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Littlewood–Richardson coefficients and birational combinatorics

Darij Grinberg

14 October 2020

Drexel University, Philadelphia, PA

slides: http:

//www.cip.ifi.lmu.de/~grinberg/algebra/drexel2020.pdf paper: arXiv:2008.06128 aka http:

//www.cip.ifi.lmu.de/~grinberg/algebra/lrhspr.pdf

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Manifest

I shall review the Littlewood–Richardson coefficients and some of their classical properties.

I will then state a “hidden symmetry” conjectured by Pelletier and Ressayre (arXiv:2005.09877) and outline how I proved it.

The proof is a nice example of birational combinatorics: the use of birational transformations in elementary combinatorics (specifically, here, in finding and proving a bijection).

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Manifest

I shall review the Littlewood–Richardson coefficients and some of their classical properties.

I will then state a “hidden symmetry” conjectured by Pelletier and Ressayre (arXiv:2005.09877) and outline how I proved it.

The proof is a nice example of birational combinatorics: the use of birational transformations in elementary combinatorics (specifically, here, in finding and proving a bijection).

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Manifest

I shall review the Littlewood–Richardson coefficients and some of their classical properties.

I will then state a “hidden symmetry” conjectured by Pelletier and Ressayre (arXiv:2005.09877) and outline how I proved it.

The proof is a nice example of birational combinatorics: the use of birational transformations in elementary combinatorics (specifically, here, in finding and proving a bijection).

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Chapter 1

Chapter 1

Littlewood–Richardson coefficients

References (among many):

Richard Stanley, Enumerative Combinatorics, vol. 2, Chapter 7.

Darij Grinberg, Victor Reiner,Hopf Algebras in Combinatorics, arXiv:1409.8356.

Emmanuel Briand, Mercedes Rosas, The 144 symmetries of the Littlewood-Richardson coefficients of SL3,

arXiv:2004.04995.

Igor Pak, Ernesto Vallejo,Combinatorics and geometry of Littlewood-Richardson cones, arXiv:math/0407170.

Emmanuel Briand, Rosa Orellana, Mercedes Rosas, Rectangular symmetries for coefficients of symmetric functions, arXiv:1410.8017.

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Reminder on symmetric functions

Fix a commutative ring kwith unity. We shall do everything overk.

Consider the ring k[[x1,x2,x3, . . .]] of formal power series in countably many indeterminates.

A formal power series f is said to be bounded-degreeif the monomials it contains are bounded (from above) in degree.

A formal power series f is said to be symmetricif it is invariant under permutations of the indeterminates. For example:

1 +x1+x23 is bounded-degree but not symmetric. (1 +x1) (1 +x2) (1 +x3)· · · is symmetric but not bounded-degree.

Let Λbe the set of all symmetric bounded-degree power series in k[[x1,x2,x3, . . .]]. This is ak-subalgebra, called thering of symmetric functions overk.

It is also known as Sym.

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Reminder on symmetric functions

Fix a commutative ring kwith unity. We shall do everything overk.

Consider the ring k[[x1,x2,x3, . . .]] of formal power series in countably many indeterminates.

A formal power series f is said to be bounded-degreeif the monomials it contains are bounded (from above) in degree.

A formal power series f is said to be symmetricif it is invariant under permutations of the indeterminates.

For example:

1 +x1+x23 is bounded-degree but not symmetric.

(1 +x1) (1 +x2) (1 +x3)· · · is symmetric but not bounded-degree.

Let Λbe the set of all symmetric bounded-degree power series in k[[x1,x2,x3, . . .]]. This is ak-subalgebra, called thering of symmetric functions overk.

It is also known as Sym.

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Reminder on symmetric functions

Fix a commutative ring kwith unity. We shall do everything overk.

Consider the ring k[[x1,x2,x3, . . .]] of formal power series in countably many indeterminates.

A formal power series f is said to be bounded-degreeif the monomials it contains are bounded (from above) in degree.

A formal power series f is said to be symmetricif it is invariant under permutations of the indeterminates.

For example:

1 +x1+x23 is bounded-degree but not symmetric.

(1 +x1) (1 +x2) (1 +x3)· · · is symmetric but not bounded-degree.

Let Λ be the set of all symmetric bounded-degree power series in k[[x1,x2,x3, . . .]]. This is ak-subalgebra, called thering of symmetric functions overk.

It is also known as Sym.

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Reminder on symmetric functions

Fix a commutative ring kwith unity. We shall do everything overk.

Consider the ring k[[x1,x2,x3, . . .]] of formal power series in countably many indeterminates.

A formal power series f is said to be bounded-degreeif the monomials it contains are bounded (from above) in degree.

A formal power series f is said to be symmetricif it is invariant under permutations of the indeterminates.

Let Λbe the set of all symmetric bounded-degree power series in k[[x1,x2,x3, . . .]]. This is ak-subalgebra, called thering of symmetric functions overk.

It is also known as Sym.

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Schur functions, part 1: Young diagrams

Let λ= (λ1, λ2, λ3, . . .) be a partition(i.e., a weakly

decreasing sequence of nonnegative integers such that λi = 0 for all i 0).

We commonly omit trailing zeroes: e.g., the partition

(4,2,2,1,0,0,0,0, . . .) is identified with the tuple (4,2,2,1).

The Young diagramof λis like a matrix, but the rows have different lengths, and are left-aligned; the i-th row hasλi cells.

Examples:

The Young diagram of (3,2) has the form .

The Young diagram of (4,2,1) has the form .

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Schur functions, part 1: Young diagrams

Let λ= (λ1, λ2, λ3, . . .) be a partition(i.e., a weakly

decreasing sequence of nonnegative integers such that λi = 0 for all i 0).

We commonly omit trailing zeroes: e.g., the partition

(4,2,2,1,0,0,0,0, . . .) is identified with the tuple (4,2,2,1).

The Young diagramof λis like a matrix, but the rows have different lengths, and are left-aligned; the i-th row hasλi cells.

Examples:

The Young diagram of (3,2) has the form .

The Young diagram of (4,2,1) has the form .

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Schur functions, part 2: semistandard tableaux

Asemistandard tableau of shapeλis the Young diagram of λ, filled with positive integers, such that

the entries in eachrow are weaklyincreasing;

the entries in eachcolumn arestrictly increasing.

Examples:

A semistandard tableau of shape (3,2) is

2 3 3

3 5 .

A semistandard tableau of shape (4,2,1) is

2 2 3 4

3 4 5

.

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Schur functions, part 2: semistandard tableaux

Asemistandard tableau of shapeλis the Young diagram of λ, filled with positive integers, such that

the entries in eachrow are weaklyincreasing;

the entries in eachcolumn arestrictly increasing.

Examples:

The semistandard tableaux of shape (3,2) are the arrays of the form

a b c d e

with a≤b≤c andd ≤e and a<d andb <e.

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Schur functions, part 3: definition of Schur functions Given a partitionλ, we define theSchur function sλ as the power series

sλ = X

T is a semistandard tableau of shapeλ

xT, where xT = Y

pis a cell ofT

xT(p)

(where T(p) denotes the entry ofT in p).

Examples:

s(3,2) = X

a≤b≤c,d≤e, a<d,b<e

xaxbxcxdxe,

because the semistandard tableau T = a b c

d e

contributes the addend xT =xaxbxcxdxe.

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Schur functions, part 3: definition of Schur functions Given a partitionλ, we define theSchur function sλ as the power series

sλ = X

T is a semistandard tableau of shapeλ

xT, where xT = Y

pis a cell ofT

xT(p)

(where T(p) denotes the entry ofT in p).

Examples:

For anyn≥0, we have s(n)= X

i1≤i2≤···≤in

xi1xi2· · ·xin,

since the semistandard tableaux of shape (n) are the fillings

T = i1 i2 · · · in with i1≤i2≤ · · · ≤in.

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Schur functions, part 3: definition of Schur functions Given a partitionλ, we define theSchur function sλ as the power series

sλ = X

T is a semistandard tableau of shapeλ

xT, where xT = Y

pis a cell ofT

xT(p)

(where T(p) denotes the entry ofT in p).

Examples:

For anyn≥0, we have s(n)= X

i1≤i2≤···≤in

xi1xi2· · ·xin,

since the semistandard tableaux of shape (n) are the fillings

T = i1 i2 · · · in with i1≤i2≤ · · · ≤in.

This symmetric function s(n) is commonly calledhn.

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Schur functions, part 3: definition of Schur functions Given a partitionλ, we define theSchur function sλ as the power series

sλ = X

T is a semistandard tableau of shapeλ

xT, where xT = Y

pis a cell ofT

xT(p)

(where T(p) denotes the entry ofT in p).

Examples:

For anyn≥0, consider the partition (1n) := (1,1, . . . ,1) (withn entries). Then,

s(1n) = X

i1<i2<···<in

xi1xi2· · ·xin,

since the semistandard tableaux of shape (1n) are the fillings T = i1

i2 ... ... in

with i1<i2 <· · ·<in.

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Schur functions, part 3: definition of Schur functions Given a partitionλ, we define theSchur function sλ as the power series

sλ = X

T is a semistandard tableau of shapeλ

xT, where xT = Y

pis a cell ofT

xT(p)

(where T(p) denotes the entry ofT in p).

Examples:

For anyn≥0, consider the partition (1n) := (1,1, . . . ,1) (withn entries). Then,

s(1n) = X

i1<i2<···<in

xi1xi2· · ·xin,

since the semistandard tableaux of shape (1n) are the fillings T = i1

i2 ... ... in

with i1<i2 <· · ·<in.

This symmetric function s(1n) is commonly called en.

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Schur functions, part 4: classical properties

Theorem: The Schur function sλ is a symmetric function (=

an element of Λ) for any partitionλ.

Theorem: The family (sλ)λis a partition is a basis of the k-module Λ.

Theorem: Fixn ≥0. Letλ= (λ1, λ2, . . . , λn) be a partition with at mostn nonzero entries. Then,

sλ(x1,x2, . . . ,xn)

= det

xiλj+n−j

1≤i,j≤n

| {z }

this is called analternant

det

xin−j

1≤i,j≤n

| {z }

= Q

1≤i<j≤n(xi−xj)

(= the Vandermonde determinant)

.

Here, for any f ∈Λ, we letf (x1,x2, . . . ,xn) denote the result of substituting 0 for xn+1,xn+2,xn+3, . . . in f; this is a symmetricpolynomial in x1,x2, . . . ,xn.

For proofs, see any text on symmetric functions (e.g., Stanley’s EC2, or Grinberg-Reiner, or Mark Wildon’s notes).

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Schur functions, part 4: classical properties

Theorem: The Schur function sλ is a symmetric function (=

an element of Λ) for any partitionλ.

Theorem: The family (sλ)λis a partition is a basis of the k-module Λ.

Theorem: Fixn ≥0. Letλ= (λ1, λ2, . . . , λn) be a partition with at mostn nonzero entries. Then,

sλ(x1,x2, . . . ,xn)

= det

xiλj+n−j

1≤i,j≤n

| {z }

this is called analternant

det

xin−j

1≤i,j≤n

| {z }

= Q

1≤i<j≤n(xi−xj)

(= the Vandermonde determinant)

.

Here, for any f ∈Λ, we letf (x1,x2, . . . ,xn) denote the result of substituting 0 for xn+1,xn+2,xn+3, . . . in f; this is a

symmetricpolynomial in x1,x2, . . . ,xn.

For proofs, see any text on symmetric functions (e.g., Stanley’s EC2, or Grinberg-Reiner, or Mark Wildon’s notes).

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Schur functions, part 4: classical properties

Theorem: The Schur function sλ is a symmetric function (=

an element of Λ) for any partitionλ.

Theorem: The family (sλ)λis a partition is a basis of the k-module Λ.

Theorem: Fixn ≥0. Letλ= (λ1, λ2, . . . , λn) be a partition with at mostn nonzero entries. Then,

sλ(x1,x2, . . . ,xn)

= det

xiλj+n−j

1≤i,j≤n

| {z }

this is called analternant

det

xin−j

1≤i,j≤n

| {z }

= Q

1≤i<j≤n(xi−xj)

(= the Vandermonde determinant)

.

Here, for any f ∈Λ, we letf (x1,x2, . . . ,xn) denote the result of substituting 0 for xn+1,xn+2,xn+3, . . . in f; this is a

symmetricpolynomial in x1,x2, . . . ,xn.

For proofs, see any text on symmetric functions (e.g., Stanley’s EC2, or Grinberg-Reiner, or Mark Wildon’s notes).

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Littlewood–Richardson coefficients: definition

Ifµ andν are two partitions, thensµsν belongs to Λ (since Λ is a ring) and thus can be written in the form

sµsν = X

λis a partition

cµ,νλ sλ for somecµ,νλ ∈k (since thesλ form a basis of Λ).

The coefficients cµ,νλ are integers, and are called the Littlewood–Richardson coefficients.

Example:

Theorem: The coefficients cµ,νλ are nonnegative integers. Various combinatorial interpretations (“Littlewood–Richardson rules”) for them are known.

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Littlewood–Richardson coefficients: definition

Ifµ andν are two partitions, thensµsν belongs to Λ (since Λ is a ring) and thus can be written in the form

sµsν = X

λis a partition

cµ,νλ sλ

for somecµ,νλ ∈k (since thesλ form a basis of Λ).

The coefficients cµ,νλ are integers, and are called the Littlewood–Richardson coefficients.

Example:

Theorem: The coefficients cµ,νλ are nonnegative integers. Various combinatorial interpretations (“Littlewood–Richardson rules”) for them are known.

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Littlewood–Richardson coefficients: definition

Ifµ andν are two partitions, thensµsν belongs to Λ (since Λ is a ring) and thus can be written in the form

sµsν = X

λis a partition

cµ,νλ sλ

for somecµ,νλ ∈k (since thesλ form a basis of Λ).

The coefficients cµ,νλ are integers, and are called the Littlewood–Richardson coefficients.

Example:

Theorem: The coefficients cµ,νλ are nonnegative integers. Various combinatorial interpretations (“Littlewood–Richardson rules”) for them are known.

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Littlewood–Richardson coefficients: definition

Ifµ andν are two partitions, thensµsν belongs to Λ (since Λ is a ring) and thus can be written in the form

sµsν = X

λis a partition

cµ,νλ sλ

for somecµ,νλ ∈k (since thesλ form a basis of Λ).

The coefficients cµ,νλ are integers, and are called the Littlewood–Richardson coefficients.

Example:

s(2,1)s(3,1)=s(3,2,1,1)+s(3,2,2)+s(3,3,1) +s(4,1,1,1)+ 2s(4,2,1)+s(4,3) +s(5,1,1)+s(5,2)

Theorem: The coefficients cµ,νλ are nonnegative integers. Various combinatorial interpretations (“Littlewood–Richardson rules”) for them are known.

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Littlewood–Richardson coefficients: definition

Ifµ andν are two partitions, thensµsν belongs to Λ (since Λ is a ring) and thus can be written in the form

sµsν = X

λis a partition

cµ,νλ sλ

for somecµ,νλ ∈k (since thesλ form a basis of Λ).

The coefficients cµ,νλ are integers, and are called the Littlewood–Richardson coefficients.

Example:

s(2,1)s(3,1)=s(3,2,1,1)+s(3,2,2)+s(3,3,1) +s(4,1,1,1)+2s(4,2,1)+s(4,3) +s(5,1,1)+s(5,2),

so c(2,1),(3,1)(4,2,1) = 2 and c(2,1),(3,1)(3,3,1) = 1.

Theorem: The coefficients cµ,νλ are nonnegative integers.

Various combinatorial interpretations (“Littlewood–Richardson rules”) for them are known.

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Littlewood–Richardson coefficients: definition

Ifµ andν are two partitions, thensµsν belongs to Λ (since Λ is a ring) and thus can be written in the form

sµsν = X

λis a partition

cµ,νλ sλ

for somecµ,νλ ∈k (since thesλ form a basis of Λ).

The coefficients cµ,νλ are integers, and are called the Littlewood–Richardson coefficients.

Example:

s(2,1)s(3,1)=s(3,2,1,1)+s(3,2,2)+s(3,3,1) +s(4,1,1,1)+2s(4,2,1)+s(4,3) +s(5,1,1)+s(5,2),

so c(2,1),(3,1)(4,2,1) = 2 and c(2,1),(3,1)(3,3,1) = 1.

Theorem: The coefficients cµ,νλ are nonnegative integers.

Various combinatorial interpretations (“Littlewood–Richardson rules”) for them are known.

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Why Littlewood–Richardson coefficients? 1

Before we say more about Littlewood–Richardson coefficients, let us see where else they appear.

For k=Z, the cohomology ring H(Gr (k,n))

of the complex Grassmannian Gr (k,n) (ofk-subspaces inCn) is isomorphic to

Λ(hn−k+1,hn−k+2, . . . ,hn,ek+1,ek+2,ek+3, . . .)ideal. The cohomology classes corresponding to the Schur functions sλ are the Schubert classes– the classes of theSchubert varieties. Roughly speaking, these subdivide Gr (k,n) according to the positions of the pivots in the row-reduced echelon form.

Thus, the Littlewood–Richardson coefficients cµ,νλ are intersection multiplicities of these Schubert varieties. For details, see:

Laurent Manivel,Symmetric Functions, Schubert Polynomials and Degeneracy Loci, AMS/SMF 1998.

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Why Littlewood–Richardson coefficients? 1 For k=Z, the cohomology ring

H(Gr (k,n))

of the complex Grassmannian Gr (k,n) (ofk-subspaces inCn) is isomorphic to

Λ(hn−k+1,hn−k+2, . . . ,hn,ek+1,ek+2,ek+3, . . .)ideal. The cohomology classes corresponding to the Schur functions sλ are the Schubert classes– the classes of theSchubert varieties. Roughly speaking, these subdivide Gr (k,n) according to the positions of the pivots in the row-reduced echelon form.

Thus, the Littlewood–Richardson coefficients cµ,νλ are intersection multiplicities of these Schubert varieties.

For details, see:

Laurent Manivel,Symmetric Functions, Schubert Polynomials and Degeneracy Loci, AMS/SMF 1998.

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Why Littlewood–Richardson coefficients? 1 For k=Z, the cohomology ring

H(Gr (k,n))

of the complex Grassmannian Gr (k,n) (ofk-subspaces inCn) is isomorphic to

Λ(hn−k+1,hn−k+2, . . . ,hn,ek+1,ek+2,ek+3, . . .)ideal. The cohomology classes corresponding to the Schur functions sλ are the Schubert classes– the classes of theSchubert varieties. Roughly speaking, these subdivide Gr (k,n) according to the positions of the pivots in the row-reduced echelon form.

Thus, the Littlewood–Richardson coefficients cµ,νλ are intersection multiplicities of these Schubert varieties.

For details, see:

Laurent Manivel,Symmetric Functions, Schubert Polynomials and Degeneracy Loci, AMS/SMF 1998.

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Why Littlewood–Richardson coefficients? 1 For k=Z, the cohomology ring

H(Gr (k,n))

of the complex Grassmannian Gr (k,n) (ofk-subspaces inCn) is isomorphic to

Λ(hn−k+1,hn−k+2, . . . ,hn,ek+1,ek+2,ek+3, . . .)ideal. The cohomology classes corresponding to the Schur functions sλ are the Schubert classes– the classes of theSchubert varieties. Roughly speaking, these subdivide Gr (k,n) according to the positions of the pivots in the row-reduced echelon form.

Thus, the Littlewood–Richardson coefficients cµ,νλ are intersection multiplicities of these Schubert varieties.

For details, see:

Laurent Manivel,Symmetric Functions, Schubert Polynomials and Degeneracy Loci, AMS/SMF 1998.

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Why Littlewood–Richardson coefficients? 2

Here is another interpretation of Littlewood–Richardson coefficients, also related to subspaces of a vector space.

Let V be a finite-dimensional vector space.

The Jordan type J(A) of a nilpotent endomorphism

A∈EndV is the partition (λ1, λ2, λ3, . . .) withλi being the size of the i-th largest Jordan block of A.

Pick a nilpotent endomorphismA∈EndV, and let λ=J(λ) be its Jordan type. Let µ andν be two further partitions. When is there an A-invariant vector subspaceW ⊆V with

J(A) =λ, J(A|W) =µ, J(A/W) =ν? (A/W is the endomorphism ofV/W induced byA.) Precisely when cµ,νλ 6= 0.

Moreover, the set of all suchW is a subvariety of Gr (k,n), and has cµ,νλ irreducible components.

For details, see:

Marc van Leeuwen,Flag Varieties and Interpretations of Young Tableau Algorithms.

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Why Littlewood–Richardson coefficients? 2 Let V be a finite-dimensional vector space.

The Jordan type J(A)of a nilpotent endomorphism

A∈EndV is the partition (λ1, λ2, λ3, . . .) withλi being the size of the i-th largest Jordan block of A.

Pick a nilpotent endomorphismA∈EndV, and let λ=J(λ) be its Jordan type. Let µ andν be two further partitions.

When is there an A-invariant vector subspaceW ⊆V with J(A) =λ, J(A|W) =µ, J(A/W) =ν?

(A/W is the endomorphism ofV/W induced byA.)

Precisely when cµ,νλ 6= 0.

Moreover, the set of all suchW is a subvariety of Gr (k,n), and has cµ,νλ irreducible components.

For details, see:

Marc van Leeuwen,Flag Varieties and Interpretations of Young Tableau Algorithms.

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Why Littlewood–Richardson coefficients? 2 Let V be a finite-dimensional vector space.

The Jordan type J(A)of a nilpotent endomorphism

A∈EndV is the partition (λ1, λ2, λ3, . . .) withλi being the size of the i-th largest Jordan block of A.

Pick a nilpotent endomorphismA∈EndV, and let λ=J(λ) be its Jordan type. Let µ andν be two further partitions.

When is there an A-invariant vector subspaceW ⊆V with J(A) =λ, J(A|W) =µ, J(A/W) =ν?

(A/W is the endomorphism ofV/W induced byA.) Precisely when cµ,νλ 6= 0.

Moreover, the set of all suchW is a subvariety of Gr (k,n), and has cµ,νλ irreducible components.

For details, see:

Marc van Leeuwen,Flag Varieties and Interpretations of Young Tableau Algorithms.

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Why Littlewood–Richardson coefficients? 2 Let V be a finite-dimensional vector space.

The Jordan type J(A)of a nilpotent endomorphism

A∈EndV is the partition (λ1, λ2, λ3, . . .) withλi being the size of the i-th largest Jordan block of A.

Pick a nilpotent endomorphismA∈EndV, and let λ=J(λ) be its Jordan type. Let µ andν be two further partitions.

When is there an A-invariant vector subspaceW ⊆V with J(A) =λ, J(A|W) =µ, J(A/W) =ν?

(A/W is the endomorphism ofV/W induced byA.) Precisely when cµ,νλ 6= 0.

Moreover, the set of all suchW is a subvariety of Gr (k,n), and has cµ,νλ irreducible components.

For details, see:

Marc van Leeuwen,Flag Varieties and Interpretations of Young Tableau Algorithms.

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Why Littlewood–Richardson coefficients? 2 Let V be a finite-dimensional vector space.

The Jordan type J(A)of a nilpotent endomorphism

A∈EndV is the partition (λ1, λ2, λ3, . . .) withλi being the size of the i-th largest Jordan block of A.

Pick a nilpotent endomorphismA∈EndV, and let λ=J(λ) be its Jordan type. Let µ andν be two further partitions.

When is there an A-invariant vector subspaceW ⊆V with J(A) =λ, J(A|W) =µ, J(A/W) =ν?

(A/W is the endomorphism ofV/W induced byA.) Precisely when cµ,νλ 6= 0.

Moreover, the set of all suchW is a subvariety of Gr (k,n), and has cµ,νλ irreducible components.

For details, see:

Marc van Leeuwen,Flag Varieties and Interpretations of Young Tableau Algorithms.

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Why Littlewood–Richardson coefficients? 3

Fix anN ≥0. The irreducible polynomial representations Vλ of the group GL (N) := GL (N,C) are indexed by partitions having ≤N entries.

Their charactersare the Schur functions sλ.

The Littlewood–Richardson coefficients tell how to decompose the tensor product of two such representations:

Vµ⊗Vν =M

λ

V⊕c

λ µ,ν

λ .

For details, see:

William Fulton,Young Tableaux, CUP 1997.

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Why Littlewood–Richardson coefficients? 3

Fix anN ≥0. The irreducible polynomial representations Vλ of the group GL (N) := GL (N,C) are indexed by partitions having ≤N entries.

Their charactersare the Schur functions sλ.

The Littlewood–Richardson coefficients tell how to decompose the tensor product of two such representations:

Vµ⊗Vν =M

λ

V⊕c

λ µ,ν

λ .

For details, see:

William Fulton,Young Tableaux, CUP 1997.

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Why Littlewood–Richardson coefficients? 3

Fix anN ≥0. The irreducible polynomial representations Vλ of the group GL (N) := GL (N,C) are indexed by partitions having ≤N entries.

Their charactersare the Schur functions sλ.

The Littlewood–Richardson coefficients tell how to decompose the tensor product of two such representations:

Vµ⊗Vν =M

λ

V⊕c

λ µ,ν

λ .

For details, see:

William Fulton,Young Tableaux, CUP 1997.

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Skew semistandard tableaux

In order to formulate the classic (or, at least, best known) Littlewood–Richardson rule, we need a

Definition:

Two partitionsλ= (λ1, λ2, λ3, . . .) and

µ= (µ1, µ2, µ3, . . .) are said to satisfyµ⊆λif each i ≥1 satisfies µi ≤λi.

(Equivalently: if the Young diagram of µis contained in that ofλ.)

Askew partition is a pair (λ, µ) of two partitions satisfying µ⊆λ. Such a pair is denoted byλ/µ.

Ifλ/µis a skew partition, then theYoung diagram of λ/µis obtained from the Young diagram λwhen all cells of the Young diagram ofµare removed.

Semistandard tableaux of shape λ/µare defined just as ones of shape λ, except that we are now only filling the cells of λ/µ.

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Skew semistandard tableaux

In order to formulate the classic (or, at least, best known) Littlewood–Richardson rule, we need a

Definition:

Two partitionsλ= (λ1, λ2, λ3, . . .) and

µ= (µ1, µ2, µ3, . . .) are said to satisfyµ⊆λif each i ≥1 satisfies µi ≤λi.

Askew partition is a pair (λ, µ) of two partitions satisfying µ⊆λ. Such a pair is denoted byλ/µ.

Ifλ/µis a skew partition, then theYoung diagram of λ/µis obtained from the Young diagram λwhen all cells of the Young diagram ofµare removed.

Semistandard tableaux of shape λ/µare defined just as ones of shape λ, except that we are now only filling the cells of λ/µ.

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Skew semistandard tableaux

In order to formulate the classic (or, at least, best known) Littlewood–Richardson rule, we need a

Definition:

Two partitionsλ= (λ1, λ2, λ3, . . .) and

µ= (µ1, µ2, µ3, . . .) are said to satisfyµ⊆λif each i ≥1 satisfies µi ≤λi.

Askew partition is a pair (λ, µ) of two partitions satisfying µ⊆λ. Such a pair is denoted byλ/µ.

Ifλ/µis a skew partition, then theYoung diagram of λ/µis obtained from the Young diagram λwhen all cells of the Young diagram ofµare removed.

Example: The Young diagram of (4,2,1)/(1,1) is

Semistandard tableaux of shape λ/µare defined just as ones of shapeλ, except that we are now only filling the cells of λ/µ.

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Skew semistandard tableaux

In order to formulate the classic (or, at least, best known) Littlewood–Richardson rule, we need a

Definition:

Two partitionsλ= (λ1, λ2, λ3, . . .) and

µ= (µ1, µ2, µ3, . . .) are said to satisfyµ⊆λif each i ≥1 satisfies µi ≤λi.

Askew partition is a pair (λ, µ) of two partitions satisfying µ⊆λ. Such a pair is denoted byλ/µ.

Ifλ/µis a skew partition, then theYoung diagram of λ/µis obtained from the Young diagram λwhen all cells of the Young diagram ofµare removed.

Semistandard tableaux of shape λ/µare defined just as ones of shapeλ, except that we are now only filling the cells of λ/µ.

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Littlewood–Richardson rule: the classical version Littlewood–Richardson rule: Letλ,µand ν be three partitions. Then,cµ,νλ is the number of semistandard tableaux T of shape λ/µsuch that contT =ν and such that

cont (T |cols≥j) is a partition for eachj. Here,

contT denotes the sequence (c1,c2,c3, . . .), where ci is the number of entries equal to i in T;

T |cols≥j is what obtained from T when the first j −1 columns are deleted.

Example: c(2,1),(3,1)(4,2,1) = 2 due to the two tableaux 1 1

1 2

and 1 1

2 1

.

The shortest proof is due to Stembridge (using ideas by Gasharov); see John R. Stembridge, A Concise Proof of the Littlewood-Richardson Rule, 2002, or Section 2.6 in

Grinberg-Reiner. 14 / 46

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Littlewood–Richardson rule: the classical version Littlewood–Richardson rule: Letλ,µand ν be three partitions. Then,cµ,νλ is the number of semistandard tableaux T of shape λ/µsuch that contT =ν and such that

cont (T |cols≥j) is a partition for eachj. Here,

contT denotes the sequence (c1,c2,c3, . . .), where ci is the number of entries equal to i in T;

T |cols≥j is what obtained from T when the first j −1 columns are deleted.

Example: c(2,1),(3,1)(4,2,1) = 2 due to the two tableaux 1 1

1 2

and 1 1

2 1

.

The shortest proof is due to Stembridge (using ideas by Gasharov); see John R. Stembridge, A Concise Proof of the Littlewood-Richardson Rule, 2002, or Section 2.6 in

Grinberg-Reiner. 14 / 46

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Basic properties of Littlewood–Richardson coefficients Gradedness: cµ,νλ = 0 unless|λ|=|µ|+|ν|, where|κ|

denotes the size(i.e., the sum of the entries) of a partitionκ.

(This is because Λ is a graded ring and the sλ are homogeneous.)

Transposition symmetry: cµ,νλ =cµλttt, whereκt denotes thetranspose of a partitionκ (i.e., the partition whose Young diagram is obtained from that of κby flipping across the main diagonal).

Commutativity: cµ,νλ =cν,µλ .

(Obvious from the definition, but hard to prove combinatorially using the Littlewood–Richardson rule.)

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Basic properties of Littlewood–Richardson coefficients Gradedness: cµ,νλ = 0 unless|λ|=|µ|+|ν|, where|κ|

denotes the size(i.e., the sum of the entries) of a partitionκ.

(This is because Λ is a graded ring and the sλ are homogeneous.)

Transposition symmetry: cµ,νλ =cµλttt, whereκt denotes thetranspose of a partitionκ (i.e., the partition whose Young diagram is obtained from that of κby flipping across the main diagonal).

Example:

t

=

Commutativity: cµ,νλ =cν,µλ .

(Obvious from the definition, but hard to prove combinatorially using the Littlewood–Richardson rule.)

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Basic properties of Littlewood–Richardson coefficients Gradedness: cµ,νλ = 0 unless|λ|=|µ|+|ν|, where|κ|

denotes the size(i.e., the sum of the entries) of a partitionκ.

(This is because Λ is a graded ring and the sλ are homogeneous.)

Transposition symmetry: cµ,νλ =cµλttt, whereκt denotes thetranspose of a partitionκ (i.e., the partition whose Young diagram is obtained from that of κby flipping across the main diagonal).

Commutativity: cµ,νλ =cν,µλ .

(Obvious from the definition, but hard to prove combinatorially using the Littlewood–Richardson rule.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Example: Ifn= 5, then

(3,1,1)∨7= (3,1,1,0,0)∨7= (7−0,7−0,7−1,7−1,7−3)

= (7,7,6,6,4).

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Illustration: Ifn= 3, then (3,2)∨4 =

∨4

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Illustration: Ifn= 3, then (3,2)∨4 =

∨4

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Illustration: Ifn= 3, then (3,2)∨4=

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Illustration: Ifn= 3, then (3,2)∨4=

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Illustration: Ifn= 3, then (3,2)∨4=

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Illustration: Ifn= 3, then

(3,2)∨4 = (4,2,1).

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k.

Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k.

Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. (This can be proved by applying skew Schur functions to x1−1,x2−1, . . . ,xn−1, or by interpreting Schur functions as fundamental classes in the cohomology of the Grassmannian.

See Exercise 2.9.15 in Grinberg-Reiner for the former proof.) Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are ≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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Littlewood–Richardson coefficients: more symmetries Fixn ∈N. LetPar[n]be the set of all partitions having at most n nonzero entries.

Ifλ= (λ1, λ2, . . . , λn)∈Par[n], and ifk ≥0 is such that all entries of λare ≤k, then λ∨k shall denote the partition

(k−λn,k−λn−1, . . . ,k−λ1)∈Par[n].

This is called thek-complementof λ.

Complementation symmetry I: Let λ, µ, ν∈Par[n] and k ≥0 be such that all entries of λ, µ, ν are≤k. Then,

cµ,νλ =cν,µλ =cλµ∨k∨k =cν,λµ∨k∨k =cµ,λν∨k∨k =cλν∨k∨k. Complementation symmetry II: Let λ, µ, ν∈Par[n] and q,r ≥0 be such that all entries of µare ≤q, and all entries of ν are ≤r. Then:

If all entries of λare ≤q+r, then cµ,νλ =cµλ∨q∨(q+r)∨r. If not, thencµ,νλ = 0.

(See, e.g., Exercise 2.9.16 in Grinberg-Reiner.)

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The Briand–Rosas symmetry

In arXiv:2004.04995, Emmanuel Briand and Mercedas Rosas have used a computer (and prior work of Rassart, Knutson and Tao, which made the problem computable) to classify all such “symmetries” of Littlewood–Richardson coefficientscµ,νλ with λ, µ, ν∈Par[n] for fixed

n ∈ {3,4, . . . ,7}.

For n∈ {4,5, . . . ,7}, they only found the complementation symmetries above, as well as the trivial translation symmetries (adding 1 to each entry of λandν does not changecµ,νλ ; nor does adding 1 to each entry ofλand µ).

For n= 3, they found an extra symmetry: c123)

12),(ν12)=c113)

11−λ221−λ2),(λ22) .

(Read the right hand side as 0 if the tuples are not partitions.) Question: Is there a non-computer proof? What is the meaning of this identity?

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