A Generalized Newton-Girard Identity
Tanay Wakhare

TL;DR
This paper generalizes the Newton-Girard identities, providing new theoretical insights and applications, along with a collection of evaluations of symmetric polynomials where these identities are applicable.
Contribution
The paper introduces a broad generalization of the Newton-Girard identities and compiles various evaluations of symmetric polynomials related to these identities.
Findings
New generalized identities for symmetric polynomials
Applications demonstrating the utility of the generalized identities
Collected evaluations of symmetric polynomials using the new identities
Abstract
We present a generalization of the Newton-Girard identities, along with some applications. As an addendum, we collect many evaluations of symmetric polynomials to which these identities apply.
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Taxonomy
TopicsAdvanced Combinatorial Mathematics · Quantum Mechanics and Non-Hermitian Physics · Quantum chaos and dynamical systems
A Generalized Newton-Girard Identity
Tanay Wakhare
University of Maryland, College Park, MD 20742, USA
Abstract.
We present a generalization of the Newton-Girard identities, along with some applications. As an addendum, we collect many evaluations of symmetric polynomials to which these identities apply.
1. Introduction
The theory of symmetric polynomials has been explored by mathematicians for centuries, and is intimately connected to many different fields, including combinatorial enumeration and the representation theory of the symmetric group. Section 4 contains many examples of special symmetric polynomials, such as binomial coefficients, -binomial coefficients, and Stirling numbers, all of which have been extensively and independently studied. Two of the fundamental identities for symmetric polynomials are the Newton-Girard identities, which state that [1, (Chapter 1, 2.10-2.11)]
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and
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Here, are the elementary symmetric functions, are the complete symmetric functions, and are the power sums. They form generating sets for the ring of symmetric functions, and satisfy the following definitions. Letting denote a (possibly infinite) set of variables, we have
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We require and . Then we have the following formal generating series and products [2]:
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We also introduce some closely related bases for the ring of symmetric functions. Let denote a partition of , so that with and . Then we define . Similarly, we have and . Finally, we define the monomial symmetric functions , where the sum is over the set of permutations giving distinct terms in the sum (so that the coefficient of any monomial in the sum is simply ). When , reduces to an elementary symmetric function.
The derivation of the Newton-Girard identities from these generating products is instructive. There are many different proofs, using everything from recursive approaches to the Cayley-Hamilton Theorem [4] [6] [12]. One of the easiest proofs, detailed by Macdonald [1, Chapter 1], formally manipulates the generating products for and . We begin with and apply the differential operator . We can take a logarithmic derivative of the product, yielding
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We recognize the sum as , which then gives
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Equating coefficients of proves Equation (1.1). Equation (1.2) is proved analogously, by applying the operator to the series and product forms for .
We explore this method in the rest of this paper: taking derivatives and logarithmic derivatives while switching between the product and series forms of , , and . In Section 2 we present a Newton type representation for the power sum . In Section 3 we present the main result of our study: a generalization of the Newton-Girard identities to two arbitrary sets of variables, given in Theorem 4. Finally, in Section 4 we collect some examples of symmetric polynomial evaluations.
2. Newton-type representation for
While Identities (1.1) and (1.2) have been extensively studied in the literature, in Theorem 1 we present a similar expression for for the first time. We note the extreme similarity to (1.1) and (1.2), except for the factor of . The first equality is given by [7, Lemma 2.1], while the second appears to be new.
Theorem 1**.**
We have the Newton-type convolutions
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Proof.
We start with the product form
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By looking at the definition of and , we also observe . This means
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Taking products of both sides and equating coefficients of completes the proof:
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and
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∎
3. Two Variable Newton Identities
We now extend the formulae (1.1) and (1.2) to two (possibly infinite) sets of variables, motivated by the result [2, (6.3)]
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In other words, and are dual bases for the ring of symmetric functions. This motivates us to consider
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In fact, these are generating products for certain symmetric polynomials. This lemma allows us to switch between the product and series forms of , which simplifies the following analysis.
Lemma 2**.**
We have the generating products
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and
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Proof.
We can expand as the generating product for using (1.7) and then factor out the contributions from , yielding
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We now explain the last equality. For what follows, let be a partition of where appears times, appears times, and so on. First, note that the coefficient of will be a polynomial in and . A general term in this polynomial will be times . When we collect terms, we then sum over all possible distinct permutations of the indices . This means that while considering terms corresponding to a particular partition , we can then factor out and then rewrite the resulting sum over monomials in the as . Every partition of will have and terms of this form corresponding to it, leading to the given coefficient.
The second identity is proven with the exact same reasoning:
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∎
When and this product identity specializes to the generating products for and . For instance, the sum reduces to since is only nonzero when consists of a single part, .
Corollary 3**.**
We have the symmetries
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Proof.
The corollary follows from the symmetry of and with respect to and , visible in the definitions (3.2) and (3.3). ∎
Using this product expansion, we can then present a generazation of the Newon-Girard identities.
Theorem 4**.**
We have the generalized Newton-Girard identities
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Proof.
We can repeat the original proof of the Newton-Girard identities for the generating products above, with some minor modifications. We consider and , then apply the differential operator and equate coefficients of . We begin by considering and taking a logarithmic derivative:
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We recognize
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Since by Lemma 2
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we equate coefficients of in
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and
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The same process, applied to , proves the second generalized Newton-Girard identity. ∎
While the classical Newton identities deal with a single set of variables, introducing a second set of variables in and allowed us to prove analogs of the Newton identities. The natural next step would be to extend our results to three or more sets of variables, and see if this reveals new structure in the Newton identities. However, the three variable extension does not appear to have a similar closed form expression.
4. Evaluation of symmetric polynomials
As an addendum, we collect several evaluations of symmetric polynomials. We can formulaically apply any of the results above, simply substituting the objects below whenever , , and appear. By applying Theorem 4 to any of the specialized sets of variables , we obtain identities of independent interest.
Firstly, if we set each to , we recover binomial coefficients since and . These follow from counting the number of unique orderings and , with . When we consider geometric progressions and set , we obtain -binomial coefficients as a consequence of the -binomial theorem. The -binomial coefficient is defined, for , as
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where
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is a q-Pochhammer symbol. We rely on the -binomial theorem [3, Chapter 1], namely
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and
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Recognizing as the generating product for elementary symmetric functions, and as generating complete symmetric functions while comparing coefficients of yields the given evaluation.
Next we consider the Jacobi-Stirling numbers, a generalization of the Stirling numbers which naturally arise in the spectral theory of the Jacobi differential expression [5]. We let denote a Jacobi-Stirling number of the first kind, and a Jacobi-Stirling number of the second kind. The article [11] proves the equalities
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and
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by showing that both sides of Identities (4.5) and (4.6) satisfy the same recurrence relations. This means that we can apply any of our theorems about and to the Jacobi-Stirling numbers, which is the main idea of [8] and [9].
We now consider , an -Whitney number of the first kind, and , an -Whitney number of the second kind. These are common generalizations of the Stirling and Whitney numbers. Results about them are systematized in the work [10], which explores them as the symmetric function evaluations
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and
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Sums of powers of arithmetic progressions have been explored several times. We have the result [10]
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where is a Bernoulli polynomial.
We now move from considering combinatorial quantities to multiple zeta values, which have been the subject of increasing study by number theorists. We define
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and
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as multiple zeta and multiple zeta star values. These are generalizations of the Riemann zeta function which are increasingly important in fields from conformal field theory to knot theory. Letting be an infinite set of variables, we see that the definitions of these multiple zeta values and our symmetric polynomials and coincide. We also recognize as the Riemann zeta function since . This point of view is extensively explored in [13].
Our last result naturally extends the multiple-zeta point of view. We take , where is the -th prime. We then see that is a summation ranging over all squarefree integers with distinct prime factors, while is a summation over all integers with distinct prime factors. This is encoded by the sums
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and
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since , with the Möbius function, is the indicator function for squarefree numbers. Additionally, denotes the number of distinct prime factors of . We then have an evaluation of in terms of the prime zeta function , defined as . The reader is referred to [14] for further details.
We note some overarching trends: letting be a natural number and then considering an infinite number of variables gives us information about multiple zeta values. Letting be a prime number gives us information about natural numbers. We have studied symmetric functions where is a polynomial of degree [math], , and in . Considering a finite number of variables gives us information about classical combinatorial objects. Are there some results that hold for the symmetric functions of when is a polynomial of arbitrary degree in ? We also note that many -series identities follow from setting to be some function of , then taking and reindexing any summations to be over powers of .
These examples highlight the vast reach of symmetric polynomial identities, and the fact that any progress on basic symmetric function identities will have many varied applications.
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The reference list from the paper itself. Each links out to its DOI / PubMed record.
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- 2[2] I. G. Macdonald, Symmetric functions and orthogonal polynomials, University Lecture Series, Vol. 12, Dean Jacqueline B. Lewis Memorial Lectures presented at Rutgers University, New Brunswick, NJ, American Mathematical Society, Providence, RI, 1998.
- 3[3] G. Gasper and M. Rahman, Basic hypergeometric series, Encyclopedia of Mathematics and its Applications, Vol. 96, 2nd ed., Cambridge University Press, Cambridge, 2004.
- 4[4] G. A. Baker Jr., A new derivation of Newton’s identities and their application to the calculation of the eigenvalues of a matrix, J. Soc. Indust. Appl. Math. 7 (1959) 143–148.
- 5[5] W. N. Everitt and K. H. Kwon and L. L. Littlejohn and R. Wellman and G. J. Yoon, A Jacobi-Stirling numbers, Jacobi polynomials, and the left-definite analysis of the classical Jacobi differential expression, Journal of Computational and Applied Mathematics 208 : 1 (2007) 29–56.
- 6[6] D. G. Mead, Newton’s Identities, Amer. Math. Monthly 99 : 8 (1992) 749–751.
- 7[7] M. Merca, New convolutions for complete and elementary symmetric functions, Integral Transforms Spec. Funct. 27 : 12 (2016) 965–973.
- 8[8] M. Merca, A connection between Jacobi-Stirling numbers and Bernoulli polynomials, Journal of Number Theory 151 (2015) 223–229.
