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6 Morse-Smale complex and the category of Morse functions [03RY]

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6 Morse-Smale complex and the category of Morse functions

6.1 Notations from Morse theory

Let (Y,gY)(Y,g_{Y}) be a compact oriented Riemannian manifold of dimension nn, f:Y→𝐑f:Y\to{{\bf R}} be a smooth Morse function. We will denote the set of critical points of ff by C​r​(f)Cr(f). If x∈C​r​(f)x\in Cr(f), we will denote by UxU_{x} (resp. SxS_{x}) the unstable (resp. stable) submanifolds associated with xx. Namely, Ux={y∈Y|l​i​mtβ†’+βˆžβ€‹eβˆ’t​g​r​a​d​(f)​y=x}U_{x}=\{y\in Y|\,lim_{t\to+\infty}e^{-t\,grad(f)}y=x\}, and Sx={y∈Y|l​i​mtβ†’+βˆžβ€‹et​g​r​a​d​(f)​y=x}S_{x}=\{y\in Y|\,lim_{t\to+\infty}e^{t\,grad(f)}y=x\}.

Let i​n​d​(x)ind(x) be the Morse index of xx, i.e. the negative rank of the quadratic form (βˆ‚2f)|TxY,x∈Cr(f)({\partial}^{2}f)_{|T_{x}Y},x\in Cr(f). The manifolds SxS_{x} and UxU_{x} are diffeomorphic to open balls of dimensions i​n​d​(x)ind(x) and nβˆ’i​n​d​(x)n-ind(x) respectively. It follows that the cohomology of SxS_{x} with compact support is a graded vector space with the only non-zero 11-dimensional component in degree i​n​d​(x)ind(x): Hcβˆ—β€‹(Sx)≃𝐙⁑[βˆ’i​n​d​(x)]H^{\ast}_{c}(S_{x})\simeq{{\bf Z}}[-ind(x)]. A choice of generator defines an orientation of SxS_{x}. If the function ff satisfies Morse-Smale transversality condition, i.e. for any x,y∈C​r​(f)x,y\in Cr(f) the manifolds SxS_{x} and UyU_{y} intersect transversally, then Y=βŠ”x∈C​r​(f)SxY=\sqcup_{x\in Cr(f)}S_{x} is a cell decomposition of YY. The cohomology Hβˆ—β€‹(Y,𝐙)H^{\ast}(Y,{{\bf Z}}) can be computed as the cohomology of the Morse complex (Mβˆ—(Y,f),βˆ‚)(M^{\ast}(Y,f),\partial), with the components Mi​(Y,f)=βˆ‘x∈C​r​(f),i​n​d​(x)=iHci​(Sx)M^{i}(Y,f)=\sum_{x\in Cr(f),ind(x)=i}H^{i}_{c}(S_{x}). Let us choose orientations of manifolds SxS_{x} for all x∈C​r​(f)x\in Cr(f). We endow UxU_{x} with the dual orientations. The graded module Mi​(Y,f)M^{i}(Y,f) can be identified with βŠ•0≀i≀n𝐙C​ri[βˆ’i]\oplus_{0\leq i\leq n}{{\bf Z}}^{Cr_{i}}[-i] where C​riCr_{i} is the set of critical points of ff of index ii. The choice of orientations gives a basis ([x])x∈C​r​(f)([x])_{x\in Cr(f)} of Mβˆ—β€‹(Y,f)M^{\ast}(Y,f).

The differential βˆ‚\partial is the standard Morse differential:

βˆ‚([x])=βˆ‘y∈C​r​(f),i​n​d​(y)=i​n​d​(x)+1d​e​g​((Ux∩Sy)/𝐑)β‹…[y],\partial([x])=\sum_{y\in Cr(f),ind(y)=ind(x)+1}deg(({U}_{x}\cap{S}_{y})/{{\bf R}})\cdot[y],

where (Ux∩Sy)/𝐑({U}_{x}\cap{S}_{y})/{{\bf R}} an oriented 00-dimensional manifold (a set of points with signs), and d​e​g​(β‹…)βˆˆπ™deg(\cdot)\in{\bf Z} denotes the total number of points counted with signs. The action of 𝐑{{\bf R}} arises from the natural reparametrization x↦x+tx\mapsto x+t of the gradient trajectories.

There is also a generalization Mβˆ—β€‹(Y,f,ρ)M^{\ast}(Y,f,\rho) of the Morse complex for a flat vector bundle ρ\rho (see [BZ], [HL]).

6.2 Morse A∞A_{\infty}-category of smooth functions

Here we will define the Morse category of smooth functions M⁑(Y)M(Y) following [FuO]. It will be an A∞A_{\infty}-pre-category over 𝐂{{\bf C}}. Objects of M⁑(Y)M(Y) are pairs (f,ρ)(f,\rho), where f:Y→𝐑f:Y\to{\bf R} is a smooth function, and ρ\rho is a local system of finite-dimensional complex vector spaces on YY. Before defining the transversality of objects, we will define the transversality of functions.

Suppose we are given a sequence of smooth functions (f0,…,fk),kβ‰₯2(f_{0},...,f_{k}),k\geq 2 such that all fiβˆ’fj,iβ‰ jf_{i}-f_{j},i\neq j are Morse functions, and a sequence of critical points xi∈C​r​(fiβˆ’fi+1),0≀i≀kβˆ’1,xk∈C​r​(f0βˆ’fk)x_{i}\in Cr(f_{i}-f_{i+1}),0\leq i\leq k-1,x_{k}\in Cr(f_{0}-f_{k}). We will use oriented binary planar trees in order to describe certain moduli spaces associated with such sequences. Let us fix a planar trivalent tree TT with k+1k+1 tails vertices. Among the tail vertices we choose one and call it the root vertex. Let us orient edges of TT along the shortest paths towards the root. Thus, TT becomes a binary tree considered as an oriented tree . We depict TT inside of the standard unit disc DβŠ‚π‘2D\subset{{\bf R}}^{2} in such a way that tail vertices of TT belong to βˆ‚D\partial D, and connected components of Dβˆ–TD\setminus T are cyclically numbered from 00 to kk in the clockwise order. We assume that numbers attached to two regions near the root vertex are 00 and kk.

[Uncaptioned image]

We define a gradient immersion of TT into YY as a continuous map j:T→Yj:T\to Y such that:

1) The restriction j|ej|_{e} is an orientation preserving homeomorphism of the edge ee onto an interval in the gradient line of fl⁑(e)βˆ’fr⁑(e)f_{l(e)}-f_{r(e)}, where the label l⁑(e)l(e) (resp. r⁑(e)r(e)) corresponds to the region of Dβˆ–TD\setminus T which is left (resp. right) to ee.

2) Each tail vertex vv is mapped to the point xv∈C​r​(flvβˆ’frv)x_{v}\in Cr(f_{l_{v}}-f_{r_{v}}), where lvl_{v} (resp. rvr_{v}) is the label of the region which is left (resp. right) to the only tail edge containing vv.

We will need immersed binary trees (let us call them gradient trees) in order to define compositions and transversal sequences in the Morse A∞A_{\infty}-pre-category. These structures can be defined in terms of certain varieties, which we are going to describe now.

Suppose that we are given a sequence of functions (f0,…,fk),kβ‰₯2(f_{0},...,f_{k}),k\geq 2 and critical points (x0,…,xk)(x_{0},\dots,x_{k}) as above, and a binary planar tree TT. Let us consider the manifold Y⁑(T)=YVi​(T)Y(T)=Y^{V_{i}(T)}, where Vi​(T)V_{i}(T) is the set of internal vertices of TT. We are going to define several submanifolds in Y⁑(T)Y(T). For each tail vertex vm,0≀m≀kβˆ’1v_{m},0\leq m\leq k-1 we define Zvm=Ο€v^mβˆ’1​(Uxm)Z_{v_{m}}=\pi_{\hat{v}_{m}}^{-1}(U_{x_{m}}) and for m=km=k we define Zvk=Ο€v^kβˆ’1​(Sxk)Z_{v_{k}}=\pi_{\hat{v}_{k}}^{-1}(S_{x_{k}}). Here v^l\hat{v}_{l} denotes the second endpoint of the edge of TT containing vlv_{l}, and Ο€v:Y⁑(T)β†’Y\pi_{v}:Y(T)\to Y is the canonical projection on the factor corresponding to v∈Vi​(T)v\in V_{i}(T).

For pair (fi,fj)(f_{i},f_{j}) we define a subset Zi,jβŠ‚YΓ—YZ_{i,j}\subset Y\times Y, consisting of pairs (y1,y2)(y_{1},y_{2}) such that y1β‰ y2y_{1}\neq y_{2} and y2=et​g​r​a​d​(fiβˆ’fj)​y1y_{2}=e^{t\,grad(f_{i}-f_{j})}y_{1} for some t>0t>0. Then Zi,jZ_{i,j} is a non-compact submanifold of YΓ—YY\times Y.

An edge ee of TT we call internal if both endpoints of it are internal vertices. The set of internal edges we denote by Ei​(T)E_{i}(T). For each internal edge e∈Ei​(T)e\in E_{i}(T), which separates two regions labeled by l⁑(e)l(e) (left) and r⁑(e)r(e) (right), we define a submanifold Ze=Ο€eβˆ’1​(Zl⁑(e),r⁑(e))Z_{e}=\pi_{e}^{-1}(Z_{l(e),r(e)}), where Ο€e:Y⁑(T)β†’YΓ—Y\pi_{e}:Y(T)\to Y\times Y is the natural projection.

It follows from the definitions that the space of gradient immersions of a given TT as above, up to homeomorphisms preserving tails, can be identified with β„³(T;f0,…,fk;x0,…,xk):=(∩0≀m≀kZvm)∩(∩e∈Ei​(T)Ze)βŠ‚YVi​(T){\cal M}(T;f_{0},...,f_{k};x_{0},...,x_{k}):=(\cap_{0\leq m\leq k}Z_{v_{m}})\cap(\cap_{e\in E_{i}(T)}Z_{e})\subset Y^{V_{i}(T)}.

Definition 18

We say that a sequence (f0,…,fk),kβ‰₯2(f_{0},\dots,f_{k}),\,k\geq 2 is TT-transversal for a given tree TT, if for any sequence of intersection points (x0,…,xk)(x_{0},\dots,x_{k}) such that

βˆ‘i=0kβˆ’1i​n​d​(xi)βˆ’i​n​d​(xk)≀kβˆ’2\sum_{i=0}^{k-1}ind(x_{i})-ind(x_{k})\leq k-2

the collection of submanifolds ((Zvm)0≀m≀k,(Ze)e∈Ei​(T))\bigl((Z_{v_{m}})_{0\leq m\leq k},(Z_{e})_{e\in E_{i}(T)}\bigr) is transversal in Y⁑(T)Y(T) (i.e. intersection of any subcollection is transversal). For k=1k=1, we say that (f0,f1)(f_{0},f_{1}) is TT-transversal (there is only one tree TT in this case) if f0βˆ’f1f_{0}-f_{1} is a Morse function, satisfying the Morse-Smale transversality condition.

Remark 15

As in the case of Fukaya category we consider here only spaces ℳ⁑(T,f0,…,fk,x0,…,xk){\cal M}(T;f_{0},...,f_{k};x_{0},...,x_{k}) of (virtual) dimensions less or equal than zero. Our condition in the case of strictly negative dimension means that the moduli space is empty.

It can be proven (see [Fu1]) that there exists a subset of second Baire category in (Cβˆžβ€‹(Y))𝐙(C^{\infty}(Y))^{{\bf Z}} such that for any element (fi)iβˆˆπ™(f_{i})_{i\in{\bf Z}} of this set and for any strictly increasing sequence of integers OPENi0<β‹―<ik)i_{0}<\dots<i_{k}) and for any planar tree TT with k+1k+1 tails, the sequence (fi0,…,fik)(f_{i_{0}},\dots,f_{i_{k}}) is TT-transversal.

Definition 19

A sequence of objects (f0,ρ0),…,(fk,ρk)(f_{0},\rho_{0}),...,(f_{k},\rho_{k}) is called transversal if for any mβ‰₯1m\geq 1 and any binary tree TT with m+1m+1 tails, an arbitrary subsequence (fi0,…,fim),i0<…<im(f_{i_{0}},...,f_{i_{m}}),i_{0}<...<i_{m} is TT-transversal.

For any two transversal objects W0=(f0,ρ0)W_{0}=(f_{0},\rho_{0}) and W1=(f1,ρ1)W_{1}=(f_{1},\rho_{1}) we define the space of morphisms H​o​mM⁑(Y)​(W0,W1)Hom_{M(Y)}(W_{0},W_{1}) as the Morse complex Mβˆ—β€‹(Y,f0βˆ’f1,ρ0βˆ—βŠ—Ο1)M^{\ast}(Y,f_{0}-f_{1},\rho_{0}^{\ast}\otimes\rho_{1}). Now we define the A∞A_{\infty}-structure on M⁑(Y)M(Y).

The map m1:H​o​m​((f0,ρ0),(f1,ρ1))β†’H​o​m​((f0,ρ0),(f1,ρ1))​[1]m_{1}:Hom((f_{0},\rho_{0}),(f_{1},\rho_{1}))\to Hom((f_{0},\rho_{0}),(f_{1},\rho_{1}))[1] is the standard differential in the Morse-Smale complex. Higher compositions mkm_{k} where kβ‰₯2k\geq 2 for transversal sequences of objects are linear maps

mk:βŠ—0≀i≀kβˆ’1Hom((fi,ρi),(fi+1,ρi+1))β†’Hom((f0,ρ0),(fk,ρk))[2βˆ’k]m_{k}:\otimes_{0\leq i\leq k-1}Hom((f_{i},\rho_{i}),(f_{i+1},\rho_{i+1}))\to Hom((f_{0},\rho_{0}),(f_{k},\rho_{k}))[2-k]

Each mkm_{k} is defined as a sum mk=βˆ‘Β±mk,Tm_{k}=\sum\pm m_{k,T} where TT runs through the set of isomorphism classes of oriented binary planar trees with (k+1)(k+1) tails. Let us describe the summands mk,Tm_{k,T}. For simplicity we will give the formulas in the case when all local systems are trivial of rank one.

Let us fix critical points xi∈C​r​(fiβˆ’fi+1),0≀i≀kβˆ’1,yk∈C​r​(f0βˆ’fk)x_{i}\in Cr(f_{i}-f_{i+1}),0\leq i\leq k-1,y_{k}\in Cr(f_{0}-f_{k}), such that βˆ‘0≀i≀kβˆ’1i​n​d​(xi)=i​n​d​(yk)+2βˆ’k\sum_{0\leq i\leq k-1}ind(x_{i})=ind(y_{k})+2-k, and orientations of manifolds Sxi,0≀i≀kS_{x_{i}},0\leq i\leq k. It follows from the definition of a transversal sequence that the moduli space of gradient trees ℳ⁑(T,f0,…,fk,y0,…,yk){\cal M}(T;f_{0},...,f_{k};y_{0},...,y_{k}) is an oriented compact zero-dimensional manifold.

Definition 20

We define compositions mk,kβ‰₯2m_{k},k\geq 2 by the formula

mk​([y0],…,[ykβˆ’1])=βˆ‘[T]βˆ‘yk∈C​r​(f0βˆ’fk)d​e​g​(ℳ⁑(T,f0,…,fk,y0,…,yk))β‹…[yk]m_{k}([y_{0}],...,[y_{k-1}])=\sum_{[T]}\sum_{y_{k}\in Cr(f_{0}-f_{k})}deg({\cal M}(T;f_{0},...,f_{k};y_{0},...,y_{k}))\cdot[y_{k}]

where [T][T] is the equivalence class of TT as an abstract oriented planar tree, and d​e​g​(β‹…)βˆˆπ™deg(\cdot)\in{\bf Z} is the total number of points counted with signs, as before.

For local systems of higher ranks one proceeds as in the case of Fukaya categories, using flat connections in order to define an analog of the holonomy of local systems.

One can obtain slightly different formulas for mkm_{k} in the following way. For any point Ξ³βˆˆβ„³β‘(T,f0,…,fk,y0,…,yk)\gamma\in{\cal M}(T;f_{0},...,f_{k};y_{0},...,y_{k}) we define the weight

wΞ³=exp(βˆ’1Ξ΅βˆ‘e∈E⁑(T)varΞ³(fl⁑(e)βˆ’fr⁑(e)))βˆˆπ‚Ξ΅.w_{\gamma}=exp(-{1\over{\varepsilon}}\sum_{e\in E(T)}var_{\gamma}(f_{l(e)}-f_{r(e)}))\in{{\bf C}}_{\varepsilon}.

Here v​a​rγ​(fl⁑(e)βˆ’fr⁑(e))>0var_{\gamma}(f_{l(e)}-f_{r(e)})>0 is a variation of fl⁑(e)βˆ’fr⁑(e)f_{l(e)}-f_{r(e)} along the gradient line γ⁑(e)\gamma(e), which is defined such as follows: v​a​rγ​(fl⁑(e)βˆ’fr⁑(e))=(fl⁑(e)βˆ’fr⁑(e))​(ym​a​x)βˆ’(fl⁑(e)βˆ’fr⁑(e))​(ym​i​n)var_{\gamma}(f_{l(e)}-f_{r(e)})=(f_{l(e)}-f_{r(e)})(y_{max})-(f_{l(e)}-f_{r(e)})(y_{min}), where ym​a​xy_{max} and ym​i​ny_{min} are the endpoints of γ⁑(e)\gamma(e), such that (fl⁑(e)βˆ’fr⁑(e))​(ym​a​x)βˆ’(fl⁑(e)βˆ’fr⁑(e))​(ym​i​n)>0(f_{l(e)}-f_{r(e)})(y_{max})-(f_{l(e)}-f_{r(e)})(y_{min})>0. After extension of scalars to 𝐂Ρ{{\bf C}}_{\varepsilon} one can choose another basis in H​o​mM⁑(Y)​(W0,W1)Hom_{M(Y)}(W_{0},W_{1}), namely [y]n​e​w=[y]​e​x​p​((f0​(y)βˆ’f1​(y))Ξ΅)[y]_{new}=[y]exp({(f_{0}(y)-f_{1}(y))\over{\varepsilon}}) for y∈C​r​(f0βˆ’f1)y\in Cr(f_{0}-f_{1}). Then the formulas for mkm_{k} will be modified. The contribution of each Ξ³\gamma will be multiplied by wΞ³w_{\gamma}. The formulas will be similar to those for the Fukaya-Oh category (see Section 5.2).

6.3 De Rham A∞A_{\infty}-category of smooth functions

The other A∞A_{\infty}-pre-category we are interested in will be a differential-graded category (dg-category for short). In other words, it is an A∞A_{\infty}-category with strict identity morphisms and vanishing compositions mn,nβ‰₯3m_{n},n\geq 3. We will call it de Rham category of YY and denote by D​R​(Y)DR(Y). Objects of D​R​(Y)DR(Y) are same as for M⁑(Y)M(Y). They are pairs (f,ρ)(f,\rho), where f:Y→𝐑f:Y\to{\bf R} is a smooth function and ρ\rho is a local system on YY. Morphisms are complexes defined by the formula

HomD​R​(Y)((f0,ρ0),(f1,ρ1))=Ξ“(Y,βˆ§βˆ—TYβˆ—βŠ—Hom(ρ0,ρ1)).Hom_{DR(Y)}((f_{0},\rho_{0}),(f_{1},\rho_{1}))=\Gamma(Y,\wedge^{\ast}T^{\ast}_{Y}\otimes Hom(\rho_{0},\rho_{1})).

Notice that the space of morphisms does not depend on f0f_{0} and f1f_{1}. The composition of morphisms is defined in the obvious way: in a local trivialization of ρ0\rho_{0} and ρ1\rho_{1} it is given by the product of matrices with the coefficients in Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y).

Now we can formulate the main result of this section.

Theorem 2

A∞A_{\infty}-pre-categories M⁑(Y)M(Y) and D​R​(Y)DR(Y) are equivalent.

The proof of the theorem will occupy the rest of the section. First, we will discuss a version of formulas from β€œhomological perturbation theory” (see [GS], [Me]). They will give an A∞A_{\infty}-structure on a subcomplex of a dg-algebra. Then we will discuss an approach to the proof based on the ideas of [HL]. It seems plausible that an alternative proof (but, presumably, much more difficult) can be obtained within the framework of Witten complex, using methods of [BZ].

6.4 A∞A_{\infty}-structure on a subcomplex

In this section we are going to restate in a convenient form some results from [GS] and [Me].

Let (A,mn),nβ‰₯1(A,m_{n}),n\geq 1 be a non-unital A∞A_{\infty}-algebra, Ξ :Aβ†’A\Pi:A\to A be an idempotent which commutes with the differential d=m1d=m_{1}. In other words, Ξ \Pi is a linear map of degree zero such that d​Π=Π​d,Ξ 2=Ξ d\Pi=\Pi d,\Pi^{2}=\Pi. Assume that we are given an homotopy H:Aβ†’A⁑[βˆ’1]H:A\to A[-1], 1βˆ’Ξ =d​H+H​d1-\Pi=dH+Hd. Let us denote the image of Ξ \Pi by BB. Then we have an embedding i:Bβ†’Ai:B\to A and a projection p:Aβ†’Bp:A\to B, such that Ξ =i∘p\Pi=i\circ p.

Let us introduce a sequence of linear operations mnB:BβŠ—nβ†’B⁑[2βˆ’n]m_{n}^{B}:B^{\otimes n}\to B[2-n] in the following way:

a) m1B:=dB=p∘m1∘im_{1}^{B}:=d^{B}=p\circ m_{1}\circ i;

b) m2B=p∘m2∘(iβŠ—i)m_{2}^{B}=p\circ m_{2}\circ(i\otimes i);

c) mnB=βˆ‘TΒ±mn,T,nβ‰₯3m_{n}^{B}=\sum_{T}\pm m_{n,T},n\geq 3.

Here the summation is taken over all oriented planar trees TT with n+1n+1 tails vertices (including the root vertex), such that the (oriented) valency |v||v| (the number of ingoing edges) of every internal vertex of TT is at least 22. In order to describe the linear map mn,T:BβŠ—nβ†’B⁑[2βˆ’n]m_{n,T}:B^{\otimes n}\to B[2-n] we need to make some preparations. Let us consider another tree TΒ―\bar{T} which is obtained from TT by the insertion of a new vertex into every internal edge. As a result, there will be two types of internal vertices in TΒ―{\bar{T}}: the β€œold” vertices, which coincide with the internal vertices of TT, and the β€œnew” ones, which can be thought geometrically as the midpoints of the internal edges of TT.

To every tail vertex of TΒ―{\bar{T}} we assign the embedding ii. To every β€œold” vertex vv we assign mkm_{k} with k=|v|k=|v|. To every β€œnew” vertex we assign the homotopy operator HH. To the root we assign the projector pp. Then moving along the tree down to the root one reads off the map mn,Tm_{n,T} as the composition of maps assigned to vertices of TΒ―\bar{T}. Here is an example of TT and TΒ―\bar{T}:

[Uncaptioned image]

[Uncaptioned image]

Proposition 4

The linear map m1Bm_{1}^{B} defines a differential in BB.

Proof. Clear. β– \blacksquare

Theorem 3

The sequence mnB,nβ‰₯1m_{n}^{B},n\geq 1 gives rise to a structure of an A∞A_{\infty}-algebra on BB.

Sketch of the proof. The proof is quite straightforward, so we just briefly show main steps of computations.

First, one observes that pp and ii are homomorphisms of complexes. In order to prove the theorem we will replace for a given nβ‰₯2n\geq 2 each summand mn,Tm_{n,T} by a different one, and then compute the result in two different ways. Let us consider a collection of trees {TΒ―e}e∈E⁑(TΒ―)\{\bar{T}_{e}\}_{e\in E(\bar{T})} such that TΒ―e\bar{T}_{e} is obtained from TΒ―\bar{T} in the following way:

a) we split the edge ee into two edges by inserting a new vertex wew_{e} inside ee;

b) the remaining part of TΒ―\bar{T} is unchanged.

We assign d=m1d=m_{1} to the vertex wew_{e} edge, and keep all other assignments untouched. In this way we obtain a map mn,TΒ―e:BβŠ—nβ†’B⁑[3βˆ’n]m_{n,\bar{T}_{e}}:B^{\otimes n}\to B[3-n].

Let us consider the following sum (with appropriate signs):

m^nB=βˆ‘Tβˆ‘e∈E⁑(TΒ―)Β±mn,TΒ―e.\hat{m}_{n}^{B}=\sum_{T}\sum_{e\in E(\bar{T})}\pm m_{n,\bar{T}_{e}}.

We can compute it in two different ways: using the relation 1βˆ’Ξ =d​H+H​d1-\Pi=dH+Hd, and using the formulas for d⁑(mj),jβ‰₯2d(m_{j}),\,j\geq 2 given by the A∞A_{\infty}-structure on AA. The case of the relation 1βˆ’Ξ =d​H+H​d=:d⁑(H)1-\Pi=dH+Hd=:d(H) gives

m^nB=d⁑(mnB)βˆ’mnB,Ξ +mnB,1\hat{m}_{n}^{B}=d(m_{n}^{B})-m_{n}^{B,\Pi}+m_{n}^{B,1}

where mnB,Ξ m_{n}^{B,\Pi} is defined analogously to mnBm_{n}^{B}, with the only difference that we assign to a new vertex operator Ξ \Pi instead of HH for some edge e∈Ei​(T)e\in E_{i}(T). Similarly, the summand mnB,1m_{n}^{B,1} is defined if we assign to a new vertex operator 1=i​dA1=id_{A} instead of HH. Formulas for d⁑(mj)d(m_{j}) are quadratic expressions in ml,l<jm_{l},\,l<j. This gives us another identity

m^nB=mnB,1\hat{m}_{n}^{B}=m_{n}^{B,1}

Thus we have d⁑(mnB)=mnB,Ξ d(m_{n}^{B})=m_{n}^{B,\Pi}, and it is exactly the A∞A_{\infty}-constraint for the collection (mnB)nβ‰₯1(m_{n}^{B})_{n\geq 1}. β– \blacksquare

Moreover, using similar technique, one can prove the following result.

Proposition 5

There is a canonical A∞A_{\infty}-morphism g:Bβ†’Ag:B\to A, which defines a quasi-isomorphism of A∞A_{\infty}-algebras.

For the convenience fo the reader we give an explicit formula for a canonical choice of gg. The operator g1:Bβ†’Ag_{1}:B\to A is defined as the inclusion ii. For nβ‰₯2n\geq 2 we define gng_{n} as the sum of terms gn,Tg_{n,T} over all planar trees TT with n+1n+1 tails. Each term gn,Tg_{n,T} is similar to the term mn,Tm_{n,T} defined above, the only difference is that we insert operator HH instead of pp into the root vertex.

One can also construct an explicit A∞A_{\infty}-quasi-isomorphism Aβ†’BA\to B.

Remark 16

a) Similar construction works in the case of an arbitrary non-unital A∞A_{\infty}-category. In that case one needs projectors Ξ X,Y\Pi_{X,Y} and homotopies HX,YH_{X,Y} for every graded space of morphisms H​o​m​(X,Y)Hom(X,Y). All formulas remain the same as in the case of A∞A_{\infty}-algebras. The resulting A∞A_{\infty}-category with the spaces of morphisms given by Ξ X,Y​(H​o​m​(X,Y))\Pi_{X,Y}(Hom(X,Y)) is equivalent to the original one. We will use this fact later.

b) Propositions 4 and 5 should hold in a much more general case of algebras over operads (see e.g. [M]).

6.5 Projectors and homotopies in Morse theory

We would like to apply formulas for the A∞A_{\infty}-structure on a subcomplex to the proof of the Theorem 2. In order to do that we need to identify the Morse complex with a direct summand of the de Rham complex. Our approach is based on the ideas of Harvey and Lawson (see [HL]).

Let YY be a compact oriented smooth manifold, d​i​m​Y=ndim\,Y=n. The space of currents D′​(Y)D^{\prime}(Y) we will identify with the space of distribution-valued differential forms. Continuous linear operators Ξ©βˆ—β€‹(Y)β†’D′​(Y)\Omega^{\ast}(Y)\to D^{\prime}(Y) are given by their Schwartz kernels, which are elements of D′​(YΓ—Y)D^{\prime}(Y\times Y). Smoothening operators D′​(Y)β†’Ξ©βˆ—β€‹(Y)D^{\prime}(Y)\to\Omega^{\ast}(Y) have kernels in Ξ©βˆ—β€‹(YΓ—Y)βŠ‚D′​(YΓ—Y)\Omega^{\ast}(Y\times Y)\subset D^{\prime}(Y\times Y).

With any oriented submanifold ZβŠ‚YZ\subset Y , dimZ=k\dim\,Z=k of finite volume we associate a canonical current [Z][Z] of degree nβˆ’kn-k (namely, we can integrate smooth kk-forms over ZZ).

Let gYg_{Y} be a Riemannian metric on YY, and ff be a Morse-Smale function. The gradient flow e​x​p​(t​g​r​a​d​(f)),tβ‰₯0exp(t\,grad(f)),t\geq 0 gives rise to a 11-parameter semigroup acting on Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y): ψt​(Ξ±)=e​x​p​(t​g​r​a​d​(f))βˆ—β€‹(Ξ±)\psi^{t}(\alpha)=exp(t\,grad(f))_{\ast}(\alpha). Schwartz kernel of ψt\psi^{t} is [Gt][G_{t}] where manifold GtβŠ‚YΓ—YG_{t}\subset Y\times Y is given by Gt:=g​r​a​p​h​(e​x​p​(t​g​r​a​d​(f)))G_{t}:=graph(exp(t\,grad(f))). We also have the identity

i​dβˆ’Οˆt=d​Ht+Ht​d,id-\psi^{t}=dH^{t}+H^{t}d,

where Ht:Ξ©βˆ—β€‹(Y)β†’Ξ©βˆ—β€‹(Y)βŠ‚D′​(Y)H^{t}:\Omega^{\ast}(Y)\to\Omega^{\ast}(Y)\subset D^{\prime}(Y) is a linear operator of degree βˆ’1-1 defined by the distributional kernel [Zt][Z_{t}], Zt:=βˆͺ0≀t′≀tgraph(exp(tβ€²grad(f)))Z_{t}:=\cup_{0\leq t^{\prime}\leq t}graph(exp(t^{\prime}\,grad(f))).

It is checked in [HL] that this picture has a limit (in certain sense) as tβ†’+∞t\to+\infty. Namely, there exist limits of currents [Gt][G_{t}] and [Zt][Z_{t}]:

[G∞]=l​i​mtβ†’+βˆžβ€‹[Gt]=βˆ‘x∈C​r​(f)[Sx]Γ—[Ux][G_{\infty}]=lim_{t\to+\infty}[G_{t}]=\sum_{x\in Cr(f)}[S_{x}]\times[U_{x}]
[Z∞]=limtβ†’+∞[Zt]=[βˆͺ0≀t<+∞Gt][Z_{\infty}]=lim_{t\to+\infty}[Z_{t}]=[\cup_{0\leq t<+\infty}G_{t}]

Linear operators ψ∞\psi^{\infty} (of degree zero) and H∞H^{\infty} (of degree βˆ’1-1), corresponding to these kernels, map Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y) to D′​(Y)D^{\prime}(Y) and satisfy the identity

iβˆ’Οˆβˆž=d​H∞+Hβˆžβ€‹d,i-\psi^{\infty}=dH^{\infty}+H^{\infty}d,

where i:Ξ©βˆ—β€‹(Y)β†’D′​(Y)i:\Omega^{\ast}(Y)\to D^{\prime}(Y) is the natural inclusion. According to the de Rham theorem this inclusion is a quasi-isomorphism of complexes, therefore ψ∞\psi^{\infty} is. Morally, Π∞:=ψ∞\Pi_{\infty}:=\psi^{\infty} should be thought of as a projector. The image Ξ βˆžβ€‹(Ξ©βˆ—β€‹(Y))βŠ‚D′​(Y)\Pi_{\infty}(\Omega^{\ast}(Y))\subset D^{\prime}(Y) coincides with βŠ•x∈C​r​(f)𝐑⋅[Ux]\oplus_{x\in Cr(f)}{{\bf R}}\cdot[U_{x}]. We have

Ξ βˆžβ€‹(Ξ±)=βˆ‘x∈C​r​(f)(∫SxΞ±)β‹…[Ux]=βˆ‘x∈C​r​(f)∫Y(α∧[Sx])β‹…[Ux].\Pi_{\infty}(\alpha)=\sum_{x\in Cr(f)}(\int_{S_{x}}\alpha)\cdot[U_{x}]=\sum_{x\in Cr(f)}\int_{Y}(\alpha\wedge[S_{x}])\cdot[U_{x}].

Moreover, the operator Π∞\Pi_{\infty} commutes with the differentials. Hence the complex Ξ βˆžβ€‹(Ξ©βˆ—β€‹(Y))\Pi_{\infty}(\Omega^{\ast}(Y)) is a finite-dimensional subcomplex of D′​(Y)D^{\prime}(Y) isomorphic to the Morse complex Mβˆ—β€‹(Y,f)M^{\ast}(Y,f). In fact it is quasi-isomorphic to both complexes Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y) and D′​(Y)D^{\prime}(Y). In this way Harvey and Lawson prove that the de Rham cohomology is isomorphic to the cohomology of Morse complex.

In order to construct actual projectors and homotopies we will proceed as follows. Let ρδ,Ξ΄β†’0\rho_{\delta},\delta\to 0 be a family of smooth closed differential nn-forms on YΓ—YY\times Y such that s​u​p​p​(ρδ)supp(\rho_{\delta}) belongs to the open Ξ΄\delta-neighborhood NΞ΄N_{\delta} of the diagonal d​i​a​gβŠ‚YΓ—Ydiag\subset Y\times Y, and the cohomology class of ρδ\rho_{\delta} in Hcn​(NΞ΄,𝐑)H^{n}_{c}(N_{\delta},{{\bf R}}) is the same as of [d​i​a​g][diag].

We define RΞ΄:D′​(Y)β†’Ξ©βˆ—β€‹(Y)R_{\delta}:D^{\prime}(Y)\to\Omega^{\ast}(Y) as the integral operator given by the kernel ρδ\rho_{\delta}.

Lemma 3

1) The operator RΞ΄R_{\delta} is a homomorphism of complexes.

2) If Z1,Z2∈YZ_{1},Z_{2}\in Y are two oriented submanifolds of finite volume such that they intersect transversally at finitely many points, and d​i​m​Z1+d​i​m​Z2=d​i​m​Ydim\,Z_{1}+dim\,Z_{2}=dim\,Y, ZΒ―1∩ZΒ―2=Z1∩Z2\overline{Z}_{1}\cap\overline{Z}_{2}={Z}_{1}\cap{Z}_{2}, then for sufficiently small Ξ΄\delta one has:

∫YRδ​([Z1])∧Rδ​([Z2])=d​e​g​(Z1∩Z2)βˆˆπ™\int_{Y}R_{\delta}([Z_{1}])\wedge R_{\delta}([Z_{2}])=deg(Z_{1}\cap Z_{2})\in{\bf Z}

3) There exists a linear operator hΞ΄:Ξ©βˆ—β€‹(Y)β†’Ξ©βˆ—β€‹(Y)h_{\delta}:\Omega^{\ast}(Y)\to\Omega^{\ast}(Y) such that its kernel has support in NΞ΄N_{\delta}, the wave front W​F​(hΞ΄)WF(h_{\delta}) is the conormal bundle of d​i​a​gβŠ‚YΓ—Ydiag\subset Y\times Y, and

dhΞ΄+hΞ΄d=idβˆ’(RΞ΄)|Ξ©βˆ—(Y).dh_{\delta}+h_{\delta}d=id-(R_{\delta})_{|\Omega^{\ast}(Y)}.

Proof . Part 1) follows from the fact that ρδ\rho_{\delta} is a closed current. Part 2) follows from the fact that RΞ΄R_{\delta} changes the supports of Zi,i=1,2Z_{i},i=1,2 by O⁑(Ξ΄)O(\delta). To prove part 3) one observes that the operators i​did and (RΞ΄)|Ξ©βˆ—(Y)(R_{\delta})_{|\Omega^{\ast}(Y)} preserve the space of smooth forms Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y), and ρδ\rho_{\delta} is cohomologous to [d​i​a​g][diag]. β– \blacksquare

Let x,y∈C​r​(f)x,y\in Cr(f) be two critical points of the same Morse index. Then d​e​g​(Sx∩Uy)=Ξ΄x​ydeg(S_{x}\cap U_{y})=\delta_{xy} (the Kronecker symbol). By the part 2) of the Lemma, for sufficiently small Ξ΄\delta we obtain the identity

∫YRδ​([Sx])∧Rδ​([Uy])=Ξ΄x​y\int_{Y}R_{\delta}([S_{x}])\wedge R_{\delta}([U_{y}])=\delta_{xy}

This implies the following result.

Proposition 6

Let us define for a sufficiently small Ξ΄\delta a linear operator D′​(Y)β†’Ξ©βˆ—β€‹(Y)D^{\prime}(Y)\to\Omega^{\ast}(Y) by the formula Πδ​(Ξ±)=βˆ‘x∈C​r​(f)(∫Yα∧Rδ​([Sx]))β‹…Rδ​([Ux]).\Pi_{\delta}(\alpha)=\sum_{x\in Cr(f)}(\int_{Y}\alpha\wedge R_{\delta}([S_{x}]))\cdot R_{\delta}([U_{x}]).

Then

1) Ξ Ξ΄2​(Ξ±)=Πδ​(Ξ±)\Pi_{\delta}^{2}(\alpha)=\Pi_{\delta}(\alpha) if Ξ±βˆˆΞ©βˆ—β€‹(Y)\alpha\in\Omega^{\ast}(Y), and Πδ​d=d​Πδ.\Pi_{\delta}d=d\Pi_{\delta}.

2) The image Πδ​(Mβˆ—β€‹(Y,f))\Pi_{\delta}(M^{\ast}(Y,f)) is a subcomplex in Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y) which is canonically isomorphic to the Morse complex Mβˆ—β€‹(Y,f)M^{\ast}(Y,f).

We define a homotopy operator HΞ΄:Ξ©βˆ—β€‹(Y)β†’Ξ©βˆ—β€‹(Y)​[βˆ’1]H_{\delta}:\Omega^{\ast}(Y)\to\Omega^{\ast}(Y)[-1] as an integral operator given by the kernel (Rδ⊠RΞ΄)​[Z∞]+(hδ⊠hΞ΄)​([d​i​a​g]).(R_{\delta}\boxtimes R_{\delta})[Z_{\infty}]+(h_{\delta}\boxtimes h_{\delta})([diag]). (The last summand is well-defined because of the condition on the wave front of hΞ΄h_{\delta}). It is easy to check that the following identity holds:

i​dβˆ’Ξ Ξ΄=d​HΞ΄+Hδ​d.id-\Pi_{\delta}=dH_{\delta}+H_{\delta}d.

Thus we have a family of homotopies and projectors parametrized by Ξ΄\delta.

Remark 17

One can define the projector Ξ Ξ΄\Pi_{\delta} using another canonical element βˆ‘x∈C​r​(f)[Sx]βŠ—Rδ​([Ux])\sum_{x\in Cr(f)}[S_{x}]\otimes R_{\delta}([U_{x}]), instead of βˆ‘x∈C​r​(f)Rδ​([Sx])βŠ—Rδ​([Ux])\sum_{x\in Cr(f)}R_{\delta}([S_{x}])\otimes R_{\delta}([U_{x}]), as we did. The above Proposition holds for the new canonical element as well.

There is a version of the previous construction, which will be useful in the next subsection. Namely, we start with a differential n+1n+1-form ρ\rho on YΓ—YΓ—(0,1)Y\times Y\times(0,1) such that for the support of s​u​p​p​(ρ)supp(\rho) belongs to βŠ”Ξ΄>0(NΞ΄,Ξ΄)\sqcup_{\delta>0}(N_{\delta},\delta) for all sufficiently small δ∈(0,1)\delta\in(0,1), and ρ\rho defines the same cohomology class in Hcn​(YΓ—YΓ—(0,1))H_{c}^{n}(Y\times Y\times(0,1)) as [d​i​a​g]Γ—(0,1)[diag]\times(0,1).

Let us consider now the spaces Ξ©0βˆ—β€‹(Y):=limβ†’Ξ΄β†’0β‘Ξ©βˆ—β€‹(YΓ—(0,Ξ΄))\Omega_{0}^{\ast}(Y):=\varinjlim_{\delta\to 0}\Omega^{\ast}(Y\times(0,\delta)) and D0′​(Y):=limβ†’Ξ΄β†’0β‘Ξ©βˆ—β€‹(0,Ξ΄)β€‹βŠ—^​D′​(Y).D_{0}^{\prime}(Y):=\varinjlim_{\delta\to 0}\Omega^{\ast}(0,\delta)\widehat{\otimes}D^{\prime}(Y). It is easy to see that both complexes Ξ©0βˆ—β€‹(Y)\Omega_{0}^{\ast}(Y) and D0′​(Y)D_{0}^{\prime}(Y) are quasi-isomorphic to Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y) .

We define a linear operator R:D0′​(Y)β†’Ξ©0βˆ—β€‹(Y)R:D_{0}^{\prime}(Y)\to\Omega_{0}^{\ast}(Y) similarly to the definition of RΞ΄R_{\delta}. Then the Lemma and the Proposition hold with obvious changes. We will denote the corresponding objects by the same letters as before, skipping the subscript Ξ΄\delta (like HH for the homotopy and Ξ \Pi for the projector). Morally, they are obtained from the old objects by extending them as differential forms β€œin the direction of Ξ΄\delta”.

6.6 Proof of the theorem

For simplicity we will assume that all local systems are trivial and have rank one. The general case is completely similar.

We are going to construct the following chain of A∞A_{\infty}-equivalences connecting D​R​(Y)DR(Y) and M⁑(Y)M(Y):

OPEND​R​(Y)β†ͺD​R0​(Y)↩D​R0t​r​(Y)↩D​R0t​r,Π​(Y))←M⁑(Y)DR(Y)\hookrightarrow DR_{0}(Y)\hookleftarrow DR_{0}^{tr}(Y)\hookleftarrow DR_{0}^{tr,\Pi}(Y))\leftarrow M(Y)

Classes of objects of all these categories will be the same, and all functors will be identical on objects.

The A∞A_{\infty}-pre-category D​R0​(Y)DR_{0}(Y) is in fact a dg-category, i.e. all sequences of objects are transversal, compositions mkm_{k} vanish for kβ‰₯3k\geq 3 and it has strict identity morphisms. The space H​o​mD​R0​(Y)​(f0,f1)Hom_{DR_{0}(Y)}(f_{0},f_{1}) is defined as limβ†’Ξ΄β†’0β‘Ξ©βˆ—β€‹(YΓ—(0,Ξ΄))=Ξ©0βˆ—β€‹(Y).\varinjlim_{\delta\to 0}\Omega^{\ast}(Y\times(0,\delta))=\Omega_{0}^{\ast}(Y). Clearly the space of morphisms does not depend on objects. Using the wedge product of differential forms we make D​R0​(Y)DR_{0}(Y) into a dg-category over the field 𝐂{\bf C}. There is a natural functor D​R​(Y)β†’D​R0​(Y)DR(Y)\to DR_{0}(Y), which is the identity map on objects. On morphisms it is the natural embedding of Ξ©βˆ—β€‹(Y)\Omega^{\ast}(Y) as the subspace of forms on YΓ—(0,Ξ΄)Y\times(0,\delta), which are pullbacks of forms on YY. Clearly it establishes an equivalence of A∞A_{\infty}-categories.

The A∞A_{\infty}-pre-category D​R0t​r​(Y)DR_{0}^{tr}(Y) is defined as the full subcategory of D​R0​(Y)DR_{0}(Y), and it differs from the latter only by the choice of transversal sequences. Namely, we use the same notion of transversality in D​R0t​r​(Y)DR_{0}^{tr}(Y) as in the Morse category.

The next A∞A_{\infty}-pre-category D​R0t​r,Π​(Y)DR_{0}^{tr,\Pi}(Y) is obtained from D​R0t​r​(Y)DR_{0}^{tr}(Y) by applying homological perturbation theory. For any two transversal objects f0,f1f_{0},f_{1} of D​R0t​r​(Y)DR_{0}^{tr}(Y) we define H​o​mD​R0t​r,Π​(Y)​(f0,f1)Hom_{DR_{0}^{tr,\Pi}(Y)}(f_{0},f_{1}) as Ξ f0,f1​(Ξ©0βˆ—β€‹(Y))\Pi_{f_{0},f_{1}}(\Omega^{\ast}_{0}(Y)). Here Ξ f0,f1\Pi_{f_{0},f_{1}} is the projector Ξ \Pi corresponding to the Morse function f0βˆ’f1f_{0}-f_{1}, it was described at the end of the previous subsection. We also have homotopies Hf0,f1H_{f_{0},f_{1}} associated with f0βˆ’f1f_{0}-f_{1}. Then formulas of homological perturbation theory (summation over trees) give rise to an A∞A_{\infty}-pre-category D​R0t​r,Π​(Y)DR_{0}^{tr,\Pi}(Y) and an equivalence D​R0t​r,Π​(Y)β†’D​R0t​r​(Y)DR_{0}^{tr,\Pi}(Y)\to DR_{0}^{tr}(Y).

The last functor Ξ¨:M(Y)β†’DR0t​r,Ξ (Y))\Psi:M(Y)\to DR_{0}^{tr,\Pi}(Y)) will have no non-trivial higher components Ξ¨n\Psi_{n} for nβ‰₯2n\geq 2. The first component Ξ¨1\Psi_{1} of it is a linear map

Ξ¨1:H​o​mM⁑(Y)​(f0,f1)β†’H​o​mD​R0t​r,Π​(Y)​(f0,f1)\Psi_{1}:Hom_{M(Y)}(f_{0},f_{1})\to Hom_{DR_{0}^{tr,\Pi}(Y)}(f_{0},f_{1})

for every transversal pair (f0,f1)(f_{0},f_{1}). Recall that H​o​mM⁑(Y)​(f0,f1)Hom_{M(Y)}(f_{0},f_{1}) has a basis {[x]}\{[x]\} labeled by critical points x∈C​r​(f0βˆ’f1)x\in Cr(f_{0}-f_{1}). We define Ξ¨1​([x])\Psi_{1}([x]) as R⁑([Sx])R([S_{x}]). It is clear that Ξ¨1\Psi_{1} gives a quasi-isomorphism of complexes for every transversal pair (f0,f1)(f_{0},f_{1}).

Now, we claim that Ξ¨\Psi is an A∞A_{\infty}-functor. This means that Ξ¨1\Psi_{1} maps all higher compositions in M⁑(Y)M(Y) to higher compositions in D​R0t​r,Π​(Y)DR_{0}^{tr,\Pi}(Y). This follows directly from the descriptions of higher compositions in both categories in terms of planar trees and the lemma in the previous subsection. Indeed, the number of functions in any given sequence is finite. For all sufficiently small Ξ΄\delta every summand in the formula for mkM⁑(Y)m_{k}^{M(Y)}, corresponding to a binary tree TT, coincides with the summand for mkM⁑(Y)m_{k}^{M(Y)} corresponding to the same TT (we can assume that Ξ΄\delta is so small that the part 2) of the Lemma can be applied). The theorem is proved. β– \blacksquare

Original mathematics by the credited authors. Source-backed reader collection; mathematical self-containment is not assessed.