Littlewood–Richardson rule

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History

Littlewood–Richardson tableaux

Example

A more geometrical description

An algorithmic form of the rule

Littlewood–Richardson coefficients

Generalizations and special cases

Examples

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Littlewood–Richardson rule

In mathematics, the Littlewood–Richardson rule is a combinatorial description of the coefficients that arise when decomposing a product of two Schur functions as a linear combination of other Schur functions. These coefficients are natural numbers, which the Littlewood–Richardson rule describes as counting certain skew tableaux. They occur in many other mathematical contexts, for instance as multiplicity in the decomposition of tensor products of irreducible representations of general linear groups (or related groups like the special linear and special unitary groups), or in the decomposition of certain induced representations in the representation theory of the symmetric group, or in the area of algebraic combinatorics dealing with Young tableaux and symmetric polynomials.

Littlewood–Richardson coefficients depend on threepartitions, say, of whichanddescribe the Schur functions being multiplied, andgives the Schur function of which this is the coefficient in the linear combination; in other words they are the coefficientssuch that

The Littlewood–Richardson rule states thatis equal to the number of Littlewood–Richardson tableaux ofskew shapeand of weight.

History

Unfortunately the Littlewood–Richardson rule is much harder to prove than was at first suspected. The author was once told that the Littlewood–Richardson rule helped to get men on the moon but was not proved until after they got there. Gordon James (1987)

The Littlewood–Richardson rule was first stated by D. E. Littlewood and A. R. Richardson (1934, theorem III p. 119) but though they claimed it as a theorem they only proved it in some fairly simple special cases. Robinson (1938) claimed to complete their proof, but his argument had gaps, though it was so obscurely written that these gaps were not noticed for some time, and his argument is reproduced in the book (Littlewood 1950). Some of the gaps were later filled by Macdonald (1995). The first rigorous proofs of the rule were given four decades after it was found, by Schützenberger (1977) and Thomas (1974), after the necessary combinatorial theory was developed by C. Schensted (1961), Schützenberger (1963), and Knuth (1970) in their work on the Robinson–Schensted correspondence. There are now several short proofs of the rule, such as (Gasharov 1998), and (Stembridge 2002) using Bender-Knuth involutions. Littelmann (1994) used the Littelmann path model to generalize the Littlewood–Richardson rule to other semisimple Lie groups.

The Littlewood–Richardson rule is notorious for the number of errors that appeared prior to its complete, published proof. Several published attempts to prove it are incomplete, and it is particularly difficult to avoid errors when doing hand calculations with it: even the original example in D. E. Littlewood and A. R. Richardson (1934) contains an error.

Littlewood–Richardson tableaux

A Littlewood–Richardson tableau is a skewsemistandard tableauwith the additional property that the sequence obtained by concatenating its reversed rows is alattice word(or lattice permutation), which means that in every initial part of the sequence any numberoccurs at least as often as the number. Another equivalent (though not quite obviously so) characterization is that the tableau itself, and any tableau obtained from it by removing some number of its leftmost columns, has a weakly decreasing weight. Many other combinatorial notions have been found that turn out to be in bijection with Littlewood–Richardson tableaux, and can therefore also be used to define the Littlewood–Richardson coefficients.

Example

Consider the case that,and. Then the fact thatcan be deduced from the fact that the two tableaux shown at the right are the only two Littlewood–Richardson tableaux of shapeand weight. Indeed, since the last box on the first nonempty line of the skew diagram can only contain an entry 1, the entire first line must be filled with entries 1 (this is true for any Littlewood–Richardson tableau); in the last box of the second row we can only place a 2 by column strictness and the fact that our lattice word cannot contain any larger entry before it contains a 2. For the first box of the second row we can now either use a 1 or a 2. Once that entry is chosen, the third row must contain the remaining entries to make the weight (3,2,1), in a weakly increasing order, so we have no choice left any more; in both case it turns out that we do find a Littlewood–Richardson tableau.

A more geometrical description

The condition that the sequence of entries read from the tableau in a somewhat peculiar order form a lattice word can be replaced by a more local and geometrical condition. Since in a semistandard tableau equal entries never occur in the same column, one can number the copies of any value from right to left, which is their order of occurrence in the sequence that should be a lattice word. Call the number so associated to each entry its index, and write an entry i with index j as i[j]. Now if some Littlewood–Richardson tableau contains an entrywith index j, then that entry i[j] should occur in a row strictly below that of(which certainly also occurs, since the entry i − 1 occurs as least as often as the entry i does). In fact the entry i[j] should also occur in a column no further to the right than that same entry(which at first sight appears to be a stricter condition). If the weight of the Littlewood–Richardson tableau is fixed beforehand, then one can form a fixed collection of indexed entries, and if these are placed in a way respecting those geometric restrictions, in addition to those ofsemistandard tableauxand the condition that indexed copies of the same entries should respect right-to-left ordering of the indexes, then the resulting tableaux are guaranteed to be Littlewood–Richardson tableaux.

An algorithmic form of the rule

The Littlewood–Richardson as stated above gives a combinatorial expression for individual Littlewood–Richardson coefficients, but gives no indication of a practical method to enumerate the Littlewood–Richardson tableaux in order to find the values of these coefficients. Indeed, for giventhere is no simple criterion to determine whether any Littlewood–Richardson tableaux of shapeand of weightexist at all (although there are a number of necessary conditions, the simplest of which is); therefore it seems inevitable that in some cases one has to go through an elaborate search, only to find that no solutions exist.

Nevertheless, the rule leads to a quite efficient procedure to determine the full decomposition of a product of Schur functions, in other words to determine all coefficientsfor fixed λ and μ, but varying ν. This fixes the weight of the Littlewood–Richardson tableaux to be constructed and the "inner part" λ of their shape, but leaves the "outer part" ν free. Since the weight is known, the set of indexed entries in the geometric description is fixed. Now for successive indexed entries, all possible positions allowed by the geometric restrictions can be tried in abacktrackingsearch. The entries can be tried in increasing order, while among equal entries they can be tried by decreasing index. The latter point is the key to efficiency of the search procedure: the entry i[j] is then restricted to be in a column to the right of, but no further to the right than(if such entries are present). This strongly restricts the set of possible positions, but *always leaves at least one valid position for*; thus every placement of an entry will give rise to at least one complete Littlewood–Richardson tableau, and thesearch treecontains no dead ends.

A similar method can be used to find all coefficientsfor fixed λ and ν, but varying μ.

Littlewood–Richardson coefficients

The Littlewood–Richardson coefficients cνλμ appear in the following interrelated ways:

They are the structure constants for the product in the ring of symmetric functions with respect to the basis of Schur functions

or equivalently c^ν
_λμ is the inner product of s_νand s_λs_μ.

They express skew Schur functions in terms of Schur functions

The cνλμ appear as intersection numbers on a Grassmannian:

where σ_μis the class of theSchubert varietyof a Grassmannian corresponding to μ.

cνλμ is the number of times the irreducible representation V**λ ⊗ V**μ of the product of symmetric groups S|λ| × S|μ| appears in the restriction of the representation V**ν of S|ν| to S|λ| × S|μ|. By Frobenius reciprocity this is also the number of times that V**ν occurs in the representation of S|ν| induced from V**λ ⊗ V**μ.
The cνλμ appear in the decomposition of the tensor product (Fulton 1997) of two Schur modules (irreducible representations of special linear groups)

cνλμ is the number of standard Young tableaux of shape ν/μ that are jeu de taquin equivalent to some fixed standard Young tableau of shape λ.
cνλμ is the number of Littlewood–Richardson tableaux of shape ν/λ and of weight μ.
cνλμ is the number of pictures between μ and ν/λ.

Generalizations and special cases

Zelevinsky (1981) extended the Littlewood–Richardson rule to skew Schur functions as follows:

where the sum is over all tableaux T on μ/ν such that for all j, the sequence of integers λ+ω(T≥j) is non-increasing, and ω is the weight.

Pieri's formula, which is the special case of the Littlewood–Richardson rule in the case when one of the partitions has only one part, states that

where S**n is the Schur function of a partition with one row and the sum is over all partitions λ obtained from μ by adding n elements to its Ferrers diagram, no two in the same column.

If both partitions are rectangular in shape, the sum is also multiplicity free (Okada 1998). Fix a, b, p, and q positive integers with pq. Denote bythe partition with p parts of length a. The partitions indexing nontrivial components ofare those partitionswith lengthsuch that

For example,

Examples

The examples of Littlewood-Richardson coefficients below are given in terms of products of Schur polynomials Sπ, indexed by partitions π, using the formula

All coefficients with ν at most 4 are given by:

S0Sπ = Sπ for any π. where S0=1 is the Schur polynomial of the empty partition
S1S1 = S2 + S11
S2S1 = S3 + S21
S11S1 = S111 + S21
S3S1 = S4 + S31
S21S1 = S31 + S22 + S211
S2S2 = S4 + S31 + S22
S2S11 = S31 + S211
S111S1 = S1111 + S211
S11S11 = S1111 + S211 + S22

Most of the coefficients for small partitions are 0 or 1, which happens in particular whenever one of the factors is of the form Sn or S11...1, because of Pieri's formula and its transposed counterpart. The simplest example with a coefficient larger than 1 happens when neither of the factors has this form:

S21S21 = S42 + S411 + S33 + 2S321 + S3111 + S222 + S2211.

For larger partitions the coefficients become more complicated. For example,

S321S321 = S642 +S6411 +S633 +2S6321 +S63111 +S6222 +S62211 +S552 +S5511 +2S543 +4S5421 +2S54111 +3S5331 +3S5322 +4S53211 +S531111 +2S52221 +S522111 +S444 +3S4431 +2S4422 +3S44211 +S441111 +3S4332 +3S43311 +4S43221 +2S432111 +S42222 +S422211 +S3333 +2S33321 +S333111 +S33222 +S332211 with 34 terms and total multiplicity 62, and the largest coefficient is 4
S4321S4321 is a sum of 206 terms with total multiplicity is 930, and the largest coefficient is 18.
S54321S54321 is a sum of 1433 terms with total multiplicity 26704, and the largest coefficient (that of S86543211) is 176.
S654321S654321 is a sum of 10873 terms with total multiplicity is 1458444 (so the average value of the coefficients is more than 100, and they can be as large as 2064).

The original example given by Littlewood & Richardson (1934, p. 122-124) was (after correcting for 3 tableaux they found but forgot to include in the final sum)

S431S221 = S652 + S6511 + S643 + 2S6421 + S64111 + S6331 + S6322 + S63211 + S553 + 2S5521 + S55111 + 2S5431 + 2S5422 + 3S54211 + S541111 + S5332 + S53311 + 2S53221 + S532111 + S4432 + S44311 + 2S44221 + S442111 + S43321 + S43222 + S432211