India-based Neutrino Observatory

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The Wright Omega function along part of the real axis

In mathematics, the Wright omega function or Wright function,[1] denoted ω, is defined in terms of the Lambert W function as:

ω(z)=WIm(z)π2π(ez).

Uses

One of the main applications of this function is in the resolution of the equation z = ln(z), as the only solution is given by z = e−ω(π i).

y = ω(z) is the unique solution, when zx±iπ for x ≤ −1, of the equation y + ln(y) = z. Except on those two rays, the Wright omega function is continuous, even analytic.

Properties

The Wright omega function satisfies the relation Wk(z)=ω(ln(z)+2πik).

It also satisfies the differential equation

dωdz=ω1+ω

wherever ω is analytic (as can be seen by performing separation of variables and recovering the equation ln(ω)+ω=z), and as a consequence its integral can be expressed as:

wndz={ωn+11n+1+ωnnif n1,ln(ω)1ωif n=1.

Its Taylor series around the point a=ωa+ln(ωa) takes the form :

ω(z)=n=0+qn(ωa)(1+ωa)2n1(za)nn!

where

qn(w)=k=0n1n+1k(1)kwk+1

in which

nk

is a second-order Eulerian number.

Values

ω(0)=W0(1)0.56714ω(1)=1ω(1±iπ)=1ω(13+ln(13)+iπ)=13ω(13+ln(13)iπ)=W1(13e13)2.237147028

Plots

Notes

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References

  1. Not to be confused with the Fox–Wright function, also known as Wright function.