The polynomials arise in:
- probability, such as the Edgeworth series;
- in combinatorics, as an example of an Appell sequence, obeying the umbral calculus;
- in numerical analysis as Gaussian quadrature;
- in physics, where they give rise to the eigenstates of the quantum harmonic oscillator;
- in systems theory in connection with nonlinear operations on Gaussian noise.
- in random matrix theory in Wigner–Dyson ensembles.
Hermite polynomials were defined by Pierre-Simon Laplace in 1810, though in scarcely recognizable form, and studied in detail by Pafnuty Chebyshev in 1859. Chebyshev's work was overlooked, and they were named later after Charles Hermite, who wrote on the polynomials in 1864, describing them as new. They were consequently not new, although Hermite was the first to define the multidimensional polynomials in his later 1865 publications.
There are two different ways of standardizing the Hermite polynomials:
- The "probabilists' Hermite polynomials" are given by
- while the "physicists' Hermite polynomials" are given by
These two definitions are not exactly identical; each is a rescaling of the other:
These are Hermite polynomial sequences of different variances; see the material on variances below.
- The first eleven probabilists' Hermite polynomials are:
- The first eleven physicists' Hermite polynomials are:
The nth-order Hermite polynomial is a polynomial of degree n. The probabilists' version Hen has leading coefficient 1, while the physicists' version Hn has leading coefficient 2n.
i.e., we have
where is the Kronecker delta.
The probabilist polynomials are thus orthogonal with respect to the standard normal probability density function.
in which the inner product is given by the integral
including the Gaussian weight function w(x) defined in the preceding section
An orthogonal basis for L2(R, w(x) dx) is a complete orthogonal system. For an orthogonal system, completeness is equivalent to the fact that the 0 function is the only function f ∈ L2(R, w(x) dx) orthogonal to all functions in the system.
Since the linear span of Hermite polynomials is the space of all polynomials, one has to show (in physicist case) that if f satisfies
for every n ≥ 0, then f = 0.
One possible way to do this is to appreciate that the entire function
vanishes identically. The fact then that F(it) = 0 for every real t means that the Fourier transform of f(x)e−x2 is 0, hence f is 0 almost everywhere. Variants of the above completeness proof apply to other weights with exponential decay.
In the Hermite case, it is also possible to prove an explicit identity that implies completeness (see section on the Completeness relation below).
An equivalent formulation of the fact that Hermite polynomials are an orthogonal basis for L2(R, w(x) dx) consists in introducing Hermite functions (see below), and in saying that the Hermite functions are an orthonormal basis for L2(R).
Hermite's differential equation
The probabilists' Hermite polynomials are solutions of the differential equation
where λ is a constant. Imposing the boundary condition that u should be polynomially bounded at infinity, the equation has solutions only if λ is a non-negative integer, and the solution is uniquely given by , where denotes a constant.
Rewriting the differential equation as an eigenvalue problem
the Hermite polynomials may be understood as eigenfunctions of the differential operator . This eigenvalue problem is called the Hermite equation, although the term is also used for the closely related equation
whose solution is uniquely given in terms of physicists' Hermite polynomials in the form , where denotes a constant, after imposing the boundary condition that u should be polynomially bounded at infinity.
The general solutions to the above second-order differential equations are in fact linear combinations of both Hermite polynomials and confluent hypergeometric functions of the first kind. For example, for the physicists' Hermite equation
the general solution takes the form
where and are constants, are physicists' Hermite polynomials (of the first kind), and are physicists' Hermite functions (of the second kind). The latter functions are compactly represented as where are Confluent hypergeometric functions of the first kind. The conventional Hermite polynomials may also be expressed in terms of confluent hypergeometric functions, see below.
With more general boundary conditions, the Hermite polynomials can be generalized to obtain more general analytic functions for complex-valued λ. An explicit formula of Hermite polynomials in terms of contour integrals (Courant & Hilbert 1989) is also possible.
The sequence of probabilists' Hermite polynomials also satisfies the recurrence relation
Individual coefficients are related by the following recursion formula:
and a0,0 = 1, a1,0 = 0, a1,1 = 1.
For the physicists' polynomials, assuming
Individual coefficients are related by the following recursion formula:
and a0,0 = 1, a1,0 = 0, a1,1 = 2.
The Hermite polynomials constitute an Appell sequence, i.e., they are a polynomial sequence satisfying the identity
Equivalently, by Taylor-expanding,
In consequence, for the mth derivatives the following relations hold:
It follows that the Hermite polynomials also satisfy the recurrence relation
These last relations, together with the initial polynomials H0(x) and H1(x), can be used in practice to compute the polynomials quickly.
Moreover, the following multiplication theorem holds:
The physicists' Hermite polynomials can be written explicitly as
These two equations may be combined into one using the floor function:
The probabilists' Hermite polynomials He have similar formulas, which may be obtained from these by replacing the power of 2x with the corresponding power of √ x and multiplying the entire sum by 2−n/:
Inverse explicit expression
The inverse of the above explicit expressions, that is, those for monomials in terms of probabilists’ Hermite polynomials He are
The Hermite polynomials are given by the exponential generating function
This equality is valid for all complex values of x and t, and can be obtained by writing the Taylor expansion at x of the entire function z → e−z2 (in the physicists' case). One can also derive the (physicists') generating function by using Cauchy's integral formula to write the Hermite polynomials as
Using this in the sum
one can evaluate the remaining integral using the calculus of residues and arrive at the desired generating function.
The moments of the standard normal (with expected value zero) may be read off directly from the relation for even indices:
where (2n − 1)!! is the double factorial. Note that the above expression is a special case of the representation of the probabilists' Hermite polynomials as moments:
holds true. For certain cases concerning a wider range of evaluation, it is necessary to include a factor for changing amplitude:
which, using Stirling's approximation, can be further simplified, in the limit, to
A better approximation, which accounts for the variation in frequency, is given by
with which one has the uniform approximation
Similar approximations hold for the monotonic and transition regions. Specifically, if
with t complex and bounded, the approximation is
where Ai is the Airy function of the first kind.
The physicists' Hermite polynomials evaluated at zero argument Hn(0) are called Hermite numbers.
which satisfy the recursion relation Hn(0) = −2(n − 1)Hn − 2(0).
In terms of the probabilists' polynomials this translates to
Relations to other functions
The Hermite polynomials can be expressed as a special case of the Laguerre polynomials:
Relation to confluent hypergeometric functions
The physicists' Hermite polynomials can be expressed as a special case of the parabolic cylinder functions:
where 1F1(a, b; z) = M(a, b; z) is Kummer's confluent hypergeometric function.
The probabilists' Hermite polynomials satisfy the identity
where D represents differentiation with respect to x, and the exponential is interpreted by expanding it as a power series. There are no delicate questions of convergence of this series when it operates on polynomials, since all but finitely many terms vanish.
Since the power-series coefficients of the exponential are well known, and higher-order derivatives of the monomial xn can be written down explicitly, this differential-operator representation gives rise to a concrete formula for the coefficients of Hn that can be used to quickly compute these polynomials.
Since the formal expression for the Weierstrass transform W is eD2, we see that the Weierstrass transform of (√)nHen(x/) is xn. Essentially the Weierstrass transform thus turns a series of Hermite polynomials into a corresponding Maclaurin series.
The existence of some formal power series g(D) with nonzero constant coefficient, such that Hen(x) = g(D)xn, is another equivalent to the statement that these polynomials form an Appell sequence. Since they are an Appell sequence, they are a fortiori a Sheffer sequence.
From the generating-function representation above, we see that the Hermite polynomials have a representation in terms of a contour integral, as
with the contour encircling the origin.
The probabilists' Hermite polynomials defined above are orthogonal with respect to the standard normal probability distribution, whose density function is
which has expected value 0 and variance 1.
of variance α, where α is any positive number. These are then orthogonal with respect to the normal probability distribution whose density function is
They are given by
then the polynomial sequence whose nth term is
is called the umbral composition of the two polynomial sequences. It can be shown to satisfy the identities
The last identity is expressed by saying that this parameterized family of polynomial sequences is known as a cross-sequence. (See the above section on Appell sequences and on the differential-operator representation, which leads to a ready derivation of it. This binomial type identity, for α = β = 1/, has already been encountered in the above section on #Recursion relations.)
the sequence that is inverse to the one similarly denoted, but without the minus sign, and thus speak of Hermite polynomials of negative variance. For α > 0, the coefficients of are just the absolute values of the corresponding coefficients of .
These arise as moments of normal probability distributions: The nth moment of the normal distribution with expected value μ and variance σ2 is
where X is a random variable with the specified normal distribution. A special case of the cross-sequence identity then says that
One can define the Hermite functions from the physicists' polynomials:
and they form an orthonormal basis of L2(R). This fact is equivalent to the corresponding statement for Hermite polynomials (see above).
and thereby to other parabolic cylinder functions.
The Hermite functions satisfy the differential equation
Following recursion relations of Hermite polynomials, the Hermite functions obey
Extending the first relation to the arbitrary mth derivatives for any positive integer m leads to
This formula can be used in connection with the recurrence relations for Hen and ψn to calculate any derivative of the Hermite functions efficiently.
For real x, the Hermite functions satisfy the following bound due to Harald Cramér and Jack Indritz:
Hermite functions as eigenfunctions of the Fourier transform
The Hermite functions ψn(x) are a set of eigenfunctions of the continuous Fourier transform F. To see this, take the physicists' version of the generating function and multiply by e−1/x2. This gives
The Fourier transform of the left side is given by
The Fourier transform of the right side is given by
Equating like powers of t in the transformed versions of the left and right sides finally yields
Wigner distributions of Hermite functions
leading to the oscillator Laguerre functions
where the Wigner distribution of a function x ∈ L2(R, C) is defined as
There are further relations between the two families of polynomials.
Combinatorial interpretation of coefficients
In the Hermite polynomial Hen(x) of variance 1, the absolute value of the coefficient of xk is the number of (unordered) partitions of an n-member set into k singletons and n − k/ (unordered) pairs. The sum of the absolute values of the coefficients gives the total number of partitions into singletons and pairs, the so-called telephone numbers
This combinatorial interpretation can be related to complete exponential Bell polynomials as
where xi = 0 for all i > 2.
The Christoffel–Darboux formula for Hermite polynomials reads
where δ is the Dirac delta function, ψn the Hermite functions, and δ(x − y) represents the Lebesgue measure on the line y = x in R2, normalized so that its projection on the horizontal axis is the usual Lebesgue measure.
The function (x, y) → E(x, y; u) is the bivariate Gaussian probability density on R2, which is, when u is close to 1, very concentrated around the line y = x, and very spread out on that line. It follows that
when f and g are continuous and compactly supported.
This yields that f can be expressed in Hermite functions as the sum of a series of vectors in L2(R), namely,
The Hermite polynomial is then represented as
With this representation for Hn(x) and Hn(y), it is evident that
and this yields the desired resolution of the identity result, using again the Fourier transform of Gaussian kernels under the substitution
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