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0002020 Mathematics Subject Classification. Primary 51F30; Secondary 20F65, 58B34.

Boundary of free products of metric spaces

Tomohiro Fukaya  and  Takumi Matsuka Tomohiro Fukaya Department of Mathematics and Information Sciences, Tokyo Metropolitan University, Minami-osawa Hachioji, Tokyo, 192-0397, Japan tmhr@tmu.ac.jp Takumi Matsuka Department of Mathematics and Information Sciences, Tokyo Metropolitan University, Minami-osawa Hachioji, Tokyo, 192-0397, Japan takumi.matsuka1@gmail.com
Abstract.

In this paper, we compute (co)homologies of ideal boundaries of free products of geodesic coarsely convex spaces in terms of those of each of the components. The (co)homology theories we consider are, KK-theory, Alexander-Spanier cohomology, KK-homology, and Steenrod homology. These computations led to the computation of KK-theory of the Roe algebra of free products of geodesic coarsely convex spaces via the coarse Baum–Connes conjecture.

Key words and phrases:
coarsely convex spaces, ideal boundary, cohomology,
The first author was supported by JSPS KAKENHI Grant number JP19K03471. The second author was supported by JST, the establishment of university fellowships towards the creation of science technology innovations, Grant number JPMJFS2139.

1. Introduction

Coarsely convex spaces are coarse geometric analogues of simply connected Riemannian manifolds of nonpositive sectional curvature introduced by Oguni and the first author. In [11], ideal boundaries of coarsely convex spaces are constructed, and it was shown that coarsely convex spaces are coarsely homotopy equivalent to the open cones over their ideal boundaries. Combining with Higson-Roe’s work on the coarse Baum-Connes conjecture for open cones [16], it was shown that the coarse Baum-Connes conjecture holds for proper coarsely convex spaces [11].

The class of coarsely convex spaces includes geodesic Gromov hyperbolic spaces, CAT(0) spaces, Busemann spaces, and systolic complexes [20]. Descombes and Lang [7] showed that proper injective metric spaces admit geodesic convex bicombings. This implies that proper injective metric spaces are coarsely convex. Recently, Chalopin, Chepoi, Genevois, Hirai, and Osajda [6] showed that Helly graphs are coarsely dense in their injective hulls, and these injective hulls are proper. It follows that Helly graphs are coarsely convex.

In [9], we constructed free products of metric spaces, which generalizes the construction by Bridson-Haefliger [3, Theorem II.11.18]. We showed that free products of geodesic coarsely convex spaces are geodesic coarsely convex. In [10], the authors introduced trees of spaces, which are generalizations of free products of metric spaces. They showed that if each of the components of a tree of spaces is geodesic coarsely convex, then the tree of spaces is geodesic coarsely convex. This generalized the main result of [9] for trees of spaces.

In this paper, we study the topology of ideal boundaries of trees of spaces whose components are coarsely convex. For this purpose, we introduce augmented spaces of trees of spaces. We determine the topological type of the ideal boundaries of augmented spaces. Then we compute KK-theory, Alexander-Spanier cohomology, and KK-homology of the ideal boundaries of the trees of spaces in terms of ideal boundaries of augmented spaces, and ideal boundaries of the components of the trees of spaces.

By applying Theorems 9.3 and 9.5 for free products, we have the following.

Theorem 1.1.

Let XX and YY be proper geodesic coarsely convex spaces with nets. Suppose that the net of XX and that of YY are coarsely dense in XX and YY, respectively, and, both XX and YY are unbounded. Let XYX*Y be the free product of XX and YY. Let X\partial X, Y\partial Y, and (XY),\partial(X*Y), denote the ideal boundaries of XX, YY, and XYX*Y, respectively. Let 𝒞\mathcal{C} denote the Cantor space.

Let M=(Mn)nM^{*}=(M^{n})_{n\in\mathbb{N}} be the KK-theory or the Alexander-Spanier cohomology. Then,

M~p((XY))\displaystyle\tilde{M}^{p}(\partial(X*Y)) M~p(𝒞)M~p(X)M~p(Y)\displaystyle\cong\tilde{M}^{p}(\mathcal{C})\oplus\bigoplus_{\mathbb{N}}\tilde{M}^{p}(\partial X)\oplus\bigoplus_{\mathbb{N}}\tilde{M}^{p}(\partial Y)

Let M=(Mn)nM_{*}=(M_{n})_{n\in\mathbb{N}} be the KK-homology or the Steenrod homology. Then,

M~p((XY))\displaystyle\tilde{M}_{p}(\partial(X*Y)) M~p(𝒞)×M~p(X)×M~p(Y).\displaystyle\cong\tilde{M}_{p}(\mathcal{C})\times\prod_{\mathbb{N}}\tilde{M}_{p}(\partial X)\times\prod_{\mathbb{N}}\tilde{M}_{p}(\partial Y).

Here M~p\tilde{M}_{p} and M~p\tilde{M}^{p} denote the reduced (co)homology corresponding to MpM_{p} and MpM^{p}.

Let YY be a metric space. We denote by C(Y)C^{*}(Y) the Roe algebra of YY. The coarse Baum-Connes conjecture states that the KK-theory of the Roe algebra C(Y)C^{*}(Y) is isomorphic to the coarse KK-homology KX(Y)KX_{*}(Y) of YY. As mentioned above, it is proved in [11] that the coarse Baum-Connes conjecture holds for proper coarsely convex spaces. It is also proved that the coarse KK-homology of a coarsely convex space YY is isomorphic to the reduced KK-homology of the ideal boundary Y\partial Y with sifting the degree by one [11, Theorem 6.7.]. Therefore we can compute the KK-theory of the Roe algebra of a free product coarsely convex spaces as follows.

For a CC^{*}-algebra AA, we denote by Kp(A)K_{p}(A) the operator KK-theory of AA. We denote by K~p()\tilde{K}_{p}(-) the reduced KK-homology.

Theorem 1.2.

Let XX and YY be proper geodesic coarsely convex spaces with nets. Suppose that the net of XX and that of YY are coarsely dense in XX and YY, respectively, and, both XX and YY are unbounded. We have

Kp(C(XY))\displaystyle K_{p}(C^{*}(X*Y)) K~p1(𝒞)×K~p1(X)×K~p1(Y).\displaystyle\cong\tilde{K}_{p-1}(\mathcal{C})\times\prod_{\mathbb{N}}\tilde{K}_{p-1}(\partial X)\times\prod_{\mathbb{N}}\tilde{K}_{p-1}(\partial Y).
Corollary 1.3.

Let XX and YY be proper geodesic coarsely convex spaces with nets satisfying the condition of Theorem 1.2. We have

Kp(C(XY))\displaystyle K_{p}(C^{*}(X*Y)) K~p1(𝒞)×Kp(C(X))×Kp(C(Y)).\displaystyle\cong\tilde{K}_{p-1}(\mathcal{C})\times\prod_{\mathbb{N}}K_{p}(C^{*}(X))\times\prod_{\mathbb{N}}K_{p}(C^{*}(Y)).

It might be interesting to compare Corollary 1.3 with a formula for KK-theories of the group CC^{*} algebras of free products of groups [2, 10.11.11 (f) to (h)].

We also study the topological dimensions of the ideal boundaries of trees of spaces. Applying Theorem 12.4 for free products of metric spaces, we obtain a formula of the dimension.

Theorem 1.4.

Let XX and YY be geodesic coarsely convex spaces with nets.

dim((XY))=max{dimX,dimY}.\displaystyle\mathop{\mathrm{dim}}\nolimits(\partial(X*Y))=\max\{\mathop{\mathrm{dim}}\nolimits\partial X,\mathop{\mathrm{dim}}\nolimits\partial Y\}.

We remark that Theorem 1.4 is an analogue of the formula for the cohomological dimensions of the free products of groups. Namely, in the setting of Theorem 1.4, if we assume that both XX and YY admits geometric action by group GG and HH, respectively, and both GG and HH admits a finite model for the classifying space BGBG and BHBH, respectively, then the above formula follows from a well-known formula on the cohomological dimensions of free products of groups. See Section 12.2 for details.

1.1. Outline

In Section 2, based on the work of Groves and Manning, we introduce combinatorial horoballs for metric spaces with lattices, and study the shape of geodesics in them.

In Sections 3, 4 and 5, we review the coarsely convex bicombings and the construction of ideal boundaries. In this paper, we only deal with geodesic coarsely convex space, so in Section 5, we restrict results in previous sections to geodesic coarsely convex bicombings, and we improve some of them.

In Section 6, we prepare some technical lemmata to show the continuity of certain retractions on ideal boundaries, which play key roles in the computations of (co)homologies.

In Sections 7 and 8, we introduce trees of spaces and augmented spaces. We construct geodesic coarsely convex bicombings on them assuming that each component admits such bicombings.

In Section 9, we compute (co)homologies of ideal boundaries of trees of geodesic coarsely convex spaces by using Mayer-Vietoris exact sequences. Key tools are retractions on ideal boundaries. We give proofs of Theorems 1.1, 1.2 and 9.7.

In Section 10, we construct the retractions used in Section 9 and show that they are continuous. Here we use the results in Section 6.

In Section 11, we study the topological type of the ideal boundary of the augmented spaces. We show (Theorem 11.4) that under certain conditions, the ideal boundaries of the augmented spaces are homeomorphic to the Cantor space.

In Section 12, we show a formula for the topological dimensions of the ideal boundaries of trees of geodesic coarsely convex spaces in terms of the dimensions of each component. In Section 12.2, we compare these results with a well known formula for the cohomological dimensions of the free products of groups.

2. Combinatorial and metric horoballs

All materials in this section are slight modifications of the work of Groves and Manning [15] on the combinatorial horoballs.

In the rest of this section, we assume that XX is a geodesic metric space.

Definition 2.1.

Let (X,dX)(X,d_{X}) be a metric space and AXA\subset X. Let C0C\geq 0.

  1. (1)

    The subset AA is CC-discrete if for all a,aAa,a^{\prime}\in A with aaa\neq a^{\prime}, we have dZ(a,a)Cd_{Z}(a,a^{\prime})\geq C.

  2. (2)

    The subset AA is CC-dense if for all xXx\in X, there exists aAa\in A such that dZ(x,a)Cd_{Z}(x,a)\leq C.

Remark 2.2.

A maximal CC-discrete subset AXA\subset X is 2C2C-dense.

Definition 2.3.

A metric space with a lattice is a pair (X,X(0))(X,X^{(0)}) of metric space (X,dX)(X,d_{X}) and 1-discrete 2-dense subset X(0)XX^{(0)}\subset X. We call X(0)X^{(0)} the lattice of XX.

Groves and Manning defined an augmented space and introduced an equivalent definition of relatively hyperbolic groups [15]. The augmented space is constructed by gluing a ”combinatorial horoballs” based on each P𝒫P\in\mathcal{P} onto the Cayley graph of GG. They defined that GG is hyperbolic relative to 𝒫\mathcal{P} if the augmented space is hyperbolic.

The construction presented here is closely modeled on Groves–Manning’s combinatorial horoballs. They constructed horoballs based on an arbitrary connected graph, and showed that such a horoball is always δ\delta–hyperbolic. A minor modification of the Groves–Manning construction produces connected horoballs based on any metric space.

Definition 2.4.

Let (X(0),dX)(X^{(0)},d_{X}) be a 1-discrete metric space. A combinatorial horoball 𝖼𝗈𝗆𝖻(X(0))\mathcal{H}_{\mathsf{comb}}(X^{(0)}) is a graph with a set of vertices 𝖼𝗈𝗆𝖻(X(0))(0)\mathcal{H}_{\mathsf{comb}}(X^{(0)})^{(0)} and a set of edges 𝖼𝗈𝗆𝖻(X(0))(1)\mathcal{H}_{\mathsf{comb}}(X^{(0)})^{(1)} defined as follows:

  1. (1)

    𝖼𝗈𝗆𝖻(X(0))(0)X(0)×({0})\mathcal{H}_{\mathsf{comb}}(X^{(0)})^{(0)}\coloneqq X^{(0)}\times(\mathbb{N}\cup\{0\}).

  2. (2)

    𝖼𝗈𝗆𝖻(X(0))(1)\mathcal{H}_{\mathsf{comb}}(X^{(0)})^{(1)} contains the following two types of edges:

    1. (a)

      For each xX(0)x\in X^{(0)} and l{0}l\in\mathbb{N}\cup\{0\}, there exists a vertical edge connecting (x,l)(x,l) and (x,l+1)(x,l+1).

    2. (b)

      For each x,yX(0)x,y\in X^{(0)} and ll\in\mathbb{N}, if 0<dX(x,y)2l0<d_{X}(x,y)\leq 2^{l} holds for some ll\in\mathbb{N}, there exists a horizontal edge connecting (x,l)(x,l) and (y,l)(y,l).

We endow (X(0),dX)(X^{(0)},d_{X}) with a graph metric such that each edge has length one, and we consider (X(0),dX)(X^{(0)},d_{X}) as a geodesic space.

Let 𝖼𝗈𝗆𝖻(X(0))\mathcal{H}_{\mathsf{comb}}(X^{(0)}) be a combinatorial horoball. A horizontal segment is a path consisting only of horizontal edges. A vertical segment is a path consisting only of vertical edges. Each x𝖼𝗈𝗆𝖻(X(0))(0)x\in\mathcal{H}_{\mathsf{comb}}(X^{(0)})^{(0)} can be identified with x=(x0,l)x=(x_{0},l), where x0X(0)x_{0}\in X^{(0)} and l{0}l\in\mathbb{N}\cup\{0\}. We say that the depth of xx is ll, denoted by D(x)=lD(x)=l. Moreover, let pp be a horizontal segment. When the depth of a point on the horizontal segment pp is ll, we say that the depth of the horizontal segment pp is ll, denoted by D(p)=lD(p)=l.

Definition 2.5.

Let (X,X(0))(X,X^{(0)}) be a metric space with a lattice. An metric horoball (X,X(0))\mathcal{H}(X,X^{(0)}) is a quotient space of X𝖼𝗈𝗆𝖻(X(0))X\sqcup\mathcal{H}_{\mathsf{comb}}(X^{(0)}) by the equivalent relation generated by

𝖼𝗈𝗆𝖻(X(0))(0)(x0,0)x0X(0)X\displaystyle\mathcal{H}_{\mathsf{comb}}(X^{(0)})^{(0)}\ni(x_{0},0)\sim x_{0}\in X^{(0)}\subset X

for any x0X(0)x_{0}\in X^{(0)}.

Geodesics in combinatorial horoballs are particularly easy to understand.

Proposition 2.6 ([15], Lemma 3.10).

Let x,y(X,X(0))x,y\in\mathcal{H}(X,X^{(0)}). There exists a geodesic segment on (X,X(0))\mathcal{H}(X,X^{(0)}) from xx to yy which consists of at most two vertical segments and a single horizontal segment of length at most 55. We say that this geodesic segment is a normal geodesic segment, denoted by 𝚗γ(x,y)\mathtt{n}\gamma(x,y). Moreover, for each geodesic segment from xx to yy, denoted by γ(x,y)\gamma(x,y), we have

dH(Im(γ(x,y)),Im(𝚗γ(x,y)))4\displaystyle d_{H}(\mathrm{Im}(\gamma(x,y)),\mathrm{Im}(\mathtt{n}\gamma(x,y)))\leq 4

,where dHd_{H} is the Hausdorff metric on XX.

Proof..

Let γ(x,y)\gamma(x,y) be a geodesic segment from xx to yy. We can put

γ(x,y)=p1p2pn\displaystyle\gamma(x,y)=p_{1}\ast p_{2}\ast\cdots\ast p_{n}

such that for all ii, we have that if pip_{i} is a horizontal segment, then pi+1p_{i+1} is a vertical segment, and if pip_{i} is a vertical segment, then pi+1p_{i+1} is a horizontal segment. We can assume that p1p_{1} and pnp_{n} are vertical segments. Let s(pi)s(p_{i}) be an initial point of pip_{i} and let t(p1)t(p_{1}) be a terminal point of pip_{i}. Note that t(pi)=s(pi+1)t(p_{i})=s(p_{i+1}), s(p1)=xs(p_{1})=x, and t(pn)=yt(p_{n})=y.

First, it is easily shown that there does not exist a vertical segment pp such that D(s(p))>D(t(p))D(s(p))>D(t(p)). We will show that as a consequence of lemmas.

Claim 2.7.

Let DMD_{M} be the maximum depth of horizontal segments which compose γ(x,y)\gamma(x,y). If there exists a horizontal segment pp which composes γ(x,y)\gamma(x,y) such that D(p)<DMD(p)<D_{M}, then the length of pp is 11.

Let pip_{i} be a horizontal segment with D(pi)<DMD(p_{i})<D_{M}. Suppose the length of pip_{i} is 22. Let s(pi)=(xi,D(pi))s(p_{i})=(x_{i},D(p_{i})) and t(pi)=(yi,D(pi))t(p_{i})=(y_{i},D(p_{i})). Note that pi+1p_{i+1} is a vertical segment and t(pi)=s(pi+1)t(p_{i})=s(p_{i+1}). We denote the depth of t(pi+1)t(p_{i+1}) by D1D_{1}. Since D(pi)<D1D(p_{i})<D_{1}, there exists a horizontal edge from (xi,D1)(x_{i},D_{1}) to (yi,D1)(y_{i},D_{1}), denoted by q2q_{2}. Let q1q_{1} be the vertical segment from s(pi)=(xi,D(pi))s(p_{i})=(x_{i},D(p_{i})) to (xi,D1)(x_{i},D_{1}). The path q1q2q_{1}\ast q_{2} is a geodesic segment from s(pi)s(p_{i}) to t(pi+1)t(p_{i+1}). The length of q1q2q_{1}\ast q_{2} is shorter than pipi+1p_{i}\ast p_{i+1}. This is a contradiction.

Claim 2.8.

There does not exist a subgeodesic h1v1h2v2h_{1}\ast v_{1}\ast h_{2}\ast v_{2} such that hih_{i} are horizontal segments and viv_{i} are vertical segments.

Suppose that there exists a subgeodesic h1v1h2v2h_{1}\ast v_{1}\ast h_{2}\ast v_{2} such that hih_{i} are horizontal segments and viv_{i} are vertical segments. Let D(h1)=D1D(h_{1})=D_{1}, D(h2)=D2D(h_{2})=D_{2}, and D(t(v2))=DD(t(v_{2}))=D. By Claim 2.7, the length of h1h_{1} and h2h_{2} are 11. We can put s(h1)=(x1,D1)s(h_{1})=(x_{1},D_{1}), s(h2)=(x2,D2)s(h_{2})=(x_{2},D_{2}), and t(v2)=(x3,D)t(v_{2})=(x_{3},D)

dX(x1,x3)\displaystyle d_{X}(x_{1},x_{3}) dX(x1,x2)+dX(x2,x3)\displaystyle\leq d_{X}(x_{1},x_{2})+d_{X}(x_{2},x_{3})
2D1+2D2\displaystyle\leq 2^{D_{1}}+2^{D_{2}}
2D2+12D.\displaystyle\leq 2^{D_{2}+1}\leq 2^{D}.

Therefore, there exits a horizontal edge q2q_{2} from (x1,D)(x_{1},D) to t(v2)t(v_{2}). Now, we define a path q1q_{1} to be a vertical segment from s(h1)=(x1,D1)s(h_{1})=(x_{1},D_{1}) to (x1,D)(x_{1},D). The length of the path q1q2q_{1}\ast q_{2} is smaller than h1v1h2v2h_{1}\ast v_{1}\ast h_{2}\ast v_{2}. This is a contradiction.

Therefore, a geodesic segment γ(x,y)\gamma(x,y) has the following form:

γ(x,y)=v1h1v2h2v3h3v4,\displaystyle\gamma(x,y)=v_{1}\ast h_{1}\ast v_{2}\ast h_{2}\ast v_{3}\ast h_{3}\ast v_{4},

where viv_{i} are vertical segments and hih_{i} are horizontal segments. Note that h2h_{2} is the highest horizontal segment. By Claim 2.7 and Claim 2.8, we have that the length of hih_{i} is 11 for i{1,3}i\in\{1,3\}. Put s(h1)=(x,D(h1))s(h_{1})=(x,D(h_{1})) and t(h3)=(y,D(h3))t(h_{3})=(y,D(h_{3})). We denote by v1v^{\prime}_{1}, a vertical segment from (x,D(h1))(x,D(h_{1})) to (x,DM)(x,D_{M}). and denote by v2v^{\prime}_{2}, a vertical segment from (y,DM)(y,D_{M}) and t(h3)=(y,D(h3))t(h_{3})=(y,D(h_{3})). There exists a geodesic segment from (x,DM)(x,D_{M}) to (y,DM)(y,D_{M}), denoted by hMh_{M}. We replace h1v2h2v3h3h_{1}\ast v_{2}\ast h_{2}\ast v_{3}\ast h_{3} with v1hMv2v^{\prime}_{1}\ast h_{M}\ast v^{\prime}_{2}. The replaced path is also a geodesic segment from xx to yy. Therefore, we obtain a normal geodesic segment from xx to yy.

For x,y(X,X(0))x,y\in\mathcal{H}(X,X^{(0)}), let 𝚗γ(x,y)=uhv\mathtt{n}\gamma(x,y)=u\ast h\ast v, where uu and vv are vertical segments and hh is a horizontal segment. Finally, we will show that the length of hh is at most 55. Suppose that the length of hh is 66. Let s(h)=(p,D(h))s(h)=(p,D(h)) and t(h)=(q,D(h))t(h)=(q,D(h)). We can connect (p,D(h)+1)(p,D(h)+1) and (q,D(h)+1)(q,D(h)+1) with three horizontal edges. Then, there exists a path of length 55 connecting s(h)s(h) and t(h)t(h). This is the contradiction.

Moreover, for each geodesic segment from xx to yy, denoted by γ(x,y)\gamma(x,y), we have

dH(Im(γ(x,y)),Im(𝚗γ(x,y)))4.\displaystyle d_{H}(\mathrm{Im}(\gamma(x,y)),\mathrm{Im}(\mathtt{n}\gamma(x,y)))\leq 4.

This completes the proof. ∎

Proposition 2.9 ([15]).

(X,X(0))\mathcal{H}(X,X^{(0)}) is a Gromov hyperbolic space.

Proof..

Let x,y,zX(0)x,y,z\in X^{(0)}. We denote by [x,y][x,y], an image of a geodesic segment on (X,X(0))\mathcal{H}(X,X^{(0)}) from xx to yy. Let p1[x,y]p_{1}\in[x,y], p2[y,z]p_{2}\in[y,z], and p3[z,x]p_{3}\in[z,x]. We define

diam{p1,p2,p3}max{dX(pi,pj):ij}.\displaystyle\mathrm{diam}\{p_{1},p_{2},p_{3}\}\coloneqq\max\{d_{X}(p_{i},p_{j})\colon i\neq j\}.

One of the equivalent definitions of Gromov hyperbolicity is that the following quantity

min{diam{p1,p2,p3}:p1[x,y],p2[y,z],p3[z,x]}\displaystyle\min\{\mathrm{diam}\{p_{1},p_{2},p_{3}\}\colon p_{1}\in[x,y],p_{2}\in[y,z],p_{3}\in[z,x]\}

is bounded by a constant independent of choices of geodesic segments and geodesic triangles. See [13, 21.- Proposition] for details. We say that this quantity is the minimum diameter of geodesic triangle [x,y][y,z][z,x][x,y]\cup[y,z]\cup[z,x].

By Proposition 2.6, there exists a normal geodesic segment connecting each two points, that is,

  • 𝚗γ(x,y)=u1h1v1\mathtt{n}\gamma(x,y)=u_{1}\ast h_{1}\ast v_{1},

  • 𝚗γ(y,z)=u2h2v2\mathtt{n}\gamma(y,z)=u_{2}\ast h_{2}\ast v_{2},

  • 𝚗γ(z,x)=u3h3v3\mathtt{n}\gamma(z,x)=u_{3}\ast h_{3}\ast v_{3},

where uiu_{i} and viv_{i} are vertical segments and each hih_{i} is a horizontal segment. Suppose D(h1)D(h2)D(h3)D(h_{1})\leq D(h_{2})\leq D(h_{3}).

It is easily shown that Im(u1)Im(v3)\mathop{\mathrm{Im}}\nolimits(u_{1})\subset\mathop{\mathrm{Im}}\nolimits(v_{3}) and Im(v1)Im(u2)\mathop{\mathrm{Im}}\nolimits(v_{1})\subset\mathop{\mathrm{Im}}\nolimits(u_{2}). Then, we have

Im(h1)N(Im(v3),3)N(Im(u2),3).\displaystyle\mathop{\mathrm{Im}}\nolimits(h_{1})\subset N(\mathop{\mathrm{Im}}\nolimits(v_{3}),3)\cup N(\mathop{\mathrm{Im}}\nolimits(u_{2}),3).

Therefore,

min{diam{p1,p2,p3}:p1Im(𝚗γ(x,y)),p2Im(𝚗γ(y,z)),p3Im(𝚗γ(z,x))}\displaystyle\min\{\mathrm{diam}\{p_{1},p_{2},p_{3}\}\colon p_{1}\in\mathop{\mathrm{Im}}\nolimits(\mathtt{n}\gamma(x,y)),p_{2}\in\mathop{\mathrm{Im}}\nolimits(\mathtt{n}\gamma(y,z)),p_{3}\in\mathop{\mathrm{Im}}\nolimits(\mathtt{n}\gamma(z,x))\}

is bounded by 55. By Proposition 2.6, for each geodesic segment from xx to yy, denoted by γ(x,y)\gamma(x,y), we have

dH(Im(γ(x,y)),Im(𝚗γ(x,y)))4.\displaystyle d_{H}(\mathrm{Im}(\gamma(x,y)),\mathrm{Im}(\mathtt{n}\gamma(x,y)))\leq 4.

For any x,y,z(X,X(0))x,y,z\in\mathcal{H}(X,X^{(0)}) and any geodesic triangle Δ(x,y,z)\Delta(x,y,z), the minimal diameter is bounded by 99. Therefore, (X,X(0))\mathcal{H}(X,X^{(0)}) is a Gromov hyperbolic space. {comment} It is easily shown that Im(u1)Im(v3)\mathop{\mathrm{Im}}\nolimits(u_{1})\subset\mathop{\mathrm{Im}}\nolimits(v_{3}) and Im(v1)Im(u2)\mathop{\mathrm{Im}}\nolimits(v_{1})\subset\mathop{\mathrm{Im}}\nolimits(u_{2}). Then, we have

Im(h1)N(Im(v3),3)N(Im(u2),3).\displaystyle\mathop{\mathrm{Im}}\nolimits(h_{1})\subset N(\mathop{\mathrm{Im}}\nolimits(v_{3}),3)\cup N(\mathop{\mathrm{Im}}\nolimits(u_{2}),3).

Next, we will show that H(h3)H(h2)H(h_{3})-H(h_{2}) is bounded. Let s(h3)=(z,H(h3))s(h_{3})=(z,H(h_{3})), t(h3)=(x,H(h3))t(h_{3})=(x,H(h_{3})), and s(h2)=(y,H(h2))s(h_{2})=(y,H(h_{2})). Since the length of hih_{i} is at most 44, we have

d(x,z)\displaystyle d(x,z) d(x,y)+d(y,z)\displaystyle\leq d(x,y)+d(y,z)
42H(h1)+42H(h2)\displaystyle\leq 4\cdot 2^{H(h_{1})}+4\cdot 2^{H(h_{2})}
82H(h2)2H(h2)+4\displaystyle\leq 8\cdot 2^{H(h_{2})}\leq 2^{H(h_{2})+4}

Therefore, we have H(h3)H(h2)+4H(h_{3})\leq H(h_{2})+4. This implies that

Im(h3)\displaystyle\mathop{\mathrm{Im}}\nolimits(h_{3}) N(Im(h2),8),\displaystyle\subset N(\mathop{\mathrm{Im}}\nolimits(h_{2}),8),
Im(h2)\displaystyle\mathop{\mathrm{Im}}\nolimits(h_{2}) N(Im(h3),8).\displaystyle\subset N(\mathop{\mathrm{Im}}\nolimits(h_{3}),8).

Finally,

Im(v3)Im(u1)\displaystyle\mathop{\mathrm{Im}}\nolimits(v_{3})\setminus\mathop{\mathrm{Im}}\nolimits(u_{1}) \displaystyle\subset

3. coarsely convex bicombing

Let (X,dX)(X,d_{X}) be a metric space. For λ1\lambda\geq 1 and k0k\geq 0, a (λ,k)(\lambda,k)-quasi-geodesic bicombing on XX is a map γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X such that for x,yXx,y\in X, we have γ(x,y,0)=x\gamma(x,y,0)=x, γ(x,y,1)=y\gamma(x,y,1)=y, and

λ1|ts|dX(x,y)kdX(γ(x,y,t),γ(x,y,s))λ|ts|dX(x,y)+k(t,s[0,1]).\displaystyle\lambda^{-1}\left\lvert t-s\right\rvert d_{X}(x,y)-k\leq d_{X}(\gamma(x,y,t),\gamma(x,y,s))\leq\lambda\left\lvert t-s\right\rvert d_{X}(x,y)+k\ \ \ \ (t,s\in[0,1]).

If the space XX admits a (λ,k)(\lambda,k)-quasi-geodesic bicombing for some λ1\lambda\geq 1 and k>0k>0, we say that XX admits a quasi-geodesic bicombing. If a group GG acts on XX by isometries, a geodesic bicombing γ:X×X×[0,1]X\gamma:X\times X\times[0,1]\to X is GG-equivariant if

gγ(x,y)(t)=γ(gx,gy)(t)\displaystyle g\cdot\gamma(x,y)(t)=\gamma(gx,gy)(t)

holds for any gGg\in G, x,yXx,y\in X, and t[0,1]t\in[0,1].

Definition 3.1.

Let λ1\lambda\geq 1, k0k\geq 0, E1E\geq 1, and C0C\geq 0 be constants. Let θ:00\theta\colon\mathbb{R}_{\geq 0}\to\mathbb{R}_{\geq 0} be a non-decreasing function.

A (λ,k,E,C,θ)(\lambda,k,E,C,\theta) -coarsely convex bicombing on a metric space (X,dX)(X,d_{X}) is a (λ,k)(\lambda,k)-quasi-geodesic bicombing γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X with the following:

  1. (i)

    Let x1,x2,y1,y2Xx_{1},x_{2},y_{1},y_{2}\in X and let a,b[0,1]a,b\in[0,1]. Set y1:=γ(x1,y1,a)y_{1}^{\prime}:=\gamma(x_{1},y_{1},a) and y2:=γ(x2,y2,b)y_{2}^{\prime}:=\gamma(x_{2},y_{2},b). Then, for c[0,1]c\in[0,1], we have

    dX(γ(x1,y1,ca),γ(x2,y2,cb))(1c)EdX(x1,x2)+cEdX(y1,y2)+C.\displaystyle d_{X}(\gamma(x_{1},y_{1},ca),\gamma(x_{2},y_{2},cb))\leq(1-c)Ed_{X}(x_{1},x_{2})+cEd_{X}(y_{1}^{\prime},y_{2}^{\prime})+C.
  2. (ii)

    Let x1,x2,y1,y2Xx_{1},x_{2},y_{1},y_{2}\in X. Then for t,s[0,1]t,s\in[0,1] we have

    |tdX(x1,y1)sdX(x2,y2)|θ(dX(x1,x2)+dX(γ(x1,y1,t),γ(x2,y2,s))).\displaystyle\left\lvert td_{X}(x_{1},y_{1})-sd_{X}(x_{2},y_{2})\right\rvert\leq\theta(d_{X}(x_{1},x_{2})+d_{X}(\gamma(x_{1},y_{1},t),\gamma(x_{2},y_{2},s))).

The following reparametrization is used to construct ideal boundaries in Section 4

Definition 3.2.

Let XX be a metric space and let γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X be a (λ,k)(\lambda,k)-quasi-geodesic bicombing on XX. A reparametrised bicombing of γ\gamma is a map

rpγ:X×X×0X\displaystyle\textup{{rp}}\gamma\colon X\times X\times\mathbb{R}_{\geq 0}\to X

defined by

rpγ(x,y,t):={γ(x,y,t/dX(x,y))if tdX(x,y)yif t>dX(x,y).\displaystyle\textup{{rp}}\gamma(x,y,t):=\begin{cases}\gamma\left(x,y,{t}/{d_{X}(x,y)}\right)&\text{if }t\leq d_{X}(x,y)\\ y&\text{if }t>d_{X}(x,y)\end{cases}.

4. Ideal boundary

In this section, we review the construction of the ideal boundary of a coarsely convex space.

Let (X,dX)(X,d_{X}) be a metric space equipped with a (λ,k,E,C,θ)(\lambda,k,E,C,\theta)-coarsely convex bicombing γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X. We choose a base point eXe\in X.

4.1. Gromov product and sequential boundary

Definition 4.1.

Set k1=λ+kk_{1}=\lambda+k, D=2(1+E)k1+CD=2(1+E)k_{1}+C, and D1=2D+2D_{1}=2D+2. We define a product ()e:X×X0(\cdot\mid\cdot)_{e}\colon X\times X\to\mathbb{R}_{\geq 0} by

(xy)e:=min{dX(e,x),dX(e,y),sup{t0:dX(rpγ(e,x,t),rpγ(e,y,t))D1}},\displaystyle(x\mid y)_{e}:=\min\{d_{X}(e,x),\ d_{X}(e,y),\ \sup\{t\in\mathbb{R}_{\geq 0}:d_{X}(\textup{{rp}}\gamma(e,x,t),\textup{{rp}}\gamma(e,y,t))\leq D_{1}\}\},

We abbreviate (xy)e(x\mid y)_{e} by (xy)(x\mid y).

Lemma 4.2 ([11, Lemma 4.8]).

Set D2:=E(D1+2k1)D_{2}:=E(D_{1}+2k_{1}). For x,y,zXx,y,z\in X, we have

(xz)D21min{(xy),(yz)}.\displaystyle(x\mid z)\geq D_{2}^{-1}\min\{(x\mid y),(y\mid z)\}.

We use a sequential model of the ideal boundary introduced in [12]. The idea is based on [14] and [13, Chapitre 7].

Definition 4.3.

Let

S(X)={(xi):(xixj) as i,j}\displaystyle S_{\infty}(X)=\{(x_{i}):(x_{i}\mid x_{j})\to\infty\text{ as }i,j\to\infty\}

and define a relation \sim on S(X)S_{\infty}(X) as follows. For every (xi),(yi)S(X)(x_{i}),(y_{i})\in S_{\infty}(X), we have (xi)(yi)(x_{i})\sim(y_{i}) if

(xiyi) as i\displaystyle(x_{i}\mid y_{i})\to\infty\text{ as }i\to\infty
Lemma 4.4.

The relation \sim is an equivalence relation on S(X)S_{\infty}(X).

Proof..

It is clear that the relation \sim is reflexive and symmetric. Lemma 4.2 implies that it is transitive. ∎

Definition 4.5.

Let

X=S(X)/ and X¯=XX.\displaystyle\partial X=S_{\infty}(X)/\sim\quad\text{ and }\quad\overline{X}=X\cup\partial X.

For xXx\in X and a sequence (xi)(x_{i}) in XX, we write (xi)x(x_{i})\in x if xi=xx_{i}=x for every ii\in\mathbb{N}. We extend the Gromov product ():X×X0(\cdot\mid\cdot)\colon X\times X\to\mathbb{R}_{\geq 0} to a symmetric function ():X¯×X¯0{}(\cdot\mid\cdot)\colon\overline{X}\times\overline{X}\to\mathbb{R}_{\geq 0}\cup\{\infty\} by letting

(1) (xy)\displaystyle(x\mid y) =sup{lim infi(xiyi):(xi)x,(yi)y}\displaystyle=\sup\{\liminf_{i\to\infty}(x_{i}\mid y_{i}):(x_{i})\in x,(y_{i})\in y\}

for x,yX¯x,y\in\overline{X}.

For nn\in\mathbb{N}, let

Vn\displaystyle V_{n} ={(x,y)X¯×X¯:(xy)>n}{(x,y)X×X:dX(x,y)<1/n},\displaystyle=\{(x,y)\in\overline{X}\times\overline{X}:(x\mid y)>n\}\cup\{(x,y)\in X\times X:d_{X}(x,y)<1/n\},
Vn[x]\displaystyle V_{n}[x] ={yX¯:(x,y)Vn},(xX¯).\displaystyle=\{y\in\overline{X}:(x,y)\in V_{n}\},\quad(x\in\overline{X}).

By [12, Lemma 2.6.], {Vn:n}\{V_{n}:n\in\mathbb{N}\} is a base of a metrizable uniformity on X¯\overline{X}. See also [11, Section 4.3].

Definition 4.6.

Let X¯\overline{X} be equipped with the topology 𝒯()\mathcal{T}_{(\cdot\mid\cdot)} generated by the family {Vn[x]:xX¯,n}\{V_{n}[x]:x\in\overline{X},n\in\mathbb{N}\}. We call the subspace X\partial X of X¯\overline{X} the Gromov boundary of XX with respect to ()(\cdot\mid\cdot). We also call X\partial X the ideal boundary of XX.

Lemma 4.7 ([12, Lemma 2.8, Theorem 2.9]).

We have the following:

  1. (i)

    The relative topology 𝒯()X\mathcal{T}_{(\cdot\mid\cdot)}\!\!\upharpoonright_{X} on XX with respect to X¯\overline{X} coincides with the topology 𝒯d\mathcal{T}_{d} induced by the metric dd.

  2. (ii)

    XX is a dense open subset in X¯\overline{X}.

  3. (iii)

    If (X,d)(X,d) is complete, then so is (X¯,d)(\overline{X},d).

  4. (iv)

    If (X,d)(X,d) is proper, then (X¯,d)(\overline{X},d) is compact.

4.2. Combing at infinity

Lemma 4.8.

Suppose that XX is proper. Then there exists a map

rpγ¯:X×X¯×0X\displaystyle\textup{{rp}}\bar{\gamma}\colon X\times\overline{X}\times\mathbb{R}_{\geq 0}\to X

satisfying the following:

  1. (i)

    For x,yXx,y\in X, we have rpγ¯(x,y,)=rpγ(x,y,)\textup{{rp}}\bar{\gamma}(x,y,-)=\textup{{rp}}\gamma(x,y,-).

  2. (ii)

    For (e,x)X×X(e,x)\in X\times\partial X, there exists a sequence (xn)(x_{n}) in XX such that the sequence of maps (rpγ(e,xn,):X)n(\textup{{rp}}\gamma(e,x_{n},-)\!\!\upharpoonright_{\mathbb{N}}:\mathbb{N}\to X)_{n} converges to rpγ¯(e,x,)\textup{{rp}}\bar{\gamma}(e,x,-)\!\!\upharpoonright_{\mathbb{N}} pointwise.

  3. (iii)

    For (e,x)X×X(e,x)\in X\times\partial X, we have

    (rpγ¯(e,x,t)x)east\displaystyle(\textup{{rp}}\bar{\gamma}(e,x,t)\mid x)_{e}\to\infty\quad\text{as}\quad t\to\infty
  4. (iv)

    For (e,x)X×X(e,x)\in X\times\partial X, the map rpγ¯(e,x,):0X\textup{{rp}}\bar{\gamma}(e,x,-)\colon\mathbb{R}_{\geq 0}\to X is a (λ,k1)(\lambda,k_{1})-quasi geodesic, where k1:=λ+kk_{1}:=\lambda+k.

Proof..

For (x,y)X×X(x,y)\in X\times X, we define rpγ(x,y,)\textup{{rp}}\gamma(x,y,-) by the equality in (i). We use [11, Proposition 4.17] to construct maps rpγ¯(e,x,)\textup{{rp}}\bar{\gamma}(e,x,-) for (e,x)X×X(e,x)\in X\times\partial X satisfying (ii) and (iii). Finally, (iv) follows from [11, Lemma 4.1]. ∎

Definition 4.9.

We call the map rpγ¯\textup{{rp}}\bar{\gamma} given in Lemma 4.8 an extended bicombing on X×X¯X\times\overline{X} corresponding to γ\gamma. For (e,x)X×X(e,x)\in X\times\partial X, we abbreviate rpγ¯(e,x,)\textup{{rp}}\bar{\gamma}(e,x,-) by γex()\gamma_{e}^{x}(-).

Lemma 4.10 ([11, Proposition 4.2]).

The extended bicombing rpγ¯\textup{{rp}}\bar{\gamma} on X×X¯X\times\overline{X} satisfies the following:

  1. (1)

    Let (e1,x1),(e2,x2)X×X(e_{1},x_{1}),(e_{2},x_{2})\in X\times\partial X and let a,b0a,b\in\mathbb{R}_{\geq 0}. Set x1:=rpγ¯(e1,x1,a)x_{1}^{\prime}:=\textup{{rp}}\bar{\gamma}(e_{1},x_{1},a) and x2:=rpγ¯(e2,x2,b)x_{2}^{\prime}:=\textup{{rp}}\bar{\gamma}(e_{2},x_{2},b). Then, for c[0,1]c\in[0,1], we have

    dX(rpγ¯(e1,x1,ca),rpγ¯(e2,x2,cb))(1c)EdX(e1,e2)+cEdX(x1,x2)+D\displaystyle d_{X}(\textup{{rp}}\bar{\gamma}(e_{1},x_{1},ca),\textup{{rp}}\bar{\gamma}(e_{2},x_{2},cb))\leq(1-c)Ed_{X}(e_{1},e_{2})+cEd_{X}(x_{1}^{\prime},x_{2}^{\prime})+D

    where D:=2(1+E)k1+CD:=2(1+E)k_{1}+C.

  2. (2)

    We define a non-decreasing function θ~:00\tilde{\theta}\colon\mathbb{R}_{\geq 0}\to\mathbb{R}_{\geq 0} by θ~(t):=θ(t+1)+1\tilde{\theta}(t):=\theta(t+1)+1. Let (e1,x1),(e2,x2)X×X(e_{1},x_{1}),(e_{2},x_{2})\in X\times\partial X Then for t,s0t,s\in\mathbb{R}_{\geq 0}, we have

    |ts|θ~(dX(e1,e2)+dX(rpγ¯(e1,x1,t),rpγ¯(e2,x2,s))).\displaystyle\left\lvert t-s\right\rvert\leq\tilde{\theta}(d_{X}(e_{1},e_{2})+d_{X}(\textup{{rp}}\bar{\gamma}(e_{1},x_{1},t),\textup{{rp}}\bar{\gamma}(e_{2},x_{2},s))).
Definition 4.11.

For x,yXx,y\in\partial X, we define

(γexγey)e:=sup{t0:dX(γex(t),γey(t))D1}.\displaystyle(\gamma_{e}^{x}\mid\gamma_{e}^{y})_{e}:=\sup\{t\in\mathbb{R}_{\geq 0}:d_{X}(\gamma_{e}^{x}(t),\gamma_{e}^{y}(t))\leq D_{1}\}.

For xXx\in\partial X and for pXp\in X, we define

(γexp)e=(pγex)e:=min{dX(e,p),sup{t0:dX(γ(e,p,t),γex(t))D1}}.\displaystyle(\gamma_{e}^{x}\mid p)_{e}=(p\mid\gamma_{e}^{x})_{e}:=\min\{d_{X}(e,p),\sup\{t\in\mathbb{R}_{\geq 0}:d_{X}(\gamma(e,p,t),\gamma_{e}^{x}(t))\leq D_{1}\}\}.
Lemma 4.12.

There exists a constant Ω1\Omega\geq 1 depending on λ,k,E,C,θ(0)\lambda,k,E,C,\theta(0) such that the following holds:

  1. (1)

    For x,yXx,y\in\partial X, we have

    (γexγey)(xy)Ω(γexγey).\displaystyle(\gamma_{e}^{x}\mid\gamma_{e}^{y})\leq(x\mid y)\leq\Omega(\gamma_{e}^{x}\mid\gamma_{e}^{y}).
  2. (2)

    For triplet x,y,zXx,y,z\in\partial X, we have

    (γexγez)Ω1min{(γexγey),(γeyγez)}.\displaystyle(\gamma_{e}^{x}\mid\gamma_{e}^{z})\geq\Omega^{-1}\min\{(\gamma_{e}^{x}\mid\gamma_{e}^{y}),(\gamma_{e}^{y}\mid\gamma_{e}^{z})\}.
  3. (3)

    For triplet x,y,zX¯x,y,z\in\overline{X}, we have

    (xz)Ω1min{(xy),(yz)}.\displaystyle(x\mid z)\geq\Omega^{-1}\min\{(x\mid y),(y\mid z)\}.
  4. (4)

    Let x,yXx,y\in\partial X. For all t0t\in\mathbb{R}_{\geq 0} with t(γexγey)t\leq(\gamma_{e}^{x}\mid\gamma_{e}^{y}), we have

    dX(γex(t),γey(t))Ω.\displaystyle d_{X}(\gamma_{e}^{x}(t),\gamma_{e}^{y}(t))\leq\Omega.
  5. (5)

    Let eXe\in X and let x,yX¯x,y\in\overline{X}. If rpγ¯(e,x,a)=rpγ¯(e,y,b)\textup{{rp}}\bar{\gamma}(e,x,a)=\textup{{rp}}\bar{\gamma}(e,y,b) for some a,b0a,b\in\mathbb{R}_{\geq 0}, then for all t[0,max{a,b}]t\in[0,\max\{a,b\}] we have

    dX(rpγ¯(e,x,t),rpγ¯(e,y,t))Ω.\displaystyle d_{X}(\textup{{rp}}\bar{\gamma}(e,x,t),\textup{{rp}}\bar{\gamma}(e,y,t))\leq\Omega.
  6. (6)

    Let eXe\in X and xXx\in\partial X. For vXv\in X and t[0,1]t\in[0,1], we have

    (xγ(e,v,t))eΩ1min{(xv)e,tdX(e,v)}.\displaystyle(x\mid\gamma(e,v,t))_{e}\geq\Omega^{-1}\min\{(x\mid v)_{e},td_{X}(e,v)\}.
Proof..

(1) to (5) are [8, Lemma 2.9.]. We give a proof of (6). By the definition, we have (xγ(e,v,t))etdX(e,v)(x\mid\gamma(e,v,t))_{e}\geq td_{X}(e,v). We suppose that (xv)tdX(e,v)(x\mid v)\leq td_{X}(e,v). Set s=(xv)s=(x\mid v). By [11, lemma 4.7.], we have dX(γex(s),rpγ(e,v,s))D1+k1d_{X}(\gamma_{e}^{x}(s),\textup{{rp}}\gamma(e,v,s))\leq D_{1}+k_{1}. Set ss/(E(D1+k1))s^{\prime}\coloneqq s/(E(D_{1}+k_{1})). Then,

dX(γex(s),rpγ(e,v,s))EE(D1+k1)dX(γex(s),rpγ(e,v,s))+DD+1D1\displaystyle d_{X}(\gamma_{e}^{x}(s^{\prime}),\textup{{rp}}\gamma(e,v,s^{\prime}))\leq\frac{E}{E(D_{1}+k_{1})}d_{X}(\gamma_{e}^{x}(s),\textup{{rp}}\gamma(e,v,s))+D\leq D+1\leq D_{1}

Thus (xγ(e,v,t))(E(D1+k1))1(xv)(x\mid\gamma(e,v,t))\geq(E(D_{1}+k_{1}))^{-1}(x\mid v).

4.3. Visual maps

Let (X,dX)(X,d_{X}) and (Y,dY)(Y,d_{Y}) be metric spaces. We say that a map f:XYf\colon X\to Y is a large scale Lipschitz map, if there exists L>1L>1 such that

dY(f(x),f(y))LdX(x,y)+L.\displaystyle d_{Y}(f(x),f(y))\leq Ld_{X}(x,y)+L.

Let γx\gamma_{x} and γy\gamma_{y} be coarsely convex bicombings on XX and YY, respectively. Let aXa\in X and bYb\in Y be base points of XX and YY, respectively.

Definition 4.13.

We say that a large scale Lipschitz map f:XYf\colon X\to Y is visual if for every pair of sequences (xn)n,(yn)n(x_{n})_{n},(y_{n})_{n} in XX with (xnyn)a(x_{n}\mid y_{n})_{a}\to\infty, we have (f(xn)f(yn))b(f(x_{n})\mid f(y_{n}))_{b}\to\infty.

Let f:XYf\colon X\to Y be a visual map. We define a map f:XY\partial f\colon\partial X\to\partial Y as follows. For xXx\in\partial X, we choose a sequence (xn)n(x_{n})_{n} representing xx. Then we define f(x)\partial f(x) to be the equivalence class of the sequence (f(xn))n(f(x_{n}))_{n}. By [8, Proposition 3.5], f(x)\partial f(x) does not depend on the choice of (xn)n(x_{n})_{n}. We say that f\partial f is induced by ff.

Proposition 4.14 ([8, Corollary 3.6]).

Let ff be a visual map. Then the induced map f:XY\partial f\colon\partial X\to\partial Y is continuous.

5. Geodesic coarsely convex spaces

5.1. Geodesic combing at infinity

Let (X,dX)(X,d_{X}) be a metric space. A geodesic bicombing on XX is a map γ:X×X×[0,1]X\gamma:X\times X\times[0,1]\to X such that for x,yXx,y\in X, we have γ(x,y,0)=x\gamma(x,y,0)=x, γ(x,y,1)=y\gamma(x,y,1)=y, and

dX(γ(x,y,t),γ(x,y,s))=|ts|dX(x,y)(t,s[0,1])\displaystyle d_{X}(\gamma(x,y,t),\gamma(x,y,s))=\left\lvert t-s\right\rvert d_{X}(x,y)\quad(t,s\in[0,1])
Definition 5.1.

Let E1E\geq 1 and C0C\geq 0 be constants. An (E,C)(E,C)-geodesic coarsely convex bicombing on a metric space (X,dX)(X,d_{X}) is a geodesic bicombing γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X satisfying the following:

Let x1,x2,y1,y2Xx_{1},x_{2},y_{1},y_{2}\in X and let a,b[0,1]a,b\in[0,1]. Set y1:=γ(x1,y1,a)y_{1}^{\prime}:=\gamma(x_{1},y_{1},a) and y2:=γ(x2,y2,b)y_{2}^{\prime}:=\gamma(x_{2},y_{2},b). Then, for c[0,1]c\in[0,1], we have

dX(γ(x1,y1,ca),γ(x2,y2,cb))(1c)EdX(x1,x2)+cEdX(y1,y2)+C.\displaystyle d_{X}(\gamma(x_{1},y_{1},ca),\gamma(x_{2},y_{2},cb))\leq(1-c)Ed_{X}(x_{1},x_{2})+cEd_{X}(y_{1}^{\prime},y_{2}^{\prime})+C.
Lemma 5.2.

An (E,C)(E,C)-geodesic coarsely convex bicombing γ\gamma on a metric space (X,dX)(X,d_{X}) is a (1,0,E,C,id0)(1,0,E,C,\mathrm{id}_{\mathbb{R}_{\geq 0}})-coarsely convex bicombing on (X,dX)(X,d_{X}).

Proof..

It follows from the definition of the (E,C)(E,C)-geodesic coarsely convex bicombing, that γ\gamma satisfies (i) of Definition 3.1.

Let x1,x2,y1,y2Xx_{1},x_{2},y_{1},y_{2}\in X. Then for t,s[0,1]t,s\in[0,1], we have

|tdX(x1,y1)sdX(x2,y2)|dX(x1,x2)+dX(γ(x1,y1,t),γ(x2,y2,s)).\displaystyle\left\lvert td_{X}(x_{1},y_{1})-sd_{X}(x_{2},y_{2})\right\rvert\leq d_{X}(x_{1},x_{2})+d_{X}(\gamma(x_{1},y_{1},t),\gamma(x_{2},y_{2},s)).

by the triangle inequality. Therefore γ\gamma satisfies (ii) of Definition 3.1 with θ=id0\theta=\textrm{id}_{\mathbb{R}_{\geq 0}}. ∎

Example 5.3.

Let (X,dX)(X,d_{X}) be a geodesic δ\delta-hyperbolic space. For x,yXx,y\in X, we choose a geodesic γx,y:[0,dX(x,y)]X\gamma_{x,y}\colon[0,d_{X}(x,y)]\to X such that γx,y(0)=x\gamma_{x,y}(0)=x and γx,y(dX(x,y))=y\gamma_{x,y}(d_{X}(x,y))=y. We define γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X by

γ(x,y,t):=γx,y(t/dX(x,y)).\displaystyle\gamma(x,y,t):=\gamma_{x,y}(t/d_{X}(x,y)).

Then γ\gamma is a (1,8δ)(1,8\delta)-geodesic coarsely convex bicombing. See [13, Chapitre 2. 25.- Proposition] for details.

Let XX be a space equipped with an (E,C)(E,C)-geodesic coarsely convex bicombing γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X.

By Lemma 5.2 and Lemma 4.8, we have an extended bicombing on X×X¯X\times\overline{X}. Since γ\gamma is a geodesic bicombing, we can upgrade it.

Lemma 5.4.

Suppose that XX is proper and γ\gamma is an (E,C)(E,C)-geodesic coarsely convex bicombing on XX. Then there exists a map

rpγ¯:X×X¯×0X\displaystyle\textup{{rp}}\bar{\gamma}\colon X\times\overline{X}\times\mathbb{R}_{\geq 0}\to X

satisfying the following:

  1. (1)

    For x,yXx,y\in X, we have rpγ¯(x,y,)=rpγ(x,y,)\textup{{rp}}\bar{\gamma}(x,y,-)=\textup{{rp}}\gamma(x,y,-).

  2. (2)

    For each (e,x)X×X(e,x)\in X\times\partial X, there exists a sequence (xn)(x_{n}) in XX such that the sequence of maps (rpγ(e,xn,):0X)n(\textup{{rp}}\gamma(e,x_{n},-):\mathbb{R}_{\geq 0}\to X)_{n} converges to rpγ¯(e,x,)\textup{{rp}}\bar{\gamma}(e,x,-) uniformly on compact sets.

  3. (3)

    For each (e,x)X×X(e,x)\in X\times\partial X, we have

    (rpγ¯(e,x,t)x)east\displaystyle(\textup{{rp}}\bar{\gamma}(e,x,t)\mid x)_{e}\to\infty\quad\text{as}\quad t\to\infty
  4. (4)

    For each (e,x)X×X(e,x)\in X\times\partial X, the map rpγ¯(e,x,):0X\textup{{rp}}\bar{\gamma}(e,x,-)\colon\mathbb{R}_{\geq 0}\to X is a geodesic.

Proof..

We can use the same construction of geodesics as the one described in [13, 5-25 Théorèm]. Here we only give a sketch of the proof.

Let (e,x)X×X(e,x)\in X\times\partial X. We choose (xn)S(X)(x_{n})\in S_{\infty}(X) such that (xn)x(x_{n})\in x. By Arzelà–Ascoli Theorem and standard diagonal arguments, We can take a subsequence xnkx_{n_{k}} such that the sequence of maps (rpγ(e,xnk,):0X)k(\textup{{rp}}\gamma(e,x_{n_{k}},-):\mathbb{R}_{\geq 0}\to X)_{k} converges uniformly on compact sets. This defines a map rpγ¯(e,x,):0X\textup{{rp}}\bar{\gamma}(e,x,-)\colon\mathbb{R}_{\geq 0}\to X. From the construction, it is easy to see that this map is a geodesic, and (rpγ¯(e,x,t)x)e(\textup{{rp}}\bar{\gamma}(e,x,t)\mid x)_{e}\to\infty as tt\to\infty. ∎

Definition 5.5.

We call the map rpγ¯\textup{{rp}}\bar{\gamma} given in Lemma 5.4 an extended geodesic bicombing on X×X¯X\times\overline{X} corresponding to γ\gamma. For (e,x)X×X(e,x)\in X\times\partial X, we abbreviate rpγ¯(e,x,)\textup{{rp}}\bar{\gamma}(e,x,-) by γex\gamma_{e}^{x}.

Lemma 5.6.

The extended geodesic bicombing rpγ¯\textup{{rp}}\bar{\gamma} on X×X¯X\times\overline{X} satisfies the following: Let (e1,x1),(e2,x2)X×X(e_{1},x_{1}),(e_{2},x_{2})\in X\times\partial X and let a,b0a,b\in\mathbb{R}_{\geq 0}. Set x1:=rpγ¯(e1,x1,a)x_{1}^{\prime}:=\textup{{rp}}\bar{\gamma}(e_{1},x_{1},a) and x2:=rpγ¯(e2,x2,b)x_{2}^{\prime}:=\textup{{rp}}\bar{\gamma}(e_{2},x_{2},b). Then, for c[0,1]c\in[0,1], we have

dX(rpγ¯(e1,x1,ca),rpγ¯(e2,x2,cb))(1c)EdX(e1,e2)+cEdX(x1,x2)+C.\displaystyle d_{X}(\textup{{rp}}\bar{\gamma}(e_{1},x_{1},ca),\textup{{rp}}\bar{\gamma}(e_{2},x_{2},cb))\leq(1-c)Ed_{X}(e_{1},e_{2})+cEd_{X}(x_{1}^{\prime},x_{2}^{\prime})+C.
Proof..

The statement follows immediately from (ii) of Lemma 5.4. ∎

Remark 5.7.

All statements in Lemma 4.12 hold for γex\gamma_{e}^{x}.

Lemma 5.8.

For e,x,yXe,x,y\in X, we have

(xy)emin{dX(e,x),dX(e,y)}2EdX(x,y).\displaystyle(x\mid y)_{e}\geq\frac{\min\{d_{X}(e,x),d_{X}(e,y)\}}{2Ed_{X}(x,y)}.
Proof..

Set u:=min{dX(e,x),dX(e,y)}u:=\min\{d_{X}(e,x),d_{X}(e,y)\}. We have

dX(rpγ(e,x,u),rpγ(e,y,u))dX(x,y)+|dX(e,x)dX(e,y)|2dX(x,y).\displaystyle d_{X}(\textup{{rp}}\gamma(e,x,u),\textup{{rp}}\gamma(e,y,u))\leq d_{X}(x,y)+\left\lvert d_{X}(e,x)-d_{X}(e,y)\right\rvert\leq 2d_{X}(x,y).

Set c:=1/(2EdX(x,y))c:=1/(2Ed_{X}(x,y)), we have

dX(rpγ(e,x,cu),rpγ(e,y,cu))cEdX(rpγ(e,x,u),rpγ(e,y,u))+C1+C.\displaystyle d_{X}(\textup{{rp}}\gamma(e,x,cu),\textup{{rp}}\gamma(e,y,cu))\leq cEd_{X}(\textup{{rp}}\gamma(e,x,u),\textup{{rp}}\gamma(e,y,u))+C\leq 1+C.

Therefore

(xy)ecu=min{dX(e,x),dX(e,y)}2EdX(x,y).\displaystyle(x\mid y)_{e}\geq cu=\frac{\min\{d_{X}(e,x),d_{X}(e,y)\}}{2Ed_{X}(x,y)}.

5.2. γ\gamma-convex subspaces

Definition 5.9.

Let XX be a metric space with (E,C)(E,C)-geodesic coarsely convex bicombing γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X. We say that a subspace YXY\subset X is γ\gamma-convex if for all x,yYx,y\in Y and all t[0,1]t\in[0,1], we have γ(x,y,t)Y\gamma(x,y,t)\in Y.

Proposition 5.10.

Let XX be a metric space with (E,C)(E,C)-geodesic coarsely convex bicombing and YXY\subset X be a γ\gamma-convex subspace. Then the restriction γY\gamma_{Y} of γ\gamma on :Y×Y×[0,1]\colon Y\times Y\times[0,1] is a (E,C)(E,C)-geodesic coarsely convex bicombing on YY. Moreover, the inclusion ι:YX\iota\colon Y\hookrightarrow X extends to a topological embedding ι¯:Y¯X¯\bar{\iota}\colon\overline{Y}\hookrightarrow\overline{X}.

Corollary 5.11.

Let XX be a metric space with (E,C)(E,C)-geodesic coarsely convex bicombing and YXY\subset X be a γ\gamma-convex subspace. Then the ideal boundary of YY with respect to γY\gamma_{Y} is homeomorphic to ι(Y)¯ι(Y)\overline{\iota(Y)}\setminus\iota(Y), where ι(Y)¯\overline{\iota(Y)} is the closure of ι(Y)\iota(Y) in X¯\overline{X}.

6. Continuous at infinity

We study maps between geodesic coarsely convex spaces which are not necessarily continuous, although, induce continuous maps between ideal boundaries. The main result of this section will be used to prove Proposition 9.2, which is a key proposition for results in Section 9

Definition 6.1.

Let XX be a space with a geodesic coarsely convex bicombing. Let AXA\subset X be a subspace and A¯\overline{A} be the closure of AA in X¯\overline{X}. Let UU be a topological space. We say that a map F:A¯UF\colon\overline{A}\to U is continuous at infinity if FF is continuous at all xA¯Ax\in\overline{A}\setminus A.

Let (X,dX)(X,d_{X}) be a space equipped with an (E,C)(E,C)-geodesic coarsely convex bicombing γ:X×X×[0,1]X\gamma\colon X\times X\times[0,1]\to X.

Lemma 6.2.

Let AXA\subset X be a subspace and A¯\overline{A} be the closure of AA in X¯\overline{X}. Let f:A¯X¯f\colon\overline{A}\to\overline{X} be a map such that:

  1. (1)

    sup{dX(x,f(x)):xA}<\sup\{d_{X}(x,f(x)):x\in A\}<\infty, and

  2. (2)

    for xXA¯x\in\partial X\cap\overline{A}, f(x)=xf(x)=x.

Then ff is continuous at infinity.

Proof..

Let xXA¯x\in\partial X\cap\overline{A}. We show that ff is continuous at xx. Set K:=sup{dX(x,f(x)):xA}K:=\sup\{d_{X}(x,f(x)):x\in A\}. Let (xn)(x_{n}) be a sequence in A¯\overline{A} converging to xx. We can assume without loss of generality that xnAx_{n}\in A for all nn. Set tn:=min{dX(e,f(xn)),dX(e,xn)})t_{n}:=\min\{d_{X}(e,f(x_{n})),d_{X}(e,x_{n})\}). Since |dX(e,f(xn))dX(e,xn)|K\left\lvert d_{X}(e,f(x_{n}))-d_{X}(e,x_{n})\right\rvert\leq K, we have

dX(rpγ(e,f(xn),tn),rpγ(e,xn,tn))K+dX(xn,f(xn))2K.\displaystyle d_{X}(\textup{{rp}}\gamma(e,f(x_{n}),t_{n}),\textup{{rp}}\gamma(e,x_{n},t_{n}))\leq K+d_{X}(x_{n},f(x_{n}))\leq 2K.

Set

pn\displaystyle p_{n} :=rpγ(e,f(xn),(1/(2KE)tn)),\displaystyle:=\textup{{rp}}\gamma(e,f(x_{n}),(1/(2KE)t_{n})),
qn\displaystyle q_{n} :=rpγ(e,xn,(1/(2KE)tn)).\displaystyle:=\textup{{rp}}\gamma(e,x_{n},(1/(2KE)t_{n})).

We have

dX(pn,qn)\displaystyle d_{X}(p_{n},q_{n}) 12KEEdX(rpγ(e,f(xn),tn),rpγ(e,xn,tn))+CC+1\displaystyle\leq\frac{1}{2KE}Ed_{X}(\textup{{rp}}\gamma(e,f(x_{n}),t_{n}),\textup{{rp}}\gamma(e,x_{n},t_{n}))+C\leq C+1

So we have (xnf(xn))e1/(2KE)tn(x_{n}\mid f(x_{n}))_{e}\geq 1/(2KE)t_{n}. Then,

(xf(xn))eΩ1min{(xxn)e,(xnf(xn))e}\displaystyle{(x\mid f(x_{n}))}_{e}\geq\Omega^{-1}\min\{{(x\mid x_{n})}_{e},{(x_{n}\mid f(x_{n}))}_{e}\}\to\infty

It follows that (f(xn))(f(x_{n})) converges to xx. ∎

6.1. Image of the exponential map

We fix a base point eXe\in X. We define a map exp:X×0X\exp\colon\partial X\times\mathbb{R}_{\geq 0}\to X by exp(x,t):=rpγ¯(e,x,t)\exp(x,t):=\textup{{rp}}\bar{\gamma}(e,x,t). Set

exp(𝒪X)\displaystyle\exp(\mathcal{O}\partial X) :={rpγ¯(e,x,t):xXk,t0}\displaystyle:=\{\textup{{rp}}\bar{\gamma}(e,x,t):x\in\partial X_{k},t\in\mathbb{R}_{\geq 0}\}
exp(𝒪X)¯\displaystyle\overline{\exp(\mathcal{O}\partial X)} :=exp(𝒪X)Xk.\displaystyle:=\exp(\mathcal{O}\partial X)\cup\partial X_{k}.

We remark that exp(𝒪X)\exp(\mathcal{O}\partial X) is not necessarily coarsely dense in XX. In [11, Section 5.5], a coarsely equivalence map φ~:Xexp(𝒪Xk)\tilde{\varphi}\colon X\to\exp(\mathcal{O}\partial X_{k}) is contracted. We review the construction.

Let X(0)X^{(0)} be a subset of XX such that X(0)X^{(0)} is 2-dense in XX and 1-discrete, that is, for all v,wX(0)v,w\in X^{(0)}, if vwv\neq w then dX(v,w)1d_{X}(v,w)\geq 1, and, for all vXv\in X, there exists vX(0)v^{\prime}\in X^{(0)} with dX(v,v)2d_{X}(v,v^{\prime})\leq 2. Set D6:=2D1E+DD_{6}:=2D_{1}E+D and Y:=BD6(exp(𝒪X))Y:=B_{D_{6}}(\exp(\mathcal{O}\partial X)).

Let χ:00\chi\colon\mathbb{R}_{\geq 0}\to\mathbb{R}_{\geq 0} is a proper map given in [11, Section 5.5]. By the construction of χ\chi, for vX(0)v\in X^{(0)}, we have rpγ(e,v,χ(dX(e,v)))Y\textup{{rp}}\gamma(e,v,\chi(d_{X}(e,v)))\in Y, so we define a map φ:X(0)Y\varphi\colon X^{(0)}\to Y by

φ(v):=rpγ(e,v,χ(dX(e,v))).\displaystyle\varphi(v):=\textup{{rp}}\gamma(e,v,\chi(d_{X}(e,v))).

We define a map φ¯:X(0)¯Y¯\overline{\varphi}\colon\overline{X^{(0)}}\to\overline{Y} by

φ¯(v):={φ(v) if vX(0)v if vX.\displaystyle\overline{\varphi}(v):=\begin{cases}\varphi(v)&\text{ if }v\in X^{(0)}\\ v&\text{ if }v\in\partial X\end{cases}.

Here we remark that X(0)¯X(0)=X\overline{X^{(0)}}\setminus X^{(0)}=\partial X since X(0)X^{(0)} is 2-dense in XX.

Lemma 6.3.

The map φ¯:X(0)¯Y¯\overline{\varphi}\colon\overline{X^{(0)}}\to\overline{Y} is continuous at infinity.

Proof..

Let xXx\in\partial X. We show that φ¯\overline{\varphi} is continuous at xx. Let (xn)(x_{n}) be a sequence in X(0)¯\overline{X^{(0)}} converging to xx. We can assume without loss of generality that xnX(0)x_{n}\in X^{(0)} for all nn. We remark (xxn)e(x\mid x_{n})_{e}\to\infty. By (6) of Lemma 4.12, we have

(xφ(xn))eΩmin{(xxn),χ(dX(e,xn))}\displaystyle(x\mid\varphi(x_{n}))_{e}\geq\Omega\min\{(x\mid x_{n}),\chi(d_{X}(e,x_{n}))\}\to\infty

since χ\chi is proper. It follows that (φ(xn))(\varphi(x_{n})) converges to xx. ∎

Let ι:XX(0)\iota\colon X\to X^{(0)} be a restriction such that for xXx\in X, we have dX(x,ι(x))2d_{X}(x,\iota(x))\leq 2. Let j:Yexp(𝒪X)j\colon Y\to\exp(\mathcal{O}\partial X) be a retraction such that, for xYx\in Y, we have dX(x,j(x))D6d_{X}(x,j(x))\leq D_{6}. Here we do not require that ii and jj are continuous. We define a map ι¯:X¯X(0)¯\overline{\iota}\colon\overline{X}\to\overline{X^{(0)}} and j¯:Y¯exp(𝒪X)¯\overline{j}\colon\overline{Y}\to\overline{\exp(\mathcal{O}\partial X)} by

ι¯(v):={ι(v) if vX(0)v if vXandj¯(v):={j(v) if vYv if vX.\displaystyle\overline{\iota}(v):=\begin{cases}\iota(v)&\text{ if }v\in X^{(0)}\\ v&\text{ if }v\in\partial X\end{cases}\quad\text{and}\quad\overline{j}(v):=\begin{cases}j(v)&\text{ if }v\in Y\\ v&\text{ if }v\in\partial X\end{cases}.

By Lemma 6.2, the maps ι¯\overline{\iota} and j¯\overline{j} are continuous at infinity. We define a map Φ:X¯exp(𝒪X)¯\Phi\colon\overline{X}\to\overline{\exp(\mathcal{O}\partial X)} by

Φ(x):={j¯φ¯ι¯(x)if xXxif xX.\displaystyle\Phi(x):=\begin{cases}\overline{j}\circ\overline{\varphi}\circ\overline{\iota}(x)&\text{if }x\in X\\ x&\text{if }x\in\partial X\end{cases}.
Lemma 6.4.

The map Φ:X¯exp(𝒪X)¯\Phi\colon\overline{X}\to\overline{\exp(\mathcal{O}\partial X)} is continuous at infinity.

6.2. Angle map

We define a map arg:exp(𝒪X)¯X\arg\colon\overline{\exp(\mathcal{O}\partial X)}\to\partial X as follows: For xexp(𝒪Xk)x\in\exp(\mathcal{O}\partial X_{k}), we choose (px,tx)Xk×0(p_{x},t_{x})\in\partial X_{k}\times\mathbb{R}_{\geq 0} such that x=rpγ¯(e,px,tx)x=\textup{{rp}}\bar{\gamma}(e,p_{x},t_{x}). Then we define

arg(x)=px.\displaystyle\arg(x)=p_{x}.
Lemma 6.5.

The map arg:exp(𝒪Xk)Xk\arg\colon\exp(\mathcal{O}\partial X_{k})\to\partial X_{k} is continuous at infinity.

We define a map Ψ:X¯X\Psi\colon\overline{X}\to\partial X

Ψ(x):={argΦ(x)if xXxif xX\displaystyle\Psi(x):=\begin{cases}\arg\circ\Phi(x)&\text{if }x\in X\\ x&\text{if }x\in\partial X\end{cases}

By Lemmata 6.4 and 6.5, we have the following.

Proposition 6.6.

The map Ψ:X¯X\Psi\colon\overline{X}\to\partial X is continuous at infinity.

7. Trees of spaces

7.1. Trees of spaces

Definition 7.1.

Let (Z,dZ)(Z,d_{Z}) be a geodesic metric space and TT be a bipartite tree. Set V(T):=KLV(T):=K\sqcup L. Let ξ:ZT\xi\colon Z\to T be a continuous map. We suppose the following:

  1. (1)

    For each lLl\in L, the inverse image ξ1(l)\xi^{-1}(l) consists of a single point.

  2. (2)

    For each kKk\in K, the inverse image Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)) is a geodesic space.

Then we say that ZZ is a tree of spaces associated with the map ξ:ZT\xi\colon Z\to T and the bipartite structure V(T)=KLV(T)=K\sqcup L.

Definition 7.2.

Let (Z,dZ)(Z,d_{Z}) be a tree of spaces associated with the map ξ:ZT\xi\colon Z\to T and the bipartite structure V(T)=KLV(T)=K\sqcup L.

Let E1E^{\prime}\geq 1 and C0C^{\prime}\geq 0 be constants. We suppose that for each kKk\in K, the inverse image Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)) admits an (E,C)(E^{\prime},C^{\prime})-geodesic coarsely convex bicombing

γk:Xk×Xk×[0,1]Xk.\displaystyle\gamma_{k}\colon X_{k}\times X_{k}\times[0,1]\to X_{k}.

Then we say that ZZ is a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex spaces.

Definition 7.3.

We say that a metric space ZZ is a tree of geodesic coarsely convex spaces if ZZ is (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space for some (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K}).

Theorem 7.4 ([10]).

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space. For kKk\in K, set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)).

Then the space ZZ admits an (E,C)(E,C)-geodesic coarsely convex bicombing

γ:Z×Z×[0,1]Z\displaystyle\gamma\colon Z\times Z\times[0,1]\to Z

where E=E+2E=E^{\prime}+2 and C=6CC=6C^{\prime}. The restriction of γ\gamma to Xk×Xk×[0,1]X_{k}\times X_{k}\times[0,1] is equal to γk\gamma_{k}.

Definition 7.5.

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space. We call the bicombing γ\gamma on ZZ constructed in Theorem 7.4 the geodesic coarsely convex bicombing associated with the family {γk}\{\gamma_{k}\}.

Remark 7.6.

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space, and let γ\gamma be the geodesic coarsely convex bicombing on ZZ associated with the family {γk}\{\gamma_{k}\}. For kKk\in K, set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)).

By the construction, it is clear that for each kKk\in K, the subspace XkX_{k} is γ\gamma-convex in ZZ. So by Corollary 5.11, the boundary of XkX_{k} in Z¯\overline{Z} is homeomorphic to Xk\partial X_{k}.

7.2. Free products of metric spaces

In [9], we introduce free products of metric spaces, which can be regarded as trees of metric spaces.

Definition 7.7.

Let (X,dX)(X,d_{X}) be a metric space and let X0X_{0} be a set with the discrete topology. Let iX:X0Xi_{X}:X_{0}\to X be a proper map. We choose a base point eXiX(X0)e_{X}\in i_{X}(X_{0}). We call (X0,iX,eX)(X_{0},i_{X},e_{X}) a net of XX. For x0X0x_{0}\in X_{0}, we denote by x0¯\overline{x_{0}} the image iX(x0)i_{X}(x_{0}). We say that (X,dX,X0,iX,eX)(X,d_{X},X_{0},i_{X},e_{X}) is a metric space with a net.

Remark 7.8.

We often abbreviate specifying a net (X0,iX,eX)(X_{0},i_{X},e_{X}) and say that (X,dX)(X,d_{X}) is a metric space with a net.

Example 7.9.

Let (X,dX,eX)(X,d_{X},e_{X}) be a metric space with a base point eXe_{X}. Let GG be a group acting on XX properly by isometries. We define a map 𝗈𝗋𝖻:GX\mathsf{orb}\colon G\to X by 𝗈𝗋𝖻(g)geX\mathsf{orb}(g)\coloneqq g\cdot e_{X}. Then (G,o(eX),eX)(G,o(e_{X}),e_{X}) is a net of XX, called G-net.

Let (X,dX)(X,d_{X}) and (Y,dY)(Y,d_{Y}) be metric spaces with nets. In [9, Section 1], we constructed the free product XYX*Y of XX and YY. In [10], we constructed a bipartite tree TT and continuous map ξ:XYT\xi\colon X*Y\to T such that XYX*Y is a tree of spaces associated with ξ\xi.

Example 7.10.

Let GG and HH be groups acting on metric spaces XX and YY. We consider a GG-net of XX, and an HH-net of YY, respectively. Then the free product GHG*H acts on XYX*Y properly. If the action of GG and HH are cocompact, then so is the action of GHG*H.

8. Augmented space

8.1. nn-th augmented spaces

Definition 8.1.

Let (Z,dZ)(Z,d_{Z}) be a tree of spaces associated with the map ξ:ZT\xi\colon Z\to T and the bipartite structure V(T)=KLV(T)=K\sqcup L.

For kKk\in K, set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}\colon=\xi^{-1}(\mathsf{star}(k)). We choose an 1-discrete, 2-dense subset Xk(0)XkX_{k}^{(0)}\subset X_{k}. So the pair (Xk,Xk(0))(X_{k},X_{k}^{(0)}) is a space with a lattice. We choose a bijection k:Kk\colon\mathbb{N}\to K.

Let n{0}n\in\mathbb{N}\sqcup\{0\}. The nn-th augmented space An(Z)A_{n}(Z) of ZZ is a tree of spaces associated with the map An(ξ):An(Z)TA_{n}(\xi)\colon A_{n}(Z)\to T satisfying the following:

  1. (1)

    For ii\in\mathbb{N} with ini\leq n, the space An(ξ)1(𝗌𝗍𝖺𝗋(k(i)))A_{n}(\xi)^{-1}(\mathsf{star}(k(i))) is isometric to Xk(i)X_{k(i)}.

  2. (2)

    For ii\in\mathbb{N} with i>ni>n, the space An(ξ)1(𝗌𝗍𝖺𝗋(k(i)))A_{n}(\xi)^{-1}(\mathsf{star}(k(i))) is isometric to the metric horoball (Xk(i),Xk(i)(0))\mathcal{H}(X_{k(i)},X_{k(i)}^{(0)}) of the space with a lattice (Xk(i),Xk(i)(0))(X_{k(i)},X_{k(i)}^{(0)}).

We call 0-th augmented space A0(Z)A_{0}(Z) the augmented space, and we denote by A(Z)A(Z).

Remark 8.2.

In the above definition, the coarse equivalence class of the nn-th augmented space does not depend on the choice of nets Xk(0)X_{k}^{(0)}. Therefore, when we consider nn-th augmented spaces, we implicitly choose nets, and we say that An(Z)A_{n}(Z) is the nn-th augmented space of ZZ, without mentioning nets. We abbreviate (Xk,Xk(0))\mathcal{H}(X_{k},X_{k}^{(0)}) by (Xk)\mathcal{H}(X_{k})

The augmented space A(Z)A(Z) does not depend on the choice of the bijection k:Kk\colon\mathbb{N}\to K.

We can explicitly construct a nn-th augmented space An(Z)A_{n}(Z) from a tree of spaces ZZ by choosing nets and gluing combinatorial horoballs along nets by the way described in Definition 2.5.

8.2. Bicombings on nn-th augmented spaces

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex spaces. Let γ\gamma be the geodesic coarsely convex bicombing associated with the family {γk}\{\gamma_{k}\}. We choose a pair of constants (E,C)(E^{\prime},C^{\prime}) such that γ\gamma is (E,C)(E^{\prime},C^{\prime}) geodesic coarsely convex.

For kKk\in K, set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}\colon=\xi^{-1}(\mathsf{star}(k)). For kKk\in K, we define an (E,C+8δ)(E^{\prime},C^{\prime}+8\delta)-geodesic coarsely convex bicombing An(γk)A_{n}(\gamma_{k}) on An(ξ)1(𝗌𝗍𝖺𝗋(k))=An(Xk)A_{n}(\xi)^{-1}(\mathsf{star}(k))=A_{n}(X_{k}) by the following:

  1. (1)

    if ini\leq n then An(γk(i))=γk(i)A_{n}(\gamma_{k(i)})=\gamma_{k(i)},

  2. (2)

    Suppose i>ni>n. Note that An(Xk(i))A_{n}(X_{k(i)}) is equal to (Xk(i))\mathcal{H}(X_{k(i)}). For x,yAn(Xk(i))x,y\in A_{n}(X_{k(i)}), we define a map

    An(γk(i))(x,y,):[0,1]An(Xk(i))\displaystyle A_{n}(\gamma_{k(i)})(x,y,-)\colon[0,1]\to A_{n}(X_{k(i)})

    to be the normal geodesic segment from xx to yy given in Proposition 2.6.

We choose a bijection k:Kk\colon\mathbb{N}\to K. Let An(Z)A_{n}(Z) be the nn-th augmented space of ZZ . Then An(Z)A_{n}(Z) is a (An(ξ),K,L,{An(γk)}kK)(A_{n}(\xi),K,L,\{A_{n}(\gamma_{k})\}_{k\in K})-tree of geodesic coarsely convex space. Let An(γ)A_{n}(\gamma) be an geodesic coarsely convex bicombing on An(Z)A_{n}(Z) associated with {An(γk)}\{A_{n}(\gamma_{k})\}.

Definition 8.3.

We call the bicombing An(Z)A_{n}(Z) constructed in the above an augmented bicombing associated with the family {γk}kK\{\gamma_{k}\}_{k\in K}.

Remark 8.4.

For ini\leq n, Xk(i)X_{k(i)} is an An(γ)A_{n}(\gamma)-convex subspace, so by Corollary 5.11, Xk(i)\partial X_{k(i)} is a closed subspace of An(Z)\partial A_{n}(Z).

For i>ni>n, (Xk(i))\mathcal{H}(X_{k(i)}) is an An(γ)A_{n}(\gamma)-convex subspace, the boundary (Xk(i))=(Xk(i))¯(Xk(i))\partial\mathcal{H}(X_{k(i)})=\overline{\mathcal{H}(X_{{k(i)}})}\setminus\mathcal{H}(X_{k(i)}) consists of a single point. We call this the center of the horoball (Xk(i))\mathcal{H}(X_{k(i)}), and denote by ck(i)c_{k(i)}.

9. (co)Homology if Ideal boundary of a tree of spaces

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex spaces. We fix a bijection k:Kk\colon\mathbb{N}\to K. Let A(Z)A(Z) be the augmented space of ZZ, and let An(γ)A_{n}(\gamma) be the augmented bicombing on An(Z)A_{n}(Z) associated with the family {γk}kK\{\gamma_{k}\}_{k\in K}.

Remark 9.1.

It is clear that the inclusion ιn:An(Z)An1(Z)\iota_{n}\colon A_{n}(Z)\hookrightarrow A_{n-1}(Z) is a visual map in the sense of Definition 4.13. By Proposition 4.14, it induces a continuous map

ιn:An(Z)An1(Z).\displaystyle\partial\iota_{n}\colon\partial A_{n}(Z)\to\partial A_{n-1}(Z).

The family {An(Z),ιn}\{\partial A_{n}(Z),\partial\iota_{n}\} forms a projective system, and the projective limit is Z\partial Z, that is,

Z=limnAn(Z).\displaystyle\partial Z=\varprojlim_{n}\partial A_{n}(Z).

The following is a key proposition for computing (co)homologies of Z\partial Z.

Proposition 9.2.

For nn\in\mathbb{N}, there exists a continuous retraction

sk(n):An(Z)Xk(n).\displaystyle s_{k(n)}\colon\partial A_{n}(Z)\to\partial X_{k(n)}.

We will prove Proposition 9.2 in Section 10

9.1. Cohomology

Let M=(Mn)nM^{*}=(M^{n})_{n\in\mathbb{N}} be the KK-theory or the Alexander-Spanier cohomology, and let M~\tilde{M}^{*} be the reduced one. For a compact Hausdorff space YY, and eYe\in Y, we have M~(Y)M(Y,{e})\tilde{M}^{*}(Y)\cong M^{*}(Y,\{e\}).

We consider the long exact sequence for the triple (An(Z),Xk(n),{en})(\partial A_{n}(Z),\partial X_{k(n)},\{e_{n}\}).

\displaystyle\dots Mp(An(Z),Xk(n))Mp(An(Z),{en})Mp(Xk(n),{en})\displaystyle\to M^{p}(\partial A_{n}(Z),\partial X_{k(n)})\to M^{p}(\partial A_{n}(Z),\{e_{n}\})\to M^{p}(\partial X_{k(n)},\{e_{n}\})
Mp+1(An(Z),Xk(n))\displaystyle\to M^{p+1}(\partial A_{n}(Z),\partial X_{k(n)})\to\cdots

By Proposition 9.2, the above exact sequence splits, so we have

(2) 0Mp(An(Z),Xk(n))M~p(An(Z))M~p(Xk(n))0\displaystyle 0\to M^{p}(\partial A_{n}(Z),\partial X_{k(n)})\to\tilde{M}^{p}(\partial A_{n}(Z))\to\tilde{M}^{p}(\partial X_{k(n)})\to 0

By the strong excision axiom, we have

Mp(An(Z),Xk(n))\displaystyle M^{p}(\partial A_{n}(Z),\partial X_{k(n)}) Mp((An(Z)Xk(n))+,{ck(n)})\displaystyle\cong M^{p}((\partial A_{n}(Z)\setminus\partial X_{k(n)})^{+},\{c_{k(n)}\})
Mp(An1(Z),{ck(n)})\displaystyle\cong M^{p}(\partial A_{n-1}(Z),\{c_{k(n)}\})
=M~p(An1(Z)).\displaystyle=\tilde{M}^{p}(\partial A_{n-1}(Z)).

Here (An(Z)Xk(n))+(\partial A_{n}(Z)\setminus\partial X_{k(n)})^{+} denotes the one-point compactification

(An(Z)Xk(n)){ck(n)}.\displaystyle(\partial A_{n}(Z)\setminus\partial X_{k(n)})\sqcup\{c_{k(n)}\}.

It follows that M~p(An(Z))M~p(An1(Z))M~p(Xk(n))\tilde{M}^{p}(\partial A_{n}(Z))\cong\tilde{M}^{p}(\partial A_{n-1}(Z))\oplus\tilde{M}^{p}(\partial X_{k(n)}). By the continuity of MM^{*}, we have M~p(Z)limM~p(An(Z))\tilde{M}^{p}(\partial Z)\cong\varinjlim\tilde{M}^{p}(\partial A_{n}(Z)). Here we summarize the computation.

Theorem 9.3.

Let ZZ be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex spaces. Suppose that ZZ is proper. Set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)). Let A(Z)A(Z) be the augmented space of ZZ. Then,

M~p(Z)M~p(A(Z))kKM~p(Xk)\displaystyle\tilde{M}^{p}(\partial Z)\cong\tilde{M}^{p}(\partial A(Z))\oplus\bigoplus_{k\in K}\tilde{M}^{p}(\partial X_{k})

Here we remark that the topological type of A(Z)\partial A(Z) is described in Theorem 11.4.

9.2. Homology

Let M=(Mn)nM_{*}=(M_{n})_{n\in\mathbb{N}} be the KK-homology or the Steenrod homology, and let M~\tilde{M}_{*} be the reduced one. For a compact Hausdorff space XX, and eXe\in X, we have M~(X)M(X,{e})\tilde{M}_{*}(X)\cong M_{*}(X,\{e\}).

Theorem 9.4 ([19, Theorem 4.]).

Let Y1Y2Y3Y_{1}\leftarrow Y_{2}\leftarrow Y_{3}\leftarrow\cdots be an inverse system of compact metric spaces. Then there exists an exact sequence

0lim1Mp+1(Yi)Mp(limYi)limMp(Yi)0.\displaystyle 0\to\varprojlim{\!}^{1}M_{p+1}(Y_{i})\to M_{p}(\varprojlim Y_{i})\to\varprojlim M_{p}(Y_{i})\to 0.

By the same argument as the one in Section 9.1, we obtain

M~p(An(Z))M~p(An1(Z))M~p(Xk(n)).\displaystyle\tilde{M}_{p}(\partial A_{n}(Z))\cong\tilde{M}_{p}(\partial A_{n-1}(Z))\oplus\tilde{M}_{p}(\partial X_{k(n)}).

By Theorem 9.4, we have

0lim1Mp+1(An(Z))Mp(Z)limMp(An(Z))0.\displaystyle 0\to\varprojlim{\!}^{1}M_{p+1}(\partial A_{n}(Z))\to M_{p}(\partial Z)\to\varprojlim M_{p}(\partial A_{n}(Z))\to 0.

By Proposition 9.2, the maps Mp+1(An+1(Z))Mp+1(An(Z))M_{p+1}(\partial A_{n+1}(Z))\to M_{p+1}(\partial A_{n}(Z)) are surjective, so the Mittag-Leffler condition holds. Thus lim1Mp+1(An(Z))\varprojlim{\!}^{1}M_{p+1}(\partial A_{n}(Z)) vanishes.

Theorem 9.5.

Let ZZ be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex spaces. Set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)). Suppose that ZZ is proper. Let A(Z)A(Z) be the augmented space of ZZ. Then,

M~p(Z)M~p(A(Z))×kKM~p(Xk).\displaystyle\tilde{M}_{p}(\partial Z)\cong\tilde{M}_{p}(\partial A(Z))\times\prod_{k\in K}\tilde{M}_{p}(\partial X_{k}).

9.3. KK-theory of the Roe algebra

Let VV be a proper metric space. We denote by C(V)C^{*}(V) the Roe algebra of VV. We also denote by KX(V)KX_{*}(V) the coarse KK-homology of VV. For detail, see [16], [21] and [17].

Suppose that VV is a proper coarsely convex space. By [11, Theorem 1.3], the following coarse assembly map is an isomorphism.

μ:KX(V)K(C(V)).\displaystyle\mu_{*}\colon KX_{*}(V)\to K_{*}(C^{*}(V)).

By [11, Theorem 6.7], the following transgression map is an isomorphism.

TV:KX(V)K~1(V).\displaystyle{T_{\partial V}}\colon KX_{*}(V)\to\tilde{K}_{*-1}(\partial V).

Thus we have an isomorphism

(3) TVμ1:K(C(V))K~1(V).\displaystyle{T_{\partial V}}\circ\mu_{*}^{-1}\colon K_{*}(C^{*}(V))\to\tilde{K}_{*-1}(\partial V).
Theorem 9.6.

Let ZZ be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex spaces. Set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)). Suppose that ZZ is proper. Let A(Z)A(Z) be the augmented space of ZZ. Then,

Kp(C(Z))\displaystyle K_{p}(C^{*}(Z)) K~p1(A(Z))×kKK~p1(Xk)\displaystyle\cong\tilde{K}_{p-1}(\partial A(Z))\times\prod_{k\in K}\tilde{K}_{p-1}(\partial X_{k})
Proof..

Combining Theorem 9.5 for KK-homology with an isomorphism

K(C(Z))K~1(Z)\displaystyle K_{*}(C^{*}(Z))\cong\tilde{K}_{*-1}(\partial Z)

obtained by applying 3 for geodesic coarsely convex space ZZ, we obtain the desired result. ∎

Corollary 9.7.

Let ZZ be the tree of geodesic coarsely convex spaces described in Theorem 9.6. We have

Kp(C(Z))\displaystyle K_{p}(C^{*}(Z)) K~p1(A(Z))×kKKp(C(Xk))\displaystyle\cong\tilde{K}_{p-1}(\partial A(Z))\times\prod_{k\in K}K_{p}(C^{*}(X_{k}))
Proof..

Combining Theorem 9.6 with isomorphisms

K(C(X))K~1(X)andK(C(Y))K~1(Y),\displaystyle K_{*}(C^{*}(X))\cong\tilde{K}_{*-1}(\partial X)\quad\text{and}\quad K_{*}(C^{*}(Y))\cong\tilde{K}_{*-1}(\partial Y),

we obtain the desired result. ∎

9.4. Case of free products

Proof of Theorems 1.1, 1.2 and 1.3.

Let XX and YY be proper geodesic coarsely convex spaces with nets. Suppose that the net of XX and that of YY are coarsely dense in XX and YY, respectively. Let XYX*Y be the free product of XX and YY. Then XYX*Y is a tree of space. Since the net of XX and YY are coarsely dense in XX and YY, respectively, by Theorem 11.4, the ideal boundary A(XY)\partial A(X*Y) of the augmented space has no isolated point. So, A(XY)\partial A(X*Y) is homeomorphic to the Cantor space 𝒞\mathcal{C}. Then applying Theorems 9.3, 9.5, 9.6 and 9.7 for XYX*Y, we obtain the desired result. ∎

10. Construction of retractions

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space. We suppose that ZZ is proper. Let γ\gamma be the geodesic coarsely convex bicombing on ZZ associated with the family {γk}kK\{\gamma_{k}\}_{k\in K}. By Remark 7.6, we can regard Xk\partial X_{k} as a closed subspace of Z\partial Z. The purpose of this section is to construct a retraction sk:ZXks_{k}\colon\partial Z\to\partial X_{k}.

Let kKk\in K. For xZx\in\partial Z, set

t(k;x):=sup{t:rpγ¯(e,x,t)Xk}.\displaystyle t(k;x):=\sup\{t\in\mathbb{R}:\textup{{rp}}\bar{\gamma}(e,x,t)\in X_{k}\}.

We define a map πk:ZXk¯\pi_{k}\colon\partial Z\to\overline{X_{k}} by

πk(x):=rpγ¯(e,x,t(k;x)).\displaystyle\pi_{k}(x):=\textup{{rp}}\bar{\gamma}(e,x,t(k;x)).
Remark 10.1.

For xZXkx\in\partial Z\setminus\partial X_{k}, we have t(k;x)=d(e,rpγ¯(e,x,t(k;x)))t(k;x)=d(e,\textup{{rp}}\bar{\gamma}(e,x,t(k;x))). For xXkx\in\partial X_{k}, we have t(k;x)=t(k;x)=\infty and πk(x)=rpγ¯(e,x,)=x\pi_{k}(x)=\textup{{rp}}\bar{\gamma}(e,x,\infty)=x.

Lemma 10.2.

We fix kKk\in K. Let eXke\in X_{k} be a base point of XkX_{k}, and let v,wXkv,w\in X_{k} such that vwv\neq w. Then for xπk1(v)x\in\pi_{k}^{-1}(v) and yπk1(w)y\in\pi_{k}^{-1}(w), we have

(xy)e<Ω(max{dZ(e,v),dZ(e,w)}+Ω).\displaystyle(x\mid y)_{e}<\Omega(\max\{d_{Z}(e,v),d_{Z}(e,w)\}+\Omega).

Here Ω\Omega is a constant given in Lemma 4.12.

Proof..

We define tt\in\mathbb{R} by

t=max{t(k;x),t(k;y)}+Ω=max{dZ(e,v),dZ(e,w)}+Ω\displaystyle t=\max\{t(k;x),t(k;y)\}+\Omega=\max\{d_{Z}(e,v),d_{Z}(e,w)\}+\Omega

The geodesic from γex(t)\gamma_{e}^{x}(t) to γey(t)\gamma_{e}^{y}(t) is obtained by concatenating γ(γex(t),v,)\gamma(\gamma_{e}^{x}(t),v,-), γ(v,w,)\gamma(v,w,-) and γ(w,γey(t),)\gamma(w,\gamma_{e}^{y}(t),-). So we have

dZ(γex(t),γey(t))\displaystyle d_{Z}(\gamma_{e}^{x}(t),\gamma_{e}^{y}(t)) =dZ(γex(t),v)+dZ(v,w)+dZ(w,γey(t))\displaystyle=d_{Z}(\gamma_{e}^{x}(t),v)+d_{Z}(v,w)+d_{Z}(w,\gamma_{e}^{y}(t))
tt(k;x)+dZ(v,w)+tt(k;y)\displaystyle\geq t-t(k;x)+d_{Z}(v,w)+t-t(k;y)
Ω.\displaystyle\geq\Omega.

Thus by (4) of Lemma 4.12, we have (γexγey)e<t(\gamma_{e}^{x}\mid\gamma_{e}^{y})_{e}<t. Then by (2) of Lemma 4.12, we have (xy)eΩ(γexγey)eΩt(x\mid y)_{e}\leq\Omega(\gamma_{e}^{x}\mid\gamma_{e}^{y})_{e}\leq\Omega t. ∎

Lemma 10.3.

We fix kKk\in K. Let eXke\in X_{k} be a base point of XkX_{k}, and let vXkv\in X_{k}. Then for xXkx\in\partial X_{k} and yπk1(v)y\in\pi_{k}^{-1}(v), we have

(xy)e<Ω(dZ(e,v)+Ω).\displaystyle(x\mid y)_{e}<\Omega(d_{Z}(e,v)+\Omega).

Here Ω\Omega is a constant given in Lemma 4.12.

Proof..

We can prove the lemma by a similar argument as the proof of Lemma 10.2. ∎

Lemma 10.4.

The map πk:ZXk¯\pi_{k}\colon\partial Z\to\overline{X_{k}} is continuous.

Proof..

Let xZx\in\partial Z. We will show that πk\pi_{k} is continuous at xx. First, we suppose that xZXkx\in\partial Z\setminus\partial X_{k}. Set v=πk(x)v=\pi_{k}(x). Then by Lemma 10.2, πk1(v)\pi_{k}^{-1}(v) is an open set. This implies that πk\pi_{k} is continuous at xx.

Now we suppose that xXkx\in\partial X_{k}. We remark that πk(x)=x\pi_{k}(x)=x. For r0r\in\mathbb{R}_{\geq 0}, set Vr[x]:={yX¯:(xy)>r}V_{r}[x]:=\{y\in\overline{X}:(x\mid y)>r\}. The family {Vn[x]:n}\{V_{n}[x]:n\in\mathbb{N}\} forms a system of the fundamental neighborhood of xx. We will show that for each nn\in\mathbb{N}, there exists T0T\in\mathbb{R}_{\geq 0} such that

(4) πk(VT[x])Vn1[πk(x)]=Vn1[x].\displaystyle\pi_{k}(V_{T}[x])\subset V_{n-1}[\pi_{k}(x)]=V_{n-1}[x].

We fix nn\in\mathbb{N}. Set T=ECΩ(n+Ω)T=EC\Omega(n+\Omega). Let yVT[x]y\in V_{T}[x]. Thus (xy)e>T(x\mid y)_{e}>T. Set v=πk(y)v=\pi_{k}(y). By Lemma 10.3, we have

t(k;y)=dZ(e,v)Ω1(xy)eΩ>ECn.\displaystyle t(k;y)=d_{Z}(e,v)\geq\Omega^{-1}(x\mid y)_{e}-\Omega>ECn.

By (4) of Lemma 4.12, we have dZ(γex(T),γey(T))Ωd_{Z}(\gamma_{e}^{x}(T),\gamma_{e}^{y}(T))\leq\Omega. Set TECnT^{\prime}\coloneqq ECn. Then we have

dZ(γey(T),rpγ(e,v,T))\displaystyle d_{Z}(\gamma_{e}^{y}(T^{\prime}),\textup{{rp}}\gamma(e,v,T^{\prime})) EdZ(v,v)+C=C\displaystyle\leq Ed_{Z}(v,v)+C=C

Here we used that γey(t(k;y))=v=rpγ(e,v,t(k;y)))\gamma_{e}^{y}(t(k;y))=v=\textup{{rp}}\gamma(e,v,t(k;y))). We have

dZ(γex(n),rpγ(e,v,n))\displaystyle d_{Z}(\gamma_{e}^{x}(n),\textup{{rp}}\gamma(e,v,n)) 1ECEdZ(γey(T),rpγ(e,v,T))+C\displaystyle\leq\frac{1}{EC}Ed_{Z}(\gamma_{e}^{y}(T^{\prime}),\textup{{rp}}\gamma(e,v,T^{\prime}))+C
C+1.\displaystyle\leq C+1.

It follows that (xv)n(x\mid v)\geq n. Thus v=πk(y)Vn1[x]v=\pi_{k}(y)\in V_{n-1}[x]. Therefore 4 holds. This implies that πk\pi_{k} is continuous at xx. ∎

Let Ψk:Xk¯Xk\Psi_{k}\colon\overline{X_{k}}\to\partial X_{k} be the map constructed in Section 6.2.

Definition 10.5.

We define a retraction sk:ZXks_{k}\colon\partial Z\to\partial X_{k} by

sk=Ψkπk.\displaystyle s_{k}=\Psi_{k}\circ\pi_{k}.
Proposition 10.6.

The map sk:ZXks_{k}\colon\partial Z\to\partial X_{k} is continuous.

Proof..

Let xZx\in\partial Z. We will show that πk\pi_{k} is continuous at xx.

Let xnx_{n} be a sequence in Z\partial Z converging to xx. Since πk\pi_{k} is continuous, the sequence πk(xn)\pi_{k}(x_{n}) converges to πk(x)Xk\pi_{k}(x)\in\partial X_{k}. Then by Proposition 6.6, the sequence (Ψk(πk(xn)))(\Psi_{k}(\pi_{k}(x_{n}))) converges to Ψk(πk(x))\Psi_{k}(\pi_{k}(x)). ∎

Proof of Proposition 9.2.

Applying Proposition 10.6 to the tree of spaces An(Z)A_{n}(Z) associated with the map An(ξ):An(Z)TA_{n}(\xi)\colon A_{n}(Z)\to T, we obtain the desired result. ∎

11. Ideal boundaries of the augmented spaces

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space. We suppose that ZZ is proper.

Let A(Z)A(Z) be the augmented space of ZZ. For simplicity, we denote by γ\gamma an augmented bicombing on A(Z)A(Z) associated with the family {γk}kK\{\gamma_{k}\}_{k\in K}.

For xA(Z)¯x\in\overline{A(Z)}, set Wn[x]={yA(Z):(γexγey)en}W_{n}[x]=\{y\in\partial A(Z):(\gamma_{e}^{x}\mid\gamma_{e}^{y})_{e}\geq n\}. Recall that 𝖼𝗈𝗆𝖻(Xk(0))(0)\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)} denotes the vertex set of the combinatorial horoball 𝖼𝗈𝗆𝖻(Xk(0))\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)}). We consider the family

𝒯:=kK{Wn[x]:x𝖼𝗈𝗆𝖻(Xk(0))(0),n}.\displaystyle\mathcal{T}:=\bigsqcup_{k\in K}\{W_{n}[x]:x\in\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)},n\in\mathbb{N}\}.

Since ZZ is proper, for any bounded subset BZB\subset Z, the cardinality of the set BXk(0)B\cap X_{k}^{(0)} is finite. It follows that 𝒯\mathcal{T} is countable.

Lemma 11.1.

The family 𝒯\mathcal{T} is a countable family of open basis of A(Z)\partial A(Z).

Proof..

We have already seen that 𝒯\mathcal{T} is countable. Let xA(Z)x\in\partial A(Z), and nn\in\mathbb{N}. We will show that there exists U𝒯U\in\mathcal{T} such that

xUVn[x]A(Z).\displaystyle x\in U\subset V_{n}[x]\cap\partial A(Z).

We choose t0t\in\mathbb{R}_{\geq 0} such that:

t\displaystyle t 4EΩ3n+2,\displaystyle\geq 4E{\Omega^{3}}n+2,
rpγ¯(e,x,t)\displaystyle\textup{{rp}}\bar{\gamma}(e,x,t) =γex(t)(Xk,Xk(0)) for some kK.\displaystyle=\gamma_{e}^{x}(t)\in\mathcal{H}(X_{k},X_{k}^{(0)})\text{ for some }k\in K.

There exists x𝖼𝗈𝗆𝖻(Xk(0))(0)x^{\prime}\in\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)} such that dA(Z)(γex(t),x)2d_{A(Z)}(\gamma_{e}^{x}(t),x^{\prime})\leq 2 since 𝖼𝗈𝗆𝖻(Xk(0))(0)\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)} is 2-dense in (Xk,Xk(0))\mathcal{H}(X_{k},X_{k}^{(0)}). By Lemma 5.8, we have

(γex(t)x)\displaystyle(\gamma_{e}^{x}(t)\mid x^{\prime}) min{dA(Z)(e,γex(t)),dA(Z)(e,x)}2EdA(Z)(γex(t),x)t24E.\displaystyle\geq\frac{\min\{d_{A(Z)}(e,\gamma_{e}^{x}(t)),\,d_{A(Z)}(e,x^{\prime})\}}{2Ed_{A(Z)}(\gamma_{e}^{x}(t),x^{\prime})}\geq\frac{t-2}{4E}.

So

(γexx)\displaystyle(\gamma_{e}^{x}\mid x^{\prime}) Ω1min{(γexγex(t)),(γex(t)x)}t24EΩΩ2n.\displaystyle\geq\Omega^{-1}\min\{(\gamma_{e}^{x}\mid\gamma_{e}^{x}(t)),(\gamma_{e}^{x}(t)\mid x^{\prime})\}\geq\frac{t-2}{4E\Omega}\geq\Omega^{2}n.

Then for all yWt[x]y\in W_{t}[x^{\prime}],

(xy)Ω2min{(xγex),(γexx),(xy)}n.\displaystyle(x\mid y)\geq\Omega^{-2}\min\{(x\mid\gamma_{e}^{x}),(\gamma_{e}^{x}\mid x^{\prime}),(x^{\prime}\mid y)\}\geq n.

Here we used that (xy)(γexγey)tn(x^{\prime}\mid y)\geq(\gamma_{e}^{x^{\prime}}\mid\gamma_{e}^{y})\geq t\geq n. Therefore xWt[x]Vn[x]A(Z)x\in W_{t}[x^{\prime}]\subset V_{n}[x]\cap\partial A(Z). This implies that 𝒯\mathcal{T} is an open basis of A(Z)\partial A(Z).∎

Lemma 11.2.

Each W𝒯W\in\mathcal{T} is a clopen set.

Proof..

Let kKk\in K. Let x𝖼𝗈𝗆𝖻(Xk(0))(0)x\in\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)} and nn\in\mathbb{N}. We will show that Wn[x]W_{n}[x] is closed. Let yA(Z)Wn[x]y\in\partial A(Z)\setminus W_{n}[x]. We will show that there exists T>0T>0 such that

W2T[y]A(Z)Wn[x].\displaystyle W_{2T}[y]\subset\partial A(Z)\setminus W_{n}[x].

For pA(Z)p\in\partial A(Z), set

s(k;p):=inf{t:rpγ¯(e,p,t)Xk(0)},t(k;p):=sup{t:rpγ¯(e,p,t)Xk}\displaystyle s(k;p):=\inf\{t\in\mathbb{R}:\textup{{rp}}\bar{\gamma}(e,p,t)\in X_{k}^{(0)}\},\quad t(k;p):=\sup\{t\in\mathbb{R}:\textup{{rp}}\bar{\gamma}(e,p,t)\in X_{k}\}

Here we use the convention that inf=\inf\emptyset=\infty and sup=\sup\emptyset=-\infty. First, we suppose y=ck𝖼𝗈𝗆𝖻(Xk(0))(0)¯y=c_{k}\in\overline{\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)}}. Then s(k;y)<s(k;y)<\infty and t(k;y)=t(k;y)=\infty. We remark that the geodesic rpγ¯(γey(s(k;y)),y,)\textup{{rp}}\bar{\gamma}(\gamma_{e}^{y}(s(k;y)),y,-) consists of vertical line in (Xk,Xk(0))\mathcal{H}(X_{k},X_{k}^{(0)}). Let hh be the depth of xx in 𝖼𝗈𝗆𝖻(Xk(0))(0)\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)}. Set T:=h+s(k;y)+n+D1T:=h+s(k;y)+n+D_{1}. Let yW2T[y]y^{\prime}\in W_{2T}[y]. We have

rpγ¯(e,y,t)=rpγ¯(e,y,t)(t[0,T]).\displaystyle\textup{{rp}}\bar{\gamma}(e,y,t)=\textup{{rp}}\bar{\gamma}(e,y^{\prime},t)\qquad(\forall t\in[0,T]).

See fig. 1. If yWn[x]y^{\prime}\in W_{n}[x], then

dZ(γex(n),rpγ¯(e,y,n))=dZ(γex(n),rpγ¯(e,y,n))D1\displaystyle d_{Z}(\gamma_{e}^{x}(n),\textup{{rp}}\bar{\gamma}(e,y,n))=d_{Z}(\gamma_{e}^{x}(n),\textup{{rp}}\bar{\gamma}(e,y^{\prime},n))\leq D_{1}

Thus (γxxγey)n(\gamma_{x}^{x}\mid\gamma_{e}^{y})\geq n. This contradicts yWn[x]y\notin W_{n}[x]. Therefore yWn[x]y^{\prime}\notin W_{n}[x], so we have W2T[y]Wn[x]=W_{2T}[y]\cap W_{n}[x]=\emptyset.

Next, we suppose y𝖼𝗈𝗆𝖻(Xk(0))(0)¯y\notin\overline{\mathcal{H}_{\mathsf{comb}}(X_{k}^{(0)})^{(0)}}. If s(k;y)=s(k;y)=\infty, then set T=2n+D1T=2n+D_{1}. it is easy to see that W2T[y]Wn[x]=W_{2T}[y]\cap W_{n}[x]=\emptyset. If s(k;y)<s(k;y)<\infty, then set T=t(k;y)+2n+D1T=t(k;y)+2n+D_{1}. For yW2T[y]y^{\prime}\in W_{2T}[y], we have

rpγ¯(e,y,t)=rpγ¯(e,y,t)(t[0,T]).\displaystyle\textup{{rp}}\bar{\gamma}(e,y,t)=\textup{{rp}}\bar{\gamma}(e,y^{\prime},t)\qquad(\forall t\in[0,T]).

See fig. 2. Then by a similar argument as before, yWn[x]y^{\prime}\notin W_{n}[x]. Therefore W2T[y]Wn[x]=W_{2T}[y]\cap W_{n}[x]=\emptyset.

XkX_{k}y=cky=c_{k}eeyy^{\prime}γey(s(k;y)+h)\gamma_{e}^{y}(s(k;y)+h)γey(s(k;y))\gamma_{e}^{y}(s(k;y))
Figure 1. geodesics γey\gamma_{e}^{y} and γey\gamma_{e}^{y^{\prime}} where y=cky=c_{k}
XkX_{k}eeyyyy^{\prime}γey(s(k;y))\gamma_{e}^{y}(s(k;y))
Figure 2. geodesics γey\gamma_{e}^{y} and γey\gamma_{e}^{y^{\prime}} where ycky\neq c_{k}

Lemma 11.3.

Let kKk\in K. The center ckc_{k} of the horoball (Xk)\mathcal{H}(X_{k}) is an isolated point if and only if Xkξ1(L)X_{k}\cap\xi^{-1}(L^{\circ}) is bounded, where LL^{\circ} denotes a set of vertices lLl\in L which adjacent to at least two different vertices in KK.

Proof..

For pA(Z)p\in\partial A(Z), set

t(k;p):=sup{t:rpγ¯(e,p,t)Xk}.\displaystyle t(k;p):=\sup\{t\in\mathbb{R}:\textup{{rp}}\bar{\gamma}(e,p,t)\in X_{k}\}.

First, we suppose that ckc_{k} is an accumulation point. Thus there exists a sequence (xn)(x_{n}) in A(Z){ck}\partial A(Z)\setminus\{c_{k}\} converging to ckc_{k}. Then we see that t(k;xn)t(k;x_{n})\to\infty. We remark that rpγ¯(e,xn,t(k;xn))Xkξ1(L)\textup{{rp}}\bar{\gamma}(e,x_{n},t(k;x_{n}))\in X_{k}\cap\xi^{-1}(L^{\circ}). Therefore Xkξ1(L)X_{k}\cap\xi^{-1}(L^{\circ}) is unbounded.

Next, we suppose that Xkξ1(L)X_{k}\cap\xi^{-1}(L^{\circ}) is unbounded. Then there exists an unbounded sequence (vn)(v_{n}) in Xkξ1(L)X_{k}\cap\xi^{-1}(L^{\circ}). By the definition of LL^{\circ}, for each vnv_{n}, there exists knK{k}k_{n}\in K\setminus\{k\} which adjacent to ξ(vn)\xi(v_{n}). Then we see that cknc_{k_{n}} converges to ckc_{k}. See fig. 3

XkX_{k}ckc_{k}eev1v_{1}ck1c_{k_{1}}v2v_{2}ck2c_{k_{2}}v3v_{3}ck3c_{k_{3}}
Figure 3. cknc_{k_{n}} converges to ckc_{k}

Theorem 11.4.

Let ZZ be a tree of geodesic coarsely convex spaces, and let A(Z)A(Z) be the augmented space of ZZ.

  1. (1)

    Let A(Z)𝗂𝗌𝗈\partial A(Z)_{\mathsf{iso}} denote the set of isolated points in A(Z)\partial A(Z).

    A(Z)𝗂𝗌𝗈={ck:kK,Xkξ1(L) is bounded }\displaystyle\partial A(Z)_{\mathsf{iso}}=\{c_{k}:k\in K,\ X_{k}\cap\xi^{-1}(L^{\circ})\text{ is bounded }\}
  2. (2)

    If A(Z)\partial A(Z) has no isolated point, then A(Z)\partial A(Z) is the Cantor space.

Proof..

By Lemma 11.3,

A(Z)𝗂𝗌𝗈{ck:kK}={ck:kK,Xkξ1(L) is bounded }.\displaystyle\partial A(Z)_{\mathsf{iso}}\cap\{c_{k}:k\in K\}=\{c_{k}:k\in K,\ X_{k}\cap\xi^{-1}(L)\text{ is bounded }\}.

Let xA(Z)𝗂𝗌𝗈{ck:kK}x\in\partial A(Z)_{\mathsf{iso}}\setminus\{c_{k}:k\in K\}. Then there exists a sequence {tn}0\{t_{n}\}\subset\mathbb{R}_{\geq 0} and {kn}K\{k_{n}\}\subset K such that rpγ¯(e,x,tn)Xkn\textup{{rp}}\bar{\gamma}(e,x,t_{n})\in X_{k_{n}} for all nn\in\mathbb{N}, and knkmk_{n}\neq k_{m} for all nmn\neq m. Then a sequence {ck}\{c_{k}\} converges to xx. Thus (1) holds.

By Lemmata 11.1 and 11.2, A(Z)\partial A(Z) has countable bases consisting of clopen sets. Thus, if A(Z)\partial A(Z) has no isolated points, A(Z)\partial A(Z) is homeomorphic to the Cantor space by [4]. ∎

Remark 11.5.

It is known by [1, Lemma 4.6(2)] that the augmented space A(Z)A(Z) is a Gromov hyperbolic space. The ideal boundary of A(Z)A(Z) constructed by the geodesic bicombing coincides with the Gromov boundary of A(Z)A(Z) as a Gromov hyperbolic space.

12. Topological dimension of ideal boundaries

In this section, we study the topological dimensions of ideal boundaries of trees of spaces. Then we compare the results with a well-known formula for the cohomological dimension of free products of groups.

12.1. Topological dimension

Theorem 12.1.

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space. Suppose that ZZ is proper. For kKk\in K, set Xk:=ξ1(𝗌𝗍𝖺𝗋(k))X_{k}:=\xi^{-1}(\mathsf{star}(k)). Then,

dim(Z)=sup{dim(Xk):kK}.\displaystyle\mathop{\mathrm{dim}}\nolimits(\partial Z)=\sup\{\mathop{\mathrm{dim}}\nolimits(\partial X_{k}):k\in K\}.

Theorem 1.4 is obtained by applying Theorem 12.1 to free products of metric spaces.

Let (Z,dZ)(Z,d_{Z}) be a (ξ,K,L,{γk}kK)(\xi,K,L,\{\gamma_{k}\}_{k\in K})-tree of geodesic coarsely convex space. We fix a bijection k:Kk\colon\mathbb{N}\to K. Let A(Z)A(Z) be the augmented space of ZZ.

For simplicity, we denote by γ\gamma an augmented bicombing on An(Z)A_{n}(Z) associated with the family {γk}kK\{\gamma_{k}\}_{k\in K}.

Lemma 12.2.

Let An(Z)A_{n}(Z) be the nn-th augmented space as above.

dimAn(Z)max{dimXk(i):1in}.\displaystyle\mathop{\mathrm{dim}}\nolimits\partial A_{n}(Z)\leq\max\{\mathop{\mathrm{dim}}\nolimits\partial X_{k(i)}:1\leq i\leq n\}.
Proof..

We suppose that N:=max{dimXk(i):1in}<N:=\max\{\mathop{\mathrm{dim}}\nolimits\partial X_{k(i)}:1\leq i\leq n\}<\infty. Let 𝒰={Uα}αΛ\mathcal{U}=\{U_{\alpha}\}_{\alpha\in\Lambda} be a finite open cover of An(Z)\partial A_{n}(Z). We can suppose without loss of generality that 𝒰\mathcal{U} consists of fundamental neighbourhoods, that is, for αΛ\alpha\in\Lambda, there exists (xα,nα)An(Z)(x_{\alpha},n_{\alpha})\in A_{n}(Z)\cup\mathbb{N} such that

Uα=Vnα[xα]An(Z)={yAn(Z):(xy)>nα}.\displaystyle U_{\alpha}=V_{n_{\alpha}}[x_{\alpha}]\cap\partial A_{n}(Z)=\{y\in\partial A_{n}(Z):(x\mid y)>n_{\alpha}\}.

Furthermore, since An(Z)A_{n}(Z) is normal, and each Xk(i)\partial X_{k(i)} is closed, we can assume that for each αΛ\alpha\in\Lambda, there exists at most one i{1,,n}i\in\{1,\dots,n\} such that UαXk(i)U_{\alpha}\cap\partial X_{k(i)}\neq\emptyset. Set

Λi\displaystyle\Lambda_{i} :={α:UαXk(i)}\displaystyle:=\{\alpha:U_{\alpha}\cap\partial X_{k(i)}\neq\emptyset\}
Wi\displaystyle W_{i} :=αΛiUα.\displaystyle:=\bigcup_{\alpha\in\Lambda_{i}}U_{\alpha}.

We can assume that for iii\neq i^{\prime} and for αΛi\alpha\in\Lambda_{i} and αΛi\alpha^{\prime}\in\Lambda_{i^{\prime}}, we have

(5) Uα¯Uα¯=.\displaystyle\overline{U_{\alpha}}\cap\overline{U_{\alpha^{\prime}}}=\emptyset.

By taking a common refinement of the cover {Uα:αΛi}\{U_{\alpha}:\alpha\in\Lambda_{i}\} and {Vn[x]:(x,n)Xk(n)×}\{V_{n}[x]:(x,n)\in X_{k(n)}\times\mathbb{N}\}, we can assume that for αΛi\alpha\in\Lambda_{i}, we have (xα,nα)Xk(n)×(x_{\alpha},n_{\alpha})\in X_{k(n)}\times\mathbb{N}.

Since dimXk(i)N\mathop{\mathrm{dim}}\nolimits\partial X_{k(i)}\leq N, the cover {Uα:αΛi}\{U_{\alpha}:\alpha\in\Lambda_{i}\} has a refinement 𝒱i\mathcal{V}_{i} of order N+1N+1.

Now set

Fi:=αΛiUα=V𝒱iV,\displaystyle F_{i}:=\bigcup_{\alpha\in\Lambda_{i}}U_{\alpha}=\bigcup_{V\in\mathcal{V}_{i}}V, Z:=An(Z)(1inFi)\displaystyle Z^{\prime}:=A_{n}(Z)\setminus\left(\bigcup_{1\leq i\leq n}F_{i}\right)

Since FiF_{i}’s are open, ZZ^{\prime} is closed, so ZZ^{\prime} is a compact metrizable space.

Claim 12.3.

For each i=1,,ni=1,\dots,n, FiF_{i} is closed. Thus ZZ^{\prime} is open.

We will show the claim by a similar argument as in the proof of Lemma 11.2.

Let xAn(Z)Fix\in\partial A_{n}(Z)\setminus F_{i}. We will show that there exists Tx>0T_{x}>0 such that VTx[x]Fi=V_{T_{x}}[x]\cap F_{i}=\emptyset. Since Λi\Lambda_{i} is a finite set, it is enough to show that for each αΛi\alpha\in\Lambda_{i}, there exists Tx,α>0T_{x,\alpha}>0 such that V2Tx,α[x]Uα=V_{2T_{x,\alpha}}[x]\cap U_{\alpha}=\emptyset. We remark that Uα=Vnα[xα]U_{\alpha}=V_{n_{\alpha}}[x_{\alpha}] with (xα,nα)Xk×(x_{\alpha},n_{\alpha})\in X_{k}\times\mathbb{N}.

For k=k(i)Kk=k(i)\in K with ini\geq n, let ck=ck(i)c_{k}=c_{k(i)} be the center of the horoball (Xk)\mathcal{H}(X_{k}). First, we suppose that x=ckx=c_{k} for some kKk\in K. Set

s(k;x):=inf{t:rpγ¯(e,x,t)Xk(0)}.\displaystyle s(k;x):=\inf\{t\in\mathbb{R}:\textup{{rp}}\bar{\gamma}(e,x,t)\in X_{k}^{(0)}\}.

The geodesic rpγ¯(γex(s(k;x)),x,)\textup{{rp}}\bar{\gamma}(\gamma_{e}^{x}(s(k;x)),x,-) consists of the vertical line. Set Tx,α:=s(k;x)+4D1+nαT_{x,\alpha}:=s(k;x)+4D_{1}+n_{\alpha}. Then for yV2Tx,α[x]y\in V_{2T_{x,\alpha}}[x], we have

rpγ¯(e,x,t)=rpγ¯(e,y,t)(t[0,Tx,α])\displaystyle\textup{{rp}}\bar{\gamma}(e,x,t)=\textup{{rp}}\bar{\gamma}(e,y,t)\quad(\forall t\in[0,T_{x,\alpha}])

If yUα=Vnα[xα]y\in U_{\alpha}=V_{n_{\alpha}}[x_{\alpha}], then

dZ(rpγ¯(e,xα,nα),rpγ¯(e,x,nα))=dZ(rpγ¯(e,xα,nα),rpγ¯(e,y,nα))D1\displaystyle d_{Z}(\textup{{rp}}\bar{\gamma}(e,x_{\alpha},n_{\alpha}),\textup{{rp}}\bar{\gamma}(e,x,n_{\alpha}))=d_{Z}(\textup{{rp}}\bar{\gamma}(e,x_{\alpha},n_{\alpha}),\textup{{rp}}\bar{\gamma}(e,y,n_{\alpha}))\leq D_{1}

Thus (xxα)enα(x\mid x_{\alpha})_{e}\geq n_{\alpha}. This contradicts xUαx\notin U_{\alpha}. Therefore yUαy\notin U_{\alpha}, so we have

V2Tx,α[x]Uα=.\displaystyle V_{2T_{x,\alpha}}[x]\cap U_{\alpha}=\emptyset.

Next, we suppose xckx\neq c_{k} for all kKk\in K. Then there exists kKk\in K such that

s(k;x):=inf{t:rpγ¯(e,x,t)Xk}\displaystyle s(k;x):=\inf\{t\in\mathbb{R}:\textup{{rp}}\bar{\gamma}(e,x,t)\in X_{k}\}

is finite, and dZ(rpγ¯(e,x,s(k;x)),xα)>2nαd_{Z}(\textup{{rp}}\bar{\gamma}(e,x,s(k;x)),x_{\alpha})>2n_{\alpha}. Set Tx,α=2(s(k;x)+nα+D1)T_{x,\alpha}=2(s(k;x)+n_{\alpha}+D_{1}). Then for all yVTx,α[x]y\in V_{T_{x,\alpha}}[x], we have

rpγ¯(e,x,t)=rpγ¯(e,y,t)(t[0,nx,α])\displaystyle\textup{{rp}}\bar{\gamma}(e,x,t)=\textup{{rp}}\bar{\gamma}(e,y,t)\quad(\forall t\in[0,n_{x,\alpha}])

By the same argument as before, yUαy\notin U_{\alpha}, so we have V2Tx,α[x]Uα=V_{2T_{x,\alpha}}[x]\cap U_{\alpha}=\emptyset. This completes a proof of the claim.

Now by a similar argument as in Section 11, we see that ZZ^{\prime} has countable bases consisting of clopen sets. Thus ZZ^{\prime} is zero dimensional. So the open cover

{UαZ:αΛi, 1in}\displaystyle\{U_{\alpha}\cap Z^{\prime}:\alpha\notin\Lambda_{i},\,1\leq i\leq n\}

has a refinement 𝒱\mathcal{V}_{\infty} of order 11. It follow that 𝒰\mathcal{U} has a refinement 𝒱i𝒱i\mathcal{V}\cup\bigcup_{i}\mathcal{V}_{i} of order N+1N+1. Thus dimAn(Z)N\mathop{\mathrm{dim}}\nolimits\partial A_{n}(Z)\leq N. ∎

Proof of Theorem 12.1.

Since each Xk\partial X_{k} is a closed subset, we have

dim(Z)sup{dim(Xk):kK}.\displaystyle\mathop{\mathrm{dim}}\nolimits(\partial Z)\geq\sup\{\mathop{\mathrm{dim}}\nolimits(\partial X_{k}):k\in K\}.

By a formula for the topological dimensions of projective limits in [18], we have

dim(Z)supndimAn(Z).\displaystyle\mathop{\mathrm{dim}}\nolimits(\partial Z)\leq\sup_{n}\mathop{\mathrm{dim}}\nolimits\partial A_{n}(Z).

By Lemma 12.2, we have

supndimAn(Z)supndimXk(n).\displaystyle\sup_{n}\mathop{\mathrm{dim}}\nolimits\partial A_{n}(Z)\leq\sup_{n}\mathop{\mathrm{dim}}\nolimits\partial X_{k(n)}.

This completes the proof. ∎

12.2. Comparison with the formula for cohomological dimensions of groups

We remark that Theorem 1.4 is an analogue of a well-known formula for the cohomological dimensions of free products. For a group GG, we denote by cdG\operatorname{cd}G the cohomological dimension of GG. By [5, VIII (2.4) Proposition, (a) and (c)] we have the following.

Theorem 12.4 ([5]).

Let GG and HH be groups. Let GHG*H be the free product of GG and HH. Then we have

cd(GH)=max{cdG,cdH}.\displaystyle\operatorname{cd}(G*H)=\max\{\operatorname{cd}G,\operatorname{cd}H\}.

The following theorem relates the cohomological dimensions of group GG acting coarsely convex space XX and the topological dimension of the ideal boundary X\partial X.

Theorem 12.5 ([11, Corollary 8.10]).

Let GG be a group acting geometrically on a proper coarsely convex space XX. If GG admits a finite model for the classifying space BGBG, then

cdG=dimX+1.\displaystyle\operatorname{cd}G=\mathop{\mathrm{dim}}\nolimits\partial X+1.

Let GG and HH be groups acting on geodesic coarsely convex spaces XX and YY respectively. Suppose GG and HH admit finite models for the classifying spaces BGBG and BHBH respectively. In this case, dim(XY)\mathop{\mathrm{dim}}\nolimits\partial(X*Y) can be computed by Theorem 12.4 as follows.

By Theorem 12.5,

cd(G)=dimX+1,cd(H)=dimY+1.\displaystyle\operatorname{cd}(G)=\mathop{\mathrm{dim}}\nolimits\partial X+1,\quad\operatorname{cd}(H)=\mathop{\mathrm{dim}}\nolimits\partial Y+1.

Since the free product GHG*H is hyperbolic relative to {G,H}\{G,H\}, by [11, Theorem A.1.], GHG*H admits a finite model for the classifying spaces B(GH)B(G*H). By Example 7.10, GHG*H acts on XYX*Y geometrically, so using Theorem 12.5 again,

cd(GH)=dim((XY))+1.\displaystyle\operatorname{cd}(G*H)=\mathop{\mathrm{dim}}\nolimits(\partial(X*Y))+1.

Therefore by Theorem 12.4, we have

dim((XY))=max{dimX,dimY}.\displaystyle\mathop{\mathrm{dim}}\nolimits(\partial(X*Y))=\max\{\mathop{\mathrm{dim}}\nolimits\partial X,\mathop{\mathrm{dim}}\nolimits\partial Y\}.

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