Introduction
The relationship between Floer-theoretic knot invariants of Ozsváth and Szabó [12 ] and of Rasmussen [16 ] and quantum knot invariants of Khovanov [8 ] and of Khovanov and Rozansky [9 , 10 ] has been an active topic in topology for the past twenty-five years. These invariants categorify many knot invariants. That is, the graded Euler characteristic of the knot Floer homology of a knot returns its Alexander polynomial, and the graded Euler characteristic of the Khovanov homology of a knot returns its Jones polynomial. The first relationship between them came from a spectral sequence from the Khovanov homology of a link to the Heegaard Floer homology of its double branched cover, constructed by Ozsváth and Szabó in [14 ] . Since then, a slew of spectral sequences of that form have been discovered, yielding a variety of rank inequalities between the associated homologies as well as indicating the possibility of more interesting relationships.
Consequently, the following was a long-standing conjecture of Rasmussen [17 ] .
Theorem 1.1 (Rasmussen’s Conjecture). [2 ] For a knot K ⊂ S 3 K \subset S^3 K ⊂ S 3 , rk ( K h ~ ( K ; Q ) ) ≥ rk ( H F K ^ ( K ; Q ) ) \operatorname{rk}(\widetilde{Kh}(K;\mathbb{Q})) \ge\operatorname{rk}(\widehat{HFK}(K;\mathbb{Q})) rk ( K h ( K ; Q )) ≥ rk ( H F K ( K ; Q )) , where K h ~ \widetilde{Kh} K h denotes reduced Khovanov homology.
In [17 ] , Rasmussen suggests that constructing a spectral sequence is a promising way to address this conjecture, a strategy successfully employed by Dowlin in [1 , 2 ] . It is natural to want to complete the diagram in Figure 1 with spectral sequences from the Khovanov-Rozansky homologies, K R n ( K ) KR_n(K) K R n ( K ) , to a proposed Floer-theoretic analog. In [1 ] , Dowlin defines a candidate family of link invariants, called H F K n ( K ) HFK_n(K) H F K n ( K ) , and presents the generalized conjecture.
Figure 1. Dotted arrows are conjectured, while solid arrows have been proven in suitable versions: the curved arrows on the left are Rasmussen’s spectral sequences [18 ] , those on the right are due to Dowlin [1 Lemma 2.23] , and the bottom arrow is Dowlin’s spectral sequence from reduced Khovanov homology to H F K ^ \widehat{HFK} H F K [2 ] .
Conjecture 1.2. [[1 Conjecture 1.6] ] For a link L ⊂ S 3 L \subset S^3 L ⊂ S 3 , there are spectral sequences K R n ( L ) ⇒ H F K n ( L ) KR_n(L) \Rightarrow HFK_n(L) K R n ( L ) ⇒ H F K n ( L ) and K R ‾ n ( L ) ⇒ H F K ^ n ( L ) \overline{KR}_n(L) \Rightarrow\widehat{HFK}_n(L) K R n ( L ) ⇒ H F K n ( L ) , respecting the gradings specified in [[1 Conjecture 1.6] ].
Motivated by Conjecture 1.2, we study H F K n ( L ) HFK_n(L) H F K n ( L ) , in the case that L L L is a knot, and make the following conjecture.
Conjecture 1.3. For any knot K K K in S 3 S^3 S 3 , there is an integer N ( K ) N(K) N ( K ) such that for all n ≥ N ( K ) n \ge N(K) n ≥ N ( K ) , H F K n ( K ) HFK_n(K) H F K n ( K ) can be obtained by a change of coefficients from H F K − ( K ) HFK^{-}(K) H F K − ( K ) ; that is,
H F K n ( K ) ≅ ( H F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; Q [ U ] ( U n ) ) . HFK_n(K) \cong\left(HFK^{-}(K) \otimes_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right) \oplus\operatorname{Tor}^{\mathbb{Q}[U]}_1\left(HFK^{-}(K); \frac{\mathbb{Q}[U]}{(U^n)}\right). H F K n ( K ) ≅ ( H F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; ( U n ) Q [ U ] ) .
Although further investigation is required to prove Conjecture 1.3, much can be said about two wide classes of knots. Section 3 presents supporting examples, including the trefoil (an L L L -space knot) and the figure-eight knot (a thin knot), as well as T 3 , 4 T_{3,4} T 3 , 4 . We recall that a rational homology 3-sphere Y Y Y is an L L L -space if rk H F ^ ( Y ; Q ) = ∣ H 1 ( Y ; Z ) ∣ \operatorname{rk}\widehat{HF}(Y;\mathbb{Q})=|H_1(Y;\mathbb{Z})| rk H F ( Y ; Q ) = ∣ H 1 ( Y ; Z ) ∣ .1 A knot is an L L L -space knot if it admits a positive surgery yielding an L L L -space. By [[13 ] ], the Alexander polynomial of an L L L -space knot has the form Δ K ( t ) = ∑ j = 0 m − 1 ( − 1 ) j t e j \Delta_K(t)=\sum_{j=0}^{m-1}(-1)^j t^{e_j} Δ K ( t ) = ∑ j = 0 m − 1 ( − 1 ) j t e j with e 0 > e 1 > ⋯ > e m − 1 e_0>e_1>\cdots>e_{m-1} e 0 > e 1 > ⋯ > e m − 1 ; we call the differences e j − 1 − e j e_{j-1}-e_j e j − 1 − e j the gaps of Δ K \Delta_K Δ K . A knot K K K is Floer homologically thin if its knot Floer homology H F K ^ ( K ; Q ) \widehat{HFK}(K;\mathbb{Q}) H F K ( K ; Q ) is supported in a single δ \delta δ -grading. Indeed, our main theorem offers some initial evidence in the direction of Conjecture 1.3:
Theorem 1.4. Let n ≥ 2 n \ge2 n ≥ 2 , and let K ⊂ S 3 K \subset S^3 K ⊂ S 3 be either a thin knot, or an L L L -space knot such that every gap of Δ K \Delta_K Δ K is at most n − 1 n-1 n − 1 . Then, as ungraded Q [ U ] \mathbb{Q}[U] Q [ U ] -modules,
H F K n ( K ) ≅ ( H F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; Q [ U ] ( U n ) ) . HFK_n(K) \cong\left(HFK^{-}(K) \otimes_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right) \oplus\operatorname{Tor}^{\mathbb{Q}[U]}_1\left(HFK^{-}(K); \frac{\mathbb{Q}[U]}{(U^n)}\right). H F K n ( K ) ≅ ( H F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; ( U n ) Q [ U ] ) .
That is to say, for such knots, H F K n ( K ) HFK_n(K) H F K n ( K ) is a change of coefficients from H F K − ( K ) HFK^{-}(K) H F K − ( K ) .
Corollary 1.5. For any L L L -space knot K K K , H F K n ( K ) HFK_n(K) H F K n ( K ) is determined by its Alexander polynomial. For any thin knot K K K , H F K n ( K ) HFK_n(K) H F K n ( K ) is determined by its Alexander polynomial and τ ( K ) \tau(K) τ ( K ) ; moreover, for n ≥ 2 n \ge2 n ≥ 2 ,
H F K n ( K ) ≅ Q [ U ] ( U n ) ⊕ Q det ( K ) − 1 HFK_n(K) \cong\frac{\mathbb{Q}[U]}{(U^n)} \oplus\mathbb{Q}^{\det(K)-1} H F K n ( K ) ≅ ( U n ) Q [ U ] ⊕ Q d e t ( K ) − 1 as ungraded Q [ U ] \mathbb{Q}[U] Q [ U ] -modules.
While the first part of Corollary 1.5 is implicitly known from the definition of H F K n ( L ) HFK_n(L) H F K n ( L ) for knots and does not depend on Theorem 1.4, this follows more explicitly from [[13 ] ], where we see that the knot Floer complex (and hence H F K − ( K ) HFK^{-}(K) H F K − ( K ) ) of any L L L -space knot is determined by its Alexander polynomial, and from [[15 ] ], where we see that the knot Floer complex of any thin knot is determined from its Alexander polynomial and τ \tau τ (see Theorems 4.9 and 4.11). For quasi-alternating knots τ = − σ / 2 \tau=-\sigma/2 τ = − σ /2 [[11 ] ], so for these knots the signature may be used in place of τ \tau τ . The second part follows from Theorem 1.4 (see Remark 4.19). The work in [[15 ] ] will play a more critical role in the proof for thin knots in Section 4.
The restriction to large n n n in Theorem 1.4 is necessary. For n = 1 n=1 n = 1 , H F K 1 ( K ) ≅ H F ^ ( S 3 ) ≅ Q HFK_1(K)\cong\widehat{HF}(S^3)\cong\mathbb{Q} H F K 1 ( K ) ≅ H F ( S 3 ) ≅ Q for every knot (Remark 2.13), while the right-hand side is H F K ^ ( K ) \widehat{HFK}(K) H F K ( K ) . For L L L -space knots, Proposition 4.15 computes H F K n ( K ) HFK_n(K) H F K n ( K ) for every n ≥ 2 n\ge2 n ≥ 2 , and shows that the isomorphism of Theorem 1.4 holds if and only if an explicit count read off from the gaps of Δ K \Delta_K Δ K , vanishes. For torus knots this gives a clean answer.
Corollary 1.6. Let 2 ≤ p < q 2\le p<q 2 ≤ p < q be coprime and n ≥ 2 n\ge2 n ≥ 2 . The isomorphism of Theorem 1.4 holds for T p , q T_{p,q} T p , q if and only if n ≥ p n\ge p n ≥ p . In particular, it fails for T 3 , 4 T_{3,4} T 3 , 4 with n = 2 n=2 n = 2 , where dim Q H F K 2 ( T 3 , 4 ) = 6 \dim_{\mathbb{Q}}HFK_2(T_{3,4})=6 dim Q H F K 2 ( T 3 , 4 ) = 6 while the right-hand side has dimension 8 8 8 .
Organization
In Section 2, we introduce and review a construction of the invariants H F K n ( K ) HFK_n(K) H F K n ( K ) as in [[1 ] ]. Section 3 compares several computations of these invariants against older knot Floer homology flavors for representatives from various classes of knots. In Section 4, we prove the main theorem.
All results of this note are due to the author. Claude Opus 5.5 was used in proofreading, checking proof details, and generating and checking examples.
Acknowledgments
This note is modified from the author’s Ph.D. dissertation at Michigan State University. I am eternally grateful to my Ph.D. advisor Matthew Hedden for helpful conversation and comments on early drafts. I thank Charles Stine and Shea Vela-Vick for helpful conversations. I also thank Chris St. Clair, Dean Spyropoulos, and Chen Zhang for comments on early drafts.
I also want to thank the National Science Foundation for support with grants DMS-2104664, the RTG NSF Award DMS-2135960, DMS-1709016, and the RTG NSF Award DMS-2231492. Their financial support made this research possible.
Background
Heegaard Diagrams
A common way to depict 3-manifolds in low-dimensional topology is using a Heegaard diagram, which presents a convenient Morse decomposition of the 3-manifold. These can be enhanced to encode embedded links in the 3-manifold as well.
Definition 2.1. (cf. [1 Definition 2.1] ) A (multi-pointed) Heegaard diagram H \mathcal{H} H for an oriented link L L L in a closed, oriented 3-manifold Y Y Y is the data ( Σ , α , β , w , z ) (\Sigma,\boldsymbol{\alpha},\boldsymbol{\beta},\mathbf{w},\mathbf{z}) ( Σ , α , β , w , z ) where
Σ \Sigma Σ is a closed, oriented, genus g g g surface, called the Heegaard surface.
α \boldsymbol{\alpha} α (respectively, β \boldsymbol{\beta} β ) is a set of g + k − 1 g+k-1 g + k − 1 disjoint embedded circles { α 1 , … , α g + k − 1 } \{\alpha_1,\ldots,\alpha_{g+k-1}\} { α 1 , … , α g + k − 1 } (resp. { β 1 , … , β g + k − 1 } \{\beta_1,\ldots,\beta_{g+k-1}\} { β 1 , … , β g + k − 1 } ) in Σ \Sigma Σ such that the alpha curves intersect the beta curves transversely.
α \boldsymbol{\alpha} α and β \boldsymbol{\beta} β each span a g g g -dimensional subspace of H 1 ( Σ ; Z ) H_1(\Sigma;\mathbb{Z}) H 1 ( Σ ; Z ) .
w \mathbf{w} w and z \mathbf{z} z are each sets of k k k basepoints { w 1 , … , w k } \{w_1,\ldots,w_k\} { w 1 , … , w k } and { z 1 , … , z k } \{z_1,\ldots,z_k\} { z 1 , … , z k } , where k k k is at least the number of components of L L L , such that each component of Σ ∖ α \Sigma\setminus\boldsymbol{\alpha} Σ ∖ α and each component of Σ ∖ β \Sigma\setminus\boldsymbol{\beta} Σ ∖ β contains exactly one w w w basepoint and exactly one z z z basepoint.
The manifold Y Y Y is constructed from this data by thickening Σ \Sigma Σ to Σ × [ 0 , 1 ] \Sigma\times[0,1] Σ × [ 0 , 1 ] and attaching thickened discs along the alpha curves at Σ × { 0 } \Sigma\times\{0\} Σ × { 0 } and along the beta curves at Σ × { 1 } \Sigma\times\{1\} Σ × { 1 } and then filling in the resulting 2-sphere boundaries with 3-balls.
The link L L L in Y Y Y can be seen as follows. When thickening Σ \Sigma Σ , also thicken the w \mathbf{w} w and z \mathbf{z} z basepoints to get w ⊔ z × [ 0 , 1 ] ⊂ Σ × [ 0 , 1 ] \mathbf{w}\sqcup\mathbf{z}\times[0,1]\subset\Sigma\times[0,1] w ⊔ z × [ 0 , 1 ] ⊂ Σ × [ 0 , 1 ] . Since each component of Σ ∖ α \Sigma\setminus\boldsymbol{\alpha} Σ ∖ α has a w w w and z z z basepoint, we connect those arcs on the Σ × { 0 } \Sigma\times\{0\} Σ × { 0 } surface with an arc in the 3-ball attached to that component’s S 2 S^2 S 2 boundary. We do this similarly for the Σ × { 1 } \Sigma\times\{1\} Σ × { 1 } boundaries.
Definition 2.2. In [1 Definition 2.2] , Dowlin defined a notion of a punctured Heegaard diagram , which adds to ( Σ , α , β , w , z ) (\Sigma,\boldsymbol{\alpha},\boldsymbol{\beta},\mathbf{w},\mathbf{z}) ( Σ , α , β , w , z ) the following data:
A basepoint p p p , called the puncture .
A curve α g + k \alpha_{g+k} α g + k and β g + k \beta_{g+k} β g + k which separate p p p from the w \mathbf{w} w and z \mathbf{z} z basepoints, such that α \boldsymbol{\alpha} α and β \boldsymbol{\beta} β still intersect transversely and span a g g g -dimensional subspace of H 1 ( Σ ; Z ) H_1(\Sigma;\mathbb{Z}) H 1 ( Σ ; Z ) .
Remark 2.3. In the above construction of the pair ( Y , L ) (Y,L) ( Y , L ) , puncturing the Heegaard diagram is like considering L ⊔ U L\sqcup\mathcal{U} L ⊔ U (where U \mathcal{U} U is the unknot), where the unlinked unknot carries a pair of basepoints w 0 w_0 w 0 and z 0 z_0 z 0 which coincide at p p p ; see [1 Remark 2.3] .
Knot Floer Homology
Here, we provide the groundwork for Dowlin’s new family of invariants in [1 ] . For another overview of knot Floer homology, we direct the reader to [6 ] . For greater detail, see [12 ] .
All of our definitions will be made over Q \mathbb{Q} Q since, as in [1 , 2 ] , the tools needed depend on working with a field of characteristic zero (we need n n n , and also 2, for the spectral sequence of [2 ] , to be invertible), at the cost of keeping track of signs. However, most definitions here can be adapted to one’s preferred field for other applications. Knot Floer complexes come in a variety of flavors, but we are only interested in two: the minus flavor C F K − ( L ) CFK^{-}(L) C F K − ( L ) and the so-called master complex C F K U , V ( L ) CFK_{U,V}(L) C F K U , V ( L ) .
Given a multi-pointed unpunctured Heegaard diagram H \mathcal{H} H for a null-homologous link L ⊂ Y L\subset Y L ⊂ Y , the so-called master complex C F K U , V ( H ) CFK_{U,V}(\mathcal{H}) C F K U , V ( H ) is the free Q [ U 1 , … , U k , V 1 , … , V k ] \mathbb{Q}[U_1,\ldots,U_k,V_1,\ldots,V_k] Q [ U 1 , … , U k , V 1 , … , V k ] -module generated by T α ∩ T β \mathbb{T}_{\alpha}\cap\mathbb{T}_{\beta} T α ∩ T β , the intersection points of the totally real Lagrangian tori T α \mathbb{T}_{\alpha} T α and T β \mathbb{T}_{\beta} T β in the symplectic manifold Sym g + k − 1 ( Σ ) \operatorname{Sym}^{g+k-1}(\Sigma) Sym g + k − 1 ( Σ ) (or Sym g + k ( Σ ) \operatorname{Sym}^{g+k}(\Sigma) Sym g + k ( Σ ) for punctured diagrams), given by the symmetric product of the α \alpha α (and β \beta β , for T β \mathbb{T}_{\beta} T β ) curves on H \mathcal{H} H . The differential in this complex counts the rigid, unparametrized Maslov index 1 pseudo-holomorphic disks from a generator x x x to y y y , keeping track of which basepoints the disks cross and their multiplicities:
∂ U , V ( x ) = ∑ y ∈ T α ∩ T β ∑ ϕ ∈ π 2 ( x , y ) μ ( ϕ ) = 1 # M ^ ( ϕ ) U 1 n w 1 ( ϕ ) ⋯ U k n w k ( ϕ ) V 1 n z 1 ( ϕ ) ⋯ V k n z k ( ϕ ) y . \partial_{U,V}(x)=\sum_{y\in\mathbb{T}_{\alpha}\cap\mathbb{T}_{\beta}}\sum_{\substack{\phi\in\pi_2(x,y)\\ \mu(\phi)=1}}\#\widehat{\mathcal{M}}(\phi)U_1^{n_{w_1}(\phi)}\cdots U_k^{n_{w_k}(\phi)}V_1^{n_{z_1}(\phi)}\cdots V_k^{n_{z_k}(\phi)}y. ∂ U , V ( x ) = y ∈ T α ∩ T β ∑ ϕ ∈ π 2 ( x , y ) μ ( ϕ ) = 1 ∑ # M ( ϕ ) U 1 n w 1 ( ϕ ) ⋯ U k n w k ( ϕ ) V 1 n z 1 ( ϕ ) ⋯ V k n z k ( ϕ ) y .
Remark 2.4. [1 Lemma 2.4] In general, C F K U , V ( H ) CFK_{U,V}(\mathcal{H}) C F K U , V ( H ) is not a true chain complex, but a curved one. Let w a ( i ) w_{a(i)} w a ( i ) be the w basepoint connected to z i z_i z i via an arc in the alpha handlebody, and w b ( i ) w_{b(i)} w b ( i ) be the one connected to z i z_i z i via an arc in the beta handlebody. Then the curved complex has potential
∂ U , V 2 = ∑ i = 1 k ( U a ( i ) − U b ( i ) ) V i \partial_{U,V}^{2}=\sum_{i=1}^{k}(U_{a(i)}-U_{b(i)})V_i ∂ U , V 2 = i = 1 ∑ k ( U a ( i ) − U b ( i ) ) V i
When each component of L L L has exactly one w and z basepoint, C F K U , V ( H ) CFK_{U,V}(\mathcal{H}) C F K U , V ( H ) is a true complex.
The complex C F K − ( H ) CFK^{-}(\mathcal{H}) C F K − ( H ) is similarly defined as the free Q [ U 1 , … , U k ] \mathbb{Q}[U_1,\ldots,U_k] Q [ U 1 , … , U k ] -module generated by T α ∩ T β \mathbb{T}_{\alpha}\cap\mathbb{T}_{\beta} T α ∩ T β . In the minus flavor, the differential counts disks which only pass through w basepoints:
∂ − ( x ) = ∑ y ∈ T α ∩ T β ∑ ϕ ∈ π 2 ( x , y ) μ ( ϕ ) = 1 n z ( ϕ ) = 0 # M ^ ( ϕ ) U 1 n w 1 ( ϕ ) ⋯ U k n w k ( ϕ ) y \partial^{-}(x)=\sum_{y\in\mathbb{T}_{\alpha}\cap\mathbb{T}_{\beta}}\ \sum_{\substack{\phi\in\pi_2(x,y)\\ \mu(\phi)=1\\ n_z(\phi)=0}}\#\widehat{\mathcal{M}}(\phi)U_1^{n_{w_1}(\phi)}\cdots U_k^{n_{w_k}(\phi)}y ∂ − ( x ) = y ∈ T α ∩ T β ∑ ϕ ∈ π 2 ( x , y ) μ ( ϕ ) = 1 n z ( ϕ ) = 0 ∑ # M ( ϕ ) U 1 n w 1 ( ϕ ) ⋯ U k n w k ( ϕ ) y
The definition of C F K U , V ( L ) CFK_{U,V}(L) C F K U , V ( L ) is the same for punctured Heegaard diagrams, where the differential doesn’t count discs that go through p p p :
∂ U , V ( x ) = ∑ y ∈ T α ∩ T β ∑ ϕ ∈ π 2 ( x , y ) μ ( ϕ ) = 1 n p ( ϕ ) = 0 # M ^ ( ϕ ) U 1 n w 1 ( ϕ ) ⋯ U k n w k ( ϕ ) V 1 n z 1 ( ϕ ) ⋯ V k n z k ( ϕ ) y . \partial_{U,V}(x)=\sum_{y\in\mathbb{T}_{\alpha}\cap\mathbb{T}_{\beta}}\ \sum_{\substack{\phi\in\pi_2(x,y)\\ \mu(\phi)=1\\ n_p(\phi)=0}}\#\widehat{\mathcal{M}}(\phi)U_1^{n_{w_1}(\phi)}\cdots U_k^{n_{w_k}(\phi)}V_1^{n_{z_1}(\phi)}\cdots V_k^{n_{z_k}(\phi)}y. ∂ U , V ( x ) = y ∈ T α ∩ T β ∑ ϕ ∈ π 2 ( x , y ) μ ( ϕ ) = 1 n p ( ϕ ) = 0 ∑ # M ( ϕ ) U 1 n w 1 ( ϕ ) ⋯ U k n w k ( ϕ ) V 1 n z 1 ( ϕ ) ⋯ V k n z k ( ϕ ) y .
The chain homotopy type of each complex is an invariant of the link L L L (for the curved complex C F K U , V CFK_{U,V} C F K U , V , see [Zem19]), so we often ignore the Heegaard diagram dependence and write C F K U , V ( L ) CFK_{U,V}(L) C F K U , V ( L ) and C F K − ( L ) CFK^{-}(L) C F K − ( L ) . The complex C F K − ( L ) CFK^{-}(L) C F K − ( L ) is a true chain complex, and the homology H F K − ( L ) = H ∗ ( C F K − ( L ) ) HFK^{-}(L)=H_{*}(CFK^{-}(L)) H F K − ( L ) = H ∗ ( C F K − ( L )) is the familiar minus flavor of knot Floer homology. We make the following remarks.
Remark 2.5. The thin knots considered in this note enjoy another noteworthy trait: C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) has a model in which every arrow has length one, that is, every arrow is labeled U U U or V V V . This is discussed at length in [15 ] and presented quickly in § 4 (Theorem 4.9 ). This fails for L L L -space knots in general: C F K U , V ( T 3 , 4 ) CFK_{U,V}(T_{3,4}) C F K U , V ( T 3 , 4 ) has arrows of length two (Example 3.5).
Remark 2.6. Since, in our setting, the manifold Y Y Y will be S 3 S^3 S 3 , we needn’t worry about the splitting of these theories over Spin c \operatorname{Spin}^{c} Spin c structures. There is also a great deal of grading information in these invariants, but it isn’t needed for the main theorem, so we suppress it.
The Family H F K n HFK_n H F K n
In [1 ] , Dowlin constructs a family of link invariants designed to mimic features of the s l n \mathfrak{sl}_n sl n -homology theories of Khovanov and Rozansky [9 ] .
Definition 2.7. [1 Definition 2.5] Given a multi-pointed punctured Heegaard diagram H \mathcal{H} H for a link L L L in a 3-manifold Y Y Y , define the chain complex C F K n ( H ) CFK_n(\mathcal{H}) C F K n ( H ) to be the quotient
C F K n ( H ) = C F K U , V ( H ) / ( V i − U a ( i ) n − U b ( i ) n U a ( i ) − U b ( i ) ) CFK_n(\mathcal{H})=CFK_{U,V}(\mathcal{H})\mathbin{/}\left(V_i-\frac{U_{a(i)}^n-U_{b(i)}^n}{U_{a(i)}-U_{b(i)}}\right) C F K n ( H ) = C F K U , V ( H ) / ( V i − U a ( i ) − U b ( i ) U a ( i ) n − U b ( i ) n ) where a ( i ) a(i) a ( i ) and b ( i ) b(i) b ( i ) are as in 2.4, the difference quotient denotes the polynomial ∑ j = 0 n − 1 U a ( i ) j U b ( i ) n − 1 − j \sum_{j=0}^{n-1}U_{a(i)}^jU_{b(i)}^{n-1-j} ∑ j = 0 n − 1 U a ( i ) j U b ( i ) n − 1 − j , and the differential ∂ n \partial_n ∂ n is the induced differential from ∂ U , V \partial_{U,V} ∂ U , V .
Remark 2.8. In the case where L L L is a knot, we may only have one variable, that is, a ( 1 ) = b ( 1 ) a(1)=b(1) a ( 1 ) = b ( 1 ) . The difference quotient is then ∑ j = 0 n − 1 U j U n − 1 − j = n U n − 1 \sum_{j=0}^{n-1}U^jU^{n-1-j}=nU^{n-1} ∑ j = 0 n − 1 U j U n − 1 − j = n U n − 1 , which is the derivative
V = d d U ( U n ) = n U n − 1 . V=\frac{d}{dU}(U^n)=nU^{n-1}. V = d U d ( U n ) = n U n − 1 .
Theorem 2.9. [1 Lemma 2.6] The map ∂ n : C F K n ( H ) → C F K n ( H ) \partial_n:CFK_n(\mathcal{H})\to CFK_n(\mathcal{H}) ∂ n : C F K n ( H ) → C F K n ( H ) satisfies ∂ n 2 = 0 \partial_n^2=0 ∂ n 2 = 0 .
Let H F K n ( H ) = H ∗ ( C F K n ( H ) , ∂ n ) HFK_n(\mathcal{H})=H_*(CFK_n(\mathcal{H}),\partial_n) H F K n ( H ) = H ∗ ( C F K n ( H ) , ∂ n ) . With the following theorem, we can define the link invariants.
Theorem 2.10. [1 Theorem 2.7] If H 1 \mathcal{H}_1 H 1 and H 2 \mathcal{H}_2 H 2 are two punctured Heegaard diagrams for a null-homologous link L L L with ℓ \ell ℓ components, then C F K n ( H 1 ) CFK_n(\mathcal{H}_1) C F K n ( H 1 ) and C F K n ( H 2 ) CFK_n(\mathcal{H}_2) C F K n ( H 2 ) are chain homotopy equivalent as complexes of graded Q [ U 1 , … , U ℓ ] \mathbb{Q}[U_1,\ldots,U_\ell] Q [ U 1 , … , U ℓ ] -modules.
Definition 2.11. [[1 ] , Definition 2.8] Define H F K n ( L ) = H ∗ ( C F K n ( H ) ) HF K_n(L)=H_\ast(CFK_n(\mathcal{H})) H F K n ( L ) = H ∗ ( C F K n ( H )) where H \mathcal{H} H is any punctured Heegaard diagram for L L L .
We perform some computations in § 3 . These examples illustrate that, for knots, one has a simpler equivalent definition of H F K n ( K ) HF K_n(K) H F K n ( K ) . In fact, in the case where L = K L=K L = K is a knot, H F K n ( K ) HF K_n(K) H F K n ( K ) can be computed from C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) without a punctured Heegaard diagram.
Theorem 2.12. [[1 ] , Lemma 2.16] If H \mathcal{H} H is an unpunctured diagram for a knot K K K in S 3 S^3 S 3 with a single pair of basepoints w w w and z z z , then
H F K n ( K ) = H ∗ ( C F K U , V ( H ) ( U V , V − n U n − 1 ) ) . HF K_n(K)=H_\ast\left(\frac{CFK_{U,V}(\mathcal{H})}{(UV,V-nU^{n-1})}\right). H F K n ( K ) = H ∗ ( ( U V , V − n U n − 1 ) C F K U , V ( H ) ) .
Computational Evidence
The master complex C F K U , V ( L ) CFK_{U,V}(L) C F K U , V ( L ) is well-known for torus knots [[13 ] ]. An application of Theorem 2.12 simplifies the computations.
Example 3.2. The Trefoil.
As mentioned above, C F K U , V ( T p , q ) CFK_{U,V}(T_{p,q}) C F K U , V ( T p , q ) can be read off from its Alexander polynomial. For the trefoil, it is well-known that Δ ( T 2 , 3 ) = t − 1 − 1 + t \Delta(T_{2,3})=t^{-1}-1+t Δ ( T 2 , 3 ) = t − 1 − 1 + t . Since the spacing between the powers of t t t are only one each, we have only a single power of U U U and V V V as the maps on the complex, yielding the usual staircase picture:
The complex C F K n ( T 2 , 3 ) CFK_n(T_{2,3}) C F K n ( T 2 , 3 ) looks the same with the appropriate quotients. Both C F K − ( K ) CFK^-(K) C F K − ( K ) and C F K n ( K ) CFK_n(K) C F K n ( K ) are pictured in Figure 2 . On the level of homology, for n ≥ 2 n\geq2 n ≥ 2 , we see the following:
H F K n ( T 2 , 3 ) ≅ Q [ U ] ( U n ) ⊕ Q ⊕ Q HF K_n(T_{2,3})\cong\frac{\mathbb{Q}[U]}{(U^n)}\oplus\mathbb{Q}\oplus\mathbb{Q} H F K n ( T 2 , 3 ) ≅ ( U n ) Q [ U ] ⊕ Q ⊕ Q H F K − ( T 2 , 3 ) ≅ Q [ U ] ⊕ Q . HFK^-(T_{2,3})\cong\mathbb{Q}[U]\oplus\mathbb{Q}. H F K − ( T 2 , 3 ) ≅ Q [ U ] ⊕ Q . :::`
Figure 2. On the left: the complex C F K − ( T 2 , 3 ) CFK^-(T_{2,3}) C F K − ( T 2 , 3 ) . On the right: the complex C F K n ( T 2 , 3 ) CFK_n(T_{2,3}) C F K n ( T 2 , 3 ) .
Notice that since Tor 1 Q [ U ] ( Q ⊕ Q [ U ] , Q [ U ] ( U n ) ) ≅ Q \operatorname{Tor}_{1}^{\mathbb{Q}[U]}\left(\mathbb{Q}\oplus\mathbb{Q}[U],\frac{\mathbb{Q}[U]}{(U^{n})}\right)\cong\mathbb{Q} Tor 1 Q [ U ] ( Q ⊕ Q [ U ] , ( U n ) Q [ U ] ) ≅ Q , by the universal coefficient theorem,
H F K n ( T 2 , 3 ) ≅ H F K − ( T 2 , 3 ) ⊗ Q [ U ] Q [ U ] ( U n ) ⊕ Tor 1 Q [ U ] ( H F K − ( T 2 , 3 ) ; Q [ U ] ( U n ) ) HFK_{n}(T_{2,3})\cong HFK^{-}(T_{2,3})\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^{n})}\oplus\operatorname{Tor}_{1}^{\mathbb{Q}[U]}\left(HFK^{-}(T_{2,3});\frac{\mathbb{Q}[U]}{(U^{n})}\right) H F K n ( T 2 , 3 ) ≅ H F K − ( T 2 , 3 ) ⊗ Q [ U ] ( U n ) Q [ U ] ⊕ Tor 1 Q [ U ] ( H F K − ( T 2 , 3 ) ; ( U n ) Q [ U ] )
≅ ( Q [ U ] ⊕ Q ) ⊗ Q [ U ] Q [ U ] ( U n ) ⊕ Q \cong(\mathbb{Q}[U]\oplus\mathbb{Q})\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^{n})}\oplus\mathbb{Q} ≅ ( Q [ U ] ⊕ Q ) ⊗ Q [ U ] ( U n ) Q [ U ] ⊕ Q
≅ Q [ U ] ( U n ) ⊕ Q ⊕ Q . \cong\frac{\mathbb{Q}[U]}{(U^{n})}\oplus\mathbb{Q}\oplus\mathbb{Q}. ≅ ( U n ) Q [ U ] ⊕ Q ⊕ Q .
(For n = 1 n=1 n = 1 the answer is different: H F K 1 ( T 2 , 3 ) ≅ Q HFK_{1}(T_{2,3})\cong\mathbb{Q} H F K 1 ( T 2 , 3 ) ≅ Q by Remark 2.13 .) We see similar behavior for a knot whose master complex has boxes and is not a torus knot.
Example 3.3. The Figure-Eight.
We first look at the master complex for 4 1 4_{1} 4 1 , and then its quotients, as shown in Figure 3 . The invariants for 4 1 4_{1} 4 1 are, for n ≥ 2 n\geq2 n ≥ 2 ,
Figure 3. On the top: the complex C F K U , V ( 4 1 ) CFK_{U,V}(4_{1}) C F K U , V ( 4 1 ) , where each dot represents the module Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] . On the left: the complex C F K − ( 4 1 ) CFK^{-}(4_{1}) C F K − ( 4 1 ) , where each dot represents the module Q [ U ] \mathbb{Q}[U] Q [ U ] . On the right: the complex C F K n ( 4 1 ) CFK_{n}(4_{1}) C F K n ( 4 1 ) , where each dot represents the module Q [ U ] ( U n ) \frac{\mathbb{Q}[U]}{(U^{n})} ( U n ) Q [ U ] .
H F K n ( 4 1 ) ≅ Q ⊕ Q ⊕ Q ⊕ Q ⊕ Q [ U ] ( U n ) HFK_{n}(4_{1})\cong\mathbb{Q}\oplus\mathbb{Q}\oplus\mathbb{Q}\oplus\mathbb{Q}\oplus\frac{\mathbb{Q}[U]}{(U^{n})} H F K n ( 4 1 ) ≅ Q ⊕ Q ⊕ Q ⊕ Q ⊕ ( U n ) Q [ U ]
H F K − ( 4 1 ) ≅ Q [ U ] ⊕ Q ⊕ Q . HFK^{-}(4_{1})\cong\mathbb{Q}[U]\oplus\mathbb{Q}\oplus\mathbb{Q}. H F K − ( 4 1 ) ≅ Q [ U ] ⊕ Q ⊕ Q .
Again, the universal coefficient theorem gives us the following:
H F K n ( 4 1 ) ≅ H F K − ( 4 1 ) ⊗ Q [ U ] Q [ U ] ( U n ) ⊕ Tor 1 Q [ U ] ( H F K − ( 4 1 ) ; Q [ U ] ( U n ) ) HFK_{n}(4_{1})\cong HFK^{-}(4_{1})\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^{n})}\oplus\operatorname{Tor}_{1}^{\mathbb{Q}[U]}\left(HFK^{-}(4_{1});\frac{\mathbb{Q}[U]}{(U^{n})}\right) H F K n ( 4 1 ) ≅ H F K − ( 4 1 ) ⊗ Q [ U ] ( U n ) Q [ U ] ⊕ Tor 1 Q [ U ] ( H F K − ( 4 1 ) ; ( U n ) Q [ U ] )
≅ Q [ U ] ( U n ) ⊕ Q ⊕ Q ⊕ Q ⊕ Q ⊕ Q . \cong\frac{\mathbb{Q}[U]}{(U^{n})}\oplus\mathbb{Q}\oplus\mathbb{Q}\oplus\mathbb{Q}\oplus\mathbb{Q}\oplus\mathbb{Q}. ≅ ( U n ) Q [ U ] ⊕ Q ⊕ Q ⊕ Q ⊕ Q ⊕ Q .
Remark 3.4. While one might wish to explore examples with diagonal arrows, we note that all diagonal arrows in the master complex for a knot disappear when descending to any of the complexes at hand.
Example 3.5. The Torus Knot T 3 , 4 T_{3,4} T 3 , 4 .
Here Δ ( T 3 , 4 ) = t − 3 − t − 2 + 1 − t 2 + t 3 \Delta(T_{3,4})=t^{-3}-t^{-2}+1-t^{2}+t^{3} Δ ( T 3 , 4 ) = t − 3 − t − 2 + 1 − t 2 + t 3 , whose gaps are 1 , 2 , 2 , 1 1,2,2,1 1 , 2 , 2 , 1 , so C F K U , V ( T 3 , 4 ) CFK_{U,V}(T_{3,4}) C F K U , V ( T 3 , 4 ) is the complex
x 1 ← U x 2 x 1 ↓ V x 3 ← U 2 x 4 x 3 ↓ V x 3 x 5 \begin{aligned}
x_{1}&\xleftarrow{U}x_{2}\\
&\phantom{x_{1}}\qquad\downarrow V\\
x_{3}&\xleftarrow{U^{2}}x_{4}\\
&\phantom{x_{3}}\qquad\downarrow V\\
&\phantom{x_{3}}\qquad x_{5}
\end{aligned} x 1 x 3 U x 2 x 1 ↓ V U 2 x 4 x 3 ↓ V x 3 x 5
Take n = 2 n=2 n = 2 . Since V V V acts by 2 U 2U 2 U and U 2 = 0 U^2=0 U 2 = 0 , in C F K 2 ( T 3 , 4 ) CFK_2(T_{3,4}) C F K 2 ( T 3 , 4 ) we have ∂ 2 x 2 = U x 1 \partial_2x_2=Ux_1 ∂ 2 x 2 = U x 1 and ∂ 2 x 4 = 2 U x 5 \partial_2x_4=2Ux_5 ∂ 2 x 4 = 2 U x 5 , while in C F K − ( T 3 , 4 ) ⊗ Q [ U ] Q [ U ] ( U 2 ) CFK^-(T_{3,4})\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^2)} C F K − ( T 3 , 4 ) ⊗ Q [ U ] ( U 2 ) Q [ U ] we have ∂ x 2 = U x 1 \partial x_2=Ux_1 ∂ x 2 = U x 1 and ∂ x 4 = 0 \partial x_4=0 ∂ x 4 = 0 . Hence
H F K 2 ( T 3 , 4 ) ≅ Q [ U ] ( U 2 ) ⊕ Q 4 . HFK_2(T_{3,4})\cong\frac{\mathbb{Q}[U]}{(U^2)}\oplus\mathbb{Q}^4. H F K 2 ( T 3 , 4 ) ≅ ( U 2 ) Q [ U ] ⊕ Q 4 .
of dimension 6. On the other hand H F K − ( T 3 , 4 ) ≅ Q [ U ] ⊕ Q [ U ] ( U ) ⊕ Q [ U ] ( U 2 ) HFK^-(T_{3,4})\cong\mathbb{Q}[U]\oplus\frac{\mathbb{Q}[U]}{(U)}\oplus\frac{\mathbb{Q}[U]}{(U^2)} H F K − ( T 3 , 4 ) ≅ Q [ U ] ⊕ ( U ) Q [ U ] ⊕ ( U 2 ) Q [ U ] , and the universal coefficient theorem gives
H F K − ( T 3 , 4 ) ⊗ Q [ U ] Q [ U ] ( U 2 ) ⊕ Tor 1 Q [ U ] ( H F K − ( T 3 , 4 ) ; Q [ U ] ( U 2 ) ) ≅ ( Q [ U ] ( U 2 ) ) 3 ⊕ Q 2 . HFK^-(T_{3,4})\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^2)}\oplus\operatorname{Tor}^{\mathbb{Q}[U]}_1\left(HFK^-(T_{3,4});\frac{\mathbb{Q}[U]}{(U^2)}\right)\cong\left(\frac{\mathbb{Q}[U]}{(U^2)}\right)^3\oplus\mathbb{Q}^2. H F K − ( T 3 , 4 ) ⊗ Q [ U ] ( U 2 ) Q [ U ] ⊕ Tor 1 Q [ U ] ( H F K − ( T 3 , 4 ) ; ( U 2 ) Q [ U ] ) ≅ ( ( U 2 ) Q [ U ] ) 3 ⊕ Q 2 .
of dimension 8. The value 6 agrees with Dowlin’s computation dim Q H F K 2 ( T 3 , 3 k + 1 ) = 2 + 4 k \dim_{\mathbb{Q}}HFK_2(T_{3,3k+1})=2+4k dim Q H F K 2 ( T 3 , 3 k + 1 ) = 2 + 4 k [1 Lemma 5.9] . The discrepancy comes from the arrow x 4 → 2 U x 5 x_4\to2Ux_5 x 4 → 2 U x 5 : a vertical arrow of length one survives in C F K 2 CFK_2 C F K 2 , and there is no horizontal arrow of length at most n − 1 = 1 n-1=1 n − 1 = 1 leaving x 4 x_4 x 4 to absorb it (compare Lemma 4.13 and Proposition 4.15 ). For n ≥ 3 n\geq3 n ≥ 3 , both sides have dimension n + 6 n+6 n + 6 .
Proof of Main Theorem
Motivated by the preceding examples, we prove Theorem 1.4 using the universal coefficient theorem. In fact, since Q [ U ] \mathbb{Q}[U] Q [ U ] is a principal ideal domain and C F K − ( K ) CFK^-(K) C F K − ( K ) is a finitely generated free complex over Q [ U ] \mathbb{Q}[U] Q [ U ] [19 ] (see also [4 Theorem 6.1] ),
H ∗ ( C F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) ≅ [ H F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ] ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; Q [ U ] ( U n ) ) . H_*\left(CFK^-(K)\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^n)}\right)\cong\left[HFK^-(K)\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^n)}\right]\oplus\operatorname{Tor}^{\mathbb{Q}[U]}_1\left(HFK^-(K);\frac{\mathbb{Q}[U]}{(U^n)}\right). H ∗ ( C F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) ≅ [ H F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ] ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; ( U n ) Q [ U ] ) .
Here and below these are isomorphisms of ungraded Q [ U ] \mathbb{Q}[U] Q [ U ] -modules: the splitting is not natural, and in a graded statement the Tor summand appears with a shift in degree.
Recall that, by Theorem 2.12 , Dowlin’s complex C F K n ( K ) CFK_n(K) C F K n ( K ) for knots may be replaced by the quotient
C F K n ( K ) ≃ C F K U , V ( K ) ( U V , V − n U n − 1 ) . CFK_n(K)\simeq\frac{CFK_{U,V}(K)}{(UV,V-nU^{n-1})}. C F K n ( K ) ≃ ( U V , V − n U n − 1 ) C F K U , V ( K ) .
In Examples 3.2 and 3.3 in § 3 , for n ≥ 2 n\geq2 n ≥ 2 , this complex turns out to be isomorphic to
C F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) CFK^-(K)\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^n)} C F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ]
which we can compute using the universal coefficient theorem. This motivates us to propose another definition:
Definition 4.1. Given a finitely generated free chain complex C = ⨁ Q [ U , V ] C=\bigoplus\mathbb{Q}[U,V] C = ⨁ Q [ U , V ] over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] , define
C n : = C ( U V , V − n U n − 1 ) C_n:=\frac{C}{(UV,V-nU^{n-1})} C n := ( U V , V − n U n − 1 ) C
C ~ n : = C ( V , U n ) . \widetilde{C}_n:=\frac{C}{(V,U^n)}. C n := ( V , U n ) C .
Remark 4.2. Notice that
C ( U V , V − n U n − 1 ) ≅ C ⊗ Q [ U , V ] Q [ U , V ] ( U V , V − n U n − 1 ) , \frac{C}{(UV,V-nU^{n-1})}\cong C\otimes_{\mathbb{Q}[U,V]}\frac{\mathbb{Q}[U,V]}{(UV,V-nU^{n-1})}, ( U V , V − n U n − 1 ) C ≅ C ⊗ Q [ U , V ] ( U V , V − n U n − 1 ) Q [ U , V ] ,
and similarly that
C ( V , U n ) ≅ C ⊗ Q [ U , V ] Q [ U , V ] ( V , U n ) ≅ C ( V ) ⊗ Q [ U ] Q [ U ] ( U n ) , \frac{C}{(V,U^n)}\cong C\otimes_{\mathbb{Q}[U,V]}\frac{\mathbb{Q}[U,V]}{(V,U^n)}\cong\frac{C}{(V)}\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^n)}, ( V , U n ) C ≅ C ⊗ Q [ U , V ] ( V , U n ) Q [ U , V ] ≅ ( V ) C ⊗ Q [ U ] ( U n ) Q [ U ] ,
so C F K n ( K ) CFK_n(K) C F K n ( K ) and C F K ~ n ( K ) : = C F K U , V ( K ) / ( V , U n ) ≅ C F K − ( K ) ⊗ Q [ U ] ( U n ) \widetilde{CFK}_n(K):=CFK_{U,V}(K)/(V,U^n)\cong CFK^-(K)\otimes\frac{\mathbb{Q}[U]}{(U^n)} C F K n ( K ) := C F K U , V ( K ) / ( V , U n ) ≅ C F K − ( K ) ⊗ ( U n ) Q [ U ] are as in Definition 4.1.
In general, C n C_n C n and C ~ n \widetilde{C}_n C n are not isomorphic as Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] -modules or quasi-isomorphic, while their underlying Q [ U ] \mathbb{Q}[U] Q [ U ] -modules are isomorphic (Remark 3.1 ). In fact, we have the following counterexample:
Lemma 4.3. C n C_n C n and C ~ n \widetilde{C}_n C n do not always have the same homology.
Proof. Consider the complex C C C given by
Q [ U , V ] → V Q [ U , V ] . \mathbb{Q}[U,V]\xrightarrow{V}\mathbb{Q}[U,V]. Q [ U , V ] V Q [ U , V ] .
Then C n C_n C n is
Q [ U ] ( U n ) → n U n − 1 Q [ U ] ( U n ) . \frac{\mathbb{Q}[U]}{(U^n)}\xrightarrow{nU^{n-1}}\frac{\mathbb{Q}[U]}{(U^n)}. ( U n ) Q [ U ] n U n − 1 ( U n ) Q [ U ] .
and C ~ n \widetilde{C}_n C n is
Q [ U ] ( U n ) → 0 Q [ U ] ( U n ) . \frac{\mathbb{Q}[U]}{(U^n)}\xrightarrow{0}\frac{\mathbb{Q}[U]}{(U^n)}. ( U n ) Q [ U ] 0 ( U n ) Q [ U ] .
On the level of homology,
H ∗ ( C n ) ≅ Q [ U ] ( U n − 1 ) ⊕ Q [ U ] ( U n − 1 ) . H_*(C_n)\cong\frac{\mathbb{Q}[U]}{(U^{n-1})}\oplus\frac{\mathbb{Q}[U]}{(U^{n-1})}. H ∗ ( C n ) ≅ ( U n − 1 ) Q [ U ] ⊕ ( U n − 1 ) Q [ U ] .
H ∗ ( C ~ n ) ≅ Q [ U ] ( U n ) ⊕ Q [ U ] ( U n ) . H_*(\widetilde{C}_n)\cong\frac{\mathbb{Q}[U]}{(U^n)}\oplus\frac{\mathbb{Q}[U]}{(U^n)}. H ∗ ( C n ) ≅ ( U n ) Q [ U ] ⊕ ( U n ) Q [ U ] .
Although a general complex over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] will not lead to isomorphic specializations, we observe that the complexes are chain homotopy equivalent in many important cases.
L-space and thin knots
The aforementioned classes of knots of interest are L L L -space knots and thin knots, as defined in § 1 ; throughout, thinness refers to H F K ^ ( K ; Q ) \widehat{HFK}(K;\mathbb{Q}) H F K ( K ; Q ) . We now turn to defining the structures present in the knot Floer complexes of these kinds of knots.
Definition 4.4 (Box). A chain complex C = ⨁ i = 1 4 Q [ U , V ] ⟨ x i ⟩ C=\bigoplus_{i=1}^{4}\mathbb{Q}[U,V]\langle x_i\rangle C = ⨁ i = 1 4 Q [ U , V ] ⟨ x i ⟩ is a box complex if it is in the form
x 2 ← U k x 1 V l ↓ ↓ V l x 4 ← U k x 3 \begin{CD}
x_2 @<{U^k}<< x_1 \\
@V{V^l}VV @VV{V^l}V \\
x_4 @<{U^k}<< x_3
\end{CD} x 2 V l ↓ ⏐ x 4 U k U k x 1 ↓ ⏐ V l x 3 for some positive integers k k k and l l l , where each x i x_i x i is the generator of Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] corresponding to the i i i -th summand of C C C .
Definition 4.5 (Staircase). A chain complex C = ⨁ i = 1 m Q [ U , V ] ⟨ x i ⟩ C=\bigoplus_{i=1}^{m}\mathbb{Q}[U,V]\langle x_i\rangle C = ⨁ i = 1 m Q [ U , V ] ⟨ x i ⟩ is a staircase complex if it is in one of the forms in Figure 4 for some positive integers k i k_i k i and odd integer m ≥ 1 m\ge1 m ≥ 1 , where each x i x_i x i is the generator of Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] corresponding to the i i i -th summand of C C C . In both forms the arrow between x i x_i x i and x i + 1 x_{i+1} x i + 1 has length k i k_i k i ; in the left form the sources are the x i x_i x i with i i i even, and in the right form the x i x_i x i with i i i odd. Thus, in either form, for each source x i x_i x i ,
∂ x i = U k i − 1 x i − 1 + V k i x i + 1 , \partial x_i=U^{k_i-1}x_{i-1}+V^{k_i}x_{i+1}, ∂ x i = U k i − 1 x i − 1 + V k i x i + 1 , where terms involving x 0 x_0 x 0 or x m + 1 x_{m+1} x m + 1 are omitted. When m = 1 m=1 m = 1 , C = Q [ U , V ] ⟨ x 1 ⟩ C=\mathbb{Q}[U,V]\langle x_1\rangle C = Q [ U , V ] ⟨ x 1 ⟩ with zero differential.
Figure 4. The two possible staircase complexes: the left form and the right form.
Example 4.6. The master complex for the trefoil, C F K U , V ( T 2 , 3 ) CFK_{U,V}(T_{2,3}) C F K U , V ( T 2 , 3 ) as in Example 3.2 , is a staircase complex.
Figure 5. The tower (vector space) structure of the complex C F K n ( T 2 , 3 ) CFK_n(T_{2,3}) C F K n ( T 2 , 3 ) (the complex shown in Figure 2 ). For example, ∂ n ( x 2 ) = U x 1 + n U n − 1 x 3 \partial_n(x_2)=Ux_1+nU^{n-1}x_3 ∂ n ( x 2 ) = U x 1 + n U n − 1 x 3 and ∂ n ( U x 2 ) = U 2 x 1 \partial_n(Ux_2)=U^2x_1 ∂ n ( U x 2 ) = U 2 x 1 .
With these definitions in place, we appeal to two structure theorems concerning the master complex C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) of thin and L L L -space knots. Both are statements up to homotopy equivalence over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] . The proofs for these and Theorem 4.14 rely on the following Lemma:
Lemma 4.8 (Cancellation lemma). [4 Lemma 4.1] Let ( C , ∂ ) (C,\partial) ( C , ∂ ) be a chain complex of R R R -modules, freely generated by chains { x i } \{x_i\} { x i } , and suppose that d ( x k , x l ) d(x_k,x_l) d ( x k , x l ) is a unit in R R R , where
∂ ( x k ) = ∑ m ≠ l a m x m + d ( x k , x l ) x l . \partial(x_k)=\sum_{m\ne l}a_mx_m+d(x_k,x_l)x_l. ∂ ( x k ) = m = l ∑ a m x m + d ( x k , x l ) x l . Then we can define a complex ( C ′ , ∂ ′ ) (C',\partial') ( C ′ , ∂ ′ ) , freely generated by { x i ∣ i ≠ k , i ≠ l } \{x_i\mid i\ne k,\ i\ne l\} { x i ∣ i = k , i = l } , which is chain homotopy equivalent to ( C , ∂ ) (C,\partial) ( C , ∂ ) . Writing d ( x i , x j ) d(x_i,x_j) d ( x i , x j ) for the coefficient of x j x_j x j in ∂ x i \partial x_i ∂ x i , the differential is given by d ′ ( x i , x j ) = d ( x i , x j ) − d ( x i , x l ) d ( x k , x l ) − 1 d ( x k , x j ) d'(x_i,x_j)=d(x_i,x_j)-d(x_i,x_l)d(x_k,x_l)^{-1}d(x_k,x_j) d ′ ( x i , x j ) = d ( x i , x j ) − d ( x i , x l ) d ( x k , x l ) − 1 d ( x k , x j ) .
Theorem 4.9. (cf. [15 Lemma 7] ) If a knot K K K is Floer homologically thin, then C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) is homotopy equivalent over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] to a direct sum of one staircase complex with all k i = 1 k_i=1 k i = 1 and m = 2 ∣ τ ( K ) ∣ + 1 m=2|\tau(K)|+1 m = 2∣ τ ( K ) ∣ + 1 , of the left form in Figure 4 if τ ( K ) ≥ 0 \tau(K)\ge0 τ ( K ) ≥ 0 and of the right form if τ ( K ) < 0 \tau(K)<0 τ ( K ) < 0 , and box complexes with k = l = 1 k=l=1 k = l = 1 .
Proof. Here we need the gradings that were suppressed in § 2 . The master complex C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) is bigraded by ( gr U , gr V ) (\operatorname{gr}_U,\operatorname{gr}_V) ( gr U , gr V ) , in which U U U has bidegree ( − 2 , 0 ) (-2,0) ( − 2 , 0 ) , V V V has bidegree ( 0 , − 2 ) (0,-2) ( 0 , − 2 ) and the differential has bidegree ( − 1 , − 1 ) (-1,-1) ( − 1 , − 1 ) . The Alexander and Maslov gradings are A = 1 2 ( gr U − gr V ) A=\frac{1}{2}(\operatorname{gr}_U-\operatorname{gr}_V) A = 2 1 ( gr U − gr V ) and M = gr U M=\operatorname{gr}_U M = gr U [Zem19, Hom21].
Step 1: every arrow has length one. Applying Lemma 4.8 repeatedly to arrows whose coefficients are invertible, we obtain a complex C C C , homotopy equivalent to C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] , which is free on a homogeneous basis and satisfies ∂ C ⊂ ( U , V ) C \partial C\subset(U,V)C ∂ C ⊂ ( U , V ) C . The process terminates since there are finitely many generators, and it preserves the bigrading. Let Ω \Omega Ω be the Q \mathbb{Q} Q -span of this basis, graded by A A A as Ω = ⨁ a Ω a \Omega=\bigoplus_a\Omega_a Ω = ⨁ a Ω a . Since the differential of C / ( U , V ) C/(U,V) C / ( U , V ) vanishes, Ω ≅ H F K ^ ( K ; Q ) \Omega\cong\widehat{HFK}(K;\mathbb{Q}) Ω ≅ H F K ( K ; Q ) as graded vector spaces. Since K K K is thin, A − M = − 1 2 ( gr U + gr V ) A-M=-\frac{1}{2}(\operatorname{gr}_U+\operatorname{gr}_V) A − M = − 2 1 ( gr U + gr V ) is constant on Ω \Omega Ω . If c U i V j y cU^iV^jy c U i V j y with c ≠ 0 c\ne0 c = 0 appears in ∂ x \partial x ∂ x for basis elements x x x and y y y , then comparing gr U + gr V \operatorname{gr}_U+\operatorname{gr}_V gr U + gr V on both sides gives
( gr U + gr V ) ( y ) − 2 ( i + j ) = ( gr U + gr V ) ( x ) − 2 , (\operatorname{gr}_U+\operatorname{gr}_V)(y)-2(i+j)=(\operatorname{gr}_U+\operatorname{gr}_V)(x)-2, ( gr U + gr V ) ( y ) − 2 ( i + j ) = ( gr U + gr V ) ( x ) − 2 ,
so i + j = 1 i+j=1 i + j = 1 . Hence there are Q \mathbb{Q} Q -linear maps ξ , η : Ω → Ω \xi,\eta:\Omega\to\Omega ξ , η : Ω → Ω such that
∂ = U ξ + V η \partial=U\xi+V\eta ∂ = U ξ + V η
on C = Ω ⊗ Q [ U , V ] C=\Omega\otimes\mathbb{Q}[U,V] C = Ω ⊗ Q [ U , V ] , with ξ ( Ω a ) ⊂ Ω a + 1 \xi(\Omega_a)\subset\Omega_{a+1} ξ ( Ω a ) ⊂ Ω a + 1 and η ( Ω a ) ⊂ Ω a − 1 \eta(\Omega_a)\subset\Omega_{a-1} η ( Ω a ) ⊂ Ω a − 1 .
Step 2: an exterior algebra. Expanding ∂ 2 = U 2 ξ 2 + U V ( ξ η + η ξ ) + V 2 η 2 = 0 \partial^2=U^2\xi^2+UV(\xi\eta+\eta\xi)+V^2\eta^2=0 ∂ 2 = U 2 ξ 2 + U V ( ξ η + η ξ ) + V 2 η 2 = 0 gives
ξ 2 = 0 , η 2 = 0 , ξ η = − η ξ . (1) \xi^2=0,\qquad\eta^2=0,\qquad\xi\eta=-\eta\xi. \tag*{(1)} ξ 2 = 0 , η 2 = 0 , ξ η = − η ξ . (1)
So Ω \Omega Ω is a graded module over the exterior algebra Λ = Q ⟨ ξ , η ⟩ / ( ξ 2 , η 2 , ξ η + η ξ ) \Lambda= \mathbb{Q}\langle\xi,\eta\rangle/(\xi^2,\eta^2,\xi\eta+\eta\xi) Λ = Q ⟨ ξ , η ⟩ / ( ξ 2 , η 2 , ξ η + η ξ ) , and a decomposition Ω = Ω ′ ⊕ Ω ′ ′ \Omega=\Omega^\prime\oplus\Omega^{\prime\prime} Ω = Ω ′ ⊕ Ω ′′ into graded Λ \Lambda Λ -submodules gives a decomposition into subcomplexes
C = ( Ω ′ ⊗ Q [ U , V ] ) ⊕ ( Ω ′ ′ ⊗ Q [ U , V ] ) . C=(\Omega^\prime\otimes\mathbb{Q}[U,V])\oplus(\Omega^{\prime\prime}\otimes\mathbb{Q}[U,V]). C = ( Ω ′ ⊗ Q [ U , V ]) ⊕ ( Ω ′′ ⊗ Q [ U , V ]) .
Moreover, the complex ( Ω , ξ ) (\Omega,\xi) ( Ω , ξ ) is C ⊗ Q [ U , V ] ( U − 1 , V − 1 ) ≃ C F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U − 1 ) C\otimes\frac{\mathbb{Q}[U,V]}{(U^{-1},V^{-1})}\simeq CFK^-(K)\otimes_{\mathbb{Q}[U]}\frac{\mathbb{Q}[U]}{(U^{-1})} C ⊗ ( U − 1 , V − 1 ) Q [ U , V ] ≃ C F K − ( K ) ⊗ Q [ U ] ( U − 1 ) Q [ U ] , whose homology is H F ^ ( S 3 ) ≅ Q \widehat{HF}(S^3)\cong\mathbb{Q} H F ( S 3 ) ≅ Q [12 ] . In the same way ( Ω , η ) (\Omega,\eta) ( Ω , η ) computes H F ^ ( S 3 ) \widehat{HF}(S^3) H F ( S 3 ) using the basepoint w w w . Thus
dim Q H ∗ ( Ω , ξ ) = dim Q H ∗ ( Ω , η ) = 1. \dim_{\mathbb{Q}}H_*(\Omega,\xi)=\dim_{\mathbb{Q}}H_*(\Omega,\eta)=1. dim Q H ∗ ( Ω , ξ ) = dim Q H ∗ ( Ω , η ) = 1.
Step 3: splitting off boxes. Suppose ξ η x ≠ 0 \xi\eta x\ne0 ξ η x = 0 for some x ∈ Ω a x\in\Omega_a x ∈ Ω a . Then x x x , ξ x \xi x ξ x , η x \eta x η x and ξ η x \xi\eta x ξ η x are linearly independent: ξ x \xi x ξ x and η x \eta x η x are nonzero and lie in Ω a + 1 \Omega_{a+1} Ω a + 1 and Ω a − 1 \Omega_{a-1} Ω a − 1 , and ξ η x = c x \xi\eta x=cx ξ η x = c x is impossible, since it would give c 2 x = ( ξ η ) 2 x = − ξ 2 η 2 x = 0 c^2x=(\xi\eta)^2x=-\xi^2\eta^2x=0 c 2 x = ( ξ η ) 2 x = − ξ 2 η 2 x = 0 . So their span Γ \Gamma Γ is a free Λ \Lambda Λ -submodule of rank one. Choose a linear map λ : Ω → Q \lambda:\Omega\to\mathbb{Q} λ : Ω → Q which vanishes outside Ω a \Omega_a Ω a with λ ( x ) = 0 \lambda(x)=0 λ ( x ) = 0 and λ ( ξ η x ) = 1 \lambda(\xi\eta x)=1 λ ( ξ η x ) = 1 , and define ρ : Ω → Γ \rho:\Omega\to\Gamma ρ : Ω → Γ by
ρ ( w ) = λ ( ξ η w ) x − λ ( η w ) ξ x + λ ( ξ w ) η x + λ ( w ) ξ η x . \rho(w)=\lambda(\xi\eta w)x-\lambda(\eta w)\xi x+\lambda(\xi w)\eta x+\lambda(w)\xi\eta x. ρ ( w ) = λ ( ξ η w ) x − λ ( η w ) ξ x + λ ( ξ w ) η x + λ ( w ) ξ η x .
A direct check using the relations of Step 2 shows that ρ ξ = ξ ρ \rho\xi=\xi\rho ρ ξ = ξ ρ and ρ η = η ρ \rho\eta=\eta\rho ρ η = η ρ ; since λ \lambda λ is supported on Ω a \Omega_a Ω a , ρ \rho ρ preserves the grading; and ρ ( x ) = x \rho(x)=x ρ ( x ) = x , so ρ \rho ρ is the identity on Γ \Gamma Γ . Hence Ω = Γ ⊕ ker ρ \Omega=\Gamma\oplus\ker\rho Ω = Γ ⊕ ker ρ as graded Λ \Lambda Λ -modules. In the basis
x 1 = x , x 2 = ξ x , x 3 = − η x , x 4 = η ξ x , x_1=x,\qquad x_2=\xi x,\qquad x_3=-\eta x,\qquad x_4=\eta\xi x, x 1 = x , x 2 = ξ x , x 3 = − η x , x 4 = η ξ x ,
the complex Γ ⊗ Q [ U , V ] \Gamma\otimes\mathbb{Q}[U,V] Γ ⊗ Q [ U , V ] is the box complex of Definition 4.4 with k = l = 1 k=l=1 k = l = 1 : ∂ x 1 = U x 2 − V x 3 \partial x_1=Ux_2-Vx_3 ∂ x 1 = U x 2 − V x 3 , ∂ x 2 = V x 4 \partial x_2=Vx_4 ∂ x 2 = V x 4 and ∂ x 3 = U x 4 \partial x_3=Ux_4 ∂ x 3 = U x 4 . By induction on dim Q Ω \dim_{\mathbb{Q}}\Omega dim Q Ω ,
Ω = Γ 1 ⊕ ⋯ ⊕ Γ b ⊕ Ω ′ , \Omega=\Gamma_1\oplus\cdots\oplus\Gamma_b\oplus\Omega^\prime, Ω = Γ 1 ⊕ ⋯ ⊕ Γ b ⊕ Ω ′ ,
where each Γ i ⊗ Q [ U , V ] \Gamma_i\otimes\mathbb{Q}[U,V] Γ i ⊗ Q [ U , V ] is a box complex with k = l = 1 k=l=1 k = l = 1 and ξ η = η ξ = 0 \xi\eta=\eta\xi=0 ξ η = η ξ = 0 on Ω ′ \Omega^\prime Ω ′ .
Step 4: staircases. Let Θ = ker ξ ∩ ker η ⊂ Ω ′ \Theta=\ker\xi\cap\ker\eta\subset\Omega^\prime Θ = ker ξ ∩ ker η ⊂ Ω ′ , and let Ψ \Psi Ψ be a graded complement of Θ \Theta Θ in Ω ′ \Omega^\prime Ω ′ . Since all products of ξ \xi ξ and η \eta η vanish on Ω ′ \Omega^\prime Ω ′ , both maps send Ω ′ \Omega^\prime Ω ′ into Θ \Theta Θ and vanish on Θ \Theta Θ . So Ω ′ \Omega^\prime Ω ′ is determined by the restrictions ξ : Ψ a → Θ a + 1 \xi:\Psi_a\to\Theta_{a+1} ξ : Ψ a → Θ a + 1 and η : Ψ a → Θ a − 1 \eta:\Psi_a\to\Theta_{a-1} η : Ψ a → Θ a − 1 , which form a representation of the quiver with vertices Ψ a \Psi_a Ψ a and Θ a \Theta_a Θ a for a ∈ Z a\in\mathbb{Z} a ∈ Z and these arrows; a decomposition of this representation is a decomposition of Ω ′ \Omega^\prime Ω ′ into graded Λ \Lambda Λ -submodules. The underlying graph of the quiver is a disjoint union of two lines
⋯ − Θ a − 1 − Ψ a − Θ a + 1 − Ψ a + 2 − ⋯ , \cdots-\Theta_{a-1}-\Psi_a-\Theta_{a+1}-\Psi_{a+2}-\cdots, ⋯ − Θ a − 1 − Ψ a − Θ a + 1 − Ψ a + 2 − ⋯ ,
and since Ω ′ \Omega^\prime Ω ′ is finite-dimensional, the representation is supported on a quiver of type A. By Gabriel’s theorem [3 ] , it is a direct sum of interval representations, which are one-dimensional at each vertex of a segment of a line, zero elsewhere, and have every arrow in the segment an isomorphism. After rescaling the basis vectors along the segment, each such summand Υ \Upsilon Υ gives a staircase complex Υ ⊗ Q [ U , V ] \Upsilon\otimes\mathbb{Q}[U,V] Υ ⊗ Q [ U , V ] with all k i = 1 k_i=1 k i = 1 , whose sources are the basis vectors lying in Ψ \Psi Ψ . It is of the left form if the endpoints of the segment lie in Θ \Theta Θ (which includes the case m = 1 m=1 m = 1 ), and of the right form if they lie in Ψ \Psi Ψ .
Step 5: exactly one staircase. The complexes ( Γ i , ξ ) (\Gamma_i,\xi) ( Γ i , ξ ) and ( Γ i , η ) (\Gamma_i,\eta) ( Γ i , η ) are acyclic. If an interval summand Υ \Upsilon Υ has v v v basis vectors, it has v − 1 v-1 v − 1 arrows, say e ξ e_\xi e ξ of them given by ξ \xi ξ and e η e_\eta e η given by η \eta η , each an isomorphism between one-dimensional spaces. Hence
dim Q H ∗ ( Υ , ξ ) + dim Q H ∗ ( Υ , η ) = ( v − 2 e ξ ) + ( v − 2 e η ) = 2. \dim_{\mathbb{Q}}H_*(\Upsilon,\xi)+\dim_{\mathbb{Q}}H_*(\Upsilon,\eta)=(v-2e_\xi)+(v-2e_\eta)=2. dim Q H ∗ ( Υ , ξ ) + dim Q H ∗ ( Υ , η ) = ( v − 2 e ξ ) + ( v − 2 e η ) = 2.
By Step 2 the total of these quantities over Ω \Omega Ω is 2 2 2 , so there is exactly one interval summand Υ \Upsilon Υ , and dim Q H ∗ ( Υ , ξ ) = dim Q H ∗ ( Υ , η ) = 1 \dim_{\mathbb{Q}}H_*(\Upsilon,\xi)=\dim_{\mathbb{Q}}H_*(\Upsilon,\eta)=1 dim Q H ∗ ( Υ , ξ ) = dim Q H ∗ ( Υ , η ) = 1 forces e ξ = e η e_\xi=e_\eta e ξ = e η , so m = v = 2 e ξ + 1 m=v=2e_\xi+1 m = v = 2 e ξ + 1 is odd. Thus
C = S ⊕ B 1 ⊕ ⋯ ⊕ B b , \mathcal{C}=\mathcal{S}\oplus\mathcal{B}_1\oplus\cdots\oplus\mathcal{B}_b, C = S ⊕ B 1 ⊕ ⋯ ⊕ B b ,
where S = Υ ⊗ Q [ U , V ] \mathcal{S}=\Upsilon\otimes\mathbb{Q}[U,V] S = Υ ⊗ Q [ U , V ] is a staircase complex with all k i = 1 k_i=1 k i = 1 and each B i = Γ i ⊗ Q [ U , V ] \mathcal{B}_i=\Gamma_i\otimes\mathbb{Q}[U,V] B i = Γ i ⊗ Q [ U , V ] is a box complex with k = l = 1 k=l=1 k = l = 1 .
Step 6: the length of the staircase. We use the convention [6 ]
τ ( K ) = − max { A ( y ) : y ∈ H F K − ( K ) homogeneous , U d y ≠ 0 for all d } . \tau(K)=-\max\{A(y):y\in HFK^-(K)\text{ homogeneous},\ U^d y\ne0\text{ for all }d\}. τ ( K ) = − max { A ( y ) : y ∈ H F K − ( K ) homogeneous , U d y = 0 for all d } .
Number the generators of S \mathcal{S} S as in Definition 4.5 . Since ξ \xi ξ raises and η \eta η lowers A A A by one, in either form A ( x j ) = A ( x 1 ) − ( j − 1 ) A(x_j)=A(x_1)-(j-1) A ( x j ) = A ( x 1 ) − ( j − 1 ) . Each B i / ( V ) \mathcal{B}_i/(V) B i / ( V ) has homology Q ⟨ x 2 ⟩ ⊕ Q ⟨ x 4 ⟩ \mathbb{Q}\langle x_2\rangle\oplus\mathbb{Q}\langle x_4\rangle Q ⟨ x 2 ⟩ ⊕ Q ⟨ x 4 ⟩ , which is U U U -torsion, so the U U U -nontorsion part of H F K − ( K ) = H ∗ ( C / ( V ) ) HFK^-(K)=H_*(\mathcal{C}/(V)) H F K − ( K ) = H ∗ ( C / ( V )) comes from S / ( V ) \mathcal{S}/(V) S / ( V ) , where it is generated by x m x_m x m in the left form and by x 1 x_1 x 1 in the right form; this generator has Alexander grading − τ ( K ) -\tau(K) − τ ( K ) . The symmetry of the master complex which exchanges the roles of w w w and z z z [12 Section 3.5] interchanges U U U and V V V and replaces A A A by − A -A − A . So the V V V -nontorsion part of H ∗ ( C / ( U ) ) H_*(\mathcal{C}/(U)) H ∗ ( C / ( U )) lies in Alexander grading τ ( K ) \tau(K) τ ( K ) , and it is generated by x 1 x_1 x 1 in the left form and by x m x_m x m in the right form. In the left form, 2 τ ( K ) = A ( x 1 ) − A ( x m ) = m − 1 2\tau(K)=A(x_1)-A(x_m)=m-1 2 τ ( K ) = A ( x 1 ) − A ( x m ) = m − 1 ; in the right form, − 2 τ ( K ) = A ( x 1 ) − A ( x m ) = m − 1 -2\tau(K)=A(x_1)-A(x_m)=m-1 − 2 τ ( K ) = A ( x 1 ) − A ( x m ) = m − 1 . Hence m = 2 ∣ τ ( K ) ∣ + 1 m=2|\tau(K)|+1 m = 2∣ τ ( K ) ∣ + 1 , the staircase is of the left form if τ ( K ) ≥ 0 \tau(K)\geq0 τ ( K ) ≥ 0 , and of the right form if τ ( K ) < 0 \tau(K)<0 τ ( K ) < 0 .
Example 4.10 (The knot 5 2 5_2 5 2 ). We illustrate the proof with the knot 5 2 5_2 5 2 , which is alternating and hence thin, with
Δ 5 2 ( t ) = 2 t − 3 + 2 t − 1 \Delta_{5_2}(t)=2t-3+2t^{-1} Δ 5 2 ( t ) = 2 t − 3 + 2 t − 1 and det ( 5 2 ) = 7 \det(5_2)=7 det ( 5 2 ) = 7 . Choose its chirality so that τ ( 5 2 ) = 1 \tau(5_2)=1 τ ( 5 2 ) = 1 . Then H F K ^ ( 5 2 ; Q ) \widehat{HFK}(5_2;\mathbb{Q}) H F K ( 5 2 ; Q ) has rank 2, 3 and 2 in Alexander gradings 1, 0 and − 1 -1 − 1 , with M = A − 1 M=A-1 M = A − 1 . Consider the reduced complex C C C with basis y 1 , y 2 y_1,y_2 y 1 , y 2 in Alexander grading 1, y 3 , y 4 , y 5 y_3,y_4,y_5 y 3 , y 4 , y 5 in grading 0, and y 6 , y 7 y_6,y_7 y 6 , y 7 in grading − 1 -1 − 1 , and differential
∂ y 3 = U y 1 + V y 7 , ∂ y 4 = U y 2 − V y 6 + 2 V y 7 , ∂ y 2 = V y 5 , ∂ y 6 = U y 5 . \partial y_3=Uy_1+Vy_7,\qquad\partial y_4=Uy_2-Vy_6+2Vy_7,\qquad\partial y_2=Vy_5,\qquad\partial y_6=Uy_5. ∂ y 3 = U y 1 + V y 7 , ∂ y 4 = U y 2 − V y 6 + 2 V y 7 , ∂ y 2 = V y 5 , ∂ y 6 = U y 5 . with ∂ y 1 = ∂ y 5 = ∂ y 7 = 0 \partial y_1=\partial y_5=\partial y_7=0 ∂ y 1 = ∂ y 5 = ∂ y 7 = 0 . We have C F K U , V ( 5 2 ) CFK_{U,V}(5_2) C F K U , V ( 5 2 ) , written in a basis in which its decomposition is not clear, so we follow the proof to recover it. Here,
ξ ( y 3 ) = y 1 , ξ ( y 4 ) = y 2 , ξ ( y 6 ) = y 5 , η ( y 2 ) = y 5 , η ( y 3 ) = y 7 , η ( y 4 ) = − y 6 + 2 y 7 , \xi(y_3)=y_1,\qquad\xi(y_4)=y_2,\qquad\xi(y_6)=y_5,\qquad\eta(y_2)=y_5,\qquad\eta(y_3)=y_7,\qquad\eta(y_4)=-y_6+2y_7, ξ ( y 3 ) = y 1 , ξ ( y 4 ) = y 2 , ξ ( y 6 ) = y 5 , η ( y 2 ) = y 5 , η ( y 3 ) = y 7 , η ( y 4 ) = − y 6 + 2 y 7 , and ξ \xi ξ and η \eta η vanish on the remaining basis vectors. One checks the relations of Step 2, and that ξ \xi ξ and η \eta η each have rank 3, so dim Q H ∗ ( Ω , ξ ) = dim Q H ∗ ( Ω , η ) = 7 − 6 = 1 \dim_{\mathbb{Q}}H_*(\Omega,\xi)=\dim_{\mathbb{Q}}H_*(\Omega,\eta)=7-6=1 dim Q H ∗ ( Ω , ξ ) = dim Q H ∗ ( Ω , η ) = 7 − 6 = 1 .
For Step 3, ξ η ( y 4 ) = ξ ( − y 6 + 2 y 7 ) = − y 5 ≠ 0 \xi\eta(y_4)=\xi(-y_6+2y_7)=-y_5\ne0 ξ η ( y 4 ) = ξ ( − y 6 + 2 y 7 ) = − y 5 = 0 , so take x = y 4 x=y_4 x = y 4 and let λ \lambda λ be the linear map with λ ( y 5 ) = − 1 \lambda(y_5)=-1 λ ( y 5 ) = − 1 which vanishes on the other basis vectors. Then ρ \rho ρ fixes y 2 , y 4 y_2,y_4 y 2 , y 4 and y 5 y_5 y 5 , sends y 6 y_6 y 6 to y 6 − 2 y 7 y_6-2y_7 y 6 − 2 y 7 , and sends y 1 , y 3 y_1,y_3 y 1 , y 3 and y 7 y_7 y 7 to zero. The box is spanned by
x 1 = y 4 , x 2 = y 2 , x 3 = y 6 − 2 y 7 , x 4 = y 5 . x_1=y_4,\qquad x_2=y_2,\qquad x_3=y_6-2y_7,\qquad x_4=y_5. x 1 = y 4 , x 2 = y 2 , x 3 = y 6 − 2 y 7 , x 4 = y 5 . and indeed ∂ x 1 = U x 2 − V x 3 \partial x_1=Ux_2-Vx_3 ∂ x 1 = U x 2 − V x 3 , ∂ x 2 = V x 4 \partial x_2=Vx_4 ∂ x 2 = V x 4 and ∂ x 3 = U x 4 \partial x_3=Ux_4 ∂ x 3 = U x 4 . The change of basis y 6 ↦ y 6 − 2 y 7 y_6\mapsto y_6-2y_7 y 6 ↦ y 6 − 2 y 7 is what separates the box from the staircase.
For Step 4, Ω ′ = ker ρ \Omega'=\ker\rho Ω ′ = ker ρ is spanned by y 1 , y 3 y_1,y_3 y 1 , y 3 and y 7 y_7 y 7 , with Θ \Theta Θ spanned by y 1 y_1 y 1 and y 7 y_7 y 7 and Ψ \Psi Ψ spanned by y 3 y_3 y 3 . The single segment is Θ 1 − Ψ 0 − Θ − 1 \Theta_1-\Psi_0-\Theta_{-1} Θ 1 − Ψ 0 − Θ − 1 , whose endpoints lie in Θ \Theta Θ , so it gives the staircase of the left form with x 1 = y 1 x_1=y_1 x 1 = y 1 , x 2 = y 3 x_2=y_3 x 2 = y 3 and x 3 = y 7 x_3=y_7 x 3 = y 7 , that is, ∂ x 2 = U x 1 + V x 3 \partial x_2=Ux_1+Vx_3 ∂ x 2 = U x 1 + V x 3 . Thus
C F K U , V ( 5 2 ) ≃ C F K U , V ( T 2 , 3 ) ⊕ B , CFK_{U,V}(5_2)\simeq CFK_{U,V}(T_{2,3})\oplus\mathcal{B}, C F K U , V ( 5 2 ) ≃ C F K U , V ( T 2 , 3 ) ⊕ B , where B \mathcal{B} B is a box complex with k = l = 1 k=l=1 k = l = 1 . As in Step 6, the U U U -nontorsion generator of H F K − ( 5 2 ) HFK^-(5_2) H F K − ( 5 2 ) is x 3 = y 7 x_3=y_7 x 3 = y 7 , in Alexander grading − 1 = − τ ( 5 2 ) -1=-\tau(5_2) − 1 = − τ ( 5 2 ) , and m = 3 = 2 τ ( 5 2 ) + 1 m=3=2\tau(5_2)+1 m = 3 = 2 τ ( 5 2 ) + 1 . By Remark 4.19, H F K n ( 5 2 ) ≅ Q [ U ] ( U n ) ⊕ Q 6 HFK_n(5_2)\cong\frac{\mathbb{Q}[U]}{(U^n)}\oplus\mathbb{Q}^6 H F K n ( 5 2 ) ≅ ( U n ) Q [ U ] ⊕ Q 6 for n ≥ 2 n\geq2 n ≥ 2 .
Theorem 4.11. [13 Theorem 1.2] , [5 Remark 6.6] If a knot K K K is an L L L -space knot, then C F K U , V ( K ) CFK_{U,V}(K) C F K U , V ( K ) is homotopy equivalent over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] to a single staircase complex of the left form in Figure 4 , whose step lengths k 1 , … , k m − 1 k_1,\ldots,k_{m-1} k 1 , … , k m − 1 are the gaps of Δ K \Delta_K Δ K .
Here [15 Lemma 7] proves the decomposition of Theorem 4.9 over F 2 \mathbb{F}_2 F 2 , for the Alexander-filtered complex C F K − ( K ) CFK^-(K) C F K − ( K ) ; the proof of Theorem 4.9 above works over any field, and so recovers it. Similarly, [13 Theorem 1.2] determines H F K ^ ( K ) \widehat{HFK}(K) H F K ( K ) of an L L L -space knot, and the staircase form of the full complex is a standard consequence [5 Remark 6.6] ; over Q \mathbb{Q} Q , the signs of the arrows can be normalized by rescaling generators, since the underlying graph of a staircase is a path.
Main theorem
To prove the main theorem, we employ the following algebraic lemma along with Lemma 4.8. The second term in d ′ d' d ′ in Lemma 4.8 is the “zigzag” through the cancelled pair; it is exactly what the change of basis in the first case of the proof of Proposition 4.15 keeps track of.
Lemma 4.12. Let n ≥ 2 n\geq2 n ≥ 2 and let C C C be a box complex. If l ≥ 2 l\geq2 l ≥ 2 or k ≤ n − 1 k\leq n-1 k ≤ n − 1 , then C n ≅ C ~ n C_n\cong\widetilde{C}_n C n ≅ C n as complexes of Q [ U ] ( U n ) \frac{\mathbb{Q}[U]}{(U^n)} ( U n ) Q [ U ] -modules; in particular
H ∗ ( C n ) ≅ H ∗ ( C ~ n ) ≅ ( Q [ U ] ( U min ( k , n ) ) ) 4 H_*(C_n)\cong H_*(\widetilde{C}_n)\cong\left(\frac{\mathbb{Q}[U]}{(U^{\min(k,n)})}\right)^4 H ∗ ( C n ) ≅ H ∗ ( C n ) ≅ ( ( U m i n ( k , n ) ) Q [ U ] ) 4 is an isomorphism of Q [ U ] \mathbb{Q}[U] Q [ U ] -modules. If l = 1 l=1 l = 1 and k ≥ n k\geq n k ≥ n , then
H ∗ ( C n ) ≅ ( Q [ U ] ( U n − 1 ) ) 4 , H ∗ ( C ~ n ) ≅ ( Q [ U ] ( U n ) ) 4 . H_*(C_n)\cong\left(\frac{\mathbb{Q}[U]}{(U^{n-1})}\right)^4,\qquad H_*(\widetilde{C}_n)\cong\left(\frac{\mathbb{Q}[U]}{(U^n)}\right)^4. H ∗ ( C n ) ≅ ( ( U n − 1 ) Q [ U ] ) 4 , H ∗ ( C n ) ≅ ( ( U n ) Q [ U ] ) 4 .
Proof. Any box complex can be pictorially represented as in Definition 4.4 . Note that after the identifications V = n U n − 1 V=nU^{n-1} V = n U n − 1 and U V = 0 UV=0 U V = 0 in the ground ring, if l > 1 l>1 l > 1 (here n ≥ 2 n\ge2 n ≥ 2 is used in the third line),
V l = V ⋅ V l − 1 = n U n − 1 V l − 1 = U V ⋅ n U n − 2 V l − 2 = 0. \begin{aligned}
V^l &= V\cdot V^{l-1}\\
&=nU^{n-1}V^{l-1}\\
&=UV\cdot nU^{n-2}V^{l-2}\\
&=0.
\end{aligned} V l = V ⋅ V l − 1 = n U n − 1 V l − 1 = U V ⋅ n U n − 2 V l − 2 = 0.
So we see that if l > 1 l>1 l > 1 , the vertical arrows become zero in both C n C_n C n and C ~ n \widetilde{C}_n C n , and C n = C ~ n C_n=\widetilde{C}_n C n = C n . Thus, we restrict our attention to when l = 1 l=1 l = 1 . In this case, C n C_n C n and C ~ n \widetilde{C}_n C n are as in Figure 6 . If k ≤ n − 1 k\le n-1 k ≤ n − 1 , put x 2 ′ = x 2 − n U n − 1 − k x 3 x'_2=x_2-nU^{n-1-k}x_3 x 2 ′ = x 2 − n U n − 1 − k x 3 . Then
Figure 6. On the left: C n C_n C n for l = 1 l=1 l = 1 . On the right: C ~ n \widetilde{C}_n C n for l = 1 l=1 l = 1 .
∂ n x 1 = U k x 2 − n U n − 1 x 3 = U k x 2 ′ , ∂ n x 2 ′ = n U n − 1 x 4 − n U n − 1 − k U k x 4 = 0 , \partial_n x_1=U^k x_2-nU^{n-1}x_3=U^k x'_2,\qquad\partial_n x'_2=nU^{n-1}x_4-nU^{n-1-k}U^k x_4=0, ∂ n x 1 = U k x 2 − n U n − 1 x 3 = U k x 2 ′ , ∂ n x 2 ′ = n U n − 1 x 4 − n U n − 1 − k U k x 4 = 0 ,
so in the basis { x 1 , x 2 ′ , x 3 , x 4 } \{x_1,x'_2,x_3,x_4\} { x 1 , x 2 ′ , x 3 , x 4 } the differential of C n C_n C n is that of C ~ n \widetilde{C}_n C n . By direct computation using a similar diagram to Figure 5 ,
H ∗ ( C n ) ≅ ( Q [ U ] ( U k ) ) 4 ≅ H ∗ ( C ~ n ) . H_*(C_n)\cong\left(\frac{\mathbb{Q}[U]}{(U^k)}\right)^4\cong H_*(\widetilde{C}_n). H ∗ ( C n ) ≅ ( ( U k ) Q [ U ] ) 4 ≅ H ∗ ( C n ) .
If k ≥ n k\ge n k ≥ n , then U k = 0 U^k=0 U k = 0 in the ground ring, so C n C_n C n is the direct sum of two copies of the complex in the proof of Lemma 4.3 and C ~ n \widetilde{C}_n C n has zero differential; the stated homology follows from that computation. □
Lemma 4.13. Let n ≥ 2 n\ge2 n ≥ 2 and let C C C be a staircase complex. Suppose that every vertical arrow of length one is accompanied by a horizontal arrow of length at most n − 1 n-1 n − 1 at its source (left form) or at its target (right form); that is,
(1) if C C C is of the left form, k i − 1 ≤ n − 1 k_{i-1}\le n-1 k i − 1 ≤ n − 1 for every even i i i with $k_i=1;
(2) if C C C is of the right form, k i + 1 ≤ n − 1 k_{i+1}\le n-1 k i + 1 ≤ n − 1 for every odd i ≤ m − 2 i\le m-2 i ≤ m − 2 with $k_i=1.
Then C n ≅ C ~ n C_n\cong\widetilde{C}_n C n ≅ C n as complexes of Q [ U ] ( U n ) \frac{\mathbb{Q}[U]}{(U^n)} ( U n ) Q [ U ] -modules; in particular H ∗ ( C n ) ≅ H ∗ ( C ~ n ) H_*(C_n)\cong H_*(\widetilde{C}_n) H ∗ ( C n ) ≅ H ∗ ( C n ) is an isomorphism of Q [ U ] \mathbb{Q}[U] Q [ U ] -modules.
Proof. Any staircase complex can be pictorially represented as in Definition 4.5 . Using a similar argument as in the proof of Lemma 4.12 , every V k i V^{k_i} V k i with k i ≥ 2 k_i\ge2 k i ≥ 2 vanishes in C n C_n C n , so C n C_n C n and C ~ n \widetilde{C}_n C n differ only in the arrows x i → n U n − 1 x i + 1 x_i\to nU^{n-1}x_{i+1} x i → n U n − 1 x i + 1 coming from sources x i x_i x i with k i = 1 k_i=1 k i = 1 . Put ε i = 1 \varepsilon_i=1 ε i = 1 if k i = 1 k_i=1 k i = 1 and ε i = 0 \varepsilon_i=0 ε i = 0 otherwise, so that for each source x i x_i x i ,
∂ n x i = U k i − 1 x i − 1 + ε i n U n − 1 x i + 1 . \partial_n x_i=U^{k_i-1}x_{i-1}+\varepsilon_i nU^{n-1}x_{i+1}. ∂ n x i = U k i − 1 x i − 1 + ε i n U n − 1 x i + 1 .
Rather than cancelling over Q \mathbb{Q} Q (which is not U U U -equivariant), we change basis over Q [ U ] ( U n ) \frac{\mathbb{Q}[U]}{(U^n)} ( U n ) Q [ U ] .
(1) For even i i i , set y i − 1 = x i − 1 + ε i n U n − 1 − k i − 1 x i + 1 y_{i-1}=x_{i-1}+\varepsilon_i nU^{n-1-k_{i-1}}x_{i+1} y i − 1 = x i − 1 + ε i n U n − 1 − k i − 1 x i + 1 and y m = x m y_m=x_m y m = x m . This is a change of basis of the odd generators, and ∂ n x i = U k i − 1 y i − 1 \partial_n x_i=U^{k_{i-1}}y_{i-1} ∂ n x i = U k i − 1 y i − 1 . A visual representation of this change of basis is as in Figure 7 . Since the odd generators are cycles, the Q [ U ] ( U n ) \frac{\mathbb{Q}[U]}{(U^n)} ( U n ) Q [ U ] -linear map C ~ n → C n \widetilde{C}_n\to C_n C n → C n fixing x i x_i x i for i i i even and sending x i ↦ y i x_i\mapsto y_i x i ↦ y i for i i i odd is an isomorphism of chain complexes.
Figure 7. A local picture of the change of basis in the proof of Lemma 4.13 (left form) for some even i i i where k i = 1 k_i = 1 k i = 1 and k i − 1 ≤ n − 1 k_{i-1} \le n - 1 k i − 1 ≤ n − 1 . On the left: the complex C n C_n C n , with the arrow x i → n U n − 1 x i + 1 x_i \to nU^{n-1}x_{i+1} x i → n U n − 1 x i + 1 in red. On the right: the same complex in the basis where x i − 1 x_{i-1} x i − 1 is replaced by y i − 1 = x i − 1 + n U n − 1 − k i − 1 x i + 1 y_{i-1} = x_{i-1} + nU^{n-1-k_{i-1}}x_{i+1} y i − 1 = x i − 1 + n U n − 1 − k i − 1 x i + 1 ; the red arrow has been absorbed, and the picture agrees with C ~ n \widetilde{C}_n C n .
(2) Define recursively x m ′ = x m x'_m=x_m x m ′ = x m and x i ′ = x i − ε i n U n − 1 − k i + 1 x i + 2 ′ x'_i=x_i-\varepsilon_i nU^{n-1-k_{i+1}}x'_{i+2} x i ′ = x i − ε i n U n − 1 − k i + 1 x i + 2 ′ for odd i ≤ m − 2 i\le m-2 i ≤ m − 2 . By induction, ∂ n x i ′ = U k i − 1 x i − 1 \partial_n x'_i=U^{k_{i-1}}x_{i-1} ∂ n x i ′ = U k i − 1 x i − 1 : indeed ∂ n x i + 2 ′ = U k i + 1 x i + 1 \partial_n x'_{i+2}=U^{k_{i+1}}x_{i+1} ∂ n x i + 2 ′ = U k i + 1 x i + 1 , so the second term cancels ε i n U n − 1 x i + 1 \varepsilon_i nU^{n-1}x_{i+1} ε i n U n − 1 x i + 1 . Since the even generators are cycles, the map C ~ n → C n \widetilde{C}_n\to C_n C n → C n sending x i ↦ x i ′ x_i\mapsto x'_i x i ↦ x i ′ for i i i odd and fixing x i x_i x i for i i i even is an isomorphism of chain complexes.
We can readily compute H ∗ ( C n ) ≅ H ∗ ( C ~ n ) H_*(C_n)\cong H_*(\widetilde{C}_n) H ∗ ( C n ) ≅ H ∗ ( C n ) . The complex C ~ n \widetilde{C}_n C n is simply m − 1 2 \frac{m-1}{2} 2 m − 1 pairs of towers (as in Remark 4.7 ) with arrows given by the horizontal arrows, and one single tower with no arrows. For the left form, writing k s = min ( k 2 s − 1 , n ) k_s=\min(k_{2s-1},n) k s = min ( k 2 s − 1 , n ) ,
H ∗ ( C n ) ≅ H ∗ ( C ~ n ) ≅ ⨁ s = 1 m − 1 2 ( Q [ U ] ( U k s ) ⟨ x 2 s − 1 ⟩ ⊕ Q [ U ] ( U k s ) ⟨ U n − k s x 2 s ⟩ ) ⊕ Q [ U ] ( U n ) ⟨ x m ⟩ , H_*(C_n)\cong H_*(\widetilde{C}_n)\cong\bigoplus_{s=1}^{\frac{m-1}{2}}\left(\frac{\mathbb{Q}[U]}{(U^{k_s})}_{\langle x_{2s-1}\rangle}\oplus\frac{\mathbb{Q}[U]}{(U^{k_s})}_{\langle U^{n-k_s}x_{2s}\rangle}\right)\oplus\frac{\mathbb{Q}[U]}{(U^n)}_{\langle x_m\rangle}, H ∗ ( C n ) ≅ H ∗ ( C n ) ≅ s = 1 ⨁ 2 m − 1 ( ( U k s ) Q [ U ] ⟨ x 2 s − 1 ⟩ ⊕ ( U k s ) Q [ U ] ⟨ U n − k s x 2 s ⟩ ) ⊕ ( U n ) Q [ U ] ⟨ x m ⟩ ,
and similarly for the right form, with κ s = min ( k 2 s , n ) \kappa_s = \min(k_{2s},n) κ s = min ( k 2 s , n ) , generators x 2 s x_{2s} x 2 s and U n − κ s x 2 s + 1 U^{n-\kappa_s}x_{2s+1} U n − κ s x 2 s + 1 , and the free summand generated by x 1 x_1 x 1 . The isomorphisms above are Q [ U ] ( U n ) \frac{\mathbb{Q}[U]}{(U^n)} ( U n ) Q [ U ] -linear, so these are isomorphisms of Q [ U ] \mathbb{Q}[U] Q [ U ] -modules. □
To conclude the main Theorem 1.4 , we make full use of the fact that, among a myriad of nice properties, all L L L -space knots and thin knots have a master complex given by direct sums of staircases and boxes as defined above:
Theorem 4.14. Let n ≥ 2 n \ge2 n ≥ 2 , and let K ⊂ S 3 K \subset S^3 K ⊂ S 3 be either a thin knot, or an L L L -space knot such that every gap of Δ K \Delta_K Δ K is at most n − 1 n - 1 n − 1 . Then, as ungraded Q [ U ] \mathbb{Q}[U] Q [ U ] -modules,
H F K n ( K ) ≅ ( H F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; Q [ U ] ( U n ) ) . HF K_n(K) \cong\left(HFK^-(K) \mathbin{\otimes}_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right) \oplus\operatorname{Tor}^{\mathbb{Q}[U]}_1\left(HFK^-(K);\frac{\mathbb{Q}[U]}{(U^n)}\right). H F K n ( K ) ≅ ( H F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) ⊕ Tor 1 Q [ U ] ( H F K − ( K ) ; ( U n ) Q [ U ] ) .
Proof. The argument is a chain of isomorphisms given by Lemmata 4.13, 4.12, and the universal coefficient theorem. Let C = C F K U , V ( K ) C = CFK_{U,V}(K) C = C F K U , V ( K ) . By Theorem 2.12 , H F K n ( K ) ≅ H ∗ ( C n ) HFK_n(K) \cong H_*(C_n) H F K n ( K ) ≅ H ∗ ( C n ) ; this is an isomorphism of Q [ U ] \mathbb{Q}[U] Q [ U ] -modules, since Dowlin’s proof exhibits the punctured complex as a mapping cone of U V UV U V , which after setting V = n U n − 1 V = nU^{n-1} V = n U n − 1 is the cone of the non-zero-divisor n U n nU^n n U n on a free Q [ U ] \mathbb{Q}[U] Q [ U ] -complex. By Theorems 4.9 and 4.11 , C C C is homotopy equivalent over Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] to a direct sum of one staircase complex and (for thin knots) box complexes. The constructions C ↦ C n C \mapsto C_n C ↦ C n and C ↦ C ~ n C \mapsto\widetilde{C}_n C ↦ C n are given by tensoring with Q [ U , V ] \mathbb{Q}[U,V] Q [ U , V ] -modules (Remark 4.2), so they preserve homotopy equivalences and direct sums. For thin knots all k i = 1 ≤ n − 1 k_i = 1 \le n - 1 k i = 1 ≤ n − 1 and all boxes have k = l = 1 ≤ n − 1 k = l = 1 \le n - 1 k = l = 1 ≤ n − 1 ; for L L L -space knots the steps k i k_i k i are the gaps of Δ K \Delta_K Δ K , all at most n − 1 n - 1 n − 1 by hypothesis. Hence Lemmata 4.13 and 4.12 apply to every summand, and
H ∗ ( C n ) ≅ H ∗ ( C ~ n ) ≅ H ∗ ( C F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) . H_*(C_n) \cong H_*(\widetilde{C}_n) \cong H_*\left(CFK^-(K) \mathbin{\otimes}_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right). H ∗ ( C n ) ≅ H ∗ ( C n ) ≅ H ∗ ( C F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) .
using C / ( V ) ≃ C F K − ( K ) C/(V) \simeq CFK^-(K) C / ( V ) ≃ C F K − ( K ) over Q [ U ] \mathbb{Q}[U] Q [ U ] . The universal coefficient theorem says
H ∗ ( C F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) ≅ [ H ∗ ( C F K − ( K ) ) ⊗ Q [ U ] Q [ U ] ( U n ) ] ⊕ Tor 1 Q [ U ] ( H ∗ ( C F K − ( K ) ) ; Q [ U ] ( U n ) ) . H_*\left(CFK^-(K) \mathbin{\otimes}_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right) \cong\left[H_*(CFK^-(K)) \mathbin{\otimes}_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right] \oplus\operatorname{Tor}^{\mathbb{Q}[U]}_1\left(H_*(CFK^-(K));\frac{\mathbb{Q}[U]}{(U^n)}\right). H ∗ ( C F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) ≅ [ H ∗ ( C F K − ( K )) ⊗ Q [ U ] ( U n ) Q [ U ] ] ⊕ Tor 1 Q [ U ] ( H ∗ ( C F K − ( K )) ; ( U n ) Q [ U ] ) .
But
H F K − ( K ) = H ∗ ( C F K − ( K ) ) HFK^-(K) = H_*(CFK^-(K)) H F K − ( K ) = H ∗ ( C F K − ( K ))
and Lemmata 4.13 and 4.12 yield
H F K n ( K ) ≅ H ∗ ( C F K − ( K ) ⊗ Q [ U ] Q [ U ] ( U n ) ) . HFK_n(K) \cong H_*\left(CFK^-(K) \mathbin{\otimes}_{\mathbb{Q}[U]} \frac{\mathbb{Q}[U]}{(U^n)}\right). H F K n ( K ) ≅ H ∗ ( C F K − ( K ) ⊗ Q [ U ] ( U n ) Q [ U ] ) .
Piecing it all together gives the result. □
For L L L -space knots, the gap condition in Theorem 4.14 is sufficient but not necessary. The following proposition computes H F K n ( K ) HFK_n(K) H F K n ( K ) for every L L L -space knot and every n ≥ 2 n \ge2 n ≥ 2 . We write R = Q [ U ] ( U n ) R = \frac{\mathbb{Q}[U]}{(U^n)} R = ( U n ) Q [ U ] for brevity.
Let n ≥ 2 n \ge2 n ≥ 2 and let C C C be a staircase complex of the left form, with sources x 2 , x 4 , … , x m − 1 x_2,x_4,\ldots,x_{m-1} x 2 , x 4 , … , x m − 1 . For even i i i , write h i = k i − 1 h_i=k_{i-1} h i = k i − 1 and v i = k i v_i=k_i v i = k i for the lengths of the horizontal and vertical arrows with source x i x_i x i , respectively. Call an even i i i a defect if h i ≥ n h_i \ge n h i ≥ n and v i = 1 v_i=1 v i = 1 . For a defect i i i , let r ( i ) r(i) r ( i ) be the smallest even r > i r>i r > i such that r = m + 1 r=m+1 r = m + 1 or ( h r , v r ) ≠ ( n − 1 , 1 ) (h_r,v_r)\ne(n-1,1) ( h r , v r ) = ( n − 1 , 1 ) , and say the defect survives if r ( i ) = m + 1 r(i)=m+1 r ( i ) = m + 1 or h r ( i ) ≥ n h_{r(i)} \ge n h r ( i ) ≥ n . Let N n ( C ) N_n(C) N n ( C ) be the number of surviving defects. For an L L L -space knot K K K we write N n ( K ) N_n(K) N n ( K ) for N n ( C ) N_n(C) N n ( C ) , where C C C is the staircase of Theorem 4.11 . Then we have the following:
Proposition 4.15. As Q [ U ] \mathbb{Q}[U] Q [ U ] -modules,
H ∗ ( C n ) ≅ R ⊕ ⨁ i e v e n ( Q [ U ] ( U min ( h i , n ) ) ) 2 , H_*(C_n) \cong R \oplus\bigoplus_{i\ \mathrm{even}} \left(\frac{\mathbb{Q}[U]}{(U^{\min(h_i,n)})}\right)^2, H ∗ ( C n ) ≅ R ⊕ i even ⨁ ( ( U m i n ( h i , n ) ) Q [ U ] ) 2 , except that 2 N n ( C ) 2N_n(C) 2 N n ( C ) of the summands isomorphic to R R R are replaced by Q [ U ] ( U n − 1 ) \frac{\mathbb{Q}[U]}{(U^{n-1})} ( U n − 1 ) Q [ U ] . In particular,
dim Q H ∗ ( C n ) = n + 2 ∑ i e v e n min ( h i , n ) − 2 N n ( C ) , dim Q H ∗ ( C ~ n ) = n + 2 ∑ i e v e n min ( h i , n ) , \dim_{\mathbb{Q}} H_*(C_n)=n+2\sum_{i\ \mathrm{even}}\min(h_i,n)-2N_n(C), \qquad\dim_{\mathbb{Q}} H_*(\widetilde{C}_n)=n+2\sum_{i\ \mathrm{even}}\min(h_i,n), dim Q H ∗ ( C n ) = n + 2 i even ∑ min ( h i , n ) − 2 N n ( C ) , dim Q H ∗ ( C n ) = n + 2 i even ∑ min ( h i , n ) , and H ∗ ( C n ) ≅ H ∗ ( C ~ n ) H_*(C_n)\cong H_*(\widetilde{C}_n) H ∗ ( C n ) ≅ H ∗ ( C n ) if and only if N n ( C ) = 0 N_n(C)=0 N n ( C ) = 0 , in which case C n ≅ C ~ n C_n\cong\widetilde{C}_n C n ≅ C n as complexes of R R R -modules.
Proof. As in the proof of Lemma 4.13 , C n C_n C n is a two-term complex of free R R R -modules, from the sources x i x_i x i (i i i even) to the targets x j x_j x j (j j j odd), with ∂ n x i = U h i x i − 1 + ϵ i n U n − 1 x i + 1 \partial_nx_i=U^{h_i}x_{i-1}+\epsilon_i^nU^{n-1}x_{i+1} ∂ n x i = U h i x i − 1 + ϵ i n U n − 1 x i + 1 , where U h i = 0 U^{h_i}=0 U h i = 0 if h i ≥ n h_i\ge n h i ≥ n . We record it as a matrix D D D over R R R , with a column for each source and a row for each target; C ~ n \widetilde{C}_n C n has the matrix D ~ \widetilde{D} D with only the entries U h i U^{h_i} U h i in positions ( i − 1 , i ) (i-1,i) ( i − 1 , i ) .
We process i = 2 , 4 , … , m − 1 i=2,4,\ldots,m-1 i = 2 , 4 , … , m − 1 in order, by invertible R R R -linear changes of basis of the sources (column operations) and of the targets (row operations). We maintain the following invariant: when column i i i is reached, row i − 1 i-1 i − 1 contains, besides its entry in column i i i , at most one other nonzero entry, of the form c U n − 1 cU^{n-1} c U n − 1 with c ∈ Q × c\in\mathbb{Q}^{\times} c ∈ Q × , in an earlier column j j j which has no other nonzero entry. We call it the pending defect.
If h i ≤ n − 1 h_i\le n-1 h i ≤ n − 1 and there is a pending defect at ( i − 1 , j ) (i-1,j) ( i − 1 , j ) , replace x j x_j x j by x j − c U n − 1 − h i x i x_j-cU^{n-1-h_i}x_i x j − c U n − 1 − h i x i . This kills the entry ( i − 1 , j ) (i-1,j) ( i − 1 , j ) and writes − c ϵ i n U 2 n − 2 − h i -c\epsilon_i^nU^{2n-2-h_i} − c ϵ i n U 2 n − 2 − h i at ( i + 1 , j ) (i+1,j) ( i + 1 , j ) , which is nonzero exactly when h i = n − 1 h_i=n-1 h i = n − 1 and ϵ i = 1 \epsilon_i=1 ϵ i = 1 ; in that case it is the pending defect for row i + 1 i+1 i + 1 . Then, as in Lemma 4.13 , replace x i − 1 x_{i-1} x i − 1 by x i − 1 + ϵ i n U n − 1 − h i x i + 1 x_{i-1}+\epsilon_i^nU^{n-1-h_i}x_{i+1} x i − 1 + ϵ i n U n − 1 − h i x i + 1 ; since row i − 1 i-1 i − 1 now has a single entry, this kills ( i + 1 , i ) (i+1,i) ( i + 1 , i ) and changes nothing else.
If h i ≥ n h_i\ge n h i ≥ n , column i i i consists of the single entry ϵ i n U n − 1 \epsilon_i^nU^{n-1} ϵ i n U n − 1 at ( i + 1 , i ) (i+1,i) ( i + 1 , i ) . If i i i is a defect this is the pending defect for row i + 1 i+1 i + 1 . A pending defect in row i − 1 i-1 i − 1 , if any, is now final, since row i − 1 i-1 i − 1 has no other nonzero entry.
A new pending defect lands in row i + 1 i+1 i + 1 only if either h i ≥ n h_i\ge n h i ≥ n or ( h i , v i ) = ( n − 1 , 1 ) (h_i,v_i)=(n-1,1) ( h i , v i ) = ( n − 1 , 1 ) , and these are exclusive, so each row carries at most one; this verifies the invariant. A defect i i i is thus carried along the rows i + 1 , i + 3 , … i+1,i+3,\ldots i + 1 , i + 3 , … while ( h r , v r ) = ( n − 1 , 1 ) (h_r,v_r)=(n-1,1) ( h r , v r ) = ( n − 1 , 1 ) , and at the first even r > i r>i r > i with ( h r , v r ) ≠ ( n − 1 , 1 ) (h_r,v_r)\ne(n-1,1) ( h r , v r ) = ( n − 1 , 1 ) it is absorbed if h r ≤ n − 1 h_r\le n-1 h r ≤ n − 1 and becomes final if h r ≥ n h_r\ge n h r ≥ n ; if no such r ≤ m − 1 r\le m-1 r ≤ m − 1 exists, it becomes final in row m m m . So the final defects are exactly the surviving ones. (In the language of Lemma 4.8 , the column operation is the zigzag term created when the arrow x i → U h i x i − 1 x_i\to U^{h_i}x_{i-1} x i → U h i x i − 1 is cancelled; this is the term missed by a naive cancellation argument.)
All operations are invertible and R R R -linear, and the final matrix is D ~ \widetilde{D} D together with one entry c U n − 1 cU^{n-1} c U n − 1 for each surviving defect, placed in a column and a row which are zero in D ~ \widetilde{D} D . Its homology is a direct sum of: ( Q [ U ] ( U h i ) ) 2 \left(\frac{\mathbb{Q}[U]}{(U^{h_i})}\right)^2 ( ( U h i ) Q [ U ] ) 2 for each i i i with h i ≤ n − 1 h_i\le n-1 h i ≤ n − 1 , from R → U h i R R\xrightarrow{U^{h_i}}R R U h i R ; ( Q [ U ] ( U n − 1 ) ) 2 \left(\frac{\mathbb{Q}[U]}{(U^{n-1})}\right)^2 ( ( U n − 1 ) Q [ U ] ) 2 for each surviving defect, as in Lemma 4.3; and one copy of R R R for each remaining zero row or column. Comparing with D ~ \widetilde{D} D , each surviving defect replaces two copies of R R R by two copies of Q [ U ] ( U n − 1 ) \frac{\mathbb{Q}[U]}{(U^{n-1})} ( U n − 1 ) Q [ U ] , which gives the statement.
Remark 4.16. The staircase of the right form with steps k 1 , … , k m − 1 k_1,\ldots,k_{m-1} k 1 , … , k m − 1 is the dual of the staircase of the left form with steps k m − 1 , … , k 1 k_{m-1},\ldots,k_1 k m − 1 , … , k 1 , and the master complex of the mirror of a knot is the dual of its master complex. Since C n C_n C n is a two-term complex over the principal ideal ring R R R , its homology is determined by the Smith normal form of its matrix, which is unchanged by transposition. Hence Proposition 4.15 also computes H ∗ ( C n ) H_*(C_n) H ∗ ( C n ) for staircases of the right form, and in particular H F K n HFK_n H F K n of mirrors of L L L -space knots.
We illustrate Proposition 4.15 with two examples. The first is a staircase complex, not the master complex of a knot, chosen to show each of the three possibilities for a defect: it may survive, be carried to a later row, or be absorbed.
Example 4.17. Let C C C be the staircase complex of the left form with m = 9 m=9 m = 9 and steps
( k 1 , … , k 8 ) = ( 3 , 1 , 1 , 1 , 1 , 1 , 2 , 1 ) , (k_1,\ldots,k_8)=(3,1,1,1,1,1,2,1), ( k 1 , … , k 8 ) = ( 3 , 1 , 1 , 1 , 1 , 1 , 2 , 1 ) , so that the sources x 2 , x 4 , x 6 , x 8 x_2,x_4,x_6,x_8 x 2 , x 4 , x 6 , x 8 have
( h 2 , v 2 ) = ( 3 , 1 ) , ( h 4 , v 4 ) = ( 1 , 1 ) , ( h 6 , v 6 ) = ( 1 , 1 ) , ( h 8 , v 8 ) = ( 2 , 1 ) . (h_2,v_2)=(3,1),\qquad(h_4,v_4)=(1,1),\qquad(h_6,v_6)=(1,1),\qquad(h_8,v_8)=(2,1). ( h 2 , v 2 ) = ( 3 , 1 ) , ( h 4 , v 4 ) = ( 1 , 1 ) , ( h 6 , v 6 ) = ( 1 , 1 ) , ( h 8 , v 8 ) = ( 2 , 1 ) . The case n = 2 n=2 n = 2 . Here R = Q [ U ] ( U 2 ) R=\frac{\mathbb{Q}[U]}{(U^2)} R = ( U 2 ) Q [ U ] , and in C 2 C_2 C 2 ,
∂ 2 x 2 = 2 U x 3 , ∂ 2 x 4 = U x 3 + 2 U x 5 , ∂ 2 x 6 = U x 5 + 2 U x 7 , ∂ 2 x 8 = 2 U x 9 , \partial_2x_2=2Ux_3,\qquad\partial_2x_4=Ux_3+2Ux_5,\qquad\partial_2x_6=Ux_5+2Ux_7,\qquad\partial_2x_8=2Ux_9, ∂ 2 x 2 = 2 U x 3 , ∂ 2 x 4 = U x 3 + 2 U x 5 , ∂ 2 x 6 = U x 5 + 2 U x 7 , ∂ 2 x 8 = 2 U x 9 , since U 3 = U 2 = 0 U^3=U^2=0 U 3 = U 2 = 0 . With columns indexed by the sources x 2 , x 4 , x 6 , x 8 x_2,x_4,x_6,x_8 x 2 , x 4 , x 6 , x 8 and rows by the targets x 1 , x 3 , x 5 , x 7 , x 9 x_1,x_3,x_5,x_7,x_9 x 1 , x 3 , x 5 , x 7 , x 9 , the matrices D D D and D ~ \widetilde{D} D of the proof of Proposition 4.15 are
D = ( 0 0 0 0 2 U U 0 0 0 2 U U 0 0 0 2 U 0 0 0 0 2 U ) , D ~ = ( 0 0 0 0 0 U 0 0 0 0 U 0 0 0 0 0 0 0 0 0 ) . D=\begin{pmatrix}
0&0&0&0\\
2U&U&0&0\\
0&2U&U&0\\
0&0&2U&0\\
0&0&0&2U
\end{pmatrix},
\qquad
\widetilde{D}=\begin{pmatrix}
0&0&0&0\\
0&U&0&0\\
0&0&U&0\\
0&0&0&0\\
0&0&0&0
\end{pmatrix}. D = 0 2 U 0 0 0 0 U 2 U 0 0 0 0 U 2 U 0 0 0 0 0 2 U , D = 0 0 0 0 0 0 U 0 0 0 0 0 U 0 0 0 0 0 0 0 . Both x 2 x_2 x 2 and x 8 x_8 x 8 are defects. Following the proof of Proposition 4.15 , the entry 2 U x 3 2Ux_3 2 U x 3 of ∂ 2 x 2 \partial_2x_2 ∂ 2 x 2 is the pending defect in row x 3 x_3 x 3 . At x 4 x_4 x 4 we have h 4 = 1 ≤ n − 1 h_4=1\le n-1 h 4 = 1 ≤ n − 1 , so we replace x 2 x_2 x 2 by x 2 − 2 x 4 x_2-2x_4 x 2 − 2 x 4 ; then
∂ 2 ( x 2 − 2 x 4 ) = − 4 U x 5 . \partial_2(x_2-2x_4)=-4Ux_5. ∂ 2 ( x 2 − 2 x 4 ) = − 4 U x 5 . which is nonzero because ( h 4 , v 4 ) = ( n − 1 , 1 ) (h_4,v_4)=(n-1,1) ( h 4 , v 4 ) = ( n − 1 , 1 ) , so the defect is carried to row x 5 x_5 x 5 . Replacing x 3 x_3 x 3 by y 3 = x 3 + 2 x 5 y_3=x_3+2x_5 y 3 = x 3 + 2 x 5 gives ∂ 2 x 4 = U y 3 \partial_2x_4=Uy_3 ∂ 2 x 4 = U y 3 . In the same way, at x 6 x_6 x 6 we replace x 2 − 2 x 4 x_2-2x_4 x 2 − 2 x 4 by x 2 ′ = x 2 − 2 x 4 + 4 x 6 x'_2=x_2-2x_4+4x_6 x 2 ′ = x 2 − 2 x 4 + 4 x 6 , so that ∂ 2 x 2 ′ = 8 U x 7 \partial_2x'_2=8Ux_7 ∂ 2 x 2 ′ = 8 U x 7 , and y 5 = x 5 + 2 x 7 y_5=x_5+2x_7 y 5 = x 5 + 2 x 7 gives ∂ 2 x 6 = U y 5 \partial_2x_6=Uy_5 ∂ 2 x 6 = U y 5 . At x 8 x_8 x 8 we have h 8 = 2 ≥ n h_8=2\ge n h 8 = 2 ≥ n , so the entry 8 U x 7 8Ux_7 8 U x 7 cannot be cancelled: the defect of x 2 x_2 x 2 survives, with r ( 2 ) = 8 r(2)=8 r ( 2 ) = 8 . The defect of x 8 x_8 x 8 survives as well, since r ( 8 ) = m + 1 r(8)=m+1 r ( 8 ) = m + 1 . Thus N 2 ( C ) = 2 N_2(C)=2 N 2 ( C ) = 2 . In the bases { x 2 ′ , x 4 , x 6 , x 8 } \{x'_2,x_4,x_6,x_8\} { x 2 ′ , x 4 , x 6 , x 8 } and { x 1 , y 3 , y 5 , x 7 , x 9 } \{x_1,y_3,y_5,x_7,x_9\} { x 1 , y 3 , y 5 , x 7 , x 9 } , the matrix of ∂ 2 \partial_2 ∂ 2 is
( 0 0 0 0 0 U 0 0 0 0 U 0 8 U 0 0 0 0 0 0 2 U ) , \begin{pmatrix}
0&0&0&0\\
0&U&0&0\\
0&0&U&0\\
8U&0&0&0\\
0&0&0&2U
\end{pmatrix}, 0 0 0 8 U 0 0 U 0 0 0 0 0 U 0 0 0 0 0 0 2 U , which is D ~ \widetilde{D} D together with the two entries 8 U 8U 8 U and 2 U 2U 2 U coming from the surviving defects. Each nonzero entry contributes Q ⊕ Q \mathbb{Q}\oplus\mathbb{Q} Q ⊕ Q to the homology, and the zero row x 1 x_1 x 1 contributes R R R . Hence
H ∗ ( C 2 ) ≅ Q [ U ] ( U 2 ) ⊕ Q 8 , H ∗ ( C ~ 2 ) ≅ ( Q [ U ] ( U 2 ) ) 5 ⊕ Q 4 , H_*(C_2)\cong\frac{\mathbb{Q}[U]}{(U^2)}\oplus\mathbb{Q}^8,\qquad
H_*(\widetilde{C}_2)\cong\left(\frac{\mathbb{Q}[U]}{(U^2)}\right)^5\oplus\mathbb{Q}^4, H ∗ ( C 2 ) ≅ ( U 2 ) Q [ U ] ⊕ Q 8 , H ∗ ( C 2 ) ≅ ( ( U 2 ) Q [ U ] ) 5 ⊕ Q 4 , of dimensions 10 10 10 and 14 14 14 , in agreement with n + 2 ∑ min ( h i , n ) − 2 N 2 ( C ) = 2 + 2 ( 2 + 1 + 1 + 2 ) − 4 = 10 n+2\sum\min(h_i,n)-2N_2(C)=2+2(2+1+1+2)-4=10 n + 2 ∑ min ( h i , n ) − 2 N 2 ( C ) = 2 + 2 ( 2 + 1 + 1 + 2 ) − 4 = 10 .
The case n = 3 n=3 n = 3 . Here R = Q [ U ] ( U 3 ) R=\frac{\mathbb{Q}[U]}{(U^3)} R = ( U 3 ) Q [ U ] and ∂ 3 x 2 = 3 U 2 x 3 \partial_3x_2=3U^2x_3 ∂ 3 x 2 = 3 U 2 x 3 , so x 2 x_2 x 2 is still a defect, but now x 8 x_8 x 8 is not, since h 8 = 2 < n h_8=2<n h 8 = 2 < n . At x 4 x_4 x 4 we replace x 2 x_2 x 2 by x 2 − 3 U x 4 x_2-3Ux_4 x 2 − 3 U x 4 , and
∂ 3 ( x 2 − 3 U x 4 ) = 3 U 2 x 3 − 3 U ( U x 3 + 3 U 2 x 5 ) = − 9 U 3 x 5 = 0. \partial_3(x_2-3Ux_4)=3U^2x_3-3U(Ux_3+3U^2x_5)=-9U^3x_5=0. ∂ 3 ( x 2 − 3 U x 4 ) = 3 U 2 x 3 − 3 U ( U x 3 + 3 U 2 x 5 ) = − 9 U 3 x 5 = 0. The defect is absorbed, because ( h 4 , v 4 ) = ( 1 , 1 ) ≠ ( n − 1 , 1 ) (h_4,v_4)=(1,1)\ne(n-1,1) ( h 4 , v 4 ) = ( 1 , 1 ) = ( n − 1 , 1 ) ; in the notation of Proposition 4.15 , r ( 2 ) = 4 r(2)=4 r ( 2 ) = 4 and h 4 ≤ n − 1 h_4\le n-1 h 4 ≤ n − 1 . The remaining vertical arrows are absorbed as in Lemma 4.13 , so N 3 ( C ) = 0 N_3(C)=0 N 3 ( C ) = 0 , C 3 ≅ C ~ 3 C_3\cong\widetilde{C}_3 C 3 ≅ C 3 , and
H ∗ ( C 3 ) ≅ H ∗ ( C ~ 3 ) ≅ ( Q [ U ] ( U 3 ) ) 3 ⊕ ( Q [ U ] ( U 2 ) ) 2 ⊕ Q 4 , H_*(C_3)\cong H_*(\widetilde{C}_3)\cong\left(\frac{\mathbb{Q}[U]}{(U^3)}\right)^3\oplus\left(\frac{\mathbb{Q}[U]}{(U^2)}\right)^2\oplus\mathbb{Q}^4, H ∗ ( C 3 ) ≅ H ∗ ( C 3 ) ≅ ( ( U 3 ) Q [ U ] ) 3 ⊕ ( ( U 2 ) Q [ U ] ) 2 ⊕ Q 4 , which is dimension 17 17 17 .
Example 4.18. The torus knot T 5 , 7 T_{5,7} T 5 , 7 has genus 12 12 12 , and the gaps of Δ T 5 , 7 \Delta_{T_{5,7}} Δ T 5 , 7 are
( k 1 , … , k 16 ) = ( 1 , 4 , 1 , 1 , 1 , 2 , 1 , 1 , 1 , 2 , 1 , 1 , 1 , 4 , 1 ) . (k_1,\ldots,k_{16})=(1,4,1,1,1,2,1,1,1,2,1,1,1,4,1). ( k 1 , … , k 16 ) = ( 1 , 4 , 1 , 1 , 1 , 2 , 1 , 1 , 1 , 2 , 1 , 1 , 1 , 4 , 1 ) . So its complex is a staircase like that of Theorem 4.11 , which has m = 17 m=17 m = 17 , and its sources x 2 , x 4 , … , x 16 x_2,x_4,\ldots,x_{16} x 2 , x 4 , … , x 16 have
( h i ) = ( 1 , 1 , 1 , 1 , 2 , 1 , 4 ) , ( v i ) = ( 4 , 1 , 2 , 1 , 1 , 1 , 1 ) . (h_i)=(1,1,1,1,2,1,4),\qquad(v_i)=(4,1,2,1,1,1,1). ( h i ) = ( 1 , 1 , 1 , 1 , 2 , 1 , 4 ) , ( v i ) = ( 4 , 1 , 2 , 1 , 1 , 1 , 1 ) .
Take n = 2 n = 2 n = 2 . The defects are x 12 x_{12} x 12 , with ( h 12 , v 12 ) = ( 2 , 1 ) (h_{12},v_{12}) = (2,1) ( h 12 , v 12 ) = ( 2 , 1 ) , and x 16 x_{16} x 16 , with ( h 16 , v 16 ) = ( 4 , 1 ) (h_{16},v_{16}) = (4,1) ( h 16 , v 16 ) = ( 4 , 1 ) . The defect of x 12 x_{12} x 12 is carried through x 14 x_{14} x 14 , since ( h 14 , v 14 ) = ( 1 , 1 ) = ( n − 1 , 1 ) (h_{14},v_{14}) = (1,1) = (n-1,1) ( h 14 , v 14 ) = ( 1 , 1 ) = ( n − 1 , 1 ) , and survives at x 16 x_{16} x 16 , since h 16 ≥ n h_{16} \ge n h 16 ≥ n ; the defect of x 16 x_{16} x 16 survives since r ( 16 ) = m + 1 r(16) = m+1 r ( 16 ) = m + 1 . So N 2 ( T 5 , 7 ) = 2 N_2(T_{5,7}) = 2 N 2 ( T 5 , 7 ) = 2 , and by Proposition 4.15,
HFK 2 ( T 5 , 7 ) ≅ Q [ U ] ( U 2 ) ⊕ Q 16 , \operatorname{HFK}_2(T_{5,7}) \cong\frac{\mathbb{Q}[U]}{(U^2)} \oplus\mathbb{Q}^{16}, HFK 2 ( T 5 , 7 ) ≅ ( U 2 ) Q [ U ] ⊕ Q 16 ,
which has dimension 18, while the right-hand side of Theorem 4.14 has dimension 22. For n = 3 n = 3 n = 3 only the defect of x 16 x_{16} x 16 remains, so N 3 ( T 5 , 7 ) = 1 N_3(T_{5,7}) = 1 N 3 ( T 5 , 7 ) = 1 and the dimensions are 23 and 25; for n = 4 n = 4 n = 4 again N 4 ( T 5 , 7 ) = 1 N_4(T_{5,7}) = 1 N 4 ( T 5 , 7 ) = 1 , with dimensions 26 and 28. For n ≥ 5 n \ge5 n ≥ 5 there are no defects, in accordance with Corollary 1.6.
Remark 4.19. For a thin knot K K K with b b b boxes as in Theorem 4.9, HFK ^ − ( K ) ≅ Q [ U ] ⊕ Q ∣ τ ( K ) ∣ + 2 b \widehat{\operatorname{HFK}}^{-}(K) \cong\mathbb{Q}[U] \oplus\mathbb{Q}^{|\tau(K)|+2b} HFK − ( K ) ≅ Q [ U ] ⊕ Q ∣ τ ( K ) ∣ + 2 b , and rk HFK ^ ( K ) = 2 ∣ τ ( K ) ∣ + 1 + 4 b = det ( K ) \operatorname{rk}\widehat{\operatorname{HFK}}(K) = 2|\tau(K)| + 1 + 4b = \det(K) rk HFK ( K ) = 2∣ τ ( K ) ∣ + 1 + 4 b = det ( K ) , since HFK ^ ( K ) \widehat{\operatorname{HFK}}(K) HFK ( K ) is supported in a single δ \delta δ -grading. By Theorem 4.14, for n ≥ 2 n \ge2 n ≥ 2 ,
HFK n ( K ) ≅ Q [ U ] ( U n ) ⊕ Q det ( K ) − 1 2 ⊕ Q det ( K ) − 1 2 = Q [ U ] ( U n ) ⊕ Q det ( K ) − 1 , \operatorname{HFK}_n(K) \cong\frac{\mathbb{Q}[U]}{(U^n)} \oplus\mathbb{Q}^{\frac{\det(K)-1}{2}} \oplus\mathbb{Q}^{\frac{\det(K)-1}{2}} = \frac{\mathbb{Q}[U]}{(U^n)} \oplus\mathbb{Q}^{\det(K)-1}, HFK n ( K ) ≅ ( U n ) Q [ U ] ⊕ Q 2 d e t ( K ) − 1 ⊕ Q 2 d e t ( K ) − 1 = ( U n ) Q [ U ] ⊕ Q d e t ( K ) − 1 ,
which proves the second part of Corollary 1.5. For 2-bridge knots and n = 2 n = 2 n = 2 , this agrees with Dowlin’s computation dim Q HFK 2 ( K ) = det ( K ) + 1 \dim_{\mathbb{Q}} \operatorname{HFK}_2(K) = \det(K) + 1 dim Q HFK 2 ( K ) = det ( K ) + 1 [1 Lemma 5.4] .
Proof of Corollary 1.6. For T p , q T_{p,q} T p , q , let S ⊂ Z ≥ 0 S \subset\mathbb{Z}_{\ge0} S ⊂ Z ≥ 0 be the semigroup generated by p p p and q q q . The identity
1 − t p q ( 1 − t p ) ( 1 − t q ) = ∑ s ∈ S t s \frac{1-t^{pq}}{(1-t^p)(1-t^q)} = \sum_{s \in S} t^s ( 1 − t p ) ( 1 − t q ) 1 − t pq = s ∈ S ∑ t s
gives Δ T p , q ( t ) = ( 1 − t ) ∑ s ∈ S t s \Delta_{T_{p,q}}(t) = (1-t)\sum_{s \in S} t^s Δ T p , q ( t ) = ( 1 − t ) ∑ s ∈ S t s , normalized to have lowest degree 0. So the exponents of Δ T p , q \Delta_{T_{p,q}} Δ T p , q are the s ∈ S s \in S s ∈ S with s − 1 ∉ S s-1 \notin S s − 1 ∈ / S and the s + 1 ∉ S s+1 \notin S s + 1 ∈ / S with s ∈ S s \in S s ∈ S , and the gaps are the lengths of maximal sequences of consecutive elements of S S S and of consecutive non-elements of S S S . A sequence of non-elements has length at most p − 1 p-1 p − 1 , since s ∈ S s \in S s ∈ S implies s + p ∈ S s+p \in S s + p ∈ S , and the sequence { 1 , … , p − 1 } \{1,\ldots,p-1\} { 1 , … , p − 1 } attains this. Since Δ \Delta Δ is symmetric, its sequence of gaps is a palindrome of even length, so the sequences of elements are the sequences of non-elements in reverse order. Hence the largest gap is length p − 1 p-1 p − 1 .
If n ≥ p n \ge p n ≥ p , every gap is at most length n − 1 n-1 n − 1 , and Theorem 4.14 applies. If 2 ≤ n ≤ p − 1 2 \le n \le p-1 2 ≤ n ≤ p − 1 , the lowest terms of Δ \Delta Δ are 1 − t + t p 1-t+t^p 1 − t + t p , so the first two gaps are 1 and p − 1 p-1 p − 1 , and by symmetry so are the last two. In its staircase of the shape in Theorem 4.11, the last source x m − 1 x_{m-1} x m − 1 therefore has ( h m − 1 , v m − 1 ) = ( p − 1 , 1 ) (h_{m-1},v_{m-1}) = (p-1,1) ( h m − 1 , v m − 1 ) = ( p − 1 , 1 ) with p − 1 ≥ n p-1 \ge n p − 1 ≥ n ; it is a defect with r ( m − 1 ) = m + 1 r(m-1) = m+1 r ( m − 1 ) = m + 1 , so it survives and N n ( T p , q ) ≥ 1 N_n(T_{p,q}) \ge1 N n ( T p , q ) ≥ 1 . By Proposition 4.15, dim Q HFK n ( T p , q ) \dim_{\mathbb{Q}} \operatorname{HFK}_n(T_{p,q}) dim Q HFK n ( T p , q ) is smaller than the dimension of the right-hand side of Theorem 4.14. The case of T 3 , 4 T_{3,4} T 3 , 4 is Example 3.5. □
The same argument shows more generally that, since the top gap of the Alexander polynomial of a nontrivial L L L -space knot is 1 [7 ] , the isomorphism of Theorem 4.14 fails for every nontrivial L L L -space knot whose second gap is at least n n n .
References
DEPARTMENT OF MATHEMATICS, LOUISIANA STATE UNIVERSITY, LA 70803
Email address: trwells22@lsu.edu