Humbert series

From Wikipedia, the free encyclopedia
Jump to: navigation, search

In mathematics, Humbert series are a set of seven hypergeometric series Φ1, Φ2, Φ3, Ψ1, Ψ2, Ξ1, Ξ2 of two variables that generalize Kummer's confluent hypergeometric series 1F1 of one variable and the confluent hypergeometric limit function 0F1 of one variable. The first of these double series was introduced by Pierre Humbert (1920).

Definitions[edit]

The Humbert series Φ1 is defined for |x| < 1 by the double series:


\Phi_1(a,b,c;x,y) = \sum_{m,n=0}^\infty \frac{(a)_{m+n} (b)_m} {(c)_{m+n} \,m! \,n!} \,x^m y^n ~,

where the Pochhammer symbol (q)n represents the rising factorial:

(q)_n = \frac{\Gamma(q+n)}{\Gamma(q)} = q\,(q+1) \cdots (q+n-1) ~.

For other values of x the function Φ1 can be defined by analytic continuation.

Similarly, the function Φ2 is defined for all x, y by the series:


\Phi_2(b_1,b_2,c;x,y) = \sum_{m,n=0}^\infty \frac{(b_1)_m (b_2)_n} {(c)_{m+n} \,m! \,n!} \,x^m y^n ~,

the function Φ3 for all x, y by the series:


\Phi_3(b,c;x,y) = \sum_{m,n=0}^\infty \frac{(b)_m} {(c)_{m+n} \,m! \,n!} \,x^m y^n ~,

the function Ψ1 for |x| < 1 by the series:


\Psi_1(a,b,c_1,c_2;x,y) = \sum_{m,n=0}^\infty \frac{(a)_{m+n} (b)_m} {(c_1)_m (c_2)_n \,m! \,n!} \,x^m y^n ~,

the function Ψ2 for all x, y by the series:


\Psi_2(a,c_1,c_2;x,y) = \sum_{m,n=0}^\infty \frac{(a)_{m+n}} {(c_1)_m (c_2)_n \,m! \,n!} \,x^m y^n ~,

the function Ξ1 for |x| < 1 by the series:


\Xi_1(a_1,a_2,b,c;x,y) = \sum_{m,n=0}^\infty \frac{(a_1)_m (a_2)_n (b)_m} {(c)_{m+n} \,m! \,n!} \,x^m y^n ~,

and the function Ξ2 for |x| < 1 by the series:


\Xi_2(a,b,c;x,y) = \sum_{m,n=0}^\infty \frac{(a)_m (b)_m} {(c)_{m+n} \,m! \,n!} \,x^m y^n ~.

Related series[edit]

There are four related series of two variables, F1, F2, F3, and F4, which generalize Gauss's hypergeometric series 2F1 of one variable in a similar manner and which were introduced by Paul Émile Appell in 1880.

References[edit]