- E-function
In
mathematics , "E"-functions are a type ofpower series that satisfy particular systems of linear differential equations.Definition
A function "f"("x") is called of type "E", or an "E"-function [Carl Ludwig Siegel, "Transcendental Numbers", p.33, Princeton University Press, 1949.] , if the power series
:
satisfies the following three conditions:
* All the coefficients "cn" belong to the same
algebraic number field , "K", which has finite degree over the rational numbers;
* For all ε > 0,:,where the left hand side represents the maximum of the absolute values of all the algebraic conjugates of "cn";
* For all ε > 0 there is a sequence of natural numbers "q"0, "q"1, "q"2,… such that "qnck" is analgebraic integer in "K" for "k"=0, 1, 2,…, "n", and "n" = 0, 1, 2,… and for which:.The second condition implies that "f" is an
entire function of "x".Uses
"E"-functions were first studied by Siegel in 1929 [C.L. Siegel, "Über einige Anwendungen diophantischer Approximationen", Abh. Preuss. Akad. Wiss. 1, 1929.] . He found a method to show that the values taken by certain "E"-functions were
algebraically independent , one of the only results of the early twentieth century which established the algebraic independence of classes of numbers rather than just linear independence [Alan Baker, "Transcendental Number Theory", pp.109-112, Cambridge University Press, 1975.] . Since then these functions have proved somewhat useful innumber theory and in particular they have application in transcendence proofs anddifferential equations [Serge Lang, "Introduction to Transcendental Numbers", pp.76-77, Addison-Wesley Publishing Company, 1966.] .The Siegel-Shidlovsky theorem
Perhaps the main result connected to "E"-functions is the Siegel-Shidlovsky theorem (known also as the Shidlovsky and Shidlovskii theorem).
Suppose that we are given "n" "E"-functions, "E"1("x"),…,"E""n"("x"), that satisfy a system of homogeneous linear differential equations:where the "fij" are rational functions of "x", and the coefficients of each "E" and "f" are elements of an algebraic number field "K". Then the theorem states that if "E"1("x"),…,"E""n"("x") are algebraically independent over "K"("x"), then for any non-zero algebraic number α that is not a pole of any of the "fij" the numbers "E"1(α),…,"E""n"(α) are algebraically independent.
Examples
# Any polynomial with algebraic coefficients is a simple example of an "E"-function.
# Theexponential function is an "E"-function, in its case "cn"=1 for all of the "n".
# If λ is an algebraic number then theBessel function "J"λ is an "E"-function.
# The sum or product of two "E"-functions is an "E"-function. In particular "E"-functions form a ring.
# If "a" is an algebraic number and "f"("x") is an "E"-function then "f"("ax") will be an "E"-function.
# If "f"("x") is an "E"-function then the derivative and integral of "f" are also "E"-functions.References
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