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Hyperbolic volume and Heegaard distance

Tsuyoshi Kobayashi  and  Yo’av Rieck
(Date: August 11, 2025; Date: August 11, 2025)
Abstract.

We prove (Theorem 1.5) that there exists a constant Λ>0\Lambda>0 so that if MM is a (μ,d)(\mu,d)-generic complete hyperbolic 3-manifold of volume Vol(M)<\mbox{\rm Vol}(M)<\infty and ΣM\Sigma\subset M is a Heegaard surface of genus g(Σ)>ΛVol(M)g(\Sigma)>\Lambda\mbox{\rm Vol}(M), then d(Σ)2d(\Sigma)\leq 2, where d(Σ)d(\Sigma) denotes the distance of Σ\Sigma as defined by Hempel. The term (μ,d)(\mu,d)-generic is described precisely in Definition 1.3; see also Remark 1.4.

The key for the proof of Theorem 1.5 is Theorem 1.8 which is on independent interest. There we prove that if MM is a compact 3-manifold that can be triangulated using at most tt tetrahedra (possibly with missing or truncated vertices), and Σ\Sigma is a Heegaard surface for MM with g(Σ)76t+26g(\Sigma)\geq 76{t}+26, then d(Σ)2d(\Sigma)\leq 2.

Key words and phrases:
3-manifold, Heegaard splittings, Heegaard distance
1991 Mathematics Subject Classification:
57M99, 57M25
The first names author was supported by Grant-in-Aid for scientific research, JSPS grant number 19540083. The second named author was supported in part by the 21st century COE program “Constitution for wide-angle mathematical basis focused on knots” (Osaka City University); leader: Akio Kawauchi.

1. Introduction

All the manifolds considered in this paper are 3-dimensional, compact, connected, and orientable. By hyperbolic manifold we mean a manifold whose interior admits a complete finite volume Riemannian metric locally isometric to hyperbolic 3-space 3\mathbb{H}^{3}.

It is generally agreed that the volume of a hyperbolic manifold MM, Vol(M)\mbox{\rm Vol}(M), is a good measure of the complexity of MM. As evidence of that, arguments of M. Gromov, T. Jørgensen and W. Thurston show that the hyperbolic volume is linearly equivalent to the number of tetrahedra needed to triangulate a link exterior in MM. The argument is based on Thurston’s notes [thurston], for a detailed presentation see [gjt]; throughout this paper we follow the notation and definitions given in that paper. For a precise statement, let tc(M)t_{c}(M) be the smallest number of tetrahedra needed to triangulate MN(L)M\setminus N(L), where the minimum is taken over all links LML\subset M (possibly, L=L=\emptyset) and all possible triangulations.

Theorem 1.1 (Gromov, Jørgensen, Thurston).

There exist constants A,B>0A,\ B>0 so that for any hyperbolic manifold MM the following holds:

Atc(M)<Vol(M)<Btc(M).At_{c}(M)<\mbox{\rm Vol}(M)<Bt_{c}(M).
Remark 1.2.

In the proof of Theorem 1.1 given in [gjt] it is shown that given μ>0\mu>0, a Margulis constant for 3\mathbb{H}^{3}, and d>0d>0, there exists A>0A>0, so that Nd(Mμ)N_{d}(M_{\geq\mu}) can be triangulated using at most 1AVol(M)\frac{1}{A}\mbox{\rm Vol}(M) tetrahedra; here Nd(Mμ)N_{d}(M_{\geq\mu}) denotes the closed dd-neighborhood of the μ\mu-thick part of MM. We note that AA depends on μ\mu and dd.

Theorem 1.1 implies that manifolds of low volume admit Heegaard splittings of low genus: let MM be a hyperbolic manifold, LML\subset M a link, and 𝒯\mathcal{T} a triangulation of MN(L)M\setminus N(L) that realizes tc(M)t_{c}(M). Let Γ\Gamma be 𝒯(1)(MN(L))\mathcal{T}^{(1)}\cup\partial(M\setminus N(L)), where 𝒯(1)\mathcal{T}^{(1)} denotes the 1-skeleton of 𝒯\mathcal{T}. It is easy to see that N(Γ)\partial N(\Gamma) is a Heegaard surface for MN(L)M\setminus N(L) and its genus is at most the number of tetrahedra plus one, that is, tc(M)+1t_{c}(M)+1. Since the Heegaard genus does not increase after Dehn filling we get:

g(M)tc(M)+12tc(M)<2AVol(M).g(M)\leq t_{c}(M)+1\leq 2t_{c}(M)<\frac{2}{A}\mbox{\rm Vol}(M).

Here and throughout this paper, g(M)g(M) denotes the Heegaard genus of MM. The converse is false: it is easy to construct hyperbolic manifolds of arbitrarily high volume and Heegaard genus two (for example, consider Dehn fillings of 2-bridge knots; see [schultens2bridge]).

Our goal is to show that any Heegaard surface for a generic hyperbolic manifold MM is “simple”. This is described precisely in Theorem 1.5, and we informally explain it here. In [hempel] J. Hempel defined a complexity of Heegaard surfaces which we will call the distance, denoted by d(Σ)d(\Sigma) (the distance, which is based on Kobayashi’s idea of height of loops [KobayashiHeights], is defined in Section 4). We say that a Heegaard surface Σ\Sigma is simple if either g(Σ)g(\Sigma) is low (in terms of the volume) or d(Σ)2d(\Sigma)\leq 2. A. Casson and C. Gordon constructed a hyperbolic manifold admitting infinitely many Heegaard surfaces, and showed that these surfaces all have distance at least two (in their language, are strongly irreducible). They further showed that there is no upper bound on the genera of these surfaces; hence this result is best possible.

We now explain what a generic hyperbolic manifold is. Let XX be a compact 3-manifold (not necessarily hyperbolic) so that X\partial X consists of tori, say T1,,TnT_{1},\dots,T_{n}. Let WW be a manifold obtained from XX by Dehn filling some of its boundary components, say T1,,TmT_{1},\dots,T_{m}, mnm\leq n. Note that XWX\subset W and any Heegaard surface for XX is a Heegaard surface for WW. Rieck and E. Sedgwick [rieck][rs1][rs2] prove that on each TiT_{i} there is a finite set of slopes, denoted by BiB_{i}, so that if the slope filled on each TiT_{i} intersects every slope of BiB_{i} more than once, then any Heegaard surface for WW is a Heegaard surface for XX (after isotopy if necessary). In that case, we say that WW is a generic Dehn filling of XX. With this in mind, we define:

Definition 1.3.

Let μ\mu be a Margulis constant for 3\mathbb{H}^{3} and fix d>0d>0. Let MM be a complete hyperbolic manifold of finite volume. Let Nd(Mμ)N_{d}(M_{\geq\mu}) be the closed dd-neighborhood of the μ\mu-thick part of MM; for a discussion see [gjt], where it was observed that MM is obtained from Nd(Mμ)N_{d}(M_{\geq\mu}) by Dehn filling. We say that MM is (μ,d)(\mu,d)-generic if MM is a generic Dehn filling of Nd(Mμ)N_{d}(M_{\geq\mu}).

Remark 1.4.

In an effort to justify the term “generic” we now sketch an argument that shows that for any μ\mu and dd, there are indeed many (μ,d)(\mu,d)-generic manifold. Fix V>0V>0. By Remark 1.2 there are only finitely many topological types for the manifolds Nd(Mμ)N_{d}(M_{\geq\mu}), where MM ranges over all hyperbolic manifolds of volume less than VV. Let XX be one of these manifolds and denote the components of X\partial X by T1,,TnT_{1},\dots,T_{n}. Then for each ii there is a finite set of slopes of TiT_{i}, say FiF_{i}, with the following property: as above let WW be a manifold obtained from XX by Dehn filling some of its boundary components, say T1,,TmT_{1},\dots,T_{m}, mnm\leq n, so that slope filled is not in FiF_{i} for all ii. Then WW is hyperbolic, the short geodesics in WW coincide with the cores of the attached solid tori, and each short geodesic has a neighborhood of radius greater than dd. Thus Nd(Wμ)=XN_{d}(W_{\geq\mu})=X. We conclude that if WW is obtained by filling XX along slopes that are not in FiF_{i} and intersect every slope in BiB_{i} more than once (where BiB_{i} was defined in the paragraph preceding Definition 1.3), then WW is (μ,d)(\mu,d)-generic. This shows that if VV is at least the volume of the figure eight knot exterior (so that there are infinitely many hyperbolic manifolds of volume less than VV), then there are infinitely many (μ,d)(\mu,d)-generic manifolds that have volume less than VV.

In this paper we prove that (μ,d)(\mu,d)-generic manifolds enjoy the following property:

Theorem 1.5.

Let μ>0\mu>0 be a Margulis constant for 3\mathbb{H}^{3} and fix d>0d>0. Then there exists Λ>0\Lambda>0 so that for any complete finite volume (μ,d)(\mu,d)-generic hyperbolic manifold MM and any Heegaard surface Σ\Sigma for MM the following holds:

If g(Σ)>ΛVol(M)g(\Sigma)>\Lambda\mbox{\rm Vol}(M), then d(Σ)2d(\Sigma)\leq 2.

Remark 1.6.

Fix a hyperbolic manifold MM. It is easy to see that if dd is sufficiently large or μ\mu sufficiently small, then MM is diffeomorphic to Nd(Mμ)N_{d}(M_{\geq\mu}), and in particular MM is (μ,d)(\mu,d)-generic. Thus, the conclusion of Theorem 1.5 holds for MM. This has two consequences:

  1. (1)

    It is well known that the examples of Casson and Gordon mentioned above have distance two and arbitrarily high genus. Hence Conclusion (2) of Theorem 1.5 cannot be improved.

  2. (2)

    If there exists Λ\Lambda as in Theorem 1.5 that is independant of μ\mu and dd, then the assumption that MM is (μ,d)(\mu,d)-generic can be removed. Unfortunately, for Λ\Lambda constructed in this paper both limdΛ=\lim_{d\to\infty}\Lambda=\infty and limμ0Λ=\lim_{\mu\to 0}\Lambda=\infty hold.

Our proof of Theorem 1.5 uses Dehn filling and hence forces us to assume that MM is (μ,d)(\mu,d)-generic. However, this does not seem to be an integral part of the theory. In light of this and Remark 1.6 (2) we ask:

Question 1.7.

Is the assumption that MM is (μ,d)(\mu,d)-generic necessary?


The three ingredients necessary for the proof of Theorem 1.5 are Theorem 1.1, the work of Rieck and Sedgwick, and Theorem 1.8, which represents the bulk of the work in this paper. In this theorem we allow a flexible definition of triangulation, which we call generalized triangulation. See Definition 4.1 and Lemma 4.2 for existence.

Theorem 1.8.

Let MM be a compact orientable connected 3-manifold and Σ\Sigma a Heegaard surface for MM. Suppose that for some (possibly empty or disconnected) compact surface KMK\subset\partial M, MKM\setminus K admits a generalized triangulation with t{t} generalized tetrahedra.

If g(Σ)76t+26g(\Sigma)\geq 76{t}+26, then d(Σ)2d(\Sigma)\leq 2.

Remark 1.9.
  1. (1)

    Theorem 1.8 generalizes S. Schleimer’s [schleimer, Theorem 11.1], where it was shown that if MM is a closed manifold and g(Σ)2216t2g(\Sigma)\geq 2^{2^{16}{t}^{2}}, then d(Σ)2d(\Sigma)\leq 2.

  2. (2)

    Theorem 1.8 implies that for every manifold MM, there is gM0g_{M}\geq 0, so that if ΣM\Sigma\subset M is a Heegaard surface of genus at least gMg_{M}, then d(Σ)2d(\Sigma)\leq 2; this also follows from [schleimer, Theorem 11.1].

Outline. In Section 2, we show how Theorem 1.5 follows from Theorem 1.8. In Section 3 we explain our perspective of Theorem 1.8 and list open questions related to it. In Section 4 we explain a few preliminaries. The work begins in Section 5, where we take a strongly irreducible Heegaard surface of genus at least 76t+2676{t}+26, color it, and analyze the coloring; the climax of Section 5 is Proposition 5.6, where we prove existence of a pair of pants with certain useful properties. Finally, in Section 6 we prove Theorem 1.8.

Acknowledgment. We thank Cameron Gordon, Marc Lackenby, Kimihiko Motegi, and Saul Schleimer for interesting conversations and correspondence. We thank the anonymous referees for a careful reading of the paper and insightful comments that added to the content and improved the presentation of this work. The second named author: this work was carried out while I was visiting OCAMI at Osaka City University and Nara Women’s University. I thank Professor Akio Kawauchi and OCAMI, and Professor Tsuyoshi Kobayashi and the math department of Nara Women’s University for the hospitality I enjoyed during those visits.

2. Proof of Thoerem 1.5

We first show how Theorem 1.5 follows from Theorem 1.8. Fix the notation of Theorem 1.5. Let λ=1A\lambda=\frac{1}{A}, where A>0A>0 is the constant given in Theorem 1.1. By Remark 1.2, for any complete finite volume hyperbolic 3-manifold MM, Nd(Mμ)N_{d}(M_{\geq\mu}) can be triangulated using at most λVol(M)\lambda\mbox{\rm Vol}(M) tetrahedra.

Set Λ=76λ+29\Lambda=76\lambda+29. Let ΣM\Sigma\subset M be a Heegaard surface of genus g(Σ)ΛVol(M)g(\Sigma)\geq\Lambda\mbox{\rm Vol}(M). Using the definition of Λ\Lambda and the fact that Vol(M)>.9\mbox{\rm Vol}(M)>.9 (Gabai, Meyerhoff, and Milley [gmm]) we get:

g(Σ)\displaystyle g(\Sigma) \displaystyle\geq ΛVol(M)\displaystyle\Lambda\mbox{\rm Vol}(M)
=\displaystyle= (76λ+29)Vol(M)\displaystyle(76\lambda+29)\mbox{\rm Vol}(M)
=\displaystyle= 76λVol(M)+29Vol(M)\displaystyle 76\lambda\mbox{\rm Vol}(M)+29\mbox{\rm Vol}(M)
>\displaystyle> 76λVol(M)+26.\displaystyle 76\lambda\mbox{\rm Vol}(M)+26.

By assumption, MM is a (μ,d)(\mu,d)-generic, that is, MM is obtained from Nd(Mμ)N_{d}(M_{\geq\mu}) by a generic Dehn filling (recall Definition 1.3). Hence, after isotopy if necessary, Σ\Sigma is a Heegaard surface for Nd(Mμ)N_{d}(M_{\geq\mu}). By Remark 1.2, Nd(Mμ)N_{d}(M_{\geq\mu}) can be triangulated using tλVol(M)t\leq\lambda\mbox{\rm Vol}(M) tetrahedra. We see that g(Σ)>76λVol(M)+2676t+26g(\Sigma)>76\lambda\mbox{\rm Vol}(M)+26\geq 76t+26, and by Theorem 1.8 (applied to Σ\Sigma as a Heegaard surface of Nd(Mμ)N_{d}(M_{\geq\mu})), d(Σ)2d(\Sigma)\leq 2. It is elementary to see that distance never increases under Dehn filling, and we conclude that ΣM\Sigma\subset M is a Heegaard surface of distance at most 2, completing the proof of Theorem 1.5.

3. Open Questions

Theorem 1.8 is a constraint on the distance of surfaces of genus 76t+2676{t}+26 or more. There are other constraints on the distance known, and by far the most important is Casson and Gordon’s theorem [cg] that says that no Heegaard surface of an irreducible, non-Haken 3-manifold has distance exactly one. Other examples include W. Haken’s theorem that says that any Heegaard surface of a reducible 3-manifold has distance zero, and T. Li’s theorem [li2] that says that a non-Haken 3-manifold admits only finitely many Heegaard surfaces of positive distance. Another constraint is [schtom, Corollary 3.5], where M. Scharlemann and M. Tomova prove that if Σ1\Sigma_{1} and Σ2\Sigma_{2} are non isotopic Heegaard surfaces of a closed manifold so that d(Σ2)>2g(Σ1)d(\Sigma_{2})>2g(\Sigma_{1}), then d(Σ1)=0d(\Sigma_{1})=0 (in fact, they show that Σ1\Sigma_{1} is obtained from Σ2\Sigma_{2} by stabilization).

On the positive side, all but finitely many of the surfaces constructed by Casson and Gordon have distance exactly two (Casson and Gordon’s work show that the distance is at least 2 and Theorem 1.5 provides a new proof that the distance is at most 2). Hempel [hempel], using a construction of Kobayashi [KobayashiHeights], shows that for any g2g\geq 2 there exists a sequence of 3-manifolds MnM_{n} and Heegaard splittings Σn\Sigma_{n} for MnM_{n}, so that g(Σn)=gg(\Sigma_{n})=g and limnd(Σn)=\lim_{n\to\infty}d(\Sigma_{n})=\infty. T. Evans [evans] improved this by constructing, given g2g\geq 2 and d0d\geq 0, a Heegaard splitting of genus gg with distance at least dd. Recently, Qiu, Zou, and Guo [QiuZouGuo] and, independently, Ido, Jang and Kobayashi [IJK], constructed, given g2g\geq 2 and d1d\geq 1, a compact manifold with Heegaard splitting of genus gg and distance exactly dd. In [yoshi] Yoshizawa shows that when dd is even, a Heegaard splitting of distance exactly dd can be obtained by applying high powers of a single Dehn twist.

However, the answers to the following questions are not known in general:

Questions 3.1.
  1. (1)

    Given gi2g_{i}\geq 2 and di>0d_{i}>0 (i=1,2i=1,2), does there exist a 3-manifold admitting distinct Heegaard surfaces Σ1\Sigma_{1}, Σ2\Sigma_{2}, so that g(Σi)=gig(\Sigma_{i})=g_{i} and d(Σi)=did(\Sigma_{i})=d_{i}?

  2. (2)

    Given di>0d_{i}>0 (i=1,2i=1,2), does there exist a 3-manifold admitting distinct Heegaard surfaces Σ1\Sigma_{1}, Σ2\Sigma_{2}, so that d(Σi)=did(\Sigma_{i})=d_{i}?

Questions (1) and (2) above can naturally be generalized to more that two surfaces by setting i=1,,ni=1,\dots,n, for some chosen nn. The word “distinct” in the questions above can be interpreted as “distinct up to isotopy” or “distinct up to homeomorphism”; both yield interesting questions.

The answer for Question 3.1 (2) is known only in the following cases:

  • d1=d2=2d_{1}=d_{2}=2: As mentioned above, there are examples of Casson and Gordon of 3-manifolds admitting infinitely many Heegaard surfaces of unbounded genera and of distance invariant two. Other examples follow from S. Beiler and Y. Moriah [BleilerMoriah] (see also K. Morimoto and M. Sakuma [MorimotoSakuma]). They show that there exist 2-bridge knots KK admitting more than one minimal genus Heegaard surface (up to homeomorphism). Let Σ\Sigma be one of these surfaces. It is easy to see that d(Σ)=2d(\Sigma)=2: first, since g(Σ)=2g(\Sigma)=2, it is easy to see that d(Σ)2d(\Sigma)\geq 2. Next, Σ\Sigma is constructed by viewing KK as a torus 1-bridge knot (that is, there exists a genus 1 Heegaard splitting T1T2T_{1}\cup T_{2} so that KK intersects each TiT_{i} in a single unknotted arc) and tubing once. Meridian disks for TiT_{i} which are disjoint from KK and the tube, are also disjoint from the core of the tube, showing that d(Σ)2d(\Sigma)\leq 2.

  • d1=d2=1d_{1}=d_{2}=1: Let SS be a 4-punctured sphere and M=S×S1M=S\times S^{1}. J. Schultens [schultens] showed that g(M)=3g(M)=3. We note that MM admits two minimal genus Heegaard splittings, say Σ1\Sigma_{1} and Σ2\Sigma_{2}, such that Σ1\Sigma_{1} is obtained by tubing three boundary parallel tori, and Σ2\Sigma_{2} is obtained by tubing two boundary parallel tori, with an extra tube that wraps around a third boundary component. Since Σ1\Sigma_{1} and Σ2\Sigma_{2} induce boundary partitions with distinct numbers of components, they are distinct up to homeomorphism. By construction, d(Σ1)=d(Σ2)=1d(\Sigma_{1})=d(\Sigma_{2})=1.

  • d1=1,d2=2d_{1}=1,\ d_{2}=2: In [KRSIWR] the authors constructed a 3-manifold MM admitting minimal genus Heegaard splittings Σ1\Sigma_{1}, Σ2\Sigma_{2}, with d(Σ2)=2d(\Sigma_{2})=2 and d(Σ1)=1d(\Sigma_{1})=1. In this example, g(M)=g(Σ1)=g(Σ2)=3g(M)=g(\Sigma_{1})=g(\Sigma_{2})=3.

  • d1=d2=3d_{1}=d_{2}=3: Scharlemann [MR2823137], based on a preprint by Berge [berge], shows that there exists a closed manifold MM admitting two Heegaard splittings Σ1\Sigma_{1} and Σ2\Sigma_{2}, distinct up-to homeomorphism, so that g(M)=g(Σ1)=g(Σ2)=2g(M)=g(\Sigma_{1})=g(\Sigma_{2})=2 and d(Σ1)=d(Σ2)=3d(\Sigma_{1})=d(\Sigma_{2})=3.

We see that much is known when d1d_{1}, d23d_{2}\leq 3. By contrast, the answers to the following basic questions are unknown:

Questions 3.2.
  1. (1)

    Does there exist a 3-manifold admitting two (or more) distinct Heegaard surfaces with distance four or more?

  2. (2)

    Does there exist a 3-manifold admitting a Heegaard surface of distance three or more that is not of minimal genus?

4. Preliminaries

By manifold we mean compact, connected, orientable 3-manifold. We assume familiarity with the basic notions of 3-manifold topology (see, for example, [hempel-book] or [jaco]) and the basic facts about Heegaard splittings (see, for example, [scharlemann] or [sss]). We use the notation N()N(\ ) for open normal neighborhood, \partial for boundary, and |||\ \ | for the number of components. We define:

Definitions 4.1.
  1. (1)

    Let TT be a tetrahedron. A generalized tetrahedron is obtained by fixing two disjoint sets of vertices of TT, denoted V1V_{1}, V2V_{2}, and then removing V1V_{1} and truncating V2V_{2}; that is, a generalized tetrahedron TT^{\prime} has the form T=T(V1N(V2))T^{\prime}=T\setminus(V_{1}\cup N(V_{2})). TT^{\prime} has exactly four faces (resp. exactly six edges, at most four vertices), which are the intersection of the faces (resp. edges, vertices) of TT with TT^{\prime}. In particular, the components of N(V2)T\partial N(V_{2})\cap T^{\prime} are not considered faces. Important special cases are when V2=V_{2}=\emptyset, then TT^{\prime} is called semi-ideal, and when V1V_{1} consists of all four vertices, then TT^{\prime} is called ideal.

  2. (2)

    A generalized triangulation is obtained by gluing together finitely many generalized tetrahedra, where the gluings are done by identifying faces, edges, and vertices. Self-gluings (that is, gluing a tetrahedron to itself) are allowed, as are multiple gluings (that is, gluing two tetrahedra along more than one face). We refer the reader to [hatcher] for a detailed description in the special case when only tetrahedra are used, known there as Δ\Delta complexes. If all the generalized tetrahedra are ideal (resp. semi ideal), then the generalized triangulation is called an ideal (resp. semi ideal) triangulation. If the quotient obtained is homeomorphic to a given manifold MM it is said to be a generalized triangulation of MM.

We refer the reader to, for example, [LackenbyAlgorithm, Section 2] for a detailed discussion of generalized tetrahedra. It is well known that a very large class of 3-manifolds admits generalized triangulations, including all compact 3-manifolds. We outline the proof here. Let WW be a compact manifold and KiWK_{i}\subset\partial W (i=1,,ni=1,\dots,n) a disjoint, closed, connected subsurfaces. By crushing each KiK_{i} to a point pip_{i}, we obtain a 3-complex XX. We can triangulate XX so that each pip_{i} is a vertex of the triangulation. Removing pip_{i} we obtain a semi-ideal triangulation of N(iKi)N\setminus(\cup_{i}K_{i}). We conclude that (with KK corresponding to iKi\cup_{i}K_{i}):

Lemma 4.2.

Let MM be a compact manifold and KMK\subset\partial M a (not necessarily connected) closed subsurface. Then MKM\setminus K admits a generalized triangulation.


In [hempel] Hempel defined the distance of a Heegaard splitting:

Definition 4.3.

Let V1ΣV2V_{1}\cup_{\Sigma}V_{2} be a Heegaard splitting and d0d\geq 0 an integer. We say that the distance of Σ\Sigma is dd, denoted by d(Σ)=dd(\Sigma)=d, if dd is the smallest integer so that there exist meridian disks D1V1D_{1}\subset V_{1} and D2V2D_{2}\subset V_{2}, and essential curves αiΣ\alpha_{i}\subset\Sigma (i=0,,di=0,\dots,d), so that α0=D1\alpha_{0}=\partial D_{1}, αd=D2\alpha_{d}=\partial D_{2}, and αi1αi=\alpha_{i-1}\cap\alpha_{i}=\emptyset ( for 1id1\leq i\leq d).

The following lemma is easy and well known (see, for example [schleimer, Remark 2.6]):

Lemma 4.4.

Let V1ΣV2V_{1}\cup_{\Sigma}V_{2} be a Heegaard splitting. Suppose that one of the following holds:

  1. (1)

    for i=1,2i=1,2, there exists a properly embedded, non-boundary parallel annulus AiViA_{i}\subset V_{i}, and there exists an essential curve αΣ\alpha\subset\Sigma so that αA1A2\alpha\subset A_{1}\cap A_{2} (that is to say, A1A_{1} and A2A_{2} have an essential common boundary component), or:

  2. (2)

    there exist a meridian disk D1V1D_{1}\subset V_{1} and a properly embedded non-boundary parallel annulus A2V2A_{2}\subset V_{2}, so that D1D_{1} is disjoint from at least one component of A2\partial A_{2} that is essential in Σ\Sigma.

Then d(Σ)2d(\Sigma)\leq 2.

5. Coloring Σ\Sigma and constructing the pair of pants XX

Fix MM as in the statement of Theorem 1.8 and let V1ΣV2V_{1}\cup_{\Sigma}V_{2} be a Heegaard splitting for MM with g(Σ)76t+26g(\Sigma)\geq 76{t}+26. Let 𝒯\mathcal{T} be a generalized triangulation of MKM\setminus K (where KMK\subset\partial M is a closed subsurface) with t{t} generalized tetrahedra.

If Σ\Sigma weakly reduces, then d(Σ)1d(\Sigma)\leq 1; we assume as we may that Σ\Sigma is strongly irreducible. Rubinstein [rubinstein] (see also Stocking [stocking] and Lackenby [lackenby][LackenbyAlgorithm] when MM is not closed) show that Σ\Sigma is isotopic to an almost normal surface, that is, after isotopy the intersection of Σ\Sigma with the generalized tetrahedra of 𝒯\mathcal{T} consists of normal faces, of which there are two types:

  1. (1)

    normal disks (normal triangles and normal quadrilaterals)

  2. (2)

    an exceptional component, which is either an octagonal disk or an annulus obtained by tubing together two normal disks; at most one normal face of Σ\Sigma is an exceptional component.

Let NN be a regular neighborhood of 𝒯(1)\mathcal{T}^{(1)}, the 1-skeleton of 𝒯\mathcal{T}. For each v𝒯(1)Σv\in\mathcal{T}^{(1)}\cap\Sigma, let DvD_{v} be the component of ΣN\Sigma\cap N containing vv. Then DvD_{v} is a disk properly embedded in NN, called the vertex disk corresponding to vv. Let F^\widehat{F} be a normal face contained in a generalized tetrahedron TT. Then F=F^intNF=\widehat{F}\setminus\mbox{int}N is obtained from F^\widehat{F} by removing a neighborhood of the vertices of F^\widehat{F}. FF is called a truncated normal face. For the remainder of this paper, by a face we mean a truncated normal face or a vertex disk.

Remark 5.1.

The union of the boundaries of the faces forms a 3-valent graph in Σ\Sigma.

Let v,v𝒯(1)Σv,\ v^{\prime}\in\mathcal{T}^{(1)}\cap\Sigma be two vertices and DvD_{v}, DvD_{v^{\prime}} the corresponding vertex disks. Then DvD_{v} and DvD_{v^{\prime}} are called II-adjacent if vv and vv^{\prime} are contained in the same edge e𝒯(1)e\in\mathcal{T}^{(1)} and vv is adjacent to vv^{\prime} along ee. Note that DvD_{v} is II-adjacent to DvD_{v^{\prime}} if and only if vv and vv^{\prime} are contained in the same edge e𝒯(1)e\in\mathcal{T}^{(1)} and there exists an II-bundle over D2D^{2} with total space QNQ\subset N, so that Q(DvDv)N\partial Q\setminus(D_{v}\cup D_{v^{\prime}})\subset\partial N, QΣ=DvDvQ\cap\Sigma=D_{v}\cup D_{v^{\prime}}, and DvDvD_{v}\cup D_{v^{\prime}} is the associated I\partial I-bundle.

Let FF and FF^{\prime} be truncated normal faces. Then FF and FF^{\prime} are called II-adjacent if the corresponding normal faces are parallel and there is no normal face between the two. Note that FF and FF^{\prime} are II-adjacent if and only if they are contained in the same generalized tetrahedron TT, and there exists an II-bundle with total space QTintNQ\subset T\setminus\mbox{int}N, so that Q(FF)(TintN)\partial Q\setminus(F\cup F^{\prime})\subset\partial(T\setminus\mbox{int}N) and is disjoint from the vertices, truncated vertices, and missing vertices, QΣ=FFQ\cap\Sigma=F\cup F^{\prime}, and FFF\cup F^{\prime} is the associated I\partial I-bundle.

Clearly II-adjacency is symmetric but not, in general, transitive. The equivalence relation generated by II-adjacency is called II-equivalence, and its equivalence classes are called II-equivalent families. For example, suppose that a tetrahedron contains four quadrilaterals and denote the corresponding truncated normal faces by q1,q2,q3,q4q_{1},q_{2},q_{3},q_{4} (listed in order). If there is a truncated exceptional piece between q2q_{2} and q3q_{3}, then the truncated quadrilaterals form exactly two II-equivalent families: {q1,q2}\{q_{1},q_{2}\} and {q3,q4}\{q_{3},q_{4}\}.

Let \mathcal{F} be an II-equivalent family. Then II-adjacency induces a linear ordering on the faces in \mathcal{F}, ordered as F1,,FnF_{1},\dots,F_{n}, so that FiF_{i} is II-adjacent to Fi+1F_{i+1} (i=1,,n1i=1,\dots,n-1). This order is unique up-to reversing. We color the faces of \mathcal{F} as follows:

  1. (1)

    F1F_{1}, F2F_{2}, Fn1F_{n-1}, and FnF_{n} are colored red.

  2. (2)

    If n5n\geq 5, then F3,,Fn2F_{3},\dots,F_{n-2} are colored blue and yellow alternately. Note that this leaves us the freedom to exchange the blue and yellow colors of the faces of \mathcal{F}.

Remark.

For most of our work it suffices to color red F1F_{1} and FnF_{n}. We need to color F2F_{2} and Fn1F_{n-1} red as well for the last case of the proof of Theorem 1.8, where a further refinement of the colors will be given.

By construction, any yellow or blue face is II-adjacent to two distinct faces.

Remark 5.2.

Let DvD_{v} be a red vertex disk. By construction, DvD_{v} is outermost or next to outermost along an edge of 𝒯(1)\mathcal{T}^{(1)}. Therefore all the truncated normal faces that intersect DvD_{v} are red as well.

Lemma 5.3.

Let fr,tf_{r,t} denote the number of the red truncated triangles and fr,qf_{r,q} the number of the red truncated quadrilaterals. Then one of the following holds:

  1. (1)

    fr,t16tf_{r,t}\leq 16{t} and fr,q4t+4f_{r,q}\leq 4{t}+4.

  2. (2)

    fr,t16t+4f_{r,t}\leq 16{t}+4 and fr,q4tf_{r,q}\leq 4{t}.

Proof.

A generalized tetrahedron not containing the exceptional component admits at most four II-equivalent families of truncated triangles and one II-equivalent family of truncated quadrilaterals. If there is an exceptional component, the generalized tetrahedron containing it admits at most five II-equivalent families of truncated triangles and one II-equivalent family of truncated quadrilaterals, or at most four II-equivalent families of truncated triangles and two II-equivalent families of truncated quadrilaterals. Each family contains at most four red faces. The lemma follows. ∎

Let BB (resp. YY, RR) denote the union of the blue (resp. yellow, red) faces; note that faces are closed, so RR, YY, and BB are compact and may intersect along their boundaries. By Remark 5.1, BB, YY, RR, and BYB\cup Y are subsurfaces of Σ\Sigma.

Lemma 5.4.

χ(BY)(108t+38)\chi(B\cup Y)\leq-(108{t}+38).

Proof.

We first show that χ(R)(44t+12)\chi(R)\geq-(44{t}+12); for that, we order the red faces as F0F_{0}, F1,,FkF_{1},\dots,F_{k}, Fk+1,,FnF_{k+1},\dots,F_{n} (for some kk, nn) so that F0F_{0} is the exceptional piece (if there is one, F0=F_{0}=\emptyset otherwise), F1,,FkF_{1},\dots,F_{k} are the red truncated normal faces, and Fk+1,,FnF_{k+1},\dots,F_{n} are red vertex disks. Note that χ(F0)=0\chi(F_{0})=0 or χ(F0)=1\chi(F_{0})=1, so the worst case scenario is 0. By Remark 5.1, for 0ik0\leq i\leq k, the possibilities for Fi(j=1i1Fj)F_{i}\cap(\cup_{j=1}^{i-1}F_{j}) are: \emptyset, S1S^{1}, or a number of segments, each homeomorphic to II. Since a truncated normal triangle (respectively quadrilateral) is a hexagon (respectively octagon), the number of segments is at most 3 (respectively 4). We see that

χ(j=1iFj)χ(j=1i1Fj)2\chi(\cup_{j=1}^{i}F_{j})\geq\chi(\cup_{j=1}^{i-1}F_{j})-2

when FiF_{i} is a truncated normal triangle and

χ(j=1iFj)χ(j=1i1Fj)3\chi(\cup_{j=1}^{i}F_{j})\geq\chi(\cup_{j=1}^{i-1}F_{j})-3

when FiF_{i} is a truncated normal quadrilateral. By Remark 5.2, for ik+1i\geq k+1, FiF_{i} caps a hole of j=1i1Fi\cup_{j=1}^{i-1}F_{i}; hence

χ(j=1iFj)=χ(j=1i1Fj)+1\chi(\cup_{j=1}^{i}F_{j})=\chi(\cup_{j=1}^{i-1}F_{j})+1

in that case. Recall that fr,tf_{r,t} and fr,qf_{r,q} were defined and bounded in Lemma 5.3. Adding the contributions of the exceptional component (at worst 0), the triangles (at worst 2fr,t-2f_{r,t}), the quadrilaterals (at worst 3fr,q-3f_{r,q}), and ignoring the positive contribution of the vertex disks, Lemma 5.3 gives:

χ(R)\displaystyle\chi(R) \displaystyle\geq 02fr,t3fr,q\displaystyle 0-2f_{r,t}-3f_{r,q}
\displaystyle\geq 02(16t)3(4t+4)\displaystyle 0-2(16{t})-3(4{t}+4)
=\displaystyle= (44t+12).\displaystyle-(44{t}+12).

Since RR and BYB\cup Y are subsurfaces, Σ=R(BY)\Sigma=R\cup(B\cup Y), and R(BY)=R=(BY)R\cap(B\cup Y)=\partial R=\partial(B\cup Y) consists of circles, we have that χ(BY)=χ(Σ)χ(R)\chi(B\cup Y)=\chi(\Sigma)-\chi(R). By assumption g(Σ)76t+26g(\Sigma)\geq 76{t}+26, or equivalently χ(Σ)22(76t+26)\chi(\Sigma)\leq 2-2(76{t}+26). Hence:

χ(BY)\displaystyle\chi(B\cup Y) =\displaystyle= χ(Σ)χ(R)\displaystyle\chi(\Sigma)-\chi(R)
\displaystyle\leq [22(76t+26)]+[44t+12]\displaystyle[2-2(76{t}+26)]+[44{t}+12]
=\displaystyle= (108t+38).\displaystyle-(108{t}+38).

Lemma 5.5.

|(BY)|44t+14|\partial(B\cup Y)|\leq 44{t}+14.

Proof.

By construction (BY)=R\partial(B\cup Y)=\partial R. Bounding |R||\partial R| is similar to the proof of the previous lemma and we only paraphrase it here: we order the red faces as F0,,FnF_{0},\dots,F_{n} as in the proof of the previous lemma. It is easy to see that |F0||\partial F_{0}| is at most 2, and (similar to the Euler characteristic count on the previous lemma) for 1ik1\leq i\leq k,

|(j=1iFj)||(j=1i1Fj)|+2|\partial(\cup_{j=1}^{i}F_{j})|\leq|\partial(\cup_{j=1}^{i-1}F_{j})|+2

when FiF_{i} is a truncated normal triangle, and

|(j=1iFj)||(j=1i1Fj)|+3|\partial(\cup_{j=1}^{i}F_{j})|\leq|\partial(\cup_{j=1}^{i-1}F_{j})|+3

when FiF_{i} is a truncated normal quadrilateral. By Remark 5.2, for ik+1i\geq k+1,

|(j=1iFj)||(j=1i1Fj)|1.|\partial(\cup_{j=1}^{i}F_{j})|\leq|\partial(\cup_{j=1}^{i-1}F_{j})|-1.

Adding up the contributions of the truncated normal faces and ignoring the negative contribution of the vertex disks, Lemma 5.3 gives:

|(BY)|\displaystyle|\partial(B\cup Y)| =\displaystyle= |R|\displaystyle|\partial R|
\displaystyle\leq 2+2fr,t+3fr,q\displaystyle 2+2f_{r,t}+3f_{r,q}
\displaystyle\leq 2+2(16t)+3(4t+4)\displaystyle 2+2(16{t})+3(4{t}+4)
=\displaystyle= 44t+14.\displaystyle 44{t}+14.

By Remark 5.1, BYB\cap Y is a compact 1-manifold properly embedded in BYB\cup Y. Let ΓBY\Gamma\subset B\cup Y be the union of the arc components of BYB\cap Y. Endpoints of Γ\Gamma are the vertices of Σ\Sigma where red, blue, and yellow faces meet. By Remark 5.2 around any vertex of Σ\Sigma that is on the boundary of a red vertex disk all the colors are red; therefore the vertex disk at an endpoints of Γ\Gamma is yellow or blue.

Let 𝒱\mathcal{V} be the set of vertices of red truncated normal faces. We subdivide 𝒱\mathcal{V} into 3 disjoint sets as follows: 𝒱0\mathcal{V}_{0} are vertices that are on the boundary of at least two red faces; 𝒱+\mathcal{V}_{+} are vertices that are on the boundary of three faces so that one is red, one is yellow, and one is blue; 𝒱\mathcal{V}_{-} are vertices that are on the boundary of three faces so that one is red and two are yellow, or one is red and two are blue. By construction, 𝒱+\mathcal{V}_{+} is exactly the set of endpoints of Γ\Gamma.

By construction, at every vertex exactly one face is a vertex disk. We exchange the colors of the blue vertex disks with the colors of the yellow vertex disks; let RR^{\prime}, BB^{\prime}, YY^{\prime} and Γ\Gamma^{\prime} be defined as above, using the new coloring. By Remark 5.2, 𝒱\mathcal{V}_{-} is exactly the set of endpoints of Γ\Gamma^{\prime} (we emphasize that 𝒱\mathcal{V}_{-} is the set of vertices defined above using the original coloring). Hence, by exchanging colors if necessary, we may assume that the number of endpoints of Γ\Gamma is at most 12|𝒱|\frac{1}{2}|\mathcal{V}|. Since every arc of Γ\Gamma has two distinct endpoints and Γ\Gamma has at most 12|𝒱|\frac{1}{2}|\mathcal{V}| endpoints, we get that |Γ|14|𝒱||\Gamma|\leq\frac{1}{4}|\mathcal{V}|.

There are at most 16 vertices in 𝒱\mathcal{V} from the truncated exceptional component, at most 6 from each truncated red triangle, and at most 8 from each truncated red quadrilateral. By Lemma 5.3 we get:

|𝒱|\displaystyle|\mathcal{V}| \displaystyle\leq 16+6fr,t+8fr,q\displaystyle 16+6f_{r,t}+8f_{r,q}
\displaystyle\leq 16+6(16t)+8(4t+4)\displaystyle 16+6(16{t})+8(4{t}+4)
\displaystyle\leq 128t+48.\displaystyle 128{t}+48.

Hence:

|Γ|14|𝒱|32t+12.|\Gamma|\leq\frac{1}{4}|\mathcal{V}|\leq 32{t}+12.

Let F1,,FkF_{1},\dots,F_{k} be the components of BYB\cup Y cut open along Γ\Gamma (note that F1,,FkF_{1},\dots,F_{k} are not, in general, faces). Cutting along Γ\Gamma increases the Euler characteristic by |Γ||\Gamma| and increases the number of boundary components by at most |Γ||\Gamma|. Using Lemma 5.4 we get:

Σi=1kχ(Fi)\displaystyle\Sigma_{i=1}^{k}\chi(F_{i}) =\displaystyle= χ(i=1kFi)\displaystyle\chi(\cup_{i=1}^{k}F_{i})
=\displaystyle= χ(BY)+|Γ|\displaystyle\chi(B\cup Y)+|\Gamma|
\displaystyle\leq (108t+38)+(32t+12)\displaystyle-(108{t}+38)+(32{t}+12)
=\displaystyle= (76t+26).\displaystyle-(76{t}+26).

And using Lemma 5.5 we get:

Σi=1k|Fi|\displaystyle\Sigma_{i=1}^{k}|\partial F_{i}| =\displaystyle= |i=1kFi|\displaystyle|\partial\cup_{i=1}^{k}F_{i}|
\displaystyle\leq |(BY)|+|Γ|\displaystyle|\partial(B\cup Y)|+|\Gamma|
\displaystyle\leq (44t+14)+(32t+12)\displaystyle(44{t}+14)+(32{t}+12)
=\displaystyle= 76t+26.\displaystyle 76{t}+26.

Combining these inequalities we get:

(1) Σi=1kχ(Fi)(Σi=1k|Fi|).\Sigma_{i=1}^{k}\chi(F_{i})\leq-(\Sigma_{i=1}^{k}|\partial F_{i}|).
Proposition 5.6.

There exists a pair of pants XΣX\subset\Sigma with the following two properties:

  1. (1)

    Either Xint(B)X\subset\mbox{int}(B) or Xint(Y)X\subset\mbox{int}(Y) (say the former).

  2. (2)

    The components of X\partial X, denoted by α\alpha, β\beta, and γ\gamma, are essential in Σ\Sigma.

Proof.

By Inequality (1) above, for some ii, χ(Fi)|Fi|\chi(F_{i})\leq-|\partial F_{i}|; equivalently, g(Fi)1g(F_{i})\geq 1. Fix such ii. By construction, (BY)int(Fi)(B\cap Y)\cap\mbox{int}(F_{i}) consists of simple closed curves; see Figure 1. Let \mathcal{E} (resp. \mathcal{I}) denote the curves of (BY)intFi(B\cap Y)\cap\mbox{int}F_{i} that are essential (resp. inessential) in Σ\Sigma.

Refer to caption

Figure 1.

Let Δ\Delta be the union of the components of cl(ΣFi)\mbox{cl}(\Sigma\setminus F_{i}) that are disks (possibly, Δ=\Delta=\emptyset). Let F=FiΔF=F_{i}\cup\Delta. By construction, every component of F\partial F is essential in Σ\Sigma (possibly, F=\partial F=\emptyset). Thus, a closed curve of FF is essential in Σ\Sigma if and only if it is essential in FF. Since g(F)=g(Fi)>0g(F)=g(F_{i})>0, if F\partial F\neq\emptyset then χ(F)<0\chi(F)<0; if, on the other hand, F=\partial F=\emptyset, then F=ΣF=\Sigma and in particular, g(F)=g(Σ)76t+26>1g(F)=g(\Sigma)\geq 76t+26>1; we conclude that in either case χ(F)<0\chi(F)<0. Thus some component of FF cut open along \mathcal{E}, denoted by FF^{\prime}, has χ(F)<0\chi(F^{\prime})<0. Note that every curve of F\partial F^{\prime} is essential in Σ\Sigma. By construction, (BY)intF(B\cap Y)\cap\mbox{int}F^{\prime}\subset\mathcal{I}. Let Δ\Delta^{\prime} be the union of the disks bounded by outermost curves of F\mathcal{I}\cap F^{\prime} and the disks ΔF\Delta\cap F^{\prime}. Note that ΔintF\Delta^{\prime}\subset\mbox{int}F^{\prime} consists of disks, and FΔF^{\prime}\setminus\Delta^{\prime} is entirely blue or yellow; in Figure 1, Δ\Delta^{\prime} consists of two disks, one of each kind.

Assume first that F\partial F^{\prime}\neq\emptyset. Let cFc\subset F^{\prime} be a curve, parallel to a component of F\partial F^{\prime}, that decomposes FF^{\prime} as A′′cF′′A^{\prime\prime}\cup_{c}F^{\prime\prime}, where A′′A^{\prime\prime} is an annulus. By isotopy of cc in FF^{\prime} we may assume that ΔA′′\Delta^{\prime}\subset A^{\prime\prime}. We see that F′′F^{\prime\prime} is entirely blue or yellow, χ(F′′)=χ(F)<0\chi(F^{\prime\prime})=\chi(F^{\prime})<0, and F′′\partial F^{\prime\prime} is essential in Σ\Sigma.

Next assume that F=\partial F^{\prime}=\emptyset (that is, F=ΣF^{\prime}=\Sigma). Let cc be a separating, essential curve in FF^{\prime}. By isotopy of cc we may assume that Δ\Delta^{\prime} is contained in one component of FF^{\prime} cut open along cc. Let F′′F^{\prime\prime} be the other component. We conclude that in this case too, F′′F^{\prime\prime} is entirely blue or yellow, χ(F′′)<0\chi(F^{\prime\prime})<0, and F′′\partial F^{\prime\prime} is essential in Σ\Sigma.

Let α\alpha, β\beta, and γint(F′′)\gamma\subset\mbox{int}(F^{\prime\prime}) be three curves that are essential in F′′F^{\prime\prime} (and hence in Σ\Sigma) and co-bound a pair of pants, denoted by XX, in F′′F^{\prime\prime}. It is easy to see that XX, α\alpha, β\beta, and γ\gamma have the properties listed in Proposition 5.6. ∎

Since Xint(B)X\subset\mbox{int}(B) it is on the boundary of the total space of an II-bundle in ViV_{i} (i=1,2i=1,2). The other component of the associated I\partial I-bundle is a pair of pants denoted by XiX_{i}. The components of Xi\partial X_{i} are denoted by αi\alpha_{i}, βi\beta_{i}, and γi\gamma_{i} so that αi\alpha_{i} is parallel to α\alpha, βi\beta_{i} is parallel to β\beta, and γi\gamma_{i} is parallel to γ\gamma. Since Xint(B)X\subset\mbox{int}(B), every point of XiX_{i} is yellow or red; we conclude that XXi=X\cap X_{i}=\emptyset. Hence the II-bundle in ViV_{i} is trivial. The annulus extended from α\alpha to αi\alpha_{i} (resp. β\beta to βi\beta_{i}, γ\gamma to γi\gamma_{i}) in ViV_{i} is denoted by AiA_{i} (resp. BiB_{i}, CiC_{i}). By construction, these annuli are embedded. Note that X1X2X_{1}\cap X_{2}\neq\emptyset is possible.

Lemma 5.7.

One of the following holds:

  1. (1)

    After renaming if necessary, A1V1A_{1}\subset V_{1} and B2V2B_{2}\subset V_{2} are not boundary parallel, and A2V2A_{2}\subset V_{2}, B1V1B_{1}\subset V_{1}, and C1V1C_{1}\subset V_{1} are boundary parallel.

  2. (2)

    d(Σ)2d(\Sigma)\leq 2.

Proof.

We claim that one of AiA_{i}, BiB_{i} or CiC_{i} is not boundary parallel in ViV_{i} (i=1,2i=1,2). Suppose, for a contradiction, that AiA_{i}, BiB_{i}, CiC_{i} are all boundary parallel. Let A~iVi\widetilde{A}_{i}\subset V_{i} be the annulus that AiA_{i} is parallel to. Since XX is an essential pair of pants it is not contained in A~i\widetilde{A}_{i}; it is easy to see that the intersection of the region of parallelism between AiA_{i} and A~i\widetilde{A}_{i} and the trivial II-bundle in ViV_{i} is exactly AiA_{i}; similarly we treat BiB_{i} and CiC_{i}. We see that ViV_{i} is homeomorphic to the trivial II-bundle, and hence is a genus 2 handlebody. This contradicts our assumption that g(Σ)76t+26>2g(\Sigma)\geq 76{t}+26>2.

Therefore one of A1A_{1}, B1B_{1} or C1C_{1} is not boundary parallel, and after renaming if necessary we may assume it is A1A_{1}. We may assume A2A_{2} is boundary parallel, for otherwise d(Σ)2d(\Sigma)\leq 2 by Lemma 4.4 (1). Similarly, one of A2A_{2}, B2B_{2} or C2C_{2} is not boundary parallel, after renaming if necessary we may assume it is B2B_{2}, while B1B_{1} is boundary parallel. Finally by Lemma 4.4 (1) we may assume that C1C_{1} or C2C_{2} is boundary parallel, say C1C_{1}. ∎

Lemma 5.8.

One of the following holds:

  1. (1)

    α1\alpha_{1}, β2\beta_{2} and γ2\gamma_{2} are essential in Σ\Sigma, and α\alpha is not isotopic in Σ\Sigma to α1\alpha_{1}, β\beta or γ\gamma.

  2. (2)

    d(Σ)2d(\Sigma)\leq 2.

Refer to caption

Figure 2.
Proof.

We may assume that Conclusion (1) of Lemma 5.7 holds; thus A2A_{2}, B1B_{1} and C1C_{1} are boundary parallel. We denote by A~2,B~1,C~1Σ\widetilde{A}_{2},\widetilde{B}_{1},\widetilde{C}_{1}\subset\Sigma the annuli to which A2A_{2}, B1B_{1}, and C1C_{1} are parallel (respectively). See Figure 2, where X1X2=X_{1}\cap X_{2}=\emptyset, but this need not be the case.

If α1\alpha_{1} is inessential in Σ\Sigma, then we may cap A1A_{1} off, and after a small isotopy we obtain a meridian disk D1V1D_{1}\subset V_{1} with D1=α\partial D_{1}=\alpha. Using D1D_{1} and B2B_{2}, Lemma 4.4 (2) shows that d(Σ)2d(\Sigma)\leq 2. Similarly if β2\beta_{2} (resp. γ2\gamma_{2}) is inessential in Σ\Sigma then β\beta (resp. γ\gamma) bounds a meridian disk D2V2D_{2}\subset V_{2}. Using D2D_{2} and A1A_{1}, Lemma 4.4 (2) shows that d(Σ)2d(\Sigma)\leq 2.

If α\alpha is isotopic to α1\alpha_{1} in Σ\Sigma then either the annulus connecting the two contains XX or g(Σ)=2g(\Sigma)=2. The former is impossible since XX is an essential pair of pants and the latter contradicts the assumption g(Σ)76t+26>2g(\Sigma)\geq 76{t}+26>2.

Let cΣc\subset\Sigma be a closed curve constructed by pasting together four arcs, the first connecting β\beta to γ\gamma in XX, the second connecting γ\gamma to γ1\gamma_{1} in C~1\widetilde{C}_{1}, the third connecting γ1\gamma_{1} to β1\beta_{1} in X1X_{1}, and the final arc connecting β1\beta_{1} to β\beta in B~1\widetilde{B}_{1}. Since XX1=X\cap X_{1}=\emptyset, we have |cβ|=|cγ|=1|c\cap\beta|=|c\cap\gamma|=1. By construction |cα|=0|c\cap\alpha|=0. Therefore α\alpha is not isotopic in Σ\Sigma to either β\beta or γ\gamma. ∎

6. Proof of Theorem 1.8

With notation as in Section 5 we assume, as we may by Lemma 5.7, that A1A_{1} and B2B_{2} are not boundary parallel and that A2A_{2}, B1B_{1}, and C1C_{1} are boundary parallel. We assume, as we may by Lemma 5.8, that α1\alpha_{1}, β2\beta_{2} and γ2\gamma_{2} are essential in Σ\Sigma and α\alpha is not isotopic in Σ\Sigma to α1\alpha_{1}, β\beta or γ\gamma.

The proof is divided into the following two cases:

Case One. α1\alpha_{1} can be isotoped to be disjoint from X2X_{2}. Let A~2\widetilde{A}_{2}, B~1\widetilde{B}_{1}, and C~1\widetilde{C}_{1} be as in Lemma 5.8. Let TΣT\subset\Sigma be the twice punctured torus XB~1C~1X1X\cup\widetilde{B}_{1}\cup\widetilde{C}_{1}\cup X_{1}. Isotope α1\alpha_{1} so that α1X2=\alpha_{1}\cap X_{2}=\emptyset. After this isotopy, X2(α1X)=X_{2}\cap(\alpha_{1}\cup X)=\emptyset. Hence either X2(X1B~1C~1)X_{2}\subset(X_{1}\cup\widetilde{B}_{1}\cup\widetilde{C}_{1}) or X2T=X_{2}\cap T=\emptyset. In the former case, α2(X1B~1C~1)\alpha_{2}\subset(X_{1}\cup\widetilde{B}_{1}\cup\widetilde{C}_{1}). Since α\alpha is isotopic to α2\alpha_{2} in Σ\Sigma, α\alpha is isotopic into X1B~1C~1X_{1}\cup\widetilde{B}_{1}\cup\widetilde{C}_{1}. By Proposition 5.6(2) α\alpha is essential, and hence α\alpha is isotopic to a component of (X1B~1C~1)=α1βγ\partial(X_{1}\cup\widetilde{B}_{1}\cup\widetilde{C}_{1})=\alpha_{1}\cup\beta\cup\gamma, contradicting our assumptions.

Hence we may assume that X2T=X_{2}\cap T=\emptyset. Let D1V1D_{1}\subset V_{1} be a meridian disk obtained by compressing or boundary compressing A1A_{1}. After a small isotopy we may assume that D1A1=D1(αα1)=\partial D_{1}\cap\partial A_{1}=\partial D_{1}\cap(\alpha\cup\alpha_{1})=\emptyset, and hence either D1T\partial D_{1}\subset T (hence D1β2=\partial D_{1}\cap\beta_{2}=\emptyset) or D1T=\partial D_{1}\cap T=\emptyset (hence D1β=\partial D_{1}\cap\beta=\emptyset). Thus D1D_{1} is disjoint from at least one component of B2\partial B_{2}; by Lemma 4.4 (2), d(Σ)2d(\Sigma)\leq 2, proving Theorem 1.8 in Case One.



Before proceeding to Case Two we refine our colorings. Let \mathcal{F} be an II-equivalent family of faces, ordered as F1,,FnF_{1},\dots,F_{n} so that FiF_{i} is II-adjacent to Fi+1F_{i+1} (i=1,,n1i=1,\dots,n-1). Then the red faces are F1F_{1}, F2F_{2}, Fn1F_{n-1}, and FnF_{n}. We color F1F_{1} and FnF_{n} dark red. If n3n\geq 3 we color F2F_{2} and Fn1F_{n-1} light red.

Clearly, a face is II-adjacent to two distinct faces if and only if it is colored blue, yellow, or light red. Let pp be a point on such a face. Then pp is on the boundary of two II-fibers, on the V1V_{1} and V2V_{2} sides. Denote the other endpoints of these fibers by p1p_{1} and p2p_{2}. By construction we see that the colors at pp, p1p_{1} and p2p_{2} fulfill the conditions in Table 1.

pp p1p_{1}, p2p_{2}
blue yellow or light red
yellow blue or light red
light red one is dark red and the other can be any color

Table 1. Colors of II-adjacent points
Notation 6.1.

Every light red face is II-equivalent to a dark red face on one side. On the other side it is II-equivalent to a face that may be blue, yellow, light red or dark red. This decomposes the set of light red points into four disjoint subsets. We label a light red face that is II-equivalent to a blue (resp. yellow) face by lr[b] (resp. lr[y]).

Case Two. α1\alpha_{1} cannot be isotoped to be disjoint from X2X_{2}. Since αint(B)\alpha\subset\mbox{int}(B), each point of α1\alpha_{1} is yellow or light red. Hence α1\alpha_{1} bounds II-bundles on both sides. Let A1,2A_{1,2} be the be the (possibly immersed) II-bundle obtained by extending α1\alpha_{1} into V2V_{2}, and denote A1,2α1\partial A_{1,2}\setminus\alpha_{1} by α1,2\alpha_{1,2}; see Figure 3.

Refer to caption

Figure 3.

Since every point of α1\alpha_{1} is yellow or light red and labeled lr[b], every point of α1,2\alpha_{1,2} is blue, light red and labeled lr[y], or dark red (see Table 1 and Notation 6.1). Thus α1α1,2=\alpha_{1}\cap\alpha_{1,2}=\emptyset, and we see that A1,2A_{1,2} is trivial II-bundle, that is, an embedded annulus.

Since X2X_{2} and XX co-bound an II-bundle, every point of X2X_{2} is yellow or light red and labeled lr[b]. Thus α1,2X2=\alpha_{1,2}\cap X_{2}=\emptyset. By assumption α1\alpha_{1} cannot be isotoped off X2X_{2}. Hence α1\alpha_{1} is not isotopic to α1,2\alpha_{1,2}; this implies that A1,2A_{1,2} is not boundary parallel. By assumption A1A_{1} is not boundary parallel and α1\alpha_{1} is essential in Σ\Sigma. Applying Lemma 4.4 (1) to A1A_{1}, A1,2A_{1,2}, and α1\alpha_{1} we conclude that d(Σ)2d(\Sigma)\leq 2, completing the proof of Theorem 1.8.