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vol. 26:22024210.46298/dmtcs.108372023-01-20; 2023-01-20; 2024-01-152024-01-30

Bijective proof of a conjecture on unit interval posets

Wenjie Fang LIGM, Univ Gustave Eiffel, CNRS, ESIEE Paris, Marne-la-Vallée, France
Abstract

In a recent preprint, Matherne, Morales and Selover conjectured that two different representations of unit interval posets are related by the famous zeta map in q,tq,t-Catalan combinatorics. This conjecture was proved recently by Gélinas, Segovia and Thomas using induction. In this short note, we provide a bijective proof of the same conjecture with a reformulation of the zeta map using left-aligned colored trees, first proposed in the study of parabolic Tamari lattices.

keywords:
Dyck path, zeta map, unit interval poset, plane tree

1 Introduction

The study of unit interval posets started in statistics (Wine and Freund, 1957) and psychology (Scott, 1964). However, it has since been connected to other objects in algebraic combinatorics, such as (3+1)(3+1)-free posets Skandera and Reed (2003) and positroids Chavez and Gotti (2018). The connection to (3+1)(3+1)-free posets is particularly important, as these posets are at the center of the Stanley–Stembridge conjecture in Stanley and Stembridge (1993), which states that the chromatic symmetric function of the incomparability graph of a (3+1)(3+1)-free poset has only positive coefficients when expanded in the basis of elementary symmetric functions. Unit interval posets thus receive some attention as it can be used to study the structure of (3+1)(3+1)-free posets (Skandera and Reed, 2003; Guay-Paquet, Morales, and Rowland, 2014; Lewis and Zhang, 2013).

It is known in Wine and Freund (1957) that unit interval posets are counted by Catalan numbers, and researchers have given two different bijections to represent a unit interval poset by Dyck paths (Skandera and Reed, 2003; Guay-Paquet, Morales, and Rowland, 2014). In a recent preprint (Matherne, Morales, and Selover, ), it was conjectured that the two bijections are related by the famous zeta map in q,tq,t-Catalan combinatorics (Haglund, 2008), which was first given in (Andrews, Krattenthaler, Orsina, and Papi, 2002). In this short note, we settle this conjecture using bijections (see 4.6), in contrast to a recent inductive proof of the same conjecture by Gélinas, Segovia, and Thomas . To this end, we first introduce a bijection Ξposet\Xi_{\mathrm{poset}} between unit interval posets and plane trees. We then show that the two different known bijections from unit interval posets are conjugates of special cases of some bijections Ξsteep\Xi_{\mathrm{steep}} and Ξbounce\Xi_{\mathrm{bounce}} from Ceballos, Fang, and Mühle (2020) constructed for the study of parabolic Tamari lattices. Using the link between Ξsteep,Ξbounce\Xi_{\mathrm{steep}},\Xi_{\mathrm{bounce}} and the zeta map established in the same article, we conclude our proof.

The rest of the article is organized as follows. In Section 2 we give the basic definitions. Then we give our bijection between unit interval posets and plane trees in Section 3, along with the related bijections from Ceballos, Fang, and Mühle (2020). Finally in Section 4 we recall the two known bijections between unit interval posets and Dyck paths, and then establish their link with the bijections in Section 3, leading to a bijective proof of our main result (4.6).

Acknowledgment

We thank Adrien Segovia for bringing this conjecture to our attention. We also thank the anonymous reviewers for their detailed and helpful comments. This work is not supported by any funding with precise predefined goal, but it is supported by the publicly funded laboratory LIGM of Université Gustave Eiffel.

2 Preliminary

For convenience, we write [n][n] for the set {1,2,,n}\{1,2,\ldots,n\}. We consider finite partially order sets (or poset for short) of the form P=(Pelem,)P=(P_{\mathrm{elem}},\preceq), where PelemP_{\mathrm{elem}} is a finite set and \preceq a partial order on PelemP_{\mathrm{elem}}. Given a set SS of real numbers x1<x2<<xnx_{1}<x_{2}<\cdots<x_{n}, we define a partial order S\preceq_{S} on [n][n] by taking iSji\preceq_{S}j if and only if xi+1<xjx_{i}+1<x_{j}. The order S\preceq_{S} can also be seen as defined on intervals of unit length starting at the xix_{i}’s, where iSji\preceq_{S}j if the interval starting with xix_{i} is on the left of that with xjx_{j} without overlap. A poset PP with nn elements is a unit interval order if there is some SS\subset\mathbb{R} with nn elements such P([n],S)P\cong([n],\preceq_{S}). In this case, we call SS a starting set of PP. We sometimes represent unit interval orders as ([n],S)([n],\preceq_{S}) for some SS hereinafter.

We have the following characterization of unit interval orders.

Theorem 2.1 (Scott (1964, Theorem 2.1)).

A poset PP is a unit interval poset if and only if it is (3+1)(3+1)-free and (2+2)(2+2)-free, that is, the order induced on any four elements cannot be a chain of 33 elements plus an incomparable element, or two disjoint chains each containing 22 elements.

Unit interval orders are counted by Catalan numbers.

Proposition 2.2 (Wine and Freund (1957)).

The number of unit interval posets with nn elements is the nn-th Catalan number Catn=12n+1(2n+1n)\mathrm{Cat}_{n}=\frac{1}{2n+1}\binom{2n+1}{n}.

By definition, we may represent a unit interval poset PP by a set of real numbers SS, though the choice of SS is clearly not unique. In the following, for convenience, we use this perspective of (starting points of) intervals, which is arguably easier to manipulate. We denote by 𝒫n\mathcal{P}_{n} the set of unit interval posets with nn elements.

There are many other families of combinatorial objects counted by Catalan numbers, such as Dyck paths and plane trees. A Dyck path is a lattice path formed by north steps =(0,1)\uparrow\;=(0,1) and east steps =(1,0)\rightarrow\;=(1,0), starting at (0,0)(0,0) and ending on the diagonal y=xy=x while staying weakly above it. The size of a Dyck path is the number of its north steps. We denote by 𝒟n\mathcal{D}_{n} the set of Dyck paths of size nn. We define plane trees recursively: a plane tree TT is either a single node (a leaf) or an internal node uu linked by edges to a sequence of plane trees called sub-trees. In the latter case, the node uu is also called the root of TT, and the roots of sub-trees are called children of uu. We denote by 𝒯n\mathcal{T}_{n} the set of plane trees with nn non-root nodes. We recall the well-known fact that |𝒯n|=|𝒟n|=Catn|\mathcal{T}_{n}|=|\mathcal{D}_{n}|=\mathrm{Cat}_{n}. For a node uu in a plane tree TT, its depth, denoted by d(u)d(u), is the distance (number of edges) between uu and the root of TT.

3 Unit interval posets and plane trees

We start by a new bijection between unit interval posets and plane trees.

Construction 3.1.

Let S={x1<<xn}S=\{x_{1}<\cdots<x_{n}\} be a starting set of a unit interval poset P=([n],S)P=([n],\preceq_{S}). We define a plane tree TT as follows (see Figure 1 for an example). We set x0=x12x_{0}=x_{1}-2. We denote by viv_{i} the node of TT corresponding to xix_{i}. For i[n]i\in[n], the parent of viv_{i} is vjv_{j} if and only if jj is the largest index such that jSij\preceq_{S}i. By the definition of x0x_{0}, the parent of each viv_{i} is well-defined, and all nodes are descendants of x0x_{0}. We then order children of the same node from left to right with decreasing index. We thus conclude that TT is a well-defined plane tree. We note that TT depends only on S\preceq_{S}. We define Λposet(P)=T\Lambda_{\mathrm{poset}}(P)=T.

Refer to caption
Figure 1: Example of Λposet\Lambda_{\mathrm{poset}} from a unit interval poset defined by a set of unit intervals to a plane tree
Construction 3.2.

Given a plane tree TT with nn non-root nodes, we define an order relation S\preceq_{S} on [n][n] induced by some SS\subset\mathbb{R}. Let rTr_{T} be the root of TT, and mm the maximal arity of TT, i.e., the maximal number of children of nodes in TT. Given a node uu in TT, if it is the ii-th child of its parent from right to left, then we define c(u)=ic(u)=i. We observe that 1c(u)m1\leq c(u)\leq m. For a non-root node uu in TT, let u0=rT,u1,,ud(u)=uu_{0}=r_{T},u_{1},\ldots,u_{d(u)}=u be the nodes on the unique path from the root u0=rTu_{0}=r_{T} to ud(u)=uu_{d(u)}=u, where d(u)d(u) is the depth of uu. We then define a real number xux_{u} associated to uu using base (m+2)(m+2):

xu=d(u)+(0.c(u1)c(u2)c(ud(u)))(m+2)=+i=1d(u)c(ui)(m+2)i.x_{u}=d(u)+(0.c(u_{1})c(u_{2})\cdots c(u_{d(u)}))_{(m+2)}=\ell+\sum_{i=1}^{d(u)}c(u_{i})(m+2)^{-i}. (1)

It is clear from (1) that xux_{u} is strictly decreasing from left to right for nodes of the same depth in TT. Let SS be the set of xux_{u} for non-root nodes uu in TT. We define Ξposet(T)=([n],S)\Xi_{\mathrm{poset}}(T)=([n],\preceq_{S}).

As an example of 3.2, let TT be the tree on the right part of Figure 1, with nodes labeled as in the figure, and SS the set of numbers in the construction. The maximal arity of TT is m=4m=4, achieved by the root. The number xv12Sx_{v_{12}}\in S for the node v12v_{12} is thus xv12=3+(0.321)6=769/216x_{v_{12}}=3+(0.321)_{6}=769/216, as v12v_{12} is of depth 33, and it is the first child from right to left of its parent v8v_{8}, itself the second child from right to left of its parent v3v_{3}, which is the third child from right to left of the root.

The following lemma gives a direct connection between a plane tree and its corresponding unit interval poset obtained from Ξposet\Xi_{\mathrm{poset}}.

Lemma 3.3.

For T𝒯nT\in\mathcal{T}_{n}, we take SS to be the set constructed in 3.2, and xux_{u} the number constructed from a non-root node uu of TT. Then for non-root nodes u,vu,v, the parent of uu in TT is vv if and only if xvx_{v} is the largest element in SS smaller than 1+xu1+x_{u}.

Proof.

Suppose that TT has maximal arity mm. Let vv^{\prime} be the parent of uu. By (1), we have 1<xuxv<1+(m+2)+11<x_{u}-x_{v^{\prime}}<1+(m+2)^{-\ell+1}, with \ell the distance from vv^{\prime} to the root. Then, xvx_{v} satisfying xvxv<1+xux_{v^{\prime}}\leq x_{v}<1+x_{u} means 0xvxv<(m+2)+10\leq x_{v}-x_{v^{\prime}}<(m+2)^{-\ell+1}, which means v=vv=v^{\prime} by (1), as it requires vv and vv^{\prime} to have the same distance to the root, but in this case |xvxv||x_{v}-x_{v^{\prime}}| cannot be smaller than (m+2)+1(m+2)^{-\ell+1} if vvv\neq v^{\prime}. We thus have the equivalence. ∎

We now show that Λposet\Lambda_{\mathrm{poset}} and Ξposet\Xi_{\mathrm{poset}} are bijections and are inverse to each other.

Proposition 3.4.

For all n1n\geq 1, the map Λposet\Lambda_{\mathrm{poset}} is a bijection from 𝒫n\mathcal{P}_{n} to 𝒯n\mathcal{T}_{n}, with Ξposet\Xi_{\mathrm{poset}} its inverse.

Proof.

By 2.2, we have |𝒫n|=Catn=|𝒯n||\mathcal{P}_{n}|=\mathrm{Cat}_{n}=|\mathcal{T}_{n}|. We thus only need to show that ΛposetΞposet=id\Lambda_{\mathrm{poset}}\circ\Xi_{\mathrm{poset}}=\operatorname{id}. Given a plane tree T𝒯nT\in\mathcal{T}_{n}, let P=([n],S)=Ξposet(T)P=([n],\preceq_{S})=\Xi_{\mathrm{poset}}(T) and T=Λposet(P)T^{\prime}=\Lambda_{\mathrm{poset}}(P). Let S={x1<<xn}S=\{x_{1}<\cdots<x_{n}\} be the set of real numbers constructed in 3.2 for S\preceq_{S}. Given i[n]i\in[n], let uiu_{i} be the node in TT that gives rise to xix_{i} in SS, and uiu^{\prime}_{i} the node in TT^{\prime} that represents xix_{i}. By 3.3 and 3.1, for any i,j[n]i,j\in[n], the node uiu_{i} is the parent of uju_{j} in TT if and only if uiu^{\prime}_{i} is the parent of uju^{\prime}_{j} in TT^{\prime}. Then, TT^{\prime} has the same order of siblings as TT, as in both we order siblings with decreasing order in their corresponding real numbers in SS. We thus conclude that T=TT=T^{\prime}. ∎

We now restate two previously known bijections between plane trees and Dyck paths that will be used to prove our main result.

Construction 3.5.

Let n1n\geq 1 and T𝒯nT\in\mathcal{T}_{n}, we construct a Dyck path DD by taking the clockwise contour walk starting from the top of the root of TT (see the Dyck path on the right of Figure 2). During the walk, when we pass an edge for the first (resp. second) time, we append \uparrow (resp. \rightarrow) to DD. We define Ξsteep(T)=D\Xi_{\mathrm{steep}}(T)=D. The map Ξsteep\Xi_{\mathrm{steep}} is a bijection from 𝒯n\mathcal{T}_{n} to 𝒟n\mathcal{D}_{n} for all n1n\geq 1, and we denote its inverse by Λsteep\Lambda_{\mathrm{steep}}.

Construction 3.6.

Let n1n\geq 1 and T𝒯nT\in\mathcal{T}_{n}, we construct a Dyck path DD by appointing the number of north steps at each xx-coordinate (see the Dyck path on the left of Figure 2). Let α\alpha_{\ell} be the number of nodes of depth \ell (thus distance \ell to the root), and max\ell_{\max} the maximal depth of nodes in TT. We take s=α1++αs_{\ell}=\alpha_{1}+\cdots+\alpha_{\ell}. Given 1kn11\leq k\leq n-1, there is a unique way to write k=srk=s_{\ell}-r with 0r<α0\leq r<\alpha_{\ell} and 1max1\leq\ell\leq\ell_{\max}. In this case, the number of north steps in DD on x=kx=k is the number of children of the (r+1)(r+1)-st node of depth \ell. The number of north steps in DD on x=0x=0 is the number of children of the root. We define Ξbounce(T)=D\Xi_{\mathrm{bounce}}(T)=D. The map Ξbounce\Xi_{\mathrm{bounce}} is a bijection from 𝒯n\mathcal{T}_{n} to 𝒟n\mathcal{D}_{n} for all n1n\geq 1, see Ceballos, Fang, and Mühle (2020, Lemma 3.18), and we denote its inverse by Λbounce=Ξbounce1\Lambda_{\mathrm{bounce}}=\Xi_{\mathrm{bounce}}^{-1}.

Proposition 3.7 (Ceballos, Fang, and Mühle (2020, Theorem IV)).

Let ζ\zeta be the zeta map from 𝒟n\mathcal{D}_{n} to 𝒟n\mathcal{D}_{n} with n1n\geq 1. We have ζ=ΞbounceΛsteep\zeta=\Xi_{\mathrm{bounce}}\circ\Lambda_{\mathrm{steep}}.

See Figure 2 for an illustration of 3.7. Here, we do not give the original definition of the zeta map ζ\zeta in Andrews, Krattenthaler, Orsina, and Papi (2002), and will instead be using 3.7 in the following, as it is better suited to our approach.

Refer to caption
Figure 2: The zeta map as composition of bijections mediated by trees. The nodes of the same depth of the tree are grouped together. For the Dyck path on the left, the number of north steps on x=kx=k is the number of children of the kk-th node in the tree, ordered by increasing depth, then from right to left. The one on the right comes from a clockwise contour walk.
Remark 3.8.

Albeit the same notation, the maps Ξsteep\Xi_{\mathrm{steep}} and Ξbounce\Xi_{\mathrm{bounce}} are only special cases of the ones from Ceballos, Fang, and Mühle (2020, Construction 3.10 and Equation 14). More precisely, the central objects of Ceballos, Fang, and Mühle (2020) are called LAC trees, which are plane trees with non-root nodes divided into regions algorithmically. We are only using the special case where the region dd consists of nodes of depth dd, which is also the one used in Ceballos, Fang, and Mühle (2020, Section 3.3) to prove 3.7. In full generality, the map Ξsteep\Xi_{\mathrm{steep}} maps a LAC tree to a steep pair, which is a pair of nested Dyck paths with a steep upper path, i.e.,without two consecutive east steps except on the maximal height. The map Ξbounce\Xi_{\mathrm{bounce}} sends a LAC tree to a bounce pair, which is a pair of nested Dyck path with a bounce lower path, i.e., a concatenation of sub-paths of the form kk\uparrow^{k}\rightarrow^{k} for all kk. This explains the words “steep” and “bounce” in their notation.

Remark 3.9.

The bijection Ξsteep\Xi_{\mathrm{steep}} is classical, except that we do the contour walk from right to left instead of from left to right. The bijection Ξbounce\Xi_{\mathrm{bounce}} is quite close to the classical bijection between plane trees and Łukasiewicz words, as given in Flajolet and Sedgewick (2009, Section I.5.3)), which can be seen as sequences (z0,z1,,zn1)(z_{0},z_{1},\ldots,z_{n-1}) with zi1z_{i}\geq-1 such that i=0kzi0\sum_{i=0}^{k}z_{i}\geq 0 for 0k<n10\leq k<n-1, and the sum of all ziz_{i}’s is 1-1. However, in the classical bijection of Łukasiewicz, we deal with nodes in a depth-first order, but in Ξbounce\Xi_{\mathrm{bounce}} they are processed in a breadth-first order.

4 Unit interval posets and the zeta map

In the following, we give the two representations of unit interval posets as Dyck paths, and we detail how they are related to the bijections detailed in Section 3, leading to a proof of our main result (4.6).

We start by the first representation, which was first defined implicitly using anti-adjacency matrices of unit interval posets in Skandera and Reed (2003), only involving the poset structure. The following form was first given in Chavez and Gotti (2018).

Construction 4.1.

Given P=([n],S)P=([n],\preceq_{S}) a unit interval poset with SS\subset\mathbb{R}, we define a Dyck path DD as follows. Let S+={x+1xS}S^{+}=\{x+1\mid x\in S\}. Without loss of generality, we can choose SS such that SS+=S\cap S^{+}=\varnothing. Then suppose that SS+={y1<<y2n}S\cup S^{+}=\{y_{1}<\cdots<y_{2n}\}. For i[2n]i\in[2n], the ii-th step of DD is \uparrow if yiSy_{i}\in S, and is \rightarrow otherwise. We define φ(P)=D\varphi(P)=D. See Figure 3 for an example.

This form of the map φ\varphi in 4.1 was given in Chavez and Gotti (2018, Section 5) and proved in Lemma 5.7 therein to be equivalent to the original definition, which is the one used in Matherne, Morales, and Selover (, Section 2.3). Although defined here using the set SS, the map φ\varphi does not depend on the choice of SS.

Refer to caption
Figure 3: Example of the bijections φ\varphi and ψ\psi
Proposition 4.2.

We have φΞposet=Ξbounce\varphi\circ\Xi_{\mathrm{poset}}=\Xi_{\mathrm{bounce}}, and φ\varphi is a bijection from 𝒫n\mathcal{P}_{n} to 𝒟n\mathcal{D}_{n} for all n1n\geq 1.

Proof.

Let T𝒯nT\in\mathcal{T}_{n} and D=Ξbounce(T)D=\Xi_{\mathrm{bounce}}(T). We take P=Ξposet(T)=([n],S)𝒫nP=\Xi_{\mathrm{poset}}(T)=([n],\preceq_{S})\in\mathcal{P}_{n} with S={x1<<xn}S=\{x_{1}<\cdots<x_{n}\} given in 3.2. Let D=φ(P)D^{\prime}=\varphi(P). To show that D=DD^{\prime}=D, we first notice that a Dyck path is determined by the number of north steps on each line x=kx=k for 0kn10\leq k\leq n-1. Thus, we only need to show that for each kk, DD^{\prime} has the same number of north steps on x=kx=k as DD has according to 3.6.

For the line x=0x=0, we observe that the number of elements in SS strictly smaller than x1+1x_{1}+1 must be those with integer part equal to 11, thus those from the children of the root of TT. For 1kn11\leq k\leq n-1, from 4.1, we know that the number of north steps on the line x=kx=k is the number of elements xix_{i} such that xk1+1<xi<xk+1x_{k-1}+1<x_{i}<x_{k}+1, as xk+1x_{k}+1 corresponds to the kk-th east step in DD. Let uku_{k} be the node in TT corresponding to xkx_{k}. By 3.3, the nodes in TT corresponding to such xix_{i} are children of uku_{k}, meaning that the total number of north steps on x=kx=k is the number of children of uku_{k}. Furthermore, suppose that uku_{k} is of depth \ell, then we can write k=srk=s_{\ell}-r with 0r<α0\leq r<\alpha_{\ell} as in 3.6. We know that uku_{k} is the (r+1)(r+1)-st node of depth \ell in TT, as in 3.1 the values corresponding to nodes of the same depth are decreasing from left to right. We thus conclude that D=DD=D^{\prime}, and φΞposet=Ξbounce\varphi\circ\Xi_{\mathrm{poset}}=\Xi_{\mathrm{bounce}}. As both Ξbounce\Xi_{\mathrm{bounce}} (Ceballos, Fang, and Mühle, 2020, Lemma 3.18) and Ξposet\Xi_{\mathrm{poset}} (3.4) are bijections, we conclude that φ\varphi is also a bijection. ∎

The second presentation was first defined in Guay-Paquet, Morales, and Rowland (2014) for (3+1)(3+1)-free posets, and it takes a simpler form for unit interval posets. A more explicit presentation is given in Guay-Paquet (2013, Section 2).

Construction 4.3.

For n1n\geq 1, let D𝒟nD\in\mathcal{D}_{n} be a Dyck path of size nn. Its area vector, denoted by Area(D)\operatorname{Area}(D), is a vector (a1,,an)(a_{1},\ldots,a_{n}) with aia_{i} the number of full unit squares with the upper edge on y=iy=i between DD and the diagonal y=xy=x. Such area vectors are characterized by the conditions a1=0a_{1}=0 and aiai1+1a_{i}\leq a_{i-1}+1 for 2in2\leq i\leq n. It is clear that the area vector determines the Dyck path. We then define a poset P=([n],)P=([n],\preceq) by taking iji\prec j for i,j[n]i,j\in[n] such that

  • Either ai+2aja_{i}+2\leq a_{j};

  • Or ai+1=aja_{i}+1=a_{j} and i<ji<j.

We define ψ(D)=P\psi(D)=P, and its inverse ψ1(P)=D\psi^{-1}(P)=D. See Figure 3 for an example.

The following result ensures that ψ\psi is well-defined. It is a special case of Matherne, Morales, and Selover (, Theorem 5.2), which is obtained by combining Guay-Paquet, Morales, and Rowland (2014, Remark 3.2, Proposition 3.11). A self-contained direct proof of this special case can be found in Gélinas, Segovia, and Thomas (, Section 6).

Proposition 4.4 (Special case of Matherne, Morales, and Selover (, Theorem 5.2)).

The map ψ\psi is a bijection from Dyck paths to unit interval posets preserving sizes.

Proposition 4.5.

We have ψ=ΞposetΛsteep\psi=\Xi_{\mathrm{poset}}\circ\Lambda_{\mathrm{steep}}.

Proof.

Let P=ψ(D)P=\psi(D), T=Λsteep(D)T=\Lambda_{\mathrm{steep}}(D) and P=Ξposet(D)P^{\prime}=\Xi_{\mathrm{poset}}(D). We write P=([n],)P=([n],\preceq) and P=([n],S)P^{\prime}=([n],\preceq_{S}), with SS given in 3.2. We show that PP is isomorphic to PP^{\prime} after an implicit relabeling.

For i[n]i\in[n], let uiu_{i} be the ii-th non-root node in TT that is visited in the clockwise contour walk of TT. We note that this order on nodes of TT is different from the one used before, for instance in 3.1. Suppose that Area(D)=(a1,,an)\operatorname{Area}(D)=(a_{1},\ldots,a_{n}). By 3.5, the depth of uiu_{i} is ai+1a_{i}+1. We now define a partial order T\preceq_{T} on non-root nodes in TT by taking uiTuju_{i}\preceq_{T}u_{j} if and only if iji\preceq j in PP. We recall that the depth of vv in TT is denoted by d(v)d(v). By 4.3, two non-root nodes v,wv,w in TT satisfy vTwv\prec_{T}w if and only if

  • Either d(v)+2d(w)d(v)+2\leq d(w);

  • Or d(v)+1=d(w)d(v)+1=d(w), and the parent of ww is either vv or on the left of vv.

Now, for vv a non-root node in TT, we take xvx_{v} defined in (1). Suppose that there are two non-root nodes v,wv,w of TT such that xv+1<xwx_{v}+1<x_{w}. Then we have d(v)+1d(w)d(v)+1\leq d(w). There are two possibilities: either d(v)+1=d(w)d(v)+1=d(w), or d(v)+2d(w)d(v)+2\leq d(w). In the first case, let ww^{\prime} be the parent of ww, we have xw+1<xwx_{w^{\prime}}+1<x_{w}. By 3.3, we know that xvxwx_{v}\leq x_{w^{\prime}}. From (1), we know that either v=wv=w^{\prime} or vv is on the right of ww^{\prime}, as xvx_{v} is decreasing from left to right for nodes in TT of the same depth. Combining with the second case, we conclude that xv+1<xwx_{v}+1<x_{w} if and only if vTwv\prec_{T}w. By 3.2, we have PPP\cong P^{\prime}, which concludes the proof. ∎

Theorem 4.6 (Matherne, Morales, and Selover (, Conjecture 7.1)).

We have φψ=ζ\varphi\circ\psi=\zeta.

Proof.

Combining 4.2 and 4.5, we have φψ=ΞbounceΛsteep\varphi\circ\psi=\Xi_{\mathrm{bounce}}\circ\Lambda_{\mathrm{steep}}, and we conclude by 3.7. ∎

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