In mathematics, the Gaussian or ordinary hypergeometric function 2F1(a,b;c;z) is a special function represented by the hypergeometric series, that includes many other special functions as specific or limiting cases. It is a solution of a second-order linear ordinary differential equation (ODE). Every second-order linear ODE with three regular singular points can be transformed into this equation.
For systematic lists of some of the many thousands of published identities involving the hypergeometric function, see the reference works by Arthur Erdélyi, Wilhelm Magnus, and Fritz Oberhettinger et al. (1953), Abramowitz & Stegun (1965), and Daalhuis (2010).
Contents |
The term "hypergeometric series" was first used by John Wallis in his 1655 book Arithmetica Infinitorum. Hypergeometric series were studied by Euler, but the first full systematic treatment was given by Gauss (1813), Studies in the nineteenth century included those of Ernst Kummer (1836), and the fundamental characterisation by Bernhard Riemann of the hypergeometric function by means of the differential equation it satisfies. Riemann showed that the second-order differential equation (in z) for the 2F1, examined in the complex plane, could be characterised (on the Riemann sphere) by its three regular singularities.
The cases where the solutions are algebraic functions were found by H. A. Schwarz (Schwarz's list).
The hypergeometric function is defined for |z| < 1 by the series
provided that c is not 0, −1, −2, … Notice that the series terminates if either "a" or "b" is a negative integer. The Pochhammer symbol is defined by
For other complex values of z it can be analytically continued along any path in the complex plane that avoids the branch points 0 and 1.
Many of the common mathematical functions can be expressed in terms of the hypergeometric function, or as limiting cases of it. Some typical examples are
The confluent hypergeometric function (or Kummer's function) can be given as a limit of the hypergeometric function
so all functions that are essentially special cases of it, such as Bessel functions, can be expressed as limits of hypergeometric functions. These include most of the commonly used functions of mathematical physics.
Legendre functions are solutions of a second order differential equation with 3 regular singular points so can be expressed in terms of the hypergeometric function in many ways, for example
Several orthogonal polynomials, including Jacobi polynomials P(α,β)
n and their special cases Legendre polynomials, Chebyshev polynomials, Gegenbauer polynomials can be written in terms of hypergeometric functions using
Other polynomials that are special cases include Krawtchouk polynomials, Meixner polynomials, Meixner–Pollaczek polynomials.
Elliptic modular functions can sometimes be expressed as the inverse functions of ratios of hypergeometric functions whose arguments a, b, c are 1, 1/2, 1/3, ... or 0. For examples, if
then
is an elliptic modular function of τ.
Incomplete beta functions Bx(p,q) are related by
The complete elliptic integrals K and E are given by
The hypergeometric function is a solution of Euler's hypergeometric differential equation
which has three regular singular points: 0,1 and ∞. The generalization of this equation to three arbitrary regular singular points is given by Riemann's differential equation. Any second order differential equation with three regular singular points can be converted to the hypergeometric differential equation by a change of variables.
Solutions to the hypergeometric differential equation are built out of the hypergeometric series . The equation has two linearly independent solutions. At each of the three singular points 0, 1, ∞, there are usually two special solutions of the form xs times a holomorphic function of x, where s is one of the two roots of the indicial equation and x is a local variable vanishing at the regular singular point. This gives 3 × 2 = 6 special solutions, as follows.
Around the point z = 0, two independent solutions are, if c is not an integer,
and
Around z = 1, if c − a − b is not an integer, one has two independent solutions
and
Around z = ∞, if a − b is not an integer, one has two independent solutions
and
Any 3 of these 6 solutions satisfy a linear relation as the space of solutions is 2-dimensional, giving (6
3) = 20 linear relations between them called connection formulas.
A second order Fuchsian equation with n singular points has a group of symmetries acting (projectively) on its solutions, isomorphic to the Coxeter group Dn of order 2n-1×n!. For the hypergeometric equation n=3, so the group is of order 24 and is isomorphic to the symmetric group on 4 points, and was first described by Kummer. The isomorphism with the symmetric group is accidental and has no analogue for more than 3 singular points, and it is sometimes better to think of the group as an extension of the symmetric group on 3 points (acting as permutations of the 3 singular points) by a Klein 4-group (whose elements change the signs of the differences of the exponents at an even number of singular points). Kummer's group of 24 transformations is generated by the three transformations taking a solution F(a, b; c; z) to one of
which correspond to the transpositions (12), (23), and (34) under an isomorphism with the symmetric group on 4 points 1, 2, 3, 4.
Applying Kummer's 24=6×4 transformations to the hypergeometric function gives the 6 = 2×3 solutions above corresponding to each of the 2 possible exponents at each of the 3 singular points, each of which appears 4 times because of the identities
The hypergeometric differential equation may be brought into the Q-form
by making the substitution w = uv and eliminating the first-derivative term. One finds that
and v is given by the solution to
The Q-form is significant in its relation to the Schwarzian derivative.
The Schwarz triangle maps or Schwarz s-functions are ratios of pairs of solutions.
where k is one of the points 0, 1, ∞. The notation
is also sometimes used. Note that the connection coefficients become Möbius transformations on the triangle maps.
Note that each triangle map is regular at z ∈ {0, 1, ∞} respectively, with
and
In the special case of λ, μ and ν real, with then the s-maps are conformal maps of the upper half-plane H to triangles on the Riemann sphere, bounded by circular arcs. This mapping is a special case of a Schwarz–Christoffel mapping. The singular points 0,1 and ∞ are sent to the triangle vertices. The angles of the triangle are πλ, πμ and πν respectively.
Furthermore, in the case of λ=1/p, μ=1/q and ν=1/r for integers p, q, r, then the triangle tiles the sphere, and the s-maps are inverse functions of automorphic functions for the triangle group
The monodromy of a hypergeometric equation describes how fundamental solutions change when analytically continued around paths in the z plane that return to the same point. That is, when the path winds around a singularity of , the value of the solutions at the endpoint will differ from the starting point.
Two fundamental solutions of the hypergeometric equation are related to each other by a linear transformation; thus the monodromy is a mapping (group homomorphism):
where is the fundamental group. In other words the monodromy is a two dimensional linear representation of the fundamental group. The monodromy group of the equation is the image of this map, i.e. the group generated by the monodromy matrices.
If B is the beta function then
provided |z| < 1 or |z| = 1 and both sides converge, and can be proved by expanding (1 − zx)−a using the binomial theorem and then integrating term by term. This was given by Euler in 1748 and implies Euler's and Pfaff's hypergeometric transformations.
Other representations, corresponding to other branches, are given by taking the same integrand, but taking the path of integration to be a closed Pochhammer cycle enclosing the singularities in various orders. Such paths correspond to the monodromy action.
Barnes used the theory of residues to evaluate the Barnes integral
as
where the contour is drawn to separate the poles 0, 1, 2... from the poles −a, −a - 1, ..., −b, −b − 1, ... .
The Gauss hypergeometric function can be written as a John transform (Gelfand, Gindikin & Graev 2003, 2.1.2).
The six functions , , and are called contiguous to . Gauss showed that can be written as a linear combination of any two of its contiguous functions, with rational coefficients in terms of a,b,c, and z. This gives (6
2)=15 relations, given by identifying any two lines on the right hand side of
In the notation above, and so on.
Repeatedly applying these relations gives a linear relation between any three functions of the form , where m, n, and l are integers.
Gauss used the contiguous relations to give several ways to write a quotient of two hypergeometric functions as a continued fraction, for example:
Transformation formulas relate two hypergeometric functions at different values of the argument z.
Euler's transformation is
It follows by combining the two Pfaff transformations
which in turn follow from Euler's integral representation.
If two of the numbers 1 − c, c − 1, a − b, b − a, a + b − c, c − a − b are equal or one of them is 1/2 then there is a quadratic transformation of the hypergeometric function, connecting it to a different value of z related by a quadratic equation. The first examples were given by Kummer (1836), and a complete list was given by Goursat (1881). A typical example is
If 1−c, a−b, a+b−c differ by signs or two of them are 1/3 or −1/3 then there is a cubic transformation of the hypergeometric function, connecting it to a different value of z related by a cubic equation. The first examples were given by Goursat (1881). A typical example is
There are also some transformations of degree 4 and 6. Transformations of other degrees only exist if a, b, and c are certain rational numbers, when the hypergeometric function becomes algebraic.
See (Slater 1966, Appendix III) for a list of summation formulas at special points, most of which also appear in (Bailey 1935). (Gessel & Stanton 1982) gives further evaluations at more points. (Koepf 1995) shows how most of these identities can be verifed by computer algorithms.
Gauss's theorem, named for Carl Friedrich Gauss, is the identity
which follows from Euler's integral formula by putting z = 1. It includes the Vandermonde identity, first found by Zhu Shijie (= Chu Shi-Chieh), as a special case.
Dougall's formula generalizes this to the bilateral hypergeometric series at z = 1.
There are many cases where hypergeometric functions can be evaluated at z = −1 by using a quadratic transformation to change z = −1 to z = 1 and then using Gauss's theorem to evaluate the result. A typical example is Kummer's theorem, named for Ernst Kummer:
which follows from Kummer's quadratic transformations
and Gauss's theorem by putting z = −1 in the first identity.
Gauss's second summation theorem is
Bailey's theorem is
There are many other formulas giving the hypergeometric function as an algebraic number at special rational values of the parameters, some of which are listed in (Gessel & Stanton 1982) and (Koepf 1995). Some typical examples are given by
Generalizations of the hypergeometric function include: