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Classification of non-free Kleinian groups generated by two parabolic transformations

Hirotaka Akiyoshi Department of Mathematics
Graduate School of Science
Osaka City University
3-3-138, Sugimoto, Sumiyoshi-ku Osaka, 558-8585, Japan
[email protected]
Ken’ichi Ohshika Department of Mathematics
Faculty of Science
Gakushuin University
Mejiro 1-5-1, Toshima-ku, 171-8588, Japan
[email protected]
John Parker Department of Mathematical Sciences
Durham University, Science Laboratories
South Road, Durham, DH1 3LE, United Kingdom
[email protected]
Makoto Sakuma Department of Mathematics
Faculty of Science
Hiroshima University
Higashi-Hiroshima, 739-8526, Japan
[email protected]
 and  Han Yoshida National Institute of Technology, Nara College
22 Yata-cho, Yamatokoriyama, Nara, 639-1058, Japan
[email protected]
Abstract.

We give a full proof to Agol’s announcement on the classification of non-free Kleinian groups generated by two parabolic transformations.

2010 Mathematics Subject Classification:
Primary 57M50, Secondary 57M25

1. Introduction

Motivated by knot theory, Riley studied Kleinian groups generated by two parabolic transformations (see [44, 45, 46, 47, 48]). In particular, the construction of the complete hyperbolic structure on the figure-eight knot complement [45] inspired Thurston to establish the uniformisation theorem of Haken manifolds. The space of marked subgroups of PSL(2,)\mbox{$\mathrm{PSL}$}(2,\mathbb{C}) generated by two non-commuting parabolic transformations is parametrised by a non-zero complex number. There is an open set, {\mathcal{R}}, called the Riley slice of Schottky space, of Kleinian groups of this type that are free and discrete, and for which the quotient of the domain of discontinuity is a four times punctured sphere. For every group in {\mathcal{R}}, the Klein manifold (the quotient of union of the hyperbolic space and the domain of discontinuity) is homeomorphic to the complement of the 2-strand trivial tangle. Keen and Series [29] studied the Riley slice by applying their theory of pleating rays, and it was supplemented by Komori and Series [31]. Motivated by knot theory, Akiyoshi, Sakuma, Wada and Yamashita [6] studied the combinatorial structures of the Ford domains, by extending Jorgensen’s work [28] on punctured torus groups, which leads to a natural tessellation of {\mathcal{R}} (see Figure 0.2b in [6]). Ohshika and Miyachi [42] proved that the closure of {\mathcal{R}} is equal to the space of marked Kleinian groups with two parabolic generators which are free and discrete. Building on his joint work [24], [26] and [36] with Gehring, Hinkkanen and Marshall, respectively, Martin [35] identified the exterior of {\mathcal{R}} as the Julia set of a certain semigroup of polynomials and proved a “supergroup density theorem” for groups in the exterior of {\mathcal{R}}. The problem to detect freeness and non-freeness of (not necessarily discrete) groups generated by two non-commuting parabolic transformations has attracted attention of various researchers (see [33, 23, 56, 30] and references therein).

In this paper, we are interested in Kleinian groups that are in the complement of the closure of {\mathcal{R}}, namely the groups that are discrete but not free. The essential simple loops on the boundary of the complement of the 2-strand trivial tangle, which are not null homotopic in the ambient space, are parametrised by a slope rr in /2\mathbb{Q}/2\mathbb{Z}. The Heckoid groups, introduced by Riley [47] and formulated by Lee and Sakuma [32] following Agol [2], are Kleinian groups with two parabolic generators in which the element corresponding to the curve αr\alpha_{r} of slope rr has finite order. The most extreme case is the group G(r)G(r) where this element is the identity, in which case, the quotient of hyperbolic space by this group is the complement of a 2-bridge knot or link.

In [1, Theorem 4.3], Adams proved that a non-free and torsion-free Kleinian group Γ\Gamma is generated by two parabolic transformations if and only if the quotient hyperbolic manifold 3/Γ\mathbb{H}^{3}/\Gamma is homeomorphic to the complement of a 22-bridge link K(r)K(r) which is not a torus link. (We regard a knot as a one-component link.) This refines the result of Boileau and Zimmermann [11, Corollary 3.3] that a link in S3S^{3} is a 22-bridge link if and only if its link group is generated by two meridians.

In 2002, Agol [2] announced the following classification theorem of non-free Kleinian groups generated by two parabolic transformations, which generalises Adams’ result. The main purpose of this paper is to give a full proof to this theorem.

Theorem 1.1.

A non-free Kleinian group Γ\Gamma is generated by two non-commuting parabolic elements if and only if one of the following holds.

  1. (1)

    Γ\Gamma is conjugate to the hyperbolic 22-bridge link group, G(r)G(r), for some rational number r=q/pr=q/p, where pp and qq are coprime integers such that q±1(modp)q\not\equiv\pm 1\pmod{p}.

  2. (2)

    Γ\Gamma is conjugate to the Heckoid group, G(r;n)G(r;n), for some rr\in\mathbb{Q} and some n123n\in\frac{1}{2}\mathbb{N}_{\geq 3}.

Refer to caption
Figure 1. Weighted graphs representing 22-bridge links and Heckoid orbifolds, where the thick edges with weight \infty correspond to parabolic loci and thin edges with integral weights represent the singular set. See Definition 3.4 for the precise description of the weighted graphs.

In the remainder of the introduction, we explain the meaning of the theorem more precisely.

Recall that a 22-bridge link is a knot or a two-component link which is represented by a diagram in the xx-yy plane that has two maximal points and two minimal points with respect to the height function determined by the yy-coordinate. We may assume that the two maximal points and the two minimal points, respectively, have the same yy-coordinates. Such a diagram gives a plait (or plat) representation of the 22-bridge link consisting of two upper bridges, two lower bridges, and a 44-strand braid connecting the upper and lower bridges (see Figure 1(1)). The 22-bridge links are parametrized by the set {}\mathbb{Q}\cup\{\infty\}, and the 22-bridge link corresponding to r{}r\in\mathbb{Q}\cup\{\infty\} is denoted by K(r)K(r) and is called the 22-bridge link of slope rr (see Section 2 for the precise definition). If r=r=\infty then K(r)K(r) is the 22-component trivial link, and if rr\in\mathbb{Z} then K(r)K(r) is the trivial knot. If r=q/pr=q/p\in\mathbb{Q}, where pp and qq are coprime integers, then K(q/p)K(q/p) is hyperbolic, i.e., S3K(r)S^{3}-K(r) admits a complete hyperbolic structure of finite volume, if and only if q±1(modp)q\not\equiv\pm 1\pmod{p}. In this case, there is a torsion-free Kleinian group Γ\Gamma, unique up to conjugation, such that 3/Γ\mathbb{H}^{3}/\Gamma is homeomorphic to the link complement S3K(r)S^{3}-K(r) as oriented manifold. We denote the Kleinian group Γ\Gamma, by G(r)G(r), and call it the hyperbolic 22-bridge link group of slope rr.

The Heckoid groups were first introduced by Riley [47] as an analogy of the classical Hecke groups considered by Hecke [25]. The topological structure of their quotient orbifolds was worked out by Lee and Sakuma [32], following the description by Agol [2]. Specifically, they showed that the Heckoid groups are the orbifold fundamental groups of the Heckoid orbifolds illustrated in Figure 1(2)-(4). (See [7, 10, 19] for basic terminologies and facts concerning orbifolds.) These figures illustrate weighted graphs (S3,Σ,w)(S^{3},\Sigma,w) whose explicit descriptions are given by Definition 3.4. For each weighted graph (S3,Σ,w)(S^{3},\Sigma,w) in the figure, let (M0,P)(M_{0},P) be the pair of a compact 33-orbifold M0M_{0} and a compact 22-suborbifold PP of M0\partial M_{0} determined by the rules described below. Let Σ\Sigma_{\infty} be the subgraph of Σ\Sigma consisting of the edges with weight \infty, and let Σs\Sigma_{s} be the subgraph of Σ\Sigma consisting of the edges with integral weight.

  1. (1)

    The underlying space |M0||M_{0}| of the orbifold M0M_{0} is the complement of an open regular neighbourhood of the subgraph Σ\Sigma_{\infty}.

  2. (2)

    The singular set of M0M_{0} is Σ0:=Σs|M0|\Sigma_{0}:=\Sigma_{s}\cap|M_{0}|, where the index of each edge of the singular set is given by the weight w(e)w(e) of the corresponding edge ee of Σs\Sigma_{s}.

  3. (3)

    For an edge ee of Σ\Sigma_{\infty}, let PP be the 22-suborbifold of M0\partial M_{0} defined as follows.

    1. (a)

      In Figure 1(2), PP consists of two annuli in M0\partial M_{0} whose cores, respectively, are meridians of the two edges of Σ\Sigma_{\infty}.

    2. (b)

      In Figure 1(3), PP consists of an annulus in M0\partial M_{0} whose core is a meridian of the single edge of Σ\Sigma_{\infty}.

    3. (c)

      In Figure 1(4), PP consists of two copies of the annular orbifold D2(2,2)D^{2}(2,2) (the 22-orbifold with underlying space the disc and with two cone points of index 22) in M0\partial M_{0} each of which is bounded by a meridian of an edge of Σ\Sigma_{\infty}.

By [32, Lemmas 6.3 and 6.6], the orbifold pair (M0,P)(M_{0},P) is a Haken pared orbifold (see Definition 3.1 or [10, Definition 8.3.7]) and admits a unique complete hyperbolic structure, which is geometrically finite (see Section 3 or [32, Proposition 6.7]). Namely there is a geometrically finite Kleinian group Γ\Gamma, unique up to conjugation, such that M:=3/ΓM:=\mathbb{H}^{3}/\Gamma is isomorphic to the interior of the compact orbifold M0M_{0}, such that PP represents the parabolic locus. The pair (M0,P)(M_{0},P) is also regarded as a relative compactification of the pair consisting of a non-cuspidal part of MM and its boundary (see Section 3).

We denote the pared orbifold :=(M0,P)\mathcal{M}:=(M_{0},P) by 0(r;n)\mathcal{M}_{0}(r;n), 1(r;m)\mathcal{M}_{1}(r;m), or 2(r;m)\mathcal{M}_{2}(r;m) according as it is described by the weighted graph in Figure 1(2), (3), or (4). We also denote the Kleinian group Γ\Gamma by π1()\pi_{1}(\mathcal{M}).

Then the assertion (2) of the main Theorem 1.1 is equivalent to the following assertion (2’)

  1. (2’)

    Γ\Gamma is conjugate to the Kleinian group π1()\pi_{1}(\mathcal{M}) for some pared orbifold =0(r;n)\mathcal{M}=\mathcal{M}_{0}(r;n), 1(r;m)\mathcal{M}_{1}(r;m), or 2(r;m)\mathcal{M}_{2}(r;m) in Definition 3.4.

Agol [2] also announced the following classification of parabolic generating pairs of the groups in Theorem 1.1, which refines and extends Adams’ results that every hyperbolic 22-bridge link group has only finitely many parabolic generating pairs [1, Corollary 4.1] and that the figure-eight knot group has precisely two parabolic generating pairs up to equivalence [1, Corollary 4.6].

Theorem 1.2.

(1) If Γ\Gamma is a hyperbolic 22-bridge link group, then it has precisely two parabolic generating pairs, up to equivalence.

(2) If Γ\Gamma is a Heckoid group, then it has a unique parabolic generating pair, up to equivalence.

Here, by a parabolic generating pair of a Kleinian group Γ\Gamma, we mean an unordered pair {α,β}\{\alpha,\beta\} of parabolic transformations α\alpha and β\beta that generate Γ\Gamma. Two parabolic generating pairs {α,β}\{\alpha,\beta\} and {α,β}\{\alpha^{\prime},\beta^{\prime}\} are said to be equivalent if {α,β}\{\alpha^{\prime},\beta^{\prime}\} is equal to {αϵ1,βϵ2}\{\alpha^{\epsilon_{1}},\beta^{\epsilon_{2}}\} for some ϵ1,ϵ2{±1}\epsilon_{1},\epsilon_{2}\in\{\pm 1\} up to simultaneous conjugacy. In the companion [4] of this paper by Shunsuke Aimi, Donghi Lee, Shunsuke Sakai and the fourth author, an alternative proof of the theorem is given.

Theorems 1.1 and 1.2 are beautifully illustrated by a figure produced by Yasushi Yamashita upon request of Caroline Series, which is to be included in her article [52] in preparation. The figure is produced by using the results announced in [6, Section 3 of Preface]. (See also Figure 0.2b in [6], which was also produced by Yamashita.) For further properties of Heckoid groups, please see the article [5] in preparation.

This paper is organised as follows. In Section 2, we recall basic facts concerning 22-bridge links. In Section 3, we give the precise definitions of the Heckoid orbifolds and Heckoid groups. In Section 4, we give the classification of dihedral orbifolds, i.e., good orbifolds with dihedral orbifold fundamental groups (Theorem 4.1), which holds a key to the proof of the main theorem. In Section 5, we prove the relative tameness theorem for hyperbolic orbifolds (Theorem 5.1), following Bowditch’s proof of the tameness theorem for hyperbolic orbifolds ([15]). This theorem is used in the treatment of geometrically infinite two parabolic generator non-free Kleinian groups. In fact, it turns out there is no such groups. In Section 6, we introduce a convenient method for describing pared orbifolds (Convention 6.1) and the concept of an orbifold surgery (Definition 6.3), and then prove a simple but useful lemma for orbifold surgeries (Lemma 6.4). In Section 7, we follow Adams [1], and recall basic facts concerning two parabolic generator Kleinian groups, in particular an estimate of the length of parabolic generators with respect to the maximal cusp (Lemma 7.1). In Section 8, we give an outline of the proof of the main theorem. Sections 9, 10, and 11 are devoted to the proof of the main theorem. In the appendix, which consists of Sections 12 and 13, we give the classification of geometric dihedral orbifolds that is necessary for the proof Theorem 4.1.

Throughout this paper, we use the following notation.

Notation 1.3.

(1) For an orbifold 𝒪{\mathcal{O}}, the symbol π1(𝒪)\pi_{1}({\mathcal{O}}) denotes the orbifold fundamental group of 𝒪{\mathcal{O}}, H1(𝒪)H_{1}({\mathcal{O}}) denotes the abelianisation of π1(𝒪)\pi_{1}({\mathcal{O}}), and H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) denotes H1(𝒪)2H_{1}({\mathcal{O}})\otimes\mathbb{Z}_{2}.

(2) For a natural number nn, n\mathbb{Z}_{n} denotes the cyclic group (or the ring) /n\mathbb{Z}/n\mathbb{Z} of order nn, and (n)×(\mathbb{Z}_{n})^{\times} denotes the unit group of the ring /n\mathbb{Z}/n\mathbb{Z}.

(3) By a dihedral group, we mean a group generated by two elements of order 22. Thus it is isomorphic to the group Dn:=a,b|a2,b2,(ab)nD_{n}:=\langle a,b\,|\,a^{2},b^{2},(ab)^{n}\rangle for some n{}n\in\mathbb{N}\cup\{\infty\}. Note that DnD_{n} has order 2n2n or \infty according to whether nn\in\mathbb{N} or n=n=\infty. Note also that the order 22 cyclic group D1D_{1} is also regarded as a dihedral group.

Acknowledgement. M.S. would like to thank Ian Agol for sending the slide of his talk [2], encouraging him (and any of his collaborators) to write up the proof, and describing key ideas of the proof. He would also like to thank Michel Boileau for enlightening conversation in an early time. His sincere thanks also go to all the other authors for joining the project to give a proof to Agol’s announcement. J.P. would like to thank Sadayoshi Kojima for supporting his trip to Japan. H.A. was supported by JSPS Grants-in-Aid 19K03497. K.O. was supported by JSPS Grants-in-Aid 17H02843 and 18KK0071. M.S. was supported by JSPS Grants-in-Aid 15H03620.

2. Basic facts concerning 22-bridge links

In this section, we recall basic facts concerning 22-bridge links, which we use in the definitions of the Heckoid orbifolds and the Heckoid groups. The description of 22-bridge links given in this section is a mixture of those in [14, 51].

Let 𝒥{\mathcal{J}} be the group of isometries of the Euclidean plane 2\mathbb{R}^{2} generated by the π\pi-rotations around the points in 2\mathbb{Z}^{2}. Set (𝑺2,𝑷0)=(2,2)/𝒥(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0})=(\mathbb{R}^{2},\mathbb{Z}^{2})/{\mathcal{J}} and call it the Conway sphere. Then 𝑷0\mbox{{\boldmath$P$}}^{0} consists of four points in the 22-sphere 𝑺2\mbox{\boldmath$S$}^{2}. Let 𝑺ˇ2:=𝑺2𝑷0\check{\mbox{\boldmath$S$}}^{2}:=\mbox{\boldmath$S$}^{2}-\mbox{{\boldmath$P$}}^{0} be the complementary 44-times punctured sphere. For each s{}s\in\mathbb{Q}\cup\{\infty\}, let αs\alpha_{s} as be the simple loop in 𝑺ˇ2\check{\mbox{\boldmath$S$}}^{2} obtained as the projection of a line in 22\mathbb{R}^{2}-\mathbb{Z}^{2} of slope ss. Then αs\alpha_{s} is essential in 𝑺ˇ2\check{\mbox{\boldmath$S$}}^{2}, i.e., it does not bound a disc nor a once-punctured disc in 𝑺ˇ2\check{\mbox{\boldmath$S$}}^{2}. Conversely, any essential simple loop in 𝑺ˇ2\check{\mbox{\boldmath$S$}}^{2} is isotopic to αs\alpha_{s} for a unique s{}s\in\mathbb{Q}\cup\{\infty\}: we call ss the slope of the essential loop. For each s{}s\in\mathbb{Q}\cup\{\infty\}, let δs\delta_{s} be the pair of mutually disjoint arcs in 𝑺2\mbox{\boldmath$S$}^{2} with δs=𝑷0\partial\delta_{s}=\mbox{{\boldmath$P$}}^{0}, obtained as the image of the union of the lines in 2\mathbb{R}^{2} which intersect 2\mathbb{Z}^{2}. Note that the union δ0/1δ1/0\delta_{0/1}\cup\delta_{1/0} is a circle in 𝑺2\mbox{\boldmath$S$}^{2} containing 𝑷0\mbox{{\boldmath$P$}}^{0}, which divides 𝑺2\mbox{\boldmath$S$}^{2} into two discs 𝑺+2:=pr([0,1]×[0,1])\mbox{\boldmath$S$}^{2}_{+}:=pr([0,1]\times[0,1]) and 𝑺2:=pr([1,2]×[0,1])\mbox{\boldmath$S$}^{2}_{-}:=pr([1,2]\times[0,1]), where pr:2𝑺2pr:\mathbb{R}^{2}\to\mbox{\boldmath$S$}^{2} is the projection.

Refer to caption
Figure 2. Conway sphere (𝑺2,𝑷0)=(2,2)/𝒥(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0})=(\mathbb{R}^{2},\mathbb{Z}^{2})/{\mathcal{J}} and the homeomorphism θ:(𝑺2,𝑷0)(𝑩3,𝑷0)\theta:(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0})\to(\partial\mbox{\boldmath$B$}^{3},\mbox{\boldmath$P$}^{0})

Let 𝑩3:={(x,y,z)3|x2+y2+z22}\mbox{\boldmath$B$}^{3}:=\{(x,y,z)\in\mathbb{R}^{3}\,|\,x^{2}+y^{2}+z^{2}\leq 2\} be the round 33-ball in 33{}S3\mathbb{R}^{3}\subset\mathbb{R}^{3}\cup\{\infty\}\cong S^{3}, whose boundary contains the set P0P^{0} consisting of the four marked points

SW:=(1,1,0),SE:=(1,1,0),NE:=(1,1,0),NW:=(1,1,0).\mbox{$\mathrm{SW}$}:=(-1,-1,0),\quad\mbox{$\mathrm{SE}$}:=(1,-1,0),\quad\mbox{$\mathrm{NE}$}:=(1,1,0),\quad\mbox{$\mathrm{NW}$}:=(-1,1,0).

Fix a homeomorphism θ:(𝑺2,𝑷0)(𝑩3,P0)\theta:(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0})\to(\partial\mbox{\boldmath$B$}^{3},P^{0}) satisfying the following conditions (see Figure 2).

  1. (1)

    θ\theta maps the quadruple (pr(0,0),pr(1,0),pr(1,1),pr(0,1))(pr(0,0),pr(1,0),pr(1,1),pr(0,1)) to the quadruple (SW,SE,NE,NW)(\mbox{$\mathrm{SW}$},\mbox{$\mathrm{SE}$},\mbox{$\mathrm{NE}$},\mbox{$\mathrm{NW}$}).

  2. (2)

    θ\theta maps the circle δ0/1δ1/0\delta_{0/1}\cup\delta_{1/0} to the equatorial circle 𝑩3(2×{0})\partial\mbox{\boldmath$B$}^{3}\cap(\mathbb{R}^{2}\times\{0\}), and maps the hemispheres 𝑺+2\mbox{\boldmath$S$}^{2}_{+} and 𝑺2\mbox{\boldmath$S$}^{2}_{-} onto the hemispheres 𝑩3(2×0)\partial\mbox{\boldmath$B$}^{3}\cap(\mathbb{R}^{2}\times\mathbb{R}_{\geq 0}) to 𝑩3(2×0)\partial\mbox{\boldmath$B$}^{3}\cap(\mathbb{R}^{2}\times\mathbb{R}_{\leq 0}), respectively.

  3. (3)

    θ\theta is equivariant with respect to the natural (2)2(\mathbb{Z}_{2})^{2}-actions on (𝑺2,𝑷0)(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0}) and (𝑩3,P0)(\partial\mbox{\boldmath$B$}^{3},P^{0}). Here the natural (2)2(\mathbb{Z}_{2})^{2}-action on (𝑺2,𝑷0)(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0}) is that which lifts to the group of isometries of the Euclidean plane 2\mathbb{R}^{2} generated by the π\pi-rotations around the points in (12)2(\frac{1}{2}\mathbb{Z})^{2}, and the natural (2)2(\mathbb{Z}_{2})^{2}-action on (𝑩3,P0)(\partial\mbox{\boldmath$B$}^{3},P^{0}) is that generated by the π\pi-rotations about the coordinate axes of 3\mathbb{R}^{3}.

We identify (𝑩3,P0)(\partial\mbox{\boldmath$B$}^{3},P^{0}) with (𝑺2,𝑷0)(\mbox{\boldmath$S$}^{2},\mbox{\boldmath$P$}^{0}) through the homeomorphism θ\theta. Thus for s{}s\in\mathbb{Q}\cup\{\infty\}, αs\alpha_{s} is regarded as an essential simple loop in 𝑩3P0\partial\mbox{\boldmath$B$}^{3}-P^{0}, and δs\delta_{s} is regarded as a union of two disjoint arcs in 𝑩3\partial\mbox{\boldmath$B$}^{3} such that δs=P0\partial\delta_{s}=P^{0}. Moreover, we can choose αs\alpha_{s} and δs\delta_{s} so that they are (2)2(\mathbb{Z}_{2})^{2}-invariant.

For a rational number r=q/p{}r=q/p\in\mathbb{Q}\cup\{\infty\}, let t(r)t(r) be a pair of arcs properly embedded in 𝑩3\mbox{\boldmath$B$}^{3} such that t(r)𝑩3=t(r)=P0t(r)\cap\partial\mbox{\boldmath$B$}^{3}=\partial t(r)=P^{0}, which is obtained from δr\delta_{r} by pushing its interior into int𝑩3\operatorname{int}\mbox{\boldmath$B$}^{3}. The pair (𝑩3,t(r))(\mbox{\boldmath$B$}^{3},t(r)) is called the rational tangle of slope rr. We may assume t(r)t(r) is invariant by the natural (2)2(\mathbb{Z}_{2})^{2}-action on 𝑩3\mbox{\boldmath$B$}^{3}. In particular, the xx-axis intersects t(r)t(r) transversely in two points: Let τr\tau_{r} be the subarc of the xx-axis they bound, and call it the core tunnel of (𝑩3,t(r))(\mbox{\boldmath$B$}^{3},t(r)) (see Figure 4). Two meridional circles of t(r)t(r) near τr\partial\tau_{r} together with a subarc of τr\tau_{r} forms a graph in 𝑩3t(r)\mbox{\boldmath$B$}^{3}-t(r) homeomorphic to a pair of eyeglasses. This determines a canonical generating meridian pair of the rank 22 free group π1(𝑩3t(r))π1(𝑺ˇ2)/αr\pi_{1}(\mbox{\boldmath$B$}^{3}-t(r))\cong\pi_{1}(\check{\mbox{\boldmath$S$}}^{2})/\langle\langle\alpha_{r}\rangle\rangle.

By gluing the boundaries of the rational tangles (𝑩3,t())(\mbox{\boldmath$B$}^{3},t(\infty)) and (𝑩3,t(r))(\mbox{\boldmath$B$}^{3},t(r)) by the identity map, we obtain a link in the 33-sphere: we denote it by (S3,K(r))(S^{3},K(r)), and call it the 22-bridge link of slope r=q/pr=q/p. The number of components, |K(r)||K(r)|, of K(r)K(r) is one or two (i.e., K(r)K(r) is a knot or a two-component link) according to whether the denominator pp is odd or even. The images of the core tunnels τ\tau_{\infty} and τr\tau_{r} in (S3,K(r))(S^{3},K(r)) are called the upper tunnel and the lower tunnel of K(r)K(r), respectively. We denote them by τ+\tau_{+} and τ\tau_{-}, respectively. The canonical generating meridian pairs of π1(𝑩3t())\pi_{1}(\mbox{\boldmath$B$}^{3}-t(\infty)) and π1(𝑩3t(r))\pi_{1}(\mbox{\boldmath$B$}^{3}-t(r)) descend to generating meridian pairs of the link group π1(S3K(r))π1(𝑺ˇ2)/α,αr\pi_{1}(S^{3}-K(r))\cong\pi_{1}(\check{\mbox{\boldmath$S$}}^{2})/\langle\langle\alpha_{\infty},\alpha_{r}\rangle\rangle: we call them the upper meridian pair and the lower meridian pair, respectively.

When we need to care about the orientation of the ambient 33-sphere S3S^{3}, we regard (S3,K(r))(S^{3},K(r)) as being obtained from (𝑩3,t())(-\mbox{\boldmath$B$}^{3},t(\infty)) and (𝑩3,t(r))(\mbox{\boldmath$B$}^{3},t(r)), where 𝑩3\mbox{\boldmath$B$}^{3} inherits the standard orientation of 3\mathbb{R}^{3}. In other words, we identify the ambient 33-sphere S3S^{3} with the one-point compactification 3{}\mathbb{R}^{3}\cup\{\infty\} of 3\mathbb{R}^{3}, in such a way that the 𝑩3\mbox{\boldmath$B$}^{3} containing t(r)t(r) is identified with the original round ball 𝑩3\mbox{\boldmath$B$}^{3} via the identity map, whereas the 𝑩3\mbox{\boldmath$B$}^{3} containing t()t(\infty) is identified with cl(3{}𝑩3)\operatorname{cl}(\mathbb{R}^{3}\cup\{\infty\}-\mbox{\boldmath$B$}^{3}) via the inversion ι\iota in 𝑩3\partial\mbox{\boldmath$B$}^{3}. Thus K(r)=t(r)ι(t())3{}=S3K(r)=t(r)\cup\iota(t(\infty))\subset\mathbb{R}^{3}\cup\{\infty\}=S^{3}. Under this orientation convention, a regular projection is read from the continued fraction expansion

r=[a1,a2,,an]=1a1+1a2++1an,\displaystyle{r=[a_{1},a_{2},\cdots,a_{n}]=\cfrac{1}{a_{1}+\cfrac{1}{\raisebox{-5.0pt}[0.0pt][0.0pt]{$a_{2}\,+\,$}\raisebox{-10.0pt}[0.0pt][0.0pt]{$\,\ddots\ $}\raisebox{-12.0pt}[0.0pt][0.0pt]{$+\,\cfrac{1}{a_{n}}$}}}\ ,}

in such a way that aia_{i} corresponds to the aia_{i} right-hand or left-hand half-twists according to whether ii is odd or even (see Figure 3).

Refer to caption
Figure 3. 22-bridge link diagram

The natural (2)2(\mathbb{Z}_{2})^{2}-actions on (𝑩3,t())(\mbox{\boldmath$B$}^{3},t(\infty)) and (𝑩3,t(r))(\mbox{\boldmath$B$}^{3},t(r)) can be glued to produce a (2)2(\mathbb{Z}_{2})^{2}-action on (S3,K(r))(S^{3},K(r)). Let ff and hh be the generators of the action whose restrictions to (𝑩3,t()))(\mbox{\boldmath$B$}^{3},t(\infty))) are the π\pi-rotations about the yy-axis and xx-axis, respectively (see Figure 4). We call ff, hh, and fhfh, respectively, the vertical involution, the horizontal involution, and the planar involution of K(r)K(r). They are characterized by the following properties.

  1. (1)

    Fix(h)\operatorname{Fix}(h) contains τ+\tau_{+}, whereas each of Fix(f)\operatorname{Fix}(f) and Fix(fh)\operatorname{Fix}(fh) intersects τ+\tau_{+} transversely in a single point.

  2. (2)

    The horizontal simple loop α0\alpha_{0} in (𝑩3t())\partial(\mbox{\boldmath$B$}^{3}-t(\infty)) is mapped by ff to itself preserving orientation, and it is mapped by fhfh to itself reversing orientation.

Refer to caption
Figure 4. Natural (2)2(\mathbb{Z}_{2})^{2}-actions on (𝑩3,t())(\mbox{\boldmath$B$}^{3},t(\infty)) consisting of the vertical involution ff, the horizontal involution hh, and the planar involution fhfh

If the rational number r=q/pr=q/p satisfies the congruence q21(modp)q^{2}\equiv 1\pmod{p}, then K(r)K(r) admits an additional orientation-preserving symmetry which interchanges (𝑩3,t())(\mbox{\boldmath$B$}^{3},t(\infty)) and (𝑩3,t(r))(\mbox{\boldmath$B$}^{3},t(r)). For a description of such symmetries, see e.g. [4, Sections 4 and 6], [49, Section 3].

We finally recall the classification theorem for 22-bridge links due to Schubert [53] (cf. [17, Chapter 12]).

Proposition 2.1.

For two rational numbers r=q/pr=q/p and r=q/pr^{\prime}=q^{\prime}/p^{\prime}, with pp and pp^{\prime} positive, the following holds.

(1) There is an orientation-preserving auto-homeomorphism φ\varphi of S3S^{3} which maps K(r)K(r) to K(r)K(r^{\prime}) if and only if p=pp=p^{\prime} and either qq(modp)q\equiv q^{\prime}\pmod{p} or qq1(modp)qq^{\prime}\equiv 1\pmod{p}. Moreover the following hold.

  1. (a)

    If p=pp=p^{\prime} and qq(modp)q\equiv q^{\prime}\pmod{p}, then there there is an orientation-preserving auto-homeomorphism φ\varphi of S3S^{3} which maps (K(r),τ+,τ)(K(r),\tau_{+},\tau_{-}) to (K(r),τ+,τ)(K(r^{\prime}),\tau_{+},\tau_{-}) and respects the (2)2(\mathbb{Z}_{2})^{2}-action. Moreover, the conjugate of the vertical involution of K(r)K(r) by φ\varphi is either the vertical or planar involution of K(r)K(r^{\prime}), according to whether qq(mod2p)q^{\prime}\equiv q\pmod{2p} or qq+p(mod2p)q^{\prime}\equiv q+p\pmod{2p}.

  2. (b)

    If p=pp=p^{\prime} and qq1(modp)qq^{\prime}\equiv 1\pmod{p}, then there there is an orientation-preserving auto-homeomorphism of S3S^{3} which maps (K(r),τ+,τ)(K(r),\tau_{+},\tau_{-}) to (K(r),τ,τ+)(K(r^{\prime}),\tau_{-},\tau_{+}) which respects the (2)2(\mathbb{Z}_{2})^{2}-action.

(2) There is an orientation-reversing auto-homeomorphism φ\varphi of S3S^{3} which maps K(r)K(r) to K(r)K(r^{\prime}) if and only if p=pp=p^{\prime} and either qq(modp)q\equiv-q^{\prime}\pmod{p} or qq1(modp)qq^{\prime}\equiv-1\pmod{p}.

3. Heckoid orbifolds and Heckoid groups

In this section, we recall the definition of Heckoid orbifolds and Heckoid groups given by [32, Section 3].

Consider the quotient orbifold (𝑩3t())/(2)2(\mbox{\boldmath$B$}^{3}-t(\infty))/(\mathbb{Z}_{2})^{2}, where (2)2(\mathbb{Z}_{2})^{2} is the natural action illustrated in Figure 4. Note that its boundary is identified with 𝑺ˇ2/(2)2S2(2,2,2,)\check{\mbox{\boldmath$S$}}^{2}/(\mathbb{Z}_{2})^{2}\cong S^{2}(2,2,2,\infty), which is the quotient of 22\mathbb{R}^{2}-\mathbb{Z}^{2} by the group generated by the π\pi-rotations around the points in (12)2(\frac{1}{2}\mathbb{Z})^{2}. Note that π1(𝑺ˇ2)\pi_{1}(\check{\mbox{\boldmath$S$}}^{2}) is identified with a normal subgroup of π1(𝑺ˇ2/(2)2)\pi_{1}(\check{\mbox{\boldmath$S$}}^{2}/(\mathbb{Z}_{2})^{2}) of index 44. For each s{}s\in\mathbb{Q}\cup\{\infty\}, let βs\beta_{s} be the simple loop in 𝑺ˇ2/(2)2\check{\mbox{\boldmath$S$}}^{2}/(\mathbb{Z}_{2})^{2} obtained as the projection of a line in 2(12)2\mathbb{R}^{2}-(\frac{1}{2}\mathbb{Z})^{2} of slope ss. The simple loop αs\alpha_{s} in 𝑺ˇ2\check{\mbox{\boldmath$S$}}^{2} doubly covers βs\beta_{s}, and so we have αs=βs2\alpha_{s}=\beta_{s}^{2} as conjugacy classes in π1(𝑺ˇ2/(2)2)\pi_{1}(\check{\mbox{\boldmath$S$}}^{2}/(\mathbb{Z}_{2})^{2}).

For rr\in\mathbb{Q} and m3m\in\mathbb{N}_{\geq 3}, consider the 33-orbifold 𝑩(;2):=cl(𝑩3N(t))/(2)2\mbox{\boldmath$B$}(\infty;2):=\operatorname{cl}(\mbox{\boldmath$B$}^{3}-N(t_{\infty}))/(\mathbb{Z}_{2})^{2}, attach a 2-handle orbifold D2(m)×ID^{2}(m)\times I to it along the simple loop βr\beta_{r}. Since βr\beta_{r} divides 𝑺ˇ2/(2)2S2(2,2,2,)\check{\mbox{\boldmath$S$}}^{2}/(\mathbb{Z}_{2})^{2}\cong S^{2}(2,2,2,\infty) into D2(2,2)D^{2}(2,2) and D2(2,)D^{2}(2,\infty), the resulting 33-orbifold has a spherical boundary S2(2,2,m)S2/DmS^{2}(2,2,m)\cong S^{2}/D_{m}, where DmD_{m} is the dihedral group of order 2m2m (cf. Notation 1.3(3)). Cap this spherical boundary with the 33-handle orbifold B3(2,2,m)B3/DmB^{3}(2,2,m)\cong B^{3}/D_{m}, and denote the resulting 33-orbifold by (r;m)\mathcal{H}(r;m). (Though this orbifold was denoted by 𝒪(r;m){\mathcal{O}}(r;m) in [32], we employ this symbol, because we use the symbol 𝒪{\mathcal{O}} to mainly denote spherical dihedral orbifolds.) Then we have

π1((r;m))π1(S2(2,2,2,))/β2,βrm.\pi_{1}(\mathcal{H}(r;m))\cong\pi_{1}(S^{2}(2,2,2,\infty))/\langle\langle\beta_{\infty}^{2},\beta_{r}^{m}\rangle\rangle.

Let PP be the annular orbifold frN(t)/(2)2D2(2,2)\operatorname{fr}N(t_{\infty})/(\mathbb{Z}_{2})^{2}\cong D^{2}(2,2) on (r;m)\partial\mathcal{H}(r;m), and continue to denote the orbifold pair ((r;m),P)(\mathcal{H}(r;m),P) by the symbol (r;m)\mathcal{H}(r;m).

In [32, Section 6], it is proved that the orbifold pair (r;m)\mathcal{H}(r;m) is a pared 33-orbifold (see [10, Definition 8.3.7]).

Definition 3.1.

An orbifold pair (M0,P)(M_{0},P) is a pared 33-orbifold if it satisfies the following conditions

  1. (1)

    M0M_{0} is a compact, orientable, irreducible 33-orbifold which is very good (i.e., M0M_{0} has a finite manifold cover).

  2. (2)

    PM0P\subset\partial M_{0} is a disjoint union of incompressible toric and annular 22-suborbifolds.

  3. (3)

    Every rank 22 free abelian subgroup of π1(M0)\pi_{1}(M_{0}) is conjugate to a subgroup of some π1(Pi)\pi_{1}(P_{i}), where PiPP_{i}\subset P is a connected component.

  4. (4)

    Any properly embedded annular 22-suborbifold (A,A)(A,\partial A) of (M0,P)(M_{0},P) whose boundary rests on essential loops in PP is parallel to PP.

It is also observed in [32, Section 6] that (r;m)=((r;m),P)\mathcal{H}(r;m)=(\mathcal{H}(r;m),P) is a Haken pared orbifold (see [10, Definitions 8.0.1 and 8.3.7]). Hence, by the hyperbolization theorem of Haken pared orbifolds [10, Theorem 8.3.9], the pared orbifold (r;m)\mathcal{H}(r;m) admits a geometrically finite complete hyperbolic structure, namely, the interior of the orbifold (r;m)\mathcal{H}(r;m) admits a geometrically finite complete hyperbolic structure such that PP represents the parabolic locus (see Section 5 for definitions).

Moreover, such a hyperbolic structure is unique, because the ends of the non-cuspidal part of (r;m)\mathcal{H}(r;m) are isomorphic to (aturnover)×[0,)(\mathrm{a\ turnover})\times[0,\infty), which are quasi-isometrically rigid, and every orbifold homeomorphism between two geometrically finite structures preserving the parabolicity in both directions is isotopic to a quasi-isometry, as can be seen by the same argument as Marden’s theorem [34]. We denote the unique (up to conjugation) Kleinian group that uniformises the pared orbifold (r;m)\mathcal{H}(r;m) by the symbol π1((r;m))\pi_{1}(\mathcal{H}(r;m)).

Now the Heckoid groups and the Heckoid orbifolds are defined as follows [32, p.242 and Definition 3.2].

Definition 3.2.

For rr\in\mathbb{Q} and n=m2123n=\frac{m}{2}\in\frac{1}{2}\mathbb{N}_{\geq 3}, the Heckoid group G(r;n)G(r;n) of slope rr and index nn is the Kleinian group that is obtained as the image of the natural homomorphism

ψ:π1(cl(𝑩3N(t)))π1(cl(𝑩3N(t))/(2)2)π1((r;m))<PSL(2,).\psi:\pi_{1}(\operatorname{cl}(\mbox{\boldmath$B$}^{3}-N(t_{\infty})))\to\pi_{1}(\operatorname{cl}(\mbox{\boldmath$B$}^{3}-N(t_{\infty}))/(\mathbb{Z}_{2})^{2})\to\pi_{1}(\mathcal{H}(r;m))<\mbox{$\mathrm{PSL}$}(2,\mathbb{C}).

The Heckoid orbifold 𝒮(r;n)\mathcal{S}(r;n) of slope rr and index nn is the pared orbifold, that is obtained as the covering of the pared orbifold (r;m)\mathcal{H}(r;m) associated with the subgroup G(r;n)<π1((r;m))G(r;n)<\pi_{1}(\mathcal{H}(r;m)). We also denote the Kleinian group G(r;n)G(r;n) by π1(𝒮(r;n))\pi_{1}(\mathcal{S}(r;n)).

Then we have the following proposition. (The main Theorem 1.1 implies that the converse to the first assertion of the proposition holds.)

Proposition 3.3.

For any rr\in\mathbb{Q} and n=m2123n=\frac{m}{2}\in\frac{1}{2}\mathbb{N}_{\geq 3}, the Heckoid group is a (non-free) Kleinian group with nontrivial torsion which is generated by two non-commuting parabolic transformations. Moreover, the image of the conjugacy class of the simple loop αr\alpha_{r} in G(r;n)G(r;n) is an elliptic transformation of rotation angle 2πn=4πm\frac{2\pi}{n}=\frac{4\pi}{m}.

Proof.

Let {x,y}\{x,y\} be the canonical generating meridian pair of the rank 22 free group π1(cl(𝑩3N(t)))\pi_{1}(\operatorname{cl}(\mbox{\boldmath$B$}^{3}-N(t_{\infty}))) (see Section 2). Then G(r;n)G(r;n) is generated by the image {ψ(x),ψ(y)}π1((r;m))\{\psi(x),\psi(y)\}\subset\pi_{1}(\mathcal{H}(r;m)). Since π1((r;m))\pi_{1}(\mathcal{H}(r;m)) is the Kleinian group which uniformises the pared orbifold (r;m)\mathcal{H}(r;m), the generating pair of G(r;n)G(r;n) consists of non-commuting parabolic transformations. Since αr=βr2\alpha_{r}=\beta_{r}^{2} and since βr\beta_{r} is a meridian of the singular set of (r;n)\mathcal{H}(r;n) of index 2n=m2n=m, it follows that ψ(αr)\psi(\alpha_{r}) is an elliptic transformation of rotation angle 2πn=4πm\frac{2\pi}{n}=\frac{4\pi}{m}. ∎

Next, we recall the topological description of the Heckoid orbifolds. In Definition 3.2, the Heckoid orbifold 𝒮(r;n)\mathcal{S}(r;n) is defined as a covering of the pared orbifold (r;m)\mathcal{H}(r;m). Their explicit topological description is given by [32, Propositions 5.2 and 5.3], which says that the Heckoid orbifold 𝒮(r;n)\mathcal{S}(r;n) is isomorphic to one of the orbifold pairs depicted in Figure 1, that is specified by the following formula.

𝒮(r;n){0(r;n)if n2,1(r^;m)if n=m/2 for some odd m>2 and if p is odd,2(r^;m)if n=m/2 for some odd m>2 and if p is even,\displaystyle\mathcal{S}(r;n)\cong\begin{cases}\mathcal{M}_{0}(r;n)&\text{if $n\in\mathbb{N}_{\geq 2}$,}\\ \mathcal{M}_{1}(\hat{r};m)&\text{if $n=m/2$ for some odd $m>2$ and if $p$ is odd,}\\ \mathcal{M}_{2}(\hat{r};m)&\text{if $n=m/2$ for some odd $m>2$ and if $p$ is even,}\\ \end{cases}

where r^\hat{r} is defined from r=q/pr=q/p by the following rule.

r^={q/2pif p is odd and q is even,(p+q)/2pif p is odd and q is odd,qp/2if p is even.\hat{r}=\begin{cases}\frac{q/2}{p}&\text{if $p$ is odd and $q$ is even,}\\ \frac{(p+q)/2}{p}&\text{if $p$ is odd and $q$ is odd,}\\ \frac{q}{p/2}&\text{if $p$ is even.}\end{cases}

Thus the following precise definition of the orbifold pairs in Figure 1 gives an explicit topological picture of the Heckoid orbifold 𝒮(r;n)\mathcal{S}(r;n).

Definition 3.4.

(1) For rr\in\mathbb{Q} and for a positive integer n2n\geq 2, 0(r;n)\mathcal{M}_{0}(r;n) denotes the orbifold pair determined by the weighted graph (S3,K(r)τ,w0)(S^{3},K(r)\cup\tau_{-},w_{0}), where w0w_{0} is given by

w0(K(r))=,w0(τ)=n.w_{0}(K(r))=\infty,\quad w_{0}(\tau_{-})=n.

(2) For r=q/pr=q/p\in\mathbb{Q} with pp odd and an odd integer m3m\geq 3, 1(r;m)\mathcal{M}_{1}(r;m) denotes the orbifold pair determined by the weighted graph (S3,K(r)τ,w1)(S^{3},K(r)\cup\tau_{-},w_{1}), where w1w_{1} is given by the following rule. Let J1J_{1} and J2J_{2} be the edges of the graph K(r)τK(r)\cup\tau_{-} distinct from τ\tau_{-}. Then

w1(J1)=,w1(J2)=2,w1(τ)=m.w_{1}(J_{1})=\infty,\quad w_{1}(J_{2})=2,\quad w_{1}(\tau_{-})=m.

(3) For r=q/pr=q/p\in\mathbb{Q} and an odd integer m3m\geq 3, 2(r;m)\mathcal{M}_{2}(r;m) denotes the orbifold pair determined by the weighted graph (S3,K(r)τ+τ,w2)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},w_{2}), where w2w_{2} is given by the following rule. Let J1J_{1} and J2J_{2} be unions of two mutually disjoint edges of the graph K(r)τ+τK(r)\cup\tau_{+}\cup\tau_{-} distinct from τ±\tau_{\pm}. Moreover, if pp is even, then both J1J_{1} and J2J_{2} are preserved by the vertical involution ff of K(r)K(r). (Thus ff interchanges the two components of each of J1J_{1} and J2J_{2}.) Then

w2(J1)=,w2(J2)=2,w2(τ+)=2,w2(τ)=m.w_{2}(J_{1})=\infty,\quad w_{2}(J_{2})=2,\quad w_{2}(\tau_{+})=2,\quad w_{2}(\tau_{-})=m.

In Defunition 3.4(3), the ‘identity’ w2(J1)=w_{2}(J_{1})=\infty means that w2(e)=w_{2}(e)=\infty for each edge ee contained in J1J_{1}. Similarly, w2(J2)=2w_{2}(J_{2})=2 means that w2(e)=2w_{2}(e)=2 for each edge ee contained in J2J_{2}. We employ this kind of convention throughout the paper.

Remark 3.5.

(1) Because of the (2)2(\mathbb{Z}_{2})^{2}-symmetry of 22-bridge links, the choice of the edges J1J_{1} and J2J_{2} in (2) and (3) does not affect the isomorphism class of the resulting orbifolds (see [32, Remark 5.4]).

(2) Suppose pp is odd. Then, in the definition of 2(r;m)\mathcal{M}_{2}(r;m), the disjointness condition of J1J_{1} and J2J_{2} determines the pair (J1,J2)(J_{1},J_{2}) up to the horizontal involution hh of (S3,K(r)τ+τ)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-}). Moreover, according to whether qq is odd or even, both J1J_{1} and J2J_{2} are preserved by ff or fhfh, respectively (see Figure 5(1),(2)).

(3) Suppose pp is even. Then, in the definition of 2(r;m)\mathcal{M}_{2}(r;m), the condition that both J1J_{1} and J2J_{2} are preserved by ff is not essential in the following sense. Let Ji,1J_{i,1} and Ji,2J_{i,2} be the components of JiJ_{i} for i=1,2i=1,2, such that J1,1J2,1=J_{1,1}\cap J_{2,1}=\emptyset and J1,2J2,2=J_{1,2}\cap J_{2,2}=\emptyset. Set J1=J1,1J2,1J_{1}^{\prime}=J_{1,1}\cup J_{2,1} and J2=J1,2J2,2J_{2}^{\prime}=J_{1,2}\cup J_{2,2}. Then J1J_{1}^{\prime} and J2J_{2}^{\prime} are unions of two mutually disjoint edges of the graph K(r)τ+τK(r)\cup\tau_{+}\cup\tau_{-} distinct from τ±\tau_{\pm}, such that both J1J_{1}^{\prime} and J2J_{2}^{\prime} are preserved by the planar involution fhfh, instead of the vertical involution ff (see Figure 5(3),(4)). Let w2w_{2}^{\prime} be the weight function on the graph K(r)τ+τK(r)\cup\tau_{+}\cup\tau_{-} defined by

w2(J1)=,w2(J2)=2,w2(τ+)=2,w2(τ)=m.w_{2}^{\prime}(J_{1}^{\prime})=\infty,\quad w_{2}^{\prime}(J_{2}^{\prime})=2,\quad w_{2}^{\prime}(\tau_{+})=2,\quad w_{2}^{\prime}(\tau_{-})=m.

Then (S3,K(r)τ+τ,w2)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},w_{2}^{\prime}) represents the orbifold 2(r;m)\mathcal{M}_{2}(r^{\prime};m), where r=(p+q)/pr^{\prime}=(p+q)/p for r=q/pr=q/p. This follows from the fact that there is a homeomorphism from (S3,K(r)τ+τ)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-}) to (S3,K(r)τ+τ)(S^{3},K(r^{\prime})\cup\tau_{+}\cup\tau_{-}) sending (τ±,J1,J2)(\tau_{\pm},J_{1},J_{2}) to (τ±,J1,J2)(\tau_{\pm},J_{1}^{\prime},J_{2}^{\prime}) (see Proposition 2.1(1a)).

Refer to caption
Figure 5. The first two figures (1) and (2) illustrate Remark 3.5(2), and the last two figures (3) and (4) illustrate Remark 3.5(3). See also [4, Figures in Section 7].

4. Classification of dihedral orbifolds

In this section, we give a classification of the dihedral orbifolds, which plays a key role in the proof of the main theorem. We refer to [8, 9, 19] for standard terminologies for orbifolds.

By using the the orbifold theorem, the geometrisation theorem of compact orientable 33-manifolds, and the classification of geometric dihedral orbifolds (see Appendix), we obtain the following classification of good orbifolds with dihedral orbifold fundamental groups.

Theorem 4.1.

Let 𝒪{\mathcal{O}} be a compact orientable 33-orbifold with nonempty singular set satisfying the following conditions.

  1. (i)

    𝒪{\mathcal{O}} does not contain a bad 22-suborbifold.

  2. (ii)

    Any component of 𝒪\partial{\mathcal{O}} is not spherical.

  3. (iii)

    π1(𝒪)\pi_{1}({\mathcal{O}}) is a dihedral group.

Then 𝒪{\mathcal{O}} is isomorphic to one of the following orbifolds.

  1. (1)

    The spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) represented by the weighted graph (S3,K(r)τ+τ,w)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},w) for some rr\in\mathbb{Q} and coprime positive integers d+d_{+} and dd_{-}, where ww is given by the following rule (see Figure 6).

    w(K(r))=2,w(τ+)=d+,w(τ)=d.w(K(r))=2,\quad w(\tau_{+})=d_{+},\quad w(\tau_{-})=d_{-}.
  2. (2)

    The S2×S^{2}\times\mathbb{R} orbifold 𝒪(){\mathcal{O}}(\infty) represented by the weighted graph (S3,K(),w)(S^{3},K(\infty),w), where ww takes the value 22 at each component of the 22-bridge link K()K(\infty) of slope \infty, i.e. the 22-component trivial link.

  3. (3)

    The S2×S^{2}\times\mathbb{R} orbifold 𝒪(3,O){\mathcal{O}}(\mathbb{RP}^{3},O) represented by the weighted graph (3,O,w)(\mathbb{RP}^{3},O,w), where OO is the trivial knot in the projective 33-space 3\mathbb{RP}^{3} with w(O)=2w(O)=2.

  4. (4)

    The orbifold D2(2,2)×ID^{2}(2,2)\times I.

Remark 4.2.

For the orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}), if d+=1d_{+}=1 (resp. d=1d_{-}=1), then τ+\tau_{+} (resp. τ\tau_{-}) does not belong to the singular set (cf. Convention 6.2(1)). In particular, 𝒪(r):=𝒪(r;1,1){\mathcal{O}}(r):={\mathcal{O}}(r;1,1) is the π\pi-orbifold associated with the 22-bridge link K(r)K(r) in the sense of [11], i.e. the orbifold with underlying space S3S^{3} and with singular set K(r)K(r), whose index is 22. In Adam’s classification of torsion-free Kleinian groups generated by two parabolic transformations [1, Theorem 4.3], the π\pi-orbifolds 𝒪(r){\mathcal{O}}(r) played a key role, whereas the orbifolds 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) play the corresponding key role in this paper.

Refer to caption
Figure 6. The spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-})
Proof.

Let 𝒪{\mathcal{O}} be a 33-orbifold satisfying the three conditions. We first treat the case where 𝒪{\mathcal{O}} is irreducible, i.e., any spherical 22-suborbifold of 𝒪{\mathcal{O}} bounds a discal 33-suborbifold (a quotient of a 33-ball by a finite orthogonal group). We can observe that 𝒪{\mathcal{O}} is topologically atoroidal as follows. Suppose on the contrary that 𝒪{\mathcal{O}} contains an essential toric suborbifold FF. Then the inclusion map induces an injective homomorphism from π1(F)\pi_{1}(F) into π1(𝒪)\pi_{1}({\mathcal{O}}), as explained below. Since 𝒪{\mathcal{O}} does not contain a bad 22-suborbifold by the condition (i), 𝒪{\mathcal{O}} is very good, by [8, Corollary 1.3]. Thus by applying the equivariant loop theorem to the group action, π1(F)\pi_{1}(F) embeds into π1(𝒪)\pi_{1}({\mathcal{O}}) (see [9, Corollary 3.20]). This contradicts the fact that the dihedral group π1(𝒪)\pi_{1}({\mathcal{O}}) does not contain 2\mathbb{Z}^{2}.

Hence, by the orbifold theorem [8, Corollary 1.2], 𝒪{\mathcal{O}} is geometric, i.e., either int𝒪\operatorname{int}{\mathcal{O}} admits one of Thurston’s geometry or 𝒪{\mathcal{O}} is a discal 33-orbifold. The latter possibility does not happen by the assumption (ii), and so int𝒪\operatorname{int}{\mathcal{O}} admits one of Thurston’s geometry. If the geometry is S3S^{3}, then by Proposition 12.2, 𝒪{\mathcal{O}} is isomorphic to the orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) in (1). If the geometry is S2×S^{2}\times\mathbb{R}, then by Proposition 13.1, 𝒪{\mathcal{O}} is isomorphic to the orbifold 𝒪(){\mathcal{O}}(\infty) in (2) or the orbifold 𝒪(3,O){\mathcal{O}}(\mathbb{RP}^{3},O) in (3). (But this does not happen, because these orbifolds are reducible whereas we currently assume that 𝒪{\mathcal{O}} is irreducible.) If the geometry is one of the remaining 6 geometries, then by Proposition 13.2, 𝒪{\mathcal{O}} is isomorphic to the orbifold D2(2,2)×ID^{2}(2,2)\times I in (4).

Next, we treat the case when 𝒪{\mathcal{O}} is reducible. Note that 𝒪{\mathcal{O}} does not contain a non-separating spherical 22-suborbifold, because H1(𝒪)H_{1}({\mathcal{O}}) is finite. Thus we do not need to worry about the paradoxical problems concerning spherical splitting of 33-orbifolds pointed out by Petronio [43]. By [43, Theorems 0.1], there is a finite system of spherical 22-suborbifolds 𝒮\mathcal{S} such that (a) no component of 𝒪𝒮{\mathcal{O}}-\mathcal{S} is punctured discal (a discal 33-orbifold minus regular neighbourhoods of a finite set) and (b) all prime factors of 𝒪{\mathcal{O}} (the orbifolds obtained from the components of 𝒪𝒮{\mathcal{O}}-\mathcal{S} by capping the boundary components with discal orbifolds) are irreducible. It should be noted that some prime component may be a manifold, i.e., its branching locus is empty. By the geometrisation theorem of compact orientable 33-manifolds (see e.g. [7]) and the the geometrisation theorem of compact orientable 33-orbifolds (see e.g. [9, Theorem 3.27]), each prime component of 𝒪{\mathcal{O}} admits a canonical decomposition into geometric pieces by a family of essential toric 22-orbifolds. In particular, each prime factor has a nontrivial orbifold fundamental group. Since the only nontrivial free product decomposition of a dihedral group is the decomposition of the infinite dihedral group DD_{\infty} into the free product 22\mathbb{Z}_{2}*\mathbb{Z}_{2}, 𝒪{\mathcal{O}} is the connected sum (along a 22-sphere with empty branching set) of two irreducible 33-orbifolds 𝒪1{\mathcal{O}}_{1} and 𝒪2{\mathcal{O}}_{2}, such that π1(𝒪i)2\pi_{1}({\mathcal{O}}_{i})\cong\mathbb{Z}_{2}. Since 𝒪i{\mathcal{O}}_{i} is geometric, 𝒪i{\mathcal{O}}_{i} is isomorphic to (a) the discal 33-orbifold B3/2B^{3}/\mathbb{Z}_{2}, (b) the orbifold (S3,O,w)(S^{3},O,w), where OO is a trivial knot and w(O)=2w(O)=2, or (c) 3\mathbb{RP}^{3}. By condition (ii), 𝒪i{\mathcal{O}}_{i} cannot be a discal orbifold. Since 𝒪=𝒪1#𝒪2{\mathcal{O}}={\mathcal{O}}_{1}\#{\mathcal{O}}_{2} has nonempty ramification locus, at least one of 𝒪i{\mathcal{O}}_{i} is not isomorphic to 3\mathbb{RP}^{3}. Hence, 𝒪{\mathcal{O}} is isomorphic to the orbifold (S3,O,w)#(S3,O,w)𝒪()(S^{3},O,w)\#(S^{3},O,w)\cong{\mathcal{O}}(\infty) in (2) or the orbifold (S3,O,w)#3𝒪(3,O)(S^{3},O,w)\#\mathbb{RP}^{3}\cong{\mathcal{O}}(\mathbb{RP}^{3},O) in (3). ∎

Remark 4.3.

By considering the image of 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) by a π\pi-rotation about a horizontal axis in Figure 6, we can interchange the role of d+d_{+} and dd_{-}. To be precise, we can see from Proposition 2.1(1b) that 𝒪(q/p;d+,d)𝒪(q/p;d,d+){\mathcal{O}}(q/p;d_{+},d_{-})\cong{\mathcal{O}}(q^{\prime}/p;d_{-},d_{+}) if qq1(modp)qq^{\prime}\equiv 1\pmod{p}.

5. Relative tameness theorem for hyperbolic orbifolds

We first recall basic terminology for hyperbolic orbifolds, following [9, Chapter 6]. Let Γ\Gamma be a finitely generated Kleinian group and M=3/ΓM=\mathbb{H}^{3}/\Gamma the quotient hyperbolic orbifold. For a real number ϵ>0\epsilon>0, the ϵ\epsilon-thin part M(0,ϵ]M_{(0,\epsilon]} of MM is the set of all points xMx\in M such that d(x~,γx~)ϵd(\tilde{x},\gamma\tilde{x})\leq\epsilon for some lift x~\tilde{x} of xx to 3\mathbb{H}^{3} and some γΓ\gamma\in\Gamma of order >1/ϵ>1/\epsilon (including \infty). By the Margulis Lemma, there is a constant μ>0\mu>0, such that for any real number ϵ(0,μ]\epsilon\in(0,\mu], each component XX of M(0,ϵ]M_{(0,\epsilon]} is either a Margulis tube or a cuspidal end. Here a Margulis tube is a compact quotient of the rr-neighbourhood of a geodesic in 3\mathbb{H}^{3} by an elementary subgroup of Γ\Gamma which preserves the geodesic, and a cuspidal end is the quotient of a horoball in 3\mathbb{H}^{3} by an elementary parabolic subgroup of Γ\Gamma which preserves the horoball.

Topologically, a cuspidal end is a product F×[0,+)F\times[0,+\infty), where FF is a Euclidean 22-orbifold. Thus we have the following possibilities for FF.

  1. (1)

    FF is the open annulus S1×S^{1}\times\mathbb{R} or S2(2,2,)S^{2}(2,2,\infty), the quotient of S1×S^{1}\times\mathbb{R} by an involution.

  2. (2)

    FF is the torus T2T^{2} or S2(2,2,2,2)S^{2}(2,2,2,2), the quotient of T2T^{2} by an involution.

  3. (3)

    FF is S2(2,3,6)S^{2}(2,3,6), S2(2,4,4)S^{2}(2,4,4) or S2(3,3,3)S^{2}(3,3,3), the quotient of T2T^{2} by a finite cyclic group action of order 66, 44 or 33, respectively.

A cusp F×[0,+)F\times[0,+\infty) is said to be rigid if FS2(2,3,6)F\cong S^{2}(2,3,6), S2(2,4,4)S^{2}(2,4,4) or S2(3,3,3)S^{2}(3,3,3). Otherwise it is said to be flexible. It is well-known that a cusp F×[0,+)F\times[0,+\infty) is rigid if and only if the holonomy representation of the orbifold fundamental group π1(F×[0,+)\pi_{1}(F\times[0,+\infty) admits no nontrivial deformation (see [37, Proposition 1]).

Let M(0,ϵ]cuspM^{\mathrm{cusp}}_{(0,\epsilon]} be the union of the cuspidal ends of M(0,ϵ]M_{(0,\epsilon]}, and let M0:=MintM(0,ϵ]cuspM_{0}:=M-\operatorname{int}M^{\mathrm{cusp}}_{(0,\epsilon]} be the non-cuspidal part of MM. Then P:=M0P:=\partial M_{0} is a disjoint union of euclidean 22-orbifolds, and is called the parabolic locus of M0M_{0}. Note that MintM0M\cong\operatorname{int}M_{0} and that PP consists of (closed) toric orbifolds (closed 22-orbifolds obtained as quotients of the 22-dimensional torus) and open annular orbifolds (open 22-orbifolds obtained as quotients of the open annulus S1×S^{1}\times\mathbb{R}).

The following theorem is an orbifold version of (the relative version of) the tameness theorem established by Agol [2] and Calegari-Gabai [18] (see also Soma [55] and Bowditch [15]).

Theorem 5.1.

Let M=3/ΓM=\mathbb{H}^{3}/\Gamma be a hyperbolic 33-orbifold with finitely generated orbifold fundamental group Γ\Gamma. Then there is a compact 33-orbifold M¯0\bar{M}_{0} and a compact suborbifold P¯\bar{P} of M¯0\partial\bar{M}_{0}, such that (i) intM¯0=intM0M\operatorname{int}\bar{M}_{0}=\operatorname{int}M_{0}\cong M and (ii) the interior of P¯\bar{P} in M¯0\partial\bar{M}_{0} is equal to P=M0P=\partial M_{0}.

Proof.

We give a proof following the arguments of Bowditch [15, Section 6.6] (cf. [2, Lemma 14.3]). By Selberg’s lemma, MM admits a finite regular manifold cover, namely there is a complete hyperbolic manifold NN and a finite group GG of orientation-preserving isometries of NN such that N/GMN/G\cong M. The inverse image, N0N_{0}, of M0M_{0} in NN forms a GG-invariant non-cuspidal part of NN, and we have N0/GM0N_{0}/G\cong M_{0}. By the relative version of the tameness theorem [18, Theorem 7.3] (cf. [15, Section 6]), there is a compact 33-manifold N¯0\bar{N}_{0} and a compact submanifold Q¯\bar{Q} of N¯0\partial\bar{N}_{0}, such that (i) intN¯0=intN0\operatorname{int}\bar{N}_{0}=\operatorname{int}N_{0} and (ii) the interior of Q¯\bar{Q} in N¯0\partial\bar{N}_{0} is equal to N0\partial N_{0}. Let D(N0)D(N_{0}) and be the double of N0N_{0} along N0\partial N_{0}. Then the action of GG on N0N_{0} extends to an action on D(N0)D(N_{0}), and D(N0)/GD(N_{0})/G is isomorphic to the double, D(M0)D(M_{0}), of M0M_{0} along M0\partial M_{0}. Consider the double, D(N¯0)D(\bar{N}_{0}), of N¯0\bar{N}_{0} along Q¯\bar{Q}. Then D(N¯0)D(\bar{N}_{0}) is a compact manifold with interior D(N0)D(N_{0}). By [40, Theorem 8.5], the action of GG on D(N0)D(N_{0}) extends to an action on D(N¯0)D(\bar{N}_{0}), and int(D(N¯0)/G)=D(N0)/G\operatorname{int}(D(\bar{N}_{0})/G)=D(N_{0})/G is identified with D(M0)D(M_{0}). Let M¯0\bar{M}_{0} be the closure in D(N¯0)/GD(\bar{N}_{0})/G of one of the two copies of M0M_{0} in D(M0)D(N¯0)/GD(M_{0})\subset D(\bar{N}_{0})/G, and let P¯\bar{P} be the image of Q¯D(N¯0)\bar{Q}\subset D(\bar{N}_{0}) in D(N¯0)/GD(\bar{N}_{0})/G. Then the pair (M¯0,P¯)(\bar{M}_{0},\bar{P}) satisfies the desired conditions. ∎

The above theorem together with the following theorem enables us to reduce the treatment of geometrically infinite case to that of geometrically finite case.

Theorem 5.2.

Under the setting of Theorem 5.1, (M¯0,P¯)(\bar{M}_{0},\bar{P}) is a pared orbifold. Moreover, the pared orbifold (M¯0,P¯)(\bar{M}_{0},\bar{P}) admits a geometrically finite complete hyperbolic structure. Namely, there is a geometrically finite Kleinian group Γ\Gamma^{\prime} such that (i) the orbifold 3/Γ\mathbb{H}^{3}/\Gamma^{\prime} is isomorphic to the orbifold intM¯0M\operatorname{int}\bar{M}_{0}\cong M and (ii) PP is the parabolic locus of Γ\Gamma^{\prime}.

Proof.

The first assertion that (M¯0,P¯)(\bar{M}_{0},\bar{P}) is a pared orbifold can be proved as in the proof of [41, Corollary 6.10 in Chapter V]. So we prove the second assertion that the pared orbifold (M¯0,P¯)(\bar{M}_{0},\bar{P}) admits a geometrically finite hyperbolic structure. If the orbifold M¯0\bar{M}_{0} is Haken in the sense of [10, Definition 8.0.1] then it follows from [10, Theorem 8.3.9] that the pared orbifold (M¯0,P¯)(\bar{M}_{0},\bar{P}) admits a geometrically finite hyperbolic structure, as desired. So we may assume the orbifold M¯0\bar{M}_{0} is non-Haken, i.e., either it contains no essential 22-suborbifold or it contains an essential turnover. In the first case, M0\partial M_{0} consists only of turnovers by [9, Proposition 9.4]. This implies that every end of MintM¯0M\cong\operatorname{int}\bar{M}_{0} has a neighbourhood isomorphic to the product of (a turnover)×[0,)(\mbox{a turnover})\times[0,\infty). Since a hyperbolic turnover is always realised by a totally geodesic surface, each end has a neighbourhood containing no closed geodesics. Thus every end of the hyperbolic orbifold MM is geometrically finite and rigid. Thus MM admits a unique complete hyperbolic structure, and it is geometrically finite. In the latter case, by the turnover splitting theorem [9, Theorem 4.8], M¯0\bar{M}_{0} admits a decomposition by a finite disjoint family of essential hyperbolic turnovers into Haken orbifolds and small orbifolds. By the orbifold theorem, each piece admits a geometrically finite hyperbolic structure, respecting the parabolic locus. By gluing these hyperbolic structures along the totally geodesic hyperbolic turnovers, we obtain a geometrically finite hyperbolic structure on (M¯0,P¯)(\bar{M}_{0},\bar{P}). ∎

Remark 5.3.

In [2], Agol suggested to prove the last assertion of Theorem 5.2 by using a relative version of the work of Feighn and Mess [22, Theorem 2] which proves the existence of a compact core of an orbifold M=3/ΓM=\mathbb{H}^{3}/\Gamma with a finitely generated orbifold fundamental group Γ\Gamma. Such a relative version is proved by Matsuzaki [37, Lemma 2] under the assumption that Γ\Gamma is indecomposable (over finite cyclic groups and with respect to the parabolic subgroups) in the sense of [37, Definition in p.26]. But we are not sure if non-free two-parabolic generator Kleinian groups satisfy this property. Though Theorem 5.1, which is proved by using the deep tameness theorem, of course, guarantees the existence of a relative core of complete hyperbolic orbifolds with finitely generated fundamental groups, we are not sure if more ‘elementary’ proof is possible.

6. Orbifold surgery

In this section, we introduce a convenient method for representing pared orbifolds by weighted graphs, generalising the convention in the introduction (Convention 6.1). Then we introduce the concept of an orbifold surgery (Definition 6.3), which is a key ingredient of the proof of the main theorem, and prove a basic Lemma 6.4 for the orbifold surgery. At the end of this section, we also state another basic Lemma 6.5 concerning the 2\mathbb{Z}_{2}-homology of an orbifold, which is repeatedly used in the proof of the main theorem.

Convention 6.1.

Consider a triple (W,Σ,w)(W,\Sigma,w), where WW is a compact oriented 33-manifold, Σ\Sigma is a finite trivalent graph properly embedded in WW, and ww is a function on the edge set of Σ\Sigma which takes value in 2{}\mathbb{N}_{\geq 2}\cup\{\infty\}. Here, a loop component of Σ\Sigma is regarded as a single edge, ΣM\Sigma\cap\partial M is the set of degree 11 vertices of Σ\Sigma, and all other vertices have degree 33. For each edge ee of Σ\Sigma, its value w(e)w(e) by ww is called the weight of the edge. We call the triple (W,Σ,w)(W,\Sigma,w) a weighted graph and call ww the weight function of the weighted graph. Let Σ\Sigma_{\infty} be the subgraph of Σ\Sigma consisting of the edges with weight \infty, and let Σs\Sigma_{s} be the subgraph of Σ\Sigma consisting of the edges with integral weight.

We regard each component, FF, of W\partial W as a 22-orbifold as follows: the underling space is the complement of an open regular neighbourhood of FΣF\cap\Sigma_{\infty} in FF, and the singular set is FΣsF\cap\Sigma_{s}, where the index of a singular point is given by the weight of the corresponding edge of Σs\Sigma_{s}. We assume that the following condition (SC) is satisfied.

  • (SC)

    For any sphere component SS of W\partial W, the corresponding 22-orbifold is not a bad orbifold, a spherical orbifold, a discal orbifold, nor an annulus. Namely, (i) |SW|3|S\cap W|\geq 3 and (ii) if |SW|=3|S\cap W|=3 then i=131w(ei)1\sum_{i=1}^{3}\frac{1}{w(e_{i})}\leq 1, where eie_{i} (i=1,2,3i=1,2,3) are the (germs of) edges of Σ\Sigma which have an endpoint in FF.

A trivalent vertex vv of Σ\Sigma is said to be spherical, euclidean or hyperbolic according to whether i=131w(ei)\sum_{i=1}^{3}\frac{1}{w(e_{i})} is bigger than, equal to, or smaller than 11, where eie_{i} (i=1,2,3i=1,2,3) are the (germs of) edges incident on vv. Let VEV_{E} (resp. VHV_{H}) be the set of the euclidean (resp. hyperbolic) vertices.

Let M0M_{0} be the complement of an open regular neighbourhood of ΣVEVH\Sigma_{\infty}\cup V_{E}\cup V_{H} in MM. Then M0M_{0} has the structure of an orbifold, with singular set Σ0:=M0Σs\Sigma_{0}:=M_{0}\cap\Sigma_{s}, where the indices of the edge of Σ0\Sigma_{0} are given by ww.

For each edge ee of Σ\Sigma_{\infty}, let meM0m_{e}\subset\partial M_{0} be a meridian loop of ee, let PP_{\infty} be the disjoint union of the regular neighbourhoods in M0\partial M_{0} of mem_{e}, where ee runs over the edges of Σ\Sigma_{\infty}. The condition (SC) implies that each component of cl(M0P)\operatorname{cl}(\partial M_{0}-P_{\infty}) is either a euclidean or hyperbolic 22-orbifold. Let PP be the union of PP_{\infty} and the euclidean components of cl(M0P)\operatorname{cl}(\partial M_{0}-P_{\infty}). Then PP is a disjoint union of euclidean 22-orbifolds.

We call (M0,P)(M_{0},P) the orbifold pair determined by the weighted graph (M,Σ,w)(M,\Sigma,w).

Convention 6.2.

It is sometimes convenient to employ the following slight extension of Convention 6.1.

(1) We allow ww to have an edge ee with w(e)=1w(e)=1. In this case, we consider the weighted graph (W,Σ,w)(W,\Sigma^{\prime},w^{\prime}), where Σ\Sigma^{\prime} is the subgraph of Σ\Sigma consisting of those edges with w(e)1w(e)\neq 1 and ww^{\prime} is the restriction of ww to Σ\Sigma^{\prime}. If Σ\Sigma^{\prime} is also trivalent graph properly embedded in WW and the condition (SC) is satisfied, then we define the orbifold pair determined by (W,Σ,w)(W,\Sigma,w) to be that determined by (W,Σ,w)(W,\Sigma^{\prime},w^{\prime}).

(2) We allow a quadrivalent vertex, vv, such that the four edge germs incident on it have index 22. In this case, vv represents a parabolic locus, P(v)P(v), isomorphic to S2(2,2,2,2)S^{2}(2,2,2,2).

A key ingredient of the proof of the main theorem is an orbifold surgery.

Definition 6.3.

Let (M0,P)(M_{0},P) be a pared orbifold, represented by a weighted graph (W,Σ,w)(W,\Sigma,w) satisfying the condition (SC). By replacing the weight function ww with another weight function ww^{\prime} (which also takes value in 2{}\mathbb{N}_{\geq 2}\cup\{\infty\}), we obtain another weighted graph (W,Σ,w)(W,\Sigma,w^{\prime}). This fails to satisfy the condition (SC) only when some sphere component SS of the topological boundary W\partial W determines a spherical 22-orbifold with three singular points. In this case, we cap all such sphere boundaries of WW with a cone over (S,SΣ)(S,S\cap\Sigma) to obtain a new weighted graph, which we call the augmentation of (W,Σ,w)(W,\Sigma,w^{\prime}). It satisfies the condition (SC), and determines an orbifold pair (N0,Q)(N_{0},Q). We call the 33-orbifold 𝒪:=N0{\mathcal{O}}:=N_{0} the orbifold obtained from (M0,P)(M_{0},P) by the orbifold surgery determined by the replacement of the weight function ww with the new weight function ww^{\prime}.

The following simple lemma is used repeatedly in the proof of the main theorem.

Lemma 6.4.

Let (M0,P)(M_{0},P) be a pared orbifold, and let 𝒪{\mathcal{O}} be the orbifold obtained from (M0,P)(M_{0},P) by an orbifold surgery. Then 𝒪{\mathcal{O}} does not contain a bad 22-suborbifold and 𝒪\partial{\mathcal{O}} does not contain a spherical component. In particular, 𝒪{\mathcal{O}} is very good.

Proof.

Let (W,Σ,w)(W,\Sigma,w) be a weighted graph representing the pared orbifold (M0,P)(M_{0},P), and let ww^{\prime} be the weight function on Σ\Sigma that gives the orbifold 𝒪=N0{\mathcal{O}}=N_{0}, where (N0,Q)(N_{0},Q) is the orbifold pair that is represented by the augmentation of (W,Σ,w)(W,\Sigma,w^{\prime}). Assume to the contrary that N0N_{0} contains a bad 22-suborbifold, SS, which is either a teardrop S2(n)S^{2}(n) or a spindle S2(m,n)S^{2}(m,n) for some integers m>n2m>n\geq 2. Since the underlying space |S||S| is disjoint from the vertex set of the singular set, Σ(N0)\Sigma(N_{0}), of N0N_{0}, we may assume |S||S| is a submanifold of WW transversal to Σ\Sigma. Then it determines a suborbifold, SS^{*}, of M0M_{0}, such that |S|=|S||M0||S^{*}|=|S|\cap|M_{0}|. The singular set of SS^{*} is equal to |S|Σs|S^{*}|\cap\Sigma_{s}, where Σs\Sigma_{s} is the subgraph of Σ\Sigma consisting of the edges of integral ww-weight, and the index of each singular point is given by the ww-weight of the corresponding edge of Σs\Sigma_{s}.

First, suppose that SS2(n)S\cong S^{2}(n) for n2n\geq 2. Let ee be the edge of Σ\Sigma such that |S|e|S|\cap e is the singular point of SS. If ee is an edge of Σs\Sigma_{s}, then SS^{*} is isomorphic to the teardrop S2(w(e))S^{2}(w(e)), which contradicts the fact that M0M_{0} is good. If ee is an edge of Σ\Sigma_{\infty}, then SS^{*} is a disc whose boundary is an essential simple loop on PP. This contradicts the fact that PP is incompressible in M0M_{0}.

Next, suppose that SS2(m,n)S\cong S^{2}(m,n) for m>n2m>n\geq 2. Let e1e_{1} and e2e_{2} be the edges of Σ\Sigma corresponding to the singular point of SS of index mm and nn, respectively. Then w(e1)=mn=w(e2)w^{\prime}(e_{1})=m\neq n=w^{\prime}(e_{2}), and so e1e_{1} and e2e_{2} are distinct. If both e1e_{1} and e2e_{2} are contained in Σs\Sigma_{s}, then SS2(m,n)S^{*}\cong S^{2}(m^{*},n^{*}) for some m,n2m^{*},n^{*}\geq 2. Since M0M_{0} does not contain a bad 22-suborbifold, mm^{*} and nn^{*} must be equal, and hence SS^{*} is an spherical suborbifold of M0M_{0}. Since M0M_{0} is irreducible, SS^{*} bounds a discal 33-orbifold. This implies e1e_{1} and e2e_{2} determine the same edge of Σ(N0)\Sigma(N_{0}). By the condition (SC), this in turn implies e1=e2e_{1}=e_{2}, a contradiction. If exactly one of e1e_{1} and e2e_{2} is contained in Σs\Sigma_{s}, then SS^{*} is a discal orbifold whose boundary is an essential simple loop on PP. This contradicts the assumption that PP is incompressible in M0M_{0}. If none of e1e_{1} and e2e_{2} is contained in Σs\Sigma_{s}, then SS^{*} is an annulus whose boundary consists of a pair of essential simple loops on PP. Thus SS^{*} is parallel to PP by Definition 3.1(4), and so e1=e2e_{1}=e_{2}, a contradiction.

Thus we have proved that 𝒪=N0{\mathcal{O}}=N_{0} does not contain a bad 22-suborbifold. The assertion that 𝒪\partial{\mathcal{O}} does not contain a spherical orbifold follows from the fact that 𝒪=N0{\mathcal{O}}=N_{0} is represented by the augmentation of (W,Σ,w)(W,\Sigma,w^{\prime}). The assertion that 𝒪{\mathcal{O}} is very good follows from [8, Corollary 1.3], which is a consequence of the orbifold theorem. ∎

Another key tool for the proof of the main theorem is the homology with 2\mathbb{Z}_{2} coefficient. Under Notation 1.3, we have the following lemma, which can be easily deduced from the definition of H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) and the Alexander duality.

Lemma 6.5.

Suppose an orbifold 𝒪{\mathcal{O}} is represented by a weighted graph (S3,Σ,w)(S^{3},\Sigma,w) in S3S^{3}. Let Σeven\Sigma_{\mathrm{even}} be the subgraph of Σ\Sigma spanned by the edges of even weight. Then H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is determined by H1(Σeven;2)H_{1}(\Sigma_{\mathrm{even}};\mathbb{Z}_{2}). To be precise, we have the following natural isomorphisms.

H1(𝒪;2)H1(S3Σeven;2)H1(Σeven;2)Hom(H1(Σeven;2),2)H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong H_{1}(S^{3}-\Sigma_{\mathrm{even}};\mathbb{Z}_{2})\cong H^{1}(\Sigma_{\mathrm{even}};\mathbb{Z}_{2})\cong\mathrm{Hom}(H_{1}(\Sigma_{\mathrm{even}};\mathbb{Z}_{2}),\mathbb{Z}_{2})

In particular, the following hold.

  1. (1)

    H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is generated by the meridians of edges of Σeven\Sigma_{\mathrm{even}}.

  2. (2)

    The meridian of an edge of Σ\Sigma of odd degree represents the trivial element of H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}).

  3. (3)

    Let eie_{i} (i=1,2,3i=1,2,3) be edges of Σ\Sigma incident on a vertex of Σ\Sigma, and suppose that w(e1)w(e_{1}) is odd and w(e2)w(e_{2}) and w(e3)w(e_{3}) are even. Then the meridians of e2e_{2} and e3e_{3} represent the same element of H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}).

7. Canonical horoball pairs for Kleinian groups generated by two parabolic transformations

Throughout Sections 7 \sim 11, Γ=α,β\Gamma=\langle\alpha,\beta\rangle denotes a non-elementary Kleinian group generated by two parabolic transformations α\alpha and β\beta, and M=3/ΓM=\mathbb{H}^{3}/\Gamma denotes the quotient hyperbolic 33-orbifold. Let η\eta be the geodesic joining the parabolic fixed points of α\alpha and β\beta, and let hh be the π\pi-rotation around η\eta. Then we have

(hαh1,hβh1)=(α1,β1).(h\alpha h^{-1},h\beta h^{-1})=(\alpha^{-1},\beta^{-1}).

We call hh the inverting elliptic element for the parabolic generating pair {α,β}\{\alpha,\beta\} of the Kleinian group Γ\Gamma. As shown in [57, Section 5.4], we can find a geodesic intersecting η\eta orthogonally, such that the π\pi-rotation, ff, around it satisfies the following identity.

(fαf1,fβf1)=(β,α).(f\alpha f^{-1},f\beta f^{-1})=(\beta,\alpha).

We call ff the exchanging elliptic element for the parabolic generating pair {α,β}\{\alpha,\beta\} of the Kleinian group Γ\Gamma. It should be noted that fhfh is the exchanging elliptic element for the parabolic generating pair {α,β1}\{\alpha,\beta^{-1}\} of Γ\Gamma.

By abuse of notation, we denote the isometries of MM induced by ff and hh by the same symbols ff and hh, respectively. Each of them is either the identity map or a (nontrivial) involution of MM, i.e., its order is 11 or 22. We call the isometries ff and hh, the exchanging involution and the inverting involution of MM associated with the parabolic generating pair {α,β}\{\alpha,\beta\}. It should be noted that if Γ\Gamma is isomorphic to a hyperbolic 22-bridge link group G(K(r))G(K(r)) and {α,β}\{\alpha,\beta\} is the upper-meridian pair, then the involutions ff and hh on MS3K(r)M\cong S^{3}-K(r) are the restrictions of the vertical and horizontal involutions of K(r)K(r) (see Figure 4). This is the reason why we use the symbols ff and hh with two different meanings.

Let Γ^:=Γ,f\hat{\Gamma}:=\langle\Gamma,f\rangle be the group generated by Γ\Gamma and the exchanging elliptic element ff associated with the parabolic generating pair {α,β}\{\alpha,\beta\} of Γ\Gamma. Then Γ^\hat{\Gamma} is a Kleinian group which is either equal to Γ\Gamma or a 2\mathbb{Z}_{2}-extension of Γ\Gamma according to whether ff belongs to Γ\Gamma or not. Let M^:=3/Γ^\hat{M}:=\mathbb{H}^{3}/\hat{\Gamma} be the quotient hyperbolic orbifold, and let C^α,β\hat{C}_{\alpha,\beta} be the maximal cusp of M^\hat{M} corresponding to the conjugacy class of Γ^\hat{\Gamma} containing both α\alpha and β=fαf1\beta=f\alpha f^{-1}. Then the inverse image p1(C^α,β)p^{-1}(\hat{C}_{\alpha,\beta}) of C^α,β\hat{C}_{\alpha,\beta} by the projection p:3M^p:\mathbb{H}^{3}\to\hat{M} is a union of horoballs with disjoint interiors but whose boundaries have nonempty tangential intersections. We call it the canonical horoball system associated with the parabolic generating pair {α,β}\{\alpha,\beta\} of Γ\Gamma. If a parabolic element γ\gamma of Γ\Gamma stabilises a member of the canonical horoball system, we denote the horoball by HγH_{\gamma}. We denote the translation length of γ\gamma on the horosphere Hγ\partial H_{\gamma} by the symbol |γ|=|γ|Hγ|\gamma|=|\gamma|_{\partial H_{\gamma}}, and call it the length of γ\gamma in the canonical horosphere. We call the pair (Hα,Hβ)(H_{\alpha},H_{\beta}) the canonical horoball pair for the parabolic generating pair {α,β}\{\alpha,\beta\} of the Kleinian group Γ\Gamma.

Note that the definition of |γ||\gamma| depends on the parabolic generating pair {α,β}\{\alpha,\beta\}, because the exchanging elliptic element ff is involved in the definition. However, it actually depends only on the pair {Fix(α),Fix(β)}\{\operatorname{Fix}(\alpha),\operatorname{Fix}(\beta)\}, because any orientation-preserving isometry, which exchanges Fix(α)\operatorname{Fix}(\alpha) and Fix(β)\operatorname{Fix}(\beta), also exchanges the members HαH_{\alpha} and HβH_{\beta} of the canonical horoball pair associated with {α,β}\{\alpha,\beta\}. (Otherwise, the product of ff and an unexpected involution, which exchanges Fix(α)\operatorname{Fix}(\alpha) and Fix(β)\operatorname{Fix}(\beta) but does not exchange HαH_{\alpha} and HβH_{\beta}, gives a loxodromic transformation which fixes the parabolic fixed points Fix(α)\operatorname{Fix}(\alpha) and Fix(β)\operatorname{Fix}(\beta). This contradicts the assumption that Γ\Gamma is discrete.)

The following lemmas are proved by Adams [1, Lemma 3.1, Theorem 3.2, and p.197] (see also Brenner [16]). Since they holds a key to the proof of the main theorem and since we described the setting in a slightly different way, we include the proof.

Lemma 7.1.

Under the above setting, the following hold.

  1. (1)

    For any parabolic element γΓ\gamma\in\Gamma which stabilises a member of the canonical horoball system, we have |γ|1|\gamma|\geq 1.

  2. (2)

    1|α|=|β|1\leq|\alpha|=|\beta|.

  3. (3)

    If Γ\Gamma is non-free then |α|=|β|<2|\alpha|=|\beta|<2.

Proof.

(1) We may assume Hγ\partial H_{\gamma} is the horosphere ×{1}\mathbb{C}\times\{1\} in the upper half space model 3=×+\mathbb{H}^{3}=\mathbb{C}\times\mathbb{R}_{+}. Then some other member, HgH_{g}, of the canonical horoball system touches Hγ\partial H_{\gamma} and hence has Euclidean diameter 11. Since γ(Hg)=Hγgγ1\gamma(H_{g})=H_{\gamma g\gamma^{-1}} is also a member of the canonical horoball system, HgH_{g} and γ(Hg)\gamma(H_{g}) have disjoint interiors. Hence we have |γ|1|\gamma|\geq 1.

(2) Since α\alpha and β\beta are conjugate in Γ^\hat{\Gamma}, |α||\alpha| and |β||\beta| are equal. Moreover, |α|=|β||\alpha|=|\beta| is 1\geq 1 by (1).

(3) We refer the proof to [1, Theorem 3.2] and Brenner [16]. ∎

Lemma 7.2.

Both α\alpha and β\beta are primitive in Γ\Gamma.

Proof.

If Γ\Gamma is a free, then the assertion follows from the fact that any member of a free-generating system of a free group is primitive. So, we may assume Γ\Gamma is non-free. Suppose on the contrary that one of the two elements, say α\alpha, is imprimitive, namely there is an element α0Γ\alpha_{0}\in\Gamma and an integer n2n\geq 2 such that α=α0n\alpha=\alpha_{0}^{n}. Then |α|=n|α0|n2|\alpha|=n|\alpha_{0}|\geq n\geq 2 by Lemma 7.1(1). But, this contradicts Lemma 7.1(3). ∎

8. Outline of the proof of Theorem 1.1

We now state an outline of the proof of Theorem 1.1. Since the if part is clear (cf. Proposition 3.3), we prove the only if part. To this end, we summarise the setting of Theorem 1.1.

Assumption 8.1.

Let Γ=α,β\Gamma=\langle\alpha,\beta\rangle be a non-free Kleinian group generated by two non-commuting parabolic transformations α\alpha and β\beta, and let M=3/ΓM=\mathbb{H}^{3}/\Gamma be the quotient hyperbolic orbifold. Let M0M_{0} be the non-cuspidal part of MM, and P=M0P=\partial M_{0} the parabolic locus. By Theorem 5.1, (M0,P)(M_{0},P) admits a relative compactification (M¯0,P¯)(\bar{M}_{0},\bar{P}), which is a pared orbifold by Theorem 5.2. The pared orbifold (M¯0,P¯)(\bar{M}_{0},\bar{P}) can be represented by a weighted graph (W,Σ,w)(W,\Sigma,w), where WW is a compact 33-manifold, Σ\Sigma is a trivalent graph properly embedded in WW, and ww is a weight function on the edge set of Σ\Sigma (see Convention 6.1). We abuse notation to denote the (compact) pared orbifold (M¯0,P¯)(\bar{M}_{0},\bar{P}) by (M0,P)(M_{0},P). We denote the components of P¯\bar{P}, which is now denoted by PP, corresponding to the cusps CαC_{\alpha} and CβC_{\beta} by PαP_{\alpha} and PβP_{\beta}, respectively.

Outline of the proof of Theorem 1.1.

Under Assumption 8.1, the proof is divided into the following two cases.

  1. Case 1.

    PαPβP_{\alpha}\cong P_{\beta} is a flexible cusp (Section 9 for generic case and Section 11 for exceptional case).

  2. Case 2.

    PαPβP_{\alpha}\cong P_{\beta} is a rigid cusp (Section 10).

In both cases, the first task is to find an orbifold surgery that yields an orbifold 𝒪{\mathcal{O}} with dihedral orbifold fundamental group.

In Case 1, this can be generically done by using Lemma 7.2. In fact, if PαPβP_{\alpha}\cong P_{\beta} is a flexible cusp, then Lemma 7.2 implies that each of the parabolic elements α\alpha and β\beta can be represented by simple loops of PαP_{\alpha} and PβP_{\beta}, respectively. Generically, these simple loops are disjoint, and such an surgery obviously exists. This generic case is treated in Section 9.

However, there is an exceptional case where Pα=PβS2(2,2,2,2)P_{\alpha}=P_{\beta}\cong S^{2}(2,2,2,2) and the simple loops representing α\alpha and β\beta intersect nontrivially (Lemma 9.1). In this case, the exchanging elliptic element ff does not belong to Γ\Gamma, and we need to consider the 2\mathbb{Z}_{2}-extension Γ^:=Γ,f\hat{\Gamma}:=\langle\Gamma,f\rangle of Γ\Gamma and consider the corresponding pared orbifold (M^0,P^):=(M0,P)/f(\hat{M}_{0},\hat{P}):=(M_{0},P)/f, where P^αβ\hat{P}_{\alpha\beta} is isomorphic to the rigid cusp S2(2,4,4)S^{2}(2,4,4). The treatment of this case is deferred to Section 11, after the treatment of the rigid cusp Case 2 in Section 10, described below.

In Case 2, if PαPβP_{\alpha}\cong P_{\beta} is isomorphic to either S2(2,4,4)S^{2}(2,4,4) or S2(2,3,6)S^{2}(2,3,6), the dihedral surgery can be found by using an estimate of the shortest, second shortest, and third shortest lengths of parabolic elements on the maximal rigid cusp, which in turn is based on Lemma 7.1. If PαPβP_{\alpha}\cong P_{\beta} is isomorphic to S2(3,3,3)S^{2}(3,3,3), the inverting parabolic element hh does not belong to Γ\Gamma, and we consider the 2\mathbb{Z}_{2}-extension Γh:=Γ,h\Gamma_{h}:=\langle\Gamma,h\rangle and the corresponding pared orbifold (Mh,0,Ph):=(M0,P)/h(M_{h,0},P_{h}):=(M_{0},P)/h. The images of PαP_{\alpha} and PβP_{\beta} in this quotient is isomorphic to S2(2,3,6)S^{2}(2,3,6), and this case can be treated by using arguments in the case where PαPβS2(2,3,6)P_{\alpha}\cong P_{\beta}\cong S^{2}(2,3,6).

After finding an orbifold surgery that yields an orbifold 𝒪{\mathcal{O}} with dihedral orbifold fundamental group, we can appeal to the classification Theorem 4.1 of the dihedral orbifolds, because Lemma 6.4 guarantees that the orbifold 𝒪{\mathcal{O}} satisfies the three conditions in Theorem 4.1. So, 𝒪{\mathcal{O}} belongs to the list in the theorem. The original pared orbifold (M0,P)(M_{0},P) is obtained from the dihedral orbifold 𝒪{\mathcal{O}} by inverse surgery operations. Through case-by-case arguments, by using the homology with 2\mathbb{Z}_{2}-coefficients, a result concerning the symmetries of the spherical dihedral orbifold (Corollary 12.7), and a ‘surgery trick’ (the last paragraph in Case 1 in Section 10 and Case 1 in Section 11), we prove the following.

  1. (1)

    If PαPβP_{\alpha}\cong P_{\beta} is a flexible cusp, then, in the generic case, the pared orbifold (M0,P)(M_{0},P) is isomorphic to either a hyperbolic 22-bridge link exterior or a Heckoid orbifold (Section 9): in the exceptional case, we encounter a contradiction (Section 11).

  2. (2)

    If PαPβP_{\alpha}\cong P_{\beta} is a rigid cusp, then we encounter a contradiction (Section 10).

This ends an outline of the proof of the main Theorem 1.1. ∎

9. Proof of Theorem 1.1 - flexible cusp: generic case -

Under Assumption 8.1, suppose that PαPβP_{\alpha}\cong P_{\beta} is a flexible cusp. Then the 22-orbifold PαPβP_{\alpha}\cong P_{\beta} is isomorphic to the torus T2T^{2}, the pillowcase S2(2,2,2,2)S^{2}(2,2,2,2), the annulus A2A^{2}, or D2(2,2)D^{2}(2,2). The following fact is the starting point of this section.

Lemma 9.1.

Under the above setting, α\alpha and β\beta are represented by simple loops on PαP_{\alpha} and PβP_{\beta}, respectively. Moreover, if Pα=PβP_{\alpha}=P_{\beta}, then one of the following holds.

  1. (1)

    The parabolic elements α\alpha and β\beta are represented by the same (possibly oppositely oriented) simple loop.

  2. (2)

    Pα=PβS2(2,2,2,2)P_{\alpha}=P_{\beta}\cong S^{2}(2,2,2,2), fΓf\notin\Gamma, and Pα/f=Pβ/fS2(2,4,4)P_{\alpha}/f=P_{\beta}/f\cong S^{2}(2,4,4), where the first ff is the exchanging elliptic element associated with {α,β}\{\alpha,\beta\} and the last two ff’s denote the involution on (M0,P)(M_{0},P) induced by the exchanging elliptic element ff (see Figure 11).

Proof.

The first assertion directly follows from Lemma 7.2, because any primitive parabolic element in the orbifold fundamental group of the 22-dimensional orbifold T2T^{2}, S2(2,2,2,2)S^{2}(2,2,2,2), A2A^{2}, or D2(2,2)D^{2}(2,2) is represented by a simple loop on the 22-orbifold. For the proof of the second assertion, suppose that Pα=PβP_{\alpha}=P_{\beta}. If the exchanging elliptic element ff belongs to Γ\Gamma, then β\beta is conjugate to α\alpha in Γ\Gamma, and so they are represented by the same simple loop. Thus we may suppose fΓf\notin\Gamma. Then ff descends to a nontrivial orientation-preserving involution on MM, which we continue to denote by ff, on the flexible cusp PαP_{\alpha}. By the classification of orientation-preserving involutions on flexible cusps, we can observe that either (a) the involution ff on M0M_{0} preserves or reverses the homotopy class of each essential simple loop on PαP_{\alpha}, or (b) PαS2(2,2,2,2)P_{\alpha}\cong S^{2}(2,2,2,2) and Pα/fS2(2,4,4)P_{\alpha}/f\cong S^{2}(2,4,4). In the first case, α\alpha and β±1\beta^{\pm 1} are represented by the same simple loop, and so we obtain the desired conclusion. ∎

In this section, we treat the case where either PαPβP_{\alpha}\neq P_{\beta} or Pα=PβP_{\alpha}=P_{\beta} and the conclusion (1) in Lemma 9.1 holds. Thus we assume the following condition in the remainder of this section. The other case is treated in Section 11.

Assumption 9.2.

Under Assumption 8.1, we further assume that (a) PαPβP_{\alpha}\cong P_{\beta} is a flexible cusp and that (b) either PαPβP_{\alpha}\neq P_{\beta} or Pα=PβP_{\alpha}=P_{\beta} and the conclusion (1) in Lemma 9.1 holds. It should be noted that either α\alpha and β\beta are represented by disjoint simple loops or they are represented by the same (possibly oppositely oriented) simple loop.

Under this assumption, we can apply an orbifold surgery on (M0,P)(M_{0},P) to the pared orbifold (M0,P)(M_{0},P) to obtain a dihedral orbifold, 𝒪{\mathcal{O}}, as follows. Note that Assumption 9.2 implies that the pared orbifold (M0,P)(M_{0},P) is represented by a weighted graph (W,Σ,w~)(W,\Sigma,\tilde{w}), such that there are (possibly identical) edges eαe_{\alpha} and eβe_{\beta} of Σ\Sigma whose meridians represent α\alpha and β\beta, respectively. Let ww be a weight function on Σ\Sigma which is identical with w~\tilde{w}, except that w(eα)=w(eβ)=2w(e_{\alpha})=w(e_{\beta})=2. Then the orbifold 𝒪{\mathcal{O}} represented by the augmentation of the weighted graph (W,Σ,w)(W,\Sigma,w) is a result of an “order 22” orbifold surgery on (M0,P)(M_{0},P), and π1(𝒪)\pi_{1}({\mathcal{O}}) is dihedral, as shown below.

Note that there is a natural epimorphism from Γ=π1(M0)\Gamma=\pi_{1}(M_{0}) to π1(𝒪)\pi_{1}({\mathcal{O}}), and the images of α\alpha and β\beta in π1(𝒪)\pi_{1}({\mathcal{O}}) have order 2\leq 2. Moreover, the images of α\alpha and β\beta have the same order, because (a) if fΓf\in\Gamma then α\alpha and β\beta are conjugate in Γ\Gamma and so in π1(𝒪)\pi_{1}({\mathcal{O}}), and (b) if fΓf\notin\Gamma then ff descends to an involution on 𝒪{\mathcal{O}} which interchanges the images of α\alpha and β\beta. So π1(𝒪)\pi_{1}({\mathcal{O}}) is either the trivial group or a dihedral group. Since 𝒪{\mathcal{O}} is very good by Lemma 6.4 and since 𝒪{\mathcal{O}} has nonempty singular set, π1(𝒪)\pi_{1}({\mathcal{O}}) is nontrivial and so isomorphic to a dihedral group.

Thus 𝒪{\mathcal{O}} satisfies the three conditions in Theorem 4.1 and so 𝒪{\mathcal{O}} belongs to the list in the theorem. We have the following lemma.

Lemma 9.3.

The orbifold 𝒪{\mathcal{O}} is isomorphic to the spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) for some rr\in\mathbb{Q} and coprime positive integers d+d_{+} and dd_{-}.

Proof.

We show that the possibilities (2), (3) and (4) in Theorem 4.1 cannot happen. Suppose (2) happens. Then we can see that one of the following holds, by recalling the fact that 𝒪{\mathcal{O}} is obtained from the pared orbifold (M0,P)(M_{0},P) an order 22 orbifold surgery.

  1. (i)

    M0M_{0} is the exterior of the two-component trivial link, P=M0P=\partial M_{0}, and the singular set of M0M_{0} is empty.

  2. (ii)

    The underlying space of M0M_{0} is the solid torus (the exterior of a trivial knot), P=M0P=\partial M_{0}, and the singular set is a trivial knot in the solid torus with index 22.

In each case, (M0,P)(M_{0},P) is reducible, a contradiction.

By the same reasoning, we can see that (3) cannot happen.

If (4) happens, then as in the above, we can see that one of the following holds, where (B3,t1t2)(B^{3},t_{1}\cup t_{2}) is a two-strand trivial tangle.

  1. (i)

    (M0,P)(cl(B3N(t1t2)),frN(t1t2))(M_{0},P)\cong(\operatorname{cl}(B^{3}-N(t_{1}\cup t_{2})),\operatorname{fr}N(t_{1}\cup t_{2})) and the singular set of M0M_{0} is empty.

  2. (ii)

    (M0,P)(cl(B3N(t1)),frN(t1))(M_{0},P)\cong(\operatorname{cl}(B^{3}-N(t_{1})),\operatorname{fr}N(t_{1})) and the singular set of M0M_{0} is t2t_{2} with index 22.

In the first case, Γ=π1(M0)\Gamma=\pi_{1}(M_{0}) is a rank 22 free group, which contradicts the assumption that Γ\Gamma is non-free. In the second case, note that H1(M0)H_{1}(M_{0}), the abelianization of the orbifold fundamental group π1(M0)\pi_{1}(M_{0}), is 2\mathbb{Z}\oplus\mathbb{Z}_{2}. On the other hand, both α\alpha and β\beta are represented by the core loop of the annulus P=frN(t1)P=\operatorname{fr}N(t_{1}), and the pair {α,β}\{\alpha,\beta\} cannot generate H1(M0)H_{1}(M_{0}), a contradiction. ∎

By Lemma 9.3, the original orbifold (M0,P)(M_{0},P) is recovered from 𝒪=𝒪(r;d+,d){\mathcal{O}}={\mathcal{O}}(r;d_{+},d_{-}) by applying the inverse orbifold surgery operation. This leads us to the following proposition.

Proposition 9.4.

Under the notation in Lemma 9.3, the following hold, if necessary by replacing r=q/pr=q/p with q/pq^{\prime}/p where q=q+pq^{\prime}=q+p or qq1(modp)qq^{\prime}\equiv 1\pmod{p}.

  1. (1)

    If |K(r)|=1|K(r)|=1, then one of the following holds.

    1. (i)

      d+=d=1d_{+}=d_{-}=1 and (M0,P)(E(K(r)),E(K(r)))(M_{0},P)\cong(E(K(r)),\partial E(K(r))), where q±1(modp)q\not\equiv\pm 1\pmod{p}.

    2. (ii)

      d+=1d_{+}=1, d2d_{-}\geq 2, and (M0,P)0(r;d)(M_{0},P)\cong\mathcal{M}_{0}(r;d_{-}).

    3. (iii)

      d+=1d_{+}=1, dd_{-} is an odd integer 3\geq 3, and (M0,P)1(r;d)(M_{0},P)\cong\mathcal{M}_{1}(r;d_{-}).

    4. (iv)

      d+=2d_{+}=2, dd_{-} is an odd integer 3\geq 3, and (M0,P)2(r;d)(M_{0},P)\cong\mathcal{M}_{2}(r;d_{-}).

  2. (2)

    If |K(r)|=2|K(r)|=2, then one of the following holds.

    1. (i)

      d+=d=1d_{+}=d_{-}=1 and (M0,P)(E(K(r)),E(K(r)))(M_{0},P)\cong(E(K(r)),\partial E(K(r))), where q±1(modp)q\not\equiv\pm 1\pmod{p}.

    2. (ii)

      d+=1d_{+}=1, d2d_{-}\geq 2, and (M0,P)0(r;d)(M_{0},P)\cong\mathcal{M}_{0}(r;d_{-}).

    3. (iii)

      d+=2d_{+}=2, dd_{-} is an odd integer 3\geq 3, and (M0,P)2(r;d)(M_{0},P)\cong\mathcal{M}_{2}(r;d_{-}).

Refer to caption
Figure 7. H1(𝒪;2)H1(S3Σeven;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong H_{1}(S^{3}-\Sigma_{\mathrm{even}};\mathbb{Z}_{2}), where Σeven\Sigma_{\mathrm{even}} is the subgraph of Σ=K(r)τ+τ\Sigma=K(r)\cup\tau_{+}\cup\tau_{-} spanned by the edges of even weight.
Proof.

Recall that 𝒪=𝒪(r;d+,d){\mathcal{O}}={\mathcal{O}}(r;d_{+},d_{-}) is represented by the weighted graph (S3,K(r)τ+τ,w)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},w) for some rr\in\mathbb{Q} and for some coprime positive integers d+d_{+} and dd_{-}, and ww is given by the following rule (see Figure 6):

w(K(r))=2,w(τ+)=d+,w(τ)=dw(K(r))=2,\quad w(\tau_{+})=d_{+},\quad w(\tau_{-})=d_{-}

Then (M0,P)(M_{0},P) is represented by the weighted graph (S3,K(r)τ+τ,w~)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},\tilde{w}), where w~\tilde{w} is obtained from ww by replacing the label 22 of the edges eαe_{\alpha} and eβe_{\beta}, which correspond to PαP_{\alpha} and PβP_{\beta} respectively, with the label \infty. By Remark 4.3, we may assume 1d+d1\leq d_{+}\leq d_{-}, if necessary by replacing r=q/pr=q/p with q/pq^{\prime}/p where qq1(modp)qq^{\prime}\equiv 1\pmod{p}.

Case 1. d+=d=1d_{+}=d_{-}=1. Then Σ(𝒪)\Sigma({\mathcal{O}}) is the 22-bridge link K(r)K(r). Thus (M0,P)(S3,K(r),w~)(M_{0},P)\cong(S^{3},K(r),\tilde{w}), where either (a) w~(K(r))=\tilde{w}(K(r))=\infty or (b) K(r)K(r) is a 22-component link K1K2K_{1}\cup K_{2} and (w~(K1),w~(K2))=(,2)(\tilde{w}(K_{1}),\tilde{w}(K_{2}))=(\infty,2). In the first case, (M0,P)(E(K(r)),E(K(r)))(M_{0},P)\cong(E(K(r)),\partial E(K(r))), and so 3/Γ\mathbb{H}^{3}/\Gamma is the hyperbolic 22-bridge link complement, S3K(r)S^{3}-K(r): in particular, q±1(modp)q\not\equiv\pm 1\pmod{p}. In the second case, both α\alpha and β\beta are meridians of the component K1K_{1}, which contradicts the fact that H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2} .

Case 2. d+=1<dd_{+}=1<d_{-}.

Subcase 2.1. |K(r)|=2|K(r)|=2 (see Figure 7(1)). Then the edge set of Σ(𝒪)\Sigma({\mathcal{O}}) consists of τ\tau_{-} and the two components K1K_{1}, K2K_{2} of K(r)K(r). Let xx_{-}, x1x_{1} and x2x_{2} be the meridians of τ\tau_{-}, K1K_{1} and K2K_{2}, respectively. By Lemma 6.5, H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2} is freely generated by {x1,x2}\{x_{1},x_{2}\}, and moreover we have x=0x_{-}=0. Since H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is generated by (the images of) α\alpha and β\beta, we may assume eα=K1e_{\alpha}=K_{1} and eβ=K2e_{\beta}=K_{2}. Thus (M0,P)(M_{0},P) is represented by (S3,K(r)τ,w~)(S^{3},K(r)\cup\tau_{-},\tilde{w}), where w~(K1)=w~(K2)=\tilde{w}(K_{1})=\tilde{w}(K_{2})=\infty and w~(τ)=d\tilde{w}(\tau_{-})=d_{-}. Hence (M0,P)0(r;d)(M_{0},P)\cong\mathcal{M}_{0}(r;d_{-}).

Subcase 2.2. |K(r)|=1|K(r)|=1 (see Figure 7(2)). Then the edge set of Σ(𝒪)\Sigma({\mathcal{O}}) consists of τ\tau_{-} and the two subarcs J1J_{1} and J2J_{2} of K(r)K(r) bounded by K(r)τK(r)\cap\tau_{-}. Let xx_{-}, x1x_{1} and x2x_{2} be the meridians of τ\tau_{-}, J1J_{1} and J2J_{2}, respectively.

Suppose first that dd_{-} is odd. Then we see by Lemma 6.5 that x=0x_{-}=0 in H1(𝒪;2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong\mathbb{Z}_{2} and that H1(𝒪;2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong\mathbb{Z}_{2} is generated by x1=x2x_{1}=x_{2}. Hence one of the following holds.

  1. (1)

    {eα,eβ}={J1,J2}\{e_{\alpha},e_{\beta}\}=\{J_{1},J_{2}\} and so (M0,P)(M_{0},P) is represented by (S3,K(r)τ,w~)(S^{3},K(r)\cup\tau_{-},\tilde{w}), where w~(J1)=w~(J2)=\tilde{w}(J_{1})=\tilde{w}(J_{2})=\infty and w~(τ)=d\tilde{w}(\tau_{-})=d_{-}. Hence (M0,P)0(r;d)(M_{0},P)\cong\mathcal{M}_{0}(r;d_{-}).

  2. (2)

    eα=eβ=Jie_{\alpha}=e_{\beta}=J_{i} for i=1i=1 or 22. By the symmetry of 𝒪{\mathcal{O}}, we may assume i=1i=1 and so (M0,P)(M_{0},P) is represented by (S3,K(r)τ,w~)(S^{3},K(r)\cup\tau_{-},\tilde{w}), where w~(J1)=\tilde{w}(J_{1})=\infty, w~(J2)=2\tilde{w}(J_{2})=2 and w~(τ)=d\tilde{w}(\tau_{-})=d_{-}. Hence (M0,P)1(r;d)(M_{0},P)\cong\mathcal{M}_{1}(r;d_{-}).

Suppose next that dd_{-} is even. Then x1+x2+x=0x_{1}+x_{2}+x_{-}=0 in H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2}. Since H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is generated by α\alpha and β\beta, we have eαeβe_{\alpha}\neq e_{\beta}. This implies that the exchanging elliptic element ff for {α,β}\{\alpha,\beta\} does not belong to Γ\Gamma, and ff descends to an involution on 𝒪{\mathcal{O}} interchanging eαe_{\alpha} with eβe_{\beta}. We now use Corollary 12.7 on the symmetry of the orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}). We first consider the generic case where p1p\neq 1 (i.e., K(r)K(r) is a nontrivial knot) or d>2d_{-}>2. (Recall the current assumption d+=1d_{+}=1.) Then, by Corollary 12.7(1), any orientation-preserving involution of 𝒪{\mathcal{O}} preserves τ\tau_{-}. So, eαe_{\alpha} and eβe_{\beta} are different from τ±\tau_{\pm}, and therefore {eα,eβ}={J1,J2}\{e_{\alpha},e_{\beta}\}=\{J_{1},J_{2}\}. Hence, as in the previous case, we can conclude (M0,P)0(r;d)(M_{0},P)\cong\mathcal{M}_{0}(r;d_{-}). In the exceptional case where p=1p=1 and d=2d_{-}=2, The orbifold 𝒪𝒪(0/1;1,2){\mathcal{O}}\cong{\mathcal{O}}(0/1;1,2) has the 33-fold cyclic symmetry as illustrated in Figure 15. Thus, if necessary after applying this symmetry, we may assume {eα,eβ}={J1,J2}\{e_{\alpha},e_{\beta}\}=\{J_{1},J_{2}\}. Hence we have (M0,P)0(r;d)0(0/1;2)(M_{0},P)\cong\mathcal{M}_{0}(r;d_{-})\cong\mathcal{M}_{0}(0/1;2).

Since we repeatedly use the above argument in the remainder of the proof of Proposition 9.4, we state an expanded version of the argument as a lemma.

Lemma 9.5.

Under the setting of Proposition 9.4, suppose (d+,d)(1,1)(d_{+},d_{-})\neq(1,1) and H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2}. Then eαeβe_{\alpha}\neq e_{\beta}, and the exchanging elliptic element ff does not belong to Γ\Gamma and it descends to an orientation-preserving involution of 𝒪=𝒪(r;d+,d){\mathcal{O}}={\mathcal{O}}(r;d_{+},d_{-}) interchanging eαe_{\alpha} and eβe_{\beta}. Moreover, the following hold.

  1. (1)

    Except when p=1p=1 and {d+,d}={1,2}\{d_{+},d_{-}\}=\{1,2\}, eαe_{\alpha} and eβe_{\beta} are different from τ±\tau_{\pm}.

  2. (2)

    If d+,d2d_{+},d_{-}\geq 2, then the inverting elliptic element hh belongs to Γ\Gamma.

Proof.

We have only to prove (2). If hh does not belong to Γ\Gamma, then it descends to an orientation-preserving involution of 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) which preserves both eαe_{\alpha} and eβe_{\beta}. However, if d+,d2d_{+},d_{-}\geq 2, then by Corollary 12.7(2), no orientation-preserving involution of 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) preserves an edge of the singular set different from τ±\tau_{\pm}. This contradicts the assertion (1). ∎

Case 3. 2d+d2\leq d_{+}\leq d_{-}. Since d+d_{+} and dd_{-} are coprime, we see 2d+<d2\leq d_{+}<d_{-} and one of d+d_{+} and dd_{-} is odd.

Subcase 3.1. |K(r)|=2|K(r)|=2 (see Figure 7(3)). Let K1K_{1} and K2K_{2} be the components of K(r)K(r), and let Ji,jJ_{i,j} (1i,j21\leq i,j\leq 2) be the edges of Σ(𝒪)\Sigma({\mathcal{O}}) such that Kj=J1,jJ2,jK_{j}=J_{1,j}\cup J_{2,j} for j=1,2j=1,2 and that the vertical involution of K(r)K(r) interchanges Ji,1J_{i,1} and Ji,2J_{i,2} for i=1,2i=1,2. Let x±x_{\pm} and xi,jx_{i,j} be the meridians of τ±\tau_{\pm} and Ji,jJ_{i,j}, respectively. Then by using Lemma 6.5 and the fact that one of d+d_{+} and dd_{-} is odd, we see that H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2} is freely generated by x1:=x1,1=x2,1x_{1}:=x_{1,1}=x_{2,1} and x2:=x1,2=x2,2x_{2}:=x_{1,2}=x_{2,2}: moreover we have x±=0x_{\pm}=0. Hence, we may assume eαK1e_{\alpha}\subset K_{1} and eβK2e_{\beta}\subset K_{2}. Since the horizontal involution of K(r)K(r) interchanges J1,jJ_{1,j} and J2,jJ_{2,j} (j=1,2j=1,2), we may assume eα=J1,1K1e_{\alpha}=J_{1,1}\subset K_{1} and eβ=Ji,2K2e_{\beta}=J_{i,2}\subset K_{2} for some i=1i=1 or 22. By Lemma 9.5(2), we have hΓh\in\Gamma, and so PαPβP_{\alpha}\cong P_{\beta} is homeomorphic to D2(2,2)D^{2}(2,2) or S2(2,2,2,2)S^{2}(2,2,2,2). Since 2d+<d2\leq d_{+}<d_{-}, we must have d+=2d_{+}=2. If i=1i=1, i.e. eβ=J1,2e_{\beta}=J_{1,2}, then w~\tilde{w} is given by

w~(J1,1)=w~(J1,2)=,w~(J1,2)=w~(J2,2)=2,w~(τ+)=2,w~(τ)=d.\tilde{w}(J_{1,1})=\tilde{w}(J_{1,2})=\infty,\quad\tilde{w}(J_{1,2})=\tilde{w}(J_{2,2})=2,\quad\tilde{w}(\tau_{+})=2,\quad\tilde{w}(\tau_{-})=d_{-}.

Since the vertical involution of K(r)K(r) preserves J1:=J1,1J1,2J_{1}:=J_{1,1}\cup J_{1,2}, we see that (M0,P)(M_{0},P) is isomorphic to 2(r;d)\mathcal{M}_{2}(r;d_{-}). If i=2i=2, i.e. eβ=J2,2e_{\beta}=J_{2,2}, then the planar involution of K(r)K(r) preserves J1:=J1,1J2,2J_{1}:=J_{1,1}\cup J_{2,2}. Hence, we see by Remark 3.5 that (M0,P)(M_{0},P) is isomorphic to 2(r;d)\mathcal{M}_{2}(r^{\prime};d_{-}), where r=(p+q)/pr^{\prime}=(p+q)/p.

Subcase 3.2. |K(r)|=1|K(r)|=1 (see Figure 7(4)). Suppose first that one of d+d_{+} and dd_{-} is even. Then H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2} by Lemma 6.5. Hence, by Lemma 9.5(2), both eαe_{\alpha} and eβe_{\beta} are contained in K(r)K(r), and hΓh\in\Gamma. In particular, PαPβD2(2,2)P_{\alpha}\cong P_{\beta}\cong D^{2}(2,2) or S2(2,2,2,2)S^{2}(2,2,2,2). Let eie_{i} (1i41\leq i\leq 4) be the edges of the singular set of 𝒪{\mathcal{O}} contained in the knot K(r)K(r) in this cyclic order. We also assume that τ+=(e1e2)(e3e4)\partial\tau_{+}=(e_{1}\cap e_{2})\cup(e_{3}\cap e_{4}) and τ=(e2e3)(e4e1)\partial\tau_{-}=(e_{2}\cap e_{3})\cup(e_{4}\cap e_{1}). Since the (2)2(\mathbb{Z}_{2})^{2}-symmetry of 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) acts transitively on the edge set {ei}1i4\{e_{i}\}_{1\leq i\leq 4} (see Figure 14), we may assume e1=eαe_{1}=e_{\alpha} and so w~(e1)=\tilde{w}(e_{1})=\infty. Since eαe_{\alpha} joins τ+\tau_{+} with τ\tau_{-} and since d±d_{\pm} are coprime integers such that 2d+d2\leq d_{+}\leq d_{-}, the condition that PαD2(2,2)P_{\alpha}\cong D^{2}(2,2) or S2(2,2,2,2)S^{2}(2,2,2,2) implies that d+=2d_{+}=2 and d3d_{-}\geq 3. This in turn implies that PαPβD2(2,2)P_{\alpha}\cong P_{\beta}\cong D^{2}(2,2). Since D2(2,2)\partial D^{2}(2,2) is isotopic to the simple loop α\alpha in M0\partial M_{0}, we must have w~(e2)=2\tilde{w}(e_{2})=2. Thus eβe_{\beta} is equal to e3e_{3} or e4e_{4}. However, if eβ=e4e_{\beta}=e_{4} then eαe_{\alpha}, eβe_{\beta}, and the odd index edge τ\tau_{-} share a vertex, it follows from Lemma 6.5(3) that the meridian α\alpha of e1e_{1} and the meridian β\beta of e4e_{4} represent the same element of H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2}, a contradiction. Hence eβ=e3e_{\beta}=e_{3}. Set J1=e1e3J_{1}=e_{1}\cup e_{3} and J2=e2e4J_{2}=e_{2}\cup e_{4}. Then J1J_{1} and J2J_{2} are disjoint, K(r)=J1J2K(r)=J_{1}\cup J_{2} and the following hold.

w~(J1)=,w~(J2)=2,w~(τ+)=2,w~(τ)=d\tilde{w}(J_{1})=\infty,\ \tilde{w}(J_{2})=2,\ \tilde{w}(\tau_{+})=2,\ \tilde{w}(\tau_{-})=d_{-}

Hence we have (M0,P)2(r;d)(M_{0},P)\cong\mathcal{M}_{2}(r;d_{-}) (cf. Remark 3.5(2)).

Suppose finally that both d+d_{+} and dd_{-} are odd. Then, by Lemma 6.5, the meridians x±x_{\pm} of τ±\tau_{\pm} represent the trivial element of H1(𝒪;2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong\mathbb{Z}_{2}, and hence both eαe_{\alpha} and eβ=f(eα)e_{\beta}=f(e_{\alpha}) are contained in K(r)K(r). On the other hand, since d±>2d_{\pm}>2, we have PαPβP_{\alpha}\cong P_{\beta} is homeomorphic to an annulus, and hence the inverting elliptic element hh descends to an involution of 𝒪{\mathcal{O}} which preserves each of the two mutually different edges eαe_{\alpha} and eβe_{\beta} and restricts to an orientation-reversing involution on each of the edges. But, such an involution does not exist by Corollary 12.7(2), a contradiction.

This completes the proof of Proposition 9.4. ∎

10. Proof of Theorem 1.1 - rigid cusp case -

Under Assumption 8.1, suppose that PαPβP_{\alpha}\cong P_{\beta} is a rigid cusp. Thus the 22-orbifold PαPβP_{\alpha}\cong P_{\beta} is isomorphic to S2(p,q,r)S^{2}(p,q,r) where (p,q,r)=(2,4,4)(p,q,r)=(2,4,4), (2,3,6)(2,3,6), or (3,3,3)(3,3,3).

Let G<ΓG<\Gamma be the orbifold fundamental group π1(Pα)\pi_{1}(P_{\alpha}), and let Λ\Lambda be the subgroup of GG consisting of parabolic transformations. We may assume that (a) GG stabilises the ideal point \infty of the upper-half space model of 3\mathbb{H}^{3}, and (b) the boundary Hα\partial H_{\alpha} of the canonical horoball HαH_{\alpha} is identified with the horosphere ×{1}3\mathbb{C}\times\{1\}\subset\mathbb{H}^{3}. For each element gΛg\in\Lambda, let |g||g| be the length of gg in the canonical horosphere (see Section 7), namely |g|=|g|Hα|g|=|g|_{\partial H_{\alpha}}, the translation length of gg in Hα\partial H_{\alpha}, and simply call it the length of gg. Let L1(Λ)>0L_{1}(\Lambda)>0 be the minimum of the lengths of nontrivial elements of Λ\Lambda. More generally, for each nn\in\mathbb{N}, let Ln(Λ)L_{n}(\Lambda) be the nn-th shortest length of nontrivial elements of Λ\Lambda.

Case 1. PαS2(2,4,4)P_{\alpha}\cong S^{2}(2,4,4). Then Ga,b,c|a2,b4,c4,abcG\cong\langle a,b,c\ |\ a^{2},\ b^{4},\ c^{4},abc\rangle, and Λ\Lambda is the rank 22 free abelian group with free basis {b2a,c2a}\{b^{2}a,c^{2}a\}. We may assume the action of GG on the horosphere Hα=×1\partial H_{\alpha}=\mathbb{C}\times 1\cong\mathbb{C} is given by the following rule. There is a positive real \ell such that aa is the π\pi rotation about 0, and bb and cc are the π/2\pi/2 rotations about \ell and i\ell i, respectively. We can easily observe the following.

  1. (i)

    The shortest length L1(Λ)L_{1}(\Lambda) is equal to 22\ell, and it is attained precisely by the conjugates of b2ab^{2}a in GG. (Note that c2a=(b1a1)2a=b1a1b1=b3ab1=b(b2a)b1c^{2}a=(b^{-1}a^{-1})^{2}a=b^{-1}a^{-1}b^{-1}=b^{3}ab^{-1}=b(b^{2}a)b^{-1} is conjugate to b2ab^{2}a.)

  2. (ii)

    The second shortest length L2(Λ)L_{2}(\Lambda) is equal to 222\sqrt{2}\ell, and it is attained precisely by the conjugates of b2ac2ab^{2}ac^{2}a in GG.

  3. (iii)

    The third shortest length L3(Λ)L_{3}(\Lambda) is equal to 44\ell, and it is attained precisely by the conjugates of (b2a)2(b^{2}a)^{2} in GG.

By Lemma 7.1(1), 2=L1(Λ)12\ell=L_{1}(\Lambda)\geq 1, and so 12\ell\geq\frac{1}{2}. Since Γ\Gamma is non-free, Lemma 7.1(3) implies that the length |α||\alpha| of the parabolic element αΛ\alpha\in\Lambda is less than 22. Since L3(Λ)=42L_{3}(\Lambda)=4\ell\geq 2, |α||\alpha| is equal to either L1(Λ)L_{1}(\Lambda) or L2(Λ)L_{2}(\Lambda). By using this fact, we obtain the following lemma.

Lemma 10.1.

The parabolic element αΛ\alpha\in\Lambda is conjugate to b2ab^{2}a or b2ac2ab^{2}ac^{2}a in GG. Moreover the following hold.

  1. (1)

    If α\alpha is conjugate to b2ab^{2}a, then the images of α\alpha by the natural epimorphisms from Gπ1(S2(2,4,4))G\cong\pi_{1}(S^{2}(2,4,4)) to π1(S2(2,2,2))\pi_{1}(S^{2}(2,2,2)), π1(S2(2,2,4))\pi_{1}(S^{2}(2,2,4)), and π1(S2(2,4,2))\pi_{1}(S^{2}(2,4,2)) have order 22.

  2. (2)

    If α\alpha is conjugate to b2ac2ab^{2}ac^{2}a, then the images of α\alpha by the natural epimorphisms from Gπ1(S2(2,4,4))G\cong\pi_{1}(S^{2}(2,4,4)) to π1(S2(2,2,2))\pi_{1}(S^{2}(2,2,2)), π1(S2(2,2,4))\pi_{1}(S^{2}(2,2,4)), and π1(S2(2,4,2))\pi_{1}(S^{2}(2,4,2)) have order 11, 22 and 22, respectively. Moreover, the 2\mathbb{Z}_{2}-homology class of α\alpha vanishes.

Proof.

The assertion in the first line follows from the observations preceding the lemma. The assertions (1) and (2) can be checked easily, by using the fact that b2ab^{2}a is conjugate to c2ac^{2}a in GG. ∎

Refer to caption
Figure 8. Orbifold surgery on the rigid cusp S2(2,4,4)S^{2}(2,4,4): The parabolic locus PαP_{\alpha} of the pared orbifold (M0,P)(M_{0},P) shrinks into the vertex vαv_{\alpha} of the singular set of the orbifold 𝒪{\mathcal{O}}. By Lemma 10.2, the homology class [α]H1(𝒪;2)[\alpha]\in H_{1}({\mathcal{O}};\mathbb{Z}_{2}) determined by the parabolic element αΓ\alpha\in\Gamma is represented by the meridian of the edge eαe_{\alpha} of the singular set Σ(𝒪)\Sigma({\mathcal{O}}) incident on vαv_{\alpha} whose index in the original orbifold M0M_{0} is 22.

Now let 𝒪{\mathcal{O}} be the orbifold obtained from the pared orbifold (M0,P)(M_{0},P) by the orbifold surgery as illustrated in Figure 8. Namely, for each index 44 edge of the singular set which has an endpoint in PαP_{\alpha} or PβP_{\beta}, we replace the index 44 with the index 22, and then cap all resulting spherical boundary components with discal 33-orbifolds. Then each of PαP_{\alpha} and PβP_{\beta} shrinks into a vertex of 𝒪{\mathcal{O}} with link S2(2,2,2)S^{2}(2,2,2), which we denote by vαv_{\alpha} and vβv_{\beta}, respectively. We denote by eαe_{\alpha} (resp. eβe_{\beta}) the edge of the singular set Σ(𝒪)\Sigma({\mathcal{O}}) incident on vαv_{\alpha} (resp. vβv_{\beta}) whose index in the original orbifold M0M_{0} is 22.

Lemma 10.2.

The orbifold 𝒪{\mathcal{O}} is isomorphic to a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) for some rr\in\mathbb{Q} and coprime positive integers d+d_{+} and dd_{-}. Moreover, αΛ\alpha\in\Lambda is conjugate to b2ab^{2}a in GG, and the homology class [α]H1(𝒪;2)[\alpha]\in H_{1}({\mathcal{O}};\mathbb{Z}_{2}) determined by α\alpha is equal to the meridian of the edge eαe_{\alpha}. Similarly, the homology class [β]H1(𝒪;2)[\beta]\in H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is equal to the meridian of the edge eβe_{\beta}.

Proof.

By Lemma 10.1, α\alpha is conjugate to b2ab^{2}a or b2ac2ab^{2}ac^{2}a in G=π1(S2(2,4,4))G=\pi_{1}(S^{2}(2,4,4)), its image in π1(S2(2,2,2))\pi_{1}(S^{2}(2,2,2)) has order 22 or 11 accordingly. Hence the image of α\alpha in π1(𝒪)\pi_{1}({\mathcal{O}}) has order 2\leq 2. Moreover, the images of α\alpha and β\beta have the same order, because (a) if the exchanging involution ff belongs to Γ\Gamma then α\alpha and β\beta are conjugate in Γ\Gamma and so in π1(𝒪)\pi_{1}({\mathcal{O}}), and (b) if fΓf\notin\Gamma then ff descends to an involution on 𝒪{\mathcal{O}} which interchanges the images of α\alpha and β\beta. Hence π1(𝒪)\pi_{1}({\mathcal{O}}) is either the trivial group or a dihedral group. Since 𝒪{\mathcal{O}} is very good by Lemma 6.4 and since it has a singular point with link S2(2,2,2)S^{2}(2,2,2), π1(𝒪)\pi_{1}({\mathcal{O}}) is a noncyclic dihedral group. Hence, by Theorem 4.1, 𝒪{\mathcal{O}} is isomorphic to a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}).

We prove the remaining assertions. If αΓ\alpha\in\Gamma is conjugate to b2ac2ab^{2}ac^{2}a, then it descends to the trivial element of π1(S2(2,2,2))\pi_{1}(S^{2}(2,2,2)), and so it represents the trivial element of π1(𝒪)\pi_{1}({\mathcal{O}}). This contradicts the fact that π1(𝒪)\pi_{1}({\mathcal{O}}) is a dihedral group generated by the images of α\alpha and β\beta. Hence α\alpha is conjugate to b2ab^{2}a. This implies that the 2\mathbb{Z}_{2}-homology class [α]H1(𝒪;2)[\alpha]\in H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is equal to that represented by the element aa, and so it is the meridian of the edge eαe_{\alpha}. The existence of the exchanging elliptic element ff implies the corresponding assertion for [β][\beta]. ∎

Lemma 10.3.

The pared orbifold (M0,P)(M_{0},P) is represented by the weighted graph (S3,K(r)τ+τ,w~)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},\tilde{w}) for some rr\in\mathbb{Q}, where w~\tilde{w} is determined by the following rule (see Figure 9):

w~(J1)=2,w~(J2)=4,w~(τ+)=4,w~(τ)=m,\tilde{w}(J_{1})=2,\quad\tilde{w}(J_{2})=4,\quad\tilde{w}(\tau_{+})=4,\quad\tilde{w}(\tau_{-})=m,

for some odd integer m3m\geq 3, where J1J_{1} and J2J_{2} are unions of two mutually disjoint edges of the graph K(r)τ+τK(r)\cup\tau_{+}\cup\tau_{-} distinct from τ±\tau_{\pm}, such that K(r)=J1J2K(r)=J_{1}\cup J_{2}. Moreover, PαP_{\alpha} and PβP_{\beta} correspond to distinct endpoints of τ+\partial\tau_{+} (in the sense of Convention 6.1(3)).

Proof.

By Lemma 10.2, 𝒪{\mathcal{O}} is represented by the weighted graph (S3,K(r)τ+τ,w)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},w) for some rr\in\mathbb{Q}, where ww is given by the rule

w(K(r))=2,w(τ+)=d+,w(τ)=dw(K(r))=2,\quad w(\tau_{+})=d_{+},\quad w(\tau_{-})=d_{-}

for some coprime positive integers d+d_{+} and dd_{-}. Since 𝒪{\mathcal{O}} is obtained from (M0,P)(M_{0},P) by an orbifold surgery, there is a weight function w~\tilde{w} on the graph K(r)τ+τK(r)\cup\tau_{+}\cup\tau_{-} such that the pared orbifold (M0,P)(M_{0},P) is represented by the weighted graph (S3,K(r)τ+τ,w~)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},\tilde{w}). By Remark 4.3, we may assume dd_{-} is odd, if necessary by replacing r=q/pr=q/p with q/pq^{\prime}/p where qq1(modp)qq^{\prime}\equiv 1\pmod{p}. Hence, we see H1(𝒪;2)(2)2H_{1}({\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2} by Lemma 6.5. Since H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) is generated by [α][\alpha] and [β][\beta], which are the meridians of the edges eαe_{\alpha} and eβe_{\beta}, respectively (see Lemma 10.2), we have eαeβe_{\alpha}\neq e_{\beta}.

Since the links of vαv_{\alpha} and vβv_{\beta} are isomorphic to S2(2,2,2)S^{2}(2,2,2), we see w(τ+)=2w(\tau_{+})=2 and {vα,vβ}τ+\{v_{\alpha},v_{\beta}\}\subset\partial\tau_{+}. Since eαe_{\alpha} (resp. eβe_{\beta}) is the unique edge of the trivalent graph K(r)τ+τK(r)\cup\tau_{+}\cup\tau_{-} incident on the vertex vαv_{\alpha} (resp. vβv_{\beta}) with w~\tilde{w}-weight 22, and since eαeβe_{\alpha}\neq e_{\beta}, we see that vαv_{\alpha} and vβv_{\beta} are distinct endpoints of τ+\tau_{+}. (If vα=vβv_{\alpha}=v_{\beta}, then its ‘link’ in M0M_{0} is of the form S2(2,2,)≇S2(2,4,4)S^{2}(2,2,*)\not\cong S^{2}(2,4,4).) Hence PαP_{\alpha} and PβP_{\beta} correspond to distinct endpoints of τ+\partial\tau_{+}.

We observe that eαe_{\alpha} and eβe_{\beta} are not equal to τ+\tau_{+}. If, say eαe_{\alpha} was equal to τ+\tau_{+}, then it is incident on vβτ+v_{\beta}\in\partial\tau_{+}. Since w~(eα)=2\tilde{w}(e_{\alpha})=2, this implies we have eα=eβe_{\alpha}=e_{\beta}, a contradiction. This observation implies that both eαe_{\alpha} and eβe_{\beta} are contained in K(r)K(r).

We next observe that d3d_{-}\geq 3. If d=1d_{-}=1, then the endpoints of eαe_{\alpha} and eβe_{\beta} are all contained in τ+={vα,vβ}\partial\tau_{+}=\{v_{\alpha},v_{\beta}\}. This together with the previous observation implies that the ‘links’ of vαv_{\alpha} and vβv_{\beta} in M0M_{0} are isomorphic to S2(2,2,4)S^{2}(2,2,4), a contradiction.

We now show that eαe_{\alpha} and eβe_{\beta} are disjoint. If they are not disjoint, then they share an endpoint of τ\tau_{-}, which has odd weight dd_{-}. This implies that the meridians of eαe_{\alpha} and eβe_{\beta} represent an identical element of H1(𝒪;2)H_{1}({\mathcal{O}};\mathbb{Z}_{2}) (see Lemma 6.5(3)), and so [α]=[β][\alpha]=[\beta], a contradiction.

Set J1:=eαeβJ_{1}:=e_{\alpha}\cup e_{\beta} and let J2:=cl(K(r)J1)J_{2}:=\operatorname{cl}(K(r)-J_{1}). Then J1J_{1} and J2J_{2} satisfy the desired conclusion with m=dm=d_{-}. ∎

Refer to caption
Figure 9. The possible pared orbifold (M0,P)(M_{0},P) in Lemma 10.3 and the orbifold 𝒪{\mathcal{O}}^{\prime} obtained by the orbifold surgery. In this figure, we apply further normalisation so that J1J_{1} and J2J_{2} are invariant by the vertical involution ff (cf. Remark 3.5(3)).

We show that the situation described in Lemma 10.3 cannot happen. To this end, we perform another orbifold surgery on (M0,P)(M_{0},P) which replaces the weight 44 of τ+\tau_{+} with 22. To be precise, we consider the orbifold 𝒪{\mathcal{O}}^{\prime} represented by the weighted graph (S3,K(r)τ+τ,w~)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},\tilde{w}^{\prime}) for some rr\in\mathbb{Q}, where w~\tilde{w}^{\prime} is given by the following rule.

w~(J1)=2,w~(J2)=4,w~(τ+)=2,w~(τ)=m\tilde{w}^{\prime}(J_{1})=2,\quad\tilde{w}^{\prime}(J_{2})=4,\quad\tilde{w}^{\prime}(\tau_{+})=2,\quad\tilde{w}^{\prime}(\tau_{-})=m

Note that PαS2(2,4,4)P_{\alpha}\cong S^{2}(2,4,4) shrinks into a singular point of 𝒪{\mathcal{O}}^{\prime} with link S2(2,2,4)S^{2}(2,2,4) or S2(2,4,2)S^{2}(2,4,2). Since α\alpha is conjugate to b2ab^{2}a in π1(S2(2,4,4))<π1(M0)=Γ\pi_{1}(S^{2}(2,4,4))<\pi_{1}(M_{0})=\Gamma, we see by Lemma 10.1(1) that the image of α\alpha in π1(𝒪)\pi_{1}({\mathcal{O}}^{\prime}) has order 2\leq 2. The same argument can be applied to β\beta and we see that the image of β\beta in π1(𝒪)\pi_{1}({\mathcal{O}}^{\prime}) also has order 2\leq 2. Since 𝒪{\mathcal{O}}^{\prime} is very good by Lemma 6.4 and since the singular set of 𝒪{\mathcal{O}}^{\prime} contains a trivalent vertex, π1(𝒪)\pi_{1}({\mathcal{O}}^{\prime}) is a noncyclic dihedral group. Since the singular set of 𝒪{\mathcal{O}}^{\prime} contains four trivalent vertices, Theorem 4.1 implies that 𝒪{\mathcal{O}}^{\prime} must be isomorphic to a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r^{\prime};d_{+}^{\prime},d_{-}^{\prime}) with d+,d2d_{+}^{\prime},d_{-}^{\prime}\geq 2. In particular, the singular set Σ(𝒪)\Sigma({\mathcal{O}}^{\prime}) of 𝒪{\mathcal{O}}^{\prime} must contain precisely four or five edges with index 22. This contradicts the fact that Σ(𝒪)\Sigma({\mathcal{O}}^{\prime}) contains precisely three edges of index 22 (see Figure 9).

Case 2. PαS2(2,3,6)P_{\alpha}\cong S^{2}(2,3,6). Then Ga,b,c|a2,b3,c6,abcG\cong\langle a,b,c\ |\ a^{2},\ b^{3},\ c^{6},\ abc\rangle, and Λ\Lambda is the rank 22 free abelian group with free basis {ac3,c(ac3)c1=cac2}\{ac^{3},c(ac^{3})c^{-1}=cac^{2}\}. We may assume the action of GG on the horosphere Hα=×1\partial H_{\alpha}=\mathbb{C}\times 1\cong\mathbb{C} is given by the following rule. There is a positive real \ell such that aa is the π\pi rotation about 3\sqrt{3}\ell, bb is the 2π/32\pi/3 rotation about 2eπi/6=3+i2\ell e^{\pi i/6}=\sqrt{3}\ell+\ell i, and cc is the π/3\pi/3 rotations about 0. The action of the generators of Λ\Lambda is given by

ac3(z)=z+23,cac2(z)=z+23eπi/3.ac^{3}(z)=z+2\sqrt{3}\ell,\quad cac^{2}(z)=z+2\sqrt{3}\ell e^{\pi i/3}.

We can easily observe the following.

  1. (i)

    L1(Λ)=23L_{1}(\Lambda)=2\sqrt{3}\ell, and it is attained precisely by the conjugates of ac3ac^{3} in GG.

  2. (ii)

    L2(Λ)=6L_{2}(\Lambda)=6\ell, and it is attained precisely by the conjugates of (ac3)(cac2)=ac4ac2(ac^{3})(cac^{2})=ac^{4}ac^{2} in GG.

  3. (iii)

    L3(Λ)=43L_{3}(\Lambda)=4\sqrt{3}\ell, and it is attained precisely by the conjugates of (ac3)2(ac^{3})^{2} in GG.

By Lemma 7.1(1), 23=L1(Λ)12\sqrt{3}\ell=L_{1}(\Lambda)\geq 1, and so 123\ell\geq\frac{1}{2\sqrt{3}}. Since Γ\Gamma is non-free, Lemma 7.1(3) implies that the length |α||\alpha| of the parabolic element αΛ\alpha\in\Lambda is less than 22. Hence we obtain the following.

Lemma 10.4.

The parabolic element αΛ\alpha\in\Lambda is conjugate to ac3ac^{3} or ac4ac2ac^{4}ac^{2} in GG.

Refer to caption
Figure 10. Orbifold surgery on the rigid cusp S2(2,3,6)S^{2}(2,3,6)

Now let 𝒪{\mathcal{O}} be the orbifold obtained from the pared orbifold (M0,P)(M_{0},P) by the orbifold surgery as illustrated in Figure 10. Namely, for each edge of the singular set which has the index 66 cone point of PαP_{\alpha} or PβP_{\beta} as an endpoint, we replace the weight 66 with the new weight 33, and then cap all resulting spherical boundary components with discal 33-orbifolds. Then PαP_{\alpha} and PβP_{\beta} shrink into singular points, vαv_{\alpha} and vβv_{\beta}, of 𝒪{\mathcal{O}} with link S2(2,3,3)S^{2}(2,3,3).

Lemma 10.5.

The image of α\alpha by the natural epimorphism from π1(S2(2,3,6))\pi_{1}(S^{2}(2,3,6)) to π1(S2(2,3,3))\pi_{1}(S^{2}(2,3,3)) has order 22.

Proof.

By Lemma 10.4, α\alpha is conjugate to either ac3ac^{3} or ac4ac2ac^{4}ac^{2} in G=π1(S2(2,3,6))G=\pi_{1}(S^{2}(2,3,6)). Moreover, the images of ac3ac^{3} and ac4ac2ac^{4}ac^{2} in π1(S2(2,3,3))a,b,c|a2,b3,c3,abc\pi_{1}(S^{2}(2,3,3))\cong\langle a,b,c\ |\ a^{2},\ b^{3},\ c^{3},\ abc\rangle have order 22. This is obvious for ac3ac^{3}, and the assertion for ac4ac2ac^{4}ac^{2} is verified as follows. In π1(S2(2,3,3))\pi_{1}(S^{2}(2,3,3)), we have 1=b3=(ac1)31=b^{3}=(ac^{-1})^{3} and so ac1=(ac1)2=(ca)2ac^{-1}=(ac^{-1})^{-2}=(ca)^{2}. Hence the image of ac4ac2ac^{4}ac^{2} in π1(S2(2,3,3))\pi_{1}(S^{2}(2,3,3)) is equal to acac1=ac(ca)2=ac2aca=(ca)1a(ca)acac^{-1}=ac(ca)^{2}=ac^{2}aca=(ca)^{-1}a(ca). Thus it is conjugate to aa, and so has order 22, as desired. ∎

By the above lemma, the image of α\alpha in π1(𝒪)\pi_{1}({\mathcal{O}}) has order 2\leq 2. The existence of the exchanging elliptic element ff implies that the images of α\alpha and β\beta in π1(𝒪)\pi_{1}({\mathcal{O}}) have the same order. Thus π1(𝒪)\pi_{1}({\mathcal{O}}) is either a dihedral group or the trivial group. Since 𝒪{\mathcal{O}} is very good by Lemma 6.4 and since the singular set of 𝒪{\mathcal{O}} contains a trivalent vertex, π1(𝒪)\pi_{1}({\mathcal{O}}) is a noncyclic dihedral group. Hence, Theorem 4.1 implies that 𝒪{\mathcal{O}} must be isomorphic to a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) with (d+,d)(1,1)(d_{+},d_{-})\neq(1,1). However, the orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) does not contain a singular point with link S2(2,3,3)S^{2}(2,3,3), a contradiction.

Case 3. PαS2(3,3,3)P_{\alpha}\cong S^{2}(3,3,3). Then the inverting elliptic element hh does not belong to Γ\Gamma, and the group, Γh\Gamma_{h}, obtained from Γ\Gamma by adding hh is a 2\mathbb{Z}_{2}-extension of Γ\Gamma. Consider the hyperbolic orbifold Mh:=3/ΓhM_{h}:=\mathbb{H}^{3}/\Gamma_{h}. Then MhM_{h} is the quotient of M=3/ΓM=\mathbb{H}^{3}/\Gamma by the isometric involution induced by hh, which we continue to denote by hh. Set (Mh,0,Ph):=(M0/h,P/h)(M_{h,0},P_{h}):=(M_{0}/h,P/h), Ph,α:=Pα/hP_{h,\alpha}:=P_{\alpha}/h and Ph,β:=Pβ/hP_{h,\beta}:=P_{\beta}/h. Then Ph,αPh,βP_{h,\alpha}\cong P_{h,\beta} is isomorphic to S2(2,3,6)S^{2}(2,3,6). Thus Gh:=π1(Ph,α)a,b,c|a2,b3,c6,abcG_{h}:=\pi_{1}(P_{h,\alpha})\cong\langle a,b,c\ |\ a^{2},\ b^{3},\ c^{6},\ abc\rangle. Since the subgroup Γ\Gamma of Γh\Gamma_{h} generated by α\alpha and β\beta is non-free, we see by the arguments in Case 2 that α\alpha is conjugate to ac3ac^{3} or ac4ac2ac^{4}ac^{2} in GhG_{h}.

Let 𝒪h{\mathcal{O}}_{h} be the orbifold obtained from the pared orbifold (Mh,0,Ph)(M_{h,0},P_{h}) by the orbifold surgery as illustrated in Figure 10 at both Ph,αP_{h,\alpha} and Ph,βP_{h,\beta}. Then Ph,αP_{h,\alpha} and Ph,βP_{h,\beta} shrink into singular points, vh,αv_{h,\alpha} and vh,βv_{h,\beta}, of 𝒪h{\mathcal{O}}_{h} with link S2(2,3,3)S^{2}(2,3,3). The images of α\alpha and β\beta in π1(𝒪h)\pi_{1}({\mathcal{O}}_{h}) have the same order 2\leq 2, and so the subgroup of π1(𝒪h)\pi_{1}({\mathcal{O}}_{h}) they generate is either a dihedral group or the trivial group. This subgroup has index 2\leq 2 in π1(𝒪h)\pi_{1}({\mathcal{O}}_{h}), because Γ=α,β\Gamma=\langle\alpha,\beta\rangle has index 22 in Γh\Gamma_{h}. Hence the group π1(𝒪h)\pi_{1}({\mathcal{O}}_{h}) is a trivial group, a dihedral group, 2\mathbb{Z}_{2} (the 2\mathbb{Z}_{2}-extension of the trivial group) or a 2\mathbb{Z}_{2}-extension of a dihedral group.

Since 𝒪h{\mathcal{O}}_{h} is very good by Lemma 6.4 and 𝒪h{\mathcal{O}}_{h} contains a singular point with link S2(2,3,3)S^{2}(2,3,3), π1(𝒪)\pi_{1}({\mathcal{O}}) is either a noncyclic dihedral group or a 2\mathbb{Z}_{2}-extension of a noncyclic dihedral group. Hence Theorem 4.1 implies that 𝒪h{\mathcal{O}}_{h} is isomorphic to (a) a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) or (b) the quotient of 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) by an isometric involution, where (d+,d)(1,1)(d_{+},d_{-})\neq(1,1). Since 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) does not have a singular point with link S2(2,3,3)S^{2}(2,3,3), (a) cannot happen, and so we may assume (b) holds. Since π1(S2(2,3,3))\pi_{1}(S^{2}(2,3,3)) does not have an index 22 subgroup, the link of an inverse image of the singular point vh,αv_{h,\alpha} in the double cover 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) of 𝒪h{\mathcal{O}}_{h} is also isomorphic to S2(2,3,3)S^{2}(2,3,3). But, this is impossible. Hence PαP_{\alpha} cannot be isomorphic to S2(3,3,3)S^{2}(3,3,3).

Thus we have proved that PαPβP_{\alpha}\cong P_{\beta} cannot be a rigid cusp.

11. Proof of Theorem 1.1 - flexible cusp: exceptional case -

In this section, we treat the case where the following assumption is satisfied, and prove that this assumption is never satisfied.

Assumption 11.1.

Under Assumption 8.1, we further assume that Pα=PβP_{\alpha}=P_{\beta} and it is a flexible cusp S2(2,2,2,2)S^{2}(2,2,2,2) and that the conclusion (2) in Lemma 9.1 holds. Namely, fΓf\notin\Gamma, and Pα/f=Pβ/fS2(2,4,4)P_{\alpha}/f=P_{\beta}/f\cong S^{2}(2,4,4) (see Figure 11).

Let Γ^:=Γ,f\hat{\Gamma}:=\langle\Gamma,f\rangle be the group generated by Γ\Gamma and ff. Let M^:=3/Γ^\hat{M}:=\mathbb{H}^{3}/\hat{\Gamma} be the quotient hyperbolic orbifold. Let M^0\hat{M}_{0} be the non-cuspidal part of M^\hat{M}, and P^=M^0\hat{P}=\partial\hat{M}_{0} the parabolic locus. By abuse of notation, we denote the pared orbifold obtained as the relative compactification of (M^0,P^)(\hat{M}_{0},\hat{P}) by the same symbol (M^0,P^)(\hat{M}_{0},\hat{P}). We denote the component of the compact euclidean 22-orbifold P^\hat{P} corresponding to the conjugacy class containing α\alpha and β=fαf1\beta=f\alpha f^{-1} by P^αβ\hat{P}_{\alpha\beta}. Thus P^αβPα/f=Pβ/fS2(2,4,4)\hat{P}_{\alpha\beta}\cong P_{\alpha}/f=P_{\beta}/f\cong S^{2}(2,4,4) and (M0,P)/f(M^0,P^)(M_{0},P)/f\cong(\hat{M}_{0},\hat{P}), where ff denotes the involution on the pared orbifold (M0,P)(M_{0},P) induced by the exchanging involution ff. In particular, M0M_{0} is the double orbifold covering of M^0\hat{M}_{0}, associated with the homomorphism ξ:π1(M^0)=Γ2\xi:\pi_{1}(\hat{M}_{0})=\Gamma\to\mathbb{Z}_{2} such that ξ(α)=ξ(β)=0\xi(\alpha)=\xi(\beta)=0 and ξ(f)=1\xi(f)=1. We denote the homomorphism H1(M^0;2)2H_{1}(\hat{M}_{0};\mathbb{Z}_{2})\to\mathbb{Z}_{2} induced by ξ\xi by the same symbol.

Note that π1(P^αβ)π1(S2(2,4,4))a,b,c|a2,b4,c4,abc\pi_{1}(\hat{P}_{\alpha\beta})\cong\pi_{1}(S^{2}(2,4,4))\cong\langle a,b,c\ |\ a^{2},\ b^{4},\ c^{4},abc\rangle. As in Case 1 in Section 10, we identify π1(P^αβ)\pi_{1}(\hat{P}_{\alpha\beta}) with the stabiliser StabΓ^(Fix(α))\operatorname{Stab}_{\hat{\Gamma}}(\operatorname{Fix}(\alpha)). Then the proof of Lemma 10.1 also works in this setting, because {α,β}\{\alpha,\beta\} generates the non-free subgroup Γ\Gamma of the Kleinian group Γ^\hat{\Gamma}, and we have the following lemma.

Lemma 11.2.

The parabolic element α\alpha is conjugate to b2ab^{2}a or b2ac2ab^{2}ac^{2}a in StabΓ^(Fix(α))\operatorname{Stab}_{\hat{\Gamma}}(\operatorname{Fix}(\alpha)) \cong π1(S2(2,4,4))\pi_{1}(S^{2}(2,4,4)), and of course, the assertions (1) and (2) in Lemma 10.1 also hold.

Refer to caption
Figure 11. Assumption 11.1 assumes that fΓf\notin\Gamma descends to an involution, ff, on Pα=PβS2(2,2,2,2)P_{\alpha}=P_{\beta}\cong S^{2}(2,2,2,2) such that Pα/f=Pβ/fS2(2,4,4)P_{\alpha}/f=P_{\beta}/f\cong S^{2}(2,4,4).

Let eie_{i} and e^i\hat{e}_{i} (i=1,2,3i=1,2,3) be the edges of the singular sets Σ(M0)\Sigma(M_{0}) and Σ(M^0)\Sigma(\hat{M}_{0}) as illustrated in Figure 11. Thus e2e_{2} and e3e_{3} are contained in the fixed point set of the involution ff on M0M_{0}, and e^i\hat{e}_{i} is the image of eie_{i} by the covering projection M0M^0M_{0}\to\hat{M}_{0}. (Note that it can happen that some of them are identical, though their germs near the parabolic locus are different.) Then the following holds.

Lemma 11.3.

The homomorphism ξ:H1(M^0;2)2\xi:H_{1}(\hat{M}_{0};\mathbb{Z}_{2})\to\mathbb{Z}_{2}, that determines the double orbifold covering M0M^0M_{0}\to\hat{M}_{0}, satisfies

ξ(m1)=0,ξ(m2)=ξ(m3)=1,\xi(m_{1})=0,\quad\xi(m_{2})=\xi(m_{3})=1,

where mim_{i} denotes the meridian of the edge e^i\hat{e}_{i}. Moreover, the homology class [f]H1(M^0;2)[f]\in H_{1}(\hat{M}_{0};\mathbb{Z}_{2}) determined by fΓ^f\in\hat{\Gamma} is equal to either m2m_{2} or m3m_{3}.

Proof.

The formula for ξ\xi follows from the fact that the fixed point set of the involution ff on M0M_{0} contains e2e_{2} and e3e_{3}, which project to e^2\hat{e}_{2} and e^3\hat{e}_{3}, respectively. It is also obvious that ξ([f])=1\xi([f])=1. So, if H1(M^0;2)2H_{1}(\hat{M}_{0};\mathbb{Z}_{2})\cong\mathbb{Z}_{2}, we have [f]=m2=m3[f]=m_{2}=m_{3}. Suppose that H1(M^0;2)(2)2H_{1}(\hat{M}_{0};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2}. Then, since H1(M^0;2)H_{1}(\hat{M}_{0};\mathbb{Z}_{2}) is generated by [f][f] and [α][\alpha], we see [α]0[\alpha]\neq 0. So, α\alpha is conjugate to b2ab^{2}a by Lemma 11.2. (Otherwise α\alpha is conjugate to b2ac2ab^{2}ac^{2}a and so [α]=0[\alpha]=0.) Therefore [α]=[a]=m1[\alpha]=[a]=m_{1} is contained in Ker(ξ)2\operatorname{Ker}(\xi)\cong\mathbb{Z}_{2}. Thus Ker(ξ)\operatorname{Ker}(\xi) is generated by m1m_{1}. Since ξ([f])=ξ(m2)\xi([f])=\xi(m_{2}), it follows that [f][f] is equal to either m2m_{2} or m1+m2=m3m_{1}+m_{2}=m_{3}. ∎

Let 𝒪^\hat{\mathcal{O}} be the orbifold obtained from the pared orbifold (M^0,P^αβ)(\hat{M}_{0},\hat{P}_{\alpha\beta}) by the orbifold surgery that replaces the index 44 of the edges e^2\hat{e}_{2} and e^3\hat{e}_{3} with the index 22. Then P^αβ\hat{P}_{\alpha\beta} shrinks into a singular point, vαβv_{\alpha\beta}, with link S2(2,2,2)S^{2}(2,2,2), and the image of α\alpha in π1(𝒪^)\pi_{1}(\hat{\mathcal{O}}) has order 2\leq 2 by Lemma 11.2. Since Γ^\hat{\Gamma} is generated by ff and α\alpha, π1(𝒪^)\pi_{1}(\hat{\mathcal{O}}) is either trivial, 2=D1\mathbb{Z}_{2}=D_{1} or a noncyclic dihedral group. By using Lemma 6.4, Theorem 4.1 and the fact that 𝒪^\hat{\mathcal{O}} has a singular point with link S2(2,2,2)S^{2}(2,2,2), we see that 𝒪^\hat{\mathcal{O}} is isomorphic to a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) with noncyclic dihedral orbifold fundamental group. Moreover, we may assume that d+=2d_{+}=2 and that vαβv_{\alpha\beta} is an endpoint of τ+\tau_{+}. By Lemma 6.5, we have H1(𝒪^;2)(2)2H_{1}(\hat{\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2}.

Lemma 11.4.

Under the above setting, |K(r)|=1|K(r)|=1 and so the edges e^i\hat{e}_{i} (i=1,2,3i=1,2,3) are all distinct.

Proof.

We first observe that α\alpha cannot be conjugate to b2ac2ab^{2}ac^{2}a. In fact, if α\alpha was conjugate to b2ac2ab^{2}ac^{2}a, then its image in π1(𝒪^)\pi_{1}(\hat{\mathcal{O}}) is trivial by Lemma 11.2 (cf. Lemma 10.1(2)), and so π1(𝒪^)\pi_{1}(\hat{\mathcal{O}}) is generated by the image of ff. This contradicts the fact that π1(𝒪^)\pi_{1}(\hat{\mathcal{O}}) is a noncyclic dihedral group. This observation together with Lemma 11.2 implies that α\alpha is conjugate to b2ab^{2}a and so [α]=[a]=m1Ker(ξ)[\alpha]=[a]=m_{1}\in\operatorname{Ker}(\xi). Moreover, [f]=m2[f]=m_{2} or m3m_{3} by Lemma 11.3. Hence H1(𝒪^;2)(2)2H_{1}(\hat{\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2} is generated by the meridians of the three edges e^i\hat{e}_{i} (i=1,2,3i=1,2,3) incident on the vertex vαβτ+v_{\alpha\beta}\in\partial\tau_{+}.

Now suppose on the contrary that |K(r)|=2|K(r)|=2. Then we see, by using Lemma 6.5, that the meridian of τ+\tau_{+} represents the trivial element of H1(𝒪^;2)H_{1}(\hat{\mathcal{O}};\mathbb{Z}_{2}) and the meridians of the remaining two edges incident on vαβτ+v_{\alpha\beta}\in\partial\tau_{+} represent the identical element of H1(𝒪^;2)H_{1}(\hat{\mathcal{O}};\mathbb{Z}_{2}). This contradicts the fact that H1(𝒪^;2)(2)2H_{1}(\hat{\mathcal{O}};\mathbb{Z}_{2})\cong(\mathbb{Z}_{2})^{2}. Hence |K(r)|=1|K(r)|=1. This implies that the the edges e^i\hat{e}_{i} (i=1,2,3i=1,2,3) incident on vαβτ+v_{\alpha\beta}\in\partial\tau_{+} are all distinct, as desired. ∎

Recall that the weights of the edges e^1\hat{e}_{1}, e^2\hat{e}_{2}, e^3\hat{e}_{3} of Σ(M^0)\Sigma(\hat{M}_{0}) are 2,4,42,4,4. Since e^2e^3\hat{e}_{2}\neq\hat{e}_{3} by Lemma 11.4, we can apply the orbifold surgery on (M^0,P^)(\hat{M}_{0},\hat{P}) of “type (2,4,4)(2,2,4)(2,4,4)\to(2,2,4)”, namely we can replace the index 44 of the edge e^2\hat{e}_{2} of the singular set Σ(M^0)\Sigma(\hat{M}_{0}) with the index 22, and leave the other indices, including the index 44 of e^3\hat{e}_{3}, unchanged. We denote the resulting orbifold by 𝒪^(2,2,4)\hat{\mathcal{O}}_{(2,2,4)}. By Lemma 11.2, α\alpha has order at most 22 in π1(𝒪^(2,2,4))\pi_{1}(\hat{\mathcal{O}}_{(2,2,4)}). Hence, by using Lemma 6.4, Theorem 4.1, and the fact that 𝒪^(2,2,4)\hat{\mathcal{O}}_{(2,2,4)} has a singular point with link S2(2,2,4)S^{2}(2,2,4), we see that 𝒪^(2,2,4)\hat{\mathcal{O}}_{(2,2,4)} is isomorphic to a spherical dihedral orbifold 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) with noncyclic dihedral orbifold fundamental group. Moreover, we may assume d+=4d_{+}=4 and that the parabolic locus PαβP_{\alpha\beta} degenerates into a singular point, vαβv_{\alpha\beta}, which is an endpoint of τ+\tau_{+}. It should be noted that the edge e^3\hat{e}_{3} of Σ(M^0)\Sigma(\hat{M}_{0}) corresponds to τ+\tau_{+}. (Here, we reset the notation, and the symbols 𝒪(r;d+,d){\mathcal{O}}(r;d_{+},d_{-}) and vαβv_{\alpha\beta} now represent objects different from those they had represented in the paragraph preceding Lemma 11.4.)

Case 1. d3d_{-}\geq 3. We apply the orbifold surgery on (M^0,P^)(\hat{M}_{0},\hat{P}) of “type (2,4,4)(2,4,2)(2,4,4)\to(2,4,2)”, namely we replace the index 44 of the edge e^3=τ+\hat{e}_{3}=\tau_{+} of the singular set Σ(M^0)\Sigma(\hat{M}_{0}) with the index 22, and leave the other indices, including the index 44 of e^2\hat{e}_{2}, unchanged. (This is possible by Lemma 11.4.) We denote the resulting orbifold by 𝒪^(2,4,2)\hat{\mathcal{O}}_{(2,4,2)}. By Lemma 11.2, α\alpha has order at most 22 in π1(𝒪^(2,4,2))\pi_{1}(\hat{\mathcal{O}}_{(2,4,2)}). Hence, again by using Lemma 6.4, Theorem 4.1, and the fact that 𝒪^(2,4,2)\hat{\mathcal{O}}_{(2,4,2)} has a singular point with link S2(2,4,2)S^{2}(2,4,2), we see that 𝒪^(2,4,2)\hat{\mathcal{O}}_{(2,4,2)} is isomorphic to a spherical dihedral orbifold with noncyclic dihedral orbifold fundamental group. Note that the edges e^2\hat{e}_{2} and τ\tau_{-} of Σ(𝒪^(2,4,2))\Sigma(\hat{\mathcal{O}}_{(2,4,2)}), which have indices 44 and d3d_{-}\geq 3, respectively, share a common endpoint (see Figure 12). But this cannot happen in any spherical dihedral orbifold, a contradiction.

Refer to caption
Figure 12. Since 𝒪^(2,2,4)𝒪(r;d+,d)\hat{\mathcal{O}}_{(2,2,4)}\cong{\mathcal{O}}(r;d_{+},d_{-}) with e^3=τ+\hat{e}_{3}=\tau_{+} is as in the left figure, 𝒪^(2,4,2)\hat{\mathcal{O}}_{(2,4,2)} is as in the right figure. The latter orbifold has a singular point with link S2(2,4,d)S^{2}(2,4,d_{-}) with d3d_{-}\geq 3, and so it cannot be a spherical dihedral orbifold.

Case 2. d=1d_{-}=1. Then (M^0,P^)(\hat{M}_{0},\hat{P}) is represented by a weighted graph (S3,K(r)τ+,w^)(S^{3},K(r)\cup\tau_{+},\hat{w}), such that K(r)=e^1e^2K(r)=\hat{e}_{1}\cup\hat{e}_{2} is a knot, e^3=τ+\hat{e}_{3}=\tau_{+}, and

w^(τ+)=4,w^(e^1)=2,w^(e^2)=4.\hat{w}(\tau_{+})=4,\quad\hat{w}(\hat{e}_{1})=2,\quad\hat{w}(\hat{e}_{2})=4.

Recall that the subset e^2e^3=e^2τ^+\hat{e}_{2}\cup\hat{e}_{3}=\hat{e}_{2}\cup\hat{\tau}_{+} of Σ(M^0)\Sigma(\hat{M}_{0}) are the images of the fixed point set of the involution ff on M0M_{0}. This implies that the map |M0||M^0||M_{0}|\to|\hat{M}_{0}| induced by the orbifold covering M0M^0M_{0}\to\hat{M}_{0} is the double branched covering branched over e^2e^3\hat{e}_{2}\cup\hat{e}_{3}. Hence (M0,P)(M_{0},P) is represented by the weighted graph illustrated in Figure 13. Here, we assume the extended Convention 6.2, and the two 44-valent vertices represent parabolic loci isomorphic to S2(2,2,2,2)S^{2}(2,2,2,2). Hence we see by Lemma 6.4 that H1(M0;)(2)3H_{1}(M_{0};\mathbb{Z})\cong(\mathbb{Z}_{2})^{3}, a contradiction.

Thus we have proved that the situation in Assumption 11.1 cannot occur. This completes the proof of the main Theorem 1.1.

Refer to caption
Figure 13. Since the orbifold covering M0M^0M_{0}\to\hat{M}_{0} induces the double branched covering |M0||M^0||M_{0}|\to|\hat{M}_{0}| branched over e^2e^3=e^2τ^+\hat{e}_{2}\cup\hat{e}_{3}=\hat{e}_{2}\cup\hat{\tau}_{+}, the orbifold (M0,P)(M_{0},P) is as illustrated in the right figure.

12. Appendix 1: Spherical orbifolds with dihedral orbifold fundamental groups

In this appendix, we classify the orientable spherical 33-orbifolds with dihedral orbifold fundamental groups (Proposition 12.2), and determine the (orientation-preserving) isometry groups of these orbifolds (Propositions 12.5 and 12.6). Proposition 12.2 is used in the proof of Theorem 4.1, and Corollary 12.7 is used in Section 9. Propositions 12.5 and 12.6 are used in the companion [4] of this paper. The classification of the spherical dihedral orbifolds is implicitly contained in Dunber’s work [21], which classifies the Seifert fibered orbifolds. The isometry groups of the dihedral spherical orbifolds obtained as the π\pi-orbifolds associated with 22-bridge links are calculated by [50, 27]. Moreover, in the recent papers [38, 39], Mecchia and Seppi classified the Seifert fibered spherical 33-orbifolds and calculated the isometry groups of such orbifolds. Since every spherical dihedral orbifold is Seifert fibered, the results in this section are implicitly contained in [38, 39]. However, we give a self-contained proof, because it is not a simple task to translate their results into the form we need.

We first recall basic facts concerning the 33-dimensional spherical geometry following [54, 50]. Let \mathcal{H} be the quaternion skew field. We use the symbol qq to denote a generic quaternion

q=a+bi+cj+dk(a,b,c,d).q=a+bi+cj+dk\in\mathcal{H}\quad(a,b,c,d\in\mathbb{R}).

(We believe this does not cause any confusion, even though qq is also used to denote the numerator of a rational number r=q/pr=q/p.) For each qq\in\mathcal{H}, q¯=abicjdk\bar{q}=a-bi-cj-dk denotes its conjugate, (q)=a\Re(q)=a denotes its real part, and |q||q| denotes its norm qq¯=a2+b2+c2+d2\sqrt{q\bar{q}}=\sqrt{a^{2}+b^{2}+c^{2}+d^{2}}. We identify SnS^{n} (n=1,2,3n=1,2,3) with the following subspaces of \mathcal{H}.

S3\displaystyle S^{3} :={q||q|=1}\displaystyle:=\{q\in\mathcal{H}\,|\,|q|=1\}
S2\displaystyle S^{2} :={q||q|=1,(q)=0}\displaystyle:=\{q\in\mathcal{H}\,|\,|q|=1,\quad\Re(q)=0\}
S1\displaystyle S^{1} :={z||z|=1}\displaystyle:=\{z\in\mathbb{C}\subset\mathcal{H}\,|\,|z|=1\}

The norm |||\cdot| induces a Euclidean metric on \mathcal{H}, and SnS^{n} (n=1,2,3n=1,2,3) are endowed with the induced metrics. The subspaces S3S^{3} and S1S^{1} form a Lie group with respect to the restriction of the product in \mathcal{H}. The group S3S^{3} acts on itself by conjugation leaving S2S^{2} invariant. This gives an epimorphism ψ:S3Isom+(S2)\psi:S^{3}\to\operatorname{Isom}^{+}(S^{2}), with kerψ=1\ker\psi=\langle-1\rangle, defined by

ψ(q)(x)=qxq¯(qS3,xS2).\psi(q)(x)=qx\bar{q}\quad(q\in S^{3},\ x\in S^{2}).

If q=cosθ+q0sinθq=\cos\theta+q_{0}\sin\theta with q0S2q_{0}\in S^{2}, then ψ(q)\psi(q) is the rotation of S2S^{2}, by angle 2θ2\theta, with fixed points ±q0\pm q_{0}.

For a positive integer nn, any cyclic subgroup of order nn (resp. any dihedral subgroup of order 2n2n) of Isom+(S2)\operatorname{Isom}^{+}(S^{2}) is conjugate to the subgroup n:=ψ(n)\mathbb{Z}_{n}:=\psi(\mathbb{Z}_{n}^{*}) (resp. 𝔻n:=ψ(𝔻n)\mathbb{D}_{n}:=\psi(\mathbb{D}_{n}^{*})), where n:=ω\mathbb{Z}_{n}^{*}:=\langle\omega\rangle and 𝔻n:=ω,j\mathbb{D}_{n}^{*}:=\langle\omega,\ j\rangle with ω=exp(πi/n)\omega=\exp(\pi i/n). Note that these groups are contained in the subgroup 𝔻S:=S1,j=S1S1j\mathbb{D}_{S}:=\langle S^{1},j\rangle=S^{1}\sqcup S^{1}j of S3S^{3}. Then the following hold (see, e.g. [50, Proposition 2.6]).

Lemma 12.1.

(1) If n2n\geq 2, then the normaliser N(n)N(\mathbb{Z}_{n}^{*}) of n\mathbb{Z}_{n}^{*} in S3S^{3} is equal to 𝔻S\mathbb{D}_{S}.

(2) If n3n\geq 3, then the normaliser N(𝔻n)N(\mathbb{D}_{n}^{*}) of 𝔻n\mathbb{D}_{n}^{*} in S3S^{3} is equal to 𝔻2n\mathbb{D}_{2n}^{*}. If n=2n=2, then N(𝔻n)N(\mathbb{D}_{n}^{*}) is equal to the binary octahedral group O=ψ1(O)O^{*}=\psi^{-1}(O), where O<Isom+(S2)O<\operatorname{Isom}^{+}(S^{2}) is the octahedral group obtained as the subgroup of Isom+(S2)\operatorname{Isom}^{+}(S^{2}) preserving the regular octahedron in the 33-dimensional Euclidean subspace i,j,k\langle i,j,k\rangle of \mathcal{H} spanned by the 66 vertices {±i,±j,±k}\{\pm i,\pm j,\pm k\}.

Let ϕ:S3×S3Isom+(S3)\phi:S^{3}\times S^{3}\to\operatorname{Isom}^{+}(S^{3}) be the homomorphism defined by

ϕ(q1,q2)(q)=q1qq21.\phi(q_{1},q_{2})(q)=q_{1}qq_{2}^{-1}.

Then ϕ\phi is an ephimorphism with Kerϕ=(1,1)2\operatorname{Ker}\phi=\langle(-1,-1)\rangle\cong\mathbb{Z}_{2}.

We occasionally identify S3S^{3}\subset\mathcal{H} with the unit sphere

S3={(z1,z2)2||z1|2+|z2|2=1}S^{3}=\{(z_{1},z_{2})\in\mathbb{C}^{2}\,|\,|z_{1}|^{2}+|z_{2}|^{2}=1\}

in 2\mathbb{C}^{2} by the correspondence q=z1+z2j(z1,z2)q=z_{1}+z_{2}j\leftrightarrow(z_{1},z_{2}). Let L:S1×S1Isom+(S3){\mathrm{L}}:S^{1}\times S^{1}\to\operatorname{Isom}^{+}(S^{3}) be the injective homomorphism defined by

L(ω1,ω2)(z1,z2)=(ω1z1,ω2z2).{\mathrm{L}}(\omega_{1},\omega_{2})(z_{1},z_{2})=(\omega_{1}z_{1},\omega_{2}z_{2}).

When ω=exp(2πikn)\omega_{\ell}=\exp(2\pi i\frac{k_{\ell}}{n_{\ell}}) (=1,2{\ell}=1,2), where kn\frac{k_{\ell}}{n_{\ell}} is a rational number, we write

(1) L(ω1,ω2)=L(k1n1,k2n2),\displaystyle{\mathrm{L}}(\omega_{1},\omega_{2})={\mathrm{L}}(\frac{k_{1}}{n_{1}},\frac{k_{2}}{n_{2}}),

because its restriction to the circles S3(×{0})S^{3}\cap(\mathbb{C}\times\{0\}) and S3({0}×)S^{3}\cap(\{0\}\times\mathbb{C}) are the ‘k1n1\frac{k_{1}}{n_{1}}-rotation’ and ‘k2n2\frac{k_{2}}{n_{2}}-rotation’, respectively. Though the symbol L(,){\mathrm{L}}(\cdot,\cdot) is used in two different ways, we believe this does not cause any confusion, because its meaning is clearly understood from the context according to whether \cdot is a unit complex or a rational number.

Observe that

ϕ(η1,η2)=L(η1η¯2,η1η2)((η1,η2)S1×S1).\phi(\eta_{1},\eta_{2})={\mathrm{L}}(\eta_{1}\bar{\eta}_{2},\eta_{1}\eta_{2})\quad((\eta_{1},\eta_{2})\in S^{1}\times S^{1}).

In particular, we have

(2) ϕ(S1×S1)=L(S1×S1)<Isom+(S3).\displaystyle\phi(S^{1}\times S^{1})={\mathrm{L}}(S^{1}\times S^{1})<\operatorname{Isom}^{+}(S^{3}).

Consider the isometries J:=ϕ(j,j)J:=\phi(j,j), J1:=ϕ(1,j)J_{1}:=\phi(1,j) and J2:=ϕ(j,1)J_{2}:=\phi(j,1), which acts on S32S^{3}\subset\mathbb{C}^{2} as follows.

J(z1,z2)=(z¯1,z¯2),J1(z1,z2)=(z2,z1),J2(z1,z2)=(z¯2,z¯1)J(z_{1},z_{2})=(\bar{z}_{1},\bar{z}_{2}),\ J_{1}(z_{1},z_{2})=(z_{2},-z_{1}),\ J_{2}(z_{1},z_{2})=(-\bar{z}_{2},\bar{z}_{1})

Observe J=J1J2J=J_{1}J_{2} and that

(3) ϕ(𝔻S×𝔻S)=L(S1×S1),J,J1,J,J12×2.\displaystyle\phi(\mathbb{D}_{S}\times\mathbb{D}_{S})=\langle{\mathrm{L}}(S^{1}\times S^{1}),J,J_{1}\rangle,\quad\langle J,J_{1}\rangle\cong\mathbb{Z}_{2}\times\mathbb{Z}_{2}.

In fact, ϕ(𝔻S×𝔻S)\phi(\mathbb{D}_{S}\times\mathbb{D}_{S}) is the split extension of L(S1×S1){\mathrm{L}}(S^{1}\times S^{1}) by J,J12×2\langle J,J_{1}\rangle\cong\mathbb{Z}_{2}\times\mathbb{Z}_{2}, where the action of J,J1\langle J,J_{1}\rangle on L(S1×S1){\mathrm{L}}(S^{1}\times S^{1}) by conjugation is given by the following formula.

(4) JL(ω1,ω2)J1=L(ω¯1,ω¯2),J1L(ω1,ω2)J11=L(ω2,ω1)\displaystyle J{\mathrm{L}}(\omega_{1},\omega_{2})J^{-1}={\mathrm{L}}(\bar{\omega}_{1},\bar{\omega}_{2}),\quad J_{1}{\mathrm{L}}(\omega_{1},\omega_{2})J_{1}^{-1}={\mathrm{L}}(\omega_{2},\omega_{1})

The following proposition gives a classification of the orientable spherical 33-orbifolds with dihedral orbifold fundamental groups.

Proposition 12.2.

Let 𝒪{\mathcal{O}} be an oriented spherical 33-orbifold. Then π1(𝒪)\pi_{1}({\mathcal{O}}) is isomorphic to a dihedral group, if and only if 𝒪{\mathcal{O}} is isomorphic to the orbifold, 𝒪(r;d1,d2){\mathcal{O}}(r;d_{1},d_{2}), represented by the weighted graph (S3,K(r)τ+τ,w)(S^{3},K(r)\cup\tau_{+}\cup\tau_{-},w) in Figure 6 for some rr\in\mathbb{Q} and coprime positive integers d1d_{1} and d2d_{2}, where ww is given by the following rule.

w(K(r))=2,w(τ+)=d1,w(τ)=d2.w(K(r))=2,\quad w(\tau_{+})=d_{1},\quad w(\tau_{-})=d_{2}.

In fact, 𝒪(r;d1,d2){\mathcal{O}}(r;d_{1},d_{2}) with r=q/pr=q/p is isomorphic to S3/ΓS^{3}/\Gamma, where Γ\Gamma is the subgroup of Isom+(S3)\operatorname{Isom}^{+}(S^{3}) given by

(5) Γ=L(k1pd2,k2pd1),JDnwith n=pd1d2\displaystyle\Gamma=\left\langle{\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}}),\ J\right\rangle\cong D_{n}\quad\mbox{with $n=pd_{1}d_{2}$}

for some integers k1k_{1} and k2k_{2} such that

(6) gcd(pd2,k1)=1,gcd(pd1,k2)=1,k2qk1(modp).\displaystyle\gcd(pd_{2},k_{1})=1,\quad\gcd(pd_{1},k_{2})=1,\quad k_{2}\equiv qk_{1}\pmod{p}.

Moreover, the spherical structure of 𝒪(r;d1,d2){\mathcal{O}}(r;d_{1},d_{2}) is unique, i.e., if Γ\Gamma^{\prime} is a subgroup of Isom+(S3)\operatorname{Isom}^{+}(S^{3}) such that S3/ΓS^{3}/\Gamma^{\prime} is isomorphic to 𝒪(r;d1,d2){\mathcal{O}}(r;d_{1},d_{2}) as oriented orbifolds, then Γ\Gamma^{\prime} is conjugate to the subgroup Γ\Gamma defined by (5).

Proof.

We first prove the only if part of the first assertion. Let Γ\Gamma be a subgroup of Isom+(S3)\operatorname{Isom}^{+}(S^{3}) isomorphic to the dihedral group DnD_{n}, and let ff and hh be the elements of Γ\Gamma such that

Γf,h|fn=1,h2=1,hfh1=f1.\Gamma\cong\langle f,h\,|\,f^{n}=1,h^{2}=1,hfh^{-1}=f^{-1}\rangle.

(Though the symbols Γ\Gamma, ff and hh are used in different meanings in the previous sections, we believe this does not cause any confusion.) We show that S3/ΓS^{3}/\Gamma is isomorphic to some 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}), such that n=pd1d2n=pd_{1}d_{2}.

Claim 12.3.

After taking conjugation in Isom+(S3)\operatorname{Isom}^{+}(S^{3}), we may assume f=L(k1pd2,k2pd1)f={\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}}), where pp, d1d_{1}, d2d_{2}, k1k_{1}, and k2k_{2} are positive integers such that gcd(d1,d2)=1\gcd(d_{1},d_{2})=1, gcd(pd2,k1)=1\gcd(pd_{2},k_{1})=1, gcd(pd1,k2)=1\gcd(pd_{1},k_{2})=1, and n=pd1d2n=pd_{1}d_{2}.

Proof of Claim 12.3.

Since any element of S3S^{3} is conjugate to an element in S1S^{1}, we may assume, by taking conjugation, that fϕ(S1×S1)=L(S1×S1)f\in\phi(S^{1}\times S^{1})={\mathrm{L}}(S^{1}\times S^{1}) (see (2)). Since ff has order nn, we may assume f=L(k1n,k2n)f={\mathrm{L}}(\frac{k_{1}^{\prime}}{n},\frac{k_{2}^{\prime}}{n}) for some integers k1k_{1}^{\prime} and k2k_{2}^{\prime} such that gcd(n,k1,k2)=1\gcd(n,k_{1}^{\prime},k_{2}^{\prime})=1. For =1,2\ell=1,2, set d=gcd(n,k)d_{\ell}=\gcd(n,k_{\ell}^{\prime}), n=ndn_{\ell}=\frac{n}{d_{\ell}} and k=kdk_{\ell}=\frac{k_{\ell}^{\prime}}{d_{\ell}}, so that f=L(k1n,k2n)=L(k1n1,k2n2)f={\mathrm{L}}(\frac{k_{1}^{\prime}}{n},\frac{k_{2}^{\prime}}{n})={\mathrm{L}}(\frac{k_{1}}{n_{1}},\frac{k_{2}}{n_{2}}), where gcd(k1,n1)=gcd(k2,n2)=1\gcd(k_{1},n_{1})=\gcd(k_{2},n_{2})=1. Note also that gcd(d1,d2)=gcd(n,k1,k2)=1\gcd(d_{1},d_{2})=\gcd(n,k_{1}^{\prime},k_{2}^{\prime})=1. Set p=gcd(n1,n2)p=\gcd(n_{1},n_{2}) and n=npn_{\ell}^{\prime}=\frac{n_{\ell}}{p} (=1,2{\ell}=1,2). Then n=lcm(n1,n2)=pn1n2n=\operatorname{lcm}(n_{1},n_{2})=pn_{1}^{\prime}n_{2}^{\prime}. Thus n1d1=n=pn1n2=n1n2n_{1}d_{1}=n=pn_{1}^{\prime}n_{2}^{\prime}=n_{1}n_{2}^{\prime} and so d1=n2d_{1}=n_{2}^{\prime}. Similarly we have d2=n1d_{2}=n_{1}^{\prime}. Hence we have n=pd1d2n=pd_{1}d_{2} and f=L(k1n1,k2n2)=L(k1pd2,k2pd1)f={\mathrm{L}}(\frac{k_{1}}{n_{1}},\frac{k_{2}}{n_{2}})={\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}}). ∎

Now consider the subgroup fpd1d2\langle f^{p}\rangle\cong\mathbb{Z}_{d_{1}d_{2}} generated by fp=L(k1d2,k2d1)f^{p}={\mathrm{L}}(\frac{k_{1}}{d_{2}},\frac{k_{2}}{d_{1}}). Since gcd(d1,d2)=1\gcd(d_{1},d_{2})=1, we have

fpfpd2×fpd1d1×d2.\langle f^{p}\rangle\cong\langle f^{pd_{2}}\rangle\times\langle f^{pd_{1}}\rangle\cong\mathbb{Z}_{d_{1}}\times\mathbb{Z}_{d_{2}}.

Note that

fpd2=L(0,k2d2d1)=L(0,1d1),fpd1=L(k1d1d2,0)=L(1d2,0).\langle f^{pd_{2}}\rangle=\langle{\mathrm{L}}(0,\frac{k_{2}d_{2}}{d_{1}})\rangle=\langle{\mathrm{L}}(0,\frac{1}{d_{1}})\rangle,\quad\langle f^{pd_{1}}\rangle=\langle{\mathrm{L}}(\frac{k_{1}d_{1}}{d_{2}},0)\rangle=\langle{\mathrm{L}}(\frac{1}{d_{2}},0)\rangle.

Hence we have

fp=L(0,1d1)×L(1d2,0).\langle f^{p}\rangle=\langle{\mathrm{L}}(0,\frac{1}{d_{1}})\rangle\times\langle{\mathrm{L}}(\frac{1}{d_{2}},0)\rangle.

Thus S3/fpS^{3}/\langle f^{p}\rangle is the orbifold with underlying space S3S^{3} and with singular set the Hopf link, where one component has index d1d_{1} and the other component has index d2d_{2}. To give a precise description of this orbifold, identify S3S^{3} with the join S1S1S^{1}*S^{1}, by the correspondence (tz1,1t2z2)tz1+(1t)z2(tz_{1},\sqrt{1-t^{2}}z_{2})\leftrightarrow tz_{1}+(1-t)z_{2}. Thus the first and second factor circles of S1S1S^{1}*S^{1} correspond to the circles S1×{0}S^{1}\times\{0\} and {0}×S1\{0\}\times S^{1} in S32S^{3}\subset\mathbb{C}^{2}, respectively. For ωS1\omega\in S^{1}, let L(ω){\mathrm{L}}(\omega) be the isometry of S1S^{1} defined by L(ω)(z)=ωz{\mathrm{L}}(\omega)(z)=\omega z (zS1z\in S^{1}). Then the isometry L(ω1,ω2){\mathrm{L}}(\omega_{1},\omega_{2}) is identified with the self-homeomorphism L(ω1)L(ω2){\mathrm{L}}(\omega_{1})*{\mathrm{L}}(\omega_{2}) of S1S1S^{1}*S^{1}, defined by

(L(ω1)L(ω2))(tz1+(1t)z2)=tω1z1+(1t)ω2z2.({\mathrm{L}}(\omega_{1})*{\mathrm{L}}(\omega_{2}))(tz_{1}+(1-t)z_{2})=t\omega_{1}z_{1}+(1-t)\omega_{2}z_{2}.

Under the above convention, the orbifold S3/fpS^{3}/\langle f^{p}\rangle is described as follows. The underlying space of the orbifold is given by

|S3/fp|(S1/L(1d2))(S1/L(1d1))S1S1S3,|S^{3}/\langle f^{p}\rangle|\cong\left(S^{1}/{\mathrm{L}}(\frac{1}{d_{2}})\right)*\left(S^{1}/{\mathrm{L}}(\frac{1}{d_{1}})\right)\cong S^{1}*S^{1}\cong S^{3},

and the singular set is the union of the two circles which gives the join structure of S3S^{3}, where the first factor circle (which corresponds to S1/L(1d2)S^{1}/{\mathrm{L}}(\frac{1}{d_{2}})) has index d1d_{1} and the second factor circle (which corresponds to S1/L(1d1)S^{1}/{\mathrm{L}}(\frac{1}{d_{1}})) has index d2d_{2}. Here, L(1d){\mathrm{L}}(\frac{1}{d_{\ell}}) denotes L(e2πid){\mathrm{L}}(e^{\frac{2\pi i}{d_{\ell}}}) as in (1).

The isometry ff descends to the periodic isomorphism of the orbifold S3/fpS1S1S^{3}/\langle f^{p}\rangle\cong S^{1}*S^{1} given by L(k1p)L(k2p){\mathrm{L}}(\frac{k_{1}}{p})*{\mathrm{L}}(\frac{k_{2}}{p}), because the periodic map L(k1pd2){\mathrm{L}}(\frac{k_{1}}{pd_{2}}) (resp. L(k2pd1){\mathrm{L}}(\frac{k_{2}}{pd_{1}})) on S1S^{1} descends to the periodic map L(k1p){\mathrm{L}}(\frac{k_{1}}{p}) (resp. L(k2p){\mathrm{L}}(\frac{k_{2}}{p})) on the circle S1/L(1d2)S^{1}/{\mathrm{L}}(\frac{1}{d_{2}}) (resp. S1/L(1d1)S^{1}/{\mathrm{L}}(\frac{1}{d_{1}})). Note that L(k1p)L(k2p)=L(1p)L(qp)\langle{\mathrm{L}}(\frac{k_{1}}{p})*{\mathrm{L}}(\frac{k_{2}}{p})\rangle=\langle{\mathrm{L}}(\frac{1}{p})*{\mathrm{L}}(\frac{q}{p})\rangle, with qk11k2(modp)q\equiv k_{1}^{-1}k_{2}\pmod{p}, where k11k_{1}^{-1} is the inverse of k1k_{1} in the multiplicative group (p)×(\mathbb{Z}_{p})^{\times} (cf. Notation 1.3(2)). Hence we see that the orbifold S3/fS^{3}/\langle f\rangle is isomorphic to the orbifold, 𝒪(L(p,q),d1,d2){\mathcal{O}}(L(p,q),d_{1},d_{2}), with underlying space the lens space, L(p,q)L(p,q), and with singular set the union of the core circles of the standard genus 11 Heegaard splitting of L(p,q)L(p,q) with indices d1d_{1} and d2d_{2}, respectively. (Though the notation L(p,q)L(p,q) looks similar to the notation L(,){\mathrm{L}}(\cdot,\cdot) in (1), we believe there is no fear of confusion.)

Since h2=1h^{2}=1 and hfh1=f1hfh^{-1}=f^{-1}, we see by using Lemma 12.1(1) that h=ϕ(q1,q2)h=\phi(q_{1},q_{2}) for some (q1,q2)S1j×S1j(q_{1},q_{2})\in S^{1}j\times S^{1}j. Since any element of S1jS^{1}j is conjugate to jj by an element of S1S^{1}, we may assume h=ϕ(j,j)=Jh=\phi(j,j)=J, and so h(z1,z2)=(z¯1,z¯2)h(z_{1},z_{2})=(\bar{z}_{1},\bar{z}_{2}). This implies that the involution hh of S3S^{3} descends to the hyper-elliptic involution of |S3/f|L(p,q)|S^{3}/\langle f\rangle|\cong L(p,q). Recall that (i) the quotient map determined by the hyper-elliptic involution gives the double branched covering of S3S^{3} branched over the 22-bridge link K(q/p)K(q/p) and that (ii) the core circles of the genus 11 Heegaard splitting project to the upper and lower tunnels, respectively. Hence, the quotient S3/ΓS^{3}/\Gamma, with Γ=f,hDn\Gamma=\langle f,h\rangle\cong D_{n}, is isomorphic to the orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}). This completes the proof of the only if part of the first assertion. The proof also shows that the group Γ\Gamma is given by the formula (5) for some integers k1k_{1} and k2k_{2} satisfying the condition (6).

The if part of the first assertion follows from the above argument and the following claim.

Claim 12.4.

For any rational number r=q/pr=q/p and a pair of coprime integers (d1,d2)(d_{1},d_{2}), there is a pair (k1,k2)(k_{1},k_{2}) of integers which satisfies the condition (6).

Proof of Claim 12.4.

Consider the homomorphism

Ψ:(pd2)××(pd1)×(p)××(p)×(p)×,\Psi:(\mathbb{Z}_{pd_{2}})^{\times}\times(\mathbb{Z}_{pd_{1}})^{\times}\to(\mathbb{Z}_{p})^{\times}\times(\mathbb{Z}_{p})^{\times}\to(\mathbb{Z}_{p})^{\times},

where the first homomorphism is the product of the natural projections and the second homomorphism maps (k1,k2)(p)××(p)×(k_{1},k_{2})\in(\mathbb{Z}_{p})^{\times}\times(\mathbb{Z}_{p})^{\times} to k11k2(p)×k_{1}^{-1}k_{2}\in(\mathbb{Z}_{p})^{\times}. Then both of the two homomorphisms are surjective and so is their composition Ψ\Psi. Regard the numerator qq of the rational number r=q/pr=q/p as an element of (p)×(\mathbb{Z}_{p})^{\times}, and let (k1,k2)(k_{1},k_{2}) be a pair of integers which projects to an element in the inverse image Ψ1(q)\Psi^{-1}(q). Then (k1,k2)(k_{1},k_{2}) satisfies the condition (6). ∎

Finally we prove the uniqueness of the spherical structure on the orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}). The preceding arguments show that the triple (q/p,d1,d2)××(q/p,d_{1},d_{2})\in\mathbb{Q}\times\mathbb{N}\times\mathbb{N} uniquely determines a dihedral subgroup Γ<Isom+(S3)\Gamma<\operatorname{Isom}^{+}(S^{3}), up to conjugation, such that S3/ΓS^{3}/\Gamma is isomorphic to 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) as oriented orbifolds. Thus we have only to show that there are no unexpected orientation-preserving topological isomorphism between two orbifolds, 𝒪(q/p;d1,d2)=S3/Γ{\mathcal{O}}(q/p;d_{1},d_{2})=S^{3}/\Gamma and 𝒪(q/p;d1,d2)=S3/Γ{\mathcal{O}}(q^{\prime}/p^{\prime};d_{1}^{\prime},d_{2}^{\prime})=S^{3}/\Gamma^{\prime}.

Assume that 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) and 𝒪(q/p;d1,d2){\mathcal{O}}(q^{\prime}/p^{\prime};d_{1}^{\prime},d_{2}^{\prime}) are isomorphic as oriented orbifolds. Then pd1d2=pd1d2pd_{1}d_{2}=p^{\prime}d_{1}^{\prime}d_{2}^{\prime} and {d1,d2}={d1,d2}\{d_{1},d_{2}\}=\{d_{1}^{\prime},d_{2}^{\prime}\}, because they have isomorphic orbifold fundamental groups and the same index sets of the singular sets. In particular we have p=pp=p^{\prime}.

Suppose first that n:=pd1d23n:=pd_{1}d_{2}\geq 3. Then DnD_{n} has the unique cyclic subgroup of index 22, and so each of 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) and 𝒪(q/p;d1,d2){\mathcal{O}}(q^{\prime}/p^{\prime};d_{1}^{\prime},d_{2}^{\prime}) has the unique double orbifold covering with cyclic orbifold fundamental group. The underlying spaces of the covering orbifolds are the lens spaces L(p,q)L(p,q) and L(p,q)L(p^{\prime},q^{\prime}), respectively. Hence, by the classification of lens spaces, we have p=pp=p^{\prime} and either qq(modp)q\equiv q^{\prime}\pmod{p} or qq1(modp)qq^{\prime}\equiv 1\pmod{p}. Moreover, by using the uniqueness of the genus one Heegaard splittings (see [12, 13]), we see that 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) and 𝒪(q/p;d1,d2){\mathcal{O}}(q^{\prime}/p^{\prime};d_{1}^{\prime},d_{2}^{\prime}) are isomorphic as oriented orbifolds if and only if one of the following conditions hold.

  1. (1)

    p=pp=p^{\prime}, qq(modp)q\equiv q^{\prime}\pmod{p}, and (d1,d2)=(d1,d2)(d_{1},d_{2})=(d_{1}^{\prime},d_{2}^{\prime}).

  2. (2)

    p=pp=p^{\prime}, qq1(modp)qq^{\prime}\equiv 1\pmod{p}, and (d1,d2)=(d2,d1)(d_{1},d_{2})=(d_{2}^{\prime},d_{1}^{\prime}).

In both cases, we can see that the subgroups Γ\Gamma and Γ\Gamma^{\prime} are conjugate in Isom+(S3)\operatorname{Isom}^{+}(S^{3}).

In the exceptional case when n:=pd1d2=2n:=pd_{1}d_{2}=2, we have either (i) p=p=1p=p^{\prime}=1 and {d1,d2}={d1,d2}={1,2}\{d_{1},d_{2}\}=\{d_{1}^{\prime},d_{2}^{\prime}\}=\{1,2\} or (ii) p=p=2p=p^{\prime}=2 and d1=d2=d1=d2=1d_{1}=d_{2}=d_{1}^{\prime}=d_{2}^{\prime}=1. We can easily see that the subgroups Γ\Gamma and Γ\Gamma^{\prime} are conjugate in Isom+(S3)\operatorname{Isom}^{+}(S^{3}).

This completes the uniqueness of the spherical structure. ∎

Next, we calculate the (orientation-preserving) isometry group of the dihedral spherical 33-orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}). If (d1,d2)=(1,1)(d_{1},d_{2})=(1,1), then 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is the π\pi-orbifold, 𝒪(q/p){\mathcal{O}}(q/p), associated with the 22-bridge link K(q/p)K(q/p) (cf. [11]) and its isometry group is calculated by [50, Theorem 4.1] and [27, Corollary 3.2.11]. (There are errors in [50, Theorem 4.1] for the special case when p=1p=1, 22. There are also misprints for the generic case in the statement of Theorem 4.1, though the correct result can be found in the tables in [50, p.184].)

Proposition 12.5.

The orientation-preserving isometry group of the spherical orbifold 𝒪(q/p):=𝒪(q/p;1,1){\mathcal{O}}(q/p):={\mathcal{O}}(q/p;1,1) is described as follows.

  1. (1)

    If q±1(modp)q\not\equiv\pm 1\pmod{p}, then the following holds.

    Isom+(𝒪(q/p)){(2)2if q21(modp)D4if p is odd and q21(modp)or if p is even and q2p+1(mod2p)(2)3if p is even and q21(mod2p)\operatorname{Isom}^{+}({\mathcal{O}}(q/p))\cong\begin{cases}(\mathbb{Z}_{2})^{2}&\text{if $q^{2}\not\equiv 1\pmod{p}$}\\ D_{4}&\text{if $p$ is odd and $q^{2}\equiv 1\pmod{p}$}\\ &\text{or if $p$ is even and $q^{2}\equiv p+1\pmod{2p}$}\\ (\mathbb{Z}_{2})^{3}&\text{if $p$ is even and $q^{2}\equiv 1\pmod{2p}$}\end{cases}
  2. (2)

    If q±1(modp)q\equiv\pm 1\pmod{p}, then then the following holds.

    Isom+(𝒪(q/p)){S12if p is odd and 3S1(2)2if p is even and 4(S1×S1)(2)2if p=2(S1×S1)2if p=1\operatorname{Isom}^{+}({\mathcal{O}}(q/p))\cong\begin{cases}S^{1}\rtimes\mathbb{Z}_{2}&\text{if $p$ is odd and $\geq 3$}\\ S^{1}\rtimes(\mathbb{Z}_{2})^{2}&\text{if $p$ is even and $\geq 4$}\\ (S^{1}\times S^{1})\rtimes(\mathbb{Z}_{2})^{2}&\text{if $p=2$}\\ (S^{1}\times S^{1})\rtimes\mathbb{Z}_{2}&\text{if $p=1$}\end{cases}

In the remainder of this section, we treat the remaining case (d1,d2)(1,1)(d_{1},d_{2})\neq(1,1). In the very special case, when p=1p=1 and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}, we call 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2) the trivial θ\theta-orbifold, because its singular set is the trivial θ\theta-curve in S3S^{3}. Then we have the following proposition.

Proposition 12.6.

The orientation-preserving isometry group of the spherical dihedral orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) with (d1,d2)(1,1)(d_{1},d_{2})\neq(1,1) is described as follows.

  1. (1)

    Isom+(𝒪(q/p;d1,d2))(2)2\operatorname{Isom}^{+}({\mathcal{O}}(q/p;d_{1},d_{2}))\cong(\mathbb{Z}_{2})^{2}, except when 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is isomorphic to the trivial θ\theta-orbifold 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2), i.e. except when p=1p=1 and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}.

  2. (2)

    For the the trivial θ\theta-orbifold 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2), we have Isom+(𝒪(0/1;1,2))D3×2\operatorname{Isom}^{+}({\mathcal{O}}(0/1;1,2))\cong D_{3}\times\mathbb{Z}_{2}.

Refer to caption
Figure 14. Isom+(𝒪(q/p;d1,d2))(2)2\operatorname{Isom}^{+}({\mathcal{O}}(q/p;d_{1},d_{2}))\cong(\mathbb{Z}_{2})^{2} if (d1,d2)(1,1)(d_{1},d_{2})\neq(1,1) and 𝒪(q/p;d1,d2))≇𝒪(0/1;1,2){\mathcal{O}}(q/p;d_{1},d_{2}))\not\cong{\mathcal{O}}(0/1;1,2).
Refer to caption
Figure 15. Isom+(𝒪(0/1;1,2))D3×2\operatorname{Isom}^{+}({\mathcal{O}}(0/1;1,2))\cong D_{3}\times\mathbb{Z}_{2}. The singular set of the trivial θ\theta-orbifold 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2) is the standardly embedded θ\theta-graph in S2S3S^{2}\subset S^{3}, consisting of three geodesics joining the north and south poles, which are permuted by the 2π/32\pi/3-rotation around the earth axis. The orientation-preserving isometry group is visualised as the product of the dihedral group D3D_{3} generated by the π\pi-rotations about the three great circles containing the singular edges and cyclic group 2\mathbb{Z}_{2} generated by the π\pi-rotation about the equator.

Before proving the proposition, we give the following consequence of the proposition (and the orbifold theorem), which is used in the proof of the main theorem.

Corollary 12.7.

Consider a spherical orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) with (d1,d2)(1,1)(d_{1},d_{2})\neq(1,1), and let gg be an orientation-preserving involution of the orbifold. Then the following hold.

  1. (1)

    Except when p=1p=1 and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}, (i.e. except when 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is isomorphic to the trivial θ\theta-orbifold 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2)), gg stabilises the edges τ+\tau_{+} and τ\tau_{-} of the singular set (when it is contained in the singular set).

  2. (2)

    If d1,d22d_{1},d_{2}\geq 2, then gg does not stabilise any edge of the singular set different from τ±\tau_{\pm}.

Proof of Corollary 12.7.

By the orbifold theorem, we may assume gg is an isometry of the spherical orbifold. (This is proved by applying the orbifold theorem to the finite group action on the universal cover S3S^{3} of 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) generated by a lift of gg and the covering transformation group.) On the other hand, the action of Isom+(𝒪(q/p;d1,d2))\operatorname{Isom}^{+}({\mathcal{O}}(q/p;d_{1},d_{2})) in the generic case is as illustrated in Figure 14. (See also [4, Figure 6-8], and replace the weights \infty with 22, then we obtain the desired visualisation, besides the exceptional case.) The exceptional case where the orbifold is the trivial θ\theta-orbifold is illustrated in Figure 15. The assertion (1) is now obvious from Figure 14. The assertion (2) also follows from the figure by noting that K(r)K(r) consists of four edges if d1,d22d_{1},d_{2}\geq 2 (otherwise, K(r)K(r) consists of two edges). ∎

The proof of Proposition 12.6 presented below is parallel to that of [50, Theorem 4.1]. Consider the dihedral spherical 33-orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) with (d1,d2)(1,1)(d_{1},d_{2})\neq(1,1). By Proposition 12.2, the orbifold fundamental group π1(𝒪(q/p;d1,d2))\pi_{1}({\mathcal{O}}(q/p;d_{1},d_{2})) is identified with the subgroup

Γ=L(k1pd2,k2pd1),J=L(ω1,ω2),J<Isom+(S3)\Gamma=\left\langle{\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}}),\ J\right\rangle=\langle{\mathrm{L}}(\omega_{1},\omega_{2}),\ J\rangle<\operatorname{Isom}^{+}(S^{3})

where ω1=exp(2πik1pd2)\omega_{1}=\exp(2\pi i\frac{k_{1}}{pd_{2}}), ω2=exp(2πik2pd1)\omega_{2}=\exp(2\pi i\frac{k_{2}}{pd_{1}}) for some integers k1k_{1} and k2k_{2} satisfying the condition (6). Pick (η1,η2)S1×S1(\eta_{1},\eta_{2})\in S^{1}\times S^{1} such that (ω1,ω2)=(η1η¯2,η1η2)(\omega_{1},\omega_{2})=(\eta_{1}\bar{\eta}_{2},\eta_{1}\eta_{2}). Then Γ=ϕ(η1,η2),ϕ(j,j)\Gamma=\langle\phi(\eta_{1},\eta_{2}),\phi(j,j)\rangle. Set

Γ~:=ϕ1(Γ)=(η1,η2),(j,j)<S3×S3.\tilde{\Gamma}:=\phi^{-1}(\Gamma)=\langle(\eta_{1},\eta_{2}),(j,j)\rangle<S^{3}\times S^{3}.

Then Isom+𝒪(q/p;d1,d2)N(Γ~)/Γ~\operatorname{Isom}^{+}{\mathcal{O}}(q/p;d_{1},d_{2})\cong N(\tilde{\Gamma})/\tilde{\Gamma}, where N(Γ~)N(\tilde{\Gamma}) is the normaliser of Γ~\tilde{\Gamma} in S3×S3S^{3}\times S^{3}.

For =1,2\ell=1,2, set Γ~=pr(Γ~)\tilde{\Gamma}_{\ell}=\mathrm{pr}_{\ell}(\tilde{\Gamma}), where pr:S3×S3S3\mathrm{pr}_{\ell}:S^{3}\times S^{3}\to S^{3} is the projection to the \ell-th factor. Then Γ~=η,j=𝔻m\tilde{\Gamma}_{\ell}=\langle\eta_{\ell},j\rangle=\mathbb{D}_{m_{\ell}}^{*} for some positive integer mm_{\ell}. Then the following lemma is obvious from the definition of 𝔻m\mathbb{D}_{m_{\ell}}^{*}, where o()o(\cdot) denotes the order of a group element.

Lemma 12.8.

(1) o(η2)=mo(\eta_{\ell}^{2})=m_{\ell}.

(2) If mm_{\ell} is even, then o(η)=2mo(\eta_{\ell})=2m_{\ell}. If mm_{\ell} is odd, then o(η)o(\eta_{\ell}) is either mm_{\ell} or 2m2m_{\ell}.

Note that the orientation-reversing isometry c:S3S3c:S^{3}\to S^{3}, defined by c(q)=q¯c(q)=\bar{q}, acts on Isom+(S3)\operatorname{Isom}^{+}(S^{3}) by conjugation, as follows:

cϕ(q1,q2)c1=ϕ(q2,q1)c\phi(q_{1},q_{2})c^{-1}=\phi(q_{2},q_{1})

Hence, we assume m1m2m_{1}\leq m_{2} without loss of generality.

Lemma 12.9.

(1) 2m1m22\leq m_{1}\leq m_{2}.

(2) If m1=2m_{1}=2, then m2=2m2m_{2}=2m_{2}^{\prime} for some odd integer m2m_{2}^{\prime}, and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}. Moreover, m1=m2=2m_{1}=m_{2}=2 if and only if p=1p=1.

Proof.

(1) Suppose on the contrary that m1=1m_{1}=1. Then η1=±1\eta_{1}=\pm 1, and so (ω1,ω2)=±(η¯2,η2)(\omega_{1},\omega_{2})=\pm(\bar{\eta}_{2},\eta_{2}). This implies pd2=o(ω1)=o(ω2)=pd1pd_{2}=o(\omega_{1})=o(\omega_{2})=pd_{1} and therefore d1=d2d_{1}=d_{2}. Since gcd(d1,d2)=1\gcd(d_{1},d_{2})=1, we have d1=d2=1d_{1}=d_{2}=1, a contradiction.

(2) Suppose m1=2m_{1}=2. Then η1=±i\eta_{1}=\pm i, and so (ω1,ω2)=±(iη¯2,iη2)(\omega_{1},\omega_{2})=\pm(i\bar{\eta}_{2},i\eta_{2}). By using Lemma 12.8, we can verify the following, from which the assertion (2) follows.

  1. (i)

    If m2m_{2} is odd, then (o(ω1),o(ω2))=(4m2,4m2)(o(\omega_{1}),o(\omega_{2}))=(4m_{2},4m_{2}) and so d1=d2=1d_{1}=d_{2}=1 as in (1), a contradiction.

  2. (ii)

    If m2=2m2m_{2}=2m_{2}^{\prime} for some odd integer m2m_{2}^{\prime}, then ω1m2=ω2m2=±1\omega_{1}^{m_{2}^{\prime}}=-\omega_{2}^{m_{2}^{\prime}}=\pm 1 and so {pd2,pd1}={o(ω1),o(ω2)}={m2,2m2}\{pd_{2},pd_{1}\}=\{o(\omega_{1}),o(\omega_{2})\}=\{m_{2}^{\prime},2m_{2}^{\prime}\}. Hence we have p=m2p=m_{2}^{\prime} and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}.

  3. (iii)

    If m2=4m2m_{2}=4m_{2}^{\prime} for some integer m2m_{2}^{\prime}, then ω12m2=ω22m2=±i\omega_{1}^{2m_{2}^{\prime}}=-\omega_{2}^{2m_{2}^{\prime}}=\pm i and so o(ω1)=o(ω2)=8m2o(\omega_{1})=o(\omega_{2})=8m_{2}^{\prime}. Hence d1=d2=1d_{1}=d_{2}=1, a contradiction.

Lemma 12.10.

Except for the special case where p=1p=1 and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}, namely except when 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is the trivial θ\theta-orbifold, we have

N(Γ~)<𝔻2m1×𝔻2m2<𝔻S×𝔻S.N(\tilde{\Gamma})<\mathbb{D}_{2m_{1}}^{*}\times\mathbb{D}_{2m_{2}}^{*}<\mathbb{D}_{S}\times\mathbb{D}_{S}.
Proof.

If m13m_{1}\geq 3, then Lemma 12.1 implies N(Γ~)=𝔻2mN(\tilde{\Gamma}_{\ell})=\mathbb{D}_{2m_{\ell}}^{*} for each =1,2\ell=1,2 (because m2m1m_{2}\geq m_{1} by assumption), and hence we have N(Γ~)<N(Γ~1)×N(Γ~2)<𝔻2m1×𝔻2m2N(\tilde{\Gamma})<N(\tilde{\Gamma}_{1})\times N(\tilde{\Gamma}_{2})<\mathbb{D}_{2m_{1}}^{*}\times\mathbb{D}_{2m_{2}}^{*}.

Since m2m12m_{2}\geq m_{1}\geq 2 by Lemma 12.9(1), we have only to treat the case where m1=2m_{1}=2. Since we exclude the case where p=1p=1 and {d1,d2}={1,2}\{d_{1},d_{2}\}=\{1,2\}, Lemma 12.9(2) implies m23m_{2}\geq 3, and so N(Γ~2)=𝔻2m2N(\tilde{\Gamma}_{2})=\mathbb{D}_{2m_{2}}^{*}. On the other hand, since m1=2m_{1}=2, we see by Lemma 12.1 that N(Γ~1)=ON(\tilde{\Gamma}_{1})=O^{*}. Hence N(Γ~)<O×𝔻2m2N(\tilde{\Gamma})<O^{*}\times\mathbb{D}_{2m_{2}}^{*}.

Now observe that the decomposition 𝔻S=S1S1j\mathbb{D}_{S}=S^{1}\sqcup S^{1}j induces the decomposition of Γ~<𝔻S×𝔻S\tilde{\Gamma}<\mathbb{D}_{S}\times\mathbb{D}_{S} into the following two non-empty subsets.

Γ~(1):=Γ~(S1×S1)andΓ~(j):=Γ~(S1j×S1j).\tilde{\Gamma}^{(1)}:=\tilde{\Gamma}\cap(S^{1}\times S^{1})\quad\mbox{and}\quad\tilde{\Gamma}^{(j)}:=\tilde{\Gamma}\cap(S^{1}j\times S^{1}j).

Note that pr1(Γ~(1))=i={±1,±i}\mathrm{pr}_{1}(\tilde{\Gamma}^{(1)})=\langle i\rangle=\{\pm 1,\pm i\} and pr1(Γ~(j))=ij={±j,±k}\mathrm{pr}_{1}(\tilde{\Gamma}^{(j)})=\langle i\rangle j=\{\pm j,\pm k\}. Pick an arbitrary element (q1,q2)N(Γ~)(q_{1},q_{2})\in N(\tilde{\Gamma}). Then q2𝔻2m2<𝔻Sq_{2}\in\mathbb{D}_{2m_{2}}^{*}<\mathbb{D}_{S}, and so the inner-automorphism of S3S^{3} determined by q2q_{2} preserves the subgroup S1<𝔻SS^{1}<\mathbb{D}_{S}. Thus the inner-automorphism of S3×S3S^{3}\times S^{3} determined by (q1,q2)(q_{1},q_{2}) preserves the subset Γ~(1)\tilde{\Gamma}^{(1)} of Γ~=Γ~(1)Γ~(j)\tilde{\Gamma}=\tilde{\Gamma}^{(1)}\sqcup\tilde{\Gamma}^{(j)}. Hence the inner-automorphism of S3S^{3} determined by q1q_{1} preserves the subgroup pr1(Γ~(1))=i\mathrm{pr}_{1}(\tilde{\Gamma}^{(1)})=\langle i\rangle, and so it preserves the subset {±i}\{\pm i\}, i.e., q1iq¯1=±iq_{1}i\bar{q}_{1}=\pm i. By the description of OO^{*} in Lemma 12.1, this implies that q1𝔻2<𝔻2m1q_{1}\in\mathbb{D}_{2}^{*}<\mathbb{D}_{2m_{1}}^{*}. Hence (q1,q2)𝔻2m1×𝔻2m2(q_{1},q_{2})\in\mathbb{D}_{2m_{1}}^{*}\times\mathbb{D}_{2m_{2}}^{*}, as desired. ∎

Lemma 12.11.

The normaliser N(Γ)N(\Gamma) of Γ\Gamma in Isom+S3\operatorname{Isom}^{+}S^{3} is contained in L(S1×S1),J\langle{\mathrm{L}}(S^{1}\times S^{1}),J\rangle.

Proof.

By the formula (3) and Lemma 12.10, we have

N(Γ)=ϕ(N(Γ~))<ϕ(𝔻S×𝔻S)=L(S1×S1),J,J1.N(\Gamma)=\phi(N(\tilde{\Gamma}))<\phi(\mathbb{D}_{S}\times\mathbb{D}_{S})=\langle{\mathrm{L}}(S^{1}\times S^{1}),J,J_{1}\rangle.

Since JΓJ\in\Gamma, we have only to show that J1N(Γ)J_{1}\notin N(\Gamma). To this end, recall that Γ=L(k1pd2,k2pd1),J\Gamma=\langle{\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}}),J\rangle. Now suppose on the contrary that J1N(Γ)J_{1}\in N(\Gamma). Then the conjugation by J1J_{1} preserves the subgroup L(k1pd2,k2pd1)\langle{\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}})\rangle and we have J1L(k1pd2,k2pd1)J11=L(k2pd1,k1pd2)J_{1}{\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}})J_{1}^{-1}={\mathrm{L}}(\frac{k_{2}}{pd_{1}},\frac{k_{1}}{pd_{2}}) by (4). Thus we have d1=d2d_{1}=d_{2} and so d1=d2=1d_{1}=d_{2}=1, a contradiction. Hence J1N(Γ)J_{1}\notin N(\Gamma) as desired. ∎

Lemma 12.12.

Except when 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is the trivial θ\theta-orbifold, we have the following.

N(Γ)\displaystyle N(\Gamma) =L(k12pd2,k22pd1),L(12,0),L(0,12),J\displaystyle=\left\langle{\mathrm{L}}(\frac{k_{1}}{2pd_{2}},\frac{k_{2}}{2pd_{1}}),\ {\mathrm{L}}(\frac{1}{2},0),\ {\mathrm{L}}(0,\frac{1}{2}),\ J\right\rangle
L(k12pd2,k22pd1),L(12,0),L(0,12)J\displaystyle\cong\left\langle{\mathrm{L}}(\frac{k_{1}}{2pd_{2}},\frac{k_{2}}{2pd_{1}}),\ {\mathrm{L}}(\frac{1}{2},0),\ {\mathrm{L}}(0,\frac{1}{2})\right\rangle\rtimes\langle J\rangle
Proof.

Recall that Γ=L(ω1,ω2),J\Gamma=\langle{\mathrm{L}}(\omega_{1},\omega_{2}),J\rangle where ω1=exp(2πik1pd2)\omega_{1}=\exp(2\pi i\frac{k_{1}}{pd_{2}}) and ω2=exp(2πik2pd1)\omega_{2}=\exp(2\pi i\frac{k_{2}}{pd_{1}}). Set ω1=exp(πik1pd2)\sqrt{\omega_{1}}=\exp(\pi i\frac{k_{1}}{pd_{2}}) and ω2=exp(πik2pd1)\sqrt{\omega_{2}}=\exp(\pi i\frac{k_{2}}{pd_{1}}). Suppose an element L(ζ1,ζ2)L(S1×S1){\mathrm{L}}(\zeta_{1},\zeta_{2})\in{\mathrm{L}}(S^{1}\times S^{1}) belongs to N(Γ)N(\Gamma). Then L(ζ12,ζ22)J=L(ζ1,ζ2)JL(ζ1,ζ2)1Γ{\mathrm{L}}(\zeta_{1}^{2},\zeta_{2}^{2})J={\mathrm{L}}(\zeta_{1},\zeta_{2})J{\mathrm{L}}(\zeta_{1},\zeta_{2})^{-1}\in\Gamma, and hence (ζ1,ζ2)(\zeta_{1},\zeta_{2}) belongs to the subgroup (ω1,ω2),(1,1),(1,1)\langle(\sqrt{\omega_{1}},\sqrt{\omega_{2}}),\ (-1,1),\ (1,-1)\rangle.

Conversely, the image by L{\mathrm{L}} of any element in the above subgroup belongs to N(Γ)N(\Gamma). Hence

N(Γ)L(S1×S1)\displaystyle N(\Gamma)\cap{\mathrm{L}}(S^{1}\times S^{1}) =L(ω1,ω2),L(1,1),L(1,1)\displaystyle=\langle{\mathrm{L}}(\sqrt{\omega_{1}},\sqrt{\omega_{2}}),\ {\mathrm{L}}(-1,1),\ {\mathrm{L}}(1,-1)\rangle
=L(k12pd2,k22pd1),L(12,0),L(0,12).\displaystyle=\left\langle{\mathrm{L}}(\frac{k_{1}}{2pd_{2}},\frac{k_{2}}{2pd_{1}}),\ {\mathrm{L}}(\frac{1}{2},0),\ {\mathrm{L}}(0,\frac{1}{2})\right\rangle.

(Recall the abuse of notation given by (1).) This together with Lemma 12.11 implies the desired result. ∎

Proof of Proposition 12.6.

Consider the spherical dihedral orbifold 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) with (d1,d2)(1,1)(d_{1},d_{2})\neq(1,1). We first treat the generic case where 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is not the trivial θ\theta-orbifold 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2). Then, by using Lemma 12.12 and the fact that JΓJ\in\Gamma, Isom+𝒪(q/p;d1,d2)N(Γ)/Γ\operatorname{Isom}^{+}{\mathcal{O}}(q/p;d_{1},d_{2})\cong N(\Gamma)/\Gamma is isomorphic to the quotient of the group N:=L(k12pd2,k22pd1),L(12,0),L(0,12)N:=\langle{\mathrm{L}}(\frac{k_{1}}{2pd_{2}},\frac{k_{2}}{2pd_{1}}),{\mathrm{L}}(\frac{1}{2},0),{\mathrm{L}}(0,\frac{1}{2})\rangle by its subgroup G:=L(k1pd2,k2pd1)G:=\langle{\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}})\rangle. Set a=L(k12pd2,k22pd1)a={\mathrm{L}}(\frac{k_{1}}{2pd_{2}},\frac{k_{2}}{2pd_{1}}), b1=L(12,0)b_{1}={\mathrm{L}}(\frac{1}{2},0) and b2=L(0,12)b_{2}={\mathrm{L}}(0,\frac{1}{2}). It should be noted that b1,b2(2)2\langle b_{1},b_{2}\rangle\cong(\mathbb{Z}_{2})^{2} and that the subset {b1,b2,b1b2}\{b_{1},b_{2},b_{1}b_{2}\} is equal to the set of all order 22 elements of L(S1×S1){\mathrm{L}}(S^{1}\times S^{1}).

Note that the order of L(k12pd2)L(\frac{k_{1}}{2pd_{2}}) is equal to 2pd22pd_{2} or pd2pd_{2} according to whether k1k_{1} is odd or even. Similarly, the order of L(k22pd1)L(\frac{k_{2}}{2pd_{1}}) is equal to 2pd12pd_{1} or pd1pd_{1} according to whether k2k_{2} is odd or even. Thus the order of a=L(k12pd2,k22pd1)a={\mathrm{L}}(\frac{k_{1}}{2pd_{2}},\frac{k_{2}}{2pd_{1}}) is 2pd1d22pd_{1}d_{2} or pd1d2pd_{1}d_{2}, where the latter happens if and only if both k1k_{1} and k2k_{2} are even.

Case 1. o(a)=2pd1d2o(a)=2pd_{1}d_{2}. Then the element apd1d2L(S1×S1)a^{pd_{1}d_{2}}\in L(S^{1}\times S^{1}) has order 22. Hence it is equal to one of the elements of {b1,b2,b1b2}\{b_{1},b_{2},b_{1}b_{2}\}. Thus ab1,b22\langle a\rangle\cap\langle b_{1},b_{2}\rangle\cong\mathbb{Z}_{2}. This implies that Na|a2pd1d2b|b2N\cong\langle a\,|\,a^{2pd_{1}d_{2}}\rangle\oplus\langle b_{\ell}\,|\,b_{\ell}^{2}\rangle for some {1,2}{\ell}\in\{1,2\}. Since GG corresponds to the subgroup a2\langle a^{2}\rangle, we have

Isom+𝒪(q/p;d1,d2)N/a2a|a2b|b2(2)2.\operatorname{Isom}^{+}{\mathcal{O}}(q/p;d_{1},d_{2})\cong N/\langle a^{2}\rangle\cong\langle a\,|\,a^{2}\rangle\oplus\langle b_{\ell}\,|\,b_{\ell}^{2}\rangle\cong(\mathbb{Z}_{2})^{2}.

Case 2. o(a)=pd1d2o(a)=pd_{1}d_{2}. Since o(a2)=o(L(k1pd2,k2pd1))=pd1d2o(a^{2})=o({\mathrm{L}}(\frac{k_{1}}{pd_{2}},\frac{k_{2}}{pd_{1}}))=pd_{1}d_{2}, we have o(a)=o(a2)o(a)=o(a^{2}), and so o(a)=pd1d2o(a)=pd_{1}d_{2} is odd. Thus ab1,b2={1}\langle a\rangle\cap\langle b_{1},b_{2}\rangle=\{1\}, and therefore Na|apd1d2b1|b12b2|b22N\cong\langle a\,|\,a^{pd_{1}d_{2}}\rangle\oplus\langle b_{1}\,|\,b_{1}^{2}\rangle\oplus\langle b_{2}\,|\,b_{2}^{2}\rangle. Hence, we have

Isom+𝒪(q/p;d1,d2)N/a2N/ab1|b12b2|b22(2)2.\operatorname{Isom}^{+}{\mathcal{O}}(q/p;d_{1},d_{2})\cong N/\langle a^{2}\rangle\cong N/\langle a\rangle\cong\langle b_{1}\,|\,b_{1}^{2}\rangle\oplus\langle b_{2}\,|\,b_{2}^{2}\rangle\cong(\mathbb{Z}_{2})^{2}.

This completes the proof of Proposition 12.6 in the generic case.

In the exceptional case, where 𝒪(q/p;d1,d2){\mathcal{O}}(q/p;d_{1},d_{2}) is the trivial θ\theta-orbifold 𝒪(0/1;1,2){\mathcal{O}}(0/1;1,2), we may assume

Γ~=(i,i),(j,j)={±(1,1),±(i,i),±(j,j),±(k,k)}.\tilde{\Gamma}=\langle(i,i),(j,j)\rangle=\{\pm(1,1),\pm(i,i),\pm(j,j),\pm(k,k)\}.

Then, by using Lemma 12.1, we can see that N(Γ~)={(q,q)|qO}J1N(\tilde{\Gamma})=\{(q,q)\,|\,q\in O^{*}\}\rtimes\langle J_{1}\rangle. Hence we have

Isom+𝒪(0/1;1,2)(O/(2))2D3×2.\operatorname{Isom}^{+}{\mathcal{O}}(0/1;1,2)\cong\left(O^{*}/(\mathbb{Z}_{2})\right)\rtimes\mathbb{Z}_{2}\cong D_{3}\times\mathbb{Z}_{2}.

13. Appendix 2: Non-spherical geometric orbifolds with dihedral orbifold fundamental groups

In this section, we classify the non-spherical geometric orbifolds with dihedral orbifold fundamental groups (Propositions 13.1 and 13.2). These results are used in the proof of Theorem 4.1.

We first deal with the dihedral orbifolds with S2×S^{2}\times\mathbb{R} geometry.

Proposition 13.1.

Let 𝒪{\mathcal{O}} be a compact orientable S2×S^{2}\times\mathbb{R} orbifold with nonempty singular set which satisfies the following conditions.

  1. (i)

    No component of 𝒪\partial{\mathcal{O}} is spherical.

  2. (ii)

    π1(𝒪)\pi_{1}({\mathcal{O}}) is a dihedral group.

Then 𝒪{\mathcal{O}} is isomorphic to one of the following orbifolds.

  1. (1)

    𝒪(){\mathcal{O}}(\infty), the orbifold represented by the weighted graph (S3,K(),w)(S^{3},K(\infty),w), where ww takes the value 22 at each component of the 22-bridge link K()K(\infty) of slope \infty, i.e. the 22-component trivial link.

  2. (2)

    𝒪(3,O){\mathcal{O}}(\mathbb{RP}^{3},O), the orbifold with underlying space 3\mathbb{RP}^{3} whose singular set is the trivial knot (i.e., the boundary of an embedded disc in 3\mathbb{RP}^{3}) with index 22.

Proof.

By the assumption that 𝒪{\mathcal{O}} has the geometry S2×S^{2}\times\mathbb{R}, we have π1(𝒪)<Isom(S2×)Isom(S2)×Isom()\pi_{1}({\mathcal{O}})<\operatorname{Isom}(S^{2}\times\mathbb{R})\cong\operatorname{Isom}(S^{2})\times\operatorname{Isom}(\mathbb{R}) and int𝒪(S2×)/π1(𝒪)\operatorname{int}{\mathcal{O}}\cong(S^{2}\times\mathbb{R})/\pi_{1}({\mathcal{O}}). By the condition (ii), π1(𝒪)Dn\pi_{1}({\mathcal{O}})\cong D_{n} for some n{}n\in\mathbb{N}\cup\{\infty\}.

If nn\in\mathbb{N}, then the action of the finite dihedral group π1(𝒪)\pi_{1}({\mathcal{O}}) on S2×S^{2}\times\mathbb{R} extends to an action on the compact 33-manifold S2×[,]S^{2}\times[-\infty,\infty], where [,]I[-\infty,\infty]\cong I is a compactification of \mathbb{R}, and 𝒪{\mathcal{O}} is identified with S2×[,]/π1(𝒪)S^{2}\times[-\infty,\infty]/\pi_{1}({\mathcal{O}}). Thus 𝒪{\mathcal{O}} has a spherical boundary component, which contradicts the condition (i). So n=n=\infty and π1(𝒪)f,h|h2,hfh=f1\pi_{1}({\mathcal{O}})\cong\langle f,h\ |\ h^{2},\ hfh=f^{-1}\rangle. Since the action of π1(𝒪)\pi_{1}({\mathcal{O}}) on S2×S^{2}\times\mathbb{R} is properly discontinuous, fIsom(S2×)f\in\operatorname{Isom}(S^{2}\times\mathbb{R}) is the product of a (possibly trivial) rotation of S2S^{2} and a nontrivial translation of \mathbb{R}. Thus the orbifold 𝒪(f):=(S2×)/f{\mathcal{O}}(f):=(S^{2}\times\mathbb{R})/\langle f\rangle is homeomorphic to the manifold S2×S1S^{2}\times S^{1}. The isometry hh descends to a fiber-preserving involution of 𝒪(f)S2×S1{\mathcal{O}}(f)\cong S^{2}\times S^{1} which acts on the second factor as a reflection. Thus 𝒪=𝒪(f)/h{\mathcal{O}}={\mathcal{O}}(f)/h is the quotient of S2×[0,1]S^{2}\times[0,1] by an equivalence relation (x,0)(γ0(x),0)(x,0)\sim(\gamma_{0}(x),0) and (x,1)(γ1(x),1)(x,1)\sim(\gamma_{1}(x),1) where γ0\gamma_{0} and γ1\gamma_{1} are orientation-reversing involutions of S2S^{2}. Thus γi\gamma_{i} is conjugate to either the reflection in a great circle or the antipodal map. According to the combination (reflection, reflection), (reflection, antipodal map), or (antipodal map, antipodal map), 𝒪{\mathcal{O}} is isomorphic to 𝒪(){\mathcal{O}}(\infty), 𝒪(3,O){\mathcal{O}}(\mathbb{RP}^{3},O), or 3#3\mathbb{RP}^{3}\#\mathbb{RP}^{3}. The last case cannot happen because 𝒪{\mathcal{O}} has the empty singular set. ∎

The following proposition deals with the dihedral orbifolds with the remaining 66 geometries.

Proposition 13.2.

Let 𝒪{\mathcal{O}} be a compact orientable 33-orbifold with nonempty singular set which has one of the 66 geometries different from S3S^{3} and S2×S^{2}\times\mathbb{R} and satisfies the following conditions.

  1. (i)

    π1(𝒪)\pi_{1}({\mathcal{O}}) is a dihedral group.

  2. (ii)

    No component of 𝒪\partial{\mathcal{O}} is spherical.

Then 𝒪{\mathcal{O}} is isomorphic to D2(2,2)×ID^{2}(2,2)\times I.

Proof.

Let XX be the geometry which 𝒪{\mathcal{O}} possesses. Then XX is 3\mathbb{H}^{3}, 𝔼3\mathbb{E}^{3}, SL2()~\widetilde{SL_{2}(\mathbb{R})}, NilNil or SolSol, and int𝒪\operatorname{int}{\mathcal{O}} is isomorphic to X/ΓX/\Gamma for some discrete subgroup Γπ1(𝒪)\Gamma\cong\pi_{1}({\mathcal{O}}) of Isom(X)\operatorname{Isom}(X). Note that the underlying topological space of XX is homeomorphic to 3\mathbb{R}^{3}. The proof is divided into two cases according to whether π1(𝒪)\pi_{1}({\mathcal{O}}) is finite or infinite.

Case 1. Suppose that π1(𝒪)\pi_{1}({\mathcal{O}}) is a finite dihedral group DnD_{n}. Then, as will be shown below, the action of DnD_{n} on XX has a global fixed point xx. Then the exponential map from TxXT_{x}X, the tangent space to XX at xx, to XX is a DnD_{n}-equivariant homeomorphism. This implies that 𝒪S2(2,2,n)\partial{\mathcal{O}}\cong S^{2}(2,2,n), contradicting the condition (ii).

The existence of a global fixed point can be proved as follows. For the constant curvature case X=3X=\mathbb{H}^{3} or 𝔼3\mathbb{E}^{3}, this is well-known. We shall first deal with the case where XX is NilNil, 2×\mathbb{H}^{2}\times\mathbb{R}, or SL2~\widetilde{\mbox{$\mathrm{SL}$}_{2}\mathbb{R}}. Recall that there is an exact sequence

1Isom()Isom(X)Isom(E)1,1\to\operatorname{Isom}(\mathbb{R})\to\operatorname{Isom}(X)\to\operatorname{Isom}(E)\to 1,

where EE is the Euclidean plane 𝔼2\mathbb{E}^{2} when XX is NilNil and the hyperbolic plane 2\mathbb{H}^{2} when XX is 2×\mathbb{H}^{2}\times\mathbb{R} or SL2~\widetilde{\mbox{$\mathrm{SL}$}_{2}\mathbb{R}}. We also note that the projection Isom(X)Isom(E)\operatorname{Isom}(X)\to\operatorname{Isom}(E) above is induced by a fibration p:XEp:X\to E. Let D¯n\bar{D}_{n} be the image of DnD_{n} in Isom(E)\operatorname{Isom}(E) and KK the kernel in DD_{\infty} of the projection to D¯n\bar{D}_{n}. Then the action of D¯n\bar{D}_{n} on EE has a global fixed point yy, and the action of KK on the fibre p1(y)p^{-1}(y) has a global fixed point since both of them are finite. Thus DnD_{n} has a global fixed point on XX when XX is NilNil, 2×\mathbb{H}^{2}\times\mathbb{R}, or SL2~\widetilde{\mbox{$\mathrm{SL}$}_{2}\mathbb{R}}.

We shall now show the same property when X=SolX=Sol. In this case, there is an exact sequence

1Isom(𝔼2)Isom(Sol)Isom()1,1\to\operatorname{Isom}(\mathbb{E}^{2})\to\operatorname{Isom}(Sol)\to\operatorname{Isom}(\mathbb{R})\to 1,

and the projection Isom(Sol)Isom()\operatorname{Isom}(Sol)\to\operatorname{Isom}(\mathbb{R}) is induced by a fibration q:Solq:Sol\to\mathbb{R}. Let D¯n\bar{D}_{n} be the projection of DnD_{n} in Isom()\operatorname{Isom}(\mathbb{R}). Then D¯n\bar{D}_{n} is either trivial or 2\mathbb{Z}_{2} generated by a reflection on \mathbb{R}. In either case, it fixes a point yy on \mathbb{R}. In the former case, Dng,h|g2,h2,(gh)nD_{n}\cong\langle g,h\ |\ g^{2},h^{2},\ (gh)^{n}\rangle acts on the fibre q1(y)q^{-1}(y) by Euclidean isometries in such a way that gg and hh correspond to reflections, and hence DnD_{n} fixes a point on the fibre. In the latter case, the kernel KK of the projection DnD¯nD_{n}\to\bar{D}_{n} is isomorphic to n\mathbb{Z}_{n}, and fixes a point on the fibre in the same way. Thus we have shown that DnD_{n} has a fixed point also in the case when X=SolX=Sol.

Case 2. Suppose π1(𝒪)\pi_{1}({\mathcal{O}}) is the infinite dihedral group Dg,h|g2,h2D_{\infty}\cong\langle g,h\ |\ g^{2},h^{2}\rangle. First we shall consider the case when XX has constant curvature. Then gg and hh are order 22 elliptic transformations, and hence fix pointwise axes aga_{g} and aha_{h} respectively. They do not meet each other since otherwise the action fixes their intersection and cannot be faithful and discrete. Let \ell be the common perpendicular to aga_{g} and aha_{h} if it exists. (This does not exist when X=3X=\mathbb{H}^{3} and aga_{g} touches aha_{h} at infinity. This exceptional case will be considered later.) Let Πg\Pi_{g} be the totally geodesic plane containing aha_{h} and perpendicular to \ell. We define Πh\Pi_{h} in the same way. Then the region cobounded by Πg\Pi_{g} and Πh\Pi_{h} constitutes a fundamental domain of the action of DD_{\infty}. Suppose now that X=3X=\mathbb{H}^{3} and aga_{g} touches aha_{h} at infinity. Then there is a totally geodesic plane HH containing both aga_{g} and aha_{h} and it is preserved by DD_{\infty}. We then let Πg\Pi_{g} and Πh\Pi_{h} be totally geodesic planes containing aga_{g} and aha_{h} respectively, which are perpendicular to HH. Then a fundamental domain is cobounded by Πg\Pi_{g} and Πh\Pi_{h} again. Therefore, in either case, we can see int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R} and so 𝒪D2(2,2)×I{\mathcal{O}}\cong D^{2}(2,2)\times I.

Next, we shall consider the case when XX is NilNil or 2×\mathbb{H}^{2}\times\mathbb{R} or SL2~\widetilde{\mbox{$\mathrm{SL}$}_{2}\mathbb{R}}. As before, let D¯\bar{D}_{\infty} be the projection of DD_{\infty} to Isom(E)\operatorname{Isom}(E), and KK the kernel of the projection. We first observe that the images g¯\bar{g} and h¯\bar{h} of gg and hh in D¯\bar{D}_{\infty} are nontrivial. In fact, if say g¯\bar{g} is trivial, then gg acts on \mathbb{R} as a nontrivial order 22 isometry. Thus gg acts on \mathbb{R} by a reflection, and so the image g¯\bar{g} must be an orientation-reversing isometry on EE, which contradicts our assumption that g¯\bar{g} is trivial.

Since gg and hh have order 22, their images g¯\bar{g} and h¯\bar{h} in D¯\bar{D}_{\infty} also have order 22. We first deal with the case where both of them are orientation-preserving, i.e. π\pi-rotations. Let ygy_{g} and yhy_{h} be the centres of the π\pi-rotations g¯\bar{g} and h¯\bar{h}, respectively. Then gg and hh are π\pi-rotations about the geodesics p1(yg)p^{-1}(y_{g}) and p1(yh)p^{-1}(y_{h}), respectively. Since the action of DD_{\infty} is faithful, we have ygyhy_{g}\neq y_{h}. Now consider the geodesic line \ell in EE containing ygy_{g} and yhy_{h}, and let g\ell_{g} and h\ell_{h} be the lines which intersects \ell perpendicularly at ygy_{g} and yhy_{h}, respectively. Then g\ell_{g} and h\ell_{h} are disjoint, and they cobound a region RR in EE. We see that p1(R)p^{-1}(R) is a fundamental region of the action of DD_{\infty}, and we have int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R}.

We next treat the case where both of g¯\bar{g} and h¯\bar{h} are orientation-reversing, i.e. reflections. Let aga_{g} and aha_{h} be the axes of the reflections g¯\bar{g} and h¯\bar{h}, respectively. Then gg and hh are the ‘symmetries’ with respect to the geodesics a~g\tilde{a}_{g} and a~h\tilde{a}_{h}, respectively, where a~g\tilde{a}_{g} and a~h\tilde{a}_{h} are lifts of aga_{g} and aha_{h}, respectively. If aga_{g} and aha_{h} are disjoint, they cobound a region RR in EE, and p1(R)p^{-1}(R) is a fundamental region of the action of DD_{\infty}, and we have int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R}. If aga_{g} and aha_{h} meet each other at a point yEy\in E. Then DD_{\infty} acts effectively and discretely on the fiber p1(y)p^{-1}(y), and so the axes a~g\tilde{a}_{g} and a~h\tilde{a}_{h} intersect p1(y)p^{-1}(y) perpendicularly at distinct points, zgz_{g} and zhz_{h}, respectively. Let PgP_{g} and PhP_{h} be the ruled surfaces in XX obtained as the unions of the geodesics which intersect p1(y)p^{-1}(y) perpendicularly at zgz_{g} and zhz_{h}, respectively. Then PgP_{g} and PhP_{h} are disjoint planes in XX, and the domain they cobound is a fundamental domain of DD_{\infty}, and we can see int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R}.

We now treat the case where one of g¯\bar{g} and h¯\bar{h} is orientation-preserving and the other is orientation-reversing. We may assume g¯\bar{g} is orientation-preserving and h¯\bar{h} is orientation-reversing. Let ygy_{g} be the center of the π\pi-rotation g¯\bar{g}, and let aha_{h} be the axis of the reflection h¯\bar{h}. If ygy_{g} belongs to aha_{h}, then the axes of the π\pi-rotations of gg and hh intersect, and the action of DD_{\infty} cannot be discrete and faithful. So ygy_{g} is not contained in aga_{g}. Let \ell be a geodesic line in EE which passes through yy and is disjoint from aha_{h}. Let RR be the region in EE bounded by aha_{h} and \ell. Then p1(R)p^{-1}(R) is a fundamental region of the action of DD_{\infty}, and we have int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R}.

Finally, suppose that X=SolX=Sol. Then the projection D¯\bar{D}_{\infty} of DD_{\infty} to Isom()\operatorname{Isom}(\mathbb{R}) is either trivial or 2\mathbb{Z}_{2} or DD_{\infty} itself. In the case when D¯\bar{D}_{\infty} is trivial, the generators gg and hh act on each fibre by π\pi-rotations, and their fixed points must differ. Thus int𝒪X/D\operatorname{int}{\mathcal{O}}\cong X/D_{\infty} is a bundle over \mathbb{R} with fiber 𝔼2/DintD2(2,2)\mathbb{E}^{2}/D_{\infty}\cong\operatorname{int}D^{2}(2,2). So we have int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R}. In the case when D¯\bar{D}_{\infty} is 2\mathbb{Z}_{2}, the action of D¯\bar{D}_{\infty} is a reflection with respect to a point xx. We set P=q1(x)P=q^{-1}(x). Then the gg and hh act on PP by reflections, and by the same argument as in the previous paragraph, we have a homeomorphism int𝒪D2(2,2)×\operatorname{int}{\mathcal{O}}\cong D^{2}(2,2)\times\mathbb{R}. Finally, suppose that D¯=D\bar{D}_{\infty}=D_{\infty}. Then gg and hh fix points xgx_{g} and xhx_{h} on \mathbb{R} respectively, and they differ. We consider fibres Πg=q1(xg)\Pi_{g}=q^{-1}(x_{g}) and Πh=q1(xh)\Pi_{h}=q^{-1}(x_{h}). The elements act on Πg\Pi_{g} and Πh\Pi_{h} as reflections with axes agΠga_{g}\subset\Pi_{g} and ahΠha_{h}\subset\Pi_{h}. Then the region cobounded by Πg\Pi_{g} and Πh\Pi_{h} constitutes a fundamental region for the action of DD_{\infty}, and we see that int𝒪intD2(2,2)×\operatorname{int}{\mathcal{O}}\cong\operatorname{int}D^{2}(2,2)\times\mathbb{R}. ∎

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