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Equivariant unknotting numbers of strongly invertible knots

Keegan Boyle Department of Mathematical Sciences, New Mexico State University, USA kboyle@nmsu.edu  and  Wenzhao Chen Institute of Mathematical Sciences, ShanghaiTech University, China chenwzh@shanghaitech.edu.cn
Abstract.

We study symmetric crossing change operations for strongly invertible knots. Our main theorem is that the most natural notion of equivariant unknotting number is not additive under connected sum, in contrast with the longstanding conjecture that unknotting number is additive.

1. Introduction

The unknotting number u(K)u(K) of a knot KK is the minimum number of transverse self-intersections in a regular homotopy to the unknot. First defined in [Wen37], the unknotting number has a long history but remains mysterious. For example, according to KnotInfo [LM24], the knots with unknown unknotting number and 10 or fewer crossings are

1011,1047,1051,1054,1061,1076,1077,1079,and 10100.10_{11},10_{47},10_{51},10_{54},10_{61},10_{76},10_{77},10_{79},\mbox{and }10_{100}.

Another important open question about the unknotting number concerns its additivity under connected sum of knots.

Conjecture 1.1 (Additivity of unknotting number [Wen37]).

Let KK and KK^{\prime} be knots in S3S^{3}. Then u(K#K)=u(K)+u(K)u(K\#K^{\prime})=u(K)+u(K^{\prime}).

In light of the evident difficulty of these questions, a natural idea is to consider the unknotting number in the presence of additional structure. To this end, we study equivariant unknotting numbers for strongly invertible knots.

A strongly invertible knot is a knot KS3K\subset S^{3} along with a smooth symmetry which preserves the orientation on S3S^{3} but reverses the orientation on KK. As a consequence of geometrization, any such symmetry is conjugate in the diffeomorphism group of pairs (S3,K)(S^{3},K) to a 180180^{\circ}-rotation around an unknot which intersects KK in two points (see for example [BRW23]). For an example, see any of the diagrams appearing in the first or third row of Figure 1.

Naturally, we would like to consider an equivariant version of Conjecture 1.1. To make this precise, we define the total equivariant unknotting number (denoted by u~(K)\widetilde{u}(K); see Definition 2.2) which is the minimum number of transverse self-intersections in a regular and equivariant homotopy to the unknot. In this setting, we can resolve the equivariant version of Conjecture 1.1.

Theorem 1.2.

There are strongly invertible knots K1K_{1} and K2K_{2} and an equivariant connected sum K1#K2K_{1}\#K_{2} such that u~(K1#K2)>u~(K1)+u~(K2)\widetilde{u}(K_{1}\#K_{2})>\widetilde{u}(K_{1})+\widetilde{u}(K_{2}). In particular, the total equivariant unknotting number is not additive or even sub-additive.

Our approach to Theorem 1.2 is to consider the natural classification of equivariant transverse self-intersections into three types, which we call type A, type B, and type C. These self-intersections correspond to three types of equivariant crossing change to which we apply the same labels; see Figure 1. As a stepping stone to Theorem 1.2, we define, for X{A,B,C}X\in\{A,B,C\}, the type XX unknotting number u~X(K)\widetilde{u}_{X}(K) of a strongly invertible knot KK as the minimum number of type XX self-intersections in a regular and equivariant homotopy to the unknot, where all self-intersections are required to be type XX. For example in Figure 1, the second column demonstrates that u~B(41)=1\widetilde{u}_{B}(4_{1})=1, the third column demonstrates that u~C(41)=1\widetilde{u}_{C}(4_{1})=1, and the first column demonstrates that |u~A(41)u~A(31)|1.|\widetilde{u}_{A}(4_{1})-\widetilde{u}_{A}(3_{1})|\leq 1. In contrast with the total equivariant unknotting number, it may a priori be the case that a knot cannot be unknotted with type XX moves, in which case we say that u~X(K)=\widetilde{u}_{X}(K)=\infty.

\begin{overpic}[width=300.0pt,grid=false]{selfintersections.pdf} \put(7.5,3.0){Type A} \put(40.0,3.0){Type B} \put(74.0,3.0){Type C} \end{overpic}
Figure 1. Examples of the three types of equivariant transverse self-intersections, realized as a movie starting on the figure-eight knot. The first column is Type A (‘off the axis’), the middle column is Type B (‘through the axis’), and the right column is Type C (‘along the axis’).

The majority of this paper is concerned with studying these restricted notions of equivariant unknotting number, which will culminate in Theorem 1.2. In fact, we will see that Theorem 1.2 relies on the non-additivity of the type C unknotting number.

Theorem 1.3.

Let KK by a strongly invertible knot with three non-trivial summands. Then u~C(K)=\widetilde{u}_{C}(K)=\infty. In particular, the type C unknotting number is not additive under connected sum.

For type A and type B crossing changes, we do not know whether the corresponding equivariant unknotting numbers are additive.

Conjecture 1.4.

Let K#KK\#K^{\prime} be an equivariant connected sum of two strongly invertible knots KK and KK^{\prime}. Then u~A(K#K)=u~A(K)+u~A(K)\widetilde{u}_{A}(K\#K^{\prime})=\widetilde{u}_{A}(K)+\widetilde{u}_{A}(K^{\prime}) and u~B(K#K)=u~B(K)+u~B(K)\widetilde{u}_{B}(K\#K^{\prime})=\widetilde{u}_{B}(K)+\widetilde{u}_{B}(K^{\prime}).

In building towards Theorem 1.2, we also provide some answers to elementary questions about u~A,u~B,\widetilde{u}_{A},\widetilde{u}_{B}, and u~C\widetilde{u}_{C}, which we state in Sections 1.1 and 1.2.

1.1. Unknotting operations

Which types of equivariant crossing changes are unknotting operations? In other words, is u~X(K)<\widetilde{u}_{X}(K)<\infty? For the type A unknotting number, we have the following.

Theorem 1.5.

For any strongly invertible knot KK, we have u~A(K)<\widetilde{u}_{A}(K)<\infty.

On the other hand, we do not know if every strongly invertible knot can be unknotted with type B moves.

Question 1.6.

For any strongly invertible knot KK, is it true that u~B(K)<\widetilde{u}_{B}(K)<\infty?

Remark 1.7.

Consider the connected sum of a trefoil with its reverse K=31#r31K=3_{1}\#r3_{1} with the symmetry that exchanges the two summands. Any minimal crossing number diagram for KK does not have any on-axis crossings. Thus we find it surprising that u~B(K)\widetilde{u}_{B}(K)\neq\infty. Indeed, we can see in Figure 2 that u~B(K)4\widetilde{u}_{B}(K)\leq 4.

\begin{overpic}[width=400.0pt,grid=false]{trefoilsumtypeBunknotting.pdf} \put(5.0,27.0){\large$i$} \put(27.0,27.0){\large$i$} \put(48.0,27.0){\large$i$} \put(70.0,26.0){\large$i$} \put(90.0,26.0){\large$i$} \par\put(14.0,27.0){\large$B_{1}$} \put(36.0,27.5){\large$B_{2}$} \put(60.0,27.0){\large$i$} \put(78.0,26.5){\large$B_{1}$} \end{overpic}
Figure 2. An unknotting sequence of 31#r313_{1}\#r3_{1} consisting of equivariant isotopies indicated by arrows labelled with an ii, and type B moves indicated by arrows labelled with a Bx, where xx is the number of type B moves applied. For compactness, the axis of symmetry is horizontal in each diagram. A total of 4 type B moves are used so that u~B(31#r31)4\widetilde{u}_{B}(3_{1}\#r3_{1})\leq 4.

Another interesting observation about Question 1.6 is that a positive answer would imply a positive answer to Nakanishi’s 4-move conjecture [NS87, Conjecture B] (this problem also appears on the Kirby problem list [Kir97, 1.59(3)(a)]); see Corollary 5.3.

Finally, we give a complete classification of strongly invertible knots which can be unknotted with type C moves. In the following theorem, a (1,2)(1,2)-knot refers to a genus one 2-bridge knot. That is a knot which can be decomposed into a union of 4 arcs by the standard genus 1 Heegaard splitting of S3S^{3}, where each handlebody contains a pair of boundary-parallel arcs.

Theorem 1.8.

A strongly invertible knot KK has u~C(K)<\widetilde{u}_{C}(K)<\infty if and only if KK is a (1,2)(1,2)-knot such that the axis of symmetry is the core of one of the handlebodies in the (1,2)(1,2) decomposition.

The proof of Theorem 1.8 involves studying the symmetric mapping class group of a solid torus with 4 marked points on the boundary; we give a list of generators for this mapping class group in Proposition 6.10.

1.2. Lower bounds

We now state some lower bounds for u~A(K),u~B(K),\widetilde{u}_{A}(K),\widetilde{u}_{B}(K), and u~C(K)\widetilde{u}_{C}(K) which are useful in proving Theorem 1.2, but may be of independent interest. Our theorems are in terms of the quotient knots 𝔮1(K)\mathfrak{q}_{1}(K) and 𝔮2(K)\mathfrak{q}_{2}(K) of a strongly invertible knot KK; see Definition 2.7.

Theorem 1.9.

Let KK be a strongly invertible knot. Then u~A(K)max(u(𝔮1(K)),u(𝔮2(K))).\widetilde{u}_{A}(K)\geq\max(u(\mathfrak{q}_{1}(K)),u(\mathfrak{q}_{2}(K))).

To state our lower bound for u~B(K)\widetilde{u}_{B}(K), let u4(K)u_{4}(K) be the minimum number of 4-moves needed to unknot KK; see Section 5.

Theorem 1.10.

Let KK be a strongly invertible knot. Then u~B(K)u4(𝔮1(K))+u4(𝔮2(K))\widetilde{u}_{B}(K)\geq u_{4}(\mathfrak{q}_{1}(K))+u_{4}(\mathfrak{q}_{2}(K)).

To state our lower bound for u~C(K)\widetilde{u}_{C}(K), let unb(K)u_{nb}(K) be the minimum number of non-orientable band moves needed to unknot KK; see Section 6.

Theorem 1.11.

Let KK be a strongly invertible knot. Then u~C(K)unb(𝔮1(K))+unb(𝔮2(K))\widetilde{u}_{C}(K)\geq u_{nb}(\mathfrak{q}_{1}(K))+u_{nb}(\mathfrak{q}_{2}(K)).

As a consequence of these theorems, we are able to show that there are knots for which u~A(K)u(K)\widetilde{u}_{A}(K)-u(K) is arbitrarily large (see Corollary 4.1), and that there is a knot for which u~B(K)u(K)2\widetilde{u}_{B}(K)-u(K)\geq 2 (see Example 5.6). On the other hand for type C moves, Theorem 1.3 shows that u~C(K)u(K)\widetilde{u}_{C}(K)-u(K) can be infinite. We make the following conjecture about type B moves.

Conjecture 1.12.

There is a sequence KnK_{n} of strongly invertible knots such that u~B(Kn)u(Kn)\widetilde{u}_{B}(K_{n})-u(K_{n}) is unbounded.

1.3. Torus knots

Along with the elementary lower bounds in the previous section, we compute an upper bound on the total equivariant unknotting numbers for torus knots. This upper bound turns out to be sharp, as is recorded in the following theorem.

Theorem 1.13.

Let KK be the (p,q)(p,q)-torus knot with its unique strong inversion. Then

u~(K)=u(K)=(p1)(q1)2.\widetilde{u}(K)=u(K)=\dfrac{(p-1)(q-1)}{2}.

Furthermore, there exists a minimal length equivariant unknotting sequence consisting of only type A and type B moves.

The theorem that u(K)=(p1)(q1)2u(K)=\dfrac{(p-1)(q-1)}{2}, known as the Milnor conjecture and proved in [KM93], is closely related to ideas in algebraic geometry about links of plane curve singularities. Milnor’s conjecture originated from observations in algebraic geometry, namely that a particular resolution of a plane curve singularity produces an algebraic surface in B4B^{4} with boundary T(p,q)T(p,q). Kronheimer and Mrowka then proved that this surface has the minimum genus possible with boundary T(p,q)T(p,q), which along with the fact that the 4-genus is a lower bound on u(K)u(K) proved that u(K)(p1)(q1)2u(K)\geq\dfrac{(p-1)(q-1)}{2}. On the other hand, the upper bound on u(K)u(K), has been known for longer; see [Rud83].

For the equivariant unknotting number u~(K)\widetilde{u}(K), we also have a lower bound coming from the equivariant 4-genus; see Proposition 2.5. Furthermore, the equivariant 4-genus is equal to the 4-genus, since the resolved algebraic surfaces can be seen to be invariant under complex conjugation, so we can readily check that u~(K)(p1)(q1)2\widetilde{u}(K)\geq\dfrac{(p-1)(q-1)}{2}. Hence the content of Theorem 1.13 is the upper bound on u~(K)\widetilde{u}(K).

For this upper bound, one may be tempted to emulate [A’C98, Theorem 4], which proves that u(K)(p1)(q1)2u(K)\geq\dfrac{(p-1)(q-1)}{2}. However, we were unable to prove a symmetric version of the lemma used in this proof. Instead, we emulate Rudolph’s original diagrammatic proof [Rud83] using the braid group, which is somewhat less concise than A’Campo’s proof, and only becomes more complicated in the equivariant setting. We use a particular type of symmetric braid which we call an intravergent braid (see Definition 3.1). Our main contribution here is the following proposition, which may be of independent interest.

Proposition 1.14.

Let BB be a positive intravergent braid with s=2n+1s=2n+1 strands and length =len(B)\ell=\operatorname{len}(B) such that the closure of BB is a knot B^\widehat{B}. Then u~(B^)s+12\widetilde{u}(\widehat{B})\leq\dfrac{\ell-s+1}{2}.

1.4. Questions

Finally, we record some basic unanswered questions here.

Question 1.15.

In Figure 1, we see that for the unique (up to symmetry) strong inversion on the figure-eight knot we have u~B(41)=u~C(41)=1\widetilde{u}_{B}(4_{1})=\widetilde{u}_{C}(4_{1})=1, and that u~A(41)2\widetilde{u}_{A}(4_{1})\leq 2, since u~A(31)=1\widetilde{u}_{A}(3_{1})=1 (by inspection). Is u~A(41)=1\widetilde{u}_{A}(4_{1})=1 or is u~A(41)=2\widetilde{u}_{A}(4_{1})=2? More generally, what are the type A unknotting numbers of the strongly invertible twist knots KnK_{n} as shown in Figure 6?

Remark 1.16.

For these twist knots KnK_{n}, Theorem 1.9 gives the lower bound u~A(Kn)n\widetilde{u}_{A}(K_{n})\geq n, since the quotient (as shown in Figure 6) is T(2,2n+1)T(2,2n+1) which has unknotting number nn, and the other quotient is the unknot. However, the best upper bound we found was u~A(Kn)2n\widetilde{u}_{A}(K_{n})\leq 2n coming from the apparent sequence of type A moves.

Question 1.17.

In Remark 1.7 we saw that u~B(31#r31)4\widetilde{u}_{B}(3_{1}\#r3_{1})\leq 4, but our best lower bound comes from Theorem 1.10 which gives that u~B(31#31)2\widetilde{u}_{B}(3_{1}\#3_{1})\geq 2. What is the exact value of u~B(31#r31)\widetilde{u}_{B}(3_{1}\#r3_{1})?

1.5. Acknowledgements

We would like to thank Kenneth L. Baker and Maggie Miller for directing us to some relevant literature, and Ben Williams and Liam Watson for helpful conversations and advice. This project started while both authors were postdocs at UBC, and the second author was partially supported by the Pacific Institute for the Mathematical Sciences (PIMS).

2. Equivariant crossing changes and unknotting numbers

Fix an order 2 symmetry ρ:S1S1\rho\colon S^{1}\to S^{1} with two fixed points, and an order 2 symmetry ρ:S3S3\rho\colon S^{3}\to S^{3} with a fixed circle. Consider an equivariant homotopy h:(S1×I,ρ)(S3×I,ρ)h\colon(S^{1}\times I,\rho)\to(S^{3}\times I,\rho) between two strongly invertible knots K=h(S1,0)K=h(S^{1},0) and K=h(S1,1)K^{\prime}=h(S^{1},1), such that h(S1,t)=(S3,t)h(S^{1},t)=(S^{3},t) for all tIt\in I, and hh has only transverse self-intersections in the interior. We would like to define the equivariant unknotting number as the minimum number of self-intersection points in such a homotopy between a given strongly invertible knot and the unknot. The presence of a symmetry, however, means that these self-intersections are naturally classified into the following three types.

  1. (1)

    Self-intersections which do not lie on the axis of symmetry come in symmetric pairs. We refer to such self-intersections as type A.

  2. (2)

    Self-intersections which do lie on the axis of symmetry come in two types.

    1. (a)

      If the self-intersection point is the image of a pair of points exchanged by the symmetry on S1S^{1}, then we call the self-intersection type B.

    2. (b)

      If the self-intersection point is the image of the two fixed points on S1S^{1}, then we call the self-intersection point type C.

These three types of self-intersections can be seen diagrammatically in Figure 1, along with the corresponding crossing-change moves. Note that a type B or type C move consists of a single crossing change, but a type A move consists of a pair of crossing changes.

Definition 2.1.

For X {A,B,C}\in\{A,B,C\}, the type X unknotting number u~X(K)\widetilde{u}_{X}(K) of a strongly invertible knot KK is the minimum number of type X moves necessary to reduce KK to the unknot. If KK cannot be reduced to the unknot in a finite number of type X moves, then we say that u~X(K)=\widetilde{u}_{X}(K)=\infty.

Definition 2.2.

The total equivariant unknotting number u~(K)\widetilde{u}(K) is the minimum number of equivariant crossing changes of all types necessary to unknot KK.

Remark 2.3.

Noting that a type A move consists of two crossing changes, we have the immediate inequalities

  • u~(K)2u~A(K)\widetilde{u}(K)\leq 2\widetilde{u}_{A}(K),

  • u~(K)u~B(K)\widetilde{u}(K)\leq\widetilde{u}_{B}(K), and

  • u~(K)u~C(K)\widetilde{u}(K)\leq\widetilde{u}_{C}(K).

We could also have chosen the total equivariant unknotting number to only increment by one for each type A move. We made the choice to increment by two for each type A move so that we have a stronger lower bound on the equivariant 4-genus.

Definition 2.4.

The equivariant 4-genus g~4(K)\widetilde{g}_{4}(K) of a strongly invertible knot KK is the minimum genus of a surface Σ\Sigma smoothly properly embedded in B4B^{4} such that there is a smooth extension ρ\rho of the symmetry on S3S^{3} to B4B^{4} with ρ(Σ)=Σ\rho(\Sigma)=\Sigma.

Proposition 2.5.

Let KK be a strongly invertible knot. Then g~4(K)u~(K)\widetilde{g}_{4}(K)\leq\widetilde{u}(K).

Proof.

As in the non-equivariant setting, we can construct a cobordism between two knots related by a sequence of equivariant crossing changes, where the genus of the cobordism is equal to the number of crossing changes. Indeed, it is easy to see that the standard cobordism can be made equivariant at a type A, B, or C move. (Note that this matches the definition of u~(K)\widetilde{u}(K) since a type A move contributes two crossing changes, while a type B or C move contributes one.) ∎

Remark 2.6.

Note that for any two strongly invertible knots K1K_{1} and K2K_{2}, we have that g~4(K1#K2)g~4(K1)+g~4(K2)\widetilde{g}_{4}(K_{1}\#K_{2})\leq\widetilde{g}_{4}(K_{1})+\widetilde{g}_{4}(K_{2}), since the two minimal genus surfaces can be glued equivariantly.

Definition 2.7.

Let KK be a strongly invertible knot with axis of symmetry AA. Then in the quotient of S3S^{3} by the strong inversion, there is a quotient theta graph consisting of the image of KK and the image of AA. The three arcs of this theta graph are the image K¯\overline{K} of KK and two arcs which make up the image of AA which we refer to arbitrarily as h1h_{1} and h2h_{2}. The two quotient knots of KK are 𝔮1(K)=K¯h1\mathfrak{q}_{1}(K)=\overline{K}\cup h_{1} and 𝔮2(K)=K¯h2\mathfrak{q}_{2}(K)=\overline{K}\cup h_{2}.

3. Torus knots

In this section we will prove Theorem 1.13, which we restate here for convenience.

See 1.13

In order to prove Theorem 1.13 we will work with symmetric braids. Although symmetric braids whose closures are strongly invertible knots have been studied in [Mer24], they study braids which are symmetric under rotation around a line in the plane of the diagram, while for our application it is more convenient to use braids which are symmetric under rotation around a line orthogonal to the plane of the diagram.

Definition 3.1.

Let σi\sigma_{i} refer to the positive half-twist between the iith and i+1i+1th strands of a braid. An intravergent braid is a braid on 2n+12n+1 strands given by a word of length 2m2m such that if σi±1\sigma_{i}^{\pm 1} appears at index jj, then σ2n+1i±1\sigma_{2n+1-i}^{\pm 1} appears at index mjm-j. (See for example Figure 3.)

Refer to caption
Figure 3. An intravergent braid on 3 strands given by the word σ1σ2\sigma_{1}\sigma_{2} when read left to right. The symmetry is given by π\pi rotation around the central marked point.

Observe that the closure of an intravergent braid, if it is a knot, is a strongly invertible knot. Additionally, we will say that an intravergent braid is positive if every generator σi\sigma_{i} appears with only positive powers.

Definition 3.2.

The length of an intravergent braid BB, written len(B)\operatorname{len}(B), is the length of the underlying braid word for BB.

The following proposition is an equivariant analog of [Rud83, Proposition on page 34]. This is our contribution needed to prove Theorem 1.13.

See 1.14

To prove this proposition we will need the following lemma.

Lemma 3.3.

Let ww be a word in the (positive) generators {σi:1i2n}\{\sigma_{i}:1\leq i\leq 2n\} of the braid group B2n+1B_{2n+1} which begins with σ1\sigma_{1} and contains no other σ1\sigma_{1}s. Then ww is equivalent (as an element of B2n+1B_{2n+1}) to a word ww^{\prime} with len(w)=len(w)\operatorname{len}(w^{\prime})=\operatorname{len}(w) such that at least one of the following is true:

  1. (1)

    ww^{\prime} is the word σ1σ2σi\sigma_{1}\sigma_{2}\dots\sigma_{i} for some i2ni\leq 2n, or

  2. (2)

    ww^{\prime} is a word containing σi2\sigma_{i}^{2} for some 1<i2n1<i\leq 2n, or

  3. (3)

    ww^{\prime} is a word containing exactly one σ1\sigma_{1}, but not beginning with σ1\sigma_{1}.

Similarly, if ww ends with σ1\sigma_{1} and contains no other σ1\sigma_{1}s, then ww is equivalent to a word ww^{\prime} as above, but with the order of the letters in ww^{\prime} reversed.

Proof.

We proceed by induction on the length of ww. For the base case, we have w=σ1w=\sigma_{1}, which satisfies (1).

Now suppose that the statement is true for all words with length <m<m, and let ww be a word of length mm which starts with σ1\sigma_{1} and contains no other σ1\sigma_{1}s. If ww is the word w¯=σ1σ2σm\overline{w}=\sigma_{1}\sigma_{2}\dots\sigma_{m}, then ww satisfies (1). If not, then there is a first letter in ww which differs from w¯\overline{w}; call it σi\sigma_{i} at index jj with jij\neq i and i>1i>1 so that ww begins with σ1σ2σj2σj1σi\sigma_{1}\sigma_{2}\dots\sigma_{j-2}\sigma_{j-1}\sigma_{i}. There are then three cases.

  1. (a)

    If i=j1i=j-1, then ww satisfies (2).

  2. (b)

    If i>ji>j, then we can commute σi\sigma_{i} past all of the previous letters in ww, so that ww^{\prime} begins with σiσ1σ2\sigma_{i}\sigma_{1}\sigma_{2}\dots and hence ww satisfies (3).

  3. (c)

    If i<j1i<j-1, then we can commute σi\sigma_{i} to the left until we run into σi+1\sigma_{i+1}, so that ww is equivalent to a word beginning with σ1σ2σiσi+1σi\sigma_{1}\sigma_{2}\dots\sigma_{i}\sigma_{i+1}\sigma_{i}. We can then apply the braid relation to get an equivalent word beginning with σ1σ2σi1σi+1σiσi+1\sigma_{1}\sigma_{2}\dots\sigma_{i-1}\sigma_{i+1}\sigma_{i}\sigma_{i+1}. Now since i>1i>1, we can commute the first σi+1\sigma_{i+1} to the beginning of the word so that we have a word ww^{\prime} which begins σi+1σ1σ2σi1σiσi+1\sigma_{i+1}\sigma_{1}\sigma_{2}\dots\sigma_{i-1}\sigma_{i}\sigma_{i+1}. Hence ww satisfies (3).

Proof of Proposition 1.14.

We will induct on the pair (s,)(s,\ell) with respect to the lexicographical order. Clearly when s=1s=1 we have =0\ell=0 and hence B^\widehat{B} is the unknot. Thus the statement is true for (s,)=(1,0)(s,\ell)=(1,0).

We now suppose that the statement is true for all parameters less than (s,)(s,\ell), and consider an arbitrary braid BB with s=2n+1s=2n+1 strands and length =2m\ell=2m whose closure is a knot. We have four cases:

  1. (1)

    σ1\sigma_{1} does not appear as a letter in BB,

  2. (2)

    σ1\sigma_{1} appears exactly once as a letter in BB,

  3. (3)

    σ1\sigma_{1} appears exactly twice as a letter in BB, or

  4. (4)

    σ1\sigma_{1} appears more than twice as a letter in BB.

In case (1), either B^\widehat{B} is a link, or s=1s=1 which was already covered as the base case.

In case (2), we can apply a pair of symmetric Reidemeister 1 moves, realized on the braid as a symmetric pair of Markov moves, which reduces the number of strands to s2s-2 and the length of the word to 2\ell-2. Thus by our inductive assumption we have that

u~(B^)(2)(s2)+12=s+12.\widetilde{u}(\widehat{B})\leq\dfrac{(\ell-2)-(s-2)+1}{2}=\dfrac{\ell-s+1}{2}.

In case (3) we have two sub-cases.

  1. (3.1)

    The first case is when both appearances of σ1\sigma_{1} occur with index m\leq m or >m>m. In this case we consider the word ww which begins with the first occurrence of σ1\sigma_{1} in BB and ends with the letter preceding the second occurrence of σ1\sigma_{1}. Let x=len(w)x=\operatorname{len}(w). By Lemma 3.3 there are three possibilities.

    1. (3.1.1)

      If ww is equivalent to the word w=σ1σ2σxw^{\prime}=\sigma_{1}\sigma_{2}\dots\sigma_{x}, then observe that wσ1w^{\prime}\sigma_{1} is equivalent to σ1σ2σ1σ3σ4σx\sigma_{1}\sigma_{2}\sigma_{1}\sigma_{3}\sigma_{4}\dots\sigma_{x} by commuting the trailing σ1\sigma_{1} past all the letters excepts σ1σ2\sigma_{1}\sigma_{2}. Now we can apply the braid relation σ1σ2σ1=σ2σ1σ2\sigma_{1}\sigma_{2}\sigma_{1}=\sigma_{2}\sigma_{1}\sigma_{2} to get an equivalent word σ2σ1σ2σ3σ4σx\sigma_{2}\sigma_{1}\sigma_{2}\sigma_{3}\sigma_{4}\dots\sigma_{x}. Note that all of these alterations to ww can be symmetrically applied to the other half of BB so that BB is equivalent to an intravergent braid BB^{\prime} containing only a single σ1\sigma_{1}. This reduces us to case (2).

    2. (3.1.2)

      If ww is equivalent to a word ww^{\prime} which contains σi2\sigma_{i}^{2} for some ii, then applying a crossing change will delete σi2\sigma_{i}^{2} from ww^{\prime}. We can apply these alterations symmetrically in BB as a type A move to obtain a positive intravergent braid BB^{\prime} with length 4\ell-4 whose closure is a knot B^\widehat{B^{\prime}}. By induction, we have that u~(B^)4s+12\widetilde{u}(\widehat{B^{\prime}})\leq\dfrac{\ell-4-s+1}{2} and hence

      u~(B^)2+u~(B^)s+12.\widetilde{u}(\widehat{B})\leq 2+\widetilde{u}(\widehat{B^{\prime}})\leq\dfrac{\ell-s+1}{2}.
    3. (3.1.3)

      If ww is equivalent to a word ww^{\prime} which still contains a single σ1\sigma_{1} but does not begin with σ1\sigma_{1}, then by induction on the number of letters between the two occurrences of σ1\sigma_{1} we can reduce to case (3.1.1) or (3.1.2).

  2. (3.2)

    The second case is that σ1\sigma_{1} appears once with index m\leq m and once with index >m>m. We begin by considering the word beginning at the first occurrence of σ1\sigma_{1} and ending at index mm. This word contains no other instances of σ1\sigma_{1}, so we may apply Lemma 3.3 and alter BB symmetrically in the indices >m>m. If the result contains the square of a generator, then we may proceed as in case (3.1.2). Otherwise, the result is an equivalent intravergent braid BB^{\prime} which still contains a single σ1\sigma_{1} with index m\leq m and a single σ1\sigma_{1} with index >m>m, and for which the subword from the first σ1\sigma_{1} to the middle index mm is w=σ1σ2σiw=\sigma_{1}\sigma_{2}\dots\sigma_{i}. In particular i=len(w)i=\operatorname{len}(w). Note that by the symmetry of BB^{\prime}, the length ii word which occurs directly after ww in BB^{\prime} is w¯=σ2ni+1σ2ni+2σ2n\overline{w}=\sigma_{2n-i+1}\sigma_{2n-i+2}\dots\sigma_{2n}. We now consider 3 possibilities depending on ii and nn.

    1. (3.2.1)

      If i<ni<n, then ww commutes with w¯\overline{w} so that we can alter BB^{\prime} by replacing ww¯w\overline{w} with w¯w\overline{w}w. Furthermore, it is not hard to see that this replacement is realized by a symmetric isotopy of BB^{\prime}. The result is an intravergent braid with two occurrences of σ1\sigma_{1}, both of which occur with index >m>m. This reduces us back to case (3.1).

    2. (3.2.2)

      If i=ni=n, then w¯=σn+1σn+2σ2n\overline{w}=\sigma_{n+1}\sigma_{n+2}\dots\sigma_{2n}, and we consider the word wRHSw_{RHS} beginning with the first letter after w¯\overline{w} and ending with the σ1\sigma_{1} which has index >m>m. We may then apply Lemma 3.3 until wRHSw_{RHS} either contains the square of a positive generator, in which case we proceed as in case (3.1.2), or is the word σjσj1σ2σ1\sigma_{j}\sigma_{j-1}\dots\sigma_{2}\sigma_{1} for some j1j\geq 1. In the latter situation we have 3 cases.

      1. (3.2.2.1)

        If j<nj<n, we first commute wRHSw_{RHS} past w¯\overline{w}, and then we are in a situation similar to case (3.2.1), but with the order of the braid reversed. Hence a symmetric argument applies to reduce to case (3.1).

      2. (3.2.2.2)

        If j=nj=n, then we consider the leading σn\sigma_{n} of wRHSw_{RHS}, which we may commute past every letter of w¯\overline{w} except σn+1\sigma_{n+1}. Symmetrically, we also commute a σn+1\sigma_{n+1} past every letter of ww except the trailing σn\sigma_{n}. The result is an intravergent braid with the middle four letters σn+1σnσn+1σn\sigma_{n+1}\sigma_{n}\sigma_{n+1}\sigma_{n}. This is the situation shown on the top left in Figure 4. Applying a type B move then produces an intravergent braid B′′B^{\prime\prime} which has σn+1σnσn+1σn\sigma_{n+1}\sigma_{n}\sigma_{n+1}\sigma_{n} replaced with σnσn+1\sigma_{n}\sigma_{n+1} as shown on the top right in Figure 4. We then calculate

        u~(B^)=u~(B^)1+u~(B′′^)1+(2)s+12=s+12.\widetilde{u}(\widehat{B})=\widetilde{u}(\widehat{B^{\prime}})\leq 1+\widetilde{u}(\widehat{B^{\prime\prime}})\leq 1+\dfrac{(\ell-2)-s+1}{2}=\dfrac{\ell-s+1}{2}.
      3. (3.2.2.3)

        If j>nj>n, we will use a reductive argument to reduce to case (3.2.2.2). We begin by looking at the first letter of wRHSw_{RHS} and w¯\overline{w}. We have w¯σj=σn+1σn+2σ2nσj\overline{w}\sigma_{j}=\sigma_{n+1}\sigma_{n+2}\dots\sigma_{2n}\sigma_{j}, and commuting σj\sigma_{j} as far to the left as possible, we have σn+1σn+2σjσj+1σjσj+2σ2n\sigma_{n+1}\sigma_{n+2}\dots\sigma_{j}\sigma_{j+1}\sigma_{j}\sigma_{j+2}\dots\sigma_{2n}. We then apply the braid relation to σjσj+1σj\sigma_{j}\sigma_{j+1}\sigma_{j} to obtain σn+1σn+2σj+1σjσj+1σj+2σ2n\sigma_{n+1}\sigma_{n+2}\dots\sigma_{j+1}\sigma_{j}\sigma_{j+1}\sigma_{j+2}\dots\sigma_{2n}. We now commute the leftmost σj+1\sigma_{j+1} all the way to the left to obtain σj+1σn+1σn+2σ2n\sigma_{j+1}\sigma_{n+1}\sigma_{n+2}\dots\sigma_{2n}. Applying all of these changes symmetrically to BB^{\prime} produces a new intravergent braid B′′B^{\prime\prime} whose symmetry exchanges σj+1\sigma_{j+1} with the preceding letter, which must therefore be σ2nj\sigma_{2n-j}. We can now symmetrically commute σj+1\sigma_{j+1} with σ2nj\sigma_{2n-j} so that the right half of B′′B^{\prime\prime} begins σ2njσn+1σn+2σ2n\sigma_{2n-j}\sigma_{n+1}\sigma_{n+2}\dots\sigma_{2n}. Since j>nj>n, we have that 2nj<n2n-j<n, and hence we may commute σ2nj\sigma_{2n-j} to the right of this word. In total we have now replaced w¯wRHS\overline{w}w_{RHS} with w¯σ2njσj1σj2σ1\overline{w}\sigma_{2n-j}\sigma_{j-1}\sigma_{j-2}\dots\sigma_{1}. We can now apply the argument in part (c) of the proof of Lemma 3.3 to the word σ2njσj1σj2σ1\sigma_{2n-j}\sigma_{j-1}\sigma_{j-2}\dots\sigma_{1} to get σj1σj2σ1σ2nj+1\sigma_{j-1}\sigma_{j-2}\dots\sigma_{1}\sigma_{2n-j+1}. We may now repeat this entire process with wRHS=σj1σj2σ1w_{RHS}=\sigma_{j-1}\sigma_{j-2}\dots\sigma_{1}, that is we have reduced jj by 1. We continue until j=nj=n, which is case (3.2.2.2).

    3. (3.2.3)

      If i=n+1i=n+1, then the middle four letters of BB^{\prime}, consisting of the last two letters of ww and the first two letters of w¯\overline{w}, are σnσn+1σnσn+1\sigma_{n}\sigma_{n+1}\sigma_{n}\sigma_{n+1}. In this case we can perform a type B move to BB^{\prime}, replacing these four letters with σn+1σn\sigma_{n+1}\sigma_{n} to obtain a new intravergent braid B′′B^{\prime\prime} with len(B′′)=len(B)2\operatorname{len}(B^{\prime\prime})=\operatorname{len}(B^{\prime})-2. See Figure 4. By the inductive assumption, we then calculate

      u~(B^)=u~(B^)1+u~(B′′^)1+(2)s+12=s+12.\widetilde{u}(\widehat{B})=\widetilde{u}(\widehat{B^{\prime}})\leq 1+\widetilde{u}(\widehat{B^{\prime\prime}})\leq 1+\dfrac{(\ell-2)-s+1}{2}=\dfrac{\ell-s+1}{2}.
      Refer to caption
      Figure 4. The middle three strands of two intravergent braids with 2n+12n+1 strands. On the top left is the braid corresponding to σn+1σnσn+1σn\sigma_{n+1}\sigma_{n}\sigma_{n+1}\sigma_{n}, which becomes σnσn+1\sigma_{n}\sigma_{n+1} (top right) after performing a type B move. On the bottom left is the braid corresponding to σnσn+1σnσn+1\sigma_{n}\sigma_{n+1}\sigma_{n}\sigma_{n+1}, which becomes σn+1σn\sigma_{n+1}\sigma_{n} (bottom right) after performing a type B move.
    4. (3.2.4)

      If i>n+1i>n+1, then consider the ending portion of ww consisting of σn+1σn+2σi\sigma_{n+1}\sigma_{n+2}\dots\sigma_{i}, and the subsequent letter, which by symmetry is σ2n+1i\sigma_{2n+1-i}. Since i>n+1i>n+1, we have that σ2n+1i\sigma_{2n+1-i} commutes past σi\sigma_{i} symmetrically. In the original location of ww, we now have the word w=σ1σ2σi2σi1σ2n+1iw^{\prime}=\sigma_{1}\sigma_{2}\dots\sigma_{i-2}\sigma_{i-1}\sigma_{2n+1-i}. Referring back to the proof of case (c) in Lemma 3.3, we conclude that ww^{\prime} is equivalent to the word σ2n+2iσ1σ2σi2σi1\sigma_{2n+2-i}\sigma_{1}\sigma_{2}\dots\sigma_{i-2}\sigma_{i-1}. Finally, by induction on the length of ww, we may repeat this argument until we reduce back to case (3.2.3).

Finally, returning to case (4), there must be two occurrences of σ1\sigma_{1} with index m\leq m or two occurrences of σ1\sigma_{1} with index >m>m so that the proof is identical to case (3.1). ∎

Proof of Theorem 1.13.

First, note that torus knots are closures of positive intravergent braids. Indeed, for the torus knot K=T(p,q)K=T(p,q) we can assume without loss of generality that pp is odd, and a positive intravergent braid with closure KK is given by the word

(i=1p1σi)q\left(\prod_{i=1}^{p-1}\sigma_{i}\right)^{q}

on pp strands. Now by Proposition 1.14 we have that u~(K)(p1)qp+12=(p1)(q1)2\widetilde{u}(K)\leq\dfrac{(p-1)q-p+1}{2}=\dfrac{(p-1)(q-1)}{2}. Then since u(K)u~(K)u(K)\leq\widetilde{u}(K), and u(K)=(p1)(q1)2u(K)=\dfrac{(p-1)(q-1)}{2} by [KM93], we have the desired equality u(K)=u~(K)u(K)=\widetilde{u}(K). ∎

4. Type A unknotting

We begin by restating and proving Theorem 1.5 and Theorem 1.9.

See 1.5

Proof.

To begin, consider an intravergent diagram for a strongly invertible knot KK, that is a symmetric diagram where the axis of symmetry is orthogonal to the plane of the diagram. Since KK is strongly invertible, there is a central crossing where the knot intersects the axis of symmetry. Cutting KK at this central crossing, we have two arcs γ1\gamma_{1} and γ2\gamma_{2}. Note that changing any symmetric pair of crossings in this diagram constitutes a type A crossing change. With a sequence of such crossing changes we can ensure that γ1\gamma_{1} always passes over γ2\gamma_{2}, and furthermore that γ1\gamma_{1} (and hence by symmetry γ2\gamma_{2}) is an unknotted arc. Then an isotopy reduces the diagram to only the single central crossing, which represents the unknot. An example is shown in Figure 5. ∎

Refer to caption
Figure 5. An example of unknotting a strongly invertible knot with only type A crossing changes, by ensuring that the black arc always passes over the gray arc, and that the black and gray arcs are unknotted.

See 1.9

Proof.

Consider any type A crossing change pair, {c,ρ(c)}\{c,\rho(c)\}. Taking the quotient, the effect is a crossing change on 𝔮1(K)\mathfrak{q}_{1}(K) and a crossing change on 𝔮2(K)\mathfrak{q}_{2}(K). Thus any type A unknotting sequence for KK induces an unknotting sequence of the same length for both 𝔮1(K)\mathfrak{q}_{1}(K) and 𝔮2(K)\mathfrak{q}_{2}(K). ∎

As a consequence of this theorem, we can immediately see that the type A unknotting number can be unbounded, even for knots with a fixed unknotting number.

Corollary 4.1.

For any positive integer nn, there is a strongly invertible knot KnK_{n} such that u(Kn)=1u(K_{n})=1, but u~A(Kn)n\widetilde{u}_{A}(K_{n})\geq n. In particular the difference u~A(Kn)u(Kn)\widetilde{u}_{A}(K_{n})-u(K_{n}) is unbounded.

Proof.

Consider the twist knot KnK_{n} shown in Figure 6. By changing one of the bottom off-axis crossings we can easily see that u(Kn)=1u(K_{n})=1. However, the quotient knot 𝔮1(Kn)\mathfrak{q_{1}}(K_{n}) is T(2,2n+1)T(2,2n+1), and by Kronheimer and Mrowka’s proof of the Milnor conjecture [KM93, Corollary 1.3] we have u(T(2,2n+1))=nu(T(2,2n+1))=n. By Theorem 1.9 we conclude that u~A(Kn)n\widetilde{u}_{A}(K_{n})\geq n. ∎

\begin{overpic}[width=200.0pt,grid=false]{twistknots.pdf} \put(20.0,22.5){\large$n$} \put(78.7,22.5){\large$n$} \end{overpic}
Figure 6. A strongly invertible twist knot KnK_{n} (left) and the quotient 𝔮1(Kn)=T(2,2n+1)\mathfrak{q}_{1}(K_{n})=T(2,2n+1) (right) corresponding to the unbounded arc of the axis. The nn indicates nn full twists so that KnK_{n} is alternating with 2n+22n+2 crossings.

5. Type B unknotting

We begin by discussing 4-moves, which, as we shall see, are closely related to type B moves for strongly invertible knots.

Definition 5.1.

A 4-move on a knot KK is a local tangle replacement as shown in Figure 7. The minimum number of 4-moves necessary to unknot a knot KK is the 4-move unknotting number u4(K)u_{4}(K). If KK cannot be unknotted with 4-moves, then we say that u4(K)=u_{4}(K)=\infty.

Refer to caption
Figure 7. The 4-move as a local tangle replacement.

It is an old conjecture [NS87, Conjecture B] (which appears in the Kirby problem list [Kir97, 1.59(3)(a)]) that every knot can be unknotted with 4-moves. This conjecture has been verified through 12 crossings in [Prz16], which also contains a history of the problem.

Lemma 5.2.

Let KK be a strongly invertible knot with quotients 𝔮1(K)\mathfrak{q}_{1}(K) and 𝔮2(K)\mathfrak{q}_{2}(K). Applying a type B move to KK has the effect of applying a 4-move to one of 𝔮1(K)\mathfrak{q}_{1}(K) or 𝔮2(K)\mathfrak{q}_{2}(K), but has no effect on the other quotient knot.

Proof.

Consider a type B move on KK, and note that the crossing change must occur at a fixed point of the symmetry so that we have the situation shown in Figure 8. We then have two cases. If the type B crossing change occurs on h1h_{1}, then the dotted axis becomes an arc of 𝔮1(K)\mathfrak{q}_{1}(K) so that we have a 4-move on 𝔮1(K)\mathfrak{q}_{1}(K) but there is no effect on 𝔮2(K)\mathfrak{q}_{2}(K). If the type B crossing change occurs on h2h_{2}, then the dotted axis becomes an arc of 𝔮2(K)\mathfrak{q}_{2}(K), so that we have a 4-move on 𝔮2(K)\mathfrak{q}_{2}(K) but there is no effect on 𝔮1(K)\mathfrak{q}_{1}(K). ∎

Refer to caption
Figure 8. A type B crossing change on a strongly invertible knot KK (left) becomes a 4-move on 𝔮1(K)\mathfrak{q}_{1}(K) (right) when the shown section of the axis of symmetry is h1h_{1}.

See 1.10

Proof.

Any length nn unknotting sequence of type B moves on KK produces 4-move unknotting sequences for both 𝔮1(K)\mathfrak{q}_{1}(K) and 𝔮2(K)\mathfrak{q}_{2}(K) whose lengths sum to nn, by Lemma 5.2. ∎

Corollary 5.3.

If for every strongly invertible knot KK we have u~B(K)<\widetilde{u}_{B}(K)<\infty, then every knot can be unknotted with 4-moves.

Proof.

Let KK^{\prime} be a knot, and consider the strongly invertible knot K=K#rKK=K^{\prime}\#rK^{\prime} where the strong inversion exchanges the two factors. Note that 𝔮1(K)=𝔮2(K)=K\mathfrak{q}_{1}(K)=\mathfrak{q}_{2}(K)=K^{\prime}. Then since u~B(K)<\widetilde{u}_{B}(K)<\infty, we have that u4(K)+u4(K)<u_{4}(K^{\prime})+u_{4}(K^{\prime})<\infty by Theorem 1.10. ∎

The following theorem allows us to obstruct 2-bridge knots from having u4(K)=1u_{4}(K)=1. This theorem appears as Theorem 1.2 in [KT22]. For completeness, we provide a proof below.

Theorem 5.4 (Theorem 1.2 in [KT22]).

Let KK be a 2-bridge knot corresponding to the fraction p/qp/q. Then u4(K)=1u_{4}(K)=1 if and only if there are integers rr and ss such that

  1. (1)

    gcd(r,s)=1\gcd(r,s)=1,

  2. (2)

    4rs=±p±14rs=\pm p\pm 1, and

  3. (3)

    ±q±14s2\pm q^{\pm 1}\equiv 4s^{2} mod pp.

Proof.

For the forward direction, suppose that u4(K)=1u_{4}(K)=1. By an analog of the Montesinos trick, the 2-fold branched cover Σ(K)\Sigma(K) of S3S^{3} over KK can be obtained by D/4D/4 surgery on some knot KK^{\prime} in S3S^{3}. However, since Σ(K)=L(p,q)\Sigma(K)=L(p,q) has a cyclic fundamental group, the cyclic surgery theorem [CGLS87] tells us that the exterior of KK^{\prime} is Seifert fibered from which we can see that π1(K)\pi_{1}(K^{\prime}) has a non-trivial center. Then by [BZ66], KK^{\prime} must be a torus knot T(r,s)T(r,s). Since KK^{\prime} is a knot and not a link we immediately have (1). Now by Moser’s theorem classifying torus knot surgeries [Mos71], a D/4D/4 surgery on a torus knot which produces a lens space must be of the form SD/43(T(r,s))=L(D,4s2)S^{3}_{D/4}(T(r,s))=L(D,4s^{2}), where |4rs+D|=1|4rs+D|=1. Since we in fact obtain L(p,q)L(p,q), we have D=±pD=\pm p and 4rs=±p±14rs=\pm p\pm 1 so that (2) is satisfied. Finally, by the classification of lens spaces, we have that L(p,q)L(p,q) is orientation-preserving homeomorphic to one of L(±p,4s2)L(\pm p,4s^{2}) if and only if condition (3) is satisfied.

For the reverse direction, consider the the torus knot T(r,s)T(r,s), and let D=4rs±1D=4rs\pm 1 such that |D|=|p||D|=|p|. Now T(r,s)T(r,s) has a unique strong inversion ρ\rho which induces a symmetry which we again call ρ\rho on SD/43(T(r,s))=L(D,4s2)S^{3}_{D/4}(T(r,s))=L(D,4s^{2}). Now by [HR85, Corollary 4.12], each lens space is the double branched cover of a unique link (specifically a 2-bridge link) so that the quotient of L(D,4s2)L(D,4s^{2}) by ρ\rho must be the 2-bridge knot with fraction p/qp/q. We now compare the images of the fixed-point sets in S3/ρS^{3}/\rho and L(D,4s2)/ρL(D,4s^{2})/\rho. In S3/ρS^{3}/\rho we have a trivial tangle consisting of two arcs in a 3-ball, which is the quotient of a neighborhood of T(r,s)T(r,s). In L(D,4s2)/ρL(D,4s^{2})/\rho, the tangle becomes twisted by the D/4D/4 surgery to give us 4 half twists; that is a 4-move. ∎

Before discussing applications to u~B\widetilde{u}_{B}, we give an example of a direct application of Theorem 5.4 to the figure-eight knot.

Example 5.5.

Consider the knot K=41K=4_{1}, which is the 2-bridge knot corresponding to the fraction 5/25/2. We then consider the possible values of ss in Theorem 5.4. Since 4s4s is a factor of ±p±1={6,4,4,6}\pm p\pm 1=\{-6,-4,4,6\}, we have that |s|=1|s|=1. However, ±2±1={2,3}\pm 2^{\pm 1}=\{2,3\} mod 5, so that ±q±14s2\pm q^{\pm 1}\not\equiv 4s^{2} mod 5. We conclude that u4(K)1u_{4}(K)\neq 1. On the other hand it is not hard to see that u4(K)2u_{4}(K)\leq 2 by directly performing two 4-moves on KK; see Figure 9.

Refer to caption
Figure 9. Performing a 4-move on the figure-eight knot (left) by changing the crossings in the clasp in the shaded box produces the trefoil. After an isotopy we get the diagram shown on the right, and performing the indicated 4-move produces the unknot.

By combining Theorem 5.4 and Theorem 1.10 we find a knot KK where u~B(K)u(K)2\widetilde{u}_{B}(K)-u(K)\geq 2.

Example 5.6.

Consider the knot K=41#41K=4_{1}\#4_{1} with the strong inversion which exchanges the two components. Then 𝔮1(K)=𝔮2(K)=41\mathfrak{q}_{1}(K)=\mathfrak{q}_{2}(K)=4_{1}, and by Theorem 5.4 (see Example 5.5) we have that u4(41)=2u_{4}(4_{1})=2. Theorem 1.10 then says that u~B(K)2+2=4\widetilde{u}_{B}(K)\geq 2+2=4, in contrast with the usual unknotting number of KK, which is 2.

6. Type C unknotting

We start by proving Theorem 1.11.

Definition 6.1.

The non-orientable band unknotting number unb(K)u_{nb}(K) of a knot KK is the minimum number of non-orientable band moves needed to transform KK into the unknot.

See 1.11

Proof.

We claim that a type C crossing change on KK descends to a non-orientable band move on the quotient theta graph which restricts to a non-orientable band move on one of 𝔮1(K)\mathfrak{q}_{1}(K) and 𝔮2(K)\mathfrak{q}_{2}(K), without affecting the other. Note that when KK is the unknot both 𝔮1(K)\mathfrak{q}_{1}(K) and 𝔮2(K)\mathfrak{q}_{2}(K) are unknots, and so the theorem will follow by induction on u~C(K)\widetilde{u}_{C}(K).

We now prove the claim. Consider a type C crossing change, as shown on the left in Figure 10. We have chosen a diagram so that the isotopy corresponding to the type C crossing change is compact; considering a type C move which passes through infinity in the indicated diagram would have the effect of exchanging 𝔮1(K)\mathfrak{q}_{1}(K) and h1h_{1} with 𝔮2(K)\mathfrak{q}_{2}(K) and h2h_{2} in what follows. The quotient theta graph admits a diagram as in the center of Figure 10. Then the indicated band move restricts to an R1 move on the induced diagram of 𝔮1(K)\mathfrak{q}_{1}(K), so that the knot type of 𝔮1(K)\mathfrak{q}_{1}(K) remains unchanged, and restricts to a non-orientable band move on 𝔮2(K)\mathfrak{q}_{2}(K).

\begin{overpic}[width=230.0pt,grid=false]{typeCquotient.pdf} \put(101.0,38.0){$h_{1}$} \put(58.0,60.0){$h_{1}$} \put(101.0,50.0){$h_{2}$} \put(58.0,72.0){$h_{2}$} \end{overpic}
Figure 10. The effect of a type C crossing change (left) on the quotient theta graph (center) of a strongly invertible knot is a non-orientable band move (right). The dashed line indicates the axis of symmetry, and the solid line indicates the knot.

Remark 6.2.

There are several straightforward lower bounds on unb(K)u_{nb}(K), such as the (not necessarily orientable) band-unlinking number and the non-orientable 4-genus, and lower bounds on both of these have appeared in the literature. For example, a lower bound for the band-unlinking number is given in [HNT90, Theorem 4] in terms of the homology groups of cyclic branched coverings of KK, and lower bounds on the non-orientable 4-genus can be found in [Bat14], [OSS17], and [GM23]. Many of these lower bounds rely on knot Floer homology, but the invariants are computable in our situation. Indeed, it follow from Theorem 1.8 that the quotients of type C unknottable knots are (1,1)-knots.

6.1. Type C unknottable knots

In this section we classify which strongly invertible knots can be unknotted with a sequence of type C moves. Our main result is Theorem 1.8, which we recall here for convenience.

See 1.8

Corollary 6.3.

Let KK be a strongly invertible knot which can be equivariantly unknotted with type C moves and let t(K)t(K) be the tunnel number of KK. Then t(K)2t(K)\leq 2.

Proof.

By Theorem 1.8, KK is a (1,2)(1,2) knot. We will show that (1,2)(1,2) knots have tunnel number 2 or less. Indeed, consider the (1,2)(1,2) decomposition of KK which is the union of two handlebodies H1H2H_{1}\cup H_{2}. We may connect the two boundary parallel arcs of KH1K\cap H_{1} with a pair of arcs γ1\gamma_{1} and γ2\gamma_{2} such that γ1γ2\gamma_{1}\cup\gamma_{2} is isotopic to the core of H1H_{1}. Removing a neighborhood of Kγ1γ2K\cup\gamma_{1}\cup\gamma_{2} from S3S^{3} leaves us with a space which retracts onto H2H_{2} with a pair of thickened boundary-parallel arcs removed. This is a genus 3 handlebody, so that the tunnel number of KK is at most 2. ∎

We can now prove Theorem 1.3, which we restate here for convenience. See 1.3

Proof.

By [SS99, Theorem 14], the tunnel number of K1#K2#K3K_{1}\#K_{2}\#K_{3} is at least 3, so that by Corollary 6.3, u~C(K1#K2#K3)=\widetilde{u}_{C}(K_{1}\#K_{2}\#K_{3})=\infty. ∎

6.2. Proof of Theorem 1.8

We begin with some necessary definitions and lemmas.

Definition 6.4.

Let aa and bb be a pair of arcs in D2×S1D^{2}\times S^{1} which are symmetric under a π\pi rotation around the core {0}×S1\{0\}\times S^{1} of the handlebody. Considered up to isotopy relative to the four points on the boundary, we say that aa and bb are trivial if they match exactly the arcs shown on the left in Figure 11, where the dotted line indicates the core of the handlebody.

\begin{overpic}[width=350.0pt,grid=false]{typeCoutcomes.pdf} \put(48.0,55.3){$n/2$} \put(48.0,16.5){$n/2$} \put(82.5,9.4){$n/2$} \put(82.5,47.3){$n/2$} \end{overpic}
Figure 11. A trivial pair of arcs in D2×S1D^{2}\times S^{1} (left). The possible symmetric surgery curves corresponding to a type C crossing change are shown top center and top right, where n/2n/2 indicates nn half-twists. The resulting tangles after the type C crossing change are shown bottom center and bottom right, respectively.

For the following lemma, note that we can perform type C crossing changes on strongly invertible tangles in D2×S1D^{2}\times S^{1} (where the axis of symmetry is the core of the handlebody), using essentially the same definition as for strongly invertible knots.

Lemma 6.5.

Given a pair of trivial symmetric arcs in D2×S1D^{2}\times S^{1}, the result of a type C move, up to equivariant isotopy relative to the boundary, is one of the tangles shown in Figure 11 in the bottom center or bottom right.

Proof.

To begin, we will think of a type C move as surgery along an unknot which bounds a symmetric disk that intersects each arc once. Since this disk can intersect each arc only once and is symmetric, the disk must intersect the arcs at their fixed points. Now any order 2 symmetry of a disk has a contractible fixed set by classical results of Smith (see for example [AP93, Corollary 1.3.8]). Since we have at least two fixed points (one on each arc), the fixed set of the disk must be an arc. There are exactly two fixed arcs connecting the two known fixed points, so the disk retracts to an interval bundle over an arc contained in the axis of symmetry. The two resulting possibilities are shown in the top center or top right of Figure 11. Finally, performing +1+1-surgery along these curves produces the arcs shown in the bottom center and bottom right of Figure 11. ∎

Let Ti2T^{2}_{i} be the torus with ii punctures. Let MCG(T22)\operatorname{MCG}(T^{2}_{2}) be the mapping class group of the twice-punctured torus T22T^{2}_{2}. Let MCG((S1×D2)2)\operatorname{MCG}((S^{1}\times D^{2})_{2}) be the mapping class group of S1×D2S^{1}\times D^{2} which preserves setwise a pair of marked points on the boundary. Let SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}) be the symmetric mapping class group of S1×D2S^{1}\times D^{2} consisting of diffeomorphisms which respect the symmetry ρ\rho given by a π\pi rotation on the D2D^{2} component and preserve a ρ\rho-invariant set of four marked points. Finally, let LMCG((S1×D2)2)\operatorname{LMCG}((S^{1}\times D^{2})_{2}) be the image of SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}) in MCG((S1×D2)2)\operatorname{MCG}((S^{1}\times D^{2})_{2}) under the map induced by the quotient.

The following lemma can be thought of as a Birman-Hilden-type theorem (see e.g. [MW21]) for the two-fold branched covering of a genus one handlebody with two marked points over its core.

Lemma 6.6.

There is a short exact sequence of groups

1/2𝑖SMCG((S1×D2)4)𝑝LMCG((S1×D2)2)1,1\to\mathbb{Z}/2\mathbb{Z}\overset{i}{\to}\operatorname{SMCG}((S^{1}\times D^{2})_{4})\overset{p}{\to}\operatorname{LMCG}((S^{1}\times D^{2})_{2})\to 1,

where ii is the inclusion of the subgroup generated by the mapping class of ρ\rho, and pp is the map induced from the quotient map of the symmetry ρ\rho.

Proof.

First, observe that pip\circ i is the trivial map, since ρ\rho projects to the identity map on (S1×D2)2(S^{1}\times D^{2})_{2}. It remains to check that the kernel of pp is the subgroup generated by [ρ][\rho] in SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}). Let fSMCG((S1×D2)4)f\in\operatorname{SMCG}((S^{1}\times D^{2})_{4}) such that p(f)p(f) is trivial in LMCG((S1×D2)2)\operatorname{LMCG}((S^{1}\times D^{2})_{2}). By composing with an equivariant diffeomorphism near the core if necessary, we may assume that ff fixes the core S1×{0}S^{1}\times\{0\} pointwise. We show below that there is an isotopy HH from p(f)p(f) to the identity map IdId such that at each time tt, HtH_{t} fixes the core setwise. Since HH fixes the core, we can lift HH to an equivariant isotopy on (S1×D2)4(S^{1}\times D^{2})_{4} from ff to an element in p1(Id)p^{-1}(Id). Hence ff is in the subgroup generated by [ρ][\rho].

To construct HH, first note that since p(f)p(f) is isotopic to the identity, we may isotope p(f)p(f) near the boundary so that the boundary is pointwise fixed. This isotopy also fixes a neighborhood of the core pointwise. Now choose an annulus AA embedded in S1×D2S^{1}\times D^{2} such that the one boundary component of AA is the core, and the other boundary component lies on (S1×D2)\partial(S^{1}\times D^{2}). Now consider AA and p(f)(A)p(f)(A). By a standard argument applied to the intersection between AA and p(f)(A)p(f)(A), we can isotope across 3-balls and handlebodies bounded by Ap(f)(A)A\cup p(f)(A) to modify p(f)p(f) such that p(f)(A)=Ap(f)(A)=A, and these isotopies fix pointwise the core and the boundary. Next, we isotope p(f)p(f) (fixing (S1×D2)\partial(S^{1}\times D^{2}) pointwise, but applying full twists to the core as necessary) so that p(f)|Ap(f)|_{A} is the identity map. The problem is now reduced to finding an isotopy relative to (S1×S1)A(S^{1}\times S^{1})\cup A between p(f)p(f) and IdId. To do this, first isotope p(f)p(f) to be identity on a neighborhood ν(A(S1×S1))\nu(A\cup(S^{1}\times S^{1})). Then recall that the mapping class group of S1×D2S^{1}\times D^{2}, which is diffeomorphic to (S1×D2)(ν(AS1×S1))(S^{1}\times D^{2})-(\nu(A\cup S^{1}\times S^{1})), is a subgroup of the mapping class group of its boundary. Hence there is an isotopy between p(f)|(S1×D2)(ν(AS1×S1))p(f)|_{(S^{1}\times D^{2})-(\nu(A\cup S^{1}\times S^{1}))} and IdId, which fixes at each time its boundary. Gluing this to the identity isotopy on ν(S1×S1A)\nu(S^{1}\times S^{1}\cup A), we have an isotopy HH from p(f)p(f) to IdId which fixes pointwise at each time the boundary preserves the core setwise.

\begin{overpic}[width=300.0pt,grid=false]{MCGgens.pdf} \put(58.0,36.0){$\beta$} \put(79.0,28.0){$\alpha$} \put(58.0,11.0){$\gamma$} \put(48.0,6.5){$\delta$} \end{overpic}
Figure 12. The torus with two marked points (S1×S1)2(S^{1}\times S^{1})_{2} with the indicated curves α,β,γ\alpha,\beta,\gamma, and δ\delta. When thought of as the boundary of S1×D2S^{1}\times D^{2}, the curves β\beta and γ\gamma bound disks.

Before proceeding, we define some elements of MCG((S1×S1)2)\operatorname{MCG}((S^{1}\times S^{1})_{2}) which we will use to write down a generating set for LMCG((S1×D2)2)\operatorname{LMCG}((S^{1}\times D^{2})_{2}). We will need the following specific diffeomorphisms, which we will also use to represent the corresponding isotopy classes of diffeomorphisms. The definitions refer to the curves indicated in Figure 12.

  1. (1)

    The diffeomorphisms tαt_{\alpha}, tβt_{\beta} and tγt_{\gamma} are given by Dehn twists around the curves α\alpha, β\beta and γ\gamma respectively.

  2. (2)

    The diffeomorphism τ\tau is given by tαtβtαtγtαtβt_{\alpha}t_{\beta}t_{\alpha}t_{\gamma}t_{\alpha}t_{\beta}, which is the hyperelliptic involution which fixes the two marked points, preserves α\alpha, and swaps β\beta and γ\gamma.

  3. (3)

    The diffeomorphism σ\sigma is the identity map outside of a neighborhood of δ\delta, and swaps the marked points by a clockwise 180180^{\circ} rotation within a neighborhood of δ\delta.

  4. (4)

    The diffeomorphism mm is given by tβtγ1t_{\beta}t_{\gamma}^{-1}, which pulls one marked point around a loop parallel to β\beta.

  5. (5)

    The diffeomorphism \ell is given by tγtβ1tαtβtγ1tα1t_{\gamma}t_{\beta}^{-1}t_{\alpha}t_{\beta}t_{\gamma}^{-1}t_{\alpha}^{-1}, which pulls one marked point around a loop parallel to α\alpha.

It will also be useful to remember that MCG((S1×D2)2)\operatorname{MCG}((S^{1}\times D^{2})_{2}) is exactly the subgroup of MCG((S1×S1)2)\operatorname{MCG}((S^{1}\times S^{1})_{2}) consisting of elements which map a meridian to a meridian. Hence we can slightly abuse notation and use (compositions of) the above diffeomorphisms to refer to elements of MCG((S1×D2)2)\operatorname{MCG}((S^{1}\times D^{2})_{2}), whenever a meridian is taken to a meridian.

Lemma 6.7.

The pure mapping class group PMCG((S1×D2)2)\operatorname{PMCG}((S^{1}\times D^{2})_{2}) is generated by tβt_{\beta}, τ\tau, mm, and \ell. Moreover, every element of PMCG((S1×D2)2)\operatorname{PMCG}((S^{1}\times D^{2})_{2}) is of the form wtβiτjw\cdot t_{\beta}^{i}\cdot\tau^{j}, where ww is a word in mm and ll, ii\in\mathbb{Z}, and j{0,1}j\in\{0,1\}.

Proof.

Consider the natural map Ψ:PMCG((S1×S1)2)MCG(S1×S1)\Psi\colon\operatorname{PMCG}((S^{1}\times S^{1})_{2})\to\operatorname{MCG}(S^{1}\times S^{1}) given by forgetting the marked points. Then PMCG((S1×D2)2)=Ψ1(Ψ(tβ),Ψ(τ))\operatorname{PMCG}((S^{1}\times D^{2})_{2})=\Psi^{-1}(\langle\Psi(t_{\beta}),\Psi(\tau)\rangle). To see this we will check that Ψ(tβ)\Psi(t_{\beta}) and Ψ(τ)\Psi(\tau) generate the subgroup of MCG(S1×S1)\operatorname{MCG}(S^{1}\times S^{1}) consisting of elements which send meridians to meridians. Recalling that

MCG(S1×S1)SL2():βαβα,\operatorname{MCG}(S^{1}\times S^{1})\cong\textup{SL}_{2}(\mathbb{Z})\colon\mathbb{Z}\langle\beta\rangle\oplus\mathbb{Z}\langle\alpha\rangle\to\mathbb{Z}\langle\beta\rangle\oplus\mathbb{Z}\langle\alpha\rangle,

we have

Ψ(tβ)=[1101], and Ψ(τ)=[1001],\Psi(t_{\beta})=\begin{bmatrix}1&1\\ 0&1\end{bmatrix},\mbox{ and }\Psi(\tau)=\begin{bmatrix}-1&0\\ 0&-1\end{bmatrix},

which generate all matrices preserving β\langle\beta\rangle; that is matrices of the form

[±1n0±1].\begin{bmatrix}\pm 1&n\\ 0&\pm 1\end{bmatrix}.

Now we observe that Ψ1(Ψ(tβ),Ψ(τ))\Psi^{-1}(\langle\Psi(t_{\beta}),\Psi(\tau)\rangle) is generated by tβt_{\beta}, τ\tau, and ker(Ψ)(\Psi). However ker(Ψ)=m,(\Psi)=\langle m,\ell\rangle; see for example [CM04, Proposition 1]. Hence PMCG((S1×D2)2)=tβ,τ,m,\operatorname{PMCG}((S^{1}\times D^{2})_{2})=\langle t_{\beta},\tau,m,\ell\rangle. Finally, since every element of PMCG((S1×D2)2)\operatorname{PMCG}((S^{1}\times D^{2})_{2}) is a preimage of an element in MCG(S1×S1)\operatorname{MCG}(S^{1}\times S^{1}) of the form Ψ(tβiτj)\Psi(t_{\beta}^{i}\tau^{j}), each element can be written as wtβiτjw\cdot t_{\beta}^{i}\tau^{j} for some element ww in ker(Ψ)=m,(\Psi)=\langle m,\ell\rangle. ∎

Before the next lemma, we recall a special case of the liftability criteria from [GM20, Proposition 4.4]. We will use the notation from Figure 12, as well as the following.

Let LPMCG(Xn)\operatorname{LPMCG}(X_{n}) denote the liftable pure mapping class group of XX with nn marked points. We will be interested in Xn=(S1×S1)2X_{n}=(S^{1}\times S^{1})_{2} and Xn=(S1×D2)2X_{n}=(S^{1}\times D^{2})_{2}.

Let pp be the projection map corresponding to the 2-fold cover from the 4-punctured torus (S1×S1)4(S^{1}\times S^{1})_{4} to the 2-punctured torus (S1×S1)2(S^{1}\times S^{1})_{2} as induced by the symmetry ρ\rho above. Let

q:H1((S1×S1)2;)H1((S1×S1)2;)/pH1((S1×S1)4;)/2,q\colon H_{1}((S^{1}\times S^{1})_{2};\mathbb{Z})\to H_{1}((S^{1}\times S^{1})_{2};\mathbb{Z})/p_{*}H_{1}((S^{1}\times S^{1})_{4};\mathbb{Z})\cong\mathbb{Z}/2\mathbb{Z},

be the indicated map on homology. Note that q(β)=q(γ)=1q(\beta)=q(\gamma)=1 and q(α)=0q(\alpha)=0. Given a diffeomorphism f:(S1×S1)2(S1×S1)2f\colon(S^{1}\times S^{1})_{2}\to(S^{1}\times S^{1})_{2}, let afH1((S1×S1)2;)a_{f}\in H_{1}((S^{1}\times S^{1})_{2};\mathbb{Z}) be the element af=f(δ)δa_{f}=f(\delta)-\delta in the first homology group of (S1×S1)2(S^{1}\times S^{1})_{2} relative to the punctures. Here δ\delta is the homology class represented by the arc δ\delta in Figure 12.

Lemma 6.8 (Corollary of Proposition 4.4 of [GM20]).

The mapping class of ff is in LPMCG((S1×S1)2)\operatorname{LPMCG}((S^{1}\times S^{1})_{2}) if and only if qf(α)=0,qf(β)=qf(γ)=1qf_{*}(\alpha)=0,qf_{*}(\beta)=qf_{*}(\gamma)=1, and q(af)=0q(a_{f})=0.

Lemma 6.9.

The group LPMCG((S1×D2)2)\operatorname{LPMCG}((S^{1}\times D^{2})_{2}) is generated by tβ2,m2,mm1,,t_{\beta}^{2},m^{2},m\ell m^{-1},\ell, and τ\tau.

Proof.

We first observe that LPMCG((S1×D2)2)=LMCG((S1×S1)2)PMCG((S1×D2)2)\operatorname{LPMCG}((S^{1}\times D^{2})_{2})=\operatorname{LMCG}((S^{1}\times S^{1})_{2})\cap\operatorname{PMCG}((S^{1}\times D^{2})_{2}), by viewing MCG((S1×D2)2)\operatorname{MCG}((S^{1}\times D^{2})_{2}) as a subgroup of MCG((S1×S1)2)\operatorname{MCG}((S^{1}\times S^{1})_{2}). Then for any element xx in PMCG((S1×D2)2)\operatorname{PMCG}((S^{1}\times D^{2})_{2}), we can verify that xLPMCG((S1×D2)2)x\in\operatorname{LPMCG}((S^{1}\times D^{2})_{2}) using the conditions in Lemma 6.8. By Lemma 6.7, an arbitrary element of LPMCG((S1×D2)2)\operatorname{LPMCG}((S^{1}\times D^{2})_{2}) has the form f=wtβiτjf=wt_{\beta}^{i}\tau^{j} where ww is a word in mm and \ell, ii\in\mathbb{Z}, and j{0,1}j\in\{0,1\}. Observe that q(w(x))=q(x)q(w(x))=q(x) for all xH1((S1×S1)2;)x\in H_{1}((S^{1}\times S^{1})_{2};\mathbb{Z}), since qq factors through H1(S1×S1;)H_{1}(S^{1}\times S^{1};\mathbb{Z}), on which ww acts trivially. We then compute

qwtβiτj(α)\displaystyle qwt_{\beta}^{i}\tau^{j}(\alpha) =qwtβi((1)jα)=qwtβi(α)=qw(α+iβ)=q(α+iβ)=i,\displaystyle=qwt_{\beta}^{i}((-1)^{j}\alpha)=qwt_{\beta}^{i}(\alpha)=qw(\alpha+i\beta)=q(\alpha+i\beta)=i,
qwtβiτj(β)\displaystyle qwt_{\beta}^{i}\tau^{j}(\beta) =qwtβi((1)jβ)=qwtβi(β)=qw(β)=q(β)=1,\displaystyle=qwt_{\beta}^{i}((-1)^{j}\beta)=qwt_{\beta}^{i}(\beta)=qw(\beta)=q(\beta)=1,
qwtβiτj(γ)\displaystyle qwt_{\beta}^{i}\tau^{j}(\gamma) =qwtβi((1)jγ)=qwtβi(γ)=qw(γ)=q(γ)=1,\displaystyle=qwt_{\beta}^{i}((-1)^{j}\gamma)=qwt_{\beta}^{i}(\gamma)=qw(\gamma)=q(\gamma)=1,

so that ii must be even for wtβiτjwt_{\beta}^{i}\tau^{j} to be liftable. For last condition in Lemma 6.8, we will need to keep track of the algebraic number of mm’s and \ell’s appearing in ww, call these values |w|m|w|_{m} and |w||w|_{\ell} respectively. Also, observe that τ\tau is liftable by checking with Lemma 6.8. Indeed τ(δ)=δα\tau(\delta)=\delta-\alpha so that aτ=αa_{\tau}=-\alpha and q(α)=0q(-\alpha)=0. Then we have that wtβiτwt_{\beta}^{i}\tau is liftable if and only if wtβiwt_{\beta}^{i} is liftable. Additionally, note that for any xH1((S1×S1)2;)x\in H_{1}((S^{1}\times S^{1})_{2};\mathbb{Z}), we have m(x+δ)=x+γ+δm(x+\delta)=x+\gamma+\delta and (x+δ)=x+α+δ\ell(x+\delta)=x+\alpha+\delta, noting that any loop around a puncture is trivial in the relative homology group. We can then check

wtβi(δ)=w(δ)=δ+|w|mγ+|w|α,wt_{\beta}^{i}(\delta)=w(\delta)=\delta+|w|_{m}\gamma+|w|_{\ell}\alpha,

and so q(awtβi)=|w|mq(a_{wt_{\beta}^{i}})=|w|_{m}. We conclude that wtβiτjwt_{\beta}^{i}\tau^{j} is liftable if and only if ii and |w|m|w|_{m} are both even. Words of this form are generated by tβ2,m2,mm1,t_{\beta}^{2},m^{2},m\ell m^{-1},\ell and τ\tau, as desired. ∎

We now choose preimages of tβ2,m2,mm1,t_{\beta}^{2},m^{2},m\ell m^{-1},\ell, and τ\tau in SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}); see Lemma 6.6. We choose respectively the preimages tβ~,m~,~+,t_{\widetilde{\beta}},\widetilde{m},\widetilde{\ell}_{+}, and ~,\widetilde{\ell}_{-}, as described in Figure 13, and τ~\widetilde{\tau}, which is a hyperelliptic involution fixing the four marked points. We will also need the diffeomorphisms σ~\widetilde{\sigma}, which is the lift of σ\sigma given by swapping the four marked points in pairs, and ρ\rho, which is the deck transformation involution on (S1×D2)4(S^{1}\times D^{2})_{4}.

\begin{overpic}[width=420.0pt,grid=false]{SMCGgens.pdf} \put(76.5,7.1){$\widetilde{\gamma}$} \put(80.0,15.8){$\widetilde{\beta}$} \end{overpic}
Figure 13. Some generators of SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}). The generator tβ~t_{\widetilde{\beta}} is given by a Dehn twist around the meridian β~\widetilde{\beta}, the generator m~\widetilde{m} is given by the composition tβ~tγ~1t_{\widetilde{\beta}}t_{\widetilde{\gamma}}^{-1}, the generator ~+\widetilde{\ell}_{+} (left) is given by dragging the right two marked points around the indicated longitudes, and the generator ~\widetilde{\ell}_{-} (right) is given by dragging the right two marked points around the indicated longitudes.
Proposition 6.10.

The group SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}) is generated by tβ~,m~,~+,~,τ~,σ~,t_{\widetilde{\beta}},\widetilde{m},\widetilde{\ell}_{+},\widetilde{\ell}_{-},\widetilde{\tau},\widetilde{\sigma}, and ρ\rho.

Proof.

Note that there is an exact sequence

1LPMCG((S1×D2)2)LMCG((S1×D2)2)𝑓/21,1\to\operatorname{LPMCG}((S^{1}\times D^{2})_{2})\to\operatorname{LMCG}((S^{1}\times D^{2})_{2})\overset{f}{\to}\mathbb{Z}/2\mathbb{Z}\to 1,

such that f(σ)f(\sigma) is a generator for the /2\mathbb{Z}/2\mathbb{Z}. Hence by Lemma 6.7, LPMCG((S1×D2)2)\operatorname{LPMCG}((S^{1}\times D^{2})_{2}) is generated by tβ2,m2mm1,,τ,t_{\beta}^{2},m^{2}m\ell m^{-1},\ell,\tau, and σ\sigma. Now by Lemma 6.6, we have that SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}) is generated by lifts of the generators of LMCG((S1×D2)2)\operatorname{LMCG}((S^{1}\times D^{2})_{2}) together with ρ\rho. In particular, tβ~,m~,~+,~,τ~,σ~,t_{\widetilde{\beta}},\widetilde{m},\widetilde{\ell}_{+},\widetilde{\ell}_{-},\widetilde{\tau},\widetilde{\sigma}, and ρ\rho generate SMCG((S1×D2)4)\operatorname{SMCG}((S^{1}\times D^{2})_{4}). ∎

Lemma 6.11.

Let aa and bb be the trivial pair of ρ\rho-invariant arcs in ((S1×D2)4,ρ)((S^{1}\times D^{2})_{4},\rho) as shown on the left in Figure 11. Let wSMCG((S1×D2)4,ρ)w\in\operatorname{SMCG}((S^{1}\times D^{2})_{4},\rho) so that we may consider new boundary parallel arcs w(ab)w(a\cup b). Then w(ab)w(a\cup b) is related to aba\cup b by a sequence of type C moves.

Proof.

We will write ww as a word in the generators tβ~,m~,~+,~,τ~,σ~,t_{\widetilde{\beta}},\widetilde{m},\widetilde{\ell}_{+},\widetilde{\ell}_{-},\widetilde{\tau},\widetilde{\sigma}, and ρ\rho and proceed by induction on the length of the word ww. The base case is trivial.

For the inductive step, suppose we have a word vv such that v(ab)v(a\cup b) is a tangle obtained by a sequence CnC1C_{n}\circ\dots\circ C_{1} of type C moves applied to aba\cup b. By Proposition 6.10, we consider w=gvw=g\circ v for g{tβ~,m~,~+,~,τ~,σ~,ρ}g\in\{t_{\widetilde{\beta}},\widetilde{m},\widetilde{\ell}_{+},\widetilde{\ell}_{-},\widetilde{\tau},\widetilde{\sigma},\rho\}. Then w(ab)w(a\cup b) is obtained from g(ab)g(a\cup b) by the sequence of type C moves g(Cn)g(C1)g(C_{n})\circ\dots\circ g(C_{1}). Noting that g(Ci)g(C_{i}) is a type C move, since gg is a diffeomorphism, it remains to check that g(ab)g(a\cup b) is obtained from aba\cup b by type C moves. In the case where g{tβ~,m~,τ~,ρ}g\in\{t_{\widetilde{\beta}},\widetilde{m},\widetilde{\tau},\rho\}, observe that g(ab)=abg(a\cup b)=a\cup b, so that g(ab)g(a\cup b) is obtained by zero type C moves. In the case where g{,σ}g\in\{\ell_{-},\sigma\}, we have that σ(ab)\sigma(a\cup b) is the tangle shown in the bottom center of Figure 11 (with zero twists), and hence is obtained from aba\cup b by a single type C move. In the case where g=+g=\ell_{+}, we have that σ(ab)\sigma(a\cup b) is the tangle shown in the bottom center of Figure 11 (with n=1n=-1 half twists), and hence is also obtained from aba\cup b by a single type C move. Therefore w(ab)w(a\cup b) is obtained from aba\cup b by a sequence of type C moves. ∎

Proof of Theorem 1.8.

For the forward direction, we proceed by induction on the number of type C moves needed to unknot KK. For the unknot, the result is clear.

For the inductive step, suppose that we have a strongly invertible knot KK^{\prime} with a (1,2)(1,2) decomposition with the axis of symmetry as the core of one of the handlebodies HH. Without loss of generality, we may assume that any type C move on KK^{\prime} is supported in HH. By an appropriate diffeomorphism we may further assume that the pair of arcs of KK^{\prime} contained in HH are trivial in the sense of Definition 6.4. Then by Lemma 6.5, the result of a type C move on HH is as shown in the bottom center or bottom right of Figure 11. Since these tangles are all boundary parallel, any knot K′′K^{\prime\prime} obtained by a type C move on KK^{\prime} still has a decomposition into a pair of boundary parallel arcs in HH, and a pair of boundary parallel arcs in the complement of HH. In other words, K′′K^{\prime\prime} is also a strongly invertible (1,2)(1,2) knot in which the core of one handlebody is the axis of symmetry.

The reverse direction is an immediate corollary of Lemma 6.11. ∎

7. The total equivariant unknotting number

The main purpose of this section is to prove Theorem 1.2, which we restate now. See 1.2

Proof.

We will show that for K1=K2=T3K_{1}=K_{2}=T_{3}, the 33-twist knot, the equivariant connect sum K1#K2K_{1}\#K_{2} shown on the left in Figure 14 with n=3n=3 has equivariant unknotting number u~(K1#K2)3\widetilde{u}(K_{1}\#K_{2})\geq 3. Since T3T_{3} with the indicated strong inversion (as seen in Figure 6) can be unknotted with a single type C move, this will prove the theorem.

To begin, note that q2(K1#K2)q_{2}(K_{1}\#K_{2}), as shown on the right in Figure 14, is T(2,7)#T(2,7)T(2,7)\#T(2,7), which has signature 6+6=126+6=12, so that the unknotting number of q2(K1#K2)q_{2}(K_{1}\#K_{2}) is at least 6. Now note that a type A move on K1#K2K_{1}\#K_{2} produces a crossing change on q2(K1#K2)q_{2}(K_{1}\#K_{2}), and a type B move on K1#K2K_{1}\#K_{2} produces a 4-move on q2(K1#K2)q_{2}(K_{1}\#K_{2}) (see Theorem 1.10). Hence if K1#K2K_{1}\#K_{2} can be unknotted with two equivariant crossing changes in the form of a type A move or two type B moves, then q2(K1#K2)q_{2}(K_{1}\#K_{2}) can be unknotted with at most 4 crossing changes. Since σ(q2(K1#K2))=12\sigma(q_{2}(K_{1}\#K_{2}))=12, the unknotting number of q2(K1#K2)q_{2}(K_{1}\#K_{2}) is at least 6, and hence u~A(K1#K2)6\widetilde{u}_{A}(K_{1}\#K_{2})\geq 6 by Theorem 1.9 and u~B(K1#K2)2\widetilde{u}_{B}(K_{1}\#K_{2})\geq 2 by Theorem 1.10. We conclude that K1#K2K_{1}\#K_{2} cannot be unknotted with a type A or two type B moves. Hence an unknotting sequence in fewer than three equivariant crossing changes can only consist of two type C moves, or a type B and a type C move.

We will now show that any knot JJ obtained from K1#K2K_{1}\#K_{2} by a type C move cannot be unknotted with a single type B or C move, from which we will conclude that u~(K1#K2)3\widetilde{u}(K_{1}\#K_{2})\geq 3. There are two infinite families of knots which can be obtained from K1#K2K_{1}\#K_{2} by a type C move: the knots Jm+J_{m}^{+} as shown in Figure 15, and the knots JmJ_{m}^{-} obtained from a type C move along the unbounded half-axis. Note that the quotients q2(Jm)q_{2}(J_{m}^{-}) are all isotopic to the quotient q2(K1#K2)=T(2,7)#T(2,7)q_{2}(K_{1}\#K_{2})=T(2,7)\#T(2,7). As above, this implies that JmJ_{m}^{-} cannot be unknotted with a single type B move. Furthermore, since T(2,7)#T(2,7)T(2,7)\#T(2,7) is not the quotient of a twist knot, we have that JmJ_{m}^{-} cannot be unknotted with a single type C move.

\begin{overpic}[width=300.0pt,grid=false]{twistknotsumandquotients.pdf} \put(14.0,14.0){$n$} \put(14.0,48.0){$n$} \par\put(55.0,13.5){$n$} \put(55.0,47.5){$n$} \par\put(85.5,13.5){$n$} \put(85.5,47.7){$n$} \end{overpic}
Figure 14. When n=3n=3, the knot K1#K2K_{1}\#K_{2} (left), and the two quotient knots q1(K1#K2)q_{1}(K_{1}\#K_{2}) (center) and q2(K1#K2)q_{2}(K_{1}\#K_{2}) (right).
\begin{overpic}[width=300.0pt,grid=false]{twistknotsumtypeC1.pdf} \put(14.0,7.0){$n$} \put(13.5,25.5){$m$} \put(14.0,48.5){$n$} \par\par\put(51.5,7.5){$n$} \put(51.5,26.0){$m$} \put(52.0,49.0){$n$} \par\put(85.0,8.0){$n$} \put(84.5,26.3){$m$} \put(85.0,49.3){$n$} \end{overpic}
Figure 15. The knot Jm+J_{m}^{+} obtained from K1#K2K_{1}\#K_{2} by performing a type C move with mm twists as indicated (left), and the two quotients q1(Jm+)q_{1}(J_{m}^{+}) (center) and q2(Jm+)q_{2}(J_{m}^{+}) (right).

It remains to check that Jm+J_{m}^{+} cannot be unknotted with a single type B, or C move. We first observe that q2(Jm+)q_{2}(J_{m}^{+}), shown on the right in Figure 15 is the 2-bridge knot corresponding to the continued fraction

[6,1,2m+1,1,6]=7(14m+19)2(7m+10).[6,-1,2m+1,-1,6]=\dfrac{7(14m+19)}{2(7m+10)}.

Since this fraction is not equivalent to 2k+11\dfrac{2k+1}{1} for any kk, we conclude that q2(Jm+)q_{2}(J_{m}^{+}) is never a torus knot, and hence that Jm+J_{m}^{+} is never a twist knot. Since only twist knots can be unknotted with a single type C move, u~C(Jm+)>1\widetilde{u}_{C}(J_{m}^{+})>1. We next compute the signature σ(q2(Jm+))\sigma(q_{2}(J_{m}^{+})). The Goeritz matrix is

G=[71012m+31017],G=\begin{bmatrix}7&-1&0\\ -1&2m+3&-1\\ 0&-1&7\end{bmatrix},

with correction term 2m+32m+3, so that σ(q2(Jm+))=σ(G)(2m+3)\sigma(q_{2}(J_{m}^{+}))=\sigma(G)-(2m+3). Since GG is a 3×33\times 3 matrix, we have that 2m6σ(q2(Jm+))2m-2m-6\leq\sigma(q_{2}(J_{m}^{+}))\leq-2m. Whenever |σ(q2(Jm+))|6|\sigma(q_{2}(J_{m}^{+}))|\geq 6, we have that u(q2(Jm+))>2u(q_{2}(J_{m}^{+}))>2 so that q2(Jm+)q_{2}(J_{m}^{+}) cannot be unknotted with a single crossing change, or with a single 4-move and hence Jm+J_{m}^{+} cannot be unknotted with a single type A or type B move. On the other hand, when |σ(q2(Jm+))|<6|\sigma(q_{2}(J_{m}^{+}))|<6 we have that 6<m<3-6<m<3. For these eight knots we have the fractions

35750,,32948.\dfrac{-357}{-50},\dots,\dfrac{329}{48}.

Applying Theorem 5.4 to these knots shows that none of them can be unknotted with a single 4-move. We conclude that for all mm, Jm+J_{m}^{+} cannot be unknotted with a single type B, or C move. Hence u~(K1#K2)3\widetilde{u}(K_{1}\#K_{2})\geq 3. ∎

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