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Weinstein trisections of trivial surface bundles.

Masaki Ogawa Mathematical science center for co-creative society, Tohoku University, Aoba-6-3 Aramaki, Aoba Ward, Sendai, Miyagi 980-0845 [email protected]
Abstract.

Weinstein trisection is a trisection of a symplectic 4-manifold whose 1-handlebodies are the Weinstein domain for the symplectic structure induced from an ambient manifold. Lambert-Cole, Meier, and Starkston showed that every closed symplectic 4-manifold admits a Weinstein trisection. In this paper, we construct a Weinstein trisection of Σg×Σh\Sigma_{g}\times\Sigma_{h}. As a consequence of this construction, we construct a little explicit Weinstein trisection of S2×S2S^{2}\times S^{2}.

1. introduction

A trisection, introduced in [3] has been studied by many authors. One of the kind of the field in trisection theory is a Weinstein trisection. Lambert-Cole reproved the Thom conjecture by using trisection of P2\mathbb{C}P^{2} and inequality about an invariant induced by Khovanov homology. In the proof, he used a contact structure induced in the spine of trisection.

Recently, Lambert-Cole, Meier, and Starkston introduce a trisection adapted to a symplectic 4-manifold called a Weinstein trisection[7]. They also showed that every closed symplectic 4-manifold admits a Weinstein trisection. Weinstein trisection sometimes gives us a tool to study symplectic closed 4-manifolds and symplectic surfaces in them [5, 6].

There are some examples of Weinstein trisection. For example, Weinstein trisection of P2\mathbb{C}P^{2} and P2#P2¯\mathbb{C}P^{2}\#\overline{\mathbb{C}P^{2}} is described in [7]. On the other hand, given a finite group GG, there is a symplectic closed 4-manifold with fundamental group isomorphic GG. This means that there are so many symplectic closed 4-manifolds. Therefore, it is very important to make an example of Weinstein trisection as the first step to studying symplectic closed 4-manifolds with Weinstein trisection. The main result of this paper is the following:

Theorem 1.1.

Σg×Σh\Sigma_{g}\times\Sigma_{h} admits a genus (2g+1)(2h+1)+1(2g+1)(2h+1)+1 Weinstein trisection for some symplectic structure.

This implies that the trisection genus of Σg×Σh\Sigma_{g}\times\Sigma_{h} equals the Weinstein trisection genus of its.

Corollary 1.2.

The trisection genus of Σg×Σh\Sigma_{g}\times\Sigma_{h} equals the Weinstein trisection genus of its.

This corollary immediately follows from the result in [10]. It states that the trisection genus of Σg×Σh\Sigma_{g}\times\Sigma_{h} is (2g+1)(2h+1)+1(2g+1)(2h+1)+1.

This paper is organized as follows: In Section 2, we review definitions of trisection and Weinstein trisection. After that, we introduce a trisection of Σg×Σh\Sigma_{g}\times\Sigma_{h} which is constructed in [10] in Section 3. Then, we show this trisection can be seen as a Weinstein trisection in Section 4.

2. preliminalies

In this section, we set up the notion and objects we use in this paper. Trisection of 4-manifolds is a decomposition of a four-manifold.

Definition 2.1.

Let g,k1,k2g,k_{1},k_{2} and k3k_{3} be non-negative integers with max{k1,k2,k3}g\max\{k_{1},k_{2},k_{3}\}\leq g. A (g;k1,k2,k3)(g;k_{1},k_{2},k_{3})-trisection of a closed 4-manifold XX is a decomposition X=X1X2X3X=X_{1}\cup X_{2}\cup X_{3} such that for i,j{1,2,3}i,j\in\{1,2,3\},

  • Xiki(S1×B3)X_{i}\cong\natural^{k_{i}}(S^{1}\times B^{3}),

  • Hij=XiXjg(S1×B2)H_{ij}=X_{i}\cap X_{j}\cong\natural^{g}(S^{1}\times B^{2}) if iji\neq j, and

  • Σ=X1X2X3#g(S1×S1)\Sigma=X_{1}\cap X_{2}\cap X_{3}\cong\#^{g}(S^{1}\times S^{1}).

Symplectic 4-manifolds is a 4-manifold with non-degenerate closed 2-form ω\omega. We denote it by (X,ω)(X,\omega). In the field of symplectic topology, symplectic manifolds are considered the same if they a symplectomorphic.

Definition 2.2.

Let (X,ω)(X,\omega) be a symplectic manifold and φ\varphi a diffeomorphism between itself. We say φ\varphi is a symplectomorphism if it preserves the symplectic form ω\omega (i.e. φω=ω\varphi^{\ast}\omega=\omega).

Since ω\omega is a non-degenerate, we can obtain a volume form Ω=ωω\Omega=\omega\wedge\cdots\wedge\omega of XX after taking a wedge product n times. Hence in dimension two, the volume form of it is also a symplectic form so, volume-preserving diffeomorphism is the same as a symplectomorphism.

Lambert-Cole, Meier, and Starkston define a trisection of a symplectic closed 4-manifold adopted to the symplectic structure. The Weinstein domain, first introduced in [9], is a symplectic manifold with a contact boundary. More precisely, let (X,ω)(X,\omega) be a compact symplectic manifold with boundaries. Then, (X,ω)(X,\omega) is called a Weinstein domain if there exists a Morse function ff on XX and a gradient-like vector field XfX_{f} of ff such that XfX_{f} is Liouville vector field (i.e. d(ιXfω)=ωd(\iota_{X_{f}}\omega)=\omega).

Definition 2.3.

Let (X,ω)(X,\omega) be a symplectic closed 4-manifold and X=X1X2X3X=X_{1}\cup X_{2}\cup X_{3} a trisection of XX. We say X=X1X2X3X=X_{1}\cup X_{2}\cup X_{3} is a Weinstein trisection if there is a Morse function fi:Xf_{i}:X\rightarrow\mathbb{R} and gradient-like vector field XfX_{f} of ff such that (Xi,ω|Xi,fi,Xf)(X_{i},\omega|_{X_{i}},f_{i},X_{f}) is a Weinstein domain,

Lambert-Cole, Meier, and Starkston showed that any symplectic closed 4-manifold admits a Weinstein trisection by using a branched covering [7]. Weinstein domains induce a contact structure in their boundaries by a 1-form ιXfω\iota_{X_{f}}\omega. Also, HijH_{ij} has contact structures induced by a Weinstein structure of XiX_{i} and XjX_{j} [6].

And they give the following question.

Question 2.4.

Is a trisection genus equal to the Weinstein trisection genus?

In this paper, we answer this question for the Σg×Σh\Sigma_{g}\times\Sigma_{h}. The known trisections of symplectic four-dimensional manifolds are known as Weinstein trisections. To positively affirm that there are no trisections that are not Weinstein trisections, we still have too few examples.

3. trisection of trivial surface bundle

In this section we review the construction of a trisection of Σg×Σh\Sigma_{g}\times\Sigma_{h} in [10]. Let X=Σg×ΣhX=\Sigma_{g}\times\Sigma_{h}. First, we consider the decomposition of Σg\Sigma_{g}. We can decompose any closed surface into three disks.

Lemma 3.1 (Lemma 3.1 in [10]).

Σg\Sigma_{g} admits a decomposition Σg=B1B2B3\Sigma_{g}=B_{1}\cup B_{2}\cup B_{3} satisfies the following:

  1. (1)

    Each BiB_{i} are disks,

  2. (2)

    bij=BiBjb_{ij}=B_{i}\cap B_{j} is 2g+12g+1 disjoint arcs.

  3. (3)

    B1B2B3B_{1}\cap B_{2}\cap B_{3} is 4g+24g+2 disjoint vertices.

If g=1g=1, this decomposition is illustrated in Figure 1. To obtain the case of a higher genus, remove a neighborhood of a vertex and glue a copy of it to itself along their boundary.

Refer to caption
Figure 1. The decomposition of T2T^{2} in Lemma 3.1.

We take mutually disjoint disks NiN_{i} in Σh\Sigma_{h} for i=1,2,3i=1,2,3. Then we define the 1-handlebodies of a trisection as follows:

Xi=(Bi×(ΣhInt(Ni;Σh))(Bi+1×Ni+1).X_{i}=(B_{i}\times(\Sigma_{h}-Int(N_{i};\Sigma_{h}))\cup(B_{i+1}\times N_{i+1}).

To check XiX_{i} is a 1-handlebody, we show that (Bi×(ΣhInt(Ni;Σh))(B_{i}\times(\Sigma_{h}-Int(N_{i};\Sigma_{h})) is a 1-handlebody. Since (ΣhInt(Ni;Σh)(\Sigma_{h}-Int(N_{i};\Sigma_{h}) is a punctured genus hh surface, this can be represented by a disk and 2h2h 1-handles attached to it. Since BiB_{i} is a disk, (Bi×(ΣhInt(Ni;Σh))(B_{i}\times(\Sigma_{h}-Int(N_{i};\Sigma_{h})) is a 1-handlebody diffeomorphic to 2hS1×B3\natural^{2h}S^{1}\times B_{3}. The intersection (Bi×(ΣhInt(Ni;Σh))(B_{i}\times(\Sigma_{h}-Int(N_{i};\Sigma_{h})) and (Bi+1×Ni+1)(B_{i+1}\times N_{i+1}) is a (BiBi+1)×Ni(B_{i}\cap B_{i+1})\times N_{i}. This is a disjoint 2g+12g+1 3-balls in their boundaries. Since (Bi+1×Ni+1)(B_{i+1}\times N_{i+1}) is a 4-ball, XiX_{i} is a 1-handlebody of genus 2g+2h2g+2h.

In [10], Williams showed that X=X1X2X2X=X_{1}\cup X_{2}\cup X_{2} is a trisection.

Theorem 3.2 (Theorem 3.3 in [10]).

X=X1X2X2X=X_{1}\cup X_{2}\cup X_{2} is a genus (2g+1)(2h+1)+1(2g+1)(2h+1)+1 trisection.

The direction of this paper involves examining the above trisection in more detail to demonstrate how it will become a Weinstein trisection. To show this, we consider the Weinstein structure of Σgint(Bi)\Sigma_{g}-int(B_{i}) and Σhint(Ni)\Sigma_{h}-int(N_{i}). This is constructed in Section 5. It is easy to show that each of NiN_{i} is mutually ambient isotopic since they are disjoint disks. Also, we can show that each of BiB_{i} is mutually ambient isotopic. Actually, in Figure 1, BiB_{i} is sent to Bi+1B_{i+1} by ambient isotopy along the diagonal from bottom-left to top-right. We can extend this ambient isotopy to an arbitrary genus since we can construct a decomposition of Σg=B1B2B2\Sigma_{g}=B_{1}\cup B_{2}\cup B_{2} by connecting summing a torus by taking the regular neighborhood of a vertex depicted in Figure 1. We consider this feature with a symplectic structure in the next subsection.

3.1. symplectomorphisms compatible to the trisection.

In this subsection, we see the self-symplectomorphisms of symplectic surfaces. First of all, we provide a definition of symplectic and Hamiltonian isotopy. Let (X,ω)(X,\omega) be a closed symplectic manifold and H:XH:X\to\mathbb{R} a smooth function on XX. Then there is a unique vector field XHX_{H} such that

ιXHω=ω(XH,)=dH\iota_{X_{H}}\omega=\omega(X_{H},\cdot\ )=dH

since ω\omega is non-degenerate. We call XHX_{H} a Hamiltonian vector field associated to the Hamlltonian function HH.

Definition 3.3.

Let φt\varphi_{t} be an ambient isotopy on XX. We say φt\varphi_{t} is symplectic isotopy if φt\varphi_{t} is symplectomorphism for every t[0,1]t\in[0,1].

A symplectic isotopy is called a Hamiltonian isotopy if ιXtω\iota_{X_{t}}\omega is exact 1-form (i.e. XtX_{t} is Hamiltonian vector field for every tt) where XtX_{t} is a vecotor field such that

ddtφt=Xtφt.\frac{d}{dt}\varphi_{t}=X_{t}\circ\varphi_{t}.

By definition, a Hamiltonian isotopy is a symplectic isotopy.

In Section 5, we use the following lemmas to construct Weinstein structures of Σgint(Bi)\Sigma_{g}-int(B_{i}) and Σhint(Ni)\Sigma_{h}-int(N_{i}).

To show Lemma 3.5, we use the following lemma.

Lemma 3.4 (cf. [8], P.113).

Let (Σg,ω)(\Sigma_{g},\omega) be a symplectic closed surface and B(r)2B(r)^{2} a standard disk with radius rr for some rr\in\mathbb{R}.

[0,1]×B(r)2Σg(t,z)ψt(z)\begin{array}[]{rccc}[0,1]\ \times&B(r)^{2}&\longrightarrow&\Sigma_{g}\\ \rotatebox{90.0}{$\in$}&&&\rotatebox{90.0}{$\in$}\\ (t,z)&&\longmapsto&\psi_{t}(z)\end{array}

be a smooth map such that ψt:B(r)2Σg\psi_{t}:B(r)^{2}\rightarrow\Sigma_{g} is a symplectic embedding for every tt. Then there exists a Hamiltonian isotopy

[0,1]×ΣgΣg(t,p)ϕt(p)\begin{array}[]{rccc}[0,1]\times&\Sigma_{g}&\longrightarrow&\Sigma_{g}\\ \rotatebox{90.0}{$\in$}&&&\rotatebox{90.0}{$\in$}\\ (t,p)&&\longmapsto&\phi_{t}(p)\end{array}

such that

ϕ0=id,ϕtψ0=ψt\phi_{0}=id,\ \phi_{t}\circ\psi_{0}=\psi_{t}

for all tt.

Lemma 3.5.

Let Σg=B1B2B3\Sigma_{g}=B_{1}\cup B_{2}\cup B_{3} be a decomposition as in Lemma 3.1 and ω\omega a symplectic form of Σg\Sigma_{g}. Suppose that each area of BiB_{i} is identical for i=1,2,3i=1,2,3 with respect to ω\omega. Then there exists a symplectomorphism φi\varphi_{i} such that φi(Bi)=Bi+1\varphi_{i}(B_{i})=B_{i+1}.

Proof.

Let ψt:ΣgΣg\psi_{t}:\Sigma_{g}\rightarrow\Sigma_{g} be a ambient isotopy, such that

ψ1(Bi)=Bi+1.\psi_{1}(B_{i})=B_{i+1}.

Let pip_{i} be a point in the interior of BiB_{i}. Then, ψ(pi)\psi(p_{i}) is a point in the interior of ψ(Bi)\psi(B_{i}). Then we can construct a symplectic embedding φt(B(ri(t)))Σg\varphi^{\prime}_{t}(B(r_{i}(t)))\rightarrow\Sigma_{g} so that

φt(B(ri(t)))=ψt(Bi)\varphi^{\prime}_{t}(B(r_{i}(t)))=\psi_{t}(B_{i})

where ri(t)r_{i}(t)\in\mathbb{R} is a smooth function on [0,1][0,1] for i=1,2,3i=1,2,3. Then, we perturb φ\varphi^{\prime} so that ri(t)=rjr_{i}(t)=r_{j} for iji\neq j and any t[0,1]t\in[0,1], we obtain the follwoing family of symplectic embeddings φt\varphi^{\prime}_{t} such that

φt:B(r)Σg\varphi^{\prime}_{t}:B(r)\rightarrow\Sigma_{g}
φ0(B(r))=Bi,φ1(Bi)=Bi+1.\varphi^{\prime}_{0}(B(r))=B_{i},\varphi^{\prime}_{1}(B_{i})=B_{i+1}.

By Lemma 3.4, we obtain a Hamiltonian isotopy φt:ΣgΣg\varphi_{t}:\Sigma_{g}\rightarrow\Sigma_{g} such that

φ0=id,φtφ0=φt.\varphi_{0}=id,\ \varphi_{t}\circ\varphi^{\prime}_{0}=\varphi^{\prime}_{t}.

Then φ1\varphi_{1} is a symplectomorphism we want. ∎

From the result below, We can also assume that the NiN_{i} in Σh\Sigma_{h} are sent to each other by symplectomorphism.

Lemma 3.6 (Theorem A in [1]).

Let (Σh,ω)(\Sigma_{h},\omega) be a symplectic closed surface and {p1,,pn}\{p_{1},\ldots,p_{n}\} and {q1,,qn}\{q_{1},\ldots,q_{n}\} are two sets of distinct points of Σh\Sigma_{h}. Then there is a symplectomorphism φ\varphi such that φ(pi)=qi\varphi(p_{i})=q_{i} for i=1,,ni=1,\ldots,n that is isotopic to identity by an isotopy which preserves the structure and leaves fixed every point of Σh\Sigma_{h} outside a compact set of arbitrarily small volume.

4. Stein and Weinstein structure and Riemann surface.

4.1. Stein structure of a Riemann surface

We will review the concepts of Stein domains and that of Riemann surfaces. A Riemann surface is a 2-manifold with a complex structure JJ. A Stein manifold is a complex manifold that is embedded in N\mathbb{C}^{N}, where NN is a natural number. Grauert provided a characterization of Stein manifolds based on the function they admit (refer to [4]). This function is known as a strictly plurisubharmonic or JJ-convex function. In the context of a smooth function f:Mf:M\rightarrow\mathbb{R}, we say that it is exhausting if it is both proper and bounded from below.

Definition 4.1.

Let (M,J)(M,J) be a complex manifold and f:Mf:M\to\mathbb{R} a function. ff is called a plurisubharmonic or JJ-convex function if the 2-form

ωf:=d(dfJ)=ddf\omega_{f}:=-d(df\circ J)=-dd^{\mathbb{C}}f

satisfies

ωf(v,Jv)>0\omega_{f}(v,Jv)>0

for every non-zero tangent vector vTMv\in TM.

It is well-known that a Riemann surface is a Stein manifold if and only if it is a non-compact. Hence, Σgn\Sigma^{n}_{g} becomes a Stein domain where Σgn\Sigma^{n}_{g} is genus gg closed surface removed nn disks. Hence we obtain the following:

Lemma 4.2.

Let Σg\Sigma_{g} and Σh\Sigma_{h} be surfaces with genera gg and hh respectively, and BiB_{i} and NiN_{i} for i=1,2,3i=1,2,3 are disks in Σg\Sigma_{g} and Σh\Sigma_{h} respectively that are defined in Section 3. Then, Σhint(Ni)\Sigma_{h}-int(N_{i}) and ΣgBi+2\Sigma_{g}-B_{i+2} will be Stein domains for i=1,2,3i=1,2,3.

4.2. Weinstein structure of Riemann surface

Liouville vector field ξ\xi on symplectic manifold (X,ω)(X,\omega) is a vector field such that d(iXω)=ωd(i_{X}\omega)=\omega. If the Lie derivative of ω\omega along XX is ω\omega, then XX is a Liouville vector field. This follows from ω\omega is closed. Liouville domain is the symplectic manifold with some compatible vector fields with contact boundaries.

Definition 4.3.

Let (W,ω)(W,\omega) be a compact symplectic manifold with no empty boundary. (W,ω)(W,\omega) is called a Liouville domain if there is a Liouville vector field defined globally and it is transversally out of the boundary. We denote it by (W,ω,X)(W,\omega,X)

If the Liouville domain has a ”compatible” Morse function, it is called a Weinstein domain.

Definition 4.4.

Let (W,ω,X)(W,\omega,X) be a Liouville domain. (W,ω,X)(W,\omega,X) is called a Weinstein domain if there exists a Morse function ff it is locally constant in W\partial W and XX is gradient-like for ff.

For a given symplectic manifold, it is difficult to determine whether it admits a Weinstein structure or not. Also, generally, it is difficult to construct a Weinstein structure but we sometimes construct it from a Stein structure.

We say exhausting J-convex function ff is completely exhausting if its gradient vector fields ff\nabla_{f}f is complete where ff\nabla_{f}f is a gradient respect to a Riemann metric ωf(,J)\omega_{f}(\cdot,J\cdot) for ωf=ddf\omega_{f}=-dd^{\mathbb{C}}f. The following is a well-known theorem:

Theorem 4.5 ([2]).

Let (V,J)(V,J) be a Stein manifold and f:Vf:V\rightarrow\mathbb{R} a completely exhausting JJ-convex Morse function. Then,

(ωf:=ddf,Xf:=ff,f)(\omega_{f}:=-dd^{\mathbb{C}}f,X_{f}:=\nabla_{f}f,f)

is a Weinstein structure on VV.

Hence, we can construct a Weinstein structure of Σhint(Ni)\Sigma_{h}-int(N_{i}) from a Morse JJ-convex function fif_{i} for i=1,2,3i=1,2,3.

5. Proof of the main theorem

Let us consider a 1-handlebody

Xi=(Σhint(Ni))×BiNi+1×Bi+1X_{i}=(\Sigma_{h}-int(N_{i}))\times B_{i}\cup N_{i+1}\times B_{i+1}

that constructs a trisection prescribed in Section 3. We show that each of XiX_{i} admits a Weinstein structure with respect to a symplectic structure defined by a product structure of Σg×Σh\Sigma_{g}\times\Sigma_{h}.

Let g1:ΣgB3g_{1}:\Sigma_{g}-B_{3}\rightarrow\mathbb{R} be a JJ-convex function such that B1B_{1} contains only one critical point and its index is 0. Then we define the symplectic structure ωg\omega_{g} on Σg\Sigma_{g} so that

ωg|ΣgB3=ddg1.\omega_{g}|_{\Sigma_{g}-B_{3}}=-dd^{\mathbb{C}}g_{1}.

By Lemma 3.5, there is a symplectomorphism φ\varphi such that φ(Bi)=Bi+1\varphi(B_{i})=B_{i+1}. Then we define the JJ-convex function g2g_{2} and g3g_{3} as follows:

g2=g1φ1|ΣgB1:ΣgB1,g_{2}=g_{1}\circ\varphi^{-1}|_{\Sigma_{g}-B_{1}}:\Sigma_{g}-B_{1}\rightarrow\mathbb{R},
g3=g2φ1i|ΣgB2:ΣgB2.g_{3}=g_{2}\circ\varphi^{-1}i|_{\Sigma_{g}-B_{2}}:\Sigma_{g}-B_{2}\rightarrow\mathbb{R}.

Then we can define the Weinstein structures on ΣgBi+2\Sigma_{g}-B_{i+2} for i=1,2,3i=1,2,3 by Theorem 4.5.

Let N1N_{1} be a sufficiently small disk in Σh\Sigma_{h} and f1:ΣhN1f_{1}:\Sigma_{h}-N_{1}\rightarrow\mathbb{R} a JJ-convex function. Also, we suppose that N2N_{2} is a sufficiently small regular neighborhood of index 0 critical point of f1f_{1} and N3N_{3} a disk in the interior of Σh(N1N2)\Sigma_{h}-(N_{1}\cup N_{2}). Then we define the symplectic structure ωh\omega_{h} of Σh\Sigma_{h} so that

ωh|ΣhN1=ddf1.\omega_{h}|_{\Sigma_{h}-N_{1}}=-dd^{\mathbb{C}}f_{1}.

By Lemma 3.6, we can obtain the symplectomorphism φ2:(Σ,ωh)(Σh,ωh)\varphi_{2}:(\Sigma,\omega_{h})\rightarrow(\Sigma_{h},\omega_{h}) such that

φ(N1)=N2,φ(N2)=N3.\varphi(N_{1})=N_{2},\ \varphi(N_{2})=N_{3}.

Then, we obtain the JJ convex function f2:ΣN2f_{2}:\Sigma-N_{2}\rightarrow\mathbb{R} as follows:

f2=f1φ21|ΣhN2:ΣhN2.f_{2}=f_{1}\circ\varphi_{2}^{-1}|_{\Sigma_{h}-N_{2}}:\Sigma_{h}-N_{2}\rightarrow\mathbb{R}.

Also, we can obtain a symplectomorphism φ3:(Σ,ωh)(Σh,ωh)\varphi_{3}:(\Sigma,\omega_{h})\rightarrow(\Sigma_{h},\omega_{h}) such that

φ(N2)=N3,φ(N3)=N1.\varphi(N_{2})=N_{3},\ \varphi(N_{3})=N_{1}.

by Lemma 3.6. Then, we can define the JJ-convex function f3:ΣN3f_{3}:\Sigma-N_{3}\rightarrow\mathbb{R} as follows:

f3=f2φ31|ΣhN3:ΣhN3.f_{3}=f_{2}\circ\varphi_{3}^{-1}|_{\Sigma_{h}-N_{3}}:\Sigma_{h}-N_{3}\rightarrow\mathbb{R}.

Finally, we can construct a Weinstein structure on ΣhNi\Sigma_{h}-N_{i} for i=1,2,3i=1,2,3 by Theorem 4.5.

Proof of Theorem 1.1.

Let (Σh×Σg,ω)(\Sigma_{h}\times\Sigma_{g},\omega) be a trivial bundle over surface with symplectic structure ω=pr1ωh+pr2ωg\omega=pr_{1}^{\ast}\omega_{h}+pr_{2}^{\ast}\omega_{g} that is defined above. Now, the function fi+gif_{i}+g_{i} is a JJ-convex Morse function of (ΣhNi)×(ΣgBi+2)(\Sigma_{h}-N_{i})\times(\Sigma_{g}-B_{i+2}). So, we have to show that the gradient vector field of this Morse function is outward and it is a Liouville vector field on XiX_{i} with respect to a symplectic structure ω\omega. Let ξi\xi_{i} be the gradient vector field of fi+gif_{i}+g_{i}.

First, we show that ξi\xi_{i} is a Liouville vector field on XiX_{i} with respect to ω\omega. Now, fif_{i} and gig_{i} are JJ-convex Morse function, and ωh|ΣhNi\omega_{h}|\Sigma_{h}-N_{i} and ωg|ΣgBi+2\omega_{g}|\Sigma_{g}-B_{i+2} are symplectic structure defined by ddfi-dd^{\mathbb{C}}f_{i} and ddgi-dd^{\mathbb{C}}g_{i} respectively. Hence, by Theorem 4.5, ξi\xi_{i} gives a Liouville vector fields on (ΣhNi)×(ΣgBi+2)(\Sigma_{h}-N_{i})\times(\Sigma_{g}-B_{i+2}), particularly on XiX_{i} for ω\omega.

Next, we show that ξi\xi_{i} is transverse outwardly on the boudary of XiX_{i}. we recall that

Xi=(Σhint(Ni))×BiNi+1×Bi+1.X_{i}=(\Sigma_{h}-int(N_{i}))\times B_{i}\cup N_{i+1}\times B_{i+1}.

Since (Σhint(Ni))×int(Bi)(\Sigma_{h}-int(N_{i}))\times int(B_{i}) and Ni+1×Bi+1N_{i+1}\times B_{i+1} intersects their boundaries, Xi\partial X_{i} can be desicribed as following:

Xi=\displaystyle\partial X_{i}= (((Σhint(Ni))×Bi)((Σhint(Ni)×Bi)))\displaystyle((\partial(\Sigma_{h}-int(N_{i}))\times B_{i})\cup((\Sigma_{h}-int(N_{i})\times\partial B_{i})))
((Ni+1×Bi+1)(Ni+1Bi+1))\displaystyle\cup((\partial N_{i+1}\times B_{i+1})\cup(N_{i+1}\cup\partial B_{i+1}))
(((Σhint(Ni))×int(Bi))(Ni+1×Bi+1))\displaystyle-(((\Sigma_{h}-int(N_{i}))\times int(B_{i}))\cap(N_{i+1}\times B_{i+1}))

We note that ((Σhint(Ni))×int(Bi))(Ni+1×Bi+1)=Ni+1×(BiBi+1)((\Sigma_{h}-int(N_{i}))\times int(B_{i}))\cap(N_{i+1}\times B_{i+1})=N_{i+1}\times(B_{i}\cap B_{i+1}). Then, we will see whether ξi\xi_{i} is outward for each region. We note that BiB_{i} is a neighborhood of an index 0 critical point of gig_{i} by definition of gig_{i}. Then, the restriction of ξi\xi_{i} to BiB_{i} is transverse outwardly on its boundary. Since the restriction of ξi\xi_{i} to BiB_{i} and Σhint(Ni)\Sigma_{h}-int(N_{i}) is transverse outwardly on its boundary, ξi\xi_{i} transverse outwardly on ((Σhint(Ni))×Bi)(\partial(\Sigma_{h}-int(N_{i}))\times B_{i}) and ((Σhint(Ni)×Bi)((\Sigma_{h}-int(N_{i})\times\partial B_{i}).

We note that Ni+1N_{i+1} is a neighborhood of an index 0 critical point of fif_{i} by definition of fif_{i}. ξi\xi_{i} transverse outwardly on (Ni+1×Bi+1)\partial(N_{i+1}\times B_{i+1}) except Ni+1×(BiBi+1)N_{i+1}\times(B_{i}\cap\partial B_{i+1}) since the restriction of ξ\xi to Bi+1B_{i+1} transeverse outwardly on Bi+1\partial B_{i+1} except BiBi+1B_{i}\cap B_{i+1}. But we see that

((Σhint(Ni))×int(Bi))(Ni+1×Bi+1)=Ni+1×(BiBi+1).((\Sigma_{h}-int(N_{i}))\times int(B_{i}))\cap(N_{i+1}\times B_{i+1})=N_{i+1}\times(B_{i}\cap B_{i+1}).

Hence the region Ni+1×(BiBi+1)N_{i+1}\times(B_{i}\cap\partial B_{i+1}) is not included a boundary of XiX_{i}. Hence ξi\xi_{i} transverse outwardly on Xi\partial X_{i} entirely.

6. The case where g=h=0g=h=0.

In this section, we give an example of the Weinstein trisection of S2×S2S^{2}\times S^{2}. It is a trivial S2S^{2} bundle over S2S^{2}. We denote it S1×S2S_{1}\times S_{2}. Also, S2S_{2} has a decomposition described above. More precisely, we assume that S2S_{2} is decomposed into three disks B1B_{1}, B2B_{2}, and B3B_{3} as in Figure 1. We note that the Weinstein trisection of S2×S2S^{2}\times S^{2} is constructed in former articles [7]. But in this section, we will describe it slightly more explicitly.

We construct a Weinstein trisection of S2×S2S^{2}\times S^{2} as the following steps:

  1. Step 1:

    For a given symplectic structure on S1NiS_{1}-N_{i}, we define a Morse function fif_{i} so that Ni+1N_{i+1} is a neighborhood of index 0 critical point of fif_{i}, it does not contain the other critical point and whose gradient flow is a Liouville vector field of the symplectic structure. Furthermore, each of NiN_{i} is mutually symplectically isotopic to each other.

  2. Step 2:

    For a given symplectic structure on S2BiS_{2}-B_{i}, we define a Morse function gig_{i} so that BiB_{i} is a neighborhood of index 0 critical point of gg and does not contain the other critical points of gg, Bi+1B_{i+1} is a neighborhood of index 22 critical point of gg and does not contain the other critical points of gg and whose gradient vector field is a Liouville vector field for the symplectic structure. Furthermore, each of BiB_{i} is mutually symplectically isotopic to each other.

  3. Step 3:

    f+gf+g is a Morse function on XiX_{i} and a gradient vector field of it is a Liouville vector field for the products of the symplectic structure of S1S_{1} and S2S_{2} and (Xi,ω,g+f,grad(g+f))(X_{i},\omega,g+f,grad(g+f)) will be a Weinstein domain.

To begin the steps above, we review the Kähler structure on S2S^{2}. First of all, we review the Fubini-study form of P1\mathbb{C}P^{1}.

Let (z1,z2)(z_{1},z_{2}) be a homogenious coordinate of P1\mathbb{C}P^{1}. Then we can take a chart of P1\mathbb{C}P^{1} by taking ϕi:P1\phi_{i}:\mathbb{C}P^{1}\to\mathbb{C} for zj0z_{j}\neq 0

ϕi(z1,z2)=zizj(ij).\phi_{i}(z_{1},z_{2})=\frac{z_{i}}{z_{j}}\ (i\neq j).

We denote this chart by {Ui,ϕi}i=1,2\{U_{i},\phi_{i}\}_{i=1,2}. Then we define the Fubini-Study form by

ωFS=22log(1+|z|2)zz¯dzdz¯\omega_{FS}=2\frac{\partial^{2}\log(1+|z|^{2})}{\partial z\partial\bar{z}}dz\wedge d\bar{z}

where z=z1/z2z=z_{1}/z_{2}. It is known that this form gives us the Kähler form on U1U_{1}, and in this case, f=log(1+|z|2)f=\log(1+|z|^{2}) gives a Kähler potential. The critical point of ff is only z=0z=0. This means that z1=0z_{1}=0 since z20z_{2}\neq 0. Also, we note that this is a JJ-holomorphic function on U1U_{1}. Hence, U1U_{1} is a Stein manifold with JJ-holomorphic function ff.

Next, we review the identification between S2S^{2} and P1\mathbb{C}P^{1}. We denote the polar coordinate of the unit sphere by the following (See Figure 2):

x=\displaystyle x= sinθ1cosθ2,\displaystyle\sin\theta_{1}\cos\theta_{2},
y=\displaystyle y= sinθ1sinθ2,\displaystyle sin\theta_{1}\sin\theta_{2},
z=\displaystyle z= cosθ1.\displaystyle\cos\theta_{1}.
Refer to caption
Figure 2. This Figure represents a polar coordinate of S2S^{2}. In this figure, ϕN\phi_{N} is a stereographic projection.

Then we can represent a point on S2S^{2} by (x,y,z)S23(x,y,z)\in S^{2}\subset\mathbb{R}^{3}. We denote the stereographic projection ϕN:S2\pN2\phi_{N}:S^{2}\backslash p_{N}\to\mathbb{R}^{2} where pN=(0,0,1)p_{N}=(0,0,1). Then we can define the diffeomorphism Φ:P1S2\Phi:\mathbb{C}P^{1}\to S^{2} by

Φ(z1,z2)={ϕN(z)(z20)pN(z2=0)\Phi(z_{1},z_{2})=\begin{cases}{}\phi_{N}(z)&(z_{2}\neq 0)\\ p_{N}&(z_{2}=0)\end{cases}

where z=z1/z2z=z_{1}/z_{2}. We sometimes use this diffeomorphism to define the function on S2S^{2} below.

We identify fΦ1f\circ\Phi^{-1} and Φ1ωFS{\Phi^{-1}}^{\ast}\omega_{FS} by ff and ωFS\omega_{FS} respectively.

6.1. Step 1: Weinstein structure on S1NiS_{1}-N_{i}

We define the region N1N_{1}, N2N_{2} and N3N_{3} on S1S_{1}. Let φ\varphi be a 4/3π4/3\pi-rotation along a yy-axis. Then we denote PN=p1P_{N}=p_{1}, φ(PN)=p2\varphi(P_{N})=p_{2} and φ2(PN)=p3\varphi^{2}(P_{N})=p_{3}. Also, we denote PS=q1P_{S}=q_{1}, φ(PS)=q2\varphi(P_{S})=q_{2} and φ2(PS)=q3\varphi^{2}(P_{S})=q_{3}. Then we define N1N_{1} as a neighborhood of p1p_{1} so that it contains q3q_{3} and does not contain pip_{i} and qjq_{j} for i=2,3,j=1,2i=2,3,j=1,2. N2N_{2} and N3N_{3} are defined by φ(N1)\varphi(N_{1}) and φ2(N3)\varphi^{2}(N_{3}) respectively (See Figure 3).

Refer to caption
Figure 3. Each of NiN_{i} is a region as in this figure. They are mutually permuted by rotation φ\varphi

We take rotation φ\varphi along a yaxisy-axis such that φ(N1)N1\varphi(N_{1})\cap N_{1} is an empty set. Also, the we define φ(N1)=N2\varphi(N_{1})=N_{2} and φ(N2)=N3\varphi(N_{2})=N_{3}. Since a rotation is volume-preserving, this is a sympelctomorphism that sends NiN_{i} to each other. Then ff define the JJ-convex function on S2N1S^{2}-N_{1} respect to ωFS\omega_{FS}. By using Theorem 4.5, we can obtain the Weinstein structure on S1N1S_{1}-N_{1}. By permuting NiN_{i} by rotation, we can also obtain the Weinstein structure on S1NiS_{1}-N_{i} for i=2,3i=2,3.

6.2. Step 2: Weinstein structure on S2Bi+2S_{2}-B_{i+2}

We define the region BiB_{i} in S2S_{2} for i=1,2,3i=1,2,3 as in Lemma 1. In this case, the intersection BiBjB_{i}\cap B_{j} for iji\neq j is an arc. We define the region BiB_{i} as follows:

B1={(sinθ1cosθ2,sinθ1sinθ2,cosθ1)S2412πθ21212π},B_{1}=\left\{(\sin\theta_{1}\cos\theta_{2},\sin\theta_{1}\sin\theta_{2},\cos\theta_{1})\in S^{2}\mid\frac{4}{12}\pi\leq\theta_{2}\leq\frac{12}{12}\pi\right\},
B2={(sinθ1cosθ2,sinθ1sinθ2,cosθ1)S21212πθ22012π},B_{2}=\left\{(\sin\theta_{1}\cos\theta_{2},\sin\theta_{1}\sin\theta_{2},\cos\theta_{1})\in S^{2}\mid\frac{12}{12}\pi\leq\theta_{2}\leq\frac{20}{12}\pi\right\},
B2={(sinθ1cosθ2,sinθ1sinθ2,cosθ1)S22012πθ22412π}.B_{2}=\left\{(\sin\theta_{1}\cos\theta_{2},\sin\theta_{1}\sin\theta_{2},\cos\theta_{1})\in S^{2}\mid\frac{20}{12}\pi\leq\theta_{2}\leq\frac{24}{12}\pi\right\}.

We can see each region as in Figure 4.

Refer to caption
Figure 4. The Left Figure describes the regions BiB_{i} and the right figure is a picture view from a direction perpendicular to the xzxz plane.

It is easy to see that each of BiB_{i} is mutually permuted by rotating along a yy-axis. Also, we can define the JJ-holomorphic function g1g_{1} respect to ωFS\omega_{FS} on S2int(B3)S_{2}-int(B_{3}) from the function ff defined above. Also, composing a g1g_{1} and rotating, we can also obtain the JJ-convex function on S2int(Bi)S_{2}-int(B_{i}) for i=1,2i=1,2. We will check that the critical point of g1g_{1} is included in B2B_{2}.

g1g_{1} is a restriction of ff to S2int(B3)S^{2}-int(B_{3}) it was defined before the steps. Its critical point is z1=0z_{1}=0. This is corresponds to a point pS=(0,0,1)p_{S}=(0,0,-1) by the identification map Φ\Phi. Also, this critical point has an index 0 since by Poincare-Hopf theorem, ff is a Morse function on disk and it has only one critical point. Hence we can assume B2B_{2} is a neighborhood of index 0 critical point of g1g_{1}.

6.3. Step 3: (Xi,ωXi,(g+f)Xi,grad(g+f))(X_{i},\omega\mid_{X_{i}},(g+f)\mid_{X_{i}},grad(g+f)) is a Weinstein domain.

We remain the following: First, we have to check the gradient flow of gi+fig_{i}+f_{i} is the Liouville vector field. Next, we have to check it is outward. By Theorem 4.5, we can see that the gradient-like flow of fif_{i} and gig_{i} are Liouville vector fields with respect to ωFS\omega_{FS}. Hence we can show that the gradient-like flow of fi+gif_{i}+g_{i} is a Liouville vector field with respect to ωFS+ωFS=2ωFS\omega_{FS}+\omega_{FS}=2\omega_{FS}.

Finally, we will check it is outward. Following the construction of trisection above, XiX_{i} is a set as follows:

Xi=((S1Ni)×Bi)(Ni+1×Bi+1)X_{i}=((S_{1}-N_{i})\times B_{i})\cup(N_{i+1}\times B_{i+1})

We show the case where i=1i=1. We note that each of (S1N1)×B1(S_{1}-N_{1})\times B_{1} and N2×B2N_{2}\times B_{2} are diffeomorphic to a 4-ball since S1N1S_{1}-N_{1} is a disk. We defined the vector field on S1N1S_{1}-N_{1} and B1B2B_{1}\cup B_{2} by the gradient-like vector field of f1f_{1} and g1g_{1} respectively. They are outward on each of S1N1S_{1}-N_{1} and B1B2B_{1}\cup B_{2} respectively. We denote an arc B1B2B_{1}\cap B_{2} α\alpha. Then the intersection of two 4-ball (S1N1)×B1(S_{1}-N_{1})\times B_{1} and N2×B2N_{2}\times B_{2} is a 3-ball N2×αN_{2}\times\alpha. We shall consider the boundary of XiX_{i}. Xi\partial X_{i} is a union of {(S1N1)×B1}(N2×α)\{(S_{1}-N_{1})\times B_{1}\}-(N_{2}\times\alpha) and N2×B2N2×αN_{2}\times B_{2}-N_{2}\times\alpha. Now, the gradient-like vector field of f1+g1f_{1}+g_{1} on (S1N1)×B1(S_{1}-N_{1})\times B_{1} outward since (S1N1)(S_{1}-N_{1}) and B1B_{1} are neiborhood of index 0 critical point of f1f_{1} and g1g_{1} respectively. Also, the gradient-like vector field of f1+g1f_{1}+g_{1} on N2×B2N_{2}\times B_{2} is outward except N2×αN_{2}\times\alpha since we can assume that N2N_{2} is a neighborhood of index 0 critical point of f1f_{1} and the gradient-like vector field of g1g_{1} is outward on B1B2B_{1}\cup B_{2}. This is enough to show that f1+g1f_{1}+g_{1} is outward on X1X_{1}.

7. Acknowledgement

The author thanks Takahiro Oba for a very meaningful discussion and suggestion about research in symplectic topology, also giving comments on a draft of this paper.

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