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footnotesection

Index theorems for
uniformly elliptic operators

Alexander Engel
Abstract

We generalize Roe’s index theorem for graded generalized Dirac operators on amenable manifolds to multigraded elliptic uniform pseudodifferential operators.

The generalization will follow from a local index theorem that is valid on any manifold of bounded geometry. This local formula incorporates the uniform estimates present in the definition of uniform pseudodifferential operators.

Fakultät für Mathematik
Universität Regensburg
93040 Regensburg, GERMANY
alexander.engel@mathematik.uni-regensburg.de

1 Introduction

Recall the following index theorem of Roe for amenable manifolds (with notation adapted to the one used in this article):

Theorem ([Roe88a, Theorem 8.2]).

Let MM be a Riemannian manifold of bounded geometry and DD a generalized Dirac operator associated to a graded Dirac bundle SS of bounded geometry over MM.

Let (Mi)i(M_{i})_{i} be a Følner sequence111That is to say, for every r>0r>0 we have volBr(Mi)volMii0\frac{\operatorname{vol}B_{r}(\partial M_{i})}{\operatorname{vol}M_{i}}\stackrel{{\scriptstyle i\to\infty}}{{\longrightarrow}}0. Manifolds admitting such a sequence are called amenable. for MM, τ()\tau\in(\ell^{\infty})^{\ast} a linear functional associated to a free ultrafilter on \mathbb{N}, and θ\theta the corresponding trace on the uniform Roe algebra of MM.

Then we have

θ(μu(D))=τ(1volMiMiind(D)).\theta(\mu_{u}(D))=\tau\Big{(}\frac{1}{\operatorname{vol}M_{i}}\int_{M_{i}}\operatorname{ind}(D)\Big{)}.

Here ind(D)\operatorname{ind}(D) is the usual integrand for the topological index of DD in the Atiyah–Singer index formula, so the right hand side is topological in nature. On the left hand side of the formula we have the coarse index class μu(D)K0(Cu(M))\mu_{u}(D)\in K_{0}(C_{u}^{\ast}(M)) of DD in the KK-theory of the uniform Roe algebra of MM evaluated under the trace θ\theta. This is an analytic expression and may be computed as θ(μu(D))=τ(1volMiMitrskf(D)(x,x)𝑑x)\theta(\mu_{u}(D))=\tau\Big{(}\frac{1}{\operatorname{vol}M_{i}}\int_{M_{i}}\operatorname{tr}_{s}k_{f(D)}(x,x)\ dx\Big{)}, where kf(D)(x,y)k_{f(D)}(x,y) is the integral kernel of the smoothing operator f(D)f(D), where ff is an even Schwartz function with f(0)=1f(0)=1.

In this article we will generalize this theorem to all multigraded, elliptic, symmetric uniform pseudodifferential operators. So especially we also encompass Toeplitz operators since they are included in the ungraded case. This generalization will follow from a local index theorem that will hold on any manifold of bounded geometry, i.e., without an amenability assumption on MM.

Let us state our local index theorem in the formulation using twisted Dirac operators associated to spinc structures:

Theorem A (Theorem 1).

Let MM be an mm-dimensional spinc manifold of bounded geometry and without boundary. Denote the associated Dirac operator by DD.

Then we have the following commutative diagram:

Ku(M)\textstyle{K^{\ast}_{u}(M)\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}[D]\scriptstyle{-\cap[D]}\scriptstyle{\cong}ch()ind(D)\scriptstyle{\operatorname{ch}(-)\wedge\operatorname{ind}(D)}Kmu(M)\textstyle{K_{m-\ast}^{u}(M)\ignorespaces\ignorespaces\ignorespaces\ignorespaces}αch\scriptstyle{\alpha_{\ast}\circ\operatorname{ch}^{\ast}}Hb,dR(M)\textstyle{H_{b,\mathrm{dR}}^{\ast}(M)\ignorespaces\ignorespaces\ignorespaces\ignorespaces}\scriptstyle{\cong}Hmu,dR(M)\textstyle{H^{u,\mathrm{dR}}_{m-\ast}(M)}

where in the top row \ast is either 0 or 11 and in the bottom row \ast is either ev\mathrm{ev} or odd\mathrm{odd}.

Here Kmu(M)K_{m-\ast}^{u}(M) is uniform KK-homology of MM invented by Špakula [Špa09] and Ku(M)K_{u}^{\ast}(M) is the corresponding uniform KK-theory which we will recall in Section 2.3. The map [D]-\cap[D] is the cap product and that it is an isomorphism was shown in [Eng15a, Section 4.4]. Moreover, Hb,dR(M)H_{b,\mathrm{dR}}^{\ast}(M) denotes the bounded de Rham cohomology of MM and ind(D)\operatorname{ind}(D) the topological index class of DD in there. Furthermore, Hmu,dR(M)H^{u,\mathrm{dR}}_{m-\ast}(M) is the uniform de Rham homology of MM to be defined in Section 3.2 via Connes’ cyclic cohomology, and that it is Poincaré dual to bounded de Rham cohomology is proved in Theorem 10. Finally, let us note that we will also prove in Section 3.3 that the Chern characters induce isomorphisms after a certain completion that also kills torsion, similar to the case of compact manifolds.

Using a series of steps as in Connes’ and Moscovici’s proof of [CM90, Theorem 3.9] we will generalize the above computation of the Poincaré dual of (αch)([D])Hmu,dR(M)(\alpha_{\ast}\circ\operatorname{ch}^{\ast})([D])\in H^{u,\mathrm{dR}}_{m-\ast}(M) to symmetric and elliptic uniform pseudodifferential operators:

Theorem B (Theorem 3 and Remark 5).

Let MM be an oriented Riemannian manifold of bounded geometry and without boundary, and PP be a symmetric and elliptic uniform pseudodifferential operator of positive order.

Then ind(P)Hb,dR(M)\operatorname{ind}(P)\in H_{b,\mathrm{dR}}^{\ast}(M) is the Poincaré dual of (αch)([P])Hu,dR(M)(\alpha_{\ast}\circ\operatorname{ch}^{\ast})([P])\in H^{u,\mathrm{dR}}_{\ast}(M).

Using the above local index theorem we will derive as a corollary the following local index formula:

Corollary C (Corollary 7).

Let [φ]Hc,dRk(M)[\varphi]\in H_{c,\mathrm{dR}}^{k}(M) be a compactly supported cohomology class and define the analytic index ind[φ](P)\operatorname{ind}_{[\varphi]}(P) as Connes–Moscovici [CM90] for PP being a multigraded, symmetric, elliptic uniform pseudodifferential operator of positive order. Then we have

ind[φ](P)=Mind(P)[φ]\operatorname{ind}_{[\varphi]}(P)=\int_{M}\operatorname{ind}(P)\wedge[\varphi]

and this pairing is continuous, i.e., Mind(P)[φ]ind(P)[φ]1\int_{M}\operatorname{ind}(P)\wedge[\varphi]\leq\|\operatorname{ind}(P)\|_{\infty}\cdot\|[\varphi]\|_{1}, where \|-\|_{\infty} denotes the sup-seminorm on Hb,dRmk(M)H_{b,\mathrm{dR}}^{m-k}(M) and 1\|-\|_{1} the L1L^{1}-seminorm on Hc,dRk(M)H_{c,\mathrm{dR}}^{k}(M).

Note that the corollary reads basically the same as the local index formula of Connes and Moscovici [CM90]. The fundamentally new thing in it is the continuity statement for which we need the uniformity assumption for PP.

As a second corollary to the above local index theorem we will, as already written, derive the generalization of Roe’s index theorem for amenable manifolds.

Corollary D (Corollary 20).

Let MM be a manifold of bounded geometry and without boundary, let (Mi)i(M_{i})_{i} be a Følner sequence for MM and let τ()\tau\in(\ell^{\infty})^{\ast} be a linear functional associated to a free ultrafilter on \mathbb{N}. Denote the from the choice of Følner sequence and functional τ\tau resulting functional on K0(Cu(M))K_{0}(C_{u}^{\ast}(M)) by θ\theta.

Then for both p{0,1}p\in\{0,1\}, every class [P]Kpu(M)[P]\in K_{p}^{u}(M) with PP being a pp-graded, symmetric, elliptic uniform pseudodifferential operator over MM, and every uKup(M)u\in K_{u}^{p}(M) we have

u,[P]θ=ch(u)ind(P),[M](Mi)i,τ.\langle u,[P]\rangle_{\theta}=\langle\operatorname{ch}(u)\wedge\operatorname{ind}(P),[M]\rangle_{(M_{i})_{i},\tau}.

Roe’s theorem [Roe88a] is the special case where P=DP=D is a graded (i.e., p=0p=0) Dirac operator and u=[]u=[\mathbb{C}] is the class in Ku0(M)K_{u}^{0}(M) of the trivial, 11-dimensional vector bundle over MM.

To put the above index theorems into context, let us consider manifolds with cylindrical ends. These are the kind of non-compact manifolds which are studied to prove for example the Atiyah–Patodi–Singer index theorem. In the setting of this paper, the relevant algebra would be that of bounded functions with bounded derivatives, whereas in papers like [Mel95] or [MN08] one imposes conditions at infinity like rapid decay of the integral kernels (see the definition of the suspended algebra in [Mel95, Section 1]).

Note that this global index theorem arising from a Følner sequence is just a special case of a certain rough index theory, where one pairs classes from the so-called rough cohomology with classes in the KK-theory of the uniform Roe algebra, and Følner sequences give naturally classes in this rough cohomology. For details see the thesis [Mav95] of Mavra. It seems that it should be possible to combine the above local index theorem with this rough index theory, since it is possible in the special case of Følner sequences. The author investigated this in [Eng15b].

Let us say a few words about the proofs of the above index theorems for elliptic uniform pseudodifferential operators. Roe used in [Roe88a] the heat kernel method to prove his index theorem for amenable manifolds and therefore, since the heat kernel method does only work for Dirac operators, it can not encompass uniform pseudodifferential operators. So what we will basically do in this paper is to set up all the necessary theory in order to be able to reduce the index problem from pseudodifferential operators to Dirac operators.

The main ingredient is a version of Poincaré duality between uniform KK-homology and uniform KK-theory, which was proved by the author in [Eng15a, Section 4.4]. With this at our disposal we will then be able to reduce the index problem for elliptic uniform pseudodifferential operators to Dirac operators by proving a uniform version of the Thom isomorphism in order to conclude that symbol classes of elliptic uniform pseudodifferential operators may be represented by symbol classes of Dirac operators. So it remains to show the local index theorem for Dirac operators, but since up to this point we will already have set up all the needed machinery, this proof will be basically the same as the proof of the local index theorem of Connes and Moscovici in [CM90].

The last collection of results that we want to highlight in this introduction are all the various (duality) isomorphisms proved in this paper.

Theorem E (Theorems 14, 8 and 10).

Let MM be an mm-dimensional manifold of bounded geometry and no boundary. Then the Chern characters induce linear, continuous isomorphisms

Ku(M)¯Hb,dR(M) and Ku(M)¯Hu,dR(M),K^{\ast}_{u}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H_{b,\mathrm{dR}}^{\ast}(M)\text{ and }K^{u}_{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H^{u,\mathrm{dR}}_{\ast}(M),

and we also have the isomorphism

HPcont(W,1(M))Hu,dR(M).H\!P_{\mathrm{cont}}^{*}(W^{\infty,1}(M))\cong H^{u,\mathrm{dR}}_{*}(M).

If MM is oriented we further have the isomorphism

Hb,dR(M)Hmu,dR(M).H_{b,\mathrm{dR}}^{\ast}(M)\cong H^{u,\mathrm{dR}}_{m-\ast}(M).

If MM is spinc then we have the Poincaré duality isomorphism Ku(M)Km(M)K_{u}^{\ast}(M)\cong K^{\ast}_{m-\ast}(M), which is proved in [Eng15a, Theorem 4.29].

Acknowledgements

This article contains mostly Section 5 of the preprint [Eng15a] which is being split up for easier publication. It arose out of the Ph.D. thesis [Eng14] of the author written at the University of Augsburg.

2 Review of needed material

In this section we review the needed material from the literature. We start with the notion of bounded geometry for Riemannian manifolds, define Sobolev spaces and discuss the Sobolev embedding theorem, and at the end of Section 2.1 we prove the technical Lemma 14 about constructing covers with certain properties on manifolds of bounded geometry. In Section 2.2 we discuss the calculus of uniform pseudodifferential operators that we will use in this paper, and in Section 2.3 we recall the basic facts about uniform KK-homology and uniform KK-theory.

2.1 Manifolds of bounded geometry

We will recall in this section the notion of bounded geometry for manifolds and for vector bundles and discuss basic facts about uniform CrC^{r}-spaces and Sobolev spaces on them. Almost all material presented here is already known, and we tried to give proper credits wherever possible. As a genuine reference one might also use Eldering [Eld13, Chapter 2].

Definition 1.

We say that a Riemannian manifold MM has bounded geometry, if

  • the curvature tensor and all its derivatives are bounded, i.e.,

    supxMkRm(x)<\sup_{x\in M}\|\nabla^{k}\operatorname{Rm}(x)\|<\infty

    for all k0k\in\mathbb{N}_{0}, and

  • the injectivity radius is uniformly positive, i.e.,

    infxMinjradM(x)>0.\inf_{x\in M}\operatorname{inj-rad}_{M}(x)>0.

If EME\to M is a vector bundle with a metric and compatible connection, then EE has bounded geometry, if the curvature tensor of EE and all its derivatives are bounded.

Examples 2.

The most important examples of manifolds of bounded geometry are coverings of closed Riemannian manifolds equipped with the pull-back metric, homogeneous manifolds with an invariant metric, and leafs in a foliation of a compact Riemannian manifold (Greene [Gre78, lemma on page 91 and the paragraph thereafter]).

For vector bundles, the most important examples are of course again pull-back bundles of bundles over closed manifolds equipped with the pull-back metric and connection, and the tangent bundle of a manifold of bounded geometry. ∎

We now state an important characterization in local coordinates of bounded geometry since it allows one to show that certain local definitions are independent of the chosen normal coordinates.

Lemma 3 ([Shu92, Appendix A1.1]).

Let the injectivity radius of MM be positive.

Then the curvature tensor of MM and all its derivatives are bounded if and only if for any 0<r<injradM0<r<\operatorname{inj-rad}_{M} all the transition functions between overlapping normal coordinate charts of radius rr are uniformly bounded, as are all their derivatives (i.e., the bounds can be chosen to be the same for all transition functions).

Another fact which we will need about manifolds of bounded geometry is the existence of uniform covers by normal coordinate charts and corresponding partitions of unity. A proof may be found in, e.g., [Shu92, Appendix A1.1] (Shubin addresses the first statement about the existence of such covers actually to the paper [Gro81a] of Gromov).

Lemma 4.

Let MM be a manifold of bounded geometry.

For every 0<ε<injradM30<\varepsilon<\tfrac{\operatorname{inj-rad}_{M}}{3} exists a cover of MM by normal coordinate charts of radius ε\varepsilon with the properties that the midpoints of the charts form a uniformly discrete set and that the coordinate charts with double radius 2ε2\varepsilon form a uniformly locally finite cover of MM.

Furthermore, there is a subordinate partition of unity 1=iφi1=\sum_{i}\varphi_{i} with suppφiB2ε(xi)\operatorname{supp}\varphi_{i}\subset B_{2\varepsilon}(x_{i}), such that in normal coordinates the functions φi\varphi_{i} and all their derivatives are uniformly bounded (i.e., the bounds do not depend on ii).

If the manifold MM has bounded geometry, we have analogous equivalent local characterizations of bounded geometry for vector bundles as for manifolds. The equivalence of the first two bullet points in the next lemma is stated in, e.g., [Roe88a, Proposition 2.5]. Concerning the third bullet point, the author could not find any citable reference in the literature (though both Shubin [Shu92] and Eldering [Eld13] use this as the definition).

Lemma 5.

Let MM be a manifold of bounded geometry and EME\to M a vector bundle. Then the following are equivalent:

  • EE has bounded geometry,

  • the Christoffel symbols Γiαβ(y)\Gamma_{i\alpha}^{\beta}(y) of EE with respect to synchronous framings (considered as functions on the domain BB of normal coordinates at all points) are bounded, as are all their derivatives, and this bounds are independent of xMx\in M, yexpx(B)y\in\exp_{x}(B) and i,α,βi,\alpha,\beta, and

  • the matrix transition functions between overlapping synchronous framings are uniformly bounded, as are all their derivatives (i.e., the bounds are the same for all transition functions).

We will now give the definition of uniform CC^{\infty}-spaces together with a local characterization on manifolds of bounded geometry. The interested reader is refered to, e.g., the papers [Roe88a, Section 2] or [Shu92, Appendix A1.1] of Roe and Shubin for more information regarding these uniform CC^{\infty}-spaces.

Definition 6 (CrC^{r}-bounded functions).

Let fC(M)f\in C^{\infty}(M). We say that ff is a CbrC_{b}^{r}-function, or equivalently that it is CrC^{r}-bounded, if if<Ci\|\nabla^{i}f\|_{\infty}<C_{i} for all 0ir0\leq i\leq r.

If MM has bounded geometry, being CrC^{r}-bounded is equivalent to the statement that in every normal coordinate chart |αf(y)|<Cα|\partial^{\alpha}f(y)|<C_{\alpha} for every multiindex α\alpha with |α|r|\alpha|\leq r (where the constants CαC_{\alpha} are independent of the chart).

The definition of CrC^{r}-boundedness and its equivalent characterization in normal coordinate charts for manifolds of bounded geometry make also sense for sections of vector bundles of bounded geometry.

Definition 7 (Uniform CC^{\infty}-spaces).

Let EE be a vector bundle of bounded geometry over MM. We will denote the uniform CrC^{r}-space of all CrC^{r}-bounded sections of EE by Cbr(E)C_{b}^{r}(E).

Furthermore, we define the uniform CC^{\infty}-space Cb(E)C_{b}^{\infty}(E)

Cb(E):=rCbr(E)C_{b}^{\infty}(E):=\bigcap_{r}C_{b}^{r}(E)

which is a Fréchet space.

Now we get to Sobolev spaces on manifolds of bounded geometry. Much of the following material is from [Shu92, Appendix A1.1] and [Roe88a, Section 2], where an interested reader can find more thorough discussions of this matters.

Let sCc(E)s\in C^{\infty}_{c}(E) be a compactly supported, smooth section of some vector bundle EME\to M with metric and connection \nabla. For k0k\in\mathbb{N}_{0} and p[1,)p\in[1,\infty) we define the global Wk,pW^{k,p}-Sobolev norm of ss by

sWk,pp:=i=0kMis(x)p𝑑x.\|s\|_{W^{k,p}}^{p}:=\sum_{i=0}^{k}\int_{M}\|\nabla^{i}s(x)\|^{p}dx. (2.1)
Definition 8 (Sobolev spaces Wk,p(E)W^{k,p}(E)).

Let EE be a vector bundle which is equipped with a metric and a connection. The Wk,pW^{k,p}-Sobolev space of EE is the completion of Cc(E)C^{\infty}_{c}(E) in the norm Wk,p\|-\|_{W^{k,p}} and will be denoted by Wk,p(E)W^{k,p}(E).

If EE and MmM^{m} both have bounded geometry than the Sobolev norm (2.1) for 1<p<1<p<\infty is equivalent to the local one given by

sWk,pp=equivi=1φisWk,p(B2ε(xi))p,\|s\|_{W^{k,p}}^{p}\stackrel{{\scriptstyle\text{equiv}}}{{=}}\sum_{i=1}^{\infty}\|\varphi_{i}s\|^{p}_{W^{k,p}(B_{2\varepsilon}(x_{i}))}, (2.2)

where the balls B2ε(xi)B_{2\varepsilon}(x_{i}) and the subordinate partition of unity φi\varphi_{i} are as in Lemma 4, we have chosen synchronous framings and Wk,p(B2ε(xi))\|-\|_{W^{k,p}(B_{2\varepsilon}(x_{i}))} denotes the usual Sobolev norm on B2ε(xi)mB_{2\varepsilon}(x_{i})\subset\mathbb{R}^{m}. This equivalence enables us to define the Sobolev norms for all kk\in\mathbb{R}, see Triebel [Tri10] and Große–Schneider [GS13]. There are some issues in the case p=1p=1, see the discussion by Triebel [Tri83, Section 2.2.3], [Tri10, Remark 4 on Page 13].

Assuming bounded geometry, the usual embedding theorems are true:

Theorem 9 ([Aub98, Theorem 2.21]).

Let EE be a vector bundle of bounded geometry over a manifold MmM^{m} of bounded geometry and without boundary.

Then we have for all values (kr)/m>1/p(k-r)/m>1/p continuous embeddings

Wk,p(E)Cbr(E).W^{k,p}(E)\subset C^{r}_{b}(E).

We define the space

W,p(E):=k0Wk,p(E)W^{\infty,p}(E):=\bigcap_{k\in\mathbb{N}_{0}}W^{k,p}(E) (2.3)

and equip it with the obvious Fréchet topology. The Sobolev Embedding Theorem tells us now that we have for all pp a continuous embedding

W,p(E)Cb(E).W^{\infty,p}(E)\hookrightarrow C^{\infty}_{b}(E).

Finally, we come to a technical statement (Lemma 14) about the existence of open covers with special properties on manifolds of bounded geometry, similar to Lemma 4. As a preparation we first have to recall some facts about simplicial complexes of bounded geometry and corresponding triangulations of manifolds of bounded geometry.

Definition 10 (Bounded geometry simplicial complexes).

A simplicial complex has bounded geometry if there is a uniform bound on the number of simplices in the link of each vertex.

A subdivision of a simplicial complex of bounded geometry with the properties that

  • each simplex is subdivided a uniformly bounded number of times on its nn-skeleton, where the nn-skeleton is the union of the nn-dimensional sub-simplices of the simplex, and that

  • the distortion length(e)+length(e)1\operatorname{length}(e)+\operatorname{length}(e)^{-1} of each edge ee of the subdivided complex is uniformly bounded in the metric given by barycentric coordinates of the original complex,

is called a uniform subdivision.

Theorem 11 (Attie [Att94, Theorem 1.14]).

Let MM be a manifold of bounded geometry and without boundary.

Then MM has a triangulation as a simplicial complex of bounded geometry such that the metric given by barycentric coordinates is bi-Lipschitz equivalent222Two metric spaces XX and YY are said to be bi-Lipschitz equivalent if there is a homeomorphism f:XYf\colon X\to Y with 1CdX(x,x)dY(f(x),f(x))CdX(x,x)\tfrac{1}{C}d_{X}(x,x^{\prime})\leq d_{Y}(f(x),f(x^{\prime}))\leq Cd_{X}(x,x^{\prime}) for all x,xXx,x^{\prime}\in X and some constant C>0C>0. to the one on MM induced by the Riemannian structure. This triangulation is unique up to uniform subdivision.

Conversely, if MM is a simplicial complex of bounded geometry which is a triangulation of a smooth manifold, then this smooth manifold admits a metric of bounded geometry with respect to which it is bi-Lipschitz equivalent to MM.

Remark 12.

Attie uses in [Att94] a weaker notion of bounded geometry as we do: additionally to a uniformly positive injectivity radius he only requires the sectional curvatures to be bounded in absolute value (i.e., the curvature tensor is bounded in norm), but he assumes nothing about the derivatives (see [Att94, Definition 1.4]). But going into his proof of [Att94, Theorem 1.14], we see that the Riemannian metric constructed for the second statement of the theorem is actually of bounded geometry in our strong sense (i.e., also with bounds on the derivatives of the curvature tensor).

As a corollary we get that for any manifold of bounded geometry in Attie’s weak sense there is another Riemannian metric of bounded geometry in our strong sense that is bi-Lipschitz equivalent the original one (in fact, this bi-Lipschitz equivalence is just the identity map of the manifold, as can be seen from the proof).

The last auxiliary lemma (before we come to the crucial Lemma 14) is about coloring covers of manifolds with only finitely many colors:

Lemma 13.

Let a covering {Uα}\{U_{\alpha}\} of MM with finite multiplicity be given. Then there exists a coloring of the subsets UαU_{\alpha} with finitely many colors such that no two intersecting subsets have the same color.

Proof 2.1.

Construct a graph whose vertices are the subsets UαU_{\alpha} and two vertices are connected by an edge if the corresponding subsets intersect. We have to find a coloring of this graph with only finitely many colors where connected vertices do have different colors.

To do this, we firstly use the theorem of de Bruijin–Erdös stating that an infinite graph may be colored by kk colors if and only if every of its finite subgraphs may be colored by kk colors (one can use the Lemma of Zorn to prove this).

Secondly, since the covering has finite multiplicity it follows that the number of edges attached to each vertex in our graph is uniformly bounded from above, i.e., the maximum vertex degree of our graph is finite. But this also holds for every subgraph of our graph, with the maximum vertex degree possibly only decreasing by passing to a subgraph. Now a simple greedy algorithm shows that every finite graph may be colored with one more color than its maximum vertex degree: just start by coloring a vertex with some color, go to the next vertex and use an admissible color for it, and so on.

Lemma 14.

Let MM be a manifold of bounded geometry and without boundary.

Then there is an ε>0\varepsilon>0 and a countable collection of uniformly discretely distributed points {xi}iIM\{x_{i}\}_{i\in I}\subset M such that {Bε(xi)}iI\{B_{\varepsilon}(x_{i})\}_{i\in I} is a uniformly locally finite cover of MM. We can additionally arrange such that it has the following two properties:

  1. 1.

    It is possible to partition II into a finite amount of subsets I1,,INI_{1},\ldots,I_{N} such that for each 1jN1\leq j\leq N the subset Uj:=iIjBε(xi)U_{j}:=\bigcup_{i\in I_{j}}B_{\varepsilon}(x_{i}) is a disjoint union of balls that are a uniform distance apart from each other, and such that for each 1KN1\leq K\leq N the connected components of UK:=U1UkU_{K}:=U_{1}\cup\ldots\cup U_{k} are also a uniform distance apart from each other (see Figure 1).

  2. 2.

    Instead of choosing balls Bε(xi)B_{\varepsilon}(x_{i}) to get our cover of MM it is possible to choose other open subsets such that additionally to the property from Point 1 for any distinct 1m,nN1\leq m,n\leq N the symmetric difference UmΔUnU_{m}\Delta U_{n} consists of open subsets of MM which are a uniform distance apart from each other.333To see a non-example, in the lower part of Figure 1 this is actually not the case.

Refer to caption
Figure 1: Illustration for Lemma 14.1.
Proof 2.2.

Let us first show how to get a cover of MM satisfying Point 1 from the lemma.

We triangulate MM via the above Theorem 11. Then we may take the vertices of this triangulation as our collection of points {xi}iI\{x_{i}\}_{i\in I} and set ε\varepsilon to 2/32/3 of the length of an edge multiplied with the constant CC which we get since the metric derived from barycentric coordinates is bi-Lipschitz equivalent to the metric derived from the Riemannian structure.

Two balls Bε(xi)B_{\varepsilon}(x_{i}) and Bε(xj)B_{\varepsilon}(x_{j}) for xixjx_{i}\not=x_{j} intersect if and only if xix_{i} and xjx_{j} are adjacent vertices, and in the case that they are not adjacent, these balls are a uniform distance apart from each other. Hence it is possible to find a coloring of all these balls {Bε(xi)}iI\{B_{\varepsilon}(x_{i})\}_{i\in I} with only finitely many colors having the claimed Property 1: apply Lemma 13 to the covering {Bε(xi)}iI\{B_{\varepsilon}(x_{i})\}_{i\in I} which has finite multiplicity due to bounded geometry.

To prove Point 2, we replace in our cover of MM the balls Bε(xi)B_{\varepsilon}(x_{i}) with slightly differently chosen open subsets, as shown in the 22-dimensional case in Figure 2 (we are working in a triangulation of MM as above in the proof of Point 1).

Refer to caption
Figure 2: Illustration for Lemma 14.2.

2.2 Uniform pseudodifferential operators

In this section we will recall the definition of uniform pseudodifferential operators and some basic properties of them. This class of pseudodifferential operators was introduced by the author in his Ph.D. thesis [Eng14], but similar classes were also considered by Shubin [Shu92] and Kordyukov [Kor91].

Let MmM^{m} be an mm-dimensional manifold of bounded geometry and let EE and FF be two vector bundles of bounded geometry over MM.

Definition 15.

An operator P:Cc(E)C(F)P\colon C_{c}^{\infty}(E)\to C^{\infty}(F) is a uniform pseudodifferential operator of order kk\in\mathbb{Z}, if with respect to a uniformly locally finite covering {B2ε(xi)}\{B_{2\varepsilon}(x_{i})\} of MM with normal coordinate balls and corresponding subordinate partition of unity {φi}\{\varphi_{i}\} as in Lemma 4 we can write

P=P+iPiP=P_{-\infty}+\sum_{i}P_{i} (2.4)

satisfying the following conditions:

  • PP_{-\infty} is a quasilocal smoothing operator,444That is to say, for all k,l0k,l\in\mathbb{N}_{0} we have that P:Hk(E)Hl(F)P_{-\infty}\colon H^{-k}(E)\to H^{l}(F) has the following propety: there is a function μ:>00\mu\colon\mathbb{R}_{>0}\to\mathbb{R}_{\geq 0} with μ(R)0\mu(R)\to 0 for RR\to\infty and such that for all LML\subset M and all uHk(E)u\in H^{-k}(E) with suppuL\operatorname{supp}u\subset L we have AuHl,MBR(L)μ(R)uHk\|Au\|_{H^{l},M-B_{R}(L)}\leq\mu(R)\cdot\|u\|_{H^{-k}}.

  • for all ii the operator PiP_{i} is with respect to synchronous framings of EE and FF in the ball B2ε(xi)B_{2\varepsilon}(x_{i}) a matrix of pseudodifferential operators on m\mathbb{R}^{m} of order kk with support555An operator PP is supported in a subset KK, if suppPuK\operatorname{supp}Pu\subset K for all uu in the domain of PP and if Pu=0Pu=0 whenever we have suppuK=\operatorname{supp}u\cap K=\emptyset. in B2ε(0)mB_{2\varepsilon}(0)\subset\mathbb{R}^{m}, and

  • the constants CiαβC_{i}^{\alpha\beta} appearing in the bounds

    DxαDξβpi(x,ξ)Ciαβ(1+|ξ|)k|β|\|D_{x}^{\alpha}D_{\xi}^{\beta}p_{i}(x,\xi)\|\leq C^{\alpha\beta}_{i}(1+|\xi|)^{k-|\beta|}

    of the symbols of the operators PiP_{i} can be chosen to not depend on ii, i.e., there are Cαβ<C^{\alpha\beta}<\infty such that

    CiαβCαβC^{\alpha\beta}_{i}\leq C^{\alpha\beta} (2.5)

    for all multi-indices α,β\alpha,\beta and all ii.

To define ellipticity we have to recall the definition of symbols. We let πE\pi^{\ast}E and πF\pi^{\ast}F denote the pull-back bundles of EE and FF to the cotangent bundle π:TMM\pi\colon T^{\ast}M\to M of the mm-dimensional manifold MM.

Definition 16.

Let pp be a section of the bundle Hom(πE,πF)\operatorname{Hom}(\pi^{\ast}E,\pi^{\ast}F) over TMT^{\ast}M.

  • We call pp a symbol of order kk\in\mathbb{Z}, if the following holds: choosing a uniformly locally finite covering {B2ε(xi)}\{B_{2\varepsilon}(x_{i})\} of MM through normal coordinate balls and corresponding subordinate partition of unity {φi}\{\varphi_{i}\} as in Lemma 4, and choosing synchronous framings of EE and FF in these balls B2ε(xi)B_{2\varepsilon}(x_{i}), we can write pp as a uniformly locally finite sum p=ipip=\sum_{i}p_{i}, where pi(x,ξ):=p(x,ξ)φ(x)p_{i}(x,\xi):=p(x,\xi)\varphi(x) for xMx\in M and ξTxM\xi\in T^{\ast}_{x}M, and interpret each pip_{i} as a matrix-valued function on B2ε(xi)×mB_{2\varepsilon}(x_{i})\times\mathbb{C}^{m}. Then for all multi-indices α\alpha and β\beta there must exist a constant Cαβ<C^{\alpha\beta}<\infty such that for all ii and all x,ξx,\xi we have

    DxαDξβpi(x,ξ)Cαβ(1+|ξ|)k|β|.\|D^{\alpha}_{x}D^{\beta}_{\xi}p_{i}(x,\xi)\|\leq C^{\alpha\beta}(1+|\xi|)^{k-|\beta|}. (2.6)
  • We will call pp elliptic, if there is an R>0R>0 such that p||ξ|>Rp|_{|\xi|>R}666We restrict pp to the bundle Hom(πE,πF)\operatorname{Hom}(\pi^{\ast}E,\pi^{\ast}F) over the space {(x,ξ)TM||ξ|>R}TM\{(x,\xi)\in T^{\ast}M\ |\ |\xi|>R\}\subset T^{\ast}M. is invertible and this inverse p1p^{-1} satisfies the Inequality (2.6) for α,β=0\alpha,\beta=0 and order k-k (and of course only for |ξ|>R|\xi|>R since only there the inverse is defined). Note that as in the compact case it follows that p1p^{-1} satisfies the Inequality (2.6) for all multi-indices α\alpha, β\beta.

Definition 17.

Let PP be a uniform pseudodifferential operator. We will call PP elliptic, if its principal symbol σ(P)\sigma(P) is elliptic.

The main fact about elliptic operators that we will need later is the following one. Of course ellipticity is also crucially used to show that we can define a uniform KK-homology class for such operators (see Example 2.3).

Corollary 18 ([Eng15a, Corollary 2.47]).

Let PP be a symmetric and elliptic uniform pseudodifferential operator of positive order.

If ff is a Schwartz function, then f(P)f(P) is a quasi-local smoothing operator.

2.3 Uniform KK-homology and uniform KK-theory

Let us start with uniform KK-homology. For this we first have to recall briefly the notion of multigraded Hilbert spaces. They arise as L2L^{2}-spaces of vector bundles on which Clifford algebras act.

  • A graded Hilbert space is a Hilbert space HH with a decomposition H=H+HH=H^{+}\oplus H^{-} into closed, orthogonal subspaces. This is equivalent to the existence of a grading operator ϵ\epsilon (a selfadjoint unitary) such that its ±1\pm 1-eigenspaces are H±H^{\pm}.

  • If HH is a graded space, then its opposite is the graded space HopH^{\mathrm{op}} with underlying vector space HH but with the reversed grading, i.e., (Hop)+=H(H^{\mathrm{op}})^{+}=H^{-} and (Hop)=H+(H^{\mathrm{op}})^{-}=H^{+}. This is equivalent to ϵHop=ϵH\epsilon_{H^{\mathrm{op}}}=-\epsilon_{H}.

  • An operator on a graded space HH is called even if it maps H±H^{\pm} again to H±H^{\pm}, and it is called odd if it maps H±H^{\pm} to HH^{\mp}. Equivalently, an operator is even if it commutes with the grading operator ϵ\epsilon of HH, and it is odd if it anti-commutes with it.

Definition 19.

Let p0p\in\mathbb{N}_{0}.

  • A pp-multigraded Hilbert space is a graded Hilbert space equipped with pp odd unitary operators ϵ1,,ϵp\epsilon_{1},\ldots,\epsilon_{p} such that ϵiϵj+ϵjϵi=0\epsilon_{i}\epsilon_{j}+\epsilon_{j}\epsilon_{i}=0 for iji\not=j, and ϵj2=1\epsilon_{j}^{2}=-1 for all jj.

  • Note that a 0-multigraded Hilbert space is just a graded Hilbert space, and by convention a (1)(-1)-multigraded Hilbert space is an ungraded one.

  • Let HH be a pp-multigraded Hilbert space. Then an operator on HH will be called multigraded, if it commutes with the multigrading operators ϵ1,,ϵp\epsilon_{1},\ldots,\epsilon_{p} of HH.

To define uniform Fredholm modules we will need the following notions. Let us define

L-LipR(X):={fCc(X)|f is L-Lipschitz,diam(suppf)R and f1}.L\text{-}\operatorname{Lip}_{R}(X):=\{f\in C_{c}(X)\ |\ f\text{ is }L\text{-Lipschitz},\operatorname{diam}(\operatorname{supp}f)\leq R\text{ and }\|f\|_{\infty}\leq 1\}.
Definition 20 ([Špa09, Definition 2.3]).

Let T𝔅(H)T\in\mathfrak{B}(H) be an operator on a Hilbert space HH and ρ:C0(X)𝔅(H)\rho\colon C_{0}(X)\to\mathfrak{B}(H) a representation.

We say that TT is uniformly locally compact, if for every R,L>0R,L>0 the collection

{ρ(f)T,Tρ(f)|fL-LipR(X)}\{\rho(f)T,T\rho(f)\ |\ f\in L\text{-}\operatorname{Lip}_{R}(X)\}

is uniformly approximable.777A collection of operators 𝒜𝔎(H)\mathcal{A}\subset\mathfrak{K}(H) is said to be uniformly approximable, if for every ε>0\varepsilon>0 there is an N>0N>0 such that for every T𝒜T\in\mathcal{A} there is a rank-NN operator kk with Tk<ε\|T-k\|<\varepsilon.

We say that TT is uniformly pseudolocal, if for every R,L>0R,L>0 the collection

{[T,ρ(f)]|fL-LipR(X)}\{[T,\rho(f)]\ |\ f\in L\text{-}\operatorname{Lip}_{R}(X)\}

is uniformly approximable.

Definition 21 (Multigraded uniform Fredholm modules, cf. [Špa09, Definition 2.6]).

Let p1p\in\mathbb{Z}_{\geq-1}. A triple (H,ρ,T)(H,\rho,T) consisting of

  • a separable pp-multigraded Hilbert space HH,

  • a representation ρ:C0(X)𝔅(H)\rho\colon C_{0}(X)\to\mathfrak{B}(H) by even, multigraded operators, and

  • an odd multigraded operator T𝔅(H)T\in\mathfrak{B}(H) such that

    • the operators T21T^{2}-1 and TTT-T^{\ast} are uniformly locally compact and

    • the operator TT itself is uniformly pseudolocal

is called a pp-multigraded uniform Fredholm module over XX.

Definition 22 (Uniform KK-homology, [Špa09, Definition 2.13]).

We define the uniform KK-homology group Kpu(X)K_{p}^{u}(X) of any locally compact, separable metric space XX to be the abelian group generated by unitary equivalence classes of pp-multigraded uniform Fredholm modules with the relations:

  • if xx and yy are operator homotopic888A collection (H,ρ,Tt)(H,\rho,T_{t}) of uniform Fredholm modules is called an operator homotopy if tTt𝔅(H)t\mapsto T_{t}\in\mathfrak{B}(H) is norm continuous., then [x]=[y][x]=[y], and

  • [x]+[y]=[xy][x]+[y]=[x\oplus y],

where xx and yy are pp-multigraded uniform Fredholm modules.

Example 2.3.

Špakula [Špa09, Theorem 3.1] showed that the usual Fredholm module arising from a generalized Dirac operator is uniform if we assume bounded geometry: if DD is a generalized Dirac operator acting on a Dirac bundle SS of bounded geometry over a manifold MM of bounded geometry, then the triple (L2(S),ρ,χ(D))(L^{2}(S),\rho,\chi(D)), where ρ\rho is the representation of C0(M)C_{0}(M) on L2(S)L^{2}(S) by multiplication operators and χ\chi is a normalizing function, is a uniform Fredholm module. It is multigraded if the Dirac bundle SS has an action of a Clifford algebra.

The author [Eng15a, Theorem 3.39 and Proposition 3.40] generalized this to symmetric and elliptic uniform pseudodifferential operators over manifolds of bounded geometry, and also showed that this uniform KK-homology class only depends on the principal symbol of the operator.

Let us now recall uniform KK-theory, which was introduced by the author in his Ph.D. thesis [Eng14].

Definition 23 (Uniform KK-theory).

Let XX be a metric space. The uniform KK-theory groups of XX are defined as

Kup(X):=Kp(Cu(X)),K^{p}_{u}(X):=K_{-p}(C_{u}(X)),

where Cu(X)C_{u}(X) is the CC^{\ast}-algebra of bounded, uniformly continuous functions on XX.

On manifolds of bounded geometry we have an interpretation of uniform KK-theory via isomorphism classes of vector bundles of bounded geometry. In order to state this properly, we first have to recall the needed notion of isomorphy.

Let MM be a manifold of bounded geometry and EE and FF two complex vector bundles equipped with Hermitian metrics and compatible connections.

Definition 24 (CC^{\infty}-boundedness / CbC_{b}^{\infty}-isomorphy of vector bundle homomorphisms).

We will call a vector bundle homomorphism φ:EF\varphi\colon E\to F CC^{\infty}-bounded, if with respect to synchronous framings of EE and FF the matrix entries of φ\varphi are bounded, as are all their derivatives, and these bounds do not depend on the chosen base points for the framings or the synchronous framings themself.

EE and FF will be called CbC_{b}^{\infty}-isomorphic, if there is an isomorphism φ:EF\varphi\colon E\to F such that both φ\varphi and φ1\varphi^{-1} are CC^{\infty}-bounded.

An important property of vector bundles over compact spaces is that they are always complemented, i.e., for every bundle EE there is a bundle FF such that EFE\oplus F is isomorphic to the trivial bundle. Note that this fails in general for non-compact spaces. The following proposition shows that we have the analogous property for vector bundles of bounded geometry. We state it here since we will need the proposition later in this paper.

Definition 25 (CbC_{b}^{\infty}-complemented vector bundles).

A vector bundle EE will be called CbC_{b}^{\infty}-complemented, if there is some vector bundle EE^{\perp} such that EEE\oplus E^{\perp} is CbC_{b}^{\infty}-isomorphic to a trivial bundle with the flat connection.

Proposition 26 ([Eng15a, Proposition 4.13]).

Let MM be a manifold of bounded geometry and let EME\to M be a vector bundle of bounded geometry.

Then EE is CbC_{b}^{\infty}-complemented.

We can now state the interpretation of uniform KK-theory on manifolds of bounded geometry via vector bundles.

Theorem 27 (Interpretation of Ku0(M)K^{0}_{u}(M), [Eng15a, Theorem 4.18]).

Let MM be a Riemannian manifold of bounded geometry and without boundary.

Then every element of Ku0(M)K^{0}_{u}(M) is of the form [E][F][E]-[F], where both [E][E] and [F][F] are CbC_{b}^{\infty}-isomorphism classes of complex vector bundles of bounded geometry over MM.

Moreover, every complex vector bundle of bounded geometry over MM defines naturally a class in Ku0(M)K^{0}_{u}(M).

Note that the last statement in the above theorem is not trivial since it relies on the fact that every vector bundle of bounded geometry is suitably complemented.

Theorem 28 (Interpretation of Ku1(M)K^{1}_{u}(M), [Eng15a, Theorem 4.21]).

Let MM be a Riemannian manifold of bounded geometry and without boundary.

Then every elements of Ku1(M)K^{1}_{u}(M) is of the form [E][F][E]-[F], where both [E][E] and [F][F] are CbC_{b}^{\infty}-isomorphism classes of complex vector bundles of bounded geometry over S1×MS^{1}\times M with the following property: there is some neighbourhood US1U\subset S^{1} of 11 such that [E|U×M][E|_{U\times M}] and [F|U×M][F|_{U\times M}] are CbC_{b}^{\infty}-isomorphic to a trivial vector bundle with the flat connection (the dimension of the trivial bundle is the same for both [E|U×M][E|_{U\times M}] and [F|U×M][F|_{U\times M}]).

Moreover, every pair of complex vector bundles EE and FF of bounded geometry and with the above properties define a class [E][F][E]-[F] in Ku1(M)K_{u}^{1}(M).

We have a cap product999We need some assumptions on the space XX to construct the cap product. But because every space occuring in this paper will satisfy them, we have refrained from stating these assumptions explicitly.

:Kup(X)Kqu(X)Kqpu(X).\cap\colon K_{u}^{p}(X)\otimes K_{q}^{u}(X)\to K_{q-p}^{u}(X).

Let us collect in the next proposition some properties of it.

Proposition 29 ([Eng15a, Proposition 4.28]).

  • We have the formula

    (PQ)T=P(QT)(P\otimes Q)\cap T=P\cap(Q\cap T) (2.7)

    for all elements P,QKu(X)P,Q\in K_{u}^{\ast}(X) and TKu(X)T\in K_{\ast}^{u}(X), where \otimes is the internal product101010If the classes are represented by vector bundles, then the internal product is just given by the tensor product bundle. on uniform KK-theory.

  • We have the following compatibility with the external products:

    (P×Q)(S×T)=(1)qs(PS)×(QT),(P\times Q)\cap(S\times T)=(-1)^{qs}(P\cap S)\times(Q\cap T), (2.8)

    where PKup(X)P\in K_{u}^{p}(X), QKuq(X)Q\in K_{u}^{q}(X) and SKsu(X)S\in K^{u}_{s}(X), TKtu(X)T\in K^{u}_{t}(X).

  • If EME\to M is a vector bundle of bounded geometry over a manifold MM of bounded geometry and DD an operator of Dirac type over MM, then we have

    [E][D]=[DE]Ku(M),[E]\cap[D]=[D_{E}]\in K_{\ast}^{u}(M), (2.9)

    where DED_{E} is the twisted operator.

The main reason why we have recalled the cap product is the following duality result:

Theorem 30 (Uniform KK-Poincaré duality, [Eng15a, Theorem 4.29]).

Let MM be an mm-dimensional spinc manifold of bounded geometry and without boundary.

Then the cap product [M]:Ku(M)Kmu(M)-\cap[M]\colon K_{u}^{\ast}(M)\to K^{u}_{m-\ast}(M) with its uniform KK-fundamental class [M]Kmu(M)[M]\in K_{m}^{u}(M) is an isomorphism.

3 Uniform homology theories and Chern characters

In Section 3.1 we will recall the definition of (periodic) cyclic cohomology and construct the Chern–Connes characters ch:Ku(M)HPcont(W,1(M))\operatorname{ch}\colon K_{\ast}^{u}(M)\dashrightarrow H\!P_{\mathrm{cont}}^{\ast}(W^{\infty,1}(M)). In Section 3.2 we will then map further into uniform de Rham homology Hu,dR(M)H^{u,\mathrm{dR}}_{\ast}(M) and prove various additional results, e.g., that we have an isomorphism HPcont(W,1(M))Hu,dR(M)H\!P_{\mathrm{cont}}^{\ast}(W^{\infty,1}(M))\cong H^{u,\mathrm{dR}}_{\ast}(M) and Poincaré duality Hb,dR(M)Hmu,dR(M)H_{b,\mathrm{dR}}^{\ast}(M)\cong H^{u,\mathrm{dR}}_{m-\ast}(M). At the end of Section 3.2 we discuss the Chern character ch:Ku(M)Hu,dR(M)\operatorname{ch}\colon K^{\ast}_{u}(M)\to H_{u,\mathrm{dR}}^{\ast}(M) and the whole Section 3.3 is devoted to the proof of the Chern character isomorphism theorem.

3.1 Cyclic cocycles of uniformly finitely summable modules

The goal of this section is to construct the homological Chern character maps from uniform KK-homology Ku(M)K_{\ast}^{u}(M) of MM to continuous periodic cyclic cohomology HPcont(W,1(M))H\!P_{\mathrm{cont}}^{\ast}(W^{\infty,1}(M)) of the Sobolev space W,1(M)W^{\infty,1}(M).

First we will recall the definition of Hochschild, cyclic and periodic cyclic cohomology of a (possibly non-unital) complete locally convex algebra AA111111We consider here only algebras over the field \mathbb{C}. Furthermore, we assume that multiplication in AA is jointly continuous.. The classical reference for this is, of course, Connes’ seminal paper [Con85]. The author also found Khalkhali’s book [Kha13] a useful introduction to these matters.

Definition 1.

The continuous Hochschild cohomology HHcont(A)H\!H_{\mathrm{cont}}^{\ast}(A) of AA is the homology of the complex

Ccont0(A)bCcont1(A)b,C_{\mathrm{cont}}^{0}(A)\stackrel{{\scriptstyle b}}{{\longrightarrow}}C_{\mathrm{cont}}^{1}(A)\stackrel{{\scriptstyle b}}{{\longrightarrow}}\ldots,

where Ccontn(A)=Hom(A^(n+1),)C_{\mathrm{cont}}^{n}(A)=\operatorname{Hom}(A^{\widehat{\otimes}(n+1)},\mathbb{C}) and the boundary map bb is given by

(bφ)(a0,,an+1)=\displaystyle(b\varphi)(a_{0},\ldots,a_{n+1})= i=0n(1)iφ(a0,,aiai+1,,an+1)+\displaystyle\sum_{i=0}^{n}(-1)^{i}\varphi(a_{0},\ldots,a_{i}a_{i+1},\ldots,a_{n+1})+
+(1)n+1φ(an+1a0,a1,,an).\displaystyle+(-1)^{n+1}\varphi(a_{n+1}a_{0},a_{1},\ldots,a_{n}).

We use the completed projective tensor product ^\widehat{\otimes} and the linear functionals are assumed to be continuous. But we still factor out only the image of the boundary operator to define the homology, and not the closure of the image of bb.

Definition 2.

The continuous cyclic cohomology HCcont(A)H\!C_{\mathrm{cont}}^{\ast}(A) of AA is the homology of the following subcomplex of the Hochschild cochain complex:

Cλ,cont0(A)bCλ,cont1(A)b,C_{\lambda,\mathrm{cont}}^{0}(A)\stackrel{{\scriptstyle b}}{{\longrightarrow}}C_{\lambda,\mathrm{cont}}^{1}(A)\stackrel{{\scriptstyle b}}{{\longrightarrow}}\ldots,

where Cλ,contn(A)={φCcontn(A):φ(an,a0,,an1)=(1)nφ(a0,a1,,an)}C_{\lambda,\mathrm{cont}}^{n}(A)=\{\varphi\in C_{\mathrm{cont}}^{n}(A)\colon\varphi(a_{n},a_{0},\ldots,a_{n-1})=(-1)^{n}\varphi(a_{0},a_{1},\ldots,a_{n})\}.

There is a certain periodicity operator S:HCcontn(A)HCcontn+2(A)S\colon H\!C_{\mathrm{cont}}^{n}(A)\to H\!C_{\mathrm{cont}}^{n+2}(A). For the tedious definition of this operator on the level of cyclic cochains we refer the reader to Connes’ original paper [Con85, Lemma 11 on p. 322] or to his book [Con94, Lemma 14 on p. 198].

Definition 3.

The continuous periodic cyclic cohomology HPcont(A)H\!P_{\mathrm{cont}}^{\ast}(A) of AA is defined as the direct limit

HPcont(A)=limHCcont+2n(A)H\!P_{\mathrm{cont}}^{\ast}(A)=\underrightarrow{\lim}\ H\!C_{\mathrm{cont}}^{\ast+2n}(A)

with respect to the maps SS.

Let (H,ρ,T)(H,\rho,T) be a graded uniform Fredholm module over MM and denote by ϵ\epsilon the grading automorphism of the graded Hilbert space HH. Moreover, assume that (H,ρ,T)(H,\rho,T) is involutive121212Recall that a Fredholm module (H,ρ,T)(H,\rho,T) is called involutive if T=TT=T^{*}, T1\|T\|\leq 1 and T2=1T^{2}=1. and uniformly pp-summable, where the latter means supfL-LipR(M)[T,ρ(f)]p<\sup_{f\in L\text{-}\operatorname{Lip}_{R}(M)}\|[T,\rho(f)]\|_{p}<\infty for the Schatten pp-norm p\|-\|_{p}.

Having such an involutive, uniformly pp-summable Fredholm module at hand we define for all mm with 2m+1p2m+1\geq p a cyclic 2m2m-cocycle on W,1(M)W^{\infty,1}(M), i.e., on the Sobolev space of infinite order and L1L^{1}-integrability, by

ch0,2m(H,ρ,T)(f0,,f2m):=12(2πi)mm!tr(ϵT[T,f0][T,f2m]).\operatorname{ch}^{0,2m}(H,\rho,T)(f_{0},\ldots,f_{2m}):=\tfrac{1}{2}(2\pi i)^{m}m!\operatorname{tr}\big{(}\epsilon T[T,f_{0}]\cdots[T,f_{2m}]\big{)}.

We have the compatibility Sch0,2m=ch0,2m+2S\circ\operatorname{ch}^{0,2m}=\operatorname{ch}^{0,2m+2} and therefore we get a map

ch0:K0u(M)HPcont0(W,1(M)).\operatorname{ch}^{0}\colon K^{u}_{0}(M)\dashrightarrow H\!P_{\mathrm{cont}}^{0}(W^{\infty,1}(M)).

The dashed arrow indicates that we do not know that every uniform, even KK-homology class is represented by a uniformly finitely summable module, and we also do not know if the map is well-defined, i.e., if two such modules representing the same KK-homology class will be mapped to the same cyclic cocycle class. For spinc manifolds the first mentioned problem is solved by Poincaré duality which states that every uniform KK-homology class may be represented by the difference of two twisted Dirac operators (which are uniformly finitely summable). But the second mentioned problem about the well-definedness is much more serious and will only be solved by the local index theorem. We will state the resolution of this problem in Corollary 4.

Given an ungraded, involutive, uniformly pp-summable Fredholm module (H,ρ,T)(H,\rho,T), we define for all mm with 2mp2m\geq p a cyclic (2m1)(2m-1)-cocycle on W,1(M)W^{\infty,1}(M) by

ch1,2m1(H,ρ,T\displaystyle\operatorname{ch}^{1,2m-1}(H,\rho,T )(f0,,f2m1)=\displaystyle)(f_{0},\ldots,f_{2m-1})=
=(2πi)m12(2m1)(2m3)31tr(T[T,f0][T,f2m1]).\displaystyle=(2\pi i)^{m}\tfrac{1}{2}(2m-1)(2m-3)\cdots 3\cdot 1\operatorname{tr}\big{(}T[T,f_{0}]\cdots[T,f_{2m-1}]\big{)}.

Again, this definition is compatible with the periodicity operator SS and so defines a map

ch1:K1u(M)HPcont1(W,1(M)).\operatorname{ch}^{1}\colon K^{u}_{1}(M)\dashrightarrow H\!P_{\mathrm{cont}}^{1}(W^{\infty,1}(M)).

3.2 Uniform de Rham (co-)homology

In the previous section we constructed the characters ch:Ku(M)HPcont(W,1(M))\operatorname{ch}\colon K_{\ast}^{u}(M)\dashrightarrow H\!P_{\mathrm{cont}}^{\ast}(W^{\infty,1}(M)). The first goal of this section is to map further to uniform de Rham homology Hu,dR(M)H^{u,\mathrm{dR}}_{\ast}(M). In the second part of this section we will then prove Poincaré duality of the latter with bounded de Rham cohomology: Hb,dR(M)Hmu,dR(M)H_{b,\mathrm{dR}}^{\ast}(M)\cong H^{u,\mathrm{dR}}_{m-\ast}(M). And at the end of this section we will introduce uniform de Rham cohomology and construct the uniform Chern character from uniform KK-theory to it.

Definition 4.

We define the space of uniform de Rham pp-currents Ωpu(M)\Omega_{p}^{u}(M) to be the topological dual space of the Fréchet space W,1(Ωp(M))W^{\infty,1}(\Omega^{p}(M)), i.e.,

Ωpu(M):=Hom(W,1(Ωp(M)),).\Omega_{p}^{u}(M):=\operatorname{Hom}(W^{\infty,1}(\Omega^{p}(M)),\mathbb{C}).

Recall from Definition 8 and Equation (2.3) that W,1(Ωp(M))W^{\infty,1}(\Omega^{p}(M)) denotes the Sobolev space of pp-forms whose derivatives are all L1L^{1}-integrable.

Since the exterior derivative d:W,1(Ωp(M))W,1(Ωp+1(M))d\colon W^{\infty,1}(\Omega^{p}(M))\to W^{\infty,1}(\Omega^{p+1}(M)) is continuous we get a corresponding dual differential (also denoted by dd)

d:Ωpu(M)Ωp1u(M).d\colon\Omega_{p}^{u}(M)\to\Omega_{p-1}^{u}(M). (3.1)

We define the uniform de Rham homology Hu,dR(M)H^{u,\mathrm{dR}}_{\ast}(M) with coefficients in \mathbb{C} as the homology of the complex

dΩpu(M)dΩp1u(M)ddΩ0(M)0,\ldots\stackrel{{\scriptstyle d}}{{\longrightarrow}}\Omega_{p}^{u}(M)\stackrel{{\scriptstyle d}}{{\longrightarrow}}\Omega^{u}_{p-1}(M)\stackrel{{\scriptstyle d}}{{\longrightarrow}}\ldots\stackrel{{\scriptstyle d}}{{\longrightarrow}}\Omega_{0}(M)\to 0,

where dd is the dual differential (3.1).

Definition 5.

We define a map α:Ccontp(W,1(M))Ωpu(M)\alpha\colon C_{\mathrm{cont}}^{p}(W^{\infty,1}(M))\to\Omega_{p}^{u}(M) by

α(φ)(f0df1dfp):=1p!σ𝔖p(1)σφ(f0,fσ(1),,fσ(p)),\alpha(\varphi)(f_{0}df_{1}\wedge\ldots\wedge df_{p}):=\frac{1}{p!}\sum_{\sigma\in\mathfrak{S}_{p}}(-1)^{\sigma}\varphi(f_{0},f_{\sigma(1)},\ldots,f_{\sigma(p)}),

where 𝔖p\mathfrak{S}_{p} denotes the symmetric group on 1,,p1,\ldots,p.

The antisymmetrization that we have done in the above definition of α\alpha maps Hochschild cocycles to Hochschild cocycles and vanishes on Hochschild coboundaries. This means that α\alpha descends to a map

α:HHcont(W,1(M))Ωu(M)\alpha\colon H\!H_{\mathrm{cont}}^{\ast}(W^{\infty,1}(M))\to\Omega_{\ast}^{u}(M)

on Hochschild cohomology.

Before we can prove that α\alpha is an isomorphism we need a technical lemma:

Lemma 6.

Let MM and NN be manifolds of bounded geometry and without boundary. Then we have

W,1(M)^W,1(N)W,1(M×N),W^{\infty,1}(M)\operatorname{\hat{\otimes}}W^{\infty,1}(N)\cong W^{\infty,1}(M\times N),

where ^\operatorname{\hat{\otimes}} denotes the projective tensor product.

Proof 3.1.

This proof is an elaboration of P. Michor’s answer [Mic14] on MathOverflow. The reference that he gives is [Mic78]: combining the Theorem on p. 78 in it with Point (c) on top of the same page we get the isomorphism L1(M)^L1(N)L1(M×N)L^{1}(M)\operatorname{\hat{\otimes}}L^{1}(N)\cong L^{1}(M\times N). This result was first proven by Chevet [Che69].

Now let us generalize this to incorporate derivatives. In [KMR15, End of Section 6] it is proven131313To be concrete, they proved it only for Euclidean space, but the argument is the same for manifolds of bounded geometry. that we have a continuous inclusion W,1(M)^W,1(N)W,1(M×N)W^{\infty,1}(M)\operatorname{\hat{\otimes}}W^{\infty,1}(N)\to W^{\infty,1}(M\times N). Note that we have to use [Che69, Théorème 1 on p. 124] to conclude that the family of seminorms used in [KMR15] for W,1(M)^W,1(N)W^{\infty,1}(M)\operatorname{\hat{\otimes}}W^{\infty,1}(N) generates indeed the projective tensor product topology.

It remains to show that W,1(M×N)W,1(M)^W,1(N)W^{\infty,1}(M\times N)\to W^{\infty,1}(M)\operatorname{\hat{\otimes}}W^{\infty,1}(N) is continuous. For this we will use the fact that we may represent the projective tensor product norm on the algebraic tensor product EalgFE\otimes_{\mathrm{alg}}F of two Banach spaces by

uE^F=inf{xiEyiF},\|u\|_{E\operatorname{\hat{\otimes}}F}=\inf\Big{\{}\sum\|x_{i}\|_{E}\|y_{i}\|_{F}\Big{\}},

where the infimum ranges over all representations u=ixiyiu=\sum_{i}x_{i}\otimes y_{i}. In our case now note that we have for w:=i(Xpi)qiw:=\sum_{i}(\nabla_{X}p_{i})\otimes q_{i}, where XX is a vector field on MM with X1\|X\|_{\infty}\leq 1, the chain of inequalities

wL1(M)^L1(N)\displaystyle\|w\|_{L^{1}(M)\operatorname{\hat{\otimes}}L^{1}(N)} =(Xpi)qiL1(M)^L1(N)\displaystyle=\left\|\sum(\nabla_{X}p_{i})\otimes q_{i}\right\|_{L^{1}(M)\operatorname{\hat{\otimes}}L^{1}(N)}
C(Xpi)qiL1(M×N)\displaystyle\leq C\left\|\sum(\nabla_{X}p_{i})\cdot q_{i}\right\|_{L^{1}(M\times N)}
CpiqiW1,1(M×N),\displaystyle\leq C\|\sum p_{i}\cdot q_{i}\|_{W^{1,1}(M\times N)}, (3.2)

where the first inequality comes from the fact L1(M)^L1(N)L1(M×N)L^{1}(M)\operatorname{\hat{\otimes}}L^{1}(N)\cong L^{1}(M\times N) which we already know. Now for v:=isitiv:=\sum_{i}s_{i}\otimes t_{i} we have

vW1,1(M)^L1(N)\displaystyle\|v\|_{W^{1,1}(M)\operatorname{\hat{\otimes}}L^{1}(N)} =sitiW1,1(M)^L1(N)\displaystyle=\Big{\|}\sum s_{i}\otimes t_{i}\Big{\|}_{W^{1,1}(M)\operatorname{\hat{\otimes}}L^{1}(N)} (3.3)
=inf{(xiL1(M)+xiL1(M))yiL1(N)}\displaystyle=\inf\Big{\{}\sum\big{(}\|x_{i}\|_{L^{1}(M)}+\|\nabla x_{i}\|_{L^{1}(M)}\big{)}\|y_{i}\|_{L^{1}(N)}\Big{\}}
=inf{xiL1(M)yiL1(N)}=vL1(M)^L1(N)CvL1(M×N)+inf{xiL1(M)yiL1(N)},\displaystyle=\underbrace{\inf\Big{\{}\sum\|x_{i}\|_{L^{1}(M)}\|y_{i}\|_{L^{1}(N)}\Big{\}}}_{=\|v\|_{L^{1}(M)\operatorname{\hat{\otimes}}L^{1}(N)}\leq C\|v\|_{L^{1}(M\times N)}}+\inf\Big{\{}\sum\|\nabla x_{i}\|_{L^{1}(M)}\|y_{i}\|_{L^{1}(N)}\Big{\}},

where the infima run over all representations ixiyi\sum_{i}x_{i}\otimes y_{i} of vv. Furthermore, for a fixed compactly supported vector field XX with X1\|X\|_{\infty}\leq 1 we have

inf𝒜{XxiL1(M)yiL1(N)}=inf{eiL1(M)fiL1(N)},\inf_{\mathcal{A}}\Big{\{}\sum\|\nabla_{X}x_{i}\|_{L^{1}(M)}\|y_{i}\|_{L^{1}(N)}\Big{\}}=\inf_{\mathcal{B}}\Big{\{}\sum\|e_{i}\|_{L^{1}(M)}\|f_{i}\|_{L^{1}(N)}\Big{\}}, (3.4)

where 𝒜\mathcal{A} is the set of all representations ixiyi\sum_{i}x_{i}\otimes y_{i} of v=isitiv=\sum_{i}s_{i}\otimes t_{i} and \mathcal{B} the set of all representations ieifi\sum_{i}e_{i}\otimes f_{i} of i(Xsi)ti\sum_{i}(\nabla_{X}s_{i})\otimes t_{i}. This equality holds because every element of 𝒜\mathcal{A} gives rise to an element of \mathcal{B} by deriving the first component and also vice versa by integrating it. By Inequality (3.2) we now get that the infima in Equation (3.4) are less than or equal to CvW1,1(M×N)C\|v\|_{W^{1,1}(M\times N)}. Since this holds for any vector field XX with X1\|X\|_{\infty}\leq 1 we can combine it now with Estimate (3.3) to get

vW1,1(M)^L1(N)2CvW1,1(M×N).\|v\|_{W^{1,1}(M)\operatorname{\hat{\otimes}}L^{1}(N)}\leq 2C\|v\|_{W^{1,1}(M\times N)}.

We iterate the argument to get estimates for all higher derivatives and also for the second component. This proves the claim that the map W,1(M×N)W,1(M)^W,1(N)W^{\infty,1}(M\times N)\to W^{\infty,1}(M)\operatorname{\hat{\otimes}}W^{\infty,1}(N) is continuous and therefore completes the whole proof.

Theorem 7.

For any Riemannian manifold MM of bounded geometry and without boundary the map α:HHcontp(W,1(M))Ωpu(M)\alpha\colon H\!H_{\mathrm{cont}}^{p}(W^{\infty,1}(M))\to\Omega_{p}^{u}(M) is an isomorphism for all pp.

Proof 3.2.

The proof is analogous to the one given in [Con85, Lemma 45a on page 128] for the case of compact manifolds. We describe here only the places where we have to adjust it for non-compact manifolds.

The proof in [Con85] relies heavily on Lemma 44 there. First note that direct sums, tensor products and duals of vector bundles of bounded geometry are again of bounded geometry. Since the tangent and cotangent bundle of a manifold of bounded geometry have, of course, bounded geometry, the bundles EkE_{k} occuring in Lemma 44 of [Con85] have bounded geometry.

Furthermore, [Con85, Lemma 44] needs a nowhere vanishing vector field on MM, and since we are working here in the bounded geometry setting we need for our proof a nowhere vanishing vector field of norm one at every point and with bounded derivatives. Since we can without loss of generality assume that our manifold is non-compact (otherwise we are in the usual setting where the result that we want to prove is already known), we can always contruct a nowhere vanishing vector field on MM: we just pick a generic vector field with isolated zeros and then move the vanishing points to infinity. But if we normalize this vector field to norm one at every point, then it will usually have unbounded derivatives (since we moved the vanishing points infinitely far, i.e., we disturbed the derivatives arbitrarily large). Fortunately, Weinberger proved in [Wei09, Theorem 1] that on a manifold MM of bounded geometry a nowhere vanishing vector field of norm one and with bounded derivatives exists if and only if the Euler class e(M)Hb,dRm(M)e(M)\in H_{b,\mathrm{dR}}^{m}(M) vanishes (the latter group denotes the top-dimensional bounded de Rham cohomology of MM; see Definition 9). So if the Euler class of MM vanishes, we are ok and can move on with our proof. If the Euler class does not vanish, then we have to use the same trick that already Connes used to prove Lemma 45a in [Con85]: we take the product with S1S^{1}.

Moreover, we need the isomorphism W,1(M)^W,1(M)W,1(M×M)W^{\infty,1}(M)\operatorname{\hat{\otimes}}W^{\infty,1}(M)\cong W^{\infty,1}(M\times M). This is exactly the content of the above Lemma 6.

The fact that the modules k=W,1(M×M,Ek)\mathcal{M}_{k}=W^{\infty,1}(M\times M,E_{k}) are topologically projective, i.e., are direct summands of topological modules of the form k=W,1(M×M)^k\mathcal{M}^{\prime}_{k}=W^{\infty,1}(M\times M)\operatorname{\hat{\otimes}}\mathcal{E}_{k}, where k\mathcal{E}_{k} are complete locally convex vector spaces, follows from the fact that every vector bundle FF of bounded geometry is CbC_{b}^{\infty}-complemented, i.e., there is a vector bundle GG of bounded geometry such that FGF\oplus G is CbC_{b}^{\infty}-isomorphic to a trivial bundle with the flat connection. This is stated in Proposition 26.

With the above notes in mind, the proof of [Con85, Lemma 45a on page 128] for the case of compact manifolds works also for non-compact manifolds in our setting here. If there are constructions to be done in the proof we have to do them uniformly (e.g., controlling derivatives uniformly in the points of the manifold) by using the bounded geometry of MM.

The inverse map β:Ωpu(M)HHcontp(W,1(M))\beta\colon\Omega^{u}_{p}(M)\to H\!H_{\mathrm{cont}}^{p}(W^{\infty,1}(M)) of α\alpha is given by

β(C)(f0,f1,,fp)=C(f0df1dfp).\beta(C)(f_{0},f_{1},\ldots,f_{p})=C(f_{0}df_{1}\wedge\ldots\wedge df_{p}).

Now the proofs of Lemma 45b and Theorem 46 in [Con85] translate without change to our setting here so that we finally get:

Theorem 8.

Let MM be a Riemannian manifold with bounded geometry and no boundary.

For each n0n\in\mathbb{N}_{0} the continuous cyclic cohomology HCcontn(W,1(M))H\!C_{\mathrm{cont}}^{n}(W^{\infty,1}(M)) is canonically isomorphic to

Znu(M)Hn2u,dR(M)Hn4u,dR(M),Z_{n}^{u}(M)\oplus H^{u,\mathrm{dR}}_{n-2}(M)\oplus H^{u,\mathrm{dR}}_{n-4}(M)\oplus\ldots,

where Znu(M)Ωnu(M)Z_{n}^{u}(M)\subset\Omega_{n}^{u}(M) is the subspace of closed currents.

The periodicity operator S:HCcontn(W,1(M))HCcontn+2(W,1(M))S\colon H\!C_{\mathrm{cont}}^{n}(W^{\infty,1}(M))\to H\!C_{\mathrm{cont}}^{n+2}(W^{\infty,1}(M)) is given under the above isomorphism as the map that sends cycles of Znu(M)Z_{n}^{u}(M) to their homology classes.

And last, since periodic cyclic cohomology is the direct limit of cyclic cohomology, we finally get

α:HPcontev/odd(W,1(M))Hev/oddu,dR(M).\alpha_{\ast}\colon H\!P_{\mathrm{cont}}^{\mathrm{ev/odd}}(W^{\infty,1}(M))\stackrel{{\scriptstyle\cong}}{{\longrightarrow}}H^{u,\mathrm{dR}}_{\mathrm{ev/odd}}(M).

We denote this isomorphism by α\alpha_{\ast} since it is induced from the map α\alpha defined above.

Let us now get to the dual cohomology theory to uniform de Rham homology.

Definition 9 (Bounded de Rham cohomology).

Let Ωbp(M)\Omega_{b}^{p}(M) denote the vector space of pp-forms on MM, which are bounded in the norm

γ:=supxM{γ(x)+dγ(x)}.\|\gamma\|:=\sup_{x\in M}\{\|\gamma(x)\|+\|d\gamma(x)\|\}.

The bounded de Rham cohomology Hb,dR(M)H_{b,\mathrm{dR}}^{\ast}(M) is defined as the homology of the corresponding complex.

For an oriented manifold the Poincaré duality map between bounded de Rham cohomology and uniform de Rham homology is defined as the map induced by the following map on forms:

Ωbp(M)Ωmpu(M),γ(ωMωγ).\Omega^{p}_{b}(M)\to\Omega^{u}_{m-p}(M),\ \gamma\mapsto\big{(}\omega\mapsto\int_{M}\omega\wedge\gamma\big{)}. (3.5)
Theorem 10.

Let MmM^{m} be an oriented Riemannian manifold of bounded geometry and without boundary.

Then the Poincaré duality map (3.5) induces an isomorphism

Hb,dR(M)Hmu,dR(M)H_{b,\mathrm{dR}}^{\ast}(M)\stackrel{{\scriptstyle\cong}}{{\longrightarrow}}H^{u,\mathrm{dR}}_{m-\ast}(M)

between bounded de Rham cohomology of MM and uniform de Rham homology of MM.

Proof 3.3.

We will do a Mayer–Vietoris induction, similar as in the proof of Poincaré duality between uniform KK-theory and uniform KK-homology in [Eng15a, Section 4.4].

We invoke Lemma 14 to get a cover of MM by open subsets having Properties 1 and 2 from that lemma.141414With the additional property that the boundaries of the open subsets are smooth, but it is clear that we can arrange this. We use the notation UjU_{j} and UKU_{K} from it, and the induction will be over the index jj (and hence the proof will only consist of finitely many induction steps).

We have to show that we have the Mayer–Vietoris sequences. The arguments are the same as in the case of compact manifolds, and we will only mention where we have to be cautios because we are working in the setting of uniform theories. We will only discuss the case of bounded de Rham cohomology, since the additional arguments (because of the uniform situation) in the case of uniform de Rham homology are similar.

For bounded de Rham cohomology we have to show that the following sequence is exact in order to get a Mayer–Vietoris sequence:

0Ωb(UKUk+1)Ωb(UK)Ωb(Uk+1)Ωb(UKUk+1)0.0\to\Omega_{b}^{*}(U_{K}\cup U_{k+1})\to\Omega_{b}^{*}(U_{K})\oplus\Omega_{b}^{*}(U_{k+1})\to\Omega_{b}^{*}(U_{K}\cap U_{k+1})\to 0. (3.6)

The crucial step is to show that the map Ωb(UK)Ωb(Uk+1)Ωb(UKUk+1)\Omega_{b}^{*}(U_{K})\oplus\Omega_{b}^{*}(U_{k+1})\to\Omega_{b}^{*}(U_{K}\cap U_{k+1}) is surjectice. The usual argument in the case of compact manifolds uses a partition of unity, and here we have to make sure now that the partition of unity has uniformly bounded derivatives of all orders. The reason that we can construct such a partition of unity here is because of Property 2 of Lemma 14.

That the above defined Poincaré duality map (3.5) is a natural transformation from one Mayer–Vietoris sequence to the other may be proved analogously as in the case of compact manifolds; see, e.g., [Lee03, Exercise 16-6].

And finally, let us discuss the first step of the induction. We have collections U1U_{1}, U2U_{2} and U1U2U_{1}\cap U_{2} which are each a uniformly disjoint union of open subsets of MM which have a uniform bound on their diameters. So all three sets are boundedly homotopy equivalent151515Let f,g:MNf,g\colon M\to N be two maps of bounded dilatation. We say that they are boundedly homotopic, if there is a homotopy H:M×[0,1]NH\colon M\times[0,1]\to N from ff to gg, which itself is of bounded dilatation. Recall that a map hh has bounded dilatation, if hVCV\|h_{\ast}V\|\leq C\|V\| for all tangent vectors VV. Bounded homotopy invariance of bounded de Rham cohomology was shown by the author in [Eng14, Corollary 5.26]. to an infinite collection of open balls, for which we already know from the case of compact manifolds that the Poincaré duality map is an isomorphism.

Bounded de Rham cohomology does not perfectly fit the setting in this paper since the condition that the exterior derivative of a form is bounded does not imply that in local coordinates the coefficient functions have a uniformly bounded first derivative, and it also does not say anything about the higher derivatives. Hence the following definition and proposition.

Definition 11.

The uniform de Rham cohomology Hu,dR(M)H_{u,\mathrm{dR}}^{\ast}(M) of a Riemannian manifold MM of bounded geometry is defined by using the complex of uniform CC^{\infty}-spaces161616see Definition 7 Cb(Ω(M))C^{\infty}_{b}(\Omega^{\ast}(M)), i.e., differential forms on MM which have in normal coordinates bounded coefficient functions and all derivatives of them are also bounded.

Proposition 12.

Let MM be a manifold of bounded geometry and without boundary. Then we have

Hu,dR(M)Hb,dR(M).H_{u,\mathrm{dR}}^{\ast}(M)\cong H_{b,\mathrm{dR}}^{\ast}(M).
Proof 3.4.

The proof is analogous to the one of Theorem 10 — the important thing is that we have Mayer–Vietoris sequences and the argument given in the proof of Theorem 10 for bounded de Rham cohomology also applies to uniform de Rham cohomology.

Theorem 13 (Existence of the uniform Chern character).

Let MM be a Riemannian manifold of bounded geometry and without boundary.

Then we have a ring homomorphism ch:Ku(M)Hu,dR(M)\operatorname{ch}\colon K^{\ast}_{u}(M)\to H_{u,\mathrm{dR}}^{\ast}(M) with

ch(Ku0(M))Hu,dRev(M) and ch(Ku1(M))Hu,dRodd(M).\operatorname{ch}(K^{0}_{u}(M))\subset H_{u,\mathrm{dR}}^{\mathrm{ev}}(M)\text{ and }\operatorname{ch}(K^{1}_{u}(M))\subset H_{u,\mathrm{dR}}^{\mathrm{odd}}(M).
Proof 3.5.

The Chern character is defined via Chern–Weil theory. That we get uniform forms if we use vector bundles of bounded geometry is proven in [Roe88a, Theorem 3.8] and so we get a map ch:Ku0(M)Hu,dRev(M)\operatorname{ch}\colon K^{0}_{u}(M)\to H_{u,\mathrm{dR}}^{\mathrm{ev}}(M). That we also have a map ch:Ku1(M)Hu,dRodd(M)\operatorname{ch}\colon K^{1}_{u}(M)\to H_{u,\mathrm{dR}}^{\mathrm{odd}}(M) uses the description of Ku1(M)K^{1}_{u}(M) from Theorem 28, i.e., that it consists of suitable vector bundles over S1×MS^{1}\times M, and a corresponding suspension isomorphism for the uniform de Rham cohomology. Details (for bounded cohomology, but for uniform cohomology it is analogous) may be found in the author’s Ph.D. thesis [Eng14, Sections 5.4 & 5.5].

3.3 Uniform Chern character isomorphism theorems

The results of the last two sections tell us that we have constructed Chern characters Ku(M)Hu,dR(M)K^{\ast}_{u}(M)\to H_{u,\mathrm{dR}}^{\ast}(M) and Ku(M)Hu,dR(M)K_{\ast}^{u}(M)\to H^{u,\mathrm{dR}}_{\ast}(M). Here we already use the Corollary 4 further below which states that the uniform homological Chern character is well-defined. In the compact case the Chern characters are isomorphisms modulo torsion and it is natural to ask the same question here in the uniform setting. It is the goal of this section to answer this question positively.

The proofs use the same Mayer–Vietoris induction as the proof of Poincaré duality in [Eng15a, Section 4.4] and Theorem 10. Therefore we will discuss in this section only the parts of the proofs which need additional arguments.

The most crucial detail to discuss here is the statement of the theorem itself since we cannot just take the tensor product of the KK-groups with the complex numbers to get isomorphisms. In turns out that we additionally have to form a certain completion of the algebraic tensor product of the KK-groups with \mathbb{C}. We will discuss this completion directly after the statement of the theorem.

Theorem 14.

Let MM be a manifold of bounded geometry and without boundary. Then the Chern characters induce linear, continuous isomorphisms171717The inverse maps are in general not continuous, because Hu,dR(M)H_{u,\mathrm{dR}}^{\ast}(M), respectively Hu,dR(M)H^{u,\mathrm{dR}}_{\ast}(M), are in general (e.g., if MM is not compact) not Hausdorff, whereas Ku(M)¯K_{u}^{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}, respectively Ku(M)¯K^{u}_{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}, are. The topology on the latter spaces is defined by equipping the KK-groups with the discrete topology and then forming the completed tensor product with \mathbb{C} which will be discussed after the statement of the theorem.

Ku(M)¯Hu,dR(M) and Ku(M)¯Hu,dR(M).K_{u}^{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H_{u,\mathrm{dR}}^{\ast}(M)\text{ and }K^{u}_{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H^{u,\mathrm{dR}}_{\ast}(M).

Let us discuss why we have to take a completion at all. Consider the beginning of the Mayer–Vietoris induction where we have to show that the Chern characters induce isomorphisms on a countably infinite collection of uniformly discretely distributed points. Let these points be indexed by a set YY. Then the KK-groups of YY are given by (Y)\ell^{\infty}_{\mathbb{Z}}(Y), the group of all bounded, integer-valued sequences indexed by YY, and the de Rham groups are given by (Y)\ell^{\infty}(Y), the group of all bounded, complex valued sequences on YY. But since YY is countably infinite we have (Y)≇(Y)\ell^{\infty}_{\mathbb{Z}}(Y)\otimes\mathbb{C}\not\cong\ell^{\infty}(Y). Instead we have (Y)¯(Y)\overline{\ell^{\infty}_{\mathbb{Z}}(Y)\otimes\mathbb{C}}\cong\ell^{\infty}(Y).

To define the completed topological tensor product of an abelian group with \mathbb{C} we will need the notion of the free (abelian) topological group: if XX is any completely regular181818That is to say, every closed set KK can be separated with a continuous function from every point xKx\notin K. Note that this does not necessarily imply that XX is Hausdorff. topological space, then the free topological group F(X)F(X) on XX is a topological group such that we have

  • a topological embedding XF(X)X\hookrightarrow F(X) of XX as a closed subset, so that XX generates F(X)F(X) algebraically as a free group (i.e., the algebraic group underlying the free topological group on XX is the free group on XX), and we have

  • the following universal property: for every continuous map ϕ:XG\phi\colon X\to G, where GG is any topological group, we have a unique extension Φ:F(X)G\Phi\colon F(X)\to G of ϕ\phi to a continuous group homomorphism on F(X)F(X):

    X\textstyle{X\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}ϕ\scriptstyle{\phi}F(X)\textstyle{F(X)\ignorespaces\ignorespaces\ignorespaces\ignorespaces}!Φ\scriptstyle{\exists!\Phi}G\textstyle{G}

The free abelian topological group A(X)A(X) has the corresponding analogous properties. Furthermore, the commutator subgroup [F(X),F(X)][F(X),F(X)] of F(X)F(X) is closed and the quotient F(X)/[F(X),F(X)]F(X)/[F(X),F(X)] is both algebraically and topologically A(X)A(X).

As an easy example consider XX equipped with the discrete topology. Then F(X)F(X) and A(X)A(X) also have the discrete topology.

It seems that free (abelian) topological groups were apparently introduced by Markov in [Mar41]. But unfortunately, the author could not obtain any (neither russian nor english) copy of this article. A complete proof of the existence of such groups was given by Markov in [Mar45]. Since his proof was long and complicated, several other authors gave other proofs, e.g., Nakayama in [Nak43], Kakutani in [Kak44] and Graev in [Gra48].

Now let us construct for any abelian topological group GG the complete topological vector space G¯G\operatorname{\bar{\otimes}}\mathbb{C}. We form the topological tensor product GG\otimes\mathbb{C} of abelian topological groups in the usual way: we start with the free abelian topological group A(G×)A(G\times\mathbb{C}) over the topological space G×G\times\mathbb{C} equipped with the product topology191919Note that every topological group is automatically completely regular and therefore the product G×G\times\mathbb{C} is also completely regular. and then take the quotient A(G×)/𝒩A(G\times\mathbb{C})/\mathcal{N} of it,202020Since A(X)A(X) is both algebraically and topologically the quotient of F(X)F(X) by its commutator subgroup, we could also have started with F(G×)F(G\times\mathbb{C}) and additionally put the commutator relations into 𝒩\mathcal{N}. where 𝒩\mathcal{N} is the closure of the normal subgroup generated by the usual relations for the tensor product.212121That is to say, 𝒩\mathcal{N} contains (g1+g2)×rg1×rg2×r(g_{1}+g_{2})\times r-g_{1}\times r-g_{2}\times r, g×(r1+r2)g×r1g×r2g\times(r_{1}+r_{2})-g\times r_{1}-g\times r_{2} and zg×rz(g×r)zg\times r-z(g\times r), g×zrz(g×r)g\times zr-z(g\times r), where g,g1,g2Gg,g_{1},g_{2}\in G, r,r1,r2r,r_{1},r_{2}\in\mathbb{C} and zz\in\mathbb{Z}. Now we may put on GG\otimes\mathbb{C} the structure of a topological vector space by defining the scalar multiplication to be λ(gr):=gλr\lambda(g\otimes r):=g\otimes\lambda r.

What we now got is a topological vector space GG\otimes\mathbb{C} together with a continuous map G×GG\times\mathbb{C}\to G\otimes\mathbb{C} with the following universal property: for every continuous map ϕ:G×V\phi\colon G\times\mathbb{C}\to V into any topological vector space VV and such that ϕ\phi is bilinear222222That is to say, ϕ(,r)\phi(\raisebox{-1.07639pt}{\scalebox{1.2}{$\cdot$}},r) is a group homomorphism for all rr\in\mathbb{C} and ϕ(g,)\phi(g,\raisebox{-1.07639pt}{\scalebox{1.2}{$\cdot$}}) is a linear map for all gGg\in G. Note that we then also have ϕ(zg,r)=zϕ(g,r)=ϕ(g,zr)\phi(zg,r)=z\phi(g,r)=\phi(g,zr) for all zz\in\mathbb{Z}, gGg\in G and rr\in\mathbb{C}., there exists a unique, continuous linear map Φ:GV\Phi\colon G\otimes\mathbb{C}\to V such that the following diagram commutes:

G×\textstyle{G\times\mathbb{C}\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}ϕ\scriptstyle{\phi}G\textstyle{G\otimes\mathbb{C}\ignorespaces\ignorespaces\ignorespaces\ignorespaces}!Φ\scriptstyle{\exists!\Phi}V\textstyle{V}

Since every topological vector space may be completed we do this with GG\otimes\mathbb{C} to finally arrive at G¯G\operatorname{\bar{\otimes}}\mathbb{C}. Since every continuous linear map of topological vector spaces is automatically uniformly continuous, i.e., may be extended to the completion of the topological vector space, G¯G\operatorname{\bar{\otimes}}\mathbb{C} enjoys the following universal property which we will raise to a definition:

Definition 15 (Completed topological tensor product with \mathbb{C}).

Let GG be an abelian topological group. Then G¯G\operatorname{\bar{\otimes}}\mathbb{C} is a complete topological vector space over \mathbb{C} together with a continuous map G×G¯G\times\mathbb{C}\to G\operatorname{\bar{\otimes}}\mathbb{C} that enjoy the following universal property: for every continuous map ϕ:G×V\phi\colon G\times\mathbb{C}\to V into any complete topological vector space VV and such that ϕ\phi is bilinear232323see Footnote 22, there exists a unique, continuous linear map Φ:G¯V\Phi\colon G\operatorname{\bar{\otimes}}\mathbb{C}\to V such that

G×\textstyle{G\times\mathbb{C}\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}ϕ\scriptstyle{\phi}G¯\textstyle{G\operatorname{\bar{\otimes}}\mathbb{C}\ignorespaces\ignorespaces\ignorespaces\ignorespaces}!Φ\scriptstyle{\exists!\Phi}V\textstyle{V}

is a commutative diagram.

We will give now two examples for the computation of G¯G\operatorname{\bar{\otimes}}\mathbb{C}. The first one is easy and just a warm-up for the second which we already mentioned. Both examples are proved by checking the universal property.

Examples 16.

The first one is ¯\mathbb{Z}\operatorname{\bar{\otimes}}\mathbb{C}\cong\mathbb{C}.

For the second example consider the group \ell^{\infty}_{\mathbb{Z}} consisting of bounded, integer-valued sequences. Then ¯\ell^{\infty}_{\mathbb{Z}}\operatorname{\bar{\otimes}}\mathbb{C}\cong\ell^{\infty}. ∎

Since we want to use the completed topological tensor product with \mathbb{C} in a Mayer–Vietoris argument, we have to show that it transforms exact sequences to exact sequences.

So we have to show that the functor GG¯G\mapsto G\operatorname{\bar{\otimes}}\mathbb{C} is exact. But we have to be careful here: though taking the tensor product with \mathbb{C} is exact, passing to completions is usually not—at least if the exact sequence we started with was only algebraically exact. Let us explain this a bit more thoroughly: if we have a sequence of topological vector spaces

ViφiVi+1φi+1Vi+2\ldots\longrightarrow V_{i}\stackrel{{\scriptstyle\varphi_{i}}}{{\longrightarrow}}V_{i+1}\stackrel{{\scriptstyle\varphi_{i+1}}}{{\longrightarrow}}V_{i+2}\longrightarrow\ldots

which is exact in the algebraic sense (i.e., imφi=kerφi+1\operatorname{im}\varphi_{i}=\operatorname{ker}\varphi_{i+1}), and if the maps φi\varphi_{i} are continuous such that they extend to maps on the completions Vi¯\overline{V_{i}}, we do not necessarily get that

Vi¯φi¯Vi+1¯φi+1¯Vi+2¯\ldots\longrightarrow\overline{V_{i}}\stackrel{{\scriptstyle\overline{\varphi_{i}}}}{{\longrightarrow}}\overline{V_{i+1}}\stackrel{{\scriptstyle\overline{\varphi_{i+1}}}}{{\longrightarrow}}\overline{V_{i+2}}\longrightarrow\ldots

is again algebraically exact. The problem is that though we always have kerφi¯=kerφi¯\overline{\operatorname{ker}\varphi_{i}}=\operatorname{ker}\overline{\varphi_{i}}, we generally only get imφi¯imφi¯\overline{\operatorname{im}\varphi_{i}}\supset\operatorname{im}\overline{\varphi_{i}}. To correct this problem we have to start with an exact sequence which is also topologically exact, i.e., we need that not only imφi=kerφi+1\operatorname{im}\varphi_{i}=\operatorname{ker}\varphi_{i+1}, but we also need that φi\varphi_{i} induces a topological isomorphism Vi/kerφiimφiV_{i}/\operatorname{ker}\varphi_{i}\cong\operatorname{im}\varphi_{i}.

To prove that in this case we get imφi¯=imφi¯\overline{\operatorname{im}\varphi_{i}}=\operatorname{im}\overline{\varphi_{i}} we consider the inverse map

ψi:=φi1:imφiVi/kerφi.\psi_{i}:=\varphi_{i}^{-1}\colon\operatorname{im}\varphi_{i}\to V_{i}/\operatorname{ker}\varphi_{i}.

Since ψi\psi_{i} is continuous (this is the point which breaks down without the additional assumption that φi\varphi_{i} induces a topological isomorphism Vi/kerφiimφiV_{i}/\operatorname{ker}\varphi_{i}\cong\operatorname{im}\varphi_{i}), we may extend it to a map

ψi¯:imφi¯Vi/kerφi¯=Vi¯/kerφi¯,\overline{\psi_{i}}\colon\overline{\operatorname{im}\varphi_{i}}\to\overline{V_{i}/\operatorname{ker}\varphi_{i}}=\overline{V_{i}}/\overline{\operatorname{ker}\varphi_{i}},

which obviously is the inverse to φi¯:Vi¯/kerφi¯imφi¯\overline{\varphi_{i}}\colon\overline{V_{i}}/\overline{\operatorname{ker}\varphi_{i}}\to\overline{\operatorname{im}\varphi_{i}} showing the desired equality imφi¯=imφi¯\overline{\operatorname{im}\varphi_{i}}=\operatorname{im}\overline{\varphi_{i}}.

Coming back to our functor GG¯G\mapsto G\operatorname{\bar{\otimes}}\mathbb{C}, we may now prove the following lemma:

Lemma 17.

Let

GiφiGi+1φi+1Gi+2\ldots\longrightarrow G_{i}\stackrel{{\scriptstyle\varphi_{i}}}{{\longrightarrow}}G_{i+1}\stackrel{{\scriptstyle\varphi_{i+1}}}{{\longrightarrow}}G_{i+2}\longrightarrow\ldots

be an exact sequence of topological groups and continuous maps, which is in addition topologically exact, i.e., for all ii\in\mathbb{Z} the from φi\varphi_{i} induced map Gi/kerφiimφiG_{i}/\operatorname{ker}\varphi_{i}\to\operatorname{im}\varphi_{i} is an isomorphism of topological groups.

Then

Gi¯Gi+1¯Gi+2¯\ldots\longrightarrow G_{i}\operatorname{\bar{\otimes}}\mathbb{C}\longrightarrow G_{i+1}\operatorname{\bar{\otimes}}\mathbb{C}\longrightarrow G_{i+2}\operatorname{\bar{\otimes}}\mathbb{C}\longrightarrow\ldots

with the induced maps is an exact sequence of complete topological vector spaces, which is also topologically exact.

Proof 3.6.

We first tensor with \mathbb{C} (without the completion afterwards). This is known to be an exact functor and our sequence also stays topologically exact. To see this last claim, we need the following fact about tensor products: if φ:MM\varphi\colon M\to M^{\prime} and ψ:NN\psi\colon N\to N^{\prime} are surjective, then the kernel of φψ:MMNN\varphi\otimes\psi\colon M\otimes M^{\prime}\to N\otimes N^{\prime} is the submodule given by

ker(φψ)=(ιM1)((kerφ)N)+(1ιN)(M(kerψ)),\operatorname{ker}(\varphi\otimes\psi)=(\iota_{M}\otimes 1)\big{(}(\operatorname{ker}\varphi)\otimes N\big{)}+(1\otimes\iota_{N})\big{(}M\otimes(\operatorname{ker}\psi)\big{)},

where ιM:kerφM\iota_{M}\colon\operatorname{ker}\varphi\to M and ιN:kerψN\iota_{N}\colon\operatorname{ker}\psi\to N are the inclusion maps. We will suppress the inclusion maps from now on to shorten the notation.

We apply this with the map φ:MM\varphi\colon M\to M^{\prime} being the quotient map GiGi/kerφiG_{i}\to G_{i}/\operatorname{ker}\varphi_{i} and ψ:NN\psi\colon N\to N^{\prime} being the identity id:\operatorname{id}\colon\mathbb{C}\to\mathbb{C} to get

ker(φiid)=(kerφi).\operatorname{ker}(\varphi_{i}\otimes\operatorname{id})=(\operatorname{ker}\varphi_{i})\otimes\mathbb{C}.

Since we have (imφi)=im(φiid)(\operatorname{im}\varphi_{i})\otimes\mathbb{C}=\operatorname{im}(\varphi_{i}\otimes\operatorname{id}), we get that φid:GiGi\varphi\otimes\operatorname{id}\colon G_{i}\otimes\mathbb{C}\to G_{i}\otimes\mathbb{C} induces an algebraic isomorphism (Gi/kerφi)imφi(G_{i}/\operatorname{ker}\varphi_{i})\otimes\mathbb{C}\to\operatorname{im}\varphi_{i}\otimes\mathbb{C}. But this has now an inverse map given by tensoring the inverse of Gi/kerφiimφiG_{i}/\operatorname{ker}\varphi_{i}\to\operatorname{im}\varphi_{i} with id:\operatorname{id}\colon\mathbb{C}\to\mathbb{C}. So the isomorphism (Gi/kerφi)imφi(G_{i}/\operatorname{ker}\varphi_{i})\otimes\mathbb{C}\cong\operatorname{im}\varphi_{i}\otimes\mathbb{C} is also topological.

Now we apply the discussion before the lemma to show that the completion of this new sequence is still exact and also topologically exact.

To show Ku(M)¯Hu,dR(M)K_{u}^{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H_{u,\mathrm{dR}}^{\ast}(M) it remains to construct Mayer–Vietoris sequences with continuous maps in them (we need this since in constructing the completed tensor product with \mathbb{C} we have to pass to the completion and without continuity of the maps in both the Mayer–Vietoris sequences for uniform KK-theory and for uniform de Rham cohomology we would not be able to conclude that the squares are still commutative). If we recall from the proof of Proposition 12 how we get the boundary maps in the Mayer–Vietoris sequence for uniform de Rham cohomology, we see that we must construct a continuous split to the last non-trivial map in the sequence (3.6).242424The referenced sequence is for bounded de Rham cohomology. In this proof here we, of course, have to use the analogous sequence for uniform de Rham cohomology. But we proved surjectivity of this map in the usual way by using partitions of unity (with uniformly bounded derivatives). Hence we have already constructed the continuous split.

In the proof of Poincaré duality between uniform KK-theory and uniform KK-homology in [Eng15a, Section 4.4] we used groups denoted by Ku(OM)K^{\ast}_{u}(O\subset M) for the Mayer–Vietoris sequence for uniform KK-theory. These groups are defined as K(Cu(O,d))K_{-\ast}(C_{u}(O,d)), where (O,d)(O,d) is the metric space OO equipped with the subspace metric derived from the metric space MM. For the construction of the Chern character Ku(OM)Hu,dR(O)K^{\ast}_{u}(O\subset M)\to H_{u,\mathrm{dR}}^{\ast}(O) we have to pass to a smooth subalgebra of Cu(O,d)C_{u}(O,d). This will be of course Cb(O)Cu(O,d)C_{b}^{\infty}(O)\subset C_{u}(O,d), which is a local CC^{\ast}-algebra.252525That is to say, its operator KK-theory coincides with the operator KK-theory of its CC^{\ast}-algebra completion Cu(O,d)C_{u}(O,d). We have to argue now why it is a dense subalgebra: so let fCu(O,d)f\in C_{u}(O,d) be given. Then we know from [Eng15a, Lemma 4.36] that there is a bounded, uniformly continuous extension FF of ff to MM. Now we use [Eng15a, Lemma 4.7] to approximate FF by functions from Cb(M)C_{b}^{\infty}(M), which will give us by restriction to OO an approximation of ff by functions from Cb(O)C_{b}^{\infty}(O). Therefore we get an interpretation of Ku(OM)K^{\ast}_{u}(O\subset M) by vector bundles of bounded geometry over OO (cf. Section 2.3) and may define by Chern–Weil theory (as in Theorem 13) the Chern character Ku(OM)Hu,dR(O)K^{\ast}_{u}(O\subset M)\to H_{u,\mathrm{dR}}^{\ast}(O).

The last thing that we have to discuss is the small ambiguity in extending the maps Ku(OM)Hu,dR(O)K^{\ast}_{u}(O\subset M)\otimes\mathbb{C}\to H_{u,\mathrm{dR}}^{\ast}(O) to Ku(OM)¯K^{\ast}_{u}(O\subset M)\operatorname{\bar{\otimes}}\mathbb{C}. It occurs because the target Hu,dR(O)H_{u,\mathrm{dR}}^{\ast}(O) is not necessarily Hausdorff. What we have to make sure is that the extensions we choose in the Mayer–Vietoris argument for the subsets UkU_{k}, respectively UKU_{K}, do match up, i.e., produce at the end commuting squares in the comparison of the two Mayer–Vietoris sequences via the Chern characters.

So we have finally discussed everything that we need in order to prove

Ku(M)¯Hu,dR(M).K_{u}^{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H_{u,\mathrm{dR}}^{\ast}(M).

Proving the homological version Ku(M)¯Hu,dR(M)K^{u}_{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H^{u,\mathrm{dR}}_{\ast}(M) is also such a Mayer–Vietoris argument. But for spinc manifolds there is an easier argument by combining the cohomological result Ku(M)¯Hu,dR(M)K_{u}^{\ast}(M)\operatorname{\bar{\otimes}}\mathbb{C}\cong H_{u,\mathrm{dR}}^{\ast}(M) with Theorem 1 since taking the wedge product with ind(D)\operatorname{ind}(D) is an isomorphism on bounded de Rham cohomology, and furthermore using Poincaré duality between uniform KK-theory and uniform KK-homology (Theorem 30), respectively between bounded de Rham cohomology and uniform de Rham homology (Theorem 10).

4 Index theorems

In this section we assemble everything that we had up to now into various index theorems. In Section 4.1 we first recall the construction of the topological index classes of elliptic operators and then prove local index theorems. In Section 4.2 we prove a global index theorem, which will be a generalization of an index theorem of Roe [Roe88a]. He proved it for Dirac operators and we will generalize it to elliptic pseudodifferential operators.

4.1 Local index formulas

Let MM be a Riemannian manifold without boundary. We denote by DMDM the disk bundle {ξTM:ξ1}\{\xi\in T^{\ast}M\colon\|\xi\|\leq 1\} of its cotangent bundle and by SM=DMSM=\partial DM its boundary, i.e., SM={ξTM:ξ=1}SM=\{\xi\in T^{\ast}M\colon\|\xi\|=1\}. If MM has bounded geometry, we may equip DMDM with a Riemannian metric such that it also becomes of bounded geometry262626Though we do not have defined bounded geometry for manifolds with boundary, there is an obvious one (demanding bounds not only for the curvature tensor of MM but also for the second fundamental form of the boundary of MM, and demanding the injectivity radius being uniformly positive not only for MM but also for M\partial M with the induced metric). See [Sch01] for a further discussion. and DMMDM\to M becomes a Riemannian submersion. It follows that SMSM will also have bounded geometry. What follows will be independent of the concrete choice of metric on DMDM. Though we have discussed in Section 2.3 only uniform KK-theory for manifolds without boundary, one can of course define more generally relative uniform KK-theory and discuss it for manifolds with boundary and of bounded geometry.

Let PUΨDOk(E)P\in\mathrm{U}\Psi\mathrm{DO}^{k}(E) be a symmetric, elliptic and graded uniform pseudodifferential operator. Recall from Definition 16 of ellipticity that the principal symbol σ(P+)\sigma(P^{+}), viewed as a section of Hom(πE+,πE)TM\operatorname{Hom}(\pi^{\ast}E^{+},\pi^{\ast}E^{-})\to T^{\ast}M, where π:TMM\pi\colon T^{\ast}M\to M is the cotangent bundle, is invertible outside a uniform neighbourhood of the zero section MTMM\subset T^{\ast}M and satisfies a certain uniformity condition. Then the well-known clutching construction gives us the following symbol class of PP:

σP:=[πE+,πE;σ(P)]Ku0(DM,SM).\sigma_{P}:=[\pi^{\ast}E^{+},\pi^{\ast}E^{-};\sigma(P)]\in K_{u}^{0}(DM,SM).

If PP is ungraded, then its symbol σ(P):πEπE\sigma(P)\colon\pi^{\ast}E\to\pi^{\ast}E, where π:SMM\pi\colon SM\to M denotes now the unit sphere bundle of MM, is a uniform, self-adjoint automorphism. Hence it gives a direct sum decomposition πE=E+E\pi^{\ast}E=E^{+}\oplus E^{-}, where E+E^{+} and EE^{-} are spanned fiberwise by the eigenvectors belonging to the positive, respectively negative, eigenvalues of σ(P)\sigma(P), and we get an element

[E+]Ku0(SM).[E^{+}]\in K_{u}^{0}(SM).

Now we define in the ungraded case the symbol class of PP as

σP:=δ[E+]Ku1(DM,SM),\sigma_{P}:=\delta[E^{+}]\in K_{u}^{1}(DM,SM),

where δ:Ku0(SM)Ku1(DM,SM)\delta\colon K_{u}^{0}(SM)\to K_{u}^{1}(DM,SM) is the boundary homomorphism of the 66-term exact sequence associated to (DM,SM)(DM,SM). References for this construction in the compact case are, e.g., [BD82, Section 24] and [APS76, Proposition 3.1].

Applying the Chern character and integrating over the fibers we get in both the graded and ungraded case π!chσPHb,dR(M)\pi_{!}\operatorname{ch}\sigma_{P}\in H_{b,\mathrm{dR}}^{\ast}(M) and then the index class of PP is defined as

ind(P):=(1)n(n+1)2π!chσPTd(M)Hb,dR(M),\operatorname{ind}(P):=(-1)^{\frac{n(n+1)}{2}}\pi_{!}\operatorname{ch}\sigma_{P}\wedge\operatorname{Td}(M)\in H_{b,\mathrm{dR}}^{\ast}(M),

where n=dimMn=\dim M.

Let MM be a spinc manifold of bounded geometry and let us denote by DD the Dirac operator associated to the spinc structure of MM. Note that it is mm-multigraded, where mm is the dimension of the manifold MM, and so defines an element in Kmu(M)K_{m}^{u}(M). Hence cap product with DD is a map Ku(M)Kmu(M)K_{u}^{\ast}(M)\to K^{u}_{m-\ast}(M), which is an isomorphism (Theorem 30). We have also the Poincaré duality map Hb,dR(M)Hmu,dR(M)H_{b,\mathrm{dR}}^{\ast}(M)\to H^{u,\mathrm{dR}}_{m-\ast}(M), and the content of our local index theorem for uniform twisted Dirac operators is to put these duality maps into a commutative diagram using the homological Chern character on the right hand side and on the cohomology side the index class of the twisted operator.

Theorem 1 (Local index theorem for twisted uniform Dirac operators).

Let MM be an mm-dimensional spinc manifold of bounded geometry and without boundary. Denote the associated Dirac operator by DD.

Then we have the following commutative diagram:

Ku(M)\textstyle{K^{\ast}_{u}(M)\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}[D]\scriptstyle{-\cap[D]}\scriptstyle{\cong}ch()ind(D)\scriptstyle{\operatorname{ch}(-)\wedge\operatorname{ind}(D)}Kmu(M)\textstyle{K_{m-\ast}^{u}(M)\ignorespaces\ignorespaces\ignorespaces\ignorespaces}αch\scriptstyle{\alpha_{\ast}\circ\operatorname{ch}^{\ast}}Hb,dR(M)\textstyle{H_{b,\mathrm{dR}}^{\ast}(M)\ignorespaces\ignorespaces\ignorespaces\ignorespaces}\scriptstyle{\cong}Hmu,dR(M)\textstyle{H^{u,\mathrm{dR}}_{m-\ast}(M)}

where in the top row \ast is either 0 or 11 and in the bottom row \ast is either ev\mathrm{ev} or odd\mathrm{odd}.

Proof 4.1.

This follows from the calculations carried out by Connes and Moscovici in their paper [CM90, Section 3] by noting that the computations also apply in our case where we have bounded geometry and the uniformity conditions. Note that there the cyclic cocycles are defined using expressions in the operators etD2e^{-tD^{2}}. To translate to the definition of the homological Chern character that we use, see, e.g., [GBVF00, Section 10.2].

Remark 2.

The uniform homological Chern character αch:Ku(M)Hu,dR(M)\alpha_{\ast}\circ\operatorname{ch}^{\ast}\colon K_{\ast}^{u}(M)\dashrightarrow H^{u,\mathrm{dR}}_{\ast}(M) is a priori not well-defined (to be more precise, it is defined on uniformly finitely summable Fredholm modules and it is a priori not clear whether it descends to classes and even whether every class may be represented by a uniformly finitely summable module). But using Poincaré duality between uniform KK-homology and uniform KK-theory and the above local index theorem, we see that it is a posteriori well-defined for spinc manifolds. Note that since DD is a Dirac operator, it defines a uniformly finitely summable Fredholm module, and therefore also all its twists given by taking the cap product with uniform KK-theory classes are uniformly finitely summable.

That the uniform homological Chern character is well-defined for every manifold MM of bounded geometry is content of Corollary 4.

Let PP be a symmetric and elliptic uniform pseudodifferential operator over an oriented manifold MM of bounded geometry. It defines a uniform KK-homology class [P]Ku(M)[P]\in K_{\ast}^{u}(M) and therefore, if PP is in addition uniformly finitely summable, we may compare the class (αch)(P)Hu,dR(M)(\alpha_{\ast}\circ\operatorname{ch}^{\ast})(P)\in H^{u,\mathrm{dR}}_{\ast}(M) with ind(P)Hb,dR(M)\operatorname{ind}(P)\in H_{b,\mathrm{dR}}^{\ast}(M) using Poincaré duality. That they are equal is the content of the next theorem.

Theorem 3 (Local index formula for uniform pseudodifferential operators).

Let MM be an oriented Riemannian manifold of bounded geometry and without boundary.

Let PP be a symmetric and elliptic uniform pseudodifferential operator of positive order acting on a vector bundle EME\to M of bounded geometry, and let PP be uniformly finitely summable272727This means that PP defines a uniformly finitely summable Fredholm module, i.e., χ(P)\chi(P) is uniformly finitely summable for some normalizing function χ\chi..

Then ind(P)Hb,dR(M)\operatorname{ind}(P)\in H_{b,\mathrm{dR}}^{\ast}(M) is the Poincaré dual of (αch)(P)Hu,dR(M)(\alpha_{\ast}\circ\operatorname{ch}^{\ast})(P)\in H^{u,\mathrm{dR}}_{\ast}(M).

Proof 4.2.

This follows from the above Theorem 1 by the same arguments as in the proof of [CM90, Theorem 3.9]: if MM is odd-dimensional we take the product with S1S^{1}, and then we use the fact that for oriented, even-dimensional manifolds uniform KK-homology is spanned modulo 22-torsion by generalized signature operators. This last fact will follow from Theorem 6 below.

Corollary 4.

The uniform homological Chern character

αch:Ku(M)Hu,dR(M)\alpha_{\ast}\circ\operatorname{ch}^{\ast}\colon K_{\ast}^{u}(M)\to H^{u,\mathrm{dR}}_{\ast}(M)

is well-defined for every manifold MM of bounded geometry and without boundary.

Proof 4.3.

If MM is spinc we know by Poincaré duality that every class [x]Ku(M)[x]\in K_{\ast}^{u}(M) may be represented by a uniformly finitely summable Fredholm module and by the above Theorem 3 we conclude that (αch)([x])(\alpha_{\ast}\circ\operatorname{ch}^{\ast})([x]) is independent of the concrete choice of such a representative. (This was already mentioned in Remark 2.)

In the general case we first pass to the orientation cover XX if MM is not orientable. Note that if we know the statement that we want to prove for a finite covering of MM, then we know it also for MM itself since Hu,dR(M)H^{u,\mathrm{dR}}_{\ast}(M) is a vector space over \mathbb{C} (i.e., multiplication by some non-zero number is an isomorphism). Now we can go on as in the proof of Theorem 3: we take the product with S1S^{1} if necessary and then use the fact that on oriented, even-dimensional manifolds we can represent every uniform KK-homology class by a multiple (concretely, 2dim(M)/22^{\dim(M)/2}) of a generalized signature operator. For the latter statement see Theorem 6, respectively its proof.

Remark 5.

The condition in the above Theorem 3 that the operator PP is uniformly finitely summable may be dropped. The statement then is that (αch)([P])(\alpha_{\ast}\circ\operatorname{ch}^{\ast})([P]) is the dual of the class ind(P)Hb,dR(M)\operatorname{ind}(P)\in H_{b,\mathrm{dR}}^{\ast}(M). This makes sense since we now know that the uniform homological Chern character Ku(M)Hu,dR(M)K_{\ast}^{u}(M)\to H^{u,\mathrm{dR}}_{\ast}(M) is well-defined.

But the problem then is that in order to compute (αch)([P])(\alpha_{\ast}\circ\operatorname{ch}^{\ast})([P]) we would have to replace PP by some other operator PP^{\prime} which defines the same uniform KK-homology class as PP but which is uniformly finitely summable (so that we may compute the Chern–Connes character). This seems to be a task which is not easily carried out in practice.

Connes and Moscovici work in [CM90] with so-called θ\theta-summable Fredholm modules which are more general than finitely summable modules. So defining an appropriate version of uniformly θ\theta-summable Fredholm modules we could certainly prove the above Theorem 3 for them and therefore weakening the condition on PP that it has to be uniformly finitely summable.

Let us state now the Thom isomorphism theorem in the form that we need for the proof of the above Theorem 3.

Theorem 6 (Thom isomorphism).

Let MM be a Riemannian spinc manifold of bounded geometry and without boundary.

Then the principal symbol of the Dirac operator associated to the spinc structure of MM constitutes an orientation class in Ku(DM,SM)K_{u}^{\ast}(DM,SM), i.e., it implements the isomorphism Ku(M)Ku(DM,SM)K_{u}^{\ast}(M)\cong K_{u}^{\ast}(DM,SM).

If MM is only oriented (i.e., not necessarily spinc) and even-dimensional, the principal symbol of the signature operator of MM constitutes an orientation class in Ku(DM,SM)[12]K_{u}^{\ast}(DM,SM)[\tfrac{1}{2}].

Proof 4.4.

The usual proof as found in, e.g., [LM89, Appendix C], works in our case analogously. Note that for the proof of [LM89, Theorem C.7] we have to cover MM by such subsets as we used in our proof of Poincaré duality (see Lemma 14) since only in this case we have shown that we have a Mayer–Vietoris sequence for uniform KK-theory. For the statement for only oriented MM see, e.g., the proof of [LM89, Theorem C.12].

In [CM90, Theorem 3.9] the local index theorem was written using an index pairing with compactly supported cohomology classes. We can of course do the same also here in our uniform setting and the statement is at first glance the same.282828Remember that we have another choice of universal constants than Connes and Moscovici, i.e., in our statement they are not written since they are incorporated in the definition of the homological Chern character. But the difference is that due to the uniformness we have an additional continuity statement.

Corollary 7.

Let [φ]Hc,dRk(M)[\varphi]\in H_{c,\mathrm{dR}}^{k}(M) be a compactly supported cohomology class and define the analytic index ind[φ](P)\operatorname{ind}_{[\varphi]}(P) as in [CM90].292929Note that ind[φ](P)\operatorname{ind}_{[\varphi]}(P) is analytically defined and may be computed (up to the universal constant that we have incorporated into the definition of αch\alpha_{\ast}\circ\operatorname{ch}^{\ast}) as (αch)(P),[φ]\langle(\alpha_{\ast}\circ\operatorname{ch}^{\ast})(P),[\varphi]\rangle, where ,\langle-,-\rangle is the pairing between uniform de Rham homology and compact supported cohomology. Then we have

ind[φ](P)=Mind(P)[φ]\operatorname{ind}_{[\varphi]}(P)=\int_{M}\operatorname{ind}(P)\wedge[\varphi]

and this pairing is continuous, i.e., Mind(P)[φ]ind(P)[φ]1\int_{M}\operatorname{ind}(P)\wedge[\varphi]\leq\|\operatorname{ind}(P)\|_{\infty}\cdot\|[\varphi]\|_{1}, where \|-\|_{\infty} denotes the sup-seminorm on Hb,dRmk(M)H_{b,\mathrm{dR}}^{m-k}(M) and 1\|-\|_{1} the L1L^{1}-seminorm on Hc,dRk(M)H_{c,\mathrm{dR}}^{k}(M).

Proof 4.5.

The corollary follows from Theorem 3 (if MM is not orientable then we first have to pass to the orientation cover of it). The continuity statement follows from the definition of the seminorms. The only thing we have to know is that ind(P)\operatorname{ind}(P) is given by a bounded de Rham form.

Remark 8.

Though it may seem that the above corollary is in some sense equivalent to Theorem 3, it is in fact not. It is weaker in the following way: in case of a non-compact manifold MM the bounded de Rham cohomology Hb,dR(M)H_{b,\mathrm{dR}}^{\ast}(M) usually contains elements of seminorm =0=0 and due to the boundedness of the above pairing we see that we can not detect these elements by it.

4.2 Index pairings on amenable manifolds

In the last section we proved the local index theorems for uniform operators. The goal of this section is to use these local formulas to compute certain global indices of such operators over amenable manifolds.

So in this section we assume that our manifold MM is amenable, i.e., that it admits a Følner sequence. We will need such a sequence in order to construct the index pairings.

Definition 9 (Følner sequences).

Let MM be a manifold of bounded geometry. A sequence of compact subsets (Mi)i(M_{i})_{i} of MM will be called a Følner sequence303030In [Roe88a, Definition 6.1] such sequences were called regular. if for each r>0r>0 we have

volBr(Mi)volMii0.\frac{\operatorname{vol}B_{r}(\partial M_{i})}{\operatorname{vol}M_{i}}\stackrel{{\scriptstyle i\to\infty}}{{\longrightarrow}}0.

A Følner sequence (Mi)i(M_{i})_{i} will be called a Følner exhaustion, if (Mi)i(M_{i})_{i} is an exhaustion, i.e., M1M2M_{1}\subset M_{2}\subset\ldots and iMi=M\bigcup_{i}M_{i}=M.

Note that if MM admits a Følner sequence, then it is always possible to construct a Følner exhaustion for MM (the author did this construction in its full glory in his thesis [Eng14, Lemma 2.38]).

For example, Euclidean space m\mathbb{R}^{m} is amenable, but hyperbolic space m2\mathbb{H}^{m\geq 2} is not. Furthermore, if MM has subexponential volume growth at x0Mx_{0}\in M,313131This means that for all p>0p>0 we have eprvol(Br(x0))r0e^{-pr}\operatorname{vol}(B_{r}(x_{0}))\xrightarrow{r\to\infty}0. then MM is amenable (this is proved in [Roe88a, Proposition 6.2]; in this case a Følner exhaustion for MM is given by (Brj(x0))j\big{(}B_{r_{j}}(x_{0})\big{)}_{j\in\mathbb{N}} for suitable rjr_{j}\to\infty). Note that the converse to this last statement is wrong, i.e., there are examples of amenable spaces with exponential volume growth. Further examples of amenable manifolds arise from the theorem that the universal covering M~\widetilde{M} of a compact manifold MM is amenable (if equipped with the pull-back metric) if and only if the fundamental group π1(M)\pi_{1}(M) is amenable (this is proved in [Bro81]).

Let MmM^{m} be a connected and oriented manifold of bounded geometry. Then there is a duality isomorphism Hb,dRm(M)H0uf(M;)H_{b,\mathrm{dR}}^{m}(M)\cong H_{0}^{\mathrm{uf}}(M;\mathbb{R}), where the latter denotes the uniformly finite homology of Block and Weinberger. This isomorphism is mentioned in the remark at the end of Section 3 in [BW92] and proved explicitely in [Why01, Lemma 2.2].323232Alternatively, we could use the Poincaré duality isomorphism Hb,dRi(M)Hmi(M;)H_{b,\mathrm{dR}}^{i}(M)\cong H_{m-i}^{\infty}(M;\mathbb{R}) which is proved in [AB98, Theorem 4], where Hmi(M;)H_{m-i}^{\infty}(M;\mathbb{R}) denotes simplicial LL^{\infty}-homology and MM is triangulated according to Theorem 11, and then use the fact that H0(M;)H0uf(M;)H_{0}^{\infty}(M;\mathbb{R})\cong H_{0}^{\mathrm{uf}}(M;\mathbb{R}) under this triangulation (for this we need the assumption that MM is connected). Since we have the characterization [BW92, Theorem 3.1] of amenability stating that MM is amenable if and only if H0uf(M)0H_{0}^{\mathrm{uf}}(M)\not=0, we therefore also have a characterization of it via bounded de Rham cohomology. We are going to discuss this now a bit more closely.

First we introduce the following notions:

Definition 10 (Closed at infinity, [Sul76, Definition II.5]).

A Riemannian manifold MM is called closed at infinity if for every function ff on MM with 0<C1<f<C0<C^{-1}<f<C for some C>0C>0, we have [fdM]0Hb,dRm(M)[f\cdot dM]\not=0\in H_{b,\mathrm{dR}}^{m}(M) (where dMdM denotes the volume form of MM and m=dimMm=\dim M).

Definition 11 (Fundamental classes, [Roe88a, Definition 3.3]).

A fundamental class for the manifold MM is a positive linear functional θ:Ωbm(M)\theta\colon\Omega^{m}_{b}(M)\to\mathbb{R} such that θ(dM)0\theta(dM)\not=0 and θd=0\theta\circ d=0.

If we are given a Følner sequence for MM, we can construct a fundamental class for MM out of it; this is done in [Roe88a, Propositions 6.4 & 6.5].333333If (Mi)i(M_{i})_{i} is a Følner sequence, then the linear functionals θi(α):=1volMiMiα\theta_{i}(\alpha):=\frac{1}{\operatorname{vol}M_{i}}\int_{M_{i}}\alpha are elements of the dual of Ωbm(M)\Omega_{b}^{m}(M) and have operator norm =1=1. Now take θ\theta as a weak- limit point of (θi)i(\theta_{i})_{i}. The Følner condition for (Mi)i(M_{i})_{i} is needed to show that θ\theta vanishes on boundaries. But admitting a fundamental class implies that MM is closed at infinity.343434Just use the positivity of the fundamental class θ\theta: θ(fdM)θ(C1dM)=C1θ(dM)0\theta(f\cdot dM)\geq\theta(C^{-1}\cdot dM)=C^{-1}\cdot\theta(dM)\not=0. This means especially Hb,dRm(M)0H_{b,\mathrm{dR}}^{m}(M)\not=0. But since this is isomorphic to H0uf(M;)H_{0}^{\mathrm{uf}}(M;\mathbb{R}), we conclude that the latter does also not vanish. So MM is amenable, i.e., admits a Følner sequence, and so we are back at the beginning of our chain. Let us summarize this:

Proposition 12.

Let MM be a connected, orientable manifold of bounded geometry.

Then the following are equivalent:

  • MM admits a Følner sequence,

  • MM admits a fundamental class and

  • MM is closed at infinity.

We know that the universal cover M~\widetilde{M} of a compact manifold MM is amenable if and only if π1(M)\pi_{1}(M) is amenable. If this is the case, then we may construct fundamental classes that respect the structure of M~\widetilde{M} as a covering space:

Proposition 13 ([Roe88a, Proposition 6.6]).

Let MM be a compact Riemannian manifold, denote by M~\widetilde{M} its universal cover equipped with the pull-back metric, and let π1(M)\pi_{1}(M) be amenable.

Then M~\widetilde{M} admits a fundamental class θ\theta with the property

θ(πα)=Mα\theta(\pi^{\ast}\alpha)=\int_{M}\alpha

for every top-dimensional form α\alpha on MM and where π:M~M\pi\colon\widetilde{M}\to M is the covering projection.

At last, let us state just for the sake of completeness the relation of amenability to the linear isoparametric inequality.

Proposition 14 ([Gro81b, Subsection 4.1]).

Let MM be a connected and orientable manifold of bounded geometry.

Then MM is not amenable if and only if vol(R)Cvol(R)\operatorname{vol}(R)\leq C\cdot\operatorname{vol}(\partial R) for all RMR\subset M and a fixed constant C>0C>0.

We can also detect amenability of MM using the KK-theory of the uniform Roe algebra Cu(Γ)C_{u}^{\ast}(\Gamma) of a discretization ΓM\Gamma\subset M.353535A discretization ΓM\Gamma\subset M is a uniformly discrete subset such that there exists a c>0c>0 with Nc(Γ)=MN_{c}(\Gamma)=M, where Nc(Γ)N_{c}(\Gamma) denotes the neighbourhood of distance cc around Γ\Gamma. Recall that one possible definition for the uniform Roe algebra Cu(Γ)C_{u}^{\ast}(\Gamma) is the norm closure of the -algebra of all finite propagation operators in 𝔅(2(Γ))\mathfrak{B}(\ell^{2}(\Gamma)) with uniformly bounded coefficients.

Proposition 15 ([Ele97]).

Let MM be a manifold of bounded geometry and let ΓM\Gamma\subset M be a discretization.

Then MM is amenable if and only if [1][0]K0(Cu(Γ))[1]\not=[0]\in K_{0}(C_{u}^{\ast}(\Gamma)), where [1]K0(Cu(Γ))[1]\in K_{0}(C_{u}^{\ast}(\Gamma)) is a certain distinguished class.

The reason why we stated the above proposition is that it introduces functionals on K0(Cu(Γ))K_{0}(C_{u}^{\ast}(\Gamma)) associated to Følner sequences that we will need in the definition of our index pairings. So let us recall Elek’s argument: Let (Γi)i(\Gamma_{i})_{i} be a Følner sequence in Γ\Gamma363636This means that each Γi\Gamma_{i} is finite and for every r>0r>0 we have #rΓi#Γii0\frac{\#\partial_{r}\Gamma_{i}}{\#\Gamma_{i}}\xrightarrow{i\to\infty}0, where rΓi:={γΓ:d(γ,Γi)<r and d(γ,ΓΓi)<r}\partial_{r}\Gamma_{i}:=\{\gamma\in\Gamma\colon d(\gamma,\Gamma_{i})<r\text{ and }d(\gamma,\Gamma-\Gamma_{i})<r\} and the distance is computed in MM (which makes sense since ΓM\Gamma\subset M). and let TCu(Γ)T\in C_{u}^{\ast}(\Gamma). Then we define a bounded sequence indexed by ii by 1#ΓiγΓiT(γ,γ)\frac{1}{\#\Gamma_{i}}\sum_{\gamma\in\Gamma_{i}}T(\gamma,\gamma). Choosing a linear functional τ()\tau\in(\ell^{\infty})^{\ast} associated to a free ultrafilter on \mathbb{N}373737That is, if we evaluate τ\tau on a bounded sequence, we get the limit of some convergent subsequence. we get a linear functional θ\theta on Cu(Γ)C_{u}^{\ast}(\Gamma). The Følner condition for (Γi)i(\Gamma_{i})_{i} is needed to show that θ\theta is a trace, i.e., descends to K0(Cu(Γ))K_{0}(C_{u}^{\ast}(\Gamma)). Then θ([1])=1\theta([1])=1 and θ([0])=0\theta([0])=0 for the distinguished classes [1],[0]K0(Cu(Γ))[1],[0]\in K_{0}(C_{u}^{\ast}(\Gamma)).

Let us finally come to the definition of the index pairings that we are interested in.

Definition 16.

Let MM be a manifold of bounded geometry, (Mi)i(M_{i})_{i} a Følner sequence for MM and let τ()\tau\in(\ell^{\infty})^{\ast} a linear functional associated to a free ultrafilter on \mathbb{N}. Denote the resulting functional on K0(Cu(Γ))K_{0}(C_{u}^{\ast}(\Gamma)) by θ\theta, where ΓM\Gamma\subset M is a discretization.383838Note that here we first have to construct from the Følner sequence (Mi)i(M_{i})_{i} for MM a corresponding Følner sequence (Γi)i(\Gamma_{i})_{i} for Γ\Gamma.

Then we define for p=0,1p=0,1 an index pairing

,θ:Kup(M)Kpu(M)\langle-,-\rangle_{\theta}\colon K^{p}_{u}(M)\otimes K_{p}^{u}(M)\to\mathbb{R}

by the formula

[x],[y]θ:=θ(μu([x][y])),\langle[x],[y]\rangle_{\theta}:=\theta\big{(}\mu_{u}([x]\cap[y])\big{)},

where μu:Ku(M)K(Cu(Γ))\mu_{u}\colon K_{\ast}^{u}(M)\to K_{\ast}(C_{u}^{\ast}(\Gamma)) denotes the rough assembly map (see Špakula [Špa09] or [Eng15a, Section 3.5]).

If PP is a symmetric and elliptic, graded uniform pseudodifferential operator acting on a graded vector bundle EE, then there is a nice way of computing the above index pairing of PP with the trivial bundle []Ku0(M)[\mathbb{C}]\in K^{0}_{u}(M): recall from Corollary 18 that if f𝒮()f\in\mathcal{S}(\mathbb{R}) is a Schwartz function, then f(P)f(P) is a quasilocal smoothing operator. Hence it has a uniformly bounded integral kernel kf(P)(x,y)Cb(EE)k_{f(P)}(x,y)\in C_{b}^{\infty}(E\boxtimes E^{\ast}). Now we choose an even function f𝒮()f\in\mathcal{S}(\mathbb{R}) with f(0)=1f(0)=1 and get a bounded sequence

1volMiMitrskf(P)(x,x)𝑑M(x),\frac{1}{\operatorname{vol}M_{i}}\int_{M_{i}}\operatorname{tr}_{s}k_{f(P)}(x,x)\ dM(x),

where trs\operatorname{tr}_{s} denotes the super trace (recall that EE is graded), on which we may evaluate τ\tau. This will coincide with the pairing [],Pθ\langle[\mathbb{C}],P\rangle_{\theta} and is exactly the analytic index that was defined by Roe in [Roe88a] for Dirac operators. For details why this will coincide with [],Pθ\langle[\mathbb{C}],P\rangle_{\theta} the reader may consult, e.g., the author’s Ph.D. thesis [Eng14, Section 2.8].

Let us now define the pairing between uniform de Rham cohomology and uniform de Rham homology. So let βCb(Ωp(M))\beta\in C_{b}^{\infty}(\Omega^{p}(M)) and CΩpu(M)C\in\Omega_{p}^{u}(M), fix an ϵ>0\epsilon>0 and choose for every MiMM_{i}\subset M from a Følner sequence for MM a smooth cut-off function φiCc(M)\varphi_{i}\in C_{c}^{\infty}(M) with φi|Mi1\varphi_{i}|_{M_{i}}\equiv 1, suppφiBϵ(Mi)\operatorname{supp}\varphi_{i}\subset B_{\epsilon}(M_{i}) and such that for all k0k\in\mathbb{N}_{0} the derivatives kφi\nabla^{k}\varphi_{i} are bounded in sup-norm uniformly in the index ii. Then φiβW,1(Ωp(M))\varphi_{i}\beta\in W^{\infty,1}(\Omega^{p}(M)) and therefore we may evaluate CC on it. The sequence 1volMiC(φiβ)\frac{1}{\operatorname{vol}M_{i}}C(\varphi_{i}\beta) will be bounded and so we may apply τ()\tau\in(\ell^{\infty})^{\ast} to it. Due to the Følner condition for (Mi)i(M_{i})_{i} this pairing will descend to (co-)homology classes.

Definition 17.

Let MM be a manifold of bounded geometry, let (Mi)i(M_{i})_{i} be a Følner sequence for MM and let τ()\tau\in(\ell^{\infty})^{\ast} a linear functional associated to a free ultrafilter on \mathbb{N}.

For every p0p\in\mathbb{N}_{0} we define a pairing

,(Mi)i,τ:Hu,dRp(M)Hpu,dR(M)\langle-,-\rangle_{(M_{i})_{i},\tau}\colon H_{u,\mathrm{dR}}^{p}(M)\otimes H^{u,\mathrm{dR}}_{p}(M)\to\mathbb{C}

by evaluating τ\tau on the sequence 1volMiC(φiβ)\frac{1}{\operatorname{vol}M_{i}}C(\varphi_{i}\beta), where βHu,dRp(M)\beta\in H_{u,\mathrm{dR}}^{p}(M), CHpu,dR(M)C\in H^{u,\mathrm{dR}}_{p}(M) and the cut-off functions φi\varphi_{i} are chosen as above.

Note that this pairing is, similar to the pairing from Corollary 7, continuous against the topologies on Hu,dR(M)H_{u,\mathrm{dR}}^{\ast}(M) and on Hu,dR(M)H^{u,\mathrm{dR}}_{\ast}(M).

Recall that in the usual case of compact manifolds the index pairing for KK-theory and KK-homology is compatible with the Chern-Connes character, i.e., [x],[y]=ch([x]),ch([y])\langle[x],[y]\rangle=\langle\operatorname{ch}([x]),\operatorname{ch}([y])\rangle for [x]K(M)[x]\in K^{\ast}(M) and [y]K(M)[y]\in K_{\ast}(M). The same also holds in our case here.

Lemma 18.

Denote by ch:Ku(M)Hu,dR(M)\operatorname{ch}\colon K_{u}^{\ast}(M)\to H_{u,\mathrm{dR}}^{\ast}(M) the Chern character on uniform KK-theory and by (αch):Ku(M)Hu,dR(M)(\alpha_{\ast}\circ\operatorname{ch}^{\ast})\colon K_{\ast}^{u}(M)\to H^{u,\mathrm{dR}}_{\ast}(M) the one on uniform KK-homology.

Then we have

[x],[y]θ=ch([x]),(αch)([y])(Mi)i,τ\big{\langle}[x],[y]\big{\rangle}_{\theta}=\big{\langle}\operatorname{ch}([x]),(\alpha_{\ast}\circ\operatorname{ch}^{\ast})([y])\big{\rangle}_{(M_{i})_{i},\tau}

for all [x]Kup(M)[x]\in K_{u}^{p}(M) and [y]Kpu(M)[y]\in K^{u}_{p}(M).

The last thing that we need is the compatibility of the index pairings with cup and cap products. This is clear by definition for the index pairing for uniform KK-theory with uniform KK-homology, and for the pairing for uniform de Rham cohomology with uniform de Rham homology it is stated in the following lemma.

Lemma 19.

Let [β]Hu,dRp(M)[\beta]\in H_{u,\mathrm{dR}}^{p}(M), [γ]Hu,dRq(M)[\gamma]\in H_{u,\mathrm{dR}}^{q}(M) and [C]Hp+qu,dR(M)[C]\in H^{u,\mathrm{dR}}_{p+q}(M). Then we have

[β][γ],[C](Mi)i,τ=[β],[γ][C](Mi)i,τ.\langle[\beta]\wedge[\gamma],[C]\rangle_{(M_{i})_{i},\tau}=\langle[\beta],[\gamma]\cap[C]\rangle_{(M_{i})_{i},\tau}.

So combining the above two lemmas together with the results of Section 4.1 we finally arrive at our desired index theorem for amenable manifolds which generalizes Roe’s index theorem from [Roe88a] from graded generalized Dirac operators to arbitrarily graded, symmetric, elliptic uniform pseudodifferential operators.

Corollary 20.

Let MM be a manifold of bounded geometry and without boundary, let (Mi)i(M_{i})_{i} be a Følner sequence for MM and let τ()\tau\in(\ell^{\infty})^{\ast} be a linear functional associated to a free ultrafilter on \mathbb{N}. Denote the from the choice of Følner sequence and functional τ\tau resulting functional on K0(Cu(Γ))K_{0}(C_{u}^{\ast}(\Gamma)) by θ\theta, where ΓM\Gamma\subset M is a discretization.

Then for both p{0,1}p\in\{0,1\}, every [P]Kpu(M)[P]\in K_{p}^{u}(M) for PP a pp-graded, symmetric, elliptic uniform pseudodifferential operator over MM, and every uKup(M)u\in K_{u}^{p}(M) we have

u,[P]θ=ch(u)ind(P),[M](Mi)i,τ.\langle u,[P]\rangle_{\theta}=\langle\operatorname{ch}(u)\wedge\operatorname{ind}(P),[M]\rangle_{(M_{i})_{i},\tau}.
Remark 21.

The right hand side of the formula in the above corollary reads as

τ(1volMiMich(u)ind(P))\tau\Big{(}\frac{1}{\operatorname{vol}M_{i}}\int_{M_{i}}\operatorname{ch}(u)\wedge\operatorname{ind}(P)\Big{)}

and this is continuous against the sup-seminorm on Hb,dRm(M)H_{b,\mathrm{dR}}^{m}(M) with m=dim(M)m=\dim(M), i.e.,

u,[P]θch(u)ind(P).\langle u,[P]\rangle_{\theta}\leq\|\operatorname{ch}(u)\wedge\operatorname{ind}(P)\|_{\infty}.

So, again as in Remark 8, we see that with this pairing we can not detect operators PP whose index class ind(P)Hb,dR(M)\operatorname{ind}(P)\in H_{b,\mathrm{dR}}^{\ast}(M) has sup-seminorm =0=0 in every degree.

Note that it seems that from the results in [Sul76, Part II.§4] it follows that every element in Hb,dRm(M)H_{b,\mathrm{dR}}^{m}(M) of non-zero sup-seminorm may be detected by a Følner sequence (i.e., the dual space H¯b,dR(M)\overline{H}_{b,\mathrm{dR}}^{\ast}(M) of the reduced bounded de Rham cohomology393939Reduced bounded de Rham cohomology is defined as H¯b,dR(M):=Hb,dR(M)/[0]¯\overline{H}_{b,\mathrm{dR}}^{\ast}(M):=H_{b,\mathrm{dR}}^{\ast}(M)/\overline{[0]}, i.e., as the Hausdorffication of bounded de Rham cohomology. is spanned by Følner sequences). So the difference between the statement of the above corollary and Theorem 3 lies, at least in top-degree, exactly in the fact that Theorem 3 also encompasses all the elements of sup-seminorm =0=0.

Example 4.6.

Let us discuss quickly an example that shows that we indeed may lose information by passing to the reduced bounded de Rham cohomology groups. Roe showed in [Roe88b, Proposition 3.2] that if MmM^{m} is a connected spin manifold of bounded geometry, then A^(M),[M],=0\langle\hat{A}(M),[M]\rangle_{-,-}=0 for any choice of Følner sequence and suitable functional τ\tau if MM has non-negative scalar curvature, and later Whyte showed in [Why01, Theorem 2.3] that A^(M)=[0]Hb,dRm(M)\hat{A}(M)=[0]\in H_{b,\mathrm{dR}}^{m}(M) under these assumptions. So any connected spin manifold MM of bounded geometry with A^(M)[0]Hb,dRm(M)\hat{A}(M)\not=[0]\in H_{b,\mathrm{dR}}^{m}(M) but A^(M)=[0]H¯b,dRm(M)\hat{A}(M)=[0]\in\overline{H}_{b,\mathrm{dR}}^{m}(M) can not have non-negative scalar curvature, but this is not detected by the reduced group. In [Why01] it is also shown how one can construct examples of manifolds whose A^\hat{A}-genus vanishes in the reduced but not in the unreduced group.

5 Final remarks and open questions

In this final section we will collect some open questions arising out of the present paper.

In Theorem 13 we constructed the uniform Chern character ch:Ku(M)Hu,dR(M)\operatorname{ch}\colon K^{\ast}_{u}(M)\to H_{u,\mathrm{dR}}^{\ast}(M) for manifolds of bounded geometry by using Chern–Weil theory. In the case of compact spaces there exist definitions of the Chern character which make sense on any finite CW-complex, i.e., are not restricted to smooth manifolds. Now in our situation, uniform KK-theory is defined on all metric spaces and not just on manifolds, and since uniform de Rham cohomology is isomorphic to LL^{\infty}-simplicial cohomology if we triangulate MM as a simplicial complex of bounded geometry using Theorem 11 we can make sense out of it for more general spaces than smooth manifolds. So we arive at the following question:

Question 5.1.

How can we define the uniform Chern characters Ku(L)H(L)K_{u}^{\ast}(L)\to H^{\ast}_{\infty}(L) and Ku(L)H(L)K_{\ast}^{u}(L)\to H_{\ast}^{\infty}(L) for a simplicial complex LL of bounded geometry equipped with the metric derived from barycentric coordinates?

One approach might be to consider something like uniform (co-)homology theories: we could try to put a model structure on the category of uniform spaces modeling uniform homotopy theory and then try to show that, e.g., uniform KK-theory is nothing more but uniform homotopy classes of uniform maps into some uniform version of the KK-theory spectrum. Then the uniform Chern characters should be coming from transformations of uniform spectra and the above Question 5.1 would be solved.

In the compact case there is a generalization of the Atiyah–Singer index theorem to manifolds with boundary involving the η\eta-invariant. This version of the index theorem for compact manifolds with boundary is called the Atiyah–Patodi–Singer index theorem and was introduced in [APS75]. Of course the question whether such a theorem may also be proven in the non-compact case immediately arises.

Question 5.2.

Is there a version of the, e.g., global index theorem for amenable manifolds, for manifolds of bounded geometry and with boundary? What would be the corresponding generalization of the η\eta-invariant?

Note that even if we just stick to Dirac operators (i.e., if we don’t try to work with uniform pseudodifferential operators) the non-compact case (of bounded geometry) is of course technically much more demanding than the compact case. Results have been achieved by Ballmann–Bär [BB12] and Große–Nakad [GN14].

Some version of pseudodifferential operators on certain non-compact manifolds with boundary was investigated by Schrohe [Sch99]. Furthermore, there is also the work of Ammann–Lauter–Nistor [ALN07] and one should also ask to which extend it coincides, respectively differs from the one asked for here.

A proof of the index theorem for manifolds with boundary was given by Melrose in [Mel93]. He invented the bb-calculus, a calculus for pseudodifferential operators on manifolds with boundary, and derived the Atiyah–Patodi–Singer index theorem from it via the heat kernel approach. Therefore it would be desirable to extend his bb-calculus to open manifolds with boundary (similarly as we extended the calculus of pseudodifferential operators to open manifolds) and then prove a version of the Atiyah–Patodi–Singer index theorem on manifolds with boundary and of bounded geometry.

Question 5.3.

Can one reasonably extend the bb-calculus of Melrose to manifolds of bounded geometry and with boundary, and then prove version of large scale index theorems for manifolds with boundary?

In the case of compact manifolds with boundary Piazza [Pia91] also treated various parts of the index theorem of Atiyah–Patodi–Singer using the bb-calculus. A connection between uniform pseudodifferential operators on manifolds of bounded geometry and the bb-calculus was established by Albin [Alb08].

Another direction in which one could work is to look at higher ρ\rho-invariants: in the last years a lot of progress was made in relation to “mapping sugery to analysis”, respectively mapping the Stolz positive scalar curvature exact sequence to analysis. Without going through all the results that have been achieved, let us mention one particular application [XY14, Corollary 4.5] that seems worth reshaping into our setting: if Γ\Gamma acts properly and cocompactly on MM and hh is a Riemannian metric on M\partial M having positive scalar curvature, then it is not possible to extend hh to a complete, Γ\Gamma-invariant Riemannian metric on MM of positive scalar curvature if ρ(DM,h)0K(CL,0(M)Γ)\rho(D_{\partial M},h)\not=0\in K_{\ast}(C^{\ast}_{L,0}(\partial M)^{\Gamma}).

Question 5.4.

Can one prove a large scale version of the delocalized APS-index theorem as in [PS15, Theorem 1.22] and use this to prove an analogue of the above mentioned result [XY14, Corollary 4.5]?

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