Research Contribution

Received: 3 October 2024. Accepted: 10 October 2024.

Non-fillability of overtwisted contact manifolds via polyfolds

Wolfgang Schmaltz Fakultät für Mathematik, Ruhr-Universität Bochum,
Universitätsstraße 150, D-44801 Bochum, Germany;
email: Wolfgang.Schmaltz@rub.de
, Stefan Suhr Fakultät für Mathematik, Ruhr-Universität Bochum,
Universitätsstraße 150, D-44801 Bochum, Germany
email: Stefan.Suhr@rub.de
, and Kai Zehmisch Fakultät für Mathematik, Ruhr-Universität Bochum,
Universitätsstraße 150, D-44801 Bochum, Germany
email: Kai.Zehmisch@rub.de

Abstract

We prove that any weakly symplectically fillable contact manifold is tight. Furthermore we verify the strong Weinstein conjecture for contact manifolds that appear as the concave boundary of a directed symplectic cobordism whose positive boundary satisfies the weak-filling condition and is overtwisted. Similar results are obtained in the presence of bordered Legendrian open books whose binding–complement has vanishing second Stiefel–Whitney class. The results are obtained via polyfolds.

2010 Mathematics Subject Classification. 53D42; 53D40, 57R17, 53D45, 37J55, 34C25, 37C27

1. Introduction

In [22] Eliashberg introduced a dichotomy of closed contact \(3\)-manifolds, the tight and overtwisted contact structures. He established in [22] an \(h\)-principle in the sense of Gromov [33] for overtwisted contact structures. The higher dimensional analogue was defined by Borman–Eliashberg–Murphy [11] . One way to detect tight contact structures on a \(3\)-manifolds is to find a weak symplectic filling. In view of the filling–by–holomorphic–discs technique such fillable contact manifolds cannot be overtwisted, see [23] , [32] and cf. [29], Corollary 3.8 . In higher dimensions obstructions to overtwistedness in terms of semi-positive weak symplectic fillings were obtained by Niederkrüger [55] and Massot–Niederkrüger–Wendl [50] . The aim of this work is to remove the assumption of being semi-positive.

We consider not necessarily connected \((2n-1)\)-dimensional contact manifolds \((M,\xi )\) and assume that there is a contact form \(\alpha \) on \(M\) defining \(\xi \), i.e. \(\xi \) is the kernel of \(\alpha \). The restriction of \(\rmd \alpha \) to \(\xi \) is a symplectic form providing \(\xi \) with the symplectic orientation via \((\rmd \alpha )^{n-1}\). The contact manifold \((M,\xi )\) is oriented by \(\alpha \wedge (\rmd \alpha )^{n-1}\). These notions are independent of the choice of contact form as long as the contact form equals \(f\alpha \) for a positive smooth function \(f\) on \(M\).

A compact \(2n\)-dimensional symplectic manifold \((W,\Omega )\) provided with the symplectic orientation \(\Omega ^n\) is called a weak symplectic filling of a given \((2n-1)\)-dimensional contact manifold \((M,\xi )\), if \(\partial W=M\) as oriented manifolds, where \(\partial W\) carries the boundary orientation, such that the following condition is satisfied: For all choices of positive contact forms \(\alpha \) for \(\xi \) the differential forms

\[ \alpha \wedge \omega ^{n-1} \quad \text {and}\quad \alpha \wedge \big (\rmd \alpha +\omega \big )^{n-1}\,, \quad \text {where}\quad \omega :=\Omega |_{TM}\,, \]

are positive volume forms on \(M\), see [20] , [50] . Fixing a contact form \(\alpha \) for \(\xi \) the latter is equivalent to

\[ \alpha \wedge \big (f\rmd \alpha +\omega \big )^{n-1}>0 \]

for all non-negative smooth functions \(f\) on \(M\). A contact manifold \((M,\xi )\) is weakly symplectically fillable if it admits a weak symplectic filling.

If \((M,\xi )\) contains an overtwisted disc, then \((M,\xi )\) is called overtwisted ; otherwise \((M,\xi )\) is called tight , see [11] and Section 2.2 .

Theorem 1.
Any weakly symplectically fillable contact manifold is tight.

Potentially, Theorem 1 can be obtained with Pardon's [59] rigorously defined contact homology. An argument is indicated in Remark 1 below. We will prove Theorem 1 along the classical line of reasoning due to Gromov [32] and Eliashberg [23] , cf. [69] , [55] , [50] . In fact, Theorem 1 , will follow as a special case of Theorem 5.1.2 (ii). For that we remark, that a contact manifold, which contains an overtwisted disc, also contains a parallelisable small plastikstufe whose core is a torus, see the discussion in Section 2.2 and Theorem 70 . A plastikstufe is an example of a bordered Legendrian open book such that the book fibration is trivial, the page is a product of an interval with the binding and the binding is the core, see Section 2.1 . Whenever a bordered Legendrian open book in an ambient closed contact manifold is small , i.e. has a contractible neighbourhood, it was shown in [50], Theorem 4.4 that no semi-positive weak symplectic filling can exists. The way in which the theorem is formulated suggests the conjecture that the statement should be true even without the assumption of semi-positivity. Here we prove:

Theorem 2.
A contact manifold is not weakly symplectically fillable provided that it contains a small bordered Legendrian open book such that the complement of the binding has vanishing second Stiefel–Whitney class.

Theorem 2 implies Theorem 1 and directly follows from Theorem 5.1.2 (ii). The examples of small bordered Legendrian open books given in [50], Proposition 5.9 all have vanishing second Stiefel–Whitney class though they are sometimes not orientable and, hence, are not spin, see Example 2.1.3 . This leaves the question, whether there are contact manifolds that are (i) weakly symplectically fillable (and therefore tight with Theorem 1 ) and (ii) that admit a bordered Legendrian open book, whose binding–complement could be orientable, but is not spin. Note that non of the potential weak symplectic fillings can be semi-positive.

Restricting to weak symplectic fillings that are semi-positive for a moment Theorem 2 holds true also if the second Stiefel–Whitney class does not vanish. The reason is, that a compact \(1\)-dimensional manifold has an even number of boundary components which is used in a typical Gromov–Witten–invariant type argument performed in a potential weak symplectic filling. Taking holomorphic discs with boundary on the bordered Legendrian open book that intersect a given path connecting the binding with the boundary inside a page yields a \(1\)-dimensional moduli space. At the end of the path on the binding there is a foliation by boundary circles of Bishop discs; at the other end, which corresponds to the boundary of the page, no holomorphic disc homotopic to a Bishop disc does exist. After perturbing the almost complex structure no bubbling off takes place for the relevant moduli space in a semi-positive setting. In other words, the \(1\)-dimensional moduli space is compact with an odd number of boundary components. This is not possible thus contradicts the presence of a weak symplectic filling.

Note that this is in contrast to the \(1\)-dimensional branched manifolds that appear in the non semi-positive setting. Namely, in general, the solution space of a perturbed Cauchy–Riemann operator branches, because of the need of multisections near nodal holomorphic discs with multiply covered sphere bubbles of negative first Chern number. The vanishing assumption for the second Stiefel–Whitney class in the non semi-positive setting allows to orient the solution space (see Remark 7.4.1 ) resulting in an oriented compact \(1\)-dimensional weighted branched manifold, which has an even number of boundary components, i.e. yields the desired contradiction to weak symplectic fillability. We remark, that moduli spaces of holomorphic discs in general are not orientable in contrast to the case of spheres, see [26] .

As a consequence of Theorem 2 we can verify the conjecture stated in [50], Theorem 5.13 (a) involving circular contactisations of Liouville domains also called Giroux domaines :

Theorem 3.
A contact manifold is not weakly symplectically fillable provided that it contains a domain that is obtained from a Giroux domain with disconnected boundary, where one boundary component is blown down via a contact cut.

The construction in Example 2.1.3 yields a small bordered Legendrian open book whose binding–complement has trivial second Stiefel–Whitney class. Hence, Theorem 3 follows from Theorem 2 .

Theorem 5.1.2 also verifies instances of the Weinstein conjecture, which asks for the existence of periodic Reeb orbits for all closed contact manifolds, see [65] . For a short historical review see [21], Section 1 . Our approach, besides the usage of polyfolds, is based on the work of Hofer [35] , Albers–Hofer [6] and Niederkrüger–Rechtman [57] , and yields so-called Reeb links: A Reeb link is a finite collection of parametrised periodic Reeb orbits each of which is oriented by the corresponding Reeb vector field and possibly multiply covered, see [2] . A Reeb link is called null-homologous if the link components counted multiplicity add up to zero in homology. The strong Weinstein conjecture as formulated by Abbas–Cieliebak–Hofer in [2] asserts the existence of a null-homologous Reeb link for all contact forms on all closed contact manifolds.

Theorem 4.
The strong Weinstein conjecture holds true for all contact manifolds that appear as the concave boundary of a directed symplectic cobordism whose positive end satisfies the weak-filling condition and that are at least one of the following:

  1. (i) an overtwisted contact manifold,
  2. (ii) a contact manifold that contains a small bordered Legendrian open book such that the complement of the binding has vanishing second Stiefel–Whitney class,
  3. (iii) a contact manifold that contains a domain that is obtained from a Giroux domain with disconnected boundary, where one boundary component is blown down via a contact cut.

The relevant notions related to directed symplectic cobordisms can be found in Section 5.1 . Theorem 4 follows from Theorem 5.1.2 together with the remarks made for Theorem 1 and 3 above.

For the proof of Theorem 5.1.2 , which implies Theorem 2 and 4 , we will use the following alternative characterisation of weak symplectic fillability from [50] : A compact symplectic manifold \((W,\Omega )\) is a weak symplectic filling of a contact manifold \((M,\xi =\ker \alpha )\) if \(\partial W=M\) as oriented manifolds and if there exists an \(\Omega \)-tamed almost complex structure \(J\) on \(W\) such that \(\xi \) is \(J\)-invariant and the restriction of \(\rmd \alpha \) to \(\xi \) tames \(J\). In this situation \((W,\Omega ,J)\) is called a tamed pseudo-convex manifold, see [23] and cf. Section 4 . This point of view allows the use of holomorphic disc fillings in the sense of Bishop, see Section 3 .

It turns out that fillability questions can be perfectly described in the language of symplectic cobordisms, see Section 5 . Assuming non-existence of Reeb links of the Reeb flows that appear on the negative ends of the symplectic cobordism the Gromov–Witten–invariant type polyfolds can be defined in the sense of Hofer–Wysocki–Zehnder [36] , [37] , [38] , [39] , [40] , [41] , [42] , [43] . This was observed in [64] in the context of holomorphic spheres. Necessary modifications for the usage of holomorphic discs instead are worked out in Section 6 and 7 . Special attention we pay to orientability questions. Similar to the polyfold version of the Deligne–Mumford space we introduce a Riemann moduli space of boundary un-noded stable discs with \(3\) ordered boundary marked points in Section 6 . In Section 7 we define the relevant polyfold of stable boundary un-noded disc maps motivated by the absence of boundary disc bubbling in the Gromov compactification of the appearing moduli space of holomorphic discs.

Remark 1.
Contact homology, as a formal concept, was introduced by Eliashberg–Givental–Hofer in [24] as contact-manifold-invariant having functorial properties. Symplectic cobordisms, which are directed from the negative to the positive end, induce structure preserving maps (e.g. unital) from the contact homology at the positive end to the contact homology at the negative end. To incorporate non-exact cobordisms and weak-filling boundary conditions a change of coefficients to a Novikov completion of the group ring of the second homology (or an adapted quotient thereof) of the symplectic cobordism resp. contact manifold is necessary by compactness reasons, see Bourgeois–van Koert [14], Section 1.1 , Latschev–Wendl [49], Section 2 , and Niederkrüger–Wendl [58], Section 2.5 . Applying this, one gets that a contact manifold with vanishing contact homology (i.e. with \(1\) being a boundary) cannot be weakly symplectically fillable (i.e. symplectically null-cobordant with empty negative end), as the contact homology of the empty contact manifold equals the coefficient ring and, therefore, never vanishes meaning \(1\neq 0\).

Combining Casals–Murphy–Presas' [17], Theorem 1.1 and Bourgeois–van Koert's [14], Theorem 1.3 shows that on every overtwisted contact manifold there exists a non-degenerate, defining contact form that admits a periodic Reeb orbit that bounds precisely one finite energy plane, which additionally is Fredholm regular, implying the vanishing of the contact homology. As Pardon rigorously defined contact homology in [59] , this implies, as stated on [59], p. 835/6 , the vanishing of the contact homology of overtwisted contact manifolds. Furthermore, after reworking [59] with group ring coefficients, this yields symplectic non-fillability even in the weak sense, i.e. Theorem 1 .

Similarly and removing the word ‘strong', part (i) of Theorem 4 could follow along the same line of reasoning because the vanishing of the contact homology implies the Weinstein conjecture for the underlying contact manifold. To obtain the strong Weinstein conjecture as verified in part (i) of Theorem 4 one could argue as above in the case of non-degenerate contact forms. In order to handle degenerate contact forms one could use an approximation argument as in [64], Section 6 . A filtered version of contact homology might yield the required energy, resp., action bounds.

On [59], p. 836 Pardon addresses the vanishing of contact homology in the presence of a small bordered Legendrian open book based on an idea of Bourgeois–Niederkrüger [13], p. 69 . It would be of interest, whether Pardon's approach to broken homolorphic discs with boundary via orientation local systems could remove the assumption on the second Stiefel–Whitney class, which we made in Theorem 2 and in part (ii) of Theorem 4 in order to make our approach via boundary un-noded stable holomorphic discs feasible. The Deligne–Mumford space elaborated in Section 6 might represent a first step in this direction.

2. Singular Legendrian foliations

2.1. Legendrian open books.

Following [50] , [56] we define:

Definition 2.1.1.
A relative open book decomposition \((B,\vartheta )\) of a connected manifold \(N\) with boundary \(\partial N\) consists of

  • a non-empty codimension \(2\) submanifold \(B\) of \(\Int N\), called the binding ,
  • and a smooth, locally trivial fibration \(\vartheta \co N\setminus B\ra S^1\), whose fibres \(\vartheta ^{-1}(\theta )\), \(\theta \in S^1\), are called the pages ,

such that the following conditions are satisfied:

  • (i) All pages intersect \(\partial N\) transversally.
  • (ii) The binding \(B\) has a trivial tubular neighbourhood \(B\times D^2\) in \(N\) in which \(\vartheta \) is given by the angular coordinate in the \(D^2\)-factor.

The pages \(\vartheta ^{-1}(\theta )\) in \(N\setminus B\) are co-oriented by the orientation of \(S^1\), i.e. the linearisation \(T\vartheta \) maps positive normal vectors to positive tangent vectors of \(S^1\).

As in [50], Section 4 and [56], Section I.4 we define:

Definition 2.1.2.
A connected compact \(n\)-dimensional submanifold \(N\) with boundary \(\partial N\) of a \((2n-1)\)-dimensional contact manifold \((M,\xi )\) carries a bordered Legendrian open book \((B,\vartheta )\) if \((B,\vartheta )\) is a relative open book decomposition of \(N\) such that

  • the pages of \((B,\vartheta )\) are Legendrian submanifolds of \((M,\xi )\) and
  • the singular set of \(N\subset (M,\xi )\), i.e. the set of all points \(p\in N\) such that \(T_pN\subset \xi _p\), is equal to \(B\cup \partial N\).

In particular, the binding of a bordered Legendrian open book is an isotropic submanifold of \((M,\xi )\); the boundary \(\partial N\) is Legendrian. The complement

\[ N^*:=N\setminus \big (B\cup \partial N\big ) \]

of \(B\cup \partial N\) in \(N\) is the set of regular points of \(N\subset (M,\xi )\), i.e. the set of all points \(p\in N\) such that \(T_pN\) and \(\xi _p\) intersect transversally. The characteristic distribution \(TN^*\cap \xi \) integrates by the Frobenius theorem to the so-called characteristic foliation on \(N^*\). The characteristic leaves , which by definition are the leaves of the characteristic foliation, coincide with the pages of the open book \((B,\vartheta )\).

If, in addition, \(\xi \) is co-oriented, then \(\xi |_{N^*}\) puts a co-orientation to the pages \(\vartheta ^{-1}(\theta )\) in \(N\setminus B\). We will assume that this co-orientation coincides with the co-orientation induced by \(\vartheta \) by possibly composing \(\vartheta \) with a reflection on \(S^1=\partial D\).

It follows from [56], Theorem I.1.3 or [44], Theorem 1.4 that the germ of a contact structure \((M,\xi )\) is unique near a submanifold \(N\subset (M,\xi )\) (with boundary \(\partial N\)) that carries a bordered Legendrian open book \((B,\vartheta )\). The germ is uniquely determined by the singular characteristic distribution \(\xi \cap TN\) given by the open book decomposition on \(N\) determined by \((B,\vartheta )\).

A bordered Legendrian open book \((B,\vartheta )\) is called small if the supporting submanifold \(N\subset (M,\xi )\) is contained in a ball inside \(M\).

Example 2.1.3.
(A non-spin bordered Legendrian open book) In [50], Proposition 5.9 examples of contact manifolds \((M,\xi )\) are constructed that contain a submanifold \(N\), which carries a small bordered Legendrian open book. Some of the in [50], Proposition 5.9 constructed examples are indeed non-spin. In order to see this, we repeat the essential construction steps here.

The construction starts with a cylindrical Lagrangian submanifold \(L\) of an ideal Liouville domain \(V\) with disconnected boundary \(\partial V=\partial _+ V\cup \partial _- V\) (see [50], Theorem C ) such that \(L\) has disconnected boundary \(\partial L=\partial _+ L\cup \partial _- L\) with \(\partial _{\pm } L\subset \partial _{\pm } V\). A perturbation of \(L\times S^1\) inside the interior of the circular contactisation \(V\times S^1\) of the ideal Liouville domain \(V\) – a so-called Giroux domain – followed by a contact cut along \(\partial _-V\times S^1\) (see [50], Section 5.1 ), say, yields a bordered Legendrian open book \(N\). Gluing a Giroux domain along \(\partial _+V\times S^1\) with [50], Lemma 5.1 and eventually cutting remaining boundary components yields a contact embedding of \(N\) into a closed contact manifold \((M,\xi )\).

In the process, \(L\) is the result of Polterovich surgery (see [60] ) along, say, two transverse intersection points of a Hamiltonian deformation of two boundary parallel Lagrangian discs. If the dimension of \(L\) is even, then the Polterovich surgery result \(L\) necessarily is homotopy equivalent to a \(n\)-dimensional Klein bottle with two points removed, see [60], Paragraph 7 . Therefore, \(N^*\) is not orientable with \(w_2(N^*)=0\). If the dimension of \(L\) is odd, one can choose orientations such that \(L\) is homotopy equivalent to a \(n\)-dimensional Klein bottle or to \(S^1\times S^{n-1}\) each time with two points removed.

2.2. Overtwistedness.

A \((2n-1)\)-dimensional contact manifold \((M,\xi )\) is called overtwisted , if \((M,\xi )\) contains an overtwisted disc, see [11] . For example \(\R ^3\) equipped with the contact structure \(\ker \alpha _{\ot }\),

\[ \alpha _{\ot }:=\cos r\,\rmd z+r\sin r\,\rmd \theta \;, \]

is overtwisted, as \(D_{\ot }^2:=\{z=0,r\leq \pi \}\) is an overtwisted disc.

For a \((n-2)\)-dimensional closed smooth manifold \(Q\) we consider the contact manifold \(\R ^3\times T^*Q\) equipped with contact structure \(\xi _Q:=\ker (\alpha _{\ot }+\lambda _{T^*Q})\), where we identify \(Q\) with the zero section in \(T^*Q\) and denote the Liouville \(1\)-form of \(T^*Q\) by \(\lambda _{T^*Q}\). Following [11], Section 10 we define the model plastikstufe with core \(Q\) to be the subset \(P_Q:=D_{\ot }^2\times Q\) of \(\big (\R ^3\times T^*Q,\xi _Q\big )\).

We will say that \((P_Q,\xi _Q)\) admits a contact embedding into a \((2n-1)\)-dimensional contact manifold \((M,\xi )\) if a neighbourhood of \(P_Q\) in \(\big (\R ^3\times T^*Q,\xi _Q\big )\) does. In this case the image \(N\) of the model \(P_Q\) is called a plastikstufe with core \(Q\) and carries the structure of a bordered Legendrian open book with binding \(Q\) and pages corresponding to \(I_{\theta }\times Q\), where \(I_{\theta }\) is the straight line segment in \(D_{\ot }^2\subset \R ^2\) connecting \(0\) and \(\pi \rme ^{\rmi \theta }\). For the original definition of a plastikstufe and the relation to bordered Legendrian open books we refer to [55] , [56] .

Theorem 2.2.1.
(Borman–Eliashberg–Murphy [11] ) Let \(Q\) be a \((n-2)\)-dimensional closed smooth manifold, whose complexified tangent bundle is trivial. Then any \((2n-1)\)-dimensional overtwisted contact manifold admits a small plastikstufe with core \(Q\).

The assumption on \(Q\) is satisfied for any stably parallelisable manifold \(Q\), cf. [9], Section 1.1 . For the converse of Theorem 70 we note:

Theorem 2.2.2.
(Huang [45] ) If a contact manifold \((M,\xi )\) contains a plastikstufe, then \((M,\xi )\) is overtwisted.

A forerunner version of this result, which is [45], Theorem 1.2 , was given in [17] . Further, it is shown in [45], Theorem 1.3 that if \((M,\xi )\) admits a bordered Legendrian open book and \(\dim M=5\), then \((M,\xi )\) is overtwisted. In fact, a contact manifold \((M,\xi )\) is overtwisted precisely if \((M,\xi )\) contains a bordered Legendrian open book with pages diffeomorphic to \(P\times \Sigma \), where \(P\) is a closed manifold and \(\Sigma \) a compact surface with boundary, see [45], Corollary 1.4 .

2.3. Local model near the binding.

Let \((M,\xi )\) be a contact manifold. We consider a bordered Legendrian open book decomposition \((B,\vartheta )\) of a submanifold \(N\subset (M,\xi )\). By Definition 2.1.1 the binding \(B\subset N\) admits a tubular neighbourhood \(B\times D^2\) on which the fibre projection \(\vartheta \) is given by \((b,z=r\rme ^{\rmi \theta })\mapsto \theta \).

By [55], Proposition 4 a neighbourhood of \(B\times D^2\) in \((M,\xi )\) is contactomorphic to a neighbourhood of \(\{0\}\times D^2\times B\) in \(\big (\R \times \C \times T^*B,\ker \alpha _o\big )\), where

\[ \alpha _o:= \rmd t +\tfrac 12\big (x\rmd y-y\rmd x\big ) +\lambda _{T^*B}\;, \]

denoting by \(t,z=x+\rmi y\) the coordinates on \(\R \times \C \) and by \(\lambda _{T^*B}\) the Liouville \(1\)-form on \(T^*B\). The contactomorphism restricts to \((b,z)\mapsto (0,z,b)\) on \(B\times D^2\). Again we identify \(B\) with the zero section in \(T^*B\).

2.4. Local model near the boundary.

Consider a contact manifold \((M,\xi )\). Let \(N\subset (M,\xi )\) be a submanifold that supports a bordered Legendrian open book \((B,\vartheta )\). By Definition 2.1.1 the restriction of \(\vartheta \) to \(\partial N\) induces a locally trivial fibration over \(S^1\) with fibre \(F\). Denoting the monodromy diffeomorphism by \(\varphi \co F\ra F\) this fibration is equivalent to the mapping torus

\[ M(\varphi )= \frac {[0,2\pi ]\times F} {(2\pi ,f)\sim \big (0,\varphi (f)\big )} \]

of \(\varphi \). The induced diffeomorphism

\[ \varphi ^*:=(T\varphi ^{-1})^*\co T^*F\ra T^*F \]

naturally preserves the Liouville \(1\)-form \(\lambda _{T^*F}\) so that the mapping torus

\[ M(\varphi ^*)= \frac {T^*[0,2\pi ]\times T^*F} {\big ((r,2\pi ),u\big )\sim \big ((r,0),(T\varphi ^{-1})^*(u)\big )} \]

carries the Liouville form \(r\rmd \theta +\lambda _{T^*F}\) and can be identified with \(T^*\big (M(\varphi )\big )\). The corresponding Liouville vector field is of the form \(r\partial _r+Y_{T^*F}\) and \(M(\varphi ^*)\) fibres naturally over \((T^*S^1,r\rmd \theta )\) with fibre projection map \([(r,\theta ),u]\mapsto [(r,\theta )]\).

We equip \(\R \times M(\varphi ^*)\) with the contact form \(\alpha _{\varphi }\) induced by

\[ \alpha _{\varphi }\equiv \rmd t+r\rmd \theta +\lambda _{T^*F} \;. \]

By [50], Lemma 4.6 a neighbourhood of \(\partial N\subset (M,\xi )\) is contactomorphic to a neighbourhood of

\[ \{0\}\times M(\varphi ) \subset \big (\R \times M(\varphi ^*),\ker \alpha _{\varphi }\big ) \;, \]

so that

\[ \big (\{0\}\times \{r=0,u=0\}\big ) \equiv \{0\}\times M(\varphi ) \]

corresponds to \(\partial N\) and a neighbourhood of \(\partial N\) in \(N\subset M\) corresponds to the quotient of the set \(\{0\}\times \{r\leq 0,u=0\}\) in \(\{0\}\times M(\varphi ^*)\). We orient \(T^*S^1\equiv \R \times S^1\) by \(\rmd r\wedge \rmd \theta \). This matches the co-orientation conventions for the singular distribution determined by \(\xi \) and the pages of \((B,\vartheta )\) in Section 2.1 .

3. Holomorphic discs

3.1. A germ of Bishop disc filling.

Motivated by Section 2.3 we define a natural almost complex structure \(J\) on \(\R \times (\R \times \C \times T^*B)\) that allows a lifting of obvious holomorphic discs similar to cf. [30], Section 2 .

For that choose a Riemannian metric \(g_B\) on \(B\). Denote by \(J_{T^*B}\) the almost complex structure on \(T^*B\) that is induced by the Levi-Civita connection of \(g_B\), see [55], Appendix B or [48], Section 5 . Observe that \(J_{T^*B}\) is compatible with the symplectic form \(\rmd \lambda _{T^*B}\). Furthermore denoting by \(g_B^{\flat }\) the dual metric of \(g_B\) the kinetic energy function on \(T^*B\) is defined by \(k(u)=\frac 12g^{\flat }(u,u)\), \(u\in T^*B\), and satisfies \(\lambda _{T^*B}=-\rmd k\circ J_{T^*B}\). In other words, \(k\) is a strictly plurisubharmonic potential in the sense of [28], Section 3.1 .

On the Liouville manifold

\[ (V,\lambda _V):= \Big ( \C \times T^*B,\tfrac 12\big (x\rmd y-y\rmd x\big ) +\lambda _{T^*B} \Big ) \]

we consider the almost complex structure

\[ J_V=\rmi \oplus J_{T^*B} \;, \]

which is compatible with the symplectic form \(\rmd \lambda _V\). The function

\[ \psi (z,u):=\tfrac 14|z|^2+k(u) \]

is a strictly plurisubharmonic potential \(\psi \) on \((V,\lambda _V,J_V)\) satisfying \(\lambda _V=-\rmd \psi \circ J_V\).

The contactisation \((\R \times V,\rmd t+\lambda _V)\) of \((V,\lambda _V)\) is given by \((\R \times \C \times T^*B,\alpha _o)\) and the contact structure \(\ker \alpha _o\) is spanned by vectors of the form \(v-\lambda _V(v)\partial _t\), \(v\in TV\). Using coordinates \(s\) on the first \(\R \)-factor of \(\R \times (\R \times V)\) we define \(J\) by requiring \(J(\partial _s)=\partial _t\) and

\[ J\big (v-\lambda _V(v)\partial _t\big ) = J_Vv-\lambda _V(J_Vv)\partial _t \]

for all \(v\in TV\). In other words, \(J\) is a \(s\)-translation invariant almost complex structure on \(\R \times (\R \times V)\) that preserves the contact distributions \(\ker \alpha _o\) on all slices \(\{s\}\times \R \times V\).

Remark 3.1.1.
The form \(\rmd (s\alpha _o)=\rmd s\wedge \alpha _o+s\rmd \alpha _o\) is symplectic on \(\{s>0\}\) and compatible with \(J\). Therefore, the function \((s,t,z,u)\mapsto \tfrac 12s^2\) is strictly plurisubharmonic on \(\{s>0\}\) because \(\alpha _o=-\rmd s\circ J\).

By [55], Proposition 5 the Niederkrüger map

\[ \Phi (s,t,z,u)=\big (s-\psi (z,u)+\rmi t,z,u\big ) \]

is a biholomorphic map

\[ \Phi \co (\R \times \R \times \C \times T^*B,J) \lra (\C ^2\times T^*B,\rmi \oplus J_{T^*B}) \;, \]

which maps the hypersurface \(\{s=0\}\) onto \(\{s\circ \Phi ^{-1}=0\}=\{x_1=-\psi (z,u)\}\). As in [55], Proposition 3.2 we consider a \((n-1)\)-dimensional family of holomorphic discs

\[ \{-\varepsilon ^2\}\times \D _{2\varepsilon }\times \{b\} \]

in \((\C ^2\times T^*B,\rmi \oplus J_{T^*B})\) with parameters \(\varepsilon \in \R ^+\), \(b\in B\). Here, we denote by \(\D _r\subset \C \) the closed disc with radius \(r\) and centre \(0\). Writing \(\D \) for the closed unit disc \(\D _1\) the disc family can be parametrised by

\[ v_{\varepsilon ,b}(z)= \big ( -\varepsilon ^2,2\varepsilon \cdot z,b \big ) \]

for \(z\in \D \). The lifts \(u_{\varepsilon ,b}=\Phi ^{-1}\circ v_{\varepsilon ,b}\) via the Niederkrüger map are holomorphic maps

\[ (\D ,\partial \D )\lra \Big ( \R \times \R \times \C \times T^*B, \{0\}\times \{0\}\times \C ^*\times B \Big ) \]

given by

\[ u_{\varepsilon ,b}(z)= \Big ( \varepsilon ^2\big (|z|^2-1\big ),0,2\varepsilon \cdot z,b \Big ) \;. \]

We will refer to the \(u_{\varepsilon ,b}\) as local Bishop discs .

From [55], Proposition 6 we get local uniqueness :

Lemma 3.1.2.
For all simple \(J\)-holomorphic disc maps \(u\co \D \ra \R \times \R \times \C \times T^*B\) such that \(u(\partial \D )\subset \{0\}\times \{0\}\times \C ^*\times B\) there exist \(\varepsilon \in \R ^+\), \(b\in B\) and a Möbius transformation \(\varphi \co (\D ,\partial \D )\ra (\D ,\partial \D )\) such that \(u=u_{\varepsilon ,b}\circ \varphi \).

Proof.

Consider the Niederkrüger transform \(v=\Phi (u)\) of \(u\). The projection to the \(T^*B\)-factor is a \(J_{T^*B}\)-holomorphic disc with boundary on the zero section \(B\) and is therefore constant as by Stokes theorem the symplectic energy vanishes. So we are left with a holomorphic disc \(v=(f+\rmi g,v_2)\) in \(\C ^2\) such that the restriction to \(\partial \D \) satisfies \(f+\tfrac 14|v_2|^2=0\) and \(g=0\), because

\[ \Phi \big (\{0\}\times \{0\}\times \C ^*\times B\big ) =\big \{x_1=-\tfrac 14|z|^2,y_1=0,u=0\} \;. \]

The maximum and minimum principle implies that the harmonic function \(g\) vanishes identically so that \(f\) must be constant according to the classical Cauchy–Riemann equations. Write \(f=-\varepsilon ^2\) for some \(\varepsilon >0\). Observe, that \(\varepsilon \) indeed cannot vanish as a constant holomorphic disc is never simple. Hence, \(\frac {1}{2\varepsilon }v_2\) is a holomorphic self-map of \((\D ,\partial \D )\). Again by the simplicity assumption the degree of the restriction of \(\frac {1}{2\varepsilon }v_2\) to the boundary must be \(1\). The argument principle implies that \(\frac {1}{2\varepsilon }v_2\) is an automorphism which is given by a Möbius transformation.

We remark that the boundary circles

\[ u_{\varepsilon ,b}(\partial \D )= \{0\}\times \{0\}\times \partial \D _{2\varepsilon }\times \{b\} \]

of the local Bishop discs foliate \(\{0\}\times \{0\}\times \C ^*\times B\). Recall that a neighbourhood of \(\{0\}\times \{0\}\times \{0\}\times B\) corresponds to a neighbourhood of the binding \(B\) in \(N^*\).

3.2. Pseudo-convexity.

We consider a \(2n\)-dimensional almost complex manifold \((W,J)\) with non-empty boundary. Denote by \(M\) a boundary component \(M\subset \partial W\) and by \(\xi =TM\cap JTM\) the \(J\)-invariant hyperplane distribution along \(M\). Assume that there exists a smooth \(1\)-form \(\alpha \) on \(M\) such that \(\xi =\ker \alpha \) and that \(\rmd \alpha \) is \(J\)- positive on complex lines in \(\xi \) in the sense that \(\rmd \alpha (v,Jv)>0\) for all \(v\in \xi \), \(v\neq 0\). In other words, \((M,\xi )\) is a \(J\)- convex hypersurface of \((W,J)\) as defined in [23] .

In this situation, \(\xi \) is a contact structure with contact form \(\alpha \), cf. Remark 4.1.1 . Denoting by \(R\) the Reeb vector field of \(\alpha \) we additionally assume that \(-JR\) is outward pointing. In other words, \((M,\xi )\) is a \(J\)- convex boundary component of \((W,J)\). Observe, that \((W,J)\) is naturally oriented by the \(n\)-th power of any \(J\)-positive (and hence non-degenerate) \(2\)-form on \(W\). Therefore, the contact orientation \(\alpha \wedge (\rmd \alpha )^{n-1}\) on \(M\) and the boundary orientation on \(M\subset \partial W\) coincide.

Example 3.2.1.
The almost complex manifold \(\big ((0,1]\times \R \times \C \times T^*B,J\big )\) as constructed in Section 3.1 has \(J\)-convex boundary with strictly plurisubharmonic function \(\tfrac 12s^2\), see Remark 3.1.1 .

In fact, if \(M\) is compact, then \(M\subset \partial W\) is the regular zero-level set of a strictly plurisubharmonic function \(\varrho \) defined near \(M\) that is negative on the complement of \(M\), see [19], Lemma 2.7 . The precomposition \(\varrho \circ u\) with a holomorphic map \(u\co G\ra (W,J)\), \(G\subset \C \) open domain, is subharmonic where defined, and therefore satisfies the strong maximum principle . So, for example, non-constant holomorphic spheres in \((W,J)\) are uniformly bounded away from the boundary component \(M\subset \partial W\), which we assumed to be compact. Furthermore, in the case of a non-constant \(J\)-holomorphic disc \(u\co (\D ,\partial \D )\ra (W,M)\), we get \(u(\Int \D )\subset W\setminus M\) and the radial derivative

\[ 0< \rmd \big (\varrho \circ u\big )(\partial _r) = -\big (\rmd \varrho \circ J\big ) \Big (Tu(\partial _{\theta })\Big ) \]

is positive along \(\partial \D \) by the boundary lemma of E. Hopf . Because

\[ \xi = \ker (\rmd \varrho )\cap \ker \big (\!-\rmd \varrho \circ J\big ) \]

is co-oriented by the Reeb vector field of any contact form defining \(\xi \) as a co-oriented hyperplane distribution this means that the curve \(u(\partial \D )\subset M\) is an immersion positively transverse to \(\xi \). In particular, any such holomorphic disc \(u\) such that \(u|_{\partial \D }\) is an embedding must be simple, see [27], Lemma 4.5 .

3.3. Uniqueness of the germ near the binding.

Consider a \(2n\)-dimensional almost complex manifold \((W,J)\) that has a compact \(J\)-convex boundary component \((M,\xi )\) as described in Section 3.2 . Assume that \((M,\xi )\) contains a submanifold \(N\) supporting a bordered Legendrian open book \((B,\vartheta )\). By Section 2.3 a neighbourhood of the binding \(B\subset W\) is diffeomorphic to a neighbourhood of \(\{0\}\times \{0\}\times \{0\}\times B\) in \((-\infty ,0]\times \R \times \C \times T^*B\) such that the restriction to the boundaries \(M\) and \(\{0\}\times \R \times \C \times T^*B\) induces a contactomorphism. In addition, assume that the almost complex structure \(J\) of \(W\) corresponds to the one constructed in Section 3.1 under the diffeomorphism.

From [55], Proposition 7 we get semi-global uniqueness :

Lemma 3.3.1.
There exists a neighbourhood \(U_B\subset W\) of \(B\) such that for all simple \(J\)-holomorphic disc maps \(u\co (\D ,\partial \D )\ra (W,N^*)\) with \(u(\D )\cap U_B\neq \emptyset \) we have that \(u(\D )\) is contained in \(U_B\) and there exist \(\varepsilon \in \R ^+\), \(b\in B\) and a Möbius transformation \(\varphi \co (\D ,\partial \D )\ra (\D ,\partial \D )\) such that \(u=u_{\varepsilon ,b}\circ \varphi \).

Proof.

Using the above diffeomorphism we describe such a neighbourhood \(U_B\) as subset of \((-\infty ,0]\times \R \times \C \times T^*B\): For \(x_1<0\), \(y_1\in \R \) consider the complex hypersurfaces \(\{x_1+\rmi y_1\}\times \C \times T^*B\) in \(\big (\C ^2\times T^*B,\rmi \oplus J_{T^*B}\big )\). The intersection with the real hypersurface \(\{x_1=-\psi (z,u)\}\) is the sphere bundle in \(\underline {\C }\oplus T^*B\) given by \(|x_1|=\tfrac 14|z|^2+\frac 12g^{\flat }(u,u)\); the intersection with \(\{x_1\leq -\psi (z,u)\}\), therefore, is the corresponding disc bundle in \(\underline {\C }\oplus T^*B\). Here \(\underline {\C }\) denotes the trivial complex line bundle over \(B\). Hence, the complex hypersurfaces

\[ H_{x_1,y_1}:= \Phi ^{-1}\Big (\{x_1+\rmi y_1\}\times \C \times T^*B\Big ) \cap \{s\leq 0\} \]

foliate the complement of \(\{0\}\times \R \times \{0\}\times B\) in \(\big ((-\infty ,0]\times \R \times \C \times T^*B,J\big )\) including a foliation by their real boundaries. Then, by definition, \(U_B\) corresponds to

\[ U_B:= \Big (\{0\}\times (-\delta ,\delta )\times \{0\}\times B\Big ) \cup \bigcup _{|x_1|,|y_1|<\delta }H_{x_1,y_1} \]

for \(\delta >0\) sufficiently small, under the above mentioned identifying diffeomorphism.

Consider a simple \(J\)-holomorphic disc \(u\co (\D ,\partial \D )\ra (W,N^*)\) and suppose that \(G=u^{-1}(U_B)\) is not empty. Observe that \(G\subset \D \) is open. Restricting to \(G\) we write \(\Phi (u)=(f+\rmi g, v_2,v_3)\). If \(g\) is constant in a neighbourhood of a point in \(G\), then so is the holomorphic function \(f+\rmi g\). With the identity theorem this implies that \(f+\rmi g\) is constant on \(G\setminus \partial \D \) and, hence, on \(G\). Denoting the constant by \(f_o+\rmi g_o\) this translates into \(G=u^{-1}(H_{f_o,g_o})\) so that \(G\subset \D \) is closed also. Hence, \(G=\D \) by an open–closed argument, i.e. \(u(\D )\subset U_B\) and the claim follows with Lemma 3.1.2 .

It remains to show that the complementary case, namely that \(\{\rmd g=0\}\) has no interior points, cannot occur. Indeed, otherwise the holomorphic disc \(u(\D )\) and the complex hyperplane \(H_{x_1^*,y_1^*}\) intersect along finitely many points for \(x_1^*<0\), \(y_1^*\neq 0\). For that observe with Section 3.2 and Example 3.2.1 (suitably shifted in the \(s\)-direction) that the intersection is along interior points of \(u(\D )\). This follows because \(H_{x_1^*,y_1^*}\) and the boundary condition \(N^*\) for the holomorphic disc \(u\) are disjoint as

\[ \Phi \Big (\{0\}\times \{0\}\times \C ^*\times B\Big ) \subset \R _-\times \{y_1=0\}\times \C ^*\times B \;. \]

By positivity of local intersection numbers the total intersection number \(u\bullet H_{x_1^*,y_1^*}\) is positive. On the other hand this total intersection number is equal to the homological intersection of \([u]\in H_2(W,M)\) and \([\partial c]\in H_{2n-2}W\), where the \((2n-1)\)-chain \(c\) is given by

\[ c=\bigcup _{x\in [x_1^*,0]}H_{x,y_1^*} \;. \]

Indeed, the maximum principle implies that \(u(\Int \D )\) does not intersect \(M\) so that \(u(\D )\) and \(\partial c\cap M\) are disjoint. Hence,

\[ u\bullet H_{x_1^*,y_1^*}=[u]\cdot [\partial c]=0 \;. \]

This is a contradiction. In other words, \(\{\rmd g=0\}\) has to have an interior point.

3.4. Holomorphic model near the boundary.

As in Section 3.1 we define an almost complex structure on \(M(\varphi ^*)\): Choose a Riemannian metric \(g_{\theta }\) on \(F\) that smoothly depends on \(\theta \in \R \) such that \(g_{2\pi }=g_{\theta }=\varphi ^*g_{\theta -2\pi }\) for all \(\theta \in (2\pi -\varepsilon ,2\pi +\varepsilon )\) and \(\varepsilon >0\) small. For each \(\theta \in \R \) we define the kinetic energy on \(T^*F\) by

\[ k_{\theta }(u)=\frac 12g_{\theta }^{\flat }(u,u) \;,\quad u\in T^*F\;, \]

denoting by \(g_{\theta }^{\flat }\) the dual metric of \(g_{\theta }\). For each \(\theta \in [0,2\pi ]\) we construct an almost complex structure \(J_{\theta }\) on \(T^*F\) as on [48], Section 5.3 that is compatible with \(\rmd \lambda _{T^*F}\) and turns \(k_{\theta }\) into a strictly plurisubharmonic potential on \(T^*F\) in the sense of [28], Section 3.1 meaning that

\[ \lambda _{T^*F}=-\rmd k_{\theta }\circ J_{\theta }\;. \]

The almost complex structure \(J_{\theta }\) is uniquely determined by \(g_{\theta }\) and \(\rmd \lambda _{T^*F}\); therefore, \(J_{\theta }\) depends smoothly on \(\theta \) and satisfies \(J_{2\pi }=J_{\theta }=\varphi ^*J_{\theta -2\pi }\) for \(\theta \in (2\pi -\varepsilon ,2\pi +\varepsilon )\).

The metric on \([0,2\pi ]\times F\) obtained by taking the sum of the Euclidean metric and \(g_{\theta }\) for each \(\theta \in [0,2\pi ]\) descents to a metric \(g\) on the mapping torus \(M(\varphi )\). The induced kinetic energy function on \(M(\varphi ^*)\) is denoted by

\[ \psi (r,\theta ,u)=\tfrac 12r^2+k_{\theta }(u) \;. \]

The almost complex structure \(\rmi \oplus J_{\theta }\) on \(T^*[0,2\pi ]\times T^*F\) descents to a compatible almost complex structure \(J_g\) on \(M(\varphi ^*)\) and

\[ r\rmd \theta +\lambda _{T^*F}\equiv -\rmd \psi \circ J_g \]

modulo second order terms in \(|u|_{\theta }\), \(u\in T^*F\), in the sense of [54], Appendix E.5 . Indeed, the derivative of \(k_{\theta }(u)\) in \(\theta \)-direction contributes a term that locally is a quadratic form in the coordinates of \(u\in T^*F\). Consequently, the restriction of \(\rmd r\wedge \rmd \theta +\rmd \lambda _{T^*F}\) to \(\{u=0\}\) in \(M(\varphi ^*)\) is equal to \(-\rmd \big (\rmd \psi \circ J_g\big )\). As \(\rmd r\wedge \rmd \theta +\rmd \lambda _{T^*F}\) is positive on \((\rmi \oplus J_{\theta })\)-complex lines and equals \(-\rmd \big (\rmd \psi \circ J_g\big )\) modulo first order terms in \(|u|_{\theta }\), \(u\in T^*F\), we conclude that \(\psi \) is strictly plurisubharmonic in a neighbourhood of \(\{u=0\}\) in \(M(\varphi ^*)\).

We consider the almost complex manifold \((\C \times M(\varphi ^*),\rmi \oplus J_g)\) provided with the Liouville form \(s\rmd t+r\rmd \theta +\lambda _{T^*F}\), where we denote the coordinates on \(\C \) by \(s+\rmi t\). Observe that the almost complex structure

\[ J=\rmi \oplus J_g \]

is compatible with \(\rmd s\wedge \rmd t+\rmd r\wedge \rmd \theta +\rmd \lambda _{T^*F}\) and that the function

\[ \Psi (s+\rmi t,r,\theta ,u)=\tfrac 12s^2+\psi (r,\theta ,u) \]

is strictly plurisubharmonic in a neighbourhood of \(\{u=0\}\) in \(\C \times M(\varphi ^*)\). This holds because

\[ s\rmd t+r\rmd \theta +\lambda _{T^*F}\equiv -\rmd \Psi \circ J \]

modulo second order terms in \(|u|_{\theta }\), \(u\in T^*F\). Therefore, as above, the restriction of \(\rmd s\wedge \rmd t+\rmd r\wedge \rmd \theta +\rmd \lambda _{T^*F}\) to \(\{u=0\}\) in \(\C \times M(\varphi ^*)\) is equal to \(-\rmd \big (\rmd \Psi \circ J\big )\).

By rescaling the metric \(g_{\theta }\) on \(F\) by a constant if necessary we can assume that \(\Psi \) is strictly plurisubharmonic in a neighbourhood of \(\{\Psi =\tfrac 12\}\). The hypersurfaces \(\{\Psi =\tfrac 12\}\) and \(\{s=1\}\) are transverse to \(s\partial _s+r\partial _r+Y_{T^*F}\), which is a Liouville vector field w.r.t. the symplectic form \(\rmd s\wedge \rmd t+\rmd r\wedge \rmd \theta +\rmd \lambda _{T^*F}\). Therefore, the contraction into the symplectic form induces contact forms on both hypersurfaces. The induced contact form on \(\{s=1\}=\{1\}\times \rmi \R \times M(\varphi ^*)\) is \(\alpha _{\varphi }\); the one on \(\{\Psi =\tfrac 12\}\) is given by \(-\rmd \Psi \circ J\) along \(\{u=0\}\).

A reparametrisation of the flow of the Liouville vector field \(s\partial _s+r\partial _r+Y_{T^*F}\) yields a contact embedding of \(\{\Psi =\tfrac 12,s>0\}\) onto \(\{s=1\}\) w.r.t. the induced contact structures, see [10], Appendix A.1 . The hypersurfaces \(\{\Psi =\tfrac 12\}\) and \(\{s=1\}\) intersect along \(\{s=1,r=0,u=0\}\), on which the flow is stationary. Moreover, as we flow along the Liouville vector field \(s\partial _s+r\partial _r+Y_{T^*F}\) we observe that the multi level set \(\{\Psi =\tfrac 12,s>0, t=0, r\leq 0, u=0\}\) corresponds to \(\{1\}\times \{0\}\times \{r\leq 0, u=0\}\) in \(\{1\}\times \rmi \R \times M(\varphi ^*)\) under the contact embedding. The latter set was used in Section 2.4 to describe the germ of contact structure near the boundary of a bordered Legendrian open book; the boundary being \(\{\Psi =\tfrac 12,s>0, t=0, r=0, u=0\}\), which corresponds to \(\{1\}\times \{0\}\times \{r=0, u=0\}\).

The hypersurface \(\{\Psi =\tfrac 12\}\) carries a second contact structure given by

\[ \ker \big (\rmd \Psi \big )\cap \ker \big (\!-\rmd \Psi \circ J\big ) \,, \]

which turns \(\{\Psi =\tfrac 12\}\) into a \(J\)-convex boundary of \(\{\Psi \leq \tfrac 12\}\). The induced singular characteristic foliation on \(\{\Psi =\tfrac 12,s>0, t=0, r\leq 0, u=0\}\) coincides with the one described in the preceding paragraph, where the contact distribution this time is taken w.r.t. \(s\rmd t+r\rmd \theta +\lambda _{T^*F}\equiv -\rmd \Psi \circ J\) along \(\{u=0\}\). By uniqueness of the germ of a contact structure formulated in [50], Lemma 4.6 , a neighbourhood of \(\{\Psi =\tfrac 12,s>0, t=0, r\leq 0, u=0\}\) is contactomorphic to the contact structure we considered first. In other words, given a contact manifold \((M,\xi )\) containing a submanifold \(N\) that supports a bordered Legendrian open book, we obtain an alternative description of the germ of contact structure near the boundary \(\partial N\) presented in Section 2.4 .

3.5. Holomorphically blocking boundary.

Let \((W,J)\) be a \(2n\)-dimensional almost complex manifold so that a given contact manifold \((M,\xi )\) is a compact \(J\)-convex boundary component of \(W\), see Section 3.2 . Let \(N\) be a submanifold of \((M,\xi )\) that supports a bordered Legendrian open book \((B,\vartheta )\). In view of Section 3.4 we assume that a neighbourhood of the boundary \(\partial N\subset W\) is diffeomorphic to a neighbourhood of \(\{1\}\times \{0\}\times \{r=0, u=0\}\) in \(\{\Psi \leq \tfrac 12, s>0\}\) such that \(N\subset W\) and \(\{\Psi =\tfrac 12,s>0, t=0, r\leq 0, u=0\}\) correspond to each other diffeomorphically. Furthermore we assume that under the diffeomorphism the almost complex structure \(J\) of \(W\) corresponds to \(\rmi \oplus J_g\) on \(\{\Psi \leq \tfrac 12\}\) in \(\C \times M(\varphi ^*)\) inducing contactomorphisms on the boundary.

Similarly to [50], Lemma 4.7 we obtain the blocking lemma :

Lemma 3.5.1.
There exists a neighbourhood \(U_{\partial N}\subset W\) of \(\partial N\) such that for all \(J\)-holomorphic disc maps \(u\co (\D ,\partial \D )\ra (W,N^*)\) with \(u(\D )\cap U_{\partial N}\neq \emptyset \) are constant.

Proof.

For \(|s|<1\), \(t\in \R \) consider the complex hypersurfaces

\[ H_{s,t}:= \Big (\{s+\rmi t\}\times M(\varphi ^*)\Big ) \cap \{\Psi \leq \tfrac 12\} \]

of \(\{\Psi \leq \tfrac 12\}\) in \((\C \times M(\varphi ^*),\rmi \oplus J_g)\). Modulo the above identifying diffeomorphism \(U_{\partial N}\) corresponds to

\[ U_{\partial N}:= \Big (\{1\}\times (-\delta ,\delta )\times M(\varphi )\Big ) \cup \bigcup _{1-s,|t|<\delta }H_{s,t} \]

for \(\delta >0\) sufficiently small.

Let \(u\co (\D ,\partial \D )\ra (W,N^*)\) be a \(J\)-holomorphic disc such that the open set \(G=u^{-1}(U_{\partial N})\) is not empty. Write the restriction of \(u\) to \(G\) as \(u=(u_1=f+\rmi g, u_2)\) w.r.t. \((\C \times M(\varphi ^*),\rmi \oplus J_g)\). An argument similar to the last paragraph of the proof of Lemma 3.3.1 (that utilises \(J\)-convexity and positivity of intersections with the complex hyperplanes \(H_{s,t}\)) shows that \(\{\rmd g=0\}\) has an interior point. As in the second paragraph of the proof of Lemma 3.3.1 this shows that \(u_1=f_o+\rmi g_o\) is constant and that \(G=\D \), i.e. \(u(\D )\subset U_{\partial N}\).

The projection map \(M(\varphi ^*)\ra T^*S^1\) sends \(u_2\) to a smooth map \(v\co \D \ra T^*S^1\) such that \(v(\partial \D )\subset \{r\leq 0\}\simeq S^1\). In particular, the degree of \(v|_{\partial \D }\) must be zero so that \(v(\partial \D )\) is tangent to a fibre of \(T^*S^1\). Therefore, \(u(\partial \D )\) admits a point of tangency with a page of the Legendrian open book on \(N\). In view of the maximum principle by E. Hopf, which implies the positive transversality property formulated in Section 3.2 , this implies that \(u\) must be constant.

4. Tamed pseudo-convexity

Let \((W,J)\) be a \(2n\)-dimensional almost complex manifold that admits a compact \(J\)-convex boundary component \((M,\xi )\), see Section 3.2 . We assume that there exists a symplectic form \(\Omega \) on \(W\) that is \(J\)-positive on complex lines in \(TW\), i.e. \(J\) is tamed by \(\Omega \), cf. [23] . Define an odd-symplectic form on \(M\) by setting \(\omega :=\Omega |_{TM}\).

4.1. Magnetic symplectisation.

Let \(\alpha \) be a defining contact form for \(\xi \) on \(M\) such that \(\rmd \alpha \) is positive on complex lines in \((\xi ,J)\).

Remark 4.1.1.
As \(\omega \) is positive on complex lines in \((\xi ,J)\), it follows that for all non-zero \(v\in \xi \) the contraction \(\iota _v\omega \) does not vanish. In other words, \(\omega \) restricts to a symplectic form on \(\xi \). Choosing a symplectic basis for \((\xi ,\omega )\) of the form \(v_1,Jv_1,\ldots ,v_{n-1},Jv_{n-1}\) yields that \(\omega ^{n-1}\) is a positive volume form on \((\xi ,J)\). Furthermore the contact form \(\alpha \) does not vanish on the characteristic foliation given by \(\ker \omega \), i.e. \(\xi \) and \(\ker \omega \) intersect transversally. In fact, according to our orientation conventions, \(\alpha \wedge \omega ^{n-1}\) is a positive volume form on \(M\).

Observe, that the same reasoning applies to all \(2\)-forms that are positive on complex lines in \((\xi ,J)\). This shows positivity of \(\alpha \wedge (\rmd \alpha )^{n-1}\) which was used implicitly in Section 3.2 .

The symplectic neighbourhood theorem for hypersurfaces implies that there exist \(\varepsilon >0\) and a symplectic embedding

\[ \Big ((-\varepsilon ,0]\times M,\rmd (s\alpha )+\omega \Big ) \lra (W,\Omega ) \]

whose restriction to \(\{0\}\times M\) is the inclusion of \(M=\partial W\) into \(W\), cf. [52], Exercise 3.36 and [50], Remark 2.7 . Observe that

\[ \Big (\rmd (s\alpha )+\omega \Big )^n= \Big (\rmd s\wedge \alpha +s\rmd \alpha +\omega \Big )^n= n\rmd s\wedge \alpha \wedge \big (s\rmd \alpha +\omega \big )^{n-1} \,. \]

Therefore, we find \(\varepsilon >0\) and a large positive constant \(s_o\) such that, considered on \((-\varepsilon ,\infty )\times M\), \(\rmd (s\alpha )+\omega \) is symplectic on \((-\varepsilon ,\varepsilon )\times M\) and \((s_o,\infty )\times M\). In fact, using Remark 4.1.1 , \(\alpha \wedge \big (s\rmd \alpha +\omega \big )^{n-1}\) is a positive volume form on \(M\) for all positive \(s\) because \(\rmd \alpha \) and \(\omega \) are positive on complex lines in \((\xi ,J)\). Therefore, \(\rmd (s\alpha )+\omega \) is a symplectic form on \((-\varepsilon ,\infty )\times M\). Via gluing along \(\{0\}\times M\equiv M\subset \partial W\) using the above symplectic embedding we build a symplectic manifold, the so-called magnetic completion ,

\[ \big (\widetilde {W},\widetilde {\Omega }\big ):= (W,\Omega )\cup \Big ([0,\infty )\times M,\rmd (s\alpha )+\omega \Big ) \,. \]

4.2. Truncating the magnetic completion.

We continue the considerations in Section 4.1 . In addition, let \(N\subset (M,\xi )\) be a submanifold that carries the structure of a bordered Legendrian open book decomposition \((B,\vartheta )\). Choose contact embeddings of the model neighbourhood of the binding \(B\) (see Section 2.3 ) and of the alternative model neighbourhood of the boundary \(\partial N\) (see Section 3.4 ) into \((M,\xi =\ker \alpha )\). The push forward of the respective contact forms \(\alpha _o\) and the restriction of \(-\rmd \Psi \circ J\) to the tangent spaces of \(\{\Psi =\tfrac 12\}\) are equal to \(\rme ^h\alpha \) for a smooth function \(h\) on the images of the model neighbourhoods. Alter the contact form \(\alpha \) by cutting off \(h\) to \(0\) near the boundary of these images, so that the considered contact embeddings – after shrinking the model neighbourhoods a bit – are in fact strict. Observe that this conformal change of the contact form \(\alpha \) does not effect the property of \(\rmd \alpha \) to be positive on complex lines in \((\xi ,J)\).

Let \(s_o\) be a positive real number and consider the truncation

\[ \big (\hat {W},\hat {\Omega }\big ):= (W,\Omega )\cup \Big ([0,2s_o]\times M,\rmd (s\alpha )+\omega \Big ) \;. \]

The resulting contact embeddings of the model neighbourhoods into \(\{2s_o\}\times M\), which are strict up to conformal factor \(2s_o\) w.r.t. the contact form \(2s_o\alpha \), extend along collar directions to embeddings of the neighbourhood \(U_B\) constructed in Lemma 3.3.1 and of the neighbourhood \(U_{\partial N}\) constructed in Lemma 3.5.1 into \((-\infty ,2s_o]\times M\) in the following way: For the embedding of \(U_B\) simply cross with the identity in the \(s\)-direction; for the embedding of \(U_{\partial N}\) denote by \(Y\) the vector field on \(\{\Psi \leq \tfrac 12\}\) obtained by multiplying the Reeb vector field of the contact form \(-\rmd \Psi \circ J\) on the level sets of \(\Psi \) with \(-J\) and follow the flow lines of \(Y\) in backward time (taking time logarithmically). Observe that \(Y\) coincides with the Liouville vector field \(s\partial _s+r\partial _r+Y_{T^*F}\) along \(\{u=0\}\), see Section 3.4 .

The images of the neighbourhoods are again denoted by \(U_B\) and \(U_{\partial N}\). Taking \(s_o\) sufficiently large we achieve that \(U_B\cup U_{\partial N}\) fit into \([s_o,2s_o]\times M\). Push forward yields an almost complex structure \(J_o\) on \(U_B\cup U_{\partial N}\) that allows the conclusions of Lemmata 3.3.1 and 3.5.1 . We remark that \(J_o\) is invariant under translations in \(s\)-direction that shift off \(U_B\); along \([s_o,2s_o]\times \partial N\) the almost complex structure \(J_o\) is independent of \(s\).

Moreover, the symplectic form \(\rmd (s\alpha )\) is compatible with \(J_o\) on \(U_B\) and on \(U_{\partial N}\), see Remark 3.1.1 and Section 3.4 , resp. Furthermore \(J_o\) sends \(\partial _s\) to the Reeb vector field and preserves the contact distribution. Applying [52], Proposition 2.63(i) to the symplectic bundle

\[ \big (\xi ,\rmd (s\alpha )\big )\lra [s_o,2s_o]\times M \]

we extend \(J_o\) to an almost complex structure on \([s_o,2s_o]\times M\) keeping the properties just listed. In particular, \(\{2s_o\}\times M\) is a \(J_o\)-convex boundary independently of the conformal factor \(2s_o\), see Section 3.2 .

Placing the whole scenario to \([s_o,2s_o]\times M\) for \(s_o\) sufficiently large we can additionally assume that \(J_o\) is also tamed by the symplectic form \(\rmd (s\alpha )+\omega \) on \([s_o,2s_o]\times M\). This is possible because for \(s_o\) sufficiently large \(\rmd (s\alpha )=\rmd s\wedge \alpha +s\rmd \alpha \) dominates \(\rmd (s\alpha )+\omega =\rmd s\wedge \alpha +(s\rmd \alpha +\omega )\) on \(J_o\)-complex lines. With [52], Proposition 2.51 we extend \(J_o\) to a tamed almost complex structure \(\hat {J}\) on \(\big (\hat {W},\hat {\Omega }\big )\) that restricts to \(J\) on \(W\) and to \(J_o\) on \([s_o,2s_o]\times M\). Moreover, \(\{2s_o\}\times M\subset \partial \hat {W}\) is a \(\hat {J}\)-convex boundary component. We will refer to the construction of \(\big (\hat {W},\hat {\Omega },\hat {J}\big )\) as magnetic collar extension .

4.3. Deforming the Truncation.

Assuming exactness of \(\omega |_{TN}\) in the situation of Sections 4.1 and 4.2 the symplectic form in the magnetic collar extension \(\big (\hat {W},\hat {\Omega },\hat {J}\big )\) can be assumed to satisfy

\[ \hat {\Omega }=2s_o\rmd \alpha \qquad \text {on}\quad T\big (\{2s_o\}\times N\big ) \]

after deformation:

Write \(\omega =\rmd \beta \) in a neighbourhood of \(N\) taking a neighbourhood that strongly deformation retracts to \(N\). Extend \(\beta \) to a \(1\)-form on \(M\) that vanishes outside a larger neighbourhood. Define a \(2\)-form \(\eta :=\omega -\rmd (\varrho \beta )\) on \([s_o,2s_o]\times M\), where \(\varrho \) is a smooth function that vanishes on \(\{s\leq s_o\}\), equals \(1\) on \(\{s\geq 2s_o\}\), and satisfies \(0\leq \varrho '\leq 2/s_o\). We claim that for \(s_o\) sufficiently large

\[ \Big ([s_o,2s_o]\times M,\rmd (s\alpha )+\eta \Big ) \]

is symplectic. Indeed, spelling out the \(n\)-th power of \(\rmd (s\alpha )+\eta \) we find

\[ n\rmd s\wedge \big (\alpha -\varrho '\beta \big ) \wedge \Big (s\rmd \alpha +\omega -\varrho \rmd \beta \Big )^{n-1} \,. \]

For \(s_o\) sufficiently large \(\alpha -\varrho '\beta \) will be a contact form on all slices \(\{s\}\times M\), \(s\in [s_o,2s_o]\), so that, restricted to the related contact structures, \((s\rmd \alpha )^{n-1}\) is a positive volume form. Making \(s_o\) even larger \((s\rmd \alpha )^{n-1}\) dominates lower order terms in the \((n-1)\)-st power of \(s\rmd \alpha +\omega -\varrho \rmd \beta \) restricted to the mentioned contact structures.

Starting with the deformed symplectic structure corresponding to \(\rmd (s\alpha )+\eta \) the tamed complex structure \(\hat {J}\) can be constructed as in Section 4.2 . In order to achieve that \(\rmd (s\alpha )\) dominates

\[ \rmd (s\alpha )+\eta = \rmd s\wedge \big (\alpha -\varrho '\beta \big ) +\Big (s\rmd \alpha +\omega -\varrho \rmd \beta \Big ) \]

on \(J_o\)-complex lines on \([s_o,2s_o]\times M\) simply choose \(s_o\) sufficiently large.

We will refer to the construction of \(\big (\hat {W},\hat {\Omega },2s_o\alpha ,\hat {J}\big )\) as deformed magnetic collar extension .

4.4. Gromov compactness.

We consider a deformed magnetic collar extension of the \(\Omega \)-tamed almost complex structure \((W,J)\) as in Section 4.3 . The resulting tamed almost complex manifold together with the choice of contact form on the \(J\)-convex boundary component is denoted by \((W,\Omega ,\alpha ,J)\). In particular, the restriction of the \(2\)-forms \(\Omega \) and \(\rmd \alpha \) to the tangent spaces of the bordered Legendrian open book \((N,B,\vartheta )\subset (M,\xi =\ker \alpha )\) are equal as \(2\)-form on \(N\).

Notice, that the regular set \(N^*\) of \(N\) (see Section 2.1 ) is a totally real submanifold of \((W,J)\), i.e. \(TN^*\cap JTN^*\) is the zero section. Indeed, denoting by \(E\) the real linear span of \(v,Jv\) for a given tangent vector \(v\in T_pN^*\) the only possibility for the complex line \(E\) to be tangent to \(N^*\subset M\) is to be tangent to the page of \((B,\vartheta )\) through \(p\), which is Legendrian w.r.t. \(\xi =TM\cap JTM\). Positivity of \(\rmd \alpha \) on complex lines in \((\xi ,J)\) implies the vanishing of \(v\) because the pages of \((B,\vartheta )\) are Legendrian submanifolds, and, hence, have Lagrangian tangent spaces inside \((\xi ,\rmd \alpha )\).

Via the neighbourhood \(U_B\subset W\) of the binding \(B\subset N\) constructed in Lemma 3.3.1 we obtain an embedding relative boundary, a so-called local Bishop filling ,

\[ F\co \Big ( (0,\delta )\times \D \times B, (0,\delta )\times \partial \D \times B \Big )\lra (W,N^*) \]

for some \(\delta >0\) such that for all \((\varepsilon ,b)\in (0,\delta )\times B\) the maps \(u_{\varepsilon ,b}=F(\varepsilon ,\,.\,,b)\) are \(J\)-holomorphic discs \((\D ,\partial \D )\ra (W,N^*)\). Furthermore \(F\) extends smoothly to a map defined on \([0,\delta )\times \D \times B\) that maps \(\{0\}\times \D \times B\) to \(B\) via \((\varepsilon ,z,b)\mapsto b\).

We consider the moduli space \(\MM \) of \(J\)-holomorphic discs \(u\co (\D ,\partial \D )\ra (W,N^*)\) that are homologous in \(W\) relative \(N^*\) to one of the Bishop discs \(u_{\varepsilon ,b}\). For all \(u\in \MM \) we have the following:


  1. The degree of the map \(\vartheta \circ u\co \partial \D \ra S^1\), the so-called winding number of \(u\), is equal to \(1\). The boundary lemma of E. Hopf implies, that \(u(\partial \D )\) is an embedded curve in \(N^*\) positively transverse to \(\xi \). Hence, \(u\) is simple, see Section 3.2 .
  2. We find a \(2\)-chain \(C\) in \(N\) with boundary \(-u(\partial \D )\) such \(u(\D )+C\) is null-homologous in \(W\). Therefore, by applying Stokes theorem twice, we get that the symplectic energy of \(u\) satisfies

    \[ 0<\int _{\D }u^*\Omega =-\int _{C}\Omega =\int _{\partial \D }u^*\alpha \,, \]

    as \(\Omega =\rmd \alpha \) on \(TN\). Denote by \(\rmd \vartheta \) the pullback of \(\rmd \theta \) along \(\vartheta \co N\setminus B\ra S^1\). According to our co-orientation convention in Section 2.1 and the local models in Sections 2.3 and 2.4 we observe that \(\alpha |_{TN}=f\rmd \vartheta \) for a non-negative function \(f\) on \(N\), that vanishes precisely along the singular set \(B\cup \partial N\). Consequently, we get uniform energy bounds

    \[ 0<\int _{\D }u^*\Omega = \int _{\partial \D }u^*f\cdot (\vartheta \circ u)^*\rmd \theta \leq 2\pi \max f\,. \]

  3. The restriction of \(u\) to \(\partial \D \) is uniformly bounded away from the boundary \(\partial N\) as the intersection of \(u(\D )\) with \(U_{\partial N}\) is empty by Lemma 3.5.1 . Recall that if \(u(\D )\) intersects the neighbourhood \(U_B\) of the binding then \(u\) is a reparametrisation of a local Bishop disc \(u_{\varepsilon ,b}\), see Lemma 3.3.1 . We truncate the moduli space \(\MM \) (keeping the notation) by removing all holomorphic discs that are reparametrisations of \(u_{\varepsilon ,b}\) for \((\varepsilon ,b)\in (0,\delta /2)\times B\).

Remark 4.4.1.
Under the assumption of uniform \(C^0\) -bounds for \(\MM \), i.e. that there exists a compact subset of \(W\) that contains all holomorphic discs \(u(\D )\), \(u\in \MM \), we obtain: Any sequence of holomorphic discs in \(\MM \) admits a Gromov converging subsequence, see [25] . Observe that by \(J\)-convexity (see Section 3.2 ) no sequence of holomorphic discs \(u(\D )\), \(u\in \MM \), can escape the boundary component \(M\) of \(W\).

The total winding number of the Gromov limit \(\bfu \) must be \(1\) according to the properties of Gromov convergence, see [25] . Moreover, all individual winding numbers of non-constant disc bubbles of \(\bfu \) are positive by positive transversality, see the boundary lemma to E. Hopf in Section 3.2 . Therefore, \(\bfu \) contains precisely one disc component \(u_0\) that is necessarily simple and of winding number \(1\). In particular, \(u_0|_{\partial \D }\) is an embedding positively transverse to \(\xi \).

If the image of \(\bfu \) intersects \(U_B\), then \(\bfu \) does it along the disc component \(u_0\) by the maximum principle, see Section 3.2 . This implies that \(u_0\) is one of the Bishop discs \(u_{\varepsilon ,b}\) by Lemma 3.3.1 , so that there are in fact no bubbles in this situation. Indeed, potential sphere bubbles must be null-homologous or subject to an argument using the maximum principle. Therefore, any sequence of holomorphic discs in \(\MM \) that Gromov converges to \(\bfu \) with \(u_0(\D )\) intersecting \(U_B\) converges in \(C^{\infty }\) to \(u_0\) up to reparametrisation.

Consequently, \(\MM \) can be compactified to \(\overline {\MM }\) by adding all Gromov limits to \(\MM \). The resulting moduli space \(\overline {\MM }\) is compact in the sense that any sequence in \(\overline {\MM }\) admits a Gromov converging subsequence. The resulting limit objects \(\bfu \) share the properties mentioned in the proceeding remark. In particular, we obtain uniform gradient bounds near the boundary w.r.t. a given background metric: There exists constants \(\rho \in (0,1)\) and \(C>0\) such that for all \(\bfu \) in \(\overline {\MM }\) we have that \(|\nabla u_0|<C\) restricted to \(\D \cap \{|z|\geq \rho \}\), where \(u_0\) is the disc component of \(\bfu \) parametrised such that \(\vartheta \circ u_0(\rmi ^k)=\rmi ^k\) for \(k=0,1,2\).

5. Symplectic cobordisms

A symplectic cobordism is a compact \(2n\)-dimensional symplectic manifold \((W,\Omega )\) with boundary \(M:=\partial W\). We assume that \((W,\Omega )\) is connected and oriented via \(\Omega ^n\). The odd-symplectic form \(\omega :=\Omega |_{TM}\) is closed and maximally non-degenerate with \(1\)-dimensional kernel \(\ker \omega \). The line bundle \(\ker \omega \) on \(\partial W\) is trivialised by the restriction of the Hamiltonian vector field of a collar neighbourhood parameter to \(M=\partial W\subset W\). Therefore, one finds a \(1\)-form \(\alpha \) on \(M\) that does not vanish on \(\ker \omega \). The sign of \(\alpha \) defines an orientation on each component of \(\partial W\) via the volume form \(\alpha \wedge \omega ^{n-1}\). If the boundary orientation (induced by the outward pointing normal) coincides with the one given by \(\alpha \) we call the components of \(M=\partial W\) positive , otherwise negative . We will write

\[ \partial (W,\Omega )= -(M_-,\omega _-,\alpha _-) +(M_+,\omega _+,\alpha _+) \]

accordingly. Due to the symplectic neighbourhood theorem there exist collar neighbourhoods \([0,\varepsilon )\times M_-\), resp., \((-\varepsilon ,0]\times M_+\), such that the symplectic form \(\Omega \) can be written as \(\rmd (s\alpha _{\mp })+\omega _{\mp }\) with \(s\in [0,\varepsilon )\), resp., \(s\in (-\varepsilon ,0]\). This allows gluing of symplectic cobordisms along boundary components of opposite sign that are orientation reversing odd-symplectomorphic. The most prominent examples of symplectic cobordisms have contact type boundary, i.e. the \(1\)-form \(\alpha \) on \(M\) can be chosen such that \(\omega =\rmd \alpha \), see [51] . In the contact type context positive boundary components are called convex ; negative ones concave .

5.1. A directed symplectic cobordism.

We consider a symplectic cobordism \((W,\Omega )\). We assume that the boundary \(\partial (W,\Omega )\) decomposes into concave boundary components, whose union we denote by \((M_-,\omega _-,\alpha _-)\), and positive boundary components, whose union we denote by \((M_+,\omega _+,\alpha _+)\). In addition, we require the weak-filling condition : \(\alpha _+\) can be chosen to be a contact form, which according to our conventions implies that \(\alpha _+\wedge (\rmd \alpha _+)^{n-1}\) and \(\alpha _+\wedge \omega _+^{n-1}\) are positive, such that

\[ \alpha _+\wedge \big (f_+\rmd \alpha _++\omega _+\big )^{n-1} >0 \]

for all non-negative smooth functions \(f_+\) on \(M_+\). We call \((W,\Omega )\) a directed symplectic cobordism , cf. [24] .

Remark 5.1.1.
Observe that if \(M_-\) is empty, \((W,\Omega )\) will be a weak symplectic filling of the contact manifold \((M_+,\xi _+)\) with contact structure \(\xi _+:=\ker \alpha _+\). If additionally \((M_+,\xi _+)\) is the convex boundary of the symplectic cobordism \((W,\Omega )\) with \(M_-=\emptyset \) then \((W,\Omega )\) is a strong symplectic filling of \((M_+,\xi _+)\).

As in [28] , [64] such symplectic cobordisms \((W,\Omega )\) can be used to verify the strong Weinstein conjecture for the contact manifold that appears as the concave boundary component of \((W,\Omega )\). The \(3\)-dimensional variant is related to the ball theorem, see [29], Theorem 2.2 and Corollary 3.8 :

Theorem 5.1.2.
Let \((W,\Omega )\) be a directed symplectic cobordism. Assume that the contact manifold \((M_+,\xi _+)\) contains a submanifold \(N\) with non-empty boundary such that \(N\) supports a bordered Legendrian open book \((B,\vartheta )\) and such that \(\omega _+|_{TN}\) is exact. Furthermore assume that one of the following conditions is satisfied:

  1. (i) The symplectic cobordism \((W,\Omega )\) is semi-positive.
  2. (ii) The second Stiefel–Whitney class \(w_2(TN^*)\) of \(N^*=N\setminus (B\cup \partial N)\) vanishes; or \(N^*\) is orientable and there exists a class in \(H^2(W;\Z _2)\) that restricts to \(w_2(TN^*)\).

Then \(M_-\) necessarily is non-empty and for any \(\xi _-\)-defining contact form there exists a null-homologous Reeb link.

Theorem 5.1.2 part (i) is contained in [50] . We include a variant of the argument in Section 5.3 as guideline for the polyfold proof of part (ii). Following [54] we call a \(2n\)-dimensional symplectic manifold \((W,\Omega )\) semi-positive if the first Chern class \(c_1\) of \((W,\Omega )\) satisfies the following condition: \(c_1(A)\geq 0\) for all spherical homology \(2\)-classes \(A\) of \(W\) with \(c_1(A)\geq 3-n\) and \(\Omega (A)>0\). If \(2n\leq 6\) the condition is automatic. The proof of part (ii) of Theorem 5.1.2 is postponed to Section 7 .

We remark that the inclusion \(N^*\subset W\) induces in cohomology the restriction map \(H^2(W;\Z _2)\ra H^2(N^*;\Z _2)\). The long exact cohomology sequence with \(\Z _2\)-coefficients yields, that the restriction map is surjective if and only if the co-boundary operator \(H^2(N^*;\Z _2)\ra H^3(W,N^*;\Z _2)\) vanishes. Furthermore the choice of an orientation on \(N^*\) induces an orientation on each page \(\vartheta ^{-1}(\theta )\), \(\theta \in S^1\), via the co-orientation induced by \(\vartheta \). The binding is oriented via the boundary orientation of a page. Therefore, \(N\) is orientable if and only if \(N^*\) is.

Observe that the inclusion map \(f\co N^*\subset N\) induces \(TN^*=f^*TN\), so that naturality of the Stiefel–Whitney classes implies \(w_2(TN^*)=f^*w_2(TN)\). In particular, if \(w_2(TN)\) vanishes so does \(w_2(TN^*)\). Further, if the fibration \(\vartheta \) on \(N^*\) is trivial (as it is the case for the plastikstufe), e.g. a product of the page \(\vartheta ^{-1}(1)\) with \(S^1\), the second Stiefel–Whitney class \(w_2(TN^*)\) is equal to \(w_2\big (T\vartheta ^{-1}(1)\big )\) according to the Whitney cross product formula for the total Stiefel–Whitney class, cf. [16], Chapter 17 . In general, taking a connection on the fibration \(\vartheta \) we obtain a splitting of \(TN^*\) into the vertical \(\ker T\vartheta \) and horizontal subbundle. As the horizontal subbundle is isomorphic to the trivial bundle \(\vartheta ^*TS^1\) Whitney sum formula for the total Stiefel–Whitney class implies \(w_2(TN^*)=w_2\big (\!\ker T\vartheta \big )\). The square product of the \(2\)-dimensional Klein bottle shows that the latter not always equals the second Stiefel–Whitney class of a fibre.

Remark 5.1.3.
Consider a symplectic cobordism \((W,\Omega )\) that satisfies all the requirements of Theorem 5.1.2 . Notice that if \(M_-=\emptyset \), then \((W,\Omega )\) would be a weak symplectic filling of \((M_+,\xi _+)\). Hence, by Theorem 5.1.2 no such weak symplectic filling can exist.

Remark 5.1.4.
The exactness requirement for \(\omega _+|_{TN}\) in Theorem 5.1.2 is fulfilled e.g. if \((M_+,\xi _+)\) is the convex boundary of \((W,\Omega )\) or if the Legendrian open book \(N\) is small.

5.2. Completing the cobordism.

We consider the directed symplectic cobordism \((W,\Omega )\) from Theorem 5.1.2 . According to the contact type boundary condition along the negative boundary components of \((W,\Omega )\) the symplectic neighbourhood theorem allows a description of a collar neighbourhood of \(M_-\subset W\) as \([0,\varepsilon )\times M_-\) such that the symplectic form equals \(\Omega =\rmd (\rme ^s\alpha _-)\) with \(s\in [0,\varepsilon )\). Therefore, a partial completion over the concave boundary of \((W,\Omega )\) can be given by

\[ \Big ((-\infty ,0]\times M_-,\rmd (\rme ^s\alpha _-)\Big ) \cup (W,\Omega ) \]

via gluing along \(\{0\}\times M_-\equiv M_-\). Any other contact form defining \(\xi _-=\ker \alpha _-\) on \(M_-\) can be realised as the restriction to the tangent spaces of a graph over \(M_-\) inside \((-\infty ,\varepsilon )\times M_-\) up to a positive constant factor, cf. [28], Section 3.3 . A change of \((W,\Omega )\) by adding the super-level set of the graph to the directed symplectic cobordism will allow the verification of the strong Weinstein conjecture for a particular choice of contact form as announced in Theorem 5.1.2 . In fact, we will assume that \(\alpha _-\) is a generic perturbation of a given \(\xi _-\)-defining contact form which allows an application of the Gromov–Hofer compactness theorem as formulated in [15] . This is justifiable with the Arzelà–Ascoli theorem, cf. [28], Section 6.4 and [64], Section 6 .

On the negative end \(\big ((-\infty ,0]\times M_-,\rmd (\rme ^s\alpha _-)\big )\) we choose a shift invariant almost complex structure \(J_-\) that sends the Liouville vector field \(\partial _s\) to the Reeb vector field of \(\alpha _-\) and leaves \(\xi _-\) invariant such that \(J_-\) is compatible with the symplectic structure induced by \(\rmd \alpha _-\) on \(\xi _-\). Extend \(J_-\) to a tamed almost complex structure \(J\) on \((W,\Omega )\) such that \(\xi _+=TM_+\cap JTM_+\) and the positive boundary \((M_+,\xi _+)\) of \((W,\Omega )\) is \(J\)-convex, see [50], Theorem D . Further, we glue the deformed magnetic collar extension constructed in Sections 4.2 and 4.3 along \(M_+\equiv \{0\}\times M_+\) to build (keeping the notation) a symplectic manifold

\[ \big (\hat {W},\hat {\Omega }\big ):= \Big ((-\infty ,0]\times M_-,\rmd (\rme ^s\alpha _-)\Big ) \cup (W,\Omega )\cup \Big ([0,2s_o]\times M_+,\rmd (s\alpha _+)+\eta \Big ) \,. \]

The resulting almost complex structure is denoted by \(\hat {J}\). Notice that \(\hat {J}\) equals \(J_o\) on the neighbourhoods \(U_B\) and \(U_{\partial N}\) of \(B\) and \(\partial N\), resp. Here we think of \(B\) and \(\partial N\) as subsets of \(M_+\equiv \{2s_o\}\times M_+\). In particular, the results from Section 4.4 are available.

5.3. The semi-positivity case.

We prove Theorem 5.1.2 under assumption (i). Recall the moduli space \(\MM \) introduced in Section 4.4 . To cut out the Möbius reparametrisation group geometrically we define the moduli space \(\MM _{1,\rmi ,-1}\) to be the set of all holomorphic discs \(u\in \MM \) such that \(\vartheta \circ u(\rmi ^k)=\rmi ^k\) for \(k=0,1,2\). This allows to fix the disc reparametrisations for sequences in \(\MM _{1,\rmi ,-1}\) in the compactness formulation in Remark 4.4.1 .

We choose a base point \(b_o\) of \(B\) and an embedded curve \(\gamma \) inside the page \(\vartheta ^{-1}(1)\) that connects \(B\) and \(\partial N\) such that \(\gamma \) is given by \(\{b_o\}\times \big (D^2\cap \R _{\geq 0}\big )\) in the model description in Section 2.3 . We define the moduli space \(\MM _{\gamma }\) to be the set of all holomorphic discs \(u\in \MM _{1,\rmi ,-1}\) with \(u(1)\in \gamma \). In other words \(\MM _{\gamma }\) consists of all \(u\in \MM \) such that

\[ u(1)\in \gamma \,,\quad \vartheta \circ u(\rmi )=\rmi \,,\quad \vartheta \circ u(-1)=-1 \,. \]

The Maslov index of the Fredholm problem defined by \(\MM \) equals \(2\) (see [55], Proposition 8 or [27] ). With [68], Theorem 4.4 there is a generic choice of \(\hat {J}\) such that with the first dimension formula in [68], Theorem 3.7 (successively taking relations \(R=\emptyset \), \(R=\vartheta ^{-1}(1)\times \vartheta ^{-1}(\rmi )\times \vartheta ^{-1}(-1)\), and \(R=\gamma \times \vartheta ^{-1}(\rmi )\times \vartheta ^{-1}(-1)\)) the moduli spaces \(\MM \), \(\MM _{1,\rmi ,-1}\), and \(\MM _{\gamma }\) are smooth manifolds of dimension \(n+2\), \(n-1\), and \(1\), resp. By [68], Remark 3.6 we can assume that the generic perturbation of \(\hat {J}\) is supported in the complement of the union of the negative end \((-\infty ,0]\times M_-\) of \(\hat {W}\) and \(U_B\cup U_{\partial N}\). This is because all local Bishop discs are Fredholm regular by [55], Proposition 9 and because all holomorphic discs that are contained completely inside \(\big ((-\infty ,0]\times M_-\big )\cup U_B\cup U_{\partial N}\) are the local Bishop discs.

Moreover, the boundary component of \(\MM _{1,\rmi ,-1}\) that corresponds to the local Bishop filling \(F\) has a collar neighbourhood in \(\MM _{1,\rmi ,-1}\) diffeomorphic to \([0,1)\times B\) via \(F\). This results in a collar neighbourhood \([0,1)\times \{b_o\}\) in \(\MM _{\gamma }\), see Section 4.4 . By the blocking property of \(U_{\partial N}\) (see Section 3.5 ) the evaluation map \(\MM _{\gamma }\ra \gamma \), \(u\mapsto u(1)\), is not surjective. Invariance of the mod-\(2\) degree for proper maps, which counts the number of preimages modulo \(2\), implies that \(\MM _{\gamma }\) cannot be compact.

Proof of Theorem 5.1.2 part (i) .

Arguing by contradiction we suppose that there is a compact subset \(K\) of \(\hat {W}\) such that the holomorphic discs \(u(\D )\) are contained in \(K\) for all \(u\in \MM _{\gamma }\). In this situation \(\MM _{\gamma }\) can be compactified in the sense of Gromov, see Remark 4.4.1 . Observe that Gromov limiting stable holomorphic discs are contained in \(K\) also and have precisely one disc component that in addition must be simple. With [68] we can assume by an additional a priori perturbation of \(\hat {J}\) that the moduli spaces of simple stable maps that cover the stable maps in the Gromov compactification of \(\MM \) are cut out transversally. This perturbation can be supported in the complement of the union of \((-\infty ,0]\times M_-\) and \(U_B\cup U_{\partial N}\) because no holomorphic sphere can stay inside \(\big ((-\infty ,0]\times M_-\big )\cup U_B\cup U_{\partial N}\) completely by the maximum principle. But, similarly to the computations in [28], Section 6.3 , the moduli spaces of the covering simple stable holomorphic discs are of negative dimensions, hence, empty. This argument uses the semi-positivity assumption. Consequently, there is no bubbling off for the moduli space \(\MM _{\gamma }\); in other words \(\MM _{\gamma }\) is compact. This is a contradiction and therefore a compact subset \(K\) of \(\hat {W}\) that contains all holomorphic discs that belong to \(\MM _{\gamma }\) cannot exists.

Consequently, \(M_-\) is necessarily non-empty. Moreover, for any choice of \(\xi _-\)-defining contact form \(\alpha _-\) there exists a null-homologous Reeb link by the remarks made in Section 5.2 . The relevant formulation of Gromov–Hofer convergence is obtained by combining the convergences statements in [36] , [37] with [25] .

6. A Deligne–Mumford type space

In Section 7 the proof of Theorem 5.1.2 under assumption (ii) will be given. In preparation we discuss moduli spaces of stable nodal boundary un-noded discs. We follow [43], Section 2.1 , [18] , [42] and indicate modifications necessary in the presence of boundaries.

6.1. Boundary un-noded nodal discs.

Let \(S\) be an oriented surface that is equal to the disjoint union of one closed disc and a (possibly empty) finite collection of spheres. All connected components of \(S\) are provided with the standard orientation. Let \(j\) be an orientation preserving complex structure on \(S\) turning \((S,j)\) into a Riemann surface with boundary, i.e. \((S,j)\) admits a holomorphic atlas whose charts are given by open subsets of the closed upper half-plane.

We call a subset of \(\Int (S)\) consisting of two distinct points a nodal pair . Each finite collection \(D\) of pair-wise disjoint nodal pairs defines an equivalence relation on \(S\) calling two points equivalent if and only if they from a nodal pair. The set \(S/D\) of equivalence classes is provided with the quotient space topology.

Let \(D\) be a finite collection of pair-wise disjoint nodal pairs such the quotient space \(S/D\) is simply connected. We call \((S,j,D)\) a boundary un-noded nodal disc . A point of \(S\) that belongs to a nodal pair in \(D\) is called a nodal point . The set of nodal points is denoted by \(|D|\). Observe that \(|D|\) and \(\partial S\) are disjoint.

Let \(m_0,m_1,m_2\) be pair-wise distinct marked points on the boundary \(\partial S\) ordered according to the boundary orientation of \(\partial S\). We call \(\big (S,j,D,\{m_0,m_1,m_2\}\big )\) a marked boundary un-noded nodal disc . Two marked boundary un-noded nodal discs

\[ \big (S,j,D,\{m_0,m_1,m_2\}\big ) \quad \text {and} \quad \big (S',j',D',\{m'_0,m'_1,m'_2\}\big ) \]

are equivalent if there exists a diffeomorphism \(\varphi \co S\ra S'\) such that \(\varphi ^*j'=j\), the injection \(D\ra D'\) defined by \(\{\varphi (x),\varphi (y)\}\in D'\) for all \(\{x,y\}\in D\) is onto, and \(\varphi (m_k)=m'_k\) for \(k=0,1,2\). Observe that \(\varphi \) necessarily preserves orientations.

6.2. Domain stabilisation.

In Section 7.2 boundary un-noded nodal discs will appear as the domain of stable maps. If the domain nodal discs have sphere components, the nodal discs will be unstable. In order to obtain a natural groupoidal structure on the space of marked boundary un-noded nodal discs we have to stabilise these by adding marked points. A point that is a marked point or a nodal point is called special . We call a connected component \(C\) of \(S\) stable if the number of special points on \(C\) is greater or equal than \(3\). In particular the disc component of \(S\) is stable.

We consider equivalence classes of stable discs \(\big [S,j,D,\{m_0,m_1,m_2\},A\big ]\) where \(\big (S,j,D,\{m_0,m_1,m_2\}\big )\) is a marked boundary un-noded nodal disc as in Section 6.1 that we provide with an additional finite set of auxiliary marked points \(A\subset S\setminus \partial S\) in the complement of \(|D|\) so that \(\#\big ((A\cup |D|)\cap C\big )\geq 3\) for each sphere component \(C\) of \(S\). In particular, all components \(C\) of \(S\) are stable. The equivalence relation is given by diffeomorphisms \(\varphi \co S\ra S'\) as in Section 6.1 such that in addition \(\varphi \) maps \(A\) bijectively onto \(A'\).

The set of all equivalence classes \(\RR \) is a nodal Riemann moduli space . Given a non-negative integer \(N\) we denote by \(\RR _N\subset \RR \) the subset of stable nodal discs that are equipped with precisely \(N=\#A\) auxiliary marked points so that \(\RR \) is the disjoint union over all \(\RR _N\), \(N\geq 0\). The elements in \(\RR _N\) can be represented by stable nodal discs \(\big (S,j,D,\{m_0,m_1,m_2\},A\big )\) of different stable nodal type \(\tau \), which is an isomorphism class of weighted rooted trees. The vertices are given by the components of \(S\), where the root corresponds to the disc component. All vertices are weighted by the number of (auxiliary) marked points on the corresponding component of \(S\). The edge relation is given by the nodes in \(D\). Observe that for given \(N\) the number of stable nodal types corresponding to stable discs \(\big (S,j,D,\{m_0,m_1,m_2\},A\big )\) with \(N=\#A\) is finite so that \(\RR _N\) is a finite disjoint union of subsets of stable discs \(\RR _{\tau }\subset \RR \) of the same stable nodal type \(\tau \).

6.3. Groupoid as an orbit space.

Let \(\tau \) be a stable nodal type. In order to rewrite \(\RR _{\tau }\) as an orbit space we choose natural representatives of the stable nodal marked discs \(\big [S,j,D,\{m_0,m_1,m_2\},A\big ]\) in \(\RR _{\tau }\) as follows: We fix the oriented diffeomorphism types of \(\C P^1\) and \(\D \) for the components of \(S\) including the choice \(\{1,\rmi ,-1\}\) for the marked points \(\{m_0,m_1,m_2\}\), i.e. \(m_k=\rmi ^k\), \(k=0,1,2\). We denote by \(\sigma \) the area form on \(S\) that is the Fubini–Study form on the \(\C P^1\) components and equals \(\rmd x\wedge \rmd y\) on \(\D \) taking conformal coordinates \(x+\rmi y\). Let \(\JJ \equiv \JJ _S\) be the space of orientation preserving complex structures on \(S\), which equals the space of almost complex structures on \(S\) tamed by \(\sigma \), cf. [1] , [63] . Furthermore we fix a selection of special points \(|D|\) and \(A\). By \(\GG \equiv \GG (S,D,\{1,\rmi ,-1\},A)\) we denote the group of orientation preserving diffeomorphisms of \(S\) that preserve \(\{1,\rmi ,-1\}\) point-wise and inject \(A\) onto \(A\) and \(D\) onto \(D\), resp.

We identify the nodal Riemann moduli space \(\RR _{\tau }\) with the orbit space

\[ \RR _{\tau }=\JJ /\GG \, \qquad \text {via}\quad \big [S,j,D,\{1,\rmi ,-1\},A\big ]\equiv [j]\,, \]

cf. [61], p. 612 or [67], Section 4.2 . The action

\[ \GG \times \JJ \lra \JJ \,,\quad (\varphi ,j)\longmapsto \varphi ^*j\,, \]

of \(\GG \) on \(\JJ \) is given by the pull back

\[ \varphi ^*j:=T_{\varphi }\varphi ^{-1}\circ j_{\varphi }\circ T\varphi \]

for \(\varphi \in \GG \) and \(j\in \JJ \). By [61], Lemma 7.5 or [67], Lemma 4.2.8 this action is proper, see also Remark 6.3.2 below. The action is free if and only if all isotropy subgroups \(\GG _j\), \(j\in \JJ \), of \(j\)-holomorphic maps in \(\GG \) are trivial. The action is locally free because all isotropy subgroups \(\GG _j\) are finite by the following Remark 6.3.1 :

Remark 6.3.1.
Each connected component of \(S\) is provided with at least \(3\) special points, see Section 6.2 . Hence, all isotropy subgroups \(\GG _j\) are finite :

To see this fix a biholomorphic identification of \((S,j)\) with the surface given by the disjoint union of \((\D ,\rmi )\) and an at most finite number of copies of \((\C P^1,\rmi )\). This is possible by uniformisation, cf. [1] and [54], Theorem C.5.1 , [63], Satz 5.33 for boundary regularity. For the marked points we can assume that \(m_k=\rmi ^k\), \(k=0,1,2\). Then any automorphism in \(\GG _j\) conjugates to an \(\rmi \)-holomorphic map that restricts to the identity on \((\D ,\rmi )\) and defines Möbius transformations of \((\C P^1,\rmi )\) corresponding to the maps induced between the not necessarily identical sphere components. We get a finite number of possibilities to obtain those Möbius transformations each of which is permuting the set of special points that admits at least \(3\) points by the stability condition.

Remark 6.3.2.
In order to describe the topology for fixed stable nodal type provide \(\JJ \) with the \(C^{\infty }\)-topology, which is metrisable, complete and locally compact by the Arzelà–Ascoli theorem.

We provide \(\RR _{\tau }=\JJ /\GG \) with the quotient topology meaning that the open sets in \(\JJ /\GG \) are precisely those, whose preimage under the quotient map \([\,.\,]\co \JJ \ra \JJ /\GG \) is open. In particular, \([\,.\,]\) is continuous by definition. The quotient map \([\,.\,]\) is open because for any open subset \(\KK \) of \(\JJ \) the \([\,.\,]\)-preimage of \([\KK ]\) is equal to the union of all \(g\KK \), \(g\in \GG \), which is open. Hence, a neighbourhood base of the topology on \(\JJ /\GG \) is given by the family of subsets whose elements \([j]\) can be represented by complex structures \(j\) belonging to an open subset of \(\JJ \). Therefore, \(\JJ /\GG \) is a second countable locally compact and, hence, paracompact topological space.

In fact, \(\RR _{\tau }=\JJ /\GG \) is Hausdorff. This follows from the properness argument as follows: Consider a sequence \(u_{\nu }\) of equivalences

\[ u_{\nu }\co \big (S,j_{\nu },D,\{1,\rmi ,-1\},A\big ) \lra \big (S,k_{\nu },D,\{1,\rmi ,-1\},A\big ) \]

with \(j_{\nu }\ra j\) and \(k_{\nu }\ra k\) in \(\JJ \). We claim that \(u_{\nu }\) has a \(C^{\infty }\)-convergent subsequence whose limit \(u\) will be an equivalence

\[ u\co \big (S,j,D,\{1,\rmi ,-1\},A\big ) \lra \big (S,k,D,\{1,\rmi ,-1\},A\big ) \]

also, cf. [42], Proposition 3.25 .

It suffices to proof \(C^{\infty }\)-convergence because the limit \(u\) will be automatically an equivalence as \(u\) restricts to a degree \(1\) map on each component of \(S\). Restricting \(u_{\nu }\) to the components of \(S\) we obtain sequences of \(k_{\nu }\)-holomorphic diffeomorphisms \(v_{\nu }\) one sequence for each component of \((S,j_{\nu })\). As the degree of each \(v_{\nu }\) equals \(1\) viewed as map onto its image, the area \(\int _Cv_{\nu }^*\sigma =\pi \), \(C\) being \(\D \) or \(\C P^1\), is uniformly bounded via the transformation formula. Hence, we find a subsequence of \(u_{\nu }\) so that all corresponding sequences \(v_{\nu }\) converge in the sense of Gromov, see [25] . Again using that the degree of all \(v_{\nu }\) is \(1\) we see that only one of the potential bubbles of each Gromov limit can intersect \(0\in C\); the remaining bubbles would be necessarily constant as their area vanish. In other words, the chosen subsequence of \(u_{\nu }\) converges in \(C^{\infty }\), because the reparametrisations by \(j_{\nu }\)-holomorphic diffeomorphisms are fixed, i.e. equal \(\id \), due to the stability condition.

We verify the Hausdorff property, cf. [42], Proposition 3.19 : Assume that any pair of neighbourhoods of given points \([j]\) and \([k]\), resp., intersects non-trivially. Taking shrinking neighbourhoods of the corresponding points \(j\) and \(k\) in \(\JJ \) we find \(j_{\nu }\ra j\) and \(k_{\nu }\ra k\) in \(\JJ \) such that \([j_{\nu }]=[k_{\nu }]\) for all \(\nu \). Then the above properness argument yields \([j]=[k]\).

6.4. Infinitesimal action.

We assume the situation of Section 6.3 . Denote by \(\Omega ^0\) the Lie algebra given by the tangent space of \(\GG \) at the identity diffeomorphism, which is the space of vector fields on \((S,\partial S)\) that are stationary on the set of all special points. In other words, \(\Omega ^0\) is the set of all smooth sections of \(TS\) that are tangent to \(\partial S\) and vanish on \(|D|\cup \{1,\rmi ,-1\}\cup A\). We denote by \(\Omega ^{0,1}_j\) the space of all endomorphism fields of the tangent bundle of \(S\) that anti-commute with \(j\). Linearising the equation \(j^2=-1\) we see that \(\Omega ^{0,1}_j\) is the tangent space of \(\JJ \) at \(j\). Viewing \(\Omega ^{0,1}_j\) as the set of all \(j\)-complex anti-linear \(TS\)-valued differential forms on \(S\), the infinitesimal action is

\[ \Omega ^0\times \Omega ^{0,1}_j\lra \Omega ^{0,1}_j \,,\quad (X,y)\longmapsto L_Xj+y \,. \]

A complex linear Cauchy–Riemann operator \(D\) is a \(j\)-complex linear operator that maps smooth vector fields of \((S,j)\) to \(\Omega ^{0,1}_j\) such that \(D(fX)=\DB f\cdot X+fDX\) for all smooth vector fields \(X\) and smooth functions \(f\), where \(\DB \) is the composition of the exterior derivative with the projection of the space of smooth \(1\)-forms onto those that anti-commute with \(j\), see [54], Appendix C.1 . Complex linearity can be expressed via \(D(jX)=jDX\) for all vector fields \(X\) of \(S\).

In order to compute the Lie derivative \(L_Xj\) we denote by \(\CR j\) the uniquely determined complex linear Cauchy–Riemann operator of the holomorphic line bundle \((TS,j)\) (ignoring boundary points) that agrees with

\[ \DB X=\tfrac 12\big (TX+\rmi \circ TX\circ \rmi \big ) \]

in local holomorphic coordinates \((\C ,\rmi )\), cf. [54], Remark C.1.1 . The local holomorphic representation \(\DB \) of \(\CR j\) implies that \(\CR j\) induces a real linear Cauchy–Riemann operator on the bundle pair \(\big ((TS,T\partial S),j\big )\) taking local holomorphic coordinates in the closed upper half-plane. Nevertheless the operator \(\CR j\co \Omega ^0\ra \Omega ^{0,1}_j\) is not complex linear because \(j\) does not induce a complex linear vector space structure on \(\Omega ^0\). Indeed, \(jX\) is not tangent to \(\partial S\) for all boundary points of \(S\) for which \(X\in \Omega ^0\) does not vanish.

With this preparation we compute

\[ L_Xj=\frac {\rmd }{\rmd t}\Big |_{t=0}\varphi _t^*j\,, \]

where \(\varphi _t\) is a smooth path in \(\GG \) through \(\varphi _0=\id \) with

\[ \frac {\rmd }{\rmd t}\Big |_{t=0}\varphi _t=X\,. \]

In local holomorphic coordinates \(\varphi _t^*j\) reads as

\[ T_{\varphi _t}\varphi _t^{-1}\circ \rmi \circ T\varphi _t\,. \]

Taking the time derivative at \(t=0\) and using \(\varphi _t^{-1}=\varphi _{-t}\) yields

\[ -TX\circ \rmi +\rmi \circ TX= \rmi \big (\rmi \circ TX\circ \rmi +TX\big )\,, \]

so that the Lie derivative is equal to

\[ L_Xj=2j\CR jX \,. \]

Remark 6.4.1.
Taking a path \(\varphi _t\) in the isotropy subgroup \(\GG _j\) through \(\varphi _0=\id \), meaning that the path \(\varphi _t\) in \(\GG \) satisfies \(\varphi _t^*j=j\) for all \(t\), we obtain \(X\in \ker \CR j\) by taking time derivative. Conversely, assuming \(\CR jX=0\) for a path \(\varphi _t\) in \(\GG \) through \(\varphi _0=\id \) yields

\[ \frac {\rmd }{\rmd t}\big (\varphi _t^*j\big )= \varphi _t^*\Big (2j\CR jX\Big )=0 \,, \]

i.e. that the path \(\varphi _t^*j\) in \(\JJ \) is constant, hence, equals \(j\). In other words, the tangent space at the identity of the group of all \(j\)-holomorphic maps in \(\GG \)

\[ T_{\id }\GG _j=\ker \CR j \]

equals the space of all \(j\)-holomorphic vector fields in \(\Omega ^0\).

Remark 6.4.2.
The Cauchy–Riemann operator is conformally invariant : Let \(\varphi \co (S,j)\ra (S,k)\) be a holomorphic diffeomorphism. Then \(\varphi ^*\circ \CR k=\CR j\circ \varphi ^*\). In particular, the Cauchy–Riemann operator \(\CR j\) commutes with the automorphisms of the Riemann surface with boundary \((S,j)\).

Remark 6.4.3.
Define a Riemannian metric \(g_j\) on \((S,j)\) by setting

\[ g_j(v,w)=\tfrac 12\big (\sigma (v,jw)+\sigma (w,jv)\big ) \,,\quad v,w\in TS\,, \]

where the area form \(\sigma \) is the one chosen in Section 6.3 . In particular, the complex structure \(j\) is orthogonal, so that the bilinear form \(g_j\) is a Hermitian metric . As any \(2\)-form on a surface is closed the \(2\)-form

\[ \sigma _j:=\tfrac 12(\sigma +j^*\sigma ) \]

is symplectic and compatible with \(j\). The latter means that \(g_j(v,w)=\sigma _j(v,jw)\) for all \(v,w\in TS\), so that the symplectic form \(\sigma _j\) is compatible with \(j\).

Denoting the Levi-Civita connection of \(g_j\) by \(\nabla \equiv \nabla ^{g_j}\), [52], Lemma 4.15 says that closedness of \(\sigma _j\) and integrability of \(j\) together are equivalent to \(\nabla j=0\), cf. Remark 6.4.4 below. In particular, \(\nabla (jX)=j\nabla X\) for all vector fields \(X\) of \(S\), so that \(\nabla \) is a Hermitian connection , i.e. \(\nabla \) is a complex linear metric connection. Hence,

\[ \big (\nabla X\big )^{0,1}:=\tfrac 12\big (\nabla X+j\circ \nabla X\circ j\big ) \]

defines a complex linear Cauchy–Riemann operator on \((TS,j)\), cf. [54], Remark C.1.2 . In local holomorphic coordinates we write \(\nabla X=TX+\Gamma (\,.\,,X)\) with help of the Christoffel symbols, so that the map \(X\mapsto \Gamma (\,.\,,X)\) is \(\rmi \)-complex linear. With symmetry of \(\Gamma \) we get \(\rmi \circ \Gamma (\rmi \,.\,,X)= \rmi \circ \Gamma (X,\rmi \,.\,)= -\Gamma (\,.\,,X) \), so that \(\big (\nabla X\big )^{0,1}=\DB X\). Therefore,

\[ \big (\nabla X\big )^{0,1}=\CR jX\,. \]

Furthermore we remark that the Hermitian connection \(\nabla \) is uniquely determined by this equation, see [54], Remark C.1.2 . Consequently, \(L_Xj=2j\CR jX\) can be obtained with the computations on [54], Theorem C.5.1 or [61], p. 631 as well.

Remark 6.4.4.
We give an alternative argument for the fact that \(j\) is parallel, which we used in Remark 6.4.3 : For any non-vanishing tangent vectors \(v,w\) at any given point of \(S\) consider a curve \(c\) tangent to \(v\) and extend \(w\) to a parallel vector field \(X\) along \(c\). As \(X\) and \(jX\) are orthogonal and as the length of \(jX\) is constant \(\nabla \) being metric implies that \(\nabla _{\dot c}(jX)\) is perpendicular to the span of \(\{X,jX\}\), and hence vanishes. Therefore, with the Leibnitz rule and parallelity of \(X\) we get \((\nabla _{\dot c}j)X=0\). Consequently, \(\nabla j=0\).

Observe that the argument works for all metrics (and corresponding Levi-Civita connections) for which \(j\) is orthogonal.

Remark 6.4.5.
All elements of \(\GG _j\) are isometries of \(g_j\). Indeed, by finiteness of \(\GG _j\) one finds for each \(\psi \in \GG _j\) a natural number \(k\) such that \(\psi ^k=\id \). On the other hand \(\psi \) pulls \(g_j\) back to \(fg_j\) for some positive function \(f\) on \(S\) by the description in Remark 6.4.3 and the fact that all positive area forms on a surface are positively proportional. Therefore, the conformal factor of the pull-back of \(g_j\) by \(\psi ^k\) becomes \(f^k\), which necessarily is \(1\). Hence, \(f=1\).

Remark 6.4.6.
Let \((\varphi _t,j_t)\) be a smooth path in \(\GG \times \JJ \) through \((\varphi _0,j_0)=(\psi ,j)\) and denote the velocity vector field by

\[ \frac {\rmd }{\rmd t}(\varphi _t,j_t)=\big (X_t,y_t\big ) \in T_{\varphi _t}\GG \times T_{j_t}\JJ \,. \]

The corresponding velocity vector field of \(\varphi _t^*j_t\) equals

\[ \frac {\rmd }{\rmd t}\big (\varphi _t^*j_t\big )= \varphi _t^*\Big (2j_t\CR {j_t}X_t+y_t\Big ) \in T_{\varphi _t^*j_t}\JJ \,. \]

If \(\psi \in \GG _j\) we obtain with \((X,y)=(X_0,y_0)\) that

\[ \frac {\rmd }{\rmd t}\Big |_{t=0}\big (\varphi _t^*j_t\big )= \psi ^*\Big (2j\CR jX+y\Big ) \in T_j\JJ \,, \]

which is equal to

\[ 2j\CR j\big (\psi ^*X\big )+\psi ^*y \,. \]

Indeed, this follows with Remark 6.4.2 or with Gauß's theorema egregium which gives \(\psi ^*\circ \CR j=\CR j\circ \psi ^*\) because all \(\psi \in \GG _j\) are isometries of \(g_j\), see Remark 6.4.5 . Consequently, the corresponding infinitesimal action reads as

\[ T_{\psi }\GG \times \Omega ^{0,1}_j\lra \Omega ^{0,1}_j \,,\quad (X,y)\longmapsto 2j\CR j\big (\psi ^*X\big )+\psi ^*y \]

for all \(\psi \in \GG _j\). Observe that the infinitesimal action \(2j\CR j\oplus \mathbbm {1}\) at \((\id ,j)\) sends \(\big (\psi ^*X,\psi ^*y\big )\in \Omega ^0\times \Omega ^{0,1}_j\) to the same element in \(\Omega ^{0,1}_j\).

6.5. A Fredholm index.

We compute the Fredholm index of the \(W^{1,3}\)-Sobolev completed Cauchy–Riemann operator \(\CR j\co W^{1,3}\ra L^3\) induced by the Cauchy–Riemann operator from Section 6.4 .

Ignoring zeros for the moment, for each component \(C\) of \(S\) the Fredholm index is given by the Riemann–Roch [54], Theorem C.1.10 applied to the \(j\)-complex \(1\)-dimensional bundle pair \((TC,T\partial C)\). Namely, the Fredholm index is the sum of the Euler characteristic of \(C\) and the Maslov index of \((TC,T\partial C)\). The Maslov index for \(C=\D \) is \(2\) by normalisation; for \(C=\C P^1\) twice the first Chern number, i.e. twice the Euler characteristic, which gives \(4\), see [54], Chapter C.3 . Hence, the Fredholm index is \(3\) restricted to the disc component and \(6\) on the spheres.

Now we take the zeros into account. Component-wise, for each boundary zero we have to subtract \(1\) from the computed Fredholm index; for each interior zero we subtract \(2\). Adding up, we obtain that \(\ind \CR j\) equals

\[ 3-\#\{1,\rmi ,-1\}-2\#\big ((|D|\cup A)\cap \D \big ) +2\sum _C\Big (3-\#\big ((|D|\cup A)\cap C\big )\Big ) \,, \]

where the sum is taken over all sphere components \(C\) of \(S\). This gives

\[ \ind \CR j= -2\#|D|-2\#A +6\big (\#\{C\}-1\big ) \,, \]

where \(\#\{C\}=\#D+1\) is the number of all components of \(S\). Using \(\#|D|=2\#D\) we finally obtain

\[ \ind \CR j=2\big (\#D-\#A\big ) \,. \]

On the other hand, by a boundary version of the argument principle (see [3], Theorem A.5.4 ), the Maslov index of \((TC,T\partial C)\) for each component \(C\) of \(S\) is the weighted sum of the number of zeros counted multiplicities of a non-zero element in the kernel of \(\CR j\), where interior zeros are counted twice. As the corresponding Maslov index is \(2\) on the disc component and \(4\) on the spheres, the kernel of \(\CR j\) is trivial due to the stability condition that the number of special points on each component \(C\) of \(S\) is at least \(3\). This argument uses elliptic regularity saying that the vector fields in \(\ker \CR j\) are smooth, see [54] . Therefore, one can show triviality of \(\ker \CR j=T_{\id }\GG _j\) (see Remark 6.4.1 ) alternatively using finiteness of \(\GG _j\) under the stability condition, see Remark 6.3.1 .

Using elliptic regularity as in [54] we see that the Cauchy–Riemann operator \(\CR j\co \Omega ^0\ra \Omega ^{0,1}_j\) is injective. The image is closed and has codimension \(2\big (\#A-\#D\big )\), cf. [43], Proposition 2.5 .

6.6. Interlude: Cayley transformation.

We provide \(\Omega ^{0,1}_j\) with the norm \(|y|_j\) given by the maximum of point-wise operator norms of \(y\) w.r.t. the metric \(g_j\). Because \(y\) is self-adjoint w.r.t. \(g_j\) the norm \(|y|_j\) is equal to the maximum of the square-root of the point-wise eigenvalues of the \(j\)-complex linear endomorphism field \(y\circ y\). In particular, the resolvent \((1-y)^{-1}\) of \(y\) at \(1\) is defined provided \(|y|_j<1\). We obtain a homeomorphism

\[ \mathfrak {i}\co \Omega ^{0,1}_j\cap B_1(0)\lra \JJ \,,\quad 0\longmapsto j \,, \]

defined on the open unit ball about zero via the conjugation

\[ y\longmapsto (1-y)j(1-y)^{-1} \,, \]

whose inverse is given by the

\[ k\longmapsto (k+j)^{-1}(k-j) \,, \]

cf. [7], Proposition 1.1.6 , [53], Proposition 2.6.4 or [61], p. 634 . Because \(\GG _j\) acts by isometries of \(g_j\) (see Remark 6.4.5 ) the conjugation map \(\mathfrak {i}\) is \(\GG _j\)-equivariant.

We claim that \(\JJ \) is a submanifold of the space \(\Omega ^1\) of all endomorphism fields of the tangent bundle of \(S\) and that \(\mathfrak {i}\) is a global chart. The case of almost complex structures compatible with \(\sigma \) essentially follows with the expositions in the above cited literature [7] , [53] , [61] . We will follow [31], Chapter I.7.3 taking the modifications for the case of almost complex structures only tamed by \(\sigma \) into account:

We call a not necessarily symmetric endomorphism field \(x\in \Omega ^1\) positive and write \(x>0\) provided that for all non-zero tangent vectors \(v\in TS\) the quadratic form \(g_j(v,xv)\) is positive. As the kernel of a positive endomorphism field \(x\in \Omega ^1\) is trivial we see that the inverse \(x^{-1}\in \Omega ^1\) exists. Therefore, for positive \(x\in \Omega ^1\) the endomorphism field \(1+x\) is positive as well such that the inverse \((1+x)^{-1}\) exists. In fact, the half space of all positive endomorphism fields \(\Omega ^1\cap \{x>0\}\) is an open cone in \(\Omega ^1\) closed under taking inverses. As above we provide \(\Omega ^1\) with the norm \(|x|_j\) given by the maximum of point-wise operator norms of \(x\in \Omega ^1\) w.r.t. the metric \(g_j\).

The Cayley transform

\[ \CC (x):=(1-x)(1+x)^{-1}=:\tilde {y} \]

defines a map

\[ \Omega ^1\cap \{x>0\}\lra \Omega ^1\cap B_1(0) \,. \]

Indeed, setting \(v=(1+x)^{-1}w\) polarisation yields \(4g_j(v,xv)=|w|_j^2-|\tilde {y}w|_j^2\), so that \(x\) is positive if and only if \(|\tilde {y}|_j<1\). We remark that there is an alternative formula

\[ \CC (x)=(1+x)^{-1}(1-x) \]

for the Cayley transform because \(1+x\) and \(1-x\) commute. Setting

\[ \CC (\tilde {y}):=(1-\tilde {y})(1+\tilde {y})^{-1} \]

we obtain a map

\[ \CC \co \Omega ^1\cap B_1(0)\lra \Omega ^1\cap \{x>0\} \]

in the converse direction. Again, this uses polarisation and that \(|\tilde {y}|_j<1\) implies triviality of the kernel of \(1+\tilde {y}\). Because the Cayley transform \(\CC \) is involutive the map \(\CC \co \Omega ^1\cap \{x>0\}\ra \Omega ^1\cap B_1(0)\) is a diffeomorphism.

Extending the conjugation map \(\mathfrak {i}\co \tilde {y}\mapsto (1-\tilde {y})j(1-\tilde {y})^{-1}\) to the open set \(\Omega ^1\cap B_1(0)\) yields a smooth map \(\Omega ^1\cap B_1(0)\ra \Omega ^1\). Observe, that \(\mathfrak {i}(\tilde {y})\) is a complex structure potentially reversing orientation. Restricting \(\mathfrak {i}\) to the \(j\)-complex anti-linear part \(\Omega ^{0,1}_j\) of \(\Omega ^1\) we get \(\mathfrak {i}(y)=j\CC (-y)\) for all \(y\in \Omega ^{0,1}_j\cap B_1(0)\). This defines an injection

\[ \mathfrak {i}=j\circ \CC \circ (-1)\co \Omega ^{0,1}_j\cap B_1(0)\lra \Omega ^1 \,. \]

In order to describe the image we observe that

\[ \CC \circ (-1)\co \Omega ^{0,1}_j\cap B_1(0)\lra \Omega ^1\cap \{x>0\}\cap \{jx=x^{-1}j\} \]

is a well defined homeomorphism with inverse \((-1)\circ \CC \). Additionally, the multiplication map \(j\co \Omega ^1\ra \Omega ^1\) is a diffeomorphism with inverse \(-j\) and restricts to the homeomorphism

\[ j\co \Omega ^1\cap \{x>0\}\cap \{jx=x^{-1}j\}\lra \JJ \,. \]

Indeed, positivity of \(x\) is equivalent to the positivity of \(\sigma _j(v,jxv)\) for all \(v\in TS\). Moreover, we find a smooth function \(f\) on the surface \(S\) such that the \(2\)-forms \(\sigma \) and \(\sigma _j\) satisfy \(\sigma =f\sigma _j\). Because \(\sigma (w,jw)=f|w|_j^2\) is positive for all non-zero \(w\in TS\) the function \(f\) must be positive. Hence, positivity of \(x\) is equivalent to the positivity of \(\sigma (v,jxv)\) for all \(v\in TS\), as \(\sigma _j\) and \(\sigma \) are positively proportional. It follows that the complex structure \(jx\) is tamed by \(\sigma \), i.e. preserves the orientation of the Riemann surface \((S,j)\). In total, the conjugation map

\[ \mathfrak {i}=j\circ \CC \circ (-1)\co \Omega ^{0,1}_j\cap B_1(0)\lra \JJ \]

is a well defined homeomorphism. The inverse is \(k\mapsto -\CC (-jk)=(k+j)^{-1}(k-j)\), where equality follows with the above alternative commuted formula for the Cayley transform. Furthermore \(\mathfrak {i}=j\circ \CC \circ (-1)\) is the restriction of the diffeomorphism obtained as the composite of \(\CC \circ (-1)\co \Omega ^1\cap B_1(0)\ra \Omega ^1\cap \{x>0\}\) with \(j\co \Omega ^1\ra \Omega ^1\) where defined. In other words, the inverse \((-1)\circ \CC \circ (-j)\) of \(j\circ \CC \circ (-1)\) serves as a global submanifold chart of \(\JJ \subset \Omega ^1\) the model being \(\Omega ^{0,1}_j\cap B_1(0)\subset \Omega ^1\).

In fact, \(\JJ \) is a complex manifold: A complex structure on the vector space \(\Omega ^{0,1}_j\) is given by \(y\mapsto jy\). An almost complex structure on \(\JJ \) is given by

\[\mathfrak {i}(y)=(1-y)j(1-y)^{-1}\]

on the tangent space \(T_{\mathfrak {i}(y)}\JJ =\Omega ^{0,1}_{\mathfrak {i}(y)}\) for all \(y\in \Omega ^{0,1}_j\cap B_1(0)\). Taking derivative of the equation

\[\mathfrak {i}(y)(1-y)=(1-y)j\]

w.r.t. \(y\) we get \(T_y\mathfrak {i}(\dot y)(1-y)-\mathfrak {i}(y)\dot y= -\dot y j \) and, using \(-\dot y j=j\dot y\), that

\[ T_y\mathfrak {i}(\dot y)= \big (j+\mathfrak {i}(y)\big )\dot y(1-y)^{-1} \]

for the linearisation of \(\mathfrak {i}\) at \(y\in B_1(0)\) for all tangent vectors \(\dot y\) of \(B_1(0)\subset \Omega ^{0,1}_j\). Using \(\mathfrak {i}(y)\big (j+\mathfrak {i}(y)\big )=\big (j+\mathfrak {i}(y)\big )j\) we obtain

\[ \mathfrak {i}(y)\circ T_y\mathfrak {i}=T_y\mathfrak {i}\circ j \,. \]

In other words, the linearisation \(T_y\mathfrak {i}\) is complex linear for all \(y\in \Omega ^{0,1}_j\cap B_1(0)\). Therefore, \(\mathfrak {i}\co \Omega ^{0,1}_j\cap B_1(0)\lra \JJ \) is biholomorphism.

Remark 6.6.1.
With [5], Corollary 6.4 one finds a further action by conjugation via \(y\mapsto \rme ^yj\rme ^{-y}\) for all \(y\in \Omega ^{0,1}_j\) defining a \(\GG _j\)-equivariant diffeomorphism \(\Omega ^{0,1}_j\ra \JJ \): To see this it is enough to argue fibre-wise. Identifying any given tangent space of \(S\) with \(\R ^2\) we claim that the space of all orientation preserving complex multiplications \(\JJ \) on \(\R ^2\) is the homogeneous space \(\PSl _2(\R )/\PSO _2\). Indeed, the group \(\Gl _2^+(\R )\) of orientation preserving invertible linear maps on \(\R ^2\) acts transitively on \(\JJ \) by conjugation \(A\mapsto A\rmi A^{-1}\) and the isotropy subgroup at \(\rmi \) is isomorphic to \(\Gl _1(\C )\), cf. [52], Proposition 2.48 . Normalising via the determinant and dividing out \(\pm 1\) this action descents to a transitive and faithful action of \(\PSl _2(\R )\) with isotropy subgroup \(\PSO _2\), as a conformal linear map that preserves the area necessarily preserves the metric. In particular, we see that \(\JJ \) is the hyperbolic upper half-plane \(\PSl _2(\R )/\PSO _2\), cf. [52], Exercise 4.17 .

The Lie algebra of \(\PSl _2(\R )\) decomposes as a vector space into the Lie algebra of \(\PSO _2\) and the set \(\Omega ^{0,1}_{\rmi }\) of all \(2\times 2\) matrices that anti-commute with \(\rmi \). Observe that the elements of \(\Omega ^{0,1}_{\rmi }\) are symmetric and trace-free. Therefore, the exponential map of the tangent space of \(\PSl _2(\R )/\PSO _2\) at \([1]\) can be written as

\[ \Omega ^{0,1}_{\rmi }\lra \PSl _2(\R )/\PSO _2 \,,\quad \, Y\longmapsto \big [\rme ^Y\big ] \,. \]

This map is a diffeomorphism because any \(A\in \Sl _2(\R )\) can be written uniquely as \(A=\rme ^SR\) for \(Y\in \Omega ^{0,1}_{\rmi }\) and \(R\in \SO _2\) by the polar form theorem. Therefore, the composition with \([A]\mapsto A\rmi A^{-1}\)

\[ \Omega ^{0,1}_{\rmi }\lra \JJ \,,\quad \, Y\longmapsto \rme ^Y\rmi \rme ^{-Y} \,, \]

is the diffeomorphism we wanted.

We remark that the composition with \([A]\mapsto A\cdot \rmi \), where \(A\cdot \rmi \) denotes the action of \(\PSl _2(\R )\) on the upper half-plane by Möbius transformations (which preserve the hyperbolic metric) is the exponential map \(Y\mapsto \rme ^Y\cdot \rmi \) of the hyperbolic upper half-plane at \(\rmi \).

6.7. The Kodaira differential.

We continue the considerations from Section 6.5 . For all \(j\in \JJ \) the operator \(j\CR j\co \Omega ^0\ra \Omega ^{0,1}_j\) is injective and

\[ H^1_j:=\Omega ^{0,1}_j/\im (j\CR j) \]

has real dimension \(2\big (\#A-\#D\big )\). Moreover, the operator \(j\CR j\) is \(\GG _j\)-equivariant by Remark 6.4.2 . Alternatively, argue with the theorema egregium and with Remark 6.4.5 as done in Remark 6.4.6 . Therefore, conjugation

\[ \psi ^*y:=T_{\psi }\psi ^{-1}\circ y_{\psi }\circ T\psi \]

by elements \(\psi \in \GG _j\) leaves \(\im (j\CR j)\) invariant, so that \(\GG _j\) induces an action on \(H^1_j\) via \(\psi ^*[y]:=[\psi ^*y]\).

Observe, that the complex structure \(y\mapsto jy\) on \(\Omega ^{0,1}_j\) introduced in Section 6.6 does not descent to a complex structure on the quotient \(H^1_j\). The reason is that the subspace \(\im (j\CR j)\) of \(\Omega ^{0,1}_j\) is not \(j\)-invariant as the operator \(j\CR j\co \Omega ^0\ra \Omega ^{0,1}_j\) is not complex linear, see Section 6.4 .

Choose a \(\GG _j\)-invariant complementary subspace \(E_j\subset \Omega ^{0,1}_j\) of \(\im (j\CR j)\) so that the quotient map \(y\mapsto [y]\) of \(\Omega ^{0,1}_j\) onto \(H^1_j\) restricts to a \(\GG _j\)-equivariant linear isomorphism \(E_j\ra H^1_j\).

Example 6.7.1.
A \(\GG _j\)-invariant complementary subspace \(E_j\) can be defined as the orthogonal complement of \(\im (j\CR j)\) w.r.t. to the \(L^2\)-inner product on \(\Omega ^{0,1}_j\) induced by a \(\GG _j\)-invariant metric on \(S\). Such a metric can be obtained via averaging any given metric over the finite set \(\GG _j\). The obtained \(\GG _j\)-invariant \(L^2\)-inner product on \(\Omega ^{0,1}_j\) can be symmetrised as in Remark 6.4.3 so that the action of \(j\) will be orthogonal in addition. Alternatively, a natural choice for \(\GG _j\)-invariant metric on \(S\) would be the following: The area form \(\sigma _j\) and the metric \(g_j\), both being \(\GG _j\)-invariant, together determine a Hodge star operator on \(TS\)-valued differential forms on \(S\), namely, via \(y\mapsto -y\circ j\). Restricting to elements \(y\in \Omega ^{0,1}_j\) this yields \(y\mapsto jy\) so that we obtain a \(\GG _j\)-invariant \(L^2\)-inner product on \(\Omega ^{0,1}_j\) by

\[ \langle y_1,y_2\rangle _j:= \frac 12\int _Sy_1\wedge jy_2 \,. \]

The wedge product of two \(TS\)-valued differential forms is defined component-wise w.r.t. local \(g_j\)-orthonormal frames. Using conformal coordinates one shows that the integrand \(y_1\wedge jy_2\) equals \(2\Re (y_1\circ y_2)\,\sigma _j\), where, point-wise, \(\Re (y_1\circ y_2)\) denotes the real part of the complex eigenvalue of the \(j\)-complex linear map \(y_1\circ y_2\in \Omega ^1\) between complex lines. This shows \(j\)- and \(\GG _j\)-invariance of the metric

\[ \langle y_1,y_2\rangle _j= \int _S\Re (y_1\circ y_2)\,\sigma _j \,, \]

whose induced norm \(\|y\|_j\) is given by the square-root of the integral of the point-wise eigenvalues of the \(j\)-complex linear endomorphism field \(y\circ y\) over \(S\) against \(\sigma _j\). Nevertheless, the orthogonal complement \(E_j\) of \(\im (j\CR j)\) in \(\Omega ^{0,1}_j\) of any \(j\)-invariant metric will not be invariant under \(j\) as \(\im (j\CR j)\) is not invariant under \(j\). In Section 6.9 we will construct a complex linear complement \(E_j\).

Consider a so-called deformation of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\), which is a map

\[ \mathfrak {j}\co (V_j,0)\lra (\JJ ,j) \,,\qquad y\longmapsto j(y) \,, \]

defined on an open neighbourhood \(V_j\subset E_j\) of \(0\). If \(\mathfrak {j}\) is an embedding whose image \(\mathfrak {j}(V_j)\) is transverse to the orbits of \(\GG \), then the deformation \(\mathfrak {j}\) is called effective , cf. the [67], Definition 4.2.13 of a local slice through \(j\). Transversality can be expressed via the invertibility of the so-called Kodaira differential

\[ [T_y\mathfrak {j}]\co E_j\lra \Omega ^{0,1}_{j(y)}\lra H^1_{j(y)} \]

for all \(y\in V_j\), which is the composition of the linearisation \(T_y\mathfrak {j}\) with the quotient map \([\,.\,]\). Furthermore we call the deformation \(\mathfrak {j}\) symmetric if \(V_j\) is \(\GG _j\)-invariant (e.g. taking metric balls about \(0\in E_j\) w.r.t. to the \(L^{\infty }\)-norm \(|\,.\,|_j\) from the beginning of Section 6.6 or the \(L^2\)-norm \(\|\,.\,\|_j\) induced by \(\langle \,.\,,\,.\,\rangle _j\) from Example 6.7.1 ) and \(\mathfrak {j}\) is \(\GG _j\)-equivariant. The latter means that for all \(y\in V_j\) and \(\psi \in \GG _j\) we have that \(\psi ^*\big (\mathfrak {j}(y)\big )=\mathfrak {j}(\psi ^*y)\) so that

\[ \psi \co \big (S,j(\psi ^*y),D,\{1,\rmi ,-1\},A\big ) \lra \big (S,j(y),D,\{1,\rmi ,-1\},A\big ) \]

is a holomorphic isomorphism. Finally, the deformation \(\mathfrak {j}\) is called complex provided that the complementary subspace \(E_j\subset \Omega ^{0,1}_j\) is invariant under \(j\), i.e. is a complex linear subspace, and that \(\mathfrak {j}\) is holomorphic in the sense that the differential \(T\mathfrak {j}\) is complex linear, i.e. \(\mathfrak {j}(y)\circ T_y\mathfrak {j}=T_y\mathfrak {j}\circ j\) for all \(y\in V_j\subset E_j\).

Example 6.7.2.
The Cayley transformation from Section 6.6 or the conjugation by the exponential map studied in Remark 6.6.1 yield symmetric effective deformations \(\mathfrak {j}\) restricting

\[ y\longmapsto (1+jy)j(1+jy)^{-1} \quad \text {or}\quad y\longmapsto \rme ^{jy}j\rme ^{-jy} \]

to \(V_j=E_j\cap \Omega ^{0,1}_j\cap B_1(0)\) or to \(V_j=E_j\), resp. Indeed, the differentials at \(0\in V_j\) in direction of \(\dot y\in E_j\) are given by \(\dot y\mapsto 2\dot y\). For complex linear \(E_j\) the corresponding deformation will be complex.

Remark 6.7.3.
The Kodaira differential is natural in the following sense: Consider deformations \(\mathfrak {j}\co V_j\ni y\mapsto j(y)\) and \(\mathfrak {k}\co V_k\ni z\mapsto k(z)\) of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) and \(\big (S,k,D,\{1,\rmi ,-1\},A\big )\), resp. Choose a linear isomorphism \(\zeta \co E_j\ra E_k\), which we will write as \(\zeta \co y\mapsto z(y)\). Let \(y\mapsto \varphi (y)\) be a smooth family of diffeomorphisms

\[ \varphi (y)\co \big (S,j(y),D,\{1,\rmi ,-1\},A\big ) \lra \Big (S,k\big (z(y)\big ),D,\{1,\rmi ,-1\},A\Big ) \]

defined on \(V_j\cap \zeta ^{-1}(V_k)\) and deforming the equivalence

\[ \varphi =\varphi (0)\co \big (S,j,D,\{1,\rmi ,-1\},A\big ) \lra \big (S,k,D,\{1,\rmi ,-1\},A\big ) \,. \]

Then the Kodaira differentials at \(0\) satisfy

\[ [T_0\mathfrak {j}]= \varphi ^*\circ [T_0\mathfrak {k}]\circ \zeta \,, \]

cf. [42], Proposition 1.6 . In particular, \(\mathfrak {j}\) is effective if and only if \(\mathfrak {k}\) is.

Indeed, choose \(\dot y\in E_j\) and write \(\mathfrak {j}_t=\mathfrak {j}(t\dot y)\), \(\varphi _t=\varphi (t\dot y)\), and \(\mathfrak {k}_t=\mathfrak {k}\big (\zeta (t\dot y)\big )\) for \(t\in (-1,1)\) and take the Lie derivative of \(\mathfrak {j}_t=\varphi _t^*\mathfrak {k}_t\). By conformal invariance of the Cauchy–Riemann operator \(\varphi ^*\circ k\CR k=j\CR j\circ \varphi ^*\) (see Remark 6.4.2 ) we obtain

\[ T_0\mathfrak {j}(\dot y)= 2j\CR j(\varphi ^*X)+\varphi ^*\Big (T_0\mathfrak {k}\big (\zeta (\dot y)\big )\Big ) \]

similarly to Remark 6.4.6 , where \(X\) is the velocity vector of the path \(t\mapsto \varphi _t\) in \(\GG \) at \(0\). As the restriction of \(\varphi _t\) to the special points in \(D\cup \{1,\rmi ,-1\}\cup A\) is constant by continuity of \(t\mapsto \varphi _t\) we obtain that \(X\in \Omega ^0\). Hence, \(\varphi ^*X\in \Omega ^0\) and therefore \(2j\CR j(\varphi ^*X)\) represents the zero class. The claim follows now because \(\varphi \) defines a well–defined isomorphism \(\varphi ^*\co H^1_k\ra H^1_j\) via \(\varphi ^*[y]:=[\varphi ^*y]\),

\[ \varphi ^*y:=T_{\varphi }\varphi ^{-1}\circ y_{\varphi }\circ T\varphi \,, \]

by the previous argument. Hence,

\[ [T_0\mathfrak {j}(\dot y)]= \varphi ^*\Big [T_0\mathfrak {k}\big (\zeta (\dot y)\big )\Big ] \]

for all \(\dot y\in E_j\).

If both deformations \(\mathfrak {j}\) and \(\mathfrak {k}\) are effective, then there is a tautological choice for an isomorphism \(\zeta \) for the given diffeomorphism \(\varphi \), namely \(\zeta =[T_0\mathfrak {k}]^{-1}\circ (\varphi ^*)^{-1}\circ [T_0\mathfrak {j}]\). On the other hand, in the situation of Example 6.7.1 , where the local slices are constructed via orthogonal complements, we get \(\varphi ^*E_k=E_j\) because \(g_j\) and \(\varphi ^*g_k\) are conformally equivalent. This allows the choice \((\varphi ^*)^{-1}\co E_j\ra E_k\) for \(\zeta \) and yields

\[ [T_0\mathfrak {j}]= \varphi ^*\circ [T_0\mathfrak {k}]\circ (\varphi ^*)^{-1} \,. \]

6.8. Orbifold structure – fixed stable nodal type.

In the situation of Section 6.7 we assume for the moment that the isotropy group \(\GG _j\) is trivial. Invertibility of the Kodaira differential \([T_y\mathfrak {j}]\) implies that the linear subspace \(T_y\mathfrak {j}(E_j)\) in \(\Omega ^{0,1}_{j(y)}\) is complementary to \(\im \big (j(y)\CR {j(y)}\big )\). With the arguments from [61], p. 634/5 and [67], Theorem 4.2.14 we obtain that

\[ \GG \times V_j\lra \JJ \,,\qquad (\varphi ,y)\longmapsto \varphi ^*\big (j(y)\big ) \,, \]

is a diffeomorphism onto a neighbourhood of the \(\GG \)-orbit of \(j=\id ^*\!\big (j(0)\big )\) for a sufficiently small open neighbourhood \(V_j\subset E_j\) of \(0\). In other words, the map \((\id ,y)\mapsto j(y)\) induces a homeomorphism

\[ (\id ,y)\longmapsto \big [S,j(y),D,\{1,\rmi ,-1\},A\big ]=\big [j(y)\big ] \]

defined on \(V_j\) onto a neighbourhood of \(\big [S,j,D,\{1,\rmi ,-1\},A\big ]=[j]\) in \(\RR _{\tau }=\JJ /\GG \). The inverse serves as a chart of a smooth manifold structure on \(\RR _{\tau }\).

For \(\GG _j\) non-trivial we give an equivariant version of the above construction: Assuming the situation of Section 6.7 we consider a symmetric effective deformation \(\mathfrak {j}\co (V_j,0)\ra (\JJ ,j)\), which we also denote by \(y\mapsto j(y)\). We would like to find a \(\GG \)-equivariant diffeomorphism

\[ \GG \times _{\GG _j} V_j\lra \JJ \,,\qquad (\varphi ,y)\longmapsto \varphi ^*\big (j(y)\big ) \,, \]

onto a neighbourhood of the \(\GG \)-orbit of \(j=\id ^*\!\big (j(0)\big )\), where \(\GG \times _{\GG _j} V_j\) is the quotient of \(\GG \times V_j\) by the action \((\varphi ,y)\mapsto \big (\psi ^{-1}\circ \varphi ,\psi ^*y\big )\), \(\psi \in \GG _j\).

In order to do so we would like to find an isomorphism

\[ \varphi \co \big (S,j(y),D,\{1,\rmi ,-1\},A\big ) \lra \big (S,k,D,\{1,\rmi ,-1\},A\big ) \]

for given \(k\in \JJ \) sufficiently close to \(j\in \JJ \) and for some \(y\in V_j\). Holomorphicity of \(\varphi \) translates to \(\varphi ^*k=j(y)\). In other words, \((\varphi ,y,k)\) is a zero of the non-linear Cauchy-Riemann operator

\[ F(\varphi ,y,k):=\frac 12\Big (T\varphi +k\circ T\varphi \circ j(y)\Big ) \,, \]

which is a section into the bundle \(\EE \ra \GG \times V_j\times \JJ \), whose fibre \(\EE _{(\varphi ,y,k)}\) is the vector space of sections of the bundle of complex anti-linear bundle homomorphisms from \(\big (TS,j(y)\big )\) to \((TS,k)\).

Setting \(F_k:=F(\,.\,,\,.\,,k)\) we will write the solutions \((\varphi ,y)\) of \(F_k(\varphi ,y)=0\) as a function of \(k\) via the implicit function theorem. The linearisation

\[ T_{(\id ,0)}F_j:\Omega ^0\times E_j\lra \Omega ^{0,1}_j \]

of \((\varphi ,y)\mapsto F_j(\varphi ,y)\) at \((\id ,0)\) equals

\[ (X,\dot y)\longmapsto \CR jX+\tfrac 12j\cdot \big (T_0\mathfrak {j}\big )(\dot y) \,. \]

With Sections 6.5 and 6.7 the operator

\[ -2j\cdot T_{(\id ,0)}F_j= -2j\CR j\oplus T_0\mathfrak {j} \]

is an isomorphism.

The implicit function theorem combined with an intermediate Sobolev completion and a subsequent elliptic regularity argument as in [61], p. 634/5 or in [67], Theorem 4.2.14 implies: There exists an open neighbourhood \(\KK \subset \JJ \) of \(j\), a possibly smaller \(\GG _j\)-invariant open neighbourhood \(V_j\subset E_j\) of \(0\), an open neighbourhood \(\HH \subset \GG \) of \(\id \) such that the sets \(\psi ^*\HH \) are pair-wise disjoint for all \(\psi \in \GG _j\), and a unique map

\[ \Phi \co \big (\KK ,j\big ) \lra \Big (\HH \times V_j,(\id ,0)\Big ) \]

such that

\[ F_k(\varphi ,y)=0 \quad \Longleftrightarrow \quad (\varphi ,y)=\Phi (k) \,, \]

whenever \((\varphi ,y,k)\in \HH \times V_j\times \KK \). Notice, that uniqueness implies \(\Phi \big (j(y)\big )=(\id ,y)\) for all \(y\in V_j\).

For all \(\psi \in \GG _j\) define a map

\[ \Phi _{\psi }\co \big (\KK ,j\big ) \lra \Big (\psi ^*\HH \times V_j, (\psi ,0)\Big ) \]

setting

\[ \Phi _{\psi }(k):= \psi ^*\big (\Phi (k)\big ) \,. \]

Observe that \(\Phi _{\psi }\big (j(y)\big )=\big (\psi ,\psi ^*y\big )\) for all \(y\in V_j\). Moreover, by symmetry of the deformation \(\mathfrak {j}\), which reads as \(\psi ^*\circ \mathfrak {j}=\mathfrak {j}\circ \psi ^*\) for all \(\psi \in \GG _j\), we get \(\psi ^*\circ F_k=F_k\circ \psi ^*\), and hence \(F_k\big (\Phi _{\psi }(k)\big )=0\) for all \(k\in \JJ \) and \(\psi \in \GG _j\). In other words, for all \(\psi \in \GG _j\) there exists a unique map \(\Phi _{\psi }\) with the above properties such that

\[ F_k(\varphi ,y)=0 \quad \Longleftrightarrow \quad (\varphi ,y)=\Phi _{\psi }(k) \,, \]

whenever \((\varphi ,y,k)\in \psi ^*\HH \times V_j\times \KK \).

We get the following global uniqueness statement : There exists potentially smaller neighbourhoods \(V_j\) and \(\KK \) such that for all solutions \((\varphi ,y,k)\in \GG \times V_j\times \KK \) of \(F(\varphi ,y,k)=0\) there exists a unique \(\psi \in \GG _j\) such that \(\varphi \in \psi ^*\HH \) and \((\varphi ,y)=\Phi _{\psi }(k)\). This follows arguing by contradiction with properness of the action \(\GG \times \JJ \ra \JJ \), \((\phi ,j)\mapsto \phi ^*j\), see Remark 6.3.2 .

Based on the current results of the implicit function theorem an orbifold chart about \(j\in \JJ \) can be obtained as follows: Let \(\UU _j\) be the image of \(\KK \) under the projection \([\,.\,]\co \JJ \ra \RR _{\tau }=\JJ /\GG \), i.e.

\[\UU _j=[\KK ]\,,\]

so that, in particular, \(\UU _j\) is open according to the quotient topology described in Remark 6.3.2 . With help of \(\Phi \) we find \(\varphi \in \HH \) and \(y\in V_j\) for each given \(k\in \KK \) such that \(\varphi ^*k=j(y)\). Hence, \([k]=\big [j(y)\big ]\), so that \(\UU _j\) is the set of all isomorphism classes \(\big [S,j(y),D,\{1,\rmi ,-1\},A\big ]=\big [j(y)\big ]\) with \(y\in V_j\).

The isotropy group \(\GG _j\) acts linearly on \(V_j\) by conjugation. In view of the metric obtained by restriction of the metric described in Example 6.7.1 this action is orthogonal. Hence, the action is effective , i.e. only for \(\id \in \GG _j\) all points of \(V_j\) are fixed points. The map

\[ \mathfrak {p}_j\co V_j/\GG _j\lra \UU _j \,,\qquad [y]\longmapsto \big [j(y)\big ] \]

is well-defined by symmetry of the deformation \(\mathfrak {j}\); \(\mathfrak {p}_j\) is continuous because the deformation \(\mathfrak {j}\) is and the respective quotient maps are open and continuous as explained in Remark 6.3.2 .

We claim that

\[ \UU _j\lra V_j/\GG _j \,,\qquad [k]\longmapsto \big [\Phi ^2(k)\big ] \,, \]

is the inverse map of \(\mathfrak {p}_j\), where \(\Phi ^2(k)\) denotes the second component of \(\Phi (k)\). First of all the map is well-defined by the following compatibility condition for uniformisers : Write \(\big [j(y_1)\big ]=[k]=\big [j(y_2)\big ]\) for \(y_1,y_2\in V_j\) and choose an isomorphism

\[ \phi \co \big (S,j(y_1),D,\{1,\rmi ,-1\},A\big ) \lra \big (S,j(y_2),D,\{1,\rmi ,-1\},A\big ) \,, \]

whose existence is guaranteed by the definition of the equivalence relation. We claim that

\[ \phi \in \GG _j \quad \text {and} \quad y_1=\phi ^*y_2 \,. \]

Indeed, we get \(F\big (\phi ,y_1,j(y_2)\big )=0\), so that we find a unique \(\psi \in \GG _j\) such that \(\phi \in \psi ^*\HH \) and \((\phi ,y_1)=\Phi _{\phi }\big (j(y_2)\big )\) by the above global uniqueness statement. Because of \(\Phi _{\phi }\big (j(y_2)\big )=(\psi ,\psi ^*y_2)\) we obtain \(\phi =\psi \in \GG _j\) and \(y_1=\psi ^*y_2\). Being well-defined follows now with the equation \(\Phi \big (j(y)\big )=(\id ,y)\) for \(y\in \{y_1,y_2\}\). Similarly, in order to verify the two-sided inverse property we obtain

\[ [y]\longmapsto \big [j(y)\big ]\longmapsto \Big [\Phi ^2\big (j(y)\big )\Big ]=[y] \]

and, writing \(\varphi ^*k=j(y)\) for \(y\in V_j\),

\[ [k]\longmapsto \big [\Phi ^2(k)\big ]=[y]\longmapsto \big [j(y)\big ]=[k] \,. \]

Therefore, the assignment \([k]\mapsto \big [\Phi ^2(k)\big ]\) is the inverse map \(\mathfrak {p}_j^{-1}\co \UU _j\lra V_j/\GG _j\). The inverse \(\mathfrak {p}_j^{-1}\) is continuous as well. This follows because \(k\mapsto \Phi ^2(k)\) is is continuous and the involved quotient maps are open and continuous, cf. Remark 6.3.2 . Consequently, the \(\GG _j\)-invariant map

\[ [\mathfrak {j}]\co V_j\lra \UU _j \]

induces a homeomorphism \(\mathfrak {p}_j\) form \(V_j/\GG _j\) onto \(\UU _j\). In other words, \(\big (V_j,\GG _j,\mathfrak {p}_j^{-1}\big )\) is an orbifold chart for \(\RR _{\tau }\) about \([j]=\big [S,j,D,\{1,\rmi ,-1\},A\big ]\) and \(\big (E_j,\GG _j,V_j,\UU _j,[\mathfrak {j}]\big )\) is a \(\tau \)- uniformiser by definition.

Remark 6.8.1.
By the above implicit function theorem we find \(k\)-holomorphic maps \(\varphi \in \GG \) defined on \(\big (S,j(y)\big )\), where \(k\in \KK \) and \(y\in V_j\), so that \((\varphi ,y)\) is a solution of \(F_k=0\). By global uniqueness and a potential precomposition with the inverse of an element in \(\GG _j\) making use of the symmetry property of \(\mathfrak {j}\) we can assume that \(\varphi \in \HH \) and write \(\Phi (k)=(\varphi ,y)\). By local uniqueness and \(\GG _j\)-invariance of the solution set we obtain that \(\{F_k=0\}\) is equal to the set of all \(\big (\psi ^*\varphi ,\psi ^*y\big )\), \(\psi \in \GG _j\). Hence, for \(y=\Phi ^2(k)\) the solution set \(\big \{F_k(\,.\,,y)=0\big \}\) is given by \(\{\psi ^*\varphi \,|\,\psi \in \GG _{j,y}\}\), where \(\GG _{j,y}\) denotes the stabiliser at \(y\in V_j\) of the induced action by \(\GG _j\) on \(E_j\). For that we will also write

\[ \GG _{j,y}:=\big (\GG _j|_{E_j}\big )_y \]

Notice that \(\GG _{j,0}=\GG _j\).

For all \(\hat {\psi }\in \GG _k\) we have that \(F_k(\hat {\psi }\circ \varphi ,y)=T\hat {\psi }\circ F_k(\varphi ,y)\), so that the set \(\big \{\hat {\psi }\circ \varphi \,|\,\hat {\psi }\in \GG _k\big \}\) is contained in \(\{\psi ^*\varphi \,|\,\psi \in \GG _{j,y}\}\). For the converse observe that \(\varphi \circ \psi \circ \varphi ^{-1}\), \(\psi \in \GG _{j,y}\), is an element of \(\GG _k\) and \(\big (\varphi \circ \psi \circ \varphi ^{-1}\big )\circ \varphi =\psi ^*\varphi \). Therefore, we obtain two descriptions

\[ \Big \{\hat {\psi }\circ \varphi \,\,\big |\,\,\hat {\psi }\in \GG _k\Big \}= \big \{\psi ^*\varphi \,\,|\,\,\psi \in \GG _{j,y}\big \} \]

for the solution set \(\big \{F_k(\,.\,,y)=0\big \}\) and

\[ \GG _{j,y}\lra \GG _k \,,\qquad \psi \longmapsto \varphi \circ \psi \circ \varphi ^{-1} \]

is an isomorphism of isotropy groups with inverse \(\hat {\psi }\mapsto \varphi ^{-1}\circ \hat {\psi }\circ \varphi \).

In order to describe the transformation behaviour of orbifold charts we consider symmetric effective deformations \(\mathfrak {j}\co V_j\ni y\mapsto j(y)\) and \(\mathfrak {k}\co V_k\ni z\mapsto k(z)\) of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) and \(\big (S,k,D,\{1,\rmi ,-1\},A\big )\), resp. About the respective \(\tau \)-uniformiser \(\big (E_j,\GG _j,V_j,\UU _j,[\mathfrak {j}]\big )\) and \(\big (E_k,\GG _k,V_k,\UU _k,[\mathfrak {k}]\big )\) we assume that \(\UU _j\cap \UU _k=\emptyset \). Hence, we find \(\varphi \in \GG \) such that \(\varphi ^*k=j\).

We claim that we can assume that \(j=j(0)=k(0)=k\). Indeed, define a deformation \(\mathfrak {k'}\co V_{k'}\ni z\mapsto k'(z)\),

\[ k'(z)=\varphi ^*\Big (k\big ((\varphi ^{-1})^*z\big )\Big ) \,, \]

of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\), whose domain is the subset \(V_{k'}:=\varphi ^*V_k\) of the complementary space \(E_{k'}:=\varphi ^*E_k\). For the latter use that \(g_{k'}\) and \(\varphi ^*g_k\) are conformally equivalent. By the naturality of the Kodaira differential we have

\[ [T_0\mathfrak {k'}]= \varphi ^*\circ [T_0\mathfrak {k}]\circ (\varphi ^{-1})^* \,, \]

so that \(\mathfrak {k'}\) is effective, see Remark 6.7.3 . In view of Remark 6.8.1 the deformation \(\mathfrak {k'}\) is symmetric because for all \(\psi \in \GG _k\), for which we have \(\psi ^*\circ \mathfrak {k}=\mathfrak {k}\circ \psi ^*\), it follows that \(\big (\varphi ^{-1}\circ \psi \circ \varphi \big )^*\circ \mathfrak {k'}= \mathfrak {k'}\circ \big (\varphi ^{-1}\circ \psi \circ \varphi \big )^*\).

Therefore, we consider deformations \(\mathfrak {j}\) and \(\mathfrak {k}\) such that \(j=j(0)=k(0)=k\). In view of the implicit function theorem above there exists a \(k(z)\)-holomorphic map \(\varphi (z)\in \GG \) close to \(\id \in \GG _j\) defined on \(\big (S,j\big (y(z)\big )\big )\) via the locally unique smooth map \(\Phi \big (k(z)\big )=\big (\varphi (z),y(z)\big )\) such that \(\Phi (j)=(\id ,0)\). Switching the roles results into a \(j(y)\)-holomorphic map \(\hat {\varphi }(y)\in \GG \) close to \(\id \in \GG _j\) defined on \(\big (S,k\big (z(y)\big )\big )\) via the locally unique smooth map \(\Phi \big (j(y)\big )=\big (\hat {\varphi }(y),z(y)\big )\) such that \(\Phi (j)=(\id ,0)\). Comparing both solutions using uniqueness yields

\[ \hat {\varphi }\big (y(z)\big )=\big (\varphi (z)\big )^{-1} \]

as well as \(z=z\big (y(z)\big )\) and \(y=y\big (z(y)\big )\). Therefore, after shrinking the domains according to the implicit function theorem if necessary, which results into \(\UU _j=\UU _k\), we obtain maps

\[ V_j\lra V_k \,,\quad y\longmapsto z(y) \qquad \text {and}\qquad V_k\lra V_j \,,\quad z\longmapsto y(z) \,, \]

which are smooth and inverse to each other such that \([\mathfrak {k}]\circ \big (y\mapsto z(y)\big )=\hat {\varphi }(y)^*[\mathfrak {j}]\). This results into a coordinate change of an orbifold structure because the construction is done in a \(\GG _j\)-equivariant fashion: For that use Remark 6.8.1 and observe that the solution set \(\big \{F_{k(z)}(\,.\,,y)=0\big \}\) is given by

\[ \Big \{\hat {\psi }\circ \varphi (z)\,\,\big |\,\,\hat {\psi }\in \GG _{k(z)}\Big \}= \big \{\psi ^*\varphi (z)\,\,|\,\,\psi \in \GG _{j,y}\big \} \,. \]

As for manifolds we obtain:

Proposition 6.8.2.
The above constructed orbifold charts provide the nodal Riemann moduli space \(\RR _{\tau }\) for the stable nodal type \(\tau \) with the structure of an orbifold of real dimension \(2\big (\#A-\#D\big )\), whose isotropy groups at \([j]\in \RR _{\tau }\) are given by \(\GG _j\) up to conjugation.

Referring to the current situation we define

\[ \mathbf {T}_{j,k}:= \Big \{ (\varphi ,y,z) \,\,\big |\,\, F_{k(z)}(\varphi ,y)=0 \Big \} \subset \GG \times V_j\times V_k \]

provided with the subspace topology and call the projection \(s\co \mathbf {T}_{j,k}\ra V_j\) onto \(V_j\) the source map ; the the projection \(t\co \mathbf {T}_{j,k}\ra V_k\) onto \(V_k\) the target map . These maps come with inverses \(y\mapsto \big (\hat {\varphi }^{-1}(y),y,z(y)\big )\) and \(z\mapsto \big (\varphi (z),y(z),z\big )\), resp., where \(\hat {\varphi }\big (y(z)\big )=\big (\varphi (z)\big )^{-1}\) as above. Hence, \(s\) and \(t\) are homeomorphisms providing \(\mathbf {T}_{j,k}\) with the structure of a smooth manifold of dimension \(2\big (\#A-\#D\big )\), and \(t\circ s^{-1}\) and \(s\circ t^{-1}\) correspond to the above transition maps \(y\mapsto z(y)\) and \(z\mapsto y(z)\), resp. By the properness argument in Remark 6.3.2 the map \(s\times t\co \mathbf {T}_{j,k}\ra V_j\times V_k\) is proper.

In other words, we obtain an étale proper Lie groupoid \((R_{\tau },\mathbf {R}_{\tau })\), which means the following: Take a sequence of \(\tau \)-uniformisers \(\big (E_{j_{\nu }},\GG _{j_{\nu }},V_{j_{\nu }},\UU _{j_{\nu }},[\mathfrak {j}_{\nu }]\big )\) such that \(\bigcup _{\nu }\UU _{j_{\nu }}\) covers \(\RR _{\tau }\). The objects are given by

\[ R_{\tau }:=\bigsqcup _{\nu }V_{j_{\nu }} \]

and the morphisms are

\[ \mathbf {R}_{\tau }:=\bigsqcup _{\nu ,\mu }\mathbf {T}_{j_{\nu },j_{\mu }}\,. \]

Morphisms can be composed whenever the corresponding target and source coincide. The resulting composition is smooth, has a unit and each morphism admits a smooth inverse. Furthermore all mentioned structure maps are smooth. The nodal Riemann moduli space \(\RR _{\tau }\) for the stable nodal type \(\tau \) appears now as orbit space

\[\RR _{\tau }=R_{\tau }/\!\sim \,,\]

where two objects between which there exists a morphism are considered to be equivalent.

6.9. Skyscraper deformation.

A symmetric effective deformation \(\mathfrak {j}\) is called a skyscraper deformation if there exists a \(\GG _j\)-invariant neighbourhood \(U\subset S\) of \(\partial S\) together with the special points \(|D|\cup \{1,\rmi ,-1\}\cup A\) on which the deformation is stationary , i.e. if \(j(y)=j\) restricted to \(U\) for all \(y\in V_j\). In view of the examples of symmetric effective deformations in Section 6.6 and Remark 6.6.1 skyscraper deformations can be obtained by restriction of symmetric effective deformations to a complementary \(\GG _j\)-invariant vector space \(E_j\) of \(\im (j\CR j)\) whose elements vanish on \(U\).

In order to construct such a vector space \(E_j\) we denote by \(\XX \) the space of all smooth vector fields on \(S\) that are tangent to the boundary along \(\partial S\) and admit \(3\) zeros on each connected component of \(S\) equal to special points in \(|D|\cup \{1,\rmi ,-1\}\cup A\); on the disc component the zeros are required to be \(1,\rmi ,-1\). The operator \(j\CR j\) restricted to \(\XX \) induces an isomorphism \(\XX \ra \Omega ^{0,1}_j\).

We begin with the un-isotropic situation \(\GG _j=\{\id \}\). In order to construct a complement of \(\Omega ^0\) in \(\XX \) we write \(z_k\) for the elements of \(|D|\cup A\) and choose local holomorphic charts \((\C ,\rmi )\) for \((S,j)\) about the special points \(z_k\). We require that the chart domains are mutually disjoint and contained in \(S\setminus \partial S\). Let \(f_k\) be smooth cut off functions on \(S\) that have their supports in the interior of \(r\)-disc neighbourhoods about \(z_k\) w.r.t. \(g_j\) contained in the chosen chart domains; the \(f_k\) are required to by constantly \(1\) on the \(r/2\)-disc neighbourhoods about \(z_k\). Given \(X\in \XX \) we define vector fields \(X_k\) on \(S\). We require that the \(X_k\) are given by \(X(z_k)f_k\) in the chosen charts extended by zero to \(S\). Observe that the \(X_k\) vanish for special points that correspond to the zeros defining \(\XX \). Moreover, the \(X_k\) are holomorphic on the \(r/2\)-discs.

Let \(P\co \XX \ra \XX \) be the projector, i.e. \(P^2=P\), given by

\[ P(X):=X-\sum _kX_k \,. \]

Observe that \(P\) restricts to the identity on \(P(\XX )=\Omega ^0\). The desired complement of \(\Omega ^0\) in \(\XX \) is \((1-P)(\XX )\) as \(1-P\) is a projector as well. The elements of \(j\CR j(1-P)(\XX )\) vanish on a neighbourhood of all special points \(|D|\cup \{1,\rmi ,-1\}\cup A\) and of \(\partial S\). Moreover, the dimension of \((1-P)(\XX )\) equals

\[ 2\big (\#A-\#D\big ) \]

by the result of the computation of Section 6.5 multiplied by \(-1\).

Finally we set \(E_j:=j\CR j(1-P)(\XX )\). The elements of \(E_j\) vanish on a neighbourhood of the union of the special points \(|D|\cup \{1,\rmi ,-1\}\cup A\) and of the boundary \(\partial S\). Furthermore the isomorphism \(j\CR j\co \XX \ra \Omega ^{0,1}_j\) sends the splitting \((1-P)(\XX )\oplus \Omega ^0\) of \(\XX \) to the splitting \(E_j\oplus \im (j\CR j)\) of \(\Omega ^{0,1}_j\).

We treat the case of a non-vanishing isotropy group \(\GG _j\), which acts by permutations on \(\{z_k\}=|D|\cup A\). It suffices to change the above projector \(P\) by replacing the vector fields \(X_k\) by \(\GG _j\)-invariant vector fields \(\hat {X}_k\). For that denote by \(B_r(z_k)\), \(r>0\), the interior of the above \(r\)-discs. Observe that the disjoint union of the \(B_r(z_k)\) is \(\GG _j\)-invariant as \(\GG _j\) acts by isometries on \((S,g_j)\).

For each \(z_k\) we assign a partner point \(w_k\in B_{r/2}(z_k)\setminus \{z_k\}\) requiring that the \(\psi (w_k)\) are pair-wise distinct for all \(\psi \in \GG _j\) and all \(k\). Notice, that the distance between \(z_k\) and its partner \(w_k\) is \(\GG _j\)-invariant for all \(k\). We choose \(\varepsilon >0\) such that \(B_{\varepsilon }(w_k)\subset B_{r/2}(z_k)\setminus \{z_k\}\) for all \(k\). Furthermore, we reqiure that the \(\psi \big (B_{\varepsilon }(w_k)\big )\) are pair-wise disjoint for all \(\psi \in \GG _j\) and for all \(k\). Modify the cut off functions \(f_k\) so that \(f_k\) has support in

\[ B_r(z_k)\,\,\setminus \quad \bigsqcup _{\ell \neq k\,\,\text {and}\,\,\psi \in \GG _j} \psi \big (\overline {B_{\varepsilon /2}(w_{\ell })}\big ) \]

and is equal to \(1\) on

\[ B_{r/2}(z_k)\,\,\setminus \quad \bigsqcup _{\ell \neq k\,\,\text {and}\,\,\psi \in \GG _j} \psi \big (\overline {B_{\varepsilon }(w_{\ell })}\big ) \,. \]

In particular, for all \(k\), we get \(f_k(w_k)=1\) and \(f_k\big (\psi (w_{\ell })\big )=0\) for all \(\ell \neq k\) and \(\psi \in \GG _j\). With the cut off functions \(f_k\) modified we define \(X_k\) for given \(X\in \XX \) as in the un-isotropic case.

We define the symmetrisations via

\[ \hat {X}_k:=\sum _{\psi \in \GG _j}\psi ^*X_k \,. \]

We have \(\phi ^*\hat {X}_k=\hat {X}_k\) for all \(\phi \in \GG _j\) and for all \(k\) because \(\GG _j\) acts on itself via composition permuting \(\GG _j\). The \(\hat {X}_k\) that are assigned to the zeros \(z_k\) of \(\XX \) vanish; the remaining \(\hat {X}_k\) span a \(2\big (\#A-\#D\big )\)-dimensional vector space because

\[ \hat {X}_k(w_{\ell })=X_{\ell }(w_{\ell }) \]

for all \(k,\ell \). A basis can be obtained by taking \(X\in \XX \) with \(X(z_k)\) non-zero, so that the corresponding partners \(X_k(w_k)\) do not vanish.

Remark 6.9.1.
Observe that the elements of \((1-P)(\XX )\), which are linear combinations of the vector fields \(\hat {X}_k\) constructed above, are vector fields on \(S\) that vanish on the boundary \(\partial S\). Therefore, the complex structure \(j\) on \(S\) preserves \((1-P)(\XX )\) and defines a complex structure on \(E_j=\CR j(1-P)(\XX )\) as \(\CR j\) commutes with \(j\), so that \(E_j\) is a complex vector space of complex dimension \(\#A-\#D\). Consequently taking the complex deformations form Example 6.7.2 w.r.t. \(E_j\) yields holomorphic skyscraper deformations.

Remark 6.9.2.
In the above construction the radii \(r_k\) of the discs

\[ D_{r_k/2}(z_k):=\overline {B_{r_k/2}(z_k)} \]

are necessarily constant on the orbits of the \(\GG _j\)-action on the points \(z_k\in |D|\cup A\) because \(\GG _j\) acts on the discs \(D_{r_k/2}(z_k)\) by isometries of \((S,g_j)\); but the radii are allowed to vary on distinct orbits \(\GG _jz_k\). For a selection of orbit-wise constant radii \(r_k\) denoted by \(\mathbf {r}\) and the disjoint union

\[ \mathbf {D}_{j,\mathbf {r}}:=\bigsqcup _{z_k\in |D|\cup A}D_{r_k/2}(z_k) \]

a skyscraper deformation \(\mathfrak {j}\) that is stationary on \(\mathbf {D}_{j,\mathbf {r}}\) can be constructed by the above arguments. Given a neighbourhood \(U\) of \(|D|\cup A\) one can choose \(\mathbf {r}\) so small such that \(\mathbf {D}_{j,\mathbf {r}}\subset U\). This yields an example of a small disc structure \(\mathbf {D}_j\), which by definition is a \(\GG _j\)-invariant disjoint union of discs \(D_z\), \(z\in |D|\cup A\), contained in a given neighbourhood of \(|D|\cup A\) such that \(z\in D_z\) for all \(z\in |D|\cup A\). Furthermore the \(D_z\) are the image of a smooth embedding of the closed unit disc \(\D \) into \(S\). Observe that a \(k\)-holomorphic map \(\varphi \in \GG \) defined on \((S,j)\) sends \(\mathbf {D}_{j,\mathbf {r}}\) diffeomorphically onto a small disc structure \(\mathbf {D}_k\) on which the \(\varphi \)-push-forward skyscraper deformation \(\mathfrak {k}\) of \(\mathfrak {j}\) is stationary.

Using small disc structures \(\mathbf {D}_j\) orbifold charts \(\big (V_j,\GG _j,\mathfrak {p}_j^{-1}\big )\) and \(\tau \)-uniformiser \(\big (E_j,\GG _j,V_j,\UU _j,[\mathfrak {j}]\big )\) for \(\RR _{\tau }\) about \([j]=\big [S,j,D,\{1,\rmi ,-1\},A\big ]\) can be constructed as in Section 6.8 using skyscraper deformations \(\mathfrak {j}\) that are stationary on \(\mathbf {D}_j\) exclusively. The transformation behaviour encoded in the \(\mathbf {T}_{j,k}\) is compatible with skyscraper deformations which are stationary on disc structures. Correspondingly, a neighbourhood base of the topology on \(\RR _{\tau }=\JJ /\GG \) described in Remark 6.3.2 can be given by the family of subsets whose elements \([k]\) can be represented by complex structures \(k\) that belong to an open subset of \(\JJ \) and that satisfy \(k=j\) restricted to some small disc structure \(\mathbf {D}_j\). This follows with the implicit function theorem formulated in Section 6.8 .

Remark 6.9.3.
In view of the proceeding Remarks 6.9.1 and 6.9.2 the orbifold structure on \(\RR _{\tau }\) ensured in Proposition 6.8.2 and the subsequently described étale proper Lie groupoid structure admit subatlases generated by complex skyscraper deformations, so that the respective substructures are complex. For that one needs to verify that the transition maps \(t\circ s^{-1}\) and \(s\circ t^{-1}\) are holomorphic. In terms of complex skyscraper deformations \(\mathfrak {j}\co V_j\ni y\mapsto j(y)\) and \(\mathfrak {k}\co V_k\ni z\mapsto k(z)\) of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) and \(\big (S,k,D,\{1,\rmi ,-1\},A\big )\), resp., such that there exists \(\varphi \in \GG \) with \(\varphi ^*k=j\) the transition maps are given by \(y\mapsto z(y)\) and \(z\mapsto y(z)\), resp. With the description before Proposition 6.8.2 we get \([\mathfrak {k}]\circ \big (y\mapsto z(y)\big )=\hat {\varphi }(y)^*[\mathfrak {j}]\) and \([\mathfrak {j}]\circ \big (z\mapsto y(z)\big )=\varphi (z)^*[\mathfrak {k}]\) for smooth maps \(V_k\ra \GG \), \(z\mapsto \varphi (z)\), and \(V_j\ra \GG \), \(y\mapsto \hat {\varphi }(y)\), with \(\varphi (0)=\varphi \) and \(\hat {\varphi }(0)=\varphi ^{-1}\). By symmetry it will be sufficient to verify holomorphicity in the first situation: Taking the derivative w.r.t. \(y\in V_j\) in \(k\big (z(y)\big )=\hat {\varphi }(y)^*j(y)\) we obtain

\[ T_{z(y)}\mathfrak {k}\circ T_yz(\dot y)= 2 k\big (z(y)\big )\cdot \CR {k(z(y))}\Big (\hat {\varphi }(y)^*\big (T_y \hat {\varphi }(\dot y)\big )\Big )+ \hat {\varphi }(y)^*\big (T_y\mathfrak {j}(\dot y)\big ) \]

as in Remark 6.7.3 . Replacing \(\dot y\) by \(j\dot y\) and composing with \(-k\big (z(y)\big )\) from the left yields

\[ -T_{z(y)}\mathfrak {k}\circ k\circ T_yz(j\dot y)= 2 \cdot \CR {k(z(y))}\Big (\hat {\varphi }(y)^*\big (T_y \hat {\varphi }(j\dot y)\big )\Big )+ \hat {\varphi }(y)^*\big (T_y\mathfrak {j}(\dot y)\big ) \,. \]

The second summand on the right stays the same because \(k\big (z(y)\big )=\hat {\varphi }(y)^*j(y)\) and \(\mathfrak {j}(y)\circ T_y\mathfrak {j}=T_y\mathfrak {j}\circ j\) by complexitiy, see Remark 6.9.1 . Similarly, to deal with the left hand side use \(\mathfrak {k}(z)\circ T_z\mathfrak {k}=T_z\mathfrak {k}\circ k\). On the right hand side, the first summend is an element in

\[ \im \Big ( k\big (z(y)\big )\cdot \CR {k(z(y))} \Big ) \]

because \(j\dot y\) vanishes along the boundary \(\partial S\), so that the vector field \(\hat {\varphi }(y)^*\big (T_y \hat {\varphi }(j\dot y)\big )\) vanishes along \(\partial S\) as well, and because on boundary vanishing vector fields on \((S,\partial S)\) the Cauchy–Riemann operator is complex linear, cf. Section 6.4 . Effectivity of \(\mathfrak {k}\) yields the algebraic splitting

\[ \Omega ^{0,1}_{k(z(y))}= \,T_{z(y)}\mathfrak {k}\,(E_k) \,\oplus \, \im \Big ( k\big (z(y)\big )\cdot \CR {k(z(y))} \Big ) \,. \]

Modding out the contributions to the second summand the above two equations compare to

\[ T_{z(y)}\mathfrak {k}\circ T_yz(\dot y)= -T_{z(y)}\mathfrak {k}\circ k\circ T_yz(j\dot y) \,. \]

As \(T_{z(y)}\mathfrak {k}\) is injective this yields

\[ T_yz(\dot y)=-k\circ T_yz(j\dot y) \,, \]

i.e. \(k\circ T_yz= T_yz\circ j\) meaning that \(y\mapsto z(y)\) is holomorphic.

Consequently, we obtain a complex version of Proposition 6.8.2 , so that, in particular, \(\RR _{\tau }\) is orientable.

Proposition 6.9.4.
The nodal Riemann moduli space \(\RR _{\tau }\) admits the structure of a complex orbifold of complex dimension \(\#A-\#D\).

Remark 6.9.5.
In order to derive Proposition 6.9.4 we fixed in Section 6.3 the combinatorial data \(\big (S,D,\{m_0,m_1,m_2\},A\big )\) to represent stable nodal marked discs \(\big [S,j,D,\{m_0,m_1,m_2\},A\big ]\) and used deformations of \(j\). A direct way to obtain a complex orbifold structure would be to change the roles. Apply uniformisation as in Remark 6.3.1 in order to represent the classes \(\big [S,j,D,\{m_0,m_1,m_2\},A\big ]\) by nodal discs whose disc component equals \(\big (\D ,\rmi ,\{1,\rmi ,-1\}\big )\) and whose sphere components are given by \((\C P^1,\rmi )\). The complex orbifold structure can be read off from variations of the configurations of the nodal points \(D\) and the marked points \(A\) as such, resp.

6.10. Varying the stable nodal type via desingularisation.

For a complex number \(a\) of modulus \(|a|\leq 1\) we consider the intersection of the planar algebraic curve \(\{zw=a\}\subset \C \times \C \) with the polydisc \(\D \times \D \). For \(a=0\) this curve is the union of the discs \(\{z=0\}=\{0\}\times \D \) and \(\{w=0\}=\D \times \{0\}\) that intersect in the singularity of the curve. For \(a\neq 0\) the equation \(zw=a\) can be solved by \(w=a/z\) so that we obtain a cylinder that has no singularities: The restriction of the projection \((z,w)\mapsto z\) to the curve \(\{zw=a\}\) yields a biholomorphism onto the annulus \(\{|a|\leq |z|\leq 1\}\) in the first coordinate plane. Interchanging \(z\) and \(w\) yields a biholomorphism onto \(\{|a|\leq |w|\leq 1\}\). Both biholomorphisms constitute holomorphic charts of \(\{zw=a\}\). The transition map from the first annulus to the second is

\[z\longmapsto \frac {a}{z}\,.\]

Taking positive and negative holomorphic polar coordinates \((z,w)\mapsto -\ln z\) and \((z,w)\mapsto \ln w\), resp., i.e. writing

\[ z=\rme ^{-(s+\rmi t)} \qquad \text {and}\qquad w=\rme ^{u+\rmi v} \,, \]

the transition map gets

\[ \big [0,-\ln |a|\big ]\times S^1\lra \big [\ln |a|,0\big ]\times S^1 \,,\qquad (s,t)\longmapsto \big (s+\ln |a|,t+\arg a\big ) \,, \]

where \(S^1=\partial \D \). For the complex logarithm we use the main branch.

Observe that rotations \(z\mapsto \rme ^{-\rmi \theta _+}z\) and \(w\mapsto \rme ^{\rmi \theta _-}w\) for \(\theta _+,\theta _-\in S^1\) of the coordinate planes, which correspond to

\[ (s,t)\longmapsto \big (s,t+\theta _+\big ) \qquad \text {and}\qquad (s,t)\longmapsto \big (s,t+\theta _-\big ) \]

w.r.t. positive and negative holomorphic polar coordinates, resp., result into a change of the defining equation to

\[ zw=\rme ^{-\rmi (\theta _+-\theta _-)}a \]

as the pull back along \((z,w)\mapsto \big (\rme ^{-\rmi \theta _+}z,\rme ^{\rmi \theta _-}w\big )\) yields \(zw=a\). The coresponding transition map is

\[ (s,t)\longmapsto \Big (s+\ln |a|,t+\arg a-\big (\theta _+-\theta _-\big )\Big ) \,. \]

A switch of the coordinates \((z,w)\mapsto (w,z)\) does not effect the proceeding consideration.

Given \(\big [S,j,D,\{1,\rmi ,-1\},A\big ]\in \RR _{\tau }\) we describe a similar desingularisation about a nodal pair \(\{z_0,w_0\}\in D\) in terms of parametrised connected sum . Choose a small disc structure \(\mathbf {D}_j\) on \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\). Denote the corresponding discs about the nodal points \(z_0,w_0\in |D|\) by \(D_{z_0}\) and \(D_{w_0}\), resp., and choose boundary points \(z_{\partial }\in \partial D_{z_0}\) and \(w_{\partial }\in \partial D_{w_0}\). We call the pair \(\{z_{\partial },w_{\partial }\}\) a decoration of the nodal pair \(\{z_0,w_0\}\). By [54], Theorem C.5.1 there exists unique biholomorphic identifications of \(\big ((D_{z_0},z_0,z_{\partial }),j\big )\) and \(\big ((D_{w_0},w_0,w_{\partial }),j\big )\), resp., with \(\big ((\D ,0,1),\rmi \big )\).

For given gluing parameter \(a\in \D \), \(a\neq 0\), replace \(-\ln |a|\) by the modulus

\[ R=\rme ^{1/|a|}-\rme \]

in the discussion about the planar algebraic curve \(\{zw=a\}\). Identify the first annulus \(\{\rme ^{-R}\leq |z|\leq 1\}\) with the second \(\{\rme ^{-R}\leq |w|\leq 1\}\) via the transition map

\[ z\longmapsto \frac {\rme ^{-R+\rmi \arg (a)}}{z} \,, \]

which w.r.t. positive and negative holomorphic polar coordinates reads as

\[ [0,R]\times S^1\lra [-R,0]\times S^1 \,,\qquad (s,t)\longmapsto \big (s-R,t+\arg a\big ) \,. \]

We obtain a surface \(S_a\) from \(S\setminus \big (\Int (D_{z_0})\cup \Int (D_{w_0})\big )\) by gluing the finite cylinder \(Z_a:=[0,R]\times S^1\), which is identified with \([-R,0]\times S^1\) via the above transition map, along the respective boundary circles via the restrictions of the biholomorphic identifications of \(D_{z_0}\) and \(D_{w_0}\), resp, with \(\D \).

The construction of the surface \(S_a\) defines a complex structure \(j_a\) that coincides with \(j\) on \(S\setminus \big (\Int (D_{z_0})\cup \Int (D_{w_0})\big )\) and with \(\rmi \) on the cylinder \(Z_a\) of modulus \(R\). This results into an element \(\big [S_a,j_a,D_a,\{1,\rmi ,-1\},A\big ]\) of \(\RR _{\tau '}\) with stable nodal type \(\tau '\), which necessarily differs from \(\tau \). The respective special points are given by

\[ D_a:=D\setminus \big \{\{z_0,w_0\}\big \} \,, \]

\(\{1,\rmi ,-1\}\), and \(A\) under the inclusion of \(S\setminus \big (\Int (D_{z_0})\cup \Int (D_{w_0})\big )\) into \(S_a\).

A change of biholomorphic identifications of \(D_{z_0}\) and \(D_{w_0}\) with \(\D \) is given by a rotation of the boundary points \(z_{\partial }\) and \(w_{\partial }\), resp., which in coordinates reads as \(z\mapsto \rme ^{-\rmi \theta _+}z\) and \(w\mapsto \rme ^{\rmi \theta _-}w\), say. Gluing with the rotated identifications yields a biholomorphic copy \(\big (S_b,j_b,D_b,\{1,\rmi ,-1\},A\big )\) of \(\big (S_a,j_a,D_a,\{1,\rmi ,-1\},A\big )\), where

\[ b=\rme ^{-\rmi (\theta _+-\theta _-)}a \,. \]

To obtain a biholomorphic map take the identity map on \(S\setminus \big (\Int (D_{z_0})\cup \Int (D_{w_0})\big )\) and the rotated transition map \(Z_a\ra Z_b\) given by

\[ (s,t)\longmapsto \Big (s-R,t+\arg a-\big (\theta _+-\theta _-\big )\Big ) \]

on \(Z_a\).

Such rotations naturally appear when a automorphism \(\psi \in \GG _j\) for which the nodal points \(z_0\) and \(w_0\) are fixed-points, i.e. \(\psi (z_0)=z_0\) and \(\psi (w_0)=w_0\), acts on \(S\). Indeed, \(\psi \) preserves the complement of \(D_{z_0}\cup D_{w_0}\) in \(S\) and induces rotations on \(D_{z_0}\cup D_{w_0}\). The rotations are measured by the change of decorations from \(\{z_{\partial },w_{\partial }\}\) to \(\psi \big (\{z_{\partial },w_{\partial }\}\big )\) in terms of angles \(-\theta _+\) and \(\theta _-\), say. Therefore, we get a holomorphic diffeomorphism

\[ \big (S_a,j_a,D_a,\{1,\rmi ,-1\},A\big ) \lra \big (S_b,j_b,D_b,\{1,\rmi ,-1\},A\big ) \]

as above which this time coincides with \(\psi \) on \(S\setminus \big (\Int (D_{z_0})\cup \Int (D_{w_0})\big )\).

We denote by

\[ \D ^D \]

the set of all maps from the set of nodal points \(D\) to the set \(\D \) of complex numbers of modulus less than or equal to \(1\). Choose a small disc structure \(\mathbf {D}_j\) on \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) together with a decoration for each disc in \(\mathbf {D}_j\). The choice of decorations determine holomorphic diffeomorphisms of all discs of the disc structure with \(\D \) such that the nodal point is mapped to \(0\in \D \) and the decoration to \(1\in \D \). Given \(\bfa \in \D ^D\) we perform the described parametrised connected sum about each nodal pair \(\{z,w\}\in D\) with gluing parameter

\[ a_{\{z,w\}}:=\bfa \big (\{z,w\}\big ) \,. \]

This is done by replacing the node \(\{z,w\}\) with the cylinder \(Z_{a_{\{z,w\}}}^{\{z,w\}}\). In the case of a vanishing gluing parameter \(a_{\{z,w\}}\) formally

\[ Z_0^{\{z,w\}}:=D_z\sqcup D_w \]

is given by the disjoint union of half-infinite cylinders \([0,\infty )\times S^1\) and \((-\infty ,0]\times S^1\) of infinite modulus after removing the nodal points \(z\) and \(w\). In other words, if \(a_{\{z,w\}}=0\) we do nothing and keep the nodal pair \(\{z,w\}\in D_{\bfa }\), so that \(D_{\bfa }\) arises from \(D\) by removing all nodal pairs \(\{z,w\}\) with \(a_{\{z,w\}}\neq 0\). The resulting surface is denoted by

\[ \big (S_{\bfa },j_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ) \,. \]

Starting off with a skyscraper deformation \(V_j\ni y\mapsto j(y)\) and a small disc structure of sufficiently small discs we will get

\[ \big (S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ) \]

by the same construction.

In order to describe the effect of the \(\GG _j\)-action of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) on the desingularisation we denote by \(\kappa _{z,w}\), \(\{z,w\}\in D\), the complex anti-linear map \(T_wS\ra T_zS\) that conjugated with the linearisations of the biholomorphic identifications of the discs \(D_w\) and \(D_z\) with \(\D \) is equal to the complex conjugation map \(x+\rmi y\mapsto x-\rmi y\) on \(\C \). Interchanging the role of \(z\) and \(w\) replaces \(\kappa _{z,w}\) by its inverse \(\kappa _{w,z}=(\kappa _{z,w})^{-1}\). We call \(\kappa _{z,w}\) a compatible nodal identifier . Given \(\psi \in \GG _j\) and \(\{z,w\}\in D\) we define the phase function

\[ \Theta _{\{z,w\}}(\psi )\co T_zS\lra T_zS \]

by

\[ \Theta _{\{z,w\}}(\psi ):= \kappa _{z,w}\circ T_{\psi (w)}(\psi )^{-1}\circ \kappa _{\psi (w),\psi (z)}\circ T_z\psi \,. \]

Taking positive and negative holomorphic polar coordinates about \(z\) and \(w\), resp., so that \(\psi \) acts in coordinates by multiplication with \(\rme ^{-\rmi \theta _+}\) and \(\rme ^{\rmi \theta _-}\), resp., we get

\[ \big (\Theta _{\{z,w\}}(\psi )\big )(v)= \rme ^{-\rmi (\theta _+-\theta _-)}v \]

for all \(v\in T_zS\), which we simply declare to a multiplication operator

\[ \Theta _{\{z,w\}}(\psi )\equiv \rme ^{-\rmi (\theta _+-\theta _-)} \,. \]

This shows independence of the phase function

\[ \Theta \co D\times \GG _j\lra S^1 \,,\qquad \big (\{z,w\},\psi \big )\longmapsto \Theta _{\{z,w\}}(\psi ) \,, \]

of the chosen ordering of \(\{z,w\}\) in the definition of \(\Theta _{\{z,w\}}(\psi )\) and of the chosen parity of the holomorphic polar coordinates about \(\psi (z)\) and \(\psi (w)\). This results in a \(\GG _j\)-action on \(\D ^D\) defined by \(\psi _*\bfa =\bfb \) via

\[ b_{\{\psi (z),\psi (w)\}}:= \Theta _{\{z,w\}}(\psi )\cdot a_{\{z,w\}} \]

for all \(\{z,w\}\in D\). Consequently, for any skyscraper deformation \(V_j\ni y\mapsto j(y)\), a small disc structure of sufficiently small discs, and \(\psi \in \GG _j\) we get an isomorphism

\[ \psi _{\bfa }\co \Big (S_{\bfa },j(\psi ^*y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\Big ) \lra \Big (S_{\psi _*\bfa },j(y)_{\psi _*\bfa },D_{\psi _*\bfa },\{1,\rmi ,-1\},A\Big ) \]

by the gluing construction and symmetry of \(y\mapsto j(y)\).

6.11. Topology and orbifold structure – variable stable nodal type.

A neighbourhood base of a second countable paracompact Hausdorff topology on \(\RR _N\), \(N\geq 0\), is given by the family of subsets of \(\RR _N\), whose elements are of the form

\[ \big [S_{\bfa },k_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ] \]

with \(N=\#A\), which are obtained from a nodal disc \(\big (S,k,D,\{1,\rmi ,-1\},A\big )\) by the parametrised connected sum construction with given decorated small disc structure \(\mathbf {D}_j\), with gluing parameter \(\bfa \in \D ^D\) with \(|\bfa |<\varepsilon \) for some \(\varepsilon \in (0,1)\), with complex structures \(k\) that belong to an open neighbourhood of \(j\) in \(\JJ \) such that \(k=j\) restricted to \(\mathbf {D}_j\). This follows as in [43], Proposition 2.4 and [42], Theorem 2.15 and Theorem 5.13 because no extra argument for boundary un-noded nodal discs is needed caused by absence of boundary nodes. The Hausdorff property follows with Gromov compactness for stable holomorphic discs, see [25] .

The induced topology on \(\RR _{\tau }\) in \(\RR _N\) agrees with the one on \(\RR _{\tau }\) previously defined in Remark 6.3.2 . The induced notion of convergence of sequences in \(\RR _N\) coincides with Gromov convergence as described in [1], Chapter 1 , [66], Appendix B or in [15], Section 4 , [46], Chapter IV after Schwartz reflection along the boundary of the nodal discs for example.

In order to obtain an orbifold structure on \(\RR _N\) we consider desingularisations

\[ \big (S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ) \]

of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) as described in Section 6.10 . For \(\bfa _0\in \D ^D\) consider the set \(D\setminus D_{\bfa _0}\) of all nodal pairs \(\{z,w\}\in D\) on which the map \(\bfa _0\) is non-zero. Define a deformation

\[ \mathfrak {j}_{\bfa _0}\co V_{j_{\bfa _0}}\times \D ^{D\setminus D_{\bfa _0}} \lra \JJ _{S_{\bfa _0}} \,,\qquad (y,\bfb )\longmapsto j(y)_{\bfa _0+\bfb } \,, \]

of

\[ \big (S_{\bfa _0},j(y)_{\bfa _0},D_{\bfa _0},\{1,\rmi ,-1\},A\big ) \]

by setting \(\bfa =\bfa _0+\bfb \). For small deformation parameter \(\bfb \) the deformed family of surfaces equals

\[ \Big (S_{\bfa _0+\bfb },j(y)_{\bfa _0+\bfb },D_{\bfa _0+\bfb },\{1,\rmi ,-1\},A\Big ) \,. \]

The nodal discs family is isomorphic to

\[ \Big (S_{\bfa _0},j'(y)_{\bfb },D_{\bfa _0},\{1,\rmi ,-1\},A\Big ) \]

with corresponding deformation

\[ \mathfrak {j}'_{\bfb }\co V_{j_{\bfa _0}}\times \D ^{D\setminus D_{\bfa _0}} \lra \JJ _{S_{\bfa _0}} \,,\qquad (y,\bfb )\longmapsto j'(y)_{\bfb } \,, \]

via an isomorphism that is the identification map on the complement of the respective small disc structure, so that the deformation is given by rotations and stretchings of the cylindrical neck regions that correspond to the nodes, on which \(\bfa _0\) not vanishes. The partial Kodaira differential of \(\mathfrak {j}'_{\bfb }\) at \((y,0)\) is

\[ \big [T_{(y,0)}\mathfrak {j}'_{\bfb }\big ]\co E_{j_{\bfa _0}}\times \C ^{D\setminus D_{\bfa _0}} \lra \Omega ^{0,1}_{{j(y)}_{\bfa _0}}\lra H^1_{{j(y)}_{\bfa _0}} \,. \]

Similarly to [43], Theorem 2.13 one constructs uniformisers of an orbifold structure on \(\RR _N\) as the above desingularisations stay away from the boundary of the nodal discs in \(\RR _N\). For given \(\big [S,j,D,\{1,\rmi ,-1\},A\big ]\in \RR _N\) such a uniformiser is a deformation

\[ \VV \ni (y,\bfa )\longmapsto \big (S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ) \]

of \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) for an open subset \(\VV \) of \(V_j\times \D ^D\) such that the following holds:


  • The union of all equivalence classes \(\big [S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ]\) over all \((y,\bfa )\in \VV \) is an open subset of \(\RR _N\).
  • The map \(\VV \ra \UU \) that assigns to \((y,\bfa )\) the class \(\big [S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\big ]\) descends to a homeomorphism \(\VV /\GG _j\ra \UU \).
  • An isomorphism between the classes belonging to \((y,\bfa ),(z,\bfb )\in \VV \) is given by \(\psi _{\bfa }\) for \(\psi \in \GG _j\) and \((z,\bfb )=\big (\psi _*y,\psi _*\bfa \big )\).
  • For all points in \(\VV \) the partial Kodaira differential is an isomorphism.

Compatibility of uniformisers is expressed via the sets

\[ \mathbf {T}_{j,k}:= \Big \{ \big (\varphi ,(y,\bfa ),(z,\bfb )\big ) \Big \} \subset \GG \times (V_j \times \D ^D)\times (V_k \times \D ^D) \]

corresponding to all isomorphisms

\[ \varphi \co \Big (S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},A\Big ) \lra \Big (S_{\bfb },k(z)_{\bfb },D_{\bfb },\{1,\rmi ,-1\},A\Big ) \,, \]

which are smooth manifolds of dimension \(2\#A\), so that \(\RR _N\) supports an étale proper Lie groupoid structure as formulated after Proposition 6.8.2 . This follows with the (anti-)gluing construction ( [43], Section 2.4 ) for the non-linear Cauchy–Riemann operator along the nodes (which take place away from the boundary) known from Floer theory, cf. [43], Theorem 2.16 and [42], Theorem 2.24 . Similarly, the universal property of the construction stated in [43], Theorem 2.16 translates into the present situation. The involved variation of marked points can be treaded as in [42], Remark 3.17 . Finally, using convex interpolation between the exponential gluing profile \(\rme ^{1/r}-\rme \) we used in the gluing construction and the logarithmic gluing profile \(-\ln r\) that appeared in the desingularisation of the complex algebraic curve at the beginning of Section 6.10 naturally yields an orientation on \(\RR _N\) that extends the complex orientation on \(\RR _{\tau }\) given in Proposition 6.9.4 , see [42], Section 2.3.2 .

Theorem 6.11.1.
The nodal Riemann moduli space \(\RR _N\) of stable nodal boundary un-noded discs with \(N=\#A\) interior marked points admits a naturally oriented orbifold structure of dimension \(2\#A\).

7. Polyfold perturbations

We prove Theorem 5.1.2 under assumption (ii). For that we place ourselves into the situation of Section 5.3 and follow the line of reasoning of the proof of Theorem 5.1.2 part (i). As we will not assume semi-positivity this time regularity of relevant moduli spaces can only be achieved for simple nodal holomorphic discs via perturbing the almost complex structure, cf. Section 5.3 . For non-simple nodal holomorphic discs we will use additional abstract polyfold perturbations as introduced in [43] .

7.1. Boundary un-noded stable disc maps.

We consider the tame almost complex manifold \(\big (\hat {W},\hat {\Omega },\hat {J}\big )\) defined in Section 5.2 . For boundary un-noded nodal discs \((S,j,D)\) as introduced in Section 6.1 we consider smooth maps

\[ u\co (S,\partial S)\lra (\hat {W},N^*) \]

that descend to continuous maps on \(S/D\). If \(D\) is empty we call \(u\) un-noded . If in addition \(Tu\circ j=\hat {J}(u)\circ Tu\) we call \(u\) a nodal holomorphic disc map . Observe that we do not need to consider nodal points on the boundary due to the Gromov compactification described in Remark 4.4.1 .

More generally, we consider continuous maps \(u\co (S,\partial S)\ra (\hat {W},N^*)\) defined on a marked boundary un-noded nodal disc \(\big (S,j,D,\{m_0,m_1,m_2\}\big )\) (see Section 6.1 ) such that \(u\) descends to a continuous map on the quotient \(S/D\) and such that \(u\big (\!\Int S\big )\subset \Int \hat {W} \). Moreover, we require that \(u\) is contained in the Sobolev space of square integrable maps

\[ H^{3,\sigma }(S,j)\equiv H^{3,\sigma }\big (S,j,D,\{m_0,m_1,m_2\}\big ) \]

following [43], Definition 1.1 : We require that \(u\) is of class \(u\in H_{\loc }^3\big (S\setminus |D|\big )\) and that w.r.t. positive holomorphic polar coordinates \([0,\infty )\times S^1\), \(S^1=\R /2\pi \Z \), about the nodal points \(|D|\) (see Section 6.10 ) the map \(u\) is of weighted Sobolev class \(H^{3,\sigma }\). The weights are given by \(\rme ^{\sigma s}\), \(s\in [0,\infty )\), for some \(\sigma \in (0,1)\). In other words, \(u\) is contained in \(H^{3,\sigma }\) precisely if all weak derivatives \(D^{\alpha }u\), \(|\alpha |\leq 3\), of \(u\) on \([0,\infty )\times S^1\) exist and all \(D^{\alpha }u\cdot \rme ^{\sigma s}\), \(|\alpha |\leq 3\), are square integrable on \([0,\infty )\times S^1\). The latter is equivalent to \(u\,\rme ^{\sigma s}\in H^3\) on \([0,\infty )\times S^1\). In particular, by Sobolev embedding, \(u\) is \(C^1\) (up to the boundary \(\partial S\)) restricted to \(S\setminus |D|\). But in general \(u\) is not differentiable at the nodal points \(|D|\) on \(S\). Consider for example the continuous function \(u(z)=|z|^{\frac {1+\sigma }{2}}\) in holomorphic coordinates \(z\in \C \), which w.r.t. positive holomorphic polar coordinates reads as \((s,t)\mapsto \rme ^{-\frac {1+\sigma }{2}s}\).

The space \(H^{3,\sigma }(S,j)\) is well defined, i.e. invariant under coordinate changes after possibly shrinking the chart domains. Away from the nodes \(|D|\) this follows as for \(H_{\loc }^3\big (S\setminus |D|\big )\) via [4], Theorem 3.41 . Near the nodes we observe that the area form \(\rme ^{2\sigma s}\rmd t\wedge \rmd s\) w.r.t. positive holomorphic polar coordinates corresponds to the singular area form \(|z|^{-2(1+\sigma )}\frac {\rmi }{2}\rmd z\wedge \rmd \bar {z}\) in holomorphic coordinates about the nodal point \(0\in \C \). The area form \(\frac {\rmi }{2}\rmd z\wedge \rmd \bar {z}\) transforms under biholomorphic coordinate changes via a conformal factor, which we can assume to be bounded above and away from zero by shrinking the chart domains if necessary. The coordinate change itself is of the form \(z\mapsto zh(z)\), where \(0\) corresponds to a nodal point. Here \(h\) is a holomorphic function, whose absolute value can be assumed to be bounded above and away from zero also. Consequently, the singular area form \(|z|^{-2(1+\sigma )}\frac {\rmi }{2}\rmd z\wedge \rmd \bar {z}\) transforms via a bounded above and away from zero conformal factor also. Hence, the same holds true for \(\rme ^{2\sigma s}\rmd t\wedge \rmd s\). In fact, the above coordinate change becomes

\[ (s,t)\longmapsto (s,t)-\ln \Big (h\big (\rme ^{-(s+\rmi t)}\big )\Big ) \,, \]

whose derivatives are bounded above and whose first derivative is bounded away from zero. Therefore, invariance under coordinate changes near the nodes follows as in [4], Theorem 3.41 . By the same arguments we see that locally defined norms on \(H_{\loc }^3\) and \(H^{3,\sigma }\) transform via the respective coordinate changes to equivalent norms. This defines a topology on \(H^{3,\sigma }(S,j)\); a neighbourhood base is given by the set of those maps that restricted to one of the above charts belong to an open set in \(H_{\loc }^3\) and \(H^{3,\sigma }\), resp.

To each \(u\in H^{3,\sigma }(S,j)\) we assign the symplectic energy integral

\[ \int _Su^*\hat {\Omega } \]

by approximating the continuous map \(u\) by a \(C^1\)-map \(v\) and defining the symplectic energy integral via \(\int _Su^*\hat {\Omega }:=\int _Sv^*\hat {\Omega }\). This is well defined and, in fact, by Stokes theorem, independent of the choice of representative of the homology class \([u]\) in \(\hat {W}\) relative \(u(\partial S)\subset N^*\). This can be seen as follows: Taking approximations \(v\) of \(u\) that are equal to \(u\) restricted to the complement of disc like neighbourhoods \(B_r(0)\) in \(S\) of the nodal points \(0\in |D|\) the symplectic energy integral is given by \(\int _{S\setminus |D|}u^*\hat {\Omega }\). Indeed, take \(r>0\) so small such that the \(B_r(0)\) are contained in pair-wise disjoint chart domains of \(S\) about the nodal points \(0\) in \(|D|\) and such that the \(u\big (B_r(0)\big )\) are contained in pair-wise disjoint ball like chart domains of \(\hat {W}\). By Stokes theorem decomposing \(B_r(0)=\big (B_r(0)\setminus B_{\varepsilon }(0)\big )\cup B_{\varepsilon }(0)\) it suffices to show that the integrals

\[ \int _{B_{\varepsilon }(0)}u^*\hat {\Omega } \qquad \text {and} \qquad \int _{\partial B_{\varepsilon }(0)}u^*\lambda \]

converge to zero as \(\varepsilon \in (0,r)\) tends to \(0\), where \(\lambda \) is a local primitive of \(\hat {\Omega }\) defined on the ball like neighbourhoods of \(u(|D|)\) in \(\hat {W}\). By the transformation formula we can compute the integrals w.r.t. positive holomorphic polar coordinates via

\[ \int _{(R,\infty )\times S^1}\hat {\Omega }(u_s,u_t)\,\rmd s\wedge \rmd t \qquad \text {and} \qquad \int _{\{R\}\times S^1}\lambda (u_t)\,\rmd t \]

for \(R=-\ln \varepsilon \). By the Sobolev inequality the \(C^1\)-norm of \(u\,\rme ^{\sigma s}\) on \([0,\infty )\times S^1\) is bounded by \(\|u\|_{3,\sigma }\), so that up to a positive constant the absolute value of the integrals is bounded by

\[ \|u\|_{3,\sigma }^2\int _R^{\infty }\rme ^{-2\sigma s}\rmd s \qquad \text {and} \qquad \|u\|_{3,\sigma }\,\rme ^{-\sigma R} \,, \]

resp. In both cases the first factor is bounded by assumption; the second tends to zero for \(R\ra \infty \) and the claim follows, namely, that \(\int _Su^*\hat {\Omega }\) is well defined.

Remark 7.1.1.
The above arguments show that \(u\mapsto \int _Su^*\hat {\Omega }\) is a continuous function on \(H^{3,\sigma }(S,j)\).

We call \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\) a nodal disc map provided that the following conditions are satisfied (cf. Section 5.3 ):


  1. \(u\in H^{3,\sigma }(S,j)\),
  2. the symplectic energy integral restricted to a connected component \(C\) of \(S\)

    \[ \int _Cu^*\hat {\Omega }\geq 0 \]

    is non-negative for all spherical components \(C\) of \(S\); positive on the disc component,

  3. the continuous map on \(S/D\) induced by \(u\) is homologous to a local Bishop discs \(u_{\varepsilon ,b_o}\) relative \(N^*\), so that \([u(S)]=[u_{\varepsilon ,b_o}(\D )]\) in \(H_2(\hat {W},N^*)\), and
  4. \(u(m_0)\in \gamma \) and \(\vartheta \circ u(m_k)=\rmi ^k\) for \(k=1,2\).

For given \(\big (S,j,D,\{m_0,m_1,m_2\}\big )\) the space

\[ \HH ^{3,\sigma }(S,j) \]

of nodal disc maps is called the space of admissible maps .

It follows that the degree of the \(C^1\)-map \(\vartheta \circ u\co \partial S\ra S^1\) equals \(1\) for all nodal disc maps \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\). With the properties of the symplectic energy integral discussed above we obtain as in item (2) of Section 4.4 that

\[ \int _Su^*\hat {\Omega }= \int _{\partial S} u^*f\cdot (\vartheta \circ u)^*\rmd \theta \,, \]

where \(f\) is a smooth function on \(N\) that is positive on \(N^*\) and vanishes on \(B\cup \partial N\). As \(u\) takes values in \(N^*\) along the boundary \(\partial S\) we get that

\[ \int _Su^*\hat {\Omega } \in \big (0,2\pi \max f\big ] \]

for all nodal disc maps \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\). By non-negativity of the symplectic energy integral on each connected component \(C\) of \(S\) we get that \(\int _Cu^*\hat {\Omega }\) takes values in \(\big [0,2\pi \max f\big ]\). Moreover, as \(\int _Cu^*\hat {\Omega }\) only depends on the homology class represented by \(u(C)\) for the spherical components \(C\) of \(S\) assumption (2) puts an open condition to the space defined via \(H^{3,\sigma }(S,j)\) and the constraints given by (3) and (4), so that the space of admissible maps \(\HH ^{3,\sigma }(S,j)\) is an open subset.

In fact, \(\HH ^{3,\sigma }(S,j)\) is a Hilbert manifold whose tangent space \(\HH ^{3,\sigma }\big (u^*T\hat {W}\big )\) at \(u\in \HH ^{3,\sigma }(S,j)\) is the space of \(H^{3,\sigma }\)-sections into \(u^*T\hat {W}\) that descent to continuous sections on \(S/D\), that are tangent to \(N^*\) along \(\partial S\) as well as tangent to \(\gamma \) at \(m_0\) and to the page \(\vartheta ^{-1}(\rmi ^k)\) at \(m_k\) for \(k=1,2\). This follows with the exponential map taken w.r.t. a metric on \(\hat {W}\) for which each of the submanifolds \(N\), \(\vartheta ^{-1}(\rmi ^k)\), \(k=1,2\), and \(\gamma \) is totally geodesic. The requirement for the sections to be of class \(H^{3,\sigma }\) is understood as in Section 7.1 , so that a norm on \(\HH ^{3,\sigma }\big (u^*T\hat {W}\big )\) as on [43], p. 66 can be defined. This turns \(\HH ^{3,\sigma }(S,j)\) into a Riemannian Hilbert manifold.

By removal of singularities (see [54] ) a holomorphic \(u\in H^{3,\sigma }(S,j)\), which is continuous and has finite symplectic energy by the above discussion, is holomorphic on \(S\). Therefore, \(u\) is smooth up to the boundary including all nodal points \(|D|\) so that holomorphicity coincides with the notion of holomorphicity from the beginning of this section.

Given a nodal disc map \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\) we call a connected component \(C\) of \(S\) with vanishing symplectic energy integral a ghost bubble . Observe that a holomorphic nodal disc map restricted to a ghost bubble is constant. If \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\) is any nodal disc map such that each ghost bubble admits at least \(3\) nodal points, then we call \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\) a stable nodal disc map .

7.2. Boundary un-noded stable discs.

We call two stable nodal disc maps

\[ \big (S,j,D,\{m_0,m_1,m_2\},u\big ) \quad \text {and} \quad \big (S',j',D',\{m'_0,m'_1,m'_2\},u'\big ) \]

equivalent if there exists a diffeomorphism \(\varphi \co S\ra S'\) such that \(\varphi ^*j'=j\), the injection \(D\ra D'\) defined by \(\{\varphi (x),\varphi (y)\}\in D'\) for all \(\{x,y\}\in D\) is surjective, \(\varphi (m_k)=m'_k\) for \(k=0,1,2\), and \(u'\circ \varphi =u\). The discussions in Section 7.1 about \(H^{3,\sigma }(S,j)\) imply that this equivalence relation is well defined. The equivalence classes

\[ \mathbf u=\big [S,j,D,\{m_0,m_1,m_2\},u\big ] \]

are called stable nodal discs in \(\big (\hat {W},\hat {\Omega }\big )\) relative \(N^*\). The space of all equivalence classes is denoted by \(\ZZ \).

Fixing the diffeomorphism type of \(S\) and the combinatorial data \(\big (D,\{1,\rmi ,-1\}\big )\) of \(\big (S,j,D,\{1,\rmi ,-1\},u\big )\) as at the beginning of Section 6.3 we can write

\[ \ZZ =\Big \{ \bfu =[j,u]\,\,\text {stable} \,\Big |\, [u(S)]=[u_{\varepsilon ,b_o}(\D )] \,,\,\, u(1)\in \gamma \,,\,\, \vartheta \circ u(\rmi ^k)=\rmi ^k \,, k=1,2 \Big \} \]

for the space of all stable nodal discs

\[ \bfu =\big [S,j,D,\{1,\rmi ,-1\},u\big ]\equiv [j,u] \,,\quad u\in \HH ^{3,\sigma }(S,j)\,, \]

in \(\big (\hat {W},\hat {\Omega }\big )\) relative \(N^*\).

We define the nodal type \(\tau \) of \(\big (S,D,\{1,\rmi ,-1\}\big )\) as in Section 6.2 . Namely, the nodal type is the isomorphism class of the rooted tree given as follows: The vertices correspond to the components of \(S\). The root is given by the disc component. The edge relation is induced by the nodes in \(D\). As this time there are no auxiliary marked points all vertices different from the root are not weighted; the root has weight \(3\). The induced nodal type \(\tau \) is necessarily unstable provided that there is at least one sphere component. Indeed, in this case, any end of a branch admits only one special point.

We denote by \(\ZZ _{\tau }\) the space of all stable nodal discs of nodal type \(\tau \), so that \(\ZZ \) is the disjoint union of the \(\ZZ _{\tau }\) where \(\tau \) ranges over all nodal types just described. Each of the subspaces \(\ZZ _{\tau }\) of \(\ZZ \) is the quotient of the total space of the fibration over \(\JJ \equiv \JJ (S)\) with fibre \(\HH ^{3,\sigma }(S,j)\) over \(j\in \JJ \) by the action \(\varphi \mapsto (\varphi ^*j,u\circ \varphi )\) of the group of orientation preserving diffeomorphisms \(\varphi \) of \(S\) preserving \(\big (D,\{1,\rmi ,-1\}\big )\), cf. Section 6.3 . This puts a topology to \(\ZZ _{\tau }\) similarly to Remark 6.3.2 .

Notice that the stabiliser of the action is finite by the stability condition formulated at the end of Section 7.1 : Each automorphism of \(\bfu \) acts via the identity map on the disc component due to the ordered boundary marked points \(\{1,\rmi ,-1\}\). If \(\int _Cu^*\hat {\Omega }=0\) for a connected component \(C\) of \(S\), then the number of nodal points \(C\cap |D|\) on \(C\) is at least \(3\). Furthermore, the automorphisms of \(\bfu \) preserve those ghost components due to the transformation formula. If \(\int _Cu^*\hat {\Omega }>0\), one finds \(z\in C\setminus |D|\) such that \(u\) is immersive on \(C\cap u^{-1}\big (u(z)\big )\) defining finitely many local branches via \(C\cap u^{-1}\big (B_r\big )\subset C\setminus |D|\) for a sufficiently small ball \(B_r\subset \Int \hat {W}\) around \(u(z)\). In fact, due to the positivity of the symplectic energy integral we can find \(z\in C\setminus |D|\) and \(r>0\) sufficiently small such that \(u^*\hat {\Omega }\) is a positive area form on the branch through \(z\), which is oriented via \(j\). Observe that \(u^*\hat {\Omega }\) is a positive area form on all branches through the points of the orbit (of the automorphism group of \(\bfu \)) defined by \(z\). Identifying the sphere components with \((\C P^1,\rmi )\) as in Remark 6.3.1 the identity theorem yields that an automorphism of \(\bfu \) acts by a permutation on the local branches. This proves finiteness of the stabiliser.

In the following we describe a polyfold structure on \(\ZZ \) that glues the components \(\ZZ _{\tau }\) together. For any \(\bfu =\big [S,j,D,\{1,\rmi ,-1\},u\big ]\) in \(\ZZ \) one can choose a so-called stabilisation , which is a finite set of auxiliary marked points \(A\subset S\) disjoint from the special points \(D\cup \{1,\rmi ,-1\}\) such that the nodal disc \(\big (S,j,D,\{1,\rmi ,-1\},A\big )\) is stable in the sense of Section 6.2 . Due to the stability condition there is no need to provide the ghost bubbles with an auxiliary markt point. In addition one can assume, that the automorphisms of \(\bfu \) preserve \(A\), \(u(A)\) is disjoint from the \(u\)-image of \(D\cup \{1,\rmi ,-1\}\), and the following two conditions hold:


  1. Whenever \(z,w\in A\) are mapped to the same point \(u(z)=u(w)\) in \(\hat {W}\), then there exists an automorphism of \(\bfu \) sending \(z\) to \(w\).
  2. For all \(z\in A\) the \(2\)-form \((u^*\hat {\Omega })_z\) is positive on \((T_zS,j_z)\).

This follows with [43], Lemma 3.2 ignoring the disc component, which already is stable: Namely, successively select finite orbits of the action of the automorphism group of \(\bfu \) on local branches similarly to the above finiteness argument until all components are stable. Consequently, the underlying stable nodal disc \(\big [S,j,D,\{1,\rmi ,-1\},A\big ]\) possesses a uniformiser as described in Section 6.11 .

As in Section 5.3 we wish to achieve an index-\(1\) Fredholm problem. In view of Theorem 6.11.1 we compensate the stabilising auxiliary marked points \(A\) index-wise as follows: We choose a finite collection of pairwise disjoint codimension-\(2\) symplectic discs in \((\Int \hat {W},\hat {\Omega })\) that intersect \(u(S)\) along \(u(A)\) transversally. This is possible by condition (2) above. Namely, the image of \(Tu\) at each auxiliary marked point in \(A\) is a symplectic plane in \(T\hat {W}\). Integrating the respective symplectic normal subspaces one finds symplectic embeddings of small discs of codimension \(2\) that are normal to \(u(S)\) at the images of the auxiliary marked points \(u(A)\). We call the union of the discs \(H_{u,A}\) local transversal constraints if the intersection of \(u(S)\) and \(H_{u,A}\) equals \(u(A)\) and if each component of \(H_{u,A}\) intersects \(u(S)\) in a single point.

We denote by

\[ E_{u,A}\subset \HH ^{3,\sigma }\big (u^*T\hat {W}\big ) \]

the subspace of sections that are tangent to \(H_{u,A}\) at the stabilising auxiliary points in \(A\), which is scale-linear w.r.t. to \((3+\nu ,\sigma _{\nu })\), \(\nu \in \N _0\), for a strictly increasing sequence \(\sigma _{\nu }\) in \((0,1)\) with \(\sigma _0=\sigma \), see [43], Section 2.6 . Uniformiser about any \(\bfu =\big [S,j,D,\{1,\rmi ,-1\},u\big ]\) in \(\ZZ \) of the desired polyfold structure are obtained as in [43], Section 3.1/3.2 . To adapt to our situation start off with uniformisers for the stabilised domain \(\big [S,j,D,\{1,\rmi ,-1\},A\big ]\in \RR \) from Section 6.11 and consider the deformation

\[ (y,\bfa ,\eta ) \longmapsto \big (S_{\bfa },j(y)_{\bfa },D_{\bfa },\{1,\rmi ,-1\},\oplus _{\bfa }\exp _u(\eta )\big ) \,, \]

where \((y,\bfa )\in \VV \) for an open subset \(\VV \) of \(V_j\times \D ^D\), \(\eta \in E_{u,A}\) is a sufficiently small section that is a fixed point of the splicing projection \(\pi _{\bfa }\) and \(\oplus _{\bfa }\exp _u(\eta )\) denotes the gluing operation both introduced in [43], Section 2.4/2.5 . Choosing \(u\) to be a smooth approximation of an element in \(H^{3,\sigma }(S,j)\) we obtain scale-smooth gluing maps w.r.t. to the scale \((3+\nu ,\sigma _{\nu })\), see [43], Section 2.2/2.6 . Using Remark 6.3.2 , Section 6.11 and [43], Section 3.3/3.4 one obtains a natural second countable paracompact Hausdorff topology on \(\ZZ \) similarly to [43], Theorem 1.6 . In the same way using this time modifications in [43], Section 3.5 the space \(\ZZ \) carries the structure of a polyfold as formulated in [43], Theorem 1.7 with a scale-smooth evaluation map \(\ZZ \ra \gamma \) sending \(\bfu \) to \(u(1)\), cf. [43], Theorem 1.8 .

7.3. A nodal moduli space.

We call \(\bfu \) a stable nodal holomorphic disc if \(\bfu \) can be represented by a stable nodal holomorphic disc map \(u\). Notice, that all stable nodal disc maps \(u\) that represent a stable nodal holomorphic disc \(\bfu \) are holomorphic. Denote by

\[ \NN :=\big \{ \bfu \in \ZZ \,\big |\, \bfu \,\,\,\text {is holomorphic} \big \} \]

the nodal moduli space of all stable nodal holomorphic discs.

Using uniformisation it is convenient to represent the classes \(\mathbf u\in \NN \) by holomorphic maps \(u\in \HH ^{3,\sigma }(S,j)\) whose disc component has domain \(\big (\D ,\rmi ,\{1,\rmi ,-1\}\big )\) and for which the sphere components are given by \((\C P^1,\rmi )\), cf. Remark 6.3.1 . If \(\bfu \) is un-noded, then we obtain \(\bfu =\big [\D ,\rmi ,\emptyset ,\{1,\rmi ,-1\},u\big ]\). We abbriviate the elements \(\mathbf u=[\rmi ,u]\in \NN \) (noded or un-noded) simply by \([u]\) for the following discussion:

The boundary conditions for \(\HH ^{3,\sigma }(S,j)\) formulated in Section 7.1 are the boundary conditions used in Sections 4.4 and 5.3 . In particular, all properties formulated in the un-noded case for holomorphic discs in Section 4.4 continue to hold in the noded case, hence, for all \(\bfu =[u]\in \NN \) in the following sense:


  1. The winding number of \(\bfu =[u]\in \NN \), which by definition is the degree of the map \(\vartheta \circ u\co \partial S\ra S^1\), is equal to \(1\). In particular, \(u(\partial S)\) is an embedded curve in \(N^*\) positively transverse to \(\xi \) and the restriction of \(u\) to the disc component of \(S\) is a simple holomorphic map.
  2. The symplectic energy \(\int _{S}u^*\hat {\Omega }\) of \(\bfu =[u]\in \NN \), which is well defined and positive by Section 7.1 , is uniformly bounded.
  3. The boundary circle \(u(\partial S)\) of \(\bfu =[u]\in \NN \) is disjoint from \(U_{\partial N}\) because the restriction of \(u\) to the disc component of \(S\) must be disjoint from \(U_{\partial N}\) by Lemma 3.5.1 . If \(u(S)\) intersects \(U_B\) then \(\bfu \) is un-noded and equivalent to a local Bishop disc \(u_{\varepsilon ,b_o}\) by Lemma 3.3.1 combined with the final paragraph of Remark 4.4.1 .

The local Bishop discs \(u_{\varepsilon ,b_o}\), \(\varepsilon \in (0,\delta )\), represent elements

\[ \bfu _{\varepsilon ,b_o}= \big [\D ,\rmi ,\emptyset ,\{1,\rmi ,-1\},u_{\varepsilon ,b_o}\big ] \]

in \(\NN \). The corresponding local Bishop filling can be identified with \((0,\delta )\). We truncate the nodal moduli space \(\NN \) via

\[ \NN _{\cut }=\NN \setminus (0,\delta /2)\,. \]

Remark 7.3.1.
If there exists a compact subset \(K\) of \(\hat {W}\) such that \(\bfu (S)\) is contained in \(K\) for all \(\bfu \in \NN \), then the Gromov compactification of \(\MM _{\gamma }\) can be identified with a subset of \(\NN \) by taking equivalence classes, see [25] .

7.4. Cauchy–Riemann section.

The moduli space \(\NN \) is the zero set

\[ \NN =\big \{ \bfu \in \ZZ \,\big |\, \CR {\!\hat {J}}\mathbf u=\mathbf 0 \big \} \]

of the Cauchy–Riemann operator \(\CR {\!\hat {J}}\), which appears as a section into the bundle

\[ p\co \WW \lra \ZZ \]

over \(\ZZ \). The fibre of \(p\) over \(\mathbf u=\big [S,j,D,\{1,\rmi ,-1\},u\big ]\in \ZZ \) consists of equivalence classes \(\boldxi =\big [S,j,D,\{1,\rmi ,-1\},u,\xi \big ]\) of continuous sections \(\xi \) of \(\Hom \big (TS,u^*T\hat {W}\big )\) so that for each \(z\in S\) the map \(\xi (z)\co T_zS\ra T_{u(z)}\hat {W}\) is complex anti-linear with respect to \(j(z)\) and \(\hat {J}\big (u(z)\big )\). Moreover, \(\xi \) is of Sobolev class \(H^2_{\loc }\) on \(S\setminus |D|\) and of weighted Sobolev class \(H^{2,\sigma }\) near \(|D|\) similarly to the description at the beginning of Section 7.1 , see [43], Section 1.2 . Two such sections \(\big (S,j,D,\{m_0,m_1,m_2\},u,\xi \big )\) and \(\big (S',j',D',\{m'_0,m'_1,m'_2\},u',\xi '\big )\) are equivalent , if there exists an equivalence \(\varphi \) of stable nodal disc maps \(\big (S,j,D,\{m_0,m_1,m_2\},u\big )\) and \(\big (S',j',D',\{m'_0,m'_1,m'_2\},u'\big )\) as described at the beginning of Section 7.2 such that \(\xi '\circ T\varphi =\xi \). By adapting [43], Theorem 1.9 to the situation of the current Sections 6 and 7 we obtain a natural second countable paracompact Hausdorff topology on the total space \(\WW \) and the bundle projection \(p\co \WW \ra \ZZ \) that maps \(\big [S,j,D,\{1,\rmi ,-1\},u,\xi \big ]\) to \(\big [S,j,D,\{1,\rmi ,-1\},u\big ]\) is continuous. Furthermore \(p\co \WW \ra \ZZ \) constitutes a strong polyfold bundle in view of [43], Theorem 1.10 .

The Cauchy–Riemann operator \(\CR {\!\hat {J}}\) is the section of \(p\) given by

\[ \CR {\!\hat {J}}\mathbf u := \Big [ S,j,D,\{1,\rmi ,-1\},u,\tfrac 12\big (Tu+\hat {J}(u)\circ Tu\circ j\big ) \Big ] \]

for all \(\mathbf u=\big [S,j,D,\{1,\rmi ,-1\},u\big ]\in \ZZ \). For a representative we write \(\CR {\!\hat {J}}u\) also. As in [43], Theorem 1.11 the Cauchy–Riemann operator \(\CR {\!\hat {J}}\co \ZZ \ra \WW \) is a scale-smooth component-proper Fredholm section that admits a natural orientation which we describe in Remark 7.4.3 below. The Fredholm index of \(\CR {\!\hat {J}}\co \ZZ \ra \WW \) is \(1\) by the index computation in Section 5.3 taking local transversal constraints from Section 7.2 in view of Theorem 6.11.1 into account. As in [64], Section 5.3 the vertical differential of a local representation of \(\CR {\!\hat {J}}\) near the local Bishop discs \(\bfu _{\varepsilon ,b_o}\), \(\varepsilon \in (0,\delta )\) has a right-inverse. The same holds true for all simple stable nodal holomorphic discs in \(\ZZ \) due to the generic choice of \(\hat {J}\), see Section 5.3 .

Remark 7.4.1.
Preparing the orientation considerations in Remark 7.4.3 we will establish homotopically unique trivialisations under the assumption that the second Stiefel–Whitney class of \(N^*\) vanishes. This approach requires to build up the spaces \(\HH ^{3,\sigma }(S,j)\) with continuous maps on \(S/D\) homotopic in \((\hat {W},N^*)\) to a local Bisphop disc, see item (3) in Section 7.1 . As the relative homotopy class is preserved under Gromov convergence (see [25] ) this is not a restriction.

Consider the space of continuous maps \((\D ,\partial \D )\ra \big (\hat {W},N^*\big )\) sending the marked points \(\{1\}\) and \(\{\rmi ^k\}\) into \(\gamma \) and \(\vartheta ^{-1}(\rmi ^k)\), \(k=1,2\), resp. Denote by \(\CC \) the connected component of the Bishop disc \(u_0=u_{\delta /2,b_o}\). We claim that for all \(u\in \CC \) the pull back bundle \(u^*TN^*\) has a canonical trivialisation.

In order to specify what is meant by this we describe the situation for \(u_0\). By Section 3.1 the base point \(u_0\) of \(\CC \) is the map

\[ (\D ,\partial \D )\lra \Big ( (-\infty ,0]\times \R \times \C \times T^*B, \{0\}\times \{0\}\times \C ^*\times B \Big ) \]

given by

\[ u_0(z)= \Big ( \tfrac {\delta ^2}{4}\big (|z|^2-1\big ),0,\delta \cdot z,b_o \Big ) \;. \]

in the local model \(U_B\). The embedded path \(\gamma \) corresponds to \(\{0\}\times \{0\}\times \R ^+\times \{b_o\}\) as oriented curve and the pages \(\vartheta ^{-1}(\rmi ^k)\), \(k=1,2\), correspond to \(\{0\}\times \{0\}\times \R ^+\rmi ^k\times B\), resp. The co-orientation of the pages \(\vartheta ^{-1}(\rmi ^k)\), \(k=1,2\), given in Section 2.1 is represented by the normal vectors \((0,0,\rmi ^{k+1},0)\), resp. The local model defines a local frame \(\partial _s,\partial _t,\partial _x,\partial _y,\partial _{\bfp },\partial _{\bfq }\) of the tangent bundle \(T\hat {W}\) near \((-\infty ,0]\times \R \times \C \times \{b_o\}\) inducing a trivialisation \(\Phi \co u_0^*T\hat {W}\ra \D \times \R ^{2n}\) of the pull back bundle \(u_0^*T\hat {W}\). The trivialisation \(\Phi \) restricts to a trivialisation \(\Phi \co u_0^*TN^*\ra \partial \D \times \R ^n\) of \(u_0^*TN^*\), which corresponds to the sub-frame \(\partial _x,\partial _y,\partial _{\bfp }\). Further, \(\Phi \) restricts to isomorphisms \(\Phi \co T_{u_0(1)}\gamma \ra \{1\}\times \R \) via the vector field \(\partial _x\) and \(\Phi \co T_{u_0(\rmi ^k)}\big (\vartheta ^{-1}(\rmi ^k)\big )\ra \{\rmi ^k\}\times \R ^{n-1}\), \(k=1,2\), via the sub-frames \(\partial _y/-\partial _x,\partial _{\bfp }\). The co-orientations of the pages \(\vartheta ^{-1}(\rmi ^k)\) correspond to \(-\partial _x/-\partial _y\), resp. We remark that \(\Phi \) is not a complex trivialisation of the complex bundle pair \(\big (u_0^*T\hat {W},u_0^*TN^*\big )\) as used to compute the Maslov index to be \(2\), see [55], Proposition 8 .

Given any \(u\in \CC \) we claim that the pull back bundle \(u^*TN^*\) admits a homotopically unique trivialisation \(\Phi _u\) with the properties listed for \(\Phi _{u_0}:=\Phi |_{u_0^*TN^*}\). To see this let \(u_{\tau }\), \(\tau \in [0,1]\), be a path in \(\CC \) connecting \(u_0\) with \(u_1=u\) and define \(U\co [0,1]\times \partial \D \ra \hat {W}\) by \(U(\tau ,z):=u_{\tau }(z)\). By [47], Corollary 3.4.5 there exists a trivialisation \(\Phi _U\co U^*TN^*\ra \big ([0,1]\times \partial \D \big )\times \R ^n\) that extends \(\Phi _{u_0}\). As above we denote the coordinates of \(\R ^n\) by \((x,y,\bfp )\). We can assume that \(\Phi _U\) restricts to isomorphisms \(\Phi _U\co \big (U(\,.\,,1)\big )^*T\gamma \ra \big ([0,1]\times \{1\}\big )\times \R \) with \(\R \) provided with the coordinate \(x\) as well as \(\Phi _U\co \big (U(\,.\,,\rmi ^k)\big )^*T\big (\vartheta ^{-1}(\rmi ^k)\big )\ra \big ([0,1]\times \{\rmi ^k\}\big )\times \R ^{n-1}\), \(k=1,2\), with \(\R ^{n-1}\) provided with coordinates \((y/x,\bfp )\) and co-oriantations \(-\partial _x/-\partial _y\), resp. The claimed trivialisation \(\Phi _u\) is \(\Phi _{u_1}=\Phi _U|_{\{1\}\times \partial \D }\).

It remains to show homotopic uniqueness of \(\Phi _u\), i.e. that \(\Phi _u\) is independent of the chosen path \(u_{\tau }\) up to homotopy: We consider a loop \(u_{\tau }\) in \(\CC \) for \(\tau \in T^1=\R /2\Z \) extending a path \(u_{\tau }\), \(\tau \in [0,1]\), in \(\CC \) as above and define \(\hat {U}\co T^1\times \partial \D \ra \hat {W}\) by \(\hat {U}(\tau ,z):=u_{\tau }(z)\). The claim will follow by constructing a trivialisation \(\Phi _{\hat {U}}\) that shares the triviality properties established for \(\Phi _U\).

Restricted to \([0,1]\times \partial \D \) we define \(\Phi _{\hat {U}}\) to be equal to \(\Phi _U\). As \(\hat {U}(T^1\times \{1\})\) is a subset of the embedded interval \(\gamma =[0,1]\) and the tangent bundle \(TN^*\) is trivialised by \(\partial _x,\partial _y,\partial _{\bfp }\) along \(\gamma \cap U_B\) there exists by [47], Corollary 3.4.8 a trivialisation \(\Phi _{\gamma }\co T_{\gamma }N^*\ra [0,1]\times \R ^n\) that extends the canonical trivialisation over \(\gamma \cap U_B\) such that \((x,y,\bfp )\) are coordinates on \(\R ^n\) and such that \(\Phi _{\gamma }\co T\gamma \ra [0,1]\times \R \) is provided with the fibre coordinate \(x\).

Gluing the trivialisations \(\Phi _{\hat {U}}\) and \(\Phi _{\gamma }\) via the identity along the overlap we obtain a trivialisation (still denoted by) \(\Phi _{\hat {U}}\) over \(\big ([0,1]\times \partial \D \big )\cup \big (T^1\times \{1\}\big )\). In other words, \(\Phi _{\hat {U}}\) trivialises \(\hat {U}^*TN^*\) over the boundary of the \(2\)-disc

\[ \big (T^1\times \partial \D \big )\setminus \Big (\big ([0,1]\times \partial \D \big )\cup \big (T^1\times \{1\}\big )\Big ) \,. \]

By the assumption that the second Stiefel–Whitney class of \(N^*\) vanishes this trivialisation extends to a trivialisation of \(\hat {U}^*TN^*\), see [34], p. 75 and Section 3.3 . Hence, \(\Phi _{\hat {U}}\co \hat {U}^*TN^*\ra \big (T^1\times \partial \D \big )\times \R ^n\) is a trivialisation with fibre coordinates \((x,y,\bfp )\). By construction we have a trivialisation \(\Phi _{\hat {U}}\co \big (\hat {U}(\,.\,,1)\big )^*T\gamma \ra \big (T^1\times \{1\}\big )\times \R \) with fibre coordinate \(x\). Further, because a co-oriented linear subspace of \(\R ^n\) of codimension \(1\) is determined by the normal vector and \(S^{n-1}\), \(n\geq 3\), is simply connected we can assume that we have trivialisations \(\Phi _{\hat {U}}\co \big (\hat {U}(\,.\,,\rmi ^k)\big )^* T\big (\vartheta ^{-1}(\rmi ^k)\big )\ra \big (T^1\times \{\rmi ^k\}\big )\times \R ^{n-1}\), \(k=1,2\), with fibre coordinates \((y/x,\bfp )\) and co-oriantations \(-\partial _x/-\partial _y\), resp.

Consequently, \(u_1^*TN^*\) shares the same triviality properties as \(u_0\) independently of the chosen path \(u_t\) such that \(\Phi _{u_1}\) is homotopically unique as claimed.

Remark 7.4.2.
If the second Stiefel–Whitney class \(w_2(TN^*)\) of \(N^*\) is not trivial a variant of Remark 7.4.1 gives homotopically unique stable trivialisations assuming \(N^*\) to be orientable and that \(w_2(TN^*)\) lifts to a class in \(H^2(\hat {W};\Z _2)\).

Following [26], Chapter 8.1 we choose a triangulation of \(\hat {W}\) such that \(N\) will be a subcomplex and \(B\cup \partial N\) a subcomplex of \(N\). The assumptions made allow the choice of a relative spin structure on \((\hat {W},N^*)\) which is a choice of orientation on \(N^*\), an oriented vector bundle \(V\) over the \(3\)-skeleton \(\hat {W}_{[3]}\) of \(\hat {W}\) such that \(w_2(V)\) restricts to \(w_2(TN^*)\), and a spin structure on the vector bundle \(TN^*\oplus V\) over the \(2\)-skeleton \(N^*_{[2]}\) of \(N^*\). Such a choice of a spin structure is possible because \(w_2\) of \(TN^*\oplus V\) over \(N^*_{[2]}\) vanishes, see [12] .

As in Remark 7.4.1 we consider the space of continuous maps \((\D ,\partial \D )\ra \big (\hat {W},N^*\big )\) that map \(\{1\}\) and \(\{\rmi ^k\}\) into \(\gamma \) and \(\vartheta ^{-1}(\rmi ^k)\), \(k=1,2\), resp. By simplicial approximation (see [16], Theorem IV.22.10 ) we can replace all maps and homotopies of maps by simplicial representatives \(u\) and \(u_t\) up to homotopy. Therefore, the proof of [26], Theorem 8.1.1 yields homotopically unique trivialisations of \(u^*(TN^*\oplus V)\) and \(u^*V\). Similarly to Remark 7.4.1 we can achieve that \(T\gamma \) and \(T\big (\vartheta ^{-1}(\rmi ^k)\big )\), \(k=1,2\), correspond to \(\{1\}\times \R \) and \(\{\rmi ^k\}\times \R ^{n-1}\), resp., in the trivialisation \(\D \times \R ^{n+v}\) of \(u^*(TN^*\oplus V)\), where \(v\) denotes the rank of the vector bundle \(V\). Moreover, by possibly changing the spin structure on \(TN^*\oplus V\) over \(N^*_{[2]}\) we can assume that the obtained trivialisation of \(u_0^*(TN^*\oplus V)\) for the Bishop disc \(u_0\) is homotopic to the canonical one induced by \(\Phi _{u_0}\), see Remark 7.4.1 .

Remark 7.4.3.
The canonical trivialisations of the involved pull back bundles in Remark 7.4.1 and 7.4.2 orient the Cauchy–Riemann section \(\CR {\!\hat {J}}\co \ZZ \ra \WW \) in a natural way. This is based on [26], Lemma 8.1.4 .

Namely, given a complex bundle pair \((E,F)\) over \((\D ,\partial \D )\) such that the real sub-bundle \(F\) is trivial over \(\partial \D \) each trivialisation orients the associated linear Cauchy–Riemann operator. The complexification of the trivialisation extends to a complex trivialisation of \(E\) over an annulus neighbourhood of \(\partial \D \). Collapsing the inner boundary component of a slightly smaller annulus neighbourhood of \(\partial \D \) yields a complex bundle pair over a one-noded disc. Over the sphere component the Cauchy–Riemann operator admits the complex orientation, which is canonical. Over the disc component the Cauchy–Riemann operator is onto with kernel consisting of constant sections. Hence, the kernel is isomorphic to an Euclidean space canonically, so that the Cauchy–Riemann operator is canonically oriented over the disc component. Incorporating the matching condition of the bundles over the two components the functoriality properties of the determinant line bundle canonically determine an orientation of the Cauchy–Riemann operator on \((E,F)\), see [26], Lemma 8.1.4 and cf. [43], Section 5.10 .

Observe that this construction is compatible with point-wise boundary conditions and also allows to begin with a complex bundle pair \((E,F)\) with matching conditions over a noded disc.

In order to orient the linearised Cauchy–Riemann operator at an un-noded element \(u\) of \(\HH ^{3,\sigma }(S,j)\) apply the above construction to the complex bundle pair \(\big (u^*T\hat {W},u^*TN^*\big )\) in the context of Remark 7.4.1 (restricting to the connected component of discs homotopic to a local Bishop disc), and to the complex bundle pairs \(\big (u^*(T\hat {W}\oplus V_{\C }),u^*(TN^*\oplus V)\big )\) and \((u^*V_{\C },u^*V)\), where \(V_{\C }:=V\otimes \C \), in the context of Remark 7.4.2 , resp. For the latter use the arguments in the proof of [26], Theorem 8.1.1 and the observation that the noded discs in \(\HH ^{3,\sigma }(S,j)\) are at least of codimension \(2\). In fact, we obtain canonical orientations of the linearised Cauchy–Riemann operator at noded elements of \(\HH ^{3,\sigma }(S,j)\) also with the above construction.

With the proceeding remarks a canonical orientation of the Cauchy–Riemann section \(\CR {\!\hat {J}}\co \ZZ \ra \WW \) is obtained as in [43], Section 5.11 . Simply, replace the complex orientation of the sphere case by the canonical orientation induced by boundary trivialisations of pull back bundles in the arguments of [43], Section 5.11 . Furthermore observe that preservation of orientations of the partial Kodaira differentials on the Riemann moduli spaces is ensured by Theorem 6.11.1 , \(\ZZ _{\tau }\) is at least of codimension \(2\) for all non-trivial nodal types \(\tau \) by Proposition 6.9.4 , automorphisms of nodal discs in \(\ZZ \) restrict to the identity on the disc component as well as that we can collapse the interior boundary component of a small collar annulus in [26], Lemma 8.1.4 such that auxiliary marked points are contained on the resulting sphere components exclusively.

Proof of Theorem 5.1.2 part (ii).

We place ourselves in to the situation of Section 5.2 and 5.3 ; but this time we do not assume semi-positivity as in Theorem 5.1.2 part (i). Instead, we assume the vanishing of \(w_2(TN^*)\) or the relative spin condition as formulated in Theorem 5.1.2 part (ii) so that Remark 7.4.3 applies. The aim is to derive a contradiction to the existence of a compact subset \(K\) of \(\hat {W}\) such that \(u(S)\subset K\) for all \(\bfu =\big [S,j,D,\{1,\rmi ,-1\},u\big ]\in \NN \). Theorem 5.1.2 part (ii) will then follow as in the proof of part (i).

We argue by contradiction assuming that such a compact subset \(K\) as above exists. The arguments form Remark 4.4.1 under the assumed \(C^0\)-bounds on \(\NN \) combined with Section 7.3 show compactness of \(\NN _{\cut }\), see Remark 7.3.1 . Let \(W_{\!K}\) be a relative compact open neighbourhood of \(K\) in \(\hat {W}\). Using Sobolev embedding we choose a neighborhood \(\UU \subset \ZZ \) of \(\NN _{\cut }\) such that \(u(S)\subset W_{\!K}\setminus \big (U_B'\cup U_{\partial N}\big )\) for all \(\bfu =\big [S,j,D,\{1,\rmi ,-1\},u\big ]\) in \(\UU \), where \(U_B'\subset U_B\) is defined as \(U_B\) but with \(\delta \) replaced by \(\delta /2\) in the proof of Lemma 3.3.1 .

Let \(\lambda \co \WW \ra \Q \cap [0,\infty )\) be a scale\(^+\)-multisection of \(p\co \WW \ra \ZZ \), i.e. \(\lambda \) is a groupoidal functor which in a local presentation is given by finitely many weighted local scale\(^+\)-sections \((s_i,w_i)\), \(w_i\in \Q \cap (0,\infty )\), of total weight \(\sum w_i=1\) such that \(\lambda (\boldxi )\) is the sum of those weights \(w_i\) for which the corresponding sections \(s_i\) satisfy \(s_i\big (p(\boldxi )\big )=\boldxi \); we set \(\lambda (\boldxi )=0\) if there is no such section among the \(s_i\), cf. [40], Definition 3.34 . The support of \(\lambda \) is the smallest closed set in \(\ZZ \) outside which \(\lambda \) is trivial in the sense that \(\lambda (0_{\bfu })=1\) for these \(\bfu \in \ZZ \), see [40], Definition 3.35 . The solution set

\[ \SS =\Big \{\bfu \in \ZZ \;\Big |\;\lambda \big (\CR {\!\hat {J}}\bfu \big )>0\Big \} \]

of the pair \(\big (\CR {\!\hat {J}},\lambda \big )\) is the set of all \(\bfu =\big [S,j,D,\{1,\rmi ,-1\},u\big ]\in \ZZ \) for which in a local presentation of \(\lambda \) there exist at least one \(s_i\) such that \(\CR {\!\hat {J}}u=s_i(u)\) and \(\lambda \big (\CR {\!\hat {J}}\bfu \big )\) is the sum of all the weights \(w_i\) for which the corresponding \(s_i\) satisfy such an equation. The solution set \(\SS \) is equipped with the weight function

\[ \lambda _{\CR {\!\hat {J}}}\co \ZZ \lra \Q \cap (0,\infty ) \,, \quad \bfu \longmapsto \lambda \big (\CR {\!\hat {J}}\bfu \big ) \,, \]

see [40], Section 4.3 .

With [40], Theorem 4.17 we choose \(\lambda \) such that the support of \(\lambda \) is contained in \(\UU \) and that \(\big (\CR {\!\hat {J}},\lambda \big )\) is transverse . The latter means that the vertical differentials

\[\big (\CR {\!\hat {J}}\big )'(u)-s'_i(u)\]

of local presentations \(\CR {\!\hat {J}}u\) of \(\CR {\!\hat {J}}\bfu \) and \(s_i\) of \(\lambda \) are surjective for all \(\bfu \in \SS \) and for all (the finitely many) \(i\), see [40], Definition 4.7(1) . If \(\big (\CR {\!\hat {J}}\big )'(u)\) is onto for an un-noded \(\bfu \in \NN \), which is representable by a necessarily simple holomorphic disc map, we choose \(\lambda \) to be a single local section \(s_1\) that is identically \(0\) in a neighbourhood of \(\bfu \) in \(\ZZ \). This is possible in view of the proof of [40], Theorem 4.17 . In particular, \(\lambda \) is trivial over those \(\bfu \). As observed right before Remark 7.4.1 this applies to all local Bishop discs \(\bfu _{\varepsilon ,b_o}\), \(\varepsilon \in [\delta /2,\delta )\), so that \(\lambda \) is trivial over all local Bishop discs \(\bfu _{\varepsilon ,b_o}\). Consequently, the truncated solution set

\[ \SS _{\cut }=\SS \setminus (0,\delta /2) \]

of \(\big (\CR {\!\hat {J}},\lambda \big )\) is a \(1\)-dimensional oriented compact branched suborbifold with boundary \(\partial \SS _{\cut }\) given by the single Bishop disc \(\bfu _{\delta /2,b_o}\), see [40], Theorem 4.17 or [43], Section 1.4 . A collar neighbourhood of \(\partial \SS _{\cut }\) in \(\SS _{\cut }\) is equal to a collar neighbourhood of \(\partial \NN _{\cut }\) in \(\NN _{\cut }\) given by the local Bishop discs \(\bfu _{\varepsilon ,b_o}\), \(\varepsilon \in [\delta /2,\delta )\).

Furthermore observe that by compactness of \(\SS _{\cut }\) the intersection \(\SS _{\cut }\cap \ZZ _{\tau }\) is not empty only for finitely many nodal types \(\tau \). Therefore, we choose \(\big (\CR {\!\hat {J}},\lambda \big )\) to be transverse along the subpolyfolds \(\ZZ _{\tau }\) for these nodal types \(\tau \) turning the subsets \(\SS _{\cut }\cap \ZZ _{\tau }\) into suborbifolds of \(\SS \). As the codimensions will be at least \(2\) whenever the nodal type \(\tau \) is non-trivial, the resulting suborbifolds \(\SS _{\cut }\cap \ZZ _{\tau }\) have negative dimension, hence, are empty. Therefore, all elements in \(\SS _{\cut }\) are un-noded and have trivial isotropy as they can be represented by un-noded stable nodal disc maps with trivial automorphism group. In other words, \(\SS _{\cut }\) is a \(1\)-dimensional oriented compact branched manifold with precisely one boundary point, which has weight \(1\). This contradicts the fact that by [62], Lemma 5.11 the oriented sum of the weights taken over all boundary points vanishes.

Remark 7.4.4.
We give an alternative argument to obtain a contradiction which does not use the classification of \(1\)-dimensional oriented compact branched manifolds with boundary given in [62], Section 5.4 : We identify \(\gamma \) with the interval \([0,3\delta ]\) such that \((0,\delta )\) corresponds to the local Bishop family and \([2\delta ,3\delta ]\) is not contained in the image of the evaluation map \(\ev \co \SS \ra \gamma \) that evaluates \(\bfu \) at the first boundary marked point \(1\). Let \(f\) be a smooth function on \([0,3\delta ]\) with support in \((\delta /2,\delta )\) such that \(\int _0^{3\delta }f(x)\rmd x=1\). Because \(\ev \) restricts to a degree \(1\) map on the local Bishop discs,

\[ \int _{(\SS _{\cut },\lambda _{\DB })}\ev ^*(f\rmd x)=1 \]

writing \(\lambda _{\DB }\) for the weight function \(\lambda _{\CR {\!\hat {J}}}\). Denote by \(f_1\) the function obtained from \(f\) by shifting \(f\) by \(2\delta \) and observe that the closed \(1\)-form \((f-f_1)\rmd x\) has a primitive \(g(x)=\int _0^x\big (f(t)-f_1(t)\big )\rmd t\) with support in \((\delta /2,3\delta )\). Hence, \(\ev ^*\big ((f-f_1)\rmd x\big )\) has primitive \(\ev ^*g\) and

\[ \int _{(\SS _{\cut },\lambda _{\DB })}\ev ^*(f_1\rmd x)=0 \]

as the support of \(f_1\) is contained in \((5\delta /2,3\delta )\). With Stokes theorem [41], Theorem 1.27 for weighted integrals

\[ 1=\int _{(\SS _{\cut },\lambda _{\DB })}\ev ^*\big ((f-f_1)\rmd x\big )= \int _{(\partial \SS _{\cut },\lambda _{\DB })}\ev ^*g= g(\delta /2)\,. \]

As \(g(\delta /2)=0\) we reach the desired contradiction.

Acknowledgement.
   Part of the research of this article was initiated while S.S. and K.Z.'s stay at the Institut for Advanced Studies Princeton. We would like to thank Helmut Hofer for the invitation and for introducing us to polyfolds. K.Z. would like to thank the Mathematisches Forschungsinstitut Oberwolfach for the support. We would like to thank Katrin Wehrheim for her constant support and motivation. We thank Peter Albers, Matthew Strom Borman, Joel Fish, Hansjörg Geiges, Stefan Nemirovski, and Sven Prüfer for enlightening discussions.

Conflict of interest.
   Not Applicable

References

  • [1]  C. Abbas, An introduction to compactness results in symplectic field theory, Springer, Heidelberg, (2014), viii+252.

  • [2]  C. Abbas, K. Cieliebak, H. Hofer, The Weinstein conjecture for planar contact structures in dimension three, Comment. Math. Helv. 80 (2005), 771–793.

  • [3]  C. Abbas, H. Hofer, Holomorphic curves and global questions in contact geometry, Birkhäuser, (2019), xii+322.

  • [4]  R. A. Adams, J. J. F. Fournier, Sobolev spaces, Pure and Applied Mathematics (Amsterdam), 140, Second, Elsevier/Academic Press, Amsterdam, (2003), xiv+305.

  • [5]  B. Aebischer, M. Borer, M. Kälin, Ch. Leuenberger, H. M. Reimann, Symplectic geometry, Progress in Mathematics, 124, An introduction based on the seminar in Bern, 1992, Birkhäuser Verlag, Basel, (1994), xii+239.

  • [6]  P. Albers, H. Hofer, On the Weinstein conjecture in higher dimensions, Comment. Math. Helv. 84 (2009), 429–436.

  • [7]  M. Audin, Symplectic and almost complex manifolds, with an appendix by P. Gauduchon, Chapter II of [8], pp. 41–74.

  • [8]  M. Audin and J. Lafontaine (eds.), Holomorphic Curves in Symplectic Geometry, Progr. Math. 117, Birkhäuser Verlag, Basel (1994).

  • [9]  M. Audin, J. Lafontaine and L. Polterovich, Symplectic rigidity: Lagrangian submanifolds, Chapter X of [8], pp. 271–321.

  • [10]  K. Barth, J. Schneider, K. Zehmisch, Symplectic dynamics of contact isotropic torus complements, Münster J. Math. 12 (2019), 31–48.

  • [11]  M. S. Borman, Y. Eliashberg, E. Murphy, Existence and classification of overtwisted contact structures in all dimensions, Acta Math. 215 (2015), 281–361.

  • [12]  A. Borel, F. Hirzebruch, Characteristic Classes and Homogeneous Spaces, I, Amer. J. Math. 80 (1958), 458–538.

  • [13]  F. Bourgeois, A survey of contact homology, in: New perspectives and challenges in symplectic field theory, CRM Proc. Lecture Notes, 49, Amer. Math. Soc., Providence, RI, 2009, 45–71.

  • [14]  F. Bourgeois, O. van Koert, Contact homology of left-handed stabilizations and plumbing of open books, Commun. Contemp. Math. 12 (2010), 223–263.

  • [15]  F. Bourgeois, Y. Eliashberg, H. Hofer, K. Wysocki, E. Zehnder, Compactness results in symplectic field theory, Geom. Topol. 7 (2003), 799–888.

  • [16]  G. E. Bredon, Topology and Geometry, Grad. Texts in Math. 139, Springer-Verlag, New York (1993).

  • [17]  R. Casals, E. Murphy, F. Presas, Geometric criteria for overtwistedness, J. Amer. Math. Soc. 32 (2019), 563–604.

  • [18]  K. Cieliebak, Nonlinear Functional Analysis, lecture note, (2018).

  • [19]  K. Cieliebak, Y. Eliashberg, From Stein to Weinstein and back, American Mathematical Society Colloquium Publications, 59, Symplectic geometry of affine complex manifolds, American Mathematical Society, Providence, RI, 2012, xii+364.

  • [20]  F. Ding, H. Geiges, Contact structures on principal circle bundles, Bull. Lond. Math. Soc. 44 (2012), 1189–1202.

  • [21]  M. Dörner, H. Geiges, K. Zehmisch, Open books and the Weinstein conjecture, Q. J. Math. 65 (2014), 869–885.

  • [22]  Y. Eliashberg, Classification of overtwisted contact structures on \(3\)-manifolds, Invent. Math. 98 (1989), 623–637.

  • [23]  Y. Eliashberg, Filling by holomorphic discs and its applications, in: Geometry of Low-Dimensional Manifolds, Vol. 2 (Durham, 1989), London Math. Soc. Lecture Note Ser. 151, Cambridge University Press (1990), 45–67.

  • [24]  Y. Eliashberg, A. Givental, H. Hofer, Introduction to symplectic field theory, Geom. Funct. Anal. 2000, Special Volume, Part II, 560–673.

  • [25]  U. Frauenfelder, K. Zehmisch, Gromov compactness for holomorphic discs with totally real boundary conditions, J. Fixed Point Theory Appl. 17 (2015), 521–540.

  • [26]  K. Fukaya, Y.-G. Oh, H. Ohta, K. Ono, Lagrangian intersection Floer theory: anomaly and obstruction. Part II, AMS/IP Studies in Advanced Mathematics, 46, American Mathematical Society, Providence, RI; International Press, Somerville, MA, (2009), i–xii and 397–805.

  • [27]  H. Geiges, K. Zehmisch, Eliashberg's proof of Cerf's theorem, J. Topol. Anal. 2 (2010), 543–579.

  • [28]  H. Geiges, K. Zehmisch, Symplectic cobordisms and the strong Weinstein conjecture, Math. Proc. Cambridge Philos. Soc. 153 (2012), 261–279.

  • [29]  H. Geiges, K. Zehmisch, How to recognise a 4-ball when you see one, Münster J. Math. 6 (2013), 525–554.

  • [30]  H. Geiges, K. Zehmisch, Reeb dynamics detects odd balls, Ann. Sc. Norm. Super. Pisa Cl. Sci. (5) 15 (2016), 663–681.

  • [31]  H. Geiges, K. Zehmisch, A Course on Holomorphic Discs, Birkhäuser Advanced Texts Basler Lehrbücher, Birkhäuser/Springer, Cham, 2023, xviii+189 pp.

  • [32]  M. Gromov, Pseudoholomorphic curves in symplectic manifolds, Invent. Math. 82 (1985), 307–347.

  • [33]  M. Gromov, Partial differential relations, Ergebnisse der Mathematik und ihrer Grenzgebiete (3), 9, Springer-Verlag, Berlin, (1986), x+363.

  • [34]  A. Hatcher, Vector Bundles & K-Theory, (2017),
    http://pi.math.cornell.edu/ ̃hatcher/VBKT/VBpage.html

  • [35]  H. Hofer, Pseudoholomorphic curves in symplectizations with applications to the Weinstein conjecture in dimension three, Invent. Math. 114 (1993), 515–563.

  • [36]  H. Hofer, K. Wysocki, E. Zehnder, The dynamics on three-dimensional strictly convex energy surfaces, Ann. of Math. (2) 148 (1998), 197–289.

  • [37]  H. Hofer, K. Wysocki, E. Zehnder, Finite energy foliations of tight three-spheres and Hamiltonian dynamics, Ann. of Math. (2) 157 (2003), 125–255.

  • [38]  H. Hofer, K. Wysocki, E. Zehnder, A general Fredholm theory. I. A splicing-based differential geometry, J. Eur. Math. Soc. (JEMS) 9 (2007), 841–876.

  • [39]  H. Hofer, K. Wysocki, E. Zehnder, A general Fredholm theory. II. Implicit function theorems, Geom. Funct. Anal. 19 (2009), 206–293.

  • [40]  H. Hofer, K. Wysocki, E. Zehnder, A general Fredholm theory. III. Fredholm functors and polyfolds, Geom. Topol. 13 (2009), 2279–2387.

  • [41]  H. Hofer, K. Wysocki, E. Zehnder, Integration theory on the zero sets of polyfold Fredholm sections, Math. Ann. 346 (2010), 139–198.

  • [42]  H. Hofer, K. Wysocki, E. Zehnder, Deligne–Mumford-type spaces with a view towards symplectic field theory, preprint, (2012)

  • [43]  H. Hofer, K. Wysocki, E. Zehnder, Applications of polyfold theory I: The polyfolds of Gromov-Witten theory, Mem. Amer. Math. Soc. 248 (2017), v+218 pp.

  • [44]  Y. Huang, On Legendrian foliations in contact manifolds I: Singularities and neighborhood theorems, Math. Res. Lett. 22 (2015), 1373–1400.

  • [45]  Y. Huang, On plastikstufe, bordered Legendrian open book and overtwisted contact structures, J. Topol. 10 (2017), 720–743.

  • [46]  C. Hummel, Gromov's compactness theorem for pseudo-holomorphic curves, Progress in Mathematics, 151 Birkhäuser Verlag, Basel, (1997), viii+131.

  • [47]  D. Husemoller, Fibre bundles, Graduate Texts in Mathematics 20, Third, Springer-Verlag, New York, (1994), xx+353.

  • [48]  M. Kwon, K. Wiegand, K. Zehmisch, Diffeomorphism type via aperiodicity in Reeb dynamics, J. Fixed Point Theory Appl. 24 (2022), Paper No. 21, 26 pp.

  • [49]  J. Latschev, C. Wendl, Algebraic torsion in contact manifolds (With an appendix by Michael Hutchings.), Geom. Funct. Anal. 21 (2011), 1144–1195.

  • [50]  P. Massot, K. Niederkrüger, C. Wendl, Weak and strong fillability of higher dimensional contact manifolds, Invent. Math. 192 (2013), 287–373.

  • [51]  D. McDuff, Symplectic manifolds with contact type boundaries, Invent. Math. 103 (1991), 651–671.

  • [52]  D. McDuff, D. Salamon, Introduction to symplectic topology, Oxford Mathematical Monographs, Second, The Clarendon Press Oxford University Press, New York, (1998), 1–486.

  • [53]  D. McDuff, D. Salamon, Introduction to symplectic topology, Oxford Graduate Texts in Mathematics, Third, Oxford University Press, Oxford, (2017), xi+623.

  • [54]  D. McDuff, D. Salamon, \(J\)-holomorphic Curves and Symplectic Topology, Amer. Math. Soc. Colloq. Publ. 52, American Mathematical Society, Providence, RI (2004).

  • [55]  K. Niederkrüger, The plastikstufe – a generalization of the overtwisted disk to higher dimensions, Algebr. Geom. Topol. 6 (2006), 2473–2508.

  • [56]  K. Niederkrüger, On fillability of contact manifolds, Habilitation à diriger des recherches, Université Paul Sabatier - Toulouse III, 2013, tel-00922320.

  • [57]  K. Niederkrüger, A. Rechtman, The Weinstein conjecture in the presence of submanifolds having a Legendrian foliation, J. Topol. Anal. 3 (2011), 405–421.

  • [58]  K. Niederkrüger, C. Wendl, Weak symplectic fillings and holomorphic curves, Ann. Sci. Éc. Norm. Supér. (4) 44 (2011), 801–853.

  • [59]  J. Pardon, Contact homology and virtual fundamental cycles, J. Amer. Math. Soc. 32 (2019), 825–919.

  • [60]  L. Polterovich, The surgery of Lagrange submanifolds, Geom. Funct. Anal. 1 (1991), 198–210.

  • [61]  J. Robbin, D. Salamon, A construction of the Deligne-Mumford orbifold, J. Eur. Math. Soc. (JEMS) 8 (2006), 611–699.

  • [62]  D. Salamon, Lectures on Floer homology, in: Symplectic geometry and topology (Park City, UT, 1997), IAS/Park City Math. Ser. 7, Amer. Math. Soc., Providence, RI, (1999), 143–229.

  • [63]  D. Salamon, Funktionentheorie, Birkhäuser, Basel, (2011), viii + 218.

  • [64]  S. Suhr, K. Zehmisch, Polyfolds, cobordisms, and the strong Weinstein conjecture, Adv. Math. 305 (2017), 1250–1267.

  • [65]  A. Weinstein, On the hypotheses of Rabinowitz' periodic orbit theorems, J. Differential Equations 33 (1979), 336–352.

  • [66]  C. Wendl, Finite energy foliations and surgery on transverse links, Thesis (Ph.D.)–New York University, (2005), xii + 411.

  • [67]  C. Wendl, Lectures on Holomorphic Curves in Symplectic and Contact Geometry, preprint, arXiv: 1011.1690

  • [68]  K. Zehmisch, Holomorphic jets in symplectic manifolds, J. Fixed Point Theory Appl. 17 (2015), 379–402.

  • [69]  K. Zehmisch, The Eliashberg–Gromov tightness theorem, Diplomarbeit, Universität Leipzig (2003).