Introduction
Double posets and E E E -partitions (for E E E a double poset) have been introduced by Claudia Malvenuto and Christophe Reutenauer [19 ] ; their goal was to construct a combinatorial Hopf algebra which harbors a noticeable amount of structure, including an analogue of the Littlewood-Richardson rule and a lift of the internal product operation of the Malvenuto-Reutenauer Hopf algebra of permutations. In this note, we shall employ these same notions to restate in a simpler form, and reprove in a more elementary fashion, a formula for the antipode in the Hopf algebra QSym of quasisymmetric functions due to (the same) Malvenuto and Reutenauer [18 Theorem 3.1] . We then further generalize this formula to a setting in which a group acts on the double poset (a generalization inspired by Katharina Jochemko’s [15 ] .
In the present version of the paper, some (classical and/or straightforward) proofs are missing or sketched. A more detailed version exists, in which at least a few of these proofs are elaborated on more1 .
A short summary of this paper has been submitted to the FPSAC conference [12 ] .
Acknowledgments
Katharina Jochemko’s work [15 ] provoked this research. I learnt a lot about QSym from Victor Reiner. The SageMath computer algebra system [23 ] was used for some computations that suggested one of the proofs.
Note on the published version of this paper
The document you are reading is the preprint of a paper (of the same title) that was published in the Electronic Journal of Combinatorics in 2017 (Volume 24, Issue 2, doi:10.37236/6660). The published version differs from this preprint insubstantially2 .
Quasisymmetric functions
Let us first briefly introduce the notations that will be used in the following.
We set N = { 0 , 1 , 2 , … } \mathbb{N} = \{0,1,2,\ldots\} N = { 0 , 1 , 2 , … } . A composition means a finite sequence of positive integers. We let Comp be the set of all compositions. For n ∈ N n \in\mathbb{N} n ∈ N , a composition of n n n means a composition whose entries sum to n n n (that is, a composition ( α 1 , α 2 , … , α k ) (\alpha_1,\alpha_2,\ldots,\alpha_k) ( α 1 , α 2 , … , α k ) satisfying α 1 + α 2 + ⋯ + α k = n \alpha_1+\alpha_2+\cdots+\alpha_k=n α 1 + α 2 + ⋯ + α k = n ).
Let k \mathbf{k} k be an arbitrary commutative ring. We shall keep k \mathbf{k} k fixed throughout this paper. We consider the k \mathbf{k} k -algebra k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[[x_1,x_2,x_3,\ldots]] k [[ x 1 , x 2 , x 3 , … ]] of formal power series in finitely many (commuting) indeterminates x 1 , x 2 , x 3 , … x_1,x_2,x_3,\ldots x 1 , x 2 , x 3 , … over k \mathbf{k} k . A monomial shall always mean a monomial (without coefficients) in the variables x 1 , x 2 , x 3 , … x_1,x_2,x_3,\ldots x 1 , x 2 , x 3 , … .3
We consider the k \mathbf{k} k -algebra k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] of (commutative) power series in countably many distinct indeterminates x 1 , x 2 , x 3 , … x_1,x_2,x_3,\ldots x 1 , x 2 , x 3 , … over k \mathbf{k} k . By abuse of notation, we shall identify every monomial x 1 a 1 x 2 a 2 x 3 a 3 ⋯ ∈ Mon x_1^{a_1}x_2^{a_2}x_3^{a_3}\cdots\in\operatorname{Mon} x 1 a 1 x 2 a 2 x 3 a 3 ⋯ ∈ Mon with the corresponding element x 1 a 1 ⋅ x 2 a 2 ⋅ x 3 a 3 ⋯ x_1^{a_1}\cdot x_2^{a_2}\cdot x_3^{a_3}\cdots x 1 a 1 ⋅ x 2 a 2 ⋅ x 3 a 3 ⋯ of k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] when necessary (e.g., when we speak of the sum of two monomials or when we multiply a monomial with an element of k \mathbf{k} k ). (To be very pedantic, this identification is slightly dangerous, because it can happen that two distinct monomials in Mon \operatorname{Mon} Mon get identified with two identical elements of k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] . However, this can only happen when the ring k \mathbf{k} k is trivial, and even then it is not a real problem unless we infer the equality of monomials from the equality of their counterparts in k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] , which we are not going to do.)
We furthermore endow the ring k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] with the following topology (as in [13 Proof of Corollary 2.6.11] ):
We endow the ring k \mathbf{k} k with the discrete topology. To define a topology on the k \mathbf{k} k -algebra k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] , we (temporarily) regard every power series in k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] as the family of its coefficients (indexed by the set Mon \operatorname{Mon} Mon ). More precisely, we have a k \mathbf{k} k -module isomorphism
∏ m ∈ Mon k ⟶ k [ [ x 1 , x 2 , x 3 , … ] ] , ( λ m ) m ∈ Mon ⟼ ∑ m ∈ Mon λ m m . \prod_{m\in\operatorname{Mon}}\mathbf{k}\longrightarrow\mathbf{k}[\![x_1,x_2,x_3,\ldots]\!],\qquad(\lambda_m)_{m\in\operatorname{Mon}}\longmapsto\sum_{m\in\operatorname{Mon}}\lambda_m m. m ∈ Mon ∏ k ⟶ k [ [ x 1 , x 2 , x 3 , … ] ] , ( λ m ) m ∈ Mon ⟼ m ∈ Mon ∑ λ m m .
We use this isomorphism to transport the product topology on ∏ m ∈ Mon k \prod_{m\in\operatorname{Mon}}\mathbf{k} ∏ m ∈ Mon k to k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] .
The resulting topology on k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] turns k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] into a topological k \mathbf{k} k -algebra; this is the topology that we will be using whenever we make statements about convergence in k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] or write down infinite sums of power series. A sequence ( a n ) n ∈ N (a_n)_{n\in\mathbb{N}} ( a n ) n ∈ N of power series converges to a power series a a a with respect to this topology if and only if for every monomial m m m , all sufficiently high n ∈ N n\in\mathbb{N} n ∈ N satisfy
(the coefficient of m in a n ) = (the coefficient of m in a ) . \text{(the coefficient of $m$ in $a_n$)}=\text{(the coefficient of $m$ in $a$)}. (the coefficient of m in a n ) = (the coefficient of m in a ) .
Note that this topological k \mathbf{k} k -algebra k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] is not the completion of the polynomial ring k [ x 1 , x 2 , x 3 , … ] \mathbf{k}[x_1,x_2,x_3,\ldots] k [ x 1 , x 2 , x 3 , … ] with respect to the standard grading (in which all x i x_i x i have degree 1 1 1 ). (They are distinct even as sets.)
Inside the k \mathbf{k} k -algebra k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] is a subalgebra k [ [ x 1 , x 2 , x 3 , … ] ] b d d \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!]_{\mathrm{bdd}} k [ [ x 1 , x 2 , x 3 , … ] ] bdd consisting of the bounded-degree formal power series; these are the power series f f f for which there exists a d ∈ N d\in\mathbb{N} d ∈ N such that no monomial of degree > d >d > d appears in f f f .4 This k \mathbf{k} k -subalgebra k [ [ x 1 , x 2 , x 3 , … ] ] b d d \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!]_{\mathrm{bdd}} k [ [ x 1 , x 2 , x 3 , … ] ] bdd becomes a topological k \mathbf{k} k -algebra, by inheriting the topology from k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[\![x_1,x_2,x_3,\ldots]\!] k [ [ x 1 , x 2 , x 3 , … ] ] .
Two monomials m m m and n n n are said to be pack-equivalent 5 if they have the forms x i 1 a 1 x i 2 a 2 ⋯ x i ℓ a ℓ x_{i_1}^{a_1}x_{i_2}^{a_2}\cdots x_{i_\ell}^{a_\ell} x i 1 a 1 x i 2 a 2 ⋯ x i ℓ a ℓ and x j 1 a 1 x j 2 a 2 ⋯ x j ℓ a ℓ x_{j_1}^{a_1}x_{j_2}^{a_2}\cdots x_{j_\ell}^{a_\ell} x j 1 a 1 x j 2 a 2 ⋯ x j ℓ a ℓ for two strictly increasing sequences ( i 1 < i 2 < ⋯ < i ℓ ) (i_1<i_2<\cdots<i_\ell) ( i 1 < i 2 < ⋯ < i ℓ ) and ( j 1 < j 2 < ⋯ < j ℓ ) (j_1<j_2<\cdots<j_\ell) ( j 1 < j 2 < ⋯ < j ℓ ) of positive integers and one (common) sequence ( a 1 , a 2 , … , a ℓ ) (a_1,a_2,\ldots,a_\ell) ( a 1 , a 2 , … , a ℓ ) of positive integers.6 A power series f ∈ k [ [ x 1 , x 2 , x 3 , … ] ] f\in\mathbb{k}[[x_1,x_2,x_3,\ldots]] f ∈ k [[ x 1 , x 2 , x 3 , … ]] is said to be quasisymmetric if it satisfies the following condition: If m m m and n n n are two pack-equivalent monomials, then the coefficient of m m m in f f f equals the coefficient of n n n in f f f .
It is easy to see that the quasisymmetric power series form a k \mathbb{k} k -subalgebra of k [ [ x 1 , x 2 , x 3 , … ] ] \mathbb{k}[[x_1,x_2,x_3,\ldots]] k [[ x 1 , x 2 , x 3 , … ]] . But usually one is interested in a subset of this k \mathbb{k} k -subalgebra: namely, the set of quasisymmetric bounded-degree power series in k [ [ x 1 , x 2 , x 3 , … ] ] \mathbb{k}[[x_1,x_2,x_3,\ldots]] k [[ x 1 , x 2 , x 3 , … ]] . This latter set is a k \mathbb{k} k -subalgebra of k [ [ x 1 , x 2 , x 3 , … ] ] b d d \mathbb{k}[[x_1,x_2,x_3,\ldots]]_{\mathrm{bdd}} k [[ x 1 , x 2 , x 3 , … ] ] bdd and is known as the k \mathbb{k} k -algebra of quasisymmetric functions over k \mathbb{k} k . It is denoted by QSym.
The symmetric functions (in the usual sense of this word in combinatorics – so, really, symmetric bounded-degree power series in k [ [ x 1 , x 2 , x 3 , … ] ] \mathbb{k}[[x_1,x_2,x_3,\ldots]] k [[ x 1 , x 2 , x 3 , … ]] ) form a k \mathbb{k} k -subalgebra of QSym. The quasisymmetric functions have a rich theory which is related to, and often sheds new light on, the classical theory of symmetric functions; expositions can be found in [25 §§7.19, 7.23] and [13 §§5-6] and other sources.7
As a k \mathbb{k} k -module, QSym has a basis ( M α ) α ∈ Comp (M_\alpha)_{\alpha\in\operatorname{Comp}} ( M α ) α ∈ Comp indexed by all compositions, where the quasisymmetric function M α M_\alpha M α for a given composition α \alpha α is defined as follows: Writing α \alpha α as ( α 1 , α 2 , … , α ℓ ) (\alpha_1,\alpha_2,\ldots,\alpha_\ell) ( α 1 , α 2 , … , α ℓ ) , we set
M α = ∑ i 1 < i 2 < ⋯ < i ℓ x i 1 α 1 x i 2 α 2 ⋯ x i ℓ α ℓ = ∑ m is a monomial pack-equivalent to x 1 α 1 x 2 α 2 ⋯ x ℓ α ℓ m M_\alpha=\sum_{i_1<i_2<\cdots<i_\ell}x_{i_1}^{\alpha_1}x_{i_2}^{\alpha_2}\cdots x_{i_\ell}^{\alpha_\ell}
=\sum_{\substack{m\text{ is a monomial pack-equivalent}\\\text{to }x_1^{\alpha_1}x_2^{\alpha_2}\cdots x_\ell^{\alpha_\ell}}}m M α = i 1 < i 2 < ⋯ < i ℓ ∑ x i 1 α 1 x i 2 α 2 ⋯ x i ℓ α ℓ = m is a monomial pack-equivalent to x 1 α 1 x 2 α 2 ⋯ x ℓ α ℓ ∑ m
(where the i k i_k i k in the first sum are positive integers). This basis ( M α ) α ∈ Comp (M_\alpha)_{\alpha\in\operatorname{Comp}} ( M α ) α ∈ Comp is known as the monomial basis of QSym, and is the simplest to define among many. (We shall briefly encounter another basis in Example 3.6.)
The k \mathbb{k} k -algebra QSym can be endowed with a structure of a k \mathbb{k} k -coalgebra which, combined with its k \mathbb{k} k -algebra structure, turns it into a Hopf algebra. We refer to the literature both for the theory of coalgebras and Hopf algebras (see [21 ] , [13 §1] , [20 §1-§2] , [Abe77], [28 ] , [4 ] or [7 Chapter 7] ) and for a deeper study of the Hopf algebra QSym (see [16 ] , [14 Chapter 6] or [13 §5] ); in this note we shall need but the very basics of this structure, and so it is only them that we introduce.
In the following, all tensor products are over k \mathbb{k} k by default (i.e., the sign ⊗ \otimes ⊗ stands for ⊗ k \otimes_{\mathbb{k}} ⊗ k unless it comes with a subscript).
Now, we define two k \mathbb{k} k -linear maps Δ \Delta Δ and ε \varepsilon ε as follows.8
Δ ( M ( α 1 , α 2 , … , α ℓ ) ) = ∑ k = 0 ℓ M ( α 1 , α 2 , … , α k ) ⊗ M ( α k + 1 , α k + 2 , … , α ℓ ) (1) \Delta\left(M_{(\alpha_1,\alpha_2,\ldots,\alpha_\ell)}\right)=\sum_{k=0}^{\ell}M_{(\alpha_1,\alpha_2,\ldots,\alpha_k)}\otimes M_{(\alpha_{k+1},\alpha_{k+2},\ldots,\alpha_\ell)} \tag*{(1)} Δ ( M ( α 1 , α 2 , … , α ℓ ) ) = k = 0 ∑ ℓ M ( α 1 , α 2 , … , α k ) ⊗ M ( α k + 1 , α k + 2 , … , α ℓ ) (1)
for every ( α 1 , α 2 , … , α ℓ ) ∈ C o m p (\alpha_1,\alpha_2,\ldots,\alpha_\ell)\in\mathrm{Comp} ( α 1 , α 2 , … , α ℓ ) ∈ Comp .
ε ( M ( α 1 , α 2 , … , α ℓ ) ) = δ ℓ , 0 \varepsilon\left(M_{(\alpha_1,\alpha_2,\ldots,\alpha_\ell)}\right)=\delta_{\ell,0} ε ( M ( α 1 , α 2 , … , α ℓ ) ) = δ ℓ , 0
for every ( α 1 , α 2 , … , α ℓ ) ∈ C o m p (\alpha_1,\alpha_2,\ldots,\alpha_\ell)\in\mathrm{Comp} ( α 1 , α 2 , … , α ℓ ) ∈ Comp .
(Here, δ u , v \delta_{u,v} δ u , v is defined to be { 1 , if u = v ; 0 , if u ≠ v \begin{cases}1,&\text{if }u=v;\\0,&\text{if }u\ne v\end{cases} { 1 , 0 , if u = v ; if u = v whenever u u u and v v v are two objects.)
The map ε \varepsilon ε can also be defined in a simpler (equivalent) way: Namely, ε \varepsilon ε sends every power series f ∈ Q S y m f\in\mathrm{QSym} f ∈ QSym to the result f ( 0 , 0 , 0 , … ) f(0,0,0,\ldots) f ( 0 , 0 , 0 , … ) of substituting zeroes for the variables x 1 , x 2 , x 3 , … x_1,x_2,x_3,\ldots x 1 , x 2 , x 3 , … in f f f . The map Δ \Delta Δ can also be described in such terms, but with greater difficulty9 .
It is well-known that these maps Δ \Delta Δ and ε \varepsilon ε make the three diagrams
Q S y m → Δ Q S y m ⊗ Q S y m ↓ Δ ↓ Δ ⊗ i d Q S y m ⊗ Q S y m → i d ⊗ Δ Q S y m ⊗ Q S y m ⊗ Q S y m Q S y m → Δ Q S y m ⊗ Q S y m ↘ ≅ ↓ ε ⊗ i d k ⊗ Q S y m Q S y m → Δ Q S y m ⊗ Q S y m ↘ ≅ ↓ i d ⊗ ε Q S y m ⊗ k \begin{array}{c c c}
\mathrm{QSym} & \xrightarrow{\Delta} & \mathrm{QSym}\otimes\mathrm{QSym}\\
\downarrow{\Delta} & & \downarrow{\Delta\otimes\mathrm{id}}\\
\mathrm{QSym}\otimes\mathrm{QSym} & \xrightarrow{\mathrm{id}\otimes\Delta} & \mathrm{QSym}\otimes\mathrm{QSym}\otimes\mathrm{QSym}
\end{array}
\qquad
\begin{array}{c c c}
\mathrm{QSym} & \xrightarrow{\Delta} & \mathrm{QSym}\otimes\mathrm{QSym}\\
\searrow_{\cong} & & \downarrow{\varepsilon\otimes\mathrm{id}}\\
& k\otimes\mathrm{QSym} &
\end{array}
\qquad
\begin{array}{c c c}
\mathrm{QSym} & \xrightarrow{\Delta} & \mathrm{QSym}\otimes\mathrm{QSym}\\
\searrow_{\cong} & & \downarrow{\mathrm{id}\otimes\varepsilon}\\
& \mathrm{QSym}\otimes k &
\end{array} QSym ↓ Δ QSym ⊗ QSym Δ id ⊗ Δ QSym ⊗ QSym ↓ Δ ⊗ id QSym ⊗ QSym ⊗ QSym QSym ↘ ≅ Δ k ⊗ QSym QSym ⊗ QSym ↓ ε ⊗ id QSym ↘ ≅ Δ QSym ⊗ k QSym ⊗ QSym ↓ id ⊗ ε
(where the ≅ \cong ≅ arrows are the canonical isomorphisms) commutative, and so ( Q S y m , Δ , ε ) (\mathrm{QSym},\Delta,\varepsilon) ( QSym , Δ , ε ) is what is commonly called a k k k -coalgebra. Furthermore, Δ \Delta Δ and ε \varepsilon ε are k k k -algebra homomorphisms, which is what makes this k k k -coalgebra Q S y m \mathrm{QSym} QSym into a k k k -bialgebra. Finally, let m : Q S y m ⊗ Q S y m → Q S y m m:\mathrm{QSym}\otimes\mathrm{QSym}\to\mathrm{QSym} m : QSym ⊗ QSym → QSym be the k k k -linear map sending every pure tensor a ⊗ b a\otimes b a ⊗ b to a b ab ab , and let u : k → Q S y m u:k\to\mathrm{QSym} u : k → QSym be the k k k -linear map sending 1 ∈ k 1\in k 1 ∈ k to 1 ∈ Q S y m 1\in\mathrm{QSym} 1 ∈ QSym . Then, there exists a unique k k k -linear map S : Q S y m → Q S y m S:\mathrm{QSym}\to\mathrm{QSym} S : QSym → QSym making the diagram
Q S y m ⊗ Q S y m → S ⊗ i d Q S y m ⊗ Q S y m Δ ↗ ↘ m Q S y m → ε k → u Q S y m Δ ↘ ↗ m Q S y m ⊗ Q S y m → i d ⊗ S Q S y m ⊗ Q S y m (2) \begin{array}{c c c}
& \mathrm{QSym}\otimes\mathrm{QSym} & \xrightarrow{S\otimes\mathrm{id}} \mathrm{QSym}\otimes\mathrm{QSym}\\
{}^{\Delta}\nearrow& & \searrow^{m}\\
\mathrm{QSym} & \xrightarrow{\varepsilon} k \xrightarrow{u} \mathrm{QSym}\\
{}_{\Delta}\searrow& & \nearrow_{m}\\
& \mathrm{QSym}\otimes\mathrm{QSym} & \xrightarrow{\mathrm{id}\otimes S} \mathrm{QSym}\otimes\mathrm{QSym} \tag*{(2)}
\end{array} Δ ↗ QSym Δ ↘ QSym ⊗ QSym ε k u QSym QSym ⊗ QSym S ⊗ id QSym ⊗ QSym ↘ m ↗ m id ⊗ S QSym ⊗ QSym (2)
commutative. This map S S S is known as the antipode of QSym. It is known to be an involution and an algebra automorphism of QSym, and its action on the various quasisymmetric functions defined combinatorially is the main topic of this note. The existence of the antipode S S S makes QSym into a Hopf algebra .
Double posets
Next, we shall introduce the notion of a double poset, following Malvenuto and Reutenauer [19 ] .
Definition 3.1. (a) We shall encode posets as pairs ( E , < ) (E, <) ( E , < ) , where E E E is a set and < < < is a strict partial order (i.e., an irreflexive, transitive and antisymmetric binary relation) on the set E E E ; this relation < < < will be regarded as the smaller relation of the poset. All binary relations will be written in infix notation: i.e., we write “a < b a < b a < b ” for “a a a is related to b b b by the relation < < < ”. (If you define binary relations as sets of pairs, then “a a a is related to b b b by the relation < < < ” means that ( a , b ) (a,b) ( a , b ) is an element of the set < < < .)
(b) If < < < is a strict partial order on a set E E E , and if a a a and b b b are two elements of E E E , then we say that a a a and b b b are < < < -comparable if we have either a < b a < b a < b or a = b a = b a = b or b < a b < a b < a . A strict partial order < < < on a set E E E is said to be a total order if and only if every two elements of E E E are < < < -comparable.
(c) If < < < is a strict partial order on a set E E E , and if a a a and b b b are two elements of E E E , then we say that a a a is < < < -covered by b b b if we have a < b a < b a < b and there exists no c ∈ E c \in E c ∈ E satisfying a < c < b a < c < b a < c < b . (For instance, if < < < is the standard smaller relation on Z \mathbb{Z} Z , then each i ∈ Z i \in\mathbb{Z} i ∈ Z is < < < -covered by i + 1 i + 1 i + 1 .)
(d) A double poset is defined as a triple ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) where E E E is a finite set and < 1 <_1 < 1 and < 2 <_2 < 2 are two strict partial orders on E E E .
(e) A double poset ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) is said to be special if the relation < 2 <_2 < 2 is a total order.
(f) A double poset ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) is said to be semispecial if every two < 1 <_1 < 1 -comparable elements of E E E are < 2 <_2 < 2 -comparable.
(g) A double poset ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) is said to be tertispecial if it satisfies the following condition: If a a a and b b b are two elements of E E E such that a a a is < 1 <_1 < 1 -covered by b b b , then a a a and b b b are < 2 <_2 < 2 -comparable.
(h) If < < < is a binary relation on a set E E E , then the opposite relation of < < < is defined to be the binary relation > > > on the set E E E that is defined as follows: For any e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E , we have e > f e > f e > f if and only if f < e f < e f < e . Notice that if < < < is a strict partial order, then so is the opposite relation > > > of < < < .
Clearly, every special double poset is semispecial, and every semispecial double poset is tertispecial.10
Definition 3.2. If E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) is a double poset, then an E E E -partition shall mean a map ϕ : E → { 1 , 2 , 3 , … } \phi:E\to\{1,2,3,\ldots\} ϕ : E → { 1 , 2 , 3 , … } such that:
every e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E satisfying e < 1 f e<_{1}f e < 1 f satisfy ϕ ( e ) ≤ ϕ ( f ) \phi(e)\leq\phi(f) ϕ ( e ) ≤ ϕ ( f ) ;
every e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E satisfying e < 1 f e<_{1}f e < 1 f and f < 2 e f<_{2}e f < 2 e satisfy ϕ ( e ) < ϕ ( f ) \phi(e)<\phi(f) ϕ ( e ) < ϕ ( f ) .
Example 3.3. The notion of an E E E -partition (which was inspired by the earlier notions of P P P -partitions and ( P , ω ) (P,\omega) ( P , ω ) -partitions as studied by Gessel and Stanley11 ) generalizes various well-known combinatorial concepts. For example:
If < 2 <_{2} < 2 is the same order as < 1 <_{1} < 1 (or any extension of this order), then the E E E -partitions are the weakly increasing maps from the poset ( E , < 1 ) (E,<_{1}) ( E , < 1 ) to the totally ordered set { 1 , 2 , 3 , … } \{1,2,3,\ldots\} { 1 , 2 , 3 , … } .
If < 2 <_{2} < 2 is the opposite relation of < 1 <_{1} < 1 (or any extension of this opposite relation), then the E E E -partitions are the strictly increasing maps from the poset ( E , < 1 ) (E,<_{1}) ( E , < 1 ) to the totally ordered set { 1 , 2 , 3 , … } \{1,2,3,\ldots\} { 1 , 2 , 3 , … } .
For a more interesting example, let μ = ( μ 1 , μ 2 , μ 3 , … ) \mu=(\mu_{1},\mu_{2},\mu_{3},\ldots) μ = ( μ 1 , μ 2 , μ 3 , … ) and λ = ( λ 1 , λ 2 , λ 3 , … ) \lambda=(\lambda_{1},\lambda_{2},\lambda_{3},\ldots) λ = ( λ 1 , λ 2 , λ 3 , … ) be two partitions such that μ ⊆ λ \mu\subseteq\lambda μ ⊆ λ . (See [13 §2] for the notations we are using here.) The skew Young diagram Y ( λ / μ ) Y(\lambda/\mu) Y ( λ / μ ) is then defined as the set of all ( i , j ) ∈ { 1 , 2 , 3 , … } 2 (i,j)\in\{1,2,3,\ldots\}^{2} ( i , j ) ∈ { 1 , 2 , 3 , … } 2 satisfying μ i < j ≤ λ i \mu_{i}<j\leq\lambda_{i} μ i < j ≤ λ i . On this set Y ( λ / μ ) Y(\lambda/\mu) Y ( λ / μ ) , we define two strict partial orders < 1 <_{1} < 1 and < 2 <_{2} < 2 by
( i , j ) < 1 ( i ′ , j ′ ) ⟺ ( i ≤ i ′ and j ≤ j ′ and ( i , j ) ≠ ( i ′ , j ′ ) ) (i,j)<_{1}(i',j')\Longleftrightarrow(i\leq i'\ \text{and}\ j\leq j'\ \text{and}\ (i,j)\ne(i',j')) ( i , j ) < 1 ( i ′ , j ′ ) ⟺ ( i ≤ i ′ and j ≤ j ′ and ( i , j ) = ( i ′ , j ′ )) and
( i , j ) < 2 ( i ′ , j ′ ) ⟺ ( i ≥ i ′ and j ≤ j ′ and ( i , j ) ≠ ( i ′ , j ′ ) ) . (i,j)<_{2}(i',j')\Longleftrightarrow(i\geq i'\ \text{and}\ j\leq j'\ \text{and}\ (i,j)\ne(i',j')). ( i , j ) < 2 ( i ′ , j ′ ) ⟺ ( i ≥ i ′ and j ≤ j ′ and ( i , j ) = ( i ′ , j ′ )) . The resulting double poset Y ( λ / μ ) = ( Y ( λ / μ ) , < 1 , < 2 ) \mathbf{Y}(\lambda/\mu)=(Y(\lambda/\mu),<_{1},<_{2}) Y ( λ / μ ) = ( Y ( λ / μ ) , < 1 , < 2 ) has the property that the Y ( λ / μ ) \mathbf{Y}(\lambda/\mu) Y ( λ / μ ) -partitions are precisely the semistandard tableaux of shape λ / μ \lambda/\mu λ / μ . (Again, see [13 §2] for the meaning of these words.)
This double poset Y ( λ / μ ) \mathbf{Y}(\lambda/\mu) Y ( λ / μ ) is not special (in general), but it is tertispecial. (Indeed, if a a a and b b b are two elements of Y ( λ / μ ) Y(\lambda/\mu) Y ( λ / μ ) such that a a a is < 1 <_{1} < 1 -covered by b b b , then a a a is either the left neighbor of b b b or the top neighbor of b b b , and thus we have
either a < 2 b a <_{2} b a < 2 b (in the former case) or b < 2 a b <_{2} a b < 2 a (in the latter case).) Some authors prefer to use a special double poset instead, which is defined as follows: We define a total order < h <_{h} < h on Y ( λ / μ ) \mathcal{Y}(\lambda/\mu) Y ( λ / μ ) by
( i , j ) < h ( i ′ , j ′ ) ⟺ ( i > i ′ or ( i = i ′ and j < j ′ ) ) . (i,j) <_{h} (i',j') \Longleftrightarrow(i > i' \text{ or } (i=i' \text{ and } j<j')). ( i , j ) < h ( i ′ , j ′ ) ⟺ ( i > i ′ or ( i = i ′ and j < j ′ )) .
Then, Y h ( λ / μ ) = ( Y ( λ / μ ) , < 1 , < h ) \mathcal{Y}_{h}(\lambda/\mu)=(\mathcal{Y}(\lambda/\mu),<_{1},<_{h}) Y h ( λ / μ ) = ( Y ( λ / μ ) , < 1 , < h ) is a special double poset, and the Y h ( λ / μ ) \mathcal{Y}_{h}(\lambda/\mu) Y h ( λ / μ ) -partitions are precisely the semistandard tableaux of shape λ / μ \lambda/\mu λ / μ .
We now assign a certain formal power series to every double poset:
Definition 3.4. If E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) is a double poset, and w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } is a map, then we define a power series Γ ( E , w ) ∈ k [ [ x 1 , x 2 , x 3 , … ] ] \Gamma(E,w)\in\mathbb{k}[[x_{1},x_{2},x_{3},\ldots]] Γ ( E , w ) ∈ k [[ x 1 , x 2 , x 3 , … ]] by
Γ ( E , w ) = ∑ π is an E -partition x π , w , where x π , w = ∏ e ∈ E x π ( e ) w ( e ) . \Gamma(E,w)=\sum_{\pi\text{ is an }E\text{-partition}}x_{\pi,w},\qquad\text{where }x_{\pi,w}=\prod_{e\in E}x_{\pi(e)}^{w(e)}. Γ ( E , w ) = π is an E -partition ∑ x π , w , where x π , w = e ∈ E ∏ x π ( e ) w ( e ) .
The following fact is easy to see (but will be reproven below):
Proposition 3.5. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset, and w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map. Then, Γ ( E , w ) ∈ QSym \Gamma(E,w)\in\operatorname{QSym} Γ ( E , w ) ∈ QSym .
Example 3.6. The power series Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) generalize various well-known quasisymmetric functions.
(a) If E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) is a double poset, and w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } is the constant function sending everything to 1, then Γ ( E , w ) = ∑ π is an E -partition x π \Gamma(E,w)=\sum_{\pi\text{ is an }E\text{-partition}}x_{\pi} Γ ( E , w ) = ∑ π is an E -partition x π , where x π = ∏ e ∈ E x π ( e ) x_{\pi}=\prod_{e\in E}x_{\pi(e)} x π = ∏ e ∈ E x π ( e ) . We shall denote this power series Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) by Γ ( E ) \Gamma(E) Γ ( E ) ; it is exactly what has been called Γ ( E ) \Gamma(E) Γ ( E ) in [19 §2.2] . All results proven below for Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) can be applied to Γ ( E ) \Gamma(E) Γ ( E ) , yielding simpler (but less general) statements.
(b) If E = { 1 , 2 , … , ℓ } E=\{1,2,\ldots,\ell\} E = { 1 , 2 , … , ℓ } for some ℓ ∈ N \ell\in\mathbb{N} ℓ ∈ N , if < 1 <_{1} < 1 is the usual total order inherited from Z \mathbb{Z} Z , and if < 2 <_{2} < 2 is the opposite relation of < 1 <_{1} < 1 , then the special double poset E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) satisfies Γ ( E , w ) = M α \Gamma(E,w)=M_{\alpha} Γ ( E , w ) = M α , where α \alpha α is the composition ( w ( 1 ) , w ( 2 ) , … , w ( ℓ ) ) (w(1),w(2),\ldots,w(\ell)) ( w ( 1 ) , w ( 2 ) , … , w ( ℓ )) .
Note that every M α M_{\alpha} M α can be obtained this way (by choosing ℓ \ell ℓ and w w w appropriately). Thus, the elements of the monomial basis ( M α ) α ∈ Comp (M_{\alpha})_{\alpha\in\operatorname{Comp}} ( M α ) α ∈ Comp are special cases of the functions Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) . This shows that the Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) for varying E E E and w w w span the k \mathbb{k} k -module QSym \operatorname{QSym} QSym .
(c) Let α = ( α 1 , α 2 , … , α ℓ ) \alpha= (\alpha_1,\alpha_2,\ldots,\alpha_{\ell}) α = ( α 1 , α 2 , … , α ℓ ) be a composition of a nonnegative integer n n n . Let D ( α ) D(\alpha) D ( α ) be the set { α 1 , α 1 + α 2 , α 1 + α 2 + α 3 , … , α 1 + α 2 + ⋯ + α ℓ − 1 } \{\alpha_1,\alpha_1+\alpha_2,\alpha_1+\alpha_2+\alpha_3,\ldots,\alpha_1+\alpha_2+\cdots+\alpha_{\ell-1}\} { α 1 , α 1 + α 2 , α 1 + α 2 + α 3 , … , α 1 + α 2 + ⋯ + α ℓ − 1 } . Let E E E be the set { 1 , 2 , … , n } \{1,2,\ldots,n\} { 1 , 2 , … , n } , and let < 1 <_{1} < 1 be the total order inherited on E E E from Z \mathbb{Z} Z . Let < 2 <_{2} < 2 be some partial order on E E E with the property that
i + 1 < 2 i for every i ∈ D ( α ) i+1 <_{2} i \qquad\text{for every } i \in D(\alpha) i + 1 < 2 i for every i ∈ D ( α )
and
i < 2 i + 1 for every i ∈ { 1 , 2 , … , n − 1 } ∖ D ( α ) . i <_{2} i+1 \qquad\text{for every } i \in\{1,2,\ldots,n-1\}\setminus D(\alpha). i < 2 i + 1 for every i ∈ { 1 , 2 , … , n − 1 } ∖ D ( α ) .
(There are several choices for such an order; in particular, we can find one which is a total order.) Then,
Γ ( ( E , < 1 , < 2 ) ) = ∑ i 1 ≤ i 2 ≤ ⋯ ≤ i n ; i j < i j + 1 whenever j ∈ D ( α ) x i 1 x i 2 ⋯ x i n = ∑ β is a composition of n ; D ( β ) ⊇ D ( α ) M β . \begin{aligned}
\Gamma((E,<_{1},<_{2})) = \sum_{\substack{i_1\leq i_2\leq\cdots\leq i_n;\\ i_j<i_{j+1}\text{ whenever }j\in D(\alpha)}} x_{i_1}x_{i_2}\cdots x_{i_n} \\
&= \sum_{\substack{\beta\text{ is a composition of }n;\\ D(\beta)\supseteq D(\alpha)}} M_{\beta}.
\end{aligned} Γ (( E , < 1 , < 2 )) = i 1 ≤ i 2 ≤ ⋯ ≤ i n ; i j < i j + 1 whenever j ∈ D ( α ) ∑ x i 1 x i 2 ⋯ x i n = β is a composition of n ; D ( β ) ⊇ D ( α ) ∑ M β .
This power series is known as the α \alpha α -th fundamental quasisymmetric function , usually called F α F_{\alpha} F α (in [8 ] , [17 §2] , [3 §2.4] and [10 §2] ) or L α L_{\alpha} L α (in [25 §7.19] or [13 Definition 5.2.4] ).
(d) Let E E E be one of the two double posets Y ( λ / μ ) \mathbf{Y}(\lambda/\mu) Y ( λ / μ ) and Y h ( λ / μ ) \mathbf{Y}_{h}(\lambda/\mu) Y h ( λ / μ ) defined as in Example 3.3 for two partitions μ \mu μ and λ \lambda λ . Then, Γ ( E ) \Gamma(E) Γ ( E ) is the skew Schur function s λ / μ s_{\lambda/\mu} s λ / μ .
(e) Similarly, dual immaculate functions as defined in [3 §3.7] can be realized as Γ ( E ) \Gamma(E) Γ ( E ) for conveniently chosen E E E (see [10 Proposition 4.4] ), which helped the author to prove one of their properties [10 ] . (The E E E -partitions here are the so-called immaculate tableaux .)
(f) When the relation < 2 <_{2} < 2 of a double poset E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) is a total order (i.e., when the double poset E E E is special), the E E E -partitions are precisely the reverse ( P , ω ) (P,\omega) ( P , ω ) -partitions (for P = ( E , < 1 ) P=(E,<_{1}) P = ( E , < 1 ) and ω \omega ω being the unique bijection E → { 1 , 2 , … , ∣ E ∣ } E\to\{1,2,\ldots,|E|\} E → { 1 , 2 , … , ∣ E ∣ } satisfying ω − 1 ( 1 ) < 2 ω − 1 ( 2 ) < 2 ⋯ < 2 ω − 1 ( ∣ E ∣ ) \omega^{-1}(1)<_{2}\omega^{-1}(2)<_{2}\cdots<_{2}\omega^{-1}(|E|) ω − 1 ( 1 ) < 2 ω − 1 ( 2 ) < 2 ⋯ < 2 ω − 1 ( ∣ E ∣ ) ) in the terminology of [25 §7.19] , and the power series Γ ( E ) \Gamma(E) Γ ( E ) is the K P , ω K_{P,\omega} K P , ω of [25 §7.19] . This can also be rephrased using the notations of [13 §5.2] : When the relation < 2 <_{2} < 2 of a double poset E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) is a total order, we can relabel the elements of E E E by the integers 1 , 2 , … , n 1,2,\ldots,n 1 , 2 , … , n (where n = ∣ E ∣ n=|E| n = ∣ E ∣ ) in such a way that 1 < 2 2 < 2 ⋯ < 2 n 1<_{2}2<_{2}\cdots<_{2}n 1 < 2 2 < 2 ⋯ < 2 n ; then, the E E E -partitions are the P P P -partitions in the terminology of [13 Definition 5.2.1] , where P P P is the labelled poset ( E , < 1 ) (E,<_{1}) ( E , < 1 ) ; and furthermore, our Γ ( E ) \Gamma(E) Γ ( E ) is the F P ( x ) F_P(x) F P ( x ) of [13 Definition 5.2.1] . Conversely, if P P P is a labelled poset, then the F P ( x ) F_P(x) F P ( x ) of [13 Definition 5.2.1] is our Γ ( ( P , < P , < Z ) ) \Gamma((P,<_{P},<_{\mathbb{Z}})) Γ (( P , < P , < Z )) .
The antipode theorem
We now come to the main results of this note. We first state a theorem and a corollary which are not new, but will be reproven in a more self-contained way which allows them to take their (well-deserved) place as fundamental results rather than afterthoughts in the theory of QSym.
Definition 4.1. We let S S S denote the antipode of QSym.
Theorem 4.2. Let ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) be a tertispecial double poset. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } . Then, S ( Γ ( ( E , < 1 , < 2 ) , w ) ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) S\left(\Gamma((E,<_{1},<_{2}),w)\right)=(-1)^{|E|}\Gamma((E,>_{1},<_{2}),w) S ( Γ (( E , < 1 , < 2 ) , w ) ) = ( − 1 ) ∣ E ∣ Γ (( E , > 1 , < 2 ) , w ) , where > 1 >_{1} > 1 denotes the opposite relation of < 1 <_{1} < 1 .
Corollary 4.3. Let ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) be a tertispecial double poset. Then, S ( Γ ( ( E , < 1 , < 2 ) ) ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) ) S\left(\Gamma((E,<_{1},<_{2}))\right)=(-1)^{|E|}\Gamma((E,>_{1},<_{2})) S ( Γ (( E , < 1 , < 2 )) ) = ( − 1 ) ∣ E ∣ Γ (( E , > 1 , < 2 )) , where > 1 >_{1} > 1 denotes the opposite relation of < 1 <_{1} < 1 .
We shall give examples for consequences of these facts shortly (Example 4.8 ), but let us first explain where they have already appeared. Corollary 4.3 is equivalent to [13 Corollary 5.2.20] 12 (a result found by Malvenuto and Reutenauer [18 Lemma 3.2] ). Theorem 4.2 is equivalent to Malvenuto’s and Reutenauer’s [18 Theorem 3.1] 13 . We nevertheless believe that our versions of these facts
Let me sketch how to derive [18 Theorem 3.1] from our Theorem 4.2. Indeed, contract all undirected edges in G G G and G ′ G' G ′ , denoting the (common) vertex set of the new graphs by E E E . Then, define two strict partial orders < 1 <_{1} < 1 and < 2 <_{2} < 2 on E E E by
( a < 1 b ) ⟺ ( a ≠ b , and there exists a path from a to b in G ) (a<_{1}b)\Longleftrightarrow(a\ne b,\text{ and there exists a path from }a\text{ to }b\text{ in }G) ( a < 1 b ) ⟺ ( a = b , and there exists a path from a to b in G )
and
( a < 2 b ) ⟺ ( a ≠ b , and there exists a path from a to b in G ′ ) . (a<_{2}b)\Longleftrightarrow(a\ne b,\text{ and there exists a path from }a\text{ to }b\text{ in }G'). ( a < 2 b ) ⟺ ( a = b , and there exists a path from a to b in G ′ ) .
The map w w w sends every e ∈ E e\in E e ∈ E to the number of vertices of G G G that became e e e when the edges were contracted. To show that the resulting double poset ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) is tertispecial, we must notice that if a a a is < 1 <_{1} < 1 -covered by b b b , then G G G had an edge from one of the vertices that became a a a to one of the vertices that became b b b . The “x i x_i x i ’s in X X X satisfying a set of conditions” (in the language of [18 Section 3] ) are in 1-to-1 correspondence with ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) -partitions (at least when X = { 1 , 2 , 3 , … } X=\{1,2,3,\ldots\} X = { 1 , 2 , 3 , … } ); this is not immediately obvious but not hard to check either (the acyclicity of are slicker and simpler than the ones appearing in existing literature14 , and if not, then at least our proofs below are more natural.
To these known results, we add another, which seems to be unknown so far (probably because it is far harder to state in the terminologies of ( P , ω ) (P,\omega) ( P , ω ) -partitions or equality-and-inequality conditions appearing in literature). First, we need to introduce some notation:
Definition 4.4. Let G G G be a group, and let E E E be a G G G -set.
(a) Let < < < be a strict partial order on E E E . We say that G G G preserves the relation < < < if the following holds: For every g ∈ G g \in G g ∈ G , a ∈ E a \in E a ∈ E and b ∈ E b \in E b ∈ E satisfying a < b a < b a < b , we have g a < g b ga < gb g a < g b .
(b) Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } . We say that G G G preserves w w w if every g ∈ G g \in G g ∈ G and e ∈ E e \in E e ∈ E satisfy w ( g e ) = w ( e ) w(ge)=w(e) w ( g e ) = w ( e ) .
(c) Let g ∈ G g \in G g ∈ G . Assume that the set E E E is finite. We say that g g g is E E E -even if the action of g g g on E E E (that is, the permutation of E E E that sends every e ∈ E e \in E e ∈ E to g e ge g e ) is an even permutation of E E E .
(d) If X X X is any set, then the set X E X^E X E of all maps E → X E \to X E → X becomes a G G G -set in the following way: For any π ∈ X E \pi\in X^E π ∈ X E and g ∈ G g \in G g ∈ G , we define the element g π ∈ X E g\pi\in X^E g π ∈ X E to be the map sending each e ∈ E e \in E e ∈ E to π ( g − 1 e ) \pi(g^{-1}e) π ( g − 1 e ) .
(e) Let F F F be a further G G G -set. Assume that the set E E E is finite. An element π ∈ F \pi\in F π ∈ F is said to be E E E -coeven if every g ∈ G g \in G g ∈ G satisfying g π = π g\pi=\pi g π = π is E E E -even. A G G G -orbit O O O on F F F is said to be E E E -coeven if all elements of O O O are E E E -coeven.
Before we come to the promised result, let us state two simple facts:
Lemma 4.5. Let G G G be a group. Let F F F and E E E be G G G -sets such that E E E is finite. Let O O O be a G G G -orbit on F F F . Then, O O O is E E E -coeven if and only if at least one element of O O O is E E E -coeven.
Proposition 4.6. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset. Let Par E \operatorname{Par} E Par E denote the set of all E E E -partitions. Let G G G be a finite group which acts on E E E . Assume that G G G preserves both relations < 1 <_{1} < 1 and < 2 <_{2} < 2 .
(a) Then, Par E \operatorname{Par} E Par E is a G G G -subset of the G G G -set { 1 , 2 , 3 , … } E \{1,2,3,\ldots\}^{E} { 1 , 2 , 3 , … } E (see Definition 4.4 (d) for the definition of the latter).
G and G ′ G' G ′ is used in the proof). As a result, [18 Theorem 3.1] follows from Theorem 4.2 above. With some harder work, one can conversely derive our Theorem 4.2 from [18 Theorem 3.1] . (b) Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } . Assume that G G G preserves w w w . Let O O O be a G G G -orbit on Par E \operatorname{Par} E Par E . Then, the values of x π , w x_{\pi,w} x π , w for all π ∈ O \pi\in O π ∈ O are equal.
Theorem 4.7. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset. Let Par E \operatorname{Par} E Par E denote the set of all E E E -partitions. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } . Let G G G be a finite group which acts on E E E . Assume that G G G preserves both relations < 1 <_{1} < 1 and < 2 <_{2} < 2 , and also preserves w w w . Then, G G G acts also on the set Par E \operatorname{Par} E Par E of all E E E -partitions; namely, Par E \operatorname{Par} E Par E is a G G G -subset of the G G G -set { 1 , 2 , 3 , … } E \{1,2,3,\ldots\}^{E} { 1 , 2 , 3 , … } E (according to Proposition 4.6 (a)). For any G G G -orbit O O O on Par E \operatorname{Par} E Par E , we define a monomial x O , w x_{O,w} x O , w by
x O , w = x π , w for some element π of O . x_{O,w}=x_{\pi,w}\qquad\text{for some element }\pi\text{ of }O. x O , w = x π , w for some element π of O . (This is well-defined, since Proposition 4.6 (b) shows that x π , w x_{\pi,w} x π , w does not depend on the choice of $\pi\in O.)
Let
Γ ( E , w , G ) = ∑ O is a G -orbit on Par E x O , w \Gamma(E,w,G)=\sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par} E}}x_{O,w} Γ ( E , w , G ) = O is a G -orbit on Par E ∑ x O , w and
Γ + ( E , w , G ) = ∑ O is an E -coeven G -orbit on Par E x O , w . \Gamma^{+}(E,w,G)=\sum_{\substack{O\text{ is an }E\text{-coeven }G\text{-orbit on }\operatorname{Par} E}}x_{O,w}. Γ + ( E , w , G ) = O is an E -coeven G -orbit on Par E ∑ x O , w . Then, Γ ( E , w , G ) \Gamma(E,w,G) Γ ( E , w , G ) and Γ + ( E , w , G ) \Gamma^{+}(E,w,G) Γ + ( E , w , G ) belong to QSym \operatorname{QSym} QSym and satisfy
S ( Γ ( E , w , G ) ) = ( − 1 ) ∣ E ∣ Γ + ( ( E , > 1 , < 2 ) , w , G ) . S\bigl(\Gamma(E,w,G)\bigr)=(-1)^{|E|}\Gamma^{+}\bigl((E,>_{1},<_{2}),w,G\bigr). S ( Γ ( E , w , G ) ) = ( − 1 ) ∣ E ∣ Γ + ( ( E , > 1 , < 2 ) , w , G ) . Here, > 1 >_{1} > 1 denotes the opposite relation of < 1 <_{1} < 1 .
This theorem, which combines Theorem 4.2 with the ideas of Pólya enumeration, is inspired by Jochemko’s reciprocity result for order polynomials [15 Theorem 2.8] , which can be obtained from it by specializations (see § 10 for the details of how Jochemko’s result follows from ours).
We shall now briefly review a number of particular cases of Theorem 4.2 .
Example 4.8. (a) Corollary 4.3 follows from Theorem 4.2 by letting w w w be the function which is constantly 1.
(b) Let α = ( α 1 , α 2 , … , α ℓ ) \alpha=(\alpha_{1},\alpha_{2},\ldots,\alpha_{\ell}) α = ( α 1 , α 2 , … , α ℓ ) be a composition of a nonnegative integer n n n , and let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be the double poset defined in Example 3.6 (b). Let w : { 1 , 2 , … , ℓ } → { 1 , 2 , 3 , … } w:\{1,2,\ldots,\ell\}\to\{1,2,3,\ldots\} w : { 1 , 2 , … , ℓ } → { 1 , 2 , 3 , … } be the map sending every i i i to α i \alpha_{i} α i . As Example 3.6 (b) shows, we have Γ ( E , w ) = M α \Gamma(E,w)=M_{\alpha} Γ ( E , w ) = M α . Thus, applying Theorem 4.2 to
these E E E and w w w yields
S ( M α ) = ( − 1 ) ℓ Γ ( ( E , > 1 , < 2 ) , w ) = ( − 1 ) ℓ ∑ i 1 ≥ i 2 ≥ ⋯ ≥ i ℓ x i 1 α 1 x i 2 α 2 ⋯ x i ℓ α ℓ = ( − 1 ) ℓ ∑ i 1 ≤ i 2 ≤ ⋯ ≤ i ℓ x i 1 α ℓ x i 2 α ℓ − 1 ⋯ x i ℓ α 1 = ( − 1 ) ℓ ∑ γ is a composition of n ; D ( γ ) ⊆ D ( ( α ℓ , α ℓ − 1 , … , α 1 ) ) M γ . \begin{aligned}
S(M_\alpha)=(-1)^\ell\Gamma((E,>_1,< _2),w)=(-1)^\ell\sum_{i_1\ge i_2\ge\cdots\ge i_\ell}x_{i_1}^{\alpha_1}x_{i_2}^{\alpha_2}\cdots x_{i_\ell}^{\alpha_\ell} \\
&=(-1)^\ell\sum_{i_1\le i_2\le\cdots\le i_\ell}x_{i_1}^{\alpha_\ell}x_{i_2}^{\alpha_{\ell-1}}\cdots x_{i_\ell}^{\alpha_1}=(-1)^\ell\sum_{\substack{\gamma\text{ is a composition of }n;\\D(\gamma)\subseteq D((\alpha_\ell,\alpha_{\ell-1},\ldots,\alpha_1))}}M_\gamma.
\end{aligned} S ( M α ) = ( − 1 ) ℓ Γ (( E , > 1 , < 2 ) , w ) = ( − 1 ) ℓ i 1 ≥ i 2 ≥ ⋯ ≥ i ℓ ∑ x i 1 α 1 x i 2 α 2 ⋯ x i ℓ α ℓ = ( − 1 ) ℓ i 1 ≤ i 2 ≤ ⋯ ≤ i ℓ ∑ x i 1 α ℓ x i 2 α ℓ − 1 ⋯ x i ℓ α 1 = ( − 1 ) ℓ γ is a composition of n ; D ( γ ) ⊆ D (( α ℓ , α ℓ − 1 , … , α 1 )) ∑ M γ .
This is the formula for S ( M α ) S(M_\alpha) S ( M α ) given in [5 Proposition 3.4] , in [16 (4.26)] , in [13 Theorem 5.1.11] , and in [2 Theorem 4.1] (originally due to Ehrenborg and to Malvenuto and Reutenauer).
(c) Applying Corollary 4.3 to the double poset of Example 3.6 (c) (where the relation < 2 <_2 < 2 is chosen to be a total order) yields the formula for the antipode of a fundamental quasisymmetric function ([16 (4.27)] , [13 (5.2.7)] , [2 Theorem 5.1] ).
(d) Let us use the notations of Example 3.3. For any partition λ \lambda λ , let λ t \lambda^t λ t denote the conjugate partition of λ \lambda λ . Let μ \mu μ and λ \lambda λ be two partitions satisfying μ ⊆ λ \mu\subseteq\lambda μ ⊆ λ . Let > 1 >_1 > 1 and > 2 >_2 > 2 be the opposite relations of < 1 <_1 < 1 and < 2 <_2 < 2 . Then, there is a bijection τ : Y ( λ / μ ) → Y ( λ t / μ t ) \tau:Y(\lambda/\mu)\to Y(\lambda^t/\mu^t) τ : Y ( λ / μ ) → Y ( λ t / μ t ) sending each ( i , j ) ∈ Y ( λ / μ ) (i,j)\in Y(\lambda/\mu) ( i , j ) ∈ Y ( λ / μ ) to ( j , i ) (j,i) ( j , i ) . This bijection is an isomorphism of double posets from ( Y ( λ / μ ) , > 1 , < 2 ) (Y(\lambda/\mu),>_1,< _2) ( Y ( λ / μ ) , > 1 , < 2 ) to ( Y ( λ t / μ t ) , > 1 , > 2 ) (Y(\lambda^t/\mu^t),>_1,>_2) ( Y ( λ t / μ t ) , > 1 , > 2 ) (where the notion of an “isomorphism of double posets” is defined in the natural way – i.e., an isomorphism of double posets is a bijection ϕ \phi ϕ between their ground sets such that each of the two maps ϕ \phi ϕ and ϕ − 1 \phi^{-1} ϕ − 1 preserves each of the two orders). Hence,
Γ ( ( Y ( λ / μ ) , > 1 , < 2 ) ) = Γ ( ( Y ( λ t / μ t ) , > 1 , > 2 ) ) . (3) \Gamma((Y(\lambda/\mu),>_1,< _2))=\Gamma((Y(\lambda^t/\mu^t),>_1,>_2)). \tag*{(3)} Γ (( Y ( λ / μ ) , > 1 , < 2 )) = Γ (( Y ( λ t / μ t ) , > 1 , > 2 )) . (3)
But applying Corollary 4.3 to the tertispecial double poset Y ( λ / μ ) Y(\lambda/\mu) Y ( λ / μ ) , we obtain
S ( Γ ( Y ( λ / μ ) ) ) = ( − 1 ) ∣ λ / μ ∣ Γ ( ( Y ( λ / μ ) , > 1 , < 2 ) ) = ( − 1 ) ∣ λ / μ ∣ Γ ( ( Y ( λ t / μ t ) , > 1 , > 2 ) ) (4) S(\Gamma(Y(\lambda/\mu)))=(-1)^{|\lambda/\mu|}\Gamma((Y(\lambda/\mu),>_1,< _2))
=(-1)^{|\lambda/\mu|}\Gamma((Y(\lambda^t/\mu^t),>_1,>_2)) \tag*{(4)} S ( Γ ( Y ( λ / μ ))) = ( − 1 ) ∣ λ / μ ∣ Γ (( Y ( λ / μ ) , > 1 , < 2 )) = ( − 1 ) ∣ λ / μ ∣ Γ (( Y ( λ t / μ t ) , > 1 , > 2 )) (4)
(by (3) ). But from Example 3.6 (d), we know that Γ ( Y ( λ / μ ) ) = s λ / μ \Gamma(Y(\lambda/\mu))=s_{\lambda/\mu} Γ ( Y ( λ / μ )) = s λ / μ . Moreover, a similar argument using [13 Remark 2.2.5] shows that Γ ( ( Y ( λ / μ ) , > 1 , > 2 ) ) = s λ / μ \Gamma((Y(\lambda/\mu),>_1,>_2))=s_{\lambda/\mu} Γ (( Y ( λ / μ ) , > 1 , > 2 )) = s λ / μ . Applying this to λ t \lambda^t λ t and μ t \mu^t μ t instead of λ \lambda λ and μ \mu μ , we obtain Γ ( ( Y ( λ t / μ t ) , > 1 , > 2 ) ) = s λ t / μ t \Gamma((Y(\lambda^t/\mu^t),>_1,>_2))=s_{\lambda^t/\mu^t} Γ (( Y ( λ t / μ t ) , > 1 , > 2 )) = s λ t / μ t . Now, (4) rewrites as
S ( s λ / μ ) = ( − 1 ) ∣ λ / μ ∣ s λ t / μ t (5) S(s_{\lambda/\mu})=(-1)^{|\lambda/\mu|}s_{\lambda^t/\mu^t} \tag*{(5)} S ( s λ / μ ) = ( − 1 ) ∣ λ / μ ∣ s λ t / μ t (5)
(since Γ ( Y ( λ / μ ) ) = s λ / μ \Gamma(Y(\lambda/\mu))=s_{\lambda/\mu} Γ ( Y ( λ / μ )) = s λ / μ and Γ ( ( Y ( λ t / μ t ) , > 1 , > 2 ) ) = s λ t / μ t \Gamma((Y(\lambda^t/\mu^t),>_1,>_2))=s_{\lambda^t/\mu^t} Γ (( Y ( λ t / μ t ) , > 1 , > 2 )) = s λ t / μ t ). This is a well-known formula, and is usually stated for S S S being the antipode of the Hopf algebra of symmetric (rather than quasisymmetric) functions; but this is an equivalent statement, since the latter antipode is a restriction of the antipode of QSym.
It is also possible (but more difficult) to derive (5) by using the double poset Y h ( λ / μ ) Y_{\mathrm{h}}(\lambda/\mu) Y h ( λ / μ ) instead of Y ( λ / μ ) Y(\lambda/\mu) Y ( λ / μ ) . (This boils down to what was done in [13 proof of Corollary 5.2.22] .)
(e) A result of Benedetti and Sagan [2 Theorem 8.2] on the antipodes of immaculate functions can be obtained from Corollary 4.3 using dualization.
Remark 4.9. Corollary 4.3 has a sort of converse. Namely, let us assume that k = Z \mathbf{k} = \mathbb{Z} k = Z . If ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) is a double poset satisfying S ( Γ ( ( E , < 1 , < 2 ) ) ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) ) S\left(\Gamma((E, <_1, <_2))\right) = (-1)^{\lvert E\rvert}\Gamma((E, >_1, <_2)) S ( Γ (( E , < 1 , < 2 )) ) = ( − 1 ) ∣ E ∣ Γ (( E , > 1 , < 2 )) , then ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) is tertispecial.
More precisely, the following holds: Define the length ℓ ( α ) \ell(\alpha) ℓ ( α ) of a composition α \alpha α to be the number of entries of α \alpha α . Define the size ∣ α ∣ \lvert\alpha\rvert ∣ α ∣ of a composition α \alpha α to be the sum of the entries of α \alpha α . Let η : QSym → QSym \eta:\operatorname{QSym} \to\operatorname{QSym} η : QSym → QSym be the k \mathbf{k} k -linear map defined by
η ( M α ) = { M α , if ℓ ( α ) ≥ ∣ α ∣ − 1 ; 0 , if ℓ ( α ) < ∣ α ∣ − 1 \eta(M_\alpha) =
\begin{cases}
M_\alpha, & \text{if } \ell(\alpha) \geq\lvert\alpha\rvert- 1; \\
0, & \text{if } \ell(\alpha) < \lvert\alpha\rvert- 1
\end{cases} η ( M α ) = { M α , 0 , if ℓ ( α ) ≥ ∣ α ∣ − 1 ; if ℓ ( α ) < ∣ α ∣ − 1
for every α ∈ Comp \alpha\in\operatorname{Comp} α ∈ Comp .
Thus, η \eta η transforms a quasisymmetric function by removing all monomials m m m for which the number of indeterminates appearing in m m m is < deg m − 1 < \deg m - 1 < deg m − 1 . We partially order the ring k [ [ x 1 , x 2 , x 3 , … ] ] \mathbf{k}[[x_1,x_2,x_3,\ldots]] k [[ x 1 , x 2 , x 3 , … ]] by a coefficientwise order (i.e., two power series a a a and b b b satisfy a ≤ b a \leq b a ≤ b if and only if each coefficient of a a a is ≤ \leq ≤ to the corresponding coefficient of b b b ). Now, every double poset ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) satisfies
η ( ( − 1 ) ∣ E ∣ S ( Γ ( ( E , < 1 , < 2 ) ) ) ) ≤ η ( Γ ( ( E , > 1 , < 2 ) ) ) , (6) \eta\left((-1)^{\lvert E\rvert}S\left(\Gamma((E, <_1, <_2))\right)\right) \leq\eta\left(\Gamma((E, >_1, <_2))\right), \tag*{(6)} η ( ( − 1 ) ∣ E ∣ S ( Γ (( E , < 1 , < 2 )) ) ) ≤ η ( Γ (( E , > 1 , < 2 )) ) , (6)
and equality holds if and only if the double poset ( E , < 1 , < 2 ) (E, <_1, <_2) ( E , < 1 , < 2 ) is tertispecial. (If we omit η \eta η , then the inequality fails in general.)
The proof of (6) is somewhat technical, but not too hard. A rough outline is given in the detailed version of this paper.
Lemmas: packed E-partitions and comultiplications
We shall now prepare for the proofs of our results. To this end, we introduce the notion of a packed map .
Definition 5.1. (a) An initial interval will mean a set of the form { 1 , 2 , … , ℓ } \{1,2,\ldots,\ell\} { 1 , 2 , … , ℓ } for some ℓ ∈ N \ell\in\mathbb{N} ℓ ∈ N .
(b) If E E E is a set and π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } is a map, then π \pi π is said to be packed if π ( E ) \pi(E) π ( E ) is an initial interval. Clearly, this initial interval must be { 1 , 2 , … , ∣ π ( E ) ∣ } \{1,2,\ldots,|\pi(E)|\} { 1 , 2 , … , ∣ π ( E ) ∣ } .
Proposition 5.2. Let E E E be a finite set. Let π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } be a packed map. Let ℓ = ∣ π ( E ) ∣ \ell=|\pi(E)| ℓ = ∣ π ( E ) ∣ .
(a) We have π ( E ) = { 1 , 2 , … , ℓ } \pi(E)=\{1,2,\ldots,\ell\} π ( E ) = { 1 , 2 , … , ℓ } .
(b) Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map. For each i ∈ { 1 , 2 , … , ℓ } i\in\{1,2,\ldots,\ell\} i ∈ { 1 , 2 , … , ℓ } , define an integer α i \alpha_i α i by
α i = ∑ e ∈ π − 1 ( i ) w ( e ) . \alpha_i=\sum_{e\in\pi^{-1}(i)}w(e). α i = e ∈ π − 1 ( i ) ∑ w ( e ) . Then, ( α 1 , α 2 , … , α ℓ ) (\alpha_1,\alpha_2,\ldots,\alpha_\ell) ( α 1 , α 2 , … , α ℓ ) is a composition.
Proof of Proposition 5.2. This follows from the assumption that π \pi π be packed. (Details are left to the reader.)
Definition 5.3. Let E E E be a finite set. Let π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } be a packed map. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map. Then, the composition ( α 1 , α 2 , … , α ℓ ) (\alpha_1,\alpha_2,\ldots,\alpha_\ell) ( α 1 , α 2 , … , α ℓ ) defined in Proposition 5.2 (b) will be denoted by ev w π \operatorname{ev}_{w}\pi ev w π .
Proposition 5.4. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map. Then,
Γ ( E , w ) = ∑ φ is a packed E -partition M ev w φ . (7) \Gamma(E,w)=\sum_{\varphi\text{ is a packed }E\text{-partition}}M_{\operatorname{ev}_{w}\varphi}. \tag*{(7)} Γ ( E , w ) = φ is a packed E -partition ∑ M ev w φ . (7)
Proof of Proposition 5.4. For every finite subset T T T of { 1 , 2 , 3 , … } \{1,2,3,\ldots\} { 1 , 2 , 3 , … } , there exists a unique strictly increasing bijection { 1 , 2 , … , ∣ T ∣ } → T \{1,2,\ldots,|T|\}\to T { 1 , 2 , … , ∣ T ∣ } → T . We shall denote this bijection by r T r_T r T . For every map π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } , we define the packing of π \pi π as the map r π ( E ) − 1 ∘ π : E → { 1 , 2 , 3 , … } r_{\pi(E)}^{-1}\circ\pi:E\to\{1,2,3,\ldots\} r π ( E ) − 1 ∘ π : E → { 1 , 2 , 3 , … } ; this is a packed map (indeed, its image is { 1 , 2 , … , ∣ π ( E ) ∣ } \{1,2,\ldots,|\pi(E)|\} { 1 , 2 , … , ∣ π ( E ) ∣ } ), and will be denoted by pack π \operatorname{pack}\pi pack π . This map pack π \operatorname{pack}\pi pack π is an E E E -partition if and only if π \pi π is an E E E -partition15 . Hence, pack π \operatorname{pack}\pi pack π is a packed E E E -partition for every E E E -partition π \pi π .
We shall show that for every packed E E E -partition φ \varphi φ , we have
∑ π is an E -partition ; pack π = φ x π , w = M ev w φ . (8) \sum_{\substack{\pi\text{ is an }E\text{-partition};\\ \operatorname{pack}\pi=\varphi}}x_{\pi,w}=M_{\operatorname{ev}_{w}\varphi}. \tag*{(8)} π is an E -partition ; pack π = φ ∑ x π , w = M ev w φ . (8)
( ( pack π ) ( e ) ≤ ( pack π ) ( f ) ) ⟺ ( π ( e ) ≤ π ( f ) ) ((\operatorname{pack}\pi)(e)\leq(\operatorname{pack}\pi)(f))\Longleftrightarrow(\pi(e)\leq\pi(f)) (( pack π ) ( e ) ≤ ( pack π ) ( f )) ⟺ ( π ( e ) ≤ π ( f ))
and
( ( pack π ) ( e ) < ( pack π ) ( f ) ) ⟺ ( π ( e ) < π ( f ) ) ((\operatorname{pack}\pi)(e)<(\operatorname{pack}\pi)(f))\Longleftrightarrow(\pi(e)<\pi(f)) (( pack π ) ( e ) < ( pack π ) ( f )) ⟺ ( π ( e ) < π ( f ))
hold. Hence, pack π \operatorname{pack}\pi pack π is an E E E -partition if and only if π \pi π is an E E E -partition.
Once this is proven, it will follow that
Γ ( E , w ) = ∑ π is an E-partition x π , w = ∑ φ is a packed E-partition ∑ π is an E-partition ; pack π = φ x π , w ⏟ = M ev w φ (by (8)) = ∑ φ is a packed E-partition M ev w φ \begin{aligned}
\Gamma(E,w)
&=\sum_{\pi\text{ is an E-partition}}x_{\pi,w}\\
&=\sum_{\varphi\text{ is a packed E-partition}}
\underbrace{\sum_{\substack{\pi\text{ is an E-partition};\\\operatorname{pack}\pi=\varphi}}x_{\pi,w}}_{=M_{\operatorname{ev}_w\varphi}\ \text{(by (8))}}\\
&=\sum_{\varphi\text{ is a packed E-partition}}M_{\operatorname{ev}_w\varphi}
\end{aligned} Γ ( E , w ) = π is an E-partition ∑ x π , w = φ is a packed E-partition ∑ = M ev w φ (by (8)) π is an E-partition ; pack π = φ ∑ x π , w = φ is a packed E-partition ∑ M ev w φ
(since pack π \operatorname{pack}\pi pack π is a packed E-partition for every E-partition π \pi π )
and Proposition 5.4 will be proven.
So it remains to prove (8). Let φ \varphi φ be a packed E-partition. Let ℓ = ∣ φ ( E ) ∣ \ell=|\varphi(E)| ℓ = ∣ φ ( E ) ∣ ; thus φ ( E ) = { 1 , 2 , … , ℓ } \varphi(E)=\{1,2,\ldots,\ell\} φ ( E ) = { 1 , 2 , … , ℓ } (since φ \varphi φ is packed). Let α i = ∑ e ∈ φ − 1 ( i ) w ( e ) \alpha_i=\sum_{e\in\varphi^{-1}(i)}w(e) α i = ∑ e ∈ φ − 1 ( i ) w ( e ) for every i ∈ { 1 , 2 , … , ℓ } i\in\{1,2,\ldots,\ell\} i ∈ { 1 , 2 , … , ℓ } ; thus, ev w φ = ( α 1 , α 2 , … , α ℓ ) \operatorname{ev}_w\varphi=(\alpha_1,\alpha_2,\ldots,\alpha_\ell) ev w φ = ( α 1 , α 2 , … , α ℓ ) (by the definition of ev w φ \operatorname{ev}_w\varphi ev w φ ). Hence, the definition of M ev w φ M_{\operatorname{ev}_w\varphi} M ev w φ yields
M ev w φ = ∑ i 1 < i 2 < ⋯ < i ℓ x i 1 α 1 x i 2 α 2 ⋯ x i ℓ α ℓ = ∑ i 1 < i 2 < ⋯ < i ℓ ∏ k = 1 ℓ x i k α k = ∑ i 1 < i 2 < ⋯ < i ℓ ∏ k = 1 ℓ x i k ∑ e ∈ φ − 1 ( k ) w ( e ) = ∑ i 1 < i 2 < ⋯ < i ℓ ∏ k = 1 ℓ ∏ e ∈ E ; φ ( e ) = k x i k w ( e ) = ∑ i 1 < i 2 < ⋯ < i ℓ ∏ k = 1 ℓ ∏ e ∈ E ; φ ( e ) = k x i φ ( e ) w ( e ) = ∑ i 1 < i 2 < ⋯ < i ℓ ∏ e ∈ E x i φ ( e ) w ( e ) = ∑ T ⊆ { 1 , 2 , 3 , … } ; ∣ T ∣ = ℓ ∏ e ∈ E x r T ( φ ( e ) ) w ( e ) . \begin{aligned}
M_{\operatorname{ev}_w\varphi}
&=\sum_{i_1<i_2<\cdots<i_\ell}x_{i_1}^{\alpha_1}x_{i_2}^{\alpha_2}\cdots x_{i_\ell}^{\alpha_\ell}
=\sum_{i_1<i_2<\cdots<i_\ell}\prod_{k=1}^{\ell}x_{i_k}^{\alpha_k}\\
&=\sum_{i_1<i_2<\cdots<i_\ell}\prod_{k=1}^{\ell}
x_{i_k}^{\sum_{e\in\varphi^{-1}(k)}w(e)}
=\sum_{i_1<i_2<\cdots<i_\ell}\prod_{k=1}^{\ell}\prod_{\substack{e\in E;\\\varphi(e)=k}}x_{i_k}^{w(e)}\\
&=\sum_{i_1<i_2<\cdots<i_\ell}\prod_{k=1}^{\ell}\prod_{\substack{e\in E;\\\varphi(e)=k}}x_{i_{\varphi(e)}}^{w(e)}
=\sum_{i_1<i_2<\cdots<i_\ell}\prod_{e\in E}x_{i_{\varphi(e)}}^{w(e)}\\
&=\sum_{\substack{T\subseteq\{1,2,3,\ldots\};\\|T|=\ell}}\prod_{e\in E}x_{r_T(\varphi(e))}^{w(e)}.
\end{aligned} M ev w φ = i 1 < i 2 < ⋯ < i ℓ ∑ x i 1 α 1 x i 2 α 2 ⋯ x i ℓ α ℓ = i 1 < i 2 < ⋯ < i ℓ ∑ k = 1 ∏ ℓ x i k α k = i 1 < i 2 < ⋯ < i ℓ ∑ k = 1 ∏ ℓ x i k ∑ e ∈ φ − 1 ( k ) w ( e ) = i 1 < i 2 < ⋯ < i ℓ ∑ k = 1 ∏ ℓ e ∈ E ; φ ( e ) = k ∏ x i k w ( e ) = i 1 < i 2 < ⋯ < i ℓ ∑ k = 1 ∏ ℓ e ∈ E ; φ ( e ) = k ∏ x i φ ( e ) w ( e ) = i 1 < i 2 < ⋯ < i ℓ ∑ e ∈ E ∏ x i φ ( e ) w ( e ) = T ⊆ { 1 , 2 , 3 , … } ; ∣ T ∣ = ℓ ∑ e ∈ E ∏ x r T ( φ ( e )) w ( e ) .
Hence,
M Ev w φ = ∑ T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∏ e ∈ E x r T ( φ ( e ) ) w ( e ) = ∑ T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ x r T ∘ φ , w . (9) M_{\operatorname{Ev}_{w}}\varphi
=
\sum_{\substack{T\subseteq\{1,2,3,\ldots\}\\ |T|=\ell}}
\prod_{e\in E}x_{r_T(\varphi(e))}^{w(e)}
=
\sum_{\substack{T\subseteq\{1,2,3,\ldots\}\\ |T|=\ell}}x_{r_T\circ\varphi,w}. \tag*{(9)} M Ev w φ = T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ e ∈ E ∏ x r T ( φ ( e )) w ( e ) = T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ x r T ∘ φ , w . (9)
On the other hand, recall that φ \varphi φ is an E E E -partition. Hence, every map π \pi π satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ is an E E E -partition (because, as we know, pack π \operatorname{pack}\pi pack π is an E E E -partition if and only if π \pi π is an E E E -partition). Thus, the E E E -partitions π \pi π satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ are precisely the maps π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ . Hence,
∑ π is an E -partition pack π = φ x π , w = ∑ π : E → { 1 , 2 , 3 , … } pack π = φ x π , w = ∑ T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ π : E → { 1 , 2 , 3 , … } pack π = φ ; π ( E ) = T x π , w \begin{aligned}
\sum_{\substack{\pi\text{ is an }E\text{-partition}\\ \operatorname{pack}\pi=\varphi}}x_{\pi,w}
=
\sum_{\substack{\pi:E\to\{1,2,3,\ldots\}\\ \operatorname{pack}\pi=\varphi}}x_{\pi,w} \\
&=
\sum_{\substack{T\subseteq\{1,2,3,\ldots\}\\ |T|=\ell}}
\ \sum_{\substack{\pi:E\to\{1,2,3,\ldots\}\\ \operatorname{pack}\pi=\varphi;\ \pi(E)=T}}x_{\pi,w}
\end{aligned} π is an E -partition pack π = φ ∑ x π , w = π : E → { 1 , 2 , 3 , … } pack π = φ ∑ x π , w = T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ π : E → { 1 , 2 , 3 , … } pack π = φ ; π ( E ) = T ∑ x π , w
(because if π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } is a map satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ , then ∣ π ( E ) ∣ = ℓ |\pi(E)|=\ell ∣ π ( E ) ∣ = ℓ ). But for every ℓ \ell ℓ -element subset T T T of { 1 , 2 , 3 , … } \{1,2,3,\ldots\} { 1 , 2 , 3 , … } , there exists exactly one π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ and π ( E ) = T \pi(E)=T π ( E ) = T : namely, π = r T ∘ φ \pi=r_T\circ\varphi π = r T ∘ φ .
Claim 1: The map r T ∘ φ r_T\circ\varphi r T ∘ φ is a map π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ and π ( E ) = T \pi(E)=T π ( E ) = T .
Claim 2: If π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } is a map satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ and π ( E ) = T \pi(E)=T π ( E ) = T , then π = r T ∘ φ \pi=r_T\circ\varphi π = r T ∘ φ .
Proof of Claim 1. We have ∣ T ∣ = ℓ |T|=\ell ∣ T ∣ = ℓ (since the set T T T is ℓ \ell ℓ -element), thus ℓ = ∣ T ∣ \ell=|T| ℓ = ∣ T ∣ . We have
( r T ∘ φ ) ( E ) = r T ( φ ( E ) ) = r T ( { 1 , 2 , … , ℓ } ) = r T ( { 1 , 2 , … , ∣ T ∣ } ) = T (r_T\circ\varphi)(E)
=
r_T\left(\varphi(E)\right)
=
r_T\left(\{1,2,\ldots,\ell\}\right)
=
r_T\left(\{1,2,\ldots,|T|\}\right)
=
T ( r T ∘ φ ) ( E ) = r T ( φ ( E ) ) = r T ( { 1 , 2 , … , ℓ } ) = r T ( { 1 , 2 , … , ∣ T ∣ } ) = T
(by the definition of r T r_T r T ). Now, the definition of pack ( r T ∘ φ ) \operatorname{pack}(r_T\circ\varphi) pack ( r T ∘ φ ) shows that
pack ( r T ∘ φ ) = r ( r T ∘ φ ) ( E ) − 1 ∘ ( r T ∘ φ ) = r T − 1 ∘ ( r T ∘ φ ) \operatorname{pack}(r_T\circ\varphi)
=
r_{(r_T\circ\varphi)(E)}^{-1}\circ(r_T\circ\varphi)
=
r_T^{-1}\circ(r_T\circ\varphi) pack ( r T ∘ φ ) = r ( r T ∘ φ ) ( E ) − 1 ∘ ( r T ∘ φ ) = r T − 1 ∘ ( r T ∘ φ )
(since ( r T ∘ φ ) ( E ) = T (r_T\circ\varphi)(E)=T ( r T ∘ φ ) ( E ) = T )
Therefore, for every ℓ \ell ℓ -element subset T T T of { 1 , 2 , 3 , … } \{1,2,3,\ldots\} { 1 , 2 , 3 , … } , we have
∑ π : E → { 1 , 2 , 3 , … } pack π = φ ; π ( E ) = T x π , w = x r T ∘ φ , w . \sum_{\substack{\pi:E\to\{1,2,3,\ldots\}\\ \operatorname{pack}\pi=\varphi;\ \pi(E)=T}}x_{\pi,w}=x_{r_T\circ\varphi,w}. π : E → { 1 , 2 , 3 , … } pack π = φ ; π ( E ) = T ∑ x π , w = x r T ∘ φ , w .
Hence,
∑ π is an E -partition ; pack π = φ x π , w = ∑ T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ π : E → { 1 , 2 , 3 , … } pack π = φ ; π ( E ) = T x π , w = ∑ T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ x r T ∘ φ , w = M E v w φ \sum_{\substack{\pi\text{ is an }E\text{-partition};\ \operatorname{pack}\pi=\varphi}}x_{\pi,w}
=
\sum_{\substack{T\subseteq\{1,2,3,\ldots\}\\ |T|=\ell}}
\sum_{\substack{\pi:E\to\{1,2,3,\ldots\}\\ \operatorname{pack}\pi=\varphi;\ \pi(E)=T}}x_{\pi,w}
=
\sum_{\substack{T\subseteq\{1,2,3,\ldots\}\\ |T|=\ell}}x_{r_T\circ\varphi,w}
=M_{E v w}\varphi π is an E -partition ; pack π = φ ∑ x π , w = T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ π : E → { 1 , 2 , 3 , … } pack π = φ ; π ( E ) = T ∑ x π , w = T ⊆ { 1 , 2 , 3 , … } ∣ T ∣ = ℓ ∑ x r T ∘ φ , w = M E v w φ
(by (9)). Thus, (8) is proven, and with it Proposition 5.4.
Proof of Proposition 3.5. Proposition 3.5 follows immediately from Proposition 5.4 (since M α ∈ QSym M_\alpha\in\operatorname{QSym} M α ∈ QSym for every composition α \alpha α ).
We shall now describe the coproduct of Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) , essentially giving the proof that is left to the reader in [19 Theorem 2.2] .
Definition 5.5. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset.
(a) Then, Adm E \operatorname{Adm}E Adm E will mean the set of all pairs ( P , Q ) (P,Q) ( P , Q ) , where P P P and Q Q Q are subsets of E E E satisfying P ∩ Q = ∅ P\cap Q=\varnothing P ∩ Q = ∅ and P ∪ Q = E P\cup Q=E P ∪ Q = E and having the property that no p ∈ P p\in P p ∈ P and q ∈ Q q\in Q q ∈ Q satisfy q < 1 p q<_{1}p q < 1 p . These pairs ( P , Q ) (P,Q) ( P , Q ) are called the admissible partitions of E E E . (In the terminology of [19 ] , they are the decompositions of ( E , < 1 ) (E,<_{1}) ( E , < 1 ) .)
(b) For any subset T T T of E E E , we let E ∣ T E\mid_T E ∣ T denote the double poset ( T , < 1 , < 2 ) (T,<_{1},<_{2}) ( T , < 1 , < 2 ) , where < 1 <_{1} < 1 and < 2 <_{2} < 2 (by abuse of notation) denote the restrictions of the relations < 1 <_{1} < 1 and < 2 <_{2} < 2 to T T T .
Proposition 5.6. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map. Then,
Δ ( Γ ( E , w ) ) = ∑ ( P , Q ) ∈ Adm E Γ ( E ∣ P , w ∣ P ) ⊗ Γ ( E ∣ Q , w ∣ Q ) (10) \Delta\left(\Gamma(E,w)\right)=\sum_{(P,Q)\in\operatorname{Adm}E}\Gamma\left(E\mid_P,w\mid_P\right)\otimes\Gamma\left(E\mid_Q,w\mid_Q\right) \tag*{(10)} Δ ( Γ ( E , w ) ) = ( P , Q ) ∈ Adm E ∑ Γ ( E ∣ P , w ∣ P ) ⊗ Γ ( E ∣ Q , w ∣ Q ) (10)
Thus, the map r T ∘ φ : E → { 1 , 2 , 3 , … } r_T\circ\varphi:E\to\{1,2,3,\ldots\} r T ∘ φ : E → { 1 , 2 , 3 , … } satisfies pack ( r T ∘ φ ) = φ \operatorname{pack}(r_T\circ\varphi)=\varphi pack ( r T ∘ φ ) = φ and ( r T ∘ φ ) ( E ) = T (r_T\circ\varphi)(E)=T ( r T ∘ φ ) ( E ) = T . In other words, r T ∘ φ r_T\circ\varphi r T ∘ φ is a map π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ and π ( E ) = T \pi(E)=T π ( E ) = T . This proves Claim 1.
Proof of Claim 2. Let π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } be a map satisfying pack π = φ \operatorname{pack}\pi=\varphi pack π = φ and π ( E ) = T \pi(E)=T π ( E ) = T . The definition of pack π \operatorname{pack}\pi pack π shows that pack π = r π ( E ) − 1 ∘ π = r T − 1 ∘ π \operatorname{pack}\pi=r_{\pi(E)}^{-1}\circ\pi=r_T^{-1}\circ\pi pack π = r π ( E ) − 1 ∘ π = r T − 1 ∘ π (since π ( E ) = T \pi(E)=T π ( E ) = T ). Hence, r T − 1 ∘ π = pack π = φ r_T^{-1}\circ\pi=\operatorname{pack}\pi=\varphi r T − 1 ∘ π = pack π = φ , so that π = r T ∘ φ \pi=r_T\circ\varphi π = r T ∘ φ . This proves Claim 2.
Now, both Claims 1 and 2 are proven; hence, our proof is complete.
A particular case of Proposition 5.6 (namely, the case when w ( e ) = 1 w(e)=1 w ( e ) = 1 for each e ∈ E e\in E e ∈ E ) appears in [16 Théorème 4.16] .
The proof of Proposition 5.6 relies on a simple bijection that an experienced combinatorialist will have no trouble finding (and proving even less); let us just give a brief outline of the argument.19
Proof of Proposition 5.6. Whenever α = ( α 1 , α 2 , … , α ℓ ) \alpha=(\alpha_1,\alpha_2,\ldots,\alpha_\ell) α = ( α 1 , α 2 , … , α ℓ ) is a composition and k ∈ { 0 , 1 , … , ℓ } k\in\{0,1,\ldots,\ell\} k ∈ { 0 , 1 , … , ℓ } , we introduce the notation α [ : k ] \alpha[:k] α [ : k ] for the composition ( α 1 , α 2 , … , α k ) (\alpha_1,\alpha_2,\ldots,\alpha_k) ( α 1 , α 2 , … , α k ) , and the notation α [ k : ] \alpha[k:] α [ k : ] for the composition ( α k + 1 , α k + 2 , … , α ℓ ) (\alpha_{k+1},\alpha_{k+2},\ldots,\alpha_\ell) ( α k + 1 , α k + 2 , … , α ℓ ) . Now, the formula (1) can be rewritten as follows:
Δ ( M α ) = ∑ k = 0 ℓ M α [ : k ] ⊗ M α [ k : ] (11) \Delta(M_\alpha)=\sum_{k=0}^{\ell}M_{\alpha[:k]}\otimes M_{\alpha[k:]} \tag*{(11)} Δ ( M α ) = k = 0 ∑ ℓ M α [ : k ] ⊗ M α [ k : ] (11)
for every ℓ ∈ N \ell\in\mathbb{N} ℓ ∈ N and every composition α \alpha α with ℓ \ell ℓ entries.
Now, applying Δ \Delta Δ to the equality (7) yields
Δ ( Γ ( E , w ) ) = ∑ φ is a packed E -partition Δ ( M ev w φ ) = ∑ φ is a packed E -partition ∑ k = 0 ∣ φ ( E ) ∣ M ( ev w φ ) [ : k ] ⊗ M ( ev w φ ) [ k : ] (by (11)) = ∑ φ is a packed E -partition ∑ k = 0 ∣ φ ( E ) ∣ M ( ev w φ ) [ : k ] ⊗ M ( ev w φ ) [ k : ] . (12) \begin{aligned}
\Delta(\Gamma(E,w))=\sum_{\substack{\varphi\text{ is a packed}\\E\text{-partition}}}\Delta(M_{\operatorname{ev}_{w}\varphi}) \\
&=\sum_{\substack{\varphi\text{ is a packed}\\E\text{-partition}}}\sum_{k=0}^{|\varphi(E)|}M_{(\operatorname{ev}_{w}\varphi)[:k]}\otimes M_{(\operatorname{ev}_{w}\varphi)[k:]}
\qquad\text{(by (11))} \\
&=\sum_{\substack{\varphi\text{ is a packed}\\E\text{-partition}}}\sum_{k=0}^{|\varphi(E)|}M_{(\operatorname{ev}_{w}\varphi)[:k]}\otimes M_{(\operatorname{ev}_{w}\varphi)[k:]}. \tag*{(12)}
\end{aligned} Δ ( Γ ( E , w )) = φ is a packed E -partition ∑ Δ ( M ev w φ ) = φ is a packed E -partition ∑ k = 0 ∑ ∣ φ ( E ) ∣ M ( ev w φ ) [ : k ] ⊗ M ( ev w φ ) [ k : ] (by (11)) = φ is a packed E -partition ∑ k = 0 ∑ ∣ φ ( E ) ∣ M ( ev w φ ) [ : k ] ⊗ M ( ev w φ ) [ k : ] . (12)
On the other hand, rewriting each of the tensorands on the right hand side of (10) using (7), we obtain
∑ ( P , Q ) ∈ Adm E Γ ( E ∣ P , w ∣ P ) ⊗ Γ ( E ∣ Q , w ∣ Q ) = ∑ ( P , Q ) ∈ Adm E ( ∑ φ is a packed E ∣ P -partition M ev w ∣ P φ ) ⊗ ( ∑ φ is a packed E ∣ Q -partition M ev w ∣ Q φ ) = ∑ ( P , Q ) ∈ Adm E ( ∑ σ is a packed E ∣ P -partition M ev w ∣ P σ ) ⊗ ( ∑ τ is a packed E ∣ Q -partition M ev w ∣ Q τ ) = ∑ ( P , Q ) ∈ Adm E ∑ σ is a packed E ∣ P -partition τ is a packed E ∣ Q -partition M ev w ∣ P σ ⊗ M ev w ∣ Q τ . \begin{aligned}
\sum_{(P,Q)\in\operatorname{Adm}E}\Gamma(E|_P,w|_P)\otimes\Gamma(E|_Q,w|_Q) \\
&=\sum_{(P,Q)\in\operatorname{Adm}E}
\left(\sum_{\substack{\varphi\text{ is a packed}\\E|_P\text{-partition}}}M_{\operatorname{ev}_{w|_P}\varphi}\right)
\otimes
\left(\sum_{\substack{\varphi\text{ is a packed}\\E|_Q\text{-partition}}}M_{\operatorname{ev}_{w|_Q}\varphi}\right) \\
&=\sum_{(P,Q)\in\operatorname{Adm}E}
\left(\sum_{\substack{\sigma\text{ is a packed}\\E|_P\text{-partition}}}M_{\operatorname{ev}_{w|_P}\sigma}\right)
\otimes
\left(\sum_{\substack{\tau\text{ is a packed}\\E|_Q\text{-partition}}}M_{\operatorname{ev}_{w|_Q}\tau}\right) \\
&=\sum_{(P,Q)\in\operatorname{Adm}E}
\sum_{\substack{\sigma\text{ is a packed }E|_P\text{-partition}\\\tau\text{ is a packed }E|_Q\text{-partition}}}
M_{\operatorname{ev}_{w|_P}\sigma}\otimes M_{\operatorname{ev}_{w|_Q}\tau}.
\end{aligned} ( P , Q ) ∈ Adm E ∑ Γ ( E ∣ P , w ∣ P ) ⊗ Γ ( E ∣ Q , w ∣ Q ) = ( P , Q ) ∈ Adm E ∑ φ is a packed E ∣ P -partition ∑ M ev w ∣ P φ ⊗ φ is a packed E ∣ Q -partition ∑ M ev w ∣ Q φ = ( P , Q ) ∈ Adm E ∑ σ is a packed E ∣ P -partition ∑ M ev w ∣ P σ ⊗ τ is a packed E ∣ Q -partition ∑ M ev w ∣ Q τ = ( P , Q ) ∈ Adm E ∑ σ is a packed E ∣ P -partition τ is a packed E ∣ Q -partition ∑ M ev w ∣ P σ ⊗ M ev w ∣ Q τ .
We need to prove that the right hand sides of this equality and of (12) are equal (because then, it will follow that so are the left hand sides, and thus Proposition 5.6 will be proven). For this, it is clearly enough to exhibit a bijection between
the pairs ( φ , k ) (\varphi,k) ( φ , k ) consisting of a packed E-partition φ \varphi φ and a k ∈ { 0 , 1 , … , ∣ φ ( E ) ∣ } k \in\{0,1,\ldots,|\varphi(E)|\} k ∈ { 0 , 1 , … , ∣ φ ( E ) ∣ }
and
the triples ( ( P , Q ) , σ , τ ) ((P,Q),\sigma,\tau) (( P , Q ) , σ , τ ) consisting of a ( P , Q ) ∈ Adm E (P,Q) \in\operatorname{Adm} E ( P , Q ) ∈ Adm E , a packed E ∣ P E\mid_P E ∣ P -partition σ \sigma σ and a packed E ∣ Q E\mid_Q E ∣ Q -partition τ \tau τ
which bijection has the property that whenever it maps ( φ , k ) (\varphi,k) ( φ , k ) to ( ( P , Q ) , σ , τ ) ((P,Q),\sigma,\tau) (( P , Q ) , σ , τ ) , we have the equalities ( ev w φ ) [ : k ] = ev w ∣ P σ (\operatorname{ev}_w\varphi)[:k]=\operatorname{ev}_{w\mid_P}\sigma ( ev w φ ) [ : k ] = ev w ∣ P σ and ( ev w φ ) [ k : ] = ev w ∣ Q τ (\operatorname{ev}_w\varphi)[k:]=\operatorname{ev}_{w\mid_Q}\tau ( ev w φ ) [ k : ] = ev w ∣ Q τ . Such a bijection is easy to construct: Given ( φ , k ) (\varphi,k) ( φ , k ) , it sets P = φ − 1 ( { 1 , 2 , … , k } ) P=\varphi^{-1}(\{1,2,\ldots,k\}) P = φ − 1 ({ 1 , 2 , … , k }) , Q = φ − 1 ( { k + 1 , k + 2 , … , ∣ φ ( E ) ∣ } ) Q=\varphi^{-1}(\{k+1,k+2,\ldots,|\varphi(E)|\}) Q = φ − 1 ({ k + 1 , k + 2 , … , ∣ φ ( E ) ∣ }) , σ = φ ∣ P \sigma=\varphi\mid_P σ = φ ∣ P and τ = pack ( φ ∣ Q ) \tau=\operatorname{pack}(\varphi\mid_Q) τ = pack ( φ ∣ Q ) .20 Conversely, given ( ( P , Q ) , σ , τ ) ((P,Q),\sigma,\tau) (( P , Q ) , σ , τ ) , the inverse bijection sets k = ∣ σ ( P ) ∣ k=|\sigma(P)| k = ∣ σ ( P ) ∣ and constructs φ \varphi φ as the map E → { 1 , 2 , 3 , … } E\to\{1,2,3,\ldots\} E → { 1 , 2 , 3 , … } which sends every e ∈ E e\in E e ∈ E to { σ ( e ) , if e ∈ P ; τ ( e ) + k , if e ∈ Q . \begin{cases}\sigma(e),&\text{if }e\in P;\\ \tau(e)+k,&\text{if }e\in Q.\end{cases} { σ ( e ) , τ ( e ) + k , if e ∈ P ; if e ∈ Q . Proving that this alleged bijection and its alleged inverse bijection are well-defined and actually mutually inverse is straightforward and left to the reader.21 □
Claim 1: Every e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E satisfying e < 1 f e<_{1}f e < 1 f satisfy φ ( e ) ≤ φ ( f ) \varphi(e)\le\varphi(f) φ ( e ) ≤ φ ( f ) .
Claim 2: Every e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E satisfying e < 1 f e<_{1}f e < 1 f and f < 2 e f<_{2}e f < 2 e satisfy φ ( e ) < φ ( f ) \varphi(e)<\varphi(f) φ ( e ) < φ ( f ) .
We shall only prove Claim 1 (as the proof of Claim 2 is similar). So let e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E be such that e < 1 f e<_{1}f e < 1 f . We need to show that φ ( e ) ≤ φ ( f ) \varphi(e)\le\varphi(f) φ ( e ) ≤ φ ( f ) . We are in one of the following four cases:
Case 1: We have e ∈ P e\in P e ∈ P and f ∈ P f\in P f ∈ P .
Case 2: We have e ∈ P e\in P e ∈ P and f ∈ Q f\in Q f ∈ Q .
Case 3: We have e ∈ Q e\in Q e ∈ Q and f ∈ P f\in P f ∈ P .
Case 4: We have e ∈ Q e\in Q e ∈ Q and f ∈ Q f\in Q f ∈ Q .
In Case 1, our claim φ ( e ) ≤ φ ( f ) \varphi(e)\le\varphi(f) φ ( e ) ≤ φ ( f ) follows from the assumption that σ \sigma σ is an E ∣ P E\mid_P E ∣ P -partition (because in Case 1, we have φ ( e ) = σ ( e ) \varphi(e)=\sigma(e) φ ( e ) = σ ( e ) and φ ( f ) = σ ( f ) \varphi(f)=\sigma(f) φ ( f ) = σ ( f ) ). In Case 4, it follows from the assumption that τ \tau τ is an E ∣ Q E\mid_Q E ∣ Q -partition (since in Case 4, we have φ ( e ) = τ ( e ) + k \varphi(e)=\tau(e)+k φ ( e ) = τ ( e ) + k and φ ( f ) = τ ( f ) + k \varphi(f)=\tau(f)+k φ ( f ) = τ ( f ) + k ). In Case 2, it clearly holds (indeed, if e ∈ P e\in P e ∈ P , then the definition of φ \varphi φ yields φ ( e ) = σ ( e ) ≤ k \varphi(e)=\sigma(e)\le k φ ( e ) = σ ( e ) ≤ k , and if f ∈ Q f\in Q f ∈ Q , then the definition of φ \varphi φ yields φ ( f ) = τ ( f ) + k > k \varphi(f)=\tau(f)+k>k φ ( f ) = τ ( f ) + k > k ; in Case 2, we have φ ( e ) ≤ k < φ ( f ) \varphi(e)\le k<\varphi(f) φ ( e ) ≤ k < φ ( f ) ). Finally, Case 3 is impossible (because having e ∈ Q e\in Q e ∈ Q and f ∈ P f\in P f ∈ P and e < 1 f e<_{1}f e < 1 f would contradict ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E ). Thus, we have proven the claim in each of the four cases, and consequently Claim 1 is proven. As we have said above, Claim 2 is proven similarly.
defined to be u u u on the subset E E E of E F EF E F , and v v v on the subset F F F of E F EF E F . Here, E F EF E F is a double poset defined as in [19 §2.1] . Combined with Proposition 3.5, this fact gives a combinatorial proof for the fact that QSym is a k k k -algebra, as well as for some standard formulas for multiplications of quasisymmetric functions; similarly, Proposition 5.6 can be used to derive the well-known formulas for Δ M α \Delta M_{\alpha} Δ M α , Δ L α \Delta L_{\alpha} Δ L α , Δ s λ / μ \Delta s_{\lambda/\mu} Δ s λ / μ etc. (although, of course, we have already used the formula for Δ M α \Delta M_{\alpha} Δ M α in our proof of Proposition 5.6).
Proof of Theorem 4.2
Before we come to the proof of Theorem 4.2, let us state five lemmas:
Lemma 6.1. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset. Let P P P and Q Q Q be subsets of E E E such that P ∩ Q = ∅ P\cap Q=\varnothing P ∩ Q = ∅ and P ∪ Q = E P\cup Q=E P ∪ Q = E . Assume that there exist no p ∈ P p\in P p ∈ P and q ∈ Q q\in Q q ∈ Q such that q q q is < 1 <_{1} < 1 -covered by p p p . Then, ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E .
Proof of Lemma 6.1. For any a ∈ E a\in E a ∈ E and b ∈ E b\in E b ∈ E , we let [ a , b ] [a,b] [ a , b ] denote the subset { e ∈ E ∣ a < 1 e < 1 b } \{e\in E\mid a<_{1}e<_{1}b\} { e ∈ E ∣ a < 1 e < 1 b } of E E E . It is easy to see that if a a a , b b b and c c c are three elements of E E E satisfying a < 1 c < 1 b a<_{1}c<_{1}b a < 1 c < 1 b , then both [ a , c ] [a,c] [ a , c ] and [ c , b ] [c,b] [ c , b ] are proper subsets of [ a , b ] [a,b] [ a , b ] , and therefore
both numbers ∣ [ a , c ] ∣ and ∣ [ c , b ] ∣ are smaller than ∣ [ a , b ] ∣ . (13) \text{both numbers } |[a,c]| \text{ and } |[c,b]| \text{ are smaller than } |[a,b]|. \tag*{(13)} both numbers ∣ [ a , c ] ∣ and ∣ [ c , b ] ∣ are smaller than ∣ [ a , b ] ∣. (13)
A pair ( p , q ) ∈ P × Q (p,q)\in P\times Q ( p , q ) ∈ P × Q is said to be a malposition if it satisfies q < 1 p q<_{1}p q < 1 p . Now, let us assume (for the sake of contradiction) that there exists a malposition. Fix a malposition ( u , v ) (u,v) ( u , v ) for which the value ∣ [ v , u ] ∣ |[v,u]| ∣ [ v , u ] ∣ is minimum. Thus, ( u , v ) ∈ P × Q (u,v)\in P\times Q ( u , v ) ∈ P × Q and v < 1 u v<_{1}u v < 1 u . From ( u , v ) ∈ P × Q (u,v)\in P\times Q ( u , v ) ∈ P × Q , we obtain u ∈ P u\in P u ∈ P and v ∈ Q v\in Q v ∈ Q . Hence, v v v is not < 1 <_{1} < 1 -covered by u u u (since there exist no p ∈ P p\in P p ∈ P and q ∈ Q q\in Q q ∈ Q such that q q q is < 1 <_{1} < 1 -covered by p p p ). Hence, there exists a w ∈ E w\in E w ∈ E such that v < 1 w < 1 u v<_{1}w<_{1}u v < 1 w < 1 u (since v < 1 u v<_{1}u v < 1 u ). Consider this w w w . Applying (13) to a = v a=v a = v , c = w c=w c = w and b = u b=u b = u , we see that both numbers ∣ [ v , w ] ∣ |[v,w]| ∣ [ v , w ] ∣ and ∣ [ w , u ] ∣ |[w,u]| ∣ [ w , u ] ∣ are smaller than ∣ [ v , u ] ∣ |[v,u]| ∣ [ v , u ] ∣ , and therefore neither ( w , v ) (w,v) ( w , v ) nor ( u , w ) (u,w) ( u , w ) is a malposition (since we picked ( u , v ) (u,v) ( u , v ) to be a malposition with minimum ∣ [ v , u ] ∣ |[v,u]| ∣ [ v , u ] ∣ ). But w ∈ E = P ∪ Q w\in E=P\cup Q w ∈ E = P ∪ Q , so that either w ∈ P w\in P w ∈ P or w ∈ Q w\in Q w ∈ Q . If w ∈ P w\in P w ∈ P , then ( w , v ) (w,v) ( w , v ) is a malposition; if w ∈ Q w\in Q w ∈ Q , then ( u , w ) (u,w) ( u , w ) is a malposition. In either case, we obtain a contradiction to the fact that neither ( w , v ) (w,v) ( w , v ) nor ( u , w ) (u,w) ( u , w ) is a malposition. This contradiction shows that our assumption was wrong. Hence, there exists no malposition. In other words, there exists no ( p , q ) ∈ P × Q (p,q)\in P\times Q ( p , q ) ∈ P × Q satisfying q < 1 p q<_{1}p q < 1 p (since this is what “malposition” means). In other words, no p ∈ P p\in P p ∈ P and q ∈ Q q\in Q q ∈ Q satisfy q < 1 p q<_{1}p q < 1 p . Consequently, ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E . This proves Lemma 6.1.
Lemma 6.2. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset. Let ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E . Then, E ∣ P E|_{P} E ∣ P is a tertispecial double poset.
Proof of Lemma 6.2. Recall that we are using the symbol < 1 <_{1} < 1 to denote two different relations: a strict partial order on E E E , and its restriction to P P P . This abuse of notation is usually harmless, but in the current proof it is dangerous, because it causes the statement “a a a is < 1 <_{1} < 1 -covered by b b b ” (for two elements a a a and b b b of P P P ) to carry two meanings (depending on whether the symbol < 1 <_{1} < 1 is interpreted as the strict partial order on E E E , or as its restriction to P P P ). (These two meanings are actually equivalent, but their equivalence is not immediately obvious.)
Thus, for the duration of this proof, we shall revert to a less ambiguous notation. Namely, the notation < 1 <_{1} < 1 shall only be used for the strict partial order on E E E which constitutes part of the double poset E E E . The restriction of this partial order < 1 <_{1} < 1 to the subset P P P will be denoted by < 1 , P <_{1,P} < 1 , P (not by < 1 <_{1} < 1 ). Similarly, the restriction of the partial order < 2 <_{2} < 2 to the subset P P P will be denoted by < 2 , P <_{2,P} < 2 , P (not by < 2 <_{2} < 2 ). Thus, the double poset E ∣ P E|_{P} E ∣ P is defined as E ∣ P = ( P , < 1 , P , < 2 , P ) E|_{P}=(P,<_{1,P},<_{2,P}) E ∣ P = ( P , < 1 , P , < 2 , P ) .
We need to show that the double poset E ∣ P = ( P , < 1 , P , < 2 , P ) E|_{P}=(P,<_{1,P},<_{2,P}) E ∣ P = ( P , < 1 , P , < 2 , P ) is tertispecial. In other words, we need to show that if a a a and b b b are two elements of P P P such that a a a is < 1 , P <_{1,P} < 1 , P -covered by b b b , then a a a and b b b are < 2 , P <_{2,P} < 2 , P -comparable.
Let a a a and b b b be two elements of P P P such that a a a is < 1 , P <_{1,P} < 1 , P -covered by b b b . Thus, a < 1 , P b a<_{1,P}b a < 1 , P b , and
there exists no c ∈ P satisfying a < 1 , P c < 1 , P b . (14) \text{there exists no }c\in P\text{ satisfying }a<_{1,P}c<_{1,P}b. \tag*{(14)} there exists no c ∈ P satisfying a < 1 , P c < 1 , P b . (14)
We have a < 1 , P b a<_{1,P}b a < 1 , P b . In other words, a < 1 b a<_{1}b a < 1 b (since < 1 , P <_{1,P} < 1 , P is the restriction of the relation < 1 <_{1} < 1 to P P P ).
Now, if c ∈ E c\in E c ∈ E is such that a < 1 c < 1 b a<_{1}c<_{1}b a < 1 c < 1 b , then c c c must belong to P P P ,22 and therefore satisfy a < 1 , P c < 1 , P b a<_{1,P}c<_{1,P}b a < 1 , P c < 1 , P b 23 , which entails a contradiction to (14). Thus, there is no c ∈ E c\in E c ∈ E satisfying a < 1 c < 1 b a<_{1}c<_{1}b a < 1 c < 1 b . Therefore (and because we have a < 1 b a<_{1}b a < 1 b ), we see that a a a is < 1 <_{1} < 1 -covered by b b b . Since E E E is tertispecial, this yields that a a a and b b b are < 2 <_{2} < 2 -comparable. In other words, either a < 2 b a<_{2}b a < 2 b or a = b a=b a = b or b < 2 a b<_{2}a b < 2 a . Since a a a and b b b both belong to P P P , we can rewrite this by replacing the relation < 2 <_{2} < 2 by its restriction < 2 , P <_{2,P} < 2 , P . We thus conclude that either a < 2 , P b a<_{2,P}b a < 2 , P b or a = b a=b a = b or b < 2 , P a b<_{2,P}a b < 2 , P a . In other words, a a a and b b b are < 2 , P <_{2,P} < 2 , P -comparable.
Now, forget that we fixed a a a and b b b . Thus, we have shown that if a a a and b b b are two elements of P P P such that a a a is < 1 , P <_{1,P} < 1 , P -covered by b b b , then a a a and b b b are < 2 , P <_{2,P} < 2 , P -comparable. This completes the proof of Lemma 6.2.
(We could similarly show that E ∣ Q E|_{Q} E ∣ Q is a tertispecial double poset; but we will not use this.)
no p ∈ P and q ∈ Q satisfy q < 1 p . (15) \text{no }p\in P\text{ and }q\in Q\text{ satisfy }q<_{1}p. \tag*{(15)} no p ∈ P and q ∈ Q satisfy q < 1 p . (15)
From c ∈ E c\in E c ∈ E and c ∉ P c\notin P c ∈ / P , we obtain c ∈ E ∖ P ⊆ Q c\in E\setminus P\subseteq Q c ∈ E ∖ P ⊆ Q (since P ∪ Q = E P\cup Q=E P ∪ Q = E ). Applying (15) to p = b p=b p = b and q = c q=c q = c , we thus conclude that we cannot have c < 1 b c<_{1}b c < 1 b . This contradicts c < 1 b c<_{1}b c < 1 b . This contradiction shows that our assumption was false.
Lemma 6.3. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a double poset. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map.
(a) If E = ∅ E=\varnothing E = ∅ , then Γ ( E , w ) = 1 \Gamma(E,w)=1 Γ ( E , w ) = 1 .
(b) If E ≠ ∅ E\ne\varnothing E = ∅ , then ε ( Γ ( E , w ) ) = 0 \varepsilon(\Gamma(E,w))=0 ε ( Γ ( E , w )) = 0 .
Proof of Lemma 6.3. (a) Part (a) is obvious (since there is only one E E E -partition π \pi π when E = ∅ E=\varnothing E = ∅ , and since this E E E -partition π \pi π satisfies x π , w = 1 x_{\pi,w}=1 x π , w = 1 ).
(b) Observe that Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) is a homogeneous power series of degree
∑ e ∈ E w ( e ) \sum_{e\in E}w(e) e ∈ E ∑ w ( e )
When E ≠ ∅ E\ne\varnothing E = ∅ , this degree is > 0 >0 > 0 (since it is then a nonempty sum of positive integers), and thus the power series Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) is annihilated by ε \varepsilon ε (since ε \varepsilon ε annihilates any homogeneous power series in QSym whose degree is > 0 >0 > 0 ). ▫
Lemma 6.4. Let ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) be a double poset. Let > 1 >_{1} > 1 be the opposite relation of < 1 <_{1} < 1 . Let P P P and Q Q Q be two subsets of E E E satisfying P ∪ Q = E P\cup Q=E P ∪ Q = E . Let π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } be a map such that π ∣ P \pi|_{P} π ∣ P is a ( P , > 1 , < 2 ) (P,>_{1},<_{2}) ( P , > 1 , < 2 ) -partition. Let f ∈ P f\in P f ∈ P . Assume that
no p ∈ P and q ∈ Q satisfy q < 1 p . (16) \text{no }p\in P\text{ and }q\in Q\text{ satisfy }q<_{1}p. \tag*{(16)} no p ∈ P and q ∈ Q satisfy q < 1 p . (16) Also, assume that
π ( f ) ≤ π ( h ) for every h ∈ E . (17) \pi(f)\le\pi(h)\qquad\text{for every }h\in E. \tag*{(17)} π ( f ) ≤ π ( h ) for every h ∈ E . (17) Furthermore, assume that
π ( f ) < π ( h ) for every h ∈ E satisfying h < 2 f . (18) \pi(f)<\pi(h)\qquad\text{for every }h\in E\text{ satisfying }h<_{2}f. \tag*{(18)} π ( f ) < π ( h ) for every h ∈ E satisfying h < 2 f . (18) (a) If p ∈ P ∖ { f } p\in P\setminus\{f\} p ∈ P ∖ { f } and q ∈ Q ∪ { f } q\in Q\cup\{f\} q ∈ Q ∪ { f } are such that q < 1 p q<_{1}p q < 1 p , then we have neither q < 2 p q<_{2}p q < 2 p nor p < 2 q p<_{2}q p < 2 q .
(b) If π ∣ Q \pi|_{Q} π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition, then π ∣ Q ∪ { f } \pi|_{Q\cup\{f\}} π ∣ Q ∪ { f } is a ( Q ∪ { f } , < 1 , < 2 ) (Q\cup\{f\},<_{1},<_{2}) ( Q ∪ { f } , < 1 , < 2 ) -partition.
Proof of Lemma 6.4. From P ∪ Q = E P\cup Q=E P ∪ Q = E , we obtain E ∖ P = ( P ∪ Q ) ∖ P ⊆ Q E\setminus P=(P\cup Q)\setminus P\subseteq Q E ∖ P = ( P ∪ Q ) ∖ P ⊆ Q .
(a) Let p ∈ P ∖ { f } p\in P\setminus\{f\} p ∈ P ∖ { f } and q ∈ Q ∪ { f } q\in Q\cup\{f\} q ∈ Q ∪ { f } be such that q < 1 p q<_{1}p q < 1 p . We must show that we have neither q < 2 p q<_{2}p q < 2 p nor p < 2 q p<_{2}q p < 2 q .
Indeed, assume the contrary. Thus, we have either q < 2 p q<_{2}p q < 2 p or p < 2 q p<_{2}q p < 2 q . We have q < 1 p q<_{1}p q < 1 p and p ∈ P ∖ { f } ⊆ P p\in P\setminus\{f\}\subseteq P p ∈ P ∖ { f } ⊆ P . Hence, if we had q ∈ Q q\in Q q ∈ Q , then we would obtain a contradiction to (16). Hence, we cannot have q ∈ Q q\in Q q ∈ Q . Therefore, q = f q=f q = f (since q ∈ Q ∪ { f } q\in Q\cup\{f\} q ∈ Q ∪ { f } but not q ∈ Q ) . H e n c e , q\in Q). Hence, q ∈ Q ) . H e n ce , f=q<_{1}p$, so that p > 1 f p>_{1}f p > 1 f . Therefore, π ( p ) ≤ π ( f ) \pi(p)\le\pi(f) π ( p ) ≤ π ( f ) (since π ∣ P \pi|_{P} π ∣ P is a ( P , > 1 , < 2 ) (P,>_{1},<_{2}) ( P , > 1 , < 2 ) -partition, and since both f f f and p p p belong to P P P ).
Now, recall that we have either q < 2 p q<_{2}p q < 2 p or p < 2 q p<_{2}q p < 2 q . Since q = f q=f q = f , we can rewrite this as follows: We have either f < 2 p f<_{2}p f < 2 p or p < 2 f p<_{2}f p < 2 f . But p < 2 f p<_{2}f p < 2 f cannot hold (because if we had p < 2 f p <_{2} f p < 2 f , then (18) (applied to h = p h=p h = p ) would lead to π ( f ) < π ( p ) \pi(f)<\pi(p) π ( f ) < π ( p ) , which would contradict π ( p ) ≤ π ( f ) \pi(p)\leq\pi(f) π ( p ) ≤ π ( f ) . Thus, we must have f < 2 p f<_{2}p f < 2 p .
But π ∣ P \pi|_{P} π ∣ P is a ( P , > 1 , < 2 ) (P,>_{1},<_{2}) ( P , > 1 , < 2 ) -partition. Hence, π ( p ) < π ( f ) \pi(p)<\pi(f) π ( p ) < π ( f ) (since p > 1 f p>_{1}f p > 1 f and f < 2 p f<_{2}p f < 2 p , and since p p p and f f f both lie in P P P ). But (17) (applied to h = p h=p h = p ) shows that π ( f ) ≤ π ( p ) \pi(f)\leq\pi(p) π ( f ) ≤ π ( p ) . Hence, π ( p ) < π ( f ) ≤ π ( p ) \pi(p)<\pi(f)\leq\pi(p) π ( p ) < π ( f ) ≤ π ( p ) , a contradiction. Thus, our assumption was wrong. This completes the proof of Lemma 6.4 (a).
(b) Assume that π ∣ Q \pi|_{Q} π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition. We need to show that π ∣ Q ∪ { f } \pi|_{Q\cup\{f\}} π ∣ Q ∪ { f } is a ( Q ∪ { f } , < 1 , < 2 ) (Q\cup\{f\},<_{1},<_{2}) ( Q ∪ { f } , < 1 , < 2 ) -partition. In order to prove this, we need to verify the following two claims:
Claim 1: Every a ∈ Q ∪ { f } a\in Q\cup\{f\} a ∈ Q ∪ { f } and b ∈ Q ∪ { f } b\in Q\cup\{f\} b ∈ Q ∪ { f } satisfying a < 1 b a<_{1}b a < 1 b satisfy π ( a ) ≤ π ( b ) \pi(a)\leq\pi(b) π ( a ) ≤ π ( b ) .
Claim 2: Every a ∈ Q ∪ { f } a\in Q\cup\{f\} a ∈ Q ∪ { f } and b ∈ Q ∪ { f } b\in Q\cup\{f\} b ∈ Q ∪ { f } satisfying a < 1 b a<_{1}b a < 1 b and b < 2 a b<_{2}a b < 2 a satisfy π ( a ) < π ( b ) \pi(a)<\pi(b) π ( a ) < π ( b ) .
Proof of Claim 1: Let a ∈ Q ∪ { f } a\in Q\cup\{f\} a ∈ Q ∪ { f } and b ∈ Q ∪ { f } b\in Q\cup\{f\} b ∈ Q ∪ { f } be such that a < 1 b a<_{1}b a < 1 b . We need to prove that π ( a ) ≤ π ( b ) \pi(a)\leq\pi(b) π ( a ) ≤ π ( b ) . If a = f a=f a = f , then this follows immediately from (17) (applied to h = b h=b h = b ). Hence, we WLOG assume that a ≠ f a\neq f a = f . Thus, a ∈ Q a\in Q a ∈ Q (since a ∈ Q ∪ { f } a\in Q\cup\{f\} a ∈ Q ∪ { f } ). Now, if b ∈ P b\in P b ∈ P , then a < 1 b a<_{1}b a < 1 b contradicts (16) (applied to p = b p=b p = b and q = a q=a q = a ). Hence, we cannot have b ∈ P b\in P b ∈ P . Therefore, b ∈ E ∖ P ⊆ Q b\in E\setminus P\subseteq Q b ∈ E ∖ P ⊆ Q . Thus, π ( a ) ≤ π ( b ) \pi(a)\leq\pi(b) π ( a ) ≤ π ( b ) follows immediately from the fact that π ∣ Q \pi|_{Q} π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition (since a ∈ Q a\in Q a ∈ Q and b ∈ Q b\in Q b ∈ Q and a < 1 b a<_{1}b a < 1 b ). This proves Claim 1.
Proof of Claim 2: Let a ∈ Q ∪ { f } a\in Q\cup\{f\} a ∈ Q ∪ { f } and b ∈ Q ∪ { f } b\in Q\cup\{f\} b ∈ Q ∪ { f } be such that a < 1 b a<_{1}b a < 1 b and b < 2 a b<_{2}a b < 2 a . We need to prove that π ( a ) < π ( b ) \pi(a)<\pi(b) π ( a ) < π ( b ) . If a = f a=f a = f , then this follows immediately from (18) (applied to h = b h=b h = b ) (because if a = f a=f a = f , then b < 2 a = f b<_{2}a=f b < 2 a = f ). Hence, we WLOG assume that a ≠ f a\neq f a = f . Thus, a ∈ Q a\in Q a ∈ Q (since a ∈ Q ∪ { f } a\in Q\cup\{f\} a ∈ Q ∪ { f } ). Now, if b ∈ P b\in P b ∈ P , then a < 1 b a<_{1}b a < 1 b contradicts (16) (applied to p = b p=b p = b and q = a q=a q = a ). Hence, we cannot have b ∈ P b\in P b ∈ P . Therefore, b ∈ E ∖ P ⊆ Q b\in E\setminus P\subseteq Q b ∈ E ∖ P ⊆ Q . Thus, π ( a ) < π ( b ) \pi(a)<\pi(b) π ( a ) < π ( b ) follows immediately from the fact that π ∣ Q \pi|_{Q} π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition (since a ∈ Q a\in Q a ∈ Q and b ∈ Q b\in Q b ∈ Q and a < 1 b a<_{1}b a < 1 b and b < 2 a b<_{2}a b < 2 a ). This proves Claim 2.
Now, both Claim 1 and Claim 2 are proven. As already said, this completes the proof of Lemma 6.4 (b).
Lemma 6.5. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset satisfying ∣ E ∣ > 0 |E|>0 ∣ E ∣ > 0 . Let π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } be a map. Let > 1 >_{1} > 1 denote the opposite relation of < 1 <_{1} < 1 . Then,
∑ ( P , Q ) ∈ Adm E ; π ∣ P is a ( P , > 1 , < 2 ) -partition ; π ∣ Q is a ( Q , < 1 , < 2 ) -partition ( − 1 ) ∣ P ∣ = 0. (19) \sum_{\substack{(P,Q)\in\operatorname{Adm} E;\\
\pi|_{P}\text{ is a }(P,>_{1},<_{2})\text{-partition};\\
\pi|_{Q}\text{ is a }(Q,<_{1},<_{2})\text{-partition}}}
(-1)^{|P|}=0. \tag*{(19)} ( P , Q ) ∈ Adm E ; π ∣ P is a ( P , > 1 , < 2 ) -partition ; π ∣ Q is a ( Q , < 1 , < 2 ) -partition ∑ ( − 1 ) ∣ P ∣ = 0. (19)
Proof of Lemma 6.5. Our goal is to prove (19) . To do so, we denote by Z Z Z the set of all ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E such that π ∣ P \pi|_{P} π ∣ P is a ( P , > 1 , < 2 ) (P,>_{1},<_{2}) ( P , > 1 , < 2 ) -partition and π ∣ Q \pi|_{Q} π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition. We are going to define an involution T : Z → Z T:Z\to Z T : Z → Z of the set Z Z Z having the following property: Property P: Let ( P , Q ) ∈ Z (P,Q) \in Z ( P , Q ) ∈ Z . If we write T ( ( P , Q ) ) T((P,Q)) T (( P , Q )) in the form ( P ′ , Q ′ ) (P',Q') ( P ′ , Q ′ ) , then ( − 1 ) ∣ P ′ ∣ = − ( − 1 ) ∣ P ∣ (-1)^{|P'|} = -(-1)^{|P|} ( − 1 ) ∣ P ′ ∣ = − ( − 1 ) ∣ P ∣ .
Once such an involution T T T is found, it will be clear that it matches the addends on the left hand side of (19) into pairs of mutually cancelling addends24 , and so (19) will follow and we will be done. It thus remains to find T T T .
The definition of the map T : Z → Z T: Z \to Z T : Z → Z is simple (although it will take us a while to prove that it is well-defined): Let F F F be the subset of E E E consisting of those e ∈ E e \in E e ∈ E for which the value π ( e ) \pi(e) π ( e ) is minimum. Then, F F F is a nonempty subposet25 of the poset ( E , < 2 ) (E,<_{2}) ( E , < 2 ) , and hence has a minimal element26 f f f (that is, an element f f f such that no g ∈ F g \in F g ∈ F satisfies g < 2 f g <_{2} f g < 2 f ). Fix such an f f f . Now, the map T T T sends a ( P , Q ) ∈ Z (P,Q) \in Z ( P , Q ) ∈ Z to
{ ( P ∪ { f } , Q ∖ { f } ) , if f ∉ P ; ( P ∖ { f } , Q ∪ { f } ) , if f ∈ P . \begin{cases}
(P \cup\{f\}, Q \setminus\{f\}), & \text{if } f \notin P; \\
(P \setminus\{f\}, Q \cup\{f\}), & \text{if } f \in P.
\end{cases} { ( P ∪ { f } , Q ∖ { f }) , ( P ∖ { f } , Q ∪ { f }) , if f ∈ / P ; if f ∈ P .
In order to prove that the map T T T is well-defined, we need to prove that its output values all belong to Z Z Z . In other words, we need to prove that
\begin{cases}
(P \cup\{f\}, Q \setminus\{f\}), & \text{if } f \notin P; \\
(P \setminus\{f\}, Q \cup\{f\}), & \text{if } f \in P
\end{cases}
\in Z \tag*{(20)}\end{cases}
for every ( P , Q ) ∈ Z (P,Q) \in Z ( P , Q ) ∈ Z .
Proof of (20): Fix ( P , Q ) ∈ Z (P,Q) \in Z ( P , Q ) ∈ Z . Thus, ( P , Q ) (P,Q) ( P , Q ) is an element of Adm E \operatorname{Adm} E Adm E with the property that π ∣ P \pi|_P π ∣ P is a ( P , > 1 , < 2 ) (P,>_{1},<_{2}) ( P , > 1 , < 2 ) -partition and π ∣ Q \pi|_Q π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition (by the definition of Z Z Z ).
From ( P , Q ) ∈ Adm E (P,Q) \in\operatorname{Adm} E ( P , Q ) ∈ Adm E , we see that P ∩ Q = ∅ P \cap Q = \varnothing P ∩ Q = ∅ and P ∪ Q = E P \cup Q = E P ∪ Q = E , and furthermore that
no p ∈ P and q ∈ Q satisfy q < 1 p . (21) \text{no } p \in P \text{ and } q \in Q \text{ satisfy } q <_{1} p. \tag*{(21)} no p ∈ P and q ∈ Q satisfy q < 1 p . (21)
We know that f f f belongs to the set F F F , which is the subset of E E E consisting of those e ∈ E e \in E e ∈ E for which the value π ( e ) \pi(e) π ( e ) is minimum. Thus,
π ( f ) ≤ π ( h ) for every h ∈ E . (22) \pi(f) \leq\pi(h) \qquad\text{for every } h \in E. \tag*{(22)} π ( f ) ≤ π ( h ) for every h ∈ E . (22)
Moreover,
π ( f ) < π ( h ) for every h ∈ E satisfying h < 2 f (23) \pi(f) < \pi(h) \qquad\text{for every } h \in E \text{ satisfying } h <_{2} f \tag*{(23)} π ( f ) < π ( h ) for every h ∈ E satisfying h < 2 f (23)
We need to prove (20) . We are in one of the following two cases:
Case 1: We have f ∈ P f \in P f ∈ P .
Case 2: We have f ∉ P f \notin P f ∈ / P .
Let us first consider Case 1. In this case, we have f ∈ P f \in P f ∈ P .
Recall that P ∩ Q = ∅ P \cap Q = \varnothing P ∩ Q = ∅ and P ∪ Q = E P \cup Q = E P ∪ Q = E . From this, we easily obtain ( P ∖ { f } ) ∩ ( Q ∪ { f } ) = ∅ (P \setminus\{f\}) \cap(Q \cup\{f\}) = \varnothing ( P ∖ { f }) ∩ ( Q ∪ { f }) = ∅ and ( P ∖ { f } ) ∪ ( Q ∪ { f } ) = E (P \setminus\{f\}) \cup(Q \cup\{f\}) = E ( P ∖ { f }) ∪ ( Q ∪ { f }) = E .
Furthermore, there exist no p ∈ P ∖ { f } p \in P \setminus\{f\} p ∈ P ∖ { f } and q ∈ Q ∪ { f } q \in Q \cup\{f\} q ∈ Q ∪ { f } such that q q q is < 1 <_{1} < 1 -covered by p p p 27 . Hence, Lemma 6.1 (applied to P ∖ { f } P \setminus\{f\} P ∖ { f } and Q ∪ { f } Q \cup\{f\} Q ∪ { f } instead of P P P and Q Q Q ) shows that ( P ∖ { f } , Q ∪ { f } ) ∈ Adm E (P \setminus\{f\}, Q \cup\{f\}) \in\operatorname{Adm} E ( P ∖ { f } , Q ∪ { f }) ∈ Adm E .
Furthermore, π ∣ P \pi\mathbin{|}_{P} π ∣ P is a ( P , > 1 , < 2 ) (P, >_{1}, <_{2}) ( P , > 1 , < 2 ) -partition. Hence, π ∣ P ∖ { f } \pi\mathbin{|}_{P \setminus\{f\}} π ∣ P ∖ { f } is a ( P ∖ { f } , > 1 , < 2 ) (P \setminus\{f\}, >_{1}, <_{2}) ( P ∖ { f } , > 1 , < 2 ) -partition (since P ∖ { f } ⊆ P P \setminus\{f\} \subseteq P P ∖ { f } ⊆ P ).
Furthermore, π ∣ Q ∪ { f } \pi\mathbin{|}_{Q \cup\{f\}} π ∣ Q ∪ { f } is a ( Q ∪ { f } , < 1 , < 2 ) (Q \cup\{f\}, <_{1}, <_{2}) ( Q ∪ { f } , < 1 , < 2 ) -partition28 .
Altogether, we now know that ( P ∖ { f } , Q ∪ { f } ) ∈ Adm E (P \setminus\{f\}, Q \cup\{f\}) \in\operatorname{Adm} E ( P ∖ { f } , Q ∪ { f }) ∈ Adm E , that π ∣ P ∖ { f } \pi\mathbin{|}_{P \setminus\{f\}} π ∣ P ∖ { f } is a ( P ∖ { f } , > 1 , < 2 ) (P \setminus\{f\}, >_{1}, <_{2}) ( P ∖ { f } , > 1 , < 2 ) -partition, and that π ∣ Q ∪ { f } \pi\mathbin{|}_{Q \cup\{f\}} π ∣ Q ∪ { f } is a ( Q ∪ { f } , < 1 , < 2 ) (Q \cup\{f\}, <_{1}, <_{2}) ( Q ∪ { f } , < 1 , < 2 ) -partition. In other words, ( P ∖ { f } , Q ∪ { f } ) ∈ Z (P \setminus\{f\}, Q \cup\{f\}) \in Z ( P ∖ { f } , Q ∪ { f }) ∈ Z (by the definition of Z Z Z ). Thus,
{ ( P ∪ { f } , Q ∖ { f } ) , if f ∉ P ; ( P ∖ { f } , Q ∪ { f } ) , if f ∈ P = ( P ∖ { f } , Q ∪ { f } ) (since f ∈ P ) \begin{cases}
(P \cup\{f\}, Q \setminus\{f\}), & \text{if } f \notin P;\\
(P \setminus\{f\}, Q \cup\{f\}), & \text{if } f \in P
\end{cases}
= (P \setminus\{f\}, Q \cup\{f\}) \quad\text{(since } f \in P\text{)} { ( P ∪ { f } , Q ∖ { f }) , ( P ∖ { f } , Q ∪ { f }) , if f ∈ / P ; if f ∈ P = ( P ∖ { f } , Q ∪ { f }) (since f ∈ P )
Hence, (20) is proven in Case 1.
Let us next consider Case 2. In this case, we have f ∉ P f \notin P f ∈ / P . Hence, f ∈ E ∖ P = Q f \in E \setminus P = Q f ∈ E ∖ P = Q (since P ∩ Q = ∅ P \cap Q = \varnothing P ∩ Q = ∅ and P ∪ Q = E P \cup Q = E P ∪ Q = E ).
Recall that P ∩ Q = ∅ P \cap Q = \varnothing P ∩ Q = ∅ and P ∪ Q = E P \cup Q = E P ∪ Q = E . From this, we easily obtain ( P ∪ { f } ) ∩ ( Q ∖ { f } ) = ∅ (P \cup\{f\}) \cap(Q \setminus\{f\}) = \varnothing ( P ∪ { f }) ∩ ( Q ∖ { f }) = ∅ and ( P ∪ { f } ) ∪ ( Q ∖ { f } ) = E (P \cup\{f\}) \cup(Q \setminus\{f\}) = E ( P ∪ { f }) ∪ ( Q ∖ { f }) = E .
We have f ∈ Q f \in Q f ∈ Q and Q ∪ P = P ∪ Q = E Q \cup P = P \cup Q = E Q ∪ P = P ∪ Q = E . Furthermore, > 1 >_{1} > 1 is the opposite relation of < 1 <_{1} < 1 , and thus is a strict partial order (since < 1 <_{1} < 1 is a strict partial order). Hence, ( E , > 1 , < 2 ) (E, >_{1}, <_{2}) ( E , > 1 , < 2 ) is a double poset. Furthermore, the relation < 1 <_{1} < 1 is the opposite relation of > 1 >_1 > 1 (since > 1 >_1 > 1 is the opposite relation of < 1 <_1 < 1 ). The map π ∣ Q \pi\mathbin{|}_Q π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition. Moreover,
no p ∈ Q and q ∈ P satisfy q > 1 p (24) \text{no }p\in Q\text{ and }q\in P\text{ satisfy }q>_{1}p \tag*{(24)} no p ∈ Q and q ∈ P satisfy q > 1 p (24)
30 Hence, we can apply Lemma 6.4 to ( E , > 1 , < 2 ) (E,>_{1},<_{2}) ( E , > 1 , < 2 ) , < 1 <_{1} < 1 , Q Q Q and P P P instead of ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) , > 1 >_{1} > 1 , P P P and Q Q Q .
There exist no p ∈ P ∪ { f } p\in P\cup\{f\} p ∈ P ∪ { f } and q ∈ Q ∖ { f } q\in Q\setminus\{f\} q ∈ Q ∖ { f } such that q q q is < 1 <_{1} < 1 -covered by p p p .31 Hence, Lemma 6.1 (applied to P ∪ { f } P\cup\{f\} P ∪ { f } and Q ∖ { f } Q\setminus\{f\} Q ∖ { f } instead of P P P and Q Q Q ) shows that ( P ∪ { f } , Q ∖ { f } ) ∈ Adm E (P\cup\{f\},Q\setminus\{f\})\in\operatorname{Adm}E ( P ∪ { f } , Q ∖ { f }) ∈ Adm E .
Furthermore, π ∣ Q \pi\mathbin{|}_Q π ∣ Q is a ( Q , < 1 , < 2 ) (Q,<_{1},<_{2}) ( Q , < 1 , < 2 ) -partition. Hence, π ∣ Q ∖ { f } \pi\mathbin{|}_{Q\setminus\{f\}} π ∣ Q ∖ { f } is a ( Q ∖ { f } , < 1 , < 2 ) (Q\setminus\{f\},<_{1},<_{2}) ( Q ∖ { f } , < 1 , < 2 ) -partition (since Q ∖ { f } ⊆ Q Q\setminus\{f\}\subseteq Q Q ∖ { f } ⊆ Q ).
Furthermore, π ∣ P ∪ { f } \pi\mathbin{|}_{P\cup\{f\}} π ∣ P ∪ { f } is a ( P ∪ { f } , > 1 , < 2 ) (P\cup\{f\},>_{1},<_{2}) ( P ∪ { f } , > 1 , < 2 ) -partition.32
Altogether, we now know that ( P ∪ { f } , Q ∖ { f } ) ∈ Adm E (P\cup\{f\},Q\setminus\{f\})\in\operatorname{Adm}E ( P ∪ { f } , Q ∖ { f }) ∈ Adm E , that π ∣ P ∪ { f } \pi\mathbin{|}_{P\cup\{f\}} π ∣ P ∪ { f } is a ( P ∪ { f } , > 1 , < 2 ) (P\cup\{f\},>_{1},<_{2}) ( P ∪ { f } , > 1 , < 2 ) -partition, and that π ∣ Q ∖ { f } \pi\mathbin{|}_{Q\setminus\{f\}} π ∣ Q ∖ { f } is a ( Q ∖ { f } , < 1 , < 2 ) (Q\setminus\{f\},<_{1},<_{2}) ( Q ∖ { f } , < 1 , < 2 ) -partition. In other words, ( P ∪ { f } , Q ∖ { f } ) ∈ Z (P\cup\{f\},Q\setminus\{f\})\in Z ( P ∪ { f } , Q ∖ { f }) ∈ Z (by the definition of Z Z Z ). Thus,
{ ( P ∪ { f } , Q ∖ { f } ) , if f ∉ P ; ( P ∖ { f } , Q ∪ { f } ) , if f ∈ P = ( P ∪ { f } , Q ∖ { f } ) (since f ∉ P ) ∈ Z . \begin{cases}
(P\cup\{f\},Q\setminus\{f\}), & \text{if }f\notin P;\\
(P\setminus\{f\},Q\cup\{f\}), & \text{if }f\in P
\end{cases}
=(P\cup\{f\},Q\setminus\{f\})\quad\text{(since }f\notin P\text{)}
\in Z. { ( P ∪ { f } , Q ∖ { f }) , ( P ∖ { f } , Q ∪ { f }) , if f ∈ / P ; if f ∈ P = ( P ∪ { f } , Q ∖ { f }) (since f ∈ / P ) ∈ Z .
Hence, (20) is proven in Case 2.
We have now proven (20) in both Cases 1 and 2. Thus, (20) always holds. In other words, the map T T T is well-defined.
What the map T T T does to a pair ( P , Q ) ∈ Z (P,Q)\in Z ( P , Q ) ∈ Z can be described as moving the element f f f from the set where it resides (either P P P or Q Q Q ) to the other set. Clearly, doing this twice gives us the original pair back. Hence, the map T T T is an involution. Furthermore, for any ( P , Q ) ∈ Z (P,Q)\in Z ( P , Q ) ∈ Z , if we write T ( ( P , Q ) ) T((P,Q)) T (( P , Q )) in the form ( P ′ , Q ′ ) (P',Q') ( P ′ , Q ′ ) , then
( − 1 ) ∣ P ′ ∣ = − ( − 1 ) ∣ P ∣ (-1)^{|P'|}=-(-1)^{|P|} ( − 1 ) ∣ P ′ ∣ = − ( − 1 ) ∣ P ∣
(because P ′ = { P ∪ { f } , if f ∉ P ; P ∖ { f } , if f ∈ P P'=\begin{cases}P\cup\{f\},&\text{if }f\notin P;\\P\setminus\{f\},&\text{if }f\in P\end{cases} P ′ = { P ∪ { f } , P ∖ { f } , if f ∈ / P ; if f ∈ P and thus ∣ P ′ ∣ = ∣ P ∣ ± 1 |P'|=|P|\pm1 ∣ P ′ ∣ = ∣ P ∣ ± 1 ).
Now, forget that we fixed a a a and b b b . We thus have found a contradiction for every a ∈ Q a\in Q a ∈ Q and b ∈ P b\in P b ∈ P satisfying b > 1 a b>_{1}a b > 1 a . Hence, no a ∈ Q a\in Q a ∈ Q and b ∈ P b\in P b ∈ P satisfy b > 1 a b>_{1}a b > 1 a . Renaming a a a and b b b as p p p and q q q in this statement, we obtain the following: No p ∈ Q p\in Q p ∈ Q and q ∈ P q\in P q ∈ P satisfy q > 1 p q>_{1}p q > 1 p . This proves (24).
We know that q q q is < 1 <_{1} < 1 -covered by p p p , and thus we have q < 1 p q<_{1}p q < 1 p . In other words, p > 1 q p>_{1}q p > 1 q . Thus, Lemma 6.4 (a) (applied to ( E , > 1 , < 2 ) (E,>_{1},<_{2}) ( E , > 1 , < 2 ) , < 1 <_{1} < 1 , Q Q Q , P P P , q q q and p p p instead of ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) , > 1 >_{1} > 1 , P P P , Q Q Q , p p p and q q q ) yields that we have neither p < 2 q p<_{2}q p < 2 q nor q < 2 p q<_{2}p q < 2 p . On the other hand, q q q is < 1 <_{1} < 1 -covered by p p p . Hence, q q q and p p p are < 2 <_{2} < 2 -comparable (since E E E is tertispecial). In other words, we have either q < 2 p q<_{2}p q < 2 p or q = p q=p q = p or p < 2 q p<_{2}q p < 2 q . Hence, we must have q = p q=p q = p (since we have neither p < 2 q p<_{2}q p < 2 q nor q < 2 p q<_{2}p q < 2 p ). But this contradicts q < 1 p q<_{1}p q < 1 p . This contradiction shows that our assumption was wrong, qed. In other words, the involution T T T satisfies Property P. As we have already explained, this proves (19) . Hence, Lemma 6.5 is proven.
Proof of Theorem 4.2 . We shall prove Theorem 4.2 by strong induction over ∣ E ∣ |E| ∣ E ∣ . The induction step proceeds as follows: Consider a tertispecial double poset E = ( E , < 1 , < 2 ) \mathbf{E}=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) and a map w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } , and assume (as the induction hypothesis) that Theorem 4.2 is proven for all tertispecial double posets of smaller size33 . Our goal is to show that
S ( Γ ( ( E , < 1 , < 2 ) , w ) ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) . S\left(\Gamma\left((E,<_{1},<_{2}),w\right)\right)=(-1)^{|E|}\Gamma\left((E,>_{1},<_{2}),w\right). S ( Γ ( ( E , < 1 , < 2 ) , w ) ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) .
Here, as usual, > 1 >_{1} > 1 denotes the opposite relation of < 1 <_{1} < 1 .
If E = ∅ E=\varnothing E = ∅ , then this is easy34 . Thus, we WLOG assume that E ≠ ∅ E\ne\varnothing E = ∅ . Hence, ∣ E ∣ > 0 |E|>0 ∣ E ∣ > 0 . Moreover, Lemma 6.3 (b) shows that ε ( Γ ( E , w ) ) = 0 \varepsilon(\Gamma(E,w))=0 ε ( Γ ( E , w )) = 0 . Thus, $(u\circ\varepsilon)(\Gamma(E,w))=
u ( ε ( Γ ( E , w ) ) ⏟ = 0 ) = u ( 0 ) = 0. u\left(\underbrace{\varepsilon(\Gamma(E,w))}_{=0}\right)=u(0)=0. u = 0 ε ( Γ ( E , w )) = u ( 0 ) = 0.
The upper commutative pentagon of (2) shows that u ∘ ε = m ∘ ( S ⊗ id ) ∘ Δ u\circ\varepsilon=m\circ(S\otimes\operatorname{id})\circ\Delta u ∘ ε = m ∘ ( S ⊗ id ) ∘ Δ . Applying both sides of this equality to Γ ( E , w ) \Gamma(E,w) Γ ( E , w ) , we obtain ( u ∘ ε ) ( Γ ( E , w ) ) = ( m ∘ ( S ⊗ id ) ∘ Δ ) ( Γ ( E , w ) ) (u\circ\varepsilon)(\Gamma(E,w))=(m\circ(S\otimes\operatorname{id})\circ\Delta)(\Gamma(E,w)) ( u ∘ ε ) ( Γ ( E , w )) = ( m ∘ ( S ⊗ id ) ∘ Δ ) ( Γ ( E , w )) . Since ( u ∘ ε ) ( Γ ( E , w ) ) = 0 (u\circ\varepsilon)(\Gamma(E,w))=0 ( u ∘ ε ) ( Γ ( E , w )) = 0 , this becomes
0 = ( m ∘ ( S ⊗ id ) ∘ Δ ) ( Γ ( E , w ) ) = m ( ( S ⊗ id ) ( Δ ( Γ ( E , w ) ) ) ) = m ( ( S ⊗ id ) ( ∑ ( P , Q ) ∈ Adm E Γ ( E ∣ P , w ∣ P ) ⊗ Γ ( E ∣ Q , w ∣ Q ) ) ) (by (10)) = m ( ∑ ( P , Q ) ∈ Adm E S ( Γ ( E ∣ P , w ∣ P ) ) ⊗ Γ ( E ∣ Q , w ∣ Q ) ) = ∑ ( P , Q ) ∈ Adm E S ( Γ ( E ∣ P , w ∣ P ) ) Γ ( E ∣ Q , w ∣ Q ) = S ( Γ ( E ∣ E , w ∣ E ) ) Γ ( E ∣ ∅ , w ∣ ∅ ) + ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ S ( Γ ( E ∣ P , w ∣ P ) ) Γ ( E ∣ Q , w ∣ Q ) . (25) \begin{aligned}
0=(m\circ(S\otimes\operatorname{id})\circ\Delta)(\Gamma(E,w))=m\left((S\otimes\operatorname{id})(\Delta(\Gamma(E,w)))\right) \\
&=m\left((S\otimes\operatorname{id})\left(\sum_{(P,Q)\in\operatorname{Adm}E}\Gamma(E|_{P},w|_{P})\otimes\Gamma(E|_{Q},w|_{Q})\right)\right)\qquad\text{(by (10))} \\
&=m\left(\sum_{(P,Q)\in\operatorname{Adm}E}S(\Gamma(E|_{P},w|_{P}))\otimes\Gamma(E|_{Q},w|_{Q})\right) \\
&=\sum_{(P,Q)\in\operatorname{Adm}E}S(\Gamma(E|_{P},w|_{P}))\Gamma(E|_{Q},w|_{Q}) \\
&=S(\Gamma(E|_{E},w|_{E}))\Gamma(E|_{\varnothing},w|_{\varnothing})+
\sum_{\substack{(P,Q)\in\operatorname{Adm}E;\\|P|<|E|}}
S(\Gamma(E|_{P},w|_{P}))\Gamma(E|_{Q},w|_{Q}). \tag*{(25)}
\end{aligned} 0 = ( m ∘ ( S ⊗ id ) ∘ Δ ) ( Γ ( E , w )) = m ( ( S ⊗ id ) ( Δ ( Γ ( E , w ))) ) = m ( S ⊗ id ) ( P , Q ) ∈ Adm E ∑ Γ ( E ∣ P , w ∣ P ) ⊗ Γ ( E ∣ Q , w ∣ Q ) (by (10)) = m ( P , Q ) ∈ Adm E ∑ S ( Γ ( E ∣ P , w ∣ P )) ⊗ Γ ( E ∣ Q , w ∣ Q ) = ( P , Q ) ∈ Adm E ∑ S ( Γ ( E ∣ P , w ∣ P )) Γ ( E ∣ Q , w ∣ Q ) = S ( Γ ( E ∣ E , w ∣ E )) Γ ( E ∣ ∅ , w ∣ ∅ ) + ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ S ( Γ ( E ∣ P , w ∣ P )) Γ ( E ∣ Q , w ∣ Q ) . (25)
(since the only pair ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm}E ( P , Q ) ∈ Adm E satisfying ∣ P ∣ ≥ ∣ E ∣ |P|\ge|E| ∣ P ∣ ≥ ∣ E ∣ is ( E , ∅ ) (E,\varnothing) ( E , ∅ ) , whereas all other pairs ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm}E ( P , Q ) ∈ Adm E satisfy ∣ P ∣ < ∣ E ∣ |P|<|E| ∣ P ∣ < ∣ E ∣ ).
But whenever ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm}E ( P , Q ) ∈ Adm E is such that ∣ P ∣ < ∣ E ∣ |P|<|E| ∣ P ∣ < ∣ E ∣ , the double poset E ∣ P = ( P , < 1 , < 2 ) E|_{P}=(P,<_{1},<_{2}) E ∣ P = ( P , < 1 , < 2 ) is tertispecial (by Lemma 6.2 ), and therefore we have S ( Γ ( E ∣ P , w ∣ P ) ) = S ( Γ ( ( P , < 1 , < 2 ) , w ∣ P ) ) = ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) S(\Gamma(E|_{P},w|_{P}))=S(\Gamma((P,<_{1},<_{2}),w|_{P}))=(-1)^{|P|}\Gamma((P,>_{1},<_{2}),w|_{P}) S ( Γ ( E ∣ P , w ∣ P )) = S ( Γ (( P , < 1 , < 2 ) , w ∣ P )) = ( − 1 ) ∣ P ∣ Γ (( P , > 1 , < 2 ) , w ∣ P ) (by the induction hypothesis). Hence, (25) becomes
0 = S ( Γ ( E ∣ E , w ∣ E ⏟ = E ) ) Γ ( E ∣ ∅ , w ∣ ∅ ) ⏟ = Γ ( ( ∅ , < 1 , < 2 ) , w ∣ ∅ ) = 1 (by Lemma 6.3 (a)) + ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ S ( Γ ( E ∣ P , w ∣ P ) ) = ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) ⏟ Γ ( E ∣ Q , w ∣ Q ) = S ( Γ ( E , w ) ) + ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) . \begin{aligned}
0={}&S\left(\Gamma\left(\underbrace{\mathrm{E}|_{E},w|_{E}}_{=\mathrm{E}} \right)\right)\underbrace{\Gamma\left(\mathrm{E}|_{\varnothing},w|_{\varnothing}\right)}_{=\Gamma((\varnothing,<_{1},<_{2}),w|_{\varnothing})=1\\ \text{(by Lemma 6.3 (a))}}\\
&+\sum_{\substack{(P,Q)\in\operatorname{Adm}\mathrm{E};\\ |P|<|\mathrm{E}|}} \frac{S\left(\Gamma(\mathrm{E}|_{P},w|_{P})\right)}{\underbrace{=(-1)^{|P|}\Gamma((P,>_{1},<_{2}),w|_{P})}} \Gamma(\mathrm{E}|_{Q},w|_{Q})\\
={}&S(\Gamma(\mathrm{E},w))+\sum_{\substack{(P,Q)\in\operatorname{Adm}\mathrm{E};\\ |P|<|\mathrm{E}|}}(-1)^{|P|}\Gamma((P,>_{1},<_{2}),w|_{P})\Gamma(\mathrm{E}|_{Q},w|_{Q}).
\end{aligned} 0 = = S Γ = E E ∣ E , w ∣ E = Γ (( ∅ , < 1 , < 2 ) , w ∣ ∅ ) = 1 (by Lemma 6.3 (a)) Γ ( E ∣ ∅ , w ∣ ∅ ) + ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ = ( − 1 ) ∣ P ∣ Γ (( P , > 1 , < 2 ) , w ∣ P ) S ( Γ ( E ∣ P , w ∣ P ) ) Γ ( E ∣ Q , w ∣ Q ) S ( Γ ( E , w )) + ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ ( − 1 ) ∣ P ∣ Γ (( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) .
Thus,
S ( Γ ( E , w ) ) = − ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) . (26) S(\Gamma(\mathrm{E},w))=-\sum_{\substack{(P,Q)\in\operatorname{Adm}\mathrm{E};\\ |P|<|\mathrm{E}|}}(-1)^{|P|}\Gamma((P,>_{1},<_{2}),w|_{P})\Gamma(\mathrm{E}|_{Q},w|_{Q}). \tag*{(26)} S ( Γ ( E , w )) = − ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ ( − 1 ) ∣ P ∣ Γ (( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) . (26)
For every subset P P P of E E E , we have
Γ ( ( P , > 1 , < 2 ) , w ∣ P ) = ∑ π is a ( P , > 1 , < 2 ) -partition x π , w ∣ P (by the definition of Γ ( ( P , > 1 , < 2 ) , w ∣ P ) ) = ∑ σ is a ( P , > 1 , < 2 ) -partition x σ , w ∣ P . (27) \begin{aligned}
\Gamma((P,>_{1},<_{2}),w|_{P})
&=\sum_{\pi\ \text{is a }(P,>_{1},<_{2})\text{-partition}}\mathbf{x}_{\pi,w|_{P}}\\
&\hspace{1cm}\text{(by the definition of }\Gamma((P,>_{1},<_{2}),w|_{P})\text{)}\\
&=\sum_{\sigma\ \text{is a }(P,>_{1},<_{2})\text{-partition}}\mathbf{x}_{\sigma,w|_{P}}. \tag*{(27)}
\end{aligned} Γ (( P , > 1 , < 2 ) , w ∣ P ) = π is a ( P , > 1 , < 2 ) -partition ∑ x π , w ∣ P (by the definition of Γ (( P , > 1 , < 2 ) , w ∣ P ) ) = σ is a ( P , > 1 , < 2 ) -partition ∑ x σ , w ∣ P . (27)
(here, we have renamed the summation index π \pi π as σ \sigma σ ).
For every subset Q Q Q of E E E , we have
Γ ( E ∣ Q ⏟ = ( Q , < 1 , < 2 ) , w ∣ Q ) = Γ ( ( Q , < 1 , < 2 ) , w ∣ Q ) = ∑ π is a ( Q , < 1 , < 2 ) -partition x π , w ∣ Q (by the definition of Γ ( ( Q , < 1 , < 2 ) , w ∣ Q ) ) = ∑ τ is a ( Q , < 1 , < 2 ) -partition x τ , w ∣ Q . (28) \begin{aligned}
\Gamma\left(\underbrace{\mathrm{E}|_{Q}}_{=(Q,<_{1},<_{2})},w|_{Q}\right)
&=\Gamma((Q,<_{1},<_{2}),w|_{Q})\\
&=\sum_{\pi\ \text{is a }(Q,<_{1},<_{2})\text{-partition}}\mathbf{x}_{\pi,w|_{Q}}\\
&\hspace{1cm}\text{(by the definition of }\Gamma((Q,<_{1},<_{2}),w|_{Q})\text{)}\\
&=\sum_{\tau\ \text{is a }(Q,<_{1},<_{2})\text{-partition}}\mathbf{x}_{\tau,w|_{Q}}. \tag*{(28)}
\end{aligned} Γ = ( Q , < 1 , < 2 ) E ∣ Q , w ∣ Q = Γ (( Q , < 1 , < 2 ) , w ∣ Q ) = π is a ( Q , < 1 , < 2 ) -partition ∑ x π , w ∣ Q (by the definition of Γ (( Q , < 1 , < 2 ) , w ∣ Q ) ) = τ is a ( Q , < 1 , < 2 ) -partition ∑ x τ , w ∣ Q . (28)
(here, we have renamed the summation index π \pi π as τ \tau τ ).
Now,
\begin{aligned}
\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}
\underbrace{\Gamma\left((P,>_1,<_{2}),w|_P\right)}_{ \sum_{\sigma\text{ is a }(P,>_1,<_{2})\text{-partition}}x_{\sigma,w|_P}\text{ (by {xref}`(27)`)}}
\underbrace{\Gamma\left(E|_Q,w|_Q\right)}_{ \sum_{\tau\text{ is a }(Q,<_{1},<_{2})\text{-partition}}x_{\tau,w|_Q}\text{ (by {xref}`(28)`)}
&=
\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}
\left(\sum_{\sigma\text{ is a }(P,>_1,<_{2})\text{-partition}}x_{\sigma,w|_P}\right)
\left(\sum_{\tau\text{ is a }(Q,<_{1},<_{2})\text{-partition}}x_{\tau,w|_Q}\right)\\
&=
\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}
\sum_{\substack{\sigma\text{ is a }(P,>_1,<_{2})\text{-partition}\\
\tau\text{ is a }(Q,<_{1},<_{2})\text{-partition}}}
x_{\sigma,w|_P}x_{\tau,w|_Q}\\
&=
\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}
\sum_{\substack{\sigma:P\to\{1,2,3,\ldots\};\\
\tau:Q\to\{1,2,3,\ldots\};\\
\sigma\text{ is a }(P,>_1,<_{2})\text{-partition};\\
\tau\text{ is a }(Q,<_{1},<_{2})\text{-partition}}}
x_{\sigma,w|_P}x_{\tau,w|_Q}\\
&=
\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}
\sum_{\substack{\pi:E\to\{1,2,3,\ldots\};\\
\pi|_P\text{ is a }(P,>_1,<_{2})\text{-partition};\\
\pi|_Q\text{ is a }(Q,<_{1},<_{2})\text{-partition}}}
\underbrace{x_{\pi|_P,w|_P}x_{\pi|_Q,w|_Q}}_{=x_{\pi,w}}\\
&\quad\left(
\begin{gathered}
\text{here, we have substituted }(\pi|_P,\pi|_Q)\text{ for }(\sigma,\tau)\text{ in the inner sum,}\\
\text{since every pair }(\sigma,\tau)\text{ consisting of a map }\sigma:P\to\{1,2,3,\ldots\}\\
\text{and a map }\tau:Q\to\{1,2,3,\ldots\}\\
\text{can be written as }(\pi|_P,\pi|_Q)\text{ for a unique }\pi:E\to\{1,2,3,\ldots\}\\
\text{(namely, for the }\pi:E\to\{1,2,3,\ldots\}\text{ that is defined to send every}\\
e\in P\text{ to }\sigma(e)\text{ and to send every }e\in Q\text{ to }\tau(e)\text{)}
\end{gathered}
\right)\\
&=
\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}
\sum_{\substack{\pi:E\to\{1,2,3,\ldots\};\\
\pi|_P\text{ is a }(P,>_1,<_{2})\text{-partition};\\
\pi|_Q\text{ is a }(Q,<_{1},<_{2})\text{-partition}}}
x_{\pi,w}\\
&=
\sum_{\pi:E\to\{1,2,3,\ldots\}}
\underbrace{\sum_{\substack{(P,Q)\in\operatorname{Adm} E;\\
\pi|_P\text{ is a }(P,>_1,<_{2})\text{-partition};\\
\pi|_Q\text{ is a }(Q,<_{1},<_{2})\text{-partition}}}
(-1)^{|P|}}_{ =0\text{ (by {xref}`(19)`)}
x_{\pi,w}
=
\sum_{\pi:E\to\{1,2,3,\ldots\}}0x_{\pi,w}
=
0.}}
Thus,
0 = ∑ ( P , Q ) ∈ Adm E ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ∣ E ) Γ ( E ∣ ∅ , w ∣ ∅ ) + ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) \begin{aligned}
0={}&\sum_{(P,Q)\in\operatorname{Adm} E}(-1)^{|P|}\Gamma\bigl((P,>_1,<_{2}),w|_P\bigr)\Gamma\bigl(E|_Q,w|_Q\bigr)\\
={}&(-1)^{|E|}\Gamma\bigl((E,>_1,<_{2}),w|_E\bigr)\Gamma\bigl(E|_{\varnothing},w|_{\varnothing}\bigr)\\
&+\sum_{\substack{(P,Q)\in\operatorname{Adm} E;\\|P|<|E|}}(-1)^{|P|}\Gamma\bigl((P,>_1,<_{2}),w|_P\bigr)\Gamma\bigl(E|_Q,w|_Q\bigr)
\end{aligned} 0 = = ( P , Q ) ∈ Adm E ∑ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ∣ E ) Γ ( E ∣ ∅ , w ∣ ∅ ) + ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q )
because the only pair ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E satisfying ∣ P ∣ ≥ ∣ E ∣ |P|\geq|E| ∣ P ∣ ≥ ∣ E ∣ is ( P , Q ) = ( E , ∅ ) (P,Q)=(E,\varnothing) ( P , Q ) = ( E , ∅ ) , whereas all other pairs ( P , Q ) ∈ Adm E (P,Q)\in\operatorname{Adm} E ( P , Q ) ∈ Adm E satisfy ∣ P ∣ < ∣ E ∣ |P|<|E| ∣ P ∣ < ∣ E ∣
= ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) + ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) , \begin{aligned}
={}&(-1)^{|E|}\Gamma\bigl((E,>_1,<_{2}),w\bigr)\\
&+\sum_{\substack{(P,Q)\in\operatorname{Adm} E;\\|P|<|E|}}(-1)^{|P|}\Gamma\bigl((P,>_1,<_{2}),w|_P\bigr)\Gamma\bigl(E|_Q,w|_Q\bigr),
\end{aligned} = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) + ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) ,
so that
( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) = − ∑ ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) = S ( Γ ( ( E ⏟ = ( E , < 1 , < 2 ) , w ) ) ) (by (26)) = S ( Γ ( ( E , < 1 , < 2 ) , w ) ) , \begin{aligned}
(-1)^{|E|}\Gamma\bigl((E,>_1,<_{2}),w\bigr)
=
-\sum_{\substack{(P,Q)\in\operatorname{Adm} E;\\|P|<|E|}}(-1)^{|P|}\Gamma\bigl((P,>_1,<_{2}),w|_P\bigr)\Gamma\bigl(E|_Q,w|_Q\bigr) \\
&=S\left(\Gamma\left(\left(\underbrace{E}_{=(E,<_{1},<_{2})},w\right)\right)\right)\qquad\text{(by (26))} \\
&=S\bigl(\Gamma((E,<_{1},<_{2}),w)\bigr),
\end{aligned} ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) = − ( P , Q ) ∈ Adm E ; ∣ P ∣ < ∣ E ∣ ∑ ( − 1 ) ∣ P ∣ Γ ( ( P , > 1 , < 2 ) , w ∣ P ) Γ ( E ∣ Q , w ∣ Q ) = S Γ = ( E , < 1 , < 2 ) E , w (by (26)) = S ( Γ (( E , < 1 , < 2 ) , w ) ) ,
and thus S ( Γ ( ( E , < 1 , < 2 ) , w ) ) = ( − 1 ) ∣ E ∣ Γ ( ( E , > 1 , < 2 ) , w ) S\bigl(\Gamma((E,<_{1},<_{2}),w)\bigr)=(-1)^{|E|}\Gamma((E,>_{1},<_{2}),w) S ( Γ (( E , < 1 , < 2 ) , w ) ) = ( − 1 ) ∣ E ∣ Γ (( E , > 1 , < 2 ) , w ) . This completes the induction step and thus the proof of Theorem 4.2.
Proof of Theorem 4.7
Before we begin proving Theorem 4.7, we state a criterion for E-partitions that is less wasteful (in the sense that it requires fewer verifications) than the definition:
Lemma 7.1. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset. Let ϕ : E → { 1 , 2 , 3 , … } \phi:E\to\{1,2,3,\ldots\} ϕ : E → { 1 , 2 , 3 , … } be a map. Assume that the following two conditions hold:
Condition 1: If e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E are such that e e e is < 1 <_{1} < 1 -covered by f f f , and if we have e < 2 f e<_{2}f e < 2 f , then ϕ ( e ) ≤ ϕ ( f ) \phi(e)\leq\phi(f) ϕ ( e ) ≤ ϕ ( f ) .
Condition 2: If e ∈ E e\in E e ∈ E and f ∈ E f\in E f ∈ E are such that e e e is < 1 <_{1} < 1 -covered by f f f , and if we have f < 2 e f<_{2}e f < 2 e , then ϕ ( e ) < ϕ ( f ) \phi(e)<\phi(f) ϕ ( e ) < ϕ ( f ) .
Then, ϕ \phi ϕ is an E-partition.
Proof of Lemma 7.1. For any a ∈ E a \in E a ∈ E and b ∈ E b \in E b ∈ E , we define a subset [ a , b ] [a,b] [ a , b ] of E E E as in the proof of Lemma 6.1.
We need to show that ϕ \phi ϕ is an E-partition. In other words, we need to prove the following two claims:
Claim 1: Every e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E satisfying e < 1 f e <_1 f e < 1 f satisfy ϕ ( e ) ≤ ϕ ( f ) \phi(e) \leq\phi(f) ϕ ( e ) ≤ ϕ ( f ) .
Claim 2: Every e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E satisfying e < 1 f e <_1 f e < 1 f and f < 2 e f <_2 e f < 2 e satisfy ϕ ( e ) < ϕ ( f ) \phi(e) < \phi(f) ϕ ( e ) < ϕ ( f ) .
Proof of Claim 1: Assume the contrary. Thus, there exists a pair ( e , f ) ∈ E × E (e,f) \in E \times E ( e , f ) ∈ E × E satisfying e < 1 f e <_1 f e < 1 f but not ϕ ( e ) ≤ ϕ ( f ) \phi(e) \leq\phi(f) ϕ ( e ) ≤ ϕ ( f ) . Such a pair will be called a malrelation . Fix a malrelation ( u , v ) (u,v) ( u , v ) for which the value ∣ [ u , v ] ∣ |[u,v]| ∣ [ u , v ] ∣ is minimum (such a ( u , v ) (u,v) ( u , v ) exists, since there exists a malrelation). Thus, u ∈ E u \in E u ∈ E and v ∈ E v \in E v ∈ E and u < 1 v u <_1 v u < 1 v but not ϕ ( u ) ≤ ϕ ( v ) \phi(u) \leq\phi(v) ϕ ( u ) ≤ ϕ ( v ) .
If u u u was < 1 <_1 < 1 -covered by v v v , then we would obtain ϕ ( u ) ≤ ϕ ( v ) \phi(u) \leq\phi(v) ϕ ( u ) ≤ ϕ ( v ) 35 , which would contradict the fact that we do not have ϕ ( u ) ≤ ϕ ( v ) \phi(u) \leq\phi(v) ϕ ( u ) ≤ ϕ ( v ) . Hence, u u u is not < 1 <_1 < 1 -covered by v v v . Consequently, there exists a w ∈ E w \in E w ∈ E such that u < 1 w < 1 v u <_1 w <_1 v u < 1 w < 1 v (since u < 1 v u <_1 v u < 1 v ). Consider this w w w . Applying (13) to a = u a=u a = u , c = w c=w c = w and b = v b=v b = v , we see that both numbers ∣ [ u , w ] ∣ |[u,w]| ∣ [ u , w ] ∣ and ∣ [ w , v ] ∣ |[w,v]| ∣ [ w , v ] ∣ are smaller than ∣ [ u , v ] ∣ |[u,v]| ∣ [ u , v ] ∣ . Hence, neither ( u , w ) (u,w) ( u , w ) nor ( w , v ) (w,v) ( w , v ) is a malrelation (since we picked ( u , v ) (u,v) ( u , v ) to be a malrelation with minimum ∣ [ u , v ] ∣ |[u,v]| ∣ [ u , v ] ∣ ). Therefore, we have ϕ ( u ) ≤ ϕ ( w ) \phi(u) \leq\phi(w) ϕ ( u ) ≤ ϕ ( w ) (since u < 1 w u <_1 w u < 1 w , but ( u , w ) (u,w) ( u , w ) is not a malrelation) and ϕ ( w ) ≤ ϕ ( v ) \phi(w) \leq\phi(v) ϕ ( w ) ≤ ϕ ( v ) (since w < 1 v w <_1 v w < 1 v , but ( w , v ) (w,v) ( w , v ) is not a malrelation). Combining these two inequalities, we obtain ϕ ( u ) ≤ ϕ ( w ) ≤ ϕ ( v ) \phi(u) \leq\phi(w) \leq\phi(v) ϕ ( u ) ≤ ϕ ( w ) ≤ ϕ ( v ) . This contradicts the fact that we do not have ϕ ( u ) ≤ ϕ ( v ) \phi(u) \leq\phi(v) ϕ ( u ) ≤ ϕ ( v ) . This contradiction concludes the proof of Claim 1.
Instead of Claim 2, we shall prove the following stronger claim:
Claim 3: Every e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E satisfying e < 1 f e <_1 f e < 1 f and not e < 2 f e <_2 f e < 2 f satisfy ϕ ( e ) < ϕ ( f ) \phi(e) < \phi(f) ϕ ( e ) < ϕ ( f ) .
Proof of Claim 3: Assume the contrary. Thus, there exists a pair ( e , f ) ∈ E × E (e,f) \in E \times E ( e , f ) ∈ E × E satisfying e < 1 f e <_1 f e < 1 f and not e < 2 f e <_2 f e < 2 f but not ϕ ( e ) < ϕ ( f ) \phi(e) < \phi(f) ϕ ( e ) < ϕ ( f ) . Such a pair will be called a malrelation . Fix a malrelation ( u , v ) (u,v) ( u , v ) for which the value ∣ [ u , v ] ∣ |[u,v]| ∣ [ u , v ] ∣ is minimum (such a ( u , v ) (u,v) ( u , v ) exists, since there exists a malrelation). Thus, u ∈ E u \in E u ∈ E and v ∈ E v \in E v ∈ E and u < 1 v u <_1 v u < 1 v and not u < 2 v u <_2 v u < 2 v but not ϕ ( u ) < ϕ ( v ) \phi(u) < \phi(v) ϕ ( u ) < ϕ ( v ) . If u u u was < 1 <_{1} < 1 -covered by v v v , then we would obtain ϕ ( u ) < ϕ ( v ) \phi(u)<\phi(v) ϕ ( u ) < ϕ ( v ) easily36 , which would contradict the fact that we do not have ϕ ( u ) < ϕ ( v ) \phi(u)<\phi(v) ϕ ( u ) < ϕ ( v ) . Hence, u u u is not < 1 <_{1} < 1 -covered by v v v . Consequently, there exists a w ∈ E w\in E w ∈ E such that u < 1 w < 1 v u<_{1}w<_{1}v u < 1 w < 1 v (since u < 1 v u<_{1}v u < 1 v ). Consider this w w w . Applying (13) to a = u a=u a = u , c = w c=w c = w and b = v b=v b = v , we see that both numbers ∣ [ u , w ] ∣ \lvert[u,w]\rvert ∣[ u , w ]∣ and ∣ [ w , v ] ∣ \lvert[w,v]\rvert ∣[ w , v ]∣ are smaller than ∣ [ u , v ] ∣ \lvert[u,v]\rvert ∣[ u , v ]∣ . Hence, neither ( u , w ) (u,w) ( u , w ) nor ( w , v ) (w,v) ( w , v ) is a malrelation (since we picked ( u , v ) (u,v) ( u , v ) to be a malrelation with minimum ∣ [ u , v ] ∣ \lvert[u,v]\rvert ∣[ u , v ]∣ ).
But ϕ ( v ) ≤ ϕ ( u ) \phi(v)\leq\phi(u) ϕ ( v ) ≤ ϕ ( u ) (since we do not have ϕ ( u ) < ϕ ( v ) \phi(u)<\phi(v) ϕ ( u ) < ϕ ( v ) ). On the other hand, u < 1 w u<_{1}w u < 1 w and therefore ϕ ( u ) ≤ ϕ ( w ) \phi(u)\leq\phi(w) ϕ ( u ) ≤ ϕ ( w ) (by Claim 1, applied to e = u e=u e = u and f = w f=w f = w ). Furthermore, w < 1 v w<_{1}v w < 1 v and thus ϕ ( w ) ≤ ϕ ( v ) \phi(w)\leq\phi(v) ϕ ( w ) ≤ ϕ ( v ) (by Claim 1, applied to e = w e=w e = w and f = v f=v f = v ). The chain of inequalities ϕ ( v ) ≤ ϕ ( u ) ≤ ϕ ( w ) ≤ ϕ ( v ) \phi(v)\leq\phi(u)\leq\phi(w)\leq\phi(v) ϕ ( v ) ≤ ϕ ( u ) ≤ ϕ ( w ) ≤ ϕ ( v ) ends with the same term that it begins with; therefore, it must be a chain of equalities. In other words, we have ϕ ( v ) = ϕ ( u ) = ϕ ( w ) = ϕ ( v ) \phi(v)=\phi(u)=\phi(w)=\phi(v) ϕ ( v ) = ϕ ( u ) = ϕ ( w ) = ϕ ( v ) .
Now, using ϕ ( w ) = ϕ ( v ) \phi(w)=\phi(v) ϕ ( w ) = ϕ ( v ) , we can see that w < 2 v w<_{2}v w < 2 v 37 . The same argument (applied to u u u and w w w instead of w w w and v v v ) shows that u < 2 w u<_{2}w u < 2 w . Thus, u < 2 w < 2 v u<_{2}w<_{2}v u < 2 w < 2 v , which contradicts the fact that we do not have u < 2 v u<_{2}v u < 2 v . This contradiction proves Claim 3.
Proof of Claim 2. The condition “f < 2 e f<_{2}e f < 2 e ” is stronger than “not e < 2 f e<_{2}f e < 2 f ”. Thus, Claim 2 follows from Claim 3.
Claims 1 and 2 are now both proven, and so Lemma 7.1 follows.
Proof of Lemma 4.5 . Consider the following three logical statements:
Statement 1: The G G G -orbit O O O is E E E -coeven.
Statement 2: All elements of O O O are E E E -coeven.
Statement 3: At least one element of O O O is E E E -coeven.
Statements 1 and 2 are equivalent (according to the definition of when a G G G -orbit is E E E -coeven). Our goal is to prove that Statements 1 and 3 are equivalent (because this is precisely what Lemma 4.5 says). Thus, it suffices to show that Statements 2 and 3 are equivalent (because we already know that Statements 1 and 2 are equivalent). Since Statement 2 obviously implies Statement 3 (in fact, the G G G -orbit O O O contains at least one element), we therefore only need to show that Statement 3 implies Statement 2. Thus, assume that Statement 3 holds. We need to prove that Statement 2 holds.
There exists at least one E E E -coeven ϕ ∈ O \phi\in O ϕ ∈ O (because we assumed that Statement 3 holds). Consider this ϕ \phi ϕ . Now, let π ∈ O \pi\in O π ∈ O be arbitrary. We shall show that π \pi π is E E E -coeven. We know that ϕ \phi ϕ is E E E -coeven. In other words,
every g ∈ G satisfying g ϕ = ϕ is E -even . (29) \text{every }g \in G\text{ satisfying }g\phi=\phi\text{ is }E\text{-even}. \tag*{(29)} every g ∈ G satisfying g ϕ = ϕ is E -even . (29)
Now, let g ∈ G g \in G g ∈ G be such that g π = π g\pi=\pi g π = π . Since ϕ \phi ϕ belongs to the G G G -orbit O O O , we have O = G ϕ O=G\phi O = Gϕ . Now, π ∈ O = G ϕ \pi\in O=G\phi π ∈ O = Gϕ . In other words, there exists some h ∈ G h \in G h ∈ G such that π = h ϕ \pi=h\phi π = h ϕ . Consider this h h h . We have g π = π g\pi=\pi g π = π . Since π = h ϕ \pi=h\phi π = h ϕ , this rewrites as g h ϕ = h ϕ gh\phi=h\phi g h ϕ = h ϕ . In other words, h − 1 g h ϕ = ϕ h^{-1}gh\phi=\phi h − 1 g h ϕ = ϕ . Thus, (29) (applied to h − 1 g h h^{-1}gh h − 1 g h instead of g g g ) shows that h − 1 g h h^{-1}gh h − 1 g h is E E E -even. In other words,
the action of h − 1 g h on E is an even permutation of E . (30) \text{the action of }h^{-1}gh\text{ on }E\text{ is an even permutation of }E. \tag*{(30)} the action of h − 1 g h on E is an even permutation of E . (30)
Now, let ε \varepsilon ε be the group homomorphism from G G G to Aut E \operatorname{Aut} E Aut E 38 which describes the G G G -action on E E E . Then, ε ( h − 1 g h ) \varepsilon(h^{-1}gh) ε ( h − 1 g h ) is the action of h − 1 g h h^{-1}gh h − 1 g h on E E E , and thus is an even permutation of E E E (by (30)).
But since ε \varepsilon ε is a group homomorphism, we have ε ( h − 1 g h ) = ε ( h ) − 1 ε ( g ) ε ( h ) \varepsilon(h^{-1}gh)=\varepsilon(h)^{-1}\varepsilon(g)\varepsilon(h) ε ( h − 1 g h ) = ε ( h ) − 1 ε ( g ) ε ( h ) . Thus, the permutations ε ( h − 1 g h ) \varepsilon(h^{-1}gh) ε ( h − 1 g h ) and ε ( g ) \varepsilon(g) ε ( g ) of E E E are conjugate. Since the permutation ε ( h − 1 g h ) \varepsilon(h^{-1}gh) ε ( h − 1 g h ) is even, this shows that the permutation ε ( g ) \varepsilon(g) ε ( g ) is even. In other words, the action of g g g on E E E is an even permutation of E E E . In other words, g g g is E E E -even.
Now, let us forget that we fixed g g g . We thus have shown that every g ∈ G g \in G g ∈ G satisfying g π = π g\pi=\pi g π = π is E E E -even. In other words, π \pi π is E E E -coeven.
Let us now forget that we fixed π \pi π . Thus, we have proven that every π ∈ O \pi\in O π ∈ O is E E E -coeven. In other words, Statement 2 holds. We have thus shown that Statement 3 implies Statement 2. Consequently, Statements 2 and 3 are equivalent, and so the proof of Lemma 4.5 is complete. □
We leave the fairly straightforward proof of Proposition 4.6 to the reader. Next, we will show three simple properties of posets on which groups act. First, we introduce a notation:
Definition 7.2. Let G G G be a group. Let g ∈ G g \in G g ∈ G . Let E E E be a G G G -set. Then, the subgroup ⟨ g ⟩ \langle g\rangle ⟨ g ⟩ of G G G (this is the subgroup of G G G generated by g g g ) also acts on E E E . The ⟨ g ⟩ \langle g\rangle ⟨ g ⟩ -orbits on E E E will be called the g g g -orbits on E E E . When E E E is clear from the context, we shall simply call them the g g g -orbits.
We can also describe these g g g -orbits explicitly: For any given e ∈ E e \in E e ∈ E , the g g g -orbit of e e e (that is, the unique g g g -orbit that contains e e e ) is ⟨ g ⟩ e = { g k e ∣ k ∈ Z } \langle g\rangle e=\{g^k e\mid k\in\mathbb{Z}\} ⟨ g ⟩ e = { g k e ∣ k ∈ Z } . Equivalently, the g g g -orbits on E E E can be characterized as follows: The action of g g g on E E E is a permutation of E E E . The cycles of this permutation are the g g g -orbits on E E E (at least when E E E is finite).
Proposition 7.3. Let E E E be a set. Let < 1 <_1 < 1 be a strict partial order on E E E . Let G G G be a finite group which acts on E E E . Assume that G G G preserves the relation < 1 <_1 < 1 .
Let g ∈ G g \in G g ∈ G . Let E g E^g E g be the set of all g g g -orbits on E E E . Define a binary relation < 1 g <^g_1 < 1 g on E g E^g E g by
( u < 1 g v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 1 b ) . (u <^g_1 v) \Longleftrightarrow(\text{there exist } a \in u \text{ and } b \in v \text{ with } a <_1 b). ( u < 1 g v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 1 b ) .
Then, < 1 g <^g_1 < 1 g is a strict partial order.
Proposition 7.3 is precisely [15 Lemma 2.4] , but let us outline the proof for the sake of completeness:
Proof of Proposition 7.3. Let us first show that the relation < 1 g <^g_1 < 1 g is irreflexive. Indeed, assume the contrary. Thus, there exists a u ∈ E g u \in E^g u ∈ E g such that u < 1 g u u <^g_1 u u < 1 g u . Consider this u u u .
We have u ∈ E g u \in E^g u ∈ E g . In other words, u u u is a g g g -orbit on E E E .
Since u < 1 g u u <^g_1 u u < 1 g u , there exist a ∈ u a \in u a ∈ u and b ∈ u b \in u b ∈ u with a < 1 b a <_1 b a < 1 b (by the definition of the relation < 1 g <^g_1 < 1 g ). Consider these a a a and b b b . There exists a k ∈ Z k \in\mathbb{Z} k ∈ Z such that b = g k a b = g^k a b = g k a (since a a a and b b b both lie in one and the same g g g -orbit u u u ). Consider this k k k .
Each element of G G G has finite order (since G G G is a finite group). In particular, the element g g g of G G G has finite order. In other words, there exists a positive integer n n n such that g n = 1 G g^n = 1_G g n = 1 G . Consider this n n n . Every p ∈ Z p \in\mathbb{Z} p ∈ Z satisfies g n p = ( g n ) p = 1 G g^{np} = (g^n)^p = 1_G g n p = ( g n ) p = 1 G (since g n = 1 G g^n = 1_G g n = 1 G ). Applying this to p = k p = k p = k , we obtain g n k = 1 G g^{nk} = 1_G g nk = 1 G .
Now, a < 1 b = g k a a <_1 b = g^k a a < 1 b = g k a . Since G G G preserves the relation < 1 <_1 < 1 , this shows that h a < 1 h g k a ha <_1 hg^k a ha < 1 h g k a for every h ∈ G h \in G h ∈ G . Thus, g ℓ k a < 1 g ℓ k g k a g^{\ell k}a <_1 g^{\ell k}g^k a g ℓ k a < 1 g ℓ k g k a for every ℓ ∈ N \ell\in\mathbb{N} ℓ ∈ N . Hence, g ℓ k a < 1 g ℓ k g k a = g ( ℓ + 1 ) k a g^{\ell k}a <_1 g^{\ell k}g^k a = g^{(\ell+1)k}a g ℓ k a < 1 g ℓ k g k a = g ( ℓ + 1 ) k a for every ℓ ∈ N \ell\in\mathbb{N} ℓ ∈ N . Consequently, g 0 k a < 1 g 1 k a < 1 g 2 k a < 1 ⋯ < 1 g n k a g^{0k}a <_1 g^{1k}a <_1 g^{2k}a <_1 \cdots<_1 g^{nk}a g 0 k a < 1 g 1 k a < 1 g 2 k a < 1 ⋯ < 1 g nk a . Thus, g 0 k a < 1 g n k a ⏟ = 1 G a = a g^{0k}a <_1 \underbrace{g^{nk}a}_{=1_Ga=a} g 0 k a < 1 = 1 G a = a g nk a , which contradicts g 0 k ⏟ = g 0 = 1 G a = 1 G a = a \underbrace{g^{0k}}_{=g^0=1_G}a = 1_Ga = a = g 0 = 1 G g 0 k a = 1 G a = a . This contradiction proves that our assumption was wrong. Hence, the relation < 1 g <^g_1 < 1 g is irreflexive.
Let us next show that the relation < 1 g <^g_1 < 1 g is transitive. Indeed, let u u u , v v v and w w w be three elements of E g E^g E g such that u < 1 g v u <^g_1 v u < 1 g v and v < 1 g w v <^g_1 w v < 1 g w . We must prove that u < 1 g w u <^g_1 w u < 1 g w .
There exist a ∈ u a \in u a ∈ u and b ∈ v b \in v b ∈ v with a < 1 b a <_1 b a < 1 b (since u < 1 g v u <^g_1 v u < 1 g v ). Consider these a a a and $b.
There exist a ′ ∈ v a' \in v a ′ ∈ v and b ′ ∈ w b' \in w b ′ ∈ w with a ′ < 1 b ′ a' <_1 b' a ′ < 1 b ′ (since v < 1 g w v <^g_1 w v < 1 g w ). Consider these a ′ a' a ′ and b ′ b' b ′ .
The set v v v is a g g g -orbit (since v ∈ E g v \in E^g v ∈ E g ). The elements b b b and a ′ a' a ′ lie in one and the same g g g -orbit (namely, in v v v ). Hence, there exists some k ∈ Z k \in\mathbb{Z} k ∈ Z such that a ′ = g k b a' = g^k b a ′ = g k b . Consider this k k k . We have a < 1 b a <_1 b a < 1 b and thus g k a < 1 g k b g^k a <_1 g^k b g k a < 1 g k b (since G G G preserves the relation < 1 <_1 < 1 ). Hence, g k a < 1 g k b = a ′ < 1 b ′ g^k a <_1 g^k b = a' <_1 b' g k a < 1 g k b = a ′ < 1 b ′ . Since g k a ∈ u g^k a \in u g k a ∈ u (because a ∈ u a \in u a ∈ u , and because u u u is a g g g -orbit) and b ′ ∈ w b' \in w b ′ ∈ w , this shows that u < 1 g w u <^g_1 w u < 1 g w (by the definition of the relation < 1 g <^g_1 < 1 g ). We thus have proven that the relation < 1 g <^g_1 < 1 g is transitive.
Now, we know that the relation < 1 g <^g_1 < 1 g is irreflexive and transitive, and thus also antisymmetric (since every irreflexive and transitive binary relation is antisymmetric). In other words, < 1 g <^g_1 < 1 g is a strict partial order. This proves Proposition 7.3.
Remark 7.4. Proposition 7.3 can be generalized: Let E E E be a set. Let < 1 <_{1} < 1 be a strict partial order on E E E . Let G G G be a finite group which acts on E E E . Assume that G G G preserves the relation < 1 <_{1} < 1 . Let H H H be a subgroup of G G G . Let E H E^{H} E H be the set of all H H H -orbits on E E E . Define a binary relation < 1 H <^{H}_{1} < 1 H on E H E^{H} E H by
( u < 1 H v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 1 b ) . \left(u <^{H}_{1} v\right) \Longleftrightarrow\left(\text{there exist }a \in u\text{ and }b \in v\text{ with }a <_{1} b\right). ( u < 1 H v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 1 b ) .
Then, < 1 H <^{H}_{1} < 1 H is a strict partial order. This result (whose proof is quite similar to that of Proposition 7.3 ) implicitly appears in [27 p. 30] .
Proposition 7.5. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset. Let G G G be a finite group which acts on E E E . Assume that G G G preserves both relations < 1 <_{1} < 1 and < 2 <_{2} < 2 . Let g ∈ G g \in G g ∈ G . Let E g E^{g} E g be the set of all g g g -orbits on E E E . Define a binary relation < 1 g <^{g}_{1} < 1 g on E g E^{g} E g by
( u < 1 g v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 1 b ) . \left(u <^{g}_{1} v\right) \Longleftrightarrow\left(\text{there exist }a \in u\text{ and }b \in v\text{ with }a <_{1} b\right). ( u < 1 g v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 1 b ) . Define a binary relation < 2 g <^{g}_{2} < 2 g on E g E^{g} E g by
( u < 2 g v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 2 b ) . \left(u <^{g}_{2} v\right) \Longleftrightarrow\left(\text{there exist }a \in u\text{ and }b \in v\text{ with }a <_{2} b\right). ( u < 2 g v ) ⟺ ( there exist a ∈ u and b ∈ v with a < 2 b ) . Let E g E^{g} E g be the triple ( E g , < 1 g , < 2 g ) (E^{g},<^{g}_{1},<^{g}_{2}) ( E g , < 1 g , < 2 g ) . Then, E g E^{g} E g is a tertispecial double poset.
Proof of Proposition 7.5. Proposition 7.3 shows that < 1 g <^{g}_{1} < 1 g is a strict partial order. Similarly, < 2 g <^{g}_{2} < 2 g is a strict partial order. Thus, E g = ( E g , < 1 g , < 2 g ) E^{g}=(E^{g},<^{g}_{1},<^{g}_{2}) E g = ( E g , < 1 g , < 2 g ) is a double poset. It remains to show that this double poset E g E^{g} E g is tertispecial.
Let u u u and v v v be two elements of E g E^{g} E g such that u u u is < 1 g <^{g}_{1} < 1 g -covered by v v v . We shall prove that u u u and v v v are < 2 g <^{g}_{2} < 2 g -comparable.
We have u < 1 g v u <^{g}_{1} v u < 1 g v (since u u u is < 1 g <^{g}_{1} < 1 g -covered by v v v ). In other words, there exist a ∈ u a \in u a ∈ u and b ∈ v b \in v b ∈ v with a < 1 b a <_{1} b a < 1 b (by the definition of the relation < 1 g <^{g}_{1} < 1 g ). Consider these a a a and b b b .
If there was a c ∈ E c \in E c ∈ E satisfying a < 1 c < 1 b a <_{1} c <_{1} b a < 1 c < 1 b , then we would have u < 1 g w < 1 g v u <^{g}_{1} w <^{g}_{1} v u < 1 g w < 1 g v with w w w being the g g g -orbit of c c c , and this would contradict the condition that u u u is < 1 g <^{g}_{1} < 1 g -covered by v v v . Hence, no such c c c can exist. In other words, a a a is < 1 <_{1} < 1 -covered by b b b (since we know that a < 1 b a <_{1} b a < 1 b ). Thus, a a a and b b b are < 2 <_{2} < 2 -comparable (since the double poset E E E is tertispecial). Consequently, u u u and v v v are < 2 g <^{g}_{2} < 2 g -comparable.
Now, let us forget that we fixed u u u and v v v . We thus have shown that if u u u and v v v are two elements of E g E^{g} E g such that u u u is < 1 g <^{g}_{1} < 1 g -covered by v v v , then u u u and v v v are < 2 g <^{g}_{2} < 2 g -comparable. In other words, the double poset E g = ( E g , < 1 g , < 2 g ) E^{g}=(E^{g},<^{g}_{1},<^{g}_{2}) E g = ( E g , < 1 g , < 2 g ) is tertispecial. This proves Proposition 7.5.
Proposition 7.6. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset. Let G G G be a finite group which acts on E E E . Assume that G G G preserves both relations < 1 <_{1} < 1 and < 2 <_{2} < 2 .
Let g ∈ G g\in G g ∈ G . Define the set E g E^{g} E g , the relations < 1 g <_{1}^{g} < 1 g and < 2 g <_{2}^{g} < 2 g and the triple E g E^{g} E g as in Proposition 7.5. Thus, E g E^{g} E g is a tertispecial double poset (by Proposition 7.5).
There is a bijection Φ \Phi Φ between
the maps π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying g π = π g\pi=\pi g π = π
and
the maps π ‾ : E g → { 1 , 2 , 3 , … } \overline{\pi}:E^{g}\to\{1,2,3,\ldots\} π : E g → { 1 , 2 , 3 , … } .
Namely, this bijection Φ \Phi Φ sends any map π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying g π = π g\pi=\pi g π = π to the map π ‾ : E g → { 1 , 2 , 3 , … } \overline{\pi}:E^{g}\to\{1,2,3,\ldots\} π : E g → { 1 , 2 , 3 , … } defined by
π ‾ ( u ) = π ( a ) for every u ∈ E g and a ∈ u . \overline{\pi}(u)=\pi(a)\qquad\text{for every }u\in E^{g}\text{ and }a\in u. π ( u ) = π ( a ) for every u ∈ E g and a ∈ u . (The well-definedness of this map π ‾ \overline{\pi} π is easy to see: Indeed, from g π = π g\pi=\pi g π = π , we can conclude that any two elements a 1 a_{1} a 1 and a 2 a_{2} a 2 of a given g g g -orbit u u u satisfy π ( a 1 ) = π ( a 2 ) . \pi(a_{1})=\pi(a_{2}). π ( a 1 ) = π ( a 2 ) . )
Consider this bijection Φ \Phi Φ . Let π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } be a map satisfying g π = π g\pi=\pi g π = π .
(a) If π \pi π is an E E E -partition, then Φ ( π ) \Phi(\pi) Φ ( π ) is an E g E^{g} E g -partition.
(b) If Φ ( π ) \Phi(\pi) Φ ( π ) is an E g E^{g} E g -partition, then π \pi π is an E E E -partition.
(c) Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } be a map. Define a map w g : E g → { 1 , 2 , 3 , … } w^{g}:E^{g}\to\{1,2,3,\ldots\} w g : E g → { 1 , 2 , 3 , … } by
w g ( u ) = ∑ a ∈ u w ( a ) for every u ∈ E g . w^{g}(u)=\sum_{a\in u}w(a)\qquad\text{for every }u\in E^{g}. w g ( u ) = a ∈ u ∑ w ( a ) for every u ∈ E g . Then, x Φ ( π ) , w g = x π , w x_{\Phi(\pi),w^{g}}=x_{\pi,w} x Φ ( π ) , w g = x π , w .
Proof of Proposition 7.6 (sketched). The definition of Φ \Phi Φ shows that
( Φ ( π ) ) ( u ) = π ( a ) for every u ∈ E g and a ∈ u . (31) (\Phi(\pi))(u)=\pi(a)\qquad\text{for every }u\in E^{g}\text{ and }a\in u. \tag*{(31)} ( Φ ( π )) ( u ) = π ( a ) for every u ∈ E g and a ∈ u . (31)
(a) Assume that π \pi π is an E E E -partition. We want to show that Φ ( π ) \Phi(\pi) Φ ( π ) is an E g E^{g} E g -partition. In order to do so, we can use Lemma 7.1 (applied to E g E^{g} E g , ( E g , < 1 g , < 2 g ) (E^{g},<_{1}^{g},<_{2}^{g}) ( E g , < 1 g , < 2 g ) and Φ ( π ) \Phi(\pi) Φ ( π ) instead of E E E , ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) and ϕ \phi ϕ ); we only need to check the following two conditions:
Condition 1: If e ∈ E g e\in E^{g} e ∈ E g and f ∈ E g f\in E^{g} f ∈ E g are such that e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f , and if we have e < 2 g f e<_{2}^{g}f e < 2 g f , then ( Φ ( π ) ) ( e ) ≤ ( Φ ( π ) ) ( f ) (\Phi(\pi))(e)\leq(\Phi(\pi))(f) ( Φ ( π )) ( e ) ≤ ( Φ ( π )) ( f ) .
Condition 2: If e ∈ E g e\in E^{g} e ∈ E g and f ∈ E g f\in E^{g} f ∈ E g are such that e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f , and if we have f < 2 g e f<_{2}^{g}e f < 2 g e , then ( Φ ( π ) ) ( e ) < ( Φ ( π ) ) ( f ) (\Phi(\pi))(e)<(\Phi(\pi))(f) ( Φ ( π )) ( e ) < ( Φ ( π )) ( f ) . end_mid=1 Proof of Condition 1: Let e ∈ E g e \in E^{g} e ∈ E g and f ∈ E g f \in E^{g} f ∈ E g be such that e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f . Assume that we have e < 2 g f e <_{2}^{g} f e < 2 g f .
We have e < 1 g f e <_{1}^{g} f e < 1 g f (because e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f ). In other words, there exist a ∈ e a \in e a ∈ e and b ∈ f b \in f b ∈ f satisfying a < 1 b a <_{1} b a < 1 b . Consider these a a a and b b b . Since π \pi π is an E E E -partition, we have π ( a ) ≤ π ( b ) \pi(a) \leq\pi(b) π ( a ) ≤ π ( b ) (since a < 1 b a <_{1} b a < 1 b ). But the definition of Φ ( π ) \Phi(\pi) Φ ( π ) shows that ( Φ ( π ) ) ( e ) = π ( a ) (\Phi(\pi))(e) = \pi(a) ( Φ ( π )) ( e ) = π ( a ) (since a ∈ e a \in e a ∈ e ) and ( Φ ( π ) ) ( f ) = π ( b ) (\Phi(\pi))(f) = \pi(b) ( Φ ( π )) ( f ) = π ( b ) (since b ∈ f b \in f b ∈ f ). Thus, ( Φ ( π ) ) ( e ) = π ( a ) ≤ π ( b ) = ( Φ ( π ) ) ( f ) (\Phi(\pi))(e) = \pi(a) \leq\pi(b) = (\Phi(\pi))(f) ( Φ ( π )) ( e ) = π ( a ) ≤ π ( b ) = ( Φ ( π )) ( f ) . Hence, Condition 1 is proven.
Proof of Condition 2: Let e ∈ E g e \in E^{g} e ∈ E g and f ∈ E g f \in E^{g} f ∈ E g be such that e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f . Assume that we have f < 2 g e f <_{2}^{g} e f < 2 g e .
We have e < 1 g f e <_{1}^{g} f e < 1 g f (because e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f ). In other words, there exist a ∈ e a \in e a ∈ e and b ∈ f b \in f b ∈ f satisfying a < 1 b a <_{1} b a < 1 b . Consider these a a a and b b b .
If there was a c ∈ E c \in E c ∈ E satisfying a < 1 c < 1 b a <_{1} c <_{1} b a < 1 c < 1 b , then the g g g -orbit w w w of this c c c would satisfy e < 1 g w < 1 g f e <_{1}^{g} w <_{1}^{g} f e < 1 g w < 1 g f , which would contradict the fact that e e e is < 1 g <_{1}^{g} < 1 g -covered by f f f . Hence, there exists no such c c c . In other words, a a a is < 1 <_{1} < 1 -covered by b b b (since a < 1 b a <_{1} b a < 1 b ). Therefore, a a a and b b b are < 2 <_{2} < 2 -comparable (since E E E is tertispecial). In other words, we have either a < 2 b a <_{2} b a < 2 b or a = b a = b a = b or b < 2 a b <_{2} a b < 2 a . Since a < 2 b a <_{2} b a < 2 b is impossible (because if we had a < 2 b a <_{2} b a < 2 b , then we would have e < 2 g f e <_{2}^{g} f e < 2 g f (since a ∈ e a \in e a ∈ e and b ∈ f b \in f b ∈ f ), which would contradict f < 2 g e f <_{2}^{g} e f < 2 g e (since < 2 g <_{2}^{g} < 2 g is a strict partial order)), and since a = b a = b a = b is impossible (because a < 1 b a <_{1} b a < 1 b ), we therefore must have b < 2 a b <_{2} a b < 2 a . But since π \pi π is an E E E -partition, we have π ( a ) < π ( b ) \pi(a) < \pi(b) π ( a ) < π ( b ) (since a < 1 b a <_{1} b a < 1 b and b < 2 a b <_{2} a b < 2 a ). But the definition of Φ ( π ) \Phi(\pi) Φ ( π ) shows that ( Φ ( π ) ) ( e ) = π ( a ) (\Phi(\pi))(e) = \pi(a) ( Φ ( π )) ( e ) = π ( a ) (since a ∈ e a \in e a ∈ e ) and ( Φ ( π ) ) ( f ) = π ( b ) (\Phi(\pi))(f) = \pi(b) ( Φ ( π )) ( f ) = π ( b ) (since b ∈ f b \in f b ∈ f ). Thus, ( Φ ( π ) ) ( e ) = π ( a ) < π ( b ) = ( Φ ( π ) ) ( f ) (\Phi(\pi))(e) = \pi(a) < \pi(b) = (\Phi(\pi))(f) ( Φ ( π )) ( e ) = π ( a ) < π ( b ) = ( Φ ( π )) ( f ) . Hence, Condition 2 is proven.
Thus, Condition 1 and Condition 2 are proven. Hence, Proposition 7.6 (a) is proven.
(b) Assume that Φ ( π ) \Phi(\pi) Φ ( π ) is an E g E^{g} E g -partition. We want to show that π \pi π is an E E E -partition. In order to do so, we can use Lemma 7.1 (applied to ϕ = π \phi= \pi ϕ = π ); we only need to check the following two conditions:
Condition 1: If e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E are such that e e e is < 1 <_{1} < 1 -covered by f f f , and if we have e < 2 f e <_{2} f e < 2 f , then π ( e ) ≤ π ( f ) \pi(e) \leq\pi(f) π ( e ) ≤ π ( f ) .
Condition 2: If e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E are such that e e e is < 1 <_{1} < 1 -covered by f f f , and if we have f < 2 e f <_{2} e f < 2 e , then π ( e ) < π ( f ) \pi(e) < \pi(f) π ( e ) < π ( f ) .
Proof of Condition 1: Let e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E be such that e e e is < 1 <_{1} < 1 -covered by f f f . Assume that we have e < 2 f e <_{2} f e < 2 f .
We have e < 1 f e <_{1} f e < 1 f (since e e e is < 1 <_{1} < 1 -covered by f f f ). Let u u u and v v v be the g g g -orbits of e e e and f f f , respectively. Thus, u u u and v v v belong to E g E^{g} E g , and satisfy e ∈ u e \in u e ∈ u and f ∈ v f \in v f ∈ v . Hence, u < 1 g v u <_{1}^{g} v u < 1 g v (since e < 1 f e <_{1} f e < 1 f ). Hence, ( Φ ( π ) ) ( u ) ≤ ( Φ ( π ) ) ( v ) (\Phi(\pi))(u) \leq(\Phi(\pi))(v) ( Φ ( π )) ( u ) ≤ ( Φ ( π )) ( v ) (since Φ ( π ) \Phi(\pi) Φ ( π ) is an E g E^{g} E g -partition). But the definition of Φ ( π ) \Phi(\pi) Φ ( π ) shows that ( Φ ( π ) ) ( u ) = π ( e ) (\Phi(\pi))(u) = \pi(e) ( Φ ( π )) ( u ) = π ( e ) (since e ∈ u e \in u e ∈ u ) and ( Φ ( π ) ) ( v ) = π ( f ) (\Phi(\pi))(v) = \pi(f) ( Φ ( π )) ( v ) = π ( f ) (since f ∈ v f \in v f ∈ v ). Thus, π ( e ) = ( Φ ( π ) ) ( u ) ≤ ( Φ ( π ) ) ( v ) = π ( f ) \pi(e) = (\Phi(\pi))(u) \leq(\Phi(\pi))(v) = \pi(f) π ( e ) = ( Φ ( π )) ( u ) ≤ ( Φ ( π )) ( v ) = π ( f ) . Hence, Condition 1 is proven.
Proof of Condition 2: Let e ∈ E e \in E e ∈ E and f ∈ E f \in E f ∈ E be such that e e e is < 1 <_{1} < 1 -covered by f f f . Assume that we have f < 2 e f <_{2} e f < 2 e .
We have e < 1 f e <_{1} f e < 1 f (since e e e is < 1 <_{1} < 1 -covered by f f f ). Let u u u and v v v be the g g g -orbits of e e e and f f f , respectively. Thus, u u u and v v v belong to E g E^{g} E g , and satisfy e ∈ u e \in u e ∈ u and f ∈ v f \in v f ∈ v . Hence, u < 1 g v u <_{1}^{g} v u < 1 g v (since e < 1 f e <_{1} f e < 1 f ) and v < 2 u v <_{2} u v < 2 u (since f < 2 e f <_{2} e f < 2 e ). Hence, ( Φ ( π ) ) ( u ) < ( Φ ( π ) ) ( v ) (\Phi(\pi))(u) < (\Phi(\pi))(v) ( Φ ( π )) ( u ) < ( Φ ( π )) ( v ) (since Φ ( π ) \Phi(\pi) Φ ( π ) is an E g E^{g} E g -partition). But the definition of Φ ( π ) \Phi(\pi) Φ ( π ) shows that ( Φ ( π ) ) ( u ) = π ( e ) (\Phi(\pi))(u) = \pi(e) ( Φ ( π )) ( u ) = π ( e ) (since e ∈ u e \in u e ∈ u ) and ( Φ ( π ) ) ( v ) = π ( f ) (\Phi(\pi))(v) = \pi(f) ( Φ ( π )) ( v ) = π ( f ) (since f ∈ v f \in v f ∈ v ). Thus, π ( e ) = ( Φ ( π ) ) ( u ) < ( Φ ( π ) ) ( v ) = π ( f ) \pi(e) = (\Phi(\pi))(u) < (\Phi(\pi))(v) = \pi(f) π ( e ) = ( Φ ( π )) ( u ) < ( Φ ( π )) ( v ) = π ( f ) . Hence, Condition 2 is proven.
Thus, Condition 1 and Condition 2 are proven. Hence, Proposition 7.6 (b) is proven.
(c) The definition of x Φ ( π ) , w g x_{\Phi(\pi),w^{g}} x Φ ( π ) , w g shows that
x Φ ( π ) , w g = ∏ e ∈ E g x ( Φ ( π ) ) ( e ) w g ( e ) = ∏ u ∈ E g x ( Φ ( π ) ) ( u ) w g ( u ) = ∏ u ∈ E g ∏ a ∈ u x ( Φ ( π ) ) ( u ) w ( a ) = ∏ u ∈ E g ∏ a ∈ u x π ( a ) w ( a ) = ∏ a ∈ E x π ( a ) w ( a ) = ∏ e ∈ E x π ( e ) w ( e ) = x π , w . \begin{aligned}
x_{\Phi(\pi),w^{g}} &= \prod_{e\in E^{g}} x_{(\Phi(\pi))(e)}^{w^{g}(e)}
= \prod_{u\in E^{g}} x_{(\Phi(\pi))(u)}^{w^{g}(u)}
= \prod_{u\in E^{g}}\prod_{a\in u} x_{(\Phi(\pi))(u)}^{w(a)} \\
&= \prod_{u\in E^{g}}\prod_{a\in u} x_{\pi(a)}^{w(a)}
= \prod_{a\in E}x_{\pi(a)}^{w(a)}
= \prod_{e\in E}x_{\pi(e)}^{w(e)}
= x_{\pi,w}.
\end{aligned} x Φ ( π ) , w g = e ∈ E g ∏ x ( Φ ( π )) ( e ) w g ( e ) = u ∈ E g ∏ x ( Φ ( π )) ( u ) w g ( u ) = u ∈ E g ∏ a ∈ u ∏ x ( Φ ( π )) ( u ) w ( a ) = u ∈ E g ∏ a ∈ u ∏ x π ( a ) w ( a ) = a ∈ E ∏ x π ( a ) w ( a ) = e ∈ E ∏ x π ( e ) w ( e ) = x π , w .
(by the definition of x π , w x_{\pi,w} x π , w ). This proves Proposition 7.6 (c).
Our next lemma is a standard argument in Pólya enumeration theory (compare it with the proof of Burnside’s lemma):
Lemma 7.7. Let G G G be a finite group. Let F F F be a G G G -set. Let O O O be a G G G -orbit on F F F , and let π ∈ O \pi\in O π ∈ O .
(a) We have
1 ∣ O ∣ = 1 ∣ G ∣ ∑ g ∈ G ; g π = π 1. (32) \frac{1}{|O|}=\frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}1. \tag*{(32)} ∣ O ∣ 1 = ∣ G ∣ 1 g ∈ G ; g π = π ∑ 1. (32) (b) Let E E E be a finite G G G -set. For every g ∈ G g \in G g ∈ G , let sign E g \operatorname{sign}_{E}g sign E g denote the sign of the permutation of E E E that sends every e ∈ E e \in E e ∈ E to g e ge g e . (Thus, g ∈ G g \in G g ∈ G is E E E -even if and only if sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 .) Then,
\begin{cases}
\frac{1}{|O|}, & \text{if } O \text{ is } E\text{-coeven};\\
0, & \text{if } O \text{ is not } E\text{-coeven}
\end{cases}
=
\frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}\operatorname{sign}_{E}g. \tag*{(33)}\end{cases}
Proof of Lemma 7.7. Let Stab G π \operatorname{Stab}_{G}\pi Stab G π denote the stabilizer of π \pi π ; this is the subgroup { g ∈ G ∣ g π = π } \{g \in G \mid g\pi= \pi\} { g ∈ G ∣ g π = π } of G G G . (This subgroup is also known as the stabilizer subgroup or the isotropy group of π \pi π .) The G G G -orbit of π \pi π is O O O (since O O O is a G G G -orbit on F F F , and since π ∈ O \pi\in O π ∈ O ). In other words, O = G π O=G\pi O = G π . Therefore, ∣ O ∣ = ∣ G π ∣ = ∣ G ∣ / ∣ Stab G π ∣ |O|=|G\pi|=|G|/|\operatorname{Stab}_{G}\pi| ∣ O ∣ = ∣ G π ∣ = ∣ G ∣/∣ Stab G π ∣ (by the orbit-stabilizer theorem). Hence,
1 ∣ O ∣ = 1 ∣ G ∣ / ∣ Stab G π ∣ = ∣ Stab G π ∣ ∣ G ∣ . (34) \frac{1}{|O|}
=
\frac{1}{|G|/|\operatorname{Stab}_{G}\pi|}
=
\frac{|\operatorname{Stab}_{G}\pi|}{|G|}. \tag*{(34)} ∣ O ∣ 1 = ∣ G ∣/∣ Stab G π ∣ 1 = ∣ G ∣ ∣ Stab G π ∣ . (34)
(a) We have
∑ g ∈ G ; g π = π 1 = ∣ { g ∈ G ∣ g π = π } ∣ = ∣ Stab G π ∣ . \sum_{\substack{g\in G;\\g\pi=\pi}} 1 = \left|\{g\in G\mid g\pi=\pi\}\right| = |\operatorname{Stab}_{G}\pi|. g ∈ G ; g π = π ∑ 1 = ∣ { g ∈ G ∣ g π = π } ∣ = ∣ Stab G π ∣.
Hence,
1 ∣ G ∣ ∑ g ∈ G ; g π = π 1 = 1 ∣ G ∣ ∣ Stab G π ∣ = ∣ Stab G π ∣ ∣ G ∣ = 1 ∣ O ∣ . \frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}1
=\frac{1}{|G|}|\operatorname{Stab}_{G}\pi|
=\frac{|\operatorname{Stab}_{G}\pi|}{|G|}
=\frac{1}{|O|}. ∣ G ∣ 1 g ∈ G ; g π = π ∑ 1 = ∣ G ∣ 1 ∣ Stab G π ∣ = ∣ G ∣ ∣ Stab G π ∣ = ∣ O ∣ 1 .
(by (34) ). This proves Lemma 7.7 (a).
(b) We need to prove (33) . Assume first that O O O is E E E -coeven. Thus, all elements of O O O are E E E -coeven (by the definition of what it means for O O O to be E E E -coeven). Hence, π \pi π is E E E -coeven (since π ∈ O \pi\in O π ∈ O ). This means that every g ∈ G g\in G g ∈ G satisfying g π = π g\pi=\pi g π = π is E E E -even. Hence, every g ∈ G g\in G g ∈ G satisfying g π = π g\pi=\pi g π = π satisfies sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 (since g g g is E E E -even if and only if sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 ). Thus,
1 ∣ G ∣ ∑ g ∈ G ; g π = π sign E g = 1 ∣ G ∣ ∑ g ∈ G ; g π = π 1 = 1 ∣ O ∣ \frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}\operatorname{sign}_{E}g
=\frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}1
=\frac{1}{|O|} ∣ G ∣ 1 g ∈ G ; g π = π ∑ sign E g = ∣ G ∣ 1 g ∈ G ; g π = π ∑ 1 = ∣ O ∣ 1
(by (32) )
= { 1 ∣ O ∣ , if O is E -coeven ; 0 , if O is not E -coeven =\begin{cases}
\frac{1}{|O|}, & \text{if $O$ is $E$-coeven};\\
0, & \text{if $O$ is not $E$-coeven}
\end{cases} = { ∣ O ∣ 1 , 0 , if O is E -coeven ; if O is not E -coeven
(since O O O is E E E -coeven).
Thus, we have proven (33) under the assumption that O O O is E E E -coeven. We can therefore WLOG assume the opposite now. Thus, assume WLOG that O O O is not E E E -coeven. Hence, no element of O O O is E E E -coeven (due to the contrapositive of Lemma 4.5). In particular, π \pi π is not E E E -coeven (since π ∈ O \pi\in O π ∈ O ). In other words, not every g ∈ G g\in G g ∈ G satisfying g π = π g\pi=\pi g π = π is E E E -even. In other words, not every g ∈ Stab G π g\in\operatorname{Stab}_{G}\pi g ∈ Stab G π is E E E -even (since the elements g ∈ G g\in G g ∈ G satisfying g π = π g\pi=\pi g π = π are exactly the elements g ∈ Stab G π g\in\operatorname{Stab}_{G}\pi g ∈ Stab G π ). In other words, not every g ∈ Stab G π g\in\operatorname{Stab}_{G}\pi g ∈ Stab G π satisfies sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 (since g g g is E E E -even if and only if sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 ).
Now, the map
Stab G π ⟶ { 1 , − 1 } , g ⟼ sign E g \operatorname{Stab}_{G}\pi\longrightarrow\{1,-1\},\qquad g\longmapsto\operatorname{sign}_{E}g Stab G π ⟶ { 1 , − 1 } , g ⟼ sign E g
is a group homomorphism (since the action of G G G on E E E is a group homomorphism G → Aut E G\to\operatorname{Aut}E G → Aut E , and since the sign of a permutation is multiplicative) and is not the trivial homomorphism (since not every g ∈ Stab G π g\in\operatorname{Stab}_{G}\pi g ∈ Stab G π satisfies sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 ). Hence, it must send exactly half the elements of Stab G π \operatorname{Stab}_{G}\pi Stab G π to 1 1 1 and the other half to − 1 -1 − 1 . Therefore, the addends in the sum
∑ g ∈ Stab G π sign E g \sum_{g\in\operatorname{Stab}_{G}\pi}\operatorname{sign}_{E}g g ∈ Stab G π ∑ sign E g
cancel each other out (one half of them are 1, and the others are − 1 -1 − 1 . Therefore, ∑ g ∈ Stab G π sign E g = 0 \sum_{g\in\operatorname{Stab}_{G}\pi}\operatorname{sign}_{E}g=0 ∑ g ∈ Stab G π sign E g = 0 . Now,
1 ∣ G ∣ ∑ g ∈ G ; g π = π sign E g ⏟ = ∑ g ∈ Stab G π = 1 ∣ G ∣ ∑ g ∈ Stab G π sign E g ⏟ = 0 = 0 = { 1 ∣ O ∣ , if O is E -coeven ; 0 , if O is not E -coeven \frac{1}{|G|}\underbrace{\sum_{\substack{g\in G;\\g\pi=\pi}}\operatorname{sign}_{E}g}_{=\sum_{g\in\operatorname{Stab}_{G}\pi}}=\frac{1}{|G|}\underbrace{\sum_{g\in\operatorname{Stab}_{G}\pi}\operatorname{sign}_{E}g}_{=0}=0=\begin{cases}\frac{1}{|O|},&\text{if $O$ is $E$-coeven};\\0,&\text{if $O$ is not $E$-coeven}\end{cases} ∣ G ∣ 1 = ∑ g ∈ Stab G π g ∈ G ; g π = π ∑ sign E g = ∣ G ∣ 1 = 0 g ∈ Stab G π ∑ sign E g = 0 = { ∣ O ∣ 1 , 0 , if O is E -coeven ; if O is not E -coeven
(since O O O is not E E E -coeven). This proves (33) . Lemma 7.7 (b) is thus proven. □
Proof of Theorem 4.7 (sketched). Let g ∈ G g\in G g ∈ G . Define the set E g E^{g} E g , the relations < 1 g <_{1}^{g} < 1 g and < 2 g <_{2}^{g} < 2 g and the triple E g E^{g} E g as in Proposition 7.5. Thus, E g E^{g} E g is a tertispecial double poset (by Proposition 7.5). In other words, ( E g , < 1 g , < 2 g ) (E^{g},<_{1}^{g},<_{2}^{g}) ( E g , < 1 g , < 2 g ) is a tertispecial double poset (since E g = ( E g , < 1 g , < 2 g ) E^{g}=(E^{g},<_{1}^{g},<_{2}^{g}) E g = ( E g , < 1 g , < 2 g ) ).
Now, forget that we fixed g g g . We thus have constructed a tertispecial double poset E g = ( E g , < 1 g , < 2 g ) E^{g}=(E^{g},<_{1}^{g},<_{2}^{g}) E g = ( E g , < 1 g , < 2 g ) for every g ∈ G g\in G g ∈ G .
Moreover, for every g ∈ G g\in G g ∈ G , let us define > 1 g >_{1}^{g} > 1 g to be the opposite relation of < 1 g <_{1}^{g} < 1 g . Furthermore, for every g ∈ G g\in G g ∈ G , define a map w g : E g → { 1 , 2 , 3 , … } w^{g}:E^{g}\to\{1,2,3,\ldots\} w g : E g → { 1 , 2 , 3 , … } by w g ( u ) = ∑ a ∈ u w ( a ) w^{g}(u)=\sum_{a\in u}w(a) w g ( u ) = ∑ a ∈ u w ( a ) . (Since G G G preserves w w w , the numbers w ( a ) w(a) w ( a ) for all a ∈ u a\in u a ∈ u are equal (for given u u u ), and thus ∑ a ∈ u w ( a ) \sum_{a\in u}w(a) ∑ a ∈ u w ( a ) can be rewritten as ∣ u ∣ ⋅ w ( b ) |u|\cdot w(b) ∣ u ∣ ⋅ w ( b ) for any particular b ∈ u b\in u b ∈ u . But we shall not use this observation.) Now, every g ∈ G g\in G g ∈ G satisfies
S ( Γ ( ( E g , < 1 g , < 2 g ) , w g ) ) = ( − 1 ) ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) . (35) S\left(\Gamma\left((E^{g},<_{1}^{g},<_{2}^{g}),w^{g}\right)\right)=(-1)^{|E^{g}|}\Gamma\left((E^{g},>_{1}^{g},<_{2}^{g}),w^{g}\right). \tag*{(35)} S ( Γ ( ( E g , < 1 g , < 2 g ) , w g ) ) = ( − 1 ) ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) . (35)
(Indeed, this follows from Theorem 4.2 (applied to ( E g , < 1 g , < 2 g ) (E^{g},<_{1}^{g},<_{2}^{g}) ( E g , < 1 g , < 2 g ) and w g w^{g} w g instead of ( E , < 1 , < 2 ) (E,<_{1},<_{2}) ( E , < 1 , < 2 ) and w w w ) since the double poset ( E g , < 1 g , < 2 g ) (E^{g},<_{1}^{g},<_{2}^{g}) ( E g , < 1 g , < 2 g ) is tertispecial.)
For every g ∈ G g\in G g ∈ G , we have
∑ π is an E -partition ; g π = π x π , w = Γ ( E g , w g ) (36) \sum_{\substack{\pi\text{ is an }E\text{-partition};\\g\pi=\pi}}x_{\pi,w}=\Gamma(E^{g},w^{g}) \tag*{(36)} π is an E -partition ; g π = π ∑ x π , w = Γ ( E g , w g ) (36)
Γ ( E g , w g ) = ∑ π is an E g -partition x π , w g = ∑ π is an E ‾ g -partition x π ‾ , w g (37) \Gamma(E^{g},w^{g})=\sum_{\pi\text{ is an }E^{g}\text{-partition}}x_{\pi,w^{g}}=\sum_{\pi\text{ is an }\overline{E}^{g}\text{-partition}}x_{\overline{\pi},w^{g}} \tag*{(37)} Γ ( E g , w g ) = π is an E g -partition ∑ x π , w g = π is an E g -partition ∑ x π , w g (37)
(here, we have renamed the summation index π \pi π as π ‾ \overline{\pi} π ).
In Proposition 7.6, we have introduced a bijection Φ \Phi Φ between
the maps π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying g π = π g\pi=\pi g π = π
and
the maps π ‾ : E g → { 1 , 2 , 3 , … } \overline{\pi}:E^{g}\to\{1,2,3,\ldots\} π : E g → { 1 , 2 , 3 , … } .
It is clearly sufficient to prove Theorem 4.7 for k = Z k = \mathbb{Z} k = Z (since all the power series that we are discussing are defined functorially in k k k (and so are the Hopf algebra QSym and its antipode S S S ), and thus any identity between these series that holds over Z \mathbb{Z} Z must hold over any k k k ). Therefore, it is sufficient to prove Theorem 4.7 for k = Q k = \mathbb{Q} k = Q (since Z [ [ x 1 , x 2 , x 3 , … ] ] \mathbb{Z}[[x_1,x_2,x_3,\ldots]] Z [[ x 1 , x 2 , x 3 , … ]] embeds into Q [ [ x 1 , x 2 , x 3 , … ] ] \mathbb{Q}[[x_1,x_2,x_3,\ldots]] Q [[ x 1 , x 2 , x 3 , … ]] , and using this embedding we have QSym Z = QSym Q ∩ Z [ [ x 1 , x 2 , x 3 , … ] ] \operatorname{QSym}_{\mathbb{Z}}=\operatorname{QSym}_{\mathbb{Q}}\cap\mathbb{Z}[[x_1,x_2,x_3,\ldots]] QSym Z = QSym Q ∩ Z [[ x 1 , x 2 , x 3 , … ]] )40 . Thus, we WLOG assume that k = Q k = \mathbb{Q} k = Q . This will allow us to divide by positive integers.
Every G G G -orbit O O O on Par E \operatorname{Par} E Par E satisfies
1 ∣ O ∣ ∑ π ∈ O x π , w = 1 ∣ O ∣ ∑ π ∈ O x O , w = 1 ∣ O ∣ ∣ O ∣ x O , w = x O , w . (38) \frac{1}{|O|}\sum_{\pi\in O}x_{\pi,w}
=\frac{1}{|O|}\sum_{\pi\in O}x_{O,w}
=\frac{1}{|O|}|O|x_{O,w}=x_{O,w}. \tag*{(38)} ∣ O ∣ 1 π ∈ O ∑ x π , w = ∣ O ∣ 1 π ∈ O ∑ x O , w = ∣ O ∣ 1 ∣ O ∣ x O , w = x O , w . (38)
Parts (a) and (b) of Proposition 7.6 show that this bijection Φ \Phi Φ restricts to a bijection between
the E E E -partitions π : E → { 1 , 2 , 3 , … } \pi:E\to\{1,2,3,\ldots\} π : E → { 1 , 2 , 3 , … } satisfying g π = π g\pi=\pi g π = π
and
the E g E^g E g -partitions π ‾ : E g → { 1 , 2 , 3 , … } \overline{\pi}:E^g\to\{1,2,3,\ldots\} π : E g → { 1 , 2 , 3 , … } .
Hence, we can substitute Φ ( π ) \Phi(\pi) Φ ( π ) for π ‾ \overline{\pi} π in the sum ∑ π ‾ is an E g -partition x π ‾ , w g \sum_{\overline{\pi}\text{ is an }E^g\text{-partition}}x_{\overline{\pi},w^g} ∑ π is an E g -partition x π , w g . We thus obtain
∑ π ‾ is an E g -partition x π ‾ , w g = ∑ π is an E -partition; g π = π x Φ ( π ) , w g = ∑ π is an E -partition; g π = π x π , w , \sum_{\overline{\pi}\text{ is an }E^g\text{-partition}}x_{\overline{\pi},w^g}
=
\sum_{\substack{\pi\text{ is an }E\text{-partition;}\\g\pi=\pi}}x_{\Phi(\pi),w^g}
=
\sum_{\substack{\pi\text{ is an }E\text{-partition;}\\g\pi=\pi}}x_{\pi,w}, π is an E g -partition ∑ x π , w g = π is an E -partition; g π = π ∑ x Φ ( π ) , w g = π is an E -partition; g π = π ∑ x π , w ,
(by Proposition 7.6 (c)) whence
∑ π is an E -partition; g π = π x π , w = ∑ π ‾ is an E g -partition x π ‾ , w g = Γ ( E g , w g ) (39) \sum_{\substack{\pi\text{ is an }E\text{-partition;}\\g\pi=\pi}}x_{\pi,w}
=
\sum_{\overline{\pi}\text{ is an }E^g\text{-partition}}x_{\overline{\pi},w^g}
=
\Gamma(E^g,w^g) \tag*{(39)} π is an E -partition; g π = π ∑ x π , w = π is an E g -partition ∑ x π , w g = Γ ( E g , w g ) (39)
(by (37)). This proves (36).
Now,
Γ ( E , w , G ) = ∑ O is a G -orbit on Par E x O , w = ∑ O is a G -orbit on Par E 1 ∣ O ∣ ∑ π ∈ O x π , w = ∑ O is a G -orbit on Par E ∑ π ∈ O 1 ∣ O ∣ x π , w 1 ∣ O ∣ = 1 ∣ G ∣ ∑ g ∈ G ; g π = π 1 (by (32), applied to F = Par E ) = ∑ O is a G -orbit on Par E ∑ π ∈ O ( 1 ∣ G ∣ ∑ g ∈ G ; g π = π 1 ) x π , w = ∑ π is an E -partition ( 1 ∣ G ∣ ∑ g ∈ G ; g π = π 1 ) x π , w = 1 ∣ G ∣ ∑ π is an E -partition ∑ g ∈ G ; g π = π x π , w = 1 ∣ G ∣ ∑ g ∈ G ∑ π is an E -partition ; g π = π x π , w = 1 ∣ G ∣ ∑ g ∈ G Γ ( E g , w g ) (by (36)) = 1 ∣ G ∣ ∑ g ∈ G Γ ( ( E g , ⟨ 1 g , ⟨ 2 g ) , w g ) . (40) \begin{aligned}
\Gamma(E,w,G)
&= \sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par} E}} x_{O,w}
= \sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par} E}} \frac{1}{\lvert O\rvert}\sum_{\pi\in O}x_{\pi,w}\\
&= \sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par} E}}\sum_{\pi\in O}\frac{1}{\lvert O\rvert}x_{\pi,w}
\qquad\frac{1}{\lvert O\rvert}=\frac{1}{\lvert G\rvert}\sum_{\substack{g\in G;\\g\pi=\pi}}1
\quad\text{(by (32), applied to }F=\operatorname{Par} E\text{)}\\
&= \sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par} E}}\sum_{\pi\in O}
\left(\frac{1}{\lvert G\rvert}\sum_{\substack{g\in G;\\g\pi=\pi}}1\right)x_{\pi,w}\\
&= \sum_{\pi\text{ is an }E\text{-partition}}
\left(\frac{1}{\lvert G\rvert}\sum_{\substack{g\in G;\\g\pi=\pi}}1\right)x_{\pi,w}
= \frac{1}{\lvert G\rvert}\sum_{\pi\text{ is an }E\text{-partition}}\sum_{\substack{g\in G;\\g\pi=\pi}}x_{\pi,w}\\
&= \frac{1}{\lvert G\rvert}\sum_{g\in G}\sum_{\substack{\pi\text{ is an }E\text{-partition};\\g\pi=\pi}}x_{\pi,w}
= \frac{1}{\lvert G\rvert}\sum_{g\in G}\Gamma(E^{g},w^{g})
\qquad\text{(by (36))}\\
&= \frac{1}{\lvert G\rvert}\sum_{g\in G}\Gamma\left(\left(E^{g},\langle{}^{g}_{1},\langle{}^{g}_{2}\right),w^{g}\right). \tag*{(40)}
\end{aligned} Γ ( E , w , G ) = O is a G -orbit on Par E ∑ x O , w = O is a G -orbit on Par E ∑ ∣ O ∣ 1 π ∈ O ∑ x π , w = O is a G -orbit on Par E ∑ π ∈ O ∑ ∣ O ∣ 1 x π , w ∣ O ∣ 1 = ∣ G ∣ 1 g ∈ G ; g π = π ∑ 1 (by (32), applied to F = Par E ) = O is a G -orbit on Par E ∑ π ∈ O ∑ ∣ G ∣ 1 g ∈ G ; g π = π ∑ 1 x π , w = π is an E -partition ∑ ∣ G ∣ 1 g ∈ G ; g π = π ∑ 1 x π , w = ∣ G ∣ 1 π is an E -partition ∑ g ∈ G ; g π = π ∑ x π , w = ∣ G ∣ 1 g ∈ G ∑ π is an E -partition ; g π = π ∑ x π , w = ∣ G ∣ 1 g ∈ G ∑ Γ ( E g , w g ) (by (36)) = ∣ G ∣ 1 g ∈ G ∑ Γ ( ( E g , ⟨ 1 g , ⟨ 2 g ) , w g ) . (40)
Hence, Γ ( E , w , G ) ∈ QSym \Gamma(E,w,G)\in\operatorname{QSym} Γ ( E , w , G ) ∈ QSym (by Proposition 3.5).
Applying the map S S S to both sides of the equality (40) , we obtain
S ( Γ ( E , w , G ) ) = 1 ∣ G ∣ ∑ g ∈ G S ( Γ ( ( E g , ⟨ 1 g , ⟨ 2 g ⟩ ) , w g ) ) = 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E g ∣ Γ ( ( E g , ⟨ 1 g , ⟨ 2 g ⟩ ) , w g ) . (41) \begin{aligned}
S\bigl(\Gamma(E,w,G)\bigr)
&=\frac{1}{\lvert G\rvert}\sum_{g\in G}S\bigl(\Gamma((E^{g},\langle{}_{1}^{g},\langle{}_{2}^{g}\rangle),w^{g})\bigr)\\
&=\frac{1}{\lvert G\rvert}\sum_{g\in G}(-1)^{\lvert E^{g}\rvert}\Gamma\bigl((E^{g},\langle{}_{1}^{g},\langle{}_{2}^{g}\rangle),w^{g}\bigr). \tag*{(41)}
\end{aligned} S ( Γ ( E , w , G ) ) = ∣ G ∣ 1 g ∈ G ∑ S ( Γ (( E g , ⟨ 1 g , ⟨ 2 g ⟩) , w g ) ) = ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E g ∣ Γ ( ( E g , ⟨ 1 g , ⟨ 2 g ⟩) , w g ) . (41)
On the other hand, for every g ∈ G g\in G g ∈ G , let sign E g \operatorname{sign}_{E}g sign E g denote the sign of the permutation of E E E that sends every e ∈ E e\in E e ∈ E to g e ge g e . Thus, g ∈ G g\in G g ∈ G is E E E -even if and only if sign E g = 1 \operatorname{sign}_{E}g=1 sign E g = 1 . Now, every G G G -orbit O O O on Par E \operatorname{Par} E Par E and every π ∈ O \pi\in O π ∈ O satisfy
\begin{cases}
\dfrac{1}{\lvert O\rvert}, & \text{if }O\text{ is }E\text{-coeven};\\
0, & \text{if }O\text{ is not }E\text{-coeven}
\end{cases}
=
\frac{1}{\lvert G\rvert}\sum_{\substack{g\in G;\\g\pi=\pi}}\operatorname{sign}_{E}g \tag*{(42)}\end{cases}
((33) , applied to $F=\operatorname{Par} E). Furthermore,
sign E g = ( − 1 ) ∣ E ∣ − ∣ E g ∣ (43) \operatorname{sign}_{E}g=(-1)^{\lvert E\rvert-\lvert E^{g}\rvert} \tag*{(43)} sign E g = ( − 1 ) ∣ E ∣ − ∣ E g ∣ (43)
for every g ∈ G g\in G g ∈ G .41
The permutation ζ \zeta ζ is the permutation of E E E that sends every e ∈ E e\in E e ∈ E to g e ge g e . In other words, ζ \zeta ζ is the action of g g g on E E E . Hence, the cycles of ζ \zeta ζ are the g g g -orbits on E E E . Thus, the set of all cycles of ζ \zeta ζ is the set of all g g g -orbits on E E E ; this latter set is E g E^{g} E g . Hence, E g E^{g} E g is the set of all cycles of ζ \zeta ζ .
But if σ \sigma σ is a permutation of a finite set X X X , then the sign of σ \sigma σ is ( − 1 ) ∣ X ∣ − ∣ X σ ∣ (-1)^{\lvert X\rvert-\lvert X^{\sigma}\rvert} ( − 1 ) ∣ X ∣ − ∣ X σ ∣ , where X σ X^{\sigma} X σ is the set of all cycles of σ \sigma σ . Applying this to X = E X=E X = E , σ = ζ \sigma=\zeta σ = ζ and X σ = E g X^{\sigma}=E^{g} X σ = E g , we see that the sign of ζ \zeta ζ is ( − 1 ) ∣ E ∣ − ∣ E g ∣ (-1)^{\lvert E\rvert-\lvert E^{g}\rvert} ( − 1 ) ∣ E ∣ − ∣ E g ∣ (because E g E^{g} E g is the set of all cycles of ζ \zeta ζ ). In other words, sign E g = ( − 1 ) ∣ E ∣ − ∣ E g ∣ \operatorname{sign}_{E}g=(-1)^{\lvert E\rvert-\lvert E^{g}\rvert} sign E g = ( − 1 ) ∣ E ∣ − ∣ E g ∣ (since sign E g \operatorname{sign}_{E}g sign E g is the sign of ζ \zeta ζ ), qed.
Now,
Γ + ( E , w , G ) = ∑ O is an E -coeven G -orbit on Par E x O , w = 1 ∣ O ∣ ∑ π ∈ O x π , w = 1 ∣ O ∣ ∑ π ∈ O x π , w (by (38)) = ∑ O is a G -orbit on Par E { 1 ∣ O ∣ , if O is E -coeven ; 0 , if O is not E -coeven ∑ π ∈ O x π , w ( here, we have extended the sum to all G -orbits on Par E (not just the E -coeven ones); but all new addends are 0 and therefore do not influence the value of the sum ) = ∑ O is a G -orbit on Par E ∑ π ∈ O { 1 ∣ O ∣ , if O is E -coeven ; 0 , if O is not E -coeven x π , w = 1 ∣ G ∣ ∑ g ∈ G ; g π = π sign E g (by (41)) = ∑ O is a G -orbit on Par E ∑ π ∈ O ( 1 ∣ G ∣ ∑ g ∈ G ; g π = π sign E g ) x π , w = ∑ π is an E -partition ( 1 ∣ G ∣ ∑ g ∈ G ; g π = π sign E g ) x π , w = 1 ∣ G ∣ ∑ g ∈ G ∑ π is an E -partition ; g π = π ( sign E g ) x π , w = 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , ⟨ g 1 g , g 2 g ⟩ ) , w g ) = 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , ⟨ g 1 g , g 2 g ⟩ ) , w g ) . (44) \begin{aligned}
\Gamma^+(\mathrm{E},w,G)
&=\sum_{\substack{O\text{ is an }E\text{-coeven }G\text{-orbit on }\operatorname{Par}\mathrm{E}}} x_{O,w}
=\frac{1}{|O|}\sum_{\pi\in O}x_{\pi,w}\\
&=\frac{1}{|O|}\sum_{\pi\in O}x_{\pi,w}\qquad\text{(by (38))}\\
&=\sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par}\mathrm{E}}}
\begin{cases}
\frac{1}{|O|},&\text{if }O\text{ is }E\text{-coeven};\\
0,&\text{if }O\text{ is not }E\text{-coeven}
\end{cases}
\sum_{\pi\in O}x_{\pi,w}\\
&\qquad\left(\text{here, we have extended the sum to all }G\text{-orbits on }\operatorname{Par}\mathrm{E}\right.\\
&\qquad\left.\text{(not just the }E\text{-coeven ones); but all new addends are }0\right.\\
&\qquad\left.\text{and therefore do not influence the value of the sum}\right)\\
&=\sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par}\mathrm{E}}}
\sum_{\pi\in O}
\begin{cases}
\frac{1}{|O|},&\text{if }O\text{ is }E\text{-coeven};\\
0,&\text{if }O\text{ is not }E\text{-coeven}
\end{cases}
x_{\pi,w}\\
&=\frac{1}{|G|}\sum_{g\in G;\,g\pi=\pi}\operatorname{sign}_{E}g
\qquad\text{(by (41))}\\
&=\sum_{\substack{O\text{ is a }G\text{-orbit on }\operatorname{Par}\mathrm{E}}}
\sum_{\pi\in O}
\left(\frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}\operatorname{sign}_{E}g\right)x_{\pi,w}\\
&=\sum_{\substack{\pi\text{ is an }E\text{-partition}}}
\left(\frac{1}{|G|}\sum_{\substack{g\in G;\\g\pi=\pi}}\operatorname{sign}_{E}g\right)x_{\pi,w}\\
&=\frac{1}{|G|}\sum_{g\in G}\sum_{\substack{\pi\text{ is an }E\text{-partition};\\g\pi=\pi}}
(\operatorname{sign}_{E}g)x_{\pi,w}\\
&=\frac{1}{|G|}\sum_{g\in G}(-1)^{|E|-|E^{g}|}
\Gamma\left(\left(E^{g},\langle g^{g}_{1},g^{g}_{2}\rangle\right),w^{g}\right)\\
&=\frac{1}{|G|}\sum_{g\in G}(-1)^{|E|-|E^{g}|}
\Gamma\left(\left(E^{g},\langle g^{g}_{1},g^{g}_{2}\rangle\right),w^{g}\right). \tag*{(44)}
\end{aligned} Γ + ( E , w , G ) = O is an E -coeven G -orbit on Par E ∑ x O , w = ∣ O ∣ 1 π ∈ O ∑ x π , w = ∣ O ∣ 1 π ∈ O ∑ x π , w (by (38)) = O is a G -orbit on Par E ∑ { ∣ O ∣ 1 , 0 , if O is E -coeven ; if O is not E -coeven π ∈ O ∑ x π , w ( here, we have extended the sum to all G -orbits on Par E (not just the E -coeven ones); but all new addends are 0 and therefore do not influence the value of the sum ) = O is a G -orbit on Par E ∑ π ∈ O ∑ { ∣ O ∣ 1 , 0 , if O is E -coeven ; if O is not E -coeven x π , w = ∣ G ∣ 1 g ∈ G ; g π = π ∑ sign E g (by (41)) = O is a G -orbit on Par E ∑ π ∈ O ∑ ∣ G ∣ 1 g ∈ G ; g π = π ∑ sign E g x π , w = π is an E -partition ∑ ∣ G ∣ 1 g ∈ G ; g π = π ∑ sign E g x π , w = ∣ G ∣ 1 g ∈ G ∑ π is an E -partition ; g π = π ∑ ( sign E g ) x π , w = ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , ⟨ g 1 g , g 2 g ⟩ ) , w g ) = ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , ⟨ g 1 g , g 2 g ⟩ ) , w g ) . (44)
Hence, Γ + ( E , w , G ) ∈ Q S y m \Gamma^+(\mathrm{E},w,G)\in\mathrm{QSym} Γ + ( E , w , G ) ∈ QSym (by Proposition 3.5).
The group G G G preserves the relation > 1 >_{1} > 1 (since it preserves the relation < 1 <_{1} < 1 ). Furthermore, the double poset ( E , > 1 , < 2 ) (E, >_{1}, <_{2}) ( E , > 1 , < 2 ) is tertispecial42 . Hence, we can apply (44) to ( E , > 1 , < 2 ) (E, >_{1}, <_{2}) ( E , > 1 , < 2 ) , > 1 >_{1} > 1 and > 1 g >_{1}^{g} > 1 g instead of E E E , < 1 <_{1} < 1 and < 1 g <_{1}^{g} < 1 g . As a result, we obtain
Γ + ( ( E , > 1 , < 2 ) , w , G ) = 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) . \Gamma^{+}\left((E, >_{1}, <_{2}), w, G\right)=\frac{1}{|G|}\sum_{g\in G}(-1)^{|E|-|E^{g}|}\Gamma\left((E^{g}, >_{1}^{g}, <_{2}^{g}), w^{g}\right). Γ + ( ( E , > 1 , < 2 ) , w , G ) = ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) .
Multiplying both sides of this equality by ( − 1 ) ∣ E ∣ (-1)^{|E|} ( − 1 ) ∣ E ∣ , we transform it into
( − 1 ) ∣ E ∣ Γ + ( ( E , > 1 , < 2 ) , w , G ) = ( − 1 ) ∣ E ∣ 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) = 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E ∣ ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) = 1 ∣ G ∣ ∑ g ∈ G ( − 1 ) ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) = S ( Γ ( E , w , G ) ) (by xref‘(40)‘). \begin{aligned}
(-1)^{|E|}\Gamma^{+}\left((E, >_{1}, <_{2}), w, G\right)
&=(-1)^{|E|}\frac{1}{|G|}\sum_{g\in G}(-1)^{|E|-|E^{g}|}\Gamma\left((E^{g}, >_{1}^{g}, <_{2}^{g}), w^{g}\right)\\
&=\frac{1}{|G|}\sum_{g\in G}(-1)^{|E|}(-1)^{|E|-|E^{g}|}\Gamma\left((E^{g}, >_{1}^{g}, <_{2}^{g}), w^{g}\right)\\
&=\frac{1}{|G|}\sum_{g\in G}(-1)^{|E^{g}|}\Gamma\left((E^{g}, >_{1}^{g}, <_{2}^{g}), w^{g}\right)\\
&=S\left(\Gamma(E,w,G)\right)\qquad\text{(by {xref}`(40)`).}
\end{aligned} ( − 1 ) ∣ E ∣ Γ + ( ( E , > 1 , < 2 ) , w , G ) = ( − 1 ) ∣ E ∣ ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) = ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E ∣ ( − 1 ) ∣ E ∣ − ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) = ∣ G ∣ 1 g ∈ G ∑ ( − 1 ) ∣ E g ∣ Γ ( ( E g , > 1 g , < 2 g ) , w g ) = S ( Γ ( E , w , G ) ) (by xref ‘(40)‘).
This completes the proof of Theorem 4.7. □
Application: Jochemko's theorem
We shall now demonstrate an application of Theorem 4.7: namely, we will use it to provide an alternative proof of [15 Theorem 2.13] . The way we derive [15 Theorem 2.13] from Theorem 4.7 is classical, and in fact was what originally motivated the discovery of Theorem 4.7 (although, of course, it cannot be conversely derived from [15 Theorem 2.13] , so it is an actual generalization).
An intermediate step between [15 Theorem 2.13] and Theorem 4.7 will be the following fact:
Corollary 8.1. Let E = ( E , < 1 , < 2 ) E=(E,<_{1},<_{2}) E = ( E , < 1 , < 2 ) be a tertispecial double poset. Let w : E → { 1 , 2 , 3 , … } w:E\to\{1,2,3,\ldots\} w : E → { 1 , 2 , 3 , … } . Let G G G be a finite group which acts on E E E . Assume that G G G preserves both relations < 1 <_{1} < 1 and < 2 <_{2} < 2 , and also preserves w w w . For every q ∈ N q\in\mathbb{N} q ∈ N , let Par q E \operatorname{Par}_{q}E Par q E denote the set of all E E E -partitions whose image is contained in { 1 , 2 , … , q } \{1,2,\ldots,q\} { 1 , 2 , … , q } . Then, the group G G G also acts on Par q E \operatorname{Par}_{q}E Par q E ; namely, Par q E \operatorname{Par}_{q}E Par q E is a G G G -subset of the G G G -set { 1 , 2 , … , q } E \{1,2,\ldots,q\}^{E} { 1 , 2 , … , q } E (see Definition 4.4 (d) for the definition of the latter).
(a) There exists a unique polynomial Ω E , G ∈ Q [ X ] \Omega_{E,G}\in\mathbb{Q}[X] Ω E , G ∈ Q [ X ] such that every q ∈ N q\in\mathbb{N} q ∈ N satisfies
Ω E , G ( q ) = (the number of all G -orbits on Par q E ) . (45) \Omega_{E,G}(q)=\text{(the number of all $G$-orbits on $\operatorname{Par}_{q}E$)}. \tag*{(45)} Ω E , G ( q ) = (the number of all G -orbits on Par q E ) . (45)
(b) This polynomial satisfies
Ω E , G ( − q ) = ( − 1 ) ∣ E ∣ ( the number of all E -coeven G -orbits on Par q ( E , > 1 , < 2 ) ) = ( − 1 ) ∣ E ∣ ( the number of all E -coeven G -orbits on Par q ( E , < 1 , > 2 ) ) (46) \begin{aligned}
\Omega_{E,G}(-q) = (-1)^{|E|}\left(\text{the number of all }E\text{-coeven }G\text{-orbits on }\operatorname{Par}_{q}(E,>_{1},<_{2})\right) \\
&= (-1)^{|E|}\left(\text{the number of all }E\text{-coeven }G\text{-orbits on }\operatorname{Par}_{q}(E,<_{1},>_{2})\right) \tag*{(46)}
\end{aligned} Ω E , G ( − q ) = ( − 1 ) ∣ E ∣ ( the number of all E -coeven G -orbits on Par q ( E , > 1 , < 2 ) ) = ( − 1 ) ∣ E ∣ ( the number of all E -coeven G -orbits on Par q ( E , < 1 , > 2 ) ) (46)
for all q ∈ N q \in\mathbb{N} q ∈ N .
Proof of Corollary 8.1 (sketched). Set k = Q \mathbf{k} = \mathbb{Q} k = Q . For any f ∈ QSym f \in\operatorname{QSym} f ∈ QSym and any q ∈ N q \in\mathbb{N} q ∈ N , we define an element ps 1 ( f ) ( q ) ∈ Q \operatorname{ps}^{1}(f)(q) \in\mathbb{Q} ps 1 ( f ) ( q ) ∈ Q by
ps 1 ( f ) ( q ) = f ( 1 , 1 , … , 1 ⏟ q times , 0 , 0 , 0 , … ) . \operatorname{ps}^{1}(f)(q)=f\left(\underbrace{1,1,\ldots,1}_{q\ \text{times}},0,0,0,\ldots\right). ps 1 ( f ) ( q ) = f q times 1 , 1 , … , 1 , 0 , 0 , 0 , … .
(that is, ps 1 ( f ) ( q ) \operatorname{ps}^{1}(f)(q) ps 1 ( f ) ( q ) is the result of substituting 1 for each of the variables x 1 , x 2 , … , x q x_{1},x_{2},\ldots,x_{q} x 1 , x 2 , … , x q and 0 for each of the variables x q + 1 , x q + 2 , x q + 3 , … x_{q+1},x_{q+2},x_{q+3},\ldots x q + 1 , x q + 2 , x q + 3 , … in the power series f f f ).
(a) Consider the elements Γ ( E , w , G ) \Gamma(E,w,G) Γ ( E , w , G ) and Γ + ( E , w , G ) \Gamma^{+}(E,w,G) Γ + ( E , w , G ) of QSym \operatorname{QSym} QSym defined in Theorem 4.7. Observe that Par q E \operatorname{Par}_{q}E Par q E is a G G G -subset of Par E \operatorname{Par}E Par E .
Now, [13 Proposition 7.1.7 (i)] shows that, for any given f ∈ QSym f \in\operatorname{QSym} f ∈ QSym , there exists a unique polynomial in Q [ X ] \mathbb{Q}[X] Q [ X ] whose value on each q ∈ N q \in\mathbb{N} q ∈ N equals ps 1 ( f ) ( q ) \operatorname{ps}^{1}(f)(q) ps 1 ( f ) ( q ) . Applying this to f = Γ ( E , w , G ) f=\Gamma(E,w,G) f = Γ ( E , w , G ) , we conclude that there exists a unique polynomial in Q [ X ] \mathbb{Q}[X] Q [ X ] whose value on each q ∈ N q \in\mathbb{N} q ∈ N equals ps 1 ( Γ ( E , w , G ) ) ( q ) \operatorname{ps}^{1}(\Gamma(E,w,G))(q) ps 1 ( Γ ( E , w , G )) ( q ) . But since every q ∈ N q \in\mathbb{N} q ∈ N satisfies
ps 1 ( Γ ( E , w , G ) ) ( q ) = Γ ( E , w , G ) ⏟ O is a G -orbit on Par E ( 1 , 1 , … , 1 ⏟ q times , 0 , 0 , 0 , … ) = ∑ O is a G -orbit on Par E x O , w ( 1 , 1 , … , 1 ⏟ q times , 0 , 0 , 0 , … ) = ∑ O is a G -orbit on Par E { 1 , if O ⊆ Par q E ; 0 , if O ⊈ Par q E = ∑ O is a G -orbit on Par q E { 1 , if O ⊆ Par q E ; 0 , if O ⊈ Par q E = ∑ O is a G -orbit on Par q E 1 = ( the number of all G -orbits on Par q E ) , (47) \begin{aligned}
\operatorname{ps}^{1}(\Gamma(E,w,G))(q)
&=\underbrace{\Gamma(E,w,G)}_{ O\text{ is a }G\text{-orbit on }\operatorname{Par}E}
\left(\underbrace{1,1,\ldots,1}_{q\ \text{times}},0,0,0,\ldots\right)\\
&=\sum_{O\text{ is a }G\text{-orbit on }\operatorname{Par}E}x_{O,w}
\left(\underbrace{1,1,\ldots,1}_{q\ \text{times}},0,0,0,\ldots\right)\\
&=\sum_{O\text{ is a }G\text{-orbit on }\operatorname{Par}E}
\begin{cases}
1, & \text{if }O\subseteq\operatorname{Par}_{q}E;\\
0, & \text{if }O\not\subseteq\operatorname{Par}_{q}E
\end{cases}\\
&=\sum_{O\text{ is a }G\text{-orbit on }\operatorname{Par}_{q}E}
\begin{cases}
1, & \text{if }O\subseteq\operatorname{Par}_{q}E;\\
0, & \text{if }O\not\subseteq\operatorname{Par}_{q}E
\end{cases}\\
&=\sum_{O\text{ is a }G\text{-orbit on }\operatorname{Par}_{q}E}1
=\left(\text{the number of all }G\text{-orbits on }\operatorname{Par}_{q}E\right), \tag*{(47)}
\end{aligned} ps 1 ( Γ ( E , w , G )) ( q ) = O is a G -orbit on Par E Γ ( E , w , G ) q times 1 , 1 , … , 1 , 0 , 0 , 0 , … = O is a G -orbit on Par E ∑ x O , w q times 1 , 1 , … , 1 , 0 , 0 , 0 , … = O is a G -orbit on Par E ∑ { 1 , 0 , if O ⊆ Par q E ; if O ⊆ Par q E = O is a G -orbit on Par q E ∑ { 1 , 0 , if O ⊆ Par q E ; if O ⊆ Par q E = O is a G -orbit on Par q E ∑ 1 = ( the number of all G -orbits on Par q E ) , (47)
this rewrites as follows: There exists a unique polynomial in Q [ X ] \mathbb{Q}[X] Q [ X ] whose value on each q ∈ N q \in\mathbb{N} q ∈ N equals (the number of all G G G -orbits on Par q E \operatorname{Par}_q E Par q E ). This proves Corollary 8.1 (a).
(b) [13 Proposition 7.1.7 (i)] shows that, for any given f ∈ QSym f \in\operatorname{QSym} f ∈ QSym , there exists a unique polynomial in Q [ X ] \mathbb{Q}[X] Q [ X ] whose value on each q ∈ N q \in\mathbb{N} q ∈ N equals ps 1 ( f ) ( q ) \operatorname{ps}^{1}(f)(q) ps 1 ( f ) ( q ) . This polynomial is denoted by ps 1 ( f ) \operatorname{ps}^{1}(f) ps 1 ( f ) in [13 Proposition 7.1.7] . From our above proof of Corollary 8.1 (a), we see that
Ω E , G = ps 1 ( Γ ( E , w , G ) ) . \Omega_{E,G}=\operatorname{ps}^{1}\left(\Gamma(E,w,G)\right). Ω E , G = ps 1 ( Γ ( E , w , G ) ) .
But [13 Proposition 7.1.7 (iii)] shows that, for any f ∈ QSym f \in\operatorname{QSym} f ∈ QSym and m ∈ N m \in\mathbb{N} m ∈ N , we have ps 1 ( S ( f ) ) ( m ) = ps 1 ( f ) ( − m ) \operatorname{ps}^{1}(S(f))(m)=\operatorname{ps}^{1}(f)(-m) ps 1 ( S ( f )) ( m ) = ps 1 ( f ) ( − m ) . Applying this to f = Γ ( E , w , G ) f=\Gamma(E,w,G) f = Γ ( E , w , G ) , we obtain
ps 1 ( S ( Γ ( E , w , G ) ) ) ( m ) = ps 1 ( Γ ( E , w , G ) ) ( − m ) = Ω E , G ( − m ) . \operatorname{ps}^{1}\left(S\left(\Gamma(E,w,G)\right)\right)(m)=\operatorname{ps}^{1}\left(\Gamma(E,w,G)\right)(-m)=\Omega_{E,G}(-m). ps 1 ( S ( Γ ( E , w , G ) ) ) ( m ) = ps 1 ( Γ ( E , w , G ) ) ( − m ) = Ω E , G ( − m ) .
for any m ∈ N m \in\mathbb{N} m ∈ N . Thus, any m ∈ N m \in\mathbb{N} m ∈ N satisfies
Ω E , G ( − m ) = ps 1 ( S ( Γ ( E , w , G ) ) = ( − 1 ) ∣ E ∣ Γ + ( ( E , ≻ 1 , ≺ 2 ) , w , G ) (by Theorem 4.7) ) ( m ) = ps 1 ( ( − 1 ) ∣ E ∣ Γ + ( ( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( m ) = ( − 1 ) ∣ E ∣ ps 1 ( Γ + ( ( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( m ) . \begin{aligned}
\Omega_{E,G}(-m)=\operatorname{ps}^{1}\left(\underset{=(-1)^{|E|}\Gamma^{+}((E,\succ_{1},\prec_{2}),w,G)\text{ (by Theorem 4.7)}}{S\left(\Gamma(E,w,G)\right)}\right)(m) \\
&=\operatorname{ps}^{1}\left((-1)^{|E|}\Gamma^{+}((E,\succ_{1},\prec_{2}),w,G)\right)(m) \\
&=(-1)^{|E|}\operatorname{ps}^{1}\left(\Gamma^{+}((E,\succ_{1},\prec_{2}),w,G)\right)(m).
\end{aligned} Ω E , G ( − m ) = ps 1 ( = ( − 1 ) ∣ E ∣ Γ + (( E , ≻ 1 , ≺ 2 ) , w , G ) (by Theorem 4.7) S ( Γ ( E , w , G ) ) ) ( m ) = ps 1 ( ( − 1 ) ∣ E ∣ Γ + (( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( m ) = ( − 1 ) ∣ E ∣ ps 1 ( Γ + (( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( m ) .
Renaming m m m as q q q in this equality, we see that every q ∈ N q \in\mathbb{N} q ∈ N satisfies
Ω E , G ( − q ) = ( − 1 ) ∣ E ∣ ps 1 ( Γ + ( ( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( q ) . (48) \Omega_{E,G}(-q)=(-1)^{|E|}\operatorname{ps}^{1}\left(\Gamma^{+}((E,\succ_{1},\prec_{2}),w,G)\right)(q). \tag*{(48)} Ω E , G ( − q ) = ( − 1 ) ∣ E ∣ ps 1 ( Γ + (( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( q ) . (48)
But just as we proved (47) , we can show that every q ∈ N q \in\mathbb{N} q ∈ N satisfies
ps 1 ( Γ + ( E , w , G ) ) ( q ) = ( the number of all E -coeven G -orbits on Par q E ) . \operatorname{ps}^{1}\left(\Gamma^{+}(E,w,G)\right)(q)=(\text{the number of all }E\text{-coeven }G\text{-orbits on }\operatorname{Par}_{q}E). ps 1 ( Γ + ( E , w , G ) ) ( q ) = ( the number of all E -coeven G -orbits on Par q E ) .
Applying this to ( E , ≻ 1 , ≺ 2 ) (E,\succ_{1},\prec_{2}) ( E , ≻ 1 , ≺ 2 ) instead of E E E , we obtain
ps 1 ( Γ + ( ( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( q ) = ( the number of all E -coeven G -orbits on Par q ( E , ≻ 1 , ≺ 2 ) ) . \operatorname{ps}^{1}\left(\Gamma^{+}((E,\succ_{1},\prec_{2}),w,G)\right)(q)
=(\text{the number of all }E\text{-coeven }G\text{-orbits on }\operatorname{Par}_{q}(E,\succ_{1},\prec_{2})). ps 1 ( Γ + (( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( q ) = ( the number of all E -coeven G -orbits on Par q ( E , ≻ 1 , ≺ 2 )) .
Now, (47) becomes
Ω E , G ( − q ) = ( − 1 ) ∣ E ∣ ps 1 ( Γ + ( ( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( q ) = ( the number of all E -coeven G -orbits on Par q ( E , ≻ 1 , ≺ 2 ) ) = ( − 1 ) ∣ E ∣ ( the number of all E -coeven G -orbits on Par q ( E , ≻ 1 , ≺ 2 ) ) . \begin{aligned}
\Omega_{E,G}(-q)=(-1)^{|E|}\underset{=(\text{the number of all }E\text{-coeven }G\text{-orbits on }\operatorname{Par}_{q}(E,\succ_{1},\prec_{2}))}{\operatorname{ps}^{1}\left(\Gamma^{+}((E,\succ_{1},\prec_{2}),w,G)\right)(q)} \\
&=(-1)^{|E|}(\text{the number of all }E\text{-coeven }G\text{-orbits on }\operatorname{Par}_{q}(E,\succ_{1},\prec_{2})).
\end{aligned} Ω E , G ( − q ) = ( − 1 ) ∣ E ∣ = ( the number of all E -coeven G -orbits on Par q ( E , ≻ 1 , ≺ 2 )) ps 1 ( Γ + (( E , ≻ 1 , ≺ 2 ) , w , G ) ) ( q ) = ( − 1 ) ∣ E ∣ ( the number of all E -coeven G -orbits on Par q ( E , ≻ 1 , ≺ 2 )) .
In order to prove Corollary 8.1 (b), it thus remains to show that
(the number of all E -coeven G -orbits on Par q ( E , > 1 , < 2 ) ) = (the number of all E -coeven G -orbits on Par q ( E , < 1 , > 2 ) ) (49) \begin{aligned}
&\text{(the number of all $E$-coeven $G$-orbits on $\operatorname{Par}_q(E, >_1, <_2)$)}\\
&=\text{(the number of all $E$-coeven $G$-orbits on $\operatorname{Par}_q(E, <_1, >_2)$)} \tag*{(49)}
\end{aligned} (the number of all E -coeven G -orbits on Par q ( E , > 1 , < 2 ) ) = (the number of all E -coeven G -orbits on Par q ( E , < 1 , > 2 ) ) (49)
for every q ∈ N q \in\mathbb{N} q ∈ N .
Proof of (49) : Let q ∈ N q \in\mathbb{N} q ∈ N . Let w 0 : { 1 , 2 , … , q } → { 1 , 2 , … , q } w_0:\{1,2,\ldots,q\}\to\{1,2,\ldots,q\} w 0 : { 1 , 2 , … , q } → { 1 , 2 , … , q } be the map sending each i ∈ { 1 , 2 , … , q } i \in\{1,2,\ldots,q\} i ∈ { 1 , 2 , … , q } to q + 1 − i q+1-i q + 1 − i . Then, the map
Par q ( E , > 1 , < 2 ) ⟶ Par q ( E , < 1 , > 2 ) , π ↦ w 0 ∘ π \operatorname{Par}_q(E, >_1, <_2) \longrightarrow\operatorname{Par}_q(E, <_1, >_2), \qquad\pi\mapsto w_0 \circ\pi Par q ( E , > 1 , < 2 ) ⟶ Par q ( E , < 1 , > 2 ) , π ↦ w 0 ∘ π
is an isomorphism of G G G -sets (this is easy to check). Thus, Par q ( E , > 1 , < 2 ) ≅ Par q ( E , < 1 , > 2 ) \operatorname{Par}_q(E, >_1, <_2) \cong\operatorname{Par}_q(E, <_1, >_2) Par q ( E , > 1 , < 2 ) ≅ Par q ( E , < 1 , > 2 ) as G G G -sets. From this, (48) follows (by functoriality, if one wishes). The proof of Corollary 8.1 (b) is now complete.
Now, the second formula of [15 Theorem 2.13] follows from our (45), applied to E = ( P , ≺ , < ω ) E=(P,\prec,<_{\omega}) E = ( P , ≺ , < ω ) (where < ω <_{\omega} < ω is the partial order on P P P given by ( p < ω q ) ⟺ ( ω ( p ) < ω ( q ) ) (p<_{\omega}q)\Longleftrightarrow(\omega(p)<\omega(q)) ( p < ω q ) ⟺ ( ω ( p ) < ω ( q )) ). The first formula of [15 Theorem 2.13] can also be derived from our above arguments. We leave the details to the reader.
A final question
With the results proven above (specifically, Theorems 4.2 and 4.7 ), we have obtained formulas for a large class of quasisymmetric generating functions for maps from a double poset to { 1 , 2 , 3 , … } \{1,2,3,\ldots\} { 1 , 2 , 3 , … } . At least one question arises:
Question 9.1. In [11 ] , I have studied generalizations of Whitney’s famous non-broken-circuit theorem for graphs and matroids. One of the cornerstones of that study is the bijection Φ \Phi Φ in [11 proofs of Lemma 2.8, Lemma 5.29 and Lemma 8.25] , which is uncannily reminiscent of the involution T T T in the proof of Theorem 4.2 . (Actually, this bijection Φ \Phi Φ can be extended to an involution, thus making the analogy even more palpable.) Both Φ \Phi Φ and T T T are defined by toggling a certain element in or out of a subset; and this element is chosen as the argmin or argmax of a function defined on the ground set. Is there a connection between the two results, or even a common generalization?