}=e^{i\theta}\mathrm{\,vol\,}

where vol is the Riemannian volume form on LL induced by Yau’s Ricci-flat metric [Y] on WW. Thus vol provides a (local) orientation for LL, and reversing its sign alters the phase θ\theta by π\pi. A SLag is a Lagrangian with constant phase θ\theta.

At first sight θ\theta is multiply-valued; we always choose it to be a fixed single-valued function to ℝ\mathbb{R}, lifting ei​θ:L→S1e^{i\theta}:\,L\to S^{1} and thus providing the Lagrangian with a grading as introduced by Kontsevich [K], [S2]. Thus we only consider Lagrangians of vanishing Maslov class – for a Calabi-Yau this is the winding class π1​(L)→π1​(S1)\pi_{1}(L)\to\pi_{1}(S^{1}) of the phase map

L⟶ei​θS1,L\stackrel{{\scriptstyle e^{i\theta}\,}}{{\longrightarrow}}S^{1},

which of course vanishes for a SLag. (The definition of grading in [K], [S2] is topological and uses the universal ℤ\mathbb{Z}-cover of the bundle of Lagrangian Grassmannians; here we first pass to the ℤ/2\mathbb{Z}/2 orientation cover of the Grassmannian, choosing an orientation of our Lagrangians, and then use a complex structure to pass to the universal ℤ\mathbb{Z}-cover of this. The two definitions are of course equivalent.)

Similarly we can define a kind of average phase ϕ=ϕ⁡(L)\phi=\phi(L) of a submanifold (or homology class) L⊂WL\subset W by

∫LΩ=A​ei​ϕ​(L),\int_{L}\Omega=A\,e^{i\phi(L)},

for some real number AA; we then use Re (e−i​ϕ​(L)Ω|L)(e^{-i\phi(L)}\Omega\arrowvert_{L}) to orient LL. Reversing the sign of AA alters the phase by π\pi and reverses the orientation. Again for a graded Lagrangian L=(L,θ)L=(L,\theta), and we will always implicitly assume a grading, ϕ⁡(L)\phi(L) is canonically a real number (rather than S1S^{1}-valued). Shifting the grading [ 2​n]:θ↦θ+2​n​π[\,2n\,]:\,\theta\mapsto\theta+2n\pi gives a similar shift to the phase ϕ⁡(L)\phi(L).

The terminology comes from the fact that if there is a submanifold in the same homology class as LL that is SLag with respect to some rotation of Ω\Omega, then it is with respect to e−i​ϕ​(L)​Ωe^{-i\phi(L)}\Omega. Slope, which we define as

μ⁡(L):=tan⁡(ϕ⁡(L))=1∫LRe​Ω​∫LIm​Ω,\mu(L):=\tan(\phi(L))=\frac{1}{\int_{L}\mathrm{Re\,}\Omega}\int_{L}\,\mathrm{Im}\,\Omega,

is defined independently of grading, is monotonic in ϕ\phi in the range (−π/2,π/2)(-\pi/2,\pi/2), and is invariant under change of orientation ϕ↦ϕ±π\phi\mapsto\phi\pm\pi. This agrees with the slope of a straight line SLag in the case of T2T^{2}, as featured in [PZ], and we think of it as mirror to the slope of a mirror sheaf, as is shown for tori in [PZ] (see [DFR] for corrections in higher dimensions away from the large complex structure limit).

Joyce describes examples of SLags which we interpret as follows. We have a family of Calabi-Yau 3-folds WtW^{t} as tt ranges through (a small open subset of) the moduli space of complex structures on WW with fixed symplectic structure. That is, the holomorphic 3-form Ωt\Omega^{t} varies with tt, but the Kähler form ω\omega is fixed. We also have a family of SLag homology 3-spheres L1t,L2t⊂WtL_{1}^{t},\ L_{2}^{t}\subset W^{t} such that L1tL^{t}_{1} and Lt2L^{2}_{t} intersect at a point. If we choose a rotation of Ωt\Omega^{t} such that L2tL_{2}^{t} always has phase ϕ2t≡0\phi_{2}^{t}\equiv 0 (this is possible locally at least; in the family described later it will have to be modified slightly), then we are interested as tt varies only in the complex number

∫L1tΩt=Rt​eϕ1t\int_{L_{1}^{t}}\Omega^{t}=R^{t}e^{\phi^{t}_{1}}

and its polar phase ϕ=ϕ1t\phi=\phi^{t}_{1}; we plot this (i.e. the projection from the complex structure moduli space to ℂ\mathbb{C}\, via this map) in Figure 1.

Then in Joyce’s example, for ϕ<0\phi<0 (and Rt>0R^{t}>0) there is a SLag LtL^{t} (of some phase ϕt\phi^{t}) in the homology class [Lt]=[L1t]+[L2t][L^{t}]=[L^{t}_{1}]+[L^{t}_{2}], such that as ϕ↑0\phi\uparrow 0, this degenerates to a singular union of SLags of the same phase Lt=L1t∪L2tL^{t}=L^{t}_{1}\cup L^{t}_{2} and then disappears for ϕ>0\phi>0.

Most importantly, where LtL^{t} exists as a smooth SLag (ϕ<0\phi<0) we have the slope (and phase) inequality

μ1t<μ2t,i.e.ϕ=ϕ1t<ϕ2t≡0;\mu^{t}_{1}<\mu^{t}_{2},\qquad\mathrm{i.e.\ \,}\phi=\phi^{t}_{1}<\phi^{t}_{2}\equiv 0; (3.3)

at t=0,Ltt=0,\ L^{t} becomes the singular union of L1tL^{t}_{1} and L2tL^{t}_{2}, with

μ1t=μ2t​(ϕ1t=ϕ2t);\mu^{t}_{1}=\mu^{t}_{2}\ (\phi^{t}_{1}=\phi^{t}_{2});

then there is no SLag in LL’s homology class for

μ1t>μ2t​(ϕ1t>ϕ2t),\mu^{t}_{1}>\mu^{t}_{2}\ (\phi^{t}_{1}>\phi^{t}_{2}),

though there is a Lagrangian, of course – the symplectic structure has not changed. Though we have been using slope μ\mu in order to strengthen the analogy with the mirror (bundle) situation, from now on we shall use only the phase (lifted to ℝ\mathbb{R} using the grading). While each is monotonic in the other for small phase (as tan⁡ϕ=μ\tan\phi=\mu), slope does not see orientation as phase does; reversing orientation adds ±π\pm\pi to the phase but leaves μ\mu unchanged. This is related to the fact that we should really be working with complexes and so forth on the mirror side (the bundle analogy is too narrow) and changing orientation has no mirror analogue in terms of only stable bundles; it corresponds to shifting (complexes of) bundles by one place in the derived category. While slopes of bundles cannot go past infinity (without moving degree in the derived category at least), for Lagrangians they certainly can, and phase ϕ\phi continues monotonically upwards as its slope tan⁡ϕ\tan\phi becomes singular and then negative.

Importantly, we can think of the various SLags as independent of time when thought of as Lagrangians in the fixed symplectic manifold WtW^{t}:

Lemma 3.4

For t>0t>0 the SLags LtL^{t} are all in the same hamiltonian deformation class. Similarly for L1t,L2tL_{1}^{t},\ L^{t}_{2}, and for t<0t<0.

Proof Now choosing the phase of Ωt\Omega^{t} such that ϕ⁡(Lt)≡0\phi(L^{t})\equiv 0,

∫Ldd​t​(Im​Ωt)=∫LIm​Ω˙t=0.\int_{L}\frac{d}{dt}(\,\mathrm{Im}\,\Omega^{t})=\int_{L}\,\mathrm{Im}\,\dot{\Omega}^{t}=0. (3.5)

To show this deformation preserves the hamiltonian class of L, we need to find a corresponding first order hamiltonian deformation d​h​ ​_∣ω−1dh{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1} under which the change in Im​Ωt\,\mathrm{Im}\,\Omega^{t},

ℒd​h​_∣ω−1(ImΩt)|L=d((dh _∣ω−1) _∣ImΩt)|L,\mathcal{L}_{dh\_\hskip-1.13809pt\shortmid\hskip 1.0pt\omega^{-1}}(\,\mathrm{Im}\,\Omega^{t})\arrowvert_{L}=d((dh{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega^{-1}){\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\,\mathrm{Im}\,\Omega^{t})\arrowvert_{L},

is −-Im Ω˙t|L\dot{\Omega}^{t}\arrowvert_{L}. But as Re Ωt|L\Omega^{t}\arrowvert_{L} is the induced Riemannian volume form volt on LL, this means we want to solve

−ImΩ˙t|L=d(J(dh _∣ω) _∣ReΩt|L)=d(d​h~ _∣volt)=d(∗dh)=Δ(∗h),-\mathrm{Im\,}\dot{\Omega}^{t}\arrowvert_{L}=d(J(dh{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\omega){\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\mathrm{\,Re\,}\Omega^{t}\arrowvert_{L})=d(\widetilde{dh}{\mbox{\,}\_\hskip-4.2679pt\shortmid\hskip 1.5pt}\mathrm{\,vol}^{t})=d(*dh)=\Delta(*h),

where JJ is the complex structure and ~\,\widetilde{\ }\, is the isomorphism T∗​L→T​LT^{*}L\to TL set up by the induced metric on LL. So the equation has a solution by the Fredholm alternative and (3.5). □\square

Thus for ϕ>0\phi>0 we consider the LtL^{t}s as the same as Lagrangian submanifolds (up to hamiltonian deformation) in the fixed symplectic manifold WtW^{t}; it is only the SLag representative that changes as Ωt\Omega^{t} varies. We think of this as mirror to a fixed holomorphic bundle in a fixed complex structure, with varying HYM connection as the mirror Kähler form changes.

Lemma 3.6

In the analogous 2-dimensional situation of SLags in a K​3K3 or abelian surface, the obstruction does not occur.

Proof Choose a real path of complex structures Wt,t∈(−ϵ,ϵ)W^{t},\ t\in(-\epsilon,\epsilon) in complex structure moduli space such that there is a nodal SLag L0=L10∪L20L^{0}=L_{1}^{0}\cup L_{2}^{0} in W0W^{0}. Without loss of generality we can choose the phase of Ωt\Omega^{t} so that both ω\omega and ImΩt\,\Omega^{t} pair to zero on the homology class of L0L^{0}. Now hyperkähler rotate the complex structures so that instead the new ReΩt\,\Omega^{t} and ImΩt\,\Omega^{t} pair to zero on the homology class of L0L^{0} for all tt. L0L^{0} is now a nodal holomorphic curve CC in the central K​3K3. We can understand deformations of CC via deformations of the ideal sheaf 𝒥C\mathcal{J}_{C}, with obstructions in

Ext2​(𝒥C,𝒥C)→H0,2​(W)≅ℂ,\mathrm{Ext}^{2}(\mathcal{J}_{C},\mathcal{J}_{C})\to H^{0,2}(W)\cong\mathbb{C}\,,

where the arrow is the trace map and is an isomorphism by Serre duality. Standard deformation theory shows the obstruction is purely cohomological – it is the derivative of the H0,2H^{0,2}-component of the class

[C]∈H2​(W)≅H2,0​(W)⊕H1,1​(W)⊕H0,2​(W).[C]\in H^{2}(W)\cong H^{2,0}(W)\oplus H^{1,1}(W)\oplus H^{0,2}(W).

But we have fixed this to remain zero by the phase condition, so the curve deforms to all tt (really we should assume the family is analytic in tt here and extend to t∈ℂt\in\mathbb{C}\,, or just work with first order deformations). Hyperkähler unrotating gives back a family of SLags. □\square

There is a notion of connect summing Lagrangian submanifolds intersecting in a single point (probably due to Polterovich) – see for instance Appendix A of [S1] – which we claim gives the smoothings LtL^{t} of the singular L0=L1∪L2L^{0}=L_{1}\cup L_{2}. This follows by comparing the local models [J], [S1] for the Lagrangians; see [TY] where it is studied in more detail for a related purpose, and our conventions (slightly different from those of [S2]) are described. While topologically we are just connect summing L1L_{1} and L2L_{2} by removing a small 3-ball containing the intersection point from each and gluing the resulting boundary S3S^{3}s (there are two ways, depending on orientation), symplectically the construction does not explicitly use orientations of the submanifolds. (Effectively we are using their relative orientation – the canonical orientation of the sum of the tangent spaces of L1,L2L_{1},\ L_{2} at the intersection point given by the symplectic structure.)

Giving L1L_{1} and L2L_{2} in that order produces a Lagrangian, well defined up to hamiltonian isotopy (this will be shown in Section 4 in more generality; see (4.1)),

L1​#​L2,L_{1}\#L_{2},

with the singular union L1∪L2L_{1}\cup L_{2} a limit point in the hamiltonian isotopy class, which is not itself hamiltonian isotopic to L1​#​L2L_{1}\#L_{2} (we have seen a family of hamiltonian deformations which has limit L1∪L2L_{1}\cup L_{2}, but the deformations are singular at this limit).

There is also an obvious notion of graded connect sum, which is in fact what we shall always mean by #\#. There is a unique grading on L1L_{1} compatible with a fixed grading on L2L_{2} such that we can give a (continuous) grading to the smoothing L1​#​L2L_{1}\#L_{2}. In the case of connect summing at multiple intersection points (Section 4) there is at most one such grading; in general the graded connect sum may not exist.

In nn dimensions, if L1L_{1} and L2L_{2} are graded such that L1​#​L2L_{1}\#L_{2} exists, then on reversing the order of the LiL_{i}, the graded sum that exists is

L2​#​(L1​[2−n])in the homology class[L2]+(−1)n​[L1].L_{2}\#(L_{1}[2-n])\quad\text{in the homology class}\quad[L_{2}]+(-1)^{n}[L_{1}]. (3.7)

Here L⁡[m]L[m] means the graded Lagrangian LL with its grading changed by adding m​πm\pi to θ\theta, and the homology class of L1​#​L2L_{1}\#L_{2} is [L1]+[L2][L_{1}]+[L_{2}] using the orientations on the LiL_{i}s induced by the gradings.

This is closely related, as we shall see, to Joyce’s obstruction, and the lack of it in dimension 2 (Lemma 3.6). In 2 dimensions, L1​#​L2L_{1}\#L_{2} and L2​#​L1L_{2}\#L_{1} are in the same homology class, though by a result of Seidel [S1] not in general in the same hamiltonian isotopy class,

L1​#​L2≉L2​#​L1,L_{1}\#L_{2}\not\approx L_{2}\#L_{1},

importantly (we use ≈\approx to denote equivalence up to hamiltonian deformations). For t>0t>0 in the above family LtL^{t} is in the constant hamiltonian deformation class of L1​#​L2L_{1}\#L_{2}, for t<0t<0 it is in the different class of L2​#​L1L_{2}\#L_{1}, and at t=0t=0 it is L1∪L2L_{1}\cup L_{2} – in neither class but in the closure of both. (For complex tt the symplectic structure is no longer constant like it is for t∈ℝt\in\mathbb{R}, as one can see by following through the hyperkähler rotation; thus we do not get a contradiction to the above statement by going round t=0t=0 in ℂ\mathbb{C}\,.) In 3 dimensions, however, the corresponding obvious choice for a SLag on the other side of the π1t=0\pi^{t}_{1}=0 wall, L2​#​L1​[−1]L_{2}\#L_{1}[-1], is in the wrong homology class.

In the case that the LiL_{i} are Lagrangian spheres we can see this by going round the wall

ϕ⁡(L1t)=0≃ϕ⁡(L2t),\phi(L_{1}^{t})=0\simeq\phi(L_{2}^{t}), (3.8)

and using monodromy. In the 2-dimensional K​3K3 or T4T^{4} case this works as follows.

< ϕ ( L 2 ) ϕ ( L 1 ) < ϕ ( L 1 ) ϕ ( L 2 ) SLag ⁢ L 2 # L 1 SLag ⁢ L 1 # L 2 C = { ∫ L 1 Ω = R e ⁢ i ϕ ( L 1 ) } ≈ ⁢ T L 1 2 ( ⁢ L 1 # L 2 ) ⁢ L 2 # L 1 = ϕ ( L 1 ) ϕ ( L 2 )
Figure 1: (∫L1Ω)\left(\int_{L_{1}}\Omega\right)-space, as Ω\Omega on K​3K3 varies, with polar coordinates (R,ϕ⁡(L1))(R,\,\phi(L_{1}))

Consider a disc in complex structure moduli space over which the family of Kähler K​3K3 surfaces (with constant Kähler form) degenerates at the origin to a K​3K3 with an ordinary double point (ODP) with the Lagrangian L1≅S2L_{1}\cong S^{2} as vanishing cycle. A local model is the standard Kähler structure on x2+y2+z2=ux^{2}+y^{2}+z^{2}=u, over the parameter uu in the unit disc in ℂ\mathbb{C}\,. Now base-changing by pulling back to the double cover in uu, u↦u2u\mapsto u^{2}, we get the 3-fold

x2+y2+z2=u2,x^{2}+y^{2}+z^{2}=u^{2},

with a 3-fold ODP which has a small resolution at the origin putting in a holomorphic sphere resolving the central K​3K3 fibre u=0u=0. Choosing a nowhere-zero holomorphic section Ωu\Omega_{u} of the fibrewise (2,0)(2,0)-forms (using the fact that the relative canonical bundle of either family is trivial), this restricts to zero on the exceptional ℙ1\mathbb{P}^{1} (which is homologous to the vanishing cycle L1L_{1}). Therefore the function

∫L1Ωu\int_{L_{1}}\Omega_{u} (3.9)

has a simple zero at u=0u=0, i.e. it vanishes to order 1 in uu. (The same expression vanished only as u\sqrt{u} in the original family with the singular fibre, and as such its sign was not well defined; this is because the class [L1][L_{1}] was defined globally only up to the monodromy TL1​[L1]=−[L1]T_{L_{1}}[L_{1}]=-[L_{1}], i.e. up to a sign. In our new family the monodromy action TL12T^{2}_{L_{1}} is trivial on homology so it makes sense to talk about the homology class [L1][L_{1}] in any fibre, and (3.9) is single valued.)

Then our loop of complex structures is given by taking the loop u=ei​tu=e^{it} and setting Ωt=Ωei​t\Omega^{t}=\Omega_{e^{it}}. Pulling back the Kähler form from the original family, we get a locally trivial fibre bundle of symplectic manifolds over the circle whose monodromy is the Dehn twist TL12T_{L_{1}}^{2} (since the monodromy round the un-base-changed loop is TL1T_{L_{1}} [S1]). As the family no longer has a singular fibre this monodromy is trivial as a diffeomorphism, but it is a result of [S1], [S2] that as a symplectic automorphism it is non-trivial. This is possible because although the family is a locally trivial bundle of symplectic manifolds over the punctured disc, over u=0u=0 the symplectic form becomes degenerate since it was pulled back via the resolution map.

Measuring [L1][L_{1}] against Ωu\Omega_{u} as in (3.9) we see a principle familiar in physics (in issues of ‘marginal stability’, and taught to me by Eric Zaslow) – we detect a monodromy, like the degree 1 map S1→ℂ×S^{1}\to\mathbb{C}\,^{\!\times} given by t↦∫L1Ωtt\mapsto\int_{L_{1}}\Omega^{t} in this example, by counting wall crossing where a certain real part (here ∫L1Im​Ωt\int_{L_{1}}\,\mathrm{Im}\,\Omega^{t}, or the phase ϕ1t\phi_{1}^{t}) hits 0≃ϕ2t0\simeq\phi^{t}_{2}.

(Here we can no longer choose the phase of Ω\Omega such that ϕ2t=ϕ⁡(L2t)≡0\phi^{t}_{2}=\phi(L^{t}_{2})\equiv 0 in the whole family, as the homology class of L2L_{2} is not preserved in the family:

[TL12​L2]=[L2]+2​[L1].[T_{L_{1}}^{2}L_{2}]=[L_{2}]+2[L_{1}].

However, for a sufficiently small loop about the ODP, i.e. for |∫L1Ω|\big|\int_{L_{1}}\Omega\big| sufficiently small, this will not affect us much and we can write ϕ2t≃0\phi^{t}_{2}\simeq 0: we are only interested in topological information like winding numbers and ϕ1t\phi^{t}_{1} crossing the wall at ϕ2t≃0\phi^{t}_{2}\simeq 0, which are unaffected by small perturbations.)

So instead of going through the ϕ⁡(L1t)=ϕ⁡(L2t)≃0\phi(L_{1}^{t})=\phi(L_{2}^{t})\simeq 0 wall we can go round it. If the loop is sufficiently small we do not encounter any more walls where the homology class [L1]+[L2][L_{1}]+[L_{2}] can be split into classes of the same phase to possibly make the SLag a singular union of distinct SLags of equal phase. For instance the wall at phase 0 does not extend past u=0u=0 to phase ϕ1t=π\phi^{t}_{1}=\pi (even though there μ1t=0\mu^{t}_{1}=0) – the phase of L1L_{1} is not zero but π\pi, and is only zero for L1L_{1} with the opposite orientation, so it does not exist as a SLag (e.g. in the hyperkähler rotated situation, we are saying there is no complex curve in L1L_{1}’s homology class to possibly make LL the nodal union of L1L_{1} and something else, there is only an anti-complex curve). So we really can go round the wall; it ends at u=0u=0.

So this monodromy description shows that on the other t↑2​πt\uparrow 2\pi side of the wall the SLag deforming L2∪L1L_{2}\cup L_{1} is in the hamiltonian deformation class

TL12​L=TL12​(L1​#​L2)=TL12​(TL1−1​L2)≈TL1​L2≈L2​#​L1,T_{L_{1}}^{2}L\,=\,T_{L_{1}}^{2}(L_{1}\#L_{2})\,=\,T_{L_{1}}^{2}(T_{L_{1}}^{-1}L_{2})\,\approx\,T_{L_{1}}L_{2}\,\approx\,L_{2}\#L_{1}, (3.10)

as claimed (for the above equalities see [S1], [S2]).

Notice that the alternative connect sum description of the above Lagrangian

L2​#​L1=TL12​(L1​#​L2)≈TL12​(L1)​#​TL12​(L2)≈L1​[−2]​#​TL12​(L2),L_{2}\#L_{1}\,=\,T_{L_{1}}^{2}(L_{1}\#L_{2})\,\approx\,T_{L_{1}}^{2}(L_{1})\#T_{L_{1}}^{2}(L_{2})\,\approx\,L_{1}[-2]\#T_{L_{1}}^{2}(L_{2}), (3.11)

does not violate the phase inequality to (3.3), as

−2​π+ϵ≈ϕ⁡(L1​[−2])<ϕ⁡(TL12​(L2))≃0.-2\pi+\epsilon\approx\phi(L_{1}[-2])<\phi(T_{L_{1}}^{2}(L_{2}))\simeq 0.

This is why it is important here to keep track of gradings – assigning the phase ϵ\epsilon to ϕ⁡(TL12​(L1))\phi(T_{L_{1}}^{2}(L_{1})) would give the opposite inequality, but one would not be able to form the above graded connect sum without also shifting the phase of TL12​(L2)T_{L_{1}}^{2}(L_{2}) by −2​π-2\pi.

≈ ⁢ T L 1 ( ⁢ L 1 # L 2 ) L 2 < ϕ ( L 2 ) ϕ ( L 1 ) < ϕ ( L 1 ) ϕ ( L 2 ) SLag ⁢ L 1 # L 2 C = { ∫ L 1 Ω = R e ⁢ i ϕ ( L 1 ) } = ϕ ( L 1 ) ϕ ( L 2 ) SLag L 2
Figure 2: (∫L1Ω)\left(\int_{L_{1}}\Omega\right)-space, as Ω\Omega on a 3-fold varies, with polar coordinates (R,ϕ⁡(L1))(R,\,\phi(L_{1}))

The 3-fold case (which Dominic Joyce has also, independently, considered) is slightly different; we need only take a single Dehn twist TL1T_{L_{1}} corresponding to the local family

x2+y2+z2=u,x^{2}+y^{2}+z^{2}=u,

over u∈ℂu\in\mathbb{C}\, to get a winding number one loop in the phase of L1L_{1}. This is because

TL1​L1≈L1​[1−n]T_{L_{1}}L_{1}\approx L_{1}[1-n]

in dimension nn, so in 3 dimensions the homology class [L1][L_{1}] is preserved instead of being reversed. The corresponding picture is displayed in Figure 2.

Again there is a SLag on the other side of the ϕ=0\phi=0 wall, but it is in the wrong homology class [L2][L_{2}]:

TL1​L≈L2.T_{L_{1}}L\approx L_{2}. (3.12)

Analogously to (3.11) this has a number of decompositions as connect sums induced by monodromy,

TL1​(L1​#​L2)≈L1​[−2]​#​(L2​#​(L1​[−1]))≈L2≈(L1​#​L2)​#​(L1​[ 1]),T_{L_{1}}(L_{1}\#L_{2})\,\approx\,L_{1}[-2]\#(L_{2}\#(L_{1}[-1]))\,\approx\,L_{2}\,\approx\,(L_{1}\#L_{2})\#(L_{1}[\,1\,]),

none of which violate the phase inequality (3.3). The only other obvious choice for a (S)Lag on the other side of the ϕ=0\phi=0 wall (given the K​3K3 result) is TL12​(L1​#​L2)≈L2​#​(L1​[−1])T_{L_{1}}^{2}(L_{1}\#L_{2})\approx L_{2}\#(L_{1}[-1]); this however is also in the wrong homology class, and in any case does violate (3.3) and so, by Joyce’s analysis, should not be represented by a SLag. Thinking of TL12T_{L_{1}}^{2} as rotating through −4​π-4\pi in Figure 2, it is at roughly −3​π-3\pi that the phase inequality (3.3) gets violated, and the −π-\pi rotation of L2L_{2} splits as a SLag into the union of the −π-\pi rotations of (L1​#​L2)(L_{1}\#L_{2}) and L1​[ 1]L_{1}[\,1\,]: these both have phase approximately zero.

A holomorphic bundle example

These phenomena are similar to wall-crossing in bundle theory on the complex side – in a real one-parameter family of Kähler forms, for fixed complex structure, stable holomorphic bundles for t>0t>0 can become semistable at t=0t=0 and unstable for t<0t<0.

An example that mirrors Joyce’s is the following. Suppose we have two stable bundles (or coherent sheaves) E1E_{1} and E2E_{2} with

Ext1​(E2,E1)≅ℂ.\mathrm{Ext}^{1}(E_{2},E_{1})\cong\mathbb{C}\,.

This is H1​(E1⊗E2∗)H^{1}(E_{1}\otimes E_{2}^{*}) in the case of bundles and is the mirror [K] of the one dimensional Floer cohomology H​F∗​(L2,L1)≅ℂHF^{*}(L_{2},L_{1})\cong\mathbb{C}\, that is defined by the single intersection point of L1L_{1} and L2L_{2} (see Section 4 for more details of this, and an explanation of why we are dealing with Ext1 and H​F1HF^{1} here). We then form EE from this extension class

0→E1→E→E2→0.0\to E_{1}\to E\to E_{2}\to 0. (3.13)

Take a family of Kähler forms ωt\omega^{t} such that μt​(E2)−μt​(E1)\mu^{t}(E_{2})-\mu^{t}(E_{1}) is the same sign as tt (here μt(F)=c1(F).(ωt)n−1/\mu^{t}(F)=c_{1}(F)\,.\,(\omega^{t})^{n-1}/ rk (F)(F) is the slope of FF with respect to ωt\omega^{t}). Supposing that the EiE_{i} are stable for all t∈(−ϵ,ϵ)t\in(-\epsilon,\epsilon), we claim that EE is stable for sufficiently small t>0t>0, while it is destabilised by E1E_{1} for t≤0t\leq 0. Without loss of generality take μt​(E2)=μ\mu^{t}(E_{2})=\mu fixed, and μt​(E1)=μ−t\mu^{t}(E_{1})=\mu-t. As E2E_{2} is stable, for tt sufficiently small there are no subsheaves of E2E_{2} of slope greater than μ−t\mu-t, so for any stable destabilising subsheaf FF of EE, the composition

F↪E→E2F\hookrightarrow E\to E_{2}

cannot be an injection (unless it is an isomorphism, but (3.13) does not split. So F∩E1≠0F\cap E_{1}\neq 0, and the quotient Q=F/(F∩E1)Q=F/(F\cap E_{1}) has slope μ⁡(Q)>μ⁡(F)>μ−t\mu(Q)>\mu(F)>\mu-t by the stability of FF and instability of EE. But QQ injects into E2E_{2}, which we know is impossible.

In the 2-dimensional case, by Serre duality Ext(E1,E2)1≅{}^{1}(E_{1},E_{2})\cong\,Ext(E2,E1)∗1≅ℂ{}^{1}(E_{2},E_{1})^{*}\cong\mathbb{C}\,on K​3K3 or T4T^{4}, so for t<0t<0 we can instead form an extension

0→E2→E′→E1→0,0\to E_{2}\to E^{\prime}\to E_{1}\to 0, (3.14)

to give a new bundle E′E^{\prime} which is also stable, and has the same Mukai vector

v⁡(E′)=v⁡(E1)+v⁡(E2);v(E^{\prime})=v(E_{1})+v(E_{2});

compare (3.7). At t=0t=0 we take the (polystable) bundle

E1⊕E2.E_{1}\oplus E_{2}.

This is because the semistable extension (3.13) no longer admits a Hermitian-Yang-Mills metric, but E1⊕E2E_{1}\oplus E_{2} does. Also, the algebraic geometry of the moduli problem shows that while a semistable bundle gets identified in the moduli space with the other (“S-equivalent”) sheaves in the closure of its gauge group orbit, there is a distinguished representative of its equivalence class – the polystable direct sum (of the Jordan-Hölder filtration, which here is E1⊕E2E_{1}\oplus E_{2}).

Thus, while the HYM connections vary, the bundle has only 3 different holomorphic structures – for t>0,t=0,t>0,\ t=0, and t<0t<0. Put another way (to spell out the analogy with the Lagrangians Lt,L1,L2L^{t},\ L_{1},\ L_{2}) as ωt\omega_{t} varies with t>0t>0 we take different points in a fixed complexified gauge group orbit, and at t=0t=0 we take as limit point something in a different orbit that is nonetheless in the closure of the t>0t>0 (and t<0t<0) orbit. The stable deformations of the polystable E1⊕E2E_{1}\oplus E_{2} (which we are thinking of as the mirror of the singular union L1∪L2L_{1}\cup L_{2}, of course) are precisely (3.13) for t>0t>0 and (3.14) for t<0t<0.

In the 3-fold case, however, Serre duality gives Ext(E1,E2)2≅{}^{2}(E_{1},E_{2})\cong\,Ext(E2,E1)∗1≅ℂ{}^{1}(E_{2},E_{1})^{*}\cong\mathbb{C}\, instead, and so no stable extension (3.14). In fact one would expect there to be no stable bundle with the right Chern classes; instead the one dimensional Ext2 gives us a complex E′E^{\prime} in the derived category Db​(M)D^{b}(M) fitting into an exact sequence of complexes

0→E2→E′→E1​[−1]→0,0\to E_{2}\to E^{\prime}\to E_{1}[-1]\to 0,

where E1​[−1]E_{1}[-1] is E1E_{1} shifted in degree by one place to the right as a complex. This has Mukai vector

v⁡(E′)=v⁡(E2)−v⁡(E1),v(E^{\prime})=v(E_{2})-v(E_{1}),

compare (3.7). Thus, just as in the case of SLags, as we pass through t=0t=0 there is no natural stable object on the other side in the same homology class in 3 dimensions (though there is in 2 dimensions) and so an element of the appropriate moduli space disappears.

In fact, as in the Lagrangian example, the natural stable object on the other side of the wall is E2E_{2} if we consider monodromy. The mirror of the symplectic Dehn twists of above are described in [ST] (in the case that the bundles EiE_{i} are spherical in the sense of [ST]: Ext(Ei,Ei)k≅Hk(Sn;ℂ){}^{k}(E_{i},E_{i})\cong H^{k}(S^{n};\mathbb{C}\,); this is the natural mirror analogue of the LiL_{i}s being spheres). These are the twists TE1T_{E_{1}} of [ST] on the derived category of the Calabi-Yau that act on the extension bundle EE of (3.13) to give precisely the extension (3.14),

TE12​E=E′T_{E_{1}}^{2}E=E^{\prime}

(compare (3.10)), as a short calculation using [ST] shows. Similarly

TE1​E=E2,T_{E_{1}}E=E_{2},

the analogue of (3.12). (In both of these calculations it is important to calculate this monodromy in the derived category; in the K​3K3 case the action of TE12T_{E_{1}}^{2} is trivial on K-theory and cohomology, and we cannot distinguish between (3.13) and (3.14), but they are very different as holomorphic bundles and as elements of the derived category.)

The mirror wall crossing, with a SLag splitting into two and then disappearing, is interpreted in [DFR] (and in [SV] in a different case) as the state it represents decaying as we reach a point of ‘marginal stability’. Despite this dealing with only SLags (and so with only a priori stable Lagrangians in our mathematical sense of stability), this suggestive language does in fact have something to say about the stability, in our sense of group actions, of (non-special) Lagrangians, by considering the nodal limit L1∪L2L_{1}\cup L_{2} to be a semistable Lagrangian.

Thus the Lagrangian L1​#​L2L_{1}\#L_{2} (which always exists as a Lagrangian as the complex structure varies with fixed Kähler form) becomes semistable at t=0t=0 and is represented by something in a different orbit of the hamiltonian deformation symmetry group (but in the closure of the original orbit), and is unstable for t<0t<0 so exists there only as a Lagrangian and not as a SLag. This, and the bundle analogue described above, leads us to think of the Lagrangian L1L_{1} as destabilising L=L1​#​L2L=L_{1}\#L_{2} when ϕ⁡(L1)≥ϕ⁡(L2)\phi(L_{1})\geq\phi(L_{2}). This motivates the now obvious definition of stability in Section 5; first we explain more about the connections to mirror symmetry, and generalisations to connect sums at more intersection points.

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