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Bott-Cattaneo-Rossi invariants for long knots in asymptotic homology 3\mathbb{R}^{3}

David Leturcq111Institut Fourier, Université-Grenoble-Alpes
Abstract

In this article, we express the Alexander polynomial of null-homologous long knots in punctured rational homology 33-spheres in terms of integrals over configuration spaces. To get such an expression, we use a previously established formula, which gives generalized Bott-Cattaneo-Rossi invariants in terms of the Alexander polynomial and vice versa, and we relate these Bott-Cattaneo-Rossi invariants to the perturbative expansion of Chern-Simons theory.

Keywords: Knot theory, Configuration spaces, Alexander polynomial, Perturbative expansion of the Chern-Simons theory.

MSC: 55R80, 57K10, 57K14, 57K16.

1 Introduction

Knot invariants defined as combinations of integrals over configuration spaces or, equivalently, as combinations of algebraic counts of diagrams, emerged after the seminal work of Witten [Wit89] on the perturbative expansion of the Chern-Simons theory. Knot invariants defined from spatial configurations of unitrivalent graphs were formally defined by Guadagnini, Martellini and Mintchev [GMM90], Bar-Natan [BN95b], Altschüler and Freidel [AF97], Bott and Taubes [BT94], and others, for knots in 3\mathbb{R}^{3}. These invariants can be unified in an invariant 𝒵=(𝒵k)k\mathcal{Z}=(\mathcal{Z}_{k})_{k\in\mathbb{N}} defined by Altschüler and Freidel in [AF97] for knots in 3\mathbb{R}^{3}, and called the perturbative expansion of the Chern-Simons theory. The invariant 𝒵\mathcal{Z} takes its values in a vector space 𝒜=k𝒜k\mathcal{A}=\prod\limits_{k\in\mathbb{N}}\mathcal{A}_{k}, spanned by classes of Jacobi unitrivalent diagrams, precisely described in Definition 2.3. Altschüler and Freidel proved that 𝒵\mathcal{Z} is a universal Vassiliev invariant for knots in 3\mathbb{R}^{3}. The Kontsevich integral 𝒵K=(𝒵kK)k\mathcal{Z}^{K}=(\mathcal{Z}_{k}^{K})_{k\in\mathbb{N}} described by Bar-Natan [BN95a], and defined using integrals over spaces of planar configurations is another universal Vassiliev invariant. An article of Lescop [Les02] connects 𝒵\mathcal{Z} to 𝒵K\mathcal{Z}^{K}, up to the Bott and Taubes anomaly α\alpha, and implies that the two invariants are equivalent.

In [BNG96], Bar-Natan and Garoufalidis defined a linear form wCw_{C} on k𝒜k\bigoplus_{k\in\mathbb{N}}\mathcal{A}_{k} (see Definition 2.6), called the Conway weight system, and they expressed the Alexander polynomial Δψ\Delta_{\psi} for knots in 3\mathbb{R}^{3} as

Δψ(eh)=2sinh(h2)hk0(wC𝒵kK)(ψ)hk.\Delta_{\psi}(e^{h})=\frac{2\sinh\left(\frac{h}{2}\right)}{h}\sum\limits_{k\geq 0}(w_{C}\circ\mathcal{Z}^{K}_{k})(\psi)h^{k}.

Both hands of the formulas are also well-defined for the long knots222See Section 2.1 for a definition of long knots, in a wider setting. in 3\mathbb{R}^{3}, and

Δψ(eh)=k0(wC𝒵kK)(ψ)hk.\Delta_{\psi}(e^{h})=\sum\limits_{k\geq 0}(w_{C}\circ\mathcal{Z}^{K}_{k})(\psi)h^{k}.

The perturbative expansion of Chern-Simons theory (𝒵k)k(\mathcal{Z}_{k})_{k\in\mathbb{N}} extends to long knots in rational asymptotic homology333These spaces are defined in Section 2.1. 3\mathbb{R}^{3}, as in [Les15, Les20]. In this article, we prove the following result (Corollary 2.17).

Theorem.

For any null-homologous long knot ψ\psi of an asymptotic rational homology 3\mathbb{R}^{3},

Δψ(eh)=k0(wC𝒵k)(ψ)hk.\Delta_{\psi}(e^{h})=\sum\limits_{k\geq 0}(w_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}.

In Proposition 2.18, we use the relation of Lescop [Les02] between 𝒵\mathcal{Z} and 𝒵K\mathcal{Z}^{K} to notice that our theorem in terms of the perturbative expansion of the Chern-Simons theory is equivalent to the formula of Bar-Natan and Garoufalidis in terms of the Kontsevich integral for long knots of 3\mathbb{R}^{3}. The proof of our more general theorem relies on completely different methods, even for long knots of 3\mathbb{R}^{3}, and our theorem holds in the wider setting of null-homologous long knots in asymptotic rational homology 3\mathbb{R}^{3}. Our proof uses the direct computations of integrals over configuration spaces of our article [Let20]. For codimension two null-homologous long knots of any asymptotic homology444The definition given for n=1n=1 in Section 2.1 easily adapts to any n1n\geq 1. n+2\mathbb{R}^{n+2}, these computations allowed us to express the generalized Bott-Cattaneo-Rossi (BCR for short) invariants (ZBCR,k)k{0,1}(Z_{BCR,k})_{k\in\mathbb{N}\setminus\{0,1\}}, which we defined in [Let19], in terms of the Reidemeister torsion (or Alexander polynomials).

These generalized BCR invariants generalize invariants defined by Bott [Bot96], and Cattaneo and Rossi [CR05] for (codimension 22) long knots in odd-dimensional Euclidean spaces n+2\mathbb{R}^{n+2} with n+25n+2\geq 5. The BCR invariant ZBCR,kZ_{BCR,k} is a combination of integrals over configuration spaces associated with some diagrams with 2k2k vertices of two kinds and 2k2k edges of two kinds, called BCR diagrams. In [Let19], given a parallelized asymptotic homology n+2\mathbb{R}^{n+2} (M,τ)({{{M}^{\circ}}},\tau), we defined some particular forms on the two-point configuration spaces of n\mathbb{R}^{n} or of M{{{M}^{\circ}}}, called propagators of (M,τ)({{{M}^{\circ}}},\tau). The generalized BCR invariant ZBCR,kZ_{BCR,k} maps the data of a parallelized asymptotic homology n+2\mathbb{R}^{n+2} (M,τ)({{{M}^{\circ}}},\tau), a long knot ψ\psi, and a family of propagators FF of (M,τ)({{{M}^{\circ}}},\tau) to a real number. In [Let19], we proved that this number depends only of the diffeomorphism class of (M,ψ)({{{M}^{\circ}}},\psi) when n3n\geq 3. For n=1n=1, the definition of [Let19] still makes sense, but ZBCR,kZ_{BCR,k} might depend on the choice of the parallelization or of the propagators, and might not be an invariant. In this article, we prove the formula

ZBCR,k(ψ)=(wC𝒵k)(ψ),Z_{BCR,k}(\psi)=-\left(w^{\prime}_{C}\circ\mathcal{Z}_{k}\right)(\psi), (1)

for any long knot ψ\psi of a rational asymptotic homology 3\mathbb{R}^{3} and for the weight system wCw^{\prime}_{C} defined in Lemma 2.8, where the invariant ZBCR,kZ_{BCR,k} can be computed with any set of propagators. In particular, Formula 1 and the results of [Les20] on the perturbative expansion of Chern-Simons theory imply that for any long knot ψ\psi of an asymptotic homology 3\mathbb{R}^{3}, the number ZBCR,k(ψ)Z_{BCR,k}(\psi) does not depend on the choice of the propagators or of the parallelization, and that it is invariant under ambient diffeomorphism : this is Corollary 2.15. The proof of Formula 1 only relies on combinatorics of BCR diagrams and Jacobi unitrivalent diagrams.

The weight system wCw^{\prime}_{C} coincides with the Conway weight system wCw_{C} defined by Bar-Natan and Garoufalidis in [BNG96] on the non-empty connected unitrivalent diagrams. It vanishes on trivalent diagrams, and on non-trivial products of diagrams. It satisfies the formula

k0(wC𝒵k)(ψ)hk=exp(k1(wC𝒵k)(ψ)hk),\sum\limits_{k\geq 0}(w_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}=\exp\left(\sum\limits_{k\geq 1}(w^{\prime}_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}\right), (2)

for any long knot of an asymptotic rational homology 3\mathbb{R}^{3}, as noticed in Theorem 2.13.

For any n1n\geq 1, our flexible definition of [Let19] for the BCR invariants allows us to compute them with arbitrary propagators. In [Let20], we present an explicit computation based on so-called admissible propagators, which yields exact formulas for ZBCR,k(ψ)Z_{BCR,k}(\psi) in terms of Alexander polynomials. For a null-homologous long knot of an asymptotic rational homology 3\mathbb{R}^{3}, these formulas reduce to

Δψ(eh)=exp(k2ZBCR,k(ψ)hk).\Delta_{\psi}(e^{h})=\exp\left(-\sum\limits_{k\geq 2}Z_{BCR,k}(\psi)h^{k}\right). (3)

Formulas 1, 2 and 3 imply the theorem stated in the beginning of this introduction.

In Section 2, we review the definitions of the two invariants 𝒵k\mathcal{Z}_{k} and ZBCR,kZ_{BCR,k} of this article, and we state the forementioned results in Theorems 2.14 (Formula 1 above) and 2.16 (Formula 3 above). Section 3 is devoted to the proof of Theorem 2.14.

I thank my advisor, Christine Lescop, for her help in the redaction of this article.

2 Bott-Cattaneo-Rossi invariants and perturbative expansion of the Chern-Simons theory

2.1 Long knots in asymptotic homology 3\mathbb{R}^{3}

Let M{M} be a smooth oriented compact connected 33-manifold with the rational homology of 𝕊3\mathbb{S}^{3}. Fix a point \infty in M{M} and a closed ball B(M)B_{\infty}(M) around \infty, and set M=M{}{{{M}^{\circ}}}={M}\setminus\{\infty\}. Identify the punctured ball B(M)=B(M){}B_{\infty}^{\circ}(M)=B_{\infty}(M)\setminus\{\infty\} of M{{{M}^{\circ}}} with the complement B(){B_{\infty}()^{\circ}} of the open unit ball in 3\mathbb{R}^{3}, and let B(M)B(M) denote the closure of MB(){{{M}^{\circ}}}\setminus{B_{\infty}()^{\circ}}. The manifold M{{{M}^{\circ}}} together with the decomposition M=B(M)B(){{{M}^{\circ}}}=B(M)\cup{B_{\infty}()^{\circ}} is called an asymptotic rational homology 3\mathbb{R}^{3}.

A parallelization of an asymptotic rational homology 3\mathbb{R}^{3} is a bundle isomorphism τ:M×3TM\tau\colon{{{M}^{\circ}}}\times\mathbb{R}^{3}\rightarrow T{{{M}^{\circ}}} that coincides with the canonical trivialization of T3T\mathbb{R}^{3} on B()×3{B_{\infty}()^{\circ}}\times\mathbb{R}^{3}. Such a parallelization always exists : see for example [Les20, Proposition 5.5].

A long knot in an asymptotic rational homology 3\mathbb{R}^{3} is a smooth embedding ψ:M\psi\colon\mathbb{R}\hookrightarrow{{{M}^{\circ}}} such that, for any xx\in\mathbb{R},

  • if x[1,1]x\in[-1,1], ψ(x)B(M)\psi(x)\in B(M),

  • if x[1,1]x\not\in[-1,1], ψ(x)=(0,0,x)B()3\psi(x)=(0,0,x)\in{B_{\infty}()^{\circ}}\subset\mathbb{R}^{3}.

In the following, we let (M,τ)({{{M}^{\circ}}},\tau) be a fixed parallelized rational asymptotic homology 3\mathbb{R}^{3}.

2.2 BCR diagrams

We recall the definition of BCR diagrams, as introduced in [Let19, Section 2.2]. In all the following, if kk is a positive integer, k¯\underline{k} denotes the set {1,,k}\{1,\ldots,k\}.

Definition 2.1.

A BCR diagram is a non-empty oriented connected graph Γ\Gamma, defined by a set V(Γ)V(\Gamma) of vertices, decomposed into V(Γ)=Vi(Γ)Ve(Γ)V(\Gamma)=V_{i}(\Gamma)\sqcup V_{e}(\Gamma), and a set E(Γ)E(\Gamma) of ordered pairs of distinct vertices, decomposed into E(Γ)=Ei(Γ)Ee(Γ)E(\Gamma)=E_{i}(\Gamma)\sqcup E_{e}(\Gamma), whose elements are called edges555Note that this implies that our graphs have neither loops nor multiple edges with the same orientation., where the elements of Vi(Γ)V_{i}(\Gamma) are called internal vertices, those of Ve(Γ)V_{e}(\Gamma) external vertices, those of Ei(Γ)E_{i}(\Gamma) internal edges, and those of Ee(Γ)E_{e}(\Gamma) external edges, and such that, for any vertex vv of Γ\Gamma, one of the five following properties holds:

  1. 1.

    vv is external, with two incoming external edges and one outgoing external edge, and exactly one of the incoming edges comes from a univalent vertex.

  2. 2.

    vv is internal and trivalent, with one incoming internal edge, one outgoing internal edge, and one incoming external edge, which comes from a univalent vertex.

  3. 3.

    vv is internal and univalent, with one outgoing external edge.

  4. 4.

    vv is internal and bivalent, with one incoming external edge and one outgoing internal edge.

  5. 5.

    vv is internal and bivalent, with one incoming internal edge and one outgoing external edge.

In the following, internal edges are depicted by solid arrows, external edges by dashed arrows, internal vertices by black dots, and external vertices by white dots, as in Figure 1, where the five behaviors of Definition 2.1 appear.

Figure 1: An example of a BCR diagram of degree 6

Definition 2.1 implies that any BCR diagram consists of one cycle with some legs attached to it, where legs are external edges that come from a (necessarily internal) univalent vertex, and where the graph is a cyclic sequence of pieces as in Figure 2 with as many pieces of the first type than of the second type. In particular, a BCR diagram has an even number of vertices, and this number is also the number of its edges.

Figure 2:

The degree of a BCR diagram is the integer deg(Γ)=12Card(V(Γ))\deg(\Gamma)=\frac{1}{2}{\mathrm{Card}}(V(\Gamma)). A numbering666In this article, numberings are valued in 3k¯\underline{3k} rather than in 2k¯\underline{2k} as in [Let19] or [Let20], and only the external edges are numbered. of a degree kk BCR diagram is an injection σ:Ee(Γ)3k¯\sigma\colon E_{e}(\Gamma)\hookrightarrow\underline{3k}.

2.3 Jacobi unitrivalent diagrams

In this section, we recall the definition of unitrivalent diagrams, widely used in the theory of Vassiliev invariants.

Definition 2.2.

A Jacobi diagram is a graph Γ\Gamma, given by a set V(Γ)V(\Gamma) of vertices, decomposed into V(Γ)=Vi(Γ)Ve(Γ)V(\Gamma)=V_{i}(\Gamma)\sqcup V_{e}(\Gamma), a set E(Γ)E(\Gamma) of unordered pairs of distinct vertices called edges, such that the vertices of Ve(Γ)V_{e}(\Gamma) are trivalent, the vertices of Vi(Γ)V_{i}(\Gamma) are univalent, and the set Vi(Γ)V_{i}(\Gamma) of univalent vertices is totally ordered.

The degree deg(Γ)\deg(\Gamma) of such a diagram Γ\Gamma is half its number of vertices. A numbering of a degree kk Jacobi diagram is an injection j:E(Γ)3k¯j\colon E(\Gamma)\hookrightarrow\underline{3k}.

An orientation of a trivalent vertex vv is the choice of a cyclic order on the three half-edges adjacent to vv. A vertex-orientation of a Jacobi diagram Γ\Gamma is the choice of an orientation of any trivalent vertex. A vertex-oriented Jacobi diagram is a Jacobi diagram together with a vertex orientation.

An edge-orientation of a Jacobi diagram is the choice of an orientation for each edge. An edge-oriented Jacobi diagram is a Jacobi diagram with a given edge-orientation. A bioriented Jacobi diagram is a Jacobi diagram with both a vertex-orientation and an edge-orientation.

In the following, Jacobi diagrams will be depicted by a planar immersion of Γ\Gamma\cup\mathbb{R}, where \mathbb{R} is a plain vertical line, on which the univalent vertices of Γ\Gamma lie, and the edges of Γ\Gamma are dashed lines. The order on the univalent vertices is given by the vertical direction on the plain vertical line \mathbb{R} from bottom to top. When dealing with vertex-oriented Jacobi diagrams, the vertex-orientation will be given by the counterclockwise order in the plane. An example of Jacobi diagram is given in Figure 3.

Figure 3: An example of a degree 77 Jacobi diagram.
Definition 2.3.

Let kk be a nonnegative integer. The space 𝒜k{\mathcal{A}_{k}} is the real vector space spanned by the degree kk vertex-oriented Jacobi diagrams up to the equivalence relation spanned by the three following rules:

  • AS relation: if Γ¯\overline{\Gamma} is obtained from Γ\Gamma by reversing the orientation of one trivalent vertex, [Γ¯]=[Γ][\overline{\Gamma}]=-[\Gamma],

  • IHX relation: if Γ1\Gamma_{1}, Γ2\Gamma_{2} and Γ3\Gamma_{3} can be represented by planar immersions that coincide outside a disk and are as in the second row of Figure 4 inside this disk, [Γ1]+[Γ2]+[Γ3]=0[\Gamma_{1}]+[\Gamma_{2}]+[\Gamma_{3}]=0.

  • STU relation: if Γ\Gamma, Γ1\Gamma_{1} and Γ2\Gamma_{2} can be represented by planar immersions that coincide outside a disk and are as in the third row of Figure 4 inside this disk, [Γ]=[Γ1][Γ2][\Gamma]=[\Gamma_{1}]-[\Gamma_{2}].

We also denote the vector subspace of 𝒜k{\mathcal{A}_{k}} generated by the classes of diagrams such that any connected component contains a univalent vertex by 𝒜kˇ{\check{\mathcal{A}_{k}}}. Set 𝒜=k0𝒜k\mathcal{A}=\prod\limits_{k\geq 0}{\mathcal{A}_{k}} and 𝒜ˇ=k0𝒜kˇ\mathcal{\check{A}}=\prod\limits_{k\geq 0}{\check{\mathcal{A}_{k}}}. Note that 𝒜0=𝒜ˇ0=.[]\mathcal{A}_{0}=\mathcal{\check{A}}_{0}=\mathbb{R}.[\emptyset], where [][\emptyset] is the class of the empty diagram.

AS: = -
IHX : Γ1\Gamma_{1}+ Γ2\Gamma_{2}+ Γ3\Gamma_{3}= 0
STU: Γ\Gamma= Γ1\Gamma_{1}- Γ2\Gamma_{2}

Figure 4: The three relations of Definition 2.3.
Definition 2.4.

The product of two Jacobi diagrams Γ1\Gamma_{1} and Γ2\Gamma_{2} is the Jacobi diagram Γ\Gamma such that

  • the set of univalent vertices of Γ\Gamma is Vi(Γ)=Vi(Γ1)Vi(Γ2)V_{i}(\Gamma)=V_{i}(\Gamma_{1})\sqcup V_{i}(\Gamma_{2}),

  • the set of trivalent vertices of Γ\Gamma is Ve(Γ)=Ve(Γ1)Ve(Γ2)V_{e}(\Gamma)=V_{e}(\Gamma_{1})\sqcup V_{e}(\Gamma_{2}),

  • the set of edges of Γ\Gamma is E(Γ)=E(Γ1)E(Γ2)E(\Gamma)=E(\Gamma_{1})\sqcup E(\Gamma_{2}),

  • the order on Vi(Γ)V_{i}(\Gamma) is the unique order compatible with the injections (Vi(Γj)Vi(Γ))j=1,2\big{(}V_{i}(\Gamma_{j})\hookrightarrow V_{i}(\Gamma)\big{)}_{j=1,2} such that any element of Vi(Γ1)V_{i}(\Gamma_{1}) is before any element of Vi(Γ2)V_{i}(\Gamma_{2}).

Note that the data of vertex-orientations (resp. edge-orientations) for Γ1\Gamma_{1} and Γ2\Gamma_{2} induce a natural vertex-orientation (resp. edge-orientation) for their product Γ\Gamma.

The product of Jacobi diagrams is compatible with the relations of Definition 2.3. Bar-Natan proved in [BN95a, Theorem 7] that the induced graded algebra structure on k𝒜k\prod\limits_{k\in\mathbb{N}}\mathcal{A}_{k} is commutative.777Bar-Natan’s theorem proves that k𝒜k\prod\limits_{k\in\mathbb{N}}\mathcal{A}_{k} is a commutative and cocommutative Hopf algebra, for a given coproduct, but we do not use the coproduct in this article. This allows us to define the associated exponential map exp:k𝒜kk𝒜k\exp\colon\prod\limits_{k\in\mathbb{N}}\mathcal{A}_{k}\rightarrow\prod\limits_{k\in\mathbb{N}}\mathcal{A}_{k}.

2.4 The Conway weight system

Let us first recall the definition of the Conway weight system of [BNG96, Section 3.1].

Definition 2.5.

Let Γ\Gamma be a Jacobi diagram with only univalent vertices (such a diagram is called a chord diagram). Use the edges of Γ\Gamma to do the surgeries on the line \mathbb{R} as in Figure 5. The obtained manifold is the disjoint union of one line and cc circles. The Conway weight system wCw_{C} is defined as

wC(Γ)={1 if c=0,0otherwise.w_{C}(\Gamma)=\begin{cases}1&\text{ if $c=0$,}\\ 0&\text{otherwise.}\end{cases}

Figure 5: Surgeries involved in the definition of wCw_{C}
c=1c=1, wC(Γa)=0w_{C}(\Gamma_{a})=0Γa\Gamma_{a}
c=0c=0, wC(Γb)=1w_{C}(\Gamma_{b})=1Γb\Gamma_{b}
Figure 6: Computation of wC(Γ)w_{C}(\Gamma) for two chord diagrams.

In [BNG96], Bar-Natan and Garoufalidis proved that this definition determines a linear form wC:k𝒜kˇw_{C}\colon\bigoplus\limits_{k\in\mathbb{N}}{\check{\mathcal{A}_{k}}}\rightarrow\mathbb{R}. Set wC(Γ)=0w_{C}(\Gamma)=0 for diagrams with at least one component without univalent vertices. The form wCw_{C} naturally extends to wC:k𝒜kw_{C}\colon\bigoplus\limits_{k\in\mathbb{N}}{\mathcal{A}_{k}}\rightarrow\mathbb{R} by sending diagrams with a non-empty trivalent888A trivalent graph is a graph with only trivalent vertices. connected component to zero. Chmutov [Chm98, p. 9] proved that wCw_{C} is determined by the following properties.

Lemma 2.6.

The Conway weight system wCw_{C} is the unique linear form wC:k𝒜kw_{C}\colon\bigoplus\limits_{k\in\mathbb{N}}{\mathcal{A}_{k}}\rightarrow\mathbb{R} such that

  • wCw_{C} vanishes on 𝒜1\mathcal{A}_{1} and maps [][\emptyset] to 11,

  • for any integer k2k\geq 2, if Γk\Gamma_{k} denotes the diagram depicted in Figure 7, wC([Γk])=1(1)kw_{C}([\Gamma_{k}])=-1-(-1)^{k},

  • if the number of trivalent vertices of Γ\Gamma is greater than its degree, then wC([Γ])=0w_{C}([\Gamma])=0,

  • if Γ\Gamma is the product of two diagrams Γ1\Gamma_{1} and Γ2\Gamma_{2}, then wC([Γ])=wC([Γ1])wC([Γ2])w_{C}([\Gamma])=w_{C}([\Gamma_{1}])w_{C}([\Gamma_{2}]).

In particular, wCw_{C} vanishes on odd-degree diagrams.

Γk\Gamma_{k}
Figure 7: The degree kk Jacobi diagram Γk\Gamma_{k}

The following result directly follows from [Les20, Corollary 6.36].

Lemma 2.7.

For any k1k\geq 1, let

  • 𝒫k\mathcal{P}_{k} denote the subspace of 𝒜kˇ{\check{\mathcal{A}_{k}}} spanned by the classes of connected diagrams with at least one univalent vertex,

  • 𝒩k{\mathcal{N}_{k}} denote the subspace of 𝒜kˇ{\check{\mathcal{A}_{k}}} spanned by the classes of non-trivial products, which are products of two non-empty diagrams,

  • 𝒯k{\mathcal{T}_{k}} denote the subspace of 𝒜k{\mathcal{A}_{k}} spanned by the classes of degree kk diagrams with at least one trivalent connected component,

and set 𝒫0=𝒯0={0}\mathcal{P}_{0}=\mathcal{T}_{0}=\{0\} and 𝒩0=.[]\mathcal{N}_{0}=\mathbb{R}.[\emptyset]. For any k0k\geq 0, the space 𝒜k{\mathcal{A}_{k}} splits into 𝒜k=𝒫k𝒩k𝒯k{\mathcal{A}_{k}}=\mathcal{P}_{k}\oplus{\mathcal{N}_{k}}\oplus{\mathcal{T}_{k}}. This yields a natural projection pc:k0𝒜kk0𝒫kp^{c}\colon\bigoplus\limits_{k\geq 0}{\mathcal{A}_{k}}\rightarrow\bigoplus\limits_{k\geq 0}\mathcal{P}_{k}.

Define the logarithmic Conway weight system wCw^{\prime}_{C} as wC=wCpcw^{\prime}_{C}=w_{C}\circ p^{c}. It is characterized as follows.

Lemma 2.8.

The map wCw^{\prime}_{C} is the unique linear form wC:k𝒜kw^{\prime}_{C}\colon\bigoplus\limits_{k\in\mathbb{N}}{\mathcal{A}_{k}}\rightarrow\mathbb{R} such that

  • wCw^{\prime}_{C} vanishes on 𝒜0𝒜1\mathcal{A}_{0}\oplus\mathcal{A}_{1},

  • for any k2k\geq 2, wC([Γk])=1(1)kw^{\prime}_{C}([\Gamma_{k}])=-1-(-1)^{k},

  • if the number of trivalent vertices of Γ\Gamma is greater than its degree, then wC([Γ])=0w^{\prime}_{C}([\Gamma])=0,

  • if Γ\Gamma is a non-trivial product of Jacobi diagrams, then wC([Γ])=0w^{\prime}_{C}([\Gamma])=0.

Proof.

By Lemma 2.6, wCw^{\prime}_{C} satisfies these properties, and they characterize it on the summand k𝒫k\bigoplus\limits_{k\in\mathbb{N}}\mathcal{P}_{k} of k𝒜k\bigoplus\limits_{k\in\mathbb{N}}{\mathcal{A}_{k}}.∎

2.5 Configuration spaces

2.5.1 For BCR diagrams

Definition 2.9.

Let ψ:M\psi\colon\mathbb{R}\hookrightarrow{{{M}^{\circ}}} be a long knot. Let Γ\Gamma be a BCR diagram. The open configuration space associated to Γ\Gamma and ψ\psi is

CΓ,BCR0(ψ)={c:V(Γ)MThere exists ci:Vi(Γ),c|Vi(Γ)=ψci}.C_{\Gamma,BCR}^{0}(\psi)=\{c\colon V(\Gamma)\hookrightarrow{{{M}^{\circ}}}\mid\text{There exists }c_{i}\colon V_{i}(\Gamma)\hookrightarrow\mathbb{R},c_{|V_{i}(\Gamma)}=\psi\circ c_{i}\}.

This space is oriented as follows. Let Γ\Gamma be a BCR diagram. For any internal vertex vv, let dtv\mathrm{d}t_{v} denote the coordinate ci(v)c_{i}(v). For any external vertex vv, let (dXvi)i{1,2,3}(\mathrm{d}X_{v}^{i})_{i\in\{1,2,3\}} denote the coordinates of c(v)c(v) in an oriented chart of M{{{M}^{\circ}}}. Split any external edge ee into two half-edges ee_{-} (the tail) and e+e_{+} (the head). For any external half-edge e±e_{\pm}, define a form Ωe±\Omega_{e_{\pm}} as follows:

  • for the head e+e_{+} of an edge that is not a leg, going to an external vertex vv, Ωe+=dXv1\Omega_{e_{+}}=\mathrm{d}X_{v}^{1},

  • for the head e+e_{+} of a leg going to an external vertex vv, Ωe+=dXv2\Omega_{e_{+}}=\mathrm{d}X_{v}^{2},

  • for the tail ee_{-} of an edge coming from an external vertex vv, Ωe=dXv3\Omega_{e_{-}}=\mathrm{d}X_{v}^{3},

  • for any external half-edge e±e_{\pm} adjacent to an internal vertex vv, Ωe±=dtv\Omega_{e_{\pm}}=\mathrm{d}t_{v},

and set ε(Γ)=(1)Card(Ee(Γ))+NT(Γ)\varepsilon(\Gamma)=(-1)^{{\mathrm{Card}}(E_{e}(\Gamma))+N_{T}(\Gamma)} where NT(Γ)N_{T}(\Gamma) is the number of trivalent vertices of Γ\Gamma. With these notations, the manifold CΓ,BCR0(ψ)C_{\Gamma,BCR}^{0}(\psi) is oriented by the form Ω(Γ)=ε(Γ)eEe(Γ)(ΩeΩe+)\Omega(\Gamma)=\varepsilon(\Gamma)\bigwedge\limits_{e\in E_{e}(\Gamma)}\left(\Omega_{e_{-}}\wedge\Omega_{e_{+}}\right).

2.5.2 For Jacobi diagrams

Definition 2.10.

Let ψ:M\psi\colon\mathbb{R}\hookrightarrow{{{M}^{\circ}}} be a long knot. Let Γ\Gamma be a Jacobi diagram. The open configuration space associated to Γ\Gamma and ψ\psi is

CΓ,J0(ψ)={c:V(Γ)M|There exists an increasing map ci:Vi(Γ)such that c|Vi(Γ)=ψci}.C_{\Gamma,J}^{0}(\psi)=\left\{c\colon V(\Gamma)\hookrightarrow{{{M}^{\circ}}}\leavevmode\nobreak\ \Bigr{|}\leavevmode\nobreak\ \begin{array}[]{ll}\text{There exists an increasing map }c_{i}\colon V_{i}(\Gamma)\hookrightarrow\mathbb{R}\\ \text{such that }c_{|V_{i}(\Gamma)}=\psi\circ c_{i}\end{array}\right\}.

Let us fix a bioriented Jacobi diagram Γ\Gamma and orient the manifold CΓ,J0(ψ)C_{\Gamma,J}^{0}(\psi). We use the edge-orientation to split any edge ee of Γ\Gamma in two half-edges ee_{-} and e+e_{+} as above and, for each trivalent vertex, we fix an order on the set of its three adjacent half-edges, compatible with the cyclic order given by the vertex-orientation of the diagram. For any half-edge e±e_{\pm} of Γ\Gamma, define forms Ωe±\Omega_{e_{\pm}} such that,

  • if e±e_{\pm} is adjacent to a univalent vertex vv, Ωe±=dtv\Omega_{e_{\pm}}=\mathrm{d}t_{v},

  • if e±e_{\pm} is the ii-th half-edge adjacent to a trivalent vertex vv, Ωe±=dXvi\Omega_{e_{\pm}}=\mathrm{d}X_{v}^{i},

and set Ω(Γ)=eE(Γ)(ΩeΩe+)\Omega(\Gamma)=\bigwedge\limits_{e\in E(\Gamma)}\left(\Omega_{e_{-}}\wedge\Omega_{e_{+}}\right). Note that this form does not depend of the "compatible with the vertex-orientation" choice of the orders of the half-edges around each trivalent vertex. Note that the orientation form Ω(Γ)\Omega(\Gamma) is multiplied by 1-1 if we change the orientation of one edge or of one trivalent vertex.

2.6 Propagators and configuration space integrals

Here, we review the definition of C2(M)C_{2}({{{M}^{\circ}}}) in [Les15, Section 2.2]. Let C2(M)C_{2}({{{M}^{\circ}}}) denote the space obtained from M2M^{2} after the differential blow-up 999For example, see [Les15, Section 2.2] for more details on these blow-ups. of {(,)}\{(\infty,\infty)\} and of the closures of M×{}{{{M}^{\circ}}}\times\{\infty\}, {}×M\{\infty\}\times{{{M}^{\circ}}} and Δ={(x,x)xM}\Delta=\{(x,x)\mid x\in{{{M}^{\circ}}}\} in the obtained manifold. The manifold with boundary and corners C2(M)C_{2}({{{M}^{\circ}}}) is a compactification of C20(M)=(M)2ΔC_{2}^{0}({{{M}^{\circ}}})=({{{M}^{\circ}}})^{2}\setminus\Delta. Let Gτ:C2(M)𝕊2G_{\tau}\colon\partial C_{2}({{{M}^{\circ}}})\rightarrow\mathbb{S}^{2} denote the Gauss map as defined in101010It is called pτp_{\tau} in these sources. [Les15, Proposition 2.3] or [Les20, Proposition 3.7]. The map GτG_{\tau} is an analogue of the map G:C2(3)𝕊2G\colon C_{2}(\mathbb{R}^{3})\rightarrow\mathbb{S}^{2} that extends ((x,y)C20(3)yxyx𝕊2)\big{(}(x,y)\in C_{2}^{0}(\mathbb{R}^{3})\mapsto\frac{y-x}{||y-x||}\in\mathbb{S}^{2}\big{)}, but GτG_{\tau} is only defined on the boundary of the two-point configuration space. It depends on the parallelization τ\tau of Section 2.1.

A form ω{\omega} on C2(M)C_{2}({{{M}^{\circ}}}) is antisymmetric if T(ω)=ωT^{*}({\omega})=-{\omega}, where T:C2(M)C2(M)T\colon C_{2}({{{M}^{\circ}}})\rightarrow C_{2}({{{M}^{\circ}}}) is the smooth extension of (x,y)C20(M)(y,x)C2(M)(x,y)\in C_{2}^{0}({{{M}^{\circ}}})\mapsto(y,x)\in C_{2}({{{M}^{\circ}}}). Let us recall the definition of the external propagators of [Let19, Section 2.5]. 111111Here, we require antisymmetric propagators in order to get a simpler formula in Theorem 2.13.

Definition 2.11.

A propagator of (M,τ)({{{M}^{\circ}}},\tau) is a closed antisymmetric 22-form ω{\omega} on C2(M)C_{2}({{{M}^{\circ}}}) such that there exists a closed 22-form δω\delta_{\omega} on 𝕊2\mathbb{S}^{2} with total volume 11 such that ω|C2(M)=Gτ(δω){\omega}_{|\partial C_{2}({{{M}^{\circ}}})}={G_{\tau}}^{*}(\delta_{\omega}).

A kk-family of propagators of (M,τ)({{{M}^{\circ}}},\tau) is the data of 3k3k propagators (ωi)i3k¯({\omega}_{i})_{i\in\underline{3k}} of (M,τ)({{{M}^{\circ}}},\tau).

In 3\mathbb{R}^{3} with its canonical parallelization, the pull-back of the SO(3)SO(3)-invariant form on 𝕊2\mathbb{S}^{2} with total volume 11 under the Gauss map GG is a propagator.

Definition 2.12.

For any edge-oriented Jacobi (resp. BCR) diagram Γ\Gamma, define the following maps on the configuration space CΓ,J0(ψ)C_{\Gamma,J}^{0}(\psi) (resp. CΓ,BCR0(ψ)C_{\Gamma,BCR}^{0}(\psi)):

  • for any edge (resp. external edge) e=(v,w)e=(v,w) of Γ\Gamma, pep_{e} denotes the map (c(c(v),c(w)))\big{(}c\mapsto(c(v),c(w))\big{)} from the configuration space to C2(M)C_{2}({{{M}^{\circ}}}),

  • for any pair (v,w)(v,w) of distinct univalent (resp. internal) vertices, εv,w\varepsilon_{v,w} denotes the map (csign(ci(w)ci(v)))\big{(}c\mapsto\mathrm{sign}(c_{i}(w)-c_{i}(v))\big{)} from the configuration space to {1,1}\{-1,1\}.

Note that the map pep_{e} depends on the chosen edge-orientation of a Jacobi diagram.

For any degree kk numbered BCR diagram (Γ,σ)(\Gamma,\sigma) and any kk-family F=(ωi)i3k¯F=({\omega}_{i})_{i\in\underline{3k}} of propagators of (M,ψ,τ)({{{M}^{\circ}}},\psi,\tau), define a form ωF(Γ,σ,ψ)\omega^{F}(\Gamma,\sigma,\psi) on CΓ,BCR0(ψ)C^{0}_{\Gamma,BCR}(\psi) as

ωF(Γ,σ,ψ)=(1)Ni(Γ,)2Card(Ei(Γ))eEe(Γ)pe(ωσ(e)),\omega^{F}(\Gamma,\sigma,\psi)=\frac{(-1)^{N_{i}^{-}(\Gamma,\cdot)}}{2^{{\mathrm{Card}}(E_{i}(\Gamma))}}\bigwedge\limits_{e\in E_{e}(\Gamma)}{p_{e}}^{*}({\omega}_{\sigma(e)}),

where for any cCΓ(ψ)c\in C_{\Gamma}(\psi), Ni(Γ,c)N_{i}^{-}(\Gamma,c) is the number of internal edges from a vertex vv to a vertex ww such that εv,w(c)<0\varepsilon_{v,w}(c)<0. Note that the form ωF(Γ,σ,ψ)\omega^{F}(\Gamma,\sigma,\psi) is the analogue of the form of the same name defined in [Let19, Section 2.6], when all the internal propagators of this article are equal to the 0-form α\alpha on C2()C_{2}(\mathbb{R}) that extends ((x,y)C20()sgn(yx)2)\left((x,y)\in C_{2}^{0}(\mathbb{R})\mapsto\frac{\mathrm{sgn}(y-x)}{2}\in\mathbb{R}\right).

For any degree kk numbered edge-oriented Jacobi diagram (Γ,j)(\Gamma,j) and any kk-family F=(ωi)i3k¯F=({\omega}_{i})_{i\in\underline{3k}} of propagators of (M,τ)({{{M}^{\circ}}},\tau), define a form ωF(Γ,j,ψ)\omega^{F}(\Gamma,j,\psi) as

ωF(Γ,j,ψ)=eE(Γ)pe(ωj(e)).\omega^{F}(\Gamma,j,\psi)=\bigwedge\limits_{e\in E(\Gamma)}{p_{e}}^{*}({\omega}_{j(e)}).

Now, for any numbered BCR diagram, set

IF(Γ,σ,ψ)=CΓ,BCR0(ψ)ωF(Γ,σ,ψ),I^{F}(\Gamma,\sigma,\psi)=\int_{C_{\Gamma,BCR}^{0}(\psi)}\omega^{F}(\Gamma,\sigma,\psi),

and for any numbered bioriented Jacobi diagram, set

IF(Γ,j,ψ)=CΓ,J0(ψ)ωF(Γ,j,ψ).I^{F}(\Gamma,j,\psi)=\int_{C_{\Gamma,J}^{0}(\psi)}\omega^{F}(\Gamma,j,\psi).

These two integrals converge because of the existence of compactifications of the configuration spaces, to which the above forms extend.121212Such compactifications were first introduced by Axelrod and Singer in [AS94, Section 5] for Jacobi diagrams and by Rossi in his thesis [Ros02, Section 2.5] for BCR diagrams. See also [Les20, Section 8] for an extensive description of these compactifications for Jacobi diagrams.

2.7 The perturbative invariant 𝒵\mathcal{Z}

Let 𝒟k~\widetilde{\mathcal{D}_{k}} denote the set of degree kk (unoriented) numbered Jacobi diagrams. Let (Γ,j)𝒟k~(\Gamma,j)\in\widetilde{\mathcal{D}_{k}}, and let F=(ωi)i3k¯F=(\omega_{i})_{i\in\underline{3k}} be a family of propagators of (M,τ)({{{M}^{\circ}}},\tau). Orient both the edges and the trivalent vertices of Γ\Gamma arbitrarily. Since the propagators are antisymmetric, the orientation of CΓ,J0(ψ)C_{\Gamma,J}^{0}(\psi) and the sign of ωF(Γ,j,ψ)\omega^{F}(\Gamma,j,\psi) both change when changing the orientation of one edge of Γ\Gamma, and wC(Γ)w^{\prime}_{C}(\Gamma) remains unchanged. When the orientation of one trivalent vertex changes, the sign of wC([Γ])w^{\prime}_{C}([\Gamma]) and the orientation of CΓ,J0(ψ)C_{\Gamma,J}^{0}(\psi) both change and ωF(Γ,j,ψ)\omega^{F}(\Gamma,j,\psi) remains unchanged. Therefore, IF(Γ,j,ψ)wC([Γ])I^{F}(\Gamma,j,\psi)w^{\prime}_{C}([\Gamma]) depends neither of the vertex-orientation, nor of the edge-orientation, and is thus well-defined for (Γ,j)𝒟k~(\Gamma,j)\in\widetilde{\mathcal{D}_{k}}.

Let jj_{\emptyset} denote the only numbering of the empty diagram, let FF_{\emptyset} denote the empty family of propagators, and set IF(,j,ψ)=1I^{F_{\emptyset}}(\emptyset,j_{\emptyset},\psi)=1.

Theorem 2.13.

Let (M,τ)({{{M}^{\circ}}},\tau) be a parallelized asymptotic rational homology 3\mathbb{R}^{3}. Fix a long knot ψ\psi of M{{{M}^{\circ}}}. Fix an integer k0k\geq 0, and a kk-family F=(ωi)i3k¯F=({\omega}_{i})_{i\in\underline{3k}} of propagators of (M,τ)({{{M}^{\circ}}},\tau), and set

(wC𝒵kF)(ψ,τ)=(Γ,j)𝒟k~(3kCard(E(Γ)))!(3k)!IF(Γ,j,ψ)wC([Γ]),\left(w_{C}\circ\mathcal{Z}^{F}_{k}\right)(\psi,\tau)=\sum\limits_{(\Gamma,j)\in\widetilde{\mathcal{D}_{k}}}\frac{(3k-{\mathrm{Card}}(E(\Gamma)))!}{(3k)!}I^{F}(\Gamma,j,\psi)w_{C}([\Gamma]),
(wC𝒵kF)(ψ,τ)=(Γ,j)𝒟k~(3kCard(E(Γ)))!(3k)!IF(Γ,j,ψ)wC([Γ]).\left(w^{\prime}_{C}\circ\mathcal{Z}^{F}_{k}\right)(\psi,\tau)=\sum\limits_{(\Gamma,j)\in\widetilde{\mathcal{D}_{k}}}\frac{(3k-{\mathrm{Card}}(E(\Gamma)))!}{(3k)!}I^{F}(\Gamma,j,\psi)w^{\prime}_{C}([\Gamma]).
  • The quantity wC𝒵kFw^{\prime}_{C}\circ\mathcal{Z}_{k}^{F} does not depend on the choice of the kk-family FF of propagators of (M,τ)({{{M}^{\circ}}},\tau).

  • The quantity wC𝒵k=wC𝒵kFw^{\prime}_{C}\circ\mathcal{Z}_{k}=w^{\prime}_{C}\circ\mathcal{Z}_{k}^{F} does not depend on the choice of the parallelization τ\tau of M{{{M}^{\circ}}}.

  • The quantity wC𝒵kw^{\prime}_{C}\circ\mathcal{Z}_{k} only depends on the diffeomorphism class of (M,ψ)({{{M}^{\circ}}},\psi).

  • We have the following equality in [[h]]\mathbb{R}[[h]]:

    k0(wC𝒵k)(ψ)hk=exp(k>0(wC𝒵k)(ψ)hk).\sum\limits_{k\geq 0}(w_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}=\exp\left(\sum\limits_{k>0}(w^{\prime}_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}\right).
Proof.

[Les20, Theorem 12.32], which is a mild generalization for long knots of [Les20, Theorem 7.20], implies that

ZkF(ψ,τ)=(Γ,j)𝒟k~(3kCard(E(Γ)))!(3k)!IF(Γ,j,ψ)[Γ]Z_{k}^{F}(\psi,\tau)=\sum\limits_{(\Gamma,j)\in\widetilde{\mathcal{D}_{k}}}\frac{(3k-{\mathrm{Card}}(E(\Gamma)))!}{(3k)!}I^{F}(\Gamma,j,\psi)[\Gamma]

is independent of the choice of the family FF of propagators of (M,τ)({{{M}^{\circ}}},\tau). [Les20, Theorem 12.32], the last assertion of [Les20, Theorem 12.18] and [Les20, Theorem 6.37] imply that

k(ψ)=pcZkF(ψ,τ)14p1(τ)βkIθ(ψ,τ)αk\mathfrak{Z}_{k}(\psi)=p^{c}\circ Z_{k}^{F}(\psi,\tau)-\frac{1}{4}p_{1}(\tau)\beta_{k}-I_{\theta}(\psi,\tau)\alpha_{k}

does not depend on the parallelization and is invariant under diffeomorphism, where 14p1(τ)\frac{1}{4}p_{1}(\tau) and Iθ(ψ,τ)I_{\theta}(\psi,\tau) are some real numbers, and where αk\alpha_{k} and βk\beta_{k} are two elements of 𝒜k{\mathcal{A}_{k}}, called anomalies. [Les20, Propositions 10.14 & 10.20] imply that αk\alpha_{k} and βk\beta_{k} vanish if kk is even. Since wCw_{C} vanishes on odd-degree diagrams, this proves that wC𝒵kFw^{\prime}_{C}\circ\mathcal{Z}_{k}^{F} as defined in the theorem coincides with wCkw^{\prime}_{C}\circ\mathfrak{Z}_{k}. In particular, this implies the first three assertions of the theorem.

Set 𝒵=k0𝒵khk\mathcal{Z}=\sum\limits_{k\geq 0}\mathcal{Z}_{k}h^{k} in 𝒜[[h]]\mathcal{A}[[h]]. Since wCw_{C} is multiplicative, expwC=wCexp\exp\circ w_{C}=w_{C}\circ\exp. The last assertion of [Les20, Theorem 12.18] and [Les20, Theorem 6.37] imply that exppc𝒵=𝒵\exp\circ p^{c}\circ\mathcal{Z}=\mathcal{Z}. Therefore,

wC𝒵=wCexppc𝒵=expwCpc𝒵=expwC𝒵.w_{C}\circ\mathcal{Z}=w_{C}\circ\exp\circ p^{c}\circ\mathcal{Z}=\exp\circ w_{C}\circ p^{c}\circ\mathcal{Z}=\exp\circ w^{\prime}_{C}\circ\mathcal{Z}.\qed

2.8 The BCR invariants

The following theorem is the main result of this article. It is proved in Section 3.

Theorem 2.14.

Fix an integer k2k\geq 2, a null-homologous long knot ψ\psi of a parallelized asymptotic rational homology 3\mathbb{R}^{3} (M,τ)({{{M}^{\circ}}},\tau), and a kk-family F=(ωi)i3k¯F=({\omega}_{i})_{i\in\underline{3k}} of propagators of (M,τ)({{{M}^{\circ}}},\tau). Set

ZBCR,kF(ψ,τ)=(Γ,σ)𝒢k~(3kCard(Ee(Γ)))!(3k)!IF(Γ,σ,ψ),Z^{F}_{BCR,k}(\psi,\tau)=\sum\limits_{(\Gamma,\sigma)\in\widetilde{\mathcal{G}_{k}}}\frac{(3k-{\mathrm{Card}}(E_{e}(\Gamma)))!}{(3k)!}I^{F}(\Gamma,\sigma,\psi),

where 𝒢k~\widetilde{\mathcal{G}_{k}} denote the set of degree kk numbered BCR diagrams up to numbered graph isomorphisms. We have

ZBCR,kF(ψ,τ)=(wC𝒵k)(ψ).Z_{BCR,k}^{F}(\psi,\tau)=-(w^{\prime}_{C}\ \circ\mathcal{Z}_{k})(\psi).

Note that the coefficients (3kCard(Ee(Γ)))!(3k)!\frac{(3k-{\mathrm{Card}}(E_{e}(\Gamma)))!}{(3k)!} in the definition of ZBCR,kFZ^{F}_{BCR,k} replace the 1(2k)!\frac{1}{(2k)!} in the definition of [Let19, Theorem 2.10] since we allowed numberings to take value in 3k¯\underline{3k} and since the internal edges are not numbered anymore.

The above theorem and Theorem 2.13 imply the following corollary.

Corollary 2.15.

The quantity ZBCR,k(ψ)=ZBCR,kF(ψ,τ)Z_{BCR,k}(\psi)=Z_{BCR,k}^{F}(\psi,\tau) does not depend on the choice of the propagators of (M,τ)({{{M}^{\circ}}},\tau), nor of the parallelization, and is invariant under ambient diffeomorphism.

2.9 Relation with the Alexander polynomial

Since the propagators defined in [Let20, Section 4] are dual to propagators in the sense of Definition 2.11, [Let20, Theorem 2.31] implies the following theorem.

Theorem 2.16.

Let M{{{M}^{\circ}}} be an asymptotic rational homology 3\mathbb{R}^{3}, and let ψ:M\psi\colon\mathbb{R}\hookrightarrow{{{M}^{\circ}}} be a null-homologous long knot of M{{{M}^{\circ}}}. If Δψ(t)\Delta_{\psi}(t) denotes the Alexander polynomial of ψ\psi, then

Δψ(eh)=exp(k2ZBCR,k(ψ)hk).\Delta_{\psi}(e^{h})=\exp\left(-\sum\limits_{k\geq 2}Z_{BCR,k}(\psi)h^{k}\right).

The above theorem and Theorems 2.13 and 2.14 imply the following.

Corollary 2.17.

If M{{{M}^{\circ}}} is an asymptotic rational homology 3\mathbb{R}^{3}, and if ψ:M\psi\colon\mathbb{R}\hookrightarrow{{{M}^{\circ}}} is a null-homologous long knot of M{{{M}^{\circ}}}, then

Δψ(eh)=exp(k>0(wC𝒵k)(ψ)hk)=k0(wC𝒵k)(ψ)hk.\Delta_{\psi}(e^{h})=\exp\left(\sum\limits_{k>0}(w^{\prime}_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}\right)=\sum\limits_{k\geq 0}(w_{C}\circ\mathcal{Z}_{k})(\psi)h^{k}.

2.10 Compatibility with the formula in terms of the Kontsevich integral

In this section, we prove that Corollary 2.17 can be stated equivalently in terms of the Kontsevich integral or of the perturbative expansion of the Chern-Simons theory, for long knots of 3\mathbb{R}^{3}.

Proposition 2.18.

For any long knot ψ\psi of 3\mathbb{R}^{3},

(wC𝒵k)(ψ)=(wC𝒵kK)(ψ)(w_{C}\circ\mathcal{Z}_{k})(\psi)=(w_{C}\circ\mathcal{Z}^{K}_{k})(\psi)
Proof.

Let γ=(γk)k{0}\gamma=(\gamma_{k})_{k\in\mathbb{N}\setminus\{0\}}, where γk\gamma_{k} is a combination of degree kk diagrams with exactly two univalent vertices, and γ10\gamma_{1}\neq 0. Lescop [Les02, Definition 2.1] proved the existence of a well-defined morphism Ψ(γ):𝒜𝒜\Psi(\gamma)\colon\mathcal{A}\rightarrow\mathcal{A} such that for any Jacobi diagram Γ\Gamma, Ψ(γ)([Γ])\Psi(\gamma)([\Gamma]) is obtained as follows :

  • Write γk=iIkb(Γi,k)[Γi,k]\gamma_{k}=\sum\limits_{i\in I_{k}}b(\Gamma_{i,k})[\Gamma_{i,k}] for any k1k\geq 1, and set I={Γi,kk1,iIk}I=\{\Gamma_{i,k}\mid k\geq 1,i\in I_{k}\}.

  • In each connected component Γj\Gamma_{j} of Γ\Gamma, fix deg(Γj)\deg(\Gamma_{j}) edges, and let XX denote the set of the chosen edges.

  • For any map ξ:XI\xi\colon X\rightarrow I, let Ψ0(γ)(Γ,ξ)\Psi^{0}(\gamma)(\Gamma,\xi) denote the graph obtained from Γ\Gamma after replacing each edge ee of XX with ξ(e)\xi(e).

  • Set

    Ψ(γ)([Γ])=ξ:XI(eXb(ξ(e)))[Ψ0(γ)(Γ,ξ)].\Psi(\gamma)([\Gamma])=\sum\limits_{\xi\colon X\rightarrow I}\left(\prod\limits_{e\in X}b(\xi(e))\right)[\Psi^{0}(\gamma)(\Gamma,\xi)].

With these notations, [Les02, Theorem 2.3] states that 𝒵=Ψ(2α)(𝒵K)\mathcal{Z}=\Psi(2\alpha)(\mathcal{Z}^{K}) where α\alpha is the Bott-Taubes anomaly. [Les20, Proposition 10.20] implies that 2α12\alpha_{1} is the class of the diagram Γθ\Gamma_{\theta} with one edge between two univalent vertices.

Proposition 2.18 follows from the following lemma. ∎

Lemma 2.19.

wCΨ(2α)=wC.w_{C}\circ\Psi(2\alpha)=w_{C}.

Proof.

Set w=wCΨ(2α)w=w_{C}\circ\Psi(2\alpha), and let us check that ww satisfies the four properties of Lemma 2.6.

  • The first property is immediate.

  • For any k3k\geq 3, 2αk2\alpha_{k} is a combination of diagrams with 2k2>k2k-2>k trivalent vertices. Therefore, for any p2p\geq 2 and any ξ:XI\xi\colon X\rightarrow I as above, if ξ\xi maps at least one edge to an element different from Γθ\Gamma_{\theta}, then the number of trivalent vertices of Ψ0(2α)(Γp,ξ)\Psi^{0}(2\alpha)(\Gamma_{p},\xi) is greater than its degree. This implies that w([Γp])=wC([Γp])w([\Gamma_{p}])=w_{C}([\Gamma_{p}]).

  • If Γ\Gamma contains more than deg(Γ)\deg(\Gamma) trivalent vertices, then the same argument implies that w([Γ])=0w([\Gamma])=0.

  • If Γ\Gamma is the product of two non-empty diagrams Γ1\Gamma_{1} and Γ2\Gamma_{2}, set Xi=XE(Γi)X_{i}=X\cap E(\Gamma_{i}) for i{1,2}i\in\{1,2\}. For any ξ:XI\xi\colon X\rightarrow I, set ξi=ξ|Xi\xi_{i}=\xi_{|X_{i}} for i{1,2}i\in\{1,2\}. Note that Ψ0(2α)(Γ,ξ)\Psi^{0}(2\alpha)(\Gamma,\xi) is the product of Ψ0(2α)(Γ1,ξ1)\Psi^{0}(2\alpha)(\Gamma_{1},\xi_{1}) and Ψ0(2α)(Γ2,ξ2)\Psi^{0}(2\alpha)(\Gamma_{2},\xi_{2}). Therefore, since wCw_{C} is multiplicative,

    w([Γ])\displaystyle w([\Gamma]) =\displaystyle= ξ:XI(eXb(ξ(e)))wC([Ψ0(2α)(Γ,ξ)])\displaystyle\sum\limits_{\xi\colon X\rightarrow I}\left(\prod\limits_{e\in X}b(\xi(e))\right)w_{C}\left(\left[\Psi^{0}(2\alpha)(\Gamma,\xi)\right]\right)
    =\displaystyle= ξ1:X1Iξ2:X1I(eX1b(ξ1(e)))(eX2b(ξ2(e)))\displaystyle\sum\limits_{\xi_{1}\colon X_{1}\rightarrow I}\sum\limits_{\xi_{2}\colon X_{1}\rightarrow I}\left(\prod\limits_{e\in X_{1}}b(\xi_{1}(e))\right)\left(\prod\limits_{e\in X_{2}}b(\xi_{2}(e))\right)
    wC([Ψ0(2α)(Γ1,ξ1)])wC([Ψ0(2α)(Γ2,ξ2)])\displaystyle\ \ \ \ \ \ \ \ w_{C}\left(\left[\Psi^{0}(2\alpha)(\Gamma_{1},\xi_{1})\right]\right)w_{C}\left(\left[\Psi^{0}(2\alpha)(\Gamma_{2},\xi_{2})\right]\right)
    =\displaystyle= w([Γ1])w([Γ2]).\displaystyle w([\Gamma_{1}])w([\Gamma_{2}]).

3 Proof of Theorem 2.14

3.1 Definition of a weight system for the BCR invariants

From now on, we fix a parallelized asymptotic rational homology 3\mathbb{R}^{3} (M,τ)({{{M}^{\circ}}},\tau), a long knot ψ:nM\psi\colon\mathbb{R}^{n}\hookrightarrow{{{M}^{\circ}}}, an integer k2k\geq 2, and a kk-family F=(ωi)i3k¯F=({\omega}_{i})_{i\in\underline{3k}} of propagators of (M,τ)({{{M}^{\circ}}},\tau).

For any BCR diagram Γ\Gamma, let 𝔒(Γ){\mathfrak{O}(\Gamma)} denote the set of total orders on Vi(Γ)V_{i}(\Gamma). Represent an element of 𝔒(Γ){\mathfrak{O}(\Gamma)} by the unique increasing bijection ρ:Vi(Γ){1,,Card(Vi(Γ))}\rho\colon V_{i}(\Gamma)\rightarrow\{1,\ldots,{\mathrm{Card}}(V_{i}(\Gamma))\}. For any degree kk BCR diagram Γ\Gamma, the configuration space CΓ,BCR0(ψ)C_{\Gamma,BCR}^{0}(\psi) splits into a disjoint union of connected components ρ𝔒(Γ)CΓ,BCR,ρ0(ψ)\bigsqcup\limits_{\rho\in{\mathfrak{O}(\Gamma)}}C_{\Gamma,BCR,\rho}^{0}(\psi) where

CΓ,BCR,ρ0(ψ)={cCΓ,BCR0(ψ)|for any distinct internal vertices vwρ(v)<ρ(w)εv,w(c)>0}.C_{\Gamma,BCR,\rho}^{0}(\psi)=\left\{c\in C_{\Gamma,BCR}^{0}(\psi)\leavevmode\nobreak\ \Bigr{|}\leavevmode\nobreak\ \begin{array}[]{l}\text{for any distinct internal vertices $v$, $w$, }\\ \rho(v)<\rho(w)\Leftrightarrow\varepsilon_{v,w}(c)>0\end{array}\right\}.

Any ρ𝔒(Γ)\rho\in{\mathfrak{O}(\Gamma)} induces a bioriented Jacobi unitrivalent diagram Γρ\Gamma_{\rho} with the same degree as follows. The vertices of Γρ\Gamma_{\rho} are all the vertices of Γ\Gamma and the edges of Γρ\Gamma_{\rho} are the external edges of Γ\Gamma, so that the internal (resp. external) vertices of Γ\Gamma yield the univalent (resp. trivalent) vertices of Γρ\Gamma_{\rho}. The order of the univalent vertices of Γρ\Gamma_{\rho} is given by ρ\rho. It remains to orient the trivalent vertices of Γρ\Gamma_{\rho}, i.e. to fix a cyclic order on the half-edges adjacent to any external vertex vv. Let ee denote the external edge of the cycle going to vv, let \ell denote the leg going to vv, and let ff denote the external edge of the cycle coming from vv. The orientation of vv is given by the cyclic order (e+,+,f)(e_{+},\ell_{+},f_{-}). Note that any numbering σ\sigma of Γ\Gamma yields a canonical numbering jρ,σj_{\rho,\sigma} of Γρ\Gamma_{\rho}. With these notations, the following lemma is immediate.

Lemma 3.1.

For any BCR diagram Γ\Gamma, any order ρ𝔒(Γ)\rho\in{\mathfrak{O}(\Gamma)}, and any numbering σ\sigma of Γ\Gamma,

CΓ,BCR,ρ(ψ)ωF(Γ,σ,ψ)=ε(Γ)ε2(Γ,ρ)2Card(Ei(Γ))IF(Γρ,jρ,σ,ψ),\int_{C_{\Gamma,BCR,\rho}(\psi)}\omega^{F}(\Gamma,\sigma,\psi)=\frac{\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)}{2^{{\mathrm{Card}}(E_{i}(\Gamma))}}I^{F}(\Gamma_{\rho},j_{\rho,\sigma},\psi),

where ε(Γ)\varepsilon(\Gamma) is defined in Section 2.5.1 and ε2(Γ,ρ)=(v,w)Ei(Γ)sgn(ρ(w)ρ(v)){±1}.\varepsilon_{2}(\Gamma,\rho)=\prod\limits_{(v,w)\in E_{i}(\Gamma)}\mathrm{sgn}(\rho(w)-\rho(v))\in\{\pm 1\}.

Let us introduce the following notations.

Notation 3.2.

For any degree kk vertex-oriented numbered Jacobi diagram ΓJ\Gamma_{J}, let 𝒢(ΓJ,j)\mathcal{G}(\Gamma_{J},j) denote the set of ordered and numbered BCR diagrams (Γ,σ,ρ)(\Gamma,\sigma,\rho) such that (Γρ,jρ,σ)(\Gamma_{\rho},j_{\rho,\sigma}) coincides with (ΓJ,j)(\Gamma_{J},j), up to the orientation of the trivalent vertices and after forgetting the orientation of the edges. For such a numbered and ordered BCR diagram, let ε3(ΓJ,Γ,ρ){±1}\varepsilon_{3}(\Gamma_{J},\Gamma,\rho)\in\{\pm 1\} be such that [Γρ]=ε3(ΓJ,Γ,ρ)[ΓJ][\Gamma_{\rho}]=\varepsilon_{3}(\Gamma_{J},\Gamma,\rho)[\Gamma_{J}]. Set

wBCR(ΓJ,j)=(Γ,σ,ρ)𝒢(ΓJ,j)ε(Γ)ε2(Γ,ρ)ε3(ΓJ,Γ,ρ)22kCard(E(ΓJ)),w_{BCR}(\Gamma_{J},j)=\sum\limits_{(\Gamma,\sigma,\rho)\in\mathcal{G}(\Gamma_{J},j)}\frac{\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J},\Gamma,\rho)}{2^{2k-{\mathrm{Card}}(E(\Gamma_{J}))}},

and note that wBCR(ΓJ,j)w_{BCR}(\Gamma_{J},j) does not depend on jj. Denote it by wBCR(ΓJ)w_{BCR}(\Gamma_{J}).

We are going to prove the following proposition.

Proposition 3.3.

For any Jacobi diagram ΓJ\Gamma_{J}, wBCR(ΓJ)=wC([ΓJ])w_{BCR}(\Gamma_{J})=-w^{\prime}_{C}([\Gamma_{J}]).

Note that the above proposition and Lemma 3.1 imply Theorem 2.14. We now prove Proposition 3.3 until the end of this article. In the next subsections, we check that (wBCR)(-w_{BCR}) induces a linear map 𝒜k{\mathcal{A}_{k}}\rightarrow\mathbb{R} that satisfies the properties of Lemma 2.8. Note that it is immediate that (wBCR)(-w_{BCR}) vanishes on degree 0 and 11 diagrams, since a BCR diagram is non-empty, and since the only degree 11 BCR diagram is counted with opposite signs when the order of its two internal vertices is changed. The following lemma gives an example of diagrams with non-trivial wBCRw_{BCR} and proves the second and third property of Lemma 2.8.

Lemma 3.4.
  1. 1.

    If ΓJ\Gamma_{J} is a degree kk Jacobi diagram and has more than kk trivalent vertices, then wBCR(ΓJ)=0w_{BCR}(\Gamma_{J})=0.

  2. 2.

    If Γk\Gamma_{k} is the graph of Figure 7, then wBCR(Γk)=1+(1)kw_{BCR}(\Gamma_{k})=1+(-1)^{k}.

Proof.

The first point is immediate since any external vertex of a BCR diagram has a univalent neighbour, so that there cannot be more than kk external vertices in a degree kk BCR diagram.

For the second point, given a numbering jj of Γk\Gamma_{k}, there are exactly two elements in 𝒢(Γk,j){\mathcal{G}}(\Gamma_{k},j), and they are given by (ΓkBCR,ρa,ja)(\Gamma_{k}^{BCR},\rho_{a},j_{a}) and (ΓkBCR,ρb,jb)(\Gamma_{k}^{BCR},\rho_{b},j_{b}), as depicted in Figure 8, where viv_{i} denotes the vertex ρ1(i)\rho^{-1}(i), and the numberings jaj_{a} and jbj_{b} are uniquely determined by jj.

vkv_{k}v3v_{3}v2v_{2}v1v_{1}(ΓkBCR,ρa)(\Gamma_{k}^{BCR},\rho_{a})
v1v_{1}v2v_{2}v3v_{3}vkv_{k}(ΓkBCR,ρb)(\Gamma_{k}^{BCR},\rho_{b})
Γk\Gamma_{k}
Figure 8:

Note that ε2(ΓkBCR,ρa)=ε2(ΓkBCR,ρb)=1\varepsilon_{2}(\Gamma_{k}^{BCR},\rho_{a})=\varepsilon_{2}(\Gamma_{k}^{BCR},\rho_{b})=1, and that ε(ΓkBCR)=(1)k\varepsilon(\Gamma_{k}^{BCR})=(-1)^{k}. The graph (ΓkBCR)ρa(\Gamma_{k}^{BCR})_{\rho_{a}} has exactly the same vertex-orientation than Γk\Gamma_{k}, and (ΓkBCR)ρb(\Gamma_{k}^{BCR})_{\rho_{b}} has the opposite orientation at each trivalent vertex, so that (1)k[(ΓkBCR)ρb]=[(ΓkBCR)ρa]=[Γk](-1)^{k}[(\Gamma_{k}^{BCR})_{\rho_{b}}]=[(\Gamma_{k}^{BCR})_{\rho_{a}}]=[\Gamma_{k}]. Therefore, wBCR(Γk)=1+(1)kw_{BCR}(\Gamma_{k})=1+(-1)^{k}. ∎

3.2 Linear extension of wBCRw_{BCR} to 𝒜k{\mathcal{A}_{k}}

Lemma 3.5.

The map wBCRw_{BCR} induces a linear form on 𝒜k{\mathcal{A}_{k}}.

Proof.

It suffices to prove that wBCRw_{BCR} is compatible with the relations of Definition 2.3. The compatibility with the AS relation is immediate. For diagrams with only trivalent vertices, the IHX relation is immediate since wBCRw_{BCR} is zero on the three involved diagrams. Bar-Natan [BN95a, Theorem 6] proved that the IHX relation is a consequence of the STU relation for diagrams of 𝒜kˇ{\check{\mathcal{A}_{k}}}.

Let us now prove the STU relation. Let ΓJ\Gamma_{J}, ΓJ(1)\Gamma_{J}^{(1)} and ΓJ(2)\Gamma_{J}^{(2)} be three Jacobi diagrams connected by the STU relation of Definition 2.3, as in Figure 9. We are going to prove that wBCR(ΓJ)=wBCR(ΓJ(1))wBCR(ΓJ(2))w_{BCR}(\Gamma_{J})=w_{BCR}(\Gamma_{J}^{(1)})-w_{BCR}(\Gamma_{J}^{(2)}). Let the vertices vv, ww, tt and uu and the edges ee, ff and hh be as in Figure 9.

uutteeffhhΓJ\Gamma_{J}
vvwweeffΓJ(1)\Gamma_{J}^{(1)}
wwvveeffΓJ(2)\Gamma_{J}^{(2)}
Figure 9:

We have a natural identification E(ΓJ(1))E(ΓJ(2))E(ΓJ){h}E(\Gamma_{J}^{(1)})\cong E(\Gamma_{J}^{(2)})\cong E(\Gamma_{J})\setminus\{h\}. Fix a numbering j1j_{1} of ΓJ(1)\Gamma_{J}^{(1)}, and let j2j_{2} the associated numbering of ΓJ(2)\Gamma_{J}^{(2)}. Fix i03k¯j1(E(ΓJ(1)))i_{0}\in\underline{3k}\setminus j_{1}(E(\Gamma_{J}^{(1)})) and let jj denote the numbering of ΓJ\Gamma_{J} such that j(h)=i0j(h)=i_{0} and that induces j1j_{1} on ΓJ(1)\Gamma_{J}^{(1)}.

For i{1,2}i\in\{1,2\}, split 𝒢(ΓJ(i),ji){\mathcal{G}}(\Gamma_{J}^{(i)},j_{i}) into 𝒢1(ΓJ(i),ji){\mathcal{G}}_{1}(\Gamma_{J}^{(i)},j_{i}) and 𝒢2(ΓJ(i),ji){\mathcal{G}}_{2}(\Gamma_{J}^{(i)},j_{i}), where

𝒢1(ΓJ(i),ji)={(Γ,σ,ρ)𝒢(ΓJ(i),ji)There is exactly one internal edge between v and w},{\mathcal{G}}_{1}(\Gamma_{J}^{(i)},j_{i})=\{(\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J}^{(i)},j_{i})\mid\text{There is exactly one internal edge between $v$ and $w$}\},
𝒢2(ΓJ(i),ji)=𝒢(ΓJ(i),ji)𝒢1(ΓJ(i),ji).{\mathcal{G}}_{2}(\Gamma_{J}^{(i)},j_{i})={\mathcal{G}}(\Gamma_{J}^{(i)},j_{i})\setminus{\mathcal{G}}_{1}(\Gamma_{J}^{(i)},j_{i}).

For any (Γ,σ,ρ)𝒢(ΓJ(1),j1)(\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J}^{(1)},j_{1}), let ρ\rho^{*} denote the ordering ρρv,w\rho\circ\rho_{v,w}, where ρv,w\rho_{v,w} is the transposition of vv and ww. This induces a bijection ((Γ,σ,ρ)𝒢(ΓJ(1),j1)(Γ,σ,ρ)𝒢(ΓJ(2),j2))\big{(}(\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J}^{(1)},j_{1})\mapsto(\Gamma,\sigma,\rho^{*})\in{\mathcal{G}}(\Gamma_{J}^{(2)},j_{2})\big{)}, which preserves the above decomposition 𝒢(ΓJ(i),ji)=𝒢1(ΓJ(i),ji)𝒢2(ΓJ(i),ji){\mathcal{G}}(\Gamma_{J}^{(i)},j_{i})={\mathcal{G}}_{1}(\Gamma_{J}^{(i)},j_{i})\sqcup{\mathcal{G}}_{2}(\Gamma_{J}^{(i)},j_{i}). Note that ε3(ΓJ(1),Γ,ρ)=ε3(ΓJ(2),Γ,ρ)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho)=\varepsilon_{3}(\Gamma_{J}^{(2)},\Gamma,\rho^{*}) and that

ε2(Γ,ρ)={ε2(Γ,ρ)if (Γ,σ,ρ)𝒢1(ΓJ(1),j1),ε2(Γ,ρ)if (Γ,σ,ρ)𝒢2(ΓJ(1),j1).\varepsilon_{2}(\Gamma,\rho^{*})=\begin{cases}-\varepsilon_{2}(\Gamma,\rho)&\text{if $(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}(\Gamma_{J}^{(1)},j_{1})$,}\\ \varepsilon_{2}(\Gamma,\rho)&\text{if $(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{2}(\Gamma_{J}^{(1)},j_{1})$.}\end{cases}

This yields wBCR(ΓJ(1))wBCR(ΓJ(2))=2(Γ,σ,ρ)𝒢1(ΓJ(1),j1)ε(Γ)ε2(Γ,ρ)ε3(ΓJ(1),Γ,ρ)22kCard(E(ΓJ(1))).w_{BCR}(\Gamma_{J}^{(1)})-w_{BCR}(\Gamma_{J}^{(2)})=2\sum\limits_{(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}(\Gamma_{J}^{(1)},j_{1})}\frac{\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho)}{2^{2k-{\mathrm{Card}}\left(E\left(\Gamma_{J}^{(1)}\right)\right)}}.

Let 𝒢1a(ΓJ(1),j1){\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1}) denote the set of ordered and numbered BCR diagrams (Γ,σ,ρ)𝒢1(ΓJ(1),j1)(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}(\Gamma_{J}^{(1)},j_{1}) such that vv and ww are both trivalent in Γ\Gamma, and set 𝒢1b(ΓJ(1),j1)=𝒢1(ΓJ(1),j1)𝒢1a(ΓJ(1),j1){\mathcal{G}}_{1}^{b}(\Gamma_{J}^{(1)},j_{1})={\mathcal{G}}_{1}(\Gamma_{J}^{(1)},j_{1})\setminus{\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1}). For any (Γ,σ,ρ)𝒢1a(ΓJ(1),j1)(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1}), let xx and yy denote the univalent vertices respectively adjacent to vv and ww as in Figure 10, and set ρ=ρρx,yρv,w\rho^{*}=\rho\circ\rho_{x,y}\circ\rho_{v,w} and σ=σρe,f\sigma^{*}=\sigma\circ\rho_{e,f}. Since there is only one internal edge from vv to ww, there are internal edges (v,v)(v^{\prime},v) and (w,w)(w,w^{\prime}) where vv^{\prime} and ww^{\prime} are neither vv nor ww, and ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma,\rho^{*})=-\varepsilon_{2}(\Gamma,\rho). The orientation of the possible external vertices did not change, so ε3(ΓJ(1),Γ,ρ)=ε3(ΓJ(1),Γ,ρ)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho)=\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho^{*}). Since ((Γ,σ,ρ)𝒢1a(ΓJ(1),j1)(Γ,σ,ρ)𝒢1a(ΓJ(1),j1))\big{(}(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1})\mapsto(\Gamma,\sigma^{*},\rho^{*})\in{\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1})\big{)} is a bijection, this yields

(Γ,σ,ρ)𝒢1a(ΓJ(1),j1)ε(Γ)ε2(Γ,ρ)ε3(ΓJ(1),Γ,ρ)22kCard(E(ΓJ(1)))=0.\sum\limits_{(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1})}\frac{\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho)}{2^{2k-{\mathrm{Card}}(E(\Gamma_{J}^{(1)}))}}=0.
wwvvxxyyffee
Figure 10: Notations for a graph of 𝒢1a(ΓJ(1),j1){\mathcal{G}}_{1}^{a}(\Gamma_{J}^{(1)},j_{1}).

We now define a bijection

((Γ,σ,ρ)𝒢1b(ΓJ(1),j1)(Γ,σ,ρ)𝒢(ΓJ,j)).\big{(}(\Gamma,\sigma,\rho)\in{\mathcal{G}}^{b}_{1}(\Gamma_{J}^{(1)},j_{1})\mapsto(\Gamma^{*},\sigma^{*},\rho^{*})\in{\mathcal{G}}(\Gamma_{J},j)\big{)}.

For any (Γ,σ,ρ)𝒢1b(ΓJ(1),j1)(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}^{b}(\Gamma_{J}^{(1)},j_{1}), let Γ\Gamma^{*} denote the BCR diagram defined as follows:

  • if vv and ww are both bivalent, Γ\Gamma^{*} is obtained as in Figure 11,

    Γ\Gammavvwweeff
    Γ\Gamma^{*}tteeffhhuu
    Γ\Gammavvwweeff
    Γ\Gamma^{*}tteeffhhuu
    Figure 11:
  • if vv is trivalent and ww bivalent, Γ\Gamma^{*} is obtained as in Figure 12,

    Γ\Gammavvwweeffxx
    Γ\Gamma^{*}uutteeffhhxx
    Γ\Gammavvwweeffxx
    Γ\Gamma^{*}uutteeffhhxx
    Figure 12:
  • if vv is bivalent and ww trivalent, Γ\Gamma^{*} is obtained as in Figure 13,

    Γ\Gammavvwweeffxx
    Γ\Gamma^{*}ttuueeffhhxx
    Γ\Gammavvwweeffxx
    Γ\Gamma^{*}ttuueeffhhxx
    Figure 13:

The ordering ρ\rho induces a natural ordering ρ\rho^{*} of Γ\Gamma^{*}. Note that Ee(Γ){h}Ee(Γ)E_{e}(\Gamma^{*})\setminus\{h\}\cong E_{e}(\Gamma). Let σ\sigma^{*} denote the numbering of Γ\Gamma^{*} that coincide with σ\sigma on Ee(Γ){h}E_{e}(\Gamma^{*})\setminus\{h\} and such that σ(h)=i0\sigma^{*}(h)=i_{0}, so that (Γ,σ,ρ)𝒢(ΓJ,j)(\Gamma^{*},\sigma^{*},\rho^{*})\in{\mathcal{G}}(\Gamma_{J},j). Let us check that ε(Γ)ε2(Γ,ρ)ε3(ΓJ(1),Γ,ρ)=ε(Γ)ε2(Γ,ρ)ε3(ΓJ,Γ,ρ)\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho)=\varepsilon(\Gamma^{*})\varepsilon_{2}(\Gamma^{*},\rho^{*})\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*}).

  • If vv and ww are bivalent, since Γ\Gamma^{*} has one more external edge and one more trivalent vertex than Γ\Gamma, ε(Γ)=ε(Γ)\varepsilon(\Gamma)=\varepsilon(\Gamma^{*}).

    • If there is an internal edge from vv to ww as in the first row of Figure 11, ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma^{*},\rho^{*})=\varepsilon_{2}(\Gamma,\rho) since ρ(w)ρ(v)\rho(w)-\rho(v) is positive. The orientation of the vertex tt is given by the cyclic order (e,h,f)(e,h,f) as in ΓJ\Gamma_{J}, and ε3(ΓJ,Γ,ρ)=ε3(ΓJ(1),Γ,ρ)\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho).

    • If there is an internal edge from ww to vv as in the second row of Figure 11, ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma^{*},\rho^{*})=-\varepsilon_{2}(\Gamma,\rho) since ρ(v)ρ(w)\rho(v)-\rho(w) is negative. The orientation of the vertex tt is given by the cyclic order (f,h,e)(f,h,e). It is the opposite of the orientation of tt in ΓJ\Gamma_{J}, and ε3(ΓJ,Γ,ρ)=ε3(ΓJ(1),Γ,ρ)\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=-\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho).

  • If vv is trivalent and ww is bivalent, since Γ\Gamma^{*} has one more external edge than Γ\Gamma and as much trivalent vertices, ε(Γ)=ε(Γ)\varepsilon(\Gamma)=-\varepsilon(\Gamma^{*}).

    • If there is an internal edge from vv to ww as in the first row of Figure 12, ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma^{*},\rho^{*})=\varepsilon_{2}(\Gamma,\rho) since ρ(w)ρ(v)\rho(w)-\rho(v) is positive. The orientation of the vertex tt is given by the cyclic order (h,e,f)(h,e,f). It is the opposite of the orientation of tt in ΓJ\Gamma_{J}, and ε3(ΓJ,Γ,ρ)=ε3(ΓJ(1),Γ,ρ)\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=-\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho).

    • If there is an internal edge from ww to vv as in the second row of Figure 12, ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma^{*},\rho^{*})=-\varepsilon_{2}(\Gamma,\rho) since ρ(v)ρ(w)\rho(v)-\rho(w) is negative. The orientation of the vertex tt is given by the cyclic order (f,e,h)(f,e,h). It is the orientation of tt in ΓJ\Gamma_{J}, and ε3(ΓJ,Γ,ρ)=ε3(ΓJ(1),Γ,ρ)\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho).

  • If vv is bivalent and ww is trivalent, the same argument yields ε(Γ)=ε(Γ)\varepsilon(\Gamma^{*})=-\varepsilon(\Gamma), and we prove as above that ε2(Γ,ρ)ε3(ΓJ,Γ,ρ)=ε2(Γ,ρ)ε3(ΓJ(1),Γ,ρ)\varepsilon_{2}(\Gamma^{*},\rho^{*})\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=-\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho) in both cases of Figure 13.

Since ΓJ\Gamma_{J} has one edge more than ΓJ(1)\Gamma_{J}^{(1)},

(Γ,σ,ρ)𝒢1b(ΓJ(1),j1)ε(Γ)ε2(Γ,ρ)ε3(ΓJ(1),Γ,ρ)22k1Card(E(ΓJ(1)))\displaystyle\sum\limits_{(\Gamma,\sigma,\rho)\in{\mathcal{G}}_{1}^{b}(\Gamma_{J}^{(1)},j_{1})}\frac{\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J}^{(1)},\Gamma,\rho)}{2^{2k-1-{\mathrm{Card}}(E(\Gamma_{J}^{(1)}))}} =\displaystyle= (Γ,σ,ρ)𝒢(ΓJ,j)ε(Γ)ε2(Γ,ρ)ε3(ΓJ,Γ,ρ)22kCard(E(ΓJ))\displaystyle\sum\limits_{(\Gamma^{*},\sigma^{*},\rho^{*})\in{\mathcal{G}}(\Gamma_{J},j)}\frac{\varepsilon(\Gamma^{*})\varepsilon_{2}(\Gamma^{*},\rho^{*})\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})}{2^{2k-{\mathrm{Card}}(E(\Gamma_{J}))}}
=\displaystyle= wBCR(ΓJ).\displaystyle w_{BCR}(\Gamma_{J}).

This yields wBCR(ΓJ(1))wBCR(ΓJ(2))=wBCR(ΓJ)w_{BCR}(\Gamma_{J}^{(1)})-w_{BCR}(\Gamma_{J}^{(2)})=w_{BCR}(\Gamma_{J}) and concludes the proof of Lemma 3.5.∎

3.3 Restriction to connected diagrams

Lemma 3.6.

If ΓJ\Gamma_{J} is a non-trivial product of diagrams, then wBCR(ΓJ)=0w_{BCR}(\Gamma_{J})=0.

Proof.

Let ΓJ\Gamma_{J} be a non-trivial product, and let ΓJ(1)\Gamma_{J}^{(1)} and ΓJ(2)\Gamma_{J}^{(2)} be two Jacobi diagrams such that ΓJ\Gamma_{J} is the product of ΓJ(1)\Gamma_{J}^{(1)} and ΓJ(2)\Gamma_{J}^{(2)}. Let jj be a numbering of ΓJ\Gamma_{J}. We are going to define an involution ((Γ,σ,ρ)𝒢(ΓJ,j)(Γ,σ,ρ)𝒢(ΓJ,j))\left((\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J},j)\mapsto(\Gamma^{*},\sigma^{*},\rho^{*})\in{\mathcal{G}}(\Gamma_{J},j)\right).

For any (Γ,σ,ρ)𝒢(ΓJ,j)(\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J},j), let V(Γ)=V1V2V(\Gamma)=V_{1}\sqcup V_{2} be the partition of V(Γ)V(\Gamma) such that the vertices of ViV_{i} correspond to the vertices of ΓJ(i)\Gamma_{J}^{(i)} in ΓJ\Gamma_{J}. Let Γ\Gamma^{\prime} denote the graph obtained from Γ\Gamma by keeping only the vertices of V2V_{2} and the edges between such vertices, and let Γc\Gamma_{c} denote the connected component of Γ\Gamma^{\prime} that contains the external edge with minimal σ\sigma. Let V3V_{3} denote the set of vertices of Γc\Gamma_{c}. By construction of BCR diagrams, there is exactly one internal edge e1=(v,w)e_{1}=(v,w) from V1V_{1} to an internal vertex ww of V3V_{3}. Note that any element of ρ(V1Vi(Γ))\rho(V_{1}\cap V_{i}(\Gamma)) is before any element of ρ(V3Vi(Γ))\rho(V_{3}\cap V_{i}(\Gamma))

Let Γ\Gamma^{*} denote the BCR diagram defined as follows.

  • If ww is bivalent in Γ\Gamma, and if we have an external edge e=(w,w2)e=(w,w_{2}) from ww to another bivalent vertex w2w_{2}, then w2w_{2} is in V3V_{3} since Γc\Gamma_{c} is connected. Set w1=ww_{1}=w. The graph Γ\Gamma^{*} is obtained from Γ\Gamma after replacing the internal edge e1=(v,w1)e_{1}=(v,w_{1}) with an internal edge from vv to w2w_{2} as in Figure 14, and ρ\rho^{*} and σ\sigma^{*} are naturally deduced from ρ\rho and σ\sigma. Since w1w_{1} and w2w_{2} are in V3V_{3} and vv in V1V_{1}, ρ(w2)ρ(v)\rho(w_{2})-\rho(v) and ρ(w1)ρ(v)\rho(w_{1})-\rho(v) have the same sign, and ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma^{*},\rho^{*})=\varepsilon_{2}(\Gamma,\rho). Furthermore, we have ε(Γ)=ε(Γ)\varepsilon(\Gamma^{*})=-\varepsilon(\Gamma) since Γ\Gamma^{*} has the same external edges as Γ\Gamma but one more (internal) trivalent vertex. Since nothing changed around the external trivalent vertices, ε3(ΓJ,Γ,ρ)=ε3(ΓJ,Γ,ρ)\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=\varepsilon_{3}(\Gamma_{J},\Gamma,\rho).

  • If ww is trivalent in Γ\Gamma, set w2=ww_{2}=w. There is a leg e=(w1,w2)e=(w_{1},w_{2}) from a univalent vertex w1w_{1} to w2w_{2}. Since Γc\Gamma_{c} is connected, w1w_{1} is in V3V_{3}. In this case, Γ\Gamma^{*} is the graph obtained from Γ\Gamma after replacing the internal edge e1=(v,w2)e_{1}=(v,w_{2}) with (v,w1)(v,w_{1}) as in Figure 14, and ρ\rho^{*} and σ\sigma^{*} are naturally determined by ρ\rho and σ\sigma. As above, we have (ε(Γ),ε2(Γ,ρ),ε3(ΓJ,Γ,ρ))=(ε(Γ),ε2(Γ,ρ),ε3(ΓJ,Γ,ρ))(\varepsilon(\Gamma^{*}),\varepsilon_{2}(\Gamma^{*},\rho^{*}),\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*}))=(-\varepsilon(\Gamma),\varepsilon_{2}(\Gamma,\rho),\varepsilon_{3}(\Gamma_{J},\Gamma,\rho)).

    w2w_{2}w1w_{1}vv
    w2w_{2}w1w_{1}vv
    Figure 14: Notations for the first two cases.
    In the first case, Γ\Gamma is on the left and Γ\Gamma^{*} on the right.
    In the second case, this is the other way.
  • Otherwise, Γc\Gamma_{c} is as in Figure 15 and ww is connected to an external trivalent vertex tt, where a leg from a univalent vertex xx arrives. In this case, Γ=Γ\Gamma^{*}=\Gamma and ρ=ρρx,w\rho^{*}=\rho\circ\rho_{x,w}, where ρx,w\rho_{x,w} is the transposition of xx and ww. We have ρ(w)ρ(v)=ρ(x)ρ(v)\rho^{*}(w)-\rho^{*}(v)=\rho(x)-\rho(v). This expression has the same (positive) sign as ρ(w)ρ(v)\rho(w)-\rho(v) since xx and ww are in V3V_{3} and vv is in V1V_{1}. Therefore, ε2(Γ,ρ)=ε2(Γ,ρ)\varepsilon_{2}(\Gamma,\rho^{*})=\varepsilon_{2}(\Gamma,\rho). Since we only changed the order of two internal vertices adjacent to the trivalent vertex tt, we have ε3(ΓJ,Γ,ρ)=ε3(ΓJ,Γ,ρ)\varepsilon_{3}(\Gamma_{J},\Gamma,\rho^{*})=-\varepsilon_{3}(\Gamma_{J},\Gamma,\rho).

vvwwttxx
Figure 15: Notations for the third case.

This yields an involution ((Γ,σ,ρ)𝒢(ΓJ,j)(Γ,σ,ρ)𝒢(ΓJ,j))\left((\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J},j)\mapsto(\Gamma^{*},\sigma^{*},\rho^{*})\in{\mathcal{G}}(\Gamma_{J},j)\right) as announced and we have ε(Γ)ε2(Γ,ρ)ε3(ΓJ,Γ,ρ)=ε(Γ)ε2(Γ,ρ)ε3(ΓJ,Γ,ρ)\varepsilon(\Gamma^{*})\varepsilon_{2}(\Gamma^{*},\rho^{*})\varepsilon_{3}(\Gamma_{J},\Gamma^{*},\rho^{*})=-\varepsilon(\Gamma)\varepsilon_{2}(\Gamma,\rho)\varepsilon_{3}(\Gamma_{J},\Gamma,\rho) for any (Γ,σ,ρ)𝒢(ΓJ,j)(\Gamma,\sigma,\rho)\in{\mathcal{G}}(\Gamma_{J},j). This concludes the proof of the lemma.∎

Lemmas 3.4, 3.5 and 3.6 and Lemma 2.8 conclude the proof of Proposition 3.3 so that Theorem 2.14 is proved.

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