1. Introduction
The Chern–Simons perturbation theory, established by M. Kontsevich in [ Reference Kontsevich13 ], S. Axelrod and I. M. Singer in [ Reference Axelrod and Singer1 ], gives invariants of a 3-manifold with an acyclic representation of the fundamental group. Here a representation is said to be acyclic if the local system given by the representation is acyclic.
In the construction of the Chern–Simons perturbation theory, a 4-chain called a propagator plays an important role. A propagator is a 4-chain in the two-point configuration space of a given 3-manifold satisfying several homological conditions. There are some variations and related invariants of the Chern–Simons perturbation theory. In particular there are some variations of the homological conditions.
R. Bott and A. S. Cattaneo gave a refinement of the Chern–Simons perturbation theoretical invariants via a purely topological construction in [ Reference Bott and Cattaneo2 , Reference Bott and Cattaneo3 ]. The homological condition for a propagator used in [ Reference Bott and Cattaneo2 , Reference Bott and Cattaneo3 ] is essentially equal to that for the Chern–Simons perturbation theory for the trivial representation by G. Kuperberg and D. P. Thurston in [ Reference Kuperberg and Thurston14 ]. Due to the homological conditions used in [ Reference Bott and Cattaneo2 , Reference Bott and Cattaneo3 ], the existence of propagators is not guaranteed in some cases. In [ Reference Cattaneo and Shimizu4 , Reference Shimizu18 ], Cattaneo and the author refined the homological conditions and then showed that there exist refined propagators in any case. We note that when the representation is trivial, the homological conditions given in [ Reference Bott and Cattaneo2 , Reference Bott and Cattaneo3 ] coincide with that given in [ Reference Kuperberg and Thurston14 ].
In [
Reference Shimizu18
], the author defined an invariant d, called a defect, of an acyclic representation. The defect d measures the difference between the homological conditions for Bott-Cattaneo’s propagators and that for refined propagators. The defect d equals to 0 when the representation is trivial. The defect d was first introduced by C. Lescop in [
Reference Lescop16
] for 3-manifold with
$b_1=1$
when she defined an invariant of 3-manifolds with
$b_1=1$
. Her invariant can be considered as a generalisation of the Chern–Simons perturbation theory for the maximal free abelian representation
$\rho_0\,:\,H=\langle t\rangle\to {\mathbb{Q}}(t)^{\times}$
of the 1-dimensional homology group H of the manifold. It was proved by Lescop in [
Reference Lescop16
] that the defect d (denoted by
$I_{\Delta}(M)$
in [
Reference Lescop16
]) can be computed from the Alexander polynomial of the 3-manifold. It was essentially proved also by M. Hutchings and Y. J. Lee in [
Reference Hutchings and Lee10
].
In this paper, we define an invariant
$d'(M,\rho;\,e)$
of a closed oriented 3-manifold M with an Euler structure e and an acyclic representation
$\rho$
as a refinement of d. An Euler structure is an equivalence class of non-vanishing vector fields on the manifold. See section 2·5 for more details on Euler structures. Note that d
′ coincides with d for an Euler structure associated to a parallelisation of M.
The invariant
$d'(M,\rho;\,e)$
is defined as a “twisted self-linking homology class” of the diagonal of
$M\times M$
. Let
$\Delta$
be the diagonal of
$M\times M$
. Take a non-vanishing vector field
$v_e$
of the normal bundle of
$\Delta$
in
$M\times M$
corresponding to the Euler structure e. Then we have a framed 3-manifold
$(\Delta, v_e)$
in
$M\times M$
. We introduce a kind of a self-linking number
$\text{self.lk}(\Delta, v_e)$
of
$(\Delta, v_e)$
with a twisted coefficient. Then we define
To define the self-linking homology class, we take a 4-chain in
$M\times M$
bounded by
$\Delta$
. This 4-chain is essentially equal to a propagator in the Chern–Simons perturbation theory.
Let
$\rho_0$
be the maximal free abelian representation. We show that
$d'(M,\rho_0;\,e)$
can be computed from the Reidemeister–Turaev torsion
$\text{Tor}(M,\rho_0;\,e)$
of M and e via an operator D defined by using logarithmic derivatives:
Theorem 1 (Section 5·2).
The Alexander polynomial can be computed from the Reidemeister–Turaev torsion. Thus Theorem 1 is a generalization of Lescop, Hutchings and Lee’s formula on the defect d to any closed oriented 3-manifolds. Actually we use an analogue of Hutchings–Lee’s argument in [
Reference Hutchings and Lee10
] in the proof Theorem 1. The operator D holds information of
$\text{Tor}(M,\rho_0;\,e)$
up to constant multiplication. Namely, Theorem 1 implies that the Reidemeister–Turaev torsion
$\text{Tor}(M,\rho_0;\,e)$
can be computed from
$d'(M,\rho_0;\,e)$
up to constant. Theorem 1 gives a geometric description of the Reidemeister–Turaev torsion as a twisted self-linking class.
The outline of the proof of Theorem 1 is as follows. By using a Morse function,
$d'(M,\rho;\,e)$
can be computed by counting the trajectories connecting critical points. Thus the core of the proof is to compare this counting and the Reidemeister–Turaev torsion. Hutchings and Lee in [
Reference Hutchings and Lee10
] showed that the counting of trajectories of a circle-valued Morse functions gives a Reidemeister–Turaev torsion of a representation related to the circle-valued Morse function. The core of our proof of Theorem 1 is an analogue of the computation in the proof of lemma 3·1 of [
Reference Hutchings and Lee10
]. However we have not found a direct proof of Theorem 1 from lemma 3·1 or related theorems in [
Reference Hutchings and Lee10
].
Remark 1·1. There are several works on geometric approaches to the Reidemeister torsion. M. Hutchings and Y. J. Lee gave a description of the Reidemeister–Turaev torsion by using circle-valued Morse functions in [ Reference Hutchings9–Reference Hutchings and Lee11 ]. H. Goda and A. V. Pajitnov in [ Reference Goda and Pajitnov8 ] and Goda, Matsuda, and A. V. Pajitnov in [ Reference Goda, Matsuda and Pajitnov7 ] gave a description of Reidemeister–Turaev torsion from the viewpoint of the dynamics of the gradient vector field of a circle-valued Morse function. They also established a method of computation of the Lefschetz zeta function which counts the closed orbits by using Heegaard splitting for twist knots and the pretzel knot of type (5,5,5). T. Kitayama in [ Reference Kitayama12 ] gave Morse theoretical description for the Reidemeister torsion for non-commutative representations in some cases. F. Deloup and G. Massuyeau in [ Reference Deloup and Massuyeau5 ] showed that a quadratic function given by the Reidemeister–Turaev torsion coincides with a quadratic form given by the intersection pairing of a cobordism.
The organisation of this paper is as follows. In section 2 we prepare some notation and conventions for orientations, local systems and Euler structures. In section 3 we review a definition of the Reidemeister–Turaev torsion. In section 4 we define the invariant d
′. In section 5 we introduce an operator D and then state Theorem 1 that
$d'=D(\text{Tor})$
for the maximal free abelian representation. In section 6 we give a Morse theoretic description of d
′ to prove Theorem 1 stated in section 5. In section 7 we give a proof of Theorem 1. In section 8 we explain the relation between the invariant d
′ and Lescop’s invariant.
2. Preliminaries
2·1. Orientation conventions
First we mention some conventions to fix an orientation. An interval
$[0,1]\subset {\mathbb{R}}$
is oriented from 0 to 1. Products of manifolds are oriented by the order of the factors. Boundaries of manifolds are oriented by the outward normal first convention. Let
$A, B\subset X$
be oriented submanifolds of an oriented manifold X. We assume that A is transversal to B and
$A\cap B\not =\emptyset$
. Let
$\nu A$
be a normal bundle of A in X. We adopt the following conventions on orientations:
-
(O1)
$T_xA\oplus \nu_xA=T_xX$
, for
$x\in A$
. -
(O2)
$\nu_x(A\cap B)=\nu_x A\oplus \nu_x B$
. -
⇒ (O3)
$T_x(A\cap B)\oplus \nu_xA\oplus \nu_xB=T_xX$
. -
(O4) (The outward normal first convention) For an oriented manifold with a boundary W and
$x\in \partial W$
, Here
\begin{align*}n_x\oplus T_x\partial W=T_xW.\end{align*}
$n_x$
is a outward normal vector at
$x\in\partial W$
.
-
(O5) Let
$\pi\,:\,\widetilde X\to X$
be an F-bundle, where
$\widetilde X,X$
and F are orientable manifolds. Let
$U\subset X$
be an open set so that
$\pi|_U$
is trivial. We choose orientations of
$\widetilde X, X$
and F such that the condition
$\pi^{-1}(U)=U\times F$
holds.
2·2. Local systems
Let M be a closed oriented 3-manifold.
Let
$\Pi(M)$
be the “fundamental groupoid” of M; namely
$\Pi(M)$
is a category such that the objects are the points of M and a morphism from
$x\in M$
to
$y\in M$
is a path from x to
$y\in M$
up to homotopy relative to x, y. In particular, a morphism from a point
$x\in M$
to x is an element of the fundamental group
$\pi_1(M,x)$
. A “local system” over M is a covariant functor from
$\Pi(M)$
to a category of vector spaces. We denote by
$\gamma_*$
the isomorphism corresponding to a path
$\gamma$
via the local system. Let E be a vector space over a field F. For a representation
$\rho\,:\,\pi_1(M,x)\to \text{GL}(E)$
, there is a local system on M such that each object is isomorphic to E and
$\gamma_*=\rho(\gamma)$
for any
$\gamma\in \pi_1(M,x)$
. We call such a local system the local system corresponding to
$\rho$
and we use the same symbol
$\rho$
for the local system. We denote by
$C_*(M;\,\rho)$
or
$H_*(M;\,\rho)$
chain complexes or homology groups with the local coefficient
$\rho$
respectively.
Let
$V^*=\text{Hom}(V,F)$
be the dual vector space of V. For a representation
$\rho\,:\,\pi_1(M)\to \text{GL}(V)$
, we denote by
$\rho^*\,:\,\pi_1(M)\to \text{GL}(V^*)$
the dual representation of
$\rho$
, namely
$\rho^*$
is given by
for
$h\in \pi_1(M)$
and
$f\in V^*$
.
2·3. Chains with local coefficients
Let X be a manifold. Let E be a vector space and let
$\rho$
be a local system corresponding to a representation
$\rho\,:\,\pi_1(X)\to \text{GL}(E)$
. Let
$c\,:\,(A,a)\to (X,c(a))$
be a continuous map, where A is a compact oriented manifold with a basepoint
$a\in A$
. We denote by
$E_{c(a)}^{c_*\pi_1(A,a)}$
the invariant part of
$E_{c(a)}$
under the action of
$c_*\pi_1(A,a)\lt\pi_1(X,c(a))$
via the representation
$\rho$
. Take an element
$e\in E_{c(a)}^{c_*\pi_1(A,a)}$
. Then c and
$e\in E_{c(a)}$
give a
$(\dim A)$
-dimensional chain. We denote this chain by
or shortly,
For a chain
$\alpha=\langle c,a;\,n\in{\mathbb{Z}}\rangle \in C_*(X;\,{\mathbb{Z}})$
and an element
$e\in E_{c(a)}^{c_*\pi_1(A,a)}$
, we have a chain
$\langle c,a;\,ne\rangle \in C_*(X;\,E)$
. To simplify the notation, we denote it by
$\alpha\otimes e$
. Since any chain of
$C_*(X;\,{\mathbb{Z}})$
is given as a weighted sum of singular simplexes,
$\alpha\otimes e$
is defined for any
$\alpha\in C_*(X;\,{\mathbb{Z}})$
.
Let F be a compact oriented manifold. Let
$\pi\,:\,\widetilde X\to X$
be a F-bundle over X. A homomorphism
$\rho\circ \pi_*\,:\,\pi_1(\widetilde{X})\stackrel{\pi_*}{\to}\pi_1(X)\to \text{GL}(E)$
gives a local system on
$\widetilde X$
. Let
$c=\langle A\to X,a;\,e\rangle\in C_k(X;\,E)$
be a k-chain. We denote by
$c^*\widetilde X\to A$
the pull back of
$\pi\,:\,\widetilde X\to X$
along c. Then we have a bundle map
$\widetilde c\,:\,c^*\widetilde X\to \widetilde X$
induced by
$c\,:\,A\to X$
.

By using
$\widetilde c$
, the
$(k+\dim F)$
-chain
$\pi^!c\in C_{k+\dim F}(\widetilde X;\,\pi^*E)$
can be described as follows:
Here
$v_a\in \pi^{-1}(a)$
is any point.
2·4. The maximal free abelian representation
$\rho_0$
Let us denote
$H=H_1(M;\,{\mathbb{Z}})/\text{Tor}$
. We fix a basis
We interpret H as a multiplicative group. In this paper, however, the operations of all homology groups including
$H_1(M;\,{\mathbb{Z}})$
are summation with the exception of H:
$\quad\quad\quad\quad\quad\quad\quad\quad\quad\quad\quad\quad H=\{t_1^{n_1}\cdots t_k^{n_k}\mid n_i\in {\mathbb{Z}}\}.$
Footnote
1
For
$h\in H$
, we denote by
the element of
$H_1(M;\,{\mathbb{Z}})/\text{Tor}$
corresponding to h. For example,
$[t_1^2t_2]_+=2t_1+t_2$
.
Let
\begin{align*}{\mathbb{R}} H=\left\{\sum_{n_1,\ldots,n_k}a_{n_1,\ldots,n_k}t_1^{n_1}\cdots t_k^{n_k}\mid \text{finitely many non-zero }a_{n_1,\ldots,n_k}\in {\mathbb{R}}\right\}\end{align*}
be the group ring of H over
${\mathbb{R}}$
and let
be the quotient field of
${\mathbb{R}} H$
. By using the basis, Q(H) can be identified with
Let
$\rho_0\,:\,{\mathbb{R}} H\to Q(H)$
be the inclusion given by
$\rho_0(\,f)={f}/{1}$
. We also use the same symbol
$\rho_0$
for the restriction of
$\rho_0$
to H. Since Q(H) is a 1-dimensional vector space over Q(H), the representation
$\rho_0\,:\,H\to \text{GL}(Q(H))=Q(H)^{\times}$
gives a representation of
$\pi_1(M)$
. Then there is a local system corresponding to
$\rho_0$
.
We assume that
$\rho_0$
is acyclic. Namely, the corresponding local system is acyclic:
2·5. Euler structures
As a general reference for Euler structures, for example, see [
Reference Turaev19
]. Let
$v,v'\in\Gamma TM$
be non-vanishing vector fields on M. We say that v and v’ are homologous, denoted by
$v\sim v'$
, if
$v|_{M\setminus \mathring{B}^3}$
is homotopic to
$v'|_{M\setminus \mathring{B}^3}$
as non-vanishing vector fields on
$M\setminus \mathring{B}^3$
for a ball
$B^3\subset M$
. A smooth Euler structure, or shortly Euler structure, on M is a homology class of non-vanishing vectors field on M. We denote by
$\text{Eul}(M)$
the set of all Euler structures on M:
Let
$s\in \Gamma TM$
be a vector field on M which is transversal to the 0-section 0. Then
$s^{-1}(0)$
is a 0-dimensional manifold consisting of finitely many singular points. The orientation
$\pm1$
of each point
$p\in s^{-1}(0)$
is defined as follows: The orientation of each fiber of the tangent bundle TM is induced from the orientation of M. Then TM is oriented. An orientation of the image of a section
$s(M)\subset TM$
is induced from the orientation of M. Then an orientation of p is defined as the orientation of the intersection
$0(M)\cap s(M)$
at p. Note that if
$s=-{\textrm{grad}}\,f$
, the opposite of a gradient-like vector field of a Morse function f on M, the orientation of each singular point p coincides with
$(-1)^{\dim M-\text{ind}(p)}=(-1)^{\text{ ind}(p)+1}$
. Here
$\text{ind}(p)$
is the Morse index of p. Let
$k=\sharp s^{-1}(0)/2$
.
Definition 2·1. An Euler chain for s is an embedding
$c=\sqcup_1^k(c_i\,:\,[0,1]\to M)$
of disjoint intervals satisfying
$\sqcup_i c_i(\partial[0,1])=s^{-1}(0)$
as oriented 0-manifolds.
From s and an Euler chain c, we construct an Euler structure on M. Let
$N(c_1),\ldots, N(c_k)\subset M$
be disjoint neighbourhoods of
$c_1([0,1]),\ldots,c_k([0,1])$
respectively such that each
$N(c_i)$
is diffeomorphic to a Ball
$B^3$
. In each
$N(c_i)$
, there are two singular points. Since the orientation of the two singular points are opposite,
$s_0|_{\partial N(c_i)}$
can be extended to
$N(c_i)$
as a non-vanishing vector field. By replacing each
$s|_{N(c_i)}$
with a non-vanishing vector field, we have a non-vanishing vector field on M. We denote by
such a non-vanishing vector field. There are several choices of
$s/c$
. The Euler structure
represented by a non-vanishing vector field
$s/c$
is, however, uniquely determined from s and c.
For later sections, we give a more concrete construction of
$s/c$
. Let
$p_2\,:\,[0,1]\times M\to M$
be the projection. Then
$p_2^*TM$
is an
${\mathbb{R}}^3$
-bundle over
$[0,1]\times M$
. Let
$\widetilde c_i$
be a 1-manifold of
$[0,1]\times M$
defined by
Then
$\widetilde c_i$
is a lift of
$c_i$
along
$p_2$
. Set
$c=\sqcup_{i=1}^k\widetilde{c_i}$
.
Lemma 2·2. There exists a homotopy
$\widetilde{s}=\{s_t\in \Gamma TM\}_{t\in [0,1]}$
satisfying the following conditions:
-
(i)
$\widetilde s$
is transversal to 0 as a section of
$p_2^*TM$
; -
(ii)
$s_0=s$
; -
(iii)
$\widetilde s^{-1}(0)=\sqcup_{i=1}^k \widetilde c_i([0,1])$
. In particular,
$s_1$
is a non-vanishing vector field; -
(iv)
$s_t|_{M\setminus \sqcup_{i=1}^k \mathring{N}(c_i)}=s_0|_{M\setminus \sqcup_{i=1}^k \mathring{N}(c_i)}$
for any
$t\in [0,1]$
.
Proof. By applying the Pontrjagin–Thom construction, we can take a vector field
$\widetilde{u_i}\in \Gamma(p_2^*TM)|_{[0,1]\times N(c_i)}$
satisfying conditions (i)-(iv) on
$N(c_i)\times [0,1]$
. Then
$\widetilde s=p_2^*s_0|_{[0,1]\times (M\setminus \sqcup_{i=1}^k N(c_i))}\cup (\sqcup_i \widetilde{u_i})$
satisfies the required conditions.
Let
$\widetilde{s'}=\{s'_t\}_{t\in [0,1]}$
be an alternative choice of
$\widetilde{s}$
. By condition (iv), we have
$s_1'=s_1$
on
$M\setminus \sqcup_iN(c_i)$
. Then
$s_1$
is homologous to
$s_1'$
. Namely, the Euler structure
$[s_1]\in \text{Eul}(M)$
does not depend on the choice of
$\widetilde{s}=\{s_t\}_{t\in [0,1]}$
in lemma 2·2. Therefore we set
3. The Reidemeister–Turaev torsion
$\text{Tor}(M,\rho;\,e)$
Let e be an Euler structure on M. Let
$\rho\,:\,\pi_1(M)\to GL_F(V)$
be an acyclic representation of
$\pi_1(M)$
on a vector space V over a field F. The Reidemeister–Turaev torsion
is an invariant of
$(M,\rho;\,e)$
defined by V. Turaev as a refinement of the Reidemeister torsion. The Reidemeister–Turaev torsion is defined by using a chain complex associated with a CW structure on M. In this section, we review a definition of
$\text{Tor}(M,\rho;\,e)$
by using a Morse–Smale complex of M. As a general reference for the Reidemeister–Turaev torsion, for example, see [
Reference Turaev20
] or [
Reference Turaev21
].
Let
$f\,:\,M\to {\mathbb{R}}$
be a Morse function and let
${\textrm{grad}}\, f$
be a gradient-like vector field of f. We denote by
${\textrm{Crit}}_i(\,f)$
the set of critical points of index i. Let
${\textrm{Crit}}(\,f)=\sqcup_i{\textrm{Crit}}_i(\,f)$
. Let
$C_*^{\kern0.5pt f}=(C_i^{\kern0.5pt f}(M;\,\rho),\partial^{\kern0.5pt f}_i\,:\,C_i^{\kern0.5pt f}(M,\rho)\to C_{i-1}^{\kern0.5pt f}(M,\rho))_i$
where
$C_i^{\kern0.5pt f}(M;\,\rho)=\oplus_{p\in {\textrm{Crit}}_i(\,f)}V_p$
be the Morse–Smale complex of
$-{\textrm{grad}}\, f$
. Since
$\rho$
is acyclic, there exist homomorphisms
satisfying
Then
$\partial^{\kern0.5pt f}+g^{\kern0.5pt f}$
gives an isomorphism
Here
$C_{even}=C_2^{\kern0.5pt f}(M;\,\rho)\oplus C_0^{\kern0.5pt f}(M;\,\rho)$
and
$C_{odd}=C_3^{\kern0.5pt f}(M;\,\rho)\oplus C_1^{\kern0.5pt f}(M;\,\rho)$
.
Take an Euler chain
$c_f=\sqcup_{i=1}^k c_i$
for
$-{\textrm{grad}}\, f$
satisfying
$[-{\textrm{grad}}\, f/c_f]=e$
. Here
$k=\sharp {\textrm{Crit}}(\,f)/2$
. Each
$c_i$
gives an isomorphism from
$V_{c_i(0)}$
to
$V_{c_i(1)}$
. Then
$c_f$
gives an isomorphism between
$C_{even}$
and
$C_{odd}$
. We denote by
$(c_f)_*\,:\,C_{odd}\stackrel{\cong}{\to} C_{even}$
this isomorphism. Then we have an isomorphism
It is known that the determinant of
$(c_f)_*\circ (\partial^{\kern0.5pt f}+g^{\kern0.5pt f})$
is an invariant of M and e up to sign.
Definition 3·1. The Reidemeister–Turaev torsion of
$(M,\rho;\,e)$
is defined to be
4. The invariant
$d'(M,\rho;\,e)$
For a closed oriented 3-manifold M, an acyclic representation
$\rho\,:\,\pi_1(M)\to \text{GL}(V)$
and an Euler structure
$e\in \text{Eul}(M)$
, we define an invariant
of
$(M,\rho;\,e)$
. The invariant
$d'(M,\rho;\,e)$
is a refinement of an invariant d for M and
$\rho_0$
defined in [
Reference Shimizu18
]. See Remark 4·6 for more details.
4·1 Preparation for local systems
Thanks to the Künneth theorem,
$\rho^*\boxtimes \rho\,:\,\pi_1(M\times M)=\pi_1(M)\times \pi_1(M)\to \text{GL}(V^*\otimes V)$
gives an acyclic local system on a 6-dimensional manifold
$M\times M$
. Here
$\rho^*\boxtimes \rho$
is the exterior tensor product of
$\rho$
and
$\rho^*$
.
Let
$\Delta=\{(x,x)\mid x\in M\}\subset M\times M$
be the diagonal. We orient
$\Delta$
so that a diffeomorphism
$M\ni x\mapsto (x,x)\in \Delta$
preserves the orientation. The restriction of
$\rho^*\boxtimes \rho$
to
$\Delta$
is
$\rho^*\otimes \rho$
. The identity map
$1\in V^*\otimes V=\text{Hom}(V,V)$
is invariant under the action of
$\pi_1(M)$
via
$\rho^*\otimes \rho$
. Then for any chains
$c \in C_*(\Delta;\,{\mathbb{Z}})$
, we have a chain
$c\otimes 1\in C_*(\Delta;\,\rho^*\otimes \rho)$
.
We now consider
$\rho_0\,:\,\pi_1(M)\to Q(H)^{\times}$
. Since Q(H) is a 1-dimensional vector space,
$\rho^*\otimes \rho$
is trivial and spanned by 1. Thus we have
4·2. A twisted self-linking number of a link
The invariant
$d'(M,\rho;\,e)$
is defined as a “twisted self-linking 1-dimensional homology class” of an embedded 3-manifold in a 6-manifold with local coefficients. Then we first review the usual linking number of a link.
For a 2-component oriented link
$K_1\sqcup K_2\subset S^3$
, the linking number
$\text{lk}_{S^3}(K_1,K_2)\in {\mathbb{Z}}$
is defined as follows: Take a 2-chain
$\widetilde{K_1}\in C_2(S^3;\,{\mathbb{Z}})$
satisfying
$\partial \widetilde{K_1}=K_1$
(we note that we can take a Seifert surface of
$K_1$
as a
$\widetilde{K_1}$
). Then
$\text{lk}_{S^3}(K_1,K_2)$
is defined by
$\text{lk}_{S^3}(K_1,K_2)=[\widetilde K_1]\cap [K_2]\in H_0(K_2;\,{\mathbb{Z}})={\mathbb{Z}}$
. Let v be a normal vector field of
$K_1$
in
$S^3$
. The self-linking number
of a framed knot
$(K_1,v)$
is defined as a linking number of
$K_1$
and
$v(K_1)$
. Here
$v(K_1)$
is a copy of
$K_1$
given by pushing
$K_1$
along v.
4·3. A twisted self-linking homology class of an embedded 3-manifold
Let
$Y_1,Y_2$
be closed 3-manifolds embedded in a closed 6-manifold X satisfying
$Y_1\cap Y_2=\emptyset\subset X$
. Let
$\tau\,:\,\pi_1(X)\to \text{GL}(E)$
be a representation, where E is a vector space. We assume that they satisfy the following conditions:
-
(i)
$\tau$
is acyclic:
$H_*(X;\,\tau)=0$
; -
(ii) There is a special element
$1\in E$
such that 1 is invariant under the action of
$\pi_1(M)$
.
Since
$[Y_1]\otimes 1=0\in H_3(X;\,\tau)=0$
, there exists a 4-chain
$\widetilde{Y_1}\otimes 1\in C_4(X;\,\tau)$
satisfying
$\partial \widetilde{Y_1}=Y_1$
. The intersection of
$[\widetilde{Y_1}]\in H_4(X,Y_1;\,\tau)$
and
$[Y_2]\in H_3(Y_2;\,{\mathbb{Z}})$
gives a 1-dimensional homology class
$[\widetilde{Y_1}]\cap[Y_2]=[\widetilde{Y_1}\cap Y_2]\in H_1(Y_2;\,\tau)$
.
Lemma 4·1. Let
$\widetilde{Y_1}, \widetilde{Y_1}'\in C_4(X;\,\tau)$
be 4-chains satisfying
$\partial\widetilde{Y_1}=\partial\widetilde{Y_1}'=Y_1\otimes 1$
. Then
$[\widetilde{Y_1}]\cap [Y_2]=[\widetilde{Y_1}']\cap [Y_2]\in H_1(Y_2;\,\tau).$
Proof. The homology class
$[\widetilde{Y_1}]\cap[Y_2]-[\widetilde{Y_1}']\cap[Y_2]=[\widetilde{Y_1}-\widetilde{Y_1}']\cap [Y_2]$
is in the image of the morphism
Since
$\tau$
is acyclic,
$H_4(X;\,\tau)=0$
. Then
$[\widetilde{Y_1}-\widetilde{Y_1}']\cap [Y_2]=0$
.
This lemma implies that a twisted linking homology class is well defined:
Definition 4·2.
If there is a non-vanishing vector field v of the normal bundle of
$Y_1$
in X, we can formulate a self-linking homology class of the framed 3-manifold
$(Y_1,v)$
. Let
$v(Y_1)\subset X$
be a parallel copy of
$Y_1$
given by pushing
$Y_1$
along v.
Definition 4·3. The twisted self-linking homology class of
$(Y_1,v)$
is defined to be
More precisely,
$v(Y_1)\subset X$
is obtained as follows: Let
$\nu_{Y_1}$
be the normal bundle of
$Y_1$
in X. Set
$D\nu_{Y_1}=\{(x,v)\mid \|v\|\le 1\}$
.
$D\nu_{Y_1}$
forms a
$D^3$
-bundle over
$Y_1$
. Let
$S\nu_{Y_1}=\partial D\nu_{Y_1}$
be the unit sphere bundle. Let
$N(Y_1)\subset X$
be a closed tubular neighbourhood of
$Y_1$
. We identify
$D\nu_{Y_1}$
with
$N(Y_1)$
. We denote by
$\pi\,:\, \partial N(Y_1)\to Y_1$
and
$\pi\,:\, N(Y_1)\to Y_1$
the projections. We identify the local system
$\tau|_{N(Y_1)}=\pi^*\tau$
with
$\tau$
via
$\pi^*$
. The normalisation
${v}/{\|v\|}$
of the non-vanishing vector field v is a section of the
$S^2$
-bundle
$\partial N(Y_1)\to Y_1$
. Then set
Here
$v(Y_1)$
is oriented by
$v\,:\,Y_1\stackrel{\cong}{\to} v(Y_1)$
.
4·4. An invariant
$d'(M,\rho;\,e)$
Take a non-vanishing vector field
$v_e$
representing the Euler structure e. We identify the normal bundle
$\nu_{\Delta}$
with the tangent bundle TM via the following isomorphism:
where
$x\in M,v\in T_xM$
. Then
$v_e$
gives a non-vanishing vector field of
$\nu_{\Delta}$
. An invariant
$d'(M,\rho;\,e)$
is defined to be a twisted self-linking homology class of
$(\Delta,v_e)$
:
Definition 4·4.
Remark 4·5. The invariant
$d'(M,\rho;\,e)$
can be described by using some isomorphisms between homology groups.
Let
be the connecting homomorphism in the long exact sequence of homologies of the pair
$(M^2,M^2\setminus \mathring{N}(\Delta))$
. Here
$N(\Delta)$
is oriented as a part of
$M^2$
. Since
$H_4(M^2;\,\rho^*\boxtimes \rho)=0$
and
$H_3(M^2;\,\rho^*\boxtimes \rho)=0$
,
$\partial_*$
is an isomorphism. Let
be an excision isomorphism. Let
be the Thom isomorphism. Here the sign convention for the Thom isomorphism
$\psi$
is as follows: For a 4-chain
$\alpha$
in
$M^2$
representing a cycle in
$C_4(N(\Delta),\partial N(\Delta);\,\rho^*\boxtimes \rho)$
, an equation
$\psi(\alpha)=\alpha\cap \Delta$
holds.
Therefore we have an isomorphism
By the definition of twisted self-linking homology class,
$d'(M,\rho;\,e)$
can be written as follows:

Remark 4·6. An invariant
$d(\rho_0)$
defined in [
Reference Shimizu18
] can be computed from d′ as follows:
Here
$e_0$
is an Euler structure associated to a parallelisation of M.
5. Main theorem
To describe the main theorem, we first introduce an operator D.
5·1. An operator D
In this section, we introduce an operator
$D\,:\,Q(H)^{\times}\to\left(H_1(M;\,{\mathbb{Z}})/\text{Tor}\right)\otimes_{{\mathbb{Z}}} Q(H)$
. Recall that for
$h\in H$
,
$[h]_+\in H_1(M;\,{\mathbb{Z}})/\text{Tor}$
is the element corresponding to h. We first define D on
${\mathbb{R}} H\setminus 0$
.
Definition 5·1.
For
$f=\sum_{h\in H}a_hh\in {\mathbb{R}} H\setminus 0 (a_h\in {\mathbb{R}})$
, we set
\begin{align*}\displaystyle{D(\,f)=D\left(\sum_{h\in H}a_hh\right)=\sum_h[h]_+\otimes \frac{a_hh}{f}}.\end{align*}
Example 5·2. Let
$H=\langle t_1,t_2\rangle$
.
\begin{eqnarray*}&&D(1+t_1^3+t_1^2t_2^6)\\ &=&[1]_+\otimes \frac{1}{1+t_1^3+t_1^2t_2^6}+[t_1^3]_+\otimes\frac{t_1^3}{1+t_1^3+t_1^2t_2^6}+[t_1^2t_2^6]_+\otimes\frac{t_1^2t_2^6}{1+t_1^3+t_1^2t_2^6}\\ &=&0\otimes \frac{1}{1+t_1^3+t_1^2t_2^6}+3[t_1]_+\otimes\frac{t_1^3}{1+t_1^3+t_1^2t_2^6}+(2[t_1]_++6[t_2]_+)\otimes\frac{t_1^2t_2^6}{1+t_1^3+t_1^2t_2^6}\\ &=&[t_1]_+\otimes \frac{3t_1^3+2t_1^2t_2^6}{1+t_1^3+t_1^2t_2^6}+[t_2]_+\otimes \frac{6t_1^2t_2^6}{1+t_1^3+t_1^2t_2^6}.\end{eqnarray*}
Lemma 5·3.
-
(i) For any
$f,g\in {\mathbb{R}} H\setminus 0$
satisfying
$f+g\not=0$
,
$D(f+g)=(1\otimes \frac{f}{f+g})D(\,f)+(1\otimes \frac{g}{f+g})D(g)$
. -
(ii) For any
$f,g\in {\mathbb{R}} H\setminus 0$
,
$D(fg)=D(\,f)+D(g)$
.
Proof. (i) Let
$f=\sum_ha_hh, g=\sum_hb_hh$
. We have
\begin{eqnarray*}&&\left(1\otimes \frac{f}{f+g}\right)D(\,f)+\left(1\otimes \frac{g}{f+g}\right)D(g)\\ &=& \sum_h[h]_+\otimes \left(\frac{f}{f+g}\cdot\frac{a_hh}{f}+\frac{g}{f+g}\cdot\frac{b_hh}{g}\right)\\ &=& \sum_h[h]_+\otimes \left(\frac{a_hh}{f+g}+\frac{b_hh}{f+g}\right)\\ &=&D(f+g).\end{eqnarray*}
(ii) Let
$f=\sum_ha_hh, g=\sum_{h'}b_{h'}h'$
. Then
$fg=\sum_{h,h'}a_hb_{h'}hh'$
. We have
\begin{eqnarray*}D(fg)&=& \sum_{h,h'}[hh']_+\otimes \frac{a_hb_{h'}hh'}{fg}\\ &=& \sum_{h,h'}([h]_++[h']_+)\otimes \frac{a_hb_{h'}hh'}{fg}\\ &=& \sum_{h,h'}[h]_+\otimes \frac{a_hb_{h'}hh'}{fg}+\sum_{h,h'}[h']_+\otimes \frac{a_hb_{h'}hh'}{fg}\\ &=& \sum_{h}\left([h]_+\otimes \sum_{h'}\frac{a_hb_{h'}hh'}{fg}\right)+\sum_{h'}\left([h']_+\otimes \sum_{h}\frac{a_hb_{h'}hh'}{fg}\right)\\ &=& \sum_{h}\left([h]_+\otimes \frac{a_hh}{f}\frac{\sum_{h'}b_{h'}h'}{g}\right)+\sum_{h'}\left([h']_+\otimes \frac{b_{h'}h'}{g}\frac{\sum_ha_hh}{f}\right)\\ &=& \sum_{h}\left([h]_+\otimes \frac{a_hh}{f}\right)+\sum_{h'}\left([h']_+\otimes \frac{b_{h'}h'}{g}\right)\\ &=& D(\,f)+D(g).\end{eqnarray*}
As a direct consequence of the above lemma, we have the following corollary.
Corollary 5·4. Let
$f_1,g_1,f_2,g_2\in {\mathbb{R}} H\setminus 0$
. If
$g_1/f_1=g_2/f_2\in Q(H)$
then
Proof. It is enough to show that for any
$h\in {\mathbb{R}} H\setminus 0$
,
$D(g_1h)-D(f_1h)=D(g_1)-D(h_1)$
. Thanks to lemma 5·3 (ii), we have
The corollary guarantees that D can be extended to
$Q(H)^{\times}$
as follows:
Definition 5·5.
$D(g/f)=D(g)-D(\,f)$
for
$g/f\in Q(H)^{\times}$
.
Let
$x_1,\ldots,x_m$
be arbitrary elements of H. We next give an explicit formula of D(f) for any rational function
$f(x_1,\ldots, x_m)\in Q(H)^{\times}$
in the language of
$x_1,\ldots,x_m$
:
Proposition 5·6. For any rational function
$f(x_1,\ldots,x_m)\in Q(H)^{\times}$
of
$x_1,\ldots,x_m$
,
In particular, for any monomial
$ax_1^{n_1}\cdots x_m^{n_m}\in {\mathbb{R}} H$
, where
$a\in{\mathbb{R}}\setminus 0$
and
$n_1,\ldots,n_m\in{\mathbb{Z}}$
, we have
Proof. Set
$D'(\,f)=\sum_{i=1}^m\left([x_i]_+\otimes \frac{x_i}{f}\frac{\partial f}{\partial x_i}\right)$
for
$f=f(x_1,\ldots,x_m)$
. Clearly, D
′ satisfies the following properties:
-
(i)
$D'(a)=0$
for any
$a\in{\mathbb{R}}\setminus 0$
; -
(ii)
$D'(x_i)=[x_i]_+\otimes 1$
for
$i=1,\ldots,m$
; -
(iii)
$D'(f+g)=(1\otimes \frac{f}{f+g})D'(\,f)+(1\otimes \frac{g}{f+g})D'(g)$
for any polynomials
$f,g\in {\mathbb{R}} H\setminus 0$
satisfying
$f+g\not=0$
. -
(iv)
$D'(fg)=D'(\,f)+D'(g)$
for rational functions f, g of
$x_1,\ldots,x_m$
such that
$f\not=0, g\not=0$
.
Any rational function of
$x_1,\ldots,x_m$
can be written as a quotient of polynomials of
$x_1,\ldots,x_m$
, and any polynomial of
$x_1,\ldots,x_m$
can be written as a linear combination of products of
$x_1,\ldots,x_m$
. Thus we can compute D
′ completely by the properties (i), (ii), (iii) and (iv). Then
$D'=D$
for any rational functions of
$x_1,\ldots,x_m$
.
Example 5·7. Let
$t_1,t_2\in H$
and
$f=1+t_1^3+t_1^2t_2^6$
.
\begin{eqnarray*}D(\,f)&=&[t_1]_+\otimes \frac{t_1}{f}\frac{\partial}{\partial t_1}(1+t_1^3+t_1^2t_2^6)+[t_2]_+\otimes \frac{t_2}{f}\frac{\partial}{\partial t_2}(1+t_1^3+t_1^2t_2^6)\\ &=&[t_1]_+\otimes \frac{3t_1^3+2t_1^2t_2^6}{f}+[t_2]_+\otimes \frac{6t_1^2t_2^6}{f}.\end{eqnarray*}
Let
$T=t_1^2\in H$
. Then
$f=1+t_1^3+t_1^2t_2^6$
can be represented as
$f(t_1,t_2,T)=1+t_1T+t_2^6T$
. Then
\begin{eqnarray*}&&D(1+t_1T+t_2^6T)\\ &=&[t_1]_+\otimes \frac{t_1}{f}\frac{\partial}{\partial t_1}(1+t_1T+t_2^6T)+[t_2]_+\otimes \frac{t_2}{f}\frac{\partial}{\partial t_2}(1+t_1T+t_2^6)\\ &&+[T]_+\otimes \frac{T}{f}\frac{\partial}{\partial T}(1+t_1T+t_2^6T)\\ &=&[t_1]_+\otimes \frac{t_1T}{f}+[t_2]_+\otimes \frac{6t_2^6T}{f}+[T]_+\otimes \frac{t_1T+t_2^6T}{f}\\ &=&[t_1]_+\otimes \frac{t_1^3}{f}+[t_2]_+\otimes \frac{6t_1^3t_2^6}{f}+2[t_1]_+\otimes \frac{t_1^3+t_1^2t_2^6}{f}\\ &=&[t_1]_+\otimes \frac{3t_1^3+2t_1^2t_2^6}{f}+[t_2]_+\otimes \frac{6t_1^3t_2^6}{f}.\end{eqnarray*}
5·2. Main theorem
Recall that for the maximal free abelian representation
$\rho_0$
,
The following theorem is the main theorem of this paper.
Example 5·8. Let
$M=S^1\times S^2$
. In this case
$H=H_1(M;\,{\mathbb{Z}})=\langle t\rangle$
. Here
$t\in H$
is represented by
$S^1\times \{\text{pt}\}$
for a point
$\text{pt}\in S^2$
. It is known that, for a suitable Euler structure e, the Reidemeister–Turaev torsion is given as
Thus
6. Morse theoretic description of
$d'(M,\rho;\,e)$
To prove Theorem 1, we give a Morse theoretic description of
$d'(M,\rho;\,e)$
. In sections 6·1 and 6·2, we prepare notations on a Morse function and manifolds. In section 6·3 we give a description of
$d'(M,\rho;\,e)$
by using a Morse function.
6·1. A Morse function and a combinatorial propagator
Recall that
$d'(M,\rho;\,e)$
is defined to be a twisted self-linking homology class of
$\Delta\subset M\times M$
. Thus
$d'(M,\rho;\,e)$
can be computed from a 4-chain
$\Sigma^0_f$
of
$C_4(M^2;\,\rho_0^*\boxtimes \rho_0)$
bounded by
$v_{e}(\Delta)\otimes 1$
. We give
$\Sigma_0^{\kern0.5pt f}$
explicitly by using a Morse function. The description is related to the construction in [
Reference Shimizu17
,
Reference Shimizu18
]. It is inspired by [
Reference Fukaya6
,
Reference Watanabe22
].
Take a Morse function
$f\,:\,M\to {\mathbb{R}}$
and a gradient-like vector field
${\textrm{grad}}\, f$
of f satisfying the Morse–Smale condition. We denote by
$\text{Crit}_i(\,f)$
the set of critical points of index i and set
$\text{Crit}(\,f)=\sqcup_i\text{Crit}_i(\,f)$
.
Let
$(\Phi_t^{\kern0.5pt f}\,:\,M\stackrel{\cong}{\to} M)_{t\in{\mathbb{R}}}$
be the one-parameter family of diffeomorphisms associated to
$-{\textrm{grad}}\, f$
. For
$p\in \text{Crit}(\,f),$
let
$\mathcal{A}_p$
and
$\mathcal{D}_p$
be the ascending manifold of p and the descending manifold of p respectively:
We orient
$\mathcal A_p$
and
$\mathcal D_p$
so that the condition
$T_p\mathcal A_p\oplus T_p\mathcal D_p=T_pM$
is satisfied. Let
$\mathcal M(p,q)$
be the set of all trajectories from
$p\in\text{Crit}_i(\,f)$
to
$q\in\text{Crit}_{i-1}(\,f)$
:
Here
$s\in {\mathbb{R}}$
acts as
$s\cdot\gamma(t)=\gamma(t+s)$
. A trajectory
$\gamma$
gives an isomorphism
$\gamma_*\,:\,V_p\stackrel{\cong}{\to} V_q$
. Let
$\gamma_{\downarrow}$
be an oriented 1-manifold given by the closure of
$\gamma({\mathbb{R}})$
with the downward orientation (the direction from p to q). Let
$\gamma_{\cap}$
be an oriented 1-manifold given as a closure of
$\gamma({\mathbb{R}})$
oriented as the intersection
$\mathcal A_q\cap\mathcal D_p$
in M.
By using the orientation of
$\gamma_{\cap}$
, we assign a sign
${\varepsilon}(\gamma)\in\{+1,-1\}$
for each
$\gamma\in\mathcal M(p,q)$
such that the equality
holds. We denote by
$C_*^{\kern1.5pt f}=(C_i^{\kern1.5pt f}(M;\,\rho),\partial^{\kern0.5pt f}_i\,:\,C_i^{\kern1.5pt f}(M;\,\rho)\to C_{i-1}^{\kern1.5pt f}(M;\,\rho))_i$
the Morse–Smale complex of f, namely
$C_i^{\kern0.5pt f}(M;\,\rho)=\oplus_{p\in\text{Crit}_i(\,f)}V_p$
and
for any
$x\in V_p$
and
$p\in \text{Crit}_i(\,f)$
.
Take homomorphisms
$g^{\kern0.5pt f}=\{g_i^{\kern1pt f}\,:\,C_{i-1}^{\kern1.5pt f}(M;\,\rho)\to C_i^{\kern1.5pt f}(M;\,\rho)\}_{i=1,2,3,4}$
satisfying
as in the definition of
$\text{Tor}(M;\,\rho)$
in section 3. This
$g^{\kern0.5pt f}$
is called a combinatorial propagator in [
Reference Fukaya6
,
Reference Watanabe22
].
For
$p\in \text{Crit}_i(\,f)$
and
$q\in \text{Crit}_{i-1}(\,f)$
, we denote
where
$\pi_{V_q}\,:\,\oplus_{q'\in \text{Crit}_{i-1}(\,f)}V_{q'}\to V_q$
is the projection. Similarly, a combinatorial propagator
$g^{\kern0.5pt f}$
gives a homomorphism
where
$\pi_{V_p}\,:\,\oplus_{r\in \text{Crit}_i(\,f)}V_r\to V_p$
is the projection.
6·2. Preparation for manifolds
Recall that
$D\nu_{\Delta}=\{(x,v)\mid \|v\|\le 1\}$
is a disk bundle of the normal bundle
$\nu_{\Delta}$
of
$\Delta$
in
$M\times M$
.
$S\nu_{\Delta}=\partial D\nu_{\Delta}$
is the unit sphere bundle of
$\Delta$
. We denote by
$B\ell(M^2,\Delta)$
the real blowing up of
$M^2$
along
$\Delta$
, namely
\begin{align*}&B\ell(M^2,\Delta)\notag\\ &\quad =(M^2\setminus \Delta)\cup_{D\nu_{\Delta}\setminus \Delta}\left\{((x,tu),u)\in \nu_{\Delta}\times S\nu_{\Delta}\mid x\in \Delta, u\in (S\nu_{\Delta})_x,t\in [0,\infty) \right\}\notag\\ &\quad \cong (M^2\setminus\Delta)\cup S\nu_{\Delta}.\end{align*}
We denote by
$\pi\,:\,B\ell(M^2,\Delta)\to M^2$
the blow-down map. Namely,
$\pi|_{M^2\setminus\Delta}=\text{id}\,:\,M^2\setminus\Delta\to M^2\setminus \Delta\subset M^2$
and
$\pi|_{S\nu_{\Delta}}\,:\,S\nu_{\Delta}\to \Delta\subset M^2$
are the projections. By construction,
Recall that
$\nu_{\Delta}$
is identified with the tangent bundle TM by the bundle isomorphism given by
where
$x\in M, v\in T_xM$
. Under the identification, we have
$D\nu_{\Delta}=DTM$
and
$S\nu_{\Delta}=STM$
. We orient
$\partial B\ell(M^2,\Delta)$
as a boundary of
$B\ell(M^2,\Delta)$
. Then
$S\nu_{\Delta}$
and STM are oriented by the above identification.
Take an open tubular neighbourhood
$N(\Delta)$
of
$\Delta$
in
$M^2$
and identify
$N(\Delta)$
with
$\nu_{\Delta}$
. We can take a diffeomorphism between
$B\ell(M^2,\Delta)$
and
$M^2\setminus \mathring{D}\nu_{\Delta}$
by “shrinking” a collar of
$\partial B\ell(M^2,\Delta)$
. More precisely, we take the inclusion map
as follows: Let
$D_2\nu_{\Delta}=\{(x,v)\in \nu_{\Delta}\mid \|v\|\le 2\}\subset M^2$
. Take a
$C^{\infty}$
function
$h\,:\,[0,\infty)\to[1,\infty)$
satisfying
\begin{align*}\frac{dh}{dt}(t)\ge 0\ \forall\ t\ \text{and}\ h(t)=\begin{cases}t& (t\ge 2)\\ 1 &(t=0)\end{cases}.\end{align*}
The inclusion
$\iota\,:\,B\ell(M^2,\Delta)\hookrightarrow M^2$
is given as the canonical extension of the map
$\iota_0\,:\,(M^2\setminus\Delta=)\text{int}B\ell(M^2,\Delta)\to B\ell(M^2,\Delta)$
defined by
\begin{eqnarray*}\iota_0|_{B\ell(M^2)\setminus D_2\nu_{\Delta}}&=&\text{id},\\\iota_0|_{D_2\nu_{\Delta}\setminus \Delta}(x,v)&=& \left(x,\frac{h(\|v\|)}{\|v\|}v\right)\text{for}\ (x,v)\in D_2\nu_{\Delta}\setminus \Delta.\end{eqnarray*}
Obviously,
$\iota(B\ell(M^2,\Delta))=M^2\setminus \mathring{N}(\Delta)$
. Thus we can identify
$B\ell(M^2,\Delta)$
with
$M^2\setminus \mathring{N}(\Delta)$
via
$\iota$
. Then
$\iota(B\ell(M^2,\Delta))\subset M^2$
.
6·3. A Morse theoretic description of
$d'(M,\rho,e)$
By using the Morse function f and the gradient-like vector field
${\textrm{grad}}\, f$
, we construct a 4-chain
such that
$\partial \Sigma_f^0=v_e(\Delta)\otimes 1$
(Definition 6·5 and Proposition 6·6).
Let
$M_{\to}(\,f)$
be the set of all pairs of two points in M connected by a trajectory:
We orient
$M_{\to}(\,f)$
so that an inclusion
$(M\setminus \text{Crit}(\,f))\times (0,1]\ni(x,t)\mapsto (x,\Phi_t^{\kern0.5pt f}(x))\in M_{\to}(\,f)$
preserves the orientation. There is a compactification
$\overline{M}_{\to}(\,f)\subset B\ell(M^2,\Delta)(\subset M^2)$
which consists of all broken trajectories (see [
Reference Shimizu17
, lemma 5·13] or [
Reference Lescop15
, lemma 4·3], [
Reference Watanabe22
, proposition 3·14]).
$\overline{M}_{\to}(\,f)$
with the local coefficient given by
$1\in \text{Hom}(V,V)$
near
$\Delta$
gives a 4-chain in
$C_4(B\ell(M^2,\Delta);\,\rho^*\boxtimes \rho)$
and in
$C_4(M^2;\,\rho^*\boxtimes \rho)$
:
where pt is any point of
$\partial B\ell(M^2,\Delta)$
.
Similarly, we have compactifications
$\overline{\mathcal D_p}$
of
$\mathcal D_p$
and
$\overline{\mathcal A_q}$
of
$\mathcal A_q$
by adding all the broken trajectories (see [
Reference Shimizu17
, lemma 5·14] or [
Reference Watanabe22
, proposition 3·14]). For
$p\in\text{Crit}_i(\,f)$
and
$q\in\text{Crit}_{i-1}(\,f)$
, the combinatorial propagator
$g^{\kern0.5pt f}$
gives a homomorphism
$1\otimes g_{p,q}^{\kern0.5pt f}\,:\,V_q^*\otimes V_q\to V_q^*\otimes V_p$
. Thus we have a 4-chain
Under the identification
$V_{q}^*\otimes V_p=\text{Hom}(V_q,V_p)$
, the coefficient
$(1\otimes g_{p,q}^{\kern0.5pt f})1\in V_q^*\otimes V_p$
can be written as
$g_{p,q}^{\kern0.5pt f}\in \text{ Hom}(V_q,V_p)$
:
To simplify the notation, we use the notation on the right hand side rather than the left one. Let
be the 4-chain given from the closure of
$\overline{\mathcal A_q}\times \overline{\mathcal D_p}\setminus\Delta$
in
$B\ell(M^2,\Delta)$
. See [
Reference Watanabe22
, proposition 3·14] for more details.
Set
\begin{eqnarray*}\mathcal M_0(\,f)=\langle \overline{M}_{\to}(\,f),\text{pt};\,1\rangle+\sum_{p,q;\,\text{ind}(p)=\text{ind}(q)+1}\langle (\overline{\mathcal {A}_q}\times \overline{\mathcal{D}_p})^{B\ell},(q,p);\,g^{\kern0.5pt f}_{p,q}\rangle&&\\\in C_4(B\ell(M^2,\Delta);\,\rho^*\boxtimes \rho).&&\end{eqnarray*}
The 4-chain
$\overline{M}_{\to}(\,f)$
has
\begin{eqnarray*}\left\{\frac{-{\textrm{grad}}_x{\kern1pt f}}{\|{\textrm{grad}}_x{\kern1pt f}\|}\middle| x\in M\setminus \text{Crit}(\,f)\right\}\otimes 1&&\in C_3(\partial B\ell(M^2,\Delta);\,\rho^*\otimes \rho)\\ &&= C_3(STM;\,\rho^*\otimes \rho)\end{eqnarray*}
as a part of the boundary
$\partial \overline{M}_{\to}(\,f)$
.
Due to our orientation conventions, we have
and
Thus
$\langle(\overline{\mathcal{A}_q}\times \overline{\mathcal{D}_p})^{B\ell},(q,p);\,g_{p,q}^{\kern0.5pt f}\rangle$
has
as a part of the boundary. Here
$\pi\,:\,S\nu_{\Delta}=STM\to M$
is the projection.
By a similar argument as in [
Reference Shimizu17
, lemma 5·16] (or [
Reference Shimizu18
, proposition 6·2]), we can check that the other boundary strata of
$\partial \overline{M}_{\to}(\,f)$
and
$\sum_{p,q}\partial (\mathcal{A}_q\times \mathcal{D}_p)^{B\ell}$
with local coefficients cancel:
$\sum_{p}\langle \overline{\mathcal{A}}_p\times\overline{\mathcal{D}}_p,(p,p);\,1\rangle$
which appears with a plus sign in the boundary of
$\sum_{p,q}(\mathcal{A}_q\times \mathcal{D}_p)^{B\ell}$
and with a minus sign in the boundary of
$\overline{M}_{\to}(\,f)$
. Then we have
Lemma 6·1.
\begin{align*}&\partial\mathcal M_0(\,f)\notag\\ &\def\negativespace{}\def\negativespace{}\def\negativespace{}\quad=\overline{\left\{ \left(x,\frac{-{\textrm{grad}}_x{f}}{\|{\textrm{grad}}_x(\,f)\|}\right)\middle| x\in M\setminus \text{Crit}(\,f) \right\}}\otimes 1\\&\quad+\sum_{\substack{p,q;\\ \text{ind}(p)=\text{ind}(q)+1}}\sum_{\gamma\in\mathcal M(p,q)}\pi^!\langle\gamma_{\cap},p;\,g_{p,q}^{\kern0.5pt f}\circ\gamma_*\rangle \notag\\ &\def\negativespace{}\def\negativespace{}\def\negativespace{}\quad=\overline{\left\{ \left(x,\frac{-{\textrm{grad}}_x{f}}{\|{\textrm{grad}}_x(\,f)\|}\right)\mid x\in M\setminus \text{Crit}(\,f) \right\}} \def\negativespace{}\otimes 1\\&\quad+\sum_{\substack{p,q;\\ \text{ind}(p)=\text{ind}(q)+1}}\sum_{\gamma\in\mathcal M(p,q)}\pi^{-1}(\gamma_{\cap})\otimes (g_{p,q}^{\kern0.5pt f}\circ\gamma_*).\end{align*}
Set
\begin{eqnarray*}\Gamma&=&\sum_{p,q;\,\text{ind}(p)=\text{ind}(q)+1}\sum_{\gamma\in\mathcal M(p,q)}\langle\gamma_{\cap},p;\,g_{p,q}^{\kern0.5pt f}\circ\gamma_*\rangle\\ &=& \sum_{p,q;\,\text{ind}(p)=\text{ind}(q)+1}\sum_{\gamma\in\mathcal M(p,q)}\gamma_{\cap} \otimes (g_{p,q}^{\kern0.5pt f}\circ\gamma_*)\in C_1(M;\,\rho^*\otimes \rho).\end{eqnarray*}
Let
be the 0-chain given by critical points. The 1-chain
$\Gamma$
has the following property:
Lemma 6·2.
Proof. Let
$c_p$
be the coefficient of
$p\in \text{Crit}(\,f)$
in
$\partial \Gamma$
. We show that
$c_p=(-1)^{\text{ ind}(p)+1}$
. If a trajectory
$\gamma$
is from a critical point
$r\in \text{Crit}_{\text{ind}(p)+1}(\,f)$
to p and
$\gamma_{\cap}$
is oriented from p to r, then the coefficient of p in
$\partial \gamma_{\cap}$
is
$-1$
and
${\varepsilon}(\gamma)=-1$
. If the orientation of
$\gamma_{\cap}$
is opposite, namely from r to p, then the coefficient of p in
$\partial \gamma_{\cap}$
is
$+1$
and
${\varepsilon}(\gamma)=+1$
. If a trajectory
$\gamma_{\cap}$
connecting p and
$q\in \text{Crit}_{\text{ind}(p)-1}(\,f)$
is oriented from p to q, then the coefficient of p in
$\partial \gamma_{\cap}$
is
$-1$
and
${\varepsilon}(\gamma)=+1$
. If the orientation of
$\gamma_{\cap}$
is opposite, namely from q to p, then the coefficient of p in
$\partial\gamma_{\cap}$
is
$+1$
and
${\varepsilon}(\gamma)=-1$
. Therefore
$c_p$
is computed as follows:
\begin{eqnarray*}c_p&=&\sum_{r\in\text{Crit}_{\text{ind}(p)+1}(\,f)}\sum_{\gamma\in \mathcal M(r,p)}{\varepsilon}(\gamma)g_{r,p}^{\kern0.5pt f}\circ\gamma_*+\sum_{q\in\text{Crit}_{\text{ind}(p)-1}(\,f)}\sum_{\gamma\in\mathcal M(p,q)}-{\varepsilon}(\gamma)g_{p,q}^{\kern0.5pt f}\circ\gamma_*\\ &=& \sum_{r\in\text{Crit}_{\text{ind}(p)+1}(\,f)}(-1)^{\text{ind}(p)+1}g_{r,p}^{\kern0.5pt f}\circ\partial_{p,r}^{\kern0.5pt f}+\sum_{q\in\text{Crit}_{\text{ind}(p)-1}(\,f)}(-1)^{\text{ind}(p)+1}g_{p,q}^{\kern0.5pt f}\circ\partial_{q,p}^{\kern0.5pt f}\\ &=&(-1)^{\text{ind}(p)+1}\pi_{V_p}\circ \left(\partial^{\kern0.5pt f}\circ g^{\kern0.5pt f}+g^{\kern0.5pt f}\circ\partial^{\kern0.5pt f}\right)|_{V_p}(1)\\ &=&(-1)^{\text{ind}(p)+1}.\end{eqnarray*}
Here
$\pi_{V_p}\,:\,\sum_{p'\in \text{Crit}_{\text{ind}(p)}}V_{p'}\to V_p$
is the projection.
We prepare two more chains.
Take an Euler chain
$c_f$
for
$-{\textrm{grad}}\, f$
(see section 2·5 for more details on Euler chains). Take a section
$\widetilde s\in\Gamma p_2^*TM$
of
$p_2^*TM$
on
$[0,1]\times M$
so that
$\widetilde s|_{0\times M}=-{\textrm{grad}}\, f$
as in lemma 2·2.
Then
$\widetilde s^{-1}(0)$
is a 1-manifold of
$[0,1]\times M$
such that
$\partial \widetilde s^{-1}(0)=c^0(\,f)$
.
The restriction of
$\widetilde s|_{0\times M}=-{\textrm{grad}}\, f$
to the 4-manifold
gives a 4-chain in
$STM=\partial B\ell(M^2,\Delta)$
:
Since
$\widetilde{s}|_{\{0\}\times M}=-{\textrm{grad}}\, f$
,
$\widetilde{s}|_{\{1\}\times M}=-{\textrm{grad}}\, f/c_f$
and
$p_2(\widetilde{s}^{-1}(0))=c_f$
, we have the following lemma.
Lemma 6·3.
\begin{align*}&\partial \left(((p_2)_*\widetilde{S})\otimes 1\right)\\ & \quad = \pi^{-1}(c_f)\otimes 1\\ & \qquad -\overline{\left\{\frac{-{\textrm{grad}}_x{\kern1.5pt f}}{\|{\textrm{grad}}_x{\kern1.5pt f}\|}\middle| x\in M\setminus \text{Crit}(\,f)\right\}}\otimes 1+\left\{\frac{-({\textrm{grad}}\, f/c_f)_x}{\|({\textrm{grad}}\, f/c_f)_x\|}\middle| x\in M\right\}\otimes 1.\end{align*}
The disk bundle
$D\nu_{\Delta}=DTM$
forms a
$D^3$
-bundle over M. We orient
$D\nu_{\Delta}$
such that
$\partial D\nu_{\Delta}=-S\nu_{\Delta}=-\partial B\ell(M^2,\Delta)$
. Then
$B\ell(M^2,\Delta)\cup D\nu_{\Delta}=M^2$
. Let
$\widetilde{\pi}\,:\,D\nu_{\Delta}=DTM\to M$
be the projection. Thanks to lemma 6·2,
is a 1-cycle of
$C_1(M;\,\rho^*\otimes \rho)$
. Thus we have a 4-chain
By construction, the boundary of this chain is written as follows:
Lemma 6·4.
Here
$\pi\,:\,STM(=\partial D\nu_{\Delta})\to M$
is the projection.
Definition 6·5.
Here
$\iota\,:\,B\ell(M^2,\Delta)\to M^2$
is an inclusion defined in the last part of section 6·2.
The following proposition is a direct consequence of Lemmas 6·1, 6·3, and 6·4.
Proposition 6·6.
$d'(M,\rho;\,e)$
is defined as
$d'(M,\rho;\,e)=\text{lk}_{\rho^*\boxtimes\rho}(v_e(\Delta)\otimes 1,\Delta)=[\Sigma_0^{\kern0.5pt f}\cap \Delta]$
. Thus we have the following formula.
Proposition 6·7.
\begin{eqnarray*}d'(M,\rho;\,e)&=&[(c_f\otimes 1)+\Gamma]\\ &=&[(c_f\otimes1)+\sum_{p,q;\,\text{ind}(p)=\text{ind}(q)+1}\sum_{\gamma\in \mathcal M(p,q)}\gamma_{\cap}\otimes (g_{p,q}^{\kern0.5pt f}\circ\gamma_*)]\\ &&\in H_1(M;\,\rho^*\otimes\rho).\end{eqnarray*}
Proof. By the definition of
$d'(M,\rho;\,e)$
, we have
\begin{eqnarray*}d'(M,\rho;\,e)&=&[\Sigma_0^{\kern0.5pt f}\cap \Delta]\\ &=&[\left(\mathcal M_0(\,f)+((p_2)_*\widetilde S)\otimes 1+\widetilde{\pi}^{!}((c_f\otimes 1)+\Gamma)\right)\cap\Delta].\end{eqnarray*}
Since
$\iota_*\mathcal M_0(\,f)$
and
$(p_2)_*\widetilde S$
are in
$B\ell(M^2,\Delta)$
, these are far from
$\Delta$
. Thus we have
Let
$B_{c_f}$
be a 3-ball in M containing all neighbourhoods
$N(c_1),\ldots$
of intervals
$c_1,\ldots$
consisting
$c_f$
. Then any trajectory
$\gamma_{\downarrow}$
can be transformed into a 1-cycle called
$\gamma{}'_{\downarrow}$
by adding a 1-chain supported in
$B_{c_f}$
. Similarly, a 1-cycle
$\gamma_{\cap}'$
is given from
$\gamma_{\cap}$
. By using these cycles, we have the following slightly different description of
$d'(M,\rho;\,e)$
:
Proposition 6·8.
Here
$[\gamma_{\cap}']$
is a 1-cycle of
$H_1(M;\,{\mathbb{Z}})$
represented by
$\gamma_{\cap}'$
.
6·4. Behaviours of d ′ and Tor under replacing an Euler structure
Let
$c_f'$
be an Euler chain for f. Let
$e'=[-{\textrm{grad}}\, f/c_f']\in \text{Eul}(M)$
. Since
$\partial c_f'=\partial c_f=c^0(\,f)$
, the difference
$c_f'-c_f$
is a cycle in
$C_1(M;\,{\mathbb{Z}})$
and then it represents a homology class
$[c_f'-c_f]$
in
$H_1(M;\,{\mathbb{Z}})$
.
Lemma 6·9.
-
(i)
$d'(M,\rho;\,e')-d'(M,\rho;\,e)=[c_f'-c_f]\otimes 1$
. -
(ii)
$\text{Tor}(M,\rho;\,e')\text{Tor}(M,\rho;\,e)^{-1}=\pm\det\rho([c_f'-c_f])$
.
Proof. (i) Since
$\partial^{\kern0.5pt f},g^{\kern0.5pt f}$
and
$\gamma_*$
are independent of the choice of the Euler structure, the first equality follows from Proposition 6·7.
(ii) Let
$c_1,\ldots,c_k$
be intervals consisting
$c_f$
, namely
$c_f=\sqcup_{i=1}^kc_i$
. Here
$k=\sharp \text{ Crit}(\,f)/2$
. Similarly let
$c_f'=\sqcup_{i=1}^kc_i'$
. Take an arbitrary isomorphism
$V_x\stackrel{\cong}{\to}V$
for each
$x\in \text{Crit}(\,f)$
. Then each
$(c_i)_*$
or
$(c_i)'_*$
can be considered as an element of
$\text{Hom}(V,V)=V$
. The isomorphism
$(c_f)_*\,:\,C_{odd}\to C_{even}$
is identified with an isomorphism from
$V^{\oplus k}$
to
$V^{\oplus k}$
. Thus
$\det(c_f)_*$
is given by
$\det(c_f)_*=\pm \det(c_1)_*\ldots \det(c_k)_*$
. We have
\begin{eqnarray*}\text{Tor}(M,\rho;\,e')\text{Tor}(M,\rho;\,e)^{-1}&=&\det ((c_f')_*\circ (\partial_*^{\kern0.5pt f}+g^{\kern0.5pt f}))\det ((c_f)_*\circ \partial_*^{\kern0.5pt f}+g^{\kern0.5pt f})^{-1}\\ &=& (\det (c_f')_*)(\det (c_f)_*)^{-1} \\ &=&\det(\Pi_{i=1}^k(c_i')_*\Pi_{i=1}^k(c_i)_*^{-1})\\ &=&\det\rho([c_f'-c_f])\in F^{\times}/{\pm}.\end{eqnarray*}
7. Proof of Theorem 1
By using the Morse theoretic description of d
′, we compute
$d'(M,\rho_0;\,e)$
explicitly for the maximal free abelian representation
$\rho_0$
. In section 7·1 we give explicit descriptions of the boundary homomorphisms and related homomorphisms associated with a Morse function. By using these descriptions, in sections 7·2 and 7·3 we compute
$d'(M,\rho_0;\,e)$
and
$\text{Tor}(M,\rho_0;\,e)$
. And then in section 7·4 we compare these computations to get a proof of the theorem.
Remark 7·1. The computation given in section 7·3 is an analogue of the computation given in the proof of lemma 3·1 of [ Reference Hutchings and Lee10 ] by M. Hutchings and Y. J. Lee. However, we could not find a direct proof of Theorem 1 from lemma 3·1 of [ Reference Hutchings and Lee10 ].
7·1. An explicit description of the boundary operators
$\partial_*^{\kern0.5pt f}$
and a propagator
$g^{\kern0.5pt f}$
From now we consider
$\rho_0\,:\,\pi_1(M)\to Q(H)$
.
Thanks to lemma 6·9, it is enough to show the theorem for a special Euler structure. Then we choose a special Morse function and an Euler chain for it to simplify the computation. We take a Morse function such that
$\sharp \text{Crit}_3(\,f)=\sharp\text{Crit}_0(\,f)=1$
. Let
\begin{eqnarray*}&&\text{Crit}_3(\,f)=\{\text{NP}\},\\ &&\text{Crit}_2(\,f)=\{p_1,\ldots, p_n\},\\ &&\text{Crit}_1(\,f)=\{q_1,\ldots, q_n\},\\ &&\text{Crit}_0(\,f)= \{\text{SP}\}.\end{eqnarray*}
We denote by
\begin{eqnarray*}&&C_{\text{NP}}=C_3^{\kern0.5pt f}(M;\,\rho_0)=Q(H)_{NP},\\ &&C_{\bf p}=C_2^{\kern0.5pt f}(M;\,\rho_0)=\oplus_{i=1}^nQ(H)_{p_i},\\ &&C_{\bf q}=C_1^{\kern0.5pt f}(M;\,\rho_0)=\oplus_{i=1}^nQ(H)_{q_i},\\ &&C_{\text{SP}}=C_0^{\kern0.5pt f}(M;\,\rho_0)=Q(H)_{SP}.\end{eqnarray*}
Let
$c_f$
be an Euler chain for f and let
$e=[-{\textrm{grad}}\, f/c_f]$
. Take a 3-ball
$B_{c_f}$
in M containing all neighbourhoods
$N(c_1),\ldots,N(c_{n+1})$
of intervals
$c_1,\ldots,c_{n+1}$
consisting the Euler chain
$c_f$
. We identify
$Q(H)_{\text{NP}}$
with Q(H). Then
$Q(H)_p$
,
$p\in \text{Crit}(\,f)$
, are identified with
$Q(H)_{\text{NP}}=Q(H)$
via isomorphisms
$\phi_*$
associated to paths
$\phi$
inside
$B_{c_f}$
.
Two bases
${b}_e$
and
${b}_f$
of
$C^{\kern1pt f}_*(M;\,\rho_0)$
To simplify the computations, we first introduce two bases
$\text{b}_e$
and
$\text{b}_f$
of
$C_*^{\kern0.5pt f}(M,\rho_0)$
.
For each
$p\in \text{Crit}(\,f)$
, we denote by
$p\in Q(H)_p$
the element corresponding to the generator
$1\in Q(H)$
under the identification
$Q(H)_p=Q(H)$
. Therefore, we now have a basis
${\bf b}_e$
of
$C_*^{\kern0.5pt f}(M,\rho_0)$
:
We next introduce the basis
${\bf b}_f$
. Let
$\pi_{Q(H)_{p_1}}\,:\,C_{\bf p}\to Q(H)_{p_1}$
be the projection. Without loss of generality, we assume that
$\pi_{Q(H)_{p_1}}\circ\partial_3^{\kern0.5pt f}(\text{NP})\not=0$
. We take a basis of
$C_{\bf p}$
as
Since
$\dim_{Q(H)}\text{Im}\partial_2^{\kern0.5pt f}=n-1\not= n=\dim_{Q(H)}C_{\bf q}$
, at least one of
$q_1,\ldots,q_n$
does not belong to
$\text{Im} \partial_2^{\kern0.5pt f}\subset C_{\bf q}$
. We may assume that
$q_1\not\in \text{Im}\partial_2^{\kern0.5pt f}$
. Then
is a basis of
$C_{\bf q}$
. Since
$H_0(M;\,\rho_0)=0$
, then
$\partial_1^{\kern0.5pt f}(q_1)\not=0$
. We take
$\partial_1^{\kern0.5pt f}(q_1)$
as a basis of
$C_{\text{SP}}$
. Now we have a basis
${\bf b}_f$
:
Let
$(\partial_1^{ij})_{ij}, (\partial_2^{ij})_{ij}$
and
$(\partial_3^{ij})_{ij}$
be representation matrices of
$\partial_1^{\kern0.5pt f},\partial_2^{\kern0.5pt f}$
and
$\partial_3^{\kern0.5pt f}$
respectively under the basis
${\bf b}_e$
. Namely,
\begin{eqnarray*}\partial_3^{\kern0.5pt f}(\text{NP})&=&(p_1,\ldots,p_n)\left(\begin{array}{c}\partial^{11}_3\\\vdots\\\partial^{n1}_3\end{array}\right),\\\partial_2^{\kern0.5pt f}(p_1,\ldots,p_n)&=&(q_1,\ldots,q_n)\left(\begin{array}{ccc}\partial^{11}_2& \cdots& \partial_2^{1n}\\\vdots &\ddots &\vdots\\\partial^{n1}_2&\cdots &\partial_2^{nn}\end{array}\right),\\\partial_1^{\kern0.5pt f}(q_1,\ldots,q_n)&=&(\text{SP})(\partial_1^{11}~\cdots~\partial_1^{1n}).\end{eqnarray*}
A propagator
$g^{\kern0.5pt f}$
We give a combinatorial propagator
$g^{\kern0.5pt f}$
explicitly written by using the basis
${\bf b}_f$
as follows:
-
(i)
$g^{\kern0.5pt f}_3(\partial_3^{\kern0.5pt f}(\text{NP}))=\text{NP}$
,
$g^{\kern0.5pt f}_3(p_2)=0,\ldots,g^{\kern0.5pt f}_3(p_n)=0$
; -
(ii)
$g^{\kern0.5pt f}_2(q_1)=0$
,
$g^{\kern0.5pt f}_2(\partial^{\kern0.5pt f}_2(p_2))=p_2,\ldots,g^{\kern0.5pt f}_2(\partial^{\kern0.5pt f}_2(p_n))=p_n$
; -
(iii)
$g^{\kern0.5pt f}_1(\partial^{\kern0.5pt f}_1(q_1))=q_1$
.
Obviously, these homomorphisms
$g^{\kern0.5pt f}=\{g_i\}_i$
satisfies
$\partial_{i+1}^{\kern0.5pt f}\circ g_{i+1}^{\kern0.5pt f}+g_i^{\kern0.5pt f}\circ \partial_i^{\kern0.5pt f}=\text{id}$
for any i, namely
$g^{\kern0.5pt f}$
is a combinatorial propagator.
An explicit description of
$g^{\kern0.5pt f}$
with respect to the basis
${\bf b}_e$
.
-
(i) A description of
$g^{\kern0.5pt f}_3$
We have
$\partial^{\kern0.5pt f}_3(\text{NP})=\sum_{i=1}^n\partial_3^{i1}p_i$
. Since
$g_3^{\kern0.5pt f}(p_i)=0$
for
$i\ge 2$
, we have
$\text{NP}=g_3^{\kern0.5pt f}(\partial_3^{\kern0.5pt f}(\text{NP}))=g_3^{\kern0.5pt f}(\partial_3^{11}p_1)=\partial_3^{11}g_3^{\kern0.5pt f}(p_1)$
. Then
$g_3^{\kern0.5pt f}(p_1)=(\partial_3^{11})^{-1}(NP)$
. We have
\begin{align*}g^{\kern0.5pt f}_{\text{NP},p_1}=(\partial_3^{11})^{-1}, g^{\kern0.5pt f}_{\text{NP},p_2}=0,\ldots, g^{\kern0.5pt f}_{\text{NP},p_n}=0.\end{align*}
-
(ii) A description of
$g^{\kern0.5pt f}_2$
Since
$g_2^{\kern0.5pt f}(q_1)=0$
, it suffices to determine the restriction
$g_2^{\kern0.5pt f}|_{\langle q_2,\ldots,q_n\rangle}$
of
$g_2^{\kern0.5pt f}$
to the linear span
$\langle q_2,\ldots,q_n\rangle$
. We know that the image of
$g_2^{\kern0.5pt f}$
is the linear span
$\langle p_2,\ldots,p_n\rangle$
and that
$g_2^{\kern0.5pt f}|_{\langle q_2,\ldots,q_n\rangle}$
is the inverse of the map
$\Pi\circ \partial_2^{\kern0.5pt f}|_{\langle p_2,\ldots,p_n\rangle}$
, where
$\Pi\,:\,C_{\bf q}\to \langle q_2,\ldots,q_n\rangle$
is the projection with respect to the basis
${\bf b}_e$
. The map
$\Pi\circ \partial_2^{\kern0.5pt f}|_{\langle p_2,\ldots,p_n\rangle}$
is represented as Here the matrix
\begin{eqnarray*}\Pi\circ \partial_2^{\kern0.5pt f}|_{\langle p_2,\ldots,p_n\rangle}(p_2,\ldots,p_n)=(q_2,\ldots,q_n)A_2.\end{eqnarray*}
$A_2$
is defined by Let
\begin{align*}A_2=\left(\begin{array}{ccc}\partial_2^{22}&\cdots&\partial_2^{2n}\\ \vdots&\ddots&\vdots\\\partial_2^{n2}&\cdots&\partial_2^{nn}\end{array}\right).\end{align*}
$(A_2^{ij})$
be the (i, j)-cofactor of
$A_2$
, namely
\begin{align*}\left(\frac{1}{\det A_2}A_2^{ji}\right)_{i,j}=A_2^{-1}.\end{align*}
Therefore we have
\begin{align*}g^{\kern0.5pt f}_{p_j,q_i}=\begin{cases}\frac{1}{\det A_2}A_2^{ji}&(i,j\ge 2),\\0& i=1\text{or}\, j=1.\end{cases}\end{align*}
-
(iii) A description of
$g^{\kern0.5pt f}_1$
Since
$\partial_1^{\kern0.5pt f}(q_1)=\partial_1^{11}\text{SP}$
, we have
\begin{align*}g_1^{\kern0.5pt f}(\text{SP})=(\partial_1^{11})^{-1} g_1^{\kern0.5pt f}(\partial_1^{11}\text{SP})=(\partial_1^{11})^{-1}g_1^{\kern0.5pt f}(\partial_1^{\kern0.5pt f}(q_1))=(\partial_1^{11})^{-1}q_1.\end{align*}
Then we have
\begin{align*}g^{\kern0.5pt f}_{q_1,\text{SP}}=(\partial_1^{11})^{-1}, g^{\kern0.5pt f}_{q_2,\text{SP}}=0,\ldots, g^{\kern0.5pt f}_{q_n,\text{SP}}=0.\end{align*}
7·2. The computation of
$D(\text{Tor}(M,\rho_0;\,e))$
Under the identification
$Q(H)_p=Q(H)$
for
$p\in\text{Crit}(\,f)$
by using
$B_{c_f}$
, each
$c_i$
consisting
$c_f$
gives
$(c_i)_*=1$
. Then
$\text{Tor}(M,\rho_0;\,e)=\det(\partial^{\kern0.5pt f}+g^{\kern0.5pt f})$
.
The isomorphism
is represented by the following matrix with respect to the basis
${\bf b}_e$
:
Here
\begin{eqnarray*}T=\left(\begin{array}{ccccc}(\partial_3^{11})^{-1}&0&\cdots&0&0\\[2pt]\partial_2^{11}&\partial_2^{12}&\cdots&\partial_2^{1n}&(\partial_1^{11})^{-1}\\[3pt]\partial_2^{21}&\partial_2^{22}&\cdots&\partial_2^{2n}&0\\\vdots&\vdots&\ddots&\vdots&\vdots\\\partial_2^{n1}&\partial_2^{n2}&\cdots&\partial_2^{nn}&0\end{array}\right).\end{eqnarray*}
Therefore, we have
We next compute
$D(\text{Tor}(M,\rho_0;\,e))$
. To simplify the notations, we use same symbol
$\gamma{}'_{\downarrow}$
for an element of H represented by a cycle
$\gamma{}'_{\downarrow}$
. In other word,
$\gamma{}'_{\downarrow}=\gamma_{*}(1)\in H.$
Recall that
$[\gamma{}'_{\downarrow}]_+$
is an element of
$H_1(M;\,{\mathbb{Z}})/\text{Tor}$
corresponding to
$\gamma{}'_{\downarrow}\in H$
.
Since the boundary homomorphisms
$\partial_i^{\kern0.5pt f}$
are written by a rational function of
$\gamma{}'_{\downarrow}$
for all
$\gamma$
, the Reidemeister–Turaev torsion
$\text{Tor}(M,\rho_0;\,e)$
is also written by a rational function of all
$\gamma{}'_{\downarrow}$
. Then thanks to Proposition 5·6,
$D(\text{Tor}(M,\rho_0;\,e))$
is given by
\begin{eqnarray*}D(\text{Tor}(M,\rho_0;\,e))&=&\sum_{\gamma}\left([\gamma{}'_{\downarrow}]_+\otimes \frac{\gamma{}'_{\downarrow}}{\text{Tor}(M,\rho_0;\,e)}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\text{Tor}(M,\rho_0;\,e)\right)\\ &=&\sum_{\gamma}\left([\gamma{}'_{\downarrow}]_+\otimes \frac{\gamma{}'_{\downarrow}}{\text{Tor}(M,\rho_0;\,e)}\frac{\partial}{\partial \gamma{}'_{\downarrow}}(-1)^{n-1}(\partial_3^{11})^{-1}(\det A_2)(\partial_1^{11})^{-1}\right)\\ &=&\sum_{\gamma}\left([\gamma{}'_{\downarrow}]_+\otimes A(\gamma)\right),\end{eqnarray*}
where
$\displaystyle A(\gamma)=-\frac{\gamma{}'_{\downarrow}}{\partial_3^{11}}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\partial_3^{11}+\frac{\gamma{}'_{\downarrow}}{\det A_2}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\det A_2-\frac{\gamma{}'_{\downarrow}}{\partial_1^{11}}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\partial_1^{11}$
.
We compute
$A(\gamma)$
for each trajectory
$\gamma$
. We denote by
$s(\gamma)=p,t(\gamma)=q$
for a trajectory
$\gamma$
from p to q. We break the computation into cases depending on
$s(\gamma)$
and
$t(\gamma)$
.
Case 1:
$s(\gamma)=\text{NP},t(\gamma)=p_i$
In this case the term
$\gamma'_{\downarrow}$
only appears in
$\partial_3^{i1}$
. We note that
$\partial_3^{i1}=\sum_{\gamma\in \mathcal M(\text{NP},p_i)}-{\varepsilon}(\gamma)\gamma{}'_{\downarrow}$
. Thus
\begin{eqnarray*}A(\gamma)&=&-\frac{\gamma{}'_{\downarrow}}{\partial_3^{11}}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\partial_3^{11}=\begin{cases}{\varepsilon}(\gamma)\frac{\gamma'}{\partial_3^{11}}&(i=1),\\0&(i\not=1).\end{cases}\end{eqnarray*}
Case 2-1.
$s(\gamma)=\text{p}_i,t(\gamma)=q_j$
,
$i=1$
or
$j=1$
In this case there are no
$\gamma{}'_{\downarrow}$
in
$(\partial_3^{11})^{-1}(\det A_2)(\partial_1^{11})^{-1}$
. Then we have
Case 2-2.
$s(\gamma)=\text{p}_i,t(\gamma)=q_j$
,
$i,j\ge 2$
\begin{eqnarray*}A(\gamma)&=&\frac{\gamma{}'_{\downarrow}}{\det A_2}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\det A_2=\frac{\gamma{}'_{\downarrow}}{\det A_2}\frac{\partial}{\partial \gamma_{\downarrow'}}\left(\sum_{a=2}^n \partial_2^{ai}A_2^{ai}\right)=\frac{\gamma{}'_{\downarrow}}{\det A_2}{\varepsilon}(\gamma)A_2^{ji}.\end{eqnarray*}
Case 3.
$s(\gamma)=q_j,t(\gamma)=\text{SP}$
\begin{eqnarray*}A(\gamma)&=&-\frac{\gamma{}'_{\downarrow}}{\partial_1^{11}}\frac{\partial}{\partial \gamma{}'_{\downarrow}}\partial_1^{11}=\begin{cases}{\varepsilon}(\gamma)\frac{\gamma{}'_{\downarrow}}{\partial_1^{11}}&(j=1),\\0&(j\not=1).\end{cases}\end{eqnarray*}
Therefore,
$D(\text{Tor}(M,\rho_0;\,e))$
is given as follows:
\begin{eqnarray*}&&D(\text{Tor}(M,\rho_0;\,e))\\ &=&\sum_{\gamma\in\mathcal M(\text{NP},p_1)}[\gamma{}'_{\downarrow}]_+\otimes \frac{{\varepsilon}(\gamma)\gamma{}'_{\downarrow}}{\partial_3^{11}}+\sum_{i,j\ge 2}\sum_{\gamma\in\mathcal M(p_i,q_j)}[\gamma{}'_{\downarrow}]_+\otimes \frac{{\varepsilon}(\gamma)\gamma{}'_{\downarrow}}{\det A_2}A^{ji}_2\\ &&+\sum_{\gamma\in\mathcal M(q_1,\text{SP})}[\gamma{}'_{\downarrow}]_+\otimes \frac{{\varepsilon}(\gamma)\gamma{}'_{\downarrow}}{\partial_1^{11}}.\end{eqnarray*}
We get the following lemma:
Lemma 7·2.
\begin{eqnarray*}&&D(\text{Tor}(M,\rho_0;\,e))\\ &=&\sum_{\gamma\in\mathcal M(\text{NP},p_1)}[\gamma_{\cap}']_+\otimes \frac{\gamma{}'_{\downarrow}}{\partial_3^{11}}+\sum_{i,j\ge 2}\sum_{\gamma\in\mathcal M(p_i,q_j)}[\gamma_{\cap}']_+\otimes \frac{\gamma'_{\downarrow}}{\det A_2}A^{ji}_2\\ &&+\sum_{\gamma\in\mathcal M(q_1,\text{SP})}[\gamma_{\cap}']_+\otimes \frac{\gamma{}'_{\downarrow}}{\partial_1^{11}}.\end{eqnarray*}
7·3. The computation of
$d'(M,\rho_0;\,e)$
by using
$g^{\kern0.5pt f}$
By using the explicit description of
$g^{\kern0.5pt f}$
with respect to the basis
${\bf b}_e$
and the formula given in Proposition 6·8, we have the following description of
$d'(M,\rho_0;\,e)$
:
Lemma 7·3.
\begin{eqnarray*}&&d'(M,\rho_0;\,e)\\ &=&\sum_{\gamma\in\mathcal M(\text{NP},p_1)}[\gamma_{\cap}']_+\otimes\gamma{}'_{\downarrow}(\partial_3^{11})^{-1}+\sum_{i,j\ge 2}\sum_{\gamma\in\mathcal M(p_i,q_j)}[\gamma_{\cap}']_+\otimes \frac{\gamma{}'_{\downarrow}}{\det A_2}A_2^{ji}\\ &&+\sum_{\gamma\in\mathcal M(q_1,\text{SP})}[\gamma_{\cap}']_+\otimes\gamma{}'_{\downarrow}(\partial_1^{11})^{-1}.\end{eqnarray*}
8. Lescop’s invariant and
$d'(M,\rho_0;\,e)$
Let M be a closed oriented 3-manifold with
$b_1(M)=\text{rk} H_1(M;\,{\mathbb{Z}})=1$
. In this section we review the Lescop’s invariant
$I_{\Delta}\in Q(H)$
introduced in [
Reference Lescop16
] essentially as
$d'(M,\rho_0;\,e)$
for a special Euler structure e. Then we give an alternative proof of Lescop’s theorem ([
Reference Lescop16
, theorem 4·7]) on the relation between
$I_{\Delta}$
and the normalised Alexander polynomial
$\Delta(t)$
.
Let
$\tau\,:\,TM\to M\times {\mathbb{R}}^3$
be a framing. Take a vector
$v\in S^2\subset{\mathbb{R}}^3$
. We have a non-vanishing vector field
$\tau^{-1}(v)$
on M. Let
$e_{\tau}$
be the Euler structure determined by
$\tau^{-1}(v)$
. In our language, the invariant
$I_{\Delta}$
is defined to be an element of Q(H) characterised by the following equation:
Here
$K\subset M$
is an oriented knot satisfying
$[K]=1\in H_1(M;\,{\mathbb{Z}})$
.
Proposition 8·1 ([
Reference Lescop16
, theorem 4·7]). Let M be a closed oriented 3-manifold with
$b_1(M)=1$
. Let
$K\subset M$
be an oriented knot satisfying
$[K]=1\in H_1(M;\,{\mathbb{Z}})$
. Let
$e_{\tau}$
be an Euler structure given by a framing
$\tau\,:\,TM\to M\times {\mathbb{R}}^3$
. Then
Here t is a generator of H given as
$[K]=t$
. The Alexander polynomial
$\Delta(t)\in Q(H)$
is normalized as
$\Delta(-t)=\Delta(t)$
and
$\Delta(1)=1$
.
Proof. It is known (see [ Reference Turaev20 , chapter II, section 5·2]) that the normalised Alexander polynomial can be computed form the Reidemeister–Turaev torsion as
Thus
\begin{eqnarray*}d'(M,\rho_0;\,e_{\tau})&=&D(\text{Tor}(M,\rho_0;\,e_{\tau}))\\ &=&D\left((t-1)^{-1}(t^{-1}-1)^{-1}\Delta(t)\right)\\ &=&[t]\otimes\left(\frac{1+t}{1-t}+\frac{t\Delta'(t)}{\Delta(t)}\right).\end{eqnarray*}
This implies that
$I_{\Delta}={1+t}/{1-t}+{t\Delta'(t)}/{\Delta(t)}$
.
Acknowledgments
The author expresses his appreciation to Professor Teruaki Kitano, Professor Takahiro Kitayama and Professor Tadayuki Watanabe for their kind and helpful comments. The author would also like to thank the referee for their valuable suggestions and comments, in particular on Euler structures and computations in the proof of main theorem. This work was supported by the Research Institute for Mathematical Sciences, an International Joint Usage/Research Center located in Kyoto University, and partly supported by JSPS KAKENHI Grant Number JP18K13408.





