Exponentials

Arun Ram
Department of Mathematics and Statistics
University of Melbourne
Parkville, VIC 3010 Australia
aram@unimelb.edu.au

Last update: 04 August 2012

Abstract.
This is a typed version of I.G. Macdonald's lecture notes from lectures at the University of California San Diego from January to March of 1991.

Lattices

Let V be a real vector space of dimension r>0. A lattice in V is a subgroup L of V (hence closed under addition and subtraction) that spans V and is generated by r elements x1,...,xr (which are therefore a basis of V). So the elements of L are all linear combinations ∑i=1rnixi, ni∈ℤ (1≤i≤r). Let M be another lattice in V, with basis y1,...,yr, and suppose that M⊆L. Then each yi∈L, hence we have equations yi = ∑j=1raijxj (1≤i≤r) (aij∈ℤ). (Exp 1) The matrix A=(aij) is a nonsingular matrix of integers, because it transforms one basis of V into another.

L/M is a finite abelian group of order d = |detA|.

Proof.
By elementary transformations on rows and columns we can find r×r matrices U,V of integers with determinant ±1, such that UAV is a diagonal matrix, say UAV = d1 ⋱ dr where the di are positive integers. (We can even arrange that d1|d2|⋯|dr, though we shan't need that fact here.)

Let y′i = ∑j uijyj and xk = ∑l vkl x′l, so that the x′k (resp. the y′i) are a basis of L (resp. M). From (Exp 1) we have y′i = ∑j uijyj = ∑j,k uij ajk xk = ∑j,k,l uij ajk vkl x′l = ∑l (UAV)il x′l and therefore y′i = dix′i (1≤i≤l). So L, M have bases x′1,...,x′r, and d1x′1,...,drx′r, and therefore L/M ≅ ⨁i=1r ℤ/diℤ is a direct sum of cyclic groups of orders d1,...,dr, hence |L/M| = d1,...,dr = det(UAV) = ±detA, since U,V have determinant ±1.

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Now suppose V carries a positive definite scalar product ⟨x,y⟩, and let L be a lattice in V, as before. Let L* = {y∈V | ⟨x,y⟩∈ℤ for all x∈L}. Let x1,...,xr be a basis of L and let x1*,...,xr* be the dual basis of V: ⟨xi,xj*⟩ = δij. Then y∈L* ⇔ ⟨xi,y⟩∈ℤ for 1≤i≤r ⇔ y = ∑1r nixi*, ni∈ℤ, so that L* is a lattice in V with basis x1*,...,xr*. L* is called the dual of L. We have L**=L (because L** has basis x1,...,xr).

If M⊆L we have L*⊆M*, because if y∈L* we have ⟨x,y⟩∈ℤ for all x∈L and a fortiori for all x∈M.

M*/L* is the dual (or character group) of L/M.

(In particular L/M ≅ M*/L* — but not canonically.)

Proof.
Let η∈M*, x∈L and define χη(x+y) = e2πi⟨x,η⟩ . If y∈M we have χη(x+y) = e2πi⟨x+y,η⟩ = e2πi⟨x,η⟩ e2πi⟨y,η⟩ = χη(x) because   ⟨y,η⟩ ∈ ℤ, i.e. χη is constant on the cosets of M in L and therefore defines a character of the finite abelian group L/M. Moreover if ξ∈L* then χη+ξ = χη (because ⟨ξ,x⟩ ∈ℤ for x∈L). Hence η↦χη defines a mapping of M*/L* into the character group of L/M. Check that it is an isomorphism.

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If y1,...,yr is a basis of M, y1*,...,yr* the dual basis we have yi = ∑y=1r aijxj (aij∈ℤ) and aij = ⟨yi,xj*⟩ , so that also xj* = ∑i=1raijyi* or, interchanging i and j, xi* = ∑j=1rajiyj*.

The root lattice and the weight lattice

Let R be a reduced root system, spanning V, and let Q=Q(R) be the subgroup of V generated by the roots: so the elements of Q are all linear combinations λ = ∑α∈R ηαα,   ηα∈ℤ. If B={α1,...,αr} is a basis of R, every α∈R, and hence every λ∈Q, is uniquely of the form ∑1rηiαi with integer coefficients ηi: Q(R) = ⨁i=1rℤαi so that Q is a lattice in V, called the root lattice. Likewise Q(R∨). From above, P(R) is the dual of Q(R∨): P(R) = Q(R∨)* hence is also a lattice, called the weight lattice of R. Since ⟨β,α∨⟩∈ℤ for all α,β∈R (integrality axiom (R1)) it follows that Q(R) ⊆ P(R) (and likewise Q(R∨) ⊆ P(R∨) ).

Let ( π1,...,πr ) be the basis of V dual to ( α1∨,...,αr∨ ): ⟨πi,αj∨⟩ = δij. The πi are a basis of the weight lattice P(R): they are called the fundamental weights. They span the Weyl chamber C—.

Recall that A=(aij) is the Cartan matrix, where aij = ⟨αi∨,αj⟩ .

Example. R = {ei-ej | 1≤i,j≤r,i≠j} type   An-1. What are the fundamental weights? αi = αi∨ = ei-ei+1 (1≤i≤n-1). So ⟨πi,αj⟩ = δij say πi = ∑uiei,   ∑ui=0 ⟨πi,αj⟩ = ⟨∑uiei,ej-ej+1⟩ = uj-uj+1. So uj = uj+1 if j≠i ui-ui+1 = 1 ui+1 = ⋯=un=u say u1 = ⋯=ui=u+1 0=∑ui = i(u+1) + (n-i)u = nu+i hence u=-in { πi = 1n( (n-i) (e1+⋯+ei) - i(ei+1+⋯+en) ) πi = e1+⋯+ei-ie e = 1n ∑1nei } 1≤i≤n-1; πn=0.

Exercise: Calculate the πi for types B,C,D.

We have αj = ∑i=1r ⟨αi∨,αj⟩πi i.e., αj = ∑i=1r aijπi (1≤j≤r) and hence from Proposition 1.1

|P(R)/Q(R)| = detA.

(We know from before that detA is positive.)

The positive integer detA is traditionally denoted by f and called the index of connection: f = |P(R)/Q(R)| = |P(R∨)/Q(R∨)| by Proposition 1.2, since P(R∨) and Q(R∨) are respectively the duals of Q(R) and P(R).

Finally, W acts on everything: it acts on R, and on R∨, hence on Q(R) and Q(R∨), hence on P(R) and P(R∨). Let Q+ = ∑1rηiαi ηi≥0 and P+ = ∑1rηiπi ηi≥0 . Then P+ = P∩C—, hence (1.21).

Every W-orbit in P meets P+ in exactly one point.

The λ∈P+ are called the dominant weights.

Let λ∈P.

  1. λ-wλ∈Q, for all w∈W.
  2. λ∈P+ ⇔ λ-wλ ∈ Q+ for all w∈W.

Proof.
  1. We have λ-siλ = ⟨λ,αi∨⟩ αi ∈ Q, because ⟨λ,αi∨⟩ ∈ ℤ. Hence λ≡siλ   (modQ). Since W is generated by the si, it follows that λ≡wλ   (modQ) for all w∈W.
  2. Recall (1.24) the partial order x≥y on V:   x≥y iff x-y∈C*—, where C*— is the cone spanned by the simple roots αi. We have Q+ = Q∩C*—. Now if λ∈P we have λ∈P+ ⇔ λ∈C— ⇔ λ≥wλ for all w∈W (1.24) ⇔ λ-wλ ∈ C*—∩Q = Q+, using (i).

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Proposition 2.3 (i) says that the Weyl group W acts trivially on the finite group P/Q.

Recall ρ = 12 ∑α∈R+α is such that ⟨ρ,αi∨⟩ = 1 (1≤i≤r) (1.9). Hence

ρ = π1+⋯+πr ∈ P∩C.

Likewise let σ = 12 ∑α∈R+ α∨ (warning: ρ∨ is not a good notation, because σ ≠ 2ρ |ρ|2 ). By (1.9) applied to R∨ we have ⟨σ,αi⟩ = 1   (1≤i≤r), because (1.23) B∨ = {α1∨,...,αr∨} is a basis of R∨. Hence

For all α∈R, ht(α)=⟨σ,α⟩.

For if α = ∑1r niαi, then ⟨σ,α⟩ = ∑ni⟨σ,αi⟩ = ∑ni = ht(α). σ is the "altimeter".

Exponentials

If G is a group (finite or infinite) and k is a commutative ring, the group algebra kG consists of all formal sums a = ∑g∈G agg with coefficients ag∈k, only finitely many non-zero (i.e. kG is the free k-module with G as basis). So in particular each g∈G is an element of kG. Add and multiply in the obvious way: if b = ∑g∈G bgg is another element of kG, then a+b = ∑g∈G (ag+bg)g and ab = ∑g,h∈G agbh⋅gh i.e. the multiplication in kG is just the multiplication in G, extended by linearity.

If however the group operation in G is addition (g+h rather than gh) we have to change our notation and write e.g. eg for the element of kG corresponding to g: the e's are "formal exponentials" and satisfy eg⋅eh = eg+h, e0=1, (eg)-1 = e-g (g,h∈G). The elements of kG are now written a = ∑ageg and add and multiply as indicated.

This applies in particular to the group P, the weight lattice. Let A=ℝP denote the group algebra of P over k=ℝ. So the elements of A are finite sums f = ∑λ∈P fλeλ (fλ∈ℝ, almost all zero ) where eλ⋅eμ = eλ+μ,   e0=1. The eλ are an ℝ-basis of A.

The ring A is easily described. The fundamental weights πi   (1≤i≤r) form a basis of P, so that each λ∈P is uniquely of the form λ = ∑i=1r niπi (ni∈ℤ). Hence if we put yi=eπi we have eλ = en1π1 ⋯ enrπr = y1η1 ⋯ yrηr and therefore A = ℝ[ y1±1,...,yr±1 ] is the algebra of Laurent polynomials in y1,...,yr (i.e. polynomials in the y's and their inverses). Since ℝ[y1,...,yr] is a unique factorization domain, so is A.

Let λ,μ∈P be linearly independent (i.e. not proportional). Then 1-eλ and 1-eμ are coprime in A.

Proof.
This amounts to showing that if α,β∈ℤr are not proportional, then 1-yα and 1-yβ have no common factor. Left as exercise.

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The Weyl group W acts on P, hence on A: if f = ∑λ∈P fλeλ ∈ A then wf = ∑λ∈P fλewλ. f∈A is

  1. W-invariant (or W-symmetric) if wf=f, all w∈W.
  2. W-skew (or alternating) if wf=ε(w)f, all w∈W. ( ⇔sif = -f (1≤i≤r). )

We shall start by considering the W-skew elements of A. Let θ:A→A be the linear mapping defined by θf = ∑w∈W ε(w)wf (f∈A). We have (v∈W) θv = vθ = ∑ε(w)vw = ε(v)θ.

  1. S=θ(A) is the space of W-skew elements of A.
  2. If f∈A and sαf=f for some α∈R, then θf=0.
  3. The θ(eλ+ρ), λ∈P+, form an ℝ-basis of S.

Proof.
  1. Let f∈A. Then θf is W-skew, because if v∈W we have vθf = ε(v)θf. Conversely if f is W-skew then θf = ∑w∈W ε(w)⋅wf = |W|f so that f = θf |W| ∈ θ(A).
  2. We have θsα = ε(sα)θ = -θ, hence θf = θsαf = -θf and therefore θf=0.
  3. Suppose f = ∑μ fμeμ ∈ S. Then f = ε(w)wf = ∑με(w) fμewμ and therefore fwμ = ε(w)fμ. Since each W-orbit in P meets P+ in just one point (Prop. 2.2) it follows that f = ∑μ∈P+fμ ∑w∈W ε(w) ewμ = ∑μ∈P+ fμθ(eμ). (*) Now μ∈P+ is of the form μ = ∑miπi with mi&he;0. If mi=0 for some i then ⟨μ,αi∨⟩ = 0 and hence siμ=μ, so that θ(eμ) = 0 by (ii). Hence in (*) the sum is restricted to μ = ∑miπi with each mi≥1, hence (Prop. 2.5) μ=λ+ρ with λ∈P+. So f is a linear combination of the θ(eλ+ρ) with λ∈P+, and these are clearly linearly independent (the orbits W(λ+ρ) are disjoint).

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Next let d = eρ ∏α∈R+ (1-e-α) = ∏α∈R+ ( eα2 - e-α2 ) ∈A.

  1. d=θ(eρ) and d is W-skew (H. Weyl).
  2. Each f∈S is divisible in A by d and fd-1 is invariant. Moreover f↦fd-1 is a bijection of S onto the W-invariants.
(So d plays the same role here as p = ∏α∈R+α did for polynomials.)

Proof.
  1. si permutes the positive roots other than αi, and siαi=-αi (1.9). Hence sid = ( e- αi 2 - e αi 2 ) ∏ α∈R+ α≠αi ( eα2 - e-α2 ) = -d (1≤i≤r) from which it follows that d∈S. Hence (Prop. 3.2) d = ∑λ∈P+ dλ θ(eλ+ρ) (dλ∈ℤ) (ExpWeyl 1) where dλ= coefficient of eλ+ρ in d. Now on expansion we have d = eρ + ∑μ<ρ aμeμ (ExpWeyl 2) say; hence d0= coefficient of eρ in d=1, and if λ∈P+, λ≠0 we have λ+ρ>ρ, so that from (ExpWeyl 2) the coefficient of eλ+ρ in d is zero. So dλ=0 if λ∈P+, λ≠0, and hence (ExpWeyl 1) shows that d=θ(eρ).
  2. By Prop. 3.1 and Prop. 3.2 it is enough to show that θ(eλ+ρ) is divisible by 1-e-α for each α∈R+. Let W+ = {w∈W | ε(w)=1}, then W = W+∪sαW+ (disjoint union). Then θ(eλ+ρ) = ∑w∈W+ ε(w) ( ew(λ+ρ) - esαw(λ+ρ) ). It is enough to show that each term in this sum is divisible by 1-e-α; i.e. that eμ-esαμ (μ∈P) is divisible by 1-e-α. Now sαμ = μ-⟨μ,α∨⟩α = μ-mα say, where m∈ℤ, hence eμ-esαμ = eμ (1-e-mα) = eμ (1-e-α)( 1+e-α+⋯+e-(m-1)α ) if   m>0; and if m<0, say m=-n, then (1-e-mα) = (1-enα) = -enα (1-e-nα) and the conclusion is the same as before. (Finally eμ-esαμ=0 if m=0.)

    Finally, if f is skew then fd-1 is W-symmetric. Conversely if g∈AW then gd∈S, which proves the last statement of Proposition 3.3 (ii).

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The formula d = θ(eρ), or explicitly eρ ∏α>0 (1-e-α) = ∑w∈W ε(w) ewρ is Weyl's denominator formula. I will give an alternative, more combinatorial proof.

Example. R of type An-1, roots εi-εj   (1≤i,j≤n, i≠j). We have ρ = 12 ∑i<j (εi-εj) = 12( (n-1)ε1 + (n-3)ε2 + ⋯ + (1-n)εn ) = (n-1)ε1 + (n-2)ε2 + ⋯ + εn-1 - 12 (n-1) (ε1+⋯+εn) = δ-12(n-1)ε. Let xi=eεi, then Weyl's formula is in this case x δ-n-12ε ⋅ ∏i<j ( 1-xi-1xj ) = ∑w∈Sn ε(w) x wδ-n-12ε . Multiply both sides by (x1,...,xn) n-1 2 and we get ∏1≤i<j≤n (xi-xj) = ∑w∈Sn ε(w) xwδ (Vandermonde identity).

Exercise: Write it down explicitly for the other R of classical type (Bn,Cn,Dn).

For the second proof of Proposition 3.3 (i) we need a lemma, which will come in useful later:

For each subset E⊆R+ let σE = ∑α∈Eα. Suppose that ρ-σE is a regular element of V (i.e. does not lie in any hyperplane Hα). Then E = R(w)   ( =R+∩wR- ) for some w∈W and σE=ρ-wρ.

Proof.
We have ρ-σE ∈ wC for some w∈W (C the Weyl chamber), hence w-1 (ρ-σE) ∈ C. Now ρ-σE = 12 ∑α∈R+ uαα (ExpLem 1) where uα = { +1, if α∉E, -1, if α∈E. } (ExpLem 2) i.e. ρ-σE is of the form 12 ∑α∈R+ ±α. Hence so is w-1 (ρ-σE), hence w-1 (ρ-σE) = ρ-σF (ExpLem 3) for some F⊆R+, depending on E and w, and which we could describe explicitly if we needed. So we have ρ-σF ∈ C, hence ⟨ρ-σF,αi∨⟩ is >0 and hence ≥1 for each i=1,2,...,r. But ⟨ρ,αi∨⟩ = 1, hence ⟨σF,αi∨⟩ ≤ 0 and therefore also ⟨σF,αi⟩ ≤ 0   (1≤i≤r), so that ⟨σF,μ⟩ ≤ 0 for all μ∈Q+. But σF∈Q+, hence ⟨σF,σF⟩ ≤ 0, hence σF=0 (and so F=φ). From (ExpLem 3) it now follows that ρ-σE = wρ, i.e., σE=ρ-wρ.

Moreover, since w-1 (ρ-σE) = ρ it follows from (ExpLem 1) that 12 ∑α∈R+ uαw-1α = 12 ∑β∈R+β. Hence for each α∈R+, uα = { +1, if w-1α∈R+ -1, if w-1α∈R-. } (ExpLem 4) Hence from (ExpLem 2) and (ExpLem 4) α∈E  ⇔  w-1α ∈ R-, i.e. α∈wR-, so E = R+∩wR- = R(w).

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Second proof of Proposition 3.3 (i).
Now consider d = eρ ∏α∈R+ (1-e-α) = ∑E⊆R+ (-1)|E| eρ-σE, on multiplying out. But d is skew, hence |W|⋅d = θd = ∑E⊆R+ (-1)|E| θ(eρ-σE). If ρ-σE is not regular, θ(eρ-σE) = 0 by Proposition 3.2 (ii). If ρ-σE is regular, then E=R(w) and ρ-σE = wρ for some w∈W. So |W|⋅d = ∑w∈W ε(w) θ(ewρ) since (-1)|E| = (-1)l(w) = ε(w); and ε(w) θ(ewρ) = ε(w)θw(eρ) = θ(eρ) so that |W|⋅d = |W|θ(eρ) and hence d=θ(eρ) as required.

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The same technique can be used to prove the following identity. For each α∈R+, let tα be an indeterminate, and for each subset E⊆R+ let tE = ∏α∈Etα. Then we have

∑w∈W w ∏α∈R+ 1-tαe-α 1-e-α = ∑w∈W tR(w).

Proof.
Let L denote the left-hand side of Proposition 3.5, so that L = ∑w∈W w d-1eρ ∏α∈R+ (1-tαe-α) and therefore Ld = ∑w∈W ε(w) ewρ ∏α∈R+ (1-tαe-wα) = ∑w∈W ε(w) ∑E⊆R+ (-1)|E| tE ew(ρ-σE) on multiplying out the product, i.e., Ld = ∑E⊆R+ (-1)|E| tE θ(eρ-σE). Now by Proposition 3.2 we have θ(eρ-σE) = 0 if ρ-σE is not regular, and if ρ-σE is regular then by Proposition 3.4 E=R(w) and ρ-σE = wρ for some w∈W. Hence (since (-1)|R(w)| = (-1)l(w) = ε(w) ) Ld = ∑w∈W ε(w) tR(w) θ(ewρ) (ExpId 1) and θ(ewρ) = θw(eρ) = ε(w) θ(eρ) = ε(w)d. So we can cancel d from either side of (ExpId 1) and obtain L = ∑w∈W tR(w).

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In particular, if tα=t for all α∈R+:

∑w∈W w ∏α∈R+ 1-te-α 1-e-α = ∑w∈W tl(w) = W(t).

Here the right hand side is independent of the e-α, so we may specialize them in any way we please. Define φ:ℝQ→ℝ[t,t-1] by φ(eαi) = t-1 (1≤i≤r) so that φ(e-α) = tht(α) and therefore φ ∏α∈R+ 1-te-α 1-e-α = ∏α∈R+ 1-tht(α)+1 1-tht(α) . (Exp 2) What about φ ∏α∈R+ 1-te-wα 1-e-wα (Exp 3) when w≠1? In that case some w-1αi is a negative root -α say, so that αi=wα, some α∈R+, and then φ( 1-te-wα ) = φ( 1-teαi ) = 1-t⋅t-1 =0 so that (Exp 3) is zero when w≠1. Hence from Proposition 3.6 we obtain

∏α∈R+ 1-t1+ht(α) 1-tht(α) = ∑w∈W tl(w)

another multiplicative formula for the Poincaré polynomial W(t) = P(ℋ;t) of the harmonics. From Proposition 3.7 and (3.31) it follows that ∏i=1r 1-tdi 1-t = ∏α∈R+ 1-t1+ht(α) 1-tht(α) = ∏i≥1 ( 1-ti+1 1-ti ) hi where hi (i≥1) is the number of roots α∈R+ of height i. Since h1=r (the roots of height 1 being the αi) it follows that ∏i=1r (1-tdi) = ∏i≥1 (1-ti+1) hi-hi+1 (Exp 4) so that hi ≥ hi+1 for each i≥1, i.e. η = (h1,h2,...) is a partition of N = Card(R+) ; hi-hi+1 = mi(η′), the multiplicity of i as part of the conjugate partition η′, so that

The partitions (h1,h2,...) and (d1-1, d2-1,..., dr-1) = (e1,...,er) where (d1≥⋯≥dr) are conjugate (Shapiro, Kostant).

So the degrees di (or the exponents ei) can be read off from the root system.

Exercise: Check Proposition 3.8 for the classical root systems (i.e. compute the hi).

Bases of AW

Let AW = {f∈A | wf=f all w∈W} be the subring of W-invariants of A. I will list several ℝ-bases of AW, generalizing familiar objects from the theory of symmetric functions.

Orbit-sums (monomial symmetric functions)

Suppose f = ∑μ∈P fμeμ ∈ AW. Then for all w∈W we have f = wf = ∑μ fμewμ so that fμ = fwμ, i.e. the coefficients fμ are constant on each W-orbit in P. By Proposition 2.2 each such W-orbit is of the form Wλ,   λ∈P+, so that f = ∑λ∈P+ fλ ∑μ∈Wλ eμ from which it follows that

The orbit-sums mλ = ∑μ∈Wλeμ (λ∈P+) are an ℝ-basis of AW (indeed, a ℤ-basis of (ℤP)W ).

Weyl characters

For each λ∈P+ we define χλ = θ(eλ+ρ) d = ∑w∈W ε(w) ew(λ+ρ) ∑w∈W ε(w) ewρ , by Proposition 3.3. By Proposition 3.3 (ii) we have χλ ∈ AW. The χλ are Weyl characters. Since (Prop. 3.2 (iii)) the θ(eλ+ρ),   λ∈P+, form an ℝ-basis of the space S of W-skew elements of A, hence by Proposition 3.3 (ii) the χλ,   λ∈P+ are an ℝ-basis of AW.

We have χλ = ∑w∈W ε(w) ew(λ+ρ)-ρ ∏α∈R+ (1-e-α) = eλ +   lower terms, where by lower terms is meant a linear combination of eμ with μ<λ (because if w≠1 then w(λ+ρ) < χ+ρ, i.e. w(λ+ρ)-ρ<λ). Hence, as χλ is symmetric, we can write

χλ = ∑ μ∈P+ μ≤λ Kλμ mμ with Kλλ = 1.

In fact the coefficients Kλμ are non-negative integers, (because they are the multiplicities of the weights in the simple 𝔤-module indexed by λ).

Problem. Prove directly (i.e. without recourse to representation theory of Lie groups or Lie algebras) that the Kλμ are ≥0).

Example. R = An-1,   λ = (λ1,...,λn) ∈ P (so that ∑λi=0). Since ⟨λ,α∨⟩ is an integer for all α∈R it follows that λi-λj ∈ ℤ for all i,j, but the individual λi need not be integers: in general they will be rational numbers with denominators dividing n, as we say last time from computing the fundamental weights. In particular, λ∈P+  ⇔  λ1≥λ2≥⋯≥λn (and ∑λi=0).

So any partition μ = (μ1,...,μn) of length ≤n determines a dominant weight μ* = ( μ1-1n|μ| ,..., μn-1n|μ| ). So we have a surjective (but not bijective) mapping μ↦μ* of the set 𝒫n of partitions of length ≤n onto the cone P+ of dominant weights for the root system An-1.

As before put xi = eεi   (1≤i≤n). Then the Weyl characters χλ are essentially Schur functions: to be precise, if μ is a partition of length ≤n, then χμ* = sμ(x1,...,xn) (x1⋯xn) |μ|n (because it must have degree 0 as a polynomial in the xi±1). In particular, since πi = (ε1+⋯+εi) - in ∑1n εj, we have χπi = ei(x1,...,xn) (x1⋯xn) in = mπi, (1≤i≤n-1) ( πn = 0, χπn = χ0 = 1 ).

Return to the general case

For each i∈[1,r] let ui be an element of AW of the form ui = eπi + lower terms (Exp 5)

Examples.

  1. ui=mπi,
  2. ui=χπi.
[When R is of type An-1 these are the same, but in general they aren't.]

Then we have

AW = ℝ[u1,...,ur] and the ui are algebraically independent over ℝ.

Proof.
Consider a monomial u1n1 ,..., urnr (n1,...,nr integers ≥0). From (Exp 5) it follows that if λ = ∑niπi ∈ P+ we have uλ = u1n1 ⋯ urnr = e∑niπi + lower terms = eλ + lower terms = mλ + ∑ μMλ μ∈P+ (*)mμ for certain coefficients (*). Hence the transition matrix between the u's and the orbit sums is unitriangular, hence invertible. So by Proposition 4.1 the uλ are a basis of AW (even over ℤ), which proves Proposition 4.3.

□

Note that the χλ are defined for all λ∈P, not just λ∈P+.

Hall-Littlewood analogs

Next, we have analogs of the Hall-Littlewood symmetric functions. Let t be an indeterminate, let λ∈P+ and define P˜λ(t) = P˜λ = ∑w∈W w eλ ∏α∈R+ 1-te-α 1-e-α . Notation W(t) = ∑w∈W tl(w); so in particular P˜0 = W(t) by Proposition 3.6. We have P˜λ = ∑w∈W w eλ+ρ d ∏α∈R+ (1-te-α) = d-1 ∑w∈W ε(w) ⋅ w eλ+ρ ∏α∈R+ (1-te-α) = d-1θ eλ+ρ ∏α∈R+ (1-te-α) which shows that P˜λ ∈ AW[t].

Let Wλ = {w∈W | wλ=λ} be the subgroup of W that fixes λ. Since λ∈P+⊆C—,   Wλ is generated by the si,   i∈I. Let Rλ be the root system with basis αi   (i∈I). Then Rλ+ ⊆ R+. Now si permutes R+-{αi} and also permutes Rλ+-{αi} if i∈I. Hence si permutes R+-Rλ+ if i∈I, and hence Wλ permutes R+-Rλ+.

Now let U be a set of left coset representatives of Wλ in W, so that each w∈W is uniquely w=uv with u∈U and v∈Wλ. Then P˜λ = ∑u∈U u eλ ∏ α∈R+-Rλ+ 1-te-α 1-e-α ⋅ ∑v∈Wλ v ∏α∈Rλ+ 1-te-α 1-e-α from what we have just observed. By Proposition 3.6 it follows that P˜λ = Wλ(t) ∑u∈W/Wλ u eλ ∏α∈R+-Rλ+ 1-te-α 1-e-α and hence all the coefficients of P˜λ (which are polynomials in t) are divisible by Wλ(t), and we can define Pλ(t) = Wλ(t)-1 ∑w∈W w eλ ∏α∈R+ 1-te-α 1-e-α (Exp 6) = ∑u∈W/Wλ u eλ ∏ α∈R+ -Rλ+ 1-te-α 1-e-α (Exp 7) = eλ + lower terms = mλ + lower terms.

Particular case:

  1. t=1, then Pλ = ∑u∈W/Wλ euλ = mλ, from (Exp 7)
  2. t=0, then Pλ = ∑w∈W w eλ ∏α∈R+ 1 1-e-α = d-1 ∑w∈W ε(w) ew(λ+ρ) = χλ.
So the Pλ include the orbit sums mλ and the Weyl characters χλ as particular cases.

Kostka polynomials

These are defined by χλ = ∑ μ≤λ μ∈P+ Kλμ(t)Pμ (λ∈P+) Then Kλμ(0) = δλμ and Kλμ(1) = Kλμ and the Kλμ(t) are q-analogs of weight multiplicities. For ξ∈P let F(ξ;t) = ∑(mα) t∑mα summed over all families (mα)α∈R+ of non-negative integers such that ξ = ∑α∈R+mαα.

(So F(ξ;t)=0 unless ξ∈Q+.)

  1. Kλμ(t) = ∑w∈W ε(w) F( w(λ+ρ) - (μ+ρ) ; t ), (λ,μ∈P+) (Kato)
  2. Let K(t) = (Kλμ(t)) λ,μ∈P+. Then the transpose of K(t) is the matrix of the operator ∏α∈R+ (1-tRα)-1, where the Rα are raising operators: Rαχλ = χλ+α.

Constant term conjectures

(SIAM J. Math. Analysis 13 (1982) 988-1007)

Let R be a reduced root system, k an integer ≥0; d1,...,dr the degrees of the Weyl group W of R. If f = ∑λ∈P fλeλ ∈ A, the constant term of f is f0.

  1. (C1) The constant term in ∏α∈R (1-eα)k is ∏i=1r ( kdi k ).
  2. (C1q) The constant term in ∏α∈R+ ∏i=0k-1 (1-qieα) (1-qi+1e-α) is ∏i=1r [ kdi k ] where [ n r ] = (1-qn) (1-qn-1)⋯(1-qn-r+1) (1-q)(1-q2)⋯(1-qr) is the q-binomial coefficient or Gaussian polynomial.

Clearly (C1q)⇒(C1) by setting q=1. Consider the simplest nontrivial case, i.e. k=1. Then ∏α∈R (1-eα) = eρ ∏α∈R+ (1-e-α) ⋅ e-ρ ∏α∈R+ (1-eα) = ∑w∈W ε(w) ewρ ∑ν∈W ε(ν) e-νρ by Proposition 3.3. Since ρ∈C we have wρ=νρ  ⇔  ν=w, so the constant term is |W| = d1d2⋯dr, which is (C1) for k=1.

Next, when k=1 we have to consider the constant term C(q) in ∏α∈R+ (1-eα) (1-qe-α) = ∏α∈R (1-eα) ⋅ ∏α∈R+ 1-qe-α 1-e-α . Hence C(q) = 1|W| × constant term in ∏α∈R (1-eα) ∑w∈W w ∏α∈R+ 1-qe-α 1-e-α = ∏α∈R (1-eα) ⋅ W(q) by Proposition 3.5. But we have just seen that the constant term in ∏α∈R (1-eα) is |W|, hence C(q) = W(q) = ∏i=1r 1-qdi 1-q = ∏i=1r [di1].

Formal exponentials as functions on V

Let λ∈P. We may regard eλ as a (complex-valued) function on V, as follows eλ(x) = e2πi⟨λ,x⟩ (x∈V) where the e on the right is the usual one: 2.718...

Now let μ∈Q∨ = Q(R∨) . Then eλ(x+μ) = e2πi⟨λ,x+μ⟩ and ⟨λ,x+μ⟩ = ⟨λ,x⟩+⟨λ,μ⟩ ≡ ⟨λ,x⟩ module integers, so that eλ(x+μ) = eλ(x) (x∈V, μ∈Q∨). (Exp 8) Let T=V/Q∨ and let φ:x↦x⋅ = x+Q∨ be the canonical mapping V→T. Then (Exp 8) shows that eλ defines a function on T, eλ(x⋅) = eλ(x). Since V = ⨁ℝαi∨,   Q∨ = ⨁ℤαi∨ it follows that T is a direct sum (or direct product) of r copies of ℝ/ℤ, the circle group: (x↦e2πi) i.e., T is an r-dimensional torus: a compact commutative topological group.

Let Π be the parallelepiped Π = ∑xiαi∨ 0≤xi<1 (1≤i≤r) so that the projection φ:V→T restricted to Π is a bijection Π→˜T.

Now let f be a complex-valued continuous function on T. Lifting it back to V, we get a continuous function f˜ on V: f˜(x) = f(x⋅) = f(φ(x)) i.e. f˜=f∘φ;

f˜ is periodic: f˜(x+μ) = f˜(x) (μ∈Q∨).
Hence f˜ can be expanded as a convergent Fourier series: f˜ = ∑λ∈P fλeλ — now in general an infinite series — where fλ = ∫Π f˜(x) e-λ(x)dx := ∫T f(x⋅) e-λ(x⋅)dx⋅ and dx = dx1⋯dxr — integration from 0 to 1 in each xi.

So in particular the constant term of f˜ is f0 = ∫T f(x⋅)dx⋅. These considerations apply to the conjectures (C1) and (C1q). Consider the latter. Introduce the notation (x;q)∞ = ∏i=1∞ (1-qix) whenever the product makes sense. Then if k is an integer ≥0 (x;q)∞ (xqk;q)∞ = ∏i=0k-1 (1-qix). So in (C1q) we seek the constant term in ∏α∈R+ (eα,q)∞ (qe-α;q)∞ (qkeα;q)∞ (qk+1e-α;q)∞ . (Exp 9) Think of q now as a real number, 0≤q<1. The infinite product (eα;q)∞ = ∏i≥0 (1-qieα) converges uniformly on T to a continuous function (because ∑qieα converges). So does (qkeα;q)∞ for any real or complex k (qk = eklogq); moreover it does not vanish anywhere on T unless one of the factors 1-qk+ieα does, and this can happen only if k is an integer ≤0. So if k is not an integer <0, the expression (Exp 9) is a continuous function on the torus T, and its constant term is therefore well-defined.

To make sense of the other side when k is not an integer ≥0, we introduce the q-gamma function. Suppose first that k is an integer ≠0, then Γ(k+1) = k! is the limit as q→1 of Γq(k+1) = (1-q)(1-q2)⋯(1-qk) (1-q)k = (q;q)∞ (qk+1;q)∞ (1-q)k . This makes sense whenever k∈ℂ is not a negative integer (it has poles at the negative integers). We now interpret the Gaussian polynomial [ kdi k ] as Γq(kdi+1) Γq(k+1) Γq(k(di-1)+1) (The +1s in the notation are a nuisance, but it is 200 years too late to change.)

Kostant's partition function

If μ∈P let p(μ) = no. of sequences   (nα)α∈R+   such that   nα∈ℕ   (all  α) and   ∑α∈R+ nαα = μ. (So p(μ)=0 unless μ∈Q+.) Clearly ∏α∈R+ (1-e-α)-1 = ∑ξ∈Q+ p(ξ) e-ξ. (Exp 10) Define Kλμ by χλ = ∑μ Kλμ mμ and cλμν by χλχμ = ∑ν cλμνχν (λ,μ,ν∈P+).

  1. Kλμ = ∑w∈W ε(w) p( w(λ+ρ)-(μ+ρ) ).
  2. cλμν = ∑v,w∈W ε(vw) p( v(λ+ρ) + w(μ+ρ) - (ν+2ρ) ).

Proof.
  1. Kλμ is the coefficient of eμ in χλ = ∑w∈W ε(w) ew(λ+ρ)-ρ ∏α∈R+ (1-e-α)-1 = ∑ w∈W ξ∈Q+ ε(w) p(ξ) ew(λ+ρ)-ξ-ρ. So we must have w(λ+ρ)-ξ-ρ = μ, i.e. ξ = w(λ+ρ)-(μ+ρ) and hence we get Kλμ = ∑w∈W ε(w) p( w(λ+ρ) - (μ+ρ) ).
  2. We have θ(eλ+ρ) θ(eμ+ρ) d = ∑ν cλμν θ(eν+ρ) (Exp Kos) and therefore cλμν is the coefficient of eν+ρ in the left hand side of (Exp Kos), i.e. in ∑v,w ε(vw) e v(λ+ρ) + w(μ+ρ) - ρ ∏α∈R+ (1-e-α)-1 = ∑ v,w∈W ξ∈Q+ ε(vw) p(ξ) e v(λ+ρ) + w(μ+ρ) - ξ-ρ . So we must have ν(λ+ρ) + w(μ+ρ) - ξ-ρ = ν+ρ i.e. ξ = v(λ+ρ) + w(μ+ρ) - (ν+2ρ) and hence we get the formula (ii).

□

Both Kλμ and cλμν are integers ≥0. This is not apparent from these formulas.

References

I.G. Macdonald
Issac Newton Institute for the Mathematical Sciences
20 Clarkson Road
Cambridge CB3 OEH U.K.

Version: March 12, 2012

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