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Sublinearly Morse geodesics in CAT(0) spaces: lower divergence and hyperplane characterization

Devin Murray Department of Mathematics, University of Hawaii at Manoa, Hawaii, Hawaii murray@math.hawaii.edu Yulan Qing Shanghai Center for Mathematical Sciences, Fudan University, Shanghai yulan.qing@gmail.com  and  Abdul Zalloum Department of Mathematics, Queen’s University, Kingston, ON az32@queensu.ca
Abstract.

We introduce the notion of κ\kappa-lower divergence for geodesic rays in CAT(0) spaces. Building on work of Charney and Sultan we give various characterizations of κ\kappa-contracting geodesic rays using κ\kappa-lower divergence and κ\kappa-slim triangles. We also characterize κ\kappa-contracting geodesic rays in CAT(0) cube complexes using sequences of well-separated hyperplanes.

1. Introduction

The Gromov boundary [Gro87] has been widely used in studying algebraic, geometric, and dynamic properties of hyperbolic groups (surveyed by Kapovich and Benakli in [KB02]). In recent years, a significant amount of effort has been put into studying several different notions of “hyperbolic-like” geodesics which arise naturally in spaces which are not δ\delta-hyperbolic, but still captures some of the essence of the coarse geometry of δ\delta-hyperbolic spaces.

Three well-studied properties for geodesic rays in hyperbolic spaces are super linear lower-divergence, the uniformly contracting property, and the δ\delta-slim property. Charney and Sultan showed that, in a CAT(0) space, these properties all characterize Morse geodesics [CS15]. These properties are all widely used tools to study CAT(0) groups (see [CS11], [Ham09], [BB08],[BF09], [Mur19], [BC11] for a sampling). One of the downsides is that contracting geodesics are generally quite rare regardless of the method used to measure them, for the details on random walks see Cordes, Dussaule and Gekhtman[CDG20].

A weaker notion of a “hyperbolic-like” geodesic is that of a κ\kappa-contracting geodesic. Let κ\kappa be a sublinear function, a geodesic ray bb is said to be κ\kappa-contracting if there exists a constant 𝖼0{\sf c}\geq 0 such that projections of any disjoint ball Br(x)B_{r}(x) to bb have diameter bounded above by 𝖼κ(x),{\sf c}\kappa(||x||), where x=d(b(0),x).||x||=d(b(0),x). In [QRT19], Qing, Tiozzo and Rafi showed that the collection of κ\kappa-contracting geodesic rays can be used to define a boundary at infinity with some nice properties. In particular, the κ\kappa-contracting boundary serves as a topological model of the Poisson boundary for right-angled Artin groups. Furthermore, it was recently announced by Gekhtman, Qing and Rafi [GQR] that κ\kappa-contracting geodesics are generic in rank-1 CAT(0) spaces in various natural measures.

However, κ\kappa-contracting geodesics are still not very well studied.

1.1. Statement of Results.

In this paper we provide several new characterizations of κ\kappa-contracting geodesics. Let bb be a geodesic ray and fix some r>0r>0 and then t>rκ(t)t>r\kappa(t). Let ρκ(r,t)\rho_{\kappa}(r,t) denote the infimum of the lengths of all paths from b(trκ(t))b(t-r\kappa(t)) to b(t+rκ(t))b(t+r\kappa(t)) which lie outside the open ball of radius rκ(t)r\kappa(t) about b(t)b(t). See Figure 1. Given such a geodesic ray bb, we define the κ\kappa-lower divergence of bb to be growth rate of the function

divκ(r):=inft>rκ(t)ρκ(r,t)κ(t).div_{\kappa}(r):=\underset{t>r\kappa(t)}{\text{inf}}\,\,\frac{\rho_{\kappa}(r,t)}{\kappa(t)}.
𝔬{\mathfrak{o}}bbrκ(t)r\kappa(t)
Figure 1. Definition of κ\kappa-lower divergence.
Theorem A.

For a geodesic ray bb in a CAT(0) space. The following are equivalent:

  1. (1)

    The geodesic bb is κ\kappa-contracting.

  2. (2)

    The κ\kappa-lower divergence of bb is superlinear.

  3. (3)

    The κ\kappa-lower divergence of bb is at least quadratic.

  4. (4)

    The geodesic bb is κ\kappa-slim.

We also give a combinatorial characterization of κ\kappa-contracting geodesic rays in the context of CAT(0) cube complexes. In this setting, the combinatorial structure of a CAT(0) cube complex makes it possible to characterize the Morse and contracting properties of a geodesic ray without reference to projections of balls or wandering quasi-geodesic segments. Two disjoint hyperplanes h1,h2h_{1},h_{2} are said to be kk-well-separated if each collection of hyperplanes intersecting both h1,h2h_{1},h_{2}, which contains no facing triples, has at most cardinality kk. A facing triple is a collection of three disjoint hyperplanes, none of which separates the other two.

Theorem B.

Let XX be a locally finite CAT(0) cube complex. A geodesic ray bXb\in X is κ\kappa-contracting if and only if there exists 𝖼>0{\sf c}>0 such that bb crosses an infinite sequence of hyperplanes h1,h2,h_{1},h_{2},... at points b(ti)=bhib(t_{i})=b\cap h_{i} satisfying:

  1. (1)

    d(ti,ti+1)𝖼κ(ti+1).d(t_{i},t_{i+1})\leq{\sf c}\kappa(t_{i+1}).

  2. (2)

    hi,hi+1h_{i},h_{i+1} are 𝖼κ(ti+1){\sf c}\kappa(t_{i+1})-well-separated.

Furthermore, if XX is a cocompact CAT(0) cube complex which has a factor system in the sense of [BHS17], then condition (2) can be replaced with a uniform constant 𝖼{\sf c}^{\prime}.

We remark that Theorem B does not assume that XX is uniformly locally finite. In [Gen20b], Genevois introduced a collection of Gromov hyperbolic metric spaces (Yn,dn)(Y_{n},d_{n}) which generalize the contact graph, see Subsection 4.5. As an application to Theorem B, we show the following.

Corollary C.

Let XX be a cocompact CAT(0) cube complex with a factor system. There exists a Gromov hyperbolic space (Y,dY)(Y,d_{Y}) and a projection map p:XYp:X\rightarrow Y such that for any κ\kappa-contracting geodesic ray bb, we have dY(p(b(0)),p(b(t)))t𝖽1κ(t)𝖽2d_{Y}(p(b(0)),p(b(t)))\geq\frac{t}{{\sf d}_{1}\kappa(t)}-{\sf d}_{2} for some constants 𝖽1,𝖽2{\sf d}_{1},{\sf d}_{2} depending only on bb. In particular, κ\kappa-contracting geodesic rays project to infinite diameter subsets of Y.Y. Furthermore, when XX is the Salvetti complex of a right-angled Artin group, the space YY is the contact graph of XX.

1.2. Separated vs well-separated hyperplanes

In a CAT(0)\operatorname{CAT}(0) cube complex there are many kinds of “separation” type properties. Two hyperplanes h1,h2h_{1},h_{2} are said to be kk-separated if the number of hyperplanes crossing them both is bounded above by kk. They are kk-well-separated if any set of hyperplanes crossing both, but contains no facing triples, has size bounded above by kk. The notion of well-separated hyperplanes was introduced by Genevois, for example, see [Gen20a].

A geodesic ray bb is said to be DD-uniformly contracting if there exists a constant DD such that projections of disjoint balls to bb have diameters uniformly bounded above by DD. In [CS15], Charney and Sultan characterized uniformly contracting geodesic rays as those which cross an infinite sequence of hyperplanes {hi}i=1\{h_{i}\}^{\infty}_{i=1} at points tit_{i} where d(b(ti),b(ti+1))d(b(t_{i}),b(t_{i+1})) is uniformly bounded above by a constant rr and each two consecutive hyperplanes hi,hi+1h_{i},h_{i+1} are uniformly kk-separated for some k0k\geq 0.

A natural question to ask is whether κ\kappa-contracting geodesic rays can be similarly described using the simpler kk-separated notion. In other words, it is reasonable to expect that κ\kappa-contracting geodesic rays are characterized as ones which cross an infinite sequence of hyperplanes {hi}i=1\{h_{i}\}_{i=1}^{\infty} at points tit_{i} where d(b(ti),b(ti+1))d(b(t_{i}),b(t_{i+1})) grows like κ(ti)\kappa(t_{i}) and the separation of each two consecutive hyperplanes hi,hi+1h_{i},h_{i+1} grows like κ(ti)\kappa(t_{i}). This is, in fact, not the case. We give an example (Example 4.6) of a log2\log_{2}-contracting geodesic ray where the separation grows linearly (in particular, faster than every sublinear function). More precisely, we show the following.

Theorem D.

There is a uniformly locally finite CAT(0) cube complex XX and a log2\log_{2}-contracting geodesic ray bXb\subset X such that the following holds: For any sublinear function κ\kappa, and any collection of hyperplanes {hi}i=1\{h_{i}\}_{i=1}^{\infty} crossing bb at tit_{i}, if d(b(ti1),b(ti))𝖼κ(ti)d(b(t_{i-1}),b(t_{i}))\leq{\sf c}\kappa(t_{i}) for some 𝖼0{\sf c}\geq 0, then

limti#{hyperplanes h|h intersects hi1 and hi}ti12.\displaystyle\lim_{t_{i}\to\infty}\frac{\#\{\text{hyperplanes }h\;|\;h\text{ intersects }h_{i-1}\text{ and }h_{i}\}}{t_{i}}\geq\frac{1}{2}.

In particular, the number of hyperplanes crossing both hi1,hih_{i-1},h_{i} grows faster than every sublinear function of ti.t_{i}.

To understand the difference between kk-separation and kk-well-separation it is useful to see how these are related to the volume and diameter of a convex set. For example, consider a ball of radius DD given by BDB_{D} in the Cayley graph of F2F_{2}. The number of hyperplanes meeting such a ball is about 4.3D4.3^{D} while the diameter of this set is 2D2D. Notice however, that the number of hyperplanes meeting BDB_{D} which contain no facing triple is 2D2D. In a quantifiable way, the number of hyperplanes that meet a convex set measures the sets volume, while the number of hyperplanes that meet the set and contain no facing triples measures the diameter.

Since the κ\kappa-contracting property is a statement about the diameter of projections and not the volume, the notion of well-separation will be better suited for our characterization (in the special case of uniform contraction, bounding the diameter of the projection is equivalent to bounding its volume and the separation of hyperplanes is the simpler combinatorial property to use, hence why it was used in [CS15]).

For a slightly less trivial example, let BDB_{D} be as above and consider the space CD=BD×+C_{D}=B_{D}\times\mathbb{R}^{+}. Let bb be the geodesic ray starting in CDC_{D} at ee and going in the +\mathbb{R}^{+} direction of CDC_{D}. This geodesic ray is DD-uniformly contracting while every two hyperplanes h1,h2h_{1},h_{2} crossed by bb are 4.3D4.3^{D}-separated. Nonetheless, h1,h2h_{1},h_{2} are DD-well-separated. As illustrated in this example, the well-separation notion inter-plays with contraction in a linear fashion whereas separation does not. Since we are trying to understand κ\kappa-contracting geodesic rays where the contraction grows as the sublinear function κ\kappa, the well-separation notion is the appropriate one to use.

1.3. History

Divergence rose in the study of non-positively curved manifolds and metric spaces as a measure of how fast geodesic rays travel away from each other. In particular, Gromov conjectured that all pairs of geodesic rays in the universal cover of a closed Riemannian manifold of non-positive curvature diverge either linearly or exponentially [Gro93]. Gersten [Ger94] provided the first examples of CAT(0) spaces whose divergence did not satisfy the linear/exponential dichotomy and showed that such examples are closely tied to other areas in mathematics. Duchin and Rafi [DR09] show that both Teichmuller space (with the Teichmuller metric) and the mapping class group (with a word metric) have geodesic divergence that is intermediate between the linear rate of flat spaces and the exponential rate of hyperbolic spaces. Algom-Kfir [AK11] shows the divergence function in CVnCV_{n} is at least quadratic. In [Lev18], Levcovitz gave a classification of all right-angled Coxeter groups with quadratic divergence and showed right-angled Coxeter groups cannot exhibit a divergence function between quadratic and cubic. More recently, Arzhantseva-Cashen-Gruber-Hume [ACGH17] shows that Morse geodesic rays in proper metric spaces have superlinear divergences.

Another motivation for studying collections of geodesic rays is to introduce a boundary at infinity. The topology and dynamics of these boundaries often provides information about the geometry of the space and the algebraic behaviour of groups acting on the space. For CAT(0) spaces, there are a number of boundaries, the visual boundary, the Tits boundary, and more recently the contracting boundary and the κ\kappa-contracting boundary (see [IM] by Incerti-Medici on comparing such boundaries). Each boundary has its own advantages and disadvantages, the visual and Tits boundaries give a lot of information about the product structure and maximal flats in a space, however, neither of them are quasi-isometric invariants as shown by Croke and Kleiner [CK00]. This limits their use in studying some aspects of CAT(0) groups. The contracting boundary ([CS15] for CAT(0)\operatorname{CAT}(0) space and [Cor17] by Cordes for proper metric spaces) is a quasi-isometry invariant, however it is not a metrizable space, and in a probabilistic sense contracting geodesic rays are rare in CAT(0) spaces that contain flats [CDG20]. The κ\kappa-boundary was introduced by Qing, Rafi and Tiozzo in [QRT19] and sought to rectify some of the shortcomings found in the these other boundaries. They show that the κ\kappa-boundary is metrizable and invariant under quasi-isometries. Moreover, in [QZ19] Qing and Zalloum further studied the topology and dynamics of this boundary for CAT(0)\operatorname{CAT}(0) spaces. For example, they show that the κ\kappa-boundary is a strong visibility space and that rank one isometries have dense axes in the κ\kappa-boundary. In fact, every proper geodesic space has a κ\kappa-boundary that is QI-invariant and metrizable, and in the case of mapping class groups it can serve as Poisson boundaries as well [QRT].

Further Questions

Question 1.

For CAT(0) spaces, the notion of κ\kappa-Morse and κ\kappa-contracting are equivalent, but they are different in general. For a proper geodesic metric space can sublinearly Morse (quasi)-geodesics be characterized in terms of having superlinear κ\kappa-lower divergence?

Question 2.

Can one show the following. Let XX be a CAT(0) cube complex and let bXb\in X be a geodesic ray. If no hyperplane hh has an infinite projection on bb, then bb is sublinearly contracting (κ\kappa-contracting for some κ\kappa) if and only if it makes a sublinear progress in the contact graph of XX.

Question 3.

We claim that Corollary C implies the existence of a map i:κXYi:\partial_{\kappa}X\rightarrow\partial Y between the κ\kappa-boundary of a cocompact CAT(0) cube complex XX with a factor system to the Gromov boundary of the corresponding hyperbolic space YY. Using different tools [ABD] have shown that an analogous map the Morse boundary of a hierarchically hyperbolic space and the boundary of a hyperbolic space YY. Further, they showed that this map is continuous and 1-1 [ABD]. Can one show that i:κXYi:\partial_{\kappa}X\rightarrow\partial Y is a well-defined continuous injection?

Outline of the paper

In Section 2, we review CAT(0)\operatorname{CAT}(0) geometry and κ\kappa contracting geodesic rays. In section 3 we introduce the notion of κ\kappa-lower divergence prove Theorem A.\ref{thm: first intro thm}. In section 4, we review the combinatorics and geometry of CAT(0)\operatorname{CAT}(0) cube complexes, and prove Theorem D, Theorem B and Corollary C.

Acknowledgement.

The authors would like to thank Anthony Genevois, Mark Hagen, Merlin Incerti-Medici, Kasra Rafi, Michah Sageev and Giulio Tiozzo for helpful discussions. We especially thank Kasra Rafi for suggesting the definition of κ\kappa-lower divergence and Anthony Genevois for fruitful comments on an earlier draft of the paper. The third author is very grateful to Mark Hagen for teaching him numerous cube complex techniques which were very helpful for the development of this paper. The authors would like to thank the anonymous referee(s).

2. Preliminaries

2.1. CAT(0)\operatorname{CAT}(0) geometry

Definition 2.1 (Quasi-geodesics).

A geodesic ray in XX is an isometric embedding b:[0,)Xb:[0,\infty)\to X. We fix a base-point 𝔬X{\mathfrak{o}}\in X and always assume that b(0)=𝔬b(0)={\mathfrak{o}}, that is, a geodesic ray is always assumed to start from this fixed base-point. A quasi-geodesic ray is a continuous quasi-isometric embedding β:[0,)X\beta:[0,\infty)\to X starting from 𝔬{\mathfrak{o}}. The additional assumption that quasi-geodesics are continuous is not necessary, but it is added to make the proofs simpler.

2.2. Basic properties of CAT(0)\operatorname{CAT}(0) spaces

A proper geodesic metric space (X,dX)(X,d_{X}) is CAT(0)\operatorname{CAT}(0) if geodesic triangles in XX are at least as thin as triangles in Euclidean space with the same side lengths. To be precise, for any given geodesic triangle pqr\triangle pqr, consider the unique triangle p¯q¯r¯\triangle\overline{p}\overline{q}\overline{r} in the Euclidean plane with the same side lengths. For any pair of points on the triangle, for instance on edges [p,q][p,q] and [p,r][p,r] of the triangle pqr\triangle pqr, if we choose points x¯\overline{x} and y¯\overline{y} on edges [p¯,q¯][\overline{p},\overline{q}] and [p¯,r¯][\overline{p},\overline{r}] of the triangle p¯q¯r¯\triangle\overline{p}\overline{q}\overline{r} so that dX(p,x)=d𝔼2(p¯,x¯)d_{X}(p,x)=d_{\mathbb{E}^{2}}(\overline{p},\overline{x}) and dX(p,y)=d𝔼2(p¯,y¯)d_{X}(p,y)=d_{\mathbb{E}^{2}}(\overline{p},\overline{y}) then,

dX(x,y)d𝔼2(x¯,y¯).d_{X}(x,y)\leq d_{\mathbb{E}^{2}}(\overline{x},\overline{y}).

For the remainder of the paper, we assume (X,d)(X,d) is a proper CAT(0)\operatorname{CAT}(0) space. A metric space XX is proper if closed metric balls are compact. Here, we list some properties of proper CAT(0)\operatorname{CAT}(0) spaces that are needed later (see [BH99]).

Lemma 2.2.

A proper CAT(0)\operatorname{CAT}(0) space XX has the following properties:

  1. (1)

    It is uniquely geodesic, that is, for any two points x,yx,y in XX, there exists exactly one geodesic connecting them.

  2. (2)

    The nearest-point projection from a point xx to a geodesic line bb is a unique point denoted xbx_{b}. In fact, the closest-point projection map

    πb:Xb\pi_{b}:X\to b

    is Lipschitz.

  3. (3)

    Convexity: For any convex set ZXZ\in X, the distance function f:X+f:X\rightarrow\mathbb{R}^{+} given by f(x)=d(x,Z)f(x)=d(x,Z) is convex in the sense of [BH09] II.2.1.

2.3. κ\kappa–contracting geodesics of XX

In this section we review the definition and properties of κ\kappa–contracting geodesic rays needed for this paper, for further details see [QRT19]. We fix a function

κ:[0,)[1,)\kappa:[0,\infty)\to[1,\infty)

that is monotone increasing, concave and sublinear, that is

limtκ(t)t=0.\lim_{t\to\infty}\frac{\kappa(t)}{t}=0.

Note that using concavity, for any a>1a>1, we have

(1) κ(at)a(1aκ(at)+(11a)κ(0))aκ(t).\kappa(at)\leq a\left(\frac{1}{a}\,\kappa(at)+\left(1-\frac{1}{a}\right)\kappa(0)\right)\leq a\,\kappa(t).

The assumption that κ\kappa is increasing and concave makes certain arguments cleaner but they are not necessary. One can always replace any sublinear function κ\kappa, with another sublinear function κ¯\overline{\kappa} so that κ(t)κ¯(t)𝖢κ(t)\kappa(t)\leq\overline{\kappa}(t)\leq{\sf C}\,\kappa(t) for some constant 𝖢{\sf C} and κ¯\overline{\kappa} is monotone increasing and concave. For example, define

κ¯(t)=sup{λκ(u)+(1λ)κ(v)| 0λ1,u,v>0,andλu+(1λ)v=t}.\overline{\kappa}(t)=\sup\Big{\{}\lambda\kappa(u)+(1-\lambda)\kappa(v)\mathbin{\Big{|}}\ 0\leq\lambda\leq 1,\ u,v>0,\ \text{and}\ \lambda u+(1-\lambda)v=t\Big{\}}.

The requirement κ(t)1\kappa(t)\geq 1 is there to remove additive errors in the definition of κ\kappa–contracting geodesics.

Definition 2.3 (κ\kappa–neighborhood).

For a closed set ZZ ( here ZZ can be taken as either a geodesic or a quasi-geodesic ray) and a constant 𝗇{\sf n} define the (κ,𝗇)(\kappa,{\sf n})–neighbourhood of ZZ to be

𝒩κ(Z,𝗇)={xX|dX(x,Z)𝗇κ(x)}.\mathcal{N}_{\kappa}(Z,{\sf n})=\Big{\{}x\in X\mathbin{\Big{|}}d_{X}(x,Z)\leq{\sf n}\cdot\kappa(x)\Big{\}}.
𝔬{\mathfrak{o}}bbxxxbx_{b}𝗇κ(x){\sf n}\cdot\kappa(x)x||x||(κ,𝗇)(\kappa,{\sf n})–neighbourhood of bb
Figure 2. A κ\kappa-neighbourhood of a geodesic ray bb with multiplicative constant 𝗇{\sf n}.

Lastly, for xXx\in X, define x=dX(𝔬,x)\lVert x\rVert=d_{X}({\mathfrak{o}},x). When used inside the function κ(t)\kappa(t), we drop \lVert\cdot\rVert and write

κ(x):=κ(x).\kappa(x):=\kappa(\lVert x\rVert).
Definition 2.4 (κ\kappa–Morse).

A geodesic ray bb is κ\kappa–Morse if there is a function

𝗆b:+2+{\sf m}_{b}:{\mathbb{R}}_{+}^{2}\to{\mathbb{R}}_{+}

so that if β:[s,t]X\beta:[s,t]\to X is a (𝗊,𝖰)({\sf q},{\sf Q})–quasi-geodesic with end points on bb then

β[s,t]𝒩κ(b,𝗆b(𝗊,𝖰)).\beta[s,t]\subset\mathcal{N}_{\kappa}\big{(}b,{\sf m}_{b}({\sf q},{\sf Q})\big{)}.

We refer to 𝗆b{\sf m}_{b} as the Morse gauge for bb.

Definition 2.5 (κ\kappa–contracting).

For a geodesic ray bb of XX, we say bb is κ\kappa–contracting if there is a constant 𝖼b{\sf c}_{b} so that, for every x,yXx,y\in X

dX(x,y)dX(x,b)diamX(xbyb)𝖼bκ(x).d_{X}(x,y)\leq d_{X}(x,b)\quad\Longrightarrow\quad diam_{X}\big{(}x_{b}\cup y_{b}\big{)}\leq{\sf c}_{b}\cdot\kappa(x).

In the special case where κ=1,\kappa=1, we say that bb is uniformly contracting.

In a CAT(0) space XX, the notions of κ\kappa-Morse and κ\kappa-contracting are indeed equivalent.

Theorem 2.6 (Theorem 3.8 [QRT19]).

Let XX be a CAT(0) space and let bXb\in X be a geodesic ray. Then, b is κ\kappa-Morse if and only if it is κ\kappa-contracting.

Our next goal is to prove that the notion of κ\kappa-contracting is equivalent to another notion of contraction. In order to do so, we need the following two propositions (see [CS15], [QRT19]).

Proposition 2.7 (Proposition 3.11 [QRT19]).

Given a geodesic segment bb (possibly infinite) and points x,yXx,y\in X with d(x,y)<d(x,b)d(x,y)<d(x,b), there exists a (32,0)(32,0)-quasi-geodesic β:[s0,s1]X\beta:[s_{0},s_{1}]\rightarrow X with end points on bb such that β(s0)=xb\beta(s_{0})=x_{b},

14d(xb,yb)d(β(s0),β(s1))<d(xb,yb)\frac{1}{4}d(x_{b},y_{b})\leq d(\beta(s_{0}),\beta(s_{1}))<d(x_{b},y_{b})

and there a point p=β(t)p=\beta(t) on β\beta such that

d(p,b)180d(xb,yb).d(p,b)\geq\frac{1}{80}d(x_{b},y_{b}).

The following proposition states that if x,yx,y are within κ(x)\kappa(x) of each other, then κ(x)\kappa(x) and κ(y)\kappa(y) are multiplicatively the same.

Proposition 2.8 ([QRT19, Lemma 3.2]).

For any 𝖽0>0{\sf d}_{0}>0, there exists 𝖽1,𝖽2>0{\sf d}_{1},{\sf d}_{2}>0 depending only on 𝖽0{\sf d}_{0} and κ\kappa so that for x,yXx,y\in X, we have

d(x,y)𝖽0κ(x)𝖽1κ(x)κ(y)𝖽2κ(x).d(x,y)\leq{\sf d}_{0}\kappa(x)\implies{\sf d}_{1}\kappa(x)\leq\kappa(y)\leq{\sf d}_{2}\kappa(x).

Now we present a slightly different but equivalent contracting condition that we will frequently use in the paper:

Lemma 2.9.

A geodesic ray is κ\kappa–contracting if and only if there exists a constant 𝖼>0{\sf c}>0 such that for any x,yXx,y\in X with d(x,y)<d(x,b)d(x,y)<d(x,b), we have

d(xb,yb)𝖼κ(xb).d(x_{b},y_{b})\leq{\sf c}\kappa(x_{b}).
Proof.

(\Rightarrow) Since d(x,y)<d(x,b)d(x,y)<d(x,b), there exists a quasi-geodesic β\beta as in Proposition 2.7, and a point pβp\in\beta such that

d(xb,yb)80d(p,b).d(x_{b},y_{b})\leq 80d(p,b).

Using Theorem 2.6, since bb is κ\kappa–Morse,

d(p,b)=d(p,pb)𝗆b(32,0)κ(p)d(p,b)=d(p,p_{b})\leq{\sf m}_{b}(32,0)\kappa(p)

Applying Proposition 2.8 to points p,pbp,p_{b}, we have

(2) d(xb,yb)80d(p,pb)80𝗆b(32,0)κ(p)80𝗆b(32,0)κ(pb)/𝖽1.d(x_{b},y_{b})\leq 80d(p,p_{b})\leq 80{\sf m}_{b}(32,0)\kappa(p)\leq 80{\sf m}_{b}(32,0)\kappa(p_{b})/{\sf d}_{1}.

Consider the distance between xbx_{b} and pbp_{b}:

d(xb,pb)\displaystyle d(x_{b},p_{b}) d(xb,p)projections in CAT(0) spaces are Lipschitz.\displaystyle\leq d(x_{b},p)\quad\text{projections in $\operatorname{CAT}(0)$\,spaces are Lipschitz.}
32d(xb,yb)+0Proposition 2.7\displaystyle\leq 32d(x_{b},y_{b})+0\quad\text{Proposition\leavevmode\nobreak\ \ref{Proposition: Constructing a close quasi-geodesic}}
3280𝗆b(32,0)κ(pb)/𝖽1Equation 2\displaystyle\leq 32\cdot 80{\sf m}_{b}(32,0)\kappa(p_{b})/{\sf d}_{1}\quad\text{Equation\leavevmode\nobreak\ \ref{bound1}}

Thus applying Proposition 2.8 again, we get some constant 𝖽2{\sf d}_{2} such that κ(pb)𝖽2κ(xb)\kappa(p_{b})\leq{\sf d}_{2}\kappa(x_{b}). Combined with Equation 2, there exists 𝖽3{\sf d}_{3} such that

d(xb,yb)𝖽3κ(xb).d(x_{b},y_{b})\leq{\sf d}_{3}\kappa(x_{b}).

(\Leftarrow) Since projections are distance-decreasing in CAT(0) spaces,

d(xb,yb)𝖼κ(xb)𝖼κ(x),d(x_{b},y_{b})\leq{\sf c}\kappa(x_{b})\leq{\sf c}\kappa(x),

as desired.

3. κ\kappa-Lower Divergence and slim geodesics

In this section we study the divergence and the slimness property of κ\kappa-contracting geodesics. We first give the definitions of these measures. Divergence measures how fast the circumference of a ball grows as its radius increases. Under the lower divergence notion introduced by Charney and Sultan in [CS15], κ\kappa-contracting rays cannot be distinguished from geodesic rays which lie in a flat. We introduce a lower divergence notion which is more sensitive.

3.1. κ\kappa-lower divergence of geodesics

Definition 3.1 (κ\kappa-lower divergence).

Let bb be a geodesic ray and fix some r>0r>0 and then t>rκ(t)t>r\kappa(t). Let ρκ(r,t)\rho_{\kappa}(r,t) denote the infimum of the lengths of all paths from b(trκ(t))b(t-r\kappa(t)) to b(t+rκ(t))b(t+r\kappa(t)) which lie outside the open ball of radius rκ(t)r\kappa(t) about b(t)b(t). If there does not exist such a path, then let ρκ(r,t)=\rho_{\kappa}(r,t)=\infty. Given a geodesic ray bb, we define the κ\kappa-lower divergence of bb to be the function

divκ(r):=inft>rκ(t)ρκ(r,t)κ(t)div_{\kappa}(r):=\underset{t>r\kappa(t)}{\text{inf}}\,\,\frac{\rho_{\kappa}(r,t)}{\kappa(t)}
𝔬{\mathfrak{o}}bbrκ(t)\,r\kappa(t)
Figure 3. Definition of κ\kappa-lower divergence.

The specific κ\kappa-lower-divergence function is rarely of direct interest, instead the growth rate of the function is the primary property of interest. Two functions f(t)f(t) and g(t)g(t) have the same growth rate if the limit of their ratios is non-zero and finite,

0<limt|f(t)g(t)|<0<\lim_{t\to\infty}\left|\frac{f(t)}{g(t)}\right|<\infty

We say that the κ\kappa-lower-divergence is linear if it’s growth rate is the same as the growth rate of tt, and it is superlinear if limtdivκ(t)t=\displaystyle\lim_{t\to\infty}\frac{div_{\kappa}(t)}{t}=\infty. Similarly we say that the κ\kappa-lower-divergence is quadratic if the growth rate is the same as t2t^{2}, and we say it is exponential if there is some a>1a>1 so that it has the same growth rate as ata^{t}.

To proceed we discuss slim triangles. The idea of capturing coarse hyperbolicity by slim triangles first came by Gromov in [Gro87]. Here we give four different adaptations of the concept and we shall see in Corollary 3.7 that they are equivalent in the setting of CAT(0) spaces.

Definition 3.2.

Let bb be an infinite geodesic ray in a CAT(0) space. We describe four different conditions on the slimness of the geodesic ray:

  1. (1)

    We say that bb satisfies the κ\kappa-slim condition 1 if there exists some 𝖼0{\sf c}\geq 0 such that for any xX,yim(b)x\in X,y\in im(b), we have d(xb,[x,y])𝖼κ(xb)d(x_{b},[x,y])\leq{\sf c}\kappa(x_{b}).

  2. (2)

    We say that bb satisfies the κ\kappa-slim condition 2 if there exists some 𝖼0{\sf c}\geq 0 such that for any xX,yim(b)x\in X,y\in im(b), we have d(xb,[x,y])𝖼κ(z)d(x_{b},[x,y])\leq{\sf c}\kappa(z) for some zz between xbx_{b} and y.y.

  3. (3)

    We say that bb satisfies the κ\kappa-slim condition 3 if there exists some 𝖼0{\sf c}\geq 0 such that for any x,y,zXx,y,z\in X with [y,z]im(b)[y,z]\subset im(b), if w[y,z]w\in[y,z], we have d(w,[y,x][x,z])𝖼κ(xb)d(w,[y,x]\cup[x,z])\leq{\sf c}\kappa(x_{b}).

  4. (4)

    We say that bb satisfies the κ\kappa-slim condition 4 if there exists some 𝖼0{\sf c}\geq 0 such that for any xXx\in X, [y,z]im(b)[y,z]\subset im(b) with yxbz||y||\leq||x_{b}||\leq||z|| if w[y,z],w\in[y,z], we have d(w,[y,x][x,z])𝖼κ(z).d(w,[y,x]\cup[x,z])\leq{\sf c}\kappa(z).

We collect now the implications between these definitions:

Lemma 3.3.

Let bb be an infinite geodesic ray in a CAT(0) space.

  1. a).

    κ\kappa-slim condition 1 κ\Longrightarrow\kappa-slim condition 2.

  2. b).

    κ\kappa-slim condition 3 κ\Longrightarrow\kappa-slim condition 4.

  3. c).

    κ\kappa-slim condition 1 κ\iff\kappa-slim condition 3.

  4. d).

    κ\kappa-slim condition 4 κ\Longrightarrow\kappa-slim condition 2.

Proof.

Let bb be an infinite geodesic ray in a CAT(0) space in each statement:

  1. a).

    Choosing z=xbz=x_{b} gives the desired statement.

  2. b).

    Since xbz||x_{b}||\leq||z||, we have

    d(w,[y,x][x,z])𝖼κ(xb)d(w,[y,x][x,z])𝖼κ(z)d(w,[y,x]\cup[x,z])\leq{\sf c}\kappa(x_{b})\implies d(w,[y,x]\cup[x,z])\leq{\sf c}\kappa(z).

  3. c).

    κ\kappa-slim condition 1 κ\Rightarrow\kappa-slim condition 3: Let x,y,zXx,y,z\in X with [y,z]im(b)[y,z]\in im(b), using κ\kappa-slim condition 1, we have d(xb,[y,x])𝖼κ(xb),d(x_{b},[y,x])\leq{\sf c}\kappa(x_{b}), convexity of the CAT(0) metric then implies that d(w,[y,x])𝖼κ(xb)d(w,[y,x])\leq{\sf c}\kappa(x_{b}) for all w[y,xb].w\in[y,x_{b}]. Similarly, using κ\kappa-slim condition 1, we get that d(xb,[x,z])𝖼κ(xb)d(x_{b},[x,z])\leq{\sf c}\kappa(x_{b}). Again, by convexity of the CAT(0) metric, we get that d(w,[x,z]𝖼κ(xb))d(w,[x,z]\leq{\sf c}\kappa(x_{b})).

    κ\kappa-slim condition 3 κ\Rightarrow\kappa-slim condition 1: Let xX,yim(b)x\in X,y\in im(b). If d(xb,y)𝖼κ(xb),d(x_{b},y)\leq{\sf c}\kappa(x_{b}), then we have d(xb,[x,y])d(xb,y)𝖼κ(xb)d(x_{b},[x,y])\leq d(x_{b},y)\leq{\sf c}\kappa(x_{b}). Otherwise, if d(xb,y)>𝖼κ(xb),d(x_{b},y)>{\sf c}\kappa(x_{b}), we can choose xx^{\prime} between xbx_{b} and yy with 𝖼κ(xb)<d(x,xb)2𝖼κ(xb).{\sf c}\kappa(x_{b})<d(x^{\prime},x_{b})\leq 2{\sf c}\kappa(x_{b}). Using the κ\kappa-slim condition 3, we get d(x,[x,y])𝖼κ(xb).d(x^{\prime},[x,y])\leq{\sf c}\kappa(x_{b}). Therefore, by the triangle inequality, we have d(xb,[x,y])3𝖼κ(xb).d(x_{b},[x,y])\leq 3{\sf c}\kappa(x_{b}).

  4. d).

    Let xX,yim(b)x\in X,y\in im(b) and define z=max{xb,y}z=\text{max}\{x_{b},y\}. If d(xb,y)𝖼κ(z),d(x_{b},y)\leq{\sf c}\kappa(z), we have d(xb,[x,y])d(xb,y)𝖼κ(z).d(x_{b},[x,y])\leq d(x_{b},y)\leq{\sf c}\kappa(z). Otherwise, we can choose xx^{\prime} between xbx_{b} and yy with 𝖼κ(z)<d(x,xb)2𝖼κ(z){\sf c}\kappa(z)<d(x^{\prime},x_{b})\leq 2{\sf c}\kappa(z). Using the κ\kappa-slim condition 4, we get d(x,[x,y])𝖼κ(z).d(x^{\prime},[x,y])\leq{\sf c}\kappa(z). Therefore, by the triangle inequality, we have d(xb,[x,y])3𝖼κ(z).d(x_{b},[x,y])\leq 3{\sf c}\kappa(z).

Lemma 3.4.

Let bb be a κ\kappa-contracting geodesic ray with contracting constant 𝖼{\sf c}. For any xXx\in X and yby\in b we have

d(x,xb)+d(xb,y)𝖼κ(xb)1d(x,y)d(x,xb)+d(xb,y).d(x,x_{b})+d(x_{b},y)-{\sf c}\kappa(||x_{b}||)-1\leq d(x,y)\leq d(x,x_{b})+d(x_{b},y).
𝔬{\mathfrak{o}}xxyyxbx_{b}zzzbz_{b}
Figure 4. The distance from xx to yy is approximated by taking the projection to bb and then going along bb.
Proof.

Consider a ball around xx of radius r=d(x,xb)1r=d(x,x_{b})-1. Let zz be the point on [x,y][x,y] with d(x,z)=rd(x,z)=r. Since bb is κ\kappa-contracting, we have that

d(xb,zb)𝖼κ(xb).d(x_{b},z_{b})\leq{\sf c}\kappa(x_{b}).

Notice that

d(x,y)d(x,xb)\displaystyle d(x,y)-d(x,x_{b}) =d(x,z)+d(z,y)d(x,xb)\displaystyle=d(x,z)+d(z,y)-d(x,x_{b})
=(d(x,xb)1)+d(z,y)d(x,xb)\displaystyle=(d(x,x_{b})-1)+d(z,y)-d(x,x_{b})
=d(z,y)1\displaystyle=d(z,y)-1
d(zb,y)1\displaystyle\geq d(z_{b},y)-1
d(xb,y)d(xb,zb)1\displaystyle\geq d(x_{b},y)-d(x_{b},z_{b})-1
d(xb,y)𝖼κ(xb)1.\displaystyle\geq d(x_{b},y)-{\sf c}\kappa(x_{b})-1.

This yields

d(x,y)d(x,xb)+d(xb,y)𝖼κ(xb)1,d(x,y)\geq d(x,x_{b})+d(x_{b},y)-{\sf c}\kappa(x_{b})-1,

where the second inequality follows from triangle inequality.

Lemma 3.5.

Every κ\kappa-contracting geodesic ray is κ\kappa-slim condition 1.

Proof.

Let xXx\in X and let yby\in b. Let zz^{\prime} be the point on [x,y][x,y] with d(x,z)=d(x,b).d(x,z^{\prime})=d(x,b). Since bb is κ\kappa-contracting, using Lemma 2.9, we have d(xb,zb)𝖼κ(xb).d(x_{b},z^{\prime}_{b})\leq{\sf c}\kappa(x_{b}). Now, as

d(y,xb)+d(xb,x)d(x,y)=d(x,z)+d(z,y),d(y,x_{b})+d(x_{b},x)\geq d(x,y)=d(x,z^{\prime})+d(z^{\prime},y),

we get that d(z,y)d(y,xb).d(z^{\prime},y)\leq d(y,x_{b}). Thus, we have

(3) d(z,y)d(y,xb)d(y,zb)+𝖼κ(xb).d(z^{\prime},y)\leq d(y,x_{b})\leq d(y,z^{\prime}_{b})+{\sf c}\kappa(x_{b}).

Now, applying Lemma 3.4 to the points zz^{\prime} and yy, we get that

(4) d(z,y)d(z,zb)+d(zb,y)𝖼κ(zb)1.d(z^{\prime},y)\geq d(z^{\prime},z^{\prime}_{b})+d(z^{\prime}_{b},y)-{\sf c}\kappa(z^{\prime}_{b})-1.

Since d(xb,zb)𝖼κ(xb)d(x_{b},z^{\prime}_{b})\leq{\sf c}\kappa(x_{b}), we have zbxb,||z^{\prime}_{b}||\leq||x_{b}||, or

zbxb+𝖼κ(xb)xb+𝖼xb=(1+𝖼)xb.||z^{\prime}_{b}||\leq||x_{b}||+{\sf c}\kappa(x_{b})\leq||x_{b}||+{\sf c}||x_{b}||=(1+{\sf c})||x_{b}||.

Combining the inequalities 3 and 4, we get:

d(z,zb))𝖼κ(xb)+𝖼κ(zb)+1𝖼κ(xb)+𝖼κ((1+𝖼)xb)+1.d(z^{\prime},z^{\prime}_{b}))\leq{\sf c}\kappa(x_{b})+{\sf c}\kappa(z^{\prime}_{b})+1\leq{\sf c}\kappa(x_{b})+{\sf c}\kappa((1+{\sf c})x_{b})+1.

Therefore

d(z,zb)(𝖼+𝖼(𝖼+1))κ(xb)+1d(z^{\prime},z^{\prime}_{b})\leq({\sf c}+{\sf c}({\sf c}+1))\kappa(x_{b})+1

Thus

d(z,xb)d(z,zb)+d(zb,xb)(𝖼+𝖼(𝖼+1))κ(xb)+1+𝖼κ(xb).d(z^{\prime},x_{b})\leq d(z^{\prime},z^{\prime}_{b})+d(z^{\prime}_{b},x_{b})\leq({\sf c}+{\sf c}({\sf c}+1))\kappa(x_{b})+1+{\sf c}\kappa(x_{b}).

Which gives

d(z,xb)(3𝖼+𝖼2)κ(xb)+1(3𝖼+𝖼2)κ(xb)+κ(xb).d(z^{\prime},x_{b})\leq(3{\sf c}+{\sf c}^{2})\kappa(x_{b})+1\leq(3{\sf c}+{\sf c}^{2})\kappa(x_{b})+\kappa(x_{b}).

Thus,

d(z,xb)(3𝖼+𝖼2+1)κ(xb).d(z^{\prime},x_{b})\leq(3{\sf c}+{\sf c}^{2}+1)\kappa(x_{b}).

Choosing 𝖼=3𝖼+𝖼2+1{\sf c}^{\prime}=3{\sf c}+{\sf c}^{2}+1 gives the desired result.

Proposition 3.6.

A geodesic ray bb is κ\kappa-contracting if and only if it satisfies κ\kappa-slim condition 2.

xxxbx_{b}yyyby_{b}
Proof.

We have already shown that κ\kappa-contracting geodesic rays are κ\kappa-slim condition 1, and by Lemma 3.3 a) it also satisfies κ\kappa-slim condition 2. Suppose that bb is κ\kappa-slim condition 2, let xXx\in X and let BB be a disjoint ball around xx of radius r.r. Let yB=B(x,r)y\in B=B(x,r) and let xb,ybx_{b},y_{b} be the respective projections of x,yx,y on bb. Since bb is κ\kappa-slim condition 2, there exists a point w[xb,y]w\in[x_{b},y] with d(yb,w)𝖼κ(z)d(y_{b},w)\leq{\sf c}\kappa(z) for some z[xb,yb].z\in[x_{b},y_{b}]. Using convexity of the CAT(0) metric, since d(x,y)d(x,xb)d(x,y)\leq d(x,x_{b}), we have d(x,w)max{d(x,xb),d(x,y)}=d(x,xb).d(x,w)\leq max\{d(x,x_{b}),d(x,y)\}=d(x,x_{b}).

Therefore

d(x,yb)d(x,w)+𝖼κ(z)d(x,xb)+𝖼κ(z).d(x,y_{b})\leq d(x,w)+{\sf c}\kappa(z)\leq d(x,x_{b})+{\sf c}\kappa(z).

On the other hand, applying the κ\kappa-slim condition 2 to Δ=Δ(x,xb,yb)\Delta=\Delta(x,x_{b},y_{b}), we get a point ww^{\prime} on [x,yb][x,y_{b}] with d(xb,w)𝖼κ(z)d(x_{b},w^{\prime})\leq{\sf c}\kappa(z^{\prime}) for some z[xb,yb]z^{\prime}\in[x_{b},y_{b}]. Hence, we have

d(x,yb)\displaystyle d(x,y_{b}) =d(x,w)+d(w,yb)\displaystyle=d(x,w^{\prime})+d(w^{\prime},y_{b})
[d(x,xb)𝖼κ(z)]+[d(xb,yb)𝖼κ(z)]\displaystyle\geq[d(x,x_{b})-{\sf c}\kappa(z^{\prime})]+[d(x_{b},y_{b})-{\sf c}\kappa(z^{\prime})]
=d(x,xb)+d(xb,yb)2𝖼κ(z).\displaystyle=d(x,x_{b})+d(x_{b},y_{b})-2{\sf c}\kappa(z^{\prime}).

This implies

d(x,xb)+d(xb,yb)2𝖼κ(z)d(x,yb)d(x,xb)+𝖼κ(z).d(x,x_{b})+d(x_{b},y_{b})-2{\sf c}\kappa(z^{\prime})\leq d(x,y_{b})\leq d(x,x_{b})+{\sf c}\kappa(z).

Therefore, we have

d(xb,yb)2𝖼κ(z)+𝖼κ(z).d(x_{b},y_{b})\leq 2{\sf c}\kappa(z^{\prime})+{\sf c}\kappa(z).

We have two cases, if xbybx_{b}\leq y_{b}, then

d(xb,yb)\displaystyle d(x_{b},y_{b}) 2𝖼κ(z)+𝖼κ(z)\displaystyle\leq 2{\sf c}\kappa(z^{\prime})+{\sf c}\kappa(z)
2𝖼κ(yb)+𝖼κ(yb)\displaystyle\leq 2{\sf c}\kappa(y_{b})+{\sf c}\kappa(y_{b})
2𝖼κ(y)+2𝖼κ(y)\displaystyle\leq 2{\sf c}\kappa(y)+2{\sf c}\kappa(y)
=4𝖼κ(y)\displaystyle=4{\sf c}\kappa(y)
4𝖼κ(2x)\displaystyle\leq 4{\sf c}\kappa(2x)
8𝖼κ(x).\displaystyle\leq 8{\sf c}\kappa(x).

Now, if ybxby_{b}\leq x_{b}, then

d(xb,yb)\displaystyle d(x_{b},y_{b}) 2𝖼κ(z)+𝖼κ(z)\displaystyle\leq 2{\sf c}\kappa(z^{\prime})+{\sf c}\kappa(z)
2𝖼κ(xb)+𝖼κ(xb)\displaystyle\leq 2{\sf c}\kappa(x_{b})+{\sf c}\kappa(x_{b})
2𝖼κ(x)+2𝖼κ(x)\displaystyle\leq 2{\sf c}\kappa(x)+2{\sf c}\kappa(x)
=4𝖼κ(x).\displaystyle=4{\sf c}\kappa(x).

Corollary 3.7.

All the κ\kappa-slim conditions are equivalent.

Proof.

Using Theorem 3.6 and Lemma 3.5, we get that κ\kappa-slim condition 2 implies κ\kappa-slim condition 1. Now, applying Lemmas 3.3 we get the desired result.

Therefore we give the following definition.

Definition 3.8 (κ\kappa-slim geodesic).

A geodesic ray bb is said to be κ\kappa-slim if it satisfies any of the four κ\kappa-slim conditions.

Theorem 3.9.

The κ\kappa-lower divergence for a κ\kappa-contracting geodesic ray bb is at least quadratic.

b(t)+rκ(t)b(t)+r\kappa(t)z1z_{1}z2z_{2}z0z_{0}b(t)b(t)
Proof.

Suppose that bb is κ\kappa-contracting. Consider a ball B=Brκ(t)(b(t))B=B_{r\kappa(t)}(b(t)) with t>rκ(t)t>r\kappa(t). Let β\beta be a path avoiding BB connecting b(trκ(t))b(t-r\kappa(t)) to b(t+rκ(t))b(t+r\kappa(t)). Choose z0im(β)z_{0}\in im(\beta) with πb(z0)=b(t).\pi_{b}(z_{0})=b(t). Since d(z0,b(t))rκ(t),d(z_{0},b(t))\geq r\kappa(t), we have

d(z0,b(t+rκ(t))>rκ(t),d(z_{0},b(t+r\kappa(t))>r\kappa(t),

and hence we may choose z1im(β)z_{1}\in im(\beta) with d(z0,z1)=rκ(t)d(z_{0},z_{1})=r\kappa(t). Now, if x1=πb(z1)x_{1}=\pi_{b}(z_{1}), then d(b(t),x1)𝖼κ(2t).d(b(t),x_{1})\leq{\sf c}\kappa(2t). By triangle inequality,

d(z1,x1)rκ(t)𝖼κ(2t)d(z_{1},x_{1})\geq r\kappa(t)-{\sf c}\kappa(2t)

and hence

d(z1,b(t+rκ(t))>rκ(t)𝖼κ(2t).d(z_{1},b(t+r\kappa(t))>r\kappa(t)-{\sf c}\kappa(2t).

Thus, we may choose z2im(β)z_{2}\in im(\beta) with d(z2,z1)=rκ(t)𝖼κ(2t).d(z_{2},z_{1})=r\kappa(t)-{\sf c}\kappa(2t). We iterate this process to get a sequence z0,z1,z2,,znz_{0},z_{1},z_{2},...,z_{n} on β\beta, with respective projections b(t)=x0,x1,,xnb(t)=x_{0},x_{1},...,x_{n} such that

d(zi,zi+1)=rκ(t)i𝖼κ(2t) and d(xi,xi+1)𝖼κ(2t),d(z_{i},z_{i+1})=r\kappa(t)-i{\sf c}\kappa(2t)\quad\text{ and }\quad d(x_{i},x_{i+1})\leq{\sf c}\kappa(2t),

where nn is an integer satisfying rκ(t)𝖼κ(2t)1nrκ(t)𝖼κ(2t)\frac{r\kappa(t)}{{\sf c}\kappa(2t)}-1\leq n\leq\frac{r\kappa(t)}{{\sf c}\kappa(2t)}. We remark that since κ\kappa is an increasing function and since κ(2t)2κ(t)\kappa(2t)\leq 2\kappa(t), we have 1κ(2t)κ(t)21\leq\frac{\kappa(2t)}{\kappa(t)}\leq 2. We also have

|β|\displaystyle|\beta| d(z0,z1)++d(zn1,zn)\displaystyle\geq d(z_{0},z_{1})+...+d(z_{n-1},z_{n})
=(rκ(t))+(rκ(t)𝖼κ(2t))+(rκ(t)2𝖼κ(2t))++(rκ(t)(n1)𝖼κ(2t))\displaystyle=(r\kappa(t))+(r\kappa(t)-{\sf c}\kappa(2t))+(r\kappa(t)-2{\sf c}\kappa(2t))+...+(r\kappa(t)-(n-1){\sf c}\kappa(2t))
=nrκ(t)n(n1)𝖼κ(2t)2\displaystyle=nr\kappa(t)-\frac{n(n-1){\sf c}\kappa(2t)}{2}
nrκ(t)n2𝖼κ(2t)2.\displaystyle\geq nr\kappa(t)-\frac{n^{2}{\sf c}\kappa(2t)}{2}.

Thus

|β|rκ(t)\displaystyle\frac{|\beta|}{r\kappa(t)} nn2𝖼κ(2t)2rκ(t)\displaystyle\geq n-\frac{n^{2}{\sf c}\kappa(2t)}{2r\kappa(t)}
rκ(t)𝖼κ(2t)1(rκ(t)cκ(2t))2𝖼κ(2t)2rκ(t)\displaystyle\geq\frac{r\kappa(t)}{{\sf c}\kappa(2t)}-1-\big{(}\frac{r\kappa(t)}{c\kappa(2t)}\big{)}^{2}\frac{{\sf c}\kappa(2t)}{2r\kappa(t)}
=κ(t)𝖼κ(2t)(rr2)1\displaystyle=\frac{\kappa(t)}{{\sf c}\kappa(2t)}(r-\frac{r}{2})-1
=κ(t)r2𝖼κ(2t)1\displaystyle=\frac{\kappa(t)r}{2{\sf c}\kappa(2t)}-1
rκ(t)2𝖼2κ(t)1\displaystyle\geq\frac{r\kappa(t)}{2{\sf c}2\kappa(t)}-1
=r4𝖼1.\displaystyle=\frac{r}{4{\sf c}}-1.

Hence, we have |β|κ(t)r24cr\frac{|\beta|}{\kappa(t)}\geq\frac{r^{2}}{4c}-r. Since β\beta was an arbitrary path avoiding BB, we conclude

divκ(r)=inft>rκ(t)ρκ(r,t)κ(t)r24𝖼rdiv_{\kappa}(r)=\underset{t>r\kappa(t)}{\text{inf}}\,\,\frac{\rho_{\kappa}(r,t)}{\kappa(t)}\geq\frac{r^{2}}{4{\sf c}}-r.

Theorem 3.10.

If the κ\kappa-lower divergence of a geodesic ray bb is superlinear, then bb is κ\kappa-slim.

yry_{r}zrz_{r}xrx_{r}aaaa^{\prime}cccc^{\prime}p1p_{1}p2p_{2}trt_{r}eeee^{\prime}e′′e^{\prime\prime}3rκ(tr)3r\kappa(t_{r})rκ(tr)r\kappa(t_{r})
Proof.

Suppose that bb is not κ\kappa-slim. In particular, bb is not κ\kappa-slim with respect to condition 4. Thus, we have that for any r>0r>0, there exist three points xr,yr,zrbx_{r},y_{r},z_{r}\in b as in condition 4 with

yr(xr)bzr||y_{r}||\leq||(x_{r})_{b}||\leq||z_{r}||

and also a point tr[yr,zr]t_{r}\in[y_{r},z_{r}] such that

d(tr,[yr,xr][zr,xr])rκ(zr)rκ(tr).d(t_{r},[y_{r},x_{r}]\cup[z_{r},x_{r}])\geq r\kappa(z_{r})\geq r\kappa(t_{r}).

Note that this implies in particular that

d(yr,tr)rκ(tr) and d(zr,tr)rκ(tr)d(y_{r},t_{r})\geq r\kappa(t_{r})\text{ and }d(z_{r},t_{r})\geq r\kappa(t_{r})

Up to replacing xrx_{r} by some xrx_{r}^{\prime} in [xr,(xr)b],[x_{r},(x_{r})_{b}], we may assume

d(tr,[yr,xr][zr,xr])=rκ(tr).d(t_{r},[y_{r},x_{r}]\cup[z_{r},x_{r}])=r\kappa(t_{r}).

Thus, we have d(tr,[yr,xr])=rκ(tr)d(t_{r},[y_{r},x_{r}])=r\kappa(t_{r}) or d(tr,[zr,xr])=rκ(tr)d(t_{r},[z_{r},x_{r}])=r\kappa(t_{r}), without loss of generality, say d(tr,[yr,xr])=rκ(tr)d(t_{r},[y_{r},x_{r}])=r\kappa(t_{r}). Up to replacing [xr,zr][x_{r},z_{r}] by [xr,zr][x_{r},z_{r}^{\prime}] with zrzr,||z_{r}^{\prime}||\leq||z_{r}||, we may also assume d(tr,[xr,zr])=rκ(tr)d(t_{r},[x_{r},z_{r}])=r\kappa(t_{r}). Therefore, we have xr,yr,zr,trx_{r},y_{r},z_{r},t_{r} with

d(tr,[yr,xr])=rκ(tr)d(t_{r},[y_{r},x_{r}])=r\kappa(t_{r}) and d(tr,[zr,xr])=rκ(tr).d(t_{r},[z_{r},x_{r}])=r\kappa(t_{r}).

Let aa be the point on [yr,tr][y_{r},t_{r}] at distance 3rκ(tr)3r\kappa(t_{r}) from trt_{r} (if no such aa exists, choose a=yr)a=y_{r}) and let aa^{\prime} be the projection of aa on [yr,xr].[y_{r},x_{r}]. By convexity of the CAT(0) metric, we have

d(a,a)=d(a,[yr,xr])d(tr,[yr,xr])=rκ(tr).d(a,a^{\prime})=d(a,[y_{r},x_{r}])\leq d(t_{r},[y_{r},x_{r}])=r\kappa(t_{r}).

Similarly, if cc is the point in [tr,zr][t_{r},z_{r}] at distance 3rκ(tr)3r\kappa(t_{r}) from trt_{r} (or c=zrc=z_{r} if d(tr,zr)<3κ(tr))d(t_{r},z_{r})<3\kappa(t_{r})) and cc^{\prime} is the projection of cc on [xr,zr],[x_{r},z_{r}], then we have

d(c,c)rκ(tr).d(c,c^{\prime})\leq r\kappa(t_{r}).

Now, let ee be the point on [xr,tr][x_{r},t_{r}] at distance 3rκ(tr)3r\kappa(t_{r}) from trt_{r} (or e=xre=x_{r} if d(tr,xr)<3κ(tr)d(t_{r},x_{r})<3\kappa(t_{r})) and let e,e′′e^{\prime},e^{\prime\prime} be the projections of ee on [xr,yr],[xr,zr][x_{r},y_{r}],[x_{r},z_{r}] respectively. By the convexity of the CAT(0) metric, we have

d(e,e)rκ(tr) and d(e,e′′)rκ(tr).d(e,e^{\prime})\leq r\kappa(t_{r})\quad\text{ and }\quad d(e,e^{\prime\prime})\leq r\kappa(t_{r}).

Also, since projections in CAT(0) spaces are distance decreasing, we have

d(a,e)6rκ(tr) and d(c,e′′)6rκ(tr).d(a^{\prime},e^{\prime})\leq 6r\kappa(t_{r})\quad\text{ and }\quad d(c^{\prime},e^{\prime\prime})\leq 6r\kappa(t_{r}).

Now, consider the path β\beta connecting p1=b(trrκ(tr))p_{1}=b(t_{r}-r\kappa(t_{r})) to p2=b(tr+rκ(tr))p_{2}=b(t_{r}+r\kappa(t_{r}))

β=[p1,a][a,a][a,e][e,e][e,e′′][e′′,c][c,c][c,p2]\beta=[p_{1},a]\cup[a,a^{\prime}]\cup[a^{\prime},e^{\prime}]\cup[e^{\prime},e]\cup[e,e^{\prime\prime}]\cup[e^{\prime\prime},c^{\prime}]\cup[c^{\prime},c]\cup[c,p_{2}].

The length of this path

|β|2rκ(tr)+rκ(tr)+6rκ(tr)+rκ(tr)+rκ(tr)+6rκ(tr)+rκ(tr)+2rκ(tr)=20rκ(tr).|\beta|\leq 2r\kappa(t_{r})+r\kappa(t_{r})+6r\kappa(t_{r})+r\kappa(t_{r})+r\kappa(t_{r})+6r\kappa(t_{r})+r\kappa(t_{r})+2r\kappa(t_{r})=20r\kappa(t_{r}).

Therefore, we have |β|κ(tr)20r\frac{|\beta|}{\kappa(t_{r})}\leq 20r. It remains to show that β\beta lies outside the ball B=B(tr,rκ(tr))B=B(t_{r},r\kappa(t_{r})). Notice that we either have d(a,tr)=3rκ(tr)d(a,t_{r})=3r\kappa(t_{r}), where the distance d(a,B(tr,rκ(tr))=2rκ(tr)>rκ(tr)d(a,B(t_{r},r\kappa(t_{r}))=2r\kappa(t_{r})>r\kappa(t_{r}) and hence the geodesic [a,a][a,a^{\prime}] lies outside B=B(tr,rκ(tr))B=B(t_{r},r\kappa(t_{r})) as d(a,a)rκ(tr)d(a,a^{\prime})\leq r\kappa(t_{r}); or we have a=yra=y_{r} and aa is outside B=B(tr,rκ(tr))B=B(t_{r},r\kappa(t_{r})) by the convexity of the CAT(0) metric. Similarly, the geodesics [c,c],[e,e][c,c^{\prime}],[e,e^{\prime}] and [e,e′′][e,e^{\prime\prime}] all lie outside BB. On the other hand, the geodesics [p1,a],[a,e],[e′′,c][p_{1},a],[a^{\prime},e^{\prime}],[e^{\prime\prime},c^{\prime}] and [c,p2][c,p_{2}] also lie outside BB by construction.

4. κ\kappa–contracting geodesic rays in CAT(0) cube complexes

The main theorem we aim to prove in this section is Theorem B, restated here:

Theorem 4.1.

Let XX be a locally finite cube complex. A geodesic ray bXb\in X is κ\kappa-contracting if and only if there exists 𝖼>0{\sf c}>0 such that bb crosses an infinite sequence of hyperplanes h1,h2,h_{1},h_{2},... at points b(ti)b(t_{i}) satisfying:

  1. (1)

    d(ti,ti+1)𝖼κ(ti+1).d(t_{i},t_{i+1})\leq{\sf c}\kappa(t_{i+1}).

  2. (2)

    hi,hi+1h_{i},h_{i+1} are 𝖼κ(ti+1){\sf c}\kappa(t_{i+1})-well-separated.

First we refer to geodesic ray that satisfies the exact condition of this theorem as κ\kappa–excursion geodesics. The constant 𝖼{\sf c} will be referred to as the excursion constant.

Definition 4.2 (CAT(0)\operatorname{CAT}(0) cube complexes).

Given d0d\geq 0, a dd–cube is a copy of [0,1]d[0,1]^{d}, equipped with Euclidean metric. Its dimension is dd. A mid-cube is a subspace obtained by restricting exactly one coordinate to 1/2. Mid-cubes are (d1)(d-1)–cubes.

A cube complex is a CW complex XX such that

  • each cell is a dd–cube for some dd;

  • each cell is attached using an isometry of some face.

The dimension of XX is the supremum of the set of dimensions of cubes of XX. A CAT(0)\operatorname{CAT}(0) cube complex is a cube complex whose underlying space is a CAT(0)\operatorname{CAT}(0) space. We put an equivalence relation on the set of mid-cubes generated by the condition that two mid-cubes are equivalent if they share a face. A hyperplane is the union of all the mid-cubes in an equivalence class.

Let XX be a finite dimensional CAT(0) cube complex (not necessarily uniformly locally finite) of dimension vv. Let X(1)X^{(1)} denote the 1-skeleton of XX. We denote the distance function in the CAT(0) space XX by dd, and the 1\ell^{1}-distance by d(1).d^{(1)}. A geodesic in the dd-metric is said to be a CAT(0) geodesic while a geodesic in the d(1)d^{(1)}-metric is said to be a combinatorial geodesic. For x,yX(1)x,y\in X^{(1)}, we let 𝒞x,y\mathcal{C}_{x,y} denote the collection of hyperplanes separating xx from yy. The CAT(0)\operatorname{CAT}(0) distance between two points in a CAT(0)\operatorname{CAT}(0) cube complex is multiplicatively related to 𝒞x,y\mathcal{C}_{x,y}:

Lemma 4.3 ([CS11, Lemma 2.2]).

Let XX be a CAT(0) cube complex, then there exists a constant 𝖼{\sf c} depending only on the dimension of XX, such that for any x,yXx,y\in X, we have

d(x,y)|𝒞x,y|𝖼d(x,y)d(x,y)\leq|\mathcal{C}_{x,y}|\leq{\sf c}d(x,y).

We also need the following remark.

Remark 4.4.

If B(1)B^{(1)} is a ball of radius rr in the d(1)d^{(1)}–metric, then the d(1)d^{(1)} convex hull of B(1)B^{(1)} in X(1)X^{(1)} has diameter at most 2vr.2vr.

4.1. Counterexample to sublinear bound on separation

Two hyperplanes are said to be kk-separated if the number of hyperplanes crossing them both is bounded above by kk. In [CS15], Charney and Sultan give the following characterization for uniformly contracting geodesic rays in CAT(0) cube complexes. Recall that a geodesic ray bb is said to be uniformly contracting if it is κ\kappa-contracting with κ=1\kappa=1.

Theorem 4.5 ([CS15, Theorem 4.2]).

Let XX be a uniformly locally finite CAT(0) cube complex. There exist r>0,r>0, k0k\geq 0 such that a geodesic ray bb in XX is uniformly contracting if and only if bb crosses an infinite sequence of hyperplanes h1,h2,h3h_{1},h_{2},h_{3}, . . . at points xi=bhix_{i}=b\cap h_{i} satisfying:

  1. (1)

    hi,hi+1h_{i},h_{i+1} are kk-separated and

  2. (2)

    d(xi,xi+1)r.d(x_{i},x_{i+1})\leq r.

It may be natural to expect that κ\kappa-contracting geodesic rays are characterized where both kk and rr are replaced by the κ\kappa-function. This is in fact not the case:

Example 4.6.

Let Γn\Gamma_{n} be the graph of an nn-depth binary tree, see Figure 5. Note that Γn\Gamma_{n} embeds into Γn+1\Gamma_{n+1} by mapping the base-point of one to the other and extending upwards in the natural way.

Figure 5. Binary tree Γ2\Gamma_{2}

We can now construct the cube complex, XX. For each n{0},n\in\mathbb{N}\cup\{0\}, create the following sub-complexes Cn=Γn×[0,2n]C_{n}=\Gamma_{n}\times[0,2^{n}]. Next, for each nn glue the second face of CnC_{n} (the face Γn×{2n}\Gamma_{n}\times\{2^{n}\}) to the first face of Cn+1C_{n+1} (the face Γn+1×{0}\Gamma_{n+1}\times\{0\}) via the embedding ΓnΓn+1\Gamma_{n}\hookrightarrow\Gamma_{n+1}.

Consider the geodesic ray b(t)b(t) which is the bottom edge of the complex XX. i.e. if we orient XX so that in each CnC_{n} we have all the branches of the binary tree pointing upwards, the image of b(t)b(t) is the bottom most edge of the complex (in particular, b(0)b(0) is the bottom vertex of Γ0×{0})\Gamma_{0}\times\{0\}).

We claim the following about the complex XX and b(t)b(t):

  1. (1)

    Every point xCnx\in C_{n} is at most distance nn away from the geodesic bb.

  2. (2)

    For any tt, if b(t)Cnb(t)\in C_{n} then 2n1t2n+11.2^{n}-1\leq t\leq 2^{n+1}-1.

  3. (3)

    The geodesic ray bb is κ\kappa-contracting: (1) and (2) implies that the geodesic bb satisfies the condition of Lemma 2.9. (a quick verification of this is to look at XX sidelong and the complex will be contained under the curve of log2(x+1)\log_{2}(x+1) which is sublinear). We present the proof of (3) in more details:

    Proof.

    Let x,yXx,y\in X so that d(x,y)d(x,b)d(x,y)\leq d(x,b). Now since xXx\in X there is an nn with xCnx\in C_{n}. Claim 1 says that d(x,b)nd(x,b)\leq n, so we know that d(xb,yb)nd(x_{b},y_{b})\leq n, but since xbCnx_{b}\in C_{n} as well, by Fact 2 we see that 2n1d(b(0),xb)=xb2^{n}-1\leq d(b(0),x_{b})=||x_{b}||. This gives us that nlog2(xb+1)n\leq\log_{2}(||x_{b}||+1) and so d(xb,yb)log2(xb+1)d(x_{b},y_{b})\leq\log_{2}(||x_{b}||+1). A little algebra implies the existence of a constant 𝖼{\sf c} so that d(xb,yb)𝖼log2(xb)d(x_{b},y_{b})\leq{\sf c}\log_{2}(x_{b}) which shows that bb is log2\log_{2}-contracting, hence, we are done.

  4. (4)

    If hi1h_{i-1} and hih_{i} are a pair of hyperplanes in XX which intersect b(t)b(t) such that hi1h_{i-1} is in CnC_{n} and hih_{i} is in CmC_{m} with nmn\leq m, then hi1h_{i-1} and hih_{i} are at (2n+12)(2^{n+1}-2)–separated but are only 2n2n-well separated.

    Proof.

    Since hi1h_{i-1} intersects bb it will be isometric to the graph Γn\Gamma_{n}. The midpoint of every edge in Γn\Gamma_{n} corresponds to a hyperplane that intersects hi1h_{i-1}, and this is all of them. Each of these hyperplanes also intersects hih_{i} since hih_{i} is either also in CnC_{n} or in CmC_{m} with m>nm>n and intersects hih_{i} at the same midpoints of the edges of ΓnΓm\Gamma_{n}\subset\Gamma_{m}. Since there are exactly 2n+122^{n+1}-2 edges in Γn\Gamma_{n} then hi1h_{i-1} and hih_{i} are (2n+12)(2^{n+1}-2)–separated.

    Now consider a collection of hyperplanes that intersect hi1h_{i-1}. Since hi1h_{i-1} is isometric to Γn\Gamma_{n} we may consider the intersection points as points in Γn\Gamma_{n}. If the convex hull of these points contains a tripod then there are three hyperplanes in the collection that form a facing triple. If the convex hull doesn’t contain a tripod, then the points fall on a single geodesic line. The largest geodesic line inside of Γn\Gamma_{n} is length 2n2n. Thus any collection of hyperplanes with no facing triples can only intersect 2n2n edges and so has cardinality at most 2n2n.

4.1.1. Proof of Theorem D

Let κ(t)\kappa(t) be any sublinear function, let 𝖼{\sf c} be some constant, and let \mathcal{H} be a sequence of hyperplanes with

b(ti)hi and |titi+1|<𝖼κ(ti+1).b(t_{i})\cap h_{i}\neq\emptyset\text{ and }|t_{i}-t_{i+1}|<{\sf c}\kappa(t_{i+1}).

For each pair of hyperplanes hih_{i} and hi+1h_{i+1}, let K(ti+1)K(t_{i+1}) be the smallest number such that they are K(ti+1)K(t_{i+1})–separated.

For each tit_{i} there is a unique integer nin_{i}, so that nilog2(ti+1)ni+1n_{i}\leq\log_{2}(t_{i}+1)\leq n_{i}+1. However, this implies the following inequality

(5) 2ni1ti2ni+11.2^{n_{i}}-1\leq t_{i}\leq 2^{n_{i}+1}-1.

But by construction, this is simply the statement that b(ti)Cnib(t_{i})\in C_{n_{i}} and thus that hiCnih_{i}\in C_{n_{i}}. It follows immediately that hi+1h_{i+1} is in CmC_{m} for mnim\geq n_{i}. We can then apply fact (4) to get that hih_{i} and hi+1h_{i+1} are (2ni+12)(2^{n_{i}+1}-2)–separated. This tells us that K(ti+1)=2ni+12K(t_{i+1})=2^{n_{i}+1}-2.

Using inequality (5) we get that ti1K(ti+1)t_{i}-1\leq K(t_{i+1}), or in other words that tiK(ti+1)+1t_{i}\leq K(t_{i+1})+1. In particular this means that 1limtiK(ti+1)ti1\leq\lim_{t_{i}\to\infty}\frac{K(t_{i+1})}{t_{i}}, and so K(ti+1)K(t_{i+1}) is asymptotically linear. Since ti+1ti𝖼κ(ti+1)t_{i+1}-t_{i}\leq{\sf c}\kappa(t_{i+1}), and since κ\kappa is a sublinear function, we can choose ii large enough so that ti+1ti+𝖼κ(ti+1)ti+𝖼ti+12𝖼t_{i+1}\leq t_{i}+{\sf c}\kappa(t_{i+1})\leq t_{i}+{\sf c}\frac{t_{i+1}}{2{\sf c}} and hence ti+12ti\frac{t_{i+1}}{2}\leq t_{i} or ti+12tit_{i+1}\leq 2t_{i}. This implies that

1limtiK(ti+1)tilimti2K(ti+1)ti+1,1\leq\lim_{t_{i}\to\infty}\frac{K(t_{i+1})}{t_{i}}\leq\lim_{t_{i}\to\infty}\frac{2K(t_{i+1})}{t_{i+1}},

and hence limtiK(ti+1)ti+112\lim_{t_{i}\to\infty}\frac{K(t_{i+1})}{t_{i+1}}\geq\frac{1}{2}. Since κ(ti+1)\kappa(t_{i+1}) is a sublinear function, we get that K(ti+1)K(t_{i+1}) strictly dominates κ(ti+1)\kappa(t_{i+1}) for large enough values of tit_{i}.

On the other hand, by Lemma 2.9, b(t)b(t) is a log2\log_{2}-contracting geodesic. More precisely, if we take the sequence of hyperplanes that intersect b(t)b(t) we can see that hih_{i} and hi+1h_{i+1} are at most 2log2(ti+1)2\log_{2}(t_{i}+1)-well separated, since the longest chain of hyperplanes which intersect both is at most twice the height of the binary tree that hih_{i} lives inside.

4.2. The characterization theorem.

Now we are ready to present and prove Theorem B in the introduction.

Definition 4.7 (Facing Triples).

A collection of three hyperplanes h1,h2,h3h_{1},h_{2},h_{3} is said to form a facing triple if they are disjoint and none of the three hyperplanes separates the other two.

Notice that if a (combinatorial or CAT(0)) geodesic bb crosses three disjoint hyperplanes h1,h2h_{1},h_{2} and h3h_{3} respectively, then h2h_{2} separates h1h_{1} and h3.h_{3}. In particular, a geodesic bb cannot cross a facing triple. Conversely, if 𝒞\mathcal{C} is a collection of hyperplanes which contains no facing triple, then there is a geodesic which crosses a definite proportion of the hyperplanes in 𝒞\mathcal{C}:

Lemma 4.8 ([Hag, Corollary 3.4]).

Let XX be a CAT(0) cube complex of dimension vv. There exists a constant kk, depending only on vv, such that the following holds. If 𝒞\mathcal{C} is a collection of hyperplanes which contains no facing triple, then there exists a (combinatorial or CAT(0)) geodesic which crosses at least |𝒞|k\frac{\mathcal{|C|}}{k} hyperplanes from the collection 𝒞.\mathcal{C}.

Definition 4.9 (Well-separated hyperplanes).

Two disjoint hyperplanes h1,h2h_{1},h_{2} are said to be kk-well-separated if any collection of hyperplanes intersecting both h1,h2h_{1},h_{2}, and which does not contain any facing triple, has cardinality at most kk. We say that h1h_{1} and h2h_{2} are well-separated if they are kk-well-separated for some k.k.

Definition 4.10 (Combinatorial projections).

Let XX be a CAT(0) cube complex and let X(1)X^{(1)} be its 1-skeleton with the d(1)d^{(1)}-metric. Let ZZ be a convex sub-complex. For all xX(0)x\in X^{(0)}, the point 𝔤Z(x)Z\mathfrak{g}_{Z}(x)\in Z is defined to be the closest vertex in ZZ to xx. The vertex 𝔤Z(x)\mathfrak{g}_{Z}(x) is unique and it is characterized by the property that a hyperplane hh separates 𝔤(x)\mathfrak{g}(x) from xx if and only if hh separates xx from ZZ, for more details see [BHS17].

The following proposition states that for a convex sub-complex ZZ and for x,yZx,y\notin Z, if a hyperplane hh separates xx and yy then either hh doesn’t intersect ZZ, or if does, it separates 𝔤Z(x)\mathfrak{g}_{Z}(x) and 𝔤Z(y).\mathfrak{g}_{Z}(y).

Proposition 4.11 ([Gen20a, Proposition 2.7]).

Let ZZ be a convex sub-complex in a CAT(0) cube complex XX and let x,yx,y be two vertices of X(1)X^{(1)}. The hyperplanes separating 𝔤Z(x)\mathfrak{g}_{Z}(x) and 𝔤Z(y)\mathfrak{g}_{Z}(y) are precisely the ones separating xx and yy which intersect Z.Z.

We proceed with a few lemmas working towards the forward direction of the argument.

Lemma 4.12.

Let XX be a CAT(0) cube complex of dimension vv and suppose bb is a κ\kappa-contracting geodesic ray in XX. There exists a constant 𝖼{\sf c} such that if t,st,s\in\mathbb{R} are such that ts𝖼κ(t)t-s\geq{\sf c}\kappa(t), then [b(s),b(t)][b(s),b(t)] crosses a hyperplane whose nearest-point projection to bb is entirely between b(s)b(s) and b(t).b(t).

Proof.

Let 𝒞\mathcal{C} be the collection of hyperplanes which cross [b(s),b(t)][b(s),b(t)]. Let h𝒞,h\in\mathcal{C}, and define z=hbz=h\cap b. If hh projects outside [b(s),b(t)][b(s),b(t)], then it contains a point xx with xb=b(t)x_{b}=b(t) or xb=b(s)x_{b}=b(s). If hh contains a point xx with xb=b(t)x_{b}=b(t), then using κ\kappa-slimness of the triangle Δ=Δ(x,b(t),z),\Delta=\Delta(x,b(t),z), there exists a constant 𝖼1{\sf c}_{1} such that hB𝖼1κ(t)(b(t)).h\cap B_{{\sf c}_{1}\kappa(t)}(b(t))\neq\emptyset. Since the CAT(0) metric is bounded above and below by linear functions of the d(1)d^{(1)}-metric, depending only on the dimension vv, there exists a constant 𝖼2=𝖼2(v,𝖼1){\sf c}_{2}={\sf c}_{2}(v,{\sf c}_{1}) such that the ball B𝖼1κ(t)(b(t))B_{{\sf c}_{1}\kappa(t)}(b(t)) is contained in a combinatorial ball B(1)B^{(1)} of radius 𝖼2κ(t){\sf c}_{2}\kappa(t).

By Remark 4.4, the diameter of the convex hull ZZ of B(1)B^{(1)} is at most 2v𝖼2κ(t),2v{\sf c}_{2}\kappa(t), where vv bounds the dimension of the cube complex.

Let x,yX(1)x,y\in X^{(1)} be two vertices which are separated by every hyperplane in 𝒞\mathcal{C}. Since ZZ has diameter at most 2v𝖼2κ(t)2v{\sf c}_{2}\kappa(t), we have

d(𝔤Z(x),𝔤Z(y))2v𝖼2κ(t).d(\mathfrak{g}_{Z}(x),\mathfrak{g}_{Z}(y))\leq 2v{\sf c}_{2}\kappa(t).

Also, using Proposition 4.11, any hyperplane h𝒞h\in\mathcal{C} that crosses ZZ separates 𝔤Z(x),𝔤Z(y)\mathfrak{g}_{Z}(x),\mathfrak{g}_{Z}(y). Thus, the number of such hyperplanes is at most diam(Z)2v𝖼2κ(t)diam(Z)\leq 2v{\sf c}_{2}\kappa(t).

Therefore, 2v𝖼2κ(t)2v{\sf c}_{2}\kappa(t) bounds the number of hyperplanes h𝒞h\in\mathcal{C} that have a projection point to b(t).b(t). Similarly, 2v𝖼2κ(s)2v{\sf c}_{2}\kappa(s) bounds the number of hyperplanes h𝒞h\in\mathcal{C} which project to b(s)b(s). In turns, the number of hyperplanes h𝒞,h\in\mathcal{C}, projecting outside [b(s),b(t)][b(s),b(t)] is at most 2v𝖼2(κ(s)+κ(t))4v𝖼2κ(t),2v{\sf c}_{2}(\kappa(s)+\kappa(t))\leq 4v{\sf c}_{2}\kappa(t), where 𝖼2{\sf c}_{2} depends only on vv and 𝖼1.{\sf c}_{1}. Therefore, choosing 𝖼{\sf c} so that the number of hyperplanes crossed by [b(s),b(t)][b(s),b(t)] exceeds 4v𝖼24v{\sf c}_{2} gives the desired result.

Lemma 4.13.

Let bb be a κ\kappa-contracting geodesic ray with constant 𝖼{\sf c} and let x,yXx,y\in X and not in bb such that d(yb,b(0))d(xb,b(0))d(y_{b},b(0))\geq d(x_{b},b(0)). If d(xb,yb)3𝖼κ(yb),d(x_{b},y_{b})\geq 3{\sf c}\kappa(y_{b}), then we have the following:

d(x,y)d(x,xb)+d(xb,yb)+d(yb,y)𝖼κ(xb)𝖼κ(yb).d(x,y)\geq d(x,x_{b})+d(x_{b},y_{b})+d(y_{b},y)-{\sf c}\kappa(x_{b})-{\sf c}\kappa(y_{b}).
Proof.

First, we will show that d(x,y)d(x,xb)+d(y,yb).d(x,y)\geq d(x,x_{b})+d(y,y_{b}). For the sake of contradiction, suppose that d(x,y)<d(x,xb)+d(y,yb).d(x,y)<d(x,x_{b})+d(y,y_{b}). This implies the existence of a point z[x,y]z\in[x,y] such that d(z,x)<d(x,xb)d(z,x)<d(x,x_{b}) and d(z,y)<d(y,yb).d(z,y)<d(y,y_{b}). Since our geodesic bb is κ\kappa-contracting, we obtain that d(xb,zb)𝖼κ(xb)d(x_{b},z_{b})\leq{\sf c}\kappa(x_{b}) and d(yb,zb)𝖼κ(yb)d(y_{b},z_{b})\leq{\sf c}\kappa(y_{b}). This implies that

d(xb,yb)d(xb,zb)+d(zb,yb)𝖼κ(xb)+𝖼κ(yb)2𝖼κ(yb),d(x_{b},y_{b})\leq d(x_{b},z_{b})+d(z_{b},y_{b})\leq{\sf c}\kappa(x_{b})+{\sf c}\kappa(y_{b})\leq 2{\sf c}\kappa(y_{b}),

contradicting the assumption that d(xb,yb)3𝖼κ(yb).d(x_{b},y_{b})\geq 3{\sf c}\kappa(y_{b}). Thus we have shown that

d(x,y)d(x,xb)+d(y,yb).d(x,y)\geq d(x,x_{b})+d(y,y_{b}).

Let xx^{\prime} be the point on [x,y][x,y] at distance d(x,xb)d(x,x_{b}) from xx. Similarly, let yy^{\prime} be the point on [x,y][x,y] at distance d(y,yb)d(y,y_{b}) from yy. The projections of [x,x][x,x^{\prime}] and [y,y][y^{\prime},y] to bb have diameters at most 𝖼κ(xb){\sf c}\kappa(x_{b}) and 𝖼κ(yb){\sf c}\kappa(y_{b}), respectively. Since projections in CAT(0) are distance decreasing, we have

d(x,y)d(xb,yb)d(xb,yb)𝖼κ(xb)𝖼κ(yb).d(x^{\prime},y^{\prime})\geq d(x^{\prime}_{b},y^{\prime}_{b})\geq d(x_{b},y_{b})-{\sf c}\kappa(x_{b})-{\sf c}\kappa(y_{b}).

Now, we have

d(x,y)\displaystyle d(x,y) =d(x,x)+d(x,y)+d(y,y)\displaystyle=d(x,x^{\prime})+d(x^{\prime},y^{\prime})+d(y^{\prime},y)
=d(x,xb)+d(x,y)+d(y,yb)\displaystyle=d(x,x_{b})+d(x^{\prime},y^{\prime})+d(y,y_{b})
d(x,xb)+d(xb,yb)𝖼κ(xb)𝖼κ(yb)+d(y,yb).\displaystyle\geq d(x,x_{b})+d(x_{b},y_{b})-{\sf c}\kappa(x_{b})-{\sf c}\kappa(y_{b})+d(y,y_{b}).

Lemma 4.14.

Let bb be a κ\kappa-contracting geodesic ray starting at 𝔬{\mathfrak{o}} with constant 𝖼{\sf c}. Let x,yXx,y\in X and not in bb such that d(𝔬,xb)d(𝔬,yb)d({\mathfrak{o}},x_{b})\leq d({\mathfrak{o}},y_{b}) and d(xb,yb)4𝖼κ(yb).d(x_{b},y_{b})\geq 4{\sf c}\kappa(y_{b}). We have the following:

  1. (1)

    d(x,y)d(x,xb)+d(xb,yb)+d(yb,y)2𝖼κ(yb).d(x,y)\geq d(x,x_{b})+d(x_{b},y_{b})+d(y_{b},y)-2{\sf c}\kappa(y_{b}).

  2. (2)

    πb([x,y])N5𝖼κ(yb)([x,y]).\pi_{b}([x,y])\subseteq N_{5{\sf c}\kappa(y_{b})}([x,y]).

xxyyxbx_{b}yby_{b}d(xb,yb)4cκ(yb)d(x_{b},y_{b})\geq 4c\kappa(y_{b})[x,y][x,y]
Figure 6. d(xb,[x,y])5cκ(xb),d(yb,[x,y])5cκ(xb).d(x_{b},[x,y])\leq 5c\kappa(x_{b}),d(y_{b},[x,y])\leq 5c\kappa(x_{b}).
Proof.

The first part follows from Lemma 4.13 since κ\kappa is a non-increasing function. Let x,yx^{\prime},y^{\prime} be as in the previous problem. This gives that

d(x,y)\displaystyle d(x,y) =d(x,x)+d(x,y)+d(y,y)\displaystyle=d(x,x^{\prime})+d(x^{\prime},y^{\prime})+d(y^{\prime},y)
=d(x,xb)+d(x,y)+d(y,yb)\displaystyle=d(x,x_{b})+d(x^{\prime},y^{\prime})+d(y,y_{b})
d(x,xb)+d(xb,yb)+d(y,yb).\displaystyle\leq d(x,x_{b})+d(x_{b},y_{b})+d(y,y_{b}).

Thus, d(x,y)d(xb,yb).d(x^{\prime},y^{\prime})\leq d(x_{b},y_{b}). Now, applying part (1) to x,yx^{\prime},y^{\prime}, we get that

d(xb,yb)\displaystyle d(x_{b},y_{b}) d(x,y)\displaystyle\geq d(x^{\prime},y^{\prime})
d(x,xb)+d(xb,yb)+d(y,yb)2𝖼κ(yb)\displaystyle\geq d(x^{\prime},x^{\prime}_{b})+d(x^{\prime}_{b},y^{\prime}_{b})+d(y^{\prime},y^{\prime}_{b})-2{\sf c}\kappa(y^{\prime}_{b})
d(x,xb)+d(xb,yb)2𝖼κ(yb)+d(y,yb)2𝖼κ(yb)\displaystyle\geq d(x^{\prime},x^{\prime}_{b})+d(x_{b},y_{b})-2{\sf c}\kappa(y_{b})+d(y^{\prime},y^{\prime}_{b})-2{\sf c}\kappa(y^{\prime}_{b})
d(x,xb)+d(xb,yb)2𝖼κ(yb)+d(y,yb)2𝖼κ(yb)\displaystyle\geq d(x^{\prime},x^{\prime}_{b})+d(x_{b},y_{b})-2{\sf c}\kappa(y_{b})+d(y^{\prime},y^{\prime}_{b})-2{\sf c}\kappa(y_{b})
d(x,xb)+d(xb,yb)+d(y,yb)4𝖼κ(yb).\displaystyle\geq d(x^{\prime},x^{\prime}_{b})+d(x_{b},y_{b})+d(y^{\prime},y^{\prime}_{b})-4{\sf c}\kappa(y_{b}).

This yields that d(x,xb)+d(y,yb)4𝖼κ(yb)d(x^{\prime},x^{\prime}_{b})+d(y^{\prime},y^{\prime}_{b})\leq 4{\sf c}\kappa(y_{b}). In particular,

max{d(x,xb),d(y,yb)}4𝖼κ(yb).\{d(x^{\prime},x^{\prime}_{b}),d(y^{\prime},y^{\prime}_{b})\}\leq 4{\sf c}\kappa(y_{b}).

Using convexity of the CAT(0) metric, we get that πb([x,y])N4𝖼κ(yb)([x,y])\pi_{b}([x^{\prime},y^{\prime}])\subseteq N_{4{\sf c}\kappa(y_{b})}([x,y]), but since every point in [xb,yb][x_{b},y_{b}] is within 𝖼κ(yb){\sf c}\kappa(y_{b}) of [xb,yb][x^{\prime}_{b},y^{\prime}_{b}], the result follows.

The proof of Theorem 4.1 is presented in two parts.

The forward direction of Theorem 4.1: κ\kappa-contracting implies κ\kappa-excursion

Let bb be a κ\kappa-contracting geodesic ray with constant 𝖼{\sf c} and let 𝖽{\sf d} be a constant as in Lemma 4.12. Since κ\kappa is a sublinear function, there exists an s00s_{0}\geq 0 such that if ss0,s\geq s_{0}, we have κ(s)s2𝖽\kappa(s)\leq\frac{s}{2{\sf d}}. Choose s1s0s_{1}\geq s_{0} and divide the geodesic ray into pieces 0<s1<s1<s2<s2<<si<si<..0<s_{1}<s^{\prime}_{1}<s_{2}<s^{\prime}_{2}<...<s_{i}<s^{\prime}_{i}<.. such that for each ii, we have

sisi\displaystyle s^{\prime}_{i}-s_{i} =𝖽κ(si),\displaystyle={\sf d}\kappa(s^{\prime}_{i}),
si+1si\displaystyle s_{i+1}-s^{\prime}_{i} =4𝖼(1+2𝖽)κ(si+1).\displaystyle=4{\sf c}(1+2{\sf d})\kappa(s_{i+1}).

Therefore, si=si+𝖽κ(si)si+𝖽si2𝖽s^{\prime}_{i}=s_{i}+{\sf d}\kappa(s^{\prime}_{i})\leq s_{i}+{\sf d}\frac{s^{\prime}_{i}}{2{\sf d}} and hence si2si\frac{s^{\prime}_{i}}{2}\leq s_{i} or si2si.s^{\prime}_{i}\leq 2s_{i}.

Lemma 4.12 assures that each [b(si),b(si)][b(s_{i}),b(s_{i}^{\prime})] crosses a hyperplane hih_{i} whose projection lies entirely inside [b(si),b(si)][b(s_{i}),b(s_{i}^{\prime})]. Define b(ti):=hi[b(si),b(si)]b(t_{i}):=h_{i}\cap[b(s_{i}),b(s_{i}^{\prime})]. Since

d(b(ti),b(ti+1))\displaystyle d(b(t_{i}),b(t_{i+1})) d(si,si)+d(si,si+1)+d(si+1,si+1)\displaystyle\leq d(s_{i},s^{\prime}_{i})+d(s^{\prime}_{i},s_{i+1})+d(s_{i+1},s^{\prime}_{i+1})
𝖽κ(si)+4𝖼(1+2𝖽)κ(si+1)+𝖽κ(si+1)\displaystyle\leq{\sf d}\kappa(s^{\prime}_{i})+4{\sf c}(1+2{\sf d})\kappa(s_{i+1})+{\sf d}\kappa(s^{\prime}_{i+1})
𝖽κ(si)+4𝖼(1+2𝖽)κ(si+1)+2𝖽κ(si+1)\displaystyle\leq{\sf d}\kappa(s^{\prime}_{i})+4{\sf c}(1+2{\sf d})\kappa(s_{i+1})+2{\sf d}\kappa(s_{i+1})
𝖽κ(ti+1)+4𝖼(1+2𝖽)κ(ti+1)+2𝖽κ(ti+1)\displaystyle\leq{\sf d}\kappa(t_{i+1})+4{\sf c}(1+2{\sf d})\kappa(t_{i+1})+2{\sf d}\kappa(t_{i+1})
=(3𝖽+4𝖼(1+2𝖽))κ(ti+1).\displaystyle=(3{\sf d}+4{\sf c}(1+2{\sf d}))\kappa(t_{i+1}).

Let x,yx,y be in hi,hi+1\in h_{i},h_{i+1} respectively. Notice that as yb[b(si+1),b(si+1)]y_{b}\in[b(s_{i+1}),b(s^{\prime}_{i+1})], we have

ybsi+12si+1<(1+2𝖽)si+1.||y_{b}||\leq s^{\prime}_{i+1}\leq 2s_{i+1}<(1+2{\sf d})s_{i+1}.

Hence, we have

κ(yb)κ((1+2𝖽)si+1)(1+2𝖽)κ(si+1)(1+2𝖽)κ(ti+1).\kappa(||y_{b}||)\leq\kappa((1+2{\sf d})s_{i+1})\leq(1+2{\sf d})\kappa(s_{i+1})\leq(1+2{\sf d})\kappa(t_{i+1}).

Notice that diam(πb([x,y])4𝖼(1+2𝖽)κ(si+1)4𝖼κ(||yb||)=4𝖼κ(||yb||).(\pi_{b}([x,y])\geq 4{\sf c}(1+2{\sf d})\kappa(s_{i+1})\geq 4{\sf c}\kappa(||y_{b}||)=4{\sf c}\kappa(||y_{b}||). Using Lemma 4.14, any geodesic [x,y][x,y] connecting hih_{i} to hi+1h_{i+1} has to come 5𝖼κ(yb)5{\sf c}\kappa(y_{b}) close to every point in [ti,ti+1][t_{i},t_{i+1}]. In particular, we have [x,y]B5𝖼κ(yb)(ti+1)[x,y]\cap B_{5{\sf c}\kappa(||y_{b}||)}(t_{i+1})\neq\emptyset. Hence, using the equation above, we have

[x,y]B5𝖼(1+2𝖽)κ(ti+1)(ti+1).[x,y]\cap B_{5{\sf c}(1+2{\sf d})\kappa(t_{i+1})}(t_{i+1})\neq\emptyset.

Let 𝖼=5𝖼(1+2𝖽){\sf c}^{\prime}=5{\sf c}(1+2{\sf d}). The previous equation then implies that every hyperplane hh intersecting both hih_{i} and hi+1h_{i+1} meets B𝖼κ(ti+1)(ti+1)B_{{\sf c}^{\prime}\kappa(t_{i+1})}(t_{i+1}). Thus, if 𝒞\mathcal{C} denotes the collection of hyperplanes meeting both hi,hi+1h_{i},h_{i+1} which contain no facing triple, then |𝒞|<.|\mathcal{C}|<\infty. Since the CAT(0) metric is quasi-isometric to the d(1)d^{(1)}-metric, there exists a constant 𝖼1=𝖼1(v,𝖼){\sf c}_{1}={\sf c}_{1}(v,{\sf c}^{\prime}) such that the ball B𝖼κ(ti+1)(ti+1)B_{{\sf c}^{\prime}\kappa(t_{i+1})}(t_{i+1}) is contained in a combinatorial ball B(1)B^{(1)} of radius 𝖼1κ(ti+1){\sf c}_{1}\kappa(t_{i+1}).

Using Remark 4.4, the diameter of the convex hull ZZ of B(1)B^{(1)} is at most 2v𝖼1κ(ti+1),2v{\sf c}_{1}\kappa(t_{i+1}), where vv bounds the dimension of the cube complex.

By Lemma 4.8, there exist two points x,yX(1)x^{\prime},y^{\prime}\in X^{(1)} and 1k|𝒞|\frac{1}{k}|\mathcal{C}| hyperplanes in 𝒞\mathcal{C} which separate x,yx^{\prime},y^{\prime}, where kk is a uniform constant depending only on the dimension vv. Denote this collection by 𝒞\mathcal{C}^{\prime}. Since ZZ has diameter at most 2v𝖼1κ(ti+1)2v{\sf c}_{1}\kappa(t_{i+1}), we have d(𝔤Z(x),𝔤Z(y))2v𝖼1κ(ti+1)d(\mathfrak{g}_{Z}(x^{\prime}),\mathfrak{g}_{Z}(y^{\prime}))\leq 2v{\sf c}_{1}\kappa(t_{i+1}). Also, using Proposition 4.11, any hyperplane h𝒞h\in\mathcal{C}^{\prime} crossing ZZ separates 𝔤Z(x),𝔤Z(y)\mathfrak{g}_{Z}(x^{\prime}),\mathfrak{g}_{Z}(y^{\prime}). Thus, there can be at most diam(Z)2v𝖼1κ(ti+1)diam(Z)\leq 2v{\sf c}_{1}\kappa(t_{i+1}) such hyperplanes. Therefore, 2v𝖼1κ(ti+1)2v{\sf c}_{1}\kappa(t_{i+1}) bounds the number of hyperplanes h𝒞h\in\mathcal{C}^{\prime} which in turn implies that 2kv𝖼1κ(ti+1)2kv{\sf c}_{1}\kappa(t_{i+1}) bonds in the number of hyperplanes in 𝒞.\mathcal{C}.

4.2.1. The backward direction of Theorem 4.1: κ\kappa-excursion implies κ\kappa-contracting.

Let bb be the κ\kappa–excursion geodesic under consideration. Let [x,y][x,y] be a geodesic connecting xXx\in X to yby\in b. The following lemma states that if [x,y][x,y] meets one of the separated hyperplanes crossed by bb, it meets it at distance at most κ\kappa from bb. The following argument is inspired by the similar argument in [IM].

Lemma 4.15.

Let bb be a κ\kappa-excursion geodesic and let {hi}\{h_{i}\} be the sequence of well-separated hyperplanes crossed by bb. There exists a constant 𝖽{\sf d}, depending only on vv and the excursion constant 𝖼{\sf c}, such that the following holds:

  1. (1)

    If xhix\in h_{i} and yby\in b, with y>b(ti+2)y>b(t_{i+2}), then the geodesic [x,y][x,y] intersects hi+1h_{i+1} at distance at most 𝖽κ(ti+1){\sf d}\kappa(t_{i+1}) from b(ti+1)b(t_{i+1}).

  2. (2)

    If xhix\in h_{i} and yby\in b, with y<b(ti2)y<b(t_{i-2}), then the geodesic [x,y][x,y] intersects hi1h_{i-1} at distance at most 𝖽κ(ti1){\sf d}\kappa(t_{i-1}) from b(ti1)b(t_{i-1}).

yyxxx1x_{1}x2x_{2}C1C^{\prime}_{1}C2C^{\prime}_{2}C2C_{2}C2C_{2}C1C_{1}hih_{i}hi+1h_{i+1}hi+2h_{i+2}
Proof.

We give a detailed proof to (1), the proof for (2) is identical. Let 𝖼{\sf c} be the excursion constant of bb and let 𝖼1{\sf c}_{1} be a constant as in Lemma 4.3. Define x1=[x,y]hi+1x_{1}=[x,y]\cap h_{i+1}, x2=[x,y]hi+2x_{2}=[x,y]\cap h_{i+2} and let 𝒞\mathcal{C} denote the collection of hyperplanes intersecting [x1,b(ti+1)][x_{1},b(t_{i+1})]. The collection 𝒞\mathcal{C} contains no facing triple since every hyperplane in 𝒞\mathcal{C} is crossed by a geodesic. The collection 𝒞\mathcal{C} of hyperplanes intersects [b(ti+1),b(ti+2)][b(t_{i+1}),b(t_{i+2})], [x2,b(ti+2)][x_{2},b(t_{i+2})] or [x1,x2][x_{1},x_{2}]. Denote such hyperplanes by 𝒞1,𝒞2\mathcal{C}_{1},\mathcal{C}_{2} and 𝒞3\mathcal{C}_{3} respectively.

By Lemma 4.3, the number of hyperplanes in 𝒞\mathcal{C} intersecting both [x1,b(ti+1)][x_{1},b(t_{i+1})] and [b(ti+1),b(ti+2)][b(t_{i+1}),b(t_{i+2})] is bounded above by 𝖼1𝖼κ(ti+2).{\sf c}_{1}{\sf c}\kappa(t_{i+2}).

Since hi+1,hi+2h_{i+1},h_{i+2} are 𝖼κ(ti+2){\sf c}\kappa(t_{i+2})-well-separated, there is at most 𝖼κ(ti+2){\sf c}\kappa(t_{i+2}) hyperplanes in 𝒞\mathcal{C} that intersect [x2,b(ti+2)][x_{2},b(t_{i+2})]. Therefore, we have:

|𝒞|\displaystyle|\mathcal{C}| |𝒞1|+|𝒞2|+|𝒞3|\displaystyle\leq|\mathcal{C}_{1}|+|\mathcal{C}_{2}|+|\mathcal{C}_{3}|
𝖼1𝖼κ(ti+2)+𝖼κ(ti+2)+|𝒞3|\displaystyle\leq{\sf c}_{1}{\sf c}\kappa(t_{i+2})+{\sf c}\kappa(t_{i+2})+|\mathcal{C}_{3}|
=(𝖼1𝖼+𝖼)κ(ti+2)+|𝒞3|.\displaystyle=({\sf c}_{1}{\sf c}+{\sf c})\kappa(t_{i+2})+|\mathcal{C}_{3}|.

Every hyperplane in 𝒞3\mathcal{C}_{3} intersects [b(ti),b(ti+1)][b(t_{i}),b(t_{i+1})] or [x,b(ti)][x,b(t_{i})]. Denote such hyperplanes by 𝒞1,𝒞2\mathcal{C}^{\prime}_{1},\mathcal{C}^{\prime}_{2}, respectively.

Using Lemma 4.3, |𝒞1|𝖼1𝖼κ(ti+1)|\mathcal{C}^{\prime}_{1}|\leq{\sf c}_{1}{\sf c}\kappa(t_{i+1}). Since hi,hi+1h_{i},h_{i+1} are κ(ti+1)\kappa(t_{i+1})-well-separated, |𝒞2|𝖼κ(ti+1).|\mathcal{C}^{\prime}_{2}|\leq{\sf c}\kappa(t_{i+1}). Therefore,

|𝒞3|𝖼1𝖼κ(ti+1)+𝖼κ(ti+1)|\mathcal{C}_{3}|\leq{\sf c}_{1}{\sf c}\kappa(t_{i+1})+{\sf c}\kappa(t_{i+1})

This implies the following:

|𝒞|\displaystyle\mathcal{|C|} (𝖼1𝖼+𝖼)κ(ti+2)+|𝒞3|\displaystyle\leq({\sf c}_{1}{\sf c}+{\sf c})\kappa(t_{i+2})+|\mathcal{C}_{3}|
(𝖼1𝖼+𝖼)κ(ti+2)+𝖼1𝖼κ(ti+1)+𝖼κ(ti+1)\displaystyle\leq({\sf c}_{1}{\sf c}+{\sf c})\kappa(t_{i+2})+{\sf c}_{1}{\sf c}\kappa(t_{i+1})+{\sf c}\kappa(t_{i+1})
(𝖼1𝖼+𝖼)κ(ti+2)+𝖼1𝖼κ(ti+2)+𝖼κ(ti+2)\displaystyle\leq({\sf c}_{1}{\sf c}+{\sf c})\kappa(t_{i+2})+{\sf c}_{1}{\sf c}\kappa(t_{i+2})+{\sf c}\kappa(t_{i+2})
2(𝖼1𝖼+𝖼)κ(ti+2).\displaystyle\leq 2({\sf c}_{1}{\sf c}+{\sf c})\kappa(t_{i+2}).

Since 𝒞\mathcal{C} was defined to be the collection of hyperplanes separating intersecting the geodesic [x1,b(ti+1)][x_{1},b(t_{i+1})], using Lemma 4.3, we have d(x1,b(ti+1))2𝖼1(𝖼1𝖼+𝖼)κ(ti+2).d(x_{1},b(t_{i+1}))\leq 2{\sf c}_{1}({\sf c}_{1}{\sf c}+{\sf c})\kappa(t_{i+2}).

From Lemma 4.15 we have the following:

Corollary 4.16.

Let bb be a κ\kappa-excursion geodesic and let {hi}\{h_{i}\} be the sequence of well-separated hyperplanes crossed by bb. There exists a constant 𝖽{\sf d}, depending only on vv and the excursion constant 𝖼{\sf c}, such that the following holds:

  1. (1)

    For any xx between hi1h_{i-1} and hih_{i}, if yby\in b satisfies y>b(ti+2)y>b(t_{i+2}), then the geodesic [x,y][x,y] intersects hi+1h_{i+1} at distance at most 𝖽κ(ti+1){\sf d}\kappa(t_{i+1}) from b(ti+1)b(t_{i+1}).

  2. (2)

    For any xx between hih_{i} and hi+1h_{i+1}, if yby\in b satisfies y<b(ti2)y<b(t_{i-2}), then the geodesic [x,y][x,y] intersects hi1h_{i-1} at distance at most 𝖽κ(ti1){\sf d}\kappa(t_{i-1}) from b(ti1)b(t_{i-1}).

  3. (3)

    If xx lies between hih_{i} and hi+1h_{i+1}, then xbB𝖽κ(ti)(b(ti))x_{b}\in B_{{\sf d}\kappa(t_{i})}(b(t_{i})).

Proof.

For (1), define x:=[x,y]hix^{\prime}:=[x,y]\cap h_{i}. Applying Lemma 4.15 to the geodesic [x,y][x^{\prime},y] gives the desired claim. The proof of (2) is the exact same. For (3), if xb[b(ti2),b(ti+2)]x_{b}\in[b(t_{i-2}),b(t_{i+2})], then we are done since bb is a κ\kappa-excursion geodesic. Otherwise if xb[b(ti2),b(ti+2)]x_{b}\notin[b(t_{i-2}),b(t_{i+2})], then applying (1)(1) and (2)(2) to the geodesic [x,xb][x,x_{b}] yields the desired result.

Proof of the backward direction of Theorem 4.1

Let xXx\in X and let yby\in b, we will show that bb is κ\kappa-slim with respect to condition 1. In other words, we need to show there exists a constant 𝖼{\sf c} such that d(xb,[x,y])𝖼κ(xb),d(x_{b},[x,y])\leq{\sf c}\kappa(x_{b}), which follows from Corollary 4.16. Therefore, every κ\kappa-excursion geodesic is κ\kappa-slim and is hence κ\kappa-contracting.

4.3. Consequence for right-angled Artin groups

Recall that two hyperplanes h1,h2h_{1},h_{2} are strongly separated if they are disjoint and no hyperplane intersects both h1h_{1} and h2h_{2}. By [Gen20a], when the space in question is the Salvetti complex of a right-angled Artin group, two hyperplanes are strongly separated if and only if they are kk-well-separated for any kk. Based on this fact we have the following:

Corollary 4.17.

Let XX be the Salvetti complex complex of a right-angled Artin group, then a geodesic ray bb in XX is κ\kappa-contracting if and only if there exists constants 𝖼{\sf c} and an infinite sequence of strongly separated disjointed hyperplanes that bb crosses, labelled h1,h2,h_{1},h_{2},... at points b(ti)b(t_{i}) , such that d(b(ti),b(ti+1))=d(ti,ti+1)<𝖼κ(ti+1)d(b(t_{i}),b(t_{i+1}))=d(t_{i},t_{i+1})<{\sf c}\kappa(t_{i+1}).

Proof.

In a Salvetti complex, two hyperplanes are well-separated if and only if they are strongly separated, thus the corollary follows from Theorem 4.1. ∎

4.4. Progress in contact graphs associated with Salvetti complexes.

In [Hag13], Hagen introduced the contact graph of a CAT(0) cube complex. It is defined as follows. Recall that a hyperplane carrier is the union of all (closed) cubes intersecting a hyperplane hh, which we denote N(h)N(h).

Definition 4.18 (Contact graph).

Let XX be a CAT(0) cube complex, the contact graph of XX, denoted by 𝒳\mathcal{X}, is the intersection graph of the hyperplane carriers. In other words, it is a graph where vertices are hyperplane carriers in XX, and two vertices are connected by an edge if the corresponding hyperplanes carriers intersect. In this case we can also say the two hyperplanes have contact relation.

For a CAT(0) cube complex XX, there is a coarse map p:X𝒞Xp:X\rightarrow\mathcal{C}X: Given xX(0)x\in X^{(0)}, the set of hyperplanes hh with xN(h)x\in N(h) corresponds to a complete subgraph of 𝒞X\mathcal{C}X, which we denote p(x)p(x). Hence p:X(0)𝒞Xp:X^{(0)}\rightarrow\mathcal{C}X is a coarse map. For each edge ee of XX, we define p(e)p(e) to be the vertex corresponding to the hyperplane dual to ee. Hence we have a coarse map p:X(1)𝒞Xp:X^{(1)}\rightarrow\mathcal{C}X. More generally, if cc is an open nn–cube, n1n\geq 1, let p(c)p(c) be the complete subgraph with vertex set the hyperplanes intersecting cc.

As an application to Theorem 4.1, we will prove the Corollary C from the introduction. But first we need a lemma:

Lemma 4.19.

Let bb be a geodesic ray in a finite dimensional CAT(0)\operatorname{CAT}(0)\, cube complex and let p:X𝒞Xp:X\rightarrow\mathcal{C}X be the projection defined in the previous paragraph. If bb intersects a sequence of strongly separated hyperplanes, h1,h2,,hnh_{1},h_{2},...,h_{n} then the diameter of the projection of bb in the contact graph 𝒞X\mathcal{C}X is at least n1n-1.

Proof.

Reindexing the hih_{i} if necessary, we may assume that the hyperplanes intersect the geodesic bb in the same order as their indexing numbers.

For the sake of contradiction assume that the diameter of the projection of bb in 𝒞X\mathcal{C}X is less than n1n-1. In particular, since h1h_{1} and hnh_{n} are in the projection, we know that the distance between h1h_{1} and hnh_{n} is less than n1n-1. Let v1=h1,v2,,vk1,vk=hnv_{1}=h_{1},v_{2},...,v_{k-1},v_{k}=h_{n} be a sequence of vertices in 𝒞X\mathcal{C}X which forms an edge path geodesic from h1h_{1} to hnh_{n}. The assumption tells us the edge path is no longer than n1n-1 i.e. that k1<n1k-1<n-1, or in other words that k<nk<n.

Since the sequence of vjv_{j} forms a geodesic in 𝒞X\mathcal{C}X we know that for each jj the hyperplane carrier of vjv_{j} intersects the hyperplane carrier of vj+1v_{j+1}. Thus, in the space XX, there is a continuous path from the intersection point bh1b\cap h_{1} to bhnb\cap h_{n} which is the concatination of line segments contained inside a hyperplane carrier of vjv_{j} for some jj. Lets call this continuous path cc.

Note that h1h_{1} and hnh_{n} intersect cc (at the starting point and ending point respectively). Also notice that the sequence of planes h1,,hnh_{1},...,h_{n} cannot contain any facing triples since they all intersect the same geodesic (see the discussion after Definition 4.7). Thus for each hih_{i} with 1<i<n1<i<n, hih_{i} separates h1h_{1} from hnh_{n} and since cc is continuous, this means that hih_{i} must intersect cc.

Since for any ii, hih_{i} intersects cc there must be a jj where hih_{i} meets the hyperplane carrier of vjv_{j}. Notice that a hyperplane meets another hyperplane’s carrier if and only if both hyperplanes intersect some cube, but all hyperplanes in a given cube must intersect one another, and so for each 1in1\leq i\leq n, hih_{i} intersects at least one of the vjv_{j}. Since k<nk<n there is a 1jk1\leq j\leq k and 1iln1\leq i\neq l\leq n so that vjv_{j} intersects both hih_{i} and hlh_{l}.

However since the hih_{i} are all strongly separated no vjv_{j} intersects more than one of the hih_{i}. This gives us the needed contradiction and so the diameter of the projection of bb is at least n1n-1. ∎

Now we can prove Corollary C from the introduction in the case where XX is the Salvetti complex of a right-angled Artin group:

Proposition 4.20.

Let Γ\Gamma be a graph, AΓ,𝒮Γ~A_{\Gamma},\tilde{\mathcal{S}_{\Gamma}} be the corresponding right-angled Artin group and Salvetti complex respectively. Every κ\kappa-contracting geodesic makes a definite progress in the contact graph. More precisely, if bb is a κ\kappa-contracting geodesic ray and p:𝒮Γ~𝒞𝒮Γ~p:\tilde{\mathcal{S}_{\Gamma}}\rightarrow\mathcal{C}\tilde{\mathcal{S}_{\Gamma}} is the projection map, then there exists a constant 𝖽{\sf d} such that for any t,t, we have d(p(𝔬),p(b(t))t𝖽κ(t)2.d(p({\mathfrak{o}}),p(b(t))\geq\frac{t}{{\sf d}\kappa(t)}-2.

Proof.

The idea of the proof is that among all hyperplanes crossed by a geodesic ray bb, only strongly separated hyperplanes will contribute to distance in the contact graph. For any given t>0t>0, the number of such hyperplanes is asymptotically tκ(t)\frac{t}{\kappa(t)}.

Since bb is κ\kappa-contracting with constant, using Corollary 4.17, there exists 𝖼{\sf c}, and an infinite sequence of hyperplanes

h1,h2,,hi,h_{1},h_{2},\dots,h_{i},\dots

at points b(ti)b(t_{i}) such that hi,hi+1h_{i},h_{i+1} are strongly separated and

d(b(ti),b(ti+1))𝖼κ(ti+1).d(b(t_{i}),b(t_{i+1}))\leq{\sf c}\kappa(t_{i+1}).

Since each hi,hi+1h_{i},h_{i+1} are strongly separated, every hih_{i} is strongly separated from hjh_{j} by Theorem 2.5 in [BC11]. For each tt\in\mathbb{R}, there exists ii such that b(t)b(t) is between b(ti1)b(t_{i-1}) and b(ti)b(t_{i}). Thus

d(𝔬,b(t))\displaystyle d({\mathfrak{o}},b(t)) d(𝔬,b(t1))+d(b(t1),b(t2))++d(b(ti1),b(ti))\displaystyle\leq d({\mathfrak{o}},b(t_{1}))+d(b(t_{1}),b(t_{2}))+...+d(b(t_{i-1}),b(t_{i}))
𝖼κ(t1)+𝖼κ(t2)++𝖼κ(ti)\displaystyle\leq{\sf c}\kappa(t_{1})+{\sf c}\kappa(t_{2})+...+{\sf c}\kappa(t_{i})
𝖼κ(ti)+𝖼κ(ti)+𝖼κ(ti)(κ is monotone nondecreasing)\displaystyle\leq{\sf c}\kappa(t_{i})+{\sf c}\kappa(t_{i})...+{\sf c}\kappa(t_{i})\qquad\text{($\kappa$ is monotone nondecreasing)}
=i𝖼κ(ti).\displaystyle=i{\sf c}\kappa(t_{i}).

This implies that id(𝔬,b(t))𝖼κ(ti)i\geq\frac{d({\mathfrak{o}},b(t))}{{\sf c}\kappa(t_{i})}, where ti1tti.t_{i-1}\leq t\leq t_{i}. Applying Lemma 4.19 to the geodesic bb and the hyperplanes h1,h2,..,hih_{1},h_{2},..,h_{i} we get that d(p(𝔬),p(b(t)))i2d(p({\mathfrak{o}}),p(b(t)))\geq i-2. Using Proposition 2.8 there exists a constant 𝖽{\sf d}^{\prime} such that κ(ti)𝖽κ(t)\kappa(t_{i})\leq{\sf d}^{\prime}\kappa(t). Using the above, we get that

d(p(𝔬),p(b(t)))i2d(𝔬,b(t))𝖼κ(ti)2=t𝖼κ(ti)2t𝖼𝖽κ(t)2.d(p({\mathfrak{o}}),p(b(t)))\geq i-2\geq\frac{d({\mathfrak{o}},b(t))}{{\sf c}\kappa(t_{i})}-2=\frac{t}{{\sf c}\kappa(t_{i})}-2\geq\frac{t}{{\sf c}{\sf d}^{\prime}\kappa(t)}-2.

4.5. Bounding the well-separating constant in a factored CAT(0) cube complex

Lastly, we prove that if a CAT(0) cube complex is equipped with a factor system, then there is a uniform bound to the well-separation constant. Factor systems were introduced by [BHS17]. The Salvetti complexes are the main examples of CAT(0) cube complexes with a factor system, which we define now:

Definition 4.21 (Parallel subcomplexes).

Let XX be a finite dimensional CAT(0) cube complex. Two convex subcomplexes H1,H2H_{1},H_{2} are said to be parallel if for any hyperplane h,h, we have hH1h\cap H_{1}\neq\emptyset if and only if hH2h\cap H_{2}\neq\emptyset.

Definition 4.22 (Factor systems [BHS17]).

Let XX be a finite dimensional CAT(0) cube complex. A factor system, denoted 𝔉\mathfrak{F}, is a collection of subcomplexes of XX such that:

  1. (1)

    X𝔉X\in\mathfrak{F}.

  2. (2)

    Each F𝔉F\in\mathfrak{F} is a nonempty convex subcomplex of XX

  3. (3)

    There exists 𝖼11{\sf c}_{1}\geq 1 such that for all xX(0)x\in X^{(0)} at most 𝖼1{\sf c}_{1} elements of 𝔉\mathfrak{F} contains x.x.

  4. (4)

    Every nontrivial convex subcomplex paralell to a combinatorial hyperplane of XX is in 𝔉\mathfrak{F}.

  5. (5)

    There exists 𝖼2{\sf c}_{2} such that for all F,F𝔉F,F^{\prime}\in\mathfrak{F}, either 𝔤F(F)𝔉\mathfrak{g}_{F}(F^{\prime})\in\mathfrak{F} or

    diam(𝔤F(F))𝖼2\text{diam}(\mathfrak{g}_{F}(F^{\prime}))\leq{\sf c}_{2}

    .

We also use the following generalization of contact graph introduced in [Gen20b]:

Definition 4.23 (The well-separation space).

Let XX be a finite dimensional CAT(0) cube complex. For each integer kk, the kk-well-separation space, denoted by YkY_{k} is defined to be the set whose elements are the vertices of XX, with the following distance function. For x,yX(0)x,y\in X^{(0)}, the kk-distance between x,yx,y denoted by dk(x,y)d_{k}(x,y) is defined to be the cardinality of the maximal collection of kk-well-separated hyperplanes separating x,yx,y.

It was shown in [Gen20b] that for any CAT(0) cube complex XX, the kk-well-separation space (Yk,dk)(Y_{k},d_{k}) is hyperbolic.

Proposition 4.24 ([Gen20b, Proposition 6.53]).

Let XX be a finite dimensional CAT(0) cube complex and let YkY_{k} be the kk-well-separation space as in Definition 4.23. For any non-negative integer kk, the metric space (Yk,dk)(Y_{k},d_{k}) is 9(k+2)9(k+2) hyperbolic.

Proposition 4.25 ([Gen20b, Proposition 2.2]).

Let XX be a CAT(0) cube complex and let A,BXA,B\subseteq X be two convex subcomplexes. The hyperplanes intersecting 𝔤B(A)\mathfrak{g}_{B}(A) are precisely those which intersect both AA and B.B.

The proof of the following lemma is exactly the same as that of Lemma 6.53 in the first arXiv version of [Gen17]. However as the Genevois noted, it is only suitable under the assumption that XX is a cocompact CAT(0) cube complex with a factor system. For completeness, we present it here.

Lemma 4.26.

Let X be a cocompact CAT(0) cube complex with a factor system. There exists a constant L0L\geq 0 such that any two hyperplanes of XX either are LL-well-separated or are not well-separated.

Proof.

Let GG be the group acting cocompactly on XX. Suppose for the sake of contradiction that there exists an increasing sequence of integers (rir_{i}) and a sequence of pairs of hyperplanes (hi,ui)(h_{i},u_{i}) such that, for every i1i\geq 1, the hyperplanes hih_{i} and uiu_{i} are rir_{i}-well-separated but not (ri1)(r_{i}-1)-well-separated. Since XX is cocompact, up to passing to a subsequence of hi,h_{i}, there exists a hyperplane hh such that hi=gihh_{i}=g_{i}h, for giStab(h).g_{i}\in Stab(h). Applying gi1g^{-1}_{i} to the sequence of pairs (hi,ui)(h_{i},u_{i}), we obtain that the sequence of pairs (h,gi1ui)(h,g^{-1}_{i}u_{i}) must also be rir_{i}-well-separated but not (ri1)(r_{i}-1)-well-separated. We will denote the hyperplanes gi1uig^{-1}_{i}u_{i} by viv_{i}. Now, let xi𝔤h(vi)x_{i}\in\mathfrak{g}_{h}(v_{i}). Since the stabiliser Stab(h)Isom(X)Stab(h)\subset Isom(X) acts cocompactly on the carrier N(h)N(h), there exists a combinatorial ball of a finite radius in hh, call it BB, and infinitely many giGg^{\prime}_{i}\in G such that gixiBg^{\prime}_{i}x_{i}\in B. As BB contains only finitely many vertices, up to passing to a subsequence, we have gixi=xg^{\prime}_{i}x_{i}=x for some xB.x\in B. Thus, the hyperplanes (h,givi)(h,g^{\prime}_{i}v_{i}) are also rir_{i}-well-separated but not (ri1)(r_{i}-1)-well-separated. We will denote the hyperplanes givig^{\prime}_{i}v_{i} by wiw_{i}. Thus, 𝔤h(wi)\mathfrak{g}_{h}(w_{i}) contains xx for every i1i\geq 1. Since the hyperplanes (h,wi)(h,w_{i}) are rir_{i}-well-separated but not (ri1)(r_{i}-1)-well-separated, we deduce from Proposition 4.25 that the maximal cardinality of hyperplanes intersecting 𝔤h(wi)\mathfrak{g}_{h}(w_{i}) but not containing facing triple is precisely rir_{i}. Since rir_{i} is strictly increasing, we have 𝔤h(wi)𝔤h(wj)\mathfrak{g}_{h}(w_{i})\neq\mathfrak{g}_{h}(w_{j}) for all iji\neq j. On the other hand, since XX is a CAT(0) cube complex with a factor system FSFS, using condition 3 of Definition 4.22 there exists a constant 𝖼{\sf c} such that at most 𝖼{\sf c} elements of 𝔤h(wi)\mathfrak{g}_{h}(w_{i}) are contained in FSFS. Therefore, condition 5 of Definition 4.22 implies that there exists a constant 𝖼{\sf c}^{\prime} such that for infinitely many i,i, we have diam(𝔤h(wi))𝖼(\mathfrak{g}_{h}(w_{i}))\leq{\sf c}^{\prime}, which is a contradiction.

Therefore, in light of Lemma 4.26, we have the following.

Corollary 4.27.

Let XX be a finite dimensional cocompact CAT(0) cube complex with a factor system. There exists a constant kk such that a geodesic ray bXb\in X is κ\kappa-contracting if and only if there exists a constant 𝖼{\sf c} such that bb crosses an infinite sequence of hyperplanes h1,h2,h_{1},h_{2},... at points b(ti)b(t_{i}) satisfying:

  1. (1)

    d(ti,ti+1)𝖼κ(ti+1).d(t_{i},t_{i+1})\leq{\sf c}\kappa(t_{i+1}).

  2. (2)

    hi,hi+1h_{i},h_{i+1} are kk-well-separated.

Proof.

This is immediate by applying Lemma 4.26 to Theorem 4.1. ∎

As an application of Corollary 4.27, we show that for any CAT(0) cube complex with a factor system, κ\kappa-contracting geodesic rays project to subsets of infinite diameter in the well-separation space. In order to make this precise, we define a projection map p:XYkp:X\rightarrow Y_{k} as in the following remark.

Remark 4.28.

For each xX,x\in X, let nn be the largest integer so that x[0,1]nx\in[0,1]^{n}. We define q(x)q(x) to be a 0-cell (a vertex) of the cube [0,1]n[0,1]^{n}. Also, remark that since XX is a finite dimensional cube complex, there exists a constant 𝖽{\sf d} depending only on the dimension of XX such that for any x,yXx,y\in X, if lk(x,y)l_{k}(x,y) is the cardinality of the maximal collection of kk-well-separated hyperplanes separating x,yx,y, then we have:

dk(q(x),q(y))𝖽lk(x,y)dk(q(x),q(y))+𝖽.d_{k}(q(x),q(y))-{\sf d}\leq l_{k}(x,y)\leq d_{k}(q(x),q(y))+{\sf d}.

Now, we prove Corollary C from the introduction.

Corollary 4.29.

Let XX be a finite dimensional cocompact CAT(0) cube complex with a factor system. There exists constants 𝖽1,𝖽2{\sf d}_{1},{\sf d}_{2} and an integer kk such that for any κ\kappa-contracting geodesic ray bb with q(b(0))=𝔬,q(b(0))={\mathfrak{o}}, the projection map q:XYkq:X\rightarrow Y_{k} satisfies

dk(q(𝔬)),q(b(t)))t𝖽1κ(t)𝖽2.d_{k}(q({\mathfrak{o}})),q(b(t)))\geq\frac{t}{{\sf d}_{1}\kappa(t)}-{\sf d}_{2}.
Proof.

Let bb be some κ\kappa-contracting geodesic ray. By Corollary 4.27, there exists an integer 𝖼{\sf c} such that bb crosses an infinite sequence of hyperplanes hih_{i} at points tit_{i} satisfying d(ti,ti+1)𝖼κ(ti+1)d(t_{i},t_{i+1})\leq{\sf c}\kappa(t_{i+1}) such that hi,hi+1h_{i},h_{i+1} are 𝖼{\sf c}-well-separated. Notice that for each ii, since hihi+1=hi+1hi+2=h_{i}\cap h_{i+1}=h_{i+1}\cap h_{i+2}=\emptyset, the hyperplane hih_{i} separates hi1h_{i-1} from hi+1h_{i+1}. Thus, every hyperplane intersecting both hi,hi+2h_{i},h_{i+2} must also intersect hi,hi+1h_{i},h_{i+1}. Therefore, hi,hi+2h_{i},h_{i+2} are also 𝖼{\sf c}-well-separated. Indeed, by induction, this implies that for any j<k,j<k, the hyperplanes hj,hkh_{j},h_{k} are also 𝖼{\sf c}-well-separated. Now, let t>0t>0 and let ii be so that ti1tti.t_{i-1}\leq t\leq t_{i}.

d(𝔬,b(t))\displaystyle d({\mathfrak{o}},b(t)) d(𝔬,b(t1))+d(b(t1),b(t2))++d(b(ti1),b(ti))\displaystyle\leq d({\mathfrak{o}},b(t_{1}))+d(b(t_{1}),b(t_{2}))+...+d(b(t_{i-1}),b(t_{i}))
𝖼κ(t1)+𝖼κ(t2)++𝖼κ(ti)\displaystyle\leq{\sf c}\kappa(t_{1})+{\sf c}\kappa(t_{2})+...+{\sf c}\kappa(t_{i})
𝖼κ(ti)+𝖼κ(ti)+𝖼κ(ti)(κ is monotone nondecreasing)\displaystyle\leq{\sf c}\kappa(t_{i})+{\sf c}\kappa(t_{i})...+{\sf c}\kappa(t_{i})\qquad\text{($\kappa$ is monotone nondecreasing)}
=i𝖼κ(ti).\displaystyle=i{\sf c}\kappa(t_{i}).

This gives that it𝖼κ(t)i\geq\frac{t}{{\sf c}\kappa(t)} where i1i-1 is a lower bound on the number of 𝖼{\sf c}-well-separated hyperplanes separating b(0)b(0) and b(t)b(t). Let k=𝖼k={\sf c}, using Remark 4.28, there exists a constant 𝖽{\sf d} so that dk(q(b(0)),q(b(t)))i𝖽t𝖼κ(ti)𝖽tkκ(ti)𝖽.d_{k}(q(b(0)),q(b(t)))\geq i-{\sf d}\geq\frac{t}{{\sf c}\kappa(t_{i})}-{\sf d}\geq\frac{t}{k\kappa(t_{i})}-{\sf d}. Using Proposition 2.8, there exists a constant 𝖽{\sf d}^{\prime} such that κ(ti)𝖽κ(t),\kappa(t_{i})\leq{\sf d}^{\prime}\kappa(t), therefore, we have dk(q(𝔬),q(b(t)))i𝖽t𝖼κ(ti)𝖽t𝖼κ(ti)𝖽t𝖼𝖽κ(t)𝖽d_{k}(q({\mathfrak{o}}),q(b(t)))\geq i-{\sf d}\geq\frac{t}{{\sf c}\kappa(t_{i})}-{\sf d}\geq\frac{t}{{\sf c}\kappa(t_{i})}-{\sf d}\geq\frac{t}{{\sf c}{\sf d}^{\prime}\kappa(t)}-{\sf d}.

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